Sample records for air-sea co2 exchange

  1. 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.

  2. Biofilm-like properties of the sea surface and predicted effects on air-sea CO2 exchange

    NASA Astrophysics Data System (ADS)

    Wurl, Oliver; Stolle, Christian; Van Thuoc, Chu; The Thu, Pham; Mari, Xavier

    2016-05-01

    Because the sea surface controls various interactions between the ocean and the atmosphere, it has a profound function for marine biogeochemistry and climate regulation. The sea 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 sea surface are essential. The uppermost part of the water column is defined as the sea-surface microlayer and experiences strong spatial and temporal dynamics, mainly due to meteorological forcing. Wave-damped areas at the sea 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 Sea, and Baltic Sea. We found a significant lower enrichment of TEP (up to 6) in non-slick sea 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 air-sea CO2 exchange based on literature data. We estimate that slicks can reduce CO2

  3. Enrichment of Extracellular Carbonic Anhydrase in the Sea Surface Microlayer and Its Effect on Air-Sea CO2 Exchange

    NASA Astrophysics Data System (ADS)

    Mustaffa, N. I. H.; Striebel, M.; Wurl, O.

    2017-12-01

    This paper describes the quantification of extracellular carbonic anhydrase (eCA) concentrations in the sea 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 CO2, it has been hypothesized that its enrichment in the SML enhances the air-sea CO2 exchange. We detected concentrations in the range of 0.12 to 0.76 nM, which can enhance the exchange by up to 15% based on the model approach described in the literature.

  4. Air-sea exchange of CO2 in the central and western equatorial Pacific in 1990

    NASA Astrophysics Data System (ADS)

    Ishii, Masao; Yoshikawa Inoue, Hisayuki

    1995-09-01

    Measurements of CO2 in marine boundary air 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 pCO2(sea) 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, pCO2(sea) decreased gradually toward the west as a result of biological CO2 uptake and surface sea temperature increase. Between 179°E and 170°E, the pCO2(sea) 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, pCO2(sea) was nearly equal to pCO2(air). The distribution of the atmospheric CO2 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 CO2 flux from the sea 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 ΔpCO2 distribution and the several gas transfer coefficients reported so far. It ranged from 0.13 GtC year-1-0.29 GtC year-1. This CO2 outflux is thought to almost disappear during the period of an El Niño event.

  5. Constraining global air-sea gas exchange for CO2 with recent bomb 14C measurements

    NASA Astrophysics Data System (ADS)

    Sweeney, Colm; Gloor, Emanuel; Jacobson, Andrew R.; Key, Robert M.; McKinley, Galen; Sarmiento, Jorge L.; Wanninkhof, Rik

    2007-06-01

    The 14CO2 released into the stratosphere during bomb testing in the early 1960s provides a global constraint on air-sea gas exchange of soluble atmospheric gases like CO2. 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 CO2 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(Sc/660)-0.5 and standard partial pressure difference climatology of CO2 we obtain an net air-sea flux 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.

  6. Surfactant control of air-sea gas exchange across contrasting biogeochemical regimes

    NASA Astrophysics Data System (ADS)

    Pereira, Ryan; Schneider-Zapp, Klaus; Upstill-Goddard, Robert

    2014-05-01

    Air-sea gas exchange is important to the global partitioning of CO2.Exchange fluxes are products of an air-sea gas concentration difference, ΔC, and a gas transfer velocity, kw. The latter is controlled by the rate of turbulent diffusion at the air-sea 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 air-sea CO2 exchange ...(Takahashi et al., 2009). One important control on kw is exerted by sea 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 sea 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 Sea in 2012-2013 shows significant spatio-temporal variability in the surfactant activity of organic matter within the sea 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

  7. 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.

  8. The potential of using remote sensing data to estimate air-sea CO2 exchange in the Baltic Sea

    NASA Astrophysics Data System (ADS)

    Parard, Gaëlle; Rutgersson, Anna; Parampil, Sindu Raj; Alexandre Charantonis, Anastase

    2017-12-01

    In this article, we present the first climatological map of air-sea CO2 flux over the Baltic Sea based on remote sensing data: estimates of pCO2 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 CO2 fluxes 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 flux estimations. Furthermore, the CO2 fluxes 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 fluxes reflects the seasonal variation in pCO2 unvaryingly over the whole Baltic Sea, with high winter CO2 emissions and high pCO2 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-2 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-2 d-1) and the coastal areas act as a larger sink (annual uptake of -4.2 mmol m-2 d-1) than does the open sea (-4 mmol m-2 d-1). In its entirety, the Baltic Sea acts as a small source of 1.2 mmol m-2 d-1 on average and this annual uptake has increased from 1998 to 2012.

  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. 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

  11. CO2 exchange in a temperate marginal sea of the Mediterranean Sea: processes and carbon budget

    NASA Astrophysics Data System (ADS)

    Cossarini, G.; Querin, S.; Solidoro, C.

    2012-08-01

    Marginal seas play a potentially important role in the global carbon cycle; however, due to differences in the scales of variability and dynamics, marginal seas are seldom fully accounted for in global models or estimates. Specific high-resolution studies may elucidate the role of marginal seas and assist in the compilation of a complete global budget. In this study, we investigated the air-sea exchange and the carbon cycle dynamics in a marginal sub-basin of the Mediterranean Sea (the Adriatic Sea) by adopting a coupled transport-biogeochemical model of intermediate complexity including carbonate dynamics. The Adriatic Sea 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 CO2 sequestration in the Mediterranean Sea. The results of the model simulation show that the Adriatic Sea, as a whole, is a CO2 sink with a mean annual flux of 36 mg m-2 day-1. The northern part absorbs more carbon (68 mg m-2 day-1) due to an efficient continental shelf pump process, whereas the southern part behaves similar to an open ocean. Nonetheless, the Southern Adriatic Sea 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 CO2 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 Sea.

  12. 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.

  13. 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

  14. Atmospheric concentrations and air-sea exchanges of nonylphenol, tertiary octylphenol and nonylphenol monoethoxylate in the North Sea.

    PubMed

    Xie, Zhiyong; Lakaschus, Soenke; Ebinghaus, Ralf; Caba, Armando; Ruck, Wolfgang

    2006-07-01

    Concentrations of nonylphenol isomers (NP), tertiary octylphenol (t-OP) and nonylphenol monoethoxylate isomers (NP1EO) have been simultaneously determined in the sea water and atmosphere of the North Sea. A decreasing concentration profile appeared following the distance increasing from the coast to the central part of the North Sea. Air-sea exchanges of t-OP and NP were estimated using the two-film resistance model based upon relative air-water concentrations and experimentally derived Henry's law constant. The average of air-sea exchange fluxes was -12+/-6 ng m(-2)day(-1) for t-OP and -39+/-19 ng m(-2)day(-1) for NP, which indicates a net deposition is occurring. These results suggest that the air-sea vapour exchange is an important process that intervenes in the mass balance of alkylphenols in the North Sea.

  15. Using eddy covariance to measure the dependence of air-sea CO2 exchange rate on friction velocity

    NASA Astrophysics Data System (ADS)

    Landwehr, Sebastian; Miller, Scott D.; Smith, Murray J.; Bell, Thomas G.; Saltzman, Eric S.; Ward, Brian

    2018-03-01

    Parameterisation of the air-sea gas transfer velocity of CO2 and other trace gases under open-ocean conditions has been a focus of air-sea interaction research and is required for accurately determining ocean carbon uptake. Ships are the most widely used platform for air-sea flux 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 air-sea CO2 and momentum fluxes 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.

  16. 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

  17. Estimation of bubble-mediated air-sea gas exchange from concurrent DMS and CO2 transfer velocities at intermediate-high wind speeds

    NASA Astrophysics Data System (ADS)

    Bell, Thomas G.; Landwehr, Sebastian; Miller, Scott D.; de Bruyn, Warren J.; Callaghan, Adrian H.; Scanlon, Brian; Ward, Brian; Yang, Mingxi; Saltzman, Eric S.

    2017-07-01

    Simultaneous air-sea fluxes and concentration differences of dimethylsulfide (DMS) and carbon dioxide (CO2) 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 CO2 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.

  18. 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.

