Sample records for air-sea co2 transfer

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

    NASA Technical Reports Server (NTRS)

    McClain, Charles R.; Signorini, Sergio

    2002-01-01

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

  2. In situ evaluation of air-sea CO2 gas transfer velocity in an inner estuary using eddy covariance - with a special focus on the importance of using reliable CO2-fluxes

    NASA Astrophysics Data System (ADS)

    Jørgensen, E. T.; Sørensen, L. L.; Jensen, B.; Sejr, M. K.

    2012-04-01

    The air-sea exchange of CO2 or CO2 flux is driven by the difference in the partial pressure of CO2 in the water and the atmosphere (ΔpCO2), the solubility of CO2 (K0) and the gas transfer velocity (k) (Wanninkhof et al., 2009;Weiss, 1974) . ΔpCO2 and K0 are determined with relatively high precision and it is estimated that the biggest uncertainty when modelling the air-sea flux is the parameterization of k. As an example; the estimated global air-sea 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 CO2 in the inner estuary of Roskilde Fjord, Denmark was investigated using eddy covariance CO2 fluxes (ECM) and directly measured ΔpCO2 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 DS2; including the inertial dissipation method (IDM). The inner part of Roskilde Fjord showed to be a very biological active CO2 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 air and water influence k600. The wind speed parameterization of k600 using DS1 showed some scatter but when including IDM the r2 of DS2 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 CO2 fluxes calculated by the ECM are removed when including the IDM.

  3. 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.

  4. 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

  5. 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

  6. 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> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ACP....18.4297L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ACP....18.4297L"><span>Using eddy covariance to measure the dependence of <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange rate on friction velocity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Landwehr, Sebastian; Miller, Scott D.; Smith, Murray J.; Bell, Thomas G.; Saltzman, Eric S.; Ward, Brian</p> <p>2018-03-01</p> <p>Parameterisation of the <span class="hlt">air-sea</span> gas <span class="hlt">transfer</span> velocity of <span class="hlt">CO</span><span class="hlt">2</span> and other trace gases under open-ocean conditions has been a focus of <span class="hlt">air-sea</span> interaction research and is required for accurately determining ocean carbon uptake. Ships are the most widely used platform for <span class="hlt">air-sea</span> 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 <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> 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 <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> velocities can be parameterised with a linear fit to u*. The SOAP data are compared to previous gas <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> studies, but at high wind speeds they do not support the sharp increase in gas <span class="hlt">transfer</span> associated with bubble-mediated <span class="hlt">transfer</span> predicted by physically based models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1995TellB..47..447I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1995TellB..47..447I"><span><span class="hlt">Air-sea</span> exchange of <span class="hlt">CO</span><span class="hlt">2</span> in the central and western equatorial Pacific in 1990</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ishii, Masao; Yoshikawa Inoue, Hisayuki</p> <p>1995-09-01</p> <p>Measurements of <span class="hlt">CO</span><span class="hlt">2</span> in marine boundary <span class="hlt">air</span> and in surface seawater of the central and western Pacific west of 150°W were made during the period from September to December 1990. The meridional section along 150°W showed p<span class="hlt">CO</span><span class="hlt">2</span>(<span class="hlt">sea</span>) maximum over 410 µatm between the equator and 3°S due to strong equatorial upwelling. In the equatorial Pacific between 150°W and 179°E, p<span class="hlt">CO</span><span class="hlt">2</span>(<span class="hlt">sea</span>) decreased gradually toward the west as a result of biological <span class="hlt">CO</span><span class="hlt">2</span> uptake and surface <span class="hlt">sea</span> temperature increase. Between 179°E and 170°E, the p<span class="hlt">CO</span><span class="hlt">2</span>(<span class="hlt">sea</span>) decreased steeply from 400 µatm to 350 µatm along with a decrease of salinity. West of 170°E, where the salinity is low owing to the heavy rainfall, p<span class="hlt">CO</span><span class="hlt">2</span>(<span class="hlt">sea</span>) was nearly equal to p<span class="hlt">CO</span><span class="hlt">2</span>(<span class="hlt">air</span>). The distribution of the atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentration showed a considerable variability (±3ppm) in the area north of the Intertropical Convergence Zone due to the regional net source-sink strength of the terrestrial biosphere. The net <span class="hlt">CO</span><span class="hlt">2</span> flux from the <span class="hlt">sea</span> to the atmosphere in the equatorial region of the central and western Pacific (15°S-10°N, 140°E-150°W) was evaluated from the Δp<span class="hlt">CO</span><span class="hlt">2</span> distribution and the several gas <span class="hlt">transfer</span> coefficients reported so far. It ranged from 0.13 GtC year<img src="/entityImage/script/2212.gif" alt="-" border="0" style="font-weight: bold"></img>1-0.29 GtC year<img src="/entityImage/script/2212.gif" alt="-" border="0" style="font-weight: bold"></img>1. This <span class="hlt">CO</span><span class="hlt">2</span> outflux is thought to almost disappear during the period of an El Niño event.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014OcScD..11.1895G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014OcScD..11.1895G"><span>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>2014-07-01</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 Carbon Dioxide (<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>. f<span class="hlt">CO</span><span class="hlt">2</span> is highly sensitive to temperature and the measurements are only valid for the instantaneous <span class="hlt">sea</span> surface temperature (SST) that is measured concurrent 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 climate quality SST. This paper presents a method 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 climate quality SST data 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. 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://adsabs.harvard.edu/abs/2007GBioC..21.2015S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007GBioC..21.2015S"><span>Constraining global <span class="hlt">air-sea</span> gas exchange for <span class="hlt">CO</span><span class="hlt">2</span> with recent bomb 14C measurements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sweeney, Colm; Gloor, Emanuel; Jacobson, Andrew R.; Key, Robert M.; McKinley, Galen; Sarmiento, Jorge L.; Wanninkhof, Rik</p> <p>2007-06-01</p> <p>The 14<span class="hlt">CO</span><span class="hlt">2</span> released into the stratosphere during bomb testing in the early 1960s provides a global constraint on <span class="hlt">air-sea</span> gas exchange of soluble atmospheric gases like <span class="hlt">CO</span><span class="hlt">2</span>. Using the most complete database of dissolved inorganic radiocarbon, DI14C, available to date and a suite of ocean general circulation models in an inverse mode we recalculate the ocean inventory of bomb-produced DI14C in the global ocean and confirm that there is a 25% decrease from previous estimates using older DI14C data sets. Additionally, we find a 33% lower globally averaged gas <span class="hlt">transfer</span> velocity for <span class="hlt">CO</span><span class="hlt">2</span> compared to previous estimates (Wanninkhof, 1992) using the NCEP/NCAR Reanalysis 1 1954-2000 where the global mean winds are 6.9 m s-1. Unlike some earlier ocean radiocarbon studies, the implied gas <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> velocity ks = 0.27<u102>(Sc/660)-0.5 and standard partial pressure difference climatology of <span class="hlt">CO</span><span class="hlt">2</span> we obtain an net <span class="hlt">air-sea</span> flux estimate of 1.3 ± 0.5 PgCyr-1 for 1995. After accounting for the carbon <span class="hlt">transferred</span> from rivers to the deep ocean, our estimate of oceanic uptake (1.8 ± 0.5 PgCyr-1) compares well with estimates based on ocean inventories, ocean transport inversions using ocean concentration data, and model simulations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ACP....17.9019B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ACP....17.9019B"><span>Estimation of bubble-mediated <span class="hlt">air-sea</span> gas exchange from concurrent DMS and <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">transfer</span> velocities at intermediate-high wind speeds</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bell, Thomas G.; Landwehr, Sebastian; Miller, Scott D.; de Bruyn, Warren J.; Callaghan, Adrian H.; Scanlon, Brian; Ward, Brian; Yang, Mingxi; Saltzman, Eric S.</p> <p>2017-07-01</p> <p>Simultaneous <span class="hlt">air-sea</span> fluxes and concentration differences of dimethylsulfide (DMS) and carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) were measured during a summertime North Atlantic cruise in 2011. This data set reveals significant differences between the gas <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> of the less soluble <span class="hlt">CO</span><span class="hlt">2</span> relative to that of the more soluble DMS. However, the correlation of Δkw with whitecap fraction is no stronger than with wind speed. Models used to estimate bubble-mediated <span class="hlt">transfer</span> from in situ whitecap fraction underpredict the observations, particularly at intermediate wind speeds. Examining the differences between gas <span class="hlt">transfer</span> velocities of gases with different solubilities is a useful way to detect the impact of bubble-mediated exchange. More simultaneous gas <span class="hlt">transfer</span> measurements of different solubility gases across a wide range of oceanic conditions are needed to understand the factors controlling the magnitude and scaling of bubble-mediated gas exchange.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015CG.....77...77D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015CG.....77...77D"><span>Spatio-temporal visualization of <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> flux and carbon budget using volume rendering</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Du, Zhenhong; Fang, Lei; Bai, Yan; Zhang, Feng; Liu, Renyi</p> <p>2015-04-01</p> <p>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 <span class="hlt">air-sea</span> carbon budget and its process of accumulation are demonstrated in the spatial dimension, while the distribution pattern and variation of <span class="hlt">CO</span><span class="hlt">2</span> 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 <span class="hlt">CO</span><span class="hlt">2</span> gas with shadow effects. A data model is designed to generate four-dimensional (4D) data from satellite-derived <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> 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 <span class="hlt">Air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> Flux (Iss<span class="hlt">CO</span><span class="hlt">2</span>) for the research and assessment of <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> flux in the China <span class="hlt">Seas</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..1210167G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..1210167G"><span><span class="hlt">Air</span>-ice <span class="hlt">CO</span><span class="hlt">2</span> fluxes and p<span class="hlt">CO</span><span class="hlt">2</span> dynamics in the Arctic coastal area (Amundsen Gulf, Canada)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Geilfus, Nicolas-Xavier; Tison, Jean Louis; Carnat, Gauthier; Else, Brent; Borges, Alberto V.; Thomas, Helmuth; Shadwick, Elizabeth; Delille, Bruno</p> <p>2010-05-01</p> <p><span class="hlt">Sea</span> ice covers about 7% of the Earth surface at its maximum seasonal extent. For decades <span class="hlt">sea</span> ice was assumed to be an impermeable and inert barrier for <span class="hlt">air</span> - <span class="hlt">sea</span> exchange of <span class="hlt">CO</span><span class="hlt">2</span> so that global climate models do not include <span class="hlt">CO</span><span class="hlt">2</span> exchange between the oceans and the atmosphere in the polar regions. However, uptake of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> by <span class="hlt">sea</span> ice cover was recently reported raising the need to further investigate p<span class="hlt">CO</span><span class="hlt">2</span> dynamics in the marine cryosphere realm and related <span class="hlt">air</span>-ice <span class="hlt">CO</span><span class="hlt">2</span> fluxes. In addition, budget of <span class="hlt">CO</span><span class="hlt">2</span> fluxes are poorly constrained in high latitudes continental shelves [Borges et al., 2006]. We report measurements of <span class="hlt">air</span>-ice <span class="hlt">CO</span><span class="hlt">2</span> fluxes above the Canadian continental shelf and compare them to previous measurements carried out in Antarctica. We carried out measurements of p<span class="hlt">CO</span><span class="hlt">2</span> within brines and bulk ice, and related <span class="hlt">air</span>-ice <span class="hlt">CO</span><span class="hlt">2</span> fluxes (chamber method) in Antarctic first year pack ice ("<span class="hlt">Sea</span> 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 <span class="hlt">2</span> experiments were carried out in contrasted sites. SIMBA was carried out on <span class="hlt">sea</span> ice in early spring while CFL was carried out in from the middle of the winter to the late spring while <span class="hlt">sea</span> ice was melting. Both in Arctic and Antarctic, no <span class="hlt">air</span>-ice <span class="hlt">CO</span><span class="hlt">2</span> fluxes were detected when <span class="hlt">sea</span> 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 p<span class="hlt">CO</span><span class="hlt">2</span> of the brine exhibits a same trend in both hemispheres with a strong decrease of the p<span class="hlt">CO</span><span class="hlt">2</span> anti-correlated with the increase of <span class="hlt">sea</span> ice temperature. The p<span class="hlt">CO</span><span class="hlt">2</span> shifted from a large over-saturation at low temperature to a marked under-saturation at high temperature. These <span class="hlt">air</span>-ice <span class="hlt">CO</span><span class="hlt">2</span> fluxes are partly controlled by the permeability of the <span class="hlt">air</span>-ice interface, which depends of the temperature of this one. Moreover, <span class="hlt">air</span>-ice <span class="hlt">CO</span><span class="hlt">2</span> fluxes are</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009DSRII..56..554T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009DSRII..56..554T"><span>Climatological mean and decadal change in surface ocean p<span class="hlt">CO</span> <span class="hlt">2</span>, and net <span class="hlt">sea-air</span> <span class="hlt">CO</span> <span class="hlt">2</span> flux over the global oceans</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.; 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.</p> <p>2009-04-01</p> <p>A climatological mean distribution for the surface water p<span class="hlt">CO</span> <span class="hlt">2</span> 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 p<span class="hlt">CO</span> <span class="hlt">2</span> 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 <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. Deep-<span class="hlt">Sea</span> Res. II, 49, 1601-1622]. A time-trend analysis using deseasonalized surface water p<span class="hlt">CO</span> <span class="hlt">2</span> 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 p<span class="hlt">CO</span> <span class="hlt">2</span> 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.<span class="hlt">2</span>±0.5 and <span class="hlt">2</span>.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 p<span class="hlt">CO</span> <span class="hlt">2</span> and the <span class="hlt">sea-air</span> p<span class="hlt">CO</span> <span class="hlt">2</span> 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 p<span class="hlt">CO</span> <span class="hlt">2</span> 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 <span class="hlt">air-sea</span> <span class="hlt">CO</span> <span class="hlt">2</span> flux is estimated using the <span class="hlt">sea-air</span> p<span class="hlt">CO</span> <span class="hlt">2</span> difference and the <span class="hlt">air-sea</span> gas <span class="hlt">transfer</span> rate that is parameterized as a function of (wind speed) <span class="hlt">2</span> with a scaling factor of 0.26. This is estimated by inverting</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.5566F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.5566F"><span>Effects of <span class="hlt">sea</span>-ice and biogeochemical processes and storms on under-ice water f<span class="hlt">CO</span><span class="hlt">2</span> during the winter-spring transition in the high Arctic Ocean: Implications for <span class="hlt">sea-air</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>Fransson, Agneta; Chierici, Melissa; Skjelvan, Ingunn; Olsen, Are; Assmy, Philipp; Peterson, Algot K.; Spreen, Gunnar; Ward, Brian</p> <p>2017-07-01</p> <p>We performed measurements of carbon dioxide fugacity (f<span class="hlt">CO</span><span class="hlt">2</span>) in the surface water under Arctic <span class="hlt">sea</span> ice from January to June 2015 during the Norwegian young <span class="hlt">sea</span> 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 f<span class="hlt">CO</span><span class="hlt">2</span> observations in this region. The observed under-ice f<span class="hlt">CO</span><span class="hlt">2</span> ranged between 315 µatm in winter and 153 µatm in spring, hence was undersaturated relative to the atmospheric f<span class="hlt">CO</span><span class="hlt">2</span>. Although the <span class="hlt">sea</span> ice partly prevented direct <span class="hlt">CO</span><span class="hlt">2</span> exchange between ocean and atmosphere, frequently occurring leads and breakup of the ice sheet promoted <span class="hlt">sea-air</span> <span class="hlt">CO</span><span class="hlt">2</span> fluxes. The <span class="hlt">CO</span><span class="hlt">2</span> sink varied between 0.3 and 86 mmol C m-<span class="hlt">2</span> d-1, depending strongly on the open-water fractions (OW) and storm events. The maximum <span class="hlt">sea-air</span> <span class="hlt">CO</span><span class="hlt">2</span> fluxes occurred during storm events in February and June. In winter, the main drivers of the change in under-ice water f<span class="hlt">CO</span><span class="hlt">2</span> were dissolution of Ca<span class="hlt">CO</span>3 (ikaite) and vertical mixing. In June, in addition to these processes, primary production and <span class="hlt">sea-air</span> <span class="hlt">CO</span><span class="hlt">2</span> fluxes were important. The cumulative loss due to Ca<span class="hlt">CO</span>3 dissolution of 0.7 mol C m-<span class="hlt">2</span> in the upper 10 m played a major role in sustaining the undersaturation of f<span class="hlt">CO</span><span class="hlt">2</span> during the entire study. The relative effects of the total f<span class="hlt">CO</span><span class="hlt">2</span> change due to Ca<span class="hlt">CO</span>3 dissolution was 38%, primary production 26%, vertical mixing 16%, <span class="hlt">sea-air</span> <span class="hlt">CO</span><span class="hlt">2</span> fluxes 16%, and temperature and salinity insignificant.</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 <span class="hlt">transfer</span></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 exchange. 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 exchange. We are therefore using theory, data analysis, and numerical modeling to quantify the role of spray on <span class="hlt">air-sea</span> gas <span class="hlt">transfer</span>. In this, our first formal work on this subject, we seek the rate-limiting step in spray-mediated gas <span class="hlt">transfer</span> by evaluating the three time scales that govern the exchange: τ <span class="hlt">air</span> , which quantifies the rate of <span class="hlt">transfer</span> between the atmospheric gas reservoir and the surface of the droplet; τ int , which quantifies the exchange 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/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://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> <span class="hlt">transfer</span> of dimethyl sulfide at high wind speeds</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vlahos, Penny; Monahan, Edward C.</p> <p>2009-11-01</p> <p>The <span class="hlt">air-sea</span> exchange of dimethyl sulfide (DMS) is an important component of ocean biogeochemistry and global climate models. Both laboratory experiments and field measurements of DMS <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> rates may diverge from other gases as wind speeds increase. Herein we provide a mechanism that predicts the attenuation of DMS <span class="hlt">transfer</span> rates at high wind speeds. The model is based on the amphiphilic nature of DMS that leads to <span class="hlt">transfer</span> 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/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 <span class="hlt">Transfer</span>: Results From the High Wind Speed Gas Exchange 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 <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> 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> <span class="hlt">transfer</span> 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> <span class="hlt">transfer</span>. A modified version of the Coupled Ocean-Atmosphere Response Experiment Gas <span class="hlt">transfer</span> algorithm (COAREG ver. 3.5), incorporating a <span class="hlt">sea</span> state-dependent calculation of bubble-mediated <span class="hlt">transfer</span>, successfully reproduces the mean trend in observed k660 with wind speed for both gases. Significant suppression of gas <span class="hlt">transfer</span> by large waves was not observed during HiWinGS, in contrast to results from two prior field programs.</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/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://hdl.handle.net/2060/20140005396','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140005396"><span>Surface Ocean p<span class="hlt">CO</span><span class="hlt">2</span> Seasonality and <span class="hlt">Sea-Air</span> <span class="hlt">CO</span><span class="hlt">2</span> Flux Estimates for the North American East Coast</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Signorini, Sergio; Mannino, Antonio; Najjar, Raymond G., Jr.; Friedrichs, Marjorie A. M.; Cai, Wei-Jun; Salisbury, Joe; Wang, Zhaohui Aleck; Thomas, Helmuth; Shadwick, Elizabeth</p> <p>2013-01-01</p> <p>Underway and in situ observations of surface ocean p<span class="hlt">CO</span><span class="hlt">2</span>, combined with satellite data, were used to develop p<span class="hlt">CO</span><span class="hlt">2</span> regional algorithms to analyze the seasonal and interannual variability of surface ocean p<span class="hlt">CO</span><span class="hlt">2</span> and <span class="hlt">sea-air</span> <span class="hlt">CO</span><span class="hlt">2</span> 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 p<span class="hlt">CO</span><span class="hlt">2</span>. Estimates of the <span class="hlt">sea-air</span> <span class="hlt">CO</span><span class="hlt">2</span> flux were derived from the available p<span class="hlt">CO</span><span class="hlt">2</span> data, as well as from the p<span class="hlt">CO</span><span class="hlt">2</span> reconstructed by the algorithm. Two different gas exchange parameterizations were used. The SS, GB+NS, MAB, and SAB regions are net sinks of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> while the GoM is a weak source. The estimates vary depending on the use of surface ocean p<span class="hlt">CO</span><span class="hlt">2</span> 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 <span class="hlt">CO</span><span class="hlt">2</span> 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 <span class="hlt">CO</span><span class="hlt">2</span> /sq m/yr) over the period 2003-2010.</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://adsabs.harvard.edu/abs/2017ESD.....8.1093P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ESD.....8.1093P"><span>The potential of using remote sensing data to estimate <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange in the Baltic <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Parard, Gaëlle; Rutgersson, Anna; Parampil, Sindu Raj; Alexandre Charantonis, Anastase</p> <p>2017-12-01</p> <p>In this article, we present the first climatological map of <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> flux over the Baltic <span class="hlt">Sea</span> based on remote sensing data: estimates of p<span class="hlt">CO</span><span class="hlt">2</span> derived from satellite imaging using self-organizing map classifications along with class-specific linear regressions (SOMLO methodology) and remotely sensed wind estimates. The estimates have a spatial resolution of 4 km both in latitude and longitude and a monthly temporal resolution from 1998 to 2011. The <span class="hlt">CO</span><span class="hlt">2</span> 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 <span class="hlt">CO</span><span class="hlt">2</span> 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 p<span class="hlt">CO</span><span class="hlt">2</span> unvaryingly over the whole Baltic <span class="hlt">Sea</span>, with high winter <span class="hlt">CO</span><span class="hlt">2</span> emissions and high p<span class="hlt">CO</span><span class="hlt">2</span> uptakes. All basins act as a source for the atmosphere, with a higher degree of emission in the southern regions (mean source of 1.6 mmol m-<span class="hlt">2</span> d-1 for the South Basin and 0.9 for the Central Basin) than in the northern regions (mean source of 0.1 mmol m-<span class="hlt">2</span> d-1) and the coastal areas act as a larger sink (annual uptake of -4.<span class="hlt">2</span> mmol m-<span class="hlt">2</span> d-1) than does the open <span class="hlt">sea</span> (-4 mmol m-<span class="hlt">2</span> d-1). In its entirety, the Baltic <span class="hlt">Sea</span> acts as a small source of 1.<span class="hlt">2</span> mmol m-<span class="hlt">2</span> d-1 on average and this annual uptake has increased from 1998 to 2012.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/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('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 <span class="hlt">transfer</span> in the North Atlantic: evidence for limited interfacial gas exchange at high wind speed</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bell, T. G.; De Bruyn, W.; Miller, S. D.; Ward, B.; Christensen, K.; Saltzman, E. S.</p> <p>2013-05-01</p> <p>Shipboard measurements of eddy covariance DMS <span class="hlt">air/sea</span> fluxes and seawater concentration were carried out in the North Atlantic bloom region in June/July 2011. Gas <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span>. This effect may be more easily observed for DMS than for less soluble gases, such as <span class="hlt">CO</span><span class="hlt">2</span>, because the <span class="hlt">air/sea</span> exchange of DMS is controlled by interfacial rather than bubble-mediated gas <span class="hlt">transfer</span> under high wind speed conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PrOce.144...15W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PrOce.144...15W"><span>Biofilm-like properties of the <span class="hlt">sea</span> surface and predicted effects on <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wurl, Oliver; Stolle, Christian; Van Thuoc, Chu; The Thu, Pham; Mari, Xavier</p> <p>2016-05-01</p> <p>Because the <span class="hlt">sea</span> surface controls various interactions between the ocean and the atmosphere, it has a profound function for marine biogeochemistry and climate regulation. The <span class="hlt">sea</span> surface is the gateway for the exchange of climate-relevant gases, heat and particles. Thus, in order to determine how the ocean and the atmosphere interact and respond to environmental changes on a global scale, the characterization and understanding of the <span class="hlt">sea</span> surface are essential. The uppermost part of the water column is defined as the <span class="hlt">sea</span>-surface microlayer and experiences strong spatial and temporal dynamics, mainly due to meteorological forcing. Wave-damped areas at the <span class="hlt">sea</span> surface are caused by the accumulation of surface-active organic material and are defined as slicks. Natural slicks are observed frequently but their biogeochemical properties are poorly understood. In the present study, we found up to 40 times more transparent exopolymer particles (TEP), the foundation of any biofilm, in slicks compared to the underlying bulk water at multiple stations in the North Pacific, South China <span class="hlt">Sea</span>, and Baltic <span class="hlt">Sea</span>. We found a significant lower enrichment of TEP (up to 6) in non-slick <span class="hlt">sea</span> surfaces compared to its underlying bulk water. Moreover, slicks were characterized by a large microbial biomass, another shared feature with conventional biofilms on solid surfaces. Compared to non-slick samples (avg. pairwise similarity of 70%), the community composition of bacteria in slicks was increasingly (avg. pairwise similarity of 45%) different from bulk water communities, indicating that the TEP-matrix creates specific environments for its inhabitants. We, therefore, conclude that slicks can feature biofilm-like properties with the excessive accumulation of particles and microbes. We also assessed the potential distribution and frequency of slick-formation in coastal and oceanic regions, and their effect on <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange based on literature data. We estimate that slicks can reduce <span class="hlt">CO</span><span class="hlt">2</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/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> <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 <span class="hlt">transfer</span> in the North Atlantic: evidence for limited interfacial gas exchange at high wind speed</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bell, T. G.; De Bruyn, W.; Miller, S. D.; Ward, B.; Christensen, K.; Saltzman, E. S.</p> <p>2013-11-01</p> <p>Shipboard measurements of eddy covariance dimethylsulfide (DMS) <span class="hlt">air-sea</span> fluxes and seawater concentration were carried out in the North Atlantic bloom region in June/July 2011. Gas <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span>. This effect may be more easily observed for DMS than for less soluble gases, such as <span class="hlt">CO</span><span class="hlt">2</span>, because the <span class="hlt">air-sea</span> exchange of DMS is controlled by interfacial rather than bubble-mediated gas <span class="hlt">transfer</span> under high wind speed conditions.</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 <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> velocities are estimated for one year using a 1-D upper-ocean model (GOTM) and a modified version of the NOAA-COARE <span class="hlt">transfer</span> 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 exchange, respectively, are consistent with the global average <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> velocity of any gas, with appropriate treatment of the dependence on molecular properties including the strong solubility dependence of bubble-mediated <span class="hlt">transfer</span>. For example, an initial estimate of the global average <span class="hlt">transfer</span> 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/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> exchange, with the aim of identifying indices of ecosystem response to environmental changes. Data were analyzed to develop a non-steady-state carbon budget and an assessment of NCP against <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> 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('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 <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> 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/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/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> exchange, with the aim of documenting the ecosystem response to environmental changes. Data were analyzed to develop a non-steady-state carbon budget and an assessment of NCP against <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> 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('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 <span class="hlt">transferred</span> <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 <span class="hlt">transferred</span> <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 <span class="hlt">transferred</span> <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/2008AGUFMOS22B..07M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFMOS22B..07M"><span>Wintertime <span class="hlt">Air-Sea</span> Gas <span class="hlt">Transfer</span> 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 <span class="hlt">transfer</span> 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/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('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> </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/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('http://adsabs.harvard.edu/abs/2017GeoRL..4412324M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoRL..4412324M"><span>Enrichment of Extracellular Carbonic Anhydrase in the <span class="hlt">Sea</span> Surface Microlayer and Its Effect on <span class="hlt">Air-Sea</span> <span class="hlt">CO</span><span class="hlt">2</span> Exchange</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mustaffa, N. I. H.; Striebel, M.; Wurl, O.</p> <p>2017-12-01</p> <p>This paper describes the quantification of extracellular carbonic anhydrase (eCA) concentrations in the <span class="hlt">sea</span> surface microlayer (SML), the boundary layer between the ocean and the atmosphere of the Indo-West Pacific. We demonstrated that the SML is enriched with eCA by 1.5 ± 0.7 compared to the mixed underlying water. Enrichment remains up to a wind speed of 7 m s-1 (i.e., under typical oceanic conditions). As eCA catalyzes the interconversion of HCO3- and <span class="hlt">CO</span><span class="hlt">2</span>, it has been hypothesized that its enrichment in the SML enhances the <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange. We detected concentrations in the range of 0.12 to 0.76 n<fi>M</fi>, which can enhance the exchange by up to 15% based on the model approach described in the literature.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/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/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 <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> 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 exchange 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 exchange modulation at coastal waters. The results of the quantile regression analysis computed between FCO<span class="hlt">2</span> and (1) wind speed, (<span class="hlt">2</span>) significant wave height, (3) wave steepness and (4) water temperature, show that the significant wave height is the most correlated parameter with FCO<span class="hlt">2</span>; Nevertheless, the behavior of their relation varies along the probability distribution of FCO<span class="hlt">2</span>, with the linear regression</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1611343P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1611343P"><span>Surfactant control of <span class="hlt">air-sea</span> gas exchange across contrasting biogeochemical regimes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pereira, Ryan; Schneider-Zapp, Klaus; Upstill-Goddard, Robert</p> <p>2014-05-01</p> <p><span class="hlt">Air-sea</span> gas exchange is important to the global partitioning of <span class="hlt">CO</span><span class="hlt">2</span>.Exchange fluxes are products of an <span class="hlt">air-sea</span> gas concentration difference, ΔC, and a gas <span class="hlt">transfer</span> velocity, kw. The latter is controlled by the rate of turbulent diffusion at the <span class="hlt">air-sea</span> interface but it cannot be directly measured and has a high uncertainty that is now considered one of the greatest challenges to quantifying net global <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange ...(Takahashi et al., 2009). One important control on kw is exerted by <span class="hlt">sea</span> surface surfactants that arise both naturally from biological processes and through anthropogenic activity. They influence gas exchange in two fundamental ways: as a monolayer physical barrier and through modifying <span class="hlt">sea</span> surface hydrodynamics and hence turbulent energy <span class="hlt">transfer</span>. These effects have been demonstrated in the laboratory with artificial surfactants ...(Bock et al., 1999; Goldman et al., 1988) and through purposeful surfactant releases in coastal waters .(.).........().(Brockmann et al., 1982) and in the open ocean (Salter et al., 2011). Suppression of kwin these field experiments was ~5-55%. While changes in both total surfactant concentration and the composition of the natural surfactant pool might be expected to impact kw, the required in-situ studies are lacking. New data collected from the coastal North <span class="hlt">Sea</span> in 2012-2013 shows significant spatio-temporal variability in the surfactant activity of organic matter within the <span class="hlt">sea</span> surface microlayer that ranges from 0.07-0.94 mg/L T-X-100 (AC voltammetry). The surfactant activities show a strong winter/summer seasonal bias and general decrease in concentration with increasing distance from the coastline possibly associated with changing terrestrial vs. phytoplankton sources. Gas exchange experiments of this seawater using a novel laboratory tank and gas tracers (CH4 and SF6) demonstrate a 12-45% reduction in kw compared to surfactant-free water. Seasonally there is higher gas exchange suppression in the summer</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/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('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/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 <span class="hlt">transfer</span> 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('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('http://adsabs.harvard.edu/abs/2010AGUFM.C43E0586E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.C43E0586E"><span>Carbon Dioxide <span class="hlt">Transfer</span> 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 <span class="hlt">transfer</span> (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('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/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> exchange under steady state over a similar time scale. This assumption should be justified at the region with intensified upwelling where decoupling between upwelling and biological response may occur, where only water mass mixing and <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange should be accounted for. This presentation will also examine the seasonality of the <span class="hlt">CO</span><span class="hlt">2</span> dynamics and its controls.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007JMS....66..195F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007JMS....66..195F"><span>Application of new parameterizations of gas <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> velocities calculated using the popular wind-based k parameterizations by Wanninkhof [Wanninkhof, R., 1992. Relationship between wind speed and gas exchange 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> exchange and wind speed. Geophys. Res. Lett., 26(13): 1889-1892]. We show that despite good agreement of the globally averaged <span class="hlt">transfer</span> 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('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 <span class="hlt">transfer</span> laws, and thermodynamics of the atmosphere and ocean.</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 <span class="hlt">transferred</span> 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/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://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 exchange (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/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('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_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/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 Arctic is undergoing dramatic changes which cover the entire range of natural processes, from extreme increases in the temperatures of <span class="hlt">air</span>, soil, and water, to changes in the cryosphere, the biodiversity of Arctic waters, and land vegetation. Small changes in the largest marine carbon pool, the dissolved inorganic carbon pool, can have a profound impact on the carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) flux between the ocean and the atmosphere, and the feedback of this flux to climate. Knowledge of relevant processes in the Arctic <span class="hlt">seas</span> improves the evaluation and projection of carbon cycle dynamics under current conditions of rapid climate change. Investigation of the <span class="hlt">CO</span><span class="hlt">2</span> system in the outer shelf and continental slope waters of the Eurasian Arctic <span class="hlt">seas</span> (the Barents, Kara, Laptev, and East Siberian <span class="hlt">seas</span>) during 2006, 2007, and 2009 revealed a general trend in the surface water partial pressure of <span class="hlt">CO</span><span class="hlt">2</span> (p<span class="hlt">CO</span><span class="hlt">2</span>) distribution, which manifested as an increase in p<span class="hlt">CO</span><span class="hlt">2</span> values eastward. The existence of this trend was defined by different oceanographic and biogeochemical regimes in the western and eastern parts of the study area; the trend is likely increasing due to a combination of factors determined by contemporary change in the Arctic climate, each change in turn evoking a series of synergistic effects. A high-resolution in situ investigation of the carbonate system parameters of the four Arctic <span class="hlt">seas</span> was carried out in the warm season of 2007; this year was characterized by the next-to-lowest historic <span class="hlt">sea</span>-ice extent in the Arctic Ocean, on satellite record, to that date. The study showed the different responses of the seawater carbonate system to the environment changes in the western vs. the eastern Eurasian Arctic <span class="hlt">seas</span>. The large, open, highly productive water area in the northern Barents <span class="hlt">Sea</span> enhances atmospheric <span class="hlt">CO</span><span class="hlt">2</span> uptake. In contrast, the uptake of <span class="hlt">CO</span><span class="hlt">2</span> was strongly weakened in the outer shelf and slope waters of the East Siberian Arctic <span class="hlt">seas</span> under the 2007 environmental conditions</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012TCD.....6.1015R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012TCD.....6.1015R"><span>Ikaite crystals in melting <span class="hlt">sea</span> ice - implications for p<span class="hlt">CO</span><span class="hlt">2</span> and pH levels in Arctic surface waters</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rysgaard, S.; Glud, R. N.; Lennert, K.; Cooper, M.; Halden, N.; Leakey, R. J. G.; Hawthorne, F. C.; Barber, D.</p> <p>2012-03-01</p> <p>A major issue of Arctic marine science is to understand whether the Arctic Ocean is, or will be, a source or sink for <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange. This has been complicated by the recent discoveries of ikaite (Ca<span class="hlt">CO</span>3·6H<span class="hlt">2</span>O) in Arctic and Antarctic <span class="hlt">sea</span> ice, which indicate that multiple chemical transformations occur in <span class="hlt">sea</span> ice with a possible effect on <span class="hlt">CO</span><span class="hlt">2</span> and pH conditions in surface waters. Here we report on biogeochemical conditions, microscopic examinations and x-ray diffraction analysis of single crystals from an actively melting 1.7 km<span class="hlt">2</span> (0.5-1 m thick) drifting ice floe in the Fram Strait during summer. Our findings show that ikaite crystals are present throughout the <span class="hlt">sea</span> ice but with larger crystals appearing in the upper ice layers. Ikaite crystals placed at elevated temperatures gradually disintegrated into smaller crystallites and dissolved. During our field campaign in late June, melt reduced the ice flow thickness by ca. 0.<span class="hlt">2</span> m per week and resulted in an estimated 1.6 ppm decrease of p<span class="hlt">CO</span><span class="hlt">2</span> in the ocean surface mixed layer. This corresponds to an <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> uptake of 11 mmol m-<span class="hlt">2</span> <span class="hlt">sea</span> ice d-1 or to 3.5 ton km-<span class="hlt">2</span> ice floe week-1.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012BGD.....910331C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012BGD.....910331C"><span><span class="hlt">CO</span><span class="hlt">2</span> exchange in a temperate marginal <span class="hlt">sea</span> of the Mediterranean <span class="hlt">Sea</span>: processes and carbon budget</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cossarini, G.; Querin, S.; Solidoro, C.</p> <p>2012-08-01</p> <p>Marginal <span class="hlt">seas</span> play a potentially important role in the global carbon cycle; however, due to differences in the scales of variability and dynamics, marginal <span class="hlt">seas</span> are seldom fully accounted for in global models or estimates. Specific high-resolution studies may elucidate the role of marginal <span class="hlt">seas</span> and assist in the compilation of a complete global budget. In this study, we investigated the <span class="hlt">air-sea</span> exchange and the carbon cycle dynamics in a marginal sub-basin of the Mediterranean <span class="hlt">Sea</span> (the Adriatic <span class="hlt">Sea</span>) by adopting a coupled transport-biogeochemical model of intermediate complexity including carbonate dynamics. The Adriatic <span class="hlt">Sea</span> is a highly productive area owed to riverine fertilisation and is a site of intense dense water formation both on the northern continental shelf and in the southern sub-basin. Therefore, the study area may be an important site of <span class="hlt">CO</span><span class="hlt">2</span> sequestration in the Mediterranean <span class="hlt">Sea</span>. The results of the model simulation show that the Adriatic <span class="hlt">Sea</span>, as a whole, is a <span class="hlt">CO</span><span class="hlt">2</span> sink with a mean annual flux of 36 mg m-<span class="hlt">2</span> day-1. The northern part absorbs more carbon (68 mg m-<span class="hlt">2</span> day-1) due to an efficient continental shelf pump process, whereas the southern part behaves similar to an open ocean. Nonetheless, the Southern Adriatic <span class="hlt">Sea</span> accumulates dense, southward-flowing, carbon-rich water produced on the northern shelf. During a warm year and despite an increase in aquatic primary productivity, the sequestration of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> is reduced by approximately 15% due to alterations of the solubility pump and reduced dense water formation. The seasonal cycle of temperature and biological productivity modulates the efficiency of the carbon pump at the surface, whereas the intensity of winter cooling in the northern sub-basin leads to the export of C-rich dense water to the deep layer of the southern sub-basin and, subsequently, to the interior of the Mediterranean <span class="hlt">Sea</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19950045752&hterms=Parkinsons&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3DParkinsons','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19950045752&hterms=Parkinsons&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3DParkinsons"><span>The role of <span class="hlt">sea</span> ice in <span class="hlt">2</span> x <span class="hlt">CO</span><span class="hlt">2</span> climate model sensitivity. Part 1: The total influence of <span class="hlt">sea</span> ice thickness and extent</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rind, D.; Healy, R.; Parkinson, C.; Martinson, D.</p> <p>1995-01-01</p> <p>As a first step in investigating the effects of <span class="hlt">sea</span> ice changes on the climate sensitivity to doubled atmospheric <span class="hlt">CO</span><span class="hlt">2</span>, the authors use a standard simple <span class="hlt">sea</span> ice model while varying the <span class="hlt">sea</span> ice distributions and thicknesses in the control run. Thinner ice amplifies the atmospheric temperature senstivity in these experiments by about 15% (to a warming of 4.8 C), because it is easier for the thinner ice to be removed as the climate warms. Thus, its impact on sensitivity is similar to that of greater <span class="hlt">sea</span> ice extent in the control run, which provides more opportunity for <span class="hlt">sea</span> ice reduction. An experiment with <span class="hlt">sea</span> ice not allowed to change between the control and doubled <span class="hlt">CO</span><span class="hlt">2</span> simulations illustrates that the total effect of <span class="hlt">sea</span> ice on surface <span class="hlt">air</span> temperature changes, including cloud cover and water vapor feedbacks that arise in response to <span class="hlt">sea</span> ice variations, amounts to 37% of the temperature sensitivity to the <span class="hlt">CO</span><span class="hlt">2</span> doubling, accounting for 1.56 C of the 4.17 C global warming. This is about four times larger than the <span class="hlt">sea</span> ice impact when no feedbacks are allowed. The different experiments produce a range of results for southern high latitudes with the hydrologic budget over Antarctica implying <span class="hlt">sea</span> level increases of varying magnitude or no change. These results highlight the importance of properly constraining the <span class="hlt">sea</span> ice response to climate perturbations, necessitating the use of more realistic <span class="hlt">sea</span> ice and ocean models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012TCry....6..901R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012TCry....6..901R"><span>Ikaite crystals in melting <span class="hlt">sea</span> ice - implications for p<span class="hlt">CO</span><span class="hlt">2</span> and pH levels in Arctic surface waters</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rysgaard, S.; Glud, R. N.; Lennert, K.; Cooper, M.; Halden, N.; Leakey, R. J. G.; Hawthorne, F. C.; Barber, D.</p> <p>2012-08-01</p> <p>A major issue of Arctic marine science is to understand whether the Arctic Ocean is, or will be, a source or sink for <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange. This has been complicated by the recent discoveries of ikaite (a polymorph of Ca<span class="hlt">CO</span>3·6H<span class="hlt">2</span>O) in Arctic and Antarctic <span class="hlt">sea</span> ice, which indicate that multiple chemical transformations occur in <span class="hlt">sea</span> ice with a possible effect on <span class="hlt">CO</span><span class="hlt">2</span> and pH conditions in surface waters. Here, we report on biogeochemical conditions, microscopic examinations and x-ray diffraction analysis of single crystals from a melting 1.7 km<span class="hlt">2</span> (0.5-1 m thick) drifting ice floe in the Fram Strait during summer. Our findings show that ikaite crystals are present throughout the <span class="hlt">sea</span> ice but with larger crystals appearing in the upper ice layers. Ikaite crystals placed at elevated temperatures disintegrated into smaller crystallites and dissolved. During our field campaign in late June, melt reduced the ice floe thickness by 0.<span class="hlt">2</span> m per week and resulted in an estimated 3.8 ppm decrease of p<span class="hlt">CO</span><span class="hlt">2</span> in the ocean surface mixed layer. This corresponds to an <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> uptake of 10.6 mmol m-<span class="hlt">2</span> <span class="hlt">sea</span> ice d-1 or to 3.3 ton km-<span class="hlt">2</span> ice floe week-1. This is markedly higher than the estimated primary production within the ice floe of 0.3-1.3 mmol m-<span class="hlt">2</span> <span class="hlt">sea</span> ice d-1. Finally, the presence of ikaite in <span class="hlt">sea</span> ice and the dissolution of the mineral during melting of the <span class="hlt">sea</span> ice and mixing of the melt water into the surface oceanic mixed layer accounted for half of the estimated p<span class="hlt">CO</span><span class="hlt">2</span> uptake.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/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-exchange <span class="hlt">transfer</span> 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('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 <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> parameterizations at low wind speeds (<4 m s -1), which leads to underestimation of gas <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> velocity. We suggest therefore, that other factors like surfactants, rain or tidal current will have an impact on gas <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> parameterizations at low wind speeds (<4 m s -1), which leads to underestimation of gas <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> velocity. We suggest therefore, that other factors like surfactants, rain or tidal current will have an impact on gas <span class="hlt">transfer</span> parameterizations.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..1210133Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..1210133Z"><span><span class="hlt">Air-sea</span> fluxes of momentum and mass in the presence of wind waves</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zülicke, Christoph</p> <p>2010-05-01</p> <p>An <span class="hlt">air-sea</span> interaction model (ASIM) is developed including the effect of wind waves on momentum and mass <span class="hlt">transfer</span>. This includes the derivation of profiles of dissipation rate, flow speed and concentration from a certain height to a certain depth. Simplified assumptions on the turbulent closure, skin - bulk matching and the spectral wave model allow for an analytic treatment. Particular emphasis was put on the inclusion of primary (gravity) waves and secondary (capillary-gravity) waves. The model was tuned to match wall-flow theory and data on wave height and slope. Growing waves reduce the <span class="hlt">air</span>-side turbulent stress and lead to an increasing drag coefficient. In the <span class="hlt">sea</span>, breaking waves inject turbulent kinetic energy and accelerate the <span class="hlt">transfer</span>. Cross-reference with data on wave-related momentum and energy flux, dissipation rate and <span class="hlt">transfer</span> velocity was sufficient. The evaluation of ASIM allowed for the analytical calculation of bulk formulae for the wind-dependent gas <span class="hlt">transfer</span> velocity including information on the <span class="hlt">air</span>-side momentum <span class="hlt">transfer</span> (drag coefficient) and the <span class="hlt">sea</span>-side gas <span class="hlt">transfer</span> (Dalton number). The following regimes have been identified: the smooth waveless regime with a <span class="hlt">transfer</span> velocity proportional to (wind) × (diffusion)<span class="hlt">2</span>-3, the primary wave regime with a wind speed dependence proportional to (wind)1-4 × (diffusion)1-<span class="hlt">2</span>-(waveage)1-4 and the secondary wave regime including a more-than-linear wind speed dependence like (wind)15-8 × (diffusion)1-<span class="hlt">2</span> × (waveage)5-8. These findings complete the current understanding of <span class="hlt">air-sea</span> interaction for medium winds between <span class="hlt">2</span> and 20 m s^-1.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/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 <span class="hlt">transfer</span> 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('https://pubs.er.usgs.gov/publication/70102289','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70102289"><span><span class="hlt">Air</span>-water gas exchange and <span class="hlt">CO</span><span class="hlt">2</span> 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 <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> velocity results are consistent with turbulent kinetic energy dissipation measurements, indicating a higher rate of turbulence and gas exchange than predicted by commonly used wind speed/gas exchange parameterizations. The results have important implications for carbon fluxes in mangrove ecosystems.</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/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 <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> 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 exchange with no impact from <span class="hlt">air</span>-ice gas exchange.</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('https://eric.ed.gov/?q=chemical+AND+engineering+AND+reactions&pg=5&id=EJ945561','ERIC'); return false;" href="https://eric.ed.gov/?q=chemical+AND+engineering+AND+reactions&pg=5&id=EJ945561"><span>Combining Experiments and Simulation of Gas Absorption for Teaching Mass <span class="hlt">Transfer</span> Fundamentals: Removing <span class="hlt">CO</span><span class="hlt">2</span> from <span class="hlt">Air</span> Using Water and NaOH</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>Clark, William M.; Jackson, Yaminah Z.; Morin, Michael T.; Ferraro, Giacomo P.</p> <p>2011-01-01</p> <p>Laboratory experiments and computer models for studying the mass <span class="hlt">transfer</span> process of removing <span class="hlt">CO</span><span class="hlt">2</span> from <span class="hlt">air</span> using water or dilute NaOH solution as absorbent are presented. Models tie experiment to theory and give a visual representation of concentration profiles and also illustrate the two-film theory and the relative importance of various…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA628532','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA628532"><span><span class="hlt">Air/Sea</span> <span class="hlt">Transfer</span> of Gases and Aerosols</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>of tubing from the boom at the western end of the pier. The boom housed the inlet and a Campbell CSAT sonic anemometer, which measured three...with the return flow from breaking waves onshore. 0 5 10 15 20 25 30 35 40 45 50 0 1 <span class="hlt">2</span> 3 4 5 6 7 U10 (m/s) k 6 00 (c m /h r ) this study wanninkof...ultimately result in improved algorithms relating the state of the <span class="hlt">air/sea</span> interface to remotely sensed properties. REFERENCES Bandy, A, R ., D</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19850060100&hterms=Radon&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3DRadon','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19850060100&hterms=Radon&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3DRadon"><span>Gas exchange and <span class="hlt">CO</span><span class="hlt">2</span> 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://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('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> </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('https://www.ncbi.nlm.nih.gov/pubmed/23589251','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23589251"><span>The distribution and <span class="hlt">sea-air</span> <span class="hlt">transfer</span> of volatile mercury in waste post-desulfurization seawater discharged from a coal-fired power plant.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sun, Lumin; Lin, Shanshan; Feng, Lifeng; Huang, Shuyuan; Yuan, Dongxing</p> <p>2013-09-01</p> <p>The waste seawater discharged in coastal areas from coal-fired power plants equipped with a seawater desulfurization system might carry pollutants such as mercury from the flue gas into the adjacent <span class="hlt">seas</span>. However, only very limited impact studies have been carried out. Taking a typical plant in Xiamen as an example, the present study targeted the distribution and <span class="hlt">sea-air</span> <span class="hlt">transfer</span> flux of volatile mercury in seawater, in order to trace the fate of the discharged mercury other than into the sediments. Samples from 28 sampling sites were collected in the <span class="hlt">sea</span> area around two discharge outlets of the plant, daily and seasonally. Total mercury, dissolved gaseous mercury and dissolved total mercury in the seawater, as well as gaseous elemental mercury above the <span class="hlt">sea</span> surface, were investigated. Mean concentrations of dissolved gaseous mercury and gaseous elemental mercury in the area were 183 and 4.48 ng m(-3) in summer and 116 and 3.92 ng m(-3) in winter, which were significantly higher than those at a reference site. Based on the flux calculation, the <span class="hlt">transfer</span> of volatile mercury was from the <span class="hlt">sea</span> surface into the atmosphere, and more than 4.4 kg mercury, accounting for at least <span class="hlt">2.2</span> % of the total discharge amount of the coal-fired power plant in the sampling area (1 km(<span class="hlt">2</span>)), was emitted to the <span class="hlt">air</span> annually. This study strongly suggested that besides being deposited into the sediment and diluted with seawater, emission into the atmosphere was an important fate for the mercury from the waste seawater from coal-fired power plants.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21141036','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21141036"><span>Advances in quantifying <span class="hlt">air-sea</span> gas exchange and environmental forcing.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wanninkhof, Rik; Asher, William E; Ho, David T; Sweeney, Colm; McGillis, Wade R</p> <p>2009-01-01</p> <p>The past decade has seen a substantial amount of research on <span class="hlt">air-sea</span> gas exchange and its environmental controls. These studies have significantly advanced the understanding of processes that control gas <span class="hlt">transfer</span>, 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 <span class="hlt">transfer</span> and recent developments in gas <span class="hlt">transfer</span> theory, parameterizations, and measurement techniques in the context of the exchange of carbon dioxide. However, much of this discussion is applicable to any sparingly soluble, non-reactive gas. We show how the use of global variables of environmental forcing that have recently become available and gas exchange relationships that incorporate the main forcing factors will lead to improved estimates of global and regional <span class="hlt">air-sea</span> gas fluxes based on better fundamental physical, chemical, and biological foundations.</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 exchange between the <span class="hlt">air</span> and <span class="hlt">sea</span> in the Bay of Bengal is an important driver of atmospheric convection during the Asian Monsoon. Warm <span class="hlt">sea</span> surface temperatures resulting from salinity stratified shallow mixed layers trigger widespread showers and thunderstorms. In this study, we compare atmospheric reanalysis 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 <span class="hlt">transfer</span>, upper ocean stratification, and ocean surface temperature and salinity.</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/2013TCD.....7.6075R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013TCD.....7.6075R"><span>Dynamic ikaite production and dissolution in <span class="hlt">sea</span> ice - control by temperature, salinity and p<span class="hlt">CO</span><span class="hlt">2</span> conditions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rysgaard, S.; Wang, F.; Galley, R. J.; Grimm, R.; Lemes, M.; Geilfus, N.-X.; Chaulk, A.; Hare, A. A.; Crabeck, O.; Else, B. G. T.; Campbell, K.; Papakyriakou, T.; Sørensen, L. L.; Sievers, J.; Notz, D.</p> <p>2013-12-01</p> <p>Ikaite is a hydrous calcium carbonate mineral (Ca<span class="hlt">CO</span>3 · 6H<span class="hlt">2</span>O). It is only found in a metastable state, and decomposes rapidly once removed from near-freezing water. Recently, ikaite crystals have been found in <span class="hlt">sea</span> ice and it has been suggested that their precipitation may play an important role in <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange in ice-covered <span class="hlt">seas</span>. Little is known, however, of the spatial and temporal dynamics of ikaite in <span class="hlt">sea</span> ice. Here we present evidence for highly dynamic ikaite precipitation and dissolution in <span class="hlt">sea</span> ice grown at an out-door pool of the <span class="hlt">Sea</span>-ice Environmental Research Facility (SERF). During the experiment, ikaite precipitated in <span class="hlt">sea</span> ice with temperatures below -3 °C, creating three distinct zones of ikaite concentrations: (1) a mm to cm thin surface layer containing frost flowers and brine skim with bulk concentrations of > 2000 μmol kg-1, (<span class="hlt">2</span>) an internal layer with concentrations of 200-400 μmol kg-1 and (3) a~bottom layer with concentrations of < 100 μmol kg-1. Snowfall events caused the <span class="hlt">sea</span> ice to warm, dissolving ikaite crystals under acidic conditions. Manual removal of the snow cover allowed the <span class="hlt">sea</span> ice to cool and brine salinities to increase, resulting in rapid ikaite precipitation. The modeled (FREZCHEM) ikaite concentrations were in the same order of magnitude as observations and suggest that ikaite concentration in <span class="hlt">sea</span> ice increase with decreasing temperatures. Thus, varying snow conditions may play a key role in ikaite precipitation and dissolution in <span class="hlt">sea</span> ice. This will have implications for <span class="hlt">CO</span><span class="hlt">2</span> exchange with the atmosphere and ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/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> exchange. Our measurements confirm previous laboratory findings that growing young <span class="hlt">sea</span> ice acts as a source of <span class="hlt">CO</span><span class="hlt">2</span> to the atmosphere. Ca<span class="hlt">CO</span>3 precipitation during early ice growth appears to promote the release of <span class="hlt">CO</span><span class="hlt">2</span> to the atmosphere; however, its contribution to the overall release by newly formed ice is most likely minor.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/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> <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('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1080410','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1080410"><span>Growth Kinetics, Carbohydrate, and Leaf Phosphate Content of Clover (Trifolium subterraneum L.) after <span class="hlt">Transfer</span> to a High <span class="hlt">CO</span><span class="hlt">2</span> Atmosphere or to High Light and Ambient <span class="hlt">Air</span> 1</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Morin, Francoise; André, Marcel; Betsche, Thomas</p> <p>1992-01-01</p> <p>Intact <span class="hlt">air</span>-grown (photosynthetic photon flux density, 400 microeinsteins per square meter per second) clover plants (Trifolium subterraneum L.) were <span class="hlt">transfered</span> to high <span class="hlt">CO</span><span class="hlt">2</span> (4000 microliters <span class="hlt">CO</span><span class="hlt">2</span> per liter; photosynthetic photon flux density, 400 microeinsteins per square meter per second) or to high light (340 microliters <span class="hlt">CO</span><span class="hlt">2</span> per liter; photosynthetic photon flux density, 800 microeinsteins per square meter per second) to similarly stimulate photosynthetic net <span class="hlt">CO</span><span class="hlt">2</span> uptake. The daily increment of net <span class="hlt">CO</span><span class="hlt">2</span> uptake declined transiently in high <span class="hlt">CO</span><span class="hlt">2</span>, but not in high light, below the values in <span class="hlt">air</span>/standard light. After about 3 days in high <span class="hlt">CO</span><span class="hlt">2</span>, the daily increment of net <span class="hlt">CO</span><span class="hlt">2</span> uptake increased but did not reach the high light values. Nightly <span class="hlt">CO</span><span class="hlt">2</span> release increased immediately in high light, whereas there was a 3-day lag phase in high <span class="hlt">CO</span><span class="hlt">2</span>. During this time, starch accumulated to a high level, and leaf deterioration was observed only in high <span class="hlt">CO</span><span class="hlt">2</span>. After 12 days, starch was two- to threefold higher in high <span class="hlt">CO</span><span class="hlt">2</span> than in high light, whereas sucrose was similar. Leaf carbohydrates were determined during the first and fourth day in high <span class="hlt">CO</span><span class="hlt">2</span>. Starch increased rapidly throughout the day. Early in the day, sucrose was low and similar in high <span class="hlt">CO</span><span class="hlt">2</span> and ambient <span class="hlt">air</span> (same light). Later, sucrose increased considerably in high <span class="hlt">CO</span><span class="hlt">2</span>. The findings that (a) much more photosynthetic carbon was partitioned into the leaf starch pool in high <span class="hlt">CO</span><span class="hlt">2</span> than in high light, although net <span class="hlt">CO</span><span class="hlt">2</span> uptake was similar, and that (b) rapid starch formation occurred in high <span class="hlt">CO</span><span class="hlt">2</span> even when leaf sucrose was only slightly elevated suggest that low sink capacity was not the main constraint in high <span class="hlt">CO</span><span class="hlt">2</span>. It is proposed that carbon partitioning between starch (chloroplast) and sucrose (cytosol) was perturbed by high <span class="hlt">CO</span><span class="hlt">2</span> because of the lack of photorespiration. Total phosphate pools were determined in leaves. Concentrations based on fresh weight of orthophosphate, soluble esterified phosphate, and total phosphate markedly declined</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/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('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 <span class="hlt">transfer</span> 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> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFMOS11C1660Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMOS11C1660Z"><span>On the relationships of gas <span class="hlt">transfer</span> velocity with turbulent kinetic energy dissipation rate and wind waves</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhao, D.</p> <p>2012-12-01</p> <p>The exchange of carbon dioxide across the <span class="hlt">air-sea</span> interface is an important component of the atmospheric <span class="hlt">CO</span><span class="hlt">2</span> budget. Understanding how future changes in climate will affect oceanic uptake and releaser <span class="hlt">CO</span><span class="hlt">2</span> requires accurate estimation of <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> flux. This flux is typically expressed as the product of gas <span class="hlt">transfer</span> velocity, <span class="hlt">CO</span><span class="hlt">2</span> partial pressure difference in seawater and <span class="hlt">air</span>, and the <span class="hlt">CO</span><span class="hlt">2</span> solubility. As the key parameter, gas <span class="hlt">transfer</span> velocity has long been known to be controlled by the near-surface turbulence in water, which is affected by many factors, such as wind forcing, ocean waves, water-side convection and rainfall. Although the wind forcing is believed as the major factor dominating the near-surface turbulence, many studies have shown that the wind waves and their breaking would greatly enhance turbulence compared with the classical solid wall theory. Gas <span class="hlt">transfer</span> velocity has been parameterized in terms of wind speed, turbulent kinetic energy dissipation rate, and wave parameters on the basis of observational data or theoretical analysis. However, great discrepancies, as large as one order, exist among these formulas. In this study, we will systematically analyze the differences of gas <span class="hlt">transfer</span> velocity proposed so far, and try to find the reason that leads to their uncertainties. Finally, a new formula for gas <span class="hlt">transfer</span> velocity will be given in terms of wind speed and wind wave parameter.</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 <span class="hlt">transfer</span> 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('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 <span class="hlt">transfer</span> 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('http://adsabs.harvard.edu/abs/1998WRR....34.3245B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1998WRR....34.3245B"><span><span class="hlt">Air</span> sparging: <span class="hlt">Air</span>-water mass <span class="hlt">transfer</span> coefficients</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Braida, Washington J.; Ong, Say Kee</p> <p>1998-12-01</p> <p>Experiments investigating the mass <span class="hlt">transfer</span> of several dissolved volatile organic compounds (VOCs) across the <span class="hlt">air</span>-water interface were conducted using a single-<span class="hlt">air</span>- channel <span class="hlt">air</span>-sparging system. Three different porous media were used in the study. <span class="hlt">Air</span> velocities ranged from 0.<span class="hlt">2</span> cm s-1 to <span class="hlt">2</span>.5 cm s-1. The tortuosity factor for each porous medium and the <span class="hlt">air</span>-water mass <span class="hlt">transfer</span> coefficients were estimated by fitting experimental data to a one-dimensional diffusion model. The estimated mass <span class="hlt">transfer</span> coefficients KG ranged from 1.79 × 10-3 cm min-1 to 3.85 × 10-<span class="hlt">2</span> cm min-1. The estimated lumped gas phase mass <span class="hlt">transfer</span> coefficients KGa were found to be directly related to the <span class="hlt">air</span> diffusivity of the VOC, <span class="hlt">air</span> velocity, and particle size, and inversely related to the Henry's law constant of the VOCs. Of the four parameters investigated, the parameter that controlled or had a dominant effect on the lumped gas phase mass <span class="hlt">transfer</span> coefficient was the <span class="hlt">air</span> diffusivity of the VOC. Two empirical models were developed by correlating the Damkohler and the modified <span class="hlt">air</span> phase Sherwood numbers with the <span class="hlt">air</span> phase Peclet number, Henry's law constant, and the reduced mean particle size of porous media. The correlation developed in this study may be used to obtain better predictions of mass <span class="hlt">transfer</span> fluxes for field conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25103722','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25103722"><span>First day of an oil spill on the open <span class="hlt">sea</span>: early mass <span class="hlt">transfers</span> of hydrocarbons to <span class="hlt">air</span> and water.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gros, Jonas; Nabi, Deedar; Würz, Birgit; Wick, Lukas Y; Brussaard, Corina P D; Huisman, Johannes; van der Meer, Jan R; Reddy, Christopher M; Arey, J Samuel</p> <p>2014-08-19</p> <p>During the first hours after release of petroleum at <span class="hlt">sea</span>, crude oil hydrocarbons partition rapidly into <span class="hlt">air</span> and water. However, limited information is available about very early evaporation and dissolution processes. We report on the composition of the oil slick during the first day after a permitted, unrestrained 4.3 m(3) oil release conducted on the North <span class="hlt">Sea</span>. Rapid mass <span class="hlt">transfers</span> of volatile and soluble hydrocarbons were observed, with >50% of ≤C17 hydrocarbons disappearing within 25 h from this oil slick of <10 km(<span class="hlt">2</span>) area and <10 μm thickness. For oil sheen, >50% losses of ≤C16 hydrocarbons were observed after 1 h. We developed a mass <span class="hlt">transfer</span> model to describe the evolution of oil slick chemical composition and water column hydrocarbon concentrations. The model was parametrized based on environmental conditions and hydrocarbon partitioning properties estimated from comprehensive two-dimensional gas chromatography (GC×GC) retention data. The model correctly predicted the observed fractionation of petroleum hydrocarbons in the oil slick resulting from evaporation and dissolution. This is the first report on the broad-spectrum compositional changes in oil during the first day of a spill at the <span class="hlt">sea</span> surface. Expected outcomes under other environmental conditions are discussed, as well as comparisons to other models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PrOce.141..153Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PrOce.141..153Z"><span>The impact of dissolved organic carbon and bacterial respiration on p<span class="hlt">CO</span><span class="hlt">2</span> in experimental <span class="hlt">sea</span> ice</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhou, J.; Kotovitch, M.; Kaartokallio, H.; Moreau, S.; Tison, J.