Sample records for air-sea co2 fluxes

  1. Spatio-temporal visualization of air-sea CO2 flux and carbon budget using volume rendering

    NASA Astrophysics Data System (ADS)

    Du, Zhenhong; Fang, Lei; Bai, Yan; Zhang, Feng; Liu, Renyi

    2015-04-01

    This paper presents a novel visualization method to show the spatio-temporal dynamics of carbon sinks and sources, and carbon fluxes in the ocean carbon cycle. The air-sea carbon budget and its process of accumulation are demonstrated in the spatial dimension, while the distribution pattern and variation of CO2 flux are expressed by color changes. In this way, we unite spatial and temporal characteristics of satellite data through visualization. A GPU-based direct volume rendering technique using half-angle slicing is adopted to dynamically visualize the released or absorbed CO2 gas with shadow effects. A data model is designed to generate four-dimensional (4D) data from satellite-derived air-sea CO2 flux products, and an out-of-core scheduling strategy is also proposed for on-the-fly rendering of time series of satellite data. The presented 4D visualization method is implemented on graphics cards with vertex, geometry and fragment shaders. It provides a visually realistic simulation and user interaction for real-time rendering. This approach has been integrated into the Information System of Ocean Satellite Monitoring for Air-sea CO2 Flux (IssCO2) for the research and assessment of air-sea CO2 flux in the China Seas.

  2. Climate change impacts on sea-air fluxes of CO2 in three Arctic seas: a sensitivity study using Earth observation

    NASA Astrophysics Data System (ADS)

    Land, P. E.; Shutler, J. D.; Cowling, R. D.; Woolf, D. K.; Walker, P.; Findlay, H. S.; Upstill-Goddard, R. C.; Donlon, C. J.

    2013-12-01

    We applied coincident Earth observation data collected during 2008 and 2009 from multiple sensors (RA2, AATSR and MERIS, mounted on the European Space Agency satellite Envisat) to characterise environmental conditions and integrated sea-air fluxes of CO2 in three Arctic seas (Greenland, Barents, Kara). We assessed net CO2 sink sensitivity due to changes in temperature, salinity and sea ice duration arising from future climate scenarios. During the study period the Greenland and Barents seas were net sinks for atmospheric CO2, with integrated sea-air fluxes of -36 ± 14 and -11 ± 5 Tg C yr-1, respectively, and the Kara Sea was a weak net CO2 source with an integrated sea-air flux of +2.2 ± 1.4 Tg C yr-1. The combined integrated CO2 sea-air flux from all three was -45 ± 18 Tg C yr-1. In a sensitivity analysis we varied temperature, salinity and sea ice duration. Variations in temperature and salinity led to modification of the transfer velocity, solubility and partial pressure of CO2 taking into account the resultant variations in alkalinity and dissolved organic carbon (DOC). Our results showed that warming had a strong positive effect on the annual integrated sea-air flux of CO2 (i.e. reducing the sink), freshening had a strong negative effect and reduced sea ice duration had a small but measurable positive effect. In the climate change scenario examined, the effects of warming in just over a decade of climate change up to 2020 outweighed the combined effects of freshening and reduced sea ice duration. Collectively these effects gave an integrated sea-air flux change of +4.0 Tg C in the Greenland Sea, +6.0 Tg C in the Barents Sea and +1.7 Tg C in the Kara Sea, reducing the Greenland and Barents sinks by 11% and 53%, respectively, and increasing the weak Kara Sea source by 81%. Overall, the regional integrated flux changed by +11.7 Tg C, which is a 26% reduction in the regional sink. In terms of CO2 sink strength, we conclude that the Barents Sea is the most

  3. Deriving a sea surface climatology of CO2 fugacity in support of air-sea gas flux studies

    NASA Astrophysics Data System (ADS)

    Goddijn-Murphy, L. M.; Woolf, D. K.; Land, P. E.; Shutler, J. D.; Donlon, C.

    2014-07-01

    Climatologies, or long-term averages, of essential climate variables are useful for evaluating models and providing a baseline for studying anomalies. The Surface Ocean Carbon Dioxide (CO2) Atlas (SOCAT) has made millions of global underway sea surface measurements of CO2 publicly available, all in a uniform format and presented as fugacity, fCO2. fCO2 is highly sensitive to temperature and the measurements are only valid for the instantaneous sea surface temperature (SST) that is measured concurrent with the in-water CO2 measurement. To create a climatology of fCO2 data suitable for calculating air-sea CO2 fluxes it is therefore desirable to calculate fCO2 valid for climate quality SST. This paper presents a method for creating such a climatology. We recomputed SOCAT's fCO2 values for their respective measurement month and year using climate quality SST data from satellite Earth observation and then extrapolated the resulting fCO2 values to reference year 2010. The data were then spatially interpolated onto a 1° × 1° grid of the global oceans to produce 12 monthly fCO2 distributions for 2010. The partial pressure of CO2 (pCO2) is also provided for those who prefer to use pCO2. The CO2 concentration difference between ocean and atmosphere is the thermodynamic driving force of the air-sea CO2 flux, and hence the presented fCO2 distributions can be used in air-sea gas flux calculations together with climatologies of other climate variables.

  4. The OceanFlux Greenhouse Gases methodology for deriving a sea surface climatology of CO2 fugacity in support of air-sea gas flux studies

    NASA Astrophysics Data System (ADS)

    Goddijn-Murphy, L. M.; Woolf, D. K.; Land, P. E.; Shutler, J. D.; Donlon, C.

    2015-07-01

    Climatologies, or long-term averages, of essential climate variables are useful for evaluating models and providing a baseline for studying anomalies. The Surface Ocean CO2 Atlas (SOCAT) has made millions of global underway sea surface measurements of CO2 publicly available, all in a uniform format and presented as fugacity, fCO2. As fCO2 is highly sensitive to temperature, the measurements are only valid for the instantaneous sea surface temperature (SST) that is measured concurrently with the in-water CO2 measurement. To create a climatology of fCO2 data suitable for calculating air-sea CO2 fluxes, it is therefore desirable to calculate fCO2 valid for a more consistent and averaged SST. This paper presents the OceanFlux Greenhouse Gases methodology for creating such a climatology. We recomputed SOCAT's fCO2 values for their respective measurement month and year using monthly composite SST data on a 1° × 1° grid from satellite Earth observation and then extrapolated the resulting fCO2 values to reference year 2010. The data were then spatially interpolated onto a 1° × 1° grid of the global oceans to produce 12 monthly fCO2 distributions for 2010, including the prediction errors of fCO2 produced by the spatial interpolation technique. The partial pressure of CO2 (pCO2) is also provided for those who prefer to use pCO2. The CO2 concentration difference between ocean and atmosphere is the thermodynamic driving force of the air-sea CO2 flux, and hence the presented fCO2 distributions can be used in air-sea gas flux calculations together with climatologies of other climate variables.

  5. Sensitivity of Global Sea-Air CO2 Flux to Gas Transfer Algorithms, Climatological Wind Speeds, and Variability of Sea Surface Temperature and Salinity

    NASA Technical Reports Server (NTRS)

    McClain, Charles R.; Signorini, Sergio

    2002-01-01

    Sensitivity analyses of sea-air CO2 flux to gas transfer algorithms, climatological wind speeds, sea surface temperatures (SST) and salinity (SSS) were conducted for the global oceans and selected regional domains. Large uncertainties in the global sea-air flux estimates are identified due to different gas transfer algorithms, global climatological wind speeds, and seasonal SST and SSS data. The global sea-air flux ranges from -0.57 to -2.27 Gt/yr, depending on the combination of gas transfer algorithms and global climatological wind speeds used. Different combinations of SST and SSS global fields resulted in changes as large as 35% on the oceans global sea-air flux. An error as small as plus or minus 0.2 in SSS translates into a plus or minus 43% deviation on the mean global CO2 flux. This result emphasizes the need for highly accurate satellite SSS observations for the development of remote sensing sea-air flux algorithms.

  6. Air-ice CO2 fluxes and pCO2 dynamics in the Arctic coastal area (Amundsen Gulf, Canada)

    NASA Astrophysics Data System (ADS)

    Geilfus, Nicolas-Xavier; Tison, Jean Louis; Carnat, Gauthier; Else, Brent; Borges, Alberto V.; Thomas, Helmuth; Shadwick, Elizabeth; Delille, Bruno

    2010-05-01

    Sea ice covers about 7% of the Earth surface at its maximum seasonal extent. For decades sea ice was assumed to be an impermeable and inert barrier for air - sea exchange of CO2 so that global climate models do not include CO2 exchange between the oceans and the atmosphere in the polar regions. However, uptake of atmospheric CO2 by sea ice cover was recently reported raising the need to further investigate pCO2 dynamics in the marine cryosphere realm and related air-ice CO2 fluxes. In addition, budget of CO2 fluxes are poorly constrained in high latitudes continental shelves [Borges et al., 2006]. We report measurements of air-ice CO2 fluxes above the Canadian continental shelf and compare them to previous measurements carried out in Antarctica. We carried out measurements of pCO2 within brines and bulk ice, and related air-ice CO2 fluxes (chamber method) in Antarctic first year pack ice ("Sea Ice Mass Balance in Antarctica -SIMBA" drifting station experiment September - October 2007) and in Arctic first year land fast ice ("Circumpolar Flaw Lead" - CFL, April - June 2008). These 2 experiments were carried out in contrasted sites. SIMBA was carried out on sea ice in early spring while CFL was carried out in from the middle of the winter to the late spring while sea ice was melting. Both in Arctic and Antarctic, no air-ice CO2 fluxes were detected when sea ice interface was below -10°C. Slightly above -10°C, fluxes toward the atmosphere were observed. In contrast, at -7°C fluxes from the atmosphere to the ice were significant. The pCO2 of the brine exhibits a same trend in both hemispheres with a strong decrease of the pCO2 anti-correlated with the increase of sea ice temperature. The pCO2 shifted from a large over-saturation at low temperature to a marked under-saturation at high temperature. These air-ice CO2 fluxes are partly controlled by the permeability of the air-ice interface, which depends of the temperature of this one. Moreover, air-ice CO2 fluxes are

  7. The Effect of Breaking Waves on CO_2 Air-Sea Fluxes in the Coastal Zone

    NASA Astrophysics Data System (ADS)

    Gutiérrez-Loza, Lucía; Ocampo-Torres, Francisco J.; García-Nava, Héctor

    2018-03-01

    The influence of wave-associated parameters controlling turbulent CO_2 fluxes through the air-sea interface is investigated in a coastal region. A full year of high-quality data of direct estimates of air-sea CO_2 fluxes based on eddy-covariance measurements is presented. The study area located in Todos Santos Bay, Baja California, Mexico, is a net sink of CO_2 with a mean flux of -1.3 μmol m^{-2}s^{-1} (-41.6 mol m^{-2}yr^{-1} ). The results of a quantile-regression analysis computed between the CO_2 flux and, (1) wind speed, (2) significant wave height, (3) wave steepness, and (4) water temperature, suggest that the significant wave height is the most correlated parameter with the magnitude of the flux but the behaviour of the relation varies along the probability distribution function, with the slopes of the regression lines presenting both positive and negative values. These results imply that the presence of surface waves in coastal areas is the key factor that promotes the increase of the flux from and into the ocean. Further analysis suggests that the local characteristics of the aqueous and atmospheric layers might determine the direction of the flux.

  8. Arctic Ocean CO2 uptake: an improved multiyear estimate of the air-sea CO2 flux incorporating chlorophyll a concentrations

    NASA Astrophysics Data System (ADS)

    Yasunaka, Sayaka; Siswanto, Eko; Olsen, Are; Hoppema, Mario; Watanabe, Eiji; Fransson, Agneta; Chierici, Melissa; Murata, Akihiko; Lauvset, Siv K.; Wanninkhof, Rik; Takahashi, Taro; Kosugi, Naohiro; Omar, Abdirahman M.; van Heuven, Steven; Mathis, Jeremy T.

    2018-03-01

    We estimated monthly air-sea CO2 fluxes in the Arctic Ocean and its adjacent seas north of 60° N from 1997 to 2014. This was done by mapping partial pressure of CO2 in the surface water (pCO2w) using a self-organizing map (SOM) technique incorporating chlorophyll a concentration (Chl a), sea surface temperature, sea surface salinity, sea ice concentration, atmospheric CO2 mixing ratio, and geographical position. We applied new algorithms for extracting Chl a from satellite remote sensing reflectance with close examination of uncertainty of the obtained Chl a values. The overall relationship between pCO2w and Chl a was negative, whereas the relationship varied among seasons and regions. The addition of Chl a as a parameter in the SOM process enabled us to improve the estimate of pCO2w, particularly via better representation of its decline in spring, which resulted from biologically mediated pCO2w reduction. As a result of the inclusion of Chl a, the uncertainty in the CO2 flux estimate was reduced, with a net annual Arctic Ocean CO2 uptake of 180 ± 130 Tg C yr-1. Seasonal to interannual variation in the CO2 influx was also calculated.

  9. Effects of sea-ice and biogeochemical processes and storms on under-ice water fCO2 during the winter-spring transition in the high Arctic Ocean: Implications for sea-air CO2 fluxes

    NASA Astrophysics Data System (ADS)

    Fransson, Agneta; Chierici, Melissa; Skjelvan, Ingunn; Olsen, Are; Assmy, Philipp; Peterson, Algot K.; Spreen, Gunnar; Ward, Brian

    2017-07-01

    We performed measurements of carbon dioxide fugacity (fCO2) in the surface water under Arctic sea ice from January to June 2015 during the Norwegian young sea ICE (N-ICE2015) expedition. Over this period, the ship drifted with four different ice floes and covered the deep Nansen Basin, the slopes north of Svalbard, and the Yermak Plateau. This unique winter-to-spring data set includes the first winter-time under-ice water fCO2 observations in this region. The observed under-ice fCO2 ranged between 315 µatm in winter and 153 µatm in spring, hence was undersaturated relative to the atmospheric fCO2. Although the sea ice partly prevented direct CO2 exchange between ocean and atmosphere, frequently occurring leads and breakup of the ice sheet promoted sea-air CO2 fluxes. The CO2 sink varied between 0.3 and 86 mmol C m-2 d-1, depending strongly on the open-water fractions (OW) and storm events. The maximum sea-air CO2 fluxes occurred during storm events in February and June. In winter, the main drivers of the change in under-ice water fCO2 were dissolution of CaCO3 (ikaite) and vertical mixing. In June, in addition to these processes, primary production and sea-air CO2 fluxes were important. The cumulative loss due to CaCO3 dissolution of 0.7 mol C m-2 in the upper 10 m played a major role in sustaining the undersaturation of fCO2 during the entire study. The relative effects of the total fCO2 change due to CaCO3 dissolution was 38%, primary production 26%, vertical mixing 16%, sea-air CO2 fluxes 16%, and temperature and salinity insignificant.

  10. Mapping of the air-sea CO2 flux in the Arctic Ocean and its adjacent seas: Basin-wide distribution and seasonal to interannual variability

    NASA Astrophysics Data System (ADS)

    Yasunaka, Sayaka; Murata, Akihiko; Watanabe, Eiji; Chierici, Melissa; Fransson, Agneta; van Heuven, Steven; Hoppema, Mario; Ishii, Masao; Johannessen, Truls; Kosugi, Naohiro; Lauvset, Siv K.; Mathis, Jeremy T.; Nishino, Shigeto; Omar, Abdirahman M.; Olsen, Are; Sasano, Daisuke; Takahashi, Taro; Wanninkhof, Rik

    2016-09-01

    We produced 204 monthly maps of the air-sea CO2 flux in the Arctic north of 60°N, including the Arctic Ocean and its adjacent seas, from January 1997 to December 2013 by using a self-organizing map technique. The partial pressure of CO2 (pCO2) in surface water data were obtained by shipboard underway measurements or calculated from alkalinity and total inorganic carbon of surface water samples. Subsequently, we investigated the basin-wide distribution and seasonal to interannual variability of the CO2 fluxes. The 17-year annual mean CO2 flux shows that all areas of the Arctic Ocean and its adjacent seas were net CO2 sinks. The estimated annual CO2 uptake by the Arctic Ocean was 180 TgC yr-1. The CO2 influx was strongest in winter in the Greenland/Norwegian Seas (>15 mmol m-2 day-1) and the Barents Sea (>12 mmol m-2 day-1) because of strong winds, and strongest in summer in the Chukchi Sea (∼10 mmol m-2 day-1) because of the sea-ice retreat. In recent years, the CO2 uptake has increased in the Greenland/Norwegian Sea and decreased in the southern Barents Sea, owing to increased and decreased air-sea pCO2 differences, respectively.

  11. A Sensitivity Analysis of the Impact of Rain on Regional and Global Sea-Air Fluxes of CO2

    PubMed Central

    Shutler, J. D.; Land, P. E.; Woolf, D. K.; Quartly, G. D.

    2016-01-01

    The global oceans are considered a major sink of atmospheric carbon dioxide (CO2). Rain is known to alter the physical and chemical conditions at the sea surface, and thus influence the transfer of CO2 between the ocean and atmosphere. It can influence gas exchange through enhanced gas transfer velocity, the direct export of carbon from the atmosphere to the ocean, by altering the sea skin temperature, and through surface layer dilution. However, to date, very few studies quantifying these effects on global net sea-air fluxes exist. Here, we include terms for the enhanced gas transfer velocity and the direct export of carbon in calculations of the global net sea-air fluxes, using a 7-year time series of monthly global climate quality satellite remote sensing observations, model and in-situ data. The use of a non-linear relationship between the effects of rain and wind significantly reduces the estimated impact of rain-induced surface turbulence on the rate of sea-air gas transfer, when compared to a linear relationship. Nevertheless, globally, the rain enhanced gas transfer and rain induced direct export increase the estimated annual oceanic integrated net sink of CO2 by up to 6%. Regionally, the variations can be larger, with rain increasing the estimated annual net sink in the Pacific Ocean by up to 15% and altering monthly net flux by > ± 50%. Based on these analyses, the impacts of rain should be included in the uncertainty analysis of studies that estimate net sea-air fluxes of CO2 as the rain can have a considerable impact, dependent upon the region and timescale. PMID:27673683

  12. Climatological mean and decadal change in surface ocean pCO 2, and net sea-air CO 2 flux over the global oceans

    NASA Astrophysics Data System (ADS)

    Takahashi, Taro; Sutherland, Stewart C.; Wanninkhof, Rik; Sweeney, Colm; Feely, Richard A.; Chipman, David W.; Hales, Burke; Friederich, Gernot; Chavez, Francisco; Sabine, Christopher; Watson, Andrew; Bakker, Dorothee C. E.; Schuster, Ute; Metzl, Nicolas; Yoshikawa-Inoue, Hisayuki; Ishii, Masao; Midorikawa, Takashi; Nojiri, Yukihiro; Körtzinger, Arne; Steinhoff, Tobias; Hoppema, Mario; Olafsson, Jon; Arnarson, Thorarinn S.; Tilbrook, Bronte; Johannessen, Truls; Olsen, Are; Bellerby, Richard; Wong, C. S.; Delille, Bruno; Bates, N. R.; de Baar, Hein J. W.

    2009-04-01

    A climatological mean distribution for the surface water pCO 2 over the global oceans in non-El Niño conditions has been constructed with spatial resolution of 4° (latitude) ×5° (longitude) for a reference year 2000 based upon about 3 million measurements of surface water pCO 2 obtained from 1970 to 2007. The database used for this study is about 3 times larger than the 0.94 million used for our earlier paper [Takahashi et al., 2002. Global sea-air CO 2 flux based on climatological surface ocean pCO 2, and seasonal biological and temperature effects. Deep-Sea Res. II, 49, 1601-1622]. A time-trend analysis using deseasonalized surface water pCO 2 data in portions of the North Atlantic, North and South Pacific and Southern Oceans (which cover about 27% of the global ocean areas) indicates that the surface water pCO 2 over these oceanic areas has increased on average at a mean rate of 1.5 μatm y -1 with basin-specific rates varying between 1.2±0.5 and 2.1±0.4 μatm y -1. A global ocean database for a single reference year 2000 is assembled using this mean rate for correcting observations made in different years to the reference year. The observations made during El Niño periods in the equatorial Pacific and those made in coastal zones are excluded from the database. Seasonal changes in the surface water pCO 2 and the sea-air pCO 2 difference over four climatic zones in the Atlantic, Pacific, Indian and Southern Oceans are presented. Over the Southern Ocean seasonal ice zone, the seasonality is complex. Although it cannot be thoroughly documented due to the limited extent of observations, seasonal changes in pCO 2 are approximated by using the data for under-ice waters during austral winter and those for the marginal ice and ice-free zones. The net air-sea CO 2 flux is estimated using the sea-air pCO 2 difference and the air-sea gas transfer rate that is parameterized as a function of (wind speed) 2 with a scaling factor of 0.26. This is estimated by inverting

  13. Effect of Sampling Depth on Air-Sea CO2 Flux Estimates in River-Stratified Arctic Coastal Waters

    NASA Astrophysics Data System (ADS)

    Miller, L. A.; Papakyriakou, T. N.

    2015-12-01

    In summer-time Arctic coastal waters that are strongly influenced by river run-off, extreme stratification severely limits wind mixing, making it difficult to effectively sample the surface 'mixed layer', which can be as shallow as 1 m, from a ship. During two expeditions in southwestern Hudson Bay, off the Nelson, Hayes, and Churchill River estuaries, we confirmed that sampling depth has a strong impact on estimates of 'surface' pCO2 and calculated air-sea CO2 fluxes. We determined pCO2 in samples collected from 5 m, using a typical underway system on the ship's seawater supply; from the 'surface' rosette bottle, which was generally between 1 and 3 m; and using a niskin bottle deployed at 1 m and just below the surface from a small boat away from the ship. Our samples confirmed that the error in pCO2 derived from typical ship-board versus small-boat sampling at a single station could be nearly 90 μatm, leading to errors in the calculated air-sea CO2 flux of more than 0.1 mmol/(m2s). Attempting to extrapolate such fluxes over the 6,000,000 km2 area of the Arctic shelves would generate an error approaching a gigamol CO2/s. Averaging the station data over a cruise still resulted in an error of nearly 50% in the total flux estimate. Our results have implications not only for the design and execution of expedition-based sampling, but also for placement of in-situ sensors. Particularly in polar waters, sensors are usually deployed on moorings, well below the surface, to avoid damage and destruction from drifting ice. However, to obtain accurate information on air-sea fluxes in these areas, it is necessary to deploy sensors on ice-capable buoys that can position the sensors in true 'surface' waters.

  14. Air-sea CO2 flux pattern along the southern Bay of Bengal waters

    NASA Astrophysics Data System (ADS)

    Shanthi, R.; Poornima, D.; Naveen, M.; Thangaradjou, T.; Choudhury, S. B.; Rao, K. H.; Dadhwal, V. K.

    2016-12-01

    Physico-chemical observations made from January 2013 to March 2015 in coastal waters of the southwest Bay of Bengal show pronounced seasonal variation in physico-chemical parameters including total alkalinity (TA: 1927.390-4088.642 μmol kg-1), chlorophyll (0.13-19.41 μg l-1) and also calculated dissolved inorganic carbon (DIC: 1574.219-3790.954 μmol kg-1), partial pressure of carbon dioxide (pCO2: 155.520-1488.607 μatm) and air-sea CO2 flux (FCO2: -4.808 to 11.255 mmol Cm-2 d-1). Most of the physical parameters are at their maximum during summer due to the increased solar radiation at cloud free conditions, less or no riverine inputs, and lack of vertical mixing of water column which leads to the lowest nutrients concentration, dissolved oxygen (DO), biological production, pCO2 and negative flux of CO2 to the atmosphere. Chlorophyll and DO concentrations enhanced due to increased nutrients during premonsoon and monsoon season due to the vertical mixing of water column driven by the strong winds and external inputs at respective seasons. The constant positive loading of nutrients, TA, DIC, chlorophyll, pCO2 and FCO2 against atmospheric temperature (AT), lux, sea surface temperature (SST), pH and salinity observed in principal component analysis (PCA) suggested that physical and biological parameters play vital role in the seasonal distribution of pCO2 along the southwest Bay of Bengal. The annual variability of CO2 flux clearly depicted that the southwest Bay of Bengal switch from sink (2013) to source status in the recent years (2014 and 2015) and it act as significant source of CO2 to the atmosphere with a mean flux of 0.204 ± 1.449 mmol Cm-2 d-1.

  15. Comparison of Sea-Air CO2 Flux Estimates Using Satellite-Based Versus Mooring Wind Speed Data

    NASA Astrophysics Data System (ADS)

    Sutton, A. J.; Sabine, C. L.; Feely, R. A.; Wanninkhof, R. H.

    2016-12-01

    The global ocean is a major sink of anthropogenic CO2, absorbing approximately 27% of CO2 emissions since the beginning of the industrial revolution. Any variation or change in the ocean CO2 sink has implications for future climate. Observations of sea-air CO2 flux have relied primarily on ship-based underway measurements of partial pressure of CO2 (pCO2) combined with satellite, model, or multi-platform wind products. Direct measurements of ΔpCO2 (seawater - air pCO2) and wind speed from moored platforms now allow for high-resolution CO2 flux time series. Here we present a comparison of CO2 flux calculated from moored ΔpCO2 measured on four moorings in different biomes of the Pacific Ocean in combination with: 1) Cross-Calibrated Multi-Platform (CCMP) winds or 2) wind speed measurements made on ocean reference moorings excluded from the CCMP dataset. Preliminary results show using CCMP winds overestimates CO2 flux on average by 5% at the Kuroshio Extension Observatory, Ocean Station Papa, WHOI Hawaii Ocean Timeseries Station, and Stratus. In general, CO2 flux seasonality follows patterns of seawater pCO2 and SST with periods of CO2 outgassing during summer and CO2 uptake during winter at these locations. Any offsets or seasonal biases in CCMP winds could impact global ocean sink estimates using this data product. Here we present patterns and trends between the two CO2 flux estimates and discuss the potential implications for tracking variability and change in global ocean CO2 uptake.

  16. Surface Ocean pCO2 Seasonality and Sea-Air CO2 Flux Estimates for the North American East Coast

    NASA Technical Reports Server (NTRS)

    Signorini, Sergio; Mannino, Antonio; Najjar, Raymond G., Jr.; Friedrichs, Marjorie A. M.; Cai, Wei-Jun; Salisbury, Joe; Wang, Zhaohui Aleck; Thomas, Helmuth; Shadwick, Elizabeth

    2013-01-01

    Underway and in situ observations of surface ocean pCO2, combined with satellite data, were used to develop pCO2 regional algorithms to analyze the seasonal and interannual variability of surface ocean pCO2 and sea-air CO2 flux for five physically and biologically distinct regions of the eastern North American continental shelf: the South Atlantic Bight (SAB), the Mid-Atlantic Bight (MAB), the Gulf of Maine (GoM), Nantucket Shoals and Georges Bank (NS+GB), and the Scotian Shelf (SS). Temperature and dissolved inorganic carbon variability are the most influential factors driving the seasonality of pCO2. Estimates of the sea-air CO2 flux were derived from the available pCO2 data, as well as from the pCO2 reconstructed by the algorithm. Two different gas exchange parameterizations were used. The SS, GB+NS, MAB, and SAB regions are net sinks of atmospheric CO2 while the GoM is a weak source. The estimates vary depending on the use of surface ocean pCO2 from the data or algorithm, as well as with the use of the two different gas exchange parameterizations. Most of the regional estimates are in general agreement with previous studies when the range of uncertainty and interannual variability are taken into account. According to the algorithm, the average annual uptake of atmospheric CO2 by eastern North American continental shelf waters is found to be between 3.4 and 5.4 Tg C/yr (areal average of 0.7 to 1.0 mol CO2 /sq m/yr) over the period 2003-2010.

  17. Seasonal and spatial variations in surface pCO2 and air-sea CO2 flux in the Chesapeake Bay

    NASA Astrophysics Data System (ADS)

    Cai, W. J.; Chen, B.

    2017-12-01

    Bay-wide observations of surface water partial pressure of carbon dioxide (pCO2) were conducted in May, June, August, and October 2016 to study the spatial and seasonal variations in surface pCO2 and to estimate air-sea CO2 flux in the Chesapeake Bay. Overall, high surface pCO2 in the upper-bay decreased downstream rapidly below the atmospheric value near the bay bridge in the mid-bay and then increased slightly to the lower-bay where pCO2 approached the atmospheric level. Over the course of a year, pCO2 was higher than 1000 µatm in the upper bay and the highest pCO2 (2500 µatm) was observed in August. Significant biologically-induced pCO2 undersaturation was observed at the upper part of the mid-bay in August with pCO2 as low as 50 µatm and oversaturated DO% of 200%. In addition to biological control, vertical mixing and upwelling controlled by wind direction and tidal stage played an important role in controlling surface pCO2 in the mid-bay as is evidenced by co-occurrence of high pCO2 with low temperature and low oxygen or high salinity from the subsurface. These physical processes occurred regularly and in short time scale of hours, suggesting they must be considered in the assessment of annual air-sea CO2 flux. Seasonally, the upper-bay acted as a source for atmospheric CO2 over the course of a year. The boundary of upper and mid bay transited from a CO2 source to a sink from May to August and was a source again in October due to strong biological production in summer. In contrast, the mid-bay represented as a CO2 source with large temporal variation due to dynamic hydrographic settings. The lower-bay transited from a weak sink in May to equilibrated with the atmosphere from June to August, while became a source again in October. Moreover, the CO2 flux could be reversed very quickly under episodic severe weather events. Thus further research, including the influence of severe weather and subsequent bloom, is needed to get better understanding of the carbon

  18. Net sea-air CO2 fluxes and modelled pCO2 in the southwestern subtropical Atlantic continental shelf during spring 2010 and summer 2011

    NASA Astrophysics Data System (ADS)

    Ito, Rosane Gonçalves; Garcia, Carlos Alberto Eiras; Tavano, Virginia Maria

    2016-05-01

    Sea-air CO2 fluxes over continental shelves vary substantially in time on both seasonal and sub-seasonal scales, driven primarily by variations in surface pCO2 due to several oceanic mechanisms. Furthermore, coastal zones have not been appropriately considered in global estimates of sea-air CO2 fluxes, despite their importance to ecology and to productivity. In this work, we aimed to improve our understanding of the role played by shelf waters in controlling sea-air CO2 fluxes by investigating the southwestern Atlantic Ocean (21-35°S) region, where physical, chemical and biological measurements were made on board the Brazilian R. V. Cruzeiro do Sul during late spring 2010 and early summer 2011. Features such as discharge from the La Plata River, intrusions of tropical waters on the outer shelf due to meandering and flow instabilities of the Brazil Current, and coastal upwelling in the Santa Marta Grande Cape and São Tomé Cape were detected by both in situ measurements and ocean colour and thermal satellite imagery. Overall, shelf waters in the study area were a source of CO2 to the atmosphere, with an average of 1.2 mmol CO2 m-2 day-1 for the late spring and 11.2 mmol CO2 m-2 day-1 for the early summer cruises. The spatial variability in ocean pCO2 was associated with surface ocean properties (temperature, salinity and chlorophyll-a concentration) in both the slope and shelf waters. Empirical algorithms for predicting temperature-normalized surface ocean pCO2 as a function of surface ocean properties were shown to perform well in both shelf and slope waters, except (a) within cyclonic eddies produced by baroclinic instability of the Brazil Current as detected by satellite SST imagery and (b) in coastal upwelling regions. In these regions, surface ocean pCO2 values were higher as a result of upwelled CO2-enriched subsurface waters. Finally, a pCO2 algorithm based on both sea surface temperature and surface chlorophyll-a was developed that enabled the spatial

  19. Temporal variability of air-sea CO2 exchange in a low-emission estuary

    NASA Astrophysics Data System (ADS)

    Mørk, Eva Thorborg; Sejr, Mikael Kristian; Stæhr, Peter Anton; Sørensen, Lise Lotte

    2016-07-01

    There is the need for further study of whether global estimates of air-sea CO2 exchange in estuarine systems capture the relevant temporal variability and, as such, the temporal variability of bulk parameterized and directly measured CO2 fluxes was investigated in the Danish estuary, Roskilde Fjord. The air-sea CO2 fluxes showed large temporal variability across seasons and between days and that more than 30% of the net CO2 emission in 2013 was a result of two large fall and winter storms. The diurnal variability of ΔpCO2 was up to 400 during summer changing the estuary from a source to a sink of CO2 within the day. Across seasons the system was suggested to change from a sink of atmospheric CO2 during spring to near neutral during summer and later to a source of atmospheric CO2 during fall. Results indicated that Roskilde Fjord was an annual low-emission estuary, with an estimated bulk parameterized release of 3.9 ± 8.7 mol CO2 m-2 y-1 during 2012-2013. It was suggested that the production-respiration balance leading to the low annual emission in Roskilde Fjord, was caused by the shallow depth, long residence time and high water quality in the estuary. In the data analysis the eddy covariance CO2 flux samples were filtered according to the H2Osbnd CO2 cross-sensitivity assessment suggested by Landwehr et al. (2014). This filtering reduced episodes of contradicting directions between measured and bulk parameterized air-sea CO2 exchanges and changed the net air-sea CO2 exchange from an uptake to a release. The CO2 gas transfer velocity was calculated from directly measured CO2 fluxes and ΔpCO2 and agreed to previous observations and parameterizations.

  20. Coccolithophore surface distributions in the North Atlantic and their modulation of the air-sea flux of CO2 from 10 years of satellite Earth observation data

    NASA Astrophysics Data System (ADS)

    Shutler, J. D.; Land, P. E.; Brown, C. W.; Findlay, H. S.; Donlon, C. J.; Medland, M.; Snooke, R.; Blackford, J. C.

    2013-04-01

    Coccolithophores are the primary oceanic phytoplankton responsible for the production of calcium carbonate (CaCO3). These climatically important plankton play a key role in the oceanic carbon cycle as a major contributor of carbon to the open ocean carbonate pump (~50%) and their calcification can affect the atmosphere-to-ocean (air-sea) uptake of carbon dioxide (CO2) through increasing the seawater partial pressure of CO2 (pCO2). Here we document variations in the areal extent of surface blooms of the globally important coccolithophore, Emiliania huxleyi, in the North Atlantic over a 10-year period (1998-2007), using Earth observation data from the Sea-viewing Wide Field-of-view Sensor (SeaWiFS). We calculate the annual mean sea surface areal coverage of E. huxleyi in the North Atlantic to be 474 000 ± 104 000 km2, which results in a net CaCO3 carbon (CaCO3-C) production of 0.14-1.71 Tg CaCO3-C per year. However, this surface coverage (and, thus, net production) can fluctuate inter-annually by -54/+8% about the mean value and is strongly correlated with the El Niño/Southern Oscillation (ENSO) climate oscillation index (r=0.75, p<0.02). Our analysis evaluates the spatial extent over which the E. huxleyi blooms in the North Atlantic can increase the pCO2 and, thus, decrease the localised air-sea flux of atmospheric CO2. In regions where the blooms are prevalent, the average reduction in the monthly air-sea CO2 flux can reach 55%. The maximum reduction of the monthly air-sea CO2 flux in the time series is 155%. This work suggests that the high variability, frequency and distribution of these calcifying plankton and their impact on pCO2 should be considered if we are to fully understand the variability of the North Atlantic air-to-sea flux of CO2. We estimate that these blooms can reduce the annual N. Atlantic net sink atmospheric CO2 by between 3-28%.

  1. The impact of changing wind speeds on gas transfer and its effect on global air-sea CO2 fluxes

    NASA Astrophysics Data System (ADS)

    Wanninkhof, R.; Triñanes, J.