  19. 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

  20. 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> fluxes 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> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li class="active"><span>1</span></li> <li><a href="#" onclick='return showDiv("page_2");'>2</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><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_1 --> <div id="page_2" 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 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> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="21"> <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 <span class="hlt">Exchange</span></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 <span class="hlt">exchange</span> 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 <span class="hlt">exchange</span> 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 <span class="hlt">exchange</span>. While remaining uncertainties in the wind dependence of the spume drop production flux, and in the immediate <span class="hlt">sea</span> surface gas flux, 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 <span class="hlt">exchange</span>.<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> <span class="hlt">exchange</span> models. Based on these the contribution of spume drops to overall <span class="hlt">air</span> <span class="hlt">sea</span> gas <span class="hlt">exchange</span> at different wind speeds is then evaluated to determine the % contribution of spume. Generally below 20ms-1 spume drops contribute <1% of gas <span class="hlt">exchange</span> but may account for a significant amount of gas <span class="hlt">exchange</span> at higher wind speeds.</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> fluxes 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> fluxes in Ocean-dominated margin (OceMar) to assesses the <span class="hlt">CO</span><span class="hlt">2</span> fluxes 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> <span class="hlt">exchange</span> 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> <span class="hlt">exchange</span> 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/2018BGeo...15.1643Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018BGeo...15.1643Y"><span>Arctic Ocean <span class="hlt">CO</span><span class="hlt">2</span> uptake: an improved multiyear estimate of the <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> flux incorporating chlorophyll a concentrations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>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.</p> <p>2018-03-01</p> <p>We estimated monthly <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> fluxes in the Arctic Ocean and its adjacent <span class="hlt">seas</span> north of 60° N from 1997 to 2014. This was done by mapping partial pressure of <span class="hlt">CO</span><span class="hlt">2</span> in the surface water (p<span class="hlt">CO</span><span class="hlt">2</span>w) using a self-organizing map (SOM) technique incorporating chlorophyll a concentration (Chl a), <span class="hlt">sea</span> surface temperature, <span class="hlt">sea</span> surface salinity, <span class="hlt">sea</span> ice concentration, atmospheric <span class="hlt">CO</span><span class="hlt">2</span> 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 p<span class="hlt">CO</span><span class="hlt">2</span>w 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 p<span class="hlt">CO</span><span class="hlt">2</span>w, particularly via better representation of its decline in spring, which resulted from biologically mediated p<span class="hlt">CO</span><span class="hlt">2</span>w reduction. As a result of the inclusion of Chl a, the uncertainty in the <span class="hlt">CO</span><span class="hlt">2</span> flux estimate was reduced, with a net annual Arctic Ocean <span class="hlt">CO</span><span class="hlt">2</span> uptake of 180 ± 130 Tg C yr-1. Seasonal to interannual variation in the <span class="hlt">CO</span><span class="hlt">2</span> influx was also calculated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PolSc..10..323Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PolSc..10..323Y"><span>Mapping of the <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> flux in the Arctic Ocean and its adjacent <span class="hlt">seas</span>: Basin-wide distribution and seasonal to 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>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</p> <p>2016-09-01</p> <p>We produced 204 monthly maps of the <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> flux in the Arctic north of 60°N, including the Arctic Ocean and its adjacent <span class="hlt">seas</span>, from January 1997 to December 2013 by using a self-organizing map technique. The 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 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 <span class="hlt">CO</span><span class="hlt">2</span> fluxes. The 17-year annual mean <span class="hlt">CO</span><span class="hlt">2</span> flux shows that all areas of the Arctic Ocean and its adjacent <span class="hlt">seas</span> were net <span class="hlt">CO</span><span class="hlt">2</span> sinks. The estimated annual <span class="hlt">CO</span><span class="hlt">2</span> uptake by the Arctic Ocean was 180 TgC yr-1. The <span class="hlt">CO</span><span class="hlt">2</span> influx was strongest in winter in the Greenland/Norwegian <span class="hlt">Seas</span> (>15 mmol m-<span class="hlt">2</span> day-1) and the Barents <span class="hlt">Sea</span> (>12 mmol m-<span class="hlt">2</span> day-1) because of strong winds, and strongest in summer in the Chukchi <span class="hlt">Sea</span> (∼10 mmol m-<span class="hlt">2</span> day-1) because of the <span class="hlt">sea</span>-ice retreat. In recent years, the <span class="hlt">CO</span><span class="hlt">2</span> uptake has increased in the Greenland/Norwegian <span class="hlt">Sea</span> and decreased in the southern Barents <span class="hlt">Sea</span>, owing to increased and decreased <span class="hlt">air-sea</span> p<span class="hlt">CO</span><span class="hlt">2</span> differences, respectively.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20020044134','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20020044134"><span>Sensitivity of Global <span class="hlt">Sea-Air</span> <span class="hlt">CO</span><span class="hlt">2</span> Flux to Gas Transfer Algorithms, Climatological Wind Speeds, and Variability of <span class="hlt">Sea</span> Surface Temperature and Salinity</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>McClain, Charles R.; Signorini, Sergio</p> <p>2002-01-01</p> <p>Sensitivity analyses of <span class="hlt">sea-air</span> <span class="hlt">CO</span><span class="hlt">2</span> flux to gas transfer algorithms, climatological wind speeds, <span class="hlt">sea</span> surface temperatures (SST) and salinity (SSS) were conducted for the global oceans and selected regional domains. Large uncertainties in the global <span class="hlt">sea-air</span> flux estimates are identified due to different gas transfer algorithms, global climatological wind speeds, and seasonal SST and SSS data. The global <span class="hlt">sea-air</span> flux ranges from -0.57 to -<span class="hlt">2</span>.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 <span class="hlt">sea-air</span> flux. An error as small as plus or minus 0.<span class="hlt">2</span> in SSS translates into a plus or minus 43% deviation on the mean global <span class="hlt">CO</span><span class="hlt">2</span> flux. This result emphasizes the need for highly accurate satellite SSS observations for the development of remote sensing <span class="hlt">sea-air</span> flux algorithms.</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 <span class="hlt">exchange</span>, 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 <span class="hlt">exchange</span> 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 fluxes, 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> <span class="hlt">exchanges</span> involve a large number of physica, chemical and dynamical processes including heat flux, radiation, <span class="hlt">sea</span>-surface temperature, precipitation, winds and ocean currents. The fluxes of latent heat are studied and the potential use of satellite data in determining them evaluated. Alternative ways of inferring heat fluxes will be considered.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA282842','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA282842"><span>Oceanic Whitecaps and Associated, Bubble-Mediated, <span class="hlt">Air-Sea</span> <span class="hlt">Exchange</span> Processes</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1992-10-01</p> <p>experiments performed in laboratory conditions using <span class="hlt">Air-Sea</span> <span class="hlt">Exchange</span> Monitoring System (A-SEMS). EXPERIMENTAL SET-UP In a first look, the <span class="hlt">Air-Sea</span> <span class="hlt">Exchange</span>...Model 225, equipped with a Model 519 plug-in module. Other complementary information on A-SEMS along with results from first tests and calibration...between 9.50C and 22.40C within the first 24 hours after transferring the water sample into laboratory conditions. The results show an enhancement of</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> fluxes</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> fluxes. 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 fluxes and pools, as well as <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span>, 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> fluxes. 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('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 <span class="hlt">exchange</span> 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 <span class="hlt">exchange</span> 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 flux 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 <span class="hlt">exchange</span> 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 <span class="hlt">exchange</span> relationships that incorporate the main forcing factors will lead to improved estimates of global and regional <span class="hlt">air-sea</span> gas fluxes based on better fundamental physical, chemical, and biological foundations.</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> fluxes</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> fluxes. 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 fluxes and pools, as well as <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span>, 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> fluxes. 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/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> fluxes 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> flux 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>-fluxes</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> <span class="hlt">exchange</span> of <span class="hlt">CO</span><span class="hlt">2</span> or <span class="hlt">CO</span><span class="hlt">2</span> flux 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> flux is the parameterization of k. As an example; the estimated global <span class="hlt">air-sea</span> flux 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> fluxes (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> fluxes calculated by the ECM are removed when including the IDM.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015OcSci..11..519G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015OcSci..11..519G"><span>The OceanFlux Greenhouse Gases methodology for deriving a <span class="hlt">sea</span> surface climatology of <span class="hlt">CO</span><span class="hlt">2</span> fugacity in support of <span class="hlt">air-sea</span> gas flux studies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Goddijn-Murphy, L. M.; Woolf, D. K.; Land, P. E.; Shutler, J. D.; Donlon, C.</p> <p>2015-07-01</p> <p>Climatologies, or long-term averages, of essential climate variables are useful for evaluating models and providing a baseline for studying anomalies. The Surface Ocean <span class="hlt">CO</span><span class="hlt">2</span> Atlas (SOCAT) has made millions of global underway <span class="hlt">sea</span> surface measurements of <span class="hlt">CO</span><span class="hlt">2</span> publicly available, all in a uniform format and presented as fugacity, f<span class="hlt">CO</span><span class="hlt">2</span>. As f<span class="hlt">CO</span><span class="hlt">2</span> is highly sensitive to temperature, the measurements are only valid for the instantaneous <span class="hlt">sea</span> surface temperature (SST) that is measured concurrently with the in-water <span class="hlt">CO</span><span class="hlt">2</span> measurement. To create a climatology of f<span class="hlt">CO</span><span class="hlt">2</span> data suitable for calculating <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> fluxes, it is therefore desirable to calculate f<span class="hlt">CO</span><span class="hlt">2</span> 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 f<span class="hlt">CO</span><span class="hlt">2</span> 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 f<span class="hlt">CO</span><span class="hlt">2</span> values to reference year 2010. The data were then spatially interpolated onto a 1° × 1° grid of the global oceans to produce 12 monthly f<span class="hlt">CO</span><span class="hlt">2</span> distributions for 2010, including the prediction errors of f<span class="hlt">CO</span><span class="hlt">2</span> produced by the spatial interpolation technique. The partial pressure of <span class="hlt">CO</span><span class="hlt">2</span> (p<span class="hlt">CO</span><span class="hlt">2</span>) is also provided for those who prefer to use p<span class="hlt">CO</span><span class="hlt">2</span>. The <span class="hlt">CO</span><span class="hlt">2</span> concentration difference between ocean and atmosphere is the thermodynamic driving force of the <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> flux, and hence the presented f<span class="hlt">CO</span><span class="hlt">2</span> distributions can be used in <span class="hlt">air-sea</span> gas flux calculations together with climatologies of other climate variables.</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> <span class="hlt">exchange</span> 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 <span class="hlt">exchange</span> 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 flux 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 fluxes 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> <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 <span class="hlt">exchange</span> and <span class="hlt">CO</span><span class="hlt">2</span> flux 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> fluxes. 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> fluxes 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 <span class="hlt">exchange</span> than predicted by commonly used wind speed/gas <span class="hlt">exchange</span> parameterizations. The results have important implications for carbon fluxes in mangrove ecosystems.</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 <span class="hlt">Exchange</span> 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 fluxes, 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 <span class="hlt">exchange</span> 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 <span class="hlt">exchange</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016CSR...119...68I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016CSR...119...68I"><span>Net <span class="hlt">sea-air</span> <span class="hlt">CO</span><span class="hlt">2</span> fluxes and modelled p<span class="hlt">CO</span><span class="hlt">2</span> in the southwestern subtropical Atlantic continental shelf during spring 2010 and summer 2011</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ito, Rosane Gonçalves; Garcia, Carlos Alberto Eiras; Tavano, Virginia Maria</p> <p>2016-05-01</p> <p><span class="hlt">Sea-air</span> <span class="hlt">CO</span><span class="hlt">2</span> fluxes over continental shelves vary substantially in time on both seasonal and sub-seasonal scales, driven primarily by variations in surface p<span class="hlt">CO</span><span class="hlt">2</span> due to several oceanic mechanisms. Furthermore, coastal zones have not been appropriately considered in global estimates of <span class="hlt">sea-air</span> <span class="hlt">CO</span><span class="hlt">2</span> 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 <span class="hlt">sea-air</span> <span class="hlt">CO</span><span class="hlt">2</span> 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 <span class="hlt">CO</span><span class="hlt">2</span> to the atmosphere, with an average of 1.<span class="hlt">2</span> mmol <span class="hlt">CO</span><span class="hlt">2</span> m-<span class="hlt">2</span> day-1 for the late spring and 11.<span class="hlt">2</span> mmol <span class="hlt">CO</span><span class="hlt">2</span> m-<span class="hlt">2</span> day-1 for the early summer cruises. The spatial variability in ocean p<span class="hlt">CO</span><span class="hlt">2</span> 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 p<span class="hlt">CO</span><span class="hlt">2</span> 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 p<span class="hlt">CO</span><span class="hlt">2</span> values were higher as a result of upwelled <span class="hlt">CO</span><span class="hlt">2</span>-enriched subsurface waters. Finally, a p<span class="hlt">CO</span><span class="hlt">2</span> algorithm based on both <span class="hlt">sea</span> surface temperature and surface chlorophyll-a was developed that enabled the spatial</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26995905','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26995905"><span>[Effect of <span class="hlt">air</span> temperature and rainfall on wetland ecosystem <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> in China].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chu, Xiao-jing; Han, Guang-xuan</p> <p>2015-10-01</p> <p>Wetland can be a potential efficient sink to reduce global warming due to its higher primary productivity and lower carbon decomposition rate. While there has been a series progress on the influence mechanism of ecosystem <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> over China' s wetlands, a systematic metaanalysis of data still needs to be improved. We compiled data of ecosystem <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> of 21 typical wetland vegetation types in China from 29 papers and carried out an integrated analysis of <span class="hlt">air</span> temperature and precipitation effects on net ecosystem <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> (NEE), ecosystem respiration (Reco), gross primary productivity (GPP), the response of NEE to PAR, and the response of Reco to temperature. The results showed that there were significant responses (P<0.05) of NEE (R<span class="hlt">2</span> = 50%, R<span class="hlt">2</span>=57%), GPP (R<span class="hlt">2</span> = 60%, R<span class="hlt">2</span> = 50%) Reco (R<span class="hlt">2</span> = 44%, R<span class="hlt">2</span>=50%) with increasing <span class="hlt">air</span> temperature and enhanced precipitation on the annual scale. On the growing season scale, <span class="hlt">air</span> temperature accounted for 50% of the spatial variation of NEE, 36% of GPP and 19% of Reco, respectively. Both NEE (R<span class="hlt">2</span> = 33%) and GPP (R<span class="hlt">2</span> =25%) were correlated positively with precipitation (P<0.05). However, the relationship between Reco and precipitation was not significant (P>0.05). Across different Chinese wetlands, both precipitation and temperature had no significant effect on apparent quantum yield (α) or ecosystem respiration in the daytime (Reco,day, P>0.05). The maximum photosynthesis rate (Amax) was remarkably correlated with precipitation (P <0.01), but not with <span class="hlt">air</span> temperature. Besides, there was no significant correlation between basal respiration (Rref) and precipitation (P>0.05). Precipitation was negatively correlated with temperature sensitivity of Reco (Q10, P<0.05). Furthermore, temperature accounted for 35% and 46% of the variations in temperature sensitivity of Reco (Q10) and basal respiration (Rref P<0.05), respectively.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70040729','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70040729"><span>The impact of lower <span class="hlt">sea</span>-ice extent on Arctic greenhouse-gas <span class="hlt">exchange</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>Parmentier, Frans-Jan W.; Christensen, Torben R.; Sørensen, Lise Lotte; Rysgaard, Søren; McGuire, A. David; Miller, Paul A.; Walker, Donald A.</p> <p>2013-01-01</p> <p>In September 2012, Arctic <span class="hlt">sea</span>-ice extent plummeted to a new record low: two times lower than the 1979–2000 average. Often, record lows in <span class="hlt">sea</span>-ice cover are hailed as an example of climate change impacts in the Arctic. Less apparent, however, are the implications of reduced <span class="hlt">sea</span>-ice cover in the Arctic Ocean for marine–atmosphere <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span>. <span class="hlt">Sea</span>-ice decline has been connected to increasing <span class="hlt">air</span> temperatures at high latitudes. Temperature is a key controlling factor in the terrestrial <span class="hlt">exchange</span> of <span class="hlt">CO</span><span class="hlt">2</span> and methane, and therefore the greenhouse-gas balance of the Arctic. Despite the large potential for feedbacks, many studies do not connect the diminishing <span class="hlt">sea</span>-ice extent with changes in the interaction of the marine and terrestrial Arctic with the atmosphere. In this Review, we assess how current understanding of the Arctic Ocean and high-latitude ecosystems can be used to predict the impact of a lower <span class="hlt">sea</span>-ice cover on Arctic greenhouse-gas <span class="hlt">exchange</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMOS33A1438C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMOS33A1438C"><span>Seasonal and spatial variations in surface 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> flux in the Chesapeake Bay</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. J.; Chen, B.</p> <p>2017-12-01</p> <p>Bay-wide observations of surface water partial pressure of carbon dioxide (p<span class="hlt">CO</span><span class="hlt">2</span>) were conducted in May, June, August, and October 2016 to study the spatial and seasonal variations in surface p<span class="hlt">CO</span><span class="hlt">2</span> and to estimate <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> flux in the Chesapeake Bay. Overall, high surface p<span class="hlt">CO</span><span class="hlt">2</span> 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 p<span class="hlt">CO</span><span class="hlt">2</span> approached the atmospheric level. Over the course of a year, p<span class="hlt">CO</span><span class="hlt">2</span> was higher than 1000 µatm in the upper bay and the highest p<span class="hlt">CO</span><span class="hlt">2</span> (2500 µatm) was observed in August. Significant biologically-induced p<span class="hlt">CO</span><span class="hlt">2</span> undersaturation was observed at the upper part of the mid-bay in August with p<span class="hlt">CO</span><span class="hlt">2</span> 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 p<span class="hlt">CO</span><span class="hlt">2</span> in the mid-bay as is evidenced by <span class="hlt">co</span>-occurrence of high p<span class="hlt">CO</span><span class="hlt">2</span> 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 <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> flux. Seasonally, the upper-bay acted as a source for atmospheric <span class="hlt">CO</span><span class="hlt">2</span> over the course of a year. The boundary of upper and mid bay transited from a <span class="hlt">CO</span><span class="hlt">2</span> 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 <span class="hlt">CO</span><span class="hlt">2</span> 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 <span class="hlt">CO</span><span class="hlt">2</span> 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</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/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 <span class="hlt">exchange</span> fluxes 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 <span class="hlt">exchange</span> fluxes 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 <span class="hlt">exchange</span> of DDT was characterized by net volatilization with a marked difference in its fluxes 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 <span class="hlt">exchange</span> 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 <span class="hlt">exchange</span> flux of HCH was comparable to the dry and wet deposition fluxes 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 <span class="hlt">exchange</span> flux of DDT was about fivefold higher than the total dry and wet deposition fluxes. 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.A24C2606P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOS.A24C2606P"><span>Surfactant control of <span class="hlt">air-sea</span> gas <span class="hlt">exchange</span> from North <span class="hlt">Sea</span> coastal waters and the Atlantic Meridional Transect</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pereira, R.</p> <p>2016-02-01</p> <p>Suppression of gas transfer velocity (kw) by surfactants are well established, both in laboratory wind flumes and purposeful oceanic releases. However, the effects on kw of time and space varying concentrations of natural surfactant are inadequately studied. We have developed an automated gas <span class="hlt">exchange</span> tank for simultaneous high precision measurement of kw in unmodified seawater samples. Here we present data from two studies along a coastal North <span class="hlt">Sea</span> transect during 2012-2013 and the Atlantic Meridional Transect (AMT) 24 from September to November 2014. Measurements of surfactant activity (SA), CDOM absorbance and chlorophyll-a have enabled us to characterize the effects of variable amounts of natural surfactant on kw. North <span class="hlt">Sea</span> coastal waters range in k660 (kw normalized to the value for <span class="hlt">CO</span><span class="hlt">2</span> in freshwater at 20oC) was 6.8-24.5 cm hr-1 (n=20), with the ranges of SA, total CDOM absorbance (200-450 nm) and chlorophyll-a measured in the surface microlayer (SML) of our seawater samples were 0.08-0.38 mg l-1 T-X-100, 0.13-4.7 and 0.09-1.54 µg l-1, respectively. The AMT k660 ranged from 7.0-23.9 cm hr-1 (n=22), with SA measured in the SML and subsurface water (SSW) of our seawater samples ranging from 0.15-1.08 mg l-1 T-X-100 and 0.07-0.43 mg l-1 T-X-100, respectively. Importantly, we found 12-45% (North <span class="hlt">Sea</span>) and 1-43% (AMT) k660 suppression relative to Milli-Q water that relate to seasonal and spatial differences in SA. The North <span class="hlt">Sea</span> demonstrated notable seasonal influences on k660 suppression that were related to CDOM absorbance and chlorophyll-a. The degree of k660 suppression was highest in summer consistent with k660 control by natural surfactant. The degree of k660 suppression decreased with distance offshore in the North <span class="hlt">Sea</span> and displayed a strong relationship with SA (r<span class="hlt">2</span> = 0.51-0.64, p = 0.02, n = 20). The AMT demonstrated notable differences in k660 suppression between hemispheres and across the Longhurst Provinces but the overall relationship between k660</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.6719V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.6719V"><span><span class="hlt">Air-sea</span> <span class="hlt">exchange</span> over Black <span class="hlt">Sea</span> estimated from high resolution regional climate simulations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Velea, Liliana; Bojariu, Roxana; Cica, Roxana</p> <p>2013-04-01</p> <p>Black <span class="hlt">Sea</span> is an important influencing factor for the climate of bordering countries, showing cyclogenetic activity (Trigo et al, 1999) and influencing Mediterranean cyclones passing over. As for other <span class="hlt">seas</span>, standard observations of the atmosphere are limited in time and space and available observation-based estimations of <span class="hlt">air-sea</span> <span class="hlt">exchange</span> terms present quite large ranges of uncertainty. The reanalysis datasets (e.g. ERA produced by ECMWF) provide promising validation estimates of climatic characteristics against the ones in available climatic data (Schrum et al, 2001), while cannot reproduce some local features due to relatively coarse horizontal resolution. Detailed and realistic information on smaller-scale processes are foreseen to be provided by regional climate models, due to continuous improvements of physical parameterizations and numerical solutions and thus affording simulations at high spatial resolution. The aim of the study is to assess the potential of three regional climate models in reproducing known climatological characteristics of <span class="hlt">air-sea</span> <span class="hlt">exchange</span> over Black <span class="hlt">Sea</span>, as well as to explore the added value of the model compared to the input (reanalysis) data. We employ results of long-term (1961-2000) simulations performed within ENSEMBLE project (http://ensemblesrt3.dmi.dk/) using models ETHZ-CLM, CNRM-ALADIN, METO-HadCM, for which the integration domain covers the whole area of interest. The analysis is performed for the entire basin for several variables entering the heat and water budget terms and available as direct output from the models, at seasonal and annual scale. A comparison with independent data (ERA-INTERIM) and findings from other studies (e.g. Schrum et al, 2001) is also presented. References: Schrum, C., Staneva, J., Stanev, E. and Ozsoy, E., 2001: <span class="hlt">Air-sea</span> <span class="hlt">exchange</span> in the Black <span class="hlt">Sea</span> estimated from atmospheric analysis for the period 1979-1993, J. Marine Systems, 31, 3-19 Trigo, I. F., T. D. Davies, and G. R. Bigg (1999): Objective</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> <span class="hlt">exchange</span> fluxes 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 fluxes 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 fluxes 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 fluxes dominated the <span class="hlt">air-sea</span> gas <span class="hlt">exchange</span> 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/2015AGUFM.A43C0283L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.A43C0283L"><span><span class="hlt">Air-sea</span> <span class="hlt">Exchange</span> 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 <span class="hlt">exchange</span>. No monitoring is in place. We studied the vertical fluxes 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 fluxes were quantified based on Eddy covariance. Diffusive <span class="hlt">air-sea</span> <span class="hlt">exchange</span> fluxes 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. Fluxes 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> <span class="hlt">exchange</span>. 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> <span class="hlt">exchange</span>. The seawater surface as secondary source of pollution should be assessed based on flux measurements across seasons and over longer time periods.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018BoLMe.tmp...23G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018BoLMe.tmp...23G"><span>The Effect of Breaking Waves on <span class="hlt">CO</span>_<span class="hlt">2</span> <span class="hlt">Air-Sea</span> Fluxes 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.; García-Nava, Héctor</p> <p>2018-03-01</p> <p>The influence of wave-associated parameters controlling turbulent <span class="hlt">CO</span>_<span class="hlt">2</span> fluxes through the <span class="hlt">air-sea</span> interface is investigated in a coastal region. A full year of high-quality data of direct estimates of <span class="hlt">air-sea</span> <span class="hlt">CO</span>_<span class="hlt">2</span> fluxes based on eddy-covariance measurements is presented. The study area located in Todos Santos Bay, Baja California, Mexico, is a net sink of <span class="hlt">CO</span>_<span class="hlt">2</span> with a mean flux of -1.3 μmol m^{-<span class="hlt">2</span>}s^{-1} (-41.6 mol m^{-<span class="hlt">2</span>}yr^{-1} ). The results of a quantile-regression analysis computed between the <span class="hlt">CO</span>_<span class="hlt">2</span> flux and, (1) wind speed, (<span class="hlt">2</span>) 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.</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://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 <span class="hlt">exchange</span> and <span class="hlt">CO</span><span class="hlt">2</span> flux 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 flux 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> flux observed in the equatorial zone are examined.</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> Flux 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 <span class="hlt">exchange</span> (natural flux 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> flux 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> flux 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 fluxes into the ocean).</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> <span class="hlt">exchange</span>. 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('http://adsabs.harvard.edu/abs/2015AGUFMOS51B1988M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMOS51B1988M"><span>Effect of Sampling Depth on <span class="hlt">Air-Sea</span> <span class="hlt">CO</span><span class="hlt">2</span> Flux Estimates in River-Stratified Arctic Coastal Waters</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Miller, L. A.; Papakyriakou, T. N.</p> <p>2015-12-01</p> <p>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' p<span class="hlt">CO</span><span class="hlt">2</span> and calculated <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> fluxes. We determined p<span class="hlt">CO</span><span class="hlt">2</span> 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 p<span class="hlt">CO</span><span class="hlt">2</span> derived from typical ship-board versus small-boat sampling at a single station could be nearly 90 μatm, leading to errors in the calculated <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> flux of more than 0.1 mmol/(m<span class="hlt">2</span>s). Attempting to extrapolate such fluxes over the 6,000,000 km<span class="hlt">2</span> area of the Arctic shelves would generate an error approaching a gigamol <span class="hlt">CO</span><span class="hlt">2</span>/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 <span class="hlt">air-sea</span> fluxes in these areas, it is necessary to deploy sensors on ice-capable buoys that can position the sensors in true 'surface' waters.</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> <span class="hlt">exchange</span> 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 <span class="hlt">exchange</span> will be discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013BGeo...10.2699S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013BGeo...10.2699S"><span>Coccolithophore surface distributions in the North Atlantic and their modulation of the <span class="hlt">air-sea</span> flux of <span class="hlt">CO</span><span class="hlt">2</span> from 10 years of satellite Earth observation data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shutler, J. D.; Land, P. E.; Brown, C. W.; Findlay, H. S.; Donlon, C. J.; Medland, M.; Snooke, R.; Blackford, J. C.</p> <p>2013-04-01</p> <p>Coccolithophores are the primary oceanic phytoplankton responsible for the production of calcium carbonate (Ca<span class="hlt">CO</span>3). 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 (<span class="hlt">air-sea</span>) uptake of carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) through increasing the seawater partial pressure of <span class="hlt">CO</span><span class="hlt">2</span> (p<span class="hlt">CO</span><span class="hlt">2</span>). 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 <span class="hlt">Sea</span>-viewing Wide Field-of-view Sensor (<span class="hlt">Sea</span>WiFS). We calculate the annual mean <span class="hlt">sea</span> surface areal coverage of E. huxleyi in the North Atlantic to be 474 000 ± 104 000 km<span class="hlt">2</span>, which results in a net Ca<span class="hlt">CO</span>3 carbon (Ca<span class="hlt">CO</span>3-C) production of 0.14-1.71 Tg Ca<span class="hlt">CO</span>3-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 p<span class="hlt">CO</span><span class="hlt">2</span> and, thus, decrease the localised <span class="hlt">air-sea</span> flux of atmospheric <span class="hlt">CO</span><span class="hlt">2</span>. In regions where the blooms are prevalent, the average reduction in the monthly <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> flux can reach 55%. The maximum reduction of the monthly <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> 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 p<span class="hlt">CO</span><span class="hlt">2</span> should be considered if we are to fully understand the variability of the North Atlantic <span class="hlt">air-to-sea</span> flux of <span class="hlt">CO</span><span class="hlt">2</span>. We estimate that these blooms can reduce the annual N. Atlantic net sink atmospheric <span class="hlt">CO</span><span class="hlt">2</span> by between 3-28%.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28640914','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28640914"><span>Kinetic analysis of an anion <span class="hlt">exchange</span> absorbent 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="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Shi, Xiaoyang; Li, Qibin; Wang, Tao; Lackner, Klaus S</p> <p>2017-01-01</p> <p>This study reports a preparation method of a new moisture swing sorbent for <span class="hlt">CO</span><span class="hlt">2</span> capture from <span class="hlt">air</span>. The new sorbent components include ion <span class="hlt">exchange</span> resin (IER) and polyvinyl chloride (PVC) as a binder. The IER can absorb <span class="hlt">CO</span><span class="hlt">2</span> when surrounding is dry and release <span class="hlt">CO</span><span class="hlt">2</span> when surrounding is wet. The manuscript presents the studies of membrane structure, kinetic model of absorption process, performance of desorption process and the diffusivity of water molecules in the <span class="hlt">CO</span><span class="hlt">2</span> absorbent. It has been proved that the kinetic performance of <span class="hlt">CO</span><span class="hlt">2</span> absorption/desorption can be improved by using thin binder and hot water treatment. The fast kinetics of P-100-90C absorbent is due to the thin PVC binder, and high diffusion rate of H<span class="hlt">2</span>O molecules in the sample. The impressive is this new <span class="hlt">CO</span><span class="hlt">2</span> absorbent has the fastest <span class="hlt">CO</span><span class="hlt">2</span> absorption rate among all absorbents which have been reported by other up-to-date literatures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5480984','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5480984"><span>Kinetic analysis of an anion <span class="hlt">exchange</span> absorbent 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.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Shi, Xiaoyang; Li, Qibin; Lackner, Klaus S.</p> <p>2017-01-01</p> <p>This study reports a preparation method of a new moisture swing sorbent for <span class="hlt">CO</span><span class="hlt">2</span> capture from <span class="hlt">air</span>. The new sorbent components include ion <span class="hlt">exchange</span> resin (IER) and polyvinyl chloride (PVC) as a binder. The IER can absorb <span class="hlt">CO</span><span class="hlt">2</span> when surrounding is dry and release <span class="hlt">CO</span><span class="hlt">2</span> when surrounding is wet. The manuscript presents the studies of membrane structure, kinetic model of absorption process, performance of desorption process and the diffusivity of water molecules in the <span class="hlt">CO</span><span class="hlt">2</span> absorbent. It has been proved that the kinetic performance of <span class="hlt">CO</span><span class="hlt">2</span> absorption/desorption can be improved by using thin binder and hot water treatment. The fast kinetics of P-100-90C absorbent is due to the thin PVC binder, and high diffusion rate of H<span class="hlt">2</span>O molecules in the sample. The impressive is this new <span class="hlt">CO</span><span class="hlt">2</span> absorbent has the fastest <span class="hlt">CO</span><span class="hlt">2</span> absorption rate among all absorbents which have been reported by other up-to-date literatures. PMID:28640914</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013BGeo...10.1379C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013BGeo...10.1379C"><span>Technical Note: A simple method for <span class="hlt">air-sea</span> gas <span class="hlt">exchange</span> measurements in mesocosms and its application in carbon budgeting</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.; Ludwig, A.; Riebesell, U.</p> <p>2013-03-01</p> <p>Mesocosms as large experimental units provide the opportunity to perform elemental mass balance calculations, e.g. to derive net biological turnover rates. However, the system is in most cases not closed at the water surface and gases <span class="hlt">exchange</span> with the atmosphere. Previous attempts to budget carbon pools in mesocosms relied on educated guesses concerning the <span class="hlt">exchange</span> of <span class="hlt">CO</span><span class="hlt">2</span> with the atmosphere. Here, we present a simple method for precise determination of <span class="hlt">air-sea</span> gas <span class="hlt">exchange</span> in mesocosms using N<span class="hlt">2</span>O as a deliberate tracer. Beside the application for carbon budgeting, transfer velocities can be used to calculate <span class="hlt">exchange</span> rates of any gas of known concentration, e.g. to calculate aquatic production rates of climate relevant trace gases. Using an arctic KOSMOS (Kiel Off Shore Mesocosms for future Ocean Simulation) experiment as an exemplary dataset, it is shown that the presented method improves accuracy of carbon budget estimates substantially. Methodology of manipulation, measurement, data processing and conversion to <span class="hlt">CO</span><span class="hlt">2</span> fluxes are explained. A theoretical discussion of prerequisites for precise gas <span class="hlt">exchange</span> measurements provides a guideline for the applicability of the method under various experimental conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016DyAtO..76...14S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016DyAtO..76...14S"><span><span class="hlt">Air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> flux pattern along the southern Bay of Bengal waters</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shanthi, R.; Poornima, D.; Naveen, M.; Thangaradjou, T.; Choudhury, S. B.; Rao, K. H.; Dadhwal, V. K.</p> <p>2016-12-01</p> <p>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 (p<span class="hlt">CO</span><span class="hlt">2</span>: 155.520-1488.607 μatm) and <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> flux (FCO<span class="hlt">2</span>: -4.808 to 11.255 mmol Cm-<span class="hlt">2</span> 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, p<span class="hlt">CO</span><span class="hlt">2</span> and negative flux of <span class="hlt">CO</span><span class="hlt">2</span> 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, p<span class="hlt">CO</span><span class="hlt">2</span> and FCO<span class="hlt">2</span> against atmospheric temperature (AT), lux, <span class="hlt">sea</span> 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 p<span class="hlt">CO</span><span class="hlt">2</span> along the southwest Bay of Bengal. The annual variability of <span class="hlt">CO</span><span class="hlt">2</span> 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 <span class="hlt">CO</span><span class="hlt">2</span> to the atmosphere with a mean flux of 0.204 ± 1.449 mmol Cm-<span class="hlt">2</span> d-1.</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> fluxes 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> fluxes. 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/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 <span class="hlt">exchange</span> 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> fluxes 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 fluxes 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 flux 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> <span class="hlt">exchange</span> 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/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> <span class="hlt">exchange</span>. 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> </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/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> <span class="hlt">exchange</span> 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> <span class="hlt">exchange</span> with the atmosphere and ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22894100','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22894100"><span>Measurement of <span class="hlt">air</span> <span class="hlt">exchange</span> rates in different indoor environments using continuous <span class="hlt">CO</span><span class="hlt">2</span> sensors.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>You, Yan; Niu, Can; Zhou, Jian; Liu, Yating; Bai, Zhipeng; Zhang, Jiefeng; He, Fei; Zhang, Nan</p> <p>2012-01-01</p> <p>A new <span class="hlt">air</span> <span class="hlt">exchange</span> rate (AER) monitoring method using continuous <span class="hlt">CO</span><span class="hlt">2</span> sensors was developed and validated through both laboratory experiments and field studies. Controlled laboratory simulation tests were conducted in a 1-m3 environmental chamber at different AERs (0.1-10.0 hr(-1)). AERs were determined using the decay method based on box model assumptions. Field tests were conducted in classrooms, dormitories, meeting rooms and apartments during <span class="hlt">2</span>-5 weekdays using <span class="hlt">CO</span><span class="hlt">2</span> sensors coupled with data loggers. Indoor temperature, relative humidity (RH), and <span class="hlt">CO</span><span class="hlt">2</span> concentrations were continuously monitored while outdoor parameters combined with on-site climate conditions were recorded. Statistical results indicated that good laboratory performance was achieved: duplicate precision was within 10%, and the measured AERs were 90%-120% of the real AERs. Average AERs were 1.22, 1.37, 1.10, 1.91 and 0.73 hr(-1) in dormitories, <span class="hlt">air</span>-conditioned classrooms, classrooms with an <span class="hlt">air</span> circulation cooling system, reading rooms, and meeting rooms, respectively. In an elderly particulate matter exposure study, all the homes had AER values ranging from 0.29 to 3.46 hr(-1) in fall, and 0.12 to 1.39 hr(-1) in winter with a median AER of 1.15.</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 <span class="hlt">exchange</span> 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 fluxes of <span class="hlt">air-sea</span> gas <span class="hlt">exchange</span> 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 fluxes 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 <span class="hlt">exchange</span> of PAHs was the dominant process at the <span class="hlt">air-sea</span> interface in the YRE as the magnitude of volatilization flux of PAHs exceeded that of total dry and wet deposition. The gas PAH <span class="hlt">exchange</span> flux 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('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 <span class="hlt">exchange</span> 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> fluxes 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 fluxes 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 flux 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> <span class="hlt">exchange</span> 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/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> fluxes 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 surface seawater appears in equilibrium or slightly supersaturated by <span class="hlt">CO</span><span class="hlt">2</span> relative to atmosphere because of the increasing influence of river runoff and its input of terrestrial organic matter that mineralizes, in combination with the high surface water temperature during <span class="hlt">sea</span>-ice-free conditions. This investigation shows the importance of processes that vary on small scales, both in time and space, for estimating the <span class="hlt">air-sea</span> <span class="hlt">exchange</span> of <span class="hlt">CO</span><span class="hlt">2</span>. It stresses the need for high-resolution coverage of ocean observations as well as time series. Furthermore, time series must include multi-year studies in the dynamic regions of the Arctic Ocean during these times of environmental change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22103582','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22103582"><span>Distribution and <span class="hlt">air-sea</span> <span class="hlt">exchange</span> of current-use pesticides (CUPs) from East Asia to the high Arctic Ocean.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhong, Guangcai; Xie, Zhiyong; Cai, Minghong; Möller, Axel; Sturm, Renate; Tang, Jianhui; Zhang, Gan; He, Jianfeng; Ebinghaus, Ralf</p> <p>2012-01-03</p> <p>Surface seawater and marine boundary layer <span class="hlt">air</span> samples were collected on the ice-breaker R/V Xuelong (Snow Dragon) from the East China <span class="hlt">Sea</span> to the high Arctic (33.23-84.5° N) in July to September 2010 and have been analyzed for six current-use pesticides (CUPs): trifluralin, endosulfan, chlorothalonil, chlorpyrifos, dacthal, and dicofol. In all oceanic <span class="hlt">air</span> samples, the six CUPs were detected, showing highest level (>100 pg/m(3)) in the <span class="hlt">Sea</span> of Japan. Gaseous CUPs basically decreased from East Asia (between 36.6 and 45.1° N) toward Bering and Chukchi <span class="hlt">Seas</span>. The dissolved CUPs in ocean water ranged widely from <MDL to 111 pg/L. Latitudinal trends of α-endosulfan, chlorpyrifos, and dicofol in seawater were roughly consistent with their latitudinal trends in <span class="hlt">air</span>. Trifluralin in seawater was relatively high in the <span class="hlt">Sea</span> of Japan (35.<span class="hlt">2</span>° N) and evenly distributed between 36.9 and 72.5° N, but it remained below the detection limit at the highest northern latitudes in Chukchi <span class="hlt">Sea</span>. In contrast with other CUPs, concentrations of chlorothalonil and dacthal were more abundant in Chukchi <span class="hlt">Sea</span> and in East Asia. The <span class="hlt">air-sea</span> gas <span class="hlt">exchange</span> of CUPs was generally dominated by net deposition. Latitudinal trends of fugacity ratios of α-endosulfan, chlorothalonil, and dacthal showed stronger deposition of these compounds in East Asia than in Chukchi <span class="hlt">Sea</span>, while trifluralin showed stronger deposition in Chukchi <span class="hlt">Sea</span> (-455 ± 245 pg/m(<span class="hlt">2</span>)/day) than in the North Pacific (-241 ± 158 pg/m(<span class="hlt">2</span>)/day). <span class="hlt">Air-sea</span> gas <span class="hlt">exchange</span> of chlorpyrifos varied from net volatilizaiton in East Asia (<40° N) to equilibrium or net deposition in the North Pacific and the Arctic.</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> fluxes 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> fluxes 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> fluxes 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> fluxes 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('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>} fluxes 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 <span class="hlt">Exchange</span> 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> <span class="hlt">exchange</span> of gases, and a comparison of experimental methods to derive the <span class="hlt">exchange</span> 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 fluxes 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>} flux measurements and the bubble measurements. The latter was made as part of a larger study on the influence of bubbles on gas <span class="hlt">exchange</span> 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/2016AGUFMOS31A1997S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS31A1997S"><span>Comparison of <span class="hlt">Sea-Air</span> <span class="hlt">CO</span><span class="hlt">2</span> Flux Estimates Using Satellite-Based Versus Mooring Wind Speed Data</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.; Sabine, C. L.; Feely, R. A.; Wanninkhof, R. H.</p> <p>2016-12-01</p> <p>The global ocean is a major sink of anthropogenic <span class="hlt">CO</span><span class="hlt">2</span>, absorbing approximately 27% of <span class="hlt">CO</span><span class="hlt">2</span> emissions since the beginning of the industrial revolution. Any variation or change in the ocean <span class="hlt">CO</span><span class="hlt">2</span> sink has implications for future climate. Observations of <span class="hlt">sea-air</span> <span class="hlt">CO</span><span class="hlt">2</span> flux have relied primarily on ship-based underway measurements of partial pressure of <span class="hlt">CO</span><span class="hlt">2</span> (p<span class="hlt">CO</span><span class="hlt">2</span>) combined with satellite, model, or multi-platform wind products. Direct measurements of Δp<span class="hlt">CO</span><span class="hlt">2</span> (seawater - <span class="hlt">air</span> p<span class="hlt">CO</span><span class="hlt">2</span>) and wind speed from moored platforms now allow for high-resolution <span class="hlt">CO</span><span class="hlt">2</span> flux time series. Here we present a comparison of <span class="hlt">CO</span><span class="hlt">2</span> flux calculated from moored Δp<span class="hlt">CO</span><span class="hlt">2</span> measured on four moorings in different biomes of the Pacific Ocean in combination with: 1) Cross-Calibrated Multi-Platform (CCMP) winds or <span class="hlt">2</span>) wind speed measurements made on ocean reference moorings excluded from the CCMP dataset. Preliminary results show using CCMP winds overestimates <span class="hlt">CO</span><span class="hlt">2</span> flux on average by 5% at the Kuroshio Extension Observatory, Ocean Station Papa, WHOI Hawaii Ocean Timeseries Station, and Stratus. In general, <span class="hlt">CO</span><span class="hlt">2</span> flux seasonality follows patterns of seawater p<span class="hlt">CO</span><span class="hlt">2</span> and SST with periods of <span class="hlt">CO</span><span class="hlt">2</span> outgassing during summer and <span class="hlt">CO</span><span class="hlt">2</span> 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 <span class="hlt">CO</span><span class="hlt">2</span> flux estimates and discuss the potential implications for tracking variability and change in global ocean <span class="hlt">CO</span><span class="hlt">2</span> uptake.</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 <span class="hlt">exchange</span></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 <span class="hlt">exchange</span> 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 flux 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('http://adsabs.harvard.edu/abs/1980Tell...32..470H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1980Tell...32..470H"><span>Gas <span class="hlt">exchange</span> across the <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>Hasse, L.; Liss, P. S.</p> <p>1980-10-01</p> <p>The physics of gas <span class="hlt">exchange</span> at the <span class="hlt">air-sea</span> interface are reviewed. In order to describe the transfer of gases in the liquid near the boundary, a molecular plus eddy diffusivity concept is used, which has been found useful for smooth flow over solid surfaces. From consideration of the boundary conditions, a similar dependence of eddy diffusivity on distance from the interface can be derived for the flow beneath a gas/liquid interface, at least in the absence of waves. The influence of waves is then discussed. It is evident from scale considerations that the effect of gravity waves is small. It is known from wind tunnel work that capillary waves enhance gas transfer considerably. The existing hypotheses are apparently not sufficient to explain the observations. Examination of field data is even more frustrating since the data do not show the expected increase of gas <span class="hlt">exchange</span> with wind speed.</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> <span class="hlt">exchange</span>.</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> <span class="hlt">exchange</span>. 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 flux 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/2016E%26ES...35a2003A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016E%26ES...35a2003A"><span>The potential role of <span class="hlt">sea</span> spray droplets in facilitating <span class="hlt">air-sea</span> gas transfer</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Andreas, E. L.; Vlahos, P.; Monahan, E. C.</p> <p>2016-05-01</p> <p>For over 30 years, <span class="hlt">air-sea</span> interaction specialists have been evaluating and parameterizing the role of whitecap bubbles in <span class="hlt">air-sea</span> gas <span class="hlt">exchange</span>. To our knowledge, no one, however, has studied the mirror image process of whether <span class="hlt">sea</span> spray droplets can facilitate <span class="hlt">air-sea</span> gas <span class="hlt">exchange</span>. We are therefore using theory, data analysis, and numerical modeling to quantify the role of spray on <span class="hlt">air-sea</span> gas transfer. In this, our first formal work on this subject, we seek the rate-limiting step in spray-mediated gas transfer by evaluating the three time scales that govern the <span class="hlt">exchange</span>: τ <span class="hlt">air</span> , which quantifies the rate of transfer between the atmospheric gas reservoir and the surface of the droplet; τ int , which quantifies the <span class="hlt">exchange</span> rate across the <span class="hlt">air</span>-droplet interface; and τ aq , which quantifies gas mixing within the aqueous solution droplet.</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> flux 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> fluxes 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> fluxes, 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 fluxes 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> fluxes. 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> flux 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('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 <span class="hlt">Exchange</span> 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('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> <span class="hlt">exchange</span>. 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> <span class="hlt">exchange</span> 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/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 <span class="hlt">exchange</span> 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 fluxes of <span class="hlt">air-sea</span> gaseous <span class="hlt">exchange</span> 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 fluxes 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 <span class="hlt">exchange</span> 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 flux of PAHs exceeded that of the total dry and wet deposition. The gaseous PAH <span class="hlt">exchange</span> flux 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/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 <span class="hlt">exchange</span>: 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> <span class="hlt">exchange</span>. An atmospheric transport inversion of APO data from the Scripps flask network shows significant interannual variability in tropical APO fluxes 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 flux 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> <span class="hlt">exchange</span>. 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/2002GMS...127..141S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002GMS...127..141S"><span>A model of <span class="hlt">air-sea</span> gas <span class="hlt">exchange</span> incorporating the physics of the turbulent boundary layer and the properties of the <span class="hlt">sea</span> surface</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Soloviev, Alexander; Schluessel, Peter</p> <p></p> <p>The model presented contains interfacial, bubble-mediated, ocean mixed layer, and remote sensing components. The interfacial (direct) gas transfer dominates under conditions of low and—for quite soluble gases like <span class="hlt">CO</span><span class="hlt">2</span>—moderate wind speeds. Due to the similarity between the gas and heat transfer, the temperature difference, ΔT, across the thermal molecular boundary layer (cool skin of the ocean) and the interfacial gas transfer coefficient, Kint are presumably interrelated. A coupled parameterization for ΔT and Kint has been derived in the context of a surface renewal model [Soloviev and Schluessel, 1994]. In addition to the Schmidt, Sc, and Prandtl, Pr, numbers, the important parameters are the surface Richardson number, Rƒ0, and the Keulegan number, Ke. The more readily available cool skin data are used to determine the coefficients that enter into both parameterizations. At high wind speeds, the Ke-number dependence is further verified with the formula for transformation of the surface wind stress to form drag and white capping, which follows from the renewal model. A further extension of the renewal model includes effects of solar radiation and rainfall. The bubble-mediated component incorporates the Merlivat et al. [1993] parameterization with the empirical coefficients estimated by Asher and Wanninkhof [1998]. The oceanic mixed layer component accounts for stratification effects on the <span class="hlt">air-sea</span> gas <span class="hlt">exchange</span>. Based on the example of GasEx-98, we demonstrate how the results of parameterization and modeling of the <span class="hlt">air-sea</span> gas <span class="hlt">exchange</span> can be extended to the global scale, using remote sensing techniques.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17379807','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17379807"><span>Bottom-up determination of <span class="hlt">air-sea</span> momentum <span class="hlt">exchange</span> under a major tropical cyclone.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Jarosz, Ewa; Mitchell, Douglas A; Wang, David W; Teague, William J</p> <p>2007-03-23</p> <p>As a result of increasing frequency and intensity of tropical cyclones, an accurate forecasting of cyclone evolution and ocean response is becoming even more important to reduce threats to lives and property in coastal regions. To improve predictions, accurate evaluation of the <span class="hlt">air-sea</span> momentum <span class="hlt">exchange</span> is required. Using current observations recorded during a major tropical cyclone, we have estimated this momentum transfer from the ocean side of the <span class="hlt">air-sea</span> interface, and we discuss it in terms of the drag coefficient. For winds between 20 and 48 meters per second, this coefficient initially increases and peaks at winds of about 32 meters per second before decreasing.</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/2002EGSGA..27..874S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002EGSGA..27..874S"><span>Observational Studies of Parameters Influencing <span class="hlt">Air-sea</span> Gas <span class="hlt">Exchange</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schimpf, U.; Frew, N. M.; Bock, E. J.; Hara, T.; Garbe, C. S.; Jaehne, B.</p> <p></p> <p>A physically-based modeling of the <span class="hlt">air-sea</span> gas transfer that can be used to predict the gas transfer rates with sufficient accuracy as a function of micrometeorological parameters is still lacking. State of the art are still simple gas transfer rate/wind speed relationships. Previous measurements from Coastal Ocean Experiment in the Atlantic revealed positive correlations between mean square slope, near surface turbulent dis- sipation, and wind stress. It also demonstrated a strong negative correlation between mean square slope and the fluorescence of surface-enriched colored dissolved organic matter. Using heat as a proxy tracer for gases the <span class="hlt">exchange</span> process at the <span class="hlt">air</span>/water interface and the micro turbulence at the water surface can be investigated. The anal- ysis of infrared image sequences allow the determination of the net heat flux at the ocean surface, the temperature gradient across the <span class="hlt">air/sea</span> interface and thus the heat transfer velocity and gas transfer velocity respectively. Laboratory studies were carried out in the new Heidelberg wind-wave facility AELOTRON. Direct measurements of the Schmidt number exponent were done in conjunction with classical mass balance methods to estimate the transfer velocity. The laboratory results allowed to validate the basic assumptions of the so called controlled flux technique by applying differ- ent tracers for the gas <span class="hlt">exchange</span> in a large Schmidt number regime. Thus a modeling of the Schmidt number exponent is able to fill the gap between laboratory and field measurements field. Both, the results from the laboratory and the field measurements should be able to give a further understanding of the mechanisms controlling the trans- port processes across the aqueous boundary layer and to relate the forcing functions to parameters measured by remote sensing.</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> fluxes (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 flux measurements of <span class="hlt">air</span>-ice <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span>. 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/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> <span class="hlt">exchange</span> (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> <span class="hlt">exchange</span>. 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> <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> fluxes 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 fluxes 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> flux 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://adsabs.harvard.edu/abs/2016AGUOSEC54B1327H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSEC54B1327H"><span>First System-Wide Estimates of <span class="hlt">Air-Sea</span> <span class="hlt">Exchange</span> of Carbon Dioxide in the Chesapeake Bay</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Herrmann, M.; Najjar, R.; Menendez, A.</p> <p>2016-02-01</p> <p>Estuaries are estimated to play a major role in the global carbon cycle by degassing between 0.25 and 0.4 Pg C y-1, comparable to the uptake of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> by continental shelf waters and as much as one quarter of the uptake of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> by the open ocean. However, the global estimates of estuarine <span class="hlt">CO</span><span class="hlt">2</span> gas <span class="hlt">exchange</span> are highly uncertain mostly due to limited data availability and extreme heterogeneity of coastal systems. Notably, the <span class="hlt">air</span>-water <span class="hlt">CO</span><span class="hlt">2</span> flux for the largest U.S. estuary, the Chesapeake Bay, is yet unknown. Here we provide first system-level <span class="hlt">CO</span><span class="hlt">2</span> gas <span class="hlt">exchange</span> estimates for the Chesapeake Bay, using data from the Chesapeake Bay Water Quality Monitoring Program (CBWQMP) and other data sources. We focus on the main stem of the Chesapeake Bay; hence, tributaries, such as the tidal portions of the Potomac and James Rivers, are not included in this first estimation of the flux. The preliminary results show the Bay to be a net source of <span class="hlt">CO</span><span class="hlt">2</span> to the atmosphere, outgassing on average 0.<span class="hlt">2</span> Tg C yr-1 over the study period, between 1985 and 2013. The spatial and temporal variability of the gas <span class="hlt">exchange</span> will be discussed.</p> </li> <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> fluxes 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 flux 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 flux 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> fluxes of a cool skin on the <span class="hlt">sea</span> surface is large and ubiquitous. An opposing effect on calculated fluxes 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 <span class="hlt">exchange</span>. A salty skin and salinity anomalies in the upper ocean also affect <span class="hlt">CO</span><span class="hlt">2</span> flux calculations, though these haline effects are generally weaker than the thermal effects.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930036604&hterms=CO2+H2O&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DCO2%2BH2O','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930036604&hterms=CO2+H2O&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DCO2%2BH2O"><span><span class="hlt">Air</span>-surface <span class="hlt">exchange</span> of H<span class="hlt">2</span>O, <span class="hlt">CO</span><span class="hlt">2</span>, and O3 at a tallgrass prairie in relation to remotely sensed vegetation indices</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gao, W.; Wesely, M. L.; Cook, D. R.; Hart, R. L.</p> <p>1992-01-01</p> <p>Parameters derived from eddy correlation measurements of the <span class="hlt">air</span>-surface <span class="hlt">exchange</span> rates of H<span class="hlt">2</span>O, <span class="hlt">CO</span><span class="hlt">2</span>, and O3 over a tallgrass prairie are examined in terms of their relationships with spectral reflectance data remotely sensed from aircraft and satellites during the four 1987 intensive field campaigns of the First ISLSCP Field Experiment (FIFE). The surface conductances were strongly modulated by photosynthetically active radiation received at the surface when the grass was green and well watered; mesophyll resistances were large for <span class="hlt">CO</span><span class="hlt">2</span> but negligible for H<span class="hlt">2</span>O and O3.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A43G2558W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A43G2558W"><span><span class="hlt">Air-sea</span> <span class="hlt">exchange</span> and gas-particle partitioning of polycyclic aromatic hydrocarbons over the northwestern Pacific Ocean: Role of East Asian continental outflow</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wu, Z.; Guo, Z.</p> <p>2017-12-01</p> <p>We measured 15 parent polycyclic aromatic hydrocarbons (PAHs) in atmosphere and water during a research cruise from the East China <span class="hlt">Sea</span> (ECS) to the northwestern Pacific Ocean (NWP) in the spring of 2015 to investigate the occurrence, <span class="hlt">air-sea</span> gas <span class="hlt">exchange</span>, and gas-particle partitioning of PAHs with a particular focus on the influence of East Asian continental outflow. The gaseous PAH composition and identification of sources were consistent with PAHs from the upwind area, indicating that the gaseous PAHs (three- to five-ring PAHs) were influenced by upwind land pollution. In addition, <span class="hlt">air-sea</span> <span class="hlt">exchange</span> fluxes of gaseous PAHs were estimated to be -54.<span class="hlt">2</span> to 107.4 ng m-<span class="hlt">2</span> d-1, and was indicative of variations of land-based PAH inputs. The logarithmic gas-particle partition coefficient (logKp) of PAHs regressed linearly against the logarithmic subcooled liquid vapor pressure, with a slope of -0.25. This was significantly larger than the theoretical value (-1), implying disequilibrium between the gaseous and particulate PAHs over the NWP. The non-equilibrium of PAH gas-particle partitioning was shielded from the volatilization of three-ring gaseous PAHs from seawater and lower soot concentrations in particular when the oceanic <span class="hlt">air</span> masses prevailed. Modeling PAH absorption into organic matter and adsorption onto soot carbon revealed that the status of PAH gas-particle partitioning deviated more from the modeling Kp for oceanic <span class="hlt">air</span> masses than those for continental <span class="hlt">air</span> masses, which coincided with higher volatilization of three-ring PAHs and confirmed the influence of <span class="hlt">air-sea</span> <span class="hlt">exchange</span>. Meanwhile, significant linear regressions between logKp and logKoa (logKsa) for PAHs were observed for continental <span class="hlt">air</span> masses, suggesting the dominant effect of East Asian continental outflow on atmospheric PAHs over the NWP during the sampling campaign.</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 <span class="hlt">exchange</span> 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 <span class="hlt">exchange</span>. 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 flux 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 flux 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 flux 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 flux 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('http://adsabs.harvard.edu/abs/2016AtmEn.147..200O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AtmEn.147..200O"><span>Determination of temperature dependent Henry's law constants of polychlorinated naphthalenes: Application to <span class="hlt">air-sea</span> <span class="hlt">exchange</span> in Izmir Bay, Turkey</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Odabasi, Mustafa; Adali, Mutlu</p> <p>2016-12-01</p> <p>The Henry's law constant (H) is a crucial variable to investigate the <span class="hlt">air</span>-water <span class="hlt">exchange</span> of persistent organic pollutants. H values for 32 polychlorinated naphthalene (PCN) congeners were measured using an inert gas-stripping technique at five temperatures ranging between 5 and 35 °C. H values in deionized water (at 25 °C) varied between 0.28 ± 0.08 Pa m3 mol-1 (PCN-73) and 18.01 ± 0.69 Pa m3 mol-1 (PCN-42). The agreement between the measured and estimated H values from the octanol-water and octanol-<span class="hlt">air</span> partition coefficients was good (measured/estimated ratio = 1.00 ± 0.41, average ± SD). The calculated phase change enthalpies (ΔHH) were within the interval previously determined for other several semivolatile organic compounds (42.0-106.4 kJ mol-1). Measured H values, paired atmospheric and aqueous concentrations and meteorological variables were also used to reveal the level and direction of <span class="hlt">air-sea</span> <span class="hlt">exchange</span> fluxes of PCNs at the coast of Izmir Bay, Turkey. The net PCN <span class="hlt">air-sea</span> <span class="hlt">exchange</span> flux varied from -0.55 (volatilization, PCN-24/14) to <span class="hlt">2</span>.05 (deposition, PCN-23) ng m-<span class="hlt">2</span> day-1. PCN-19, PCN-24/14, PCN-42, and PCN-33/34/37 were mainly volatilized from seawater while the remaining congeners were mainly deposited. The overall number of the cases showing deposition was higher (67.9%) compared to volatilization (21.4%) and near equilibrium (10.7%).</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> <span class="hlt">exchange</span> 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> <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> flux 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> flux has been computed using the NCEP/NCAR 41-year mean monthly wind speeds. An annual net uptake flux 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 flux 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 flux 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('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 <span class="hlt">exchange</span> 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> fluxes, 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> flux 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://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> <span class="hlt">exchange</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>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> flux was directly measured above a small, woodland lake using the eddy covariance technique and compared with fluxes deduced from changes in measured lake-water <span class="hlt">CO</span><span class="hlt">2</span> storage and with flux predictions from boundary-layer and surface-renewal models. Over a 3-yr period, lake-atmosphere <span class="hlt">exchanges</span> 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 flux (-0.17 ??mol m-<span class="hlt">2</span> s-1) to the lake's surface, while late fall flux 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 fluxes well above the detection limits of eddy covariance instruments, facilitating the testing of different gas flux methodologies and <span class="hlt">air</span>-water gas-transfer models. Although there was an overall agreement in fluxes 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 flux measurements and fluxes 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> flux, indicates that in most instances the surface-renewal model underpredicts actual flux. 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/1998IJBm...42...16T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1998IJBm...42...16T"><span>Increase in the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> rate of leaves of Ilex rotunda with elevated atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentration in an urban canyon</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Takagi, M.; Gyokusen, Koichiro; Saito, Akira</p> <p></p> <p>It was found that the atmospheric carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) concentration in an urban canyon in Fukuoka city, Japan during August 1997 was about 30 µmol mol-1 higher than that in the suburbs. When fully exposed to sunlight, in situ the rate of photosynthesis in single leaves of Ilex rotunda planted in the urban canyon was higher when the atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentration was elevated. A biochemically based model was able to predict the in situ rate of photosynthesis well. The model also predicted an increase in the daily <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> rate for leaves in the urban canyon with an increase in atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentration. However, in situ such an increase in the daily <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> rate may be offset by diminished sunlight, a higher <span class="hlt">air</span> temperature and a lower relative humidity. Thus, the daily <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> rate predicted using the model based soleley on the environmental conditions prevailing in the urban canyon was lower than that predicted based only on environmental factors found in the suburbs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28675854','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28675854"><span><span class="hlt">Air-sea</span> <span class="hlt">exchange</span> and gas-particle partitioning of polycyclic aromatic hydrocarbons over the northwestern Pacific Ocean: Role of East Asian continental outflow.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wu, Zilan; Lin, Tian; Li, Zhongxia; Jiang, Yuqing; Li, Yuanyuan; Yao, Xiaohong; Gao, Huiwang; Guo, Zhigang</p> <p>2017-11-01</p> <p>We measured 15 parent polycyclic aromatic hydrocarbons (PAHs) in atmosphere and water during a research cruise from the East China <span class="hlt">Sea</span> (ECS) to the northwestern Pacific Ocean (NWP) in the spring of 2015 to investigate the occurrence, <span class="hlt">air-sea</span> gas <span class="hlt">exchange</span>, and gas-particle partitioning of PAHs with a particular focus on the influence of East Asian continental outflow. The gaseous PAH composition and identification of sources were consistent with PAHs from the upwind area, indicating that the gaseous PAHs (three-to five-ring PAHs) were influenced by upwind land pollution. In addition, <span class="hlt">air-sea</span> <span class="hlt">exchange</span> fluxes of gaseous PAHs were estimated to be -54.<span class="hlt">2</span>-107.4 ng m -<span class="hlt">2</span> d -1 , and was indicative of variations of land-based PAH inputs. The logarithmic gas-particle partition coefficient (logK p ) of PAHs regressed linearly against the logarithmic subcooled liquid vapor pressure (logP L 0 ), with a slope of -0.25. This was significantly larger than the theoretical value (-1), implying disequilibrium between the gaseous and particulate PAHs over the NWP. The non-equilibrium of PAH gas-particle partitioning was shielded from the volatilization of three-ring gaseous PAHs from seawater and lower soot concentrations in particular when the oceanic <span class="hlt">air</span> masses prevailed. Modeling PAH absorption into organic matter and adsorption onto soot carbon revealed that the status of PAH gas-particle partitioning deviated more from the modeling K p for oceanic <span class="hlt">air</span> masses than those for continental <span class="hlt">air</span> masses, which coincided with higher volatilization of three-ring PAHs and confirmed the influence of <span class="hlt">air-sea</span> <span class="hlt">exchange</span>. Meanwhile, significant linear regressions between logK p and logK oa (logK sa ) for PAHs were observed for continental <span class="hlt">air</span> masses, suggesting the dominant effect of East Asian continental outflow on atmospheric PAHs over the NWP during the sampling campaign. Copyright © 2017 Elsevier Ltd. All rights reserved.</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> flux 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/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> Fluxes 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> fluxes 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> fluxes in this region.</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> <span class="hlt">exchange</span> 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> <span class="hlt">exchange</span> 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) flux, 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) fluxes 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) fluxes 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/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> </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('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> flux 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-<span class="hlt">exchange</span> transfer velocity were then used to calculate Hg0 <span class="hlt">sea-air</span> fluxes 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> flux was thus determined. In winter, the flux was low and changed in direction. In summer, a strong emission flux 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/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 <span class="hlt">exchanges</span> 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('https://www.ncbi.nlm.nih.gov/pubmed/29192766','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29192766"><span>Cation-<span class="hlt">Exchanged</span> Zeolitic Chalcogenides for <span class="hlt">CO</span><span class="hlt">2</span> Adsorption.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yang, Huajun; Luo, Min; Chen, Xitong; Zhao, Xiang; Lin, Jian; Hu, Dandan; Li, Dongsheng; Bu, Xianhui; Feng, Pingyun; Wu, Tao</p> <p>2017-12-18</p> <p>We report here the intrinsic advantages of a special family of porous chalcogenides for <span class="hlt">CO</span> <span class="hlt">2</span> adsorption in terms of high selectivity of <span class="hlt">CO</span> <span class="hlt">2</span> /N <span class="hlt">2</span> , large uptake capacity, and robust structure due to their first-ever unique integration of the chalcogen-soft surface, high porosity, all-inorganic crystalline framework, and the tunable charge-to-volume ratio of <span class="hlt">exchangeable</span> cations. Although tuning the <span class="hlt">CO</span> <span class="hlt">2</span> adsorption properties via the type of <span class="hlt">exchangeable</span> cations has been well-studied in oxides and MOFs, little is known about the effects of inorganic <span class="hlt">exchangeable</span> cations in porous chalcogenides, in part because ion <span class="hlt">exchange</span> in chalcogenides can be very sluggish and incomplete due to their soft character. We have demonstrated that, through a methodological change to progressively tune the host-guest interactions, both facile and nearly complete ion <span class="hlt">exchange</span> can be accomplished. Herein, a series of cation-<span class="hlt">exchanged</span> zeolitic chalcogenides (denoted as M@RWY) were studied for the first time for <span class="hlt">CO</span> <span class="hlt">2</span> adsorption. Samples were prepared through a sequential ion-<span class="hlt">exchange</span> strategy, and Cs + -, Rb + -, and K + -<span class="hlt">exchanged</span> samples demonstrated excellent <span class="hlt">CO</span> <span class="hlt">2</span> adsorption performance. Particularly, K@RWY has the superior <span class="hlt">CO</span> <span class="hlt">2</span> /N <span class="hlt">2</span> selectivity with the N <span class="hlt">2</span> adsorption even undetected at either 298 or 273 K. It also has the large uptake of 6.3 mmol/g (141 cm 3 /g) at 273 K and 1 atm with an isosteric heat of 35-41 kJ mol -1 , the best among known porous chalcogenides. Moreover, it permits a facile regeneration and exhibits an excellent recyclability, as shown by the multicycling adsorption experiments. Notably, K@RWY also demonstrates a strong tolerance toward water.</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('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 fluxes derived from the Weather Research and Forecasting model and <span class="hlt">sea</span> surface temperature (SST) from the Regional Ocean Modeling System are <span class="hlt">exchanged</span> 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 fluxes 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 flux dominates the upper ocean heat content variations. Results clearly show that dynamic air–<span class="hlt">sea</span> interactions affecting momentum and buoyancy flux <span class="hlt">exchanges</span> in ETCs need to be resolved accurately in a coupled atmosphere–ocean modeling framework.</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> <span class="hlt">exchange</span> 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) flux. 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) flux (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) flux: 3.6 ± <span class="hlt">2</span>.8 ng m(-<span class="hlt">2</span>) h(-1)). The emission flux 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/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> <span class="hlt">exchange</span> 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><span class="hlt">Exchange</span> 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 flux 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 flux. 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 flux 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('http://adsabs.harvard.edu/abs/2017JGRC..122.8034B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.8034B"><span>Wind Speed and <span class="hlt">Sea</span> State Dependencies of <span class="hlt">Air-Sea</span> Gas Transfer: Results From the High Wind Speed Gas <span class="hlt">Exchange</span> Study (HiWinGS)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Blomquist, B. W.; Brumer, S. E.; Fairall, C. W.; Huebert, B. J.; Zappa, C. J.; Brooks, I. M.; Yang, M.; Bariteau, L.; Prytherch, J.; Hare, J. E.; Czerski, H.; Matei, A.; Pascal, R. W.</p> <p>2017-10-01</p> <p>A variety of physical mechanisms are jointly responsible for facilitating <span class="hlt">air-sea</span> gas transfer through turbulent processes at the atmosphere-ocean interface. The nature and relative importance of these mechanisms evolves with increasing wind speed. Theoretical and modeling approaches are advancing, but the limited quantity of observational data at high wind speeds hinders the assessment of these efforts. The HiWinGS project successfully measured gas transfer coefficients (k660) with coincident wave statistics under conditions with hourly mean wind speeds up to 24 m s-1 and significant wave heights to 8 m. Measurements of k660 for carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) and dimethylsulfide (DMS) show an increasing trend with respect to 10 m neutral wind speed (U10N), following a power law relationship of the form: k660 <span class="hlt">CO</span><span class="hlt">2</span>˜U10N1.68 and k660 dms˜U10N1.33. Among seven high wind speed events, <span class="hlt">CO</span><span class="hlt">2</span> transfer responded to the intensity of wave breaking, which depended on both wind speed and <span class="hlt">sea</span> state in a complex manner, with k660 <span class="hlt">CO</span><span class="hlt">2</span> increasing as the wind <span class="hlt">sea</span> approaches full development. A similar response is not observed for DMS. These results confirm the importance of breaking waves and bubble injection mechanisms in facilitating <span class="hlt">CO</span><span class="hlt">2</span> transfer. A modified version of the Coupled Ocean-Atmosphere Response Experiment Gas transfer algorithm (COAREG ver. 3.5), incorporating a <span class="hlt">sea</span> state-dependent calculation of bubble-mediated transfer, successfully reproduces the mean trend in observed k660 with wind speed for both gases. Significant suppression of gas transfer by large waves was not observed during HiWinGS, in contrast to results from two prior field programs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1996AnGeo..14..342S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1996AnGeo..14..342S"><span>Seasonal change in <span class="hlt">CO</span><span class="hlt">2</span> and H<span class="hlt">2</span>O <span class="hlt">exchange</span> between grassland and atmosphere</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Saigusa, N.; Liu, S.; Oikawa, T.; Watanabe, T.</p> <p>1996-03-01</p> <p>The seasonal change in <span class="hlt">CO</span><span class="hlt">2</span> flux over an artificial grassland was analyzed from the ecological and meteorological point of view. This grassland contains C3 and C4 plants; the three dominant species belonging to the Gramineae; Festuca elatior (C3) dominated in early spring, and Imperata cylindrica (C4) and Andropogon virginicus (C4) grew during early summer and became dominant in mid-summer. <span class="hlt">CO</span><span class="hlt">2</span> flux was measured by the gradient method, and the routinely observed data for the surface-heat budget were used to analyze the <span class="hlt">CO</span><span class="hlt">2</span> and H<span class="hlt">2</span>O <span class="hlt">exchange</span> between the grassland and atmosphere. From August to October in 1993, <span class="hlt">CO</span><span class="hlt">2</span> flux was reduced to around half under the same solar-radiation conditions, while H<span class="hlt">2</span>O flux decreased 20% during the same period. The monthly values of water use efficiency, i.e., ratio of <span class="hlt">CO</span><span class="hlt">2</span> flux to H<span class="hlt">2</span>O flux decreased from 5.8 to 3.3 mg <span class="hlt">CO</span><span class="hlt">2</span>/g H<span class="hlt">2</span>O from August to October, the Bowen ratio increased from 0.20 to 0.30, and the ratio of the bulk latent heat transfer coefficient CE to the sensible heat transfer coefficient CH was maintained around 0.40-0.50. The increase in the Bowen ratio was explained by the decrease in <span class="hlt">air</span> temperature from 22.3 °C in August to 16.6 °C in October without considering biological effects such as stomatal closure on the individual leaves. The nearly constant CE/CH ratios suggested that the contribution ratio of canopy resistance to aerodynamic resistance did not change markedly, although the meteorological conditions changed seasonally. The decrease in the water use efficiency, however, suggested that the photosynthetic rate decreased for individual leaves from August to October under the same radiation conditions. Diurnal variations of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> were simulated by the multi-layer canopy model taking into account the differences in the stomatal conductance and photosynthetic pathway between C3 and C4 plants. The results suggested that C4 plants played a major role in the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> in August, the contribution of C4 plants</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> <span class="hlt">exchange</span> 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> <span class="hlt">exchange</span> 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> <span class="hlt">exchange</span> 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://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/2017EGUGA..1917686R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1917686R"><span>Uncertainty of the global oceanic <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> at the <span class="hlt">air</span>-water interface induced by the choice of the gas <span class="hlt">exchange</span> velocity formulation and the wind product: quantification and spatial analysis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Roobaert, Alizee; Laruelle, Goulven; Landschützer, Peter; Regnier, Pierre</p> <p>2017-04-01</p> <p>In lakes, rivers, estuaries and the ocean, the quantification of <span class="hlt">air</span>-water <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> (FCO<span class="hlt">2</span>) is still characterized by large uncertainties partly due to the lack of agreement over the parameterization of the gas <span class="hlt">exchange</span> velocity (k). Although the ocean is generally regarded as the best constrained system because k is only controlled by the wind speed, numerous formulations are still currently used, leading to potentially large differences in FCO<span class="hlt">2</span>. Here, a quantitative global spatial analysis of FCO<span class="hlt">2</span> is presented using several k-wind speed formulations in order to compare the effect of the choice of parameterization of k on FCO<span class="hlt">2</span>. This analysis is performed at a 1 degree resolution using a <span class="hlt">sea</span> surface p<span class="hlt">CO</span><span class="hlt">2</span> product generated using a two-step artificial neuronal network by Landschützer et al. (2015) over the 1991-2011 period. Four different global wind speed datasets (CCMP, ERA, NCEP 1 and NCEP <span class="hlt">2</span>) are also used to assess the effect of the choice of one wind speed product over the other when calculating the global and regional oceanic FCO<span class="hlt">2</span>. Results indicate that this choice of wind speed product only leads to small discrepancies globally (6 %) except with NCEP <span class="hlt">2</span> which produces a more intense global FCO<span class="hlt">2</span> compared to the other wind products. Regionally, theses differences are even more pronounced. For a given wind speed product, the choice of parametrization of k yields global FCO<span class="hlt">2</span> differences ranging from 7 % to 16 % depending on the wind product used. We also provide latitudinal profiles of FCO<span class="hlt">2</span> and its uncertainty calculated combining all combinations between the different k-relationships and the four wind speed products. Wind speeds >14 m s-1, which only account for 7 % of all observations, contributes disproportionately to the global oceanic FCO<span class="hlt">2</span> and, for this range of wind speeds, the uncertainty induced by the choice of formulation for k is maximum ( 50 %).</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> fluxes makes their accurate estimation an arduous task. This is more pronounced in the Baltic <span class="hlt">Sea</span>, where the mechanisms driving the fluxes 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> flux, 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/2013EGUGA..15.5758P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.5758P"><span>The Impact of a Lower <span class="hlt">Sea</span> Ice Extent on Arctic Greenhouse Gas <span class="hlt">Exchange</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Parmentier, Frans-Jan W.; Christensen, Torben R.; Lotte Sørensen, Lise; Rysgaard, Søren; McGuire, A. David; Miller, Paul A.; Walker, Donald A.</p> <p>2013-04-01</p> <p> years has the potential to influence greenhouse gas <span class="hlt">exchange</span> across terrestrial ecosystems and the Arctic Ocean, but the overall impact remains unclear. In this study, we therefore try to reduce this uncertainty by addressing the influence of the decline in <span class="hlt">sea</span> ice extent on all affected greenhouse gas fluxes in the high latitudes. Also, we will address the need for more research, on the ocean and on the land, to understand the impact of a lower <span class="hlt">sea</span> ice extent on Arctic greenhouse gas <span class="hlt">exchange</span>. References: Bates, N. R., Moran, S. B., Hansell, D. A. and Mathis, J. T.: An increasing <span class="hlt">CO</span><span class="hlt">2</span> sink in the Arctic Ocean due to <span class="hlt">sea</span>-ice loss, Geophys. Res. Lett., 33, L23609, doi:10.1029/2006GL027028, 2006. Cai, W.-J., Chen, L., Chen, B., Gao, Z., Lee, S. H., Chen, J., Pierrot, D., Sullivan, K., Wang, Y., Hu, X., Huang, W.-J., et al.: Decrease in the <span class="hlt">CO</span><span class="hlt">2</span> Uptake Capacity in an Ice-Free Arctic Ocean Basin, Science, 329(5991), 556-559, doi:10.1126/science.1189338, 2010. Kort, E. A., Wofsy, S. C., Daube, B. C., Diao, M., Elkins, J. W., Gao, R. S., Hintsa, E. J., Hurst, D. F., Jimenez, R., Moore, F. L., Spackman, J. R., et al.: Atmospheric observations of Arctic Ocean methane emissions up to 82 degrees north, Nature Geosci., 5(5), 318-321, doi:10.1038/NGEO1452, 2012. Nomura, D., Yoshikawa-Inoue, H. and Toyota, T.: The effect of <span class="hlt">sea</span>-ice growth on <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> flux in a tank experiment, vol. 58, pp. 418-426. 2006. Post, E., Forchhammer, M. C., Bret-Harte, M. S., Callaghan, T. V., Christensen, T. R., Elberling, B., Fox, A. D., Gilg, O., Hik, D. S., Høye, T. T., Ims, R. A., et al.: Ecological Dynamics Across the Arctic Associated with Recent Climate Change, Science, 325(5946), 1355-1358, doi:10.1126/science.1173113, 2009. Rysgaard, S., Glud, R. N., Sejr, M. K., Bendtsen, J. and Christensen, P. B.: Inorganic carbon transport during <span class="hlt">sea</span> ice growth and decay: A carbon pump in polar <span class="hlt">seas</span>, J. Geophys. Res., 112, C03016, doi:10.1029/2006JC003572, 2007. Schuur, E. A. G., Abbott, B. and Network, P. C</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeCoA.217..112B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeCoA.217..112B"><span>Constraining the subsoil carbon source to cave-<span class="hlt">air</span> <span class="hlt">CO</span><span class="hlt">2</span> and speleothem calcite in central Texas</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bergel, Shelly J.; Carlson, Peter E.; Larson, Toti E.; Wood, Chris T.; Johnson, Kathleen R.; Banner, Jay L.; Breecker, Daniel O.</p> <p>2017-11-01</p> <p>Canonical models for speleothem formation and the subsurface carbon cycle invoke soil respiration as the dominant carbon source. However, evidence from some karst regions suggests that belowground <span class="hlt">CO</span><span class="hlt">2</span> originates from a deeper, older source. We therefore investigated the carbon sources to central Texas caves. Drip-water chemistry of two caves in central Texas implies equilibration with calcite at <span class="hlt">CO</span><span class="hlt">2</span> concentrations (PCO<span class="hlt">2</span>_sat) higher than the maximum <span class="hlt">CO</span><span class="hlt">2</span> concentrations observed in overlying soils. This observation suggests that <span class="hlt">CO</span><span class="hlt">2</span> is added to waters after they percolate through the soils, which requires a subsoil carbon source. We directly evaluate the carbon isotope composition of the subsoil carbon source using δ13C measurements on cave-<span class="hlt">air</span> <span class="hlt">CO</span><span class="hlt">2</span>, which we independently demonstrate has little to no contribution from host rock carbon. We do so using the oxidative ratio, OR, defined as the number of moles of O<span class="hlt">2</span> consumed per mole of <span class="hlt">CO</span><span class="hlt">2</span> produced during respiration. However, additional belowground processes that affect O<span class="hlt">2</span> and <span class="hlt">CO</span><span class="hlt">2</span> concentrations, such as gas-water <span class="hlt">exchange</span> and/or diffusion, may also influence the measured oxidative ratio, yielding an apparent OR (ORapparent). Cave <span class="hlt">air</span> in Natural Bridge South Cavern has ORapparent values (1.09 ± 0.06) indistinguishable from those expected for respiration alone (1.08 ± 0.06). Pore space gases from soils above the cave have lower values (ORapparent = 0.67 ± 0.05) consistent with respiration and gas transport by diffusion. The simplest explanation for these observations is that cave <span class="hlt">air</span> in NB South is influenced by respiration in open-system bedrock fractures such that neither diffusion nor <span class="hlt">exchange</span> with water influence the composition of the cave <span class="hlt">air</span>. The radiocarbon activities of NB South cave-<span class="hlt">air</span> <span class="hlt">CO</span><span class="hlt">2</span> suggest the subsoil carbon source is hundreds of years old. The calculated δ13C values of the subsoil carbon source are consistent with tree-sourced carbon (perhaps decomposing root matter), the δ13C values of which</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 <span class="hlt">Exchange</span> 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 fluxes. Accurate representation of these fluxes 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 <span class="hlt">exchange</span> 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 fluxes 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/2009AGUFM.B51A0295S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.B51A0295S"><span>Seasonal Differences in the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Exchange</span> of a Short-Hydroperiod Florida Everglades Marsh</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schedlbauer, J. L.; Oberbauer, S. F.; Starr, G.; Jimenez, K. L.</p> <p>2009-12-01</p> <p>Although wetlands are among the world’s most productive ecosystems, little is known of long-term <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> in tropical and subtropical wetlands. As human pressure on wetlands increases and climate change proceeds, there is growing need to increase our knowledge of wetland ecosystem function. The Everglades is a highly managed wetlands complex occupying >6000 km<span class="hlt">2</span> in south Florida. This ecosystem is oligotrophic, but extremely high rates of productivity have been previously reported. To evaluate annual and seasonal (dry vs. wet season) ecosystem production, <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> was determined by eddy covariance in a short-hydroperiod marl marsh. Rates of net ecosystem <span class="hlt">exchange</span> and ecosystem respiration were small year-round and declined in the wet season relative to the dry season. Inundation submerged approximately half of the marsh’s leaf area, substantially limiting gross ecosystem production. While light and <span class="hlt">air</span> temperature exerted the primary controls on net ecosystem <span class="hlt">exchange</span> and ecosystem respiration in the dry season, inundation weakened these relationships. The ecosystem shifted from a <span class="hlt">CO</span><span class="hlt">2</span> sink in the dry season to a <span class="hlt">CO</span><span class="hlt">2</span> source in the wet season; however, the marsh was a small carbon sink on an annual basis. Net ecosystem production, ecosystem respiration, and gross ecosystem production were -27.9, 394.3, and 422.