-L.; Kattner, G.; Dieckmann, G.; Thomas, D. N.; Delille, B.</p> <p>2016-02-01</p> <p>Previous observations have shown that the partial pressure of carbon dioxide (p<span class="hlt">CO</span><span class="hlt">2</span>) in <span class="hlt">sea</span> ice brines is generally higher in Arctic <span class="hlt">sea</span> ice compared to those from the Antarctic <span class="hlt">sea</span> ice, especially in winter and early spring. We hypothesized that these differences result from the higher dissolved organic carbon (DOC) content in Arctic seawater: Higher concentrations of DOC in seawater would be reflected in a greater DOC incorporation into <span class="hlt">sea</span> ice, enhancing bacterial respiration, which in turn would increase the p<span class="hlt">CO</span><span class="hlt">2</span> in the ice. To verify this hypothesis, we performed an experiment using two series of mesocosms: one was filled with seawater (SW) and the other one with seawater with an addition of filtered humic-rich river water (SWR). The addition of river water increased the DOC concentration of the water from a median of 142 μmol Lwater-1 in SW to 249 μmol Lwater-1 in SWR. <span class="hlt">Sea</span> ice was grown in these mesocosms under the same physical conditions over 19 days. Microalgae and protists were absent, and only bacterial activity has been detected. We measured the DOC concentration, bacterial respiration, total alkalinity and p<span class="hlt">CO</span><span class="hlt">2</span> in <span class="hlt">sea</span> ice and the underlying seawater, and we calculated the changes in dissolved inorganic carbon (DIC) in both media. We found that bacterial respiration in ice was higher in SWR: median bacterial respiration was 25 nmol C Lice-1 h-1 compared to 10 nmol C Lice-1 h-1 in SW. p<span class="hlt">CO</span><span class="hlt">2</span> in ice was also higher in SWR with a median of 430 ppm compared to 356 ppm in SW. However, the differences in p<span class="hlt">CO</span><span class="hlt">2</span> were larger within the ice interiors than at the surfaces or the bottom layers of the ice, where exchanges at the <span class="hlt">air</span>-ice and ice-water interfaces might have reduced the differences. In addition, we used a model to simulate the differences of p<span class="hlt">CO</span><span class="hlt">2</span> and DIC based on bacterial respiration. The model simulations support the experimental findings and further suggest that bacterial growth efficiency in the ice might approach 0.15 and 0.<span class="hlt">2</span>. It is thus credible</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://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> </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.osti.gov/biblio/1252848-measuring-nitrous-oxide-mass-transfer-non-aqueous-co2bol-co2-capture-solvents','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1252848-measuring-nitrous-oxide-mass-transfer-non-aqueous-co2bol-co2-capture-solvents"><span>Measuring Nitrous Oxide Mass <span class="hlt">Transfer</span> into Non-Aqueous <span class="hlt">CO</span><span class="hlt">2</span>BOL <span class="hlt">CO</span><span class="hlt">2</span> Capture Solvents</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>Whyatt, Greg A.; Freeman, Charles J.; Zwoster, Andy</p> <p>2016-03-28</p> <p>This paper investigates <span class="hlt">CO</span><span class="hlt">2</span> absorption behavior in <span class="hlt">CO</span><span class="hlt">2</span>BOL solvents by decoupling the physical and chemical effects using N<span class="hlt">2</span>O as a non-reactive mimic. Absorption measurements were performed using a wetted-wall contactor. Testing was performed using a “first generation” <span class="hlt">CO</span><span class="hlt">2</span> binding organic liquid (<span class="hlt">CO</span><span class="hlt">2</span>BOL), comprised of an independent base and alcohol. Measurements were made with N<span class="hlt">2</span>O at a lean (0.06 mol <span class="hlt">CO</span><span class="hlt">2</span>/mol BOL) and rich (0.26 mol <span class="hlt">CO</span><span class="hlt">2</span>/mol BOL) loading, each at three temperatures (35, 45 and 55 °C). Liquid-film mass <span class="hlt">transfer</span> coefficients (kg') were calculated by subtracting the gas film resistance – determined from a correlation from literature – from themore » overall mass <span class="hlt">transfer</span> measurement. The resulting kg' values for N<span class="hlt">2</span>O in <span class="hlt">CO</span><span class="hlt">2</span>BOLs were found to be higher than that of 5 M aqueous MEA under comparable conditions, which is supported by published measurements of Henry’s coefficients for N<span class="hlt">2</span>O in various solvents. These results suggest that the physical solubility contribution for <span class="hlt">CO</span><span class="hlt">2</span> absorption in <span class="hlt">CO</span><span class="hlt">2</span>BOLs is greater than that of aqueous amines, an effect that may pertain to other non-aqueous solvents.« less</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://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 exchange. 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('http://adsabs.harvard.edu/abs/2016AGUOSPO34A3029C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSPO34A3029C"><span>Comparison of seawater <span class="hlt">CO</span><span class="hlt">2</span> system in summer between the East China <span class="hlt">Sea</span> shelf and the Peter the Great Bay of the Japan (East) <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chuang, K. Y.; Tishchenko, P. Y.; Gong, G. C.; Chou, W. C.; Tishchenko, P. P.; Shkirnikova, E. M.</p> <p>2016-02-01</p> <p>Continental shelves are active sites of <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange and represent an important component of the global carbon budget. In this study, we investigated the <span class="hlt">CO</span><span class="hlt">2</span> system and pertinent hydrographic parameters in two distinct continental shelf systems in the Northwest Pacific in summer 2014: the East China <span class="hlt">Sea</span> shelf (ECSS) and the Peter the Great Bay (PGB) of the Japan/East <span class="hlt">Sea</span>. The results show that the average temperature, pH, chlorophyll a and nutrients in the ECSS are higher, but salinity, dissolved inorganic carbon, and fugacity of <span class="hlt">CO</span><span class="hlt">2</span> are lower than those in the PGB. Meanwhile, the ECSS acted as a sink of atmospheric <span class="hlt">CO</span><span class="hlt">2</span>, but the PGB was a source. We suggest that the observed divergent behaviors in terms of <span class="hlt">CO</span><span class="hlt">2</span> absorption between the ECSS and the PGB may be associated with their difference in riverine runoff. Under the influence of the Yangtze River, the nutrient discharge into the ECSS is much higher than that into the PGB, where only a few small rivers empty into. The high nutrient discharge into the ECSS may stimulate high biological production, which may drawdown <span class="hlt">CO</span><span class="hlt">2</span> and thereby driving the ECSS to act as a <span class="hlt">CO</span><span class="hlt">2</span> sink despite high temperature in summer. On the contrary, the warming effect may dominate over the effect of biological production in the PGB due to the limited nutrient discharge, and thus turn the PGB to be a source of atmospheric <span class="hlt">CO</span><span class="hlt">2</span>. The results of this study imply that riverine nutrient discharge may exert a large control on net ecosystem productivity in shelf areas, which may subsequently play a critical role on determining whether a shelf system acts as a source or a sink of atmospheric <span class="hlt">CO</span><span class="hlt">2</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1714679M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1714679M"><span>Carbon speciation at the <span class="hlt">air-sea</span> interface during rain</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>McGillis, Wade; Hsueh, Diana; Takeshita, Yui; Donham, Emily; Markowitz, Michele; Turk, Daniela; Martz, Todd; Price, Nicole; Langdon, Chris; Najjar, Raymond; Herrmann, Maria; Sutton, Adrienne; Loose, Brice; Paine, Julia; Zappa, Christopher</p> <p>2015-04-01</p> <p>This investigation demonstrates the surface ocean dilution during rain events on the ocean and quantifies the lowering of surface p<span class="hlt">CO</span><span class="hlt">2</span> affecting the <span class="hlt">air-sea</span> exchange of carbon dioxide. Surface salinity was measured during rain events in Puerto Rico, the Florida Keys, East Coast USA, Panama, and the Palmyra Atoll. End-member analysis is used to determine the subsequent surface ocean carbonate speciation. Surface ocean carbonate chemistry was measured during rain events to verify any approximations made. The physical processes during rain (cold, fresh water intrusion and buoyancy, surface waves and shear, microscale mixing) are described. The role of rain on surface mixing, biogeochemistry, and <span class="hlt">air-sea</span> gas exchange will be discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('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> Exchange 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> Exchange Monitoring System (A-SEMS). EXPERIMENTAL SET-UP In a first look, the <span class="hlt">Air-Sea</span> Exchange...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 <span class="hlt">transferring</span> 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/2006GeoRL..3314803Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006GeoRL..3314803Z"><span>Impacts of winter storms on <span class="hlt">air-sea</span> gas exchange</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, Weiqing; Perrie, Will; Vagle, Svein</p> <p>2006-07-01</p> <p>The objective of this study is to investigate <span class="hlt">air-sea</span> gas exchange during winter storms, using field measurements from Ocean Station Papa in the Northeast Pacific (50°N, 145°W). We show that increasing gas <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> velocity during the peaks of the storms, increasing the flux rates by up to 20%. Gas <span class="hlt">transfer</span> 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/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 exchange 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 <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span>, the temperature difference, ΔT, across the thermal molecular boundary layer (cool skin of the ocean) and the interfacial gas <span class="hlt">transfer</span> 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 exchange. 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 exchange can be extended to the global scale, using remote sensing techniques.</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> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27450088','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27450088"><span>Inhibited proton <span class="hlt">transfer</span> enhances Au-catalyzed <span class="hlt">CO</span><span class="hlt">2</span>-to-fuels selectivity.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wuttig, Anna; Yaguchi, Momo; Motobayashi, Kenta; Osawa, Masatoshi; Surendranath, Yogesh</p> <p>2016-08-09</p> <p><span class="hlt">CO</span><span class="hlt">2</span> reduction in aqueous electrolytes suffers efficiency losses because of the simultaneous reduction of water to H<span class="hlt">2</span> We combine in situ surface-enhanced IR absorption spectroscopy (SEIRAS) and electrochemical kinetic studies to probe the mechanistic basis for kinetic bifurcation between H<span class="hlt">2</span> and <span class="hlt">CO</span> production on polycrystalline Au electrodes. Under the conditions of <span class="hlt">CO</span><span class="hlt">2</span> reduction catalysis, electrogenerated <span class="hlt">CO</span> species are irreversibly bound to Au in a bridging mode at a surface coverage of ∼0.<span class="hlt">2</span> and act as kinetically inert spectators. Electrokinetic data are consistent with a mechanism of <span class="hlt">CO</span> production involving rate-limiting, single-electron <span class="hlt">transfer</span> to <span class="hlt">CO</span><span class="hlt">2</span> with concomitant adsorption to surface active sites followed by rapid one-electron, two-proton <span class="hlt">transfer</span> and <span class="hlt">CO</span> liberation from the surface. In contrast, the data suggest an H<span class="hlt">2</span> evolution mechanism involving rate-limiting, single-electron <span class="hlt">transfer</span> coupled with proton <span class="hlt">transfer</span> from bicarbonate, hydronium, and/or carbonic acid to form adsorbed H species followed by rapid one-electron, one-proton, or H recombination reactions. The disparate proton coupling requirements for <span class="hlt">CO</span> and H<span class="hlt">2</span> production establish a mechanistic basis for reaction selectivity in electrocatalytic fuel formation, and the high population of spectator <span class="hlt">CO</span> species highlights the complex heterogeneity of electrode surfaces under conditions of fuel-forming electrocatalysis.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016QuRes..85...87C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016QuRes..85...87C"><span>Variability of 14C reservoir age and <span class="hlt">air-sea</span> 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('https://www.osti.gov/biblio/1355087-measuring-co-mass-transfer-gap-co-capture-solvents-varied-water-loadings','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1355087-measuring-co-mass-transfer-gap-co-capture-solvents-varied-water-loadings"><span>Measuring <span class="hlt">CO</span> <span class="hlt">2</span> and N <span class="hlt">2</span> O Mass <span class="hlt">Transfer</span> into GAP-1 <span class="hlt">CO</span> <span class="hlt">2</span> –Capture Solvents at Varied Water Loadings</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>Whyatt, Greg A.; Zwoster, Andy; Zheng, Feng</p> <p></p> <p>This paper investigates the <span class="hlt">CO</span> <span class="hlt">2</span> and N <span class="hlt">2</span> O absorption behavior in the water-lean gamma amino propyl (GAP)-1/TEG solvent system using a wetted-wall contactor. Testing was performed on a blend of GAP-1 aminosilicone in triethylene glycol at varied water loadings in the solvent. Measurements were made with <span class="hlt">CO</span> <span class="hlt">2</span> and N <span class="hlt">2</span> O at representative lean (0.04 mol <span class="hlt">CO</span> <span class="hlt">2</span>/mol alkalinity), middle (0.13 mol <span class="hlt">CO</span> <span class="hlt">2</span> /mol alkalinity) and rich (0.46 mol <span class="hlt">CO</span> <span class="hlt">2</span> /mol alkalinity) solvent loadings at 0, 5, 10 and 15 wt% water loadings at 40, 60 and 80C° and N <span class="hlt">2</span> O at (0.08-0.09 molmore » <span class="hlt">CO</span> <span class="hlt">2</span> /mol alkalinity) at 5 wt% water at 40, 60 and 80C°. <span class="hlt">CO</span> <span class="hlt">2</span> flux was found to be non-linear with respect to log mean pressure driving force (LMPD). Liquid-film mass <span class="hlt">transfer</span> coefficients (k'g) were calculated by subtracting the gas film resistance (determined from a correlation from literature) from the overall mass <span class="hlt">transfer</span> measurement. The resulting k'g values for <span class="hlt">CO</span> <span class="hlt">2</span> and N <span class="hlt">2</span> O in GAP-1/TEG mixtures were found to be higher than that of 5M aqueous monoethanolamine under comparable driving force albeit at higher solvent viscosities. The k'g values for <span class="hlt">CO</span> <span class="hlt">2</span> were also found to decrease with increasing solvent water content and increase with a decrease in temperature. These observations indicate that mass <span class="hlt">transfer</span> of <span class="hlt">CO</span> <span class="hlt">2</span> in GAP-1/TEG is linked to the physical solubility of <span class="hlt">CO</span> <span class="hlt">2</span> , which is higher in organic solvents compared to water. This paper expands on the understanding of the unique mass <span class="hlt">transfer</span> behavior and kinetics of <span class="hlt">CO</span> <span class="hlt">2</span> capture in water-lean solvents.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JQSRT.197...45Q','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JQSRT.197...45Q"><span>Calculations of thermal radiation <span class="hlt">transfer</span> of C<span class="hlt">2</span>H<span class="hlt">2</span> and C<span class="hlt">2</span>H4 together with H<span class="hlt">2</span>O, <span class="hlt">CO</span><span class="hlt">2</span>, and <span class="hlt">CO</span> in a one-dimensional enclosure using LBL and SNB models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Qi, Chaobo; Zheng, Shu; Zhou, Huaichun</p> <p>2017-08-01</p> <p>Generally, the involvement of hydrocarbons such as C<span class="hlt">2</span>H4 and its derivative C<span class="hlt">2</span>H<span class="hlt">2</span> in thermal radiation has not been accounted in the numerical simulation of their flames, which may cause serious error for estimation of temperature in the early stage of combustion. At the first, the Statistical Narrow-Band (SNB) model parameters for C<span class="hlt">2</span>H<span class="hlt">2</span> and C<span class="hlt">2</span>H4 are generated from line by line (LBL) calculations. The distributions of the concentrations of radiating gases such as H<span class="hlt">2</span>O, <span class="hlt">CO</span><span class="hlt">2</span>, <span class="hlt">CO</span>, C<span class="hlt">2</span>H<span class="hlt">2</span> and C<span class="hlt">2</span>H4, and the temperature along the centerline of a laminar ethylene/<span class="hlt">air</span> diffusion flame were chosen to form a one-dimensional, planar enclosure to be tested in this study. Thermal radiation <span class="hlt">transfer</span> in such an enclosure was calculated using the LBL approach and the SNB model, most of the relative errors are less than 8% and the results of these two models shows an excellent agreement. Below the height of 20 mm, which is the early stage of the flame, the average fraction contributed by C<span class="hlt">2</span>H<span class="hlt">2</span> and C<span class="hlt">2</span>H4 in the radiative heat source is 33.8%, while that by <span class="hlt">CO</span> is only 5.8%. This result indicates that the involvement of C<span class="hlt">2</span>H<span class="hlt">2</span> and C<span class="hlt">2</span>H4 in radiation heat <span class="hlt">transfer</span> needs to be taken into account in the numerical modeling of the ethylene/<span class="hlt">air</span> diffusion flame, especially in the early stage of combustion.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4237463','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4237463"><span>Net uptake of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> by coastal submerged aquatic vegetation</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Tokoro, Tatsuki; Hosokawa, Shinya; Miyoshi, Eiichi; Tada, Kazufumi; Watanabe, Kenta; Montani, Shigeru; Kayanne, Hajime; Kuwae, Tomohiro</p> <p>2014-01-01</p> <p>‘Blue Carbon’, which is carbon captured by marine living organisms, has recently been highlighted as a new option for climate change mitigation initiatives. In particular, coastal ecosystems have been recognized as significant carbon stocks because of their high burial rates and long-term sequestration of carbon. However, the direct contribution of Blue Carbon to the uptake of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> through <span class="hlt">air-sea</span> gas exchange remains unclear. We performed in situ measurements of carbon flows, including <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> 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('http://adsabs.harvard.edu/abs/2018JGRC..123..166F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRC..123..166F"><span>Non-Redfieldian Dynamics Explain Seasonal p<span class="hlt">CO</span><span class="hlt">2</span> Drawdown in the Gulf of Bothnia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fransner, Filippa; Gustafsson, Erik; Tedesco, Letizia; Vichi, Marcello; Hordoir, Robinson; Roquet, Fabien; Spilling, Kristian; Kuznetsov, Ivan; Eilola, Kari; Mörth, Carl-Magnus; Humborg, Christoph; Nycander, Jonas</p> <p>2018-01-01</p> <p>High inputs of nutrients and organic matter make coastal <span class="hlt">seas</span> places of intense <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange. Due to their complexity, the role of coastal <span class="hlt">seas</span> in the global <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange is, however, still uncertain. Here, we investigate the role of phytoplankton stoichiometric flexibility and extracellular DOC production for the seasonal nutrient and <span class="hlt">CO</span><span class="hlt">2</span> partial pressure (p<span class="hlt">CO</span><span class="hlt">2</span>) dynamics in the Gulf of Bothnia, Northern Baltic <span class="hlt">Sea</span>. A 3-D ocean biogeochemical-physical model with variable phytoplankton stoichiometry is for the first time implemented in the area and validated against observations. By simulating non-Redfieldian internal phytoplankton stoichiometry, and a relatively large production of extracellular dissolved organic carbon (DOC), the model adequately reproduces observed seasonal cycles in macronutrients and p<span class="hlt">CO</span><span class="hlt">2</span>. The uptake of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> is underestimated by 50% if instead using the Redfield ratio to determine the carbon assimilation, as in other Baltic <span class="hlt">Sea</span> models currently in use. The model further suggests, based on the observed drawdown of p<span class="hlt">CO</span><span class="hlt">2</span>, that observational estimates of organic carbon production in the Gulf of Bothnia, derived with the 14C method, may be heavily underestimated. We conclude that stoichiometric variability and uncoupling of carbon and nutrient assimilation have to be considered in order to better understand the carbon cycle in coastal <span class="hlt">seas</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29127830','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29127830"><span>Development and modelling of a steel slag filter effluent neutralization process with <span class="hlt">CO</span><span class="hlt">2</span>-enriched <span class="hlt">air</span> from an upstream bioprocess.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bove, Patricia; Claveau-Mallet, Dominique; Boutet, Étienne; Lida, Félix; Comeau, Yves</p> <p>2018-02-01</p> <p>The main objective of this project was to develop a steel slag filter effluent neutralization process by acidification with <span class="hlt">CO</span> <span class="hlt">2</span> -enriched <span class="hlt">air</span> coming from a bioprocess. Sub-objectives were to evaluate the neutralization capacity of different configurations of neutralization units in lab-scale conditions and to propose a design model of steel slag effluent neutralization. Two lab-scale column neutralization units fed with two different types of influent were operated at hydraulic retention time of 10 h. Tested variables were mode of flow (saturated or percolating), type of media (none, gravel, Bionest and AnoxKaldnes K3), type of <span class="hlt">air</span> (ambient or <span class="hlt">CO</span> <span class="hlt">2</span> -enriched) and airflow rate. One neutralization field test (saturated and no media, 2000-5000 ppm <span class="hlt">CO</span> <span class="hlt">2</span> , sequential feeding, hydraulic retention time of 7.8 h) was conducted for 7 days. Lab-scale and field-scale tests resulted in effluent pH of 7.5-9.5 when the aeration rate was sufficiently high. A model was implemented in the PHREEQC software and was based on the carbonate system, <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">transfer</span> and calcite precipitation; and was calibrated on ambient <span class="hlt">air</span> lab tests. The model was validated with <span class="hlt">CO</span> <span class="hlt">2</span> -enriched <span class="hlt">air</span> lab and field tests, providing satisfactory validation results over a wide range of <span class="hlt">CO</span> <span class="hlt">2</span> concentrations. The flow mode had a major impact on <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">transfer</span> and hydraulic efficiency, while the type of media had little influence. The flow mode also had a major impact on the calcite surface concentration in the reactor: it was constant in saturated mode and was increasing in percolating mode. Predictions could be made for different steel slag effluent pH and different operation conditions (hydraulic retention time, <span class="hlt">CO</span> <span class="hlt">2</span> concentration, media and mode of flow). The pH of the steel slag filter effluent and the <span class="hlt">CO</span> <span class="hlt">2</span> concentration of the enriched <span class="hlt">air</span> were factors that influenced most the effluent pH of the neutralization process. An increased concentration in <span class="hlt">CO</span> <span class="hlt">2</span> in the enriched <span class="hlt">air</span> reduced calcite precipitation</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> </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.osti.gov/biblio/1332125-sea-urchin-likenicoo2-nanocompositesforli-ionbatteries-supercapacitors','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1332125-sea-urchin-likenicoo2-nanocompositesforli-ionbatteries-supercapacitors"><span><span class="hlt">Sea</span> urchin-likeNi<span class="hlt">Co</span>O<span class="hlt">2</span>@C nanocompositesforLi-ionbatteries and supercapacitors</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>Liang, Jin; Xi, Kai; Tan, Guoqiang</p> <p></p> <p>The rational construction of battery electrode architecture that offers both high energy and power densities on a gravimetric and volumetric basis is a critical concern but achieving this aim is beset by many fundamental and practical challenges. Here we report a new <span class="hlt">sea</span> urchin-like Ni<span class="hlt">Co</span>O<span class="hlt">2</span>@C composite electrode architecture composed of Ni<span class="hlt">Co</span>O<span class="hlt">2</span> nanosheets grown on hollow concave carbon disks. Such a unique structural design not only preserves all the advantages of hollow structures but also increases the packing density of the active materials. Ni<span class="hlt">Co</span>O<span class="hlt">2</span> nanosheets grown on carbon disks promote a high utilization of active materials in redox reactions by reducingmore » the path length for Li+ ions and for electron <span class="hlt">transfer</span>. Meanwhile, the hollow concave carbon not only reduces the volume change, but also improves the volumetric energy density of the entire composite electrode. As a result, the nanocomposites exhibit superior electrochemical performance measured in terms of high capacity/capacitance, stable cycling performance and good rate capability in both Li-ion battery and supercapacitor applications. Such nanostructured composite electrode may also have great potential for application in other electrochemical devices.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/5224949','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/5224949"><span>Elevated <span class="hlt">CO</span><span class="hlt">2</span> stimulates marsh elevation gain, counterbalancing <span class="hlt">sea</span>-level rise</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Langley, J.A.; McKee, K.L.; Cahoon, D.R.; Cherry, J.A.; Megonigala, J.P.</p> <p>2009-01-01</p> <p>Tidal wetlands experiencing increased rates of <span class="hlt">sea</span>-level rise (SLR) must increase rates of soil elevation gain to avoid permanent conversion to open water. The maximal rate of SLR that these ecosystems can tolerate depends partly on mineral sediment deposition, but the accumulation of organic matter is equally important for many wetlands. Plant productivity drives organic matter dynamics and is sensitive to global change factors, such as rising atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentration. It remains unknown how global change will influence organic mechanisms that determine future tidal wetland viability. Here, we present experimental evidence that plant response to elevated atmospheric [<span class="hlt">CO</span><span class="hlt">2</span>] stimulates biogenic mechanisms of elevation gain in a brackish marsh. Elevated <span class="hlt">CO</span><span class="hlt">2</span> (ambient + 340 ppm) accelerated soil elevation gain by 3.9 mm yr−1in this <span class="hlt">2</span>-year field study, an effect mediated by stimulation of below-ground plant productivity. Further, a companion greenhouse experiment revealed that the <span class="hlt">CO</span><span class="hlt">2</span> effect was enhanced under salinity and flooding conditions likely to accompany future SLR. Our results indicate that by stimulating biogenic contributions to marsh elevation, increases in the greenhouse gas, <span class="hlt">CO</span><span class="hlt">2</span>, may paradoxically aid some coastal wetlands in counterbalancing rising <span class="hlt">seas</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19325121','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19325121"><span>Elevated <span class="hlt">CO</span><span class="hlt">2</span> stimulates marsh elevation gain, counterbalancing <span class="hlt">sea</span>-level rise.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Langley, J Adam; McKee, Karen L; Cahoon, Donald R; Cherry, Julia A; Megonigal, J Patrick</p> <p>2009-04-14</p> <p>Tidal wetlands experiencing increased rates of <span class="hlt">sea</span>-level rise (SLR) must increase rates of soil elevation gain to avoid permanent conversion to open water. The maximal rate of SLR that these ecosystems can tolerate depends partly on mineral sediment deposition, but the accumulation of organic matter is equally important for many wetlands. Plant productivity drives organic matter dynamics and is sensitive to global change factors, such as rising atmospheric <span class="hlt">CO</span>(<span class="hlt">2</span>) concentration. It remains unknown how global change will influence organic mechanisms that determine future tidal wetland viability. Here, we present experimental evidence that plant response to elevated atmospheric [<span class="hlt">CO</span>(<span class="hlt">2</span>)] stimulates biogenic mechanisms of elevation gain in a brackish marsh. Elevated <span class="hlt">CO</span>(<span class="hlt">2</span>) (ambient + 340 ppm) accelerated soil elevation gain by 3.9 mm yr(-1) in this <span class="hlt">2</span>-year field study, an effect mediated by stimulation of below-ground plant productivity. Further, a companion greenhouse experiment revealed that the <span class="hlt">CO</span>(<span class="hlt">2</span>) effect was enhanced under salinity and flooding conditions likely to accompany future SLR. Our results indicate that by stimulating biogenic contributions to marsh elevation, increases in the greenhouse gas, <span class="hlt">CO</span>(<span class="hlt">2</span>), may paradoxically aid some coastal wetlands in counterbalancing rising <span class="hlt">seas</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2661312','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2661312"><span>Elevated <span class="hlt">CO</span><span class="hlt">2</span> stimulates marsh elevation gain, counterbalancing <span class="hlt">sea</span>-level rise</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Langley, J. Adam; McKee, Karen L.; Cahoon, Donald R.; Cherry, Julia A.; Megonigal, J. Patrick</p> <p>2009-01-01</p> <p>Tidal wetlands experiencing increased rates of <span class="hlt">sea</span>-level rise (SLR) must increase rates of soil elevation gain to avoid permanent conversion to open water. The maximal rate of SLR that these ecosystems can tolerate depends partly on mineral sediment deposition, but the accumulation of organic matter is equally important for many wetlands. Plant productivity drives organic matter dynamics and is sensitive to global change factors, such as rising atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentration. It remains unknown how global change will influence organic mechanisms that determine future tidal wetland viability. Here, we present experimental evidence that plant response to elevated atmospheric [<span class="hlt">CO</span><span class="hlt">2</span>] stimulates biogenic mechanisms of elevation gain in a brackish marsh. Elevated <span class="hlt">CO</span><span class="hlt">2</span> (ambient + 340 ppm) accelerated soil elevation gain by 3.9 mm yr−1 in this <span class="hlt">2</span>-year field study, an effect mediated by stimulation of below-ground plant productivity. Further, a companion greenhouse experiment revealed that the <span class="hlt">CO</span><span class="hlt">2</span> effect was enhanced under salinity and flooding conditions likely to accompany future SLR. Our results indicate that by stimulating biogenic contributions to marsh elevation, increases in the greenhouse gas, <span class="hlt">CO</span><span class="hlt">2</span>, may paradoxically aid some coastal wetlands in counterbalancing rising <span class="hlt">seas</span>. PMID:19325121</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1984STIN...8431617D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1984STIN...8431617D"><span>A blackbody-pumped <span class="hlt">CO</span><span class="hlt">2</span>-N<span class="hlt">2</span> <span class="hlt">transfer</span> laser</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Deyoung, R. J.; Higdon, N. S.</p> <p>1984-08-01</p> <p>A compact blackbody-pumped <span class="hlt">CO</span><span class="hlt">2</span>-N<span class="hlt">2</span> <span class="hlt">transfer</span> laser was constructed and the significant operating parameters were investigated. Lasing was achieved at 10.6 microns by passing preheated N<span class="hlt">2</span> through a 1.5-mm-diameter nozzle to a laser cavity where the N<span class="hlt">2</span> was mixed with <span class="hlt">CO</span><span class="hlt">2</span> and He. An intrinsic efficiency of 0.7 percent was achieved for an oven temperature of 1473 K and N<span class="hlt">2</span> oven pressure of 440 torr. The optimum laser cavity consisted of a back mirror with maximum reflectivity and an output mirror with 97.5-percent reflectivity. The optimum gas mixture was 1<span class="hlt">CO</span><span class="hlt">2</span>/.5He/6N<span class="hlt">2</span>. The variation of laser output was measured as a function of oven temperature, nozzle diameter, N<span class="hlt">2</span> oven pressure, He and <span class="hlt">CO</span><span class="hlt">2</span> partial pressures, nozzle-to-oven separation, laser cell temperature, and output laser mirror reflectivity. With these parameters optimized, outputs approaching 1.4 watts were achieved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19840023547','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19840023547"><span>A blackbody-pumped <span class="hlt">CO</span><span class="hlt">2</span>-N<span class="hlt">2</span> <span class="hlt">transfer</span> laser</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Deyoung, R. J.; Higdon, N. S.</p> <p>1984-01-01</p> <p>A compact blackbody-pumped <span class="hlt">CO</span><span class="hlt">2</span>-N<span class="hlt">2</span> <span class="hlt">transfer</span> laser was constructed and the significant operating parameters were investigated. Lasing was achieved at 10.6 microns by passing preheated N<span class="hlt">2</span> through a 1.5-mm-diameter nozzle to a laser cavity where the N<span class="hlt">2</span> was mixed with <span class="hlt">CO</span><span class="hlt">2</span> and He. An intrinsic efficiency of 0.7 percent was achieved for an oven temperature of 1473 K and N<span class="hlt">2</span> oven pressure of 440 torr. The optimum laser cavity consisted of a back mirror with maximum reflectivity and an output mirror with 97.5-percent reflectivity. The optimum gas mixture was 1<span class="hlt">CO</span><span class="hlt">2</span>/.5He/6N<span class="hlt">2</span>. The variation of laser output was measured as a function of oven temperature, nozzle diameter, N<span class="hlt">2</span> oven pressure, He and <span class="hlt">CO</span><span class="hlt">2</span> partial pressures, nozzle-to-oven separation, laser cell temperature, and output laser mirror reflectivity. With these parameters optimized, outputs approaching 1.4 watts were achieved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AMT.....5.2689N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AMT.....5.2689N"><span>Effect of <span class="hlt">air</span> composition (N<span class="hlt">2</span>, O<span class="hlt">2</span>, Ar, and H<span class="hlt">2</span>O) on <span class="hlt">CO</span><span class="hlt">2</span> and CH4 measurement by wavelength-scanned cavity ring-down spectroscopy: calibration and measurement strategy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nara, H.; Tanimoto, H.; Tohjima, Y.; Mukai, H.; Nojiri, Y.; Katsumata, K.; Rella, C. W.</p> <p>2012-11-01</p> <p>We examined potential interferences from water vapor and atmospheric background gases (N<span class="hlt">2</span>, O<span class="hlt">2</span>, and Ar), and biases by isotopologues of target species, on accurate measurement of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> and CH4 by means of wavelength-scanned cavity ring-down spectroscopy (WS-CRDS). Changes of the background gas mole fractions in the sample <span class="hlt">air</span> substantially impacted the <span class="hlt">CO</span><span class="hlt">2</span> and CH4 measurements: variation of <span class="hlt">CO</span><span class="hlt">2</span> and CH4 due to relative increase of each background gas increased as Ar < O<span class="hlt">2</span> < N<span class="hlt">2</span>, suggesting similar relation for the pressure-broadening effects (PBEs) among the background gas. The pressure-broadening coefficients due to variations in O<span class="hlt">2</span> and Ar for <span class="hlt">CO</span><span class="hlt">2</span> and CH4 are empirically determined from these experimental results. Calculated PBEs using the pressure-broadening coefficients are linearly correlated with the differences between the mole fractions of O<span class="hlt">2</span> and Ar and their ambient abundances. Although the PBEs calculation showed that impact of natural variation of O<span class="hlt">2</span> is negligible on the <span class="hlt">CO</span><span class="hlt">2</span> and CH4 measurements, significant bias was inferred for the measurement of synthetic standard gases. For gas standards balanced with purified <span class="hlt">air</span>, the PBEs were estimated to be marginal (up to 0.05 ppm for <span class="hlt">CO</span><span class="hlt">2</span> and 0.01 ppb for CH4) although the PBEs were substantial (up to 0.87 ppm for <span class="hlt">CO</span><span class="hlt">2</span> and 1.4 ppb for CH4) for standards balanced with synthetic <span class="hlt">air</span>. For isotopic biases on <span class="hlt">CO</span><span class="hlt">2</span> measurements, we compared experimental results and theoretical calculations, which showed excellent agreement within their uncertainty. We derived instrument-specific water correction functions empirically for three WS-CRDS instruments (Picarro EnviroSense 3000i, G-1301, and G-2301), and evaluated the <span class="hlt">transferability</span> of the water correction function from G-1301 among these instruments. Although the <span class="hlt">transferability</span> was not proven, no significant difference was found in the water vapor correction function for the investigated WS-CRDS instruments as well as the instruments reported in the past studies</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1340454-co2-capture-from-ambient-air-crystallization-guanidine-sorbent','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1340454-co2-capture-from-ambient-air-crystallization-guanidine-sorbent"><span><span class="hlt">CO</span> <span class="hlt">2</span> Capture from Ambient <span class="hlt">Air</span> by Crystallization with a Guanidine Sorbent</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Seipp, Charles A.; Univ. of Texas, Austin, TX; Williams, Neil J.; ...</p> <p>2016-12-21</p> <p>Carbon capture and storage is an important strategy for stabilizing the increasing concentration of atmospheric <span class="hlt">CO</span> <span class="hlt">2</span> and the global temperature. A possible approach toward reversing this trend and decreasing the atmospheric <span class="hlt">CO</span> <span class="hlt">2</span> concentration is to remove the <span class="hlt">CO</span> <span class="hlt">2</span> directly from <span class="hlt">air</span> (direct <span class="hlt">air</span> capture). In this paper, we report a simple aqueous guanidine sorbent that captures <span class="hlt">CO</span> <span class="hlt">2</span> from ambient <span class="hlt">air</span> and binds it as a crystalline carbonate salt by guanidinium hydrogen bonding. The resulting solid has very low aqueous solubility (K sp=1.0(4)×10 -8), which facilitates its separation from solution by filtration. The bound <span class="hlt">CO</span> <span class="hlt">2</span> canmore » be released by relatively mild heating of the crystals at 80–120 °C, which regenerates the guanidine sorbent quantitatively. Finally and thus, this crystallization-based approach to <span class="hlt">CO</span> <span class="hlt">2</span> separation from <span class="hlt">air</span> requires minimal energy and chemical input, and offers the prospect for low-cost direct <span class="hlt">air</span> capture technologies.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/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 <span class="hlt">transfer</span> 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 exchange. 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> <span class="hlt">transfer</span> 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 exchanging gases between the atmosphere and ocean than younger less developed <span class="hlt">seas</span> which occur during the rapid passage of a hurricane.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26256597','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26256597"><span>Simultaneous Online Measurement of H<span class="hlt">2</span>O and <span class="hlt">CO</span><span class="hlt">2</span> in the Humid <span class="hlt">CO</span><span class="hlt">2</span> Adsorption/Desorption Process.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yu, Qingni; Ye, Sha; Zhu, Jingke; Lei, Lecheng; Yang, Bin</p> <p>2015-01-01</p> <p>A dew point meter (DP) and an infrared (IR) <span class="hlt">CO</span><span class="hlt">2</span> analyzer were assembled in a humid <span class="hlt">CO</span><span class="hlt">2</span> adsorption/desorption system in series for simultaneous online measurements of H<span class="hlt">2</span>O and <span class="hlt">CO</span><span class="hlt">2</span>, respectively. The humidifier, by using surface-flushing on a saturated brine solution was self-made for the generation of humid <span class="hlt">air</span> flow. It was found that by this method it became relatively easy to obtain a low H<span class="hlt">2</span>O content in <span class="hlt">air</span> flow and that its fluctuation could be reduced compared to the bubbling method. Water calibration for the DP-IR detector is necessary to be conducted for minimizing the measurement error of H<span class="hlt">2</span>O. It demonstrated that the relative error (RA) for simultaneous online measurements H<span class="hlt">2</span>O and <span class="hlt">CO</span><span class="hlt">2</span> in the desorption process is lower than 0.1%. The high RA in the adsorption of H<span class="hlt">2</span>O is attributed to H<span class="hlt">2</span>O adsorption on the <span class="hlt">transfer</span> pipe and amplification of the measurement error. The high accuracy of simultaneous online measurements of H<span class="hlt">2</span>O and <span class="hlt">CO</span><span class="hlt">2</span> is promising for investigating their <span class="hlt">co</span>-adsorption/desorption behaviors, especially for direct <span class="hlt">CO</span><span class="hlt">2</span> capture from ambient <span class="hlt">air</span>.</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/2005JGRC..110.3010A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005JGRC..110.3010A"><span>Iron in the Ross <span class="hlt">Sea</span>: <span class="hlt">2</span>. Impact of discrete iron addition strategies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Arrigo, Kevin R.; Tagliabue, Alessandro</p> <p>2005-03-01</p> <p>Presented are results of a regional-scale numerical investigation into the effectiveness of Fe fertilization as a means to increase the efficiency of the biological pump in Fe-limited waters of the Ross <span class="hlt">Sea</span>, Antarctica. This investigation was conducted using a modified version of the Coupled Ice And Ocean (CIAO) ecosystem model of the Ross <span class="hlt">Sea</span> sector of the Southern Ocean. Four sets of experiments were performed, investigating the impacts of differences in (1) timing of fertilization, (<span class="hlt">2</span>) duration of fertilization, (3) amount of Fe added, and (4) size of the fertilized patch. Results show that the stimulation of <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange (FCO<span class="hlt">2</span>) depends primarily on the timing of fertilization, regardless of the amount of Fe added. When Fe was added at the optimal time of year, FCO<span class="hlt">2</span> from the atmosphere into the Ross <span class="hlt">Sea</span> was increased by 3-22%, depending on fertilization strategy. Increasing patch size produced the largest response, and increasing initial Fe concentration produced the smallest. In all cases, as the intensity of Fe fertilization increased, the fertilization efficiency (increase in <span class="hlt">CO</span><span class="hlt">2</span> uptake per unit added Fe) dropped. Strategies that maximized the fertilization efficiency resulted in relatively little additional <span class="hlt">CO</span><span class="hlt">2</span> being drawn out of the atmosphere. To markedly increase oceanic uptake of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> would require the addition of large amounts of Fe due to the low fertilization efficiencies associated with maximum <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> exchange. Our results also show that differences in the fertilization strategy should be kept in mind when comparing the results of different Fe fertilization experiments.</p> </li> <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/2016AGUOS.A24C2606P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOS.A24C2606P"><span>Surfactant control of <span class="hlt">air-sea</span> gas exchange 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 <span class="hlt">transfer</span> 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 exchange 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('https://www.gpo.gov/fdsys/pkg/FR-2010-03-23/pdf/2010-6303.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2010-03-23/pdf/2010-6303.pdf"><span>75 FR 13803 - <span class="hlt">SeaCo</span> Ltd.; Notice of Application</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2010-03-23</p> <p>...] <span class="hlt">SeaCo</span> Ltd.; Notice of Application March 17, 2010. AGENCY: Securities and Exchange Commission... (``Act''). SUMMARY: Summary of Application: <span class="hlt">SeaCo</span> Ltd. (``<span class="hlt">SeaCo</span>'') seeks an order under section 3(b)(<span class="hlt">2</span>..., reinvesting, owning, holding or trading in securities. <span class="hlt">SeaCo</span> is primarily engaged in the shipping container...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25207956','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25207956"><span>Reducing the cost of Ca-based direct <span class="hlt">air</span> capture of <span class="hlt">CO</span><span class="hlt">2</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zeman, Frank</p> <p>2014-10-07</p> <p>Direct <span class="hlt">air</span> capture, the chemical removal of <span class="hlt">CO</span><span class="hlt">2</span> directly from the atmosphere, may play a role in mitigating future climate risk or form the basis of a sustainable transportation infrastructure. The current discussion is centered on the estimated cost of the technology and its link to "overshoot" trajectories, where atmospheric <span class="hlt">CO</span><span class="hlt">2</span> levels are actively reduced later in the century. The American Physical Society (APS) published a report, later updated, estimating the cost of a one million tonne <span class="hlt">CO</span><span class="hlt">2</span> per year <span class="hlt">air</span> capture facility constructed today that highlights several fundamental concepts of chemical <span class="hlt">air</span> capture. These fundamentals are viewed through the lens of a chemical process that cycles between removing <span class="hlt">CO</span><span class="hlt">2</span> from the <span class="hlt">air</span> and releasing the absorbed <span class="hlt">CO</span><span class="hlt">2</span> in concentrated form. This work builds on the APS report to investigate the effect of modifications to the <span class="hlt">air</span> capture system based on suggestions in the report and subsequent publications. The work shows that reduced carbon electricity and plastic packing materials (for the contactor) may have significant effects on the overall price, reducing the APS estimate from $610 to $309/t<span class="hlt">CO</span><span class="hlt">2</span> avoided. Such a reduction does not challenge postcombustion capture from point sources, estimated at $80/t<span class="hlt">CO</span><span class="hlt">2</span>, but does make <span class="hlt">air</span> capture a feasible alternative for the transportation sector and a potential negative emissions technology. Furthermore, <span class="hlt">air</span> capture represents atmospheric reductions rather than simply avoided emissions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23504873','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23504873"><span>Tidal marsh plant responses to elevated <span class="hlt">CO</span><span class="hlt">2</span> , nitrogen fertilization, and <span class="hlt">sea</span> level rise.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Adam Langley, J; Mozdzer, Thomas J; Shepard, Katherine A; Hagerty, Shannon B; Patrick Megonigal, J</p> <p>2013-05-01</p> <p>Elevated <span class="hlt">CO</span><span class="hlt">2</span> and nitrogen (N) addition directly affect plant productivity and the mechanisms that allow tidal marshes to maintain a constant elevation relative to <span class="hlt">sea</span> level, but it remains unknown how these global change drivers modify marsh plant response to <span class="hlt">sea</span> level rise. Here we manipulated factorial combinations of <span class="hlt">CO</span><span class="hlt">2</span> concentration (two levels), N availability (two levels) and relative <span class="hlt">sea</span> level (six levels) using in situ mesocosms containing a tidal marsh community composed of a sedge, Schoenoplectus americanus, and a grass, Spartina patens. Our objective is to determine, if elevated <span class="hlt">CO</span><span class="hlt">2</span> and N alter the growth and persistence of these plants in coastal ecosystems facing rising <span class="hlt">sea</span> levels. After two growing seasons, we found that N addition enhanced plant growth particularly at <span class="hlt">sea</span> levels where plants were most stressed by flooding (114% stimulation in the + 10 cm treatment), and N effects were generally larger in combination with elevated <span class="hlt">CO</span><span class="hlt">2</span> (288% stimulation). N fertilization shifted the optimal productivity of S. patens to a higher <span class="hlt">sea</span> level, but did not confer S. patens an enhanced ability to tolerate <span class="hlt">sea</span> level rise. S. americanus responded strongly to N only in the higher <span class="hlt">sea</span> level treatments that excluded S. patens. Interestingly, addition of N, which has been suggested to accelerate marsh loss, may afford some marsh plants, such as the widespread sedge, S. americanus, the enhanced ability to tolerate inundation. However, if chronic N pollution reduces the availability of propagules of S. americanus or other flood-tolerant species on the landscape scale, this shift in species dominance could render tidal marshes more susceptible to marsh collapse. © 2013 Blackwell Publishing Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/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/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> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li class="active"><span>7</span></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_7 --> <div id="page_8" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li class="active"><span>8</span></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="141"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/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/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 Exchange</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 <span class="hlt">transfer</span> that can be used to predict the gas <span class="hlt">transfer</span> rates with sufficient accuracy as a function of micrometeorological parameters is still lacking. State of the art are still simple gas <span class="hlt">transfer</span> 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 exchange 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 <span class="hlt">transfer</span> velocity and gas <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> 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 exchange 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('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://www.agu.org/journals/jc/v096/iC04/90JC02642/','USGSPUBS'); return false;" href="http://www.agu.org/journals/jc/v096/iC04/90JC02642/"><span>Atmospheric organochlorine pollutants and <span class="hlt">air-sea</span> exchange of hexachlorocyclohexane in the Bering and Chukchi <span class="hlt">Seas</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Hinckley, D.A.; Bidleman, T.F.; Rice, C.P.</p> <p>1991-01-01</p> <p>Organochlorine pesticides have been found in Arctic fish, marine mammals, birds, and plankton for some time. The lack of local sources and remoteness of the region imply long-range transport and deposition of contaminants into the Arctic from sources to the south. While on the third Soviet-American Joint Ecological Expedition to the Bering and Chukchi <span class="hlt">Seas</span> (August 1988), high-volume <span class="hlt">air</span> samples were taken and analyzed for organochlorine pesticides. Hexachlorocyclohexane (HCH), hexachlorobenzene, polychlorinated camphenes, and chlordane (listed in order of abundance, highest to lowest) were quantified. The <span class="hlt">air-sea</span> gas exchange of HCH was estimated at 18 stations during the cruise. Average alpha-HCH concentrations in concurrent atmosphere and surface water samples were 250 pg m-3 and <span class="hlt">2</span>.4 ng L-1, respectively, and average gamma-HCH concentrations were 68 pg m-3 in the atmosphere and 0.6 ng L-1 in surface water. Calculations based on experimentally derived Henry's law constants showed that the surface water was undersaturated with respect to the atmosphere at most stations (alpha-HCH, average 79% saturation; gamma-HCH, average 28% saturation). The 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://www.ncbi.nlm.nih.gov/pubmed/27544762','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27544762"><span>Aircraft measurements of SO<span class="hlt">2</span>, NOx, <span class="hlt">CO</span>, and O3 over the coastal and offshore area of Yellow <span class="hlt">Sea</span> of China.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yang, Xiaoyang; Wang, Xinhua; Yang, Wen; Xu, Jun; Ren, Lihong; He, Youjiang; Liu, Bing; Bai, Zhipeng; Meng, Fan; Hu, Min</p> <p>2016-09-01</p> <p>In order to investigate long-range transport of the <span class="hlt">air</span> pollution in the East Asia, <span class="hlt">air</span> pollutants, including SO<span class="hlt">2</span>, NOx, <span class="hlt">CO</span>, and O3, were observed by aircraft measurement over the coastal and offshore area of Yellow <span class="hlt">Sea</span> of China in April 2011. NOx and SO<span class="hlt">2</span> seemed to become moderate in recent years, and the concentrations during the whole observations ranged from 0.49 to 9.57 ppb and from 0.10 to 16.02 ppb, respectively. The high concentrations of <span class="hlt">CO</span> were measured with an average value of 0.98 ppm. The measured O3 average concentration was 76.25 ppb, which showed a higher level comparing with the results from some previous studies. Most of the results for the concentration values generally followed the typical characteristic of vertical and spatial distribution, which were "low altitude > high altitude" and "land/coastal > <span class="hlt">sea</span>," respectively. Transport of polluted <span class="hlt">air</span> mass from the continent to the aircraft measurement area was confirmed in some days during the observation by the meteorological analysis, while the measurement results supposed to represent the background level of the pollutants in rest days. Additionally, some small-scale <span class="hlt">air</span> pollution plumes were observed. Significant positive correlations between NOx and SO<span class="hlt">2</span> indicated that these two species originated from the same region. On the other hand, good positive correlations between NOx and O3 found during <span class="hlt">2</span>-day flight suggested that the O3 formation was probably under "NOx-limited" regime in these days.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/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/2009AGUFM.A51E0162M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.A51E0162M"><span><span class="hlt">Sea</span> spray contributions to the <span class="hlt">air-sea</span> fluxes at moderate and hurricane wind speeds</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mueller, J. A.; Veron, F.</p> <p>2009-12-01</p> <p>At sufficiently high wind speed conditions, the surface of the ocean separates to form a substantial number of <span class="hlt">sea</span> spray drops, which can account for a significant fraction of the total <span class="hlt">air-sea</span> surface area and thus make important contributions to the aggregate <span class="hlt">air-sea</span> momentum, heat and mass fluxes. Although consensus around the qualitative impacts of these drops has been building in recent years, the quantification of their impacts has remained elusive. Ultimately, the spray-mediated fluxes depend on three controlling factors: the number and size of drops formed at the surface, the duration of suspension within the atmospheric marine boundary layer, and the rate of momentum, heat and mass <span class="hlt">transfer</span> between the drops and the atmosphere. While the latter factor can be estimated from an established, physically-based theory, the estimates for the former two are not well established. Using a recent, physically-based model of the <span class="hlt">sea</span> spray source function along with the results from Lagrangian stochastic simulations of individual drops, we estimate the aggregate spray-mediated fluxes, finding reasonable agreement with existing models and estimates within the empirical range of wind speed conditions. At high wind speed conditions that are outside the empirical range, however, we find somewhat lower spray-mediated fluxes than previously reported in the literature, raising new questions about the relative <span class="hlt">air-sea</span> fluxes at high wind speeds as well as the development and sustainment of hurricanes.</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('https://www.ncbi.nlm.nih.gov/pubmed/22682963','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22682963"><span>Effect of <span class="hlt">air</span> bubble localization after <span class="hlt">transfer</span> on embryo <span class="hlt">transfer</span> outcomes.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tiras, Bulent; Korucuoglu, Umit; Polat, Mehtap; Saltik, Ayse; Zeyneloglu, Hulusi Bulent; Yarali, Hakan</p> <p>2012-09-01</p> <p>Our study aimed to provide information about the effects of <span class="hlt">air</span> bubble localization after <span class="hlt">transfer</span> on embryo <span class="hlt">transfer</span> outcomes. Retrospective analysis of 7489 ultrasound-guided embryo <span class="hlt">transfers</span>. Group 1 included 6631 embryo <span class="hlt">transfers</span> in which no movement of the <span class="hlt">air</span> bubbles was observed after <span class="hlt">transfer</span>. Group <span class="hlt">2</span> consisted of 407 embryo <span class="hlt">transfers</span> in which the <span class="hlt">air</span> bubbles moved towards the uterine fundus spontaneously, a little time after <span class="hlt">transfer</span>. Group 3 included 370 embryo <span class="hlt">transfers</span> in which the <span class="hlt">air</span> bubbles moved towards the uterine fundus with ejection, immediately after <span class="hlt">transfer</span>. Group 4 consisted of 81 embryo <span class="hlt">transfers</span> in which the <span class="hlt">air</span> bubbles moved towards the cervical canal. The four patient groups were different from one another with respect to positive pregnancy tests. Post hoc test revealed that this difference was between group 4 and other groups. An initial finding of our study was significantly decreased positive pregnancy test rates and clinical pregnancy rates with <span class="hlt">air</span> bubbles moving towards the cervical canal after <span class="hlt">transfer</span>. Although <span class="hlt">air</span> bubbles moving towards the uterine fundus with ejection were associated with higher pregnancy rates, higher miscarriage rates and similar live birth rates were observed compared to <span class="hlt">air</span> bubbles remaining stable after <span class="hlt">transfer</span>. Copyright © 2012 Elsevier Ireland Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2010-title50-vol8/pdf/CFR-2010-title50-vol8-sec648-13.pdf','CFR'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2010-title50-vol8/pdf/CFR-2010-title50-vol8-sec648-13.pdf"><span>50 CFR 648.13 - <span class="hlt">Transfers</span> at <span class="hlt">sea</span>.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2010&page.go=Go">Code of Federal Regulations, 2010 CFR</a></p> <p></p> <p>2010-10-01</p> <p>... 50 Wildlife and Fisheries 8 2010-10-01 2010-10-01 false <span class="hlt">Transfers</span> at <span class="hlt">sea</span>. 648.13 Section 648.13... <span class="hlt">sea</span>. (a) Only vessels issued a Loligo and butterfish moratorium or Illex moratorium permit under § 648... purchased at <span class="hlt">sea</span>. (c) All persons are prohibited from <span class="hlt">transferring</span> or attempting to <span class="hlt">transfer</span> NE multispecies...</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 exchange of momentum, heat, freshwater, and gas between the atmosphere and ocean. These exchange processes are critical to a broad range of research questions spanning length scales from meters to thousands of kilometers and time scales from hours to decades. Examples are discussed (section <span class="hlt">2</span>). The estimation of surface turbulent 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 <span class="hlt">transferred</span> 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/2017JGRD..122.7216O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRD..122.7216O"><span><span class="hlt">Sea-to-air</span> flux of dimethyl sulfide in the South and North Pacific Ocean as measured by proton <span class="hlt">transfer</span> reaction-mass spectrometry coupled with the gradient flux technique</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Omori, Yuko; Tanimoto, Hiroshi; Inomata, Satoshi; Ikeda, Kohei; Iwata, Toru; Kameyama, Sohiko; Uematsu, Mitsuo; Gamo, Toshitaka; Ogawa, Hiroshi; Furuya, Ken</p> <p>2017-07-01</p> <p>Exchange of dimethyl sulfide (DMS) between the surface ocean and the lower atmosphere was examined by using proton <span class="hlt">transfer</span> reaction-mass spectrometry coupled with the gradient flux (PTR-MS/GF) system. We deployed the PTR-MS/GF system and observed vertical gradients of atmospheric DMS just above the <span class="hlt">sea</span> surface in the subtropical and transitional South Pacific Ocean and the subarctic North Pacific Ocean. In total, we obtained 370 in situ profiles, and of these we used 46 data sets to calculate the <span class="hlt">sea-to-air</span> flux of DMS. The DMS flux determined was in the range from 1.9 to 31 μmol m-<span class="hlt">2</span> d-1 and increased with wind speed and biological activity, in reasonable accordance with previous observations in the open ocean. The gas <span class="hlt">transfer</span> velocity of DMS derived from the PTR-MS/GF measurements was similar to either that of DMS determined by the eddy covariance technique or that of insoluble gases derived from the dual tracer experiments, depending on the observation sites located in different geographic regions. When atmospheric conditions were strongly stable during the daytime in the subtropical ocean, the PTR-MS/GF observations captured a daytime versus nighttime difference in DMS mixing ratios in the surface <span class="hlt">air</span> overlying the ocean surface. The difference was mainly due to the <span class="hlt">sea-to-air</span> DMS emissions and stable atmospheric conditions, thus affecting the gradient of DMS. This indicates that the DMS gradient is strongly controlled by diurnal variations in the vertical structure of the lower atmosphere above the ocean surface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16271812','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16271812"><span>Atmospheric concentrations and <span class="hlt">air-sea</span> exchanges of nonylphenol, tertiary octylphenol and nonylphenol monoethoxylate in the North <span class="hlt">Sea</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Xie, Zhiyong; Lakaschus, Soenke; Ebinghaus, Ralf; Caba, Armando; Ruck, Wolfgang</p> <p>2006-07-01</p> <p>Concentrations of nonylphenol isomers (NP), tertiary octylphenol (t-OP) and nonylphenol monoethoxylate isomers (NP1EO) have been simultaneously determined in the <span class="hlt">sea</span> water and atmosphere of the North <span class="hlt">Sea</span>. A decreasing concentration profile appeared following the distance increasing from the coast to the central part of the North <span class="hlt">Sea</span>. <span class="hlt">Air-sea</span> exchanges of t-OP and NP were estimated using the two-film resistance model based upon relative <span class="hlt">air</span>-water concentrations and experimentally derived Henry's law constant. The average of <span class="hlt">air-sea</span> exchange fluxes was -12+/-6 ng m(-<span class="hlt">2</span>)day(-1) for t-OP and -39+/-19 ng m(-<span class="hlt">2</span>)day(-1) for NP, which indicates a net deposition is occurring. These results suggest that the <span class="hlt">air-sea</span> vapour exchange is an important process that intervenes in the mass balance of alkylphenols in the North <span class="hlt">Sea</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5544137','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5544137"><span>Simultaneously reducing <span class="hlt">CO</span><span class="hlt">2</span> and particulate exposures via fractional recirculation of vehicle cabin <span class="hlt">air</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Jung, Heejung S.; Grady, Michael L.; Victoroff, Tristan; Miller, Arthur L.</p> <p>2017-01-01</p> <p>Prior studies demonstrate that <span class="hlt">air</span> recirculation can reduce exposure to nanoparticles in vehicle cabins. However when people occupy confined spaces, <span class="hlt">air</span> recirculation can lead to carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) accumulation which can potentially lead to deleterious effects on cognitive function. This study proposes a fractional <span class="hlt">air</span> recirculation system for reducing nanoparticle concentration while simultaneously suppressing <span class="hlt">CO</span><span class="hlt">2</span> levels in the cabin. Several recirculation scenarios were tested using a custom-programmed HVAC (heat, ventilation, <span class="hlt">air</span> conditioning) unit that varied the recirculation door angle in the test vehicle. Operating the recirculation system with a standard cabin filter reduced particle concentrations to 1000 particles/cm3, although <span class="hlt">CO</span><span class="hlt">2</span> levels rose to 3000 ppm. When as little as 25% fresh <span class="hlt">air</span> was introduced (75% recirculation), <span class="hlt">CO</span><span class="hlt">2</span> levels dropped to 1000 ppm, while particle concentrations remained below 5000 particles/cm3. We found that nanoparticles were removed selectively during recirculation and demonstrated the trade-off between cabin <span class="hlt">CO</span><span class="hlt">2</span> concentration and cabin particle concentration using fractional <span class="hlt">air</span> recirculation. Data showed significant increases in <span class="hlt">CO</span><span class="hlt">2</span> levels during 100% recirculation. For various fan speeds, recirculation fractions of 50–75% maintained lower <span class="hlt">CO</span><span class="hlt">2</span> levels in the cabin, while still reducing particulate levels. We recommend fractional recirculation as a simple method to reduce occupants’ exposures to particulate matter and <span class="hlt">CO</span><span class="hlt">2</span> in vehicles. A design with several fractional recirculation settings could allow <span class="hlt">air</span> exchange adequate for reducing both particulate and <span class="hlt">CO</span><span class="hlt">2</span> exposures. Developing this technology could lead to reductions in airborne nanoparticle exposure, while also mitigating safety risks from <span class="hlt">CO</span><span class="hlt">2</span> accumulation. PMID:28781568</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28781568','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28781568"><span>Simultaneously reducing <span class="hlt">CO</span><span class="hlt">2</span> and particulate exposures via fractional recirculation of vehicle cabin <span class="hlt">air</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Jung, Heejung S; Grady, Michael L; Victoroff, Tristan; Miller, Arthur L</p> <p>2017-07-01</p> <p>Prior studies demonstrate that <span class="hlt">air</span> recirculation can reduce exposure to nanoparticles in vehicle cabins. However when people occupy confined spaces, <span class="hlt">air</span> recirculation can lead to carbon dioxide (<span class="hlt">CO</span> <span class="hlt">2</span> ) accumulation which can potentially lead to deleterious effects on cognitive function. This study proposes a fractional <span class="hlt">air</span> recirculation system for reducing nanoparticle concentration while simultaneously suppressing <span class="hlt">CO</span> <span class="hlt">2</span> levels in the cabin. Several recirculation scenarios were tested using a custom-programmed HVAC (heat, ventilation, <span class="hlt">air</span> conditioning) unit that varied the recirculation door angle in the test vehicle. Operating the recirculation system with a standard cabin filter reduced particle concentrations to 1000 particles/cm 3 , although <span class="hlt">CO</span> <span class="hlt">2</span> levels rose to 3000 ppm. When as little as 25% fresh <span class="hlt">air</span> was introduced (75% recirculation), <span class="hlt">CO</span> <span class="hlt">2</span> levels dropped to 1000 ppm, while particle concentrations remained below 5000 particles/cm 3 . We found that nanoparticles were removed selectively during recirculation and demonstrated the trade-off between cabin <span class="hlt">CO</span> <span class="hlt">2</span> concentration and cabin particle concentration using fractional <span class="hlt">air</span> recirculation. Data showed significant increases in <span class="hlt">CO</span> <span class="hlt">2</span> levels during 100% recirculation. For various fan speeds, recirculation fractions of 50-75% maintained lower <span class="hlt">CO</span> <span class="hlt">2</span> levels in the cabin, while still reducing particulate levels. We recommend fractional recirculation as a simple method to reduce occupants' exposures to particulate matter and <span class="hlt">CO</span> <span class="hlt">2</span> in vehicles. A design with several fractional recirculation settings could allow <span class="hlt">air</span> exchange adequate for reducing both particulate and <span class="hlt">CO</span> <span class="hlt">2</span> exposures. Developing this technology could lead to reductions in airborne nanoparticle exposure, while also mitigating safety risks from <span class="hlt">CO</span> <span class="hlt">2</span> accumulation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AtmEn.160...77J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AtmEn.160...77J"><span>Simultaneously reducing <span class="hlt">CO</span><span class="hlt">2</span> and particulate exposures via fractional recirculation of vehicle cabin <span class="hlt">air</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jung, Heejung S.; Grady, Michael L.; Victoroff, Tristan; Miller, Arthur L.</p> <p>2017-07-01</p> <p>Prior studies demonstrate that <span class="hlt">air</span> recirculation can reduce exposure to nanoparticles in vehicle cabins. However when people occupy confined spaces, <span class="hlt">air</span> recirculation can lead to carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) accumulation which can potentially lead to deleterious effects on cognitive function. This study proposes a fractional <span class="hlt">air</span> recirculation system for reducing nanoparticle concentration while simultaneously suppressing <span class="hlt">CO</span><span class="hlt">2</span> levels in the cabin. Several recirculation scenarios were tested using a custom-programmed HVAC (heat, ventilation, <span class="hlt">air</span> conditioning) unit that varied the recirculation door angle in the test vehicle. Operating the recirculation system with a standard cabin filter reduced particle concentrations to 1000 particles/cm3, although <span class="hlt">CO</span><span class="hlt">2</span> levels rose to 3000 ppm. When as little as 25% fresh <span class="hlt">air</span> was introduced (75% recirculation), <span class="hlt">CO</span><span class="hlt">2</span> levels dropped to 1000 ppm, while particle concentrations remained below 5000 particles/cm3. We found that nanoparticles were removed selectively during recirculation and demonstrated the trade-off between cabin <span class="hlt">CO</span><span class="hlt">2</span> concentration and cabin particle concentration using fractional <span class="hlt">air</span> recirculation. Data showed significant increases in <span class="hlt">CO</span><span class="hlt">2</span> levels during 100% recirculation. For various fan speeds, recirculation fractions of 50-75% maintained lower <span class="hlt">CO</span><span class="hlt">2</span> levels in the cabin, while still reducing particulate levels. We recommend fractional recirculation as a simple method to reduce occupants' exposures to particulate matter and <span class="hlt">CO</span><span class="hlt">2</span> in vehicles. A design with several fractional recirculation settings could allow <span class="hlt">air</span> exchange adequate for reducing both particulate and <span class="hlt">CO</span><span class="hlt">2</span> exposures. Developing this technology could lead to reductions in airborne nanoparticle exposure, while also mitigating safety risks from <span class="hlt">CO</span><span class="hlt">2</span> accumulation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AtmEn..99..546A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AtmEn..99..546A"><span>Quantifying the <span class="hlt">air</span> quality-<span class="hlt">CO</span><span class="hlt">2</span> tradeoff potential for airports</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ashok, Akshay; Dedoussi, Irene C.; Yim, Steve H. L.; Balakrishnan, Hamsa; Barrett, Steven R. H.