Sample records for air sea fluxes

  1. Observational analysis of air-sea fluxes and sea water temperature offshore South China Sea

    NASA Astrophysics Data System (ADS)

    Bi, X.; Huang, J.; Gao, Z.; Liu, Y.

    2017-12-01

    This paper investigates the air-sea 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 Sea from January 2009 to December 2016 and sea 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 sea averages about 15 m. This study presents the in-situ measurements of continuous air-sea fluxes and SWT at different depths. Seasonal and diurnal variations in air-sea fluxes and SWT on different depths are examined. Results show that air-sea fluxes and all SWT changed seasonally; sea-land breeze circulation appears all the year round. Unlike winters where SWT on different depths are fairly consistent, the difference between sea surface temperature (SST) and sea temperature at 10 m water depth fluctuates dramatically and the maximum value reaches 7 °C during summer.

  2. Variability of the gaseous elemental mercury sea-air flux of the Baltic Sea.

    PubMed

    Kuss, Joachim; Schneider, Bernd

    2007-12-01

    The importance of the sea 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 sea areas. The concentration of elemental mercury (Hg0) in sea surface water and in the marine atmosphere of the Baltic Sea was measured at high spatial resolution in February, April, July, and November 2006. Wind-speed records and the gas-exchange transfer velocity were then used to calculate Hg0 sea-air fluxes on the basis of Hg0 sea-air 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 air equilibrated with water instead of quantitative extraction of Hg0 from seawater samples. A spatial and highly seasonal variability of the Hg0 sea-air 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(-2) day(-1) in the central Baltic Sea was recorded. The total emission of Hg0 from the studied area (235000 km2) was 4300 +/- 1600 kg in 2006 and exceeded deposition estimates.

  3. Intercomparison of Air-Sea Fluxes in the Bay of Bengal

    NASA Astrophysics Data System (ADS)

    Buckley, J.; Weller, R. A.; Farrar, J. T.; Tandon, A.

    2016-02-01

    Heat and momentum exchange between the air and sea in the Bay of Bengal is an important driver of atmospheric convection during the Asian Monsoon. Warm sea surface temperatures resulting from salinity stratified shallow mixed layers trigger widespread showers and thunderstorms. In this study, we compare atmospheric reanalysis flux products to air-sea flux values calculated from shipboard observations from four cruises and an air-sea flux mooring in the Bay of Bengal as part of the Air-Sea 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 air-sea flux mooring reveals significant errors on shorter timescales (2-4 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 air 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 air can reduce net heat into the ocean for minutes to a few days, significantly effecting air-sea heat transfer, upper ocean stratification, and ocean surface temperature and salinity.

  4. On the physical air-sea fluxes for climate modeling

    NASA Astrophysics Data System (ADS)

    Bonekamp, J. G.

    2001-02-01

    At the sea 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 air-sea 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 air-sea fluxes are generated. A good example is the 15-year atmospheric reanalysis of the European Centre for Medium--Range Weather Forecasts (ECMWF). Air-sea 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 air-sea 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 air-sea 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

  5. Wintertime Air-Sea Gas Transfer Rates and Air Injection Fluxes at Station Papa in the NE Pacific

    NASA Astrophysics Data System (ADS)

    McNeil, C.; Steiner, N.; Vagle, S.

    2008-12-01

    In recent studies of air-sea fluxes of N2 and O2 in hurricanes, McNeil and D'Asaro (2007) used a simplified model formulation of air-sea gas flux to estimate simultaneous values of gas transfer rate, KT, and air injection flux, VT. The model assumes air-sea gas fluxes at high to extreme wind speeds can be explained by a combination of two processes: 1) air injection, by complete dissolution of small bubbles drawn down into the ocean boundary layer by turbulent currents, and 2) near-surface equilibration processes, such as occurs within whitecaps. This analysis technique relies on air-sea gas flux estimates for two gases, N2 and O2, 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.

  6. Sea spray contributions to the air-sea fluxes at moderate and hurricane wind speeds

    NASA Astrophysics Data System (ADS)

    Mueller, J. A.; Veron, F.

    2009-12-01

    At sufficiently high wind speed conditions, the surface of the ocean separates to form a substantial number of sea spray drops, which can account for a significant fraction of the total air-sea surface area and thus make important contributions to the aggregate air-sea 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 transfer between the drops and the atmosphere. While the latter factor can be estimated from an established, physically-based theory, the estimates for the former two are not well established. Using a recent, physically-based model of the sea 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 air-sea fluxes at high wind speeds as well as the development and sustainment of hurricanes.

  7. 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.