<span class="hlt">2</span> g C m-<span class="hlt">2</span> year-1, respectively. Unexpectedly low <span class="hlt">CO</span><span class="hlt">2</span> flux rates and annual production distinguish the Everglades from many other wetlands. Nonetheless, impending changes in water management and climate are likely to alter the <span class="hlt">CO</span><span class="hlt">2</span> balance of this wetland and may increase the source strength of these extensive short-hydroperiod marshes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.B21F0488S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.B21F0488S"><span>Temporally-resolved Study of Atmosphere-lake Net <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Exchange</span> at Lochaber Lake, Nova Scotia, Canada</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Spafford, L. A.; Risk, D. A.</p> <p>2016-12-01</p> <p>Lakes are carbon gateways with immense processing capacity, acting as either sinks or sources for <span class="hlt">CO</span><span class="hlt">2</span>. As climate change exacerbates weather extremes, carbon stored within permafrost and soils is liberated to water systems, altering aquatic carbon budgets and light availability for photosynthesis. The functional response of lakes to climate change is uncertain, and continuous data of lake respiration and its drivers are lacking. This study used high-frequency measurements of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> during a growing season by a novel technique to quantify the net flux of carbon at a small deep oligotrophic lake in eastern Nova Scotia, Canada, and to examine the influence of environmental forcings. We installed 3 floating Forced Diffusion dynamic membrane chambers on the lake, coupled to a valving multiplexer and a single Vaisala GMP 343 <span class="hlt">CO</span><span class="hlt">2</span> analyzer. This low-power system sampled lake-atmosphere <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> at several points from shore every hour for over 100 days in the growing season. At the same frequency we also collected automated measurements of wind velocity, photosynthetically active radiation (PAR), dissolved <span class="hlt">CO</span><span class="hlt">2</span>, <span class="hlt">air</span> and water temperature. Manual measurement campaigns measured chlorophyll `a', DOC, surface methane (CH4), and <span class="hlt">CO</span><span class="hlt">2</span> flux by manual static floating chamber to confirm the automated measurements. The lake was a net source for carbon, on average emitting 0.038 µmol <span class="hlt">CO</span><span class="hlt">2</span>/m<span class="hlt">2</span>/s or 4.967 g <span class="hlt">CO</span><span class="hlt">2</span>/s over the entire lake, but we did observe significant temporal variation across diel cycles, and along with changing weather. Approximately 48 hours after every rain event, we observed an increase in littoral <span class="hlt">CO</span><span class="hlt">2</span> release by the lake. Wind speed, <span class="hlt">air</span> temperature, and distance from shore were also drivers of variation, as the littoral zone tended to release less <span class="hlt">CO</span><span class="hlt">2</span> during the course of our study. This work shows the variable influence of environmental drivers of lake carbon flux, as well as the utility of low-power automated chambers for observing aquatic net <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</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_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('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> flux</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> <span class="hlt">exchange</span>. 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> flux was calculated. Results show that <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> 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> flux 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('http://adsabs.harvard.edu/abs/2013BGeo...10.5793S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013BGeo...10.5793S"><span>Biology and <span class="hlt">air-sea</span> gas <span class="hlt">exchange</span> controls on the distribution of carbon isotope ratios (δ13C) in the ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schmittner, A.; Gruber, N.; Mix, A. C.; Key, R. M.; Tagliabue, A.; Westberry, T. K.</p> <p>2013-09-01</p> <p>Analysis of observations and sensitivity experiments with a new three-dimensional global model of stable carbon isotope cycling elucidate processes that control the distribution of δ13C of dissolved inorganic carbon (DIC) in the contemporary and preindustrial ocean. Biological fractionation and the sinking of isotopically light δ13C organic matter from the surface into the interior ocean leads to low δ13CDIC values at depths and in high latitude surface waters and high values in the upper ocean at low latitudes with maxima in the subtropics. <span class="hlt">Air-sea</span> gas <span class="hlt">exchange</span> has two effects. First, it acts to reduce the spatial gradients created by biology. Second, the associated temperature-dependent fractionation tends to increase (decrease) δ13CDIC values of colder (warmer) water, which generates gradients that oppose those arising from biology. Our model results suggest that both effects are similarly important in influencing surface and interior δ13CDIC distributions. However, since <span class="hlt">air-sea</span> gas <span class="hlt">exchange</span> is slow in the modern ocean, the biological effect dominates spatial δ13CDIC gradients both in the interior and at the surface, in contrast to conclusions from some previous studies. Calcium carbonate cycling, pH dependency of fractionation during <span class="hlt">air-sea</span> gas <span class="hlt">exchange</span>, and kinetic fractionation have minor effects on δ13CDIC. Accumulation of isotopically light carbon from anthropogenic fossil fuel burning has decreased the spatial variability of surface and deep δ13CDIC since the industrial revolution in our model simulations. Analysis of a new synthesis of δ13CDIC measurements from years 1990 to 2005 is used to quantify preformed and remineralized contributions as well as the effects of biology and <span class="hlt">air-sea</span> gas <span class="hlt">exchange</span>. The model reproduces major features of the observed large-scale distribution of δ13CDIC as well as the individual contributions and effects. Residual misfits are documented and analyzed. Simulated surface and subsurface δ13CDIC are influenced by</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.H53A1376G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.H53A1376G"><span>The Effect of Thermal Convection on Earth-Atmosphere <span class="hlt">CO</span><span class="hlt">2</span> Gas <span class="hlt">Exchange</span> in Aggregated Soil</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ganot, Y.; Weisbrod, N.; Dragila, M. I.</p> <p>2011-12-01</p> <p>Gas transport in soils and surface-atmosphere gas <span class="hlt">exchange</span> are important processes that affect different aspects of soil science such as soil aeration, nutrient bio-availability, sorption kinetics, soil and groundwater pollution and soil remediation. Diffusion and convection are the two main mechanisms that affect gas transport, fate and emissions in the soils and in the upper vadose zone. In this work we studied <span class="hlt">CO</span><span class="hlt">2</span> soil-atmosphere gas <span class="hlt">exchange</span> under both day-time and night-time conditions, focusing on the impact of thermal convection (TCV) during the night. Experiments were performed in a climate-controlled laboratory. One meter long columns were packed with matrix of different grain size (sand, gravel and soil aggregates). <span class="hlt">Air</span> with 2000 ppm <span class="hlt">CO</span><span class="hlt">2</span> was injected into the bottom of the columns and <span class="hlt">CO</span><span class="hlt">2</span> concentration within the columns was continuously monitored by an Infra Red Gas Analyzer. Two scenarios were compared for each soil: (1) isothermal conditions, representing day time conditions; and (<span class="hlt">2</span>) thermal gradient conditions, i.e., atmosphere colder than the soil, representing night time conditions. Our results show that under isothermal conditions, diffusion is the major mechanism for surface-atmosphere gas <span class="hlt">exchange</span> for all grain sizes; while under night time conditions the prevailing mechanism is dependent on the <span class="hlt">air</span> permeability of the matrix: for sand and gravel it is diffusion, and for soil aggregates it is TCV. Calculated <span class="hlt">CO</span><span class="hlt">2</span> flux for the soil aggregates column shows that the TCV flux was three orders of magnitude higher than the diffusive flux.</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> <span class="hlt">exchange</span> 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> flux 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/2016AGUOSPO51D..01B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSPO51D..01B"><span>Intercomparison of <span class="hlt">Air-Sea</span> Fluxes 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 <span class="hlt">exchange</span> 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 flux products to <span class="hlt">air-sea</span> flux values calculated from shipboard observations from four cruises and an <span class="hlt">air-sea</span> flux 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> flux 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/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> fluxes, complicates the accurate estimation of these mechanisms. This is particularly pronounced in the Baltic <span class="hlt">Sea</span>, where the mechanisms driving the fluxes 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> flux, 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('http://adsabs.harvard.edu/abs/2018AIPC.1942m0055M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AIPC.1942m0055M"><span><span class="hlt">Exchange</span> bias effect in <span class="hlt">Co</span>Al<span class="hlt">2</span>O4</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mohanty, Prachi; Marik, Sourav; Singh, Ravi P.</p> <p>2018-04-01</p> <p>Herein, we report the appearance of a significant <span class="hlt">exchange</span> bias (EB) effect for the highly frustrated spinel material <span class="hlt">Co</span>Al<span class="hlt">2</span>O4. It shows a large value of frustration parameter as observed from the dc susceptibility measurements. <span class="hlt">Co</span>Al<span class="hlt">2</span>O4 exhibits the <span class="hlt">exchange</span> bias effect below 8 K when it is cooled in the presence of a magnetic field. Detailed magnetization measurements indicate that the <span class="hlt">exchange</span> bias properties of this compound are associated with the frustration present in this material.</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 fluxes, 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 flux 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 <span class="hlt">exchange</span> in the coastal zone. Direct estimates of the flux 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 flux 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 <span class="hlt">exchange</span> 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://hdl.handle.net/2060/20110022999','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110022999"><span>Improvement of the GEOS-5 AGCM upon Updating the <span class="hlt">Air-Sea</span> Roughness Parameterization</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Garfinkel, C. I.; Molod, A.; Oman, L. D.; Song, I.-S.</p> <p>2011-01-01</p> <p>The impact of an <span class="hlt">air-sea</span> roughness parameterization over the ocean that more closely matches recent observations of <span class="hlt">air-sea</span> <span class="hlt">exchange</span> is examined in the NASA Goddard Earth Observing System, version 5 (GEOS-5) atmospheric general circulation model. Surface wind biases in the GEOS-5 AGCM are decreased by up to 1.<span class="hlt">2</span>m/s. The new parameterization also has implications aloft as improvements extend into the stratosphere. Many other GCMs (both for operational weather forecasting and climate) use a similar class of parameterization for their <span class="hlt">air-sea</span> roughness scheme. We therefore expect that results from GEOS-5 are relevant to other models as well.</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 <span class="hlt">exchanges</span> 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 <span class="hlt">exchange</span> fluxes 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 <span class="hlt">exchange</span> is an important process that intervenes in the transport and fate for neutral PFASs in the marine environment.</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/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> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFMOS42B..07P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFMOS42B..07P"><span>Carbon Dioxide Impacts in the Deep-<span class="hlt">Sea</span>: Is Maintaining a Metabolically Required <span class="hlt">CO</span><span class="hlt">2</span> Efflux Rate Challenging?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Peltzer, E. T.; Hofmann, A. F.; Brewer, P. G.</p> <p>2011-12-01</p> <p>Increasing ocean acidification from fossil fuel <span class="hlt">CO</span><span class="hlt">2</span> invasion, from temperature driven changes in respiration, and from possible leakage from sub-seabed geologic <span class="hlt">CO</span><span class="hlt">2</span> disposal has aroused concern over the impacts of elevated <span class="hlt">CO</span><span class="hlt">2</span> concentrations on marine life. Here we describe the rate problem for animals who must export <span class="hlt">CO</span><span class="hlt">2</span> at about the same rate at which O<span class="hlt">2</span> is consumed. We analyze the basic properties controlling <span class="hlt">CO</span><span class="hlt">2</span> export within the diffusive boundary of marine animals in a changing ocean in order to compare the challenges posed by O<span class="hlt">2</span> uptake under stress with the equivalent problem of <span class="hlt">CO</span><span class="hlt">2</span> expulsion. The problem is more complex than that for a non-reactive gas since, as with gas <span class="hlt">exchange</span> of <span class="hlt">CO</span><span class="hlt">2</span> at the <span class="hlt">air-sea</span> interface, the influence of the ensemble of reactions within the <span class="hlt">CO</span><span class="hlt">2</span> - HCO3- - <span class="hlt">CO</span>3= acid-base system needs to be considered. These reactions appear as an enhancement factor which significantly facilitates <span class="hlt">CO</span><span class="hlt">2</span> efflux compared to O<span class="hlt">2</span> intake at equal temperature, pressure and flow rate under typical oceanic concentrations. Possibly as an adaptation to this chemical advantage marine animals typically can respond to external <span class="hlt">CO</span><span class="hlt">2</span> stress simply by metabolic adjustment. This is energetically more favorable than having to resort to mechanically increasing flow over their surface to thin the boundary layer as is required to alleviate O<span class="hlt">2</span> stress. Regionally as with O<span class="hlt">2</span> the combination of T, P, and pH/p<span class="hlt">CO</span><span class="hlt">2</span> creates a zone of maximum <span class="hlt">CO</span><span class="hlt">2</span> stress at around 1000 m depth. But the net result is that the combination of an increase in T combined with declining O<span class="hlt">2</span> poses a greater respiratory challenge to marine life than does increasing <span class="hlt">CO</span><span class="hlt">2</span>. The relationships developed here allow a more accurate prediction of the impacts on marine life from the combined effects of changing T, O<span class="hlt">2</span>, and <span class="hlt">CO</span><span class="hlt">2</span> than can be estimated from single variable studies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17330461','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17330461"><span>[Simulation of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> between forest canopy and atmosphere].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Diao, Yiwei; Wang, Anzhi; Jin, Changjie; Guan, Dexin; Pei, Tiefan</p> <p>2006-12-01</p> <p>Estimating the scalar source/sink distribution of <span class="hlt">CO</span><span class="hlt">2</span> and its vertical fluxes within and above forest canopy continues to be a critical research problem in biosphere-atmosphere <span class="hlt">exchange</span> processes and plant ecology. With broad-leaved Korean pine forest in Changbai Mountains as test object, and based on Raupach's localized near field theory, the source/sink and vertical flux distribution of <span class="hlt">CO</span><span class="hlt">2</span> within and above forest canopy were modeled through an inverse Lagrangian dispersion analysis. This model correctly predicted a strong positive <span class="hlt">CO</span><span class="hlt">2</span> source strength in the deeper layers of the canopy due to soil-plant respiration, and a strong <span class="hlt">CO</span><span class="hlt">2</span> sink in the upper layers of the canopy due to the assimilation by sunlit foliage. The foliage in the top layer of canopy changed from a <span class="hlt">CO</span><span class="hlt">2</span> source in the morning to a <span class="hlt">CO</span><span class="hlt">2</span> sink in the afternoon, while the soil constituted a strong <span class="hlt">CO</span><span class="hlt">2</span> source all the day. The simulation results accorded well with the eddy covariance <span class="hlt">CO</span><span class="hlt">2</span> flux measurements within and above the canopy, and the average precision was 89%. The <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> predicted by the analysis was averagely 15% higher than that of the eddy correlation, but exhibited identical temporal trend. Atmospheric stability remarkably affected the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> between forest canopy and atmosphere.</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('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> flux 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> flux 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 <span class="hlt">exchange</span> 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> flux 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> fluxes 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://ntrs.nasa.gov/search.jsp?R=20060040203&hterms=Carr+2000&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DCarr%2B2000','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060040203&hterms=Carr+2000&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DCarr%2B2000"><span><span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> coefficients from remotely-sensed wind speed measurements: SSM/I versus QuikSCAT in 2000</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Carr, M.; Tang, W.; Liu, W. T.</p> <p>2002-01-01</p> <p>We compare here the <span class="hlt">air-sea</span> <span class="hlt">exchange</span> coefficient for C02 estimated with monthly mean wind speed measured by the Special Sensing Microwave Imager (SSM/I), Ks , and by the scatterometer QuikSCAT, Kq, for the year 2000.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.3451H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.3451H"><span>Influence of soil erosion on <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> within the CarboZALF manipulation experiment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hoffmann, Mathias; Augustin, Jürgen; Sommer, Michael</p> <p>2014-05-01</p> <p>Agriculture in the hummocky ground moraine landscape of NE-Germany is characterized by an increase in energy crop cultivation, like maize or sorghum. Both enhance lateral C fluxes by erosion and induce feedbacks on C dynamics of agroecosystems as a result of the time limited land cover and the vigorous crop growth. However, the actual impact of these phenomena on the <span class="hlt">CO</span><span class="hlt">2</span>-sink/-source function of agricultural landscapes, is still not clear. Therefore we established the interdisciplinary project 'CarboZALF' in 2009. In our field experiment CarboZALF-D we are monitoring <span class="hlt">CO</span><span class="hlt">2</span> fluxes for soil-plant systems, which cover all landscape relevant soil states in respect to erosion and deposition, like Albic Cutanic Luvisol, Calcic Cutanic Luvisol, Calcaric Regosol and Endogleyic Colluvic Regosol. Furthermore, we induced erosion / deposition in a manipulation experiment. Automated chamber systems (<span class="hlt">2</span>.5 m, basal area 1 m<span class="hlt">2</span>, transparent) are placed at the manipulated sites as well as at one site neither influenced by erosion, nor by deposition. <span class="hlt">CO</span><span class="hlt">2</span> flux modelling of high temporal resolution includes ecosystem respiration (Reco), gross primary productivity (GPP) and net ecosystem <span class="hlt">exchange</span> (NEE) based on parallel and continuous measurements of the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span>, soil and <span class="hlt">air</span> temperatures as well as photosynthetic active radiation (PAR). Modelling includes gap filling which is needed in case of chamber malfunctions and abrupt disturbances by farming practice. In our presentation we would like to show results of the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> measurements for one year. Differences are most pronounced between the non-eroded and the colluvial soil: The Endogleyic Colluvic Regosol showed higher flux rates for Reco and NEE compared to the Albic Cutanic Luvisol. The eroded soil (Calcic Cutanic Luvisol) demonstrated <span class="hlt">CO</span><span class="hlt">2</span>fluxes intermediate between the non-affected and depositional site. Site-specific consequences for the soil C stocks will be also discussed in the presentation.</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> fluxes</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> flux 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> fluxes 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> fluxes</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> flux 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> fluxes 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> </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://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> <span class="hlt">exchange</span> 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 fluxes (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/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> flux.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP52A..01H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP52A..01H"><span>Westerly Winds and the Southern Ocean <span class="hlt">CO</span><span class="hlt">2</span> Sink Since the Last Glacial-Interglacial Transition</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hodgson, D. A.; Saunders, K. M.; Roberts, S. J.; Perren, B.; Butz, C.; Sime, L. C.; Davies, S. J.; Grosjean, M.</p> <p>2017-12-01</p> <p>The capacity of the Southern Ocean carbon sink is partly controlled by the Southern Hemisphere westerly winds (SHW) and <span class="hlt">sea</span> ice. These regulate the upwelling of dissolved carbon-rich deep water to Antarctic surface waters, determine the surface area for <span class="hlt">air-sea</span> gas <span class="hlt">exchange</span> and therefore modulate the net uptake of atmospheric <span class="hlt">CO</span><span class="hlt">2</span>. Some models have proposed that strengthened SHW will result in a weakening of the Southern Ocean <span class="hlt">CO</span><span class="hlt">2</span> sink. If these models are correct, then one would expect that reconstructions of changes in SHW intensity on centennial to millennial timescales would show clear links with Antarctic ice core and Southern Ocean marine geological records of atmospheric <span class="hlt">CO</span><span class="hlt">2</span>, temperature and <span class="hlt">sea</span> ice. Here, we present a 12,300 year reconstruction of past wind strength based on three independent proxies that track the changing inputs of <span class="hlt">sea</span> salt aerosols and minerogenic particles into lake sediments on sub-Antarctic Macquarie Island. The proxies are consistent in showing that periods of high wind intensity corresponded with the increase in <span class="hlt">CO</span><span class="hlt">2</span> across the late Last Glacial-Interglacial Transition and in the last 7,000 years, suggesting that the winds have contributed to the long term outgassing of <span class="hlt">CO</span><span class="hlt">2</span> from the ocean during these periods.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1053848','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1053848"><span>Materials, Turbomachinery and Heat <span class="hlt">Exchangers</span> for Supercritical <span class="hlt">CO</span><span class="hlt">2</span> Systems</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>Anderson, Mark; Nellis, Greg; Corradini, Michael</p> <p>2012-10-19</p> <p>The objective of this project is to produce the necessary data to evaluate the performance of the supercritical carbon dioxide cycle. The activities include a study of materials compatibility of various alloys at high temperatures, the heat transfer and pressure drop in compact heat <span class="hlt">exchanger</span> units, and turbomachinery issues, primarily leakage rates through dynamic seals. This experimental work will serve as a test bed for model development and design calculations, and will help define further tests necessary to develop high-efficiency power conversion cycles for use on a variety of reactor designs, including the sodium fast reactor (SFR) and very high-temperaturemore » gas reactor (VHTR). The research will be broken into three separate tasks. The first task deals with the analysis of materials related to the high-temperature S-<span class="hlt">CO</span>{sub <span class="hlt">2</span>} Brayton cycle. The most taxing materials issues with regard to the cycle are associated with the high temperatures in the reactor side heat <span class="hlt">exchanger</span> and in the high-temperature turbine. The system could experience pressures as high as 20MPa and temperatures as high as 650°C. The second task deals with optimization of the heat <span class="hlt">exchangers</span> required by the S-<span class="hlt">CO</span>{sub <span class="hlt">2</span>} cycle; the S-<span class="hlt">CO</span>{sub <span class="hlt">2</span>} flow passages in these heat <span class="hlt">exchangers</span> are required whether the cycle is coupled with a VHTR or an SFR. At least three heat <span class="hlt">exchangers</span> will be required: the pre-cooler before compression, the recuperator, and the heat <span class="hlt">exchanger</span> that interfaces with the reactor coolant. Each of these heat <span class="hlt">exchangers</span> is unique and must be optimized separately. The most challenging heat <span class="hlt">exchanger</span> is likely the pre-cooler, as there is only about a 40°C temperature change but it operates close to the <span class="hlt">CO</span>{sub <span class="hlt">2</span>} critical point, therefore inducing substantial changes in properties. The proposed research will focus on this most challenging component. The third task examines seal leakage through various dynamic seal designs under the conditions expected in the S-<span class="hlt">CO</span>{sub <span class="hlt">2</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.4408H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.4408H"><span>Clustering XCO<span class="hlt">2</span> temporal change to assess <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchanging</span> strength of biosphere-atmosphere with GOSAT observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>He, Zhonghua; Lei, Liping; Bie, Nian; Yang, Shaoyuan; Wu, Changjiang; Zeng, Zhao-Cheng</p> <p>2017-04-01</p> <p>The temporal change of atmospheric carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) concentration, greatly related to the local activities of <span class="hlt">CO</span><span class="hlt">2</span> uptake and emission, including biospheric <span class="hlt">exchange</span> and anthropogenic emission, is one of important information for regions identification of carbon source and sink. Satellite observations of <span class="hlt">CO</span><span class="hlt">2</span> has been used for detecting the change of <span class="hlt">CO</span><span class="hlt">2</span> concentration for a long time. In this study, we used the grid data of 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>) with the spatial resolution of 1 degree and the temporal resolution of 3 days from 1 June 2009 to 31 May 2014 over the land area of 30° - 60° N to implement a clustering of temporal changing characteristics for the Greenhouse Gases Observing Satellite (GOSAT) XCO<span class="hlt">2</span> retrievals. Grid data is derived using the gap filling method of spatio-temporal geostatistics. The clustering method is one adjusted K-mean for the gap existed time-series data. As a result, types and number of clusters are specified based on the temporal characteristic of XCO<span class="hlt">2</span> by using the optimal clustering parameters. The biospheric absorption and surface emission of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> is discussed through the analysis of the different yearly increase and seasonal amplitude of XCO<span class="hlt">2</span> each cluster combined with correlation analysis with vegetation index from the Moderate-resolution Imaging Spectroradiometer (MODIS) and fossil fuel <span class="hlt">CO</span><span class="hlt">2</span> emission data from Open-source Data Inventory for Anthropogenic <span class="hlt">CO</span><span class="hlt">2</span> (Odiac). Regions of strong or weak biosphere-atmosphere <span class="hlt">exchange</span>, or significant disturbance from anthropogenic activities can be identified. In conclusion, gap filled XCO<span class="hlt">2</span> from satellite observations can help us to take an analysis of atmospheric <span class="hlt">CO</span><span class="hlt">2</span>, results of the coupled biosphere-atmosphere, by their spatio-temporal characteristics as well as the relationship with the other remote sensing parameters e.g. MODIS related with biospheric photosynthetic or respiration activities.</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 flux 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> <span class="hlt">exchange</span> 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('http://adsabs.harvard.edu/abs/2012BGD.....915787H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012BGD.....915787H"><span>Kinetic bottlenecks to chemical <span class="hlt">exchange</span> rates for deep-<span class="hlt">sea</span> animals II: Carbon dioxide</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hofmann, A. F.; Peltzer, E. T.; Brewer, P. G.</p> <p>2012-11-01</p> <p>Increased ocean acidification from fossil fuel <span class="hlt">CO</span><span class="hlt">2</span> invasion, from temperature-driven changes in respiration, and from possible leakage from sub-seabed geologic <span class="hlt">CO</span><span class="hlt">2</span> disposal has aroused concern over the impacts of elevated <span class="hlt">CO</span><span class="hlt">2</span> concentrations on marine life. Discussion of these impacts has so far focused only on changes in the oceanic bulk fluid properties (ΔpH, Δ[∑<span class="hlt">CO</span><span class="hlt">2</span>] etc.) as the critical variable and with a major focus on carbonate shell dissolution. Here we describe the rate problem for animals that must export <span class="hlt">CO</span><span class="hlt">2</span> at about the same rate at which O<span class="hlt">2</span> is consumed. We analyze the basic properties controlling <span class="hlt">CO</span><span class="hlt">2</span> export within the diffusive boundary layer around marine animals in an ocean changing in temperature (T) and <span class="hlt">CO</span><span class="hlt">2</span> concentration in order to compare the challenges posed by O<span class="hlt">2</span> uptake under stress with the equivalent problem of <span class="hlt">CO</span><span class="hlt">2</span> expulsion. The problem is more complex than that for a non-reactive gas since, as with gas <span class="hlt">exchange</span> of <span class="hlt">CO</span><span class="hlt">2</span> at the <span class="hlt">air-sea</span> interface, the influence of the ensemble of reactions within the <span class="hlt">CO</span><span class="hlt">2</span>-HCO3--<span class="hlt">CO</span>32- acid-base system needs to be considered. These reactions significantly facilitate <span class="hlt">CO</span><span class="hlt">2</span> efflux compared to O<span class="hlt">2</span> intake at equal temperature, pressure and flow rate under typical oceanic concentrations.The effect of these reactions can be described by an enhancement factor. For organisms, this means mechanically increasing flow over their surface to thin the boundary layer as is required to alleviate O<span class="hlt">2</span> stress seems not necessary to facilitate <span class="hlt">CO</span><span class="hlt">2</span> efflux. Nevertheless the elevated p<span class="hlt">CO</span><span class="hlt">2</span> cost most likely is non-zero. Regionally as with O<span class="hlt">2</span> the combination of T, P, and pH/p<span class="hlt">CO</span><span class="hlt">2</span> creates a zone of maximum <span class="hlt">CO</span><span class="hlt">2</span> stress at around 1000 m depth. But the net result is that, for the problem of gas <span class="hlt">exchange</span> with the bulk ocean, the combination of an increasing T combined with declining O<span class="hlt">2</span> poses a greater challenge to marine life than does increasing <span class="hlt">CO</span><span class="hlt">2</span>. The relationships developed here allow a more accurate prediction of the impacts on marine life</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1225427-implications-room-temperature-oxidation-crystal-structure-exchange-bias-effect-co-coo-nanoparticles','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1225427-implications-room-temperature-oxidation-crystal-structure-exchange-bias-effect-co-coo-nanoparticles"><span>Implications of room temperature oxidation on crystal structure and <span class="hlt">exchange</span> bias effect in <span class="hlt">Co/Co</span>O nanoparticles</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Feygenson, Mikhail; Formo, Eric V.; Freeman, Katherine; ...</p> <p>2015-11-02</p> <p>In this study, we describe how the <span class="hlt">exchange</span> bias effect in <span class="hlt">Co/Co</span>O nanoparticles depends on the size focusing and temperature treatment of precursor <span class="hlt">Co</span> nanoparticles before oxidation at ambient conditions. By appealing to magnetization, microscopy, neutron and synchrotron x-ray measurements we found that as-synthesized <span class="hlt">Co</span> nanoparticles readily oxidize in <span class="hlt">air</span> only after 20 days. The highest <span class="hlt">exchange</span> bias field of 814 Oe is observed at T = <span class="hlt">2</span>K. When the same nanoparticles are centrifuged and annealed at 70 °C in vacuum prior to oxidation, the <span class="hlt">exchange</span> bias field is increased to 2570 Oe. Annealing of <span class="hlt">Co</span> nanoparticles in vacuum improvesmore » their crystallinity and prevents complete oxidation, so that <span class="hlt">Co-core/Co</span>O-shell structure is preserved even after 120 days. The crystal structure of <span class="hlt">Co</span>O shell in both samples is different from its bulk counterpart. Implications of such distorted <span class="hlt">Co</span>O shells on <span class="hlt">exchange</span> bias are discussed. Coating of <span class="hlt">Co</span> nanoparticles with amorphous silica shell makes them resistant to oxidation, but ultimately modifies the crystal structure of both <span class="hlt">Co</span> core and SiO <span class="hlt">2</span> shell.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOS.A34C2670V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOS.A34C2670V"><span>Setting an Upper Limit on Gas <span class="hlt">Exchange</span> Through <span class="hlt">Sea</span>-Spray</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vlahos, P.; Monahan, E. C.; Andreas, E. L.</p> <p>2016-02-01</p> <p><span class="hlt">Air-sea</span> gas <span class="hlt">exchange</span> parameterization is critical to understanding both climate forcing and feedbacks and is key in biogeochemistry cycles. Models based on wind speed have provided empirical estimates of gas <span class="hlt">exchange</span> that are useful though it is likely that at high wind speeds of over 10 m/s there are important gas <span class="hlt">exchange</span> parameters including bubbles and <span class="hlt">sea</span> spray that have not been well constrained. Here we address the <span class="hlt">sea</span>-spray component of gas <span class="hlt">exchange</span> at these high wind speeds to set sn upper boundary condition for the gas <span class="hlt">exchange</span> of the six model gases including; nobel gases helium, neon and argon, diatomic gases nitrogen and oxygen and finally, the more complex gas carbon dioxide. Estimates are based on the spray generation function of Andreas and Monahan and the gases are tested under three scenarios including 100 percent saturation and complete droplet evaporation, 100 percent saturation and a more realistic scenario in which a fraction of droplets evaporate completely, a fraction evaporate to some degree and a fraction returns to the water side without significant evaporation. Finally the latter scenario is applied to representative under saturated concentrations of the gases.</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> Fluxes 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 fluxes determine the <span class="hlt">exchange</span> of momentum, heat, freshwater, and gas between the atmosphere and ocean. These <span class="hlt">exchange</span> 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 fluxes 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 fluxes 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 fluxes are called surface turbulent fluxes because the mixing and transport are due to turbulence. Examples of nonturbulent processes are radiative fluxes (e.g., solar radiation) and precipitation (Schmitt et al., 2010). Turbulent fluxes are strongly dependent on wind speed; therefore, observations of wind speed are critical for the calculation of all turbulent surface fluxes. 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 fluxes. For long-term processes, transport can be very important but again is usually small compared to surface fluxes.</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 <span class="hlt">exchange</span> 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 flux. 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> flux 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 flux 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> fluxes. 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/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> flux 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> flux 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> fluxes 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> flux 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> flux 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> fluxes. 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> flux is strongly influenced by the local wind speed.</p> </li> <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/2014AGUFM.B44A..04G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.B44A..04G"><span>Enhanced Seasonal <span class="hlt">Exchange</span> of <span class="hlt">CO</span><span class="hlt">2</span> by Northern Ecosystems - Observations and Models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Graven, H. D.; Keeling, R. F.; Piper, S. C.; Patra, P. K.; Stephens, B. B.; Wofsy, S. C.; Welp, L. R.; Sweeney, C.; Tans, P. P.; Kelley, J. J.; Daube, B. C.; Kort, E. A.; Santoni, G.; Bent, J. D.; Thomas, R.; Prentice, I. C.</p> <p>2014-12-01</p> <p>Long-term measurements of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> have revealed increasing amplitude in seasonal variations at Northern Hemisphere sites. In a recent paper1, we extended the analysis of seasonal <span class="hlt">CO</span><span class="hlt">2</span> amplitude using aircraft data from 1958-61 and 2009-11 and found large increases of 50% in the mid-troposphere north of 45°N. Changes in amplitude south of 45°N were less than 25%. The observations indicate that seasonal <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchanges</span> with northern terrestrial ecosystems must have increased by 30-60% over the past 50 years. The increased <span class="hlt">exchange</span> is likely widespread over northern ecosystems but it must be focused in boreal forests to match the observed spatial pattern in the aircraft data. Small decreases in seasonal <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> of subtropical and tropical regions may also contribute to <span class="hlt">CO</span><span class="hlt">2</span> amplitude changes. The required increases in seasonal <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> in northern ecosystems are larger than simulated by terrestrial models, indicating the models do not capture substantial ecological changes occurring since 1960. This presentation will give an overview of the recent paper1, highlighting the atmospheric evidence for a dominant influence from boreal forests and from the main growing season months. It will also expand on the investigation of modeled changes in seasonal <span class="hlt">CO</span><span class="hlt">2</span> flux using CMIP5 and other model intercomparisons, including the modeled influences of carbon vs climate drivers. 1. Graven et al. 2013, Enhanced Seasonal <span class="hlt">Exchange</span> of <span class="hlt">CO</span><span class="hlt">2</span> by Northern Ecosystems Since 1960, Science, 341, 6150, 1085-1089. DOI: 10.1126/science.1239207</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.2781S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.2781S"><span>Boundary layers at a dynamic interface: <span class="hlt">Air-sea</span> <span class="hlt">exchange</span> 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 J.</p> <p>2017-04-01</p> <p><span class="hlt">Exchange</span> 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 anthropogenic gases involved in the study of climate. The goal in this research area is to determine the gas flux from <span class="hlt">air</span> to <span class="hlt">sea</span> or vice versa. For sparingly soluble nonreactive 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 w' and gas concentration c' are known, then it is possible to determine the turbulent contribution to the gas flux. However, there is no suitable fundamental direct approach in the general case where neither w' nor c' can be easily measured. A new approach is presented to deduce key aspects about the near-surface turbulent motions from measurements that can be taken by an infrared (IR) camera. An equation is derived with inputs being the surface temperature and heat flux, and a solution method developed for the surface-normal strain experienced over time by boundary layers at the interface. Because the thermal and concentration boundary layers experience the same near-surface fluid motions, the solution for the surface-normal strain determines the gas flux or gas transfer velocity. Examples illustrate the approach in the cases of complete surface renewal, partial surface renewal, and insolation. The prospects for use of the approach in flows characterized by sheared interfaces or rapid boundary layer straining are explored.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27187527','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27187527"><span>Biological and physical controls in the Southern Ocean on past millennial-scale atmospheric <span class="hlt">CO</span><span class="hlt">2</span> changes.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gottschalk, Julia; Skinner, Luke C; Lippold, Jörg; Vogel, Hendrik; Frank, Norbert; Jaccard, Samuel L; Waelbroeck, Claire</p> <p>2016-05-17</p> <p>Millennial-scale climate changes during the last glacial period and deglaciation were accompanied by rapid changes in atmospheric <span class="hlt">CO</span><span class="hlt">2</span> that remain unexplained. While the role of the Southern Ocean as a 'control valve' on ocean-atmosphere <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> has been emphasized, the exact nature of this role, in particular the relative contributions of physical (for example, ocean dynamics and <span class="hlt">air-sea</span> gas <span class="hlt">exchange</span>) versus biological processes (for example, export productivity), remains poorly constrained. Here we combine reconstructions of bottom-water [O<span class="hlt">2</span>], export production and (14)C ventilation ages in the sub-Antarctic Atlantic, and show that atmospheric <span class="hlt">CO</span><span class="hlt">2</span> pulses during the last glacial- and deglacial periods were consistently accompanied by decreases in the biological export of carbon and increases in deep-ocean ventilation via southern-sourced water masses. These findings demonstrate how the Southern Ocean's 'organic carbon pump' has exerted a tight control on atmospheric <span class="hlt">CO</span><span class="hlt">2</span>, and thus global climate, specifically via a synergy of both physical and biological processes.</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> flux (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> <span class="hlt">exchange</span> 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/2006JPhy4.139..211E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006JPhy4.139..211E"><span>Occurrence and <span class="hlt">air/sea-exchange</span> of novel organic pollutants in the marine environment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ebinghaus, R.; Xie, Z.</p> <p>2006-12-01</p> <p>A number of studies have demonstrated that several classes of chemicals act as biologically relevant signalling substances. Among these chemicals, many, including PCBs, DDT and dioxins, are semi-volatile, persistent, and are capable of long-range atmospheric transport via atmospheric circulation. Some of these compounds, e.g. phthalates and alkylphenols (APs) are still manufactured and consumed worldwide even though there is clear evidence that they are toxic to aquatic organisms and can act as endocrine disruptors. Concentrations of NP, t-OP and NP1EO, DMP, DEP, DBP, BBP, and DEHP have been simultaneously determined in the surface <span class="hlt">sea</span> water and atmosphere of the North <span class="hlt">Sea</span>. Atmospheric concentrations of NP and t-OP ranged from 7 to 110 pg m - 3, which were one to three orders of magnitude below coastal atmospheric concentrations already reported. NP1EO was detected in both vapor and particle phases, which ranged from 4 to 50 pg m - 3. The concentrations of the phthalates in the atmosphere ranged from below the method detection limit to 3.4 ng m - 3. The concentrations of t-OP, NP, and NP1EO in dissolved phase were 13-300, 90-1400, and 17-1660 pg L - 1. DBP, BBP, and DEHP were determined in the water phase with concentrations ranging from below the method detection limit to 6.6 ng L - 1. This study indicates that atmospheric deposition of APs and phthalates into the North <span class="hlt">Sea</span> is an important input pathway. The net fluxes indicate that the <span class="hlt">air</span> <span class="hlt">sea</span> <span class="hlt">exchange</span> is significant and, consequently the open ocean and polar areas will be an extensive sink for APs and phthalates.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002AGUSMGC32A..05K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002AGUSMGC32A..05K"><span><span class="hlt">CO</span><span class="hlt">2</span> Capture from the <span class="hlt">Air</span>: Technology Assessment and Implications for Climate Policy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Keith, D. W.</p> <p>2002-05-01</p> <p>It is physically possible to capture <span class="hlt">CO</span><span class="hlt">2</span> directly from the <span class="hlt">air</span> and immobilize it in geological structures. Today, there are no large-scale technologies that achieve <span class="hlt">air</span> capture at reasonable cost. Yet, strong arguments suggest that it will comparatively easy to develop practical <span class="hlt">air</span> capture technologies on the timescales relevant to climate policy [1]. This paper first analyzes the cost of <span class="hlt">air</span> capture and then assesses the implications for climate policy. We first analyze the lower bound on the cost needed for <span class="hlt">air</span> capture, describing the thermodynamic and physical limits to the use of energy and land. We then compare the costs of <span class="hlt">air</span> capture to the cost of capture from combustion exhaust streams. While the intrinsic minimum energy requirement is larger for <span class="hlt">air</span> capture, we argue that <span class="hlt">air</span> capture has important structural advantages, such as the reduction of transport costs and the larger potential for economies of scale. These advantages suggest that, in the long-run <span class="hlt">air</span> capture be competitive with other methods of achieving deep emissions reductions. We provide a preliminary engineering-economic analysis of an <span class="hlt">air</span> capture system based on CaO to Ca<span class="hlt">CO</span>3 chemical looping [1]. We analyze the possibility of doing the calcination in a modified pressurized fluidized bed combustor (PFBC) burning coal in a <span class="hlt">CO</span><span class="hlt">2</span> rich atmosphere with oxygen supplied by an <span class="hlt">air</span> separation unit. The Ca<span class="hlt">CO</span>3-to-coal ratio would be ~<span class="hlt">2</span>:1 and the system would be nearly thermally neutral. PFBC systems have been demonstrated at capacities of over 100 MW. Such systems already include Ca<span class="hlt">CO</span>3 injection for sulfur control, and operate at suitable temperatures and pressures for calcination. We assess the potential to recover heat from the dissolution of CaO in order to reduce the overall energy requirements. We analyze the possibility of adapting existing large water/<span class="hlt">air</span> heat <span class="hlt">exchangers</span> for use as contacting systems to capture <span class="hlt">CO</span><span class="hlt">2</span> from the <span class="hlt">air</span> using the calcium hydroxide solution. The implications of <span class="hlt">air</span> capture</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 fluxes 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> <span class="hlt">exchange</span> 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> flux 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> </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('http://adsabs.harvard.edu/abs/2003GBioC..17.1070O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003GBioC..17.1070O"><span>Partitioning net ecosystem carbon <span class="hlt">exchange</span> into net assimilation and respiration using 13<span class="hlt">CO</span><span class="hlt">2</span> measurements: A cost-effective sampling strategy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>OgéE, J.; Peylin, P.; Ciais, P.; Bariac, T.; Brunet, Y.; Berbigier, P.; Roche, C.; Richard, P.; Bardoux, G.; Bonnefond, J.-M.</p> <p>2003-06-01</p> <p>The current emphasis on global climate studies has led the scientific community to set up a number of sites for measuring the long-term biosphere-atmosphere net <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> (net ecosystem <span class="hlt">exchange</span>, NEE). Partitioning this flux into its elementary components, net assimilation (FA), and respiration (FR), remains necessary in order to get a better understanding of biosphere functioning and design better surface <span class="hlt">exchange</span> models. Noting that FR and FA have different isotopic signatures, we evaluate the potential of isotopic 13<span class="hlt">CO</span><span class="hlt">2</span> measurements in the <span class="hlt">air</span> (combined with <span class="hlt">CO</span><span class="hlt">2</span> flux and concentration measurements) to partition NEE into FR and FA on a routine basis. The study is conducted at a temperate coniferous forest where intensive isotopic measurements in <span class="hlt">air</span>, soil, and biomass were performed in summer 1997. The multilayer soil-vegetation-atmosphere transfer model MuSICA is adapted to compute 13<span class="hlt">CO</span><span class="hlt">2</span> flux and concentration profiles. Using MuSICA as a "perfect" simulator and taking advantage of the very dense spatiotemporal resolution of the isotopic data set (341 flasks over a 24-hour period) enable us to test each hypothesis and estimate the performance of the method. The partitioning works better in midafternoon when isotopic disequilibrium is strong. With only 15 flasks, i.e., two 13<span class="hlt">CO</span><span class="hlt">2</span> nighttime profiles (to estimate the isotopic signature of FR) and five daytime measurements (to perform the partitioning) we get mean daily estimates of FR and FA that agree with the model within 15-20%. However, knowledge of the mesophyll conductance seems crucial and may be a limitation to the method.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.8897H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.8897H"><span>Climate warming impacts on boreal landscape net <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Helbig, Manuel; Kljun, Natascha; E Chasmer, Laura; Desai, Ankur R.; Quinton, William L.; Sonnentag, Oliver</p> <p>2017-04-01</p> <p>In boreal peatlands of the North American sporadic permafrost zone, climate change causes permafrost thaw and induces changes in vegetation composition and structure. Boreal landscape net carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) fluxes in these regions will thus be modified directly through the changes in the meteorological forcing of ecosystem processes and indirectly through changes in landscape functioning associated with thaw-induced land cover changes. How the combined effects alter net ecosystem <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> of these landscapes (NEELAND), resulting from changes in gross primary productivity (GPP) and ecosystem respiration (ER), remains unknown. Here, we quantify indirect land cover and direct climate change impacts on NEELAND for a boreal forest-wetland landscape in the organic-rich Taiga Plains of northwestern Canada. Using 1.5 years of nested eddy covariance flux tower measurements, we observe both larger GPP and ER at the landscape-level (50% forested permafrost plateaus & 50% permafrost-free wetlands) compared to the wetland-level (100% permafrost-free wetland). However, the resulting annual NEELAND (-20±6 g C m-<span class="hlt">2</span>) was similar to NEE of the wetland (-24±8 g C m-<span class="hlt">2</span>). Indirect thaw-induced wetland expansion effects thus appear to have negligible effects on NEELAND. In contrast, we find larger direct climate change impacts when modeling end-of-the-21st-century NEELAND (2091-2100) using downscaled <span class="hlt">air</span> temperature and incoming shortwave radiation projections. Modeled GPP indicates large spring and fall increases due to reduced temperature-limitation. At the same time, light-limitation of GPP becomes more frequent in fall. The projected warmer <span class="hlt">air</span> temperatures increase ER year-round in the absence of moisture stress. As a result, larger net <span class="hlt">CO</span><span class="hlt">2</span> uptake is projected for the shoulder seasons while the peak growing season net <span class="hlt">CO</span><span class="hlt">2</span> uptake declines. The modeled annual NEELAND is projected to decline by 25±15 g C m-<span class="hlt">2</span> for a moderate (RCP 4.5) and 103±37 g C m-<span class="hlt">2</span> for a high warming</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4951643','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4951643"><span>Biopolymers form a gelatinous microlayer at the <span class="hlt">air-sea</span> interface when Arctic <span class="hlt">sea</span> ice melts</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Galgani, Luisa; Piontek, Judith; Engel, Anja</p> <p>2016-01-01</p> <p>The interface layer between ocean and atmosphere is only a couple of micrometers thick but plays a critical role in climate relevant processes, including the <span class="hlt">air-sea</span> <span class="hlt">exchange</span> of gas and heat and the emission of primary organic aerosols (POA). Recent findings suggest that low-level cloud formation above the Arctic Ocean may be linked to organic polymers produced by marine microorganisms. <span class="hlt">Sea</span> ice harbors high amounts of polymeric substances that are produced by cells growing within the <span class="hlt">sea</span>-ice brine. Here, we report from a research cruise to the central Arctic Ocean in 2012. Our study shows that microbial polymers accumulate at the <span class="hlt">air-sea</span> interface when the <span class="hlt">sea</span> ice melts. Proteinaceous compounds represented the major fraction of polymers supporting the formation of a gelatinous interface microlayer and providing a hitherto unrecognized potential source of marine POA. Our study indicates a novel link between <span class="hlt">sea</span> ice-ocean and atmosphere that may be sensitive to climate change. PMID:27435531</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20140002076&hterms=european+union&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Deuropean%2Bunion','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20140002076&hterms=european+union&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Deuropean%2Bunion"><span>Monitoring <span class="hlt">Exchange</span> of <span class="hlt">CO</span><span class="hlt">2</span> - A KISS Workshop Report 2009</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Miller, Charles; Wennberg, Paul</p> <p>2009-01-01</p> <p>The problem and context: Can top-down estimates of carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) fluxes resolve the anthropogenic emissions of China, India, the United States, and the European Union with an accuracy of +/-10% or better?The workshop "Monitoring <span class="hlt">Exchange</span> of Carbon Dioxide" was convened at the Keck Institute for Space Studies in Pasadena, California in February 2010 to address this question. The Workshop brought together an international, interdisciplinary group of 24 experts in carbon cycle science, remote sensing, emissions inventory estimation, and inverse modeling. The participants reviewed the potential of space-based and sub-orbital observational and modeling approaches to monitor anthropogenic <span class="hlt">CO</span><span class="hlt">2</span> emissions in the presence of much larger natural fluxes from the <span class="hlt">exchange</span> of <span class="hlt">CO</span><span class="hlt">2</span> between the land, atmosphere, and ocean. This particular challenge was motivated in part by the NRC Report "Verifying Greenhouse Gas Emissions" [Pacala et al., 2010]. This workshop report includes several recommendations for improvements to observing strategies and modeling frameworks for optimal and cost-effective monitoring of carbon <span class="hlt">exchange</span></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('http://files.eric.ed.gov/fulltext/ED259926.pdf','ERIC'); return false;" href="http://files.eric.ed.gov/fulltext/ED259926.pdf"><span>Heat Recovery Ventilation for Housing: <span class="hlt">Air-to-Air</span> Heat <span class="hlt">Exchangers</span>.</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Corbett, Robert J.; Miller, Barbara</p> <p></p> <p>The <span class="hlt">air-to-air</span> heat <span class="hlt">exchanger</span> (a fan powered ventilation device that recovers heat from stale outgoing <span class="hlt">air</span>) is explained in this six-part publication. Topic areas addressed are: (1) the nature of <span class="hlt">air-to-air</span> heat <span class="hlt">exchangers</span> and how they work; (<span class="hlt">2</span>) choosing and sizing the system; (3) installation, control, and maintenance of the system; (4) heat…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19950031262&hterms=biome&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dbiome','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19950031262&hterms=biome&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dbiome"><span><span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> in the Hudson Bay lowlands: Community characteristics and multispectral reflectance properties</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Whiting, Gary J.</p> <p>1994-01-01</p> <p>Net ecosystem <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> was measured during the 1990 growing season (June to August) along a transect starting 10 km inland from James Bay and extending 100 km interior to Kinosheo Lake, Ontario. Sites were chosen in three distinct areas: a coastal fen, an interior fen, and a bog. For the most productive sites in the bog, net daily uptake rates reached a maximum of <span class="hlt">2</span>.5 g C-<span class="hlt">CO</span><span class="hlt">2</span> m(exp -<span class="hlt">2</span>)/d with an area-weighted <span class="hlt">exchange</span> of 0.3 g C-<span class="hlt">CO</span><span class="hlt">2</span> m(exp -<span class="hlt">2</span>)/d near midsummer. This site was estimated to be a net carbon source of 9 g C-<span class="hlt">CO</span><span class="hlt">2</span> m(exp -<span class="hlt">2</span>) to the atmosphere over a 153-day growing season. The interior fen was less productive on a daily basis with a net maximum uptake of 0.5 g C-<span class="hlt">CO</span><span class="hlt">2</span> m(exp -<span class="hlt">2</span>)/d and with corresponding area-weighted uptake of 0.1 g C-<span class="hlt">CO</span><span class="hlt">2</span> m(exp -<span class="hlt">2</span>)/d during midsummer. Early and late season release of carbon to the atmosphere resulted in a net loss of 21 g C-<span class="hlt">CO</span><span class="hlt">2</span> m(exp -<span class="hlt">2</span>) over the growing season from this site. The coastal fen was the most productive site with uptake rates peaking near 1.7 g C-<span class="hlt">CO</span><span class="hlt">2</span> m(exp -<span class="hlt">2</span>)/d which corresponded to an area-weighted uptake of 0.8 g C-<span class="hlt">CO</span><span class="hlt">2</span> m(exp -<span class="hlt">2</span>)/d during midsummer and an estimated net uptake of 6 g C-<span class="hlt">CO</span><span class="hlt">2</span> m(exp -<span class="hlt">2</span>) for the growing season. Associated with net <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> measurements, multispectral reflectance properties of the sites were measured over the growing season using portable radiometers. These properties were related to <span class="hlt">exchange</span> rates with the goal of examining the potential for satellite remote sensing to monitor biosphere/atmosphere <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> in this biome. The normalized difference vegetation index (NDVI) computed from surface reflectance was correlated with net <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> for all sites with the exception of areas with large proportions of Sphagnum moss cover. These mosses have greater near-infrared reflectance than typical surrounding vegetation and may require special adjustment for regional <span class="hlt">exchange</span>/remote sensing applications.</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 <span class="hlt">exchanges</span> 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 flux using a range of <span class="hlt">air-sea</span> gas <span class="hlt">exchange</span> parameterizations. We then compared this oxygen flux to the rate of change of the measured oxygen inventory. Where the inventory and flux 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 <span class="hlt">exchanges</span> 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/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> <span class="hlt">exchanges</span> 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> fluxes 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> fluxes observed in two microtidal, lagoonal estuaries. <span class="hlt">Air</span>-water <span class="hlt">CO</span><span class="hlt">2</span> fluxes 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> fluxes 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> fluxes in this system. Although annual <span class="hlt">CO</span><span class="hlt">2</span> fluxes 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> <span class="hlt">Exchanges</span> 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> fluxes 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> fluxes observed in two microtidal, lagoonal estuaries. <span class="hlt">Air</span>-water <span class="hlt">CO</span><span class="hlt">2</span> fluxes 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> fluxes 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> fluxes 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> fluxes 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/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> <span class="hlt">exchange</span> 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> flux 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('http://adsabs.harvard.edu/abs/2017BGeo...14.5595B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017BGeo...14.5595B"><span>Continuous measurement of <span class="hlt">air</span>-water gas <span class="hlt">exchange</span> by underwater 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>Berg, Peter; Pace, Michael L.</p> <p>2017-12-01</p> <p><span class="hlt">Exchange</span> of gases, such as O<span class="hlt">2</span>, <span class="hlt">CO</span><span class="hlt">2</span>, and CH4, over the <span class="hlt">air</span>-water interface is an important component in aquatic ecosystem studies, but <span class="hlt">exchange</span> rates are typically measured or estimated with substantial uncertainties. This diminishes the precision of common ecosystem assessments associated with gas <span class="hlt">exchanges</span> such as primary production, respiration, and greenhouse gas emission. Here, we used the aquatic eddy covariance technique - originally developed for benthic O<span class="hlt">2</span> flux measurements - right below the <span class="hlt">air</span>-water interface (˜ 4 cm) to determine gas <span class="hlt">exchange</span> rates and coefficients. Using an acoustic Doppler velocimeter and a fast-responding dual O<span class="hlt">2</span>-temperature sensor mounted on a floating platform the 3-D water velocity, O<span class="hlt">2</span> concentration, and temperature were measured at high-speed (64 Hz). By combining these data, concurrent vertical fluxes of O<span class="hlt">2</span> and heat across the <span class="hlt">air</span>-water interface were derived, and gas <span class="hlt">exchange</span> coefficients were calculated from the former. Proof-of-concept deployments at different river sites gave standard gas <span class="hlt">exchange</span> coefficients (k600) in the range of published values. A 40 h long deployment revealed a distinct diurnal pattern in <span class="hlt">air</span>-water <span class="hlt">exchange</span> of O<span class="hlt">2</span> that was controlled largely by physical processes (e.g., diurnal variations in <span class="hlt">air</span> temperature and associated <span class="hlt">air</span>-water heat fluxes) and not by biological activity (primary production and respiration). This physical control of gas <span class="hlt">exchange</span> can be prevalent in lotic systems and adds uncertainty to assessments of biological activity that are based on measured water column O<span class="hlt">2</span> concentration changes. For example, in the 40 h deployment, there was near-constant river flow and insignificant winds - two main drivers of lotic gas <span class="hlt">exchange</span> - but we found gas <span class="hlt">exchange</span> coefficients that varied by several fold. This was presumably caused by the formation and erosion of vertical temperature-density gradients in the surface water driven by the heat flux into or out of the river that affected the turbulent</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1036239','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1036239"><span>Iron Fertilization of the Southern Ocean: Regional Simulation and Analysis of C-Sequestration in the Ross <span class="hlt">Sea</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>Kevin Arrigo</p> <p>2012-03-13</p> <p>A modified version of the dynamic 3-dimensional mesoscale Coupled Ice, Atmosphere, and Ocean model (CIAO) of the Ross <span class="hlt">Sea</span> ecosystem has been used to simulate the impact of environmental perturbations upon primary production and biogenic <span class="hlt">CO</span><span class="hlt">2</span> uptake. The Ross <span class="hlt">Sea</span> supports two taxonomically, and spatially distinct phytoplankton populations; the haptophyte Phaeocystis antarctica and diatoms. Nutrient utilization ratios predict that P. antarctica and diatoms will be driven to nitrate and phosphate limitation, respectively. Model and field data have confirmed that the Ross <span class="hlt">Sea</span> is iron limited with only two-thirds of the macronutrients consumed by the phytoplankton by the end of themore » growing season. In this study, the CIAO model was improved to simulate a third macronutrient (phosphate), dissolved organic carbon, <span class="hlt">air-sea</span> gas <span class="hlt">exchange</span>, and the carbonate system. This enabled us to effectively model p<span class="hlt">CO</span><span class="hlt">2</span> and subsequently oceanic <span class="hlt">CO</span><span class="hlt">2</span> uptake via gas <span class="hlt">exchange</span>, allowing investigations into the affect of alleviating iron limitation on both p<span class="hlt">CO</span><span class="hlt">2</span> and nutrient drawdown.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013BGD....10.8415S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013BGD....10.8415S"><span>Biology and <span class="hlt">air-sea</span> gas <span class="hlt">exchange</span> controls on the distribution of carbon isotope ratios (δ13C) in the ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schmittner, A.; Gruber, N.; Mix, A. C.; Key, R. M.; Tagliabue, A.; Westberry, T. K.</p> <p>2013-05-01</p> <p>Analysis of observations and sensitivity experiments with a new three-dimensional global model of stable carbon isotope cycling elucidate the processes that control the distribution of δ13C in the contemporary and preindustrial ocean. Biological fractionation dominates the distribution of δ13CDIC of dissolved inorganic carbon (DIC) due to the sinking of isotopically light δ13C organic matter from the surface into the interior ocean. This process leads to low δ13CDIC values at dephs and in high latitude surface waters and high values in the upper ocean at low latitudes with maxima in the subtropics. <span class="hlt">Air-sea</span> gas <span class="hlt">exchange</span> provides an important secondary influence due to two effects. First, it acts to reduce the spatial gradients created by biology. Second, the associated temperature dependent fractionation tends to increase (decrease) δ13CDIC values of colder (warmer) water, which generates gradients that oppose those arising from biology. Our model results suggest that both effects are similarly important in influencing surface and interior δ13CDIC distributions. However, <span class="hlt">air-sea</span> gas <span class="hlt">exchange</span> is slow, so biological effect dominate spatial δ13CDIC gradients both in the interior and at the surface, in constrast to conclusions from some previous studies. Analysis of a new synthesis of δ13CDIC measurements from years 1990 to 2005 is used to quantify preformed (δ13Cpre) and remineralized (δ13Crem) contributions as well as the effects of biology (Δδ13Cbio) and <span class="hlt">air-sea</span> gas <span class="hlt">exchange</span> (δ13C*). The model reproduces major features of the observed large-scale distribution of δ13CDIC, δ13Cpre, δ13Crem, δ13C*, and Δδ13Cbio. Residual misfits are documented and analyzed. Simulated surface and subsurface δ13CDIC are influenced by details of the ecosystem model formulation. For example, inclusion of a simple parameterization of iron limitation of phytoplankton growth rates and temperature-dependent zooplankton grazing rates improves the agreement with δ13CDIC</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21963172','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21963172"><span><span class="hlt">Co</span><span class="hlt">2</span>+-<span class="hlt">exchange</span> mechanism of birnessite and its application for the removal of Pb<span class="hlt">2</span>+ and As(III).</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yin, Hui; Liu, Fan; Feng, Xionghan; Liu, Mingming; Tan, Wenfeng; Qiu, Guohong</p> <p>2011-11-30</p> <p><span class="hlt">Co</span>-containing birnessites were obtained by ion <span class="hlt">exchange</span> at different initial concentrations of <span class="hlt">Co</span>(<span class="hlt">2</span>+). Ion <span class="hlt">exchange</span> of <span class="hlt">Co</span>(<span class="hlt">2</span>+) had little effect on birnessite crystal structure and micromorphology, but resulted in an increase in specific surface areas from 19.26 to 33.35 m(<span class="hlt">2</span>)g(-1), and a decrease in both crystallinity and manganese average oxidation state. It was due to that Mn(IV) in the layer structure was reduced to Mn(III) during the oxidation process of <span class="hlt">Co</span>(<span class="hlt">2</span>+) to <span class="hlt">Co</span>(III). The hydroxyl groups on the surface of <span class="hlt">Co</span>-containing birnessites gradually decreased with an increase of <span class="hlt">Co</span>/Mn molar ratio owing to the occupance of <span class="hlt">Co</span>(III) into vacancies and the location of large amounts of <span class="hlt">Co</span>(<span class="hlt">2</span>+/3+) and Mn(<span class="hlt">2</span>+/3+) above/below the vacant sites. This greatly accounted for the monotonous reduction in Pb(<span class="hlt">2</span>+) adsorption capacity, from 2538 mmol kg(-1) for the unmodified birnessite to 1500 mmol kg(-1) for the <span class="hlt">Co</span>(<span class="hlt">2</span>+) ion-<span class="hlt">exchanged</span> birnessite with a <span class="hlt">Co</span>/Mn molar ratio of 0.16. The amount of As(III) oxidized by birnessite was enhanced after ion <span class="hlt">exchange</span>, but the apparent initial reaction rate was greatly decreased. The present work demonstrates that <span class="hlt">Co</span>(<span class="hlt">2</span>+) ion <span class="hlt">exchange</span> has great influence on the adsorption and oxidation behavior of inorganic toxic metal ions by birnessite in water environments. Copyright © 2011 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A53F2321H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A53F2321H"><span>Indoor Levels of Formaldehyde and Other Pollutants and Relationship to <span class="hlt">Air</span> <span class="hlt">Exchange</span> Rates and Human Activities</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Huangfu, Y.; O'Keeffe, P.; Kirk, M.; Walden, V. P.; Lamb, B. K.; Jobson, B. T.</p> <p>2017-12-01</p> <p>This paper reports results on an indoor <span class="hlt">air</span> quality study conducted on six homes in summer and winter, contrasting indoor and outdoor concentrations of O3, <span class="hlt">CO</span>, <span class="hlt">CO</span><span class="hlt">2</span>, NOx, PM<span class="hlt">2</span>.5, and selected volatile organic hydrocarbons measured by PTR-MS. Data were collected as 1 minute averages. <span class="hlt">Air</span> <span class="hlt">exchange</span> rates of the homes were determined by <span class="hlt">CO</span><span class="hlt">2</span> tracer release. Smart home sensors, recording human activity level in various places in the home, and window and doors openings, were utilized to better understand the link between human activity and indoor <span class="hlt">air</span> pollution. From our study, averaged <span class="hlt">air</span> <span class="hlt">exchange</span> rates of the homes ranged from 0.<span class="hlt">2</span> to 1.<span class="hlt">2</span> hour-1 and were greatly affected by the ventilation system type and window and door openings. In general, a negative correlation between <span class="hlt">air</span> <span class="hlt">exchange</span> rate and indoor VOCs levels was observed, with large variation of pollutant levels between the homes. For most of the VOCs measured in the house, including formaldehyde and acetaldehyde, summer levels were much higher than winter levels. In some homes formaldehyde levels displayed a time of day variation that was linked to changes in indoor temperature. During a wildfire period in the summer of 2015, outdoor levels of PM<span class="hlt">2</span>.5, formaldehyde, and benzene dramatically increased, significantly impacting indoor levels due to infiltration. Human activities, such as cooking, can significantly change the levels of most of the compounds measured in the house and the levels can be significantly elevated for short periods of time, with peak levels can be several orders higher compared with typical levels. The data suggest that an outcome of state energy codes that require new homes to be energy efficient, and as a consequence built with lower <span class="hlt">air</span> <span class="hlt">exchange</span> rates, will be unacceptable levels of <span class="hlt">air</span> toxics, notably formaldehyde.</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> <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> </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/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> flux 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> flux 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 flux in this region.</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> Fluxes 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> fluxes 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> flux 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> flux. In this study, we used Argo profiling floats with modified oxygen sensors to estimate O<span class="hlt">2</span> fluxes 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 flux 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> fluxes 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> flux. Mean annual <span class="hlt">air-sea</span> oxygen fluxes (positive fluxes 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> flux due to bubbles was greater than 50% of the total flux for winter months and essential for determining the magnitude and, in some cases, direction of the cumulative mean annual flux. Increases in solubility due to wintertime</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JETP..125.1096S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JETP..125.1096S"><span><span class="hlt">Exchange</span> Bias in Layered GdBa<span class="hlt">Co</span><span class="hlt">2</span>O5.5 Cobaltite</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Solin, N. I.; Naumov, S. V.; Telegin, S. V.; Korolev, A. V.</p> <p>2017-12-01</p> <p>It is established that excess oxygen content δ influences the <span class="hlt">exchange</span> bias (EB) in layered GdBa-<span class="hlt">Co</span><span class="hlt">2</span>O5 + δ cobaltite. The EB effect arises in p-type (δ > 0.5) cobaltite and disappears in n-type (δ < 0.5) cobaltite. The main parameters of EB in GdBa<span class="hlt">Co</span><span class="hlt">2</span>O5.52(<span class="hlt">2</span>) polycrystals are determined, including the field and temperature dependences of EB field H EB , blocking temperature T B , <span class="hlt">exchange</span> coupling energy J i of antiferromagnet-ferromagnet (AFM-FM) interface, and dimensions of FM clusters. The training effect inherent in systems with EB has been studied. The results are explained in terms of <span class="hlt">exchange</span> interaction between the FM and AFM phases. It is assumed that the EB originates from the coexistence of <span class="hlt">Co</span>3+ and <span class="hlt">Co</span>4+ ions that leads to the formation of monodomain FM clusters in the AFM matrix of cobaltite.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4849023','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4849023"><span>Changes in <span class="hlt">Air</span> <span class="hlt">CO</span><span class="hlt">2</span> Concentration Differentially Alter Transcript Levels of NtAQP1 and NtPIP<span class="hlt">2</span>;1 Aquaporin Genes in Tobacco Leaves</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Secchi, Francesca; Schubert, Andrea; Lovisolo, Claudio</p> <p>2016-01-01</p> <p>The aquaporin specific control on water versus carbon pathways in leaves is pivotal in controlling gas <span class="hlt">exchange</span> and leaf hydraulics. We investigated whether Nicotiana tabacum aquaporin 1 (NtAQP1) and Nicotiana tabacum plasma membrane intrinsic protein <span class="hlt">2</span>;1 (NtPIP<span class="hlt">2</span>;1) gene expression varies in tobacco leaves subjected to treatments with different <span class="hlt">CO</span><span class="hlt">2</span> concentrations (ranging from 0 to 800 ppm), inducing changes in photosynthesis, stomatal regulation and water evaporation from the leaf. Changes in <span class="hlt">air</span> <span class="hlt">CO</span><span class="hlt">2</span> concentration ([<span class="hlt">CO</span><span class="hlt">2</span>]) affected net photosynthesis (Pn) and leaf substomatal [<span class="hlt">CO</span><span class="hlt">2</span>] (Ci). Pn was slightly negative at 0 ppm <span class="hlt">air</span> <span class="hlt">CO</span><span class="hlt">2</span>; it was one-third that of ambient controls at 200 ppm, and not different from controls at 800 ppm. Leaves fed with 800 ppm [<span class="hlt">CO</span><span class="hlt">2</span>] showed one-third reduced stomatal conductance (gs) and transpiration (E), and their gs was in turn slightly lower than in 200 ppm– and in 0 ppm–treated leaves. The 800 ppm <span class="hlt">air</span> [<span class="hlt">CO</span><span class="hlt">2</span>] strongly impaired both NtAQP1 and NtPIP<span class="hlt">2</span>;1 gene expression, whereas 0 ppm <span class="hlt">air</span> [<span class="hlt">CO</span><span class="hlt">2</span>], a concentration below any in vivo possible conditions and specifically chosen to maximize the gene expression alteration, increased only the NtAQP1 transcript level. We propose that NtAQP1 expression, an aquaporin devoted to <span class="hlt">CO</span><span class="hlt">2</span> transport, positively responds to <span class="hlt">CO</span><span class="hlt">2</span> scarcity in the <span class="hlt">air</span> in the whole range 0–800 ppm. On the contrary, expression of NtPIP<span class="hlt">2</span>;1, an aquaporin not devoted to <span class="hlt">CO</span><span class="hlt">2</span> transport, is related to water balance in the leaf, and changes in parallel with gs. These observations fit in a model where upregulation of leaf aquaporins is activated at low Ci, while downregulation occurs when high Ci saturates photosynthesis and causes stomatal closure. PMID:27089333</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19770025778','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19770025778"><span>Regenerable device for scrubbing breathable <span class="hlt">air</span> of <span class="hlt">CO</span><span class="hlt">2</span> and moisture without special heat <span class="hlt">exchanger</span> equipment</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Tepper, E. H. (Inventor)</p> <p>1977-01-01</p> <p>The device concerns the circulation of cabin <span class="hlt">air</span> through canisters which absorb and adsorb carbon dioxide, together with excess moisture, and return the scrubbed <span class="hlt">air</span> to the cabin for recirculation. A coating on an inert substrate in granular form absorbs and adsorbs the impurities at standard temperatures and pressures, but desorbs such impurities at low pressures (vacuum) and standard temperatures. This fact is exploited by making the device in a stack of cells consisting of layers or cells which are isolated from one another flow-wise and are connected to separate manifolds and valving systems into two separate subsets. A first subset may be connected for the flow breathable <span class="hlt">air</span> therethrough until the polyethyleneimine of its cells is saturated with <span class="hlt">CO</span><span class="hlt">2</span> and H<span class="hlt">2</span>O. During the same period the second subset of cells is manifolded to a vacuum source.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19990094165&hterms=clear+pool&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dclear%2Bpool','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19990094165&hterms=clear+pool&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dclear%2Bpool"><span>Tropical Intraseasonal <span class="hlt">Air-Sea</span> <span class="hlt">Exchanges</span> during the 1997 Pacific Warming</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sui, C.-H.; Lau, K.-M.; Chou, S.-H.; Wang, Zihou</p> <p>1999-01-01</p> <p>The Madden Julian Oscillations (MJO) and associated westerly wind (WW) events account for much of the tropical intraseasonal variability (TISV). The TISV has been suggested as an important stochastic forcing that may be one of the underlying causes for the observed irregularities of the El Nino-Southern Oscillation (ENSO). Recent observational studies and theories of interannual to interdecadal-scale variability suggest that ENSO may arise from different mechanisms depending on the basic states. The Pacific warming event of 1997, being associated with a period of strong MJO and WW events, serves as a natural experiment for studying the possible role of TISV in triggering an ENSO event. We have performed a combined statistical and composite analysis of surface WW events based on the assimilated surface wind and <span class="hlt">sea</span> level pressure for the period of 1980-1993, the SSM/I wind for the period of 1988-1997, and OLR. Results indicates that extratropical forcing contribute significantly to the evolution of MJO and establishment of WW events over the Pacific warm pool. Following the major WW events, there appeared an eastward extension of equatorial warm SST anomalies from the western Pacific warm pool. Such tropical-extratropical interaction is particularly clear in the winter of 96-97 that leads to the recent warming event in 1997/98. From the above discussion, our current study on this subject is based on the hypothesis that 1) there is an enhanced <span class="hlt">air-sea</span> interaction associated with TISV and the northerly surges from the extratropics in the initial phase of the 97/98 warming event, and <span class="hlt">2</span>) the relevant mechanisms are functions of the basic state of the coupled system (in terms of SST distribution and atmospheric mean circulation) that varies at the interannual and interdecadal time scale. We are analyzing the space-time structure of the northerly surges, their association with <span class="hlt">air-sea</span> fluxes and upper ocean responses during the period of September 1996 to June 1997. The</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 fluxes, 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> fluxes, 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> fluxes, ikaite formation, and net primary production, are secondary factors. In terms of ice-atmosphere <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchanges</span>, <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> flux 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> fluxes 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> fluxes 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/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 fluxes, 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> fluxes, 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> fluxes, ikaite formation, and net primary production, are secondary factors. In terms of ice-atmosphere <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchanges</span>, <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> flux 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> fluxes 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> fluxes 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/2017JGRG..122.1343B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRG..122.1343B"><span><span class="hlt">Exchange</span> of carbonyl sulfide (OCS) between soils and atmosphere under various <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>Bunk, Rüdiger; Behrendt, Thomas; Yi, Zhigang; Andreae, Meinrat O.; Kesselmeier, Jürgen</p> <p>2017-06-01</p> <p>A new continuous integrated cavity output spectroscopy analyzer and an automated soil chamber system were used to investigate the <span class="hlt">exchange</span> processes of carbonyl sulfide (OCS) between soils and the atmosphere under laboratory conditions. The <span class="hlt">exchange</span> patterns of OCS between soils and the atmosphere were found to be highly dependent on soil moisture and ambient <span class="hlt">CO</span><span class="hlt">2</span> concentration. With increasing soil moisture, OCS <span class="hlt">exchange</span> ranged from emission under dry conditions to an uptake within an optimum moisture range, followed again by emission at high soil moisture. Elevated <span class="hlt">CO</span><span class="hlt">2</span> was found to have a significant impact on the <span class="hlt">exchange</span> rate and direction as tested with several soils. There is a clear tendency toward a release of OCS at higher <span class="hlt">CO</span><span class="hlt">2</span> levels (up to 7600 ppm), which are typical for the upper few centimeters within soils. At high soil moisture, the release of OCS increased sharply. Measurements after chloroform vapor application show that there is a biotic component to the observed OCS <span class="hlt">exchange</span>. Furthermore, soil treatment with the fungi inhibitor nystatin showed that fungi might be the dominant OCS consumers in the soils we examined. We discuss the influence of soil moisture and elevated <span class="hlt">CO</span><span class="hlt">2</span> on the OCS <span class="hlt">exchange</span> as a change in the activity of microbial communities. Physical factors such as diffusivity that are governed by soil moisture also play a role. Comparing KM values of the enzymes to projected soil water <span class="hlt">CO</span><span class="hlt">2</span> concentrations showed that competitive inhibition is unlikely for carbonic anhydrase and PEPCO but might occur for Rubis<span class="hlt">CO</span> at higher <span class="hlt">CO</span><span class="hlt">2</span> concentrations.</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('http://adsabs.harvard.edu/abs/2016AGUFM.B11B0442B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.B11B0442B"><span>Regulation of leaf-gas <span class="hlt">exchange</span> strategies of woody plants under elevated <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>Belmecheri, S.; Guerrieri, R.; Voelker, S.</p> <p>2016-12-01</p> <p>Estimates of vegetation water use efficiency (WUE) have increasingly been assessed using both eddy covariance and plant stable isotope techniques but these data have often lead to differing conclusions. Eddy covariance can provide forest ecosystem-level responses of coupled carbon and water <span class="hlt">exchanges</span> to recent global change phenomena. These direct observations, however, are generally less than one or two decades, thus documenting ecosystem-level responses at elevated [<span class="hlt">CO</span><span class="hlt">2</span>] concentrations (350-400 ppm). Therefore, eddy covariance data cannot directly address plant physiological mechanisms and adaptation to climate variability and anthropogenic factors, e.g., increasing atmospheric [<span class="hlt">CO</span><span class="hlt">2</span>]. By contrast, tree based carbon isotope approaches can retrospectively assess intrinsic WUE over long periods and have documented physiological responses to ambient atmospheric [<span class="hlt">CO</span><span class="hlt">2</span>] (ca), which have often been contextualized within generalized strategies for stomatal regulation of leaf gas-<span class="hlt">exchange</span>. These include maintenance of a constant leaf internal [<span class="hlt">CO</span><span class="hlt">2</span>] (ci), a constant drawdown in [<span class="hlt">CO</span><span class="hlt">2</span>] (ca - ci), and a constant ci/ca . Tree carbon isotope studies, however, cannot account for changes in leaf area of individual trees or canopies, which makes scaling up a difficult task. The limitations of these different approaches to understanding how forest water use efficiency has been impacted by rising [<span class="hlt">CO</span><span class="hlt">2</span>] has contributed to the uncertainty in global terrestrial carbon cycling and the "missing" terrestrial carbon sink. We examined stable C isotope ratios (d13C) from woody plants over a wide range of [<span class="hlt">CO</span><span class="hlt">2</span>] (200-400 ppm) to test for patterns of ci-regulation in response to rising ca. The analyses are not consistent with any of the leaf gas-<span class="hlt">exchange</span> regulation strategies noted above. The data suggest that ca - ci is still recently increasing in most species but that the rate of increase is less than expected from paleo trees which grew at much lower [<span class="hlt">CO</span><span class="hlt">2</span>]. This evidence demonstrates that a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014TCry....8.1469R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014TCry....8.1469R"><span>Temporal dynamics of ikaite 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>Rysgaard, S.; Wang, F.; Galley, R. J.; Grimm, R.; Notz, D.; Lemes, M.; Geilfus, N.-X.; Chaulk, A.; Hare, A. A.; Crabeck, O.; Else, B. G. T.; Campbell, K.; Sørensen, L. L.; Sievers, J.; Papakyriakou, T.</p> <p>2014-08-01</p> <p>Ikaite (Ca<span class="hlt">CO</span>3 · 6H<span class="hlt">2</span>O) is a metastable phase of calcium carbonate that normally forms in a cold environment and/or under high pressure. 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> <span class="hlt">exchange</span> 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 outdoor pool of the <span class="hlt">Sea</span>-ice Environmental Research Facility (SERF) in Manitoba, Canada. During the experiment, ikaite precipitated in <span class="hlt">sea</span> ice when temperatures were below -4 °C, creating three distinct zones of ikaite concentrations: (1) a millimeter-to-centimeter-thin surface layer containing frost flowers and brine skim with bulk ikaite concentrations of >2000 μmol kg-1, (<span class="hlt">2</span>) an internal layer with ikaite concentrations of 200-400 μmol kg-1, and (3) a bottom layer with ikaite concentrations of <100 μmol kg-1. Snowfall events caused the <span class="hlt">sea</span> ice to warm and ikaite crystals to dissolve. 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 observed ikaite concentrations were on the same order of magnitude as modeled by FREZCHEM, which further supports the notion that ikaite concentration in <span class="hlt">sea</span> ice increases with decreasing temperature. Thus, varying snow conditions may play a key role in ikaite precipitation and dissolution in <span class="hlt">sea</span> ice. This could have a major implication for <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> with the atmosphere and ocean that has not been accounted for previously.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22563649','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22563649"><span>Photodissociation dynamics of gaseous Cp<span class="hlt">Co(CO</span>)<span class="hlt">2</span> and ligand <span class="hlt">exchange</span> reactions of Cp<span class="hlt">Co</span>H<span class="hlt">2</span> with C3H4, C3H6, and NH3.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Oana, Melania; Nakatsuka, Yumiko; Albert, Daniel R; Davis, H Floyd</p> <p>2012-05-31</p> <p>The photodissociation dynamics of Cp<span class="hlt">Co(CO</span>)(<span class="hlt">2</span>) was studied in a molecular beam using photofragment translational energy spectroscopy with 157 nm photoionization detection of the metallic products. At 532 and 355 nm excitation, the dominant one-photon channel involved loss of a single <span class="hlt">CO</span> ligand producing Cp<span class="hlt">CoCO</span>. The product angular distributions were isotropic, and a large fraction of excess energy appeared as product vibrational excitation. Production of Cp<span class="hlt">CO</span> + <span class="hlt">2</span><span class="hlt">CO</span> resulted from two-photon absorption processes. The two-photon dissociation of mixtures containing Cp<span class="hlt">Co(CO</span>)(<span class="hlt">2</span>) and H(<span class="hlt">2</span>) at the orifice of a pulsed nozzle was used to produce a novel 16-electron unsaturated species, Cp<span class="hlt">Co</span>H(<span class="hlt">2</span>). Transition metal ligand <span class="hlt">exchange</span> reactions, Cp<span class="hlt">Co</span>H(<span class="hlt">2</span>) + L → Cp<span class="hlt">Co</span>L + H(<span class="hlt">2</span>) (L = propyne, propene, or ammonia), were studied under single-collision conditions for the first time. In all cases, ligand <span class="hlt">exchange</span> occurred via 18-electron association complexes with lifetimes comparable to their rotational periods. Although ligand <span class="hlt">exchange</span> reactions were not detected from Cp<span class="hlt">Co</span>H(<span class="hlt">2</span>) collisions with methane or propane (L = CH(4) or C(3)H(8)), a molecular beam containing Cp<span class="hlt">Co</span>CH(4) was produced by photolysis of mixtures containing Cp<span class="hlt">Co(CO</span>)(<span class="hlt">2</span>) and CH(4).</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> flux <span class="hlt">exchange</span> across the <span class="hlt">sea</span>-ice covered areas.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22661254-abundance-atmospheric-co-sub-ocean-exoplanets-novel-co-sub-deposition-mechanism','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22661254-abundance-atmospheric-co-sub-ocean-exoplanets-novel-co-sub-deposition-mechanism"><span>The Abundance of Atmospheric <span class="hlt">CO</span>{sub <span class="hlt">2</span>} in Ocean Exoplanets: a Novel <span class="hlt">CO</span>{sub <span class="hlt">2</span>} Deposition Mechanism</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>Levi, A.; Sasselov, D.; Podolak, M., E-mail: amitlevi.planetphys@gmail.com</p> <p></p> <p>We consider super-Earth sized planets which have a water mass fraction large enough to form an external mantle composed of high-pressure water-ice polymorphs and also lack a substantial H/He atmosphere. We consider such planets in their habitable zone, so that their outermost condensed mantle is a global, deep, liquid ocean. For these ocean planets, we investigate potential internal reservoirs of <span class="hlt">CO</span>{sub <span class="hlt">2</span>}, the amount of <span class="hlt">CO</span>{sub <span class="hlt">2</span>} dissolved in the ocean for the various saturation conditions encountered, and the ocean-atmosphere <span class="hlt">exchange</span> flux of <span class="hlt">CO</span>{sub <span class="hlt">2</span>}. We find that, in a steady state, the abundance of <span class="hlt">CO</span>{sub <span class="hlt">2</span>} in the atmospheremore » has two possible states. When wind-driven circulation is the dominant <span class="hlt">CO</span>{sub <span class="hlt">2</span>} <span class="hlt">exchange</span> mechanism, an atmosphere of tens of bars of <span class="hlt">CO</span>{sub <span class="hlt">2</span>} results, where the exact value depends on the subtropical ocean surface temperature and the deep ocean temperature. When <span class="hlt">sea</span>-ice formation, acting on these planets as a <span class="hlt">CO</span>{sub <span class="hlt">2</span>} deposition mechanism, is the dominant <span class="hlt">exchange</span> mechanism, an atmosphere of a few bars of <span class="hlt">CO</span>{sub <span class="hlt">2</span>} is established. The exact value depends on the subpolar surface temperature. Our results suggest the possibility of a negative feedback mechanism, unique to water planets, where a reduction in the subpolar temperature drives more <span class="hlt">CO</span>{sub <span class="hlt">2</span>} into the atmosphere to increase the greenhouse effect.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/632170','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/632170"><span>Control of ventilation during intravenous <span class="hlt">CO</span><span class="hlt">2</span> loading in the awake dog.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Stremel, R W; Huntsman, D J; Casaburi, R; Whipp, B J; Wasserman, K</p> <p>1978-02-01</p> <p>The ventilatory response to venous <span class="hlt">CO</span><span class="hlt">2</span> loading and its effect on arterial <span class="hlt">CO</span><span class="hlt">2</span> tension was determined in five awake dogs. Blood, 200-500 ml/min, was diverted from a catheter in the right common carotid artery through a membrane gas <span class="hlt">exchanger</span> and returned to the right jugular vein. <span class="hlt">CO</span><span class="hlt">2</span> loading was accomplished by changing the gas ventilating the gas <span class="hlt">exchanger</span> from a mixture of 5% <span class="hlt">CO</span><span class="hlt">2</span> in <span class="hlt">air</span> to 100% <span class="hlt">CO</span><span class="hlt">2</span>. The ventilatory responses to this procedure were compared with those resulting from increased inspired <span class="hlt">CO</span><span class="hlt">2</span> concentrations (during which ventilation of the gas <span class="hlt">exchanger</span> with the <span class="hlt">air</span> and 5% <span class="hlt">CO</span><span class="hlt">2</span> mixture continued). The ventilatory response to each form of <span class="hlt">CO</span><span class="hlt">2</span> loading was computed as deltaVE/deltaPaco9. The mean ventilatory response to airway <span class="hlt">CO</span><span class="hlt">2</span> loading was 1.61 1/min per Torr Pa<span class="hlt">CO</span><span class="hlt">2</span>. The mean response for the venous <span class="hlt">CO</span><span class="hlt">2</span> loading was significantly higher and not significantly different from "infinite" <span class="hlt">CO</span><span class="hlt">2</span> sensitivity (i.e., isocapnic response). The results provide further evidence for a <span class="hlt">CO</span><span class="hlt">2</span>-linked hyperpnea, not mediated by significant changes in mean arterial PCO<span class="hlt">2</span>.</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/2015APS..MARS34010M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015APS..MARS34010M"><span>Energy requirements for <span class="hlt">CO</span><span class="hlt">2</span> capture from ambient <span class="hlt">air</span> (DAC) competitive with capture from flue-gas (PCC)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Meinrenken, Christoph</p> <p>2015-03-01</p> <p>Capture of <span class="hlt">CO</span><span class="hlt">2</span>, whether from a flue gas source (PCC) or from distributed sources via ambient <span class="hlt">air</span> (DAC), is a key enabling technology to provide carbon for sustainable synthetic energy carriers such as solar fuels. Based on thermodynamic minimum considerations, DAC is often expected to require about 3 times more energy (per ton <span class="hlt">CO</span><span class="hlt">2</span> captured) than PCC because <span class="hlt">CO</span><span class="hlt">2</span> in ambient <span class="hlt">air</span> is more dilute. Here, we calculate the energy required for a humidity swing-based DAC installation that uses an anionic <span class="hlt">exchange</span> resin as sorbent. The calculation uses recently measured equilibrium <span class="hlt">CO</span><span class="hlt">2</span> loadings of the sorbent as function of partial <span class="hlt">CO</span><span class="hlt">2</span> pressure, temperature, and humidity. We calculate the installation's electricity consumption to be about 45 kJ per mole of pure <span class="hlt">CO</span><span class="hlt">2</span> at 1 bar (scenario-dependent). Furthermore, we estimate the amount of heat provided by ambient <span class="hlt">air</span> and thus provide context of the overall energy and entropy balance and thermodynamic minimum views. The electricity consumption is competitive with typical parasitic loads of PCC-equipped coal-fired power plants (40-50 kJ per mole at same pressure) and significantly lower than predicted for other DAC installations such as Na(OH) sorbent-based systems. Our analyses elucidate why DAC is not always more energy-intensive that PCC, thus alleviating often cited concerns of significant cost impediments. Financial support by ABB for research presented herein is gratefully acknowledged.