    2017-06-01

    An increase in global wind speeds over time is affecting the global uptake of CO2 by the ocean. We determine the impact of changing winds on gas transfer and CO2 uptake by using the recently updated, global high-resolution, cross-calibrated multiplatform wind product (CCMP-V2) and a fixed monthly pCO2 climatology. In particular, we assess global changes in the context of regional wind speed changes that are attributed to large-scale climate reorganizations. The impact of wind on global CO2 gas fluxes as determined by the bulk formula is dependent on several factors, including the functionality of the gas exchange-wind speed relationship and the regional and seasonal differences in the air-water partial pressure of CO2 gradient (ΔpCO2). The latter also controls the direction of the flux. Fluxes out of the ocean are influenced more by changes in the low-to-intermediate wind speed range, while ingassing is impacted more by changes in higher winds because of the regional correlations between wind and ΔpCO2. Gas exchange-wind speed parameterizations with a quadratic and third-order polynomial dependency on wind, each of which meets global constraints, are compared. The changes in air-sea CO2 fluxes resulting from wind speed trends are greatest in the equatorial Pacific and cause a 0.03-0.04 Pg C decade-1 increase in outgassing over the 27 year time span. This leads to a small overall decrease of 0.00 to 0.02 Pg C decade-1 in global net CO2 uptake, contrary to expectations that increasing winds increase net CO2 uptake.Plain Language SummaryThe effects of changing winds are isolated from the total change in trends in global <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> over the last 27 years. The overall effect of increasing winds over time has a smaller impact than expected as the impact in regions of outgassing is greater than for the regions acting as a <span class="hlt">CO</span><span class="hlt">2</span> sink.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.8634D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.8634D"><span>Interannual variability of primary production and <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> in the Atlantic and Indian sectors of the Southern Ocean.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dufour, Carolina; Merlivat, Liliane; Le Sommer, Julien; Boutin, Jacqueline; Antoine, David</p> <p>2013-04-01</p> <p>As one of the major oceanic sinks of anthropogenic <span class="hlt">CO</span><span class="hlt">2</span>, the Southern Ocean plays a critical role in the climate system. However, due to the scarcity of observations, little is known about physical and biological processes that control <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> and how these processes might respond to climate change. It is well established that primary production is one of the major drivers of <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>, consuming surface Dissolved Inorganic Carbon (DIC) during Summer. Southern Ocean primary production is though constrained by several limiting factors such as iron and light availability, which are both sensitive to mixed layer depth. Mixed layer depth is known to be affected by current changes in wind stress or freshwater <span class="hlt">fluxes</span> over the Southern Ocean. But we still don't know how primary production may respond to anomalous mixed layer depth neither how physical processes may balance this response to set the seasonal cycle of <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. In this study, we investigate the impact of anomalous mixed layer depth on surface DIC in the Atlantic and Indian sectors of the Subantarctic zone of the Southern Ocean (60W-60E, 38S-55S) with a combination of in situ data, satellite data and model experiment. We use both a regional eddy permitting ocean biogeochemical model simulation based on NEMO-PISCES and data-based reconstruction of biogeochemical fields based on CARIOCA buoys and <span class="hlt">Sea</span>WiFS data. A decomposition of the physical and biological processes driving the seasonal variability of surface DIC is performed with both the model data and observations. A good agreement is found between the model and the data for the amplitude of biological and <span class="hlt">air-sea</span> <span class="hlt">flux</span> contributions. The model data are further used to investigate the impact of winter and summer anomalies in mixed layer depth on surface DIC over the period 1990-2004. The relative changes of each physical and biological process contribution are quantified and discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JMS...140...26M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JMS...140...26M"><span>Spatio-temporal dynamics of biogeochemical processes and <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in the Western English Channel based on two years of FerryBox deployment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marrec, P.; Cariou, T.; Latimier, M.; Macé, E.; Morin, P.; Vernet, M.; Bozec, Y.</p> <p>2014-12-01</p> <p>From January 2011 to January 2013, a FerryBox system was installed on a Voluntary Observing Ship (VOS), which crossed the Western English Channel (WEC) between Roscoff (France) and Plymouth (UK) up to 3 times a day. The FerryBox continuously measured <span class="hlt">sea</span> surface temperature (SST), <span class="hlt">sea</span> surface salinity (SSS), dissolved oxygen (DO), fluorescence and partial pressure of <span class="hlt">CO</span><span class="hlt">2</span> (from April 2012) along the ferry track. Sensors were calibrated based on 714 bimonthly surface samplings with precisions of 0.016 for SSS, 3.3 μM for DO, 0.40 μg L- 1 for Chlorophyll-a (Chl-a) (based on fluorescence measurements) and 5.<span class="hlt">2</span> μatm for p<span class="hlt">CO</span><span class="hlt">2</span>. Over the <span class="hlt">2</span> years of deployment (900 crossings), we reported 9% of data lost due to technical issues and quality checked data was obtained to allow investigation of the dynamics of biogeochemical processes related to <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in the WEC. Based on this unprecedented high-frequency dataset, the physical structure of the WEC was assessed using SST anomalies and the presence of a thermal front was observed around the latitude 49.5°N, which divided the WEC in two main provinces: the seasonally stratified northern WEC (nWEC) and the all-year well-mixed southern WEC (sWEC). These hydrographical properties strongly influenced the spatial and inter-annual distributions of phytoplankton blooms, which were mainly limited by nutrients and light availability in the nWEC and the sWEC, respectively. <span class="hlt">Air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> were also highly related to hydrographical properties of the WEC between late April and early September 2012, with the sWEC a weak source of <span class="hlt">CO</span><span class="hlt">2</span> to the atmosphere of 0.9 mmol m- <span class="hlt">2</span> d- 1, whereas the nWEC acted as a sink for atmospheric <span class="hlt">CO</span><span class="hlt">2</span> of 6.9 mmol m- <span class="hlt">2</span> d- 1. The study of short time-scale dynamics of <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> revealed that an intense and short (less than 10 days) summer bloom in the nWEC contributed to 29% of the <span class="hlt">CO</span><span class="hlt">2</span> sink during the productive period, highlighting the necessity for high frequency observations in coastal</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMOS33A1448Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMOS33A1448Z"><span>Seasonal variation of <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in the Terra Nova Bay of the Ross <span class="hlt">Sea</span>, Antarctica, based on year-round p<span class="hlt">CO</span><span class="hlt">2</span> observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zappa, C. J.; Rhee, T. S.; Kwon, Y. S.; Choi, T.; Yang, E. J.; Kim, J.</p> <p>2017-12-01</p> <p>The polar oceans are rapidly changing in response to climate variability. In particular, augmented inflow of glacial melt water and shrinking <span class="hlt">sea</span>-ice extent impacts the polar coastal oceans, which may in turn shift the biogeochemistry into an unprecedented paradigm not experienced previously. Nonetheless, most research in the polar oceans is limited to the summer season. Here, we present the first direct observations of ocean and atmospheric p<span class="hlt">CO</span><span class="hlt">2</span> measured near the coast of Terra Nova Bay in the Ross <span class="hlt">Sea</span>, Antarctica, ongoing since February, 2015 at Jang Bogo Station. The coastal area is covered by landfast <span class="hlt">sea</span>-ice from spring to fall while continually exposed to the atmosphere during summer season only. The p<span class="hlt">CO</span><span class="hlt">2</span> in seawater swung from 120 matm in February to 425 matm in early October. Although <span class="hlt">sea</span>-ice still covers the coastal area, p<span class="hlt">CO</span><span class="hlt">2</span> already started decreasing after reaching the peak in October. In November, the p<span class="hlt">CO</span><span class="hlt">2</span> suddenly dropped as much as 100 matm in a week. This decrease of p<span class="hlt">CO</span><span class="hlt">2</span> continued until late February when the <span class="hlt">sea</span>-ice concentration was minimal. With growing <span class="hlt">sea</span> ice, the p<span class="hlt">CO</span><span class="hlt">2</span> increased logarithmically reaching the atmospheric concentration in June/July, depending on the year, and continued to increase until October. Daily mean <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> in the coastal area widely varied from -70 mmol m-<span class="hlt">2</span> d-1 to 20 mmol m-<span class="hlt">2</span> d-1. Based on these observations of p<span class="hlt">CO</span><span class="hlt">2</span> in Terra Nova Bay, the annual uptake of <span class="hlt">CO</span><span class="hlt">2</span> is 8 g C m-<span class="hlt">2</span>, estimated using the fraction of <span class="hlt">sea</span>-ice concentration estimated from AMSR<span class="hlt">2</span> microwave emission imagery. Extrapolating to all polynyas surrounding Antarctica, we expect the annual uptake of 8 Tg C in the atmosphere. This is comparable to the amount of <span class="hlt">CO</span><span class="hlt">2</span> degassed into the atmosphere south of the Antarctic Polar Front (62°S).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..14..742J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..14..742J"><span>In situ evaluation of <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> gas transfer velocity in an inner estuary using eddy covariance - with a special focus on the importance of using reliable <span class="hlt">CO</span><span class="hlt">2</span>-<span class="hlt">fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jørgensen, E. T.; Sørensen, L. L.; Jensen, B.; Sejr, M. K.</p> <p>2012-04-01</p> <p>The <span class="hlt">air-sea</span> exchange of <span class="hlt">CO</span><span class="hlt">2</span> or <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> is driven by the difference in the partial pressure of <span class="hlt">CO</span><span class="hlt">2</span> in the water and the atmosphere (Δp<span class="hlt">CO</span><span class="hlt">2</span>), the solubility of <span class="hlt">CO</span><span class="hlt">2</span> (K0) and the gas transfer velocity (k) (Wanninkhof et al., 2009;Weiss, 1974) . Δp<span class="hlt">CO</span><span class="hlt">2</span> and K0 are determined with relatively high precision and it is estimated that the biggest uncertainty when modelling the <span class="hlt">air-sea</span> <span class="hlt">flux</span> is the parameterization of k. As an example; the estimated global <span class="hlt">air-sea</span> <span class="hlt">flux</span> increases by 70 % when using the parameterization by Wanninkhof and McGillis (1999) instead of Wanninkhof (1992) (Rutgersson et al., 2008). In coastal areas the uncertainty is even higher and only few studies have focused on determining transfer velocity for the coastal waters and even fewer on estuaries (Borges et al., 2004;Rutgersson et al., 2008). The transfer velocity (k600) of <span class="hlt">CO</span><span class="hlt">2</span> in the inner estuary of Roskilde Fjord, Denmark was investigated using eddy covariance <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> (ECM) and directly measured Δp<span class="hlt">CO</span><span class="hlt">2</span> during May and June 2010. The data was strictly sorted to heighten the certainty of the results and the outcome was; DS1; using only ECM, and DS<span class="hlt">2</span>; including the inertial dissipation method (IDM). The inner part of Roskilde Fjord showed to be a very biological active <span class="hlt">CO</span><span class="hlt">2</span> sink and preliminary results showed that the average k600 was more than 10 times higher than transfer velocities from similar studies of other coastal areas. The much higher transfer velocities were estimated to be caused by the greater fetch and shallower water in Roskilde Fjord, which indicated that turbulence in both <span class="hlt">air</span> and water influence k600. The wind speed parameterization of k600 using DS1 showed some scatter but when including IDM the r<span class="hlt">2</span> of DS<span class="hlt">2</span> reached 0.93 with an exponential parameterization, where U10 was based on the Businger-Dyer relationships using friction velocity and atmospheric stability. This indicates that some of the uncertainties coupled with <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> calculated by the ECM are removed when including the IDM.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMOS33A1443Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMOS33A1443Y"><span>Diagnosing <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> and seasonality in the Arabian <span class="hlt">Sea</span> as an Ocean-Dominated Margin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, W.; Dai, M.</p> <p>2017-12-01</p> <p>The Arabian <span class="hlt">Sea</span> is a large marginal <span class="hlt">sea</span> of the Indian Ocean characterized by highly predictable annual circulation cycle driven by Asian monsoon. The Arabian <span class="hlt">Sea</span> is generally sources to atmospheric <span class="hlt">CO</span><span class="hlt">2</span>. In this study, we applied the physical-biogeochemical coupled approach previously adopted for diagnosis of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in Ocean-dominated margin (OceMar) to assesses the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> and their seasonality in Arabian <span class="hlt">Sea</span> using data collected during five US JGOFS Arabian <span class="hlt">Sea</span> Process Study cruises (ttn-043, ttn-045, ttn-049, ttn-053, ttn-054) conducted from September 1994 to December 1995. The p<span class="hlt">CO</span><span class="hlt">2</span> estimated during the 5 cruises was 396±5μatm, 359±7 μatm, 373±7 μatm, 379±9 μatm and 387±12 μatm, respectively, which agreed well with the p<span class="hlt">CO</span><span class="hlt">2</span> observed during the cruises of 389±8 μatm, 361±6 μatm, 366±6 μatm, 371±8 μatm and 367±11 μatm from underway measurements. This strongly suggests that our semi-analytical diagnostic approach in the OceMar framework can evaluate the p<span class="hlt">CO</span><span class="hlt">2</span> in Arabian <span class="hlt">Sea</span>. Our coupled diagnostic approach assumes that water mass mixing, biological response and <span class="hlt">air-sea</span> exchange under steady state over a similar time scale. This assumption should be justified at the region with intensified upwelling where decoupling between upwelling and biological response may occur, where only water mass mixing and <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange should be accounted for. This presentation will also examine the seasonality of the <span class="hlt">CO</span><span class="hlt">2</span> dynamics and its controls.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013BGD....1015641F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013BGD....1015641F"><span>Synoptic evaluation of carbon cycling in Beaufort <span class="hlt">Sea</span> during summer: contrasting river inputs, ecosystem metabolism and <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Forest, A.; Coupel, P.; Else, B.; Nahavandian, S.; Lansard, B.; Raimbault, P.; Papakyriakou, T.; Gratton, Y.; Fortier, L.; Tremblay, J.-É.; Babin, M.</p> <p>2013-10-01</p> <p>The accelerated decline in Arctic <span class="hlt">sea</span> ice combined with an ongoing trend toward a more dynamic atmosphere is modifying carbon cycling in the Arctic Ocean. A critical issue is to understand how net community production (NCP; the balance between gross primary production and community respiration) responds to changes and modulates <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. Using data collected as part of the ArcticNet-Malina 2009 expedition in southeastern Beaufort <span class="hlt">Sea</span> (Arctic Ocean), we synthesize information on <span class="hlt">sea</span> ice, wind, river, water column properties, metabolism of the planktonic food web, organic carbon <span class="hlt">fluxes</span> and pools, as well as <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange, with the aim of identifying indices of ecosystem response to environmental changes. Data were analyzed to develop a non-steady-state carbon budget and an assessment of NCP against <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. The mean atmospheric forcing was a mild upwelling-favorable wind (~5 km h-1) blowing from the N-E and a decaying ice cover (<80% concentration) was observed beyond the shelf, the latter being fully exposed to the atmosphere. We detected some areas where the surface mixed layer was net autotrophic owing to high rates of primary production (PP), but the ecosystem was overall net heterotrophic. The region acted nonetheless as a sink for atmospheric <span class="hlt">CO</span><span class="hlt">2</span> with a mean uptake rate of -<span class="hlt">2</span>.0 ± 3.3 mmol C m-<span class="hlt">2</span>d-1. We attribute this discrepancy to: (1) elevated PP rates (>600 mg C m-<span class="hlt">2</span>d-1) over the shelf prior to our survey, (<span class="hlt">2</span>) freshwater dilution by river runoff and ice melt, and (3) the presence of cold surface waters offshore. Only the Mackenzie River delta and localized shelf areas directly affected by upwelling were identified as substantial sources of <span class="hlt">CO</span><span class="hlt">2</span> to the atmosphere (>10mmol C m-<span class="hlt">2</span>d-1). Although generally <100 mg C m-<span class="hlt">2</span>d-1, daily PP rates cumulated to a total PP of ~437.6 × 103 t C, which was roughly twice higher than the organic carbon delivery by river inputs (~241.<span class="hlt">2</span> × 103 t C). Subsurface PP represented 37.4% of total PP for the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16..583M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16..583M"><span>Dynamics of <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> based on FerryBox measurements and satellite-based prediction of p<span class="hlt">CO</span><span class="hlt">2</span> in the Western English Channel</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marrec, Pierre; Thierry, Cariou; Eric, Mace; Pascal, Morin; Marc, Vernet; Yann, Bozec</p> <p>2014-05-01</p> <p>Since April 2012, we installed an autonomous FerryBox system on a Voluntary Observing Ship (VOS), which crosses the Western English Channel (WEC) between Roscoff and Plymouth on a daily basis. High-frequency data of <span class="hlt">sea</span> surface temperature (SST), salinity (SSS), fluorescence, dissolved oxygen (DO) and partial pressure of <span class="hlt">CO</span><span class="hlt">2</span> (p<span class="hlt">CO</span><span class="hlt">2</span>) were recorded for two years across the all-year mixed southern WEC (sWEC) and the seasonally stratified northern WEC (nWEC). These contrasting hydrographical provinces strongly influenced the spatio-temporal distributions of p<span class="hlt">CO</span><span class="hlt">2</span> and <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. During the productive period (from May to September), the nWEC acted as a sink for atmospheric <span class="hlt">CO</span><span class="hlt">2</span> of -5.6 mmolC m-<span class="hlt">2</span> d-1 and -4.6 mmolC m-<span class="hlt">2</span> d-1, in 2012 and 2013, respectively. During the same period, the sWEC showed significant inter-annual variability degassing <span class="hlt">CO</span><span class="hlt">2</span> to the atmosphere in 2012 (1.4 mmolC m-<span class="hlt">2</span> d-1) and absorbing atmospheric <span class="hlt">CO</span><span class="hlt">2</span> in 2013 (-1.6 mmolC m-<span class="hlt">2</span> d-1). In 2012, high-frequency data revealed that an intense and short (less than 10 days) summer phytoplankton bloom in the nWEC contributed to 31% of the total <span class="hlt">CO</span><span class="hlt">2</span> drawdown during the productive period, highlighting the necessity of p<span class="hlt">CO</span><span class="hlt">2</span> high-frequency measurements in coastal ecosystems. Based on this multi-annual dataset, we developed p<span class="hlt">CO</span><span class="hlt">2</span> algorithms using multiple linear regression (MLR) based on SST, SSS, chlorophyll-a (Chl-a) concentration, time, latitude and mixed layer depth to predict p<span class="hlt">CO</span><span class="hlt">2</span> in the two hydrographical provinces of the WEC. MLR were performed based on more than 200,000 underway observations spanning the range from 150 to 480 µatm. The root mean square errors (RMSE) of the MLR fit to the data were 17.<span class="hlt">2</span> µatm and 21.5 µatm for the s WEC and the nWEC with correlation coefficient (r²) of 0.71 and 0.79, respectively. We applied these algorithms to satellite SST and Chl-a products and to modeled SSS estimates in the entire WEC. Based on these high-frequency and satellite approaches, we will discuss the main</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014BGeo...11.2827F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014BGeo...11.2827F"><span>Synoptic evaluation of carbon cycling in the Beaufort <span class="hlt">Sea</span> during summer: contrasting river inputs, ecosystem metabolism and <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Forest, A.; Coupel, P.; Else, B.; Nahavandian, S.; Lansard, B.; Raimbault, P.; Papakyriakou, T.; Gratton, Y.; Fortier, L.; Tremblay, J.-É.; Babin, M.</p> <p>2014-05-01</p> <p>The accelerated decline in Arctic <span class="hlt">sea</span> ice and an ongoing trend toward more energetic atmospheric and oceanic forcings are modifying carbon cycling in the Arctic Ocean. A critical issue is to understand how net community production (NCP; the balance between gross primary production and community respiration) responds to changes and modulates <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. Using data collected as part of the ArcticNet-Malina 2009 expedition in the southeastern Beaufort <span class="hlt">Sea</span> (Arctic Ocean), we synthesize information on <span class="hlt">sea</span> ice, wind, river, water column properties, metabolism of the planktonic food web, organic carbon <span class="hlt">fluxes</span> and pools, as well as <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange, with the aim of documenting the ecosystem response to environmental changes. Data were analyzed to develop a non-steady-state carbon budget and an assessment of NCP against <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. During the field campaign, the mean wind field was a mild upwelling-favorable wind (~ 5 km h-1) from the NE. A decaying ice cover (< 80% concentration) was observed beyond the shelf, the latter being fully exposed to the atmosphere. We detected some areas where the surface mixed layer was net autotrophic owing to high rates of primary production (PP), but the ecosystem was overall net heterotrophic. The region acted nonetheless as a sink for atmospheric <span class="hlt">CO</span><span class="hlt">2</span>, with an uptake rate of -<span class="hlt">2</span>.0 ± 3.3 mmol C m-<span class="hlt">2</span> d-1 (mean ± standard deviation associated with spatial variability). We attribute this discrepancy to (1) elevated PP rates (> 600 mg C m-<span class="hlt">2</span> d-1) over the shelf prior to our survey, (<span class="hlt">2</span>) freshwater dilution by river runoff and ice melt, and (3) the presence of cold surface waters offshore. Only the Mackenzie River delta and localized shelf areas directly affected by upwelling were identified as substantial sources of <span class="hlt">CO</span><span class="hlt">2</span> to the atmosphere (> 10 mmol C m-<span class="hlt">2</span> d-1). Daily PP rates were generally < 100 mg C m-<span class="hlt">2</span> d-1 and cumulated to a total PP of ~ 437.6 × 103 t C for the region over a 35-day period. This amount was about twice the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JMS...173...70C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JMS...173...70C"><span><span class="hlt">Air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> for the Brazilian northeast continental shelf in a climatic transition region</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carvalho, A. C. O.; Marins, R. V.; Dias, F. J. S.; Rezende, C. E.; Lefèvre, N.; Cavalcante, M. S.; Eschrique, S. A.</p> <p>2017-09-01</p> <p>Oceanographic cruises were carried out in October 2012 (3°S-5°S and 38,5°W-35,5°W) and in September 2014 (1°S-4°S and 43°W-37°W), measuring atmospheric and <span class="hlt">sea</span> surface <span class="hlt">CO</span><span class="hlt">2</span> fugacity (f<span class="hlt">CO</span><span class="hlt">2</span>) underway in the northeast coast of Brazil. <span class="hlt">Sea</span> surface water samples were also collected for chlorophyll a, nutrients and DOC analysis. During the second cruise, the sampling area covered a transition between semi-arid to more humid areas of the coast, with different hydrologic and rainfall regimes. The seawater f<span class="hlt">CO</span><span class="hlt">2</span>sw, in October 2012, was in average 400.9 ± 7.3μatm and 391.1 ± 6.3 μatm in September 2014. For the atmosphere, the f<span class="hlt">CO</span><span class="hlt">2</span><span class="hlt">air</span> in October 2012 was 375.8 ± <span class="hlt">2</span>.0 μatm and in September 2014, 368.9 ± <span class="hlt">2.2</span> μatm. The super-saturation of the seawater in relation to the atmosphere indicates a source of <span class="hlt">CO</span><span class="hlt">2</span> to the atmosphere. The entire study area presents oligotrophic conditions. Despite the low concentrations, Chl a and nutrients presented significant influence on f<span class="hlt">CO</span><span class="hlt">2</span>sw, particularly in the westernmost and more humid part of the northeast coast, where river <span class="hlt">fluxes</span> are three orders of magnitude larger than eastern rivers and rainfall events are more intense and constant. f<span class="hlt">CO</span><span class="hlt">2</span>sw spatial distribution presented homogeneity along the same transect and longitudinal heterogeneity, between east and west, reinforcing the hypothesis of transition between two regions of different behaviour. The f<span class="hlt">CO</span><span class="hlt">2</span>sw at the eastern portion was controlled by parameters such as temperature and salinity. At the western portion, f<span class="hlt">CO</span><span class="hlt">2</span>sw was influenced by nutrient and Chl a. Calculated instantaneous <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> ranged from + 1.66 to + 7.24 mmol m- <span class="hlt">2</span> d- 1 in the first cruise and + 0.89 to + 14.62 mmol m- <span class="hlt">2</span> d- 1 in the second cruise.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150002122','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150002122"><span>Natural <span class="hlt">Air-Sea</span> <span class="hlt">Flux</span> of <span class="hlt">CO</span><span class="hlt">2</span> in Simulations of the NASA-GISS Climate Model: Sensitivity to the Physical Ocean Model Formulation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Romanou, A.; Gregg, Watson W.; Romanski, J.; Kelley, M.; Bleck, R.; Healy, R.; Nazarenko, L.; Russell, G.; Schmidt, G. A.; Sun, S.; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20150002122'); toggleEditAbsImage('author_20150002122_show'); toggleEditAbsImage('author_20150002122_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20150002122_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20150002122_hide"></p> <p>2013-01-01</p> <p>Results from twin control simulations of the preindustrial <span class="hlt">CO</span><span class="hlt">2</span> gas exchange (natural <span class="hlt">flux</span> of <span class="hlt">CO</span><span class="hlt">2</span>) between the ocean and the atmosphere are presented here using the NASA-GISS climate model, in which the same atmospheric component (modelE<span class="hlt">2</span>) is coupled to two different ocean models, the Russell ocean model and HYCOM. Both incarnations of the GISS climate model are also coupled to the same ocean biogeochemistry module (NOBM) which estimates prognostic distributions for biotic and abiotic fields that influence the <span class="hlt">air-sea</span> <span class="hlt">flux</span> of <span class="hlt">CO</span><span class="hlt">2</span>. Model intercomparison is carried out at equilibrium conditions and model differences are contrasted with biases from present day climatologies. Although the models agree on the spatial patterns of the <span class="hlt">air-sea</span> <span class="hlt">flux</span> of <span class="hlt">CO</span><span class="hlt">2</span>, they disagree on the strength of the North Atlantic and Southern Ocean sinks mainly because of kinematic (winds) and chemistry (p<span class="hlt">CO</span><span class="hlt">2</span>) differences rather than thermodynamic (SST) ones. Biology/chemistry dissimilarities in the models stem from the different parameterizations of advective and diffusive processes, such as overturning, mixing and horizontal tracer advection and to a lesser degree from parameterizations of biogeochemical processes such as gravitational settling and sinking. The global meridional overturning circulation illustrates much of the different behavior of the biological pump in the two models, together with differences in mixed layer depth which are responsible for different SST, DIC and nutrient distributions in the two models and consequently different atmospheric feedbacks (in the wind, net heat and freshwater <span class="hlt">fluxes</span> into the ocean).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ESD.....8.1093P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ESD.....8.1093P"><span>The potential of using remote sensing data to estimate <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange in the Baltic <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Parard, Gaëlle; Rutgersson, Anna; Parampil, Sindu Raj; Alexandre Charantonis, Anastase</p> <p>2017-12-01</p> <p>In this article, we present the first climatological map of <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> over the Baltic <span class="hlt">Sea</span> based on remote sensing data: estimates of p<span class="hlt">CO</span><span class="hlt">2</span> derived from satellite imaging using self-organizing map classifications along with class-specific linear regressions (SOMLO methodology) and remotely sensed wind estimates. The estimates have a spatial resolution of 4 km both in latitude and longitude and a monthly temporal resolution from 1998 to 2011. The <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> are estimated using two types of wind products, i.e. reanalysis winds and satellite wind products, the higher-resolution wind product generally leading to higher-amplitude <span class="hlt">flux</span> estimations. Furthermore, the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> were also estimated using two methods: the method of Wanninkhof et al. (2013) and the method of Rutgersson and Smedman (2009). The seasonal variation in <span class="hlt">fluxes</span> reflects the seasonal variation in p<span class="hlt">CO</span><span class="hlt">2</span> unvaryingly over the whole Baltic <span class="hlt">Sea</span>, with high winter <span class="hlt">CO</span><span class="hlt">2</span> emissions and high p<span class="hlt">CO</span><span class="hlt">2</span> uptakes. All basins act as a source for the atmosphere, with a higher degree of emission in the southern regions (mean source of 1.6 mmol m-<span class="hlt">2</span> d-1 for the South Basin and 0.9 for the Central Basin) than in the northern regions (mean source of 0.1 mmol m-<span class="hlt">2</span> d-1) and the coastal areas act as a larger sink (annual uptake of -4.<span class="hlt">2</span> mmol m-<span class="hlt">2</span> d-1) than does the open <span class="hlt">sea</span> (-4 mmol m-<span class="hlt">2</span> d-1). In its entirety, the Baltic <span class="hlt">Sea</span> acts as a small source of 1.<span class="hlt">2</span> mmol m-<span class="hlt">2</span> d-1 on average and this annual uptake has increased from 1998 to 2012.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.9663B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.9663B"><span>Surface Water p<span class="hlt">CO</span><span class="hlt">2</span> Variations and <span class="hlt">Sea-Air</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Fluxes</span> During Summer in the Eastern Canadian Arctic</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Burgers, T. M.; Miller, L. A.; Thomas, H.; Else, B. G. T.; Gosselin, M.; Papakyriakou, T.</p> <p>2017-12-01</p> <p>Based on a <span class="hlt">2</span> year data set, the eastern Canadian Arctic Archipelago and Baffin Bay appear to be a modest summertime sink of atmospheric <span class="hlt">CO</span><span class="hlt">2</span>. We measured surface water <span class="hlt">CO</span><span class="hlt">2</span> partial pressure (p<span class="hlt">CO</span><span class="hlt">2</span>), salinity, and temperature throughout northern Baffin Bay, Nares Strait, and Lancaster Sound from the CCGS Amundsen during its 2013 and 2014 summer cruises. Surface water p<span class="hlt">CO</span><span class="hlt">2</span> displayed considerable variability (144-364 μatm) but never exceeded atmospheric concentrations, and average calculated <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in 2013 and 2014 were -12 and -3 mmol C m-<span class="hlt">2</span> d-1 (into the ocean), respectively. Ancillary measurements of chlorophyll a reveal low summertime productivity in surface waters. Based on total alkalinity and stable oxygen isotopes (δ18O) data, a strong riverine signal in northern Nares Strait coincided with relatively high surface p<span class="hlt">CO</span><span class="hlt">2</span>, whereas areas of <span class="hlt">sea</span>-ice melt occur with low surface p<span class="hlt">CO</span><span class="hlt">2</span>. Further assessments, extending the seasonal observation period, are needed to properly constrain both seasonal and annual <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in this region.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002DSRII..49.1601T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002DSRII..49.1601T"><span>Global <span class="hlt">sea-air</span> <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">flux</span> based on climatological surface ocean p<span class="hlt">CO</span> <span class="hlt">2</span>, and seasonal biological and temperature effects</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Takahashi, Taro; Sutherland, Stewart C.; Sweeney, Colm; Poisson, Alain; Metzl, Nicolas; Tilbrook, Bronte; Bates, Nicolas; Wanninkhof, Rik; Feely, Richard A.; Sabine, Christopher; Olafsson, Jon; Nojiri, Yukihiro</p> <p></p> <p>Based on about 940,000 measurements of surface-water p<span class="hlt">CO</span> <span class="hlt">2</span> obtained since the International Geophysical Year of 1956-59, the climatological, monthly distribution of p<span class="hlt">CO</span> <span class="hlt">2</span> in the global surface waters representing mean non-El Niño conditions has been obtained with a spatial resolution of 4°×5° for a reference year 1995. The monthly and annual net <span class="hlt">sea-air</span> <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">flux</span> has been computed using the NCEP/NCAR 41-year mean monthly wind speeds. An annual net uptake <span class="hlt">flux</span> of <span class="hlt">CO</span> <span class="hlt">2</span> by the global oceans has been estimated to be <span class="hlt">2.2</span> (+22% or -19%) Pg C yr -1 using the (wind speed) <span class="hlt">2</span> dependence of the <span class="hlt">CO</span> <span class="hlt">2</span> gas transfer velocity of Wanninkhof (J. Geophys. Res. 97 (1992) 7373). The errors associated with the wind-speed variation have been estimated using one standard deviation (about±<span class="hlt">2</span> m s -1) from the mean monthly wind speed observed over each 4°×5° pixel area of the global oceans. The new global uptake <span class="hlt">flux</span> obtained with the Wanninkhof (wind speed) <span class="hlt">2</span> dependence is compared with those obtained previously using a smaller number of measurements, about 250,000 and 550,000, respectively, and are found to be consistent within±0.<span class="hlt">2</span> Pg C yr -1. This estimate for the global ocean uptake <span class="hlt">flux</span> is consistent with the values of <span class="hlt">2</span>.0±0.6 Pg C yr -1 estimated on the basis of the observed changes in the atmospheric <span class="hlt">CO</span> <span class="hlt">2</span> and oxygen concentrations during the 1990s (Nature 381 (1996) 218; Science 287 (2000) 2467). However, if the (wind speed) 3 dependence of Wanninkhof and McGillis (Res. Lett. 26 (1999) 1889) is used instead, the annual ocean uptake as well as the sensitivity to wind-speed variability is increased by about 70%. A zone between 40° and 60° latitudes in both the northern and southern hemispheres is found to be a major sink for atmospheric <span class="hlt">CO</span> <span class="hlt">2</span>. In these areas, poleward-flowing warm waters meet and mix with the cold subpolar waters rich in nutrients. The p<span class="hlt">CO</span> <span class="hlt">2</span> in the surface water is decreased by the cooling effect on warm waters and by the biological drawdown of p<span class="hlt">CO</span> <span class="hlt">2</span> in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOS.A43A..03B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOS.A43A..03B"><span>Seasonal Oxygen Supersaturation and <span class="hlt">Air-Sea</span> <span class="hlt">Fluxes</span> from Profiling Floats in the Pacific</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bushinsky, S. M.; Emerson, S. R.</p> <p>2016-02-01</p> <p>The Pacific Ocean is a heterogeneous basin that includes regions of strong <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> to and from the atmosphere. The Kuroshio Extension (KE) is a current associated with the largest <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> into the Pacific Ocean, which extends across the Pacific basin between the subarctic and subtropical regions. The relative importance of the biological and physical processes controlling this sink is uncertain. The stoichiometric relationship between O<span class="hlt">2</span> and dissolved inorganic carbon during photosynthesis and respiration may allow in situ O<span class="hlt">2</span> measurements to help determine the processes driving this large <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span>. In this study, we used Argo profiling floats with modified oxygen sensors to estimate O<span class="hlt">2</span> <span class="hlt">fluxes</span> in several areas of the Pacific. In situ <span class="hlt">air</span> calibrations of these sensors allowed us to accurately measure <span class="hlt">air-sea</span> O<span class="hlt">2</span> differences, which largely control the <span class="hlt">flux</span> of O<span class="hlt">2</span> to and from the atmosphere. In this way, we determine <span class="hlt">air-sea</span> O<span class="hlt">2</span> <span class="hlt">fluxes</span> from profiling floats, which previously did not measure O<span class="hlt">2</span> accurately enough to make these calculations. To characterize different areas within the KE, we separated O<span class="hlt">2</span> measurements from floats into 3 regions based on geographical position and temperature-salinity relationships: North KE, Central KE, and South KE. We then used these regions and floats in the Alaska Gyre and subtropical South Pacific gyre to develop seasonal climatologies of ΔO<span class="hlt">2</span> and <span class="hlt">air-sea</span> <span class="hlt">flux</span>. Mean annual <span class="hlt">air-sea</span> oxygen <span class="hlt">fluxes</span> (positive <span class="hlt">fluxes</span> represent addition of O<span class="hlt">2</span> to the ocean) were calculated for the Alaska Gyre of -0.3 mol m-<span class="hlt">2</span> yr-1 (2012-2015), for the northern KE, central KE, and southern KE (2013-2015) of 6.8, 10.5, and 0.5 mol m-<span class="hlt">2</span> yr-1, respectively, and for the south subtropical Pacific (2014-2015) of 0.6 mol m-<span class="hlt">2</span> yr-1. The <span class="hlt">air-sea</span> <span class="hlt">flux</span> due to bubbles was greater than 50% of the total <span class="hlt">flux</span> for winter months and essential for determining the magnitude and, in some cases, direction of the cumulative mean annual <span class="hlt">flux</span>. Increases in solubility due to wintertime</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018CSR...162...27C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018CSR...162...27C"><span>Diurnal variability of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> at coastal zone of Taiwan based on eddy covariance observation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chien, Hwa; Zhong, Yao-Zhao; Yang, Kang-Hung; Cheng, Hao-Yuan</p> <p>2018-06-01</p> <p>In this study, we employed shore-based eddy covariance systems for a continuous measurement of the coastal <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> near the northwestern coast of Taiwan from 2011 to 2015. To ensure the validity of the analysis, the data was selected and filtered with a footprint model and an empirical mode decomposition method. The results indicate that the nearshore <span class="hlt">air-sea</span> and <span class="hlt">air</span>-land <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> exhibited a significant diurnal variability and a substantial day-night difference. The net <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> was -1.75 ± 0.98 μmol-C m-<span class="hlt">2</span> s-1, whereas the net <span class="hlt">air</span>-land <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> was 0.54 ± 7.35 μmol-C m-<span class="hlt">2</span> s-1, which indicated that in northwestern Taiwan, the coastal water acts as a sink of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> but the coastal land acts as a source. The Random Forest Method was applied to hierarchize the influence of Chl-a, SST, DO, pH and U10 on <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. The result suggests that the strength of the diurnal <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> is strongly influenced by the local wind speed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19850060100&hterms=Radon&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3DRadon','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19850060100&hterms=Radon&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3DRadon"><span>Gas exchange and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> in the tropical Atlantic Ocean determined from Rn-222 and p<span class="hlt">CO</span><span class="hlt">2</span> measurements</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Smethie, W. M., Jr.; Takahashi, T.; Chipman, D. W.; Ledwell, J. R.</p> <p>1985-01-01</p> <p>The piston velocity for the tropical Atlantic Ocean has been determined from 29 radon profiles measured during the TTO Tropical Atlantic Study. By combining these data with the p<span class="hlt">CO</span><span class="hlt">2</span> data measured in the surface water and <span class="hlt">air</span> samples, the net <span class="hlt">flux</span> of <span class="hlt">CO</span><span class="hlt">2</span> across the <span class="hlt">sea-air</span> interface has been calculated for the tropical Atlantic. The dependence of the piston velocity on wind speed is discussed, and possible causes for the high <span class="hlt">sea-to-air</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> observed in the equatorial zone are examined.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011BGeo....8..505M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011BGeo....8..505M"><span>Changes in ocean circulation and carbon storage are decoupled from <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marinov, I.; Gnanadesikan, A.</p> <p>2011-02-01</p> <p>The spatial distribution of the <span class="hlt">air-sea</span> <span class="hlt">flux</span> of carbon dioxide is a poor indicator of the underlying ocean circulation and of ocean carbon storage. The weak dependence on circulation arises because mixing-driven changes in solubility-driven and biologically-driven <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> largely cancel out. This cancellation occurs because mixing driven increases in the poleward residual mean circulation result in more transport of both remineralized nutrients and heat from low to high latitudes. By contrast, increasing vertical mixing decreases the storage associated with both the biological and solubility pumps, as it decreases remineralized carbon storage in the deep ocean and warms the ocean as a whole.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010BGD.....7.7985M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010BGD.....7.7985M"><span>Changes in ocean circulation and carbon storage are decoupled from <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marinov, I.; Gnanadesikan, A.</p> <p>2010-11-01</p> <p>The spatial distribution of the <span class="hlt">air-sea</span> <span class="hlt">flux</span> of carbon dioxide is a poor indicator of the underlying ocean circulation and of ocean carbon storage. The weak dependence on circulation arises because mixing-driven changes in solubility-driven and biologically-driven <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> largely cancel out. This cancellation occurs because mixing driven increases in the poleward residual mean circulation results in more transport of both remineralized nutrients and heat from low to high latitudes. By contrast, increasing vertical mixing decreases the storage associated with both the biological and solubility pumps, as it decreases remineralized carbon storage in the deep ocean and warms the ocean as a whole.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A51A2037B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A51A2037B"><span>Observational analysis of <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> and <span class="hlt">sea</span> water temperature offshore South China <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bi, X.; Huang, J.; Gao, Z.; Liu, Y.</p> <p>2017-12-01</p> <p>This paper investigates the <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> (momentum <span class="hlt">flux</span>, sensible heat <span class="hlt">flux</span> and latent heat <span class="hlt">flux</span>) from eddy covariance method based on data collected at an offshore observation tower in the South China <span class="hlt">Sea</span> from January 2009 to December 2016 and <span class="hlt">sea</span> water temperature (SWT) on six different levels based on data collected from November 2011 to June 2013. The depth of water at the tower over the <span class="hlt">sea</span> averages about 15 m. This study presents the in-situ measurements of continuous <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> and SWT at different depths. Seasonal and diurnal variations in <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> and SWT on different depths are examined. Results show that <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> and all SWT changed seasonally; <span class="hlt">sea</span>-land breeze circulation appears all the year round. Unlike winters where SWT on different depths are fairly consistent, the difference between <span class="hlt">sea</span> surface temperature (SST) and <span class="hlt">sea</span> temperature at 10 m water depth fluctuates dramatically and the maximum value reaches 7 °C during summer.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_1");'>1</a></li> <li class="active"><span>2</span></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_2 --> <div id="page_3" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_1");'>1</a></li> <li><a href="#" onclick='return showDiv("page_2");'>2</a></li> <li class="active"><span>3</span></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="41"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JGRC..121.1229W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JGRC..121.1229W"><span>On the calculation of <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> of <span class="hlt">CO</span><span class="hlt">2</span> in the presence of temperature and salinity gradients</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Woolf, D. K.; Land, P. E.; Shutler, J. D.; Goddijn-Murphy, L. M.; Donlon, C. J.</p> <p>2016-02-01</p> <p>The presence of vertical temperature and salinity gradients in the upper ocean and the occurrence of variations in temperature and salinity on time scales from hours to many years complicate the calculation of the <span class="hlt">flux</span> of carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) across the <span class="hlt">sea</span> surface. Temperature and salinity affect the interfacial concentration of aqueous <span class="hlt">CO</span><span class="hlt">2</span> primarily through their effect on solubility with lesser effects related to saturated vapor pressure and the relationship between fugacity and partial pressure. The effects of temperature and salinity profiles in the water column and changes in the aqueous concentration act primarily through the partitioning of the carbonate system. Climatological calculations of <span class="hlt">flux</span> require attention to variability in the upper ocean and to the limited validity of assuming "constant chemistry" in transforming measurements to climatological values. Contrary to some recent analysis, it is shown that the effect on <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> of a cool skin on the <span class="hlt">sea</span> surface is large and ubiquitous. An opposing effect on calculated <span class="hlt">fluxes</span> is related to the occurrence of warm layers near the surface; this effect can be locally large but will usually coincide with periods of low exchange. A salty skin and salinity anomalies in the upper ocean also affect <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> calculations, though these haline effects are generally weaker than the thermal effects.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016GBioC..30..983L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GBioC..30..983L"><span>Quantifying the drivers of ocean-atmosphere <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lauderdale, Jonathan M.; Dutkiewicz, Stephanie; Williams, Richard G.; Follows, Michael J.</p> <p>2016-07-01</p> <p>A mechanistic framework for quantitatively mapping the regional drivers of <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> at a global scale is developed. The framework evaluates the interplay between (1) surface heat and freshwater <span class="hlt">fluxes</span> that influence the potential saturated carbon concentration, which depends on changes in <span class="hlt">sea</span> surface temperature, salinity and alkalinity, (<span class="hlt">2</span>) a residual, disequilibrium <span class="hlt">flux</span> influenced by upwelling and entrainment of remineralized carbon- and nutrient-rich waters from the ocean interior, as well as rapid subduction of surface waters, (3) carbon uptake and export by biological activity as both soft tissue and carbonate, and (4) the effect on surface carbon concentrations due to freshwater precipitation or evaporation. In a steady state simulation of a coarse-resolution ocean circulation and biogeochemistry model, the sum of the individually determined components is close to the known total <span class="hlt">flux</span> of the simulation. The leading order balance, identified in different dynamical regimes, is between the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> driven by surface heat <span class="hlt">fluxes</span> and a combination of biologically driven carbon uptake and disequilibrium-driven carbon outgassing. The framework is still able to reconstruct simulated <span class="hlt">fluxes</span> when evaluated using monthly averaged data and takes a form that can be applied consistently in models of different complexity and observations of the ocean. In this way, the framework may reveal differences in the balance of drivers acting across an ensemble of climate model simulations or be applied to an analysis and interpretation of the observed, real-world <span class="hlt">air-sea</span> <span class="hlt">flux</span> of <span class="hlt">CO</span><span class="hlt">2</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/18186331','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/18186331"><span>Variability of the gaseous elemental mercury <span class="hlt">sea-air</span> <span class="hlt">flux</span> of the Baltic <span class="hlt">Sea</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kuss, Joachim; Schneider, Bernd</p> <p>2007-12-01</p> <p>The importance of the <span class="hlt">sea</span> as a sink for atmospheric mercury has been established quantitatively through models based on wet and dry deposition data, but little is known about the release of mercury from <span class="hlt">sea</span> areas. The concentration of elemental mercury (Hg0) in <span class="hlt">sea</span> surface water and in the marine atmosphere of the Baltic <span class="hlt">Sea</span> was measured at high spatial resolution in February, April, July, and November 2006. Wind-speed records and the gas-exchange transfer velocity were then used to calculate Hg0 <span class="hlt">sea-air</span> <span class="hlt">fluxes</span> on the basis of Hg0 <span class="hlt">sea-air</span> concentration differences. Our results show that the spatial resolution of the surface water Hg0 data can be significantly improved by continuous measurements of Hg0 in <span class="hlt">air</span> equilibrated with water instead of quantitative extraction of Hg0 from seawater samples. A spatial and highly seasonal variability of the Hg0 <span class="hlt">sea-air</span> <span class="hlt">flux</span> was thus determined. In winter, the <span class="hlt">flux</span> was low and changed in direction. In summer, a strong emission <span class="hlt">flux</span> of up to 150 ng m(-<span class="hlt">2</span>) day(-1) in the central Baltic <span class="hlt">Sea</span> was recorded. The total emission of Hg0 from the studied area (235000 km<span class="hlt">2</span>) was 4300 +/- 1600 kg in 2006 and exceeded deposition estimates.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1995TellB..47..447I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1995TellB..47..447I"><span><span class="hlt">Air-sea</span> exchange of <span class="hlt">CO</span><span class="hlt">2</span> in the central and western equatorial Pacific in 1990</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ishii, Masao; Yoshikawa Inoue, Hisayuki</p> <p>1995-09-01</p> <p>Measurements of <span class="hlt">CO</span><span class="hlt">2</span> in marine boundary <span class="hlt">air</span> and in surface seawater of the central and western Pacific west of 150°W were made during the period from September to December 1990. The meridional section along 150°W showed p<span class="hlt">CO</span><span class="hlt">2</span>(<span class="hlt">sea</span>) maximum over 410 µatm between the equator and 3°S due to strong equatorial upwelling. In the equatorial Pacific between 150°W and 179°E, p<span class="hlt">CO</span><span class="hlt">2</span>(<span class="hlt">sea</span>) decreased gradually toward the west as a result of biological <span class="hlt">CO</span><span class="hlt">2</span> uptake and surface <span class="hlt">sea</span> temperature increase. Between 179°E and 170°E, the p<span class="hlt">CO</span><span class="hlt">2</span>(<span class="hlt">sea</span>) decreased steeply from 400 µatm to 350 µatm along with a decrease of salinity. West of 170°E, where the salinity is low owing to the heavy rainfall, p<span class="hlt">CO</span><span class="hlt">2</span>(<span class="hlt">sea</span>) was nearly equal to p<span class="hlt">CO</span><span class="hlt">2</span>(<span class="hlt">air</span>). The distribution of the atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentration showed a considerable variability (±3ppm) in the area north of the Intertropical Convergence Zone due to the regional net source-sink strength of the terrestrial biosphere. The net <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> from the <span class="hlt">sea</span> to the atmosphere in the equatorial region of the central and western Pacific (15°S-10°N, 140°E-150°W) was evaluated from the Δp<span class="hlt">CO</span><span class="hlt">2</span> distribution and the several gas transfer coefficients reported so far. It ranged from 0.13 GtC year<img src="/entityImage/script/2212.gif" alt="-" border="0" style="font-weight: bold"></img>1-0.29 GtC year<img src="/entityImage/script/2212.gif" alt="-" border="0" style="font-weight: bold"></img>1. This <span class="hlt">CO</span><span class="hlt">2</span> outflux is thought to almost disappear during the period of an El Niño event.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSPO51D..01B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSPO51D..01B"><span>Intercomparison of <span class="hlt">Air-Sea</span> <span class="hlt">Fluxes</span> in the Bay of Bengal</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Buckley, J.; Weller, R. A.; Farrar, J. T.; Tandon, A.</p> <p>2016-02-01</p> <p>Heat and momentum exchange between the <span class="hlt">air</span> and <span class="hlt">sea</span> in the Bay of Bengal is an important driver of atmospheric convection during the Asian Monsoon. Warm <span class="hlt">sea</span> surface temperatures resulting from salinity stratified shallow mixed layers trigger widespread showers and thunderstorms. In this study, we compare atmospheric reanalysis <span class="hlt">flux</span> products to <span class="hlt">air-sea</span> <span class="hlt">flux</span> values calculated from shipboard observations from four cruises and an <span class="hlt">air-sea</span> <span class="hlt">flux</span> mooring in the Bay of Bengal as part of the <span class="hlt">Air-Sea</span> Interactions in the Northern Indian Ocean (ASIRI) experiment. Comparisons with months of mooring data show that most long timescale reanalysis error arises from the overestimation of longwave and shortwave radiation. Ship observations and select data from the <span class="hlt">air-sea</span> <span class="hlt">flux</span> mooring reveals significant errors on shorter timescales (<span class="hlt">2</span>-4 weeks) which are greatly influenced by errors in shortwave radiation and latent and sensible heat. During these shorter periods, the reanalyses fail to properly show sharp decreases in <span class="hlt">air</span> temperature, humidity, and shortwave radiation associated with mesoscale convective systems. Simulations with the Price-Weller-Pinkel (PWP) model show upper ocean mixing and deepening mixed layers during these events that effect the long term upper ocean stratification. Mesoscale convective systems associated with cloudy skies and cold and dry <span class="hlt">air</span> can reduce net heat into the ocean for minutes to a few days, significantly effecting <span class="hlt">air-sea</span> heat transfer, upper ocean stratification, and ocean surface temperature and salinity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017OcSci..13..997P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017OcSci..13..997P"><span>The spatial and interannual dynamics of the surface water carbonate system and <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in the outer shelf and slope of the Eurasian Arctic Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pipko, Irina I.; Pugach, Svetlana P.; Semiletov, Igor P.; Anderson, Leif G.; Shakhova, Natalia E.; Gustafsson, Örjan; Repina, Irina A.; Spivak, Eduard A.; Charkin, Alexander N.; Salyuk, Anatoly N.; Shcherbakova, Kseniia P.; Panova, Elena V.; Dudarev, Oleg V.</p> <p>2017-11-01</p> <p>The Arctic is undergoing dramatic changes which cover the entire range of natural processes, from extreme increases in the temperatures of <span class="hlt">air</span>, soil, and water, to changes in the cryosphere, the biodiversity of Arctic waters, and land vegetation. Small changes in the largest marine carbon pool, the dissolved inorganic carbon pool, can have a profound impact on the carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) <span class="hlt">flux</span> between the ocean and the atmosphere, and the feedback of this <span class="hlt">flux</span> to climate. Knowledge of relevant processes in the Arctic <span class="hlt">seas</span> improves the evaluation and projection of carbon cycle dynamics under current conditions of rapid climate change. Investigation of the <span class="hlt">CO</span><span class="hlt">2</span> system in the outer shelf and continental slope waters of the Eurasian Arctic <span class="hlt">seas</span> (the Barents, Kara, Laptev, and East Siberian <span class="hlt">seas</span>) during 2006, 2007, and 2009 revealed a general trend in the surface water partial pressure of <span class="hlt">CO</span><span class="hlt">2</span> (p<span class="hlt">CO</span><span class="hlt">2</span>) distribution, which manifested as an increase in p<span class="hlt">CO</span><span class="hlt">2</span> values eastward. The existence of this trend was defined by different oceanographic and biogeochemical regimes in the western and eastern parts of the study area; the trend is likely increasing due to a combination of factors determined by contemporary change in the Arctic climate, each change in turn evoking a series of synergistic effects. A high-resolution in situ investigation of the carbonate system parameters of the four Arctic <span class="hlt">seas</span> was carried out in the warm season of 2007; this year was characterized by the next-to-lowest historic <span class="hlt">sea</span>-ice extent in the Arctic Ocean, on satellite record, to that date. The study showed the different responses of the seawater carbonate system to the environment changes in the western vs. the eastern Eurasian Arctic <span class="hlt">seas</span>. The large, open, highly productive water area in the northern Barents <span class="hlt">Sea</span> enhances atmospheric <span class="hlt">CO</span><span class="hlt">2</span> uptake. In contrast, the uptake of <span class="hlt">CO</span><span class="hlt">2</span> was strongly weakened in the outer shelf and slope waters of the East Siberian Arctic <span class="hlt">seas</span> under the 2007 environmental conditions</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFMOS22B..07M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFMOS22B..07M"><span>Wintertime <span class="hlt">Air-Sea</span> Gas Transfer Rates and <span class="hlt">Air</span> Injection <span class="hlt">Fluxes</span> at Station Papa in the NE Pacific</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>McNeil, C.; Steiner, N.; Vagle, S.</p> <p>2008-12-01</p> <p>In recent studies of <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> of N<span class="hlt">2</span> and O<span class="hlt">2</span> in hurricanes, McNeil and D'Asaro (2007) used a simplified model formulation of <span class="hlt">air-sea</span> gas <span class="hlt">flux</span> to estimate simultaneous values of gas transfer rate, KT, and <span class="hlt">air</span> injection <span class="hlt">flux</span>, VT. The model assumes <span class="hlt">air-sea</span> gas <span class="hlt">fluxes</span> at high to extreme wind speeds can be explained by a combination of two processes: 1) <span class="hlt">air</span> injection, by complete dissolution of small bubbles drawn down into the ocean boundary layer by turbulent currents, and <span class="hlt">2</span>) near-surface equilibration processes, such as occurs within whitecaps. This analysis technique relies on <span class="hlt">air-sea</span> gas <span class="hlt">flux</span> estimates for two gases, N<span class="hlt">2</span> and O<span class="hlt">2</span>, to solve for the two model parameters, KT and VT. We present preliminary results of similar analysis of time series data collected during winter storms at Station Papa in the NE Pacific during 2003/2004. The data show a clear increase in KT and VT with increasing NCEP derived wind speeds and acoustically measured bubble penetration depth.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AMT.....9.5509Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AMT.....9.5509Y"><span>Comparison of two closed-path cavity-based spectrometers for measuring <span class="hlt">air</span>-water <span class="hlt">CO</span><span class="hlt">2</span> and CH4 <span class="hlt">fluxes</span> by eddy covariance</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, Mingxi; Prytherch, John; Kozlova, Elena; Yelland, Margaret J.; Parenkat Mony, Deepulal; Bell, Thomas G.</p> <p>2016-11-01</p> <p>In recent years several commercialised closed-path cavity-based spectroscopic instruments designed for eddy covariance <span class="hlt">flux</span> measurements of carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>), methane (CH4), and water vapour (H<span class="hlt">2</span>O) have become available. Here we compare the performance of two leading models - the Picarro G2311-f and the Los Gatos Research (LGR) Fast Greenhouse Gas Analyzer (FGGA) at a coastal site. Both instruments can compute dry mixing ratios of <span class="hlt">CO</span><span class="hlt">2</span> and CH4 based on concurrently measured H<span class="hlt">2</span>O, temperature, and pressure. Additionally, we used a high throughput Nafion dryer to physically remove H<span class="hlt">2</span>O from the Picarro airstream. Observed <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> and CH4 <span class="hlt">fluxes</span> from these two analysers, averaging about 12 and 0.12 mmol m-<span class="hlt">2</span> day-1 respectively, agree within the measurement uncertainties. For the purpose of quantifying dry <span class="hlt">CO</span><span class="hlt">2</span> and CH4 <span class="hlt">fluxes</span> downstream of a long inlet, the numerical H<span class="hlt">2</span>O corrections appear to be reasonably effective and lead to results that are comparable to physical removal of H<span class="hlt">2</span>O with a Nafion dryer in the mean. We estimate the high-frequency attenuation of <span class="hlt">fluxes</span> in our closed-path set-up, which was relatively small ( ≤ 10 %) for <span class="hlt">CO</span><span class="hlt">2</span> and CH4 but very large for the more polar H<span class="hlt">2</span>O. The Picarro showed significantly lower noise and <span class="hlt">flux</span> detection limits than the LGR. The hourly <span class="hlt">flux</span> detection limit for the Picarro was about <span class="hlt">2</span> mmol m-<span class="hlt">2</span> day-1 for <span class="hlt">CO</span><span class="hlt">2</span> and 0.02 mmol m-<span class="hlt">2</span> day-1 for CH4. For the LGR these detection limits were about 8 and 0.05 mmol m-<span class="hlt">2</span> day-1. Using global maps of monthly mean <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> as reference, we estimate that the Picarro and LGR can resolve hourly <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> from roughly 40 and 4 % of the world's oceans respectively. Averaging over longer timescales would be required in regions with smaller <span class="hlt">fluxes</span>. Hourly <span class="hlt">flux</span> detection limits of CH4 from both instruments are generally higher than the expected emissions from the open ocean, though the signal to noise of this measurement may improve closer to the coast.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.C43E0586E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.C43E0586E"><span>Carbon Dioxide Transfer Through <span class="hlt">Sea</span> Ice: Modelling <span class="hlt">Flux</span> in Brine Channels</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Edwards, L.; Mitchelson-Jacob, G.; Hardman-Mountford, N.</p> <p>2010-12-01</p> <p>For many years <span class="hlt">sea</span> ice was thought to act as a barrier to the <span class="hlt">flux</span> of <span class="hlt">CO</span><span class="hlt">2</span> between the ocean and atmosphere. However, laboratory-based and in-situ observations suggest that while <span class="hlt">sea</span> ice may in some circumstances reduce or prevent transfer (e.g. in regions of thick, superimposed multi-year ice), it may also be highly permeable (e.g. thin, first year ice) with some studies observing significant <span class="hlt">fluxes</span> of <span class="hlt">CO</span><span class="hlt">2</span>. <span class="hlt">Sea</span> ice covered regions have been observed to act both as a sink and a source of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> with the permeability of <span class="hlt">sea</span> ice and direction of <span class="hlt">flux</span> related to <span class="hlt">sea</span> ice temperature and the presence of brine channels in the ice, as well as seasonal processes such as whether the ice is freezing or thawing. Brine channels concentrate dissolved inorganic carbon (DIC) as well as salinity and as these dense waters descend through both the <span class="hlt">sea</span> ice and the surface ocean waters, they create a sink for <span class="hlt">CO</span><span class="hlt">2</span>. Calcium carbonate (ikaite) precipitation in the <span class="hlt">sea</span> ice is thought to enhance this process. Micro-organisms present within the <span class="hlt">sea</span> ice will also contribute to the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> dynamics. Recent evidence of decreasing <span class="hlt">sea</span> ice extent and the associated change from a multi-year ice to first-year ice dominated system suggest the potential for increased <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> through regions of thinner, more porous <span class="hlt">sea</span> ice. A full understanding of the processes and feedbacks controlling the <span class="hlt">flux</span> in these regions is needed to determine their possible contribution to global <span class="hlt">CO</span><span class="hlt">2</span> levels in a future warming climate scenario. Despite the significance of these regions, the <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> in <span class="hlt">sea</span> ice covered regions is not currently included in global climate models. Incorporating this carbon <span class="hlt">flux</span> system into Earth System models requires the development of a well-parameterised <span class="hlt">sea</span> ice-<span class="hlt">air</span> <span class="hlt">flux</span> model. In our work we use the Los Alamos <span class="hlt">sea</span> ice model, CICE, with a modification to incorporate the movement of <span class="hlt">CO</span><span class="hlt">2</span> through brine channels including the addition of DIC processes and ice algae production to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/467708-measurements-co-sub-fluxes-bubbles-from-tower-during-asgasex','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/467708-measurements-co-sub-fluxes-bubbles-from-tower-during-asgasex"><span>Measurements of <span class="hlt">CO</span>{sub <span class="hlt">2</span>} <span class="hlt">fluxes</span> and bubbles from a tower during ASGASEX</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Leeuw, G. de; Kunz, G.J.; Larsen, S.E.</p> <p>1994-12-31</p> <p>The <span class="hlt">Air-Sea</span> Gas Exchange experiment ASGASEX was conducted from August 30 until October 1st from the Meetpost Noordwijk (MPN), a research tower in the North <span class="hlt">Sea</span> at 9 km from the Dutch coast. The objective of ASGASEX was a study of parameters affecting the <span class="hlt">air-sea</span> exchange of gases, and a comparison of experimental methods to derive the exchange coefficient for <span class="hlt">CO</span>{sub <span class="hlt">2</span>}. A detailed description of the ASGASEX experiment is presented in Oost. The authors` contribution to ASGASEX was a micro-meteorological package to measure the <span class="hlt">fluxes</span> of <span class="hlt">CO</span>{sub <span class="hlt">2</span>}, momentum, heat and water vapor, and an instrument to measure themore » size distribution of bubbles just below the <span class="hlt">sea</span> surface. In this contribution the authors report preliminary results from the <span class="hlt">CO</span>{sub <span class="hlt">2</span>} <span class="hlt">flux</span> measurements and the bubble measurements. The latter was made as part of a larger study on the influence of bubbles on gas exchange in cooperation with the University of Southampton and the University of Galway.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PrOce.144...15W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PrOce.144...15W"><span>Biofilm-like properties of the <span class="hlt">sea</span> surface and predicted effects on <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wurl, Oliver; Stolle, Christian; Van Thuoc, Chu; The Thu, Pham; Mari, Xavier</p> <p>2016-05-01</p> <p>Because the <span class="hlt">sea</span> surface controls various interactions between the ocean and the atmosphere, it has a profound function for marine biogeochemistry and climate regulation. The <span class="hlt">sea</span> surface is the gateway for the exchange of climate-relevant gases, heat and particles. Thus, in order to determine how the ocean and the atmosphere interact and respond to environmental changes on a global scale, the characterization and understanding of the <span class="hlt">sea</span> surface are essential. The uppermost part of the water column is defined as the <span class="hlt">sea</span>-surface microlayer and experiences strong spatial and temporal dynamics, mainly due to meteorological forcing. Wave-damped areas at the <span class="hlt">sea</span> surface are caused by the accumulation of surface-active organic material and are defined as slicks. Natural slicks are observed frequently but their biogeochemical properties are poorly understood. In the present study, we found up to 40 times more transparent exopolymer particles (TEP), the foundation of any biofilm, in slicks compared to the underlying bulk water at multiple stations in the North Pacific, South China <span class="hlt">Sea</span>, and Baltic <span class="hlt">Sea</span>. We found a significant lower enrichment of TEP (up to 6) in non-slick <span class="hlt">sea</span> surfaces compared to its underlying bulk water. Moreover, slicks were characterized by a large microbial biomass, another shared feature with conventional biofilms on solid surfaces. Compared to non-slick samples (avg. pairwise similarity of 70%), the community composition of bacteria in slicks was increasingly (avg. pairwise similarity of 45%) different from bulk water communities, indicating that the TEP-matrix creates specific environments for its inhabitants. We, therefore, conclude that slicks can feature biofilm-like properties with the excessive accumulation of particles and microbes. We also assessed the potential distribution and frequency of slick-formation in coastal and oceanic regions, and their effect on <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange based on literature data. We estimate that slicks can reduce <span class="hlt">CO</span><span class="hlt">2</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ACP....18.4297L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ACP....18.4297L"><span>Using eddy covariance to measure the dependence of <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange rate on friction velocity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Landwehr, Sebastian; Miller, Scott D.; Smith, Murray J.; Bell, Thomas G.; Saltzman, Eric S.; Ward, Brian</p> <p>2018-03-01</p> <p>Parameterisation of the <span class="hlt">air-sea</span> gas transfer velocity of <span class="hlt">CO</span><span class="hlt">2</span> and other trace gases under open-ocean conditions has been a focus of <span class="hlt">air-sea</span> interaction research and is required for accurately determining ocean carbon uptake. Ships are the most widely used platform for <span class="hlt">air-sea</span> <span class="hlt">flux</span> measurements but the quality of the data can be compromised by airflow distortion and sensor cross-sensitivity effects. Recent improvements in the understanding of these effects have led to enhanced corrections to the shipboard eddy covariance (EC) measurements.Here, we present a revised analysis of eddy covariance measurements of <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> and momentum <span class="hlt">fluxes</span> from the Southern Ocean Surface Ocean Aerosol Production (SOAP) study. We show that it is possible to significantly reduce the scatter in the EC data and achieve consistency between measurements taken on station and with the ship underway. The gas transfer velocities from the EC measurements correlate better with the EC friction velocity (u*) than with mean wind speeds derived from shipboard measurements corrected with an airflow distortion model. For the observed range of wind speeds (u10 N = 3-23 m s-1), the transfer velocities can be parameterised with a linear fit to u*. The SOAP data are compared to previous gas transfer parameterisations using u10 N computed from the EC friction velocity with the drag coefficient from the Coupled Ocean-Atmosphere Response Experiment (COARE) model version 3.5. The SOAP results are consistent with previous gas transfer studies, but at high wind speeds they do not support the sharp increase in gas transfer associated with bubble-mediated transfer predicted by physically based models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSAH44A0084L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSAH44A0084L"><span><span class="hlt">Air</span>-water <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Fluxes</span> In Seasonal Hypoxia-influenced Green Bay, Lake Michigan</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lin, P.; Klump, J. V.; Guo, L.</p> <p>2016-02-01</p> <p>Increasing anthropogenic nutrient enrichment has led to seasonal hypoxia in Green Bay, the largest freshwater estuary in the Laurentian Great Lakes, but change in carbon dynamics associated with the development of hypoxia remains poorly understood. Variations in alkalinity, abundance of carbon species, and <span class="hlt">air</span>-water <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> were quantified under contrasting hypoxic conditions during summer 2014. Green Bay was characterized with high pH (average 8.62 ± 0.16 in August), high DIC concentrations (2113 - 3213 µmol/kg) and high p<span class="hlt">CO</span><span class="hlt">2</span> in the water column. p<span class="hlt">CO</span><span class="hlt">2</span> was mostly >700 µatm in June, resulting in a net <span class="hlt">CO</span><span class="hlt">2</span> source to the <span class="hlt">air</span>, while p<span class="hlt">CO</span><span class="hlt">2</span> was mostly <650 µatm in August when hypoxic conditions occurred in Green Bay. In central Green Bay, p<span class="hlt">CO</span><span class="hlt">2</span> was the highest during both sampling months, accompanying by low dissolved oxygen (DO) and lower pH in the water column. In August, p<span class="hlt">CO</span><span class="hlt">2</span> was inversely correlated with DOC concentration and increased with DOC/DOP ratio, suggesting a control by organic matter on <span class="hlt">air</span>-water <span class="hlt">CO</span><span class="hlt">2</span> dynamics and consumption of DO in Green Bay. Positive <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> to the atmosphere during August were only observed in northern bay but a <span class="hlt">CO</span><span class="hlt">2</span> sink was found in southern Green Bay ( 40% of study area) with high biological production and terrestrial DOM. Daily <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> ranged from 10.9 to 48.5 mmol-C m-<span class="hlt">2</span> d-1 in June with an average of 18.29 ± 7.44 mmol-C m-<span class="hlt">2</span> d-1, whereas it varied from 1.82 ± 1.18 mmol m-<span class="hlt">2</span> d-1 in the north to -<span class="hlt">2</span>.05 ± 1.89 mmol m-<span class="hlt">2</span> d-1 in the south of Green Bay in August. Even though strong biological production reduced the <span class="hlt">CO</span><span class="hlt">2</span> emission, daily <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> from Green Bay to the <span class="hlt">air</span> were as high as 7.4 × 107 mole-C in June and 4.6 × 106 mole-C in August, suggesting a significant role of high-DIC lakes in global <span class="hlt">CO</span><span class="hlt">2</span> budget and cycling.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110014594','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110014594"><span>Ocean Winds and Turbulent <span class="hlt">Air-Sea</span> <span class="hlt">Fluxes</span> Inferred From Remote Sensing</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bourassa, Mark A.; Gille, Sarah T.; Jackson, Daren L.; Roberts, J. Brent; Wick, Gary A.</p> <p>2010-01-01</p> <p><span class="hlt">Air-sea</span> turbulent <span class="hlt">fluxes</span> determine the exchange of momentum, heat, freshwater, and gas between the atmosphere and ocean. These exchange processes are critical to a broad range of research questions spanning length scales from meters to thousands of kilometers and time scales from hours to decades. Examples are discussed (section <span class="hlt">2</span>). The estimation of surface turbulent <span class="hlt">fluxes</span> from satellite is challenging and fraught with considerable errors (section 3); however, recent developments in retrievals (section 3) will greatly reduce these errors. Goals for the future observing system are summarized in section 4. Surface <span class="hlt">fluxes</span> are defined as the rate per unit area at which something (e.g., momentum, energy, moisture, or <span class="hlt">CO</span> Z ) is transferred across the <span class="hlt">air/sea</span> interface. Wind- and buoyancy-driven surface <span class="hlt">fluxes</span> are called surface turbulent <span class="hlt">fluxes</span> because the mixing and transport are due to turbulence. Examples of nonturbulent processes are radiative <span class="hlt">fluxes</span> (e.g., solar radiation) and precipitation (Schmitt et al., 2010). Turbulent <span class="hlt">fluxes</span> are strongly dependent on wind speed; therefore, observations of wind speed are critical for the calculation of all turbulent surface <span class="hlt">fluxes</span>. Wind stress, the vertical transport of horizontal momentum, also depends on wind direction. Stress is very important for many ocean processes, including upper ocean currents (Dohan and Maximenko, 2010) and deep ocean currents (Lee et al., 2010). On short time scales, this horizontal transport is usually small compared to surface <span class="hlt">fluxes</span>. For long-term processes, transport can be very important but again is usually small compared to surface <span class="hlt">fluxes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016QuRes..85...87C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016QuRes..85...87C"><span>Variability of 14C reservoir age and <span class="hlt">air-sea</span> <span class="hlt">flux</span> of <span class="hlt">CO</span><span class="hlt">2</span> in the Peru-Chile upwelling region during the past 12,000 years</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carré, Matthieu; Jackson, Donald; Maldonado, Antonio; Chase, Brian M.; Sachs, Julian P.</p> <p>2016-01-01</p> <p>The variability of radiocarbon marine reservoir age through time and space limits the accuracy of chronologies in marine paleo-environmental archives. We report here new radiocarbon reservoir ages (ΔR) from the central coast of Chile ( 32°S) for the Holocene period and compare these values to existing reservoir age reconstructions from southern Peru and northern Chile. Late Holocene ΔR values show little variability from central Chile to Peru. Prior to 6000 cal yr BP, however, ΔR values were markedly increased in southern Peru and northern Chile, while similar or slightly lower-than-modern ΔR values were observed in central Chile. This extended dataset suggests that the early Holocene was characterized by a substantial increase in the latitudinal gradient of marine reservoir age between central and northern Chile. This change in the marine reservoir ages indicates that the early Holocene <span class="hlt">air-sea</span> <span class="hlt">flux</span> of <span class="hlt">CO</span><span class="hlt">2</span> could have been up to five times more intense than in the late Holocene in the Peruvian upwelling, while slightly reduced in central Chile. Our results show that oceanic circulation changes in the Humboldt system during the Holocene have substantially modified the <span class="hlt">air-sea</span> carbon <span class="hlt">flux</span> in this region.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17874769','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17874769"><span><span class="hlt">Air-sea</span> exchange <span class="hlt">fluxes</span> of synthetic polycyclic musks in the North <span class="hlt">Sea</span> and the Arctic.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Xie, Zhiyong; Ebinghaus, Ralf; Temme, Christian; Heemken, Olaf; Ruck, Wolfgang</p> <p>2007-08-15</p> <p>Synthetic polycyclic musk fragrances Galaxolide (HHCB) and Tonalide (AHTN) were measured simultaneously in <span class="hlt">air</span> and seawater in the Arctic and the North <span class="hlt">Sea</span> and in the rural <span class="hlt">air</span> of northern Germany. Median concentrations of gas-phase HHCB and AHTN were 4 and 18 pg m(-3) in the Arctic, 28 and 18 pg m(-3) in the North <span class="hlt">Sea</span>, and 71 and 21 pg m(-3) in northern Germany, respectively. Various ratios of HHCB/AHTN implied that HHCB is quickly removed by atmospheric degradation, while AHTN is relatively persistent in the atmosphere. Dissolved concentrations ranged from 12 to 2030 pg L(-1) for HHCB and from below the method detection limit (3 pg L(-1)) to 965 pg L(-1) for AHTN with median values of 59 and 23 pg L(-1), respectively. The medians of volatilization <span class="hlt">fluxes</span> for HHCB and AHTN were 27.<span class="hlt">2</span> and 14.<span class="hlt">2</span> ng m(-<span class="hlt">2</span>) day(-1) and the depositional <span class="hlt">fluxes</span> were 5.9 and 3.3 ng m(-<span class="hlt">2</span>) day(-1), respectively, indicating water-to-<span class="hlt">air</span> volatilization is a significant process to eliminate HHCB and AHTN from the North <span class="hlt">Sea</span>. In the Arctic, deposition <span class="hlt">fluxes</span> dominated the <span class="hlt">air-sea</span> gas exchange of HHCB and AHTN, suggesting atmospheric input controls the levels of HHCB and AHTN in the polar region.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001PhDT.......266B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001PhDT.......266B"><span>On the physical <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> for climate modeling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bonekamp, J. G.</p> <p>2001-02-01</p> <p>At the <span class="hlt">sea</span> surface, the atmosphere and the ocean exchange momentum, heat and freshwater. Mechanisms for the exchange are wind stress, turbulent mixing, radiation, evaporation and precipitation. These surface <span class="hlt">fluxes</span> are characterized by a large spatial and temporal variability and play an important role in not only the mean atmospheric and oceanic circulation, but also in the generation and sustainment of coupled climate fluctuations such as the El Niño/La Niña phenomenon. Therefore, a good knowledge of <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> is required for the understanding and prediction of climate changes. As part of long-term comprehensive atmospheric reanalyses with `Numerical Weather Prediction/Data assimilation' systems, data sets of global <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> are generated. A good example is the 15-year atmospheric reanalysis of the European Centre for Medium--Range Weather Forecasts (ECMWF). <span class="hlt">Air-sea</span> <span class="hlt">flux</span> data sets from these reanalyses are very beneficial for climate research, because they combine a good spatial and temporal coverage with a homogeneous and consistent method of calculation. However, atmospheric reanalyses are still imperfect sources of <span class="hlt">flux</span> information due to shortcomings in model variables, model parameterizations, assimilation methods, sampling of observations, and quality of observations. Therefore, assessments of the errors and the usefulness of <span class="hlt">air-sea</span> <span class="hlt">flux</span> data sets from atmospheric (re-)analyses are relevant contributions to the quantitative study of climate variability. Currently, much research is aimed at assessing the quality and usefulness of the reanalysed <span class="hlt">air-sea</span> <span class="hlt">fluxes</span>. Work in this thesis intends to contribute to this assessment. In particular, it attempts to answer three relevant questions. The first question is: What is the best parameterization of the momentum <span class="hlt">flux</span>? A comparison is made of the wind stress parameterization of the ERA15 reanalysis, the currently generated ERA40 reanalysis and the wind stress measurements over the open ocean. The</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018BGeo...15.3331N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018BGeo...15.3331N"><span><span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> over young and snow-covered Arctic pack ice in winter and spring</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nomura, Daiki; Granskog, Mats A.; Fransson, Agneta; Chierici, Melissa; Silyakova, Anna; Ohshima, Kay I.; Cohen, Lana; Delille, Bruno; Hudson, Stephen R.; Dieckmann, Gerhard S.</p> <p>2018-06-01</p> <p>Rare <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> measurements from Arctic pack ice show that two types of ice contribute to the release of <span class="hlt">CO</span><span class="hlt">2</span> from the ice to the atmosphere during winter and spring: young, thin ice with a thin layer of snow and older (several weeks), thicker ice with thick snow cover. Young, thin <span class="hlt">sea</span> ice is characterized by high salinity and high porosity, and snow-covered thick ice remains relatively warm ( > -7.5 °C) due to the insulating snow cover despite <span class="hlt">air</span> temperatures as low as -40 °C. Therefore, brine volume fractions of these two ice types are high enough to provide favorable conditions for gas exchange between <span class="hlt">sea</span> ice and the atmosphere even in mid-winter. Although the potential <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> from <span class="hlt">sea</span> ice decreased due to the presence of the snow, the snow surface is still a <span class="hlt">CO</span><span class="hlt">2</span> source to the atmosphere for low snow density and thin snow conditions. We found that young <span class="hlt">sea</span> ice that is formed in leads without snow cover produces <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> an order of magnitude higher than those in snow-covered older ice (+1.0 ± 0.6 mmol C m-<span class="hlt">2</span> day-1 for young ice and +0.<span class="hlt">2</span> ± 0.<span class="hlt">2</span> mmol C m-<span class="hlt">2</span> day-1 for older ice).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70102289','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70102289"><span><span class="hlt">Air</span>-water gas exchange and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> in a mangrove-dominated estuary</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Ho, David T.; Ferrón, Sara; Engel, Victor C.; Larsen, Laurel G.; Barr, Jordan G.</p> <p>2014-01-01</p> <p>Mangrove forests are highly productive ecosystems, but the fate of mangrove-derived carbon remains uncertain. Part of that uncertainty stems from the fact that gas transfer velocities in mangrove-surrounded waters are not well determined, leading to uncertainty in <span class="hlt">air</span>-water <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. Two SF6 tracer release experiments were conducted to determine gas transfer velocities (k(600) = 8.3 ± 0.4 and 8.1 ± 0.6 cm h−1), along with simultaneous measurements of p<span class="hlt">CO</span><span class="hlt">2</span> to determine the <span class="hlt">air</span>-water <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> from Shark River, Florida (232.11 ± 23.69 and 171.13 ± 20.28 mmol C m−<span class="hlt">2</span> d−1), an estuary within the largest contiguous mangrove forest in North America. The gas transfer velocity results are consistent with turbulent kinetic energy dissipation measurements, indicating a higher rate of turbulence and gas exchange than predicted by commonly used wind speed/gas exchange parameterizations. The results have important implications for carbon <span class="hlt">fluxes</span> in mangrove ecosystems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25377990','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25377990"><span>A <span class="hlt">flux</span>-gradient system for simultaneous measurement of the CH4, <span class="hlt">CO</span><span class="hlt">2</span>, and H<span class="hlt">2</span>O <span class="hlt">fluxes</span> at a lake-<span class="hlt">air</span> interface.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Xiao, Wei; Liu, Shoudong; Li, Hanchao; Xiao, Qitao; Wang, Wei; Hu, Zhenghua; Hu, Cheng; Gao, Yunqiu; Shen, Jing; Zhao, Xiaoyan; Zhang, Mi; Lee, Xuhui</p> <p>2014-12-16</p> <p>Inland lakes play important roles in water and greenhouse gas cycling in the environment. This study aims to test the performance of a <span class="hlt">flux</span>-gradient system for simultaneous measurement of the <span class="hlt">fluxes</span> of water vapor, <span class="hlt">CO</span><span class="hlt">2</span>, and CH4 at a lake-<span class="hlt">air</span> interface. The concentration gradients over the water surface were measured with an analyzer based on the wavelength-scanned cavity ring-down spectroscopy technology, and the eddy diffusivity was measured with a sonic anemometer. Results of a zero-gradient test indicate a <span class="hlt">flux</span> measurement precision of 4.8 W m(-<span class="hlt">2</span>) for water vapor, 0.010 mg m(-<span class="hlt">2</span>) s(-1) for <span class="hlt">CO</span><span class="hlt">2</span>, and 0.029 μg m(-<span class="hlt">2</span>) s(-1) for CH4. During the 620 day measurement period, 97%, 69%, and 67% of H<span class="hlt">2</span>O, <span class="hlt">CO</span><span class="hlt">2</span>, and CH4 hourly <span class="hlt">fluxes</span> were higher in magnitude than the measurement precision, which confirms that the <span class="hlt">flux</span>-gradient system had adequate precision for the measurement of the lake-<span class="hlt">air</span> exchanges. This study illustrates four strengths of the <span class="hlt">flux</span>-gradient method: (1) the ability to simultaneously measure the <span class="hlt">flux</span> of H<span class="hlt">2</span>O, <span class="hlt">CO</span><span class="hlt">2</span>, and CH4; (<span class="hlt">2</span>) negligibly small density corrections; (3) the ability to resolve small CH4 gradient and <span class="hlt">flux</span>; and (4) continuous and noninvasive operation. The annual mean CH4 <span class="hlt">flux</span> (1.8 g CH4 m(-<span class="hlt">2</span>) year(-1)) at this hypereutrophic lake was close to the median value for inland lakes in the world (1.6 g CH4 m(-<span class="hlt">2</span>) year(-1)). The system has adequate precision for CH4 <span class="hlt">flux</span> for broad applications but requires further improvement to resolve small <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> in many lakes.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_1");'>1</a></li> <li><a href="#" onclick='return showDiv("page_2");'>2</a></li> <li class="active"><span>3</span></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_3 --> <div id="page_4" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_2");'>2</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li class="active"><span>4</span></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="61"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.1180C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.1180C"><span>On which timescales do gas transfer velocities control North Atlantic <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> variability?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Couldrey, Matthew; Oliver, Kevin; Yool, Andrew; Halloran, Paul; Achterberg, Eric</p> <p>2016-04-01</p> <p>The North Atlantic is an important basin for the global ocean's uptake of anthropogenic and natural carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>), but the mechanisms controlling this carbon <span class="hlt">flux</span> are not fully understood. The <span class="hlt">air-sea</span> <span class="hlt">flux</span> of <span class="hlt">CO</span><span class="hlt">2</span>, F, is the product of a gas transfer velocity, k, the <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span>concentration gradient, Δp<span class="hlt">CO</span><span class="hlt">2</span>, and the temperature and salinity-dependent solubility coefficient, α. k is difficult to constrain, representing the dominant uncertainty in F on short (instantaneous to interannual) timescales. Previous work shows that in the North Atlantic, Δp<span class="hlt">CO</span><span class="hlt">2</span>and k both contribute significantly to interannual F variability, but that k is unimportant for multidecadal variability. On some timescale between interannual and multidecadal, gas transfer velocity variability and its associated uncertainty become negligible. Here, we quantify this critical timescale for the first time. Using an ocean model, we determine the importance of k, Δp<span class="hlt">CO</span><span class="hlt">2</span>and α on a range of timescales. On interannual and shorter timescales, both Δp<span class="hlt">CO</span><span class="hlt">2</span>and k are important controls on F. In contrast, pentadal to multidecadal North Atlantic <span class="hlt">flux</span> variability is driven almost entirely by Δp<span class="hlt">CO</span><span class="hlt">2</span>; k contributes less than 25%. Finally, we explore how accurately one can estimate North Atlantic F without a knowledge of non-seasonal k variability, finding it possible for interannual and longer timescales. These findings suggest that continued efforts to better constrain gas transfer velocities are necessary to quantify interannual variability in the North Atlantic carbon sink. However, uncertainty in k variability is unlikely to limit the accuracy of estimates of longer term <span class="hlt">flux</span> variability.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016GBioC..30..787C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GBioC..30..787C"><span>On which timescales do gas transfer velocities control North Atlantic <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> variability?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Couldrey, Matthew P.; Oliver, Kevin I. C.; Yool, Andrew; Halloran, Paul R.; Achterberg, Eric P.</p> <p>2016-05-01</p> <p>The North Atlantic is an important basin for the global ocean's uptake of anthropogenic and natural carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>), but the mechanisms controlling this carbon <span class="hlt">flux</span> are not fully understood. The <span class="hlt">air-sea</span> <span class="hlt">flux</span> of <span class="hlt">CO</span><span class="hlt">2</span>, F, is the product of a gas transfer velocity, k, the <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> concentration gradient, Δp<span class="hlt">CO</span><span class="hlt">2</span>, and the temperature- and salinity-dependent solubility coefficient, α. k is difficult to constrain, representing the dominant uncertainty in F on short (instantaneous to interannual) timescales. Previous work shows that in the North Atlantic, Δp<span class="hlt">CO</span><span class="hlt">2</span> and k both contribute significantly to interannual F variability but that k is unimportant for multidecadal variability. On some timescale between interannual and multidecadal, gas transfer velocity variability and its associated uncertainty become negligible. Here we quantify this critical timescale for the first time. Using an ocean model, we determine the importance of k, Δp<span class="hlt">CO</span><span class="hlt">2</span>, and α on a range of timescales. On interannual and shorter timescales, both Δp<span class="hlt">CO</span><span class="hlt">2</span> and k are important controls on F. In contrast, pentadal to multidecadal North Atlantic <span class="hlt">flux</span> variability is driven almost entirely by Δp<span class="hlt">CO</span><span class="hlt">2</span>; k contributes less than 25%. Finally, we explore how accurately one can estimate North Atlantic F without a knowledge of nonseasonal k variability, finding it possible for interannual and longer timescales. These findings suggest that continued efforts to better constrain gas transfer velocities are necessary to quantify interannual variability in the North Atlantic carbon sink. However, uncertainty in k variability is unlikely to limit the accuracy of estimates of longer-term <span class="hlt">flux</span> variability.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSAH23A..06C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSAH23A..06C"><span>On which timescales do gas transfer velocities control North Atlantic <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> variability?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Couldrey, M.; Oliver, K. I. C.; Yool, A.; Halloran, P. R.; Achterberg, E. P.</p> <p>2016-02-01</p> <p>The North Atlantic is an important basin for the global ocean's uptake of anthropogenic and natural carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>), but the mechanisms controlling this carbon <span class="hlt">flux</span> are not fully understood. The <span class="hlt">air-sea</span> <span class="hlt">flux</span> of <span class="hlt">CO</span><span class="hlt">2</span>, F, is the product of a gas transfer velocity, k, the <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> concentration gradient, Δp<span class="hlt">CO</span><span class="hlt">2</span>, and the temperature and salinity-dependent solubility coefficient, α. k is difficult to constrain, representing the dominant uncertainty in F on short (instantaneous to interannual) timescales. Previous work shows that in the North Atlantic, Δp<span class="hlt">CO</span><span class="hlt">2</span> and k both contribute significantly to interannual F variability, but that k is unimportant for multidecadal variability. On some timescale between interannual and multidecadal, gas transfer velocity variability and its associated uncertainty become negligible. Here, we quantify this critical timescale for the first time. Using an ocean model, we determine the importance of k, Δp<span class="hlt">CO</span><span class="hlt">2</span> and α on a range of timescales. On interannual and shorter timescales, both Δp<span class="hlt">CO</span><span class="hlt">2</span> and k are important controls on F. In contrast, pentadal to multidecadal North Atlantic <span class="hlt">flux</span> variability is driven almost entirely by Δp<span class="hlt">CO</span><span class="hlt">2</span>; k contributes less than 25%. Finally, we explore how accurately one can estimate North Atlantic F without a knowledge of non-seasonal k variability, finding it possible for interannual and longer timescales. These findings suggest that continued efforts to better constrain gas transfer velocities are necessary to quantify interannual variability in the North Atlantic carbon sink. However, uncertainty in k variability is unlikely to limit the accuracy of estimates of longer term <span class="hlt">flux</span> variability.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.4722B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.4722B"><span>Regulation of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Air</span> <span class="hlt">Sea</span> <span class="hlt">Fluxes</span> by Sediments in the North <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Burt, William; Thomas, Helmuth; Hagens, Mathilde; Brenner, Heiko; Pätsch, Johannes; Clargo, Nicola; Salt, Lesley</p> <p>2016-04-01</p> <p>A multi-tracer approach is applied to assess the impact of boundary <span class="hlt">fluxes</span> (e.g. benthic input from sediments or lateral inputs from the coastline) on the acid-base buffering capacity, and overall biogeochemistry, of the North <span class="hlt">Sea</span>. Analyses of both basin-wide observations in the North <span class="hlt">Sea</span> and transects through tidal basins at the North-Frisian coastline, reveal that surface distributions of the δ13C signature of dissolved inorganic carbon (DIC) are predominantly controlled by a balance between biological production and respiration. In particular, variability in metabolic DIC throughout stations in the well-mixed southern North <span class="hlt">Sea</span> indicates the presence of an external carbon source, which is traced to the European continental coastline using naturally-occurring radium isotopes (224Ra and 228Ra). 228Ra is also shown to be a highly effective tracer of North <span class="hlt">Sea</span> total alkalinity (AT) compared to the more conventional use of salinity. Coastal inputs of metabolic DIC and AT are calculated on a basin-wide scale, and ratios of these inputs suggest denitrification as a primary metabolic pathway for their formation. The AT input paralleling the metabolic DIC release prevents a significant decline in pH as compared to aerobic (i.e. unbuffered) release of metabolic DIC. Finally, long-term pH trends mimic those of riverine nitrate loading, highlighting the importance of coastal AT production via denitrification in regulating pH in the southern North <span class="hlt">Sea</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.A51E0162M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.A51E0162M"><span><span class="hlt">Sea</span> spray contributions to the <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> at moderate and hurricane wind speeds</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mueller, J. A.; Veron, F.</p> <p>2009-12-01</p> <p>At sufficiently high wind speed conditions, the surface of the ocean separates to form a substantial number of <span class="hlt">sea</span> spray drops, which can account for a significant fraction of the total <span class="hlt">air-sea</span> surface area and thus make important contributions to the aggregate <span class="hlt">air-sea</span> momentum, heat and mass <span class="hlt">fluxes</span>. Although consensus around the qualitative impacts of these drops has been building in recent years, the quantification of their impacts has remained elusive. Ultimately, the spray-mediated <span class="hlt">fluxes</span> depend on three controlling factors: the number and size of drops formed at the surface, the duration of suspension within the atmospheric marine boundary layer, and the rate of momentum, heat and mass transfer between the drops and the atmosphere. While the latter factor can be estimated from an established, physically-based theory, the estimates for the former two are not well established. Using a recent, physically-based model of the <span class="hlt">sea</span> spray source function along with the results from Lagrangian stochastic simulations of individual drops, we estimate the aggregate spray-mediated <span class="hlt">fluxes</span>, finding reasonable agreement with existing models and estimates within the empirical range of wind speed conditions. At high wind speed conditions that are outside the empirical range, however, we find somewhat lower spray-mediated <span class="hlt">fluxes</span> than previously reported in the literature, raising new questions about the relative <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> at high wind speeds as well as the development and sustainment of hurricanes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.8460M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.8460M"><span>Revisiting the estimation of the North <span class="hlt">Sea</span> <span class="hlt">air-sea</span> <span class="hlt">flux</span> of <span class="hlt">CO</span><span class="hlt">2</span> in 2001/02</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Meyer, Maybritt; Paetsch, Johannes; Geyer, Beate; Thomas, Helmuth</p> <p>2017-04-01</p> <p>Based on seasonal observations of p<span class="hlt">CO</span><span class="hlt">2</span> and 6-hourly wind data derived from ERA-40 reanalysis data Thomas et al. (2004) estimated the annual North <span class="hlt">Sea</span> net uptake of <span class="hlt">CO</span><span class="hlt">2</span> for the years 2001/02. The wind data were provided by the ECMWF with a spatial resolution of 1.125˚ (ECMWF, 2005). An updated estimate has now been achieved by using the more appropriate wind data set coastDat<span class="hlt">2</span> (Geyer, 2014) resulting from atmospheric hourly hindcast for Europe and the North Atlantic using COSMO-CLM version 4.8_clm_11 with spectral nudging from 1948-2015. The model uses a grid point distance of 0.22 degrees with an extension of about 68˚ W to 82˚ E, 25.6˚ N to 81.4˚ N. It could be shown that coastDat<span class="hlt">2</span> rather than ERA-40 data fit to observed hourly observations at the German Weather Service station Helgoland (54.175˚ N, 7.892˚ E). In most cases the coastDat<span class="hlt">2</span> values are larger than the ERA-40 values. The comparison of North <span class="hlt">Sea</span> wide <span class="hlt">CO</span><span class="hlt">2</span> uptake yields 1.3 for ERA-40 and 1.8 mol <span class="hlt">CO</span><span class="hlt">2</span> m-<span class="hlt">2</span> a-1 for coastDat<span class="hlt">2</span> wind fields. References Geyer, B., 2014. Earth System Science Data, 6(1): 147-164. Doi:10.5194/essd-6-147-2014. ECMWF, 2005. http://www.ecmwf.int Thomas, H., Bozec, Y., Elkalay, K., de Baar, H.J.W., 2004. Science, 304: 1005-1008.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007GBioC..21.2015S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007GBioC..21.2015S"><span>Constraining global <span class="hlt">air-sea</span> gas exchange for <span class="hlt">CO</span><span class="hlt">2</span> with recent bomb 14C measurements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sweeney, Colm; Gloor, Emanuel; Jacobson, Andrew R.; Key, Robert M.; McKinley, Galen; Sarmiento, Jorge L.; Wanninkhof, Rik</p> <p>2007-06-01</p> <p>The 14<span class="hlt">CO</span><span class="hlt">2</span> released into the stratosphere during bomb testing in the early 1960s provides a global constraint on <span class="hlt">air-sea</span> gas exchange of soluble atmospheric gases like <span class="hlt">CO</span><span class="hlt">2</span>. Using the most complete database of dissolved inorganic radiocarbon, DI14C, available to date and a suite of ocean general circulation models in an inverse mode we recalculate the ocean inventory of bomb-produced DI14C in the global ocean and confirm that there is a 25% decrease from previous estimates using older DI14C data sets. Additionally, we find a 33% lower globally averaged gas transfer velocity for <span class="hlt">CO</span><span class="hlt">2</span> compared to previous estimates (Wanninkhof, 1992) using the NCEP/NCAR Reanalysis 1 1954-2000 where the global mean winds are 6.9 m s-1. Unlike some earlier ocean radiocarbon studies, the implied gas transfer velocity finally closes the gap between small-scale deliberate tracer studies and global-scale estimates. Additionally, the total inventory of bomb-produced radiocarbon in the ocean is now in agreement with global budgets based on radiocarbon measurements made in the stratosphere and troposphere. Using the implied relationship between wind speed and gas transfer velocity ks = 0.27<u102>(Sc/660)-0.5 and standard partial pressure difference climatology of <span class="hlt">CO</span><span class="hlt">2</span> we obtain an net <span class="hlt">air-sea</span> <span class="hlt">flux</span> estimate of 1.3 ± 0.5 PgCyr-1 for 1995. After accounting for the carbon transferred from rivers to the deep ocean, our estimate of oceanic uptake (1.8 ± 0.5 PgCyr-1) compares well with estimates based on ocean inventories, ocean transport inversions using ocean concentration data, and model simulations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1431413','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1431413"><span>Sniffle: a step forward to measure in situ <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">fluxes</span> with the floating chamber technique</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Ribas-Ribas, Mariana; Kilcher, Levi F.; Wurl, Oliver</p> <p></p> <p>Understanding how the ocean absorbs anthropogenic <span class="hlt">CO</span> <span class="hlt">2</span> is critical for predicting climate change. We designed Sniffle, a new autonomous drifting buoy with a floating chamber, to measure gas transfer velocities and <span class="hlt">air-sea</span> <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">fluxes</span> with high spatiotemporal resolution. Currently, insufficient in situ data exist to verify gas transfer parameterizations at low wind speeds (<4 m s -1), which leads to underestimation of gas transfer velocities and, therefore, of <span class="hlt">air-sea</span> <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">fluxes</span>. The Sniffle is equipped with a sensor to consecutively measure aqueous and atmospheric p<span class="hlt">CO</span> <span class="hlt">2</span> and to monitor increases or decreases of <span class="hlt">CO</span> <span class="hlt">2</span> inside themore » chamber. During autonomous operation, a complete cycle lasts 40 minutes, with a new cycle initiated after flushing the chamber. The Sniffle can be deployed for up to 15 hours at wind speeds up to 10 m s -1. Floating chambers often overestimate <span class="hlt">fluxes</span> because they create additional turbulence at the water surface. We correct <span class="hlt">fluxes</span> by measuring turbulence with two acoustic Doppler velocimeters, one positioned directly under the floating chamber and the other positioned sideways, to compare artificial disturbance caused by the chamber and natural turbulence. The first results of deployment in the North <span class="hlt">Sea</span> during the summer of 2016 demonstrate that the new drifting buoy is a useful tool that can improve our understanding of gas transfer velocity with in situ measurements. At low and moderate wind speeds and different conditions, the results obtained indicate that the observed tidal basin was acting as a source of atmospheric <span class="hlt">CO</span> <span class="hlt">2</span>. Wind speed and turbulence alone could not fully explain the variance in gas transfer velocity. We suggest therefore, that other factors like surfactants, rain or tidal current will have an impact on gas transfer parameterizations.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1431413-sniffle-step-forward-measure-situ-co2-fluxes-floating-chamber-technique','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1431413-sniffle-step-forward-measure-situ-co2-fluxes-floating-chamber-technique"><span>Sniffle: a step forward to measure in situ <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">fluxes</span> with the floating chamber technique</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Ribas-Ribas, Mariana; Kilcher, Levi F.; Wurl, Oliver</p> <p>2018-01-09</p> <p>Understanding how the ocean absorbs anthropogenic <span class="hlt">CO</span> <span class="hlt">2</span> is critical for predicting climate change. We designed Sniffle, a new autonomous drifting buoy with a floating chamber, to measure gas transfer velocities and <span class="hlt">air-sea</span> <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">fluxes</span> with high spatiotemporal resolution. Currently, insufficient in situ data exist to verify gas transfer parameterizations at low wind speeds (<4 m s -1), which leads to underestimation of gas transfer velocities and, therefore, of <span class="hlt">air-sea</span> <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">fluxes</span>. The Sniffle is equipped with a sensor to consecutively measure aqueous and atmospheric p<span class="hlt">CO</span> <span class="hlt">2</span> and to monitor increases or decreases of <span class="hlt">CO</span> <span class="hlt">2</span> inside themore » chamber. During autonomous operation, a complete cycle lasts 40 minutes, with a new cycle initiated after flushing the chamber. The Sniffle can be deployed for up to 15 hours at wind speeds up to 10 m s -1. Floating chambers often overestimate <span class="hlt">fluxes</span> because they create additional turbulence at the water surface. We correct <span class="hlt">fluxes</span> by measuring turbulence with two acoustic Doppler velocimeters, one positioned directly under the floating chamber and the other positioned sideways, to compare artificial disturbance caused by the chamber and natural turbulence. The first results of deployment in the North <span class="hlt">Sea</span> during the summer of 2016 demonstrate that the new drifting buoy is a useful tool that can improve our understanding of gas transfer velocity with in situ measurements. At low and moderate wind speeds and different conditions, the results obtained indicate that the observed tidal basin was acting as a source of atmospheric <span class="hlt">CO</span> <span class="hlt">2</span>. Wind speed and turbulence alone could not fully explain the variance in gas transfer velocity. We suggest therefore, that other factors like surfactants, rain or tidal current will have an impact on gas transfer parameterizations.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1614514V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1614514V"><span>CLIVAR-GSOP/GODAE Ocean Synthesis Inter-Comparison of Global <span class="hlt">Air-Sea</span> <span class="hlt">Fluxes</span> From Ocean and Coupled Reanalyses</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Valdivieso, Maria</p> <p>2014-05-01</p> <p>.I. and E.C. Kent (2009), A New <span class="hlt">Air-Sea</span> Interaction Gridded Dataset from ICOADS with Uncertainty Estimates. Bull. Amer. Meteor. Soc 90(5), 645-656. doi: 10.1175/2008BAMS2639.1. Dee, D. P. et al. (2011), The ERA-Interim reanalysis: configuration and performance of the data assimilation system. Q.J.R. Meteorol. Soc., 137: 553-597. doi: 10.1002/qj.828. Kanamitsu M., Ebitsuzaki W., Woolen J., Yang S.K., Hnilo J.J., Fiorino M., Potter G. (2002), NCEP-DOE AMIP-II reanalysis (R-<span class="hlt">2</span>). Bull. Amer. Meteor. Soc., 83:1631-1643. Large, W. and Yeager, S. (2009), The global climatology of an interannually varying <span class="hlt">air-sea</span> <span class="hlt">flux</span> data set. Clim. Dynamics, Volume 33, pp 341-364 Valdivieso, M. and <span class="hlt">co</span>-authors (2014): Heat <span class="hlt">fluxes</span> from ocean and coupled reanalyses, Clivar Exchanges. Issue 64. Yu, L., X. Jin, and R. A. Weller (2008), Multidecade Global <span class="hlt">Flux</span> Datasets from the Objectively Analyzed <span class="hlt">Air-sea</span> <span class="hlt">Fluxes</span> (OAFlux) Project: Latent and Sensible Heat <span class="hlt">Fluxes</span>, Ocean Evaporation, and Related Surface Meteorological Variables. Technical Report OAFlux Project (OA2008-01), Woods Hole Oceanographic Institution. Zhang, Y., WB Rossow, AA Lacis, V Oinas, MI Mishchenk (2004), Calculation of radiative <span class="hlt">fluxes</span> from the surface to top of atmsophere based on ISCCP and other global data sets. Journal of Geophysical Research: Atmospheres (1984-2012) 109 (D19).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRD..122.7664L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRD..122.7664L"><span>Atmospheric deposition and <span class="hlt">air-sea</span> gas exchange <span class="hlt">fluxes</span> of DDT and HCH in the Yangtze River Estuary, East China <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Zhongxia; Lin, Tian; Li, Yuanyuan; Jiang, Yuqing; Guo, Zhigang</p> <p>2017-07-01</p> <p>The Yangtze River Estuary (YRE) is strongly influenced by the Yangtze River and lies on the pathway of the East Asian Monsoon. This study examined atmospheric deposition and <span class="hlt">air-sea</span> gas exchange <span class="hlt">fluxes</span> of dichlorodiphenyltrichloroethane (DDT) and hexachlorocyclohexane (HCH) to determine whether the YRE is a sink or source of selected pesticides at the <span class="hlt">air</span>-water interface under the influences of river input and atmospheric transport. The <span class="hlt">air-sea</span> gas exchange of DDT was characterized by net volatilization with a marked difference in its <span class="hlt">fluxes</span> between summer (140 ng/m<span class="hlt">2</span>/d) and the other three seasons (12 ng/m<span class="hlt">2</span>/d), possibly due to the high surface seawater temperatures and larger riverine input in summer. However, there was no obvious seasonal variation in the atmospheric HCH deposition, and the <span class="hlt">air-sea</span> gas exchange reached equilibrium because of low HCH levels in the <span class="hlt">air</span> and seawater after the long-term banning of HCH and the degradation. The gas exchange <span class="hlt">flux</span> of HCH was comparable to the dry and wet deposition <span class="hlt">fluxes</span> at the <span class="hlt">air</span>-water interface. This suggests that the influences from the Yangtze River input and East Asian continental outflow on the fate of HCH in the YRE were limited. The gas exchange <span class="hlt">flux</span> of DDT was about fivefold higher than the total dry and wet deposition <span class="hlt">fluxes</span>. DDT residues in agricultural soil transported by enhanced riverine runoff were responsible for sustaining such a high net volatilization in summer. Moreover, our results indicated that there were fresh sources of DDT from the local environment to sustain net volatilization throughout the year.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOS.A21A..04P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOS.A21A..04P"><span>Motion-Correlated Flow Distortion and Wave-Induced Biases in <span class="hlt">Air-Sea</span> <span class="hlt">Flux</span> Measurements From Ships</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Prytherch, J.; Yelland, M. J.; Brooks, I. M.; Tupman, D. J.; Pascal, R. W.; Moat, B. I.; Norris, S. J.</p> <p>2016-02-01</p> <p>Direct measurements of the turbulent <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> of momentum, heat, moisture and gases are often made using sensors mounted on ships. Ship-based turbulent wind measurements are corrected for platform motion using well established techniques, but biases at scales associated with wave and platform motion are often still apparent in the <span class="hlt">flux</span> measurements. It has been uncertain whether this signal is due to time-varying distortion of the <span class="hlt">air</span> flow over the platform, or to wind-wave interactions impacting the turbulence. Methods for removing such motion-scale biases from scalar measurements have previously been published but their application to momentum <span class="hlt">flux</span> measurements remains controversial. Here we use eddy covariance momentum <span class="hlt">flux</span> measurements obtained onboard RRS James Clark Ross as part of the Waves, Aerosol and Gas Exchange Study (WAGES), a programme of near-continuous measurements using the autonomous Auto<span class="hlt">Flux</span> system (Yelland et al., 2009). Measurements were made in 2013 in locations throughout the North and South Atlantic, the Southern Ocean and the Arctic Ocean, at latitudes ranging from 62°S to 75°N. We show that the measured motion-scale bias has a dependence on the horizontal ship velocity, and that a correction for it reduces the dependence of the measured momentum <span class="hlt">flux</span> on the orientation of the ship to the wind. We conclude that the bias is due to experimental error, and that time-varying motion-dependent flow distortion is the likely source. Yelland, M., Pascal, R., Taylor, P. and Moat, B.: Auto<span class="hlt">Flux</span>: an autonomous system for the direct measurement of the <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> of <span class="hlt">CO</span><span class="hlt">2</span>, heat and momentum. J. Operation. Oceanogr., 15-23, doi:10.1080/1755876X.2009.11020105, 2009.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.8661B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.8661B"><span>Oxygen in the Southern Ocean From Argo Floats: Determination of Processes Driving <span class="hlt">Air-Sea</span> <span class="hlt">Fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bushinsky, Seth M.; Gray, Alison R.; Johnson, Kenneth S.; Sarmiento, Jorge L.</p> <p>2017-11-01</p> <p>The Southern Ocean is of outsized significance to the global oxygen and carbon cycles with relatively poor measurement coverage due to harsh winters and seasonal ice cover. In this study, we use recent advances in the parameterization of <span class="hlt">air-sea</span> oxygen <span class="hlt">fluxes</span> to analyze 9 years of oxygen data from a recalibrated Argo oxygen data set and from <span class="hlt">air</span>-calibrated oxygen floats deployed as part of the Southern Ocean Carbon and Climate Observations and Modeling (SOCCOM) project. From this combined data set of 150 floats, we find a total Southern Ocean oxygen sink of -183 ± 80 Tmol yr-1 (positive to the atmosphere), greater than prior estimates. The uptake occurs primarily in the Polar-Frontal Antarctic Zone (PAZ, -94 ± 30 Tmol O<span class="hlt">2</span> yr-1) and Seasonal Ice Zone (SIZ, -111 ± 9.3 Tmol O<span class="hlt">2</span> yr-1). This <span class="hlt">flux</span> is driven by wintertime ventilation, with a large portion of the <span class="hlt">flux</span> in the SIZ passing through regions with fractional <span class="hlt">sea</span> ice. The Subtropical Zone (STZ) is seasonally driven by thermal <span class="hlt">fluxes</span> and exhibits a net outgassing of 47 ± 29 Tmol O<span class="hlt">2</span> yr-1 that is likely driven by biological production. The Subantarctic Zone (SAZ) uptake is -25 ± 12 Tmol O<span class="hlt">2</span> yr-1. Total oxygen <span class="hlt">fluxes</span> were separated into a thermal and nonthermal component. The nonthermal <span class="hlt">flux</span> is correlated with net primary production and mixed layer depth in the STZ, SAZ, and PAZ, but not in the SIZ where seasonal <span class="hlt">sea</span> ice slows the <span class="hlt">air-sea</span> gas <span class="hlt">flux</span> response to the entrainment of deep, low-oxygen waters.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014BGD....1112255P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014BGD....1112255P"><span>Remote sensing algorithm for <span class="hlt">sea</span> surface <span class="hlt">CO</span><span class="hlt">2</span> in the Baltic <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Parard, G.; Charantonis, A. A.; Rutgerson, A.</p> <p>2014-08-01</p> <p>Studies of coastal <span class="hlt">seas</span> in Europe have brought forth the high variability in the <span class="hlt">CO</span><span class="hlt">2</span> system. This high variability, generated by the complex mechanisms driving the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> makes their accurate estimation an arduous task. This is more pronounced in the Baltic <span class="hlt">Sea</span>, where the mechanisms driving the <span class="hlt">fluxes</span> have not been as highly detailed as in the open oceans. In adition, the joint availability of in-situ measurements of <span class="hlt">CO</span><span class="hlt">2</span> and of <span class="hlt">sea</span>-surface satellite data is limited in the area. In this paper, a combination of two existing methods (Self-Organizing-Maps and Multiple Linear regression) is used to estimate ocean surface p<span class="hlt">CO</span><span class="hlt">2</span> in the Baltic <span class="hlt">Sea</span> from remotely sensed surface temperature, chlorophyll, coloured dissolved organic matter, net primary production and mixed layer depth. The outputs of this research have an horizontal resolution of 4 km, and cover the period from 1998 to 2011. The reconstructed p<span class="hlt">CO</span><span class="hlt">2</span> values over the validation data set have a correlation of 0.93 with the in-situ measurements, and a root mean square error is of 38 μatm. The removal of any of the satellite parameters degraded this reconstruction of the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span>, and we chose therefore to complete any missing data through statistical imputation. The <span class="hlt">CO</span><span class="hlt">2</span> maps produced by this method also provide a confidence level of the reconstruction at each grid point. The results obtained are encouraging given the sparsity of available data and we expect to be able to produce even more accurate reconstructions in the coming years, in view of the predicted acquisitions of new data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015ECSS..166...13L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015ECSS..166...13L"><span>Net ecosystem production, calcification and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> on a reef flat in Northeastern Brazil</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Longhini, Cybelle M.; Souza, Marcelo F. L.; Silva, Ananda M.</p> <p>2015-12-01</p> <p>The carbon cycle in coral reefs is usually dominated by the organic carbon metabolism and precipitation-dissolution of Ca<span class="hlt">CO</span>3, processes that control the <span class="hlt">CO</span><span class="hlt">2</span> partial pressure (p<span class="hlt">CO</span><span class="hlt">2</span>) in seawater and the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> through the <span class="hlt">air-sea</span> interface. In order to characterize these processes and the carbonate system, four sampling surveys were conducted at the reef flat of Coroa Vermelha during low tide (exposed flat). Net ecosystem production (NEP), net precipitation-dissolution of Ca<span class="hlt">CO</span>3 (G) and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> across the <span class="hlt">air</span>-water interface were calculated. The reef presented net autotrophy and calcification at daytime low tide. The NEP ranged from -8.7 to 31.6 mmol C m-<span class="hlt">2</span> h-1 and calcification from -13.1 to 26.0 mmol C m-<span class="hlt">2</span> h-1. The highest calcification rates occurred in August 2007, coinciding with the greater NEP rates. The daytime <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> varied from -9.7 to 22.6 μmol <span class="hlt">CO</span><span class="hlt">2</span> m-<span class="hlt">2</span> h-1, but reached up to 13,900 μmol <span class="hlt">CO</span><span class="hlt">2</span> m-<span class="hlt">2</span> h-1 during nighttime. Carbon dioxide influx to seawater was predominant in the reef flat during low tide. The regions adjacent to the reef showed a supersaturation of <span class="hlt">CO</span><span class="hlt">2</span>, acting as a source of <span class="hlt">CO</span><span class="hlt">2</span> to the atmosphere (from -22.8 to -<span class="hlt">2</span>.6 mol <span class="hlt">CO</span><span class="hlt">2</span> m-<span class="hlt">2</span> h-1) in the reef flat during ebbing tide. Nighttime gas release to the atmosphere indicates a net <span class="hlt">CO</span><span class="hlt">2</span> release from the Coroa Vermelha reef flat within 24 h, and that these <span class="hlt">fluxes</span> can be important to carbon budget in coral reefs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017OcMod.120...27F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017OcMod.120...27F"><span>Kinetic energy <span class="hlt">flux</span> budget across <span class="hlt">air-sea</span> interface</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fan, Yalin; Hwang, Paul</p> <p>2017-12-01</p> <p>The kinetic energy (KE) <span class="hlt">fluxes</span> into subsurface currents (EFc) is an important boundary condition for ocean circulation models. Traditionally, numerical models assume the KE <span class="hlt">flux</span> from wind (EFair) is identical to EFc, that is, no net KE is gained (or lost) by surface waves. This assumption, however, is invalid when the surface wave field is not fully developed, and acquires KE when it grows in space or time. In this study, numerical experiments are performed to investigate the KE <span class="hlt">flux</span> budget across the <span class="hlt">air-sea</span> interface under both uniform and idealized tropical cyclone (TC) winds. The wave fields are simulated using the WAVEWATCH III model under different wind forcing. The difference between EFair and EFc is estimated using an <span class="hlt">air-sea</span> KE budget model. To address the uncertainty of these estimates resides in the variation of source functions, two source function packages are used for this study: the ST4 source package (Ardhuin et al, 2010), and the ST6 source package (Babanin, 2011). The modeled EFc is significantly reduced relative to EFair under growing <span class="hlt">seas</span> for both the uniform and TC experiments. The reduction can be as large as 20%, and the variation of this ratio is highly dependent on the choice of source function for the wave model. Normalized EFc are found to be consistent with analytical expressions by Hwang and Sletten (2008) and Hwang and Walsh (2016) and field observations by Terray et al. (1996) and Drennan et al. (1996), while the scatters are more widely in the TC cases due to the complexity of the associated wave field. The waves may even give up KE to subsurface currents in the left rear quadrant of fast moving storms. Our results also suggest that the normalized KE <span class="hlt">fluxes</span> may depend on both wave age and friction velocity (u*).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015BGeo...12.3369P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015BGeo...12.3369P"><span>Remote sensing the <span class="hlt">sea</span> surface <span class="hlt">CO</span><span class="hlt">2</span> of the Baltic <span class="hlt">Sea</span> using the SOMLO methodology</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Parard, G.; Charantonis, A. A.; Rutgerson, A.</p> <p>2015-06-01</p> <p>Studies of coastal <span class="hlt">seas</span> in Europe have noted the high variability of the <span class="hlt">CO</span><span class="hlt">2</span> system. This high variability, generated by the complex mechanisms driving the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>, complicates the accurate estimation of these mechanisms. This is particularly pronounced in the Baltic <span class="hlt">Sea</span>, where the mechanisms driving the <span class="hlt">fluxes</span> have not been characterized in as much detail as in the open oceans. In addition, the joint availability of in situ measurements of <span class="hlt">CO</span><span class="hlt">2</span> and of <span class="hlt">sea</span>-surface satellite data is limited in the area. In this paper, we used the SOMLO (self-organizing multiple linear output; Sasse et al., 2013) methodology, which combines two existing methods (i.e. self-organizing maps and multiple linear regression) to estimate the ocean surface partial pressure of <span class="hlt">CO</span><span class="hlt">2</span> (p<span class="hlt">CO</span><span class="hlt">2</span>) in the Baltic <span class="hlt">Sea</span> from the remotely sensed <span class="hlt">sea</span> surface temperature, chlorophyll, coloured dissolved organic matter, net primary production, and mixed-layer depth. The outputs of this research have a horizontal resolution of 4 km and cover the 1998-2011 period. These outputs give a monthly map of the Baltic <span class="hlt">Sea</span> at a very fine spatial resolution. The reconstructed p<span class="hlt">CO</span><span class="hlt">2</span> values over the validation data set have a correlation of 0.93 with the in situ measurements and a root mean square error of 36 μatm. Removing any of the satellite parameters degraded this reconstructed <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span>, so we chose to supply any missing data using statistical imputation. The p<span class="hlt">CO</span><span class="hlt">2</span> maps produced using this method also provide a confidence level of the reconstruction at each grid point. The results obtained are encouraging given the sparsity of available data, and we expect to be able to produce even more accurate reconstructions in coming years, given the predicted acquisition of new data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28334669','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28334669"><span>Distribution and <span class="hlt">sea-to-air</span> <span class="hlt">flux</span> of isoprene in the East China <span class="hlt">Sea</span> and the South Yellow <span class="hlt">Sea</span> during summer.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Li, Jian-Long; Zhang, Hong-Hai; Yang, Gui-Peng</p> <p>2017-07-01</p> <p>Spatial distribution and <span class="hlt">sea-to-air</span> <span class="hlt">flux</span> of isoprene in the East China <span class="hlt">Sea</span> and the South Yellow <span class="hlt">Sea</span> in July 2013 were investigated. This study is the first to report the concentrations of isoprene in the China marginal <span class="hlt">seas</span>. Isoprene concentrations in the surface seawater during summer ranged from 32.46 to 173.5 pM, with an average of 83.62 ± 29.22 pM. Distribution of isoprene in the study area was influenced by the diluted water from the Yangtze River, which stimulated higher in-situ phytoplankton production of isoprene rather than direct freshwater input. Variations in isoprene concentrations were found to be diurnal, with high values observed during daytime. A significant correlation was observed between isoprene and chlorophyll a in the study area. Relatively higher isoprene concentrations were recorded at stations where the phytoplankton biomass was dominated by Chaetoceros, Skeletonema, Pennate-nitzschia, and Thalassiosira. Positive correlation was observed between isoprene and methyl iodide. In addition, <span class="hlt">sea-to-air</span> <span class="hlt">fluxes</span> of isoprene approximately ranged from 22.17 nmol m -<span class="hlt">2</span>  d -1 -537.<span class="hlt">2</span> nmol m -<span class="hlt">2</span>  d -1 , with an average of 161.5 ± 133.3 nmol m -<span class="hlt">2</span>  d -1 . These results indicate that the coastal and shelf areas may be important sources of atmospheric isoprene. Copyright © 2017 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018CSR...152...14Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018CSR...152...14Z"><span><span class="hlt">Air-sea</span> heat <span class="hlt">flux</span> control on the Yellow <span class="hlt">Sea</span> Cold Water Mass intensity and implications for its prediction</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhu, Junying; Shi, Jie; Guo, Xinyu; Gao, Huiwang; Yao, Xiaohong</p> <p>2018-01-01</p> <p>The Yellow <span class="hlt">Sea</span> Cold Water Mass (YSCWM), which occurs during summer in the central Yellow <span class="hlt">Sea</span>, plays an important role in the hydrodynamic field, nutrient cycle and biological species. Based on water temperature observations during the summer from 1978 to 1998 in the western Yellow <span class="hlt">Sea</span>, five specific YSCWM years were identified, including two strong years (1984 and 1985), two weak years (1989 and 1995) and one normal year (1992). Using a three-dimensional hydrodynamic model, the YSCWM formation processes in these five years were simulated and compared with observations. In general, the YSCWM began forming in spring, matured in summer and gradually disappeared in autumn of every year. The 8 °C isotherm was used to indicate the YSCWM boundary. The modelled YSCWM areas in the two strong years were approximately two times larger than those in the two weak years. Based on the simulations in the weak year of 1995, ten numerical experiments were performed to quantify the key factors influencing the YSCWM intensity by changing the initial water condition in the previous autumn, <span class="hlt">air-sea</span> heat <span class="hlt">flux</span>, wind, evaporation, precipitation and <span class="hlt">sea</span> level pressure to those in the strong year of 1984, respectively. The results showed that the <span class="hlt">air-sea</span> heat <span class="hlt">flux</span> was the dominant factor influencing the YSCWM intensity, which contributed about 80% of the differences of the YSCWM average water temperature at a depth of 50 m. In addition, the <span class="hlt">air-sea</span> heat <span class="hlt">flux</span> in the previous winter had a determining effect, contributing more than 50% of the differences between the strong and weak YSCWM years. Finally, a simple formula for predicting the YSCWM intensity was established by using the key influencing factors, i.e., the <span class="hlt">sea</span> surface temperature before the cooling season and the <span class="hlt">air-sea</span> heat <span class="hlt">flux</span> during the cooling season from the previous December to the current February. With this formula, instead of a complicated numerical model, we were able to roughly predict the YSCWM intensity for the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25639080','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25639080"><span>[Distribution, <span class="hlt">flux</span> and biological consumption of carbon monoxide in the East China <span class="hlt">Sea</span> and the South Yellow <span class="hlt">Sea</span> in summer].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Jing; Lu, Xiao-Lan; Yang, Gui-Peng; Xu, Guan-Qiu</p> <p>2014-11-01</p> <p>Carbon monoxide (<span class="hlt">CO</span>) concentration distribution, <span class="hlt">sea-to-air</span> <span class="hlt">flux</span> and microbial consumption rate constant, along with atmospheric <span class="hlt">CO</span> mixing ratio, were measured in the East China <span class="hlt">Sea</span> and the South Yellow <span class="hlt">Sea</span> in summer. Atmospheric <span class="hlt">CO</span> mixing ratios varied from 68 x 10(-9) -448 x 10(-9), with an average of 117 x 10(-9) (SD = 68 x 10(-9), n = 36). Overall, the concentrations of atmospheric <span class="hlt">CO</span> displayed a decreasing trend from the coastal stations to the offshore stations. The surface water <span class="hlt">CO</span> concentrations in the investigated area ranged from 0.23-7.10 nmol x L(-1), with an average of <span class="hlt">2</span>.49 nmol x L(-1) (SD = <span class="hlt">2</span>.11, n = 36). The surface water <span class="hlt">CO</span> concentrations were significantly affected by sunlight. Vertical profiles showed that <span class="hlt">CO</span> concentrations rapidly declined with depth, with the maximum values appearing in the surface water. <span class="hlt">CO</span> concentrations exhibited obvious diurnal variations in the study area, with the maximum values being 6-40 folds higher than the minimum values. Minimal concentrations of <span class="hlt">CO</span> all occurred before dawn. However, the maximal concentrations of <span class="hlt">CO</span> occurred at noon. Marked diurnal variation in the concentrations of <span class="hlt">CO</span> in the water column indicated that <span class="hlt">CO</span> was produced primarily by photochemistry. The surface <span class="hlt">CO</span> concentrations were oversaturated relative to the atmospheric concentrations and the saturation factors ranged from 1.99-99.18, with an average of 29.36 (SD = 24.42, n = 29). The East China <span class="hlt">Sea</span> and the South Yellow <span class="hlt">Sea</span> was a net source of atmospheric <span class="hlt">CO</span>. The <span class="hlt">sea-to-air</span> <span class="hlt">fluxes</span> of <span class="hlt">CO</span> in the East China <span class="hlt">Sea</span> and the South Yellow <span class="hlt">Sea</span> ranged 0.37-44.84 μmol x (m<span class="hlt">2</span> x d)(-1), with an average of 12.73 μmol x (m<span class="hlt">2</span> x d)(-1) (SD = 11.40, n = 29). In the incubation experiments, <span class="hlt">CO</span> concentrations decreased exponentially with incubation time and the processes conformed to the first order reaction characteristics. The microbial <span class="hlt">CO</span> consumption rate constants (K(<span class="hlt">co</span>)) in the surface water ranged from 0.12 to 1.45 h(-1), with an average of 0.47 h(-1) (SD = 0</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_2");'>2</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li class="active"><span>4</span></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_4 --> <div id="page_5" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li class="active"><span>5</span></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="81"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014ACPD...1422587Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014ACPD...1422587Z"><span>Constraining terrestrial ecosystem <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> by integrating models of biogeochemistry and atmospheric transport and data of surface carbon <span class="hlt">fluxes</span> and atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentrations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhu, Q.; Zhuang, Q.; Henze, D.; Bowman, K.; Chen, M.; Liu, Y.; He, Y.; Matsueda, H.; Machida, T.; Sawa, Y.; Oechel, W.</p> <p>2014-09-01</p> <p>Regional net carbon <span class="hlt">fluxes</span> of terrestrial ecosystems could be estimated with either biogeochemistry models by assimilating surface carbon <span class="hlt">flux</span> measurements or atmospheric <span class="hlt">CO</span><span class="hlt">2</span> inversions by assimilating observations of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentrations. Here we combine the ecosystem biogeochemistry modeling and atmospheric <span class="hlt">CO</span><span class="hlt">2</span> inverse modeling to investigate the magnitude and spatial distribution of the terrestrial ecosystem <span class="hlt">CO</span><span class="hlt">2</span> sources and sinks. First, we constrain a terrestrial ecosystem model (TEM) at site level by assimilating the observed net ecosystem production (NEP) for various plant functional types. We find that the uncertainties of model parameters are reduced up to 90% and model predictability is greatly improved for all the plant functional types (coefficients of determination are enhanced up to 0.73). We then extrapolate the model to a global scale at a 0.5° × 0.5° resolution to estimate the large-scale terrestrial ecosystem <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>, which serve as prior for atmospheric <span class="hlt">CO</span><span class="hlt">2</span> inversion. Second, we constrain the large-scale terrestrial <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> by assimilating the GLOBALVIEW-<span class="hlt">CO</span><span class="hlt">2</span> and mid-tropospheric <span class="hlt">CO</span><span class="hlt">2</span> retrievals from the Atmospheric Infrared Sounder (<span class="hlt">AIRS</span>) into an atmospheric transport model (GEOS-Chem). The transport inversion estimates that: (1) the annual terrestrial ecosystem carbon sink in 2003 is -<span class="hlt">2</span>.47 Pg C yr-1, which agrees reasonably well with the most recent inter-comparison studies of <span class="hlt">CO</span><span class="hlt">2</span> inversions (-<span class="hlt">2</span>.82 Pg C yr-1); (<span class="hlt">2</span>) North America temperate, Europe and Eurasia temperate regions act as major terrestrial carbon sinks; and (3) The posterior transport model is able to reasonably reproduce the atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentrations, which are validated against Comprehensive Observation Network for TRace gases by <span class="hlt">AIr</span>Liner (CONTRAIL) <span class="hlt">CO</span><span class="hlt">2</span> concentration data. This study indicates that biogeochemistry modeling or atmospheric transport and inverse modeling alone might not be able to well quantify regional terrestrial carbon <span class="hlt">fluxes</span>. However, combining</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005GeoRL..32.8606C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005GeoRL..32.8606C"><span>Control of <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> disequilibria in the subtropical NE Atlantic by planktonic metabolism under the ocean skin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Calleja, María Ll.; Duarte, Carlos M.; Navarro, Nuria; Agustí, Susana</p> <p>2005-04-01</p> <p>The <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> gradient at the subtropical NE Atlantic was strongly dependent on the metabolism of the planktonic community within the top cms, but independent of that of the communities deeper in the water column. Gross primary production (GPP) and community respiration (R) of the planktonic community within the top cms exceeded those of the communities deeper in the water column by >10-fold and >7 fold, respectively. Net autotrophic metabolism (GPP > R) at the top cms of the water column in some stations drove <span class="hlt">CO</span><span class="hlt">2</span> uptake by creating a <span class="hlt">CO</span><span class="hlt">2</span> deficit at the ocean surface, while net heterotrophic metabolism (GPP < R) at the top cms of the water column in other stations resulted in strong <span class="hlt">CO</span><span class="hlt">2</span> supersaturation, driving <span class="hlt">CO</span><span class="hlt">2</span> emissions. These results suggest a strong control of the <span class="hlt">air-sea</span> p<span class="hlt">CO</span><span class="hlt">2</span> anomaly by intense biological processes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23778238','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23778238"><span>An inorganic <span class="hlt">CO</span><span class="hlt">2</span> diffusion and dissolution process explains negative <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in saline/alkaline soils.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ma, Jie; Wang, Zhong-Yuan; Stevenson, Bryan A; Zheng, Xin-Jun; Li, Yan</p> <p>2013-01-01</p> <p>An 'anomalous' negative <span class="hlt">flux</span>, in which carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) enters rather than is released from the ground, was studied in a saline/alkaline soil. Soil sterilization disclosed an inorganic process of <span class="hlt">CO</span><span class="hlt">2</span> dissolution into (during the night) and out of (during the day) the soil solution, driven by variation in soil temperature. Experimental and modeling analysis revealed that pH and soil moisture were the most important determinants of the magnitude of this inorganic <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span>. In the extreme cases of <span class="hlt">air</span>-dried saline/alkaline soils, this inorganic process was predominant. While the diurnal <span class="hlt">flux</span> measured was zero sum, leaching of the dissolved inorganic carbon in the soil solution could potentially effect net carbon ecosystem exchange. This finding implies that an inorganic module should be incorporated when dealing with the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> of saline/alkaline land. Neglecting this inorganic <span class="hlt">flux</span> may induce erroneous or misleading conclusions in interpreting <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> of these ecosystems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3685845','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3685845"><span>An inorganic <span class="hlt">CO</span><span class="hlt">2</span> diffusion and dissolution process explains negative <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in saline/alkaline soils</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Ma, Jie; Wang, Zhong-Yuan; Stevenson, Bryan A.; Zheng, Xin-Jun; Li, Yan</p> <p>2013-01-01</p> <p>An ‘anomalous' negative <span class="hlt">flux</span>, in which carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) enters rather than is released from the ground, was studied in a saline/alkaline soil. Soil sterilization disclosed an inorganic process of <span class="hlt">CO</span><span class="hlt">2</span> dissolution into (during the night) and out of (during the day) the soil solution, driven by variation in soil temperature. Experimental and modeling analysis revealed that pH and soil moisture were the most important determinants of the magnitude of this inorganic <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span>. In the extreme cases of <span class="hlt">air</span>-dried saline/alkaline soils, this inorganic process was predominant. While the diurnal <span class="hlt">flux</span> measured was zero sum, leaching of the dissolved inorganic carbon in the soil solution could potentially effect net carbon ecosystem exchange. This finding implies that an inorganic module should be incorporated when dealing with the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> of saline/alkaline land. Neglecting this inorganic <span class="hlt">flux</span> may induce erroneous or misleading conclusions in interpreting <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> of these ecosystems. PMID:23778238</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5012129','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5012129"><span>The carbon dioxide system on the Mississippi River‐dominated continental shelf in the northern Gulf of Mexico: 1. Distribution and air‐<span class="hlt">sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Huang, Wei‐Jen; Wang, Yongchen; Lohrenz, Steven E.; Murrell, Michael C.</p> <p>2015-01-01</p> <p>Abstract River‐dominated continental shelf environments are active sites of air‐<span class="hlt">sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange. We conducted 13 cruises in the northern Gulf of Mexico, a region strongly influenced by fresh water and nutrients delivered from the Mississippi and Atchafalaya River system. The <span class="hlt">sea</span> surface partial pressure of carbon dioxide (p<span class="hlt">CO</span><span class="hlt">2</span>) was measured, and the air‐<span class="hlt">sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> was calculated. Results show that <span class="hlt">CO</span><span class="hlt">2</span> exchange exhibited a distinct seasonality: the study area was a net sink of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> during spring and early summer, and it was neutral or a weak source of <span class="hlt">CO</span><span class="hlt">2</span> to the atmosphere during midsummer, fall, and winter. Along the salinity gradient, across the shelf, the <span class="hlt">sea</span> surface shifted from a source of <span class="hlt">CO</span><span class="hlt">2</span> in low‐salinity zones (0≤S<17) to a strong <span class="hlt">CO</span><span class="hlt">2</span> sink in the middle‐to‐high‐salinity zones (17≤S<33), and finally was a near‐neutral state in the high‐salinity areas (33≤S<35) and in the open gulf (S≥35). High p<span class="hlt">CO</span><span class="hlt">2</span> values were only observed in narrow regions near freshwater sources, and the distribution of undersaturated p<span class="hlt">CO</span><span class="hlt">2</span> generally reflected the influence of freshwater inputs along the shelf. Systematic analyses of p<span class="hlt">CO</span><span class="hlt">2</span> variation demonstrated the importance of riverine nitrogen export; that is, riverine nitrogen‐enhanced biological removal, along with mixing processes, dominated p<span class="hlt">CO</span><span class="hlt">2</span> variation along the salinity gradient. In addition, extreme or unusual weather events were observed to alter the alongshore p<span class="hlt">CO</span><span class="hlt">2</span> distribution and to affect regional air‐<span class="hlt">sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> estimates. Overall, the study region acted as a net <span class="hlt">CO</span><span class="hlt">2</span> sink of 0.96 ± 3.7 mol m−<span class="hlt">2</span> yr−1 (1.15 ± 4.4 Tg C yr−1). PMID:27656331</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25898645','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25898645"><span>[Partial pressure of <span class="hlt">CO</span><span class="hlt">2</span> and <span class="hlt">CO</span><span class="hlt">2</span> degassing <span class="hlt">fluxes</span> of Huayuankou and Xiaolangdi Station affected by Xiaolangdi Reservoir].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhang, Yong-ling; Yang, Xiao-lin; Zhang, Dong</p> <p>2015-01-01</p> <p>According to periodic sampling analysis per month in Xiaolangdi station and Huayuankou station from November 2011 to October 2012, combined with continuous sampling analysis of Xiaolangdi Reservoir during runoff and sediment control period in 2012, partial pressure of <span class="hlt">CO</span><span class="hlt">2</span> (p<span class="hlt">CO</span><span class="hlt">2</span>) in surface water were calculated based on Henry's Law, p<span class="hlt">CO</span><span class="hlt">2</span> features and <span class="hlt">air</span>-water <span class="hlt">CO</span><span class="hlt">2</span> degassing <span class="hlt">fluxes</span> of Huayuankou station and Xiaolangdi station affected by Xiaolangdi Reservoir were studied. The results were listed as follows, when Xiaolangdi Reservoir operated normally, p<span class="hlt">CO</span><span class="hlt">2</span> in surface water of Xiaolangdi station and Huayuankou station varied from 82 to 195 Pa and from 99 to 228 Pa, moreover, p<span class="hlt">CO</span><span class="hlt">2</span> in surface water from July to September were distinctly higher than those in other months; meanwhile, p<span class="hlt">CO</span>, in surface water from Huayuankou station were higher than that from Xiaolangdi station. During runoff and sediment control period of Xiaolangdi Reservoir, two hydrological stations commonly indicated that p<span class="hlt">CO</span><span class="hlt">2</span> in surface water during water draining were obviously lower than those during sediment releasing. Whether in the period of normal operation or runoff and sediment control, p<span class="hlt">CO</span><span class="hlt">2</span> in surface water had positive relations to DIC content in two hydrological stations. Since the Ep<span class="hlt">CO</span>,/AOU value was higher than the theoretical value of 0. 62, the biological aerobic respiration effect had distinct contribution to p<span class="hlt">CO</span><span class="hlt">2</span>. Throughout the whole year, <span class="hlt">air</span>-water <span class="hlt">CO</span><span class="hlt">2</span> degassing <span class="hlt">fluxes</span> from Xiaolangdi station and Huayuankou station were 0.486 p.mol (m<span class="hlt">2</span> s) -l and 0.588 pmol (m<span class="hlt">2</span> x s)(-1) respectively; When Xiaolangdi Reservoir operated normally, <span class="hlt">air</span>-water <span class="hlt">CO</span>, degassing <span class="hlt">fluxes</span> in Huayuankou station were higher than that in Xiaolangdi station; during runoff and sediment control from Xiaolangdi Reservoir, two hydrological stations had one observation result in common, namely, <span class="hlt">air</span>-water <span class="hlt">CO</span><span class="hlt">2</span> degassing <span class="hlt">fluxes</span> in the period of water draining were obviously lower than that in the period of sediment releasing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013CorRe..32..239W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013CorRe..32..239W"><span>Spatiotemporal variations in <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> in a fringing reef simulated using a novel carbonate system dynamics model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Watanabe, A.; Yamamoto, T.; Nadaoka, K.; Maeda, Y.; Miyajima, T.; Tanaka, Y.; Blanco, A. C.</p> <p>2013-03-01</p> <p>A carbonate system dynamics (CSD) model was developed in a fringing reef on the east coast of Ishigaki Island, southwest Japan, by incorporating organic and inorganic carbon <span class="hlt">fluxes</span> (photosynthesis and calcification), <span class="hlt">air-sea</span> gas exchanges, and benthic cover of coral and seagrass into a three-dimensional hydrodynamic model. The CSD model could reproduce temporal variations in dissolved inorganic carbon (DIC) and total alkalinity in coral zones, but not in seagrass meadows. The poor reproduction in seagrass meadows can be attributed to significant contributions of submarine groundwater discharge as well as misclassification of remotely sensed megabenthos in this area. In comparison with offshore areas, the reef acted as a <span class="hlt">CO</span><span class="hlt">2</span> sink during the observation period when it was averaged over 24 h. The CSD model also indicated large spatiotemporal differences in the carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) sink/source, possibly related to hydrodynamic features such as effective offshore seawater exchange and neap/spring tidal variation. This suggests that the data obtained from a single point observation may lead to misinterpretation of the overall trend and thus should be carefully considered. The model analysis also showed that the advective <span class="hlt">flux</span> of DIC from neighboring grids is several times greater than local biological <span class="hlt">flux</span> of DIC and is three orders of magnitude greater than the <span class="hlt">air-sea</span> gas <span class="hlt">flux</span> at the coral zone. Sensitivity tests in which coral or seagrass covers were altered revealed that the <span class="hlt">CO</span><span class="hlt">2</span> sink potential was much more sensitive to changes in coral cover than seagrass cover.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMGC23K..14F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMGC23K..14F"><span>Carbon <span class="hlt">fluxes</span> in North American coastal and shelf <span class="hlt">seas</span>: Current status and trends</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fennel, K.; Alin, S. R.; Barbero, L.; Evans, W.; Martin Hernandez-Ayon, J. M.; Hu, X.; Lohrenz, S. E.; Muller-Karger, F. E.; Najjar, R.; Robbins, L. L.; Shadwick, E. H.; Siedlecki, S. A.; Steiner, N.; Turk, D.; Vlahos, P.; Wang, A. Z.