  8. 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

  9. Air-sea exchange fluxes of synthetic polycyclic musks in the North Sea and the Arctic.

    PubMed

    Xie, Zhiyong; Ebinghaus, Ralf; Temme, Christian; Heemken, Olaf; Ruck, Wolfgang

    2007-08-15

    Synthetic polycyclic musk fragrances Galaxolide (HHCB) and Tonalide (AHTN) were measured simultaneously in air and seawater in the Arctic and the North Sea and in the rural air 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 Sea, 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 27.2 and 14.2 ng m(-2) day(-1) and the depositional fluxes were 5.9 and 3.3 ng m(-2) day(-1), respectively, indicating water-to-air volatilization is a significant process to eliminate HHCB and AHTN from the North Sea. In the Arctic, deposition fluxes dominated the air-sea gas exchange of HHCB and AHTN, suggesting atmospheric input controls the levels of HHCB and AHTN in the polar region.

  10. Seasonal Oxygen Supersaturation and Air-Sea Fluxes from Profiling Floats in the Pacific

    NASA Astrophysics Data System (ADS)

    Bushinsky, S. M.; Emerson, S. R.

    2016-02-01

    The Pacific Ocean is a heterogeneous basin that includes regions of strong CO2 fluxes to and from the atmosphere. The Kuroshio Extension (KE) is a current associated with the largest CO2 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 O2 and dissolved inorganic carbon during photosynthesis and respiration may allow in situ O2 measurements to help determine the processes driving this large CO2 flux. In this study, we used Argo profiling floats with modified oxygen sensors to estimate O2 fluxes in several areas of the Pacific. In situ air calibrations of these sensors allowed us to accurately measure air-sea O2 differences, which largely control the flux of O2 to and from the atmosphere. In this way, we determine air-sea O2 fluxes from profiling floats, which previously did not measure O2 accurately enough to make these calculations. To characterize different areas within the KE, we separated O2 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 ΔO2 and air-sea flux. Mean annual air-sea oxygen fluxes (positive fluxes represent addition of O2 to the ocean) were calculated for the Alaska Gyre of -0.3 mol m-2 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-2 yr-1, respectively, and for the south subtropical Pacific (2014-2015) of 0.6 mol m-2 yr-1. The air-sea 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

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

    NASA Astrophysics Data System (ADS)

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

    2015-04-01

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

  12. Kinetic energy flux budget across air-sea interface

    NASA Astrophysics Data System (ADS)

    Fan, Yalin; Hwang, Paul

    2017-12-01

    The kinetic energy (KE) fluxes into subsurface currents (EFc) is an important boundary condition for ocean circulation models. Traditionally, numerical models assume the KE flux from wind (EFair) is identical to EFc, that is, no net KE is gained (or lost) by surface waves. This assumption, however, is invalid when the surface wave field is not fully developed, and acquires KE when it grows in space or time. In this study, numerical experiments are performed to investigate the KE flux budget across the air-sea interface under both uniform and idealized tropical cyclone (TC) winds. The wave fields are simulated using the WAVEWATCH III model under different wind forcing. The difference between EFair and EFc is estimated using an air-sea KE budget model. To address the uncertainty of these estimates resides in the variation of source functions, two source function packages are used for this study: the ST4 source package (Ardhuin et al, 2010), and the ST6 source package (Babanin, 2011). The modeled EFc is significantly reduced relative to EFair under growing seas for both the uniform and TC experiments. The reduction can be as large as 20%, and the variation of this ratio is highly dependent on the choice of source function for the wave model. Normalized EFc are found to be consistent with analytical expressions by Hwang and Sletten (2008) and Hwang and Walsh (2016) and field observations by Terray et al. (1996) and Drennan et al. (1996), while the scatters are more widely in the TC cases due to the complexity of the associated wave field. The waves may even give up KE to subsurface currents in the left rear quadrant of fast moving storms. Our results also suggest that the normalized KE fluxes may depend on both wave age and friction velocity (u*).

  13. Air-sea heat flux control on the Yellow Sea Cold Water Mass intensity and implications for its prediction

    NASA Astrophysics Data System (ADS)

    Zhu, Junying; Shi, Jie; Guo, Xinyu; Gao, Huiwang; Yao, Xiaohong

    2018-01-01

    The Yellow Sea Cold Water Mass (YSCWM), which occurs during summer in the central Yellow Sea, 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 Sea, 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, air-sea heat flux, wind, evaporation, precipitation and sea level pressure to those in the strong year of 1984, respectively. The results showed that the air-sea 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 air-sea 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 sea surface temperature before the cooling season and the air-sea 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

  14. Atmospheric deposition and air-sea gas exchange fluxes of DDT and HCH in the Yangtze River Estuary, East China Sea

    NASA Astrophysics Data System (ADS)

    Li, Zhongxia; Lin, Tian; Li, Yuanyuan; Jiang, Yuqing; Guo, Zhigang

    2017-07-01

    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 air-sea gas exchange fluxes of dichlorodiphenyltrichloroethane (DDT) and hexachlorocyclohexane (HCH) to determine whether the YRE is a sink or source of selected pesticides at the air-water interface under the influences of river input and atmospheric transport. The air-sea gas exchange of DDT was characterized by net volatilization with a marked difference in its fluxes between summer (140 ng/m2/d) and the other three seasons (12 ng/m2/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 air-sea gas exchange reached equilibrium because of low HCH levels in the air 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 air-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.