</p> <p>2014-12-01</p> <p>Aircraft movements on the airport surface are responsible for <span class="hlt">CO</span><span class="hlt">2</span> emissions that contribute to climate change and other emissions that affect <span class="hlt">air</span> quality and human health. While the potential for optimizing aircraft surface movements to minimize <span class="hlt">CO</span><span class="hlt">2</span> emissions has been assessed, the implications of <span class="hlt">CO</span><span class="hlt">2</span> emissions minimization for <span class="hlt">air</span> quality have not been quantified. In this paper, we identify conditions in which there is a tradeoff between <span class="hlt">CO</span><span class="hlt">2</span> emissions and population exposure to O3 and secondary PM<span class="hlt">2</span>.5 - i.e. where decreasing fuel burn (which is directly proportional to <span class="hlt">CO</span><span class="hlt">2</span> emissions) results in increased exposure. Fuel burn and emissions are estimated as a function of thrust setting for five common gas turbine engines at 34 US airports. Regional <span class="hlt">air</span> quality impacts, which are dominated by ozone and secondary PM<span class="hlt">2</span>.5, are computed as a function of airport location and time using the adjoint of the GEOS-Chem chemistry-transport model. Tradeoffs between <span class="hlt">CO</span><span class="hlt">2</span> emissions and population exposure to PM<span class="hlt">2</span>.5 and O3 occur between <span class="hlt">2</span>-18% and 5-60% of the year, respectively, depending on airport location, engine type, and thrust setting. The total duration of tradeoff conditions is 5-12 times longer at maximum thrust operations (typical for takeoff) relative to 4% thrust operations (typical for taxiing). Per kilogram of additional fuel burn at constant thrust setting during tradeoff conditions, reductions in population exposure to PM<span class="hlt">2</span>.5 and O3 are 6-13% and 32-1060% of the annual average (positive) population exposure per kilogram fuel burn, where the ranges encompass the medians over the 34 airports. For fuel burn increases due to thrust increases (i.e. for constant operating time), reductions in both PM<span class="hlt">2</span>.5 and O3 exposure are 1.5-6.4 times larger in magnitude than those due to increasing fuel burn at constant thrust (i.e. increasing operating time). Airports with relatively high population exposure reduction potentials - which occur due to a combination of high duration and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/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://hdl.handle.net/2060/20140002626','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140002626"><span>Development of a Prototype Algal Reactor for Removing <span class="hlt">CO</span><span class="hlt">2</span> from Cabin <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>Patel, Vrajen; Monje, Oscar</p> <p>2013-01-01</p> <p>Controlling carbon dioxide in spacecraft cabin <span class="hlt">air</span> may be accomplished using algal photobioreactors (PBRs). The purpose of this project was to evaluate the use of a commercial microcontroller, the Arduino Mega 2560, for measuring key photioreactor variables: dissolved oxygen, pH, temperature, light, and carbon dioxide. The Arduino platform is an opensource physical computing platform composed of a compact microcontroller board and a C++/C computer language (Arduino 1.0.5). The functionality of the Arduino platform can be expanded by the use of numerous add-ons or 'shields'. The Arduino Mega 2560 was equipped with the following shields: datalogger, BNC shield for reading pH sensor, a Mega Moto shield for controlling <span class="hlt">CO</span><span class="hlt">2</span> addition, as well as multiple sensors. The dissolved oxygen (DO) probe was calibrated using a nitrogen bubbling technique and the pH probe was calibrated via an Omega pH simulator. The PBR was constructed using a <span class="hlt">2</span> L beaker, a 66 L box for addition of <span class="hlt">CO</span><span class="hlt">2</span>, a micro porous membrane, a diaphragm pump, four 25 watt light bulbs, a MasterFiex speed controller, and a fan. The algae (wild type Synechocystis PCC6803) was grown in an aerated flask until the algae was dense enough to used in the main reactor. After the algae was grown, it was <span class="hlt">transferred</span> to the <span class="hlt">2</span> L beaker where <span class="hlt">CO</span><span class="hlt">2</span> consumption and O<span class="hlt">2</span> production was measured using the microcontroller sensor suite. The data was recorded via the datalogger and <span class="hlt">transferred</span> to a computer for analysis.</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> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li class="active"><span>8</span></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_8 --> <div id="page_9" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li class="active"><span>9</span></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="161"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.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 Exchange experiment ASGASEX was conducted from August 30 until October 1st from the Meetpost Noordwijk (MPN), a research tower in the North <span class="hlt">Sea</span> at 9 km from the Dutch coast. The objective of ASGASEX was a study of parameters affecting the <span class="hlt">air-sea</span> exchange of gases, and a comparison of experimental methods to derive the exchange coefficient for <span class="hlt">CO</span>{sub <span class="hlt">2</span>}. A detailed description of the ASGASEX experiment is presented in Oost. The authors` contribution to ASGASEX was a micro-meteorological package to measure the 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 exchange in cooperation with the University of Southampton and the University of Galway.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/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.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 <span class="hlt">Transfer</span> Modeling for the Development of Particle/Supercritical-<span class="hlt">CO</span><span class="hlt">2</span> Heat Exchanger</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-<span class="hlt">transfer</span> 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-<span class="hlt">transfer</span> medium that is inexpensive and stable at high temperatures above 1,000 degrees C. The particle/heat exchanger 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 exchanger 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-<span class="hlt">transfer</span> modeling to inform the particle/s-<span class="hlt">CO</span><span class="hlt">2</span> heat-exchanger design and assess design tradeoffs. The heat-<span class="hlt">transfer</span> process was modeled based on a particle/s-<span class="hlt">CO</span><span class="hlt">2</span> counterflow configuration. Empirical heat-<span class="hlt">transfer</span> correlations for the fluidized bed and s-<span class="hlt">CO</span><span class="hlt">2</span> were used in calculating the heat-<span class="hlt">transfer</span> 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-<span class="hlt">transfer</span> analysis, and cost was estimated from the sizing of the heat exchanger. The paper shows the path in achieving the cost and performance objectives for a heat-exchanger design.« less</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> <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.osti.gov/pages/biblio/1379705-pore-scale-supercritical-co2-dissolution-mass-transfer-under-drainage-conditions','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1379705-pore-scale-supercritical-co2-dissolution-mass-transfer-under-drainage-conditions"><span>Pore-scale supercritical <span class="hlt">CO</span> <span class="hlt">2</span> dissolution and mass <span class="hlt">transfer</span> under drainage conditions</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Chang, Chun; Zhou, Quanlin; Oostrom, Mart; ...</p> <p>2016-12-05</p> <p>Recently, both core- and pore-scale imbibition experiments have shown non-equilibrium dissolution of supercritical <span class="hlt">CO</span> <span class="hlt">2</span> (sc<span class="hlt">CO</span> <span class="hlt">2</span>) and a prolonged depletion of residual sc<span class="hlt">CO</span> <span class="hlt">2</span>. In this paper, pore-scale sc<span class="hlt">CO</span> <span class="hlt">2</span> dissolution and mass <span class="hlt">transfer</span> under drainage conditions were investigated using a two-dimensional heterogeneous micromodel and a novel fluorescent water dye with a sensitive pH range between 3.7 and 6.5. Drainage experiments were conducted at 9 MPa and 40 °C by injecting sc<span class="hlt">CO</span> <span class="hlt">2</span> into the sandstone-analogue pore network initially saturated by water without dissolved <span class="hlt">CO</span> <span class="hlt">2</span> (ds<span class="hlt">CO</span> <span class="hlt">2</span>). During the experiments, time-lapse images of dye intensity, reflecting water pH,more » were obtained. These images show non-uniform pH in individual pores and pore clusters, with average pH levels gradually decreasing with time. Further analysis on selected pores and pore clusters shows that (1) rate-limited mass <span class="hlt">transfer</span> prevails with slowly decreasing pH over time when the sc<span class="hlt">CO</span> <span class="hlt">2</span>-water interface area is low with respect to the volume of water-filled pores and pore clusters, (<span class="hlt">2</span>) fast sc<span class="hlt">CO</span> <span class="hlt">2</span> dissolution and phase equilibrium occurs when sc<span class="hlt">CO</span> <span class="hlt">2</span> bubbles invade into water-filled pores, significantly enhancing the area-to-volume ratio, and (3) a transition from rate-limited to diffusion-limited mass <span class="hlt">transfer</span> occurs in a single pore when a medium area-to-volume ratio is prevalent. The analysis also shows that two fundamental processes – sc<span class="hlt">CO</span> <span class="hlt">2</span> dissolution at phase interfaces and diffusion of ds<span class="hlt">CO</span> <span class="hlt">2</span> at the pore scale (10–100 µm) observed after sc<span class="hlt">CO</span> <span class="hlt">2</span> bubble invasion into water-filled pores without pore throat constraints – are relatively fast. The overall slow dissolution of sc<span class="hlt">CO</span> <span class="hlt">2</span> in the millimeter-scale micromodel can be attributed to the small area-to-volume ratios that represent pore-throat configurations and characteristics of phase interfaces. Finally, this finding is applicable for the behavior of dissolution at pore, core, and field scales when water-filled pores and pore</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1379705','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1379705"><span>Pore-scale supercritical <span class="hlt">CO</span> <span class="hlt">2</span> dissolution and mass <span class="hlt">transfer</span> under drainage conditions</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>Chang, Chun; Zhou, Quanlin; Oostrom, Mart</p> <p></p> <p>Recently, both core- and pore-scale imbibition experiments have shown non-equilibrium dissolution of supercritical <span class="hlt">CO</span> <span class="hlt">2</span> (sc<span class="hlt">CO</span> <span class="hlt">2</span>) and a prolonged depletion of residual sc<span class="hlt">CO</span> <span class="hlt">2</span>. In this paper, pore-scale sc<span class="hlt">CO</span> <span class="hlt">2</span> dissolution and mass <span class="hlt">transfer</span> under drainage conditions were investigated using a two-dimensional heterogeneous micromodel and a novel fluorescent water dye with a sensitive pH range between 3.7 and 6.5. Drainage experiments were conducted at 9 MPa and 40 °C by injecting sc<span class="hlt">CO</span> <span class="hlt">2</span> into the sandstone-analogue pore network initially saturated by water without dissolved <span class="hlt">CO</span> <span class="hlt">2</span> (ds<span class="hlt">CO</span> <span class="hlt">2</span>). During the experiments, time-lapse images of dye intensity, reflecting water pH,more » were obtained. These images show non-uniform pH in individual pores and pore clusters, with average pH levels gradually decreasing with time. Further analysis on selected pores and pore clusters shows that (1) rate-limited mass <span class="hlt">transfer</span> prevails with slowly decreasing pH over time when the sc<span class="hlt">CO</span> <span class="hlt">2</span>-water interface area is low with respect to the volume of water-filled pores and pore clusters, (<span class="hlt">2</span>) fast sc<span class="hlt">CO</span> <span class="hlt">2</span> dissolution and phase equilibrium occurs when sc<span class="hlt">CO</span> <span class="hlt">2</span> bubbles invade into water-filled pores, significantly enhancing the area-to-volume ratio, and (3) a transition from rate-limited to diffusion-limited mass <span class="hlt">transfer</span> occurs in a single pore when a medium area-to-volume ratio is prevalent. The analysis also shows that two fundamental processes – sc<span class="hlt">CO</span> <span class="hlt">2</span> dissolution at phase interfaces and diffusion of ds<span class="hlt">CO</span> <span class="hlt">2</span> at the pore scale (10–100 µm) observed after sc<span class="hlt">CO</span> <span class="hlt">2</span> bubble invasion into water-filled pores without pore throat constraints – are relatively fast. The overall slow dissolution of sc<span class="hlt">CO</span> <span class="hlt">2</span> in the millimeter-scale micromodel can be attributed to the small area-to-volume ratios that represent pore-throat configurations and characteristics of phase interfaces. Finally, this finding is applicable for the behavior of dissolution at pore, core, and field scales when water-filled pores and pore</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1344032-pore-scale-supercritical-co2-dissolution-mass-transfer-under-drainage-conditions','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1344032-pore-scale-supercritical-co2-dissolution-mass-transfer-under-drainage-conditions"><span>Pore-scale supercritical <span class="hlt">CO</span> <span class="hlt">2</span> dissolution and mass <span class="hlt">transfer</span> under drainage conditions</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>Chang, Chun; Zhou, Quanlin; Oostrom, Mart</p> <p></p> <p>Abstract: Recently, both core- and pore-scale imbibition experiments have shown non-equilibrium dissolution of supercritical <span class="hlt">CO</span> <span class="hlt">2</span> (sc<span class="hlt">CO</span> <span class="hlt">2</span>) and a prolonged depletion of residual sc<span class="hlt">CO</span> <span class="hlt">2</span>. In this study, pore-scale sc<span class="hlt">CO</span> <span class="hlt">2</span> dissolution and mass <span class="hlt">transfer</span> under drainage conditions were investigated using a two-dimensional heterogeneous micromodel and a novel fluorescent water dye with a sensitive pH range between 3.7 and 6.5. Drainage experiments were conducted at 9 MPa and 40 °C by injecting sc<span class="hlt">CO</span> <span class="hlt">2</span> into the sandstone-analogue pore network initially saturated by water without dissolved <span class="hlt">CO</span> <span class="hlt">2</span> (ds<span class="hlt">CO</span> <span class="hlt">2</span>). During the experiments, time-lapse images of dye intensity, reflecting watermore » pH, were obtained. These images show non-uniform pH in individual pores and pore clusters, with average pH levels gradually decreasing with time. Further analysis on selected pores and pore clusters shows that (1) rate-limited mass <span class="hlt">transfer</span> prevails with slowly decreasing pH over time when the sc<span class="hlt">CO</span> <span class="hlt">2</span>-water interface area is low with respect to the volume of water-filled pores and pore clusters, (<span class="hlt">2</span>) fast sc<span class="hlt">CO</span> <span class="hlt">2</span> dissolution and phase equilibrium occurs when sc<span class="hlt">CO</span> <span class="hlt">2</span> bubbles invade into water-filled pores, significantly enhancing the area-to-volume ratio, and (3) a transition from rate-limited to diffusion-limited mass <span class="hlt">transfer</span> occurs in a single pore when a medium area-to-volume ratio is prevalent. The analysis also shows that two fundamental processes – sc<span class="hlt">CO</span> <span class="hlt">2</span> dissolution at phase interfaces and diffusion of ds<span class="hlt">CO</span> <span class="hlt">2</span> at the pore scale (10-100 µm) observed after sc<span class="hlt">CO</span> <span class="hlt">2</span> bubble invasion into water-filled pores without pore throat constraints – are relatively fast. The overall slow dissolution of sc<span class="hlt">CO</span> <span class="hlt">2</span> in the millimeter-scale micromodel can be attributed to the small area-to-volume ratios that represent pore-throat configurations and characteristics of phase interfaces. This finding is applicable for the behavior of dissolution at pore, core, and field scales when water-filled pores and pore</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('https://www.ncbi.nlm.nih.gov/pubmed/29520546','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29520546"><span>Study on embodied <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">transfer</span> between the Jing-Jin-Ji region and other regions in China: a quantification using an interregional input-output model.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chen, Mengmeng; Wu, Sanmang; Lei, Yalin; Li, Shantong</p> <p>2018-05-01</p> <p>Jing-Jin-Ji region (i.e., Beijing, Tianjin, and Hebei) is China's key development region, but it is also the leading and most serious <span class="hlt">air</span> pollution region in China. High fossil fuel consumption is the major source of both carbon dioxide (<span class="hlt">CO</span> <span class="hlt">2</span> ) emissions and <span class="hlt">air</span> pollutants. Therefore, it is important to reveal the source of <span class="hlt">CO</span> <span class="hlt">2</span> emissions to control the <span class="hlt">air</span> pollution in the Jing-Jin-Ji region. In this study, an interregional input-output model was applied to quantitatively estimate the embodied <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">transfer</span> between Jing-Jin-Ji region and other region in China using China's interregional input-output data in 2010. The results indicated that there was a significant difference in the production-based <span class="hlt">CO</span> <span class="hlt">2</span> emissions in China, and furthermore, the Jing-Jin-Ji region and its surrounding regions were the main regions of the production-based <span class="hlt">CO</span> <span class="hlt">2</span> emissions in China. Hebei Province exported a large amount of embodied <span class="hlt">CO</span> <span class="hlt">2</span> to meet the investment, consumption, and export demands of Beijing and Tianjin. The Jing-Jin-Ji regions exported a great deal of embodied <span class="hlt">CO</span> <span class="hlt">2</span> to the coastal provinces of southeast China and imported it from neighboring provinces.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2014-title50-vol12/pdf/CFR-2014-title50-vol12-sec635-29.pdf','CFR2014'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2014-title50-vol12/pdf/CFR-2014-title50-vol12-sec635-29.pdf"><span>50 CFR 635.29 - <span class="hlt">Transfer</span> at <span class="hlt">sea</span>.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2014&page.go=Go">Code of Federal Regulations, 2014 CFR</a></p> <p></p> <p>2014-10-01</p> <p>... 50 Wildlife and Fisheries 12 2014-10-01 2014-10-01 false <span class="hlt">Transfer</span> at <span class="hlt">sea</span>. 635.29 Section 635.29..., DEPARTMENT OF COMMERCE ATLANTIC HIGHLY MIGRATORY SPECIES Management Measures § 635.29 <span class="hlt">Transfer</span> at <span class="hlt">sea</span>. (a... at <span class="hlt">sea</span> in the Atlantic Ocean, regardless of where the fish was harvested. Notwithstanding the...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2012-title50-vol12/pdf/CFR-2012-title50-vol12-sec635-29.pdf','CFR2012'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2012-title50-vol12/pdf/CFR-2012-title50-vol12-sec635-29.pdf"><span>50 CFR 635.29 - <span class="hlt">Transfer</span> at <span class="hlt">sea</span>.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2012&page.go=Go">Code of Federal Regulations, 2012 CFR</a></p> <p></p> <p>2012-10-01</p> <p>... 50 Wildlife and Fisheries 12 2012-10-01 2012-10-01 false <span class="hlt">Transfer</span> at <span class="hlt">sea</span>. 635.29 Section 635.29..., DEPARTMENT OF COMMERCE ATLANTIC HIGHLY MIGRATORY SPECIES Management Measures § 635.29 <span class="hlt">Transfer</span> at <span class="hlt">sea</span>. (a... at <span class="hlt">sea</span> in the Atlantic Ocean, regardless of where the fish was harvested. Notwithstanding the...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2012-title50-vol12/pdf/CFR-2012-title50-vol12-sec648-13.pdf','CFR2012'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2012-title50-vol12/pdf/CFR-2012-title50-vol12-sec648-13.pdf"><span>50 CFR 648.13 - <span class="hlt">Transfers</span> at <span class="hlt">sea</span>.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2012&page.go=Go">Code of Federal Regulations, 2012 CFR</a></p> <p></p> <p>2012-10-01</p> <p>... 50 Wildlife and Fisheries 12 2012-10-01 2012-10-01 false <span class="hlt">Transfers</span> at <span class="hlt">sea</span>. 648.13 Section 648.13... <span class="hlt">sea</span>. (a) Only vessels issued a longfin squid and butterfish moratorium or Illex moratorium permit... for any small-mesh multispecies purchased at <span class="hlt">sea</span>. (c) All persons are prohibited from <span class="hlt">transferring</span> or...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2011-title50-vol10/pdf/CFR-2011-title50-vol10-sec635-29.pdf','CFR2011'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2011-title50-vol10/pdf/CFR-2011-title50-vol10-sec635-29.pdf"><span>50 CFR 635.29 - <span class="hlt">Transfer</span> at <span class="hlt">sea</span>.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2011&page.go=Go">Code of Federal Regulations, 2011 CFR</a></p> <p></p> <p>2011-10-01</p> <p>... 50 Wildlife and Fisheries 10 2011-10-01 2011-10-01 false <span class="hlt">Transfer</span> at <span class="hlt">sea</span>. 635.29 Section 635.29..., DEPARTMENT OF COMMERCE ATLANTIC HIGHLY MIGRATORY SPECIES Management Measures § 635.29 <span class="hlt">Transfer</span> at <span class="hlt">sea</span>. (a... at <span class="hlt">sea</span> in the Atlantic Ocean, regardless of where the fish was harvested. Notwithstanding the...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2013-title50-vol12/pdf/CFR-2013-title50-vol12-sec648-13.pdf','CFR2013'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2013-title50-vol12/pdf/CFR-2013-title50-vol12-sec648-13.pdf"><span>50 CFR 648.13 - <span class="hlt">Transfers</span> at <span class="hlt">sea</span>.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2013&page.go=Go">Code of Federal Regulations, 2013 CFR</a></p> <p></p> <p>2013-10-01</p> <p>... 50 Wildlife and Fisheries 12 2013-10-01 2013-10-01 false <span class="hlt">Transfers</span> at <span class="hlt">sea</span>. 648.13 Section 648.13... <span class="hlt">sea</span>. (a) Only vessels issued a longfin squid and butterfish moratorium or Illex moratorium permit... for any small-mesh multispecies purchased at <span class="hlt">sea</span>. (c) All persons are prohibited from <span class="hlt">transferring</span> or...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2013-title50-vol12/pdf/CFR-2013-title50-vol12-sec635-29.pdf','CFR2013'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2013-title50-vol12/pdf/CFR-2013-title50-vol12-sec635-29.pdf"><span>50 CFR 635.29 - <span class="hlt">Transfer</span> at <span class="hlt">sea</span>.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2013&page.go=Go">Code of Federal Regulations, 2013 CFR</a></p> <p></p> <p>2013-10-01</p> <p>... 50 Wildlife and Fisheries 12 2013-10-01 2013-10-01 false <span class="hlt">Transfer</span> at <span class="hlt">sea</span>. 635.29 Section 635.29..., DEPARTMENT OF COMMERCE ATLANTIC HIGHLY MIGRATORY SPECIES Management Measures § 635.29 <span class="hlt">Transfer</span> at <span class="hlt">sea</span>. (a... at <span class="hlt">sea</span> in the Atlantic Ocean, regardless of where the fish was harvested. Notwithstanding the...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2014-title50-vol12/pdf/CFR-2014-title50-vol12-sec648-13.pdf','CFR2014'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2014-title50-vol12/pdf/CFR-2014-title50-vol12-sec648-13.pdf"><span>50 CFR 648.13 - <span class="hlt">Transfers</span> at <span class="hlt">sea</span>.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2014&page.go=Go">Code of Federal Regulations, 2014 CFR</a></p> <p></p> <p>2014-10-01</p> <p>... 50 Wildlife and Fisheries 12 2014-10-01 2014-10-01 false <span class="hlt">Transfers</span> at <span class="hlt">sea</span>. 648.13 Section 648.13... <span class="hlt">sea</span>. (a) Only vessels issued a longfin squid and butterfish moratorium or Illex moratorium permit... for any small-mesh multispecies purchased at <span class="hlt">sea</span>. (c) All persons are prohibited from <span class="hlt">transferring</span> or...</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('http://adsabs.harvard.edu/abs/2018AdWR..113..100S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AdWR..113..100S"><span>Measurement and modeling of <span class="hlt">CO</span><span class="hlt">2</span> mass <span class="hlt">transfer</span> in brine at reservoir conditions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shi, Z.; Wen, B.; Hesse, M. A.; Tsotsis, T. T.; Jessen, K.</p> <p>2018-03-01</p> <p>In this work, we combine measurements and modeling to investigate the application of pressure-decay experiments towards delineation and interpretation of <span class="hlt">CO</span><span class="hlt">2</span> solubility, uptake and mass <span class="hlt">transfer</span> in water/brine systems at elevated pressures of relevance to <span class="hlt">CO</span><span class="hlt">2</span> storage operations in saline aquifers. Accurate measurements and modeling of mass <span class="hlt">transfer</span> in this context are crucial to an improved understanding of the longer-term fate of <span class="hlt">CO</span><span class="hlt">2</span> that is injected into the subsurface for storage purposes. Pressure-decay experiments are presented for <span class="hlt">CO</span><span class="hlt">2</span>/water and <span class="hlt">CO</span><span class="hlt">2</span>/brine systems with and without the presence of unconsolidated porous media. We demonstrate, via high-resolution numerical calculations in <span class="hlt">2</span>-D, that natural convection will complicate the interpretation of the experimental observations if the particle size is not sufficiently small. In such settings, we demonstrate that simple 1-D interpretations can result in an overestimation of the uptake (diffusivity) by two orders of magnitude. Furthermore, we demonstrate that high-resolution numerical calculations agree well with the experimental observations for settings where natural convection contributes substantially to the overall mass <span class="hlt">transfer</span> process.</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/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/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://www.gpo.gov/fdsys/pkg/CFR-2010-title50-vol8/pdf/CFR-2010-title50-vol8-sec635-29.pdf','CFR'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2010-title50-vol8/pdf/CFR-2010-title50-vol8-sec635-29.pdf"><span>50 CFR 635.29 - <span class="hlt">Transfer</span> at <span class="hlt">sea</span>.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2010&page.go=Go">Code of Federal Regulations, 2010 CFR</a></p> <p></p> <p>2010-10-01</p> <p>... 50 Wildlife and Fisheries 8 2010-10-01 2010-10-01 false <span class="hlt">Transfer</span> at <span class="hlt">sea</span>. 635.29 Section 635.29..., DEPARTMENT OF COMMERCE ATLANTIC HIGHLY MIGRATORY SPECIES Management Measures § 635.29 <span class="hlt">Transfer</span> at <span class="hlt">sea</span>. Link... tuna, blue marlin, white marlin, or swordfish at <span class="hlt">sea</span> in the Atlantic Ocean, regardless of where the...</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('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4319967','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4319967"><span>Microclimatic Performance of a Free-<span class="hlt">Air</span> Warming and <span class="hlt">CO</span><span class="hlt">2</span> Enrichment Experiment in Windy Wyoming, USA</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>LeCain, Daniel; Smith, David; Morgan, Jack; Kimball, Bruce A.; Pendall, Elise; Miglietta, Franco</p> <p>2015-01-01</p> <p>In order to plan for global changing climate experiments are being conducted in many countries, but few have monitored the effects of the climate change treatments (warming, elevated <span class="hlt">CO</span><span class="hlt">2</span>) on the experimental plot microclimate. During three years of an eight year study with year-round feedback-controlled infra-red heater warming (1.5/3.0°C day/night) and growing season free-<span class="hlt">air</span> <span class="hlt">CO</span><span class="hlt">2</span> enrichment (600 ppm) in the mixed-grass prairie of Wyoming, USA, we monitored soil, leaf, canopy-<span class="hlt">air</span>, above-canopy-<span class="hlt">air</span> temperatures and relative humidity of control and treated experimental plots and evaluated ecologically important temperature differentials. Leaves were warmed somewhat less than the target settings (1.1 & 1.5°C day/night) but soil was warmed more creating an average that matched the target settings extremely well both during the day and night plus the summer and winter. The site typically has about 50% bare or litter covered soil, therefore soil heat <span class="hlt">transfer</span> is more critical than in dense canopy ecosystems. The Wyoming site commonly has strong winds (5 ms-1 average) and significant daily and seasonal temperature fluctuations (as much as 30°C daily) but the warming system was nearly always able to maintain the set temperatures regardless of abiotic variation. The within canopy-<span class="hlt">air</span> was only slightly warmed and above canopy-<span class="hlt">air</span> was not warmed by the system, therefore convective warming was minor. Elevated <span class="hlt">CO</span><span class="hlt">2</span> had no direct effect nor interaction with the warming treatment on microclimate. Relative humidity within the plant canopy was only slightly reduced by warming. Soil water content was reduced by warming but increased by elevated <span class="hlt">CO</span><span class="hlt">2</span>. This study demonstrates the importance of monitoring the microclimate in manipulative field global change experiments so that critical physiological and ecological conclusions can be determined. Highly variable energy demand fluctuations showed that passive IR heater warming systems will not maintain desired warming for much of the</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/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://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 exchangers 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/2014PhDT........25E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014PhDT........25E"><span>Non-catalytic <span class="hlt">transfer</span> hydrogenation in supercritical <span class="hlt">CO</span><span class="hlt">2</span> for coal liquefaction</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Elhussien, Hussien</p> <p></p> <p>This thesis presents the results of the investigation on developing and evaluating a low temperature (<150°C) non - catalytic process using a hydrogen <span class="hlt">transfer</span> agent (instead of molecu-lar hydrogen) for coal dissolution in supercritical <span class="hlt">CO</span><span class="hlt">2</span>. The main idea behind the thesis was that one hydrogen atom from water and one hydrogen atom from the hydrogen <span class="hlt">transfer</span> agent (HTA) were used to hydrogenate the coal. The products of coal dissolution were non-polar and polar while the supercritical <span class="hlt">CO</span><span class="hlt">2</span>, which enhanced the rates of hydrogenation and dissolution of the non-polar molecules and removal from the reaction site, was non-polar. The polar modifier (PM) for <span class="hlt">CO</span><span class="hlt">2</span> was added to the freed to aid in the dissolution and removal of the polar components. The addition of a phase <span class="hlt">transfer</span> agent (PTA) allowed a seamless transport of the ions and by-product between the aqueous and organic phases. DDAB, used as the PTA, is an effective phase <span class="hlt">transfer</span> catalyst and showed enhancement to the coal dissolution process. COAL + DH- +H <span class="hlt">2</span>O → COAL.H<span class="hlt">2</span> + DHO-- This process has a great feature due to the fact that the chemicals were obtained without requir-ing to first convert coal to <span class="hlt">CO</span> and H<span class="hlt">2</span> units as in indirect coal liquefaction. The experiments were conducted in a unique reactor set up that can be connected through two lines. one line to feed the reactor with supercritical <span class="hlt">CO</span> <span class="hlt">2</span> and the other connected to gas chromatograph. The use of the supercritical <span class="hlt">CO</span><span class="hlt">2</span> enhanced the solvent option due to the chemical extraction, in addition to the low environmental impact and energy cost. In this thesis the experiment were conducted at five different temperatures from atmos-pheric to 140°C, 3000 - 6000 psi with five component of feed mixture, namely water, HTA, PTA, coal, and PM in semi batch vessels reactor system with a volume of 100 mL. The results show that the chemicals were obtained without requiring to first convert coal to <span class="hlt">CO</span> and H<span class="hlt">2</span> units as in indirect coal liquefaction. The results show that</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28535344','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28535344"><span>Clarifying the Controversial Catalytic Performance of <span class="hlt">Co</span>(OH)<span class="hlt">2</span> and <span class="hlt">Co</span>3O4 for Oxygen Reduction/Evolution Reactions toward Efficient Zn-<span class="hlt">Air</span> Batteries.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Song, Zhishuang; Han, Xiaopeng; Deng, Yida; Zhao, Naiqin; Hu, Wenbin; Zhong, Cheng</p> <p>2017-07-12</p> <p>Cobalt-based nanomaterials have been widely studied as catalysts for the oxygen reduction reaction (ORR) and oxygen evolution reaction (OER) due to their remarkable bifunctional catalytic activity, low cost, and easy availability. However, controversial results concerning OER/ORR performance exist between different types of cobalt-based catalysts, especially for <span class="hlt">Co</span>(OH) <span class="hlt">2</span> and <span class="hlt">Co</span> 3 O 4 . To address this issue, we develop a facile electrochemical deposition method to grow <span class="hlt">Co</span>(OH) <span class="hlt">2</span> directly on the skeleton of carbon cloth, and further <span class="hlt">Co</span> 3 O 4 was obtained by post thermal treatment. The entire synthesis strategy removes the use of any binders and also avoids the additional preparation process (e.g., <span class="hlt">transfer</span> and slurry coating) of final electrodes. This leads to a true comparison of the ORR/OER catalytic performance between <span class="hlt">Co</span>(OH) <span class="hlt">2</span> and <span class="hlt">Co</span> 3 O 4 , eliminating uncertainties arising from the electrode preparation procedures. The surface morphologies, microstructures, and electrochemical behaviors of prepared <span class="hlt">Co</span>(OH) <span class="hlt">2</span> and <span class="hlt">Co</span> 3 O 4 catalysts were systemically investigated by scanning electron microscopy, transmission electron microscopy, atomic force microscopy, and electrochemical characterization methods. The results revealed that the electrochemically deposited <span class="hlt">Co</span>(OH) <span class="hlt">2</span> was in the form of vertically aligned nanosheets with average thickness of about 4.5 nm. After the thermal treatment in an <span class="hlt">air</span> atmosphere, <span class="hlt">Co</span>(OH) <span class="hlt">2</span> nanosheets were converted into mesoporous <span class="hlt">Co</span> 3 O 4 nanosheets with remarkably increased electrochemical active surface area (ECSA). Although the ORR/OER activity normalized by the geometric surface area of mesoporous <span class="hlt">Co</span> 3 O 4 nanosheets is higher than that of <span class="hlt">Co</span>(OH) <span class="hlt">2</span> nanosheets, the performance normalized by the ECSA of the former is lower than that of the latter. Considering the superior apparent overall activity and durability, the <span class="hlt">Co</span> 3 O 4 catalyst has been further evaluated by integrating it into a Zn-<span class="hlt">air</span> battery prototype. The <span class="hlt">Co</span> 3 O 4 nanosheets in</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 exchange 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/21329341','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21329341"><span>Modeling <span class="hlt">CO</span><span class="hlt">2</span> mass <span class="hlt">transfer</span> in amine mixtures: PZ-AMP and PZ-MDEA.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Puxty, Graeme; Rowland, Robert</p> <p>2011-03-15</p> <p>The most common method of carbon dioxide (<span class="hlt">CO</span>(<span class="hlt">2</span>)) capture is the absorption of <span class="hlt">CO</span>(<span class="hlt">2</span>) into a falling thin film of an aqueous amine solution. Modeling of mass <span class="hlt">transfer</span> during <span class="hlt">CO</span>(<span class="hlt">2</span>) absorption is an important way to gain insight and understanding about the underlying processes that are occurring. In this work a new software tool has been used to model <span class="hlt">CO</span>(<span class="hlt">2</span>) absorption into aqueous piperazine (PZ) and binary mixtures of PZ with <span class="hlt">2</span>-amino-<span class="hlt">2</span>-methyl-1-propanol (AMP) or methyldiethanolamine (MDEA). The tool solves partial differential and simultaneous equations describing diffusion and chemical reaction automatically derived from reactions written using chemical notation. It has been demonstrated that by using reactions that are chemically plausible the mass <span class="hlt">transfer</span> in binary mixtures can be fully described by combining the chemical reactions and their associated parameters determined for single amines. The observed enhanced mass <span class="hlt">transfer</span> in binary mixtures can be explained through chemical interactions occurring in the mixture without need to resort to using additional reactions or unusual transport phenomena such as the "shuttle mechanism".</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('http://adsabs.harvard.edu/abs/2017BGeo...14..447L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017BGeo...14..447L"><span>Ciliate and mesozooplankton community response to increasing <span class="hlt">CO</span><span class="hlt">2</span> levels in the Baltic <span class="hlt">Sea</span>: insights from a large-scale mesocosm experiment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lischka, Silke; Bach, Lennart T.; Schulz, Kai-Georg; Riebesell, Ulf</p> <p>2017-01-01</p> <p>Community approaches to investigating ocean acidification (OA) effects suggest a high tolerance of micro- and mesozooplankton to carbonate chemistry changes expected to occur within this century. Plankton communities in the coastal areas of the Baltic <span class="hlt">Sea</span> frequently experience pH variations partly exceeding projections for the near future both on a diurnal and seasonal basis. We conducted a large-scale mesocosm <span class="hlt">CO</span><span class="hlt">2</span> enrichment experiment ( ˜ 55 m3) enclosing the natural plankton community in Tvärminne-Storfjärden for 8 weeks during June-August 2012 and studied community and species-taxon response of ciliates and mesozooplankton to <span class="hlt">CO</span><span class="hlt">2</span> elevations expected for this century. In addition to the response to f<span class="hlt">CO</span><span class="hlt">2</span>, we also considered temperature and chlorophyll a variations in our analyses. Shannon diversity of ciliates significantly decreased with f<span class="hlt">CO</span><span class="hlt">2</span> and temperature with a greater dominance of smaller species. The mixotrophic Myrionecta rubra seemed to indirectly and directly benefit from higher <span class="hlt">CO</span><span class="hlt">2</span> concentrations in the post-bloom phase through increased occurrence of picoeukaryotes (most likely Cryptophytes) and Dinophyta at higher <span class="hlt">CO</span><span class="hlt">2</span> levels. With respect to mesozooplankton, we did not detect significant effects for either total abundance or for Shannon diversity. The cladocera Bosmina sp. occurred at distinctly higher abundance for a short time period during the second half of the experiment in three of the <span class="hlt">CO</span><span class="hlt">2</span>-enriched mesocosms except for the highest <span class="hlt">CO</span><span class="hlt">2</span> level. The ratio of Bosmina sp. with empty to embryo- or resting-egg-bearing brood chambers, however, was significantly affected by <span class="hlt">CO</span><span class="hlt">2</span>, temperature, and chlorophyll a. An indirect <span class="hlt">CO</span><span class="hlt">2</span> effect via increased food availability (Cyanobacteria) stimulating Bosmina sp. reproduction cannot be ruled out. Although increased regenerated primary production diminishes trophic <span class="hlt">transfer</span> in general, the presence of organisms able to graze on bacteria such as cladocerans may positively impact organic matter <span class="hlt">transfer</span> to higher</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://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2214981','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2214981"><span>Proton transport by phosphate diffusion--a mechanism of facilitated <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">transfer</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></p> <p>1976-01-01</p> <p>We have measured <span class="hlt">CO</span><span class="hlt">2</span> fluxes across phosphate solutions at different carbonic anhydrase concentrations, bicarbonate concentration gradients, phosphate concentrations, and mobilities. Temperature was 22-25 degrees C, the pH of the phosphate solutions was 7.0-7.3. We found that under physiological conditions of pH and p<span class="hlt">CO</span><span class="hlt">2</span> a facilitated diffusion of <span class="hlt">CO</span><span class="hlt">2</span> occurs in addition to free diffusion when (a) sufficient carbonic anhydrase is present, and (b) a concentration gradient of HCO3- is established along with a p<span class="hlt">CO</span><span class="hlt">2</span> gradient, and (c) the phosphate buffer has a mobility comparable to that of bicarbonate. When the phosphate was immobilized by attaching 0.25-mm-long cellulose particles, no facilitation of <span class="hlt">CO</span><span class="hlt">2</span> diffusion was detectable. A mechanism of facilitated <span class="hlt">CO</span><span class="hlt">2</span> diffusion in phosphate solutions analogous to that in albumin solutions was proposed on the basis of these findings: bicarbonate diffusion together with a facilitated proton transport by phosphate diffusion. A mathematical model of this mechanism was formulated. The <span class="hlt">CO</span><span class="hlt">2</span> fluxed predicted by the model agree quantitatively with the experimentally determined fluxes. It is concluded that a highly effective proton transport mechanism acts in solutions of mobile phosphate buffers. By this mechanism; <span class="hlt">CO</span><span class="hlt">2</span> <span class="hlt">transfer</span> may be increased up to fivefold and proton <span class="hlt">transfer</span> may be increased to 10,000-fold. PMID:6619</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> </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://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 exchange 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 exchange is required. Using current observations recorded during a major tropical cyclone, we have estimated this momentum <span class="hlt">transfer</span> 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> <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/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> <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.ncbi.nlm.nih.gov/pubmed/29100692','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29100692"><span>Ground <span class="hlt">air</span>: A first approximation of the Earth's second largest reservoir of carbon dioxide gas.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Baldini, James U L; Bertram, Rachel A; Ridley, Harriet E</p> <p>2018-03-01</p> <p>It is becoming increasingly clear that a substantial reservoir of carbon exists in the unsaturated zone of aquifers, though the total size of this reservoir on a global scale remains unquantified. Here we provide the first broad estimate of the amount of carbon dioxide gas found in this terrestrial reservoir. We calculate that between <span class="hlt">2</span> and 53 PgC exists as gaseous <span class="hlt">CO</span> <span class="hlt">2</span> in aquifers worldwide, generated by the slow microbial oxidation of organic particles transported into aquifers by percolating groundwater. Importantly, this carbon reservoir is in the form of <span class="hlt">CO</span> <span class="hlt">2</span> gas, and is therefore <span class="hlt">transferable</span> to the Earth's atmosphere without any phase change. On a coarse scale, water table depths are partially controlled by local <span class="hlt">sea</span> level; <span class="hlt">sea</span> level lowering therefore allows slow carbon sequestration into the reservoir and <span class="hlt">sea</span> level increases force rapid <span class="hlt">CO</span> <span class="hlt">2</span> outgassing from this reservoir. High-resolution cave <span class="hlt">air</span> p<span class="hlt">CO</span> <span class="hlt">2</span> data demonstrate that <span class="hlt">sea</span> level variability does affect <span class="hlt">CO</span> <span class="hlt">2</span> outgassing rates from the unsaturated zone, and that the <span class="hlt">CO</span> <span class="hlt">2</span> outgassing due to <span class="hlt">sea</span> level rise currently occurs on daily (tidal) timescales. We suggest that global mean water table depth must modulate the global unsaturated zone volume and the size of this carbon reservoir, potentially affecting atmospheric <span class="hlt">CO</span> <span class="hlt">2</span> on geological timescales. Copyright © 2017 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001JSMEB..44..274C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001JSMEB..44..274C"><span>Heat <span class="hlt">Transfer</span> of Confined Impinging <span class="hlt">Air</span>-water Mist Jet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chang, Shyy Woei; Su, Lo May</p> <p></p> <p>This paper describes the detailed heat <span class="hlt">transfer</span> distributions of an atomized <span class="hlt">air</span>-water mist jet impinging orthogonally onto a confined target plate with various water-to-<span class="hlt">air</span> mass-flow ratios. A transient technique was used to measure the full field heat <span class="hlt">transfer</span> coefficients of the impinging surface. Results showed that the high momentum mist-jet interacting with the water-film and wall-jet flows created a variety of heat <span class="hlt">transfer</span> contours on the impinging surface. The trade-off between the competing influences of the different heat <span class="hlt">transfer</span> mechanisms involving in an impinging mist jet made the nonlinear variation tendency of overall heat <span class="hlt">transfer</span> against the increase of water-to-<span class="hlt">air</span> mass-flow ratio and extended the effective cooling region. With separation distances of 10, 8, 6 and 4 jet-diameters, the spatially averaged heat <span class="hlt">transfer</span> values on the target plate could respectively reach about <span class="hlt">2</span>.01, 1.83, <span class="hlt">2</span>.43 and <span class="hlt">2</span>.12 times of the equivalent <span class="hlt">air</span>-jet values, which confirmed the applicability of impinging mist-jet for heat <span class="hlt">transfer</span> enhancement. The optimal choices of water-to-<span class="hlt">air</span> mass-flow ratio for the atomized mist jet required the considerations of interactive and combined effects of separation distance, <span class="hlt">air</span>-jet Reynolds number and the water-to-<span class="hlt">air</span> mass-flow ratio into the atomized nozzle.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17874769','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17874769"><span><span class="hlt">Air-sea</span> exchange 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 exchange of HHCB and AHTN, suggesting atmospheric input controls the levels of HHCB and AHTN in the polar region.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/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('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 <span class="hlt">transfer</span> 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-exchange with the atmosphere. The deep ocean, on the other hand, can be a sink at least at time scales of the ocean turnover. <span class="hlt">Transfer</span> 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/28567633','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28567633"><span>Technical insight on the requirements for <span class="hlt">CO</span><span class="hlt">2</span>-saturated growth of microalgae in photobioreactors.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yuvraj; Padmanabhan, Padmini</p> <p>2017-06-01</p> <p>Microalgal cultures are usually sparged with <span class="hlt">CO</span> <span class="hlt">2</span> -enriched <span class="hlt">air</span> to preclude <span class="hlt">CO</span> <span class="hlt">2</span> limitation during photoautotrophic growth. However, the <span class="hlt">CO</span> <span class="hlt">2</span> vol% specifically required at operating conditions to meet the carbon requirement of algal cells in photobioreactor is never determined and 1-10% v/v <span class="hlt">CO</span> <span class="hlt">2</span> -enriched <span class="hlt">air</span> is arbitrarily used. A scheme is proposed and experimentally validated for Chlorella vulgaris that allows computing <span class="hlt">CO</span> <span class="hlt">2</span> -saturated growth feasible at given <span class="hlt">CO</span> <span class="hlt">2</span> vol% and volumetric O <span class="hlt">2</span> mass-<span class="hlt">transfer</span> coefficient (k L a) O . <span class="hlt">CO</span> <span class="hlt">2</span> sufficiency in an experiment can be theoretically established to adjust conditions for <span class="hlt">CO</span> <span class="hlt">2</span> -saturated growth. The methodology completely eliminates the requirement of <span class="hlt">CO</span> <span class="hlt">2</span> electrode for online estimation of dissolved <span class="hlt">CO</span> <span class="hlt">2</span> to determine critical <span class="hlt">CO</span> <span class="hlt">2</span> concentration (C crit ), specific <span class="hlt">CO</span> <span class="hlt">2</span> uptake rate (SCUR), and volumetric <span class="hlt">CO</span> <span class="hlt">2</span> mass-<span class="hlt">transfer</span> coefficient (k L a) C required for the governing <span class="hlt">CO</span> <span class="hlt">2</span> mass-<span class="hlt">transfer</span> equation. C crit was estimated from specific O <span class="hlt">2</span> production rate (SOPR) measurements at different dissolved <span class="hlt">CO</span> <span class="hlt">2</span> concentrations. SCUR was calculated from SOPR and photosynthetic quotient (PQ) determined from the balanced stoichiometric equation of growth. Effect of light attenuation and nutrient depletion on biomass estimate is also discussed. Furthermore, a simple design of photosynthetic activity measurement system was used, which minimizes light attenuation by hanging a low depth (ca. 10 mm) culture over the light source.</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/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/2016EGUGA..1810951B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1810951B"><span>Gas <span class="hlt">transfer</span> under high wind and its dependence on wave breaking and <span class="hlt">sea</span> state</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brumer, Sophia; Zappa, Christopher; Fairall, Christopher; Blomquist, Byron; Brooks, Ian; Yang, Mingxi</p> <p>2016-04-01</p> <p>Quantifying greenhouse gas fluxes on regional and global scales relies on parameterizations of the gas <span class="hlt">transfer</span> velocity K. To first order, K is dictated by wind speed (U) and is typically parameterized as a non-linear functions of U. There is however a large spread in K predicted by the traditional parameterizations at high wind speed. This is because a large variety of environmental forcing and processes (Wind, Currents, Rain, Waves, Breaking, Surfactants, Fetch) actually influence K and wind speed alone cannot capture the variability of <span class="hlt">air</span>-water gas exchange. At high wind speed especially, breaking waves become a key factor to take into account when estimating gas fluxes. The High Wind Gas exchange Study (HiWinGS) presents the unique opportunity to gain new insights on this poorly understood aspects of <span class="hlt">air-sea</span> interaction under high winds. The HiWinGS cruise took place in the North Atlantic during October and November 2013. Wind speeds exceeded 15 m s-1 25% of the time, including 48 hrs with U10 > 20 m s-1. Continuous measurements of turbulent fluxes of heat, momentum, and gas (<span class="hlt">CO</span><span class="hlt">2</span>, DMS, acetone and methanol) were taken from the bow of the R/V Knorr. The wave field was sampled by a wave rider buoy and breaking events were tracked in visible imagery was acquired from the port and starboard side of the flying bridge during daylight hours at 20Hz. Taking advantage of the range of physical forcing and wave conditions sampled during HiWinGS, we test existing parameterizations and explore ways of better constraining K based on whitecap coverage, <span class="hlt">sea</span> state and breaking statistics contrasting pure windseas to swell dominated periods. We distinguish between windseas and swell based on a separation algorithm applied to directional wave spectra for mixed <span class="hlt">seas</span>, system alignment is considered when interpreting results. The four gases sampled during HiWinGS ranged from being mostly waterside controlled to almost entirely airside controlled. While bubble-mediated <span class="hlt">transfer</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PolSc..13...13Q','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PolSc..13...13Q"><span>Dimethylsulfide model calibration and parametric sensitivity analysis for the Greenland <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Qu, Bo; Gabric, Albert J.; Zeng, Meifang; Xi, Jiaojiao; Jiang, Limei; Zhao, Li</p> <p>2017-09-01</p> <p><span class="hlt">Sea-to-air</span> fluxes of marine biogenic aerosols have the potential to modify cloud microphysics and regional radiative budgets, and thus moderate Earth's warming. Polar regions play a critical role in the evolution of global climate. In this work, we use a well-established biogeochemical model to simulate the DMS flux from the Greenland <span class="hlt">Sea</span> (20°W-10°E and 70°N-80°N) for the period 2003-2004. Parameter sensitivity analysis is employed to identify the most sensitive parameters in the model. A genetic algorithm (GA) technique is used for DMS model parameter calibration. Data from phase 5 of the Coupled Model Intercomparison Project (CMIP5) are used to drive the DMS model under 4 × <span class="hlt">CO</span><span class="hlt">2</span> conditions. DMS flux under quadrupled <span class="hlt">CO</span><span class="hlt">2</span> levels increases more than 300% compared with late 20th century levels (1 × <span class="hlt">CO</span><span class="hlt">2</span>). Reasons for the increase in DMS flux include changes in the ocean state-namely an increase in <span class="hlt">sea</span> surface temperature (SST) and loss of <span class="hlt">sea</span> ice-and an increase in DMS <span class="hlt">transfer</span> velocity, especially in spring and summer. Such a large increase in DMS flux could slow the rate of warming in the Arctic via radiative budget changes associated with DMS-derived aerosols.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('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 exchanged via the Model Coupling Toolkit. Comparisons are made between the modeled and observed wind velocity, <span class="hlt">sea</span> level pressure, 10 m <span class="hlt">air</span> temperature, and <span class="hlt">sea</span> surface temperature time series, as well as a comparison between the model and one glider transect. Vertical profiles of modeled <span class="hlt">air</span> temperature and winds in the marine atmospheric boundary layer and temperature variations in the upper ocean during a 3-day storm period are examined at various cross-shelf transects along the eastern seaboard. It is found that the air–<span class="hlt">sea</span> interactions near the Gulf Stream are important for generating and sustaining the ETC. In particular, locally enhanced winds over a warm <span class="hlt">sea</span> (relative to the land temperature) induce large surface heat 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 exchanges in ETCs need to be resolved accurately in a coupled atmosphere–ocean modeling framework.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1980Tell...32..470H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1980Tell...32..470H"><span>Gas exchange 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 exchange at the <span class="hlt">air-sea</span> interface are reviewed. In order to describe the <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> 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 exchange with wind speed.</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('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 exchange 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 exchange with the atmosphere. Previous attempts to budget carbon pools in mesocosms relied on educated guesses concerning the exchange 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 exchange in mesocosms using N<span class="hlt">2</span>O as a deliberate tracer. Beside the application for carbon budgeting, <span class="hlt">transfer</span> velocities can be used to calculate exchange 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 exchange measurements provides a guideline for the applicability of the method under various experimental conditions.</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('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/2016AGUFMOS23B2025O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS23B2025O"><span>Field Observations of Coastal <span class="hlt">Air-Sea</span> Interaction</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ortiz-Suslow, D. G.; Haus, B. K.; Williams, N. J.; Graber, H. C.</p> <p>2016-12-01</p> <p>In the nearshore zone wind, waves, and currents generated from different forcing mechanisms converge in shallow water. This can profoundly affect the physical nature of the ocean surface, which can significantly modulate the exchange of momentum, heat, and mass across the <span class="hlt">air-sea</span> interface. For decades, the focus of <span class="hlt">air-sea</span> interaction research has been on the open ocean while the shallow water regime has been relatively under-explored. This bears implications for efforts to understand and model various coastal processes, such as mixing, surface transport, and <span class="hlt">air-sea</span> gas 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/2001AGUFMOS32B0482E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001AGUFMOS32B0482E"><span>The Coupled Boundary Layers and <span class="hlt">Air-Sea</span> <span class="hlt">Transfer</span> (CBLAST) Experiments at the Martha's Vineyard Coastal Observatory</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Edson, J. B.</p> <p>2001-12-01</p> <p>The Woods Hole Oceanographic Institution (WHOI) completed the initial phase of the Martha's Vineyard Coastal Observatory (MVCO) in July of 2001. The MVCO is being using to monitor coastal atmospheric and oceanic processes. Specifically, the observatory is expected to: - Provide continuous long-term observations for climate studies. - Provide a reliable system and rugged sensors that allow opportunistic sampling of extreme events. - Provide a local climatology for intensive, short duration field campaigns. - Further facilitate regional studies of coastal processes by providing infrastructure that supports easy access to power and data. This talk provides an example of the last two objectives using the low wind component of the Office of Naval Research's (ONR) Coupled Boundary Layers and <span class="hlt">Air-Sea</span> <span class="hlt">Transfer</span> (CBLAST) program. CBLAST-LOW has been designed to investigate <span class="hlt">air-sea</span> interaction and coupled atmospheric and oceanic boundary layer dynamics at low wind speeds where the dynamic processes are driven and/or strongly modulated by thermal forcing. This effort is being carried out by scientists at WHOI, NPS, NOAA, NRL, Rutgers, UW/APL, JH/APL, OSU, NCAR, and other institutions, and includes observational and modeling components. The MVCO is providing observations and infrastructure in support of several intensive operating periods in the summers of 2001, 2002, and possibly 2003. During these periods, the observational network around the observatory was and will be greatly expanded using traditional oceanographic moorings and bottom mounted instrumentation, innovative <span class="hlt">2</span>- and 3-D moored and drifting arrays, survey ships, AUVs, satellite remote sensing, and heavily instrumented aircraft. In addition, the MVCO cabled components will be extended out to the 20-m isobath where we plan to deploy a 35-m tower. The tower will be instrumented from 15-m above the ocean surface to the ocean bottom with instruments capable of directly measuring the momentum, heat, and radiative</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/2017APS..DFDL20011S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..DFDL20011S"><span>Boundary layers at a dynamic interface: <span class="hlt">air-sea</span> exchange of heat and mass</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Szeri, Andrew</p> <p>2017-11-01</p> <p>Exchange of mass or heat across a turbulent liquid-gas interface is a problem of critical interest, especially in <span class="hlt">air-sea</span> <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> 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/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/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 exchange 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> <span class="hlt">transfer</span> in the <span class="hlt">sea</span> ice zone, we require accurate estimates of the <span class="hlt">air-sea</span> gas <span class="hlt">transfer</span> velocity. In the open ocean, the gas <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> 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 exchange forcing, which may include a range of <span class="hlt">sea</span> ice cover conditions. Here, we compare individual estimates of the gas <span class="hlt">transfer</span> 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> <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://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/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('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 <span class="hlt">transfer</span>. In order to better understand these fluxes, empirical relationships were developed to quantify the interfacial exchange rates in terms of easily observed parameters (e.g., wind speed). However, mounting evidence suggests that these empirical formulae are only valid over the relatively narrow parametric space, i.e. open ocean conditions in light to moderate winds. Several near-surface processes have been observed to cause significant variance in the <span class="hlt">air-sea</span> 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 exchange; in order to achieve this, a broad investigation into <span class="hlt">air-sea</span> coupling was undertaken. The primary focus of this work was to use a combination of field and laboratory observations and numerical modeling, in regimes where conventional theories would be expected to breakdown, namely: the nearshore and in very high winds. These seemingly disparate environments represent the marine atmospheric boundary layer at its physical limit. In the nearshore, the convergence of land, <span class="hlt">air</span>, and <span class="hlt">sea</span> in a depth-limited domain marks the transition from a marine to a terrestrial boundary layer. Under extreme winds, the physical nature of the boundary layer remains unknown as an intermediate substrate layer, <span class="hlt">sea</span> spray, develops between the atmosphere and ocean surface. At these ends of the MABL physical spectrum, direct measurements of the near-surface processes were made and directly related to local sources of variance. Our results suggest that the conventional treatment of <span class="hlt">air-sea</span> fluxes in terms of empirical relationships developed from a relatively narrow set of</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('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 exchange between <span class="hlt">sea</span> ice and the atmosphere even in mid-winter. Although the potential <span class="hlt">CO</span><span class="hlt">2</span> 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('http://adsabs.harvard.edu/abs/2015Nanos...7.1830L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015Nanos...7.1830L"><span><span class="hlt">Co</span>3O4 nanoparticles decorated carbon nanofiber mat as binder-free <span class="hlt">air</span>-cathode for high performance rechargeable zinc-<span class="hlt">air</span> batteries</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Bing; Ge, Xiaoming; Goh, F. W. Thomas; Hor, T. S. Andy; Geng, Dongsheng; Du, Guojun; Liu, Zhaolin; Zhang, Jie; Liu, Xiaogang; Zong, Yun</p> <p>2015-01-01</p> <p>An efficient, durable and low cost <span class="hlt">air</span>-cathode is essential for a high performance metal-<span class="hlt">air</span> battery for practical applications. Herein, we report a composite bifunctional catalyst, <span class="hlt">Co</span>3O4 nanoparticles-decorated carbon nanofibers (CNFs), working as an efficient <span class="hlt">air</span>-cathode in high performance rechargeable Zn-<span class="hlt">air</span> batteries (ZnABs). The particles-on-fibers nanohybrid materials were derived from electrospun metal-ion containing polymer fibers followed by thermal carbonization and a post annealing process in <span class="hlt">air</span> at a moderate temperature. Electrochemical studies suggest that the nanohybrid material effectively catalyzes oxygen reduction reaction via an ideal 4-electron <span class="hlt">transfer</span> process and outperforms Pt/C in catalyzing oxygen evolution reactions. Accordingly, the prototype ZnABs exhibit a low discharge-charge voltage gap (e.g. 0.7 V, discharge-charge at <span class="hlt">2</span> mA cm-<span class="hlt">2</span>) with higher stability and longer cycle life compared to their counterparts constructed using Pt/C in <span class="hlt">air</span>-cathode. Importantly, the hybrid nanofiber mat readily serves as an integrated <span class="hlt">air</span>-cathode without the need of any further modification. Benefitting from its efficient catalytic activities and structural advantages, particularly the 3D architecture of highly conductive CNFs and the high loading density of strongly attached <span class="hlt">Co</span>3O4 NPs on their surfaces, the resultant ZnABs show significantly improved performance with respect to the rate capability, cycling stability and current density, promising good potential in practical applications.An efficient, durable and low cost <span class="hlt">air</span>-cathode is essential for a high performance metal-<span class="hlt">air</span> battery for practical applications. Herein, we report a composite bifunctional catalyst, <span class="hlt">Co</span>3O4 nanoparticles-decorated carbon nanofibers (CNFs), working as an efficient <span class="hlt">air</span>-cathode in high performance rechargeable Zn-<span class="hlt">air</span> batteries (ZnABs). The particles-on-fibers nanohybrid materials were derived from electrospun metal-ion containing polymer fibers followed by thermal carbonization</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/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> exchange also influence variability. The linear slope of time series p<span class="hlt">CO</span><span class="hlt">2</span>w increases by 5.<span class="hlt">2</span> ± 1.4 μatm y-1 with FCO<span class="hlt">2</span> increasing 51-70 mmol m-<span class="hlt">2</span> y-1. The net FCO<span class="hlt">2</span> sign can switch interannually with the magnitude varying greatly. Non-thermal p<span class="hlt">CO</span><span class="hlt">2</span>w is also increasing over the time series, likely indicating that terrestrial export and net biological processes drive the long term p<span class="hlt">CO</span><span class="hlt">2</span>w increase.</p> </li> </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('https://www.gpo.gov/fdsys/pkg/CFR-2011-title50-vol10/pdf/CFR-2011-title50-vol10-sec648-13.pdf','CFR2011'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2011-title50-vol10/pdf/CFR-2011-title50-vol10-sec648-13.pdf"><span>50 CFR 648.13 - <span class="hlt">Transfers</span> at <span class="hlt">sea</span>.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2011&page.go=Go">Code of Federal Regulations, 2011 CFR</a></p> <p></p> <p>2011-10-01</p> <p>... 50 Wildlife and Fisheries 10 2011-10-01 2011-10-01 false <span class="hlt">Transfers</span> at <span class="hlt">sea</span>. 648.13 Section 648.13... <span class="hlt">sea</span>. Link to an amendment published at 76 FR 60615, Sept. 29, 2011. (a) Only vessels issued a Loligo... receiving vessel possesses a written receipt for any small-mesh multispecies purchased at <span class="hlt">sea</span>. (c) All...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015BGD....1220025L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015BGD....1220025L"><span>Micro- and mesozooplankton community response to increasing <span class="hlt">CO</span><span class="hlt">2</span> levels in the Baltic <span class="hlt">Sea</span>: insights from a large-scale mesocosm experiment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lischka, S.; Bach, L. T.; Schulz, K.-G.; Riebesell, U.</p> <p>2015-12-01</p> <p>Community approaches investigating ocean acidification (OA) effects suggest a high tolerance of micro- and mesozooplankton to carbonate chemistry changes expected to occur within this century. Plankton communities in the coastal areas of the Baltic <span class="hlt">Sea</span> frequently experience pH variations partly exceeding projections for the near future both on a diurnal and seasonal basis, thus some level of tolerance/adaptation may be expected. We conducted a large-scale mesocosm <span class="hlt">CO</span><span class="hlt">2</span> enrichment experiment (~ 55 m3) enclosing the natural plankton community in Tvärminne/Storfjärden for eight weeks during June-August 2012 and studied community and species/taxon response of microzooplankton (ciliates) and mesozooplankton to <span class="hlt">CO</span><span class="hlt">2</span> elevations expected for this century. Besides the response to f<span class="hlt">CO</span><span class="hlt">2</span> and associate changes in carbonate chemistry speciation, we also considered temperature and chlorophyll a variations in our analyses. Shannon diversity of microzooplankton significantly decreased with f<span class="hlt">CO</span><span class="hlt">2</span> and temperature with a greater dominance of smaller species. Small sized ciliates (Myrionecta rubra, Balanion comatum, Strombidium cf. epidemum, Strobilidium sp.) showed significant relations with one or more of the factors. The phototrophic Myrionecta rubra seemed to directly benefit from higher <span class="hlt">CO</span><span class="hlt">2</span> concentrations and showed increased abundance in the pre-bloom phase. With respect to meszooplankton, we neither detected significant effects for total abundance nor for Shannon diversity. The cladocera Bosmina occurred at distinctly higher abundance (more than twice as high compared to the control mesocosms) for a short time period during the second half of the experiment in three of the <span class="hlt">CO</span><span class="hlt">2</span>-enriched mesocosms except for the highest <span class="hlt">CO</span><span class="hlt">2</span> level. The ratio of Bosmina with empty to embryo/resting egg bearing brood chambers, however, was significantly affected by all three factors. An indirect <span class="hlt">CO</span><span class="hlt">2</span> effect via increased food availability stimulating Bosmina reproduction is suggested, but too low</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.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('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/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/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('http://adsabs.harvard.edu/abs/2016AGUFM.A32F..08C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.A32F..08C"><span>Constraining the Stratosphere-Troposphere Exchange of Radiocarbon using <span class="hlt">Air</span>Core 14<span class="hlt">CO</span><span class="hlt">2</span> Measurements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, H.</p> <p>2016-12-01</p> <p>Radiocarbon (14C) plays an important role in the carbon cycle studies to understand both natural and anthropogenic carbon 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 exchange of 14C using the correlation between 14<span class="hlt">CO</span><span class="hlt">2</span> and N<span class="hlt">2</span>O, and the estimated N<span class="hlt">2</span>O loss rate. Besides this, we assess the impact of the mean age of <span class="hlt">air</span> on 14<span class="hlt">CO</span><span class="hlt">2</span> profiles. Furthermore, we will evaluate the influence of different cosmogenic 14C production scenarios and the uncertainties in the OH field on the seasonal cycles of radiocarbon and on the stratosphere-troposphere exchange.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1287223-large-co2-effluxes-night-during-synoptic-weather-events-significantly-contribute-co2-emissions-from-reservoir','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1287223-large-co2-effluxes-night-during-synoptic-weather-events-significantly-contribute-co2-emissions-from-reservoir"><span>Large <span class="hlt">CO</span> <span class="hlt">2</span> effluxes at night and during synoptic weather events significantly contribute to <span class="hlt">CO</span> <span class="hlt">2</span> emissions from a reservoir</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Liu, Heping; Zhang, Qianyu; Katul, Gabriel G.; ...</p> <p>2016-05-24</p> <p><span class="hlt">CO</span> <span class="hlt">2</span> emissions from inland waters are commonly determined by indirect methods that are based on the product of a gas <span class="hlt">transfer</span> coefficient and the concentration gradient at the <span class="hlt">air</span> water interface (e.g., wind-based gas <span class="hlt">transfer</span> models). The measurements of concentration gradient are typically collected during the day in fair weather throughout the course of a year. Direct measurements of eddy covariance <span class="hlt">CO</span> <span class="hlt">2</span> fluxes from a large inland water body (Ross Barnett reservoir, Mississippi, USA) show that <span class="hlt">CO</span> <span class="hlt">2</span> effluxes at night are approximately 70% greater than those during the day. At longer time scales, frequent synoptic weather eventsmore » associated with extratropical cyclones induce <span class="hlt">CO</span> <span class="hlt">2</span> flux pulses, resulting in further increase in annual <span class="hlt">CO</span> <span class="hlt">2</span> effluxes by 16%. Therefore, <span class="hlt">CO</span> <span class="hlt">2</span> emission rates from this reservoir, if these diel and synoptic processes are under-sampled, are likely to be underestimated by approximately 40%. Our results also indicate that the <span class="hlt">CO</span> <span class="hlt">2</span> emission rates from global inland waters reported in the literature, when based on indirect methods, are likely underestimated. Field samplings and indirect modeling frameworks that estimate <span class="hlt">CO</span> <span class="hlt">2</span> emissions should account for both daytime-nighttime efflux difference and enhanced emissions during synoptic weather events. Furthermore, the analysis here can guide carbon emission sampling to improve regional carbon estimates.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1287223','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1287223"><span>Large <span class="hlt">CO</span> <span class="hlt">2</span> effluxes at night and during synoptic weather events significantly contribute to <span class="hlt">CO</span> <span class="hlt">2</span> emissions from a reservoir</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>Liu, Heping; Zhang, Qianyu; Katul, Gabriel G.