</p> <p>2016-12-01</p> <p>Coastal and shelf <span class="hlt">seas</span> represent an interface between all major components of the global carbon cycle: land, atmosphere, marine sediments and the ocean. <span class="hlt">Fluxes</span> and transformations of carbon in coastal systems are complex and highly variable in space and time. The First State of the Carbon Cycle Report (http://cdiac.ornl.gov/SOCCR/final.html, Chapter 15, Chavez et al. 2007) concluded that carbon budgets of North American ocean margins were not well quantified because of insufficient observations and the complexity and highly localized spatial variability of coastal carbon dynamics. Since then significant progress has been made through the expansion of carbon observing networks, the implementation of modeling capabilities, and national and international coordination and synthesis activities. We will review the current understanding of coastal carbon <span class="hlt">fluxes</span> around the North American continent including along the Atlantic and Pacific coasts, the northern Gulf of Mexico, and the North American Arctic region and provide a compilation of regional estimates of <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> of <span class="hlt">CO</span><span class="hlt">2</span>. We will discuss generalizable patterns in coastal <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange and other carbon <span class="hlt">fluxes</span> as well as reasons underlying spatial heterogeneity. After providing an overview of the principal modes of carbon export from coastal systems, we will apply these mechanisms to the North American continent, and discuss observed and projected trends of key properties and <span class="hlt">fluxes</span>. The presentation will illustrate that despite significant advances in capabilities and understanding, large uncertainties remain.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140005809','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140005809"><span><span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Flux</span> Estimation Errors Associated with Moist Atmospheric Processes</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Parazoo, N. C.; Denning, A. S.; Kawa, S. R.; Pawson, S.; Lokupitiya, R.</p> <p>2012-01-01</p> <p>Vertical transport by moist sub-grid scale processes such as deep convection is a well-known source of uncertainty in <span class="hlt">CO</span><span class="hlt">2</span> source/sink inversion. However, a dynamical link between vertical transport, satellite based retrievals of column mole fractions of <span class="hlt">CO</span><span class="hlt">2</span>, and source/sink inversion has not yet been established. By using the same offline transport model with meteorological fields from slightly different data assimilation systems, we examine sensitivity of frontal <span class="hlt">CO</span><span class="hlt">2</span> transport and retrieved <span class="hlt">fluxes</span> to different parameterizations of sub-grid vertical transport. We find that frontal transport feeds off background vertical <span class="hlt">CO</span><span class="hlt">2</span> gradients, which are modulated by sub-grid vertical transport. The implication for source/sink estimation is two-fold. First, <span class="hlt">CO</span><span class="hlt">2</span> variations contained in moist poleward moving <span class="hlt">air</span> masses are systematically different from variations in dry equatorward moving <span class="hlt">air</span>. Moist poleward transport is hidden from orbital sensors on satellites, causing a sampling bias, which leads directly to small but systematic <span class="hlt">flux</span> retrieval errors in northern mid-latitudes. Second, differences in the representation of moist sub-grid vertical transport in GEOS-4 and GEOS-5 meteorological fields cause differences in vertical gradients of <span class="hlt">CO</span><span class="hlt">2</span>, which leads to systematic differences in moist poleward and dry equatorward <span class="hlt">CO</span><span class="hlt">2</span> transport and therefore the fraction of <span class="hlt">CO</span><span class="hlt">2</span> variations hidden in moist <span class="hlt">air</span> from satellites. As a result, sampling biases are amplified and regional scale <span class="hlt">flux</span> errors enhanced, most notably in Europe (0.43+/-0.35 PgC /yr). These results, cast from the perspective of moist frontal transport processes, support previous arguments that the vertical gradient of <span class="hlt">CO</span><span class="hlt">2</span> is a major source of uncertainty in source/sink inversion.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1167255','SCIGOV-DOEDE'); return false;" href="https://www.osti.gov/servlets/purl/1167255"><span><span class="hlt">CO</span><span class="hlt">2</span> CH4 <span class="hlt">flux</span> <span class="hlt">Air</span> temperature Soil temperature and Soil moisture, Barrow, Alaska 2013 ver. 1</span></a></p> <p><a target="_blank" href="http://www.osti.gov/dataexplorer">DOE Data Explorer</a></p> <p>Margaret Torn</p> <p>2015-01-14</p> <p>This dataset consists of field measurements of <span class="hlt">CO</span><span class="hlt">2</span> and CH4 <span class="hlt">flux</span>, as well as soil properties made during 2013 in Areas A-D of Intensive Site 1 at the Next-Generation Ecosystem Experiments (NGEE) Arctic site near Barrow, Alaska. Included are i) measurements of <span class="hlt">CO</span><span class="hlt">2</span> and CH4 <span class="hlt">flux</span> made from June to September (ii) Calculation of corresponding Gross Primary Productivity (GPP) and CH4 exchange (transparent minus opaque) between atmosphere and the ecosystem (ii) Measurements of Los Gatos Research (LGR) chamber <span class="hlt">air</span> temperature made from June to September (ii) measurements of surface layer depth, type of surface layer, soil temperature and soil moisture from June to September.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28132774','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28132774"><span>Distribution and <span class="hlt">sea-to-air</span> <span class="hlt">fluxes</span> of volatile halocarbons in the Bohai <span class="hlt">Sea</span> and North Yellow <span class="hlt">Sea</span> during spring.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>He, Zhen; Liu, Qiu-Lin; Zhang, Ying-Jie; Yang, Gui-Peng</p> <p>2017-04-15</p> <p>Concentrations of volatile halocarbons (VHCs), such as CHBr <span class="hlt">2</span> Cl, CHBr 3 , C <span class="hlt">2</span> HCl 3 , and C <span class="hlt">2</span> Cl 4 , in the Bohai <span class="hlt">Sea</span> (BS) and North Yellow <span class="hlt">Sea</span> (NYS) were measured during the spring of 2014. The VHC concentrations varied widely and decreased with distance from the coast in the investigated area, with low values observed in the open <span class="hlt">sea</span>. Depth profiles of the VHCs were characterized by the highest concentration generally found in the upper water column. The distributions of the VHCs in the BS and NYS were clearly influenced by the combined effects of biological production, anthropogenic activities, and riverine input. The <span class="hlt">sea-to-air</span> <span class="hlt">fluxes</span> of CHBr <span class="hlt">2</span> Cl, CHBr 3 , C <span class="hlt">2</span> HCl 3 , and C <span class="hlt">2</span> Cl 4 in the study area were estimated to be 47.17, 56.63, 162.56, and 104.37nmolm -<span class="hlt">2</span> d -1 , respectively, indicating that the investigated area may be a source of atmospheric CHBr <span class="hlt">2</span> Cl, CHBr 3 , C <span class="hlt">2</span> HCl 3 , and C <span class="hlt">2</span> Cl 4 in spring. Copyright © 2017 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013JGRC..118..244G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013JGRC..118..244G"><span>First estimates of the contribution of Ca<span class="hlt">CO</span>3 precipitation to the release of <span class="hlt">CO</span><span class="hlt">2</span> to the atmosphere during young <span class="hlt">sea</span> ice growth</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Geilfus, N.-X.; Carnat, G.; Dieckmann, G. S.; Halden, N.; Nehrke, G.; Papakyriakou, T.; Tison, J.-L.; Delille, B.</p> <p>2013-01-01</p> <p>report measurements of pH, total alkalinity, <span class="hlt">air</span>-ice <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> (chamber method), and Ca<span class="hlt">CO</span>3 content of frost flowers (FF) and thin landfast <span class="hlt">sea</span> ice. As the temperature decreases, concentration of solutes in the brine skim increases. Along this gradual concentration process, some salts reach their solubility threshold and start precipitating. The precipitation of ikaite (Ca<span class="hlt">CO</span>3.6H<span class="hlt">2</span>O) was confirmed in the FF and throughout the ice by Raman spectroscopy and X-ray analysis. The amount of ikaite precipitated was estimated to be 25 µmol kg-1 melted FF, in the FF and is shown to decrease from 19 to 15 µmol kg-1 melted ice in the upper part and at the bottom of the ice, respectively. <span class="hlt">CO</span><span class="hlt">2</span> release due to precipitation of Ca<span class="hlt">CO</span>3 is estimated to be 50 µmol kg-1 melted samples. The dissolved inorganic carbon (DIC) normalized to a salinity of 10 exhibits significant depletion in the upper layer of the ice and in the FF. This DIC loss is estimated to be 2069 µmol kg-1 melted sample and corresponds to a <span class="hlt">CO</span><span class="hlt">2</span> release from the ice to the atmosphere ranging from 20 to 40 mmol m-<span class="hlt">2</span> d-1. This estimate is consistent with <span class="hlt">flux</span> measurements of <span class="hlt">air</span>-ice <span class="hlt">CO</span><span class="hlt">2</span> exchange. Our measurements confirm previous laboratory findings that growing young <span class="hlt">sea</span> ice acts as a source of <span class="hlt">CO</span><span class="hlt">2</span> to the atmosphere. Ca<span class="hlt">CO</span>3 precipitation during early ice growth appears to promote the release of <span class="hlt">CO</span><span class="hlt">2</span> to the atmosphere; however, its contribution to the overall release by newly formed ice is most likely minor.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeoRL..4412324M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoRL..4412324M"><span>Enrichment of Extracellular Carbonic Anhydrase in the <span class="hlt">Sea</span> Surface Microlayer and Its Effect on <span class="hlt">Air-Sea</span> <span class="hlt">CO</span><span class="hlt">2</span> Exchange</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mustaffa, N. I. H.; Striebel, M.; Wurl, O.</p> <p>2017-12-01</p> <p>This paper describes the quantification of extracellular carbonic anhydrase (eCA) concentrations in the <span class="hlt">sea</span> surface microlayer (SML), the boundary layer between the ocean and the atmosphere of the Indo-West Pacific. We demonstrated that the SML is enriched with eCA by 1.5 ± 0.7 compared to the mixed underlying water. Enrichment remains up to a wind speed of 7 m s-1 (i.e., under typical oceanic conditions). As eCA catalyzes the interconversion of HCO3- and <span class="hlt">CO</span><span class="hlt">2</span>, it has been hypothesized that its enrichment in the SML enhances the <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange. We detected concentrations in the range of 0.12 to 0.76 n<fi>M</fi>, which can enhance the exchange by up to 15% based on the model approach described in the literature.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMOS24A..04D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMOS24A..04D"><span>Diagnosis of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Fluxes</span> in the Coastal Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dai, M.; Cao, Z.; Yang, W.; Guo, X.; Yin, Z.; Zhao, Y.</p> <p>2017-12-01</p> <p>Coastal ocean carbon is an important component of the global carbon cycle. However, its mechanistic-based conceptualization, a prerequisite of coastal carbon modeling and its inclusion in the Earth System Model, remains difficult due to the highest variability in both time and space. Here we show that the inter-seasonal change of the global coastal p<span class="hlt">CO</span><span class="hlt">2</span> is more determined by non-temperature factors such as biological drawdown and water mass mixing, the latter of which features the dynamic boundary processes of the coastal ocean at both land-margin and margin-open ocean interfaces. Considering these unique features, we resolve the coastal <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> using a semi-analytical approach coupling physics-biogeochemistry and carbon-nutrients and conceptualize the coastal carbon cycle into Ocean-dominated Margins (OceMar) and River-dominated Ocean Margins (RiOMar). The diagnostic result of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in the South China <span class="hlt">Sea</span> basin and the Arabian <span class="hlt">Sea</span> as OceMars and in the Pearl River Plume as a RioMar is consistent with field observations. Our mechanistic-based diagnostic approach therefore helps better understand and model coastal carbon cycle yet the stoichiometry of carbon-nutrients coupling needs scrutiny when applying our approach.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012BGD.....910331C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012BGD.....910331C"><span><span class="hlt">CO</span><span class="hlt">2</span> exchange in a temperate marginal <span class="hlt">sea</span> of the Mediterranean <span class="hlt">Sea</span>: processes and carbon budget</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cossarini, G.; Querin, S.; Solidoro, C.</p> <p>2012-08-01</p> <p>Marginal <span class="hlt">seas</span> play a potentially important role in the global carbon cycle; however, due to differences in the scales of variability and dynamics, marginal <span class="hlt">seas</span> are seldom fully accounted for in global models or estimates. Specific high-resolution studies may elucidate the role of marginal <span class="hlt">seas</span> and assist in the compilation of a complete global budget. In this study, we investigated the <span class="hlt">air-sea</span> exchange and the carbon cycle dynamics in a marginal sub-basin of the Mediterranean <span class="hlt">Sea</span> (the Adriatic <span class="hlt">Sea</span>) by adopting a coupled transport-biogeochemical model of intermediate complexity including carbonate dynamics. The Adriatic <span class="hlt">Sea</span> is a highly productive area owed to riverine fertilisation and is a site of intense dense water formation both on the northern continental shelf and in the southern sub-basin. Therefore, the study area may be an important site of <span class="hlt">CO</span><span class="hlt">2</span> sequestration in the Mediterranean <span class="hlt">Sea</span>. The results of the model simulation show that the Adriatic <span class="hlt">Sea</span>, as a whole, is a <span class="hlt">CO</span><span class="hlt">2</span> sink with a mean annual <span class="hlt">flux</span> of 36 mg m-<span class="hlt">2</span> day-1. The northern part absorbs more carbon (68 mg m-<span class="hlt">2</span> day-1) due to an efficient continental shelf pump process, whereas the southern part behaves similar to an open ocean. Nonetheless, the Southern Adriatic <span class="hlt">Sea</span> accumulates dense, southward-flowing, carbon-rich water produced on the northern shelf. During a warm year and despite an increase in aquatic primary productivity, the sequestration of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> is reduced by approximately 15% due to alterations of the solubility pump and reduced dense water formation. The seasonal cycle of temperature and biological productivity modulates the efficiency of the carbon pump at the surface, whereas the intensity of winter cooling in the northern sub-basin leads to the export of C-rich dense water to the deep layer of the southern sub-basin and, subsequently, to the interior of the Mediterranean <span class="hlt">Sea</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A43C2468M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A43C2468M"><span>Constraints on Southern Ocean <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Fluxes</span> and Seasonality from Atmospheric Vertical Gradients Observed on Multiple Airborne Campaigns</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>McKain, K.; Sweeney, C.; Stephens, B. B.; Long, M. C.; Jacobson, A. R.; Basu, S.; Chatterjee, A.; Weir, B.; Wofsy, S. C.; Atlas, E. L.; Blake, D. R.; Montzka, S. A.; Stern, R.</p> <p>2017-12-01</p> <p>The Southern Ocean plays an important role in the global carbon cycle and climate system, but net <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> into the Southern Ocean is difficult to measure and model because it results from large opposing and seasonally-varying <span class="hlt">fluxes</span> due to thermal forcing, biological uptake, and deep-water mixing. We present an analysis to constrain the seasonal cycle of net <span class="hlt">CO</span><span class="hlt">2</span> exchange with the Southern Ocean, and the magnitude of summer uptake, using the vertical gradients in atmospheric <span class="hlt">CO</span><span class="hlt">2</span> observed during three aircraft campaigns in the southern polar region. The O<span class="hlt">2</span>/N<span class="hlt">2</span> Ratio and <span class="hlt">CO</span><span class="hlt">2</span> Airborne Southern Ocean Study (ORCAS) was an airborne campaign that intensively sampled the atmosphere at 0-13 km altitude and 45-75 degrees south latitude in the austral summer (January-February) of 2016. The global airborne campaigns, the HIAPER Pole-to-Pole Observations (HIPPO) study and the Atmospheric Tomography Mission (ATom), provide additional measurements over the Southern Ocean from other seasons and multiple years (2009-2011, 2016-2017). Derivation of <span class="hlt">fluxes</span> from measured vertical gradients requires robust estimates of the residence time of <span class="hlt">air</span> in the polar tropospheric domain, and of the contribution of long-range transport from northern latitudes outside the domain to the <span class="hlt">CO</span><span class="hlt">2</span> gradient. We use diverse independent approaches to estimate both terms, including simulations using multiple transport and <span class="hlt">flux</span> models, and observed gradients of shorter-lived tracers with specific sources regions and well-known loss processes. This study demonstrates the utility of aircraft profile measurements for constraining large-scale <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> for the Southern Ocean, in contrast to those derived from the extrapolation of sparse ocean and atmospheric measurements and uncertain <span class="hlt">flux</span> parameterizations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..1210133Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..1210133Z"><span><span class="hlt">Air-sea</span> <span class="hlt">fluxes</span> of momentum and mass in the presence of wind waves</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zülicke, Christoph</p> <p>2010-05-01</p> <p>An <span class="hlt">air-sea</span> interaction model (ASIM) is developed including the effect of wind waves on momentum and mass transfer. This includes the derivation of profiles of dissipation rate, flow speed and concentration from a certain height to a certain depth. Simplified assumptions on the turbulent closure, skin - bulk matching and the spectral wave model allow for an analytic treatment. Particular emphasis was put on the inclusion of primary (gravity) waves and secondary (capillary-gravity) waves. The model was tuned to match wall-flow theory and data on wave height and slope. Growing waves reduce the <span class="hlt">air</span>-side turbulent stress and lead to an increasing drag coefficient. In the <span class="hlt">sea</span>, breaking waves inject turbulent kinetic energy and accelerate the transfer. Cross-reference with data on wave-related momentum and energy <span class="hlt">flux</span>, dissipation rate and transfer velocity was sufficient. The evaluation of ASIM allowed for the analytical calculation of bulk formulae for the wind-dependent gas transfer velocity including information on the <span class="hlt">air</span>-side momentum transfer (drag coefficient) and the <span class="hlt">sea</span>-side gas transfer (Dalton number). The following regimes have been identified: the smooth waveless regime with a transfer velocity proportional to (wind) × (diffusion)<span class="hlt">2</span>-3, the primary wave regime with a wind speed dependence proportional to (wind)1-4 × (diffusion)1-<span class="hlt">2</span>-(waveage)1-4 and the secondary wave regime including a more-than-linear wind speed dependence like (wind)15-8 × (diffusion)1-<span class="hlt">2</span> × (waveage)5-8. These findings complete the current understanding of <span class="hlt">air-sea</span> interaction for medium winds between <span class="hlt">2</span> and 20 m s^-1.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOS.B34A0337O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOS.B34A0337O"><span>Are changes in the phytoplankton community structure altering the <span class="hlt">flux</span> of <span class="hlt">CO</span><span class="hlt">2</span> in regions of the North Atlantic?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ostle, C.; Landschutzer, P.; Johnson, M.; Schuster, U.; Watson, A. J.; Edwards, M.; Robinson, C.</p> <p>2016-02-01</p> <p>The North Atlantic Ocean is a globally important sink of carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>). However, the strength of the sink varies temporally and regionally. This study uses a neural network method to map the surface ocean p<span class="hlt">CO</span><span class="hlt">2</span> (partial pressure of <span class="hlt">CO</span><span class="hlt">2</span>) and <span class="hlt">flux</span> of <span class="hlt">CO</span><span class="hlt">2</span>from the atmosphere to the ocean alongside measurements of plankton abundance collected from the Continuous Plankton Recorder (CPR) survey to determine the relationship between regional changes in phytoplankton community structure and regional differences in carbon <span class="hlt">flux</span>. Despite increasing <span class="hlt">sea</span> surface temperatures, the Grand Banks of Newfoundland show a decrease in <span class="hlt">sea</span> surface p<span class="hlt">CO</span><span class="hlt">2</span> of -<span class="hlt">2</span> µatm yr-1 from 1993 to 2011. The carbon <span class="hlt">flux</span> in the North <span class="hlt">Sea</span> is variable over the same period. This is in contrast to most of the open ocean within the North Atlantic, where increases in <span class="hlt">sea</span> surface p<span class="hlt">CO</span><span class="hlt">2</span> follow the trend of increasing <span class="hlt">CO</span><span class="hlt">2</span> in the atmosphere, i.e. the <span class="hlt">flux</span> or sink remains constant. The increasing <span class="hlt">CO</span><span class="hlt">2</span> sink in the Grand Banks of Newfoundland and the variable sink in the North <span class="hlt">Sea</span> correlate with changes in phytoplankton community composition. This study investigates the biogeochemical and oceanographic mechanisms potentially linking increasing <span class="hlt">sea</span> surface temperature, changes in phytoplankton community structure and the changing carbon sink in these two important regions of the Atlantic Ocean. The use of volunteer ships to concurrently collect these datasets demonstrates the potential to investigate relationships between plankton community structure and carbon <span class="hlt">flux</span> in a cost-effective way. These results not only have implications for plankton-dynamic biogeochemical models, but also likely influence carbon export, as different phytoplankton communities have different carbon export efficiencies. Extending and maintaining such datasets is critical to improving our understanding of and monitoring carbon cycling in the surface ocean and improving climate model accuracy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.B41B0407B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.B41B0407B"><span>Field evaluation of open and closed-path <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> systems over asphalt surface</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bogoev, I.; Santos, E.</p> <p>2016-12-01</p> <p>Eddy covariance (EC) is a widely used method for quantifying surface <span class="hlt">fluxes</span> of heat, water vapor and carbon dioxide between ecosystems and the atmosphere. A typical EC system consists of an ultrasonic anemometer measuring the 3D wind vector and a fast-response infrared gas analyzer for sensing the water vapor and <span class="hlt">CO</span><span class="hlt">2</span> density in the <span class="hlt">air</span>. When using an open-path analyzer that detects the constituent's density in situ a correction for concurrent <span class="hlt">air</span> temperature and humidity fluctuations must be applied, Webb et al. (1980). In environments with small magnitudes of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> (<5µmol m-<span class="hlt">2</span> s-1) and in the presence of high sensible heat <span class="hlt">flux</span>, like wintertime over boreal forest, open-path <span class="hlt">flux</span> measurements have been challenging since the magnitude of the density corrections are as large as the uncorrected <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> itself. A new technology merging the sensing paths of the gas analyzer and the sonic anemometer has been recently developed. This new integrated instrument allows a direct measurement of <span class="hlt">CO</span><span class="hlt">2</span> mixing ratio in the open <span class="hlt">air</span> and has the potential to improve the quality of the temperature related density corrections by synchronously measuring the sensible heat <span class="hlt">flux</span> in the optical path of the gas analyzer. We evaluate the performance and the accuracy of this new sensor over a large parking lot with an asphalt surface where the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> are considered low and the interfering sensible heat <span class="hlt">fluxes</span> are above 200 Wm-<span class="hlt">2</span>. A <span class="hlt">co</span>-located closed-path EC system is used as a reference measurement to examine any systematic biases and apparent <span class="hlt">CO</span><span class="hlt">2</span> uptake observed with open-path sensors under high sensible heat <span class="hlt">flux</span> regimes. Half-hour mean and variance of <span class="hlt">CO</span><span class="hlt">2</span> and water vapor concentrations are evaluated. The relative spectral responses, covariances and corrected turbulent <span class="hlt">fluxes</span> using a common sonic anemometer are analyzed. The influence of sensor separation and frequency response attenuation on the density corrections is discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20010022991','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20010022991"><span>BOREAS TF-3 Automated Chamber <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Flux</span> Data from the NSA-OBS</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Goulden, Michael L.; Crill, Patrick M.; Hall, Forrest G. (Editor); Conrad, Sara (Editor)</p> <p>2000-01-01</p> <p>The BOReal Ecosystem Atmosphere Study Tower <span class="hlt">Flux</span> (BOREAS TF-3) and Trace Gas Biogeochemistry (TGB-1) teams collected automated <span class="hlt">CO</span><span class="hlt">2</span> chamber <span class="hlt">flux</span> data in their efforts to fully describe the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> at the Northern Study Area-Old Black Spruce (NSA-OBS) site. This data set contains <span class="hlt">fluxes</span> of <span class="hlt">CO</span><span class="hlt">2</span> at the NSA-OBS site measured using automated chambers. In addition to reporting the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span>, it reports chamber <span class="hlt">air</span> temperature, moss temperature, and light levels during each measurement. The data set covers the period from 23-Sep-1995 through 26-Oct-1995 and from 28-May-1996 through 21-Oct-1996. The data are stored in tabular ASCII files.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li class="active"><span>5</span></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_5 --> <div id="page_6" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li class="active"><span>6</span></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="101"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20010022990','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20010022990"><span>BOREAS TF-4 <span class="hlt">CO</span><span class="hlt">2</span> and CH4 Chamber <span class="hlt">Flux</span> Data from the SSA</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Anderson, Dean; Striegl, Robert; Wickland, Kimberly; Hall, Forrest G. (Editor); Conrad, Sara (Editor)</p> <p>2000-01-01</p> <p>The BOREAS TF-4 team measured <span class="hlt">fluxes</span> of <span class="hlt">CO</span><span class="hlt">2</span> and CH4 across the soil-<span class="hlt">air</span> interface in four ages of jack pine forest at the BOREAS SSA during August 1993 to March 1995. Gross and net <span class="hlt">flux</span> of <span class="hlt">CO</span><span class="hlt">2</span> and <span class="hlt">flux</span> of CH4 between soil and <span class="hlt">air</span> are presented for 24 chamber sites in mature jack pine forest, 20-year-old, 4-year-old, and clear cut areas. The data are stored in tabular ASCII files.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1611343P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1611343P"><span>Surfactant control of <span class="hlt">air-sea</span> gas exchange across contrasting biogeochemical regimes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pereira, Ryan; Schneider-Zapp, Klaus; Upstill-Goddard, Robert</p> <p>2014-05-01</p> <p><span class="hlt">Air-sea</span> gas exchange is important to the global partitioning of <span class="hlt">CO</span><span class="hlt">2</span>.Exchange <span class="hlt">fluxes</span> are products of an <span class="hlt">air-sea</span> gas concentration difference, ΔC, and a gas transfer velocity, kw. The latter is controlled by the rate of turbulent diffusion at the <span class="hlt">air-sea</span> interface but it cannot be directly measured and has a high uncertainty that is now considered one of the greatest challenges to quantifying net global <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange ...(Takahashi et al., 2009). One important control on kw is exerted by <span class="hlt">sea</span> surface surfactants that arise both naturally from biological processes and through anthropogenic activity. They influence gas exchange in two fundamental ways: as a monolayer physical barrier and through modifying <span class="hlt">sea</span> surface hydrodynamics and hence turbulent energy transfer. These effects have been demonstrated in the laboratory with artificial surfactants ...(Bock et al., 1999; Goldman et al., 1988) and through purposeful surfactant releases in coastal waters .(.).........().(Brockmann et al., 1982) and in the open ocean (Salter et al., 2011). Suppression of kwin these field experiments was ~5-55%. While changes in both total surfactant concentration and the composition of the natural surfactant pool might be expected to impact kw, the required in-situ studies are lacking. New data collected from the coastal North <span class="hlt">Sea</span> in 2012-2013 shows significant spatio-temporal variability in the surfactant activity of organic matter within the <span class="hlt">sea</span> surface microlayer that ranges from 0.07-0.94 mg/L T-X-100 (AC voltammetry). The surfactant activities show a strong winter/summer seasonal bias and general decrease in concentration with increasing distance from the coastline possibly associated with changing terrestrial vs. phytoplankton sources. Gas exchange experiments of this seawater using a novel laboratory tank and gas tracers (CH4 and SF6) demonstrate a 12-45% reduction in kw compared to surfactant-free water. Seasonally there is higher gas exchange suppression in the summer</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.2784W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.2784W"><span>Sustained Observations of <span class="hlt">Air-Sea</span> <span class="hlt">Fluxes</span> and <span class="hlt">Air-Sea</span> Interaction at the Stratus Ocean Reference Station</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Weller, Robert</p> <p>2014-05-01</p> <p>Since October 2000, a well-instrumented surface mooring has been maintained some 1,500 km west of the coast of northern Chile, roughly in the location of the climatological maximum in marine stratus clouds. Statistically significant increases in wind stress and decreases in annual net <span class="hlt">air-sea</span> heat <span class="hlt">flux</span> and in latent heat <span class="hlt">flux</span> have been observed. If the increased oceanic heat loss continues, the region will within the next decade change from one of net annual heat gain by the ocean to one of neat annual heat loss. Already, annual evaporation of about 1.5 m of <span class="hlt">sea</span> water a year acts to make the warm, salty surface layer more dense. Of interest is examining whether or not increased oceanic heat loss has the potential to change the structure of the upper ocean and potentially remove the shallow warm, salty mixed layer that now buffers the atmosphere from the interior ocean. Insights into how that warm, shallow layer is formed and maintained come from looking at oceanic response to the atmosphere at diurnal tie scales. Restratification each spring and summer is found to depend upon the occurrence of events in which the trade winds decay, allowing diurnal warming in the near-surface ocean to occur, and when the winds return resulting in a net upward step in <span class="hlt">sea</span> surface temperature. This process is proving hard to accurately model.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001JGR...10632139N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001JGR...10632139N"><span>Turbulent aerosol <span class="hlt">fluxes</span> over the Arctic Ocean: <span class="hlt">2</span>. Wind-driven sources from the <span class="hlt">sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nilsson, E. D.; Rannik, Ü.; Swietlicki, E.; Leck, C.; Aalto, P. P.; Zhou, J.; Norman, M.</p> <p>2001-12-01</p> <p>An eddy-covariance <span class="hlt">flux</span> system was successfully applied over open <span class="hlt">sea</span>, leads and ice floes during the Arctic Ocean Expedition in July-August 1996. Wind-driven upward aerosol number <span class="hlt">fluxes</span> were observed over open <span class="hlt">sea</span> and leads in the pack ice. These particles must originate from droplets ejected into the <span class="hlt">air</span> at the bursting of small <span class="hlt">air</span> bubbles at the water surface. The source <span class="hlt">flux</span> F (in 106 m-<span class="hlt">2</span> s-1) had a strong dependency on wind speed, log>(F>)=0.20U¯-1.71 and 0.11U¯-1.93, over the open <span class="hlt">sea</span> and leads, respectively (where U¯ is the local wind speed at about 10 m height). Over the open <span class="hlt">sea</span> the wind-driven aerosol source <span class="hlt">flux</span> consisted of a film drop mode centered at ˜100 nm diameter and a jet drop mode centered at ˜1 μm diameter. Over the leads in the pack ice, a jet drop mode at ˜<span class="hlt">2</span> μm diameter dominated. The jet drop mode consisted of <span class="hlt">sea</span>-salt, but oxalate indicated an organic contribution, and bacterias and other biogenic particles were identified by single particle analysis. Particles with diameters less than -100 nm appear to have contributed to the <span class="hlt">flux</span>, but their chemical composition is unknown. Whitecaps were probably the bubble source at open <span class="hlt">sea</span> and on the leads at high wind speed, but a different bubble source is needed in the leads owing to their small fetch. Melting of ice in the leads is probably the best candidate. The <span class="hlt">flux</span> over the open <span class="hlt">sea</span> was of such a magnitude that it could give a significant contribution to the condensation nuclei (CCN) population. Although the <span class="hlt">flux</span> from the leads were roughly an order of magnitude smaller and the leads cover only a small fraction of the pack ice, the local source may till be important for the CCN population in Arctic fogs. The primary marine aerosol source will increase both with increased wind speed and with decreased ice fraction and extent. The local CCN production may therefore increase and influence cloud or fog albedo and lifetime in response to greenhouse warming in the Arctic Ocean region.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOS.A24A2561T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOS.A24A2561T"><span>Impact of Ocean Surface Waves on <span class="hlt">Air-Sea</span> Momentum <span class="hlt">Flux</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tamura, H.; Drennan, W. M.; Collins, C. O., III; Graber, H. C.</p> <p>2016-02-01</p> <p>In this study, we investigated the structure of turbulent <span class="hlt">air</span> flow over ocean waves. Observations of wind and waves were retrieved by <span class="hlt">air-sea</span> interaction spar (ASIS) buoys during the shoaling waves experiment (SHOWEX) in Duck, NC in 1999. It is shown that the turbulent velocity spectra and <span class="hlt">co</span>-spectra for pure wind <span class="hlt">sea</span> conditions follow the universal forms estimated by Miyake et al [1970]. In the presence of strong swells, the wave boundary layer was extended and the universal spectral scaling of u'w' broke down [Drennan et al, 1999]. On the other hand, the use of the peak wave frequency (fp) to reproduce the "universal spectra" succeeded at explaining the spectral structure of turbulent flow field. The u'w' <span class="hlt">co</span>-spectra become negative near the fp, which suggests the upward momentum transport (i.e., negative wind stress) induced by ocean waves. Finally, we propose three turbulent flow structures for different wind-wave regimes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010PalOc..25.3201J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010PalOc..25.3201J"><span>Response of <span class="hlt">air-sea</span> carbon <span class="hlt">fluxes</span> and climate to orbital forcing changes in the Community Climate System Model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jochum, M.; Peacock, S.; Moore, K.; Lindsay, K.</p> <p>2010-07-01</p> <p>A global general circulation model coupled to an ocean ecosystem model is used to quantify the response of carbon <span class="hlt">fluxes</span> and climate to changes in orbital forcing. Compared to the present-day simulation, the simulation with the Earth's orbital parameters from 115,000 years ago features significantly cooler northern high latitudes but only moderately cooler southern high latitudes. This asymmetry is explained by a 30% reduction of the strength of the Atlantic Meridional Overturning Circulation that is caused by an increased Arctic <span class="hlt">sea</span> ice export and a resulting freshening of the North Atlantic. The strong northern high-latitude cooling and the direct insolation induced tropical warming lead to global shifts in precipitation and winds to the order of 10%-20%. These climate shifts lead to regional differences in <span class="hlt">air-sea</span> carbon <span class="hlt">fluxes</span> of the same order. However, the differences in global net <span class="hlt">air-sea</span> carbon <span class="hlt">fluxes</span> are small, which is due to several effects, two of which stand out: first, colder <span class="hlt">sea</span> surface temperature leads to a more effective solubility pump but also to increased <span class="hlt">sea</span> ice concentration which blocks <span class="hlt">air-sea</span> exchange, and second, the weakening of Southern Ocean winds that is predicted by some idealized studies occurs only in part of the basin, and is compensated by stronger winds in other parts.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4237463','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4237463"><span>Net uptake of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> by coastal submerged aquatic vegetation</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Tokoro, Tatsuki; Hosokawa, Shinya; Miyoshi, Eiichi; Tada, Kazufumi; Watanabe, Kenta; Montani, Shigeru; Kayanne, Hajime; Kuwae, Tomohiro</p> <p>2014-01-01</p> <p>‘Blue Carbon’, which is carbon captured by marine living organisms, has recently been highlighted as a new option for climate change mitigation initiatives. In particular, coastal ecosystems have been recognized as significant carbon stocks because of their high burial rates and long-term sequestration of carbon. However, the direct contribution of Blue Carbon to the uptake of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> through <span class="hlt">air-sea</span> gas exchange remains unclear. We performed in situ measurements of carbon flows, including <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>, dissolved inorganic carbon changes, net ecosystem production, and carbon burial rates in the boreal (Furen), temperate (Kurihama), and subtropical (Fukido) seagrass meadows of Japan from 2010 to 2013. In particular, the <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> was measured using three methods: the bulk formula method, the floating chamber method, and the eddy covariance method. Our empirical results show that submerged autotrophic vegetation in shallow coastal waters can be functionally a sink for atmospheric <span class="hlt">CO</span><span class="hlt">2</span>. This finding is contrary to the conventional perception that most near-shore ecosystems are sources of atmospheric <span class="hlt">CO</span><span class="hlt">2</span>. The key factor determining whether or not coastal ecosystems directly decrease the concentration of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> may be net ecosystem production. This study thus identifies a new ecosystem function of coastal vegetated systems; they are direct sinks of atmospheric <span class="hlt">CO</span><span class="hlt">2</span>. PMID:24623530</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5031984','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5031984"><span>A new frontier in <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> measurements using a highly portable DIAL laser system</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Queiβer, Manuel; Granieri, Domenico; Burton, Mike</p> <p>2016-01-01</p> <p>Volcanic <span class="hlt">CO</span><span class="hlt">2</span> emissions play a key role in the geological carbon cycle, and monitoring of volcanic <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> helps to forecast eruptions. The quantification of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> is challenging due to rapid dilution of magmatic <span class="hlt">CO</span><span class="hlt">2</span> in <span class="hlt">CO</span><span class="hlt">2</span>-rich ambient <span class="hlt">air</span> and the diffuse nature of many emissions, leading to large uncertainties in the global magmatic <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> inventory. Here, we report measurements using a new DIAL laser remote sensing system for volcanic <span class="hlt">CO</span><span class="hlt">2</span> (<span class="hlt">CO</span><span class="hlt">2</span>DIAL). Two sites in the volcanic zone of Campi Flegrei (Italy) were scanned, yielding <span class="hlt">CO</span><span class="hlt">2</span> path-amount profiles used to compute <span class="hlt">fluxes</span>. Our results reveal a relatively high <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> from Campi Flegrei, consistent with an increasing trend. Unlike previous methods, the <span class="hlt">CO</span><span class="hlt">2</span>DIAL is able to measure integrated <span class="hlt">CO</span><span class="hlt">2</span> path-amounts at distances up to 2000 m using virtually any solid surface as a reflector, whilst also being highly portable. This opens a new frontier in quantification of geological and anthropogenic <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. PMID:27652775</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..1514237M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..1514237M"><span>Soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> in alley-cropping systems composed of black locust and poplar trees, Germany</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Medinski, Tetiana; Freese, Dirk; Boehm, Christian</p> <p>2013-04-01</p> <p>The understanding of soil carbon dynamics after establishment of alley-cropping systems is crucial for mitigation of greenhouse <span class="hlt">CO</span><span class="hlt">2</span> gas. This study investigates soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in alley-cropping systems composed of strips of black locust (Robinia pseudoacacia L.) and poplar (Max 1) trees and adjacent to them crop strips (Lupinus). Soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> was measured monthly over a period from March to November 2012, using a LI-COR LI-8100A automated device. Concurrently with <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> measurements, soil and <span class="hlt">air</span> temperature and soil moisture were recorded within 10 cm of each collar. Soil samples were collected nearby each soil collar for microbial C and hot water-extractable C analyses. At each study plot, root biomass was measured to a depth of 15 cm. In all vegetation types, soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> increased from May to August, showing a significant positive correlation with <span class="hlt">air</span> and soil temperature, which can be a reflection of increase in photosynthesis over the warm summer months. <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> was the highest in poplar followed by black locust and lupines. The relationships between <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span>, microbial biomass and hot water-extractable carbon were not straightforward. Among the measured parameters, root density was found to be the main factor to explain the higher <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> in tree strips.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20140002146&hterms=climate+change+ocean&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dclimate%2Bchange%2Bocean','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20140002146&hterms=climate+change+ocean&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dclimate%2Bchange%2Bocean"><span>Monitoring Ocean <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Fluxes</span> from Space: GOSAT and OCO-<span class="hlt">2</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Crisp, David</p> <p>2012-01-01</p> <p>The ocean is a major component of the global carbon cycle, emitting over 330 billion tons of carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) into the atmosphere each year, or about 10 times that emitted fossil fuel combustion and all other human activities [1, <span class="hlt">2</span>]. The ocean reabsorbs a comparable amount of <span class="hlt">CO</span><span class="hlt">2</span> each year, along with 25% of the <span class="hlt">CO</span><span class="hlt">2</span> emitted by these human activities. The nature and geographic distribution of the processes controlling these ocean <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> are still poorly constrained by observations. A better understanding of these processes is essential to predict how this important <span class="hlt">CO</span><span class="hlt">2</span> sink may evolve as the climate changes.While in situ measurements of ocean <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> can be very precise, the sampling density is far too sparse to quantify ocean <span class="hlt">CO</span><span class="hlt">2</span> sources and sinks over much of the globe. One way to improve the spatial resolution, coverage, and sampling frequency is to make observations of the column averaged <span class="hlt">CO</span><span class="hlt">2</span> dry <span class="hlt">air</span> mole fraction, XCO<span class="hlt">2</span>, from space [4, 5, 6]. Such measurements could provide global coverage at high resolution (< 100 km) on monthly time scales. High precision (< 1 part per million, ppm) is essential to resolve the small, near-surface <span class="hlt">CO</span><span class="hlt">2</span> variations associated with ocean <span class="hlt">fluxes</span> and to better constrain the <span class="hlt">CO</span><span class="hlt">2</span> transport over the ocean. The Japanese Greenhouse gases Observing Satellite (GOSAT) and the NASA Orbiting Carbon Observatory (OCO) were first two space based sensors designed specifically for this task. GOSAT was successfully launched on January 23, 2009, and has been returning measurements of XCO<span class="hlt">2</span> since April 2009. The OCO mission was lost in February 2009, when its launch vehicle malfunctioned and failed to reach orbit. In early 2010, NASA authorized a re-flight of OCO, called OCO-<span class="hlt">2</span>, which is currently under development.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5400058','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5400058"><span>Revisiting the choice of the driving temperature for eddy covariance <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> partitioning</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Wohlfahrt, Georg; Galvagno, Marta</p> <p>2017-01-01</p> <p>So-called <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> partitioning algorithms are widely used to partition the net ecosystem <span class="hlt">CO</span><span class="hlt">2</span> exchange into the two component <span class="hlt">fluxes</span>, gross primary productivity and ecosystem respiration. Common <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> partitioning algorithms conceptualize ecosystem respiration to originate from a single source, requiring the choice of a corresponding driving temperature. Using a conceptual dual-source respiration model, consisting of an above- and a below-ground respiration source each driven by a corresponding temperature, we demonstrate that the typical phase shift between <span class="hlt">air</span> and soil temperature gives rise to a hysteresis relationship between ecosystem respiration and temperature. The hysteresis proceeds in a clockwise fashion if soil temperature is used to drive ecosystem respiration, while a counter-clockwise response is observed when ecosystem respiration is related to <span class="hlt">air</span> temperature. As a consequence, nighttime ecosystem respiration is smaller than daytime ecosystem respiration when referenced to soil temperature, while the reverse is true for <span class="hlt">air</span> temperature. We confirm these qualitative modelling results using measurements of day and night ecosystem respiration made with opaque chambers in a short-statured mountain grassland. Inferring daytime from nighttime ecosystem respiration or vice versa, as attempted by <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> partitioning algorithms, using a single-source respiration model is thus an oversimplification resulting in biased estimates of ecosystem respiration. We discuss the likely magnitude of the bias, options for minimizing it and conclude by emphasizing that the systematic uncertainty of gross primary productivity and ecosystem respiration inferred through <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> partitioning needs to be better quantified and reported. PMID:28439145</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.B33C0620I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.B33C0620I"><span>Analysis of uncertainties in GOSAT-inferred regional <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ishizawa, M.; Shirai, T.; Maksyutov, S. S.; Yoshida, Y.; Morino, I.; Inoue, M.; Nakatsuru, T.; Uchino, O.; Mabuchi, K.</p> <p>2016-12-01</p> <p>Satellite-based <span class="hlt">CO</span><span class="hlt">2</span> measurements have potential for improving our understanding global carbon cycle because of more spatiotemporal coverage than those from ground-based observations. Since the Greenhouse gases Observing Satellite (GOSAT) was launched in January 2009, it has been measuring the column-average dry <span class="hlt">air</span>-mole function of <span class="hlt">CO</span><span class="hlt">2</span> (XCO<span class="hlt">2</span>) from the space. To utilize the GOSAT XCO<span class="hlt">2</span> for better <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> estimates, several challenges should be overcome. Systematic errors (biases) in XCO<span class="hlt">2</span> retrievals are a major factor which leads to large differences among inverted <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. Temporally variable data coverage and density are also taken into account when interpreting the estimated surface <span class="hlt">fluxes</span>. In this study, we employ an atmospheric inverse model to investigate the impacts of retrievals biases and temporally varying global distribution of GOSAT XCO<span class="hlt">2</span> on surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> estimates. Inversions are performed for 2009-2013, with several subsets of the 5-year record of GOSAT XCO<span class="hlt">2</span> (v<span class="hlt">2</span>.21) and its bias-corrected XCO<span class="hlt">2</span>. GOSAT XCO<span class="hlt">2</span> data consist of three types: H-gain for vegetated lands, M-gain for bright surfaces (desert areas), and sun-glint for ocean surface. The results show that the global spatial distributions of estimated <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> depend on the subset of XCO<span class="hlt">2</span> used. M-gain XCO<span class="hlt">2</span> results in unrealistically high <span class="hlt">CO</span><span class="hlt">2</span> emissions in and around the Middle East, including the neighboring ocean regions. On the other hand, M-gain XCO<span class="hlt">2</span> causes compensating unrealistic uptakes far beyond M-gain regions in low latitudes, also partially contributing on the summer uptake in Europe. The joint inversions with both surface measurements and GOSAT XCO<span class="hlt">2</span> data obtain larger <span class="hlt">flux</span> gradient between the northern extra-tropics and the tropics than the inversion with surface measurements only for the first <span class="hlt">2</span> years. Recently, these North-South gradients seem to be gradually reducing as the tropics become a weaker source or turn into a sink, while the net emission strength in East Asia is increasing</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28944134','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28944134"><span><span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> from Javanese mud volcanism.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Queißer, M; Burton, M R; Arzilli, F; Chiarugi, A; Marliyani, G I; Anggara, F; Harijoko, A</p> <p>2017-06-01</p> <p>Studying the quantity and origin of <span class="hlt">CO</span> <span class="hlt">2</span> emitted by back-arc mud volcanoes is critical to correctly model fluid-dynamical, thermodynamical, and geochemical processes that drive their activity and to constrain their role in the global geochemical carbon cycle. We measured <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">fluxes</span> of the Bledug Kuwu mud volcano on the Kendeng Fold and thrust belt in the back arc of Central Java, Indonesia, using scanning remote sensing absorption spectroscopy. The data show that the expelled gas is rich in <span class="hlt">CO</span> <span class="hlt">2</span> with a volume fraction of at least 16 vol %. A lower limit <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">flux</span> of 1.4 kg s -1 (117 t d -1 ) was determined, in line with the <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">flux</span> from the Javanese mud volcano LUSI. Extrapolating these results to mud volcanism from the whole of Java suggests an order of magnitude total <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">flux</span> of 3 kt d -1 , comparable with the expected back-arc efflux of magmatic <span class="hlt">CO</span> <span class="hlt">2</span> . After discussing geochemical, geological, and geophysical evidence we conclude that the source of <span class="hlt">CO</span> <span class="hlt">2</span> observed at Bledug Kuwu is likely a mixture of thermogenic, biogenic, and magmatic <span class="hlt">CO</span> <span class="hlt">2</span> , with faulting controlling potential pathways for magmatic fluids. This study further demonstrates the merit of man-portable active remote sensing instruments for probing natural gas releases, enabling bottom-up quantification of <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">fluxes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRB..122.4191Q','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRB..122.4191Q"><span><span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> from Javanese mud volcanism</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Queißer, M.; Burton, M. R.; Arzilli, F.; Chiarugi, A.; Marliyani, G. I.; Anggara, F.; Harijoko, A.</p> <p>2017-06-01</p> <p>Studying the quantity and origin of <span class="hlt">CO</span><span class="hlt">2</span> emitted by back-arc mud volcanoes is critical to correctly model fluid-dynamical, thermodynamical, and geochemical processes that drive their activity and to constrain their role in the global geochemical carbon cycle. We measured <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> of the Bledug Kuwu mud volcano on the Kendeng Fold and thrust belt in the back arc of Central Java, Indonesia, using scanning remote sensing absorption spectroscopy. The data show that the expelled gas is rich in <span class="hlt">CO</span><span class="hlt">2</span> with a volume fraction of at least 16 vol %. A lower limit <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> of 1.4 kg s-1 (117 t d-1) was determined, in line with the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> from the Javanese mud volcano LUSI. Extrapolating these results to mud volcanism from the whole of Java suggests an order of magnitude total <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> of 3 kt d-1, comparable with the expected back-arc efflux of magmatic <span class="hlt">CO</span><span class="hlt">2</span>. After discussing geochemical, geological, and geophysical evidence we conclude that the source of <span class="hlt">CO</span><span class="hlt">2</span> observed at Bledug Kuwu is likely a mixture of thermogenic, biogenic, and magmatic <span class="hlt">CO</span><span class="hlt">2</span>, with faulting controlling potential pathways for magmatic fluids. This study further demonstrates the merit of man-portable active remote sensing instruments for probing natural gas releases, enabling bottom-up quantification of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA578419','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA578419"><span>Predicting the Turbulent <span class="hlt">Air-Sea</span> Surface <span class="hlt">Fluxes</span>, Including Spray Effects, from Weak to Strong Winds</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2012-09-30</p> <p>almost complete decoupling of the wind field from the <span class="hlt">sea</span> surface . As a result of the weak surface stress, the flow becomes almost free from the...shore flow . In turn, wave growth and the associated surface roughness (z0) are limited. Consequently, the stability increases further in a...1 DISTRIBUTION STATEMENT A. Approved for public release; distribution is unlimited. Predicting the Turbulent <span class="hlt">Air-Sea</span> Surface <span class="hlt">Fluxes</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoRL..45..418Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoRL..45..418Z"><span>The Influence of <span class="hlt">Air-Sea</span> <span class="hlt">Fluxes</span> on Atmospheric Aerosols During the Summer Monsoon Over the Tropical Indian Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zavarsky, Alex; Booge, Dennis; Fiehn, Alina; Krüger, Kirstin; Atlas, Elliot; Marandino, Christa</p> <p>2018-01-01</p> <p>During the summer monsoon, the western tropical Indian Ocean is predicted to be a hot spot for dimethylsulfide emissions, the major marine sulfur source to the atmosphere, and an important aerosol precursor. Other aerosol relevant <span class="hlt">fluxes</span>, such as isoprene and <span class="hlt">sea</span> spray, should also be enhanced, due to the steady strong winds during the monsoon. Marine <span class="hlt">air</span> masses dominate the area during the summer monsoon, excluding the influence of continentally derived pollutants. During the SO234-<span class="hlt">2</span>/235 cruise in the western tropical Indian Ocean from July to August 2014, directly measured eddy covariance DMS <span class="hlt">fluxes</span> confirm that the area is a large source of sulfur to the atmosphere (cruise average 9.1 μmol m-<span class="hlt">2</span> d-1). The directly measured <span class="hlt">fluxes</span>, as well as computed isoprene and <span class="hlt">sea</span> spray <span class="hlt">fluxes</span>, were combined with FLEXPART backward and forward trajectories to track the emissions in space and time. The <span class="hlt">fluxes</span> show a significant positive correlation with aerosol data from the Terra and Suomi-NPP satellites, indicating a local influence of marine emissions on atmospheric aerosol numbers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20030025770','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20030025770"><span>Version <span class="hlt">2</span> Goddard Satellite-Based Surface Turbulent <span class="hlt">Fluxes</span> (GSSTF<span class="hlt">2</span>)</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chou, Shu-Hsien; Nelkin, Eric; Ardizzone, Joe; Atlas, Robert M.; Shie, Chung-Lin; Starr, David O'C. (Technical Monitor)</p> <p>2002-01-01</p> <p>Information on the turbulent <span class="hlt">fluxes</span> of momentum, moisture, and heat at the <span class="hlt">air-sea</span> interface is essential in improving model simulations of climate variations and in climate studies. We have derived a 13.5-year (July 1987-December 2000) dataset of daily surface turbulent <span class="hlt">fluxes</span> over global oceans from the Special Sensor Mcrowave/Imager (SSM/I) radiance measurements. This dataset, version <span class="hlt">2</span> Goddard Satellite-based Surface Turbulent <span class="hlt">Fluxes</span> (GSSTF<span class="hlt">2</span>), has a spatial resolution of 1 degree x 1 degree latitude-longitude and a temporal resolution of 1 day. Turbulent <span class="hlt">fluxes</span> are derived from the SSM/I surface winds and surface <span class="hlt">air</span> humidity, as well as the <span class="hlt">2</span>-m <span class="hlt">air</span> and <span class="hlt">sea</span> surface temperatures (SST) of the NCEP/NCAR reanalysis, using a bulk aerodynamic algorithm based on the surface layer similarity theory.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5586201','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5586201"><span><span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> from Javanese mud volcanism</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Burton, M. R.; Arzilli, F.; Chiarugi, A.; Marliyani, G. I.; Anggara, F.; Harijoko, A.</p> <p>2017-01-01</p> <p>Abstract Studying the quantity and origin of <span class="hlt">CO</span><span class="hlt">2</span> emitted by back‐arc mud volcanoes is critical to correctly model fluid‐dynamical, thermodynamical, and geochemical processes that drive their activity and to constrain their role in the global geochemical carbon cycle. We measured <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> of the Bledug Kuwu mud volcano on the Kendeng Fold and thrust belt in the back arc of Central Java, Indonesia, using scanning remote sensing absorption spectroscopy. The data show that the expelled gas is rich in <span class="hlt">CO</span><span class="hlt">2</span> with a volume fraction of at least 16 vol %. A lower limit <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> of 1.4 kg s−1 (117 t d−1) was determined, in line with the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> from the Javanese mud volcano LUSI. Extrapolating these results to mud volcanism from the whole of Java suggests an order of magnitude total <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> of 3 kt d−1, comparable with the expected back‐arc efflux of magmatic <span class="hlt">CO</span><span class="hlt">2</span>. After discussing geochemical, geological, and geophysical evidence we conclude that the source of <span class="hlt">CO</span><span class="hlt">2</span> observed at Bledug Kuwu is likely a mixture of thermogenic, biogenic, and magmatic <span class="hlt">CO</span><span class="hlt">2</span>, with faulting controlling potential pathways for magmatic fluids. This study further demonstrates the merit of man‐portable active remote sensing instruments for probing natural gas releases, enabling bottom‐up quantification of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. PMID:28944134</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014BGD....1117543L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014BGD....1117543L"><span>Rapid establishment of the <span class="hlt">CO</span><span class="hlt">2</span> sink associated with Kerguelen's bloom observed during the KEOPS<span class="hlt">2</span>/OISO20 cruise</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lo Monaco, C.; Metzl, N.; D'Ovidio, F.; Llort, J.; Ridame, C.</p> <p>2014-12-01</p> <p>Iron and light are the main factors limiting the biological pump of <span class="hlt">CO</span><span class="hlt">2</span> in the Southern Ocean. Iron fertilization experiments have demonstrated the potential for increased uptake of atmospheric <span class="hlt">CO</span><span class="hlt">2</span>, but little is known about the evolution of fertilized environnements. This paper presents observations collected in one of the largest phytoplankton bloom of the Southern Ocean sustained by iron originating from the Kerguelen Plateau. We first complement previous studies by investigating the mechanisms that control <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> over and downstream of the Kerguelen Plateau at the onset of the bloom based on measurements obtained in October-November 2011. These new observations show the rapid establishment of a strong <span class="hlt">CO</span><span class="hlt">2</span> sink in waters fertilized with iron as soon as vertical mixing is reduced. The magnitude of the <span class="hlt">CO</span><span class="hlt">2</span> sink was closely related to chlorophyll a and iron concentrations. Because iron concentration strongly depends on the distance from the iron source and the mode of delivery, we identified lateral advection as the main mechanism controlling <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> downtream the Kerguelen Plateau during the growing season. In the southern part of the bloom, situated over the Plateau (iron source), the <span class="hlt">CO</span><span class="hlt">2</span> sink was stronger and spatially more homogeneous than in the plume offshore. However, we also witnessed a substantial reduction in the uptake of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> over the Plateau following a strong winds event. Next, we used all the data available in this region in order to draw the seasonal evolution of <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. The <span class="hlt">CO</span><span class="hlt">2</span> sink is rapidly reduced during the course of the growing season, which we attribute to iron and silicic acid depletion. South of the Polar Front, where nutrients depletion is delayed, we suggest that the amplitude and duration of the <span class="hlt">CO</span><span class="hlt">2</span> sink is mainly controlled by vertical mixing. The impact of iron fertilization on <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> is revealed by comparing the uptake of <span class="hlt">CO</span><span class="hlt">2</span> integrated over the productive season in the bloom</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.agu.org/journals/jc/v096/iC04/90JC02642/','USGSPUBS'); return false;" href="http://www.agu.org/journals/jc/v096/iC04/90JC02642/"><span>Atmospheric organochlorine pollutants and <span class="hlt">air-sea</span> exchange of hexachlorocyclohexane in the Bering and Chukchi <span class="hlt">Seas</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Hinckley, D.A.; Bidleman, T.F.; Rice, C.P.</p> <p>1991-01-01</p> <p>Organochlorine pesticides have been found in Arctic fish, marine mammals, birds, and plankton for some time. The lack of local sources and remoteness of the region imply long-range transport and deposition of contaminants into the Arctic from sources to the south. While on the third Soviet-American Joint Ecological Expedition to the Bering and Chukchi <span class="hlt">Seas</span> (August 1988), high-volume <span class="hlt">air</span> samples were taken and analyzed for organochlorine pesticides. Hexachlorocyclohexane (HCH), hexachlorobenzene, polychlorinated camphenes, and chlordane (listed in order of abundance, highest to lowest) were quantified. The <span class="hlt">air-sea</span> gas exchange of HCH was estimated at 18 stations during the cruise. Average alpha-HCH concentrations in concurrent atmosphere and surface water samples were 250 pg m-3 and <span class="hlt">2</span>.4 ng L-1, respectively, and average gamma-HCH concentrations were 68 pg m-3 in the atmosphere and 0.6 ng L-1 in surface water. Calculations based on experimentally derived Henry's law constants showed that the surface water was undersaturated with respect to the atmosphere at most stations (alpha-HCH, average 79% saturation; gamma-HCH, average 28% saturation). The <span class="hlt">flux</span> for alpha-HCH ranged from -47 ng m-<span class="hlt">2</span> day-1 (<span class="hlt">sea</span> to <span class="hlt">air</span>) to 122 ng m-<span class="hlt">2</span> d-1 (<span class="hlt">air</span> to <span class="hlt">sea</span>) and averaged 25 ng m-<span class="hlt">2</span> d-1 <span class="hlt">air</span> to <span class="hlt">sea</span>. All <span class="hlt">fluxes</span> of gamma-HCH were from <span class="hlt">air</span> to <span class="hlt">sea</span>, ranged from 17 to 54 ng m-<span class="hlt">2</span> d-1, and averaged 31 ng m-<span class="hlt">2</span> d-1.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li class="active"><span>6</span></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_6 --> <div id="page_7" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li class="active"><span>7</span></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="121"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012TCD.....6.5037R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012TCD.....6.5037R"><span>Ikaite crystal distribution in Arctic winter <span class="hlt">sea</span> ice and implications for <span class="hlt">CO</span><span class="hlt">2</span> system dynamics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rysgaard, S.; Søgaard, D. H.; Cooper, M.; Pućko, M.; Lennert, K.; Papakyriakou, T. N.; Wang, F.; Geilfus, N. X.; Glud, R. N.; Ehn, J.; McGinnnis, D. F.; Attard, K.; Sievers, J.; Deming, J. W.; Barber, D.</p> <p>2012-12-01</p> <p>The precipitation of ikaite (Ca<span class="hlt">CO</span>3·6H<span class="hlt">2</span>O) in polar <span class="hlt">sea</span> ice is critical to the efficiency of the <span class="hlt">sea</span> ice-driven carbon pump and potentially important to the global carbon cycle, yet the spatial and temporal occurrence of ikaite within the ice is poorly known. We report unique observations of ikaite in unmelted ice and vertical profiles of ikaite abundance and concentration in <span class="hlt">sea</span> ice for the crucial season of winter. Ice was examined from two locations: a 1 m thick land-fast ice site and a 0.3 m thick polynya site, both in the Young Sound area (74° N, 20° W) of NE Greenland. Ikaite crystals, ranging in size from a few µm to 700 µm were observed to concentrate in the interstices between the ice platelets in both granular and columnar <span class="hlt">sea</span> ice. In vertical <span class="hlt">sea</span>-ice profiles from both locations, ikaite concentration determined from image analysis, decreased with depth from surfaceice values of 700-900 µmol kg-1 ice (~ 25 × 106 crystals kg-1) to bottom-layer values of 100-200 µmol kg-1 ice (1-7 × 106 kg-1), all of which are much higher (4-10 times) than those reported in the few previous studies. Direct measurements of total alkalinity (TA) in surface layers fell within the same range as ikaite concentration whereas TA concentrations in bottom layers were twice as high. This depth-related discrepancy suggests interior ice processes where ikaite crystals form in surface <span class="hlt">sea</span> ice layers and partly dissolved in bottom layers. From these findings and model calculations we relate <span class="hlt">sea</span> ice formation and melt to observed p<span class="hlt">CO</span><span class="hlt">2</span> conditions in polar surface waters, and hence, the <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70120200','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70120200"><span><span class="hlt">Air-sea</span> interactions during strong winter extratropical storms</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Nelson, Jill; He, Ruoying; Warner, John C.; Bane, John</p> <p>2014-01-01</p> <p>A high-resolution, regional coupled atmosphere–ocean model is used to investigate strong air–<span class="hlt">sea</span> interactions during a rapidly developing extratropical cyclone (ETC) off the east coast of the USA. In this two-way coupled system, surface momentum and heat <span class="hlt">fluxes</span> derived from the Weather Research and Forecasting model and <span class="hlt">sea</span> surface temperature (SST) from the Regional Ocean Modeling System are exchanged via the Model Coupling Toolkit. Comparisons are made between the modeled and observed wind velocity, <span class="hlt">sea</span> level pressure, 10 m <span class="hlt">air</span> temperature, and <span class="hlt">sea</span> surface temperature time series, as well as a comparison between the model and one glider transect. Vertical profiles of modeled <span class="hlt">air</span> temperature and winds in the marine atmospheric boundary layer and temperature variations in the upper ocean during a 3-day storm period are examined at various cross-shelf transects along the eastern seaboard. It is found that the air–<span class="hlt">sea</span> interactions near the Gulf Stream are important for generating and sustaining the ETC. In particular, locally enhanced winds over a warm <span class="hlt">sea</span> (relative to the land temperature) induce large surface heat <span class="hlt">fluxes</span> which cool the upper ocean by up to <span class="hlt">2</span> °C, mainly during the cold <span class="hlt">air</span> outbreak period after the storm passage. Detailed heat budget analyses show the ocean-to-atmosphere heat <span class="hlt">flux</span> dominates the upper ocean heat content variations. Results clearly show that dynamic air–<span class="hlt">sea</span> interactions affecting momentum and buoyancy <span class="hlt">flux</span> exchanges in ETCs need to be resolved accurately in a coupled atmosphere–ocean modeling framework.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.A53L3379W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.A53L3379W"><span><span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Fluxes</span> and Concentrations in a Residential Area in the Southern Hemisphere</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Weissert, L. F.; Salmond, J. A.; Turnbull, J. C.; Schwendenmann, L.</p> <p>2014-12-01</p> <p>While cities are generally major sources of anthropogenic carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) emissions, recent research has shown that parts of urban areas may also act as <span class="hlt">CO</span><span class="hlt">2</span> sinks due to <span class="hlt">CO</span><span class="hlt">2</span> uptake by vegetation. However, currently available results are related to a large degree of uncertainty due to the limitations of the applied methods and the limited number of studies available from urban areas, particularly from the southern hemisphere. In this study, we explore the potential of eddy covariance and tracer measurements (13C and 14C isotopes of <span class="hlt">CO</span><span class="hlt">2</span>) to quantify and partition <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> and concentrations in a residential urban area in Auckland, New Zealand. Based on preliminary results from autumn and winter (March to July 2014) the residential area is a small source of <span class="hlt">CO</span><span class="hlt">2</span> (0.11 mol <span class="hlt">CO</span><span class="hlt">2</span> m-<span class="hlt">2</span> day-1). <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> and concentrations follow a distinct diurnal cycle with a morning peak between 7:00 and 9:00 (max: 0.25 mol <span class="hlt">CO</span><span class="hlt">2</span> m-<span class="hlt">2</span> day-1/412 ppm) and midday low with negative <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> (min: -0.17 mol <span class="hlt">CO</span><span class="hlt">2</span> m-<span class="hlt">2</span> day-1/392 ppm) between 10:00 and 15:00 local time, likely due to photosynthetic <span class="hlt">CO</span><span class="hlt">2</span> uptake by local vegetation. Soil <span class="hlt">CO</span><span class="hlt">2</span> efflux may explain that <span class="hlt">CO</span><span class="hlt">2</span> concentrations increase and remain high (401 ppm) throughout the night. Mean diurnal winter δ13C values are in anti-phase with <span class="hlt">CO</span><span class="hlt">2</span> concentrations and vary between -9.0 - -9.7‰. The depletion of δ13C compared to clean atmospheric <span class="hlt">air</span> (-8.<span class="hlt">2</span>‰) is likely a result of local <span class="hlt">CO</span><span class="hlt">2</span> sources dominated by gasoline combustion (appr. 60%) during daytime. A sector analysis (based on prevailing wind) of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> and concentrations indicates lower <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> and concentrations from the vegetation-dominated sector, further demonstrating the influence of vegetation on local <span class="hlt">CO</span><span class="hlt">2</span> concentrations. These results provide an insight into the temporal and spatial variability <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>/concentrations and potential <span class="hlt">CO</span><span class="hlt">2</span> sinks and sources from a city in the southern hemisphere and add valuable information to the global database of urban <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20160013874&hterms=Change+climate&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3DChange%2Bclimate','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20160013874&hterms=Change+climate&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3DChange%2Bclimate"><span>The <span class="hlt">Flux</span>-Anomaly-Forced Model Intercomparison Project (FAFMIP) Contribution to CMIP6: Investigation of <span class="hlt">Sea</span>-Level and Ocean Climate Change in Response to <span class="hlt">CO</span><span class="hlt">2</span> Forcing</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gregory, Jonathan M.; Bouttes, Nathaelle; Griffies, Stephen M.; Haak, Helmuth; Hurlin, William J.; Jungclaus, Johann; Kelley, Maxwell; Lee, Warren G.; Marshall, John; Romanou, Anastasia; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20160013874'); toggleEditAbsImage('author_20160013874_show'); toggleEditAbsImage('author_20160013874_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20160013874_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20160013874_hide"></p> <p>2016-01-01</p> <p>The <span class="hlt">Flux</span>-Anomaly-Forced Model Intercomparison Project (FAFMIP) aims to investigate the spread in simulations of <span class="hlt">sea</span>-level and ocean climate change in response to <span class="hlt">CO</span><span class="hlt">2</span> forcing by atmosphere-ocean general circulation models (AOGCMs). It is particularly motivated by the uncertainties in projections of ocean heat uptake, global-mean sealevel rise due to thermal expansion and the geographical patterns of <span class="hlt">sea</span>-level change due to ocean density and circulation change. FAFMIP has three tier-1 experiments, in which prescribed surface <span class="hlt">flux</span> perturbations of momentum, heat and freshwater respectively are applied to the ocean in separate AOGCM simulations. All other conditions are as in the pre-industrial control. The prescribed fields are typical of pattern and magnitude of changes in these <span class="hlt">fluxes</span> projected by AOGCMs for doubled <span class="hlt">CO</span><span class="hlt">2</span> concentration. Five groups have tested the experimental design with existing AOGCMs. Their results show diversity in the pattern and magnitude of changes, with some common qualitative features. Heat and water <span class="hlt">flux</span> perturbation cause the dipole in <span class="hlt">sea</span>-level change in the North Atlantic, while momentum and heat <span class="hlt">flux</span> perturbation cause the gradient across the Antarctic Circumpolar Current. The Atlantic meridional overturning circulation (AMOC) declines in response to the heat <span class="hlt">flux</span> perturbation, and there is a strong positive feedback on this effect due to the consequent cooling of <span class="hlt">sea</span>-surface temperature in the North Atlantic, which enhances the local heat input to the ocean. The momentum and water <span class="hlt">flux</span> perturbations do not substantially affect the AMOC. Heat is taken up largely as a passive tracer in the Southern Ocean, which is the region of greatest heat input, while the weakening of the AMOC causes redistribution of heat towards lower latitudes. Future analysis of these and other phenomena with the wider range of CMIP6 FAFMIP AOGCMs will benefit from new diagnostics of temperature and salinity tendencies, which will enable investigation of the model</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013ACPD...1326529C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013ACPD...1326529C"><span>Atmospheric inversion of the surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> with 13<span class="hlt">CO</span><span class="hlt">2</span> constraint</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, J. M.; Mo, G.; Deng, F.</p> <p>2013-10-01</p> <p>Observations of 13<span class="hlt">CO</span><span class="hlt">2</span> at 73 sites compiled in the GLOBALVIEW database are used for an additional constraint in a global atmospheric inversion of the surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> using <span class="hlt">CO</span><span class="hlt">2</span> observations at 210 sites for the 2002-2004 period for 39 land regions and 11 ocean regions. This constraint is implemented using the 13<span class="hlt">CO</span><span class="hlt">2</span>/<span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> ratio modeled with a terrestrial ecosystem model and an ocean model. These models simulate 13<span class="hlt">CO</span><span class="hlt">2</span> discrimination rates of terrestrial photosynthesis and respiration and ocean-atmosphere diffusion processes. In both models, the 13<span class="hlt">CO</span><span class="hlt">2</span> disequilibrium between <span class="hlt">fluxes</span> to and from the atmosphere is considered due to the historical change in atmospheric 13<span class="hlt">CO</span><span class="hlt">2</span> concentration. For the 2002-2004 period, the 13<span class="hlt">CO</span><span class="hlt">2</span> constraint on the inversion increases the total land carbon sink from 3.40 to 3.70 Pg C yr-1 and decreases the total oceanic carbon sink from 1.48 to 1.12 Pg C yr-1. The largest changes occur in tropical areas: a considerable decrease in the carbon source in the Amazon forest, and this decrease is mostly compensated by increases in the ocean region immediately west of the Amazon and the southeast Asian land region. Our further investigation through different treatments of the 13<span class="hlt">CO</span><span class="hlt">2</span>/<span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> ratio used in the inversion suggests that variable spatial distributions of the 13<span class="hlt">CO</span><span class="hlt">2</span> isotopic discrimination rate simulated by the models over land and ocean have considerable impacts on the spatial distribution of the inverted <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> over land and the inversion results are not sensitive to errors in the estimated disequilibria over land and ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ACP....17.9019B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ACP....17.9019B"><span>Estimation of bubble-mediated <span class="hlt">air-sea</span> gas exchange from concurrent DMS and <span class="hlt">CO</span><span class="hlt">2</span> transfer velocities at intermediate-high wind speeds</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bell, Thomas G.; Landwehr, Sebastian; Miller, Scott D.; de Bruyn, Warren J.; Callaghan, Adrian H.; Scanlon, Brian; Ward, Brian; Yang, Mingxi; Saltzman, Eric S.</p> <p>2017-07-01</p> <p>Simultaneous <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> and concentration differences of dimethylsulfide (DMS) and carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) were measured during a summertime North Atlantic cruise in 2011. This data set reveals significant differences between the gas transfer velocities of these two gases (Δkw) over a range of wind speeds up to 21 m s-1. These differences occur at and above the approximate wind speed threshold when waves begin breaking. Whitecap fraction (a proxy for bubbles) was also measured and has a positive relationship with Δkw, consistent with enhanced bubble-mediated transfer of the less soluble <span class="hlt">CO</span><span class="hlt">2</span> relative to that of the more soluble DMS. However, the correlation of Δkw with whitecap fraction is no stronger than with wind speed. Models used to estimate bubble-mediated transfer from in situ whitecap fraction underpredict the observations, particularly at intermediate wind speeds. Examining the differences between gas transfer velocities of gases with different solubilities is a useful way to detect the impact of bubble-mediated exchange. More simultaneous gas transfer measurements of different solubility gases across a wide range of oceanic conditions are needed to understand the factors controlling the magnitude and scaling of bubble-mediated gas exchange.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.1485G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.1485G"><span>Extreme <span class="hlt">air-sea</span> surface turbulent <span class="hlt">fluxes</span> in mid latitudes - estimation, origins and mechanisms</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gulev, Sergey; Natalia, Tilinina</p> <p>2014-05-01</p> <p>Extreme turbulent heat <span class="hlt">fluxes</span> in the North Atlantic and North Pacific mid latitudes were estimated from the modern era and first generation reanalyses (NCEP-DOE, ERA-Interim, MERRA NCEP-CFSR, JRA-25) for the period from 1979 onwards. We used direct surface turbulent <span class="hlt">flux</span> output as well as reanalysis state variables from which <span class="hlt">fluxes</span> have been computed using COARE-3 bulk algorithm. For estimation of extreme <span class="hlt">flux</span> values we analyzed surface <span class="hlt">flux</span> probability density distribution which was approximated by Modified Fisher-Tippett distribution. In all reanalyses extreme turbulent heat <span class="hlt">fluxes</span> amount to 1500-2000 W/m<span class="hlt">2</span> (for the 99th percentile) and can exceed 2000 W/m<span class="hlt">2</span> for higher percentiles in the western boundary current extension (WBCE) regions. Different reanalyses show significantly different shape of MFT distribution, implying considerable differences in the estimates of extreme <span class="hlt">fluxes</span>. The highest extreme turbulent latent heat <span class="hlt">fluxes</span> are diagnosed in NCEP-DOE, ERA-Interim and NCEP-CFSR reanalyses with the smallest being in MERRA. These differences may not necessarily reflect the differences in mean values. Analysis shows that differences in statistical properties of the state variables are the major source of differences in the shape of PDF of <span class="hlt">fluxes</span> and in the estimates of extreme <span class="hlt">fluxes</span> while the contribution of computational schemes used in different reanalyses is minor. The strongest differences in the characteristics of probability distributions of surface <span class="hlt">fluxes</span> and extreme surface <span class="hlt">flux</span> values between different reanalyses are found in the WBCE extension regions and high latitudes. In the next instance we analyzed the mechanisms responsible for forming surface turbulent <span class="hlt">fluxes</span> and their potential role in changes of midlatitudinal heat balance. Midlatitudinal cyclones were considered as the major mechanism responsible for extreme turbulent <span class="hlt">fluxes</span> which are typically occur during the cold <span class="hlt">air</span> outbreaks in the rear parts of cyclones when atmospheric conditions</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011JVGR..207..130C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011JVGR..207..130C"><span>Diffuse <span class="hlt">CO</span> <span class="hlt">2</span> soil degassing and <span class="hlt">CO</span> <span class="hlt">2</span> and H <span class="hlt">2</span>S concentrations in <span class="hlt">air</span> and related hazards at Vulcano Island (Aeolian arc, Italy)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carapezza, M. L.; Barberi, F.; Ranaldi, M.; Ricci, T.; Tarchini, L.; Barrancos, J.; Fischer, C.; Perez, N.; Weber, K.; Di Piazza, A.; Gattuso, A.</p> <p>2011-10-01</p> <p>La Fossa crater on Vulcano Island is quiescent since 1890. Periodically it undergoes "crises" characterized by marked increase of temperature (T), gas output and concentration of magmatic components in the crater fumaroles (T may exceed 600 °C). During these crises, which so far did not lead to any eruptive reactivation, the diffuse <span class="hlt">CO</span> <span class="hlt">2</span> soil degassing also increases and in December 2005 an anomalous <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">flux</span> of 1350 tons/day was estimated by 1588 measurements over a surface of 1.66 km <span class="hlt">2</span> extending from La Fossa crater to the inhabited zone of Vulcano Porto. The crater area and two other anomalously degassing sites (Levante Beach and Palizzi) have been periodically investigated from December 2004 to August 2010 for diffuse <span class="hlt">CO</span> <span class="hlt">2</span> soil <span class="hlt">flux</span>. They show a marked variation with time of the degassing rate, with synchronous maxima in December 2005. Carbon dioxide soil <span class="hlt">flux</span> and environmental parameters have been also continuously monitored for over one year by an automatic station at Vulcano Porto. In order to assess the hazard of the endogenous gas emissions, <span class="hlt">CO</span> <span class="hlt">2</span> and H <span class="hlt">2</span>S <span class="hlt">air</span> concentrations have been measured by Tunable Diode Laser profiles near the fumaroles of the crater rim and of the Levante Beach area, where also the viscous gas <span class="hlt">flux</span> has been estimated. In addition, <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">air</span> concentration has been measured both indoor and outdoor in an inhabited sector of Vulcano Porto. Results show that in some sites usually frequented by tourists there is a dangerous H <span class="hlt">2</span>S <span class="hlt">air</span> concentration and <span class="hlt">CO</span> <span class="hlt">2</span> exceeds the hazardous thresholds in some Vulcano houses. These zones should be immediately monitored for gas hazard should a new crisis arise.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.V31E..03C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.V31E..03C"><span><span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> from diffuse degassing in Italy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cardellini, C.; Chiodini, G.; Frondini, F.; Caliro, S.</p> <p>2016-12-01</p> <p>Central and southern Italy are affected by an intense process of <span class="hlt">CO</span><span class="hlt">2</span> Earth degassing from both active volcanoes, and tectonically active areas. Regional scale studies, based on C mass balance of groundwater of regional aquifers in not volcanically active areas, highlighted the presence of two large <span class="hlt">CO</span><span class="hlt">2</span> degassing structures that, for magnitude and the geochemical-isotopic features, were related to a regional process of mantle degassing. Quantitative estimates provided a <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> of 9 Mt/y for the region (62000 km<span class="hlt">2</span>). Besides the magnitude of the process, a strong link between the deep <span class="hlt">CO</span><span class="hlt">2</span> degassing and the seismicity of the region and a strict correlation between migration of deep <span class="hlt">CO</span><span class="hlt">2</span>-rich fluids and the heat <span class="hlt">flux</span> have been highlighted. In addition, the region is also characterised by the presence of many cold gas emissions where deeply derived <span class="hlt">CO</span><span class="hlt">2</span> is released by vents and soil diffuse degassing areas. Both direct <span class="hlt">CO</span><span class="hlt">2</span> expulsion at the surface and C-rich groundwater are different manifestations of the same process, in fact, the deeply produced gas can be dissolved by groundwater or emitted directly to the atmosphere depending on the gas <span class="hlt">flux</span> rate, and the geological-structural and hydrogeological settings. Quantitative estimations of the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> are available only for a limited number ( 30) of the about 270 catalogued gas manifestations allowing an estimations of a <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> of 1.4 Mt/y. Summing the two estimates the non-volcanic <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> from the region results globally relevant, being from <span class="hlt">2</span> to 10% of the estimated present-day global <span class="hlt">CO</span><span class="hlt">2</span> discharge from subaerial volcanoes. Large amounts of <span class="hlt">CO</span><span class="hlt">2</span> is also discharged by soil diffuse degassing in volcanic-hydrothermal systems. Specific surveys at Solfatara of Pozzuoli (Campi Flegrei Caldera) pointed out the relevance of this process. <span class="hlt">CO</span><span class="hlt">2</span> diffuse degassing at Solfatara, measured since 1998 shows a persistent <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> of 1300 t/d (± 390 t/d), a <span class="hlt">flux</span> comparable to an erupting volcano. The quantification of diffuse <span class="hlt">CO</span><span class="hlt">2</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS23B2025O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS23B2025O"><span>Field Observations of Coastal <span class="hlt">Air-Sea</span> Interaction</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ortiz-Suslow, D. G.; Haus, B. K.; Williams, N. J.; Graber, H. C.</p> <p>2016-12-01</p> <p>In the nearshore zone wind, waves, and currents generated from different forcing mechanisms converge in shallow water. This can profoundly affect the physical nature of the ocean surface, which can significantly modulate the exchange of momentum, heat, and mass across the <span class="hlt">air-sea</span> interface. For decades, the focus of <span class="hlt">air-sea</span> interaction research has been on the open ocean while the shallow water regime has been relatively under-explored. This bears implications for efforts to understand and model various coastal processes, such as mixing, surface transport, and <span class="hlt">air-sea</span> gas <span class="hlt">flux</span>. The results from a recent study conducted at the New River Inlet in North Carolina showed that directly measured <span class="hlt">air-sea</span> <span class="hlt">flux</span> parameters, such as the atmospheric drag coefficient, are strong functions of space as well as the ambient conditions (i.e. wind speed and direction). The drag is typically used to parameterize the wind stress magnitude. It is generally assumed that the wind direction is the direction of the atmospheric forcing (i.e. wind stress), however significant wind stress steering off of the azimuthal wind direction was observed and was found to be related to the horizontal surface current shear. The authors have just returned from a field campaign carried out within Monterey Bay in California. Surface observations made from two research vessels were complimented by an array of beach and inland <span class="hlt">flux</span> stations, high-resolution wind forecasts, and satellite image acquisitions. This is a rich data set and several case studies will be analyzed to highlight the importance of various processes for understanding the <span class="hlt">air-sea</span> <span class="hlt">fluxes</span>. Preliminary findings show that interactions between the local wind-<span class="hlt">sea</span> and the shoaling, incident swell can have a profound effect on the wind stress magnitude. The Monterey Bay coastline contains a variety of topographical features and the importance of land-<span class="hlt">air-sea</span> interactions will also be investigated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1714877S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1714877S"><span>Accounting for observational uncertainties in the evaluation of low latitude turbulent <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> simulated in a suite of IPSL model versions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Servonnat, Jerome; Braconnot, Pascale; Gainusa-Bogdan, Alina</p> <p>2015-04-01</p> <p>Turbulent momentum and heat (sensible and latent) <span class="hlt">fluxes</span> at the <span class="hlt">air-sea</span> interface are key components of the whole energetic of the Earth's climate and their good representation in climate models is of prime importance. In this work, we use the methodology developed by Braconnot & Frankignoul (1993) to perform a Hotelling T<span class="hlt">2</span> test on spatio-temporal fields (annual cycles). This statistic provides a quantitative measure accounting for an estimate of the observational uncertainty for the evaluation of low-latitude turbulent <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> in a suite of IPSL model versions. The spread within the observational ensemble of turbulent <span class="hlt">flux</span> data products assembled by Gainusa-Bogdan et al (submitted) is used as an estimate of the observational uncertainty for the different turbulent <span class="hlt">fluxes</span>. The methodology holds on a selection of a small number of dominating variability patterns (EOFs) that are common to both the model and the observations for the comparison. Consequently it focuses on the large-scale variability patterns and avoids the possibly noisy smaller scales. The results show that different versions of the IPSL couple model share common large scale model biases, but also that there the skill on <span class="hlt">sea</span> surface temperature is not necessarily directly related to the skill in the representation of the different turbulent <span class="hlt">fluxes</span>. Despite the large error bars on the observations the test clearly distinguish the different merits of the different model version. The analyses of the common EOF patterns and related time series provide guidance on the major differences with the observations. This work is a first attempt to use such statistic on the evaluation of the spatio-temporal variability of the turbulent <span class="hlt">fluxes</span>, accounting for an observational uncertainty, and represents an efficient tool for systematic evaluation of simulated <span class="hlt">air</span>-seafluxes, considering both the <span class="hlt">fluxes</span> and the related atmospheric variables. References Braconnot, P., and C. Frankignoul (1993), Testing Model</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1351785','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1351785"><span>Nonlinear <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">flux</span> response to 7 years of experimentally induced permafrost thaw</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Mauritz, Marguerite; Bracho, Rosvel; Celis, Gerardo</p> <p></p> <p>Rapid Arctic warming is expected to increase global greenhouse gas concentrations as permafrost thaw exposes immense stores of frozen carbon (C) to microbial decomposition. Permafrost thaw also stimulates plant growth, which could offset C loss. Using data from 7 years of experimental <span class="hlt">Air</span> and Soil warming in moist acidic tundra, we show that Soil warming had a much stronger effect on <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">flux</span> than <span class="hlt">Air</span> warming. Soil warming caused rapid permafrost thaw and increased ecosystem respiration (R eco), gross primary productivity (GPP), and net summer <span class="hlt">CO</span> <span class="hlt">2</span> storage (NEE). Over 7 years R eco, GPP, and NEE also increasedmore » in Control (i.e., ambient plots), but this change could be explained by slow thaw in Control areas. In the initial stages of thaw, R eco, GPP, and NEE increased linearly with thaw across all treatments, despite different rates of thaw. As thaw in Soil warming continued to increase linearly, ground surface subsidence created saturated microsites and suppressed R eco, GPP, and NEE. However R eco and GPP remained high in areas with large Eriophorum vaginatum biomass. In general NEE increased with thaw, but was more strongly correlated with plant biomass than thaw, indicating that higher R eco in deeply thawed areas during summer months was balanced by GPP. Summer <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">flux</span> across treatments fit a single quadratic relationship that captured the functional response of <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">flux</span> to thaw, water table depth, and plant biomass. These results demonstrate the importance of indirect thaw effects on <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">flux</span>: plant growth and water table dynamics. Nonsummer R eco models estimated that the area was an annual <span class="hlt">CO</span> <span class="hlt">2</span> source during all years of observation. As a result, nonsummer <span class="hlt">CO</span> <span class="hlt">2</span> loss in warmer, more deeply thawed soils exceeded the increases in summer GPP, and thawed tundra was a net annual <span class="hlt">CO</span> <span class="hlt">2</span> source.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1351785-nonlinear-co2-flux-response-nbsp-years-experimentally-induced-permafrost-thaw','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1351785-nonlinear-co2-flux-response-nbsp-years-experimentally-induced-permafrost-thaw"><span>Nonlinear <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">flux</span> response to 7 years of experimentally induced permafrost thaw</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Mauritz, Marguerite; Bracho, Rosvel; Celis, Gerardo; ...</p> <p>2017-02-16</p> <p>Rapid Arctic warming is expected to increase global greenhouse gas concentrations as permafrost thaw exposes immense stores of frozen carbon (C) to microbial decomposition. Permafrost thaw also stimulates plant growth, which could offset C loss. Using data from 7 years of experimental <span class="hlt">Air</span> and Soil warming in moist acidic tundra, we show that Soil warming had a much stronger effect on <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">flux</span> than <span class="hlt">Air</span> warming. Soil warming caused rapid permafrost thaw and increased ecosystem respiration (R eco), gross primary productivity (GPP), and net summer <span class="hlt">CO</span> <span class="hlt">2</span> storage (NEE). Over 7 years R eco, GPP, and NEE also increasedmore » in Control (i.e., ambient plots), but this change could be explained by slow thaw in Control areas. In the initial stages of thaw, R eco, GPP, and NEE increased linearly with thaw across all treatments, despite different rates of thaw. As thaw in Soil warming continued to increase linearly, ground surface subsidence created saturated microsites and suppressed R eco, GPP, and NEE. However R eco and GPP remained high in areas with large Eriophorum vaginatum biomass. In general NEE increased with thaw, but was more strongly correlated with plant biomass than thaw, indicating that higher R eco in deeply thawed areas during summer months was balanced by GPP. Summer <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">flux</span> across treatments fit a single quadratic relationship that captured the functional response of <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">flux</span> to thaw, water table depth, and plant biomass. These results demonstrate the importance of indirect thaw effects on <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">flux</span>: plant growth and water table dynamics. Nonsummer R eco models estimated that the area was an annual <span class="hlt">CO</span> <span class="hlt">2</span> source during all years of observation. As a result, nonsummer <span class="hlt">CO</span> <span class="hlt">2</span> loss in warmer, more deeply thawed soils exceeded the increases in summer GPP, and thawed tundra was a net annual <span class="hlt">CO</span> <span class="hlt">2</span> source.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28208232','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28208232"><span>Nonlinear <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> response to 7 years of experimentally induced permafrost thaw.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mauritz, Marguerite; Bracho, Rosvel; Celis, Gerardo; Hutchings, Jack; Natali, Susan M; Pegoraro, Elaine; Salmon, Verity G; Schädel, Christina; Webb, Elizabeth E; Schuur, Edward A G</p> <p>2017-09-01</p> <p>Rapid Arctic warming is expected to increase global greenhouse gas concentrations as permafrost thaw exposes immense stores of frozen carbon (C) to microbial decomposition. Permafrost thaw also stimulates plant growth, which could offset C loss. Using data from 7 years of experimental <span class="hlt">Air</span> and Soil warming in moist acidic tundra, we show that Soil warming had a much stronger effect on <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">flux</span> than <span class="hlt">Air</span> warming. Soil warming caused rapid permafrost thaw and increased ecosystem respiration (R eco ), gross primary productivity (GPP), and net summer <span class="hlt">CO</span> <span class="hlt">2</span> storage (NEE). Over 7 years R eco , GPP, and NEE also increased in Control (i.e., ambient plots), but this change could be explained by slow thaw in Control areas. In the initial stages of thaw, R eco , GPP, and NEE increased linearly with thaw across all treatments, despite different rates of thaw. As thaw in Soil warming continued to increase linearly, ground surface subsidence created saturated microsites and suppressed R eco , GPP, and NEE. However R eco and GPP remained high in areas with large Eriophorum vaginatum biomass. In general NEE increased with thaw, but was more strongly correlated with plant biomass than thaw, indicating that higher R eco in deeply thawed areas during summer months was balanced by GPP. Summer <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">flux</span> across treatments fit a single quadratic relationship that captured the functional response of <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">flux</span> to thaw, water table depth, and plant biomass. These results demonstrate the importance of indirect thaw effects on <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">flux</span>: plant growth and water table dynamics. Nonsummer R eco models estimated that the area was an annual <span class="hlt">CO</span> <span class="hlt">2</span> source during all years of observation. Nonsummer <span class="hlt">CO</span> <span class="hlt">2</span> loss in warmer, more deeply thawed soils exceeded the increases in summer GPP, and thawed tundra was a net annual <span class="hlt">CO</span> <span class="hlt">2</span> source. © 2017 John Wiley & Sons Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20080015856&hterms=Fuel+co2&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DFuel%2Bco2','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20080015856&hterms=Fuel+co2&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DFuel%2Bco2"><span>Using <span class="hlt">CO</span><span class="hlt">2</span>:<span class="hlt">CO</span> Correlations to Improve Inverse Analyses of Carbon <span class="hlt">Fluxes</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Palmer, Paul I.; Suntharalingam, Parvadha; Jones, Dylan B. A.; Jacob, Daniel J.; Streets, David G.; Fu, Qingyan; Vay, Stephanie A.; Sachse, Glen W.</p> <p>2006-01-01</p> <p>Observed correlations between atmospheric concentrations of <span class="hlt">CO</span><span class="hlt">2</span> and <span class="hlt">CO</span> represent potentially powerful information for improving <span class="hlt">CO</span><span class="hlt">2</span> surface <span class="hlt">flux</span> estimates through coupled <span class="hlt">CO</span><span class="hlt">2</span>-<span class="hlt">CO</span> inverse analyses. We explore the value of these correlations in improving estimates of regional <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in east Asia by using aircraft observations of <span class="hlt">CO</span><span class="hlt">2</span> and <span class="hlt">CO</span> from the TRACE-P campaign over the NW Pacific in March 2001. Our inverse model uses regional <span class="hlt">CO</span><span class="hlt">2</span> and <span class="hlt">CO</span> surface <span class="hlt">fluxes</span> as the state vector, separating biospheric and combustion contributions to <span class="hlt">CO</span><span class="hlt">2</span>. <span class="hlt">CO</span><span class="hlt">2</span>-<span class="hlt">CO</span> error correlation coefficients are included in the inversion as off-diagonal entries in the a priori and observation error covariance matrices. We derive error correlations in a priori combustion source estimates of <span class="hlt">CO</span><span class="hlt">2</span> and <span class="hlt">CO</span> by propagating error estimates of fuel consumption rates and emission factors. However, we find that these correlations are weak because <span class="hlt">CO</span> source uncertainties are mostly determined by emission factors. Observed correlations between atmospheric <span class="hlt">CO</span><span class="hlt">2</span> and <span class="hlt">CO</span> concentrations imply corresponding error correlations in the chemical transport model used as the forward model for the inversion. These error correlations in excess of 0.7, as derived from the TRACE-P data, enable a coupled <span class="hlt">CO</span><span class="hlt">2</span>-<span class="hlt">CO</span> inversion to achieve significant improvement over a <span class="hlt">CO</span><span class="hlt">2</span>-only inversion for quantifying regional <span class="hlt">fluxes</span> of <span class="hlt">CO</span><span class="hlt">2</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19850005886&hterms=heat+exchange&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dheat%2Bexchange','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19850005886&hterms=heat+exchange&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dheat%2Bexchange"><span><span class="hlt">Air-sea</span> heat exchange, an element of the water cycle</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chahine, M. T.</p> <p>1984-01-01</p> <p>The distribution and variation of water vapor, clouds and precipitation are examined. Principal driving forces for these distributions are energy exchange and evaporation at the <span class="hlt">air-sea</span> interface, which are also important elements of <span class="hlt">air-sea</span> interaction studies. The overall aim of <span class="hlt">air-sea</span> interaction studies is to quantitatively determine mass, momentum and energy <span class="hlt">fluxes</span>, with the goal of understanding the mechanisms controlling them. The results of general circulation simulations indicate that the atmosphere in mid-latitudes responds to changes in the oceanic surface conditions in the tropics. This correlation reflects the strong interaction between tropical and mid-latitude conditions caused by the transport of heat and momentum from the tropics. Studies of <span class="hlt">air-sea</span> exchanges involve a large number of physica, chemical and dynamical processes including heat <span class="hlt">flux</span>, radiation, <span class="hlt">sea</span>-surface temperature, precipitation, winds and ocean currents. The <span class="hlt">fluxes</span> of latent heat are studied and the potential use of satellite data in determining them evaluated. Alternative ways of inferring heat <span class="hlt">fluxes</span> will be considered.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOS.A54C2732S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOS.A54C2732S"><span>Enhanced Ahead-of-Eye TC Coastal Ocean Cooling Processes and their Impact on <span class="hlt">Air-Sea</span> Heat <span class="hlt">Fluxes</span> and Storm Intensity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Seroka, G. N.; Miles, T. N.; Glenn, S. M.; Xu, Y.; Forney, R.; Roarty, H.; Schofield, O.; Kohut, J. T.</p> <p>2016-02-01</p> <p>Any landfalling tropical cyclone (TC) must first traverse the coastal ocean. TC research, however, has focused over the deep ocean, where TCs typically spend the vast majority of their lifetime. This paper will show that the ocean's response to TCs can be different between deep and shallow water, and that the additional shallow water processes must be included in coupled models for accurate <span class="hlt">air-sea</span> <span class="hlt">flux</span> treatment and TC intensity prediction. The authors will present newly observed coastal ocean processes that occurred in response to Hurricane Irene (2011), due to the presence of a coastline, an ocean bottom, and highly stratified conditions. These newly observed processes led to enhanced ahead-of-eye SST cooling that significantly impacted <span class="hlt">air-sea</span> heat <span class="hlt">fluxes</span> and Irene's operationally over-predicted storm intensity. Using semi-idealized modeling, we find that in shallow water in Irene, only 6% of cooling due to <span class="hlt">air-sea</span> heat <span class="hlt">fluxes</span>, 17% of cooling due to 1D vertical mixing, and 50% of cooling due to all processes (1D mixing, <span class="hlt">air-sea</span> heat <span class="hlt">fluxes</span>, upwelling, and advection) occurred ahead-of-eye—consistent with previous studies. Observations from an underwater glider and buoys, however, indicated 75-100% of total SST cooling over the continental shelf was ahead-of-eye. Thus, the new coastal ocean cooling processes found in this study must occur almost completely ahead-of-eye. We show that Irene's intense cooling was not captured by basic satellite SST products and coupled ocean-atmosphere hurricane models, and that including the cooling in WRF modeling mitigated the high bias in model predictions. Finally, we provide evidence that this SST cooling—not track, wind shear, or dry <span class="hlt">air</span> intrusion—was the key missing contribution to Irene's decay just prior to NJ landfall. Ongoing work is exploring the use of coupled WRF-ROMS modeling in the coastal zone.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.A42F..07L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.A42F..07L"><span>Simultaneous assimilation of <span class="hlt">AIRS</span> and GOSAT <span class="hlt">CO</span><span class="hlt">2</span> observations with Ensemble Kalman filter</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liu, J.; Kalnay, E.; Fung, I.; Kang, J.</p> <p>2012-12-01</p> <p>Lack of <span class="hlt">CO</span><span class="hlt">2</span> vertical information could lead to bias in the surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> estimation (Stephens et al., 2007). Liu et al. (2012) showed that assimilating <span class="hlt">AIRS</span> <span class="hlt">CO</span><span class="hlt">2</span> observations, which are sensitive to middle to upper troposphere <span class="hlt">CO</span><span class="hlt">2</span>, improves <span class="hlt">CO</span><span class="hlt">2</span> concentration, especially in the middle to upper troposphere. GOSAT is sensitive to <span class="hlt">CO</span><span class="hlt">2</span> over the whole column, but the spatial coverage is sparser than <span class="hlt">AIRS</span>. In this study, we assimilate <span class="hlt">AIRS</span> and GOSAT <span class="hlt">CO</span><span class="hlt">2</span> observations simultaneously along with surface flask <span class="hlt">CO</span><span class="hlt">2</span> observations and meteorology observations with Ensemble Kalman filter (EnKF) to constrain <span class="hlt">CO</span><span class="hlt">2</span> vertical profiles simulated by NCAR carbon-climate model. We will show the impact of assimilating <span class="hlt">AIRS</span> and GOSAT <span class="hlt">CO</span><span class="hlt">2</span> on the <span class="hlt">CO</span><span class="hlt">2</span> vertical gradient, seasonal cycle and spatial gradient by assimilating only GOSAT or <span class="hlt">AIRS</span> and comparing to the control experiment. The quality of <span class="hlt">CO</span><span class="hlt">2</span> analysis will be examined by validating against independent <span class="hlt">CO</span><span class="hlt">2</span> aircraft observations, and analyzing the relationship between <span class="hlt">CO</span><span class="hlt">2</span> analysis fields and major circulation, such as Madden Julian Oscillation. We will also discuss the deficiencies of the observation network in understanding the carbon cycle.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.A43H..07F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.A43H..07F"><span>Evaluation of NASA's Carbon Monitoring System (CMS) <span class="hlt">Flux</span> Pilot: Terrestrial <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fisher, J. B.; Polhamus, A.; Bowman, K. W.; Collatz, G. J.; Potter, C. S.; Lee, M.; Liu, J.; Jung, M.; Reichstein, M.</p> <p>2011-12-01</p> <p>NASA's Carbon Monitoring System (CMS) <span class="hlt">flux</span> pilot project combines NASA's Earth System models in land, ocean and atmosphere to track surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. The system is constrained by atmospheric measurements of XCO<span class="hlt">2</span> from the Japanese GOSAT satellite, giving a "big picture" view of total <span class="hlt">CO</span><span class="hlt">2</span> in Earth's atmosphere. Combining two land models (CASA-Ames and CASA-GFED), two ocean models (ECCO<span class="hlt">2</span> and NOBM) and two atmospheric chemistry and inversion models (GEOS-5 and GEOS-Chem), the system brings together the stand-alone component models of the Earth System, all of which are run diagnostically constrained by a multitude of other remotely sensed data. Here, we evaluate the biospheric land surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> (i.e., net ecosystem exchange, NEE) as estimated from the atmospheric <span class="hlt">flux</span> inversion. We compare against the prior bottom-up estimates (e.g., the CASA models) as well. Our evaluation dataset is the independently derived global wall-to-wall MPI-BGC product, which uses a machine learning algorithm and model tree ensemble to "scale-up" a network of in situ <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> measurements from 253 globally-distributed sites in the FLUXNET network. The measurements are based on the eddy covariance method, which uses observations of <span class="hlt">co</span>-varying <span class="hlt">fluxes</span> of <span class="hlt">CO</span><span class="hlt">2</span> (and water and energy) from instruments on towers extending above ecosystem canopies; the towers integrate <span class="hlt">fluxes</span> over large spatial areas (~1 km<span class="hlt">2</span>). We present global maps of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> and differences between products, summaries of <span class="hlt">fluxes</span> by TRANSCOM region, country, latitude, and biome type, and assess the time series, including timing of minimum and maximum <span class="hlt">fluxes</span>. This evaluation shows both where the CMS is performing well, and where improvements should be directed in further work.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JGRC..120..471M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JGRC..120..471M"><span>Drivers of inorganic carbon dynamics in first-year <span class="hlt">sea</span> ice: A model study</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moreau, Sébastien; Vancoppenolle, Martin; Delille, Bruno; Tison, Jean-Louis; Zhou, Jiayun; Kotovitch, Marie; Thomas, David N.; Geilfus, Nicolas-Xavier; Goosse, Hugues</p> <p>2015-01-01</p> <p><span class="hlt">Sea</span> ice is an active source or a sink for carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>), although to what extent is not clear. Here, we analyze <span class="hlt">CO</span><span class="hlt">2</span> dynamics within <span class="hlt">sea</span> ice using a one-dimensional halothermodynamic <span class="hlt">sea</span> ice model including gas physics and carbon biogeochemistry. The ice-ocean <span class="hlt">fluxes</span>, and vertical transport, of total dissolved inorganic carbon (DIC) and total alkalinity (TA) are represented using fluid transport equations. Carbonate chemistry, the consumption, and release of <span class="hlt">CO</span><span class="hlt">2</span> by primary production and respiration, the precipitation and dissolution of ikaite (Ca<span class="hlt">CO</span>3·6H<span class="hlt">2</span>O) and ice-<span class="hlt">air</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>, are also included. The model is evaluated using observations from a 6 month field study at Point Barrow, Alaska, and an ice-tank experiment. At Barrow, results show that the DIC budget is mainly driven by physical processes, wheras brine-<span class="hlt">air</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>, ikaite formation, and net primary production, are secondary factors. In terms of ice-atmosphere <span class="hlt">CO</span><span class="hlt">2</span> exchanges, <span class="hlt">sea</span> ice is a net <span class="hlt">CO</span><span class="hlt">2</span> source and sink in winter and summer, respectively. The formulation of the ice-atmosphere <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> impacts the simulated near-surface <span class="hlt">CO</span><span class="hlt">2</span> partial pressure (p<span class="hlt">CO</span><span class="hlt">2</span>), but not the DIC budget. Because the simulated ice-atmosphere <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> are limited by DIC stocks, and therefore <<span class="hlt">2</span> mmol m-<span class="hlt">2</span> d-1, we argue that the observed much larger <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> from eddy covariance retrievals cannot be explained by a <span class="hlt">sea</span> ice direct source and must involve other processes or other sources of <span class="hlt">CO</span><span class="hlt">2</span>. Finally, the simulations suggest that near-surface TA/DIC ratios of ˜<span class="hlt">2</span>, sometimes used as an indicator of calcification, would rather suggest outgassing.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li class="active"><span>7</span></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_7 --> <div id="page_8" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li class="active"><span>8</span></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="141"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1711342M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1711342M"><span>Drivers of inorganic carbon dynamics in first-year <span class="hlt">sea</span> ice: A model study</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moreau, Sébastien; Vancoppenolle, Martin; Delille, Bruno; Tison, Jean-Louis; Zhou, Jiayun; Kotovich, Marie; Thomas, David; Geilfus, Nicolas-Xavier; Goosse, Hugues</p> <p>2015-04-01</p> <p><span class="hlt">Sea</span> ice is an active source or a sink for carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>), although to what extent is not clear. Here, we analyze <span class="hlt">CO</span><span class="hlt">2</span> dynamics within <span class="hlt">sea</span> ice using a one-dimensional halo-thermodynamic <span class="hlt">sea</span> ice model including gas physics and carbon biogeochemistry. The ice-ocean <span class="hlt">fluxes</span>, and vertical transport, of total dissolved inorganic carbon (DIC) and total alkalinity (TA) are represented using fluid transport equations. Carbonate chemistry, the consumption and release of <span class="hlt">CO</span><span class="hlt">2</span> by primary production and respiration, the precipitation and dissolution of ikaite (Ca<span class="hlt">CO</span>3•6H<span class="hlt">2</span>O) and ice-<span class="hlt">air</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>, are also included. The model is evaluated using observations from a 6-month field study at Point Barrow, Alaska and an ice-tank experiment. At Barrow, results show that the DIC budget is mainly driven by physical processes, wheras brine-<span class="hlt">air</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>, ikaite formation, and net primary production, are secondary factors. In terms of ice-atmosphere <span class="hlt">CO</span><span class="hlt">2</span> exchanges, <span class="hlt">sea</span> ice is a net <span class="hlt">CO</span><span class="hlt">2</span> source and sink in winter and summer, respectively. The formulation of the ice-atmosphere <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> impacts the simulated near-surface <span class="hlt">CO</span><span class="hlt">2</span> partial pressure (p<span class="hlt">CO</span><span class="hlt">2</span>), but not the DIC budget. Because the simulated ice-atmosphere <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> are limited by DIC stocks, and therefore < <span class="hlt">2</span> mmol m-<span class="hlt">2</span> day-1, we argue that the observed much larger <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> from eddy covariance retrievals cannot be explained by a <span class="hlt">sea</span> ice direct source and must involve other processes or other sources of <span class="hlt">CO</span><span class="hlt">2</span>. Finally, the simulations suggest that near surface TA/DIC ratios of ~<span class="hlt">2</span>, sometimes used as an indicator of calcification, would rather suggest outgassing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.4005G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.4005G"><span>Characterization of extreme <span class="hlt">air-sea</span> turbulent <span class="hlt">fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gulev, Sergey; Belyaev, Konstantin</p> <p>2017-04-01</p> <p>Extreme ocean-atmosphere turbulent <span class="hlt">fluxes</span> play a critical role in the convective processes in the mid and subpolar latitudes and may also affect a variety of atmospheric processes, such as generation and re-intensification of extreme cyclones in the areas of the mid latitude storm tracks. From the ocean dynamics perspective, specifically for quantifying extreme vertical mixing, characterization of the extreme <span class="hlt">fluxes</span> requires, besides estimation of the extreme events, also consideration of the relative extremeness of surface <span class="hlt">fluxes</span> and their timing, e.g. the duration of periods of high surface <span class="hlt">fluxes</span>. In order to comprehensively characterize extreme turbulent <span class="hlt">fluxes</span> at <span class="hlt">sea</span> surface we propose a formalism based upon probability density distributions of surface turbulent <span class="hlt">fluxes</span> and <span class="hlt">flux</span>-related variables. Individual absolute <span class="hlt">flux</span> extremes were derived using Modified Fisher-Tippett (MFT) distribution of turbulent <span class="hlt">fluxes</span>. Then, we extend this distribution to the fractional distribution, characterizing the fraction of time-integrated turbulent heat <span class="hlt">flux</span> provided by the <span class="hlt">fluxes</span> exceeding a given percentile. Finally, we consider the time durations during which <span class="hlt">fluxes</span> of a given intensity provide extreme accumulations of heat loss from the surface. For estimation of these characteristics of surface <span class="hlt">fluxes</span> we use <span class="hlt">fluxes</span> recomputed from the state variables available from modern era reanalyses (ERA-Interim, MERRA and CFSR) for the period from 1979 onwards. Applications of the formalism to the VOS (Voluntary Observing Ship) - based surface <span class="hlt">fluxes</span> are also considered. We discuss application of the new metrics of mesoscale and synoptic variability of surface <span class="hlt">fluxes</span> to the dynamics of mixed layer depth in the North Atlantic.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.1015G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.1015G"><span>Evaluation of the swell effect on the <span class="hlt">air-sea</span> gas transfer in the coastal zone</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gutiérrez-Loza, Lucía; Ocampo-Torres, Francisco J.</p> <p>2016-04-01</p> <p><span class="hlt">Air-sea</span> gas transfer processes are one of the most important factors regarding global climate and long-term global climate changes. Despite its importance, there is still a huge uncertainty on how to better parametrize these processes in order to include them on the global climate models. This uncertainty exposes the need to increase our knowledge on gas transfer controlling mechanisms. In the coastal regions, breaking waves become a key factor to take into account when estimating gas <span class="hlt">fluxes</span>, however, there is still a lack of information and the influence of the ocean surface waves on the <span class="hlt">air-sea</span> interaction and gas <span class="hlt">flux</span> behavior must be validated. In this study, as part of the "<span class="hlt">Sea</span> Surface Roughness as <span class="hlt">Air-Sea</span> Interaction Control" project, we evaluate the effect of the ocean surface waves on the gas exchange in the coastal zone. Direct estimates of the <span class="hlt">flux</span> of <span class="hlt">CO</span><span class="hlt">2</span> (FCO<span class="hlt">2</span>) and water vapor (FH<span class="hlt">2</span>O) through eddy covariance, were carried out from May 2014 to April 2015 in a coastal station located at the Northwest of Todos Santos Bay, Baja California, México. For the same period, ocean surface waves are recorded using an Acoustic Doppler Current Profiler (Workhorse Sentinel, Teledyne RD Instruments) with a sampling rate of <span class="hlt">2</span> Hz and located at 10 m depth about 350 m away from the tower. We found the study area to be a weak sink of <span class="hlt">CO</span><span class="hlt">2</span> under moderate wind and wave conditions with a mean <span class="hlt">flux</span> of -1.32 μmol/m<span class="hlt">2</span>s. The correlation between the wind speed and FCO<span class="hlt">2</span> was found to be weak, suggesting that other physical processes besides wind may be important factors for the gas exchange modulation at coastal waters. The results of the quantile regression analysis computed between FCO<span class="hlt">2</span> and (1) wind speed, (<span class="hlt">2</span>) significant wave height, (3) wave steepness and (4) water temperature, show that the significant wave height is the most correlated parameter with FCO<span class="hlt">2</span>; Nevertheless, the behavior of their relation varies along the probability distribution of FCO<span class="hlt">2</span>, with the linear regression</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.A53E0229L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.A53E0229L"><span>A Synthesized Model-Observation Approach to Constraining Gross Urban <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Fluxes</span> Using 14<span class="hlt">CO</span><span class="hlt">2</span> and carbonyl sulfide</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>LaFranchi, B. W.; Campbell, J. E.; Cameron-Smith, P. J.; Bambha, R.; Michelsen, H. A.</p> <p>2013-12-01</p> <p>Urbanized regions are responsible for a disproportionately large percentage (30-40%) of global anthropogenic greenhouse gas (GHG) emissions, despite covering only <span class="hlt">2</span>% of the Earth's surface area [Satterthwaite, 2008]. As a result, policies enacted at the local level in these urban areas can, in aggregate, have a large global impact, both positive and negative. In order to address the scientific questions that are required to drive these policy decisions, methods are needed that resolve gross <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> components from the net <span class="hlt">flux</span>. Recent work suggests that the critical knowledge gaps in <span class="hlt">CO</span><span class="hlt">2</span> surface <span class="hlt">fluxes</span> could be addressed through the combined analysis of atmospheric carbonyl sulfide (COS) and radiocarbon in atmospheric <span class="hlt">CO</span><span class="hlt">2</span> (14<span class="hlt">CO</span><span class="hlt">2</span>) [e.g. Campbell et al., 2008; Graven et al., 2009]. The 14<span class="hlt">CO</span><span class="hlt">2</span> approach relies on mass balance assumptions about atmospheric <span class="hlt">CO</span><span class="hlt">2</span> and the large differences in 14<span class="hlt">CO</span><span class="hlt">2</span> abundance between fossil and natural sources of <span class="hlt">CO</span><span class="hlt">2</span> [Levin et al., 2003]. COS, meanwhile, is a potentially transformative tracer of photosynthesis because its variability in the atmosphere has been found to be influenced primarily by vegetative uptake, scaling linearly will gross primary production (GPP) [Kettle et al., 20027]. Taken together, these two observations provide constraints on two of the three main components of the <span class="hlt">CO</span><span class="hlt">2</span> budget at the urban scale: photosynthesis and fossil fuel emissions. The third component, respiration, can then be determined by difference if the net <span class="hlt">flux</span> is known. Here we present a general overview of our synthesized model-observation approach for improving surface <span class="hlt">flux</span> estimates of <span class="hlt">CO</span><span class="hlt">2</span> for the upwind fetch of a ~30m tower located in Livermore, CA, USA, a suburb (pop. ~80,000) at the eastern edge of the San Francisco Bay Area. Additionally, we will present initial results from a one week observational intensive, which includes continuous <span class="hlt">CO</span><span class="hlt">2</span>, CH4, <span class="hlt">CO</span>, SO<span class="hlt">2</span>, NOx, and O3 observations in addition to measurements of 14<span class="hlt">CO</span><span class="hlt">2</span> and COS from <span class="hlt">air</span> samples</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013ACPD...1313285B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013ACPD...1313285B"><span><span class="hlt">Air/sea</span> DMS gas transfer in the North Atlantic: evidence for limited interfacial gas exchange at high wind speed</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bell, T. G.; De Bruyn, W.; Miller, S. D.; Ward, B.; Christensen, K.; Saltzman, E. S.</p> <p>2013-05-01</p> <p>Shipboard measurements of eddy covariance DMS <span class="hlt">air/sea</span> <span class="hlt">fluxes</span> and seawater concentration were carried out in the North Atlantic bloom region in June/July 2011. Gas transfer coefficients (k660) show a linear dependence on mean horizontal wind speed at wind speeds up to 11 m s-1. At higher wind speeds the relationship between k660 and wind speed weakens. At high winds, measured DMS <span class="hlt">fluxes</span> were lower than predicted based on the linear relationship between wind speed and interfacial stress extrapolated from low to intermediate wind speeds. In contrast, the transfer coefficient for sensible heat did not exhibit this effect. The apparent suppression of <span class="hlt">air/sea</span> gas <span class="hlt">flux</span> at higher wind speeds appears to be related to <span class="hlt">sea</span> state, as determined from shipboard wave measurements. These observations are consistent with the idea that long waves suppress near surface water side turbulence, and decrease interfacial gas transfer. This effect may be more easily observed for DMS than for less soluble gases, such as <span class="hlt">CO</span><span class="hlt">2</span>, because the <span class="hlt">air/sea</span> exchange of DMS is controlled by interfacial rather than bubble-mediated gas transfer under high wind speed conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.B43H0528Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.B43H0528Y"><span>Effects of a holiday week on urban soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span>: an intensive study in Xiamen, southeastern China</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ye, H.; Wang, K.; Chen, F.</p> <p>2012-12-01</p> <p>To study the effects of a holiday period on urban soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span>, <span class="hlt">CO</span><span class="hlt">2</span> efflux from grassland soil in a traditional park in the city of Xiamen was measured hourly from 28th Sep to 11th Oct, a period that included China's National Day holiday week in 2009. The results of this study revealed that: a) The urban soil <span class="hlt">CO</span><span class="hlt">2</span> emissions were higher before and after the holiday week and lower during the National Day holiday reflecting changes in the traffic cycles; b) A diurnal cycle where the soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> decreased from early morning to noon was associated with <span class="hlt">CO</span><span class="hlt">2</span> uptake by vegetation which strongly offset vehicle <span class="hlt">CO</span><span class="hlt">2</span> emissions. The soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> increased from night to early morning, associated with reduced <span class="hlt">CO</span><span class="hlt">2</span> uptake by vegetation; c) During the National Day holiday week in 2009, lower rates of soil respiration were measured after Mid-Autumn Day than earlier in the week, and this was related to a reduced level of human activities and vehicle traffic, reducing the <span class="hlt">CO</span><span class="hlt">2</span> concentration in the <span class="hlt">air</span>. Urban holidays have a clear effect on soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> through the interactions between vehicle, visitor and vegetation <span class="hlt">CO</span><span class="hlt">2</span> emissions which indirectly control the use of carbon by plant roots, the rhizosphere and soil microorganisms. Consequently, appropriate traffic controls and tourism travel plans can have positive effects on the soil carbon store and may improve local <span class="hlt">air</span> quality.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017DyAtO..80...47D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017DyAtO..80...47D"><span>An assessment of Trop<span class="hlt">Flux</span> and NCEP <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> on ROMS simulations over the Bay of Bengal region</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dey, Dipanjan; Sil, Sourav; Jana, Sudip; Pramanik, Saikat; Pandey, P. C.</p> <p>2017-12-01</p> <p>This study presents an assessment of the Trop<span class="hlt">Flux</span> and the National Centers for Environmental Prediction (NCEP) reanalysis <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> in simulating the surface and subsurface oceanic parameters over the Bay of Bengal (BoB) region during 2002-2014 using the Regional Ocean Modelling System (ROMS). The assessment has been made by comparing the simulated fields with in-situ and satellite observations. The simulated surface and subsurface temperatures in the Trop<span class="hlt">Flux</span> forced experiment (Trop<span class="hlt">Flux</span>-E) show better agreement with the Research Moored Array for African-Asian-Australian Monsoon Analysis (RAMA) and Argo observations than the NCEP forced experiment (NCEP-E). The BoB domain averaged <span class="hlt">sea</span> surface temperature (SST) simulated in the NCEP-E is consistently cooler than the satellite SST, with a root mean square error (RMSE) of 0.79 °C. Moreover, NCEP-E shows a limitation in simulating the observed seasonal cycle of the SST due to substantial underestimation of the pre-monsoon SST peak. These limitations are mostly due to the lower values of the NCEP net heat <span class="hlt">flux</span>. The seasonal and interannual variations of SST in the Trop<span class="hlt">Flux</span>-E are better comparable to the observations with correlations and skills more than 0.80 and 0.90 respectively. However, SST is overestimated during summer monsoon periods mainly due to higher net heat <span class="hlt">flux</span>. The superiority of Trop<span class="hlt">Flux</span> forcing over the NCEP reanalysis can also be seen when simulating the interannual variabilities of the magnitude and vertical extent of Wyrtki jets at two equatorial RAMA buoy locations. The jet is weaker in the NCEP-E relative to the Trop<span class="hlt">Flux</span>-E and observations. The simulated <span class="hlt">sea</span> surface height anomalies (SSHA) from both the experiments are able to capture the regions of positive and negative SSHA with respect to satellite-derived altimeter data with better performance in the Trop<span class="hlt">Flux</span>-E. The speed of the westward propagating Rossby wave along 18°N in the Trop<span class="hlt">Flux</span>-E is found to be about 4.7 cm/s, which is close to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMOS21A1356K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMOS21A1356K"><span>Methanethiol Concentrations and <span class="hlt">Sea-Air</span> <span class="hlt">Fluxes</span> in the Subarctic NE Pacific Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kiene, R. P.; Williams, T. E.; Esson, K.; Tortell, P. D.; Dacey, J. W. H.</p> <p>2017-12-01</p> <p>Exchange of volatile organic sulfur from the ocean to the atmosphere impacts the global sulfur cycle and the climate system and is thought to occur mainly via the gas dimethylsulfide (DMS). DMS is produced during degradation of the abundant phytoplankton osmolyte dimethylsulfoniopropionate (DMSP) but bacteria can also convert dissolved DMSP into the sulfur gas methanethiol (MeSH). MeSH has been difficult to measure in seawater because of its high chemical and biological reactivity and, thus, information on MeSH concentrations, distribution and <span class="hlt">sea-air</span> <span class="hlt">fluxes</span> is limited. We measured MeSH in the northeast subarctic Pacific Ocean in July 2016, along transects with strong phytoplankton abundance gradients. Water samples obtained with Niskin bottles were analyzed for MeSH by purge-and-trap gas chromatography. Depth profiles showed that MeSH concentrations were high near the surface and declined with depth. Surface waters (5 m depth) had an average MeSH concentration of 0.75 nM with concentrations reaching up to 3nM. MeSH concentrations were correlated (r = 0.47) with microbial turnover of dissolved DMSP which ranged up to 236 nM per day. MeSH was also correlated with total DMSP (r = 0.93) and dissolved DMS (r = 0.63), supporting the conclusion that DMSP was a major precursor of MeSH. Surface water MeSH:DMS concentration ratios averaged 0.19 and ranged up to 0.50 indicating that MeSH was a significant fraction of the volatile sulfur pool in surface waters. <span class="hlt">Sea-air</span> <span class="hlt">fluxes</span> of MeSH averaged 15% of the combined DMS+MeSH <span class="hlt">flux</span>, therefore MeSH contributed an important fraction of the sulfur emitted to the atmosphere from the subarctic NE Pacific Ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16271812','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16271812"><span>Atmospheric concentrations and <span class="hlt">air-sea</span> exchanges of nonylphenol, tertiary octylphenol and nonylphenol monoethoxylate in the North <span class="hlt">Sea</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Xie, Zhiyong; Lakaschus, Soenke; Ebinghaus, Ralf; Caba, Armando; Ruck, Wolfgang</p> <p>2006-07-01</p> <p>Concentrations of nonylphenol isomers (NP), tertiary octylphenol (t-OP) and nonylphenol monoethoxylate isomers (NP1EO) have been simultaneously determined in the <span class="hlt">sea</span> water and atmosphere of the North <span class="hlt">Sea</span>. A decreasing concentration profile appeared following the distance increasing from the coast to the central part of the North <span class="hlt">Sea</span>. <span class="hlt">Air-sea</span> exchanges of t-OP and NP were estimated using the two-film resistance model based upon relative <span class="hlt">air</span>-water concentrations and experimentally derived Henry's law constant. The average of <span class="hlt">air-sea</span> exchange <span class="hlt">fluxes</span> was -12+/-6 ng m(-<span class="hlt">2</span>)day(-1) for t-OP and -39+/-19 ng m(-<span class="hlt">2</span>)day(-1) for NP, which indicates a net deposition is occurring. These results suggest that the <span class="hlt">air-sea</span> vapour exchange is an important process that intervenes in the mass balance of alkylphenols in the North <span class="hlt">Sea</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006ThApC..84..117V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006ThApC..84..117V"><span>Temporal dynamics of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> and profiles over a Central European city</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vogt, R.; Christen, A.; Rotach, M. W.; Roth, M.; Satyanarayana, A. N. V.</p> <p>2006-02-01</p> <p>In Summer 2002 eddy covariance <span class="hlt">flux</span> measurements of <span class="hlt">CO</span><span class="hlt">2</span> were performed over a dense urban surface. The month-long measurements were carried out in the framework of the Basel Urban Boundary Layer Experiment (BUBBLE). Two Li7500 open path analysers were installed at z/z H = 1.0 and <span class="hlt">2.2</span> above a street canyon with z H the average building height of 14.6 m and z the height above street level. Additionally, profiles of <span class="hlt">CO</span><span class="hlt">2</span> concentration were sampled at 10 heights from street level up to <span class="hlt">2</span> z H . The minimum and maximum of the average diurnal course of <span class="hlt">CO</span><span class="hlt">2</span> concentration at <span class="hlt">2</span> z H were 362 and 423 ppmv in late afternoon and early morning, respectively. Daytime <span class="hlt">CO</span><span class="hlt">2</span> concentrations were not correlated to local sources, e.g. the minimum occurred together with the maximum in traffic load. During night-time <span class="hlt">CO</span><span class="hlt">2</span> is in general accumulated, except when inversion development is suppressed by frontal passages. <span class="hlt">CO</span><span class="hlt">2</span> concentrations were always decreasing with height and correspondingly, the <span class="hlt">fluxes</span> on average always directed upward. At z/z H = <span class="hlt">2.2</span> low values of about 3 µmol m-<span class="hlt">2</span> s-1 were measured during the second half of the night. During daytime average values reached up to 14 µmol m-<span class="hlt">2</span> s-1. The <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> are well correlated with the traffic load, with their maxima occurring together in late afternoon. Daytime minimum <span class="hlt">CO</span><span class="hlt">2</span> concentrations fell below regional background values. Besides vertical mixing and entrainment, it is suggested that this is also due to advection of rural <span class="hlt">air</span> with reduced <span class="hlt">CO</span><span class="hlt">2</span> concentration. Comparison with other urban observations shows a large range of differences among urban sites in terms of both <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> and concentrations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.8085Q','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.8085Q"><span>A practical <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> remote sensing technique</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Queisser, Manuel; Burton, Mike</p> <p>2017-04-01</p> <p>An accurate quantification of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> from both natural and anthropogenic sources is of great interest in various areas of the Earth, environmental and atmospheric sciences. As emitted excess <span class="hlt">CO</span><span class="hlt">2</span> quickly dilutes into the 400 ppm ambient <span class="hlt">CO</span><span class="hlt">2</span> concentration and degassing often occurs diffusively, measuring <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> is challenging. Therefore, <span class="hlt">fluxes</span> are usually derived from grids of in-situ measurements, which are labour intensive measurements. Other than a safe measurement distance, remote sensing offers quick, spatially integrated and thus a more thorough measurement of gas <span class="hlt">fluxes</span>. Active remote sensing combines these merits with operation independent of sunlight or clear sky conditions. Due to their weight and size, active remote sensing platforms for <span class="hlt">CO</span><span class="hlt">2</span>, such as LIDAR, cannot easily be applied in the field or transported overseas. Moreover, their complexity requires a rather lengthy setup procedure to be undertaken by skilled personal. To meet the need for a rugged, practical <span class="hlt">CO</span><span class="hlt">2</span> remote sensing technique to scan volcanic plumes, we have developed the <span class="hlt">CO</span><span class="hlt">2</span> LIDAR. It measures 1-D column densities of <span class="hlt">CO</span><span class="hlt">2</span> with sufficient sensitivity to reveal the contribution of magmatic <span class="hlt">CO</span><span class="hlt">2</span>. The <span class="hlt">CO</span><span class="hlt">2</span> LIDAR has been mounted inside a small aircraft and used to measure atmospheric column <span class="hlt">CO</span><span class="hlt">2</span> concentrations between the aircraft and the ground. It was further employed on the ground, measuring <span class="hlt">CO</span><span class="hlt">2</span> emissions from mud volcanism. During the measurement campaign the <span class="hlt">CO</span><span class="hlt">2</span> LIDAR demonstrated reliability, portability, quick set-up time (10 to 15 min) and platform independence. This new technique opens the possibility of rapid, comprehensive surveys of point source, open-vent <span class="hlt">CO</span><span class="hlt">2</span> emissions, as well as emissions from more diffuse sources such as lakes and fumarole fields. Currently, within the proof-of-concept ERC project CarbSens, a further reduction in size, weight and operational complexity is underway with the goal to commercialize the platform. Areas of potential applications include fugitive</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013ACP....1311073B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013ACP....1311073B"><span><span class="hlt">Air-sea</span> dimethylsulfide (DMS) gas transfer in the North Atlantic: evidence for limited interfacial gas exchange at high wind speed</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bell, T. G.; De Bruyn, W.; Miller, S. D.; Ward, B.; Christensen, K.; Saltzman, E. S.</p> <p>2013-11-01</p> <p>Shipboard measurements of eddy covariance dimethylsulfide (DMS) <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> and seawater concentration were carried out in the North Atlantic bloom region in June/July 2011. Gas transfer coefficients (k660) show a linear dependence on mean horizontal wind speed at wind speeds up to 11 m s-1. At higher wind speeds the relationship between k660 and wind speed weakens. At high winds, measured DMS <span class="hlt">fluxes</span> were lower than predicted based on the linear relationship between wind speed and interfacial stress extrapolated from low to intermediate wind speeds. In contrast, the transfer coefficient for sensible heat did not exhibit this effect. The apparent suppression of <span class="hlt">air-sea</span> gas <span class="hlt">flux</span> at higher wind speeds appears to be related to <span class="hlt">sea</span> state, as determined from shipboard wave measurements. These observations are consistent with the idea that long waves suppress near-surface water-side turbulence, and decrease interfacial gas transfer. This effect may be more easily observed for DMS than for less soluble gases, such as <span class="hlt">CO</span><span class="hlt">2</span>, because the <span class="hlt">air-sea</span> exchange of DMS is controlled by interfacial rather than bubble-mediated gas transfer under high wind speed conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRG..122.1615H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRG..122.1615H"><span>Effect of hydroperiod on <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> at the <span class="hlt">air</span>-water interface in the Mediterranean coastal wetlands of Doñana</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Huertas, I. Emma; Flecha, Susana; Figuerola, Jordi; Costas, Eduardo; Morris, Edward P.</p> <p>2017-07-01</p> <p>Wetlands are productive ecosystems that play an important role in the Earth's carbon cycle and thus global carbon budgets. Climate variability affects amount of material entering and the metabolic balance of wetlands, thereby modifying carbon dynamics. This study presents spatiotemporal changes in <span class="hlt">air</span>-water <span class="hlt">CO</span><span class="hlt">2</span> exchange in the vast wetlands of Doñana (Spain) in relation to different hydrological cycles. Water sources feeding Doñana, including groundwater and streams, ultimately depend on the fluctuating balance between annual precipitation and evapotranspiration. Hence, in order to examine the contribution of the rainfall pattern to the emission/capture of <span class="hlt">CO</span><span class="hlt">2</span> by a range of aquatic habitats in Doñana, we took monthly measurements during severely wet, dry, and normal hydrological years (2010-2013). During wet hydrological cycles, <span class="hlt">CO</span><span class="hlt">2</span> outgassing from flooded marshes markedly decreased in comparison to that observed during subsequent dry-normal cycles, with mean values of 25.84 ± 19 and 5.<span class="hlt">2</span> ± 8 mmol m-<span class="hlt">2</span> d-1, respectively. Under drier meteorological conditions, <span class="hlt">air</span>-water <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> also diminished in permanent floodplains and ponds, which even behaved as mild sinks for atmospheric <span class="hlt">CO</span><span class="hlt">2</span> during certain periods. Increased inputs of dissolved <span class="hlt">CO</span><span class="hlt">2</span> from the underground aquifer and the stream following periods of high rainfall are believed to be behind this pattern. Large lagoons with a managed water supply from an adjacent estuary took up atmospheric <span class="hlt">CO</span><span class="hlt">2</span> nearly permanently. Regional <span class="hlt">air</span>-water carbon transport was 15.<span class="hlt">2</span> GgC yr-1 under wet and 1.24 GgC yr-1 under dry meteorological conditions, well below the estimated net primary production for Doñana wetlands, indicating that the ecosystem acts as a large <span class="hlt">CO</span><span class="hlt">2</span> sink.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1364062','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1364062"><span>Radiocarbon in Ecosystem Respiration and Soil Pore-Space <span class="hlt">CO</span><span class="hlt">2</span> with Surface Gas <span class="hlt">Flux</span>, <span class="hlt">Air</span> Temperature, and Soil Temperature and Moisture, Barrow, Alaska, 2012-2014</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Lydia Vaughn; Margaret Torn; Rachel Porras</p> <p></p> <p>Dataset includes Delta14C measurements made from <span class="hlt">CO</span><span class="hlt">2</span> that was collected and purified in 2012-2014 from surface soil chambers, soil pore space, and background atmosphere. In addition to 14<span class="hlt">CO</span><span class="hlt">2</span> data, dataset includes <span class="hlt">co</span>-located measurements of <span class="hlt">CO</span><span class="hlt">2</span> and CH4 <span class="hlt">flux</span>, soil and <span class="hlt">air</span> temperature, and soil moisture. Measurements and field samples were taken from intensive study site 1 areas A, B, and C, and the site 0 and AB transects, from specified positions in high-centered, flat-centered, and low centered polygons.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRD..122.7216O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRD..122.7216O"><span><span class="hlt">Sea-to-air</span> <span class="hlt">flux</span> of dimethyl sulfide in the South and North Pacific Ocean as measured by proton transfer reaction-mass spectrometry coupled with the gradient <span class="hlt">flux</span> technique</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Omori, Yuko; Tanimoto, Hiroshi; Inomata, Satoshi; Ikeda, Kohei; Iwata, Toru; Kameyama, Sohiko; Uematsu, Mitsuo; Gamo, Toshitaka; Ogawa, Hiroshi; Furuya, Ken</p> <p>2017-07-01</p> <p>Exchange of dimethyl sulfide (DMS) between the surface ocean and the lower atmosphere was examined by using proton transfer reaction-mass spectrometry coupled with the gradient <span class="hlt">flux</span> (PTR-MS/GF) system. We deployed the PTR-MS/GF system and observed vertical gradients of atmospheric DMS just above the <span class="hlt">sea</span> surface in the subtropical and transitional South Pacific Ocean and the subarctic North Pacific Ocean. In total, we obtained 370 in situ profiles, and of these we used 46 data sets to calculate the <span class="hlt">sea-to-air</span> <span class="hlt">flux</span> of DMS. The DMS <span class="hlt">flux</span> determined was in the range from 1.9 to 31 μmol m-<span class="hlt">2</span> d-1 and increased with wind speed and biological activity, in reasonable accordance with previous observations in the open ocean. The gas transfer velocity of DMS derived from the PTR-MS/GF measurements was similar to either that of DMS determined by the eddy covariance technique or that of insoluble gases derived from the dual tracer experiments, depending on the observation sites located in different geographic regions. When atmospheric conditions were strongly stable during the daytime in the subtropical ocean, the PTR-MS/GF observations captured a daytime versus nighttime difference in DMS mixing ratios in the surface <span class="hlt">air</span> overlying the ocean surface. The difference was mainly due to the <span class="hlt">sea-to-air</span> DMS emissions and stable atmospheric conditions, thus affecting the gradient of DMS. This indicates that the DMS gradient is strongly controlled by diurnal variations in the vertical structure of the lower atmosphere above the ocean surface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016GeoRL..4311726A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GeoRL..4311726A"><span>A comparison of <span class="hlt">CO</span><span class="hlt">2</span> dynamics and <span class="hlt">air</span>-water <span class="hlt">fluxes</span> in a river-dominated estuary and a mangrove-dominated marine estuary</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Akhand, Anirban; Chanda, Abhra; Manna, Sudip; Das, Sourav; Hazra, Sugata; Roy, Rajdeep; Choudhury, S. B.; Rao, K. H.; Dadhwal, V. K.; Chakraborty, Kunal; Mostofa, K. M. G.; Tokoro, T.; Kuwae, Tomohiro; Wanninkhof, Rik</p> <p>2016-11-01</p> <p>The fugacity of <span class="hlt">CO</span><span class="hlt">2</span> (f<span class="hlt">CO</span><span class="hlt">2</span> (water)) and <span class="hlt">air</span>-water <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> were compared between a river-dominated anthropogenically disturbed open estuary, the Hugli, and a comparatively pristine mangrove-dominated semiclosed marine estuary, the Matla, on the east coast of India. Annual mean salinity of the Hugli Estuary (≈7.1) was much less compared to the Matla Estuary (≈20.0). All the stations of the Hugli Estuary were highly supersaturated with <span class="hlt">CO</span><span class="hlt">2</span> (annual mean 2200 µatm), whereas the Matla was marginally oversaturated (annual mean 530 µatm). During the postmonsoon season, the outer station of the Matla Estuary was under saturated with respect to <span class="hlt">CO</span><span class="hlt">2</span> and acted as a sink. The annual mean <span class="hlt">CO</span><span class="hlt">2</span> emission from the Hugli Estuary (32.4 mol C m-<span class="hlt">2</span> yr-1) was 14 times higher than the Matla Estuary (<span class="hlt">2</span>.3 mol C m-<span class="hlt">2</span> yr-1). <span class="hlt">CO</span><span class="hlt">2</span> efflux rate from the Hugli Estuary has increased drastically in the last decade, which is attributed to increased runoff from the river-dominated estuary.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009BGD.....6.3481Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009BGD.....6.3481Z"><span>Conditional <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> analysis of a managed grassland with the aid of stable isotopes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zeeman, M. J.; Tuzson, B.; Emmenegger, L.; Knohl, A.; Buchmann, N.; Eugster, W.