  15. Ocean Winds and Turbulent Air-Sea Fluxes Inferred From Remote Sensing

    NASA Technical Reports Server (NTRS)

    Bourassa, Mark A.; Gille, Sarah T.; Jackson, Daren L.; Roberts, J. Brent; Wick, Gary A.

    2010-01-01

    Air-sea 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 2). 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 CO Z ) is transferred across the air/sea 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.

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

    NASA Astrophysics Data System (ADS)

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

    2014-07-01

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

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

    NASA Astrophysics Data System (ADS)

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

    2015-07-01

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

  18. Oxygen in the Southern Ocean From Argo Floats: Determination of Processes Driving Air-Sea Fluxes

    NASA Astrophysics Data System (ADS)

    Bushinsky, Seth M.; Gray, Alison R.; Johnson, Kenneth S.; Sarmiento, Jorge L.

    2017-11-01

    The Southern Ocean is of outsized significance to the global oxygen and carbon cycles with relatively poor measurement coverage due to harsh winters and seasonal ice cover. In this study, we use recent advances in the parameterization of air-sea oxygen fluxes to analyze 9 years of oxygen data from a recalibrated Argo oxygen data set and from air-calibrated oxygen floats deployed as part of the Southern Ocean Carbon and Climate Observations and Modeling (SOCCOM) project. From this combined data set of 150 floats, we find a total Southern Ocean oxygen sink of -183 ± 80 Tmol yr-1 (positive to the atmosphere), greater than prior estimates. The uptake occurs primarily in the Polar-Frontal Antarctic Zone (PAZ, -94 ± 30 Tmol O2 yr-1) and Seasonal Ice Zone (SIZ, -111 ± 9.3 Tmol O2 yr-1). This flux is driven by wintertime ventilation, with a large portion of the flux in the SIZ passing through regions with fractional sea ice. The Subtropical Zone (STZ) is seasonally driven by thermal fluxes and exhibits a net outgassing of 47 ± 29 Tmol O2 yr-1 that is likely driven by biological production. The Subantarctic Zone (SAZ) uptake is -25 ± 12 Tmol O2 yr-1. Total oxygen fluxes were separated into a thermal and nonthermal component. The nonthermal flux is correlated with net primary production and mixed layer depth in the STZ, SAZ, and PAZ, but not in the SIZ where seasonal sea ice slows the air-sea gas flux response to the entrainment of deep, low-oxygen waters.

  19. Changes in ocean circulation and carbon storage are decoupled from air-sea CO2 fluxes

    NASA Astrophysics Data System (ADS)

    Marinov, I.; Gnanadesikan, A.

    2011-02-01

    The spatial distribution of the air-sea 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 air-sea 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.

  20. Changes in ocean circulation and carbon storage are decoupled from air-sea CO2 fluxes

    NASA Astrophysics Data System (ADS)

    Marinov, I.; Gnanadesikan, A.

    2010-11-01

    The spatial distribution of the air-sea 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 air-sea 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.

  1. Sustained Observations of Air-Sea Fluxes and Air-Sea Interaction at the Stratus Ocean Reference Station

    NASA Astrophysics Data System (ADS)

    Weller, Robert

    2014-05-01

    Since October 2000, a well-instrumented surface mooring has been maintained some 1,500 km west of the coast of northern Chile, roughly in the location of the climatological maximum in marine stratus clouds. Statistically significant increases in wind stress and decreases in annual net air-sea heat flux and in latent heat flux have been observed. If the increased oceanic heat loss continues, the region will within the next decade change from one of net annual heat gain by the ocean to one of neat annual heat loss. Already, annual evaporation of about 1.5 m of sea water a year acts to make the warm, salty surface layer more dense. Of interest is examining whether or not increased oceanic heat loss has the potential to change the structure of the upper ocean and potentially remove the shallow warm, salty mixed layer that now buffers the atmosphere from the interior ocean. Insights into how that warm, shallow layer is formed and maintained come from looking at oceanic response to the atmosphere at diurnal tie scales. Restratification each spring and summer is found to depend upon the occurrence of events in which the trade winds decay, allowing diurnal warming in the near-surface ocean to occur, and when the winds return resulting in a net upward step in sea surface temperature. This process is proving hard to accurately model.

  2. Response of air-sea carbon fluxes and climate to orbital forcing changes in the Community Climate System Model

    NASA Astrophysics Data System (ADS)

    Jochum, M.; Peacock, S.; Moore, K.; Lindsay, K.

    2010-07-01

    A global general circulation model coupled to an ocean ecosystem model is used to quantify the response of carbon fluxes and climate to changes in orbital forcing. Compared to the present-day simulation, the simulation with the Earth's orbital parameters from 115,000 years ago features significantly cooler northern high latitudes but only moderately cooler southern high latitudes. This asymmetry is explained by a 30% reduction of the strength of the Atlantic Meridional Overturning Circulation that is caused by an increased Arctic sea ice export and a resulting freshening of the North Atlantic. The strong northern high-latitude cooling and the direct insolation induced tropical warming lead to global shifts in precipitation and winds to the order of 10%-20%. These climate shifts lead to regional differences in air-sea carbon fluxes of the same order. However, the differences in global net air-sea carbon fluxes are small, which is due to several effects, two of which stand out: first, colder sea surface temperature leads to a more effective solubility pump but also to increased sea ice concentration which blocks air-sea exchange, and second, the weakening of Southern Ocean winds that is predicted by some idealized studies occurs only in part of the basin, and is compensated by stronger winds in other parts.