</p> <p></p> <p><span class="hlt">CO</span> <span class="hlt">2</span> emissions from inland waters are commonly determined by indirect methods that are based on the product of a gas <span class="hlt">transfer</span> coefficient and the concentration gradient at the <span class="hlt">air</span> water interface (e.g., wind-based gas <span class="hlt">transfer</span> models). The measurements of concentration gradient are typically collected during the day in fair weather throughout the course of a year. Direct measurements of eddy covariance <span class="hlt">CO</span> <span class="hlt">2</span> fluxes from a large inland water body (Ross Barnett reservoir, Mississippi, USA) show that <span class="hlt">CO</span> <span class="hlt">2</span> effluxes at night are approximately 70% greater than those during the day. At longer time scales, frequent synoptic weather eventsmore » associated with extratropical cyclones induce <span class="hlt">CO</span> <span class="hlt">2</span> flux pulses, resulting in further increase in annual <span class="hlt">CO</span> <span class="hlt">2</span> effluxes by 16%. Therefore, <span class="hlt">CO</span> <span class="hlt">2</span> emission rates from this reservoir, if these diel and synoptic processes are under-sampled, are likely to be underestimated by approximately 40%. Our results also indicate that the <span class="hlt">CO</span> <span class="hlt">2</span> emission rates from global inland waters reported in the literature, when based on indirect methods, are likely underestimated. Field samplings and indirect modeling frameworks that estimate <span class="hlt">CO</span> <span class="hlt">2</span> emissions should account for both daytime-nighttime efflux difference and enhanced emissions during synoptic weather events. Furthermore, the analysis here can guide carbon emission sampling to improve regional carbon estimates.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFMOS34B..01S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMOS34B..01S"><span>Tropical Cyclone Induced <span class="hlt">Air-Sea</span> Interactions Over Oceanic Fronts</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shay, L. K.</p> <p>2012-12-01</p> <p>Recent severe tropical cyclones underscore the inherent importance of warm background ocean fronts and their interactions with the atmospheric boundary layer. Central to the question of heat and moisture fluxes, the amount of heat available to the tropical cyclone is predicated by the initial mixed layer depth and strength of the stratification that essentially set the level of entrainment mixing at the base of the mixed layer. In oceanic regimes where the ocean mixed layers are thin, shear-induced mixing tends to cool the upper ocean to form cold wakes which reduces the <span class="hlt">air-sea</span> fluxes. This is an example of negative feedback. By contrast, in regimes where the ocean mixed layers are deep (usually along the western part of the gyres), warm water advection by the nearly steady currents reduces the levels of turbulent mixing by shear instabilities. As these strong near-inertial shears are arrested, more heat and moisture <span class="hlt">transfers</span> are available through the enthalpy fluxes (typically 1 to 1.5 kW m-<span class="hlt">2</span>) into the hurricane boundary layer. When tropical cyclones move into favorable or neutral atmospheric conditions, tropical cyclones have a tendency to rapidly intensify as observed over the Gulf of Mexico during Isidore and Lili in 2002, Katrina, Rita and Wilma in 2005, Dean and Felix in 2007 in the Caribbean <span class="hlt">Sea</span>, and Earl in 2010 just north of the Caribbean Islands. To predict these tropical cyclone deepening (as well as weakening) cycles, coupled models must have ocean models with realistic ocean conditions and accurate <span class="hlt">air-sea</span> and vertical mixing parameterizations. Thus, to constrain these models, having complete 3-D ocean profiles juxtaposed with atmospheric profiler measurements prior, during and subsequent to passage is an absolute necessity framed within regional scale satellite derived fields.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('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> exchange. We conducted 13 cruises in the northern Gulf of Mexico, a region strongly influenced by fresh water and nutrients delivered from the Mississippi and Atchafalaya River system. The <span class="hlt">sea</span> surface partial pressure of carbon dioxide (p<span class="hlt">CO</span><span class="hlt">2</span>) was measured, and the air‐<span class="hlt">sea</span> <span class="hlt">CO</span><span class="hlt">2</span> flux was calculated. Results show that <span class="hlt">CO</span><span class="hlt">2</span> exchange exhibited a distinct seasonality: the study area was a net sink of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> during spring and early summer, and it was neutral or a weak source of <span class="hlt">CO</span><span class="hlt">2</span> to the atmosphere during midsummer, fall, and winter. Along the salinity gradient, across the shelf, the <span class="hlt">sea</span> surface shifted from a source of <span class="hlt">CO</span><span class="hlt">2</span> in low‐salinity zones (0≤S<17) to a strong <span class="hlt">CO</span><span class="hlt">2</span> sink in the middle‐to‐high‐salinity zones (17≤S<33), and finally was a near‐neutral state in the high‐salinity areas (33≤S<35) and in the open gulf (S≥35). High p<span class="hlt">CO</span><span class="hlt">2</span> values were only observed in narrow regions near freshwater sources, and the distribution of undersaturated p<span class="hlt">CO</span><span class="hlt">2</span> generally reflected the influence of freshwater inputs along the shelf. Systematic analyses of p<span class="hlt">CO</span><span class="hlt">2</span> variation demonstrated the importance of riverine nitrogen export; that is, riverine nitrogen‐enhanced biological removal, along with mixing processes, dominated p<span class="hlt">CO</span><span class="hlt">2</span> variation along the salinity gradient. In addition, extreme or unusual weather events were observed to alter the alongshore p<span class="hlt">CO</span><span class="hlt">2</span> distribution and to affect regional air‐<span class="hlt">sea</span> <span class="hlt">CO</span><span class="hlt">2</span> 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/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 exchange 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.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://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('https://pubs.er.usgs.gov/publication/70021683','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70021683"><span>Estimating lake-atmosphere <span class="hlt">CO</span><span class="hlt">2</span> exchange</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Anderson, D.E.; Striegl, Robert G.; Stannard, D.I.; Michmerhuizen, C.M.; McConnaughey, T.A.; LaBaugh, J.W.</p> <p>1999-01-01</p> <p>Lake-atmosphere <span class="hlt">CO</span><span class="hlt">2</span> 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 exchanges of <span class="hlt">CO</span><span class="hlt">2</span> were measured over 5 weeks in spring, summer, and fall. Observed springtime <span class="hlt">CO</span><span class="hlt">2</span> efflux was large (<span class="hlt">2.3-2</span>.7 ??mol m-<span class="hlt">2</span> s-1) immediately after lake-thaw. That efflux decreased exponentially with time to less than 0.<span class="hlt">2</span> ??mol m-<span class="hlt">2</span> s-1 within <span class="hlt">2</span> weeks. Substantial interannual variability was found in the magnitudes of springtime efflux, surface water <span class="hlt">CO</span><span class="hlt">2</span> concentrations, lake <span class="hlt">CO</span><span class="hlt">2</span> storage, and meteorological conditions. Summertime measurements show a weak diurnal trend with a small average downward 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-<span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> 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/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> </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('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/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('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('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> exchange during Bora high wind events. The unique combination of these environmental processes and relatively small size of the area makes the region an excellent study site for investigations of <span class="hlt">air-sea</span> interaction, and changes in biology and carbon chemistry. However, there is a dearth of current data or information from the region. Here we present the first measurements of <span class="hlt">air</span> and water <span class="hlt">CO</span><span class="hlt">2</span> 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> <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('https://www.ncbi.nlm.nih.gov/pubmed/11890817','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/11890817"><span>Molecular structures and excited states of CpM(<span class="hlt">CO</span>)(<span class="hlt">2</span>) (Cp = eta(5)-C(5)H(5); M = Rh, Ir) and [Cl(<span class="hlt">2</span>)Rh(<span class="hlt">CO</span>)(<span class="hlt">2</span>)](-). Theoretical evidence for a competitive charge <span class="hlt">transfer</span> mechanism.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hu, Zhenming; Boyd, Russell J; Nakatsuji, Hiroshi</p> <p>2002-03-20</p> <p>Molecular structures and excited states of CpM(<span class="hlt">CO</span>)(<span class="hlt">2</span>) (Cp = eta(5)-C(5)H(5); M = Rh, Ir) and [Cl(<span class="hlt">2</span>)Rh(<span class="hlt">CO</span>)(<span class="hlt">2</span>)](-) complexes have been investigated using the B3LYP and the symmetry-adapted cluster (SAC)/SAC-configuration interaction (SAC-CI) theoretical methods. All the dicarbonyl complexes have singlet ground electronic states with large singlet-triplet separations. Thermal dissociations of <span class="hlt">CO</span> from the parent dicarbonyls are energetically unfavorable. <span class="hlt">CO</span> thermal dissociation is an activation process for [Cl(<span class="hlt">2</span>)Rh(<span class="hlt">CO</span>)(<span class="hlt">2</span>)](-) while it is a repulsive potential for CpM(<span class="hlt">CO</span>)(<span class="hlt">2</span>). The natures of the main excited states of CpM(<span class="hlt">CO</span>)(<span class="hlt">2</span>) and [Cl(<span class="hlt">2</span>)Rh(<span class="hlt">CO</span>)(<span class="hlt">2</span>)](-) are found to be quite different. For [Cl(<span class="hlt">2</span>)Rh(<span class="hlt">CO</span>)(<span class="hlt">2</span>)](-), all the strong transitions are identified to be metal to ligand <span class="hlt">CO</span> charge <span class="hlt">transfer</span> (MLCT) excitations. A significant feature of the excited states of CpM(<span class="hlt">CO</span>)(<span class="hlt">2</span>) is that both MLCT excitation and a ligand Cp to metal and <span class="hlt">CO</span> charge <span class="hlt">transfer</span> excitation are strongly mixed in the higher energy states with the latter having the largest oscillator strength. A competitive charge <span class="hlt">transfer</span> excited state has therefore been identified theoretically for CpRh(<span class="hlt">CO</span>)(<span class="hlt">2</span>) and CpIr(<span class="hlt">CO</span>)(<span class="hlt">2</span>). The wavelength dependence of the quantum efficiencies for the photoreactions of CpM(<span class="hlt">CO</span>)(<span class="hlt">2</span>) reported by Lees et al. can be explained by the existence of two different types of excited states. The origin of the low quantum efficiencies for the C-H/S-H bond activations of CpM(<span class="hlt">CO</span>)(<span class="hlt">2</span>) can be attributed to the smaller proportion of the MLCT excitation in the higher energy states.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1910878A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1910878A"><span>In situ observations of ocean productivity using the <span class="hlt">Sea</span>Cycler mooring in the central Labrador <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Atamanchuk, Dariia; Koelling, Jannes; Devred, Emmanuel; Siddall, Greg; Send, Uwe; Wallace, Douglas</p> <p>2017-04-01</p> <p>The Central Labrador <span class="hlt">Sea</span> is a major deep-convection region in the NW Atlantic which is the most intense sink for anthropogenic carbon in the global ocean (de Vries et al, 2013). <span class="hlt">CO</span><span class="hlt">2</span> enters the ocean by <span class="hlt">air-sea</span> exchange and is transported into the ocean's interior mainly though the biological pump (Longhurst et al., 1989). Despite its important role for <span class="hlt">CO</span><span class="hlt">2</span> uptake and high natural variability, the Labrador <span class="hlt">Sea</span> is undersampled due to rough conditions and an overall lack of volunteer observing ship (VOS) transits. The <span class="hlt">Sea</span>Cycler moored profiler is currently providing year-round data from the central Labrador <span class="hlt">Sea</span> and resolves daily changes of inorganic carbon and related properties from the upper 150m of the water column. <span class="hlt">Sea</span>Cycler's sensor float is equipped with 13 physical, chemical and biooptical sensors which measure temperature, salinity, dissolved gases, nutrients and optical properties of seawater. A combination of Pro-CV (Pro-Oceanus Inc, Canada) and <span class="hlt">CO</span><span class="hlt">2</span> optode (Aanderaa, Norway) sensors in profiling mode provides a detailed description of Dissolved Inorganic Carbon (DIC) dynamics in the upper 150m over the productive season. This allows, for the first time, high-resolution carbon-based estimates of ocean productivity from throughout the euphotic zone over an annual cycle which can be compared to estimates derived from simultaneous oxygen and nitrate (Deep SUNA, Satlantic LP, Canada) profiles. These in situ carbon, nitrogen and oxygen-based estimates of using in-situ data are further compared with remotely-sensed estimates from MODIS satellite data. The <span class="hlt">Sea</span>Cycler data allow estimation of the annual cycle of the <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> 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/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/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('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('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 exchange 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 exchange 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/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://www.dtic.mil/docs/citations/ADA488079','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA488079"><span>At <span class="hlt">Sea</span> Personnel <span class="hlt">Transfer</span> Concepts</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2006-07-28</p> <p><span class="hlt">transfer</span> at <span class="hlt">sea</span>. Personnel can be <span class="hlt">transferred</span> with relatively short notice using a 4” double braided , polyester synthetic highline instead of steel...supporting 1000 lbs at the tip of the ladder, and sustaining a 60000 gal/hr hose firing at any angle. The ladders are capable of supporting this...significant burden for the bridges. To further reduce the tip weight, the vacuum pumps will be stored on the deck of the ship and hosing will be run</p> </li> <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('https://www.ncbi.nlm.nih.gov/pubmed/27617333','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27617333"><span>Persistent organochlorine pesticides and polychlorinated biphenyls in <span class="hlt">air</span> of the North <span class="hlt">Sea</span> region and <span class="hlt">air-sea</span> exchange.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mai, Carolin; Theobald, Norbert; Hühnerfuss, Heinrich; Lammel, Gerhard</p> <p>2016-12-01</p> <p>Organochlorine pesticides (OCPs) and polychlorinated biphenyls (PCBs) were studied to determine occurrence, levels and spatial distribution in the marine atmosphere and surface seawater during cruises in the German Bight and the wider North <span class="hlt">Sea</span> in spring and summer 2009-2010. In general, the concentrations found in <span class="hlt">air</span> are similar to, or below, the levels at coastal or near-coastal sites in Europe. Hexachlorobenzene and α-hexachlorocyclohexane (α-HCH) were close to phase equilibrium, whereas net atmospheric deposition was observed for γ-HCH. The results suggest that declining trends of HCH in seawater have been continuing for γ-HCH but have somewhat levelled off for α-HCH. Dieldrin displayed a close to phase equilibrium in nearly all the sampling sites, except in the central southwestern part of the North <span class="hlt">Sea</span>. Here atmospheric deposition dominates the <span class="hlt">air-sea</span> exchange. This region, close to the English coast, showed remarkably increased surface seawater concentrations. This observation depended neither on riverine input nor on the elevated abundances of dieldrin in the <span class="hlt">air</span> masses of central England. A net depositional 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('https://www.osti.gov/biblio/5852468-mechanism-energy-conversion-transfer-bioluminescence-final-report-sea-pansy-renilla-reniformis','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5852468-mechanism-energy-conversion-transfer-bioluminescence-final-report-sea-pansy-renilla-reniformis"><span>Mechanism of energy conversion and <span class="hlt">transfer</span> in bioluminescence. Final report. [<span class="hlt">Sea</span> pansy Renilla reniformis</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>Cormier, M.J.</p> <p>1979-01-01</p> <p>Bioluminescence in the <span class="hlt">sea</span> pansy, Renilla reniformis, a marine anthozoan coelenterate, is a complex process involving the participation of three proteins specific to anthozoan coelenterate-type systems. These are: (1) the luciferin binding protein, (<span class="hlt">2</span>) the enzyme luciferase, and (3) the green-fluorescent protein. Each of these have been purified and characterized and the structure of luciferin has been confirmed by synthesis. Luciferin binding protein (BP-LH/sub <span class="hlt">2</span>/) is a specific substrate binding protein which binds one molecule of coelenterate-type luciferin per molecule of protein and which then releases luciferin in the presence of Ca/sup + +/. Luciferase is the enzyme which catalyzesmore » oxidation (by O/sub <span class="hlt">2</span>/) of coelenterate-type luciferin, leading to the production of <span class="hlt">CO</span>/sub <span class="hlt">2</span>/ and enzyme-bound, excited-state oxyluciferin. Oxyluciferin may then emit blue light by a direct de-excitation pathway or may <span class="hlt">transfer</span> excitation energy to the green-fluorescent protein (GFP). GFP is a non-catalytic accessory protein which accepts excitation energy from oxyluciferin, by radiationless energy <span class="hlt">transfer</span>, and then emits green bioluminescence. The Renilla bioluminescence system is thus the first radiationless energy <span class="hlt">transfer</span> system the individual components of which have been purified to homogeneity, characterized, and then reassembled in vitro with restoration of the energy <span class="hlt">transfer</span> function.« less</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> </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/2012JGRC..117.5035A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012JGRC..117.5035A"><span>Statistics of surface divergence and their relation to <span class="hlt">air</span>-water gas <span class="hlt">transfer</span> velocity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Asher, William E.; Liang, Hanzhuang; Zappa, Christopher J.; Loewen, Mark R.; Mukto, Moniz A.; Litchendorf, Trina M.; Jessup, Andrew T.</p> <p>2012-05-01</p> <p><span class="hlt">Air-sea</span> gas fluxes are generally defined in terms of the <span class="hlt">air</span>/water concentration difference of the gas and the gas <span class="hlt">transfer</span> velocity,kL. Because it is difficult to measure kLin the ocean, it is often parameterized using more easily measured physical properties. Surface divergence theory suggests that infrared (IR) images of the water surface, which contain information concerning the movement of water very near the <span class="hlt">air</span>-water interface, might be used to estimatekL. Therefore, a series of experiments testing whether IR imagery could provide a convenient means for estimating the surface divergence applicable to <span class="hlt">air-sea</span> exchange were conducted in a synthetic jet array tank embedded in a wind tunnel. Gas <span class="hlt">transfer</span> velocities were measured as a function of wind stress and mechanically generated turbulence; laser-induced fluorescence was used to measure the concentration of carbon dioxide in the top 300 μm of the water surface; IR imagery was used to measure the spatial and temporal distribution of the aqueous skin temperature; and particle image velocimetry was used to measure turbulence at a depth of 1 cm below the <span class="hlt">air</span>-water interface. It is shown that an estimate of the surface divergence for both wind-shear driven turbulence and mechanically generated turbulence can be derived from the surface skin temperature. The estimates derived from the IR images are compared to velocity field divergences measured by the PIV and to independent estimates of the divergence made using the laser-induced fluorescence data. Divergence is shown to scale withkLvalues measured using gaseous tracers as predicted by conceptual models for both wind-driven and mechanically generated turbulence.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhDT........20S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhDT........20S"><span>Multiple Electron Charge <span class="hlt">Transfer</span> Chemistries for Electrochemical Energy Storage Systems: The Metal Boride and Metal <span class="hlt">Air</span> Battery</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stuart, Jessica F.</p> <p></p> <p>The primary focus of this work has been to develop high-energy capacity batteries capable of undergoing multiple electron charge <span class="hlt">transfer</span> redox reactions to address the growing demand for improved electrical energy storage systems that can be applied to a range of applications. As the levels of carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) increase in the Earth's atmosphere, the effects on climate change become increasingly apparent. According to the Energy Information Administration (EIA), the U.S. electric power sector is responsible for the release of <span class="hlt">2</span>,039 million metric tons of <span class="hlt">CO</span><span class="hlt">2</span> annually, equating to 39% of total U.S. energy-related <span class="hlt">CO</span><span class="hlt">2</span> emissions. Both nationally and abroad, there are numerous issues associated with the generation and use of electricity aside from the overwhelming dependence on fossil fuels and the subsequent carbon emissions, including reliability of the grid and the utilization of renewable energies. Renewable energy makes up a relatively small portion of total energy contributions worldwide, accounting for only 13% of the 3,955 billion kilowatt-hours of electricity produced each year, as reported by the EIA. As the demand to reduce our dependence on fossils fuels and transition to renewable energy sources increases, cost effective large-scale electrical energy storage must be established for renewable energy to become a sustainable option for the future. A high capacity energy storage system capable of leveling the intermittent nature of energy sources such as solar, wind, and water into the electric grid and provide electricity at times of high demand will facilitate this transition. In 2008, the Licht Group presented the highest volumetric energy capacity battery, the vanadium diboride (VB<span class="hlt">2</span>) <span class="hlt">air</span> battery, exceedingly proficient in <span class="hlt">transferring</span> eleven electrons per molecule. This body of work focuses on new developments to this early battery such as fundamentally understanding the net discharge mechanism of the system, evaluation of the properties and</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/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('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/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> <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.osti.gov/biblio/22258772-first-principles-study-spin-transfer-torque-co-sub-mnsi-al-co-sub-mnsi-spin-valve','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22258772-first-principles-study-spin-transfer-torque-co-sub-mnsi-al-co-sub-mnsi-spin-valve"><span>First-principles study of spin-<span class="hlt">transfer</span> torque in <span class="hlt">Co</span>{sub <span class="hlt">2</span>}MnSi/Al/<span class="hlt">Co</span>{sub <span class="hlt">2</span>}MnSi 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>Tang, Ling, E-mail: lingtang@zjut.edu.cn; Yang, Zejin, E-mail: zejinyang@zjut.edu.cn</p> <p></p> <p>The spin-<span class="hlt">transfer</span> torque (STT) in <span class="hlt">Co</span>{sub <span class="hlt">2</span>}MnSi(CMS)/Al/<span class="hlt">Co</span>{sub <span class="hlt">2</span>}MnSi spin-valve system with and without interfacial disorder is studied by a first-principles noncollinear wave-function-matching method. It is shown that in the case of clean interface the angular dependence of STT for <span class="hlt">CoCo</span>/Al (the asymmetry parameter Λ≈4.5) is more skewed than that for MnSi/Al (Λ≈<span class="hlt">2</span>.9), which suggests the clean <span class="hlt">CoCo</span>/Al architecture is much more efficient for the application on radio frequency oscillation. We also find that even with interfacial disorder the spin-valve of half-metallic CMS still has a relatively large parameter Λ compared to that of conventional ferromagnet. In addition, for clean interfacemore » the in-plane torkance of MnSi/Al is about twice as large as that of <span class="hlt">CoCo</span>/Al. However, as long as the degree of interfacial disorder is sufficiently large, the <span class="hlt">CoCo</span>/Al and MnSi/Al will show approximately the same magnitude of in-plane torkance. Furthermore, our results demonstrate that CMS/Al/CMS system has very high efficiency of STT to switch the magnetic layer of spin-valve.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19930000880','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19930000880"><span><span class="hlt">Air-sea</span> interaction and remote sensing</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Katsaros, Kristina B.; Ataktuerk, Serhad S.</p> <p>1992-01-01</p> <p>The first part of the proposed research was a joint effort between our group and the Applied Physics Laboratory (APL), University of Washington. Our own research goal is to investigate the relation between the <span class="hlt">air-sea</span> exchange processes and the <span class="hlt">sea</span> state over the open ocean and to compare these findings with our previous results obtained over a small body of water namely, Lake Washington. The goals of the APL researchers are to study (1) the infrared <span class="hlt">sea</span> surface temperature (SST) signature of breaking waves and surface slicks, and (<span class="hlt">2</span>) microwave and acoustic scattering from water surface. The task of our group in this joint effort is to conduct measurements of surface 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('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('http://hdl.handle.net/2060/19980003332','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19980003332"><span>Measurement of Momentum <span class="hlt">Transfer</span> Coefficients for H<span class="hlt">2</span>, N<span class="hlt">2</span>, <span class="hlt">CO</span>, and <span class="hlt">CO</span><span class="hlt">2</span> Incident Upon Spacecraft Surfaces</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Cook, Steven R.; Hoffbauer, Mark A.</p> <p>1997-01-01</p> <p>Measurements of momentum <span class="hlt">transfer</span> coefficients were made for gas-surface interactions between the Space Shuttle reaction control jet plume gases and the solar panel array materials to be used on the International Space Station. Actual conditions were simulated using a supersonic nozzle source to produce beams of the gases with approximately the same average velocities as the gases have in the Shuttle plumes. Samples of the actual solar panel materials were mounted on a torsion balance that was used to measure the force exerted on the surfaces by the molecular beams. Measurements were made with H<span class="hlt">2</span>, N<span class="hlt">2</span>, <span class="hlt">CO</span>, and <span class="hlt">CO</span><span class="hlt">2</span> incident upon the solar array material, Kapton, SiO<span class="hlt">2</span>-coated Kapton, and Z93-coated Al. The measurements showed that molecules scatter from the surfaces more specularly as the angle of incidence increases and that the scattering behavior has a strong dependence upon both the incident gas and velocity. These results show that for some technical surfaces the simple assumption of diffuse scattering with complete thermal accommodation is entirely inadequate. It is clear that additional measurements are required to produce models that more accurately describe the gas-surface interactions encountered in rarefied flow regimes.</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 exchange 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('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('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> exchange 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('http://hdl.handle.net/2060/20040110936','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20040110936"><span>Hypervelocity Heat-<span class="hlt">Transfer</span> Measurements in an Expansion Tube</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hollis, Brian R.; Perkins, John N.</p> <p>1996-01-01</p> <p>A series of experiments has been conducted in the NASA HYPULSE Expansion Tube, in both <span class="hlt">CO</span><span class="hlt">2</span> and <span class="hlt">air</span> test gases, in order to obtain data for comparison with computational results and to assess the capability for performing hypervelocity heat-<span class="hlt">transfer</span> studies in this facility. Heat-<span class="hlt">transfer</span> measurements were made in both test gases on 70 deg sphere-cone models and on hemisphere models of various radii. HYPULSE freestream flow conditions in these test gases were found to be repeatable to within 3-10%, and aerothermodynamic test times of 150 microsec in <span class="hlt">CO</span><span class="hlt">2</span> and 125 microsec in <span class="hlt">air</span> were identified. Heat-<span class="hlt">transfer</span> measurement uncertainty was estimated to be 10-15%. Comparisons were made with computational results from the non-equilibrium Navier-Stokes solver NEQ<span class="hlt">2</span>D. Measured and computed heat-<span class="hlt">transfer</span> rates agreed to within 10% on the hemispheres and on the sphere-cone forebodies, and to within 10% in <span class="hlt">CO</span><span class="hlt">2</span> and 25% in <span class="hlt">air</span> on the afterbodies and stings of the sphere-cone models.</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('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> </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('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('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> exchanges, <span class="hlt">sea</span> ice is a net <span class="hlt">CO</span><span class="hlt">2</span> source and sink in winter and summer, respectively. The formulation of the ice-atmosphere <span class="hlt">CO</span><span class="hlt">2</span> 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> exchanges, <span class="hlt">sea</span> ice is a net <span class="hlt">CO</span><span class="hlt">2</span> source and sink in winter and summer, respectively. The formulation of the ice-atmosphere <span class="hlt">CO</span><span class="hlt">2</span> 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('https://ntrs.nasa.gov/search.jsp?R=19850005886&hterms=heat+exchange&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dheat%2Bexchange','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19850005886&hterms=heat+exchange&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dheat%2Bexchange"><span><span class="hlt">Air-sea</span> heat exchange, an element of the water cycle</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chahine, M. T.</p> <p>1984-01-01</p> <p>The distribution and variation of water vapor, clouds and precipitation are examined. Principal driving forces for these distributions are energy exchange and evaporation at the <span class="hlt">air-sea</span> interface, which are also important elements of <span class="hlt">air-sea</span> interaction studies. The overall aim of <span class="hlt">air-sea</span> interaction studies is to quantitatively determine mass, momentum and energy 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> exchanges 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://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('http://hdl.handle.net/2060/19830018879','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19830018879"><span>Heat-<span class="hlt">transfer</span> distributions on biconics at incidence in hypersonic-hypervelocity He, N<span class="hlt">2</span>, <span class="hlt">air</span>, and <span class="hlt">CO</span><span class="hlt">2</span> flows</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Miller, C. G.; Micol, J. R.; Gnoffo, P. A.; Wilder, S. E.</p> <p>1983-01-01</p> <p>Laminar heat <span class="hlt">transfer</span> rates were measured on spherically blunted, 13 deg/7 deg on axis and bent biconics (fore cone bent 7 deg upward relative to aft cone) at hypersonic hypervelocity flow conditions in the Langley Expansion Tube. Freestream velocities from 4.5 to 6.9 km/sec and Mach numbers from 6 to 9 were generated using helium, nitrogen, <span class="hlt">air</span>, and carbon dioxide test gases, resulting in normal shock density ratios from 4 to 19. Angle of attack, referenced to the axis of the aft cone, was varied from 0 to 20 deg in 4 deg increments. The effect of nose bend, angle of attack, and real gas phenomena on heating distributions are presented along with comparisons of measurement to prediction from a code which solves the three dimensional parabolized Navier-Stokes equations.</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/2017IJT....38..170H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017IJT....38..170H"><span>Comparative Investigation on the Heat <span class="hlt">Transfer</span> Characteristics of Gaseous <span class="hlt">CO</span><span class="hlt">2</span> and Gaseous Water Flowing Through a Single Granite Fracture</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>He, Yuanyuan; Bai, Bing; Li, Xiaochun</p> <p>2017-11-01</p> <p><span class="hlt">CO</span><span class="hlt">2</span> and water are two commonly employed heat transmission fluids in several fields. Their temperature and pressure determine their phase states, thus affecting the heat <span class="hlt">transfer</span> performance of the water/<span class="hlt">CO</span><span class="hlt">2</span>. The heat <span class="hlt">transfer</span> characteristics of gaseous <span class="hlt">CO</span><span class="hlt">2</span> and gaseous water flowing through fractured hot dry rock still need a great deal of investigation, in order to understand and evaluate the heat extraction in enhanced geothermal systems. In this work, we develop a <span class="hlt">2</span>D numerical model to compare the heat <span class="hlt">transfer</span> performance of gaseous <span class="hlt">CO</span><span class="hlt">2</span> and gaseous water flowing through a single fracture aperture of 0.<span class="hlt">2</span> mm in a φ 50 × 50 mm cylindrical granite sample with a confining temperature of 200°C under different inlet mass flow rates. Our results indicate that: (1) the final outlet temperatures of the fluid are very close to the outer surface temperature under low inlet mass flow rate, regardless of the sample length. (<span class="hlt">2</span>) Both the temperature of the fluid (gaseous <span class="hlt">CO</span><span class="hlt">2</span>/gaseous water) and inner surface temperature rise sharply at the inlet, and the inner surface temperature is always higher than the fluid temperature. However, their temperature difference becomes increasingly small. (3) Both the overall heat <span class="hlt">transfer</span> coefficient (OHTC) and local heat <span class="hlt">transfer</span> coefficient (LHTC) of gaseous <span class="hlt">CO</span><span class="hlt">2</span> and gaseous water increase with increasing inlet mass flow rates. (4) Both the OHTC and LHTC of gaseous <span class="hlt">CO</span><span class="hlt">2</span> are lower than those of gaseous water under the same conditions; therefore, the heat mining performance of gaseous water is superior to gaseous <span class="hlt">CO</span><span class="hlt">2</span> under high temperature and low pressure.</p> </li> <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/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('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> exchange was also detected, due to the combined effects of seawater temperature, river discharge, and water circulation. On annual scale the system was a sink of atmospheric <span class="hlt">CO</span><span class="hlt">2</span>. However, in summer and during elevated riverine discharges, the area close to the river's mouth acted as a source of carbon dioxide. Also the wind speed was crucial in controlling the <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.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/2018AIPC.1942n0005P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AIPC.1942n0005P"><span>Energy <span class="hlt">transfer</span> mechanism of Sm3+/Eu3+ <span class="hlt">co</span>-doped <span class="hlt">2</span>CaO-B<span class="hlt">2</span>O3-P<span class="hlt">2</span>O5 phosphors</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Prasad, V. Reddy; Damodaraiah, S.; Ratnakaram, Y. C.</p> <p>2018-04-01</p> <p>Sm3+/Eu3+ <span class="hlt">co</span>-doped calcium borophosphate phosphors were synthesized by solid state reaction method. <span class="hlt">2</span>CaO-B<span class="hlt">2</span>O3-P<span class="hlt">2</span>O5: Sm3+/Eu3+ <span class="hlt">co</span>-doped phosphors were characterized by XRD, SEM, 31P solid state NMR, excitation, photoluminescence (PL) and decay profiles.. XRD profiles showed that the prepared phosphors exhibit a hexagonal phase in crystal structure and SEM results showed that the particles are more irregular morphologies. From 31P NMR spectra of Sm3+/Eu3+ <span class="hlt">co</span>-doped <span class="hlt">2</span>CaO-B<span class="hlt">2</span>O3-P<span class="hlt">2</span>O5 phosphors, the chemical shifts located in the positive frequency region indicating the presence of mono-phosphate complexes Q0-(PO43 - ) . Photoluminescence spectra of Sm3+/Eu3+ <span class="hlt">co</span>-doped <span class="hlt">2</span>CaO-B<span class="hlt">2</span>O3-P<span class="hlt">2</span>O5 phosphors show enhancement in emission intensity of Eu3+ ion due to <span class="hlt">co</span>-doping with Sm3+ ions through energy <span class="hlt">transfer</span> process. The energy level mechanism between Sm3+ and Eu3+ ions has been clearly explained. The energy <span class="hlt">transfer</span> process has also been evidenced by lifetime decay profiles. These results suggest that the prepared phosphors are potential red luminescent optical materials.</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/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('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 exchange processes, biogeochemical responses to dust depositions and its modeling. We also</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('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://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> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_16 --> <div id="page_17" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li class="active"><span>17</span></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="321"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/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('http://adsabs.harvard.edu/abs/2016AGUFM.C31D..07M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C31D..07M"><span><span class="hlt">Sea</span> Ice Retreat and its Impact on the Intensity of Open-Ocean Convection in the Greenland and Iceland <span class="hlt">Seas</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moore, K.; Våge, K.; Pickart, R. S.; Renfrew, I.</p> <p>2016-12-01</p> <p>The <span class="hlt">air-sea</span> <span class="hlt">transfer</span> of heat and freshwater plays a critical role in the global climate system. This is particularly true for the Greenland and Iceland <span class="hlt">Seas</span>, where these fluxes drive ocean convection that contributes to Denmark Strait Overflow Water, the densest component of the lower limb of the Atlantic Meridional Overturning Circulation (AMOC). This buoyancy <span class="hlt">transfer</span> is most pronounced during the winter downstream of the ice edge, where the cold and dry Arctic <span class="hlt">air</span> first comes in contact with the relatively warm ocean surface. Here we show that the wintertime retreat of <span class="hlt">sea</span> ice in the region, combined with different rates of warming for the atmosphere and <span class="hlt">sea</span> surface of the Greenland and Iceland <span class="hlt">Seas</span>, has resulted in statistically significant reductions of approximately 20% in the magnitude of the winter <span class="hlt">air-sea</span> heat fluxes since 1979. Furthermore, it is demonstrated that modes of climate variability other than the North Atlantic Oscillation (NAO) are required to fully characterize the regional <span class="hlt">air-sea</span> interaction in this region. Mixed-layer model simulations imply that a continued decrease in atmospheric forcing will exceed a threshold for the Greenland <span class="hlt">Sea</span> whereby convection will become depth limited, reducing the ventilation of mid-depth waters in the Nordic <span class="hlt">Seas</span>. In the Iceland <span class="hlt">Sea</span>, further reductions have the potential to decrease the supply of the densest overflow waters to the AMOC.</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> exchange 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> exchange 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/2016AGUFMPP43C2339Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMPP43C2339Z"><span>The alkenone method for p<span class="hlt">CO</span><span class="hlt">2</span> reconstructions: challenges and strategies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, Y.; Pearson, A.; Benthien, A.; Dong, L.; Henderiks, J.; Huybers, P. J.</p> <p>2016-12-01</p> <p>The alkenone-p<span class="hlt">CO</span><span class="hlt">2</span> method is one of the most widely used approaches to reconstruct atmospheric <span class="hlt">CO</span><span class="hlt">2</span> in the Cenozoic. The method depends upon fractionation of stable carbon isotopes, expressed as ɛp37:<span class="hlt">2</span>, and a physiological scaling parameter, b, that accounts for algal growth rate and cell size. Alkenone-derived <span class="hlt">CO</span><span class="hlt">2</span> records for the late Pleistocene, however, often are poorly correlated with ice core <span class="hlt">CO</span><span class="hlt">2</span> records. We show that poor correlation largely results from (1) systematic overestimation of b and (<span class="hlt">2</span>) low sensitivity of ɛp37:<span class="hlt">2</span> to atmospheric <span class="hlt">CO</span><span class="hlt">2</span> variations at low-productivity sites [1]. Records are presented from two sites with high ɛp37:<span class="hlt">2</span> sensitivity: the South China <span class="hlt">Sea</span> (SCS) and the tropical Altantic Ocean. Values of b are back calculated to determine their full range over glacial-interglacial cycles using ɛp37:<span class="hlt">2</span>, ice core p<span class="hlt">CO</span><span class="hlt">2</span> records, and ocean temperature reconstructions. <span class="hlt">Air-sea</span> equilibrium of <span class="hlt">CO</span><span class="hlt">2</span> is assumed at both sites, and the high-resolution temperature record from the SCS site is tuned to ice core p<span class="hlt">CO</span><span class="hlt">2</span> to eliminate age model discrepancies. The mean value of b is applied to obtain p<span class="hlt">CO</span><span class="hlt">2</span> estimates. By definition, this approach must yield the correct mean value for p<span class="hlt">CO</span><span class="hlt">2</span>, but observed amplitudes are also reproduced. We further explore the relationship between coccolithophore cell size and growth rate using coccolith size measurements and back-calculated values of b, which suggests a potential proxy to constrain the history of phytoplankton growth rate and b. [1] Zhang, Y.G., Pearson, A., Huybers, P. and Pagani, M, 2016, Refining the alkenone-p<span class="hlt">CO</span><span class="hlt">2</span> method: The role of algal growth conditions, Paleoceanography, in review</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA00429.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA00429.html"><span>Hurricane Isabel, <span class="hlt">AIRS</span> Infrared and <span class="hlt">Sea</span>Winds Scatterometer Data Combined</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2003-09-20</p> <p>These two images show Hurricane Isabel as viewed by <span class="hlt">AIRS</span> and <span class="hlt">Sea</span>Winds scatterometers on NASA ADEOS-<span class="hlt">2</span> and QuikScat satellites in September, 2003. <span class="hlt">AIRS</span> data are used to create global three-dimensional maps of temperature, humidity and clouds, while scatterometers measure surface wind speed and direction. http://photojournal.jpl.nasa.gov/catalog/PIA00429</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19910054028&hterms=study+motivation&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dstudy%2Bmotivation','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19910054028&hterms=study+motivation&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dstudy%2Bmotivation"><span>Overview of the Frontal <span class="hlt">Air-Sea</span> Interaction Experiment (FASINEX) - A study of <span class="hlt">air-sea</span> interaction in a region of strong oceanic gradients</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Weller, Robert A.</p> <p>1991-01-01</p> <p>From 1984 to 1986 the cooperative Frontal <span class="hlt">Air-Sea</span> Interaction Experiment (FASINEX) was conducted in the subtropical convergence zone southwest of Bermuda. The overall objective of the experiment was to study <span class="hlt">air-sea</span> interaction on 1- to 100-km horizontal scales in a region of the open ocean characterized by strong horizontal gradients in upper ocean and <span class="hlt">sea</span> surface properties. Ocean fronts provided both large spatial gradients in <span class="hlt">sea</span> surface temperature and strong jetlike flows in the upper ocean. The motivation for and detailed objectives of FASINEX are reviewed. Then the components of the field program are summarized. Finally, selected results are presented in order to provide an overview of the outcome of FASINEX.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016BGeo...13.4595W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016BGeo...13.4595W"><span>Effect of ocean acidification and elevated f<span class="hlt">CO</span><span class="hlt">2</span> on trace gas production by a Baltic <span class="hlt">Sea</span> summer phytoplankton community</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Webb, Alison L.; Leedham-Elvidge, Emma; Hughes, Claire; Hopkins, Frances E.; Malin, Gill; Bach, Lennart T.; Schulz, Kai; Crawfurd, Kate; Brussaard, Corina P. D.; Stuhr, Annegret; Riebesell, Ulf; Liss, Peter S.</p> <p>2016-08-01</p> <p>The Baltic <span class="hlt">Sea</span> is a unique environment as the largest body of brackish water in the world. Acidification of the surface oceans due to absorption of anthropogenic <span class="hlt">CO</span><span class="hlt">2</span> emissions is an additional stressor facing the pelagic community of the already challenging Baltic <span class="hlt">Sea</span>. To investigate its impact on trace gas biogeochemistry, a large-scale mesocosm experiment was performed off Tvärminne Research Station, Finland, in summer 2012. During the second half of the experiment, dimethylsulfide (DMS) concentrations in the highest-f<span class="hlt">CO</span><span class="hlt">2</span> mesocosms (1075-1333 µatm) were 34 % lower than at ambient <span class="hlt">CO</span><span class="hlt">2</span> (350 µatm). However, the net production (as measured by concentration change) of seven halocarbons analysed was not significantly affected by even the highest <span class="hlt">CO</span><span class="hlt">2</span> levels after 5 weeks' exposure. Methyl iodide (CH3I) and diiodomethane (CH<span class="hlt">2</span>I<span class="hlt">2</span>) showed 15 and 57 % increases in mean mesocosm concentration (3.8 ± 0.6 increasing to 4.3 ± 0.4 pmol L-1 and 87.4 ± 14.9 increasing to 134.4 ± 24.1 pmol L-1 respectively) during Phase II of the experiment, which were unrelated to <span class="hlt">CO</span><span class="hlt">2</span> and corresponded to 30 % lower Chl a concentrations compared to Phase I. No other iodocarbons increased or showed a peak, with mean chloroiodomethane (CH<span class="hlt">2</span>ClI) concentrations measured at 5.3 (±0.9) pmol L-1 and iodoethane (C<span class="hlt">2</span>H5I) at 0.5 (±0.1) pmol L-1. Of the concentrations of bromoform (CHBr3; mean 88.1 ± 13.<span class="hlt">2</span> pmol L-1), dibromomethane (CH<span class="hlt">2</span>Br<span class="hlt">2</span>; mean 5.3 ± 0.8 pmol L-1), and dibromochloromethane (CHBr<span class="hlt">2</span>Cl, mean 3.0 ± 0.5 pmol L-1), only CH<span class="hlt">2</span>Br<span class="hlt">2</span> showed a decrease of 17 % between Phases I and II, with CHBr3 and CHBr<span class="hlt">2</span>Cl showing similar mean concentrations in both phases. Outside the mesocosms, an upwelling event was responsible for bringing colder, high-<span class="hlt">CO</span><span class="hlt">2</span>, low-pH water to the surface starting on day t16 of the experiment; this variable <span class="hlt">CO</span><span class="hlt">2</span> system with frequent upwelling events implies that the community of the Baltic <span class="hlt">Sea</span> is acclimated to regular significant declines in pH caused by up to 800 µatm f<span class="hlt">CO</span><span class="hlt">2</span>. After</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JMS...159...89X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JMS...159...89X"><span>Monthly <span class="hlt">CO</span><span class="hlt">2</span> at A4HDYD station in a productive shallow marginal <span class="hlt">sea</span> (Yellow <span class="hlt">Sea</span>) with a seasonal thermocline: Controlling processes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xu, Xuemei; Zang, Kunpeng; Zhao, Huade; Zheng, Nan; Huo, Cheng; Wang, Juying</p> <p>2016-07-01</p> <p>Based upon 21 field surveys conducted from March 2011 to November 2013, monthly variation of carbon dioxide partial pressure (p<span class="hlt">CO</span><span class="hlt">2</span>) and other carbon system parameters were investigated for the first time (to our knowledge) at A4HDYD station (38°40‧N, 122°10‧E) located in the North Yellow <span class="hlt">Sea</span>, a region with a seasonal thermocline. Surface p<span class="hlt">CO</span><span class="hlt">2</span> was undersaturated from March to May and nearly in equilibrium with the atmosphere from June to August. During September and November, p<span class="hlt">CO</span><span class="hlt">2</span> declined to a lower level than that from June to August, but reached the highest level in December. In contrast, p<span class="hlt">CO</span><span class="hlt">2</span> declined to atmospheric <span class="hlt">CO</span><span class="hlt">2</span> levels in February. Overall, the study area was a net <span class="hlt">CO</span><span class="hlt">2</span> sink at a rate of 0.85 ± 0.59 mol C m- <span class="hlt">2</span> yr- 1. The underlying processes governing the variation of p<span class="hlt">CO</span><span class="hlt">2</span> were also examined. In general, temperature had an important influence on the monthly variation of p<span class="hlt">CO</span><span class="hlt">2</span>, but its effect was counterbalanced by biological production in spring and vertical mixing in early winter. Our study indicated that dynamic mechanism studies based on high temporal resolution observations are urgently needed to understand the complexity of the carbon cycle and detect biogeochemical changes or ecosystem responses to climate change on continental margins.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26975003','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26975003"><span><span class="hlt">Air-sea</span> exchange of gaseous mercury in the East China <span class="hlt">Sea</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Chunjie; Ci, Zhijia; Wang, Zhangwei; Zhang, Xiaoshan</p> <p>2016-05-01</p> <p>Two oceanographic cruises were carried out in the East China <span class="hlt">Sea</span> (ECS) during the summer and fall of 2013. The main objectives of this study are to identify the spatial-temporal distributions of gaseous elemental mercury (GEM) in <span class="hlt">air</span> and dissolved gaseous mercury (DGM) in surface seawater, and then to estimate the Hg(0) 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/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 exchange across the <span class="hlt">sea</span>-ice covered areas.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014OptLT..56..158Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014OptLT..56..158Z"><span>Study of metal <span class="hlt">transfer</span> in <span class="hlt">CO</span><span class="hlt">2</span> laser+GMAW-P hybrid welding using argon-helium mixtures</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, Wang; Hua, Xueming; Liao, Wei; Li, Fang; Wang, Min</p> <p>2014-03-01</p> <p>The metal <span class="hlt">transfer</span> in <span class="hlt">CO</span><span class="hlt">2</span> Laser+GMAW-P hybrid welding by using argon-helium mixtures was investigated and the effect of the laser on the mental <span class="hlt">transfer</span> is discussed. A 650 nm laser, in conjunction with the shadow graph technique, is used to observe the metal <span class="hlt">transfer</span> process. In order to analyze the heat input to the droplet and the droplet internal current line distribution. An optical emission spectroscopy system was employed to estimate default parameter and optimized plasma temperature, electron number densities distribution. The results indicate that the <span class="hlt">CO</span><span class="hlt">2</span> plasma plume have a significant impact to the electrode melting, droplet formation, detachment, impingement onto the workpiece and weld morphology. Since the current distribution direction flow changes to the keyhole, to obtain a metal <span class="hlt">transfer</span> mode of one droplet per pulse, the welding parameters should be adjusted to a higher pulse time (TP) and a lower voltage.</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 exchange 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 exchange 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 exchange 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 exchange 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/2015AGUFM.A43C0283L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.A43C0283L"><span><span class="hlt">Air-sea</span> Exchange of Polycyclic Aromatic Hydrocarbons (PAHs), Polychlorinated Biphenyls (PCBs), Organochlorine Pesticides (OCPs) and Polybrominated Diphenyl Ethers (PBDEs) in the Mediterranean <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lammel, G. P.; Heil, A.; Kukucka, P.; Meixner, F. X.; Mulder, M. D.; Prybilova, P.; Prokes, R.; Rusina, T. S.; Song, G. Z.; Vrana, B.</p> <p>2015-12-01</p> <p>The marine atmospheric environment is a receptor for persistent organic pollutants (POPs) which are advected from sources on land, primary, such as biomass burning by-products (PAHs, dioxins), and secondary, such as volatilization from contaminated soils (PCBs, pesticides). Primary sources do not exist in the marine environment, except for PAHs (ship engines) but following previous atmospheric deposition, the <span class="hlt">sea</span> surface may turn to a secondary source by reversal of diffusive <span class="hlt">air-sea</span> mass exchange. No monitoring is in place. We studied the vertical 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> exchange 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> exchange. Recgional fire activity records in combination with box model simulations suggest that deposition of retene during summer is followed by a reversal of <span class="hlt">air-sea</span> exchange. The seawater surface as secondary source of pollution should be assessed based on flux measurements across seasons and over longer time periods.</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> exchange 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> exchange 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> exchange 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> exchange (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('http://adsabs.harvard.edu/abs/2006AGUFM.H34B..07F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFM.H34B..07F"><span>Water <span class="hlt">Transfers</span>, <span class="hlt">Air</span> Quality, Ecosystems and Population Growth at the US-Mexico Border: An Integrated Model of the Mexicali and Imperial Valleys</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Forster, C. B.; Gonzalez, T.; Peach, J.; Kjelland, M.; Collins, K.; Grant, W. E.</p> <p>2006-12-01</p> <p>Borderland communities in the Imperial-Mexicali Valleys (IMVs) of California (U.S.A.) and Mexicali (Mexico) are experiencing socioeconomic and environmental changes driven by policy makers and environmental conditions both within and outside the IMVs. The Colorado River Quantification Settlement Agreement (QSA) of 2003 will <span class="hlt">transfer</span> 30 million acre-feet of Colorado River water from Imperial Valley (IV) agricultural users to Southern California urban users over a 75-year period. Because the water level of the Salton <span class="hlt">Sea</span> is supported by agricultural runoff, reduced water flows to the <span class="hlt">sea</span> raise concerns that: 1) <span class="hlt">air</span> quality will be degraded as dust is generated by the drying <span class="hlt">Sea</span>-bed, and <span class="hlt">2</span>) declining fish populations due to increasing salinity will no longer support birds migrating along a key avian flyway. Rapid population growth in the Mexican border-city of Mexicali, combined with new power plants and plans for water reuse, raises concerns that: 1) the quantity and quality of water supplied to the Salton <span class="hlt">Sea</span> will decline, and <span class="hlt">2</span>) increased vehicle use and electrical power generation will lead to declining <span class="hlt">air</span> quality in the binational <span class="hlt">air</span> basin. Each concern may be affected by climate change. As environmental factors change, so too may the agricultural economy of the Imperial Valley that, in turn, depends on the availability of both water and manual labor. The economy of Mexicali is dominated by the maquiladora (manufacturing) industry that depends upon the availability of power, labor and water. A system dynamics model, with annual time step, simulates this complex binational system. The model was developed by an academic team with input from local experts/decision-makers from both Mexico and the US. We are preparing to engage community stakeholders and decision-makers in exploring the model. Insights gained from model results yield better understanding of the consequences of alternative future scenarios that include: QSA water <span class="hlt">transfers</span> and land fallowing plans</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29255277','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29255277"><span>Satellite Observations of Imprint of Oceanic Current on Wind Stress by <span class="hlt">Air-Sea</span> Coupling.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Renault, Lionel; McWilliams, James C; Masson, Sebastien</p> <p>2017-12-18</p> <p>Mesoscale eddies are present everywhere in the ocean and partly determine the mean state of the circulation and ecosystem. The current feedback on the surface wind stress modulates the <span class="hlt">air-sea</span> <span class="hlt">transfer</span> of momentum by providing a sink of mesoscale eddy energy as an atmospheric source. Using nine years of satellite measurements of surface stress and geostrophic currents over the global ocean, we confirm that the current-induced surface stress curl is linearly related to the current vorticity. The resulting coupling coefficient between current and surface stress (s τ [N s m -3 ]) is heterogeneous and can be roughly expressed as a linear function of the mean surface wind. s τ expresses the sink of eddy energy induced by the current feedback. This has important implications for <span class="hlt">air-sea</span> interaction and implies that oceanic mean and mesoscale circulations and their effects on surface-layer ventilation and carbon uptake are better represented in oceanic models that include this feedback.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29559990','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29559990"><span>Can Elevated <span class="hlt">Air</span> [<span class="hlt">CO</span><span class="hlt">2</span>] Conditions Mitigate the Predicted Warming Impact on the Quality of Coffee Bean?</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ramalho, José C; Pais, Isabel P; Leitão, António E; Guerra, Mauro; Reboredo, Fernando H; Máguas, Cristina M; Carvalho, Maria L; Scotti-Campos, Paula; Ribeiro-Barros, Ana I; Lidon, Fernando J C; DaMatta, Fábio M</p> <p>2018-01-01</p> <p>Climate changes, mostly related to high temperature, are predicted to have major negative impacts on coffee crop yield and bean quality. Recent studies revealed that elevated <span class="hlt">air</span> [<span class="hlt">CO</span> <span class="hlt">2</span> ] mitigates the impact of heat on leaf physiology. However, the extent of the interaction between elevated <span class="hlt">air</span> [<span class="hlt">CO</span> <span class="hlt">2</span> ] and heat on coffee bean quality was never addressed. In this study, the single and combined impacts of enhanced [<span class="hlt">CO</span> <span class="hlt">2</span> ] and temperature in beans of Coffea arabica cv. Icatu were evaluated. Plants were grown at 380 or 700 μL <span class="hlt">CO</span> <span class="hlt">2</span> L -1 <span class="hlt">air</span>, and then submitted to a gradual temperature rise from 25°C up to 40°C during ca. 4 months. Fruits were harvested at 25°C, and in the ranges of 30-35 or 36-40°C, and bean physical and chemical attributes with potential implications on quality were then examined. These included: color, phenolic content, soluble solids, chlorogenic, caffeic and p -coumaric acids, caffeine, trigonelline, lipids, and minerals. Most of these parameters were mainly affected by temperature (although without a strong negative impact on bean quality), and only marginally, if at all, by elevated [<span class="hlt">CO</span> <span class="hlt">2</span> ]. However, the [<span class="hlt">CO</span> <span class="hlt">2</span> ] vs. temperature interaction strongly attenuated some of the negative impacts promoted by heat (e.g., total chlorogenic acids), thus maintaining the bean characteristics closer to those obtained under adequate temperature conditions (e.g., soluble solids, caffeic and p -coumaric acids, trigonelline, chroma, Hue angle, and color index), and increasing desirable features (acidity). Fatty acid and mineral pools remained quite stable, with only few modifications due to elevated <span class="hlt">air</span> [<span class="hlt">CO</span> <span class="hlt">2</span> ] (e.g., phosphorous) and/or heat. In conclusion, exposure to high temperature in the last stages of fruit maturation did not strongly depreciate bean quality, under the conditions of unrestricted water supply and moderate irradiance. Furthermore, the superimposition of elevated <span class="hlt">air</span> [<span class="hlt">CO</span> <span class="hlt">2</span> ] contributed to preserve bean quality by modifying and mitigating</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5845708','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5845708"><span>Can Elevated <span class="hlt">Air</span> [<span class="hlt">CO</span><span class="hlt">2</span>] Conditions Mitigate the Predicted Warming Impact on the Quality of Coffee Bean?</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Ramalho, José C.; Pais, Isabel P.; Leitão, António E.; Guerra, Mauro; Reboredo, Fernando H.; Máguas, Cristina M.; Carvalho, Maria L.; Scotti-Campos, Paula; Ribeiro-Barros, Ana I.; Lidon, Fernando J. C.; DaMatta, Fábio M.</p> <p>2018-01-01</p> <p>Climate changes, mostly related to high temperature, are predicted to have major negative impacts on coffee crop yield and bean quality. Recent studies revealed that elevated <span class="hlt">air</span> [<span class="hlt">CO</span><span class="hlt">2</span>] mitigates the impact of heat on leaf physiology. However, the extent of the interaction between elevated <span class="hlt">air</span> [<span class="hlt">CO</span><span class="hlt">2</span>] and heat on coffee bean quality was never addressed. In this study, the single and combined impacts of enhanced [<span class="hlt">CO</span><span class="hlt">2</span>] and temperature in beans of Coffea arabica cv. Icatu were evaluated. Plants were grown at 380 or 700 μL <span class="hlt">CO</span><span class="hlt">2</span> L-1 <span class="hlt">air</span>, and then submitted to a gradual temperature rise from 25°C up to 40°C during ca. 4 months. Fruits were harvested at 25°C, and in the ranges of 30–35 or 36–40°C, and bean physical and chemical attributes with potential implications on quality were then examined. These included: color, phenolic content, soluble solids, chlorogenic, caffeic and p-coumaric acids, caffeine, trigonelline, lipids, and minerals. Most of these parameters were mainly affected by temperature (although without a strong negative impact on bean quality), and only marginally, if at all, by elevated [<span class="hlt">CO</span><span class="hlt">2</span>]. However, the [<span class="hlt">CO</span><span class="hlt">2</span>] vs. temperature interaction strongly attenuated some of the negative impacts promoted by heat (e.g., total chlorogenic acids), thus maintaining the bean characteristics closer to those obtained under adequate temperature conditions (e.g., soluble solids, caffeic and p-coumaric acids, trigonelline, chroma, Hue angle, and color index), and increasing desirable features (acidity). Fatty acid and mineral pools remained quite stable, with only few modifications due to elevated <span class="hlt">air</span> [<span class="hlt">CO</span><span class="hlt">2</span>] (e.g., phosphorous) and/or heat. In conclusion, exposure to high temperature in the last stages of fruit maturation did not strongly depreciate bean quality, under the conditions of unrestricted water supply and moderate irradiance. Furthermore, the superimposition of elevated <span class="hlt">air</span> [<span class="hlt">CO</span><span class="hlt">2</span>] contributed to preserve bean quality by modifying and mitigating the heat impact</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29644611','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29644611"><span>Atmospheric fossil fuel <span class="hlt">CO</span><span class="hlt">2</span> traced by 14<span class="hlt">CO</span><span class="hlt">2</span> and <span class="hlt">air</span> quality index pollutant observations in Beijing and Xiamen, China.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Niu, Zhenchuan; Zhou, Weijian; Feng, Xue; Feng, Tian; Wu, Shugang; Cheng, Peng; Lu, Xuefeng; Du, Hua; Xiong, Xiaohu; Fu, Yunchong</p> <p>2018-06-01</p> <p>Radiocarbon ( 14 C) is the most accurate tracer available for quantifying atmospheric <span class="hlt">CO</span> <span class="hlt">2</span> derived from fossil fuel (<span class="hlt">CO</span> <span class="hlt">2</span>ff ), but it is expensive and time-consuming to measure. Here, we used common hourly <span class="hlt">Air</span> Quality Index (AQI) pollutants (AQI, PM <span class="hlt">2</span>.5 , PM 10 , and <span class="hlt">CO</span>) to indirectly trace diurnal <span class="hlt">CO</span> <span class="hlt">2</span>ff variations during certain days at the urban sites in Beijing and Xiamen, China, based on linear relationships between AQI pollutants and <span class="hlt">CO</span> <span class="hlt">2</span>ff traced by 14 C ([Formula: see text]) for semimonthly samples obtained in 2014. We validated these indirectly traced <span class="hlt">CO</span> <span class="hlt">2</span>ff (<span class="hlt">CO</span> <span class="hlt">2</span>ff-in ) concentrations against [Formula: see text] concentrations traced by simultaneous diurnal 14 <span class="hlt">CO</span> <span class="hlt">2</span> observations. Significant (p < 0.05) strong correlations were observed between each of the separate AQI pollutants and [Formula: see text] for the semimonthly samples. Diurnal variations in <span class="hlt">CO</span> <span class="hlt">2</span>ff traced by each of the AQI pollutants generally showed similar trends to those of [Formula: see text], with high agreement at the sampling site in Beijing and relatively poor agreement at the sampling site in Xiamen. AQI pollutant tracers showed high normalized root-mean-square (NRMS) errors for the summer diurnal samples due to low [Formula: see text] concentrations. After the removal of these summer samples, the NRMS errors for AQI pollutant tracers were in the range of 31.6-64.<span class="hlt">2</span>%. <span class="hlt">CO</span> generally showed a high agreement and low NRMS errors among these indirect tracers. Based on these linear relationships, monthly <span class="hlt">CO</span> <span class="hlt">2</span>ff averages at the sampling sites in Beijing and Xiamen were traced using <span class="hlt">CO</span> concentration as a tracer. The monthly <span class="hlt">CO</span> <span class="hlt">2</span>ff averages at the Beijing site showed a shallow U-type variation. These results indicate that <span class="hlt">CO</span> can be used to trace <span class="hlt">CO</span> <span class="hlt">2</span>ff variations in Chinese cities with <span class="hlt">CO</span> <span class="hlt">2</span>ff concentrations above 5 ppm.</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('http://adsabs.harvard.edu/abs/2015AGUFM.B11C0441C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.B11C0441C"><span>Assessing model sensitivity and uncertainty across multiple Free-<span class="hlt">Air</span> <span class="hlt">CO</span><span class="hlt">2</span> Enrichment experiments.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cowdery, E.; Dietze, M.</p> <p>2015-12-01</p> <p>As atmospheric levels of carbon dioxide levels continue to increase, it is critical that terrestrial ecosystem models can accurately predict ecological responses to the changing environment. Current predictions of net primary productivity (NPP) in response to elevated atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentrations are highly variable and contain a considerable amount of uncertainty. It is necessary that we understand which factors are driving this uncertainty. The Free-<span class="hlt">Air</span> <span class="hlt">CO</span><span class="hlt">2</span> Enrichment (FACE) experiments have equipped us with a rich data source that can be used to calibrate and validate these model predictions. To identify and evaluate the assumptions causing inter-model differences we performed model sensitivity and uncertainty analysis across ambient and elevated <span class="hlt">CO</span><span class="hlt">2</span> treatments using the Data Assimilation Linked Ecosystem Carbon (DALEC) model and the Ecosystem Demography Model (ED<span class="hlt">2</span>), two process-based models ranging from low to high complexity respectively. These modeled process responses were compared to experimental data from the Kennedy Space Center Open Top Chamber Experiment, the Nevada Desert Free <span class="hlt">Air</span> <span class="hlt">CO</span><span class="hlt">2</span> Enrichment Facility, the Rhinelander FACE experiment, the Wyoming Prairie Heating and <span class="hlt">CO</span><span class="hlt">2</span> Enrichment Experiment, the Duke Forest Face experiment and the Oak Ridge Experiment on <span class="hlt">CO</span><span class="hlt">2</span> Enrichment. By leveraging data access proxy and data tilling services provided by the BrownDog data curation project alongside analysis modules available in the Predictive Ecosystem Analyzer (PEcAn), we produced automated, repeatable benchmarking workflows that are generalized to incorporate different sites and ecological models. Combining the observed patterns of uncertainty between the two models with results of the recent FACE-model data synthesis project (FACE-MDS) can help identify which processes need further study and additional data constraints. These findings can be used to inform future experimental design and in turn can provide informative starting point for data assimilation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMGC23D1175M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMGC23D1175M"><span><span class="hlt">Sea</span> ice-induced cold <span class="hlt">air</span> advection as a mechanism controlling tundra primary productivity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Macias-Fauria, M.; Karlsen, S. R.</p> <p>2015-12-01</p> <p>The recent sharp decline in Arctic <span class="hlt">sea</span> ice extent, concentration, and volume leaves urgent questions regarding its effects on ecological processes. Changes in tundra productivity have been associated with <span class="hlt">sea</span> ice dynamics on the basis that most tundra ecosystems lay close to the <span class="hlt">sea</span>. Although some studies have addressed the potential effect of <span class="hlt">sea</span> ice decline on the primary productivity of terrestrial arctic ecosystems (Bhatt et al., 2010), a clear picture of the mechanisms and patterns linking both processes remains elusive. We hypothesised that <span class="hlt">sea</span> ice might influence tundra productivity through 1) cold <span class="hlt">air</span> advection during the growing season (direct/weather effect) or <span class="hlt">2</span>) changes in regional climate induced by changes in <span class="hlt">sea</span> ice (indirect/climate effect). We present a test on the direct/weather effect hypothesis: that is, tundra productivity is coupled with <span class="hlt">sea</span> ice when <span class="hlt">sea</span> ice remains close enough from land vegetation during the growing season for cold <span class="hlt">air</span> advection to limit temperatures locally. We employed weekly MODIS-derived Normalised Difference Vegetation Index (as a proxy for primary productivity) and <span class="hlt">sea</span> ice data at a spatial resolution of 232m for the period 2000-2014 (included), covering the Svalbard Archipelago. Our results suggest that <span class="hlt">sea</span> ice-induced cold <span class="hlt">air</span> advection is a likely mechanism to explain patterns of NDVI trends and heterogeneous spatial dynamics in the Svalbard archipelago. The mechanism offers the potential to explain <span class="hlt">sea</span> ice/tundra productivity dynamics in other Arctic areas.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29090614','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29090614"><span><span class="hlt">CO</span><span class="hlt">2</span> clearance by membrane lungs.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sun, Liqun; Kaesler, Andreas; Fernando, Piyumindri; Thompson, Alex J; Toomasian, John M; Bartlett, Robert H</p> <p>2018-05-01</p> <p>Commercial membrane lungs are designed to <span class="hlt">transfer</span> a specific amount of oxygen per unit of venous blood flow. Membrane lungs are much more efficient at removing <span class="hlt">CO</span> <span class="hlt">2</span> than adding oxygen, but the range of <span class="hlt">CO</span> <span class="hlt">2</span> <span class="hlt">transfer</span> is rarely reported. Commercial membrane lungs were studied with the goal of evaluating <span class="hlt">CO</span> <span class="hlt">2</span> removal capacity. <span class="hlt">CO</span> <span class="hlt">2</span> removal was measured in 4 commercial membrane lungs under standardized conditions. <span class="hlt">CO</span> <span class="hlt">2</span> clearance can be greater than 4 times that of oxygen at a given blood flow when the gas to blood flow ratio is elevated to 4:1 or 8:1. The <span class="hlt">CO</span> <span class="hlt">2</span> clearance was less dependent on surface area and configuration than oxygen <span class="hlt">transfer</span>. Any ECMO system can be used for selective <span class="hlt">CO</span> <span class="hlt">2</span> removal.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ApSS..429....2C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ApSS..429....2C"><span>Selectivity of photoelectrochemical <span class="hlt">CO</span><span class="hlt">2</span> reduction modulated with electron <span class="hlt">transfer</span> from size-tunable quantized energy states of CdSe nanocrystals</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cho, Hyunjin; Kim, Whi Dong; Lee, Kangha; Lee, Seokwon; Kang, Gil-Seong; Joh, Han-Ik; Lee, Doh C.