</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> flux 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/2014AGUFM.C11A0352L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.C11A0352L"><span>Radon and radium in the ice-covered Arctic Ocean, and what they reveal about gas <span class="hlt">exchange</span> in the <span class="hlt">sea</span> ice zone.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Loose, B.; Kelly, R. P.; Bigdeli, A.; Moran, S. B.</p> <p>2014-12-01</p> <p>The polar <span class="hlt">sea</span> ice zones are regions of high primary productivity and interior water mass formation. Consequently, the seasonal <span class="hlt">sea</span> ice cycle appears important to both the solubility and biological carbon pumps. To estimate net <span class="hlt">CO</span><span class="hlt">2</span> transfer in the <span class="hlt">sea</span> ice zone, we require accurate estimates of the <span class="hlt">air-sea</span> gas transfer velocity. In the open ocean, the gas transfer velocity is driven by wind, waves and bubbles - all of which are strongly altered by the presence of <span class="hlt">sea</span> ice, making it difficult to translate open ocean estimates of gas transfer to the ice zone. In this study, we present profiles of 222Rn and 226Ra throughout the mixed-layer and euphotic zone. Profiles were collected spanning a range of <span class="hlt">sea</span> ice cover conditions from 40 to 100%. The profiles of Rn/Ra can be used to estimate the gas transfer velocity, but the 3.8 day half-life of 222Rn implies that mixed layer radon will have a memory of the past ~20 days of gas <span class="hlt">exchange</span> forcing, which may include a range of <span class="hlt">sea</span> ice cover conditions. Here, we compare individual estimates of the gas transfer velocity to the turbulent forcing conditions constrained from shipboard and regional reanalysis data to more appropriately capture the time history upper ocean Rn/Ra.</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('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> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19820015568','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19820015568"><span>Size distribution of oceanic <span class="hlt">air</span> bubbles entrained in <span class="hlt">sea</span>-water by wave-breaking</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Resch, F.; Avellan, F.</p> <p>1982-01-01</p> <p>The size of oceanic <span class="hlt">air</span> bubbles produced by whitecaps and wave-breaking is determined. The production of liquid aerosols at the <span class="hlt">sea</span> surface is predicted. These liquid aerosols are at the origin of most of the particulate materials <span class="hlt">exchanged</span> between the ocean and the atmosphere. A prototype was designed and built using an optical technique based on the principle of light scattering at an angle of ninety degrees from the incident light beam. The output voltage is a direct function of the bubble diameter. Calibration of the probe was carried out within a range of 300 microns to 1.<span class="hlt">2</span> mm. Bubbles produced by wave-breaking in a large <span class="hlt">air-sea</span> interaction simulating facility. Experimental results are given in the form of size spectrum.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19770000092&hterms=Auxillary&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DAuxillary','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19770000092&hterms=Auxillary&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DAuxillary"><span>Removing <span class="hlt">CO</span><span class="hlt">2</span> and moisture from <span class="hlt">air</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Tepper, E. H.</p> <p>1977-01-01</p> <p>Foamed-aluminum blocks act as passive heat <span class="hlt">exchanger</span> to improve efficiency. Improved closed-cycle atmospheric scrubber, level of carbon dioxide, and water vapor are reduced without affecting temperature of airstream. <span class="hlt">Exchangers</span> draw impurities from <span class="hlt">air</span> without additional heaters of auxillary equipment.</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('https://www.ncbi.nlm.nih.gov/pubmed/12557667','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/12557667"><span>[Determination of net <span class="hlt">exchange</span> of <span class="hlt">CO</span><span class="hlt">2</span> between paddy fields and atmosphere with static poaque-chamber-based measurements].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zheng, Xunhua; Xu, Zhongjun; Wang, Yuesi; Han, Shenghui; Huang, Yao; Cai, Zucong; Zhu, Jianguo</p> <p>2002-10-01</p> <p>We firstly introduced the method for determining the net ecosystem <span class="hlt">exchange</span> fluxes of <span class="hlt">CO</span><span class="hlt">2</span> (NEE) between croplands and atmosphere, based on field measurements using static opaquechamber/gas chromatography methods was introduced, and the application of this method in the FACE (free-<span class="hlt">air</span> <span class="hlt">CO</span><span class="hlt">2</span> enrichment) study to examine the effects of elevated <span class="hlt">CO</span><span class="hlt">2</span> on the NEE over a typical paddy ecosystem was carried out, because of lacking in observation data for some necessary parameters, e.g., dark maintenance respiration coefficient, only the minimum value of NEE (NEEmin) was calculated based on opaque-chamber measurements. The NEEmin data indicate that <span class="hlt">CO</span><span class="hlt">2</span> elevated by 200 +/- 40 mumol.mol-1 significantly increased the ecosystem uptake of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> by a factor ca. 3. To accurately determine the NEE based on opaquechamber measurements, dark maintenance respiration coefficient, above-ground biomass and root: shoot, i.e. R:S, ratio of root to shoot should be observed over the whole growing season.</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('http://adsabs.harvard.edu/abs/2013PhDT.......178W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013PhDT.......178W"><span>Aqueous turbulence structure immediately adjacent to the <span class="hlt">air</span> - water interface and interfacial gas <span class="hlt">exchange</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Binbin</p> <p></p> <p><span class="hlt">Air-sea</span> interaction and the interfacial <span class="hlt">exchange</span> of gas across the <span class="hlt">air</span>-water interface are of great importance in coupled atmospheric-oceanic environmental systems. Aqueous turbulence structure immediately adjacent to the <span class="hlt">air</span>-water interface is the combined result of wind, surface waves, currents and other environmental forces and plays a key role in energy budgets, gas fluxes and hence the global climate system. However, the quantification of turbulence structure sufficiently close to the <span class="hlt">air</span>-water interface is extremely difficult. The physical relationship between interfacial gas <span class="hlt">exchange</span> and near surface turbulence remains insufficiently investigated. This dissertation aims to measure turbulence in situ in a complex environmental forcing system on Lake Michigan and to reveal the relationship between turbulent statistics and the <span class="hlt">CO</span><span class="hlt">2</span> flux across the <span class="hlt">air</span>-water interface. The major objective of this dissertation is to investigate the physical control of the interfacial gas <span class="hlt">exchange</span> and to provide a universal parameterization of gas transfer velocity from environmental factors, as well as to propose a mechanistic model for the global <span class="hlt">CO</span><span class="hlt">2</span> flux that can be applied in three dimensional climate-ocean models. Firstly, this dissertation presents an advanced measurement instrument, an in situ free floating Particle Image Velocimetry (FPIV) system, designed and developed to investigate the small scale turbulence structure immediately below the <span class="hlt">air</span>-water interface. Description of hardware components, design of the system, measurement theory, data analysis procedure and estimation of measurement error were provided. Secondly, with the FPIV system, statistics of small scale turbulence immediately below the <span class="hlt">air</span>-water interface were investigated under a variety of environmental conditions. One dimensional wave-number spectrum and structure function sufficiently close to the water surface were examined. The vertical profiles of turbulent dissipation rate were intensively studied</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1175556','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/1175556"><span><span class="hlt">Co</span>-flow anode/cathode supply heat <span class="hlt">exchanger</span> for a solid-oxide fuel cell assembly</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Haltiner, Jr., Karl J.; Kelly, Sean M.</p> <p>2005-11-22</p> <p>In a solid-oxide fuel cell assembly, a <span class="hlt">co</span>-flow heat <span class="hlt">exchanger</span> is provided in the flow paths of the reformate gas and the cathode <span class="hlt">air</span> ahead of the fuel cell stack, the reformate gas being on one side of the <span class="hlt">exchanger</span> and the cathode <span class="hlt">air</span> being on the other. The reformate gas is at a substantially higher temperature than is desired in the stack, and the cathode gas is substantially cooler than desired. In the <span class="hlt">co</span>-flow heat <span class="hlt">exchanger</span>, the temperatures of the reformate and cathode streams converge to nearly the same temperature at the outlet of the <span class="hlt">exchanger</span>. Preferably, the heat <span class="hlt">exchanger</span> is formed within an integrated component manifold (ICM) for a solid-oxide fuel cell assembly.</p> </li> <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://adsabs.harvard.edu/abs/2017DSRI..122...17M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017DSRI..122...17M"><span>The <span class="hlt">air-sea</span> <span class="hlt">exchange</span> of mercury in the low latitude Pacific and Atlantic Oceans</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mason, Robert P.; Hammerschmidt, Chad R.; Lamborg, Carl H.; Bowman, Katlin L.; Swarr, Gretchen J.; Shelley, Rachel U.</p> <p>2017-04-01</p> <p><span class="hlt">Air-sea</span> <span class="hlt">exchange</span> is an important component of the global mercury (Hg) cycle as it mediates the rate of increase in ocean Hg, and therefore the rate of change in levels of methylmercury (MeHg), the most toxic and bioaccumulative form of Hg in seafood and the driver of human health concerns. Gas evasion of elemental Hg (Hg0) from the ocean is an important sink for ocean Hg with previous studies suggesting that evasion is not uniform across ocean basins. To understand further the factors controlling Hg0 evasion, and its relationship to atmospheric Hg deposition, we made measurements of dissolved Hg0 (DHg0) in surface waters, along with measurements of Hg in precipitation and on aerosols, and Hg0 in marine <span class="hlt">air</span>, during two GEOTRACES cruises; GP16 in the equatorial South Pacific and GA03 in the North Atlantic. We contrast the concentrations and estimated evasion fluxes of Hg0 during these cruises, and the factors influencing this <span class="hlt">exchange</span>. Concentrations of DHg0 and fluxes were lower during the GP16 cruise than during the GA03 cruise, and likely reflect the lower atmospheric deposition in the South Pacific. An examination of Hg/Al ratios for aerosols from the cruises suggests that they were anthropogenically-enriched relative to crustal material, although to a lesser degree for the South Pacific than the aerosols over the North Atlantic. Both regions appear to be net sources of Hg0 to the atmosphere (evasion>deposition) and the reasons for this are discussed. Overall, the studies reported here provide further clarification on the factors controlling evasion of Hg0 from the ocean surface, and the role of anthropogenic inputs in influencing ocean Hg concentrations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22036791-bi-quadratic-interlayer-exchange-coupling-co-sub-mnsi-ag-co-sub-mnsi-pseudo-spin-valve','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22036791-bi-quadratic-interlayer-exchange-coupling-co-sub-mnsi-ag-co-sub-mnsi-pseudo-spin-valve"><span>Bi-quadratic interlayer <span class="hlt">exchange</span> coupling in <span class="hlt">Co</span>{sub <span class="hlt">2</span>}MnSi/Ag/<span class="hlt">Co</span>{sub <span class="hlt">2</span>}MnSi pseudo spin-valve</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>Goripati, Hari S.; Hono, K.; Graduate School of Pure and Applied Sciences, University of Tsukuba, Tsukuba 305-0047</p> <p>2011-12-15</p> <p>Bi-quadratic interlayer <span class="hlt">exchange</span> coupling is found below 100 K in a <span class="hlt">Co</span>{sub <span class="hlt">2</span>}MnSi/Ag/<span class="hlt">Co</span>{sub <span class="hlt">2</span>}MnSi current-perpendicular-to-plane pseudo spin valves. The bi-quadratic coupling constant J{sub <span class="hlt">2</span>} was estimated to be {approx}-0.30 erg/cm{sup <span class="hlt">2</span>} at 5 K and the strong temperature dependence of the coupling strength points its likely origin to the ''loose spin'' model. Application of current of {approx}<span class="hlt">2</span> x 10{sup 7} A/cm{sup <span class="hlt">2</span>} below 100 K leads to an increase in the magnetoresistance (MR), indicating current induced antiparallel alignment of the two magnetic layers. These results strongly suggest that the presence of the bi-quadratic interlayer <span class="hlt">exchange</span> coupling causes the reduction ofmore » the magnetoresistance at low temperature and illustrates the importance of understanding the influence of interlayer <span class="hlt">exchange</span> coupling on magnetization configuration in magnetic nanostructures.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.B21A0457G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.B21A0457G"><span>Towards a Better Understanding of the Oxygen Isotope Signature of Atmospheric <span class="hlt">CO</span><span class="hlt">2</span>: Determining the 18O-<span class="hlt">Exchange</span> Between <span class="hlt">CO</span><span class="hlt">2</span> and H<span class="hlt">2</span>O in Leaves and Soil On-line with Laser-Based Spectroscopy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gangi, L.; Rothfuss, Y.; Vereecken, H.; Brueggemann, N.</p> <p>2013-12-01</p> <p>The oxygen isotope signature of carbon dioxide (δ18O-<span class="hlt">CO</span><span class="hlt">2</span>) is a powerful tool to disentangle <span class="hlt">CO</span><span class="hlt">2</span> fluxes in terrestrial ecosystems, as <span class="hlt">CO</span><span class="hlt">2</span> attains a contrasting 18O signature by the interaction with isotopically different soil and leaf water pools during soil respiration and photosynthesis, respectively. However, using the δ18O-<span class="hlt">CO</span><span class="hlt">2</span> signal to quantify plant-soil-atmosphere <span class="hlt">CO</span><span class="hlt">2</span> fluxes is still challenging due to a lack of knowledge concerning the magnitude and effect of individual fractionation processes during <span class="hlt">CO</span><span class="hlt">2</span> and H<span class="hlt">2</span>O diffusion and during <span class="hlt">CO</span><span class="hlt">2</span>-H<span class="hlt">2</span>O isotopic <span class="hlt">exchange</span> in soils and leaves, especially related to short-term changes in environmental conditions (non-steady state). This study addresses this research gap by combined on-line monitoring of the oxygen isotopic signature of <span class="hlt">CO</span><span class="hlt">2</span> and water vapor during gas <span class="hlt">exchange</span> in soil and plant leaves with laser-based spectroscopy, using soil columns and plant chambers. In both experimental setups, the measured δ18O of water vapor was used to infer the δ18O of liquid water, and, together with the δ18O-<span class="hlt">CO</span><span class="hlt">2</span>, the degree of oxygen isotopic equilibrium between the two species (θ). Gas <span class="hlt">exchange</span> experiments with different functional plant types (C3 coniferous, C3 monocotyledonous, C3 dicotyledonous, C4) revealed that θ and the influence of the plant on the ambient δ18O-<span class="hlt">CO</span><span class="hlt">2</span> (<span class="hlt">CO</span>18O-isoforcing) not only varied on a diurnal timescale but also when plants were exposed to limited water availability, elevated <span class="hlt">air</span> temperature, and abrupt changes in light intensity (sunflecks). Maximum θ before treatments ranged between 0.7 and 0.8 for the C3 dicotyledonous (poplar) and C3 monocotyledonous (wheat) plants, and between 0.5 and 0.6 for the conifer (spruce) and C4 plant (maize) while maximum <span class="hlt">CO</span>18O-isoforcing was highest in wheat (0.03 m s-1 ‰), similar in poplar and maize (0.02 m s-1 ‰), and lowest in spruce (0.01 m s-1 ‰). Multiple regression analysis showed that up to 97 % of temporal dynamics in <span class="hlt">CO</span>18O-isoforcing could be</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhLA..381..524L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhLA..381..524L"><span>Modulated <span class="hlt">exchange</span> bias in NiFe/<span class="hlt">Co</span>O/α-Fe<span class="hlt">2</span>O3 trilayers and NiFe/<span class="hlt">Co</span>O bilayers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, X.; Lin, K.-W.; Yeh, W.-C.; Desautels, R. D.; van Lierop, J.; Pong, Philip W. T.</p> <p>2017-02-01</p> <p>While the <span class="hlt">exchange</span> bias in ferromagnetic/antiferromagnetic (FM/AF) bilayer and FM1/AF/FM<span class="hlt">2</span> trilayer configurations has been widely investigated, the role of an AF<span class="hlt">2</span> layer in FM/AF1/AF<span class="hlt">2</span> trilayer configurations is still not well understood. In this work, the magnetic properties of NiFe/<span class="hlt">Co</span>O, NiFe/α-Fe<span class="hlt">2</span>O3 bilayers, and NiFe/<span class="hlt">Co</span>O/α-Fe<span class="hlt">2</span>O3 trilayer were studied comparatively. The microstructure and chemical composition were characterized. Temperature dependent magnetometry reveals increased irreversibility temperature in NiFe/<span class="hlt">Co</span>O/α-Fe<span class="hlt">2</span>O3 trilayer compared with NiFe/<span class="hlt">Co</span>O bilayer. The magnetic hysteresis loops show that the <span class="hlt">exchange</span> bias (Hex) and coercivity (Hc) depend strongly on the anisotropy of AF layer (<span class="hlt">Co</span>O, α-Fe<span class="hlt">2</span>O3 and <span class="hlt">Co</span>O/α-Fe<span class="hlt">2</span>O3). Our work shows that the AF1/AF<span class="hlt">2</span> interfacial interactions can be used effectively for tuning the <span class="hlt">exchange</span> bias in FM/AF1/AF<span class="hlt">2</span> trilayers.</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> flux 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 fluxes (photosynthesis and calcification), <span class="hlt">air-sea</span> gas <span class="hlt">exchanges</span>, 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 <span class="hlt">exchange</span> 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 flux of DIC from neighboring grids is several times greater than local biological flux of DIC and is three orders of magnitude greater than the <span class="hlt">air-sea</span> gas flux 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/2015JGRC..120..716Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JGRC..120..716Z"><span>Typhoon <span class="hlt">air-sea</span> drag coefficient in coastal regions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhao, Zhong-Kuo; Liu, Chun-Xia; Li, Qi; Dai, Guang-Feng; Song, Qing-Tao; Lv, Wei-Hua</p> <p>2015-02-01</p> <p>The <span class="hlt">air-sea</span> drag during typhoon landfalls is investigated for a 10 m wind speed as high as U10 ≈ 42 m s-1, based on multilevel wind measurements from a coastal tower located in the South China <span class="hlt">Sea</span>. The drag coefficient (CD) plotted against the typhoon wind speed is similar to that of open ocean conditions; however, the CD curve shifts toward a regime of lower winds, and CD increases by a factor of approximately 0.5 relative to the open ocean. Our results indicate that the critical wind speed at which CD peaks is approximately 24 m s-1, which is 5-15 m s-1 lower than that from deep water. Shoaling effects are invoked to explain the findings. Based on our results, the proposed CD formulation, which depends on both water depth and wind speed, is applied to a typhoon forecast model. The forecasts of typhoon track and surface wind speed are improved. Therefore, a water-depth-dependence formulation of CD may be particularly pertinent for parameterizing <span class="hlt">air-sea</span> momentum <span class="hlt">exchanges</span> over shallow water.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1437530-dynamic-adsorption-co2-n2-cation-exchanged-chabazite-ssz-breakthrough-analysis','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1437530-dynamic-adsorption-co2-n2-cation-exchanged-chabazite-ssz-breakthrough-analysis"><span>Dynamic adsorption of <span class="hlt">CO</span><span class="hlt">2</span>/N<span class="hlt">2</span> on cation-<span class="hlt">exchanged</span> chabazite SSZ-13: A breakthrough analysis</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>Bower, Jamey K.; Barpaga, Dushyant; Prodinger, Sebastian</p> <p>2018-04-17</p> <p>Alkali <span class="hlt">exchanged</span> SSZ-13 adsorbents were investigated for their applicability in separating N<span class="hlt">2</span> from <span class="hlt">CO</span><span class="hlt">2</span> in flue gas streams using a dynamic breakthrough method. In contrast to IAST calculations based on equilibrium isotherms, K+ <span class="hlt">exchanged</span> SSZ-13 was found to yield the best N<span class="hlt">2</span> productivity under dynamic conditions where diffusion properties play a significant role. This was attributed to the selective, partial blockage of access to the CHA cavities enhancing the separation potential in a 15/85 <span class="hlt">CO</span><span class="hlt">2</span>/N<span class="hlt">2</span> binary gas mixture.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1437530-dynamic-adsorption-co2-cation-exchanged-chabazite-ssz-breakthrough-analysis','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1437530-dynamic-adsorption-co2-cation-exchanged-chabazite-ssz-breakthrough-analysis"><span>Dynamic Adsorption of <span class="hlt">CO</span> <span class="hlt">2</span> /N <span class="hlt">2</span> on Cation-<span class="hlt">Exchanged</span> Chabazite SSZ-13: A Breakthrough Analysis</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>Bower, Jamey K.; Barpaga, Dushyant; Prodinger, Sebastian</p> <p>2018-03-30</p> <p>Alkali <span class="hlt">exchanged</span> SSZ-13 adsorbents were investigated for their applicability in separating N<span class="hlt">2</span> from <span class="hlt">CO</span> <span class="hlt">2</span> in flue gas streams using a dynamic breakthrough method. In contrast to IAST calculations based on equilibrium isotherms, K+ <span class="hlt">exchanged</span> SSZ-13 was found to yield the best N<span class="hlt">2</span> productivity under dynamic conditions where diffusion properties play a significant role. This was attributed to the selective, partial blockage of access to the CHA cavities enhancing the separation potential in a 15/85 <span class="hlt">CO</span><span class="hlt">2</span>/N<span class="hlt">2</span> binary gas mixture.</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.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('https://www.osti.gov/biblio/1399837-fluidized-bed-heat-transfer-modeling-development-particle-supercritical-co2-heat-exchanger','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1399837-fluidized-bed-heat-transfer-modeling-development-particle-supercritical-co2-heat-exchanger"><span>Fluidized-Bed Heat Transfer Modeling for the Development of Particle/Supercritical-<span class="hlt">CO</span><span class="hlt">2</span> Heat <span class="hlt">Exchanger</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>Ma, Zhiwen; Martinek, Janna G</p> <p></p> <p>Concentrating solar power (CSP) technology is moving toward high-temperature and high-performance design. One technology approach is to explore high-temperature heat-transfer fluids and storage, integrated with a high-efficiency power cycle such as the supercritical carbon dioxide (s-<span class="hlt">CO</span><span class="hlt">2</span>) Brayton power cycle. The s-<span class="hlt">CO</span><span class="hlt">2</span> Brayton power system has great potential to enable the future CSP system to achieve high solar-to-electricity conversion efficiency and to reduce the cost of power generation. Solid particles have been proposed as a possible high-temperature heat-transfer medium that is inexpensive and stable at high temperatures above 1,000 degrees C. The particle/heat <span class="hlt">exchanger</span> provides a connection between the particles andmore » s-<span class="hlt">CO</span><span class="hlt">2</span> fluid in the emerging s-<span class="hlt">CO</span><span class="hlt">2</span> power cycles in order to meet CSP power-cycle performance targets of 50% thermal-to-electric efficiency, and dry cooling at an ambient temperature of 40 degrees C. The development goals for a particle/s-<span class="hlt">CO</span><span class="hlt">2</span> heat <span class="hlt">exchanger</span> are to heat s-<span class="hlt">CO</span><span class="hlt">2</span> to =720 degrees C and to use direct thermal storage with low-cost, stable solid particles. This paper presents heat-transfer modeling to inform the particle/s-<span class="hlt">CO</span><span class="hlt">2</span> heat-<span class="hlt">exchanger</span> design and assess design tradeoffs. The heat-transfer process was modeled based on a particle/s-<span class="hlt">CO</span><span class="hlt">2</span> counterflow configuration. Empirical heat-transfer correlations for the fluidized bed and s-<span class="hlt">CO</span><span class="hlt">2</span> were used in calculating the heat-transfer area and optimizing the tube layout. A <span class="hlt">2</span>-D computational fluid-dynamics simulation was applied for particle distribution and fluidization characterization. The operating conditions were studied from the heat-transfer analysis, and cost was estimated from the sizing of the heat <span class="hlt">exchanger</span>. The paper shows the path in achieving the cost and performance objectives for a heat-<span class="hlt">exchanger</span> design.« less</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/2015EGUGA..1713847C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1713847C"><span>Off-shore enhanced oil recovery in the north <span class="hlt">sea</span>: matching <span class="hlt">CO</span>_<span class="hlt">2</span> demand and supply given uncertain market conditions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Compernolle, Tine; Welkenhuysen, Kris; Huisman, Kuno; Piessens, Kris; Kort, Peter</p> <p>2015-04-01</p> <p>Introduction <span class="hlt">CO</span><span class="hlt">2</span> enhanced oil recovery (<span class="hlt">CO</span><span class="hlt">2</span>-EOR) entails the injection of <span class="hlt">CO</span><span class="hlt">2</span> in mature oil fields in order to mobilize the oil. In particular, the injected <span class="hlt">CO</span><span class="hlt">2</span> reduces the oil's viscosity and acts as a propellant, resulting in an increased oil extraction rate (Leach et al., 2011). Given uncertainty in both oil price and <span class="hlt">CO</span><span class="hlt">2</span> price under the EU ETS system, aim of this study is to analyze under which economic conditions a <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> can be established between a <span class="hlt">CO</span><span class="hlt">2</span> supplier (an electricity producer for whom <span class="hlt">CO</span><span class="hlt">2</span> is a by-product) and a <span class="hlt">CO</span><span class="hlt">2</span> user (an offshore oil company that exploits oil fields in the North <span class="hlt">Sea</span> and needs <span class="hlt">CO</span><span class="hlt">2</span> for enhanced oil recovery). Methodology A techno-economic simulation tool, PSS IV, was developed to provide investment decision support on integrated <span class="hlt">CO</span><span class="hlt">2</span>-EOR projects (Welkenhuysen et al., 2014). Until now, a fixed onshore supply of <span class="hlt">CO</span><span class="hlt">2</span> was presumed. An economic optimization model is now developed for both the <span class="hlt">CO</span><span class="hlt">2</span> producer and the <span class="hlt">CO</span><span class="hlt">2</span> user. Because net present value and discounted cash flow methods are inadequate to deal with issues like uncertainty and the irreversibility of an investment decision, the real options theory is applied (Dixit and Pindyck, 1994). The way in which cooperation between the companies can take place, will be studied using game theoretical concepts (Lukas and Welling, 2014). Economic and technical data on <span class="hlt">CO</span><span class="hlt">2</span> capture are available from the PSS database (Piessens et al., 2012). Data on EOR performance, <span class="hlt">CO</span><span class="hlt">2</span> requirements and various costs are taken from literature (BERR, 2007; Klokk et al., 2010; Pershad et al., 2012). Results/Findings It will be shown what the impact of price uncertainty is on the investment decision of the electricity producer to capture and sell <span class="hlt">CO</span><span class="hlt">2</span>, and on the decision of the oil producer to make the necessary investments to inject <span class="hlt">CO</span><span class="hlt">2</span> for enhanced oil recovery. Based on these results, it will be determined under which economic conditions a <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> and transport can take place. Furthermore, also the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JPhCS.908a2046X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JPhCS.908a2046X"><span>Functional design of heat <span class="hlt">exchange</span> for pneumatic vehicles</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xu, Z. G.; Yang, D. Y.; Shen, W. D.; Liu, T. T.</p> <p>2017-10-01</p> <p>With the increasingly serious environmental problems, especially the impact of fog and haze, the development of <span class="hlt">air</span> powered vehicles has become an important research direction of new energy vehicles. Quadrature test was done with different materials, i.e. stainless steel and aluminum alloy, at different inlet pressures, using different expansion gases, i.e. <span class="hlt">air</span>, <span class="hlt">CO</span><span class="hlt">2</span>, for heat <span class="hlt">exchanging</span> properties for pneumatic vehicles. The mathematics as well as simulation methods are used to analyze the different heat <span class="hlt">exchanging</span> effects in the multistage cylinder. The research results showed that the stainless steel has better effects in heat <span class="hlt">exchanging</span> than Aluminum Alloy; the intake pressure has little effect on <span class="hlt">CO</span><span class="hlt">2</span> than the <span class="hlt">air</span> in heat <span class="hlt">exchanging</span> effect. <span class="hlt">CO</span><span class="hlt">2</span> is better in heat <span class="hlt">exchanging</span> than <span class="hlt">air</span>.</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> Fluxes 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 fluxes (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/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 fluxes 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 fluxes, empirical relationships were developed to quantify the interfacial <span class="hlt">exchange</span> 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> fluxes 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 <span class="hlt">exchange</span>; 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> fluxes 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/2010AGUFM.B33J..01T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.B33J..01T"><span>Western Pacific <span class="hlt">Air-Sea</span> Interaction Study (W-PASS), Introduction and Highlights (Invited)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tsuda, A.</p> <p>2010-12-01</p> <p>Western Pacific <span class="hlt">Air-Sea</span> Interaction Study (W-PASS), Introduction and Highlights Atsushi Tsuda Atmosphere and Ocean Research Institute, The University of Tokyo In the western Pacific (WESTPAC) region, dust originating from Asian and Australian arid regions to the North and South Pacific, biomass burning emissions from the Southeast Asia to sub-tropical Pacific, and other anthropogenic substances are transported regionally and globally to affect cloud and rainfall patterns, <span class="hlt">air</span> quality, and radiative budgets downwind. Deposition of these compounds into the Asian marginal <span class="hlt">seas</span> and onto the Pacific Ocean influence surface primary productivity and species composition. In the WESTPAC region, subarctic, subtropical oceans and marginal <span class="hlt">seas</span> are located relatively narrow latitudinal range and these areas are influenced by the dust and anthropogenic inputs. Moreover, anthropogenic emission areas are located between the arid region and the oceans. The W-PASS (Western Pacific <span class="hlt">Air-Sea</span> interaction Study) project has been funded for 5 years as a part of SOLAS-Japan activity in the summer of 2006. We aim to resolve <span class="hlt">air-sea</span> interaction through field observation studies mainly using research vessels and island observatories over the western Pacific. We have carried out 5 cruises to the western North Pacific focusing on <span class="hlt">air-sea</span> interactions. Also, an intensive marine atmospheric observation including direct atmospheric deposition measurement was accomplished by a dozen W-PASS research groups at the NIES Atmospheric and Aerosol Monitoring Station of Cape Hedo in the northernmost tip of the Okinawa main Island facing the East China <span class="hlt">Sea</span> in the spring 2008. A few weak Kosa (dust) events, anthropogenic <span class="hlt">air</span> outflows, typical local <span class="hlt">air</span> and occupation of marine background <span class="hlt">air</span> were identified during the campaign period. The W-PASS has four research groups mainly focusing on VOC emissions, <span class="hlt">air-sea</span> gas <span class="hlt">exchange</span> processes, biogeochemical responses to dust depositions and its modeling. We also</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('http://www.ars.usda.gov/research/publications/publication/?seqNo115=333300','TEKTRAN'); return false;" href="http://www.ars.usda.gov/research/publications/publication/?seqNo115=333300"><span><span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> and evapotranspiration across dryland ecosystems of southwestern North America</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>Global-scale studies suggest that dryland ecosystems dominate an increasing trend in the magnitude and interannual variability of the land <span class="hlt">CO</span><span class="hlt">2</span> sink. However, such analyses are poorly constrained by measured <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> in drylands. Here we address this observation gap with eddy covariance data fr...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.3696L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.3696L"><span>How well does wind speed predict <span class="hlt">air-sea</span> gas transfer in the <span class="hlt">sea</span> ice zone? A synthesis of radon deficit profiles in the upper water column of the 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>Loose, B.; Kelly, R. P.; Bigdeli, A.; Williams, W.; Krishfield, R.; Rutgers van der Loeff, M.; Moran, S. B.</p> <p>2017-05-01</p> <p>We present 34 profiles of radon-deficit from the ice-ocean boundary layer of the Beaufort <span class="hlt">Sea</span>. Including these 34, there are presently 58 published radon-deficit estimates of <span class="hlt">air-sea</span> gas transfer velocity (k) in the Arctic Ocean; 52 of these estimates were derived from water covered by 10% <span class="hlt">sea</span> ice or more. The average value of k collected since 2011 is 4.0 ± 1.<span class="hlt">2</span> m d-1. This exceeds the quadratic wind speed prediction of weighted kws = <span class="hlt">2</span>.85 m d-1 with mean-weighted wind speed of 6.4 m s-1. We show how ice cover changes the mixed-layer radon budget, and yields an "effective gas transfer velocity." We use these 58 estimates to statistically evaluate the suitability of a wind speed parameterization for k, when the ocean surface is ice covered. Whereas the six profiles taken from the open ocean indicate a statistically good fit to wind speed parameterizations, the same parameterizations could not reproduce k from the <span class="hlt">sea</span> ice zone. We conclude that techniques for estimating k in the open ocean cannot be similarly applied to determine k in the presence of <span class="hlt">sea</span> ice. The magnitude of k through gaps in the ice may reach high values as ice cover increases, possibly as a result of focused turbulence dissipation at openings in the free surface. These 58 profiles are presently the most complete set of estimates of k across seasons and variable ice cover; as dissolved tracer budgets they reflect <span class="hlt">air-sea</span> gas <span class="hlt">exchange</span> with no impact from <span class="hlt">air</span>-ice gas <span class="hlt">exchange</span>.</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('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> fluxes 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 <span class="hlt">exchange</span> momentum, heat and freshwater. Mechanisms for the <span class="hlt">exchange</span> are wind stress, turbulent mixing, radiation, evaporation and precipitation. These surface fluxes 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> fluxes 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> fluxes 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> flux 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 flux 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> flux 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> fluxes. 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 flux? 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('https://www.ncbi.nlm.nih.gov/pubmed/25827140','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25827140"><span><span class="hlt">Air</span>-Seawater <span class="hlt">Exchange</span> of Organochlorine Pesticides along the Sediment Plume of a Large Contaminated River.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lin, Tian; Guo, Zhigang; Li, Yuanyuan; Nizzetto, Luca; Ma, Chuanliang; Chen, Yingjun</p> <p>2015-05-05</p> <p>Gaseous <span class="hlt">exchange</span> fluxes of organochlorine pesticides (OCPs) across the <span class="hlt">air</span>-water interface of the coastal East China <span class="hlt">Sea</span> were determined in order to assess whether the contaminated plume of the Yangtze River could be an important regional source of OCPs to the atmosphere. Hexachlorocyclohexanes (HCHs), chlordane compounds (CHLs), and dichlorodiphenyltrichloroethanes (DDTs) were the most frequently detected OCPs in <span class="hlt">air</span> and water. <span class="hlt">Air</span>-water <span class="hlt">exchange</span> was mainly characterized by net volatilization for all measured OCPs. The net gaseous <span class="hlt">exchange</span> flux ranged 10-240 ng/(m<span class="hlt">2</span>·day) for γ-HCH, 60-370 ng/(m<span class="hlt">2</span>·day) for trans-CHL, 97-410 ng/(m<span class="hlt">2</span>·day) for cis-CHL, and ∼0 (e.g., equilibrium) to 490 ng/(m<span class="hlt">2</span>·day) for p,p'-DDE. We found that the plume of the large contaminated river can serve as a significant regional secondary atmospheric source of legacy contaminants released in the catchment. In particular, the sediment plume represented the relevant source of DDT compounds (especially p,p'-DDE) sustaining net degassing when clean <span class="hlt">air</span> masses from the open ocean reached the plume area. In contrast, a mass balance showed that, for HCHs, contaminated river discharge (water and sediment) plumes were capable of sustaining volatilization throughout the year. These results demonstrate the inconsistencies in the fate of HCHs and DDTs in this large estuarine system with declining primary sources.</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> <span class="hlt">exchange</span> rate of the chamber. Photosynthetic photon flux (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/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 <span class="hlt">exchanges</span>, 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 <span class="hlt">exchanges</span>. 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 flux anomalies, while LR has negative correlation. For HR, we decompose lateral advective heat fluxes in the upper ocean into mean (slowly varying) and mesoscale-eddy (fast fluctuations) components. We find that the eddy flux divergence/convergence dominates the lateral advection and correlates well with the SST anomalies and <span class="hlt">air-sea</span> latent heat <span class="hlt">exchanges</span>. This result suggests that oceanic mesoscale advection supports warm SST anomalies that in turn feed surface heat flux. 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 flux convergence at submonthly time scales and have an identifiable imprint on surface turbulent heat flux, atmospheric circulation, and convective precipitation in the northwest portion of an averaged anticyclone.</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('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 flux <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 flux, 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 flux made from June to September (ii) Calculation of corresponding Gross Primary Productivity (GPP) and CH4 <span class="hlt">exchange</span> (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> </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/2017AGUFM.A51A2037B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A51A2037B"><span>Observational analysis of <span class="hlt">air-sea</span> fluxes 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> fluxes (momentum flux, sensible heat flux and latent heat flux) 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> fluxes and SWT at different depths. Seasonal and diurnal variations in <span class="hlt">air-sea</span> fluxes and SWT on different depths are examined. Results show that <span class="hlt">air-sea</span> fluxes 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> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.B23H0500W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.B23H0500W"><span>Measurements of Forest-Atmosphere Isotopic <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Exchange</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>Wehr, R. A.; Munger, J. W.; Nelson, D. D.; McManus, J. B.; Zahniser, M. S.; Saleska, S. R.</p> <p>2010-12-01</p> <p>Isotopic <span class="hlt">CO</span><span class="hlt">2</span> flux measurements are a promising means for partitioning the net ecosystem <span class="hlt">exchange</span> of <span class="hlt">CO</span><span class="hlt">2</span> into photosynthetic and respiratory components. This approach to partitioning is possible in principle because of the distinct isotopic signatures of respired and photosynthesized <span class="hlt">CO</span><span class="hlt">2</span>, but has been infeasible in practice—especially in forests—because of the difficulty of measuring isotopic ratios with sufficient precision and time response for use in eddy covariance (EC) flux calculations. Recent advances in laser spectroscopic instrumentation have changed that. We report measurements of isotopic (13C and 18O) <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> made by eddy covariance at Harvard Forest between April and December, 2010. The measurements were made using a continuous-wave quantum cascade laser spectrometer (Aerodyne Research Inc.) sampling at 4 Hz and are, to our knowledge, the first EC isotopic flux measurements at a forest site. The spectrometer can measure δ13C and δ18O with internal precisions (standard deviation of 1-minute averages) of 0.03 ‰, and [<span class="hlt">CO</span><span class="hlt">2</span>] with an internal precision of 15 ppb; the instrumental accuracy, calibration, and long-term stability are discussed in detail. The isotopic data are considered in relation to environmental variables (PAR, temperature, humidity, soil temperature and moisture), and a first attempt at flux partitioning using the isotopic fluxes is presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930032546&hterms=climate+exchange&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dclimate%2Bexchange','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930032546&hterms=climate+exchange&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dclimate%2Bexchange"><span>Biosphere/atmosphere <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> in tundra ecosystems - Community characteristics and relationships with multispectral surface reflectance</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Whiting, Gary J.; Bartlett, David S.; Fan, Song-Miao; Bakwin, Peter S.; Wofsy, Steven C.</p> <p>1992-01-01</p> <p><span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> rates were measured at selected tundra sites near Bethel, Alaska using portable, climate-controlled, instrumented enclosures. The empirically modeled <span class="hlt">exchange</span> rate for a representative area of vegetated tundra was 1.<span class="hlt">2</span> +/- 1.<span class="hlt">2</span> g/sq m/d, compared to a tower-measured <span class="hlt">exchange</span> over the same time period of 1.1 +.0- 1.<span class="hlt">2</span> g/sq m/d. Net <span class="hlt">exchange</span> in response to varying light levels was compared to wet meadow and dry upland tundra, and to the net <span class="hlt">exchange</span> measured by the micrometeoroidal tower technique. The multispectral reflectance properties of the sites were measured and related to <span class="hlt">exchange</span> rates in order to provide a quantitative foundation for the use of satellite remote sensing to monitor biosphere/atmosphere <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> in the tundra biome.</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/2010OcMod..31...28J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010OcMod..31...28J"><span>Tuning a physically-based model of the <span class="hlt">air-sea</span> gas transfer velocity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jeffery, C. D.; Robinson, I. S.; Woolf, D. K.</p> <p></p> <p><span class="hlt">Air-sea</span> gas transfer velocities are estimated for one year using a 1-D upper-ocean model (GOTM) and a modified version of the NOAA-COARE transfer velocity parameterization. Tuning parameters are evaluated with the aim of bringing the physically based NOAA-COARE parameterization in line with current estimates, based on simple wind-speed dependent models derived from bomb-radiocarbon inventories and deliberate tracer release experiments. We suggest that A = 1.3 and B = 1.0, for the sub-layer scaling parameter and the bubble mediated <span class="hlt">exchange</span>, respectively, are consistent with the global average <span class="hlt">CO</span> <span class="hlt">2</span> transfer velocity k. Using these parameters and a simple <span class="hlt">2</span>nd order polynomial approximation, with respect to wind speed, we estimate a global annual average k for <span class="hlt">CO</span> <span class="hlt">2</span> of 16.4 ± 5.6 cm h -1 when using global mean winds of 6.89 m s -1 from the NCEP/NCAR Reanalysis 1 1954-2000. The tuned model can be used to predict the transfer velocity of any gas, with appropriate treatment of the dependence on molecular properties including the strong solubility dependence of bubble-mediated transfer. For example, an initial estimate of the global average transfer velocity of DMS (a relatively soluble gas) is only 11.9 cm h -1 whilst for less soluble methane the estimate is 18.0 cm h -1.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AtmRe.196...62S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AtmRe.196...62S"><span>Intense <span class="hlt">air-sea</span> <span class="hlt">exchanges</span> and heavy orographic precipitation over Italy: The role of Adriatic <span class="hlt">sea</span> surface temperature uncertainty</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stocchi, Paolo; Davolio, Silvio</p> <p>2017-11-01</p> <p>Strong and persistent low-level winds blowing over the Adriatic basin are often associated with intense precipitation events over Italy. Typically, in case of moist southeasterly wind (Sirocco), rainfall affects northeastern Italy and the Alpine chain, while with cold northeasterly currents (Bora) precipitations are localized along the eastern slopes of the Apennines and central Italy coastal areas. These events are favoured by intense <span class="hlt">air-sea</span> interactions and it is reasonable to hypothesize that the Adriatic <span class="hlt">sea</span> surface temperature (SST) can affect the amount and location of precipitation. High-resolution simulations of different Bora and Sirocco events leading to severe precipitation are performed using a convection-permitting model (MOLOCH). Sensitivity experiments varying the SST initialization field are performed with the aim of evaluating the impact of SST uncertainty on precipitation forecasts, which is a relevant topic for operational weather predictions, especially at local scales. Moreover, diagnostic tools to compute water vapour fluxes across the Italian coast and atmospheric water budget over the Adriatic <span class="hlt">Sea</span> have been developed and applied in order to characterize the <span class="hlt">air</span> mass that feeds the precipitating systems. Finally, the investigation of the processes through which the SST influences location and intensity of heavy precipitation allows to gain a better understanding on mechanisms conducive to severe weather in the Mediterranean area and in the Adriatic basin in particular. Results show that the effect of the Adriatic SST (uncertainty) on precipitation is complex and can vary considerably among different events. For both Bora and Sirocco events, SST does not influence markedly the atmospheric water budget or the degree of moistening of <span class="hlt">air</span> that flows over the Adriatic <span class="hlt">Sea</span>. SST mainly affects the stability of the atmospheric boundary layer, thus influencing the flow dynamics and the orographic flow regime, and in turn, the precipitation pattern.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/18959327','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/18959327"><span>Sensitivity of mesquite shrubland <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> to precipitation in contrasting landscape settings.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Potts, Daniel L; Scott, Russell L; Cable, Jessica M; Huxman, Travis E; Williams, David G</p> <p>2008-10-01</p> <p>In semiarid ecosystems, physiography (landscape setting) may interact with woody-plant and soil microbe communities to constrain seasonal <span class="hlt">exchanges</span> of material and energy at the ecosystem scale. In an upland and riparian shrubland, we examined the seasonally dynamic linkage between ecosystem <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span>, woody-plant water status and photosynthesis, and soil respiration responses to summer rainfall. At each site, we compared tower-based measurements of net ecosystem <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> (NEE) with ecophysiological measurements among velvet mesquite (Prosopis velutina Woot.) in three size classes and soil respiration in sub-canopy and inter-canopy micro-sites. Monsoonal rainfall influenced a greater shift in the magnitude of ecosystem <span class="hlt">CO</span><span class="hlt">2</span> assimilation in the upland shrubland than in the riparian shrubland. Mesquite water status and photosynthetic gas <span class="hlt">exchange</span> were closely linked to the onset of the North American monsoon in the upland shrubland. In contrast, the presence of shallow alluvial groundwater in the riparian shrubland caused larger size classes of mesquite to be physiologically insensitive to monsoonal rains. In both shrublands, soil respiration was greatest beneath mesquite canopies and was coupled to shallow soil moisture abundance. Physiography, through its constraint on the physiological sensitivity of deeply rooted woody plants, may interact with plant-mediated rates of soil respiration to affect the sensitivity of semiarid-ecosystem carbon <span class="hlt">exchange</span> in response to episodic rainfall.</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('https://www.ncbi.nlm.nih.gov/pubmed/23630324','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23630324"><span>Influence of temperature on measurements of the <span class="hlt">CO</span><span class="hlt">2</span> compensation point: differences between the Laisk and O<span class="hlt">2</span>-<span class="hlt">exchange</span> methods.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Walker, Berkley J; Cousins, Asaph B</p> <p>2013-04-01</p> <p>The <span class="hlt">CO</span><span class="hlt">2</span> compensation point in the absence of day respiration (Γ*) is a key parameter for modelling leaf <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span>. Γ* links the kinetics of ribulose-1,5-bisphosphate carboxylase-oxygenase (Rubisco) with the stoichiometry of <span class="hlt">CO</span><span class="hlt">2</span> released per Rubisco oxygenation from photorespiration (α), two essential components of biochemical models of photosynthesis. There are two main gas-<span class="hlt">exchange</span> methods for measuring Γ*: (i) the Laisk method, which requires estimates of mesophyll conductance to <span class="hlt">CO</span><span class="hlt">2</span> (g m) and (ii) measurements of O<span class="hlt">2</span> isotope <span class="hlt">exchange</span>, which assume constant values of α and a fixed stoichiometry between O<span class="hlt">2</span> uptake and Rubisco oxygenation. In this study, the temperature response of Γ* measured using the Laisk and O<span class="hlt">2</span>-<span class="hlt">exchange</span> methods was compared under ambient (25 °C) and elevated (35 °C) temperatures to determine whether both methods yielded similar results. Previously published temperature responses of Γ* estimated with the Laisk and O<span class="hlt">2</span>-<span class="hlt">exchange</span> methods in Nicotiana tabacum demonstrated that the Laisk-derived model of Γ* was more sensitive to temperature compared with the O<span class="hlt">2</span>-<span class="hlt">exchange</span> model. Measurements in Arabidopsis thaliana indicated that the Laisk and O<span class="hlt">2</span>-<span class="hlt">exchange</span> methods produced similar Γ* at 25 °C; however, Γ* values from O<span class="hlt">2</span> <span class="hlt">exchange</span> were lower at 35 °C compared with the Laisk method. Compared with a photorespiratory mutant (pmdh1pmdh<span class="hlt">2</span>hpr) with increased α, wild-type (WT) plants had lower Laisk values of Γ* at 25 °C but were not significantly different at 35 °C. These differences between Laisk and O<span class="hlt">2</span> <span class="hlt">exchange</span> values of Γ* at 35 °C could be explained by temperature sensitivity of α in WT and/or errors in the assumptions of O<span class="hlt">2</span> <span class="hlt">exchange</span>. The differences between Γ* measured using the Laisk and O<span class="hlt">2</span>-<span class="hlt">exchange</span> method with temperature demonstrate that assumptions used to measure Γ*, and possibly the species-specific validity of these assumptions, need to be considered when modelling the temperature response of photosynthesis.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C31D..01L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C31D..01L"><span>Gas <span class="hlt">exchange</span> in the ice zone: the role of small waves and big animals</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Loose, B.; Takahashi, A.; Bigdeli, A.</p> <p>2016-12-01</p> <p>The balance of <span class="hlt">air-sea</span> gas <span class="hlt">exchange</span> and net biological carbon fixation determine the transport and transformation of carbon dioxide and methane in the ocean. <span class="hlt">Air-sea</span> gas <span class="hlt">exchange</span> is mostly driven by upper ocean physics, but biology can also play a role. In the open ocean, gas <span class="hlt">exchange</span> increases proportionate to the square of wind speed. When <span class="hlt">sea</span> ice is present, this dependence breaks down in part because breaking waves and <span class="hlt">air</span> bubble entrainment are damped out by interactions between <span class="hlt">sea</span> ice and the wave field. At the same time, <span class="hlt">sea</span> ice motions, formation, melt, and even <span class="hlt">sea</span> ice-associated organisms can act to introduce turbulence and <span class="hlt">air</span> bubbles into the upper ocean, thereby enhancing <span class="hlt">air-sea</span> gas <span class="hlt">exchange</span>. We take advantage of the knowledge advances of upper ocean physics including bubble dynamics to formulate a model for <span class="hlt">air-sea</span> gas <span class="hlt">exchange</span> in the <span class="hlt">sea</span> ice zone. Here, we use the model to examine the role of small-scale waves and diving animals that trap <span class="hlt">air</span> for insulation, including penguins, seals and polar bears. We compare these processes to existing parameterizations of wave and bubble dynamics in the open ocean, to observe how <span class="hlt">sea</span> ice both mitigates and locally enhances <span class="hlt">air-sea</span> gas transfer.</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('http://adsabs.harvard.edu/abs/2018MRE.....5c5029M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018MRE.....5c5029M"><span>Large <span class="hlt">exchange</span> bias effect in NiFe<span class="hlt">2</span>O4/<span class="hlt">Co</span>O nanocomposites</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mohan, Rajendra; Prasad Ghosh, Mritunjoy; Mukherjee, Samrat</p> <p>2018-03-01</p> <p>In this work, we report the <span class="hlt">exchange</span> bias effect of NiFe<span class="hlt">2</span>O4/<span class="hlt">Co</span>O nanocomposites, synthesized via chemical <span class="hlt">co</span>-precipitation method. Four samples of different particle size ranging from 4 nm to 31 nm were prepared with the annealing temperature varying from 200 °C to 800 °C. X-ray diffraction analysis of all the samples confirmed the presence of cubic spinel phase of Nickel ferrite along with <span class="hlt">Co</span>O phase without trace of any impurity. Sizes of the particles were studied from transmission electron micrographs and were found to be in agreement with those estimated from x-ray diffraction. Field cooled (FC) hysteresis loops at 5 K revealed an <span class="hlt">exchange</span> bias (HE) of <span class="hlt">2.2</span> kOe for the sample heated at 200 °C which decreased with the increase of particle size. <span class="hlt">Exchange</span> bias expectedly vanished at 300 K due to high thermal energy (kBT) and low effective surface anisotropy. M-T curves revealed a blocking temperature of 135 K for the sample with smaller particle size.</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> flux 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 fluxes 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 <span class="hlt">exchange</span> 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/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/2012EGUGA..14.5028O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..14.5028O"><span>Modeling approaches to describe H<span class="hlt">2</span>O and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> in mare ecosystems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Olchev, A.; Novenko, E.; Volkova, E.</p> <p>2012-04-01</p> <p>The modern climatic conditions is strongly influenced by both internal variability of climatic system, and various external natural and anthropogenic factors (IPCC 2007). Significant increase of concentration of greenhouse gases in the atmosphere and especially the growth of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> due to human activity are considered as the main factors that are responsible for global warming and climate changes. A significant part of anthropogenic <span class="hlt">CO</span><span class="hlt">2</span> is absorbed from the atmosphere by land biota and especially by vegetation cover. However, it is still not completely clear what is the role of different land ecosystems and especially forests and mares in global cycles of H<span class="hlt">2</span>O and <span class="hlt">CO</span><span class="hlt">2</span> and what is a sensitivity of these ecosystems to climate changes. Within the frameworks of this study the spatial and temporal variability of H<span class="hlt">2</span>O and <span class="hlt">CO</span><span class="hlt">2</span> fluxes in different types of mare ecosystems of the forest-steppe zone in European part of Russia was described using modeling approaches and results of field measurements. For this modeling and experimental study the mare ecosystems of Tula region were selected. The Tula region is located mostly in the forest-steppe zone and it is unique area for such studies because almost all existed types of mare ecosystems of Northern Eurasia distinguished by a geomorphological position, water and mineral supply can be found there. Most mares in Tula region have a relatively small size and surrounded by very heterogeneous forests that make not possible an application of the classical measuring and modeling approaches e.g. an eddy covariance technique or one-dimensional H<span class="hlt">2</span>O and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> models for flux estimation in such sites. In our study to describe the radiation, sensible heat, H<span class="hlt">2</span>O and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> between such heterogeneous mare ecosystems and the atmosphere a three-dimensional model Forbog-3D and one-dimensional Mixfor-SVAT were applied. The main concept used in the Forbog-3D and Mixfor-SVAT models is an aggregated description of physical and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29593081','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29593081"><span>Cuticular gas <span class="hlt">exchange</span> by Antarctic <span class="hlt">sea</span> spiders.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lane, Steven J; Moran, Amy L; Shishido, Caitlin M; Tobalske, Bret W; Woods, H Arthur</p> <p>2018-04-25</p> <p>Many marine organisms and life stages lack specialized respiratory structures, like gills, and rely instead on cutaneous respiration, which they facilitate by having thin integuments. This respiratory mode may limit body size, especially if the integument also functions in support or locomotion. Pycnogonids, or <span class="hlt">sea</span> spiders, are marine arthropods that lack gills and rely on cutaneous respiration but still grow to large sizes. Their cuticle contains pores, which may play a role in gas <span class="hlt">exchange</span>. Here, we examined alternative paths of gas <span class="hlt">exchange</span> in <span class="hlt">sea</span> spiders: (1) oxygen diffuses across pores in the cuticle, a common mechanism in terrestrial eggshells, (<span class="hlt">2</span>) oxygen diffuses directly across the cuticle, a common mechanism in small aquatic insects, or (3) oxygen diffuses across both pores and cuticle. We examined these possibilities by modeling diffusive oxygen fluxes across all pores in the body of <span class="hlt">sea</span> spiders and asking whether those fluxes differed from measured metabolic rates. We estimated fluxes across pores using Fick's law parameterized with measurements of pore morphology and oxygen gradients. Modeled oxygen fluxes through pores closely matched oxygen consumption across a range of body sizes, which means the pores facilitate oxygen diffusion. Furthermore, pore volume scaled hypermetrically with body size, which helps larger species facilitate greater diffusive oxygen fluxes across their cuticle. This likely presents a functional trade-off between gas <span class="hlt">exchange</span> and structural support, in which the cuticle must be thick enough to prevent buckling due to external forces but porous enough to allow sufficient gas <span class="hlt">exchange</span>. © 2018. Published by The Company of Biologists Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JGRC..121.7495L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JGRC..121.7495L"><span>Vernal distribution and turnover of dimethylsulfide (DMS) in the surface water of the Yellow <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, Cheng-Xuan; Yang, Gui-Peng; Wang, Bao-Dong; Xu, Zong-Jun</p> <p>2016-10-01</p> <p>The spatial and interannual variations of dimethylsulfide (DMS) and its precursors, dissolved and particulate dimethylsulfoniopropionate (DMSP), were discussed on the basis of field observations in the surface waters of the Yellow <span class="hlt">Sea</span> during spring 2007. Maxima of dimethylated sulfur compounds and low chlorophyll a concentrations were found in the central southern Yellow <span class="hlt">Sea</span>, whereas low concentrations of DMS and DMSP were detected at the boundary between the northern and southern parts of the Yellow <span class="hlt">Sea</span>. This frontal region is influenced by active water currents, <span class="hlt">air-sea</span> interface <span class="hlt">exchanges</span>, and biological turnover. The horizontal variations in DMS production and consumption rates showed a decreasing tendency from the coastal to offshore areas mainly due to the complicated biological features. DMS positively correlated with dissolved CH4 and <span class="hlt">CO</span><span class="hlt">2</span> but negatively correlated with nutrients (nitrite and phosphate). Particulate DMSP concentrations and DMS production rates positively correlated with dinoflagellate abundances but negatively correlated with diatom cell densities. DMS and DMSP concentrations, as well as DMS production and consumption rates, exhibited approximately <span class="hlt">2.0-2</span>.8 fold increases from 2005 to 2012. This finding was likely caused by shifts in the phytoplankton communities from diatoms to dinoflagellates and the increases in abundances of zooplankton and bacteria. Average <span class="hlt">sea-to-air</span> DMS fluxes were estimated to be 8.12 ± 1.24 µmol·(m-<span class="hlt">2</span>·d-1), and DMS microbial consumption was approximately 1.68 times faster than the DMS <span class="hlt">sea-air</span> <span class="hlt">exchange</span>. These findings imply that biological consumption, relative to ventilation, is a predominant mechanism in DMS removal from the surface water.</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> fluxes 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> fluxes 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> fluxes. 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> fluxes 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://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> flux 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('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> fluxes 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> </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/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> <span class="hlt">exchange</span> 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 flux, the <span class="hlt">sea</span>-spray-mediated heat flux, and a combination of the former two processes with the <span class="hlt">sea</span>-spray-mediated momentum flux 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 fluxes are applied in conjunction with the <span class="hlt">sea</span>-state-dependent momentum flux, they result in a slightly weaker TC, albeit stronger compared to the control simulation. However, when a spray-mediated momentum flux is applied together with spray heat fluxes, 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('https://www.ncbi.nlm.nih.gov/pubmed/28795814','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28795814"><span>Anion-<span class="hlt">Exchange</span> Membrane Fuel Cells with Improved <span class="hlt">CO</span><span class="hlt">2</span> Tolerance: Impact of Chemically Induced Bicarbonate Ion Consumption.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Katayama, Yu; Yamauchi, Kosuke; Hayashi, Kohei; Okanishi, Takeou; Muroyama, Hiroki; Matsui, Toshiaki; Kikkawa, Yuuki; Negishi, Takayuki; Watanabe, Shin; Isomura, Takenori; Eguchi, Koichi</p> <p>2017-08-30</p> <p>Over the last few decades, because of the significant development of anion <span class="hlt">exchange</span> membranes, increasing efforts have been devoted the realization of anion <span class="hlt">exchange</span> membrane fuel cells (AEMFCs) that operate with the supply of hydrogen generated on-site. In this paper, ammonia was selected as a hydrogen source, following which the effect of conceivable impurities, unreacted NH 3 and atmospheric <span class="hlt">CO</span> <span class="hlt">2</span> , on the performance of AEMFCs was established. As expected, we show that these impurities worsen the performance of AEMFCs significantly. Furthermore, with the help of in situ attenuated total reflection infrared (ATR-IR) spectroscopy, it was revealed that the degradation of the cell performance was primarily due to the inhibition of the hydrogen oxidation reaction (HOR). This is attributed to the active site occupation by <span class="hlt">CO</span>-related adspecies derived from (bi)carbonate adspecies. Interestingly, this degradation in the HOR activity is suppressed in the presence of both NH 3 and HCO 3 - because of the bicarbonate ion consumption reaction induced by the existence of NH 3 . Further analysis using in situ ATR-IR and electrochemical methods revealed that the poisonous <span class="hlt">CO</span>-related adspecies were completely removed under NH 3 -HCO 3 - conditions, accompanied by the improvement in HOR activity. Finally, a fuel cell test was conducted by using the practical AEMFC with the supply of NH 3 -contained H <span class="hlt">2</span> gas to the anode and ambient <span class="hlt">air</span> to the cathode. The result confirmed the validity of this positive effect of NH 3 -HCO 3 - coexistence on <span class="hlt">CO</span> <span class="hlt">2</span> -tolerence of AEMFCs. The cell performance achieved nearly 95% of that without any impurity in the fuels. These results clearly show the impact of the chemically induced bicarbonate ion consumption reaction on the realization of highly <span class="hlt">CO</span> <span class="hlt">2</span> -tolerent AEMFCs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20100032897&hterms=nz&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dnz','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20100032897&hterms=nz&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dnz"><span>Validation of <span class="hlt">AIRS</span> Retrievals of <span class="hlt">CO</span><span class="hlt">2</span> via Comparison to In Situ Measurements</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Olsen, Edward T.; Chahine, Moustafa T.; Chen, Luke L.; Jiang, Xun; Pagano, Thomas S.; Yung, Yuk L.</p> <p>2008-01-01</p> <p>Topics include <span class="hlt">AIRS</span> on Aqua, 2002-present with discussion about continued operation to 2011 and beyond and background, including spectrum, weighting functions, and initialization; comparison with aircraft and FTIR measurements in Masueda (CONTRAIL) JAL flask measurements, Park Falls, WI FTIR, Bremen, GDF, and Spitsbergen, Norway; <span class="hlt">AIRS</span> retrievals over addition FTIR sites in Darwin, AU and Lauder, NZ; and mid-tropospheric carbon dioxide weather and contribution from major surface sources. Slide titles include typical <span class="hlt">AIRS</span> infrared spectrum, <span class="hlt">AIRS</span> sensitivity for retrieving <span class="hlt">CO</span><span class="hlt">2</span> profiles, independence of <span class="hlt">CO</span><span class="hlt">2</span> solution with respect to the initial guess, available in situ measurements for validation and comparison, comparison of collocated V1.5x <span class="hlt">AIRS</span> <span class="hlt">CO</span><span class="hlt">2</span> (N_coll greater than or equal to 9) with INTEX-NA and SPURT;</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26359720','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26359720"><span>Different Apparent Gas <span class="hlt">Exchange</span> Coefficients for <span class="hlt">CO</span><span class="hlt">2</span> and CH4: Comparing a Brown-Water and a Clear-Water Lake in the Boreal Zone during the Whole Growing Season.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Rantakari, Miitta; Heiskanen, Jouni; Mammarella, Ivan; Tulonen, Tiina; Linnaluoma, Jessica; Kankaala, Paula; Ojala, Anne</p> <p>2015-10-06</p> <p>The <span class="hlt">air</span>-water <span class="hlt">exchange</span> of carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) and methane (CH4) is a central process during attempts to establish carbon budgets for lakes and landscapes containing lakes. Lake-atmosphere diffusive gas <span class="hlt">exchange</span> is dependent on the concentration gradient between <span class="hlt">air</span> and surface water and also on the gas transfer velocity, often described with the gas transfer coefficient k. We used the floating-chamber method in connection with surface water gas concentration measurements to estimate the gas transfer velocity of <span class="hlt">CO</span><span class="hlt">2</span> (k<span class="hlt">CO</span><span class="hlt">2</span>) and CH4 (kCH4) weekly throughout the entire growing season in two contrasting boreal lakes, a humic oligotrophic lake and a clear-water productive lake, in order to investigate the earlier observed differences between k<span class="hlt">CO</span><span class="hlt">2</span> and kCH4. We found that the seasonally averaged gas transfer velocity of CH4 was the same for both lakes. When the lakes were sources of <span class="hlt">CO</span><span class="hlt">2</span>, the gas transfer velocity of <span class="hlt">CO</span><span class="hlt">2</span> was also similar between the two study lakes. The gas transfer velocity of CH4 was constantly higher than that of <span class="hlt">CO</span><span class="hlt">2</span> in both lakes, a result also found in other studies but for reasons not yet fully understood. We found no differences between the lakes, demonstrating that the difference between k<span class="hlt">CO</span><span class="hlt">2</span> and kCH4 is not dependent on season or the characteristics of the lake.</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 Flux</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/2017AGUFM.A13L..03H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A13L..03H"><span>Assessing the influence of regional transport from Mainland China over the Korean Peninsula during the 2016 KORUS-AQ Field Campaign with <span class="hlt">CO/CO</span><span class="hlt">2</span> ratios</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Halliday, H. S.; DiGangi, J. P.; Diskin, G. S.; Choi, Y.; Pusede, S.; Rana, M.; Nowak, J. B.</p> <p>2017-12-01</p> <p>The industrial growth in East Asia has resulted in widespread growth and prosperity, but has been accompanied by degraded <span class="hlt">air</span> quality. These poor <span class="hlt">air</span> quality events have both local and regional effects, and long range transportation of pollution can greatly increase the affected populations. South Korea has a technologically oriented economy with vibrant urban regions, but suffers from poor <span class="hlt">air</span> quality arising from both local emissions on the Korean peninsula and from the transport of pollution from Mainland China. The KORUS-AQ field campaign was an international collaboration to characterize and understand the <span class="hlt">air</span> quality over the Korean peninsula in the spring of 2016. We use the aircraft in situ data from the DC-8 aircraft to examine trace gas ratios over three major analysis regions: the Seoul Metropolitan region, the South Korean peninsula, and the West <span class="hlt">Sea</span> (Yellow <span class="hlt">Sea</span>). We look specifically at the correlations between <span class="hlt">CO</span> and <span class="hlt">CO</span><span class="hlt">2</span> as an indicator of emissions type, with low ratios generally indicative of more efficient combustion and high emission ratios indicating low efficiency combustion. At low altitudes, higher incidences of low <span class="hlt">CO/CO</span><span class="hlt">2</span> ratios were observed in the Seoul and Peninsula regions, compared to higher ratios of <span class="hlt">CO/CO</span><span class="hlt">2</span> over the West <span class="hlt">Sea</span>. We examine the meteorological dependence of these carbon species ratios, their relationships to VOC tracers, and their vertical behavior to evaluate the <span class="hlt">air</span> mass contributions from Mainland China and assess the percentage contributions of these regional emissions to the measurements over the Korean Peninsula.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16661912','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16661912"><span>Crassulacean Acid Metabolism in the Epiphyte Tillandsia usneoides L. (Spanish Moss) : RESPONSES OF <span class="hlt">CO</span>(<span class="hlt">2</span>) <span class="hlt">EXCHANGE</span> TO CONTROLLED ENVIRONMENTAL CONDITIONS.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Martin, C E; Siedow, J N</p> <p>1981-08-01</p> <p>Patterns of <span class="hlt">CO</span>(<span class="hlt">2</span>) <span class="hlt">exchange</span> in Spanish moss under various experimental conditions were measured using an infrared gas analysis system. Plants were collected from a study site in North Carolina and placed in a gas <span class="hlt">exchange</span> chamber for several days of continuous measurements. No substantial seasonal effects on <span class="hlt">CO</span>(<span class="hlt">2</span>) <span class="hlt">exchange</span> were observed. High rates of nocturnal <span class="hlt">CO</span>(<span class="hlt">2</span>) uptake were observed under day/night temperature regimes of 25/10, 25/15, 25/20, 30/20, and 35/20 C; however, daytime temperatures of 40 C eliminated nighttime <span class="hlt">CO</span>(<span class="hlt">2</span>) uptake and a nighttime temperature of 5 C eliminated nocturnal <span class="hlt">CO</span>(<span class="hlt">2</span>) uptake, regardless of day temperature. Constant chamber conditions also inhibited nocturnal <span class="hlt">CO</span>(<span class="hlt">2</span>) uptake. Constant high relative humidity (RH) slightly stimulated <span class="hlt">CO</span>(<span class="hlt">2</span>) uptake while low nighttime RH reduced nocturnal <span class="hlt">CO</span>(<span class="hlt">2</span>) uptake.Reductions in daytime irradiance to approximately 25% full sunlight had no effect on <span class="hlt">CO</span>(<span class="hlt">2</span>) <span class="hlt">exchange</span>. Continuous darkness resulted in continuous <span class="hlt">CO</span>(<span class="hlt">2</span>) loss by the plants, but a <span class="hlt">CO</span>(<span class="hlt">2</span>) <span class="hlt">exchange</span> pattern similar to normal day/night conditions was observed under constant illumination. High tissue water content inhibited <span class="hlt">CO</span>(<span class="hlt">2</span>) uptake. Wetting of the tissue at any time of day or night resulted in net <span class="hlt">CO</span>(<span class="hlt">2</span>) loss. Abrupt increases in temperature or decreases in RH resulted in sharp decreases in net <span class="hlt">CO</span>(<span class="hlt">2</span>) uptake.The results indicate that Spanish moss is tolerant of a wide range of temperatures, irradiances, and water contents. They also indicate that high nighttime RH is a prerequisite for high rates of <span class="hlt">CO</span>(<span class="hlt">2</span>) uptake.</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 fluxes 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 flux 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 fluxes 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 fluxes 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 fluxes 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 flux detection limits than the LGR. The hourly flux 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> flux as reference, we estimate that the Picarro and LGR can resolve hourly <span class="hlt">CO</span><span class="hlt">2</span> fluxes from roughly 40 and 4 % of the world's oceans respectively. Averaging over longer timescales would be required in regions with smaller fluxes. Hourly flux 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('https://www.ncbi.nlm.nih.gov/pubmed/29714795','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29714795"><span>Humidity-swing mechanism 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="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yang, Hao; Singh, Manmilan; Schaefer, Jacob</p> <p>2018-05-10</p> <p>A humidity-swing polymeric sorbent captures <span class="hlt">CO</span><span class="hlt">2</span> from ambient <span class="hlt">air</span> at room temperature simply by changing the humidity level. To date there has been no direct experimental evidence to characterize the chemical mechanism for this process. In this report we describe the use of solid-state NMR to study the humidity-swing <span class="hlt">CO</span><span class="hlt">2</span> absorption/desorption cycle directly. We find that at low humidity levels <span class="hlt">CO</span><span class="hlt">2</span> is absorbed as HCO3-. At high humidity levels, HCO3- is replaced by hydrated OH- and the absorbed <span class="hlt">CO</span><span class="hlt">2</span> is released.</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 Fluxes 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> fluxes 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 flux to estimate simultaneous values of gas transfer rate, KT, and <span class="hlt">air</span> injection flux, VT. The model assumes <span class="hlt">air-sea</span> gas fluxes 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 flux 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/2014NatSR...4E5148L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014NatSR...4E5148L"><span>Acceleration of modern acidification in the South China <span class="hlt">Sea</span> driven by anthropogenic <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>Liu, Yi; Peng, Zicheng; Zhou, Renjun; Song, Shaohua; Liu, Weiguo; You, Chen-Feng; Lin, Yen-Po; Yu, Kefu; Wu, Chung-Che; Wei, Gangjian; Xie, Luhua; Burr, George S.; Shen, Chuan-Chou</p> <p>2014-06-01</p> <p>Modern acidification by the uptake of anthropogenic <span class="hlt">CO</span><span class="hlt">2</span> can profoundly affect the physiology of marine organisms and the structure of ocean ecosystems. Centennial-scale global and regional influences of anthropogenic <span class="hlt">CO</span><span class="hlt">2</span> remain largely unknown due to limited instrumental pH records. Here we present coral boron isotope-inferred pH records for two periods from the South China <span class="hlt">Sea</span>: AD 1048-1079 and AD 1838-2001. There are no significant pH differences between the first period at the Medieval Warm Period and AD 1830-1870. However, we find anomalous and unprecedented acidification during the 20th century, pacing the observed increase in atmospheric <span class="hlt">CO</span><span class="hlt">2</span>. Moreover, pH value also varies in phase with inter-decadal changes in Asian Winter Monsoon intensity. As the level of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> keeps rising, the coupling global warming via weakening the winter monsoon intensity could exacerbate acidification of the South China <span class="hlt">Sea</span> and threaten this expansive shallow water marine ecosystem.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4042124','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4042124"><span>Acceleration of modern acidification in the South China <span class="hlt">Sea</span> driven by anthropogenic <span class="hlt">CO</span><span class="hlt">2</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>Liu, Yi; Peng, Zicheng; Zhou, Renjun; Song, Shaohua; Liu, Weiguo; You, Chen-Feng; Lin, Yen-Po; Yu, Kefu; Wu, Chung-Che; Wei, Gangjian; Xie, Luhua; Burr, George S.; Shen, Chuan-Chou</p> <p>2014-01-01</p> <p>Modern acidification by the uptake of anthropogenic <span class="hlt">CO</span><span class="hlt">2</span> can profoundly affect the physiology of marine organisms and the structure of ocean ecosystems. Centennial-scale global and regional influences of anthropogenic <span class="hlt">CO</span><span class="hlt">2</span> remain largely unknown due to limited instrumental pH records. Here we present coral boron isotope-inferred pH records for two periods from the South China <span class="hlt">Sea</span>: AD 1048–1079 and AD 1838–2001. There are no significant pH differences between the first period at the Medieval Warm Period and AD 1830–1870. However, we find anomalous and unprecedented acidification during the 20th century, pacing the observed increase in atmospheric <span class="hlt">CO</span><span class="hlt">2</span>. Moreover, pH value also varies in phase with inter-decadal changes in Asian Winter Monsoon intensity. As the level of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> keeps rising, the coupling global warming via weakening the winter monsoon intensity could exacerbate acidification of the South China <span class="hlt">Sea</span> and threaten this expansive shallow water marine ecosystem. PMID:24888785</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=307735&keyword=environmental+AND+assessment+AND+natural+AND+environment&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=307735&keyword=environmental+AND+assessment+AND+natural+AND+environment&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>Review of <span class="hlt">Air</span> <span class="hlt">Exchange</span> Rate Models for <span class="hlt">Air</span> Pollution Exposure Assessments</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>A critical aspect of <span class="hlt">air</span> pollution exposure assessments is estimation of the <span class="hlt">air</span> <span class="hlt">exchange</span> rate (AER) for various buildings, where people spend their time. The AER, which is rate the <span class="hlt">exchange</span> of indoor <span class="hlt">air</span> with outdoor <span class="hlt">air</span>, is an important determinant for entry of outdoor <span class="hlt">air</span> pol...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007JMS....66..195F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007JMS....66..195F"><span>Application of new parameterizations of gas transfer velocity and their impact on regional and global marine <span class="hlt">CO</span> <span class="hlt">2</span> budgets</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fangohr, Susanne; Woolf, David K.</p> <p>2007-06-01</p> <p> independently. We then apply our parameterization to a monthly TOPEX altimeter gridded 1.5° × 1.5° data set and compare our results to transfer velocities calculated using the popular wind-based k parameterizations by Wanninkhof [Wanninkhof, R., 1992. Relationship between wind speed and gas <span class="hlt">exchange</span> over the ocean. J. Geophys. Res., 97: 7373-7382.] and Wanninkhof and McGillis [Wanninkhof, R. and McGillis, W., 1999. A cubic relationship between <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> and wind speed. Geophys. Res. Lett., 26(13): 1889-1892]. We show that despite good agreement of the globally averaged transfer velocities, global and regional fluxes differ by up to 100%. These discrepancies are a result of different spatio-temporal distributions of the processes involved in the parameterizations of k, indicating the importance of wave field parameters and a need for further validation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28378907','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28378907"><span>Advanced buffer materials for indoor <span class="hlt">air</span> <span class="hlt">CO</span><span class="hlt">2</span> control in commercial buildings.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Rajan, P E; Krishnamurthy, A; Morrison, G; Rezaei, F</p> <p>2017-11-01</p> <p>In this study, we evaluated solid sorbents for their ability to passively control indoor <span class="hlt">CO</span> <span class="hlt">2</span> concentration in buildings or rooms with cyclic occupancy (eg, offices, bedrooms). Silica supported amines were identified as suitable candidates and systematically evaluated in the removal of <span class="hlt">CO</span> <span class="hlt">2</span> from indoor <span class="hlt">air</span> by equilibrium and dynamic techniques. In particular, sorbents with various amine loadings were synthesized using tetraethylenepentamine (TEPA), poly(ethyleneimine) (PEI) and a silane coupling agent 3-aminopropyltriethoxysilane (APS). TGA analysis indicates that TEPA impregnated silica not only displays a relatively high adsorption capacity when exposed to ppm level <span class="hlt">CO</span> <span class="hlt">2</span> concentrations, but also is capable of desorbing the majority of <span class="hlt">CO</span> <span class="hlt">2</span> by <span class="hlt">air</span> flow (eg, by concentration gradient). In 10 L flow-through chamber experiments, TEPA-based sorbents reduced outlet <span class="hlt">CO</span> <span class="hlt">2</span> by up to 5% at 50% RH and up to 93% of <span class="hlt">CO</span> <span class="hlt">2</span> adsorbed over 8 hours was desorbed within 16 hours. In 8 m 3 flow-through chamber experiments, 18 g of the sorbent powder spread over a <span class="hlt">2</span> m <span class="hlt">2</span> area removed approximately 8% of <span class="hlt">CO</span> <span class="hlt">2</span> injected. By extrapolating these results to real buildings, we estimate that meaningful reductions in the <span class="hlt">CO</span> <span class="hlt">2</span> can be achieved, which may help reduce energy requirements for ventilation and/or improve <span class="hlt">air</span> quality. © 2017 John Wiley & Sons A/S. Published by John Wiley & Sons Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013TCry....7..707R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013TCry....7..707R"><span>Ikaite crystal distribution in 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.; McGinnis, D. F.; Attard, K.; Sievers, J.; Deming, J. W.; Barber, D.</p> <p>2013-04-01</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 surface-ice values of 700-900 μmol kg-1 ice (~25 × 106 crystals kg-1) to values of 100-200 μmol kg-1 ice (1-7 × 106 crystals kg-1) near the <span class="hlt">sea</span> ice-water interface, 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 the lower half of the <span class="hlt">sea</span> ice 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 dissolve in layers below. Melting of <span class="hlt">sea</span> ice and dissolution of observed concentrations of ikaite would result in meltwater with a p<span class="hlt">CO</span><span class="hlt">2</span> of <15 μatm. This value is far below atmospheric values of 390 μatm and surface water concentrations of 315 μatm. Hence, the meltwater increases the potential for seawater uptake of <span class="hlt">CO</span><span class="hlt">2</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoRL..45..880P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoRL..45..880P"><span>Simulated Impact of Glacial Runoff on <span class="hlt">CO</span><span class="hlt">2</span> Uptake in the Gulf of Alaska</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pilcher, Darren J.; Siedlecki, Samantha A.; Hermann, Albert J.; Coyle, Kenneth O.; Mathis, Jeremy T.; Evans, Wiley</p> <p>2018-01-01</p> <p>The Gulf of Alaska (GOA) receives substantial summer freshwater runoff from glacial meltwater. The alkalinity of this runoff is highly dependent on the glacial source and can modify the coastal carbon cycle. We use a regional ocean biogeochemical model to simulate <span class="hlt">CO</span><span class="hlt">2</span> uptake in the GOA under different alkalinity-loading scenarios. The GOA is identified as a current net sink of carbon, though low-alkalinity tidewater glacial runoff suppresses summer coastal carbon uptake. Our model shows that increasing the alkalinity generates an increase in annual <span class="hlt">CO</span><span class="hlt">2</span> uptake of 1.9-<span class="hlt">2</span>.7 TgC/yr. This transition is comparable to a projected change in glacial runoff composition (i.e., from tidewater to land-terminating) due to continued climate warming. Our results demonstrate an important local carbon-climate feedback that can significantly increase coastal carbon uptake via enhanced <span class="hlt">air-sea</span> <span class="hlt">exchange</span>, with potential implications to the coastal ecosystems in glaciated areas around the world.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1248789-exfoliation-propensity-oxide-scale-heat-exchangers-used-supercritical-co2-power-cycles','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1248789-exfoliation-propensity-oxide-scale-heat-exchangers-used-supercritical-co2-power-cycles"><span>Exfoliation Propensity of Oxide Scale in Heat <span class="hlt">Exchangers</span> Used for Supercritical <span class="hlt">CO</span><span class="hlt">2</span> Power Cycles</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>Sabau, Adrian S; Shingledecker, John P.; Kung, Steve</p> <p>2016-01-01</p> <p>Supercritical <span class="hlt">CO</span><span class="hlt">2</span> (s<span class="hlt">CO</span><span class="hlt">2</span>) Brayton cycle systems offer the possibility of improved efficiency in future fossil energy power generation plants operating at temperatures of 650 C and above. As there are few data on the oxidation/corrosion behavior of structural alloys in s<span class="hlt">CO</span><span class="hlt">2</span> at these temperatures, modeling to predict the propensity for oxide exfoliation is not well developed, thus hindering materials selection for these novel cycles. The ultimate goal of this effort is to provide needed data on scale exfoliation behavior in s<span class="hlt">CO</span><span class="hlt">2</span> for confident alloy selection. To date, a model developed by ORNL and EPRI for the exfoliation of oxide scalesmore » formed on boiler tubes in high-temperature, high-pressure steam has proven useful for managing exfoliation in conventional steam plants. A major input provided by the model is the ability to predict the likelihood of scale failure and loss based on understanding of the evolution of the oxide morphologies and the conditions that result in susceptibility to exfoliation. This paper describes initial steps taken to extend the existing model for exfoliation of steam-side oxide scales to s<span class="hlt">CO</span><span class="hlt">2</span> conditions. The main differences between high-temperature, high-pressure steam and s<span class="hlt">CO</span><span class="hlt">2</span> that impact the model involve (i) significant geometrical differences in the heat <span class="hlt">exchangers</span>, ranging from standard pressurized tubes seen typically in steam-producing boilers to designs for s<span class="hlt">CO</span><span class="hlt">2</span> that employ variously-curved thin walls to create shaped flow paths for extended heat transfer area and small channel cross-sections to promote thermal convection and support pressure loads; (ii) changed operating characteristics with s<span class="hlt">CO</span><span class="hlt">2</span> due to the differences in physical and thermal properties compared to steam; and (iii) possible modification of the scale morphologies, hence properties that influence exfoliation behavior, due to reaction with carbon species from s<span class="hlt">CO</span><span class="hlt">2</span>. The numerical simulations conducted were based on an assumed s<span class="hlt">CO</span><span class="hlt">2</span> operating schedule and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3421162','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3421162"><span>The urgency of the development 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="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Lackner, Klaus S.; Brennan, Sarah; Matter, Jürg M.; Park, A.-H. Alissa; Wright, Allen; van der Zwaan, Bob</p> <p>2012-01-01</p> <p><span class="hlt">CO</span><span class="hlt">2</span> capture and storage (CCS) has the potential to develop into an important tool to address climate change. Given society’s present reliance on fossil fuels, widespread adoption of CCS appears indispensable for meeting stringent climate targets. We argue that for conventional CCS to become a successful climate mitigation technology—which by necessity has to operate on a large scale—it may need to be complemented with <span class="hlt">air</span> capture, removing <span class="hlt">CO</span><span class="hlt">2</span> directly from the atmosphere. <span class="hlt">Air</span> capture of <span class="hlt">CO</span><span class="hlt">2</span> could act as insurance against <span class="hlt">CO</span><span class="hlt">2</span> leaking from storage and furthermore may provide an option for dealing with emissions from mobile dispersed sources such as automobiles and airplanes. PMID:22843674</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1810126C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1810126C"><span>Towards constraining the stratosphere-troposphere <span class="hlt">exchange</span> of radiocarbon: strategies of stratospheric 14<span class="hlt">CO</span><span class="hlt">2</span> measurements using <span class="hlt">Air</span>Core</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, Huilin; Paul, Dipayan; Meijer, Harro; Miller, John; Kivi, Rigel; Krol, Maarten</p> <p>2016-04-01</p> <p>Radiocarbon (14C) plays an important role in the carbon cycle studies to understand both natural and anthropogenic carbon fluxes, 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 stratosphere due to the cosmogenic production. To this end, better understanding the stratospheric radiocarbon source is very useful to advance the use of radiocarbon for these applications. However, stratospheric 14C observations have been very limited so that there are large uncertainties on 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 14C measurements using <span class="hlt">Air</span>Core samples from Sodankylä, Northern Finland. <span class="hlt">Air</span>Core is an innovative atmospheric sampling system, which passively collects atmospheric <span class="hlt">air</span> samples into a long piece of coiled stainless steel tubing during the descent of a balloon flight. Due to the relatively low cost of the consumables, there is a potential to make such <span class="hlt">Air</span>Core profiling in other parts of the world on a regular basis. In this study, we simulate the 14C in the atmosphere and assess the stratosphere-troposphere <span class="hlt">exchange</span> of radiocarbon using the TM5 model. The Sodankylä radiocarbon measurements will be used to verify the performance of the model at high latitude. Besides this, we will also 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 <span class="hlt">exchange</span>, and based on the results design a strategy to set up a 14C measurement program using <span class="hlt">Air</span>Core.</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('http://adsabs.harvard.edu/abs/2016AGUFMGC23C1252C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMGC23C1252C"><span>Achieving Negative <span class="hlt">CO</span><span class="hlt">2</span> Emissions by Protecting Ocean Chemistry</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cannara, A.</p> <p>2016-12-01</p> <p>Industrial Age <span class="hlt">CO</span><span class="hlt">2</span> added 1.8 trillion tons to the atmosphere. About ¼ has dissolved in <span class="hlt">seas</span>. The rest still dissolves, bolstered by present emissions of >30 gigatons/year. Airborne & oceanic <span class="hlt">CO</span><span class="hlt">2</span> have induced <span class="hlt">sea</span> warming & ocean acidification*. This paper suggests a way to induce a negative <span class="hlt">CO</span><span class="hlt">2</span>-emissions environment for climate & oceans - preserve the planet`s dominant <span class="hlt">CO</span><span class="hlt">2</span>-sequestration system ( 1 gigaton/year via calcifying <span class="hlt">sea</span> life**) by promptly protecting ocean chemistry via expansion of clean power for both lime production & replacement of <span class="hlt">CO</span><span class="hlt">2</span>-emitting sources. Provide natural alkali (CaO, MgO…) to oceans to maintain average pH above 8.0, as indicated by marine biologists. That alkali (lime) is available from past calcifying life's limestone deposits, so can be returned safely to <span class="hlt">seas</span> once its <span class="hlt">CO</span><span class="hlt">2</span> is removed & permanently sequestered (Carbfix, BSCP, etc.