  3. Distribution and sea-to-air flux of isoprene in the East China Sea and the South Yellow Sea during summer.

    PubMed

    Li, Jian-Long; Zhang, Hong-Hai; Yang, Gui-Peng

    2017-07-01

    Spatial distribution and sea-to-air flux of isoprene in the East China Sea and the South Yellow Sea in July 2013 were investigated. This study is the first to report the concentrations of isoprene in the China marginal seas. 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, sea-to-air fluxes of isoprene approximately ranged from 22.17 nmol m -2  d -1 -537.2 nmol m -2  d -1 , with an average of 161.5 ± 133.3 nmol m -2  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.

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

    NASA Astrophysics Data System (ADS)

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

    2018-03-01

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

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

    NASA Astrophysics Data System (ADS)

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

    2016-09-01

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

  7. CLIVAR-GSOP/GODAE Ocean Synthesis Inter-Comparison of Global Air-Sea Fluxes From Ocean and Coupled Reanalyses

    NASA Astrophysics Data System (ADS)

    Valdivieso, Maria

    2014-05-01

    The GODAE OceanView and CLIVAR-GSOP ocean synthesis program has been assessing the degree of consistency between global air-sea flux data sets obtained from ocean or coupled reanalyses (Valdivieso et al., 2014). So far, fifteen global air-sea heat flux products obtained from ocean or coupled reanalyses have been examined: seven are from low-resolution ocean reanalyses (BOM PEODAS, ECMWF ORAS4, JMA/MRI MOVEG2, JMA/MRI MOVECORE, Hamburg Univ. GECCO2, JPL ECCOv4, and NCEP GODAS), five are from eddy-permitting ocean reanalyses developed as part of the EU GMES MyOcean program (Mercator GLORYS2v1, Reading Univ. UR025.3, UR025.4, UKMO GloSea5, and CMCC C-GLORS), and the remaining three are couple reanalyses based on coupled climate models (JMA/MRI MOVE-C, GFDL ECDA and NCEP CFSR). The global heat closure in the products over the period 1993-2009 spanned by all data sets is presented in comparison with observational and atmospheric reanalysis estimates. Then, global maps of ensemble spread in the seasonal cycle, and of the Signal to Noise Ratio of interannual flux variability over the 17-yr common period are shown to illustrate the consistency between the products. We have also studied regional variability in the products, particularly at the OceanSITES project locations (such as, for instance, the TAO/TRITON and PIRATA arrays in the Tropical Pacific and Atlantic, respectively). Comparisons are being made with other products such as OAFlux latent and sensible heat fluxes (Yu et al., 2008) combined with ISCCP satellite-based radiation (Zhang et al., 2004), the ship-based NOC2.0 product (Berry and Kent, 2009), the Large and Yeager (2009) hybrid flux dataset CORE.2, and two atmospheric reanalysis products, the ECMWF ERA-Interim reanalysis (referred to as ERAi, Dee et al., 2011) and the NCEP/DOE reanalysis R2 (referred to as NCEP-R2, Kanamitsu et al., 2002). Preliminary comparisons with the observational flux products from OceanSITES are also underway. References Berry, D

  8. Predicting the Turbulent Air-Sea Surface Fluxes, Including Spray Effects, from Weak to Strong Winds

    DTIC Science & Technology

    2012-09-30

    almost complete decoupling of the wind field from the sea surface . As a result of the weak surface stress, the flow becomes almost free from the...shore flow . In turn, wave growth and the associated surface roughness (z0) are limited. Consequently, the stability increases further in a...1 DISTRIBUTION STATEMENT A. Approved for public release; distribution is unlimited. Predicting the Turbulent Air-Sea Surface Fluxes

  9. Motion-Correlated Flow Distortion and Wave-Induced Biases in Air-Sea Flux Measurements From Ships

    NASA Astrophysics Data System (ADS)

    Prytherch, J.; Yelland, M. J.; Brooks, I. M.; Tupman, D. J.; Pascal, R. W.; Moat, B. I.; Norris, S. J.