</p> <p>2018-01-01</p> <p>We investigate the product selectivity of <span class="hlt">CO</span><span class="hlt">2</span> reduction using NiO photocathodes decorated with CdSe quantum dots (QDs) of varying size in a photoelectrochemical (PEC) cell. Size-tunable and quantized energy states of conduction band in CdSe QDs enable systematic control of electron <span class="hlt">transfer</span> kinetics from CdSe QDs to NiO. It turns out that different size of CdSe QDs results in variation in product selectivity for <span class="hlt">CO</span><span class="hlt">2</span> reduction. The energy gap between conduction band edge and redox potential of each reduction product (e.g., <span class="hlt">CO</span> and CH4) correlates with their production rate. The size dependence of the electron <span class="hlt">transfer</span> rate estimated from the energy gap is in agreement with the selectivity of <span class="hlt">CO</span><span class="hlt">2</span> reduction products for all reduction products but <span class="hlt">CO</span>. The deviation in the case of <span class="hlt">CO</span> is attributed to sequential conversion of <span class="hlt">CO</span> into CH4 with <span class="hlt">CO</span> adsorbed on electrode surface. Based on a premise that the CdSe QDs would exhibit similar surface configuration regardless of QD size, it is concluded that the electron <span class="hlt">transfer</span> kinetics proves to alter the selectivity of <span class="hlt">CO</span><span class="hlt">2</span> reduction.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1999SPIE.3829...68S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1999SPIE.3829...68S"><span>13<span class="hlt">CO</span><span class="hlt">2</span>/12<span class="hlt">CO</span><span class="hlt">2</span> ratio analysis in exhaled <span class="hlt">air</span> by lead-salt tunable diode lasers for noninvasive diagnostics in gastroenterology</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stepanov, Eugene V.; Zyrianov, Pavel V.; Miliaev, Valerii A.; Selivanov, Yurii G.; Chizhevskii, Eugene G.; Os'kina, Svetlana; Ivashkin, Vladimir T.; Nikitina, Elena I.</p> <p>1999-07-01</p> <p>An analyzer of 13<span class="hlt">CO</span><span class="hlt">2</span>/12<span class="hlt">CO</span><span class="hlt">2</span> ratio in exhaled <span class="hlt">air</span> based on lead-salt tunable diode lasers is presented. High accuracy of the carbon isotope ratio detection in exhaled carbon dioxide was achieved with help of very simple optical schematics. It was based on the use of MBE laser diodes operating in pulse mode and on recording the resonance <span class="hlt">CO</span><span class="hlt">2</span> absorption at 4.<span class="hlt">2</span> micrometers . Special fast acquisition electronics and software were applied for spectral data collection and processing. Developed laser system was tested in a clinical train aimed to assessment eradication efficiency in therapy of gastritis associated with Helicobacter pylori infection. Data on the 13C-urea breath test used for P.pylori detection and obtained with tunable diode lasers in the course of the trail was compared with the results of Mass-Spectroscopy analysis and histology observations. The analyzer can be used also for 13<span class="hlt">CO</span><span class="hlt">2</span>/12<span class="hlt">CO</span><span class="hlt">2</span> ratio detection in exhalation to perform gastroenterology breath test based on using other compounds labeled with stable isotopes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23564676','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23564676"><span>Lower responsiveness of canopy evapotranspiration rate than of leaf stomatal conductance to open-<span class="hlt">air</span> <span class="hlt">CO</span><span class="hlt">2</span> elevation in rice.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Shimono, Hiroyuki; Nakamura, Hirofumi; Hasegawa, Toshihiro; Okada, Masumi</p> <p>2013-08-01</p> <p>An elevated atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentration ([<span class="hlt">CO</span><span class="hlt">2</span> ]) can reduce stomatal conductance of leaves for most plant species, including rice (Oryza sativa L.). However, few studies have quantified seasonal changes in the effects of elevated [<span class="hlt">CO</span><span class="hlt">2</span> ] on canopy evapotranspiration, which integrates the response of stomatal conductance of individual leaves with other responses, such as leaf area expansion, changes in leaf surface temperature, and changes in developmental stages, in field conditions. We conducted a field experiment to measure seasonal changes in stomatal conductance of the uppermost leaves and in the evapotranspiration, transpiration, and evaporation rates using a lysimeter method. The study was conducted for flooded rice under open-<span class="hlt">air</span> <span class="hlt">CO</span><span class="hlt">2</span> elevation. Stomatal conductance decreased by 27% under elevated [<span class="hlt">CO</span><span class="hlt">2</span> ], averaged throughout the growing season, and evapotranspiration decreased by an average of 5% during the same period. The decrease in daily evapotranspiration caused by elevated [<span class="hlt">CO</span><span class="hlt">2</span> ] was more significantly correlated with <span class="hlt">air</span> temperature and leaf area index (LAI) rather than with other parameters of solar radiation, days after transplanting, vapor-pressure deficit and FAO reference evapotranspiration. This indicates that higher <span class="hlt">air</span> temperatures, within the range from 16 to 27 °C, and a larger LAI, within the range from 0 to 4 m(<span class="hlt">2</span>)  m(-<span class="hlt">2</span>) , can increase the magnitude of the decrease in evapotranspiration rate caused by elevated [<span class="hlt">CO</span><span class="hlt">2</span> ]. The crop coefficient (i.e. the evapotranspiration rate divided by the FAO reference evapotranspiration rate) was 1.24 at ambient [<span class="hlt">CO</span><span class="hlt">2</span> ] and 1.17 at elevated [<span class="hlt">CO</span><span class="hlt">2</span> ]. This study provides the first direct measurement of the effects of elevated [<span class="hlt">CO</span><span class="hlt">2</span> ] on rice canopy evapotranspiration under open-<span class="hlt">air</span> conditions using the lysimeter method, and the results will improve future predictions of water use in rice fields. © 2013 John Wiley & Sons Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E3SWC..3110008W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E3SWC..3110008W"><span>The Design of The Monitoring Tools Of Clean <span class="hlt">Air</span> Condition And Dangerous Gas <span class="hlt">CO</span>, <span class="hlt">CO</span><span class="hlt">2</span> CH4 In Chemical Laboratory By Using Fuzzy Logic Based On Microcontroller</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Widodo, Slamet; Miftakul, Amin M.; Sutrisman, Adi</p> <p>2018-02-01</p> <p>There are many phenomena that human are exposed to toxins from certain types such as of <span class="hlt">CO</span><span class="hlt">2</span>, <span class="hlt">CO</span><span class="hlt">2</span> and CH4 gases. The device used to detect large amounts of <span class="hlt">CO</span>, <span class="hlt">CO</span><span class="hlt">2</span>, and CH4 gas in <span class="hlt">air</span> in enclosed spaces using MQ 135 gas sensors of different types based on the three sensitivity of the Gas. The results of testing the use of sensors MQ 135 on the gas content of <span class="hlt">CO</span>, <span class="hlt">CO</span><span class="hlt">2</span> and CH4 received by the sensor is still in the form of ppm based on the maximum ppm detection range of each sensor. Active sensor detects <span class="hlt">CO</span> 120 ppm gas, <span class="hlt">CO</span><span class="hlt">2</span> 1600 ppm and CH4 1ppm "standby 1" <span class="hlt">air</span> condition with intermediate rotary fan. Active sensor detects <span class="hlt">CO</span> 30 ppm gas, <span class="hlt">CO</span><span class="hlt">2</span> 490 ppm and CH4 7 ppm "Standby <span class="hlt">2</span>" with low rotating fan output. Fuzzy rulebase logic for motor speed when gas detection sensor <span class="hlt">CO</span>, <span class="hlt">CO</span><span class="hlt">2</span>, and CH4 output controls the motion speed of the fan blower. Active sensors detect <span class="hlt">CO</span> 15 ppm, <span class="hlt">CO</span><span class="hlt">2</span> 320 ppm and CH4 45 ppm "Danger" <span class="hlt">air</span> condition with high fan spin fan. At the gas level of <span class="hlt">CO</span> 15 ppm, <span class="hlt">CO</span><span class="hlt">2</span> 390 ppm and CH4 3 ppm detect "normal" AC sensor with fan output stop spinning.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21548105','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21548105"><span>Amine-tethered solid adsorbents coupling high adsorption capacity and regenerability 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>Choi, Sunho; Gray, McMahan L; Jones, Christopher W</p> <p>2011-05-23</p> <p>Silica supported poly(ethyleneimine) (PEI) materials are prepared via impregnation and demonstrated to be promising adsorbents for <span class="hlt">CO</span>(<span class="hlt">2</span>) capture from ultra-dilute gas streams such as ambient <span class="hlt">air</span>. A prototypical class 1 adsorbent, containing 45 wt% PEI (PEI/silica), and two new modified PEI-based aminosilica adsorbents, derived from PEI modified with 3-aminopropyltrimethoxysilane (A-PEI/silica) or tetraethyl orthotitanate (T-PEI/silica), are prepared and characterized by using thermogravimetric analysis and FTIR spectroscopy. The modifiers are shown to enhance the thermal stability of the polymer-oxide composites, leading to higher PEI decomposition temperatures. The modified adsorbents present extremely high <span class="hlt">CO</span>(<span class="hlt">2</span>) adsorption capacities under conditions simulating ambient <span class="hlt">air</span> (400 ppm <span class="hlt">CO</span>(<span class="hlt">2</span>) in inert gas), exceeding <span class="hlt">2</span> mol(CO (<span class="hlt">2</span>)) kg(sorbent)(-1), as well as enhanced adsorption kinetics compared to conventional class 1 sorbents. The new adsorbents show excellent stability in cyclic adsorption-desorption operations, even under dry conditions in which aminosilica adsorbents are known to lose capacity due to urea formation. Thus, the adsorbents of this type can be considered promising materials for the direct capture of <span class="hlt">CO</span>(<span class="hlt">2</span>) from ultra-dilute gas streams such as ambient <span class="hlt">air</span>. Copyright © 2011 WILEY-VCH Verlag GmbH & <span class="hlt">Co</span>. KGaA, Weinheim.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3647119','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3647119"><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="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</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 35S 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. PMID:23658555</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1394443','SCIGOV-DOEDE'); return false;" href="https://www.osti.gov/servlets/purl/1394443"><span>Atmospheric <span class="hlt">CO</span><span class="hlt">2</span> Concentrations from Aircraft for 1972-1981, CSIRO Monitoring Program</span></a></p> <p><a target="_blank" href="http://www.osti.gov/dataexplorer">DOE Data Explorer</a></p> <p>Beardsmore, David J. [Commonwealth Scientific and Industrial Research Organization (CSIRO), Victoria, Australia; Pearman, Graeme I. [Commonwealth Scientific and Industrial Research Organization (CSIRO), Victoria, Australia</p> <p>2012-01-01</p> <p>From 1972 through 1981, <span class="hlt">air</span> samples were collected in glass flasks from aircraft at a variety of latitudes and altitudes over Australia, New Zealand, and Antarctica. The samples were analyzed for <span class="hlt">CO</span><span class="hlt">2</span> concentrations with nondispersive infrared gas analysis. The resulting data contain the sampling dates, type of aircraft, flight number, flask identification number, sampling time, geographic sector, distance in kilometers from the listed distance measuring equipment (DME) station, station number of the radio navigation distance measuring equipment, altitude of the aircraft above mean <span class="hlt">sea</span> level, sample analysis date, flask pressure, tertiary standards used for the analysis, analyzer used, and <span class="hlt">CO</span><span class="hlt">2</span> concentration. These data represent the first published record of <span class="hlt">CO</span><span class="hlt">2</span> concentrations in the Southern Hemisphere expressed in the WMO 1981 <span class="hlt">CO</span><span class="hlt">2</span> Calibration Scale and provide a precise record of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentrations in the troposphere and lower stratosphere over Australia and New Zealand.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040090299&hterms=Phytoplankton&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3DPhytoplankton','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040090299&hterms=Phytoplankton&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3DPhytoplankton"><span>Fractionation of carbon isotopes by phytoplankton and estimates of ancient <span class="hlt">CO</span><span class="hlt">2</span> levels</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Freeman, K. H.; Hayes, J. M.</p> <p>1992-01-01</p> <p>Reports of the 13C content of marine particulate organic carbon are compiled and on the basis of GEOSECS data and temperatures, concentrations, and isotopic compositions of dissolved <span class="hlt">CO</span><span class="hlt">2</span> in the waters in which the related phytoplankton grew are estimated. In this way, the fractionation of carbon isotopes during photosynthetic fixation of <span class="hlt">CO</span><span class="hlt">2</span> is found to be significantly correlated with concentrations of dissolved <span class="hlt">CO</span><span class="hlt">2</span>. Because ancient carbon isotopic fractionations have been determined from analyses of sedimentary porphyrins [Popp et al., 1989], the relationship between isotopic fractionation and concentrations of dissolved <span class="hlt">CO</span><span class="hlt">2</span> developed here can be employed to estimate concentrations of <span class="hlt">CO</span><span class="hlt">2</span> dissolved in ancient oceans and, in turn, partial pressures of <span class="hlt">CO</span><span class="hlt">2</span> in ancient atmospheres. The calculations take into account the temperature dependence of chemical and isotopic equilibria in the dissolved-inorganic-carbon system and of <span class="hlt">air-sea</span> equilibria. Paleoenvironmental temperatures for each sample are estimated from reconstructions of paleogeography, latitudinal temperature gradients, and secular changes in low-latitude <span class="hlt">sea</span> surface temperature. It is estimated that atmospheric partial pressures of <span class="hlt">CO</span><span class="hlt">2</span> were over 1000 micro atm 160 - 100 Ma ago, then declined to values near 300 micro atm during the next 100 Ma. Analysis of a high-resolution record of carbon isotopic fractionation at the Cenomanian-Turonian boundary suggests that the partial pressure of <span class="hlt">CO</span><span class="hlt">2</span> in the atmosphere was drawn down from values near 840 micro atm to values near 700 micro atm during the anoxic event.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015BGeo...12.7251R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015BGeo...12.7251R"><span>Data-based estimates of the ocean carbon sink variability - first results of the Surface Ocean p<span class="hlt">CO</span><span class="hlt">2</span> Mapping intercomparison (SOCOM)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rödenbeck, C.; Bakker, D. C. E.; Gruber, N.; Iida, Y.; Jacobson, A. R.; Jones, S.; Landschützer, P.; Metzl, N.; Nakaoka, S.; Olsen, A.; Park, G.-H.; Peylin, P.; Rodgers, K. B.; Sasse, T. P.; Schuster, U.; Shutler, J. D.; Valsala, V.; Wanninkhof, R.; Zeng, J.</p> <p>2015-12-01</p> <p>Using measurements of the surface-ocean <span class="hlt">CO</span><span class="hlt">2</span> partial pressure (p<span class="hlt">CO</span><span class="hlt">2</span>) and 14 different p<span class="hlt">CO</span><span class="hlt">2</span> mapping methods recently collated by the Surface Ocean p<span class="hlt">CO</span><span class="hlt">2</span> Mapping intercomparison (SOCOM) initiative, variations in regional and global <span class="hlt">sea-air</span> <span class="hlt">CO</span><span class="hlt">2</span> fluxes are investigated. Though the available mapping methods use widely different approaches, we find relatively consistent estimates of regional p<span class="hlt">CO</span><span class="hlt">2</span> seasonality, in line with previous estimates. In terms of interannual variability (IAV), all mapping methods estimate the largest variations to occur in the eastern equatorial Pacific. Despite considerable spread in the detailed variations, mapping methods that fit the data more closely also tend to agree more closely with each other in regional averages. Encouragingly, this includes mapping methods belonging to complementary types - taking variability either directly from the p<span class="hlt">CO</span><span class="hlt">2</span> data or indirectly from driver data via regression. From a weighted ensemble average, we find an IAV amplitude of the global <span class="hlt">sea-air</span> <span class="hlt">CO</span><span class="hlt">2</span> flux of 0.31 PgC yr-1 (standard deviation over 1992-2009), which is larger than simulated by biogeochemical process models. From a decadal perspective, the global ocean <span class="hlt">CO</span><span class="hlt">2</span> uptake is estimated to have gradually increased since about 2000, with little decadal change prior to that. The weighted mean net global ocean <span class="hlt">CO</span><span class="hlt">2</span> sink estimated by the SOCOM ensemble is -1.75 PgC yr-1 (1992-2009), consistent within uncertainties with estimates from ocean-interior carbon data or atmospheric oxygen trends.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015BGD....1214049R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015BGD....1214049R"><span>Data-based estimates of the ocean carbon sink variability - first results of the Surface Ocean p<span class="hlt">CO</span><span class="hlt">2</span> Mapping intercomparison (SOCOM)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rödenbeck, C.; Bakker, D. C. E.; Gruber, N.; Iida, Y.; Jacobson, A. R.; Jones, S.; Landschützer, P.; Metzl, N.; Nakaoka, S.; Olsen, A.; Park, G.-H.; Peylin, P.; Rodgers, K. B.; Sasse, T. P.; Schuster, U.; Shutler, J. D.; Valsala, V.; Wanninkhof, R.; Zeng, J.</p> <p>2015-08-01</p> <p>Using measurements of the surface-ocean <span class="hlt">CO</span><span class="hlt">2</span> partial pressure (p<span class="hlt">CO</span><span class="hlt">2</span>) and 14 different p<span class="hlt">CO</span><span class="hlt">2</span> mapping methods recently collated by the Surface Ocean p<span class="hlt">CO</span><span class="hlt">2</span> Mapping intercomparison (SOCOM) initiative, variations in regional and global <span class="hlt">sea-air</span> <span class="hlt">CO</span><span class="hlt">2</span> fluxes have been investigated. Though the available mapping methods use widely different approaches, we find relatively consistent estimates of regional p<span class="hlt">CO</span><span class="hlt">2</span> seasonality, in line with previous estimates. In terms of interannual variability (IAV), all mapping methods estimate the largest variations to occur in the Eastern equatorial Pacific. Despite considerable spead in the detailed variations, mapping methods with closer match to the data also tend to be more consistent with each other. Encouragingly, this includes mapping methods belonging to complementary types - taking variability either directly from the p<span class="hlt">CO</span><span class="hlt">2</span> data or indirectly from driver data via regression. From a weighted ensemble average, we find an IAV amplitude of the global <span class="hlt">sea-air</span> <span class="hlt">CO</span><span class="hlt">2</span> flux of 0.31 PgC yr-1 (standard deviation over 1992-2009), which is larger than simulated by biogeochemical process models. On a decadal perspective, the global <span class="hlt">CO</span><span class="hlt">2</span> uptake is estimated to have gradually increased since about 2000, with little decadal change prior to 2000. The weighted mean total ocean <span class="hlt">CO</span><span class="hlt">2</span> sink estimated by the SOCOM ensemble is consistent within uncertainties with estimates from ocean-interior carbon data or atmospheric oxygen trends.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28106932','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28106932"><span>Metal-<span class="hlt">CO</span><span class="hlt">2</span> Batteries on the Road: <span class="hlt">CO</span><span class="hlt">2</span> from Contamination Gas to Energy Source.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Xie, Zhaojun; Zhang, Xin; Zhang, Zhang; Zhou, Zhen</p> <p>2017-04-01</p> <p>Rechargeable nonaqueous metal-<span class="hlt">air</span> batteries attract much attention for their high theoretical energy density, especially in the last decade. However, most reported metal-<span class="hlt">air</span> batteries are actually operated in a pure O <span class="hlt">2</span> atmosphere, while <span class="hlt">CO</span> <span class="hlt">2</span> and moisture in ambient <span class="hlt">air</span> can significantly impact the electrochemical performance of metal-O <span class="hlt">2</span> batteries. In the study of <span class="hlt">CO</span> <span class="hlt">2</span> contamination on metal-O <span class="hlt">2</span> batteries, it has been gradually found that <span class="hlt">CO</span> <span class="hlt">2</span> can be utilized as the reactant gas alone; namely, metal-<span class="hlt">CO</span> <span class="hlt">2</span> batteries can work. On the other hand, investigations on <span class="hlt">CO</span> <span class="hlt">2</span> fixation are in focus due to the potential threat of <span class="hlt">CO</span> <span class="hlt">2</span> on global climate change, especially for its steadily increasing concentration in the atmosphere. The exploitation of <span class="hlt">CO</span> <span class="hlt">2</span> in energy storage systems represents an alternative approach towards clean recycling and utilization of <span class="hlt">CO</span> <span class="hlt">2</span> . Here, the aim is to provide a timely summary of recent achievements in metal-<span class="hlt">CO</span> <span class="hlt">2</span> batteries, and inspire new ideas for new energy storage systems. Moreover, critical issues associated with reaction mechanisms and potential directions for future studies are discussed. © 2017 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/15825257','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15825257"><span>Effects of <span class="hlt">air</span> velocity on photosynthesis of plant canopies under elevated <span class="hlt">CO</span><span class="hlt">2</span> levels in a plant culture system.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kitaya, Y; Shibuya, T; Yoshida, M; Kiyota, M</p> <p>2004-01-01</p> <p>To obtain basic data for adequate <span class="hlt">air</span> circulation for promoting plant growth in closed plant production modules in bioregenerative life support systems in space, effects of <span class="hlt">air</span> velocities ranging from 0.1 to 0.8 m s-1 on photosynthesis in tomato seedlings canopies were investigated under atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentrations of 0.4 and 0.8 mmol mol-1. The canopy of tomato seedlings on a plug tray (0.4 x 0.4 m<span class="hlt">2</span>) was set in a wind-tunnel-type chamber (0.6 x 0.4 x 0.3 m3) installed in a semi-closed-type assimilation chamber (0.9 x 0.5 x 0.4 m3). The net photosynthetic rate in the plant canopy was determined with the differences in <span class="hlt">CO</span><span class="hlt">2</span> concentrations between the inlet and outlet of the assimilation chamber multiplied by the volumetric <span class="hlt">air</span> exchange rate of the chamber. Photosynthetic photon 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/2014AGUFMOS44A..01M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMOS44A..01M"><span>Developments in Airborne Oceanography and <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>Melville, W. K.</p> <p>2014-12-01</p> <p>, just as aircraft carriers "project force". Now we can measure winds, waves, temperatures, currents, radiative <span class="hlt">transfer</span>, images and <span class="hlt">air-sea</span> fluxes from aircraft over the ocean.I will review some of the history of airborne oceanography and present examples of how it can extend our knowledge and understanding of <span class="hlt">air-sea</span> interaction.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28841262','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28841262"><span>Measuring 13 C-enriched <span class="hlt">CO</span><span class="hlt">2</span> in <span class="hlt">air</span> with a cavity ring-down spectroscopy gas analyser: Evaluation and calibration.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Dickinson, Dane; Bodé, Samuel; Boeckx, Pascal</p> <p>2017-11-30</p> <p>Cavity ring-down spectroscopy (CRDS) is becoming increasingly popular for δ 13 C-<span class="hlt">CO</span> <span class="hlt">2</span> analysis of <span class="hlt">air</span>. However, little is known about the effect of high 13 C abundances on the performance of CRDS. Overlap between 12 <span class="hlt">CO</span> <span class="hlt">2</span> and 13 <span class="hlt">CO</span> <span class="hlt">2</span> spectral lines may adversely affect isotopic-<span class="hlt">CO</span> <span class="hlt">2</span> CRDS measurements of 13 C-enriched samples. Resolving this issue is important so that CRDS analysers can be used in <span class="hlt">CO</span> <span class="hlt">2</span> flux studies involving 13 C-labelled tracers. We tested a Picarro G2131-i CRDS isotopic-<span class="hlt">CO</span> <span class="hlt">2</span> gas analyser with specialty gravimetric standards of widely varying 13 C abundance (from natural to 20.1 atom%) and <span class="hlt">CO</span> <span class="hlt">2</span> mole fraction (x<span class="hlt">CO</span> <span class="hlt">2</span> : <0.1 to 2116 ppm) in synthetic <span class="hlt">air</span>. The presence of spectroscopic interference between 12 <span class="hlt">CO</span> <span class="hlt">2</span> and 13 <span class="hlt">CO</span> <span class="hlt">2</span> bands was assessed by analysing errors in measurements of the standards. A multi-component calibration strategy was adopted, incorporating isotope ratio and mole fraction data to ensure accuracy and consistency in corrected values of δ 13 C-<span class="hlt">CO</span> <span class="hlt">2</span> , x 12 <span class="hlt">CO</span> <span class="hlt">2</span> , and x 13 <span class="hlt">CO</span> <span class="hlt">2</span> . CRDS measurements of x 13 <span class="hlt">CO</span> <span class="hlt">2</span> were found to be accurate throughout the tested range (<0.005 to 100 ppm). On the other hand, spectral cross-talk in x 12 <span class="hlt">CO</span> <span class="hlt">2</span> measurements of standards containing elevated levels of 13 <span class="hlt">CO</span> <span class="hlt">2</span> led to inaccuracy in x 12 <span class="hlt">CO</span> <span class="hlt">2</span> , total-x<span class="hlt">CO</span> <span class="hlt">2</span> (x 12 <span class="hlt">CO</span> <span class="hlt">2</span>  + x 13 <span class="hlt">CO</span> <span class="hlt">2</span> ), and δ 13 C-<span class="hlt">CO</span> <span class="hlt">2</span> data. An empirical relationship for x 12 <span class="hlt">CO</span> <span class="hlt">2</span> measurements that incorporated the 13 C/ 12 C isotope ratio (i.e. 13 <span class="hlt">CO</span> <span class="hlt">2</span> / 12 <span class="hlt">CO</span> <span class="hlt">2</span> , RCO<span class="hlt">2</span>) as a secondary (non-linear) variable was found to compensate for the perturbations, and enabled accurate instrument calibration for all <span class="hlt">CO</span> <span class="hlt">2</span> compositions covered by our standard gases. 13 C-enrichement in <span class="hlt">CO</span> <span class="hlt">2</span> leads to minor errors in CRDS measurements of x 12 <span class="hlt">CO</span> <span class="hlt">2</span> . We propose an empirical correction for measurements of 13 C-enriched <span class="hlt">CO</span> <span class="hlt">2</span> in <span class="hlt">air</span> by CRDS instruments such as the Picarro G2131-i. Copyright © 2017 John Wiley & Sons, Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1389357','SCIGOV-DOEDE'); return false;" href="https://www.osti.gov/servlets/purl/1389357"><span>Atmospheric <span class="hlt">CO</span><span class="hlt">2</span> Records from Sites in the Main Geophysical Observatory <span class="hlt">Air</span> Sampling Network (1983 - 1993)</span></a></p> <p><a target="_blank" href="http://www.osti.gov/dataexplorer">DOE Data Explorer</a></p> <p>Brounshtein, A. M. [Main Geophysical Observatory, St. Petersburg, Russia; Shaskov, A. A. [Main Geophysical Observatory, St. Petersburg, Russia; Paramonova, N. N. [Main Geophysical Observatory, St. Petersburg, Russia; Privalov, V. I. [Main Geophysical Observatory, St. Petersburg, Russia; Starodubtsev, Y. A. [Main Geophysical Observatory, St. Petersburg, Russia</p> <p>1997-01-01</p> <p><span class="hlt">Air</span> samples were collected from five sites in the Main Geophysical Observatory <span class="hlt">air</span> sampling network to monitor the atmospheric <span class="hlt">CO</span><span class="hlt">2</span> from 1983 - 1993. Airwas collected generally four times per month in pairs of 1.5-L stainless steel electropolished flasks with one greaseless stainless steel stopcock. Sampling was performed by opening the stopcock of the flasks, which have been evacuated at the central laboratory at the Main Geophysical Observatory (MGO). The <span class="hlt">air</span> was not dried during sample collection. Attempts were made to obtain samples when the wind speed was >5 m/s and the wind direction corresponded to the predetermined "clean <span class="hlt">air</span>" sector. The period of record at Bering Island is too short to identify any long-term trends in atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentrations; however, the yearly mean atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentration at Bering Island rose from approximately 346 parts per million by volume (ppmv) in 1986 to 362.6 ppmv in 1993. Measurements from this station are considered indicative of maritime <span class="hlt">air</span> masses. The period of record at Kotelny Island is too short to identify any long-term trends in atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentrations; however, the yearly mean atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentration at Kotelny Island rose from 356.08 parts per million by volume (ppmv) in 1988 to 358.8 ppmv in 1993. Because Kotelny Island is the northernmost Russian sampling site, measurements from this site serve as a useful comparison to other northern sites (e.g., Alert, Northwest Territories). In late 1989, <span class="hlt">air</span> sampling began at the Russian site of Kyzylcha, located in the Republic of Uzbekistan. Unfortunately, the desert site at Kyzylcha has been out of operation since mid-1991 due to financial difficulties in Russia. The annual mean value of 359.02 parts per million by volume (ppmv) for 1990, the lone full year of operation, is higher than measurements from other monitoring programs at this latitude [e.g., Niwot Ridge (354.7 ppmv in 1990) and Tae-ahn Peninsula]. Station "C," an open ocean site, in the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24479263','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24479263"><span>Managing acute coronary syndrome during medical <span class="hlt">air</span> evacuation from a remote location at <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>Westmoreland, Andrew H</p> <p>2014-01-01</p> <p>Coronary emergencies at <span class="hlt">sea</span> requiring <span class="hlt">air</span> evacuation are not uncommon. On board a Nimitz-class aircraft carrier while in a remote location, an active duty sailor suffered a myocardial infarction. A medical evacuation by helicopter was necessary. <span class="hlt">Transfer</span> proved difficult due to the ship's location, poor flying conditions, and the patient's deteriorating condition. This case stresses the importance of expeditious diagnosis, treatment, and <span class="hlt">air</span> <span class="hlt">transfer</span> to shore-based facilities capable of providing definitive coronary care. A 33-yr-old man recently started on trazodone due to depression complained of chest pain. The patient was hemodynamically unstable and electrocardiogram showed ST segment elevation and Q waves in the anterior, inferior, and lateral leads. He was <span class="hlt">air</span>-lifted to the nearest accepting facility with cardiac catheterization capabilities, which was over 300 miles away. Poor weather conditions hindered the pilot's ability to fly the original course. The patient remained critical and medication choices were limited. Even with all of these obstacles, everyone involved performed his or her duties admirably. The patient's condition improved by the time the helicopter landed. He was then rushed by ambulance to the hospital's coronary care unit, where he was successfully treated. This case highlights the need to keep a high index of suspicion when patients complain of chest pain, regardless of age. It is of the utmost importance that individuals capable of thinking and acting quickly are assigned to medical evacuation teams, and that they continue to train regularly, as coronary events at <span class="hlt">sea</span> are not uncommon.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20090035581&hterms=air+measurement&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dair%2Bmeasurement','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20090035581&hterms=air+measurement&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dair%2Bmeasurement"><span>Retrieval of Mid-tropospheric <span class="hlt">CO</span><span class="hlt">2</span> Directly from <span class="hlt">AIRS</span> 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.; Pagano, Thomas S.</p> <p>2008-01-01</p> <p>We apply the method of Vanishing Partial Derivatives (VPD) to <span class="hlt">AIRS</span> spectra to retrieve daily the global distribution of <span class="hlt">CO</span><span class="hlt">2</span> at a nadir geospatial resolution of 90 km x 90 km without requiring a first-guess input beyond the global average. Our retrievals utilize the 15 (micro)m band radiances, a complex spectral region. This method may be of value in other applications, in which spectral signatures of multiple species are not well isolated spectrally from one another.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_18 --> <div id="page_19" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="361"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1811365W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1811365W"><span>Impacts of South East Biomass Burning on local <span class="hlt">air</span> quality in 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>Wai-man Yeung, Irene; Fat Lam, Yun; Eniolu Morakinyo, Tobi</p> <p>2016-04-01</p> <p>Biomass burning is a significant source of carbon monoxide and particulate matter, which is not only contribute to the local <span class="hlt">air</span> pollution, but also regional <span class="hlt">air</span> pollution. This study investigated the impacts of biomass burning emissions from Southeast Asia (<span class="hlt">SEA</span>) as well as its contribution to the local <span class="hlt">air</span> pollution in East and South China <span class="hlt">Sea</span>, including Hong Kong and Taiwan. Three years (2012 - 2014) of the Hybrid Single Particle Lagrangian-Integrated Trajectory (HYSPLIT) with particles dispersion analyses using NCEP (Final) Operational Global Analysis data (FNL) data (2012 - 2014) were analyzed to track down all possible long-range transport from <span class="hlt">SEA</span> with a sinking motion that worsened the surface <span class="hlt">air</span> quality (tropospheric downwash from the free troposphere). The major sources of <span class="hlt">SEA</span> biomass burning emissions were first identified using high fire emissions from the Global Fire Emission Database (GFED), followed by the HYSPLIT backward trajectory dispersion modeling analysis. The analyses were compared with the local observation data from Tai Mo Shan (1,000 msl) and Tap Mun (60 msl) in Hong Kong, as well as the data from Lulin mountain (<span class="hlt">2</span>,600 msl) in Taiwan, to assess the possible impacts of <span class="hlt">SEA</span> biomass burning on local <span class="hlt">air</span> quality. The correlation between long-range transport events from the particles dispersion results and locally observed <span class="hlt">air</span> quality data indicated that the background concentrations of ozone, PM<span class="hlt">2</span>.5 and PM10 at the surface stations were enhanced by 12 μg/m3, 4 μg/m3 and 7 μg/m3, respectively, while the long-range transport contributed to enhancements of 4 μg/m3, 4 μg/m3 and 8 μg/m3 for O3, PM<span class="hlt">2</span>.5 and PM10, respectively at the lower free atmosphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16777959','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16777959"><span>An inorganic carbon transport system responsible for acclimation specific to <span class="hlt">air</span> levels of <span class="hlt">CO</span><span class="hlt">2</span> in Chlamydomonas reinhardtii.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Yingjun; Spalding, Martin H</p> <p>2006-06-27</p> <p>Many photosynthetic microorganisms acclimate to <span class="hlt">CO</span>(<span class="hlt">2</span>) limited environments by induction and operation of <span class="hlt">CO</span>(<span class="hlt">2</span>)-concentrating mechanisms (CCMs). Despite their central role in CCM function, inorganic carbon (Ci) transport systems never have been identified in eukaryotic photosynthetic organisms. In the green alga Chlamydomonas reinhardtii, a mutant, pmp1, was described in 1983 with deficiencies in Ci transport, and a Pmp1 protein-associated Ci uptake system has been proposed to be responsible for Ci uptake in low <span class="hlt">CO</span>(<span class="hlt">2</span>) (<span class="hlt">air</span> level)-acclimated cells. However, even though pmp1 represents the only clear genetic link to Ci transport in microalgae and is one of only a very few mutants directly affecting the CCM itself, the identity of Pmp1 has remained unknown. Physiological analyses indicate that C. reinhardtii possesses multiple Ci transport systems responsible for acclimation to different levels of limiting <span class="hlt">CO</span>(<span class="hlt">2</span>) and that the Pmp1-associated transport system is required specifically for low (<span class="hlt">air</span> level) <span class="hlt">CO</span>(<span class="hlt">2</span>) acclimation. In the current study, we identified and characterized a pmp1 allelic mutant, <span class="hlt">air</span> dier 1 (ad1) that, like pmp1, cannot grow in low <span class="hlt">CO</span>(<span class="hlt">2</span>) (350 ppm) but can grow either in high <span class="hlt">CO</span>(<span class="hlt">2</span>) (5% <span class="hlt">CO</span>(<span class="hlt">2</span>)) or in very low <span class="hlt">CO</span>(<span class="hlt">2</span>) (<200 ppm). Molecular analyses revealed that the Ad1/Pmp1 protein is encoded by LciB, a gene previously identified as a <span class="hlt">CO</span>(<span class="hlt">2</span>)-responsive gene. LciB and three related genes in C. reinhardtii compose a unique gene family that encode four closely related, apparently soluble plastid proteins with no clearly identifiable conserved motifs.</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> exchange 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('http://adsabs.harvard.edu/abs/2017AMT....10.2163M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AMT....10.2163M"><span><span class="hlt">Air</span>Core-HR: a high-resolution column sampling to enhance the vertical description of CH4 and <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>Membrive, Olivier; Crevoisier, Cyril; Sweeney, Colm; Danis, François; Hertzog, Albert; Engel, Andreas; Bönisch, Harald; Picon, Laurence</p> <p>2017-06-01</p> <p>An original and innovative sampling system called <span class="hlt">Air</span>Core was presented by NOAA in 2010 Karion et al.(2010). It consists of a long ( > 100 m) and narrow ( < 1 cm) stainless steel tube that can retain a profile of atmospheric <span class="hlt">air</span>. The captured <span class="hlt">air</span> sample has then to be analyzed with a gas analyzer for trace mole fraction. In this study, we introduce a new <span class="hlt">Air</span>Core aiming to improve resolution along the vertical with the objectives to (i) better capture the vertical distribution of <span class="hlt">CO</span><span class="hlt">2</span> and CH4, (ii) provide a tool to compare <span class="hlt">Air</span>Cores and validate the estimated vertical resolution achieved by <span class="hlt">Air</span>Cores. This (high-resolution) <span class="hlt">Air</span>Core-HR consists of a 300 m tube, combining 200 m of 0.125 in. (3.175 mm) tube and a 100 m of 0.25 in. (6.35 mm) tube. This new configuration allows us to achieve a vertical resolution of 300 m up to 15 km and better than 500 m up to 22 km (if analysis of the retained sample is performed within 3 h). The <span class="hlt">Air</span>Core-HR was flown for the first time during the annual StratoScience campaign from CNES in August 2014 from Timmins (Ontario, Canada). High-resolution vertical profiles of <span class="hlt">CO</span><span class="hlt">2</span> and CH4 up to 25 km were successfully retrieved. These profiles revealed well-defined transport structures in the troposphere (also seen in CAMS-ECMWF high-resolution forecasts of <span class="hlt">CO</span><span class="hlt">2</span> and CH4 profiles) and captured the decrease of <span class="hlt">CO</span><span class="hlt">2</span> and CH4 in the stratosphere. The multi-instrument gondola also carried two other low-resolution <span class="hlt">Air</span>Core-GUF that allowed us to perform direct comparisons and study the underlying processing method used to convert the sample of <span class="hlt">air</span> to greenhouse gases vertical profiles. In particular, degrading the <span class="hlt">Air</span>Core-HR derived profiles to the low resolution of <span class="hlt">Air</span>Core-GUF yields an excellent match between both sets of CH4 profiles and shows a good consistency in terms of vertical structures. This fully validates the theoretical vertical resolution achievable by <span class="hlt">Air</span>Cores. Concerning <span class="hlt">CO</span><span class="hlt">2</span> although a good agreement is found in terms of vertical structure</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.afdc.energy.gov/case/2329','SCIGOVWS'); return false;" href="https://www.afdc.energy.gov/case/2329"><span>Alternative Fuels Data Center: <span class="hlt">Sea</span>-Tac and Alaska <span class="hlt">Air</span> Group Achieve</span></a></p> <p><a target="_blank" href="http://www.science.gov/aboutsearch.html">Science.gov Websites</a></p> <p></p> <p></p> <p>pilot project, Alaska <span class="hlt">Air</span> <em>Group</em> encountered a few hurdles during the switch to eGSE. <em>One</em> was Sky-High Results with Electric Ground Support Equipment</A> <span class="hlt">Sea</span>-Tac and Alaska <span class="hlt">Air</span> <em>Group</em> Achieve Data Center: <span class="hlt">Sea</span>-Tac and Alaska <span class="hlt">Air</span> <em>Group</em> Achieve Sky-High Results with Electric Ground Support</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20675550','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20675550"><span>Hypercarbic cardiorespiratory reflexes in the facultative <span class="hlt">air</span>-breathing fish jeju (Hoplerythrinus unitaeniatus): the role of branchial <span class="hlt">CO</span><span class="hlt">2</span> chemoreceptors.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>de Lima Boijink, Cheila; Florindo, Luiz Henrique; Leite, Cleo A Costa; Kalinin, Ana Lúcia; Milsom, William K; Rantin, Francisco Tadeu</p> <p>2010-08-15</p> <p>The aim of the present study was to determine the roles that externally versus internally oriented <span class="hlt">CO</span>(<span class="hlt">2</span>)/H(+)-sensitive chemoreceptors might play in promoting cardiorespiratory responses to environmental hypercarbia in the <span class="hlt">air</span>-breathing fish, Hoplerythrinus unitaeniatus (jeju). Fish were exposed to graded hypercarbia (1, <span class="hlt">2</span>.5, 5, 10 and 20% <span class="hlt">CO</span>(<span class="hlt">2</span>)) and also to graded levels of environmental acidosis (pH approximately 7.0, 6.0, 5.8, 5.6, 5.3 and 4.7) equal to the pH levels of the hypercarbic water to distinguish the relative roles of <span class="hlt">CO</span>(<span class="hlt">2</span>) versus H(+). We also injected boluses of <span class="hlt">CO</span>(<span class="hlt">2</span>)-equilibrated solutions (5, 10 and 20% <span class="hlt">CO</span>(<span class="hlt">2</span>)) and acid solutions equilibrated to the same pH as the <span class="hlt">CO</span>(<span class="hlt">2</span>) boluses into the caudal vein (internal) and buccal cavity (external) to distinguish between internal and external stimuli. The putative location of the chemoreceptors was determined by bilateral denervation of branches of cranial nerves IX (glossopharyngeal) and X (vagus) to the gills. The data indicate that the chemoreceptors eliciting bradycardia, hypertension and gill ventilatory responses (increased frequency and amplitude) to hypercarbia are exclusively branchial, externally oriented and respond specifically to changes in <span class="hlt">CO</span>(<span class="hlt">2</span>) and not H(+). Those involved in producing the cardiovascular responses appeared to be distributed across all gill arches while those involved in the gill ventilatory responses were located primarily on the first gill arch. Higher levels of aquatic <span class="hlt">CO</span>(<span class="hlt">2</span>) depressed gill ventilation and stimulated <span class="hlt">air</span> breathing. The chemoreceptors involved in producing <span class="hlt">air</span> breathing in response to hypercarbia also appeared to be branchial, distributed across all gill arches and responded specifically to changes in aquatic <span class="hlt">CO</span>(<span class="hlt">2</span>). This would suggest that chemoreceptor groups with different orientations (blood versus water) are involved in eliciting <span class="hlt">air</span>-breathing responses to hypercarbia in jeju.</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 exchange from the North <span class="hlt">Sea</span>. Wind, tides, and freshwater supply act very differently, but dominantly structure the ecosystem dynamics on spatial and temporal scales. The biological community is also different. Cyanobacteria, which are important due to their ability to fix atmospheric nitrogen, and they are only present in the Baltic <span class="hlt">Sea</span>. These differentiating features have a strong impact in the biogeochemical cycles and ultimately shape the variations in the carbonate chemistry. Here the ECOSMO model was employed on the North <span class="hlt">Sea</span> and Baltic <span class="hlt">Sea</span>. The model is set so both are modelled at the same time, instead of having them run separately. ECOSMO is a 3-D coupled</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29093514','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29093514"><span>Causes of variation among rice models in yield response to <span class="hlt">CO</span><span class="hlt">2</span> examined with Free-<span class="hlt">Air</span> <span class="hlt">CO</span><span class="hlt">2</span> Enrichment and growth chamber experiments.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hasegawa, Toshihiro; Li, Tao; Yin, Xinyou; Zhu, Yan; Boote, Kenneth; Baker, Jeffrey; Bregaglio, Simone; Buis, Samuel; Confalonieri, Roberto; Fugice, Job; Fumoto, Tamon; Gaydon, Donald; Kumar, Soora Naresh; Lafarge, Tanguy; Marcaida Iii, Manuel; Masutomi, Yuji; Nakagawa, Hiroshi; Oriol, Philippe; Ruget, Françoise; Singh, Upendra; Tang, Liang; Tao, Fulu; Wakatsuki, Hitomi; Wallach, Daniel; Wang, Yulong; Wilson, Lloyd Ted; Yang, Lianxin; Yang, Yubin; Yoshida, Hiroe; Zhang, Zhao; Zhu, Jianguo</p> <p>2017-11-01</p> <p>The <span class="hlt">CO</span> <span class="hlt">2</span> fertilization effect is a major source of uncertainty in crop models for future yield forecasts, but coordinated efforts to determine the mechanisms of this uncertainty have been lacking. Here, we studied causes of uncertainty among 16 crop models in predicting rice yield in response to elevated [<span class="hlt">CO</span> <span class="hlt">2</span> ] (E-[<span class="hlt">CO</span> <span class="hlt">2</span> ]) by comparison to free-<span class="hlt">air</span> <span class="hlt">CO</span> <span class="hlt">2</span> enrichment (FACE) and chamber experiments. The model ensemble reproduced the experimental results well. However, yield prediction in response to E-[<span class="hlt">CO</span> <span class="hlt">2</span> ] varied significantly among the rice models. The variation was not random: models that overestimated at one experiment simulated greater yield enhancements at the others. The variation was not associated with model structure or magnitude of photosynthetic response to E-[<span class="hlt">CO</span> <span class="hlt">2</span> ] but was significantly associated with the predictions of leaf area. This suggests that modelled secondary effects of E-[<span class="hlt">CO</span> <span class="hlt">2</span> ] on morphological development, primarily leaf area, are the sources of model uncertainty. Rice morphological development is conservative to carbon acquisition. Uncertainty will be reduced by incorporating this conservative nature of the morphological response to E-[<span class="hlt">CO</span> <span class="hlt">2</span> ] into the models. Nitrogen levels, particularly under limited situations, make the prediction more uncertain. Improving models to account for [<span class="hlt">CO</span> <span class="hlt">2</span> ] × N interactions is necessary to better evaluate management practices under climate change.</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 exchange 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/2015Nanot..26W4001R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015Nanot..26W4001R"><span>Metallic <span class="hlt">Co</span>S<span class="hlt">2</span> nanowire electrodes for high cycling performance supercapacitors</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ren, Ren; Faber, Matthew S.; Dziedzic, Rafal; Wen, Zhenhai; Jin, Song; Mao, Shun; Chen, Junhong</p> <p>2015-12-01</p> <p>We report metallic cobalt pyrite (<span class="hlt">Co</span>S<span class="hlt">2</span>) nanowires (NWs) prepared directly on current collecting electrodes, e.g., carbon cloth or graphite disc, for high-performance supercapacitors. These <span class="hlt">Co</span>S<span class="hlt">2</span> NWs have a variety of advantages for supercapacitor applications. Because the metallic <span class="hlt">Co</span>S<span class="hlt">2</span> NWs are synthesized directly on the current collector, the good electrical connection enables efficient charge <span class="hlt">transfer</span> between the active <span class="hlt">Co</span>S<span class="hlt">2</span> materials and the current collector. In addition, the open spaces between the <span class="hlt">sea</span> urchin structure NWs lead to a large accessible surface area and afford rapid mass transport. Moreover, the robust <span class="hlt">Co</span>S<span class="hlt">2</span> NW structure results in high stability of the active materials during long-term operation. Electrochemical characterization reveals that the <span class="hlt">Co</span>S<span class="hlt">2</span> NWs enable large specific capacitance (828.<span class="hlt">2</span> F g-1 at a scan rate of 0.01 V s-1) and excellent long term cycling stability (0-<span class="hlt">2</span>.5% capacity loss after 4250 cycles at 5 A g-1) for pseudocapacitors. This example of metallic <span class="hlt">Co</span>S<span class="hlt">2</span> NWs for supercapacitor applications expands the opportunities for transition metal sulfide-based nanostructures in emerging energy storage applications.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1389354','SCIGOV-DOEDE'); return false;" href="https://www.osti.gov/servlets/purl/1389354"><span>Atmospheric <span class="hlt">CO</span><span class="hlt">2</span> Records from Sites in the Umweltbundesamt (UBA) <span class="hlt">Air</span> Sampling Network (1972 - 1997)</span></a></p> <p><a target="_blank" href="http://www.osti.gov/dataexplorer">DOE Data Explorer</a></p> <p>Fricke, W. [Umweltbundesamt, Offenbach/Main, Germany; Wallasch, M. [Umweltbundesamt, Offenbach/Main, Germany; Uhse, Karin [Umweltbundesamt, Offenbach/Main, Germany; Schmidt, Martina [University of Heidelberg, Heidelberg, Germany; Levin, Ingeborg [University of Heidelberg, Heidelberg, Germany</p> <p>1998-01-01</p> <p><span class="hlt">Air</span> samples for the purpose of monitoring atmospheric <span class="hlt">CO</span><span class="hlt">2</span> were collected from five sites in the UBA <span class="hlt">air</span> sampling network. Annual atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentrations at Brotjacklriegel rose from 331.63 parts per million by volume (ppmv) in 1972 to 353.12 ppmv in 1988. Because of the site's forest location, the monthly atmospheric <span class="hlt">CO</span><span class="hlt">2</span> record from Brotjacklriegel exhibits very large seasonal amplitude. This amplitude reached almost 40 ppmv in 1985. Minimum mixing ratios are recorded at Brotjacklriegel during July-September; maximum values, during November-March. <span class="hlt">CO</span><span class="hlt">2</span> concentrations at Deuselbach rose from 340.82 parts per million by volume (ppmv) in 1972 to 363.76 ppmv in 1989. The monthly atmospheric <span class="hlt">CO</span><span class="hlt">2</span> record from Deuselbach is influenced by local agricultural activities and photosynthetic depletion but does not exhibit the large seasonal amplitude observed at other UBA monitoring sites. Minimum monthly atmospheric <span class="hlt">CO</span><span class="hlt">2</span> mixing ratios at Deuselbach are typically observed in August but may appear as early as June. Maximum values are seen in the record for November-March. Atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentrations at Schauinsland rose from ~328 parts per million by volume (ppmv) in 1972 to ~365 ppmv in 1997. This represents a growth rate of approximately 1.5 ppmv per year. The Schauinsland site is considered the least contaminated of the UBA sites. <span class="hlt">CO</span><span class="hlt">2</span> concentrations at Waldhof rose from 346.82 parts per million by volume (ppmv) in 1972 to 372.09 ppmv in 1993. The Waldhof site is subject to pollution sources; consequently, the monthly atmospheric <span class="hlt">CO</span><span class="hlt">2</span> record exhibits a large seasonal amplitude. Atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentrations at Westerland rose from ~329 parts per million by volume (ppmv) in 1973 to ~364 ppmv in 1997. The atmospheric <span class="hlt">CO</span><span class="hlt">2</span> record from Westerland shows a seasonal pattern similar to other UBA sites; minimum values are recorded during July-September; maximum mixing ratios during November-March.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JPS...379..298L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JPS...379..298L"><span>Elementary reaction modeling of reversible <span class="hlt">CO/CO</span><span class="hlt">2</span> electrochemical conversion on patterned nickel electrodes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Luo, Yu; Shi, Yixiang; Li, Wenying; Cai, Ningsheng</p> <p>2018-03-01</p> <p><span class="hlt">CO/CO</span><span class="hlt">2</span> are the major gas reactant/product in the fuel electrode of reversible solid oxide cells (RSOC). This study proposes a two-charge-<span class="hlt">transfer</span>-step mechanism to describe the reaction and <span class="hlt">transfer</span> processes of <span class="hlt">CO-CO</span><span class="hlt">2</span> electrochemical conversion on a patterned Ni electrode of RSOC. An elementary reaction model is developed to couple two charge <span class="hlt">transfer</span> reactions, C(Ni)+O<span class="hlt">2</span>-(YSZ) ↔ <span class="hlt">CO</span>(Ni)+(YSZ) +<span class="hlt">2</span>e- and <span class="hlt">CO</span>(Ni)+O<span class="hlt">2</span>-(YSZ) ↔ <span class="hlt">CO</span><span class="hlt">2</span>(Ni)+(YSZ)+<span class="hlt">2</span>e-, with adsorption/desorption, surface chemical reactions and surface diffusion. This model well validates in both solid oxide electrolysis cell (SOEC) and solid oxide fuel cell (SOFC) modes by the experimental data from a patterned Ni electrode with 10 μm stripe width at different p<span class="hlt">CO</span> (0-0.25 atm), p<span class="hlt">CO</span><span class="hlt">2</span> (0-0.35 atm) and operating temperature (600-700 °C). This model indicates SOEC mode is dominated by charge <span class="hlt">transfer</span> step C(Ni)+O<span class="hlt">2</span>-(YSZ)↔<span class="hlt">CO</span>(Ni)+(YSZ) +<span class="hlt">2</span>e-, while SOFC mode by <span class="hlt">CO</span>(Ni)+ O<span class="hlt">2</span>-(YSZ)↔<span class="hlt">CO</span><span class="hlt">2</span>(Ni)+(YSZ)+<span class="hlt">2</span>e- on the patterned Ni electrode. The sensitivity analysis shows charge <span class="hlt">transfer</span> step is the major rate-determining step for RSOC, besides, surface diffusion of <span class="hlt">CO</span> and <span class="hlt">CO</span><span class="hlt">2</span> as well as <span class="hlt">CO</span><span class="hlt">2</span> adsorption also plays a significant role in the electrochemical reaction of SOEC while surface diffusion of <span class="hlt">CO</span> and <span class="hlt">CO</span><span class="hlt">2</span> desorption could be <span class="hlt">co</span>-limiting in SOFC.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23636599','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23636599"><span>Neutral poly- and perfluoroalkyl substances in <span class="hlt">air</span> and seawater of the North <span class="hlt">Sea</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Xie, Zhiyong; Zhao, Zhen; Möller, Axel; Wolschke, Hendrik; Ahrens, Lutz; Sturm, Renate; Ebinghaus, Ralf</p> <p>2013-11-01</p> <p>Concentrations of neutral poly- and perfluoroalkyl substances (PFASs), such as fluorotelomer alcohols (FTOHs), perfluoroalkane sulfonamides (FASAs), perfluoroalkane sufonamidoethanols (FASEs), and fluorotelomer acrylates (FTACs), have been simultaneously determined in surface seawater and the atmosphere of the North <span class="hlt">Sea</span>. Seawater and <span class="hlt">air</span> samples were taken aboard the German research vessel Heincke on the cruise 303 from 15 to 24 May 2009. The concentrations of FTOHs, FASAs, FASEs, and FTACs in the dissolved phase were <span class="hlt">2</span>.6-74, <0.1-19, <0.1-63, and <1.0-9.0 pg L(-1), respectively. The highest concentrations were determined in the estuary of the Weser and Elbe rivers and a decreasing concentration profile appeared with increasing distance from the coast toward the central part of the North <span class="hlt">Sea</span>. Gaseous FTOHs, FASAs, FASEs, and FTACs were in the range of 36-126, 3.1-26, 3.7-19, and 0.8-5.6 pg m(-3), which were consistent with the concentrations determined in 2007 in the North <span class="hlt">Sea</span>, and approximately five times lower than those reported for an urban area of Northern Germany. These results suggested continuous continental emissions of neutral PFASs followed by transport toward the marine environment. <span class="hlt">Air</span>-seawater gas exchanges of neutral PFASs were estimated using fugacity ratios and the two-film resistance model based upon paired <span class="hlt">air</span>-seawater concentrations and estimated Henry's law constant values. Volatilization dominated for all neutral PFASs in the North <span class="hlt">Sea</span>. The <span class="hlt">air</span>-seawater gas exchange 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 exchange 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('http://adsabs.harvard.edu/abs/2016AGUOS.A23A..04C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOS.A23A..04C"><span><span class="hlt">Air-Sea</span> Momentum and Enthalpy Exchange in Coupled Atmosphere-Wave-Ocean Modeling of Tropical Cyclones</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Curcic, M.; Chen, S. S.</p> <p>2016-02-01</p> <p>The atmosphere and ocean are coupled through momentum, enthalpy, and mass 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 exchange in TCs. In particular, we focus on the explicit treatment of wave growth and dissipation for calculating atmospheric and oceanic stress, and its role in upper ocean mixing and surface cooling in the wake of the storm. Wind-wave misalignment and local wave disequilibrium result in difference between atmospheric and oceanic stress being largest on the left side of the storm. We find that explicit wave calculation in the coupled model reduces momentum <span class="hlt">transfer</span> 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/2003AGUFM.A51D0717M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003AGUFM.A51D0717M"><span>Field and Laboratory Measurements of Carbon Dioxide Mixing Ratios in <span class="hlt">Air</span> Using the LI-COR LI-7000 <span class="hlt">CO</span><span class="hlt">2</span>/H<span class="hlt">2</span>O Analyzer</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Murphy, P. C.; Lerner, B. M.; Williams, E. J.</p> <p>2003-12-01</p> <p><span class="hlt">Air</span> measurements of <span class="hlt">CO</span><span class="hlt">2</span> were made with a LI-COR LI-7000 <span class="hlt">CO</span><span class="hlt">2</span>/H<span class="hlt">2</span>O analyzer on the NOAA ship Ronald H. Brown during the New England <span class="hlt">Air</span> Quality Study (NEAQS 2002) field campaign. This instrument is an improved version of the older model LI-6262 <span class="hlt">CO</span><span class="hlt">2</span>/H<span class="hlt">2</span>O analyzer, which uses a non-dispersive IR radiation absorption technique. During NEAQS, we operated the LI-7000 without temperature regulation, using a simple <span class="hlt">2</span>-point calibration scheme. An intercomparison between our measurements of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> mixing ratios and those measured by a more sophisticated method, using temperature-regulation and a multipoint calibration with a LI-6252 <span class="hlt">CO</span><span class="hlt">2</span> analyzer (operated by AOML) shows generally good results ([<span class="hlt">CO</span><span class="hlt">2</span>]AL = [<span class="hlt">CO</span><span class="hlt">2</span>]AOML x 1.015 (0.010) - 5.7 (3.8) ppmv; R<span class="hlt">2</span> = 0.9889) in highly variable <span class="hlt">air</span> masses. During subsequent laboratory studies, we evaluated the instrument for the manufacturer's claims of improvement in signal noise, sample gas temperature equilibration and zero drift with temperature. Further work examined the instrument's susceptibility to rapid temperature changes, which has been previously demonstrated to introduce error of several ppmv ° C-1 in the LI-6252. A change in the LI-7000 optical bench temperature of 12 ° C in 1 hour caused a sampling error of ˜3 ppmv <span class="hlt">CO</span><span class="hlt">2</span>. Therefore, our lab investigations indicate that the LI-7000 would benefit from a temperature-controlled enclosure, as is used by the AOML group.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20020034734','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20020034734"><span>Mean Ages of Stratospheric <span class="hlt">Air</span> Derived From in Situ Observations of <span class="hlt">CO</span><span class="hlt">2</span>, CH4, and N<span class="hlt">2</span>O</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Andrews, A. E.; Boering, K. A.; Daube, B. C.; Wofsy, S. C.; Loewenstein, M.; Jost, H.; Podolske, J. R.; Webster, C. R.; Herman, R. L.; Scott, D. C.; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20020034734'); toggleEditAbsImage('author_20020034734_show'); toggleEditAbsImage('author_20020034734_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20020034734_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20020034734_hide"></p> <p>2001-01-01</p> <p>Accurate mean ages for stratospheric <span class="hlt">air</span> have been derived from a spatially and temporally comprehensive set of in situ observations of <span class="hlt">CO</span><span class="hlt">2</span>, CH4, and N<span class="hlt">2</span>O obtained from 1992 to 1998 from the NASA ER-<span class="hlt">2</span> aircraft and balloon flights. Errors associated with the tropospheric <span class="hlt">CO</span><span class="hlt">2</span> seasonal cycle and interannual variations in the <span class="hlt">CO</span><span class="hlt">2</span> growth rate are less than 0.5 year throughout the stratosphere and less than 0.3 year for <span class="hlt">air</span> older than <span class="hlt">2</span> years (N<span class="hlt">2</span>O less than 275 ppbv), indicating that the age spectra are broad enough to attenuate these influences over the time period covered by these observations. The distribution of mean age with latitude and altitude provides detailed, quantitative information about the general circulation of the stratosphere. At 20 km, sharp meridional gradients in the mean age are observed across the subtropics. Between 20 and 30 km, the average difference in mean age between the tropics and midlatitudes is approximately <span class="hlt">2</span> years, with slightly smaller differences at higher and lower altitudes. The mean age in the midlatitude middle stratosphere (approx. 25-32 km) is relatively constant with respect to altitude at 5 plus or minus 0.5 years. Comparison with earlier balloon observations of <span class="hlt">CO</span><span class="hlt">2</span> dating back to the 1970s indicates that the mean age of <span class="hlt">air</span> in this region has remained within 11 year of its current value over the last 25 years. A climatology of mean age is derived from the observed compact relationship between mean age and N<span class="hlt">2</span>O. These characteristics of the distribution of mean age in the stratosphere will serve as critically needed diagnostics for models of stratospheric transport.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1818509O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1818509O"><span>Exploring the influence of surface waves in the carbon dioxide <span class="hlt">transfer</span> velocity between the ocean and atmosphere in the coastal region</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ocampo-Torres, Francisco Javier; Francisco Herrera, Carlos; Gutiérrez-Loza, Lucía; Osuna, Pedro</p> <p>2016-04-01</p> <p>Field measurements have been carried out in order to better understand the possible influence of ocean surface waves in the <span class="hlt">transfer</span> of carbon dioxide between the ocean and atmosphere in the coastal zone. The <span class="hlt">CO</span><span class="hlt">2</span> fluxes are being analysed and results are shown in a contribution by Gutiérrez-Loza et al., in this session. Here we try to highlight the findings regarding the <span class="hlt">transfer</span> velocity (k<span class="hlt">CO</span><span class="hlt">2</span>) once we have incorporated direct measurements of carbon dioxide concentration in the water side. In this study direct measurements of <span class="hlt">CO</span><span class="hlt">2</span> fluxes were obtained with an eddy covariance tower located in the shoreline equipped with an infrared open-path gas analyzer (LI-7500, LI-COR) and a sonic anemometer (R3-100 Professional Anemometer, Gill Instruments), both at about 13 m above the mean <span class="hlt">sea</span> level, and sampling at 20 Hz. For some period of time simultaneous information of waves was recorded with a sampling rate of <span class="hlt">2</span> Hz using an Acoustic Doppler Current Profiler (Workhorse Sentinel, Teledyne RD Instruments) at 10 m depth and 350 m away from the tower. Besides, recently the concentration of <span class="hlt">CO</span><span class="hlt">2</span> in water has also been recorded making use of a SAMI-<span class="hlt">CO</span><span class="hlt">2</span> instrument. A subtle effect of the wave field is detected in the estimated k<span class="hlt">CO</span><span class="hlt">2</span>. Looking into details of the surface currents being detected very near the <span class="hlt">air-sea</span> interface through an ADPC, a certain association can be found with the gas <span class="hlt">transfer</span> velocity. Furthermore, some of the possible effects of breaking wave induced turbulence in the coastal zone is to be addressed. This work represents a RugDiSMar Project (CONACYT 155793) contribution. The support from CB-2011-01-168173 CONACYT project is greatly acknowledged.</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> exchange 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> exchange and transport can take place. Furthermore, also the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1389346','SCIGOV-DOEDE'); return false;" href="https://www.osti.gov/servlets/purl/1389346"><span>Atmospheric <span class="hlt">CO</span><span class="hlt">2</span> Records from Sites in the Scripps Institution of Oceanography (SIO) <span class="hlt">Air</span> Sampling Network (1985 - 2007)</span></a></p> <p><a target="_blank" href="http://www.osti.gov/dataexplorer">DOE Data Explorer</a></p> <p>Keeling, R. F. [Scripps Institution of Oceanography (SIO) University of California, La Jolla, California (USA); Piper, S. C. [Scripps Institution of Oceanography (SIO) University of California, La Jolla, California (USA); Bollenbacher, A. F. [Scripps Institution of Oceanography (SIO) University of California, La Jolla, California (USA); Walker , J. S. [Scripps Institution of Oceanography (SIO) University of California, La Jolla, California (USA)</p> <p>2008-05-01</p> <p>At Alert weekly <span class="hlt">air</span> samples are collected in 5-L evacuated glass flasks exposed in triplicate. Flasks are returned to the SIO for <span class="hlt">CO</span><span class="hlt">2</span> determinations, which are made using an Applied Physics Corporation nondispersive infrared gas analyzer. In May 1983, the <span class="hlt">CO</span><span class="hlt">2</span>-in-N<span class="hlt">2</span> calibration gases were replaced with <span class="hlt">CO</span><span class="hlt">2</span>-in-<span class="hlt">air</span> calibration gases, which are currently used (Keeling et al. 2002). Data are in terms of the Scripps "03A" calibration scale. On the basis of flask samples collected at Alert and analyzed by SIO, the annual average of the fitted monthly concentrations <span class="hlt">CO</span><span class="hlt">2</span> rose from 348.48 ppmv in 1986 to 384.84 ppmv in 2007. This represents an average annual growth rate of 1.73 ppmv per year at Alert.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26463894','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26463894"><span>Rice grain yield and quality responses to free-<span class="hlt">air</span> <span class="hlt">CO</span><span class="hlt">2</span> enrichment combined with soil and water warming.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Usui, Yasuhiro; Sakai, Hidemitsu; Tokida, Takeshi; Nakamura, Hirofumi; Nakagawa, Hiroshi; Hasegawa, Toshihiro</p> <p>2016-03-01</p> <p>Rising <span class="hlt">air</span> temperatures are projected to reduce rice yield and quality, whereas increasing atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentrations ([<span class="hlt">CO</span><span class="hlt">2</span> ]) can increase grain yield. For irrigated rice, ponded water is an important temperature environment, but few open-field evaluations are available on the combined effects of temperature and [<span class="hlt">CO</span><span class="hlt">2</span> ], which limits our ability to predict future rice production. We conducted free-<span class="hlt">air</span> <span class="hlt">CO</span><span class="hlt">2</span> enrichment and soil and water warming experiments, for three growing seasons to determine the yield and quality response to elevated [<span class="hlt">CO</span><span class="hlt">2</span> ] (+200 μmol mol(-1) , E-[<span class="hlt">CO</span><span class="hlt">2</span> ]) and soil and water temperatures (+<span class="hlt">2</span> °C, E-T). E-[<span class="hlt">CO</span><span class="hlt">2</span> ] significantly increased biomass and grain yield by approximately 14% averaged over 3 years, mainly because of increased panicle and spikelet density. E-T significantly increased biomass but had no significant effect on the grain yield. E-T decreased days from transplanting to heading by approximately 1%, but days to the maximum tiller number (MTN) stage were reduced by approximately 8%, which limited the panicle density and therefore sink capacity. On the other hand, E-[<span class="hlt">CO</span><span class="hlt">2</span> ] increased days to the MTN stage by approximately 4%, leading to a greater number of tillers. Grain appearance quality was decreased by both treatments, but E-[<span class="hlt">CO</span><span class="hlt">2</span> ] showed a much larger effect than did E-T. The significant decrease in undamaged grains (UDG) by E-[<span class="hlt">CO</span><span class="hlt">2</span> ] was mainly the result of an increased percentage of white-base grains (WBSG), which were negatively correlated with grain protein content. A significant decrease in grain protein content by E-[<span class="hlt">CO</span><span class="hlt">2</span> ] accounted in part for the increased WBSG. The dependence of WBSG on grain protein content, however, was different among years; the slope and intercept of the relationship were positively correlated with a heat dose above 26 °C. Year-to-year variation in the response of grain appearance quality demonstrated that E-[<span class="hlt">CO</span><span class="hlt">2</span> ] and rising <span class="hlt">air</span> temperatures synergistically reduce grain appearance quality of</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/2013AGUFMPP31B1871D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMPP31B1871D"><span>Terrestrial soil pH and MAAT records based on the MBT/CBT in the southern South China <span class="hlt">Sea</span>: implications for the atmospheric <span class="hlt">CO</span><span class="hlt">2</span> evolution in Southeast Asia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dong, L.; Li, L.; Li, Q.; Zhang, C.</p> <p>2013-12-01</p> <p>Liang Dong1, Li Li1, Qianyu Li1,<span class="hlt">2</span>, Chuanlun L. Zhang1,3 1State Key Laboratory of Marine Geology, Tongji University, Shanghai 200092, China <span class="hlt">2</span>School of Earth and Environment Sciences, University of Adelaide, SA 5005, Australia 3Department of Marine Sciences, University of Georgia, Athens, GA 30602, USA The methylation index of branched tetraethers (MBT) and/or the cyclization ratio of branched tetraethers (CBT) are derived from the branched glycerol dialkyl Glycerol tetraethers (GDGTs) of bacterial origin and are widely used to reconstruct the terrestrial soil pH and mean annual <span class="hlt">air</span> temperature (MAAT); however, these proxies are less frequently used in the oceanic settings. Here we provide the first high resolution records of soil pH and MAAT since the last glacial maximum based on the sedimentary core of MD05-2896 in the southern South China <span class="hlt">Sea</span>. The MAAT record exhibited typical glacial and interglacial cycles and was consistent with the winter insolation variation. The pH values were lower (6.4-7) in the glacial time and higher (7-8.4) in the interglacial time. Changes in soil pH allowed the evaluation of changes in soil <span class="hlt">CO</span><span class="hlt">2</span> based on the atmosphere-soil <span class="hlt">CO</span><span class="hlt">2</span> balance. The results imply that the lower winter MAAT variation with a lower winter atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentration might have resulted in a higher pH in the interglacial period. Our records provide a new insight into the evolution of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> between glacial and interglacial cycles in East Asia. Key words: South China <span class="hlt">Sea</span>, MBT/CBT, b-GDGTs, MAAT, pH</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010OcSci...6..913J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010OcSci...6..913J"><span>A numerical scheme to calculate temperature and salinity dependent <span class="hlt">air</span>-water <span class="hlt">transfer</span> velocities for any gas</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Johnson, M. T.</p> <p>2010-10-01</p> <p>The ocean-atmosphere flux of a gas can be calculated from its measured or estimated concentration gradient across the <span class="hlt">air-sea</span> interface and the <span class="hlt">transfer</span> velocity (a term representing the conductivity of the layers either side of the interface with respect to the gas of interest). Traditionally the <span class="hlt">transfer</span> velocity has been estimated from empirical relationships with wind speed, and then scaled by the Schmidt number of the gas being <span class="hlt">transferred</span>. Complex, physically based models of <span class="hlt">transfer</span> velocity (based on more physical forcings than wind speed alone), such as the NOAA COARE algorithm, have more recently been applied to well-studied gases such as carbon dioxide and DMS (although many studies still use the simpler approach for these gases), but there is a lack of validation of such schemes for other, more poorly studied gases. The aim of this paper is to provide a flexible numerical scheme which will allow the estimation of <span class="hlt">transfer</span> velocity for any gas as a function of wind speed, temperature and salinity, given data on the solubility and liquid molar volume of the particular gas. New and existing parameterizations (including a novel empirical parameterization of the salinity-dependence of Henry's law solubility) are brought together into a scheme implemented as a modular, extensible program in the R computing environment which is available in the supplementary online material accompanying this paper; along with input files containing solubility and structural data for ~90 gases of general interest, enabling the calculation of their total <span class="hlt">transfer</span> velocities and component parameters. Comparison of the scheme presented here with alternative schemes and methods for calculating <span class="hlt">air-sea</span> flux parameters shows good agreement in general. It is intended that the various components of this numerical scheme should be applied only in the absence of experimental data providing robust values for parameters for a particular gas of interest.