</p> <p>2009-04-01</p> <p>Short statured managed ecosystems, such as agricultural grasslands, exhibit high temporal changes in carbon dioxide assimilation and respiration <span class="hlt">fluxes</span> for which measurements of the net <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span>, e.g. by using the eddy covariance (EC) method, give only limited insight. We have therefore adopted a recently proposed concept for conditional EC <span class="hlt">flux</span> analysis of forest to grasslands, in order to identify and quantify daytime sub-canopy respiration <span class="hlt">fluxes</span>. To validate the concept, high frequency (≈5 Hz) stable carbon isotope analyis of <span class="hlt">CO</span><span class="hlt">2</span> was used. We made eddy covariance measurements of <span class="hlt">CO</span><span class="hlt">2</span> and its isotopologues during four days in August 2007, using a novel quantum cascade laser absorption spectrometer, capable of high time resolution stable isotope analysis. The effects of a grass cut during the measurement period could be detected and resulted in a sub-canopy source conditional <span class="hlt">flux</span> classification, for which the isotope composition of the <span class="hlt">CO</span><span class="hlt">2</span> could be confirmed to be of a respiration source. However, the conditional <span class="hlt">flux</span> method did not work for an undisturbed grassland canopy. We attribute this to the <span class="hlt">flux</span> measurement height that was chosen well above the roughness sublayer, where the natural isotopic tracer (δ13C) of respiration was too well mixed with background <span class="hlt">air</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150001279','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150001279"><span>Quantifying the Observability of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Flux</span> Uncertainty in Atmospheric <span class="hlt">CO</span><span class="hlt">2</span> Records Using Products from Nasa's Carbon Monitoring <span class="hlt">Flux</span> Pilot Project</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ott, Lesley; Pawson, Steven; Collatz, Jim; Watson, Gregg; Menemenlis, Dimitris; Brix, Holger; Rousseaux, Cecile; Bowman, Kevin; Bowman, Kevin; Liu, Junjie; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20150001279'); toggleEditAbsImage('author_20150001279_show'); toggleEditAbsImage('author_20150001279_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20150001279_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20150001279_hide"></p> <p>2014-01-01</p> <p>NASAs Carbon Monitoring System (CMS) <span class="hlt">Flux</span> Pilot Project (FPP) was designed to better understand contemporary carbon <span class="hlt">fluxes</span> by bringing together state-of-the art models with remote sensing datasets. Here we report on simulations using NASAs Goddard Earth Observing System Model, version 5 (GEOS-5) which was used to evaluate the consistency of two different sets of observationally constrained land and ocean <span class="hlt">fluxes</span> with atmospheric <span class="hlt">CO</span><span class="hlt">2</span> records. Despite the strong data constraint, the average difference in annual terrestrial biosphere <span class="hlt">flux</span> between the two land (NASA Ames CASA and CASA-GFED) models is 1.7 Pg C for 2009-2010. Ocean models (NOBM and ECCO<span class="hlt">2</span>-Darwin) differ by 35 in their global estimates of carbon <span class="hlt">flux</span> with particularly strong disagreement in high latitudes. Based upon combinations of terrestrial and ocean <span class="hlt">fluxes</span>, GEOS-5 reasonably simulated the seasonal cycle observed at northern hemisphere surface sites and by the Greenhouse gases Observing SATellite (GOSAT) while the model struggled to simulate the seasonal cycle at southern hemisphere surface locations. Though GEOS-5 was able to reasonably reproduce the patterns of XCO<span class="hlt">2</span> observed by GOSAT, it struggled to reproduce these aspects of <span class="hlt">AIRS</span> observations. Despite large differences between land and ocean <span class="hlt">flux</span> estimates, resulting differences in atmospheric mixing ratio were small, typically less than 5 ppmv at the surface and 3 ppmv in the XCO<span class="hlt">2</span> column. A statistical analysis based on the variability of observations shows that <span class="hlt">flux</span> differences of these magnitudes are difficult to distinguish from natural variability, regardless of measurement platform.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014ACP....1413281T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014ACP....1413281T"><span>A joint data assimilation system (Tan-Tracker) to simultaneously estimate surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> and 3-D atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentrations from observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tian, X.; Xie, Z.; Liu, Y.; Cai, Z.; Fu, Y.; Zhang, H.; Feng, L.</p> <p>2014-12-01</p> <p> precision for both <span class="hlt">CO</span><span class="hlt">2</span> concentrations and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>, mainly due to the simultaneous estimation of <span class="hlt">CO</span><span class="hlt">2</span> concentrations and CFs in our Tan-Tracker data assimilation system. A experiment for assimilating the real dry-<span class="hlt">air</span> column <span class="hlt">CO</span><span class="hlt">2</span> retrievals (XCO<span class="hlt">2</span>) from the Japanese Greenhouse Gases Observation Satellite (GOSAT) further demonstrates its potential wide applications.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.A43C0283L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.A43C0283L"><span><span class="hlt">Air-sea</span> Exchange of Polycyclic Aromatic Hydrocarbons (PAHs), Polychlorinated Biphenyls (PCBs), Organochlorine Pesticides (OCPs) and Polybrominated Diphenyl Ethers (PBDEs) in the Mediterranean <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lammel, G. P.; Heil, A.; Kukucka, P.; Meixner, F. X.; Mulder, M. D.; Prybilova, P.; Prokes, R.; Rusina, T. S.; Song, G. Z.; Vrana, B.</p> <p>2015-12-01</p> <p>The marine atmospheric environment is a receptor for persistent organic pollutants (POPs) which are advected from sources on land, primary, such as biomass burning by-products (PAHs, dioxins), and secondary, such as volatilization from contaminated soils (PCBs, pesticides). Primary sources do not exist in the marine environment, except for PAHs (ship engines) but following previous atmospheric deposition, the <span class="hlt">sea</span> surface may turn to a secondary source by reversal of diffusive <span class="hlt">air-sea</span> mass exchange. No monitoring is in place. We studied the vertical <span class="hlt">fluxes</span> of a wide range of primary and secondary emitted POPs based on measurements in <span class="hlt">air</span> and surface seawater at a remote coastal site in the eastern Mediterranean (2012). To this end, silicon rubbers were used as passive water samplers, vertical concentration gradients were determined in <span class="hlt">air</span> and <span class="hlt">fluxes</span> were quantified based on Eddy covariance. Diffusive <span class="hlt">air-sea</span> exchange <span class="hlt">fluxes</span> of hexachlorocyclohexanes (HCHs) and semivolatile PAHs were found close to phase equilibrium, except one PAH, retene, a wood burning tracer, was found seasonally net-volatilisational. Some PCBs, p,p'-DDE, penta- and hexachlorobenzene (PeCB, HCB) were mostly net-depositional, while PBDEs were net-volatilizational. <span class="hlt">Fluxes</span> determined at a a remote coastal site ranged -33 - +<span class="hlt">2</span>.4 µg m-<span class="hlt">2</span> d-1 for PAHs and -4.0 - +0.3 µg m-<span class="hlt">2</span> d-1for halogenated compounds (< 0 means net-deposition, > 0 means net-volatilization). It is concluded that nowadays in open <span class="hlt">seas</span> more pollutants are undergoing reversal of the direction of <span class="hlt">air-sea</span> exchange. Recgional fire activity records in combination with box model simulations suggest that deposition of retene during summer is followed by a reversal of <span class="hlt">air-sea</span> exchange. The seawater surface as secondary source of pollution should be assessed based on <span class="hlt">flux</span> measurements across seasons and over longer time periods.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li class="active"><span>8</span></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_8 --> <div id="page_9" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li class="active"><span>9</span></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="161"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28645049','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28645049"><span>Gaseous elemental mercury in the marine boundary layer and <span class="hlt">air-sea</span> <span class="hlt">flux</span> in the Southern Ocean in austral summer.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Jiancheng; Xie, Zhouqing; Wang, Feiyue; Kang, Hui</p> <p>2017-12-15</p> <p>Gaseous elemental mercury (GEM) in the marine boundary layer (MBL), and dissolved gaseous mercury (DGM) in surface seawater of the Southern Ocean were measured in the austral summer from December 13, 2014 to February 1, 2015. GEM concentrations in the MBL ranged from 0.4 to 1.9ngm -3 (mean±standard deviation: 0.9±0.<span class="hlt">2</span>ngm -3 ), whereas DGM concentrations in surface seawater ranged from 7.0 to 75.9pgL -1 (mean±standard deviation: 23.7±13.<span class="hlt">2</span>pgL -1 ). The occasionally observed low GEM in the MBL suggested either the occurrence of atmospheric mercury depletion in summer, or the transport of GEM-depleted <span class="hlt">air</span> from the Antarctic Plateau. Elevated GEM concentrations in the MBL and DGM concentrations in surface seawater were consistently observed in the ice-covered region of the Ross <span class="hlt">Sea</span> implying the influence of the <span class="hlt">sea</span> ice environment. Diminishing <span class="hlt">sea</span> ice could cause more mercury evasion from the ocean to the <span class="hlt">air</span>. Using the thin film gas exchange model, the <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> of gaseous mercury in non-ice-covered area during the study period were estimated to range from 0.0 to 6.5ngm -<span class="hlt">2</span> h -1 with a mean value of 1.5±1.8ngm -<span class="hlt">2</span> h -1 , revealing GEM (re-)emission from the East Southern Ocean in summer. Copyright © 2017 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018BGeo...15.1011M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018BGeo...15.1011M"><span>Inorganic carbon <span class="hlt">fluxes</span> on the Mackenzie Shelf of the Beaufort <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mol, Jacoba; Thomas, Helmuth; Myers, Paul G.; Hu, Xianmin; Mucci, Alfonso</p> <p>2018-02-01</p> <p>The Mackenzie Shelf in the southeastern Beaufort <span class="hlt">Sea</span> is a region that has experienced large changes in the past several decades as warming, <span class="hlt">sea</span>-ice loss, and increased river discharge have altered carbon cycling. Upwelling and downwelling events are common on the shelf, caused by strong, fluctuating along-shore winds, resulting in cross-shelf Ekman transport, and an alternating estuarine and anti-estuarine circulation. Downwelling carries dissolved inorganic carbon (DIC) and other remineralization products off the shelf and into the deep basin for possible long-term storage in the world's oceans. Upwelling carries DIC and nutrient-rich waters from the Pacific-origin upper halocline layer (UHL) onto the shelf. Profiles of DIC and total alkalinity (TA) taken in August and September of 2014 are used to investigate the cycling of carbon on the Mackenzie Shelf. The along-shore transport of water and the cross-shelf transport of DIC are quantified using velocity field output from a simulation of the Arctic and Northern Hemisphere Atlantic (ANHA4) configuration of the Nucleus of European Modelling of the Ocean (NEMO) framework. A strong upwelling event prior to sampling on the Mackenzie Shelf took place, bringing <span class="hlt">CO</span><span class="hlt">2</span>-rich (elevated p<span class="hlt">CO</span><span class="hlt">2</span>) water from the UHL onto the shelf bottom. The maximum on-shelf DIC <span class="hlt">flux</span> was estimated at 16.9×103 mol C d-1 m-<span class="hlt">2</span> during the event. The maximum on-shelf transport of DIC through the upwelling event was found to be 65±15×10-3 Tg C d-1. TA and the oxygen isotope ratio of water (δ18O-H<span class="hlt">2</span>O) are used to examine water-mass distributions in the study area and to investigate the influence of Pacific Water, Mackenzie River freshwater, and <span class="hlt">sea</span>-ice melt on carbon dynamics and <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> of carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) in the surface mixed layer. Understanding carbon transfer in this seasonally dynamic environment is key to quantify the importance of Arctic shelf regions to the global carbon cycle and provide a basis for understanding how it will</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19890052278&hterms=heat+exchange&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dheat%2Bexchange','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19890052278&hterms=heat+exchange&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dheat%2Bexchange"><span>A study of oceanic surface heat <span class="hlt">fluxes</span> in the Greenland, Norwegian, and Barents <span class="hlt">Seas</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hakkinen, Sirpa; Cavalieri, Donald J.</p> <p>1989-01-01</p> <p>This study examines oceanic surface heat <span class="hlt">fluxes</span> in the Norwegian, Greenland, and Barents <span class="hlt">seas</span> using the gridded Navy Fleet Numerical Oceanography Central surface analysis and the First GARP Global Experiment (FGGE) IIc cloudiness data bases. Monthly and annual means of net and turbulent heat <span class="hlt">fluxes</span> are computed for the FGGE year 1979. The FGGE IIb data base consisting of individual observations provides particularly good data coverage in this region for a comparison with the gridded Navy winds and <span class="hlt">air</span> temperatures. The standard errors of estimate between the Navy and FGGE IIb winds and <span class="hlt">air</span> temperatures are 3.6 m/s and <span class="hlt">2</span>.5 C, respectively. The computations for the latent and sensible heat <span class="hlt">fluxes</span> are based on bulk formulas with the same constant heat exchange coefficient of 0.0015. The results show extremely strong wintertime heat <span class="hlt">fluxes</span> in the northern Greenland <span class="hlt">Sea</span> and especially in the Barents <span class="hlt">Sea</span> in contrast to previous studies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007JGRD..11210301G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007JGRD..11210301G"><span>Retrieval of average <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> by combining in situ <span class="hlt">CO</span><span class="hlt">2</span> measurements and backscatter lidar information</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gibert, Fabien; Schmidt, Martina; Cuesta, Juan; Ciais, Philippe; Ramonet, Michel; Xueref, IrèNe; Larmanou, Eric; Flamant, Pierre Henri</p> <p>2007-05-01</p> <p>The present paper deals with a boundary layer budgeting method which makes use of observations from various in situ and remote sensing instruments to infer regional average net ecosystem exchange (NEE) of <span class="hlt">CO</span><span class="hlt">2</span>. Measurements of <span class="hlt">CO</span><span class="hlt">2</span> within and above the atmospheric boundary layer (ABL) by in situ sensors, in conjunction with a precise knowledge of the change in ABL height by lidar and radiosoundings, enable to infer diurnal and seasonal NEE variations. Near-ground in situ <span class="hlt">CO</span> measurements are used to discriminate natural and anthropogenic contributions of <span class="hlt">CO</span><span class="hlt">2</span> diurnal variations in the ABL. The method yields mean NEE that amounts to 5 μmol m-<span class="hlt">2</span> s-1 during the night and -20 μmol m-<span class="hlt">2</span> s-1 in the middle of the day between May and July. A good agreement is found with the expected NEE accounting for a mixed wheat field and forest area during winter season, representative of the mesoscale ecosystems in the Paris area according to the trajectory of an <span class="hlt">air</span> column crossing the landscape. Daytime NEE is seen to follow the vegetation growth and the change in the ratio diffuse/direct radiation. The <span class="hlt">CO</span><span class="hlt">2</span> vertical mixing <span class="hlt">flux</span> during the rise of the atmospheric boundary layer is also estimated and seems to be the main cause of the large decrease of <span class="hlt">CO</span><span class="hlt">2</span> mixing ratio in the morning. The outcomes on <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> estimate are compared to eddy-covariance measurements on a barley field. The importance of various sources of error and uncertainty on the retrieval is discussed. These errors are estimated to be less than 15%; the main error resulted from anthropogenic emissions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3594177','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3594177"><span>Responses of Soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Fluxes</span> to Short-Term Experimental Warming in Alpine Steppe Ecosystem, Northern Tibet</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Lu, Xuyang; Fan, Jihui; Yan, Yan; Wang, Xiaodan</p> <p>2013-01-01</p> <p>Soil carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) emission is one of the largest <span class="hlt">fluxes</span> in the global carbon cycle. Therefore small changes in the size of this <span class="hlt">flux</span> can have a large effect on atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentrations and potentially constitute a powerful positive feedback to the climate system. Soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in the alpine steppe ecosystem of Northern Tibet and their responses to short-term experimental warming were investigated during the growing season in 2011. The results showed that the total soil <span class="hlt">CO</span><span class="hlt">2</span> emission <span class="hlt">fluxes</span> during the entire growing season were 55.82 and 104.31 g C m-<span class="hlt">2</span> for the control and warming plots, respectively. Thus, the soil <span class="hlt">CO</span><span class="hlt">2</span> emission <span class="hlt">fluxes</span> increased 86.86% with the <span class="hlt">air</span> temperature increasing 3.74°C. Moreover, the temperature sensitivity coefficient (Q 10) of the control and warming plots were <span class="hlt">2</span>.10 and 1.41, respectively. The soil temperature and soil moisture could partially explain the temporal variations of soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. The relationship between the temporal variation of soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> and the soil temperature can be described by exponential equation. These results suggest that warming significantly promoted soil <span class="hlt">CO</span><span class="hlt">2</span> emission in the alpine steppe ecosystem of Northern Tibet and indicate that this alpine ecosystem is very vulnerable to climate change. In addition, soil temperature and soil moisture are the key factors that controls soil organic matter decomposition and soil <span class="hlt">CO</span><span class="hlt">2</span> emission, but temperature sensitivity significantly decreases due to the rise in temperature. PMID:23536854</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23536854','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23536854"><span>Responses of soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> to short-term experimental warming in alpine steppe ecosystem, Northern Tibet.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lu, Xuyang; Fan, Jihui; Yan, Yan; Wang, Xiaodan</p> <p>2013-01-01</p> <p>Soil carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) emission is one of the largest <span class="hlt">fluxes</span> in the global carbon cycle. Therefore small changes in the size of this <span class="hlt">flux</span> can have a large effect on atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentrations and potentially constitute a powerful positive feedback to the climate system. Soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in the alpine steppe ecosystem of Northern Tibet and their responses to short-term experimental warming were investigated during the growing season in 2011. The results showed that the total soil <span class="hlt">CO</span><span class="hlt">2</span> emission <span class="hlt">fluxes</span> during the entire growing season were 55.82 and 104.31 g C m(-<span class="hlt">2</span>) for the control and warming plots, respectively. Thus, the soil <span class="hlt">CO</span><span class="hlt">2</span> emission <span class="hlt">fluxes</span> increased 86.86% with the <span class="hlt">air</span> temperature increasing 3.74°C. Moreover, the temperature sensitivity coefficient (Q 10) of the control and warming plots were <span class="hlt">2</span>.10 and 1.41, respectively. The soil temperature and soil moisture could partially explain the temporal variations of soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. The relationship between the temporal variation of soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> and the soil temperature can be described by exponential equation. These results suggest that warming significantly promoted soil <span class="hlt">CO</span><span class="hlt">2</span> emission in the alpine steppe ecosystem of Northern Tibet and indicate that this alpine ecosystem is very vulnerable to climate change. In addition, soil temperature and soil moisture are the key factors that controls soil organic matter decomposition and soil <span class="hlt">CO</span><span class="hlt">2</span> emission, but temperature sensitivity significantly decreases due to the rise in temperature.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017BGeo...14.5727K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017BGeo...14.5727K"><span>Low p<span class="hlt">CO</span><span class="hlt">2</span> under <span class="hlt">sea</span>-ice melt in the Canada Basin of the western Arctic Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kosugi, Naohiro; Sasano, Daisuke; Ishii, Masao; Nishino, Shigeto; Uchida, Hiroshi; Yoshikawa-Inoue, Hisayuki</p> <p>2017-12-01</p> <p>In September 2013, we observed an expanse of surface water with low <span class="hlt">CO</span><span class="hlt">2</span> partial pressure (p<span class="hlt">CO</span><span class="hlt">2</span><span class="hlt">sea</span>) (< 200 µatm) in the Chukchi <span class="hlt">Sea</span> of the western Arctic Ocean. The large undersaturation of <span class="hlt">CO</span><span class="hlt">2</span> in this region was the result of massive primary production after the <span class="hlt">sea</span>-ice retreat in June and July. In the surface of the Canada Basin, salinity was low (< 27) and p<span class="hlt">CO</span><span class="hlt">2</span><span class="hlt">sea</span> was closer to the <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> equilibrium (˜ 360 µatm). From the relationships between salinity and total alkalinity, we confirmed that the low salinity in the Canada Basin was due to the larger fraction of meltwater input (˜ 0.16) rather than the riverine discharge (˜ 0.1). Such an increase in p<span class="hlt">CO</span><span class="hlt">2</span><span class="hlt">sea</span> was not so clear in the coastal region near Point Barrow, where the fraction of riverine discharge was larger than that of <span class="hlt">sea</span>-ice melt. We also identified low p<span class="hlt">CO</span><span class="hlt">2</span><span class="hlt">sea</span> (< 250 µatm) in the depth of 30-50 m under the halocline of the Canada Basin. This subsurface low p<span class="hlt">CO</span><span class="hlt">2</span><span class="hlt">sea</span> was attributed to the advection of Pacific-origin water, in which dissolved inorganic carbon is relatively low, through the Chukchi <span class="hlt">Sea</span> where net primary production is high. Oxygen supersaturation (> 20 µmol kg-1) in the subsurface low p<span class="hlt">CO</span><span class="hlt">2</span><span class="hlt">sea</span> layer in the Canada Basin indicated significant net primary production undersea and/or in preformed condition. If these low p<span class="hlt">CO</span><span class="hlt">2</span><span class="hlt">sea</span> layers surface by wind mixing, they will act as additional <span class="hlt">CO</span><span class="hlt">2</span> sinks; however, this is unlikely because intensification of stratification by <span class="hlt">sea</span>-ice melt inhibits mixing across the halocline.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS54B..01D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS54B..01D"><span>Carbon Cycle in South China <span class="hlt">Sea</span>: <span class="hlt">Flux</span>, Controls and Global Implications</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dai, M.; Cao, Z.; Yang, W.; Guo, X.; Yin, Z.; Gan, J.</p> <p>2016-12-01</p> <p>The contemporary coastal ocean is generally seen as a significant <span class="hlt">CO</span><span class="hlt">2</span> sink of 0.<span class="hlt">2</span>-0.4 Pg C/yr at the global scale. However, mechanistic understanding of the coastal ocean carbon cycle remains limited, leading to the unanswered question of why some coastal systems are sources while others are sinks of atmospheric <span class="hlt">CO</span><span class="hlt">2</span>. As the largest marginal <span class="hlt">sea</span> of Northern Pacific, the South China <span class="hlt">Sea</span> (SCS) is a mini-ocean with wide shelves in both its southern and northern parts. Its northern shelf, which receives significant land inputs from the Pearl River, a world major river, can be categorized as a River-Dominated Margin (RioMar) during peak discharges, and is characterized as a <span class="hlt">CO</span><span class="hlt">2</span> sink to the atmosphere. The SCS basin is identified as an Ocean-Dominated Margin (OceMar) and a <span class="hlt">CO</span><span class="hlt">2</span> source. OceMar is characterized by exchange with the open ocean via a two-dimensional (at least) process, i.e., the horizontal intrusion of open ocean water and subsequent vertical mixing and upwelling. Depending on the different ratios of dissolved inorganic carbon (DIC) and nutrients from the source waters into the continental margins, the relative consumption or removal bwtween DIC and nutrients, when being transported into the euphotic zones where biogeochemical processes take over, determines the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. Thus, excess DIC relative to nutrients existing in the upper layer will lead to <span class="hlt">CO</span><span class="hlt">2</span> degassing. The <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in both RioMars and OceMars can be quantified using a semi-analytical diagnostic approach by coupling the physical dynamics and biogeochemical processes. We extended our mechanistic studies in the SCS to other OceMars including the Caribbean <span class="hlt">Sea</span>, the Arabian <span class="hlt">Sea</span>, and the upwelling system off the Oregon-California coast, and RioMars including the East China <span class="hlt">Sea</span> and Amazon River plume to demonstrate the global implications of our SCS carbon studies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GBioC..31..591W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GBioC..31..591W"><span>Calculating surface ocean p<span class="hlt">CO</span><span class="hlt">2</span> from biogeochemical Argo floats equipped with pH: An uncertainty analysis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Williams, N. L.; Juranek, L. W.; Feely, R. A.; Johnson, K. S.; Sarmiento, J. L.; Talley, L. D.; Dickson, A. G.; Gray, A. R.; Wanninkhof, R.; Russell, J. L.; Riser, S. C.; Takeshita, Y.</p> <p>2017-03-01</p> <p>More than 74 biogeochemical profiling floats that measure water column pH, oxygen, nitrate, fluorescence, and backscattering at 10 day intervals have been deployed throughout the Southern Ocean. Calculating the surface ocean partial pressure of carbon dioxide (p<span class="hlt">CO</span><span class="hlt">2</span>sw) from float pH has uncertainty contributions from the pH sensor, the alkalinity estimate, and carbonate system equilibrium constants, resulting in a relative standard uncertainty in p<span class="hlt">CO</span><span class="hlt">2</span>sw of <span class="hlt">2</span>.7% (or 11 µatm at p<span class="hlt">CO</span><span class="hlt">2</span>sw of 400 µatm). The calculated p<span class="hlt">CO</span><span class="hlt">2</span>sw from several floats spanning a range of oceanographic regimes are compared to existing climatologies. In some locations, such as the subantarctic zone, the float data closely match the climatologies, but in the polar Antarctic zone significantly higher p<span class="hlt">CO</span><span class="hlt">2</span>sw are calculated in the wintertime implying a greater <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> efflux estimate. Our results based on four representative floats suggest that despite their uncertainty relative to direct measurements, the float data can be used to improve estimates for <span class="hlt">air-sea</span> carbon <span class="hlt">flux</span>, as well as to increase knowledge of spatial, seasonal, and interannual variability in this <span class="hlt">flux</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007BoLMe.124..161Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007BoLMe.124..161Y"><span>Influence of leaf water potential on diurnal changes in <span class="hlt">CO</span><span class="hlt">2</span> and water vapour <span class="hlt">fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yu, Qiang; Xu, Shouhua; Wang, Jing; Lee, Xuhui</p> <p>2007-08-01</p> <p>Mass and energy <span class="hlt">fluxes</span> between the atmosphere and vegetation are driven by meteorological variables, and controlled by plant water status, which may change more markedly diurnally than soil water. We tested the hypothesis that integration of dynamic changes in leaf water potential may improve the simulation of <span class="hlt">CO</span><span class="hlt">2</span> and water <span class="hlt">fluxes</span> over a wheat canopy. Simulation of leaf water potential was integrated into a comprehensive model (the ChinaAgrosys) of heat, water and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> and crop growth. Photosynthesis from individual leaves was integrated to the canopy by taking into consideration the attenuation of radiation when penetrating the canopy. Transpiration was calculated with the Shuttleworth-Wallace model in which canopy resistance was taken as a link between energy balance and physiological regulation. A revised version of the Ball-Woodrow-Berry stomatal model was applied to produce a new canopy resistance model, which was validated against measured <span class="hlt">CO</span><span class="hlt">2</span> and water vapour <span class="hlt">fluxes</span> over winter wheat fields in Yucheng (36°57' N, 116°36' E, 28 m above <span class="hlt">sea</span> level) in the North China Plain during 1997, 2001 and 2004. Leaf water potential played an important role in causing stomatal conductance to fall at midday, which caused diurnal changes in photosynthesis and transpiration. Changes in soil water potential were less important. Inclusion of the dynamics of leaf water potential can improve the precision of the simulation of <span class="hlt">CO</span><span class="hlt">2</span> and water vapour <span class="hlt">fluxes</span>, especially in the afternoon under water stress conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20020015705','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20020015705"><span>Modeling Biogeochemical-Physical Interactions and Carbon <span class="hlt">Flux</span> in the Sargasso <span class="hlt">Sea</span> (Bermuda Atlantic Time-series Study site)</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Signorini, Sergio R.; McClain, Charles R.; Christian, James R.</p> <p>2001-01-01</p> <p>An ecosystem-carbon cycle model is used to analyze the biogeochemical-physical interactions and carbon <span class="hlt">fluxes</span> in the Bermuda Atlantic Time-series Study (BATS) site for the period of 1992-1998. The model results compare well with observations (most variables are within 8% of observed values). The <span class="hlt">sea-air</span> <span class="hlt">flux</span> ranges from -0.32 to -0.50 mol C/sq m/yr, depending upon the gas transfer algorithm used. This estimate is within the range (-0.22 to -0.83 mol C/sq m/yr) of previously reported values which indicates that the BATS region is a weak sink of atmospheric <span class="hlt">CO</span><span class="hlt">2</span>. The overall carbon balance consists of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> uptake of 0.3 Mol C/sq m/yr, upward dissolved inorganic carbon (DIC) bottom <span class="hlt">flux</span> of 1.1 Mol C/sq m/yr, and carbon export of 1.4 mol C/sq m/yr via sedimentation. Upper ocean DIC levels increased between 1992 and 1996 at a rate of approximately 1.<span class="hlt">2</span> (micro)mol/kg/yr, consistent with observations. However, this trend was reversed during 1997-1998 to -<span class="hlt">2</span>.7 (micro)mol/kg/yr in response to hydrographic changes imposed by the El Nino-La Nina transition, which were manifested in the Sargasso <span class="hlt">Sea</span> by the warmest SST and lowest surface salinity of the period (1992-1998).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012TCD.....6.1015R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012TCD.....6.1015R"><span>Ikaite crystals in melting <span class="hlt">sea</span> ice - implications for p<span class="hlt">CO</span><span class="hlt">2</span> and pH levels in Arctic surface waters</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rysgaard, S.; Glud, R. N.; Lennert, K.; Cooper, M.; Halden, N.; Leakey, R. J. G.; Hawthorne, F. C.; Barber, D.</p> <p>2012-03-01</p> <p>A major issue of Arctic marine science is to understand whether the Arctic Ocean is, or will be, a source or sink for <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange. This has been complicated by the recent discoveries of ikaite (Ca<span class="hlt">CO</span>3·6H<span class="hlt">2</span>O) in Arctic and Antarctic <span class="hlt">sea</span> ice, which indicate that multiple chemical transformations occur in <span class="hlt">sea</span> ice with a possible effect on <span class="hlt">CO</span><span class="hlt">2</span> and pH conditions in surface waters. Here we report on biogeochemical conditions, microscopic examinations and x-ray diffraction analysis of single crystals from an actively melting 1.7 km<span class="hlt">2</span> (0.5-1 m thick) drifting ice floe in the Fram Strait during summer. Our findings show that ikaite crystals are present throughout the <span class="hlt">sea</span> ice but with larger crystals appearing in the upper ice layers. Ikaite crystals placed at elevated temperatures gradually disintegrated into smaller crystallites and dissolved. During our field campaign in late June, melt reduced the ice flow thickness by ca. 0.<span class="hlt">2</span> m per week and resulted in an estimated 1.6 ppm decrease of p<span class="hlt">CO</span><span class="hlt">2</span> in the ocean surface mixed layer. This corresponds to an <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> uptake of 11 mmol m-<span class="hlt">2</span> <span class="hlt">sea</span> ice d-1 or to 3.5 ton km-<span class="hlt">2</span> ice floe week-1.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5504290','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5504290"><span><span class="hlt">Sea</span> level fall during glaciation stabilized atmospheric <span class="hlt">CO</span><span class="hlt">2</span> by enhanced volcanic degassing</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Hasenclever, Jörg; Knorr, Gregor; Rüpke, Lars H.; Köhler, Peter; Morgan, Jason; Garofalo, Kristin; Barker, Stephen; Lohmann, Gerrit; Hall, Ian R.</p> <p>2017-01-01</p> <p>Paleo-climate records and geodynamic modelling indicate the existence of complex interactions between glacial <span class="hlt">sea</span> level changes, volcanic degassing and atmospheric <span class="hlt">CO</span><span class="hlt">2</span>, which may have modulated the climate system’s descent into the last ice age. Between ∼85 and 70 kyr ago, during an interval of decreasing axial tilt, the orbital component in global temperature records gradually declined, while atmospheric <span class="hlt">CO</span><span class="hlt">2</span>, instead of continuing its long-term correlation with Antarctic temperature, remained relatively stable. Here, based on novel global geodynamic models and the joint interpretation of paleo-proxy data as well as biogeochemical simulations, we show that a <span class="hlt">sea</span> level fall in this interval caused enhanced pressure-release melting in the uppermost mantle, which may have induced a surge in magma and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> from mid-ocean ridges and oceanic hotspot volcanoes. Our results reveal a hitherto unrecognized negative feedback between glaciation and atmospheric <span class="hlt">CO</span><span class="hlt">2</span> predominantly controlled by marine volcanism on multi-millennial timescales of ∼5,000–15,000 years. PMID:28681844</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20080023465','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20080023465"><span>A Preliminary Study of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Flux</span> Measurements by Lidar</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gibert, Fabien; Koch, Grady J.; Beyon, Jeffrey Y.; Hilton, T.; Davis, Kenneth J.; Andrews, Arlyn; Ismail, Syed; Singh, Upendra N.</p> <p>2008-01-01</p> <p>A mechanistic understanding of the global carbon cycle requires quantification of terrestrial ecosystem <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> at regional scales. In this paper, we analyze the potential of a Doppler DIAL system to make <span class="hlt">flux</span> measurements of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> using the eddy-covariance and boundary layer budget methods and present results from a ground based experiment. The goal of this study is to put <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> point measurements in a mesoscale context. In June 2007, a field experiment combining a <span class="hlt">2</span>-m Doppler Heterodyne Differential Absorption Lidar (HDIAL) and in-situ sensors of a 447-m tall tower (WLEF) took place in Wisconsin. The HDIAL measures simultaneously: 1) <span class="hlt">CO</span><span class="hlt">2</span> mixing ratio, <span class="hlt">2</span>) atmosphere structure via aerosol backscatter and 3) radial velocity. We demonstrate how to synthesize these data into regional <span class="hlt">flux</span> estimates. Lidar-inferred <span class="hlt">fluxes</span> are compared with eddy-covariance <span class="hlt">fluxes</span> obtained in-situ at 396m AGL from the tower. In cases where the lidar was not yet able to measure the <span class="hlt">fluxes</span> with acceptable precision, we discuss possible modifications to improve system performance.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19950045752&hterms=Parkinsons&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3DParkinsons','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19950045752&hterms=Parkinsons&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3DParkinsons"><span>The role of <span class="hlt">sea</span> ice in <span class="hlt">2</span> x <span class="hlt">CO</span><span class="hlt">2</span> climate model sensitivity. Part 1: The total influence of <span class="hlt">sea</span> ice thickness and extent</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rind, D.; Healy, R.; Parkinson, C.; Martinson, D.</p> <p>1995-01-01</p> <p>As a first step in investigating the effects of <span class="hlt">sea</span> ice changes on the climate sensitivity to doubled atmospheric <span class="hlt">CO</span><span class="hlt">2</span>, the authors use a standard simple <span class="hlt">sea</span> ice model while varying the <span class="hlt">sea</span> ice distributions and thicknesses in the control run. Thinner ice amplifies the atmospheric temperature senstivity in these experiments by about 15% (to a warming of 4.8 C), because it is easier for the thinner ice to be removed as the climate warms. Thus, its impact on sensitivity is similar to that of greater <span class="hlt">sea</span> ice extent in the control run, which provides more opportunity for <span class="hlt">sea</span> ice reduction. An experiment with <span class="hlt">sea</span> ice not allowed to change between the control and doubled <span class="hlt">CO</span><span class="hlt">2</span> simulations illustrates that the total effect of <span class="hlt">sea</span> ice on surface <span class="hlt">air</span> temperature changes, including cloud cover and water vapor feedbacks that arise in response to <span class="hlt">sea</span> ice variations, amounts to 37% of the temperature sensitivity to the <span class="hlt">CO</span><span class="hlt">2</span> doubling, accounting for 1.56 C of the 4.17 C global warming. This is about four times larger than the <span class="hlt">sea</span> ice impact when no feedbacks are allowed. The different experiments produce a range of results for southern high latitudes with the hydrologic budget over Antarctica implying <span class="hlt">sea</span> level increases of varying magnitude or no change. These results highlight the importance of properly constraining the <span class="hlt">sea</span> ice response to climate perturbations, necessitating the use of more realistic <span class="hlt">sea</span> ice and ocean models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012TCry....6..901R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012TCry....6..901R"><span>Ikaite crystals in melting <span class="hlt">sea</span> ice - implications for p<span class="hlt">CO</span><span class="hlt">2</span> and pH levels in Arctic surface waters</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rysgaard, S.; Glud, R. N.; Lennert, K.; Cooper, M.; Halden, N.; Leakey, R. J. G.; Hawthorne, F. C.; Barber, D.</p> <p>2012-08-01</p> <p>A major issue of Arctic marine science is to understand whether the Arctic Ocean is, or will be, a source or sink for <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange. This has been complicated by the recent discoveries of ikaite (a polymorph of Ca<span class="hlt">CO</span>3·6H<span class="hlt">2</span>O) in Arctic and Antarctic <span class="hlt">sea</span> ice, which indicate that multiple chemical transformations occur in <span class="hlt">sea</span> ice with a possible effect on <span class="hlt">CO</span><span class="hlt">2</span> and pH conditions in surface waters. Here, we report on biogeochemical conditions, microscopic examinations and x-ray diffraction analysis of single crystals from a melting 1.7 km<span class="hlt">2</span> (0.5-1 m thick) drifting ice floe in the Fram Strait during summer. Our findings show that ikaite crystals are present throughout the <span class="hlt">sea</span> ice but with larger crystals appearing in the upper ice layers. Ikaite crystals placed at elevated temperatures disintegrated into smaller crystallites and dissolved. During our field campaign in late June, melt reduced the ice floe thickness by 0.<span class="hlt">2</span> m per week and resulted in an estimated 3.8 ppm decrease of p<span class="hlt">CO</span><span class="hlt">2</span> in the ocean surface mixed layer. This corresponds to an <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> uptake of 10.6 mmol m-<span class="hlt">2</span> <span class="hlt">sea</span> ice d-1 or to 3.3 ton km-<span class="hlt">2</span> ice floe week-1. This is markedly higher than the estimated primary production within the ice floe of 0.3-1.3 mmol m-<span class="hlt">2</span> <span class="hlt">sea</span> ice d-1. Finally, the presence of ikaite in <span class="hlt">sea</span> ice and the dissolution of the mineral during melting of the <span class="hlt">sea</span> ice and mixing of the melt water into the surface oceanic mixed layer accounted for half of the estimated p<span class="hlt">CO</span><span class="hlt">2</span> uptake.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25046608','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25046608"><span><span class="hlt">Flux</span> measurements in the surface Marine Atmospheric Boundary Layer over the Aegean <span class="hlt">Sea</span>, Greece.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kostopoulos, V E; Helmis, C G</p> <p>2014-10-01</p> <p>Micro-meteorological measurements within the surface Marine Atmospheric Boundary Layer took place at the shoreline of two islands at northern and south-eastern Aegean <span class="hlt">Sea</span> of Greece. The primary goal of these experimental campaigns was to study the momentum, heat and humidity <span class="hlt">fluxes</span> over this part of the north-eastern Mediterranean <span class="hlt">Sea</span>, characterized by limited spatial and temporal scales which could affect these exchanges at the <span class="hlt">air-sea</span> interface. The great majority of the obtained records from both sites gave higher values up to factor of two, compared with the estimations from the most widely used parametric formulas that came mostly from measurements over open <span class="hlt">seas</span> and oceans. Friction velocity values from both campaigns varied within the same range and presented strong correlation with the wind speed at 10 m height while the calculated drag coefficient values at the same height for both sites were found to be constant in relation with the wind speed. Using eddy correlation analysis, the heat <span class="hlt">flux</span> values were calculated (virtual heat <span class="hlt">fluxes</span> varied from -60 to 40 W/m(<span class="hlt">2</span>)) and it was found that they are affected by the limited spatial and temporal scales of the responding <span class="hlt">air-sea</span> interaction mechanism. Similarly, the humidity <span class="hlt">fluxes</span> appeared to be strongly influenced by the observed intense spatial heterogeneity of the <span class="hlt">sea</span> surface temperature. Copyright © 2014 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GSL.....4....9S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GSL.....4....9S"><span>Implications of overestimated anthropogenic <span class="hlt">CO</span><span class="hlt">2</span> emissions on East Asian and global land <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> inversion</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Saeki, Tazu; Patra, Prabir K.</p> <p>2017-12-01</p> <p>Measurement and modelling of regional or country-level carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) <span class="hlt">fluxes</span> are becoming critical for verification of the greenhouse gases emission control. One of the commonly adopted approaches is inverse modelling, where <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> (emission: positive <span class="hlt">flux</span>, sink: negative <span class="hlt">flux</span>) from the terrestrial ecosystems are estimated by combining atmospheric <span class="hlt">CO</span><span class="hlt">2</span> measurements with atmospheric transport models. The inverse models assume anthropogenic emissions are known, and thus the uncertainties in the emissions introduce systematic bias in estimation of the terrestrial (residual) <span class="hlt">fluxes</span> by inverse modelling. Here we show that the <span class="hlt">CO</span><span class="hlt">2</span> sink increase, estimated by the inverse model, over East Asia (China, Japan, Korea and Mongolia), by about 0.26 PgC year-1 (1 Pg = 1012 g) during 2001-2010, is likely to be an artifact of the anthropogenic <span class="hlt">CO</span><span class="hlt">2</span> emissions increasing too quickly in China by 1.41 PgC year-1. Independent results from methane (CH4) inversion suggested about 41% lower rate of East Asian CH4 emission increase during 2002-2012. We apply a scaling factor of 0.59, based on CH4 inversion, to the rate of anthropogenic <span class="hlt">CO</span><span class="hlt">2</span> emission increase since the anthropogenic emissions of both <span class="hlt">CO</span><span class="hlt">2</span> and CH4 increase linearly in the emission inventory. We find no systematic increase in land <span class="hlt">CO</span><span class="hlt">2</span> uptake over East Asia during 1993-2010 or 2000-2009 when scaled anthropogenic <span class="hlt">CO</span><span class="hlt">2</span> emissions are used, and that there is a need of higher emission increase rate for 2010-2012 compared to those calculated by the inventory methods. High bias in anthropogenic <span class="hlt">CO</span><span class="hlt">2</span> emissions leads to stronger land sinks in global land-ocean <span class="hlt">flux</span> partitioning in our inverse model. The corrected anthropogenic <span class="hlt">CO</span><span class="hlt">2</span> emissions also produce measurable reductions in the rate of global land <span class="hlt">CO</span><span class="hlt">2</span> sink increase post-2002, leading to a better agreement with the terrestrial biospheric model simulations that include <span class="hlt">CO</span><span class="hlt">2</span>-fertilization and climate effects.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GBioC..31.1192G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GBioC..31.1192G"><span>Global evaluation of particulate organic carbon <span class="hlt">flux</span> parameterizations and implications for atmospheric p<span class="hlt">CO</span><span class="hlt">2</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gloege, Lucas; McKinley, Galen A.; Mouw, Colleen B.; Ciochetto, Audrey B.</p> <p>2017-07-01</p> <p>The shunt of photosynthetically derived particulate organic carbon (POC) from the euphotic zone and deep remineralization comprises the basic mechanism of the "biological carbon pump." POC raining through the "twilight zone" (euphotic depth to 1 km) and "midnight zone" (1 km to 4 km) is remineralized back to inorganic form through respiration. Accurately modeling POC <span class="hlt">flux</span> is critical for understanding the "biological pump" and its impacts on <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange and, ultimately, long-term ocean carbon sequestration. Yet commonly used parameterizations have not been tested quantitatively against global data sets using identical modeling frameworks. Here we use a single one-dimensional physical-biogeochemical modeling framework to assess three common POC <span class="hlt">flux</span> parameterizations in capturing POC <span class="hlt">flux</span> observations from moored sediment traps and thorium-234 depletion. The exponential decay, Martin curve, and ballast model are compared to data from 11 biogeochemical provinces distributed across the globe. In each province, the model captures satellite-based estimates of surface primary production within uncertainties. Goodness of fit is measured by how well the simulation captures the observations, quantified by bias and the root-mean-square error and displayed using "target diagrams." Comparisons are presented separately for the twilight zone and midnight zone. We find that the ballast hypothesis shows no improvement over a globally or regionally parameterized Martin curve. For all provinces taken together, Martin's b that best fits the data is [0.70, 0.98]; this finding reduces by at least a factor of 3 previous estimates of potential impacts on atmospheric p<span class="hlt">CO</span><span class="hlt">2</span> of uncertainty in POC export to a more modest range [-16 ppm, +12 ppm].</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.B53C0683C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.B53C0683C"><span>Coupling of N<span class="hlt">2</span>O and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> from agriculture in Michigan</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cui, M.; Tang, J.; Hastings, M. G.; Gelfand, I.; Tao, L.; Sun, K.</p> <p>2012-12-01</p> <p><span class="hlt">CO</span><span class="hlt">2</span> has been known to cause global warming, and N<span class="hlt">2</span>O is the largest contributor to the greenhouse gas burden of cropping systems in the United States due to application of fertilizer. In our study, <span class="hlt">fluxes</span> of N<span class="hlt">2</span>O and <span class="hlt">CO</span><span class="hlt">2</span> were measured at two maize fields and one reference grassland from Kellogg Biological Station in Southwest Michigan. Here we compared two measuring systems, traditional GC method and LGR/Li-Cor system. Our initial results show that the two measuring systems are consistent (N<span class="hlt">2</span>O slope=0.96, R<span class="hlt">2</span>=0.96; and <span class="hlt">CO</span><span class="hlt">2</span> slope= 1.03, R<span class="hlt">2</span>=0.86 measuring from the same chamber). Measurements done in pairs of chambers suggest great spatial variations, despite that the chambers were only 0.5 meter apart. The two systems are still comparable by averaging 8 pairs of chambers distributed within one site. Increase of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> were observed the second day after fertilization, but no significant change of N<span class="hlt">2</span>O <span class="hlt">fluxes</span> was shown. After artificial rainfall, boosting N<span class="hlt">2</span>O <span class="hlt">fluxes</span> and further increase in <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> were demonstrated. Our result indicates that precipitation is necessary before a prominent N<span class="hlt">2</span>O peak. In our LGR/Li-Cor system, <span class="hlt">CO</span> was also measured from chambers. Interesting <span class="hlt">CO</span> <span class="hlt">fluxes</span> were shown in our experiment. Soil, which is usually considered as a <span class="hlt">CO</span> sink, emits <span class="hlt">CO</span> in some chambers during our measurement, which is probably related to the nationwide forest fires and lack of precipitation during the period.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li class="active"><span>9</span></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_9 --> <div id="page_10" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li class="active"><span>10</span></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="181"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.2190Q','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.2190Q"><span>Development of a laser remote sensing instrument to measure sub-aerial volcanic <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Queisser, Manuel; Burton, Mike</p> <p>2016-04-01</p> <p>A thorough quantification of volcanic <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> would lead to an enhanced understanding of the role of volcanoes in the geological carbon cycle. This would enable a more subtle understanding of human impact on that cycle. Furthermore, variations in volcanic <span class="hlt">CO</span><span class="hlt">2</span> emissions are a key to understanding volcanic processes such as eruption phenomenology. However, measuring <span class="hlt">fluxes</span> of volcanic <span class="hlt">CO</span><span class="hlt">2</span> is challenging as volcanic <span class="hlt">CO</span><span class="hlt">2</span> concentrations are modest compared with the ambient <span class="hlt">CO</span><span class="hlt">2</span> concentration (~400 ppm) . Volcanic <span class="hlt">CO</span><span class="hlt">2</span> quickly dilutes with the background <span class="hlt">air</span>. For Mt. Etna (Italy), for instance, 1000 m downwind from the crater, dispersion modelling yields a signal of ~4 ppm only. It is for this reason that many magmatic <span class="hlt">CO</span><span class="hlt">2</span> concentration measurements focus on in situ techniques, such as direct sampling Giggenbach bottles, chemical sensors, IR absorption spectrometers or mass spectrometers. However, emission rates are highly variable in time and space. Point measurements fail to account for this variability. Inferring 1-D or <span class="hlt">2</span>-D gas concentration profiles, necessary to estimate gas <span class="hlt">fluxes</span>, from point measurements may thus lead to erroneous <span class="hlt">flux</span> estimations. Moreover, in situ probing is time consuming and, since many volcanoes emit toxic gases and are dangerous as mountains, may raise safety concerns. In addition, degassing is often diffuse and spatially extended, which makes a measurement approach with spatial coverage desirable. There are techniques that allow to indirectly retrieve <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> from correlated SO<span class="hlt">2</span> concentrations and <span class="hlt">fluxes</span>. However, they still rely on point measurements of <span class="hlt">CO</span><span class="hlt">2</span> and are prone to errors of SO<span class="hlt">2</span> <span class="hlt">fluxes</span> due to light dilution and depend on blue sky conditions. Here, we present a new remote sensing instrument, developed with the ERC project <span class="hlt">CO</span><span class="hlt">2</span>Volc, which measures 1-D column amounts of <span class="hlt">CO</span><span class="hlt">2</span> in the atmosphere with sufficient sensitivity to reveal the contribution of magmatic <span class="hlt">CO</span><span class="hlt">2</span>. Based on differential absorption LIDAR (DIAL) the instrument measures</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMIN12C..01H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMIN12C..01H"><span>Evaluation of Deep Learning Models for Predicting <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Flux</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Halem, M.; Nguyen, P.; Frankel, D.</p> <p>2017-12-01</p> <p>Artificial neural networks have been employed to calculate surface <span class="hlt">flux</span> measurements from station data because they are able to fit highly nonlinear relations between input and output variables without knowing the detail relationships between the variables. However, the accuracy in performing neural net estimates of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> from observations of <span class="hlt">CO</span><span class="hlt">2</span> and other atmospheric variables is influenced by the architecture of the neural model, the availability, and complexity of interactions between physical variables such as wind, temperature, and indirect variables like latent heat, and sensible heat, etc. We evaluate two deep learning models, feed forward and recurrent neural network models to learn how they each respond to the physical measurements, time dependency of the measurements of <span class="hlt">CO</span><span class="hlt">2</span> concentration, humidity, pressure, temperature, wind speed etc. for predicting the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span>. In this paper, we focus on a) building neural network models for estimating <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> based on DOE data from tower Atmospheric Radiation Measurement data; b) evaluating the impact of choosing the surface variables and model hyper-parameters on the accuracy and predictions of surface <span class="hlt">flux</span>; c) assessing the applicability of the neural network models on estimate <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> by using OCO-<span class="hlt">2</span> satellite data; d) studying the efficiency of using GPU-acceleration for neural network performance using IBM Power AI deep learning software and packages on IBM Minsky system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.1791W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.1791W"><span>Modelling storm development and the impact when introducing waves, <span class="hlt">sea</span> spray and heat <span class="hlt">fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wu, Lichuan; Rutgersson, Anna; Sahlée, Erik</p> <p>2015-04-01</p> <p>In high wind speed conditions, <span class="hlt">sea</span> spray generated due to intensity breaking waves have big influence on the wind stress and heat <span class="hlt">fluxes</span>. Measurements show that drag coefficient will decrease in high wind speed. <span class="hlt">Sea</span> spray generation function (SSGF), an important term of wind stress parameterization in high wind speed, usually treated as a function of wind speed/friction velocity. In this study, we introduce a wave state depended SSGG and wave age depended Charnock number into a high wind speed wind stress parameterization (Kudryavtsev et al., 2011; 2012). The proposed wind stress parameterization and <span class="hlt">sea</span> spray heat <span class="hlt">fluxes</span> parameterization from Andreas et al., (2014) were applied to an atmosphere-wave coupled model to test on four storm cases. Compared with measurements from the FINO1 platform in the North <span class="hlt">Sea</span>, the new wind stress parameterization can reduce the forecast errors of wind in high wind speed range, but not in low wind speed. Only <span class="hlt">sea</span> spray impacted on wind stress, it will intensify the storms (minimum <span class="hlt">sea</span> level pressure and maximum wind speed) and lower the <span class="hlt">air</span> temperature (increase the errors). Only the <span class="hlt">sea</span> spray impacted on the heat <span class="hlt">fluxes</span>, it can improve the model performance on storm tracks and the <span class="hlt">air</span> temperature, but not change much in the storm intensity. If both of <span class="hlt">sea</span> spray impacted on the wind stress and heat <span class="hlt">fluxes</span> are taken into account, it has the best performance in all the experiment for minimum <span class="hlt">sea</span> level pressure and maximum wind speed and <span class="hlt">air</span> temperature. Andreas, E. L., Mahrt, L., and Vickers, D. (2014). An improved bulk <span class="hlt">air-sea</span> surface <span class="hlt">flux</span> algorithm, including spray-mediated transfer. Quarterly Journal of the Royal Meteorological Society. Kudryavtsev, V. and Makin, V. (2011). Impact of ocean spray on the dynamics of the marine atmospheric boundary layer. Boundary-layer meteorology, 140(3):383-410. Kudryavtsev, V., Makin, V., and S, Z. (2012). On the <span class="hlt">sea</span>-surface drag and heat/mass transfer at strong winds. Technical report, Royal</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.2671L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.2671L"><span>On the role of <span class="hlt">sea</span>-state in bubble-mediated <span class="hlt">air-sea</span> gas <span class="hlt">flux</span> during a winter storm</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liang, Jun-Hong; Emerson, Steven R.; D'Asaro, Eric A.; McNeil, Craig L.; Harcourt, Ramsey R.; Sullivan, Peter P.; Yang, Bo; Cronin, Meghan F.</p> <p>2017-04-01</p> <p>Oceanic bubbles play an important role in the <span class="hlt">air-sea</span> exchange of weakly soluble gases at moderate to high wind speeds. A Lagrangian bubble model embedded in a large eddy simulation model is developed to study bubbles and their influence on dissolved gases in the upper ocean. The transient evolution of mixed-layer dissolved oxygen and nitrogen gases at Ocean Station Papa (50°N, 145°W) during a winter storm is reproduced with the model. Among different physical processes, gas bubbles are the most important in elevating dissolved gas concentrations during the storm, while atmospheric pressure governs the variability of gas saturation anomaly (the relative departure of dissolved gas concentration from the saturation concentration). For the same wind speed, bubble-mediated gas <span class="hlt">fluxes</span> are larger during rising wind with smaller wave age than during falling wind with larger wave age. Wave conditions are the primary cause for the bubble gas <span class="hlt">flux</span> difference: when wind strengthens, waves are less-developed with respect to wind, resulting in more frequent large breaking waves. Bubble generation in large breaking waves is favorable for a large bubble-mediated gas <span class="hlt">flux</span>. The wave-age dependence is not included in any existing bubble-mediated gas <span class="hlt">flux</span> parameterizations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.A34B..03F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.A34B..03F"><span>Estimating regional <span class="hlt">CO</span><span class="hlt">2</span> and CH4 <span class="hlt">fluxes</span> using GOSAT XCO<span class="hlt">2</span> and XCH4 observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fraser, A. C.; Palmer, P. I.; Feng, L.; Parker, R.; Boesch, H.; Cogan, A. J.</p> <p>2012-12-01</p> <p>We infer regional monthly surface <span class="hlt">flux</span> estimates for <span class="hlt">CO</span><span class="hlt">2</span> and CH4, June 2009-December 2010, from proxy dry-<span class="hlt">air</span> column-averaged mole fractions of <span class="hlt">CO</span><span class="hlt">2</span> and CH4 from the Greenhouse gases Observing SATellite (GOSAT) using an ensemble Kalman Filter combined with the GEOS-Chem chemistry transport model. We compare these <span class="hlt">flux</span> estimates with estimates inferred from in situ surface mole fraction measurements and from combining in situ and GOSAT measurements in order to quantify the added value of GOSAT data above the conventional surface measurement network. We find that the error reduction, a measure of how much the posterior <span class="hlt">fluxes</span> are being informed by the assimilated data, at least doubles when GOSAT measurements are used versus the surface only inversions, with the exception of regions that are well covered by the surface network at the spatial and temporal resolution of our <span class="hlt">flux</span> estimation calculation. We have incorporated a new online bias correction scheme to account for GOSAT biases. We report global and regional <span class="hlt">flux</span> estimates inferred from GOSAT and/or in situ measurements. While the global posterior <span class="hlt">fluxes</span> from GOSAT and in situ measurements agree, we find significant differences in the regional <span class="hlt">fluxes</span>, particularly over the tropics. We evaluate the posterior <span class="hlt">fluxes</span> by comparing them against independent surface mole fraction, column, and aircraft measurements using the GEOS-Chem model as an intermediary.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007BGD.....4.2279K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007BGD.....4.2279K"><span><span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> determination by closed-chamber methods can be seriously biased by inappropriate application of linear regression</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kutzbach, L.; Schneider, J.; Sachs, T.; Giebels, M.; Nykänen, H.; Shurpali, N. J.; Martikainen, P. J.; Alm, J.; Wilmking, M.</p> <p>2007-07-01</p> <p>Closed (non-steady state) chambers are widely used for quantifying carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) <span class="hlt">fluxes</span> between soils or low-stature canopies and the atmosphere. It is well recognised that covering a soil or vegetation by a closed chamber inherently disturbs the natural <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> by altering the concentration gradients between the soil, the vegetation and the overlying <span class="hlt">air</span>. Thus, the driving factors of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> are not constant during the closed chamber experiment, and no linear increase or decrease of <span class="hlt">CO</span><span class="hlt">2</span> concentration over time within the chamber headspace can be expected. Nevertheless, linear regression has been applied for calculating <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in many recent, partly influential, studies. This approach was justified by keeping the closure time short and assuming the concentration change over time to be in the linear range. Here, we test if the application of linear regression is really appropriate for estimating <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> using closed chambers over short closure times and if the application of nonlinear regression is necessary. We developed a nonlinear exponential regression model from diffusion and photosynthesis theory. This exponential model was tested with four different datasets of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> measurements (total number: 1764) conducted at three peatland sites in Finland and a tundra site in Siberia. The <span class="hlt">flux</span> measurements were performed using transparent chambers on vegetated surfaces and opaque chambers on bare peat surfaces. Thorough analyses of residuals demonstrated that linear regression was frequently not appropriate for the determination of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> by closed-chamber methods, even if closure times were kept short. The developed exponential model was well suited for nonlinear regression of the concentration over time c(t) evolution in the chamber headspace and estimation of the initial <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> at closure time for the majority of experiments. <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> estimates by linear regression can be as low as 40% of the <span class="hlt">flux</span> estimates of exponential regression for</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017BGeo...14.5765F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017BGeo...14.5765F"><span>Quantification of dimethyl sulfide (DMS) production in the <span class="hlt">sea</span> anemone Aiptasia sp. to simulate the <span class="hlt">sea-to-air</span> <span class="hlt">flux</span> from coral reefs</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Franchini, Filippo; Steinke, Michael</p> <p>2017-12-01</p> <p>The production of dimethyl sulfide (DMS) is poorly quantified in tropical reef environments but forms an essential process that couples marine and terrestrial sulfur cycles and affects climate. Here we quantified net aqueous DMS production and the concentration of its cellular precursor dimethylsulfoniopropionate (DMSP) in the <span class="hlt">sea</span> anemone Aiptasia sp., a model organism to study coral-related processes. Bleached anemones did not show net DMS production whereas symbiotic anemones produced DMS concentrations (mean ± standard error) of 160.7 ± 44.22 nmol g-1 dry weight (DW) after 48 h incubation. Symbiotic and bleached individuals showed DMSP concentrations of 32.7 ± 6.00 and 0.6 ± 0.19 µmol g-1 DW, respectively. We applied these findings to a Monte Carlo simulation to demonstrate that net aqueous DMS production accounts for only 20 % of gross aqueous DMS production. Monte Carlo-based estimations of <span class="hlt">sea-to-air</span> <span class="hlt">fluxes</span> of gaseous DMS showed that reefs may release 0.1 to 26.3 µmol DMS m-<span class="hlt">2</span> coral surface area (CSA) d-1 into the atmosphere with 40 % probability for rates between 0.5 and 1.5 µmol m-<span class="hlt">2</span> CSA d-1. These predictions were in agreement with directly quantified <span class="hlt">fluxes</span> in previous studies. Conversion to a <span class="hlt">flux</span> normalised to <span class="hlt">sea</span> surface area (SSA) (range 0.1 to 17.4, with the highest probability for 0.3 to 1.0 µmol DMS m-<span class="hlt">2</span> SSA d-1) suggests that coral reefs emit gaseous DMS at lower rates than the average global oceanic DMS <span class="hlt">flux</span> of 4.6 µmol m-<span class="hlt">2</span> SSA d-1 (19.6 Tg sulfur per year). The large difference between simulated gross and quantified net aqueous DMS production in corals suggests that the current and future potential for its production in tropical reefs is critically governed by DMS consumption processes. Hence, more research is required to assess the sensitivity of DMS-consumption pathways to ongoing environmental change in order to address the impact of predicted degradation of coral reefs on DMS production in tropical coastal ecosystems and its impact on</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26975003','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26975003"><span><span class="hlt">Air-sea</span> exchange of gaseous mercury in the East China <span class="hlt">Sea</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Chunjie; Ci, Zhijia; Wang, Zhangwei; Zhang, Xiaoshan</p> <p>2016-05-01</p> <p>Two oceanographic cruises were carried out in the East China <span class="hlt">Sea</span> (ECS) during the summer and fall of 2013. The main objectives of this study are to identify the spatial-temporal distributions of gaseous elemental mercury (GEM) in <span class="hlt">air</span> and dissolved gaseous mercury (DGM) in surface seawater, and then to estimate the Hg(0) <span class="hlt">flux</span>. The GEM concentration was lower in summer (1.61 ± 0.32 ng m(-3)) than in fall (<span class="hlt">2</span>.20 ± 0.58 ng m(-3)). The back-trajectory analysis revealed that the <span class="hlt">air</span> masses with high GEM levels during fall largely originated from the land, while the <span class="hlt">air</span> masses with low GEM levels during summer primarily originated from ocean. The spatial distribution patterns of total Hg (THg), fluorescence, and turbidity were consistent with the pattern of DGM with high levels in the nearshore area and low levels in the open <span class="hlt">sea</span>. Additionally, the levels of percentage of DGM to THg (%DGM) were higher in the open <span class="hlt">sea</span> than in the nearshore area, which was consistent with the previous studies. The THg concentration in fall was higher (1.47 ± 0.51 ng l(-1)) than those of other open oceans. The DGM concentration (60.1 ± 17.6 pg l(-1)) and Hg(0) <span class="hlt">flux</span> (4.6 ± 3.6 ng m(-<span class="hlt">2</span>) h(-1)) in summer were higher than those in fall (DGM: 49.6 ± 12.5 pg l(-1) and Hg(0) <span class="hlt">flux</span>: 3.6 ± <span class="hlt">2</span>.8 ng m(-<span class="hlt">2</span>) h(-1)). The emission <span class="hlt">flux</span> of Hg(0) from the ECS was estimated to be 27.6 tons yr(-1), accounting for ∼0.98% of the global Hg oceanic evasion though the ECS only accounts for ∼0.21% of global ocean area, indicating that the ECS plays an important role in the oceanic Hg cycle. Copyright © 2016 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.4068S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.4068S"><span><span class="hlt">Air-sea</span> heat <span class="hlt">flux</span> climatologies in the Mediterranean <span class="hlt">Sea</span>: Surface energy balance and its consistency with ocean heat storage</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Song, Xiangzhou; Yu, Lisan</p> <p>2017-05-01</p> <p>This study provides an analysis of the Mediterranean <span class="hlt">Sea</span> surface energy budget using nine surface heat <span class="hlt">flux</span> climatologies. The ensemble mean estimation shows that the net downward shortwave radiation (192 ± 19 W m-<span class="hlt">2</span>) is balanced by latent heat <span class="hlt">flux</span> (-98 ± 10 W m-<span class="hlt">2</span>), followed by net longwave radiation (-78 ± 13 W m-<span class="hlt">2</span>) and sensible heat <span class="hlt">flux</span> (-13 ± 4 W m-<span class="hlt">2</span>). The resulting net heat budget (Qnet) is <span class="hlt">2</span> ± 12 W m-<span class="hlt">2</span> into the ocean, which appears to be warm biased. The annual-mean Qnet should be -5.6 ± 1.6 W m-<span class="hlt">2</span> when estimated from the observed net transport through the Strait of Gibraltar. To diagnose the uncertainty in nine Qnet climatologies, we constructed Qnet from the heat budget equation by using historic hydrological observations to determine the heat content changes and advective heat <span class="hlt">flux</span>. We also used the Qnet from a data-assimilated global ocean state estimation as an additional reference. By comparing with the two reference Qnet estimates, we found that seven products (NCEP 1, NCEP <span class="hlt">2</span>, CFSR, ERA-Interim, MERRA, NOCSv<span class="hlt">2</span>.0, and OAFlux+ISCCP) overestimate Qnet, with magnitude ranging from 6 to 27 W m-<span class="hlt">2</span>, while two products underestimate Qnet by -6 W m-<span class="hlt">2</span> (JRA55) and -14 W m-<span class="hlt">2</span> (CORE.<span class="hlt">2</span>). Together with the previous warm pool work of Song and Yu (2013), we show that CFSR, MERRA, NOCSv<span class="hlt">2</span>.0, and OAFlux+ISCCP are warm-biased not only in the western Pacific warm pool but also in the Mediterranean <span class="hlt">Sea</span>, while CORE.<span class="hlt">2</span> is cold-biased in both regions. The NCEP 1, <span class="hlt">2</span>, and ERA-Interim are cold-biased over the warm pool but warm-biased in the Mediterranean <span class="hlt">Sea</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110005616','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110005616"><span>Comparing Global Atmospheric <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Flux</span> and Transport Models with Remote Sensing (and Other) Observations</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kawa, S. R.; Collatz, G. J.; Pawson, S.; Wennberg, P. O.; Wofsy, S. C.; Andrews, A. E.</p> <p>2010-01-01</p> <p>We report recent progress derived from comparison of global <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> and transport models with new remote sensing and other sources of <span class="hlt">CO</span><span class="hlt">2</span> data including those from satellite. The overall objective of this activity is to improve the process models that represent our understanding of the workings of the atmospheric carbon cycle. Model estimates of <span class="hlt">CO</span><span class="hlt">2</span> surface <span class="hlt">flux</span> and atmospheric transport processes are required for initial constraints on inverse analyses, to connect atmospheric observations to the location of surface sources and sinks, to provide the basic framework for carbon data assimilation, and ultimately for future projections of carbon-climate interactions. Models can also be used to test consistency within and between <span class="hlt">CO</span><span class="hlt">2</span> data sets under varying geophysical states. Here we focus on simulated <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> from terrestrial vegetation and atmospheric transport mutually constrained by analyzed meteorological fields from the Goddard Modeling and Assimilation Office for the period 2000 through 2009. Use of assimilated meteorological data enables direct model comparison to observations across a wide range of scales of variability. The biospheric <span class="hlt">fluxes</span> are produced by the CASA model at 1x1 degrees on a monthly mean basis, modulated hourly with analyzed temperature and sunlight. Both physiological and biomass burning <span class="hlt">fluxes</span> are derived using satellite observations of vegetation, burned area (as in GFED-3), and analyzed meteorology. For the purposes of comparison to <span class="hlt">CO</span><span class="hlt">2</span> data, fossil fuel and ocean <span class="hlt">fluxes</span> are also included in the transport simulations. In this presentation we evaluate the model's ability to simulate <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> and mixing ratio variability in comparison to remote sensing observations from TCCON, GOSAT, and <span class="hlt">AIRS</span> as well as relevant in situ observations. Examples of the influence of key process representations are shown from both forward and inverse model comparisons. We find that the model can resolve much of the synoptic, seasonal, and interannual</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AtmEn.178...31J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AtmEn.178...31J"><span>Seasonal atmospheric deposition and <span class="hlt">air-sea</span> gas exchange of polycyclic aromatic hydrocarbons over the Yangtze River Estuary, East China <span class="hlt">Sea</span>: Implications for source-sink processes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jiang, Yuqing; Lin, Tian; Wu, Zilan; Li, Yuanyuan; Li, Zhongxia; Guo, Zhigang; Yao, Xiaohong</p> <p>2018-04-01</p> <p>In this work, <span class="hlt">air</span> samples and surface seawater samples covering four seasons from March 2014 to January 2015 were collected from a background receptor site in the YRE to explore the seasonal <span class="hlt">fluxes</span> of <span class="hlt">air-sea</span> gas exchange and dry and wet deposition of 15 polycyclic aromatic hydrocarbons (PAHs) and their source-sink processes at the <span class="hlt">air-sea</span> interface. The average dry and wet deposition <span class="hlt">fluxes</span> of 15 PAHs were estimated as 879 ± 1393 ng m-<span class="hlt">2</span> d-1 and 755 ± 545 ng m-<span class="hlt">2</span> d-1, respectively. Gaseous PAH release from seawater to the atmosphere averaged 3114 ± 1999 ng m-<span class="hlt">2</span> d-1 in a year round. The <span class="hlt">air-sea</span> gas exchange of PAHs was the dominant process at the <span class="hlt">air-sea</span> interface in the YRE as the magnitude of volatilization <span class="hlt">flux</span> of PAHs exceeded that of total dry and wet deposition. The gas PAH exchange <span class="hlt">flux</span> was dominated by three-ring PAHs, with the highest value in summer and lowest in winter, indicating a marked seasonal variation owing to differences in Henry's law constants associated with temperature, as well as wind speed and gaseous-dissolved gradient among seasons. Based on the simplified mass balance estimation, a net 11 tons y-1 of PAHs (mainly three-ring PAHs) were volatilized from seawater to the atmosphere in a ∼20,000 km<span class="hlt">2</span> area in the YRE. Other than the year-round Yangtze River input and ocean ship emissions, the selective release of low-molecular-weight PAHs from bottom sediments in winter due to resuspension triggered by the East Asian winter monsoon is another potential source of PAHs. This work suggests that the source-sink processes of PAHs at the <span class="hlt">air-sea</span> interface in the YRE play a crucial role in regional cycling of PAHs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70020545','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70020545"><span>Winter <span class="hlt">fluxes</span> of <span class="hlt">CO</span><span class="hlt">2</span> and CH4 from subalpine soils in Rocky Mountain National Park, Colorado</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Mast, M. Alisa; Wickland, Kimberly P.; Striegl, Robert G.; Clow, David W.</p> <p>1998-01-01</p> <p><span class="hlt">Fluxes</span> of <span class="hlt">CO</span><span class="hlt">2</span> and CH4 through a seasonal snowpack were measured in and adjacent to a subalpine wetland in Rocky Mountain National Park, Colorado. Gas diffusion through the snow was controlled by gas production or consumption in the soil and by physical snowpack properties. The snowpack insulated soils from cold midwinter <span class="hlt">air</span> temperatures allowing microbial activity to continue through the winter. All soil types studied were net sources of <span class="hlt">CO</span><span class="hlt">2</span> to the atmosphere through the winter, whereas saturated soils in the wetland center were net emitters of CH4 and soils adjacent to the wetland were net CH4 consumers. Most sites showed similar temporal patterns in winter gas <span class="hlt">fluxes</span>; the lowest <span class="hlt">fluxes</span> occurred in early winter, and maximum <span class="hlt">fluxes</span> occurred at the onset of snowmelt. Temporal changes in <span class="hlt">fluxes</span> probably were related to changes in soil-moisture conditions and hydrology because soil temperatures were relatively constant under the snowpack. Average winter <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> were 42.3, 31.<span class="hlt">2</span>, and 14.6 mmol m−<span class="hlt">2</span> d−1 over dry, moist, and saturated soils, respectively, which accounted for 8 to 23% of the gross annual <span class="hlt">CO</span><span class="hlt">2</span>emissions from these soils. Average winter CH4 <span class="hlt">fluxes</span> were −0.016, 0.274, and <span class="hlt">2</span>.87 mmol m−<span class="hlt">2</span> d−1over dry, moist, and saturated soils, respectively. Microbial activity under snow cover accounted for 12% of the annual CH4 consumption in dry soils and 58 and 12% of the annual CH4 emitted from moist and saturated soils, respectively. The observed ranges in <span class="hlt">CO</span><span class="hlt">2</span> and CH4 <span class="hlt">flux</span> through snow indicated that winter <span class="hlt">fluxes</span> are an important part of the annual carbon budget in seasonally snow-covered terrains.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/4575','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/4575"><span>Quantitative comparison of in situ soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> measurement methods</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Jennifer D. Knoepp; James M. Vose</p> <p>2002-01-01</p> <p>Development of reliable regional or global carbon budgets requires accurate measurement of soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span>. We conducted laboratory and field studies to determine the accuracy and comparability of methods commonly used to measure in situ soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. Methods compared included <span class="hlt">CO</span><span class="hlt">2</span>...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.A43H..02B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.A43H..02B"><span>Optimization of <span class="hlt">CO</span><span class="hlt">2</span> Surface <span class="hlt">Flux</span> using GOSAT Total Column <span class="hlt">CO</span><span class="hlt">2</span>: First Results for 2009-2010</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Basu, S.; Houweling, S.</p> <p>2011-12-01</p> <p>Constraining surface <span class="hlt">flux</span> estimates of <span class="hlt">CO</span><span class="hlt">2</span> using satellite measurements has been one of the long-standing goals of the atmospheric inverse modeling community. We present the first results of inverting GOSAT total column <span class="hlt">CO</span><span class="hlt">2</span> measurements for obtaining global monthly <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> maps over one year (June 2009 to May 2010). We use the SRON RemoTeC retrieval of <span class="hlt">CO</span><span class="hlt">2</span> for our inversions. The SRON retrieval has been shown to have no bias when compared to TCCON total column measurements, and latitudinal gradients of the retrieved <span class="hlt">CO</span><span class="hlt">2</span> are consistent with gradients deduced from the surface flask network [Butz et al, 2011]. This makes this retrieval an ideal candidate for atmospheric inversions, which are highly sensitive to spurious gradients. Our inversion system is analogous to the CarbonTracker (CT) data assimilation system; it is initialized with the prior <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> of CT, and uses the same atmospheric transport model, i.e., TM5. The two major differences are (a) we add GOSAT <span class="hlt">CO</span><span class="hlt">2</span> data to the inversion in addition to flask data, and (b) we use a 4DVAR optimization system instead of a Kalman filter. We compare inversions using (a) only GOSAT total column <span class="hlt">CO</span><span class="hlt">2</span> measurements, (b) only surface flask <span class="hlt">CO</span><span class="hlt">2</span> measurements, and (c) the joint data set of GOSAT and surface flask measurements. We validate GOSAT-only inversions against the NOAA surface flask network and joint inversions against CONTRAIL and other aircraft campaigns. We see that inverted <span class="hlt">fluxes</span> from a GOSAT-only inversion are consistent with <span class="hlt">fluxes</span> from a stations-only inversion, reaffirming the low biases in SRON retrievals. From the joint inversion, we estimate the amount of added constraints upon adding GOSAT total column measurements to existing surface layer measurements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28484018','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28484018"><span>Enhanced <span class="hlt">CO</span><span class="hlt">2</span> uptake at a shallow Arctic Ocean seep field overwhelms the positive warming potential of emitted methane.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Pohlman, John W; Greinert, Jens; Ruppel, Carolyn; Silyakova, Anna; Vielstädte, Lisa; Casso, Michael; Mienert, Jürgen; Bünz, Stefan</p> <p>2017-05-23</p> <p>Continued warming of the Arctic Ocean in coming decades is projected to trigger the release of teragrams (1 Tg = 10 6 tons) of methane from thawing subsea permafrost on shallow continental shelves and dissociation of methane hydrate on upper continental slopes. On the shallow shelves (<100 m water depth), methane released from the seafloor may reach the atmosphere and potentially amplify global warming. On the other hand, biological uptake of carbon dioxide (<span class="hlt">CO</span> <span class="hlt">2</span> ) has the potential to offset the positive warming potential of emitted methane, a process that has not received detailed consideration for these settings. Continuous <span class="hlt">sea-air</span> gas <span class="hlt">flux</span> data collected over a shallow ebullitive methane seep field on the Svalbard margin reveal atmospheric <span class="hlt">CO</span> <span class="hlt">2</span> uptake rates (-33,300 ± 7,900 μmol m -<span class="hlt">2</span> ⋅d -1 ) twice that of surrounding waters and ∼1,900 times greater than the diffusive <span class="hlt">sea-air</span> methane efflux (17.3 ± 4.8 μmol m -<span class="hlt">2</span> ⋅d -1 ). The negative radiative forcing expected from this <span class="hlt">CO</span> <span class="hlt">2</span> uptake is up to 231 times greater than the positive radiative forcing from the methane emissions. Surface water characteristics (e.g., high dissolved oxygen, high pH, and enrichment of 13 C in <span class="hlt">CO</span> <span class="hlt">2</span> ) indicate that upwelling of cold, nutrient-rich water from near the seafloor accompanies methane emissions and stimulates <span class="hlt">CO</span> <span class="hlt">2</span> consumption by photosynthesizing phytoplankton. These findings challenge the widely held perception that areas characterized by shallow-water methane seeps and/or strongly elevated <span class="hlt">sea-air</span> methane <span class="hlt">flux</span> always increase the global atmospheric greenhouse gas burden.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.B31E0447B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.B31E0447B"><span>Assessing the impact of urban land cover composition on <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Becker, K.; Hinkle, C.</p> <p>2013-12-01</p> <p>Urbanization is an ever increasing trend in global land use change, and has been identified as a key driver of <span class="hlt">CO</span><span class="hlt">2</span> emissions. Therefore, understanding how urbanization affects <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> across a range of climatic zones and development patterns is critical to projecting the impact of future land use on <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> dynamics. A growing number of studies are applying the eddy covariance method to urban areas to quantify the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> dynamics of these systems. However, interpretation of eddy covariance data in these urban systems presents a challenge, particularly in areas with high heterogeneity due to a mixing of built and green space. Here we present a study aimed at establishing a relationship between land cover composition and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> for a heterogeneous urban area of Orlando, FL. <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> has been measured at this site for > 4 years using an open path eddy covariance system. Land cover at this site was classified into built and green space, and relative weight of both land covers were calculated for each 30 min <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> measurement using the Schuepp model and a source area based on +/- one standard deviation of wind direction. The results of this analysis established a relationship between built land cover and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> within the measured footprint of this urban area. These results, in combination with future projected land use data, will be a valuable resource for providing insight into the impact of future urbanization on <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> dynamics in this region.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFMOS53C1336T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFMOS53C1336T"><span>Carbon Dioxide Variability in the Gulf of Trieste (GOT) in the Northern Adriatic <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Turk, D.; McGillis, W. R.; Malacic, V.; Degrandpre, M.</p> <p>2008-12-01</p> <p>Coastal marine regions such as the Gulf of Trieste GOT in the Northern Adriatic <span class="hlt">Sea</span> serve as the link between carbon cycling on land and the ocean interior and potentially contribute large uncertainties in the estimate of anthropogenic <span class="hlt">CO</span><span class="hlt">2</span> uptake. This system may be either a sink or a source for atmospheric <span class="hlt">CO</span><span class="hlt">2</span>. Understanding the sources and sinks as a result of biological and physical controls for <span class="hlt">air-sea</span> carbon dioxide <span class="hlt">fluxes</span> in coastal waters may substantially alter the current view of the global carbon budget for unique terrestrial and ocean regions such as the GOT. GOT is a semi-enclosed Mediterranean basin situated in the northern part of Adriatic <span class="hlt">Sea</span>. It is one of the most productive regions in the Mediterranean and is affected by extreme fresh river input, phytoplankton blooms, and large changes of <span class="hlt">air-sea</span> exchange during Bora high wind events. The unique combination of these environmental processes and relatively small size of the area makes the region an excellent study site for investigations of <span class="hlt">air-sea</span> interaction, and changes in biology and carbon chemistry. However, there is a dearth of current data or information from the region. Here we present the first measurements of <span class="hlt">air</span> and water <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> in the GOT. The aqueous <span class="hlt">CO</span><span class="hlt">2</span> was measured at the Coastal Oceanographic buoy Piran, Slovenia using the SAMI <span class="hlt">CO</span><span class="hlt">2</span> sensor during spring and late summer and fall 2007. <span class="hlt">CO</span><span class="hlt">2</span> measurements were combined with hydrological and biological observations to evaluate the processes that control carbon cycling in the region.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA519623','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA519623"><span>The <span class="hlt">Air</span> Land <span class="hlt">Sea</span> Bulletin. Issue No. 2006-<span class="hlt">2</span>, May 2006</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2006-05-01</p> <p>THE <span class="hlt">AIR</span> LAND <span class="hlt">SEA</span> BULLETIN Issue No. 2006-<span class="hlt">2</span> <span class="hlt">Air</span> Land <span class="hlt">Sea</span> Application (ALSA) Center May 2006 IN HOUSE Director’s Comments— Final Thoughts...4 US <span class="hlt">Air</span> Force Predator UAVs Have Moved Into a More Overt Strike Role [Jane’s Defence Weekly Reprint] ........................6...SUBTITLE The <span class="hlt">Air</span> Land <span class="hlt">Sea</span> Bulletin. Issue No. 2006-<span class="hlt">2</span>, May 2006 5a. CONTRACT NUMBER 5b. GRANT NUMBER 5c. PROGRAM ELEMENT NUMBER 6. AUTHOR(S) 5d. PROJECT</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007BGeo....4.1005K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007BGeo....4.1005K"><span><span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> determination by closed-chamber methods can be seriously biased by inappropriate application of linear regression</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kutzbach, L.; Schneider, J.; Sachs, T.; Giebels, M.; Nykänen, H.; Shurpali, N. J.; Martikainen, P. J.; Alm, J.; Wilmking, M.</p> <p>2007-11-01</p> <p>Closed (non-steady state) chambers are widely used for quantifying carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) <span class="hlt">fluxes</span> between soils or low-stature canopies and the atmosphere. It is well recognised that covering a soil or vegetation by a closed chamber inherently disturbs the natural <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> by altering the concentration gradients between the soil, the vegetation and the overlying <span class="hlt">air</span>. Thus, the driving factors of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> are not constant during the closed chamber experiment, and no linear increase or decrease of <span class="hlt">CO</span><span class="hlt">2</span> concentration over time within the chamber headspace can be expected. Nevertheless, linear regression has been applied for calculating <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in many recent, partly influential, studies. This approach has been justified by keeping the closure time short and assuming the concentration change over time to be in the linear range. Here, we test if the application of linear regression is really appropriate for estimating <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> using closed chambers over short closure times and if the application of nonlinear regression is necessary. We developed a nonlinear exponential regression model from diffusion and photosynthesis theory. This exponential model was tested with four different datasets of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> measurements (total number: 1764) conducted at three peatlands sites in Finland and a tundra site in Siberia. Thorough analyses of residuals demonstrated that linear regression was frequently not appropriate for the determination of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> by closed-chamber methods, even if closure times were kept short. The developed exponential model was well suited for nonlinear regression of the concentration over time c(t) evolution in the chamber headspace and estimation of the initial <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> at closure time for the majority of experiments. However, a rather large percentage of the exponential regression functions showed curvatures not consistent with the theoretical model which is considered to be caused by violations of the underlying model assumptions. Especially the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhDT........41W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhDT........41W"><span>The Response of the Ocean Thermal Skin Layer to <span class="hlt">Air-Sea</span> Surface Heat <span class="hlt">Fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wong, Elizabeth Wing-See</p> <p></p> <p>There is much evidence that the ocean is heating as a result of an increase in concentrations of greenhouse gases (GHGs) in the atmosphere from human activities. GHGs absorb infrared radiation and re-emit infrared radiation back to the ocean's surface which is subsequently absorbed. However, the incoming infrared radiation is absorbed within the top micrometers of the ocean's surface which is where the thermal skin layer exists. Thus the incident infrared radiation does not directly heat the upper few meters of the ocean. We are therefore motivated to investigate the physical mechanism between the absorption of infrared radiation and its effect on heat transfer at the <span class="hlt">air-sea</span> boundary. The hypothesis is that since heat lost through the <span class="hlt">air-sea</span> interface is controlled by the thermal skin layer, which is directly influenced by the absorption and emission of infrared radiation, the heat flow through the thermal skin layer adjusts to maintain the surface heat loss, assuming the surface heat loss does not vary, and thus modulates the upper ocean heat content. This hypothesis is investigated through utilizing clouds to represent an increase in incoming longwave radiation and analyzing retrieved thermal skin layer vertical temperature profiles from a shipboard infrared spectrometer from two research cruises. The data are limited to night-time, no precipitation and low winds of less than <span class="hlt">2</span> m/s to remove effects of solar radiation, wind-driven shear and possibilities of thermal skin layer disruption. The results show independence of the turbulent <span class="hlt">fluxes</span> and emitted radiation on the incident radiative <span class="hlt">fluxes</span> which rules out the immediate release of heat from the absorption of the cloud infrared irradiance back into the atmosphere through processes such as evaporation and increase infrared emission. Furthermore, independence was confirmed between the incoming and outgoing radiative <span class="hlt">flux</span> which implies the heat sink for upward flowing heat at the <span class="hlt">air-sea</span> interface is more</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li class="active"><span>10</span></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_10 --> <div id="page_11" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="201"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMOS24A..02V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMOS24A..02V"><span>Watershed-scale drivers of <span class="hlt">air</span>-water <span class="hlt">CO</span><span class="hlt">2</span> exchanges in two lagoonal, North Carolina (USA) estuaries</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Van Dam, B.; Crosswell, J.; Anderson, I. C.; Paerl, H. W.</p> <p>2017-12-01</p> <p>Riverine loading of nutrients and organic matter act in concert to modulate <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in estuaries, yet quantitative relationships between these factors remain poorly defined. This study explored watershed-scale mechanisms responsible for the relatively low <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> observed in two microtidal, lagoonal estuaries. <span class="hlt">Air</span>-water <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> were quantified with 74 high-resolution spatial surveys in the neighboring New River Estuary (NewRE) and Neuse River Estuary (NeuseRE), North Carolina, which experience a common climatology, but differ in marine versus riverine influence. Annually, both estuaries were relatively small sources of <span class="hlt">CO</span><span class="hlt">2</span> to the atmosphere, 12.5 and 16.3 mmol C m<span class="hlt">2</span> d-1 in the NeuseRE and NewRE, respectively. Variations in riverine alkalinity and inorganic carbon loading caused zones of minimum buffering capacity to occur at different locations in each estuary, enhancing the sensitivity of estuarine inorganic C chemistry to acidification. Large-scale p<span class="hlt">CO</span><span class="hlt">2</span> variations were driven by changes in freshwater age (akin to residence time), which modulate nutrient and organic carbon supply and phytoplankton flushing. Greatest p<span class="hlt">CO</span><span class="hlt">2</span> under-saturation was observed at intermediate freshwater ages, between <span class="hlt">2</span>-3 weeks. Biological controls on <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> were obscured by variable inputs of river-borne <span class="hlt">CO</span><span class="hlt">2</span>, which drove <span class="hlt">CO</span><span class="hlt">2</span> degassing in the river-dominated NeuseRE. Internally produced <span class="hlt">CO</span><span class="hlt">2</span> exceeded river-borne <span class="hlt">CO</span><span class="hlt">2</span> in the marine-dominated NewRE, suggesting that net ecosystem heterotrophy, rather than riverine inputs, drove <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in this system. Although annual <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> were similar between systems, watershed-specific hydrologic factors led to disparate controls on internal carbonate chemistry, which can influence overall ecosystem health and response to future perturbation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRG..123..271V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRG..123..271V"><span>Watershed-Scale Drivers of <span class="hlt">Air</span>-Water <span class="hlt">CO</span><span class="hlt">2</span> Exchanges in Two Lagoonal North Carolina (USA) Estuaries</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Van Dam, Bryce R.; Crosswell, Joseph R.; Anderson, Iris C.; Paerl, Hans W.</p> <p>2018-01-01</p> <p>Riverine loading of nutrients and organic matter act in concert to modulate <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in estuaries, yet quantitative relationships between these factors remain poorly defined. This study explored watershed-scale mechanisms responsible for the relatively low <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> observed in two microtidal, lagoonal estuaries. <span class="hlt">Air</span>-water <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> were quantified with 74 high-resolution spatial surveys in the neighboring New River Estuary (NewRE) and Neuse River Estuary (NeuseRE), North Carolina, which experience a common climatology but differ in marine versus riverine influence. Annually, both estuaries were relatively small sources of <span class="hlt">CO</span><span class="hlt">2</span> to the atmosphere, 12.5 and 16.3 mmol C m-<span class="hlt">2</span> d-1 in the NeuseRE and NewRE, respectively. Large-scale p<span class="hlt">CO</span><span class="hlt">2</span> variations were driven by changes in freshwater age, which modulates nutrient and organic carbon supply and phytoplankton flushing. Greatest p<span class="hlt">CO</span><span class="hlt">2</span> undersaturation was observed at intermediate freshwater ages, between <span class="hlt">2</span> and 3 weeks. Biological controls on <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> were obscured by variable inputs of river-borne <span class="hlt">CO</span><span class="hlt">2</span>, which drove <span class="hlt">CO</span><span class="hlt">2</span> degassing in the river-dominated NeuseRE. Internally produced <span class="hlt">CO</span><span class="hlt">2</span> exceeded river-borne <span class="hlt">CO</span><span class="hlt">2</span> in the marine-dominated NewRE, suggesting that net ecosystem heterotrophy, rather than riverine inputs, drove <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in this system. Variations in riverine alkalinity and inorganic carbon loading caused zones of minimum buffering capacity to occur at different locations in each estuary, enhancing the sensitivity of estuarine inorganic C chemistry to acidification. Although annual <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> were similar between systems, watershed-specific hydrologic factors led to disparate controls on internal carbonate chemistry, which can influence ecosystem biogeochemical cycling, trophic state, and response to future perturbations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E%26PSL.489..123S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26PSL.489..123S"><span>Infiltration-driven metamorphism, New England, USA: Regional <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> and implications for Devonian climate and extinctions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stewart, E. M.; Ague, Jay J.</p> <p>2018-05-01</p> <p>We undertake thermodynamic pseudosection modeling of metacarbonate rocks in the Wepawaug Schist, Connecticut, USA, and examine the implications for <span class="hlt">CO</span><span class="hlt">2</span> outgassing from collisional orogenic belts. Two broad types of pseudosections are calculated: (1) a fully closed-system model with no fluid infiltration and (<span class="hlt">2</span>) a fluid-buffered model including an H<span class="hlt">2</span>O-<span class="hlt">CO</span><span class="hlt">2</span> fluid of a fixed composition. This fluid-buffered model is used to approximate a system open to infiltration by a water-bearing fluid. In all cases the fully closed-system model fails to reproduce the observed major mineral zones, mineral compositions, reaction temperatures, and fluid compositions. The fluid-infiltrated models, on the other hand, successfully reproduce these observations when the XCO<span class="hlt">2</span> of the fluid is in the range ∼0.05 to ∼0.15. Fluid-infiltrated models predict significant progressive <span class="hlt">CO</span><span class="hlt">2</span> loss, peaking at ∼50% decarbonation at amphibolite facies. The closed-system models dramatically underestimate the degree of decarbonation, predicting only ∼15% <span class="hlt">CO</span><span class="hlt">2</span> loss at peak conditions, and, remarkably, <1% <span class="hlt">CO</span><span class="hlt">2</span> loss below ∼600 °C. We propagate the results of fluid-infiltrated pseudosections to determine an areal <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> for the Wepawaug Schist. This yields ∼1012 mol <span class="hlt">CO</span><span class="hlt">2</span> km-<span class="hlt">2</span> Myr-1, consistent with multiple independent estimates of the metamorphic <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span>, and comparable in magnitude to <span class="hlt">fluxes</span> from mid-ocean ridges and volcanic arcs. Extrapolating to the area of the Acadian orogenic belt, we suggest that metamorphic <span class="hlt">CO</span><span class="hlt">2</span> degassing is a plausible driver of global warming, <span class="hlt">sea</span> level rise, and, perhaps, extinction in the mid- to late-Devonian.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JMS...173...49L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JMS...173...49L"><span>Controlling mechanisms of surface partial pressure of <span class="hlt">CO</span><span class="hlt">2</span> in Jiaozhou Bay during summer and the influence of heavy rain</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Yunxiao; Yang, Xufeng; Han, Ping; Xue, Liang; Zhang, Longjun</p> <p>2017-09-01</p> <p>Due to the combined effects of natural processes and human activities, carbon source/sink processes and mechanisms in the coastal ocean are becoming more and more important in current ocean carbon cycle research. Based on differences in the ratio of total alkalinity (TA) to dissolved inorganic carbon (DIC) associated with terrestrial input, biological process (production and respiration), calcium carbonate (Ca<span class="hlt">CO</span>3) process (precipitation and dissolution) and <span class="hlt">CO</span><span class="hlt">2</span> evasion/invasion, we discuss the mechanisms controlling the surface partial pressure of <span class="hlt">CO</span><span class="hlt">2</span> (p<span class="hlt">CO</span><span class="hlt">2</span>) in Jiaozhou Bay (JZB) during summer and the influence of heavy rain, via three cruises performed in mid-June, early July and late July of 2014. In mid-June and in early July, without heavy rain or obvious river input, <span class="hlt">sea</span> surface p<span class="hlt">CO</span><span class="hlt">2</span> ranged from 521 to 1080 μatm and from 547 to 998 μatm, respectively. The direct input of DIC from sewage and the intense respiration produced large DIC additions and the highest p<span class="hlt">CO</span><span class="hlt">2</span> values in the northeast of the bay near the downtown of Qingdao. However, in the west of the bay, significant Ca<span class="hlt">CO</span>3 precipitation led to DIC removal but no obvious increase in p<span class="hlt">CO</span><span class="hlt">2</span>, which was just close to that in the central area. Due to the shallow depth and longer water residence time in this region, this pattern may be related to the sustained release of <span class="hlt">CO</span><span class="hlt">2</span> into the atmosphere. In late July, heavy rain promoted river input in the western and eastern portions of JZB. Strong primary production led to a significant decrease in p<span class="hlt">CO</span><span class="hlt">2</span> in the western area, with the lowest p<span class="hlt">CO</span><span class="hlt">2</span> value of 252 μatm. However, in the northeastern area, the intense respiration remained, and the highest p<span class="hlt">CO</span><span class="hlt">2</span> value was 1149 μatm. The average <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> in mid-June and early July was 20.23 mmol m- <span class="hlt">2</span> d- 1 and 23.56 mmol m- <span class="hlt">2</span> d- 1, respectively. In contrast, in late July, sources became sinks for atmospheric <span class="hlt">CO</span><span class="hlt">2</span> in the western and central areas of the bay, halving the average <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> to a value of 10.58 mmol m- <span class="hlt">2</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeoRL..44.5627S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoRL..44.5627S"><span>Variability and trends in surface seawater p<span class="hlt">CO</span><span class="hlt">2</span> and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> in the Pacific Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sutton, A. J.; Wanninkhof, R.; Sabine, C. L.; Feely, R. A.; Cronin, M. F.; Weller, R. A.</p> <p>2017-06-01</p> <p>Variability and change in the ocean sink of anthropogenic carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) have implications for future climate and ocean acidification. Measurements of surface seawater <span class="hlt">CO</span><span class="hlt">2</span> partial pressure (p<span class="hlt">CO</span><span class="hlt">2</span>) and wind speed from moored platforms are used to calculate high-resolution <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> time series. Here we use the moored <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> to examine variability and its drivers over a range of time scales at four locations in the Pacific Ocean. There are significant surface seawater p<span class="hlt">CO</span><span class="hlt">2</span>, salinity, and wind speed trends in the North Pacific subtropical gyre, especially during winter and spring, which reduce <span class="hlt">CO</span><span class="hlt">2</span> uptake over the 10 year record of this study. Starting in late 2013, elevated seawater p<span class="hlt">CO</span><span class="hlt">2</span> values driven by warm anomalies cause this region to be a net annual <span class="hlt">CO</span><span class="hlt">2</span> source for the first time in the observational record, demonstrating how climate forcing can influence the timing of an ocean region shift from <span class="hlt">CO</span><span class="hlt">2</span> sink to source.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23932146','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23932146"><span>The <span class="hlt">sea-air</span> exchange of mercury (Hg) in the marine boundary layer of the Augusta basin (southern Italy): concentrations and evasion <span class="hlt">flux</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bagnato, E; Sproveri, M; Barra, M; Bitetto, M; Bonsignore, M; Calabrese, S; Di Stefano, V; Oliveri, E; Parello, F; Mazzola, S</p> <p>2013-11-01</p> <p>The first attempt to systematically investigate the atmospheric mercury (Hg) in the MBL of the Augusta basin (SE Sicily, Italy) has been undertaken. In the past the basin was the receptor for Hg from an intense industrial activity which contaminated the bottom sediments of the Bay, making this area a potential source of pollution for the surrounding Mediterranean. Three oceanographic cruises have been thus performed in the basin during the winter and summer 2011/2012, where we estimated averaged Hgatm concentrations of about 1.5±0.4 (range 0.9-3.1) and <span class="hlt">2</span>.1±0.98 (range 1.1-3.1) ng m(-3) for the two seasons, respectively. These data are somewhat higher than the background Hg atm value measured over the land (range 1.1±0.3 ng m(-3)) at downtown Augusta, while are similar to those detected in other polluted regions elsewhere. Hg evasion <span class="hlt">fluxes</span> estimated at the <span class="hlt">sea/air</span> interface over the Bay range from 3.6±0.3 (unpolluted site) to 72±0.1 (polluted site of the basin) ng m(-<span class="hlt">2</span>) h(-1). By extending these measurements to the entire area of the Augusta basin (~23.5 km(<span class="hlt">2</span>)), we calculated a total <span class="hlt">sea-air</span> Hg evasion <span class="hlt">flux</span> of about 9.7±0.1 g d(-1) (~0.004 tyr(-1)), accounting for ~0.0002% of the global Hg oceanic evasion (2000 tyr(-1)). The new proposed data set offers a unique and original study on the potential outflow of Hg from the <span class="hlt">sea-air</span> interface at the basin, and it represents an important step for a better comprehension of the processes occurring in the marine biogeochemical cycle of this element. Copyright © 2013 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016GBioC..30.1509B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GBioC..30.1509B"><span>The role of metabolism in modulating <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in boreal lakes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bogard, Matthew J.; del Giorgio, Paul A.</p> <p>2016-10-01</p> <p>Lake <span class="hlt">CO</span><span class="hlt">2</span> emissions are increasingly recognized as an important component of the global <span class="hlt">CO</span><span class="hlt">2</span> cycle, yet the origin of these emissions is not clear, as specific contributions from metabolism and in-lake cycling, versus external inputs, are not well defined. To assess the coupling of lake metabolism with <span class="hlt">CO</span><span class="hlt">2</span> concentrations and <span class="hlt">fluxes</span>, we estimated steady state ratios of gross primary production to respiration (GPP:R) and rates of net ecosystem production (NEP = GPP-R) from surface water O<span class="hlt">2</span> dynamics (concentration and stable isotopes) in 187 boreal lakes spanning long environmental gradients. Our findings suggest that internal metabolism plays a dominant role in regulating <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in most lakes, but this pattern only emerges when examined at a resolution that accounts for the vastly differing relationships between lake metabolism and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. <span class="hlt">Fluxes</span> of <span class="hlt">CO</span><span class="hlt">2</span> exceeded those from NEP in over half the lakes, but unexpectedly, these effects were most common and typically largest in a subset ( 30% of total) of net autotrophic lakes that nevertheless emitted <span class="hlt">CO</span><span class="hlt">2</span>. Equally surprising, we found no environmental characteristics that distinguished this category from the more common net heterotrophic, <span class="hlt">CO</span><span class="hlt">2</span> outgassing lakes. Excess <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> relative to NEP were best predicted by catchment structure and hydrologic properties, and we infer from a combination of methods that both catchment inputs and internal anaerobic processes may have contributed this excess <span class="hlt">CO</span><span class="hlt">2</span>. Together, our findings show that the link between lake metabolism and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> is often strong but can vary widely across the boreal biome, having important implications for catchment-wide C budgets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009GeoRL..3621605V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009GeoRL..3621605V"><span>A generalized model for the <span class="hlt">air-sea</span> transfer of dimethyl sulfide at high wind speeds</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vlahos, Penny; Monahan, Edward C.</p> <p>2009-11-01</p> <p>The <span class="hlt">air-sea</span> exchange of dimethyl sulfide (DMS) is an important component of ocean biogeochemistry and global climate models. Both laboratory experiments and field measurements of DMS transfer rates have shown that the <span class="hlt">air-sea</span> <span class="hlt">flux</span> of DMS is analogous to that of other significant greenhouse gases such as <span class="hlt">CO</span><span class="hlt">2</span> at low wind speeds (<10 m/s) but that these DMS transfer rates may diverge from other gases as wind speeds increase. Herein we provide a mechanism that predicts the attenuation of DMS transfer rates at high wind speeds. The model is based on the amphiphilic nature of DMS that leads to transfer delay at the water-bubble interface and becomes significant at wind speeds above >10 m/s. The result is an attenuation of the dimensionless Henry's Law constant (H) where (Heff = H/(1 + (Cmix/Cw) ΦB) by a solubility enhancement Cmix/Cw, and the fraction of bubble surface area per m<span class="hlt">2</span> surface ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003AGUFMOS22D..03C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003AGUFMOS22D..03C"><span>Do Continental Shelves Act as an Atmospheric <span class="hlt">CO</span><span class="hlt">2</span> Sink?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cai, W.</p> <p>2003-12-01</p> <p>Recent <span class="hlt">air-to-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> measurements at several major continental shelves (European Atlantic Shelves, East China <span class="hlt">Sea</span> and U.S. Middle Atlantic Bight) suggest that shelves may act as a one-way pump and absorb atmospheric <span class="hlt">CO</span><span class="hlt">2</span> into the ocean. These observations also favor the argument that continental shelves are autotrophic (i.e., net production of organic carbon, OC). The U.S. South Atlantic Bight (SAB) contrasts these findings in that it acts as a strong source of <span class="hlt">CO</span><span class="hlt">2</span> to the atmosphere while simultaneously exporting dissolved inorganic carbon (DIC) to the open ocean. We report p<span class="hlt">CO</span><span class="hlt">2</span>, DIC, and alkalinity data from the SAB collected in 8 cruises along a transect from the shore to the shelf break in the central SAB. The shelf-wide net heterotrophy and carbon exports in the SAB are subsidized by the export of OC from the abundant intertidal marshes, which are a sink for atmospheric <span class="hlt">CO</span><span class="hlt">2</span>. It is proposed here that the SAB represents a marsh-dominated heterotrophic ocean margin as opposed to river-dominated autotrophic margins. To further investigate why margins may behave differently in term of <span class="hlt">CO</span><span class="hlt">2</span> sink/source, the physical and biological conditions of several western boundary current margins are compared. Based on this and other studies, DIC export <span class="hlt">flux</span> from margins to the open ocean must be significant in the overall global ocean carbon budget.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1713324C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1713324C"><span>Spatial sensitivity of inorganic carbon to model setup: North <span class="hlt">Sea</span> and Baltic <span class="hlt">Sea</span> with ECOSMO</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Castano Primo, Rocio; Schrum, Corinna; Daewel, Ute</p> <p>2015-04-01</p> <p>In ocean biogeochemical models it is critical to capture the key processes adequately so they do not only reproduce the observations but that those processes are reproduced correctly. One key issue is the choice of parameters, which in most cases are estimates with large uncertainties. This can be the product of actual lack of detailed knowledge of the process, or the manner the processes are implemented, more or less complex. In addition, the model sensitivity is not necessarily homogenous across the spatial domain modelled, which adds another layer of complexity to biogeochemical modelling. In the particular case of the inorganic carbon cycle, there are several sets of carbonate constants that can be chosen. The calculated <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> is largely dependent on the parametrization chosen. In addition, the different parametrizations all the underlying processes that in some way impact the carbon cycle beyond the carbonate dissociation and <span class="hlt">fluxes</span> give results that can be significantly different. Examples of these processes are phytoplankton growth rates or remineralization rates. Despite their geographical proximity, the North and Baltic <span class="hlt">Seas</span> exhibit very different dynamics. The North <span class="hlt">Sea</span> receives important inflows of Atlantic waters, while the Baltic <span class="hlt">Sea</span> is an almost enclosed system, with very little exchange from the North <span class="hlt">Sea</span>. Wind, tides, and freshwater supply act very differently, but dominantly structure the ecosystem dynamics on spatial and temporal scales. The biological community is also different. Cyanobacteria, which are important due to their ability to fix atmospheric nitrogen, and they are only present in the Baltic <span class="hlt">Sea</span>. These differentiating features have a strong impact in the biogeochemical cycles and ultimately shape the variations in the carbonate chemistry. Here the ECOSMO model was employed on the North <span class="hlt">Sea</span> and Baltic <span class="hlt">Sea</span>. The model is set so both are modelled at the same time, instead of having them run separately. ECOSMO is a 3-D coupled</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003JGRD..108.8224W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003JGRD..108.8224W"><span>Soil surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> in a boreal black spruce fire chronosequence</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Chuankuan; Bond-Lamberty, Ben; Gower, Stith T.</p> <p>2003-02-01</p> <p>Understanding the effects of wildfire on the carbon (C) cycle of boreal forests is essential to quantifying the role of boreal forests in the global carbon cycle. Soil surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> (Rs), the second largest C <span class="hlt">flux</span> in boreal forests, is directly and indirectly affected by fire and is hypothesized to change during forest succession following fire. The overall objective of this study was to measure and model Rs for a black spruce (Picea mariana [Mill.] BSP) postfire chronosequence in northern Manitoba, Canada. The experiment design was a nested factorial that included two soil drainage classes (well and poorly drained) × seven postfire aged stands. Specific objectives were (1) to quantify the relationship between Rs and soil temperature for different aged boreal black spruce forests in well-drained and poorly drained soil conditions, (<span class="hlt">2</span>) to examine Rs dynamics along postfire successional stands, and (3) to estimate annual soil surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> for these ecosystems. Soil surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> was significantly affected by soil drainage class (p = 0.014) and stand age (p = 0.006). Soil surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> was positively correlated to soil temperature (R<span class="hlt">2</span> = 0.78, p < 0.001), but different models were required for each drainage class × aged stand combination. Soil surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> was significantly greater at the well-drained than the poorly drained stands (p = 0.007) during growing season. Annual soil surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> for the 1998, 1995, 1989, 1981, 1964, 1930, and 1870 burned stands averaged 226, 412, 357, 413, 350, 274, and 244 g C m-<span class="hlt">2</span> yr-1 in the well-drained stands and 146, 380, 300, 303, 256, 233, and 264 g C m-<span class="hlt">2</span> yr-1 in the poorly drained stands. Soil surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> during the winter (from 1 November to 30 April) comprised from 5 to 19% of the total annual Rs. We speculate that the smaller soil surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> in the recently burned than the older stands is mainly caused by decreased root respiration.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002JGRD..107.8224W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002JGRD..107.8224W"><span>Soil surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> in a boreal black spruce fire chronosequence</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Chuankuan; Bond-Lamberty, Ben; Gower, Stith T.</p> <p>2002-02-01</p> <p>Understanding the effects of wildfire on the carbon (C) cycle of boreal forests is essential to quantifying the role of boreal forests in the global carbon cycle. Soil surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> (Rs), the second largest C <span class="hlt">flux</span> in boreal forests, is directly and indirectly affected by fire and is hypothesized to change during forest succession following fire. The overall objective of this study was to measure and model Rs for a black spruce (Picea mariana [Mill.] BSP) postfire chronosequence in northern Manitoba, Canada. The experiment design was a nested factorial that included two soil drainage classes (well and poorly drained) × seven postfire aged stands. Specific objectives were (1) to quantify the relationship between Rs and soil temperature for different aged boreal black spruce forests in well-drained and poorly drained soil conditions, (<span class="hlt">2</span>) to examine Rs dynamics along postfire successional stands, and (3) to estimate annual soil surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> for these ecosystems. Soil surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> was significantly affected by soil drainage class (p = 0.014) and stand age (p = 0.006). Soil surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> was positively correlated to soil temperature (R<span class="hlt">2</span> = 0.78, p < 0.001), but different models were required for each drainage class × aged stand combination. Soil surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> was significantly greater at the well-drained than the poorly drained stands (p = 0.007) during growing season. Annual soil surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> for the 1998, 1995, 1989, 1981, 1964, 1930, and 1870 burned stands averaged 226, 412, 357, 413, 350, 274, and 244 g C m-<span class="hlt">2</span> yr-1 in the well-drained stands and 146, 380, 300, 303, 256, 233, and 264 g C m-<span class="hlt">2</span> yr-1 in the poorly drained stands. Soil surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> during the winter (from 1 November to 30 April) comprised from 5 to 19% of the total annual Rs. We speculate that the smaller soil surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> in the recently burned than the older stands is mainly caused by decreased root respiration.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150000330','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150000330"><span>Sensitivity of Simulated Global Ocean Carbon <span class="hlt">Flux</span> Estimates to Forcing by Reanalysis Products</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gregg, Watson W.; Casey, Nancy W.; Rousseaux, Cecile S.</p> <p>2015-01-01</p> <p>Reanalysis products from MERRA, NCEP<span class="hlt">2</span>, NCEP1, and ECMWF were used to force an established ocean biogeochemical model to estimate <span class="hlt">air-sea</span> carbon <span class="hlt">fluxes</span> (FCO<span class="hlt">2</span>) and partial pressure of carbon dioxide (p<span class="hlt">CO</span><span class="hlt">2</span>) in the global oceans. Global <span class="hlt">air-sea</span> carbon <span class="hlt">fluxes</span> and p<span class="hlt">CO</span><span class="hlt">2</span> were relatively insensitive to the choice of forcing reanalysis. All global FCO<span class="hlt">2</span> estimates from the model forced by the four different reanalyses were within 20% of in situ estimates (MERRA and NCEP1 were within 7%), and all models exhibited statistically significant positive correlations with in situ estimates across the 12 major oceanographic basins. Global p<span class="hlt">CO</span><span class="hlt">2</span> estimates were within 1% of in situ estimates with ECMWF being the outlier at 0.6%. Basin correlations were similar to FCO<span class="hlt">2</span>. There were, however, substantial departures among basin estimates from the different reanalysis forcings. The high latitudes and tropics had the largest ranges in estimated <span class="hlt">fluxes</span> among the reanalyses. Regional p<span class="hlt">CO</span><span class="hlt">2</span> differences among the reanalysis forcings were muted relative to the FCO<span class="hlt">2</span> results. No individual reanalysis was uniformly better or worse in the major oceanographic basins. The results provide information on the characterization of uncertainty in ocean carbon models due to choice of reanalysis forcing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26324399','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26324399"><span>New ground-based lidar enables volcanic <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> measurements.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Aiuppa, Alessandro; Fiorani, Luca; Santoro, Simone; Parracino, Stefano; Nuvoli, Marcello; Chiodini, Giovanni; Minopoli, Carmine; Tamburello, Giancarlo</p> <p>2015-09-01</p> <p>There have been substantial advances in the ability to monitor the activity of hazardous volcanoes in recent decades. However, obtaining early warning of eruptions remains challenging, because the patterns and consequences of volcanic unrests are both complex and nonlinear. Measuring volcanic gases has long been a key aspect of volcano monitoring since these mobile fluids should reach the surface long before the magma. There has been considerable progress in methods for remote and in-situ gas sensing, but measuring the <span class="hlt">flux</span> of volcanic <span class="hlt">CO</span><span class="hlt">2</span>-the most reliable gas precursor to an eruption-has remained a challenge. Here we report on the first direct quantitative measurements of the volcanic <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> using a newly designed differential absorption lidar (DIAL), which were performed at the restless Campi Flegrei volcano. We show that DIAL makes it possible to remotely obtain volcanic <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> time series with a high temporal resolution (tens of minutes) and accuracy (<30%). The ability of this lidar to remotely sense volcanic <span class="hlt">CO</span><span class="hlt">2</span> represents a major step forward in volcano monitoring, and will contribute improved volcanic <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> inventories. Our results also demonstrate the unusually strong degassing behavior of Campi Flegrei fumaroles in the current ongoing state of unrest.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.4204Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.4204Z"><span>Global <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> inversions from remote-sensing data with systematic errors using hierarchical statistical models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zammit-Mangion, Andrew; Stavert, Ann; Rigby, Matthew; Ganesan, Anita; Rayner, Peter; Cressie, Noel</p> <p>2017-04-01</p> <p>The Orbiting Carbon Observatory-<span class="hlt">2</span> (OCO-<span class="hlt">2</span>) satellite was launched on <span class="hlt">2</span> July 2014, and it has been a source of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> data since September 2014. The OCO-<span class="hlt">2</span> dataset contains a number of variables, but the one of most interest for <span class="hlt">flux</span> inversion has been the column-averaged dry-<span class="hlt">air</span> mole fraction (in units of ppm). These global level-<span class="hlt">2</span> data offer the possibility of inferring <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> at Earth's surface and tracking those <span class="hlt">fluxes</span> over time. However, as well as having a component of random error, the OCO-<span class="hlt">2</span> data have a component of systematic error that is dependent on the instrument's mode, namely land nadir, land glint, and ocean glint. Our statistical approach to <span class="hlt">CO</span><span class="hlt">2</span>-<span class="hlt">flux</span> inversion starts with constructing a statistical model for the random and systematic errors with parameters that can be estimated from the OCO-<span class="hlt">2</span> data and possibly in situ sources from flasks, towers, and the Total Column Carbon Observing Network (TCCON). Dimension reduction of the <span class="hlt">flux</span> field is achieved through the use of physical basis functions, while temporal evolution of the <span class="hlt">flux</span> is captured by modelling the basis-function coefficients as a vector autoregressive process. For computational efficiency, <span class="hlt">flux</span> inversion uses only three months of sensitivities of mole fraction to changes in <span class="hlt">flux</span>, computed using MOZART; any residual variation is captured through the modelling of a stochastic process that varies smoothly as a function of latitude. The second stage of our statistical approach is to simulate from the posterior distribution of the basis-function coefficients and all unknown parameters given the data using a fully Bayesian Markov chain Monte Carlo (MCMC) algorithm. Estimates and posterior variances of the <span class="hlt">flux</span> field can then be obtained straightforwardly from this distribution. Our statistical approach is different than others, as it simultaneously makes inference (and quantifies uncertainty) on both the error components' parameters and the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. We compare it to more classical</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70023234','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70023234"><span>High <span class="hlt">CO</span><span class="hlt">2</span> emissions through porous media: Transport mechanisms and implications for <span class="hlt">flux</span> measurement and fractionation</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Evans, William C.; Sorey, M.L.; Kennedy, B.M.; Stonestrom, David A.; Rogie, J.D.; Shuster, D.L.</p> <p>2001-01-01</p> <p>Diffuse emissions of <span class="hlt">CO</span><span class="hlt">2</span> are known to be large around some volcanoes and hydrothermal areas. Accumulation-chamber measurements of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> are increasingly used to estimate the total magmatic or metamorphic <span class="hlt">CO</span><span class="hlt">2</span> released from such areas. To assess the performance of accumulation chamber systems at <span class="hlt">fluxes</span> one to three orders of magnitude higher than normally encountered in soil respiration studies, a test system was constructed in the laboratory where known <span class="hlt">fluxes</span> could be maintained through dry sand. Steady-state gas concentration profiles and fractionation effects observed in the 30-cm sand column nearly match those predicted by the Stefan-Maxwell equations, indicating that the test system was functioning successfully as a uniform porous medium. Eight groups of investigators tested their accumulation chamber equipment, all configured with continuous infrared gas analyzers (IRGA), in this system. Over a <span class="hlt">flux</span> range of ~ 200-12,000 g m-<span class="hlt">2</span> day-1, 90% of their 203 <span class="hlt">flux</span> measurements were 0-25% lower than the imposed <span class="hlt">flux</span> with a mean difference of - 12.5%. Although this difference would seem to be within the range of acceptability for many geologic investigations, some potential sources for larger errors were discovered. A steady-state pressure gradient of -20 Pa/m was measured in the sand column at a <span class="hlt">flux</span> of 11,200 g m-<span class="hlt">2</span> day-1. The derived permeability (50 darcies) was used in the dusty-gas model (DGM) of transport to quantify various diffusive and viscous <span class="hlt">flux</span> components. These calculations were used to demonstrate that accumulation chambers, in addition to reducing the underlying diffusive gradient, severely disrupt the steady-state pressure gradient. The resultant diversion of the net gas flow is probably responsible for the systematically low <span class="hlt">flux</span> measurements. It was also shown that the fractionating effects of a viscous <span class="hlt">CO</span><span class="hlt">2</span> efflux against a diffusive influx of <span class="hlt">air</span> will have a major impact on some important geochemical indicators, such as N<span class="hlt">2</span>/Ar, ??15N-N<span class="hlt">2</span>, and 4He/22</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120004203','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120004203"><span>The <span class="hlt">SeaFlux</span> Turbulent <span class="hlt">Flux</span> Dataset Version 1.0 Documentation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Clayson, Carol Anne; Roberts, J. Brent; Bogdanoff, Alec S.</p> <p>2012-01-01</p> <p>Under the auspices of the World Climate Research Programme (WCRP) Global Energy and Water cycle EXperiment (GEWEX) Data and Assessment Panel (GDAP), the <span class="hlt">SeaFlux</span> Project was created to investigate producing a high-resolution satellite-based dataset of surface turbulent <span class="hlt">fluxes</span> over the global oceans. The most current release of the <span class="hlt">SeaFlux</span> product is Version 1.0; this represents the initial release of turbulent surface heat <span class="hlt">fluxes</span>, associated near-surface variables including a diurnally varying <span class="hlt">sea</span> surface temperature.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A14G..06A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A14G..06A"><span>Studying emissions of <span class="hlt">CO</span><span class="hlt">2</span> in the Baltimore/Washington area using airborne measurements: source attribution, <span class="hlt">flux</span> quantification, and model comparison</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ahn, D.; Hansford, J. R.; Salawitch, R. J.; Ren, X.; Cohen, M.; Karion, A.; Whetstone, J. R.; Salmon, O. E.; Shepson, P. B.; Gurney, K. R.; Osterman, G. B.; Dickerson, R. R.</p> <p>2017-12-01</p> <p>We study emissions of <span class="hlt">CO</span><span class="hlt">2</span> in the Baltimore-Washington area using airborne in-situ measurements, obtained during the February 2015 <span class="hlt">Fluxes</span> of Greenhouse Gases in Maryland (FLAGG-MD) campaign. In this study, we attributed enhanced signals of <span class="hlt">CO</span><span class="hlt">2</span> to several power plants and two urban areas (Baltimore City and Washington, DC), using the NOAA HYSPLIT <span class="hlt">air</span> parcel trajectory model as well as the analysis of chemical ratios to quantify the source/receptor relationship. Then, the <span class="hlt">fluxes</span> of attributed <span class="hlt">CO</span><span class="hlt">2</span> are estimated using a mass balance approach. The uncertainty in the aircraft-based mass balance approach is estimated by conducting a detailed sensitivity analysis of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>, considering factors such as the background mixing ratio of <span class="hlt">CO</span><span class="hlt">2</span>, wind direction and speed, PBL heights, the horizontal boundary, and vertical interpolation methods. Estimated <span class="hlt">fluxes</span> of <span class="hlt">CO</span><span class="hlt">2</span> with estimated uncertainty ranges are then compared to output from various emissions data and models, such as CEMS, CarbonTracker, FFDAS, and ODIAC. Finally, column <span class="hlt">CO</span><span class="hlt">2</span> data over the Baltimore-Washington region observed by the OCO-<span class="hlt">2</span> satellite instrument are statistically compared to aircraft in-situ observations, to assess how well OCO-<span class="hlt">2</span> is able to quantify geographic and synoptic-scale variability.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20110011454&hterms=Koch&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DKoch','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20110011454&hterms=Koch&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DKoch"><span>Can <span class="hlt">CO</span><span class="hlt">2</span> Turbulent <span class="hlt">Flux</span> Be Measured by Lidar? A Preliminary Study</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gilbert, Fabien; Koch, Grady; Beyon, Jeffrey Y.; Hilton, Timothy W.; Davis, Kenneth J.; Andrews, Arlyn; Flamant, Pierre H.; Singh, Upendra N.</p> <p>2011-01-01</p> <p>The vertical profiling of<span class="hlt">CO</span><span class="hlt">2</span> turbulent <span class="hlt">fluxes</span> in the atmospheric boundary layer (ABL) is investigated using a coherent differential absorption lidar (CDIAL) operated nearby a tall tower in Wisconsin during June 2007. A CDIAL can perform simultaneous range-resolved <span class="hlt">CO</span><span class="hlt">2</span> DIAL and velocity measurements. The lidar eddy covariance technique is presented. The aims of the study are (i) an assessment of performance and current limitation of available CDIAL for <span class="hlt">CO</span><span class="hlt">2</span> turbulent <span class="hlt">fluxes</span> and (ii) the derivation of instrument specifications to build a future CDIAL to perform accurate range-resolved <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. Experimental lidar <span class="hlt">CO</span><span class="hlt">2</span> mixing ratio and vertical velocity profiles are successfully compared with in situ sensors measurements. Time and space integral scales of turbulence in the ABL are addressed that result in limitation for time averaging and range accumulation. A first attempt to infer <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> using an eddy covariance technique with currently available <span class="hlt">2</span>-mm CDIAL dataset is reported.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003AGUFMGC31B0184C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003AGUFMGC31B0184C"><span>Carbon Dioxide and Water Vapor <span class="hlt">Fluxes</span> at Reduced and Elevated <span class="hlt">CO</span><span class="hlt">2</span> Concentrations in Southern California Chaparral</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cheng, Y.; Oechel, W. C.; Hastings, S. J.; Bryant, P. J.; Qian, Y.</p> <p>2003-12-01</p> <p>This research took two different approaches to measuring carbon and water vapor <span class="hlt">fluxes</span> at the plot level (<span class="hlt">2</span> x <span class="hlt">2</span> meter and 1 x 1 meter plots) to help understand and predict ecosystem responses to elevated <span class="hlt">CO</span><span class="hlt">2</span> concentrations and concomitant environmental changes. The first measurement approach utilized a <span class="hlt">CO</span><span class="hlt">2</span>-controlled, ambient lit, temperature controlled (<span class="hlt">CO</span><span class="hlt">2</span>LT) null-balance chamber system run in a chaparral ecosystem in southern California, with six different <span class="hlt">CO</span><span class="hlt">2</span> concentrations ranging from 250 to 750 ppm <span class="hlt">CO</span><span class="hlt">2</span> concentrations with 100 ppm difference between treatments. The second measurement approach used a free <span class="hlt">air</span> <span class="hlt">CO</span><span class="hlt">2</span> enrichment (FACE) system operated at 550 ppm <span class="hlt">CO</span><span class="hlt">2</span> concentration. These manipulations allowed the study of responses of naturally-growing chaparral to varying levels of <span class="hlt">CO</span><span class="hlt">2</span>, under both chamber and open <span class="hlt">air</span> conditions. There was a statistically significant <span class="hlt">CO</span><span class="hlt">2</span> effect on annual NEE (net ecosystem exchange) during the period of this study, 1997 to 2000. The effects of elevated <span class="hlt">CO</span><span class="hlt">2</span> on <span class="hlt">CO</span><span class="hlt">2</span> and water vapor <span class="hlt">flux</span> showed strong seasonal patterns. Elevated <span class="hlt">CO</span><span class="hlt">2</span> delayed the development of water stress, enhanced leaf-level photosynthesis, and decreased transpiration and conductance rates. These effects were observed regardless of water availability. Ecosystem <span class="hlt">CO</span><span class="hlt">2</span> sink strength and plant water status were significantly enhanced by elevated <span class="hlt">CO</span><span class="hlt">2</span> when water availability was restricted. Comparing the FACE treatment and the FACE control, the ecosystem was either a stronger sink or a weaker source to the atmosphere throughout the dry seasons, but there was no statistically significant difference during the wet seasons. Annual average leaf transpiration decreased with the increasing of the atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentration. Although leaf level water-use efficiency (WUE) increased with the growth <span class="hlt">CO</span><span class="hlt">2</span> concentration increase, annual evapotranspiration (ET) during these four years also increased with the increase of the atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentrations. These results indicate that</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_11 --> <div id="page_12" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="221"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/42020','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/42020"><span>Seasonal soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> under big sagebrush (Artemisia tridentata Nutt.)</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Michael C. Amacher; Cheryl L. Mackowiak</p> <p>2011-01-01</p> <p>Soil respiration is a major contributor to atmospheric <span class="hlt">CO</span><span class="hlt">2</span>, but accurate landscape-scale estimates of soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> for many ecosystems including shrublands have yet to be established. We began a project to measure, with high spatial and temporal resolution, soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> in a stand (11 x 25 m area) of big sagebrush (Artemisia tridentata Nutt.) at the Logan, Utah,...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.A41B0088V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.A41B0088V"><span><span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> from a tropical neighborhood: sources and sinks</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Velasco, E.; Roth, M.; Tan, S.; Quak, M.; Britter, R.; Norford, L.</p> <p>2011-12-01</p> <p>Cities are the main contributors to the <span class="hlt">CO</span><span class="hlt">2</span> rise in the atmosphere. The <span class="hlt">CO</span><span class="hlt">2</span> released from the various emission sources is typically quantified by a bottom-up aggregation process that accounts for emission factors and fossil fuel consumption data. This approach does not consider the heterogeneity and variability of the urban emission sources, and error propagation can result in large uncertainties. In this context, direct measurements of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> that include all major and minor anthropogenic and natural sources and sinks from a specific district can be used to evaluate emission inventories. This study reports and compares <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> measured directly using the eddy covariance method with emissions estimated by emissions factors and activity data for a residential neighborhood of Singapore, a highly populated and urbanized tropical city. The <span class="hlt">flux</span> measurements were conducted during one year. No seasonal variability was found as a consequence of the constant climate conditions of tropical places; but a clear diurnal pattern with morning and late afternoon peaks in phase with the rush-hour traffic was observed. The magnitude of the <span class="hlt">fluxes</span> throughout daylight hours is modulated by the urban vegetation, which is abundant in terms of biomass but not of land-cover (15%). Even though the carbon uptake by vegetation is significant, it does not exceed the anthropogenic emissions and the monitored district is a net <span class="hlt">CO</span><span class="hlt">2</span> source of 20.3 ton km-<span class="hlt">2</span> day-1 on average. The carbon uptake by vegetation is investigated as the difference between the estimated emissions and the measured <span class="hlt">fluxes</span> during daytime.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.B51D0296M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.B51D0296M"><span>Microbial imprint on soil-atmosphere H<span class="hlt">2</span>, COS, and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Meredith, L. K.; Commane, R.; Munger, J. W.; Wofsy, S. C.; Prinn, R. G.</p> <p>2013-12-01</p> <p>Microorganisms drive large trace gas <span class="hlt">fluxes</span> between soil and atmosphere, but the signal can be difficult to detect and quantify in the presence of stronger exchange processes in an ecosystem. Partitioning methods are often needed to estimate trace gas budgets and to develop process-based models to explore the sensitivity of microbe-mediated <span class="hlt">fluxes</span>. In this study, we test the performance of trace gases with predominantly microbe-mediated soil <span class="hlt">fluxes</span> as a metric of the soil microbial uptake activity of other trace gases. Using simultaneous, collocated measurements at Harvard Forest, we consider three trace gases with microbe-mediated soil <span class="hlt">fluxes</span> of various importance relative to their other (mainly plant-mediated) ecosystem <span class="hlt">fluxes</span>: molecular hydrogen (H<span class="hlt">2</span>), carbonyl sulfide (COS), and carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>). These gases probe different aspects of the soil trace-gas microbiology. Soil H<span class="hlt">2</span> uptake is a redox reaction driving the energy metabolism of a portion of the microbial community, while soil <span class="hlt">CO</span><span class="hlt">2</span> respiration is a partial proxy for the overall soil microbial metabolism. In comparison, very little is understood about the microbiological and environmental drivers of soil COS uptake and emissions. In this study, we find that H<span class="hlt">2</span>, COS, and <span class="hlt">CO</span><span class="hlt">2</span> soil uptake rates are often correlated, but the relative soil uptake between gases is not constant, and is influenced by seasonality and local environmental conditions. We also consider how differences in the microbial communities and pathways involved in the soil <span class="hlt">fluxes</span> may explain differences in the observations. Our results are important for informing previous studies using tracer approaches. For example, H<span class="hlt">2</span> has been used to estimate COS soil uptake, which must be accounted for to use COS as a carbon cycle tracer. Furthermore, the global distribution of H<span class="hlt">2</span> deposition velocity has been inferred from net primary productivity (<span class="hlt">CO</span><span class="hlt">2</span>). Given that insufficient measurement frequency and spatial distribution exists to partition global net</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006TellB..58...73W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006TellB..58...73W"><span>The role of Southern Ocean mixing and upwelling in glacial-interglacial atmospheric <span class="hlt">CO</span><span class="hlt">2</span> change</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Watson, Andrew J.; Naveira Garabato, Alberto C.</p> <p>2006-02-01</p> <p>Decreased ventilation of the Southern Ocean in glacial time is implicated in most explanations of lower glacial atmospheric <span class="hlt">CO</span><span class="hlt">2</span>. Today, the deep (>2000 m) ocean south of the Polar Front is rapidly ventilated from below, with the interaction of deep currents with topography driving high mixing rates well up into the water column. We show from a buoyancy budget that mixing rates are high in all the deep waters of the Southern Ocean. Between the surface and ~2000 m depth, water is upwelled by a residual meridional overturning that is directly linked to buoyancy <span class="hlt">fluxes</span> through the ocean surface. Combined with the rapid deep mixing, this upwelling serves to return deep water to the surface on a short time scale. We propose two new mechanisms by which, in glacial time, the deep Southern Ocean may have been more isolated from the surface. Firstly, the deep ocean appears to have been more stratified because of denser bottom water resulting from intense <span class="hlt">sea</span> ice formation near Antarctica. The greater stratification would have slowed the deep mixing. Secondly, subzero atmospheric temperatures may have meant that the present-day buoyancy <span class="hlt">flux</span> from the atmosphere to the ocean surface was reduced or reversed. This in turn would have reduced or eliminated the upwelling (contrary to a common assumption, upwelling is not solely a function of the wind stress but is coupled to the <span class="hlt">air-sea</span> buoyancy <span class="hlt">flux</span> too). The observed very close link between Antarctic temperatures and atmospheric <span class="hlt">CO</span><span class="hlt">2</span> could then be explained as a natural consequence of the connection between the <span class="hlt">air-sea</span> buoyancy <span class="hlt">flux</span> and upwelling in the Southern Ocean, if slower ventilation of the Southern Ocean led to lower atmospheric <span class="hlt">CO</span><span class="hlt">2</span>. Here we use a box model, similar to those of previous authors, to show that weaker mixing and reduced upwelling in the Southern Ocean can explain the low glacial atmospheric <span class="hlt">CO</span><span class="hlt">2</span> in such a formulation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRG..122.3238C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRG..122.3238C"><span>Grain Yield Observations Constrain Cropland <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Fluxes</span> Over Europe</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Combe, M.; de Wit, A. J. W.; Vilà-Guerau de Arellano, J.; van der Molen, M. K.; Magliulo, V.; Peters, W.</p> <p>2017-12-01</p> <p>Carbon exchange over croplands plays an important role in the European carbon cycle over daily to seasonal time scales. A better description of this exchange in terrestrial biosphere models—most of which currently treat crops as unmanaged grasslands—is needed to improve atmospheric <span class="hlt">CO</span><span class="hlt">2</span> simulations. In the framework we present here, we model gross European cropland <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> with a crop growth model constrained by grain yield observations. Our approach follows a two-step procedure. In the first step, we calculate day-to-day crop carbon <span class="hlt">fluxes</span> and pools with the WOrld FOod STudies (WOFOST) model. A scaling factor of crop growth is optimized regionally by minimizing the final grain carbon pool difference to crop yield observations from the Statistical Office of the European Union. In a second step, we re-run our WOFOST model for the full European 25 × 25 km gridded domain using the optimized scaling factors. We combine our optimized crop <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> with a simple soil respiration model to obtain the net cropland <span class="hlt">CO</span><span class="hlt">2</span> exchange. We assess our model's ability to represent cropland <span class="hlt">CO</span><span class="hlt">2</span> exchange using 40 years of observations at seven European <span class="hlt">Flux</span>Net sites and compare it with carbon <span class="hlt">fluxes</span> produced by a typical terrestrial biosphere model. We conclude that our new model framework provides a more realistic and strongly observation-driven estimate of carbon exchange over European croplands. Its products will be made available to the scientific community through the ICOS Carbon Portal and serve as a new cropland component in the CarbonTracker Europe inverse model.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21141036','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21141036"><span>Advances in quantifying <span class="hlt">air-sea</span> gas exchange and environmental forcing.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wanninkhof, Rik; Asher, William E; Ho, David T; Sweeney, Colm; McGillis, Wade R</p> <p>2009-01-01</p> <p>The past decade has seen a substantial amount of research on <span class="hlt">air-sea</span> gas exchange and its environmental controls. These studies have significantly advanced the understanding of processes that control gas transfer, led to higher quality field measurements, and improved estimates of the <span class="hlt">flux</span> of climate-relevant gases between the ocean and atmosphere. This review discusses the fundamental principles of <span class="hlt">air-sea</span> gas transfer and recent developments in gas transfer theory, parameterizations, and measurement techniques in the context of the exchange of carbon dioxide. However, much of this discussion is applicable to any sparingly soluble, non-reactive gas. We show how the use of global variables of environmental forcing that have recently become available and gas exchange relationships that incorporate the main forcing factors will lead to improved estimates of global and regional <span class="hlt">air-sea</span> gas <span class="hlt">fluxes</span> based on better fundamental physical, chemical, and biological foundations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23712111','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23712111"><span>Dynamics of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> and environmental responses in the rain-fed winter wheat ecosystem of the Loess Plateau, China.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Wen; Liao, Yuncheng; Wen, Xiaoxia; Guo, Qiang</p> <p>2013-09-01</p> <p>Chinese Loess Plateau plays an important role in carbon balance of terrestrial ecosystems. Continuous measurement of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in cropland ecosystem is of great significance to accurately evaluate the carbon sequestration potential and to better explain the carbon cycle process in this region. By using the eddy covariance system we conducted a long-term (from Sep 2009 to Jun 2010) <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> measurement in the rain-fed winter wheat field of the Chinese Loess Plateau and elaborated the responses of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> to environmental factors. The results show that the winter wheat ecosystem has distinct seasonal dynamics of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. The total net ecosystem <span class="hlt">CO</span><span class="hlt">2</span> exchange (NEE) of -218.9±11.5 gC m(-<span class="hlt">2</span>) in the growing season, however, after considering the harvested grain, the agro-ecosystem turned into a weak carbon sink (-36.