    2016-02-01

    Direct measurements of the turbulent air-sea fluxes of momentum, heat, moisture and gases are often made using sensors mounted on ships. Ship-based turbulent wind measurements are corrected for platform motion using well established techniques, but biases at scales associated with wave and platform motion are often still apparent in the flux measurements. It has been uncertain whether this signal is due to time-varying distortion of the air flow over the platform, or to wind-wave interactions impacting the turbulence. Methods for removing such motion-scale biases from scalar measurements have previously been published but their application to momentum flux measurements remains controversial. Here we use eddy covariance momentum flux measurements obtained onboard RRS James Clark Ross as part of the Waves, Aerosol and Gas Exchange Study (WAGES), a programme of near-continuous measurements using the autonomous AutoFlux system (Yelland et al., 2009). Measurements were made in 2013 in locations throughout the North and South Atlantic, the Southern Ocean and the Arctic Ocean, at latitudes ranging from 62°S to 75°N. We show that the measured motion-scale bias has a dependence on the horizontal ship velocity, and that a correction for it reduces the dependence of the measured momentum flux on the orientation of the ship to the wind. We conclude that the bias is due to experimental error, and that time-varying motion-dependent flow distortion is the likely source. Yelland, M., Pascal, R., Taylor, P. and Moat, B.: AutoFlux: an autonomous system for the direct measurement of the air-sea fluxes of CO2, heat and momentum. J. Operation. Oceanogr., 15-23, doi:10.1080/1755876X.2009.11020105, 2009.

  10. Field Observations of Coastal Air-Sea Interaction

    NASA Astrophysics Data System (ADS)

    Ortiz-Suslow, D. G.; Haus, B. K.; Williams, N. J.; Graber, H. C.

    2016-12-01

    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 air-sea interface. For decades, the focus of air-sea 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 air-sea gas flux. The results from a recent study conducted at the New River Inlet in North Carolina showed that directly measured air-sea 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 air-sea fluxes. Preliminary findings show that interactions between the local wind-sea 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-air-sea interactions will also be investigated.

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

    NASA Astrophysics Data System (ADS)

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

    2015-12-01

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

  12. Air-sea fluxes of momentum and mass in the presence of wind waves

    NASA Astrophysics Data System (ADS)

    Zülicke, Christoph

    2010-05-01

    An air-sea interaction model (ASIM) is developed including the effect of wind waves on momentum and mass transfer. This includes the derivation of profiles of dissipation rate, flow speed and concentration from a certain height to a certain depth. Simplified assumptions on the turbulent closure, skin - bulk matching and the spectral wave model allow for an analytic treatment. Particular emphasis was put on the inclusion of primary (gravity) waves and secondary (capillary-gravity) waves. The model was tuned to match wall-flow theory and data on wave height and slope. Growing waves reduce the air-side turbulent stress and lead to an increasing drag coefficient. In the sea, breaking waves inject turbulent kinetic energy and accelerate the transfer. Cross-reference with data on wave-related momentum and energy flux, dissipation rate and transfer velocity was sufficient. The evaluation of ASIM allowed for the analytical calculation of bulk formulae for the wind-dependent gas transfer velocity including information on the air-side momentum transfer (drag coefficient) and the sea-side gas transfer (Dalton number). The following regimes have been identified: the smooth waveless regime with a transfer velocity proportional to (wind) × (diffusion)2-3, the primary wave regime with a wind speed dependence proportional to (wind)1-4 × (diffusion)1-2-(waveage)1-4 and the secondary wave regime including a more-than-linear wind speed dependence like (wind)15-8 × (diffusion)1-2 × (waveage)5-8. These findings complete the current understanding of air-sea interaction for medium winds between 2 and 20 m s^-1.

  13. Air-sea heat exchange, an element of the water cycle

    NASA Technical Reports Server (NTRS)

    Chahine, M. T.

    1984-01-01

    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 air-sea interface, which are also important elements of air-sea interaction studies. The overall aim of air-sea 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 air-sea exchanges involve a large number of physica, chemical and dynamical processes including heat flux, radiation, sea-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.

  14. Enhanced Ahead-of-Eye TC Coastal Ocean Cooling Processes and their Impact on Air-Sea Heat Fluxes and Storm Intensity

    NASA Astrophysics Data System (ADS)

    Seroka, G. N.; Miles, T. N.; Glenn, S. M.; Xu, Y.; Forney, R.; Roarty, H.; Schofield, O.; Kohut, J. T.

    2016-02-01

    Any landfalling tropical cyclone (TC) must first traverse the coastal ocean. TC research, however, has focused over the deep ocean, where TCs typically spend the vast majority of their lifetime. This paper will show that the ocean's response to TCs can be different between deep and shallow water, and that the additional shallow water processes must be included in coupled models for accurate air-sea flux treatment and TC intensity prediction. The authors will present newly observed coastal ocean processes that occurred in response to Hurricane Irene (2011), due to the presence of a coastline, an ocean bottom, and highly stratified conditions. These newly observed processes led to enhanced ahead-of-eye SST cooling that significantly impacted air-sea heat fluxes and Irene's operationally over-predicted storm intensity. Using semi-idealized modeling, we find that in shallow water in Irene, only 6% of cooling due to air-sea heat fluxes, 17% of cooling due to 1D vertical mixing, and 50% of cooling due to all processes (1D mixing, air-sea heat fluxes, upwelling, and advection) occurred ahead-of-eye—consistent with previous studies. Observations from an underwater glider and buoys, however, indicated 75-100% of total SST cooling over the continental shelf was ahead-of-eye. Thus, the new coastal ocean cooling processes found in this study must occur almost completely ahead-of-eye. We show that Irene's intense cooling was not captured by basic satellite SST products and coupled ocean-atmosphere hurricane models, and that including the cooling in WRF modeling mitigated the high bias in model predictions. Finally, we provide evidence that this SST cooling—not track, wind shear, or dry air intrusion—was the key missing contribution to Irene's decay just prior to NJ landfall. Ongoing work is exploring the use of coupled WRF-ROMS modeling in the coastal zone.