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JPS...356..389O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JPS...356..389O"><span>Separator electrode assembly (<span class="hlt">SEA</span>) with 3-dimensional bioanode and removable <span class="hlt">air</span>-cathode boosts microbial fuel cell performance</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Oliot, M.; Etcheverry, L.; Mosdale, A.; Basseguy, R.; Délia, M.-L.; Bergel, A.</p> <p>2017-07-01</p> <p>Separator electrode assemblies (<span class="hlt">SEAs</span>) were designed by associating a microbial anode with an <span class="hlt">air</span>-cathode on each side of three different kinds of separator: plastic grid, J-cloth and baking paper. The <span class="hlt">SEA</span> was designed to allow the <span class="hlt">air</span>-cathode be removed and replaced without disturbing the bioanode. Power densities up to 6.4 W m-<span class="hlt">2</span> were produced by the Grid-<span class="hlt">SEAs</span> (on average 5.9 ± 0.5 W m-<span class="hlt">2</span>) while JCloth-<span class="hlt">SEAs</span> and Paper-<span class="hlt">SEAs</span> produced 4.8 ± 0.3 and 1.8 ± 0.1 W m-<span class="hlt">2</span>, respectively. Power densities decreased with time mainly because of fast deterioration of the cathode kinetics. They always increased again when the <span class="hlt">air</span>-cathodes were replaced by new ones; the Grid-<span class="hlt">SEAs</span> were thus boosted above 4 W m-<span class="hlt">2</span> after 7 weeks of operation. The theoretical analysis of <span class="hlt">SEA</span> functioning suggested that the high performance of the Grid-<span class="hlt">SEAs</span> was due to the combination of several virtuous phenomena: the efficient pH balance thanks to free diffusion through the large-mesh grid, the likely mitigation of oxygen crossover thanks to the 3-dimensional structure of the bioanode and the possibility of overcoming cathode fouling by replacing it during MFC operation. Finally, the microbial community of all bioanodes showed stringent selection of Proteiniphilum acetatigenes in proportion with the performance.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/11805831','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/11805831"><span>The effect of millennial-scale changes in Arabian <span class="hlt">Sea</span> denitrification on atmospheric <span class="hlt">CO</span><span class="hlt">2</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Altabet, Mark A; Higginson, Matthew J; Murray, David W</p> <p>2002-01-10</p> <p>Most global biogeochemical processes are known to respond to climate change, some of which have the capacity to produce feedbacks through the regulation of atmospheric greenhouse gases. Marine denitrification-the reduction of nitrate to gaseous nitrogen-is an important process in this regard, affecting greenhouse gas concentrations directly through the incidental production of nitrous oxide, and indirectly through modification of the marine nitrogen inventory and hence the biological pump for <span class="hlt">CO</span><span class="hlt">2</span>. Although denitrification has been shown to vary with glacial-interglacial cycles, its response to more rapid climate change has not yet been well characterized. Here we present nitrogen isotope ratio, nitrogen content and chlorin abundance data from sediment cores with high accumulation rates on the Oman continental margin that reveal substantial millennial-scale variability in Arabian <span class="hlt">Sea</span> denitrification and productivity during the last glacial period. The detailed correspondence of these changes with Dansgaard-Oeschger events recorded in Greenland ice cores indicates rapid, century-scale reorganization of the Arabian <span class="hlt">Sea</span> ecosystem in response to climate excursions, mediated through the intensity of summer monsoonal upwelling. Considering the several-thousand-year residence time of fixed nitrogen in the ocean, the response of global marine productivity to changes in denitrification would have occurred at lower frequency and appears to be related to climatic and atmospheric <span class="hlt">CO</span><span class="hlt">2</span> oscillations observed in Antarctic ice cores between 20 and 60 kyr ago.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016CliPa..12..339W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016CliPa..12..339W"><span>Effects of eustatic <span class="hlt">sea</span>-level change, ocean dynamics, and nutrient utilization on atmospheric p<span class="hlt">CO</span><span class="hlt">2</span> and seawater composition over the last 130 000 years: 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>Wallmann, K.; Schneider, B.; Sarnthein, M.</p> <p>2016-02-01</p> <p>We have developed and employed an Earth system model to explore the forcings of atmospheric p<span class="hlt">CO</span><span class="hlt">2</span> change and the chemical and isotopic evolution of seawater over the last glacial cycle. Concentrations of dissolved phosphorus (DP), reactive nitrogen, molecular oxygen, dissolved inorganic carbon (DIC), total alkalinity (TA), 13C-DIC, and 14C-DIC were calculated for 24 ocean boxes. The bi-directional water fluxes between these model boxes were derived from a 3-D circulation field of the modern ocean (Opa 8.<span class="hlt">2</span>, NEMO) and tuned such that tracer distributions calculated by the box model were consistent with observational data from the modern ocean. To model the last 130 kyr, we employed records of past changes in <span class="hlt">sea</span>-level, ocean circulation, and dust deposition. According to the model, about half of the glacial p<span class="hlt">CO</span><span class="hlt">2</span> drawdown may be attributed to marine regressions. The glacial <span class="hlt">sea</span>-level low-stands implied steepened ocean margins, a reduced burial of particulate organic carbon, phosphorus, and neritic carbonate at the margin seafloor, a decline in benthic denitrification, and enhanced weathering of emerged shelf sediments. In turn, low-stands led to a distinct rise in the standing stocks of DIC, TA, and nutrients in the global ocean, promoted the glacial sequestration of atmospheric <span class="hlt">CO</span><span class="hlt">2</span> in the ocean, and added 13C- and 14C-depleted DIC to the ocean as recorded in benthic foraminifera signals. The other half of the glacial drop in p<span class="hlt">CO</span><span class="hlt">2</span> was linked to inferred shoaling of Atlantic meridional overturning circulation and more efficient utilization of nutrients in the Southern Ocean. The diminished ventilation of deep water in the glacial Atlantic and Southern Ocean led to significant 14C depletions with respect to the atmosphere. According to our model, the deglacial rapid and stepwise rise in atmospheric p<span class="hlt">CO</span><span class="hlt">2</span> was induced by upwelling both in the Southern Ocean and subarctic North Pacific and promoted by a drop in nutrient utilization in the Southern Ocean. The deglacial <span class="hlt">sea</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27242536','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27242536"><span>Assessment of the Brain's Macro- and Micro-Circulatory Blood Flow Responses to <span class="hlt">CO</span><span class="hlt">2</span> via <span class="hlt">Transfer</span> Function Analysis.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Müller, Martin W-D; Österreich, Mareike; Müller, Andreas; Lygeros, John</p> <p>2016-01-01</p> <p>At present, there is no standard bedside method for assessing cerebral autoregulation (CA) with high temporal resolution. We combined the two methods most commonly used for this purpose, transcranial Doppler sonography (TCD, macro-circulation level), and near-infrared spectroscopy (NIRS, micro-circulation level), in an attempt to identify the most promising approach. In eight healthy subjects (5 women; mean age, 38 ± 10 years), CA disturbance was achieved by adding carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) to the breathing <span class="hlt">air</span>. We simultaneously recorded end-tidal <span class="hlt">CO</span><span class="hlt">2</span> (ETCO<span class="hlt">2</span>), blood pressure (BP; non-invasively at the fingertip), and cerebral blood flow velocity (CBFV) in both middle cerebral arteries using TCD and determined oxygenated and deoxygenated hemoglobin levels using NIRS. For the analysis, we used <span class="hlt">transfer</span> function calculations in the low-frequency band (0.07-0.15 Hz) to compare BP-CBFV, BP-oxygenated hemoglobin (OxHb), BP-tissue oxygenation index (TOI), CBFV-OxHb, and CBFV-TOI. ETCO<span class="hlt">2</span> increased from 37 ± <span class="hlt">2</span> to 44 ± 3 mmHg. The <span class="hlt">CO</span><span class="hlt">2</span>-induced CBFV increase significantly correlated with the OxHb increase (R (<span class="hlt">2</span>) = 0.526, p < 0.001). Compared with baseline, the mean <span class="hlt">CO</span><span class="hlt">2</span> administration phase shift (in radians) significantly increased (p < 0.005) from -0.67 ± 0.20 to -0.51 ± 0.25 in the BP-CBFV system, and decreased from 1.21 ± 0.81 to -0.05 ± 0.91 in the CBFV-OxHb system, and from 0.94 ± 1.22 to -0.24 ± 1.0 in the CBFV-TOI system; no change was observed for BP-OxHb (0.38 ± 1.17 to 0.41 ± 1.42). Gain changed significantly only in the BP-CBFV system. The correlation between the ETCO<span class="hlt">2</span> change and phase change was higher in the CBFV-OxHb system [r = -0.60; 95% confidence interval (CI): -0.16, -0.84; p < 0.01] than in the BP-CBFV system (r = 0.52; 95% CI: 0.03, 0.08; p < 0.05). The <span class="hlt">transfer</span> function characterizes the blood flow transition from macro- to micro-circulation by time delay only. The CBFV-OxHb system response with a broader phase shift distribution offers the prospect</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMGC23C1247L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMGC23C1247L"><span>Modeling Effects of Bicarbonate Release on Carbonate Chemistry and pH of the North <span class="hlt">Sea</span>: A Pilot Study for Atmospheric <span class="hlt">CO</span><span class="hlt">2</span> Reduction</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lettmann, K.; Kirchner, J.; Schnetger, B.; Wolff, J. O.; Brumsack, H. J.</p> <p>2016-12-01</p> <p>Rising <span class="hlt">CO</span><span class="hlt">2</span>-emissions accompanying the industrial revolution are the main drivers for climate change and ocean acidification. Several methods have been developed to capture <span class="hlt">CO</span><span class="hlt">2</span> from effluents and reduce emission. Here, we consider a promising approach that mimics natural limestone weathering: <span class="hlt">CO</span><span class="hlt">2</span> in effluent gas streams reacts with calcium carbonate in a limestone suspension. The resulting bicarbonate-rich solution can be released into natural systems. In comparison to classical carbon capture and storage (CCS) methods this artificial limestone weathering is cheaper and does not involve using toxic chemical compounds. Additionally there is no need for the controversially discussed storage of <span class="hlt">CO</span><span class="hlt">2</span> underground. The reduction of <span class="hlt">CO</span><span class="hlt">2</span>-emissions becomes more important for European industries as the EU introduced a system that limits the amount of allowable <span class="hlt">CO</span><span class="hlt">2</span>-emissions. Therefore, large <span class="hlt">CO</span><span class="hlt">2</span> emitters are forced to find cheap methods for emission reduction, as they often cannot circumvent <span class="hlt">CO</span><span class="hlt">2</span>-production. The method mentioned above is especially of interest for power plants located close to the coast that are already using seawater for cooling purposes. Thus, it is important to estimate the environmental effects if several coastal power plants will release high amounts of bicarbonate-rich waters into coastal waters, e.g. the North <span class="hlt">Sea</span>. In a first pilot study, the unstructured-grid finite-volume community ocean model (FVCOM) was combined with a chemical submodul (mocsy <span class="hlt">2</span>.0) to model the hydrodynamic circulation and mixing of bicarbonate-rich effluents from a gas power plant located at the German North <span class="hlt">Sea</span> coast. Here, we present the first preliminary results of this project, which include modelled changes of the North <span class="hlt">Sea</span> carbonate system and changes in pH value after the introduction of these bicarbonate-rich waters on short time scales up to one year.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AMT....10.2669T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AMT....10.2669T"><span>Abundances of isotopologues and calibration of <span class="hlt">CO</span><span class="hlt">2</span> greenhouse gas measurements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tans, Pieter P.; Crotwell, Andrew M.; Thoning, Kirk W.</p> <p>2017-07-01</p> <p>We have developed a method to calculate the fractional distribution of <span class="hlt">CO</span><span class="hlt">2</span> across all of its component isotopologues based on measured δ13C and δ18O values. The fractional distribution can be used with known total <span class="hlt">CO</span><span class="hlt">2</span> to calculate the amount of substance fraction (mole fraction) of each component isotopologue in <span class="hlt">air</span> individually. The technique is applicable to any molecule where isotopologue-specific values are desired. We used it with a new <span class="hlt">CO</span><span class="hlt">2</span> calibration system to account for isotopic differences among the primary <span class="hlt">CO</span><span class="hlt">2</span> standards that define the WMO X2007 <span class="hlt">CO</span><span class="hlt">2</span>-in-<span class="hlt">air</span> calibration scale and between the primary standards and standards in subsequent levels of the calibration hierarchy. The new calibration system uses multiple laser spectroscopic techniques to measure mole fractions of the three major <span class="hlt">CO</span><span class="hlt">2</span> isotopologues (16O12C16O, 16O13C16O, and 16O12C18O) individually. The three measured values are then combined into total <span class="hlt">CO</span><span class="hlt">2</span> (accounting for the rare unmeasured isotopologues), δ13C, and δ18O values. The new calibration system significantly improves our ability to <span class="hlt">transfer</span> the WMO <span class="hlt">CO</span><span class="hlt">2</span> calibration scale with low uncertainty through our role as the World Meteorological Organization Global Atmosphere Watch Central Calibration Laboratory for <span class="hlt">CO</span><span class="hlt">2</span>. Our current estimates for reproducibility of the new calibration system are ±0.01 µmol mol-1 <span class="hlt">CO</span><span class="hlt">2</span>, ±0.<span class="hlt">2</span> ‰ δ13C, and ±0.<span class="hlt">2</span> ‰ δ18O, all at 68 % confidence interval (CI).</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> exchange 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> exchange 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> exchange 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> exchange 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/22103582','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22103582"><span>Distribution and <span class="hlt">air-sea</span> exchange 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 exchange 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 exchange 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/2012EGUGA..1413625S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..1413625S"><span>Temporal evolution of the anthropogenic <span class="hlt">CO</span><span class="hlt">2</span> and acidification of the northwestern Mediterranean <span class="hlt">Sea</span>, from the mid-1990s to the mid-2000s</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Savy, J.-P.; Yao, K. M.; Touratier, F.; Goyet, C.</p> <p>2012-04-01</p> <p>Since the beginning of the industrial era, humankind consumption of fossil fuels at increasing rates has led to increases in atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentrations by approximately 105 ppm. In the same time, the Mediterranean coastal regions experienced a brutal population growth, from 94 million habitants in 1950 to 274 million in 2000, generating a strong anthropogenic pressure on the Mediterranean marine ecosystems. To follow the man-induced changes on the Mediterranean carbonate system properties (pH; total alkalinity, AT; total inorganic carbon CT, and <span class="hlt">CO</span><span class="hlt">2</span> partial pressure, p<span class="hlt">CO</span><span class="hlt">2</span>), an entire body-research has recently emerged in order to quantify both the present and future penetration of anthropogenic carbon (CANT) in the Mediterranean <span class="hlt">Sea</span> and the inferred acidification of its waters. From monthly observations accumulated over more than a decade (from 1993 to 2005) at DYFAMED time-series station (DYnamique des Flux Atmosphériques en MEDiterranée) located in the central part of the Ligurian <span class="hlt">Sea</span>, Touratier and Goyet (2009) have estimated the temporal evolution of CANT of the western Mediterranean <span class="hlt">Sea</span>. This study highlights that concentrations of anthropogenic <span class="hlt">CO</span><span class="hlt">2</span> are much higher at DYFAMED site (> 50 mol.kg-1) than those found in the Atlantic Ocean. Our study, conducted with measurements performed at 10 meters depth from 1995 to 2011 at the same location, allowed us to investigate the temporal evolution of CANT into the upper seawater layer. Our results indicate an averaged annual CANT increase of 3 µmol.kg-1 and a linked pH drop of 0.0032 per year confirming the ongoing acidification of the Mediterranean water masses. These results suggest the vulnerability and the endangerment of the Mediterranean ecosystems by the massive human-induced <span class="hlt">CO</span><span class="hlt">2</span> emissions. Touratier F. and C. Goyet (2009). Decadal evolution of anthropogenic <span class="hlt">CO</span><span class="hlt">2</span> in the north western Mediterranean <span class="hlt">Sea</span> (at the Dyfamed site) from the mid-1990's to the mid-2000's. Deep <span class="hlt">Sea</span> Research Part I, 56, 1708-1716</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.9500M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.9500M"><span>Spume Drops: Their Potential Role in <span class="hlt">Air-Sea</span> Gas Exchange</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Monahan, Edward C.; Staniec, Allison; Vlahos, Penny</p> <p>2017-12-01</p> <p>After summarizing the time scales defining the change of the physical properties of spume and other droplets cast up from the <span class="hlt">sea</span> surface, the time scales governing drop-atmosphere gas exchange are compared. Following a broad review of the spume drop production functions described in the literature, a subset of these functions is selected via objective criteria, to represent typical, upper bound, and lower bound production functions. Three complementary mechanisms driving spume-atmosphere gas exchange are described, and one is then used to estimate the relative importance, over a broad range of wind speeds, of this spume drop mechanism compared to the conventional, diffusional, <span class="hlt">sea</span> surface mechanism in <span class="hlt">air-sea</span> gas exchange. While remaining uncertainties in the wind dependence of the spume drop production 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 exchange.<abstract type="synopsis"><title type="main">Plain Language SummaryThis paper evaluates the existing spume drop generation functions available to date and selects a reasonable upper, lower and mid range function that are reasonable for use in <span class="hlt">air</span> <span class="hlt">sea</span> exchange models. Based on these the contribution of spume drops to overall <span class="hlt">air</span> <span class="hlt">sea</span> gas exchange at different wind speeds is then evaluated to determine the % contribution of spume. Generally below 20ms-1 spume drops contribute <1% of gas exchange but may account for a significant amount of gas exchange at higher wind speeds.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/34913','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/34913"><span>Re-assessment of plant carbon dynamics at the Duke free-<span class="hlt">air</span> <span class="hlt">CO</span><span class="hlt">2</span> enrichment site: interactions of atmospheric [<span class="hlt">CO</span><span class="hlt">2</span>] with nitrogen and water availability over stand development</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Heather R. McCarthy; Ram Oren; Kurt H Johnsen; Anne Gallet-Budynek; Seth G. Pritchard; Charles W Cook; Shannon L. LaDeau; Robert B. Jackson; Adrien C. Finzi</p> <p>2010-01-01</p> <p>The potential for elevated [<span class="hlt">CO</span><span class="hlt">2</span>]-induced changes to plant carbon (C) storage, through modifications in plant production and allocation of C among plant pools, is an important source of uncertainty when predicting future forest function. Utilizing 10 yr of data from the Duke free-<span class="hlt">air</span> <span class="hlt">CO</span><span class="hlt">2</span> enrichment site, we evaluated the...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AtmEn.178...31J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AtmEn.178...31J"><span>Seasonal atmospheric deposition and <span class="hlt">air-sea</span> gas exchange of polycyclic aromatic hydrocarbons over the Yangtze River Estuary, East China <span class="hlt">Sea</span>: Implications for source-sink processes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jiang, Yuqing; Lin, Tian; Wu, Zilan; Li, Yuanyuan; Li, Zhongxia; Guo, Zhigang; Yao, Xiaohong</p> <p>2018-04-01</p> <p>In this work, <span class="hlt">air</span> samples and surface seawater samples covering four seasons from March 2014 to January 2015 were collected from a background receptor site in the YRE to explore the seasonal fluxes of <span class="hlt">air-sea</span> gas exchange and dry and wet deposition of 15 polycyclic aromatic hydrocarbons (PAHs) and their source-sink processes at the <span class="hlt">air-sea</span> interface. The average dry and wet deposition 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 exchange 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 exchange 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/2014ChJOL..32..358Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014ChJOL..32..358Z"><span>Pyropia yezoensis can utilize <span class="hlt">CO</span><span class="hlt">2</span> in the <span class="hlt">air</span> during moderate dehydration</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhou, Wei; He, Linwen; Yang, Fang; Lin, Apeng; Zhang, Baoyu; Niu, Jianfeng; Wang, Guangce</p> <p>2014-03-01</p> <p>Pyropia yezoensis, an intertidal seaweed, experiences regular dehydration and rehydration with the tides. In this study, the responses of P. yezoensis to dehydration and rehydration under high and low <span class="hlt">CO</span><span class="hlt">2</span> concentrations ((600-700)×10-6 and (40-80)×10-6, named Group I and Group II respectively) were investigated. The thalli of Group I had a significantly higher effective photosystem II quantum yield than the thalli of Group II at 71% absolute water content (AWC). There was little difference between thalli morphology, total Rubisco activity and total protein content at 100% and 71% AWC, which might be the basis for the normal performance of photosynthesis during moderate dehydration. A higher effective photosystem I quantum yield was observed in the thalli subjected to a low <span class="hlt">CO</span><span class="hlt">2</span> concentration during moderate dehydration, which might be caused by the enhancement of cyclic electron flow. These results suggested that P. yezoensis can directly utilize <span class="hlt">CO</span><span class="hlt">2</span> in ambient <span class="hlt">air</span> during moderate dehydration.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AtmEn..92..280D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AtmEn..92..280D"><span>Spatial analysis on China's regional <span class="hlt">air</span> pollutants and <span class="hlt">CO</span><span class="hlt">2</span> emissions: emission pattern and regional disparity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dong, Liang; Liang, Hanwei</p> <p>2014-08-01</p> <p>China has suffered from serious <span class="hlt">air</span> pollution and <span class="hlt">CO</span><span class="hlt">2</span> emission. Challenges of emission reduction policy not only come from technology advancement, but also generate from the fact that, China has pronounced disparity between regions, in geographical and socioeconomic. How to deal with regional disparity is important to achieve the reduction target effectively and efficiently. This research conducts a spatial analysis on the emission patterns of three <span class="hlt">air</span> pollutants named SO<span class="hlt">2</span>, NOx and PM<span class="hlt">2</span>.5, and <span class="hlt">CO</span><span class="hlt">2</span>, in China's 30 provinces, applied with spatial auto-correlation and multi regression modeling. We further analyze the regional disparity and inequity issues with the approach of Lorenz curve and Gini coefficient. Results highlight that: there is evident cluster effect for the regional <span class="hlt">air</span> pollutants and <span class="hlt">CO</span><span class="hlt">2</span> emissions. While emission amount increases from western regions to eastern regions, the emission per GDP is in inverse trend. The Lorenz curve shows an even larger unequal distribution of GDP/emissions than GDP/capita in 30 regions. Certain middle and western regions suffers from a higher emission with lower GDP, which reveal the critical issue of emission leakage. Future policy making to address such regional disparity is critical so as to promote the emission control policy under the “equity and efficiency” principle.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E%26PSL.491..121C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26PSL.491..121C"><span>Benchmarking of vertically-integrated <span class="hlt">CO</span><span class="hlt">2</span> flow simulations at the Sleipner Field, 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>Cowton, L. R.; Neufeld, J. A.; White, N. J.; Bickle, M. J.; Williams, G. A.; White, J. C.; Chadwick, R. A.</p> <p>2018-06-01</p> <p>Numerical modeling plays an essential role in both identifying and assessing sub-surface reservoirs that might be suitable for future carbon capture and storage projects. Accuracy of flow simulations is tested by benchmarking against historic observations from on-going <span class="hlt">CO</span><span class="hlt">2</span> injection sites. At the Sleipner project located in the North <span class="hlt">Sea</span>, a suite of time-lapse seismic reflection surveys enables the three-dimensional distribution of <span class="hlt">CO</span><span class="hlt">2</span> at the top of the reservoir to be determined as a function of time. Previous attempts have used Darcy flow simulators to model <span class="hlt">CO</span><span class="hlt">2</span> migration throughout this layer, given the volume of injection with time and the location of the injection point. Due primarily to computational limitations preventing adequate exploration of model parameter space, these simulations usually fail to match the observed distribution of <span class="hlt">CO</span><span class="hlt">2</span> as a function of space and time. To circumvent these limitations, we develop a vertically-integrated fluid flow simulator that is based upon the theory of topographically controlled, porous gravity currents. This computationally efficient scheme can be used to invert for the spatial distribution of reservoir permeability required to minimize differences between the observed and calculated <span class="hlt">CO</span><span class="hlt">2</span> distributions. When a uniform reservoir permeability is assumed, inverse modeling is unable to adequately match the migration of <span class="hlt">CO</span><span class="hlt">2</span> at the top of the reservoir. If, however, the width and permeability of a mapped channel deposit are allowed to independently vary, a satisfactory match between the observed and calculated <span class="hlt">CO</span><span class="hlt">2</span> distributions is obtained. Finally, the ability of this algorithm to forecast the flow of <span class="hlt">CO</span><span class="hlt">2</span> at the top of the reservoir is assessed. By dividing the complete set of seismic reflection surveys into training and validation subsets, we find that the spatial pattern of permeability required to match the training subset can successfully predict <span class="hlt">CO</span><span class="hlt">2</span> migration for the validation subset. This ability suggests that it</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70174955','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70174955"><span>Sensitivity of Pliocene Arctic climate to orbital forcing, atmospheric <span class="hlt">CO</span><span class="hlt">2</span> and <span class="hlt">sea</span> ice albedo parameterisation</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Howell, Fergus W.; Haywood, Alan M.; Dowsett, Harry J.; Pickering, Steven J.</p> <p>2016-01-01</p> <p>With varying <span class="hlt">CO</span><span class="hlt">2</span>, orbit and <span class="hlt">sea</span> ice albedo values we are able to reproduce proxy temperature records that lean towards modest levels of high latitude warming, but other proxy data showing greater warming remain beyond the reach of our model. This highlights the importance of additional proxy records at high latitudes and ongoing efforts to compare proxy signals between sites.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.ars.usda.gov/research/publications/publication/?seqNo115=315803','TEKTRAN'); return false;" href="http://www.ars.usda.gov/research/publications/publication/?seqNo115=315803"><span>Responses of soybeans and wheat to elevated <span class="hlt">CO</span><span class="hlt">2</span> in free-<span class="hlt">air</span> and open top chamber systems</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>With increasing demand for agricultural products, more confidence is needed concerning impacts of rising atmospheric <span class="hlt">CO</span><span class="hlt">2</span> on crop yields. Despite debate about the merits of free-<span class="hlt">air</span> <span class="hlt">CO</span><span class="hlt">2</span> enrichment (FACE) and open top chamber (OTC) systems, there has been only one reported experiment directly compari...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017CSR...149...69K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017CSR...149...69K"><span>Carbonate system parameters and anthropogenic <span class="hlt">CO</span><span class="hlt">2</span> in the North Aegean <span class="hlt">Sea</span> during October 2013</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Krasakopoulou, E.; Souvermezoglou, E.; Giannoudi, L.; Goyet, C.</p> <p>2017-10-01</p> <p>Data of AT (total alkalinity) and CT (total inorganic carbon) collected during October 2013, on a N-S transect crossing the North of Lemnos basin allowed to identify the peculiarities of the <span class="hlt">CO</span><span class="hlt">2</span> system in the North Aegean <span class="hlt">Sea</span> and estimate the anthropogenic <span class="hlt">CO</span><span class="hlt">2</span> (CANT) concentrations. Extremely high concentrations of AT and CT were recorded in the upper layer of the North Aegean reflecting the high loads of AT and CT by the brackish BSW (Black <span class="hlt">Sea</span> Water) outflowing through the Dardanelles strait and by the rivers runoff. Both AT and CT exhibit strong negative linear correlation with salinity in the upper layer (0-20 m). Investigation of the AT-S relationship along with the salinity adjustment of AT revealed excess alkalinity throughout the water column in relation to the surface waters implying a possible occurrence of non-carbonate alkalinity inputs as well as of other processes that take place probably over the extended shelves and contribute to the alkalinity surplus. The intermediate layer occupied by the Modified Levantine Intermediate Water (MLIW) mass exhibits the lowest CT and AT concentrations, while rather elevated AT and CT concentrations characterize the North Aegean Deep Water (NAgDW) mass filling the deep layer of the North of Lemnos basin linked to previous dense water formation episodes. High anthropogenic <span class="hlt">CO</span><span class="hlt">2</span> content was detected at intermediate and deep layers of the North Aegean reflecting the effective transportation of the absorbed atmospheric <span class="hlt">CO</span><span class="hlt">2</span> from the surface to the deeper waters via the dense water formation episodes. The MLIW layer is more affected by the penetration of CANT than the NAgDW that fills the deep part of the basin. The observed variability of CANT distribution reflects the influence of the intensity of dense water formation events, of the different θ/S properties of the newly formed dense waters as well as of the diverse submarine pathways followed by the cascading dense waters. The invasion of CANT has lead to more acidic</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('http://adsabs.harvard.edu/abs/2017AGUFM.A41C2277B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A41C2277B"><span>Understanding the Role of <span class="hlt">Air-Sea</span> Interaction on Extreme Rainfall in Aquaplanet and Earth-like CESM<span class="hlt">2</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Benedict, J. J.; Clement, A. C.; Medeiros, B.</p> <p>2017-12-01</p> <p>Extreme precipitation events are associated with anomalous, latitudinally dependent dynamical and convective weather systems. For example, plumes of excessive poleward water vapor transport and topographical effects drive extreme precipitation events in the midlatitudes, while intense tropical precipitation is associated with organized convective systems. In both cases, <span class="hlt">air-sea</span> fluxes have the potential to contribute significantly to the moisture budget of these storms, but the roles of surface fluxes and upper-ocean processes and their impact on precipitation extremes have yet to be explored in sufficient detail. To examine such mechanisms, we implement a climate model hierarchy that encompasses a spectrum of ocean models, from prescribed-SST to fully dynamic, as well as both aquaplanet and Earth-like lower boundary types within version <span class="hlt">2</span> of the Community Earth System Model (CESM<span class="hlt">2</span>). Using the CESM<span class="hlt">2</span> hierarchy and comparing to observations, we identify key moisture processes and related <span class="hlt">air-sea</span> interactions that drive extreme precipitation events across different latitudes in Earth-like models and then generalize the analyses in aquaplanet configurations to highlight the most salient features. The analyses are applied to both present-day and global warming conditions to investigate how these fundamental mechanisms might change extreme precipitation events in the future climate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A53E2309Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A53E2309Y"><span>Effects of Northern Hemisphere <span class="hlt">Sea</span> Surface Temperature Changes on the Global <span class="hlt">Air</span> Quality</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yi, K.; Liu, J.</p> <p>2017-12-01</p> <p>The roles of regional <span class="hlt">sea</span> surface temperature (SST) variability on modulating the climate system and consequently the <span class="hlt">air</span> quality are investigated using the Community Earth System Model (CESM). Idealized, spatially uniform SST anomalies of +/- 1 °C are superimposed onto the North Pacific, North Atlantic, and North Indian Oceans individually. Ignoring the response of natural emissions, our simulations suggest large seasonal and regional variability of surface O3 and PM<span class="hlt">2</span>.5 concentrations in response to SST anomalies, especially during boreal summers. Increasing the SST by 1 °C in one of the oceans generally decreases the surface O3 concentrations from 1 to 5 ppbv while increases the anthropogenic PM<span class="hlt">2</span>.5 concentrations from 0.5 to 3 µg m-3. We implement the integrated process rate (IPR) analysis in CESM and find that meteorological transport in response to SST changes is the key process causing <span class="hlt">air</span> pollutant perturbations in most cases. During boreal summers, the increase in tropical SST over different ocean basins enhances deep convection, which significantly increases the <span class="hlt">air</span> temperature over the upper troposphere and trigger large-scale subsidence over nearby and remote regions. These processes tend to increase tropospheric stability and suppress rainfall at lower mid-latitudes. Consequently, it reduces the vertical transport of O3 to the surface while facilitating the accumulation of PM<span class="hlt">2</span>.5 concentrations over most regions. In addition, this regional SST warming may also considerably suppress intercontinental transport of <span class="hlt">air</span> pollution as confirmed with idealized <span class="hlt">CO</span>-like tracers. Our findings indicate a robust linkage between basin-scale SST variability and regional <span class="hlt">air</span> quality, which can help local <span class="hlt">air</span> quality management.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040014954&hterms=air+compressed&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dair%2Bcompressed','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040014954&hterms=air+compressed&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dair%2Bcompressed"><span>Development of a Next-Generation Membrane-Integrated Adsorption Processor for <span class="hlt">CO</span><span class="hlt">2</span> Removal and Compression for Closed-Loop <span class="hlt">Air</span> Revitalization Systems</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mulloth, Lila; LeVan, Douglas</p> <p>2002-01-01</p> <p>The current <span class="hlt">CO</span><span class="hlt">2</span> removal technology of NASA is very energy intensive and contains many non-optimized subsystems. This paper discusses the concept of a next-generation, membrane integrated, adsorption processor for <span class="hlt">CO</span><span class="hlt">2</span> removal nd compression in closed-loop <span class="hlt">air</span> revitalization systems. This processor will use many times less power than NASA's current <span class="hlt">CO</span><span class="hlt">2</span> removal technology and will be capable of maintaining a lower <span class="hlt">CO</span><span class="hlt">2</span> concentration in the cabin than that can be achieved by the existing <span class="hlt">CO</span><span class="hlt">2</span> removal systems. The compact, consolidated, configuration of gas dryer, <span class="hlt">CO</span><span class="hlt">2</span> separator, and <span class="hlt">CO</span><span class="hlt">2</span> compressor will allow continuous recycling of humid <span class="hlt">air</span> in the cabin and supply of compressed <span class="hlt">CO</span><span class="hlt">2</span> to the reduction unit for oxygen recovery. The device has potential application to the International Space Station and future, long duration, transit, and planetary missions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRD..122.7664L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRD..122.7664L"><span>Atmospheric deposition and <span class="hlt">air-sea</span> gas exchange 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 exchange 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 exchange 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 exchange reached equilibrium because of low HCH levels in the <span class="hlt">air</span> and seawater after the long-term banning of HCH and the degradation. The gas exchange 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 exchange 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/2016JGRE..121..965O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JGRE..121..965O"><span>Radiative <span class="hlt">transfer</span> in <span class="hlt">CO</span><span class="hlt">2</span>-rich atmospheres: 1. Collisional line mixing implies a colder early Mars</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ozak, N.; Aharonson, O.; Halevy, I.</p> <p>2016-06-01</p> <p>Fast and accurate radiative <span class="hlt">transfer</span> methods are essential for modeling <span class="hlt">CO</span><span class="hlt">2</span>-rich atmospheres, relevant to the climate of early Earth and Mars, present-day Venus, and some exoplanets. Although such models already exist, their accuracy may be improved as better theoretical and experimental constraints become available. Here we develop a unidimensional radiative <span class="hlt">transfer</span> code for <span class="hlt">CO</span><span class="hlt">2</span>-rich atmospheres, using the correlated k approach and with a focus on modeling early Mars. Our model differs from existing models in that it includes the effects of <span class="hlt">CO</span><span class="hlt">2</span> collisional line mixing in the calculation of the line-by-line absorption coefficients. Inclusion of these effects results in model atmospheres that are more transparent to infrared radiation and, therefore, in colder surface temperatures at radiative-convective equilibrium, compared with results of previous studies. Inclusion of water vapor in the model atmosphere results in negligible warming due to the low atmospheric temperatures under a weaker early Sun, which translate into climatically unimportant concentrations of water vapor. Overall, the results imply that sustained warmth on early Mars would not have been possible with an atmosphere containing only <span class="hlt">CO</span><span class="hlt">2</span> and water vapor, suggesting that other components of the early Martian climate system are missing from current models or that warm conditions were not long lived.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002QuEle..32..981S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002QuEle..32..981S"><span>LASER BIOLOGY AND MEDICINE: Laser analysis of the 13C/12C isotope ratio in <span class="hlt">CO</span><span class="hlt">2</span> in exhaled <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>Stepanov, E. V.</p> <p>2002-11-01</p> <p>Tunable diode lasers (TDLs) are applied to the diagnostics of gastroenterological diseases using respiratory tests and preparations enriched with the stable 13C isotope. This method of the analysis of the 13C/12C isotope ratio in <span class="hlt">CO</span><span class="hlt">2</span> in exhaled <span class="hlt">air</span> is based on the selective measurement of the resonance absorption at the vibrational — rotational structure of 12<span class="hlt">CO</span><span class="hlt">2</span> and 13<span class="hlt">CO</span><span class="hlt">2</span>. The <span class="hlt">CO</span><span class="hlt">2</span> transmission spectra in the region of 4.35 μm were measured with a PbEuSe double-heterostructure TDL. The accuracy of carbon isotope ratio measurements in <span class="hlt">CO</span><span class="hlt">2</span> of exhaled <span class="hlt">air</span> performed with the TDL was ~0.5%. The data of clinical tests of the developed laser-based analyser are presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013A%26A...557A...6K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013A%26A...557A...6K"><span>Clouds in the atmospheres of extrasolar planets. IV. On the scattering greenhouse effect of <span class="hlt">CO</span><span class="hlt">2</span> ice particles: Numerical radiative <span class="hlt">transfer</span> studies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kitzmann, D.; Patzer, A. B. C.; Rauer, H.</p> <p>2013-09-01</p> <p>Context. Owing to their wavelength-dependent absorption and scattering properties, clouds have a strong impact on the climate of planetary atmospheres. The potential greenhouse effect of <span class="hlt">CO</span><span class="hlt">2</span> ice clouds in the atmospheres of terrestrial extrasolar planets is of particular interest because it might influence the position and thus the extension of the outer boundary of the classic habitable zone around main sequence stars. Such a greenhouse effect, however, is a complicated function of the <span class="hlt">CO</span><span class="hlt">2</span> ice particles' optical properties. Aims: We study the radiative effects of <span class="hlt">CO</span><span class="hlt">2</span> ice particles obtained by different numerical treatments to solve the radiative <span class="hlt">transfer</span> equation. To determine the effectiveness of the scattering greenhouse effect caused by <span class="hlt">CO</span><span class="hlt">2</span> ice clouds, the radiative <span class="hlt">transfer</span> calculations are performed over the relevant wide range of particle sizes and optical depths, employing different numerical methods. Methods: We used Mie theory to calculate the optical properties of particle polydispersion. The radiative <span class="hlt">transfer</span> calculations were done with a high-order discrete ordinate method (DISORT). Two-stream radiative <span class="hlt">transfer</span> methods were used for comparison with previous studies. Results: The comparison between the results of a high-order discrete ordinate method and simpler two-stream approaches reveals large deviations in terms of a potential scattering efficiency of the greenhouse effect. The two-stream methods overestimate the transmitted and reflected radiation, thereby yielding a higher scattering greenhouse effect. For the particular case of a cool M-type dwarf, the <span class="hlt">CO</span><span class="hlt">2</span> ice particles show no strong effective scattering greenhouse effect by using the high-order discrete ordinate method, whereas a positive net greenhouse effect was found for the two-stream radiative <span class="hlt">transfer</span> schemes. As a result, previous studies of the effects of <span class="hlt">CO</span><span class="hlt">2</span> ice clouds using two-stream approximations overrated the atmospheric warming caused by the scattering greenhouse effect</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007BGD.....4.3863J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007BGD.....4.3863J"><span>The impact on atmospheric <span class="hlt">CO</span><span class="hlt">2</span> of iron fertilization induced changes in the ocean's biological pump</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jin, X.; Gruber, N.; Frenzel, H.; Doney, S. C.; McWilliams, J. C.</p> <p>2007-10-01</p> <p>Using numerical simulations, we quantify the impact of changes in the ocean's biological pump on the <span class="hlt">air-sea</span> balance of <span class="hlt">CO</span><span class="hlt">2</span> by fertilizing a small surface patch in the high-nutrient, low-chlorophyll region of the eastern tropical Pacific with iron. Decade-long fertilization experiments are conducted in a basin-scale, eddy-permitting coupled physical biogeochemical ecological model. In contrast to previous studies, we find that most of the dissolved inorganic carbon (DIC) removed from the euphotic zone by the enhanced biological export is replaced by uptake of <span class="hlt">CO</span><span class="hlt">2</span> from the atmosphere. Atmospheric uptake efficiencies, the ratio of the perturbation in <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> flux to the perturbation in export flux across 100 m, are 0.75 to 0.93 in our patch size-scale experiments. The atmospheric uptake efficiency is insensitive to the duration of the experiment. The primary factor controlling the atmospheric uptake efficiency is the vertical distribution of the enhanced biological production. Iron fertilization at the surface tends to induce production anomalies primarily near the surface, leading to high efficiencies. In contrast, mechanisms that induce deep production anomalies (e.g. altered light availability) tend to have a low uptake efficiency, since most of the removed DIC is replaced by lateral and vertical transport and mixing. Despite high atmospheric uptake efficiencies, patch-scale iron fertilization of the ocean's biological pump tends to remove little <span class="hlt">CO</span><span class="hlt">2</span> from the atmosphere over the decadal timescale considered here.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008BGeo....5..385J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008BGeo....5..385J"><span>The impact on atmospheric <span class="hlt">CO</span><span class="hlt">2</span> of iron fertilization induced changes in the ocean's biological pump</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jin, X.; Gruber, N.; Frenzel, H.; Doney, S. C.; McWilliams, J. C.</p> <p>2008-03-01</p> <p>Using numerical simulations, we quantify the impact of changes in the ocean's biological pump on the <span class="hlt">air-sea</span> balance of <span class="hlt">CO</span><span class="hlt">2</span> by fertilizing a small surface patch in the high-nutrient, low-chlorophyll region of the eastern tropical Pacific with iron. Decade-long fertilization experiments are conducted in a basin-scale, eddy-permitting coupled physical/biogeochemical/ecological model. In contrast to previous studies, we find that most of the dissolved inorganic carbon (DIC) removed from the euphotic zone by the enhanced biological export is replaced by uptake of <span class="hlt">CO</span><span class="hlt">2</span> from the atmosphere. Atmospheric uptake efficiencies, the ratio of the perturbation in <span class="hlt">air-sea</span> <span class="hlt">CO</span><span class="hlt">2</span> flux to the perturbation in export flux across 100 m, integrated over 10 years, are 0.75 to 0.93 in our patch size-scale experiments. The atmospheric uptake efficiency is insensitive to the duration of the experiment. The primary factor controlling the atmospheric uptake efficiency is the vertical distribution of the enhanced biological production and export. Iron fertilization at the surface tends to induce production anomalies primarily near the surface, leading to high efficiencies. In contrast, mechanisms that induce deep production anomalies (e.g. altered light availability) tend to have a low uptake efficiency, since most of the removed DIC is replaced by lateral and vertical transport and mixing. Despite high atmospheric uptake efficiencies, patch-scale iron fertilization of the ocean's biological pump tends to remove little <span class="hlt">CO</span><span class="hlt">2</span> from the atmosphere over the decadal timescale considered here.</p> </li> <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> exchange of heat and mass</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Szeri, Andrew J.</p> <p>2017-04-01</p> <p>Exchange of mass or heat across a turbulent liquid-gas interface is a problem of critical interest, especially in <span class="hlt">air-sea</span> <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> 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/25811418','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25811418"><span>Impacts of potential <span class="hlt">CO</span><span class="hlt">2</span>-reduction policies on <span class="hlt">air</span> quality in the United States.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Trail, Marcus A; Tsimpidi, Alexandra P; Liu, Peng; Tsigaridis, Kostas; Hu, Yongtao; Rudokas, Jason R; Miller, Paul J; Nenes, Athanasios; Russell, Armistead G</p> <p>2015-04-21</p> <p>Impacts of emissions changes from four potential U.S. <span class="hlt">CO</span><span class="hlt">2</span> emission reduction policies on 2050 <span class="hlt">air</span> quality are analyzed using the community multiscale <span class="hlt">air</span> quality model (CMAQ). Future meteorology was downscaled from the Goddard Institute for Space Studies (GISS) ModelE General Circulation Model (GCM) to the regional scale using the Weather Research Forecasting (WRF) model. We use emissions growth factors from the EPAUS9r MARKAL model to project emissions inventories for two climate tax scenarios, a combined transportation and energy scenario, a biomass energy scenario and a reference case. Implementation of a relatively aggressive carbon tax leads to improved PM<span class="hlt">2</span>.5 <span class="hlt">air</span> quality compared to the reference case as incentives increase for facilities to install flue-gas desulfurization (FGD) and carbon capture and sequestration (CCS) technologies. However, less capital is available to install NOX reduction technologies, resulting in an O3 increase. A policy aimed at reducing <span class="hlt">CO</span><span class="hlt">2</span> from the transportation sector and electricity production sectors leads to reduced emissions of mobile source NOX, thus reducing O3. Over most of the U.S., this scenario leads to reduced PM<span class="hlt">2</span>.5 concentrations. However, increased primary PM<span class="hlt">2</span>.5 emissions associated with fuel switching in the residential and industrial sectors leads to increased organic matter (OM) and PM<span class="hlt">2</span>.5 in some cities.</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 Exchange 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 exchange 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 exchange is dependent on the concentration gradient between <span class="hlt">air</span> and surface water and also on the gas <span class="hlt">transfer</span> velocity, often described with the gas <span class="hlt">transfer</span> coefficient k. We used the floating-chamber method in connection with surface water gas concentration measurements to estimate the gas <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> 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 <span class="hlt">transfer</span> velocity of <span class="hlt">CO</span><span class="hlt">2</span> was also similar between the two study lakes. The gas <span class="hlt">transfer</span> 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('https://www.ncbi.nlm.nih.gov/pubmed/19603146','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19603146"><span>Genotypes of Brassica rapa respond differently to plant-induced variation in <span class="hlt">air</span> <span class="hlt">CO</span><span class="hlt">2</span> concentration in growth chambers with standard and enhanced venting.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Edwards, Christine E; Haselhorst, Monia S H; McKnite, Autumn M; Ewers, Brent E; Williams, David G; Weinig, Cynthia</p> <p>2009-10-01</p> <p>Growth chambers allow measurement of phenotypic differences among genotypes under controlled environment conditions. However, unintended variation in growth chamber <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>]) may affect the expression of diverse phenotypic traits, and genotypes may differ in their response to variation in [<span class="hlt">CO</span><span class="hlt">2</span>]. We monitored [<span class="hlt">CO</span><span class="hlt">2</span>] and quantified phenotypic responses of 22 Brassica rapa genotypes in growth chambers with either standard or enhanced venting. [<span class="hlt">CO</span><span class="hlt">2</span>] in chambers with standard venting dropped to 280 micromol mol(-1) during the period of maximum canopy development, approximately 80 micromol mol(-1) lower than in chambers with enhanced venting. The stable carbon isotope ratio of <span class="hlt">CO</span><span class="hlt">2</span> in chamber <span class="hlt">air</span> (delta13C(<span class="hlt">air</span>)) was negatively correlated with [<span class="hlt">CO</span><span class="hlt">2</span>], suggesting that photosynthesis caused observed [<span class="hlt">CO</span><span class="hlt">2</span>] decreases. Significant genotype x chamber-venting interactions were detected for 12 of 20 traits, likely due to differences in the extent to which [<span class="hlt">CO</span><span class="hlt">2</span>] changed in relation to genotypes' phenology or differential sensitivity of genotypes to low [<span class="hlt">CO</span><span class="hlt">2</span>]. One trait, 13C discrimination (delta13C), was particularly influenced by unaccounted-for fluctuations in delta13C(<span class="hlt">air</span>) and [<span class="hlt">CO</span><span class="hlt">2</span>]. Observed responses to [<span class="hlt">CO</span><span class="hlt">2</span>] suggest that genetic variance components estimated in poorly vented growth chambers may be influenced by the expression of genes involved in <span class="hlt">CO</span><span class="hlt">2</span> stress responses; genotypic values estimated in these chambers may likewise be misleading such that some mapped quantitative trait loci may regulate responses to <span class="hlt">CO</span><span class="hlt">2</span> stress rather than a response to the environmental factor of interest. These results underscore the importance of monitoring, and where possible, controlling [<span class="hlt">CO</span><span class="hlt">2</span>].</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29882379','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29882379"><span>Fabricating Ir/C Nanofiber Networks as Free-Standing <span class="hlt">Air</span> Cathodes for Rechargeable Li-<span class="hlt">CO</span><span class="hlt">2</span> Batteries.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Chengyi; Zhang, Qinming; Zhang, Xin; Wang, Xin-Gai; Xie, Zhaojun; Zhou, Zhen</p> <p>2018-06-07</p> <p>Li-<span class="hlt">CO</span> <span class="hlt">2</span> batteries are promising energy storage systems by utilizing <span class="hlt">CO</span> <span class="hlt">2</span> at the same time, though there are still some critical barriers before its practical applications such as high charging overpotential and poor cycling stability. In this work, iridium/carbon nanofibers (Ir/CNFs) are prepared via electrospinning and subsequent heat treatment, and are used as cathode catalysts for rechargeable Li-<span class="hlt">CO</span> <span class="hlt">2</span> batteries. Benefitting from the unique porous network structure and the high activity of ultrasmall Ir nanoparticles, Ir/CNFs exhibit excellent <span class="hlt">CO</span> <span class="hlt">2</span> reduction and evolution activities. The Li-<span class="hlt">CO</span> <span class="hlt">2</span> batteries present extremely large discharge capacity, high coulombic efficiency, and long cycling life. Moreover, free-standing Ir/CNF films are used directly as <span class="hlt">air</span> cathodes to assemble Li-<span class="hlt">CO</span> <span class="hlt">2</span> batteries, which show high energy density and ultralong operation time, demonstrating great potential for practical applications. © 2018 WILEY-VCH Verlag GmbH & <span class="hlt">Co</span>. KGaA, Weinheim.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1416677-cooperative-electrocatalytic-reduction-involving-co-salophen-hydroquinone-electronproton-transfer-mediator','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1416677-cooperative-electrocatalytic-reduction-involving-co-salophen-hydroquinone-electronproton-transfer-mediator"><span>Cooperative Electrocatalytic O <span class="hlt">2</span> Reduction Involving <span class="hlt">Co</span>(salophen) with p- Hydroquinone as an Electron–Proton <span class="hlt">Transfer</span> Mediator</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>Anson, Colin W.; Stahl, Shannon S.</p> <p>2017-12-01</p> <p>The molecular cobalt complex, <span class="hlt">Co</span>(salophen), and para-hydroquinone (H<span class="hlt">2</span>Q) serve as effective cocatalysts for the electrochemical reduction of O<span class="hlt">2</span> to water. Mechanistic studies reveal redox cooperativity between <span class="hlt">Co</span>(salophen) and H<span class="hlt">2</span>Q. H<span class="hlt">2</span>Q serves as an electron-proton <span class="hlt">transfer</span> mediator (EPTM) that enables electrochemical O<span class="hlt">2</span> reduction at higher potentials and with faster rates than is observed with <span class="hlt">Co</span>(salophen) alone. Replacement of H<span class="hlt">2</span>Q with the higher potential EPTM, <span class="hlt">2</span>-chloro-H<span class="hlt">2</span>Q, allows for faster O<span class="hlt">2</span> reduction rates at higher applied potential. These results demonstrate a unique strategy to achieve improved performance with molecular electrocatalyst systems.</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 exchange 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 exchange 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 <span class="hlt">transfer</span> into the Red <span class="hlt">Sea</span> during the winter and a net <span class="hlt">transfer</span> 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> exchange 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('https://ntrs.nasa.gov/search.jsp?R=19860034311&hterms=current+feedback&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dcurrent%2Bfeedback','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19860034311&hterms=current+feedback&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dcurrent%2Bfeedback"><span><span class="hlt">Sea</span> surface temperature anomalies, planetary waves, and <span class="hlt">air-sea</span> feedback in the middle latitudes</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Frankignoul, C.</p> <p>1985-01-01</p> <p>Current analytical models for large-scale <span class="hlt">air-sea</span> interactions in the middle latitudes are reviewed in terms of known <span class="hlt">sea</span>-surface temperature (SST) anomalies. The scales and strength of different atmospheric forcing mechanisms are discussed, along with the damping and feedback processes controlling the evolution of the SST. Difficulties with effective SST modeling are described in terms of the techniques and results of case studies, numerical simulations of mixed-layer variability and statistical modeling. The relationship between SST and diabatic heating anomalies is considered and a linear model is developed for the response of the stationary atmosphere to the <span class="hlt">air-sea</span> feedback. The results obtained with linear wave models are compared with the linear model results. Finally, sample data are presented from experiments with general circulation models into which specific SST anomaly data for the middle latitudes were introduced.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4004332','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4004332"><span>Parity-Dependent Rotational Energy <span class="hlt">Transfer</span> in CN(A<span class="hlt">2</span>Π, ν = 4, jF1ε) + N<span class="hlt">2</span>, O<span class="hlt">2</span>, and <span class="hlt">CO</span><span class="hlt">2</span> Collisions</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>2015-01-01</p> <p>We report state-resolved total removal cross sections and state-to-state rotational energy <span class="hlt">transfer</span> (RET) cross sections for collisions of CN(A<span class="hlt">2</span>Π, ν = 4, jF1ε) with N<span class="hlt">2</span>, O<span class="hlt">2</span>, and <span class="hlt">CO</span><span class="hlt">2</span>. CN(X<span class="hlt">2</span>Σ+) was produced by 266 nm photolysis of ICN in a thermal bath (296 K) of the collider gas. A circularly polarized pulse from a dye laser prepared CN(A<span class="hlt">2</span>Π, ν = 4) in a range of F1e rotational states, j = <span class="hlt">2</span>.5, 3.5, 6.5, 11.5, 13.5, and 18.5. These prepared states were monitored using the circularly polarized output of an external cavity diode laser by frequency-modulated (FM) spectroscopy on the CN(A–X)(4,<span class="hlt">2</span>) band. The FM Doppler profiles were analyzed as a function of pump–probe delay to determine the time dependence of the population of the initially prepared states. Kinetic analysis of the resulting time dependences was used to determine total removal cross sections from the initially prepared levels. In addition, a range of j′ F1e and j′ F<span class="hlt">2</span>f product states resulting from rotational energy <span class="hlt">transfer</span> out of the j = 6.5 F1e initial state were probed, from which state-to-state RET cross sections were measured. The total removal cross sections lie in the order <span class="hlt">CO</span><span class="hlt">2</span> > N<span class="hlt">2</span> > O<span class="hlt">2</span>, with evidence for substantial cross sections for electronic and/or reactive quenching of CN(A, ν = 4) to unobserved products with <span class="hlt">CO</span><span class="hlt">2</span> and O<span class="hlt">2</span>. This is supported by the magnitude of the state-to-state RET cross sections, where a deficit of <span class="hlt">transferred</span> population is apparent for <span class="hlt">CO</span><span class="hlt">2</span> and O<span class="hlt">2</span>. A strong propensity for conservation of rotational parity in RET is observed for all three colliders. Spin–orbit-changing cross sections are approximately half of those of the respective conserving cross sections. These results are in marked disagreement with previous experimental observations with N<span class="hlt">2</span> as a collider but are in good agreement with quantum scattering calculations from the same study (Khachatrian et al. J. Phys. Chem. A2009, 113, 392219215110). Our results with <span class="hlt">CO</span><span class="hlt">2</span> as a collider are similarly in strong</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26931659','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26931659"><span><span class="hlt">Air-sea</span> exchange of gaseous mercury in the tropical coast (Luhuitou fringing reef) of the South China <span class="hlt">Sea</span>, the Hainan Island, China.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ci, Zhijia; Zhang, Xiaoshan; Wang, Zhangwei</p> <p>2016-06-01</p> <p>The <span class="hlt">air-sea</span> exchange of gaseous mercury (mainly Hg(0)) in the tropical ocean is an important part of the global Hg biogeochemical cycle, but the related investigations are limited. In this study, we simultaneously measured Hg(0) concentrations in surface waters and overlaying <span class="hlt">air</span> in the tropical coast (Luhuitou fringing reef) of the South China <span class="hlt">Sea</span> (SCS), Hainan Island, China, for 13 days on January-February 2015. The purpose of this study was to explore the temporal variation of Hg(0) concentrations in <span class="hlt">air</span> and surface waters, estimate the <span class="hlt">air-sea</span> Hg(0) 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://hdl.handle.net/2060/20040053519','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20040053519"><span>Material Properties Governing <span class="hlt">Co</span>-Current Flame Spread: The Effect of <span class="hlt">Air</span> Entrainment</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Coutin, Mickael; Rangwala, Ali S.; Torero, Jose L.; Buckley, Steven G.</p> <p>2003-01-01</p> <p>A study on the effects of lateral <span class="hlt">air</span> entrainment on an upward spreading flame has been conducted. The fuel is a flat PMMA plate of constant length and thickness but variable width. Video images and surface temperatures have allowed establishing the progression of the pyrolyis front and on the flame stand-off distance. These measurements have been incorporated into a theoretical formulation to establish characteristic mass <span class="hlt">transfer</span> numbers ("B" numbers). The mass <span class="hlt">transfer</span> number is deemed as a material related parameter that could be used to assess the potential of a material to sustain <span class="hlt">co</span>-current flame spread. The experimental results show that the theoretical formulation fails to describe heat exchange between the flame and the surface. The discrepancies seem to be associated to lateral <span class="hlt">air</span> entrainment that lifts the flame off the surface and leads to an over estimation of the local mass <span class="hlt">transfer</span> number. Particle Image Velocimetry (PIV) measurements are in the process of being acquired. These measurements are intended to provide insight on the effect of <span class="hlt">air</span> entrainment on the flame stand-off distance. A brief description of the methodology to be followed is presented here.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_21 --> <div id="page_22" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="421"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA571554','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA571554"><span>Integration of an Emerging Highly Sensitive Optical <span class="hlt">CO</span><span class="hlt">2</span> Sensor for Ocean Monitoring on an Existing Data Acquisition System <span class="hlt">Sea</span>Keeper 1000 (trademark)</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2012-09-30</p> <p>be deployed in geat numbers to autonomously monitor the overall patterns of <span class="hlt">CO</span><span class="hlt">2</span> emissions and ocean acidification . OBJECTIVES  Meet the...Integration of an Emerging Highly Sensitive Optical <span class="hlt">CO</span><span class="hlt">2</span> Sensor for Ocean Monitoring on an Existing Data Acquisition System <span class="hlt">Sea</span>Keeper 1000TM Annual...challenging requirements for ocean p<span class="hlt">CO</span><span class="hlt">2</span> monitoring using an innovative sensor design based on high sensitivity fluorescence detection.  Assemble the system</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA555149','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA555149"><span>Integration of an Emerging Highly Sensitive Optical <span class="hlt">CO</span><span class="hlt">2</span> Sensor for Ocean Monitoring on an Existing Data Acquisition System <span class="hlt">Sea</span>Keeper 1000(TM)</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2011-09-30</p> <p>be deployed in geat numbers to autonomously monitor the overall patterns of <span class="hlt">CO</span><span class="hlt">2</span> emissions and ocean acidification . OBJECTIVES  Meet the...Integration of an Emerging Highly Sensitive Optical <span class="hlt">CO</span><span class="hlt">2</span> Sensor for Ocean Monitoring on an Existing Data Acquisition System <span class="hlt">Sea</span>Keeper 1000TM Annual...challenging requirements for ocean p<span class="hlt">CO</span><span class="hlt">2</span> monitoring using an innovative sensor design based on high sensitivity fluorescence detection.  Assemble the system</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 exchange momentum, heat and freshwater. Mechanisms for the exchange 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/29740977','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29740977"><span>Coupling Glucose Dehydrogenation with <span class="hlt">CO</span><span class="hlt">2</span> Hydrogenation by Hydrogen <span class="hlt">Transfer</span> in Aqueous Media at Room Temperature.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ding, Guodong; Su, Ji; Zhang, Cheng; Tang, Kan; Yang, Lisha; Lin, Hongfei</p> <p>2018-05-08</p> <p>Conversion of carbon dioxide into value-added chemicals and fuels provides a direct solution to reduce excessive <span class="hlt">CO</span><span class="hlt">2</span> in the atmosphere. Herein, a novel catalytic reaction system is presented by coupling the dehydrogenation of glucose with the hydrogenation of a <span class="hlt">CO</span><span class="hlt">2</span> derived salt, ammonium carbonate, in the ethanol-water mixture. For the first time, the hydrogenation of <span class="hlt">CO</span><span class="hlt">2</span> into formate by glucose has been achieved under ambient conditions. Under the optimal reaction conditions, the highest yield of formate reached ~ 46 %. We find that the apparent pH value in the ethanol-water mixture plays a central role in determining the performance of the hydrogen <span class="hlt">transfer</span> reaction. Based on the 13C NMR and ESI-MS results, a possible pathway of the coupled glucose dehydrogenation and <span class="hlt">CO</span><span class="hlt">2</span> hydrogenation reactions was proposed. © 2018 WILEY-VCH Verlag GmbH & <span class="hlt">Co</span>. KGaA, Weinheim.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1389382','SCIGOV-DOEDE'); return false;" href="https://www.osti.gov/servlets/purl/1389382"><span>Mixing Ratios of <span class="hlt">CO</span>, <span class="hlt">CO</span><span class="hlt">2</span>, CH4, and Isotope Ratios of Associated 13C, 18O, and <span class="hlt">2</span>H in <span class="hlt">Air</span> Samples from Niwot Ridge, Colorado\\, and Montana de Oro, California, USA (January 2004)</span></a></p> <p><a target="_blank" href="http://www.osti.gov/dataexplorer">DOE Data Explorer</a></p> <p>Tyler, Stanley C. [Department of Earth System Science, University of California, Irvine, CA (USA)</p> <p>2004-01-01</p> <p><span class="hlt">Air</span> samples from Niwot Ridge, Colorado (41°N, 105°W) and Montaña de Oro, CA (35°N, 121°W) have been collected at approximately semi-monthly to monthly intervals since the mid 1990s. Such time series can provide information about: (1) seasonal cycling of <span class="hlt">CO</span>, <span class="hlt">CO</span><span class="hlt">2</span>, and CH4 sources and sinks in background <span class="hlt">air</span>, (<span class="hlt">2</span>) trends in atmospheric concentrations of <span class="hlt">CO</span><span class="hlt">2</span> and CH4 and their stable carbon, oxygen, and hydrogen isotopes, (3) the distribution of the hydroxyl (OH) radical in the atmosphere, and (4) the role of the terrestrial biosphere as a source or sink of atmospheric <span class="hlt">CO</span><span class="hlt">2</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/862075','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/862075"><span>Numerical Studies of Fluid Leakage from a Geologic DisposalReservoir for <span class="hlt">CO</span><span class="hlt">2</span> Show Self-Limiting Feedback between Fluid Flow and Heat<span class="hlt">Transfer</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>Pruess, Karsten</p> <p>2005-03-22</p> <p>Leakage of <span class="hlt">CO</span><span class="hlt">2</span> from a hypothetical geologic storage reservoir along an idealized fault zone has been simulated, including transitions between supercritical, liquid, and gaseous <span class="hlt">CO</span><span class="hlt">2</span>. We find strong non-isothermal effects due to boiling and Joule-Thomson cooling of expanding <span class="hlt">CO</span><span class="hlt">2</span>. Leakage fluxes are limited by limitations in conductive heat <span class="hlt">transfer</span> to the fault zone. The interplay between multiphase flow and heat <span class="hlt">transfer</span> effects produces non-monotonic leakage behavior.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1038534','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1038534"><span>A <span class="hlt">Sea</span> Floor Gravity Survey of the Sleipner Field to Monitor <span class="hlt">CO</span><span class="hlt">2</span> Migration</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>Mark Zumberge</p> <p></p> <p>Carbon dioxide gas (<span class="hlt">CO</span>{sub <span class="hlt">2</span>}) is a byproduct of many wells that produce natural gas. Frequently the <span class="hlt">CO</span>{sub <span class="hlt">2</span>} separated from the valuable fossil fuel gas is released into the atmosphere. This adds to the growing problem of the climatic consequences of greenhouse gas contamination. In the Sleipner North <span class="hlt">Sea</span> natural gas production facility, the separated <span class="hlt">CO</span>{sub <span class="hlt">2</span>} is injected into an underground saline aquifer to be forever sequestered. Monitoring the fate of such sequestered material is important - and difficult. Local change in Earth's gravity field over the injected gas is one way to detect the <span class="hlt">CO</span>{sub <span class="hlt">2</span>} andmore » track its migration within the reservoir over time. The density of the injected gas is less than that of the brine that becomes displaced from the pore space of the formation, leading to slight but detectable decrease in gravity observed on the seafloor above the reservoir. Using equipment developed at Scripps Institution of Oceanography, we have been monitoring gravity over the Sleipner <span class="hlt">CO</span>{sub <span class="hlt">2</span>} sequestration reservoir since 2002. We surveyed the field in 2009 in a project jointly funded by a consortium of European oil and gas companies and the US Department of Energy. The value of gravity at some 30 benchmarks on the seafloor, emplaced at the beginning of the monitoring project, was observed in a week-long survey with a remotely operated vehicle. Three gravity meters were deployed on the benchmarks multiple times in a campaign-style survey, and the measured gravity values compared to those collected in earlier surveys. A clear signature in the map of gravity differences is well correlated with repeated seismic surveys.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015ECSS..166...13L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015ECSS..166...13L"><span>Net ecosystem production, calcification and <span class="hlt">CO</span><span class="hlt">2</span> fluxes on a reef flat in Northeastern Brazil</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Longhini, Cybelle M.; Souza, Marcelo F. L.; Silva, Ananda M.