<span class="hlt">2</span> gC m(-<span class="hlt">2</span>)). On the other hand, the responses of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> to environmental factors depended on different growth stages of winter wheat and different ranges of environmental variables, suggesting that the variations in <span class="hlt">CO</span><span class="hlt">2</span> exchange were sensitive to the changes in controlling factors. Particularly, we found the pulse response of ecosystem respiration (Reco) to a large rainfall event, and the strong fluctuations of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> usually appeared after effective rainfall events (daily precipitation > 5 mm) during middle growing season. Such phenomenon also occurred in the case of the drastic changes in <span class="hlt">air</span> temperature and within 5 days after field management (e.g. tillage and plough). Copyright © 2013 The Authors. Published by Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PolSc..13...13Q','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PolSc..13...13Q"><span>Dimethylsulfide model calibration and parametric sensitivity analysis for the Greenland <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Qu, Bo; Gabric, Albert J.; Zeng, Meifang; Xi, Jiaojiao; Jiang, Limei; Zhao, Li</p> <p>2017-09-01</p> <p><span class="hlt">Sea-to-air</span> <span class="hlt">fluxes</span> of marine biogenic aerosols have the potential to modify cloud microphysics and regional radiative budgets, and thus moderate Earth's warming. Polar regions play a critical role in the evolution of global climate. In this work, we use a well-established biogeochemical model to simulate the DMS <span class="hlt">flux</span> from the Greenland <span class="hlt">Sea</span> (20°W-10°E and 70°N-80°N) for the period 2003-2004. Parameter sensitivity analysis is employed to identify the most sensitive parameters in the model. A genetic algorithm (GA) technique is used for DMS model parameter calibration. Data from phase 5 of the Coupled Model Intercomparison Project (CMIP5) are used to drive the DMS model under 4 × <span class="hlt">CO</span><span class="hlt">2</span> conditions. DMS <span class="hlt">flux</span> under quadrupled <span class="hlt">CO</span><span class="hlt">2</span> levels increases more than 300% compared with late 20th century levels (1 × <span class="hlt">CO</span><span class="hlt">2</span>). Reasons for the increase in DMS <span class="hlt">flux</span> include changes in the ocean state-namely an increase in <span class="hlt">sea</span> surface temperature (SST) and loss of <span class="hlt">sea</span> ice-and an increase in DMS transfer velocity, especially in spring and summer. Such a large increase in DMS <span class="hlt">flux</span> could slow the rate of warming in the Arctic via radiative budget changes associated with DMS-derived aerosols.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20180002067','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20180002067"><span>The Impact of Prior Biosphere Models in the Inversion of Global Terrestrial <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Fluxes</span> by Assimilating OCO-<span class="hlt">2</span> Retrievals</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Philip, Sajeev; Johnson, Matthew S.</p> <p>2018-01-01</p> <p>Atmospheric mixing ratios of carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) are largely controlled by anthropogenic emissions and biospheric <span class="hlt">fluxes</span>. The processes controlling terrestrial biosphere-atmosphere carbon exchange are currently not fully understood, resulting in terrestrial biospheric models having significant differences in the quantification of biospheric <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. Atmospheric transport models assimilating measured (in situ or space-borne) <span class="hlt">CO</span><span class="hlt">2</span> concentrations to estimate "top-down" <span class="hlt">fluxes</span>, generally use these biospheric <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> as a priori information. Most of the <span class="hlt">flux</span> inversion estimates result in substantially different spatio-temporal posteriori estimates of regional and global biospheric <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. The Orbiting Carbon Observatory <span class="hlt">2</span> (OCO-<span class="hlt">2</span>) satellite mission dedicated to accurately measure column <span class="hlt">CO</span><span class="hlt">2</span> (XCO<span class="hlt">2</span>) allows for an improved understanding of global biospheric <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. OCO-<span class="hlt">2</span> provides much-needed <span class="hlt">CO</span><span class="hlt">2</span> observations in data-limited regions facilitating better global and regional estimates of "top-down" <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> through inversion model simulations. The specific objectives of our research are to: 1) conduct GEOS-Chem 4D-Var assimilation of OCO-<span class="hlt">2</span> observations, using several state-of-the-science biospheric <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> models as a priori information, to better constrain terrestrial <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>, and <span class="hlt">2</span>) quantify the impact of different biospheric model prior <span class="hlt">fluxes</span> on OCO-<span class="hlt">2</span>-assimilated a posteriori <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> estimates. Here we present our assessment of the importance of these a priori <span class="hlt">fluxes</span> by conducting Observing System Simulation Experiments (OSSE) using simulated OCO-<span class="hlt">2</span> observations with known "true" <span class="hlt">fluxes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A43C2466P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A43C2466P"><span>Assessing the Importance of Prior Biospheric <span class="hlt">Fluxes</span> on Inverse Model Estimates of <span class="hlt">CO</span><span class="hlt">2</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Philip, S.; Johnson, M. S.; Potter, C. S.; Genovese, V. B.</p> <p>2017-12-01</p> <p>Atmospheric mixing ratios of carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) are largely controlled by anthropogenic emissions and biospheric sources/sinks. The processes controlling terrestrial biosphere-atmosphere carbon exchange are currently not fully understood, resulting in models having significant differences in the quantification of biospheric <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. Currently, atmospheric chemical transport models (CTM) and global climate models (GCM) use multiple different biospheric <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> models resulting in large differences in simulating the global carbon cycle. The Orbiting Carbon Observatory <span class="hlt">2</span> (OCO-<span class="hlt">2</span>) satellite mission was designed to allow for the improved understanding of the processes involved in the exchange of carbon between terrestrial ecosystems and the atmosphere, and therefore allowing for more accurate assessment of the seasonal/inter-annual variability of <span class="hlt">CO</span><span class="hlt">2</span>. OCO-<span class="hlt">2</span> provides much-needed <span class="hlt">CO</span><span class="hlt">2</span> observations in data-limited regions allowing for the evaluation of model simulations of greenhouse gases (GHG) and facilitating global/regional estimates of "top-down" <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. We conduct a 4-D Variation (4D-Var) data assimilation with the GEOS-Chem (Goddard Earth Observation System-Chemistry) CTM using 1) OCO-<span class="hlt">2</span> land nadir and land glint retrievals and <span class="hlt">2</span>) global in situ surface flask observations to constrain biospheric <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. We apply different state-of-the-science year-specific <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> models (e.g., NASA-CASA (NASA-Carnegie Ames Stanford Approach), CASA-GFED (Global Fire Emissions Database), Simple Biosphere Model version 4 (SiB-4), and LPJ (Lund-Postdam-Jena)) to assess the impact of "a priori" <span class="hlt">flux</span> predictions to "a posteriori" estimates. We will present the "top-down" <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> estimates for the year 2015 using OCO-<span class="hlt">2</span> and in situ observations, and a complete indirect evaluation of the a priori and a posteriori <span class="hlt">flux</span> estimates using independent in situ observations. We will also present our assessment of the variability of "top-down" <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> estimates when using different</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.B22E..06O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.B22E..06O"><span>Progress Toward Measuring <span class="hlt">CO</span><span class="hlt">2</span> Isotopologue <span class="hlt">Fluxes</span> <em>in situ</em> with the LLNL Miniature, Laser-based <span class="hlt">CO</span><span class="hlt">2</span> Sensor</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Osuna, J. L.; Bora, M.; Bond, T.</p> <p>2015-12-01</p> <p>One method to constrain photosynthesis and respiration independently at the ecosystem scale is to measure the <span class="hlt">fluxes</span> of <span class="hlt">CO</span><span class="hlt">2</span>­ isotopologues. Instrumentation is currently available to makes these measurements but they are generally costly, large, bench-top instruments. Here, we present progress toward developing a laser-based sensor that can be deployed directly to a canopy to passively measure <span class="hlt">CO</span><span class="hlt">2</span> isotopologue <span class="hlt">fluxes</span>. In this study, we perform initial proof-of-concept and sensor characterization tests in the laboratory and in the field to demonstrate performance of the Lawrence Livermore National Laboratory (LLNL) tunable diode laser <span class="hlt">flux</span> sensor. The results shown herein demonstrate measurement of bulk <span class="hlt">CO</span><span class="hlt">2</span> as a first step toward achieving <span class="hlt">flux</span> measurements of <span class="hlt">CO</span><span class="hlt">2</span> isotopologues. The sensor uses a Vertical Cavity Surface Emitting Laser (VCSEL) in the 2012 nm range. The laser is mounted in a multi-pass White Cell. In order to amplify the absorption signal of <span class="hlt">CO</span><span class="hlt">2</span> in this range we employ wave modulation spectroscopy, introducing an alternating current (AC) bias component where f is the frequency of modulation on the laser drive current in addition to the direct current (DC) emission scanning component. We observed a strong linear relationship (r<span class="hlt">2</span> = 0.998 and r<span class="hlt">2</span> = 0.978 at all and low <span class="hlt">CO</span><span class="hlt">2</span> concentrations, respectively) between the <span class="hlt">2</span>f signal and the <span class="hlt">CO</span><span class="hlt">2</span> concentration in the cell across the range of <span class="hlt">CO</span><span class="hlt">2</span> concentrations relevant for <span class="hlt">flux</span> measurements. We use this calibration to interpret <span class="hlt">CO</span><span class="hlt">2</span> concentration of a gas flowing through the White cell in the laboratory and deployed over a grassy field. We will discuss sensor performance in the lab and in situ as well as address steps toward achieving canopy-deployed, passive measurements of <span class="hlt">CO</span><span class="hlt">2</span> isotopologue <span class="hlt">fluxes</span>. This work performed under the auspices of the U.S. Department of Energy by Lawrence Livermore National Laboratory under Contract DE-AC52-07NA27344. LLNL-ABS-675788</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006JESS..115..461N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006JESS..115..461N"><span>Monsoon control on trace metal <span class="hlt">fluxes</span> in the deep Arabian <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nair, T. M. Balakrishnan</p> <p>2006-08-01</p> <p>Particulate <span class="hlt">fluxes</span> of aluminium, iron, magnesium and titanium were measured using six time-series sediment traps deployed in the eastern, central and western Arabian <span class="hlt">Sea</span>. Annual Al <span class="hlt">fluxes</span> at shallow and deep trap depths were 0.47 and 0.46 g m-<span class="hlt">2</span> in the western Arabian <span class="hlt">Sea</span>, and 0.33 and 0.47 g m-<span class="hlt">2</span> in the eastern Arabian <span class="hlt">Sea</span>. There is a difference of about 0.9-1.8 g m-<span class="hlt">2</span>y-1 in the lithogenic <span class="hlt">fluxes</span> determined analytically (residue remaining after leaching out all biogenic particles) and estimated from the Al <span class="hlt">fluxes</span> in the western Arabian <span class="hlt">Sea</span>. This arises due to higher <span class="hlt">fluxes</span> of Mg (as dolomite) in the western Arabian <span class="hlt">Sea</span> (6-11 times higher than the eastern Arabian <span class="hlt">Sea</span>). The estimated dolomite <span class="hlt">fluxes</span> at the western Arabian <span class="hlt">Sea</span> site range from 0.9 to 1.35gm-<span class="hlt">2</span>y-1. Fe <span class="hlt">fluxes</span> in the Arabian <span class="hlt">Sea</span> were less than that of the reported atmospheric <span class="hlt">fluxes</span> without any evidence for the presence of labile fraction/excess of Fe in the settling particles. More than 75% of Al, Fe, Ti and Mg <span class="hlt">fluxes</span> occurred during the southwest (SW) monsoon in the western Arabian <span class="hlt">Sea</span>. In the eastern Arabian <span class="hlt">Sea</span>, peak Al, Fe, Mg and Ti <span class="hlt">fluxes</span> were recorded during both the northeast (NE) and SW monsoons. During the SW monsoon, there exists a time lag of around one month between the increases in lithogenic and dolomite <span class="hlt">fluxes</span>. Total lithogenic <span class="hlt">fluxes</span> increase when the southern branch of dust bearing northwesterlies is dragged by the SW monsoon winds to the trap locations. However, the dolomite <span class="hlt">fluxes</span> increase only when the northern branch of the northwesterlies (which carries a huge amount of dolomite accounting 60% of the total dust load) is dragged, from further north, by SW monsoon winds. The potential for the use of Mg/Fe ratio as a paleo-monsoonal proxy is examined.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015BGeo...12.7251R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015BGeo...12.7251R"><span>Data-based estimates of the ocean carbon sink variability - first results of the Surface Ocean p<span class="hlt">CO</span><span class="hlt">2</span> Mapping intercomparison (SOCOM)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rödenbeck, C.; Bakker, D. C. E.; Gruber, N.; Iida, Y.; Jacobson, A. R.; Jones, S.; Landschützer, P.; Metzl, N.; Nakaoka, S.; Olsen, A.; Park, G.-H.; Peylin, P.; Rodgers, K. B.; Sasse, T. P.; Schuster, U.; Shutler, J. D.; Valsala, V.; Wanninkhof, R.; Zeng, J.</p> <p>2015-12-01</p> <p>Using measurements of the surface-ocean <span class="hlt">CO</span><span class="hlt">2</span> partial pressure (p<span class="hlt">CO</span><span class="hlt">2</span>) and 14 different p<span class="hlt">CO</span><span class="hlt">2</span> mapping methods recently collated by the Surface Ocean p<span class="hlt">CO</span><span class="hlt">2</span> Mapping intercomparison (SOCOM) initiative, variations in regional and global <span class="hlt">sea-air</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> are investigated. Though the available mapping methods use widely different approaches, we find relatively consistent estimates of regional p<span class="hlt">CO</span><span class="hlt">2</span> seasonality, in line with previous estimates. In terms of interannual variability (IAV), all mapping methods estimate the largest variations to occur in the eastern equatorial Pacific. Despite considerable spread in the detailed variations, mapping methods that fit the data more closely also tend to agree more closely with each other in regional averages. Encouragingly, this includes mapping methods belonging to complementary types - taking variability either directly from the p<span class="hlt">CO</span><span class="hlt">2</span> data or indirectly from driver data via regression. From a weighted ensemble average, we find an IAV amplitude of the global <span class="hlt">sea-air</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> of 0.31 PgC yr-1 (standard deviation over 1992-2009), which is larger than simulated by biogeochemical process models. From a decadal perspective, the global ocean <span class="hlt">CO</span><span class="hlt">2</span> uptake is estimated to have gradually increased since about 2000, with little decadal change prior to that. The weighted mean net global ocean <span class="hlt">CO</span><span class="hlt">2</span> sink estimated by the SOCOM ensemble is -1.75 PgC yr-1 (1992-2009), consistent within uncertainties with estimates from ocean-interior carbon data or atmospheric oxygen trends.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015BGD....1214049R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015BGD....1214049R"><span>Data-based estimates of the ocean carbon sink variability - first results of the Surface Ocean p<span class="hlt">CO</span><span class="hlt">2</span> Mapping intercomparison (SOCOM)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rödenbeck, C.; Bakker, D. C. E.; Gruber, N.; Iida, Y.; Jacobson, A. R.; Jones, S.; Landschützer, P.; Metzl, N.; Nakaoka, S.; Olsen, A.; Park, G.-H.; Peylin, P.; Rodgers, K. B.; Sasse, T. P.; Schuster, U.; Shutler, J. D.; Valsala, V.; Wanninkhof, R.; Zeng, J.</p> <p>2015-08-01</p> <p>Using measurements of the surface-ocean <span class="hlt">CO</span><span class="hlt">2</span> partial pressure (p<span class="hlt">CO</span><span class="hlt">2</span>) and 14 different p<span class="hlt">CO</span><span class="hlt">2</span> mapping methods recently collated by the Surface Ocean p<span class="hlt">CO</span><span class="hlt">2</span> Mapping intercomparison (SOCOM) initiative, variations in regional and global <span class="hlt">sea-air</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> have been investigated. Though the available mapping methods use widely different approaches, we find relatively consistent estimates of regional p<span class="hlt">CO</span><span class="hlt">2</span> seasonality, in line with previous estimates. In terms of interannual variability (IAV), all mapping methods estimate the largest variations to occur in the Eastern equatorial Pacific. Despite considerable spead in the detailed variations, mapping methods with closer match to the data also tend to be more consistent with each other. Encouragingly, this includes mapping methods belonging to complementary types - taking variability either directly from the p<span class="hlt">CO</span><span class="hlt">2</span> data or indirectly from driver data via regression. From a weighted ensemble average, we find an IAV amplitude of the global <span class="hlt">sea-air</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> of 0.31 PgC yr-1 (standard deviation over 1992-2009), which is larger than simulated by biogeochemical process models. On a decadal perspective, the global <span class="hlt">CO</span><span class="hlt">2</span> uptake is estimated to have gradually increased since about 2000, with little decadal change prior to 2000. The weighted mean total ocean <span class="hlt">CO</span><span class="hlt">2</span> sink estimated by the SOCOM ensemble is consistent within uncertainties with estimates from ocean-interior carbon data or atmospheric oxygen trends.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017SolE....8.1017Q','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017SolE....8.1017Q"><span>Increasing <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> at Pisciarelli, Campi Flegrei, Italy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Queißer, Manuel; Granieri, Domenico; Burton, Mike; Arzilli, Fabio; Avino, Rosario; Carandente, Antonio</p> <p>2017-09-01</p> <p>The Campi Flegrei caldera is located in the metropolitan area of Naples (Italy) and has been undergoing different stages of unrest since 1950, evidenced by episodes of significant ground uplift followed by minor subsidence, increasing and fluctuating emission strengths of water vapor and <span class="hlt">CO</span><span class="hlt">2</span> from fumaroles, and periodic seismic crises. We deployed a scanning laser remote-sensing spectrometer (LARSS) that measured path-integrated <span class="hlt">CO</span><span class="hlt">2</span> concentrations in the Pisciarelli area in May 2017. The resulting mean <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> is 578 ± 246 t d-1. Our data suggest a significant increase in <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> at this site since 2015. Together with recent geophysical observations, this suggests a greater contribution of the magmatic source to the degassing and/or an increase in permeability at shallow levels. Thanks to the integrated path soundings, LARSS may help to give representative measurements from large regions containing different <span class="hlt">CO</span><span class="hlt">2</span> sources, including fumaroles, low-temperature vents, and degassing soils, helping to constrain the contribution of deep gases and their migration mechanisms towards the surface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3690887','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3690887"><span>Direct electrolytic dissolution of silicate minerals for <span class="hlt">air</span> <span class="hlt">CO</span><span class="hlt">2</span> mitigation and carbon-negative H<span class="hlt">2</span> production</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Rau, Greg H.; Carroll, Susan A.; Bourcier, William L.; Singleton, Michael J.; Smith, Megan M.; Aines, Roger D.</p> <p>2013-01-01</p> <p>We experimentally demonstrate the direct coupling of silicate mineral dissolution with saline water electrolysis and H<span class="hlt">2</span> production to effect significant <span class="hlt">air</span> <span class="hlt">CO</span><span class="hlt">2</span> absorption, chemical conversion, and storage in solution. In particular, we observed as much as a 105-fold increase in OH− concentration (pH increase of up to 5.3 units) relative to experimental controls following the electrolysis of 0.25 M Na<span class="hlt">2</span>SO4 solutions when the anode was encased in powdered silicate mineral, either wollastonite or an ultramafic mineral. After electrolysis, full equilibration of the alkalized solution with <span class="hlt">air</span> led to a significant pH reduction and as much as a 45-fold increase in dissolved inorganic carbon concentration. This demonstrated significant spontaneous <span class="hlt">air</span> <span class="hlt">CO</span><span class="hlt">2</span> capture, chemical conversion, and storage as a bicarbonate, predominantly as NaHCO3. The excess OH− initially formed in these experiments apparently resulted via neutralization of the anolyte acid, H<span class="hlt">2</span>SO4, by reaction with the base mineral silicate at the anode, producing mineral sulfate and silica. This allowed the NaOH, normally generated at the cathode, to go unneutralized and to accumulate in the bulk electrolyte, ultimately reacting with atmospheric <span class="hlt">CO</span><span class="hlt">2</span> to form dissolved bicarbonate. Using nongrid or nonpeak renewable electricity, optimized systems at large scale might allow relatively high-capacity, energy-efficient (<300 kJ/mol of <span class="hlt">CO</span><span class="hlt">2</span> captured), and inexpensive (<$100 per tonne of <span class="hlt">CO</span><span class="hlt">2</span> mitigated) removal of excess <span class="hlt">air</span> <span class="hlt">CO</span><span class="hlt">2</span> with production of carbon-negative H<span class="hlt">2</span>. Furthermore, when added to the ocean, the produced hydroxide and/or (bi)carbonate could be useful in reducing <span class="hlt">sea-to-air</span> <span class="hlt">CO</span><span class="hlt">2</span> emissions and in neutralizing or offsetting the effects of ongoing ocean acidification. PMID:23729814</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017DSRI..123..118I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017DSRI..123..118I"><span>Anthropogenic <span class="hlt">CO</span><span class="hlt">2</span> in a dense water formation area of the Mediterranean <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ingrosso, Gianmarco; Bensi, Manuel; Cardin, Vanessa; Giani, Michele</p> <p>2017-05-01</p> <p>There is growing evidence that the on-going ocean acidification of the Mediterranean <span class="hlt">Sea</span> could be favoured by its active overturning circulation. The areas of dense water formation are, indeed, preferential sites for atmospheric carbon dioxide absorption and through them the ocean acidification process can quickly propagate into the deep layers. In this study we estimated the concentration of anthropogenic <span class="hlt">CO</span><span class="hlt">2</span> (Cant) in the dense water formation areas of the middle and southern Adriatic <span class="hlt">Sea</span>. Using the composite tracer TrOCA (Tracer combining Oxygen, inorganic Carbon, and total Alkalinity) and carbonate chemistry data collected throughout March 2013, our results revealed that a massive amount of Cant has invaded all the identified water masses. High Cant concentration was detected at the bottom layer of the Pomo Pit (middle Adriatic, 96.8±9.7 μmol kg-1) and Southern Adriatic Pit (SAP, 85.<span class="hlt">2</span>±9.4 μmol kg-1), associated respectively with the presence of North Adriatic Dense Water (NAdDW) and Adriatic Dense Water (AdDW). This anthropogenic contamination was clearly linked to the dense water formation events, which govern strong <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> from the atmosphere to the <span class="hlt">sea</span> and the sinking of dense, <span class="hlt">CO</span><span class="hlt">2</span>-rich surface waters to the deep <span class="hlt">sea</span>. However, a very high Cant level (94.5±12.5 μmol kg-1) was also estimated at the intermediate layer, as a consequence of a recent vertical mixing that determined the physical and biogeochemical modification of the water of Levantine origin (i.e. Modified Levantine Intermediate Water, MLIW) and favoured the atmospheric <span class="hlt">CO</span><span class="hlt">2</span> intrusion. The penetration of Cant in the Adriatic <span class="hlt">Sea</span> determined a significant pH reduction since the pre-industrial era (- 0.139±0.019 pH units on average). This estimation was very similar to the global Mediterranean <span class="hlt">Sea</span> acidification, but it was again more pronounced at the bottom of the Pomo Pit, within the layer occupied by NAdDW (- 0.157±0.018 pH units), and at the intermediate layer of the recently formed MLIW</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.B23A0388H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.B23A0388H"><span>Solution for Minimizing Surface Heating Effect for Fast Open-Path <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Flux</span> Measurements in Cold Environments</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hupp, J. R.; Burba, G. G.; McDermitt, D. K.; Anderson, D. J.; Eckles, R. D.</p> <p>2010-12-01</p> <p>Open-path design of the high speed gas analyzers is a well-established configuration widely used for measurements of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> and concentrations. This configuration has advantages and deficiencies. Advantages include excellent frequency response, long-term stability, low sensitivity to window contamination, low-power pump-free operation, and infrequent calibration requirements. Deficiencies include susceptibility to precipitation and icing, and a potential need for instrument surface heating correction in extremely cold environments. In spite of the deficiencies, open-path measurements often provide data coverage that would not have been possible using traditional closed-path approach. Data loss from precipitation and icing may not always be prevented for the open-path instruments, while heating effect does not pose a problem for <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> in warm environments. Even in cold environments, the impact of heating on <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> is much smaller than other well-known effects, such as Webb-Pearman-Leuning terms, or frequency response corrections for closed-path analyzers. Nonetheless, instrument surface heating effect in cold environments could be addressed scientifically, via developing the theoretical corrections, and instrumentally, via measuring fast integrated <span class="hlt">air</span> temperature in the optical path, or via enclosing the open-path instrument into a low-power short-intake design. Here we provide an alternative way to minimize or eliminate open-path heating effect, achieved by minimizing or eliminating the temperature gradient between the instrument surface and ambient <span class="hlt">air</span>. Open-path low temperature controlled design is discussed in comparison with two other approaches (e.g., traditional open-path design and closed-path design) in terms of their field performance for Eddy Covariance <span class="hlt">flux</span> measurements in the cold. This study presents field data from a new open-path <span class="hlt">CO</span><span class="hlt">2</span>/H<span class="hlt">2</span>O gas analyzer, LI-7500A, based on the LI-7500 model modified to produce substantially less heat during</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A43G2559J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A43G2559J"><span>Seasonal atmospheric deposition and <span class="hlt">air-sea</span> gaseous exchange of polycyclic aromatic hydrocarbons over the Yangtze River Estuary, East China <span class="hlt">Sea</span>: Implication for the source-sink processes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jiang, Y.; Guo, Z.</p> <p>2017-12-01</p> <p>As the home of the largest port in the world, the Yangtze River Estuary (YRE) in the East China <span class="hlt">Sea</span> (ECS) is adjacent to the largest economic zone in China with more than 10% of Chinese population and provides one-fifth of national GDP. The YRE is under the path of contaminated East Asian continental outflow. These make the YRE unique for the pollutant biogeochemical cycling in the world. In this work, 94 pairs of <span class="hlt">air</span> samples and 20 surface seawater samples covering four seasons were collected from a remote receptor site in the YRE from March 2014 to January 2015, in order to explore the seasonal <span class="hlt">fluxes</span> of <span class="hlt">air-sea</span> gaseous exchange and atmospheric dry and wet deposition of 15 polycyclic aromatic hydrocarbons (PAHs) and their source-sink processes at the <span class="hlt">air-sea</span> interface. The average dry and wet deposition <span class="hlt">fluxes</span> of 15 PAHs were estimated as 879 ± 1393 ng m-<span class="hlt">2</span> d-1 and 755 ± 545 ng m-<span class="hlt">2</span> d-1, respectively. The gaseous PAHs were released from seawater to atmosphere during the whole year with an average of 3039 ± 2030 ng m-<span class="hlt">2</span> d-1. The gaseous exchange of PAHs was referred as the dominant process at the <span class="hlt">air-sea</span> interface in the YRE as the magnitude of volatilization <span class="hlt">flux</span> of PAHs exceeded that of the total dry and wet deposition. The gaseous PAH exchange <span class="hlt">flux</span> was dominated by 3-ring PAHs, with the highest value in summer while lowest in winter, depicting a strong seasonal variation due to temperature, wind speed and <span class="hlt">air-sea</span> concentration gradient difference among seasons. Based on the simplified mass balance estimation, net 9.6 tons/y of PAHs was volatilized from seawater to atmosphere with an area of approximately 20000 km<span class="hlt">2</span> in the YRE. Apart from Yangtze River input and ocean ship emissions in the entire year, the selective release of low molecular weight PAHs from sediments in winter due to re-suspension triggered by the East Asian winter monsoon could be another possible source for dissolved PAHs. This work suggests that the source-sink processes of PAHs at <span class="hlt">air-sea</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013BGD....10.1899D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013BGD....10.1899D"><span>Saturated <span class="hlt">CO</span><span class="hlt">2</span> inhibits microbial processes in <span class="hlt">CO</span><span class="hlt">2</span>-vented deep-<span class="hlt">sea</span> sediments</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>de Beer, D.; Haeckel, M.; Neumann, J.; Wegener, G.; Inagaki, F.; Boetius, A.</p> <p>2013-02-01</p> <p>This study focused on biogeochemical processes and microbial activity in sediments of a natural deep-<span class="hlt">sea</span> <span class="hlt">CO</span><span class="hlt">2</span> seepage area (Yonaguni Knoll IV hydrothermal system, Japan). The aim was to assess the influence of the geochemical conditions occurring in highly acidic and <span class="hlt">CO</span><span class="hlt">2</span> saturated sediments on sulphate reduction (SR) and anaerobic methane oxidation (AOM). Porewater chemistry was investigated from retrieved sediment cores and in situ by microsensor profiling. The sites sampled around a sediment-hosted hydrothermal <span class="hlt">CO</span><span class="hlt">2</span> vent were very heterogeneous in porewater chemistry, indicating a complex leakage pattern. Near the vents, droplets of liquid <span class="hlt">CO</span><span class="hlt">2</span> were observed to emanate from the sediments, and the pH reached approximately 4.5 in a sediment depth >6 cm, as determined in situ by microsensors. Methane and sulphate <span class="hlt">co</span>-occurred in most sediment samples from the vicinity of the vents down to a depth of at least 3 m. However, SR and AOM were restricted to the upper 7-15 cm below seafloor, although neither temperature, low pH, nor the availability of methane and sulphate could be limiting microbial activity. We argue that the extremely high subsurface concentrations of dissolved <span class="hlt">CO</span><span class="hlt">2</span> (1000-1700 mM), through the ensuing high H<span class="hlt">2</span><span class="hlt">CO</span>3 levels (approx. 1-<span class="hlt">2</span> mM) uncouples the proton-motive-force (PMF) and thus inhibits biological energy conservation by ATPase-driven phosphorylation. This limits life to the surface sediment horizons above the liquid <span class="hlt">CO</span><span class="hlt">2</span> phase, where less extreme conditions prevail. Our results may have to be taken into consideration in assessing the consequences of deep-<span class="hlt">sea</span> <span class="hlt">CO</span><span class="hlt">2</span> sequestration on benthic element cycling and on the local ecosystem state.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_12 --> <div id="page_13" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="241"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16...26P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16...26P"><span>Volcanic <span class="hlt">CO</span><span class="hlt">2</span> mapping and <span class="hlt">flux</span> measurements at Campi Flegrei by Tunable Diode Laser absorption Spectroscopy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pedone, Maria; Aiuppa, Alessandro; Giudice, Gaetano; Grassa, Fausto; Chiodini, Giovanni; Valenza, Mariano</p> <p>2014-05-01</p> <p>Near-infrared room-temperature Tunable Diode Lasers (TDL) have recently found increased usage in atmospheric chemistry and <span class="hlt">air</span> monitoring research, but applications in Volcanology are still limited to a few examples. Here, we explored the potentiality of a commercial infrared laser unit (GasFinder <span class="hlt">2</span>.0 from Boreal Laser Ltd) to measurement of volcanic <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> emissions. Our field tests were conducted at Campi Flegrei (near Pozzuoli, Southern Italy), where the GasFinder was used (during three campaigns in October 2012, January 2013 and May 2013) to repeatedly measure the path-integrated concentrations of <span class="hlt">CO</span><span class="hlt">2</span> along cross-sections of the atmospheric plumes of the two main fumarolic fields in the area (Solfatara and Pisciarelli). By using ad-hoc designed field-set-up and a tomographic post-processing routine, we resolved, for each of the <span class="hlt">2</span> manifestations, the contour maps of <span class="hlt">CO</span><span class="hlt">2</span> concentrations in their atmospheric plumes, from the integration of which (and after multiplication by the plumes' transport speeds) the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> were finally obtained [1]. The so-calculated <span class="hlt">fluxes</span> average of 490 tons/day, which agrees well with independent evaluations of Aiuppa et al. (2013) [<span class="hlt">2</span>] (460 tons/day on average), and support a significant contribution of fumaroles to the total <span class="hlt">CO</span><span class="hlt">2</span> budget. The cumulative (fumarole [this study] +soil [<span class="hlt">2</span>]) <span class="hlt">CO</span><span class="hlt">2</span> output from Campi Flegrei is finally evaluated at 1600 tons/day. The application of lasers to volcanic gas studies is still an emerging (though intriguing) research field, and requires more testing and validation experiments. We conclude that TDL technique may valuably assist <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> quantification at a number of volcanic targets worldwide. [1] Pedone M. et al. (2013) Gold2013:abs:5563, Goldschmidt Conference, session 11a. [<span class="hlt">2</span>] Aiuppa A. et al. (2013) Geochemistry Geophysics Geosystems. doi: 10.1002/ggge.20261. [3] Chiodini G. et al. (2010) Journal of Geophysical Research, Volume 115, B03205. doi:10.1029/2008JB006258.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A41C2277B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A41C2277B"><span>Understanding the Role of <span class="hlt">Air-Sea</span> Interaction on Extreme Rainfall in Aquaplanet and Earth-like CESM<span class="hlt">2</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Benedict, J. J.; Clement, A. C.; Medeiros, B.</p> <p>2017-12-01</p> <p>Extreme precipitation events are associated with anomalous, latitudinally dependent dynamical and convective weather systems. For example, plumes of excessive poleward water vapor transport and topographical effects drive extreme precipitation events in the midlatitudes, while intense tropical precipitation is associated with organized convective systems. In both cases, <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> have the potential to contribute significantly to the moisture budget of these storms, but the roles of surface <span class="hlt">fluxes</span> and upper-ocean processes and their impact on precipitation extremes have yet to be explored in sufficient detail. To examine such mechanisms, we implement a climate model hierarchy that encompasses a spectrum of ocean models, from prescribed-SST to fully dynamic, as well as both aquaplanet and Earth-like lower boundary types within version <span class="hlt">2</span> of the Community Earth System Model (CESM<span class="hlt">2</span>). Using the CESM<span class="hlt">2</span> hierarchy and comparing to observations, we identify key moisture processes and related <span class="hlt">air-sea</span> interactions that drive extreme precipitation events across different latitudes in Earth-like models and then generalize the analyses in aquaplanet configurations to highlight the most salient features. The analyses are applied to both present-day and global warming conditions to investigate how these fundamental mechanisms might change extreme precipitation events in the future climate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002EGSGA..27.5473S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002EGSGA..27.5473S"><span>Summer Distribution of <span class="hlt">Co</span><span class="hlt">2</span> Partial Pressure In The Ross <span class="hlt">Sea</span>, Antarctica, and Relations With Biological Activity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sandrini, S.; Tositti, L.; Tubertini, O.; Ceradini, S.; Palucci, A.; Barbini, R.; Fantoni, R.; Colao, F.; Ferrari, G. M.</p> <p></p> <p>The oceans play a key role in the processes responsible for global climate changes, in fact the oceanic uptake of anthropogenic atmospheric carbon dioxide is estimated to be 17-39The Southern Ocean and Antarctic marginal <span class="hlt">seas</span> are considered to absorb up to half of this fraction. The Ross <span class="hlt">Sea</span>, during the summer pack-ice melting, expe- riences rapid seasonal outgrowths, giving rise to phytoplankton blooms, especially in polynya areas near the coast line. This has a direct influence on p<span class="hlt">CO</span><span class="hlt">2</span> concentration in surface water, and hence on <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> between ocean and atmosphere. Both the Ross <span class="hlt">Sea</span> and the Southern Ocean transect between New Zealand and Antarctica are sys- tematically investigated during Italian Antarctic oceanographic campaigns onboard of the R/V Italica. During the XVI expedition, which took place in January and Febru- ary 2001, simultaneous measurements of surface p<span class="hlt">CO</span><span class="hlt">2</span> and Chlorophyll-a by laser remote-sensing apparatus were collected. Chlorophyll-a and p<span class="hlt">CO</span><span class="hlt">2</span> showed a general anticorrelation along the cruise. The survey has revealed the presence of high produc- tive regions in the polynya and close to the ice edge. The linear regression analysis of the chl-a vs p<span class="hlt">CO</span><span class="hlt">2</span> values improved our knowledge of the time evolution of the phyto- planktonic growth, independently measured by means of the laser yield, thus allowing for discrimination between different initial and final blooms in the Antarctic Ross <span class="hlt">Sea</span>. The results obtained are here presented and discussed. They confirm the importance of biological production in the net absorption of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> in continental shelf zones.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=85598&Lab=NERL&keyword=control+AND+group+AND+experimental&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50','EPA-EIMS'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=85598&Lab=NERL&keyword=control+AND+group+AND+experimental&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50"><span>SOIL <span class="hlt">FLUXES</span> OF <span class="hlt">CO</span><span class="hlt">2</span>, <span class="hlt">CO</span>, NO AND N<span class="hlt">2</span>O FROM AN OLD-PASTURE AND FROM NATIVE SAVANNA IN BRAZIL</span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p>We compared <span class="hlt">fluxes</span> of <span class="hlt">CO</span><span class="hlt">2</span>, <span class="hlt">CO</span>, NO and N<span class="hlt">2</span>O, soil microbial biomass, and N-mineralization rates in a 20-year old Brachiaria pasture and a native cerrado area (savanna in Central Brazil). In order to assess the spatial variability of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>, we tested the relation between elect...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27363345','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27363345"><span>Grazing effects on ecosystem <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> differ among temperate steppe types in Eurasia.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hou, Longyu; Liu, Yan; Du, Jiancai; Wang, Mingya; Wang, Hui; Mao, Peisheng</p> <p>2016-07-01</p> <p>Grassland ecosystems play a critical role in regulating <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> into and out of the Earth's surface. Whereas previous studies have often addressed single <span class="hlt">fluxes</span> of <span class="hlt">CO</span><span class="hlt">2</span> separately, few have addressed the relation among and controls of multiple <span class="hlt">CO</span><span class="hlt">2</span> sub-<span class="hlt">fluxes</span> simultaneously. In this study, we examined the relation among and controls of individual <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> (i.e., GEP, NEP, SR, ER, CR) in three contrasting temperate steppes of north China, as affected by livestock grazing. Our findings show that climatic controls of the seasonal patterns in <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> were both individual <span class="hlt">flux</span>- and steppe type-specific, with significant grazing impacts observed for canopy respiration only. In contrast, climatic controls of the annual patterns were only individual <span class="hlt">flux</span>-specific, with minor grazing impacts on the individual <span class="hlt">fluxes</span>. Grazing significantly reduced the mean annual soil respiration rate in the typical and desert steppes, but significantly enhanced both soil and canopy respiration in the meadow steppe. Our study suggests that a reassessment of the role of livestock grazing in regulating GHG exchanges is imperative in future studies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1713074S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1713074S"><span><span class="hlt">Air-sea</span> <span class="hlt">fluxes</span> and satellite-based estimation of water masses formation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sabia, Roberto; Klockmann, Marlene; Fernandez-Prieto, Diego; Donlon, Craig</p> <p>2015-04-01</p> <p>Recent work linking satellite-based measurements of <span class="hlt">sea</span> surface salinity (SSS) and <span class="hlt">sea</span> surface temperature (SST) with traditional physical oceanography has demonstrated the capability of generating routinely satellite-derived surface T-S diagrams [1] and analyze the distribution/dynamics of SSS and its relative surface density with respect to in-situ measurements. Even more recently [<span class="hlt">2</span>,3], this framework has been extended by exploiting these T-S diagrams as a diagnostic tool to derive water masses formation rates and areas. A water mass describes a water body with physical properties distinct from the surrounding water, formed at the ocean surface under specific conditions which determine its temperature and salinity. The SST and SSS (and thus also density) at the ocean surface are largely determined by <span class="hlt">fluxes</span> of heat and freshwater. The surface density <span class="hlt">flux</span> is a function of the latter two and describes the change of the density of seawater at the surface. To obtain observations of water mass formation is of great interest, since they serve as indirect observations of the thermo-haline circulation. The SSS data which has become available through the SMOS [4] and Aquarius [5] satellite missions will provide the possibility of studying also the effect of temporally-varying SSS fields on water mass formation. In the present study, the formation of water masses as a function of SST and SSS is derived from the surface density <span class="hlt">flux</span> by integrating the latter over a specific area and time period in bins of SST and SSS and then taking the derivative of the total density <span class="hlt">flux</span> with respect to density. This study presents a test case using SMOS SSS, OSTIA SST, as well as Argo ISAS SST and SSS for comparison, heat <span class="hlt">fluxes</span> from the NOCS Surface <span class="hlt">Flux</span> Data Set v<span class="hlt">2</span>.0, OAFlux evaporation and CMORPH precipitation. The study area, initially referred to the North Atlantic, is extended over two additional ocean basins and the study period covers the 2011-2012 timeframe. Yearly, seasonal</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.7939Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.7939Z"><span>Application of Relaxed Eddy Accumulation (REA) method to estimate <span class="hlt">CO</span><span class="hlt">2</span> and CH4 surface <span class="hlt">fluxes</span> in the city of Krakow, southern Poland.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zimnoch, Miroslaw; Gorczyca, Zbigniew; Pieniazek, Katarzyna; Jasek, Alina; Chmura, Lukasz; Rozanski, Kazimierz</p> <p>2013-04-01</p> <p>There is a growing interest in the recent years in studies aimed at quantifying carbon cycling in urban centres. Worldwide migration of human population from rural to urban areas and corresponding growth of extensive urban agglomerations and megacities leads to intensification of anthropogenic emissions of carbon and strong disruption of natural carbon cycle on these areas. Therefore, a deeper understanding of the carbon "metabolism" of such regions is required. Apart of better quantification of surface carbon <span class="hlt">fluxes</span>, also a thorough understanding of the functioning of biosphere under strong anthropogenic influence is needed. Nowadays, covariance methods are widely applied for studying gas exchange between the atmosphere and the Earth's surface. Relaxed Eddy Accumulation method (REA), combined with the <span class="hlt">CO</span><span class="hlt">2</span> and CH4 CRDS analyser allows simultaneous measurements of surface <span class="hlt">fluxes</span> of carbon dioxide and methane within the chosen footprint of the detection system, thus making possible thorough characterisation of the overall exchange of those gases between the atmosphere and the urban surface across diverse spatial and temporal scales. Here we present preliminary results of the study aimed at quantifying surface <span class="hlt">fluxes</span> of <span class="hlt">CO</span><span class="hlt">2</span> and CH4 in Krakow, southern Poland. The REA system for <span class="hlt">CO</span><span class="hlt">2</span> and CH4 <span class="hlt">flux</span> measurements has been installed on top of a 20m high tower mounted on the roof of the faculty building, close to the city centre of Krakow. The sensors were installed ca 42 m above the local ground. Gill Windmaster-Pro sonic anemometer was coupled with self-made system, designed by the Poznan University of Life Sciences, Poland, for collecting <span class="hlt">air</span> samples in two pairs of 10-liter Tedlar bags, and with Picarro G2101-i CRDS analyser. The <span class="hlt">air</span> was collected in 30-min intervals. The <span class="hlt">CO</span><span class="hlt">2</span> and CH4 mixing ratios in these cumulative downdraft and updraft <span class="hlt">air</span> samples were determined by the CRDS analyser after each sampling interval. Based on the measured mixing ratios difference and the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ClDy...49.2219S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ClDy...49.2219S"><span>Accounting for observation uncertainties in an evaluation metric of low latitude turbulent <span class="hlt">air-sea</span> <span class="hlt">fluxes</span>: application to the comparison of a suite of IPSL model versions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Servonnat, Jérôme; Găinuşă-Bogdan, Alina; Braconnot, Pascale</p> <p>2017-09-01</p> <p>Turbulent momentum and heat (sensible heat and latent heat) <span class="hlt">fluxes</span> at the <span class="hlt">air-sea</span> interface are key components of the whole energetic of the Earth's climate. The evaluation of these <span class="hlt">fluxes</span> in the climate models is still difficult because of the large uncertainties associated with the reference products. In this paper we present an objective metric accounting for reference uncertainties to evaluate the annual cycle of the low latitude turbulent <span class="hlt">fluxes</span> of a suite of IPSL climate models. This metric consists in a Hotelling T <span class="hlt">2</span> test between the simulated and observed field in a reduce space characterized by the dominant modes of variability that are common to both the model and the reference, taking into account the observational uncertainty. The test is thus more severe when uncertainties are small as it is the case for <span class="hlt">sea</span> surface temperature (SST). The results of the test show that for almost all variables and all model versions the model-reference differences are not zero. It is not possible to distinguish between model versions for sensible heat and meridional wind stress, certainly due to the large observational uncertainties. All model versions share similar biases for the different variables. There is no improvement between the reference versions of the IPSL model used for CMIP3 and CMIP5. The test also reveals that the higher horizontal resolution fails to improve the representation of the turbulent surface <span class="hlt">fluxes</span> compared to the other versions. The representation of the <span class="hlt">fluxes</span> is further degraded in a version with improved atmospheric physics with an amplification of some of the biases in the Indian Ocean and in the intertropical convergence zone. The ranking of the model versions for the turbulent <span class="hlt">fluxes</span> is not correlated with the ranking found for SST. This highlights that despite the fact that SST gradients are important for the large-scale atmospheric circulation patterns, other factors such as wind speed, and <span class="hlt">air-sea</span> temperature contrast play an</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.H23D1006B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.H23D1006B"><span>Multi-channel Auto-dilution System for Remote Continuous Monitoring of High Soil-<span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Barr, J. L.; Amonette, J. E.</p> <p>2008-12-01</p> <p>We describe a novel field instrument that takes input from up to 27 soil <span class="hlt">flux</span> chambers and measures <span class="hlt">flux</span> using the steady-state method. <span class="hlt">CO</span><span class="hlt">2</span> concentrations are determined with an infrared gas analyzer (IRGA, 0- 3000 ppmv range) with corrections for temperature, barometric pressure, and moisture content. The concentrations are monitored during data collection and, if they exceed the range of the IRGA, a stepped dilution program is automatically implemented that allows up to 50-fold dilution of the incoming gas stream with N<span class="hlt">2</span> supplied by boil-off from a large dewar. The upper concentration limit of the system with dilution is extended to at least 150,000 ppmv <span class="hlt">CO</span><span class="hlt">2</span>. The data are stored on a datalogger having a cellular modem connection that allows remote control of the system as well as transmittal of data. The system is designed to operate for six weeks with no on-site maintenance required. Longer periods are possible with modifications to allow on-site generation of N<span class="hlt">2</span> from <span class="hlt">air</span>. Example data from a recent <span class="hlt">CO</span><span class="hlt">2</span> test injection at the Zero- Emission Research and Technology (ZERT) field site in Bozeman, MT are presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19930000880','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19930000880"><span><span class="hlt">Air-sea</span> interaction and remote sensing</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Katsaros, Kristina B.; Ataktuerk, Serhad S.</p> <p>1992-01-01</p> <p>The first part of the proposed research was a joint effort between our group and the Applied Physics Laboratory (APL), University of Washington. Our own research goal is to investigate the relation between the <span class="hlt">air-sea</span> exchange processes and the <span class="hlt">sea</span> state over the open ocean and to compare these findings with our previous results obtained over a small body of water namely, Lake Washington. The goals of the APL researchers are to study (1) the infrared <span class="hlt">sea</span> surface temperature (SST) signature of breaking waves and surface slicks, and (<span class="hlt">2</span>) microwave and acoustic scattering from water surface. The task of our group in this joint effort is to conduct measurements of surface <span class="hlt">fluxes</span> (of momentum, sensible heat, and water vapor) and atmospheric radiation (longwave and shortwave) to achieve our research goal as well as to provide crucial complementary data for the APL studies. The progress of the project is summarized.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.B33C0609S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.B33C0609S"><span>Decadal trends in regional <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> estimated from atmospheric inversions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Saeki, T.; Patra, P. K.</p> <p>2016-12-01</p> <p>Top-down approach (or atmospheric inversion) using atmospheric transport models and <span class="hlt">CO</span><span class="hlt">2</span> observations are an effective way to optimize surface <span class="hlt">fluxes</span> at subcontinental scales and monthly time intervals. We used the CCSR/NIES/FRCGC AGCM-based Chemistry Transport Model (JAMSTEC's ACTM) and atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentrations at NOAA, CSIRO, JMA, NIES, NIES-MRI sites from Obspack GLOBALVIEW-<span class="hlt">CO</span><span class="hlt">2</span> data product (2013) for estimating <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> for the period of 1990-2011. Carbon <span class="hlt">fluxes</span> were estimated for 84 partitions (54 lands + 30 oceans) of the globe by using a Bayesian synthesis inversion framework. A priori <span class="hlt">fluxes</span> are (1) atmosphere-ocean exchange from Takahashi et al. (2009), (<span class="hlt">2</span>) 3-hourly terrestrial biosphere <span class="hlt">fluxes</span> (annually balanced) from CASA model, and (3) fossil fuel <span class="hlt">fluxes</span> from CDIAC global totals and EDGAR4.<span class="hlt">2</span> spatial distributions. Four inversion cases have been tested with 1) 21 sites (sites which have real data fraction of 90 % or more for 1989-2012), <span class="hlt">2</span>) 21 sites + CONTRAIL data, 3) 66 sites (over 70 % coverage), and 4) 157 sites. As a result of time-dependent inversions, mean total <span class="hlt">flux</span> (excluding fossil fuel) for the period 1990-2011 is estimated to be -3.09 ±0.16 PgC/yr (mean and standard deviation of the four cases), where land (incl. biomass burning and land use change) and ocean absorb an average rate of -1.80 ±0.18 and -1.29 ±0.08 PgC/yr, respectively. The average global total sink from 1991-2000 to 2001-2010 increases by about 0.5 PgC/yr, mainly due to the increase in northern and tropical land sinks (Africa, Boreal Eurasia, East Asia and Europe), while ocean sinks show no clear trend. Inversion with CONTRAIL data estimates large positive <span class="hlt">flux</span> anomalies in late 1997 associated with the 1997/98 El-Nino, while inversion without CONTARIL data between Japan and Australia fails to estimate such large anomalies. Acknowledgements. This work is supported by the Environment Research and Technology Development Fund (<span class="hlt">2</span>-1401) of the Ministry of the Environment</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.B21E1987B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.B21E1987B"><span>Carbon Dioxide and Water Vapor Concentrations, <span class="hlt">Co</span>-spectra and <span class="hlt">Fluxes</span> from Latest Standardized Automated <span class="hlt">CO</span><span class="hlt">2</span>/H<span class="hlt">2</span>O <span class="hlt">Flux</span> Systems versus Established Analyzer Models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Burba, G. G.; Kathilankal, J. C.; Begashaw, I.; Franzen, D.; Welles, J.; McDermitt, D. K.</p> <p>2017-12-01</p> <p>Spatial and temporal <span class="hlt">flux</span> data coverage have improved significantly in recent years, due to standardization, automation and management of data collection, and better handling of the generated data. With more stations and networks, larger data streams from each station, and smaller operating budgets, modern tools are required to effectively and efficiently handle the entire process.These tools should produce standardized verifiable datasets, and provide a way to cross-share the standardized data with external collaborators to leverage available funding, and promote data analyses and publications. In 2015, new open-path and enclosed <span class="hlt">flux</span> measurement systems1 were developed, based on established gas analyzer models<span class="hlt">2</span>,3, with the goal of improving stability in the presence of contamination, refining temperature control and compensation, and providing more accurate gas concentration measurements. In 2017, the new open-path system was further refined to simplify hardware configuration, and to reduce power consumption and cost. Additionally, all new systems incorporate complete automated on-site <span class="hlt">flux</span> calculations using EddyPro® Software4 run by a weatherized remotely-accessible microcomputer to provide standardized traceable data sets for <span class="hlt">fluxes</span> and supporting variables. This presentation will describe details and results from the field tests of the new <span class="hlt">flux</span> systems, in comparison to older models and reference instruments. References:1 Burba G., W. Miller, I. Begashaw, G. Fratini, F. Griessbaum, J. Kathilankal, L. Xu, D. Franz, E. Joseph, E. Larmanou, S. Miller, D. Papale, S. Sabbatini, T. Sachs, R. Sakai, D. McDermitt, 2017. Comparison of <span class="hlt">CO</span><span class="hlt">2</span> Concentrations, <span class="hlt">Co</span>-spectra and <span class="hlt">Flux</span> Measurements between Latest Standardized Automated <span class="hlt">CO</span><span class="hlt">2</span>/H<span class="hlt">2</span>O <span class="hlt">Flux</span> Systems and Older Gas Analysers. 10th ICDC Conference, Switzerland: 21-25/08 <span class="hlt">2</span> Metzger, S., G. Burba, S. Burns, P. Blanken, J. Li, H. Luo, R. Zulueta, 2016. Optimization of an enclosed gas analyzer sampling system for measuring eddy</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ACP....18.7189B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ACP....18.7189B"><span>The impact of transport model differences on <span class="hlt">CO</span><span class="hlt">2</span> surface <span class="hlt">flux</span> estimates from OCO-<span class="hlt">2</span> retrievals of column average <span class="hlt">CO</span><span class="hlt">2</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Basu, Sourish; Baker, David F.; Chevallier, Frédéric; Patra, Prabir K.; Liu, Junjie; Miller, John B.</p> <p>2018-05-01</p> <p>We estimate the uncertainty of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> estimates in atmospheric inversions stemming from differences between different global transport models. Using a set of observing system simulation experiments (OSSEs), we estimate this uncertainty as represented by the spread between five different state-of-the-art global transport models (ACTM, LMDZ, GEOS-Chem, PCTM and TM5), for both traditional in situ <span class="hlt">CO</span><span class="hlt">2</span> inversions and inversions of XCO<span class="hlt">2</span> estimates from the Orbiting Carbon Observatory <span class="hlt">2</span> (OCO-<span class="hlt">2</span>). We find that, in the absence of relative biases between in situ <span class="hlt">CO</span><span class="hlt">2</span> and OCO-<span class="hlt">2</span> XCO<span class="hlt">2</span>, OCO-<span class="hlt">2</span> estimates of terrestrial <span class="hlt">flux</span> for TRANSCOM-scale land regions can be more robust to transport model differences than corresponding in situ <span class="hlt">CO</span><span class="hlt">2</span> inversions. This is due to a combination of the increased spatial coverage of OCO-<span class="hlt">2</span> samples and the total column nature of OCO-<span class="hlt">2</span> estimates. We separate the two effects by constructing hypothetical in situ networks with the coverage of OCO-<span class="hlt">2</span> but with only near-surface samples. We also find that the transport-driven uncertainty in <span class="hlt">fluxes</span> is comparable between well-sampled northern temperate regions and poorly sampled tropical regions. Furthermore, we find that spatiotemporal differences in sampling, such as between OCO-<span class="hlt">2</span> land and ocean soundings, coupled with imperfect transport, can produce differences in <span class="hlt">flux</span> estimates that are larger than <span class="hlt">flux</span> uncertainties due to transport model differences. This highlights the need for sampling with as complete a spatial and temporal coverage as possible (e.g., using both land and ocean retrievals together for <span style="" class="text">OCO-<span class="hlt">2</span>) to minimize the impact of selective sampling. Finally, our annual and monthly estimates of transport-driven uncertainties can be used to evaluate the robustness of conclusions drawn from real OCO-<span class="hlt">2</span> and in situ <span class="hlt">CO</span><span class="hlt">2</span> inversions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27811286','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27811286"><span>Observed Arctic <span class="hlt">sea</span>-ice loss directly follows anthropogenic <span class="hlt">CO</span><span class="hlt">2</span> emission.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Notz, Dirk; Stroeve, Julienne</p> <p>2016-11-11</p> <p>Arctic <span class="hlt">sea</span> ice is retreating rapidly, raising prospects of a future ice-free Arctic Ocean during summer. Because climate-model simulations of the <span class="hlt">sea</span>-ice loss differ substantially, we used a robust linear relationship between monthly-mean September <span class="hlt">sea</span>-ice area and cumulative carbon dioxide (<span class="hlt">CO</span> <span class="hlt">2</span> ) emissions to infer the future evolution of Arctic summer <span class="hlt">sea</span> ice directly from the observational record. The observed linear relationship implies a sustained loss of 3 ± 0.3 square meters of September <span class="hlt">sea</span>-ice area per metric ton of <span class="hlt">CO</span> <span class="hlt">2</span> emission. On the basis of this sensitivity, Arctic <span class="hlt">sea</span> ice will be lost throughout September for an additional 1000 gigatons of <span class="hlt">CO</span> <span class="hlt">2</span> emissions. Most models show a lower sensitivity, which is possibly linked to an underestimation of the modeled increase in incoming longwave radiation and of the modeled transient climate response. Copyright © 2016, American Association for the Advancement of Science.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26931659','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26931659"><span><span class="hlt">Air-sea</span> exchange of gaseous mercury in the tropical coast (Luhuitou fringing reef) of the South China <span class="hlt">Sea</span>, the Hainan Island, China.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ci, Zhijia; Zhang, Xiaoshan; Wang, Zhangwei</p> <p>2016-06-01</p> <p>The <span class="hlt">air-sea</span> exchange of gaseous mercury (mainly Hg(0)) in the tropical ocean is an important part of the global Hg biogeochemical cycle, but the related investigations are limited. In this study, we simultaneously measured Hg(0) concentrations in surface waters and overlaying <span class="hlt">air</span> in the tropical coast (Luhuitou fringing reef) of the South China <span class="hlt">Sea</span> (SCS), Hainan Island, China, for 13 days on January-February 2015. The purpose of this study was to explore the temporal variation of Hg(0) concentrations in <span class="hlt">air</span> and surface waters, estimate the <span class="hlt">air-sea</span> Hg(0) <span class="hlt">flux</span>, and reveal their influencing factors in the tropical coastal environment. The mean concentrations (±SD) of Hg(0) in <span class="hlt">air</span> and total Hg (THg) in waters were <span class="hlt">2</span>.34 ± 0.26 ng m(-3) and 1.40 ± 0.48 ng L(-1), respectively. Both Hg(0) concentrations in waters (53.7 ± 18.8 pg L(-1)) and Hg(0)/THg ratios (3.8 %) in this study were significantly higher than those of the open water of the SCS in winter. Hg(0) in waters usually exhibited a clear diurnal variation with increased concentrations in daytime and decreased concentrations in nighttime, especially in cloudless days with low wind speed. Linear regression analysis suggested that Hg(0) concentrations in waters were positively and significantly correlated to the photosynthetically active radiation (PAR) (R (<span class="hlt">2</span>) = 0.42, p < 0.001). Surface waters were always supersaturated with Hg(0) compared to <span class="hlt">air</span> (the degree of saturation, <span class="hlt">2</span>.46 to 13.87), indicating that the surface water was one of the atmospheric Hg(0) sources. The <span class="hlt">air-sea</span> Hg(0) <span class="hlt">fluxes</span> were estimated to be 1.73 ± 1.25 ng m(-<span class="hlt">2</span>) h(-1) with a large range between 0.01 and 6.06 ng m(-<span class="hlt">2</span>) h(-1). The high variation of Hg(0) <span class="hlt">fluxes</span> was mainly attributed to the greatly temporal variation of wind speed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013TCD.....7.6075R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013TCD.....7.6075R"><span>Dynamic ikaite production and dissolution in <span class="hlt">sea</span> ice - control by temperature, salinity and p<span class="hlt">CO</span><span class="hlt">2</span> conditions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rysgaard, S.; Wang, F.; Galley, R. J.; Grimm, R.; Lemes, M.; Geilfus, N.-X.; Chaulk, A.; Hare, A. A.; Crabeck, O.; Else, B. G. T.; Campbell, K.; Papakyriakou, T.; Sørensen, L. L.; Sievers, J.; Notz, D.</p> <p>2013-12-01</p> <p>Ikaite is a hydrous calcium carbonate mineral (Ca<span class="hlt">CO</span>3 · 6H<span class="hlt">2</span>O). It is only found in a metastable state, and decomposes rapidly once removed from near-freezing water. Recently, ikaite crystals have been found in <span class="hlt">sea</span> ice and it has been suggested that their precipitation may play an important role in <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange in ice-covered <span class="hlt">seas</span>. Little is known, however, of the spatial and temporal dynamics of ikaite in <span class="hlt">sea</span> ice. Here we present evidence for highly dynamic ikaite precipitation and dissolution in <span class="hlt">sea</span> ice grown at an out-door pool of the <span class="hlt">Sea</span>-ice Environmental Research Facility (SERF). During the experiment, ikaite precipitated in <span class="hlt">sea</span> ice with temperatures below -3 °C, creating three distinct zones of ikaite concentrations: (1) a mm to cm thin surface layer containing frost flowers and brine skim with bulk concentrations of > 2000 μmol kg-1, (<span class="hlt">2</span>) an internal layer with concentrations of 200-400 μmol kg-1 and (3) a~bottom layer with concentrations of < 100 μmol kg-1. Snowfall events caused the <span class="hlt">sea</span> ice to warm, dissolving ikaite crystals under acidic conditions. Manual removal of the snow cover allowed the <span class="hlt">sea</span> ice to cool and brine salinities to increase, resulting in rapid ikaite precipitation. The modeled (FREZCHEM) ikaite concentrations were in the same order of magnitude as observations and suggest that ikaite concentration in <span class="hlt">sea</span> ice increase with decreasing temperatures. Thus, varying snow conditions may play a key role in ikaite precipitation and dissolution in <span class="hlt">sea</span> ice. This will have implications for <span class="hlt">CO</span><span class="hlt">2</span> exchange with the atmosphere and ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..1410939S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..1410939S"><span>Bioproductivity in the Southern Ocean since the last Interglacial - new high-resolution biogenic opal <span class="hlt">flux</span> records from the Scotia <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sprenk, D.; Weber, M. E.; Kuhn, G.; Rosén, P.; Röhling, H.-G.</p> <p>2012-04-01</p> <p>The Southern Ocean plays an important role in transferring <span class="hlt">CO</span><span class="hlt">2</span> via wind-induced upwelling from the deep <span class="hlt">sea</span> to the atmosphere. It is therefore one of the key areas to study climate change. Bioproductivity in the Southern Ocean is mostly influenced by the extent of <span class="hlt">sea</span> ice, upwelling of cold nutrient- and silica-rich water, and the availability of light. Biogenic opal (BSi) is a significant nutrient in the Southern Ocean, and according to recent investigations only marginally affected by preservation changes. It can therefore be used as bioproductivity proxy. Here we present several methods to determine BSi, discuss them and put the results into context with respect to regional bioproductivity changes in Southern Ocean during the last glacial cycle. We studied deep-<span class="hlt">sea</span> sediment core sites MD07-3133 and MD07-3134 from the central Scotia <span class="hlt">Sea</span> with extraordinary high sedimentation rates of up to <span class="hlt">2</span>.1 to 1.<span class="hlt">2</span> m/kyr, respectively covering the last 92.5 kyr. BSi leaching according to Müller & Schneider (1993) is very time-consuming and expensive, so we measured only 253 samples from large-amplitude variation core sections. In addition, we determined BSi using non-destructive measurements of sediment colour b*, wet-bulk density, and Ti/Si count ratios. Furthermore, we provide the first attempts to estimate BSi in marine sediment using Fourier transform infrared spectroscopy (FTIRS), a cost-efficient method, which requires only 11 mg of sediment. All estimation methods capture the main BSi trends, however FTIRS seems to be the most promising one. In the central Scotia <span class="hlt">Sea</span>, south of the modern Antarctic Polar Front, the BSi <span class="hlt">flux</span> reflects a relatively complicated glacial-to-interglacial pattern with large-amplitude, millennial-scale fluctuations in bioproductivity. During Antarctic Isotopic Maxima, BSi <span class="hlt">fluxes</span> were generally increased. Lowest bioproductivity occur at the Last Glacial Maximum, while upwelling of mid-depth water was reduced, atmospheric <span class="hlt">CO</span><span class="hlt">2</span> low, and <span class="hlt">sea</span>-ice cover</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.A44A..06N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.A44A..06N"><span>Imposing strong constraints on tropical terrestrial <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> using passenger aircraft based measurements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Niwa, Y.; Machida, T.; Sawa, Y.; Matsueda, H.; Schuck, T. J.; Brenninkmeijer, C. A.; Imasu, R.; Satoh, M.</p> <p>2011-12-01</p> <p>Better understanding of the global and regional carbon budget is needed to perform a reliable prediction of future climate with an earth system model. However, the reliability of <span class="hlt">CO</span><span class="hlt">2</span> source/sink estimation by inverse modeling, which is one of the promising methods to estimate regional carbon budget, is limited because of sparse observational data coverage. Very few observational data are available in tropics. Therefore, especially the reconstruction of tropical terrestrial <span class="hlt">fluxes</span> has considerable uncertainties. In this study, regional <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> for 2006-2008 are estimated by inverse modeling using the Comprehensive Observation Network for Trace gases by Airliner (CONTRAIL) in addition to the surface measurement dataset of GLOBALVIEW-<span class="hlt">CO</span><span class="hlt">2</span>. CONTRAIL is a recently established <span class="hlt">CO</span><span class="hlt">2</span> measurement network using in-situ measurement instruments on board commercial aircraft. Five CONTRAIL aircraft travel back and forth between Japan and many areas: Europe, North America, Southeast Asia, South Asia, and Australia. The Bayesian synthesis approach is used to estimate monthly <span class="hlt">fluxes</span> for 42 regions using NICAM-TM simulations with existing <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> datasets and monthly mean observational data. It is demonstrated that the aircraft data have great impact on estimated tropical terrestrial <span class="hlt">fluxes</span>. By adding the aircraft data to the surface data, the analyzed uncertainty of tropical <span class="hlt">fluxes</span> has been reduced by 15 % and more than 30 % uncertainty reduction rate is found in Southeast and South Asia. Specifically, for annual net <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>, nearly neutral <span class="hlt">fluxes</span> of Indonesia, which is estimated using the surface dataset alone, turn to positive <span class="hlt">fluxes</span>, i.e. carbon sources. In Indonesia, a remarkable carbon release during the severe drought period of October-December in 2006 is estimated, which suggests that biosphere respiration or biomass burning was larger than the prior <span class="hlt">fluxes</span>. Comparison of the optimized atmospheric <span class="hlt">CO</span><span class="hlt">2</span> with independent aircraft measurements of CARIBIC tends to validate</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007BGD.....4.3863J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007BGD.....4.3863J"><span>The impact on atmospheric <span class="hlt">CO</span><span class="hlt">2</span> of iron fertilization induced changes in the ocean's biological pump</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jin, X.; Gruber, N.; Frenzel, H.; Doney, S. C.; McWilliams, J. C.</p> <p>2007-10-01</p> <p>Using numerical simulations, we quantify the impact of changes in the ocean's biological pump on the <span class="hlt">air-sea</span> balance of <span class="hlt">CO</span><span class="hlt">2</span> by fertilizing a small surface patch in the high-nutrient, low-chlorophyll region of the eastern tropical Pacific with iron. Decade-long fertilization experiments are conducted in a basin-scale, eddy-permitting coupled physical biogeochemical ecological model. In contrast to previous studies, we find that most of the dissolved inorganic carbon (DIC) removed from the euphotic zone by the enhanced biological export is replaced by uptake of <span class="hlt">CO</span><span class="hlt">2</span> from the atmosphere. Atmospheric uptake efficiencies, the ratio of the perturbation in <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> to the perturbation in export <span class="hlt">flux</span> across 100 m, are 0.75 to 0.93 in our patch size-scale experiments. The atmospheric uptake efficiency is insensitive to the duration of the experiment. The primary factor controlling the atmospheric uptake efficiency is the vertical distribution of the enhanced biological production. Iron fertilization at the surface tends to induce production anomalies primarily near the surface, leading to high efficiencies. In contrast, mechanisms that induce deep production anomalies (e.g. altered light availability) tend to have a low uptake efficiency, since most of the removed DIC is replaced by lateral and vertical transport and mixing. Despite high atmospheric uptake efficiencies, patch-scale iron fertilization of the ocean's biological pump tends to remove little <span class="hlt">CO</span><span class="hlt">2</span> from the atmosphere over the decadal timescale considered here.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008BGeo....5..385J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008BGeo....5..385J"><span>The impact on atmospheric <span class="hlt">CO</span><span class="hlt">2</span> of iron fertilization induced changes in the ocean's biological pump</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jin, X.; Gruber, N.; Frenzel, H.; Doney, S. C.; McWilliams, J. C.</p> <p>2008-03-01</p> <p>Using numerical simulations, we quantify the impact of changes in the ocean's biological pump on the <span class="hlt">air-sea</span> balance of <span class="hlt">CO</span><span class="hlt">2</span> by fertilizing a small surface patch in the high-nutrient, low-chlorophyll region of the eastern tropical Pacific with iron. Decade-long fertilization experiments are conducted in a basin-scale, eddy-permitting coupled physical/biogeochemical/ecological model. In contrast to previous studies, we find that most of the dissolved inorganic carbon (DIC) removed from the euphotic zone by the enhanced biological export is replaced by uptake of <span class="hlt">CO</span><span class="hlt">2</span> from the atmosphere. Atmospheric uptake efficiencies, the ratio of the perturbation in <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> to the perturbation in export <span class="hlt">flux</span> across 100 m, integrated over 10 years, are 0.75 to 0.93 in our patch size-scale experiments. The atmospheric uptake efficiency is insensitive to the duration of the experiment. The primary factor controlling the atmospheric uptake efficiency is the vertical distribution of the enhanced biological production and export. Iron fertilization at the surface tends to induce production anomalies primarily near the surface, leading to high efficiencies. In contrast, mechanisms that induce deep production anomalies (e.g. altered light availability) tend to have a low uptake efficiency, since most of the removed DIC is replaced by lateral and vertical transport and mixing. Despite high atmospheric uptake efficiencies, patch-scale iron fertilization of the ocean's biological pump tends to remove little <span class="hlt">CO</span><span class="hlt">2</span> from the atmosphere over the decadal timescale considered here.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_13 --> <div id="page_14" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="261"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C33B1201H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C33B1201H"><span>The Impact of Moisture Intrusions from Lower Latitudes on Arctic Net Surface Radiative <span class="hlt">Fluxes</span> and <span class="hlt">Sea</span> Ice Growth in Fall and Winter</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hegyi, B. M.; Taylor, P. C.</p> <p>2017-12-01</p> <p>The fall and winter seasons mark an important period in the evolution of Arctic <span class="hlt">sea</span> ice, where energy is transferred away from the surface to facilitate the cooling of the surface and the growth of Arctic <span class="hlt">sea</span> ice extent and thickness. Climatologically, these seasons are characterized by distinct periods of increased and reduced surface cooling and <span class="hlt">sea</span> ice growth. Periods of reduced <span class="hlt">sea</span> ice growth and surface cooling are associated with cloudy conditions and the transport of warm and moist <span class="hlt">air</span> from lower latitudes, termed moisture intrusions. In the research presented, we explore the regional and Arctic-wide impact of moisture intrusions on the surface net radiative <span class="hlt">fluxes</span> and <span class="hlt">sea</span> ice growth for each fall and winter season from 2000/01-2015/16, utilizing MERRA<span class="hlt">2</span> reanalysis data, PIOMAS <span class="hlt">sea</span> ice thickness data, and daily CERES radiative <span class="hlt">flux</span> data. Consistent with previous studies, we find that positive anomalies in downwelling longwave surface <span class="hlt">flux</span> are associated with increased temperature and water vapor content in the atmospheric column contained within the moisture intrusions. Interestingly, there are periods of increased downwelling LW <span class="hlt">flux</span> anomalies that persist for one week or longer (i.e. longer than synoptic timescales) that are associated with persistent poleward <span class="hlt">flux</span> of warm, moist <span class="hlt">air</span> from lower latitudes. These persistent anomalies significantly reduce the regional growth of Arctic <span class="hlt">sea</span> ice, and may in part explain the interannual variability of fall and winter Arctic <span class="hlt">sea</span> ice growth.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.B53G0599C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.B53G0599C"><span>Year-round Regional <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Fluxes</span> from Boreal and Tundra Ecosystems in Alaska</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Commane, R.; Lindaas, J.; Benmergui, J. S.; Luus, K. A.; Chang, R. Y. W.; Daube, B. C.; Euskirchen, E. S.; Henderson, J.; Karion, A.; Miller, J. B.; Miller, S. M.; Parazoo, N.; Randerson, J. T.; Sweeney, C.; Tans, P. P.; Thoning, K. W.; Veraverbeke, S.; Miller, C. E.; Wofsy, S. C.</p> <p>2016-12-01</p> <p>High-latitude ecosystems could release large amounts of carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) to the atmosphere in a warmer climate. We derive temporally and spatially resolved year-round <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in Alaska from a synthesis of airborne and tower <span class="hlt">CO</span><span class="hlt">2</span> observations in 2012-2014. We find that tundra ecosystems were net sources of atmospheric <span class="hlt">CO</span><span class="hlt">2</span>. We discuss these <span class="hlt">flux</span> estimates in the context of long-term <span class="hlt">CO</span><span class="hlt">2</span> measurements at Barrow, AK, to asses the long term trend in carbon <span class="hlt">fluxes</span> in the Arctic. Many Earth System Models incorrectly simulate net carbon uptake in Alaska presently. Our results imply that annual net emission of <span class="hlt">CO</span><span class="hlt">2</span> to the atmosphere may have increased markedly in this region of the Arctic in response to warming climate, supporting the view that climate-carbon feedback is strongly positive in the high Arctic.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ClDy..tmp...93L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ClDy..tmp...93L"><span>Influence of <span class="hlt">air-sea</span> coupling on Indian Ocean tropical cyclones</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lengaigne, Matthieu; Neetu, S.; Samson, Guillaume; Vialard, Jérôme; Krishnamohan, K. S.; Masson, Sébastien; Jullien, Swen; Suresh, I.; Menkes, Christophe E.</p> <p>2018-02-01</p> <p>This paper assesses the impact of <span class="hlt">air-sea</span> coupling on Indian Ocean tropical cyclones (TCs) by comparing a 20-year long simulation of a ¼° regional coupled ocean-atmosphere model with a twin experiment, where the atmospheric component is forced by <span class="hlt">sea</span> surface temperature from the coupled simulation. The coupled simulation reproduces the observed spatio-temporal TCs distribution and TC-induced surface cooling reasonably well, but overestimates the number of TCs. <span class="hlt">Air-sea</span> coupling does not affect the cyclogenesis spatial distribution but reduces the number of TCs by 20% and yields a better-resolved bimodal seasonal distribution in the northern hemisphere. Coupling also affects intensity distribution, inducing a four-fold decrease in the proportion of intense TCs (Cat-<span class="hlt">2</span> and stronger). <span class="hlt">Air-sea</span> coupling damps TCs growth through a reduction of inner-core upward enthalpy <span class="hlt">fluxes</span> due to the TC-induced cooling. This reduction is particularly large for the most intense TCs of the northern Indian Ocean (up to 250 W m-<span class="hlt">2</span>), due to higher ambient surface temperatures and larger TC-induced cooling there. The negative feedback of <span class="hlt">air-sea</span> coupling on strongest TCs is mainly associated with slow-moving storms, which spend more time over the cold wake they induce. Sensitivity experiments using a different convective parameterization yield qualitatively similar results, with a larger ( 65%) reduction in the number of TCs. Because of their relatively coarse resolution (¼°), both set of experiments however fail to reproduce the most intense observed TCs. Further studies with finer resolution models in the Bay of Bengal will be needed to assess the expectedly large impact of <span class="hlt">air-sea</span> coupling on those intense and deadly TCs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhDT........17O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhDT........17O"><span>Observations and Modeling of Turbulent <span class="hlt">Air-Sea</span> Coupling in Coastal and Strongly Forced Condition</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ortiz-Suslow, David G.</p> <p></p> <p>The turbulent <span class="hlt">fluxes</span> of momentum, mass, and energy across the ocean-atmosphere boundary are fundamental to our understanding of a myriad of geophysical processes, such as wind-wave generation, oceanic circulation, and <span class="hlt">air-sea</span> gas transfer. In order to better understand these <span class="hlt">fluxes</span>, empirical relationships were developed to quantify the interfacial exchange rates in terms of easily observed parameters (e.g., wind speed). However, mounting evidence suggests that these empirical formulae are only valid over the relatively narrow parametric space, i.e. open ocean conditions in light to moderate winds. Several near-surface processes have been observed to cause significant variance in the <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> not predicted by the conventional functions, such as a heterogeneous surfaces, swell waves, and wave breaking. Further study is needed to fully characterize how these types of processes can modulate the interfacial exchange; in order to achieve this, a broad investigation into <span class="hlt">air-sea</span> coupling was undertaken. The primary focus of this work was to use a combination of field and laboratory observations and numerical modeling, in regimes where conventional theories would be expected to breakdown, namely: the nearshore and in very high winds. These seemingly disparate environments represent the marine atmospheric boundary layer at its physical limit. In the nearshore, the convergence of land, <span class="hlt">air</span>, and <span class="hlt">sea</span> in a depth-limited domain marks the transition from a marine to a terrestrial boundary layer. Under extreme winds, the physical nature of the boundary layer remains unknown as an intermediate substrate layer, <span class="hlt">sea</span> spray, develops between the atmosphere and ocean surface. At these ends of the MABL physical spectrum, direct measurements of the near-surface processes were made and directly related to local sources of variance. Our results suggest that the conventional treatment of <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> in terms of empirical relationships developed from a relatively narrow set of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013BVol...75..757M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013BVol...75..757M"><span>Soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> baseline in an urban monogenetic volcanic field: the Auckland Volcanic Field, New Zealand</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mazot, Agnès; Smid, Elaine R.; Schwendenmann, Luitgard; Delgado-Granados, Hugo; Lindsay, Jan</p> <p>2013-11-01</p> <p>The Auckland Volcanic Field (AVF) is a dormant monogenetic basaltic field located in Auckland, New Zealand. Though soil gas <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> are routinely used to monitor volcanic regions, there have been no published studies of soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> or soil gas <span class="hlt">CO</span><span class="hlt">2</span> concentrations in the AVF to date or many other monogenetic fields worldwide. We measured soil gas <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> and soil gas <span class="hlt">CO</span><span class="hlt">2</span> concentrations in 2010 and 2012 in varying settings, seasons, and times of day to establish a baseline soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> and to determine the major sources of and controlling influences on Auckland's soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span>. Soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> measurements varied from 0 to 203 g m-<span class="hlt">2</span> day-1, with an average of 27.1 g m-<span class="hlt">2</span> day-1. Higher <span class="hlt">fluxes</span> were attributed to varying land use properties (e.g., landfill). Using a graphical statistical approach, two populations of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> were identified. Isotope analyses of δ13<span class="hlt">CO</span><span class="hlt">2</span> confirmed that the source of <span class="hlt">CO</span><span class="hlt">2</span> in the AVF is biogenic with no volcanic component. These data may be used to assist with eruption forecasting in the event of precursory activity in the AVF, and highlight the importance of knowing land use history when assessing soil gas <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in urban environments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70021683','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70021683"><span>Estimating lake-atmosphere <span class="hlt">CO</span><span class="hlt">2</span> exchange</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Anderson, D.E.; Striegl, Robert G.; Stannard, D.I.; Michmerhuizen, C.M.; McConnaughey, T.A.; LaBaugh, J.W.</p> <p>1999-01-01</p> <p>Lake-atmosphere <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> was directly measured above a small, woodland lake using the eddy covariance technique and compared with <span class="hlt">fluxes</span> deduced from changes in measured lake-water <span class="hlt">CO</span><span class="hlt">2</span> storage and with <span class="hlt">flux</span> predictions from boundary-layer and surface-renewal models. Over a 3-yr period, lake-atmosphere exchanges of <span class="hlt">CO</span><span class="hlt">2</span> were measured over 5 weeks in spring, summer, and fall. Observed springtime <span class="hlt">CO</span><span class="hlt">2</span> efflux was large (<span class="hlt">2.3-2</span>.7 ??mol m-<span class="hlt">2</span> s-1) immediately after lake-thaw. That efflux decreased exponentially with time to less than 0.<span class="hlt">2</span> ??mol m-<span class="hlt">2</span> s-1 within <span class="hlt">2</span> weeks. Substantial interannual variability was found in the magnitudes of springtime efflux, surface water <span class="hlt">CO</span><span class="hlt">2</span> concentrations, lake <span class="hlt">CO</span><span class="hlt">2</span> storage, and meteorological conditions. Summertime measurements show a weak diurnal trend with a small average downward <span class="hlt">flux</span> (-0.17 ??mol m-<span class="hlt">2</span> s-1) to the lake's surface, while late fall <span class="hlt">flux</span> was trendless and smaller (-0.0021 ??mol m-<span class="hlt">2</span> s-1). Large springtime efflux afforded an opportunity to make direct measurement of lake-atmosphere <span class="hlt">fluxes</span> well above the detection limits of eddy covariance instruments, facilitating the testing of different gas <span class="hlt">flux</span> methodologies and <span class="hlt">air</span>-water gas-transfer models. Although there was an overall agreement in <span class="hlt">fluxes</span> determined by eddy covariance and those calculated from lake-water storage change in <span class="hlt">CO</span><span class="hlt">2</span>, agreement was inconsistent between eddy covariance <span class="hlt">flux</span> measurements and <span class="hlt">fluxes</span> predicted by boundary-layer and surface-renewal models. Comparison of measured and modeled transfer velocities for <span class="hlt">CO</span><span class="hlt">2</span>, along with measured and modeled cumulative <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span>, indicates that in most instances the surface-renewal model underpredicts actual <span class="hlt">flux</span>. Greater underestimates were found with comparisons involving homogeneous boundary-layer models. No physical mechanism responsible for the inconsistencies was identified by analyzing coincidentally measured environmental variables.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS42A..08S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS42A..08S"><span>Southern Ocean Carbon Dioxide and Oxygen <span class="hlt">Fluxes</span> Detected by SOCCOM Biogeochemical Profiling Floats</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sarmiento, J. L.; Bushinksy, S.; Gray, A. R.</p> <p>2016-12-01</p> <p>The Southern Ocean is known to play an important role in the global carbon cycle, yet historically our measurements of this remote region have been sparse and heavily biased towards summer. Here we present new estimates of <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> of carbon dioxide and oxygen calculated with measurements from autonomous biogeochemical profiling floats. At high latitudes in and southward of the Antarctic Circumpolar Current, we find a significant <span class="hlt">flux</span> of <span class="hlt">CO</span><span class="hlt">2</span> from the ocean to the atmosphere during 2014-2016, which is particularly enhanced during winter months. These results suggest that previous estimates may be biased towards stronger Southern Ocean <span class="hlt">CO</span><span class="hlt">2</span> uptake due to undersampling in winter. We examine various implications of having a source of <span class="hlt">CO</span><span class="hlt">2</span> that is higher than previous estimates. We also find that <span class="hlt">CO</span><span class="hlt">2</span>:O<span class="hlt">2</span> <span class="hlt">flux</span> ratios north of the Subtropical Front are positive, consistent with the <span class="hlt">fluxes</span> being driven by changes in solubility, while south of the Polar Front biological processes and upwelling of deep water combine to produce a negative <span class="hlt">CO</span><span class="hlt">2</span>:O<span class="hlt">2</span> <span class="hlt">flux</span> ratio.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1255257-co2-fluxing-collapses-metal-mobility-magmatic-vapour','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1255257-co2-fluxing-collapses-metal-mobility-magmatic-vapour"><span><span class="hlt">CO</span> <span class="hlt">2</span>-<span class="hlt">fluxing</span> collapses metal mobility in magmatic vapour</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>van Hinsberg, V. J.; Berlo, K.; Migdisov, A. A.; ...</p> <p>2016-05-18</p> <p>Magmatic systems host many types of ore deposits, including world-class deposits of copper and gold. Magmas are commonly an important source of metals and ore-forming fluids in these systems. In many magmatic-hydrothermal systems, low-density aqueous fluids, or vapours, are significant metal carriers. Such vapours are water-dominated shallowly, but <span class="hlt">fluxing</span> of <span class="hlt">CO</span> <span class="hlt">2</span>-rich vapour exsolved from deeper magma is now recognised as ubiquitous during open-system magma degassing. Furthermore, we show that such <span class="hlt">CO</span> <span class="hlt">2</span>-<span class="hlt">fluxing</span> leads to a sharp drop in element solubility, up to a factor of 10,000 for Cu, and thereby provides a highly efficient, but as yet unrecognised mechanismmore » for metal deposition.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.9500M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.9500M"><span>Spume Drops: Their Potential Role in <span class="hlt">Air-Sea</span> Gas Exchange</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Monahan, Edward C.; Staniec, Allison; Vlahos, Penny</p> <p>2017-12-01</p> <p>After summarizing the time scales defining the change of the physical properties of spume and other droplets cast up from the <span class="hlt">sea</span> surface, the time scales governing drop-atmosphere gas exchange are compared. Following a broad review of the spume drop production functions described in the literature, a subset of these functions is selected via objective criteria, to represent typical, upper bound, and lower bound production functions. Three complementary mechanisms driving spume-atmosphere gas exchange are described, and one is then used to estimate the relative importance, over a broad range of wind speeds, of this spume drop mechanism compared to the conventional, diffusional, <span class="hlt">sea</span> surface mechanism in <span class="hlt">air-sea</span> gas exchange. While remaining uncertainties in the wind dependence of the spume drop production <span class="hlt">flux</span>, and in the immediate <span class="hlt">sea</span> surface gas <span class="hlt">flux</span>, preclude a definitive conclusion, the findings of this study strongly suggest that, at high wind speeds (>20 m s-1 for dimethyl sulfide and >30 m s-1 for gases such a carbon dioxide), spume drops do make a significant contribution to <span class="hlt">air-sea</span> gas exchange.<abstract type="synopsis"><title type="main">Plain Language SummaryThis paper evaluates the existing spume drop generation functions available to date and selects a reasonable upper, lower and mid range function that are reasonable for use in <span class="hlt">air</span> <span class="hlt">sea</span> exchange models. Based on these the contribution of spume drops to overall <span class="hlt">air</span> <span class="hlt">sea</span> gas exchange at different wind speeds is then evaluated to determine the % contribution of spume. Generally below 20ms-1 spume drops contribute <1% of gas exchange but may account for a significant amount of gas exchange at higher wind speeds.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.B41E0110R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.B41E0110R"><span><span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Flux</span> From Antarctic Dry Valley Soils: Determining the Source and Environmental Controls</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Risk, D. A.; Macintyre, C. M.; Shanhun, F.; Almond, P. C.; Lee, C.; Cary, C.</p> <p>2014-12-01</p> <p>Soils within the McMurdo Dry Valleys are known to respire carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>), but considerable debate surrounds the contributing sources and mechanisms that drive temporal variability. While some of the <span class="hlt">CO</span><span class="hlt">2</span> is of biological origin, other known contributors to variability include geochemical sources within, or beneath, the soil column. The relative contribution from each of these sources will depend on seasonal and environmental drivers such as temperature and wind that exert influence on temporal dynamics. To supplement a long term <span class="hlt">CO</span><span class="hlt">2</span>­ surface <span class="hlt">flux</span> monitoring station that has now recorded <span class="hlt">fluxes</span> over three full annual cycles, in January 2014 an automated <span class="hlt">flux</span> and depth concentration monitoring system was installed in the Spaulding Pond area of Taylor Valley, along with standard meteorological sensors, to assist in defining source contributions through time. During two weeks of data we observed marked diel variability in <span class="hlt">CO</span><span class="hlt">2</span> concentrations within the profile (~100 ppm <span class="hlt">CO</span><span class="hlt">2</span> above or below atmospheric), and of <span class="hlt">CO</span><span class="hlt">2</span> moving across the soil surface. The pattern at many depths suggested an alternating diel-scale transition from source to sink that seemed clearly correlated with temperature-driven changes in the solubility of <span class="hlt">CO</span><span class="hlt">2</span> in water films. This <span class="hlt">CO</span><span class="hlt">2</span> solution storage <span class="hlt">flux</span> was very highly coupled to soil temperature. A small depth source of unknown origin also appeared to be present. A controlled laboratory soil experiment was conducted to confirm the magnitude of <span class="hlt">fluxes</span> into and out of soil water films, and confirmed the field results and temperature dependence. Ultimately, this solution storage <span class="hlt">flux</span> needs to be well understood if the small biological <span class="hlt">fluxes</span> from these soils are to be properly quantified and monitored for change. Here, we present results from the 2013/2014 field season and these supplementary experiments, placed in the context of 3 year long term continuous measurement of soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> within the Dry Valleys.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.A32F..08C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.A32F..08C"><span>Constraining the Stratosphere-Troposphere Exchange of Radiocarbon using <span class="hlt">Air</span>Core 14<span class="hlt">CO</span><span class="hlt">2</span> Measurements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, H.</p> <p>2016-12-01</p> <p>Radiocarbon (14C) plays an important role in the carbon cycle studies to understand both natural and anthropogenic carbon <span class="hlt">fluxes</span>, but also in atmospheric chemistry to constrain hydroxyl radical (OH) concentrations in the atmosphere. Apart from the enormous 14C emissions from nuclear bomb testing in the 1950s and 1960s, radiocarbon is primarily produced in the upper atmosphere due to reactions of nitrogen nuclei with thermal neutrons that are induced by cosmic rays. 14C is quickly oxidized to 14<span class="hlt">CO</span>, which is then further oxidized to 14<span class="hlt">CO</span><span class="hlt">2</span> by OH. To this end, better understanding the radiocarbon source is very useful to advance the use of radiocarbon for these applications. However, upper atmospheric 14C observations have been very sparse to constrain the magnitude and the location of the 14C production as well as the transport of radiocarbon from the stratosphere to the troposphere. Recently we have successfully made stratospheric 14<span class="hlt">CO</span><span class="hlt">2</span> measurements using <span class="hlt">Air</span>Core samples from Sodankylä, Northern Finland, along with regular <span class="hlt">Air</span>Core profiles of <span class="hlt">CO</span><span class="hlt">2</span>, CH4, and <span class="hlt">CO</span> since 2013. In this study, we calculate the stratosphere-troposphere exchange of 14C using the correlation between 14<span class="hlt">CO</span><span class="hlt">2</span> and N<span class="hlt">2</span>O, and the estimated N<span class="hlt">2</span>O loss rate. Besides this, we assess the impact of the mean age of <span class="hlt">air</span> on 14<span class="hlt">CO</span><span class="hlt">2</span> profiles. Furthermore, we will evaluate the influence of different cosmogenic 14C production scenarios and the uncertainties in the OH field on the seasonal cycles of radiocarbon and on the stratosphere-troposphere exchange.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018BGeo...15.2851P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018BGeo...15.2851P"><span>The seasonal cycle of p<span class="hlt">CO</span><span class="hlt">2</span> and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in the Southern Ocean: diagnosing anomalies in CMIP5 Earth system models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Precious Mongwe, N.; Vichi, Marcello; Monteiro, Pedro M. S.</p> <p>2018-05-01</p> <p>The Southern Ocean forms an important component of the Earth system as a major sink of <span class="hlt">CO</span><span class="hlt">2</span> and heat. Recent studies based on the Coupled Model Intercomparison Project version 5 (CMIP5) Earth system models (ESMs) show that CMIP5 models disagree on the phasing of the seasonal cycle of the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> (FCO<span class="hlt">2</span>) and compare poorly with available observation products for the Southern Ocean. Because the seasonal cycle is the dominant mode of <span class="hlt">CO</span><span class="hlt">2</span> variability in the Southern Ocean, its simulation is a rigorous test for models and their long-term projections. Here we examine the competing roles of temperature and dissolved inorganic carbon (DIC) as drivers of the seasonal cycle of p<span class="hlt">CO</span><span class="hlt">2</span> in the Southern Ocean to explain the mechanistic basis for the seasonal biases in CMIP5 models. We find that despite significant differences in the spatial characteristics of the mean annual <span class="hlt">fluxes</span>, the intra-model homogeneity in the seasonal cycle of FCO<span class="hlt">2</span> is greater than observational products. FCO<span class="hlt">2</span> biases in CMIP5 models can be grouped into two main categories, i.e., group-SST and group-DIC. Group-SST models show an exaggeration of the seasonal rates of change of <span class="hlt">sea</span> surface temperature (SST) in autumn and spring during the cooling and warming peaks. These higher-than-observed rates of change of SST tip the control of the seasonal cycle of p<span class="hlt">CO</span><span class="hlt">2</span> and FCO<span class="hlt">2</span> towards SST and result in a divergence between the observed and modeled seasonal cycles, particularly in the Sub-Antarctic Zone. While almost all analyzed models (9 out of 10) show these SST-driven biases, 3 out of 10 (namely NorESM1-ME, HadGEM-ES and MPI-ESM, collectively the group-DIC models) compensate for the solubility bias because of their overly exaggerated primary production, such that biologically driven DIC changes mainly regulate the seasonal cycle of FCO<span class="hlt">2</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.7685S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.7685S"><span>Concurrent <span class="hlt">CO</span><span class="hlt">2</span> and COS <span class="hlt">fluxes</span> across major biomes in Europe</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Spielmann, Felix M.; Kitz, Florian; Hammerle, Albin; Gerdel, Katharina; Ibrom, Andreas; Kolle, Olaf; Migliavacca, Mirco; Moreno, Gerardo; Noe, Steffen M.; Wohlfahrt, Georg</p> <p>2017-04-01</p> <p>The trace gas carbonyl sulfide (COS) has been proposed as a tracer for canopy gross primary production (GPP), canopy transpiration and stomatal conductance of plant canopies in the last few years. COS enters the plant leaf through the stomata and diffuses through the intercellular space, the cell wall, the plasma membrane and the cytosol like carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>). It is then catalyzed by the enzyme carbonic anhydrase in a one-way reaction to hydrogen sulfide and <span class="hlt">CO</span><span class="hlt">2</span>. This one-way <span class="hlt">flux</span> into the leaf makes COS a promising tracer for the GPP. However, this approach assumes that the ratio of the deposition velocities between COS and <span class="hlt">CO</span><span class="hlt">2</span> is constant, which must be determined in field experiments covering a wide variety of ecosystems. The overarching objective of this study was to quantify the relationship between the ecosystem-scale exchange of COS and <span class="hlt">CO</span><span class="hlt">2</span> and thus, to test for the potential of COS to be used as a universal tracer for the plant canopy <span class="hlt">CO</span><span class="hlt">2</span> exchange. Between spring 2015 and summer 2016 we set up our quantum cascade laser at different field sites across Europe. These sites included a managed temperate mountain grassland (AUT), a savanna (ESP), a temperate beech forest (DEN) and a hemiboreal forest (EST). On each of these sites, we conducted ecosystem scale eddy covariance and soil chamber measurements. Since the soil COS <span class="hlt">flux</span> contribution, especially in grass dominated ecosystems, could not be neglected, we had to derive the actual canopy COS <span class="hlt">fluxes</span> for all the measurement sites. Using these <span class="hlt">fluxes</span> we compared the ecosystem relative uptake (ERU) of the sites and searched for factors affecting its variability. We then used the influential factors to scale the ERU to be comparable under different field sites and conditions. Furthermore we also calculated the GPP using conventional <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> partitioning and compared the results with the approach of using the leaf relative uptake.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20103140','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20103140"><span><span class="hlt">CO</span><span class="hlt">2</span> volume <span class="hlt">fluxes</span> outgassing from champagne glasses: the impact of champagne ageing.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Liger-Belair, Gérard; Villaume, Sandra; Cilindre, Clara; Jeandet, Philippe</p> <p>2010-02-15</p> <p>It was demonstrated that <span class="hlt">CO</span>(<span class="hlt">2</span>) volume <span class="hlt">fluxes</span> outgassing from a flute poured with a young champagne (elaborated in 2007) are much higher than those outgassing from the same flute poured with an older champagne (elaborated in the early 1990s). The difference in dissolved-<span class="hlt">CO</span>(<span class="hlt">2</span>) concentrations between the two types of champagne samples was found to be a crucial parameter responsible for differences in <span class="hlt">CO</span>(<span class="hlt">2</span>) volume <span class="hlt">fluxes</span> outgassing from one champagne to another. Nevertheless, it was shown that, for a given identical dissolved-<span class="hlt">CO</span>(<span class="hlt">2</span>) concentration in both champagne types, the <span class="hlt">CO</span>(<span class="hlt">2</span>) volume <span class="hlt">flux</span> outgassing from the flute poured with the old champagne is, in average, significantly lower than that outgassing from the flute poured with the young one. Therefore, <span class="hlt">CO</span>(<span class="hlt">2</span>) seems to "escape" more easily from the young champagne than from the older one. The diffusion coefficient of <span class="hlt">CO</span>(<span class="hlt">2</span>) in both champagne types was pointed as a key parameter to thoroughly determine in the future, in order to unravel our experimental observation. Copyright 2009 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ACP....18.6001G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ACP....18.6001G"><span>The effects of <span class="hlt">sea</span> spray and atmosphere-wave coupling on <span class="hlt">air-sea</span> exchange during a tropical cyclone</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Garg, Nikhil; Kwee Ng, Eddie Yin; Narasimalu, Srikanth</p> <p>2018-04-01</p> <p>The study investigates the role of the <span class="hlt">air-sea</span> interface using numerical simulations of Hurricane Arthur (2014) in the Atlantic. More specifically, the present study aims to discern the role ocean surface waves and <span class="hlt">sea</span> spray play in modulating the intensity and structure of a tropical cyclone (TC). To investigate the effects of ocean surface waves and <span class="hlt">sea</span> spray, numerical simulations were carried out using a coupled atmosphere-wave model, whereby a <span class="hlt">sea</span> spray microphysical model was incorporated within the coupled model. Furthermore, this study also explores how <span class="hlt">sea</span> spray generation can be modelled using wave energy dissipation due to whitecaps; whitecaps are considered as the primary mode of spray droplets generation at hurricane intensity wind speeds. Three different numerical simulations including the <span class="hlt">sea</span>- state-dependent momentum <span class="hlt">flux</span>, the <span class="hlt">sea</span>-spray-mediated heat <span class="hlt">flux</span>, and a combination of the former two processes with the <span class="hlt">sea</span>-spray-mediated momentum <span class="hlt">flux</span> were conducted. The foregoing numerical simulations were evaluated against the National Data Buoy Center (NDBC) buoy and satellite altimeter measurements as well as a control simulation using an uncoupled atmosphere model. The results indicate that the model simulations were able to capture the storm track and intensity: the surface wave coupling results in a stronger TC. Moreover, it is also noted that when only spray-mediated heat <span class="hlt">fluxes</span> are applied in conjunction with the <span class="hlt">sea</span>-state-dependent momentum <span class="hlt">flux</span>, they result in a slightly weaker TC, albeit stronger compared to the control simulation. However, when a spray-mediated momentum <span class="hlt">flux</span> is applied together with spray heat <span class="hlt">fluxes</span>, it results in a comparably stronger TC. The results presented here allude to the role surface friction plays in the intensification of a TC.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A31O..02S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A31O..02S"><span>Interpreting OCO-<span class="hlt">2</span> Constrained <span class="hlt">CO</span><span class="hlt">2</span> Surface <span class="hlt">Flux</span> Estimates Through the Lens of Atmospheric Transport Uncertainty.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schuh, A. E.; Jacobson, A. R.; Basu, S.; Weir, B.; Baker, D. F.; Bowman, K. W.; Chevallier, F.; Crowell, S.; Deng, F.; Denning, S.; Feng, L.; Liu, J.</p> <p>2017-12-01</p> <p>The orbiting carbon observatory (OCO-<span class="hlt">2</span>) was launched in July 2014 and has collected three years of column mean <span class="hlt">CO</span><span class="hlt">2</span> (XCO<span class="hlt">2</span>) data. The OCO-<span class="hlt">2</span> model inter-comparison project (MIP) was formed to provide a means of analysis of results from many different atmospheric inversion modeling systems. Certain facets of the inversion systems, such as observations and fossil fuel <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> were standardized to remove first order sources of difference between the systems. Nevertheless, large variations amongst the <span class="hlt">flux</span> results from the systems still exist. In this presentation, we explore one dimension of this uncertainty, the impact of different atmospheric transport fields, i.e. wind speeds and directions. Early results illustrate a large systematic difference between two classes of atmospheric transport, arising from winds in the parent GEOS-DAS (NASA-GMAO) and ERA-Interim (ECMWF) data assimilation models. We explore these differences and their effect on inversion-based estimates of surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> by using a combination of simplified inversion techniques as well as the full OCO-<span class="hlt">2</span> MIP suite of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> estimates.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20527160','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20527160"><span>[Characteristics of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> before and in the heating period at urban complex underlying surface area].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Jia, Qing-yu; Zhou, Guang-sheng; Wang, Yu; Liu, Xiao-mei</p> <p>2010-04-01</p> <p>Urban areas were significant contributors to global carbon dioxide emissions. The eddy covariance (EC) was used to measure carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) concentration and <span class="hlt">flux</span> data at urban area in Shenyang. This research analyzed the characteristics of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentration and <span class="hlt">flux</span> in October 2008 to November 2008 period before and in the heating period. The results showed that the daily variation of <span class="hlt">CO</span><span class="hlt">2</span> concentration was two-peak curve. The first peak time appeared as same as sunrise time, while the second peak time impacted by vehicles and heating. The result of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> showed that urban atmospheric <span class="hlt">CO</span><span class="hlt">2</span> was net emissions, vegetation photosynthesis absorbed <span class="hlt">CO</span><span class="hlt">2</span> of traffic, the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> peak appeared at 17:15-18:15 in the heating period, <span class="hlt">CO</span><span class="hlt">2</span> emission increased 29.37 g x (m<span class="hlt">2</span> x d)(-1) in the heating period than that before the heating period; there was corresponding relationship between <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> and the time when temperature peak and sensible heating <span class="hlt">flux</span> (Hc) turn positive. The results also indicated that atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentration and its <span class="hlt">flux</span> were affected seriously by both wind direction and carbon sources.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/sir/2009/5061/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/sir/2009/5061/"><span>Soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Flux</span> in the Amargosa Desert, Nevada, during El Nino 1998 and La Nina 1999</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Riggs, Alan C.; Stannard, David I.; Maestas, Florentino B.; Karlinger, Michael R.; Striegl, Robert G.</p> <p>2009-01-01</p> <p>Mean annual soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> from normally bare mineral soil in the Amargosa Desert in southern Nevada, United States, measured with clear and opaque soil <span class="hlt">CO</span><span class="hlt">2</span>-<span class="hlt">flux</span> chambers (autochambers) were small - <5 millimoles per square meter per day - during both El Nino 1998 and La Nina 1999. The 1998 opaque-chamber <span class="hlt">flux</span> exceeded 1999 opaque-chamber <span class="hlt">flux</span> by an order of magnitude, whereas the 1998 clear-chamber <span class="hlt">flux</span> exceeded 1999 clear-chamber <span class="hlt">flux</span> by less than a factor of two. These data suggest that above-normal soil moisture stimulated increased metabolic activity, but that much of the extra <span class="hlt">CO</span><span class="hlt">2</span> produced was recaptured by plants. <span class="hlt">Fluxes</span> from warm moist soil were the largest sustained <span class="hlt">fluxes</span> measured, and their hourly pattern is consistent with enhanced soil metabolic activity at some depth in the soil and photosynthetic uptake of a substantial portion of the <span class="hlt">CO</span><span class="hlt">2</span> released. <span class="hlt">Flux</span> from cool moist soil was smaller than <span class="hlt">flux</span> from warm moist soil. <span class="hlt">Flux</span> from hot dry soil was intermediate between warm-moist and cool-moist <span class="hlt">fluxes</span>, and clear-chamber <span class="hlt">flux</span> was more than double the opaque-chamber <span class="hlt">flux</span>, apparently due to a chamber artifact stemming from a thermally controlled <span class="hlt">CO</span><span class="hlt">2</span> reservoir near the soil surface. There was no demonstrable metabolic contribution to the very small <span class="hlt">flux</span> from cool dry soil, which was dominated by diffusive up-<span class="hlt">flux</span> of <span class="hlt">CO</span><span class="hlt">2</span> from the water table and temperature-controlled <span class="hlt">CO</span><span class="hlt">2</span>-reservoir up- and down-<span class="hlt">fluxes</span>. These <span class="hlt">flux</span> patterns suggest that transfer of <span class="hlt">CO</span><span class="hlt">2</span> across the land surface is a complex process that is difficult to accurately measure.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22445955','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22445955"><span>Responses of CH(4), <span class="hlt">CO</span>(<span class="hlt">2</span>) and N(<span class="hlt">2</span>)O <span class="hlt">fluxes</span> to increasing nitrogen deposition in alpine grassland of the Tianshan Mountains.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Li, Kaihui; Gong, Yanming; Song, Wei; He, Guixiang; Hu, Yukun; Tian, Changyan; Liu, Xuejun</p> <p>2012-06-01</p> <p>To assess the effects of nitrogen (N) deposition on greenhouse gas (GHG) <span class="hlt">fluxes</span> in alpine grassland of the Tianshan Mountains in central Asia, CH(4), <span class="hlt">CO</span>(<span class="hlt">2</span>) and N(<span class="hlt">2</span>)O <span class="hlt">fluxes</span> were measured from June 2010 to May 2011. Nitrogen deposition tended to significantly increase CH(4) uptake, <span class="hlt">CO</span>(<span class="hlt">2</span>) and N(<span class="hlt">2</span>)O emissions at sites receiving N addition compared with those at site without N addition during the growing season, but no significant differences were found for all sites outside the growing season. <span class="hlt">Air</span> temperature, soil temperature and water content were the important factors that influence <span class="hlt">CO</span>(<span class="hlt">2</span>) and N(<span class="hlt">2</span>)O emissions at year-round scale, indicating that increased temperature and precipitation in the future will exert greater impacts on <span class="hlt">CO</span>(<span class="hlt">2</span>) and N(<span class="hlt">2</span>)O emissions in the alpine grassland. In addition, plant coverage in July was also positively correlated with <span class="hlt">CO</span>(<span class="hlt">2</span>) and N(<span class="hlt">2</span>)O emissions under elevated N deposition rates. The present study will deepen our understanding of N deposition impacts on GHG balance in the alpine grassland ecosystem, and help us assess the global N effects, parameterize Earth System models and inform decision makers. Copyright © 2012 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.2333B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.2333B"><span>On the importance of high-frequency <span class="hlt">air</span>-temperature fluctuations for spectroscopic corrections of open-path carbon dioxide <span class="hlt">flux</span> measurements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bogoev, Ivan; Helbig, Manuel; Sonnentag, Oliver</p> <p>2015-04-01</p> <p>A growing number of studies report systematic differences in <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> estimates obtained with the two main types of gas analyzers: compared to eddy-covariance systems based on closed-path (CP) gas analyzers, systems with open-path (OP) gas analyzers systematically overestimate <span class="hlt">CO</span><span class="hlt">2</span> uptake during daytime periods with high positive sensible heat <span class="hlt">fluxes</span>, while patterns for differences in nighttime <span class="hlt">CO</span><span class="hlt">2</span> exchange are less obvious. These biases have been shown to correlate with the sign and the magnitude of the sensible heat <span class="hlt">flux</span> and to introduce large uncertainties when calculating annual <span class="hlt">CO</span><span class="hlt">2</span> budgets. In general, CP and OP gas analyzers commonly used to measure the <span class="hlt">CO</span><span class="hlt">2</span> density in the atmosphere operate on the principle of infrared light absorption approximated by Beer-Lambert's law. Non-dispersive interference-based optical filter elements are used to select spectral bands with strong attenuation of light transmission, characteristic to the gas of interest. The intensity of the light passing through the optical sensing path depends primarily on the amount of absorber gas in the measurement volume. Besides the density of the gas, barometric pressure and <span class="hlt">air</span> temperature are additional factors affecting the strength and the half-width of the absorption lines. These so-called spectroscopic effects are accounted for by measuring barometric pressure and <span class="hlt">air</span> temperature in the sensing path and scaling the light-intensity measurements before applying the calibration equation. This approach works well for CP gas analyzers with an intake tube that acts as a low-pass filter on fast <span class="hlt">air</span>-temperature fluctuations. Low-frequency response temperature sensors in the measurement cell are therefore sufficient to account for spectroscopic temperature effects. In contrast, OP gas analyzers are exposed to high-frequency <span class="hlt">air</span>-temperature fluctuations associated with the atmospheric surface-layer turbulent heat exchange. If not corrected adequately, these fast <span class="hlt">air</span>-temperature variations can cause</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_14 --> <div id="page_15" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="281"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20000038180&hterms=dependency&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Ddependency','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20000038180&hterms=dependency&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Ddependency"><span>The Role of <span class="hlt">Sea</span> Ice in <span class="hlt">2</span> x <span class="hlt">CO</span><span class="hlt">2</span> Climate Model Sensitivity. Part <span class="hlt">2</span>; Hemispheric Dependencies</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rind, D.; Healy, R.; Parkinson, C.; Martinson, D.</p> <p>1997-01-01</p> <p>How sensitive are doubled <span class="hlt">CO</span><span class="hlt">2</span> simulations to GCM control-run <span class="hlt">sea</span> ice thickness and extent? This issue is examined in a series of 10 control-run simulations with different <span class="hlt">sea</span> ice and corresponding doubled <span class="hlt">CO</span><span class="hlt">2</span> simulations. Results show that with increased control-run <span class="hlt">sea</span> ice coverage in the Southern Hemisphere, temperature sensitivity with climate change is enhanced, while there is little effect on temperature sensitivity of (reasonable) variations in control-run <span class="hlt">sea</span> ice thickness. In the Northern Hemisphere the situation is reversed: <span class="hlt">sea</span> ice thickness is the key parameter, while (reasonable) variations in control-run <span class="hlt">sea</span> ice coverage are of less importance. In both cases, the quantity of <span class="hlt">sea</span> ice that can be removed in the warmer climate is the determining factor. Overall, the Southern Hemisphere <span class="hlt">sea</span> ice coverage change had a larger impact on global temperature, because Northern Hemisphere <span class="hlt">sea</span> ice was sufficiently thick to limit its response to doubled <span class="hlt">CO</span><span class="hlt">2</span>, and <span class="hlt">sea</span> ice changes generally occurred at higher latitudes, reducing the <span class="hlt">sea</span> ice-albedo feedback. In both these experiments and earlier ones in which <span class="hlt">sea</span> ice was not allowed to change, the model displayed a sensitivity of -0.02 C global warming per percent change in Southern Hemisphere <span class="hlt">sea</span> ice coverage.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012JGRD..11711303N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012JGRD..11711303N"><span>Imposing strong constraints on tropical terrestrial <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> using passenger aircraft based measurements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Niwa, Yosuke; Machida, Toshinobu; Sawa, Yousuke; Matsueda, Hidekazu; Schuck, Tanja J.; Brenninkmeijer, Carl A. M.; Imasu, Ryoichi; Satoh, Masaki</p> <p>2012-06-01</p> <p>Because very few measurements of atmospheric carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) are available in the tropics, estimates of surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in tropical regions are beset with considerable uncertainties. To improve estimates of tropical terrestrial <span class="hlt">fluxes</span>, atmospheric <span class="hlt">CO</span><span class="hlt">2</span> inversion was performed using passenger aircraft based measurements of the Comprehensive Observation Network for Trace gases by Airliner (CONTRAIL) project in addition to the surface measurement data set of GLOBALVIEW-<span class="hlt">CO</span><span class="hlt">2</span>. Regional monthly <span class="hlt">fluxes</span> at the earth's surface were estimated using the Bayesian synthesis approach focusing on the period 2006-2008 using the Nonhydrostatic Icosahedral Atmospheric Model-based Transport Model (NICAM-TM). By adding the aircraft to the surface data, the posterior <span class="hlt">flux</span> errors were greatly reduced; specifically, error reductions of up to 64% were found for tropical Asia regions. This strong impact is closely related to efficient vertical transport in the tropics. The optimized surface <span class="hlt">fluxes</span> using the CONTRAIL data were evaluated by comparing the simulated atmospheric <span class="hlt">CO</span><span class="hlt">2</span> distributions with independent aircraft measurements of the Civil Aircraft for the Regular Investigation of the atmosphere Based on an Instrument Container (CARIBIC) project. The inversion with the CONTRAIL data yields the global carbon sequestration rates of <span class="hlt">2</span>.22 ± 0.28 Pg C yr-1 for the terrestrial biosphere and <span class="hlt">2</span>.24 ± 0.27 Pg C yr-1 for the oceans (the both are adjusted by riverine input of <span class="hlt">CO</span><span class="hlt">2</span>). For the first time the CONTRAIL <span class="hlt">CO</span><span class="hlt">2</span> measurements were used in an inversion system to identify the areas of greatest impact in terms of reducing <span class="hlt">flux</span> uncertainties.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA462427','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA462427"><span>Residual-Mean Analysis of the <span class="hlt">Air-Sea</span> <span class="hlt">Fluxes</span> and Associated Oceanic Meridional Overturning</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2006-12-01</p> <p>the adiabatic component of the MOC which is based entirely on the <span class="hlt">sea</span> surface data . The coordinate system introduced in this study is somewhat...heat capacity of water. The technique utilizes the observational data based on meteorological re- analysis (density <span class="hlt">flux</span> at the <span class="hlt">sea</span> surface) and...Figure 8. Annual mean and temporal standard deviation of the zonally-averaged mixed- layer depth. The plotted data are based on Levitus 94 climatology</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.6688K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.6688K"><span>Comparison of Source Partitioning Methods for <span class="hlt">CO</span><span class="hlt">2</span> and H<span class="hlt">2</span>O <span class="hlt">Fluxes</span> Based on High Frequency Eddy Covariance Data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Klosterhalfen, Anne; Moene, Arnold; Schmidt, Marius; Ney, Patrizia; Graf, Alexander</p> <p>2017-04-01</p> <p>Source partitioning of eddy covariance (EC) measurements of <span class="hlt">CO</span><span class="hlt">2</span> into respiration and photosynthesis is routinely used for a better understanding of the exchange of greenhouse gases, especially between terrestrial ecosystems and the atmosphere. The most frequently used methods are usually based either on relations of <span class="hlt">fluxes</span> to environmental drivers or on chamber measurements. However, they often depend strongly on assumptions or invasive measurements and do usually not offer partitioning estimates for latent heat <span class="hlt">fluxes</span> into evaporation and transpiration. SCANLON and SAHU (2008) and SCANLON and KUSTAS (2010) proposed an promising method to estimate the contributions of transpiration and evaporation using measured high frequency time series of <span class="hlt">CO</span><span class="hlt">2</span> and H<span class="hlt">2</span>O <span class="hlt">fluxes</span> - no extra instrumentation necessary. This method (SK10 in the following) is based on the spatial separation and relative strength of sources and sinks of <span class="hlt">CO</span><span class="hlt">2</span> and water vapor among the sub-canopy and canopy. Assuming that <span class="hlt">air</span> from those sources and sinks is not yet perfectly mixed before reaching EC sensors, partitioning is estimated based on the separate application of the <span class="hlt">flux</span>-variance similarity theory to the stomatal and non-stomatal components of the regarded <span class="hlt">fluxes</span>, as well as on additional assumptions on stomatal water use efficiency (WUE). The <span class="hlt">CO</span><span class="hlt">2</span> partitioning method after THOMAS et al. (2008) (TH08 in the following) also follows the argument that the dissimilarities of sources and sinks in and below a canopy affect the relation between H<span class="hlt">2</span>O and <span class="hlt">CO</span><span class="hlt">2</span> fluctuations. Instead of involving assumptions on WUE, TH08 directly screens their scattergram for signals of joint respiration and evaporation events and applies a conditional sampling methodology. In spite of their different main targets (H<span class="hlt">2</span>O vs. <span class="hlt">CO</span><span class="hlt">2</span>), both methods can yield partitioning estimates on both <span class="hlt">fluxes</span>. We therefore compare various sub-methods of SK10 and TH08 including own modifications (e.g., cluster analysis) to each other, to established</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017CSR...145...95R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017CSR...145...95R"><span>Time series p<span class="hlt">CO</span><span class="hlt">2</span> at a coastal mooring: Internal consistency, seasonal cycles, and interannual variability</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Reimer, Janet J.; Cai, Wei-Jun; Xue, Liang; Vargas, Rodrigo; Noakes, Scott; Hu, Xinping; Signorini, Sergio R.; Mathis, Jeremy T.; Feely, Richard A.; Sutton, Adrienne J.; Sabine, Christopher; Musielewicz, Sylvia; Chen, Baoshan; Wanninkhof, Rik</p> <p>2017-08-01</p> <p>Marine carbonate system monitoring programs often consist of multiple observational methods that include underway cruise data, moored autonomous time series, and discrete water bottle samples. Monitored parameters include all, or some of the following: partial pressure of <span class="hlt">CO</span><span class="hlt">2</span> of the water (p<span class="hlt">CO</span><span class="hlt">2</span>w) and <span class="hlt">air</span>, dissolved inorganic carbon (DIC), total alkalinity (TA), and pH. Any combination of at least two of the aforementioned parameters can be used to calculate the others. In this study at the Gray's Reef (GR) mooring in the South Atlantic Bight (SAB) we: examine the internal consistency of p<span class="hlt">CO</span><span class="hlt">2</span>w from underway cruise, moored autonomous time series, and calculated from bottle samples (DIC-TA pairing); describe the seasonal to interannual p<span class="hlt">CO</span><span class="hlt">2</span>w time series variability and <span class="hlt">air-sea</span> <span class="hlt">flux</span> (FCO<span class="hlt">2</span>), as well as describe the potential sources of p<span class="hlt">CO</span><span class="hlt">2</span>w variability; and determine the source/sink for atmospheric p<span class="hlt">CO</span><span class="hlt">2</span>. Over the 8.5 years of GR mooring time series, mooring-underway and mooring-bottle calculated-p<span class="hlt">CO</span><span class="hlt">2</span>w strongly correlate with r-values > 0.90. p<span class="hlt">CO</span><span class="hlt">2</span>w and FCO<span class="hlt">2</span> time series follow seasonal thermal patterns; however, seasonal non-thermal processes, such as terrestrial export, net biological production, and <span class="hlt">air-sea</span> exchange also influence variability. The linear slope of time series p<span class="hlt">CO</span><span class="hlt">2</span>w increases by 5.<span class="hlt">2</span> ± 1.4 μatm y-1 with FCO<span class="hlt">2</span> increasing 51-70 mmol m-<span class="hlt">2</span> y-1. The net FCO<span class="hlt">2</span> sign can switch interannually with the magnitude varying greatly. Non-thermal p<span class="hlt">CO</span><span class="hlt">2</span>w is also increasing over the time series, likely indicating that terrestrial export and net biological processes drive the long term p<span class="hlt">CO</span><span class="hlt">2</span>w increase.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.B24D..03F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.B24D..03F"><span>Variation in salt marsh <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> across a latitudinal gradient along the US Atlantic coast</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Forbrich, I.; Nahrawi, H. B.; Leclerc, M.; O'Connell, J. L.; Mishra, D. R.; Fogarty, M. C.; Edson, J. B.; Lule, A. V.; Vargas, R.; Giblin, A. E.; Alber, M.</p> <p>2017-12-01</p> <p>Salt marshes occur at the dynamic interface of land and ocean, where they play an important role as sink and source of nutrients, carbon (C) and sediment. They often are strong carbon sinks, because they continuously accumulate soil organic matter and sediment to keep their position relative to <span class="hlt">sea</span> level. Decadal average C sequestration rates can be inferred from soil carbon density and mass accumulation rates, but little information about biological and climatic controls on C cycling and storage in these systems exists. In this study, we report measurements of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> exchange from salt marshes along the US Atlantic coast from Massachusetts to Georgia. These measurements were made over periods from one to five years. Spartina alterniflora is the dominant vegetation at all sites. At the northern most site, Plum Island Ecosystems (PIE) LTER, and the southern most site, Georgia Coastal Ecosystems (GCE) LTER, <span class="hlt">flux</span> measurements over several years have shown variations in the net <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> influenced by the local climate. For example, annual net C uptake at the PIE LTER over 5 years (2013-2017) depends on rainfall in the growing season (June-August) which modulates soil salinity levels. This pattern is not as evident at the GCE LTER (2014-2015). Furthermore, the growing season length differs between both sites. Based on the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> measurements, a temperature threshold of 15o C limits the net C uptake at both sites and daily rates of net C uptake are generally smaller during the longer growing season in Georgia. Nevertheless, gross primary production (GPP) is similar for both sites. We will extend this analysis to include sites from Delaware and North Carolina to assess controls (e.g. leaf area using MODIS vegetation indices, temperature, photoperiod) on Spartina phenology and <span class="hlt">CO</span><span class="hlt">2</span> exchange.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUFM.C21A0064F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFM.C21A0064F"><span>Measurements of Turbulent <span class="hlt">Fluxes</span> over <span class="hlt">Sea</span> Ice Region in the <span class="hlt">Sea</span> of Okhotsk.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fujisaki, A.; Yamaguchi, H.; Toyota, T.; Futatsudera, A.; Miyanaga, M.</p> <p>2007-12-01</p> <p>The measurements of turbulent <span class="hlt">fluxes</span> over <span class="hlt">sea</span> ice area were done in the southern part of the <span class="hlt">Sea</span> of Okhotsk, during the cruises of the ice-breaker P/V 'Soya' in 2000-2005. The <span class="hlt">air</span>-ice drag coefficients CDN were 3.57×10-3 over small floes \\left(diameter:φ=20- 100m\\right), 3.38×10-3 over medium floes \\left(φ=100-500m\\right), and <span class="hlt">2</span>.12×10-3 over big floes \\left( φ=500m-<span class="hlt">2</span>km\\right), which showed a decrease with the increase of floe size. This is because the smaller floes contribue to the roughness of <span class="hlt">sea</span>-ice area by their edges more than the larger ones. The average CDN values showed a gradual upslope with ice concentration, which is simply due to the rougher surface of <span class="hlt">sea</span> ice than that of open water, while they showed a slight decline at ice concentration 100%, which is possibly due to the lack of freeboard effect of lateral side of floes. We also compared the relation between the roughness length zM and the friction velocity u* with the model developed in the previous study. The zM-u* relation well corresponded with the model results, while the range of zM we obtained was larger than those obtained at the Ice Station Weddell and during the Surface Heat Budget of the Arctic Ocean project. The sensible heat transfer coefficients CHN were 1.35×10-3 at 80-90% ice concentration, and 0.95×10-3 at 100% ice concentration, which are comparable with the results of the past reaserches. On the other hand, we obtained a maximum CHN value of <span class="hlt">2</span>.39×10-3at 20-50% ice concentration, and <span class="hlt">2</span>.35×10-3 over open water, which are more than twice as the typical value of 1.0×10-3 over open water. These large CHN values are due to the significant upward sensible heat <span class="hlt">flux</span> during the measurements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17706251','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17706251"><span><span class="hlt">Air--sea</span> gaseous exchange of PCB at the Venice lagoon (Italy).</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Manodori, L; Gambaro, A; Moret, I; Capodaglio, G; Cescon, P</p> <p>2007-10-01</p> <p>Water bodies are important storage media for persistent organic pollutants (POPs) such as polychlorinated biphenyls (PCBs) and this function is increased in coastal regions because their inputs are higher than those to the open <span class="hlt">sea</span>. The <span class="hlt">air</span>-water interface is extensively involved with the global cycling of PCBs because it is the place where they accumulate due to depositional processes and where they may be emitted by gaseous exchange. In this work the parallel collection of <span class="hlt">air</span>, microlayer and sub-superficial water samples was performed in July 2005 at a site in the Venice lagoon to evaluate the summer gaseous <span class="hlt">flux</span> of PCBs. The total concentration of PCBs (sum of 118 congeners) in <span class="hlt">air</span> varies from 87 to 273 pg m(-3), whereas in the operationally defined dissolved phase of microlayer and sub-superficial water samples it varies from 159 to 391 pg L(-1). No significant enrichment of dissolved PCB into the microlayer has been observed, although a preferential accumulation of most hydrophobic congeners occurs. Due to this behaviour, we believe that the modified two-layer model was the most suitable approach for the evaluation of the <span class="hlt">flux</span> at the <span class="hlt">air-sea</span> interface, because it takes into account the influence of the microlayer. From its application it appears that PCB volatilize from the lagoon waters with a net <span class="hlt">flux</span> varying from 58 to 195 ng m(-<span class="hlt">2</span>)d(-1) (uncertainty: +/-50-64%) due to the strong influence of wind speed. This <span class="hlt">flux</span> is greater than those reported in the literature for the atmospheric deposition and rivers input and reveals that PCB are actively emitted from the Venice lagoon in summer months.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1355135-how-can-mountaintop-co2-observations-used-constrain-regional-carbon-fluxes','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1355135-how-can-mountaintop-co2-observations-used-constrain-regional-carbon-fluxes"><span>How can mountaintop <span class="hlt">CO</span> <span class="hlt">2</span> observations be used to constrain regional carbon <span class="hlt">fluxes</span>?</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Lin, John C.; Mallia, Derek V.; Wu, Dien; ...</p> <p>2017-05-03</p> <p>Despite the need for researchers to understand terrestrial biospheric carbon <span class="hlt">fluxes</span> to account for carbon cycle feedbacks and predict future <span class="hlt">CO</span> <span class="hlt">2</span> concentrations, knowledge of these <span class="hlt">fluxes</span> at the regional scale remains poor. This is particularly true in mountainous areas, where complex meteorology and lack of observations lead to large uncertainties in carbon <span class="hlt">fluxes</span>. Yet mountainous regions are often where significant forest cover and biomass are found – i.e., areas that have the potential to serve as carbon sinks. As <span class="hlt">CO</span> <span class="hlt">2</span> observations are carried out in mountainous areas, it is imperative that they are properly interpreted to yield informationmore » about carbon <span class="hlt">fluxes</span>. In this paper, we present <span class="hlt">CO</span> <span class="hlt">2</span> observations at three sites in the mountains of the western US, along with atmospheric simulations that attempt to extract information about biospheric carbon <span class="hlt">fluxes</span> from the <span class="hlt">CO</span> <span class="hlt">2</span> observations, with emphasis on the observed and simulated diurnal cycles of <span class="hlt">CO</span> <span class="hlt">2</span>. We show that atmospheric models can systematically simulate the wrong diurnal cycle and significantly misinterpret the <span class="hlt">CO</span> <span class="hlt">2</span> observations, due to erroneous atmospheric flows as a result of terrain that is misrepresented in the model. This problem depends on the selected vertical level in the model and is exacerbated as the spatial resolution is degraded, and our results indicate that a fine grid spacing of ~4 km or less may be needed to simulate a realistic diurnal cycle of <span class="hlt">CO</span> <span class="hlt">2</span> for sites on top of the steep mountains examined here in the American Rockies. In conclusion, in the absence of higher resolution models, we recommend coarse-scale models to focus on assimilating afternoon <span class="hlt">CO</span> <span class="hlt">2</span> observations on mountaintop sites over the continent to avoid misrepresentations of nocturnal transport and influence.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ACP....17.5561L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ACP....17.5561L"><span>How can mountaintop <span class="hlt">CO</span><span class="hlt">2</span> observations be used to constrain regional carbon <span class="hlt">fluxes</span>?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lin, John C.; Mallia, Derek V.; Wu, Dien; Stephens, Britton B.</p> <p>2017-05-01</p> <p>Despite the need for researchers to understand terrestrial biospheric carbon <span class="hlt">fluxes</span> to account for carbon cycle feedbacks and predict future <span class="hlt">CO</span><span class="hlt">2</span> concentrations, knowledge of these <span class="hlt">fluxes</span> at the regional scale remains poor. This is particularly true in mountainous areas, where complex meteorology and lack of observations lead to large uncertainties in carbon <span class="hlt">fluxes</span>. Yet mountainous regions are often where significant forest cover and biomass are found - i.e., areas that have the potential to serve as carbon sinks. As <span class="hlt">CO</span><span class="hlt">2</span> observations are carried out in mountainous areas, it is imperative that they are properly interpreted to yield information about carbon <span class="hlt">fluxes</span>. In this paper, we present <span class="hlt">CO</span><span class="hlt">2</span> observations at three sites in the mountains of the western US, along with atmospheric simulations that attempt to extract information about biospheric carbon <span class="hlt">fluxes</span> from the <span class="hlt">CO</span><span class="hlt">2</span> observations, with emphasis on the observed and simulated diurnal cycles of <span class="hlt">CO</span><span class="hlt">2</span>. We show that atmospheric models can systematically simulate the wrong diurnal cycle and significantly misinterpret the <span class="hlt">CO</span><span class="hlt">2</span> observations, due to erroneous atmospheric flows as a result of terrain that is misrepresented in the model. This problem depends on the selected vertical level in the model and is exacerbated as the spatial resolution is degraded, and our results indicate that a fine grid spacing of ˜ 4 km or less may be needed to simulate a realistic diurnal cycle of <span class="hlt">CO</span><span class="hlt">2</span> for sites on top of the steep mountains examined here in the American Rockies. In the absence of higher resolution models, we recommend coarse-scale models to focus on assimilating afternoon <span class="hlt">CO</span><span class="hlt">2</span> observations on mountaintop sites over the continent to avoid misrepresentations of nocturnal transport and influence.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.C43A0587P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.C43A0587P"><span>Heat <span class="hlt">flux</span> variations over <span class="hlt">sea</span>-ice observed at the coastal area of the Sejong Station, Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Park, S.; Choi, T.; Kim, S.</p> <p>2012-12-01</p> <p>This study presents variations of sensible heat <span class="hlt">flux</span> and latent heat <span class="hlt">flux</span> over <span class="hlt">sea</span>-ice observed in 2011 from the 10-m <span class="hlt">flux</span> tower located at the coast of the Sejong Station on King George Island, Antarctica. A period from June to November was divided into three parts: "Freezing", "Frozen", and "Melting" periods based on daily monitoring of <span class="hlt">sea</span> state and hourly photos looking at the Marian Cove in front of the Sejong Station. The division of periods enabled us to look into the heat <span class="hlt">flux</span> variations depending on the <span class="hlt">sea</span>-ice conditions. Over freezing <span class="hlt">sea</span> surface during the freezing period of late June, daily mean sensible heat <span class="hlt">flux</span> was -11.9 Wm-<span class="hlt">2</span> and daily mean latent heat <span class="hlt">flux</span> was +16.3 Wm-<span class="hlt">2</span>. Over the frozen <span class="hlt">sea</span>-ice, daily mean sensible heat <span class="hlt">flux</span> was -10.4 Wm-<span class="hlt">2</span> while daily mean latent heat <span class="hlt">flux</span> was +<span class="hlt">2</span>.4 Wm-<span class="hlt">2</span>. During the melting period of mid-October to early November, magnitudes of sensible heat <span class="hlt">flux</span> increased to -14.<span class="hlt">2</span> Wm-<span class="hlt">2</span> and latent heat <span class="hlt">flux</span> also increased to +13.5 Wm-<span class="hlt">2</span>. In short, latent heat <span class="hlt">flux</span> was usually upward over <span class="hlt">sea</span>-ice most of the time while sensible heat <span class="hlt">flux</span> was downward from atmosphere to <span class="hlt">sea</span>-ice. Magnitudes of the <span class="hlt">fluxes</span> were small but increased when freezing or melting of <span class="hlt">sea</span>-ice was occurring. Especially, latent heat <span class="hlt">flux</span> increased five to six times compared to that of "frozen" period implying that early melting of <span class="hlt">sea</span>-ice may cause five to six times larger supply of moisture to the atmosphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMOS43A1400S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMOS43A1400S"><span>Validation of the Fully-Coupled <span class="hlt">Air-Sea</span>-Wave COAMPS System</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Smith, T.; Campbell, T. J.; Chen, S.; Gabersek, S.; Tsu, J.; Allard, R. A.</p> <p>2017-12-01</p> <p>A fully-coupled, <span class="hlt">air-sea</span>-wave numerical model, COAMPS®, has been developed by the Naval Research Laboratory to further enhance understanding of oceanic, atmospheric, and wave interactions. The fully-coupled <span class="hlt">air-sea</span>-wave system consists of an atmospheric component with full physics parameterizations, an ocean model, NCOM (Navy Coastal Ocean Model), and two wave components, SWAN (Simulating Waves Nearshore) and WaveWatch III. <span class="hlt">Air-sea</span> interactions between the atmosphere and ocean components are accomplished through bulk <span class="hlt">flux</span> formulations of wind stress and sensible and latent heat <span class="hlt">fluxes</span>. Wave interactions with the ocean include the Stokes' drift, surface radiation stresses, and enhancement of the bottom drag coefficient in shallow water due to the wave orbital velocities at the bottom. In addition, NCOM surface currents are provided to SWAN and WaveWatch III to simulate wave-current interaction. The fully-coupled COAMPS system was executed for several regions at both regional and coastal scales for the entire year of 2015, including the U.S. East Coast, Western Pacific, and Hawaii. Validation of COAMPS® includes observational data comparisons and evaluating operational performance on the High Performance Computing (HPC) system for each of these regions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/5413','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/5413"><span>Forest Floor <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Flux</span> From Two Contrasting Ecosystems in the Southern Appalachians</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>James M. Vose; Barton D. Clinton; Verl Emrick</p> <p>1995-01-01</p> <p>We measured forest floor <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> in two contrasting ecosystems (white pine plantation and northern hardwood ecosystems at low and high elevations, respectively) in May and September 1993 to quantify differences and determine factors regulating <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. An automated IRGA based, flow through system was used with chambers...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6085685-co-sub-fluxes-tropical-atlantic-during-focal-cruises','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6085685-co-sub-fluxes-tropical-atlantic-during-focal-cruises"><span><span class="hlt">CO</span>/sub <span class="hlt">2</span>/ <span class="hlt">fluxes</span> in the tropical Atlantic during FOCAL cruises</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Andrie, C.; Oudot, C.; Genthon, C.</p> <p>1986-10-15</p> <p><span class="hlt">CO</span>/sub <span class="hlt">2</span>/ partial pressures in the atmosphere and in surface seawater have been measured in the equatorial Atlantic Ocean during Programme Francais Ocean-Climat en Atlantique Equatorial cruises extending from July 1982 to August 1984 along the 4/degree/W, 22/degree/W, and 35/degree/W meridians. Gas transfer coefficients based on recently reported field data combined with information deduced from wind tunnel experiments are used to compute the <span class="hlt">CO</span>/sub <span class="hlt">2</span>/ <span class="hlt">fluxes</span>. The global mean net <span class="hlt">flux</span> between 5/degree/N and 5/degree/S is equal to 1.05 mmol m/sup /minus/<span class="hlt">2</span>/ d/sup /minus/1/ and is from the ocean to the atmosphere. The escape of <span class="hlt">CO</span>/sub <span class="hlt">2</span>/ increases strongly frommore » the east to the west and is always lower in the north than in the south. The importance of wind speed, p<span class="hlt">CO</span>/sub <span class="hlt">2</span>/ in atmosphere, PCO/sub <span class="hlt">2</span>/ in surface seawater, and temperature on the <span class="hlt">flux</span> variability is discussed. The relative influence of the equatorial upwelling on one hand and of the advection and warming of surface waters on the other hand is studied in order to explain high partial pressure in seawater. 59 refs., 15 figs., 5 tabs.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.ars.usda.gov/research/publications/publication/?seqNo115=246298','TEKTRAN'); return false;" href="http://www.ars.usda.gov/research/publications/publication/?seqNo115=246298"><span>Atmospheric deposition <span class="hlt">flux</span> estimates for chlorpyrifos and trifluralin in the chukchi <span class="hlt">sea</span></span></a></p> <p><a target="_blank" href="https://www.ars.usda.gov/research/publications/find-a-publication/">USDA-ARS?s Scientific Manuscript database</a></p> <p></p> <p></p> <p>During the 1993 U.S.-Russian BERPAC expedition, residues of agricultural pesticides were detected in seawater, ice, surface microlayer, fog, and <span class="hlt">air</span> of the Bering and Chukchi <span class="hlt">Seas</span>. Gas exchange, wet deposition, and dry particle deposition <span class="hlt">fluxes</span> of trifluralin and chlorpyrifos were estimated using m...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15..856N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15..856N"><span>Human Effects and Soil Surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in Tropical Urban Green Areas, Singapore</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ng, Bernard; Gandois, Laure; Kai, Fuu Ming; Chua, Amy; Cobb, Alex; Harvey, Charles; Hutyra, Lucy</p> <p>2013-04-01</p> <p>Urban green spaces are appreciated for their amenity value, with increasing interest in the ecosystem services they could provide (e.g. climate amelioration and increasingly as possible sites for carbon sequestration). In Singapore, turfgrass occupies approximately 20% of the total land area and is readily found on both planned and residual spaces. This project aims at understanding carbon <span class="hlt">fluxes</span> in tropical urban green areas, including controls of soil environmental factors and the effect of urban management techniques. Given the large pool of potentially labile carbon, management regimes are recognised to have an influence on soil environmental factors (temperature and moisture), this would affect soil respiration and feedbacks to the greenhouse effect. A modified closed dynamic chamber method was employed to measure total soil respiration <span class="hlt">fluxes</span>. In addition to soil respiration rates, environmental factors such as soil moisture and temperature, and ambient <span class="hlt">air</span> temperature were monitored for the site in an attempt to evaluate their control on the observed <span class="hlt">fluxes</span>. Measurements of soil-atmosphere <span class="hlt">CO</span><span class="hlt">2</span> exchanges are reported for four experimental plots within the Singtel-Kranji Radio Transmission Station (103o43'49E, 1o25'53N), an area dominated by Axonopus compressus. Different treatments such as the removal of turf, and application of clippings were effected as a means to determine the <span class="hlt">fluxes</span> from the various components (respiration of soil and turf, and decomposition of clippings), and to explore the effects of human intervention on observed effluxes. The soil surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> observed during the daylight hours ranges from <span class="hlt">2</span>.835 + 0.772 umol m-<span class="hlt">2</span> s-1 for the bare plot as compared to 6.654 + 1.134 umol m-<span class="hlt">2</span> s-1 for the turfed plot; this could be attributed to both autotrophic and heterotrophic respiration. Strong controls of both soil temperature and soil moisture are observed on measured soil <span class="hlt">fluxes</span>. On the base soils, <span class="hlt">fluxes</span> were positively correlated to soil</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeoRL..44.6352P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoRL..44.6352P"><span>Importance of ocean mesoscale variability for <span class="hlt">air-sea</span> interactions in the Gulf of Mexico</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Putrasahan, D. A.; Kamenkovich, I.; Le Hénaff, M.; Kirtman, B. P.