***). Limestone is a dense source of <span class="hlt">CO</span><span class="hlt">2</span> - efficient processing per mole sequestered. Distribution of enough lime is possible via cargo-ship transits - 10,000 tons lime/transit, 1 million transits/year. New Panamax ships carry 120,000 tons. Just 10,000/transit allows gradual reduction of present & past <span class="hlt">CO</span><span class="hlt">2</span> emissions effects, if coupled with combustion-power reductions. <span class="hlt">CO</span><span class="hlt">2</span> separation from limestone, as in cement plants, consumes 400kWHrs of thermal energy per ton of output lime (or <span class="hlt">CO</span><span class="hlt">2</span>). To combat yearly <span class="hlt">CO</span><span class="hlt">2</span> dissolution in <span class="hlt">seas</span>, we must produce & distribute about 10gigatons of lime/year. Only nuclear power produces the clean energy (thousands of terawatt hours) to meet this need - 1000 dedicated 1GWe reactors, processing 12 cubic miles of limestone/year & sequestering <span class="hlt">CO</span><span class="hlt">2</span> into a similar mass of basalt. Basalt is common in the world. Researchers*** report it provides good, mineralized <span class="hlt">CO</span><span class="hlt">2</span> sequestration. The numbers above allow gradual <span class="hlt">CO</span><span class="hlt">2</span> reduction in <span class="hlt">air</span> and <span class="hlt">seas</span>, if we return to President Kennedy's energy path: http://tinyurl.com/6xgpkfa We're on an environmental precipice due to failure to eliminate</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA629222','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA629222"><span>Microphysics of <span class="hlt">Air-Sea</span> <span class="hlt">Exchanges</span></span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2003-09-30</p> <p>intensities of the three color components at each point of the image . The ISG imaged an area of the water surface of up to 45 cm (downwind) x 30 cm...notwithstanding any other provision of law, no person shall be subject to a penalty for failing to comply with a collection of information if it does not...satellite-derived <span class="hlt">sea</span>-surface temperature (SST) fields into meaningful climatologies and to more physically-based applications of satellite data to studies</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> fluxes 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> <span class="hlt">exchange</span> 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> fluxes 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('http://adsabs.harvard.edu/abs/2017EaFut...5..633N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EaFut...5..633N"><span>Increasing transnational <span class="hlt">sea</span>-ice <span class="hlt">exchange</span> in a changing 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>Newton, Robert; Pfirman, Stephanie; Tremblay, Bruno; DeRepentigny, Patricia</p> <p>2017-06-01</p> <p>The changing Arctic <span class="hlt">sea</span>-ice cover is likely to impact the trans-border <span class="hlt">exchange</span> of <span class="hlt">sea</span> ice between the exclusive economic zones (EEZs) of the Arctic nations, affecting the risk of ice-rafted contamination. We apply the Lagrangian Ice Tracking System (LITS) to identify <span class="hlt">sea</span>-ice formation events and track <span class="hlt">sea</span> ice to its melt locations. Most ice (52%) melts within 100 km of where it is formed; ca. 21% escapes from its EEZ. Thus, most contaminants will be released within an ice parcel's originating EEZ, while material carried by over 1 00,000 km<span class="hlt">2</span> of ice—an area larger than France and Germany combined—will be released to other nations' waters. Between the periods 1988-1999 and 2000-2014, <span class="hlt">sea</span>-ice formation increased by ˜17% (roughly 6 million km<span class="hlt">2</span> vs. 5 million km<span class="hlt">2</span> annually). Melting peaks earlier; freeze-up begins later; and the central Arctic Ocean is more prominent in both formation and melt in the later period. The total area of ice transported between EEZs increased, while transit times decreased: for example, Russian ice reached melt locations in other nations' EEZs an average of 46% faster while North American ice reached destinations in Eurasian waters an average of 37% faster. Increased trans-border <span class="hlt">exchange</span> is mainly a result of increased speed (˜14% per decade), allowing first-year ice to escape the summer melt front, even as the front extends further north. Increased trans-border <span class="hlt">exchange</span> over shorter times is bringing the EEZs of the Arctic nations closer together, which should be taken into account in policy development—including establishment of marine-protected areas.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17650840','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17650840"><span>[<span class="hlt">CO</span><span class="hlt">2</span> turbulent <span class="hlt">exchange</span> in a broadleaved Korean pine forest in Changbai Mountains].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wu, Jia-bing; Guan, De-xin; Sun, Xiao-min; Shi, Ting-ting; Han, Shi-jie; Jin, Chang-jie</p> <p>2007-05-01</p> <p>The measurement of <span class="hlt">CO</span><span class="hlt">2</span> turbulent <span class="hlt">exchange</span> in a broadleaved Korean pine forest in Changbai Mountains by an open-path eddy covariance system showed that with near neutral atmospheric stratification, the <span class="hlt">CO</span><span class="hlt">2</span> and vertical wind components over canopy in inertial subrange followed the expected -<span class="hlt">2</span>/3 power law, and the dominant vertical eddy scale was about 40 m. The frequency ranges of eddy contributions to <span class="hlt">CO</span><span class="hlt">2</span> fluxes were mostly within 0.01-<span class="hlt">2</span>.0 Hz, and the eddy translated by low frequency over canopy contributed more of <span class="hlt">CO</span><span class="hlt">2</span> fluxes. The open-path eddy covariance system could satisfy the estimation of turbulent fluxes over canopy, but the <span class="hlt">CO</span><span class="hlt">2</span> fluxes between forest and atmosphere were generally underestimated at night because the increment of non turbulent processes, suggesting that the <span class="hlt">CO</span><span class="hlt">2</span> fluxes estimated under weak turbulence needed to revise correspondingly.</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> Fluxes 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> fluxes 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> fluxes 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> flux 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> fluxes 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('https://www.ncbi.nlm.nih.gov/pubmed/25985484','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25985484"><span>[<span class="hlt">CO</span><span class="hlt">2</span>-<span class="hlt">exchange</span> in tundra ecosystems of Vaygach Island during the unusually warm and dry vegetation season].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zamolodchikov, D G</p> <p>2015-01-01</p> <p>In summer of 2013, field studies of <span class="hlt">CO</span><span class="hlt">2</span>-<span class="hlt">exchange</span> in tundra ecosystems of Vaygach Island have been conducted using the chamber method. The models are developed that establish relationships between <span class="hlt">CO</span><span class="hlt">2</span> fluxes and key ecological factors such as temperature, photosynthetic active radiation, leaf mass of vascular plants, and depth of thawing. According to the model estimates, in 2013 vegetation season tundra ecosystems of Vaygach Island have been appearing to be a <span class="hlt">CO</span><span class="hlt">2</span> source to the atmosphere (31.9 ± 17.1 g C m(-<span class="hlt">2</span>) season(-1)) with gross primary production equal to 136.6 ± 18.9 g C m(-<span class="hlt">2</span>) season(-1) and ecosystem respiration of 168.5 ± ± 18.4 g C m(-<span class="hlt">2</span>) season(-1). Emission of <span class="hlt">CO</span><span class="hlt">2</span> from the soil surface (soil respiration) has been equal, on the average, to 67.3% of the ecosystem respiration. The reason behind carbon losses by tundra ecosystems seems to be unusually warm and dry weather conditions in 2013 summer. The <span class="hlt">air</span> temperature during summer months has been twice as high as the climatic norm for 1961-1990. Last decades, researches in the circumpolar Arctic revealed a growing trend to the carbon sink from the atmosphere to tundra ecosystems. This trend can be interrupted by unusually warm weather situations becoming more frequent and of larger scale.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19900065057&hterms=climate+exchange&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dclimate%2Bexchange','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19900065057&hterms=climate+exchange&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dclimate%2Bexchange"><span>Atmosphere-biosphere <span class="hlt">exchange</span> of <span class="hlt">CO</span><span class="hlt">2</span> and O3 in the Central Amazon Forest</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Fan, Song-Miao; Wofsy, Steven C.; Bakwin, Peter S.; Jacob, Daniel J.; Fitzjarrald, David R.</p> <p>1990-01-01</p> <p>An eddy correlation measurement of O3 deposition and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> at a level 10 m above the canopy of the Amazon forest, conducted as part of the NASA/INPE ABLE<span class="hlt">2</span>b mission during the wet season of 1987, is presented. It was found that the ecosystem <span class="hlt">exchange</span> of <span class="hlt">CO</span><span class="hlt">2</span> undergoes a well-defined diurnal variation driven by the input of solar radiation. A curvilinear relationship was found between solar irradiance and uptake of <span class="hlt">CO</span><span class="hlt">2</span>, with net <span class="hlt">CO</span><span class="hlt">2</span> uptake at a given solar irradiance equal to rates observed over forests in other climate zones. The carbon balance of the system appeared sensitive to cloud cover on the time scale of the experiment, suggesting that global carbon storage might be affected by changes in insolation associated with tropical climate fluctuations. The forest was found to be an efficient sink for O3 during the day, and evidence indicates that the Amazon forests could be a significant sink for global ozone during the nine-month wet period and that deforestation could dramatically alter O3 budgets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1349784-pressure-dependence-carbonate-exchange-npo2-co3-aqueous-solutions','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1349784-pressure-dependence-carbonate-exchange-npo2-co3-aqueous-solutions"><span>Pressure dependence of carbonate <span class="hlt">exchange</span> with [NpO <span class="hlt">2</span>(<span class="hlt">CO</span> 3) 3] 4– in aqueous solutions</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Pilgrim, Corey D.; Zavarin, Mavrik; Casey, William H.</p> <p>2016-12-13</p> <p>Here, the rates of ligand <span class="hlt">exchange</span> into the geochemically important [NpO <span class="hlt">2</span>(<span class="hlt">CO</span> 3) 3] 4– aqueous complex are measured as a function of pressure in order to complement existing data on the isostructural [UO <span class="hlt">2</span>(<span class="hlt">CO</span> 3) 3] 4– complex. Experiments are conducted at pH conditions where the rate of <span class="hlt">exchange</span> is independent of the proton concentration. Unexpectedly, the experiments show a distinct difference in the pressure dependencies of rates of <span class="hlt">exchange</span> for the uranyl and neptunyl complexes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29574192','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29574192"><span>Comprehensive analysis of differentially expressed genes reveals the molecular response to elevated <span class="hlt">CO</span><span class="hlt">2</span> levels in two <span class="hlt">sea</span> buckthorn cultivars.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhang, Guoyun; Zhang, Tong; Liu, Juanjuan; Zhang, Jianguo; He, Caiyun</p> <p>2018-06-20</p> <p>Atmospheric carbon dioxide (<span class="hlt">CO</span> <span class="hlt">2</span> ) concentration increases every year. It is critical to understand the elevated <span class="hlt">CO</span> <span class="hlt">2</span> response molecular mechanisms of plants using genomic techniques. Hippophae rhamnoides L. is a high stress resistance plant species widely distributed in Europe and Asia. However, the molecular mechanism of elevated <span class="hlt">CO</span> <span class="hlt">2</span> response in H. rhamnoides has been limited. In this study, transcriptomic analysis of two <span class="hlt">sea</span> buckthorn cultivars under different <span class="hlt">CO</span> <span class="hlt">2</span> concentrations was performed, based on the next-generation illumina sequencing platform and de novo assembly. We identified 4740 differentially expressed genes in <span class="hlt">sea</span> buckthorn response to elevated <span class="hlt">CO</span> <span class="hlt">2</span> concentrations. According to the gene ontology (GO) results, photosystem I, photosynthesis and chloroplast thylakoid membrane were the main enriched terms in 'xiangyang' <span class="hlt">sea</span> buckthorn. In 'zhongguo' <span class="hlt">sea</span> buckthorn, photosynthesis was also the main significantly enriched term. However, the number of photosynthesis related differentially expressed genes were different between two <span class="hlt">sea</span> buckthorn cultivars. Our GO and pathway analyses indicated that the expression levels of the transcription factors WRKY, MYB and NAC were significantly different between the two <span class="hlt">sea</span> buckthorn cultivars. This study provides a reliable transcriptome sequence resource and is a valuable resource for genetic and genomic researches for plants under high <span class="hlt">CO</span> <span class="hlt">2</span> concentration in the future. Copyright © 2018 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20090038923&hterms=heat+exchanger&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dheat%2Bexchanger','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20090038923&hterms=heat+exchanger&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dheat%2Bexchanger"><span>Investigating Liquid <span class="hlt">CO</span><span class="hlt">2</span> as a Coolant for a MTSA Heat <span class="hlt">Exchanger</span> Design</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Paul, Heather L.; Padilla, Sebastian; Powers, Aaron; Iacomini, Christie</p> <p>2009-01-01</p> <p>Metabolic heat regenerated Temperature Swing Adsorption (MTSA) technology is being developed for thermal and carbon dioxide (<span class="hlt">CO</span> <span class="hlt">2</span>) control for a future Portable Life Support System (PLSS), as well as water recycling. <span class="hlt">CO</span> <span class="hlt">2</span> removal and rejection is accomplished by driving a sorbent through a temperature swing of approximately 210 K to 280 K . The sorbent is cooled to these sub-freezing temperatures by a Sublimating Heat <span class="hlt">Exchanger</span> (SHX) with liquid coolant expanded to sublimation temperatures. Water is the baseline coolant available on the moon, and if used, provides a competitive solution to the current baseline PLSS schematic. Liquid <span class="hlt">CO</span><span class="hlt">2</span> (LCO<span class="hlt">2</span>) is another non-cryogenic coolant readily available from Martian resources which can be produced and stored using relatively low power and minimal infrastructure. LCO <span class="hlt">2</span> expands from high pressure liquid (5800 kPa) to Mars ambient (0.8 kPa) to produce a gas / solid mixture at temperatures as low as 156 K. Analysis and experimental work are presented to investigate factors that drive the design of a heat <span class="hlt">exchanger</span> to effectively use this sink. Emphasis is given to enabling efficient use of the <span class="hlt">CO</span> <span class="hlt">2</span> cooling potential and mitigation of heat <span class="hlt">exchanger</span> clogging due to solid formation. Minimizing mass and size as well as coolant delivery are also considered. The analysis and experimental work is specifically performed in an MTSA-like application to enable higher fidelity modeling for future optimization of a SHX design. In doing so, the work also demonstrates principles and concepts so that the design can be further optimized later in integrated applications (including Lunar application where water might be a choice of coolant).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1394176','SCIGOV-DOEDE'); return false;" href="https://www.osti.gov/servlets/purl/1394176"><span>Atmospheric <span class="hlt">CO</span><span class="hlt">2</span> Record from In Situ Measurements at Amsterdam Island (1980-1995)</span></a></p> <p><a target="_blank" href="http://www.osti.gov/dataexplorer">DOE Data Explorer</a></p> <p>Gaudry, A. [Centre des Faibles Radioactivites, Laboratoire de Modelisation du Climat et de l'Environnement, Centre d'Etudes de Saclay, France; Kazan, V. [Centre des Faibles Radioactivites, Laboratoire de Modelisation du Climat et de l'Environnement, Centre d'Etudes de Saclay, France; Monfray, P. [Centre des Faibles Radioactivites, Laboratoire de Modelisation du Climat et de l'Environnement, Centre d'Etudes de Saclay, France</p> <p>1996-09-01</p> <p>Until 1993 <span class="hlt">air</span> samples were collected continuously through an <span class="hlt">air</span> intake located at the top of a tower, 9 m above ground and 65 m above mean <span class="hlt">sea</span> level. Since 1994, the intake has been situated 20 m above ground and 76 m above mean <span class="hlt">sea</span> level. The tower is located at the north-northwest end of the island on the edge of a 55 m cliff. The <span class="hlt">air</span> is dried by means of a cryogenic water trap at -60°C. Until 1990, determinations of <span class="hlt">CO</span><span class="hlt">2</span> were made by using successively two Hartmann-Braun URAS <span class="hlt">2</span>T nondispersive infrared (NDIR) analyzers. Since 1991, <span class="hlt">CO</span><span class="hlt">2</span> determinations have been made using a Siemens ULTRAMAT 5F NDIR. Standard gases in use from October 1980 to December of 1984 were <span class="hlt">CO</span><span class="hlt">2</span>-in-N<span class="hlt">2</span> mixtures certified by Scripps Institution of Oceanography (SIO). The N<span class="hlt">2</span> scale was corrected for the carrier gas effect to obtain the <span class="hlt">air</span> scale (WMO mole fraction scale). In 1985, <span class="hlt">CO</span><span class="hlt">2</span>-in-<span class="hlt">air</span> mixtures expressed in the 1985 WMO mole fraction in <span class="hlt">air</span> scale were introduced. In 1990, a new series of 12 primary standard gases were gravimetrically prepared, then linearly adjusted at the laboratory and checked several times (i.e., 1990, 1992, and 1993) through intercalibrations with DSIR in New Zealand and NOAA/CMDL, which both used the 1985 mole fraction scale. The agreement was always better than 0.1 ppm (Monfray et al. 1992). Since 1993, the 1993 mole fraction scale has been used thanks to a new series of 10 cylinders provided by SIO.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JMMM..452..153W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JMMM..452..153W"><span>Perpendicular <span class="hlt">exchange</span> coupling effects in ferrimagnetic TbFe<span class="hlt">Co/GdFeCo</span> hard/soft structures</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Ke; Wang, Yahong; Ling, Fujin; Xu, Zhan</p> <p>2018-04-01</p> <p>Bilayers consisting of magnetically hard TbFe<span class="hlt">Co</span> and soft GdFe<span class="hlt">Co</span> alloy were fabricated. <span class="hlt">Exchange</span>-spring and sharp switching in a step-by-step fashion were observed in the TbFe<span class="hlt">Co/GdFeCo</span> hard/soft bilayers with increasing GdFe<span class="hlt">Co</span> thickness. A perpendicular <span class="hlt">exchange</span> bias field of several hundred Oersteds is observed from the shift of minor loops pinned by TbFe<span class="hlt">Co</span> layer. The perpendicular <span class="hlt">exchange</span> energy is derived to be in the range of 0.18-0.30 erg/cm<span class="hlt">2</span>. The <span class="hlt">exchange</span> energy is shown to increase with the thickness of GdFe<span class="hlt">Co</span> layer in the bilayers, which can be attributed to the enhanced perpendicular anisotropy of GdFe<span class="hlt">Co</span> layer in our experimental range.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMGC31A1030K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMGC31A1030K"><span>Timing of insolation forcing, <span class="hlt">CO</span><span class="hlt">2</span> and <span class="hlt">sea</span> level changes around the current and last four interglacial periods</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kawamura, K.; Aoki, S.; Nakazawa, T.; Abe-Ouchi, A.; Saito, F.</p> <p>2013-12-01</p> <p>Investigation of the roles of different forcings (e.g. orbital variations and greenhouse gases) on climate and <span class="hlt">sea</span> level requires a paleoclimate chronology with high accuracy. Such a chronology for the past 360 ky was constructed through orbital tuning of O<span class="hlt">2</span>/N<span class="hlt">2</span> ratio of trapped <span class="hlt">air</span> in the Dome Fuji and Vostok ice cores with local summer insolation (Kawamura et al., 2007). We extend the O<span class="hlt">2</span>/N<span class="hlt">2</span> chronology back to ~500 kyr by analyzing the second Dome Fuji ice core, and find the duration of 11 ka, 5 ka, 9 ka, and 20 ka for MIS 5e, 7e, 9e and 11c interglacial periods in Antarctica, with similar variations in atmospheric <span class="hlt">CO</span><span class="hlt">2</span>. The termination timings are consistent with the rising phase of Northern Hemisphere summer insolation. Marine sediment cores from northern North Atlantic contain millennial-scale signatures in various proxy records (e.g. SST, IRD), including abrupt climatic shifts and bipolar seesaw. Based on the bipolar correlation of millennial-scale events, it is possible to transfer our accurate chronology to marine cores from the North Atlantic. As a first attempt, we correlate the planktonic δ18O and IRD records from the marine core ODP 980 with the ice-core δ18O and CH4 around MIS 11. We find that the durations of interglacial plateaus of planktonic δ18O (proxy for <span class="hlt">sea</span> surface environments) and benthic δ18O (proxy for ice volume and deep-<span class="hlt">sea</span> temperature) for MIS 11c are 20 and 15 ka, respectively, which are significantly shorter than originally suggested. These durations are similar to that of Antarctic climate and atmospheric <span class="hlt">CO</span><span class="hlt">2</span>. However, the onsets of interglacial levels in ODP980 for MIS 11 are significantly later than those in Antarctic δ18O and atmospheric <span class="hlt">CO</span><span class="hlt">2</span> (by as much as ~10 ka), suggesting very long duration (more than one precession cycle) for the complete deglaciation and northern high-latitude warming for Termination V. Atmospheric <span class="hlt">CO</span><span class="hlt">2</span> may have been the critical forcing for this termination. The long duration of Termination V is consistent</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.1064S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.1064S"><span><span class="hlt">Exchanges</span> between the open Black <span class="hlt">Sea</span> and its North West shelf</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shapiro, Georgy; Wobus, Fred; Zhou, Feng</p> <p>2014-05-01</p> <p> offshore flow over a large section of the shelf break. Due to the short duration of strong wind effects (4-7 days) the horizontal extent of cross-shelf-break <span class="hlt">exchanges</span> is limited to the outer shelf. The effect of Ekman drift is confined to the upper layers. In contrast, eddies and meanders penetrate deep down to the bottom, but they are restricted laterally. During the strong wind events of April 15 - 22 and July 1 - 4, some 0.66×1012 and 0.44×1012 m3of water were removed from the northwestern shelf respectively. In comparison, the single long-lived Sevastopol Eddy generated a much larger offshore transfer of <span class="hlt">2</span>.84×1012 m3 over the period April 23 to June 30, which is equivalent to 102% of the volume of northwestern shelf waters. This result is consistent with the data obtained from satellite derived information (Shapiro et al, 2010). The open Black <span class="hlt">Sea</span> is generally warmer and more saline than the northwest shelf. Hence the <span class="hlt">exchanges</span> contribute to the increase in both salinity and temperature of shelf waters. Over the study period, salt <span class="hlt">exchanges</span> increased the average density of the shelf waters by 0.67 kg m-3 and reduced the density contrast between the shelf and deep <span class="hlt">sea</span>, while lateral heat <span class="hlt">exchanges</span> reduced the density of the shelf waters by 0.16 kg m-3 and thus enhanced density contrast across the shelf break. This study was supported by the EU (via PERSEUS grant FP7-OCEAN-2011-287600 and MyOcean SPA.2011.1.5-01 grant 283367), Ministry of Science and Technology of China (Grant 2011CB409803), the Natural Science Foundation of China (Grant 41276031), Zhejiang Association for International <span class="hlt">Exchange</span> of Personnel, and the University of Plymouth Marine Institute Innovation Fund. References Huthnance, J. M., 1995. Circulation, <span class="hlt">exchange</span> and water masses at the ocean margin: the role of physical processes at the shelf edge, Prog Oceanogr, 35(4), 353-431, Ivanov L.I., Besiktepe S., Ozsoy E., 1997. In: E.Ozsoy and A.Mikaelyan (eds). Sensitivity to change: Black <span class="hlt">Sea</span> , Baltic <span class="hlt">Sea</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.B41C0042T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.B41C0042T"><span>Net ecosystem <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> of a primary tropical peat swamp forest in 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>Tang Che Ing, A.; Stoy, P. C.; Melling, L.</p> <p>2014-12-01</p> <p>Tropical peat swamp forests are widely recognized as one of the world's most efficient ecosystems for the sequestration and storage of carbon through both their aboveground biomass and underlying thick deposits of peat. As the peat characteristics exhibit high spatial and temporal variability as well as the structural and functional complexity of forests, tropical peat ecosystems can act naturally as both carbon sinks and sources over their life cycles. Nonetheless, few reports of studies on the ecosystem-scale <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> of tropical peat swamp forests are available to-date and their present roles in the global carbon cycle remain uncertain. To quantify <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> and unravel the prevailing factors and potential underlying mechanism regulating net <span class="hlt">CO</span><span class="hlt">2</span> fluxes, an eddy covariance tower was erected in a tropical peat swamp forest in Sarawak, Malaysia. We observed that the diurnal and seasonal patterns of net ecosystem <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> (NEE) and its components (gross primary productivity (GPP) and ecosystem respiration (RE)) varied between seasons and years. Rates of NEE declined in the wet season relative to the dry season. Conversely, both the gross primary productivity (GPP) and ecosystem respiration (RE) were found to be higher during the wet season than the dry season, in which GPP was strongly negatively correlated with NEE. The average annual NEE was 385 ± 74 g C m-<span class="hlt">2</span> yr-1, indicating the primary peat swamp forest functioned as net source of <span class="hlt">CO</span><span class="hlt">2</span> to the atmosphere over the observation period.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28741826','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28741826"><span><span class="hlt">Sea</span> anemones may thrive in a high <span class="hlt">CO</span><span class="hlt">2</span> world.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Suggett, David J; Hall-Spencer, Jason M; Rodolfo-Metalpa, Riccardo; Boatman, Toby G; Payton, Ross; Tye Pettay, D; Johnson, Vivienne R; Warner, Mark E; Lawson, Tracy</p> <p>2012-10-01</p> <p>Increased seawater p<span class="hlt">CO</span> <span class="hlt">2</span> , and in turn 'ocean acidification' (OA), is predicted to profoundly impact marine ecosystem diversity and function this century. Much research has already focussed on calcifying reef-forming corals (Class: Anthozoa) that appear particularly susceptible to OA via reduced net calcification. However, here we show that OA-like conditions can simultaneously enhance the ecological success of non-calcifying anthozoans, which not only play key ecological and biogeochemical roles in present day benthic ecosystems but also represent a model organism should calcifying anthozoans exist as less calcified (soft-bodied) forms in future oceans. Increased growth (abundance and size) of the <span class="hlt">sea</span> anemone (Anemonia viridis) population was observed along a natural <span class="hlt">CO</span> <span class="hlt">2</span> gradient at Vulcano, Italy. Both gross photosynthesis (P G ) and respiration (R) increased with p<span class="hlt">CO</span> <span class="hlt">2</span> indicating that the increased growth was, at least in part, fuelled by bottom up (<span class="hlt">CO</span> <span class="hlt">2</span> stimulation) of metabolism. The increase of P G outweighed that of R and the genetic identity of the symbiotic microalgae (Symbiodinium spp.) remained unchanged (type A19) suggesting proximity to the vent site relieved <span class="hlt">CO</span> <span class="hlt">2</span> limitation of the anemones' symbiotic microalgal population. Our observations of enhanced productivity with p<span class="hlt">CO</span> <span class="hlt">2</span> , which are consistent with previous reports for some calcifying corals, convey an increase in fitness that may enable non-calcifying anthozoans to thrive in future environments, i.e. higher seawater p<span class="hlt">CO</span> <span class="hlt">2</span> . Understanding how <span class="hlt">CO</span> <span class="hlt">2</span> -enhanced productivity of non- (and less-) calcifying anthozoans applies more widely to tropical ecosystems is a priority where such organisms can dominate benthic ecosystems, in particular following localized anthropogenic stress. © 2012 Blackwell Publishing Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24169104','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24169104"><span>Spring photosynthetic recovery of boreal Norway spruce under conditions of elevated [<span class="hlt">CO</span>(<span class="hlt">2</span>)] and <span class="hlt">air</span> temperature.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wallin, Göran; Hall, Marianne; Slaney, Michelle; Räntfors, Mats; Medhurst, Jane; Linder, Sune</p> <p>2013-11-01</p> <p>Accumulated carbon uptake, apparent quantum yield (AQY) and light-saturated net <span class="hlt">CO</span><span class="hlt">2</span> assimilation (Asat) were used to assess the responses of photosynthesis to environmental conditions during spring for three consecutive years. Whole-tree chambers were used to expose 40-year-old field-grown Norway spruce trees in northern Sweden to an elevated atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentration, [<span class="hlt">CO</span><span class="hlt">2</span>], of 700 μmol <span class="hlt">CO</span><span class="hlt">2</span> mol(-1) (CE) and an <span class="hlt">air</span> temperature (T) between <span class="hlt">2</span>.8 and 5.6 °C above ambient T (TE), during summer and winter. Net shoot <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> (Anet) was measured continuously on 1-year-old shoots and was used to calculate the accumulated carbon uptake and daily Asat and AQY. The accumulated carbon uptake, from 1 March to 30 June, was stimulated by 33, 44 and 61% when trees were exposed to CE, TE, and CE and TE combined, respectively. <span class="hlt">Air</span> temperature strongly influenced the timing and extent of photosynthetic recovery expressed as AQY and Asat during the spring. Under elevated T (TE), the recovery of AQY and Asat commenced ∼10 days earlier and the activity of these parameters was significantly higher throughout the recovery period. In the absence of frost events, the photosynthetic recovery period was less than a week. However, frost events during spring slowed recovery so that full recovery could take up to 60 days to complete. Elevated [<span class="hlt">CO</span><span class="hlt">2</span>] stimulated AQY and Asat on average by ∼10 and ∼50%, respectively, throughout the recovery period, but had minimal or no effect on the onset and length of the photosynthetic recovery period during the spring. However, AQY, Asat and Anet all recovered at significantly higher T (average +<span class="hlt">2.2</span> °C) in TE than in TA, possibly caused by acclimation or by shorter days and lower light levels during the early part of the recovery in TE compared with TA. The results suggest that predicted future climate changes will cause prominent stimulation of photosynthetic <span class="hlt">CO</span><span class="hlt">2</span> uptake in boreal Norway spruce forest during spring, mainly caused by elevated T</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26363332','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26363332"><span>Randomized, double-blind trial of <span class="hlt">CO</span><span class="hlt">2</span> versus <span class="hlt">air</span> insufflation in children undergoing colonoscopy.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Homan, Matjaž; Mahkovic, Dora; Orel, Rok; Mamula, Petar</p> <p>2016-05-01</p> <p>Studies in adults have shown that postprocedural abdominal pain is reduced with the use of carbon dioxide (<span class="hlt">CO</span>(<span class="hlt">2</span>)) instead of <span class="hlt">air</span> for insufflation during colonoscopy. The aim of our study was to compare postprocedural abdominal pain and girth in children undergoing colonoscopy using <span class="hlt">CO</span>(<span class="hlt">2</span>) or <span class="hlt">air</span> for insufflation. This was a prospective, randomized, double-blind study that included 76 consecutive pediatric patients undergoing colonoscopy for various indications. Patients were randomly assigned to either <span class="hlt">CO</span>(<span class="hlt">2</span>) or <span class="hlt">air</span> insufflation. At <span class="hlt">2</span>, 4, and 24 hours after the examination, the patients' pain was assessed by using the 11-point numerical rating scale. The waist circumference was measured 10 minutes and <span class="hlt">2</span> and 4 hours after colonoscopy. A significantly higher proportion of patients had no pain after colonoscopy in the <span class="hlt">CO</span>(<span class="hlt">2</span>) group compared with the <span class="hlt">air</span> group (82 vs 37% at <span class="hlt">2</span> hours and 95% vs. 63% at 4 hours, P < .001). Mean abdominal pain scores <span class="hlt">2</span> and 4 hours after the procedure were statistically significantly lower in the <span class="hlt">CO</span>(<span class="hlt">2</span>) group compared with the control <span class="hlt">air</span> group (0.5 vs <span class="hlt">2</span>.6 at <span class="hlt">2</span> hours and 0.1 vs 1.<span class="hlt">2</span> at 4 hours, P < .001). There was no difference in waist circumference between the <span class="hlt">2</span> groups at all time intervals. The results of this randomized trial show clear benefits of <span class="hlt">CO</span>(<span class="hlt">2</span>) insufflation for colonoscopy in reducing postprocedural discomfort. ( NCT02407639.). Copyright © 2016 American Society for Gastrointestinal Endoscopy. Published by Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4348458','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4348458"><span>Experimental and modeling study on effects of N<span class="hlt">2</span> and <span class="hlt">CO</span><span class="hlt">2</span> on ignition characteristics of methane/<span class="hlt">air</span> mixture</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Zeng, Wen; Ma, Hongan; Liang, Yuntao; Hu, Erjiang</p> <p>2014-01-01</p> <p>The ignition delay times of methane/<span class="hlt">air</span> mixture diluted by N<span class="hlt">2</span> and <span class="hlt">CO</span><span class="hlt">2</span> were experimentally measured in a chemical shock tube. The experiments were performed over the temperature range of 1300–2100 K, pressure range of 0.1–1.0 MPa, equivalence ratio range of 0.5–<span class="hlt">2</span>.0 and for the dilution coefficients of 0%, 20% and 50%. The results suggest that a linear relationship exists between the reciprocal of temperature and the logarithm of the ignition delay times. Meanwhile, with ignition temperature and pressure increasing, the measured ignition delay times of methane/<span class="hlt">air</span> mixture are decreasing. Furthermore, an increase in the dilution coefficient of N<span class="hlt">2</span> or <span class="hlt">CO</span><span class="hlt">2</span> results in increasing ignition delays and the inhibition effect of <span class="hlt">CO</span><span class="hlt">2</span> on methane/<span class="hlt">air</span> mixture ignition is stronger than that of N<span class="hlt">2</span>. Simulated ignition delays of methane/<span class="hlt">air</span> mixture using three kinetic models were compared to the experimental data. Results show that GRI_3.0 mechanism gives the best prediction on ignition delays of methane/<span class="hlt">air</span> mixture and it was selected to identify the effects of N<span class="hlt">2</span> and <span class="hlt">CO</span><span class="hlt">2</span> on ignition delays and the key elementary reactions in the ignition chemistry of methane/<span class="hlt">air</span> mixture. Comparisons of the calculated ignition delays with the experimental data of methane/<span class="hlt">air</span> mixture diluted by N<span class="hlt">2</span> and <span class="hlt">CO</span><span class="hlt">2</span> show excellent agreement, and sensitivity coefficients of chain branching reactions which promote mixture ignition decrease with increasing dilution coefficient of N<span class="hlt">2</span> or <span class="hlt">CO</span><span class="hlt">2</span>. PMID:25750753</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/2014EGUGA..16.3224K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.3224K"><span>Different nature of glacial Ca<span class="hlt">CO</span>3 constituents between MIS <span class="hlt">2</span> and MIS 12 in the East <span class="hlt">Sea</span>/Japan <span class="hlt">Sea</span> and its paleoceanographic implication</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Khim, Boo-Keun; Tada, Ryuji; Itaki, Takuya</p> <p>2014-05-01</p> <p>Two piston cores (PC-05 and PC-08) were collected on the Yamato Rise in the East <span class="hlt">Sea</span>/Japan <span class="hlt">Sea</span> during the KR07-12 cruise. A composite core was achieved with the successful replacement of almost half of the upper part of core PC-05 by the entirety of core PC-08 based on the <span class="hlt">co</span>-equivalence of L* values and the dark layers, because an interval (170 cm to 410 cm) of core PC-05 was considerably disturbed due to fluidization during the core execution. Chronostratigraphy of the composite core was constructed by the direct comparison of L* values to the well-dated core MD01-2407 that was obtained in the Oki Ridge. The lower-bottom of the composite core reached back to Marine Isotope Stage (MIS) 14, based on the age estimate by LR04 stacks. Downcore opal variation of the composite core exhibited the distinct orbital-scale cyclic changes; high during the interglacial and low during the glacial periods. However, downcore Ca<span class="hlt">CO</span>3 variation showed no corresponding orbital-scale cyclic change between glacial and interglacial periods. Some intervals of both periods were high in Ca<span class="hlt">CO</span>3 content. Frequent and large fluctuations in Ca<span class="hlt">CO</span>3 content seemed to be more related to the presence of dark layers containing thin lamination (TL) within the glacial and interglacial intervals. It is worthy to note that MIS <span class="hlt">2</span> and MIS 12 are characterized by distinctly high Ca<span class="hlt">CO</span>3 content, showing up to 18% and 73%, respectively, among the glacial periods. Furthermore, in terms of lithology, MIS <span class="hlt">2</span> was characterized by a thick dark layer (low L* values) with TL, whereas MIS 12 preserved the distinctly light layer (high L* values) with parallel laminations. Another remarkable dissimilarity between MIS <span class="hlt">2</span> and MIS 12 was the nature of their Ca<span class="hlt">CO</span>3 constituent; the Ca<span class="hlt">CO</span>3 constituent of MIS <span class="hlt">2</span> consisted of mostly planktonic foraminifera, whereas that of MIS 12 was mostly dump of coccolithophorids, regardless the presence of planktonic foraminifera. The distinctness of the Ca<span class="hlt">CO</span>3 constituents between MIS <span class="hlt">2</span> and MIS</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> fluxes</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> fluxes at a global scale is developed. The framework evaluates the interplay between (1) surface heat and freshwater fluxes 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 flux 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 flux 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> fluxes driven by surface heat fluxes and a combination of biologically driven carbon uptake and disequilibrium-driven carbon outgassing. The framework is still able to reconstruct simulated fluxes 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> flux of <span class="hlt">CO</span><span class="hlt">2</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/53171','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/53171"><span>A dynamic leaf gas-<span class="hlt">exchange</span> strategy is conserved in woody plants under changing ambient <span class="hlt">CO</span><span class="hlt">2</span> : evidence from carbon isotope discrimination in paleo and <span class="hlt">CO</span><span class="hlt">2</span> enrichment studies</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Steven L. Voelker; J. Renee Brooks; Frederick C. Meinzer; Rebecca Anderson; Martin K.-F. Bader; Giovanna Battipaglia; Katie M. Becklin; David Beerling; Didier Bert; Julio L. Betancourt; Todd E. Dawson; Jean-Christophe Domec; Richard P. Guyette; Christian K??rner; Steven W. Leavitt; Sune Linder; John D. Marshall; Manuel Mildner; Jerome Ogee; Irina Panyushkina; Heather J. Plumpton; Kurt S. Pregitzer; Matthias Saurer; Andrew R. Smith; Rolf T. W. Siegwolf; Michael C. Stambaugh; Alan F. Talhelm; Jacques C. Tardif; Peter K. Van de Water; Joy K. Ward; Lisa Wingate</p> <p>2016-01-01</p> <p>Rising atmospheric [<span class="hlt">CO</span><span class="hlt">2</span>], ca, is expected to affect stomatal regulation of leaf gas-<span class="hlt">exchange</span> of woody plants, thus influencing energy fluxes as well as carbon (C), water, and nutrient cycling of forests. Researchers have proposed various strategies for stomatal regulation of leaf gas-<span class="hlt">exchange</span> that include maintaining a constant leaf internal [<span class="hlt">CO</span>...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGC21F0995B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC21F0995B"><span>Reconciling top-down and bottom-up estimates of <span class="hlt">CO</span><span class="hlt">2</span> fluxes to understand increased seasonal <span class="hlt">exchange</span> in Northern ecosystems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bastos, A.; Ciais, P.; Zhu, D.; Maignan, F.; Wang, X.; Chevallier, F.; Ballantyne, A.</p> <p>2017-12-01</p> <p>Continuous atmospheric <span class="hlt">CO</span><span class="hlt">2</span> monitoring data indicate enhanced seasonal <span class="hlt">exchange</span> in the high-latitudes in the Northern Hemisphere (above 40oN), mainly attributed to terrestrial ecosystems. Whether this enhancement is mostly explained by increased vegetation growth due to <span class="hlt">CO</span><span class="hlt">2</span> fertilization and warming, or by changes in land-use and land-management practices is still an unsettled question (e.g. Forkel et al. (2016) and Zeng et al. (2013)). Previous studies have shown that models present variable performance in capturing trends in <span class="hlt">CO</span><span class="hlt">2</span> amplitude at <span class="hlt">CO</span><span class="hlt">2</span> monitoring sites, and that Earth System Models present large spread in their estimates of such trends. Here we integrate data of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> in terrestrial ecosystems by a set of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> inversions and a range of land-surface models to evaluate the ability of models to reproduce changes in <span class="hlt">CO</span><span class="hlt">2</span> seasonal <span class="hlt">exchange</span> within the observation uncertainty. We then analyze the factors that explain the model spread to understand if the trend in seasonal <span class="hlt">CO</span><span class="hlt">2</span> amplitude may indeed be a useful metric to constrain future changes in terrestrial photosynthesis (Wenzel et al., 2016). We then compare model simulations with satellite and other observation-based datasets of vegetation productivity, biomass stocks and land-cover change to test the contribution of natural (<span class="hlt">CO</span><span class="hlt">2</span> fertilization, climate) and human (land-use change) factors to the increasing trend in seasonal <span class="hlt">CO</span><span class="hlt">2</span> amplitude. Forkel, Matthias, et al. "Enhanced seasonal <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> caused by amplified plant productivity in northern ecosystems." Science 351.6274 (2016): 696-699. Wenzel, Sabrina, et al. "Projected land photosynthesis constrained by changes in the seasonal cycle of atmospheric <span class="hlt">CO</span><span class="hlt">2</span>." Nature 538, no. 7626 (2016): 499-501.Zeng, Ning, et al. "Agricultural Green Revolution as a driver of increasing atmospheric <span class="hlt">CO</span><span class="hlt">2</span> seasonal amplitude." Nature 515.7527 (2014): 394.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4737892','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4737892"><span>A Comparative Data-Based Modeling Study on Respiratory <span class="hlt">CO</span><span class="hlt">2</span> Gas <span class="hlt">Exchange</span> during Mechanical Ventilation</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Kim, Chang-Sei; Ansermino, J. Mark; Hahn, Jin-Oh</p> <p>2016-01-01</p> <p>The goal of this study is to derive a minimally complex but credible model of respiratory <span class="hlt">CO</span><span class="hlt">2</span> gas <span class="hlt">exchange</span> that may be used in systematic design and pilot testing of closed-loop end-tidal <span class="hlt">CO</span><span class="hlt">2</span> controllers in mechanical ventilation. We first derived a candidate model that captures the essential mechanisms involved in the respiratory <span class="hlt">CO</span><span class="hlt">2</span> gas <span class="hlt">exchange</span> process. Then, we simplified the candidate model to derive two lower-order candidate models. We compared these candidate models for predictive capability and reliability using experimental data collected from 25 pediatric subjects undergoing dynamically varying mechanical ventilation during surgical procedures. A two-compartment model equipped with transport delay to account for <span class="hlt">CO</span><span class="hlt">2</span> delivery between the lungs and the tissues showed modest but statistically significant improvement in predictive capability over the same model without transport delay. Aggregating the lungs and the tissues into a single compartment further degraded the predictive fidelity of the model. In addition, the model equipped with transport delay demonstrated superior reliability to the one without transport delay. Further, the respiratory parameters derived from the model equipped with transport delay, but not the one without transport delay, were physiologically plausible. The results suggest that gas transport between the lungs and the tissues must be taken into account to accurately reproduce the respiratory <span class="hlt">CO</span><span class="hlt">2</span> gas <span class="hlt">exchange</span> process under conditions of wide-ranging and dynamically varying mechanical ventilation conditions. PMID:26870728</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22420805-sodium-citrate-assisted-anion-exchange-strategy-construction-bi-sub-sub-co-sub-bioi-photocatalysts','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22420805-sodium-citrate-assisted-anion-exchange-strategy-construction-bi-sub-sub-co-sub-bioi-photocatalysts"><span>Sodium citrate-assisted anion <span class="hlt">exchange</span> strategy for construction of Bi{sub <span class="hlt">2</span>}O{sub <span class="hlt">2</span>}<span class="hlt">CO</span>{sub 3}/BiOI photocatalysts</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>Song, Peng-Yuan; Xu, Ming; Zhang, Wei-De, E-mail: zhangwd@scut.edu.cn</p> <p></p> <p>Highlights: • Heterostructured Bi{sub <span class="hlt">2</span>}O{sub <span class="hlt">2</span>}<span class="hlt">CO</span>{sub 3}/BiOI microspheres were prepared via anion <span class="hlt">exchange</span>. • Sodium citrate-assisted anion <span class="hlt">exchange</span> for construction of composite photocatalysts. • Bi{sub <span class="hlt">2</span>}O{sub <span class="hlt">2</span>}<span class="hlt">CO</span>{sub 3}/BiOI composites show high visible light photocatalytic activity. - Abstract: Bi{sub <span class="hlt">2</span>}O{sub <span class="hlt">2</span>}<span class="hlt">CO</span>{sub 3}/BiOI heterojuncted photocatalysts were constructed through a facile partial anion <span class="hlt">exchange</span> strategy starting from BiOI microspheres and urea with the assistance of sodium citrate. The content of Bi{sub <span class="hlt">2</span>}O{sub <span class="hlt">2</span>}<span class="hlt">CO</span>{sub 3} in the catalysts was regulated by modulating the amount of urea as a precursor, which was decomposed to generate <span class="hlt">CO</span>{sub 3}{sup <span class="hlt">2</span>−} in the hydrothermal process. Citrate anion playsmore » a key role in controlling the morphology and composition of the products. The Bi{sub <span class="hlt">2</span>}O{sub <span class="hlt">2</span>}<span class="hlt">CO</span>{sub 3}/BiOI catalysts display much higher photocatalytic activity than pure BiOI and Bi{sub <span class="hlt">2</span>}O{sub <span class="hlt">2</span>}<span class="hlt">CO</span>{sub 3} towards the degradation of rhodamine B (RhB) and bisphenol A (BPA). The enhancement of photocatalytic activity of the heterojuncted catalysts is attributed to the formation of p–n junction between p-BiOI and n-Bi{sub <span class="hlt">2</span>}O{sub <span class="hlt">2</span>}<span class="hlt">CO</span>{sub 3}, which is favorable for retarding the recombination of photoinduced electron-hole pairs. Moreover, the holes are demonstrated to be the main active species for the degradation of RhB and BPA.« less</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> Flux 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> fluxes 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 flux 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 flux measurements remains controversial. Here we use eddy covariance momentum flux measurements obtained onboard RRS James Clark Ross as part of the Waves, Aerosol and Gas <span class="hlt">Exchange</span> Study (WAGES), a programme of near-continuous measurements using the autonomous AutoFlux 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 flux 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.: AutoFlux: an autonomous system for the direct measurement of the <span class="hlt">air-sea</span> fluxes 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('https://www.osti.gov/biblio/1347013-structure-property-relationships-cation-exchanged-zk-zeolites-co-adsorption','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1347013-structure-property-relationships-cation-exchanged-zk-zeolites-co-adsorption"><span>On the Structure-Property Relationships of Cation-<span class="hlt">Exchanged</span> ZK-5 Zeolites for <span class="hlt">CO</span> <span class="hlt">2</span> Adsorption</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>Pham, Trong D.; Hudson, Matthew R.; Brown, Craig M.</p> <p>2017-02-16</p> <p>The <span class="hlt">CO</span> <span class="hlt">2</span> adsorption properties of cation-<span class="hlt">exchanged</span> Li-, Na-, K-, and Mg-ZK-5 zeolites were correlated to the molecular structures determined by Rietveld refinements of synchrotron powder X-ray diffraction patterns. Li-, K-, and Na-ZK-5 all exhibited high isosteric heats of adsorption (Qst) at low <span class="hlt">CO</span> <span class="hlt">2</span> coverage, with Na-ZK-5 having the highest Qst (ca. 49 kJ mol -1). Mg<span class="hlt">2</span>+ was located at the center of the zeolite hexagonal prism with the cation inaccessible to <span class="hlt">CO</span> <span class="hlt">2</span>, leading to a much lower Qst (ca. 30 kJ mol-1) and lower overall uptake capacity. Multiple <span class="hlt">CO</span> <span class="hlt">2</span> adsorption sites were identified at a givenmore » <span class="hlt">CO</span> <span class="hlt">2</span> loading amount for all four cation-<span class="hlt">exchanged</span> ZK-5 adsorbents. Site A at the flat eight-membered ring windows and site B/B* in the γ-cages were the primary adsorption sites in Li - and Na-ZK-5 zeolites. Relatively strong dual-cation adsorption sites contributed significantly to an enhanced electrostatic interaction for <span class="hlt">CO</span> <span class="hlt">2</span> in all ZK-5 samples. This interaction gives rise to a migration of Li + and Mg <span class="hlt">2</span>+ cations from their original locations at the center of the hexagonal prisms toward the α-cages, in which they interact more strongly with the adsorbed <span class="hlt">CO</span> <span class="hlt">2</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A33G2449C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A33G2449C"><span>Influence of the biosphere and circulation on atmospheric <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>Corbett, A.; Jiang, X.; La, J.; Olsen, E. T.; Licata, S. J.; Yung, Y. L.</p> <p>2017-12-01</p> <p>Using multiple satellite <span class="hlt">CO</span><span class="hlt">2</span> retrievals (e.g., <span class="hlt">AIRS</span>, GOSAT, and OCO-<span class="hlt">2</span>), we have investigated seasonal changes of <span class="hlt">CO</span><span class="hlt">2</span> as a function of latitudes and altitudes. The annual cycle of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> is closely related to the <span class="hlt">exchange</span> of <span class="hlt">CO</span><span class="hlt">2</span> between the biosphere and the atmosphere, so we also examine solar-induced fluorescence (SIF). High SIF value means more <span class="hlt">CO</span><span class="hlt">2</span> uptake by photosynthesis, which will lead to lower atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentrations. The satellite data demonstrate a negative correlation between atmospheric <span class="hlt">CO</span><span class="hlt">2</span> and SIF. SIF can be influenced by precipitation and evaporation. We have found a positive correlation between SIF and the difference of precipitation and evaporation, suggesting there is more <span class="hlt">CO</span><span class="hlt">2</span> uptake by vegetation when more water is available. In addition to the annual cycle, large-scale circulation, such as South Atlantic Walker Circulation, can also modulate atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentrations. As seen from <span class="hlt">AIRS</span>, GOSAT, and OCO-<span class="hlt">2</span> <span class="hlt">CO</span><span class="hlt">2</span> retrievals, there is less <span class="hlt">CO</span><span class="hlt">2</span> over the South Atlantic Ocean than over South America from December to March. Results in this study will help us better understand interactions between the biosphere, circulation, and atmospheric <span class="hlt">CO</span><span class="hlt">2</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017APS..MARB12008G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..MARB12008G"><span><span class="hlt">Exchange</span>-coupled Fe3O4/<span class="hlt">Co</span>Fe<span class="hlt">2</span>O4 nanoparticles for advanced magnetic hyperthermia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Glassell, M.; Robles, J.; Das, R.; Phan, M. H.; Srikanth, H.</p> <p></p> <p>Iron oxide nanoparticles especially Fe3O4, γ-Fe<span class="hlt">2</span>O3 have been extensively studied for magnetic hyperthermia because of their tunable magnetic properties and stable suspension in superparamagnetic regime. However, their relatively low heating capacity hindered practical application. Recently, a large improvement in heating efficiency has been reported in <span class="hlt">exchange</span>-coupled nanoparticles with <span class="hlt">exchange</span> coupling between soft and hard magnetic phases. Here, we systematically studied the effect of core and shell size on the heating efficiency of the Fe3O4/<span class="hlt">Co</span>Fe<span class="hlt">2</span>O4 core/shell nanoparticles. The nanoparticles were synthesized using thermal decomposition of organometallic precursors. Transmission electron microscopy (TEM) showed formation of spherical shaped Fe3O4 and Fe3O-/<span class="hlt">Co</span>Fe<span class="hlt">2</span>O4 nanoparticles. Magnetic measurements showed high magnetization (≅70 emu/g) and superparamagnetic behavior for the nanoparticles at room temperature. Magnetic hyperthermia results showed a large increase in specific absorption rate (SAR) for 8nm Fe3O4/<span class="hlt">Co</span>Fe<span class="hlt">2</span>O4 compared to Fe3O4 nanoparticles of the same size. The heating efficiency of the Fe3O4/<span class="hlt">Co</span>Fe<span class="hlt">2</span>O4 with 1 nm <span class="hlt">Co</span>Fe<span class="hlt">2</span>O4 (shell) increased from 207 to 220 W/g (for 800 Oe) with increase in core size from 6 to 8 nm. The heating efficiency of the Fe3O4/<span class="hlt">Co</span>Fe<span class="hlt">2</span>O4 with <span class="hlt">2</span> nm <span class="hlt">Co</span>Fe<span class="hlt">2</span>O4 (shell) and core size of 8 nm increased from 220 to 460 W/g (for 800 Oe). These <span class="hlt">exchange</span>-coupled Fe3O4/<span class="hlt">Co</span>Fe<span class="hlt">2</span>O4 core/shell nanoparticles can be a good candidate for advanced hyperthermia application.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20627898','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20627898"><span>Effects of elevated root zone <span class="hlt">CO</span><span class="hlt">2</span> and <span class="hlt">air</span> temperature on photosynthetic gas <span class="hlt">exchange</span>, nitrate uptake, and total reduced nitrogen content in aeroponically grown lettuce plants.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>He, Jie; Austin, Paul T; Lee, Sing Kong</p> <p>2010-09-01</p> <p>Effects of elevated root zone (RZ) <span class="hlt">CO</span>(<span class="hlt">2</span>) and <span class="hlt">air</span> temperature on photosynthesis, productivity, nitrate (NO(3)(-)), and total reduced nitrogen (N) content in aeroponically grown lettuce plants were studied. Three weeks after transplanting, four different RZ [<span class="hlt">CO</span>(<span class="hlt">2</span>)] concentrations [ambient (360 ppm) and elevated concentrations of 2000, 10,000, and 50,000 ppm] were imposed on plants grown at two <span class="hlt">air</span> temperature regimes of 28 degrees C/22 degrees C (day/night) and 36 degrees C/30 degrees C. Photosynthetic <span class="hlt">CO</span>(<span class="hlt">2</span>) assimilation (A) and stomatal conductance (g(s)) increased with increasing photosynthetically active radiation (PAR). When grown at 28 degrees C/22 degrees C, all plants accumulated more biomass than at 36 degrees C/30 degrees C. When measured under a PAR >or=600 micromol m(-<span class="hlt">2</span>) s(-1), elevated RZ [<span class="hlt">CO</span>(<span class="hlt">2</span>)] resulted in significantly higher A, lower g(s), and higher midday leaf relative water content in all plants. Under elevated RZ [<span class="hlt">CO</span>(<span class="hlt">2</span>)], the increase of biomass was greater in roots than in shoots, causing a lower shoot/root ratio. The percentage increase in growth under elevated RZ [<span class="hlt">CO</span>(<span class="hlt">2</span>)] was greater at 36 degrees C/30 degrees C although the total biomass was higher at 28 degrees C/22 degrees C. NO(3)(-) and total reduced N concentrations of shoot and root were significantly higher in all plants under elevated RZ [<span class="hlt">CO</span>(<span class="hlt">2</span>)] than under ambient RZ [<span class="hlt">CO</span>(<span class="hlt">2</span>)] of 360 ppm at both temperature regimes. At each RZ [<span class="hlt">CO</span>(<span class="hlt">2</span>)], NO(3)(-) and total reduced N concentration of shoots were greater at 28 degrees C/22 degrees C than at 36 degrees C/30 degrees C. At all RZ [<span class="hlt">CO</span>(<span class="hlt">2</span>)], roots of plants at 36 degrees C/30 degrees C had significantly higher NO(3)(-) and total reduced N concentrations than at 28 degrees C/22 degrees C. Since increased RZ [<span class="hlt">CO</span>(<span class="hlt">2</span>)] caused partial stomatal closure, maximal A and maximal g(s) were negatively correlated, with a unique relationship for each <span class="hlt">air</span> temperature. However, across all RZ [<span class="hlt">CO</span>(<span class="hlt">2</span>)] and temperature treatments, there was a close correlation between</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AIPA....7e6225W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AIPA....7e6225W"><span><span class="hlt">Exchange</span>-coupled hard magnetic Fe-<span class="hlt">Co/Co</span>Pt nanocomposite films fabricated by electro-infiltration</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wen, Xiao; Andrew, Jennifer S.; Arnold, David P.</p> <p>2017-05-01</p> <p>This paper introduces a potentially scalable electro-infiltration process to produce <span class="hlt">exchange</span>-coupled hard magnetic nanocomposite thin films. Fe-<span class="hlt">Co/Co</span>Pt nanocomposite films are fabricated by deposition of <span class="hlt">Co</span>Fe<span class="hlt">2</span>O4 nanoparticles onto Si substrate, followed by electroplating of <span class="hlt">Co</span>Pt. Samples are subsequently annealed under H<span class="hlt">2</span> to reduce the <span class="hlt">Co</span>Fe<span class="hlt">2</span>O4 to magnetically soft Fe-<span class="hlt">Co</span> and also induce L10 ordering in the <span class="hlt">Co</span>Pt. Resultant films exhibit 0.97 T saturation magnetization, 0.70 T remanent magnetization, 127 kA/m coercivity and 21.8 kJ/m3 maximum energy density. First order reversal curve (FORC) analysis and δM plot are used to prove the <span class="hlt">exchange</span> coupling between soft and hard magnetic phases.</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> fluxes 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('http://adsabs.harvard.edu/abs/2008JNuM..374..123L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008JNuM..374..123L"><span>Change of properties after oxidation of IG-11 graphite by <span class="hlt">air</span> and <span class="hlt">CO</span> <span class="hlt">2</span> gas</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lim, Yun-Soo; Chi, Se-Hwan; Cho, Kwang-Yun</p> <p>2008-02-01</p> <p>Artificial graphite is typically manufactured by carbonization of a shaped body of a kneaded mixture using granular cokes as a filler and pitch as a binder. It undergoes a pitch impregnation process if necessary and finally applying graphitization heat treatment. The effect of thermal oxidation in <span class="hlt">air</span> or a <span class="hlt">CO</span> <span class="hlt">2</span> atmosphere on IG-11 graphite samples is investigated in this study. The results show a localized oxidation process that progressively reveals the large coke particles with increasing level of overall weight loss in <span class="hlt">air</span>. The surface of the graphite was peeled off and no change was found in the specific gravity after <span class="hlt">air</span> oxidation. However, the specific gravity of graphite was continuously decreased by <span class="hlt">CO</span> <span class="hlt">2</span> oxidation. The decrease in the specific gravity by <span class="hlt">CO</span> <span class="hlt">2</span> oxidation was due to <span class="hlt">CO</span> <span class="hlt">2</span> gas that progressed from the surface to the interior. The pore shape after <span class="hlt">CO</span> <span class="hlt">2</span> oxidation differed from that under <span class="hlt">air</span> oxidation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/11746880','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/11746880"><span>Extraction of <span class="hlt">CO</span><span class="hlt">2</span> from <span class="hlt">air</span> samples for isotopic analysis and limits to ultra high precision delta18O determination in <span class="hlt">CO</span><span class="hlt">2</span> gas.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Werner, R A; Rothe, M; Brand, W A</p> <p>2001-01-01</p> <p>The determination of delta18O values in <span class="hlt">CO</span><span class="hlt">2</span> at a precision level of +/-0.02 per thousand (delta-notation) has always been a challenging, if not impossible, analytical task. Here, we demonstrate that beyond the usually assumed major cause of uncertainty - water contamination - there are other, hitherto underestimated sources of contamination and processes which can alter the oxygen isotope composition of <span class="hlt">CO</span><span class="hlt">2</span>. Active surfaces in the preparation line with which <span class="hlt">CO</span><span class="hlt">2</span> comes into contact, as well as traces of <span class="hlt">air</span> in the sample, can alter the apparent delta18O value both temporarily and permanently. We investigated the effects of different surface materials including electropolished stainless steel, Duran glass, gold and quartz, the latter both untreated and silanized. <span class="hlt">CO</span><span class="hlt">2</span> frozen with liquid nitrogen showed a transient alteration of the 18O/16O ratio on all surfaces tested. The time to recover from the alteration as well as the size of the alteration varied with surface type. Quartz that had been ultrasonically cleaned for several hours with high purity water (0.05 microS) exhibited the smallest effect on the measured oxygen isotopic composition of <span class="hlt">CO</span><span class="hlt">2</span> before and after freezing. However, quartz proved to be mechanically unstable with time when subjected to repeated large temperature changes during operation. After several days of operation the gas released from the freezing step contained progressively increasing trace amounts of O<span class="hlt">2</span> probably originating from inclusions within the quartz, which precludes the use of quartz for cryogenically trapping <span class="hlt">CO</span><span class="hlt">2</span>. Stainless steel or gold proved to be suitable materials after proper pre-treatment. To ensure a high trapping efficiency of <span class="hlt">CO</span><span class="hlt">2</span> from a flow of gas, a cold trap design was chosen comprising a thin wall 1/4" outer tube and a 1/8" inner tube, made respectively from electropolished stainless steel and gold. Due to a considerable 18O specific isotope effect during the release of <span class="hlt">CO</span><span class="hlt">2</span> from the cold surface, the thawing time had to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=81674&keyword=face+AND+time&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=81674&keyword=face+AND+time&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>REDUCED STOMATAL CONDUCTANCE IN SWEETGUM (LIQUIDAMBAR STYRACIFLUA) SUSTAINED OVER LONG-TERM <span class="hlt">CO</span><span class="hlt">2</span> ENRICHMENT</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>Over four years (1998-2001), we examined the effects of <span class="hlt">CO</span><span class="hlt">2</span> enrichment on stomatal conductance (gs) of sun and shade leaves of overstory sweetgum (Liquidambar styraciflua L.) grown at the Duke Forest Free <span class="hlt">Air</span> Carbon <span class="hlt">CO</span><span class="hlt">2</span> Enrichment (FACE) experiment. Gas <span class="hlt">exchange</span> measurements were...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.2220H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.2220H"><span>Effects of winter temperature and summer drought on net ecosystem <span class="hlt">exchange</span> of <span class="hlt">CO</span><span class="hlt">2</span> in a temperate peatland</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Helfter, Carole; Campbell, Claire; Dinsmore, Kerry; Drewer, Julia; Coyle, Mhairi; Anderson, Margaret; Skiba, Ute; Nemitz, Eiko; Billett, Michael; Sutton, Mark</p> <p>2014-05-01</p> <p>Northern peatlands are one of the most important global sinks of atmospheric carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>); their ability to sequester C is a natural feedback mechanism controlled by climatic variables such as precipitation, temperature, length of growing season and period of snow cover. In the UK it has been predicted that peatlands could become a net source of carbon in response to climate change with climate models predicting a rise in global temperature of ca. 3oC between 1961-1990 and 2100. Land-atmosphere <span class="hlt">exchange</span> of <span class="hlt">CO</span><span class="hlt">2</span>in peatlands exhibits marked seasonal and inter-annual variations, which have significant short- and long-term effects on carbon sink strength. Net ecosystem <span class="hlt">exchange</span> (NEE) of <span class="hlt">CO</span><span class="hlt">2</span> has been measured continuously by eddy-covariance (EC) at Auchencorth Moss (55° 47'32 N, 3° 14'35 W, 267 m a.s.l.), a temperate peatland in central Scotland, since 2002. Auchencorth Moss is a low-lying, ombrotrophic peatland situated ca. 20 km south-west of Edinburgh. Peat depth ranges from 5 m and the site has a mean annual precipitation of 1155 mm. The vegetation present within the flux measurement footprint comprises mixed grass species, heather and substantial areas of moss species (Sphagnum spp. and Polytrichum spp.). The EC system consists of a LiCOR 7000 closed-path infrared gas analyser for the simultaneous measurement of <span class="hlt">CO</span><span class="hlt">2</span> and water vapour and of a Gill Windmaster Pro ultrasonic anemometer. Over the 10 year period, the site was a consistent yet variable sink of <span class="hlt">CO</span><span class="hlt">2</span> ranging from -34.1 to -135.9 g <span class="hlt">CO</span><span class="hlt">2</span>-C m-<span class="hlt">2</span> yr-1 (mean of -69.1 ± 33.6 g <span class="hlt">CO</span><span class="hlt">2</span>-C m-<span class="hlt">2</span> yr-1). Inter-annual variability in NEE was positively correlated to the length of the growing seasons and mean winter <span class="hlt">air</span> temperature explained 93% of the variability in summertime sink strength, indicating a phenological memory-effect. Plant development and productivity were stunted by colder winters causing a net reduction in the annual carbon sink strength of this peatland where autotrophic processes are thought to be</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015PrOce.138...18D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PrOce.138...18D"><span>Nitrous oxide and methane in Atlantic and Mediterranean waters in the Strait of Gibraltar: <span class="hlt">Air-sea</span> fluxes and inter-basin <span class="hlt">exchange</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>de la Paz, M.; Huertas, I. E.; Flecha, S.; Ríos, A. F.; Pérez, F. F.</p> <p>2015-11-01</p> <p>The global ocean plays an important role in the overall budget of nitrous oxide (N<span class="hlt">2</span>O) and methane (CH4), as both gases are produced within the ocean and released to the atmosphere. However, for large parts of the open and coastal oceans there is little or no spatial data coverage for N<span class="hlt">2</span>O and CH4. Hence, a better assessment of marine emissions estimates is necessary. As a contribution to remedying the scarcity of data on marine regions, N<span class="hlt">2</span>O and CH4 concentrations have been determined in the Strait of Gibraltar at the ocean Fixed Time series (GIFT). During six cruises performed between July 2011 and November 2014 samples were collected at the surface and various depths in the water column, and subsequently measured using gas chromatography. From this we were able to quantify the temporal variability of the gas <span class="hlt">air-sea</span> <span class="hlt">exchange</span> in the area and examine the vertical distribution of N<span class="hlt">2</span>O and CH4 in Atlantic and Mediterranean waters. Results show that surface Atlantic waters are nearly in equilibrium with the atmosphere whereas deeper Mediterranean waters are oversaturated in N<span class="hlt">2</span>O, and a gradient that gradually increases with depth was detected in the water column. Temperature was found to be the main factor responsible for the seasonal variability of N<span class="hlt">2</span>O in the surface layer. Furthermore, although CH4 levels did not reveal any feature clearly associated with the circulation of water masses, vertical distributions showed that higher concentrations are generally observed in the Atlantic layer, and that the deeper Mediterranean waters are considerably undersaturated (by up to 50%). Even though surface waters act as a source of atmospheric N<span class="hlt">2</span>O during certain periods, on an annual basis the net N<span class="hlt">2</span>O flux in the Strait of Gibraltar is only 0.35 ± 0.27 μmol m-<span class="hlt">2</span> d-1, meaning that these waters are almost in a neutral status with respect to the atmosphere. Seasonally, the region behaves as a slight sink for atmospheric CH4 in winter and as a source in spring and fall. Approximating</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27110991','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27110991"><span>Geospatial variability of soil <span class="hlt">CO</span><span class="hlt">2</span>-C <span class="hlt">exchange</span> in the main terrestrial ecosystems of Keller Peninsula, Maritime Antarctica.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Thomazini, A; Francelino, M R; Pereira, A B; Schünemann, A L; Mendonça, E S; Almeida, P H A; Schaefer, C E G R</p> <p>2016-08-15</p> <p>Soils and vegetation play an important role in the carbon <span class="hlt">exchange</span> in Maritime Antarctica but little is known on the spatial variability of carbon processes in Antarctic terrestrial environments. The objective of the current study was to investigate (i) the soil development and (ii) spatial variability of ecosystem respiration (ER), net ecosystem <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> (NEE), gross primary production (GPP), soil temperature (ST) and soil moisture (SM) under four distinct vegetation types and a bare soil in Keller Peninsula, King George Island, Maritime Antarctica, as follows: site 1: moss-turf community; site <span class="hlt">2</span>: moss-carpet community; site 3: phanerogamic antarctic community; site 4: moss-carpet community (predominantly colonized by Sanionia uncinata); site 5: bare soil. Soils were sampled at different layers. A regular 40-point (5×8 m) grid, with a minimum separation distance of 1m, was installed at each site to quantify the spatial variability of carbon <span class="hlt">exchange</span>, soil moisture and temperature. Vegetation characteristics showed closer relation with soil development across the studied sites. ER reached <span class="hlt">2</span>.26μmol<span class="hlt">CO</span><span class="hlt">2</span>m(-<span class="hlt">2</span>)s(-1) in site 3, where ST was higher (7.53°C). A greater sink effect was revealed in site 4 (net uptake of 1.54μmol<span class="hlt">CO</span><span class="hlt">2</span>m(-<span class="hlt">2</span>)s(-1)) associated with higher SM (0.32m(3)m(-3)). Spherical models were fitted to describe all experimental semivariograms. Results indicate that ST and SM are directly related to the spatial variability of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span>. Heterogeneous vegetation patches showed smaller range values. Overall, poorly drained terrestrial ecosystems act as <span class="hlt">CO</span><span class="hlt">2</span> sink. Conversely, where ER is more pronounced, they are associated with intense soil carbon mineralization. The formations of new ice-free areas, depending on the local soil drainage condition, have an important effect on <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span>. With increasing ice/snow melting, and resulting widespread waterlogging, increasing <span class="hlt">CO</span><span class="hlt">2</span> sink in terrestrial ecosystems is expected for Maritime Antarctica. Copyright </p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AMT.....9.3687J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AMT.....9.3687J"><span>A new set-up for simultaneous high-precision measurements of <span class="hlt">CO</span><span class="hlt">2</span>, δ13C-<span class="hlt">CO</span><span class="hlt">2</span> and δ18O-<span class="hlt">CO</span><span class="hlt">2</span> on small ice core samples</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jenk, Theo Manuel; Rubino, Mauro; Etheridge, David; Ciobanu, Viorela Gabriela; Blunier, Thomas</p> <p>2016-08-01</p> <p>Palaeoatmospheric records of carbon dioxide and its stable carbon isotope composition (δ13C) obtained from polar ice cores provide important constraints on the natural variability of the carbon cycle. However, the measurements are both analytically challenging and time-consuming; thus only data exist from a limited number of sampling sites and time periods. Additional analytical resources with high analytical precision and throughput are thus desirable to extend the existing datasets. Moreover, consistent measurements derived by independent laboratories and a variety of analytical systems help to further increase confidence in the global <span class="hlt">CO</span><span class="hlt">2</span> palaeo-reconstructions. Here, we describe our new set-up for simultaneous measurements of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> mixing ratios and atmospheric δ13C and δ18O-<span class="hlt">CO</span><span class="hlt">2</span> in <span class="hlt">air</span> extracted from ice core samples. The centrepiece of the system is a newly designed needle cracker for the mechanical release of <span class="hlt">air</span> entrapped in ice core samples of 8-13 g operated at -45 °C. The small sample size allows for high resolution and replicate sampling schemes. In our method, <span class="hlt">CO</span><span class="hlt">2</span> is cryogenically and chromatographically separated from the bulk <span class="hlt">air</span> and its isotopic composition subsequently determined by continuous flow isotope ratio mass spectrometry (IRMS). In combination with thermal conductivity measurement of the bulk <span class="hlt">air</span>, the <span class="hlt">CO</span><span class="hlt">2</span> mixing ratio is calculated. The analytical precision determined from standard <span class="hlt">air</span> sample measurements over ice is ±1.9 ppm for <span class="hlt">CO</span><span class="hlt">2</span> and ±0.09 ‰ for δ13C. In a laboratory intercomparison study with CSIRO (Aspendale, Australia), good agreement between <span class="hlt">CO</span><span class="hlt">2</span> and δ13C results is found for Law Dome ice core samples. Replicate analysis of these samples resulted in a pooled standard deviation of <span class="hlt">2</span>.0 ppm for <span class="hlt">CO</span><span class="hlt">2</span> and 0.11 ‰ for δ13C. These numbers are good, though they are rather conservative estimates of the overall analytical precision achieved for single ice sample measurements. Facilitated by the small sample requirement</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('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> flux 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 <span class="hlt">exchange</span> model, the <span class="hlt">air-sea</span> fluxes 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/2010TCD.....4..153D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010TCD.....4..153D"><span>Brief communication: ikaite (Ca<span class="hlt">CO</span>3*6H<span class="hlt">2</span>O) discovered in Arctic <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>Dieckmann, G. S.; Nehrke, G.; Uhlig, C.; Göttlicher, J.; Gerland, S.; Granskog, M. A.; Thomas, D. N.</p> <p>2010-02-01</p> <p>We report for the first time on the discovery of calcium carbonate crystals as ikaite (Ca<span class="hlt">CO</span>3*6H<span class="hlt">2</span>O) in <span class="hlt">sea</span> ice from the Arctic (Kongsfjorden, Svalbard). This finding demonstrates that the precipitation of calcium carbonate during the freezing of <span class="hlt">sea</span> ice is not restricted to the Antarctic, where it was observed for the first time in 2008. This finding is an important step in the quest to quantify its impact on the <span class="hlt">sea</span> ice driven carbon cycle and should in the future enable improvement parametrization <span class="hlt">sea</span> ice carbon models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013BGeo...10.2409H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013BGeo...10.2409H"><span>Kinetic bottlenecks to chemical <span class="hlt">exchange</span> rates for deep-<span class="hlt">sea</span> animals - Part <span class="hlt">2</span>: Carbon Dioxide</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hofmann, A. F.; Peltzer, E. T.; Brewer, P. G.</p> <p>2013-04-01</p> <p>Increased ocean acidification from fossil fuel <span class="hlt">CO</span><span class="hlt">2</span> invasion, from temperature-driven changes in respiration, and from possible leakage from sub-seabed geologic <span class="hlt">CO</span><span class="hlt">2</span> disposal has aroused concern over the impacts of elevated <span class="hlt">CO</span><span class="hlt">2</span> concentrations on marine life. Discussion of these impacts has so far focused only on changes in the oceanic bulk fluid properties (ΔpH, Δ[∑ <span class="hlt">CO</span><span class="hlt">2</span>], etc.) as the critical variable and with a major focus on carbonate shell formation. Here we describe the rate problem for animals that must export <span class="hlt">CO</span><span class="hlt">2</span> at about the same rate at which O<span class="hlt">2</span> is consumed. We analyse the basic properties controlling <span class="hlt">CO</span><span class="hlt">2</span> export within the diffusive boundary layer around marine animals in an ocean changing in temperature (T) and <span class="hlt">CO</span><span class="hlt">2</span> concentration in order to compare the challenges posed by O<span class="hlt">2</span> uptake under stress with the equivalent problem of <span class="hlt">CO</span><span class="hlt">2</span> expulsion. The problem is more complex than that for a non-reactive gas, since with <span class="hlt">CO</span><span class="hlt">2</span> the influence of the seawater carbonate acid-base system needs to be considered. These reactions significantly facilitate <span class="hlt">CO</span><span class="hlt">2</span> efflux compared to O<span class="hlt">2</span> intake at equal temperature, pressure and fluid flow rate under typical oceanic concentrations. The effect of these reactions can be described by an enhancement factor, similar to that widely used for <span class="hlt">CO</span><span class="hlt">2</span> invasion at the <span class="hlt">sea</span> surface. While organisms do need to actively regulate flow over their surface to thin the boundary layer to take up enough O<span class="hlt">2</span>, this seems to be not necessary to facilitate <span class="hlt">CO</span><span class="hlt">2</span> efflux. Instead, the main impacts of rising oceanic <span class="hlt">CO</span><span class="hlt">2</span> will most likely be those associated with classical ocean acidification science. Regionally, as with O<span class="hlt">2</span>, the combination of T, P and pH/p<span class="hlt">CO</span><span class="hlt">2</span> creates a zone of maximum <span class="hlt">CO</span><span class="hlt">2</span> stress at around 1000 m depth.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFMOS31B1279F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFMOS31B1279F"><span>Anomalously Low p<span class="hlt">CO</span><span class="hlt">2</span> Measured in the San Francisco Estuary</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fuller, J. R.; Wilkerson, F.; Parker, A. E.; Marchi, A.</p> <p>2008-12-01</p> <p>Estuaries have been identified as potential net sources of <span class="hlt">CO</span><span class="hlt">2</span> to the atmosphere. Bacterial respiration of organic matter entering the estuary leads to supersaturated levels of p<span class="hlt">CO</span><span class="hlt">2</span>. The southern embayment of the San Francisco Estuary (SFE) is no exception due in part to wastewater treatment practices. Persistently high levels of p<span class="hlt">CO</span><span class="hlt">2</span> between 600 and 1000 μatm have been reported for this embayment by the U.S. Geological Survey over the period 1976-1980 and more recently (2007-2008) by the authors. However, both studies also found notable exceptions to the high p<span class="hlt">CO</span><span class="hlt">2</span> levels during the spring phytoplankton bloom. An average level of 375 μatm, slightly above the contemporary atmospheric level, was observed during an April 1980 transect. Our recent measurements over the same transect have observed an even greater drawdown of p<span class="hlt">CO</span><span class="hlt">2</span> to as low as 175 μatm. In addition the p<span class="hlt">CO</span><span class="hlt">2</span> drawdown persisted from early March 2008 until the end of May. These anomalously low levels correspond directly with an algal bloom as evidenced by high concentrations of chlorophyll a and supersaturated dissolved oxygen. To our knowledge these are the lowest levels reported for the SFE and they indicate that portions of the estuary are a sink for atmospheric <span class="hlt">CO</span><span class="hlt">2</span> during bloom conditions. The hydrology of the southern embayment is dominated at times by the input of wastewater which is often treated to the advanced secondary level with inorganic nitrate as the product. This possibly contributes to a healthy estuarine algal population that helps to maintain current p<span class="hlt">CO</span><span class="hlt">2</span> levels in the SFE to those of 30 years ago despite significant urban growth around the estuary over that period. These findings have major implications both to estuarine management and to estimates of the estuarine component in global <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016cosp...41E1965U','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016cosp...41E1965U"><span><span class="hlt">CO</span><span class="hlt">2</span> and O<span class="hlt">2</span> Gas <span class="hlt">Exchange</span> in an Experimental Model of the Btlss with Plant Wastes and Human Wastes Included in the Mass <span class="hlt">Exchange</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ushakova, Sofya; Tikhomirov, Alexander A.; Velichko, Vladimir; Tikhomirova, Natalia; Trifonov, Sergey V.</p> <p>2016-07-01</p> <p>Mass <span class="hlt">exchange</span> processes in the new experimental model of the biotechnical life support system (BTLSS) constructed at the Institute of Biophysics SB RAS have a higher degree of closure than in the previous BTLSS, and, thus, the technologies employed in the new system are more complex. Therefore, before closing the loops of mass <span class="hlt">exchange</span> processes for several months, the new model of the BTLSS was run to match the technologies employed to cultivate plants and the methods used to involve inedible plant parts and human wastes into the mass <span class="hlt">exchange</span> with the <span class="hlt">CO</span><span class="hlt">2</span> absorption rate and the amount of the resulting O<span class="hlt">2</span>. The plant compartment included vegetables grown on the soil-like substrate (SLS) (chufa, beet, carrot, radish, and lettuce), plants hydroponically grown on expanded clay aggregate (wheat, soybean, watercress), and plants grown in aquaculture (common glasswort and watercress). Nutrient solutions for hydroponically grown plants were prepared by using products of physicochemical mineralization of human wastes. Growing the plants in aquaculture enabled maintaining NaCl concentration in the irrigation solution for hydroponically grown plants at a level safe for the plants. Inedible plant biomass was added to the SLS. Three cycles of closing the system were run, which lasted 7, 7, and 10 days. The comparison of the amount of <span class="hlt">CO</span><span class="hlt">2</span> fed into the system over 24 h (simulating human respiration) and the amount of <span class="hlt">CO</span><span class="hlt">2</span> daily exhaled by a 70-kg middle-aged human showed that between 1% and 4% of the daily emissions of <span class="hlt">CO</span><span class="hlt">2</span> were assimilated in the system, and about 3% of the average human daily O<span class="hlt">2</span> requirement accumulated in the system. Plant productivity was between 4 and 4.7% of the human daily vegetable requirement, or between 3 and 3.5% of the total human daily food requirement. Thus, testing of the BTLSS showed a match between the technologies employed to arrange mass <span class="hlt">exchange</span> processes. This study was supported by the grant of the Russian Science Foundation (Project No. 14-14-00599).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19940030883','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19940030883"><span>A model of the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchanges</span> between biosphere and atmosphere in the tundra</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Labgaa, Rachid R.; Gautier, Catherine</p> <p>1992-01-01</p> <p>A physical model of the soil thermal regime in a permafrost terrain has been developed and validated with soil temperature measurements at Barrow, Alaska. The model calculates daily soil temperatures as a function of depth and average moisture contents of the organic and mineral layers using a set of five climatic variables, i.e., <span class="hlt">air</span> temperature, precipitation, cloudiness, wind speed, and relative humidity. The model is not only designed to study the impact of climate change on the soil temperature and moisture regime, but also to provide the input to a decomposition and net primary production model. In this context, it is well known that <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchanges</span> between the terrestrial biosphere and the atmosphere are driven by soil temperature through decomposition of soil organic matter and root respiration. However, in tundra ecosystems, net <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> is extremely sensitive to soil moisture content; therefore it is necessary to predict variations in soil moisture in order to assess the impact of climate change on carbon fluxes. To this end, the present model includes the representation of the soil moisture response to changes in climatic conditions. The results presented in the foregoing demonstrate that large errors in soil temperature and permafrost depth estimates arise from neglecting the dependence of the soil thermal regime on soil moisture contents. Permafrost terrain is an example of a situation where soil moisture and temperature are particularly interrelated: drainage conditions improve when the depth of the permafrost increases; a decrease in soil moisture content leads to a decrease in the latent heat required for the phase transition so that the heat penetrates faster and deeper, and the maximum depth of thaw increases; and as excepted, soil thermal coefficients increase with moisture.</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> <span class="hlt">exchange</span> 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> flux 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> flux 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('https://ntrs.nasa.gov/search.jsp?R=19930032543&hterms=THC&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3DTHC','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930032543&hterms=THC&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3DTHC"><span>Micrometeorological measurements of CH4 and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> between the atmosphere and subarctic tundra</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Fan, S. M.; Wofsy, S. C.; Bakwin, P. S.; Jacob, D. J.; Anderson, S. M.; Kebabian, P. L.; Mcmanus, J. B.; Kolb, C. E.; Fitzjarrald, D. R.</p> <p>1992-01-01</p> <p>Eddy correlation flux measurements and concentration profiles of total hydrocarbons (THC) and <span class="hlt">CO</span><span class="hlt">2</span> were combined to provide a comprehensive record of atmosphere-biosphere <span class="hlt">exchange</span> for these gases over a 30-day period in July-August 1988 in the Yukon-Kuskokwin River Delta of Alaska. Over 90 percent of net ecosystem <span class="hlt">exchanges</span> of THC were due to methane. Lakes and wet meadow tundra provided the major sources of methane. The average fluxes from lake, dry tundra, and wet tundra were 11 +/- 3, 29 +/- 3, and 57 +/- 6 mg CH4/sq m/d, respectively. The mean remission rate for the site was 25 mg/sq m/d. Maximum uptake of <span class="hlt">CO</span><span class="hlt">2</span> by the tundra was 1.4 gC/sq m/d between 1000 and 1500 hrs, and nocturnal respiration averaged 0.73 gC/sq m/d. Net uptake of <span class="hlt">CO</span><span class="hlt">2</span> was 0.30 gC/sq m/d for the 30 days of measurement; methane flux accounted for 6 percent of <span class="hlt">CO</span><span class="hlt">2</span> net uptake.</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> flux 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 flux. They show a marked variation with time of the degassing rate, with synchronous maxima in December 2005. Carbon dioxide soil flux 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 flux 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/2018ClDy...50...83B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ClDy...50...83B"><span>Greenland coastal <span class="hlt">air</span> temperatures linked to Baffin Bay and Greenland <span class="hlt">Sea</span> ice conditions during autumn through regional blocking patterns</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ballinger, Thomas J.; Hanna, Edward; Hall, Richard J.; Miller, Jeffrey; Ribergaard, Mads H.; Høyer, Jacob L.</p> <p>2018-01-01</p> <p>Variations in <span class="hlt">sea</span> ice freeze onset and regional <span class="hlt">sea</span> surface temperatures (SSTs) in Baffin Bay and Greenland <span class="hlt">Sea</span> are linked to autumn surface <span class="hlt">air</span> temperatures (SATs) around coastal Greenland through 500 hPa blocking patterns, 1979-2014. We find strong, statistically significant correlations between Baffin Bay freeze onset and SSTs and SATs across the western and southernmost coastal areas, while weaker and fewer significant correlations are found between eastern SATs, SSTs, and freeze periods observed in the neighboring Greenland <span class="hlt">Sea</span>. Autumn Greenland Blocking Index values and the incidence of meridional circulation patterns have increased over the modern <span class="hlt">sea</span> ice monitoring era. Increased anticyclonic blocking patterns promote poleward transport of warm <span class="hlt">air</span> from lower latitudes and local warm <span class="hlt">air</span> advection onshore from ocean-atmosphere sensible heat <span class="hlt">exchange</span> through ice-free or thin ice-covered <span class="hlt">seas</span> bordering the coastal stations. Temperature composites by years of extreme late freeze conditions, occurring since 2006 in Baffin Bay, reveal positive monthly SAT departures that often exceed 1 standard deviation from the 1981-2010 climate normal over coastal areas that exhibit a similar spatial pattern as the peak correlations.</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 flux-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 fluxes 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 flux-gradient system for simultaneous measurement of the fluxes 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 flux 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 fluxes were higher in magnitude than the measurement precision, which confirms that the flux-gradient system had adequate precision for the measurement of the lake-<span class="hlt">air</span> <span class="hlt">exchanges</span>. This study illustrates four strengths of the flux-gradient method: (1) the ability to simultaneously measure the flux 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 flux; and (4) continuous and noninvasive operation. The annual mean CH4 flux (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 flux for broad applications but requires further improvement to resolve small <span class="hlt">CO</span><span class="hlt">2</span> flux in many lakes.</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 <span class="hlt">Exchange</span> 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> fluxes 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> flux 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> fluxes. 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('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> fluxes 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 flux, 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> flux. In the extreme cases of <span class="hlt">air</span>-dried saline/alkaline soils, this inorganic process was predominant. While the diurnal flux measured was zero sum, leaching of the dissolved inorganic carbon in the soil solution could potentially effect net carbon ecosystem <span class="hlt">exchange</span>. This finding implies that an inorganic module should be incorporated when dealing with the <span class="hlt">CO</span><span class="hlt">2</span> flux of saline/alkaline land. Neglecting this inorganic flux may induce erroneous or misleading conclusions in interpreting <span class="hlt">CO</span><span class="hlt">2</span> fluxes 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> fluxes 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 flux, 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> flux. In the extreme cases of <span class="hlt">air</span>-dried saline/alkaline soils, this inorganic process was predominant. While the diurnal flux measured was zero sum, leaching of the dissolved inorganic carbon in the soil solution could potentially effect net carbon ecosystem <span class="hlt">exchange</span>. This finding implies that an inorganic module should be incorporated when dealing with the <span class="hlt">CO</span><span class="hlt">2</span> flux of saline/alkaline land. Neglecting this inorganic flux may induce erroneous or misleading conclusions in interpreting <span class="hlt">CO</span><span class="hlt">2</span> fluxes of these ecosystems. PMID:23778238</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26910987','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26910987"><span>[Summer Greenhouse Gases <span class="hlt">Exchange</span> Flux Across Water-<span class="hlt">air</span> Interface in Three Water Reservoirs Located in Different Geologic Setting in Guangxi, China].</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-hong; Pu, Jun-bing; Sun, Ping-an; Yuan, Dao-xian; Liu, Wen; Zhang, Tao; Mo, Xue</p> <p>2015-11-01</p> <p>Due to special hydrogeochemical characteristics of calcium-rich, alkaline and DIC-rich ( dissolved inorganic carbon) environment controlled by the weathering products from carbonate rock, the <span class="hlt">exchange</span> characteristics, processes and controlling factors of greenhouse gas (<span class="hlt">CO</span><span class="hlt">2</span> and CH4) across water-<span class="hlt">air</span> interface in karst water reservoir show obvious differences from those of non-karst water reservoir. Three water reservoirs (Dalongdong reservoir-karst reservoir, Wulixia reservoir--semi karst reservoir, Si'anjiang reservoir-non-karst reservoir) located in different geologic setting in Guangxi Zhuang Autonomous Region, China were chosen to reveal characteristics and controlling factors of greenhouse gas <span class="hlt">exchange</span> flux across water-<span class="hlt">air</span> interface. Two common approaches, floating chamber (FC) and thin boundary layer models (TBL), were employed to research and contrast greenhouse gas <span class="hlt">exchange</span> flux across water-<span class="hlt">air</span> interface from three reservoirs. The results showed that: (1) surface-layer water in reservoir area and discharging water under dam in Dalongdong water reservoir were the source of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> and CH4. Surface-layer water in reservoir area in Wulixia water reservoir was the sink of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> and the source of atmospheric CH4, while discharging water under dam was the source of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> and CH4. Surface-layer water in Si'anjiang water reservoir was the sink of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> and source of atmospheric CH4. (<span class="hlt">2</span>) <span class="hlt">CO</span><span class="hlt">2</span> and CH4 effluxes in discharging water under dam were much more than those in surface-layer water in reservoir area regardless of karst reservoir or non karst reservoir. Accordingly, more attention should be paid to the <span class="hlt">CO</span><span class="hlt">2</span> and CH4 emission from discharging water under dam. (3) In the absence of submerged soil organic matters and plants, the difference of CH4 effluxes between karst groundwater-fed reservoir ( Dalongdong water reservoir) and non-karst area ( Wulixia water reservoir and Si'anjiang water reservoir) was less. However, <span class="hlt">CO</span><span class="hlt">2</span></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> Fluxes 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> flux data set. Clim. Dynamics, Volume 33, pp 341-364 Valdivieso, M. and <span class="hlt">co</span>-authors (2014): Heat fluxes from ocean and coupled reanalyses, Clivar <span class="hlt">Exchanges</span>. Issue 64. Yu, L., X. Jin, and R. A. Weller (2008), Multidecade Global Flux Datasets from the Objectively Analyzed <span class="hlt">Air-sea</span> Fluxes (OAFlux) Project: Latent and Sensible Heat Fluxes, 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 fluxes 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('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=62405&keyword=FAN&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=62405&keyword=FAN&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>FACTORS AFFECTING <span class="hlt">AIR</span> <span class="hlt">EXCHANGE</span> IN TWO HOUSES</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><span class="hlt">Air</span> <span class="hlt">exchange</span> rate is critical to determining the relationship between indoor and outdoor concentrations of hazardous pollutants. Approximately 150 <span class="hlt">air</span> <span class="hlt">exchange</span> experiments were completed in two residences: a two-story detached house located in Redwood City, CA and a three-story...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28542645','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28542645"><span><span class="hlt">CO</span><span class="hlt">2</span> insufflation versus <span class="hlt">air</span> insufflation for endoscopic submucosal dissection: A meta-analysis of randomized controlled trials.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Li, Xuan; Dong, Hao; Zhang, Yifeng; Zhang, Guoxin</p> <p>2017-01-01</p> <p>Carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) insufflation is increasingly used for endoscopic submucosal dissection (ESD) owing to the faster absorption of <span class="hlt">CO</span><span class="hlt">2</span> as compared to that of <span class="hlt">air</span>. Studies comparing <span class="hlt">CO</span><span class="hlt">2</span> insufflation and <span class="hlt">air</span> insufflation have reported conflicting results. This meta-analysis is aimed to assess the efficacy and safety of use of <span class="hlt">CO</span><span class="hlt">2</span> insufflation for ESD. Clinical trials of <span class="hlt">CO</span><span class="hlt">2</span> insufflation versus <span class="hlt">air</span> insufflation for ESD were searched in PubMed, Embase, the Cochrane Library and Chinese Biomedical Literature Database. We performed a meta-analysis of all randomized controlled trials (RCTs). Eleven studies which compared the use of <span class="hlt">CO</span><span class="hlt">2</span> insufflation and <span class="hlt">air</span> insufflation, with a combined study population of 1026 patients, were included in the meta-analysis (n = 506 for <span class="hlt">CO</span><span class="hlt">2</span> insufflation; n = 522 for <span class="hlt">air</span> insufflation). Abdominal pain and VAS scores at 6h and 24h post-procedure in the <span class="hlt">CO</span><span class="hlt">2</span> insufflation group were significantly lower than those in the <span class="hlt">air</span> insufflation group, but not at 1h and 3h after ESD. The percentage of patients who experienced pain 1h and 24h post-procedure was obviously decreased. Use of <span class="hlt">CO</span><span class="hlt">2</span> insufflation was associated with lower VAS scores for abdominal distention at 1h after ESD, but not at 24h after ESD. However, no significant differences were observed with respect to postoperative transcutaneous partial pressure carbon dioxide (Ptc<span class="hlt">CO</span><span class="hlt">2</span>), arterial blood carbon dioxide partial pressure (Pa<span class="hlt">CO</span><span class="hlt">2</span>), oxygen saturation (SpO<span class="hlt">2</span>%), abdominal circumference, hospital stay, white blood cell (WBC) counts, C-Reactive protein (CRP) level, dosage of sedatives used, incidence of dysphagia and other complications. Use of <span class="hlt">CO</span><span class="hlt">2</span> insufflation for ESD was safe and effective with regard to abdominal discomfort, procedure time, and the residual gas volume. However, there appeared no significant differences with respect to other parameters namely, Ptc<span class="hlt">CO</span><span class="hlt">2</span>, Pa<span class="hlt">CO</span><span class="hlt">2</span>, SpO<span class="hlt">2</span>%, abdominal circumference, hospital stay, sedation dosage, complications, WBC, CRP, and dysphagia.