</p> <p>2015-12-01</p> <p>The carbon cycle in coral reefs is usually dominated by the organic carbon metabolism and precipitation-dissolution of Ca<span class="hlt">CO</span>3, processes that control the <span class="hlt">CO</span><span class="hlt">2</span> partial pressure (p<span class="hlt">CO</span><span class="hlt">2</span>) in seawater and the <span class="hlt">CO</span><span class="hlt">2</span> fluxes through the <span class="hlt">air-sea</span> interface. In order to characterize these processes and the carbonate system, four sampling surveys were conducted at the reef flat of Coroa Vermelha during low tide (exposed flat). Net ecosystem production (NEP), net precipitation-dissolution of Ca<span class="hlt">CO</span>3 (G) and <span class="hlt">CO</span><span class="hlt">2</span> fluxes across the <span class="hlt">air</span>-water interface were calculated. The reef presented net autotrophy and calcification at daytime low tide. The NEP ranged from -8.7 to 31.6 mmol C m-<span class="hlt">2</span> h-1 and calcification from -13.1 to 26.0 mmol C m-<span class="hlt">2</span> h-1. The highest calcification rates occurred in August 2007, coinciding with the greater NEP rates. The daytime <span class="hlt">CO</span><span class="hlt">2</span> fluxes varied from -9.7 to 22.6 μmol <span class="hlt">CO</span><span class="hlt">2</span> m-<span class="hlt">2</span> h-1, but reached up to 13,900 μmol <span class="hlt">CO</span><span class="hlt">2</span> m-<span class="hlt">2</span> h-1 during nighttime. Carbon dioxide influx to seawater was predominant in the reef flat during low tide. The regions adjacent to the reef showed a supersaturation of <span class="hlt">CO</span><span class="hlt">2</span>, acting as a source of <span class="hlt">CO</span><span class="hlt">2</span> to the atmosphere (from -22.8 to -<span class="hlt">2</span>.6 mol <span class="hlt">CO</span><span class="hlt">2</span> m-<span class="hlt">2</span> h-1) in the reef flat during ebbing tide. Nighttime gas release to the atmosphere indicates a net <span class="hlt">CO</span><span class="hlt">2</span> release from the Coroa Vermelha reef flat within 24 h, and that these fluxes can be important to carbon budget in coral reefs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMED11D0171C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMED11D0171C"><span>Measurements of <span class="hlt">CO</span><span class="hlt">2</span> Mole Fractionand δ13C in Archived <span class="hlt">Air</span> Samples from Cape Meares, Oregon (USA) 1977 - 1998</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Clark, O.; Rice, A. L.</p> <p>2017-12-01</p> <p>Carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) is the most abundant, anthropogenically forced greenhouse gas (GHG) in the global atmosphere. Emissions of <span class="hlt">CO</span><span class="hlt">2</span> account for approximately 75% of the world's total GHG emissions. Atmospheric concentrations of <span class="hlt">CO</span><span class="hlt">2</span> are higher now than they've been at any other time in the past 800,000 years. Currently, the global mean concentration exceeds 400 ppm. Today, global networks regularly monitor <span class="hlt">CO</span><span class="hlt">2</span> concentrations and isotopic composition (δ13C and δ18O). However, past data is sparse. Over 200 ambient <span class="hlt">air</span> samples from Cape Meares, Oregon (45.5°N, 124.0°W), a coastal site in Western United States, were obtained by researchers at Oregon Institute of Science and Technology (OGI, now Oregon Health & Science University), between the years of 1977 and 1998 as part of a global monitoring program of six different sites in the polar, middle, and tropical latitudes of the Northern and Southern Hemispheres. <span class="hlt">Air</span> liquefaction was used to compress approximately 1000L of <span class="hlt">air</span> (STP) to 30bar, into 33L electropolished (SUMMA) stainless steel canisters. Select archived <span class="hlt">air</span> samples from the original network are maintained at Portland State University (PSU) Department of Physics. These archived samples are a valuable look at changing atmospheric concentrations of <span class="hlt">CO</span><span class="hlt">2</span> and δ13C, which can contribute to a better understanding of changes in sources during this time. <span class="hlt">CO</span><span class="hlt">2</span> concentrations and δ13C of <span class="hlt">CO</span><span class="hlt">2</span> were measured at PSU, with a Picarro Cavity Ringdown Spectrometer, model G1101-i analytical system. This study presents the analytical methods used, calibration techniques, precision, and reproducibility. Measurements of select samples from the archive show rising <span class="hlt">CO</span><span class="hlt">2</span> concentrations and falling δ13C over the 1977 to 1998 period, compatible with previous observations and rising anthropogenic sources of <span class="hlt">CO</span><span class="hlt">2</span>. The resulting data set was statistically analyzed in MATLAB. Results of preliminary seasonal and secular trends from the archive samples are presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013CorRe..32..937B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013CorRe..32..937B"><span>Direct and indirect effects of high p<span class="hlt">CO</span><span class="hlt">2</span> on algal grazing by coral reef herbivores from the Gulf of Aqaba (Red <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>Borell, E. M.; Steinke, M.; Fine, M.</p> <p>2013-12-01</p> <p>Grazing on marine macroalgae is a key structuring process for coral reef communities. However, ocean acidification from rising atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentrations is predicted to adversely affect many marine animals, while seaweed communities may benefit and prosper. We tested how exposure to different p<span class="hlt">CO</span><span class="hlt">2</span> (400, 1,800 and 4,000 μatm) may affect grazing on the green alga Ulva lactuca by herbivorous fish and <span class="hlt">sea</span> urchins from the coral reefs in the northern Gulf of Aqaba (Red <span class="hlt">Sea</span>), either directly, by changing herbivore behaviour, or indirectly via changes in algal palatability. We also determined the effects of p<span class="hlt">CO</span><span class="hlt">2</span> on algal tissue concentrations of protein and the grazing-deterrent secondary metabolite dimethylsulfoniopropionate (DMSP). Grazing preferences and overall consumption were tested in a series of multiple-choice feeding experiments in the laboratory and in situ following exposure for 14 d (algae) and 28 d (herbivores). 4,000 μatm had a significant effect on the biochemical composition and palatability of U. lactuca. No effects were observed at 1,800 relative to 400 μatm (control). Exposure of U. lactuca to 4,000 μatm resulted in a significant decrease in protein and increase in DMSP concentration. This coincided with a reduced preference for these algae by the <span class="hlt">sea</span> urchin Tripneustes gratilla and different herbivorous fish species in situ (Acanthuridae, Siganidae and Pomacanthidae). No feeding preferences were observed for the rabbitfish Siganus rivulatus under laboratory conditions. Exposure to elevated p<span class="hlt">CO</span><span class="hlt">2</span> had no direct effect on the overall algal consumption by T. gratilla and S. rivulatus. Our results show that <span class="hlt">CO</span><span class="hlt">2</span> has the potential to alter algal palatability to different herbivores which could have important implications for algal abundance and coral community structure. The fact that p<span class="hlt">CO</span><span class="hlt">2</span> effects were observed only at a p<span class="hlt">CO</span><span class="hlt">2</span> of 4,000 μatm, however, indicates that algal-grazer interactions may be resistant to predicted p<span class="hlt">CO</span><span class="hlt">2</span> concentrations in the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012BGD.....917939L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012BGD.....917939L"><span>Effects of increased p<span class="hlt">CO</span><span class="hlt">2</span> and geographic origin on purple <span class="hlt">sea</span> urchin (Strongylocentrotus purpuratus) calcite elemental composition</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>LaVigne, M.; Hill, T. M.; Sanford, E.; Gaylord, B.; Russell, A. D.; Lenz, E. A.; Hosfelt, J. D.; Young, M. K.</p> <p>2012-12-01</p> <p>Ocean acidification will likely have negative impacts on invertebrates producing skeletons composed of calcium carbonate. Skeletal solubility is partly controlled by the incorporation of "foreign" ions (such as Mg and Sr) into the crystal lattice of these skeletal structures, a process that is sensitive to a variety of biological and environmental factors. Here we explore the effects of life stage, oceanographic region of origin, and changes in the partial pressure of carbon dioxide in seawater (p<span class="hlt">CO</span><span class="hlt">2</span>) on trace elemental composition in the purple <span class="hlt">sea</span> urchin (Strongylocentrotus purpuratus). We show that, similar to other urchin taxa, adult purple <span class="hlt">sea</span> urchins have the ability to precipitate skeleton composed of a range of biominerals spanning low to high magnesium calcites. Mg/Ca and Sr/Ca ratios were substantially lower in adult spines compared to adult tests. On the other hand, trace elemental composition was invariant among adults collected from four oceanographically distinct regions along the US west coast (Oregon, Northern California, Central California, and Southern California). Skeletons of newly settled juvenile urchins that originated from adults from the four regions exhibited intermediate Mg/Ca and Sr/Ca between adult spine and test endmembers, indicating that skeleton precipitated during early life stages is more soluble than adult spines and less soluble than adult tests. Mean skeletal Mg/Ca or Sr/Ca of juvenile skeleton did not vary with source region when larvae were reared under present-day, global-average seawater carbonate conditions (400 ppm; pH = 8.02 ± 0.03 1 SD; Ωcalcite = 3.3 ± 0.<span class="hlt">2</span> 1 SD). However, when reared under elevated <span class="hlt">CO</span><span class="hlt">2</span> (900 ppm; pH = 7.72 ± 0.03; Ωcalcite = 1.8 ± 0.1), skeletal Sr/Ca in juveniles exhibited increased variance across the four regions. Although larvae from the northern populations (Oregon, Northern California, Central California) did not exhibit differences in Mg or Sr incorporation under elevated <span class="hlt">CO</span><span class="hlt">2</span> (Sr/Ca = <span class="hlt">2</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA503215','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA503215"><span>Transition Delay in a Hypervelocity Boundary Layer using Nonequilibrium <span class="hlt">CO</span><span class="hlt">2</span> Injection</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2008-10-28</p> <p>flows than for either <span class="hlt">air</span> or N<span class="hlt">2</span> flows. The explanation for this phenomenon lies in the fact that when <span class="hlt">CO</span><span class="hlt">2</span> is in vibrational and chemical ... chemical non-equilibrium, these relax- ation processes absorb energy from acoustic disturbances whose growth is responsible for transition in high...atmosphere at hypersonic speeds, they must somehow provide for, avoid, or otherwise accommodate the enormous heat-<span class="hlt">transfer</span> rates to the vehicle engen</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1810686G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1810686G"><span>Emissions of <span class="hlt">CO</span><span class="hlt">2</span> and criteria <span class="hlt">air</span> pollutants from mobile sources: Insights from integrating real-time traffic data into local <span class="hlt">air</span> quality models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gately, Conor; Hutyra, Lucy</p> <p>2016-04-01</p> <p>In 2013, on-road mobile sources were responsible for over 26% of U.S. fossil fuel carbon dioxide (ff<span class="hlt">CO</span><span class="hlt">2</span>) emissions, and over 34% of both <span class="hlt">CO</span> and NOx emissions. However, accurate representations of these emissions at the scale of urban areas remains a difficult challenge. Quantifying emissions at the scale of local streets and highways is critical to provide policymakers with the information needed to develop appropriate mitigation strategies and to guide research into the underlying process that drive mobile emissions. Quantification of vehicle ff<span class="hlt">CO</span><span class="hlt">2</span> emissions at high spatial and temporal resolutions requires a detailed synthesis of data on traffic activity, roadway attributes, fleet characteristics and vehicle speeds. To accurately characterize criteria <span class="hlt">air</span> pollutant emissions, information on local meteorology is also critical, as the temperature and relative humidity can affect emissions rates of these pollutants by as much as 400%. As the health impacts of <span class="hlt">air</span> pollutants are more severe for residents living in close proximity (<500m) to road sources, it is critical that inventories of these emissions rely on highly resolved source data to locate potential hot-spots of exposure. In this study we utilize real-time GPS estimates of vehicle speeds to estimate ff<span class="hlt">CO</span><span class="hlt">2</span> and criteria <span class="hlt">air</span> pollutant emissions at multiple spatial and temporal scales across a large metropolitan area. We observe large variations in emissions associated with diurnal activity patterns, congestion, sporting and civic events, and weather anomalies. We discuss the advantages and challenges of using highly-resolved source data to quantify emissions at a roadway scale, and the potential of this methodology for forecasting the <span class="hlt">air</span> quality impacts of changes in infrastructure, urban planning policies, and regional climate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.A23P..02G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.A23P..02G"><span>Emissions of <span class="hlt">CO</span><span class="hlt">2</span> and criteria <span class="hlt">air</span> pollutants from mobile sources: Insights from integrating real-time traffic data into local <span class="hlt">air</span> quality models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gately, C.; Hutyra, L.; Sue Wing, I.; Peterson, S.; Janetos, A.</p> <p>2015-12-01</p> <p>In 2013, on-road mobile sources were responsible for over 26% of U.S. fossil fuel carbon dioxide (ff<span class="hlt">CO</span><span class="hlt">2</span>) emissions, and over 34% of both <span class="hlt">CO</span> and NOx emissions. However, accurate representations of these emissions at the scale of urban areas remains a difficult challenge. Quantifying emissions at the scale of local streets and highways is critical to provide policymakers with the information needed to develop appropriate mitigation strategies and to guide research into the underlying process that drive mobile emissions. Quantification of vehicle ff<span class="hlt">CO</span><span class="hlt">2</span> emissions at high spatial and temporal resolutions requires a detailed synthesis of data on traffic activity, roadway attributes, fleet characteristics and vehicle speeds. To accurately characterize criteria <span class="hlt">air</span> pollutant emissions, information on local meteorology is also critical, as the temperature and relative humidity can affect emissions rates of these pollutants by as much as 400%. As the health impacts of <span class="hlt">air</span> pollutants are more severe for residents living in close proximity (<500m) to road sources, it is critical that inventories of these emissions rely on highly resolved source data to locate potential hot-spots of exposure. In this study we utilize real-time GPS estimates of vehicle speeds to estimate ff<span class="hlt">CO</span><span class="hlt">2</span> and criteria <span class="hlt">air</span> pollutant emissions at multiple spatial and temporal scales across a large metropolitan area. We observe large variations in emissions associated with diurnal activity patterns, congestion, sporting and civic events, and weather anomalies. We discuss the advantages and challenges of using highly-resolved source data to quantify emissions at a roadway scale, and the potential of this methodology for forecasting the <span class="hlt">air</span> quality impacts of changes in infrastructure, urban planning policies, and regional climate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017BGeo...14.3831C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017BGeo...14.3831C"><span>Alterations in microbial community composition with increasing f<span class="hlt">CO</span><span class="hlt">2</span>: a mesocosm study in the eastern 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>Crawfurd, Katharine J.; Alvarez-Fernandez, Santiago; Mojica, Kristina D. A.; Riebesell, Ulf; Brussaard, Corina P. D.</p> <p>2017-08-01</p> <p>Ocean acidification resulting from the uptake of anthropogenic carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) by the ocean is considered a major threat to marine ecosystems. Here we examined the effects of ocean acidification on microbial community dynamics in the eastern Baltic <span class="hlt">Sea</span> during the summer of 2012 when inorganic nitrogen and phosphorus were strongly depleted. Large-volume in situ mesocosms were employed to mimic present, future and far future <span class="hlt">CO</span><span class="hlt">2</span> scenarios. All six groups of phytoplankton enumerated by flow cytometry ( < 20 µm cell diameter) showed distinct trends in net growth and abundance with <span class="hlt">CO</span><span class="hlt">2</span> enrichment. The picoeukaryotic phytoplankton groups Pico-I and Pico-II displayed enhanced abundances, whilst Pico-III, Synechococcus and the nanoeukaryotic phytoplankton groups were negatively affected by elevated fugacity of <span class="hlt">CO</span><span class="hlt">2</span> (f<span class="hlt">CO</span><span class="hlt">2</span>). Specifically, the numerically dominant eukaryote, Pico-I, demonstrated increases in gross growth rate with increasing f<span class="hlt">CO</span><span class="hlt">2</span> sufficient to double its abundance. The dynamics of the prokaryote community closely followed trends in total algal biomass despite differential effects of f<span class="hlt">CO</span><span class="hlt">2</span> on algal groups. Similarly, viral abundances corresponded to prokaryotic host population dynamics. Viral lysis and grazing were both important in controlling microbial abundances. Overall our results point to a shift, with increasing f<span class="hlt">CO</span><span class="hlt">2</span>, towards a more regenerative system with production dominated by small picoeukaryotic phytoplankton.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JPhCS.655a2035D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JPhCS.655a2035D"><span>Modelling heat and mass <span class="hlt">transfer</span> in a membrane-based <span class="hlt">air-to-air</span> enthalpy exchanger</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dugaria, S.; Moro, L.; Del, D., Col</p> <p>2015-11-01</p> <p>The diffusion of total energy recovery systems could lead to a significant reduction in the energy demand for building <span class="hlt">air</span>-conditioning. With these devices, sensible heat and humidity can be recovered in winter from the exhaust airstream, while, in summer, the incoming <span class="hlt">air</span> stream can be cooled and dehumidified by <span class="hlt">transferring</span> the excess heat and moisture to the exhaust <span class="hlt">air</span> stream. Membrane based enthalpy exchangers are composed by different channels separated by semi-permeable membranes. The membrane allows moisture <span class="hlt">transfer</span> under vapour pressure difference, or water concentration difference, between the two sides and, at the same time, it is ideally impermeable to <span class="hlt">air</span> and other contaminants present in exhaust <span class="hlt">air</span>. Heat <span class="hlt">transfer</span> between the airstreams occurs through the membrane due to the temperature gradient. The aim of this work is to develop a detailed model of the coupled heat and mass <span class="hlt">transfer</span> mechanisms through the membrane between the two airstreams. After a review of the most relevant models published in the scientific literature, the governing equations are presented and some simplifying assumptions are analysed and discussed. As a result, a steady-state, two-dimensional finite difference numerical model is setup. The developed model is able to predict temperature and humidity evolution inside the channels. Sensible and latent heat <span class="hlt">transfer</span> rate, as well as moisture <span class="hlt">transfer</span> rate, are determined. A sensitive analysis is conducted in order to determine the more influential parameters on the thermal and vapour <span class="hlt">transfer</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ApSS..439..876M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ApSS..439..876M"><span>Two-step growth mechanism of supported <span class="hlt">Co</span>3O4-based <span class="hlt">sea</span>-urchin like hierarchical nanostructures</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Maurizio, Chiara; Edla, Raju; Michieli, Niccolo'; Orlandi, Michele; Trapananti, Angela; Mattei, Giovanni; Miotello, Antonio</p> <p>2018-05-01</p> <p>Supported 3D hierarchical nanostructures of transition metal oxides exhibit enhanced photocatalytic performances and long-term stability under working conditions. The growth mechanisms crucially determine their intimate structure, that is a key element to optimize their properties. We report on the formation mechanism of supported <span class="hlt">Co</span>3O4 hierarchical <span class="hlt">sea</span> urchin-like nanostructured catalyst, starting from <span class="hlt">Co</span>-O-B layers deposited by Pulsed Laser Deposition (PLD). The particles deposited on the layer surface, that constitute the seeds for the urchin formation, have been investigated after separation from the underneath deposited layer, by X-ray diffraction, X-ray absorption spectroscopy and scanning electron microscopy. The comparison with PLD deposited layers without O and/or B indicates a crucial role of B for the urchin formation that (i) limits <span class="hlt">Co</span> oxidation during the deposition process and (ii) induces a chemical reduction of <span class="hlt">Co</span>, especially in the particle core, in the first step of <span class="hlt">air</span> annealing (<span class="hlt">2</span> h, 500 °C). After <span class="hlt">2</span> h heating <span class="hlt">Co</span> oxidation proceeds and <span class="hlt">Co</span> atoms outdiffuse from the <span class="hlt">Co</span> fcc particle core likely through fast diffusion channel present in the shell and form <span class="hlt">Co</span>3O4 nano-needles. The growth of nano-needles from the layer beneath the particles is prevented by a faster <span class="hlt">Co</span> oxidation and a minimum fraction of metallic <span class="hlt">Co</span>. This investigation shows how diffusion mechanisms and chemical effects can be effectively coupled to obtain hierarchical structures of transition metal oxides.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29441620','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29441620"><span>Heterogeneous Single-Atom Catalyst for Visible-Light-Driven High-Turnover <span class="hlt">CO</span><span class="hlt">2</span> Reduction: The Role of Electron <span class="hlt">Transfer</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gao, Chao; Chen, Shuangming; Wang, Ying; Wang, Jiawen; Zheng, Xusheng; Zhu, Junfa; Song, Li; Zhang, Wenkai; Xiong, Yujie</p> <p>2018-03-01</p> <p>Visible-light-driven conversion of <span class="hlt">CO</span> <span class="hlt">2</span> into chemical fuels is an intriguing approach to address the energy and environmental challenges. In principle, light harvesting and catalytic reactions can be both optimized by combining the merits of homogeneous and heterogeneous photocatalysts; however, the efficiency of charge <span class="hlt">transfer</span> between light absorbers and catalytic sites is often too low to limit the overall photocatalytic performance. In this communication, it is reported that the single-atom <span class="hlt">Co</span> sites coordinated on the partially oxidized graphene nanosheets can serve as a highly active and durable heterogeneous catalyst for <span class="hlt">CO</span> <span class="hlt">2</span> conversion, wherein the graphene bridges homogeneous light absorbers with single-atom catalytic sites for the efficient <span class="hlt">transfer</span> of photoexcited electrons. As a result, the turnover number for <span class="hlt">CO</span> production reaches a high value of 678 with an unprecedented turnover frequency of 3.77 min -1 , superior to those obtained with the state-of-the-art heterogeneous photocatalysts. This work provides fresh insights into the design of catalytic sites toward photocatalytic <span class="hlt">CO</span> <span class="hlt">2</span> conversion from the angle of single-atom catalysis and highlights the role of charge kinetics in bridging the gap between heterogeneous and homogeneous photocatalysts. © 2018 WILEY-VCH Verlag GmbH & <span class="hlt">Co</span>. KGaA, Weinheim.</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 Exchanges. 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://www.ncbi.nlm.nih.gov/pubmed/12557686','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/12557686"><span>[Responses of agricultural crops of 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="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kimball, B A; Zhu, Jianguo; Cheng, Lei; Kobayashi, K; Bindi, M</p> <p>2002-10-01</p> <p>Over the past decade, free-<span class="hlt">air</span> <span class="hlt">CO</span><span class="hlt">2</span> enrichment (FACE) experiments have been conducted on several agricultural crops: wheat(Triticum aestivum L.), perennial ryegrass (Lolium perenne), and rice(Oryza sativa L.) which are C3 grasses; sorghum (Sorghum bicolor (L.) Möench), a C4 grass; white clover (Trifolium repens), a C3 legume; potato (Solanum tuberosum L.), a C3 forb with tuber storage; and cotton (Gossypium hirsutum L.) and grape (Vitis vinifera L.) which are C3 woody perennials. Using reports from these experiments, the relative responses of these crops was discussed with regard to photosynthesis, stomatal conductance, canopy temperature, water use, water potential, leaf area index, shoot and root biomass accumulation, agricultural yield, radiation use efficiency, specific leaf area, tissue nitrogen concentration, nitrogen yield, carbohydrate concentration, phenology, soil microbiology, soil respiration, trace gas emissions, and soil carbon sequestration. Generally, the magnitude of these responses varied with the functional type of plant and with the soil nitrogen and water status. As expected, the elevated <span class="hlt">CO</span><span class="hlt">2</span> increased photosynthesis and biomass production and yield substantially in C3 species, but little in C4, and it decreased stomatal conductance and transpiration in both C3 and C4 species and greatly improved water-use efficiency in all the crops. Growth stimulations were as large or larger under water-stress compared to well-watered conditions. Growth stimulations of non-legumes were reduced at low soil nitrogen, whereas elevated <span class="hlt">CO</span><span class="hlt">2</span> strongly stimulated the growth of the clover legume both at ample and under low N conditions. Roots were generally stimulated more than shoots. Woody perennials had larger growth responses to elevated <span class="hlt">CO</span><span class="hlt">2</span>, while at the same time, their reductions in stomatal conductance were smaller. Tissue nitrogen concentrations went down while carbohydrate and some other carbon-based compounds went up due to elevated <span class="hlt">CO</span><span class="hlt">2</span>, with leaves and</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_22 --> <div id="page_23" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="441"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018CSR...152...14Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018CSR...152...14Z"><span><span class="hlt">Air-sea</span> heat flux control on the Yellow <span class="hlt">Sea</span> Cold Water Mass intensity and implications for its prediction</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhu, Junying; Shi, Jie; Guo, Xinyu; Gao, Huiwang; Yao, Xiaohong</p> <p>2018-01-01</p> <p>The Yellow <span class="hlt">Sea</span> Cold Water Mass (YSCWM), which occurs during summer in the central Yellow <span class="hlt">Sea</span>, plays an important role in the hydrodynamic field, nutrient cycle and biological species. Based on water temperature observations during the summer from 1978 to 1998 in the western Yellow <span class="hlt">Sea</span>, five specific YSCWM years were identified, including two strong years (1984 and 1985), two weak years (1989 and 1995) and one normal year (1992). Using a three-dimensional hydrodynamic model, the YSCWM formation processes in these five years were simulated and compared with observations. In general, the YSCWM began forming in spring, matured in summer and gradually disappeared in autumn of every year. The 8 °C isotherm was used to indicate the YSCWM boundary. The modelled YSCWM areas in the two strong years were approximately two times larger than those in the two weak years. Based on the simulations in the weak year of 1995, ten numerical experiments were performed to quantify the key factors influencing the YSCWM intensity by changing the initial water condition in the previous autumn, <span class="hlt">air-sea</span> heat flux, wind, evaporation, precipitation and <span class="hlt">sea</span> level pressure to those in the strong year of 1984, respectively. The results showed that the <span class="hlt">air-sea</span> heat flux was the dominant factor influencing the YSCWM intensity, which contributed about 80% of the differences of the YSCWM average water temperature at a depth of 50 m. In addition, the <span class="hlt">air-sea</span> heat flux in the previous winter had a determining effect, contributing more than 50% of the differences between the strong and weak YSCWM years. Finally, a simple formula for predicting the YSCWM intensity was established by using the key influencing factors, i.e., the <span class="hlt">sea</span> surface temperature before the cooling season and the <span class="hlt">air-sea</span> heat flux during the cooling season from the previous December to the current February. With this formula, instead of a complicated numerical model, we were able to roughly predict the YSCWM intensity for the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1411443-mo-co-doped-carbon-zn-co-vital-roles-inactive-zn-highly-efficient-activity-toward-oxygen-reduction-evolution-reactions-rechargeable-zn-air-battery','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1411443-mo-co-doped-carbon-zn-co-vital-roles-inactive-zn-highly-efficient-activity-toward-oxygen-reduction-evolution-reactions-rechargeable-zn-air-battery"><span>MO-<span class="hlt">Co</span>@N-Doped Carbon (M = Zn or <span class="hlt">Co</span>): Vital Roles of Inactive Zn and Highly Efficient Activity toward Oxygen Reduction/Evolution Reactions for Rechargeable Zn-<span class="hlt">Air</span> Battery</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>Chen, Biaohua; He, Xiaobo; Yin, Fengxiang</p> <p></p> <p>A highly efficient bifunctional oxygen catalyst is required for practical applications of fuel cells and metal-<span class="hlt">air</span> batteries, as oxygen reduction reaction (ORR) and oxygen evolution reaction (OER) are their core electrode reactions. Here, the MO-<span class="hlt">Co</span>@ N-doped carbon (NC, M = Zn or <span class="hlt">Co</span>) is developed as a highly active ORR/OER bifunctional catalyst via pyrolysis of a bimetal metal-organic framework containing Zn and <span class="hlt">Co</span>, i.e., precursor (<span class="hlt">Co</span>Zn). The vital roles of inactive Zn in developing highly active bifunctional oxygen catalysts are unraveled. When the precursors include Zn, the surface contents of pyridinic N for ORR and the surface contents of <span class="hlt">Co</span>-N-xmore » and <span class="hlt">Co</span>3+/<span class="hlt">Co</span><span class="hlt">2</span>+ ratios for OER are enhanced, while the high specific surface areas, high porosity, and high electrochemical active surface areas are also achieved. Furthermore, the synergistic effects between Zn-based and <span class="hlt">Co</span>-based species can promote the well growth of multiwalled carbon nanotubes (MWCNTs) at high pyrolysis temperatures (>= 700 degrees C), which is favorable for charge <span class="hlt">transfer</span>. The optimized <span class="hlt">Co</span>Zn-NC-700 shows the highly bifunctional ORR/OER activity and the excellent durability during the ORR/OER processes, even better than 20 wt% Pt/C (for ORR) and IrO<span class="hlt">2</span> (for OER). <span class="hlt">Co</span>Zn-NC-700 also exhibits the prominent Zn-<span class="hlt">air</span> battery performance and even outperforms the mixture of 20 wt% Pt/C and IrO<span class="hlt">2</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.A54A..05M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.A54A..05M"><span>Gulf of Mexico <span class="hlt">Air/Sea</span> Interaction: Measurements and Initial Data Characterization</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>MacDonald, C.; Huang, C. H.; Roberts, P. T.; Bariteau, L.; Fairall, C. W.; Gibson, W.; Ray, A.</p> <p>2011-12-01</p> <p>Corporate, government, and university researchers collaborated to develop an atmospheric boundary layer environmental observations program on an offshore platform in the Gulf of Mexico. The primary goals of this project were to provide data to (1) improve our understanding of boundary layer processes and <span class="hlt">air-sea</span> interaction over the Gulf of Mexico; (<span class="hlt">2</span>) improve regional-scale meteorological and <span class="hlt">air</span> quality modeling; and (3) provide a framework for advanced offshore measurements to support future needs such as emergency response, exploration and lease decisions, wind energy research and development, and meteorological and <span class="hlt">air</span> quality forecasting. In October 2010, meteorological and oceanographic sensors were deployed for an extended period (approximately 12 months) on a Chevron service platform (ST 52B, 90.5W, 29N) to collect boundary layer and <span class="hlt">sea</span> surface data sufficient to support these objectives. This project has significant importance given the large industrial presence in the Gulf, sizeable regional population nearby, and the recognized need for precise and timely pollutant forecasts. Observations from this project include surface meteorology; sodar marine boundary layer winds; microwave radiometer profiles of temperature, relative humidity, and liquid water; ceilometer cloud base heights; water temperature and current profiles; <span class="hlt">sea</span> surface temperature; wave height statistics; downwelling solar and infrared radiation; and <span class="hlt">air-sea</span> turbulent momentum and heat fluxes. This project resulted in the collection of an unprecedented set of boundary layer measurements over the Gulf of Mexico that capture the range of meteorological and oceanographic interactions and processes that occur over an entire year. This presentation will provide insight into the logistical and scientific issues associated with the deployment and operations of unique measurements in offshore areas and provide results from an initial data analysis of boundary layer processes over the Gulf of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JVGR..320...50I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JVGR..320...50I"><span>Geochemical characterisation of gases along the dead <span class="hlt">sea</span> rift: Evidences of mantle-<span class="hlt">co</span><span class="hlt">2</span> degassing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Inguaggiato, C.; Censi, P.; D'Alessandro, W.; Zuddas, P.</p> <p>2016-06-01</p> <p>The Dead <span class="hlt">Sea</span> Transform (DST) fault system, where a lateral displacement between the African and Arabian plates occurs, is characterised by anomalous heat flux in the Israeli area close to the border with Syria and Jordan. The concentration of He and <span class="hlt">CO</span><span class="hlt">2</span>, and isotopic composition of He and total dissolved inorganic carbon were studied in cold and thermal waters collected along the DST, in order to investigate the source of volatiles and their relationship with the tectonic framework of the DST. The waters with higher temperature (up to 57.<span class="hlt">2</span> °C) are characterised by higher amounts of <span class="hlt">CO</span><span class="hlt">2</span> and helium (up to 55.72 and 1.91 ∗ 10- <span class="hlt">2</span> cc l- 1, respectively). Helium isotopic data (R/Ra from 0.11 to <span class="hlt">2</span>.14) and 4He/20Ne ratios (0.41-106.86) show the presence of deep-deriving fluids consisting of a variable mixture of mantle and crust end-members, with the former reaching up to 35%. Carbon isotope signature of total dissolved carbon from hot waters falls within the range of magmatic values, suggesting the delivery of deep-seated <span class="hlt">CO</span><span class="hlt">2</span>. The geographical distribution of helium isotopic data and isotopic carbon (<span class="hlt">CO</span><span class="hlt">2</span>) values coupled with (<span class="hlt">CO</span><span class="hlt">2</span>/3He ratios) indicate a larger contribution of mantle-derived fluids affecting the northern part of the investigated area, where the waters reach the highest temperature. These evidences suggest the occurrence of a favourable tectonic framework, including a Moho discontinuity up-rise and/or the presence of a deep fault system coupled with the recent magmatic activity recognised in the northern part of Israel.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('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><span class="hlt">Air-sea</span> interaction dramatically changes from moderate to very high wind speed conditions (Donelan et al. 2004). Unresolved physics of the <span class="hlt">air-sea</span> interface are one of the weakest components in tropical cyclone prediction models. Rapid disruption of the <span class="hlt">air</span>-water interface under very high wind speed conditions was reported in laboratory experiments (Koga 1981) and numerical simulations (Soloviev et al. 2012), which resembled the Kelvin-Helmholtz instability at an interface with very large density difference. Kelly (1965) demonstrated that the KH instability at the <span class="hlt">air-sea</span> interface can develop through parametric amplification of waves. Farrell and Ioannou (2008) showed that gustiness results in the parametric KH instability of the <span class="hlt">air-sea</span> interface, while the gusts are due to interacting waves and turbulence. The stochastic forcing enters multiplicatively in this theory and produces an exponential wave growth, augmenting the growth from the Miles (1959) theory as the turbulence level increases. Here we complement this concept by adding the effect of the two-phase environment near the mean interface, which introduces additional viscosity in the system (turning it into a rheological system). The two-phase environment includes <span class="hlt">air</span>-bubbles and re-entering spray (spume), which eliminates a portion of the wind-wave wavenumber spectrum that is responsible for a substantial part of the <span class="hlt">air</span> <span class="hlt">sea</span> drag coefficient. The previously developed KH-type interfacial parameterization (Soloviev and Lukas 2010) is unified with two versions of the wave growth model. The unified parameterization in both cases exhibits the increase of the drag coefficient with wind speed until approximately 30 m/s. Above this wind speed threshold, the drag coefficient either nearly levels off or even slightly drops (for the wave growth model that accounts for the shear) and then starts again increasing above approximately 65 m/s wind speed. Remarkably, the unified parameterization reveals a local minimum</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006TellB..58...73W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006TellB..58...73W"><span>The role of Southern Ocean mixing and upwelling in glacial-interglacial atmospheric <span class="hlt">CO</span><span class="hlt">2</span> change</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Watson, Andrew J.; Naveira Garabato, Alberto C.</p> <p>2006-02-01</p> <p>Decreased ventilation of the Southern Ocean in glacial time is implicated in most explanations of lower glacial atmospheric <span class="hlt">CO</span><span class="hlt">2</span>. Today, the deep (>2000 m) ocean south of the Polar Front is rapidly ventilated from below, with the interaction of deep currents with topography driving high mixing rates well up into the water column. We show from a buoyancy budget that mixing rates are high in all the deep waters of the Southern Ocean. Between the surface and ~2000 m depth, water is upwelled by a residual meridional overturning that is directly linked to buoyancy fluxes through the ocean surface. Combined with the rapid deep mixing, this upwelling serves to return deep water to the surface on a short time scale. We propose two new mechanisms by which, in glacial time, the deep Southern Ocean may have been more isolated from the surface. Firstly, the deep ocean appears to have been more stratified because of denser bottom water resulting from intense <span class="hlt">sea</span> ice formation near Antarctica. The greater stratification would have slowed the deep mixing. Secondly, subzero atmospheric temperatures may have meant that the present-day buoyancy flux from the atmosphere to the ocean surface was reduced or reversed. This in turn would have reduced or eliminated the upwelling (contrary to a common assumption, upwelling is not solely a function of the wind stress but is coupled to the <span class="hlt">air-sea</span> buoyancy flux too). The observed very close link between Antarctic temperatures and atmospheric <span class="hlt">CO</span><span class="hlt">2</span> could then be explained as a natural consequence of the connection between the <span class="hlt">air-sea</span> buoyancy flux and upwelling in the Southern Ocean, if slower ventilation of the Southern Ocean led to lower atmospheric <span class="hlt">CO</span><span class="hlt">2</span>. Here we use a box model, similar to those of previous authors, to show that weaker mixing and reduced upwelling in the Southern Ocean can explain the low glacial atmospheric <span class="hlt">CO</span><span class="hlt">2</span> in such a formulation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.6603V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.6603V"><span>Detection of <span class="hlt">CO</span><span class="hlt">2</span> leaks from carbon capture and storage sites to the atmosphere with combined <span class="hlt">CO</span><span class="hlt">2</span> and O<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>van Leeuwen, Charlotte; Meijer, Harro A. J.</p> <p>2015-04-01</p> <p>One of the main issues in carbon capture and storage (CCS) is the possibility of leakage of <span class="hlt">CO</span><span class="hlt">2</span> from the storage reservoir to the atmosphere, both from a public health and a climate change combat perspective. Detecting these leaks in the atmosphere is difficult due to the rapid mixing of the emitted <span class="hlt">CO</span><span class="hlt">2</span> with the surrounding <span class="hlt">air</span> masses and the high natural variability of the atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentration. Instead of measuring only the <span class="hlt">CO</span><span class="hlt">2</span> concentration of the atmosphere, its isotopes or chemical tracers that are released together with the <span class="hlt">CO</span><span class="hlt">2</span>, our method uses O<span class="hlt">2</span> measurements in addition to <span class="hlt">CO</span><span class="hlt">2</span> measurements to detect a leak from a CCS site. <span class="hlt">CO</span><span class="hlt">2</span> and O<span class="hlt">2</span> are coupled in most processes on earth. In photosynthesis, plants take up <span class="hlt">CO</span><span class="hlt">2</span> and release O<span class="hlt">2</span> at the same time. In respiration and fossil fuel burning, O<span class="hlt">2</span> is consumed while <span class="hlt">CO</span><span class="hlt">2</span> is released. In case of a leak from a CCS site, however, there is no relationship between <span class="hlt">CO</span><span class="hlt">2</span> and O<span class="hlt">2</span>. A <span class="hlt">CO</span><span class="hlt">2</span> leak can therefore be distinguished from other sources of <span class="hlt">CO</span><span class="hlt">2</span> by looking at the atmospheric <span class="hlt">CO</span><span class="hlt">2</span>-O<span class="hlt">2</span> ratio. A natural increase of the <span class="hlt">CO</span><span class="hlt">2</span> concentration is accompanied by a drop in the O<span class="hlt">2</span> concentration, while an increase in the <span class="hlt">CO</span><span class="hlt">2</span> concentration caused by a leak from a CCS site does not have any effect on the O<span class="hlt">2</span> concentration. To demonstrate this leak detection strategy we designed and built a transportable <span class="hlt">CO</span><span class="hlt">2</span> and O<span class="hlt">2</span> measurement system, that is capable of measuring the relatively minute (ppm's variations on a 21% concentration) changes in the O<span class="hlt">2</span> concentration. The system comprises of three cases that contain the instrumentation and gas handling equipment, the gas cylinders used as reference and calibration gases and a drying system, respectively. <span class="hlt">Air</span> is pumped to the system from an <span class="hlt">air</span> inlet that is placed in a small tower in the field. At the conference, we will demonstrate the success of leak detection with our system by showing measurements of several <span class="hlt">CO</span><span class="hlt">2</span> release experiments, where <span class="hlt">CO</span><span class="hlt">2</span> was released at a small distance from the <span class="hlt">air</span> inlet of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A43G2559J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A43G2559J"><span>Seasonal atmospheric deposition and <span class="hlt">air-sea</span> gaseous exchange of polycyclic aromatic hydrocarbons over the Yangtze River Estuary, East China <span class="hlt">Sea</span>: Implication for the source-sink processes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jiang, Y.; Guo, Z.</p> <p>2017-12-01</p> <p>As the home of the largest port in the world, the Yangtze River Estuary (YRE) in the East China <span class="hlt">Sea</span> (ECS) is adjacent to the largest economic zone in China with more than 10% of Chinese population and provides one-fifth of national GDP. The YRE is under the path of contaminated East Asian continental outflow. These make the YRE unique for the pollutant biogeochemical cycling in the world. In this work, 94 pairs of <span class="hlt">air</span> samples and 20 surface seawater samples covering four seasons were collected from a remote receptor site in the YRE from March 2014 to January 2015, in order to explore the seasonal fluxes of <span class="hlt">air-sea</span> gaseous exchange and atmospheric dry and wet deposition of 15 polycyclic aromatic hydrocarbons (PAHs) and their source-sink processes at the <span class="hlt">air-sea</span> interface. The average dry and wet deposition 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 exchange of PAHs was referred as the dominant process at the <span class="hlt">air-sea</span> interface in the YRE as the magnitude of volatilization flux of PAHs exceeded that of the total dry and wet deposition. The gaseous PAH exchange 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('https://www.osti.gov/biblio/22483295-children-exposure-indoor-air-urban-nurseries-part-co-sub-comfort-assessment','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22483295-children-exposure-indoor-air-urban-nurseries-part-co-sub-comfort-assessment"><span>Children's exposure to indoor <span class="hlt">air</span> in urban nurseries-part I: <span class="hlt">CO</span>{sub <span class="hlt">2</span>} and comfort assessment</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>Branco, P.T.B.S.; Alvim-Ferraz, M.C.M.; Martins, F.G.</p> <p>2015-07-15</p> <p>Indoor <span class="hlt">air</span> quality (IAQ) in nurseries is an emerging case-study. Thus, this study, as the Part I of the larger study “Children's exposure to indoor <span class="hlt">air</span> in urban nurseries”, aimed to: i) evaluate nurseries’ indoor concentrations of carbon dioxide (<span class="hlt">CO</span>{sub <span class="hlt">2</span>}), a global IAQ indicator, in class and lunch rooms; ii) assess indoor comfort parameters–temperature (T) and relative humidity (RH); and iii) analyse them according to guidelines and references for IAQ, comfort and children's health. Indoor continuous measurements were performed. Non-compliances with guidelines were found in comfort parameters, which could cause discomfort situations and also microbial proliferation. Exceedances in <span class="hlt">CO</span>{submore » <span class="hlt">2</span>} concentrations were also found and they were caused by poor ventilation and high classroom occupation. More efficient ventilation and control of comfort parameters, as well as to reduce occupation by reviewing Portuguese legislation on that matter, would certainly improve IAQ and comfort in nurseries and consequently safeguard children's health. - Highlights: • High occupation and poor ventilation were main determinants of IAQ in nurseries. • T and RH indoor values found in nurseries are likely to cause thermal discomfort. • Building characteristics and an inadequate ventilation determined T and RH values. • High <span class="hlt">CO</span>{sub <span class="hlt">2</span>} concentrations found could indicate accumulation of other <span class="hlt">air</span> pollutants.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27522173','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27522173"><span>The impact of <span class="hlt">CO</span><span class="hlt">2</span>-driven ocean acidification on early development and calcification in the <span class="hlt">sea</span> urchin Strongylocentrotus intermedius.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhan, Yaoyao; Hu, Wanbin; Zhang, Weijie; Liu, Minbo; Duan, Lizhu; Huang, Xianya; Chang, Yaqing; Li, Cong</p> <p>2016-11-15</p> <p>The impact of <span class="hlt">CO</span> <span class="hlt">2</span> -driven ocean acidification(OA) on early development and calcification in the <span class="hlt">sea</span> urchin Strongylocentrotus intermedius cultured in northern Yellow <span class="hlt">Sea</span> was investigated by comparing fertilization success, early cleavage rate, hatching rate of blastulae, larvae survival rate at 70h post-fertilization, larval morphology and calcification under present natural seawater condition (pH=8.00±0.03) and three laboratory-controlled acidified conditions (OA 1 , △pH=-0.3units; OA <span class="hlt">2</span> , △pH=-0.4units; OA 3 , △pH=-0.5units) projected by IPCC for 2100. Results showed that pH decline had no effect on the overall fertilization, however, with decreased pH, delayed early embryonic cleavage, reduced hatching rate of blastulae and four-armed larvae survival rate at 70h post-fertilization, impaired larval symmetry, shortened larval spicules, and corrosion spicule structure were observed in all OA-treated groups as compared to control, which indicated that <span class="hlt">CO</span> <span class="hlt">2</span> -driven OA affected early development and calcification in S. intermedius negatively. Copyright © 2016 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013NatCC...3..885W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013NatCC...3..885W"><span><span class="hlt">Co</span>-benefits of mitigating global greenhouse gas emissions for future <span class="hlt">air</span> quality and human health</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>West, J. Jason; Smith, Steven J.; Silva, Raquel A.; Naik, Vaishali; Zhang, Yuqiang; Adelman, Zachariah; Fry, Meridith M.; Anenberg, Susan; Horowitz, Larry W.; Lamarque, Jean-Francois</p> <p>2013-10-01</p> <p>Actions to reduce greenhouse gas (GHG) emissions often reduce <span class="hlt">co</span>-emitted <span class="hlt">air</span> pollutants, bringing <span class="hlt">co</span>-benefits for <span class="hlt">air</span> quality and human health. Past studies typically evaluated near-term and local <span class="hlt">co</span>-benefits, neglecting the long-range transport of <span class="hlt">air</span> pollutants, long-term demographic changes, and the influence of climate change on <span class="hlt">air</span> quality. Here we simulate the <span class="hlt">co</span>-benefits of global GHG reductions on <span class="hlt">air</span> quality and human health using a global atmospheric model and consistent future scenarios, via two mechanisms: reducing <span class="hlt">co</span>-emitted <span class="hlt">air</span> pollutants, and slowing climate change and its effect on <span class="hlt">air</span> quality. We use new relationships between chronic mortality and exposure to fine particulate matter and ozone, global modelling methods and new future scenarios. Relative to a reference scenario, global GHG mitigation avoids 0.5+/-0.<span class="hlt">2</span>, 1.3+/-0.5 and <span class="hlt">2.2</span>+/-0.8 million premature deaths in 2030, 2050 and 2100. Global average marginal <span class="hlt">co</span>-benefits of avoided mortality are US$50-380 per tonne of <span class="hlt">CO</span><span class="hlt">2</span>, which exceed previous estimates, exceed marginal abatement costs in 2030 and 2050, and are within the low range of costs in 2100. East Asian <span class="hlt">co</span>-benefits are 10-70 times the marginal cost in 2030. <span class="hlt">Air</span> quality and health <span class="hlt">co</span>-benefits, especially as they are mainly local and near-term, provide strong additional motivation for transitioning to a low-carbon future.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://dx.doi.org/10.1007/s10750-011-0946-3','USGSPUBS'); return false;" href="http://dx.doi.org/10.1007/s10750-011-0946-3"><span>Can elevated <span class="hlt">CO</span><span class="hlt">2</span> modify regeneration from seed banks of floating freshwater marshes subjected to rising <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>Middleton, Beth A.; McKee, Karen L.</p> <p>2012-01-01</p> <p>Higher atmospheric concentrations of <span class="hlt">CO</span><span class="hlt">2</span> can offset the negative effects of flooding or salinity on plant species, but previous studies have focused on mature, rather than regenerating vegetation. This study examined how interacting environments of <span class="hlt">CO</span><span class="hlt">2</span>, water regime, and salinity affect seed germination and seedling biomass of floating freshwater marshes in the Mississippi River Delta, which are dominated by C3 grasses, sedges, and forbs. Germination density and seedling growth of the dominant species depended on multifactor interactions of <span class="hlt">CO</span><span class="hlt">2</span> (385 and 720 μl l-1) with flooding (drained, +8-cm depth, +8-cm depth-gradual) and salinity (0, 6% seawater) levels. Of the three factors tested, salinity was the most important determinant of seedling response patterns. Species richness (total = 19) was insensitive to <span class="hlt">CO</span><span class="hlt">2</span>. Our findings suggest that for freshwater marsh communities, seedling response to <span class="hlt">CO</span><span class="hlt">2</span> is species-specific and secondary to salinity and flooding effects. Elevated <span class="hlt">CO</span><span class="hlt">2</span> did not ameliorate flooding or salinity stress. Consequently, climate-related changes in <span class="hlt">sea</span> level or human-caused alterations in hydrology may override atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentrations in driving shifts in this plant community. The results of this study suggest caution in making extrapolations from species-specific responses to community-level predictions without detailed attention to the nuances of multifactor responses.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20020069012','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20020069012"><span>Coastal Atmosphere and <span class="hlt">Sea</span> Time Series (<span class="hlt">Co</span>ASTS)</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hooker, Stanford B. (Editor); Firestone, Elaine R. (Editor); Zibordi, Giuseppe; Berthon, Jean-Francoise; Doyle, John P.; Grossi, Stefania; vanderLinde, Dirk; Targa, Cristina; Alberotanza, Luigi; McClain, Charles R. (Technical Monitor)</p> <p>2002-01-01</p> <p>The Coastal Atmosphere and <span class="hlt">Sea</span> Time Series (<span class="hlt">Co</span>ASTS) Project aimed at supporting ocean color research and applications, from 1995 up to the time of publication of this document, has ensured the collection of a comprehensive atmospheric and marine data set from an oceanographic tower located in the northern Adriatic <span class="hlt">Sea</span>. The instruments and the measurement methodologies used to gather quantities relevant for bio-optical modeling and for the calibration and validation of ocean color sensors, are described. Particular emphasis is placed on four items: (1) the evaluation of perturbation effects in radiometric data (i.e., tower-shading, instrument self-shading, and bottom effects); (<span class="hlt">2</span>) the intercomparison of seawater absorption coefficients from in situ measurements and from laboratory spectrometric analysis on discrete samples; (3) the intercomparison of two filter techniques for in vivo measurement of particulate absorption coefficients; and (4) the analysis of repeatability and reproducibility of the most relevant laboratory measurements carried out on seawater samples (i.e., particulate and yellow substance absorption coefficients, and pigment and total suspended matter concentrations). Sample data are also presented and discussed to illustrate the typical features characterizing the <span class="hlt">Co</span>ASTS measurement site in view of supporting the suitability of the <span class="hlt">Co</span>ASTS data set for bio-optical modeling and ocean color calibration and validation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1158425','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1158425"><span><span class="hlt">Air</span> Leakage and <span class="hlt">Air</span> <span class="hlt">Transfer</span> Between Garage and Living Space</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>Rudd, A.</p> <p>2014-09-01</p> <p>This research project focused on evaluation of <span class="hlt">air</span> <span class="hlt">transfer</span> between the garage and living space in a single-family detached home constructed by a production homebuilder in compliance with the 2009 International Residential Code and the 2009 International Energy Conservation Code. The project gathered important information about the performance of whole-building ventilation systems and garage ventilation systems as they relate to minimizing flow of contaminated <span class="hlt">air</span> from garage to living space. A series of 25 multi-point fan pressurization tests and additional zone pressure diagnostic testing characterized the garage and house <span class="hlt">air</span> leakage, the garage-to-house <span class="hlt">air</span> leakage, and garage and house pressuremore » relationships to each other and to outdoors using automated fan pressurization and pressure monitoring techniques. While the relative characteristics of this house may not represent the entire population of new construction configurations and <span class="hlt">air</span> tightness levels (house and garage) throughout the country, the technical approach was conservative and should reasonably extend the usefulness of the results to a large spectrum of house configurations from this set of parametric tests in this one house. Based on the results of this testing, the two-step garage-to-house <span class="hlt">air</span> leakage test protocol described above is recommended where whole-house exhaust ventilation is employed. For houses employing whole-house supply ventilation (positive pressure) or balanced ventilation (same pressure effect as the Baseline condition), adherence to the EPA Indoor <span class="hlt">air</span>PLUS house-to-garage <span class="hlt">air</span> sealing requirements should be sufficient to expect little to no garage-to-house <span class="hlt">air</span> <span class="hlt">transfer</span>.« less</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 exchanges over shallow water.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24437566','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24437566"><span>Dicobalt-μ-oxo polyoxometalate compound, [(α(<span class="hlt">2</span>)-P<span class="hlt">2</span>W17O61<span class="hlt">Co</span>)<span class="hlt">2</span>O](14-): a potent species for water oxidation, C-H bond activation, and oxygen <span class="hlt">transfer</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Barats-Damatov, Delina; Shimon, Linda J W; Weiner, Lev; Schreiber, Roy E; Jiménez-Lozano, Pablo; Poblet, Josep M; de Graaf, Coen; Neumann, Ronny</p> <p>2014-02-03</p> <p>High-valent oxo compounds of transition metals are often implicated as active species in oxygenation of hydrocarbons through carbon-hydrogen bond activation or oxygen <span class="hlt">transfer</span> and also in water oxidation. Recently, several examples of cobalt-catalyzed water oxidation have been reported, and cobalt(IV) species have been suggested as active intermediates. A reactive species, formally a dicobalt(IV)-μ-oxo polyoxometalate compound [(α<span class="hlt">2</span>-P<span class="hlt">2</span>W17O61<span class="hlt">Co</span>)<span class="hlt">2</span>O](14-), [(POMCo)<span class="hlt">2</span>O], has now been isolated and characterized by the oxidation of a monomeric [α<span class="hlt">2</span>-P<span class="hlt">2</span>W17O61<span class="hlt">Co</span>(II)(H<span class="hlt">2</span>O)](8-), [POMCo(II)H<span class="hlt">2</span>O], with ozone in water. The crystal structure shows a nearly linear <span class="hlt">Co-O-Co</span> moiety with a <span class="hlt">Co</span>-O bond length of ∼1.77 Å. In aqueous solution [(POMCo)<span class="hlt">2</span>O] was identified by (31)P NMR, Raman, and UV-vis spectroscopy. Reactivity studies showed that [(POMCo)<span class="hlt">2</span>O]<span class="hlt">2</span>O] is an active compound for the oxidation of H<span class="hlt">2</span>O to O<span class="hlt">2</span>, direct oxygen <span class="hlt">transfer</span> to water-soluble sulfoxides and phosphines, indirect epoxidation of alkenes via a Mn porphyrin, and the selective oxidation of alcohols by carbon-hydrogen bond activation. The latter appears to occur via a hydrogen atom <span class="hlt">transfer</span> mechanism. Density functional and CASSCF calculations strongly indicate that the electronic structure of [(POMCo)<span class="hlt">2</span>O]<span class="hlt">2</span>O] is best defined as a compound having two cobalt(III) atoms with two oxidized oxygen atoms.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004GeCoA..68.1749P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004GeCoA..68.1749P"><span>Experimental evidence for carbonate precipitation and <span class="hlt">CO</span> <span class="hlt">2</span> degassing during <span class="hlt">sea</span> ice formation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Papadimitriou, S.; Kennedy, H.; Kattner, G.; Dieckmann, G. S.; Thomas, D. N.</p> <p>2004-04-01</p> <p>Chemical and stable carbon isotopic modifications during the freezing of artificial seawater were measured in four 4 m 3 tank incubations. Three of the four incubations were inoculated with a nonaxenic Antarctic diatom culture. The 18 days of freezing resulted in 25 to 27 cm thick ice sheets overlying the residual seawater. The ice phase was characterized by a decrease in temperature from -1.9 to -<span class="hlt">2.2</span>°C in the under-ice seawater down to -6.7°C in the upper 4 cm of the ice sheet, with a concurrent increase in the salinity of the under-ice seawater and brine inclusions of the ice sheet as a result of physical concentration of major dissolved salts by expulsion from the solid ice matrix. Measurements of pH, total dissolved inorganic carbon (C T) and its stable isotopic composition (δ 13C T) all exhibited changes, which suggest minimal effect by biological activity during the experiment. A systematic drop in pH and salinity-normalized C T by up to 0.37 pH SWS units and 376 μmol C kg -1 respectively at the lowest temperature and highest salinity part of the ice sheet were coupled with an equally systematic 13C enrichment of the C T. Calculations based on the direct pH and C T measurements indicated a steady increase in the in situ concentration of dissolved carbon dioxide (<span class="hlt">CO</span> <span class="hlt">2</span>(aq)) with time and increasing salinity within the ice sheet, partly due to changes in the dissociation constants of carbonic acid in the low temperature-high salinity range within <span class="hlt">sea</span> ice. The combined effects of temperature and salinity on the solubility of <span class="hlt">CO</span> <span class="hlt">2</span> over the range of conditions encountered during this study was a slight net decrease in the equilibrium <span class="hlt">CO</span> <span class="hlt">2</span>(aq) concentration as a result of the salting-out overriding the increase in solubility with decreasing temperature. Hence, the increase in the in situ <span class="hlt">CO</span> <span class="hlt">2</span>(aq) concentration lead to saturation or supersaturation of the brine inclusions in the ice sheet with respect to atmospheric p<span class="hlt">CO</span> <span class="hlt">2</span> (≈3.5 × 10 -4 atm). When all physico</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JSSCh.215..128W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JSSCh.215..128W"><span>Phase equilibria and crystal chemistry of the CaO-1/<span class="hlt">2</span> >Nd<span class="hlt">2</span>O3-<span class="hlt">Co</span>Oz system at 885 °C 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>Wong-Ng, W.; Laws, W.; Talley, K. R.; Huang, Q.; Yan, Y.; Martin, J.; Kaduk, J. A.</p> <p>2014-07-01</p> <p>The phase diagram of the CaO-1/<span class="hlt">2</span> >Nd<span class="hlt">2</span>O3-<span class="hlt">Co</span>Oz system at 885 °C in <span class="hlt">air</span> has been determined. The system consists of two calcium cobaltate compounds that have promising thermoelectric properties, namely, the <span class="hlt">2</span>D thermoelectric oxide solid solution, (Ca3-xNdx)<span class="hlt">Co</span>4O9-z (0≤x≤0.5), which has a misfit layered structure, and Ca3<span class="hlt">Co</span><span class="hlt">2</span>O6 which consists of 1D chains of alternating <span class="hlt">Co</span>O6 trigonal prisms and <span class="hlt">Co</span>O6 octahedra. Ca3<span class="hlt">Co</span><span class="hlt">2</span>O6 was found to be a point compound without the substitution of Nd on the Ca site. The reported Nd<span class="hlt">2</span><span class="hlt">Co</span>O4 phase was not observed at 885 °C. A ternary (Ca1-xNd1+x)<span class="hlt">Co</span>O4-z (x=0) phase, or (CaNd<span class="hlt">Co</span>)O4-z, was found to be stable at this temperature. A solid solution region of distorted perovskite (Nd1-xCax)<span class="hlt">Co</span>O3-z (0≤x≤0.25, space group Pnma) was established. In the peripheral binary systems, while a solid solution region was identified for (Nd1-xCax)<span class="hlt">2</span>O3-z (0≤x≤0.<span class="hlt">2</span>), Nd was not found to substitute in the Ca site of CaO. Six solid solution tie-line regions and six three-phase regions were determined in the CaO-Nd<span class="hlt">2</span>O3-<span class="hlt">Co</span>Oz system in <span class="hlt">air</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3619508','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3619508"><span>Temperature and <span class="hlt">CO</span><span class="hlt">2</span> additively regulate physiology, morphology and genomic responses of larval <span class="hlt">sea</span> urchins, Strongylocentrotus purpuratus</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Padilla-Gamiño, Jacqueline L.; Kelly, Morgan W.; Evans, Tyler G.; Hofmann, Gretchen E.</p> <p>2013-01-01</p> <p>Ocean warming and ocean acidification, both consequences of anthropogenic production of <span class="hlt">CO</span><span class="hlt">2</span>, will combine to influence the physiological performance of many species in the marine environment. In this study, we used an integrative approach to forecast the impact of future ocean conditions on larval purple <span class="hlt">sea</span> urchins (Strongylocentrotus purpuratus) from the northeast Pacific Ocean. In laboratory experiments that simulated ocean warming and ocean acidification, we examined larval development, skeletal growth, metabolism and patterns of gene expression using an orthogonal comparison of two temperature (13°C and 18°C) and p<span class="hlt">CO</span><span class="hlt">2</span> (400 and 1100 μatm) conditions. Simultaneous exposure to increased temperature and p<span class="hlt">CO</span><span class="hlt">2</span> significantly reduced larval metabolism and triggered a widespread downregulation of histone encoding genes. p<span class="hlt">CO</span><span class="hlt">2</span> but not temperature impaired skeletal growth and reduced the expression of a major spicule matrix protein, suggesting that skeletal growth will not be further inhibited by ocean warming. Importantly, shifts in skeletal growth were not associated with developmental delay. Collectively, our results indicate that global change variables will have additive effects that exceed thresholds for optimized physiological performance in this keystone marine species. PMID:23536595</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21905731','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21905731"><span>Atomic alignment effect in the dissociative energy <span class="hlt">transfer</span> reaction of metal carbonyls (Fe(<span class="hlt">CO</span>)5, Ni(<span class="hlt">CO</span>)4) with oriented Ar (3P<span class="hlt">2</span>, M(J) = <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>Ohoyama, H; Matsuura, Y</p> <p>2011-10-13</p> <p>The atomic alignment effect has been studied for the dissociative energy <span class="hlt">transfer</span> reaction of metal carbonyls (Fe(<span class="hlt">CO</span>)(5), Ni(<span class="hlt">CO</span>)(4)) with the oriented Ar ((3)P(<span class="hlt">2</span>), M(J) = <span class="hlt">2</span>). The emission intensity from the excited metal products (Fe*, Ni*) has been measured as a function of the atomic alignment in the collision frame. The selectivity of the atomic orbital alignment of Ar ((3)P(<span class="hlt">2</span>), M(J) = <span class="hlt">2</span>) (rank <span class="hlt">2</span> moment, a(<span class="hlt">2</span>)) is found to be opposite for the two reaction systems; the Fe(<span class="hlt">CO</span>)(5) reaction is favorable at the Π configuration (positive a(<span class="hlt">2</span>)), while the Ni(<span class="hlt">CO</span>)(4) reaction is favorable at the Σ configuration (negative a(<span class="hlt">2</span>)). Moreover, a significant spin alignment effect (rank 4 moment, a(4)) is recognized only in the Ni(<span class="hlt">CO</span>)(4) reaction. The atomic alignment effect turns out to be essentially different between the two reaction systems; the Fe(<span class="hlt">CO</span>)(5) reaction is controlled by the configuration of the half-filled 3p atomic orbital of Ar ((3)P(<span class="hlt">2</span>)) in the collision frame (L dependence), whereas the Ni(<span class="hlt">CO</span>)(4) reaction is controlled by the configuration of the total angular moment J (including spin) of Ar ((3)P(<span class="hlt">2</span>)) in the collision frame (J dependence). As the origin of J dependence observed only in the Ni(<span class="hlt">CO</span>)(4) reaction, the correlation (and/or the interference) between two electron exchange processes via the electron rearrangements is proposed.</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://hdl.handle.net/2060/20120001243','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120001243"><span>Advanced <span class="hlt">CO</span><span class="hlt">2</span> Removal and Reduction System</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Alptekin, Gokhan; Dubovik, Margarita; Copeland, Robert J.</p> <p>2011-01-01</p> <p>An advanced system for removing <span class="hlt">CO</span><span class="hlt">2</span> and H<span class="hlt">2</span>O from cabin <span class="hlt">air</span>, reducing the <span class="hlt">CO</span><span class="hlt">2</span>, and returning the resulting O<span class="hlt">2</span> to the <span class="hlt">air</span> is less massive than is a prior system that includes two assemblies . one for removal and one for reduction. Also, in this system, unlike in the prior system, there is no need to compress and temporarily store <span class="hlt">CO</span><span class="hlt">2</span>. In this present system, removal and reduction take place within a single assembly, wherein removal is effected by use of an alkali sorbent and reduction is effected using a supply of H<span class="hlt">2</span> and Ru catalyst, by means of the Sabatier reaction, which is <span class="hlt">CO</span><span class="hlt">2</span> + 4H<span class="hlt">2</span> CH4 + O<span class="hlt">2</span>. The assembly contains two fixed-bed reactors operating in alternation: At first, <span class="hlt">air</span> is blown through the first bed, which absorbs <span class="hlt">CO</span><span class="hlt">2</span> and H<span class="hlt">2</span>O. Once the first bed is saturated with <span class="hlt">CO</span><span class="hlt">2</span> and H<span class="hlt">2</span>O, the flow of <span class="hlt">air</span> is diverted through the second bed and the first bed is regenerated by supplying it with H<span class="hlt">2</span> for the Sabatier reaction. Initially, the H<span class="hlt">2</span> is heated to provide heat for the regeneration reaction, which is endothermic. In the later stages of regeneration, the Sabatier reaction, which is exothermic, supplies the heat for regeneration.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16668401','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16668401"><span>Relationships between the Efficiencies of Photosystems I and II and Stromal Redox State in <span class="hlt">CO</span>(<span class="hlt">2</span>)-Free <span class="hlt">Air</span> : Evidence for Cyclic Electron Flow in Vivo.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Harbinson, J; Foyer, C H</p> <p>1991-09-01</p> <p>The responses of the efficiencies of photosystems I and II, stromal redox state (as indicated by NADP-malate dehydrogenase activation state), and activation of the Benson-Calvin cycle enzymes ribulose 1,5-bisphosphate carboxylase and fructose 1,6-bisphosphatase to varying irradiance were measured in pea (Pisum sativum L.) leaves operating close to the <span class="hlt">CO</span>(<span class="hlt">2</span>) compensation point. A comparison of the relationships among these parameters obtained from leaves in <span class="hlt">air</span> was made with those obtained when the leaves were maintained in <span class="hlt">air</span> from which the <span class="hlt">CO</span>(<span class="hlt">2</span>) had been removed. P700 was more oxidized at any measured irradiance in <span class="hlt">CO</span>(<span class="hlt">2</span>)-free <span class="hlt">air</span> than in <span class="hlt">air</span>. The relationship between the quantum efficiencies of the photosystems in <span class="hlt">CO</span>(<span class="hlt">2</span>)-free <span class="hlt">air</span> was distinctly curvilinear in contrast to the predominantly linear relationship obtained with leaves in <span class="hlt">air</span>. This nonlinearity may be consistent with the operation of cyclic electron flow around photosystem I because the quantum efficiency of photosystem II was much more restricted than the quantum efficiency of photosystem I. In <span class="hlt">CO</span>(<span class="hlt">2</span>)-free <span class="hlt">air</span>, measured NADP-malate dehydrogenase activities varied considerably at low irradiances. However, at high irradiance the activity of the enzyme was low, implying that the stroma was oxidized. In contrast, fructose-1,6-bisphosphatase activities tended to increase with increasing electron 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.