</p> <p>2017-06-01</p> <p>Mesoscale variability of currents in the Gulf of Mexico (GoM) can affect oceanic heat advection and <span class="hlt">air-sea</span> heat exchanges, which can influence climate extremes over North America. This study is aimed at understanding the influence of the oceanic mesoscale variability on the lower atmosphere and <span class="hlt">air-sea</span> heat exchanges. The study contrasts global climate model (GCM) with 0.1° ocean resolution (high resolution; HR) with its low-resolution counterpart (1° ocean resolution with the same 0.5° atmosphere resolution; LR). The LR simulation is relevant to current generation of GCMs that are still unable to resolve the oceanic mesoscale. Similar to observations, HR exhibits positive correlation between <span class="hlt">sea</span> surface temperature (SST) and surface turbulent heat <span class="hlt">flux</span> anomalies, while LR has negative correlation. For HR, we decompose lateral advective heat <span class="hlt">fluxes</span> in the upper ocean into mean (slowly varying) and mesoscale-eddy (fast fluctuations) components. We find that the eddy <span class="hlt">flux</span> divergence/convergence dominates the lateral advection and correlates well with the SST anomalies and <span class="hlt">air-sea</span> latent heat exchanges. This result suggests that oceanic mesoscale advection supports warm SST anomalies that in turn feed surface heat <span class="hlt">flux</span>. We identify anticyclonic warm-core circulation patterns (associated Loop Current and rings) which have an average diameter of 350 km. These warm anomalies are sustained by eddy heat <span class="hlt">flux</span> convergence at submonthly time scales and have an identifiable imprint on surface turbulent heat <span class="hlt">flux</span>, atmospheric circulation, and convective precipitation in the northwest portion of an averaged anticyclone.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.A51C0127L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.A51C0127L"><span>Modeling Global Atmospheric <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Fluxes</span> and Transport Using NASA MERRA Reanalysis Data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liu, Y.; Kawa, S. R.; Collatz, G. J.</p> <p>2010-12-01</p> <p>We present our first results of <span class="hlt">CO</span><span class="hlt">2</span> surface biosphere <span class="hlt">fluxes</span> and global atmospheric <span class="hlt">CO</span><span class="hlt">2</span> transport using NASA’s new MERRA reanalysis data. MERRA is the Modern Era Retrospective-Analysis For Research And Applications based on the Goddard Global Modeling and Assimilation Office GEOS-5 data assimilation system. After some application testing and analysis, we have generated biospheric <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> at 3-hourly temporal resolution from an updated version of the CASA carbon cycle model using the 1x1.25-degree reanalysis data. The experiment covers a period of 9 years from 2000 -2008. The affects of US midwest crop (largely corn and soy) carbon uptake and removal by harvest are explicitly included in this version of CASA. Across the agricultural regions of the Midwest US, USDA crop yield data are used to scale vegetation <span class="hlt">fluxes</span> producing a strong sink in the growing season and a comparatively weaker source from respiration after harvest. Comparisons of the new <span class="hlt">fluxes</span> to previous ones generated using GEOS-4 data are provided. The Parameterized Chemistry/Transport Model (PCTM) is then used with the analyzed meteorology in offline <span class="hlt">CO</span><span class="hlt">2</span> transport. In the simulation of <span class="hlt">CO</span><span class="hlt">2</span> transport, we have a higher vertical resolution from MERRA (the lowest 56 of 72 levels are used in our simulation). A preliminary analysis of the <span class="hlt">CO</span><span class="hlt">2</span> simulation results is carried out, including diurnal, seasonal and latitudinal variability. We make comparisons of our simulation to continuous <span class="hlt">CO</span><span class="hlt">2</span> analyzer sites, especially those in agricultural regions. The results show that the model captures reasonably well the observed synoptic variability due to transport changes and biospheric <span class="hlt">fluxes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016ACP....16.5665B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016ACP....16.5665B"><span>Separation of biospheric and fossil fuel <span class="hlt">fluxes</span> of <span class="hlt">CO</span><span class="hlt">2</span> by atmospheric inversion of <span class="hlt">CO</span><span class="hlt">2</span> and 14<span class="hlt">CO</span><span class="hlt">2</span> measurements: Observation System Simulations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Basu, Sourish; Bharat Miller, John; Lehman, Scott</p> <p>2016-05-01</p> <p>National annual total <span class="hlt">CO</span><span class="hlt">2</span> emissions from combustion of fossil fuels are likely known to within 5-10 % for most developed countries. However, uncertainties are inevitably larger (by unknown amounts) for emission estimates at regional and monthly scales, or for developing countries. Given recent international efforts to establish emission reduction targets, independent determination and verification of regional and national scale fossil fuel <span class="hlt">CO</span><span class="hlt">2</span> emissions are likely to become increasingly important. Here, we take advantage of the fact that precise measurements of 14C in <span class="hlt">CO</span><span class="hlt">2</span> provide a largely unbiased tracer for recently added fossil-fuel-derived <span class="hlt">CO</span><span class="hlt">2</span> in the atmosphere and present an atmospheric inversion technique to jointly assimilate observations of <span class="hlt">CO</span><span class="hlt">2</span> and 14<span class="hlt">CO</span><span class="hlt">2</span> in order to simultaneously estimate fossil fuel emissions and biospheric exchange <span class="hlt">fluxes</span> of <span class="hlt">CO</span><span class="hlt">2</span>. Using this method in a set of Observation System Simulation Experiments (OSSEs), we show that given the coverage of 14<span class="hlt">CO</span><span class="hlt">2</span> measurements available in 2010 (969 over North America, 1063 globally), we can recover the US national total fossil fuel emission to better than 1 % for the year and to within 5 % for most months. Increasing the number of 14<span class="hlt">CO</span><span class="hlt">2</span> observations to ˜ 5000 per year over North America, as recently recommended by the National Academy of Science (NAS) (Pacala et al., 2010), we recover monthly emissions to within 5 % for all months for the US as a whole and also for smaller, highly emissive regions over which the specified data coverage is relatively dense, such as for the New England states or the NY-NJ-PA tri-state area. This result suggests that, given continued improvement in state-of-the art transport models, a measurement program similar in scale to that recommended by the NAS can provide for independent verification of bottom-up inventories of fossil fuel <span class="hlt">CO</span><span class="hlt">2</span> at the regional and national scale. In addition, we show that the dual tracer inversion framework can detect and minimize biases in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013ACPD...13.7267V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013ACPD...13.7267V"><span>The role of vegetation in the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> from a tropical urban neighbourhood</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Velasco, E.; Roth, M.; Tan, S. H.; Quak, M.; Nabarro, S. D. A.; Norford, L.</p> <p>2013-03-01</p> <p>Urban surfaces are usually net sources of <span class="hlt">CO</span><span class="hlt">2</span>. Vegetation can potentially have an important role in reducing the <span class="hlt">CO</span><span class="hlt">2</span> emitted by anthropogenic activities in cities, particularly when vegetation is extensive and/or evergreen. Negative daytime <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>, for example have been observed during the growing season at suburban sites characterized by abundant vegetation and low population density. A direct and accurate estimation of carbon uptake by urban vegetation is difficult due to the particular characteristics of the urban ecosystem and high variability in tree distribution and species. Here, we investigate the role of urban vegetation in the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> from a residential neighbourhood in Singapore using two different approaches. <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> measured directly by eddy covariance are compared with emissions estimated from emissions factors and activity data. The latter includes contributions from vehicular traffic, household combustion, soil respiration and human breathing. The difference between estimated emissions and measured <span class="hlt">fluxes</span> should approximate the biogenic <span class="hlt">flux</span>. In addition, a tree survey was conducted to estimate the annual <span class="hlt">CO</span><span class="hlt">2</span> sequestration using allometric equations and an alternative model of the metabolic theory of ecology for tropical forests. Palm trees, banana plants and turfgrass were also included in the survey with their annual <span class="hlt">CO</span><span class="hlt">2</span> uptake obtained from published growth rates. Both approaches agree within <span class="hlt">2</span>% and suggest that vegetation captures 8% of the total emitted <span class="hlt">CO</span><span class="hlt">2</span> in the residential neighbourhood studied. A net uptake of 1.4 ton km-<span class="hlt">2</span> day-1 (510 ton km-<span class="hlt">2</span> yr-1 ) was estimated from the difference between the daily <span class="hlt">CO</span><span class="hlt">2</span> uptake by photosynthesis (3.95 ton km-<span class="hlt">2</span> ) and release by respiration (<span class="hlt">2</span>.55 ton km-<span class="hlt">2</span>). The study shows the importance of urban vegetation at the local scale for climate change mitigation in the tropics.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_15 --> <div id="page_16" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="301"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1918160M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1918160M"><span>Application of a two-dimensional hydrodynamic model for calculating the <span class="hlt">CO</span>_{<span class="hlt">2</span>} and H_{<span class="hlt">2</span>}O <span class="hlt">fluxes</span> over complex terrain</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mukhartova, Yulia; Krupenko, Alexandr; Levashova, Natalia; Olchev, Alexandr</p> <p>2017-04-01</p> <p>Within the framework of the study a two dimensional hydrodynamic model of turbulent transfer of greenhouse gases was developed and applied for calculating the <span class="hlt">CO</span><span class="hlt">2</span> and H<span class="hlt">2</span>O turbulent <span class="hlt">fluxes</span> within the atmospheric surface layer over the heterogeneous land surface with mosaic vegetation and complex topography. The vegetation cover in the model is represented as the two-phase medium containing the elements of vegetation and the <span class="hlt">air</span>. The model is based on solving the system of averaged Navier-Stokes and continuity equations for the wind velocity components (⃗V = {V1,V<span class="hlt">2</span>}), using the 1.5-order closure scheme (Wilcox 1998, Wyngaard 2010). The system of the main equations includes also the diffusion and advection equations for turbulent transfer of sensible heat, <span class="hlt">CO</span><span class="hlt">2</span> concentration (Cs) and specific humidity (q) at soil - vegetation -atmosphere interface (Sogachev, Panferov 2006, Mukhartova et al. 2015, Mamkin et al. 2016): ( ) { ( )} ∂Vi+ ⃗V,∇ V = -1ṡ-∂-δP -∂- <span class="hlt">2</span>δ ¯e- K ṡ ∂Vi-+ ∂Vj- +gṡδTv+F , i,j = 1,<span class="hlt">2</span>, ∂t i ρ0 ∂xi ∂xj 3 ij ∂xj ∂xi T0 i div⃗V = 0, ∂T ( ) Tv γa ∂T 1 ( ) H ∂t-+ ⃗V ,∇ T+ γaṡT-ṡV<span class="hlt">2</span> = div (KT ṡ∇T )+ T-ṡKT ṡ∂x-+ρ-c- ⃗V,∇ δP -ρ-c-, 0 0 <span class="hlt">2</span> 0 p 0 p ∂Cs- (⃗ ) ∂q- (⃗ ) E- ∂t + V ,∇ Cs = div(KC ṡ∇Cs )+FC, ∂t+ V ,∇ q = div(Kv ṡ∇q )+ ρ , where x1,x<span class="hlt">2</span> - horizontal and vertical coordinates respectively, ρ0 - the density of dry <span class="hlt">air</span>, δP - the deviation of mean <span class="hlt">air</span> pressure from the hydrostatic distribution, ¯e - the turbulent kinetic energy, T - the temperature of the <span class="hlt">air</span>, δTv = T ṡ(1+ 0.61q) -T0 - the deviation of virtual temperature from the adiabatic temperature T0(x<span class="hlt">2</span>) for dry <span class="hlt">air</span>, Fi - the components of the viscous drag forces induced by the presence of vegetation, K,KT,KC,Kv - turbulent exchange coefficients for momentum, sensible heat, <span class="hlt">CO</span><span class="hlt">2</span>and H<span class="hlt">2</span>O respectively, γa = g/ cp, cp - the specific heat of the <span class="hlt">air</span> at constant atmospheric pressure, FC - the sources/sinks of <span class="hlt">CO</span><span class="hlt">2</span>in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70134376','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70134376"><span>Decadal and annual changes in biogenic opal and carbonate <span class="hlt">fluxes</span> to the deep Sargasso <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Deuser, W.G.; Jickells, T.D.; Commeau, Judith A.</p> <p>1995-01-01</p> <p>Analyses of samples from a 14-year series of sediment-trap deployments in the deep Sargasso <span class="hlt">Sea</span> reveal a significant trend in the ratio of the sinking <span class="hlt">fluxes</span> of biogenic calcium carbonate and silica. Although there are pronounced seasonal cycles for both <span class="hlt">flux</span> components, the overall opal/Ca<span class="hlt">CO</span>3 ratio changed by 50% from 1978 to 1991 (largely due to a decrease of opal <span class="hlt">flux</span>), while total <span class="hlt">flux</span> had no significant trend. These results suggest that plankton communities respond rapidly to subtle climate change, such as is evident in regional variations of wind speed, precipitation, wintertime ventilation and midwater temperatures. If the trends we observe in the makeup of sinking particulate matter occur on a large scale, they may in turn modify climate by modulating ocean-atmosphere <span class="hlt">CO</span><span class="hlt">2</span> exchange and albedo over the ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4948307','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4948307"><span>Detecting regional patterns of changing <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> in Alaska</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Parazoo, Nicholas C.; Wofsy, Steven C.; Koven, Charles D.; Sweeney, Colm; Lawrence, David M.; Lindaas, Jakob; Chang, Rachel Y.-W.; Miller, Charles E.</p> <p>2016-01-01</p> <p>With rapid changes in climate and the seasonal amplitude of carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) in the Arctic, it is critical that we detect and quantify the underlying processes controlling the changing amplitude of <span class="hlt">CO</span><span class="hlt">2</span> to better predict carbon cycle feedbacks in the Arctic climate system. We use satellite and airborne observations of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> with climatically forced <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> simulations to assess the detectability of Alaskan carbon cycle signals as future warming evolves. We find that current satellite remote sensing technologies can detect changing uptake accurately during the growing season but lack sufficient cold season coverage and near-surface sensitivity to constrain annual carbon balance changes at regional scale. Airborne strategies that target regular vertical profile measurements within continental interiors are more sensitive to regional <span class="hlt">flux</span> deeper into the cold season but currently lack sufficient spatial coverage throughout the entire cold season. Thus, the current <span class="hlt">CO</span><span class="hlt">2</span> observing network is unlikely to detect potentially large <span class="hlt">CO</span><span class="hlt">2</span> sources associated with deep permafrost thaw and cold season respiration expected over the next 50 y. Although continuity of current observations is vital, strategies and technologies focused on cold season measurements (active remote sensing, aircraft, and tall towers) and systematic sampling of vertical profiles across continental interiors over the full annual cycle are required to detect the onset of carbon release from thawing permafrost. PMID:27354511</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1259729-detecting-regional-patterns-changing-co2-flux-alaska','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1259729-detecting-regional-patterns-changing-co2-flux-alaska"><span>Detecting regional patterns of changing <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">flux</span> in Alaska</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Parazoo, Nicholas C.; Commane, Roisin; Wofsy, Steven C.; ...</p> <p>2016-06-27</p> <p>With rapid changes in climate and the seasonal amplitude of carbon dioxide (<span class="hlt">CO</span> <span class="hlt">2</span>) in the Arctic, it is critical that we detect and quantify the underlying processes controlling the changing amplitude of <span class="hlt">CO</span> <span class="hlt">2</span> to better predict carbon cycle feedbacks in the Arctic climate system. We use satellite and airborne observations of atmospheric <span class="hlt">CO</span> <span class="hlt">2</span> with climatically forced <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">flux</span> simulations to assess the detectability of Alaskan carbon cycle signals as future warming evolves. We find that current satellite remote sensing technologies can detect changing uptake accurately during the growing season but lack sufficient cold season coverage andmore » near-surface sensitivity to constrain annual carbon balance changes at regional scale. Airborne strategies that target regular vertical profile measurements within continental interiors are more sensitive to regional <span class="hlt">flux</span> deeper into the cold season but currently lack sufficient spatial coverage throughout the entire cold season. Thus, the current <span class="hlt">CO</span> <span class="hlt">2</span> observing network is unlikely to detect potentially large <span class="hlt">CO</span> <span class="hlt">2</span> sources associated with deep permafrost thaw and cold season respiration expected over the next 50 y. In conclusion, although continuity of current observations is vital, strategies and technologies focused on cold season measurements (active remote sensing, aircraft, and tall towers) and systematic sampling of vertical profiles across continental interiors over the full annual cycle are required to detect the onset of carbon release from thawing permafrost.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMGC13C0652T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMGC13C0652T"><span>Southern Ocean <span class="hlt">air-sea</span> heat <span class="hlt">flux</span>, SST spatial anomalies, and implications for multi-decadal upper ocean heat content trends.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tamsitt, V. M.; Talley, L. D.; Mazloff, M. R.</p> <p>2014-12-01</p> <p>The Southern Ocean displays a zonal dipole (wavenumber one) pattern in <span class="hlt">sea</span> surface temperature (SST), with a cool zonal anomaly in the Atlantic and Indian sectors and a warm zonal anomaly in the Pacific sector, associated with the large northward excursion of the Malvinas and southeastward flow of the Antarctic Circumpolar Current (ACC). To the north of the cool Indian sector is the warm, narrow Agulhas Return Current (ARC). <span class="hlt">Air-sea</span> heat <span class="hlt">flux</span> is largely the inverse of this SST pattern, with ocean heat gain in the Atlantic/Indian, cooling in the southeastward-flowing ARC, and cooling in the Pacific, based on adjusted <span class="hlt">fluxes</span> from the Southern Ocean State Estimate (SOSE), a ⅙° eddy permitting model constrained to all available in situ data. This heat <span class="hlt">flux</span> pattern is dominated by turbulent heat loss from the ocean (latent and sensible), proportional to perturbations in the difference between SST and surface <span class="hlt">air</span> temperature, which are maintained by ocean advection. Locally in the Indian sector, intense heat loss along the ARC is contrasted by ocean heat gain of 0.11 PW south of the ARC. The IPCC AR5 50 year depth-averaged 0-700 m temperature trend shows surprising similarities in its spatial pattern, with upper ocean warming in the ARC contrasted by cooling to the south. Using diagnosed heat budget terms from the most recent (June 2014) 6-year run of the SOSE we find that surface cooling in the ARC is balanced by heating from south-eastward advection by the current whereas heat gain in the ACC is balanced by cooling due to northward Ekman transport driven by strong westerly winds. These results suggest that spatial patterns in multi-decadal upper ocean temperature trends depend on regional variations in upper ocean dynamics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AtmEn..74...60L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AtmEn..74...60L"><span>Variability of <span class="hlt">CO</span><span class="hlt">2</span> concentrations and <span class="hlt">fluxes</span> in and above an urban street canyon</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lietzke, Björn; Vogt, Roland</p> <p>2013-08-01</p> <p>The variability of <span class="hlt">CO</span><span class="hlt">2</span> concentrations and <span class="hlt">fluxes</span> in dense urban environments is high due to the inherent heterogeneity of these complex areas and their spatio-temporally variable anthropogenic sources. With a focus on micro- to local-scale <span class="hlt">CO</span><span class="hlt">2</span>-exchange processes, measurements were conducted in a street canyon in the city of Basel, Switzerland in 2010. <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> were sampled at the top of the canyon (19 m) and at 39 m while vertical <span class="hlt">CO</span><span class="hlt">2</span> concentration profiles were measured in the center and at a wall of the canyon. <span class="hlt">CO</span><span class="hlt">2</span> concentration distributions in the street canyon and exchange processes with the layers above show, apart from expected general diurnal patterns due mixing layer heights, a strong dependence on wind direction relative to the canyon. As a consequence of the resulting corkscrew-like canyon vortex, accumulation of <span class="hlt">CO</span><span class="hlt">2</span> inside the canyon is modulated with distinct distribution patterns. The evaluation of diurnal traffic data provides good explanations for the vertical and horizontal differences in <span class="hlt">CO</span><span class="hlt">2</span>-distribution inside the canyon. Diurnal <span class="hlt">flux</span> characteristics at the top of the canyon can almost solely be explained with traffic density expressed by the strong linear dependence. Even the diurnal course of the <span class="hlt">flux</span> at 39 m shows a remarkable relationship to traffic density for east wind conditions while, for west wind situations, a change toward source areas with lower emissions leads to a reduced <span class="hlt">flux</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.1398B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.1398B"><span>Top-down estimate of surface <span class="hlt">flux</span> in the Los Angeles Basin using a mesoscale inverse modeling technique: assessing anthropogenic emissions of <span class="hlt">CO</span>, NOx and <span class="hlt">CO</span><span class="hlt">2</span> and their impacts</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brioude, Jerome; Angevine, Wayne; Ahmadov, Ravan; Kim, Si Wan; Evan, Stephanie; McKeen, Stuart; Hsie, Eirh Yu; Frost, Greg; Neuman, Andy; Pollack, Ilana; Peischl, Jeff; Ryerson, Tom; Holloway, John; Brown, Steeve; Nowak, John; Roberts, Jim; Wofsy, Steeve; Santoni, Greg; Trainer, Michael</p> <p>2013-04-01</p> <p>We present top-down estimates of anthropogenic <span class="hlt">CO</span>, NOx and <span class="hlt">CO</span><span class="hlt">2</span> surface <span class="hlt">fluxes</span> at mesoscale using a Lagrangian model in combination with three different WRF model configurations, driven by data from aircraft flights during the CALNEX campaign in southern California in May-June 2010. The US EPA National Emission Inventory 2005 (NEI 2005) was the prior in the <span class="hlt">CO</span> and NOx inversion calculations. The <span class="hlt">flux</span> ratio inversion method, based on linear relationships between chemical species, was used to calculate the <span class="hlt">CO</span><span class="hlt">2</span> inventory without prior knowledge of <span class="hlt">CO</span><span class="hlt">2</span> surface <span class="hlt">fluxes</span>. The inversion was applied to each flight to estimate the variability of single-flight-based <span class="hlt">flux</span> estimates. In Los Angeles (LA) County, the uncertainties on <span class="hlt">CO</span> and NOx <span class="hlt">fluxes</span> were 10% and 15%, respectively. Compared with NEI 2005, the <span class="hlt">CO</span> posterior emissions were lower by 43% ± 6% in LA County and by 37% ± 10% in the South Coast <span class="hlt">Air</span> Basin (SoCAB). NOx posterior emissions were lower by 32% ± 10% in LA County and by 27% ± 15% in the SoCAB. NOx posterior emissions were 40% lower on weekends relative to weekdays. The <span class="hlt">CO</span><span class="hlt">2</span> posterior estimates were 183 ± 18 Tg yr-1 in SoCAB. A flight during ITCT in 2002 was used to estimate emissions in the LA Basin in 2002. From 2002 to 2010, the <span class="hlt">CO</span> and NOx posterior emissions decreased by 41% and 37%, respectively, in agreement with previous studies. Over the same time period, <span class="hlt">CO</span><span class="hlt">2</span> emissions increased by 10% ± 14% in LA County but decreased by 4% ± 10% in the SoCAB, a statistically insignificant change. Overall, the posterior estimates were in good agreement with the California <span class="hlt">Air</span> Resources Board (CARB) inventory, with differences of 15% or less. However, the posterior spatial distribution in the basin was significantly different from CARB for NOx emissions. WRF-Chem mesoscale chemical-transport model simulations allowed an evaluation of differences in chemistry using different inventory assumptions, including NEI 2005, CARB 2010 and the posterior inventories derived in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013ACP....13.3661B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013ACP....13.3661B"><span>Top-down estimate of surface <span class="hlt">flux</span> in the Los Angeles Basin using a mesoscale inverse modeling technique: assessing anthropogenic emissions of <span class="hlt">CO</span>, NOx and <span class="hlt">CO</span><span class="hlt">2</span> and their impacts</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brioude, J.; Angevine, W. M.; Ahmadov, R.; Kim, S.-W.; Evan, S.; McKeen, S. A.; Hsie, E.-Y.; Frost, G. J.; Neuman, J. A.; Pollack, I. B.; Peischl, J.; Ryerson, T. B.; Holloway, J.; Brown, S. S.; Nowak, J. B.; Roberts, J. M.; Wofsy, S. C.; Santoni, G. W.; Oda, T.; Trainer, M.</p> <p>2013-04-01</p> <p>We present top-down estimates of anthropogenic <span class="hlt">CO</span>, NOx and <span class="hlt">CO</span><span class="hlt">2</span> surface <span class="hlt">fluxes</span> at mesoscale using a Lagrangian model in combination with three different WRF model configurations, driven by data from aircraft flights during the CALNEX campaign in southern California in May-June 2010. The US EPA National Emission Inventory 2005 (NEI 2005) was the prior in the <span class="hlt">CO</span> and NOx inversion calculations. The <span class="hlt">flux</span> ratio inversion method, based on linear relationships between chemical species, was used to calculate the <span class="hlt">CO</span><span class="hlt">2</span> inventory without prior knowledge of <span class="hlt">CO</span><span class="hlt">2</span> surface <span class="hlt">fluxes</span>. The inversion was applied to each flight to estimate the variability of single-flight-based <span class="hlt">flux</span> estimates. In Los Angeles (LA) County, the uncertainties on <span class="hlt">CO</span> and NOx <span class="hlt">fluxes</span> were 10% and 15%, respectively. Compared with NEI 2005, the <span class="hlt">CO</span> posterior emissions were lower by 43% in LA County and by 37% in the South Coast <span class="hlt">Air</span> Basin (SoCAB). NOx posterior emissions were lower by 32% in LA County and by 27% in the SoCAB. NOx posterior emissions were 40% lower on weekends relative to weekdays. The <span class="hlt">CO</span><span class="hlt">2</span> posterior estimates were 183 Tg yr-1 in SoCAB. A flight during ITCT (Intercontinental Transport and Chemical Transformation) in 2002 was used to estimate emissions in the LA Basin in 2002. From 2002 to 2010, the <span class="hlt">CO</span> and NOx posterior emissions decreased by 41% and 37%, respectively, in agreement with previous studies. Over the same time period, <span class="hlt">CO</span><span class="hlt">2</span> emissions increased by 10% in LA County but decreased by 4% in the SoCAB, a statistically insignificant change. Overall, the posterior estimates were in good agreement with the California <span class="hlt">Air</span> Resources Board (CARB) inventory, with differences of 15% or less. However, the posterior spatial distribution in the basin was significantly different from CARB for NOx emissions. WRF-Chem mesoscale chemical-transport model simulations allowed an evaluation of differences in chemistry using different inventory assumptions, including NEI 2005, a gridded CARB inventory and the posterior</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012ACPD...1231439B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012ACPD...1231439B"><span>Top-down estimate of surface <span class="hlt">flux</span> in the Los Angeles Basin using a mesoscale inverse modeling technique: assessing anthropogenic emissions of <span class="hlt">CO</span>, NOx and <span class="hlt">CO</span><span class="hlt">2</span> and their impacts</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brioude, J.; Angevine, W. M.; Ahmadov, R.; Kim, S.-W.; Evan, S.; McKeen, S. A.; Hsie, E.-Y.; Frost, G. J.; Neuman, J. A.; Pollack, I. B.; Peischl, J.; Ryerson, T. B.; Holloway, J.; Brown, S. S.; Nowak, J. B.; Roberts, J. M.; Wofsy, S. C.; Santoni, G. W.; Trainer, M.</p> <p>2012-12-01</p> <p>We present top-down estimates of anthropogenic <span class="hlt">CO</span>, NOx and <span class="hlt">CO</span><span class="hlt">2</span> surface <span class="hlt">fluxes</span> at mesoscale using a Lagrangian model in combination with three different WRF model configurations, driven by data from aircraft flights during the CALNEX campaign in southern California in May-June 2010. The US EPA National Emission Inventory 2005 (NEI 2005) was the prior in the <span class="hlt">CO</span> and NOx inversion calculations. The <span class="hlt">flux</span> ratio inversion method, based on linear relationships between chemical species, was used to calculate the <span class="hlt">CO</span><span class="hlt">2</span> inventory without prior knowledge of <span class="hlt">CO</span><span class="hlt">2</span> surface <span class="hlt">fluxes</span>. The inversion was applied to each flight to estimate the variability of single-flight-based <span class="hlt">flux</span> estimates. In Los Angeles (LA) County, the uncertainties on <span class="hlt">CO</span> and NOx <span class="hlt">fluxes</span> were 10% and 15%, respectively. Compared with NEI 2005, the <span class="hlt">CO</span> posterior emissions were lower by 43% ± 6% in LA County and by 37% ± 10% in the South Coast <span class="hlt">Air</span> Basin (SoCAB). NOx posterior emissions were lower by 32% ± 10% in LA County and by 27% ± 15% in the SoCAB. NOx posterior emissions were 40% lower on weekends relative to weekdays. The <span class="hlt">CO</span><span class="hlt">2</span> posterior estimates were 183 ± 18 Tg yr-1 in SoCAB. A flight during ITCT in 2002 was used to estimate emissions in the LA Basin in 2002. From 2002 to 2010, the <span class="hlt">CO</span> and NOx posterior emissions decreased by 41% and 37%, respectively, in agreement with previous studies. Over the same time period, <span class="hlt">CO</span><span class="hlt">2</span> emissions increased by 10% ± 14% in LA County but decreased by 4% ± 10% in the SoCAB, a statistically insignificant change. Overall, the posterior estimates were in good agreement with the California <span class="hlt">Air</span> Resources Board (CARB) inventory, with differences of 15% or less. However, the posterior spatial distribution in the basin was significantly different from CARB for NOx emissions. WRF-Chem mesoscale chemical-transport model simulations allowed an evaluation of differences in chemistry using different inventory assumptions, including NEI 2005, CARB 2010 and the posterior inventories derived in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSPO54B3246W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSPO54B3246W"><span>Using Argo-O<span class="hlt">2</span> data to examine the impact of deep-water formation events on oxygen uptake in the Labrador <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wolf, M. K.; Hamme, R. C.; Gilbert, D.; Yashayaev, I.</p> <p>2016-02-01</p> <p>Deep-water formation allows the deep ocean to communicate with the atmosphere, facilitating exchanges of heat as well as important gases such as <span class="hlt">CO</span><span class="hlt">2</span> and oxygen. The Labrador <span class="hlt">Sea</span> is the most studied location of deep convection in the North Atlantic Ocean and a strong contributor to the global thermohaline circulation. Since there are no internal sources of oxygen below the euphotic zone, deep-water formation is vital for oxygen transport to the deep ocean. Recent studies document large interannual variability in the strength and depth of convection in the Labrador <span class="hlt">Sea</span>, from mixed layers of 100m to greater than 1000m. A weakening of this deep convection starves the deep ocean of oxygen, disrupting crucial deep <span class="hlt">sea</span> biological processes, as well as reducing oceanic <span class="hlt">CO</span><span class="hlt">2</span> uptake and ocean circulation. We used data from the extensive Argo float network to examine these deep-water formation events in the Labrador <span class="hlt">Sea</span>. The oxygen optodes onboard many Argo floats suffer from biases whose amplitude must be determined; therefore we investigated and applied various optode calibration methods. Using calibrated vertical profiles of oxygen, temperature, and salinity, we observed the timing, magnitude, and location of deep convection, restratification, and spring phytoplankton blooms. In addition, we used surface oxygen values along with NCEP wind speeds to calculate the <span class="hlt">air-sea</span> oxygen <span class="hlt">flux</span> using a range of <span class="hlt">air-sea</span> gas exchange parameterizations. We then compared this oxygen <span class="hlt">flux</span> to the rate of change of the measured oxygen inventory. Where the inventory and <span class="hlt">flux</span> did not agree, we identified other oceanic processes such as biological activity or lateral advection of water masses occurring, or advection of the float itself into a new area. The large role that horizontal advection of water or the float has on oxygen uptake and cycling leads us to conclude that this data cannot be easily interpreted as a 1-D system. Oxygen exchanges with the atmosphere at a faster rate than <span class="hlt">CO</span><span class="hlt">2</span>, is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ISPAn44W2...77W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ISPAn44W2...77W"><span>Spatiotemporal Visualization of Time-Series Satellite-Derived <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Flux</span> Data Using Volume Rendering and Gpu-Based Interpolation on a Cloud-Driven Digital Earth</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wu, S.; Yan, Y.; Du, Z.; Zhang, F.; Liu, R.</p> <p>2017-10-01</p> <p>The ocean carbon cycle has a significant influence on global climate, and is commonly evaluated using time-series satellite-derived <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> data. Location-aware and globe-based visualization is an important technique for analyzing and presenting the evolution of climate change. To achieve realistic simulation of the spatiotemporal dynamics of ocean carbon, a cloud-driven digital earth platform is developed to support the interactive analysis and display of multi-geospatial data, and an original visualization method based on our digital earth is proposed to demonstrate the spatiotemporal variations of carbon sinks and sources using time-series satellite data. Specifically, a volume rendering technique using half-angle slicing and particle system is implemented to dynamically display the released or absorbed <span class="hlt">CO</span><span class="hlt">2</span> gas. To enable location-aware visualization within the virtual globe, we present a 3D particlemapping algorithm to render particle-slicing textures onto geospace. In addition, a GPU-based interpolation framework using CUDA during real-time rendering is designed to obtain smooth effects in both spatial and temporal dimensions. To demonstrate the capabilities of the proposed method, a series of satellite data is applied to simulate the <span class="hlt">air-sea</span> carbon cycle in the China <span class="hlt">Sea</span>. The results show that the suggested strategies provide realistic simulation effects and acceptable interactive performance on the digital earth.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JGRC..121.8787G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JGRC..121.8787G"><span>Assessing recent <span class="hlt">air-sea</span> freshwater <span class="hlt">flux</span> changes using a surface temperature-salinity space framework</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Grist, Jeremy P.; Josey, Simon A.; Zika, Jan D.; Evans, Dafydd Gwyn; Skliris, Nikolaos</p> <p>2016-12-01</p> <p>A novel assessment of recent changes in <span class="hlt">air-sea</span> freshwater <span class="hlt">fluxes</span> has been conducted using a surface temperature-salinity framework applied to four atmospheric reanalyses. Viewed in the T-S space of the ocean surface, the complex pattern of the longitude-latitude space mean global Precipitation minus Evaporation (PME) reduces to three distinct regions. The analysis is conducted for the period 1979-2007 for which there is most evidence for a broadening of the (atmospheric) tropical belt. All four of the reanalyses display an increase in strength of the water cycle. The range of increase is between <span class="hlt">2</span>% and 30% over the period analyzed, with an average of 14%. Considering the average across the reanalyses, the water cycle changes are dominated by changes in tropical as opposed to mid-high latitude precipitation. The increases in the water cycle strength, are consistent in sign, but larger than in a 1% greenhouse gas run of the HadGEM3 climate model. In the model a shift of the precipitation/evaporation cells to higher temperatures is more evident, due to the much stronger global warming signal. The observed changes in freshwater <span class="hlt">fluxes</span> appear to be reflected in changes in the T-S distribution of the Global Ocean. Specifically, across the diverse range of atmospheric reanalyses considered here, there was an acceleration of the hydrological cycle during 1979-2007 which led to a broadening of the ocean's salinity distribution. Finally, although the reanalyses indicate that the warm temperature tropical precipitation dominated water cycle change, ocean observations suggest that ocean processes redistributed the freshening to lower ocean temperatures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PrOce.141..153Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PrOce.141..153Z"><span>The impact of dissolved organic carbon and bacterial respiration on p<span class="hlt">CO</span><span class="hlt">2</span> in experimental <span class="hlt">sea</span> ice</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhou, J.; Kotovitch, M.; Kaartokallio, H.; Moreau, S.; Tison, J.-L.; Kattner, G.; Dieckmann, G.; Thomas, D. N.; Delille, B.</p> <p>2016-02-01</p> <p>Previous observations have shown that the partial pressure of carbon dioxide (p<span class="hlt">CO</span><span class="hlt">2</span>) in <span class="hlt">sea</span> ice brines is generally higher in Arctic <span class="hlt">sea</span> ice compared to those from the Antarctic <span class="hlt">sea</span> ice, especially in winter and early spring. We hypothesized that these differences result from the higher dissolved organic carbon (DOC) content in Arctic seawater: Higher concentrations of DOC in seawater would be reflected in a greater DOC incorporation into <span class="hlt">sea</span> ice, enhancing bacterial respiration, which in turn would increase the p<span class="hlt">CO</span><span class="hlt">2</span> in the ice. To verify this hypothesis, we performed an experiment using two series of mesocosms: one was filled with seawater (SW) and the other one with seawater with an addition of filtered humic-rich river water (SWR). The addition of river water increased the DOC concentration of the water from a median of 142 μmol Lwater-1 in SW to 249 μmol Lwater-1 in SWR. <span class="hlt">Sea</span> ice was grown in these mesocosms under the same physical conditions over 19 days. Microalgae and protists were absent, and only bacterial activity has been detected. We measured the DOC concentration, bacterial respiration, total alkalinity and p<span class="hlt">CO</span><span class="hlt">2</span> in <span class="hlt">sea</span> ice and the underlying seawater, and we calculated the changes in dissolved inorganic carbon (DIC) in both media. We found that bacterial respiration in ice was higher in SWR: median bacterial respiration was 25 nmol C Lice-1 h-1 compared to 10 nmol C Lice-1 h-1 in SW. p<span class="hlt">CO</span><span class="hlt">2</span> in ice was also higher in SWR with a median of 430 ppm compared to 356 ppm in SW. However, the differences in p<span class="hlt">CO</span><span class="hlt">2</span> were larger within the ice interiors than at the surfaces or the bottom layers of the ice, where exchanges at the <span class="hlt">air</span>-ice and ice-water interfaces might have reduced the differences. In addition, we used a model to simulate the differences of p<span class="hlt">CO</span><span class="hlt">2</span> and DIC based on bacterial respiration. The model simulations support the experimental findings and further suggest that bacterial growth efficiency in the ice might approach 0.15 and 0.<span class="hlt">2</span>. It is thus credible</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMPP22B..05H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMPP22B..05H"><span>Shifting locus of carbonate sedimentation and the trajectory of Paleozoic p<span class="hlt">CO</span><span class="hlt">2</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Husson, J. M.; Peters, S. E.</p> <p>2016-12-01</p> <p>The burial of calcium carbonate is a determinant of planetary habitability, dictated by <span class="hlt">CO</span><span class="hlt">2</span> input to the surface environment and rates of chemical weathering. An important source of <span class="hlt">CO</span><span class="hlt">2</span> is the metamorphism of carbon-bearing sediments, which is responsive to the locus of sedimentation. For example, deep <span class="hlt">sea</span> sediments are prone to recycling as <span class="hlt">sea</span> floor is consumed at convergent margins; by contrast, sediments deposited on continental crust can be stable for billions of years.The predominant feature in the empirical sedimentary rock record, as measured by Macrostrat (https://macrostrat.org) and global geological syntheses, is a step-wise increase in continental sedimentation at the Neoproterozoic-Paleozoic transition. Although early Paleozoic carbonate volumes are sufficient to account for a <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> 5x greater than present, Proterozoic continental burial <span class="hlt">fluxes</span> were likely below the modern estimate. This observation implies that most carbonate sedimentation in the Proterozoic took place on the deep <span class="hlt">sea</span> floor. The establishment of persistent, widespread continental flooding during the Paleozoic shifted the locus of carbonate sedimentation to continental interiors. A major implication of this shift is that <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> declined during the Paleozoic as carbonate-laden Precambrian seafloor was metamorphosed and recycled. This prediction is consistent with independent proxy records and our model for Phanerozoic carbonate burial. An important corollary is that as carbonate-rich Precambrian seafloor was progressively destroyed, the carbonate content of deep <span class="hlt">sea</span> sediments decreased concordantly because Paleozoic continents effectively captured global alkalinity <span class="hlt">fluxes</span>. This process culminated near the Permian/Triassic, with metamorphic <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> at a Phanerozoic minimum and the global ocean uniquely unbuffered against acidification. Such a condition could enhance the environmental effects of transient <span class="hlt">CO</span><span class="hlt">2</span> injections. Because the mid-Mesozoic appearance of pelagic calcifiers and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19970021275','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19970021275"><span>Low p<span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Air</span>-Polarized <span class="hlt">CO</span><span class="hlt">2</span> Concentrator Development</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Schubert, Franz H.</p> <p>1997-01-01</p> <p>Life Systems completed a Ground-based Space Station Experiment Development Study Program which verifies through testing the performance and applicability of the electrochemical <span class="hlt">Air</span>-Polarized Carbon Dioxide Concentrator (APC) process technology for space missions requiring low (i.e., less than 3 mm Hg) <span class="hlt">CO</span><span class="hlt">2</span> partial pressure (p<span class="hlt">CO</span><span class="hlt">2</span>) in the cabin atmosphere. Required test hardware was developed and testing was accomplished at an approximate one-person capacity <span class="hlt">CO</span><span class="hlt">2</span> removal level. Initially, two five-cell electrochemical modules using flight-like 0.5 sq ft cell hardware were tested individually, following by their testing at the integrated APC system level. Testing verified previously projected performance and established a database for sizing of APC systems. A four person capacity APC system was sized and compared with four candidate <span class="hlt">CO</span><span class="hlt">2</span> removal systems. At its weight of 252 lb, a volume of 7 cu ft and a power consumption of 566 W while operating at <span class="hlt">2.2</span> mm Hg p<span class="hlt">CO</span><span class="hlt">2</span>, the APC was surpassed only by an Electrochemical Depolarized <span class="hlt">CO</span><span class="hlt">2</span> Concentrator (EDC) (operating with H<span class="hlt">2</span>), when compared on a total equivalent basis.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3557064','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3557064"><span>Relationship between <span class="hlt">sea</span> level and climate forcing by <span class="hlt">CO</span><span class="hlt">2</span> on geological timescales</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Foster, Gavin L.; Rohling, Eelco J.</p> <p>2013-01-01</p> <p>On 103- to 106-year timescales, global <span class="hlt">sea</span> level is determined largely by the volume of ice stored on land, which in turn largely reflects the thermal state of the Earth system. Here we use observations from five well-studied time slices covering the last 40 My to identify a well-defined and clearly sigmoidal relationship between atmospheric <span class="hlt">CO</span><span class="hlt">2</span> and <span class="hlt">sea</span> level on geological (near-equilibrium) timescales. This strongly supports the dominant role of <span class="hlt">CO</span><span class="hlt">2</span> in determining Earth’s climate on these timescales and suggests that other variables that influence long-term global climate (e.g., topography, ocean circulation) play a secondary role. The relationship between <span class="hlt">CO</span><span class="hlt">2</span> and <span class="hlt">sea</span> level we describe portrays the “likely” (68% probability) long-term <span class="hlt">sea</span>-level response after Earth system adjustment over many centuries. Because it appears largely independent of other boundary condition changes, it also may provide useful long-range predictions of future <span class="hlt">sea</span> level. For instance, with <span class="hlt">CO</span><span class="hlt">2</span> stabilized at 400–450 ppm (as required for the frequently quoted “acceptable warming” of <span class="hlt">2</span> °C), or even at AD 2011 levels of 392 ppm, we infer a likely (68% confidence) long-term <span class="hlt">sea</span>-level rise of more than 9 m above the present. Therefore, our results imply that to avoid significantly elevated <span class="hlt">sea</span> level in the long term, atmospheric <span class="hlt">CO</span><span class="hlt">2</span> should be reduced to levels similar to those of preindustrial times. PMID:23292932</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20060044030&hterms=SLP&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DSLP','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060044030&hterms=SLP&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DSLP"><span>Ross <span class="hlt">sea</span> ice motion, area <span class="hlt">flux</span>, and deformation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>kwok, Ron</p> <p>2005-01-01</p> <p>The <span class="hlt">sea</span> ice motion, area export, and deformation of the Ross <span class="hlt">Sea</span> ice cover are examined with satellite passive microwave and RADARSAT observations. The record of high-resolution synthetic aperture radar (SAR) data, from 1998 and 2000, allows the estimation of the variability of ice deformation at the small scale (10 km) and to assess the quality of the longer record of passive microwave ice motion. Daily and subdaily deformation fields and RADARSAT imagery highlight the variability of motion and deformation in the Ross <span class="hlt">Sea</span>. With the passive microwave ice motion, the area export at a <span class="hlt">flux</span> gate positioned between Cape Adare and Land Bay is estimated. Between 1992 and 2003, a positive trend can be seen in the winter (March-November) ice area <span class="hlt">flux</span> that has a mean of 990 x 103 km<span class="hlt">2</span> and ranges from a low of 600 x 103 km<span class="hlt">2</span> in 1992 to a peak of 1600 x 103 km<span class="hlt">2</span> in 2001. In the mean, the southern Ross <span class="hlt">Sea</span> produces almost twice its own area of <span class="hlt">sea</span> ice during the winter. Cross-gate <span class="hlt">sea</span> level pressure (SLP) gradients explain 60% of the variance in the ice area <span class="hlt">flux</span>. A positive trend in this gradient, from reanalysis products, suggests a 'spinup' of the Ross <span class="hlt">Sea</span> Gyre over the past 12 yr. In both the NCEP-NCAR and ERA-40 surface pressure fields, longer-term trends in this gradient and mean SLP between 1979 and 2002 are explored along with positive anomalies in the monthly cross-gate SLP gradient associated with the positive phase of the Southern Hemisphere annular mode and the extrapolar Southern Oscillation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1910878A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1910878A"><span>In situ observations of ocean productivity using the <span class="hlt">Sea</span>Cycler mooring in the central Labrador <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Atamanchuk, Dariia; Koelling, Jannes; Devred, Emmanuel; Siddall, Greg; Send, Uwe; Wallace, Douglas</p> <p>2017-04-01</p> <p>The Central Labrador <span class="hlt">Sea</span> is a major deep-convection region in the NW Atlantic which is the most intense sink for anthropogenic carbon in the global ocean (de Vries et al, 2013). <span class="hlt">CO</span><span class="hlt">2</span> enters the ocean by <span class="hlt">air-sea</span> exchange and is transported into the ocean's interior mainly though the biological pump (Longhurst et al., 1989). Despite its important role for <span class="hlt">CO</span><span class="hlt">2</span> uptake and high natural variability, the Labrador <span class="hlt">Sea</span> is undersampled due to rough conditions and an overall lack of volunteer observing ship (VOS) transits. The <span class="hlt">Sea</span>Cycler moored profiler is currently providing year-round data from the central Labrador <span class="hlt">Sea</span> and resolves daily changes of inorganic carbon and related properties from the upper 150m of the water column. <span class="hlt">Sea</span>Cycler's sensor float is equipped with 13 physical, chemical and biooptical sensors which measure temperature, salinity, dissolved gases, nutrients and optical properties of seawater. A combination of Pro-CV (Pro-Oceanus Inc, Canada) and <span class="hlt">CO</span><span class="hlt">2</span> optode (Aanderaa, Norway) sensors in profiling mode provides a detailed description of Dissolved Inorganic Carbon (DIC) dynamics in the upper 150m over the productive season. This allows, for the first time, high-resolution carbon-based estimates of ocean productivity from throughout the euphotic zone over an annual cycle which can be compared to estimates derived from simultaneous oxygen and nitrate (Deep SUNA, Satlantic LP, Canada) profiles. These in situ carbon, nitrogen and oxygen-based estimates of using in-situ data are further compared with remotely-sensed estimates from MODIS satellite data. The <span class="hlt">Sea</span>Cycler data allow estimation of the annual cycle of the <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> and carbon export. Concurrently recorded in-situ bio-optical data allow direct comparison of optical measurements of biomass change and reveal key patterns in the seasonal succession of phytoplankton groups responsible for carbon drawdown.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/48404','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/48404"><span>Diffusional <span class="hlt">flux</span> of <span class="hlt">CO</span><span class="hlt">2</span> through snow: Spatial and temporal variability among alpine-subalpine sites</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Richard A. Sommerfeld; William J. Massman; Robert C. Musselman</p> <p>1996-01-01</p> <p>Three alpine and three subalpine sites were monitored for up to 4 years to acquire data on the temporal and spatial variability of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> through snowpacks. We conclude that the snow formed a passive cap which controlled the concentration of <span class="hlt">CO</span><span class="hlt">2</span> at the snow-soil interface, while the <span class="hlt">flux</span> of <span class="hlt">CO</span><span class="hlt">2</span> into the atmosphere was controlled by <span class="hlt">CO</span><span class="hlt">2</span> production in the soil....</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSPO34A3029C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSPO34A3029C"><span>Comparison of seawater <span class="hlt">CO</span><span class="hlt">2</span> system in summer between the East China <span class="hlt">Sea</span> shelf and the Peter the Great Bay of the Japan (East) <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chuang, K. Y.; Tishchenko, P. Y.; Gong, G. C.; Chou, W. C.; Tishchenko, P. P.; Shkirnikova, E. M.</p> <p>2016-02-01</p> <p>Continental shelves are active sites of <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange and represent an important component of the global carbon budget. In this study, we investigated the <span class="hlt">CO</span><span class="hlt">2</span> system and pertinent hydrographic parameters in two distinct continental shelf systems in the Northwest Pacific in summer 2014: the East China <span class="hlt">Sea</span> shelf (ECSS) and the Peter the Great Bay (PGB) of the Japan/East <span class="hlt">Sea</span>. The results show that the average temperature, pH, chlorophyll a and nutrients in the ECSS are higher, but salinity, dissolved inorganic carbon, and fugacity of <span class="hlt">CO</span><span class="hlt">2</span> are lower than those in the PGB. Meanwhile, the ECSS acted as a sink of atmospheric <span class="hlt">CO</span><span class="hlt">2</span>, but the PGB was a source. We suggest that the observed divergent behaviors in terms of <span class="hlt">CO</span><span class="hlt">2</span> absorption between the ECSS and the PGB may be associated with their difference in riverine runoff. Under the influence of the Yangtze River, the nutrient discharge into the ECSS is much higher than that into the PGB, where only a few small rivers empty into. The high nutrient discharge into the ECSS may stimulate high biological production, which may drawdown <span class="hlt">CO</span><span class="hlt">2</span> and thereby driving the ECSS to act as a <span class="hlt">CO</span><span class="hlt">2</span> sink despite high temperature in summer. On the contrary, the warming effect may dominate over the effect of biological production in the PGB due to the limited nutrient discharge, and thus turn the PGB to be a source of atmospheric <span class="hlt">CO</span><span class="hlt">2</span>. The results of this study imply that riverine nutrient discharge may exert a large control on net ecosystem productivity in shelf areas, which may subsequently play a critical role on determining whether a shelf system acts as a source or a sink of atmospheric <span class="hlt">CO</span><span class="hlt">2</span>.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_16 --> <div id="page_17" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li class="active"><span>17</span></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="321"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.A54A..05M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.A54A..05M"><span>Gulf of Mexico <span class="hlt">Air/Sea</span> Interaction: Measurements and Initial Data Characterization</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>MacDonald, C.; Huang, C. H.; Roberts, P. T.; Bariteau, L.; Fairall, C. W.; Gibson, W.; Ray, A.</p> <p>2011-12-01</p> <p>Corporate, government, and university researchers collaborated to develop an atmospheric boundary layer environmental observations program on an offshore platform in the Gulf of Mexico. The primary goals of this project were to provide data to (1) improve our understanding of boundary layer processes and <span class="hlt">air-sea</span> interaction over the Gulf of Mexico; (<span class="hlt">2</span>) improve regional-scale meteorological and <span class="hlt">air</span> quality modeling; and (3) provide a framework for advanced offshore measurements to support future needs such as emergency response, exploration and lease decisions, wind energy research and development, and meteorological and <span class="hlt">air</span> quality forecasting. In October 2010, meteorological and oceanographic sensors were deployed for an extended period (approximately 12 months) on a Chevron service platform (ST 52B, 90.5W, 29N) to collect boundary layer and <span class="hlt">sea</span> surface data sufficient to support these objectives. This project has significant importance given the large industrial presence in the Gulf, sizeable regional population nearby, and the recognized need for precise and timely pollutant forecasts. Observations from this project include surface meteorology; sodar marine boundary layer winds; microwave radiometer profiles of temperature, relative humidity, and liquid water; ceilometer cloud base heights; water temperature and current profiles; <span class="hlt">sea</span> surface temperature; wave height statistics; downwelling solar and infrared radiation; and <span class="hlt">air-sea</span> turbulent momentum and heat <span class="hlt">fluxes</span>. This project resulted in the collection of an unprecedented set of boundary layer measurements over the Gulf of Mexico that capture the range of meteorological and oceanographic interactions and processes that occur over an entire year. This presentation will provide insight into the logistical and scientific issues associated with the deployment and operations of unique measurements in offshore areas and provide results from an initial data analysis of boundary layer processes over the Gulf of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1714679M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1714679M"><span>Carbon speciation at the <span class="hlt">air-sea</span> interface during rain</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>McGillis, Wade; Hsueh, Diana; Takeshita, Yui; Donham, Emily; Markowitz, Michele; Turk, Daniela; Martz, Todd; Price, Nicole; Langdon, Chris; Najjar, Raymond; Herrmann, Maria; Sutton, Adrienne; Loose, Brice; Paine, Julia; Zappa, Christopher</p> <p>2015-04-01</p> <p>This investigation demonstrates the surface ocean dilution during rain events on the ocean and quantifies the lowering of surface p<span class="hlt">CO</span><span class="hlt">2</span> affecting the <span class="hlt">air-sea</span> exchange of carbon dioxide. Surface salinity was measured during rain events in Puerto Rico, the Florida Keys, East Coast USA, Panama, and the Palmyra Atoll. End-member analysis is used to determine the subsequent surface ocean carbonate speciation. Surface ocean carbonate chemistry was measured during rain events to verify any approximations made. The physical processes during rain (cold, fresh water intrusion and buoyancy, surface waves and shear, microscale mixing) are described. The role of rain on surface mixing, biogeochemistry, and <span class="hlt">air-sea</span> gas exchange will be discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70188140','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70188140"><span>Historical patterns of acidification and increasing <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> associated with Florida springs</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Barrera, Kira E.; Robbins, Lisa L.</p> <p>2017-01-01</p> <p>Florida has one of the highest concentrations of springs in the world, with many discharging into rivers and predominantly into eastern Gulf of Mexico coast, and they likely influence the hydrochemistry of these adjacent waters; however, temporal and spatial trends have not been well studied. We present over 20 yr of hydrochemical, seasonally sampled data to identify temporal and spatial trends of pH, alkalinity, partial pressure of carbon dioxide (p<span class="hlt">CO</span><span class="hlt">2</span>), and <span class="hlt">CO</span><span class="hlt">2</span><span class="hlt">flux</span> from five first-order-magnitude (springs that discharge greater than <span class="hlt">2</span>.83 m3 s−1) coastal spring groups fed by the Floridan Aquifer System that ultimately discharge into the Gulf of Mexico. All spring groups had p<span class="hlt">CO</span><span class="hlt">2</span> levels (averages 3174.3–6773.<span class="hlt">2</span> μatm) that were much higher than atmospheric levels of <span class="hlt">CO</span><span class="hlt">2</span> and demonstrated statistically significant temporal decreases in pH and increases in <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span>, p<span class="hlt">CO</span><span class="hlt">2</span>, and alkalinity. Total carbon <span class="hlt">flux</span> emissions increased from each of the spring groups by between 3.48 × 107 and <span class="hlt">2</span>.856 × 108 kg C yr−1 over the time period. By 2013 the Springs Groups in total emitted more than 1.1739 × 109 kg C yr−1. Increases in alkalinity and p<span class="hlt">CO</span><span class="hlt">2</span> varied from 90.9 to 347.6 μmol kg−1 and 1262.3 to 2666.7 μatm, respectively. Coastal data show higher <span class="hlt">CO</span><span class="hlt">2</span> evasion than the open Gulf of Mexico, which suggests spring water influences nearshore waters. The results of this study have important implications for spring water quality, dissolution of the Florida carbonate platform, and identification of the effect and partitioning of carbon <span class="hlt">fluxes</span> to and within coastal and marine ecosystems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27617333','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27617333"><span>Persistent organochlorine pesticides and polychlorinated biphenyls in <span class="hlt">air</span> of the North <span class="hlt">Sea</span> region and <span class="hlt">air-sea</span> exchange.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mai, Carolin; Theobald, Norbert; Hühnerfuss, Heinrich; Lammel, Gerhard</p> <p>2016-12-01</p> <p>Organochlorine pesticides (OCPs) and polychlorinated biphenyls (PCBs) were studied to determine occurrence, levels and spatial distribution in the marine atmosphere and surface seawater during cruises in the German Bight and the wider North <span class="hlt">Sea</span> in spring and summer 2009-2010. In general, the concentrations found in <span class="hlt">air</span> are similar to, or below, the levels at coastal or near-coastal sites in Europe. Hexachlorobenzene and α-hexachlorocyclohexane (α-HCH) were close to phase equilibrium, whereas net atmospheric deposition was observed for γ-HCH. The results suggest that declining trends of HCH in seawater have been continuing for γ-HCH but have somewhat levelled off for α-HCH. Dieldrin displayed a close to phase equilibrium in nearly all the sampling sites, except in the central southwestern part of the North <span class="hlt">Sea</span>. Here atmospheric deposition dominates the <span class="hlt">air-sea</span> exchange. This region, close to the English coast, showed remarkably increased surface seawater concentrations. This observation depended neither on riverine input nor on the elevated abundances of dieldrin in the <span class="hlt">air</span> masses of central England. A net depositional <span class="hlt">flux</span> of p,p'-DDE into the North <span class="hlt">Sea</span> was indicated by both its abundance in the marine atmosphere and the changes in metabolite pattern observed in the surface water from the coast towards the open <span class="hlt">sea</span>. The long-term trends show that the atmospheric concentrations of DDT and its metabolites are not declining. Riverine input is a major source of PCBs in the German Bight and the wider North <span class="hlt">Sea</span>. Atmospheric deposition of the lower molecular weight PCBs (PCB28 and PCB52) was indicated as a major source for surface seawater pollution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.B53I..03W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.B53I..03W"><span>Warming trumps <span class="hlt">CO</span><span class="hlt">2</span>: future climate conditions suppress carbon <span class="hlt">fluxes</span> in two dominant boreal tree species</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Way, D.; Dusenge, M. E.; Madhavji, S.</p> <p>2017-12-01</p> <p>Increases in <span class="hlt">CO</span><span class="hlt">2</span> are expected to raise <span class="hlt">air</span> temperatures in northern latitudes by up to 8 °C by the end of the century. Boreal forests in these regions play a large role in the global carbon cycle, and the responses of boreal tree species to climate drivers will thus have considerable impacts on the trajectory of future <span class="hlt">CO</span><span class="hlt">2</span> increases. We grew two dominant North American boreal tree species at a range of future climate conditions to assess how carbon <span class="hlt">fluxes</span> were altered by high <span class="hlt">CO</span><span class="hlt">2</span> and warming. Black spruce (Picea mariana) and tamarack (Larix laricina) were grown from seed under either ambient (400 ppm) or elevated <span class="hlt">CO</span><span class="hlt">2</span> concentrations (750 ppm) and either ambient temperatures, moderate warming (ambient +4 °C), or extreme warming (ambient +8 °C) for six months. We measured temperature responses of net photosynthesis, maximum rates of Rubisco carboxylation (Vcmax) and electron transport (Jmax) and dark respiration to determine acclimation to the climate treatments. Overall, growth temperature had a strong effect on carbon <span class="hlt">fluxes</span>, while there were no significant effects of growth <span class="hlt">CO</span><span class="hlt">2</span>. In both species, the photosynthetic thermal optimum increased and maximum photosynthetic rates were reduced in warm-grown seedlings, but the strength of these changes varied between species. Vcmax and Jmax were also reduced in warm-grown seedlings, and this correlated with reductions in leaf N concentrations. Warming increased the activation energy for Vcmax and the thermal optimum for Jmax in both species. Respiration acclimated to elevated growth temperatures, but there were no treatment effects on the Q10 of respiration (the increase in respiration for a 10 °C increase in leaf temperature). Our results show that climate warming is likely to reduce carbon <span class="hlt">fluxes</span> in these boreal conifers, and that photosynthetic parameters used to model photosynthesis in dynamic global vegetation models acclimate to increased temperatures, but show little response to elevated <span class="hlt">CO</span><span class="hlt">2</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGC21C0952K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC21C0952K"><span>Quantifying the impact of El Niño-driven variations in temperature and precipitation on regional atmospheric <span class="hlt">CO</span><span class="hlt">2</span> growth rate variations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Keppel-Aleks, G.; Butterfield, Z.; Doney, S. C.; Dlugokencky, E. J.; Miller, J.; Morton, D. C.</p> <p>2017-12-01</p> <p>Quantifying the climatic drivers of variations in atmospheric <span class="hlt">CO</span><span class="hlt">2</span> observations over a range of timescales is necessary to develop a mechanistic understanding of the global carbon cycle that will enable prediction of future changes. Here, we combine NOAA cooperative global <span class="hlt">air</span> sampling network <span class="hlt">CO</span><span class="hlt">2</span> observations, remote sensing data, and a <span class="hlt">flux</span> perturbation model to quantify the feedbacks between interannual variability in physical climate and the atmospheric <span class="hlt">CO</span><span class="hlt">2</span> growth rate. In particular, we focus on the differences between the 1997/1998 El Niño and the 2015/2016 El Niño during which atmospheric <span class="hlt">CO</span><span class="hlt">2</span> increased at an unprecedented rate. The <span class="hlt">flux</span> perturbation model was trained on data from 1997 to 2012, and then used to predict regional atmospheric <span class="hlt">CO</span><span class="hlt">2</span> growth rate anomalies for the period from 2013 through 2016. Given gridded temperature anomalies from the Hadley Center's Climate Research Unit (CRU), precipitation anomalies from the Global Precipitation Climatology Project (GPCP), and fire emissions from the Global Fire Emissions Database (GFEDv4s), the model was able to the reproduce regional growth rate variations observed at marine boundary layer stations in the NOAA network, including the rapid <span class="hlt">CO</span><span class="hlt">2</span> growth rate in 2015/2016. The <span class="hlt">flux</span> perturbation model output suggests that the carbon cycle responses differed for1997 and 2015 El Niño periods, with tropical precipitation anomalies causing a much larger net <span class="hlt">flux</span> of <span class="hlt">CO</span><span class="hlt">2</span> to the atmosphere during the latter period, while direct fire emissions dominated the former. The <span class="hlt">flux</span> perturbation model also suggests that high temperature stress in the Northern Hemisphere extratropics contributed almost one-third of the <span class="hlt">CO</span><span class="hlt">2</span> growth rate enhancement during the 2015 El Niño. We use satellite-based metrics for atmospheric column <span class="hlt">CO</span><span class="hlt">2</span>, vegetation, and moisture to corroborate the regional El Niño impacts from the <span class="hlt">flux</span> perturbation model. Finally, we discuss how these observational results and independent data on ocean <span class="hlt">air-sea</span> <span class="hlt">flux</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20090025444','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20090025444"><span>Turbulent <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Flux</span> Measurements by Lidar: Length Scales, Results and Comparison with In-Situ Sensors</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gilbert, Fabien; Koch, Grady J.; Beyon, Jeffrey Y.; Hilton, Timothy W.; Davis, Kenneth J.; Andrews, Arlyn; Ismail, Syed; Singh, Upendra N.</p> <p>2009-01-01</p> <p>The vertical <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> in the atmospheric boundary layer (ABL) is investigated with a Doppler differential absorption lidar (DIAL). The instrument was operated next to the WLEF instrumented tall tower in Park Falls, Wisconsin during three days and nights in June 2007. Profiles of turbulent <span class="hlt">CO</span><span class="hlt">2</span> mixing ratio and vertical velocity fluctuations are measured by in-situ sensors and Doppler DIAL. Time and space scales of turbulence are precisely defined in the ABL. The eddy-covariance method is applied to calculate turbulent <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> both by lidar and in-situ sensors. We show preliminary mean lidar <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> measurements in the ABL with a time and space resolution of 6 h and 1500 m respectively. The <span class="hlt">flux</span> instrumental errors decrease linearly with the standard deviation of the <span class="hlt">CO</span><span class="hlt">2</span> data, as expected. Although turbulent fluctuations of <span class="hlt">CO</span><span class="hlt">2</span> are negligible with respect to the mean (0.1 %), we show that the eddy-covariance method can provide <span class="hlt">2</span>-h, 150-m range resolved <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> estimates as long as the <span class="hlt">CO</span><span class="hlt">2</span> mixing ratio instrumental error is no greater than 10 ppm and the vertical velocity error is lower than the natural fluctuations over a time resolution of 10 s.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.9319M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.9319M"><span><span class="hlt">CO</span><span class="hlt">2</span> and heat <span class="hlt">fluxes</span> in a recently clear-cut spruce forest in European Russia: experimental and modeling studies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mamkin, Vadim; Kurbatova, Julia; Avilov, Vitaly; Mukhartova, Yulia; Krupenko, Alexander; Ivanov, Dmitry; Levashova, Natalia; Olchev, Alexander</p> <p>2017-04-01</p> <p>Ecosystem carbon dioxide, energy, and water <span class="hlt">fluxes</span> were measured using eddy covariance and portable chambers in a fresh clear-cut surrounded by a mixed spruce-birch-aspen forest in the boreal zone of European Russia. Measurements were initiated in spring 2016 following timber harvest and continued for seven months until the end of October. The influence of surrounding forest on <span class="hlt">air</span> flow and turbulent <span class="hlt">fluxes</span> within the clear-cut were examined using a process-based two-dimensional (<span class="hlt">2</span>D) hydrodynamic turbulent exchange model. Clear-cut was a permanent source of <span class="hlt">CO</span><span class="hlt">2</span> to the atmosphere. During the period the mean daily latent (LE) and sensible (H) heat <span class="hlt">fluxes</span> were very similar and the Bowen ratio (β=H/LE) averaged about 1.0. During the late spring and summer months the net ecosystem exchange of <span class="hlt">CO</span><span class="hlt">2</span> (NEE) remained slightly positive following onset of vegetation growth, while β was changing in the range from 0.6 to 4.0. There was strong diurnal variability in NEE, LE and H over the measurement period that was governed by solar radiation and temperature as well as the leaf area index (LAI) of regrown vegetation. Modeled vertical <span class="hlt">CO</span><span class="hlt">2</span> and H<span class="hlt">2</span>O <span class="hlt">fluxes</span> along a transect that crossed the clear-cut and coincided with the dominate wind direction showed that the clear-cut strongly influenced turbulent <span class="hlt">fluxes</span> within the atmospheric surface layer. Furthermore, modeled atmospheric dynamics suggested that the clear-cut had a large influence on turbulent <span class="hlt">fluxes</span> in the downwind forest, but little impact on the upwind side. An aggregated approach including field measurements and process-based models can be used to estimate energy, water and carbon dioxide <span class="hlt">fluxes</span> in non-uniform forest landscapes. This study was supported by a grant from the Russian Science Foundation (14-14-00956).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1616784M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1616784M"><span><span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Fluxes</span> Monitoring at the Level of Field Agroecosystem in Moscow Region of Russia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Meshalkina, Joulia; Mazirov, Ilya; Samardzic, Miljan; Yaroslavtsev, Alexis; Valentini, Riccardo; Vasenev, Ivan</p> <p>2014-05-01</p> <p>The Central Russia is still one of the less GHG-investigated European areas especially in case of agroecosystem-level carbon dioxide <span class="hlt">fluxes</span> monitoring by eddy covariance method. The eddy covariance technique is a statistical method to measure and calculate vertical turbulent <span class="hlt">fluxes</span> within atmospheric boundary layers. The major assumption of the metod is that measurements at a point can represent an entire upwind area. Eddy covariance researches, which could be considered as repeated for the same area, are very rare. The research has been carried out on the Precision Farming Experimental Field of the Russian Timiryazev State Agricultural University (Moscow, Russia) in 2013 under the support of RF Government grant No. 11.G34.31.0079. Arable derno-podzoluvisls have around 1 The results have shown high daily and seasonal dynamic of agroecosystem <span class="hlt">CO</span><span class="hlt">2</span> emission. Sowing activates soil microbiological activity and the average soil <span class="hlt">CO</span><span class="hlt">2</span> emission and adsorption are rising at the same time. <span class="hlt">CO</span><span class="hlt">2</span> streams are intensified after crop emerging from values of 3 to 7 μmol/s-m<span class="hlt">2</span> for emission, and from values of 5 to 20 μmol/s-m<span class="hlt">2</span> for adsorption. Stabilization of the flow has come at achieving plants height of 10-12 cm. The vegetation period is characterized by high average soil <span class="hlt">CO</span><span class="hlt">2</span> emission and adsorption at the same time, but the adsorption is significantly higher. The resulted <span class="hlt">CO</span><span class="hlt">2</span> absorption during the day is approximately <span class="hlt">2</span>-5 times higher than emissions at night. For example, in mid-June, the absorption value was about 0.45 mol/m<span class="hlt">2</span> during the day-time, and the emission value was about 0.1 mol/m<span class="hlt">2</span> at night. After harvesting <span class="hlt">CO</span><span class="hlt">2</span> emission is becoming essentially higher than adsorption. Autumn and winter data are fluctuate around zero, but for some periods a small predominance of <span class="hlt">CO</span><span class="hlt">2</span> emissions over the absorption may be observed. The daily dynamics of <span class="hlt">CO</span><span class="hlt">2</span> emissions depends on the <span class="hlt">air</span> temperature with the correlation coefficient changes between 0.4 and 0.8. Crop stage, agrotechnological</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSPC43A..04B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSPC43A..04B"><span>Temporal Variability of North Atlantic Carbon <span class="hlt">Fluxes</span> and their Sensitivity to the Meridional Overturning Circulation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brown, P.; McDonagh, E.; Sanders, R.; King, B.; Watson, A. J.; Schuster, U.; Henson, S.</p> <p>2016-02-01</p> <p>The North Atlantic plays a critical role in the global carbon cycle both as a region of substantial <span class="hlt">air-sea</span> carbon dioxide uptake and as a location for the transfer of <span class="hlt">CO</span><span class="hlt">2</span> to depth on climatically-important timescales. While the magnitude of surface <span class="hlt">fluxes</span> is relatively well constrained, our understanding of the processes that drive variability in ocean-atmosphere exchange and subsequent subsurface carbon accumulation is not as well defined. Here we present observation-derived high-resolution estimates of short-term 10-day meridional ocean carbon transport variability across the subtropical North Atlantic for 2004-2012. Substantial seasonal, sub-annual and interannual transport variability is observed that is highly sensitive to the strength of the Atlantic Meridional Overturning Circulation. While the recently identified multi-year decrease in AMOC strength similarly impacts carbon transports, its full effect is masked by the northwards transport of increasing surface <span class="hlt">CO</span><span class="hlt">2</span> levels. A 30% slowdown in the meridional circulation in 2009-2010 and the anomalous effects it had on the transport, storage and divergence of heat and freshwater in the subtropical and subpolar gyres and local wind regimes are investigated for their impact on local <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. Temperature and salt content anomalies identified in each gyre are found to drive (subtropics) or hinder (subpolar) additional carbon uptake from the atmosphere by affecting the physical solubility pump for <span class="hlt">CO</span><span class="hlt">2</span>. Additionally their simultaneous effect on mixed layer depth and the vertical supply of nutrients to the surface is shown to magnify the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> observed by driving anomalous primary production rates.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1710530G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1710530G"><span>Potentials and challenges associated with automated closed dynamic chamber measurements of soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Görres, Carolyn-Monika; Kammann, Claudia; Ceulemans, Reinhart</p> <p>2015-04-01</p> <p>Soil respiration <span class="hlt">fluxes</span> are influenced by natural factors such as climate and soil type, but also by anthropogenic activities in managed ecosystems. As a result, soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> show a large intra- and interannual as well as intra- and intersite variability. Most of the available soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> data giving insights into this variability have been measured with manually closed static chambers, but technological advances in the past 15 years have also led to an increased use of automated closed chamber systems. The great advantage of automated chambers in comparison to manually operated chambers is the higher temporal resolution of the <span class="hlt">flux</span> data. This is especially important if we want to better understand the effects of short-term events, e.g. fertilization or heavy rainfall, on soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> variability. However, the chamber method is an invasive measurement method which can potentially alter soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> and lead to biased measurement results. In the peer-reviewed literature, many papers compare the field performance and results of different closed static chamber designs, or compare manual chambers with automated chamber systems, to identify potential biases in <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> measurements, and thus help to reduce uncertainties in the <span class="hlt">flux</span> data. However, inter-comparisons of different automated closed dynamic chamber systems are still lacking. Here we are going to present a field comparison of the most-cited automated chamber system, the LI-8100A Automated Soil <span class="hlt">Flux</span> System, with the also commercially available Greenhouse Gas Monitoring System AGPS. Both measurement systems were installed side by side at a recently harvested poplar bioenergy plantation (POPFULL, http://uahost.uantwerpen.be/popfull/) from April 2014 until August 2014. The plantation provided optimal comparison conditions with a bare field situation after the harvest and a regrowing canopy resulting in a broad variety of microclimates. Furthermore, the plantation was planted in a double-row system with</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFMOS34B..01S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMOS34B..01S"><span>Tropical Cyclone Induced <span class="hlt">Air-Sea</span> Interactions Over Oceanic Fronts</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shay, L. K.</p> <p>2012-12-01</p> <p>Recent severe tropical cyclones underscore the inherent importance of warm background ocean fronts and their interactions with the atmospheric boundary layer. Central to the question of heat and moisture <span class="hlt">fluxes</span>, the amount of heat available to the tropical cyclone is predicated by the initial mixed layer depth and strength of the stratification that essentially set the level of entrainment mixing at the base of the mixed layer. In oceanic regimes where the ocean mixed layers are thin, shear-induced mixing tends to cool the upper ocean to form cold wakes which reduces the <span class="hlt">air-sea</span> <span class="hlt">fluxes</span>. This is an example of negative feedback. By contrast, in regimes where the ocean mixed layers are deep (usually along the western part of the gyres), warm water advection by the nearly steady currents reduces the levels of turbulent mixing by shear instabilities. As these strong near-inertial shears are arrested, more heat and moisture transfers are available through the enthalpy <span class="hlt">fluxes</span> (typically 1 to 1.5 kW m-<span class="hlt">2</span>) into the hurricane boundary layer. When tropical cyclones move into favorable or neutral atmospheric conditions, tropical cyclones have a tendency to rapidly intensify as observed over the Gulf of Mexico during Isidore and Lili in 2002, Katrina, Rita and Wilma in 2005, Dean and Felix in 2007 in the Caribbean <span class="hlt">Sea</span>, and Earl in 2010 just north of the Caribbean Islands. To predict these tropical cyclone deepening (as well as weakening) cycles, coupled models must have ocean models with realistic ocean conditions and accurate <span class="hlt">air-sea</span> and vertical mixing parameterizations. Thus, to constrain these models, having complete 3-D ocean profiles juxtaposed with atmospheric profiler measurements prior, during and subsequent to passage is an absolute necessity framed within regional scale satellite derived fields.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A51M..01A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A51M..01A"><span>North American <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> for 2007-2015 from NOAA's CarbonTracker-Lagrange Regional Inverse Modeling Framework</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Andrews, A. E.; Hu, L.; Thoning, K. W.; Nehrkorn, T.; Mountain, M. E.; Jacobson, A. R.; Michalak, A.; Dlugokencky, E. J.; Sweeney, C.; Worthy, D. E. J.; Miller, J. B.; Fischer, M. L.; Biraud, S.; van der Velde, I. R.; Basu, S.; Tans, P. P.</p> <p>2017-12-01</p> <p>CarbonTracker-Lagrange (CT-L) is a new high-resolution regional inverse modeling system for improved estimation of North American <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. CT-L uses footprints from the Stochastic Time-Inverted Lagrangian Transport (STILT) model driven by high-resolution (10 to 30 km) meteorological fields from the Weather Research and Forecasting (WRF) model. We performed a suite of synthetic-data experiments to evaluate a variety of inversion configurations, including (1) solving for scaling factors to an a priori <span class="hlt">flux</span> versus additive corrections, (<span class="hlt">2</span>) solving for <span class="hlt">fluxes</span> at 3-hrly resolution versus at coarser temporal resolution, (3) solving for <span class="hlt">fluxes</span> at 1o × 1o resolution versus at large eco-regional scales. Our framework explicitly and objectively solves for the optimal solution with a full error covariance matrix with maximum likelihood estimation, thereby enabling rigorous uncertainty estimates for the derived <span class="hlt">fluxes</span>. In the synthetic-data inversions, we find that solving for weekly scaling factors of a priori Net Ecosystem Exchange (NEE) at 1o × 1o resolution with optimization of diurnal cycles of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> yields faithful retrieval of the specified "true" <span class="hlt">fluxes</span> as those solved at 3-hrly resolution. In contrast, a scheme that does not allow for optimization of diurnal cycles of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> suffered from larger aggregation errors. We then applied the optimal inversion setup to estimate North American <span class="hlt">fluxes</span> for 2007-2015 using real atmospheric <span class="hlt">CO</span><span class="hlt">2</span> observations, multiple prior estimates of NEE, and multiple boundary values estimated from the NOAA's global Eulerian CarbonTracker (CarbonTracker) and from an empirical approach. Our derived North American land <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> show larger seasonal amplitude than those estimated from the CarbonTracker, removing seasonal biases in the CarbonTracker's simulated <span class="hlt">CO</span><span class="hlt">2</span> mole fractions. Independent evaluations using in-situ <span class="hlt">CO</span><span class="hlt">2</span> eddy covariance <span class="hlt">flux</span> measurements and independent aircraft profiles also suggest an improved estimation on North</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140013403','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140013403"><span>Trends and Variations of Ocean Surface Latent Heat <span class="hlt">Flux</span>: Results from GSSTF<span class="hlt">2</span>c Data Set</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gao, Si; Chiu, Long S.; Shie, Chung-Lin</p> <p>2013-01-01</p> <p>Trends and variations of Goddard Satellite-based Surface Turbulent <span class="hlt">Fluxes</span> (GSSTF) version <span class="hlt">2</span>c (GSSTF<span class="hlt">2</span>c) latent heat <span class="hlt">flux</span> (LHF) are examined. This version of LHF takes account of the correction in Earth incidence angle. The trend of global mean LHF for GSSTF<span class="hlt">2</span>c is much reduced relative to GSSTF version <span class="hlt">2</span>b Set 1 and Set <span class="hlt">2</span> for the same period 1988-2008. Temporal increase of GSSTF<span class="hlt">2</span>c LHF in the two decades is 11.0%, in which 3.1%, 5.8%, and <span class="hlt">2</span>.1% are attributed to the increase in wind, the increase in <span class="hlt">sea</span> surface saturated <span class="hlt">air</span> humidity, and the decrease in near-surface <span class="hlt">air</span> humidity, respectively. The first empirical orthogonal function of LHF is a conventional El Nino Southern Oscillation (ENSO) mode. However, the trends in LHF are independent of conventional ENSO phenomena. After removing ENSO signal, the pattern of LHF trends is primarily determined by the pattern of <span class="hlt">air-sea</span> humidity difference trends.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017CSR...141...38L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017CSR...141...38L"><span>A source of <span class="hlt">CO</span><span class="hlt">2</span> to the atmosphere throughout the year in the Maranhense continental shelf (<span class="hlt">2</span>°30'S, Brazil)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lefèvre, Nathalie; da Silva Dias, Francisco Jose; de Torres, Audálio Rebelo; Noriega, Carlos; Araujo, Moacyr; de Castro, Antonio Carlos Leal; Rocha, Carlos; Jiang, Shan; Ibánhez, J. Severino P.</p> <p>2017-06-01</p> <p>To reduce uncertainty regarding the contribution of continental shelf areas in low latitude regions to the <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange, more data are required to understand the carbon turnover in these regions and cover gaps in coverage. For the first time, inorganic carbon and alkalinity were measured along a cross-shelf transect off the coast of Maranhão (North Brazil) in 9 cruises spawning from April 2013 to September 2014. On the last 4 transects, dissolved organic matter and nutrients were also measured. The highest inorganic and organic carbon concentrations are observed close to land. As a result of low productivity and significant remineralization, heterotrophy dominates along the transect throughout the year. Although the temporal variability is significantly reduced at the offshore station with carbon concentrations decreasing seaward, the fugacity of <span class="hlt">CO</span><span class="hlt">2</span> (f<span class="hlt">CO</span><span class="hlt">2</span>) at this station remains significantly higher, especially during the wet season, than the open ocean values measured routinely by a merchant ship further west. Overall, the continental shelf is a weak source of <span class="hlt">CO</span><span class="hlt">2</span> to the atmosphere throughout the year with an annual mean <span class="hlt">flux</span> of 1.81±0.84 mmol m-<span class="hlt">2</span> d-1. The highest magnitudes of f<span class="hlt">CO</span><span class="hlt">2</span> are observed during the wet season when the winds are the weakest. As a result, the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> does not show a clear seasonal pattern. Further offshore, f<span class="hlt">CO</span><span class="hlt">2</span> is significantly lower than on the continental shelf. However, the oceanic <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span>, with an annual mean of <span class="hlt">2</span>.32±1.09 mmol m-<span class="hlt">2</span> d-1, is not statistically different from the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> at the continental shelf because the wind is stronger in the open ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUSM.U32A..01G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUSM.U32A..01G"><span>Measurement of Urban <span class="hlt">fluxes</span> of <span class="hlt">CO</span><span class="hlt">2</span> and water</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Grimmond, S.; Crawford, B.; Offerle, B.; Hom, J.</p> <p>2006-05-01</p> <p>Measurements of surface-atmosphere <span class="hlt">fluxes</span> of carbon dioxide (FCO<span class="hlt">2</span>) and latent heat in urban environments are rare even though cities are a major source of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> and users of water. In this paper, an overview of urban FCO<span class="hlt">2</span> measurements will be presented to illustrate how and where such measurements are being conducted and emerging results to date. Most of these studies have been conducted over short periods of time; few studies have considered annual sources/sinks. More investigations have been conducted, and are planned, in European cities than elsewhere, most commonly in areas of medium density urban development. The most dense urban sites are significant net sources of carbon. However, in areas where there is large amounts of vegetation present, there is a net sink of carbon during the summertime. In the second part of the presentation, more detailed attention will be directed to an ongoing measurement program in Baltimore, MD (part of the Baltimore Ecosystem Study). Eddy covariance instrumentation mounted on a tall-tower at 41.<span class="hlt">2</span> m has continuously measured local-scale <span class="hlt">fluxes</span> of carbon dioxide from a suburban environment since 2001. Several features make this particular study unique: 1) for an urban area, the study site is extensively vegetated, <span class="hlt">2</span>) the period of record (2001-2005) is among the longest available for urban FCO<span class="hlt">2</span> measurements, 3) both closed-path and open-path infrared gas analyzers are used for observations, and 4) several unique data quality control and gap-filling methods have been developed for use in an urban environment. Additionally, detailed surface datasets and GIS software are used to perform <span class="hlt">flux</span> source area analysis. Results from Baltimore indicate that FCO<span class="hlt">2</span> is very dependent on source area land-cover characteristics, particularly the proportion of vegetated and built surfaces. Over the course of a year, the urban surface is a strong net source of <span class="hlt">CO</span><span class="hlt">2</span>, though there is considerable inter-annual variability depending on</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1917180Q','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1917180Q"><span>Land use and rainfall effect on soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in a Mediterranean agroforestry system</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Quijano, Laura; Álvaro-Fuentes, Jorge; Lizaga, Iván; Navas, Ana</p> <p>2017-04-01</p> <p>Soils are the largest C reservoir of terrestrial ecosystems and play an important role in regulating the concentration of <span class="hlt">CO</span><span class="hlt">2</span> in the atmosphere. The exchange of <span class="hlt">CO</span><span class="hlt">2</span> between the atmosphere and soil controls the balance of C in soils. The <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> may be influenced by climate conditions and land use and cover change especially in the upper soil organic layer. Understanding C dynamics is important for maintaining C stocks to sustain and improve soil quality and to enhance sink C capacity of soils. This study focuses on the response of the <span class="hlt">CO</span><span class="hlt">2</span> emitted to rainfall events from different land uses (i.e. forest, abandoned cultivated soils and winter cereal cultivated soils) in a representative Mediterranean agroforestry ecosystem in the central part of the Ebro basin, NE Spain (30T 4698723N 646424E). A total of 30 measurement points with the same soil type (classified as Calcisols) were selected. Soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> was measured in situ using a portable EGM-4 <span class="hlt">CO</span><span class="hlt">2</span> analyzer PPSystems connected to a dynamic chamber system (model CFX-1, PPSystems) weekly during autumn 2016. Eleven different rainfall events were measured at least 24 hours before (n=7) and after the rainfall event (n=4). Soil water content and temperature were measured at each sampling point within the first 5 cm. Soil samples were taken at the beginning of the experiment to determine soil organic carbon (SOC) content using a LECO RC-612. The mean SOC for forest, abandoned and cultivated soils were <span class="hlt">2</span>.5, <span class="hlt">2</span>.7 and 0.6 %, respectively. The results indicated differences in soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> between land uses. The field measurements of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> show that before cereal sowing the highest values were recorded in the abandoned soils varying from 56.1 to 171.9 mg <span class="hlt">CO</span><span class="hlt">2</span>-C m-<span class="hlt">2</span> h-1 whereas after cereal sowing the highest values were recorded in cultivated soils ranged between 37.8 and 116.<span class="hlt">2</span> mg <span class="hlt">CO</span><span class="hlt">2</span>-C m-<span class="hlt">2</span> h-1 indicating the agricultural impact on <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. In cultivated soils, lower mean <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> were measured after direct seeding</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=340834&Lab=NHEERL&keyword=Change+AND+climate&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50','EPA-EIMS'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=340834&Lab=NHEERL&keyword=Change+AND+climate&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50"><span>Nitrous oxide <span class="hlt">flux</span> under changing temperature and <span class="hlt">CO</span><span class="hlt">2</span></span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p>We are investigating nitrous oxide <span class="hlt">flux</span> seasonal trends and response to temperature and <span class="hlt">CO</span><span class="hlt">2</span> increases in a boreal peatland. Peatlands located in boreal regions make up a third of global wetland area and are expected to have the highest temperature increases in response to climat...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1306691-direct-capture-co2-from-ambient-air','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1306691-direct-capture-co2-from-ambient-air"><span>Direct capture of <span class="hlt">CO</span> <span class="hlt">2</span> from ambient <span class="hlt">air</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Sanz-Perez, Eloy S.; Murdock, Christopher R.; Didas, Stephanie A.</p> <p></p> <p>The increase in the global atmospheric <span class="hlt">CO</span> <span class="hlt">2</span> concentration resulting from over a century of combustion of fossil fuels has been associated with significant global climate change. With the global population increase driving continued increases in fossil fuel use, humanity’s primary reliance on fossil energy for the next several decades is assured. Traditional modes of carbon capture such as precombustion and postcombustion <span class="hlt">CO</span> <span class="hlt">2</span> capture from large point sources can help slow the rate of increase of the atmospheric <span class="hlt">CO</span> <span class="hlt">2</span> concentration, but only the direct removal of <span class="hlt">CO</span> <span class="hlt">2</span> from the <span class="hlt">air</span>, or “direct <span class="hlt">air</span> capture” (DAC), can actuallymore » reduce the global atmospheric <span class="hlt">CO</span> <span class="hlt">2</span> concentration. The past decade has seen a steep rise in the use of chemical sorbents that are cycled through sorption and desorption cycles for <span class="hlt">CO</span> <span class="hlt">2</span> removal from ultradilute gases such as <span class="hlt">air</span>. This Review provides a historical overview of the field of DAC, along with an exhaustive description of the use of chemical sorbents targeted at this application. Solvents and solid sorbents that interact strongly with <span class="hlt">CO</span> <span class="hlt">2</span> are described, including basic solvents, supported amine and ammonium materials, and metal-organic frameworks (MOFs), as the primary classes of chemical sorbents. Hypothetical processes for the deployment of such sorbents are discussed, as well as the limited array of technoeconomic analyses published on DAC. Overall, it is concluded that there are many new materials that could play a role in emerging DAC technologies. Furthermore, these materials need to be further investigated and developed with a practical sorbent-<span class="hlt">air</span> contacting process in mind if society is to make rapid progress in deploying DAC as a means of mitigating climate change.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1306691-direct-capture-co2-from-ambient-air','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1306691-direct-capture-co2-from-ambient-air"><span>Direct capture of <span class="hlt">CO</span> <span class="hlt">2</span> from ambient <span class="hlt">air</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Sanz-Perez, Eloy S.; Murdock, Christopher R.; Didas, Stephanie A.; ...</p> <p>2016-08-25</p> <p>The increase in the global atmospheric <span class="hlt">CO</span> <span class="hlt">2</span> concentration resulting from over a century of combustion of fossil fuels has been associated with significant global climate change. With the global population increase driving continued increases in fossil fuel use, humanity’s primary reliance on fossil energy for the next several decades is assured. Traditional modes of carbon capture such as precombustion and postcombustion <span class="hlt">CO</span> <span class="hlt">2</span> capture from large point sources can help slow the rate of increase of the atmospheric <span class="hlt">CO</span> <span class="hlt">2</span> concentration, but only the direct removal of <span class="hlt">CO</span> <span class="hlt">2</span> from the <span class="hlt">air</span>, or “direct <span class="hlt">air</span> capture” (DAC), can actuallymore » reduce the global atmospheric <span class="hlt">CO</span> <span class="hlt">2</span> concentration. The past decade has seen a steep rise in the use of chemical sorbents that are cycled through sorption and desorption cycles for <span class="hlt">CO</span> <span class="hlt">2</span> removal from ultradilute gases such as <span class="hlt">air</span>. This Review provides a historical overview of the field of DAC, along with an exhaustive description of the use of chemical sorbents targeted at this application. Solvents and solid sorbents that interact strongly with <span class="hlt">CO</span> <span class="hlt">2</span> are described, including basic solvents, supported amine and ammonium materials, and metal-organic frameworks (MOFs), as the primary classes of chemical sorbents. Hypothetical processes for the deployment of such sorbents are discussed, as well as the limited array of technoeconomic analyses published on DAC. Overall, it is concluded that there are many new materials that could play a role in emerging DAC technologies. Furthermore, these materials need to be further investigated and developed with a practical sorbent-<span class="hlt">air</span> contacting process in mind if society is to make rapid progress in deploying DAC as a means of mitigating climate change.« less</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li class="active"><span>17</span></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_17 --> <div id="page_18" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="341"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/43522','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/43522"><span>High-frequency pressure variations in the vicinity of a surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> chamber</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Eugene S. Takle; James R. Brandle; R. A. Schmidt; Rick Garcia; Irina V. Litvina; William J. Massman; Xinhua Zhou; Geoffrey Doyle; Charles W. Rice</p> <p>2003-01-01</p> <p>We report measurements of <span class="hlt">2</span>Hz pressure fluctuations at and below the soil surface in the vicinity of a surface-based <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> chamber. These measurements were part of a field experiment to examine the possible role of pressure pumping due to atmospheric pressure fluctuations on measurements of surface <span class="hlt">fluxes</span> of <span class="hlt">CO</span><span class="hlt">2</span>. Under the moderate wind speeds, warm temperatures,...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1915402S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1915402S"><span>Results from twelve years of continuous monitoring of the soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> at the Ketzin <span class="hlt">CO</span><span class="hlt">2</span> storage pilot site, Germany</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Szizybalski, Alexandra; Zimmer, Martin; Pilz, Peter; Liebscher, Axel</p> <p>2017-04-01</p> <p>Under the coordination of the GFZ German Research Centre for Geosciences the complete life-cycle of a geological storage site for <span class="hlt">CO</span><span class="hlt">2</span> has been investigated and studied in detail over the past 12 years at Ketzin near Berlin, Germany. The test site is located at the southern flank of an anticlinal structure. Beginning with an exploration phase in 2004, drilling of the first three wells took place in 2007. From June 2008 to August 2013 about 67 kt of <span class="hlt">CO</span><span class="hlt">2</span> were injected into Upper Triassic sandstones at a depth of 630 to 650 m overlain by more than 165 m of shaley cap rocks. A comprehensive operational and scientific monitoring program forms the central part of the Ketzin project targeting at the reservoir itself, its overburden or above-zone and the surface. The surface monitoring is done by continuous soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> measurements. These already started in 2005, more than three years prior to the injection phase using a survey chamber from LI-COR Inc. Twenty sampling locations were selected in the area of the anticline covering about 3 x 3 km. In order to obtain information on seasonal trends, measurements are performed at least once a month. The data set obtained prior to the injection serves as a basis for comparison with all further measurements during the injection and storage operations [Zimmer et al., 2010]. To refine the monitoring network, eight automatic, permanent soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> stations were additionally installed in 2011 in the direct vicinity of the boreholes. Using this system, the <span class="hlt">CO</span><span class="hlt">2</span> soil <span class="hlt">flux</span> is measured on an hourly basis. Over the whole monitoring time, soil temperature and moisture are recorded simultaneously and soil samples down to 70 cm depth were studied for their structure, carbon and nitrogen content. ver the whole monitoring time. Both, diurnal and seasonal <span class="hlt">flux</span> variations can be detected and hence, provide a basis for interpretation of the measured data. Detailed analysis of the long-term monitoring at each station clearly reveals the influence</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1080961','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1080961"><span>Relationships between the Efficiencies of Photosystems I and II and Stromal Redox State in <span class="hlt">CO</span><span class="hlt">2</span>-Free <span class="hlt">Air</span> 1</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Harbinson, Jeremy; Foyer, Christine H.</p> <p>1991-01-01</p> <p>The responses of the efficiencies of photosystems I and II, stromal redox state (as indicated by NADP-malate dehydrogenase activation state), and activation of the Benson-Calvin cycle enzymes ribulose 1,5-bisphosphate carboxylase and fructose 1,6-bisphosphatase to varying irradiance were measured in pea (Pisum sativum L.) leaves operating close to the <span class="hlt">CO</span><span class="hlt">2</span> compensation point. A comparison of the relationships among these parameters obtained from leaves in <span class="hlt">air</span> was made with those obtained when the leaves were maintained in <span class="hlt">air</span> from which the <span class="hlt">CO</span><span class="hlt">2</span> had been removed. P700 was more oxidized at any measured irradiance in <span class="hlt">CO</span><span class="hlt">2</span>-free <span class="hlt">air</span> than in <span class="hlt">air</span>. The relationship between the quantum efficiencies of the photosystems in <span class="hlt">CO</span><span class="hlt">2</span>-free <span class="hlt">air</span> was distinctly curvilinear in contrast to the predominantly linear relationship obtained with leaves in <span class="hlt">air</span>. This nonlinearity may be consistent with the operation of cyclic electron flow around photosystem I because the quantum efficiency of photosystem II was much more restricted than the quantum efficiency of photosystem I. In <span class="hlt">CO</span><span class="hlt">2</span>-free <span class="hlt">air</span>, measured NADP-malate dehydrogenase activities varied considerably at low irradiances. However, at high irradiance the activity of the enzyme was low, implying that the stroma was oxidized. In contrast, fructose-1,6-bisphosphatase activities tended to increase with increasing electron <span class="hlt">flux</span> through the photosystems. Ribulose-1,5-bisphosphate carboxylase activity remained relatively constant with respect to irradiance in <span class="hlt">CO</span><span class="hlt">2</span>-free <span class="hlt">air</span>, with an activation state 50% of maximum. We conclude that, at the <span class="hlt">CO</span><span class="hlt">2</span> compensation point and high irradiance, low redox states are favored and that cyclic electron flow may be substantial. These two features may be the requirements necessary to trigger and maintain the dissipative processes in the thylakoid membrane. PMID:16668401</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3251141','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3251141"><span>Economic and energetic analysis of capturing <span class="hlt">CO</span><span class="hlt">2</span> from ambient <span class="hlt">air</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>House, Kurt Zenz; Baclig, Antonio C.; Ranjan, Manya; van Nierop, Ernst A.; Wilcox, Jennifer; Herzog, Howard J.</p> <p>2011-01-01</p> <p>Capturing carbon dioxide from the atmosphere (“<span class="hlt">air</span> capture”) in an industrial process has been proposed as an option for stabilizing global <span class="hlt">CO</span><span class="hlt">2</span> concentrations. Published analyses suggest these <span class="hlt">air</span> capture systems may cost a few hundred dollars per tonne of <span class="hlt">CO</span><span class="hlt">2</span>, making it cost competitive with mainstream <span class="hlt">CO</span><span class="hlt">2</span> mitigation options like renewable energy, nuclear power, and carbon dioxide capture and storage from large <span class="hlt">CO</span><span class="hlt">2</span> emitting point sources. We investigate the thermodynamic efficiencies of commercial separation systems as well as trace gas removal systems to better understand and constrain the energy requirements and costs of these <span class="hlt">air</span> capture systems. Our empirical analyses of operating commercial processes suggest that the energetic and financial costs of capturing <span class="hlt">CO</span><span class="hlt">2</span> from the <span class="hlt">air</span> are likely to have been underestimated. Specifically, our analysis of existing gas separation systems suggests that, unless <span class="hlt">air</span> capture significantly outperforms these systems, it is likely to require more than 400 kJ of work per mole of <span class="hlt">CO</span><span class="hlt">2</span>, requiring it to be powered by <span class="hlt">CO</span><span class="hlt">2</span>-neutral power sources in order to be <span class="hlt">CO</span><span class="hlt">2</span> negative. We estimate that total system costs of an <span class="hlt">air</span> capture system will be on the order of $1,000 per tonne of <span class="hlt">CO</span><span class="hlt">2</span>, based on experience with as-built large-scale trace gas removal systems. PMID:22143760</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013ACP....13.7607C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013ACP....13.7607C"><span>Improved simulation of regional <span class="hlt">CO</span><span class="hlt">2</span> surface concentrations using GEOS-Chem and <span class="hlt">fluxes</span> from VEGAS</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, Z. H.; Zhu, J.; Zeng, N.</p> <p>2013-08-01</p> <p><span class="hlt">CO</span><span class="hlt">2</span> measurements have been combined with simulated <span class="hlt">CO</span><span class="hlt">2</span> distributions from a transport model in order to produce the optimal estimates of <span class="hlt">CO</span><span class="hlt">2</span> surface <span class="hlt">fluxes</span> in inverse modeling. However, one persistent problem in using model-observation comparisons for this goal relates to the issue of compatibility. Observations at a single station reflect all underlying processes of various scales. These processes usually cannot be fully resolved by model simulations at the grid points nearest the station due to lack of spatial or temporal resolution or missing processes in the model. In this study the stations in one region were grouped based on the amplitude and phase of the seasonal cycle at each station. The regionally averaged <span class="hlt">CO</span><span class="hlt">2</span> at all stations in one region represents the regional <span class="hlt">CO</span><span class="hlt">2</span> concentration of this region. The regional <span class="hlt">CO</span><span class="hlt">2</span> concentrations from model simulations and observations were used to evaluate the regional model results. The difference of the regional <span class="hlt">CO</span><span class="hlt">2</span> concentration between observation and modeled results reflects the uncertainty of the large-scale <span class="hlt">flux</span> in the region where the grouped stations are. We compared the regional <span class="hlt">CO</span><span class="hlt">2</span> concentrations between model results with biospheric <span class="hlt">fluxes</span> from the Carnegie-Ames-Stanford Approach (CASA) and VEgetation-Global-Atmosphere-Soil (VEGAS) models, and used observations from GLOBALVIEW-<span class="hlt">CO</span><span class="hlt">2</span> to evaluate the regional model results. The results show the largest difference of the regionally averaged values between simulations with <span class="hlt">fluxes</span> from VEGAS and observations is less than 5 ppm for North American boreal, North American temperate, Eurasian boreal, Eurasian temperate and Europe, which is smaller than the largest difference between CASA simulations and observations (more than 5 ppm). There is still a large difference between two model results and observations for the regional <span class="hlt">CO</span><span class="hlt">2</span> concentration in the North Atlantic, Indian Ocean, and South Pacific tropics. The regionally averaged <span class="hlt">CO</span><span class="hlt">2</span> concentrations will be helpful for</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.2264C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.2264C"><span>METEOPOLE-<span class="hlt">FLUX</span>: an observatory of terrestrial water, energy, and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in Toulouse</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Calvet, Jean-Christophe; Roujean, Jean-Louis; Zhang, Sibo; Maurel, William; Piguet, Bruno; Barrié, Joël; Bouhours, Gilles; Couzinier, Jacques; Garrouste, Olivier; Girres, Sandrine; Suquia, David; Tzanos, Diane</p> <p>2016-04-01</p> <p>The METEOPOLE-<span class="hlt">FLUX</span> project (http://www.cnrm.meteo.fr/spip.php?article874&lang=en) aims at monitoring a large suburban set-aside field in the city of Toulouse (43.572898 N, 1.374384 E). Since June 2012, these data contribute to the international effort to monitor terrestrial ecosystems (grasslands in particular), to the validation of land surface models, and to the near real time quality monitoring of operational weather forecast models. Various variables are monitored at a subhourly rate: wind speed, <span class="hlt">air</span> temperature, <span class="hlt">air</span> humidity, atmospheric pressure, precipitation, turbulent <span class="hlt">fluxes</span> (H, LE, <span class="hlt">CO</span><span class="hlt">2</span>), downwelling and upwelling solar and infrared radiation, downwelling and upwelling PAR, fraction of diffuse incoming PAR, presence of water intercepted by vegetation (rain, dew), soil moisture profile, soil temperature profile, surface albedo, transmissivity of PAR in vegetation canopy. Moreover, local observations are performed using remote sensing techniques: infrared radiometry, GNSS reflectometry, and multi-band surface reflectometry using an aerosol photometer from the AERONET network. Destructive measurements of LAI, green/brown above-ground biomass, and necromass are performed twice a year. This site is characterized by a large fraction of gravels and stones in the soil, ranging from 17% to 35% in the top soil layer (down to 0.6 m), and peaking at 81% at 0.7 m. The impact of gravels and stones on thermal and moisture <span class="hlt">fluxes</span> in the soil has not been much addressed in the past and is not represented in most land surface models. Their impact on the available water content for plant transpiration and plant growth is not much documented so far. The long term monitoring of this site will therefore improve the knowledge on land processes. The data will be used together with urban meteorological data to characterize the urban heat island. Finally, this site will be used for the CAL/VAL of various satellite products in conjunction with the SMOSMANIA soil moisture network</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.C43B0498M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.C43B0498M"><span><span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> monitoring using Continuous Timeseries-Forced Diffusion (CT-FD): Development, Validation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>McArthur, G. S.; Risk, D. A.; Nickerson, N. R.; Creelman, C. A.; Beltrami, H.</p> <p>2009-12-01</p> <p>Land-based <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> measurements are a key indicator of the biological, chemical and physical processes occurring in the soil. While highly dense temporal <span class="hlt">flux</span> measurements can be acquired using Eddy Covariance towers, or <span class="hlt">flux</span> chambers, the challenge of gathering data that is rich both temporally and spatially persists. Over the past two years we have developed a new technique for measuring soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>, called continuous timeseries-forced diffusion (CT-FD) attempts to satisfy the need for spatially and temporally rich data. The CT-FD probe consists of a Vaisala <span class="hlt">CO</span><span class="hlt">2</span> sensor, embodied in a PVC casing, with tear/UV resistant Tyvek membranes at both the inlet and outlet. The probe delivers continuous <span class="hlt">flux</span> data and can be inexpensively replicated across the landscape.The CT-FD technique works by forcing a known diffusive regime between the soil and the atmosphere, allowing the calculation of <span class="hlt">fluxes</span> across the soil/atmosphere boundary to be made from; the internal concentration of a CT-FD probe placed at the soil surface; and a common reference probe designed to capture the atmospheric <span class="hlt">CO</span><span class="hlt">2</span>. For every concentration measurement, the difference between the probe and the reference concentration is indicative of a unique <span class="hlt">flux</span> value. Here we examine properties of the instrument and method, as documented by a long series of developmental studies involving numerical gas transport modeling, laboratory and field experiments. A suite of 1D and 3D modeling experiments were needed to optimize embodiment and geometries of the probe. These show that the probe should have a relatively long collar, with relatively high diffusivity made possible by having large, highly diffusive membranes, both of which help to induce 1D movement of gases into the probe and reduce the lateral diffusion around the probe. Modeling also shows that correction for lateral diffusion is feasible. As for error, sensor error transfers linearly to errors in the <span class="hlt">flux</span>, and that the sensor can be used in non free</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22066218','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22066218"><span>Forest soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> as a function of understory removal and N-fixing species addition.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Li, Haifang; Fu, Shenglei; Zhao, Hongting; Xia, Hanping</p> <p>2011-01-01</p> <p>We report on the effects of forest management practices of understory removal and N-fixing species (Cassia alata) addition on soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in an Eucalyptus urophylla plantation (EUp), Acacia crassicarpa plantation (ACp), 10-species-mixed plantation (Tp), and 30-species-mixed plantation (THp) using the static chamber method in southern China. Four forest management treatments, including (1) understory removal (UR); (<span class="hlt">2</span>) C. alata addition (CA); (3) understory removal and replacement with C. alata (UR+CA); and (4) control without any disturbances (CK), were applied in the above four forest plantations with three replications for each treatment. The results showed that soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> rates remained at a high level during the rainy season (from April to September), followed by a rapid decrease after October reaching a minimum in February. Soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> were significantly higher (P < 0.01) in EUp (132.6 mg/(m<span class="hlt">2</span> x hr)) and ACp (139.8 mg/(m<span class="hlt">2</span> x hr)) than in Tp (94.0 mg/(m<span class="hlt">2</span> x hr)) and THp (102.9 mg/(m<span class="hlt">2</span> x hr)). Soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in UR and CA were significantly higher (P < 0.01) among the four treatments, with values of 105.7, 120.4, 133.6 and 112.<span class="hlt">2</span> mg/(m<span class="hlt">2</span> x hr) for UR+CA, UR, CA and CK, respectively. Soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> were positively correlated with soil temperature (P < 0.01), soil moisture (P < 0.01), NO3(-)-N (P < 0.05), and litterfall (P < 0.01), indicating that all these factors might be important controlling variables for soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. This study sheds some light on our understanding of soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> dynamics in forest plantations under various management practices.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.V21C3048H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.V21C3048H"><span>Controls on the fore-arc <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> along the Central America margin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hilton, D. R.; Barry, P. H.; Ramirez, C. J.; Kulongoski, J. T.; Patel, B. S.; Virrueta, C.; Blackmon, K.</p> <p>2015-12-01</p> <p>The subduction of carbon to the deep mantle via subduction zones is interrupted by outputs via the fore-arc, volcanic front, and back-arc regions. Whereas output <span class="hlt">fluxes</span> for arc and back-arc locales are well constrained for the Central America Volcanic Arc (CAVA) [1-<span class="hlt">2</span>], the fore-arc <span class="hlt">flux</span> via cold seeps and ground waters is poorly known. We present new He and <span class="hlt">CO</span><span class="hlt">2</span> data (isotopes and relative abundances) for the volcanic front and inner fore-arc of western Panama to complement on-going studies of fore-arc C-<span class="hlt">fluxes</span> in Costa Rica [3-4] and to determine tectonic controls on the fore-arc C-outgassing <span class="hlt">fluxes</span>. Helium isotope (3He/4He) values at Baru, La Yeguada, and El Valle volcanoes are high (5-8RA), consistent with results for other Central America volcanoes. However, <span class="hlt">CO</span><span class="hlt">2</span>/3He values are variable (from > 1012 to < 108). Baru has an arc-like δ13C of - 4‰, whereas the other volcanoes have δ13C < -10 ‰. Cold seeps collected in the coastal fore-arc of Panama show a trend of decreasing He-isotopes from west (~6RA) to east (~1RA). This trend is mirrored by δ13C (-5‰ to <-20‰) values. <span class="hlt">CO</span><span class="hlt">2</span>/3He values of the seeps are also variable and fall between 106 and 1012. Using <span class="hlt">CO</span><span class="hlt">2</span>/3He-δ13C mixing plots with conventional endmember values for Limestone, Organic Sediment and Mantle <span class="hlt">CO</span><span class="hlt">2</span>, we show that several Panama samples have been extensively modified by crustal processes. Nevertheless, there are clear west-to east trends (both volcanoes and coastal seeps), whereby L dominates the <span class="hlt">CO</span><span class="hlt">2</span> inventory in the west, similar to Costa Rica, and S-derived <span class="hlt">CO</span><span class="hlt">2</span> increases eastward towards central Panama. Previously [4], we limited the Costa Rica subaerial fore-arc <span class="hlt">flux</span> to ~ 6 × 107 gCkm-1yr-1, or ~ 4% of the total incoming sedimentary C-load. This <span class="hlt">flux</span> diminishes to zero within ~400 km to the east of Baru volcano. The transition from orthogonal subduction of the Cocos Plate to oblique subduction of the Nazca Plate, relative to the common over-riding Caribbean Plate, is the major impediment to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003EAEJA....11433I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003EAEJA....11433I"><span>Short-term effects of rainfall on <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> above rangelands dominated by Artemisia, Bromus tectorum, and Agropyron</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ivans, S.; Saliendra, N. Z.; Johnson, D. A.</p> <p>2003-04-01</p> <p>The short-term effects of rainfall on carbon dioxide (<span class="hlt">CO</span>_<span class="hlt">2</span>) <span class="hlt">fluxes</span> have not been well documented in rangelands of the Intermountain Region of the western USA. We used the Bowen ratio-energy balance technique to continuously measure <span class="hlt">CO</span>_<span class="hlt">2</span> <span class="hlt">fluxes</span> above three rangeland sites in Idaho and Utah dominated by: 1) Artemisia (sagebrush) near Malta, Idaho; <span class="hlt">2</span>) Bromus tectorum (cheatgrass) near Malta, Idaho; and 3) Agropyron (crested wheatgrass) in Rush Valley, Utah. We examined <span class="hlt">CO</span>_<span class="hlt">2</span> <span class="hlt">fluxes</span> immediately before and after rainfall during periods of 10--19 July 2001 (Summer), 8--17 October 2001 (Autumn), and 16--30 May 2002 (Spring). On sunny days before rainfall during Spring, all three sites were sinks for <span class="hlt">CO</span>_<span class="hlt">2</span>. After rainfall in Spring, all three sites became sources of <span class="hlt">CO</span>_<span class="hlt">2</span> for about two days and after that became <span class="hlt">CO</span>_<span class="hlt">2</span> sinks again. During Summer and Autumn when water was limiting, sites were small sources of <span class="hlt">CO</span>_<span class="hlt">2</span> and became larger sources for one day after rainfall. In all three seasons, daytime <span class="hlt">CO</span>_<span class="hlt">2</span> <span class="hlt">fluxes</span> decreased and nighttime <span class="hlt">CO</span>_<span class="hlt">2</span> <span class="hlt">fluxes</span> increased after rainfall, suggesting that rainfall stimulated belowground respiration at all three sites. Results from this study indicated that <span class="hlt">CO</span>_<span class="hlt">2</span> <span class="hlt">fluxes</span> above rangeland sites in the Intermountain West changed markedly after rainfall, especially during Spring when <span class="hlt">fluxes</span> were highest. KEY WORDS: Bowen ratio-energy balance, Intermountain West, rangelands, sagebrush, cheatgrass, crested wheatgrass</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUSM.B11A..01C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUSM.B11A..01C"><span>Proposed Gulf of Mexico Intensive Study on Carbon <span class="hlt">Fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Coble, P. G.; Robbins, L.; Lohrenz, S.; Cai, W.</p> <p>2009-05-01</p> <p>The Gulf of Mexico is an ideal site for the study of land-ocean carbon cycle coupling processes. A recent synthesis suggests that Gulf of Mexico <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> may dominate the net <span class="hlt">flux</span> of the entire North American margin because of the Gulf's large size and strong carbon signals. Northern Gulf waters appear to be a strong local <span class="hlt">CO</span><span class="hlt">2</span> sink due to high primary productivity stimulated by river input of anthropogenic nutrients from the North American continent. Nutrient discharge from the Mississippi River has been implicated in widespread hypoxia on the shelf. The surface drainage system of the Gulf covers more than 60% of the U.S. and more than 40% of Mexico; thus, large-scale changes in land-use and water-management practices in both countries, as well as changes in temperature and rainfall due to climate change, will profoundly affect Gulf carbon <span class="hlt">fluxes</span>. Nevertheless, major sources of uncertainty in the North American carbon budget remain because of largely unsampled areas, undocumented key <span class="hlt">fluxes</span>, such as <span class="hlt">air-sea</span> exchange of carbon dioxide, associated carbon <span class="hlt">fluxes</span>, and poorly characterized control mechanisms. An intensive study in which the Gulf is considered as a whole system, including watersheds, margins, open Gulf of Mexico, overlying atmosphere, and underlying sediments, will be discussed. The study is best addressed using a three-pronged approach that incorporates remote sensing observations, field observations and experiments, and physical and biogeochemical modeling. Societal issues related to carbon management and land-use/land-change must be an integral part of such a study. International cooperation with Mexico, Canada, and Cuba will be essential for the success of this study.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1080410','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1080410"><span>Growth Kinetics, Carbohydrate, and Leaf Phosphate Content of Clover (Trifolium subterraneum L.) after Transfer to a High <span class="hlt">CO</span><span class="hlt">2</span> Atmosphere or to High Light and Ambient <span class="hlt">Air</span> 1</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Morin, Francoise; André, Marcel; Betsche, Thomas</p> <p>1992-01-01</p> <p>Intact <span class="hlt">air</span>-grown (photosynthetic photon <span class="hlt">flux</span> density, 400 microeinsteins per square meter per second) clover plants (Trifolium subterraneum L.) were transfered to high <span class="hlt">CO</span><span class="hlt">2</span> (4000 microliters <span class="hlt">CO</span><span class="hlt">2</span> per liter; photosynthetic photon <span class="hlt">flux</span> density, 400 microeinsteins per square meter per second) or to high light (340 microliters <span class="hlt">CO</span><span class="hlt">2</span> per liter; photosynthetic photon <span class="hlt">flux</span> density, 800 microeinsteins per square meter per second) to similarly stimulate photosynthetic net <span class="hlt">CO</span><span class="hlt">2</span> uptake. The daily increment of net <span class="hlt">CO</span><span class="hlt">2</span> uptake declined transiently in high <span class="hlt">CO</span><span class="hlt">2</span>, but not in high light, below the values in <span class="hlt">air</span>/standard light. After about 3 days in high <span class="hlt">CO</span><span class="hlt">2</span>, the daily increment of net <span class="hlt">CO</span><span class="hlt">2</span> uptake increased but did not reach the high light values. Nightly <span class="hlt">CO</span><span class="hlt">2</span> release increased immediately in high light, whereas there was a 3-day lag phase in high <span class="hlt">CO</span><span class="hlt">2</span>. During this time, starch accumulated to a high level, and leaf deterioration was observed only in high <span class="hlt">CO</span><span class="hlt">2</span>. After 12 days, starch was two- to threefold higher in high <span class="hlt">CO</span><span class="hlt">2</span> than in high light, whereas sucrose was similar. Leaf carbohydrates were determined during the first and fourth day in high <span class="hlt">CO</span><span class="hlt">2</span>. Starch increased rapidly throughout the day. Early in the day, sucrose was low and similar in high <span class="hlt">CO</span><span class="hlt">2</span> and ambient <span class="hlt">air</span> (same light). Later, sucrose increased considerably in high <span class="hlt">CO</span><span class="hlt">2</span>. The findings that (a) much more photosynthetic carbon was partitioned into the leaf starch pool in high <span class="hlt">CO</span><span class="hlt">2</span> than in high light, although net <span class="hlt">CO</span><span class="hlt">2</span> uptake was similar, and that (b) rapid starch formation occurred in high <span class="hlt">CO</span><span class="hlt">2</span> even when leaf sucrose was only slightly elevated suggest that low sink capacity was not the main constraint in high <span class="hlt">CO</span><span class="hlt">2</span>. It is proposed that carbon partitioning between starch (chloroplast) and sucrose (cytosol) was perturbed by high <span class="hlt">CO</span><span class="hlt">2</span> because of the lack of photorespiration. Total phosphate pools were determined in leaves. Concentrations based on fresh weight of orthophosphate, soluble esterified phosphate, and total phosphate markedly declined</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.9924L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.9924L"><span>Soil methane and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in rainforest and rubber plantations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lang, Rong; Blagodatsky, Sergey; Goldberg, Stefanie; Xu, Jianchu</p> <p>2017-04-01</p> <p>Expansion of rubber plantations in South-East Asia has been a land use transformation trend leading to losses of natural forest cover in the region. Besides impact on ecosystem carbon stocks, this conversion influences the dynamics of greenhouse gas <span class="hlt">fluxes</span> from soil driven by microbial activity, which has been insufficiently studied. Aimed to understand how land use change affects the soil <span class="hlt">CO</span><span class="hlt">2</span> and CH4 <span class="hlt">fluxes</span>, we measured surface gas <span class="hlt">fluxes</span>, gas concentration gradient, and 13C signature in CH4 and soil organic matter in profiles in a transect in Xishuangbanna, including a rainforest site and three rubber plantation sites with age gradient. Gas <span class="hlt">fluxes</span> were measured by static chamber method and open chamber respiration system. Soil gases were sampled from installed gas samplers at 5, 10, 30, and 75cm depth at representative time in dry and rainy season. The soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> was comparable in rainforest and old rubber plantations, while young rubber plantation had the lowest rate. Total carbon content in the surface soil well explained the difference of soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> between sites. All sites were CH4 sinks in dry season and uptake decreased in the order of rainforest, old rubber plantations and young rubber plantation. From dry season to rainy season, CH4 consumption decreased with increasing CH4 concentration in the soil profile at all depths. The enrichment of methane by 13CH4 shifted towards to lowerδ13C, being the evidence of enhanced CH4 production process while net surface methane <span class="hlt">flux</span> reflected the consumption in wet condition. Increment of CH4 concentration in the profile from dry to rainy season was higher in old rubber plantation compared to rainforest, while the shifting of δ13CH4 was larger in rainforest than rubber sites. Turnover rates of soil <span class="hlt">CO</span><span class="hlt">2</span> and CH4 suggested that the 0-5 cm surface soil was the most active layer for gaseous carbon exchange. δ13C in soil organic matter and soil moisture increased from rainforest, young rubber plantation to old</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A33G2447M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A33G2447M"><span>High-resolution <span class="hlt">CO</span><span class="hlt">2</span> and CH4 <span class="hlt">flux</span> inverse modeling combining GOSAT, OCO-<span class="hlt">2</span> and ground-based observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Maksyutov, S. S.; Oda, T.; Saito, M.; Ito, A.; Janardanan Achari, R.; Sasakawa, M.; Machida, T.; Kaiser, J. W.; Belikov, D.; Valsala, V.; O'Dell, C.; Yoshida, Y.; Matsunaga, T.</p> <p>2017-12-01</p> <p>We develop a high-resolution <span class="hlt">CO</span><span class="hlt">2</span> and CH4 <span class="hlt">flux</span> inversion system that is based on the Lagrangian-Eulerian coupled tracer transport model, and is designed to estimate surface <span class="hlt">fluxes</span> from atmospheric <span class="hlt">CO</span><span class="hlt">2</span> and CH4 data observed by the GOSAT and OCO-<span class="hlt">2</span> satellites and by global in-situ networks, including observation in Siberia. We use the Lagrangian particle dispersion model (LPDM) FLEXPART to estimate the surface <span class="hlt">flux</span> footprints for each observation at 0.1-degree spatial resolution for three days of transport. The LPDM is coupled to a global atmospheric tracer transport model (NIES-TM). The adjoint of the coupled transport model is used in an iterative optimization procedure based on either quasi-Newtonian algorithm or singular value decomposition. Combining surface and satellite data for use in inversion requires correcting for biases present in satellite observation data, that is done in a two-step procedure. As a first step, bi-weekly corrections to prior <span class="hlt">flux</span> fields are estimated for the period of 2009 to 2015 from in-situ <span class="hlt">CO</span><span class="hlt">2</span> and CH4 data from global observation network, included in Obspack-GVP (for <span class="hlt">CO</span><span class="hlt">2</span>), WDCGG (CH4) and JR-STATION datasets. High-resolution prior <span class="hlt">fluxes</span> were prepared for anthropogenic emissions (ODIAC and EDGAR), biomass burning (GFAS), and the terrestrial biosphere. The terrestrial biosphere <span class="hlt">flux</span> was constructed using a vegetation mosaic map and separate simulations of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> by the VISIT model for each vegetation type present in a grid. The prior <span class="hlt">flux</span> uncertainty for land is scaled proportionally to monthly mean GPP by the MODIS product for <span class="hlt">CO</span><span class="hlt">2</span> and EDGAR emissions for CH4. Use of the high-resolution transport leads to improved representation of the anthropogenic plumes, often observed at continental continuous observation sites. OCO-<span class="hlt">2</span> observations are aggregated to 1 second averages, to match the 0.1 degree resolution of the transport model. Before including satellite observations in the inversion, the monthly varying latitude-dependent bias is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/39384','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/39384"><span>Do plant species influence soil <span class="hlt">CO</span><span class="hlt">2</span> and N<span class="hlt">2</span>O <span class="hlt">fluxes</span> in a diverse tropical forest?</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>J.L.M. van Haren; R.C. de Oliveira; N. Restrepo-Coupe; L. Hutyra; P. B. de Camargo; Michael Keller; S.R. Saleska</p> <p>2010-01-01</p> <p>[1] To test whether plant species influence greenhouse gas production in diverse ecosystems, we measured wet season soil <span class="hlt">CO</span><span class="hlt">2</span> and N<span class="hlt">2</span>O <span class="hlt">fluxes</span> close to 300 large (>35 cm in diameter at breast height (DBH)) trees of 15 species at three clay‐rich forest sites in central Amazonia. We found that soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> were 38% higher near large trees than at control sites >10...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018Ocgy...58..240P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018Ocgy...58..240P"><span>Sediment <span class="hlt">Flux</span> of Particulate Organic Phosphorus in the Open Black <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Parkhomenko, A. V.; Kukushkin, A. S.</p> <p>2018-03-01</p> <p>The interannual variation of the monthly average (weighted average) concentrations of particulate organic phosphorus (PPOM) in the photosynthetic layer, oxycline, redox zone, and H<span class="hlt">2</span>S zone in the open Black <span class="hlt">Sea</span> is estimated based on long-term observation data. The suspension sedimentation rates from the studied layers are assessed using model calculations and published data. The annual variation of PPOM sediment <span class="hlt">fluxes</span> from the photosynthetic layer, oxycline, redox zone, and upper H<span class="hlt">2</span>S zone to the anaerobic zone of the <span class="hlt">sea</span> and the correspondingly annual average values are estimated for the first time. A regular decrease in the PPOM annual average <span class="hlt">flux</span> with depth in the upper active layer is demonstrated. A correlation between the annual average values of PPOM sediment <span class="hlt">flux</span> from the photosynthetic layer and ascending phosphate <span class="hlt">flux</span> to this layer is shown, which suggests their balance in the open <span class="hlt">sea</span>. The results are discussed in terms of the phosphorus biogeochemical cycle and the concept of new and regenerative primary production in the open Black <span class="hlt">Sea</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.B51D0457D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.B51D0457D"><span>Comparing Amazon Basin <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> from an atmospheric inversion with TRENDY biosphere models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Diffenbaugh, N. S.; Alden, C. B.; Harper, A. B.; Ahlström, A.; Touma, D. E.; Miller, J. B.; Gatti, L. V.; Gloor, M.</p> <p>2015-12-01</p> <p>Net exchange of carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) between the atmosphere and the terrestrial biosphere is sensitive to environmental conditions, including extreme heat and drought. Of particular importance for local and global carbon balance and climate are the expansive tracts of tropical rainforest located in the Amazon Basin. Because of the Basin's size and ecological heterogeneity, net biosphere <span class="hlt">CO</span><span class="hlt">2</span> exchange with the atmosphere remains largely un-constrained. In particular, the response of net <span class="hlt">CO</span><span class="hlt">2</span> exchange to changes in environmental conditions such as temperature and precipitation are not yet well known. However, proper representation of these relationships in biosphere models is a necessary constraint for accurately modeling future climate and climate-carbon cycle feedbacks. In an effort to compare biosphere response to climate across different biosphere models, the TRENDY model intercomparison project coordinated the simulation of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> between the biosphere and atmosphere, in response to historical climate forcing, by 9 different Dynamic Global Vegetation Models. We examine the TRENDY model results in the Amazon Basin, and compare this "bottom-up" method with <span class="hlt">fluxes</span> derived from a "top-down" approach to estimating net <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>, obtained through atmospheric inverse modeling using <span class="hlt">CO</span><span class="hlt">2</span> measurements sampled by aircraft above the basin. We compare the "bottom-up" and "top-down" <span class="hlt">fluxes</span> in 5 sub-regions of the Amazon basin on a monthly basis for 2010-2012. Our results show important periods of agreement between some models in the TRENDY suite and atmospheric inverse model results, notably the simulation of increased biosphere <span class="hlt">CO</span><span class="hlt">2</span> loss during wet season heat in the Central Amazon. During the dry season, however, model ability to simulate observed response of net <span class="hlt">CO</span><span class="hlt">2</span> exchange to drought was varied, with few models able to reproduce the "top-down" inversion <span class="hlt">flux</span> signals. Our results highlight the value of atmospheric trace gas observations for helping to narrow the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23873747','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23873747"><span>Environmental controls of temporal and spatial variability in <span class="hlt">CO</span><span class="hlt">2</span> and CH4 <span class="hlt">fluxes</span> in a neotropical peatland.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wright, Emma L; Black, Colin R; Turner, Benjamin L; Sjögersten, Sofie</p> <p>2013-12-01</p> <p>Tropical peatlands play an important role in the global storage and cycling of carbon (C) but information on carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) and methane (CH4) <span class="hlt">fluxes</span> from these systems is sparse, particularly in the Neotropics. We quantified short and long-term temporal and small scale spatial variation in <span class="hlt">CO</span><span class="hlt">2</span> and CH4 <span class="hlt">fluxes</span> from three contrasting vegetation communities in a domed ombrotrophic peatland in Panama. There was significant variation in <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> among vegetation communities in the order Campnosperma panamensis > Raphia taedigera > Cyperus. There was no consistent variation among sites and no discernible seasonal pattern of CH4 <span class="hlt">flux</span> despite the considerable range of values recorded (e.g. -1.0 to 12.6 mg m(-<span class="hlt">2</span>) h(-1) in 2007). <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> varied seasonally in 2007, being greatest in drier periods (300-400 mg m(-<span class="hlt">2</span>) h(-1)) and lowest during the wet period (60-132 mg m(-<span class="hlt">2</span>) h(-1)) while very high emissions were found during the 2009 wet period, suggesting that peak <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> may occur following both low and high rainfall. In contrast, only weak relationships between CH4 <span class="hlt">flux</span> and rainfall (positive at the C. panamensis site) and solar radiation (negative at the C. panamensis and Cyperus sites) was found. <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> showed a diurnal pattern across sites and at the Cyperus sp. site <span class="hlt">CO</span><span class="hlt">2</span> and CH4 <span class="hlt">fluxes</span> were positively correlated. The amount of dissolved carbon and nutrients were strong predictors of small scale within-site variability in gas release but the effect was site-specific. We conclude that (i) temporal variability in <span class="hlt">CO</span><span class="hlt">2</span> was greater than variation among vegetation communities; (ii) rainfall may be a good predictor of <span class="hlt">CO</span><span class="hlt">2</span> emissions from tropical peatlands but temporal variation in CH4 does not follow seasonal rainfall patterns; and (iii) diurnal variation in <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> across different vegetation communities can be described by a Fourier model. © 2013 John Wiley & Sons Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.B51A0302O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.B51A0302O"><span>Soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Fluxes</span> Following Wetting Events: Field Observations and Modeling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>O'Donnell, F. C.; Caylor, K. K.</p> <p>2009-12-01</p> <p>Carbon exchange data from eddy <span class="hlt">flux</span> towers in drylands suggest that the Birch Effect, a pulse of soil <span class="hlt">CO</span><span class="hlt">2</span> efflux triggered by the first rain following a dry period, may contribute significantly to the annual carbon budget of these ecosystems. Laboratory experiments on dryland soils have shown that microbes adapted to live in arid ecosystems may be able to remain dormant in dry soil for much longer than expected and an osmotic shock response to sudden increases in soil water potential may play a role in the Birch Effect. However, little has been done to understand how a dry soil profile responds to a rainfall event. We measured soil <span class="hlt">CO</span><span class="hlt">2</span> production during experimental wetting events in treatment plots at a site on the Botswana portion of the Kalahari Transect (KT). We buried small, solid-state sensors that continuously measure <span class="hlt">CO</span><span class="hlt">2</span> concentration in the soil <span class="hlt">air</span> space at four depths and the soil surface and applied wetting treatments intended to simulate typical rainfall for the region to the plots, including single 10 mm wettings (the mean storm depth for the KT), single 20 mm wettings, and repeated 10 mm wettings. We solved a finite difference approximation of the governing equation for <span class="hlt">CO</span><span class="hlt">2</span> in the soil airspace to determine the source rate of <span class="hlt">CO</span><span class="hlt">2</span> during and after the wetting treatments, using Richard’s equation to approximate the change in <span class="hlt">air</span>-filled porosity due to infiltrating water. The wetting treatments induced a rapid spike in the source rate of <span class="hlt">CO</span><span class="hlt">2</span> in the soil, the timing and magnitude of which were consistent with laboratory experiments that observed a microbial osmotic shock response. The source rate averaged over the first three hours after wetting showed that a 20 mm wetting produced a larger response than the 10 mm wettings. It also showed that a second wetting event produced a smaller response than the first and though it was not significant, an upward trend in response was apparent through the two month period. These results suggest that there may be</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001AGUSM...B41A03D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001AGUSM...B41A03D"><span>Multiple <span class="hlt">Flux</span> Footprints, <span class="hlt">Flux</span> Divergences and Boundary Layer Mixing Ratios: Studies of Ecosystem-Atmosphere <span class="hlt">CO</span><span class="hlt">2</span> Exchange Using the WLEF Tall Tower.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Davis, K. J.; Bakwin, P. S.; Yi, C.; Cook, B. D.; Wang, W.; Denning, A. S.; Teclaw, R.; Isebrands, J. G.</p> <p>2001-05-01</p> <p>Long-term, tower-based measurements using the eddy-covariance method have revealed a wealth of detail about the temporal dynamics of netecosystem-atmosphere exchange (NEE) of <span class="hlt">CO</span><span class="hlt">2</span>. The data also provide a measure of the annual net <span class="hlt">CO</span><span class="hlt">2</span> exchange. The area represented by these <span class="hlt">flux</span> measurements, however, is limited, and doubts remain about possible systematic errors that may bias the annual net exchange measurements. <span class="hlt">Flux</span> and mixing ratio measurements conducted at the WLEF tall tower as part of the Chequamegon Ecosystem-Atmosphere Study (ChEAS) allow for unique assessment of the uncertainties in NEE of <span class="hlt">CO</span><span class="hlt">2</span>. The synergy between <span class="hlt">flux</span> and mixing ratio observations shows the potential for comparing inverse and eddy-covariance methods of estimating NEE of <span class="hlt">CO</span><span class="hlt">2</span>. Such comparisons may strengthen confidence in both results and begin to bridge the huge gap in spatial scales (at least 3 orders of magnitude) between continental or hemispheric scale inverse studies and kilometer-scale eddy covariance <span class="hlt">flux</span> measurements. Data from WLEF and Willow Creek, another ChEAS tower, are used to estimate random and systematic errors in NEE of <span class="hlt">CO</span><span class="hlt">2</span>. Random uncertainty in seasonal exchange rates and the annual integrated NEE, including both turbulent sampling errors and variability in enviromental conditions, is small. Systematic errors are identified by examining changes in <span class="hlt">flux</span> as a function of atmospheric stability and wind direction, and by comparing the multiple level <span class="hlt">flux</span> measurements on the WLEF tower. Nighttime drainage is modest but evident. Systematic horizontal advection occurs during the morning turbulence transition. The potential total systematic error appears to be larger than random uncertainty, but still modest. The total systematic error, however, is difficult to assess. It appears that the WLEF region ecosystems were a small net sink of <span class="hlt">CO</span><span class="hlt">2</span> in 1997. It is clear that the summer uptake rate at WLEF is much smaller than that at most deciduous forest sites, including the nearby</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_18 --> <div id="page_19" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="361"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A14C..03J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A14C..03J"><span><span class="hlt">Air-Sea</span> Interaction in the Somali Current Region</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jensen, T. G.; Rydbeck, A.</p> <p>2017-12-01</p> <p>The western Indian Ocean is an area of high eddy-kinetic energy generated by local wind-stress curl, instability of boundary currents as well as Rossby waves from the west coast of India and the equatorial wave guide as they reflect off the African coast. The presence of meso-scale eddies and coastal upwelling during the Southwest Monsoon affects the <span class="hlt">air-sea</span> interaction on those scales. The U.S. Navy's Coupled Ocean-Atmosphere Mesoscale Prediction System (COAMPS) is used to understand and quantify the surface <span class="hlt">flux</span>, effects on surface waves and the role of <span class="hlt">Sea</span> Surface Temperature anomalies on ocean-atmosphere coupling in that area. The COAMPS atmosphere model component with 9 km resolution is fully coupled to the Navy Coastal Ocean Model (NCOM) with 3.5 km resolution and the Simulating WAves Nearshore (SWAN) wave model with 10 km resolution. Data assimilation using a 3D-variational approach is included in hindcast runs performed daily since June 1, 2015. An interesting result is that a westward jet associated with downwelling equatorial Rossy waves initiated the reversal from the southward Somali Current found during the northeast monsoon to a northward flow in March 2016 more than a month before the beginning of the southwest monsoon. It is also found that warm SST anomalies in the Somali Current eddies, locally increase surface wind speed due to an increase in the atmospheric boundary layer height. This results in an increase in significant wave height and also an increase in heat <span class="hlt">flux</span> to the atmosphere. Cold SST anomalies over upwelling filaments have the opposite impacts on <span class="hlt">air-sea</span> <span class="hlt">fluxes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018CSR...156....1G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018CSR...156....1G"><span>Spatial and temporal variability of seawater p<span class="hlt">CO</span><span class="hlt">2</span> within the Canadian Arctic Archipelago and Baffin Bay during the summer and autumn 2011</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Geilfus, N.-X.; Pind, M. L.; Else, B. G. T.; Galley, R. J.; Miller, L. A.; Thomas, H.; Gosselin, M.; Rysgaard, S.; Wang, F.; Papakyriakou, T. N.</p> <p>2018-03-01</p> <p>The partial pressure of <span class="hlt">CO</span><span class="hlt">2</span> in surface water (p<span class="hlt">CO</span><span class="hlt">2</span>sw) measured within the Canadian Arctic Archipelago (CAA) and Baffin Bay was highly variable with values ranging from strongly undersaturated (118 μatm) to slightly supersaturated (419 μatm) with respect to the atmospheric levels ( 386 μatm) during summer and autumn 2011. During summer, melting <span class="hlt">sea</span> ice contributed to cold and fresh surface water and enhanced the ice-edge bloom, resulting in strong p<span class="hlt">CO</span><span class="hlt">2</span>sw undersaturation. Coronation Gulf was the only area with supersaturated p<span class="hlt">CO</span><span class="hlt">2</span>sw, likely due to warm <span class="hlt">CO</span><span class="hlt">2</span>-enriched freshwater input from the Coppermine River. During autumn, the entire CAA (including Coronation Gulf) was undersaturated, despite generally increasing p<span class="hlt">CO</span><span class="hlt">2</span>sw. Coronation Gulf was the one place where p<span class="hlt">CO</span><span class="hlt">2</span>sw decreased, likely due to seasonal reduction in discharge from the Coppermine River and the decreasing <span class="hlt">sea</span> surface temperature. The seasonal summer-to-autumn increase in p<span class="hlt">CO</span><span class="hlt">2</span>sw across the archipelago is attributed in part to the continuous uptake of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> through both summer and autumn and to the seasonal deepening of the surface mixed layer, bringing <span class="hlt">CO</span><span class="hlt">2</span>-rich waters to the surface. These observations demonstrate how freshwater from <span class="hlt">sea</span> ice melt and rivers affect p<span class="hlt">CO</span><span class="hlt">2</span>sw differently. The general p<span class="hlt">CO</span><span class="hlt">2</span>sw undersaturation during summer-autumn 2011 throughout the CAA and Baffin Bay give an estimated net oceanic sink for atmospheric <span class="hlt">CO</span><span class="hlt">2</span> over the study period of 11.4 mmol <span class="hlt">CO</span><span class="hlt">2</span> m-<span class="hlt">2</span> d-1, assuming no <span class="hlt">sea-air</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> exchange across the <span class="hlt">sea</span>-ice covered areas.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A43C2464G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A43C2464G"><span>The use of fair-weather cases from the ACT-America Summer 2016 field campaign to better constrain regional biogenic <span class="hlt">CO</span><span class="hlt">2</span> surface <span class="hlt">fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gaudet, B. J.; Davis, K. J.; DiGangi, J. P.; Feng, S.; Hoffman, K.; Jacobson, A. R.; Lauvaux, T.; McGill, M. J.; Miles, N.; Pal, S.; Pauly, R.; Richardson, S.