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.B22E..03M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.B22E..03M"><span>Microbial, Physical and Chemical Drivers of COS and 18O-<span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Exchange</span> in Soils</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.; Boye, K.; Whelan, M.; Pang, E.; von Sperber, C.; Brueggemann, N.; Berry, J. A.; Welander, P. V.</p> <p>2015-12-01</p> <p>Carbonyl sulfide (COS) and the oxygen isotope composition (δ18O) of <span class="hlt">CO</span><span class="hlt">2</span> are potential tools for differentiating the contributions of photosynthesis and respiration to the balance of global carbon cycling. These processes are coupled at the leaf level via the enzyme carbonic anhydrase (CA), which hydrolyzes <span class="hlt">CO</span><span class="hlt">2</span> in the first biochemical step of the photosynthetic pathway (<span class="hlt">CO</span><span class="hlt">2</span> + H<span class="hlt">2</span>O ⇌ HCO3- + H+) and correspondingly structural analogue COS (COS + H<span class="hlt">2</span>O → <span class="hlt">CO</span><span class="hlt">2</span> + H<span class="hlt">2</span>S). CA also accelerates the <span class="hlt">exchange</span> of oxygen isotopes between <span class="hlt">CO</span><span class="hlt">2</span> and H<span class="hlt">2</span>O leading to a distinct isotopic imprint [1]. The biogeochemical cycles of these tracers include significant, yet poorly characterized soil processes that challenge their utility for probing the carbon cycle. In soils, microbial CA also hydrolyze COS and accelerate O isotope <span class="hlt">exchange</span> between <span class="hlt">CO</span><span class="hlt">2</span> and soil water. Soils have been observed to emit COS by undetermined processes. To account for these soil processes, measurements are needed to identify the key microbial, chemical, and physical factors. In this study, we survey COS and δ18O <span class="hlt">exchange</span> in twenty different soils spanning a variety of biomes and soil properties. By comparing COS fluxes and δ18O-<span class="hlt">CO</span><span class="hlt">2</span> values emitted from moist soils we investigate whether the same types of CA catalyze these two processes. Additionally, we seek to identify the potential chemical drivers of COS emissions by measuring COS fluxes in dry soils. These data are compared with soil physical (bulk density, volumetric water content, texture), chemical (pH, elemental analysis, sulfate, sulfur K-edge XANES), and microbial measurements (biomass and phylogeny). Furthermore, we determine the abundance and diversity of CA-encoding genes to directly link CA with measured soil function. This work will define the best predictors for COS fluxes and δ18O-<span class="hlt">CO</span><span class="hlt">2</span> values from our suite of biogeochemical measurements. The suitability of identified predictor variables can be tested in follow-up studies and applied for modeling</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27974151','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27974151"><span>Using a passive <span class="hlt">air</span> sampler to monitor <span class="hlt">air</span>-soil <span class="hlt">exchange</span> of organochlorine pesticides in the pasture of the central Tibetan Plateau.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Chuanfei; Wang, Xiaoping; Ren, Jiao; Gong, Ping; Yao, Tandong</p> <p>2017-02-15</p> <p><span class="hlt">Air</span>-soil <span class="hlt">exchange</span> is a key process controlling the fate of persistent organic pollutants (POPs). However, the "sink effect" of soil for POPs in Tibetan pasture has not been clear. In Nam<span class="hlt">Co</span>, in the central Tibetan Plateau (TP) where the land is covered by grass, a modified passive <span class="hlt">air</span> sampler (PAS) (thickness: <span class="hlt">2</span>cm) was tested. Using the PAS, the atmospheric gaseous phase organochlorine pesticides (OCPs) at 11 heights from close-to-surface (<span class="hlt">2</span>cm) to 200cm above ground, in summer and in winter, were measured. Concentrations of OCPs in summer were higher than those in winter. Both in summer and winter, atmospheric concentrations of OCPs decreased with decreasing height from 200 to <span class="hlt">2</span>cm, indicating that OCPs were being deposited from <span class="hlt">air</span> to soil. <span class="hlt">Air</span> deposition of OCPs was possibly driven by wind speed. Furthermore, based on <span class="hlt">air</span> OCPs at 0-3cm near the surface, the interface <span class="hlt">exchange</span> of OCPs between <span class="hlt">air</span> and soil was studied by the fugacity method. The results showed that pastural soil in the TP was a "sink" of OCPs even in summer. The mean deposition fluxes of α-HCH, γ-HCH and o,p'-DDT were 0.72, 0.24 and 0.54pg/h/m <span class="hlt">2</span> , respectively, and it was estimated that the level of these pollutants in the soil will double every 24, 66 and 206years, respectively. This study will contribute to the further understanding of global cycling of POPs in different land covers. Copyright © 2016 Elsevier B.V. All rights reserved.</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://edg.epa.gov/metadata/catalog/search/resource/details.page?uuid=%7B393704A5-B912-4686-BE1B-A9F8EFF2F565%7D','PESTICIDES'); return false;" href="https://edg.epa.gov/metadata/catalog/search/resource/details.page?uuid=%7B393704A5-B912-4686-BE1B-A9F8EFF2F565%7D"><span>Updating <span class="hlt">sea</span> spray aerosol emissions in the Community Multiscale <span class="hlt">Air</span> Quality (CMAQ) model version 5.0.<span class="hlt">2</span></span></a></p> <p><a target="_blank" href="http://www.epa.gov/pesticides/search.htm">EPA Pesticide Factsheets</a></p> <p></p> <p></p> <p>The uploaded data consists of the BRACE Na aerosol observations paired with CMAQ model output, the updated model's parameterization of <span class="hlt">sea</span> salt aerosol emission size distribution, and the model's parameterization of the <span class="hlt">sea</span> salt emission factor as a function of <span class="hlt">sea</span> surface temperature. This dataset is associated with the following publication:Gantt , B., J. Kelly , and J. Bash. Updating <span class="hlt">sea</span> spray aerosol emissions in the Community Multiscale <span class="hlt">Air</span> Quality (CMAQ) model version 5.0.<span class="hlt">2</span>. Geoscientific Model Development. Copernicus Publications, Katlenburg-Lindau, GERMANY, 8: 3733-3746, (2015).</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 fluxes 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 <span class="hlt">exchange</span>. The direct bubble flux 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 flux, 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 <span class="hlt">exchanging</span> 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/2013EGUGA..1512690S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..1512690S"><span>The <span class="hlt">Air-Sea</span> Interface and Surface Stress under 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>Soloviev, Alexander; Lukas, Roger; Donelan, Mark; Ginis, Isaac</p> <p>2013-04-01</p> <p> of the drag coefficient wind speed dependence around 65 m/s. This minimum may contribute to the rapid intensification of storms to major tropical cyclones. The subsequent slow increase of the drag coefficient with wind above 65 m/s serves as an obstacle for further intensification of tropical cyclones. Such dependence may explain the observed bi-modal distribution of tropical cyclone intensity. Implementation of the new parameterization into operational models is expected to improve predictions of tropical cyclone intensity and the associated wave field. References: Donelan, M. A., B. K. Haus, N. Reul, W. Plant, M. Stiassnie, H. Graber, O. Brown, and E. Saltzman, 2004: On the limiting aerodynamic roughness of the ocean in very strong winds, Farrell, B.F, and P.J. Ioannou, 2008: The stochastic parametric mechanism for growth of wind-driven surface water waves. Journal of Physical Oceanography 38, 862-879. Kelly, R.E., 1965: The stability of an unsteady Kelvin-Helmholtz flow. J. Fluid Mech. 22, 547-560. Koga, M., 1981: Direct production of droplets from breaking wind-waves-Its observation by a multi-colored overlapping exposure technique, Tellus 33, 552-563. Miles, J.W., 1959: On the generation of surface waves by shear flows, part 3. J. Fluid. Mech. 6, 583-598. Soloviev, A.V. and R. Lukas, 2010: Effects of bubbles and <span class="hlt">sea</span> spray on <span class="hlt">air-sea</span> <span class="hlt">exchanges</span> in hurricane conditions. Boundary-Layer Meteorology 136, 365-376. Soloviev, A., A. Fujimura, and S. Matt, 2012: <span class="hlt">Air-sea</span> interface in hurricane conditions. J. Geophys. Res. 117, C00J34.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JMS...148..122G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JMS...148..122G"><span>Modelling the 13C and 12C isotopes of inorganic and organic carbon 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>Gustafsson, Erik; Mörth, Carl-Magnus; Humborg, Christoph; Gustafsson, Bo G.</p> <p>2015-08-01</p> <p>In this study, 12C and 13C contents of all carbon containing state variables (dissolved inorganic and organic carbon, detrital carbon, and the carbon content of autotrophs and heterotrophs) have for the first time been explicitly included in a coupled physical-biogeochemical Baltic <span class="hlt">Sea</span> model. Different processes in the carbon cycling have distinct fractionation values, resulting in specific isotopic fingerprints. Thus, in addition to simulating concentrations of different tracers, our new model formulation improves the possibility to constrain the rates of processes such as <span class="hlt">CO</span><span class="hlt">2</span> assimilation, mineralization, and <span class="hlt">air-sea</span> <span class="hlt">exchange</span>. We demonstrate that phytoplankton production and respiration, and the related <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> fluxes, are to a large degree controlling the isotopic composition of organic and inorganic carbon in the system. The isotopic composition is further, but to a lesser extent, influenced by river loads and deep water inflows as well as transformation of terrestrial organic carbon within the system. Changes in the isotopic composition over the 20th century have been dominated by two processes - the preferential release of 12C to the atmosphere in association with fossil fuel burning, and the eutrophication of the Baltic <span class="hlt">Sea</span> related to increased nutrient loads under the second half of the century.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15683168','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15683168"><span><span class="hlt">Air</span>-water gas <span class="hlt">exchange</span> of chlorinated pesticides in four lakes spanning a 1,205 meter elevation range in the Canadian Rocky Mountains.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wilkinson, Andrew C; Kimpe, Lynda E; Blais, Jules M</p> <p>2005-01-01</p> <p>Concentrations of selected persistent organic pollutants (POPs) in <span class="hlt">air</span> and water were measured from four lakes that transect the Canadian Rocky Mountains. These data were used in combination with wind velocity and temperature-adjusted Henry's law constants to estimate the direction and magnitude of chemical <span class="hlt">exchange</span> across the <span class="hlt">air</span>-water interface of these lakes. Bow Lake (1,975 m above <span class="hlt">sea</span> level [masl]) was studied during the summers of 1998 through 2000; Donald (770 masl) was studied during the summer of 1999; Dixon Dam Lake (946 masl) and Kananaskis Lake (1,667 masl) were studied during the summer of 2000. Hexachlorobenzene (HCB) and dieldrin volatilized from Bow Lake in spring and summer of 1998 to 2000 at a rate of 0.92 +/-1.1 and 0.55+/-0.37 ng m(-<span class="hlt">2</span>) d(-1), respectively. The alpha-endosulfan deposited to Bow Lake at a rate of 3.4+/-<span class="hlt">2.2</span> ng m(-<span class="hlt">2</span>) d(-1). Direction of gas <span class="hlt">exchange</span> for gamma-hexachlorocyclohexane (gamma-HCH) changed from net deposition in 1998 to net volatilization in 1999, partly because of a surge in y-HCH concentrations in the water at Bow Lake in 1999. Average gamma-HCH concentrations in <span class="hlt">air</span> declined steadily over the three-year period, from 0.021 ng m(-3) in 1998, to 0.0023 ng m(-3) in 2000, and to volatilization in 1999 and 2000. Neither the concentrations of organochlorine compounds (OCs) in <span class="hlt">air</span> and water, nor the direction and rate of <span class="hlt">air</span>-water gas <span class="hlt">exchange</span> correlate with temperature or elevation. In general, losses of pesticides by outflow were greater than the amount <span class="hlt">exchanged</span> across the <span class="hlt">air</span>-water interface in these lakes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.5946L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.5946L"><span>Modeling forest C and N allocation responses to free-<span class="hlt">air</span> <span class="hlt">CO</span><span class="hlt">2</span> enrichment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Luus, Kristina; De Kauwe, Martin; Walker, Anthony; Werner, Christian; Iversen, Colleen; McCarthy, Heather; Medlyn, Belinda; Norby, Richard; Oren, Ram; Zak, Donald; Zaehle, Sönke</p> <p>2015-04-01</p> <p>Vegetation allocation patterns and soil-vegetation partitioning of C and N are predicted to change in response to rising atmospheric concentrations of <span class="hlt">CO</span><span class="hlt">2</span>. These allocation responses to rising <span class="hlt">CO</span><span class="hlt">2</span> have been examined at the ecosystem level through through free-<span class="hlt">air</span> <span class="hlt">CO</span><span class="hlt">2</span> enrichment (FACE) experiments, and their global implications for the timing of progressive N limitation (PNL) and C sequestration have been predicted for ~100 years using a variety of ecosystem models. However, recent FACE model-data syntheses studies [1,<span class="hlt">2</span>,3] have indicated that ecosystem models do not capture the 5-10 year site-level ecosystem allocation responses to elevated <span class="hlt">CO</span><span class="hlt">2</span>. This may be due in part to the missing representation of the rhizosphere interactions between plants and soil biota in models. Ecosystem allocation of C and N is altered by interactions between soil and vegetation through the priming effect: as plant N availability diminishes, plants respond physiologically by altering their tissue allocation strategies so as to increase rates of root growth and rhizodeposition. In response, either soil organic material begins to accumulate, which hastens the onset of PNL, or soil microbes start to decompose C more rapidly, resulting in increased N availability for plant uptake, which delays PNL. In this study, a straightforward approach for representing rhizosphere interactions in ecosystem models was developed through which C and N allocation to roots and rhizodeposition responds dynamically to elevated <span class="hlt">CO</span><span class="hlt">2</span> conditions, modifying soil decomposition rates without pre-specification of the direction in which soil C and N accumulation should shift in response to elevated <span class="hlt">CO</span><span class="hlt">2</span>. This approach was implemented in a variety of ecosystem models ranging from stand (G'DAY), to land surface (CLM 4.5, O-CN), to dynamic global vegetation (LPJ-GUESS) models. Comparisons against data from three forest FACE sites (Duke, Oak Ridge & Rhinelander) indicated that representing rhizosphere interactions allowed</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015CG.....79...15M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015CG.....79...15M"><span>Analysis of <span class="hlt">CO</span><span class="hlt">2</span> trapping capacities and long-term migration for geological formations in the Norwegian North <span class="hlt">Sea</span> using MRST-<span class="hlt">co</span><span class="hlt">2</span>lab</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Møll Nilsen, Halvor; Lie, Knut-Andreas; Andersen, Odd</p> <p>2015-06-01</p> <p>MRST-<span class="hlt">co</span><span class="hlt">2</span>lab is a collection of open-source computational tools for modeling large-scale and long-time migration of <span class="hlt">CO</span><span class="hlt">2</span> in conductive aquifers, combining ideas from basin modeling, computational geometry, hydrology, and reservoir simulation. Herein, we employ the methods of MRST-<span class="hlt">co</span><span class="hlt">2</span>lab to study long-term <span class="hlt">CO</span><span class="hlt">2</span> storage on the scale of hundreds of megatonnes. We consider public data sets of two aquifers from the Norwegian North <span class="hlt">Sea</span> and use geometrical methods for identifying structural traps, percolation-type methods for identifying potential spill paths, and vertical-equilibrium methods for efficient simulation of structural, residual, and solubility trapping in a thousand-year perspective. In particular, we investigate how data resolution affects estimates of storage capacity and discuss workflows for identifying good injection sites and optimizing injection strategies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.B43D2156L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.B43D2156L"><span>Biosphere-atmosphere <span class="hlt">Exchange</span> of <span class="hlt">CO</span><span class="hlt">2</span> in a Subtropical Mangrove Wetland in Hong Kong</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.; Neogi, S.; Lai, D. Y. F.</p> <p>2017-12-01</p> <p>Mangrove ecosystems play an important role in the global carbon cycle due to their high primary productivity, carbon-rich sediment, and sensitivity to climate change. Yet, there is currently a paucity of studies that quantify the biosphere-atmosphere <span class="hlt">exchange</span> of GHGs in mangrove wetlands continuously at the ecosystem level. In this study, the temporal variability of net ecosystem <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> (NEE) between the Kandelia obovata mangrove and the atmosphere was determined in the Mai Po Marshes Nature Reserve of subtropical Hong Kong using an eddy covariance system between February 2016 and January 2017. The daytime half-hourly NEE ranged between -5.0 and +3.3 µmol m-<span class="hlt">2</span> s-1, while the maximum nighttime NEE could reach +5.0 µmol m-<span class="hlt">2</span> s-1 during the wet, warm season. Temperature, photosynthetic photon flux density (PPFD), vapor pressure deficit (VPD), and surface water salinity were some key physical and hydrological controls of NEE. Tidal activity could also exert profound influence on <span class="hlt">CO</span><span class="hlt">2</span> fluxes in this mangrove ecosystem by exporting dissolved carbon to adjacent estuary and inhibiting soil respiration during the inundation period. Overall, this coastal mangrove was a net sink of atmospheric <span class="hlt">CO</span><span class="hlt">2</span>. Our results suggest that the ability of subtropical mangrove ecosystems in sequestering <span class="hlt">CO</span><span class="hlt">2</span> could be highly dependent on future changes in temperature, precipitation, and salinity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20000037970&hterms=gas+natural&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dgas%2Bnatural','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20000037970&hterms=gas+natural&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dgas%2Bnatural"><span>The Effect of Rain on <span class="hlt">Air</span>-Water Gas <span class="hlt">Exchange</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ho, David T.; Bliven, Larry F.; Wanninkhof, Rik; Schlosser, Peter</p> <p>1997-01-01</p> <p>The relationship between gas transfer velocity and rain rate was investigated at NASA's Rain-<span class="hlt">Sea</span> Interaction Facility (RSIF) using several SF, evasion experiments. During each experiment, a water tank below the rain simulator was supersaturated with SF6, a synthetic gas, and the gas transfer velocities were calculated from the measured decrease in SF6 concentration with time. The results from experiments with IS different rain rates (7 to 10 mm/h) and 1 of <span class="hlt">2</span> drop sizes (<span class="hlt">2</span>.8 or 4.<span class="hlt">2</span> mm diameter) confirm a significant and systematic enhancement of <span class="hlt">air</span>-water gas <span class="hlt">exchange</span> by rainfall. The gas transfer velocities derived from our experiment were related to the kinetic energy flux calculated from the rain rate and drop size. The relationship obtained for mono-dropsize rain at the RSIF was extrapolated to natural rain using the kinetic energy flux of natural rain calculated from the Marshall-Palmer raindrop size distribution. Results of laboratory experiments at RSIF were compared to field observations made during a tropical rainstorm in Miami, Florida and show good agreement between laboratory and field data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRC..123.2293B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRC..123.2293B"><span>Wave Attenuation and Gas <span class="hlt">Exchange</span> Velocity in Marginal <span class="hlt">Sea</span> Ice Zone</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bigdeli, A.; Hara, T.; Loose, B.; Nguyen, A. T.</p> <p>2018-03-01</p> <p>The gas transfer velocity in marginal <span class="hlt">sea</span> ice zones exerts a strong control on the input of anthropogenic gases into the ocean interior. In this study, a <span class="hlt">sea</span> state-dependent gas <span class="hlt">exchange</span> parametric model is developed based on the turbulent kinetic energy dissipation rate. The model is tuned to match the conventional gas <span class="hlt">exchange</span> parametrization in fetch-unlimited, fully developed <span class="hlt">seas</span>. Next, fetch limitation is introduced in the model and results are compared to fetch limited experiments in lakes, showing that the model captures the effects of finite fetch on gas <span class="hlt">exchange</span> with good fidelity. Having validated the results in fetch limited waters such as lakes, the model is next applied in <span class="hlt">sea</span> ice zones using an empirical relation between the <span class="hlt">sea</span> ice cover and the effective fetch, while accounting for the <span class="hlt">sea</span> ice motion effect that is unique to <span class="hlt">sea</span> ice zones. The model results compare favorably with the available field measurements. Applying this parametric model to a regional Arctic numerical model, it is shown that, under the present conditions, gas flux into the Arctic Ocean may be overestimated by 10% if a conventional parameterization is used.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004AGUFM.B23A0934B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004AGUFM.B23A0934B"><span>Estimation of Regional Net <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Exchange</span> over the Southern Great Plains</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Biraud, S. C.; Riley, W. J.; Fischer, M. L.; Torn, M. S.; Cooley, H. S.</p> <p>2004-12-01</p> <p>Estimating spatially distributed ecosystem <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> is an important component of the North American Carbon Program. We describe here a methodology to estimate Net Ecosystem <span class="hlt">Exchange</span> (NEE) over the Southern Great Plains, using: (1) data from the Department Of Energy's Atmospheric Radiation Measurement (ARM) sites in Oklahoma and Kansas; (<span class="hlt">2</span>) meteorological forcing data from the Mesonet facilities; (3) soil and vegetation types from 1 km resolution USGS databases; (4) vegetation status (e.g., LAI) from 1 km satellite measurements of surface reflectance (MODIS); (5) a tested land-surface model; and (6) a coupled land-surface and meteorological model (MM5/ISOLSM). This framework allows us to simulate regional surface fluxes in addition to ABL and free troposphere concentrations of <span class="hlt">CO</span><span class="hlt">2</span> at a continental scale with fine-scale nested grids centered on the ARM central facility. We use the offline land-surface and coupled models to estimate regional NEE, and compare predictions to measurements from the 9 Extended Facility sites with eddy correlation measurements. Site level comparisons to portable ECOR measurements in several crop types are also presented. Our approach also allows us to extend bottom-up estimates to periods and areas where meteorological forcing data are unavailable.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1998GBioC..12..703B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1998GBioC..12..703B"><span>Seasonal patterns and controls on net ecosystem <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> in a boreal peatland complex</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bubier, Jill L.; Crill, Patrick M.; Moore, Tim R.; Savage, Kathleen; Varner, Ruth K.</p> <p>1998-12-01</p> <p>We measured seasonal patterns of net ecosystem <span class="hlt">exchange</span> (NEE) of <span class="hlt">CO</span><span class="hlt">2</span> in a diverse peatland complex underlain by discontinuous permafrost in northern Manitoba, Canada, as part of the Boreal Ecosystems Atmosphere Study (BOREAS). Study sites spanned the full range of peatland trophic and moisture gradients found in boreal environments from bog (pH 3.9) to rich fen (pH 7.<span class="hlt">2</span>). During midseason (July-August, 1996), highest rates of NEE and respiration followed the trophic sequence of bog (5.4 to -3.9 μmol <span class="hlt">CO</span><span class="hlt">2</span> m-<span class="hlt">2</span> s-1) < poor fen (6.3 to -6.5 μmol <span class="hlt">CO</span><span class="hlt">2</span> m-<span class="hlt">2</span> s-1) < intermediate fen (10.5 to -7.8 μmol <span class="hlt">CO</span><span class="hlt">2</span> m-<span class="hlt">2</span> s-1) < rich fen (14.9 to -8.7 μmol <span class="hlt">CO</span><span class="hlt">2</span>m-<span class="hlt">2</span> s-1). The sequence changed during spring (May-June) and fall (September-October) when ericaceous shrub (e.g., Chamaedaphne calyculata) bogs and sedge (Carex spp.) communities in poor to intermediate fens had higher maximum <span class="hlt">CO</span><span class="hlt">2</span> fixation rates than deciduous shrub-dominated (Salix spp. and Betula spp.) rich fens. Timing of snowmelt and differential rates of peat surface thaw in microtopographic hummocks and hollows controlled the onset of carbon uptake in spring. Maximum photosynthesis and respiration were closely correlated throughout the growing season with a ratio of approximately 1/3 ecosystem respiration to maximum carbon uptake at all sites across the trophic gradient. Soil temperatures above the water table and timing of surface thaw and freeze-up in the spring and fall were more important to net <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> than deep soil warming. This close coupling of maximum <span class="hlt">CO</span><span class="hlt">2</span> uptake and respiration to easily measurable variables, such as trophic status, peat temperature, and water table, will improve models of wetland carbon <span class="hlt">exchange</span>. Although trophic status, aboveground net primary productivity, and surface temperatures were more important than water level in predicting respiration on a daily basis, the mean position of the water table was a good predictor (r<span class="hlt">2</span> = 0.63) of mean respiration rates across the range of plant community</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002AGUSM.B51A..08G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002AGUSM.B51A..08G"><span>COCA: deriving urban emissions and the carbon <span class="hlt">exchange</span> 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>Geiss, H.; Schmitgen, S.; Ciais, P.; Neininger, B.; Baeumle, M.; Brunet, Y.; Kley, D.</p> <p>2002-05-01</p> <p>A crucial challenge in measuring the partitioning of sources and sinks of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> is the separation of regional anthropogenic <span class="hlt">CO</span><span class="hlt">2</span> sources from biogenic activity. The aim of the COCA project is to quantify the fossil fuel and biogenic <span class="hlt">CO</span><span class="hlt">2</span> fractions using continuous airborne <span class="hlt">CO</span><span class="hlt">2</span> and <span class="hlt">CO</span> measurements, where <span class="hlt">CO</span> acts as a tracer for anthropogenic <span class="hlt">CO</span><span class="hlt">2</span>. At first part of the project COCA an attempt was made to measure daytime biogenic <span class="hlt">CO</span><span class="hlt">2</span> fluxes over a forest area (about 15 by 30 km size). The 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> flux and concentration measurements a Lagrangian budgeting approach was chosen to measure regional <span class="hlt">CO</span><span class="hlt">2</span> deposition fluxes. 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 estimating the influence of anthropogenic <span class="hlt">CO</span><span class="hlt">2</span> advected into the area First results of the summer flight on June 23rd will be shown, where fair wind speeds (~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 summer flights with very low wind speeds, local effects dominate the observations 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. During a second campaign the variance of anthropogenic <span class="hlt">CO</span> and <span class="hlt">CO</span><span class="hlt">2</span> emissions of a large city unaffected by biogenic processes has been studied. This campaign was carried out on February 16 and 17, 2002 over the Paris metropolitan area</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 fluxes 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('https://www.ncbi.nlm.nih.gov/pubmed/28295911','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28295911"><span><span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> and evapotranspiration across dryland ecosystems of southwestern North America.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Biederman, Joel A; Scott, Russell L; Bell, Tom W; Bowling, David R; Dore, Sabina; Garatuza-Payan, Jaime; Kolb, Thomas E; Krishnan, Praveena; Krofcheck, Dan J; Litvak, Marcy E; Maurer, Gregory E; Meyers, Tilden P; Oechel, Walter C; Papuga, Shirley A; Ponce-Campos, Guillermo E; Rodriguez, Julio C; Smith, William K; Vargas, Rodrigo; Watts, Christopher J; Yepez, Enrico A; Goulden, Michael L</p> <p>2017-10-01</p> <p>Global-scale studies suggest that dryland ecosystems dominate an increasing trend in the magnitude and interannual variability of the land <span class="hlt">CO</span> <span class="hlt">2</span> sink. However, such analyses are poorly constrained by measured <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">exchange</span> in drylands. Here we address this observation gap with eddy covariance data from 25 sites in the water-limited Southwest region of North America with observed ranges in annual precipitation of 100-1000 mm, annual temperatures of <span class="hlt">2</span>-25°C, and records of 3-10 years (150 site-years in total). Annual fluxes were integrated using site-specific ecohydrologic years to group precipitation with resulting ecosystem <span class="hlt">exchanges</span>. We found a wide range of carbon sink/source function, with mean annual net ecosystem production (NEP) varying from -350 to +330 gCm -<span class="hlt">2</span> across sites with diverse vegetation types, contrasting with the more constant sink typically measured in mesic ecosystems. In this region, only forest-dominated sites were consistent carbon sinks. Interannual variability of NEP, gross ecosystem production (GEP), and ecosystem respiration (R eco ) was larger than for mesic regions, and half the sites switched between functioning as C sinks/C sources in wet/dry years. The sites demonstrated coherent responses of GEP and NEP to anomalies in annual evapotranspiration (ET), used here as a proxy for annually available water after hydrologic losses. Notably, GEP and R eco were negatively related to temperature, both interannually within site and spatially across sites, in contrast to positive temperature effects commonly reported for mesic ecosystems. Models based on MODIS satellite observations matched the cross-site spatial pattern in mean annual GEP but consistently underestimated mean annual ET by ~50%. Importantly, the MODIS-based models captured only 20-30% of interannual variation magnitude. These results suggest the contribution of this dryland region to variability of regional to global <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">exchange</span> may be up to 3-5 times larger than current</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4270789','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4270789"><span>El Niño Southern Oscillation (ENSO) Enhances <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Exchange</span> Rates in Freshwater Marsh Ecosystems in the Florida Everglades</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Malone, Sparkle L.; Staudhammer, Christina L.; Oberbauer, Steven F.; Olivas, Paulo; Ryan, Michael G.; Schedlbauer, Jessica L.; Loescher, Henry W.; Starr, Gregory</p> <p>2014-01-01</p> <p>This research examines the relationships between El Niño Southern Oscillation (ENSO), water level, precipitation patterns and carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) <span class="hlt">exchange</span> rates in the freshwater wetland ecosystems of the Florida Everglades. Data was obtained over a 5-year study period (2009–2013) from two freshwater marsh sites located in Everglades National Park that differ in hydrology. At the short-hydroperiod site (Taylor Slough; TS) and the long-hydroperiod site (Shark River Slough; SRS) fluctuations in precipitation patterns occurred with changes in ENSO phase, suggesting that extreme ENSO phases alter Everglades hydrology which is known to have a substantial influence on ecosystem carbon dynamics. Variations in both ENSO phase and annual net <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> rates <span class="hlt">co</span>-occurred with changes in wet and dry season length and intensity. Combined with site-specific seasonality in <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchanges</span> rates, El Niño and La Niña phases magnified season intensity and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> rates at both sites. At TS, net <span class="hlt">CO</span><span class="hlt">2</span> uptake rates were higher in the dry season, whereas SRS had greater rates of carbon sequestration during the wet season. As La Niña phases were concurrent with drought years and extended dry seasons, TS became a greater sink for <span class="hlt">CO</span><span class="hlt">2</span> on an annual basis (−11 to −110 g <span class="hlt">CO</span><span class="hlt">2</span> m−<span class="hlt">2</span> yr−1) compared to El Niño and neutral years (−5 to −43.5 g <span class="hlt">CO</span><span class="hlt">2</span> m−<span class="hlt">2</span> yr−1). SRS was a small source for <span class="hlt">CO</span><span class="hlt">2</span> annually (1.81 to 80 g <span class="hlt">CO</span><span class="hlt">2</span> m−<span class="hlt">2</span> yr−1) except in one exceptionally wet year that was associated with an El Niño phase (−16 g <span class="hlt">CO</span><span class="hlt">2</span> m−<span class="hlt">2</span> yr−1). Considering that future climate predictions suggest a higher frequency and intensity in El Niño and La Niña phases, these results indicate that changes in extreme ENSO phases will significantly alter <span class="hlt">CO</span><span class="hlt">2</span> dynamics in the Florida Everglades. PMID:25521299</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70157303','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70157303"><span>Response of salt marsh and mangrove wetlands to changes in atmospheric <span class="hlt">CO</span><span class="hlt">2</span>, climate, and <span class="hlt">sea</span>-level</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Mckee, Karen L.; Rogers, Kerrylee; Saintilan, Neil; Middleton, Beth A.</p> <p>2012-01-01</p> <p>Coastal salt marsh and mangrove ecosystems are particularly vulnerable to changes in atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentrations and associated climate and climate-induced changes. We provide a review of the literature detailing theoretical predictions and observed responses of coastal wetlands to a range of climate change stressors, including <span class="hlt">CO</span><span class="hlt">2</span>, temperature, rainfall, and <span class="hlt">sea</span>-level rise. This review incorporates a discussion of key processes controlling responses in different settings and thresholds of resilience derived from experimental and observational studies. We specifically consider the potential and observed effects on salt marsh and mangrove vegetation of changes in (1) elevated [<span class="hlt">CO</span><span class="hlt">2</span>] on physiology, growth, and distribution; (<span class="hlt">2</span>) temperature on distribution and diversity; (3) rainfall and salinity regimes on growth and competitive interactions; and (4) <span class="hlt">sea</span> level on geomorphological, hydrological, and biological processes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19648403','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19648403"><span>Transcriptomic response of <span class="hlt">sea</span> urchin larvae Strongylocentrotus purpuratus to <span class="hlt">CO</span><span class="hlt">2</span>-driven seawater acidification.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Todgham, Anne E; Hofmann, Gretchen E</p> <p>2009-08-01</p> <p>Ocean acidification from the uptake of anthropogenic <span class="hlt">CO</span>(<span class="hlt">2</span>) is expected to have deleterious consequences for many calcifying marine animals. Forecasting the vulnerability of these marine organisms to climate change is linked to an understanding of whether species possess the physiological capacity to compensate for the potentially adverse effects of ocean acidification. We carried out a microarray-based transcriptomic analysis of the physiological response of larvae of a calcifying marine invertebrate, the purple <span class="hlt">sea</span> urchin, Strongylocentrotus purpuratus, to <span class="hlt">CO</span>(<span class="hlt">2</span>)-driven seawater acidification. In lab-based cultures, larvae were raised under conditions approximating current ocean pH conditions (pH 8.01) and at projected, more acidic pH conditions (pH 7.96 and 7.88) in seawater aerated with <span class="hlt">CO</span>(<span class="hlt">2</span>) gas. Targeting expression of approximately 1000 genes involved in several biological processes, this study captured changes in gene expression patterns that characterize the transcriptomic response to <span class="hlt">CO</span>(<span class="hlt">2</span>)-driven seawater acidification of developing <span class="hlt">sea</span> urchin larvae. In response to both elevated <span class="hlt">CO</span>(<span class="hlt">2</span>) scenarios, larvae underwent broad scale decreases in gene expression in four major cellular processes: biomineralization, cellular stress response, metabolism and apoptosis. This study underscores that physiological processes beyond calcification are impacted greatly, suggesting that overall physiological capacity and not just a singular focus on biomineralization processes is essential for forecasting the impact of future <span class="hlt">CO</span>(<span class="hlt">2</span>) conditions on marine organisms. Conducted on targeted and vulnerable species, genomics-based studies, such as the one highlighted here, have the potential to identify potential ;weak links' in physiological function that may ultimately determine an organism's capacity to tolerate future ocean conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28975183','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28975183"><span>The catalytic effect of H<span class="hlt">2</span>O on the hydrolysis of <span class="hlt">CO</span>32- in hydrated clusters and its implication in the humidity driven <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">air</span> capture.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Xiao, Hang; Shi, Xiaoyang; Zhang, Yayun; Liao, Xiangbiao; Hao, Feng; Lackner, Klaus S; Chen, Xi</p> <p>2017-10-18</p> <p>The hydration of ions in nanoscale hydrated clusters is ubiquitous and essential in many physical and chemical processes. Here we show that the hydrolysis reaction is strongly affected by relative humidity. The hydrolysis of <span class="hlt">CO</span> 3 <span class="hlt">2</span>- with n = 1-8 water molecules is investigated using an ab initio method. For n = 1-5 water molecules, all the reactants follow a stepwise pathway to the transition state. For n = 6-8 water molecules, all the reactants undergo a direct proton transfer to the transition state with overall lower activation free energy. The activation free energy of the reaction is dramatically reduced from 10.4 to <span class="hlt">2</span>.4 kcal mol -1 as the number of water molecules increases from 1 to 6. Meanwhile, the degree of hydrolysis of <span class="hlt">CO</span> 3 <span class="hlt">2</span>- is significantly increased compared to the bulk water solution scenario. Incomplete hydration shells facilitate the hydrolysis of <span class="hlt">CO</span> 3 <span class="hlt">2</span>- with few water molecules to be not only thermodynamically favorable but also kinetically favorable. We showed that the chemical kinetics is not likely to constrain the speed of <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">air</span> capture driven by the humidity-swing. Instead, the pore-diffusion of ions is expected to be the time-limiting step in the humidity driven <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">air</span> capture. The effect of humidity on the speed of <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">air</span> capture was studied by conducting a <span class="hlt">CO</span> <span class="hlt">2</span> absorption experiment using IER with a high ratio of <span class="hlt">CO</span> 3 <span class="hlt">2</span>- to H <span class="hlt">2</span> O molecules. Our result is able to provide valuable insights into designing efficient <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">air</span>-capture sorbents.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70030985','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70030985"><span><span class="hlt">CO</span><span class="hlt">2</span> transport over complex terrain</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Sun, Jielun; Burns, Sean P.; Delany, A.C.; Oncley, S.P.; Turnipseed, A.A.; Stephens, B.B.; Lenschow, D.H.; LeMone, M.A.; Monson, Russell K.; Anderson, D.E.</p> <p>2007-01-01</p> <p><span class="hlt">CO</span><span class="hlt">2</span> transport processes relevant for estimating net ecosystem <span class="hlt">exchange</span> (NEE) at the Niwot Ridge AmeriFlux site in the front range of the Rocky Mountains, Colorado, USA, were investigated during a pilot experiment. We found that cold, moist, and <span class="hlt">CO</span><span class="hlt">2</span>-rich <span class="hlt">air</span> was transported downslope at night and upslope in the early morning at this forest site situated on a ???5% east-facing slope. We found that <span class="hlt">CO</span><span class="hlt">2</span> advection dominated the total <span class="hlt">CO</span><span class="hlt">2</span> transport in the NEE estimate at night although there are large uncertainties because of partial cancellation of horizontal and vertical advection. The horizontal <span class="hlt">CO</span><span class="hlt">2</span> advection captured not only the <span class="hlt">CO</span><span class="hlt">2</span> loss at night, but also the <span class="hlt">CO</span><span class="hlt">2</span> uptake during daytime. We found that horizontal <span class="hlt">CO</span><span class="hlt">2</span> advection was significant even during daytime especially when turbulent mixing was not significant, such as in early morning and evening transition periods and within the canopy. Similar processes can occur anywhere regardless of whether flow is generated by orography, synoptic pressure gradients, or surface heterogeneity as long as <span class="hlt">CO</span><span class="hlt">2</span> concentration is not well mixed by turbulence. The long-term net effect of all the <span class="hlt">CO</span><span class="hlt">2</span> budget terms on estimates of NEE needs to be investigated. ?? 2007 Elsevier B.V. All rights reserved.</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('https://ntrs.nasa.gov/search.jsp?R=19950044646&hterms=environnement&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Denvironnement','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19950044646&hterms=environnement&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Denvironnement"><span>Sensitivity analysis of a model of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> in tundra ecosystems by the adjoint method</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Waelbroek, C.; Louis, J.-F.</p> <p>1995-01-01</p> <p>A model of net primary production (NPP), decomposition, and nitrogen cycling in tundra ecosystems has been developed. The adjoint technique is used to study the sensitivity of the computed annual net <span class="hlt">CO</span><span class="hlt">2</span> flux to perturbation in initial conditions, climatic inputs, and model's main parameters describing current seasonal <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> in wet sedge tundra at Barrow, Alaska. The results show that net <span class="hlt">CO</span><span class="hlt">2</span> flux is most sensitive to parameters characterizing litter chemical composition and more sensitive to decomposition parameters than to NPP parameters. This underlines the fact that in nutrient-limited ecosystems, decomposition drives net <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> by controlling mineralization of main nutrients. The results also indicate that the short-term (1 year) response of wet sedge tundra to <span class="hlt">CO</span><span class="hlt">2</span>-induced warming is a significant increase in <span class="hlt">CO</span><span class="hlt">2</span> emission, creating a positive feedback to atmosphreic <span class="hlt">CO</span><span class="hlt">2</span> accumulation. However, a cloudiness increase during the same year can severely alter this response and lead to either a slight decrease or a strong increase in emitted <span class="hlt">CO</span><span class="hlt">2</span>, depending on its exact timing. These results demonstrate that the adjoint method is well suited to study systems encountering regime changes, as a single run of the adjoint model provides sensitivities of the net <span class="hlt">CO</span><span class="hlt">2</span> flux to perturbations in all parameters and variables at any time of the year. Moreover, it is shown that large errors due to the presence of thresholds can be avoided by first delimiting the range of applicability of the adjoint results.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.B52B..07K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.B52B..07K"><span>Interannual variability in <span class="hlt">CO</span><span class="hlt">2</span> and CH4 <span class="hlt">exchange</span> in a brackish tidal marsh in Northern California</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Knox, S. H.; Windham-Myers, L.; Anderson, F. E.; Bergamaschi, B. A.</p> <p>2017-12-01</p> <p>Carbon (C) cycling in coastal wetlands is difficult to measure and model due to extremely dynamic atmospheric and hydrologic fluxes, as well as sensitivities to dynamic land- and ocean-based drivers. To date, few studies have begun continuous measurements of net ecosystem <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> (NEE) in these systems, and as such our understanding of the key drivers of NEE in coastal wetlands remain poorly understood. Recent eddy covariance measurements of NEE in these environments show considerable variability both within and across sites, with daily <span class="hlt">CO</span><span class="hlt">2</span> uptake and annual net <span class="hlt">CO</span><span class="hlt">2</span> budgets varying by nearly an order of magnitude between years and across locations. Furthermore, measurements of CH4 fluxes in these systems are even more limited, despite the potential for CH4 emissions from brackish and freshwater coastal wetlands. Here we present 3 years of near-continuous eddy covariance measurements of <span class="hlt">CO</span><span class="hlt">2</span> and CH4 fluxes from a brackish tidal marsh in Northern California and explore the drivers of interannual variability in <span class="hlt">CO</span><span class="hlt">2</span> and CH4 <span class="hlt">exchange</span>. <span class="hlt">CO</span><span class="hlt">2</span> fluxes showed significant interannual variability; net <span class="hlt">CO</span><span class="hlt">2</span> uptake was near-zero in 2014 (6 ± 26 g C-<span class="hlt">CO</span><span class="hlt">2</span> m-<span class="hlt">2</span> yr-1), while much greater uptake was observed in 2015 and 2016 (209 ± 27 g C- <span class="hlt">CO</span><span class="hlt">2</span> m-<span class="hlt">2</span> yr-1 and 243 ± 26 g C-<span class="hlt">CO</span><span class="hlt">2</span> m-<span class="hlt">2</span> yr-1, respectively). Conversely, annual CH4 emissions were small and consistent across years, with the wetland emitting on average 1 ± 0.1 g C-CH4 m-<span class="hlt">2</span> yr-1. With respect to the net atmospheric GHG budget (assuming a sustained global warming potential (SGWP) of 45, expressed in units of <span class="hlt">CO</span><span class="hlt">2</span> equivalents), the wetland was near neutral in 2014, but a net GHG sink of 706 ± 105 g <span class="hlt">CO</span><span class="hlt">2</span> eq m-<span class="hlt">2</span> yr-1 and 836 ± 83 g <span class="hlt">CO</span><span class="hlt">2</span> eq m-<span class="hlt">2</span> yr-1 in 2015 and 2016, respectively. The large interannual variability in <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> was driven by notable year-to-year differences in temperature and precipitation as California experienced a severe drought and record high temperatures from 2012 to 2015. The large interannual variability in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.1657O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.1657O"><span>Net ecosystem <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> and evapotranspiration of a sphagnum mire: field measurements and model simulations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Olchev, Alexander; Volkova, Elena; Karataeva, Tatiana; Zatsarinnaya, Dina; Novenko, Elena</p> <p>2014-05-01</p> <p>The spatial and temporal variability of net ecosystem <span class="hlt">exchange</span> of <span class="hlt">CO</span><span class="hlt">2</span> (NEE) and evapotranspiration (ET) of a karst-hole sphagnum peat mire situated at the boundary between broad-leaved and forest-steppe zones in the central part of European Russia (54.06N, 37.59E, 260 m a.s.l.) was described using results of field measurements and simulations with Mixfor-3D model. The area of the mire is about 1.<span class="hlt">2</span> ha and it is surrounded by a broadleaved forest stand. It is a typical peat mire according to water and mineral supply as well as to vegetation composition. The vegetation of the peripheral parts of the mire is typical eutrophic whereas the vegetation in its central part is represented by meso-oligothrophic plant communities. To describe the spatial variability of NEE and ET within the mire a portable measuring system consisting of a transparent ventilated chamber combined with an infrared <span class="hlt">CO</span><span class="hlt">2</span> and H<span class="hlt">2</span>O analyzer LI-840A (Li-Cor, USA) was used. The measurements were provided along a transect from the southern peripheral part of the mire to its center under sunny clear-sky weather conditions in the period from May to September of 2012 and from May 2013 to October 2013. The chamber method was used for measurements of NEE and ET fluxes because of small size of the mire, a very uniform surrounding forest stand and the mosaic mire vegetation. All these factors promote very heterogeneous <span class="hlt">exchange</span> conditions within the mire and make it difficult to apply, for example, an eddy covariance method that is widely used for flux measurements in the field. The results of the field measurements showed a significant spatial and temporal variability of NEE and ET that was mainly influenced by incoming solar radiation, <span class="hlt">air</span> temperature and ground water level. During the entire growing season the central part of the mire was a sink of <span class="hlt">CO</span><span class="hlt">2</span> for the atmosphere (up to 6.8±4.<span class="hlt">2</span> µmol m-<span class="hlt">2</span> s-1 in June) whereas its peripheral part, due to strong shading by the surrounding forest, was mainly a source of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001GeCoA..65.1907H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001GeCoA..65.1907H"><span>Carbon isotope <span class="hlt">exchange</span> in the system <span class="hlt">CO</span> <span class="hlt">2</span>-CH 4 at elevated temperatures</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Horita, Juske</p> <p>2001-06-01</p> <p>Carbon isotope <span class="hlt">exchange</span> was investigated for the system <span class="hlt">CO</span> <span class="hlt">2</span>-CH 4 at 150 to 600°C in the presence of several potential catalysts by use of isotopically normal or 13C-enriched gases. Silica gel, graphite, molecular sieve Linde 4A, magnetite, and hematite oxidized small amounts of CH 4 in starting <span class="hlt">CO</span> <span class="hlt">2</span>-CH 4 mixtures to <span class="hlt">CO</span> and <span class="hlt">CO</span> <span class="hlt">2</span> but failed to enhance the net rate of carbon isotope <span class="hlt">exchange</span> between <span class="hlt">CO</span> <span class="hlt">2</span> and CH 4, even after 169 to 1833 h at 400 to 500°C. In contrast, several commercial transition-metal catalysts (Ni, Pd, Rh, and Pt) promoted reactions significantly toward chemical and isotopic equilibrium. With the Ni catalyst, the attainment of carbon isotopic equilibrium between <span class="hlt">CO</span> <span class="hlt">2</span> and CH 4 was demonstrated for the first time at temperatures from 200 to 600°C by complete isotopic reversal from opposite directions. The experimentally determined carbon isotope fractionation factors between <span class="hlt">CO</span> <span class="hlt">2</span> and CH 4 (10 3lnα) were similar to, but slightly greater than (0.7-1.1‰, 0.89‰ on average), those of statistical-mechanical calculations by Richet et al. (1977). The experimental results can be described by the following equation between 200 and 600°C only: 10 3lnα(<span class="hlt">CO</span> <span class="hlt">2</span>-CH 4) = 26.70 - 49.137(10 3/T) + 40.828(10 6/T <span class="hlt">2</span>) - 7.512(10 9/T 3) (T = 473.15-873.15 K, 1σ = ±0.14‰, n = 44). Alternatively, an equation generated by fitting Richet et al. (1977) data in the temperature range from 0 to 1300°C can be modified by adding +0.89‰ to its constant; 10 3lnα(<span class="hlt">CO</span> <span class="hlt">2</span>-CH 4) = 0.16 + 11.754(10 6/T <span class="hlt">2</span>) - <span class="hlt">2</span>.3655(10 9/T 3) + 0.2054(10 12/T 4) (T = 273-1573 K, 1σ = ±0.21‰, n = 44). This and other recent experimental studies in the literature demonstrate that transition metals, which are widespread in many natural materials, can catalyze reactions among natural gases at relatively low temperatures (≤200°C). The role of natural catalysts, "geocatalysts," in the abiogenic formation of methane, hydrocarbons, and simple organic compounds has important implications, ranging</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA615405','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA615405"><span>Forecasting Foreign Currency <span class="hlt">Exchange</span> Rates for <span class="hlt">Air</span> Force Budgeting</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2015-03-26</p> <p>FORECASTING FOREIGN CURRENCY <span class="hlt">EXCHANGE</span> RATES FOR <span class="hlt">AIR</span> FORCE BUDGETING THESIS MARCH 2015...States. AFIT-ENV-MS-15-M-178 FORECASTING FOREIGN CURRENCY <span class="hlt">EXCHANGE</span> RATES FOR <span class="hlt">AIR</span> FORCE BUDGETING THESIS Presented to the Faculty...FORECASTING FOREIGN CURRENCY <span class="hlt">EXCHANGE</span> RATES FOR <span class="hlt">AIR</span> FORCE BUDGETING Nicholas R. Gardner, BS Captain, USAF Committee Membership: Lt Col Jonathan</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24375933','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24375933"><span>Conversion of <span class="hlt">CO</span><span class="hlt">2</span> and C<span class="hlt">2</span>H6 to propanoic acid over a Au-<span class="hlt">exchanged</span> MCM-22 zeolite.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sangthong, Winyoo; Probst, Michael; Limtrakul, Jumras</p> <p>2014-02-24</p> <p>Finding novel catalysts for the direct conversion of <span class="hlt">CO</span><span class="hlt">2</span> to fuels and chemicals is a primary goal in energy and environmental research. In this work, density functional theory (DFT) is used to study possible reaction mechanisms for the conversion of <span class="hlt">CO</span><span class="hlt">2</span> and C<span class="hlt">2</span>H6 to propanoic acid over a gold-<span class="hlt">exchanged</span> MCM-22 zeolite catalyst. The reaction begins with the activation of ethane to produce a gold ethyl hydride intermediate. Hydrogen transfers to the framework oxygen leads then to gold ethyl adsorbed on the Brønsted-acid site. The energy barriers for these steps of ethane activation are 9.3 and 16.3 kcal mol(-1), respectively. Two mechanisms of propanoic acid formation are investigated. In the first one, the insertion of <span class="hlt">CO</span><span class="hlt">2</span> into the Au-H bond of the first intermediate yields gold carboxyl ethyl as subsequent intermediate. This is then converted to propanoic acid by forming the relevant C-C bond. The activation energy of the rate-determining step of this pathway is 48.<span class="hlt">2</span> kcal mol(-1). In the second mechanism, <span class="hlt">CO</span><span class="hlt">2</span> interacts with gold ethyl adsorbed on the Brønsted-acid site. Propanoic acid is formed via protonation of <span class="hlt">CO</span><span class="hlt">2</span> by the Brønsted acid and the simultaneous formation of a bond between <span class="hlt">CO</span><span class="hlt">2</span> and the ethyl group. The activation energy there is 44.<span class="hlt">2</span> kcal mol(-1), favoring this second pathway at least at low temperatures. Gold-<span class="hlt">exchanged</span> MCM-22 zeolite can therefore, at least in principle, be used as the catalyst for producing propanoic acid from <span class="hlt">CO</span><span class="hlt">2</span> and ethane. Copyright © 2014 WILEY-VCH Verlag GmbH & <span class="hlt">Co</span>. KGaA, Weinheim.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16604407','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16604407"><span>Potential <span class="hlt">air</span> contamination during <span class="hlt">CO</span><span class="hlt">2</span> angiography using a hand-held syringe: theoretical considerations and gas chromatography.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Cho, David R; Cho, Kyung J; Hawkins, Irvin F</p> <p>2006-01-01</p> <p>To assess <span class="hlt">air</span> contamination in the hand-held syringes currently used for <span class="hlt">CO</span><span class="hlt">2</span> delivery and to determine whether there is an association between their position and the rate of <span class="hlt">air</span> contamination. Assessment of <span class="hlt">air</span> contamination in the syringe (20 ml) included theoretical modeling, mathematical calculation, and gas chromatography (GC). The model was used with Fick's first law to calculate the diffusion of <span class="hlt">CO</span><span class="hlt">2</span> and the amount of <span class="hlt">air</span> contamination. For GC studies, the syringes were placed in the upright, horizontal, and inverted positions and gas samples were obtained after 5, 10, 20, 30, and 60 min. All trials with each position for each sampling time were performed five times. The amounts of <span class="hlt">air</span> contamination with time calculated mathematically were 5-10% less than those of GC. With the diffusivity of <span class="hlt">air-CO</span><span class="hlt">2</span> at 0.1599 cm<span class="hlt">2</span>/sec (9.594 cm<span class="hlt">2</span>/min), <span class="hlt">air</span> contamination was calculated to be 60% at 60 min. With GC <span class="hlt">air</span> contamination was 13% at 5 min, 31% at 20 min, 43% at 30 min, and 68% at 60 min. There was no difference in <span class="hlt">air</span> contamination between the different syringe positions. <span class="hlt">Air</span> contamination occurs in hand-held syringes filled with <span class="hlt">CO</span><span class="hlt">2</span> when they are open to the ambient <span class="hlt">air</span>. The amounts of <span class="hlt">air</span> contamination over time are similar among syringes placed in the upright, horizontal, and inverted positions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/12010472','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/12010472"><span>Water relations and gas <span class="hlt">exchange</span> in poplar and willow under water stress and elevated 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>Johnson, Jon D; Tognetti, Roberto; Paris, Piero</p> <p>2002-05-01</p> <p>Predictions of shifts in rainfall patterns as atmospheric [<span class="hlt">CO</span><span class="hlt">2</span>] increases could impact the growth of fast growing trees such as Populus spp. and Salix spp. and the interaction between elevated <span class="hlt">CO</span><span class="hlt">2</span> and water stress in these species is unknown. The objectives of this study were to characterize the responses to elevated <span class="hlt">CO</span><span class="hlt">2</span> and water stress in these two species, and to determine if elevated <span class="hlt">CO</span><span class="hlt">2</span> mitigated drought stress effects. Gas <span class="hlt">exchange</span>, water potential components, whole plant transpiration and growth response to soil drying and recovery were assessed in hybrid poplar (clone 53-246) and willow (Salix sagitta) rooted cuttings growing in either ambient (350 &mgr;mol mol-1) or elevated (700 &mgr;mol mol-1) atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentration ([<span class="hlt">CO</span><span class="hlt">2</span>]). Predawn water potential decreased with increasing water stress while midday water potentials remained unchanged (isohydric response). Turgor potentials at both predawn and midday increased in elevated [<span class="hlt">CO</span><span class="hlt">2</span>], indicative of osmotic adjustment. Gas <span class="hlt">exchange</span> was reduced by water stress while elevated [<span class="hlt">CO</span><span class="hlt">2</span>] increased photosynthetic rates, reduced leaf conductance and nearly doubled instantaneous transpiration efficiency in both species. Dark respiration decreased in elevated [<span class="hlt">CO</span><span class="hlt">2</span>] and water stress reduced Rd in the trees growing in ambient [<span class="hlt">CO</span><span class="hlt">2</span>]. Willow had 56% lower whole plant hydraulic conductivity than poplar, and showed a 14% increase in elevated [<span class="hlt">CO</span><span class="hlt">2</span>] while poplar was unresponsive. The physiological responses exhibited by poplar and willow to elevated [<span class="hlt">CO</span><span class="hlt">2</span>] and water stress, singly, suggest that these species respond like other tree species. The interaction of [<span class="hlt">CO</span><span class="hlt">2</span>] and water stress suggests that elevated [<span class="hlt">CO</span><span class="hlt">2</span>] did mitigate the effects of water stress in willow, but not in poplar.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/1208301','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/1208301"><span>[Comparative study of respiratory <span class="hlt">exchanging</span> surfaces in birds and mammals].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Jammes, Y</p> <p>1975-01-01</p> <p>Anatomical studies of the respiratory apparatus of birds show evidences for a gas <span class="hlt">exchanging</span> tubular system (parabronchi and <span class="hlt">air</span> capillaries); these <span class="hlt">exchanging</span> structures are entirely dissociated from the ventilatory drive acting on the <span class="hlt">air</span> sacs. A "cross-current" gas <span class="hlt">exchanging</span> system (perpendicular disposition of <span class="hlt">air</span> and blood capillaries) allow a good wash-out of carbon dioxide (Pa<span class="hlt">CO</span><span class="hlt">2</span> lower than PECO<span class="hlt">2</span>). The great efficiency of this lung is allowed by its very large diffusive surface (ASa) and by the high values of lung specific oxygen diffusing capacity (DO<span class="hlt">2</span>/ASa) and of O<span class="hlt">2</span> extraction coefficient in inspired <span class="hlt">air</span>. The ventilatory pattern of birds is characterized by a greater tidal volume and a smaller respiratory frequency than in mammals of same weight. Respiratory centers of birds receive afferences from lung stretch receptors, <span class="hlt">CO</span><span class="hlt">2</span>-sensitive lung receptors and arterial chemoreceptors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27885723','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27885723"><span>Formation of Onion-Like Ni<span class="hlt">Co</span><span class="hlt">2</span> S4 Particles via Sequential Ion-<span class="hlt">Exchange</span> for Hybrid Supercapacitors.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Guan, Bu Yuan; Yu, Le; Wang, Xiao; Song, Shuyan; Lou, Xiong Wen David</p> <p>2017-02-01</p> <p>Onion-like Ni<span class="hlt">Co</span> <span class="hlt">2</span> S 4 particles with unique hollow structured shells are synthesized by a sequential ion-<span class="hlt">exchange</span> strategy. With the structural and compositional advantages, these unique onion-like Ni<span class="hlt">Co</span> <span class="hlt">2</span> S 4 particles exhibit enhanced electrochemical performance as an electrode material for hybrid supercapacitors. © 2016 WILEY-VCH Verlag GmbH & <span class="hlt">Co</span>. KGaA, Weinheim.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28709096','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28709096"><span>Extensive green roof <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> and its seasonal variation quantified by eddy covariance measurements.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Heusinger, Jannik; Weber, Stephan</p> <p>2017-12-31</p> <p>The <span class="hlt">CO</span> <span class="hlt">2</span> surface-atmosphere <span class="hlt">exchange</span> of an unirrigated, extensive green roof in Berlin, Germany was measured by means of the eddy covariance method over a full annual cycle. The present analysis focusses on the cumulative green roof net ecosystem <span class="hlt">exchange</span> of <span class="hlt">CO</span> <span class="hlt">2</span> (NEE), on its seasonal variation and on green roof physiological characteristics by applying a canopy (A-g s ) model. The green roof was a carbon sink with an annual cumulative NEE of -313g<span class="hlt">CO</span> <span class="hlt">2</span> m -<span class="hlt">2</span> year - 1 , equivalent to -85gCm -<span class="hlt">2</span> year - 1 . Three established <span class="hlt">CO</span> <span class="hlt">2</span> flux gap-filling methods were applied to estimate NEE and to study the performance during different meteorological situations. A best estimate NEE time series was established, which chooses the gap filling method with the highest performance. During dry periods daytime carbon uptake was shown to decline linearly with substrate moisture below a threshold of 0.05m 3 m -3 , whereas night-time respiration was unaffected by substrate moisture variation. The roof turned into a temporary C source during dry conditions in summer 2015. We conclude that the carbon uptake of the present green roof can be optimized when substrate moisture is kept above 0.05m 3 m -3 . Copyright © 2017 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24083613','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24083613"><span><span class="hlt">Co</span>-control of local <span class="hlt">air</span> pollutants and <span class="hlt">CO</span><span class="hlt">2</span> in the Chinese iron and steel industry.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mao, Xianqiang; Zeng, An; Hu, Tao; Zhou, Ji; Xing, Youkai; Liu, Shengqiang</p> <p>2013-01-01</p> <p>The present study proposes an integrated multipollutant cocontrol strategy framework in the context of the Chinese iron and steel industry. The unit cost of pollutant reduction (UCPR) was used to examine the cost-effectiveness of each emission reduction measure. The marginal abatement cost (MAC) curves for SO<span class="hlt">2</span>, NOx, PM<span class="hlt">2</span>.5, and <span class="hlt">CO</span><span class="hlt">2</span> were drawn based on the UCPR and the abatement potential. <span class="hlt">Air</span> pollutant equivalence (APeq) captures the nature of the damage value-weights of various <span class="hlt">air</span> pollutants and acts as uniformization multiple <span class="hlt">air</span> pollutants index. Single pollutant abatement routes designed in accordance with the corresponding reduction targets revealed that the cocontrol strategy has promising potential. Moreover, with the same reduction cost limitations as the single pollutant abatement routes, the multipollutant cocontrol routes are able to obtain more desirable pollution reduction and health benefits. <span class="hlt">Co</span>-control strategy generally shows cost-effective advantage over single-pollutant abatement strategy. The results are robust to changing parameters according to sensitivity analysis. <span class="hlt">Co</span>-control strategy would be an important step to achieve energy/carbon intensity targets and pollution control targets in China. Though cocontrol strategy has got some traction in policy debates, there are barriers to integrate it into policy making in the near future in China.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5250046-exchange-coupled-copd-tbco-magneto-optic-storage-films','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5250046-exchange-coupled-copd-tbco-magneto-optic-storage-films"><span><span class="hlt">Exchange</span> coupled <span class="hlt">CoPd/TbCo</span> magneto-optic storage films</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>Gambino, R.J.; Ruf, R.R.; Rishi, R.</p> <p>1989-09-01</p> <p>Films of <span class="hlt">Co</span>Pd with weak perpendicular anisotropy are shown to <span class="hlt">exchange</span> couple to square loop Tb<span class="hlt">Co</span> films on both the Tb and <span class="hlt">Co</span> sides of compensation. The <span class="hlt">exchange</span> is sensitive to reactive impurities at the interface and is broken under conditions that produce as little as one monolayer of paramagnetic compound. Even when the coupling at the interface is strong, the authors show that only a limited thickness of the <span class="hlt">Co</span>Pd layer is spin oriented perpendicular.</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> <span class="hlt">exchange</span> 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 flux 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 fluxes were significantly lower than mean DMS fluxes. While rare, intense monoterpene <span class="hlt">sea-to-air</span> fluxes were observed, coincident with elevated monoterpene mixing ratios. A statistically significant correlation between isoprene vertical flux 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('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=166406&keyword=Dark+AND+net&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=166406&keyword=Dark+AND+net&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>ELEVATED <span class="hlt">CO</span><span class="hlt">2</span> AND TEMPERATURE ALTER THE ECOSYSTEM C <span class="hlt">EXCHANGE</span> IN A YOUNG DOUGLAS FIR MESOCOSM EXPERIMENT</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 investigated the effects of elevated <span class="hlt">CO</span><span class="hlt">2</span> (EC) [ambient <span class="hlt">CO</span><span class="hlt">2</span> (AC) + 190 ppm] and elevated temperature (ET) [ambient temperature (AT) + 3.6 °C] on net ecosystem <span class="hlt">exchange</span> (NEE) of seedling Douglas fir (Pseudotsuga menziesii) mesocosms. As the study utilized seedlings in reconstruc...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012JAP...111gD725W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012JAP...111gD725W"><span>Interface roughness induced asymmetric magnetic property in sputter-deposited <span class="hlt">Co/CoO/Co</span> <span class="hlt">exchange</span> coupled trilayers</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.; Sannomiya, T.; Shi, J.; Nakamura, Y.</p> <p>2012-04-01</p> <p>The effect of interface roughness on magnetic properties of <span class="hlt">exchange</span> coupled polycrystalline <span class="hlt">Co/CoO(tAF)/Co</span> trilayers has been investigated by varying antiferromagnetic layer (<span class="hlt">Co</span>O) thickness. It has been found that the upper <span class="hlt">CoO/Co</span> interface becomes rougher with increasing <span class="hlt">Co</span>O layer thickness, resulting in stronger <span class="hlt">exchange</span> bias of the upper interface than the lower one. The interfacial <span class="hlt">exchange</span> coupling is strengthened by the increase of defect-generated uncompensated antiferromagnetic spins; such spins form coupling with spins in the <span class="hlt">Co</span> layer at the interface. As a result, the <span class="hlt">Co</span>O layer thickness dependence of <span class="hlt">exchange</span> bias is much enhanced for the upper <span class="hlt">Co</span> layer. The transition from anisotropic magnetoresistance to isotropic magnetoresistance for the top <span class="hlt">Co</span> layer has also been found. This could be attributed to the defects, probably partial thin oxide layers, between <span class="hlt">Co</span> grains in the top <span class="hlt">Co</span> layer that leads a switch from spin-orbit scattering related magnetoresistance to spin-dependent electron scattering dominated magnetoresistance.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23758262','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23758262"><span>Toward a lithium-"<span class="hlt">air</span>" battery: the effect of <span class="hlt">CO</span><span class="hlt">2</span> on the chemistry of a lithium-oxygen cell.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lim, Hyung-Kyu; Lim, Hee-Dae; Park, Kyu-Young; Seo, Dong-Hwa; Gwon, Hyeokjo; Hong, Jihyun; Goddard, William A; Kim, Hyungjun; Kang, Kisuk</p> <p>2013-07-03</p> <p>Lithium-oxygen chemistry offers the highest energy density for a rechargeable system as a "lithium-<span class="hlt">air</span> battery". Most studies of lithium-<span class="hlt">air</span> batteries have focused on demonstrating battery operations in pure oxygen conditions; such a battery should technically be described as a "lithium-dioxygen battery". Consequently, the next step for the lithium-"<span class="hlt">air</span>" battery is to understand how the reaction chemistry is affected by the constituents of ambient <span class="hlt">air</span>. Among the components of <span class="hlt">air</span>, <span class="hlt">CO</span><span class="hlt">2</span> is of particular interest because of its high solubility in organic solvents and it can react actively with O<span class="hlt">2</span>(-•), which is the key intermediate species in Li-O<span class="hlt">2</span> battery reactions. In this work, we investigated the reaction mechanisms in the Li-O<span class="hlt">2</span>/<span class="hlt">CO</span><span class="hlt">2</span> cell under various electrolyte conditions using quantum mechanical simulations combined with experimental verification. Our most important finding is that the subtle balance among various reaction pathways influencing the potential energy surfaces can be modified by the electrolyte solvation effect. Thus, a low dielectric electrolyte tends to primarily form Li<span class="hlt">2</span>O<span class="hlt">2</span>, while a high dielectric electrolyte is effective in electrochemically activating <span class="hlt">CO</span><span class="hlt">2</span>, yielding only Li<span class="hlt">2</span><span class="hlt">CO</span>3. Most surprisingly, we further discovered that a high dielectric medium such as DMSO can result in the reversible reaction of Li<span class="hlt">2</span><span class="hlt">CO</span>3 over multiple cycles. We believe that the current mechanistic understanding of the chemistry of <span class="hlt">CO</span><span class="hlt">2</span> in a Li-<span class="hlt">air</span> cell and the interplay of <span class="hlt">CO</span><span class="hlt">2</span> with electrolyte solvation will provide an important guideline for developing Li-<span class="hlt">air</span> batteries. Furthermore, the possibility for a rechargeable Li-O<span class="hlt">2</span>/<span class="hlt">CO</span><span class="hlt">2</span> battery based on Li<span class="hlt">2</span><span class="hlt">CO</span>3 may have merits in enhancing cyclability by minimizing side reactions.</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 flux, as well as to increase knowledge of spatial, seasonal, and interannual variability in this flux.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.B41I2086K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.B41I2086K"><span>Impacts of Vegetation on <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span>, permafrost thaw depth, and NDVI in Alaskan tundra.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kerr, L.; Steltzer, H.; Natali, S.; Schade, J. D.; Mann, P. J.; Holmes, R. M.; Melton, S.</p> <p>2017-12-01</p> <p>Changes in terrestrial carbon cycling in response to a warming climate in the Arctic will, in large part, be driven by current and future composition of the plant community. To better understand the variation in plant community structure and impacts on carbon cycling, we examined relationships between vegetation composition, NDVI, <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span>, and permafrost thaw depth in the Yukon Kuskokwim Delta (YKD) in southwest Alaska. Our study sites included lichen-dominated peat plateaus, tussock tundra, fens, and drained lakes. We found a significant and positive relationship between NDVI and net ecosystem <span class="hlt">exchange</span> across sites. Dominant functional groups across sites included lichen, moss, and graminoid vegetation, but variability in vegetation cover was high both within and across sites. Tussock-dominated tundra, peat plateaus, and drained lakes shared many of the same species, while the fen site had several unique species. Areas with higher lichen cover were associated with low NDVI, low gross primary productivity (GPP), and low net ecosystem <span class="hlt">exchange</span> (NEE) in comparison with areas with little or no lichen cover. Because lichen comprises a large portion of this region's biomass, it is an important variable to consider in the context of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> in the arctic tundra.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1711535S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1711535S"><span>Estimating gas <span class="hlt">exchange</span> of <span class="hlt">CO</span><span class="hlt">2</span> and CH4 between headwater systems and the atmosphere in Southwest Sweden</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Somlai, Celia; Natchimuthu, Sivakiruthika; Bastviken, David; Lorke, Andreas</p> <p>2015-04-01</p> <p>Quantifying the role of inland water systems in terms of carbon sinks and sources and their connection to the terrestrial ecosystems and landscapes is fundamental for improving the balance approach of regional and global carbon budgets. Recent research showed that freshwater bodies emit significant amounts of <span class="hlt">CO</span><span class="hlt">2</span> and CH4 into the atmosphere. The extent of the emissions from small streams and headwaters, however, remains uncertain due to a limited availability of data. Studies have shown that headwater systems receive most of the terrestrial organic carbon, have the highest dissolved <span class="hlt">CO</span><span class="hlt">2</span> concentration and the highest gas <span class="hlt">exchange</span> velocities and cover the largest fractional surface area within fluvial networks. The gas <span class="hlt">exchange</span> between inland waters and the atmosphere is controlled by two factors: the difference between the dissolved gas concentration and its atmospheric equilibrium concentration, and the gas <span class="hlt">exchange</span> velocity. The direct measurement of the dissolved gas concentration of greenhouse gases can be measured straightforwardly, for example, by gas chromatography from headspace extraction of water sample. In contrast, direct measurement of gas <span class="hlt">exchange</span> velocity is more complex and time consuming, as simultaneous measurements with a volatile and nonvolatile inert tracer gas are needed. Here we analyze measurements of gas <span class="hlt">exchange</span> velocities, concentrations and fluxes of dissolved <span class="hlt">CO</span><span class="hlt">2</span> and CH4, as well as loads of total organic and inorganic carbon in 10 reaches in headwater streams in Southwest Sweden. We compare the gas <span class="hlt">exchange</span> velocities measured directly through tracer injections with those estimated through various empirical approaches, which are based on modelled and measured current velocity, stream depth and slope. Furthermore, we estimate the resulting uncertainties of the flux estimates. We also present different time series of dissolved <span class="hlt">CO</span><span class="hlt">2</span>, CH4 and O<span class="hlt">2</span> concentration, water temperature, barometric pressure, electro conductivity, and pH values</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('http://adsabs.harvard.edu/abs/2015EGUGA..1710440H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1710440H"><span>Dynamics of <span class="hlt">CO</span><span class="hlt">2</span>-<span class="hlt">exchange</span> and C-budgets due to soil erosion: Insights from a 4 years observation period</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hoffmann, Mathias; Albiac Borraz, Elisa; Garcia Alba, Juana; Augustin, Jürgen; Sommer, Michael</p> <p>2015-04-01</p> <p>Agriculture in the hummocky ground moraine landscape of NE-Germany is characterized by an increase in energy crop cultivation, like maize or sorghum. Both enhance lateral C fluxes by erosion and induce feedbacks on C dynamics of agroecosystems as a result of reduced wintertime plant cover and vigorous crop growth during summer. However, the actual impact of these phenomena on the <span class="hlt">CO</span><span class="hlt">2</span>-sink/-source function of agricultural landscapes, is still not clear. Therefore, the interdisciplinary project "CarboZALF" was established in Dedelow/Prenzlau (NE-Germany) in 2009. Within the field experiment CarboZALF-D, <span class="hlt">CO</span><span class="hlt">2</span> fluxes for the soil-plant systems were monitored, covering typical landscape relevant soil states in respect to erosion and deposition, like Calcic Cutanic Luvisol and Endogleyic Colluvic Regosol. Automated chamber systems, each consisting of four transparent chambers (<span class="hlt">2</span>.5 m height, basal area <span class="hlt">2</span>.25 m<span class="hlt">2</span>), were placed along gradients at both measurement sites. Monitored <span class="hlt">CO</span><span class="hlt">2</span> fluxes were gap-filled on a high-temporal resolution by modelling ecosystem respiration (Reco), gross primary productivity (GPP) and net ecosystem <span class="hlt">exchange</span> (NEE) based on parallel and continuous measurements of the <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span>, soil and <span class="hlt">air</span> temperatures as well as photosynthetic active radiation (PAR). Gap-filling was e.g. needed in case of chamber malfunctions and abrupt disturbances by farming practice. The monitored crop rotation was corn-winter wheat (<span class="hlt">2</span> a), sorghum-winter triticale and alfalfa (1.5 a). In our presentation we would like to show insights from a 4 years observation period, with prounounced differences between the eroded and the colluvial soil: The Endogleyic Colluvic Regosol showed higher flux rates for Reco, GPP and NEE compared to the Calcic Cutanic Luvisol. Site-specific NEE and C-balances were positively related to soil C-stocks as well as biomass production, and generated a minor C-sink in case of the Calcic Cutanic Luvisol and a highly variable C-source in case of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1426239-understanding-reactive-adsorption-h2s-co2-sodium-exchanged-zeolites','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1426239-understanding-reactive-adsorption-h2s-co2-sodium-exchanged-zeolites"><span>Understanding the Reactive Adsorption of H <span class="hlt">2</span>S and <span class="hlt">CO</span> <span class="hlt">2</span> in Sodium-<span class="hlt">Exchanged</span> Zeolites</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Fetisov, Evgenii O.; Shah, Mansi S; Knight, Christopher; ...</p> <p>2018-02-19</p> <p>Purifying sour natural gas streams containing hydrogen sulfide and carbon dioxide has been a long-standing environmental and economic challenge. In the presence of cation-<span class="hlt">exchanged</span> zeolites, these two acid gases can react to form carbonyl sulfide and water (H <span class="hlt">2</span>S+<span class="hlt">CO</span> <span class="hlt">2</span>H <span class="hlt">2</span>O+COS), but this reaction is rarely accounted for. In this work, we carry out reactive first-principles Monte Carlo (RxFPMC) simulations for mixtures of H <span class="hlt">2</span>S and <span class="hlt">CO</span> <span class="hlt">2</span> in all-silica and Na-<span class="hlt">exchanged</span> forms of zeolite beta to understand the governing principles driving the enhanced conversion. The RxFPMC simulations show that the presence of Na + cations can change the equilibriummore » constant by several orders of magnitude compared to the gas phase or in all-silica beta. The shift in the reaction equilibrium is caused by very strong interactions of H <span class="hlt">2</span>O with Na + that reduce the reaction enthalpy by about 20 kJmol -1. The simulations also demonstrate that the siting of Al atoms in the framework plays an important role. Lastly, the RxFPMC method presented here is applicable to any chemical conversion in any confined environment, where strong interactions of guest molecules with the host framework and high activation energies limit the use of other computational approaches to study reaction equilibria.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=315010&Lab=NHEERL&keyword=smith&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=315010&Lab=NHEERL&keyword=smith&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>A dynamic leaf gas-<span class="hlt">exchange</span> strategy is conserved in woody plants under changing ambient <span class="hlt">CO</span><span class="hlt">2</span>: evidence from carbon isotope discrimination in paleo and <span class="hlt">CO</span><span class="hlt">2</span> enrichment studies</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>Rising atmospheric [<span class="hlt">CO</span><span class="hlt">2</span>], ca, is expected to affect stomatal regulation of leaf gas-<span class="hlt">exchange</span> of woody plants, thus influencing energy fluxes as well as carbon (C), water and nutrient cycling of forests. Researchers have reported that stomata regulate leaf gas-<span class="hlt">exchange</span> around “set...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23190335','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23190335"><span>Oxidation mechanisms of CF<span class="hlt">2</span>Br<span class="hlt">2</span> and CH<span class="hlt">2</span>Br<span class="hlt">2</span> induced by <span class="hlt">air</span> nonthermal plasma.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Schiorlin, Milko; Marotta, Ester; Dal Molin, Marta; Paradisi, Cristina</p> <p>2013-01-02</p> <p>Oxidation mechanisms in <span class="hlt">air</span> nonthermal plasma (NTP) at room temperature and atmospheric pressure were investigated in a corona reactor energized by +dc, -dc, or +pulsed high voltage.. The two bromomethanes CF(<span class="hlt">2</span>)Br(<span class="hlt">2</span>) and CH(<span class="hlt">2</span>)Br(<span class="hlt">2</span>) were chosen as model organic pollutants because of their very different reactivities with OH radicals. Thus, they served as useful mechanistic probes: they respond differently to the presence of humidity in the <span class="hlt">air</span> and give different products. By FT-IR analysis of the postdischarge gas the following products were detected and quantified: <span class="hlt">CO</span>(<span class="hlt">2</span>) and <span class="hlt">CO</span> in the case of CH(<span class="hlt">2</span>)Br(<span class="hlt">2</span>), <span class="hlt">CO</span>(<span class="hlt">2</span>) and F(<span class="hlt">2</span>)C ═ O in the case of CF(<span class="hlt">2</span>)Br(<span class="hlt">2</span>). F(<span class="hlt">2</span>)C ═ O is a long-lived oxidation intermediate due to its low reactivity with atmospheric radicals. It is however removed from the NTP processed gas by passage through a water scrubber resulting in hydrolysis to <span class="hlt">CO</span>(<span class="hlt">2</span>) and HF. Other noncarbon containing products of the discharge were also monitored by FT-IR analysis, including HNO(3) and N(<span class="hlt">2</span>)O. Ozone, an important product of <span class="hlt">air</span> NTP, was never detected in experiments with CF(<span class="hlt">2</span>)Br(<span class="hlt">2</span>) and CH(<span class="hlt">2</span>)Br(<span class="hlt">2</span>) because of the highly efficient ozone depleting cycles catalyzed by BrOx species formed from the bromomethanes. It is concluded that, regardless of the type of corona applied, CF(<span class="hlt">2</span>)Br(<span class="hlt">2</span>) reacts in <span class="hlt">air</span> NTP via a common intermediate, the CF(<span class="hlt">2</span>)Br radical. The possible reactions leading to this radical are discussed, including, for -dc activation, charge <span class="hlt">exchange</span> with O(<span class="hlt">2</span>)(-), a species detected by APCI mass spectrometry.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20050156073','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20050156073"><span>Cost Effective Measures to Reduce <span class="hlt">CO</span><span class="hlt">2</span> Emissions in the <span class="hlt">Air</span> Freight Sector</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Blinge, Magnus</p> <p>2003-01-01</p> <p>This paper presents cost effective measures to reduce <span class="hlt">CO</span><span class="hlt">2</span> emissions in the <span class="hlt">air</span> freight sector. One door-to-door transport chain is studied in detail from a Scandinavian city to a city in southern Europe. The transport chain was selected by a group of representatives from the <span class="hlt">air</span> freight sector in order to encompass general characteristics within the sector. Three different ways of shipping <span class="hlt">air</span> cargo are studied, i.e., by <span class="hlt">air</span> freighter, as belly freight (in passenger aircrafts) and trucking. <span class="hlt">CO</span><span class="hlt">2</span> emissions are calculated for each part of the transport chain and its relative importance towards the total amount <span class="hlt">CO</span><span class="hlt">2</span> emitted during the whole transport chain is shown. It is confirmed that the most <span class="hlt">CO</span><span class="hlt">2</span> emitting part of the transport chain is the actual flight and that it is in the take-off and climbing phases that most fuel are burned. It is also known that the technical development of aircraft implies a reduction in fuel consumption for each new generation of aircraft. Thus, the aircraft manufacturers have an important role in this development. Having confirmed these observations, this paper focuses on other factors that significantly affects the fuel consumption. Analyzed factors are, e.g., optimization of speed and altitude, traffic management, congestion on and around the airfields, tankering, "latest acceptance time" for goods and improving the load factor. The different factors relative contribution to the total emission levels for the transport chain has been estimated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29368776','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29368776"><span>Thermodynamic evidence of flexibility in H<span class="hlt">2</span>O and <span class="hlt">CO</span><span class="hlt">2</span> absorption of transition metal ion <span class="hlt">exchanged</span> zeolite LTA.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Guo, Xin; Wu, Lili; Navrotsky, Alexandra</p> <p>2018-02-07</p> <p>Gas absorption calorimetry has been employed to probe the intercation of water and carbon dioxide with transition metal ion (TM = Mn <span class="hlt">2</span>+ , Fe <span class="hlt">2</span>+ , <span class="hlt">Co</span> <span class="hlt">2</span>+ , Cu <span class="hlt">2</span>+ , and Zn <span class="hlt">2</span>+ ) <span class="hlt">exchanged</span> zeolite A samples. There appears to be a two-phase region, indicative of a guest-induced flexibility transition, separating hydrated zeolite A and its dehydrated form, both of which have variable water content in the single phase region. The differential enthalpy of absorption as a function of water loading directly identifies different strengths of multiple interactions along with possible binding mechanisms of Zn-A and Mn-A exhibiting the highest water absorption with most exothermic initial enthalpies of -125.28 ± 4.82 and -115.30 ± <span class="hlt">2</span>.56 kJ mol -1 . Zn-A and Mn-A also show moderately good capture ability for <span class="hlt">CO</span> <span class="hlt">2</span> with zero-coverage negative enthalpies of -55.59 ± <span class="hlt">2</span>.48 and -44.07 ± 1.53 kJ mol -1 . The thermodynamic information derived from differential enthalpy, chemical potential and differential entropy elucidated the multistage interactive behavior of small guest molecules (H <span class="hlt">2</span> O/<span class="hlt">CO</span> <span class="hlt">2</span> ) and ion-<span class="hlt">exchanged</span> frameworks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013PrOce.109..104C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013PrOce.109..104C"><span><span class="hlt">Sea</span> surface microlayers: A unified physicochemical and biological perspective of the <span class="hlt">air</span>-ocean interface</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cunliffe, Michael; Engel, Anja; Frka, Sanja; Gašparović, Blaženka; Guitart, Carlos; Murrell, J. Colin; Salter, Matthew; Stolle, Christian; Upstill-Goddard, Robert; Wurl, Oliver</p> <p>2013-02-01</p> <p>The <span class="hlt">sea</span> surface microlayer (SML) covers more than 70% of the Earth's surface and is the boundary layer interface between the ocean and the atmosphere. This important biogeochemical and ecological system is critical to a diverse range of Earth system processes, including the synthesis, transformation and cycling of organic material, and the <span class="hlt">air-sea</span> <span class="hlt">exchange</span> of gases, particles and aerosols. In this review we discuss the SML paradigm, taking into account physicochemical and biological characteristics that define SML structure and function. These include enrichments in biogenic molecules such as carbohydrates, lipids and proteinaceous material that contribute to organic carbon cycling, distinct microbial assemblages that participate in <span class="hlt">air-sea</span> gas <span class="hlt">exchange</span>, the generation of climate-active aerosols and the accumulation of anthropogenic pollutants with potentially serious implications for the health of the ocean. Characteristically large physical, chemical and biological gradients thus separate the SML from the underlying water and the available evidence implies that the SML retains its integrity over wide ranging environmental conditions. In support of this we present previously unpublished time series data on bacterioneuston composition and SML surfactant activity immediately following physical SML disruption; these imply timescales of the order of minutes for the reestablishment of the SML following disruption. A progressive approach to understanding the SML and hence its role in global biogeochemistry can only be achieved by considering as an integrated whole, all the key components of this complex environment.</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 fluxes 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 fluxes 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 fluxes of the same order. However, the differences in global net <span class="hlt">air-sea</span> carbon fluxes 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> <span class="hlt">exchange</span>, 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.osti.gov/biblio/7074100-feasibility-co-sub-monitoring-assess-air-quality-mines-using-diesel-equipment','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/7074100-feasibility-co-sub-monitoring-assess-air-quality-mines-using-diesel-equipment"><span>Feasibility of <span class="hlt">CO</span>/sub <span class="hlt">2</span>/ monitoring to assess <span class="hlt">air</span> quality in mines using diesel equipment</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>Daniel, J.H. Jr.</p> <p>1987-01-01</p> <p>The methodology includes: (1) establishing pollutant to <span class="hlt">CO</span>/sub <span class="hlt">2</span>/ ratios for in-service equipment, (<span class="hlt">2</span>) estimating pollutant concentrations from the ratios and in-mine <span class="hlt">CO</span>/sub <span class="hlt">2</span>/ measurements, and (3) using an <span class="hlt">air</span> quality index to combine the pollutants into a single number, which indicates the health hazard associated with the pollutants. For the methodology to be valid, the pollutant to <span class="hlt">CO</span>/sub <span class="hlt">2</span>/ ratios must remain constant if engine operating conditions do not significantly change. However, due to the complex dynamics of the fuel injection system, the fuel-<span class="hlt">air</span> combustion process, and the engine speed-load governing system, the pollutant to <span class="hlt">CO</span>/sub <span class="hlt">2</span>/ ratios maymore » vary during repetitive, but transient engine speed-and-load operation. These transient effects were investigated. In addition, the influence of changing engine conditions due to engine maladjustment, and a practical means to evaluate engine condition were investigated to advance the methodology. The laboratory investigation determined that <span class="hlt">CO</span>/sub <span class="hlt">2</span>/ is an effective indicator of engine exhaust pollutants. It was shown that the exhaust concentrations of carbon monoxide, carbon dioxide, oxides of nitrogen, hydrocarbons, and particulate matter do not significantly vary among repetitive, but transient engine speed-and-load duty cycles typical of in-service equipment. Based on an <span class="hlt">air</span> quality index and threshold limit values, particulate matter exhibited the greatest adverse effect on <span class="hlt">air</span> quality. Particulate mass was separated into volatile (organic soluble fraction) and nonvolatile (insoluble carbon fraction) components. Due to particulate concentrations, the engine operating conditions of overfueling and advanced injector timing had greater adverse effects on <span class="hlt">air</span> quality than the conditions of retarded injector timing, intake <span class="hlt">air</span> restriction, and Federal certification specifications.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23841677','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23841677"><span>Methods to reduce the <span class="hlt">CO</span>(<span class="hlt">2</span>) concentration of educational buildings utilizing internal ventilation by transferred <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>Kalema, T; Viot, M</p> <p>2014-02-01</p> <p>The aim of this study is to develop internal ventilation by transferred <span class="hlt">air</span> to achieve a good indoor climate with low energy consumption in educational buildings with constant <span class="hlt">air</span> volume (CAV) ventilation. Both measurements of <span class="hlt">CO</span><span class="hlt">2</span> concentration and a multi-room calculation model are presented. The study analyzes how to use more efficiently the available spaces and the capacity of CAV ventilation systems in existing buildings and the impact this has on the indoor <span class="hlt">air</span> quality and the energy consumption of the ventilation. The temperature differences can be used to create natural ventilation airflows between neighboring spaces. The behavior of temperature-driven airflows between rooms was studied and included in the calculation model. The effect of openings between neighboring spaces, such as doors or large apertures in the walls, on the <span class="hlt">CO</span><span class="hlt">2</span> concentration was studied in different classrooms. The <span class="hlt">air</span> temperatures and <span class="hlt">CO</span><span class="hlt">2</span> concentrations were measured using a wireless, internet-based measurement system. The multi-room calculation model predicted the <span class="hlt">CO</span><span class="hlt">2</span> concentration in the rooms, which was then compared with the measured ones. Using transferred <span class="hlt">air</span> between occupied and unoccupied spaces can noticeably reduce the total mechanical ventilation rates needed to keep a low <span class="hlt">CO</span><span class="hlt">2</span> concentration. © 2013 John Wiley & Sons A/S. Published by John Wiley & Sons Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..14.4933P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..14.4933P"><span>Growth strategy of Norway spruce under <span class="hlt">air</span> elevated [<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>Pokorny, R.; Urban, O.; Holisova, P.; Sprtova, M.; Sigut, L.; Slipkova, R.