  15. Characterization of extreme air-sea turbulent fluxes

    NASA Astrophysics Data System (ADS)

    Gulev, Sergey; Belyaev, Konstantin

    2017-04-01

    Extreme ocean-atmosphere turbulent fluxes play a critical role in the convective processes in the mid and subpolar latitudes and may also affect a variety of atmospheric processes, such as generation and re-intensification of extreme cyclones in the areas of the mid latitude storm tracks. From the ocean dynamics perspective, specifically for quantifying extreme vertical mixing, characterization of the extreme fluxes requires, besides estimation of the extreme events, also consideration of the relative extremeness of surface fluxes and their timing, e.g. the duration of periods of high surface fluxes. In order to comprehensively characterize extreme turbulent fluxes at sea surface we propose a formalism based upon probability density distributions of surface turbulent fluxes and flux-related variables. Individual absolute flux extremes were derived using Modified Fisher-Tippett (MFT) distribution of turbulent fluxes. Then, we extend this distribution to the fractional distribution, characterizing the fraction of time-integrated turbulent heat flux provided by the fluxes exceeding a given percentile. Finally, we consider the time durations during which fluxes of a given intensity provide extreme accumulations of heat loss from the surface. For estimation of these characteristics of surface fluxes we use fluxes recomputed from the state variables available from modern era reanalyses (ERA-Interim, MERRA and CFSR) for the period from 1979 onwards. Applications of the formalism to the VOS (Voluntary Observing Ship) - based surface fluxes are also considered. We discuss application of the new metrics of mesoscale and synoptic variability of surface fluxes to the dynamics of mixed layer depth in the North Atlantic.

  16. Distribution and sea-to-air fluxes of volatile halocarbons in the Bohai Sea and North Yellow Sea during spring.

    PubMed

    He, Zhen; Liu, Qiu-Lin; Zhang, Ying-Jie; Yang, Gui-Peng

    2017-04-15

    Concentrations of volatile halocarbons (VHCs), such as CHBr 2 Cl, CHBr 3 , C 2 HCl 3 , and C 2 Cl 4 , in the Bohai Sea (BS) and North Yellow Sea (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 sea. 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 sea-to-air fluxes of CHBr 2 Cl, CHBr 3 , C 2 HCl 3 , and C 2 Cl 4 in the study area were estimated to be 47.17, 56.63, 162.56, and 104.37nmolm -2 d -1 , respectively, indicating that the investigated area may be a source of atmospheric CHBr 2 Cl, CHBr 3 , C 2 HCl 3 , and C 2 Cl 4 in spring. Copyright © 2017 Elsevier B.V. All rights reserved.

  17. An assessment of TropFlux and NCEP air-sea fluxes on ROMS simulations over the Bay of Bengal region

    NASA Astrophysics Data System (ADS)

    Dey, Dipanjan; Sil, Sourav; Jana, Sudip; Pramanik, Saikat; Pandey, P. C.

    2017-12-01

    This study presents an assessment of the TropFlux and the National Centers for Environmental Prediction (NCEP) reanalysis air-sea fluxes in simulating the surface and subsurface oceanic parameters over the Bay of Bengal (BoB) region during 2002-2014 using the Regional Ocean Modelling System (ROMS). The assessment has been made by comparing the simulated fields with in-situ and satellite observations. The simulated surface and subsurface temperatures in the TropFlux forced experiment (TropFlux-E) show better agreement with the Research Moored Array for African-Asian-Australian Monsoon Analysis (RAMA) and Argo observations than the NCEP forced experiment (NCEP-E). The BoB domain averaged sea surface temperature (SST) simulated in the NCEP-E is consistently cooler than the satellite SST, with a root mean square error (RMSE) of 0.79 °C. Moreover, NCEP-E shows a limitation in simulating the observed seasonal cycle of the SST due to substantial underestimation of the pre-monsoon SST peak. These limitations are mostly due to the lower values of the NCEP net heat flux. The seasonal and interannual variations of SST in the TropFlux-E are better comparable to the observations with correlations and skills more than 0.80 and 0.90 respectively. However, SST is overestimated during summer monsoon periods mainly due to higher net heat flux. The superiority of TropFlux forcing over the NCEP reanalysis can also be seen when simulating the interannual variabilities of the magnitude and vertical extent of Wyrtki jets at two equatorial RAMA buoy locations. The jet is weaker in the NCEP-E relative to the TropFlux-E and observations. The simulated sea surface height anomalies (SSHA) from both the experiments are able to capture the regions of positive and negative SSHA with respect to satellite-derived altimeter data with better performance in the TropFlux-E. The speed of the westward propagating Rossby wave along 18°N in the TropFlux-E is found to be about 4.7 cm/s, which is close to

  18. Methanethiol Concentrations and Sea-Air Fluxes in the Subarctic NE Pacific Ocean

    NASA Astrophysics Data System (ADS)

    Kiene, R. P.; Williams, T. E.; Esson, K.; Tortell, P. D.; Dacey, J. W. H.