</p> <p>2017-12-01</p> <p>The Atmospheric Carbon and Transport - America (ACT-America) study is a multi-year NASA-funded project designed to increase our understanding of regional-scale greenhouse gas (GHG) <span class="hlt">fluxes</span> over North America through aircraft, satellite, and tower-based observations. This is being accomplished through a series of field campaigns that cover three focus regions (Mid-Atlantic, Gulf Coast, and Midwest), and all four seasons (summer, winter, fall, and spring), as well as a variety of meteorological conditions. While constraints on GHG <span class="hlt">fluxes</span> can be derived on the global scale (through remote-site concentration measurements and global <span class="hlt">flux</span> inversion models) and the local scale (through eddy-covariance <span class="hlt">flux</span> tower measurements), observational constraints on the intermediate scales are not as readily available. Biogenic <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> are particularly challenging because of their strong seasonal and diurnal cycles and large spatial variability. During the summer 2016 ACT field campaign, fair weather days were targeted for special flight patterns designed to estimate surface <span class="hlt">fluxes</span> at scales on the order of 105 km<span class="hlt">2</span> using a modified mass-balance approach. For some onshore flow cases in the Gulf Coast, atmospheric boundary layer (ABL) flight transects were performed both inland and offshore when it could be reasonably inferred that the homogeneous Gulf <span class="hlt">air</span> provided the background GHG field for the inland transect. On other days, two-day flight sequences were performed, where the second-day location of the flight patterns was designed to encompass the <span class="hlt">air</span> mass that was sampled on the first day. With these flight patterns, the average regional <span class="hlt">flux</span> can be estimated from the ABL <span class="hlt">CO</span><span class="hlt">2</span> concentration change. Direct measurements of ABL depth from both aircraft profiles and high-resolution airborne lidar will be used, while winds and free-tropospheric <span class="hlt">CO</span><span class="hlt">2</span> can be determined from model output and in situ aircraft observations. Here we will present examples of this <span class="hlt">flux</span> estimation for both Gulf</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/18044541','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/18044541"><span>Energy and material balance of <span class="hlt">CO</span><span class="hlt">2</span> capture from ambient <span class="hlt">air</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zeman, Frank</p> <p>2007-11-01</p> <p>Current Carbon Capture and Storage (CCS) technologies focus on large, stationary sources that produce approximately 50% of global <span class="hlt">CO</span><span class="hlt">2</span> emissions. We propose an industrial technology that captures <span class="hlt">CO</span><span class="hlt">2</span> directly from ambient <span class="hlt">air</span> to target the remaining emissions. First, a wet scrubbing technique absorbs <span class="hlt">CO</span><span class="hlt">2</span> into a sodium hydroxide solution. The resultant carbonate is transferred from sodium ions to calcium ions via causticization. The captured <span class="hlt">CO</span><span class="hlt">2</span> is released from the calcium carbonate through thermal calcination in a modified kiln. The energy consumption is calculated as 350 kJ/mol of <span class="hlt">CO</span><span class="hlt">2</span> captured. It is dominated by the thermal energy demand of the kiln and the mechanical power required for <span class="hlt">air</span> movement. The low concentration of <span class="hlt">CO</span><span class="hlt">2</span> in <span class="hlt">air</span> requires a throughput of 3 million cubic meters of <span class="hlt">air</span> per ton of <span class="hlt">CO</span><span class="hlt">2</span> removed, which could result in significant water losses. Electricity consumption in the process results in <span class="hlt">CO</span><span class="hlt">2</span> emissions and the use of coal power would significantly reduce to net amount captured. The thermodynamic efficiency of this process is low but comparable to other "end of pipe" capture technologies. As another carbon mitigation technology, <span class="hlt">air</span> capture could allow for the continued use of liquid hydrocarbon fuels in the transportation sector.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19215133','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19215133"><span>Kinetics of <span class="hlt">CO</span>(<span class="hlt">2</span>) <span class="hlt">fluxes</span> outgassing from champagne glasses in tasting conditions: the role of temperature.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Liger-Belair, Gérard; Villaume, Sandra; Cilindre, Clara; Jeandet, Philippe</p> <p>2009-03-11</p> <p>Measurements of <span class="hlt">CO</span>(<span class="hlt">2</span>) <span class="hlt">fluxes</span> outgassing from a flute poured with a standard Champagne wine initially holding about 11 g L(-1) of dissolved <span class="hlt">CO</span>(<span class="hlt">2</span>) were presented, in tasting conditions, all along the first 10 min following the pouring process. Experiments were performed at three sets of temperature, namely, 4 degrees C, 12 degrees C, and 20 degrees C, respectively. It was demonstrated that the lower the champagne temperature, the lower <span class="hlt">CO</span>(<span class="hlt">2</span>) volume <span class="hlt">fluxes</span> outgassing from the flute. Therefore, the lower the champagne temperature, the lower its progressive loss of dissolved <span class="hlt">CO</span>(<span class="hlt">2</span>) concentration with time, which constitutes the first analytical proof that low champagne temperatures prolong the drink's chill and helps retains its effervescence. A correlation was also proposed between <span class="hlt">CO</span>(<span class="hlt">2</span>) volume <span class="hlt">fluxes</span> outgassing from the flute poured with champagne and its continuously decreasing dissolved <span class="hlt">CO</span>(<span class="hlt">2</span>) concentration. Finally, the contribution of effervescence to the global kinetics of <span class="hlt">CO</span>(<span class="hlt">2</span>) release was discussed and modeled by the use of results developed over recent years. The temperature dependence of the champagne viscosity was found to play a major role in the kinetics of <span class="hlt">CO</span>(<span class="hlt">2</span>) outgassing from a flute. On the basis of this bubbling model, the theoretical influence of champagne temperature on <span class="hlt">CO</span>(<span class="hlt">2</span>) volume <span class="hlt">fluxes</span> outgassing from a flute was discussed and found to be in quite good accordance with our experimental results.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFMGC51G..04D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMGC51G..04D"><span>Retrieval of Paris <span class="hlt">CO</span><span class="hlt">2</span> and <span class="hlt">CO</span> emissions using a boundary layer budget method in the framework of the <span class="hlt">CO</span><span class="hlt">2</span>-MEGAPARIS project</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dieudonné, E.; Gibert, F.; Xueref-remy, I. C.; Lopez, M.; Schmidt, M.; Ravetta, F.</p> <p>2012-12-01</p> <p>. These anthropogenic <span class="hlt">fluxes</span> are compared to the CITEPA and IER emission inventories using the <span class="hlt">air</span> mass footprint from a Lagrangian Particle Dispersion Model in backward mode. Results from a case study in March 2012 are presented to assess the propagation of Paris <span class="hlt">CO</span><span class="hlt">2</span> and <span class="hlt">CO</span> plume, the precision of the method and its ability to provide an independent verification of urban emission inventories. References: [a] Xueref-Remy et al., Abstract n°A13F-0277, AGU Fall Meeting 2010, San Francisco, USA [b] http://<span class="hlt">co</span><span class="hlt">2</span>-megaparis.lsce.ipsl.fr/ [c] Gibert et al., J. Geophys. Research, 112, D10301 (2007) [d] http://www.icos-infrastructure.eu/</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018APJAS..54....1K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018APJAS..54....1K"><span>Effect of Data Assimilation Parameters on The Optimized Surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Flux</span> in Asia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kim, Hyunjung; Kim, Hyun Mee; Kim, Jinwoong; Cho, Chun-Ho</p> <p>2018-02-01</p> <p>In this study, CarbonTracker, an inverse modeling system based on the ensemble Kalman filter, was used to evaluate the effects of data assimilation parameters (assimilation window length and ensemble size) on the estimation of surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in Asia. Several experiments with different parameters were conducted, and the results were verified using <span class="hlt">CO</span><span class="hlt">2</span> concentration observations. The assimilation window lengths tested were 3, 5, 7, and 10 weeks, and the ensemble sizes were 100, 150, and 300. Therefore, a total of 12 experiments using combinations of these parameters were conducted. The experimental period was from January 2006 to December 2009. Differences between the optimized surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> of the experiments were largest in the Eurasian Boreal (EB) area, followed by Eurasian Temperate (ET) and Tropical Asia (TA), and were larger in boreal summer than in boreal winter. The effect of ensemble size on the optimized biosphere <span class="hlt">flux</span> is larger than the effect of the assimilation window length in Asia, but the importance of them varies in specific regions in Asia. The optimized biosphere <span class="hlt">flux</span> was more sensitive to the assimilation window length in EB, whereas it was sensitive to the ensemble size as well as the assimilation window length in ET. The larger the ensemble size and the shorter the assimilation window length, the larger the uncertainty (i.e., spread of ensemble) of optimized surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. The 10-week assimilation window and 300 ensemble size were the optimal configuration for CarbonTracker in the Asian region based on several verifications using <span class="hlt">CO</span><span class="hlt">2</span> concentration measurements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMOS31B1395R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMOS31B1395R"><span>Monthly <span class="hlt">Sea</span> Surface Salinity and Freshwater <span class="hlt">Flux</span> Monitoring</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ren, L.; Xie, P.; Wu, S.</p> <p>2017-12-01</p> <p>Taking advantages of the complementary nature of the <span class="hlt">Sea</span> Surface Salinity (SSS) measurements from the in-situ (CTDs, shipboard, Argo floats, etc.) and satellite retrievals from Soil Moisture Ocean Salinity (SMOS) satellite of the European Space Agency (ESA), the Aquarius of a joint venture between US and Argentina, and the Soil Moisture Active Passive (SMAP) of national Aeronautics and Space Administration (NASA), a technique is developed at NOAA/NCEP/CPC to construct an analysis of monthly SSS, called the NOAA Blended Analysis of <span class="hlt">Sea</span>-Surface Salinity (BASS). The algorithm is a two-steps approach, i.e. to remove the bias in the satellite data through Probability Density Function (PDF) matching against <span class="hlt">co</span>-located in situ measurements; and then to combine the bias-corrected satellite data with the in situ measurements through the Optimal Interpolation (OI) method. The BASS SSS product is on a 1° by 1° grid over the global ocean for a 7-year period from 2010. Combined with the NOAA/NCEP/CPC CMORPH satellite precipitation (P) estimates and the Climate Forecast System Reanalysis (CFSR) evaporation (E) fields, a suite of monthly package of the SSS and oceanic freshwater <span class="hlt">flux</span> (E and P) was developed to monitor the global oceanic water cycle and SSS on a monthly basis. The SSS in BASS product is a suite of long-term SSS and fresh water <span class="hlt">flux</span> data sets with temporal homogeneity and inter-component consistency better suited for the examination of the long-term changes and monitoring. It presents complete spatial coverage and improved resolution and accuracy, which facilitates the diagnostic analysis of the relationship and <span class="hlt">co</span>-variability among SSS, freshwater <span class="hlt">flux</span>, mixed layer processes, oceanic circulation, and assimilation of SSS into global models. At the AGU meeting, we will provide more details on the CPC salinity and fresh water <span class="hlt">flux</span> data package and its applications in the monitoring and analysis of SSS variations in association with the ENSO and other major climate</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19820011907','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19820011907"><span>Estimating ocean-<span class="hlt">air</span> heat <span class="hlt">fluxes</span> during cold <span class="hlt">air</span> outbreaks by satellite</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chou, S. H.; Atlas, D.</p> <p>1981-01-01</p> <p>Nomograms of mean column heating due to surface sensible and latent heat <span class="hlt">fluxes</span> were developed. Mean sensible heating of the cloud free region is related to the cloud free path (CFP, the distance from the shore to the first cloud formation) and the difference between land <span class="hlt">air</span> and <span class="hlt">sea</span> surface temperatures, theta sub 1 and theta sub 0, respectively. Mean latent heating is related to the CFP and the difference between land <span class="hlt">air</span> and <span class="hlt">sea</span> surface humidities q sub 1 and q sub 0 respectively. Results are also applicable to any path within the cloud free region. Corresponding heat <span class="hlt">fluxes</span> may be obtained by multiplying the mean heating by the mean wind speed in the boundary layer. The sensible heating estimated by the present method is found to be in good agreement with that computed from the bulk transfer formula. The sensitivity of the solutions to the variations in the initial coastal soundings and large scale subsidence is also investigated. The results are not sensitive to divergence but are affected by the initial lapse rate of potential temperature; the greater the stability, the smaller the heating, other things being equal. Unless one knows the lapse rate at the shore, this requires another independent measurement. For this purpose the downwind slope of the square of the boundary layer height is used, the mean value of which is also directly proportional to the mean sensible heating. The height of the boundary layer should be measurable by future spaceborn lidar systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..12.3916I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..12.3916I"><span>Regional variability of grassland <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in Tyrol/Austria</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Irschick, Christoph; Hammerle, Albin; Haslwanter, Alois; Wohlfahrt, Georg</p> <p>2010-05-01</p> <p>The FLUXNET project [1] aims at quantifying the magnitude and controls on the <span class="hlt">CO</span><span class="hlt">2</span>, H<span class="hlt">2</span>O and energy exchange of terrestrial ecosystems. Ideally, the various biomes of the Earth would be sampled in proportion to their spatial extent - in reality, however, study site selection is usually based on other (more practical) criteria so that a bias exists towards certain biomes and ecosystem types. This may be problematic because FLUXNET data are used to calibrate/parameterize models at various scales - if certain ecosystems are poorly replicated this may bias model predictions. Here we present data from a project in Tyrol/Austria where we have been investigating the <span class="hlt">CO</span><span class="hlt">2</span>, H<span class="hlt">2</span>O and energy exchange of five grassland sites during 2005-2007. The five permanent grassland sites were exposed to similar climate, but differed slightly in management. In a FLUXNET style approach, any of these sites might have been selected for making long-term <span class="hlt">flux</span> measurements - the aim of this project was to examine the representativeness of these sites and, if evident, elucidate the causes for and controls on differences between sites. To this end we conducted continuous eddy covariance <span class="hlt">flux</span> measurements at one (anchor) site [<span class="hlt">2</span>, 3], and episodic, month long <span class="hlt">flux</span> measurements at the four additional sites using a roving eddy covariance tower. These data were complemented by measurements of environmental drivers, the amount of above ground phytomass and basic data on vegetation and soil type, as well as management. Data are subject to a rigorous statistical analysis in order to quantify significant differences in the <span class="hlt">CO</span><span class="hlt">2</span>, H<span class="hlt">2</span>O and energy exchange between the sites and to identify the factors which are responsible for these differences. In the present contribution we report results on <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. Our major findings are that (i) site-identity of the surveyed grassland ecosystems was a significant factor for the net ecosystem <span class="hlt">CO</span><span class="hlt">2</span> exchange (NEE), somewhat less for gross primary production (GPP) and not for</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRC..123..166F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRC..123..166F"><span>Non-Redfieldian Dynamics Explain Seasonal p<span class="hlt">CO</span><span class="hlt">2</span> Drawdown in the Gulf of Bothnia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fransner, Filippa; Gustafsson, Erik; Tedesco, Letizia; Vichi, Marcello; Hordoir, Robinson; Roquet, Fabien; Spilling, Kristian; Kuznetsov, Ivan; Eilola, Kari; Mörth, Carl-Magnus; Humborg, Christoph; Nycander, Jonas</p> <p>2018-01-01</p> <p>High inputs of nutrients and organic matter make coastal <span class="hlt">seas</span> places of intense <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange. Due to their complexity, the role of coastal <span class="hlt">seas</span> in the global <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange is, however, still uncertain. Here, we investigate the role of phytoplankton stoichiometric flexibility and extracellular DOC production for the seasonal nutrient and <span class="hlt">CO</span><span class="hlt">2</span> partial pressure (p<span class="hlt">CO</span><span class="hlt">2</span>) dynamics in the Gulf of Bothnia, Northern Baltic <span class="hlt">Sea</span>. A 3-D ocean biogeochemical-physical model with variable phytoplankton stoichiometry is for the first time implemented in the area and validated against observations. By simulating non-Redfieldian internal phytoplankton stoichiometry, and a relatively large production of extracellular dissolved organic carbon (DOC), the model adequately reproduces observed seasonal cycles in macronutrients and p<span class="hlt">CO</span><span class="hlt">2</span>. The uptake of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> is underestimated by 50% if instead using the Redfield ratio to determine the carbon assimilation, as in other Baltic <span class="hlt">Sea</span> models currently in use. The model further suggests, based on the observed drawdown of p<span class="hlt">CO</span><span class="hlt">2</span>, that observational estimates of organic carbon production in the Gulf of Bothnia, derived with the 14C method, may be heavily underestimated. We conclude that stoichiometric variability and uncoupling of carbon and nutrient assimilation have to be considered in order to better understand the carbon cycle in coastal <span class="hlt">seas</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..1511498F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..1511498F"><span>Aircraft observations of the urban <span class="hlt">CO</span><span class="hlt">2</span> dome in London and calculated daytime <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> at the urban-regional scale</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Font, Anna; Morgui, Josep Anton; Grimmond, Sue; Barratt, Benjamin</p> <p>2013-04-01</p> <p> dispersed downwind, with peak concentrations displaced from the urban centre along the main wind direction. The urban-regional surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> was calculated for four days in October 2011 by either the Integrative Mass Boundary Layer (IMBL) or the Column Integration method (CIM), dependent on meteorological conditions. The diurnal <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> in London obtained from the aircraft observations ranged from 36 to 71 μmol <span class="hlt">CO</span><span class="hlt">2</span> m-<span class="hlt">2</span> s-1 during the day time. This compared well with continuous measurements of <span class="hlt">CO</span><span class="hlt">2</span> exchange by an eddy-covariance system located in central London. The day-to-day variability observed in the calculated <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> responded to the spatial variability of the influence area and emissions that observations were sensitive to. This study provides an example how aircraft surveys in urban areas can be used to estimate <span class="hlt">CO</span><span class="hlt">2</span> surface <span class="hlt">fluxes</span> at the urban-regional scale. It also presents an important cross-validation of two independent measurement-based methods to infer the contribution of urban areas to climate change in terms of <span class="hlt">CO</span><span class="hlt">2</span> emissions that complement bottom-up emissions inventories. References Committee on Methods for Estimating Greenhouse Gas Emissions (2010), The National Academia Press. DECC (2012), http://www.decc.gov.uk/en/content/cms/statistics/indicators/ni186/ni186.aspx</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.P43C2897W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.P43C2897W"><span><span class="hlt">Sea</span> Ice as a Sink for <span class="hlt">CO</span><span class="hlt">2</span> and Biogeochemical Material: a Novel Sampling Method and Astrobiological Applications</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wilner, J.; Hofmann, A.; Hand, K. P.</p> <p>2017-12-01</p> <p>Accurately modelling the intensification of greenhouse gas effects in the polar regions ("polar amplification") necessitates a thorough understanding of the geochemical balance between atmospheric, <span class="hlt">sea</span> ice, and oceanic layers. <span class="hlt">Sea</span> ice is highly permeable to <span class="hlt">CO</span><span class="hlt">2</span> and therefore represents a major sink of oceanic <span class="hlt">CO</span><span class="hlt">2</span> in winter and of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> in summer, sinks that are typically either poorly constrained in or fully absent from global climate models. We present a novel method for sampling both trapped and dissolved gases (<span class="hlt">CO</span><span class="hlt">2</span>, CH4 and δ13CH4) in <span class="hlt">sea</span> ice with a Picarro 2132-i Methane Analyzer, taking the following sampling considerations into account: minimization of water and <span class="hlt">air</span> contamination, full headspace sampling, prevention of inadvertent sample bag double-puncturing, and ease of use. This method involves melting of vacuum-sealed ice cores to evacuate trapped gases to the headspace and sampling the headspace gas with a blunt needle sheathed by a beveled puncturing needle. A gravity catchment tube prevents input of dangerous levels of liquid water to the Picarro cavity. Subsequent ultrasonic degassing allows for dissolved gas measurement. We are in the process of using this method to sample gases trapped and dissolved in Arctic autumn <span class="hlt">sea</span> ice cores and atmospheric samples collected during the 2016 Polarstern Expedition and during a May 2017 field campaign north of Barrow, Alaska. We additionally employ this method, together with inductively coupled plasma mass spectrometry (ICP-MS), to analyze the transfer of potential biogeochemical signatures of underlying hydrothermal plumes to <span class="hlt">sea</span> ice. This has particular relevance to Europa and Enceladus, where hypothetical hydrothermal plumes may deliver seafloor chemicals to the overlying ice shell. Hence, we are presently investigating the entrainment of methane and other hydrothermal material in <span class="hlt">sea</span> ice cores collected along the Gakkel Ridge that may serve as biosignatures of methanogenic organisms in seafloor</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A54C..02M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A54C..02M"><span>Continuous Flow Hygroscopicity-Resolved Relaxed Eddy Accumulation (Hy-Res REA) Method of Measuring Size-Resolved <span class="hlt">Sea</span>-Salt Particle <span class="hlt">Fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Meskhidze, N.; Royalty, T. M.; Phillips, B.; Dawson, K. W.; Petters, M. D.; Reed, R.; Weinstein, J.; Hook, D.; Wiener, R.</p> <p>2017-12-01</p> <p>The accurate representation of aerosols in climate models requires direct ambient measurement of the size- and composition-dependent particle production <span class="hlt">fluxes</span>. Here we present the design, testing, and analysis of data collected through the first instrument capable of measuring hygroscopicity-based, size-resolved particle <span class="hlt">fluxes</span> using a continuous-flow Hygroscopicity-Resolved Relaxed Eddy Accumulation (Hy-Res REA) technique. The different components of the instrument were extensively tested inside the US Environmental Protection Agency's Aerosol Test Facility for <span class="hlt">sea</span>-salt and ammoniums sulfate particle <span class="hlt">fluxes</span>. The new REA system design does not require particle accumulation, therefore avoids the diffusional wall losses associated with long residence times of particles inside the <span class="hlt">air</span> collectors of the traditional REA devices. The Hy-Res REA system used in this study includes a 3-D sonic anemometer, two fast-response solenoid valves, two Condensation Particle Counters (CPCs), a Scanning Mobility Particle Sizer (SMPS), and a Hygroscopicity Tandem Differential Mobility Analyzer (HTDMA). A linear relationship was found between the <span class="hlt">sea</span>-salt particle <span class="hlt">fluxes</span> measured by eddy covariance and REA techniques, with comparable theoretical (0.34) and measured (0.39) proportionality constants. The <span class="hlt">sea</span>-salt particle detection limit of the Hy-Res REA <span class="hlt">flux</span> system is estimated to be 6x105 m-<span class="hlt">2</span>s-1. For the conditions of ammonium sulfate and <span class="hlt">sea</span>-salt particles of comparable source strength and location, the continuous-flow Hy-Res REA instrument was able to achieve better than 90% accuracy of measuring the <span class="hlt">sea</span>-salt particle <span class="hlt">fluxes</span>. In principle, the instrument can be applied to measure <span class="hlt">fluxes</span> of particles of variable size and distinct hygroscopic properties (i.e., mineral dust, black carbon, etc.).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150002539','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150002539"><span>Assessing <span class="hlt">Air-Sea</span> Interaction in the Evolving NASA GEOS Model</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Clayson, Carol Anne; Roberts, J. Brent</p> <p>2015-01-01</p> <p>In order to understand how the climate responds to variations in forcing, one necessary component is to understand the full distribution of variability of exchanges of heat and moisture between the atmosphere and ocean. Surface heat and moisture <span class="hlt">fluxes</span> are critical to the generation and decay of many coupled <span class="hlt">air-sea</span> phenomena. These mechanisms operate across a number of scales and contain contributions from interactions between the anomalous (i.e. non-mean), often extreme-valued, <span class="hlt">flux</span> components. Satellite-derived estimates of the surface turbulent and radiative heat <span class="hlt">fluxes</span> provide an opportunity to assess results from modeling systems. Evaluation of only time mean and variability statistics, however only provides limited traceability to processes controlling what are often regime-dependent errors. This work will present an approach to evaluate the representation of the turbulent <span class="hlt">fluxes</span> at the <span class="hlt">air-sea</span> interface in the current and evolving Goddard Earth Observing System (GEOS) model. A temperature and moisture vertical profile-based clustering technique is used to identify robust weather regimes, and subsequently intercompare the turbulent <span class="hlt">fluxes</span> and near-surface parameters within these regimes in both satellite estimates and GEOS-driven data sets. Both model reanalysis (MERRA) and seasonal-to-interannual coupled GEOS model simulations will be evaluated. Particular emphasis is placed on understanding the distribution of the <span class="hlt">fluxes</span> including extremes, and the representation of near-surface forcing variables directly related to their estimation. Results from these analyses will help identify the existence and source of regime-dependent biases in the GEOS model ocean surface turbulent <span class="hlt">fluxes</span>. The use of the temperature and moisture profiles for weather-state clustering will be highlighted for its potential broad application to 3-D output typical of model simulations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.A41P..05C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.A41P..05C"><span>Assessing <span class="hlt">air-sea</span> interaction in the evolving NASA GEOS model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Clayson, C. A.; Roberts, J. B.</p> <p>2014-12-01</p> <p>In order to understand how the climate responds to variations in forcing, one necessary component is to understand the full distribution of variability of exchanges of heat and moisture between the atmosphere and ocean. Surface heat and moisture <span class="hlt">fluxes</span> are critical to the generation and decay of many coupled <span class="hlt">air-sea</span> phenomena. These mechanisms operate across a number of scales and contain contributions from interactions between the anomalous (i.e. non-mean), often extreme-valued, <span class="hlt">flux</span> components. Satellite-derived estimates of the surface turbulent and radiative heat <span class="hlt">fluxes</span> provide an opportunity to assess results from modeling systems. Evaluation of only time mean and variability statistics, however only provides limited traceability to processes controlling what are often regime-dependent errors. This work will present an approach to evaluate the representation of the turbulent <span class="hlt">fluxes</span> at the <span class="hlt">air-sea</span> interface in the current and evolving Goddard Earth Observing System (GEOS) model. A temperature and moisture vertical profile-based clustering technique is used to identify robust weather regimes, and subsequently intercompare the turbulent <span class="hlt">fluxes</span> and near-surface parameters within these regimes in both satellite estimates and GEOS-driven data sets. Both model reanalysis (MERRA) and seasonal-to-interannual coupled GEOS model simulations will be evaluated. Particular emphasis is placed on understanding the distribution of the <span class="hlt">fluxes</span> including extremes, and the representation of near-surface forcing variables directly related to their estimation. Results from these analyses will help identify the existence and source of regime-dependent biases in the GEOS model ocean surface turbulent <span class="hlt">fluxes</span>. The use of the temperature and moisture profiles for weather-state clustering will be highlighted for its potential broad application to 3-D output typical of model simulations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003EAEJA....11892I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003EAEJA....11892I"><span><span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> response to precipitation events in Juniperus osteosperma and Artemisia tridentata ecosystems using eddy covariance measurements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ivans, S.; Hipps, L. E.</p> <p>2003-04-01</p> <p>Eddy covariance measurements were used to determine the seasonal changes of net <span class="hlt">CO</span>_<span class="hlt">2</span> <span class="hlt">flux</span>, and the response to intermittent precipitation events in juniper (Juniperus osteosperma) and sagebrush (Artemisia tridentata) plant communities in a semi-arid region in the Great Basin of the United States over the entire growing seasons of 2001 and 2002. The net <span class="hlt">CO</span>_<span class="hlt">2</span> <span class="hlt">fluxes</span> were negative or downward in each community during the spring when soil water availability was largest. During this time, rain events resulted in large increases of net <span class="hlt">CO</span>_<span class="hlt">2</span> uptake in juniper within 24 hours after the rain. The relative increases were larger in the dry spring of 2001 compared to the wetter conditions of 2002. Response of sage to rain events in the spring was smaller in magnitude. During the dry periods of summer and early fall net <span class="hlt">CO</span>_<span class="hlt">2</span> <span class="hlt">flux</span> was upward at each site in both years. In these periods the respiration of soil and vegetation apparently exceeded any assimilation by the plants. During these dry periods increases in <span class="hlt">CO</span>_<span class="hlt">2</span> efflux were observed at both sites following rain events, presumably as a result of increases in soil respiration. The response of <span class="hlt">CO</span>_<span class="hlt">2</span> <span class="hlt">fluxes</span> to these events lasted generally <span class="hlt">2</span> to 3 days. During late fall and early winter, no significant changes in <span class="hlt">CO</span>_<span class="hlt">2</span> <span class="hlt">fluxes</span> were observed at either site in response to rainfall because of significantly lower temperatures and plant dormancy in the year 2001. However in 2002, because of warmer weather, rainfall events triggered a temporary change in the <span class="hlt">flux</span> direction at both sites from <span class="hlt">CO</span>_<span class="hlt">2</span> efflux to <span class="hlt">CO</span>_<span class="hlt">2</span> uptake, suggesting that the plants were actively photosynthesizing. Energy balance closure values for both sites ranged from 0.75--0.80 in the moist conditions of spring, and increased to 0.80--0.85 in the dry conditions of summer and fall. It is not yet clear why energy balance closure is dependent upon the relative sizes of sensible and latent heat <span class="hlt">fluxes</span>. The issue of whether or not to force closure by adding to the <span class="hlt">fluxes</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/5224949','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/5224949"><span>Elevated <span class="hlt">CO</span><span class="hlt">2</span> stimulates marsh elevation gain, counterbalancing <span class="hlt">sea</span>-level rise</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Langley, J.A.; McKee, K.L.; Cahoon, D.R.; Cherry, J.A.; Megonigala, J.P.</p> <p>2009-01-01</p> <p>Tidal wetlands experiencing increased rates of <span class="hlt">sea</span>-level rise (SLR) must increase rates of soil elevation gain to avoid permanent conversion to open water. The maximal rate of SLR that these ecosystems can tolerate depends partly on mineral sediment deposition, but the accumulation of organic matter is equally important for many wetlands. Plant productivity drives organic matter dynamics and is sensitive to global change factors, such as rising atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentration. It remains unknown how global change will influence organic mechanisms that determine future tidal wetland viability. Here, we present experimental evidence that plant response to elevated atmospheric [<span class="hlt">CO</span><span class="hlt">2</span>] stimulates biogenic mechanisms of elevation gain in a brackish marsh. Elevated <span class="hlt">CO</span><span class="hlt">2</span> (ambient + 340 ppm) accelerated soil elevation gain by 3.9 mm yr−1in this <span class="hlt">2</span>-year field study, an effect mediated by stimulation of below-ground plant productivity. Further, a companion greenhouse experiment revealed that the <span class="hlt">CO</span><span class="hlt">2</span> effect was enhanced under salinity and flooding conditions likely to accompany future SLR. Our results indicate that by stimulating biogenic contributions to marsh elevation, increases in the greenhouse gas, <span class="hlt">CO</span><span class="hlt">2</span>, may paradoxically aid some coastal wetlands in counterbalancing rising <span class="hlt">seas</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19325121','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19325121"><span>Elevated <span class="hlt">CO</span><span class="hlt">2</span> stimulates marsh elevation gain, counterbalancing <span class="hlt">sea</span>-level rise.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Langley, J Adam; McKee, Karen L; Cahoon, Donald R; Cherry, Julia A; Megonigal, J Patrick</p> <p>2009-04-14</p> <p>Tidal wetlands experiencing increased rates of <span class="hlt">sea</span>-level rise (SLR) must increase rates of soil elevation gain to avoid permanent conversion to open water. The maximal rate of SLR that these ecosystems can tolerate depends partly on mineral sediment deposition, but the accumulation of organic matter is equally important for many wetlands. Plant productivity drives organic matter dynamics and is sensitive to global change factors, such as rising atmospheric <span class="hlt">CO</span>(<span class="hlt">2</span>) concentration. It remains unknown how global change will influence organic mechanisms that determine future tidal wetland viability. Here, we present experimental evidence that plant response to elevated atmospheric [<span class="hlt">CO</span>(<span class="hlt">2</span>)] stimulates biogenic mechanisms of elevation gain in a brackish marsh. Elevated <span class="hlt">CO</span>(<span class="hlt">2</span>) (ambient + 340 ppm) accelerated soil elevation gain by 3.9 mm yr(-1) in this <span class="hlt">2</span>-year field study, an effect mediated by stimulation of below-ground plant productivity. Further, a companion greenhouse experiment revealed that the <span class="hlt">CO</span>(<span class="hlt">2</span>) effect was enhanced under salinity and flooding conditions likely to accompany future SLR. Our results indicate that by stimulating biogenic contributions to marsh elevation, increases in the greenhouse gas, <span class="hlt">CO</span>(<span class="hlt">2</span>), may paradoxically aid some coastal wetlands in counterbalancing rising <span class="hlt">seas</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2661312','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2661312"><span>Elevated <span class="hlt">CO</span><span class="hlt">2</span> stimulates marsh elevation gain, counterbalancing <span class="hlt">sea</span>-level rise</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Langley, J. Adam; McKee, Karen L.; Cahoon, Donald R.; Cherry, Julia A.; Megonigal, J. Patrick</p> <p>2009-01-01</p> <p>Tidal wetlands experiencing increased rates of <span class="hlt">sea</span>-level rise (SLR) must increase rates of soil elevation gain to avoid permanent conversion to open water. The maximal rate of SLR that these ecosystems can tolerate depends partly on mineral sediment deposition, but the accumulation of organic matter is equally important for many wetlands. Plant productivity drives organic matter dynamics and is sensitive to global change factors, such as rising atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentration. It remains unknown how global change will influence organic mechanisms that determine future tidal wetland viability. Here, we present experimental evidence that plant response to elevated atmospheric [<span class="hlt">CO</span><span class="hlt">2</span>] stimulates biogenic mechanisms of elevation gain in a brackish marsh. Elevated <span class="hlt">CO</span><span class="hlt">2</span> (ambient + 340 ppm) accelerated soil elevation gain by 3.9 mm yr−1 in this <span class="hlt">2</span>-year field study, an effect mediated by stimulation of below-ground plant productivity. Further, a companion greenhouse experiment revealed that the <span class="hlt">CO</span><span class="hlt">2</span> effect was enhanced under salinity and flooding conditions likely to accompany future SLR. Our results indicate that by stimulating biogenic contributions to marsh elevation, increases in the greenhouse gas, <span class="hlt">CO</span><span class="hlt">2</span>, may paradoxically aid some coastal wetlands in counterbalancing rising <span class="hlt">seas</span>. PMID:19325121</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_19 --> <div id="page_20" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="381"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25826919','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25826919"><span>[Distributions and <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> of dissolved nitrous oxide in the Yangtze River estuary and its adjacent marine area in spring and summer].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Lan; Zhang, Gui-ling; Sun, Ming-shuang; Ren, Jing-ling</p> <p>2014-12-01</p> <p>Distributions and <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> of nitrous oxide (N<span class="hlt">2</span>O) in the seawaters of the Yangtze River estuary and its adjacent marine area were investigated during two cruises in March and July 2012. Dissolved N<span class="hlt">2</span>O concentrations in surface waters ranged from 9.34 to 49.08 nmol x L(-1) with an average of (13.27 ± 6.40) nmol x L(-1) in spring and ranged from 7.27 to 27.81 nmol x L(-1) with an average of (10.62 ± 5.03) nmol x L(-1) in summer. There was no obvious difference between surface and bottom N<span class="hlt">2</span>O concentrations. N<span class="hlt">2</span>O concentrations in both surface and bottom waters decreased along the freshwater plume from the river mouth to the open <span class="hlt">sea</span>. High values of dissolved N<span class="hlt">2</span>O were found in turbidity maximum zone, which suggests that maximal turbidity enhances nitrification. Temperature had dual effects on dissolved N<span class="hlt">2</span>O concentrations. N<span class="hlt">2</span>O saturations in surface waters ranged from 86.9% to 351.3% with an average of (111.5 ± 41.4)% in spring and ranged from 111.7% to 396.0% with an average of (155.9 ± 68.4)% in summer. N<span class="hlt">2</span>O were over-saturated at most stations. The <span class="hlt">sea-to-air</span> <span class="hlt">fluxes</span> of N<span class="hlt">2</span>O were estimated to be (3.<span class="hlt">2</span> ± 10.9), (5.5 ± 19.3) and (12.<span class="hlt">2</span> ±52.3) μmol x (m<span class="hlt">2</span> x d)(-1) in spring and (7.3 ± 12.4), (12.7 ± 20.4) and (20.4 ± 35.9) μmol x (m<span class="hlt">2</span> x d)(-1) in summer using the LM86, W92 and RC01 relationships, respectively. The annual emissions of N<span class="hlt">2</span>O from the Yangtze River estuary and its adjacent marine area were estimated to be 0.6 x 10(-<span class="hlt">2</span>) Tg x a(-1) (LM86), 1.1 x 10(-<span class="hlt">2</span>) Tg x a(-1) (W92) and <span class="hlt">2</span>.0 x 10(-<span class="hlt">2</span>) Tg x a(-1) (RC01). Although the area of the Yangtze River estuary and its adjacent marine area only accounts for 0.02% of the total area of the world's oceans, their emission of N<span class="hlt">2</span>O accounts for 0.06% of global oceanic N<span class="hlt">2</span>O emission, indicating that the Yangtze River estuary and its adjacent marine area is an active area to produce and emit N<span class="hlt">2</span>O.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeoRL..44.3887K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoRL..44.3887K"><span><span class="hlt">Air-Sea</span> exchange of biogenic volatile organic compounds and the impact on aerosol particle size distributions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kim, Michelle J.; Novak, Gordon A.; Zoerb, Matthew C.; Yang, Mingxi; Blomquist, Byron W.; Huebert, Barry J.; Cappa, Christopher D.; Bertram, Timothy H.</p> <p>2017-04-01</p> <p>We report simultaneous, underway eddy covariance measurements of the vertical <span class="hlt">flux</span> of isoprene, total monoterpenes, and dimethyl sulfide (DMS) over the Northern Atlantic Ocean during fall. Mean isoprene and monoterpene <span class="hlt">sea-to-air</span> vertical <span class="hlt">fluxes</span> were significantly lower than mean DMS <span class="hlt">fluxes</span>. While rare, intense monoterpene <span class="hlt">sea-to-air</span> <span class="hlt">fluxes</span> were observed, coincident with elevated monoterpene mixing ratios. A statistically significant correlation between isoprene vertical <span class="hlt">flux</span> and short wave radiation was not observed, suggesting that photochemical processes in the surface microlayer did not enhance isoprene emissions in this study region. Calculations of secondary organic aerosol production rates (PSOA) for mean isoprene and monoterpene emission rates sampled here indicate that PSOA is on average <0.1 μg m-3 d-1. Despite modest PSOA, low particle number concentrations permit a sizable role for condensational growth of monoterpene oxidation products in altering particle size distributions and the concentration of cloud condensation nuclei during episodic monoterpene emission events from the ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005TellB..57....1M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005TellB..57....1M"><span>Soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> from three ecosystems in tropical peatland of Sarawak, Malaysia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Melling, Lulie; Hatano, Ryusuke; Goh, Kah Joo</p> <p>2005-02-01</p> <p>Soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> was measured monthly over a year from tropical peatland of Sarawak, Malaysia using a closed-chamber technique. The soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> ranged from 100 to 533 mg C m<img src="/entityImage/script/2212.gif" alt="-" border="0" style="font-weight: bold"></img><span class="hlt">2</span> h<img src="/entityImage/script/2212.gif" alt="-" border="0" style="font-weight: bold"></img>1 for the forest ecosystem, 63 to 245 mg C m<img src="/entityImage/script/2212.gif" alt="-" border="0" style="font-weight: bold"></img><span class="hlt">2</span> h<img src="/entityImage/script/2212.gif" alt="-" border="0" style="font-weight: bold"></img>1 for the sago and 46 to 335 mg C m<img src="/entityImage/script/2212.gif" alt="-" border="0" style="font-weight: bold"></img><span class="hlt">2</span> h<img src="/entityImage/script/2212.gif" alt="-" border="0" style="font-weight: bold"></img>1 for the oil palm. Based on principal component analysis (PCA), the environmental variables over all sites could be classified into three components, namely, climate, soil moisture and soil bulk density, which accounted for 86% of the seasonal variability. A regression tree approach showed that <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> in each ecosystem was related to different underlying environmental factors. They were relative humidity for forest, soil temperature at 5 cm for sago and water-filled pore space for oil palm. On an annual basis, the soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> was highest in the forest ecosystem with an estimated production of <span class="hlt">2</span>.1 kg C m<img src="/entityImage/script/2212.gif" alt="-" border="0" style="font-weight: bold"></img><span class="hlt">2</span> yr<img src="/entityImage/script/2212.gif" alt="-" border="0" style="font-weight: bold"></img>1 followed by oil palm at 1.5 kg C m<img src="/entityImage/script/2212.gif" alt="-" border="0" style="font-weight: bold"></img><span class="hlt">2</span> yr<img src="/entityImage/script/2212.gif" alt="-" border="0" style="font-weight: bold"></img>1 and sago at 1.1 kg C m<img src="/entityImage/script/2212.gif" alt="-" border="0" style="font-weight: bold"></img><span class="hlt">2</span> yr<img src="/entityImage/script/2212.gif" alt</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.7783Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.7783Z"><span>Impact of <span class="hlt">sea</span> spray on the Yellow and East China <span class="hlt">Seas</span> thermal structure during the passage of Typhoon Rammasun (2002)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, Lianxin; Zhang, Xuefeng; Chu, P. C.; Guan, Changlong; Fu, Hongli; Chao, Guofang; Han, Guijun; Li, Wei</p> <p>2017-10-01</p> <p>Strong winds lead to large amounts of <span class="hlt">sea</span> spray in the lowest part of the atmospheric boundary layer. The spray droplets affect the <span class="hlt">air-sea</span> heat <span class="hlt">fluxes</span> due to their evaporation and the momentum due to the change of <span class="hlt">sea</span> surface, and in turn change the upper ocean thermal structure. In this study, impact of <span class="hlt">sea</span> spray on upper ocean temperatures in the Yellow and East China <span class="hlt">Seas</span> (YES) during typhoon Rammasun's passage is investigated using the POMgcs ocean model with a <span class="hlt">sea</span> spray parameterization scheme, in which the <span class="hlt">sea</span> spray-induced heat <span class="hlt">fluxes</span> are based on an improved Fairall's <span class="hlt">sea</span> spray heat <span class="hlt">fluxes</span> algorithm, and the <span class="hlt">sea</span> spray-induced momentum <span class="hlt">fluxes</span> are derived from an improved COARE version <span class="hlt">2</span>.6 bulk model. The distribution of the <span class="hlt">sea</span> spray mediated turbulent <span class="hlt">fluxes</span> was primarily located at Rammasun eye-wall region, in accord with the maximal wind speeds regions. When Rammasun enters the Yellow <span class="hlt">sea</span>, the <span class="hlt">sea</span> spray mediated latent (sensible) heat <span class="hlt">flux</span> maximum is enhanced by 26% (13.5%) compared to that of the interfacial latent (sensible) heat <span class="hlt">flux</span>. The maximum of the total <span class="hlt">air-sea</span> momentum <span class="hlt">fluxes</span> is enhanced by 43% compared to the counterpart of the interfacial momentum <span class="hlt">flux</span>. Furthermore, the <span class="hlt">sea</span> spray plays a key role in enhancing the intensity of the typhoon-induced "cold suction" and "heat pump" processes. When the effect of <span class="hlt">sea</span> spray is considered, the maximum of the <span class="hlt">sea</span> surface cooling in the right side of Rammasun's track is increased by 0.5°C, which is closer to the available satellite observations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ACP....17...47S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ACP....17...47S"><span>Atmospheric <span class="hlt">CO</span><span class="hlt">2</span> observations and models suggest strong carbon uptake by forests in New Zealand</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Steinkamp, Kay; Mikaloff Fletcher, Sara E.; Brailsford, Gordon; Smale, Dan; Moore, Stuart; Keller, Elizabeth D.; Baisden, W. Troy; Mukai, Hitoshi; Stephens, Britton B.</p> <p>2017-01-01</p> <p>A regional atmospheric inversion method has been developed to determine the spatial and temporal distribution of <span class="hlt">CO</span><span class="hlt">2</span> sinks and sources across New Zealand for 2011-2013. This approach infers net <span class="hlt">air-sea</span> and <span class="hlt">air</span>-land <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> from measurement records, using back-trajectory simulations from the Numerical Atmospheric dispersion Modelling Environment (NAME) Lagrangian dispersion model, driven by meteorology from the New Zealand Limited Area Model (NZLAM) weather prediction model. The inversion uses in situ measurements from two fixed sites, Baring Head on the southern tip of New Zealand's North Island (41.408° S, 174.871° E) and Lauder from the central South Island (45.038° S, 169.684° E), and ship board data from monthly cruises between Japan, New Zealand, and Australia. A range of scenarios is used to assess the sensitivity of the inversion method to underlying assumptions and to ensure robustness of the results. The results indicate a strong seasonal cycle in terrestrial land <span class="hlt">fluxes</span> from the South Island of New Zealand, especially in western regions covered by indigenous forest, suggesting higher photosynthetic and respiratory activity than is evident in the current a priori land process model. On the annual scale, the terrestrial biosphere in New Zealand is estimated to be a net <span class="hlt">CO</span><span class="hlt">2</span> sink, removing 98 (±37) Tg <span class="hlt">CO</span><span class="hlt">2</span> yr-1 from the atmosphere on average during 2011-2013. This sink is much larger than the reported 27 Tg <span class="hlt">CO</span><span class="hlt">2</span> yr-1 from the national inventory for the same time period. The difference can be partially reconciled when factors related to forest and agricultural management and exports, fossil fuel emission estimates, hydrologic <span class="hlt">fluxes</span>, and soil carbon change are considered, but some differences are likely to remain. Baseline uncertainty, model transport uncertainty, and limited sensitivity to the northern half of the North Island are the main contributors to <span class="hlt">flux</span> uncertainty.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20070023316&hterms=casa&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dcasa','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20070023316&hterms=casa&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dcasa"><span>Progress in Modeling Global Atmospheric <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Fluxes</span> and Transport: Results from Simulations with Diurnal <span class="hlt">Fluxes</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Collatz, G. James; Kawa, R.</p> <p>2007-01-01</p> <p>Progress in better determining <span class="hlt">CO</span><span class="hlt">2</span> sources and sinks will almost certainly rely on utilization of more extensive and intensive <span class="hlt">CO</span><span class="hlt">2</span> and related observations including those from satellite remote sensing. Use of advanced data requires improved modeling and analysis capability. Under NASA Carbon Cycle Science support we seek to develop and integrate improved formulations for 1) atmospheric transport, <span class="hlt">2</span>) terrestrial uptake and release, 3) biomass and 4) fossil fuel burning, and 5) observational data analysis including inverse calculations. The transport modeling is based on meteorological data assimilation analysis from the Goddard Modeling and Assimilation Office. Use of assimilated met data enables model comparison to <span class="hlt">CO</span><span class="hlt">2</span> and other observations across a wide range of scales of variability. In this presentation we focus on the short end of the temporal variability spectrum: hourly to synoptic to seasonal. Using <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> at varying temporal resolution from the SIB <span class="hlt">2</span> and CASA biosphere models, we examine the model's ability to simulate <span class="hlt">CO</span><span class="hlt">2</span> variability in comparison to observations at different times, locations, and altitudes. We find that the model can resolve much of the variability in the observations, although there are limits imposed by vertical resolution of boundary layer processes. The influence of key process representations is inferred. The high degree of fidelity in these simulations leads us to anticipate incorporation of realtime, highly resolved observations into a multiscale carbon cycle analysis system that will begin to bridge the gap between top-down and bottom-up <span class="hlt">flux</span> estimation, which is a primary focus of NACP.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.B41C0458G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.B41C0458G"><span>Effects of experimental warming and elevated <span class="hlt">CO</span><span class="hlt">2</span> on surface methane and CO­<span class="hlt">2</span> <span class="hlt">fluxes</span> from a boreal black spruce peatland</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gill, A. L.; Finzi, A.; Giasson, M. A.</p> <p>2015-12-01</p> <p>High latitude peatlands represent a major terrestrial carbon store sensitive to climate change, as well as a globally significant methane source. While elevated atmospheric carbon dioxide concentrations and warming temperatures may increase peat respiration and C losses to the atmosphere, reductions in peatland water tables associated with increased growing season evapotranspiration may alter the nature of trace gas emission and increase peat C losses as <span class="hlt">CO</span><span class="hlt">2</span> relative to methane (CH4). As CH4 is a greenhouse gas with twenty times the warming potential of <span class="hlt">CO</span><span class="hlt">2</span>, it is critical to understand how surface <span class="hlt">fluxes</span> of <span class="hlt">CO</span><span class="hlt">2</span> and CH4 will be influenced by factors associated with global climate change. We used automated soil respiration chambers to assess the influence of elevated atmospheric <span class="hlt">CO</span><span class="hlt">2</span> and whole ecosystem warming on peatland CH4 and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> at the SPRUCE (Spruce and Peatland Responses Under Climatic and Environmental Change) Experiment in northern Minnesota. Belowground warming treatments were initiated in July 2014 and whole ecosystem warming and elevated <span class="hlt">CO</span><span class="hlt">2</span> treatments began in August 2015. Here we report soil i<span class="hlt">CO</span><span class="hlt">2</span> and iCH4 <span class="hlt">flux</span> responses to the first year of belowground warming and the first two months of whole ecosystem manipulation. We also leverage the spatial and temporal density of measurements across the twenty autochambers to assess how physical (i.e., plant species composition, microtopography) and environmental (i.e., peat temperature, water table position, oxygen availability) factors influence observed rates of CH4 and <span class="hlt">CO</span><span class="hlt">2</span> loss. We find that methane <span class="hlt">fluxes</span> increased significantly across warming treatments following the first year of belowground warming, while belowground warming alone had little influence on soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. Peat microtopography strongly influenced trace gas emission rates, with higher CH4 <span class="hlt">fluxes</span> in hollow locations and higher <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in hummock locations. While there was no difference in the isotopic composition of the methane</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/12898382','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/12898382"><span>Elevated <span class="hlt">CO</span><span class="hlt">2</span> reduces sap <span class="hlt">flux</span> in mature deciduous forest trees.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Cech, Patrick G; Pepin, Steeve; Körner, Christian</p> <p>2003-10-01</p> <p>We enriched in <span class="hlt">CO</span><span class="hlt">2</span> the canopy of 14 broad-leaved trees in a species-rich, ca. 30-m-tall forest in NW Switzerland to test whether elevated <span class="hlt">CO</span><span class="hlt">2</span> reduces water use in mature forest trees. Measurements of sap <span class="hlt">flux</span> density (JS) were made prior to <span class="hlt">CO</span><span class="hlt">2</span> enrichment (summer 2000) and throughout the first whole growing season of <span class="hlt">CO</span><span class="hlt">2</span> exposure (2001) using the constant heat-flow technique. The short-term responses of sap <span class="hlt">flux</span> to brief (1.5-3 h) interruptions of <span class="hlt">CO</span><span class="hlt">2</span> enrichment were also examined. There were no significant a priori differences in morphological and physiological traits between trees which were later exposed to elevated <span class="hlt">CO</span><span class="hlt">2</span> (n=14) and trees later used as controls (n=19). Over the entire growing season, <span class="hlt">CO</span><span class="hlt">2</span> enrichment resulted in an average 10.7% reduction in mean daily JS across all species compared to control trees. Responses were most pronounced in Carpinus, Acer, Prunus and Tilia, smaller in Quercus and close to zero in Fagus trees. The JS of treated trees significantly increased by 7% upon transient exposure to ambient <span class="hlt">CO</span><span class="hlt">2</span> concentrations at noon. Hence, responses of the different species were, in the short term, similar in magnitude to those observed over the whole season (though opposite because of the reversed treatment). The reductions in mean JS of <span class="hlt">CO</span><span class="hlt">2</span>-enriched trees were high (22%) under conditions of low evaporative demand (vapour pressure deficit, VPD <5 hPa) and small (<span class="hlt">2</span>%) when mean daily VPD was greater than 10 hPa. During a relatively dry period, the effect of elevated <span class="hlt">CO</span><span class="hlt">2</span> on JS even appeared to be reversed. These results suggest that daily water savings by <span class="hlt">CO</span><span class="hlt">2</span>-enriched trees may have accumulated to a significantly improved water status by the time when control trees were short of soil moisture. Our data indicate that the magnitude of <span class="hlt">CO</span><span class="hlt">2</span> effects on stand transpiration will depend on rainfall regimes and the relative abundance of the different species, being more pronounced under humid conditions and in stands dominated by species such as Carpinus and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A43F2533S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A43F2533S"><span>Measurement of NOx and <span class="hlt">CO</span> <span class="hlt">Fluxes</span> from a Tall Tower in Beijing.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Squires, F. A.; Drysdale, W. S.; Hamilton, J.; Lee, J. D.; Vaughan, A. R.; Wild, O.; Mullinger, N.; Nemitz, E.; Metzger, S.; Zhang, Q.</p> <p>2017-12-01</p> <p>China's <span class="hlt">air</span> quality problems are well publicised; in 2010, 1.<span class="hlt">2</span> million premature deaths were attributed to outdoor <span class="hlt">air</span> pollution in China. One of the major <span class="hlt">air</span> quality issues is high concentrations of nitrogen oxides (NOx). China is the largest NOx emitter, contributing an estimated 18 % to global NOx emissions. Beijing itself is reported to have NO<span class="hlt">2</span> concentrations 42 % higher than the annual national standard. Given the high levels of pollution, increased focus has been placed on improving emissions estimates which are typically developed using a `bottom-up' approach where emissions are predicted from their sources. Emission inventories in China have large uncertainties and are rapidly changing with time in response to economic development, environmental regulation and new technologies. In fact, China is the largest contributor to the uncertainty in the source and the magnitude of <span class="hlt">air</span> pollutants in <span class="hlt">air</span> quality models. Recent studies have shown a discrepancy between NOx inventories and measured NOx emissions for UK cities, highlighting the limitations of bottom-up emissions inventories and the importance of accurate measurement data to improve the estimates. 5 Hz measurements of NOx and <span class="hlt">CO</span> concentration were made as part of the <span class="hlt">Air</span> Pollutants in Beijing (AIRPOLL-Beijing) project during two field campaigns in Nov-Dec 2016 and May-June 2017. Sampling took place from an inlet <span class="hlt">co</span>-located with a sonic anemometer at 102 m on a meteorological tower in central Beijing. Analysis of the covariance between vertical wind speed and concentration enabled the calculation of emission <span class="hlt">flux</span>, with an estimated footprint of between <span class="hlt">2</span> - 5 km from the tower (which typically included some major ring roads and expressways). <span class="hlt">Fluxes</span> were quantified using the continuous wavelet transformation (CWT) method, which enabled one minute resolved <span class="hlt">fluxes</span> to be calculated. These data were compared to existing emissions estimates from the Multi-resolution Emission Inventory for China (MEIC). It is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.4632A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.4632A"><span>Diffuse <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> from Santiago and Congro volcanic lakes (São Miguel, Azores archipelago)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Andrade, César; Cruz, José; Viveiros, Fátima; Branco, Rafael</p> <p>2017-04-01</p> <p>Diffuse <span class="hlt">CO</span><span class="hlt">2</span> degassing occurring in Santiago and Congro lakes, both located in depressions associated to maars from São Miguel Island (Azores, Portugal), was studied through detailed <span class="hlt">flux</span> measurements. Four sampling campaigns were developed between 2013 and 2016 in each water body, split by the cold and wet seasons. São Miguel has an area of 744.6 km<span class="hlt">2</span>, being the largest island of the archipelago. The geology of the island is dominated by three quiescent central volcanoes (Sete Cidades, Fogo and Furnas), linked by volcanic fissural zones (Picos and Congro Fissural Volcanic systems). The oldest volcanic systems of the island are located in its eastern part (Povoação-Nordeste). Santiago lake, with a surface area of 0.26 km<span class="hlt">2</span> and a depth of 30.5 m, is located inside a maar crater in the Sete Cidades volcano at an altitude of 355 m. The watershed of the lake has an area of 0.97 km<span class="hlt">2</span> and a surface flow estimated as 1.54x10 m3/a. A total of 1612 <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> measurements using the accumulation chamber method were made at Santiago lake, 253 in the first campaign (November 2013), and 462, 475 and 422 in the three other campaigns, respectively, in April 2014, September 2016 and December 2016. The total <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> estimated for this lake varies between 0.4 t d-1 and 0.59 t d-1, for the surveys performed, respectively, in November 2013 and September 2016; higher <span class="hlt">CO</span><span class="hlt">2</span> outputs of 1.57 and 5.87 t d-1 were calculated for the surveys carried out in April 2014 and December 2016. These higher <span class="hlt">CO</span><span class="hlt">2</span> emissions were associated with a period without water column stratification. Similarly to Santiago lake, Congro lake is located inside a maar, in the Congro Fissural Volcanic system, and has a surface area of 0.04 km<span class="hlt">2</span> with 18.5 m depth and a storage of about <span class="hlt">2</span>.4x105 m3/a. The lake, located at an altitude of 420 m, is fed by a watershed with an area of 0.33 km<span class="hlt">2</span> and a runoff estimated as about 8x104 m3/a. In Congro lake a total of 713 <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> measurements were performed during four surveys from</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017DSRI..126...62L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017DSRI..126...62L"><span>Long-term variation of mesopelagic biogenic <span class="hlt">flux</span> in the central South China <span class="hlt">Sea</span>: Impact of monsoonal seasonality and mesoscale eddy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Hongliang; Wiesner, Martin G.; Chen, Jianfang; Ling, Zheng; Zhang, Jingjing; Ran, Lihua</p> <p>2017-08-01</p> <p>The East Asian Monsoon and mesoscale eddies are known to regulate primary production in South China <span class="hlt">Sea</span> (SCS), the largest tropical marginal <span class="hlt">sea</span>; however, their contributions to the deep biogenic <span class="hlt">flux</span> are yet to be quantified. Based on 7-year time series sediment trap observations at the depth of 1200 m in the central SCS, we used the monthly average sinking biogenic <span class="hlt">fluxes</span> to evaluate the impact of the monsoon and mesoscale cyclonic eddies on biogenic <span class="hlt">fluxes</span> in combination with remote sensing physical parameters. The monthly average particulate organic carbon (POC) and opal <span class="hlt">fluxes</span>, ranging from 3.0 to 5.<span class="hlt">2</span> and 14.8-34.9 mg m-<span class="hlt">2</span> d-1, respectively, were higher during the northeastern monsoon period. This corresponded to the deeper mixed layer depth and higher net primary production in this area, due to nutrient replenishment from the subsurface induced by monsoon transition and surface cooling. In contrast, lower POC and opal <span class="hlt">fluxes</span> occurred during well-stratified inter-monsoon periods. In addition, Ca<span class="hlt">CO</span>3 <span class="hlt">flux</span> (23.6-37.0 mg m-<span class="hlt">2</span> d-1) exhibited less seasonality and was assumed to originate from foraminifera. In terms of the long-term record, the combined effect of cyclonic eddies and mixing in the upper ocean could effectively regulate the temporal variation in the biogenic <span class="hlt">flux</span>. In particular, the opal and POC <span class="hlt">fluxes</span> in cyclonic eddies were 116% and 41% higher on average, respectively, than those during the non-cyclonic eddy period. Since the cyclonic eddies mainly occurred during the northeastern monsoon period, their contributions to biogenic <span class="hlt">flux</span> via diatom blooms might overlap the regular winter <span class="hlt">flux</span> peak, which could make the biological carbon pump more efficient at <span class="hlt">CO</span><span class="hlt">2</span> sequestration during this period thus amplifying the impact of seasonal transition.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JMS...155...35I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JMS...155...35I"><span>Carbonate chemistry dynamics and biological processes along a river-<span class="hlt">sea</span> gradient (Gulf of Trieste, northern Adriatic <span class="hlt">Sea</span>)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ingrosso, Gianmarco; Giani, Michele; Cibic, Tamara; Karuza, Ana; Kralj, Martina; Del Negro, Paola</p> <p>2016-03-01</p> <p>In this paper we investigated, for two years and with a bi-monthly frequency, how physical, chemical, and biological processes affect the marine carbonate system in a coastal area characterized by high alkalinity riverine discharge (Gulf of Trieste, northern Adriatic <span class="hlt">Sea</span>, Mediterranean <span class="hlt">Sea</span>). By combining synoptic measurements of the carbonate system with in situ determinations of the primary production (14C incorporation technique) and secondary prokaryotic carbon production (3H-leucine incorporation) along a river-<span class="hlt">sea</span> gradient, we showed that the conservative mixing between river endmember and off-shore waters was the main driver of the dissolved inorganic carbon (DIC) distribution and seasonal variation. However, during spring and summer seasons also the influence of biological uptake and release of DIC was significant. In the surface water of June 2012, the spreading and persistence of nutrient-rich freshwater stimulated the primary production (3.21 μg C L- 1 h- 1) and net biological DIC decrease (- 100 μmol kg- 1), reducing the dissolved <span class="hlt">CO</span><span class="hlt">2</span> concentration and increasing the pHT. Below the pycnocline of August 2012, instead, an elevated bacterial carbon production rate (0.92 μg C L- 1 h- 1) was related with net DIC increase (92 μmol kg- 1), low dissolved oxygen concentration, and strong pHT reduction, suggesting the predominance of bacterial heterotrophic respiration over primary production. The <span class="hlt">flux</span> of carbon dioxide estimated at the <span class="hlt">air-sea</span> interface exerted a low influence on the seasonal variation of the carbonate system. A complex temporal and spatial dynamic of the <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange was also detected, due to the combined effects of seawater temperature, river discharge, and water circulation. On annual scale the system was a sink of atmospheric <span class="hlt">CO</span><span class="hlt">2</span>. However, in summer and during elevated riverine discharges, the area close to the river's mouth acted as a source of carbon dioxide. Also the wind speed was crucial in controlling the <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1340454-co2-capture-from-ambient-air-crystallization-guanidine-sorbent','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1340454-co2-capture-from-ambient-air-crystallization-guanidine-sorbent"><span><span class="hlt">CO</span> <span class="hlt">2</span> Capture from Ambient <span class="hlt">Air</span> by Crystallization with a Guanidine Sorbent</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Seipp, Charles A.; Univ. of Texas, Austin, TX; Williams, Neil J.; ...</p> <p>2016-12-21</p> <p>Carbon capture and storage is an important strategy for stabilizing the increasing concentration of atmospheric <span class="hlt">CO</span> <span class="hlt">2</span> and the global temperature. A possible approach toward reversing this trend and decreasing the atmospheric <span class="hlt">CO</span> <span class="hlt">2</span> concentration is to remove the <span class="hlt">CO</span> <span class="hlt">2</span> directly from <span class="hlt">air</span> (direct <span class="hlt">air</span> capture). In this paper, we report a simple aqueous guanidine sorbent that captures <span class="hlt">CO</span> <span class="hlt">2</span> from ambient <span class="hlt">air</span> and binds it as a crystalline carbonate salt by guanidinium hydrogen bonding. The resulting solid has very low aqueous solubility (K sp=1.0(4)×10 -8), which facilitates its separation from solution by filtration. The bound <span class="hlt">CO</span> <span class="hlt">2</span> canmore » be released by relatively mild heating of the crystals at 80–120 °C, which regenerates the guanidine sorbent quantitatively. Finally and thus, this crystallization-based approach to <span class="hlt">CO</span> <span class="hlt">2</span> separation from <span class="hlt">air</span> requires minimal energy and chemical input, and offers the prospect for low-cost direct <span class="hlt">air</span> capture technologies.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013NatGe...6..457Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013NatGe...6..457Z"><span>Millennial-scale changes in atmospheric <span class="hlt">CO</span><span class="hlt">2</span> levels linked to the Southern Ocean carbon isotope gradient and dust <span class="hlt">flux</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ziegler, Martin; Diz, Paula; Hall, Ian R.; Zahn, Rainer</p> <p>2013-06-01</p> <p>The rise in atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentrations observed at the end of glacial periods has, at least in part, been attributed to the upwelling of carbon-rich deep water in the Southern Ocean. The magnitude of outgassing of dissolved <span class="hlt">CO</span><span class="hlt">2</span>, however, is influenced by the biological fixation of upwelled inorganic carbon and its transfer back to the deep <span class="hlt">sea</span> as organic carbon. The efficiency of this biological pump is controlled by the extent of nutrient utilization, which can be stimulated by the delivery of iron by atmospheric dust particles. Changes in nutrient utilization should be reflected in the δ13C gradient between intermediate and deep waters. Here we use the δ13C values of intermediate- and bottom-dwelling foraminifera to reconstruct the carbon isotope gradient between thermocline and abyssal water in the subantarctic zone of the South Atlantic Ocean over the past 360,000 years. We find millennial-scale oscillations of the carbon isotope gradient that correspond to changes in dust <span class="hlt">flux</span> and atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentrations as reported from Antarctic ice cores. We interpret this correlation as a relationship between the efficiency of the biological pump and fertilization by dust-borne iron. As the correlation is exponential, we suggest that the sensitivity of the biological pump to dust-borne iron fertilization may be increased when the background dust <span class="hlt">flux</span> is low.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.B44D..06G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.B44D..06G"><span>Effects of experimental warming and elevated <span class="hlt">CO</span><span class="hlt">2</span> on surface methane and CO­<span class="hlt">2</span> <span class="hlt">fluxes</span> from a boreal black spruce peatland</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gill, A. L.; Finzi, A.; Hsieh, I. F.; Giasson, M. A.</p> <p>2016-12-01</p> <p>High latitude peatlands represent a major terrestrial carbon store sensitive to climate change, as well as a globally significant methane source. While elevated atmospheric carbon dioxide concentrations and warming temperatures may increase peat respiration and C losses to the atmosphere, reductions in peatland water tables associated with increased growing season evapotranspiration may alter the nature of trace gas emission and increase peat C losses as <span class="hlt">CO</span><span class="hlt">2</span> relative to methane (CH4). As CH4 is a greenhouse gas with twenty times the warming potential of <span class="hlt">CO</span><span class="hlt">2</span>, it is critical to understand how surface <span class="hlt">fluxes</span> of <span class="hlt">CO</span><span class="hlt">2</span> and CH4 will be influenced by factors associated with global climate change. We used automated soil respiration chambers to assess the influence of elevated atmospheric <span class="hlt">CO</span><span class="hlt">2</span> and whole ecosystem warming on peatland CH4 and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> at the SPRUCE (Spruce and Peatland Responses Under Climatic and Environmental Change) Experiment in northern Minnesota. Here we report soil i<span class="hlt">CO</span><span class="hlt">2</span> and iCH4 <span class="hlt">flux</span> responses to the first year of belowground warming and the first season of whole ecosystem warming and elevated <span class="hlt">CO</span><span class="hlt">2</span> treatments. We find that peat methane <span class="hlt">fluxes</span> are more sensitive to warming treatments than peat <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>, particularly in hollow peat microforms. Surface <span class="hlt">CO</span><span class="hlt">2</span>:CH4 <span class="hlt">flux</span> ratios decreased across warming treatments, suggesting that the temperature sensitivity of methane production overshadows the effect of peat drying and surface aeration in the short term. δ13C of the emitted methane was more depleted in the early and late growing season, indicating a transition from hydrogenotrophic to acetoclastic methanogenesis during periods of high photosynthetic input. The measurement record demonstrates that belowground warming has measureable impacts on the nature of peat greenhouse gas emission within one year of treatment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1224019-amineoxide-hybrid-materials-co-capture-from-ambient-air','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1224019-amineoxide-hybrid-materials-co-capture-from-ambient-air"><span>Amine–Oxide Hybrid Materials for <span class="hlt">CO</span> <span class="hlt">2</span> Capture from Ambient <span class="hlt">Air</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Didas, Stephanie A.; Choi, Sunho; Chaikittisilp, Watcharop; ...</p> <p>2015-09-10</p> <p>CONSPECTUS: Oxide supports functionalized with amine moieties have been used for decades as catalysts and chromatographic media. Owing to the recognized impact of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> on global climate change, the study of the use of amine-oxide hybrid materials as <span class="hlt">CO</span><span class="hlt">2</span> sorbents has exploded in the past decade. While the majority of the work has concerned separation of <span class="hlt">CO</span><span class="hlt">2</span> from dilute mixtures such as flue gas from coal-fired power plants, it has been recognized by us and others that such supported amine materials are also perhaps uniquely suited to extract <span class="hlt">CO</span><span class="hlt">2</span> from ultradilute gas mixtures, such as ambient <span class="hlt">air</span>. As unique,more » low temperature chemisorbents, they can operate under ambient conditions, spontaneously extracting <span class="hlt">CO</span><span class="hlt">2</span> from ambient <span class="hlt">air</span>, while being regenerated under mild conditions using heat or the combination of heat and vacuum. This Account describes the evolution of our activities on the design of amine-functionalized silica materials for catalysis to the design, characterization, and utilization of these materials in <span class="hlt">CO</span><span class="hlt">2</span> separations. New materials developed in our laboratory, such as hyperbranched aminosilica materials, and previously known amine-oxide hybrid compositions, have been extensively studied for <span class="hlt">CO</span><span class="hlt">2</span> extraction from simulated ambient <span class="hlt">air</span> (400 ppm of <span class="hlt">CO</span><span class="hlt">2</span>). The role of amine type and structure (molecular, polymeric), support type and structure, the stability of the various compositions under simulated operating conditions, and the nature of the adsorbed <span class="hlt">CO</span><span class="hlt">2</span> have been investigated in detail. The requirements for an effective, practical <span class="hlt">air</span> capture process have been outlined and the ability of amine−oxide hybrid materials to meet these needs has been discussed. Ultimately, the practicality of such a “direct <span class="hlt">air</span> capture” process is predicated not only on the physicochemical properties of the sorbent, but also how the sorbent operates in a practical process that offers a scalable gas−solid contacting strategy. In this regard, the utility of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1224019-amineoxide-hybrid-materials-co2-capture-from-ambient-air','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1224019-amineoxide-hybrid-materials-co2-capture-from-ambient-air"><span>Amine–Oxide Hybrid Materials for <span class="hlt">CO</span> <span class="hlt">2</span> Capture from Ambient <span class="hlt">Air</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Didas, Stephanie A.; Choi, Sunho; Chaikittisilp, Watcharop; ...</p> <p>2015-09-10</p> <p>Oxide supports functionalized with amine moieties have been used for decades as catalysts and chromatographic media. Owing to the recognized impact of atmospheric <span class="hlt">CO</span> <span class="hlt">2</span> on global climate change, the study of the use of amine-oxide hybrid materials as <span class="hlt">CO</span> <span class="hlt">2</span> sorbents has exploded in the past decade. While the majority of the work has concerned separation of <span class="hlt">CO</span> <span class="hlt">2</span> from dilute mixtures such as flue gas from coal-fired power plants, it has been recognized by us and others that such supported amine materials are also perhaps uniquely suited to extract <span class="hlt">CO</span> <span class="hlt">2</span> from ultradilute gas mixtures, such as ambientmore » <span class="hlt">air</span>. As unique, low temperature chemisorbents, they can operate under ambient conditions, spontaneously extracting <span class="hlt">CO</span> <span class="hlt">2</span> from ambient <span class="hlt">air</span>, while being regenerated under mild conditions using heat or the combination of heat and vacuum. This Account describes the evolution of our activities on the design of amine-functionalized silica materials for catalysis to the design, characterization, and utilization of these materials in <span class="hlt">CO</span> <span class="hlt">2</span> separations. New materials developed in our laboratory, such as hyperbranched aminosilica materials, and previously known amine-oxide hybrid compositions, have been extensively studied for <span class="hlt">CO</span> <span class="hlt">2</span> extraction from simulated ambient <span class="hlt">air</span> (400 ppm of <span class="hlt">CO</span> <span class="hlt">2</span>). The role of amine type and structure (molecular, polymeric), support type and structure, the stability of the various compositions under simulated operating conditions, and the nature of the adsorbed <span class="hlt">CO</span> <span class="hlt">2</span> have been investigated in detail. The requirements for an effective, practical <span class="hlt">air</span> capture process have been outlined and the ability of amine-oxide hybrid materials to meet these needs has been discussed. Ultimately, the practicality of such a “direct <span class="hlt">air</span> capture” process is predicated not only on the physicochemical properties of the sorbent, but also how the sorbent operates in a practical process that offers a scalable gas-solid contacting strategy. In conclusion, the utility of low</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/43512','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/43512"><span>Consequences of incomplete surface energy balance closure for <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> from open-path <span class="hlt">CO</span><span class="hlt">2</span>/H<span class="hlt">2</span>O infrared gas analyzers</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Heping Liu; James T. Randerson; Jamie Lindfors; William J. Massman; Thomas Foken</p> <p>2006-01-01</p> <p>We present an approach for assessing the impact of systematic biases in measured energy <span class="hlt">fluxes</span> on <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> estimates obtained from open-path eddy-covariance systems. In our analysis, we present equations to analyse the propagation of errors through the Webb, Pearman, and Leuning (WPL) algorithm [Quart. J. Roy. Meteorol. Soc. 106, 85­100, 1980] that is widely used to...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.B51B0309S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.B51B0309S"><span>An analytical model for the distribution of <span class="hlt">CO</span><span class="hlt">2</span> sources and sinks, <span class="hlt">fluxes</span>, and mean concentration within the roughness sub-layer</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Siqueira, M. B.; Katul, G. G.</p> <p>2009-12-01</p> <p>A one-dimensional analytical model that predicts foliage <span class="hlt">CO</span><span class="hlt">2</span> uptake rates, turbulent <span class="hlt">fluxes</span>, and mean concentration throughout the roughness sub-layer (RSL), a layer that extends from the ground surface up to 5 times the canopy height (h), is proposed. The model combines the mean continuity equation for <span class="hlt">CO</span><span class="hlt">2</span> with first-order closure principles for turbulent <span class="hlt">fluxes</span> and simplified physiological and radiative transfer schemes for foliage uptake. This combination results in a second-order ordinary differential equation in which it is imposed soil respiration (RE) as lower and <span class="hlt">CO</span><span class="hlt">2</span> concentration well above the RSL as upper boundary conditions. An inverse version of the model was tested against data sets from two contrasting ecosystems: a tropical forest (TF, h=40 m) and a managed irrigated rice canopy (RC, h=0.7 m) - with good agreement noted between modeled and measured mean <span class="hlt">CO</span><span class="hlt">2</span> concentration profiles within the entire RSL (see figure). Sensitivity analysis on the model parameters revealed a plausible scaling regime between them and a dimensionless parameter defined by the ratio between external (RE) and internal (stomatal conductance) characteristics controlling the <span class="hlt">CO</span><span class="hlt">2</span> exchange process. The model can be used to infer the thickness of the RSL for <span class="hlt">CO</span><span class="hlt">2</span> exchange, the inequality in zero-plane displacement between <span class="hlt">CO</span><span class="hlt">2</span> and momentum, and its consequences on modeled <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. A simplified version of the solution is well suited for being incorporated into large-scale climate models. Furthermore, the model framework here can be used to a priori estimate relative contributions from the soil surface and the atmosphere to canopy-<span class="hlt">air</span> <span class="hlt">CO</span><span class="hlt">2</span> concentration thereby making it synergetic to stable isotopes studies. Panels a) and c): Profiles of normalized measured leaf area density distribution (a) for TF and RC, respectively. Continuous lines are the constant a used in the model and dashed lines represent data-derived profiles. Panels b) and d) are modeled and ensemble-averaged measured</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005JGRC..110.3010A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005JGRC..110.3010A"><span>Iron in the Ross <span class="hlt">Sea</span>: <span class="hlt">2</span>. Impact of discrete iron addition strategies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Arrigo, Kevin R.; Tagliabue, Alessandro</p> <p>2005-03-01</p> <p>Presented are results of a regional-scale numerical investigation into the effectiveness of Fe fertilization as a means to increase the efficiency of the biological pump in Fe-limited waters of the Ross <span class="hlt">Sea</span>, Antarctica. This investigation was conducted using a modified version of the Coupled Ice And Ocean (CIAO) ecosystem model of the Ross <span class="hlt">Sea</span> sector of the Southern Ocean. Four sets of experiments were performed, investigating the impacts of differences in (1) timing of fertilization, (<span class="hlt">2</span>) duration of fertilization, (3) amount of Fe added, and (4) size of the fertilized patch. Results show that the stimulation of <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange (FCO<span class="hlt">2</span>) depends primarily on the timing of fertilization, regardless of the amount of Fe added. When Fe was added at the optimal time of year, FCO<span class="hlt">2</span> from the atmosphere into the Ross <span class="hlt">Sea</span> was increased by 3-22%, depending on fertilization strategy. Increasing patch size produced the largest response, and increasing initial Fe concentration produced the smallest. In all cases, as the intensity of Fe fertilization increased, the fertilization efficiency (increase in <span class="hlt">CO</span><span class="hlt">2</span> uptake per unit added Fe) dropped. Strategies that maximized the fertilization efficiency resulted in relatively little additional <span class="hlt">CO</span><span class="hlt">2</span> being drawn out of the atmosphere. To markedly increase oceanic uptake of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> would require the addition of large amounts of Fe due to the low fertilization efficiencies associated with maximum <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange. Our results also show that differences in the fertilization strategy should be kept in mind when comparing the results of different Fe fertilization experiments.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_20 --> <div id="page_21" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="401"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25616188','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25616188"><span>Evaluation of the sinks and sources of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> by artificial upwelling.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Pan, Yiwen; Fan, Wei; Huang, Ting-Hsuan; Wang, Shu-Lun; Chen, Chen-Tung Arthur</p> <p>2015-04-01</p> <p>Artificial upwelling is considered a promising way to reduce the accumulation of anthropogenic carbon dioxide in the atmosphere. This practice could transport nutrient-rich deep water to the euphotic zone, enhance phytoplankton growth and consequently increase organic carbon exportation to the deep ocean via the biological pump. However, only a few studies quantitatively assess changes in oceanic <span class="hlt">CO</span><span class="hlt">2</span> uptake resulting from artificial upwelling. This article uses a simulation to examine the effect of hypothetical artificial upwelling-induced variations of <span class="hlt">CO</span><span class="hlt">2</span> fugacity in seawater (f<span class="hlt">CO</span><span class="hlt">2</span>) using observed carbon and nutrient data from 14 stations, ranging from 21 to 43°N, in the West Philippine <span class="hlt">Sea</span> (WPS), the East China <span class="hlt">Sea</span> (ECS) and the <span class="hlt">Sea</span> of Japan. Calculations are based on two basic assumptions: First, a near-field mixing of a nutrient-rich deep-ocean water plume in a stratified ocean environment is assumed to form given the presence of an artificial upwelling devise with appropriate technical parameters. Second, it is assumed that photosynthesis of marine phytoplankton could deplete all available nutrients following the stoichiometry of the modified Redfield ratio C/H/O/N/S/P=103.1/181.7/93.4/11.7/<span class="hlt">2</span>.1/1. Results suggest artificial upwelling has significant effects on regional changes in <span class="hlt">sea-air</span> differences (Δf<span class="hlt">CO</span><span class="hlt">2</span><span class="hlt">sea-air</span>) and the carbon sequestration potential (Δf<span class="hlt">CO</span><span class="hlt">2</span>mixed-amb). Large variations of Δf<span class="hlt">CO</span><span class="hlt">2</span><span class="hlt">sea-air</span> and Δf<span class="hlt">CO</span><span class="hlt">2</span>mixed-amb are shown to be associated with different regions, seasons and technical parameters of the artificial upwelling device. With proper design, it is possible to reverse the contribution of artificial upwelling from a strong <span class="hlt">CO</span><span class="hlt">2</span> source to sink. Thus, artificial upwelling has the potential to succeed as a geoengineering technique to sequester anthropogenic <span class="hlt">CO</span><span class="hlt">2</span>, with appropriate technical parameters in the right region and season. Copyright © 2014 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19820009925','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19820009925"><span>Sensitivity of a climatologically-driven <span class="hlt">sea</span> ice model to the ocean heat <span class="hlt">flux</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Parkinson, C. L.; Good, M. R.</p> <p>1982-01-01</p> <p>Ocean heat <span class="hlt">flux</span> sensitivity was studied on a numerical model of <span class="hlt">sea</span> ice covering the Weddell <span class="hlt">Sea</span> region of the southern ocean. The model is driven by mean monthly climatological atmospheric variables. For each model run, the ocean heat <span class="hlt">flux</span> is uniform in both space and time. Ocean heat <span class="hlt">fluxes</span> below 20 W m to the minus <span class="hlt">2</span> power do not provide sufficient energy to allow the ice to melt to its summertime thicknesses and concentrations by the end of the 14 month simulation, whereas ocean heat <span class="hlt">fluxes</span> of 30 W m to the minus <span class="hlt">2</span> power and above result in too much ice melt, producing the almost total disappearance of ice in the Weddell <span class="hlt">Sea</span> by the end of the 14 months. These results are dependent on the atmospheric forcing fields.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMED41A0839B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMED41A0839B"><span>Effect of Wildfire on Sequoiadendron giganteum Growth and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Flux</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Barwegen, S.</p> <p>2016-12-01</p> <p>Due to global warming, parts of the United States are becoming drier than ever before. In 2015, we surpassed 9 million acres burned by wildfires nationally (Rice 2015). Wildfires are most common in the Western United States due to drought, and the fact that the summer months are drier than other areas such as the East Coast, so there is a higher risk for wildland fires (Donegan 2016). These high-growth forests that are more frequently burned by wildfires each year are located near mountain ranges on the west side of the United States. They are important to tourism, contain many endangered species, and need to maintain the natural cycle of fire and regrowth for the continued success of the native plant life. This project investigated the effect of burnt soil on Sequoiadendron giganteum trees. Three were grown in burnt potting soil that had been roasted over a grill for 45 minutes (which is the average destructive fire time), and the other three were the control group in unburned potting soil. We assessed growth by measuring height, color, photosynthetically active radiation (PAR), and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> to evaluate the health of the trees in the two soil conditions. We noted that after two weeks the trunks of the trees growing in burnt soil began to brown in color, and they lost leaves. Over the course of the experiment, the trees growing in burnt soil had reduced levels of photosynthesis as compared to the unburned soil (as measured by the net change in <span class="hlt">CO</span><span class="hlt">2</span> concentration in a sealed chamber over the course of fifteen minutes intervals). On average, the trees growing in burnt soil had <span class="hlt">flux</span> rates that were 19.59 ppm <span class="hlt">CO</span><span class="hlt">2</span> /min. more than those growing in unburned soil. In the dark reactions, the burnt soil <span class="hlt">flux</span> was 54.5 ppm <span class="hlt">CO</span><span class="hlt">2</span>/min., while the unburned soil averaged 40.5 ppm <span class="hlt">CO</span><span class="hlt">2</span>/min. Our results help quantify the impact of fire on delicate ecosystems that are experiencing an increase in fire activity caused by global warming.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A41E2327D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A41E2327D"><span>Controlling factors of evaporation and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> over an open water lake in southeastern margin of Tibetan Plateau</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Du, Q.; Liu, H.; Liu, Y.; Wang, L.; Xu, L.</p> <p>2017-12-01</p> <p>Erhai lake is located in the southeastern margin of Tibetan Plateau. Based on the 4 years measurement over Erhai lake with eddy covariance technique (EC) from 2012 to 2015, the diurnal and seasonal variations of latent and sensible heat and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>, and their controlling factors over different time scales were analyzed. The diurnal average LE ranged from 31 to 171 Wm-<span class="hlt">2</span>, while Hs ranged from -31 to 21 Wm-<span class="hlt">2</span>. Bowen ratio was larger during January and May and smaller during June and October. The lake continued storing heat during January and June, and releasing heat since July. The diurnal average <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> during nighttime were higher than the daytime, and carbon uptake was almost observed during the midday time of the day for the whole study period. The annual carbon budget fluctuated from 117.5 to 161.7 g C m-<span class="hlt">2</span> a-1, while annual total evaporation (ET) from 1120.8 to 1228.5 mm for the four-years period. The Erhai Lake behaved as a net carbon source over the whole period but carbon uptake was observed during the middle time of each year. The difference between water surface and <span class="hlt">air</span> temperature (DeltaT) and the product of DeltaT and wind speed were the main controlling factors for Hs from halfhourly to monthly scale. There was significant relationship between wind speed, the product of wind speed and vapor pressure deficit (VPD) and LE on halfhourly and daily scales. The total cloud amount and net radiation (Rn) had a large effect on monthly variation of LE. Photosynthetic active radiation (PAR) and wind speed was mainly responsible for the variation of halfhourly and daily <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>, respectively. The total cloud amount was the most important factors controlling for annual total ET. The annual rainfall, water surface temperature was observed to be negatively related with annual <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/35420','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/35420"><span>LBA-ECO TG-07 Soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Flux</span> by Automated Chamber, Para, Brazil: 2001-2003</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>R.K. Varner; M.M. Keller</p> <p>2009-01-01</p> <p>Measurements of the soil-atmosphere <span class="hlt">flux</span> of <span class="hlt">CO</span><span class="hlt">2</span> were made at the km 67 <span class="hlt">flux</span> tower site in the Tapajos National Forest, Santarem, Para, Brazil. Eight chambers were set up to measure trace gas exchange between the soil and atmosphere about 5 times a day (during daylight and night) at this undisturbed forest site from April 2001 to April 2003. <span class="hlt">CO</span><span class="hlt">2</span> soil efflux data are...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.B11F0421L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.B11F0421L"><span>Carbon dioxide(<span class="hlt">CO</span><span class="hlt">2</span>) and nitrous oxide (N<span class="hlt">2</span>O) <span class="hlt">fluxes</span> in an agro-ecosystems under changing physical and biological conditions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liang, L.; Eberwein, J.; Oikawa, P.; Jenerette, D.; Grantz, D. A.</p> <p>2013-12-01</p> <p>Liyin Liang1, Jennifer Eberwein1, Patty Oikawa1, Darrel Jenerette1, David Grantz1 1Department of Botany and Plant Sciences, University of California, Riverside, CA 92521, USA Carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) and nitrous oxide (N<span class="hlt">2</span>O) are the major greenhouse gases and together produce a strong positive radiative forcing in the atmosphere. The <span class="hlt">fluxes</span> of <span class="hlt">CO</span><span class="hlt">2</span> and N<span class="hlt">2</span>O from soil to atmosphere vary with physical and biological factors, e.g., temperature, soil moisture, pH value, soil organic carbon contents, microorganism communities and so on. Understanding the interactions among these factors is critical to estimation of <span class="hlt">CO</span><span class="hlt">2</span> and N<span class="hlt">2</span>O emissions. We investigate these <span class="hlt">fluxes</span> in an extreme production environment with very high maximum temperatures, at the agricultural experiment station of University of California-Desert Research Center in the Imperial Valley of southern California. In this research, we measured the <span class="hlt">CO</span><span class="hlt">2</span> and N<span class="hlt">2</span>O <span class="hlt">fluxes</span> from soil incubation under controlled laboratory conditions, in surface chambers under field conditions and by eddy covariance. We explore the variation of <span class="hlt">CO</span><span class="hlt">2</span> and N<span class="hlt">2</span>O <span class="hlt">fluxes</span> and relationship between them in this extreme biofuel production environment. The discrete chamber measurements showed that the N<span class="hlt">2</span>O <span class="hlt">flux</span> in our field sites is <span class="hlt">2</span>.39×0.70 μg N m-<span class="hlt">2</span> hr-1, with a 95% confidence interval (CI) from 0.86 to 3.92 μg N m-<span class="hlt">2</span> hr-1. Compared to the previous reported value (0.45~26.26 μg N m-<span class="hlt">2</span> hr-1) of N<span class="hlt">2</span>O <span class="hlt">flux</span> in California, the N<span class="hlt">2</span>O <span class="hlt">flux</span> from biofuel crop land is in the lower level, although more observations should be took to confirm it. The N<span class="hlt">2</span>O <span class="hlt">flux</span> also shows very high variability within a field of biomass Sorghum, ranging from 0.40 to 8.19 μg N m-<span class="hlt">2</span> hr-1 across 11 sites owning to the high variability of physical and biological factors. Soil incubation measurements will be conducted to identify the sources of this variability. The eddy covariance measurements will allow calculation of the <span class="hlt">CO</span><span class="hlt">2</span> and N<span class="hlt">2</span>O emissions at the ecosystem level as a step in quantifying</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2010-03-23/pdf/2010-6303.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2010-03-23/pdf/2010-6303.pdf"><span>75 FR 13803 - <span class="hlt">SeaCo</span> Ltd.; Notice of Application</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2010-03-23</p> <p>...] <span class="hlt">SeaCo</span> Ltd.; Notice of Application March 17, 2010. AGENCY: Securities and Exchange Commission... (``Act''). SUMMARY: Summary of Application: <span class="hlt">SeaCo</span> Ltd. (``<span class="hlt">SeaCo</span>'') seeks an order under section 3(b)(<span class="hlt">2</span>..., reinvesting, owning, holding or trading in securities. <span class="hlt">SeaCo</span> is primarily engaged in the shipping container...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25207956','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25207956"><span>Reducing the cost of Ca-based direct <span class="hlt">air</span> capture of <span class="hlt">CO</span><span class="hlt">2</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zeman, Frank</p> <p>2014-10-07</p> <p>Direct <span class="hlt">air</span> capture, the chemical removal of <span class="hlt">CO</span><span class="hlt">2</span> directly from the atmosphere, may play a role in mitigating future climate risk or form the basis of a sustainable transportation infrastructure. The current discussion is centered on the estimated cost of the technology and its link to "overshoot" trajectories, where atmospheric <span class="hlt">CO</span><span class="hlt">2</span> levels are actively reduced later in the century. The American Physical Society (APS) published a report, later updated, estimating the cost of a one million tonne <span class="hlt">CO</span><span class="hlt">2</span> per year <span class="hlt">air</span> capture facility constructed today that highlights several fundamental concepts of chemical <span class="hlt">air</span> capture. These fundamentals are viewed through the lens of a chemical process that cycles between removing <span class="hlt">CO</span><span class="hlt">2</span> from the <span class="hlt">air</span> and releasing the absorbed <span class="hlt">CO</span><span class="hlt">2</span> in concentrated form. This work builds on the APS report to investigate the effect of modifications to the <span class="hlt">air</span> capture system based on suggestions in the report and subsequent publications. The work shows that reduced carbon electricity and plastic packing materials (for the contactor) may have significant effects on the overall price, reducing the APS estimate from $610 to $309/t<span class="hlt">CO</span><span class="hlt">2</span> avoided. Such a reduction does not challenge postcombustion capture from point sources, estimated at $80/t<span class="hlt">CO</span><span class="hlt">2</span>, but does make <span class="hlt">air</span> capture a feasible alternative for the transportation sector and a potential negative emissions technology. Furthermore, <span class="hlt">air</span> capture represents atmospheric reductions rather than simply avoided emissions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23504873','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23504873"><span>Tidal marsh plant responses to elevated <span class="hlt">CO</span><span class="hlt">2</span> , nitrogen fertilization, and <span class="hlt">sea</span> level rise.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Adam Langley, J; Mozdzer, Thomas J; Shepard, Katherine A; Hagerty, Shannon B; Patrick Megonigal, J</p> <p>2013-05-01</p> <p>Elevated <span class="hlt">CO</span><span class="hlt">2</span> and nitrogen (N) addition directly affect plant productivity and the mechanisms that allow tidal marshes to maintain a constant elevation relative to <span class="hlt">sea</span> level, but it remains unknown how these global change drivers modify marsh plant response to <span class="hlt">sea</span> level rise. Here we manipulated factorial combinations of <span class="hlt">CO</span><span class="hlt">2</span> concentration (two levels), N availability (two levels) and relative <span class="hlt">sea</span> level (six levels) using in situ mesocosms containing a tidal marsh community composed of a sedge, Schoenoplectus americanus, and a grass, Spartina patens. Our objective is to determine, if elevated <span class="hlt">CO</span><span class="hlt">2</span> and N alter the growth and persistence of these plants in coastal ecosystems facing rising <span class="hlt">sea</span> levels. After two growing seasons, we found that N addition enhanced plant growth particularly at <span class="hlt">sea</span> levels where plants were most stressed by flooding (114% stimulation in the + 10 cm treatment), and N effects were generally larger in combination with elevated <span class="hlt">CO</span><span class="hlt">2</span> (288% stimulation). N fertilization shifted the optimal productivity of S. patens to a higher <span class="hlt">sea</span> level, but did not confer S. patens an enhanced ability to tolerate <span class="hlt">sea</span> level rise. S. americanus responded strongly to N only in the higher <span class="hlt">sea</span> level treatments that excluded S. patens. Interestingly, addition of N, which has been suggested to accelerate marsh loss, may afford some marsh plants, such as the widespread sedge, S. americanus, the enhanced ability to tolerate inundation. However, if chronic N pollution reduces the availability of propagules of S. americanus or other flood-tolerant species on the landscape scale, this shift in species dominance could render tidal marshes more susceptible to marsh collapse. © 2013 Blackwell Publishing Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C13C0833H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C13C0833H"><span>A New Fast, Reliable Technique for the Sampling of Dissolved Inorganic Carbon in <span class="hlt">Sea</span> Ice</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hu, Y.; Wang, F.; Rysgaard, S.; Barber, D. G.</p> <p>2015-12-01</p> <p>For a long time, <span class="hlt">sea</span> ice was considered to act as a lid over seawater preventing <span class="hlt">CO</span><span class="hlt">2</span> exchange between the atmosphere and ocean. Recent observations suggest that <span class="hlt">sea</span> ice can be an active source or a sink for <span class="hlt">CO</span><span class="hlt">2</span>, although its magnitude is not very clear. The direct measurements on <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> based on the chamber method and eddy covariance often do not agree with each other. It is therefore important to measure the dissolved inorganic carbon (DIC) stock in <span class="hlt">sea</span> ice precisely in order to better understand the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> through <span class="hlt">sea</span> ice. The challenges in <span class="hlt">sea</span> ice DIC sampling is how to melt the ice core without being exposed to the <span class="hlt">air</span> gaining or losing <span class="hlt">CO</span><span class="hlt">2</span>. A common practice is to seal the ice core in a self-prepared gas-tight plastic bag and suck the <span class="hlt">air</span> out of the bag gently using a syringe (together with a needle) through a valve mounted on one side of the bag. However, this method is time consuming (takes up to several minutes to suck the <span class="hlt">air</span> out) and very often there is large headspace found in the bag after the ice melts due to the imperfect bag-preparation, which might affect the DIC concentration in melt ice-water. We developed a new technique by using a commercially available plastic bag with a vacuum sealer to seal the ice core. In comparison to syringe-based method, this technique is fast and easy to operate; it takes less than 10 seconds to vacuum and seal the bag all in one button with no headspace left in the bag. Experimental tests with replicate ice cores sealed by those two methods showed that there is no difference in the DIC concentration measured after these two methods, suggesting that there is no loss of DIC during the course of vacuum sealing. In addition, a time series experiment on DIC in melt ice-water stored in the new bag shows that when the samples were not poisoned, the DIC concentration remains unchanged for at least 3 days in the bag; while poisoned by HgCl<span class="hlt">2</span>, there is no change in DIC for at least 21 days, indicating that this new bag is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.B41D0082M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.B41D0082M"><span>Annual Greenhouse Gas (<span class="hlt">CO</span><span class="hlt">2</span>, CH4, and N<span class="hlt">2</span>O) <span class="hlt">Fluxes</span> Via Ebullition from a Temperate Emergent Wetland</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mcnicol, G.; Sturtevant, C. S.; Knox, S. H.; Baldocchi, D. D.; Silver, W. L.</p> <p>2014-12-01</p> <p>Quantifying wetland greenhouse gas exchange is necessary to evaluate their potential for mitigating climate change via carbon sequestration. However measuring greenhouse gas <span class="hlt">fluxes</span> of carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>), methane (CH4), and nitrous oxide (N<span class="hlt">2</span>O) in wetlands is difficult due to high spatial and temporal variability, and multiple transport pathways of emission. Transport of biogenic soil gas via highly sporadic ebullition (bubbling) events is often ignored or quantified poorly in wetland greenhouse gas budgets, but can rapidly release large volumes of gas to the atmosphere. To quantify a robust annual ebullition <span class="hlt">flux</span> we measured rates continuously for a year (2013-2014) using custom-built chambers deployed in a restored emergent wetland located in the Sacramento-San Joaquin Delta, CA. We combined ebullition <span class="hlt">flux</span> rates with observations of gas concentrations to estimate annual ebullition emissions of <span class="hlt">CO</span><span class="hlt">2</span>, CH4, and N<span class="hlt">2</span>O and compare <span class="hlt">flux</span> rates to whole-ecosystem exchange of <span class="hlt">CO</span><span class="hlt">2</span> and CH4 measured simultaneously by eddy covariance.Mean ebullition <span class="hlt">flux</span> rates were 18.3 ± 5.6 L m-<span class="hlt">2</span> yr-1. Ebullition CH4 concentrations were very high and ranged from 23-76 % with a mean of 47 ± <span class="hlt">2</span>.9 %; <span class="hlt">CO</span><span class="hlt">2</span> concentrations were lower and ranged from 0.7-6.6 % with a mean of <span class="hlt">2</span>.8 ± 0.3 %; N<span class="hlt">2</span>O concentrations were below atmospheric concentrations and ranged from 130-389 ppb(v) with a mean of 257 ± 13 ppb(v). We calculated well-constrained annual ebullition <span class="hlt">fluxes</span> of: 6.<span class="hlt">2</span> ± 1.9 g CH4 m-<span class="hlt">2</span> yr-1, 1.0 ± 0.3 g <span class="hlt">CO</span><span class="hlt">2</span> m-<span class="hlt">2</span> yr-1 and 9.3 ± <span class="hlt">2</span>.8 mg N<span class="hlt">2</span>O m-<span class="hlt">2</span> yr-1. Methane emissions via ebullition were very large, representing 15-25 % of total wetland CH4 emissions measured at this site, whereas ebullition released only relatively small quantities of <span class="hlt">CO</span><span class="hlt">2</span> and N<span class="hlt">2</span>O. Our results demonstrate that large releases of CH4 via ebullition from open water surfaces can be a significant component of restored wetland greenhouse gas budgets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013ACPD...13.2243C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013ACPD...13.2243C"><span>Improved simulation of group averaged <span class="hlt">CO</span><span class="hlt">2</span> surface concentrations using GEOS-Chem and <span class="hlt">fluxes</span> from VEGAS</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, Z. H.; Zhu, J.; Zeng, N.</p> <p>2013-01-01</p> <p><span class="hlt">CO</span><span class="hlt">2</span> measurements have been combined with simulated <span class="hlt">CO</span><span class="hlt">2</span> distributions from a transport model in order to produce the optimal estimates of <span class="hlt">CO</span><span class="hlt">2</span> surface <span class="hlt">fluxes</span> in inverse modeling. However one persistent problem in using model-observation comparisons for this goal relates to the issue of compatibility. Observations at a single site reflect all underlying processes of various scales that usually cannot be fully resolved by model simulations at the grid points nearest the site due to lack of spatial or temporal resolution or missing processes in models. In this article we group site observations of multiple stations according to atmospheric mixing regimes and surface characteristics. The group averaged values of <span class="hlt">CO</span><span class="hlt">2</span> concentration from model simulations and observations are used to evaluate the regional model results. Using the group averaged measurements of <span class="hlt">CO</span><span class="hlt">2</span> reduces the noise of individual stations. The difference of group averaged values between observation and modeled results reflects the uncertainties of the large scale <span class="hlt">flux</span> in the region where the grouped stations are. We compared the group averaged values between model results with two biospheric <span class="hlt">fluxes</span> from the model Carnegie-Ames-Stanford-Approach (CASA) and VEgetation-Global-Atmosphere-Soil (VEGAS) and observations to evaluate the regional model results. Results show that the modeling group averaged values of <span class="hlt">CO</span><span class="hlt">2</span> concentrations in all regions with <span class="hlt">fluxes</span> from VEGAS have significant improvements for most regions. There is still large difference between two model results and observations for grouped average values in North Atlantic, Indian Ocean, and South Pacific Tropics. This implies possible large uncertainties in the <span class="hlt">fluxes</span> there.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E%26PSL.488...36L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26PSL.488...36L"><span>Precession and atmospheric <span class="hlt">CO</span><span class="hlt">2</span> modulated variability of <span class="hlt">sea</span> ice in the central Okhotsk <span class="hlt">Sea</span> since 130,000 years ago</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lo, Li; Belt, Simon T.; Lattaud, Julie; Friedrich, Tobias; Zeeden, Christian; Schouten, Stefan; Smik, Lukas; Timmermann, Axel; Cabedo-Sanz, Patricia; Huang, Jyh-Jaan; Zhou, Liping; Ou, Tsong-Hua; Chang, Yuan-Pin; Wang, Liang-Chi; Chou, Yu-Min; Shen, Chuan-Chou; Chen, Min-Te; Wei, Kuo-Yen; Song, Sheng-Rong; Fang, Tien-Hsi; Gorbarenko, Sergey A.; Wang, Wei-Lung; Lee, Teh-Quei; Elderfield, Henry; Hodell, David A.</p> <p>2018-04-01</p> <p>Recent reduction in high-latitude <span class="hlt">sea</span> ice extent demonstrates that <span class="hlt">sea</span> ice is highly sensitive to external and internal radiative forcings. In order to better understand <span class="hlt">sea</span> ice system responses to external orbital forcing and internal oscillations on orbital timescales, here we reconstruct changes in <span class="hlt">sea</span> ice extent and summer <span class="hlt">sea</span> surface temperature (SSST) over the past 130,000 yrs in the central Okhotsk <span class="hlt">Sea</span>. We applied novel organic geochemical proxies of <span class="hlt">sea</span> ice (IP25), SSST (TEX86L) and open water marine productivity (a tri-unsaturated highly branched isoprenoid and biogenic opal) to marine sediment core MD01-2414 (53°11.77‧N, 149°34.80‧E, water depth 1123 m). To complement the proxy data, we also carried out transient Earth system model simulations and sensitivity tests to identify contributions of different climatic forcing factors. Our results show that the central Okhotsk <span class="hlt">Sea</span> was ice-free during Marine Isotope Stage (MIS) 5e and the early-mid Holocene, but experienced variable <span class="hlt">sea</span> ice cover during MIS <span class="hlt">2</span>-4, consistent with intervals of relatively high and low SSST, respectively. Our data also show that the <span class="hlt">sea</span> ice extent was governed by precession-dominated insolation changes during intervals of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentrations ranging from 190 to 260 ppm. However, the proxy record and the model simulation data show that the central Okhotsk <span class="hlt">Sea</span> was near ice-free regardless of insolation forcing throughout the penultimate interglacial, and during the Holocene, when atmospheric <span class="hlt">CO</span><span class="hlt">2</span> was above ∼260 ppm. Past <span class="hlt">sea</span> ice conditions in the central Okhotsk <span class="hlt">Sea</span> were therefore strongly modulated by both orbital-driven insolation and <span class="hlt">CO</span><span class="hlt">2</span>-induced radiative forcing during the past glacial/interglacial cycle.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.B42C..03H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.B42C..03H"><span>Response of surface CH4 and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> to whole ecosystem warming and elevated <span class="hlt">CO</span><span class="hlt">2</span> in a boreal black spruce peatland, northern Minnesota</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hsieh, I. F.; Gill, A. L.; Finzi, A.</p> <p>2017-12-01</p> <p>Potential increase in peatland C losses by environmental change has been presented by impacting the balance of <span class="hlt">CO</span><span class="hlt">2</span> and CH4 sequestration and release. While temperature warming may accelerate the temperature-sensitive processes and release <span class="hlt">CO</span><span class="hlt">2</span> and CH4 from peat C stores, factors associated with warming and that associated with elevated <span class="hlt">CO</span><span class="hlt">2</span> concentration may alter the intrinsic characteristics of <span class="hlt">CO</span><span class="hlt">2</span> and CH4 emission from peatland. By leveraging Spruce and Peatland Responses Under Changing Environments (SPRUCE) experiment, we measured peat surface <span class="hlt">CO</span><span class="hlt">2</span> and CH4 <span class="hlt">fluxes</span> and their i13C signatures across a gradient of warming temperatures in a boreal black spruce peat bog in 2015 and 2016 growing seasons. Elevated <span class="hlt">CO</span><span class="hlt">2</span> (e<span class="hlt">CO</span><span class="hlt">2</span>) treatment was added to the warming experiment in June, 2016. Our results show both CH4 and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> increased with warming temperature in the two-year measurement period. Total emission for both gases were higher in 2016 with whole ecosystem warming than that in 2015 with deep peat heat warming. The 2016 increase in <span class="hlt">CO</span><span class="hlt">2</span> emission was significantly larger in the hummock microtopographic position compared to hollows. The opposite was true for CH4 <span class="hlt">fluxes</span>, where the increase was strongest in the hollows. In fact, CH4 <span class="hlt">flux</span> from hummocks declined in 2016 compared to 2015, suggesting lower overall rates of CH4 production and/or greater rates of methanotrophy. The increase (less depleted) in i13C -CH4 signatures suggest acetoclastic methanogensis increased its contribution to total CH4 production across the growing season and in response to experimental warming, while hydrogenotrophic methanogenesis dominated total CH4 production. On the contrary, results of i13C-<span class="hlt">CO</span><span class="hlt">2</span> show no significant change in the contribution of different sources to total <span class="hlt">CO</span><span class="hlt">2</span> emission through time or across warming temperature. On the other hand, i13C-<span class="hlt">CO</span><span class="hlt">2</span> signatures under <span class="hlt">CO</span><span class="hlt">2</span> fumigation in 2016 was significantly depleted since the e<span class="hlt">CO</span><span class="hlt">2</span> initiation, indicating a rapid increase in plant</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20010022518','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20010022518"><span>BOREAS TGB-5 <span class="hlt">CO</span><span class="hlt">2</span>, CH4 and <span class="hlt">CO</span> Chamber <span class="hlt">Flux</span> Data Over the NSA</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Burke, Roger; Hall, Forrest G. (Editor); Conrad, Sara K. (Editor); Zepp, Richard</p> <p>2000-01-01</p> <p>The BOReal Ecosystem-Atmosphere Study Trace Gas Biogeochemistry (BOREAS TGB-5) team collected a variety of trace gas concentration and <span class="hlt">flux</span> measurements at several NSA sites. This data set contains carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>), methane (CH4), and carbon monoxide (<span class="hlt">CO</span>) chamber <span class="hlt">flux</span> measurements conducted in 1994 at upland forest sites that experienced stand-replacement fires. These measurements were acquired to understand the impact of fires on soil biogeochemistry and related changes in trace gas exchange in boreal forest soils. Relevant ancillary data, including data concerning the soil temperature, solar irradiance, and information from nearby un-burned control sites, are included to provide a basis for modeling the regional impacts of fire and climate changes on trace gas biogeochemistry. The data are provided in tabular ASCII files.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.B43E2180T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.B43E2180T"><span><span class="hlt">CO</span><span class="hlt">2</span> and CH4 <span class="hlt">fluxes</span> in a Spartina salt marsh and brackish Phragmites marsh in Massachusetts</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tang, J.; Wang, F.; Kroeger, K. D.; Gonneea, M. E.</p> <p>2017-12-01</p> <p>Coastal salt marshes play an important role in global and regional carbon cycling. Tidally restricted marshes reduce salinity and provide a habitat suitable for Phragmites invasion. We measured greenhouse gas (GHG) emissions (<span class="hlt">CO</span><span class="hlt">2</span> and CH4) continuously with the eddy covariance method and biweekly with the static chamber method in a Spartina salt marsh and a Phragmites marsh on Cape Cod, Massachusetts, USA. We did not find significant difference in <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> between the two sites, but the CH4 <span class="hlt">fluxes</span> were much higher in the Phragmites site than the Spartina marsh. Temporally, tidal cycles influence the <span class="hlt">CO</span><span class="hlt">2</span> and CH4 <span class="hlt">fluxes</span> in both sites. We found that the salt marsh was a significant carbon sink when <span class="hlt">CO</span><span class="hlt">2</span> and CH4 <span class="hlt">fluxes</span> were combined. Restoring tidally restricted marshes will significantly reduce CH4 emissions and provide a strong ecosystem carbon service.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006JCrGr.289..605W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006JCrGr.289..605W"><span><span class="hlt">Flux</span> growth of high-quality <span class="hlt">Co</span>Fe <span class="hlt">2</span>O 4 single crystals and their characterization</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, W. H.; Ren, X.</p> <p>2006-04-01</p> <p>We report the growth of high-quality <span class="hlt">Co</span>Fe <span class="hlt">2</span>O 4 single crystals using a borax <span class="hlt">flux</span> method. The crystals were characterized by powder X-ray diffraction, electron probe microanalysis and Raman spectroscopy. We found the crystals are <span class="hlt">flux</span>-free and highly homogeneous in composition. X-ray rocking curves of the <span class="hlt">Co</span>Fe <span class="hlt">2</span>O 4 single crystals showed a full-width at half-maximum of 0.15°. The saturation magnetization of the <span class="hlt">Co</span>Fe <span class="hlt">2</span>O 4 single crystals was measured to be 90 emu/g or equivalently 3.65 μ B/f.u. at 5 K.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.B51I1941B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.B51I1941B"><span>A Spatial-Temporal Comparison of Lake Mendota <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Fluxes</span> and Collection Methods</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Baldocchi, A. K.; Reed, D. E.; Desai, A. R.; Loken, L. C.; Schramm, P.; Stanley, E. H.</p> <p>2017-12-01</p> <p>Monitoring of carbon <span class="hlt">fluxes</span> at the lake/atmosphere interface can help us determine baselines from which to understand responses in both space and time that may result from our warming climate or increasing nutrient inputs. Since recent research has shown lakes to be hotspots of global carbon cycling, it is important to quantify carbon sink and source dynamics as well as to verify observations between multiple methods in the context of long-term data collection efforts. Here we evaluate a new method for measuring space and time variation in <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> based on novel speedboat-based collection method of aquatic greenhouse gas concentrations and a <span class="hlt">flux</span> computation and interpolation algorithm. Two-hundred and forty-nine consecutive days of spatial <span class="hlt">flux</span> maps over the 2016 open ice period were compared to ongoing eddy covariance tower <span class="hlt">flux</span> measurements on the shore of Lake Mendota, Wisconsin US using a <span class="hlt">flux</span> footprint analysis. Spatial and temporal alignments of the <span class="hlt">fluxes</span> from these two observational datasets revealed both similar trends from daily to seasonal timescales as well as biases between methods. For example, throughout the Spring carbon <span class="hlt">fluxes</span> showed strong correlation although off by an order of magnitude. Isolating physical patterns of agreement between the two methods of the lake/atmosphere <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> allows us to pinpoint where biology and physical drivers contribute to the global carbon cycle and help improve modelling of lakes and utilize lakes as leading indicators of climate change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017APS..DFDL20011S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..DFDL20011S"><span>Boundary layers at a dynamic interface: <span class="hlt">air-sea</span> exchange of heat and mass</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Szeri, Andrew</p> <p>2017-11-01</p> <p>Exchange of mass or heat across a turbulent liquid-gas interface is a problem of critical interest, especially in <span class="hlt">air-sea</span> transfer of natural and man-made gases involved in climate change. The goal in this research area is to determine the gas <span class="hlt">flux</span> from <span class="hlt">air</span> to <span class="hlt">sea</span> or vice versa. For sparingly soluble non-reactive gases, this is controlled by liquid phase turbulent velocity fluctuations that act on the thin species concentration boundary layer on the liquid side of the interface. If the fluctuations in surface-normal velocity and gas concentration differences are known, then it is possible to determine the turbulent contribution to the gas <span class="hlt">flux</span>. However, there is no suitable fundamental direct approach in the general case where neither of these quantities can be easily measured. A new approach is presented to deduce key aspects about the near-surface turbulent motions from remote measurements, which allows one to determine the gas transfer velocity, or gas <span class="hlt">flux</span> per unit area if overall concentration differences are known. The approach is illustrated with conceptual examples.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23636599','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23636599"><span>Neutral poly- and perfluoroalkyl substances in <span class="hlt">air</span> and seawater of the North <span class="hlt">Sea</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Xie, Zhiyong; Zhao, Zhen; Möller, Axel; Wolschke, Hendrik; Ahrens, Lutz; Sturm, Renate; Ebinghaus, Ralf</p> <p>2013-11-01</p> <p>Concentrations of neutral poly- and perfluoroalkyl substances (PFASs), such as fluorotelomer alcohols (FTOHs), perfluoroalkane sulfonamides (FASAs), perfluoroalkane sufonamidoethanols (FASEs), and fluorotelomer acrylates (FTACs), have been simultaneously determined in surface seawater and the atmosphere of the North <span class="hlt">Sea</span>. Seawater and <span class="hlt">air</span> samples were taken aboard the German research vessel Heincke on the cruise 303 from 15 to 24 May 2009. The concentrations of FTOHs, FASAs, FASEs, and FTACs in the dissolved phase were <span class="hlt">2</span>.6-74, <0.1-19, <0.1-63, and <1.0-9.0 pg L(-1), respectively. The highest concentrations were determined in the estuary of the Weser and Elbe rivers and a decreasing concentration profile appeared with increasing distance from the coast toward the central part of the North <span class="hlt">Sea</span>. Gaseous FTOHs, FASAs, FASEs, and FTACs were in the range of 36-126, 3.1-26, 3.7-19, and 0.8-5.6 pg m(-3), which were consistent with the concentrations determined in 2007 in the North <span class="hlt">Sea</span>, and approximately five times lower than those reported for an urban area of Northern Germany. These results suggested continuous continental emissions of neutral PFASs followed by transport toward the marine environment. <span class="hlt">Air</span>-seawater gas exchanges of neutral PFASs were estimated using fugacity ratios and the two-film resistance model based upon paired <span class="hlt">air</span>-seawater concentrations and estimated Henry's law constant values. Volatilization dominated for all neutral PFASs in the North <span class="hlt">Sea</span>. The <span class="hlt">air</span>-seawater gas exchange <span class="hlt">fluxes</span> were in the range of <span class="hlt">2</span>.5×10(3)-3.6×10(5) pg m(-<span class="hlt">2</span>) for FTOHs, 1.8×10(<span class="hlt">2</span>)-1.0×10(5) pg m(-<span class="hlt">2</span>) for FASAs, 1.1×10(<span class="hlt">2</span>)-3.0×10(5) pg m(-<span class="hlt">2</span>) for FASEs and 6.3×10(<span class="hlt">2)-2</span>.0×10(4) pg m(-<span class="hlt">2</span>) for FTACs, respectively. These results suggest that the <span class="hlt">air</span>-seawater gas exchange is an important process that intervenes in the transport and fate for neutral PFASs in the marine environment.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_21 --> <div id="page_22" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="421"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.ars.usda.gov/research/publications/publication/?seqNo115=309452','TEKTRAN'); return false;" href="http://www.ars.usda.gov/research/publications/publication/?seqNo115=309452"><span>Changes in <span class="hlt">fluxes</span> of heat, H<span class="hlt">2</span>O, <span class="hlt">CO</span><span class="hlt">2</span> caused by a large wind farm</span></a></p> <p><a target="_blank" href="https://www.ars.usda.gov/research/publications/find-a-publication/">USDA-ARS?s Scientific Manuscript database</a></p> <p></p> <p></p> <p>The Crop Wind Energy Experiment (CWEX) provides a platform to investigate the effect of wind turbines and large wind farms on surface <span class="hlt">fluxes</span> of momentum, heat, moisture and carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>). In 2010 and 2011, eddy covariance <span class="hlt">flux</span> stations were installed between two lines of turbines at the south...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMIN13B0074H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMIN13B0074H"><span>Comparisons of a Quantum Annealing and Classical Computer Neural Net Approach for Inferring Global Annual <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Fluxes</span> over Land</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Halem, M.; Radov, A.; Singh, D.</p> <p>2017-12-01</p> <p>Investigations of mid to high latitude atmospheric <span class="hlt">CO</span><span class="hlt">2</span> show growing amplitudes in seasonal variations over the past several decades. Recent high-resolution satellite measurements of <span class="hlt">CO</span><span class="hlt">2</span> concentration are now available for three years from the Orbiting Carbon Observatory-<span class="hlt">2</span>. The Atmospheric Radiation Measurement (ARM) program of DOE has been making long-term <span class="hlt">CO</span><span class="hlt">2</span>-<span class="hlt">flux</span> measurements (in addition to <span class="hlt">CO</span><span class="hlt">2</span> concentration and an array of other meteorological quantities) at several towers and mobile sites located around the globe at half-hour frequencies. Recent papers have shown <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> inferred by assimilating <span class="hlt">CO</span><span class="hlt">2</span> observations into ecosystem models are largely inconsistent with station observations. An investigation of how the biosphere has reacted to changes in atmospheric <span class="hlt">CO</span><span class="hlt">2</span> is essential to our understanding of potential climate-vegetation feedbacks. Thus, new approaches for calculating <span class="hlt">CO</span><span class="hlt">2</span>-<span class="hlt">flux</span> for assimilation into land surface models are necessary for improving the prediction of annual carbon uptake. In this study, we calculate and compare the predicted <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> results employing a Feed Forward Backward Propagation Neural Network model on two architectures, (i) an IBM Minsky Computer node and (ii) a hybrid version of the ARC D-Wave quantum annealing computer. We compare the neural net results of predictions of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> from ARM station data for three different DOE ecosystem sites; an arid plains near Oklahoma City, a northern arctic site at Barrows AL, and a tropical rainforest site in the Amazon. Training times and predictive results for the calculating annual <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> for the two architectures for each of the three sites are presented. Comparative results of predictions as measured by RMSE and MAE are discussed. Plots and correlations of observed vs predicted <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> are also presented for all three sites. We show the estimated training times for quantum and classical calculations when extended to calculating global annual Carbon Uptake over land. We also</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15825257','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15825257"><span>Effects of <span class="hlt">air</span> velocity on photosynthesis of plant canopies under elevated <span class="hlt">CO</span><span class="hlt">2</span> levels in a plant culture system.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kitaya, Y; Shibuya, T; Yoshida, M; Kiyota, M</p> <p>2004-01-01</p> <p>To obtain basic data for adequate <span class="hlt">air</span> circulation for promoting plant growth in closed plant production modules in bioregenerative life support systems in space, effects of <span class="hlt">air</span> velocities ranging from 0.1 to 0.8 m s-1 on photosynthesis in tomato seedlings canopies were investigated under atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentrations of 0.4 and 0.8 mmol mol-1. The canopy of tomato seedlings on a plug tray (0.4 x 0.4 m<span class="hlt">2</span>) was set in a wind-tunnel-type chamber (0.6 x 0.4 x 0.3 m3) installed in a semi-closed-type assimilation chamber (0.9 x 0.5 x 0.4 m3). The net photosynthetic rate in the plant canopy was determined with the differences in <span class="hlt">CO</span><span class="hlt">2</span> concentrations between the inlet and outlet of the assimilation chamber multiplied by the volumetric <span class="hlt">air</span> exchange rate of the chamber. Photosynthetic photon <span class="hlt">flux</span> (PPF) on the plant canopy was kept at 0.25 mmol m-<span class="hlt">2</span> s-1, <span class="hlt">air</span> temperature at 23 degrees C and relative humidity at 55%. The leaf area indices (LAIs) of the plant canopies were 0.6-<span class="hlt">2</span>.5 and plant heights were 0.05-0.<span class="hlt">2</span> m. The net photosynthetic rate of the plant canopy increased with increasing <span class="hlt">air</span> velocities inside plant canopies and saturated at 0.<span class="hlt">2</span> m s-1. The net photosynthetic rate at the <span class="hlt">air</span> velocity of 0.4 m s-1 was 1.3 times that at 0.1 m s-1 under <span class="hlt">CO</span><span class="hlt">2</span> concentrations of 0.4 and 0.8 mmol mol-1. The net photosynthetic rate under <span class="hlt">CO</span><span class="hlt">2</span> concentrations of 0.8 mmol mol-1 was 1.<span class="hlt">2</span> times that under 0.4 mmol mol-1 at the <span class="hlt">air</span> velocity ranging from 0.1 to 0.8 m s-1. The results confirmed the importance of controlling <span class="hlt">air</span> movement for enhancing the canopy photosynthesis under an elevated <span class="hlt">CO</span><span class="hlt">2</span> level as well as under a normal <span class="hlt">CO</span><span class="hlt">2</span> level in the closed plant production modules. c2004 COSPAR. Published by Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005AGUFM.B33E1085H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005AGUFM.B33E1085H"><span>Simultaneous Micrometeorological <span class="hlt">Flux</span> Observations of <span class="hlt">CO</span><span class="hlt">2</span> and CH4 at a Sub-Arctic Black-Spruce Forest in Alaska</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Harazono, Y.; Ueyama, M.; Miyata, A.</p> <p>2005-12-01</p> <p>Carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) and methane (CH4) <span class="hlt">fluxes</span> were measured at a black spruce forest over discontinuous permafrost in central Alaska since November 2002. <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> was measured by open-path eddy correlation system and CH4 <span class="hlt">flux</span> was measured by gradient method continuously. <span class="hlt">CO</span><span class="hlt">2</span> uptake was observed during daytime after DOY 60 when the forest floor was snow-covered with low temperature (<-10 °C). At the moment, CH4 <span class="hlt">flux</span> was negative (uptake) during daytime and nearing to zero at night, which varied with surface temperature. During snow melt and following permafrost thawing periods (around DOY 110-140, 2003), nocturnal <span class="hlt">CO</span><span class="hlt">2</span> efflux was larger than daytime uptake resulted in a daily <span class="hlt">CO</span><span class="hlt">2</span> source, and CH4 <span class="hlt">flux</span> became small positive in daytime and nearing zero at night resulted in a weak daily CH4 source. After DOY 140 in 2003, <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> was strong uptake and the maximum level was 1.0 g m-<span class="hlt">2</span> h-1 in late July around 10:30h when 3 hr earlier than solar noon. During mid summer (DOY 180-230, 2003), daytime CH4 uptake was weak and was near zero at night resulted in a weak daily CH4 sink. 2004 was low snow fall and draught summer, the seasonal patterns of <span class="hlt">CO</span><span class="hlt">2</span> and CH4 <span class="hlt">fluxes</span> shifted more than 3-weeks earlier than that in 2003, resulted in high <span class="hlt">CO</span><span class="hlt">2</span> and CH4 emissions in early summer. Daily amount of CH4 <span class="hlt">flux</span> in mid summer 2003 and 2004 were 1.<span class="hlt">2</span> and 0.5 mg CH4 m-<span class="hlt">2</span> d-1, respectively. Sum of observed NEE and <span class="hlt">CO</span><span class="hlt">2</span> storage term within the canopy, NEP were -482 and -366.6 g<span class="hlt">CO</span><span class="hlt">2</span> m-<span class="hlt">2</span> y-1 in 2003 and 2004. However, application of u* filtering correction made NEP reduce to the ranges between -434.8 and -315.9 g<span class="hlt">CO</span><span class="hlt">2</span> m-<span class="hlt">2</span> y-1 (under u<0.05 ms-1 and u<0.<span class="hlt">2</span> ms-1) in 2003 and to -282.5 and -215.9 g<span class="hlt">CO</span><span class="hlt">2</span> m-<span class="hlt">2</span> y-1 in 2004. The low NEP in 2004 was caused by high temperature and low precipitation during growing season. CH4 emission was also higher in 2004. <span class="hlt">CO</span><span class="hlt">2</span> and CH4 exchanges at sub-arctic forest were quite sensitive to draught and summer temperature.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013APJAS..49..443P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013APJAS..49..443P"><span>Heat <span class="hlt">flux</span> variations over <span class="hlt">sea</span> ice observed at the coastal area of the Sejong Station, Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Park, Sang-Jong; Choi, Tae-Jin; Kim, Seong-Joong</p> <p>2013-08-01</p> <p>This study presents variations of sensible heat <span class="hlt">flux</span> and latent heat <span class="hlt">flux</span> over <span class="hlt">sea</span> ice observed in 2011 from the 10-m <span class="hlt">flux</span> tower located at the coast of the Sejong Station on King George Island, Antarctica. A period from July to September was selected as a <span class="hlt">sea</span> ice period based on daily record of <span class="hlt">sea</span> state and hourly photos looking at the Marian Cove in front of the Sejong Station. For the <span class="hlt">sea</span> ice period, mean sensible heat <span class="hlt">flux</span> is about -11 Wm-<span class="hlt">2</span>, latent heat <span class="hlt">flux</span> is about +<span class="hlt">2</span> W m-<span class="hlt">2</span>, net radiation is -12 W m-<span class="hlt">2</span>, and residual energy is -3 W m-<span class="hlt">2</span> with clear diurnal variations. Estimated mean values of surface exchange coefficients for momentum, heat and moisture are 5.15 × 10-3, 1.19 × 10-3, and 1.87 × 10-3, respectively. The observed exchange coefficients of heat shows clear diurnal variations while those of momentum and moisture do not show diurnal variation. The parameterized exchange coefficients of heat and moisture produces heat <span class="hlt">fluxes</span> which compare well with the observed diurnal variations of heat <span class="hlt">fluxes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeCoA.207...43G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeCoA.207...43G"><span>Continuous <span class="hlt">CO</span><span class="hlt">2</span> escape from the hypersaline Dead <span class="hlt">Sea</span> caused by aragonite precipitation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Golan, Rotem; Lazar, Boaz; Wurgaft, Eyal; Lensky, Nadav; Ganor, Jiwchar; Gavrieli, Ittai</p> <p>2017-06-01</p> <p>Chemical precipitation of Ca<span class="hlt">CO</span>3 occurs in diverse marine and lacustrine environments. In the hypersaline Ca-chloride lakes that have been occupying the Dead <span class="hlt">Sea</span> basin since the late Pleistocene, Ca<span class="hlt">CO</span>3 precipitated, mostly as aragonite. The aragonite sediments precipitated mainly during periods of high lake level stands as a result of mixing of bicarbonate-rich freshwater runoff with Dead <span class="hlt">Sea</span> brine, that is Ca-rich and have high Mg/Ca ratio. During periods of arid conditions with limited freshwater inflow, water level declined, salinity increased and gypsum and halite became the dominant evaporitic minerals to precipitate. The present study investigates the carbon cycle of the Dead <span class="hlt">Sea</span> under the current limited water and bicarbonate supply to the brine, representing periods of extremely arid conditions. The decrease of inflows to the Dead <span class="hlt">Sea</span> in recent years stems mainly from diversion of freshwater from the drainage basin and results in dramatic water level decline and massive halite precipitation. During 2013-2014, bi-monthly depth profiles of total alkalinity, dissolved inorganic carbon (DIC) and its isotopic composition (δ13C) were conducted in the Dead <span class="hlt">Sea</span>, from surface down to the bottom of the lake (290 m). Mass balance calculations conducted for the period 1993-2013 show that while inventories of conservative ions such as Mg<span class="hlt">2</span>+ remained constant, the net DIC inventory of the lake decreased by ∼10%. DIC supply to the lake during this period, however, amounted to ∼10% of lake's inventory indicating that during 20 years, the lake lost ∼20% of its 1993s inventory. Compilation of historical data with our data shows that during the past two decades the lake's low DIC (∼1 mmol kg-1) and very high PCO<span class="hlt">2</span> (1800 ppm V) remained relatively constant, suggesting that a quasi-steady-state situation prevails. In spite of the surprisingly stable DIC and <span class="hlt">CO</span><span class="hlt">2</span> concentrations, during this 20 year period δ13CDIC increased significantly, from 1.4‰ to <span class="hlt">2</span>.7‰. An isotopic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001asi..book.....C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001asi..book.....C"><span><span class="hlt">Air-Sea</span> Interaction</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Csanady, G. T.</p> <p>2001-03-01</p> <p>In recent years <span class="hlt">air-sea</span> interaction has emerged as a subject in its own right, encompassing small-scale and large-scale processes in both <span class="hlt">air</span> and <span class="hlt">sea</span>. <span class="hlt">Air-Sea</span> Interaction: Laws and Mechanisms is a comprehensive account of how the atmosphere and the ocean interact to control the global climate, what physical laws govern this interaction, and its prominent mechanisms. The topics covered range from evaporation in the oceans, to hurricanes, and on to poleward heat transport by the oceans. By developing the subject from basic physical (thermodynamic) principles, the book is accessible to graduate students and research scientists in meteorology, oceanography, and environmental engineering. It will also be of interest to the broader physics community involved in the treatment of transfer laws, and thermodynamics of the atmosphere and ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28841262','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28841262"><span>Measuring 13 C-enriched <span class="hlt">CO</span><span class="hlt">2</span> in <span class="hlt">air</span> with a cavity ring-down spectroscopy gas analyser: Evaluation and calibration.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Dickinson, Dane; Bodé, Samuel; Boeckx, Pascal</p> <p>2017-11-30</p> <p>Cavity ring-down spectroscopy (CRDS) is becoming increasingly popular for δ 13 C-<span class="hlt">CO</span> <span class="hlt">2</span> analysis of <span class="hlt">air</span>. However, little is known about the effect of high 13 C abundances on the performance of CRDS. Overlap between 12 <span class="hlt">CO</span> <span class="hlt">2</span> and 13 <span class="hlt">CO</span> <span class="hlt">2</span> spectral lines may adversely affect isotopic-<span class="hlt">CO</span> <span class="hlt">2</span> CRDS measurements of 13 C-enriched samples. Resolving this issue is important so that CRDS analysers can be used in <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">flux</span> studies involving 13 C-labelled tracers. We tested a Picarro G2131-i CRDS isotopic-<span class="hlt">CO</span> <span class="hlt">2</span> gas analyser with specialty gravimetric standards of widely varying 13 C abundance (from natural to 20.1 atom%) and <span class="hlt">CO</span> <span class="hlt">2</span> mole fraction (x<span class="hlt">CO</span> <span class="hlt">2</span> : <0.1 to 2116 ppm) in synthetic <span class="hlt">air</span>. The presence of spectroscopic interference between 12 <span class="hlt">CO</span> <span class="hlt">2</span> and 13 <span class="hlt">CO</span> <span class="hlt">2</span> bands was assessed by analysing errors in measurements of the standards. A multi-component calibration strategy was adopted, incorporating isotope ratio and mole fraction data to ensure accuracy and consistency in corrected values of δ 13 C-<span class="hlt">CO</span> <span class="hlt">2</span> , x 12 <span class="hlt">CO</span> <span class="hlt">2</span> , and x 13 <span class="hlt">CO</span> <span class="hlt">2</span> . CRDS measurements of x 13 <span class="hlt">CO</span> <span class="hlt">2</span> were found to be accurate throughout the tested range (<0.005 to 100 ppm). On the other hand, spectral cross-talk in x 12 <span class="hlt">CO</span> <span class="hlt">2</span> measurements of standards containing elevated levels of 13 <span class="hlt">CO</span> <span class="hlt">2</span> led to inaccuracy in x 12 <span class="hlt">CO</span> <span class="hlt">2</span> , total-x<span class="hlt">CO</span> <span class="hlt">2</span> (x 12 <span class="hlt">CO</span> <span class="hlt">2</span>  + x 13 <span class="hlt">CO</span> <span class="hlt">2</span> ), and δ 13 C-<span class="hlt">CO</span> <span class="hlt">2</span> data. An empirical relationship for x 12 <span class="hlt">CO</span> <span class="hlt">2</span> measurements that incorporated the 13 C/ 12 C isotope ratio (i.e. 13 <span class="hlt">CO</span> <span class="hlt">2</span> / 12 <span class="hlt">CO</span> <span class="hlt">2</span> , RCO<span class="hlt">2</span>) as a secondary (non-linear) variable was found to compensate for the perturbations, and enabled accurate instrument calibration for all <span class="hlt">CO</span> <span class="hlt">2</span> compositions covered by our standard gases. 13 C-enrichement in <span class="hlt">CO</span> <span class="hlt">2</span> leads to minor errors in CRDS measurements of x 12 <span class="hlt">CO</span> <span class="hlt">2</span> . We propose an empirical correction for measurements of 13 C-enriched <span class="hlt">CO</span> <span class="hlt">2</span> in <span class="hlt">air</span> by CRDS instruments such as the Picarro G2131-i. Copyright © 2017 John Wiley & Sons, Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1910783S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1910783S"><span>Estimation of the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> between the ocean and atmosphere for the hurricane wind forces using remote sensing data.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sergeev, Daniil; Soustova, Irina; Balandina, Galina</p> <p>2017-04-01</p> <p><span class="hlt">CO</span><span class="hlt">2</span> transfer between the hydrosphere and atmosphere in the boundary layer is an important part of the global cycle of the main greenhouse gas. Gas <span class="hlt">flux</span> is determined by the difference of the partial pressures of the gas between the atmosphere and hydrosphere, near the border, as well as to a large extent processes involving turbulent boundary layer. The last is usually characterized by power dependence on the equivalent wind speed (10-m height). Hurricane-force winds lead to intensive wave breaking, with formation of spray in the <span class="hlt">air</span>, and bubbles in the water. Such multiphase turbulent processes at the interface strongly intensify gas transfer. Currently, data characterizing the dependence of the gas exchange of the wind speed for the hurricane conditions demonstrate a strong variation. On the other hand there is an obvious problem of obtaining reliable data on the wind speed. Widely used reanalysis data typically underestimate wind speed, due to the low spatial and temporal resolution One of the most promising ways to measure near water wind speed is the use of the data of remote sensing. The present study used technique to obtain near water wind speed based on the processing of remote sensing of the ocean surface data obtained with C-band scattermeter of RADARSAT using geophysical model function, developed in a laboratory conditions for a wide range of wind speeds, including hurricanes (see [1]). This function binds wind speed with effective radar cross-section in cross-polarized mode. We used two different parameterizations of gas transfer velocity of the wind speed. Widely used in [<span class="hlt">2</span>], and obtained by processing results of recent experiment in modeling winds up to hurricane on wind-wave facility [3]. The new method of calculating was tested by the example of hurricane Earl image (09.2010). Estimates showed 13-18 times excess <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> rates in comparison with monitoring data NOAA (see. [4]). 1. Troitskaya Yu., Abramov V., Ermoshkin A., Zuikova E., Kazakov V</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ClDy...50..101R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ClDy...50..101R"><span>Evaluation of energy <span class="hlt">fluxes</span> in the NCEP climate forecast system version <span class="hlt">2</span>.0 (CFSv<span class="hlt">2</span>)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rai, Archana; Saha, Subodh Kumar</p> <p>2018-01-01</p> <p>The energy <span class="hlt">fluxes</span> at the surface and top of the atmosphere (TOA) from a long free run by the NCEP climate forecast system version <span class="hlt">2</span>.0 (CFSv<span class="hlt">2</span>) are validated against several observation and reanalysis datasets. This study focuses on the annual mean energy <span class="hlt">fluxes</span> and tries to link it with the systematic cold biases in the <span class="hlt">2</span> m <span class="hlt">air</span> temperature, particularly over the land regions. The imbalance in the long term mean global averaged energy <span class="hlt">fluxes</span> are also evaluated. The global averaged imbalance at the surface and at the TOA is found to be 0.37 and 6.43 Wm-<span class="hlt">2</span>, respectively. It is shown that CFSv<span class="hlt">2</span> overestimates the land surface albedo, particularly over the snow region, which in turn contributes to the cold biases in <span class="hlt">2</span> m <span class="hlt">air</span> temperature. On the other hand, surface albedo is highly underestimated over the coastal region around Antarctica and that may have contributed to the warm bias over that oceanic region. This study highlights the need for improvements in the parameterization of snow/<span class="hlt">sea</span>-ice albedo scheme for a realistic simulation of surface temperature and that may have implications on the global energy imbalance in the model.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AtmEn.143..164W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AtmEn.143..164W"><span>Temporal variability in the sources and <span class="hlt">fluxes</span> of <span class="hlt">CO</span><span class="hlt">2</span> in a residential area in an evergreen subtropical city</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Weissert, L. F.; Salmond, J. A.; Turnbull, J. C.; Schwendenmann, L.</p> <p>2016-10-01</p> <p>Measurements of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in temperate climates have shown that urban areas are a net source of <span class="hlt">CO</span><span class="hlt">2</span> and that photosynthetic <span class="hlt">CO</span><span class="hlt">2</span> uptake is generally not sufficient to offset local <span class="hlt">CO</span><span class="hlt">2</span> emissions. However, little is known about the role of vegetation in cities where biogenic <span class="hlt">CO</span><span class="hlt">2</span> uptake is not limited to a <span class="hlt">2</span>-8 months growing season. This study used the eddy covariance technique to quantify the atmospheric <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> over a period of 12 months in a residential area in subtropical Auckland, New Zealand, where the vegetation cover (surface cover fraction: 47%) is dominated by evergreen vegetation. Radiocarbon isotope measurements of <span class="hlt">CO</span><span class="hlt">2</span> were conducted at three different times of the day (06:00-09:00, 12:00-15:00, 01:00-04:00) for four consecutive weekdays in summer and winter to differentiate anthropogenic sources of <span class="hlt">CO</span><span class="hlt">2</span> (fossil fuel combustion) from biogenic sources (ecosystem respiration, combustion of biofuel/biomass). The results reveal previously unreported patterns for <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>, with no seasonal variability and negative (net uptake) <span class="hlt">CO</span><span class="hlt">2</span> midday <span class="hlt">fluxes</span> throughout the year, demonstrating photosynthetic uptake by the evergreen vegetation all year-round. The winter radiocarbon measurements showed that 85% of the <span class="hlt">CO</span><span class="hlt">2</span> during the morning rush hour was attributed to fossil fuel emissions, when wind was from residential areas. However, for all other time periods radiocarbon measurements showed that fossil fuel combustion was not a large source of <span class="hlt">CO</span><span class="hlt">2</span>, suggesting that biogenic processes likely dominate <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> at this residential site. Overall, our findings highlight the importance of vegetation in residential areas to mitigate local <span class="hlt">CO</span><span class="hlt">2</span> emissions, particularly in cities with a climate that allows evergreen vegetation to maintain high photosynthetic rates over winter. As urban areas grow, urban planners need to consider the role of urban greenspace to mitigate urban <span class="hlt">CO</span><span class="hlt">2</span> emissions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A23G2450D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A23G2450D"><span>Measurements and models of <span class="hlt">CO</span><span class="hlt">2</span> and CH4 <span class="hlt">Flux</span> in the Baltimore/Washington area.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dickerson, R. R.; Ren, X.; Salawitch, R. J.; Ahn, D.; Karion, A.; Shepson, P. B.; Whetstone, J. R.; Martin, C.</p> <p>2017-12-01</p> <p>Direct measurements of concentrations of pollutants such as <span class="hlt">CO</span><span class="hlt">2</span> and CH4 can be combined with wind fields to determine the <span class="hlt">flux</span> of these species and to evaluate emissions inventories or models. The mass balance approach, assumng linear flow into and out of a volume set over a city, works best where wind fields are simplest. Over typical American east coast cities, upwind sources and complex circulation (e.g., the <span class="hlt">sea</span> breeze) complicate such analyses. We will present findings from a coupled measurement and modeling project involving a network of surface-based tower measurements, aircraft observations, and remote sensing that constrain model calculations. Summer and winter scenarios are contrasted, and results help evaluate the emissions of short-lived pollutants. Determinations are compared to several emissions inventories and are being used to help States evaluate evaluate plans for pollution control.