</p> <p>2012-04-01</p> <p>Plants will respond to globally increasing atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentration ([<span class="hlt">CO</span><span class="hlt">2</span>]) by acclimation or adaptation at physiological and morphological levels. Considering the temporal onset, physiological responses may be categorized as short-term and morphological ones as long-term responses. The degree of plant growth responses, including cell division and cell expansion, is highly variable. It depends mainly on the specie's genetic predisposition, environment, mineral nutrition status, duration of <span class="hlt">CO</span><span class="hlt">2</span> enrichment, and/or synergetic effects of other stresses. Elevated [<span class="hlt">CO</span><span class="hlt">2</span>] causes changes in tissue anatomy, quantity, size, shape and spatial orientation and can result in altered sink strength. Since, there are many experimental facilities for the investigation of elevated [<span class="hlt">CO</span><span class="hlt">2</span>] effects on trees: i) closed systems or open top chambers (OTCs), ii) semi-open systems (for example glass domes with adjustable lamella windows - DAWs), and iii) free-<span class="hlt">air</span> [<span class="hlt">CO</span><span class="hlt">2</span>] enrichments (FACE); the results are still unsatisfactory due to: i) relatively short-term duration of experiments, ii) cultivation of young plants with different growth strategy comparing to old ones, iii) plant cultivation under artificial soil and weather conditions, and iv) in non-representative stand structure. In this contribution we are discussing the physiological and morphological responses of Norway spruce trees cultivated in DAWs during eight consecutive growing seasons in the context with other results from Norway spruce cultivation under <span class="hlt">air</span>-elevated [<span class="hlt">CO</span><span class="hlt">2</span>] conditions. On the level of physiological responses, we discuss the changes in the rate of <span class="hlt">CO</span><span class="hlt">2</span> assimilation, assimilation capacity, photorespiration, dark respiration, stomatal conductance, water potential and transpiration, and the sensitivity of these physiological processes to temperature. On the level of morphological responses, we discuss the changes in bud and growth phenology, needle and shoot morphology, architecture of crown and root system, wood</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/12095811','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/12095811"><span>Effects of humidified and dry <span class="hlt">air</span> on corneal endothelial cells during vitreal fluid-<span class="hlt">air</span> <span class="hlt">exchange</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Cekiç, Osman; Ohji, Masahito; Hayashi, Atsushi; Fang, Xiao Y; Kusaka, Shunji; Tano, Yasuo</p> <p>2002-07-01</p> <p>To report the immediate anatomic and functional alterations in corneal endothelial cells following use of humidified <span class="hlt">air</span> and dry <span class="hlt">air</span> during vitreal fluid-<span class="hlt">air</span> <span class="hlt">exchange</span> in rabbits. Experimental study. Rabbits undergoing pars plana vitrectomy and lensectomy were perfused with either dry or humidified <span class="hlt">air</span> during fluid-<span class="hlt">air</span> <span class="hlt">exchange</span> for designated durations. Three different experiments were performed. First, control and experimental corneas were examined by scanning electron microscopy (SEM). Second, corneas were stained with Phalloidin-FITC and examined by fluorescein microscopy. Finally, third, transendothelial permeability for carboxyfluorescein was determined using a diffusion chamber. While different from the corneal endothelial cells, those cells exposed to humidified <span class="hlt">air</span> were less stressed than cells exposed to dry <span class="hlt">air</span> by SEM. Actin cytoskeleton was found highly disorganized with dry <span class="hlt">air</span> exposure. Humidified <span class="hlt">air</span> maintained the normal actin cytoskeleton throughout the 20 minutes of fluid-<span class="hlt">air</span> <span class="hlt">exchange</span>. Paracellular carboxyfluorescein leakage was significantly higher in dry <span class="hlt">air</span> insufflated eyes compared with that of the humidified <span class="hlt">air</span> after 5, 10, and 20 minutes of fluid-<span class="hlt">air</span> <span class="hlt">exchange</span> (P =.002, P =.004, and P =.002, respectively). Dry <span class="hlt">air</span> stress during fluid-<span class="hlt">air</span> <span class="hlt">exchange</span> causes significant immediate alterations in monolayer appearance, actin cytoskeleton, and barrier function of corneal endothelium in aphakic rabbit eyes. Use of humidified <span class="hlt">air</span> largely prevents the alterations in monolayer appearance, actin cytoskeleton, and barrier function of corneal endothelial cells.</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, flux 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> flux 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> fluxes 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> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29513512','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29513512"><span>Binding <span class="hlt">CO</span><span class="hlt">2</span> from <span class="hlt">Air</span> by a Bulky Organometallic Cation Containing Primary Amines.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Luo, Yang-Hui; Chen, Chen; Hong, Dan-Li; He, Xiao-Tong; Wang, Jing-Wen; Ding, Ting; Wang, Bo-Jun; Sun, Bai-Wang</p> <p>2018-03-21</p> <p>The organometallic cation 1 (Fe(bipy-NH <span class="hlt">2</span> ) 3 <span class="hlt">2</span>+ , bipy-NH <span class="hlt">2</span> = 4,4'-diamino-<span class="hlt">2,2</span>'-bipyridine), which was constructed in situ in solution, can bind <span class="hlt">CO</span> <span class="hlt">2</span> from <span class="hlt">air</span> effectively with a stoichiometric ratio of 1:4 (1/<span class="hlt">CO</span> <span class="hlt">2</span> ), through the formation of "H-bonded <span class="hlt">CO</span> <span class="hlt">2</span> " species: [<span class="hlt">CO</span> <span class="hlt">2</span> -OH-<span class="hlt">CO</span> <span class="hlt">2</span> ] - and [<span class="hlt">CO</span> <span class="hlt">2</span> -<span class="hlt">CO</span> <span class="hlt">2</span> -OH] - . These two species, along with the captured individual <span class="hlt">CO</span> <span class="hlt">2</span> molecules, connected 1 into a novel 3D (three-dimensional) architecture, that was crystal 1·<span class="hlt">2</span>(OH - )·4(<span class="hlt">CO</span> <span class="hlt">2</span> ). The adsorption isotherms, recycling investigations, and the heat capacity of 1 have been investigated; the results revealed that the organometallic cation 1 can be recycled at least 10 times for the real-world <span class="hlt">CO</span> <span class="hlt">2</span> capture applications. The strategies presented here may provide new hints for the development of new alkanolamine-related absorbents or technologies for <span class="hlt">CO</span> <span class="hlt">2</span> capture and sequestration.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.6354H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.6354H"><span>Sustaining nutrient supply and carbon export in a seasonally-stratifying shelf <span class="hlt">sea</span> through inconsistent production and remineralisation stoichiometry</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Humphreys, Matthew; Moore, Mark; Achterberg, Eric; Chowdhury, Mohammed; Griffiths, Alex; Hartman, Susan; Hopkins, Joanne; Hull, Tom; Kivimäe, Caroline; Sivyer, Dave; Smilenova, Angelina; Wihsgott, Juliane; Woodward, Malcolm</p> <p>2017-04-01</p> <p>Continental shelf <span class="hlt">seas</span> support 15-20% of global primary productivity despite covering only about 5% of the Earth's ocean surface area. As a result, they may have a significant role in oceanic uptake and storage of carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) from the atmosphere, through the 'continental shelf pump' mechanism. The northwest European continental shelf, in particular the Celtic <span class="hlt">Sea</span> (50°N 8°W), was the target of extensive biogeochemical sampling from March 2014 to September 2015, as part of the UK Shelf <span class="hlt">Sea</span> Biogeochemistry research programme (UK-SSB). Here, we use the UK-SSB carbonate chemistry and macronutrient measurements to investigate the biogeochemical seasonality in the temperate, seasonally-stratifying Celtic <span class="hlt">Sea</span>. During the spring-summer, near-surface biological activity removed dissolved inorganic carbon and nutrients, some of which were then exported into the deeper layer. We calculated vertical inventories of these variables throughout 1.5 seasonal cycles and attempted to correct these for <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span>, advection and denitrification, thus isolating the combined effect of net community production and remineralisation on the inorganic macronutrient inventories, and revealing fluctuating deviations from Redfield stoichiometry. Here, we discuss the capacity of these stoichiometric inconsistencies to sustain the Celtic <span class="hlt">Sea</span> nutrient supply, and thus examine whether an effective continental shelf pump for <span class="hlt">CO</span><span class="hlt">2</span> could operate in this region.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.B33B0403C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.B33B0403C"><span>Direct Measurements of Leaf Level CH4 and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Exchange</span> in a Boreal Forest</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Crill, P.; Lindroth, A.; Vestin, P.; Båth, A.</p> <p>2008-12-01</p> <p>Reports of aerobic CH4 sources from leaves and litter of a variety of forests and plant functional types have added a potential mystery to our understanding of CH4 dynamics especially if these sources contribute enough to have a significant impact on the global budget. We have made direct measurements of leaf level CH4 and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> using a quartz branch cuvette in a boreal forest in Norunda, Sweden since August of this year. The cuvette was temperature controlled and was designed to close for 5 minutes every 30 minutes. <span class="hlt">Air</span> was circulated to a Los Gatos CH4/<span class="hlt">CO</span><span class="hlt">2</span> infrared absorption laser spectrometer. <span class="hlt">Air</span> and cuvette temperatures, PAR and UV radiation (Kipp and Zonen, CUV4; spectral range 300-380 nm) were measured at the branch chamber. The study was made in the Norunda 100 years old stand consisting of a mixture of Scots pine (Pinus sylvestris L.) , Birch (Betula sp.) and Norway spruce (Picea abies (L.) Karst.). The cuvette was moved between trees at roughly 5 day intervals. A null empty cuvette period was included in the rotation. The initial data show the expected <span class="hlt">CO</span><span class="hlt">2</span> uptake correlated with incident PAR and low rates of emission at night. However, there was no clear pattern of emissions detectable in the CH4. We estimate that we should be able to resolve a change of 0.5 ppbv CH4 min- 1 with our analytical setup. Both the daytime (1000-1600) and nighttime (2200-0400) averages were less than our detection. Even on very sunny days with high PAR and UV flux values, no consistent pattern was detectable. The lack of a distinct signal may be due to the fact that the past month has been very rainy, it is late in the growth season at these latitudes and sun angles are increasing quickly. The trees were at the northern edge of a clearing and we were also measuring mid height (<span class="hlt">2</span>-3 m) leaves and branches of young trees. The branch cuvette design can also be optimized to improve its sensitivity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1711910C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1711910C"><span>Observations of changes in the dissolved <span class="hlt">CO</span><span class="hlt">2</span> system in the North <span class="hlt">Sea</span>, in four summers of the 2001-2011 decade</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Clargo, Nicola; Salt, Lesley; Thomas, Helmuth; de Baar, Hein</p> <p>2015-04-01</p> <p>Since the industrial revolution, atmospheric concentrations of carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) have risen dramatically, largely due to the combustion of fossil fuels, changes in land-use patterns and the production of cement. The oceans have absorbed a large amount of this <span class="hlt">CO</span><span class="hlt">2</span>, with resulting impacts on ocean chemistry. Coastal <span class="hlt">seas</span> play a significant role in the mitigation of anthropogenic atmospheric <span class="hlt">CO</span><span class="hlt">2</span> as they contribute approximately 10-30% of global primary productivity despite accounting for only 7% of the surface area. The North <span class="hlt">Sea</span> is a perfect natural laboratory in which to study the <span class="hlt">CO</span><span class="hlt">2</span> system as it consists of two biogeochemically distinct regions displaying both oceanic and relatively coastal behaviour. It has also been identified as a continental shelf pump with respect to <span class="hlt">CO</span><span class="hlt">2</span>, transporting it to the deeper waters of the North Atlantic. Large scale forcing has been shown to have a significant impact on the <span class="hlt">CO</span><span class="hlt">2</span> system over varying time scales, often masking the effects of anthropogenic influence. Here, we present data from the North <span class="hlt">Sea</span> spanning the 2001-2011 decade. In order to investigate the dynamics of the dissolved <span class="hlt">CO</span><span class="hlt">2</span> system in this region in the face of climate change, four basin-wide cruises were conducted during the summers of 2001, 2005, 2008 and 2011. The acquired Dissolved Inorganic Carbon (DIC) and alkalinity data were then used to fully resolve the carbon system in order to assess trends over the 2001-2011 decade. We find significant interannual variability, but with a consistent, notable trend in decreasing pH. We found that surface alkalinity remained relatively constant over the decade, whereas DIC increased, indicating that the pH decline is DIC-driven. We also found that the partial pressure of <span class="hlt">CO</span><span class="hlt">2</span> (p<span class="hlt">CO</span><span class="hlt">2</span>) increased faster than concurrent atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentrations, and that the <span class="hlt">CO</span><span class="hlt">2</span> buffering capacity of the North <span class="hlt">Sea</span> decreased over the decade, with implications for future <span class="hlt">CO</span><span class="hlt">2</span> uptake.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/866467','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/866467"><span>Alkali injection system with controlled <span class="hlt">CO</span>.sub.<span class="hlt">2</span> /O.sub.<span class="hlt">2</span> ratios for combustion of coal</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Berry, Gregory F.</p> <p>1988-01-01</p> <p>A high temperature combustion process for an organic fuel containing sulfur n which the nitrogen of <span class="hlt">air</span> is replaced by carbon dioxide for combination with oxygen with the ratio of <span class="hlt">CO</span>.sub.<span class="hlt">2</span> /O.sub.<span class="hlt">2</span> being controlled to generate combustion temperatures above 2000 K. for a gas-gas reaction with SO.sub.<span class="hlt">2</span> and an alkali metal compound to produce a sulfate and in which a portion of the carbon-dioxide rich gas is recycled for mixing with oxygen and/or for injection as a cooling gas upstream from heating <span class="hlt">exchangers</span> to limit fouling of the <span class="hlt">exchangers</span>, with the remaining carbon-dioxide rich gas being available as a source of <span class="hlt">CO</span>.sub.<span class="hlt">2</span> for oil recovery and other purposes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002JGRC..107.3196S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002JGRC..107.3196S"><span>An Oceanic General Circulation Model (OGCM) investigation of the Red <span class="hlt">Sea</span> circulation, 1. <span class="hlt">Exchange</span> between the Red <span class="hlt">Sea</span> and the 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>Sofianos, Sarantis S.; Johns, William E.</p> <p>2002-11-01</p> <p>The mechanisms involved in the seasonal <span class="hlt">exchange</span> between the Red <span class="hlt">Sea</span> and the Indian Ocean are studied using an Oceanic General Circulation Model (OGCM), namely the Miami Isopycnic Coordinate Ocean Model (MICOM). The model reproduces the basic characteristics of the seasonal circulation observed in the area of the strait of Bab el Mandeb. There is good agreement between model results and available observations on the strength of the <span class="hlt">exchange</span> and the characteristics of the water masses involved, as well as the seasonal flow pattern. During winter, this flow consists of a typical inverse estuarine circulation, while during summer, the surface flow reverses, there is an intermediate inflow of relatively cold and fresh water, and the hypersaline outflow at the bottom of the strait is significantly reduced. Additional experiments with different atmospheric forcing (seasonal winds, seasonal thermohaline <span class="hlt">air-sea</span> fluxes, or combinations) were performed in order to assess the role of the atmospheric forcing fields in the <span class="hlt">exchange</span> flow at Bab el Mandeb. The results of both the wind- and thermohaline-driven experiments exhibit a strong seasonality at the area of the strait, which is in phase with the observations. However, it is the combination of both the seasonal pattern of the wind stress and the seasonal thermohaline forcing that can reproduce the observed seasonal variability at the strait. The importance of the seasonal cycle of the thermohaline forcing on the <span class="hlt">exchange</span> flow pattern is also emphasized by these results. In the experiment where the thermohaline forcing is represented by its annual mean, the strength of the <span class="hlt">exchange</span> is reduced almost by half.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.7721Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.7721Z"><span>Role of advection for the ecosystem-atmosphere <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> of alpine grasslands</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhao, Peng; Wohlfahrt, Georg</p> <p>2017-04-01</p> <p>The neglect of the advection contribution could bring uncertainties to the estimation of the net ecosystem <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> (NEE) between ecosystems and the atmosphere, especially in complex terrain and stable atmospheric conditions. In order to quantify the advection flux of <span class="hlt">CO</span><span class="hlt">2</span>, we carried out four monthly field campaigns at different grasslands in the mountainous areas of Italy, Austria, and Germany in 2015 and 2016. The measurement was based on the advection completed mass balance (ACMB) concept. A home-assembled solenoid valve system, together with multiple sampling inlets and a gas analyser, was used to measure <span class="hlt">CO</span><span class="hlt">2</span> concentration online at three heights on the four sides of a control volume of 20 m by 20 m. Advection of <span class="hlt">CO</span><span class="hlt">2</span> was then calculated from the measurement of wind components and <span class="hlt">CO</span><span class="hlt">2</span> gradients. The turbulent flux of <span class="hlt">CO</span><span class="hlt">2</span> was measured by the eddy-covariance technique. Three clear automatic chambers measured NEE as reference. Results showed that both the horizontal and vertical advection contributed more significantly to <span class="hlt">CO</span><span class="hlt">2</span> flux at night time than at daytime. At most sites, the horizontal advection played a more important role than the vertical advection. The above-canopy advection contributed more <span class="hlt">CO</span><span class="hlt">2</span> flux than within-canopy advection due to the short canopy heights. Large variability of NEE measured by the three chambers indicates the challenge of comparing chamber and micrometeorological fluxes resulting from the heterogeneity of the surface.</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/17901296','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17901296"><span>Southern Hemisphere and deep-<span class="hlt">sea</span> warming led deglacial atmospheric <span class="hlt">CO</span><span class="hlt">2</span> rise and tropical warming.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Stott, Lowell; Timmermann, Axel; Thunell, Robert</p> <p>2007-10-19</p> <p>Establishing what caused Earth's largest climatic changes in the past requires a precise knowledge of both the forcing and the regional responses. We determined the chronology of high- and low-latitude climate change at the last glacial termination by radiocarbon dating benthic and planktonic foraminiferal stable isotope and magnesium/calcium records from a marine core collected in the western tropical Pacific. Deep-<span class="hlt">sea</span> temperatures warmed by approximately <span class="hlt">2</span> degrees C between 19 and 17 thousand years before the present (ky B.P.), leading the rise in atmospheric <span class="hlt">CO</span><span class="hlt">2</span> and tropical-surface-ocean warming by approximately 1000 years. The cause of this deglacial deep-water warming does not lie within the tropics, nor can its early onset between 19 and 17 ky B.P. be attributed to <span class="hlt">CO</span><span class="hlt">2</span> forcing. Increasing austral-spring insolation combined with <span class="hlt">sea</span>-ice albedo feedbacks appear to be the key factors responsible for this warming.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20130000016&hterms=Administration+Global&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DAdministration%2BGlobal','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20130000016&hterms=Administration+Global&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DAdministration%2BGlobal"><span>Global and Regional Seasonal Variability of Mid-Tropospheric <span class="hlt">CO</span><span class="hlt">2</span> as Measured by the Atmospheric Infrared Sounder (<span class="hlt">AIRS</span>)</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Pagano, Thomas S.; Olsen, Edward T.; Nguyen, Hai</p> <p>2012-01-01</p> <p>The Atmospheric Infrared Sounder (<span class="hlt">AIRS</span>) is a hyperspectral infrared instrument on the Earth Observing System (EOS) Aqua Spacecraft, launched on May 4, 2002 into a near polar sun-synchronous orbit. <span class="hlt">AIRS</span> has 2378 infrared channels ranging from 3.7 ?m to 15.4 ?m and a 13.5 km footprint at nadir. <span class="hlt">AIRS</span>, in conjunction with the Advanced Microwave Sounding Unit (AMSU), produces temperature profiles with 1K/km accuracy on a global scale, as well as water vapor profiles and trace gas amounts for <span class="hlt">CO</span><span class="hlt">2</span>, <span class="hlt">CO</span>, SO<span class="hlt">2</span>, O3 and CH4. <span class="hlt">AIRS</span> <span class="hlt">CO</span><span class="hlt">2</span> climatologies have been shown to be useful for identifying anomalies associated with geophysical events such as El Nino-Southern Oscillation or Madden-Julian oscillation. In this study, monthly representations of mid-tropospheric <span class="hlt">CO</span><span class="hlt">2</span> are constructed from 10 years of <span class="hlt">AIRS</span> Version 5 monthly Level 3 data. We compare the <span class="hlt">AIRS</span> mid-tropospheric <span class="hlt">CO</span><span class="hlt">2</span> representations to ground-based measurements from the Scripps and National Oceanic and Atmospheric Administration Climate Modeling and Diagnostics Laboratory (NOAA CMDL) ground networks to better understand the phase lag of the <span class="hlt">CO</span><span class="hlt">2</span> seasonal cycle between the surface and middle troposphere. Results show only a small phase lag in the tropics that grows to approximately two months in the northern latitudes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1394545','SCIGOV-DOEDE'); return false;" href="https://www.osti.gov/servlets/purl/1394545"><span>Atmospheric <span class="hlt">CO</span><span class="hlt">2</span> Concentrations--The Canadian Background <span class="hlt">Air</span> Pollution Monitoring Network (1993) (NDP-034)</span></a></p> <p><a target="_blank" href="http://www.osti.gov/dataexplorer">DOE Data Explorer</a></p> <p>Trivett, N. B. A. [Environment Canada, Atmospheric Environment Service, Downsview, Ontario, Canada; Hudec, V. C. [Environment Canada, Atmospheric Environment Service, Downsview, Ontario, Canada; Wong, C. S. [Marine Carbon Research Centre, Institute of Ocean Sciences, Sidney, British Columbia, Canada</p> <p>1993-01-01</p> <p>Flask <span class="hlt">air</span> samples collected at roughly weekly intervals at three Canadian sites [Alert, Northwest Territories (July 1975 through July 1992); Sable Island, Nova Scotia (March 1975 through July 1992); and Cape St. James, British Columbia (May 1979 through July 1992)] were analyzed for <span class="hlt">CO</span><span class="hlt">2</span> concentration with the measurements directly traceable to the WMO primary <span class="hlt">CO</span><span class="hlt">2</span> standards. Each record includes the date, atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentration, and flask classification code. They provide an accurate record of <span class="hlt">CO</span><span class="hlt">2</span> concentration levels in Canada during the past two decades. Because these data are directly traceable to WMO standards, this record may be compared with records from other Background <span class="hlt">Air</span> Pollution Monitoring Network (BAPMoN) stations. The data are in three files (one for each of the monitoring stations) ranging in size from 9.4 to 20.1 kB.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16047319','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16047319"><span>Atmospheric O<span class="hlt">2</span>, <span class="hlt">CO</span><span class="hlt">2</span> and delta13C measurements from aircraft sampling over Griffin Forest, Perthshire, UK.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sturm, Patrick; Leuenberger, Markus; Moncrieff, John; Ramonet, Michel</p> <p>2005-01-01</p> <p>Regular vertical aircraft sampling has been performed in the lower troposphere above Griffin Forest, near Aberfeldy, Perthshire, UK (56 degrees 37'N, 3 degrees 47'W), between February 2003 and May 2004, for analysis of O<span class="hlt">2</span>/N<span class="hlt">2</span>, <span class="hlt">CO</span><span class="hlt">2</span> and delta13C of <span class="hlt">CO</span><span class="hlt">2</span>. We sampled flasks between 800 and 3100 m above <span class="hlt">sea</span> level. The peak-to-peak amplitude of the seasonal cycle of O<span class="hlt">2</span>/N<span class="hlt">2</span> decreases from 171 per meg at 800 m to 113 per meg at 3100 m. Furthermore, the seasonal cycle is shifted from low to high altitudes with a lag of about 1 month. The same features are observed for <span class="hlt">CO</span><span class="hlt">2</span> with a decrease in the peak-to-peak amplitude of the seasonal cycle from 17.6 ppm at 800 m to 11.4 ppm at 3100 m. The vertical profiles show decreasing O<span class="hlt">2</span>/N<span class="hlt">2</span> ratios in summer and increasing O<span class="hlt">2</span>/N<span class="hlt">2</span> ratios in wintertime with increasing sampling height, due to surface <span class="hlt">exchange</span> of oxygen with the land biosphere and the ocean. The O<span class="hlt">2</span>:<span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> ratios of the vertical profiles vary between -1.5 and -<span class="hlt">2</span>.4 mol O<span class="hlt">2</span>/mol <span class="hlt">CO</span><span class="hlt">2</span>. Copyright (c) 2005 John Wiley & Sons, Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20060029193&hterms=air+measurement&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dair%2Bmeasurement','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060029193&hterms=air+measurement&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dair%2Bmeasurement"><span><span class="hlt">Sea</span> surface temperature measurements with <span class="hlt">AIRS</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Aumann, H.</p> <p>2003-01-01</p> <p>The comparison of global <span class="hlt">sea</span> surface skin temperature derived from cloud-free <span class="hlt">AIRS</span> super window channel at 2616 cm-1 (sst2616) with the Real-Time Global <span class="hlt">Sea</span> Surface Temperature for September 2002 shows surprisingly small standard deviation of 0.44K.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1612517W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1612517W"><span>Seasonal variability of the Red <span class="hlt">Sea</span>, from GRACE time-variable gravity and altimeter <span class="hlt">sea</span> surface height measurements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wahr, John; Smeed, David; Leuliette, Eric; Swenson, Sean</p> <p>2014-05-01</p> <p>Seasonal variability of <span class="hlt">sea</span> surface height and mass within the Red <span class="hlt">Sea</span>, occurs mostly through the <span class="hlt">exchange</span> of heat with the atmosphere and wind-driven inflow and outflow of water through the strait of Bab el Mandab that opens into the Gulf of Aden to the south. The seasonal effects of precipitation and evaporation, of water <span class="hlt">exchange</span> through the Suez Canal to the north, and of runoff from the adjacent land, are all small. The flow through the Bab el Mandab involves a net mass transfer into the Red <span class="hlt">Sea</span> during the winter and a net transfer out during the summer. But that flow has a multi-layer pattern, so that in the summer there is actually an influx of cool water at intermediate (~100 m) depths. Thus, summer water in the southern Red <span class="hlt">Sea</span> is warmer near the surface due to higher <span class="hlt">air</span> temperatures, but cooler at intermediate depths (especially in the far south). Summer water in the northern Red <span class="hlt">Sea</span> experiences warming by <span class="hlt">air-sea</span> <span class="hlt">exchange</span> only. The temperature profile affects the water density, which impacts the <span class="hlt">sea</span> surface height but has no effect on vertically integrated mass. Here, we study this seasonal cycle by combining GRACE time-variable mass estimates, altimeter (Jason-1, Jason-<span class="hlt">2</span>, and Envisat) measurements of <span class="hlt">sea</span> surface height, and steric <span class="hlt">sea</span> surface height contributions derived from depth-dependent, climatological values of temperature and salinity obtained from the World Ocean Atlas. We find good consistency, particularly in the northern Red <span class="hlt">Sea</span>, between these three data types. Among the general characteristics of our results are: (1) the mass contributions to seasonal SSHT variations are much larger than the steric contributions; (<span class="hlt">2</span>) the mass signal is largest in winter, consistent with winds pushing water into the Red <span class="hlt">Sea</span> through the Strait of Bab el Mandab in winter, and out during the summer; and (3) the steric signal is largest in summer, consistent with summer <span class="hlt">sea</span> surface warming.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRG..123..787K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRG..123..787K"><span>Direct and Indirect Effects of Tides on Ecosystem-Scale <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Exchange</span> in a Brackish Tidal Marsh in Northern California</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Knox, S. H.; Windham-Myers, L.; Anderson, F.; Sturtevant, C.; Bergamaschi, B.</p> <p>2018-03-01</p> <p>We investigated the direct and indirect influence of tides on net ecosystem <span class="hlt">exchange</span> (NEE) of carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) in a temperate brackish tidal marsh. NEE displayed a tidally driven pattern with obvious characteristics at the multiday scale, with greater net <span class="hlt">CO</span><span class="hlt">2</span> uptake during spring tides than neap tides. Based on the relative mutual information between NEE and biophysical variables, this was driven by a combination of higher water table depth (WTD), cooler <span class="hlt">air</span> temperature, and lower vapor pressure deficit (VPD) during spring tides relative to neap tides, as the fortnightly tidal cycle not only influenced water levels but also strongly modulated water and <span class="hlt">air</span> temperature and VPD. Tides also influenced NEE at shorter timescales, with a reduction in nighttime fluxes during growing season spring tides when the higher of the two semidiurnal tides caused inundation at the site. WTD significantly influenced ecosystem respiration (Reco), with lower Reco during spring tides than neap tides. While WTD did not appear to affect ecosystem photosynthesis (gross ecosystem production, GPP) directly, the impact of tides on temperature and VPD influenced GPP, with higher daily light-use efficiency and photosynthetic activity during spring tides than neap tides when temperature and VPD were lower. The strong direct and indirect influence of tides on NEE across the diel and multiday timescales has important implications for modeling NEE in tidal wetlands and can help inform the timing and frequency of chamber measurements as annual or seasonal net <span class="hlt">CO</span><span class="hlt">2</span> uptake may be underestimated if measurements are only taken during nonflooded periods.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JMS...137...67S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JMS...137...67S"><span>Species and gamete-specific fertilization success of two <span class="hlt">sea</span> urchins under near future levels of 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>Sung, Chan-Gyung; Kim, Tae Won; Park, Young-Gyu; Kang, Seong-Gil; Inaba, Kazuo; Shiba, Kogiku; Choi, Tae Seob; Moon, Seong-Dae; Litvin, Steve; Lee, Kyu-Tae; Lee, Jung-Suk</p> <p>2014-09-01</p> <p>Since the Industrial Revolution, rising atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentration has driven an increase in the partial pressure of <span class="hlt">CO</span><span class="hlt">2</span> in seawater (p<span class="hlt">CO</span><span class="hlt">2</span>), thus lowering ocean pH. We examined the separate effects of exposure of gametes to elevated p<span class="hlt">CO</span><span class="hlt">2</span> and low pH on fertilization success of the <span class="hlt">sea</span> urchin Strongylocentrotus nudus. Sperm and eggs were independently exposed to seawater with p<span class="hlt">CO</span><span class="hlt">2</span> levels ranging from 380 (pH 7.96-8.3) to 6000 ppmv (pH 7.15-7.20). When sperm were exposed, fertilization rate decreased drastically with increased p<span class="hlt">CO</span><span class="hlt">2</span>, even at a concentration of 450 ppmv (pH range: 7.94 to 7.96). Conversely, fertilization of Hemicentrotus pulcherrimus was not significantly changed even when sperm was exposed to p<span class="hlt">CO</span><span class="hlt">2</span> concentrations as high as 750 ppmv. Exposure of S. nudus eggs to seawater with high p<span class="hlt">CO</span><span class="hlt">2</span> did not affect fertilization success, suggesting that the effect of increased p<span class="hlt">CO</span><span class="hlt">2</span> on sperm is responsible for reduced fertilization success. Surprisingly, this result was not related to sperm motility, which was insensitive to p<span class="hlt">CO</span><span class="hlt">2</span>. When seawater was acidified using HCl, leaving p<span class="hlt">CO</span><span class="hlt">2</span> constant, fertilization success in S. nudus remained high (> 80%) until pH decreased to 7.3. While further studies are required to elucidate the physiological mechanism by which elevated p<span class="hlt">CO</span><span class="hlt">2</span> impairs sperm and reduces S. nudus fertilization, this study suggests that in the foreseeable future, <span class="hlt">sea</span> urchin survival may be threatened due to lower fertilization success driven by elevated p<span class="hlt">CO</span><span class="hlt">2</span> rather than by decreased pH in seawater.</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 flux 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 flux always increase the global atmospheric greenhouse gas burden.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JOUC...17..320W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JOUC...17..320W"><span>Distributions and Relationships of <span class="hlt">CO</span><span class="hlt">2</span>, O<span class="hlt">2</span>, and Dimethylsulfide in the Changjiang (Yangtze) Estuary and Its Adjacent Waters in Summer</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wu, Xi; Tan, Tingting; Liu, Chunying; Li, Tie; Liu, Xiaoshou; Yang, Guipeng</p> <p>2018-04-01</p> <p>The distributions and relationships of O<span class="hlt">2</span>, <span class="hlt">CO</span><span class="hlt">2</span>, and dimethylsulfide (DMS) in the Changjiang (Yangtze) Estuary and its adjacent waters were investigated in June 2014. In surface water, mean O<span class="hlt">2</span> saturation level, partial pressure of <span class="hlt">CO</span><span class="hlt">2</span> (p<span class="hlt">CO</span><span class="hlt">2</span>), and DMS concentrations (and ranges) were 110% (89%-167%), 374 μatm (91-640 μatm), and 8.53 nmol L-1 (1.10-27.50 nmol L-1), respectively. The <span class="hlt">sea-to-air</span> fluxes (and ranges) of DMS and <span class="hlt">CO</span><span class="hlt">2</span> were 8.24 μmol m-<span class="hlt">2</span> d-1 (0.26-62.77 μmol m-<span class="hlt">2</span> d-1), and -4.7 mmol m-<span class="hlt">2</span> d-1 (-110.8-31.7 mmol m-<span class="hlt">2</span> d-1), respectively. Dissolved O<span class="hlt">2</span> was oversaturated, DMS concentrations were relatively high, and this region served as a sink of atmospheric <span class="hlt">CO</span><span class="hlt">2</span>. The p<span class="hlt">CO</span><span class="hlt">2</span> was significantly and negatively correlated with the O<span class="hlt">2</span> saturation level, while the DMS concentration showed different positive relationships with the O<span class="hlt">2</span> saturation level in different water masses. In vertical profiles, a hypoxic zone existed below 20 m at a longitude of 123°E. The stratification of temperature and salinity caused by the Taiwan Warm Current suppressed seawater <span class="hlt">exchange</span> between upper and lower layers, resulting in the formation of a hypoxic zone. Oxidative decomposition of organic detritus carried by the Changjiang River Diluted Water (CRDW) consumed abundant O<span class="hlt">2</span> and produced additional <span class="hlt">CO</span><span class="hlt">2</span>. The DMS concentrations decreased because of low phytoplankton biomass in the hypoxic zone. Strong correlations appeared between the O<span class="hlt">2</span> saturation level, p<span class="hlt">CO</span><span class="hlt">2</span> and DMS concentrations in vertical profiles. Our results strongly suggested that CRDW played an important role in the distributions and relationships of O<span class="hlt">2</span>, <span class="hlt">CO</span><span class="hlt">2</span>, and DMS.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.H11H1010J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.H11H1010J"><span>Alteration of bentonite when contacted with supercritical <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>Jinseok, K.; Jo, H. Y.; Yun, S. T.</p> <p>2014-12-01</p> <p>Deep saline formations overlaid by impermeable caprocks with a high sealing capacity are attractive <span class="hlt">CO</span><span class="hlt">2</span> storage reservoirs. Shales, which consist of mainly clay minerals, are potential caprocks for the <span class="hlt">CO</span><span class="hlt">2</span> storage reservoirs. The properties of clay minerals in shales may affect the sealing capacity of shales. In this study, changes in clay minerals' properties when contacted with supercritical (SC) <span class="hlt">CO</span><span class="hlt">2</span> at various conditions were investigated. Bentonite, whichis composed of primarily montmorillonite, was used as the clay material in this study. Batch reactor tests on wet bentonite samples in the presence of SC <span class="hlt">CO</span><span class="hlt">2</span> with or without aqueous phases were conducted at high pressure (12 MPa) and moderate temperature (50 oC) conditions for a week. Results show that the bentonite samples obtained from the tests with SC <span class="hlt">CO</span><span class="hlt">2</span> had less change in porosity than those obtained from the tests without SC <span class="hlt">CO</span><span class="hlt">2</span> (vacuum-drying) at a given reaction time, indicating that the bentonite samples dried in the presence of SC <span class="hlt">CO</span><span class="hlt">2</span> maintained their structure. These results suggest that <span class="hlt">CO</span><span class="hlt">2</span> molecules can diffuse into interlayer of montmorillonite, which is a primary mineral of bentonite, and form a single <span class="hlt">CO</span><span class="hlt">2</span> molecule layer or double <span class="hlt">CO</span><span class="hlt">2</span> molecule layers. The <span class="hlt">CO</span><span class="hlt">2</span> molecules can displace water molecules in the interlayer, resulting in maintaining the interlayer spacing when dehydration occurs. Noticeable changes in reacted bentonite samples obtained from the tests with an aqueous phase (NaCl, CaCl<span class="hlt">2</span>, or <span class="hlt">sea</span> water) are decreases in the fraction of plagioclase and pyrite and formation of carbonate minerals (i.e., calcite and dolomite) and halite. In addition, no significant <span class="hlt">exchanges</span> of Na or Ca on the <span class="hlt">exchangeable</span> complex of the montmorillonite in the presence of SC <span class="hlt">CO</span><span class="hlt">2</span> occurred, resulting in no significant changes in the swelling capacity of bentonite samples after reacting with SC <span class="hlt">CO</span><span class="hlt">2</span> in the presence of aqueous phases. These results might be attributed by the <span class="hlt">CO</span><span class="hlt">2</span> molecule layer, which prevents</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015BGeo...12.2247E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015BGeo...12.2247E"><span>Effects of <span class="hlt">CO</span><span class="hlt">2</span> and iron availability on rbcL gene expression in Bering <span class="hlt">Sea</span> diatoms</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Endo, H.; Sugie, K.; Yoshimura, T.; Suzuki, K.</p> <p>2015-04-01</p> <p>Iron (Fe) can limit phytoplankton productivity in approximately 40% of the global ocean, including in high-nutrient, low-chlorophyll (HNLC) waters. However, there is little information available on the impact of <span class="hlt">CO</span><span class="hlt">2</span>-induced seawater acidification on natural phytoplankton assemblages in HNLC regions. We therefore conducted an on-deck experiment manipulating <span class="hlt">CO</span><span class="hlt">2</span> and Fe using Fe-deficient Bering <span class="hlt">Sea</span> water during the summer of 2009. The concentrations of <span class="hlt">CO</span><span class="hlt">2</span> in the incubation bottles were set at 380 and 600 ppm in the non-Fe-added (control) bottles and 180, 380, 600, and 1000 ppm in the Fe-added bottles. The phytoplankton assemblages were primarily composed of diatoms followed by haptophytes in all incubation bottles as estimated by pigment signatures throughout the 5-day (control) or 6-day (Fe-added treatment) incubation period. At the end of incubation, the relative contribution of diatoms to chlorophyll a biomass was significantly higher in the 380 ppm <span class="hlt">CO</span><span class="hlt">2</span> treatment than in the 600 ppm treatment in the controls, whereas minimal changes were found in the Fe-added treatments. These results indicate that, under Fe-deficient conditions, the growth of diatoms could be negatively affected by the increase in <span class="hlt">CO</span><span class="hlt">2</span> availability. To further support this finding, we estimated the expression and phylogeny of rbcL (which encodes the large subunit of RuBis<span class="hlt">CO</span>) mRNA in diatoms by quantitative reverse transcription polymerase chain reaction (PCR) and clone library techniques, respectively. Interestingly, regardless of Fe availability, the transcript abundance of rbcL decreased in the high <span class="hlt">CO</span><span class="hlt">2</span> treatments (600 and 1000 ppm). The present study suggests that the projected future increase in seawater p<span class="hlt">CO</span><span class="hlt">2</span> could reduce the RuBis<span class="hlt">CO</span> transcription of diatoms, resulting in a decrease in primary productivity and a shift in the food web structure of the Bering <span class="hlt">Sea</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014BGD....1118105E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014BGD....1118105E"><span>Effects of <span class="hlt">CO</span><span class="hlt">2</span> and iron availability on rbcL gene expression in Bering <span class="hlt">Sea</span> diatoms</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Endo, H.; Sugie, K.; Yoshimura, T.; Suzuki, K.</p> <p>2014-12-01</p> <p>Iron (Fe) can limit phytoplankton productivity in approximately 40% of the global ocean, including high-nutrient, low-chlorophyll (HNLC) waters. However, there is little information available on the impact of <span class="hlt">CO</span><span class="hlt">2</span>-induced seawater acidification on natural phytoplankton assemblages in HNLC regions. We therefore conducted an on-deck experiment manipulating <span class="hlt">CO</span><span class="hlt">2</span> and Fe using Fe-deficient Bering <span class="hlt">Sea</span> waters during the summer of 2009. The concentrations of <span class="hlt">CO</span><span class="hlt">2</span> in the incubation bottles were set at 380 and 600 ppm in the non-Fe-added (control) bottles and 180, 380, 600, and 1000 ppm in the Fe-added bottles. The phytoplankton assemblages were primarily composed of diatoms followed by haptophytes in all incubation bottles as estimated by pigment signatures throughout the 7 day incubation period. At the end of incubation, the relative contributions of diatoms to chlorophyll a biomass decreased significantly with increased <span class="hlt">CO</span><span class="hlt">2</span> levels in the controls, whereas minimal changes were found in the Fe-added treatments. These results indicate that, under Fe-deficient conditions, the growth of diatoms was negatively affected by the increase in <span class="hlt">CO</span><span class="hlt">2</span> availability. To confirm this, we estimated the expression and phylogeny of rbcL (which encodes the large subunit of Rubis<span class="hlt">CO</span>) mRNA in diatoms by quantitative reverse transcription PCR and clone library techniques, respectively. Interestingly, regardless of Fe availability, the expression and diversity of rbcL cDNA decreased in the high <span class="hlt">CO</span><span class="hlt">2</span> treatments (600 and 1000 ppm). The present study suggests that the projected future increase in seawater p<span class="hlt">CO</span><span class="hlt">2</span> could reduce the Rubis<span class="hlt">CO</span> activity of diatoms, resulting in a decrease in primary productivity and a shift in the food web structure of the Bering <span class="hlt">Sea</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23301774','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23301774"><span>Effects of <span class="hlt">co</span>-fermentation by Saccharomyces cerevisiae and Issatchenkia orientalis on <span class="hlt">sea</span> buckthorn juice.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Negi, Bharti; Dey, Gargi</p> <p>2013-06-01</p> <p>This work relates to the development of a <span class="hlt">co</span>-fermented product of <span class="hlt">sea</span> buckthorn (Hippophae rhamnoides L.) with Saccharomyces cerevisiae and Issatchenkia orientalis. Besides malic acid degradation, the parameters of present production technology were also standardized with emphasis on the retainability of total phenolic content (TPC) of <span class="hlt">sea</span> buckthorn juice. The effect of <span class="hlt">co</span>-fermentation on physico-chemical characteristics, organic acids, flavonoids, TPC and antioxidant activities was studied. The high-performance liquid chromatography (HPLC) analysis showed 55% reduction in malic acid content after the <span class="hlt">co</span>-fermentation of <span class="hlt">sea</span> buckthorn juice. The TPC of <span class="hlt">sea</span> buckthorn product was <span class="hlt">2</span>.18 g gallic acid equivalent (GAE)/l. The estimated scavenging effect on <span class="hlt">2,2</span>-diphenyl-1-picrylhydrazyl free radicals was <span class="hlt">2</span>.63 Trolox equivalent (TE) mmol/l. Ferric-reducing antioxidant power and <span class="hlt">2,2</span>'-azino-bis(3-ethylbenz-thiazoline-6-sulphonic acid) assays also showed that <span class="hlt">sea</span> buckthorn product was on a par with commercial wines (Cabernet Shiraz and Beaujolais). We conclude that the process of <span class="hlt">co</span>-fermentation resulted in a significant antioxidant potential of <span class="hlt">sea</span> buckthorn product.</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> fluxes 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 <span class="hlt">exchange</span>. 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 fluxes 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('https://www.ncbi.nlm.nih.gov/pubmed/25244869','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25244869"><span>[Steam and <span class="hlt">air</span> <span class="hlt">co</span>-injection in removing TCE in <span class="hlt">2</span>D-sand box].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Ning; Peng, Sheng; Chen, Jia-Jun</p> <p>2014-07-01</p> <p>Steam and <span class="hlt">air</span> <span class="hlt">co</span>-injection is a newly developed and promising soil remediation technique for non-aqueous phase liquids (NAPLs) in vadose zone. In this study, in order to investigate the mechanism of the remediation process, trichloroethylene (TCE) removal using steam and <span class="hlt">air</span> <span class="hlt">co</span>-injection was carried out in a <span class="hlt">2</span>-dimensional sandbox with different layered sand structures. The results showed that <span class="hlt">co</span>-injection perfectly improved the "tailing" effect compared to soil vapor extraction (SVE), and the remediation process of steam and <span class="hlt">air</span> <span class="hlt">co</span>-injection could be divided into SVE stage, steam strengthening stage and heat penetration stage. Removal ratio of the experiment with scattered contaminant area was higher and removal speed was faster. The removal ratios from the two experiments were 93.5% and 88.<span class="hlt">2</span>%, and the removal periods were 83.9 min and 90.6 min, respectively. Steam strengthened the heat penetration stage. The temperature transition region was wider in the scattered NAPLs distribution experiment, which reduced the accumulation of TCE. Slight downward movement of TCE was observed in the experiment with TCE initially distributed in a fine sand zone. And such downward movement of TCE reduced the TCE removal ratio.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2013-08-14/pdf/2013-19756.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2013-08-14/pdf/2013-19756.pdf"><span>78 FR 49484 - <span class="hlt">Exchange</span> of <span class="hlt">Air</span> Force Real Property for Non-<span class="hlt">Air</span> Force Real Property</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>2013-08-14</p> <p>... DEPARTMENT OF DEFENSE Department of <span class="hlt">Air</span> Force <span class="hlt">Exchange</span> of <span class="hlt">Air</span> Force Real Property for Non-<span class="hlt">Air</span> Force Real Property SUMMARY: Notice identifies excess Federal real property under administrative jurisdiction of the United States <span class="hlt">Air</span> Force it intends to <span class="hlt">exchange</span> for real property not currently owned by the...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19740057434&hterms=CO2+H2O&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3DCO2%2BH2O','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19740057434&hterms=CO2+H2O&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3DCO2%2BH2O"><span><span class="hlt">Exchange</span> of adsorbed H<span class="hlt">2</span>O and <span class="hlt">CO</span><span class="hlt">2</span> between the regolith and atmosphere of Mars caused by changes in surface insolation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Fanale, F. P.; Cannon, W. A.</p> <p>1974-01-01</p> <p>Estimates have been made of the capacity of the Martian regolith to <span class="hlt">exchange</span> adsorbed H<span class="hlt">2</span>O and <span class="hlt">CO</span><span class="hlt">2</span> with the atmosphere-plus-cap system (APCS). These estimates are based upon measured isotherms for H<span class="hlt">2</span>O and <span class="hlt">CO</span><span class="hlt">2</span> adsorption on pulverized basalt at low temperatures and on theoretical considerations. A unit column (1 sq cm) of regolith with a deep subsurface temperature of -77 C, considered average for the disk, will contain about 0.4 g of adsorbed <span class="hlt">CO</span><span class="hlt">2</span> and about 1 g of adsorbed H<span class="hlt">2</span>O per meter of depth. Under favorable circumstances the top 3 cm can <span class="hlt">exchange</span> much more H<span class="hlt">2</span>O with the lower atmosphere each day than is necessary to produce the diurnal brightening. The process appears to be seasonally reversible. The total regolith may contain, in the adsorbed phase alone, as much as 1% of the H<span class="hlt">2</span>O and 5% of the <span class="hlt">CO</span><span class="hlt">2</span> surface inventories expected for a hypothetical Mars that has experienced degassing as intensive as that of earth.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5179930','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5179930"><span>Flue-gas and direct-<span class="hlt">air</span> capture of <span class="hlt">CO</span><span class="hlt">2</span> by porous metal–organic materials</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p></p> <p>2017-01-01</p> <p>Sequestration of <span class="hlt">CO</span><span class="hlt">2</span>, either from gas mixtures or directly from <span class="hlt">air</span> (direct <span class="hlt">air</span> capture), is a technological goal important to large-scale industrial processes such as gas purification and the mitigation of carbon emissions. Previously, we investigated five porous materials, three porous metal–organic materials (MOMs), a benchmark inorganic material, Zeolite 13X and a chemisorbent, TEPA-SBA-15, for their ability to adsorb <span class="hlt">CO</span><span class="hlt">2</span> directly from <span class="hlt">air</span> and from simulated flue-gas. In this contribution, a further 10 physisorbent materials that exhibit strong interactions with <span class="hlt">CO</span><span class="hlt">2</span> have been evaluated by temperature-programmed desorption for their potential utility in carbon capture applications: four hybrid ultramicroporous materials, SIFSIX-3-Cu, DICRO-3-Ni-i, SIFSIX-<span class="hlt">2</span>-Cu-i and MOOFOUR-1-Ni; five microporous MOMs, DMOF-1, ZIF-8, MIL-101, UiO-66 and UiO-66-NH<span class="hlt">2</span>; an ultramicroporous MOM, Ni-4-PyC. The performance of these MOMs was found to be negatively impacted by moisture. Overall, we demonstrate that the incorporation of strong electrostatics from inorganic moieties combined with ultramicropores offers improved <span class="hlt">CO</span><span class="hlt">2</span> capture performance from even moist gas mixtures but not enough to compete with chemisorbents. This article is part of the themed issue ‘Coordination polymers and metal–organic frameworks: materials by design’. PMID:27895255</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MS%26E..227a2104P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MS%26E..227a2104P"><span>Numerical calculation of a <span class="hlt">sea</span> water heta <span class="hlt">exchanger</span> using Simulink softwear</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Preda, A.; Popescu, L. L.; Popescu, R. S.</p> <p>2017-08-01</p> <p>To highlight the heat <span class="hlt">exchange</span> taking place between seawater as primary agent and the working fluid (water, glycol or Freon) as secondary agent, I have used the Simulink softwear in order to creat a new sequence for numerical calculation of heat <span class="hlt">exchanging</span>. For optimum heat transfer we opted for a counter movement. The model developed to view the dynamic behavior of the <span class="hlt">exchanger</span> consists of four interconnected levelsess. In the simulations was found that a finer mesh of the whole <span class="hlt">exchanger</span> lead to results much closer to reality. There have been various models meshing, starting from a single cell and then advancing noticed an improvement in resultsSimulations were made in both the summer and the winter, using as a secondary agent process water and glycol solution. Studying heat transfer that occurs in the primary <span class="hlt">exchanger</span> of a heat pump, having the primary fluid <span class="hlt">sea</span> water with this program, we get the data plausible and worthy of consideration. Inserting into the program, the seasonal water temperatures of Black <span class="hlt">Sea</span> water layers, we get a encouraging picture about storage capacity and heat transfer of <span class="hlt">sea</span> water.</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('https://www.osti.gov/biblio/20013654-oxygen-mobility-ceo-sub-ce-sub-zr-sub-sub-compounds-study-co-transient-oxidation-sup-sup-isotopic-exchange','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/20013654-oxygen-mobility-ceo-sub-ce-sub-zr-sub-sub-compounds-study-co-transient-oxidation-sup-sup-isotopic-exchange"><span>Oxygen mobility in CeO{sub <span class="hlt">2</span>} and Ce{sub x}Zr({sub 1-x})O{sub <span class="hlt">2</span>} compounds: Study by <span class="hlt">CO</span> transient oxidation and {sup 18}O/{sup 16}O isotopic <span class="hlt">exchange</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>Madier, Y.; Descorme, C.; Govic, A.M. Le</p> <p></p> <p>Cerium-zirconium mixed oxides (Ce{sub x}Zr{sub 1{minus}x}O{sub <span class="hlt">2</span>}), precalcined at 900 C in dry <span class="hlt">air</span>, were supplied by Rhodia Terres Rares as monophasic solid solutions. Introduction of some zirconium atoms in the ceria lattice by isomorphous substitution clearly influences the final properties of these materials as long as the cubic structure of ceria is maintained. Modifications in oxygen storage capacity (OSC measurements), redox properties (<span class="hlt">CO</span> TPR), and oxygen <span class="hlt">exchange</span> processes (TPIE) were studied. Ce{sub 0.63}Zr{sub 0.37}O{sub <span class="hlt">2</span>} was shown to have the most promising properties with the largest OSC at 400 C and the highest reactivity in O{sub <span class="hlt">2</span>} <span class="hlt">exchange</span>. Allmore » mixed oxides are able to <span class="hlt">exchange</span> very large amounts of oxygen compared to ceria, implying the participation of bulk oxygen. Furthermore, on Ce{sub x}Zr{sub (1{minus}x)}O{sub <span class="hlt">2</span>} samples, oxygen is predominantly <span class="hlt">exchanged</span> via a multiple heteroexchange mechanism involving surface dioxygen species as superoxides or peroxides.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28369320','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28369320"><span>High wind speeds prevent formation of a distinct bacterioneuston community in the <span class="hlt">sea</span>-surface microlayer.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Rahlff, Janina; Stolle, Christian; Giebel, Helge-Ansgar; Brinkhoff, Thorsten; Ribas-Ribas, Mariana; Hodapp, Dorothee; Wurl, Oliver</p> <p>2017-05-01</p> <p>The <span class="hlt">sea</span>-surface microlayer (SML) at the boundary between atmosphere and hydrosphere represents a demanding habitat for bacteria. Wind speed is a crucial but poorly studied factor for its physical integrity. Increasing atmospheric burden of <span class="hlt">CO</span><span class="hlt">2</span>, as suggested for future climate scenarios, may particularly act on this habitat at the <span class="hlt">air-sea</span> interface. We investigated the effect of increasing wind speeds and different p<span class="hlt">CO</span><span class="hlt">2</span> levels on SML microbial communities in a wind-wave tunnel, which offered the advantage of low spatial and temporal variability. We found that enrichment of bacteria in the SML occurred solely at a U10 wind speed of ≤5.6 m s-1 in the tunnel and ≤4.1 m s-1 in the Baltic <span class="hlt">Sea</span>. High p<span class="hlt">CO</span><span class="hlt">2</span> levels further intensified the bacterial enrichment in the SML during low wind speed. In addition, low wind speed and p<span class="hlt">CO</span><span class="hlt">2</span> induced the formation of a distinctive bacterial community as revealed by 16S rRNA gene fingerprints and influenced the presence or absence of individual taxonomic units within the SML. We conclude that physical stability of the SML below a system-specific wind speed threshold induces specific bacterial communities in the SML entailing strong implications for ecosystem functioning by wind-driven impacts on habitat properties, gas <span class="hlt">exchange</span> and matter cycling processes. © FEMS 2017.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFMOS21D1539B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFMOS21D1539B"><span>Real Time Control of <span class="hlt">CO</span><span class="hlt">2</span> Enrichment Experiments on the <span class="hlt">Sea</span> Floor Enabled by the MARS Cabled Observatory</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brewer, P. G.; Mbari Foce Team</p> <p>2010-12-01</p> <p>We report on progress on FOCE (Free Ocean <span class="hlt">CO</span><span class="hlt">2</span> Enrichment) techniques designed to accomplish realistic (that is not contained within land-based aquaria) experiments on the response of deep-<span class="hlt">sea</span> animals and biogeochemical cycles to ocean acidification. Such experiments have long been carried out on ecosystems on land, and the outcome has differed significantly from <span class="hlt">CO</span><span class="hlt">2</span> enrichment in enclosed greenhouse systems, thereby undoing much of the hope for an increase in the large-scale biosphere draw down of atmospheric <span class="hlt">CO</span><span class="hlt">2</span>. It is a far bigger step if deep-<span class="hlt">sea</span> animals and systems are removed from their cold, dark, high pressure and low oxygen native habitat. The equivalent problem in the ocean is far more difficult because of (1) the very different physical forcing; (<span class="hlt">2</span>) the complex reaction rates between <span class="hlt">CO</span><span class="hlt">2</span> and water require delay times between addition and entry to the experimental space; (3) the lack of supporting infrastructure and of adequate sensors; and (4) the need for sophisticated and robust control techniques in both hardware and software. We have overcome almost all of these challenges, and related working systems have already been successfully deployed on the Great Barrier Reef coralline flats with Australian colleagues. We have used the MBARI MARS (Monterey Accelerated Research System) cabled observatory to carry out deep-ocean (880m depth) experiments. The basic experimental unit is a 1m x 1m x 50cm chamber with side arms of ~ 3m length to provide the required chemical delay times for the reaction between admixed <span class="hlt">CO</span><span class="hlt">2</span> enriched <span class="hlt">sea</span> water and emergence of the flow into the main chamber. Controllable thrusters, operated by user commands, help maintain a steady flow of seawater through the experiment. The site is slightly below the depth of the O<span class="hlt">2</span> minimum where small changes in either O<span class="hlt">2</span> from ocean warming, or <span class="hlt">CO</span><span class="hlt">2</span> from ocean acidification can lead to the formation of dead zones. Shallow (near shore) experiments are now also in the late planning stages. We have</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/10369593','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/10369593"><span>Effect of humidity on posterior lens opacification during fluid-<span class="hlt">air</span> <span class="hlt">exchange</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Harlan, J B; Lee, E T; Jensen, P S; de Juan, E</p> <p>1999-06-01</p> <p>To study the relationship of humidity and the rate of lens opacity formation during fluid-<span class="hlt">air</span> <span class="hlt">exchange</span> using an animal model. Vitrectomy and fluid-<span class="hlt">air</span> <span class="hlt">exchange</span> was carried out using 16 eyes of 8 pigmented rabbits. One eye of each rabbit was exposed to dry <span class="hlt">air</span> and the fellow eye received humidified <span class="hlt">air</span> using an intraocular <span class="hlt">air</span> humidifier. In each case, the percent humidity of the intraocular <span class="hlt">air</span> was measured using an in-line hygrometer. Elapsed time from initial <span class="hlt">air</span> entry to lens feathering was recorded for each eye, with the surgeon-observer unaware of the percent humidity of the <span class="hlt">air</span> infusion. In each rabbit, use of humidified <span class="hlt">air</span> resulted in a delay in lens feathering (P<.02), with an overall increase in time to feathering of 80% for humidified <span class="hlt">air</span> vs room <span class="hlt">air</span>. Use of a humidifier during fluid-<span class="hlt">air</span> <span class="hlt">exchange</span> prolongs intraoperative lens clarity in the rabbit model, suggesting that humidified <span class="hlt">air</span> should prolong lens clarity during phakic fluid-<span class="hlt">air</span> <span class="hlt">exchange</span> in patients. Use of humidified <span class="hlt">air</span> during vitrectomy and fluid-<span class="hlt">air</span> <span class="hlt">exchange</span> may retard the intraoperative loss of lens clarity, promoting better visualization of the posterior segment and enhancing surgical performance.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012BGD.....911885C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012BGD.....911885C"><span>Element budgets in an Arctic mesocosm <span class="hlt">CO</span><span class="hlt">2</span> perturbation study</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.; Siljakova, A.; Riebesell, U.</p> <p>2012-08-01</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 the 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 fluxes, in particular due to uncertainties in constraining <span class="hlt">air/sea</span> gas <span class="hlt">exchange</span>, particle sinking, and wall growth. In an Arctic mesocosm study on ocean acidification using KOSMOS (Kiel Off-Shore Mesocosms for future Ocean Simulation) all relevant element pools and fluxes of carbon, nitrogen and phosphorus were measured, using an improved experimental design intended to narrow down some of the mentioned uncertainties. Water column concentrations of particulate and dissolved organic and inorganic constituents were determined daily. New approaches for quantitative estimates of material sinking to the bottom of the mesocosms and gas <span class="hlt">exchange</span> in 48 h temporal resolution, as well as estimates of wall growth were developed to close the gaps in element budgets. Future elevated p<span class="hlt">CO</span><span class="hlt">2</span> was found to enhance net autotrophic community carbon uptake in <span class="hlt">2</span> of the 3 experimental phases but did not significantly affect particle elemental composition. Enhanced carbon consumption appears to result in accumulation of dissolved organic compounds under nutrient recycling summer conditions. This carbon over-consumption effect becomes evident from budget calculations, but was too small to be resolved by direct measurements of dissolved organics. The out-competing of large diatoms by comparatively small algae in nutrient uptake caused reduced production rates under future ocean <span class="hlt">CO</span><span class="hlt">2</span> conditions in the end of the experiment. This <span class="hlt">CO</span><span class="hlt">2</span> induced shift away from diatoms towards smaller phytoplankton and enhanced cycling of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.ars.usda.gov/research/publications/publication/?seqNo115=343528','TEKTRAN'); return false;" href="http://www.ars.usda.gov/research/publications/publication/?seqNo115=343528"><span>The SMAP level 4 carbon product for monitoring ecosystem land-atmosphere <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</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>The NASA Soil Moisture Active Passive (SMAP) mission Level 4 Carbon (L4C) product provides model estimates of Net Ecosystem <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> (NEE) incorporating SMAP soil moisture information. The L4C product includes NEE, computed as total ecosystem respiration less gross photosynthesis, at a daily ti...</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 Flux 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 flux 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 fluxes 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 flux 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> flux 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> flux through regions of thinner, more porous <span class="hlt">sea</span> ice. A full understanding of the processes and feedbacks controlling the flux 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> flux in <span class="hlt">sea</span> ice covered regions is not currently included in global climate models. Incorporating this carbon flux system into Earth System models requires the development of a well-parameterised <span class="hlt">sea</span> ice-<span class="hlt">air</span> flux 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/467654-air-sea-interaction-subtropical-convergence-south-africa','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/467654-air-sea-interaction-subtropical-convergence-south-africa"><span><span class="hlt">Air-sea</span> interaction at the subtropical convergence south of Africa</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>Rouault, M.; Lutjeharms, J.R.E.; Ballegooyen, R.C. van</p> <p>1994-12-31</p> <p>The oceanic region south of Africa plays a key role in the control of Southern Africa weather and climate. This is particularly the case for the Subtropical Convergence region, the northern border of the Southern Ocean. An extensive research cruise to investigate this specific front was carried out during June and July 1993. A strong front, the Subtropical Convergence was identified, however its geographic disposition was complicated by the presence of an intense warm eddy detached from the Agulhas current. The warm surface water in the eddy created a strong contrast between it and the overlying atmosphere. Oceanographic measurements (XBTmore » and CTD) were jointly made with radiosonde observations and <span class="hlt">air-sea</span> interaction measurements. The <span class="hlt">air-sea</span> interaction measurement system included a Gill sonic anemometer, an Ophir infrared hygrometer, an Eppley pyranometer, an Eppley pyrgeometer and a Vaissala temperature and relative humidity probe. Turbulent fluxes of momentum, sensible heat and latent heat were calculated in real time using the inertial dissipation method and the bulk method. All these measurements allowed a thorough investigation of the net heat loss of the ocean, the deepening of the mixed layer during a severe storm as well as the structure of the atmospheric boundary layer and ocean-atmosphere <span class="hlt">exchanges</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27304708','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27304708"><span>Poly(ethylenimine)-Functionalized Monolithic Alumina Honeycomb Adsorbents for <span class="hlt">CO</span><span class="hlt">2</span> Capture from <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>Sakwa-Novak, Miles A; Yoo, Chun-Jae; Tan, Shuai; Rashidi, Fereshteh; Jones, Christopher W</p> <p>2016-07-21</p> <p>The development of practical and effective gas-solid contactors is an important area in the development of <span class="hlt">CO</span><span class="hlt">2</span> capture technologies. Target <span class="hlt">CO</span><span class="hlt">2</span> capture applications, such as postcombustion carbon capture and sequestration (CCS) from power plant flue gases or <span class="hlt">CO</span><span class="hlt">2</span> extraction directly from ambient <span class="hlt">air</span> (DAC), require high flow rates of gas to be processed at low cost. Extruded monolithic honeycomb structures, such as those employed in the catalytic converters of automobiles, have excellent potential as structured contactors for <span class="hlt">CO</span><span class="hlt">2</span> adsorption applications because of the low pressure drop imposed on fluid moving through the straight channels of such structures. Here, we report the impregnation of poly(ethylenimine) (PEI), an effective aminopolymer reported commonly for <span class="hlt">CO</span><span class="hlt">2</span> separation, into extruded monolithic alumina to form structured <span class="hlt">CO</span><span class="hlt">2</span> sorbents. These structured sorbents are first prepared on a small scale, characterized thoroughly, and compared with powder sorbents with a similar composition. Despite consistent differences observed in the filling of mesopores with PEI between the monolithic and powder sorbents, their performance in <span class="hlt">CO</span><span class="hlt">2</span> adsorption is similar across a range of PEI contents. A larger monolithic cylinder (1 inch diameter, 4 inch length) is evaluated under conditions closer to those that might be used in large-scale applications and shows a similar performance to the smaller monoliths and powders tested initially. This larger structure is evaluated over five cycles of <span class="hlt">CO</span><span class="hlt">2</span> adsorption and steam desorption and demonstrates a volumetric capacity of 350 mol<span class="hlt">CO</span><span class="hlt">2</span>  m-3monolith and an equilibration time of 350 min under a 0.4 m s(-1) linear flow velocity through the monolith channels using 400 ppm <span class="hlt">CO</span><span class="hlt">2</span> in N<span class="hlt">2</span> as the adsorption gas at 30 °C. This volumetric capacity surpasses that of a similar technology considered previously, which suggested that <span class="hlt">CO</span><span class="hlt">2</span> could be removed from <span class="hlt">air</span> at an operating cost as low as $100 per ton. © 2016 WILEY-VCH Verlag</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSHE53B..08B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSHE53B..08B"><span>Effect of increased temperature, <span class="hlt">CO</span><span class="hlt">2</span>, and iron on nitrate uptake and primary productivity in the coastal Ross <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>Bronk, D. A.; Spackeen, J.; Sipler, R. E.; Bertrand, E. M.; Roberts, Q. N.; Xu, K.; Baer, S. E.; McQuaid, J.; Zhu, Z.; Walworth, N. G.; Hutchins, D. A.; Allen, A. E.</p> <p>2016-02-01</p> <p>Western Antarctic <span class="hlt">Seas</span> are rapidly changing as a result of elevated concentrations of <span class="hlt">CO</span><span class="hlt">2</span> and rising <span class="hlt">sea</span> surface temperatures. It is critical to determine how the structure and function of microbial communities will be impacted by these changes in the future because the Southern Ocean has seasonally high rates of primary production, is an important sink for anthropogenic <span class="hlt">CO</span><span class="hlt">2</span>, and supports a diverse assemblage of higher trophic level organisms. During the Austral summer of 2013 and 2015, a collaborative research group conducted a series of experiments to understand how the individual and combined effects of temperature, <span class="hlt">CO</span><span class="hlt">2</span>, and iron impact Ross <span class="hlt">Sea</span> microorganisms. Our project used a variety of approaches, including batch experiments, semi-continuous experiments, and continuous-culturing over extended time intervals, to determine how future changes may shift Ross <span class="hlt">Sea</span> microbial communities and how nutrient cycling and carbon biogeochemistry may subsequently be altered. Chemical and biological parameters were measured throughout the experiments to assess changes in community composition and nutrient cycling, including uptake rate measurements of nitrate and bicarbonate by different size fractions of microorganisms. Relative to the control, nitrate uptake rates significantly increased when temperature and iron were elevated indicating that temperature and iron are important physical drivers that influence nutrient cycling. Elevations in temperature and iron independently and synergistically produced higher rates than elevated <span class="hlt">CO</span><span class="hlt">2</span>. Our nutrient uptake results also suggest that the physiology of large microorganisms will be more impacted by climate change variables than small microorganisms.</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> <span class="hlt">exchange</span>, 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 flux 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> flux 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> flux, 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> flux 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/1993GPC.....8...17I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1993GPC.....8...17I"><span>The abiotically driven biological pump in the ocean and short-term fluctuations in atmospheric <span class="hlt">CO</span> <span class="hlt">2</span> contents</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ittekkot, Venugopalan</p> <p>1993-07-01</p> <p>Current debates on the significance of the oceanic "biological pump" in the removal of atmospheric <span class="hlt">CO</span> <span class="hlt">2</span> pay more attention to the act of biological carbon-dioxide fixation (primary productivity) in the <span class="hlt">sea</span>, but pay less or no attention to the equally relevant aspect of the transfer of the fixed carbon to a sink before its oxidation back to <span class="hlt">CO</span> <span class="hlt">2</span>. The upper ocean obviously disqualifies as a sink for biologically fixed <span class="hlt">CO</span> <span class="hlt">2</span> because of gas-<span class="hlt">exchange</span> with the atmosphere. The deep ocean, on the other hand, can be a sink at least at time scales of the ocean turnover. Transfer of newly-fixed <span class="hlt">CO</span> <span class="hlt">2</span> to the deep <span class="hlt">sea</span> can be accelerated by abiogenic matter introduced to the <span class="hlt">sea</span> surface from terrestrial sources. This matter acts as ballast and increases the density and settling rates of aggregates of freshly synthesized organic matter thereby facilitating their rapid removal from the upper ocean. Higher supply of abiogenic matter enhances the sequestering of fresh organic matter and in effect shifts the zone of organic matter remineralization from the upper ocean to the deep <span class="hlt">sea</span>. Consistent with this abiogenic forcing, the rate of organic matter remineralization and the subsequent storage of the remineralized carbon in the deep <span class="hlt">sea</span> are linked to bulk fluxes (mass accumulation rates) in the deep <span class="hlt">sea</span>. This mechanism acts as an "abiotic boost" in the workings of the oceanic "biological pump" and results in an increase in deep <span class="hlt">sea</span> carbon storage; the magnitude of carbon thus stored could have caused the observed short term fluctuations in atmospheric <span class="hlt">CO</span> <span class="hlt">2</span>-contents during the glacial-interglacial cycles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19913293','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19913293"><span><span class="hlt">Sea</span> urchin fertilization in a warm, acidified and high p<span class="hlt">CO</span><span class="hlt">2</span> ocean across a range of sperm densities.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Byrne, Maria; Soars, Natalie; Selvakumaraswamy, Paulina; Dworjanyn, Symon A; Davis, Andrew R</p> <p>2010-05-01</p> <p>Marine invertebrate gametes are being spawned into an ocean simultaneously warming, acidifying and increasing in p<span class="hlt">CO</span>(<span class="hlt">2</span>). Decreased pH/increased p<span class="hlt">CO</span>(<span class="hlt">2</span>) narcotizes sperm indicating that acidification may impair fertilization, exacerbating problems of sperm limitation, with dire implications for marine life. In contrast, increased temperature may have a stimulatory effect, enhancing fertilization. We investigated effects of ocean change on <span class="hlt">sea</span> urchin fertilization across a range of sperm densities. We address two predictions: (1) low pH/increased p<span class="hlt">CO</span>(<span class="hlt">2</span>) reduces fertilization at low sperm density and (<span class="hlt">2</span>) increased temperature enhances fertilization, buffering negative effects of acidification and increased p<span class="hlt">CO</span>(<span class="hlt">2</span>). Neither prediction was supported. Fertilization was only affected by sperm density. Increased acidification and p<span class="hlt">CO</span>(<span class="hlt">2</span>) did not reduce fertilization even at low sperm density and increased temperature did not enhance fertilization. It is important to identify where vulnerabilities lie across life histories and our results indicate that <span class="hlt">sea</span> urchin fertilization is robust to climate change stressors. However, developmental stages may be vulnerable to ocean change. Copyright 2009 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4873644','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4873644"><span>Biological and physical controls in the Southern Ocean on past millennial-scale atmospheric <span class="hlt">CO</span><span class="hlt">2</span> changes</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Gottschalk, Julia; Skinner, Luke C.; Lippold, Jörg; Vogel, Hendrik; Frank, Norbert; Jaccard, Samuel L.; Waelbroeck, Claire</p> <p>2016-01-01</p> <p>Millennial-scale climate changes during the last glacial period and deglaciation were accompanied by rapid changes in atmospheric <span class="hlt">CO</span><span class="hlt">2</span> that remain unexplained. While the role of the Southern Ocean as a 'control valve' on ocean–atmosphere <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> has been emphasized, the exact nature of this role, in particular the relative contributions of physical (for example, ocean dynamics and air–<span class="hlt">sea</span> gas <span class="hlt">exchange</span>) versus biological processes (for example, export productivity), remains poorly constrained. Here we combine reconstructions of bottom-water [O<span class="hlt">2</span>], export production and 14C ventilation ages in the sub-Antarctic Atlantic, and show that atmospheric <span class="hlt">CO</span><span class="hlt">2</span> pulses during the last glacial- and deglacial periods were consistently accompanied by decreases in the biological export of carbon and increases in deep-ocean ventilation via southern-sourced water masses. These findings demonstrate how the Southern Ocean's 'organic carbon pump' has exerted a tight control on atmospheric <span class="hlt">CO</span><span class="hlt">2</span>, and thus global climate, specifically via a synergy of both physical and biological processes. PMID:27187527</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> flux 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> flux 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/2016NatSR...619919S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016NatSR...619919S"><span>Interactions and <span class="hlt">exchange</span> of <span class="hlt">CO</span><span class="hlt">2</span> and H<span class="hlt">2</span>O in coals: an investigation by low-field NMR relaxation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sun, Xiaoxiao; Yao, Yanbin; Liu, Dameng; Elsworth, Derek; Pan, Zhejun</p> <p>2016-01-01</p> <p>The mechanisms by which <span class="hlt">CO</span><span class="hlt">2</span> and water interact in coal remain unclear and these are key questions for understanding ECBM processes and defining the long-term behaviour of injected <span class="hlt">CO</span><span class="hlt">2</span>. In our experiments, we injected helium/<span class="hlt">CO</span><span class="hlt">2</span> to displace water in eight water-saturated samples. We used low-field NMR relaxation to investigate <span class="hlt">CO</span><span class="hlt">2</span> and water interactions in these coals across a variety of time-scales. The injection of helium did not change the T<span class="hlt">2</span> spectra of the coals. In contrast, the T<span class="hlt">2</span> spectra peaks of micro-capillary water gradually decreased and those of macro-capillary and bulk water increased with time after the injection of <span class="hlt">CO</span><span class="hlt">2</span>. We assume that the <span class="hlt">CO</span><span class="hlt">2</span> diffuses through and/or dissolves into the capillary water to access the coal matrix interior, which promotes desorption of water molecules from the surfaces of coal micropores and mesopores. The replaced water mass is mainly related to the Langmuir adsorption volume of <span class="hlt">CO</span><span class="hlt">2</span> and increases as the <span class="hlt">CO</span><span class="hlt">2</span> adsorption capacity increases. Other factors, such as mineral composition, temperature and pressure, also influence the effective <span class="hlt">exchange</span> between water and <span class="hlt">CO</span><span class="hlt">2</span>. Finally, we built a quantified model to evaluate the efficiency of water replacement by <span class="hlt">CO</span><span class="hlt">2</span> injection with respect to temperature and pressure.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26817784','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26817784"><span>Interactions and <span class="hlt">exchange</span> of <span class="hlt">CO</span><span class="hlt">2</span> and H<span class="hlt">2</span>O in coals: an investigation by low-field NMR relaxation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sun, Xiaoxiao; Yao, Yanbin; Liu, Dameng; Elsworth, Derek; Pan, Zhejun</p> <p>2016-01-28</p> <p>The mechanisms by which <span class="hlt">CO</span><span class="hlt">2</span> and water interact in coal remain unclear and these are key questions for understanding ECBM processes and defining the long-term behaviour of injected <span class="hlt">CO</span><span class="hlt">2</span>. In our experiments, we injected helium/<span class="hlt">CO</span><span class="hlt">2</span> to displace water in eight water-saturated samples. We used low-field NMR relaxation to investigate <span class="hlt">CO</span><span class="hlt">2</span> and water interactions in these coals across a variety of time-scales. The injection of helium did not change the T<span class="hlt">2</span> spectra of the coals. In contrast, the T<span class="hlt">2</span> spectra peaks of micro-capillary water gradually decreased and those of macro-capillary and bulk water increased with time after the injection of <span class="hlt">CO</span><span class="hlt">2</span>. We assume that the <span class="hlt">CO</span><span class="hlt">2</span> diffuses through and/or dissolves into the capillary water to access the coal matrix interior, which promotes desorption of water molecules from the surfaces of coal micropores and mesopores. The replaced water mass is mainly related to the Langmuir adsorption volume of <span class="hlt">CO</span><span class="hlt">2</span> and increases as the <span class="hlt">CO</span><span class="hlt">2</span> adsorption capacity increases. Other factors, such as mineral composition, temperature and pressure, also influence the effective <span class="hlt">exchange</span> between water and <span class="hlt">CO</span><span class="hlt">2</span>. Finally, we built a quantified model to evaluate the efficiency of water replacement by <span class="hlt">CO</span><span class="hlt">2</span> injection with respect to temperature and pressure.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017BGeo...14.4467L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017BGeo...14.4467L"><span><span class="hlt">Exchange</span> of <span class="hlt">CO</span><span class="hlt">2</span> in Arctic tundra: impacts of meteorological variations and biological disturbance</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>López-Blanco, Efrén; Lund, Magnus; Williams, Mathew; Tamstorf, Mikkel P.; Westergaard-Nielsen, Andreas; Exbrayat, Jean-François; Hansen, Birger U.; Christensen, Torben R.</p> <p>2017-10-01</p> <p>An improvement in our process-based understanding of carbon (C) <span class="hlt">exchange</span> in the Arctic and its climate sensitivity is critically needed for understanding the response of tundra ecosystems to a changing climate. In this context, we analysed the net ecosystem <span class="hlt">exchange</span> (NEE) of <span class="hlt">CO</span><span class="hlt">2</span> in West Greenland tundra (64° N) across eight snow-free periods in 8 consecutive years, and characterized the key processes of net ecosystem <span class="hlt">exchange</span> and its two main modulating components: gross primary production (GPP) and ecosystem respiration (Reco). Overall, the ecosystem acted as a consistent sink of <span class="hlt">CO</span><span class="hlt">2</span>, accumulating -30 g C m-<span class="hlt">2</span> on average (range of -17 to -41 g C m-<span class="hlt">2</span>) during the years 2008-2015, except 2011 (source of 41 g C m-<span class="hlt">2</span>), which was associated with a major pest outbreak. The results do not reveal a marked meteorological effect on the net <span class="hlt">CO</span><span class="hlt">2</span> uptake despite the high interannual variability in the timing of snowmelt and the start and duration of the growing season. The ranges in annual GPP (-182 to -316 g C m-<span class="hlt">2</span>) and Reco (144 to 279 g C m-<span class="hlt">2</span>) were > 5 fold larger than the range in NEE. Gross fluxes were also more variable (coefficients of variation are 3.6 and 4.1 % respectively) than for NEE (0.7 %). GPP and Reco were sensitive to insolation and temperature, and there was a tendency towards larger GPP and Reco during warmer and wetter years. The relative lack of sensitivity of NEE to meteorology was a result of the correlated response of GPP and Reco. During the snow-free season of the anomalous year of 2011, a biological disturbance related to a larvae outbreak reduced GPP more strongly than Reco. With continued warming temperatures and longer growing seasons, tundra systems will increase rates of C cycling. However, shifts in sink strength will likely be triggered by factors such as biological disturbances, events that will challenge our forecasting of C states.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018HMT....54...69Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018HMT....54...69Z"><span>A numerical study of the supercritical <span class="hlt">CO</span><span class="hlt">2</span> plate heat <span class="hlt">exchanger</span> subject to U-type, Z-type, and multi-pass arrangements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhu, Chen-Xi; Wang, Chi-Chuan</p> <p>2018-01-01</p> <p>This study proposes a numerical model for plate heat <span class="hlt">exchanger</span> that is capable of handling supercritical <span class="hlt">CO</span><span class="hlt">2</span> fluid. The plate heat <span class="hlt">exchangers</span> under investigation include Z-type (1-pass), U-type (1-pass), and 1-<span class="hlt">2</span> pass configurations. The plate spacing is <span class="hlt">2</span>.9 mm with a plate thickness of 0.8 mm, and the size of the plate is 600 mm wide and 218 mm in height with 60 degrees chevron angle. The proposed model takes into account the influence of gigantic change of <span class="hlt">CO</span><span class="hlt">2</span> properties. The simulation is first compared with some existing data for water-to-water plate heat <span class="hlt">exchangers</span> with good agreements. The flow distribution, pressure drop, and heat transfer performance subject to the supercritical <span class="hlt">CO</span><span class="hlt">2</span> in plate heat <span class="hlt">exchangers</span> are then investigated. It is found that the flow velocity increases consecutively from the entrance plate toward the last plate for the Z-type arrangement, and this is applicable for either water side or <span class="hlt">CO</span><span class="hlt">2</span> side. However, the flow distribution of the U-type arrangement in the water side shows opposite trend. Conversely, the flow distribution for U-type arrangement of <span class="hlt">CO</span><span class="hlt">2</span> depends on the specific flow ratio (C*). A lower C* like 0.1 may reverse the distribution, i.e. the flow velocity increases moderately alongside the plate channel like Z-type while a large C* of 1 would resemble the typical distribution in water channel. The flow distribution of <span class="hlt">CO</span><span class="hlt">2</span> side at the first and last plate shows a pronounced drop/surge phenomenon while the channels in water side does not reveal this kind of behavior. The performance of <span class="hlt">2</span>-pass plate heat <span class="hlt">exchanger</span>, in terms of heat transfer rate, is better than that of 1-pass design only when C* is comparatively small (C* < 0.5). Multi-pass design is more effective when the dominant thermal resistance falls in the <span class="hlt">CO</span><span class="hlt">2</span> side.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22869804','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22869804"><span>An <span class="hlt">air</span>-liquid contactor for large-scale capture of <span class="hlt">CO</span><span class="hlt">2</span> from <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>Holmes, Geoffrey; Keith, David W</p> <p>2012-09-13</p> <p>We present a conceptually simple method for optimizing the design of a gas-liquid contactor for capture of carbon dioxide from ambient <span class="hlt">air</span>, or '<span class="hlt">air</span> capture'. We apply the method to a slab geometry contactor that uses components, design and fabrication methods derived from cooling towers. We use mass transfer data appropriate for capture using a strong NaOH solution, combined with engineering and cost data derived from engineering studies performed by Carbon Engineering Ltd, and find that the total costs for <span class="hlt">air</span> contacting alone-no regeneration-can be of the order of $60 per tonne <span class="hlt">CO</span>(<span class="hlt">2</span>). We analyse the reasons why our cost estimate diverges from that of other recent reports and conclude that the divergence arises from fundamental design choices rather than from differences in costing methodology. Finally, we review the technology risks and conclude that they can be readily addressed by prototype testing.</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('https://pubs.er.usgs.gov/publication/70033070','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70033070"><span>Elevated <span class="hlt">CO</span><span class="hlt">2</span> enhances biological contributions to elevation change in coastal wetlands by offsetting stressors associated with <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>Cherry, J.A.; McKee, K.L.; Grace, J.B.</p> <p>2009-01-01</p> <p>1. <span class="hlt">Sea</span>-level rise, one indirect consequence of increasing atmospheric <span class="hlt">CO</span><span class="hlt">2</span>, poses a major challenge to long-term stability of coastal wetlands. An important question is whether direct effects of elevated <span class="hlt">CO</span> <span class="hlt">2</span> on the capacity of marsh plants to accrete organic material and to maintain surface elevations outweigh indirect negative effects of stressors associated with <span class="hlt">sea</span>-level rise (salinity and flooding). <span class="hlt">2</span>. In this study, we used a mesocosm approach to examine potential direct and indirect effects of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentration, salinity and flooding on elevation change in a brackish marsh community dominated by a C3 species, Schoenoplectus americanus, and a C4 grass, Spartina patens. This experimental design permitted identification of mechanisms and their role in controlling elevation change, and the development of models that can be tested in the field. 3. To test hypotheses related to <span class="hlt">CO</span><span class="hlt">2</span> and <span class="hlt">sea</span>-level rise, we used conventional anova procedures in conjunction with structural equation modelling (SEM). SEM explained 78% of the variability in elevation change and showed the direct, positive effect of S. americanus production on elevation. The SEM indicated that C3 plant response was influenced by interactive effects between <span class="hlt">CO</span><span class="hlt">2</span> and salinity on plant growth, not a direct <span class="hlt">CO</span><span class="hlt">2</span> fertilization effect. Elevated <span class="hlt">CO</span><span class="hlt">2</span> ameliorated negative effects of salinity on S. americanus and enhanced biomass contribution to elevation. 4. The positive relationship between S. americanus production and elevation change can be explained by shoot-base expansion under elevated <span class="hlt">CO</span> <span class="hlt">2</span> conditions, which led to vertical soil displacement. While the response of this species may differ under other environmental conditions, shoot-base expansion and the general contribution of C3 plant production to elevation change may be an important mechanism contributing to soil expansion and elevation gain in other coastal wetlands. 5. Synthesis. Our results revealed previously unrecognized interactions and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.B51G0644L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.B51G0644L"><span>Temperature effects on microbial respiration assessed with <span class="hlt">CO</span><span class="hlt">2</span>-<span class="hlt">exchange</span> and continuous culture techniques</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lehmeier, C.; Min, K.; Song, C.; Ballantyne, F.; Billings, S. A.</p> <p>2012-12-01</p> <p>Recent work attempts to incorporate requirements of soil microorganisms for carbon and other resources, and how these requirements may respond to temperature, into theoretical concepts of soil organic matter decomposition and climate change. Because of the difficulties of measuring resource fluxes in natural soils, empirical data to guide these concepts remain scarce. Here, we present an experimental system that combines continuous culture techniques with <span class="hlt">CO</span><span class="hlt">2</span> measurements to study carbon fluxes through microbes in a reductionist, controlled environment amenable to experimental manipulation. In this pilot study, we quantified mass specific respiration rates (MSR) and δ13C of respired <span class="hlt">CO</span><span class="hlt">2</span> of Pseudomonas fluorescens, a Gram-negative bacterium common to soils, grown at 15°C and 25°C with otherwise identical environmental conditions. The microbes were grown in a 1.9 L bioreactor, in 0.9 L of nutrient medium with C:N:P atomic ratios of 100:10:3, and with 10 mM cellobiose as the carbon source. A peristaltic pump continuously supplied the bioreactor with sterile medium, and removed medium from the bioreactor, at a rate of 63 mL h-1. Both vessels were contained within a temperature incubator, and stir bars provided continuously well mixed volumes. <span class="hlt">CO</span><span class="hlt">2</span>-free <span class="hlt">air</span> was continuously bubbled through the reactor medium so to provide the microbes with O<span class="hlt">2</span>; a cavity ring down spectrometer withdrew reactor headspace <span class="hlt">air</span> and measured concentration and δ13C of the <span class="hlt">CO</span><span class="hlt">2</span>. <span class="hlt">Air</span> supply was regulated with a pressure/mass flow controller to approx. 27 mL min-1. In both temperature regimes, the pH of the bioreactor as well as concentration and δ13C of the <span class="hlt">CO</span><span class="hlt">2</span> in the head space <span class="hlt">air</span> were constant over the course of 1 d, such that any imbalances in the <span class="hlt">CO</span><span class="hlt">2</span>-H<span class="hlt">2</span><span class="hlt">CO</span>3 equilibrium were considered negligible in the assessment of microbial respiration rates and the δ13C of respired <span class="hlt">CO</span><span class="hlt">2</span>. After this time period, reactor medium was passed through a 0.22 μm filter and the filtrate dried for 24 h to obtain</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24455157','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24455157"><span>Growing season net ecosystem <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> of two desert ecosystems with alkaline soils in Kazakhstan.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Li, Longhui; Chen, Xi; van der Tol, Christiaan; Luo, Geping; Su, Zhongbo</p> <p>2014-01-01</p> <p>Central Asia is covered by vast desert ecosystems, and the majority of these ecosystems have alkaline soils. Their contribution to global net ecosystem <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> (NEE) is of significance simply because of their immense spatial extent. Some of the latest research reported considerable abiotic <span class="hlt">CO</span><span class="hlt">2</span> absorption by alkaline soil, but the rate of <span class="hlt">CO</span><span class="hlt">2</span> absorption has been questioned by peer communities. To investigate the issue of carbon cycle in Central Asian desert ecosystems with alkaline soils, we have measured the NEE using eddy covariance (EC) method at two alkaline sites during growing season in Kazakhstan. The diurnal course of mean monthly NEE followed a clear sinusoidal pattern during growing season at both sites. Both sites showed significant net carbon uptake during daytime on sunny days with high photosynthetically active radiation (PAR) but net carbon loss at nighttime and on cloudy and rainy days. NEE has strong dependency on PAR and the response of NEE to precipitation resulted in an initial and significant carbon release to the atmosphere, similar to other ecosystems. These findings indicate that biotic processes dominated the carbon processes, and the contribution of abiotic carbon process to net ecosystem <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> may be trivial in alkaline soil desert ecosystems over Central Asia.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3894884','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3894884"><span>Growing season net ecosystem <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> of two desert ecosystems with alkaline soils in Kazakhstan</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Li, Longhui; Chen, Xi; van der Tol, Christiaan; Luo, Geping; Su, Zhongbo</p> <p>2014-01-01</p> <p>Central Asia is covered by vast desert ecosystems, and the majority of these ecosystems have alkaline soils. Their contribution to global net ecosystem <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> (NEE) is of significance simply because of their immense spatial extent. Some of the latest research reported considerable abiotic <span class="hlt">CO</span><span class="hlt">2</span> absorption by alkaline soil, but the rate of <span class="hlt">CO</span><span class="hlt">2</span> absorption has been questioned by peer communities. To investigate the issue of carbon cycle in Central Asian desert ecosystems with alkaline soils, we have measured the NEE using eddy covariance (EC) method at two alkaline sites during growing season in Kazakhstan. The diurnal course of mean monthly NEE followed a clear sinusoidal pattern during growing season at both sites. Both sites showed significant net carbon uptake during daytime on sunny days with high photosynthetically active radiation (PAR) but net carbon loss at nighttime and on cloudy and rainy days. NEE has strong dependency on PAR and the response of NEE to precipitation resulted in an initial and significant carbon release to the atmosphere, similar to other ecosystems. These findings indicate that biotic processes dominated the carbon processes, and the contribution of abiotic carbon process to net ecosystem <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> may be trivial in alkaline soil desert ecosystems over Central Asia. PMID:24455157</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=65336&keyword=Austria&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=65336&keyword=Austria&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><span class="hlt">CO</span><span class="hlt">2</span> AND O3 ALTER PHOTOSYNTHESIS AND WATER VAPOR <span class="hlt">EXCHANGE</span> FOR PINUS PONDEROSA NEEDLES</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>1. Effects of <span class="hlt">CO</span><span class="hlt">2</span> and O3 were determined for a key component of ecosystem carbon and water cycling: needle gas <span class="hlt">exchange</span> (photosynthesis, conductance, transpiration and water use efficiency). The measurements were made on Pinus ponderosa seedlings grown in outdoor, sunlit, mesoc...