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018OSJ...tmp...26P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018OSJ...tmp...26P"><span>Acidification at the Surface in the East <span class="hlt">Sea</span>: A Coupled Climate-carbon Cycle 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>Park, Young-Gyu; Seol, Kyung-Hee; Boo, Kyung-On; Lee, Johan; Cho, Chunho; Byun, Young-Hwa; Seo, Seongbong</p> <p>2018-05-01</p> <p>This modeling study investigates the impacts of increasing atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentration on acidification in the East <span class="hlt">Sea</span>. A historical simulation for the past three decades (1980 to 2010) was performed using the Hadley Centre Global Environmental Model (version <span class="hlt">2</span>), a coupled climate model with atmospheric, terrestrial and ocean cycles. As the atmospheric <span class="hlt">CO</span><span class="hlt">2</span> concentration increased, acidification progressed in the surface waters of the marginal <span class="hlt">sea</span>. The acidification was similar in magnitude to observations and models of acidification in the global ocean. However, in the global ocean, the acidification appears to be due to increased in-situ oceanic <span class="hlt">CO</span><span class="hlt">2</span> uptake, whereas local processes had stronger effects in the East <span class="hlt">Sea</span>. pH was lowered by surface warming and by the influx of water with higher dissolved inorganic carbon (DIC) from the northwestern Pacific. Due to the enhanced advection of DIC, the partial pressure of <span class="hlt">CO</span><span class="hlt">2</span> increased faster than in the overlying <span class="hlt">air</span>; consequently, the in-situ oceanic uptake of <span class="hlt">CO</span><span class="hlt">2</span> decreased.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28257180','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28257180"><span>Diverse Reactivity of ECp* (E = Al, Ga) toward Low-Coordinate Transition Metal Amides [TM(N(SiMe3)<span class="hlt">2)2</span>] (TM = Fe, <span class="hlt">Co</span>, Zn): Insertion, Cp* <span class="hlt">Transfer</span>, and Orthometalation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Weßing, Jana; Göbel, Christoph; Weber, Birgit; Gemel, Christian; Fischer, Roland A</p> <p>2017-03-20</p> <p>The reactivity of the carbenoid group 13 metal ligands ECp* (E = Al, Ga) toward low valent transition metal complexes [TM(btsa) <span class="hlt">2</span> ] (TM = Fe, <span class="hlt">Co</span>, Zn; btsa = bis(trimethylsilyl)amide) was investigated, revealing entirely different reaction patterns for E = Al and Ga. Treatment of [<span class="hlt">Co</span>(btsa) <span class="hlt">2</span> ] with AlCp* yields [Cp*<span class="hlt">Co</span>(μ-H)(Al(κ <span class="hlt">2</span> -(CH <span class="hlt">2</span> SiMe <span class="hlt">2</span> )NSiMe 3 )(btsa))] (1) featuring an unusual heterometallic bicyclic structure that results from the insertion of AlCp* into the TM-N bond with concomitant ligand rearrangement including C-H activation at one amide ligand. For [Fe(btsa) <span class="hlt">2</span> ], complete ligand exchange gives FeCp* <span class="hlt">2</span> , irrespective of the employed stoichiometric ratio of the reactants. In contrast, treatment of [TM(btsa) <span class="hlt">2</span> ] (TM = Fe, <span class="hlt">Co</span>) with GaCp* forms the 1:1 and 1:<span class="hlt">2</span> adducts [(GaCp*)<span class="hlt">Co</span>(btsa) <span class="hlt">2</span> ] (<span class="hlt">2</span>) and [(GaCp*) <span class="hlt">2</span> Fe(btsa) <span class="hlt">2</span> ] (3), respectively. The tendency of AlCp* to undergo Cp* <span class="hlt">transfer</span> to the TM center appears to be dependent on the nature of the TM center: For [Zn(btsa) <span class="hlt">2</span> ], no Cp* <span class="hlt">transfer</span> is observed on reaction with AlCp*; instead, the insertion product [Zn(Al(η <span class="hlt">2</span> -Cp*)(btsa)) <span class="hlt">2</span> ] (4) is formed. In the reaction of [<span class="hlt">Co</span>(btsa) <span class="hlt">2</span> ] with the trivalent [Cp*AlH <span class="hlt">2</span> ], <span class="hlt">transfer</span> of the amide ligands without further ligand rearrangement is observed, leading to [<span class="hlt">Co</span>(μ-H) 4 (Al(η <span class="hlt">2</span> -Cp*)(btsa)) <span class="hlt">2</span> ] (5).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/7323727-effects-co-sub-accumulation-phytoalexin-phaseollin-phaseolus-vulgaris-response-mechanical-injury-infection-colletotrichum-lindemuthianum','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/7323727-effects-co-sub-accumulation-phytoalexin-phaseollin-phaseolus-vulgaris-response-mechanical-injury-infection-colletotrichum-lindemuthianum"><span>Effects of 15% <span class="hlt">CO</span>/sub <span class="hlt">2</span>/ on the accumulation of the phytoalexin phaseollin in Phaseolus vulgaris in response to mechanical injury and to infection by Colletotrichum lindemuthianum</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>Arnold, R.M.; Rahe, J.E.</p> <p>1977-04-15</p> <p>Accumulation of phaseollin at sites of point-freezing injury on etiolated hypocotyls of Phaseolus vulgaris occurred in <span class="hlt">air</span> but was prevented when seedlings were placed in <span class="hlt">air</span> containing 15 percent <span class="hlt">CO</span>/sub <span class="hlt">2</span>/ immediately after injury. The inhibitory effect was partially overcome when <span class="hlt">CO</span>/sub <span class="hlt">2</span>/-treated seedlings were returned to <span class="hlt">air</span>. Phaseollin accumulation in 15 percent <span class="hlt">CO</span>/sub <span class="hlt">2</span>/ did occur, however, when injured seedlings were maintained in <span class="hlt">air</span> for 3-9 h before being <span class="hlt">transferred</span> to <span class="hlt">CO</span>/sub <span class="hlt">2</span>/, indicating that the sensitivity to <span class="hlt">CO</span>/sub <span class="hlt">2</span>/ lies at an early stage of the process leading to phaseollin production. In contrast, phaseollin accumulation at sites ofmore » infection of P. vulgaris by an incompatible race of Colletotrichum lindemuthianum was not inhibited by 15 percent <span class="hlt">CO</span>/sub <span class="hlt">2</span>/. These results indicate that the processes leading to the accumulation of phaseollin at incompatible infection sites and at injury sites may be regulated differently.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSPO54B3246W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSPO54B3246W"><span>Using Argo-O<span class="hlt">2</span> data to examine the impact of deep-water formation events on oxygen uptake in the Labrador <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wolf, M. K.; Hamme, R. C.; Gilbert, D.; Yashayaev, I.</p> <p>2016-02-01</p> <p>Deep-water formation allows the deep ocean to communicate with the atmosphere, facilitating exchanges of heat as well as important gases such as <span class="hlt">CO</span><span class="hlt">2</span> and oxygen. The Labrador <span class="hlt">Sea</span> is the most studied location of deep convection in the North Atlantic Ocean and a strong contributor to the global thermohaline circulation. Since there are no internal sources of oxygen below the euphotic zone, deep-water formation is vital for oxygen transport to the deep ocean. Recent studies document large interannual variability in the strength and depth of convection in the Labrador <span class="hlt">Sea</span>, from mixed layers of 100m to greater than 1000m. A weakening of this deep convection starves the deep ocean of oxygen, disrupting crucial deep <span class="hlt">sea</span> biological processes, as well as reducing oceanic <span class="hlt">CO</span><span class="hlt">2</span> uptake and ocean circulation. We used data from the extensive Argo float network to examine these deep-water formation events in the Labrador <span class="hlt">Sea</span>. The oxygen optodes onboard many Argo floats suffer from biases whose amplitude must be determined; therefore we investigated and applied various optode calibration methods. Using calibrated vertical profiles of oxygen, temperature, and salinity, we observed the timing, magnitude, and location of deep convection, restratification, and spring phytoplankton blooms. In addition, we used surface oxygen values along with NCEP wind speeds to calculate the <span class="hlt">air-sea</span> oxygen flux using a range of <span class="hlt">air-sea</span> gas exchange 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 exchanges with the atmosphere at a faster rate than <span class="hlt">CO</span><span class="hlt">2</span>, is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.A11M0228S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.A11M0228S"><span><span class="hlt">Air</span> quality <span class="hlt">co</span>-benefits and costs under state, regional, or national cooperation to regulate <span class="hlt">CO</span><span class="hlt">2</span> from existing power plants</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Saari, R.; Selin, N. E.</p> <p>2015-12-01</p> <p>We examine the effect of state, regional, and national cooperation on the costs and <span class="hlt">air</span> quality <span class="hlt">co</span>-benefits of a policy to limit the carbon intensity of existing electricity generation. Electricity generation is a significant source of both greenhouse gases and <span class="hlt">air</span> pollutant emissions that harm human health. Previous studies have shown that <span class="hlt">air</span> quality <span class="hlt">co</span>-benefits can be substantial compared to the costs of limiting carbon emissions in the energy system. The EPA's proposed Clean Power Plan seeks to impose carbon intensity limits for each state, but allows states to cooperate in order to meet combined limits. We explore how such cooperation might produce trade-offs between lower costs, widespread pollution reductions, and local reductions. We employ a new state-level model of the US energy system and economy to examine the costs and emissions as states reduce demand or deploy cleaner generation. We use an advanced <span class="hlt">air</span> quality impacts modeling system, including SMOKE, CAMx, and BenMAP, to estimate health-related <span class="hlt">air</span> quality <span class="hlt">co</span>-benefits and compare these to costs under different levels of cooperation. We draw conclusions about the potential impacts of cooperation on economic welfare at various scales.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25511936','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25511936"><span>Drop <span class="hlt">transfer</span> between superhydrophobic wells using <span class="hlt">air</span> logic control.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Vuong, Thach; Cheong, Brandon Huey-Ping; Huynh, So Hung; Muradoglu, Murat; Liew, Oi Wah; Ng, Tuck Wah</p> <p>2015-02-21</p> <p>Superhydrophobic surfaces aid biochemical analysis by limiting sample loss. A system based on wells here tolerated tilting up to 20° and allowed <span class="hlt">air</span> logic <span class="hlt">transfer</span> with evidence of mixing. Conditions for intact <span class="hlt">transfer</span> on 15 to 60 μL drops using compressed <span class="hlt">air</span> pressure operation were also mapped.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24820033','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24820033"><span>Rising <span class="hlt">sea</span> level, temperature, and precipitation impact plant and ecosystem responses to elevated <span class="hlt">CO</span><span class="hlt">2</span> on a Chesapeake Bay wetland: review of a 28-year study.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Drake, Bert G</p> <p>2014-11-01</p> <p>An ongoing field study of the effects of elevated atmospheric <span class="hlt">CO</span><span class="hlt">2</span> on a brackish wetland on Chesapeake Bay, started in 1987, is unique as the longest continually running investigation of the effects of elevated <span class="hlt">CO</span><span class="hlt">2</span> on an ecosystem. Since the beginning of the study, atmospheric <span class="hlt">CO</span><span class="hlt">2</span> increased 18%, <span class="hlt">sea</span> level rose 20 cm, and growing season temperature varied with approximately the same range as predicted for global warming in the 21st century. This review looks back at this study for clues about how the effects of rising <span class="hlt">sea</span> level, temperature, and precipitation interact with high atmospheric <span class="hlt">CO</span><span class="hlt">2</span> to alter the physiology of C3 and C4 photosynthetic species, carbon assimilation, evapotranspiration, plant and ecosystem nitrogen, and distribution of plant communities in this brackish wetland. Rising <span class="hlt">sea</span> level caused a shift to higher elevations in the Scirpus olneyi C3 populations on the wetland, displacing the Spartina patens C4 populations. Elevated <span class="hlt">CO</span><span class="hlt">2</span> stimulated carbon assimilation in the Scirpus C3 species measured by increased shoot and root density and biomass, net ecosystem production, dissolved organic and inorganic carbon, and methane production. But elevated <span class="hlt">CO</span><span class="hlt">2</span> also decreased biomass of the grass, S. patens C4. The elevated <span class="hlt">CO</span><span class="hlt">2</span> treatment reduced tissue nitrogen concentration in shoots, roots, and total canopy nitrogen, which was associated with reduced ecosystem respiration. Net ecosystem production was mediated by precipitation through soil salinity: high salinity reduced the <span class="hlt">CO</span><span class="hlt">2</span> effect on net ecosystem production, which was zero in years of severe drought. The elevated <span class="hlt">CO</span><span class="hlt">2</span> stimulation of shoot density in the Scirpus C3 species was sustained throughout the 28 years of the study. Results from this study suggest that rising <span class="hlt">CO</span><span class="hlt">2</span> can add substantial amounts of carbon to ecosystems through stimulation of carbon assimilation, increased root exudates to supply nitrogen fixation, reduced dark respiration, and improved water and nitrogen use efficiency. Published</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/380353','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/380353"><span>The photosynthetic and stomatal response of Medicago sativa cv. saranac to free-<span class="hlt">air</span> <span class="hlt">CO</span>{sub <span class="hlt">2</span>} enrichment (F.A.C.E.) and nitrogen</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>Bridson, N.P.</p> <p>1996-08-01</p> <p>Plots of Medicago sativa cv. saranac were grown in the field at ambient (355 {mu}mol <span class="hlt">CO</span>{sub <span class="hlt">2</span>} mol{sup -1} <span class="hlt">air</span>) or elevated (600{mu}mol <span class="hlt">CO</span>{sub <span class="hlt">2</span>} mol{sup -1} <span class="hlt">air</span>) <span class="hlt">CO</span>{sub <span class="hlt">2</span>} concentrations. High (200kg yr{sup -1}) or low (20kg yr{sup -1}) nitrogen levels were applied to two isogeneic lines, one able and one unable to use nitrogen fixing bacteria. Plants were in the second year of field growth. Exposure to elevated <span class="hlt">CO</span>{sub <span class="hlt">2</span>} was via a Free-<span class="hlt">Air</span> <span class="hlt">CO</span>{sub <span class="hlt">2</span>} Enrichment System (FACE). Elevated <span class="hlt">CO</span>{sub <span class="hlt">2</span>} increased diurnal assimilation by between 12% and 92%. Analysis of A/C{sub i} responses showed that effectivemore » nitrogen fertilisation was more important to rubis<span class="hlt">CO</span> and RuBP activity than elevated <span class="hlt">CO</span>{sub <span class="hlt">2</span>}. No acclimation was consistently observed. Leaves lower down the canopy were found to have lower Vc{sub max} and J{sub max} values, though age may be the cause of the latter effect. FACE conditions have only a small effect on these responses. There was some evidence found for the down-regulation of photosynthesis in the late afternoon. The FACE conditions had no affect on stomatal density but did increase epidermal cell density.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20120013806&hterms=japanese&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Djapanese','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20120013806&hterms=japanese&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Djapanese"><span>Space-Based Measurements of <span class="hlt">CO</span><span class="hlt">2</span> from the Japanese Greenhouse Gases Observing Satellite (GOSAT) and the NASA Orbiting Carbon Observatory-<span class="hlt">2</span> (OCO-<span class="hlt">2</span>) Missions</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Crisp, David</p> <p>2011-01-01</p> <p>Space-based remote sensing observations hold substantial promise for future long-term monitoring of <span class="hlt">CO</span><span class="hlt">2</span> and other greenhouse gases. The principal advantages of space based measurements include: (1) Spatial coverage (especially over oceans and tropical land) (<span class="hlt">2</span>) Sampling density (needed to resolve <span class="hlt">CO</span><span class="hlt">2</span> weather). The principal challenge is the need for high precision To reach their full potential, space based <span class="hlt">CO</span><span class="hlt">2</span> measurements must be validated against surface measurements to ensure their accuracy. The TCCON network is providing the <span class="hlt">transfer</span> standard There is a need for a long-term vision to establish and address community priorities (1) Must incorporate ground, <span class="hlt">air</span>, space-based assets and models (<span class="hlt">2</span>) Must balance calls for new observations with need to maintain climate data records.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25629220','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25629220"><span>Fast and reversible direct <span class="hlt">CO</span><span class="hlt">2</span> capture from <span class="hlt">air</span> onto all-polymer nanofibrillated cellulose-polyethylenimine foams.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sehaqui, Houssine; Gálvez, María Elena; Becatinni, Viola; cheng Ng, Yi; Steinfeld, Aldo; Zimmermann, Tanja; Tingaut, Philippe</p> <p>2015-03-03</p> <p>Fully polymeric and biobased <span class="hlt">CO</span><span class="hlt">2</span> sorbents composed of oxidized nanofibrillated cellulose (NFC) and a high molar mass polyethylenimine (PEI) have been prepared via a freeze-drying process. This resulted in NFC/PEI foams displaying a sheet structure with porosity above 97% and specific surface area in the range <span class="hlt">2</span>.7-8.3 m(<span class="hlt">2</span>)·g(-1). Systematic studies on the impact of both PEI content and relative humidity on the <span class="hlt">CO</span><span class="hlt">2</span> capture capacity of the amine functionalized sorbents have been conducted under atmospheric conditions (moist <span class="hlt">air</span> with ∼400 ppm of <span class="hlt">CO</span><span class="hlt">2</span>). At 80% RH and an optimum PEI content of 44 wt %, a <span class="hlt">CO</span><span class="hlt">2</span> capacity of <span class="hlt">2</span>.22 mmol·g(-1), a stability over five cycles, and an exceptionally low adsorption half time of 10.6 min were achieved. In the 20-80% RH range studied, the increase in relative humidity increased <span class="hlt">CO</span><span class="hlt">2</span> capacity of NFC/PEI foams at the expense of a high H<span class="hlt">2</span>O uptake in the range 3.8-28 mmol·g(-1).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28351822','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28351822"><span>Thermal decomposition of sewage sludge under N<span class="hlt">2</span>, <span class="hlt">CO</span><span class="hlt">2</span> and <span class="hlt">air</span>: Gas characterization and kinetic analysis.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hernández, Ana Belén; Okonta, Felix; Freeman, Ntuli</p> <p>2017-07-01</p> <p>Thermochemical valorisation processes that allow energy to be recovered from sewage sludge, such as pyrolysis and gasification, have demonstrated great potential as convenient alternatives to conventional sewage sludge disposal technologies. Moreover, these processes may benefit from <span class="hlt">CO</span> <span class="hlt">2</span> recycling. Today, the scaling up of these technologies requires an advanced knowledge of the reactivity of sewage sludge and the characteristics of the products, specific to the thermochemical process. In this study the behaviour of sewage sludge during thermochemical conversion, under different atmospheres (N <span class="hlt">2</span> , <span class="hlt">CO</span> <span class="hlt">2</span> and <span class="hlt">air</span>), was studied, using TGA-FTIR, in order to understand the effects of different atmospheric gases on the kinetics of degradation and on the gaseous products. The different steps observed during the solid degradation were related with the production of different gaseous compounds. A higher oxidative degree of the atmosphere surrounding the sample resulted in higher reaction rates and a shift of the degradation mechanisms to lower temperatures, especially for the mechanisms taking place at temperatures above 400 °C. Finally, a multiple first-order reaction model was proposed to compare the kinetic parameters obtained under different atmospheres. Overall, the highest activation energies were obtained for combustion. This work proves that <span class="hlt">CO</span> <span class="hlt">2</span> , an intermediate oxidative atmosphere between N <span class="hlt">2</span> and <span class="hlt">air</span>, results in an intermediate behaviour (intermediate peaks in the derivative thermogravimetric curves and intermediate activation energies) during the thermochemical decomposition of sewage sludge. Overall, it can be concluded that the kinetics of these different processes require a different approach for their scaling up and specific consideration of their characteristic reaction temperatures and rates should be evaluated. Copyright © 2017 Elsevier Ltd. All rights reserved.</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> exchange (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://ntrs.nasa.gov/search.jsp?R=19790033167&hterms=laser+darpa&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dlaser%2Bdarpa','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19790033167&hterms=laser+darpa&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dlaser%2Bdarpa"><span>Ground-to-space optical power <span class="hlt">transfer</span>. [using laser propulsion for orbit <span class="hlt">transfer</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mevers, G. E.; Hayes, C. L.; Soohoo, J. F.; Stubbs, R. M.</p> <p>1978-01-01</p> <p>Using laser radiation as the energy input to a rocket, it is possible to consider the <span class="hlt">transfer</span> of large payloads economically between low initial orbits and higher energy orbits. In this paper we will discuss the results of an investigation to use a ground-based High Energy Laser (HEL) coupled to an adaptive antenna to transmit multi-megawatts of power to a satellite in low-earth orbit. Our investigation included diffraction effects, atmospheric transmission efficiency, adaptive compensation for atmospheric turbulence effects, including the servo bandwidth requirements for this correction, and the adaptive compensation for thermal blooming. For these evaluations we developed vertical profile models of atmospheric absorption, strength of optical turbulence (CN<span class="hlt">2</span>), wind, temperature, and other parameters necessary to calculate system performance. Our atmospheric investigations were performed for <span class="hlt">CO</span><span class="hlt">2</span>, 12C18O<span class="hlt">2</span> isotope, <span class="hlt">CO</span> and DF wavelengths. For all of these considerations, output antenna locations of both <span class="hlt">sea</span> level and mountain top (3.5 km above <span class="hlt">sea</span> level) were used. Several adaptive system concepts were evaluated with a multiple source phased array concept being selected. This system uses an adaption technique of phase locking independent laser oscillators. When both system losses and atmospheric effects were assessed, the results predicted an overall power <span class="hlt">transfer</span> efficiency of slightly greater than 50%.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMOS12A..07V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMOS12A..07V"><span>The footprint of <span class="hlt">CO</span><span class="hlt">2</span> leakage in the water-column: Insights from numerical modeling based on a North <span class="hlt">Sea</span> gas release experiment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vielstädte, L.; Linke, P.; Schmidt, M.; Sommer, S.; Wallmann, K.; McGinnis, D. F.; Haeckel, M.</p> <p>2013-12-01</p> <p>Assessing the environmental impact of potential <span class="hlt">CO</span><span class="hlt">2</span> leakage from offshore carbon dioxide storage sites necessitates the investigation of the corresponding pH change in the water-column. Numerical models have been developed to simulate the buoyant rise and dissolution of <span class="hlt">CO</span><span class="hlt">2</span> bubbles in the water-column and the subsequent near-field dispersion of dissolved <span class="hlt">CO</span><span class="hlt">2</span> in seawater under ocean current and tidal forcing. In order to test and improve numerical models a gas release experiment has been conducted at 80 m water-depth within the Sleipner area (North <span class="hlt">Sea</span>). <span class="hlt">CO</span><span class="hlt">2</span> and Kr (used as inert tracer gas) were released on top of a benthic lander at varying gas flows (<140 kg/day) and bubble sizes (de: 1-6 mm). p<span class="hlt">CO</span><span class="hlt">2</span> and pH were measured by in situ sensors to monitor the spread of the solute in different vertical heights and distances downstream of the artificial leak. The experiment and numerical analysis show that the impact of such leakage rates is limited to the near-field bottom waters, due to the rapid dissolution of <span class="hlt">CO</span><span class="hlt">2</span> bubbles in seawater (<span class="hlt">CO</span><span class="hlt">2</span> is being stripped within the first two to five meters of bubble rise). In particular, small bubbles, which will dissolve close to the seafloor, may cause a dangerous low-pH environment for the marine benthos. However, on the larger scale, the advective transport by e.g. tidal currents, dominates the <span class="hlt">CO</span><span class="hlt">2</span> dispersal in the North <span class="hlt">Sea</span> and dilutes the <span class="hlt">CO</span><span class="hlt">2</span> peak quickly. The model results show that at the small scales (<100 m) of the <span class="hlt">CO</span><span class="hlt">2</span> plume the lateral eddy diffusion (~0.01 m<span class="hlt">2</span>/s) has only a negligible effect. Overall, we can postulate that <span class="hlt">CO</span><span class="hlt">2</span> leakage at a rate of ~ 100 kg per day as in our experiment will only have a localized impact on the marine environment, thereby reducing pH substantially (by 0.4 units) within a diameter of less than 50 m around the release spot (depending on the duration of leakage and the current velocities). Strong currents and tidal cycles significantly reduce the spreading of low-pH water masses into the far</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19970036015','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19970036015"><span>Research in Observations of Oceanic <span class="hlt">Air/Sea</span> Interaction</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Long, David G.; Arnold, David V.</p> <p>1995-01-01</p> <p>The primary purpose of this research has been: (1) to develop an innovative research radar scatterometer system capable of directly measuring both the radar backscatter and the small-scale and large-scale ocean wave field simultaneously and (<span class="hlt">2</span>) deploy this instrument to collect data to support studies of <span class="hlt">air/sea</span> interaction. The instrument has been successfully completed and deployed. The system deployment lasted for six months during 1995. Results to date suggest that the data is remarkably useful in <span class="hlt">air/sea</span> interaction studies. While the data analysis is continuing, two journal and fifteen conference papers have been published. Six papers are currently in review with two additional journal papers scheduled for publication. Three Master's theses on this research have been completed. A Ph.D. student is currently finalizing his dissertation which should be completed by the end of the calendar year. We have received additional 'mainstream' funding from the NASA oceans branch to continue data analysis and instrument operations. We are actively pursuing results from the data expect additional publications to follow. This final report briefly describes the instrument system we developed and results to-date from the deployment. Additional detail is contained in the attached papers selected from the bibliography.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28402293','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28402293"><span>Influence of relative <span class="hlt">air</span>/water flow velocity on oxygen mass <span class="hlt">transfer</span> in gravity sewers.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Carrera, Lucie; Springer, Fanny; Lipeme-Kouyi, Gislain; Buffiere, Pierre</p> <p>2017-04-01</p> <p>Problems related to hydrogen sulfide may be serious for both network stakeholders and the public in terms of health, sustainability of the sewer structure and urban comfort. H <span class="hlt">2</span> S emission models are generally theoretical and simplified in terms of environmental conditions. Although <span class="hlt">air</span> transport characteristics in sewers must play a role in the fate of hydrogen sulfide, only a limited number of studies have investigated this issue. The aim of this study was to better understand H <span class="hlt">2</span> S liquid to gas <span class="hlt">transfer</span> by highlighting the link between the mass <span class="hlt">transfer</span> coefficient and the turbulence in the <span class="hlt">air</span> flow and the water flow. For experimental safety reasons, O <span class="hlt">2</span> was taken as a model compound. The oxygen mass <span class="hlt">transfer</span> coefficients were obtained using a mass balance in plug flow. The mass <span class="hlt">transfer</span> coefficient was not impacted by the range of the interface <span class="hlt">air</span>-flow velocity values tested (0.55-<span class="hlt">2</span>.28 m·s -1 ) or the water velocity values (0.06-0.55 m·s -1 ). Using the ratio between k L,O <span class="hlt">2</span> to k L,H <span class="hlt">2</span> S , the H <span class="hlt">2</span> S mass <span class="hlt">transfer</span> behavior in a gravity pipe in the same hydraulic conditions can be predicted.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1130720-co-benefits-mitigating-global-greenhouse-gas-emissions-future-air-quality-human-health','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1130720-co-benefits-mitigating-global-greenhouse-gas-emissions-future-air-quality-human-health"><span><span class="hlt">Co</span>-benefits of mitigating global greenhouse gas emissions for future <span class="hlt">air</span> quality and human health</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>West, Jason; Smith, Steven J.; Silva, Raquel</p> <p>2013-10-01</p> <p>Reducing greenhouse gas (GHG) emissions also influences <span class="hlt">air</span> quality. We simulate the <span class="hlt">co</span>-benefits of global GHG reductions on <span class="hlt">air</span> quality and human health via two mechanisms: a) reducing <span class="hlt">co</span>-emitted <span class="hlt">air</span> pollutants, and b) slowing climate change and its effect on <span class="hlt">air</span> quality. Relative to a reference scenario, global GHG mitigation in the RCP4.5 scenario avoids 0.5±0.<span class="hlt">2</span>, 1.3±0.6, and <span class="hlt">2.2</span>±1.6 million premature deaths in 2030, 2050, and 2100, from changes in fine particulate matter and ozone. Global average marginal <span class="hlt">co</span>-benefits of avoided mortality are $40-400 (ton <span class="hlt">CO</span><span class="hlt">2</span>)-1, exceeding marginal abatement costs in 2030 and 2050, and within the low range ofmore » costs in 2100. East Asian <span class="hlt">co</span>-benefits are 10-80 times the marginal cost in 2030. These results indicate that transitioning to a low-carbon future might be justified by <span class="hlt">air</span> quality and health <span class="hlt">co</span>-benefits.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1816702N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1816702N"><span>A spectroscopic <span class="hlt">transfer</span> standard for accurate atmospheric <span class="hlt">CO</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>Nwaboh, Javis A.; Li, Gang; Serdyukov, Anton; Werhahn, Olav; Ebert, Volker</p> <p>2016-04-01</p> <p>Atmospheric carbon monoxide (<span class="hlt">CO</span>) is a precursor of essential climate variables and has an indirect effect for enhancing global warming. Accurate and reliable measurements of atmospheric <span class="hlt">CO</span> concentration are becoming indispensable. WMO-GAW reports states a compatibility goal of ±<span class="hlt">2</span> ppb for atmospheric <span class="hlt">CO</span> concentration measurements. Therefore, the EMRP-HIGHGAS (European metrology research program - high-impact greenhouse gases) project aims at developing spectroscopic <span class="hlt">transfer</span> standards for <span class="hlt">CO</span> concentration measurements to meet this goal. A spectroscopic <span class="hlt">transfer</span> standard would provide results that are directly traceable to the SI, can be very useful for calibration of devices operating in the field, and could complement classical gas standards in the field where calibration gas mixtures in bottles often are not accurate, available or stable enough [1][<span class="hlt">2</span>]. Here, we present our new direct tunable diode laser absorption spectroscopy (dTDLAS) sensor capable of performing absolute ("calibration free") <span class="hlt">CO</span> concentration measurements, and being operated as a spectroscopic <span class="hlt">transfer</span> standard. To achieve the compatibility goal stated by WMO for <span class="hlt">CO</span> concentration measurements and ensure the traceability of the final concentration results, traceable spectral line data especially line intensities with appropriate uncertainties are needed. Therefore, we utilize our new high-resolution Fourier-transform infrared (FTIR) spectroscopy <span class="hlt">CO</span> line data for the <span class="hlt">2</span>-0 band, with significantly reduced uncertainties, for the dTDLAS data evaluation. Further, we demonstrate the capability of our sensor for atmospheric <span class="hlt">CO</span> measurements, discuss uncertainty calculation following the guide to the expression of uncertainty in measurement (GUM) principles and show that <span class="hlt">CO</span> concentrations derived using the sensor, based on the TILSAM (traceable infrared laser spectroscopic amount fraction measurement) method, are in excellent agreement with gravimetric values. Acknowledgement Parts of this work have been</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('https://www.ncbi.nlm.nih.gov/pubmed/26717443','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26717443"><span>Attempts To Catalyze the Electrochemical <span class="hlt">CO</span><span class="hlt">2</span>-to-Methanol Conversion by Biomimetic <span class="hlt">2</span>e(-) + <span class="hlt">2</span>H(+) <span class="hlt">Transferring</span> Molecules.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Saveant, Jean-Michel; Tard, Cédric</p> <p>2016-01-27</p> <p>In the context of the electrochemical and photochemical conversion of <span class="hlt">CO</span><span class="hlt">2</span> to liquid fuels, one of the most important issues of contemporary energy and environmental issues, the possibility of pushing the reduction beyond the <span class="hlt">CO</span> and formate level and catalytically generate products such as methanol is particularly attractive. Biomimetic <span class="hlt">2</span>e(-) + <span class="hlt">2</span>H(+) is often viewed as a potential hydride donor. This has been the object of a recent interesting attempt (J. Am. Chem. Soc. 2014, 136, 14007) in which 6,7-dimethyl-4-hydroxy-<span class="hlt">2</span>-mercaptopteridine was reported as a catalyst of the electrochemical conversion of <span class="hlt">CO</span><span class="hlt">2</span> to methanol and formate, based on cyclic voltammetric, (13)C NMR, IR, and GC analyses. After checking electrolysis at the reported potential and at a more negative potential to speed up the reaction, it appears, on (1)H NMR and gas chromatographic grounds, that there is neither catalysis nor methanol and nor formate production. (1)H NMR (with H<span class="hlt">2</span>O presaturation) brings about an unambiguous answer to the eventual production of methanol and formate, much more so than (13)C NMR, which can even be misleading when no internal standard is used as in the above-mentioned paper. IR analysis is even less conclusive. Use of a GC technique with sufficient sensitivity confirmed the lack of methanol formation. The direct or indirect hydride <span class="hlt">transfer</span> electrochemical reduction of <span class="hlt">CO</span><span class="hlt">2</span> to formate and to methanol remains an open question. Original ideas and efforts such as those discussed here are certainly worth tempting. However, in view of the importance of the stakes, it appears necessary to carefully check reports in this area.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFMOS53C1999S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMOS53C1999S"><span>Ca<span class="hlt">CO</span>3 dissolution by holothurians (<span class="hlt">sea</span> cucumber): a case study from One Tree Reef, Great Barrier Reef</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schneider, K.; Silverman, J.; Kravitz, B.; Woolsey, E.; Eriksson, H.; Schneider-Mor, A.; Barbosa, S.; Rivlin, T.; Byrne, M.; Caldeira, K.</p> <p>2012-12-01</p> <p>Holothurians (<span class="hlt">sea</span> cucumbers) are among the largest and most important deposit feeder in coral reefs. They play a role in nutrient and Ca<span class="hlt">CO</span>3 cycling within the reef structure. As a result of their digestive process they secrete alkalinity due to Ca<span class="hlt">CO</span>3 dissolution and organic matter degradation forming <span class="hlt">CO</span><span class="hlt">2</span> and ammonium. In a survey at station DK13 on One Three Reef we found that the population density of holothurians was > 1 individual m-<span class="hlt">2</span>. The dominant <span class="hlt">sea</span> cucumber species Holothuria leucospilota was collected from DK13. The increase in alkalinity due to Ca<span class="hlt">CO</span>3 dissolution in aquaria incubations was measured to be 47±7 μmol kg-1 in average per individual. Combining this dissolution rate with the <span class="hlt">sea</span> cucumbers concentrations at DK13 suggest that they may account for a dissolution rate of 34.9±17.8 mmol m-<span class="hlt">2</span> day-1, which is equivalent to about half of night time community dissolution measured in DK13. This indicates that in reefs where the <span class="hlt">sea</span> cucumber population is healthy and protected from fishing they can be locally important in the Ca<span class="hlt">CO</span>3 cycle. Preliminary result suggests that the Ca<span class="hlt">CO</span>3 dissolution rates are not affected by the chemistry of the <span class="hlt">sea</span> water they are incubated in. Measurements of the empty digestive track volume of two <span class="hlt">sea</span> cucumbers H. atra and Stichopus herrmanni were 36 ± 4 ml and 151 ± 14 ml, respectively. Based on these measurements it is estimated that these species process 19 ± <span class="hlt">2</span>kg and 80 ± 7kg Ca<span class="hlt">CO</span>3 sand yr-1 per individual, respectively. The annual dissolution rates of H. atra and S. herrmanni are 6.5±1.9g and 9.6±1.4g, respectively, suggest that 0.05±0.02% and 0.1±0.02% of the Ca<span class="hlt">CO</span>3 processed through their gut annually is dissolved. During the incubations the Ca<span class="hlt">CO</span>3 dissolution was 0.07±0.01%, 0.04±0.01% and 0.21±0.05% of the fecal casts for H. atra, H. leucospilota and S. herrmanni, respectively. Our result that the primary parameter determining the Ca<span class="hlt">CO</span>3 dissolution by <span class="hlt">sea</span> cucumber is the amount of carbonate send in their gut</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010pot..book..883Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010pot..book..883Z"><span>Numerical Simulation on Hydrodynamics and Combustion in a Circulating Fluidized Bed under O<span class="hlt">2</span>/<span class="hlt">CO</span><span class="hlt">2</span> and <span class="hlt">Air</span> Atmospheres</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhou, W.; Zhao, C. S.; Duan, L. B.; Qu, C. R.; Lu, J. Y.; Chen, X. P.</p> <p></p> <p>Oxy-fuel circulating fluidized bed (CFB) combustion technology is in the stage of initial development for carbon capture and storage (CCS). Numerical simulation is helpful to better understanding the combustion process and will be significant for CFB scale-up. In this paper, a computational fluid dynamics (CFD) model was employed to simulate the hydrodynamics of gas-solid flow in a CFB riser based on the Eulerian-Granular multiphase model. The cold model predicted the main features of the complex gas-solid flow, including the cluster formation of the solid phase along the walls, the flow structure of up-flow in the core and downward flow in the annular region. Furthermore, coal devolatilization, char combustion and heat <span class="hlt">transfer</span> were considered by coupling semi-empirical sub-models with CFD model to establish a comprehensive model. The gas compositions and temperature profiles were predicted and the outflow gas fractions are validated with the experimental data in <span class="hlt">air</span> combustion. With the experimentally validated model being applied, the concentration and temperature distributions in O<span class="hlt">2</span>/<span class="hlt">CO</span><span class="hlt">2</span> combustion were predicted. The model is useful for the further development of a comprehensive model including more sub-models, such as pollutant emissions, and better understanding the combustion process in furnace.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014APS..DFD.R5003P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014APS..DFD.R5003P"><span>Dissolution of spherical cap <span class="hlt">CO</span><span class="hlt">2</span> bubbles attached to flat surfaces in <span class="hlt">air</span>-saturated water</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Peñas, Pablo; Parrales, Miguel A.; Rodriguez-Rodriguez, Javier</p> <p>2014-11-01</p> <p>Bubbles attached to flat surfaces immersed in quiescent liquid environments often display a spherical cap (SC) shape. Their dissolution is a phenomenon commonly observed experimentally. Modelling these bubbles as fully spherical may lead to an inaccurate estimate of the bubble dissolution rate. We develop a theoretical model for the diffusion-driven dissolution or growth of such multi-component SC gas bubbles under constant pressure and temperature conditions. Provided the contact angle of the bubble with the surface is large, the concentration gradients in the liquid may be approximated as spherically symmetric. The area available for mass <span class="hlt">transfer</span> depends on the instantaneous bubble contact angle, whose dynamics is computed from the adhesion hysteresis model [Hong et al., Langmuir, vol. 27, 6890-6896 (2011)]. Numerical simulations and experimental measurements on the dissolution of SC <span class="hlt">CO</span><span class="hlt">2</span> bubbles immersed in <span class="hlt">air</span>-saturated water support the validity of our model. We verify that contact line pinning slows down the dissolution rate, and the fact that any bubble immersed in a saturated gas-liquid solution eventually attains a final equilibrium size. Funded by the Spanish Ministry of Economy and Competitiveness through Grant DPI2011-28356-C03-0.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25898645','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25898645"><span>[Partial pressure of <span class="hlt">CO</span><span class="hlt">2</span> and <span class="hlt">CO</span><span class="hlt">2</span> degassing fluxes of Huayuankou and Xiaolangdi Station affected by Xiaolangdi Reservoir].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhang, Yong-ling; Yang, Xiao-lin; Zhang, Dong</p> <p>2015-01-01</p> <p>According to periodic sampling analysis per month in Xiaolangdi station and Huayuankou station from November 2011 to October 2012, combined with continuous sampling analysis of Xiaolangdi Reservoir during runoff and sediment control period in 2012, partial pressure of <span class="hlt">CO</span><span class="hlt">2</span> (p<span class="hlt">CO</span><span class="hlt">2</span>) in surface water were calculated based on Henry's Law, p<span class="hlt">CO</span><span class="hlt">2</span> features and <span class="hlt">air</span>-water <span class="hlt">CO</span><span class="hlt">2</span> degassing fluxes of Huayuankou station and Xiaolangdi station affected by Xiaolangdi Reservoir were studied. The results were listed as follows, when Xiaolangdi Reservoir operated normally, p<span class="hlt">CO</span><span class="hlt">2</span> in surface water of Xiaolangdi station and Huayuankou station varied from 82 to 195 Pa and from 99 to 228 Pa, moreover, p<span class="hlt">CO</span><span class="hlt">2</span> in surface water from July to September were distinctly higher than those in other months; meanwhile, p<span class="hlt">CO</span>, in surface water from Huayuankou station were higher than that from Xiaolangdi station. During runoff and sediment control period of Xiaolangdi Reservoir, two hydrological stations commonly indicated that p<span class="hlt">CO</span><span class="hlt">2</span> in surface water during water draining were obviously lower than those during sediment releasing. Whether in the period of normal operation or runoff and sediment control, p<span class="hlt">CO</span><span class="hlt">2</span> in surface water had positive relations to DIC content in two hydrological stations. Since the Ep<span class="hlt">CO</span>,/AOU value was higher than the theoretical value of 0. 62, the biological aerobic respiration effect had distinct contribution to p<span class="hlt">CO</span><span class="hlt">2</span>. Throughout the whole year, <span class="hlt">air</span>-water <span class="hlt">CO</span><span class="hlt">2</span> degassing fluxes from Xiaolangdi station and Huayuankou station were 0.486 p.mol (m<span class="hlt">2</span> s) -l and 0.588 pmol (m<span class="hlt">2</span> x s)(-1) respectively; When Xiaolangdi Reservoir operated normally, <span class="hlt">air</span>-water <span class="hlt">CO</span>, degassing fluxes in Huayuankou station were higher than that in Xiaolangdi station; during runoff and sediment control from Xiaolangdi Reservoir, two hydrological stations had one observation result in common, namely, <span class="hlt">air</span>-water <span class="hlt">CO</span><span class="hlt">2</span> degassing fluxes in the period of water draining were obviously lower than that in the period of sediment releasing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/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> exchange in ice-covered <span class="hlt">seas</span>. Little is known, however, of the spatial and temporal dynamics of ikaite in <span class="hlt">sea</span> ice. Here we present evidence for highly dynamic ikaite precipitation and dissolution in <span class="hlt">sea</span> ice grown at an 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> exchange with the atmosphere and ocean that has not been accounted for previously.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19830047182&hterms=atmospheric+rivers&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Datmospheric%2Brivers','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19830047182&hterms=atmospheric+rivers&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Datmospheric%2Brivers"><span>Marine biological controls on atmospheric <span class="hlt">CO</span><span class="hlt">2</span> and climate</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mcelroy, M. B.</p> <p>1983-01-01</p> <p>It is argued that the ocean is losing N gas faster than N is being returned to the ocean, and that replenishment of the N supply in the ocean usually occurs during ice ages. Available N from river and estruarine transport and from rainfall after formation by lightning are shown to be at a rate too low to compensate for the 10,000 yr oceanic lifetime of N. Ice sheets advance and <span class="hlt">transfer</span> moraine N to the ocean, lower the <span class="hlt">sea</span> levels, erode the ocean beds, promote greater biological productivity, and reduce <span class="hlt">CO</span><span class="hlt">2</span>. Ice core samples have indicated a variability in the atmospheric N content that could be attributed to the ice age scenario.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22158529','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22158529"><span>Randomised controlled crossover trial of the effect on Pt<span class="hlt">CO</span><span class="hlt">2</span> of oxygen-driven versus <span class="hlt">air</span>-driven nebulisers in severe chronic obstructive pulmonary disease.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Edwards, Llifon; Perrin, Kyle; Williams, Mathew; Weatherall, Mark; Beasley, Richard</p> <p>2012-11-01</p> <p>The comparative safety of oxygen versus <span class="hlt">air</span>-driven nebulised bronchodilators in patients with acute exacerbations of chronic obstructive pulmonary disease (COPD) is uncertain. A randomised controlled trial was performed to assess the effect on the arterial partial pressure of carbon dioxide of nebulised bronchodilator driven with oxygen versus <span class="hlt">air</span> in stable severe COPD. In an open label randomised study, 18 subjects with stable severe COPD attended on <span class="hlt">2</span> days to receive nebulised bronchodilator therapy driven by <span class="hlt">air</span> or oxygen. Subjects received 5 mg salbutamol and 0.5 mg ipratropium bromide by nebulisation over 15 min, then, after 5 min, 5 mg salbutamol nebulised over 15 min, followed by 15 min of observation. Transcutaneous carbon dioxide tension (Pt<span class="hlt">CO</span>(<span class="hlt">2</span>)) and oxygen saturations were recorded at 5 min intervals during the study. The primary outcome was the Pt<span class="hlt">CO</span>(<span class="hlt">2</span>) after the completion of the second bronchodilator treatment. Pt<span class="hlt">CO</span>(<span class="hlt">2</span>) was higher with nebulised bronchodilator therapy delivered by oxygen, but decreased back to the level associated with <span class="hlt">air</span> nebulisation 15 min after completion of the second nebulised dose. One subject experienced an increase in Pt<span class="hlt">CO</span>(<span class="hlt">2</span>) of 11 mm Hg after the first bronchodilator nebulisation driven by oxygen. The mean Pt<span class="hlt">CO</span>(<span class="hlt">2</span>) difference between the oxygen and <span class="hlt">air</span> groups after the second nebulisation was 3.1 mm Hg (95% CI 1.6 to 4.5, p<0.001). Nebulisers driven with oxygen result in significantly higher levels of Pt<span class="hlt">CO</span>(<span class="hlt">2</span>) than those driven with <span class="hlt">air</span> in patients with severe COPD. The study was registered on the Australian New Zealand Clinical Trials Registry (ACTRN12610000080022).</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> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMOS11B1654B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMOS11B1654B"><span>Skin Temperature Processes in the Presence of <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>Brumer, S. E.; Zappa, C. J.; Brown, S.; McGillis, W. R.; Loose, B.</p> <p>2013-12-01</p> <p>Monitoring the <span class="hlt">sea</span>-ice margins of polar oceans and understanding the physical processes at play at the ice-ocean-<span class="hlt">air</span> interface is essential in the perspective of a changing climate in which we face an accelerated decline of ice caps and <span class="hlt">sea</span> ice. Remote sensing and in particular InfraRed (IR) imaging offer a unique opportunity not only to observe physical processes at <span class="hlt">sea</span>-ice margins, but also to measure <span class="hlt">air-sea</span> exchanges near ice. It permits monitoring ice and ocean temperature variability, and can be used for derivation of surface flow field allowing investigating turbulence and shearing at the ice-ocean interface as well as ocean-atmosphere gas <span class="hlt">transfer</span>. Here we present experiments conducted with the aim of gaining an insight on how the presence of <span class="hlt">sea</span> ice affects the momentum exchange between the atmosphere and ocean and investigate turbulence production in the interplay of ice-water shear, convection, waves and wind. A set of over 200 high resolution IR imagery records was taken at the US Army Cold Regions Research and Engineering Laboratory (CRREL, Hanover NH) under varying ice coverage, fan and pump settings. In situ instruments provided <span class="hlt">air</span> and water temperature, salinity, subsurface currents and wave height. <span class="hlt">Air</span> side profiling provided environmental parameters such as wind speed, humidity and heat fluxes. The study aims to investigate what can be gained from small-scale high-resolution IR imaging of the ice-ocean-<span class="hlt">air</span> interface; in particular how <span class="hlt">sea</span> ice modulates local physics and gas <span class="hlt">transfer</span>. The relationship between water and ice temperatures with current and wind will be addressed looking at the ocean and ice temperature variance. Various skin temperature and gas <span class="hlt">transfer</span> parameterizations will be evaluated at ice margins under varying environmental conditions. Furthermore the accuracy of various techniques used to determine surface flow will be assessed from which turbulence statistics will be determined. This will give an insight on how ice presence</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> exchange in the vast wetlands of Doñana (Spain) in relation to different hydrological cycles. Water sources feeding Doñana, including groundwater and streams, ultimately depend on the fluctuating balance between annual precipitation and evapotranspiration. Hence, in order to examine the contribution of the rainfall pattern to the emission/capture of <span class="hlt">CO</span><span class="hlt">2</span> by a range of aquatic habitats in Doñana, we took monthly measurements during severely wet, dry, and normal hydrological years (2010-2013). During wet hydrological cycles, <span class="hlt">CO</span><span class="hlt">2</span> outgassing from flooded marshes markedly decreased in comparison to that observed during subsequent dry-normal cycles, with mean values of 25.84 ± 19 and 5.<span class="hlt">2</span> ± 8 mmol m-<span class="hlt">2</span> d-1, respectively. Under drier meteorological conditions, <span class="hlt">air</span>-water <span class="hlt">CO</span><span class="hlt">2</span> 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('https://www.ncbi.nlm.nih.gov/pubmed/29403458','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29403458"><span>Contribution of Bicarbonate Assimilation to Carbon Pool Dynamics in the Deep Mediterranean <span class="hlt">Sea</span> and Cultivation of Actively Nitrifying and <span class="hlt">CO</span><span class="hlt">2</span>-Fixing Bathypelagic Prokaryotic Consortia.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>La Cono, Violetta; Ruggeri, Gioachino; Azzaro, Maurizio; Crisafi, Francesca; Decembrini, Franco; Denaro, Renata; La Spada, Gina; Maimone, Giovanna; Monticelli, Luis S; Smedile, Francesco; Giuliano, Laura; Yakimov, Michail M</p> <p>2018-01-01</p> <p>Covering two-thirds of our planet, the global deep ocean plays a central role in supporting life on Earth. Among other processes, this biggest ecosystem buffers the rise of atmospheric <span class="hlt">CO</span> <span class="hlt">2</span> . Despite carbon sequestration in the deep ocean has been known for a long time, microbial activity in the meso- and bathypelagic realm via the " assimilation of bicarbonate in the dark " (ABD) has only recently been described in more details. Based on recent findings, this process seems primarily the result of chemosynthetic and anaplerotic reactions driven by different groups of deep-<span class="hlt">sea</span> prokaryoplankton. We quantified bicarbonate assimilation in relation to total prokaryotic abundance, prokaryotic heterotrophic production and respiration in the meso- and bathypelagic Mediterranean <span class="hlt">Sea</span>. The measured ABD values, ranging from 133 to 370 μg C m -3 d -1 , were among the highest ones reported worldwide for similar depths, likely due to the elevated temperature of the deep Mediterranean <span class="hlt">Sea</span> (13-14°C also at abyssal depths). Integrated over the dark water column (≥200 m depth), bicarbonate assimilation in the deep-<span class="hlt">sea</span> ranged from 396 to 873 mg C m -<span class="hlt">2</span> d -1 . This quantity of produced de novo organic carbon amounts to about 85-424% of the phytoplankton primary production and covers up to 62% of deep-<span class="hlt">sea</span> prokaryotic total carbon demand. Hence, the ABD process in the meso- and bathypelagic Mediterranean <span class="hlt">Sea</span> might substantially contribute to the inorganic and organic pool and significantly sustain the deep-<span class="hlt">sea</span> microbial food web. To elucidate the ABD key-players, we established three actively nitrifying and <span class="hlt">CO</span> <span class="hlt">2</span> -fixing prokaryotic enrichments. Consortia were characterized by the <span class="hlt">co</span>-occurrence of chemolithoautotrophic Thaumarchaeota and chemoheterotrophic proteobacteria. One of the enrichments, originated from Ionian bathypelagic waters (3,000 m depth) and supplemented with low concentrations of ammonia, was dominated by the Thaumarchaeota "low-ammonia-concentration" deep-<span class="hlt">sea</span> ecotype</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5780414','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5780414"><span>Contribution of Bicarbonate Assimilation to Carbon Pool Dynamics in the Deep Mediterranean <span class="hlt">Sea</span> and Cultivation of Actively Nitrifying and <span class="hlt">CO</span><span class="hlt">2</span>-Fixing Bathypelagic Prokaryotic Consortia</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>La Cono, Violetta; Ruggeri, Gioachino; Azzaro, Maurizio; Crisafi, Francesca; Decembrini, Franco; Denaro, Renata; La Spada, Gina; Maimone, Giovanna; Monticelli, Luis S.; Smedile, Francesco; Giuliano, Laura; Yakimov, Michail M.</p> <p>2018-01-01</p> <p>Covering two-thirds of our planet, the global deep ocean plays a central role in supporting life on Earth. Among other processes, this biggest ecosystem buffers the rise of atmospheric <span class="hlt">CO</span><span class="hlt">2</span>. Despite carbon sequestration in the deep ocean has been known for a long time, microbial activity in the meso- and bathypelagic realm via the “assimilation of bicarbonate in the dark” (ABD) has only recently been described in more details. Based on recent findings, this process seems primarily the result of chemosynthetic and anaplerotic reactions driven by different groups of deep-<span class="hlt">sea</span> prokaryoplankton. We quantified bicarbonate assimilation in relation to total prokaryotic abundance, prokaryotic heterotrophic production and respiration in the meso- and bathypelagic Mediterranean <span class="hlt">Sea</span>. The measured ABD values, ranging from 133 to 370 μg C m−3 d−1, were among the highest ones reported worldwide for similar depths, likely due to the elevated temperature of the deep Mediterranean <span class="hlt">Sea</span> (13–14°C also at abyssal depths). Integrated over the dark water column (≥200 m depth), bicarbonate assimilation in the deep-<span class="hlt">sea</span> ranged from 396 to 873 mg C m−<span class="hlt">2</span> d−1. This quantity of produced de novo organic carbon amounts to about 85–424% of the phytoplankton primary production and covers up to 62% of deep-<span class="hlt">sea</span> prokaryotic total carbon demand. Hence, the ABD process in the meso- and bathypelagic Mediterranean <span class="hlt">Sea</span> might substantially contribute to the inorganic and organic pool and significantly sustain the deep-<span class="hlt">sea</span> microbial food web. To elucidate the ABD key-players, we established three actively nitrifying and <span class="hlt">CO</span><span class="hlt">2</span>-fixing prokaryotic enrichments. Consortia were characterized by the <span class="hlt">co</span>-occurrence of chemolithoautotrophic Thaumarchaeota and chemoheterotrophic proteobacteria. One of the enrichments, originated from Ionian bathypelagic waters (3,000 m depth) and supplemented with low concentrations of ammonia, was dominated by the Thaumarchaeota “low-ammonia-concentration” deep-<span class="hlt">sea</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1224862-role-additives-composite-pei-oxide-co2-adsorbents-enhancement-amine-efficiency-supported-pei-peg-co2-capture-from-simulated-ambient-air','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1224862-role-additives-composite-pei-oxide-co2-adsorbents-enhancement-amine-efficiency-supported-pei-peg-co2-capture-from-simulated-ambient-air"><span>Role of Additives in Composite PEI/Oxide <span class="hlt">CO</span> <span class="hlt">2</span> Adsorbents: Enhancement in the Amine Efficiency of Supported PEI by PEG in <span class="hlt">CO</span> <span class="hlt">2</span> Capture from Simulated Ambient <span class="hlt">Air</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Sakwa-Novak, Miles A.; Tan, Shuai; Jones, Christopher W.</p> <p>2015-10-20</p> <p>Supported amines are promising candidate adsorbents for the removal of <span class="hlt">CO</span> <span class="hlt">2</span> from flue gases and directly from ambient <span class="hlt">air</span>. The incorporation of additives into polymeric amines such as poly(ethylenimine) (PEI) supported on mesoporous oxides is an effective strategy to improve the performance of the materials. Here, several practical aspects of this strategy are addressed with regards to direct <span class="hlt">air</span> capture. The influence of three additives (CTAB, PEG200, PEG1000) was systematically explored under dry simulated <span class="hlt">air</span> capture conditions (400 ppm of <span class="hlt">CO</span> <span class="hlt">2</span>, 30 °C). With SBA-15 as a model support for poly(ethylenimine) (PEI), the nature of the additive inducedmore » heterogeneities in the deposition of organic on the interior and exterior of the particles, an important consideration for future scale up to practical systems. The PEG200 additive increased the observed thermodynamic performance (~60% increase in amine efficiency) of the adsorbents regardless of the PEI content, while the other molecules had less positive effects. A threshold PEG200/PEI value was identified at which the diffusional limitations of <span class="hlt">CO</span> <span class="hlt">2</span> within the materials were nearly eliminated. The threshold PEG/PEI ratio may have physical origin in the interactions between PEI and PEG, as the optimal ratio corresponded to nearly equimolar OH/reactive (1°, <span class="hlt">2</span>°) amine ratios. As a result, the strategy is shown to be robust to the characteristics of the host support, as PEG200 improved the amine efficiency of PEI when supported on two varieties of mesoporous γ-alumina with PEI.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1224862-role-additives-composite-pei-oxide-co2-adsorbents-enhancement-amine-efficiency-supported-pei-peg-co2-capture-from-simulated-ambient-air','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1224862-role-additives-composite-pei-oxide-co2-adsorbents-enhancement-amine-efficiency-supported-pei-peg-co2-capture-from-simulated-ambient-air"><span>Role of Additives in Composite PEI/Oxide <span class="hlt">CO</span> <span class="hlt">2</span> Adsorbents: Enhancement in the Amine Efficiency of Supported PEI by PEG in <span class="hlt">CO</span> <span class="hlt">2</span> Capture from Simulated 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>Sakwa-Novak, Miles A.; Tan, Shuai; Jones, Christopher W.</p> <p></p> <p>Supported amines are promising candidate adsorbents for the removal of <span class="hlt">CO</span> <span class="hlt">2</span> from flue gases and directly from ambient <span class="hlt">air</span>. The incorporation of additives into polymeric amines such as poly(ethylenimine) (PEI) supported on mesoporous oxides is an effective strategy to improve the performance of the materials. Here, several practical aspects of this strategy are addressed with regards to direct <span class="hlt">air</span> capture. The influence of three additives (CTAB, PEG200, PEG1000) was systematically explored under dry simulated <span class="hlt">air</span> capture conditions (400 ppm of <span class="hlt">CO</span> <span class="hlt">2</span>, 30 °C). With SBA-15 as a model support for poly(ethylenimine) (PEI), the nature of the additive inducedmore » heterogeneities in the deposition of organic on the interior and exterior of the particles, an important consideration for future scale up to practical systems. The PEG200 additive increased the observed thermodynamic performance (~60% increase in amine efficiency) of the adsorbents regardless of the PEI content, while the other molecules had less positive effects. A threshold PEG200/PEI value was identified at which the diffusional limitations of <span class="hlt">CO</span> <span class="hlt">2</span> within the materials were nearly eliminated. The threshold PEG/PEI ratio may have physical origin in the interactions between PEI and PEG, as the optimal ratio corresponded to nearly equimolar OH/reactive (1°, <span class="hlt">2</span>°) amine ratios. As a result, the strategy is shown to be robust to the characteristics of the host support, as PEG200 improved the amine efficiency of PEI when supported on two varieties of mesoporous γ-alumina with PEI.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ClDy...49.3851H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ClDy...49.3851H"><span>Effects of <span class="hlt">air-sea</span> coupling over the North <span class="hlt">Sea</span> and the Baltic <span class="hlt">Sea</span> on simulated summer precipitation over Central Europe</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ho-Hagemann, Ha Thi Minh; Gröger, Matthias; Rockel, Burkhardt; Zahn, Matthias; Geyer, Beate; Meier, H. E. Markus</p> <p>2017-12-01</p> <p>This study introduces a new approach to investigate the potential effects of <span class="hlt">air-sea</span> coupling on simulated precipitation inland over Central Europe. We present an inter-comparison of two regional climate models (RCMs), namely, the COSMO-CLM (hereafter CCLM) and RCA4 models, which are configured for the EURO-CORDEX domain in the coupled and atmosphere-only modes. Two versions of the CCLM model, namely, 4.8 and 5.0, join the inter-comparison being almost two different models while providing pronouncedly different summer precipitation simulations because of many changes in the dynamics and physics of CCLM in version 5.0. The coupling effect on the prominent summer dry bias over Central Europe is analysed using seasonal (JJA) mean statistics for the 30-year period from 1979 to 2009, with a focus on extreme precipitation under specific weather regimes. The weather regimes are compared between the coupled and uncoupled simulations to better understand the mechanism of the coupling effects. The comparisons of the coupled systems with the atmosphere-only models show that coupling clearly reduces the dry bias over Central Europe for CCLM 4.8, which has a large dry summer bias, but not for CCLM 5.0 and RCA4, which have smaller dry biases. This result implies that if the atmosphere-only model already yields reasonable summer precipitation over Central Europe, not much room for improvement exists that can be caused by the <span class="hlt">air-sea</span> coupling over the North <span class="hlt">Sea</span> and the Baltic <span class="hlt">Sea</span>. However, if the atmosphere-only model shows a pronounced summer dry bias because of a lack of moisture transport from the <span class="hlt">seas</span> into the region, the considered coupling may create an improved simulation of summer precipitation over Central Europe, such as for CCLM 4.8. For the latter, the benefit of coupling varies over the considered timescales. The precipitation simulations that are generated by the coupled system COSTRICE 4.8 and the atmosphere-only CCLM 4.8 are mostly identical for the summer mean</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A43D2493M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A43D2493M"><span>Remarkable separability of the circulation response to Arctic <span class="hlt">sea</span> ice loss and greenhouse gas forcing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>McCusker, K. E.; Kushner, P. J.; Fyfe, J. C.; Sigmond, M.; Kharin, V. V.; Bitz, C. M.</p> <p>2017-12-01</p> <p>Arctic <span class="hlt">sea</span> ice loss has an important effect on local climate through increases in ocean to atmosphere heat flux and associated feedbacks, and may influence midlatitude climate by changing large-scale circulation that can enhance or counter changes that are due to greenhouse gases. The extent to which climate change in a warming world can be understood as greenhouse gas-induced changes that are modulated by Arctic <span class="hlt">sea</span> ice loss depends on how additive the responses to the separate influences are. Here we use a novel <span class="hlt">sea</span> ice nudging methodology in the Canadian Earth System Model, which has a fully coupled ocean, to isolate the effects of Arctic <span class="hlt">sea</span> ice loss and doubled atmospheric carbon dioxide (<span class="hlt">CO</span><span class="hlt">2</span>) to determine their additivity and sensitivity to mean state. We find that the separate effects of Arctic <span class="hlt">sea</span> ice loss and doubled <span class="hlt">CO</span><span class="hlt">2</span> are remarkably additive and relatively insensitive to mean climate state. This separability is evident in several thermodynamic and dynamic fields throughout most of the year, from hemispheric to synoptic scales. The extent to which the regional response to <span class="hlt">sea</span> ice loss sometimes agrees with and sometimes cancels the response to <span class="hlt">CO</span><span class="hlt">2</span> is quantified. In this model, Arctic <span class="hlt">sea</span> ice loss enhances the <span class="hlt">CO</span><span class="hlt">2</span>-induced surface <span class="hlt">air</span> temperature changes nearly everywhere and zonal wind changes over the Pacific sector, whereas <span class="hlt">sea</span> ice loss counters <span class="hlt">CO</span><span class="hlt">2</span>-induced <span class="hlt">sea</span> level pressure changes nearly everywhere over land and zonal wind changes over the Atlantic sector. This separability of the response to Arctic <span class="hlt">sea</span> ice loss from the response to <span class="hlt">CO</span><span class="hlt">2</span> doubling gives credence to the body of work in which Arctic <span class="hlt">sea</span> ice loss is isolated from the forcing that modified it, and might provide a means to better interpret the diverse array of modeling and observational studies of Arctic change and influence.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006JChPh.124n4302H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006JChPh.124n4302H"><span>Vibrational and rotational energy <span class="hlt">transfers</span> involving the CH B <span class="hlt">2</span>Σ- v=1 vibrational level in collisions with Ar, <span class="hlt">CO</span>, and N<span class="hlt">2</span>O</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Huang, Hong-Yi; Tsai, Ming-Tsang; Lin, King-Chuen</p> <p>2006-04-01</p> <p>With photolysis-probe technique, we have studied vibrational and rotational energy <span class="hlt">transfers</span> of CH involving the B Σ-<span class="hlt">2</span> (v =1, 0⩽N⩽6, F) state by collisions with Ar, <span class="hlt">CO</span>, and N<span class="hlt">2</span>O. For the vibrational energy <span class="hlt">transfer</span> (VET) measurements, the time-resolved fluorescence of the B-X(0,0) band is monitored following the (1,0) band excitation. For the rotational energy <span class="hlt">transfer</span> (RET) measurements, the laser-induced fluorescence of the initially populated state is dispersed using a step-scan Fourier transform spectrometer. The time-resolved spectra obtained in the nanosecond regime may yield the RET information under a single pressure of the collider. The rate constants of intramolecular energy <span class="hlt">transfers</span> are evaluated with simulation of kinetic models. The VET lies in the range of 4×10-12to4×10-11cm3molecule-1s-1, with efficiency following the order of Ar <<span class="hlt">CO</span><N<span class="hlt">2</span>O, reflecting the average over Boltzmann rotational distribution. The RET rates are more rapid by one to two orders of magnitude, comparable to the gas kinetic, with the trend of Ar <<span class="hlt">CO</span><N<span class="hlt">2</span>O. The <span class="hlt">transfer</span> rates decrease with increasing N and ΔN, proceeding via the ΔN =-1 transitions slightly larger than ΔN =+1. With the fine-structure labels resolved up to N =6, the fine-structure-conserving collisions prevail increasingly with increasing N in ΔN ≠0. The rate constants for the F<span class="hlt">2</span>→F1 transitions are larger than the reverse F1→F<span class="hlt">2</span> transitions in ΔN =0 for the Ar and <span class="hlt">CO</span> collisions. The trend of fine-structure conservation is along the order of N<span class="hlt">2</span>O<CO˜Ar. For the CH-Ar collisions, the fine-structure conservation is less pronounced as compared with the v =0 level reported previously. In general, the propensity rules obeyed in the v =0 collision with Ar are valid in v =1, but the latter case shows a weaker tendency. It might be caused by the anisotropy difference of interaction potential when vibrational excitation is considered. For the polyatomic collider, the strong long-range dipole-dipole interaction</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1346208-mechanistic-study-co-photoreduction-cu-tio-nanocomposites-situ-ray-absorption-infrared-spectroscopies','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1346208-mechanistic-study-co-photoreduction-cu-tio-nanocomposites-situ-ray-absorption-infrared-spectroscopies"><span>Mechanistic Study of <span class="hlt">CO</span> <span class="hlt">2</span> Photoreduction with H <span class="hlt">2</span> O on Cu/TiO <span class="hlt">2</span> Nanocomposites by in Situ X-ray Absorption and Infrared Spectroscopies</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>Liu, Lianjun; Zhao, Cunyu; Miller, Jeffrey T.</p> <p>2016-12-15</p> <p>Cu/TiO<span class="hlt">2</span> composites are extensively studied for photocatalytic reduction of <span class="hlt">CO</span><span class="hlt">2</span> with H<span class="hlt">2</span>O, but the roles of Cu species (Cu<span class="hlt">2</span>+, Cu+, or Cu0) is not well understood, and the photocatalyst deactivation mechanism is seldom addressed. In this work, we have employed in situ techniques, i.e., X-ray absorption spectroscopy (XAS) and diffuse reflectance infrared Fourier transform spectroscopy (DRIFTS), to explore the surface chemistry of Cu/TiO<span class="hlt">2</span> composites under <span class="hlt">CO</span><span class="hlt">2</span> photoreduction environment. We found that the <span class="hlt">air</span>-calcined Cu/TiO<span class="hlt">2</span> (Cu/Ti(<span class="hlt">air</span>)) surface was dominated by isolated Cu<span class="hlt">2</span>+ sites, while the one post-treated with H<span class="hlt">2</span> at 200 °C (Cu/Ti(H<span class="hlt">2</span>)) was rich in Cu+ and oxygen vacancy (VO).more » Cu/Ti(H<span class="hlt">2</span>) showed more than 50% higher activity than Cu/Ti(<span class="hlt">air</span>) for <span class="hlt">CO</span><span class="hlt">2</span> photoreduction to <span class="hlt">CO</span>, mainly resulting from the synergy of Cu+, OH groups, and VO that could scavenge holes to enhance electron <span class="hlt">transfer</span>, provide <span class="hlt">CO</span><span class="hlt">2</span> adsorption sites, and facilitate the activation and conversion of the adsorbed <span class="hlt">CO</span><span class="hlt">2</span> (HCO3– and <span class="hlt">CO</span><span class="hlt">2</span>–). Meanwhile, the consumption of OH groups and Cu+ active sites by holes may result in the deactivation of Cu/Ti(H<span class="hlt">2</span>). Moreover, in situ XAS results directly demonstrated that (1) the photoinduced oxidation of Cu+ to Cu<span class="hlt">2</span>+ changed the surrounding environments of Cu by increasing the coordination number; (<span class="hlt">2</span>) thermal treatment by H<span class="hlt">2</span> could not fully recover the OH and Cu+ sites to their original states; and (3) adding hole scavengers (e.g., methanol) maintained or even increased the more active Cu+ species from the photoreduction of Cu<span class="hlt">2</span>+, thus leading to a higher and more stable <span class="hlt">CO</span><span class="hlt">2</span> reduction activity. Findings in this work and the application of in situ XAS technique will help develop a more efficient photocatalyst for <span class="hlt">CO</span><span class="hlt">2</span> photoreduction and advance the understanding of the reaction mechanism and surface chemistry.« less</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 exchange</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>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> exchange. <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 exchange 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 exchange.</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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