    2017-12-01

    Exchange of volatile organic sulfur from the ocean to the atmosphere impacts the global sulfur cycle and the climate system and is thought to occur mainly via the gas dimethylsulfide (DMS). DMS is produced during degradation of the abundant phytoplankton osmolyte dimethylsulfoniopropionate (DMSP) but bacteria can also convert dissolved DMSP into the sulfur gas methanethiol (MeSH). MeSH has been difficult to measure in seawater because of its high chemical and biological reactivity and, thus, information on MeSH concentrations, distribution and sea-air fluxes is limited. We measured MeSH in the northeast subarctic Pacific Ocean in July 2016, along transects with strong phytoplankton abundance gradients. Water samples obtained with Niskin bottles were analyzed for MeSH by purge-and-trap gas chromatography. Depth profiles showed that MeSH concentrations were high near the surface and declined with depth. Surface waters (5 m depth) had an average MeSH concentration of 0.75 nM with concentrations reaching up to 3nM. MeSH concentrations were correlated (r = 0.47) with microbial turnover of dissolved DMSP which ranged up to 236 nM per day. MeSH was also correlated with total DMSP (r = 0.93) and dissolved DMS (r = 0.63), supporting the conclusion that DMSP was a major precursor of MeSH. Surface water MeSH:DMS concentration ratios averaged 0.19 and ranged up to 0.50 indicating that MeSH was a significant fraction of the volatile sulfur pool in surface waters. Sea-air fluxes of MeSH averaged 15% of the combined DMS+MeSH flux, therefore MeSH contributed an important fraction of the sulfur emitted to the atmosphere from the subarctic NE Pacific Ocean.

  19. Interannual variability of primary production and air-sea CO2 flux in the Atlantic and Indian sectors of the Southern Ocean.

    NASA Astrophysics Data System (ADS)

    Dufour, Carolina; Merlivat, Liliane; Le Sommer, Julien; Boutin, Jacqueline; Antoine, David

    2013-04-01

    As one of the major oceanic sinks of anthropogenic CO2, 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 air-sea CO2 fluxes and how these processes might respond to climate change. It is well established that primary production is one of the major drivers of air-sea CO2 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 air-sea CO2 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 SeaWiFS 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 air-sea 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.

  20. Air-sea interactions during strong winter extratropical storms

    USGS Publications Warehouse

    Nelson, Jill; He, Ruoying; Warner, John C.; Bane, John

    2014-01-01

    A high-resolution, regional coupled atmosphere–ocean model is used to investigate strong air–sea 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 sea 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, sea level pressure, 10 m air temperature, and sea surface temperature time series, as well as a comparison between the model and one glider transect. Vertical profiles of modeled air 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–sea interactions near the Gulf Stream are important for generating and sustaining the ETC. In particular, locally enhanced winds over a warm sea (relative to the land temperature) induce large surface heat fluxes which cool the upper ocean by up to 2 °C, mainly during the cold air 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–sea interactions affecting momentum and buoyancy flux exchanges in ETCs need to be resolved accurately in a coupled atmosphere–ocean modeling framework.

  1. Carbon Dioxide Transfer Through Sea Ice: Modelling Flux in Brine Channels

    NASA Astrophysics Data System (ADS)

    Edwards, L.; Mitchelson-Jacob, G.; Hardman-Mountford, N.

    2010-12-01

    For many years sea ice was thought to act as a barrier to the flux of CO2 between the ocean and atmosphere. However, laboratory-based and in-situ observations suggest that while sea ice may in some circumstances reduce or prevent transfer (e.g. in regions of thick, superimposed multi-year ice), it may also be highly permeable (e.g. thin, first year ice) with some studies observing significant fluxes of CO2. Sea ice covered regions have been observed to act both as a sink and a source of atmospheric CO2 with the permeability of sea ice and direction of flux related to sea 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 sea ice and the surface ocean waters, they create a sink for CO2. Calcium carbonate (ikaite) precipitation in the sea ice is thought to enhance this process. Micro-organisms present within the sea ice will also contribute to the CO2 flux dynamics. Recent evidence of decreasing sea ice extent and the associated change from a multi-year ice to first-year ice dominated system suggest the potential for increased CO2 flux through regions of thinner, more porous sea ice. A full understanding of the processes and feedbacks controlling the flux in these regions is needed to determine their possible contribution to global CO2 levels in a future warming climate scenario. Despite the significance of these regions, the air-sea CO2 flux in sea 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 sea ice-air flux model. In our work we use the Los Alamos sea ice model, CICE, with a modification to incorporate the movement of CO2 through brine channels including the addition of DIC processes and ice algae production to