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013DSRII..92..249B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013DSRII..92..249B"><span>The response of abyssal organisms to low pH conditions during a series of <span class="hlt">CO</span><span class="hlt">2</span>-release experiments simulating deep-<span class="hlt">sea</span> carbon sequestration</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Barry, J. P.; Buck, K. R.; Lovera, C.; Brewer, P. G.; Seibel, B. A.; Drazen, J. C.; Tamburri, M. N.; Whaling, P. J.; Kuhnz, L.; Pane, E. F.</p> <p>2013-08-01</p> <p>The effects of low-pH, high-p<span class="hlt">CO</span><span class="hlt">2</span> conditions on deep-<span class="hlt">sea</span> organisms were examined during four deep-<span class="hlt">sea</span> <span class="hlt">CO</span><span class="hlt">2</span> release experiments simulating deep-ocean C sequestration by the direct injection of <span class="hlt">CO</span><span class="hlt">2</span> into the deep <span class="hlt">sea</span>. We examined the survival of common deep-<span class="hlt">sea</span>, benthic organisms (microbes; macrofauna, dominated by Polychaeta, Nematoda, Crustacea, Mollusca; megafauna, Echinodermata, Mollusca, Pisces) exposed to low-pH waters emanating as a dissolution plume from pools of liquid carbon dioxide released on the seabed during four abyssal <span class="hlt">CO</span><span class="hlt">2</span>-release experiments. Microbial abundance in deep-<span class="hlt">sea</span> sediments was unchanged in one experiment, but increased under environmental hypercapnia during another, where the microbial assemblage may have benefited indirectly from the negative impact of low-pH conditions on other taxa. Lower abyssal metazoans exhibited low survival rates near <span class="hlt">CO</span><span class="hlt">2</span> pools. No urchins or holothurians survived during 30-42 days of exposure to episodic, but severe environmental hypercapnia during one experiment (E1; pH reduced by as much as ca. 1.4 units). These large pH reductions also caused 75% mortality for the deep-<span class="hlt">sea</span> amphipod, Haploops lodo, near <span class="hlt">CO</span><span class="hlt">2</span> pools. Survival under smaller pH reductions (ΔpH<0.4 units) in other experiments (E<span class="hlt">2</span>, E3, E5) was higher for all taxa, including echinoderms. Gastropods, cephalopods, and fish were more tolerant than most other taxa. The gastropod Retimohnia sp. and octopus Benthoctopus sp. survived exposure to pH reductions that episodically reached -0.3 pH units. Ninety percent of abyssal zoarcids (Pachycara bulbiceps) survived exposure to pH changes reaching ca. -0.3 pH units during 30-42 day-long experiments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/14740816','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/14740816"><span>Milk pH as a function of <span class="hlt">CO</span><span class="hlt">2</span> concentration, temperature, and pressure in a heat <span class="hlt">exchanger</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ma, Y; Barbano, D M</p> <p>2003-12-01</p> <p>Raw skim milk, with or without added <span class="hlt">CO</span><span class="hlt">2</span>, was heated, held, and cooled in a small pilot-scale tubular heat <span class="hlt">exchanger</span> (372 ml/min). The experiment was replicated twice, and, for each replication, milk was first carbonated at 0 to 1 degree C to contain 0 (control), 600, 1200, 1800, and 2400 ppm added <span class="hlt">CO</span><span class="hlt">2</span> using a continuous carbonation unit. After storage at 0 to 1 degree C, portions of milk at each <span class="hlt">CO</span><span class="hlt">2</span> concentration were heated to 40, 56, 72, and 80 degrees C, held at the desired temperature for 30 s (except 80 degrees C, holding 20 s) and cooled to 0 to 1 degree C. At each temperature, five pressures were applied: 69, 138, 207, 276, and 345 kPa. Pressure was controlled with a needle valve at the heat <span class="hlt">exchanger</span> exit. Both the pressure gauge and pH probe were inline at the end of the holding section. Milk pH during heating depended on <span class="hlt">CO</span><span class="hlt">2</span> concentration, temperature, and pressure. During heating of milk without added <span class="hlt">CO</span><span class="hlt">2</span>, pH decreased linearly as a function of increasing temperature but was independent of pressure. In general, the pH of milk with added <span class="hlt">CO</span><span class="hlt">2</span> decreased with increasing <span class="hlt">CO</span><span class="hlt">2</span> concentration and pressure. For milk with added <span class="hlt">CO</span><span class="hlt">2</span>, at a fixed <span class="hlt">CO</span><span class="hlt">2</span> concentration, the effect of pressure on pH decrease was greater at a higher temperature. At a fixed temperature, the effect of pressure on pH decrease was greater for milk with a higher <span class="hlt">CO</span><span class="hlt">2</span> concentration. Thermal death of bacteria during pasteurization of milk without added <span class="hlt">CO</span><span class="hlt">2</span> is probably due not only to temperature but also to the decrease in pH that occurs during the process. Increasing milk <span class="hlt">CO</span><span class="hlt">2</span> concentration and pressure decreases the milk pH even further during heating and may further enhance the microbial killing power of pasteurization.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010TCry....4..227D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010TCry....4..227D"><span>Brief Communication: Ikaite (Ca<span class="hlt">CO</span>3·6H<span class="hlt">2</span>O) discovered in Arctic <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>Dieckmann, G. S.; Nehrke, G.; Uhlig, C.; Göttlicher, J.; Gerland, S.; Granskog, M. A.; Thomas, D. N.</p> <p>2010-05-01</p> <p>We report for the first time on the discovery of calcium carbonate crystals as ikaite (Ca<span class="hlt">CO</span>3·6H<span class="hlt">2</span>O) in <span class="hlt">sea</span> ice from the Arctic (Kongsfjorden, Svalbard) as confirmed by morphology and indirectly by X-ray diffraction as well as XANES spectroscopy of its amorophous decomposition product. This finding demonstrates that the precipitation of calcium carbonate during the freezing of <span class="hlt">sea</span> ice is not restricted to the Antarctic, where it was observed for the first time in 2008. This observation is an important step in the quest to quantify its impact on the <span class="hlt">sea</span> ice driven carbon cycle.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27291890','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27291890"><span>Cation <span class="hlt">Exchange</span> Strategy for the Encapsulation of a Photoactive <span class="hlt">CO</span>-Releasing Organometallic Molecule into Anionic Porous Frameworks.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Carmona, Francisco J; Rojas, Sara; Sánchez, Purificación; Jeremias, Hélia; Marques, Ana R; Romão, Carlos C; Choquesillo-Lazarte, Duane; Navarro, Jorge A R; Maldonado, Carmen R; Barea, Elisa</p> <p>2016-07-05</p> <p>The encapsulation of the photoactive, nontoxic, water-soluble, and <span class="hlt">air</span>-stable cationic CORM [Mn(tacn)(<span class="hlt">CO</span>)3]Br (tacn = 1,4,7-triazacyclononane) in different inorganic porous matrixes, namely, the metalorganic framework bio-MOF-1, (NH<span class="hlt">2</span>(CH3)<span class="hlt">2)2</span>[Zn8(adeninate)4(BPDC)6]·8DMF·11H<span class="hlt">2</span>O (BPDC = 4,4'-biphenyldicarboxylate), and the functionalized mesoporous silicas MCM-41-SO3H and SBA-15-SO3H, is achieved by a cation <span class="hlt">exchange</span> strategy. The <span class="hlt">CO</span> release from these loaded materials, under simulated physiological conditions, is triggered by visible light. The results show that the silica matrixes, which are unaltered under physiological conditions, slow the kinetics of <span class="hlt">CO</span> release, allowing a more controlled <span class="hlt">CO</span> supply. In contrast, bio-MOF-1 instability leads to the complete leaching of the CORM. Nevertheless, the degradation of the MOF matrix gives rise to an enhanced <span class="hlt">CO</span> release rate, which is related to the presence of free adenine in the solution.</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> flux 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> flux 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> fluxes 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://www.dtic.mil/docs/citations/ADA466972','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA466972"><span>Microphysics of <span class="hlt">Air-Sea</span> <span class="hlt">Exchanges</span></span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2006-06-30</p> <p>these variables: S- rMss g A <span class="hlt">co</span> Figure 3 shows the correlation between It and the measured F at 6cm depth: e = 9.3 x 10-5 (mssgA(o0) 75 The Imaging ...camera to directly observe the water surface slope through the relative intensities of the three color components at each point of the image . The ISG...law,no peraon shall be subject any penalty for fling to comply wit a collection of information if it do" n&T display a cur, eniy valid OMB control</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.B53A0471C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.B53A0471C"><span>The Seasonal and Diurnal Patterns of net Ecosystem <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">Exchange</span> in a Subtropical Montane Cloud Forest.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chu, H.; Lai, C.; Wu, C.; Hsia, Y.</p> <p>2008-12-01</p> <p> difference suggested that water droplets deposited on leaves might partially block the pathway of the gas <span class="hlt">exchange</span> through stomata as canopy immersed in the very humid <span class="hlt">air</span>. However, <span class="hlt">CO</span><span class="hlt">2</span> fluxes did not cease during foggy periods, as also supported by sap flow and leaf chamber measurements, the morphological characteristics of leaf or/and canopy structure might contribute to the well adaptability of this subtropical montane cloud forest to the humid environment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22823525','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22823525"><span>Concurrent separation of <span class="hlt">CO</span><span class="hlt">2</span> and H<span class="hlt">2</span>O from <span class="hlt">air</span> by a temperature-vacuum swing adsorption/desorption cycle.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wurzbacher, Jan Andre; Gebald, Christoph; Piatkowski, Nicolas; Steinfeld, Aldo</p> <p>2012-08-21</p> <p>A temperature-vacuum swing (TVS) cyclic process is applied to an amine-functionalized nanofibrilated cellulose sorbent to concurrently extract <span class="hlt">CO</span>(<span class="hlt">2</span>) and water vapor from ambient <span class="hlt">air</span>. The promoting effect of the relative humidity on the <span class="hlt">CO</span>(<span class="hlt">2</span>) capture capacity and on the amount of coadsorbed water is quantified. The measured specific <span class="hlt">CO</span>(<span class="hlt">2</span>) capacities range from 0.32 to 0.65 mmol/g, and the corresponding specific H(<span class="hlt">2</span>)O capacities range from 0.87 to 4.76 mmol/g for adsorption temperatures varying between 10 and 30 °C and relative humidities varying between 20 and 80%. Desorption of <span class="hlt">CO</span>(<span class="hlt">2</span>) is achieved at 95 °C and 50 mbar(abs) without dilution by a purge gas, yielding a purity exceeding 94.4%. Sorbent stability and a closed mass balance for both H(<span class="hlt">2</span>)O and <span class="hlt">CO</span>(<span class="hlt">2</span>) are demonstrated for ten consecutive adsorption-desorption cycles. The specific energy requirements of the TVS process based on the measured H(<span class="hlt">2</span>)O and <span class="hlt">CO</span>(<span class="hlt">2</span>) capacities are estimated to be 12.5 kJ/mol(<span class="hlt">CO</span><span class="hlt">2</span>) of mechanical (pumping) work and between 493 and 640 kJ/mol(<span class="hlt">CO</span><span class="hlt">2</span>) of heat at below 100 °C, depending on the <span class="hlt">air</span> relative humidity. For a targeted <span class="hlt">CO</span>(<span class="hlt">2</span>) capacity of <span class="hlt">2</span> mmol/g, the heat requirement would be reduced to between 272 and 530 kJ/mol(<span class="hlt">CO</span><span class="hlt">2</span>), depending strongly on the amount of coadsorbed water.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFMGC51C0985G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFMGC51C0985G"><span><span class="hlt">Co</span>-location of <span class="hlt">air</span> capture, sub-ocean <span class="hlt">CO</span><span class="hlt">2</span> storage and energy production on the Kerguelen plateau</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Goldberg, D.; Han, P.; Lackner, K.; Wang, T.</p> <p>2011-12-01</p> <p>How can carbon capture and storage activities be sustained from an energy perspective while keeping the entire activity out of sight and away from material risk and social refrain near populated areas? In light of reducing the atmospheric <span class="hlt">CO</span><span class="hlt">2</span> level to mitigate its effect on climate change, the combination of new <span class="hlt">air</span>-capture technologies and large offshore storage reservoirs, supplemented by carbon neutral renewable energy, could address both of these engineering and public policy concerns. Because <span class="hlt">CO</span><span class="hlt">2</span> mixes rapidly in the atmosphere, <span class="hlt">air</span> capture scrubbers could be located anywhere in the world. Although the power requirements for this technology may reduce net efficiencies, the local availability of carbon-neutral renewable energy for this purpose would eliminate some net energy loss. Certain locations where wind speeds are high and steady, such as those observed at high latitude and across the open ocean, appeal as carbon-neutral energy sources in close proximity to immense and secure reservoirs for geological sequestration of captured <span class="hlt">CO</span><span class="hlt">2</span>. In particular, sub-ocean basalt flows are vast and carry minimal risks of leakage and damages compared to on-land sites. Such implementation of a localized renewable energy source coupled with carbon capture and storage infrastructure could result in a global impact of lowered <span class="hlt">CO</span><span class="hlt">2</span> levels. We consider an extreme location on the Kerguelen plateau in the southern Indian Ocean, where high wind speeds and basalt storage reservoirs are both plentiful. Though endowed with these advantages, this mid-ocean location incurs clear material and economic challenges due to its remoteness and technological challenges for <span class="hlt">CO</span><span class="hlt">2</span> capture due to constant high humidity. We study the wind energy-<span class="hlt">air</span> capture power balance and consider related factors in the feasibility of this location for carbon capture and storage. Other remote oceanic sites where steady winds blow and near large geological reservoirs may be viable as well, although all would require</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRG..122.3174G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRG..122.3174G"><span>Mathematical Modelling of Arctic Polygonal Tundra with Ecosys: <span class="hlt">2</span>. Microtopography Determines How <span class="hlt">CO</span><span class="hlt">2</span> and CH4 <span class="hlt">Exchange</span> Responds to Changes in Temperature and Precipitation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Grant, R. F.; Mekonnen, Z. A.; Riley, W. J.; Arora, B.; Torn, M. S.</p> <p>2017-12-01</p> <p>Differences of surface elevation in arctic polygonal landforms cause spatial variation in soil water contents (θ), active layer depths (ALD), and thereby in <span class="hlt">CO</span><span class="hlt">2</span> and CH4 <span class="hlt">exchange</span>. Here we test hypotheses in ecosys for topographic controls on <span class="hlt">CO</span><span class="hlt">2</span> and CH4 <span class="hlt">exchange</span> in trough, rim, and center features of low- and flat-centered polygons (LCP and FCP) against chamber and eddy covariance (EC) measurements during 2013 at Barrow, Alaska. Larger <span class="hlt">CO</span><span class="hlt">2</span> influxes and CH4 effluxes were measured with chambers and modeled with ecosys in LCPs than in FCPs and in lower features (troughs) than in higher (rims) within LCPs and FCPs. Spatially aggregated <span class="hlt">CO</span><span class="hlt">2</span> and CH4 fluxes from ecosys were significantly correlated with EC flux measurements. Lower features were modeled as C sinks (52-56 g C m-<span class="hlt">2</span> yr-1) and CH4 sources (4-6 g C m-<span class="hlt">2</span> yr-1), and higher features as near C neutral (-<span class="hlt">2</span>-15 g C m-<span class="hlt">2</span> yr-1) and CH4 neutral (0.0-0.1 g C m-<span class="hlt">2</span> yr-1). Much of the spatial and temporal variations in <span class="hlt">CO</span><span class="hlt">2</span> and CH4 fluxes were modeled from topographic effects on water and snow movement and thereby on θ, ALD, and soil O<span class="hlt">2</span> concentrations. Model results forced with meteorological data from 1981 to 2015 indicated increasing net primary productivity in higher features and CH4 emissions in some lower and higher features since 2008, attributed mostly to recent rises in precipitation. Small-scale variation in surface elevation causes large spatial variation of greenhouse gas (GHG) <span class="hlt">exchanges</span> and therefore should be considered in estimates of GHG <span class="hlt">exchange</span> in polygonal landscapes.</p> </li> <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> flux 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 flux are not fully understood. The <span class="hlt">air-sea</span> flux 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 flux 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 flux 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> flux 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 flux are not fully understood. The <span class="hlt">air-sea</span> flux 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 flux 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 flux 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> flux 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 flux are not fully understood. The <span class="hlt">air-sea</span> flux 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 flux 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 flux variability.</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> <span class="hlt">exchange</span> of mercury (Hg) in the marine boundary layer of the Augusta basin (southern Italy): concentrations and evasion flux.</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 fluxes 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 flux 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/2017AGUFM.H42D..02O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.H42D..02O"><span>Modeling of Single and Dual Reservoir Porous Media Compressed Gas (<span class="hlt">Air</span> and <span class="hlt">CO</span><span class="hlt">2</span>) Storage Systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Oldenburg, C. M.; Liu, H.; Borgia, A.; Pan, L.</p> <p>2017-12-01</p> <p>Intermittent renewable energy sources are causing increasing demand for energy storage. The deep subsurface offers promising opportunities for energy storage because it can safely contain high-pressure gases. Porous media compressed <span class="hlt">air</span> energy storage (PM-CAES) is one approach, although the only facilities in operation are in caverns (C-CAES) rather than porous media. Just like in C-CAES, PM-CAES operates generally by injecting working gas (<span class="hlt">air</span>) through well(s) into the reservoir compressing the cushion gas (existing <span class="hlt">air</span> in the reservoir). During energy recovery, high-pressure <span class="hlt">air</span> from the reservoir is mixed with fuel in a combustion turbine to produce electricity, thereby reducing compression costs. Unlike in C-CAES, the storage of energy in PM-CAES occurs variably across pressure gradients in the formation, while the solid grains of the matrix can release/store heat. Because <span class="hlt">air</span> is the working gas, PM-CAES has fairly low thermal efficiency and low energy storage density. To improve the energy storage density, we have conceived and modeled a closed-loop two-reservoir compressed <span class="hlt">CO</span><span class="hlt">2</span> energy storage system. One reservoir is the low-pressure reservoir, and the other is the high-pressure reservoir. <span class="hlt">CO</span><span class="hlt">2</span> is cycled back and forth between reservoirs depending on whether energy needs to be stored or recovered. We have carried out thermodynamic and parametric analyses of the performance of an idealized two-reservoir <span class="hlt">CO</span><span class="hlt">2</span> energy storage system under supercritical and transcritical conditions for <span class="hlt">CO</span><span class="hlt">2</span> using a steady-state model. Results show that the transcritical compressed <span class="hlt">CO</span><span class="hlt">2</span> energy storage system has higher round-trip efficiency and exergy efficiency, and larger energy storage density than the supercritical compressed <span class="hlt">CO</span><span class="hlt">2</span> energy storage. However, the configuration of supercritical compressed <span class="hlt">CO</span><span class="hlt">2</span> energy storage is simpler, and the energy storage densities of the two systems are both higher than that of PM-CAES, which is advantageous in terms of storage volume for a given</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/2018NatCC...8..398L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018NatCC...8..398L"><span><span class="hlt">Air</span> quality <span class="hlt">co</span>-benefits of carbon pricing in China</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Mingwei; Zhang, Da; Li, Chiao-Ting; Mulvaney, Kathleen M.; Selin, Noelle E.; Karplus, Valerie J.</p> <p>2018-05-01</p> <p>Climate policies targeting energy-related <span class="hlt">CO</span><span class="hlt">2</span> emissions, which act on a global scale over long time horizons, can result in localized, near-term reductions in both <span class="hlt">air</span> pollution and adverse human health impacts. Focusing on China, the largest energy-using and <span class="hlt">CO</span><span class="hlt">2</span>-emitting nation, we develop a cross-scale modelling approach to quantify these <span class="hlt">air</span> quality <span class="hlt">co</span>-benefits, and compare them to the economic costs of climate policy. We simulate the effects of an illustrative climate policy, a price on <span class="hlt">CO</span><span class="hlt">2</span> emissions. In a policy scenario consistent with China's recent pledge to reach a peak in <span class="hlt">CO</span><span class="hlt">2</span> emissions by 2030, we project that national health <span class="hlt">co</span>-benefits from improved <span class="hlt">air</span> quality would partially or fully offset policy costs depending on chosen health valuation. Net health <span class="hlt">co</span>-benefits are found to rise with increasing policy stringency.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4730140','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4730140"><span>Interactions and <span class="hlt">exchange</span> of <span class="hlt">CO</span><span class="hlt">2</span> and H<span class="hlt">2</span>O in coals: an investigation by low-field NMR relaxation</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Sun, Xiaoxiao; Yao, Yanbin; Liu, Dameng; Elsworth, Derek; Pan, Zhejun</p> <p>2016-01-01</p> <p>The mechanisms by which <span class="hlt">CO</span><span class="hlt">2</span> and water interact in coal remain unclear and these are key questions for understanding ECBM processes and defining the long-term behaviour of injected <span class="hlt">CO</span><span class="hlt">2</span>. In our experiments, we injected helium/<span class="hlt">CO</span><span class="hlt">2</span> to displace water in eight water-saturated samples. We used low-field NMR relaxation to investigate <span class="hlt">CO</span><span class="hlt">2</span> and water interactions in these coals across a variety of time-scales. The injection of helium did not change the T<span class="hlt">2</span> spectra of the coals. In contrast, the T<span class="hlt">2</span> spectra peaks of micro-capillary water gradually decreased and those of macro-capillary and bulk water increased with time after the injection of <span class="hlt">CO</span><span class="hlt">2</span>. We assume that the <span class="hlt">CO</span><span class="hlt">2</span> diffuses through and/or dissolves into the capillary water to access the coal matrix interior, which promotes desorption of water molecules from the surfaces of coal micropores and mesopores. The replaced water mass is mainly related to the Langmuir adsorption volume of <span class="hlt">CO</span><span class="hlt">2</span> and increases as the <span class="hlt">CO</span><span class="hlt">2</span> adsorption capacity increases. Other factors, such as mineral composition, temperature and pressure, also influence the effective <span class="hlt">exchange</span> between water and <span class="hlt">CO</span><span class="hlt">2</span>. Finally, we built a quantified model to evaluate the efficiency of water replacement by <span class="hlt">CO</span><span class="hlt">2</span> injection with respect to temperature and pressure. PMID:26817784</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26608560','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26608560"><span>The impact of elevated <span class="hlt">CO</span><span class="hlt">2</span> and temperature on grain quality of rice grown under open-<span class="hlt">air</span> field conditions.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Jing, Liquan; Wang, Juan; Shen, Shibo; Wang, Yunxia; Zhu, Jianguo; Wang, Yulong; Yang, Lianxin</p> <p>2016-08-01</p> <p>Rising atmospheric <span class="hlt">CO</span><span class="hlt">2</span> is accompanied by global warming. However, interactive effects of elevated <span class="hlt">CO</span><span class="hlt">2</span> and temperature have not been well studied on grain quality of rice. A japonica cultivar was grown in the field using a free-<span class="hlt">air</span> <span class="hlt">CO</span><span class="hlt">2</span> enrichment facility in combination with a canopy <span class="hlt">air</span> temperature increase system in 2014. The gas fumigation (200 µmol mol(-1) above ambient <span class="hlt">CO</span><span class="hlt">2</span> ) and temperature increase (1 °C above ambient <span class="hlt">air</span> temperature) were performed from tillering until maturity. Compared with the control (ambient <span class="hlt">CO</span><span class="hlt">2</span> and <span class="hlt">air</span> temperature), elevated <span class="hlt">CO</span><span class="hlt">2</span> increased grain length and width as well as grain chalkiness but decreased protein concentrations. In contrast, the increase in canopy <span class="hlt">air</span> temperature had less effect on these parameters except for grain chalkiness. The starch pasting properties of rice flour and taste analysis of cooked rice indicated that the palatability of rice was improved by <span class="hlt">CO</span><span class="hlt">2</span> and/or temperature elevation, with the combination of the two treatments showing the most significant changes compared with ambient rice. It is concluded that projected <span class="hlt">CO</span><span class="hlt">2</span> in 2050 may have larger effects on rice grain quality than the projected temperature increase. Although deterioration in milling suitability, grain appearance and nutritional quality can be expected, the taste of cooked rice might be better in the future environment. © 2015 Society of Chemical Industry. © 2015 Society of Chemical Industry.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4707055','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4707055"><span><span class="hlt">CO</span><span class="hlt">2</span> sensing and <span class="hlt">CO</span><span class="hlt">2</span> regulation of stomatal conductance: advances and open questions</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Engineer, Cawas; Hashimoto-Sugimoto, Mimi; Negi, Juntaro; Israelsson-Nordstrom, Maria; Azoulay-Shemer, Tamar; Rappel, Wouter-Jan; Iba, Koh; Schroeder, Julian</p> <p>2015-01-01</p> <p>Guard cells form epidermal stomatal gas <span class="hlt">exchange</span> valves in plants and regulate the aperture of stomatal pores in response to changes in the carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) concentration in leaves. Moreover, the development of stomata is repressed by elevated <span class="hlt">CO</span><span class="hlt">2</span> in diverse plant species. Evidence suggests that plants can sense <span class="hlt">CO</span><span class="hlt">2</span> concentration changes via guard cells and via mesophyll tissues in mediating stomatal movements. We review new discoveries and open questions on mechanisms mediating <span class="hlt">CO</span><span class="hlt">2</span>-regulated stomatal movements and <span class="hlt">CO</span><span class="hlt">2</span> modulation of stomatal development, which together function in <span class="hlt">CO</span><span class="hlt">2</span>-regulation of stomatal conductance and gas <span class="hlt">exchange</span> in plants. Research in this area is timely in light of the necessity of selecting and developing crop cultivars which perform better in a shifting climate. PMID:26482956</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> Fluxes 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> flux into the Southern Ocean is difficult to measure and model because it results from large opposing and seasonally-varying fluxes 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> <span class="hlt">exchange</span> 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 fluxes 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 flux 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> fluxes for the Southern Ocean, in contrast to those derived from the extrapolation of sparse ocean and atmospheric measurements and uncertain flux parameterizations.</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 flux 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.ncbi.nlm.nih.gov/pubmed/23921896','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23921896"><span>Comparison of <span class="hlt">CO</span><span class="hlt">2</span> in <span class="hlt">air</span> versus carbogen for the measurement of cerebrovascular reactivity with magnetic resonance imaging.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hare, Hannah V; Germuska, Michael; Kelly, Michael E; Bulte, Daniel P</p> <p>2013-11-01</p> <p>Measurement of cerebrovascular reactivity (CVR) can give valuable information about existing pathology and the risk of adverse events, such as stroke. A common method of obtaining regional CVR values is by measuring the blood flow response to carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>)-enriched <span class="hlt">air</span> using arterial spin labeling (ASL) or blood oxygen level-dependent (BOLD) imaging. Recently, several studies have used carbogen gas (containing only <span class="hlt">CO</span><span class="hlt">2</span> and oxygen) as an alternative stimulus. A direct comparison was performed between CVR values acquired by ASL and BOLD imaging using stimuli of (1) 5% <span class="hlt">CO</span><span class="hlt">2</span> in <span class="hlt">air</span> and (<span class="hlt">2</span>) 5% <span class="hlt">CO</span><span class="hlt">2</span> in oxygen (carbogen-5). Although BOLD and ASL CVR values are shown to be correlated for <span class="hlt">CO</span><span class="hlt">2</span> in <span class="hlt">air</span> (mean response 0.11±0.03% BOLD, 4.46±1.80% ASL, n=16 hemispheres), this correlation disappears during a carbogen stimulus (0.36±0.06% BOLD, 4.97±1.30% ASL). It is concluded that BOLD imaging should generally not be used in conjunction with a carbogen stimulus when measuring CVR, and that care must be taken when interpreting CVR as measured by ASL, as values obtained from different stimuli (<span class="hlt">CO</span><span class="hlt">2</span> in <span class="hlt">air</span> versus carbogen) are not directly comparable.</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 fluxes 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. Fluxes 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 fluxes 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> fluxes 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> <span class="hlt">exchange</span> and other carbon fluxes 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 fluxes. The presentation will illustrate that despite significant advances in capabilities and understanding, large uncertainties remain.</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> fluxes 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> fluxes 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/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> flux 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 flux 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('https://www.osti.gov/biblio/6295083-use-free-air-co-sub-enrichment-face-study-effects-co-sub-cotton-preliminary-summary-report','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6295083-use-free-air-co-sub-enrichment-face-study-effects-co-sub-cotton-preliminary-summary-report"><span>Use of Free <span class="hlt">Air</span> <span class="hlt">CO</span>/sub <span class="hlt">2</span>/ Enrichment (FACE) to study effects of <span class="hlt">CO</span>/sub <span class="hlt">2</span>/ on cotton: Preliminary summary report -- 1988</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>Biswas, P.K.; Hileman, D.R.; Bhattacharya, N.C.</p> <p>1988-01-01</p> <p>In the summer of 1988, Tuskegee University, along with Brookhaven National Laboratory, Manhattan College, and USDA laboratories in Tallahassee, FL and Phoenix, AZ, participated in joint program to evaluate the feasibility of using a Free <span class="hlt">Air</span> <span class="hlt">CO</span>/sub <span class="hlt">2</span>/ Enrichment (FACE) system to conduct experiments on the effects of elevated <span class="hlt">CO</span>/sub <span class="hlt">2</span>/ on cotton. The experiments were conducted in Yazoo City, MS, under the direction of the US Department of Energy, Carbon Dioxide Research Division. Tuskegee University's role in the project included the following objectives: (1)Soil moisture and nutrient analysis before planting and at harvest. (<span class="hlt">2</span>) Photosynthesis and stomatal conductance measurementsmore » at ambient and enriched <span class="hlt">CO</span>/sub <span class="hlt">2</span>/ atmosphere. (3) Leaf water potential measurements. (4) <span class="hlt">CO</span>/sub <span class="hlt">2</span>/ distribution patterns in the FACE array. 12 figs., 14 tabs.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19343739','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19343739"><span>A system for high-quality <span class="hlt">CO</span><span class="hlt">2</span> isotope analyses of <span class="hlt">air</span> samples collected by the CARIBIC Airbus A340-600.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Assonov, S; Taylor, P; Brenninkmeijer, C A M</p> <p>2009-05-01</p> <p>In 2007, JRC-IRMM began a series of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> isotope measurements, with the focus on understanding instrumental effects, corrections as well as metrological aspects. The calibration approach at JRC-IRMM is based on use of a plain <span class="hlt">CO</span><span class="hlt">2</span> sample (working reference <span class="hlt">CO</span><span class="hlt">2</span>) as a calibration carrier and <span class="hlt">CO</span><span class="hlt">2</span>-<span class="hlt">air</span> mixtures (in high-pressure cylinders) to determine the method-related correction under actual analytical conditions (another calibration carrier, in the same form as the samples). Although this approach differs from that in other laboratories, it does give a direct link to the primary reference NBS-19-<span class="hlt">CO</span><span class="hlt">2</span>. It also helps to investigate the magnitude and nature for each of the instrumental corrections and allows for the quantification of the uncertainty introduced. Critical tests were focused on the instrumental corrections. It was confirmed that the use of non-symmetrical capillary crimping (an approach used here to deal with small samples) systematically modifies delta13C(<span class="hlt">CO</span><span class="hlt">2</span>) and delta18O(<span class="hlt">CO</span><span class="hlt">2</span>), with a clear dependence on the amount of extracted <span class="hlt">CO</span><span class="hlt">2</span>. However, the calibration of <span class="hlt">CO</span><span class="hlt">2</span>-<span class="hlt">air</span> mixtures required the use of the symmetrical dual-inlet mode. As a proof of our approach, we found that delta13C(<span class="hlt">CO</span><span class="hlt">2</span>) on extracts from mixtures agreed (within 0.010 per thousand) with values obtained from the 'mother' <span class="hlt">CO</span><span class="hlt">2</span> used for the mixtures. It was further found that very low levels of hydrocarbons in the pumping systems and the isotope ratio mass spectrometry (IRMS) instrument itself were critical. The m/z 46 values (consequently the calculated delta18O(<span class="hlt">CO</span><span class="hlt">2</span>) values) are affected by several other effects with traces of <span class="hlt">air</span> <span class="hlt">co</span>-trapped with frozen <span class="hlt">CO</span><span class="hlt">2</span> being the most critical. A careful cryo-distillation of the extracted <span class="hlt">CO</span><span class="hlt">2</span> is recommended. After extensive testing, optimisation, and routine automated use, the system was found to give precise data on <span class="hlt">air</span> samples that can be traced with confidence to the primary standards. The typical total combined uncertainty in delta13C(<span class="hlt">CO</span><span class="hlt">2</span>) and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28447675','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28447675"><span>Back-<span class="hlt">exchange</span>: a novel approach to quantifying oxygen diffusion and surface <span class="hlt">exchange</span> in ambient atmospheres.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Cooper, Samuel J; Niania, Mathew; Hoffmann, Franca; Kilner, John A</p> <p>2017-05-17</p> <p>A novel two-step Isotopic <span class="hlt">Exchange</span> (IE) technique has been developed to investigate the influence of oxygen containing components of ambient <span class="hlt">air</span> (such as H <span class="hlt">2</span> O and <span class="hlt">CO</span> <span class="hlt">2</span> ) on the effective surface <span class="hlt">exchange</span> coefficient (k*) of a common mixed ionic electronic conductor material. The two step 'back-<span class="hlt">exchange</span>' technique was used to introduce a tracer diffusion profile, which was subsequently measured using Time-of-Flight Secondary Ion Mass Spectrometry (ToF-SIMS). The isotopic fraction of oxygen in a dense sample as a function of distance from the surface, before and after the second <span class="hlt">exchange</span> step, could then be used to determine the surface <span class="hlt">exchange</span> coefficient in each atmosphere. A new analytical solution was found to the diffusion equation in a semi-infinite domain with a variable surface <span class="hlt">exchange</span> boundary, for the special case where D* and k* are constant for all <span class="hlt">exchange</span> steps. This solution validated the results of a numerical, Crank-Nicolson type finite-difference simulation, which was used to extract the parameters from the experimental data. When modelling electrodes, D* and k* are important input parameters, which significantly impact performance. In this study La 0.6 Sr 0.4 <span class="hlt">Co</span> 0.<span class="hlt">2</span> Fe 0.8 O 3-δ (LSCF6428) was investigated and it was found that the rate of <span class="hlt">exchange</span> was increased by around 250% in ambient <span class="hlt">air</span> compared to high purity oxygen at the same pO <span class="hlt">2</span> . The three experiments performed in this study were used to validate the back-<span class="hlt">exchange</span> approach and show its utility.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26391334','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26391334"><span>A dynamic leaf gas-<span class="hlt">exchange</span> strategy is conserved in woody plants under changing ambient <span class="hlt">CO</span><span class="hlt">2</span> : evidence from carbon isotope discrimination in paleo and <span class="hlt">CO</span><span class="hlt">2</span> enrichment studies.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Voelker, Steven L; Brooks, J Renée; Meinzer, Frederick C; Anderson, Rebecca; Bader, Martin K-F; Battipaglia, Giovanna; Becklin, Katie M; Beerling, David; Bert, Didier; Betancourt, Julio L; Dawson, Todd E; Domec, Jean-Christophe; Guyette, Richard P; Körner, Christian; Leavitt, Steven W; Linder, Sune; Marshall, John D; Mildner, Manuel; Ogée, Jérôme; Panyushkina, Irina; Plumpton, Heather J; Pregitzer, Kurt S; Saurer, Matthias; Smith, Andrew R; Siegwolf, Rolf T W; Stambaugh, Michael C; Talhelm, Alan F; Tardif, Jacques C; Van de Water, Peter K; Ward, Joy K; Wingate, Lisa</p> <p>2016-02-01</p> <p>Rising atmospheric [<span class="hlt">CO</span><span class="hlt">2</span> ], ca , is expected to affect stomatal regulation of leaf gas-<span class="hlt">exchange</span> of woody plants, thus influencing energy fluxes as well as carbon (C), water, and nutrient cycling of forests. Researchers have proposed various strategies for stomatal regulation of leaf gas-<span class="hlt">exchange</span> that include maintaining a constant leaf internal [<span class="hlt">CO</span><span class="hlt">2</span> ], ci , a constant drawdown in <span class="hlt">CO</span><span class="hlt">2</span> (ca  - ci ), and a constant ci /ca . These strategies can result in drastically different consequences for leaf gas-<span class="hlt">exchange</span>. The accuracy of Earth systems models depends in part on assumptions about generalizable patterns in leaf gas-<span class="hlt">exchange</span> responses to varying ca . The concept of optimal stomatal behavior, exemplified by woody plants shifting along a continuum of these strategies, provides a unifying framework for understanding leaf gas-<span class="hlt">exchange</span> responses to ca . To assess leaf gas-<span class="hlt">exchange</span> regulation strategies, we analyzed patterns in ci inferred from studies reporting C stable isotope ratios (δ(13) C) or photosynthetic discrimination (∆) in woody angiosperms and gymnosperms that grew across a range of ca spanning at least 100 ppm. Our results suggest that much of the ca -induced changes in ci /ca occurred across ca spanning 200 to 400 ppm. These patterns imply that ca  - ci will eventually approach a constant level at high ca because assimilation rates will reach a maximum and stomatal conductance of each species should be constrained to some minimum level. These analyses are not consistent with canalization toward any single strategy, particularly maintaining a constant ci . Rather, the results are consistent with the existence of a broadly conserved pattern of stomatal optimization in woody angiosperms and gymnosperms. This results in trees being profligate water users at low ca , when additional water loss is small for each unit of C gain, and increasingly water-conservative at high ca , when photosystems are saturated and water loss is large for each unit C gain. </p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70178114','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70178114"><span>A dynamic leaf gas-<span class="hlt">exchange</span> strategy is conserved in woody plants under changing ambient <span class="hlt">CO</span><span class="hlt">2</span>: evidence from carbon isotope discrimination in paleo and <span class="hlt">CO</span><span class="hlt">2</span> enrichment studies</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Voelker, Steven L.; Brooks, J. Renée; Meinzer, Frederick C.; Anderson, Rebecca D.; Bader, Martin K.-F.; Battipaglia, Giovanna; Becklin, Katie M.; Beerling, David; Bert, Didier; Betancourt, Julio L.; Dawson, Todd E.; Domec, Jean-Christophe; Guyette, Richard P.; Körner, Christian; Leavitt, Steven W.; Linder, Sune; Marshall, John D.; Mildner, Manuel; Ogée, Jérôme; Panyushkina, Irina P.; Plumpton, Heather J.; Pregitzer, Kurt S.; Saurer, Matthias; Smith, Andrew R.; Siegwolf, Rolf T.W.; Stambaugh, Michael C.; Talhelm, Alan F.; Tardif, Jacques C.; Van De Water, Peter K.; Ward, Joy K.; Wingate, Lisa</p> <p>2016-01-01</p> <p>Rising atmospheric [<span class="hlt">CO</span><span class="hlt">2</span>], ca, is expected to affect stomatal regulation of leaf gas-<span class="hlt">exchange</span> of woody plants, thus influencing energy fluxes as well as carbon (C), water, and nutrient cycling of forests. Researchers have proposed various strategies for stomatal regulation of leaf gas-<span class="hlt">exchange</span> that include maintaining a constant leaf internal [<span class="hlt">CO</span><span class="hlt">2</span>], ci, a constant drawdown in <span class="hlt">CO</span><span class="hlt">2</span>(ca − ci), and a constant ci/ca. These strategies can result in drastically different consequences for leaf gas-<span class="hlt">exchange</span>. The accuracy of Earth systems models depends in part on assumptions about generalizable patterns in leaf gas-<span class="hlt">exchange</span> responses to varying ca. The concept of optimal stomatal behavior, exemplified by woody plants shifting along a continuum of these strategies, provides a unifying framework for understanding leaf gas-<span class="hlt">exchange</span> responses to ca. To assess leaf gas-<span class="hlt">exchange</span> regulation strategies, we analyzed patterns in ci inferred from studies reporting C stable isotope ratios (δ13C) or photosynthetic discrimination (∆) in woody angiosperms and gymnosperms that grew across a range of ca spanning at least 100 ppm. Our results suggest that much of the ca-induced changes in ci/ca occurred across ca spanning 200 to 400 ppm. These patterns imply that ca − ci will eventually approach a constant level at high ca because assimilation rates will reach a maximum and stomatal conductance of each species should be constrained to some minimum level. These analyses are not consistent with canalization toward any single strategy, particularly maintaining a constant ci. Rather, the results are consistent with the existence of a broadly conserved pattern of stomatal optimization in woody angiosperms and gymnosperms. This results in trees being profligate water users at low ca, when additional water loss is small for each unit of C gain, and increasingly water-conservative at high ca, when photosystems are saturated and water loss is large for each unit C gain.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017APS..DFDF32010S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..DFDF32010S"><span>Modeling and optimal design of <span class="hlt">CO</span><span class="hlt">2</span> Direct <span class="hlt">Air</span> Capture systems in large arrays</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sadri Irani, Samaneh; Luzzatto-Fegiz, Paolo</p> <p>2017-11-01</p> <p>As noted by the 2014 IPCC report, while the rise in atmospheric <span class="hlt">CO</span><span class="hlt">2</span> would be slowed by emissions reductions, removing atmospheric <span class="hlt">CO</span><span class="hlt">2</span> is an important part of possible paths to climate stabilization. Direct <span class="hlt">Air</span> Capture of <span class="hlt">CO</span><span class="hlt">2</span> with chemicals (DAC) is one of several proposed carbon capture technologies. There is an ongoing debate on whether DAC is an economically viable approach to alleviate climate change. In addition, like all <span class="hlt">air</span> capture strategies, DAC is strongly constrained by the net-carbon problem, namely the need to control <span class="hlt">CO</span><span class="hlt">2</span> emissions associated with the capture process (for example, if DAC not powered by renewables). Research to date has focused on the chemistry and economics of individual DAC devices. However, the fluid mechanics of their large-scale deployment has not been examined in the literature, to the best of our knowledge. In this presentation, we develop a model for flow through an array of DAC devices, varying their lateral extent and their separation. We build on a recent theory of canopy flows, introducing terms for <span class="hlt">CO</span><span class="hlt">2</span> entrainment into the array boundary layer, and transport into the farm. In addition, we examine the possibility of driving flow passively by wind, thereby reducing energy consumption. The optimal operational design is established considering the total cost, drag force, energy consumption and total <span class="hlt">CO</span><span class="hlt">2</span> capture.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25181008','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25181008"><span>External <span class="hlt">CO</span><span class="hlt">2</span> and water supplies for enhancing electrical power generation of <span class="hlt">air</span>-cathode microbial fuel cells.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ishizaki, So; Fujiki, Itto; Sano, Daisuke; Okabe, Satoshi</p> <p>2014-10-07</p> <p>Alkalization on the cathode electrode limits the electrical power generation of <span class="hlt">air</span>-cathode microbial fuel cells (MFCs), and thus external proton supply to the cathode electrode is essential to enhance the electrical power generation. In this study, the effects of external <span class="hlt">CO</span><span class="hlt">2</span> and water supplies to the cathode electrode on the electrical power generation were investigated, and then the relative contributions of <span class="hlt">CO</span><span class="hlt">2</span> and water supplies to the total proton consumption were experimentally evaluated. The <span class="hlt">CO</span><span class="hlt">2</span> supply decreased the cathode pH and consequently increased the power generation. Carbonate dissolution was the main proton source under ambient <span class="hlt">air</span> conditions, which provides about 67% of total protons consumed for the cathode reaction. It is also critical to adequately control the water content on the cathode electrode of <span class="hlt">air</span>-cathode MFCs because the carbonate dissolution was highly dependent on water content. On the basis of these experimental results, the power density was increased by 400% (143.0 ± 3.5 mW/m(<span class="hlt">2</span>) to 575.0 ± 36.0 mW/m(<span class="hlt">2</span>)) by supplying a humid gas containing 50% <span class="hlt">CO</span><span class="hlt">2</span> to the cathode chamber. This study demonstrates that the simultaneous <span class="hlt">CO</span><span class="hlt">2</span> and water supplies to the cathode electrode were effective to increase the electrical power generation of <span class="hlt">air</span>-cathode MFCs for the first time.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018Cryo...91..128W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018Cryo...91..128W"><span>Experimental study on <span class="hlt">CO</span><span class="hlt">2</span> frosting and clogging in a brazed plate heat <span class="hlt">exchanger</span> for natural gas liquefaction process</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wu, Jitan; He, Tianbiao; Ju, Yonglin</p> <p>2018-04-01</p> <p>The plate-fin heat <span class="hlt">exchanger</span> (PFHE), which has been widely used in natural gas liquefaction (LNG) industry at present, has some disadvantages such as being sensitive to the impurities in the feed gas, such as water, <span class="hlt">CO</span><span class="hlt">2</span> and H<span class="hlt">2</span>S. Compared with the PFHE, the brazed plate heat <span class="hlt">exchanger</span> (BPHE), which has been applied in some boil off gas (BOG) recycling LNG plants of small to middle size, has simpler inherent structure and higher impurity tolerance. In this study the BPHE is suggested to replace the PFHE to simplify or even omit the massive <span class="hlt">CO</span><span class="hlt">2</span> purification equipment for the LNG process. A set of experimental apparatus is designed and constructed to investigate the influence of the <span class="hlt">CO</span><span class="hlt">2</span> concentration of the natural gas on solid precipitation inside a typical BPHE meanly by considering the flow resistance throughout the LNG process. The results show that the maximum allowable <span class="hlt">CO</span><span class="hlt">2</span> concentration of the natural gas liquefied in the BPHE is two orders of magnitude higher than that in the PFHE under the same condition. In addition, the solid-liquid separation for the <span class="hlt">CO</span><span class="hlt">2</span> impurity is studied and the reasonable separating temperature is obtained. The solid <span class="hlt">CO</span><span class="hlt">2</span> should be separated below 135 K under the pressure of 3 MPa.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1433102-mathematical-modelling-arctic-polygonal-tundra-ecosys-microtopography-determines-how-co2-ch4-exchange-responds-changes-temperature-precipitation','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1433102-mathematical-modelling-arctic-polygonal-tundra-ecosys-microtopography-determines-how-co2-ch4-exchange-responds-changes-temperature-precipitation"><span>Mathematical Modelling of Arctic Polygonal Tundra with Ecosys: <span class="hlt">2</span>. Microtopography Determines How <span class="hlt">CO</span> <span class="hlt">2</span> and CH 4 <span class="hlt">Exchange</span> Responds to Changes in Temperature and Precipitation</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>Grant, R. F.; Mekonnen, Z. A.; Riley, W. J.</p> <p></p> <p>Differences of surface elevation in arctic polygonal landforms cause spatial variation in soil water contents (θ), active layer depths (ALD), and thereby in <span class="hlt">CO</span> <span class="hlt">2</span> and CH 4 <span class="hlt">exchange</span>. In this paper, we test hypotheses in ecosys for topographic controls on <span class="hlt">CO</span> <span class="hlt">2</span> and CH 4 <span class="hlt">exchange</span> in trough, rim, and center features of low- and flat-centered polygons (LCP and FCP) against chamber and eddy covariance (EC) measurements during 2013 at Barrow, Alaska. Larger <span class="hlt">CO</span> <span class="hlt">2</span> influxes and CH 4 effluxes were measured with chambers and modeled with ecosys in LCPs than in FCPs and in lower features (troughs) thanmore » in higher (rims) within LCPs and FCPs. Spatially aggregated <span class="hlt">CO</span> <span class="hlt">2</span> and CH 4 fluxes from ecosys were significantly correlated with EC flux measurements. Lower features were modeled as C sinks (52–56 g C m -<span class="hlt">2</span> yr -1) and CH 4 sources (4–6 g C m -<span class="hlt">2</span> yr -1), and higher features as near C neutral (-<span class="hlt">2</span>–15 g C m -<span class="hlt">2</span> yr -1) and CH 4 neutral (0.0–0.1 g C m -<span class="hlt">2</span> yr -1). Much of the spatial and temporal variations in <span class="hlt">CO</span> <span class="hlt">2</span> and CH 4 fluxes were modeled from topographic effects on water and snow movement and thereby on θ, ALD, and soil O <span class="hlt">2</span> concentrations. Model results forced with meteorological data from 1981 to 2015 indicated increasing net primary productivity in higher features and CH 4 emissions in some lower and higher features since 2008, attributed mostly to recent rises in precipitation. Finally, small-scale variation in surface elevation causes large spatial variation of greenhouse gas (GHG) <span class="hlt">exchanges</span> and therefore should be considered in estimates of GHG <span class="hlt">exchange</span> in polygonal landscapes.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1433102-mathematical-modelling-arctic-polygonal-tundra-ecosys-microtopography-determines-how-co2-ch4-exchange-responds-changes-temperature-precipitation','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1433102-mathematical-modelling-arctic-polygonal-tundra-ecosys-microtopography-determines-how-co2-ch4-exchange-responds-changes-temperature-precipitation"><span>Mathematical Modelling of Arctic Polygonal Tundra with Ecosys: <span class="hlt">2</span>. Microtopography Determines How <span class="hlt">CO</span> <span class="hlt">2</span> and CH 4 <span class="hlt">Exchange</span> Responds to Changes in Temperature and Precipitation</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Grant, R. F.; Mekonnen, Z. A.; Riley, W. J.; ...</p> <p>2017-11-17</p> <p>Differences of surface elevation in arctic polygonal landforms cause spatial variation in soil water contents (θ), active layer depths (ALD), and thereby in <span class="hlt">CO</span> <span class="hlt">2</span> and CH 4 <span class="hlt">exchange</span>. In this paper, we test hypotheses in ecosys for topographic controls on <span class="hlt">CO</span> <span class="hlt">2</span> and CH 4 <span class="hlt">exchange</span> in trough, rim, and center features of low- and flat-centered polygons (LCP and FCP) against chamber and eddy covariance (EC) measurements during 2013 at Barrow, Alaska. Larger <span class="hlt">CO</span> <span class="hlt">2</span> influxes and CH 4 effluxes were measured with chambers and modeled with ecosys in LCPs than in FCPs and in lower features (troughs) thanmore » in higher (rims) within LCPs and FCPs. Spatially aggregated <span class="hlt">CO</span> <span class="hlt">2</span> and CH 4 fluxes from ecosys were significantly correlated with EC flux measurements. Lower features were modeled as C sinks (52–56 g C m -<span class="hlt">2</span> yr -1) and CH 4 sources (4–6 g C m -<span class="hlt">2</span> yr -1), and higher features as near C neutral (-<span class="hlt">2</span>–15 g C m -<span class="hlt">2</span> yr -1) and CH 4 neutral (0.0–0.1 g C m -<span class="hlt">2</span> yr -1). Much of the spatial and temporal variations in <span class="hlt">CO</span> <span class="hlt">2</span> and CH 4 fluxes were modeled from topographic effects on water and snow movement and thereby on θ, ALD, and soil O <span class="hlt">2</span> concentrations. Model results forced with meteorological data from 1981 to 2015 indicated increasing net primary productivity in higher features and CH 4 emissions in some lower and higher features since 2008, attributed mostly to recent rises in precipitation. Finally, small-scale variation in surface elevation causes large spatial variation of greenhouse gas (GHG) <span class="hlt">exchanges</span> and therefore should be considered in estimates of GHG <span class="hlt">exchange</span> in polygonal landscapes.« 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 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/2014AGUFMGC21J..06H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMGC21J..06H"><span>Direct <span class="hlt">Air</span> Capture of <span class="hlt">CO</span><span class="hlt">2</span> - an Overview of Carbon Engineering's Technology and Pilot Plant Development</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Holmes, G.; Corless, A.</p> <p>2014-12-01</p> <p>At Carbon Engineering, we are developing and commercializing technology to scrub <span class="hlt">CO</span><span class="hlt">2</span> directly from atmospheric <span class="hlt">air</span> at industrial scale. By providing atmospheric <span class="hlt">CO</span><span class="hlt">2</span> for use in fuel production, we can enable production of transportation fuels with ultra-low carbon intensities, which command price premiums in the growing set of constrained fuels markets such as California's LCFS. We are a Calgary based startup founded in 2009 with 10 employees, and we are considered a global leader in the direct <span class="hlt">air</span> capture (DAC) field. We will review CE's DAC technology, based on a wet-scrubbing "<span class="hlt">air</span> contactor" which absorbs <span class="hlt">CO</span><span class="hlt">2</span> into aqueous solution, and a chemical looping "regeneration" component, which liberates pure <span class="hlt">CO</span><span class="hlt">2</span> from this aqueous solution while re-making the original absorption chemical. CE's DAC tecnology exports purified atmospheric <span class="hlt">CO</span><span class="hlt">2</span>, combined with the combustion <span class="hlt">CO</span><span class="hlt">2</span> from plant energy usage, as the end product. We will also discuss CE's 2014-2015 end-to-end Pilot Demonstration Unit. This is a $7M technology demonstration plant that CE is building with the help of key industrial partners and equipment vendors. Vendor design and engineering requirements have been used to specify the pilot <span class="hlt">air</span> contactor, pellet reactor, calciner, and slaker modules, as well as auxiliary systems. These modules will be run for several months to obtain the engineering and performance data needed for subsequent commercial plant design, as well as to test the residual integration risks associated with CE's process. By the time of the AGU conference, the pilot is expected to be in late stages of fabrication or early stages of site installation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24843913','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24843913"><span>Toward verifying fossil fuel <span class="hlt">CO</span><span class="hlt">2</span> emissions with the CMAQ model: motivation, model description and initial simulation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Liu, Zhen; Bambha, Ray P; Pinto, Joseph P; Zeng, Tao; Boylan, Jim; Huang, Maoyi; Lei, Huimin; Zhao, Chun; Liu, Shishi; Mao, Jiafu; Schwalm, Christopher R; Shi, Xiaoying; Wei, Yaxing; Michelsen, Hope A</p> <p>2014-04-01</p> <p>Motivated by the question of whether and how a state-of-the-art regional chemical transport model (CTM) can facilitate characterization of <span class="hlt">CO</span><span class="hlt">2</span> spatiotemporal variability and verify <span class="hlt">CO</span><span class="hlt">2</span> fossil-fuel emissions, we for the first time applied the Community Multiscale <span class="hlt">Air</span> Quality (CMAQ) model to simulate <span class="hlt">CO</span><span class="hlt">2</span>. This paper presents methods, input data, and initial results for <span class="hlt">CO</span><span class="hlt">2</span> simulation using CMAQ over the contiguous United States in October 2007. Modeling experiments have been performed to understand the roles of fossil-fuel emissions, biosphere-atmosphere <span class="hlt">exchange</span>, and meteorology in regulating the spatial distribution of <span class="hlt">CO</span><span class="hlt">2</span> near the surface over the contiguous United States. Three sets of net ecosystem <span class="hlt">exchange</span> (NEE) fluxes were used as input to assess the impact of uncertainty of NEE on <span class="hlt">CO</span><span class="hlt">2</span> concentrations simulated by CMAQ. Observational data from six tall tower sites across the country were used to evaluate model performance. In particular, at the Boulder Atmospheric Observatory (BAO), a tall tower site that receives urban emissions from Denver <span class="hlt">CO</span>, the CMAQ model using hourly varying, high-resolution <span class="hlt">CO</span><span class="hlt">2</span> fossil-fuel emissions from the Vulcan inventory and Carbon Tracker optimized NEE reproduced the observed diurnal profile of <span class="hlt">CO</span><span class="hlt">2</span> reasonably well but with a low bias in the early morning. The spatial distribution of <span class="hlt">CO</span><span class="hlt">2</span> was found to correlate with NO(x), SO<span class="hlt">2</span>, and <span class="hlt">CO</span>, because of their similar fossil-fuel emission sources and common transport processes. These initial results from CMAQ demonstrate the potential of using a regional CTM to help interpret <span class="hlt">CO</span><span class="hlt">2</span> observations and understand <span class="hlt">CO</span><span class="hlt">2</span> variability in space and time. The ability to simulate a full suite of <span class="hlt">air</span> pollutants in CMAQ will also facilitate investigations of their use as tracers for <span class="hlt">CO</span><span class="hlt">2</span> source attribution. This work serves as a proof of concept and the foundation for more comprehensive examinations of <span class="hlt">CO</span><span class="hlt">2</span> spatiotemporal variability and various uncertainties in the future. Atmospheric <span class="hlt">CO</span><span class="hlt">2</span> has long been modeled</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26713663','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26713663"><span>Conversion of <span class="hlt">CO</span><span class="hlt">2</span> from <span class="hlt">Air</span> into Methanol Using a Polyamine and a Homogeneous Ruthenium Catalyst.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kothandaraman, Jotheeswari; Goeppert, Alain; Czaun, Miklos; Olah, George A; Prakash, G K Surya</p> <p>2016-01-27</p> <p>A highly efficient homogeneous catalyst system for the production of CH3OH from <span class="hlt">CO</span><span class="hlt">2</span> using pentaethylenehexamine and Ru-Macho-BH (1) at 125-165 °C in an ethereal solvent has been developed (initial turnover frequency = 70 h(-1) at 145 °C). Ease of separation of CH3OH is demonstrated by simple distillation from the reaction mixture. The robustness of the catalytic system was shown by recycling the catalyst over five runs without significant loss of activity (turnover number > 2000). Various sources of <span class="hlt">CO</span><span class="hlt">2</span> can be used for this reaction including <span class="hlt">air</span>, despite its low <span class="hlt">CO</span><span class="hlt">2</span> concentration (400 ppm). For the first time, we have demonstrated that <span class="hlt">CO</span><span class="hlt">2</span> captured from <span class="hlt">air</span> can be directly converted to CH3OH in 79% yield using a homogeneous catalytic system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23658555','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23658555"><span>The pH and p<span class="hlt">CO</span><span class="hlt">2</span> dependence of sulfate reduction in shallow-<span class="hlt">sea</span> hydrothermal <span class="hlt">CO</span><span class="hlt">2</span> - venting sediments (Milos Island, Greece).</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bayraktarov, Elisa; Price, Roy E; Ferdelman, Timothy G; Finster, Kai</p> <p>2013-01-01</p> <p>Microbial sulfate reduction (SR) is a dominant process of organic matter mineralization in sulfate-rich anoxic environments at neutral pH. Recent studies have demonstrated SR in low pH environments, but investigations on the microbial activity at variable pH and <span class="hlt">CO</span><span class="hlt">2</span> partial pressure are still lacking. In this study, the effect of pH and p<span class="hlt">CO</span><span class="hlt">2</span> on microbial activity was investigated by incubation experiments with radioactive (35)S targeting SR in sediments from the shallow-<span class="hlt">sea</span> hydrothermal vent system of Milos, Greece, where pH is naturally decreased by <span class="hlt">CO</span><span class="hlt">2</span> release. Sediments differed in their physicochemical characteristics with distance from the main site of fluid discharge. Adjacent to the vent site (T ~40-75°C, pH ~5), maximal sulfate reduction rates (SRR) were observed between pH 5 and 6. SR in hydrothermally influenced sediments decreased at neutral pH. Sediments unaffected by hydrothermal venting (T ~26°C, pH ~8) expressed the highest SRR between pH 6 and 7. Further experiments investigating the effect of p<span class="hlt">CO</span><span class="hlt">2</span> on SR revealed a steep decrease in activity when the partial pressure increased from <span class="hlt">2</span> to 3 bar. Findings suggest that sulfate reducing microbial communities associated with hydrothermal vent system are adapted to low pH and high <span class="hlt">CO</span><span class="hlt">2</span>, while communities at control sites required a higher pH for optimal activity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015BGeo...12..399K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015BGeo...12..399K"><span>North America's net terrestrial <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> with the atmosphere 1990-2009</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>King, A. W.; Andres, R. J.; Davis, K. J.; Hafer, M.; Hayes, D. J.; Huntzinger, D. N.; de Jong, B.; Kurz, W. A.; McGuire, A. D.; Vargas, R.; Wei, Y.; West, T. O.; Woodall, C. W.</p> <p>2015-01-01</p> <p>Scientific understanding of the global carbon cycle is required for developing national and international policy to mitigate fossil fuel <span class="hlt">CO</span><span class="hlt">2</span> emissions by managing terrestrial carbon uptake. Toward that understanding and as a contribution to the REgional Carbon Cycle Assessment and Processes (RECCAP) project, this paper provides a synthesis of net land-atmosphere <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> for North America (Canada, United States, and Mexico) over the period 1990-2009. Only <span class="hlt">CO</span><span class="hlt">2</span> is considered, not methane or other greenhouse gases. This synthesis is based on results from three different methods: atmospheric inversion, inventory-based methods and terrestrial biosphere modeling. All methods indicate that the North American land surface was a sink for atmospheric <span class="hlt">CO</span><span class="hlt">2</span>, with a net transfer from atmosphere to land. Estimates ranged from -890 to -280 Tg C yr-1, where the mean of atmospheric inversion estimates forms the lower bound of that range (a larger land sink) and the inventory-based estimate using the production approach the upper (a smaller land sink). This relatively large range is due in part to differences in how the approaches represent trade, fire and other disturbances and which ecosystems they include. Integrating across estimates, "best" estimates (i.e., measures of central tendency) are -472 ± 281 Tg C yr-1 based on the mean and standard deviation of the distribution and -360 Tg C yr-1 (with an interquartile range of -496 to -337) based on the median. Considering both the fossil fuel emissions source and the land sink, our analysis shows that North America was, however, a net contributor to the growth of <span class="hlt">CO</span><span class="hlt">2</span> in the atmosphere in the late 20th and early 21st century. With North America's mean annual fossil fuel <span class="hlt">CO</span><span class="hlt">2</span> emissions for the period 1990-2009 equal to 1720 Tg C yr-1 and assuming the estimate of -472 Tg C yr-1 as an approximation of the true terrestrial <span class="hlt">CO</span><span class="hlt">2</span> sink, the continent's source : sink ratio for this time period was 1720:472, or nearly 4:1.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1332937-transient-load-following-control-analysis-advanced-co2-power-conversion-dry-air-cooling','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1332937-transient-load-following-control-analysis-advanced-co2-power-conversion-dry-air-cooling"><span>Transient Load Following and Control Analysis of Advanced S-<span class="hlt">CO</span><span class="hlt">2</span> Power Conversion with Dry <span class="hlt">Air</span> Cooling</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>Moisseytsev, Anton; Sienicki, James J.</p> <p>2016-01-01</p> <p>Supercritical carbon dioxide (S-<span class="hlt">CO</span><span class="hlt">2</span>) Brayton cycles are under development as advanced energy converters for advanced nuclear reactors, especially the Sodium-Cooled Fast Reactor (SFR). The use of dry <span class="hlt">air</span> cooling for direct heat rejection to the atmosphere ultimate heat sink is increasingly becoming a requirement in many regions due to restrictions on water use. The transient load following and control behavior of an SFR with an S-<span class="hlt">CO</span><span class="hlt">2</span> cycle power converter utilizing dry <span class="hlt">air</span> cooling have been investigated. With extension and adjustment of the previously existing control strategy for direct water cooling, S-<span class="hlt">CO</span><span class="hlt">2</span> cycle power converters can also be used for loadmore » following operation in regions where dry <span class="hlt">air</span> cooling is a requirement« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.1533S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.1533S"><span>Inter-annual variability of <span class="hlt">exchange</span> processes at the outer Black <span class="hlt">Sea</span> shelf</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shapiro, Georgy; Wobus, Fred; Yuan, Dongliang; Wang, Zheng</p> <p>2014-05-01</p> <p> vertical discretisation (s-on-top-of-z) and other improved parameters of the model set-up as in Shapiro et al. (2013). The model was run for the period from 1979 to 2012 with water discharges from 8 main rivers, <span class="hlt">exchanges</span> through Bosporus and meteo forcing from the Drakkar Forcing Set 5.<span class="hlt">2</span> (Brodeau et al, 2010). The model was spun-up from climatological temperature and salinity in January using a semi-diagnostic adjustment method. Each annual simulation started from the same initial state on 1 January without data assimilation. The data for the warm period from 1 May to 31 October of each year were used for the following analysis. The model has been validated against in-situ (based on 77867 stations) and night-time satellite monthly mean SST observations. The model also captures well the major features seen on snapshot satellite images. A simulated daily climatology was created by averaging the temperature values over the 34-year simulation. Anomalies were calculated as the deviations of the snapshot temperatures from their climatological values. The correlation between the temperature anomalies of BSW on the outer shelf and those in the CIL waters in the deep <span class="hlt">sea</span> were computed as well as water transports between these water masses across the shelf break. The BSW on the outer shelf are defined as the waters between the density level σθ=14.<span class="hlt">2</span> kg m3 (i.e. the bottom of the surface mixed layer) and the seabed (max z=150 m at the shelf break). The corresponding data from open <span class="hlt">sea</span> CIL waters in the northwest part of the deep Black <span class="hlt">Sea</span> were taken from the depth range between σθ=14.<span class="hlt">2</span> and z=150 m. The computed Pierson correlation between summer temperatures of BSW and the deep <span class="hlt">sea</span> CIL is R = 0.90. This significant correlation is in agreement with the analysis from observational data of Shapiro et al. (2011). In order to reveal a physical link between the BSW and CIL, the in-out transports of water with σθ ≥14.<span class="hlt">2</span> across the shelf break were computed for each day and then</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeCoA.211...28H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeCoA.211...28H"><span>Carbon isotope <span class="hlt">exchange</span> between gaseous <span class="hlt">CO</span><span class="hlt">2</span> and thin solution films: Artificial cave experiments and a complete diffusion-reaction model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hansen, Maximilian; Scholz, Denis; Froeschmann, Marie-Louise; Schöne, Bernd R.; Spötl, Christoph</p> <p>2017-08-01</p> <p>Speleothem stable carbon isotope (δ13C) records provide important paleoclimate and paleo-environmental information. However, the interpretation of these records in terms of past climate or environmental change remains challenging because of various processes affecting the δ13C signals. A process that has only been sparsely discussed so far is carbon isotope <span class="hlt">exchange</span> between the gaseous <span class="hlt">CO</span><span class="hlt">2</span> of the cave atmosphere and the dissolved inorganic carbon (DIC) contained in the thin solution film on the speleothem, which may be particularly important for strongly ventilated caves. Here we present a novel, complete reaction diffusion model describing carbon isotope <span class="hlt">exchange</span> between gaseous <span class="hlt">CO</span><span class="hlt">2</span> and the DIC in thin solution films. The model considers all parameters affecting carbon isotope <span class="hlt">exchange</span>, such as diffusion into, out of and within the film, the chemical reactions occurring within the film as well as the dependence of diffusion and the reaction rates on isotopic mass and temperature. To verify the model, we conducted laboratory experiments under completely controlled, cave-analogue conditions at three different temperatures (10, 20, 30 °C). We exposed thin (≈0.1 mm) films of a NaHCO3 solution with four different concentrations (1, <span class="hlt">2</span>, 5 and 10 mmol/l, respectively) to a nitrogen atmosphere containing a specific amount of <span class="hlt">CO</span><span class="hlt">2</span> (1000 and 3000 ppmV). The experimentally observed temporal evolution of the pH and δ13C values of the DIC is in good agreement with the model predictions. The carbon isotope <span class="hlt">exchange</span> times in our experiments range from ca. 200 to ca. 16,000 s and strongly depend on temperature, film thickness, atmospheric p<span class="hlt">CO</span><span class="hlt">2</span> and the concentration of DIC. For low p<span class="hlt">CO</span><span class="hlt">2</span> (between 500 and 1000 ppmV, as for strongly ventilated caves), our time constants are substantially lower than those derived in a previous study, suggesting a potentially stronger influence of carbon isotope <span class="hlt">exchange</span> on speleothem δ13C values. However, this process should only have an</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015DSRI...97....1K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015DSRI...97....1K"><span>Design, construction, and operation of an actively controlled deep-<span class="hlt">sea</span> <span class="hlt">CO</span><span class="hlt">2</span> enrichment experiment using a cabled observatory system</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kirkwood, William J.; Walz, Peter M.; Peltzer, Edward T.; Barry, James P.; Herlien, Robert A.; Headley, Kent L.; Kecy, Chad; Matsumoto, George I.; Maughan, Thom; O'Reilly, Thomas C.; Salamy, Karen A.; Shane, Farley; Brewer, Peter G.</p> <p>2015-03-01</p> <p>We describe the design, testing, and performance of an actively controlled deep-<span class="hlt">sea</span> Free Ocean <span class="hlt">CO</span><span class="hlt">2</span> Enrichment (dp-FOCE) system for the execution of seafloor experiments relating to the impacts of ocean acidification on natural ecosystems. We used the 880 m deep MARS (Monterey Accelerated Research System) cable site offshore Monterey Bay, California for this work, but the Free Ocean <span class="hlt">CO</span><span class="hlt">2</span> Enrichment (FOCE) system concept is designed to be scalable and can be modified to be used in a wide variety of ocean depths and locations. The main frame is based on a flume design with active thruster control of flow and a central experimental chamber. The unit was allowed to free fall to the seafloor and connected to the cable node by remotely operated vehicle (ROV) manipulation. For operation at depth we designed a liquid <span class="hlt">CO</span><span class="hlt">2</span> containment reservoir which provided the <span class="hlt">CO</span><span class="hlt">2</span> enriched working fluid as ambient seawater was drawn through the reservoir beneath the more buoyant liquid <span class="hlt">CO</span><span class="hlt">2</span>. Our design allowed for the significant lag time associated with the hydration of the dissolved <span class="hlt">CO</span><span class="hlt">2</span> molecule, resulting in an e-folding time, τ, of 97 s between fluid injection and pH sensing at the mean local T=4.31±0.14 °C and pHT of 7.625±0.011. The system maintained a pH offset of 0.4 pH units compared to the surrounding ocean for a period of 1 month. The unit allows for the emplacement of deep-<span class="hlt">sea</span> animals for testing. We describe the components and software used for system operation and show examples of each. The demonstrated ability for active control of experimental systems opens new possibilities for deep-<span class="hlt">sea</span> biogeochemical perturbation experiments of several kinds and our developments in open source control systems software and hardware described here are applicable to this end.</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> fluxes 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> fluxes 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> fluxes. 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 fluxes because they create additional turbulence at the water surface. We correct fluxes 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> fluxes 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> fluxes 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> fluxes. 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 fluxes because they create additional turbulence at the water surface. We correct fluxes 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.ncbi.nlm.nih.gov/pubmed/26990845','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26990845"><span>The effect of anthropogenic activity on BTEX, NO<span class="hlt">2</span>, SO<span class="hlt">2</span>, and <span class="hlt">CO</span> concentrations in urban <span class="hlt">air</span> of the spa city of Sopot and medium-industrialized city of Tczew located in North Poland.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Marć, Mariusz; Bielawska, Michalina; Simeonov, Vasil; Namieśnik, Jacek; Zabiegała, Bożena</p> <p>2016-05-01</p> <p>The major goal of the present study is to compare the <span class="hlt">air</span> quality of two urban locations situated in Northern Poland - the spa City of Sopot and the medium-industrialized city of Tczew using chemometric methods. As a criterion for the assessment of atmospheric <span class="hlt">air</span> quality, measurements of benzene, toluene, ethylbenzene and total xylenes were used (collected from atmospheric <span class="hlt">air</span> using diffusion-type passive samplers) as well as measurements of inorganic compounds - <span class="hlt">CO</span>, NO<span class="hlt">2</span> and SO<span class="hlt">2</span>, which were subject to routine control and determined by means of automatic analysers. Studies related to determination of defined chemical compounds in the urban <span class="hlt">air</span> in the monitored area were performed from January 2013 to December 2014. By interpreting the results obtained and using basic multivariate statistical tools (cluster analysis and principal components analysis), major sources of emissions of determined pollutants in the <span class="hlt">air</span> in urbanized areas were defined. The study also shows the potential influence of the <span class="hlt">sea</span> breeze on concentrations of chemical compounds in the atmospheric <span class="hlt">air</span> in the spa city of Sopot. Copyright © 2016 Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28308642','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28308642"><span>[Different NaCl-dependence of the circadian <span class="hlt">CO</span><span class="hlt">2</span>-gas-<span class="hlt">exchange</span> of some halophil growing coastal plants].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Treichel, Siegfried; Bauer, Peter</p> <p>1974-03-01</p> <p><span class="hlt">CO</span> <span class="hlt">2</span> -<span class="hlt">exchange</span>, diurnal changes in malate- and ion concentrations of the halophytes Carpobrotus edulis, Crithmum maritimum, Mesembryanthemum nodiflorum, Salicornia fruticosa, Suaeda maritima, and Trifolium fragiferum were investigated after culture at different NaCl concentrations. In Carp. edulis and Mes. nodiflorum the diurnal rhythm of <span class="hlt">CO</span> <span class="hlt">2</span> -<span class="hlt">exchange</span> is in accordance with that of crassulacean acid metabolism (CAM), in Sal. fruticosa, Crithm. maritimum, Suaeda maritima, and Trif. fragiferum with that of Benson-Calvin metabolism (C 3 ). Malate concentration and <span class="hlt">CO</span> <span class="hlt">2</span> uptake in the sap latter group are not influenced. On the other hand, Carp. edulis and Mes. nodiflorum show an accumulation of malate during the night, which can be interpreted as a further indication of CAM.The two species most resistant to NaCl, Carp. edulis and Sal. fruticosa, greatly differ very much in their NaCl content. NaCl concentration in Salicornia is four times higher than in Carpobrotus.The different metabolic properties studied might be of ecological importance for the plants in their natural habitats. The effect of NaCl on metabolic processes is discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70169234','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70169234"><span>Assessment of model estimates of land-atmosphere <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> across northern Eurasia</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Rawlins, M.A.; McGuire, A.D.; Kimball, J.S.; Dass, P.; Lawrence, D.; Burke, E.; Chen, X.; Delire, C.; Koven, C.; MacDougall, A.; Peng, S.; Rinke, A.; Saito, K.; Zhang, W.; Alkama, R.; Bohn, T. J.; Ciais, P.; Decharme, B.; Gouttevin, I.; Hajima, T.; Ji, D.; Krinner, G.; Lettenmaier, D.P.; Miller, P.; Moore, J.C.; Smith, B.; Sueyoshi, T.</p> <p>2015-01-01</p> <p>A warming climate is altering land-atmosphere <span class="hlt">exchanges</span> of carbon, with a potential for increased vegetation productivity as well as the mobilization of permafrost soil carbon stores. Here we investigate land-atmosphere carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) cycling through analysis of net ecosystem productivity (NEP) and its component fluxes of gross primary productivity (GPP) and ecosystem respiration (ER) and soil carbon residence time, simulated by a set of land surface models (LSMs) over a region spanning the drainage basin of Northern Eurasia. The retrospective simulations cover the period 1960–2009 at 0.5° resolution, which is a scale common among many global carbon and climate model simulations. Model performance benchmarks were drawn from comparisons against both observed <span class="hlt">CO</span><span class="hlt">2</span> fluxes derived from site-based eddy covariance measurements as well as regional-scale GPP estimates based on satellite remote-sensing data. The site-based comparisons depict a tendency for overestimates in GPP and ER for several of the models, particularly at the two sites to the south. For several models the spatial pattern in GPP explains less than half the variance in the MODIS MOD17 GPP product. Across the models NEP increases by as little as 0.01 to as much as 0.79 g C m−<span class="hlt">2</span> yr−<span class="hlt">2</span>, equivalent to 3 to 340 % of the respective model means, over the analysis period. For the multimodel average the increase is 135 % of the mean from the first to last 10 years of record (1960–1969 vs. 2000–2009), with a weakening <span class="hlt">CO</span><span class="hlt">2</span> sink over the latter decades. Vegetation net primary productivity increased by 8 to 30 % from the first to last 10 years, contributing to soil carbon storage gains. The range in regional mean NEP among the group is twice the multimodel mean, indicative of the uncertainty in <span class="hlt">CO</span><span class="hlt">2</span> sink strength. The models simulate that inputs to the soil carbon pool exceeded losses, resulting in a net soil carbon gain amid a decrease in residence time. Our analysis points to improvements in model</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010OcSci...6...91F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010OcSci...6...91F"><span>Thermodynamic properties of <span class="hlt">sea</span> <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>Feistel, R.; Wright, D. G.; Kretzschmar, H.-J.; Hagen, E.; Herrmann, S.; Span, R.</p> <p>2010-02-01</p> <p>Very accurate thermodynamic potential functions are available for fluid water, ice, seawater and humid <span class="hlt">air</span> covering wide ranges of temperature and pressure conditions. They permit the consistent computation of all equilibrium properties as, for example, required for coupled atmosphere-ocean models or the analysis of observational or experimental data. With the exception of humid <span class="hlt">air</span>, these potential functions are already formulated as international standards released by the International Association for the Properties of Water and Steam (IAPWS), and have been adopted in 2009 for oceanography by IOC/UNESCO. In this paper, we derive a collection of formulas for important quantities expressed in terms of the thermodynamic potentials, valid for typical phase transitions and composite systems of humid <span class="hlt">air</span> and water/ice/seawater. Particular attention is given to equilibria between seawater and humid <span class="hlt">air</span>, referred to as "<span class="hlt">sea</span> <span class="hlt">air</span>" here. In a related initiative, these formulas will soon be implemented in a source-code library for easy practical use. The library is primarily aimed at oceanographic applications but will be relevant to <span class="hlt">air-sea</span> interaction and meteorology as well. The formulas provided are valid for any consistent set of suitable thermodynamic potential functions. Here we adopt potential functions from previous publications in which they are constructed from theoretical laws and empirical data; they are briefly summarized in the appendix. The formulas make use of the full accuracy of these thermodynamic potentials, without additional approximations or empirical coefficients. They are expressed in the temperature scale ITS-90 and the 2008 Reference-Composition Salinity Scale.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009OcScD...6.2193F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009OcScD...6.2193F"><span>Thermodynamic properties of <span class="hlt">sea</span> <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>Feistel, R.; Kretzschmar, H.-J.; Span, R.; Hagen, E.; Wright, D. G.; Herrmann, S.</p> <p>2009-10-01</p> <p>Very accurate thermodynamic potential functions are available for fluid water, ice, seawater and humid <span class="hlt">air</span> covering wide ranges of temperature and pressure conditions. They permit the consistent computation of all equilibrium properties as, for example, required for coupled atmosphere-ocean models or the analysis of observational or experimental data. With the exception of humid <span class="hlt">air</span>, these potential functions are already formulated as international standards released by the International Association for the Properties of Water and Steam (IAPWS), and have been adopted in 2009 for oceanography by IOC/UNESCO. In this paper, we derive a collection of formulas for important quantities expressed in terms of the thermodynamic potentials, valid for typical phase transitions and composite systems of humid <span class="hlt">air</span> and water/ice/seawater. Particular attention is given to equilibria between seawater and humid <span class="hlt">air</span>, referred to as ''<span class="hlt">sea</span> <span class="hlt">air</span>'' here. In a related initiative, these formulas will soon be implemented in a source-code library for easy practical use. The library is primarily aimed at oceanographic applications but will be relevant to <span class="hlt">air-sea</span> interaction and meteorology as well. The formulas provided are valid for any consistent set of suitable thermodynamic potential functions. Here we adopt potential functions from previous publications in which they are constructed from theoretical laws and empirical data; they are briefly summarized in the appendix. The formulas make use of the full accuracy of these thermodynamic potentials, without additional approximations or empirical coefficients. They are expressed in the temperature scale ITS-90 and the 2008 Reference-Composition Salinity Scale.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4085958','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4085958"><span>Nocturnal versus diurnal <span class="hlt">CO</span><span class="hlt">2</span> uptake: how flexible is Agave angustifolia?</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Winter, Klaus; Garcia, Milton; Holtum, Joseph A. M.</p> <p>2014-01-01</p> <p>Agaves exhibit the water-conserving crassulacean acid metabolism (CAM) photosynthetic pathway. Some species are potential biofuel feedstocks because they are highly productive in seasonally dry landscapes. In plants with CAM, high growth rates are often believed to be associated with a significant contribution of C3 photosynthesis to total carbon gain when conditions are favourable. There has even been a report of a shift from CAM to C3 in response to overwatering a species of Agave. We investigated whether C3 photosynthesis can contribute substantially to carbon uptake and growth in young and mature Agave angustifolia collected from its natural habitat in Panama. In well-watered plants, <span class="hlt">CO</span><span class="hlt">2</span> uptake in the dark contributed about 75% of daily carbon gain. This day/night pattern of <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> was highly conserved under a range of environmental conditions and was insensitive to intensive watering. Elevated <span class="hlt">CO</span><span class="hlt">2</span> (800 ppm) stimulated <span class="hlt">CO</span><span class="hlt">2</span> fixation predominantly in the light. Exposure to <span class="hlt">CO</span><span class="hlt">2</span>-free <span class="hlt">air</span> at night markedly enhanced <span class="hlt">CO</span><span class="hlt">2</span> uptake during the following light period, but <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">exchange</span> rapidly reverted to its standard pattern when <span class="hlt">CO</span><span class="hlt">2</span> was supplied during the subsequent 24h. Although A. angustifolia consistently engages in CAM as its principal photosynthetic pathway, its relatively limited photosynthetic plasticity does not preclude it from occupying a range of habitats, from relatively mesic tropical environments in Panama to drier habitats in Mexico. PMID:24648568</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20170007354&hterms=Fuel+co2&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DFuel%2Bco2','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20170007354&hterms=Fuel+co2&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DFuel%2Bco2"><span>Young People's Burden: Requirement of Negative <span class="hlt">CO</span><span class="hlt">2</span> Emissions</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hansen, James; Sato, Makiko; Kharecha, Pushker; Von Schuckmann, Karina; Beerling, David J.; Cao, Junji; Marcott, Shaun; Masson-Delmotte, Valerie; Prather, Michael J.; Rohling, Eelco J.; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20170007354'); toggleEditAbsImage('author_20170007354_show'); toggleEditAbsImage('author_20170007354_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20170007354_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20170007354_hide"></p> <p>2017-01-01</p> <p>Global temperature is a fundamental climate metric highly correlated with <span class="hlt">sea</span> level, which implies that keeping shorelines near their present location requires keeping global temperature within or close to its preindustrial Holocene range. However, global temperature excluding short-term variability now exceeds +1 C relative to the 1880 - 1920 mean and annual 2016 global temperature was almost +1.3 C. We show that global temperature has risen well out of the Holocene range and Earth is now as warm as it was during the prior (Eemian) interglacial period, when <span class="hlt">sea</span> level reached 6 - 9 m higher than today. Further, Earth is out of energy balance with present atmospheric composition, implying that more warming is in the pipeline, and we show that the growth rate of greenhouse gas climate forcing has accelerated markedly in the past decade. The rapidity of ice sheet and <span class="hlt">sea</span> level response to global temperature is difficult to predict, but is dependent on the magnitude of warming. Targets for limiting global warming thus, at minimum, should aim to avoid leaving global temperature at Eemian or higher levels for centuries. Such targets now require "negative emissions", i.e., extraction of <span class="hlt">CO</span><span class="hlt">2</span> from the <span class="hlt">air</span>. If phasedown of fossil fuel emissions begins soon, improved agricultural and forestry practices, including reforestation and steps to improve soil fertility and increase its carbon content, may provide much of the necessary <span class="hlt">CO</span><span class="hlt">2</span> extraction. In that case, the magnitude and duration of global temperature excursion above the natural range of the current interglacial (Holocene) could be limited and irreversible climate impacts could be minimized. In contrast, continued high fossil fuel emissions today place a burden on young people to undertake massive technological <span class="hlt">CO</span><span class="hlt">2</span> extraction if they are to limit climate change and its consequences. Proposed methods of extraction such as bioenergy with carbon capture and storage (BECCS) or <span class="hlt">air</span> capture of <span class="hlt">CO</span><span class="hlt">2</span> have minimal estimated costs</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ESD.....8..577H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ESD.....8..577H"><span>Young people's burden: requirement of negative <span class="hlt">CO</span><span class="hlt">2</span> emissions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hansen, James; Sato, Makiko; Kharecha, Pushker; von Schuckmann, Karina; Beerling, David J.; Cao, Junji; Marcott, Shaun; Masson-Delmotte, Valerie; Prather, Michael J.; Rohling, Eelco J.; Shakun, Jeremy; Smith, Pete; Lacis, Andrew; Russell, Gary; Ruedy, Reto</p> <p>2017-07-01</p> <p>Global temperature is a fundamental climate metric highly correlated with <span class="hlt">sea</span> level, which implies that keeping shorelines near their present location requires keeping global temperature within or close to its preindustrial Holocene range. However, global temperature excluding short-term variability now exceeds +1 °C relative to the 1880-1920 mean and annual 2016 global temperature was almost +1.3 °C. We show that global temperature has risen well out of the Holocene range and Earth is now as warm as it was during the prior (Eemian) interglacial period, when <span class="hlt">sea</span> level reached 6-9 m higher than today. Further, Earth is out of energy balance with present atmospheric composition, implying that more warming is in the pipeline, and we show that the growth rate of greenhouse gas climate forcing has accelerated markedly in the past decade. The rapidity of ice sheet and <span class="hlt">sea</span> level response to global temperature is difficult to predict, but is dependent on the magnitude of warming. Targets for limiting global warming thus, at minimum, should aim to avoid leaving global temperature at Eemian or higher levels for centuries. Such targets now require <q>negative emissions</q>, i.e., extraction of <span class="hlt">CO</span><span class="hlt">2</span> from the <span class="hlt">air</span>. If phasedown of fossil fuel emissions begins soon, improved agricultural and forestry practices, including reforestation and steps to improve soil fertility and increase its carbon content, may provide much of the necessary <span class="hlt">CO</span><span class="hlt">2</span> extraction. In that case, the magnitude and duration of global temperature excursion above the natural range of the current interglacial (Holocene) could be limited and irreversible climate impacts could be minimized. In contrast, continued high fossil fuel emissions today place a burden on young people to undertake massive technological <span class="hlt">CO</span><span class="hlt">2</span> extraction if they are to limit climate change and its consequences. Proposed methods of extraction such as bioenergy with carbon capture and storage (BECCS) or <span class="hlt">air</span> capture of <span class="hlt">CO</span><span class="hlt">2</span> have minimal estimated</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22577839','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22577839"><span>Fe atom <span class="hlt">exchange</span> between aqueous Fe<span class="hlt">2</span>+ and magnetite.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gorski, Christopher A; Handler, Robert M; Beard, Brian L; Pasakarnis, Timothy; Johnson, Clark M; Scherer, Michelle M</p> <p>2012-11-20</p> <p>The reaction between magnetite and aqueous Fe(<span class="hlt">2</span>+) has been extensively studied due to its role in contaminant reduction, trace-metal sequestration, and microbial respiration. Previous work has demonstrated that the reaction of Fe(<span class="hlt">2</span>+) with magnetite (Fe(3)O(4)) results in the structural incorporation of Fe(<span class="hlt">2</span>+) and an increase in the bulk Fe(<span class="hlt">2</span>+) content of magnetite. It is unclear, however, whether significant Fe atom <span class="hlt">exchange</span> occurs between magnetite and aqueous Fe(<span class="hlt">2</span>+), as has been observed for other Fe oxides. Here, we measured the extent of Fe atom <span class="hlt">exchange</span> between aqueous Fe(<span class="hlt">2</span>+) and magnetite by reacting isotopically "normal" magnetite with (57)Fe-enriched aqueous Fe(<span class="hlt">2</span>+). The extent of Fe atom <span class="hlt">exchange</span> between magnetite and aqueous Fe(<span class="hlt">2</span>+) was significant (54-71%), and went well beyond the amount of Fe atoms found at the near surface. Mössbauer spectroscopy of magnetite reacted with (56)Fe(<span class="hlt">2</span>+) indicate that no preferential <span class="hlt">exchange</span> of octahedral or tetrahedral sites occurred. <span class="hlt">Exchange</span> experiments conducted with <span class="hlt">Co</span>-ferrite (<span class="hlt">Co</span>(<span class="hlt">2</span>+)Fe(<span class="hlt">2</span>)(3+)O(4)) showed little impact of <span class="hlt">Co</span> substitution on the rate or extent of atom <span class="hlt">exchange</span>. Bulk electron conduction, as previously invoked to explain Fe atom <span class="hlt">exchange</span> in goethite, is a possible mechanism, but if it is occurring, conduction does not appear to be the rate-limiting step. The lack of significant impact of <span class="hlt">Co</span> substitution on the kinetics of Fe atom <span class="hlt">exchange</span>, and the relatively high diffusion coefficients reported for magnetite suggest that for magnetite, unlike goethite, Fe atom diffusion is a plausible mechanism to explain the rapid rates of Fe atom <span class="hlt">exchange</span> in magnetite.</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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