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/23725','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/23725"><span>Seasonal patterns in soil surface <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> under snow cover in 50 and 300 year old subalpine forests</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Robert M. Hubbard; Michael G. Ryan; Kelly Elder; Charles C. Rhoades</p> <p>2005-01-01</p> <p>Soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> can contribute as much as 60-80% of total ecosystem respiration in forests. Although considerable research has focused on quantifying this <span class="hlt">flux</span> during the growing season, comparatively little effort has focused on non-growing season <span class="hlt">fluxes</span>. We measured soil <span class="hlt">CO</span><span class="hlt">2</span> efflux through snow in 50 and 300 year old subalpine forest stands near Fraser <span class="hlt">CO</span>. Our...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002EGSGA..27.3717S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002EGSGA..27.3717S"><span>The Coca-campaign: An Attempt To Derive The Carbon Exchange of A Forested Region Using Airborne <span class="hlt">Co</span><span class="hlt">2</span> and <span class="hlt">Co</span> Observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schmitgen, S.; Ciais, P.; Geiß, H.; Kley, D.; Neininger, B.; Baeumle, M.; Fuchs, W.; Brunet, Y.</p> <p></p> <p>As part of the project COCA an attempt was made to measure the daytime biogenic <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> over a forest area (about 15 by 30 km). This campaign took place around the CARBOEUROFLUX site "Le Bray" (Pinus pinaster) close to Bordeaux in France end of June 2001. Based on continuous airborne <span class="hlt">CO</span><span class="hlt">2</span>, H<span class="hlt">2</span>O and <span class="hlt">CO</span> <span class="hlt">flux</span> and concen- tration measurements a Lagrangian budgeting approach was chosen for the determi- nation of the regional <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. The objective is to determine the <span class="hlt">CO</span><span class="hlt">2</span> uptake of the extended forest area from the <span class="hlt">CO</span><span class="hlt">2</span>/<span class="hlt">CO</span> gradients up- and downwind of the ecosystem, using <span class="hlt">CO</span> as <span class="hlt">air</span> mass tracer and such eliminating the influence of anthropogenic <span class="hlt">CO</span><span class="hlt">2</span> advected into the area. First results will be shown of a flight on June 23rd, where fair wind speeds (about 5 m/s) and a low CBL height led to the observation of a clear decrease in <span class="hlt">CO</span><span class="hlt">2</span> at the downwind flight stacks with basically constant <span class="hlt">CO</span> concentrations. For other flights with very low wind speeds, local effects dominate the observa- tions leading to a larger variability in the observations. Both, correlations and anti- correlations of <span class="hlt">CO</span><span class="hlt">2</span> with the anthropogenic tracer <span class="hlt">CO</span> have been observed. Positive correlations indicate fresh plumes of anthropogenic <span class="hlt">CO</span><span class="hlt">2</span>. Negative correlations are indicative of entrainment of free tropospheric <span class="hlt">air</span>, that was marked by relatively higher <span class="hlt">CO</span><span class="hlt">2</span> and lower <span class="hlt">CO</span> concentrations than the average CBL concentrations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ACP....17.4781F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ACP....17.4781F"><span>Consistent regional <span class="hlt">fluxes</span> of CH4 and <span class="hlt">CO</span><span class="hlt">2</span> inferred from GOSAT proxy XCH4 : XCO<span class="hlt">2</span> retrievals, 2010-2014</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Feng, Liang; Palmer, Paul I.; Bösch, Hartmut; Parker, Robert J.; Webb, Alex J.; Correia, Caio S. C.; Deutscher, Nicholas M.; Domingues, Lucas G.; Feist, Dietrich G.; Gatti, Luciana V.; Gloor, Emanuel; Hase, Frank; Kivi, Rigel; Liu, Yi; Miller, John B.; Morino, Isamu; Sussmann, Ralf; Strong, Kimberly; Uchino, Osamu; Wang, Jing; Zahn, Andreas</p> <p>2017-04-01</p> <p>We use the GEOS-Chem global 3-D model of atmospheric chemistry and transport and an ensemble Kalman filter to simultaneously infer regional <span class="hlt">fluxes</span> of methane (CH4) and carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) directly from GOSAT retrievals of XCH4 : XCO<span class="hlt">2</span>, using sparse ground-based CH4 and <span class="hlt">CO</span><span class="hlt">2</span> mole fraction data to anchor the ratio. This work builds on the previously reported theory that takes into account that (1) these ratios are less prone to systematic error than either the full-physics data products or the proxy CH4 data products; and (<span class="hlt">2</span>) the resulting CH4 and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> are self-consistent. We show that a posteriori <span class="hlt">fluxes</span> inferred from the GOSAT data generally outperform the <span class="hlt">fluxes</span> inferred only from in situ data, as expected. GOSAT CH4 and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> are consistent with global growth rates for <span class="hlt">CO</span><span class="hlt">2</span> and CH4 reported by NOAA and have a range of independent data including new profile measurements (0-7 km) over the Amazon Basin that were collected specifically to help validate GOSAT over this geographical region. We find that large-scale multi-year annual a posteriori <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> inferred from GOSAT data are similar to those inferred from the in situ surface data but with smaller uncertainties, particularly over the tropics. GOSAT data are consistent with smaller peak-to-peak seasonal amplitudes of <span class="hlt">CO</span><span class="hlt">2</span> than either the a priori or in situ inversion, particularly over the tropics and the southern extratropics. Over the northern extratropics, GOSAT data show larger uptake than the a priori but less than the in situ inversion, resulting in small net emissions over the year. We also find evidence that the carbon balance of tropical South America was perturbed following the droughts of 2010 and 2012 with net annual <span class="hlt">fluxes</span> not returning to an approximate annual balance until 2013. In contrast, GOSAT data significantly changed the a priori spatial distribution of CH4 emission with a 40 % increase over tropical South America and tropical Asia and a smaller decrease over Eurasia and temperate</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27400026','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27400026"><span>Contrasting ecosystem <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> of inland and coastal wetlands: a meta-analysis of eddy covariance data.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lu, Weizhi; Xiao, Jingfeng; Liu, Fang; Zhang, Yue; Liu, Chang'an; Lin, Guanghui</p> <p>2017-03-01</p> <p>Wetlands play an important role in regulating the atmospheric carbon dioxide (<span class="hlt">CO</span> <span class="hlt">2</span> ) concentrations and thus affecting the climate. However, there is still lack of quantitative evaluation of such a role across different wetland types, especially at the global scale. Here, we conducted a meta-analysis to compare ecosystem <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">fluxes</span> among various types of wetlands using a global database compiled from the literature. This database consists of 143 site-years of eddy covariance data from 22 inland wetland and 21 coastal wetland sites across the globe. Coastal wetlands had higher annual gross primary productivity (GPP), ecosystem respiration (R e ), and net ecosystem productivity (NEP) than inland wetlands. On a per unit area basis, coastal wetlands provided large <span class="hlt">CO</span> <span class="hlt">2</span> sinks, while inland wetlands provided small <span class="hlt">CO</span> <span class="hlt">2</span> sinks or were nearly <span class="hlt">CO</span> <span class="hlt">2</span> neutral. The annual <span class="hlt">CO</span> <span class="hlt">2</span> sink strength was 93.15 and 208.37 g C m -<span class="hlt">2</span> for inland and coastal wetlands, respectively. Annual <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">fluxes</span> were mainly regulated by mean annual temperature (MAT) and mean annual precipitation (MAP). For coastal and inland wetlands combined, MAT and MAP explained 71%, 54%, and 57% of the variations in GPP, R e , and NEP, respectively. The <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">fluxes</span> of wetlands were also related to leaf area index (LAI). The <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">fluxes</span> also varied with water table depth (WTD), although the effects of WTD were not statistically significant. NEP was jointly determined by GPP and R e for both inland and coastal wetlands. However, the NEP/R e and NEP/GPP ratios exhibited little variability for inland wetlands and decreased for coastal wetlands with increasing latitude. The contrasting of <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">fluxes</span> between inland and coastal wetlands globally can improve our understanding of the roles of wetlands in the global C cycle. Our results also have implications for informing wetland management and climate change policymaking, for example, the efforts being made by international organizations and enterprises to restore coastal</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24489821','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24489821"><span>The response of Antarctic <span class="hlt">sea</span> ice algae to changes in pH and <span class="hlt">CO</span><span class="hlt">2</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>McMinn, Andrew; Müller, Marius N; Martin, Andrew; Ryan, Ken G</p> <p>2014-01-01</p> <p>Ocean acidification substantially alters ocean carbon chemistry and hence pH but the effects on <span class="hlt">sea</span> ice formation and the <span class="hlt">CO</span><span class="hlt">2</span> concentration in the enclosed brine channels are unknown. Microbial communities inhabiting <span class="hlt">sea</span> ice ecosystems currently contribute 10-50% of the annual primary production of polar <span class="hlt">seas</span>, supporting overwintering zooplankton species, especially Antarctic krill, and seeding spring phytoplankton blooms. Ocean acidification is occurring in all surface waters but the strongest effects will be experienced in polar ecosystems with significant effects on all trophic levels. Brine algae collected from McMurdo Sound (Antarctica) <span class="hlt">sea</span> ice was incubated in situ under various carbonate chemistry conditions. The carbon chemistry was manipulated with acid, bicarbonate and bases to produce a p<span class="hlt">CO</span><span class="hlt">2</span> and pH range from 238 to 6066 µatm and 7.19 to 8.66, respectively. Elevated p<span class="hlt">CO</span><span class="hlt">2</span> positively affected the growth rate of the brine algal community, dominated by the unique ice dinoflagellate, Polarella glacialis. Growth rates were significantly reduced when pH dropped below 7.6. However, when the pH was held constant and the p<span class="hlt">CO</span><span class="hlt">2</span> increased, growth rates of the brine algae increased by more than 20% and showed no decline at p<span class="hlt">CO</span><span class="hlt">2</span> values more than five times current ambient levels. We suggest that projected increases in seawater p<span class="hlt">CO</span><span class="hlt">2</span>, associated with OA, will not adversely impact brine algal communities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/12916843','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/12916843"><span>Improving mercury <span class="hlt">flux</span> chamber measurements over water surface.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lanzillotra, E; Ceccarini, C; Ferrara, R</p> <p>2003-07-01</p> <p>A modified floating <span class="hlt">flux</span> chamber was designed and used to measure mercury evasional <span class="hlt">fluxes</span> in a coastal area of the Mediterranean <span class="hlt">Sea</span> in different meteo-marine conditions during the hours of maximum insolation (PAR intensity 360-430 W m(-<span class="hlt">2</span>)) in the summer season. The chamber has been modified providing a flap at the inlet port preventing the back-flow of <span class="hlt">air</span> from the interior of the chamber. Results demonstrate that the modified <span class="hlt">flux</span> chamber gives <span class="hlt">flux</span> values noticeably higher both in rippled <span class="hlt">sea</span> conditions (mean value 7.88 +/- 1.45 ng m(-<span class="hlt">2</span>) h(-1)) and in rough <span class="hlt">sea</span> conditions (mean value 21.71 +/- <span class="hlt">2</span>.17 ng m(-<span class="hlt">2</span>) h(-1)) with respect to those obtained by using the unmodified chamber (respectively 5.23 +/- 0.67 and 14.15 +/- 1.03 ng m(-<span class="hlt">2</span>) h(-1)).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.8639K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.8639K"><span>Net drainage effects on <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> of a permafrost ecosystem through eddy-covariance measurements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kittler, Fanny; Burjack, Ina; Zimov, Nikita; Zimov, Sergey; Heimann, Martin; Göckede, Mathias</p> <p>2015-04-01</p> <p>Permafrost landscapes in the Northern high latitudes with their massive organic carbon stocks are critically important for the global carbon cycle, yet feedback processes with the atmosphere under future climate conditions are uncertain. To improve the understanding of mechanisms and drivers dominating permafrost carbon cycling, we established a continuous observation program in moist tussock tundra ecosystem near Cherskiy in North-eastern Siberia (68.75°N, 161.33°E). The experiment has been designed to monitor carbon cycle <span class="hlt">fluxes</span> at different scales with different approaches, including e.g. the eddy-covariance technique, and their environmental drivers. Recent observations started mid July 2013 and are still ongoing, while 'historic' measurements are available for the period 2002-2005. Since 2004 part of the observation area has been disturbed by a drainage ditch ring, altering the soil water conditions in the surrounding area in a way that is expected for degrading ice-rich permafrost under a warming climate. With parallel observations over the disturbed (drained) area and a reference area nearby, respectively, we aim to evaluate the disturbance effect on the carbon cycle budgets and the dominating biogeochemical mechanisms. Here, findings based on over 1.5 years of continuous eddy-covariance <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> measurements (July 2013 - March 2015) for both observation areas are presented. Results show systematic shifts in the tundra ecosystem as a result of 10 years of disturbance in the drained area, with significant effects on biotic and abiotic site conditions as well as on the carbon cycle dynamics. Comparing the net budget <span class="hlt">fluxes</span> between both observations areas indicates a reduction of the net sink strength for <span class="hlt">CO</span><span class="hlt">2</span> of the drained ecosystem during the summer season in comparison to natural conditions, mostly caused by reduced <span class="hlt">CO</span><span class="hlt">2</span> uptake with low water levels in late summer. Regarding the long-term <span class="hlt">CO</span><span class="hlt">2</span> uptake dynamics of the disturbance regime (2005 vs. 2013/14) the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20060032490&hterms=sonar&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dsonar','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060032490&hterms=sonar&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dsonar"><span>Combined Satellite - and ULS-Derived <span class="hlt">Sea</span>-Ice <span class="hlt">Flux</span> in the Weddell <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Drinkwater, M.; Liu, X.; Harms, S.</p> <p>2000-01-01</p> <p>Several years of daily microwave satellite ice-drift are combined with moored Upward Looking Sonar (ULS) ice-drafts into an ice volume <span class="hlt">flux</span> record at points along a <span class="hlt">flux</span> gate across the Weddell <span class="hlt">Sea</span>, Antarctica.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_22 --> <div id="page_23" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="441"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.ars.usda.gov/research/publications/publication/?seqNo115=321468','TEKTRAN'); return false;" href="http://www.ars.usda.gov/research/publications/publication/?seqNo115=321468"><span>Comparing <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> data from eddy covariance methods with bowen ratio energy balance methods from contrasting soil management</span></a></p> <p><a target="_blank" href="https://www.ars.usda.gov/research/publications/find-a-publication/">USDA-ARS?s Scientific Manuscript database</a></p> <p></p> <p></p> <p>Measuring <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> from contrasting soil management practices is important for understanding the role of agriculture in source-sink relationship with <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span>. There are several micrometeorological methods for measuring <span class="hlt">CO</span><span class="hlt">2</span> emissions, however all are expensive and thus do not easily lend themselve...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27544762','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27544762"><span>Aircraft measurements of SO<span class="hlt">2</span>, NOx, <span class="hlt">CO</span>, and O3 over the coastal and offshore area of Yellow <span class="hlt">Sea</span> of China.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yang, Xiaoyang; Wang, Xinhua; Yang, Wen; Xu, Jun; Ren, Lihong; He, Youjiang; Liu, Bing; Bai, Zhipeng; Meng, Fan; Hu, Min</p> <p>2016-09-01</p> <p>In order to investigate long-range transport of the <span class="hlt">air</span> pollution in the East Asia, <span class="hlt">air</span> pollutants, including SO<span class="hlt">2</span>, NOx, <span class="hlt">CO</span>, and O3, were observed by aircraft measurement over the coastal and offshore area of Yellow <span class="hlt">Sea</span> of China in April 2011. NOx and SO<span class="hlt">2</span> seemed to become moderate in recent years, and the concentrations during the whole observations ranged from 0.49 to 9.57 ppb and from 0.10 to 16.02 ppb, respectively. The high concentrations of <span class="hlt">CO</span> were measured with an average value of 0.98 ppm. The measured O3 average concentration was 76.25 ppb, which showed a higher level comparing with the results from some previous studies. Most of the results for the concentration values generally followed the typical characteristic of vertical and spatial distribution, which were "low altitude > high altitude" and "land/coastal > <span class="hlt">sea</span>," respectively. Transport of polluted <span class="hlt">air</span> mass from the continent to the aircraft measurement area was confirmed in some days during the observation by the meteorological analysis, while the measurement results supposed to represent the background level of the pollutants in rest days. Additionally, some small-scale <span class="hlt">air</span> pollution plumes were observed. Significant positive correlations between NOx and SO<span class="hlt">2</span> indicated that these two species originated from the same region. On the other hand, good positive correlations between NOx and O3 found during <span class="hlt">2</span>-day flight suggested that the O3 formation was probably under "NOx-limited" regime in these days.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006GeoRL..3314803Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006GeoRL..3314803Z"><span>Impacts of winter storms on <span class="hlt">air-sea</span> gas exchange</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, Weiqing; Perrie, Will; Vagle, Svein</p> <p>2006-07-01</p> <p>The objective of this study is to investigate <span class="hlt">air-sea</span> gas exchange during winter storms, using field measurements from Ocean Station Papa in the Northeast Pacific (50°N, 145°W). We show that increasing gas transfer rates are coincident with increasing winds and deepening depth of bubble penetration, and that this process depends on <span class="hlt">sea</span> state. Wave-breaking is shown to be an important factor in the gas transfer velocity during the peaks of the storms, increasing the <span class="hlt">flux</span> rates by up to 20%. Gas transfer rates and concentrations can exhibit asymmetry, reflecting a sudden increase with the onset of a storm, and gradual recovery stages.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24066532','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24066532"><span>[Temperature sensitivity of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> from rhizosphere soil mineralization and root decomposition in Pinus massoniana and Castanopsis sclerophylla forests].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Liu, Yu; Hu, Xiao-Fei; Chen, Fu-Sheng; Yuan, Ping-Cheng</p> <p>2013-06-01</p> <p>Rhizospheric and non-rhizospheric soils and the absorption, transition, and storage roots were sampled from the mid-subtropical Pinus massoniana and Castanopsis sclerophylla forests to study the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> from soil mineralization and root decomposition in the forests. The samples were incubated in closed jars at 15 degrees C, 25 degrees C, 35 degrees C, and 45 degrees C, respectively, and alkali absorption method was applied to measure the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> during 53 days incubation. For the two forests, the rhizospheric effect (ratio of rhizospheric to non-rhizospheric soil) on the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> from soil mineralization across all incubation temperature ranged from 1.12 to 3.09, with a decreasing trend along incubation days. There was no significant difference in the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> from soil mineralization between the two forests at 15 degrees C, but the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> was significantly higher in P. massoniana forest than in C. sclerophylla forest at 25 degrees C and 35 degrees C, and in an opposite pattern at 45 degrees C. At all incubation temperature, the <span class="hlt">CO</span><span class="hlt">2</span> release from the absorption root decomposition was higher than that from the transition and storage roots decomposition, and was smaller in P. massoniana than in C. sclerophylla forest for all the root functional types. The Q10 values of the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> from the two forests were higher for soils (1.21-1.83) than for roots (0.96-1.36). No significant differences were observed in the Q10 values of the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> from soil mineralization between the two forests, but the Q10 value of the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> from root decomposition was significantly higher in P. massoniana than in C. sclerophylla forest. It was suggested that the increment of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> from soil mineralization under global warming was far higher than that from root decomposition, and for P. massoniana than for C. sclerophylla forest. In subtropics of China, the adaptability of zonal climax community to global warming would be stronger than that of pioneer community.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..1413625S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..1413625S"><span>Temporal evolution of the anthropogenic <span class="hlt">CO</span><span class="hlt">2</span> and acidification of the northwestern Mediterranean <span class="hlt">Sea</span>, from the mid-1990s to the mid-2000s</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Savy, J.-P.; Yao, K. M.; Touratier, F.; Goyet, C.</p> <p>2012-04-01</p> <p>Since the beginning of the industrial era, humankind consumption of fossil fuels at increasing rates has led to increases in atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentrations by approximately 105 ppm. In the same time, the Mediterranean coastal regions experienced a brutal population growth, from 94 million habitants in 1950 to 274 million in 2000, generating a strong anthropogenic pressure on the Mediterranean marine ecosystems. To follow the man-induced changes on the Mediterranean carbonate system properties (pH; total alkalinity, AT; total inorganic carbon CT, and <span class="hlt">CO</span><span class="hlt">2</span> partial pressure, p<span class="hlt">CO</span><span class="hlt">2</span>), an entire body-research has recently emerged in order to quantify both the present and future penetration of anthropogenic carbon (CANT) in the Mediterranean <span class="hlt">Sea</span> and the inferred acidification of its waters. From monthly observations accumulated over more than a decade (from 1993 to 2005) at DYFAMED time-series station (DYnamique des <span class="hlt">Flux</span> Atmosphériques en MEDiterranée) located in the central part of the Ligurian <span class="hlt">Sea</span>, Touratier and Goyet (2009) have estimated the temporal evolution of CANT of the western Mediterranean <span class="hlt">Sea</span>. This study highlights that concentrations of anthropogenic <span class="hlt">CO</span><span class="hlt">2</span> are much higher at DYFAMED site (> 50 mol.kg-1) than those found in the Atlantic Ocean. Our study, conducted with measurements performed at 10 meters depth from 1995 to 2011 at the same location, allowed us to investigate the temporal evolution of CANT into the upper seawater layer. Our results indicate an averaged annual CANT increase of 3 µmol.kg-1 and a linked pH drop of 0.0032 per year confirming the ongoing acidification of the Mediterranean water masses. These results suggest the vulnerability and the endangerment of the Mediterranean ecosystems by the massive human-induced <span class="hlt">CO</span><span class="hlt">2</span> emissions. Touratier F. and C. Goyet (2009). Decadal evolution of anthropogenic <span class="hlt">CO</span><span class="hlt">2</span> in the north western Mediterranean <span class="hlt">Sea</span> (at the Dyfamed site) from the mid-1990's to the mid-2000's. Deep <span class="hlt">Sea</span> Research Part I, 56, 1708-1716</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOS.A23A..04C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOS.A23A..04C"><span><span class="hlt">Air-Sea</span> Momentum and Enthalpy Exchange in Coupled Atmosphere-Wave-Ocean Modeling of Tropical Cyclones</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Curcic, M.; Chen, S. S.</p> <p>2016-02-01</p> <p>The atmosphere and ocean are coupled through momentum, enthalpy, and mass <span class="hlt">fluxes</span>. Accurate representation of these <span class="hlt">fluxes</span> in a wide range of weather and climate conditions is one of major challenges in prediction models. Their current parameterizations are based on sparse observations in low-to-moderate winds and are not suited for high wind conditions such as tropical cyclones (TCs) and winter storms. In this study, we use the Unified Wave INterface - Coupled Model (UWIN-CM), a high resolution, fully-coupled atmosphere-wave-ocean model, to better understand the role of ocean surface waves in mediating <span class="hlt">air-sea</span> momentum and enthalpy exchange in TCs. In particular, we focus on the explicit treatment of wave growth and dissipation for calculating atmospheric and oceanic stress, and its role in upper ocean mixing and surface cooling in the wake of the storm. Wind-wave misalignment and local wave disequilibrium result in difference between atmospheric and oceanic stress being largest on the left side of the storm. We find that explicit wave calculation in the coupled model reduces momentum transfer into the ocean by more than 10% on average, resulting in reduced cooling in TC's wake and subsequent weakening of the storm. We also investigate the impacts of <span class="hlt">sea</span> surface temperature and upper ocean parameterization on <span class="hlt">air-sea</span> enthalpy <span class="hlt">fluxes</span> in the fully coupled model. High-resolution UWIN-CM simulations of TCs with various intensities and structure are conducted in this study to better understand the complex TC-ocean interaction and improve the representation of <span class="hlt">air-sea</span> coupling processes in coupled prediction models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1918076S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1918076S"><span>True eddy accumulation and eddy covariance methods and instruments intercomparison for <span class="hlt">fluxes</span> of <span class="hlt">CO</span><span class="hlt">2</span>, CH4 and H<span class="hlt">2</span>O above the Hainich Forest</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Siebicke, Lukas</p> <p>2017-04-01</p> <p>The eddy covariance (EC) method is state-of-the-art in directly measuring vegetation-atmosphere exchange of <span class="hlt">CO</span><span class="hlt">2</span> and H<span class="hlt">2</span>O at ecosystem scale. However, the EC method is currently limited to a small number of atmospheric tracers by the lack of suitable fast-response analyzers or poor signal-to-noise ratios. High resource and power demands may further restrict the number of spatial sampling points. True eddy accumulation (TEA) is an alternative method for direct and continuous <span class="hlt">flux</span> observations. Key advantages are the applicability to a wider range of <span class="hlt">air</span> constituents such as greenhouse gases, isotopes, volatile organic compounds and aerosols using slow-response analyzers. In contrast to relaxed eddy accumulation (REA), true eddy accumulation (Desjardins, 1977) has the advantage of being a direct method which does not require proxies. True Eddy Accumulation has the potential to overcome above mentioned limitations of eddy covariance but has hardly ever been successfully demonstrated in practice in the past. This study presents <span class="hlt">flux</span> measurements using an innovative approach to true eddy accumulation by directly, continuously and automatically measuring trace gas <span class="hlt">fluxes</span> using a flow-through system. We merge high-frequency <span class="hlt">flux</span> contributions from TEA with low-frequency covariances from the same sensors. We show <span class="hlt">flux</span> measurements of <span class="hlt">CO</span><span class="hlt">2</span>, CH4 and H<span class="hlt">2</span>O by TEA and EC above an old-growth forest at the ICOS <span class="hlt">flux</span> tower site "Hainich" (DE-Hai). We compare and evaluate the performance of the two direct turbulent <span class="hlt">flux</span> measurement methods eddy covariance and true eddy accumulation using side-by-side trace gas <span class="hlt">flux</span> observations. We further compare performance of seven instrument complexes, i.e. combinations of sonic anemometers and trace gas analyzers. We compare gas analyzers types of open-path, enclosed-path and closed-path design. We further differentiate data from two gas analysis technologies: infrared gas analysis (IRGA) and laser spectrometry (open path and CRDS closed</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.V21A2484W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.V21A2484W"><span>Gas composition and soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> at Changbaishan intra-plate volcano, NE China</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>wen, H.; Yang, T. F.; Guo, Z.; Fu, C.; Zhang, M.</p> <p>2011-12-01</p> <p>Changbaishan, located on the border of China and North Korea, is one of the most active volcanoes in China. This volcano violently erupted 1000 years ago and produced massive magma and widespread volcanic ash, resulting in one of the largest explosive eruptions during the last 2000 years. Recent gas emissions and seismic events in the Tianchi area suggested potential increasing volcanic activities. If that is so, then 1 million residents living on the crater flank shall be endangered by enormous volcanic hazards, including the threat of <span class="hlt">2</span> billion tons of water in the crater lake . In order to better understand current status of Changbaishan, we investigated gas geochemistry in samples from the Tianchi crater lake and surrounding areas. Bubbling gas from hot springs were collected and analyzed. The results show that <span class="hlt">CO</span><span class="hlt">2</span> is the major component gas for most samples. The maximum value of helium isotopic ratio 5.8 RA (where RA = 3He/4He in <span class="hlt">air</span>) implies more than 60% of helium is contributed by mantle component, while carbon isotope values fall in the range of -5.8 to -<span class="hlt">2</span>.0% (vs. PDB), indicating magmatic source signatures as well. Nitrogen dominated samples, 18Dawgo, have helium isotopic ratio 0.7 RA and carbon isotope value -11.4% implying the gas source might be associated with regional crustal components in 18Dawgo. The first-time systematic soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> measurements indicate the <span class="hlt">flux</span> is 22.8 g m-<span class="hlt">2</span> day-1 at the western flank of Changbaishan, which is at the same level as the background value in the Tatun Volcano Group (24.6 g m-<span class="hlt">2</span> day-1), implying that it may not be as active as TVG.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20150005617&hterms=infrared+temperature+sensor&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dinfrared%2Btemperature%2Bsensor','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20150005617&hterms=infrared+temperature+sensor&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dinfrared%2Btemperature%2Bsensor"><span>Sensitivity Analysis for Atmospheric Infrared Sounder (<span class="hlt">AIRS</span>) <span class="hlt">CO</span><span class="hlt">2</span> Retrieval</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gat, Ilana</p> <p>2012-01-01</p> <p>The Atmospheric Infrared Sounder (<span class="hlt">AIRS</span>) is a thermal infrared sensor able to retrieve the daily atmospheric state globally for clear as well as partially cloudy field-of-views. The <span class="hlt">AIRS</span> spectrometer has 2378 channels sensing from 15.4 micrometers to 3.7 micrometers, of which a small subset in the 15 micrometers region has been selected, to date, for <span class="hlt">CO</span><span class="hlt">2</span> retrieval. To improve upon the current retrieval method, we extended the retrieval calculations to include a prior estimate component and developed a channel ranking system to optimize the channels and number of channels used. The channel ranking system uses a mathematical formalism to rapidly process and assess the retrieval potential of large numbers of channels. Implementing this system, we identifed a larger optimized subset of <span class="hlt">AIRS</span> channels that can decrease retrieval errors and minimize the overall sensitivity to other iridescent contributors, such as water vapor, ozone, and atmospheric temperature. This methodology selects channels globally by accounting for the latitudinal, longitudinal, and seasonal dependencies of the subset. The new methodology increases accuracy in <span class="hlt">AIRS</span> <span class="hlt">CO</span><span class="hlt">2</span> as well as other retrievals and enables the extension of retrieved <span class="hlt">CO</span><span class="hlt">2</span> vertical profiles to altitudes ranging from the lower troposphere to upper stratosphere. The extended retrieval method for <span class="hlt">CO</span><span class="hlt">2</span> vertical profile estimation using a maximum-likelihood estimation method. We use model data to demonstrate the beneficial impact of the extended retrieval method using the new channel ranking system on <span class="hlt">CO</span><span class="hlt">2</span> retrieval.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002JApMe..41..241B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002JApMe..41..241B"><span>An Integrated Approach to Estimate Instantaneous Near-Surface <span class="hlt">Air</span> Temperature and Sensible Heat <span class="hlt">Flux</span> Fields during the SEMAPHORE Experiment.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bourras, Denis; Eymard, Laurence; Liu, W. Timothy; Dupuis, Hélène</p> <p>2002-03-01</p> <p>A new technique was developed to retrieve near-surface instantaneous <span class="hlt">air</span> temperatures and turbulent sensible heat <span class="hlt">fluxes</span> using satellite data during the Structure des Echanges Mer-Atmosphere, Proprietes des Heterogeneites Oceaniques: Recherche Experimentale (SEMAPHORE) experiment, which was conducted in 1993 under mainly anticyclonic conditions. The method is based on a regional, horizontal atmospheric temperature advection model whose inputs are wind vectors, <span class="hlt">sea</span> surface temperature fields, <span class="hlt">air</span> temperatures around the region under study, and several constants derived from in situ measurements. The intrinsic rms error of the method is 0.7°C in terms of <span class="hlt">air</span> temperature and 9 W m<span class="hlt">2</span> for the <span class="hlt">fluxes</span>, both at 0.16° × 0.16° and 1.125° × 1.125° resolution. The retrieved <span class="hlt">air</span> temperature and <span class="hlt">flux</span> horizontal structures are in good agreement with fields from two operational general circulation models. The application to SEMAPHORE data involves the First European Remote Sensing Satellite (ERS-1) wind fields, Advanced Very High Resolution Radiometer (AVHRR) SST fields, and European Centre for Medium-Range Weather Forecasts (ECMWF) <span class="hlt">air</span> temperature boundary conditions. The rms errors obtained by comparing the estimations with research vessel measurements are 0.3°C and 5 W m<span class="hlt">2</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.A51F..06C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.A51F..06C"><span>Comparing inversion techniques for constraining <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in the Brazilian Amazon Basin with aircraft observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chow, V. Y.; Gerbig, C.; Longo, M.; Koch, F.; Nehrkorn, T.; Eluszkiewicz, J.; Ceballos, J. C.; Longo, K.; Wofsy, S. C.</p> <p>2012-12-01</p> <p>The Balanço Atmosférico Regional de Carbono na Amazônia (BARCA) aircraft program spanned the dry to wet and wet to dry transition seasons in November 2008 & May 2009 respectively. It resulted in ~150 vertical profiles covering the Brazilian Amazon Basin (BAB). With the data we attempt to estimate a carbon budget for the BAB, to determine if regional aircraft experiments can provide strong constraints for a budget, and to compare inversion frameworks when optimizing <span class="hlt">flux</span> estimates. We use a LPDM to integrate satellite-, aircraft-, & surface-data with mesoscale meteorological fields to link bottom-up and top-down models to provide constraints and error bounds for regional <span class="hlt">fluxes</span>. The Stochastic Time-Inverted Lagrangian Transport (STILT) model driven by meteorological fields from BRAMS, ECMWF, and WRF are coupled to a biosphere model, the Vegetation Photosynthesis Respiration Model (VPRM), to determine regional <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> for the BAB. The VPRM is a prognostic biosphere model driven by MODIS 8-day EVI and LSWI indices along with shortwave radiation and temperature from tower measurements and mesoscale meteorological data. VPRM parameters are tuned using eddy <span class="hlt">flux</span> tower data from the Large-Scale Biosphere Atmosphere experiment. VPRM computes hourly <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> by calculating Gross Ecosystem Exchange (GEE) and Respiration (R) for 8 different vegetation types. The VPRM <span class="hlt">fluxes</span> are scaled up to the BAB by using time-averaged drivers (shortwave radiation & temperature) from high-temporal resolution runs of BRAMS, ECMWF, and WRF and vegetation maps from SYNMAP and IGBP2007. Shortwave radiation from each mesoscale model is validated using surface data and output from GL 1.<span class="hlt">2</span>, a global radiation model based on GOES 8 visible imagery. The vegetation maps are updated to 2008 and 2009 using landuse scenarios modeled by Sim Amazonia <span class="hlt">2</span> and Sim Brazil. A priori <span class="hlt">fluxes</span> modeled by STILT-VPRM are optimized using data from BARCA, eddy covariance sites, and flask measurements. The</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20020054331&hterms=Organic+fertilizers&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DOrganic%2Bfertilizers','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20020054331&hterms=Organic+fertilizers&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DOrganic%2Bfertilizers"><span>Interannual Variability in Soil Trace Gas (<span class="hlt">CO</span><span class="hlt">2</span>, N<span class="hlt">2</span>O, NO) <span class="hlt">Fluxes</span> and Analysis of Controllers</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Potter, C.; Klooster, S.; Peterson, David L. (Technical Monitor)</p> <p>1997-01-01</p> <p>Interannual variability in <span class="hlt">flux</span> rates of biogenic trace gases must be quantified in order to understand the differences between short-term trends and actual long-term change in biosphere-atmosphere interactions. We simulated interannual patterns (1983-1988) of global trace gas <span class="hlt">fluxes</span> from soils using the NASA Ames model version of CASA (Carnegie-Ames-Stanford Approach) in a transient simulation mode. This ecosystem model has been recalibrated for simulations driven by satellite vegetation index data from the NOAA Advanced Very High Resolution Radiometer (AVHRR) over the mid-1980s. The predicted interannual pattern of soil heterotropic <span class="hlt">CO</span><span class="hlt">2</span> emissions indicates that relatively large increases in global carbon <span class="hlt">flux</span> from soils occurred about three years following the strong El Nino Southern Oscillation (ENSO) event of 1983. Results for the years 1986 and 1987 showed an annual increment of +1 Pg (1015 g) C-<span class="hlt">CO</span><span class="hlt">2</span> emitted from soils, which tended to dampen the estimated global increase in net ecosystem production with about a two year lag period relative to plant carbon fixation. Zonal discrimination of model results implies that 80-90 percent of the yearly positive increments in soil <span class="hlt">CO</span><span class="hlt">2</span> emission during 1986-87 were attributable to soil organic matter decomposition in the low-latitudes (between 30 N and 30 S). Soils of the northern middle-latitude zone (between 30 N and 60 N) accounted for the residual of these annual increments. Total annual emissions of nitrogen trace gases (N<span class="hlt">2</span>O and NO) from soils were estimated to vary from <span class="hlt">2</span>-4 percent over the time period modeled, a level of variability which is consistent with predicted interannual fluctuations in global soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. Interannual variability of precipitation in tropical and subtropical zones (30 N to 20 S appeared to drive the dynamic inverse relationship between higher annual emissions of NO versus emissions of N<span class="hlt">2</span>O. Global mean emission rates from natural (heterotrophic) soil sources over the period modeled (1983</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.B41C0071S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.B41C0071S"><span>Sampling Soil <span class="hlt">CO</span><span class="hlt">2</span> for Isotopic <span class="hlt">Flux</span> Partitioning: Non Steady State Effects and Methodological Biases</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Snell, H. S. K.; Robinson, D.; Midwood, A. J.</p> <p>2014-12-01</p> <p>Measurements of δ13C of soil <span class="hlt">CO</span><span class="hlt">2</span> are used to partition the surface <span class="hlt">flux</span> into autotrophic and heterotrophic components. Models predict that the δ13<span class="hlt">CO</span><span class="hlt">2</span> of the soil efflux is perturbed by non-steady state (NSS) diffusive conditions. These could be large enough to render δ13<span class="hlt">CO</span><span class="hlt">2</span> unsuitable for accurate <span class="hlt">flux</span> partitioning. Field studies sometimes find correlations between efflux δ13<span class="hlt">CO</span><span class="hlt">2</span> and <span class="hlt">flux</span> or temperature, or that efflux δ13<span class="hlt">CO</span><span class="hlt">2</span> is not correlated as expected with biological drivers. We tested whether NSS effects in semi-natural soil were comparable with those predicted. We compared chamber designs and their sensitivity to changes in efflux δ13<span class="hlt">CO</span><span class="hlt">2</span>. In a natural soil mesocosm, we controlled temperature to generate NSS conditions of <span class="hlt">CO</span><span class="hlt">2</span> production. We measured the δ13C of soil <span class="hlt">CO</span><span class="hlt">2</span> using in situ probes to sample the subsurface, and dynamic and forced-diffusion chambers to sample the surface efflux. Over eight hours we raised soil temperature by 4.5 OC to increase microbial respiration. Subsurface <span class="hlt">CO</span><span class="hlt">2</span> concentration doubled, surface efflux became 13C-depleted by 1 ‰ and subsurface <span class="hlt">CO</span><span class="hlt">2</span> became 13C-enriched by around <span class="hlt">2</span> ‰. Opposite changes occurred when temperature was lowered and <span class="hlt">CO</span><span class="hlt">2</span> production was decreasing. Different chamber designs had inherent biases but all detected similar changes in efflux δ13<span class="hlt">CO</span><span class="hlt">2</span>, which were comparable to those predicted. Measurements using dynamic chambers were more 13C-enriched than expected, probably due to advection of <span class="hlt">CO</span><span class="hlt">2</span> into the chamber. In the mesocosm soil, δ13<span class="hlt">CO</span><span class="hlt">2</span> of both efflux and subsurface was determined by physical processes of <span class="hlt">CO</span><span class="hlt">2</span> production and diffusion. Steady state conditions are unlikely to prevail in the field, so spot measurements of δ13<span class="hlt">CO</span><span class="hlt">2</span> and assumptions based on the theoretical 4.4 ‰ diffusive fractionation will not be accurate for estimating source δ13<span class="hlt">CO</span><span class="hlt">2</span>. Continuous measurements could be integrated over a period suitable to reduce the influence of transient NSS conditions. It will be difficult to disentangle</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013BGeo...10.3109C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013BGeo...10.3109C"><span>Implications of elevated <span class="hlt">CO</span><span class="hlt">2</span> on pelagic carbon <span class="hlt">fluxes</span> in an Arctic mesocosm study - an elemental mass balance approach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Czerny, J.; Schulz, K. G.; Boxhammer, T.; Bellerby, R. G. J.; Büdenbender, J.; Engel, A.; Krug, S. A.; Ludwig, A.; Nachtigall, K.; Nondal, G.; Niehoff, B.; Silyakova, A.; Riebesell, U.</p> <p>2013-05-01</p> <p>Recent studies on the impacts of ocean acidification on pelagic communities have identified changes in carbon to nutrient dynamics with related shifts in elemental stoichiometry. In principle, mesocosm experiments provide the opportunity of determining temporal dynamics of all relevant carbon and nutrient pools and, thus, calculating elemental budgets. In practice, attempts to budget mesocosm enclosures are often hampered by uncertainties in some of the measured pools and <span class="hlt">fluxes</span>, in particular due to uncertainties in constraining <span class="hlt">air-sea</span> gas exchange, particle sinking, and wall growth. In an Arctic mesocosm study on ocean acidification applying KOSMOS (Kiel Off-Shore Mesocosms for future Ocean Simulation), all relevant element pools and <span class="hlt">fluxes</span> of carbon, nitrogen and phosphorus were measured, using an improved experimental design intended to narrow down the mentioned uncertainties. Water-column concentrations of particulate and dissolved organic and inorganic matter were determined daily. New approaches for quantitative estimates of material sinking to the bottom of the mesocosms and gas exchange in 48 h temporal resolution as well as estimates of wall growth were developed to close the gaps in element budgets. However, losses elements from the budgets into a sum of insufficiently determined pools were detected, and are principally unavoidable in mesocosm investigation. The comparison of variability patterns of all single measured datasets revealed analytic precision to be the main issue in determination of budgets. Uncertainties in dissolved organic carbon (DOC), nitrogen (DON) and particulate organic phosphorus (POP) were much higher than the summed error in determination of the same elements in all other pools. With estimates provided for all other major elemental pools, mass balance calculations could be used to infer the temporal development of DOC, DON and POP pools. Future elevated p<span class="hlt">CO</span><span class="hlt">2</span> was found to enhance net autotrophic community carbon uptake in two of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.B51B0544R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.B51B0544R"><span>Year-round record of Dry Valley soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> provides insights into Antarctic soil dynamics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Risk, D. A.; Lee, C.; Macintyre, C. M.; Cary, C.</p> <p>2012-12-01</p> <p>The McMurdo Dry Valleys of Antarctica host extreme soil microbial communities that have been extensively studied within the past decade. Activity of microbial communities is routinely measured via soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span>, and some useful Antarctic measurements have been made during short Austral summers. These studies are mostly spatial in nature, but temporal patterns are also valuable and may provide insights into critical thresholds and the interplay between various mechanisms that drive <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> and its variation. New membrane-based Forced Diffusion (FD) soil efflux techniques offer promise for this application. The purpose of this study was to use a specially designed FD instrument in Hidden Valley of the Antarctic Dry Valleys to evaluate hardware performance in year-round deployments, and to identify features of interest with respect to soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> variation. Overall, the deployment was successful. Small but sustained positive <span class="hlt">fluxes</span> were present only twice during the year. The first such event was small but consistent and of long duration, occurring in the Austral winter. The second was more volatile and likely of microbial origin, and appeared for roughly a month at the end of the calendar year within the Austral summer. The observed patterns suggest that Hidden Valley soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> are not solely biological in nature, but likely modulated by a combination of biological, geological, and physical processes, which will be discussed in this presentation. In future studies, additional measurement locations, and simultaneous subsurface and lower atmospheric gradient concentration measurements (power-permitting) would be extremely valuable for interpreting measured <span class="hlt">fluxes</span>, to help identify advective depletion events, the depth source of <span class="hlt">fluxes</span>, and changes in soil and atmospheric diffusivities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.B41G2054B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.B41G2054B"><span>Carbon <span class="hlt">Fluxes</span> and Transport Along the Terrestrial Aquatic Continuum</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Butman, D. E.; Kolka, R.; Fennel, K.; Stackpoole, S. M.; Trettin, C.; Windham-Myers, L.</p> <p>2017-12-01</p> <p>Terrestrial wetlands, inland surface waters, tidal wetlands and estuaries, and the coastal ocean are distinct aquatic ecosystems that integrate carbon (C) <span class="hlt">fluxes</span> and processing among the major earth system components: the continents, oceans, and atmosphere. The development of the <span class="hlt">2</span>nd State of the Carbon Cycle Report (SOCCR<span class="hlt">2</span>) noted that incorporating the C cycle dynamics for these ecosystems was necessary to reconcile some of the gaps associated with the North American C budget. We present major C stocks and <span class="hlt">fluxes</span> for Canada, Mexico and the United States. North America contains nearly 42% of the global terrestrial wetland area. Terrestrial wetlands, defined as soils that are seasonally or permanently inundated or saturated, contain significant C stocks equivalent to 174,000 Tg C in the top 40 cm of soil. While terrestrial wetlands are a C sink of approximately 64 Tg C yr-1, they also emit 21 Tg of CH4 yr-1. Inland waters are defined as lakes, reservoirs, rivers, and streams. Carbon <span class="hlt">fluxes</span>, which include lateral C export to the coast, riverine and lacustrine <span class="hlt">CO</span><span class="hlt">2</span> emissions, and C burial in lakes and reservoirs are estimated at 507 Tg yr-1. Estuaries and tidal wetlands assimilate C and nutrients from uplands and rivers, and their total C stock is 1,323 Tg C in the top 1 m of soils and sediment. Accounting for soil accretion, lateral C <span class="hlt">flux</span>, and <span class="hlt">CO</span><span class="hlt">2</span> assimilation and emission, tidal wetlands and estuaries are net sinks with a total <span class="hlt">flux</span> equal to 6 Tg C yr-1. The coastal ocean and <span class="hlt">sea</span> shelfs, defined as non-estuarine waters within 200 nautical miles (370 km) of the coast, function as net sinks, with the <span class="hlt">air-sea</span> exchange of <span class="hlt">CO</span><span class="hlt">2</span> estimated at 150 Tg C yr-1. In total, <span class="hlt">fluxes</span> from these four aquatic ecosystems are equal to a loss of 302 Tg C yr-1. Including these four discrete <span class="hlt">fluxes</span> in this assessment demonstrates the importance of linking hydrology and biogeochemical cycling to evaluate the impacts of climate change and human activities on carbon <span class="hlt">fluxes</span> across the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.A33F0242W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.A33F0242W"><span>An Inversion Analysis of Recent Variability in Natural <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Fluxes</span> Using GOSAT and In Situ Observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, J. S.; Kawa, S. R.; Baker, D. F.; Collatz, G. J.; Ott, L. E.</p> <p>2015-12-01</p> <p>About one-half of the global <span class="hlt">CO</span><span class="hlt">2</span> emissions from fossil fuel combustion and deforestation accumulates in the atmosphere, where it contributes to global warming. The rest is taken up by vegetation and the ocean. The precise contribution of the two sinks, and their location and year-to-year variability are, however, not well understood. We use two different approaches, batch Bayesian synthesis inversion and variational data assimilation, to deduce the global spatiotemporal distributions of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> during 2009-2010. One of our objectives is to assess different sources of uncertainties in inferred <span class="hlt">fluxes</span>, including uncertainties in prior <span class="hlt">flux</span> estimates and observations, and differences in inversion techniques. For prior constraints, we utilize <span class="hlt">fluxes</span> and uncertainties from the CASA-GFED model of the terrestrial biosphere and biomass burning driven by satellite observations and interannually varying meteorology. We also use measurement-based ocean <span class="hlt">flux</span> estimates and two sets of fixed fossil <span class="hlt">CO</span><span class="hlt">2</span> emissions. Here, our inversions incorporate column <span class="hlt">CO</span><span class="hlt">2</span> measurements from the GOSAT satellite (ACOS retrieval, filtered and bias-corrected) and in situ observations (individual flask and afternoon-average continuous observations) to estimate <span class="hlt">fluxes</span> in 108 regions over 8-day intervals for the batch inversion and at 3° x 3.75° weekly for the variational system. Relationships between <span class="hlt">fluxes</span> and atmospheric concentrations are derived consistently for the two inversion systems using the PCTM atmospheric transport model driven by meteorology from the MERRA reanalysis. We compare the posterior <span class="hlt">fluxes</span> and uncertainties derived using different data sets and the two inversion approaches, and evaluate the posterior atmospheric concentrations against independent data including aircraft measurements. The optimized <span class="hlt">fluxes</span> generally resemble those from other studies. For example, the results indicate that the terrestrial biosphere is a net <span class="hlt">CO</span><span class="hlt">2</span> sink, and a GOSAT-only inversion suggests a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160000370','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160000370"><span>An Inversion Analysis of Recent Variability in Natural <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Fluxes</span> Using GOSAT and In Situ Observations</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wang, James S.; Kawa, S. Randolph; Collatz, G. James; Baker, David F.; Ott, Lesley</p> <p>2015-01-01</p> <p>About one-half of the global <span class="hlt">CO</span><span class="hlt">2</span> emissions from fossil fuel combustion and deforestation accumulates in the atmosphere, where it contributes to global warming. The rest is taken up by vegetation and the ocean. The precise contribution of the two sinks, and their location and year-to-year variability are, however, not well understood. We use two different approaches, batch Bayesian synthesis inversion and variational data assimilation, to deduce the global spatiotemporal distributions of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> during 2009-2010. One of our objectives is to assess different sources of uncertainties in inferred <span class="hlt">fluxes</span>, including uncertainties in prior <span class="hlt">flux</span> estimates and observations, and differences in inversion techniques. For prior constraints, we utilize <span class="hlt">fluxes</span> and uncertainties from the CASA-GFED model of the terrestrial biosphere and biomass burning driven by satellite observations and interannually varying meteorology. We also use measurement-based ocean <span class="hlt">flux</span> estimates and two sets of fixed fossil <span class="hlt">CO</span><span class="hlt">2</span> emissions. Here, our inversions incorporate column <span class="hlt">CO</span><span class="hlt">2</span> measurements from the GOSAT satellite (ACOS retrieval, filtered and bias-corrected) and in situ observations (individual flask and afternoon-average continuous observations) to estimate <span class="hlt">fluxes</span> in 108 regions over 8-day intervals for the batch inversion and at 3 x 3.75 weekly for the variational system. Relationships between <span class="hlt">fluxes</span> and atmospheric concentrations are derived consistently for the two inversion systems using the PCTM atmospheric transport model driven by meteorology from the MERRA reanalysis. We compare the posterior <span class="hlt">fluxes</span> and uncertainties derived using different data sets and the two inversion approaches, and evaluate the posterior atmospheric concentrations against independent data including aircraft measurements. The optimized <span class="hlt">fluxes</span> generally resemble those from other studies. For example, the results indicate that the terrestrial biosphere is a net <span class="hlt">CO</span><span class="hlt">2</span> sink, and a GOSAT-only inversion suggests a shift in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28434669','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28434669"><span>Diurnal variation of <span class="hlt">CO</span><span class="hlt">2</span>, CH4, and N<span class="hlt">2</span>O emission <span class="hlt">fluxes</span> continuously monitored in-situ in three environmental habitats in a subtropical estuarine wetland.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yang, Wen-Bin; Yuan, Chung-Shin; Tong, Chuan; Yang, Pin; Yang, Lei; Huang, Bang-Qin</p> <p>2017-06-15</p> <p>Wetlands play a crucial role in modulating atmospheric concentrations of greenhouse gases (GHGs) such as carbon dioxide (<span class="hlt">CO</span> <span class="hlt">2</span> ), methane (CH 4 ), and nitrous oxide (N <span class="hlt">2</span> O). The key factors controlling GHG emission from subtropical estuarine wetlands were investigated in this study, which continuously monitored the uptake/emission of GHGs (<span class="hlt">CO</span> <span class="hlt">2</span> , CH 4 , and N <span class="hlt">2</span> O) by/from a subtropical estuarine wetland located in the Minjiang estuary in the coastal region of southeastern China. A self-designed floating chamber was used to collect <span class="hlt">air</span> samples on-site at three environmental habitats (Phragmites australis marsh, mudflats, and river water). The <span class="hlt">CO</span> <span class="hlt">2</span> , CH 4 , and N <span class="hlt">2</span> O concentrations were then measured using an automated nondispersive infrared analyzer. The magnitudes of the <span class="hlt">CO</span> <span class="hlt">2</span> and N <span class="hlt">2</span> O emission <span class="hlt">fluxes</span> at the three habitats were ordered as river water>P. australis>mudflats. P. australis emitted GHGs through photosynthesis and respiration processes. Emissions of CH 4 from P. australis and the mudflats were revealed to be slightly higher than those from the river water. The total GHG emission <span class="hlt">fluxes</span> at the three environmental habitats were quite similar (4.68-4.78gm -<span class="hlt">2</span> h -1 ). However, when the total carbon dioxide equivalent <span class="hlt">fluxes</span> (<span class="hlt">CO</span> <span class="hlt">2</span> -e) were considered, the river water was discovered to emit the most <span class="hlt">CO</span> <span class="hlt">2</span> -e compared with P. australis and the mudflats. Based on its potential to increase global warming, N <span class="hlt">2</span> O was the main contributor to the total GHG emission, with that emitted from the river water being the most considerable. Tidal water carried onto the marsh had its own GHG content and thus has acted as a source or sink of GHGs. However, water quality had a large effect on GHG emissions from the river water whereas the tidal water height did not. Both high salinity and large amounts of sulfates in the wetlands explicitly inhibited the activity of CH 4 -producing bacteria, particularly at nighttime. Copyright © 2017 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20080030789&hterms=erickson&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Derickson','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20080030789&hterms=erickson&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Derickson"><span>Evaluating the Capacity of Global <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Flux</span> and Atmospheric Transport Models to Incorporate New Satellite Observations</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kawa, S. R.; Collatz, G. J.; Erickson, D. J.; Denning, A. S.; Wofsy, S. C.; Andrews, A. E.</p> <p>2007-01-01</p> <p>As we enter the new era of satellite remote sensing for <span class="hlt">CO</span><span class="hlt">2</span> and other carbon cyclerelated quantities, advanced modeling and analysis capabilities are required to fully capitalize on the new observations. Model estimates of <span class="hlt">CO</span><span class="hlt">2</span> surface <span class="hlt">flux</span> and atmospheric transport are required for initial constraints on inverse analyses, to connect atmospheric observations to the location of surface sources and sinks, and ultimately for future projections of carbon-climate interactions. For application to current, planned, and future remotely sensed <span class="hlt">CO</span><span class="hlt">2</span> data, it is desirable that these models are accurate and unbiased at time scales from less than daily to multi-annual and at spatial scales from several kilometers or finer to global. Here we focus on simulated <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> from terrestrial vegetation and atmospheric transport mutually constrained by analyzed meteorological fields from the Goddard Modeling and Assimilation Office for the period 1998 through 2006. Use of assimilated meteorological data enables direct model comparison to observations across a wide range of scales of variability. The biospheric <span class="hlt">fluxes</span> are produced by the CASA model at lxi degrees on a monthly mean basis, modulated hourly with analyzed temperature and sunlight. Both physiological and biomass burning <span class="hlt">fluxes</span> are derived using satellite observations of vegetation, burned area (as in GFED-<span class="hlt">2</span>), and analyzed meteorology. For the purposes of comparison to <span class="hlt">CO</span><span class="hlt">2</span> data, fossil fuel and ocean <span class="hlt">fluxes</span> are also included in the transport simulations. In this presentation we evaluate the model's ability to simulate <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> and mixing ratio variability in comparison to in situ observations at sites in Northern mid latitudes and the continental tropics. The influence of key process representations is inferred. We find that the model can resolve much of the hourly to synoptic variability in the observations, although there are limits imposed by vertical resolution of boundary layer processes. The seasonal cycle and its</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_23 --> <div id="page_24" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="461"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUSM.A23B..01K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUSM.A23B..01K"><span><span class="hlt">Air-Sea</span> Interaction in the Gulf of Tehuantepec</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Khelif, D.; Friehe, C. A.; Melville, W. K.</p> <p>2007-05-01</p> <p>Measurements of meteorological fields and turbulence were made during gap wind events in the Gulf of Tehuantepec using the NSF C-130 aircraft. The flight patterns started at the shore and progressed to approximately 300km offshore with low-level (30m) tracks, stacks and soundings. Parameterizations of the wind stress, sensible and latent heat <span class="hlt">fluxes</span> were obtained from approximately 700 5 km low-level tracks. Structure of the marine boundary layer as it evolved off-shore was obtained with stack patterns, aircraft soundings and deployment of dropsondes. The <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> approximately follow previous parameterizations with some evidence of the drag coefficient leveling out at about 20 meters/sec with the latent heat <span class="hlt">flux</span> slightly increasing. The boundary layer starts at shore as a gap wind low-level jet, thins as the jet expands out over the gulf, exhibits a hydraulic jump, and then increases due to turbulent mixing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.B21F2017D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.B21F2017D"><span>Characterization And Partitioning Of CH4 And <span class="hlt">CO</span><span class="hlt">2</span> Eddy <span class="hlt">Flux</span> Data Measured at NGEE-Arctic Sites</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dengel, S.; Chafe, O.; Curtis, J. B.; Biraud, S.; Torn, M. S.; Wullschleger, S. D.</p> <p>2017-12-01</p> <p>The high latitudes are experiencing rapid warming with permafrost ecosystems being highly vulnerable to this change. Since the advancement in Eddy Covariance (EC) measurements, the number of high latitude sites measuring greenhouse gases and energy (<span class="hlt">CO</span><span class="hlt">2</span>, CH4 and H<span class="hlt">2</span>O) <span class="hlt">fluxes</span> is steadily increasing, with new sites being established each year. Data from these sites are not only valuable for annual carbon budget calculations, but also vital to the modeling community for improving their predictions of emission rates and trends. CH4 <span class="hlt">flux</span> measurements are not as straightforward as <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. They tend to be less predictable or as easily interpretable as <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. Understanding CH4 emission patterns are often challenging. Moreover, gas <span class="hlt">flux</span> fluctuations are spatially and temporally diverse, and in many cases event-based. An improvement in understanding would also contribute to improvements in the fidelity of model predictions. These rely on having high quality data, and thus will entail developing new QA/QC and gap-filling methods for Arctic systems, in particularly for CH4. Contributing to these challenges is the limited number of ancillary measurements carried out at many sites and the lack of standardized data processing, QA/QC, and gap-filling procedures, in particular for CH4. <span class="hlt">CO</span><span class="hlt">2</span>, CH4, and energy <span class="hlt">flux</span> measurements are ongoing at, both NGEE-Arctic/Ameri<span class="hlt">Flux</span>, US-NGB (Arctic coastal plain), and US-NGC (subarctic tussock tundra) sites. The sites, with underlying continuous permafrost, show a high degree of inter-annual and seasonal variability in CH4 <span class="hlt">fluxes</span>. In order to interpret this variability, we apply a variety of models, such as footprint characterization, generalized additive models, as well as artificial neural networks, in an attempt to decipher these diverse <span class="hlt">fluxes</span>, patterns and events.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JVGR..320...50I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JVGR..320...50I"><span>Geochemical characterisation of gases along the dead <span class="hlt">sea</span> rift: Evidences of mantle-<span class="hlt">co</span><span class="hlt">2</span> degassing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Inguaggiato, C.; Censi, P.; D'Alessandro, W.; Zuddas, P.</p> <p>2016-06-01</p> <p>The Dead <span class="hlt">Sea</span> Transform (DST) fault system, where a lateral displacement between the African and Arabian plates occurs, is characterised by anomalous heat <span class="hlt">flux</span> in the Israeli area close to the border with Syria and Jordan. The concentration of He and <span class="hlt">CO</span><span class="hlt">2</span>, and isotopic composition of He and total dissolved inorganic carbon were studied in cold and thermal waters collected along the DST, in order to investigate the source of volatiles and their relationship with the tectonic framework of the DST. The waters with higher temperature (up to 57.<span class="hlt">2</span> °C) are characterised by higher amounts of <span class="hlt">CO</span><span class="hlt">2</span> and helium (up to 55.72 and 1.91 ∗ 10- <span class="hlt">2</span> cc l- 1, respectively). Helium isotopic data (R/Ra from 0.11 to <span class="hlt">2</span>.14) and 4He/20Ne ratios (0.41-106.86) show the presence of deep-deriving fluids consisting of a variable mixture of mantle and crust end-members, with the former reaching up to 35%. Carbon isotope signature of total dissolved carbon from hot waters falls within the range of magmatic values, suggesting the delivery of deep-seated <span class="hlt">CO</span><span class="hlt">2</span>. The geographical distribution of helium isotopic data and isotopic carbon (<span class="hlt">CO</span><span class="hlt">2</span>) values coupled with (<span class="hlt">CO</span><span class="hlt">2</span>/3He ratios) indicate a larger contribution of mantle-derived fluids affecting the northern part of the investigated area, where the waters reach the highest temperature. These evidences suggest the occurrence of a favourable tectonic framework, including a Moho discontinuity up-rise and/or the presence of a deep fault system coupled with the recent magmatic activity recognised in the northern part of Israel.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5544137','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5544137"><span>Simultaneously reducing <span class="hlt">CO</span><span class="hlt">2</span> and particulate exposures via fractional recirculation of vehicle cabin <span class="hlt">air</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Jung, Heejung S.; Grady, Michael L.; Victoroff, Tristan; Miller, Arthur L.</p> <p>2017-01-01</p> <p>Prior studies demonstrate that <span class="hlt">air</span> recirculation can reduce exposure to nanoparticles in vehicle cabins. However when people occupy confined spaces, <span class="hlt">air</span> recirculation can lead to carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) accumulation which can potentially lead to deleterious effects on cognitive function. This study proposes a fractional <span class="hlt">air</span> recirculation system for reducing nanoparticle concentration while simultaneously suppressing <span class="hlt">CO</span><span class="hlt">2</span> levels in the cabin. Several recirculation scenarios were tested using a custom-programmed HVAC (heat, ventilation, <span class="hlt">air</span> conditioning) unit that varied the recirculation door angle in the test vehicle. Operating the recirculation system with a standard cabin filter reduced particle concentrations to 1000 particles/cm3, although <span class="hlt">CO</span><span class="hlt">2</span> levels rose to 3000 ppm. When as little as 25% fresh <span class="hlt">air</span> was introduced (75% recirculation), <span class="hlt">CO</span><span class="hlt">2</span> levels dropped to 1000 ppm, while particle concentrations remained below 5000 particles/cm3. We found that nanoparticles were removed selectively during recirculation and demonstrated the trade-off between cabin <span class="hlt">CO</span><span class="hlt">2</span> concentration and cabin particle concentration using fractional <span class="hlt">air</span> recirculation. Data showed significant increases in <span class="hlt">CO</span><span class="hlt">2</span> levels during 100% recirculation. For various fan speeds, recirculation fractions of 50–75% maintained lower <span class="hlt">CO</span><span class="hlt">2</span> levels in the cabin, while still reducing particulate levels. We recommend fractional recirculation as a simple method to reduce occupants’ exposures to particulate matter and <span class="hlt">CO</span><span class="hlt">2</span> in vehicles. A design with several fractional recirculation settings could allow <span class="hlt">air</span> exchange adequate for reducing both particulate and <span class="hlt">CO</span><span class="hlt">2</span> exposures. Developing this technology could lead to reductions in airborne nanoparticle exposure, while also mitigating safety risks from <span class="hlt">CO</span><span class="hlt">2</span> accumulation. PMID:28781568</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28781568','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28781568"><span>Simultaneously reducing <span class="hlt">CO</span><span class="hlt">2</span> and particulate exposures via fractional recirculation of vehicle cabin <span class="hlt">air</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Jung, Heejung S; Grady, Michael L; Victoroff, Tristan; Miller, Arthur L</p> <p>2017-07-01</p> <p>Prior studies demonstrate that <span class="hlt">air</span> recirculation can reduce exposure to nanoparticles in vehicle cabins. However when people occupy confined spaces, <span class="hlt">air</span> recirculation can lead to carbon dioxide (<span class="hlt">CO</span> <span class="hlt">2</span> ) accumulation which can potentially lead to deleterious effects on cognitive function. This study proposes a fractional <span class="hlt">air</span> recirculation system for reducing nanoparticle concentration while simultaneously suppressing <span class="hlt">CO</span> <span class="hlt">2</span> levels in the cabin. Several recirculation scenarios were tested using a custom-programmed HVAC (heat, ventilation, <span class="hlt">air</span> conditioning) unit that varied the recirculation door angle in the test vehicle. Operating the recirculation system with a standard cabin filter reduced particle concentrations to 1000 particles/cm 3 , although <span class="hlt">CO</span> <span class="hlt">2</span> levels rose to 3000 ppm. When as little as 25% fresh <span class="hlt">air</span> was introduced (75% recirculation), <span class="hlt">CO</span> <span class="hlt">2</span> levels dropped to 1000 ppm, while particle concentrations remained below 5000 particles/cm 3 . We found that nanoparticles were removed selectively during recirculation and demonstrated the trade-off between cabin <span class="hlt">CO</span> <span class="hlt">2</span> concentration and cabin particle concentration using fractional <span class="hlt">air</span> recirculation. Data showed significant increases in <span class="hlt">CO</span> <span class="hlt">2</span> levels during 100% recirculation. For various fan speeds, recirculation fractions of 50-75% maintained lower <span class="hlt">CO</span> <span class="hlt">2</span> levels in the cabin, while still reducing particulate levels. We recommend fractional recirculation as a simple method to reduce occupants' exposures to particulate matter and <span class="hlt">CO</span> <span class="hlt">2</span> in vehicles. A design with several fractional recirculation settings could allow <span class="hlt">air</span> exchange adequate for reducing both particulate and <span class="hlt">CO</span> <span class="hlt">2</span> exposures. Developing this technology could lead to reductions in airborne nanoparticle exposure, while also mitigating safety risks from <span class="hlt">CO</span> <span class="hlt">2</span> accumulation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AtmEn.160...77J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AtmEn.160...77J"><span>Simultaneously reducing <span class="hlt">CO</span><span class="hlt">2</span> and particulate exposures via fractional recirculation of vehicle cabin <span class="hlt">air</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jung, Heejung S.; Grady, Michael L.; Victoroff, Tristan; Miller, Arthur L.</p> <p>2017-07-01</p> <p>Prior studies demonstrate that <span class="hlt">air</span> recirculation can reduce exposure to nanoparticles in vehicle cabins. However when people occupy confined spaces, <span class="hlt">air</span> recirculation can lead to carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) accumulation which can potentially lead to deleterious effects on cognitive function. This study proposes a fractional <span class="hlt">air</span> recirculation system for reducing nanoparticle concentration while simultaneously suppressing <span class="hlt">CO</span><span class="hlt">2</span> levels in the cabin. Several recirculation scenarios were tested using a custom-programmed HVAC (heat, ventilation, <span class="hlt">air</span> conditioning) unit that varied the recirculation door angle in the test vehicle. Operating the recirculation system with a standard cabin filter reduced particle concentrations to 1000 particles/cm3, although <span class="hlt">CO</span><span class="hlt">2</span> levels rose to 3000 ppm. When as little as 25% fresh <span class="hlt">air</span> was introduced (75% recirculation), <span class="hlt">CO</span><span class="hlt">2</span> levels dropped to 1000 ppm, while particle concentrations remained below 5000 particles/cm3. We found that nanoparticles were removed selectively during recirculation and demonstrated the trade-off between cabin <span class="hlt">CO</span><span class="hlt">2</span> concentration and cabin particle concentration using fractional <span class="hlt">air</span> recirculation. Data showed significant increases in <span class="hlt">CO</span><span class="hlt">2</span> levels during 100% recirculation. For various fan speeds, recirculation fractions of 50-75% maintained lower <span class="hlt">CO</span><span class="hlt">2</span> levels in the cabin, while still reducing particulate levels. We recommend fractional recirculation as a simple method to reduce occupants' exposures to particulate matter and <span class="hlt">CO</span><span class="hlt">2</span> in vehicles. A design with several fractional recirculation settings could allow <span class="hlt">air</span> exchange adequate for reducing both particulate and <span class="hlt">CO</span><span class="hlt">2</span> exposures. Developing this technology could lead to reductions in airborne nanoparticle exposure, while also mitigating safety risks from <span class="hlt">CO</span><span class="hlt">2</span> accumulation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.B22A..03W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.B22A..03W"><span>Annual dynamics of N<span class="hlt">2</span>O, CH4 and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> from the agricultural irrigation watersheds in southeast China</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wu, S.; Zou, J.; Liu, S.; Chen, J.; Kong, D.; Geng, Y.</p> <p>2017-12-01</p> <p>Agricultural irrigation watershed covers a large area in southeast of China and is a potentially important source of carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>), methane (CH4) and nitrous oxide (N<span class="hlt">2</span>O). However, the <span class="hlt">flux</span> magnitudes contribution to the overall catchment greenhouse gas (GHGs) <span class="hlt">fluxes</span> and their drivers of seasonal variability are limited in agricultural irrigation watersheds. An in-situ observation was performed to measure annual <span class="hlt">CO</span><span class="hlt">2</span>, CH4 and N<span class="hlt">2</span>O <span class="hlt">fluxes</span> from an agricultural irrigation watershed in southeast of China from September 2014 to September 2016. GHGs <span class="hlt">fluxes</span> were measured using floating chambers and a gas exchange model was also used to predict CH4 and N<span class="hlt">2</span>O <span class="hlt">fluxes</span>. All GHGs showed varied seasonally with highest <span class="hlt">fluxes</span> in early summer (July) and lowest in winter. Estimated seasonal CH4-C <span class="hlt">fluxes</span> (11.5-97.6 mg m-<span class="hlt">2</span> hr-1) and N<span class="hlt">2</span>O-N <span class="hlt">fluxes</span> (<span class="hlt">2</span>.8-80.8μg m-<span class="hlt">2</span> hr-1) were in relative agreement with measured CH4-C <span class="hlt">fluxes</span> (0.05-74.9mg m-<span class="hlt">2</span> hr-1) and N<span class="hlt">2</span>O-N <span class="hlt">fluxes</span> (3.9-68.7μg m-<span class="hlt">2</span> hr-1) <span class="hlt">fluxes</span> using floating chambers. Both CH4 and N<span class="hlt">2</span>O <span class="hlt">fluxes</span> were positively related to water temperature. The CH4 <span class="hlt">fluxes</span> were negatively related to water dissolved oxygen (DO) concentration but positively related to sediment dissolved organic carbon (DOC). The N<span class="hlt">2</span>O <span class="hlt">fluxes</span> were positively related to water NH4+ and NO3-. The calculated EF5-r value in this study (mean = 0.0016; range = 0.0013-0.0018) was below the current IPCC (2006) default value of 0.0025. This implied that IPCC methodology may over estimates of N<span class="hlt">2</span>O emissions associated with nitrogen leaching and runoff from agriculture.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016BGeo...13.6107V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016BGeo...13.6107V"><span>The role of Phragmites in the CH4 and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> in a minerotrophic peatland in southwest Germany</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>van den Berg, Merit; Ingwersen, Joachim; Lamers, Marc; Streck, Thilo</p> <p>2016-11-01</p> <p>Peatlands are interesting as a carbon storage option, but are also natural emitters of the greenhouse gas methane (CH4). Phragmites peatlands are particularly interesting due to the global abundance of this wetland plant (Phragmites australis) and the highly efficient internal gas transport mechanism, which is called humidity-induced convection (HIC). The research aims were to (1) clarify how this plant-mediated gas transport influences the CH4 <span class="hlt">fluxes</span>, (<span class="hlt">2</span>) which other environmental variables influence the <span class="hlt">CO</span><span class="hlt">2</span> and CH4 <span class="hlt">fluxes</span>, and (3) whether Phragmites peatlands are a net source or sink of greenhouse gases. <span class="hlt">CO</span><span class="hlt">2</span> and CH4 <span class="hlt">fluxes</span> were measured with the eddy covariance technique within a <span style="" class="text">Phragmites-dominated fen in southwest Germany. One year of <span class="hlt">flux</span> data (March 2013-February 2014) shows very clear diurnal and seasonal patterns for both <span class="hlt">CO</span><span class="hlt">2</span> and CH4. The diurnal pattern of CH4 <span class="hlt">fluxes</span> was only visible when living, green reed was present. In August the diurnal cycle of CH4 was the most distinct, with 11 times higher midday <span class="hlt">fluxes</span> (15.7 mg CH4 m-<span class="hlt">2</span> h-1) than night <span class="hlt">fluxes</span> (1.41 mg CH4 m-<span class="hlt">2</span> h-1). This diurnal cycle has the highest correlation with global radiation, which suggests a high influence of the plants on the CH4 <span class="hlt">flux</span>. But if the cause were the HIC, it would be expected that relative humidity would correlate stronger with CH4 <span class="hlt">flux</span>. Therefore, we conclude that in addition to HIC, at least one additional mechanism must be involved in the creation of the convective flow within the Phragmites plants. Overall, the fen was a sink for carbon and greenhouse gases in the measured year, with a total carbon uptake of 221 g C m-<span class="hlt">2</span> yr-1 (26 % of the total assimilated carbon). The net uptake of greenhouse gases was 52 g <span class="hlt">CO</span><span class="hlt">2</span> eq. m-<span class="hlt">2</span> yr-1, which is obtained from an uptake of <span class="hlt">CO</span><span class="hlt">2</span> of 894 g <span class="hlt">CO</span><span class="hlt">2</span> eq. m-<span class="hlt">2</span> yr-1 and a release of CH4 of 842 g <span class="hlt">CO</span><span class="hlt">2</span> eq. m-<span class="hlt">2</span> yr-1.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.B51H0526M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.B51H0526M"><span>Estimating <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Fluxes</span> Pre and Post Drought Using Remote Sensing Data in the Sierra Nevada Range</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mazzi, J. R.; Grigsby, S.; Goulden, M.; Ustin, S.</p> <p>2015-12-01</p> <p>The recent California drought presents an opportunity to study <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> changes over time due to insufficient water uptake by plant life using remote sensing data. Three <span class="hlt">flux</span> towers were used to create linear regressions between AVIRIS derived Net Ecosystem Exchange (NEE = PRI * NDVI * PAR) and tower measured <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> in the San Joaquin Experimental Range. To estimate <span class="hlt">CO</span><span class="hlt">2</span> from NEE, two linear regressions were used based on time of day and season, with R<span class="hlt">2</span> values of 0.85 and 0.87 respectively. Per-pixel <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> was estimated for AVIRIS flights flown in June 2013, 2014, and 2015, as well as September 2011 and October 2014. There was a significant decrease in post drought photosynthetic <span class="hlt">CO</span><span class="hlt">2</span> uptake over the 6,700 km<span class="hlt">2</span> studied, totaling <span class="hlt">2</span>,977 grams per minute less (15.9% decrease) from June 2013 to June 2014. Data from the 2015 HyspIRI flights suggest a continuation of this trend for June 2015. Pre-drought conditions over a 33 km<span class="hlt">2</span> area show that the photosynthetic <span class="hlt">CO</span><span class="hlt">2</span> uptake dropped from 74 mg per minute on September 24, 2011, to 35 mg per minute on October 6, 2014 (a 53% decrease). HyspIRI flight lines also include 434 km<span class="hlt">2</span> of the Rim Fire, an area that saw a decrease in <span class="hlt">CO</span><span class="hlt">2</span> uptake of 413 grams per minute (71.7% decrease from June 2013 to June 2014) from the burn alone. It is estimated that the entire Rim Fire (1,041 km<span class="hlt">2</span>) has caused a total decrease in photosynthetic <span class="hlt">CO</span><span class="hlt">2</span> uptake totaling 988 grams less per minute from 2013 to 2014, with some recovery evident in 2015.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AtmEn..99..546A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AtmEn..99..546A"><span>Quantifying the <span class="hlt">air</span> quality-<span class="hlt">CO</span><span class="hlt">2</span> tradeoff potential for airports</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ashok, Akshay; Dedoussi, Irene C.; Yim, Steve H. L.; Balakrishnan, Hamsa; Barrett, Steven R. H.</p> <p>2014-12-01</p> <p>Aircraft movements on the airport surface are responsible for <span class="hlt">CO</span><span class="hlt">2</span> emissions that contribute to climate change and other emissions that affect <span class="hlt">air</span> quality and human health. While the potential for optimizing aircraft surface movements to minimize <span class="hlt">CO</span><span class="hlt">2</span> emissions has been assessed, the implications of <span class="hlt">CO</span><span class="hlt">2</span> emissions minimization for <span class="hlt">air</span> quality have not been quantified. In this paper, we identify conditions in which there is a tradeoff between <span class="hlt">CO</span><span class="hlt">2</span> emissions and population exposure to O3 and secondary PM<span class="hlt">2</span>.5 - i.e. where decreasing fuel burn (which is directly proportional to <span class="hlt">CO</span><span class="hlt">2</span> emissions) results in increased exposure. Fuel burn and emissions are estimated as a function of thrust setting for five common gas turbine engines at 34 US airports. Regional <span class="hlt">air</span> quality impacts, which are dominated by ozone and secondary PM<span class="hlt">2</span>.5, are computed as a function of airport location and time using the adjoint of the GEOS-Chem chemistry-transport model. Tradeoffs between <span class="hlt">CO</span><span class="hlt">2</span> emissions and population exposure to PM<span class="hlt">2</span>.5 and O3 occur between <span class="hlt">2</span>-18% and 5-60% of the year, respectively, depending on airport location, engine type, and thrust setting. The total duration of tradeoff conditions is 5-12 times longer at maximum thrust operations (typical for takeoff) relative to 4% thrust operations (typical for taxiing). Per kilogram of additional fuel burn at constant thrust setting during tradeoff conditions, reductions in population exposure to PM<span class="hlt">2</span>.5 and O3 are 6-13% and 32-1060% of the annual average (positive) population exposure per kilogram fuel burn, where the ranges encompass the medians over the 34 airports. For fuel burn increases due to thrust increases (i.e. for constant operating time), reductions in both PM<span class="hlt">2</span>.5 and O3 exposure are 1.5-6.4 times larger in magnitude than those due to increasing fuel burn at constant thrust (i.e. increasing operating time). Airports with relatively high population exposure reduction potentials - which occur due to a combination of high duration and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1613217Q','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1613217Q"><span>Temporal changes in soil water repellency linked to the soil respiration and CH4 and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Qassem, Khalid; Urbanek, Emilia; van Keulen, Geertje</p> <p>2014-05-01</p> <p>Soil water repellency (SWR) is known to be a spatially and temporally variable phenomenon. The seasonal changes in soil moisture lead to development of soil water repellency, which in consequence may affect the microbial activity and in consequence alter the <span class="hlt">CO</span><span class="hlt">2</span> and CH4 <span class="hlt">fluxes</span> from soils. Soil microbial activity is strongly linked to the temperature and moisture status of the soil. In terms of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> intermediate moisture contents are most favourable for the optimal microbial activity and highest <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. Methanogenesis occurs primarily in anaerobic water-logged habitats while methanotrophy is a strictly aerobic process. In the study we hypothesise that the changes in <span class="hlt">CO</span><span class="hlt">2</span> and CH4 <span class="hlt">fluxes</span> are closely linked to critical moisture thresholds for soil water repellency. This research project aims to adopt a multi-disciplinary approach to comprehensively determine the effect of SWR on <span class="hlt">CO</span><span class="hlt">2</span> and CH4 <span class="hlt">fluxes</span>. Research is conducted in situ at four sites exhibiting SWR in the southern UK. <span class="hlt">Flux</span> measurements are carried out concomitant with meteorological and SWR observations Field observations are supported by laboratory measurements carried out on intact soil samples collected at the above identified field sites. The laboratory analyses are conducted under constant temperatures with controlled changes of soil moisture content. Methanogenic and Methanotrophic microbial populations are being analysed at different SWR and moisture contents using the latest metagenomic and metatranscriptomic approaches. Currently available data show that greenhouse gas <span class="hlt">flux</span> are closely linked with soil moisture thresholds for SWR development.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/11538164','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/11538164"><span>Return of the coral reef hypothesis: basin to shelf partitioning of Ca<span class="hlt">CO</span>3 and its effect on atmospheric <span class="hlt">CO</span><span class="hlt">2</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Opdyke, B N; Walker, J C</p> <p>1992-08-01</p> <p>Differences in the rate of coral reef carbonate deposition from the Pleistocene to the Holocene may account for the Quaternary variation of atmospheric <span class="hlt">CO</span><span class="hlt">2</span>. Volumes of carbonate associated with Holocene reefs require an average deposition rate of <span class="hlt">2</span>.0 x 10(13) mol/yr for the past 5 ka. In light of combined riverine, midocean ridge, and ground-water <span class="hlt">fluxes</span> of calcium to the oceans of <span class="hlt">2</span>.3 x 10(13) mol/yr, the current <span class="hlt">flux</span> of calcium carbonate to pelagic sediments must be far below the Pleistocene average of 1.<span class="hlt">2</span> x 10(13) mol/yr. We suggest that <span class="hlt">sea</span>-level change shifts the locus of carbonate deposition from the deep <span class="hlt">sea</span> to the shelves as the normal glacial-interglacial pattern of deposition for Quaternary global carbonates. To assess the impact of these changes on atmospheric <span class="hlt">CO</span><span class="hlt">2</span>, a simple numerical simulation of the global carbon cycle was developed. Atmospheric <span class="hlt">CO</span><span class="hlt">2</span> as well as calcite saturation depth and sediment responses to these carbonate deposition changes are examined. Atmospheric <span class="hlt">CO</span><span class="hlt">2</span> changes close to those observed in the Vostok ice core, approximately 80 ppm <span class="hlt">CO</span><span class="hlt">2</span>, for the Quaternary are observed as well as the approximate depth changes in percent carbonate of sediments measured in the Pacific Ocean over the same time interval.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70038049','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70038049"><span>Soil greenhouse gas <span class="hlt">fluxes</span> during wetland forest retreat along the lower Savannah River, Georgia (USA)</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Krauss, Ken W.; Whitbeck, Julie L.</p> <p>2012-01-01</p> <p>Tidal freshwater forested wetlands (tidal swamps) are periodically affected by salinity intrusion at seaward transitions with marsh, which, along with altered hydrology, may affect the balance of gaseous carbon (C) and nitrogen (N) losses from soils. We measured greenhouse gas emissions (<span class="hlt">CO</span><span class="hlt">2</span>, CH4, N<span class="hlt">2</span>O) from healthy, moderately degraded, and degraded tidal swamp soils undergoing <span class="hlt">sea</span>-level-rise-induced retreat along the lower Savannah River, Georgia, USA. Soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> ranged from 90.<span class="hlt">2</span> to 179.1 mg <span class="hlt">CO</span><span class="hlt">2</span> m-<span class="hlt">2</span> h-1 among study sites, and was the dominant greenhouse gas emitted. <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> differed among sites in some months, while CH4 and N<span class="hlt">2</span>O <span class="hlt">fluxes</span> were 0.18 mg CH4 m-<span class="hlt">2</span> h-1 and 1.23 μg N<span class="hlt">2</span>O m-<span class="hlt">2</span> h-1, respectively, with no differences among sites. Hydrology, soil temperature, and <span class="hlt">air</span> temperature, but not salinity, controlled the annual balance of soil <span class="hlt">CO</span><span class="hlt">2</span> emissions from tidal swamp soils. No clear drivers were found for CH4 or N<span class="hlt">2</span>O emissions. On occasion, large ebbing or very low tides were even found to draw <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> into the soil (dark <span class="hlt">CO</span><span class="hlt">2</span> uptake), along with CH4 and N<span class="hlt">2</span>O. Overall, we hypothesized a much greater role for salinity and site condition in controlling the suite of greenhouse gases emitted from tidal swamps than we discovered, and found that <span class="hlt">CO</span><span class="hlt">2</span> emissions-not CH4 or N<span class="hlt">2</span>O-contributed most to the global warming potential from these tidal swamp soils.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70005962','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70005962"><span>Soil greenhouse gas <span class="hlt">fluxes</span> during wetland forest retreat along the Lower Savannah River, Georgia (USA)</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Krauss, Ken W.; Whitbeck, Julie L.</p> <p>2012-01-01</p> <p>Tidal freshwater forested wetlands (tidal swamps) are periodically affected by salinity intrusion at seaward transitions with marsh, which, along with altered hydrology, may affect the balance of gaseous carbon (C) and nitrogen (N) losses from soils. We measured greenhouse gas emissions (<span class="hlt">CO</span><span class="hlt">2</span>, CH4, N<span class="hlt">2</span>O) from healthy, moderately degraded, and degraded tidal swamp soils undergoing <span class="hlt">sea</span>-level-rise-induced retreat along the lower Savannah River, Georgia, USA. Soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> ranged from 90.<span class="hlt">2</span> to 179.1 mg <span class="hlt">CO</span><span class="hlt">2</span> m-<span class="hlt">2</span> h-1 among study sites, and was the dominant greenhouse gas emitted. <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> differed among sites in some months, while CH4 and N<span class="hlt">2</span>O <span class="hlt">fluxes</span> were 0.18 mg CH4 m-<span class="hlt">2</span> h-1 and 1.23 μg N<span class="hlt">2</span>O m-<span class="hlt">2</span> h-1, respectively, with no differences among sites. Hydrology, soil temperature, and <span class="hlt">air</span> temperature, but not salinity, controlled the annual balance of soil <span class="hlt">CO</span><span class="hlt">2</span> emissions from tidal swamp soils. No clear drivers were found for CH4 or N<span class="hlt">2</span>O emissions. On occasion, large ebbing or very low tides were even found to draw <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> into the soil (dark <span class="hlt">CO</span><span class="hlt">2</span> uptake), along with CH4 and N<span class="hlt">2</span>O. Overall, we hypothesized a much greater role for salinity and site condition in controlling the suite of greenhouse gases emitted from tidal swamps than we discovered, and found that <span class="hlt">CO</span><span class="hlt">2</span> emissions–not CH4 or N<span class="hlt">2</span>O–contributed most to the global warming potential from these tidal swamp soils.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19950031260&hterms=biodegradation&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dbiodegradation','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19950031260&hterms=biodegradation&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dbiodegradation"><span><span class="hlt">Flux</span> to the atmosphere of CH4 and <span class="hlt">CO</span><span class="hlt">2</span> from wetland ponds on the Hudson Bay lowlands (HBLs)</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hamilton, J. David; Kelly, Carol A.; Rudd, John W. M.; Hesslein, Raymond H.; Roulet, Nigel T.</p> <p>1994-01-01</p> <p>Ponds on peatlands of the Hudson Bay lowlands (HBLs) are complex ecosystems in which the <span class="hlt">fluxes</span> to the atmosphere of CH4 and <span class="hlt">CO</span><span class="hlt">2</span> were controlled by interacting physical and biological factors. This resulted in strong diel variations of both dissolved gas concentrations and gas <span class="hlt">fluxes</span> to the atmosphere, necessitating frequent sampling on a 24-hour schedule to enable accurate estimates of daily <span class="hlt">fluxes</span>. Ponds at three sites on the HBL were constant net sources of CH4 and <span class="hlt">CO</span><span class="hlt">2</span> to the atmosphere at mean rates of 110-180 mg CH4 m(exp -<span class="hlt">2</span>)/d and 3700-11,000 mg <span class="hlt">CO</span><span class="hlt">2</span> m(exp -<span class="hlt">2</span>)/d. Rates peaked in August and September. For CH4 the pond <span class="hlt">fluxes</span> were 3-30 times higher than adjacent vegetated surfaces. For <span class="hlt">CO</span><span class="hlt">2</span> the net pond <span class="hlt">fluxes</span> were similar in magnitude to the vegetated <span class="hlt">fluxes</span> but the direction of the <span class="hlt">flux</span> was opposite, toward atmosphere. Even though ponds cover only 8-12% of the HBL area, they accounted for 30% of its total CH4 <span class="hlt">flux</span> to the atmosphere. There is some circumstantial evidence that the ponds are being formed by decomposition of the underlying peat and that this decomposition is being stimulated by the activity of N<span class="hlt">2</span> fixing cyanobacteria that grow in mats at the peat-water interface. The fact that the gas <span class="hlt">fluxes</span> from the ponds were so different from the surrounding vegetated surfaces means that any change in the ratio of pond to vegetated area, as may occur in response to climate change, would affect the total HBL <span class="hlt">fluxes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.B24D..03H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.B24D..03H"><span>High-resolution mapping of biogenic carbon <span class="hlt">fluxes</span> to improve urban <span class="hlt">CO</span><span class="hlt">2</span> monitoring, reporting, and verification</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hardiman, B. S.; Hutyra, L.; Gately, C.; Raciti, S. M.</p> <p>2014-12-01</p> <p>Urban areas are home to 80% of the US population and 70% of energy related fossil fuel emissions originate from urban areas. Efforts to accurately monitor, report, and verify anthropogenic <span class="hlt">CO</span><span class="hlt">2</span> missions using atmospheric measurements require reliable partitioning of anthropogenic and biogenic sources. Anthropogenic emissions peak during the daytime, coincident with biogenic drawdown of <span class="hlt">CO</span><span class="hlt">2</span>. In contrast, biogenic respiration emissions peak at night when anthropogenic emissions are lower. This temporal aliasing of <span class="hlt">fluxes</span> requires careful modeling of both biogenic and anthropogenic <span class="hlt">fluxes</span> for accurate source attribution through inverse modeling. Biogenic <span class="hlt">fluxes</span> in urban regions can be a significant component of the urban carbon cycle. However, vegetation in urban areas is subject to longer growing seasons, reduced competition, higher rates of nitrogen deposition, and altered patterns of biomass inputs, all interacting to elevate C turnover rates relative to analogous non-urban ecosystems. These conditions suggest that models that ignore urban vegetation or base biogenic <span class="hlt">flux</span> estimates on non-urban forests are likely to produce inaccurate estimates of anthropogenic <span class="hlt">CO</span><span class="hlt">2</span> emissions. Biosphere models often omit biogenic <span class="hlt">fluxes</span> in urban areas despite potentially extensive vegetation coverage. For example, in Massachusetts, models mask out as much as 40% of land area, effectively assuming they have no biological <span class="hlt">flux</span>. This results in a ~32% underestimate of aboveground biomass (AGB) across the state as compared to higher resolution vegetation maps. Our analysis suggests that some common biomass maps may underestimate forest biomass by ~520 Tg C within the state of Massachusetts. Moreover, omitted portions of the state have the highest population density, indicating that we know least about regions where most people live. We combine remote sensing imagery of urban vegetation cover with ground surveys of tree growth and mortality to improve estimates of aboveground biomass and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AMT.....6..817W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AMT.....6..817W"><span>Jena Reference <span class="hlt">Air</span> Set (JRAS): a multi-point scale anchor for isotope measurements of <span class="hlt">CO</span><span class="hlt">2</span> in <span class="hlt">air</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wendeberg, M.; Richter, J. M.; Rothe, M.; Brand, W. A.</p> <p>2013-03-01</p> <p>The need for a unifying scale anchor for isotopes of <span class="hlt">CO</span><span class="hlt">2</span> in <span class="hlt">air</span> was brought to light at the 11th WMO/IAEA Meeting of Experts on Carbon Dioxide in Tokyo 2001. During discussions about persistent discrepancies in isotope measurements between the worlds leading laboratories, it was concluded that a unifying scale anchor for Vienna Pee Dee Belemnite (VPDB) of <span class="hlt">CO</span><span class="hlt">2</span> in <span class="hlt">air</span> was desperately needed. Ten years later, at the 2011 Meeting of Experts on Carbon Dioxide in Wellington, it was recommended that the Jena Reference <span class="hlt">Air</span> Set (JRAS) become the official scale anchor for isotope measurements of <span class="hlt">CO</span><span class="hlt">2</span> in <span class="hlt">air</span> (Brailsford, 2012). The source of <span class="hlt">CO</span><span class="hlt">2</span> used for JRAS is two calcites. After releasing <span class="hlt">CO</span><span class="hlt">2</span> by reaction with phosphoric acid, the gases are mixed into <span class="hlt">CO</span><span class="hlt">2</span>-free <span class="hlt">air</span>. This procedure ensures both isotopic stability and longevity of the <span class="hlt">CO</span><span class="hlt">2</span>. That the reference <span class="hlt">CO</span><span class="hlt">2</span> is generated from calcites and supplied as an <span class="hlt">air</span> mixture is unique to JRAS. This is made to ensure that any measurement bias arising from the extraction procedure is eliminated. As every laboratory has its own procedure for extracting the <span class="hlt">CO</span><span class="hlt">2</span>, this is of paramount importance if the local scales are to be unified with a common anchor. For a period of four years, JRAS has been evaluated through the IMECC1 program, which made it possible to distribute sets of JRAS gases to 13 laboratories worldwide. A summary of data from the six laboratories that have reported the full set of results is given here along with a description of the production and maintenance of the JRAS scale anchors. 1 IMECC refers to the EU project "Infrastructure for Measurements of the European Carbon Cycle" (<a href="http://imecc.ipsl.jussieu.fr/"target="_blank">http://imecc.ipsl.jussieu.fr/</a>).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24952420','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24952420"><span>Methods, <span class="hlt">fluxes</span> and sources of gas phase alkyl nitrates in the coastal <span class="hlt">air</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Dirtu, Alin C; Buczyńska, Anna J; Godoi, Ana F L; Favoreto, Rodrigo; Bencs, László; Potgieter-Vermaak, Sanja S; Godoi, Ricardo H M; Van Grieken, René; Van Vaeck, Luc</p> <p>2014-10-01</p> <p>The daily and seasonal atmospheric concentrations, deposition <span class="hlt">fluxes</span> and emission sources of a few C3-C9 gaseous alkyl nitrates (ANs) at the Belgian coast (De Haan) on the Southern North <span class="hlt">Sea</span> were determined. An adapted sampler design for low- and high-volume <span class="hlt">air</span>-sampling, optimized sample extraction and clean-up, as well as identification and quantification of ANs in <span class="hlt">air</span> samples by means of gas chromatography mass spectrometry, are reported. The total concentrations of ANs ranged from 0.03 to 85 pptv and consisted primarily of the nitro-butane and nitro-pentane isomers. <span class="hlt">Air</span> mass backward trajectories were calculated by the Hybrid Single-Particle Lagrangian Integrated Trajectory (HYSPLIT) model to determine the influence of main <span class="hlt">air</span> masses on AN levels in the <span class="hlt">air</span>. The shorter chain ANs have been the most abundant in the Atlantic/Channel/UK <span class="hlt">air</span> masses, while longer chain ANs prevailed in continental <span class="hlt">air</span>. The overall mean N <span class="hlt">fluxes</span> of the ANs were slightly higher for summer than those for winter-spring, although their contributions to the total nitrogen <span class="hlt">flux</span> were low. High correlations between AN and HNO₂ levels were observed during winter/spring. During summer, the shorter chain ANs correlated well with precipitation. Source apportionment by means of principal component analysis indicated that most of the gas phase ANs could be attributed to traffic/combustion, secondary photochemical formation and biomass burning, although marine sources may also have been present and a contributing factor.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.B21H0573M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.B21H0573M"><span>Beyond the Methanogenic Black-Box: Greenhouse Gas <span class="hlt">Fluxes</span> (<span class="hlt">CO</span><span class="hlt">2</span>, CH4, N<span class="hlt">2</span>O) as Evidence for Wetlands as Dynamic Redox Systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mcnicol, G.; Knox, S. H.; Sturtevant, C. S.; Baldocchi, D. D.; Silver, W. L.</p> <p>2015-12-01</p> <p>Seminal wetland research in the 1990s demonstrated that annual methane (CH4) <span class="hlt">fluxes</span> scaled positively with ecosystem production across distinctive wetlands globally. This relationship implies a model of flooded wetland ecosystems as 'methanogenic black-boxes'; poised at a low redox state, and tending to release a fixed fraction of incoming annual productivity as CH4. In contrast, recent studies have reported high ratios of carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) to CH4 emissions, and are adding to a body of evidence suggesting wetlands can vary more widely in their redox state. To explore this apparent incongruence we used principles of redox thermodynamics and laboratory experiments to develop predictions of wetland greenhouse gas (GHG) <span class="hlt">fluxes</span> under different redox regimes. We then used a field study to test the hypothesis that ecosystem seasonality in gross primary productivity (GPP) and temperature would drive changes in GHG emissions, mediated by a dynamic - as opposed to static - redox regime. We estimated wetland GHG emissions from an emergent marsh in the Sacramento Delta, CA from March 2014-2015. We measured <span class="hlt">CO</span><span class="hlt">2</span>, CH4 and N<span class="hlt">2</span>O emissions via diffusion and ebullition with manual sampling, and whole-ecosystem <span class="hlt">fluxes</span> of <span class="hlt">CO</span><span class="hlt">2</span> and CH4 using eddy-covariance. Ebullition and diffusive CH4 <span class="hlt">fluxes</span> were strongly seasonal, with minimum rates (0.86 and 0.35 mg C-CH­­4 m-<span class="hlt">2</span> yr-1, respectively) during winter, and maximum rates (1.3 and 1.8 g C-CH­­4 m-<span class="hlt">2</span> yr-1, respectively) during the summer growing season. In contrast, winter diffusive <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> (494 g C-<span class="hlt">CO</span><span class="hlt">2</span> m-<span class="hlt">2</span> yr-1) and fall bubble <span class="hlt">CO</span><span class="hlt">2</span> concentrations (1.49%) were highest, despite being seasons of lower GPP, temperature, and CH4 <span class="hlt">flux</span>. Further, diffusive and ebullition <span class="hlt">fluxes</span> of N<span class="hlt">2</span>O showed zero net <span class="hlt">flux</span> only during spring and summer months, whereas the wetland was a significant source of N<span class="hlt">2</span>O during winter (81.<span class="hlt">2</span> ± 24.4 mg N-N<span class="hlt">2</span>O m-<span class="hlt">2</span> yr-1). These seasonal <span class="hlt">flux</span> dynamics contradict a 'methanogenic black box' model of wetland redox, which</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21096927','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21096927"><span>Tactile communication using a <span class="hlt">CO</span>(<span class="hlt">2</span>) <span class="hlt">flux</span> stimulation for blind or deafblind people.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>da Cunha, Jose Carlos; Bordignon, Luiz Alberto; Nohama, Percy</p> <p>2010-01-01</p> <p>This paper describes a tactile stimulation system for producing nonvisual image patterns to blind or deafblind people. The stimulator yields a <span class="hlt">CO</span>(<span class="hlt">2</span>) pulsatile <span class="hlt">flux</span> directed to the user's skin throughout a needle that is coupled to a <span class="hlt">2</span>-D tactile plotter. The fluxtactile plotter operates with two step motor mounted on a wood structure, controlled by a program developed to produce alphanumerical characters and geometric figures of different size and speed, which will be used to investigate the psychophysical properties of this kind of tactile communication. <span class="hlt">CO</span>(<span class="hlt">2</span>) is provided by a cylinder that delivers a stable <span class="hlt">flux</span>, which is converted to a pulsatile mode through a high frequency solenoid valve that can chop it up to 1 kHz. Also, system temperature is controlled by a Peltier based device. Tests on the prototype indicate that the system is a valuable tool to investigate the psychophysical properties of the skin in response to stimulation by <span class="hlt">CO</span>(<span class="hlt">2</span>) jet, allowing a quantitative and qualitative analysis as a function of stimulation parameters. With the system developed, it was possible to plot the geometric figures proposed: triangles, rectangles and octagons, in different sizes and speeds, and verify the control of the frequency of <span class="hlt">CO</span>(<span class="hlt">2</span>) jet stimuli.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_24 --> <div id="page_25" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li class="active"><span>25</span></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="481"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A33A2334Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A33A2334Z"><span>Constraining biosphere <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> at regional scale with WRF-<span class="hlt">CO</span><span class="hlt">2</span> 4DVar assimilation system</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zheng, T.</p> <p>2017-12-01</p> <p>The WRF-<span class="hlt">CO</span><span class="hlt">2</span> 4DVar assimilation system is updated to include (1) operators for tower based observations (<span class="hlt">2</span>) chemistry initial and boundary condition in the state vector (3) mechanism for aggregation from simulation model grid to state vector space. The update system is first tested with synthetic data to ensure its accuracy. The system is then used to test regional scale <span class="hlt">CO</span><span class="hlt">2</span> inversion at MCI (Midcontinental intensive) sites where <span class="hlt">CO</span><span class="hlt">2</span> mole fraction data were collected at multiple high towers during 2007-2008. The model domain is set to center on Iowa and include 8 towers within its boundary, and it is of 12x12km horizontal grid spacing. First, the relative impacts of the initial and boundary condition are assessed by the system's adjoint model. This is done with 24, 48, 72 hour time span. Second, we assessed the impacts of the transport error, including the misrepresentation of the boundary layer and cumulus activities. Third, we evaluated the different aggregation approach from the native model grid to the control variables (including scaling factors for <span class="hlt">flux</span>, initial and boundary conditions). Four, we assessed the inversion performance using <span class="hlt">CO</span><span class="hlt">2</span> observation with different time-interval, and from different tower levels. We also examined the appropriate treatment of the background and observation error covariance in relation with these varying observation data sets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFMGC51A1177T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMGC51A1177T"><span>Our trial to develop a risk assessment tool for <span class="hlt">CO</span><span class="hlt">2</span> geological storage (GERAS-<span class="hlt">CO</span><span class="hlt">2</span>GS)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tanaka, A.; Sakamoto, Y.; Komai, T.</p> <p>2012-12-01</p> <p>We will introduce our researches about to develop a risk assessment tool named 'GERAS-<span class="hlt">CO</span><span class="hlt">2</span>GS' (Geo-environmental Risk Assessment System, <span class="hlt">CO</span><span class="hlt">2</span> Geological Storage Risk Assessment System) for 'Carbon Dioxide Geological Storage (Geological CCS)'. It aims to facilitate understanding of size of impact of risks related with upper migration of injected <span class="hlt">CO</span><span class="hlt">2</span>. For gaining public recognition about feasibility of Geological CCS, quantitative estimation of risks is essential, to let public knows the level of the risk: whether it is negligible or not. Generally, in preliminary hazard analysis procedure, potential hazards could be identified within Geological CCS's various facilities such as: reservoir, cap rock, upper layers, <span class="hlt">CO</span><span class="hlt">2</span> injection well, <span class="hlt">CO</span><span class="hlt">2</span> injection plant and <span class="hlt">CO</span><span class="hlt">2</span> transport facilities. Among them, hazard of leakage of injected C02 is crucial, because it is the clue to estimate risks around a specific injection plan in terms of safety, environmental protection effect and economy. Our risk assessment tool named GERAS-<span class="hlt">CO</span><span class="hlt">2</span>GS evaluates volume and rate of retention and leakage of injected <span class="hlt">CO</span><span class="hlt">2</span> in relation with fractures and/or faults, and then it estimates impact of seepages on the surface of the earth. GERAS-<span class="hlt">CO</span><span class="hlt">2</span>GS has four major processing segments: (a) calculation of <span class="hlt">CO</span><span class="hlt">2</span> retention and leakage volume and rate, (b) data processing of <span class="hlt">CO</span><span class="hlt">2</span> dispersion on the surface and ambient <span class="hlt">air</span>, (c) risk data definition and (d) evaluation of risk. Concerning to the injection site, we defined a model, which is consisted from an injection well and a geological strata model: which involves a reservoir, a cap rock, an upper layer, faults, seabed, <span class="hlt">sea</span>, the surface of the earth and the surface of the <span class="hlt">sea</span>. For retention rate of each element of <span class="hlt">CO</span><span class="hlt">2</span> injection site model, we use results of our experimental and numerical studies on <span class="hlt">CO</span><span class="hlt">2</span> migration within reservoirs and faults with specific lithological conditions. For given <span class="hlt">CO</span><span class="hlt">2</span> injection rate, GERAS-<span class="hlt">CO</span><span class="hlt">2</span>GS calculates <span class="hlt">CO</span><span class="hlt">2</span> retention and leakage of each segment</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1615572B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1615572B"><span>Towards Improved Estimates of Ocean Heat <span class="hlt">Flux</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bentamy, Abderrahim; Hollman, Rainer; Kent, Elisabeth; Haines, Keith</p> <p>2014-05-01</p> <p>Recommendations and priorities for ocean heat <span class="hlt">flux</span> research are for instance outlined in recent CLIVAR and WCRP reports, eg. Yu et al (2013). Among these is the need for improving the accuracy, the consistency, and the spatial and temporal resolution of <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> over global as well as at region scales. To meet the main <span class="hlt">air-sea</span> <span class="hlt">flux</span> requirements, this study is aimed at obtaining and analyzing all the heat <span class="hlt">flux</span> components (latent, sensible and radiative) at the ocean surface over global oceans using multiple satellite sensor observations in combination with in-situ measurements and numerical model analyses. The <span class="hlt">fluxes</span> will be generated daily and monthly for the 20-year (1992-2011) period, between 80N and 80S and at 0.25deg resolution. Simultaneous estimates of all surface heat <span class="hlt">flux</span> terms have not yet been calculated at such large scale and long time period. Such an effort requires a wide range of expertise and data sources that only recently are becoming available. Needed are methods for integrating many data sources to calculate energy <span class="hlt">fluxes</span> (short-wave, long wave, sensible and latent heat) across the <span class="hlt">air-sea</span> interface. We have access to all the relevant, recently available satellite data to perform such computations. Yu, L., K. Haines, M. Bourassa, M. Cronin, S. Gulev, S. Josey, S. Kato, A. Kumar, T. Lee, D. Roemmich: Towards achieving global closure of ocean heat and freshwater budgets: Recommendations for advancing research in <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> through collaborative activities. INTERNATIONAL CLIVAR PROJECT OFFICE, 2013: International CLIVAR Publication Series No 189. http://www.clivar.org/sites/default/files/ICPO189_WHOI_<span class="hlt">fluxes</span>_workshop.pdf</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016BGeo...13..691M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016BGeo...13..691M"><span>Fate of terrestrial organic carbon and associated <span class="hlt">CO</span><span class="hlt">2</span> and <span class="hlt">CO</span> emissions from two Southeast Asian estuaries</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Müller, D.; Warneke, T.; Rixen, T.; Müller, M.; Mujahid, A.; Bange, H. W.; Notholt, J.</p> <p>2016-02-01</p> <p>Southeast Asian rivers convey large amounts of organic carbon, but little is known about the fate of this terrestrial material in estuaries. Although Southeast Asia is, by area, considered a hotspot of estuarine carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) emissions, studies in this region are very scarce. We measured dissolved and particulate organic carbon, as well as <span class="hlt">CO</span><span class="hlt">2</span> partial pressures and carbon monoxide (<span class="hlt">CO</span>) concentrations in two tropical estuaries in Sarawak, Malaysia, whose coastal area is covered by carbon-rich peatlands. We surveyed the estuaries of the rivers Lupar and Saribas during the wet and dry season, respectively. Carbon-to-nitrogen ratios suggest that dissolved organic matter (DOM) is largely of terrestrial origin. We found evidence that a large fraction of this carbon is respired. The median p<span class="hlt">CO</span><span class="hlt">2</span> in the estuaries ranged between 640 and 5065 µatm with little seasonal variation. <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> were determined with a floating chamber and estimated to amount to 14-268 mol m-<span class="hlt">2</span> yr-1, which is high compared to other studies from tropical and subtropical sites. Estimates derived from a merely wind-driven turbulent diffusivity model were considerably lower, indicating that these models might be inappropriate in estuaries, where tidal currents and river discharge make an important contribution to the turbulence driving water-<span class="hlt">air</span> gas exchange. Although an observed diurnal variability of <span class="hlt">CO</span> concentrations suggested that <span class="hlt">CO</span> was photochemically produced, the overall concentrations and <span class="hlt">fluxes</span> were relatively moderate (0.4-1.3 nmol L-1 and 0.7-1.8 mmol m-<span class="hlt">2</span> yr-1) if compared to published data for oceanic or upwelling systems. We attributed this to the large amounts of suspended matter (4-5004 mg L-1), limiting the light penetration depth and thereby inhibiting <span class="hlt">CO</span> photoproduction. We concluded that estuaries in this region function as an efficient filter for terrestrial organic carbon and release large amounts of <span class="hlt">CO</span><span class="hlt">2</span> to the atmosphere. The Lupar and Saribas rivers deliver 0.3 ± 0.<span class="hlt">2</span> Tg C</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003AGUFM.B41A..07P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003AGUFM.B41A..07P"><span>Land-use change effects on <span class="hlt">fluxes</span> and isotopic composition of <span class="hlt">CO</span><span class="hlt">2</span> and CH4 in Panama, and possible insights into the atmospheric H<span class="hlt">2</span> cycle</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pendall, E.; Schwendenmann, L.; Potvin, C.</p> <p>2003-12-01</p> <p>Land-use changes in tropical regions are believed to release a quantity of C to the atmosphere which is similar in magnitude to the entire "missing" sink for anthropogenic <span class="hlt">CO</span><span class="hlt">2</span>. Our research attempts to evaluate carbon cycling in three land-cover systems in central Panama: cow pasture, native tree plantation, and undisturbed moist forest. In this ongoing project, we are collecting samples of <span class="hlt">air</span> from profiles in the stable, nocturnal boundary layer, which is dominated by ecosystem respiration. Samples are analyzed for <span class="hlt">CO</span><span class="hlt">2</span> and its isotopes, CH4 and its C isotopic composition, N<span class="hlt">2</span>O, H<span class="hlt">2</span>, <span class="hlt">CO</span>, and SF6. We use a <span class="hlt">flux</span>-gradient method to estimate ecosystem-scale <span class="hlt">fluxes</span> of trace gases from soil to the atmosphere. Keeling plot intercepts reflect the respiratory contribution of C3 and C4 biomass under contrasting land cover systems, and how this varies with pronounced wet-dry seasonal cycles. C isotopes of methane and gradients of molecular hydrogen provide insight into the source of methane production from pasture and plantation soils. Rainforest soils, in contrast, are sinks for both atmospheric methane and hydrogen. The process oriented nature of this field experiment will contribute to parameterization of carbon cycle models at a variety of spatial scales.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010JGRC..11512054V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010JGRC..11512054V"><span>Upper ocean bubble measurements from the NE Pacific and estimates of their role in <span class="hlt">air-sea</span> gas transfer of the weakly soluble gases nitrogen and oxygen</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vagle, Svein; McNeil, Craig; Steiner, Nadja</p> <p>2010-12-01</p> <p>Simultaneous observations of upper-ocean bubble clouds, and dissolved gaseous nitrogen (N<span class="hlt">2</span>) and oxygen (O<span class="hlt">2</span>) from three winter storms are presented and analyzed. The data were collected on the Canadian Surface Ocean Lower Atmosphere Study (C-SOLAS) mooring located near Ocean Station Papa (OSP) at 50°N, 145°W in the NE Pacific during winter of 2003/2004. The bubble field was measured using an upward looking 200 kHz echosounder. Direct estimates of bubble mediated gas <span class="hlt">fluxes</span> were made using assumed bubble size spectra and the upward looking echosounder data. A one-dimensional biogeochemical model was used to help compare data and various existing models of bubble mediated <span class="hlt">air-sea</span> gas exchange. The direct bubble <span class="hlt">flux</span> calculations show an approximate quadratic/cubic dependence on mean bubble penetration depth. After scaling from N<span class="hlt">2</span>/O<span class="hlt">2</span> to carbon dioxide, near surface, nonsupersaturating, <span class="hlt">air-sea</span> transfer rates, KT, for U10 > 12 m s-1 fall between quadratic and cubic relationships. Estimates of the subsurface bubble induced <span class="hlt">air</span> injection <span class="hlt">flux</span>, VT, show an approximate quadratic/cubic dependence on mean bubble penetration depth. Both KT and VT are much higher than those measured during Hurricane Frances over the wind speed range 12 < U10 < 23 m s-1. This result implies that over the open ocean and this wind speed range, older and more developed <span class="hlt">seas</span> which occur during winter storms are more effective in exchanging gases between the atmosphere and ocean than younger less developed <span class="hlt">seas</span> which occur during the rapid passage of a hurricane.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JVGR..327..208R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JVGR..327..208R"><span>Diffuse degassing at Longonot volcano, Kenya: Implications for <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> in continental rifts</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Robertson, Elspeth; Biggs, Juliet; Edmonds, Marie; Clor, Laura; Fischer, Tobias P.; Vye-Brown, Charlotte; Kianji, Gladys; Koros, Wesley; Kandie, Risper</p> <p>2016-11-01</p> <p>Magma movement, fault structures and hydrothermal systems influence volatile emissions at rift volcanoes. Longonot is a Quaternary caldera volcano located in the southern Kenyan Rift, where regional extension controls recent shallow magma ascent. Here we report the results of a soil carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) survey in the vicinity of Longonot volcano, as well as fumarolic gas compositions and carbon isotope data. The total non-biogenic <span class="hlt">CO</span><span class="hlt">2</span> degassing is estimated at < 300 kg d- 1, and is largely controlled by crater faults and fractures close to the summit. Thus, recent volcanic structures, rather than regional tectonics, control fluid pathways and degassing. Fumarolic gases are characterised by a narrow range in carbon isotope ratios (δ13C), from - 4.7‰ to - 6.4‰ (vs. PDB) suggesting a magmatic origin with minor contributions from biogenic <span class="hlt">CO</span><span class="hlt">2</span>. Comparison with other degassing measurements in the East African Rift shows that records of historical eruptions or unrest do not correspond directly to the magnitude of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> from volcanic centres, which may instead reflect the current size and characteristics of the subsurface magma reservoir. Interestingly, the integrated <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> from faulted rift basins is reported to be an order of magnitude higher than that from any of the volcanic centres for which <span class="hlt">CO</span><span class="hlt">2</span> surveys have so far been reported.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.A41F0091W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.A41F0091W"><span>An Inversion Analysis of Recent Variability in <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Fluxes</span> Using GOSAT and In Situ Observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, J. S.; Kawa, S. R.; Baker, D. F.; Collatz, G. J.</p> <p>2016-12-01</p> <p>About one-half of the global <span class="hlt">CO</span><span class="hlt">2</span> emissions from fossil fuel combustion and deforestation accumulates in the atmosphere, where it contributes to global warming. The rest is taken up by vegetation and the ocean. The precise contribution of the two sinks and their location and year-to-year variability are not well understood. We use two different approaches, batch Bayesian synthesis inversion and variational data assimilation, to deduce the global spatiotemporal distributions of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> during 2009-2010. One of our objectives is to assess different sources of uncertainties in inferred <span class="hlt">fluxes</span>, including uncertainties in prior <span class="hlt">flux</span> estimates and observations, and differences in inversion techniques. For prior constraints, we utilize <span class="hlt">fluxes</span> and uncertainties from the CASA-GFED model of the terrestrial biosphere and biomass burning driven by satellite observations. We also use measurement-based ocean <span class="hlt">flux</span> estimates and fixed fossil <span class="hlt">CO</span><span class="hlt">2</span> emissions. Our inversions incorporate column <span class="hlt">CO</span><span class="hlt">2</span> measurements from the GOSAT satellite (ACOS retrieval, bias-corrected) and in situ observations (individual flask and afternoon-average continuous observations) to estimate <span class="hlt">fluxes</span> in 108 regions over 8-day intervals for the batch inversion and at 3° x 3.75° weekly for the variational system. Relationships between <span class="hlt">fluxes</span> and atmospheric concentrations are derived consistently for the two inversion systems using the PCTM transport model with MERRA meteorology. We compare the posterior <span class="hlt">fluxes</span> and uncertainties derived using different data sets and the two inversion approaches, and evaluate the posterior atmospheric concentrations against independent data including aircraft measurements. The optimized <span class="hlt">fluxes</span> generally resemble each other and those from other studies. For example, a GOSAT-only inversion suggests a shift in the global sink from the tropics/south to the north relative to the prior and to an in-situ-only inversion. The posterior <span class="hlt">fluxes</span> of the GOSAT inversion are better</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GBioC..31..901E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GBioC..31..901E"><span>Impacts of ENSO on <span class="hlt">air-sea</span> oxygen exchange: Observations and mechanisms</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Eddebbar, Yassir A.; Long, Matthew C.; Resplandy, Laure; Rödenbeck, Christian; Rodgers, Keith B.; Manizza, Manfredi; Keeling, Ralph F.</p> <p>2017-05-01</p> <p>Models and observations of atmospheric potential oxygen (APO ≃ O<span class="hlt">2</span> + 1.1 * <span class="hlt">CO</span><span class="hlt">2</span>) are used to investigate the influence of El Niño-Southern Oscillation (ENSO) on <span class="hlt">air-sea</span> O<span class="hlt">2</span> exchange. An atmospheric transport inversion of APO data from the Scripps flask network shows significant interannual variability in tropical APO <span class="hlt">fluxes</span> that is positively correlated with the Niño3.4 index, indicating anomalous ocean outgassing of APO during El Niño. Hindcast simulations of the Community Earth System Model (CESM) and the Institut Pierre-Simon Laplace model show similar APO sensitivity to ENSO, differing from the Geophysical Fluid Dynamics Laboratory model, which shows an opposite APO response. In all models, O<span class="hlt">2</span> accounts for most APO <span class="hlt">flux</span> variations. Detailed analysis in CESM shows that the O<span class="hlt">2</span> response is driven primarily by ENSO modulation of the source and rate of equatorial upwelling, which moderates the intensity of O<span class="hlt">2</span> uptake due to vertical transport of low-O<span class="hlt">2</span> waters. These upwelling changes dominate over counteracting effects of biological productivity and thermally driven O<span class="hlt">2</span> exchange. During El Niño, shallower and weaker upwelling leads to anomalous O<span class="hlt">2</span> outgassing, whereas deeper and intensified upwelling during La Niña drives enhanced O<span class="hlt">2</span> uptake. This response is strongly localized along the central and eastern equatorial Pacific, leading to an equatorial zonal dipole in atmospheric anomalies of APO. This dipole is further intensified by ENSO-related changes in winds, reconciling apparently conflicting APO observations in the tropical Pacific. These findings suggest a substantial and complex response of the oceanic O<span class="hlt">2</span> cycle to climate variability that is significantly (>50%) underestimated in magnitude by ocean models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.B43J..06P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.B43J..06P"><span>Responses of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Fluxes</span> to Arctic Browning Events in a Range of High Latitude, Shrub-Dominated Ecosystems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Phoenix, G. K.; Treharne, R.; Emberson, L.; Tømmervik, H. A.; Bjerke, J. W.</p> <p>2017-12-01</p> <p>Climatic and biotic extreme events can result in considerable damage to arctic vegetation, often at landscape and larger scale. These acute events therefore contribute to the browning observed in some arctic regions. It is of considerable concern, therefore, that such extreme events are increasing in frequency as part of climate change. However, despite the increasing importance of browning events, and the considerable impact they can have on ecosystems, to date there is little understanding of their impacts on ecosystem carbon <span class="hlt">fluxes</span>. To address this, the impacts of a number of different, commonly occurring, extreme events and their subsequent browning (vegetation damage) on key ecosystem <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> were assessed during the growing season at a range of event damaged sites of shrub dominated vegetation. Sites were located from the boreal to High Arctic (64˚N-79˚N) and had been previously been damaged by events of frost-drought, extreme winter warming, ground icing and caterpillar (Epirrita autumnata) outbreaks. Plot-level <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> of Ecosystem Exchange (NEE), Gross Primary Productivity (GPP) and Ecosystem Respiration (Reco) were assessed using vegetation chambers. At a sub-set of sites, NDVI (greenness) in <span class="hlt">flux</span> plots was also assessed by hand-held proximal sensor, allowing the relationship between NDVI of damage plots to <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> to be calculated. Despite the contrasting sites and drivers, damage had consistent, major impacts on all <span class="hlt">fluxes</span>. All sites showed reductions in GPP and NEE with increasing damage, despite efflux from Reco also declining with damage. When scaled to site-level, reductions of up to 81% of NEE, 51% of GPP and 37% of Reco were observed. In the plot-level NDVI-<span class="hlt">flux</span> relationship, NDVI was shown to explain up to 91% of variation in GPP, and therefore supports the use of NDVI for estimating changes in ecosystem <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> at larger scales in regions where browning has been driven by extreme events. This work is the first attempt to quantify the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1996PCE....21..409I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1996PCE....21..409I"><span>Eddy-correlation measurements of <span class="hlt">fluxes</span> of <span class="hlt">CO</span> <span class="hlt">2</span> and H <span class="hlt">2</span>O above a spruce stand</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ibrom, A.; Schütz, C.; Tworek, T.; Morgenstern, K.; Oltchev, A.; Falk, M.; Constantin, J.; Gravenhorst, G.</p> <p>1996-12-01</p> <p>Atmospheric <span class="hlt">fluxes</span> of <span class="hlt">CO</span> <span class="hlt">2</span> and H <span class="hlt">2</span>O above a mature spruce stand ( Picea abies (L.) Karst.) have been investigated using the eddy- correlation technique. A closed path sensor adapted to the special requirements of long-term studies has been developed and tested. Field measurements have been performed since April 1995. Estimates of fetch showed a very narrow source area dimension under instable stratification (≤ 200 m). Fetch requirements at night are not met in some directions. Energy balance closure was influenced systematically by the wind direction indicating a substantial attenuation of the vertical wind motion by the tower (up to 40 %). Even for optimal flow directions, energy balance closure was about 88%. Intercomparison of the used ultra sonic anemometer (USAT-3) with a GILL - anemometer showed systematically lower values of vertical wind speed fluctuations (13 %). Average <span class="hlt">CO</span> <span class="hlt">2</span>-<span class="hlt">fluxes</span> ranged between -13 at noon to 3 μ mol m-<span class="hlt">2</span>, s-1 at night in summer. In November and December the stand released <span class="hlt">CO</span> <span class="hlt">2</span> on a daily basis. A preliminary estimate of the cumulative net carbon balance over the observed period of 9 months is 4-5 t, Cha-1.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1611798J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1611798J"><span>Chambers versus Relaxed Eddy Accumulation: an intercomparison study of two methods for short-term measurements of biogenic <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jasek, Alina; Zimnoch, Miroslaw; Gorczyca, Zbigniew; Chmura, Lukasz; Necki, Jaroslaw</p> <p>2014-05-01</p> <p>The presented work is a part of comprehensive study aimed at thorough characterization of carbon cycle in the urban environment of Krakow, southern Poland. In the framework of this study two independent methods were employed to quantify biogenic <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> in the city: (i) closed chambers, and (ii) Relaxed Eddy Accumulation (REA). The results of a three-day intensive intercomparison campaign performed in July 2013 and utilizing both measurement methods are reported here. The chamber method is a widely used approach for measurements of gas exchange between the soil and the atmosphere. The system implemented in this study consisted of a single chamber operating in a closed-dynamic mode, combined with Vaisala CarboCAP infrared <span class="hlt">CO</span><span class="hlt">2</span> sensor in a mobile setup. An alternative <span class="hlt">flux</span> measurement method, covering larger area is represented by REA, which is a modification of the eddy covariance method. It consists of a 3D anemometer (Gill Windmaster Pro) and the system collecting updraft and downdraft samples to 5-litre Tedlar bags. The <span class="hlt">CO</span><span class="hlt">2</span> mixing ratios in the collected samples are measured by Picarro G2101i analyzer. The setup consists of two sets of bags so that the sampling can be performed continuously with 15-min temporal resolution. A 48-hectares open meadow located close the city center was chosen as a test site for comparison of the two methods of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> measurements outlined above. In the middle of the meadow a 3-metre high tripod was installed with the anemometer and REA inlet system. For a period of 46 hours the system was measuring net <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> from the surrounding area. A meteorological conditions and intensity of photosynthetically active radiation (PAR) were also recorded. In the same time, <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> from several points around the REA inlet was measured with the chamber system, resulting in 93 values for both respiration and net <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span>. Chamber results show rather homogenous distribution of the soil <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> (the mean value equal to 40.9 ± <span class="hlt">2.2</span> mmol/m<span class="hlt">2</span>h), with</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFMGC23D0949W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFMGC23D0949W"><span>The Oceanic <span class="hlt">Flux</span> Program: A three decade time-series of particle <span class="hlt">flux</span> in the deep Sargasso <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Weber, J. C.; Conte, M. H.</p> <p>2010-12-01</p> <p>The Oceanic <span class="hlt">Flux</span> Program (OFP), 75 km SE of Bermuda, is the longest running time-series of its kind. Initiated in 1978, the OFP has produced an unsurpassed, nearly continuous record of temporal variability in deep ocean <span class="hlt">fluxes</span>, with a >90% temporal coverage at 3200m depth. The OFP, in conjunction with the <span class="hlt">co</span>-located Bermuda-Atlantic Time Series (BATS) and the Bermuda Testbed Mooring (BTM) time-series, has provided key observations enabling detailed assessment of how seasonal and non-seasonal variability in the deep ocean is linked with the overlying physical and biogeochemical environment. This talk will focus on the short-term <span class="hlt">flux</span> variability that overlies the seasonal <span class="hlt">flux</span> pattern in the Sargasso <span class="hlt">Sea</span>, emphasizing episodic extreme <span class="hlt">flux</span> events. Extreme <span class="hlt">flux</span> events are responsible for much of the year-to-year variability in mean annual <span class="hlt">flux</span> and are most often observed during early winter and late spring when surface stratification is weak or transient. In addition to biological phenomena (e.g. salp blooms), passage of productive meso-scale features such as eddies, which alter surface water mixing characteristics and surface export <span class="hlt">fluxes</span>, may initiate some extreme <span class="hlt">flux</span> events. Yet other productive eddies show a minimal influence on the deep <span class="hlt">flux</span>, underscoring the importance of upper ocean ecosystem structure and midwater processes on the coupling between the surface ocean environment and deep <span class="hlt">fluxes</span>. Using key organic and inorganic tracers, causative processes that influence deep <span class="hlt">flux</span> generation and the strength of the coupling with the surface ocean environment can be identified.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.B33A0392D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.B33A0392D"><span>Global Monthly <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Flux</span> Inversion Based on Results of Terrestrial Ecosystem Modeling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Deng, F.; Chen, J.; Peters, W.; Krol, M.</p> <p>2008-12-01</p> <p>Most of our understanding of the sources and sinks of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> has come from inverse studies of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentration measurements. However, the number of currently available observation stations and our ability to simulate the diurnal planetary boundary layer evolution over continental regions essentially limit the number of regions that can be reliably inverted globally, especially over continental areas. In order to overcome these restrictions, a nested inverse modeling system was developed based on the Bayesian principle for estimating carbon <span class="hlt">fluxes</span> of 30 regions in North America and 20 regions for the rest of the globe. Inverse modeling was conducted in monthly steps using <span class="hlt">CO</span><span class="hlt">2</span> concentration measurements of 5 years (2000 - 2005) with the following two models: (a) An atmospheric transport model (TM5) is used to generate the transport matrix where the diurnal variation n of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentration is considered to enhance the use of the afternoon-hour average <span class="hlt">CO</span><span class="hlt">2</span> concentration measurements over the continental sites. (b) A process-based terrestrial ecosystem model (BEPS) is used to produce hourly step carbon <span class="hlt">fluxes</span>, which could minimize the limitation due to our inability to solve the inverse problem in a high resolution, as the background of our inversion. We will present our recent results achieved through a combination of the bottom-up modeling with BEPS and the top-down modeling based on TM5 driven by offline meteorological fields generated by the European Centre for Medium Range Weather Forecast (ECMFW).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.A52C..03K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.A52C..03K"><span>Evaluation of Diagnostic <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Flux</span> and Transport Modeling in NU-WRF and GEOS-5</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kawa, S. R.; Collatz, G. J.; Tao, Z.; Wang, J. S.; Ott, L. E.; Liu, Y.; Andrews, A. E.; Sweeney, C.</p> <p>2015-12-01</p> <p>We report on recent diagnostic (constrained by observations) model simulations of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> and transport using a newly developed facility in the NASA Unified-Weather Research and Forecast (NU-WRF) model. The results are compared to <span class="hlt">CO</span><span class="hlt">2</span> data (ground-based, airborne, and GOSAT) and to corresponding simulations from a global model that uses meteorology from the NASA GEOS-5 Modern Era Retrospective analysis for Research and Applications (MERRA). The objective of these intercomparisons is to assess the relative strengths and weaknesses of the respective models in pursuit of an overall carbon process improvement at both regional and global scales. Our guiding hypothesis is that the finer resolution and improved land surface representation in NU-WRF will lead to better comparisons with <span class="hlt">CO</span><span class="hlt">2</span> data than those using global MERRA, which will, in turn, inform process model development in global prognostic models. Initial intercomparison results, however, have generally been mixed: NU-WRF is better at some sites and times but not uniformly. We are examining the model transport processes in detail to diagnose differences in the <span class="hlt">CO</span><span class="hlt">2</span> behavior. These comparisons are done in the context of a long history of simulations from the Parameterized Chemistry and Transport Model, based on GEOS-5 meteorology and Carnegie Ames-Stanford Approach-Global Fire Emissions Database (CASA-GFED) <span class="hlt">fluxes</span>, that capture much of the <span class="hlt">CO</span><span class="hlt">2</span> variation from synoptic to seasonal to global scales. We have run the NU-WRF model using unconstrained, internally generated meteorology within the North American domain, and with meteorological 'nudging' from Global Forecast System and North American Regional Reanalysis (NARR) in an effort to optimize the <span class="hlt">CO</span><span class="hlt">2</span> simulations. Output results constrained by NARR show the best comparisons to data. Discrepancies, of course, may arise either from <span class="hlt">flux</span> or transport errors and compensating errors are possible. Resolving their interplay is also important to using the data in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16668401','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16668401"><span>Relationships between the Efficiencies of Photosystems I and II and Stromal Redox State in <span class="hlt">CO</span>(<span class="hlt">2</span>)-Free <span class="hlt">Air</span> : Evidence for Cyclic Electron Flow in Vivo.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Harbinson, J; Foyer, C H</p> <p>1991-09-01</p> <p>The responses of the efficiencies of photosystems I and II, stromal redox state (as indicated by NADP-malate dehydrogenase activation state), and activation of the Benson-Calvin cycle enzymes ribulose 1,5-bisphosphate carboxylase and fructose 1,6-bisphosphatase to varying irradiance were measured in pea (Pisum sativum L.) leaves operating close to the <span class="hlt">CO</span>(<span class="hlt">2</span>) compensation point. A comparison of the relationships among these parameters obtained from leaves in <span class="hlt">air</span> was made with those obtained when the leaves were maintained in <span class="hlt">air</span> from which the <span class="hlt">CO</span>(<span class="hlt">2</span>) had been removed. P700 was more oxidized at any measured irradiance in <span class="hlt">CO</span>(<span class="hlt">2</span>)-free <span class="hlt">air</span> than in <span class="hlt">air</span>. The relationship between the quantum efficiencies of the photosystems in <span class="hlt">CO</span>(<span class="hlt">2</span>)-free <span class="hlt">air</span> was distinctly curvilinear in contrast to the predominantly linear relationship obtained with leaves in <span class="hlt">air</span>. This nonlinearity may be consistent with the operation of cyclic electron flow around photosystem I because the quantum efficiency of photosystem II was much more restricted than the quantum efficiency of photosystem I. In <span class="hlt">CO</span>(<span class="hlt">2</span>)-free <span class="hlt">air</span>, measured NADP-malate dehydrogenase activities varied considerably at low irradiances. However, at high irradiance the activity of the enzyme was low, implying that the stroma was oxidized. In contrast, fructose-1,6-bisphosphatase activities tended to increase with increasing electron <span class="hlt">flux</span> through the photosystems. Ribulose-1,5-bisphosphate carboxylase activity remained relatively constant with respect to irradiance in <span class="hlt">CO</span>(<span class="hlt">2</span>)-free <span class="hlt">air</span>, with an activation state 50% of maximum. We conclude that, at the <span class="hlt">CO</span>(<span class="hlt">2</span>) compensation point and high irradiance, low redox states are favored and that cyclic electron flow may be substantial. These two features may be the requirements necessary to trigger and maintain the dissipative processes in the thylakoid membrane.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.ars.usda.gov/research/publications/publication/?seqNo115=314066','TEKTRAN'); return false;" href="http://www.ars.usda.gov/research/publications/publication/?seqNo115=314066"><span>Seasonal variation in measured H<span class="hlt">2</span>O and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> of irrigated rice in the Mid-South</span></a></p> <p><a target="_blank" href="https://www.ars.usda.gov/research/publications/find-a-publication/">USDA-ARS?s Scientific Manuscript database</a></p> <p></p> <p></p> <p>Rice production in the Lower Mississippi River Basin constitutes over half of US rice production, but little research has been done on water and carbon <span class="hlt">flux</span> in this region at the field scale. Eddy covariance measurements of water and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> allow for an integrated field measurement of the interac...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.B41B0409L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.B41B0409L"><span>A gap-filling model for eddy covariance <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span>: Estimating carbon assimilated by a subtropical evergreen broad-leaved forest at the Lien-Hua-Chih <span class="hlt">flux</span> observation site</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lan, C. Y.; Li, M. H.; Chen, Y. Y.</p> <p>2016-12-01</p> <p>Appropriate estimations of gaps appeared in eddy covariance (EC) <span class="hlt">flux</span> observations are critical to the reliability of long-term EC applications. In this study we present a semi-parametric multivariate gap-filling model for tower-based measurement of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span>. The raw EC data passing QC/QA was separated into two groups, clear sky, having net radiation greater than 50 W/m<span class="hlt">2</span>, and nighttime/cloudy. For the clear sky conditions, the principle component analysis (PCA) was used to resolve the multicollinearity relationships among various environmental variables, including net radiation, wind speed, vapor pressure deficit, soil moisture deficit, leaf area index, and soil temperature, in association with <span class="hlt">CO</span><span class="hlt">2</span> assimilated by forest. After the principal domains were determined by the PCA, the relationships between <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> and selected PCs (key factors) were built up by nonlinear interpolations to estimate the gap-filled <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span>. In view of limited photosynthesis at nighttime/cloudy conditions, respiration rate of the forest ecosystem was estimated by the Lloyd-Tylor equation. Artificial gaps were randomly selected to exam the applicability of our PCA approach. Based on tower-based measurement of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">flux</span> at the Lien-Hua-Chih site, a total of 5.8 ton-C/ha/yr was assimilated in 2012.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002EGSGA..27.6028L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002EGSGA..27.6028L"><span>Using New Remotely-sensed Biomass To Estimate <span class="hlt">Co</span><span class="hlt">2</span> <span class="hlt">Fluxes</span> Over Siberia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lafont, S.; Kergoat, L.; Dedieu, G.; Le Toan, T.</p> <p></p> <p>Two european programs recently focused on Siberia. The first one, Eurosiberian Car- bonflux was a faisability study for an observation system of the regional <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span>. The second one, SIBERIA was a big effort to develop and validate a biomass map on Siberia using radar data from satelltes (J-ERS, ERS). Here, we extend the simula- tion of NPP performed for the first program by using the biomass data of the second program. The TURC model, used here, is a global NPP model, based on light use efficiency, where photosynthetic assimilation is driven by satellite vegetation index, and au- totrophic respiration is driven by biomass. In this study, we will present a n´ zoom z on siberian region. The TURC model was run with a fine resolution (few kilometers) and a daily time step. We will discuss the impact of a new biomass dataset description on Net Primary Pro- ductivity (NPP) and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">fluxes</span> estimation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6207452-monitoring-seasonal-state-mapping-species-alaskan-taiga-using-imaging-radar-input-co-sub-flux-models','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6207452-monitoring-seasonal-state-mapping-species-alaskan-taiga-using-imaging-radar-input-co-sub-flux-models"><span>Monitoring seasonal state and mapping species in Alaskan taiga using imaging radar as input to <span class="hlt">CO</span>[sub <span class="hlt">2</span>] <span class="hlt">flux</span> models</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Way, J.B.; Rignot, E.; McDonald, K.</p> <p>1993-06-01</p> <p>Changes in the seasonal <span class="hlt">CO</span>[sub <span class="hlt">2</span>] <span class="hlt">flux</span> of the boreal forests may result from increased atmospheric <span class="hlt">CO</span>[sub <span class="hlt">2</span>] concentrations and associated atmospheric warming. To monitor this potential change, a combination of remote sensing information and ecophysiological models are required. In this paper we address the use of synthetic aperture radar (SAR) data to provide some of the input to the ecophysiological models: forest type, freeze/thaw state which limits the growing season for conifers, and leaf on/off state which limits the growing season for deciduous species. AIRSAR data collected in March 1988 during an early thaw event and May 1991 duringmore » spring breakup are used to generate species maps and to determine the sensitivity of SAR to canopy freeze/thaw transitions. These data are also used to validate a microwave scattering model which is then used to determine the sensitivity of SAR to leaf on/off and soil freeze/thaw transitions. Finally, a <span class="hlt">CO</span>[sub <span class="hlt">2</span>] <span class="hlt">flux</span> algorithm which utilizes SAR data and an ecophysiological model to estimate <span class="hlt">CO</span>[sub <span class="hlt">2</span>] <span class="hlt">flux</span> is presented. <span class="hlt">CO</span>[sub <span class="hlt">2</span>] <span class="hlt">flux</span> maps are generated from which areal estimates of <span class="hlt">CO</span>[sub <span class="hlt">2</span>] <span class="hlt">flux</span> are derived. This work was carried out at the Jet Propulsion Laboratory under contract to the NASA.« less</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li class="active"><span>25</span></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_25 --> <div class="footer-extlink text-muted" style="margin-bottom:1rem; text-align:center;">Some links on this page may take you to non-federal websites. 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