  2. Accounting for observational uncertainties in the evaluation of low latitude turbulent air-sea fluxes simulated in a suite of IPSL model versions

    NASA Astrophysics Data System (ADS)

    Servonnat, Jerome; Braconnot, Pascale; Gainusa-Bogdan, Alina

    2015-04-01

    Turbulent momentum and heat (sensible and latent) fluxes at the air-sea interface are key components of the whole energetic of the Earth's climate and their good representation in climate models is of prime importance. In this work, we use the methodology developed by Braconnot & Frankignoul (1993) to perform a Hotelling T2 test on spatio-temporal fields (annual cycles). This statistic provides a quantitative measure accounting for an estimate of the observational uncertainty for the evaluation of low-latitude turbulent air-sea fluxes in a suite of IPSL model versions. The spread within the observational ensemble of turbulent flux data products assembled by Gainusa-Bogdan et al (submitted) is used as an estimate of the observational uncertainty for the different turbulent fluxes. The methodology holds on a selection of a small number of dominating variability patterns (EOFs) that are common to both the model and the observations for the comparison. Consequently it focuses on the large-scale variability patterns and avoids the possibly noisy smaller scales. The results show that different versions of the IPSL couple model share common large scale model biases, but also that there the skill on sea surface temperature is not necessarily directly related to the skill in the representation of the different turbulent fluxes. Despite the large error bars on the observations the test clearly distinguish the different merits of the different model version. The analyses of the common EOF patterns and related time series provide guidance on the major differences with the observations. This work is a first attempt to use such statistic on the evaluation of the spatio-temporal variability of the turbulent fluxes, accounting for an observational uncertainty, and represents an efficient tool for systematic evaluation of simulated air-seafluxes, considering both the fluxes and the related atmospheric variables. References Braconnot, P., and C. Frankignoul (1993), Testing Model

  3. Extreme air-sea surface turbulent fluxes in mid latitudes - estimation, origins and mechanisms

    NASA Astrophysics Data System (ADS)

    Gulev, Sergey; Natalia, Tilinina

    2014-05-01

    provide locally high winds and air-sea temperature gradients. For this purpose we linked characteristics of cyclone activity over the midlatitudinal oceans with the extreme surface turbulent heat fluxes. Cyclone tracks and parameters of cyclone life cycle (deepening rates, propagation velocities, life time and clustering) were derived from the same reanalyses using state of the art numerical tracking algorithm. The main questions addressed in this study are (i) through which mechanisms extreme surface fluxes are associated with cyclone activity? and (ii) which types of cyclones are responsible for forming extreme turbulent fluxes? Our analysis shows that extreme surface fluxes are typically associated not with cyclones themselves but rather with cyclone-anticyclone interaction zones. This implies that North Atlantic and North Pacific series of intense cyclones do not result in the anomalous surface fluxes. Alternatively, extreme fluxes are most frequently associated with blocking situations, particularly with the intensification of the Siberian and North American Anticyclones providing cold-air outbreaks over WBC regions.

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

    NASA Astrophysics Data System (ADS)

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

    2017-07-01

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

  5. The Influence of Air-Sea Fluxes on Atmospheric Aerosols During the Summer Monsoon Over the Tropical Indian Ocean

    NASA Astrophysics Data System (ADS)

    Zavarsky, Alex; Booge, Dennis; Fiehn, Alina; Krüger, Kirstin; Atlas, Elliot; Marandino, Christa

    2018-01-01

    During the summer monsoon, the western tropical Indian Ocean is predicted to be a hot spot for dimethylsulfide emissions, the major marine sulfur source to the atmosphere, and an important aerosol precursor. Other aerosol relevant fluxes, such as isoprene and sea spray, should also be enhanced, due to the steady strong winds during the monsoon. Marine air masses dominate the area during the summer monsoon, excluding the influence of continentally derived pollutants. During the SO234-2/235 cruise in the western tropical Indian Ocean from July to August 2014, directly measured eddy covariance DMS fluxes confirm that the area is a large source of sulfur to the atmosphere (cruise average 9.1 μmol m-2 d-1). The directly measured fluxes, as well as computed isoprene and sea spray fluxes, were combined with FLEXPART backward and forward trajectories to track the emissions in space and time. The fluxes show a significant positive correlation with aerosol data from the Terra and Suomi-NPP satellites, indicating a local influence of marine emissions on atmospheric aerosol numbers.

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

    NASA Astrophysics Data System (ADS)

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

    2013-04-01

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

  7. Modelling storm development and the impact when introducing waves, sea spray and heat fluxes

    NASA Astrophysics Data System (ADS)

    Wu, Lichuan; Rutgersson, Anna; Sahlée, Erik

    2015-04-01

    In high wind speed conditions, sea spray generated due to intensity breaking waves have big influence on the wind stress and heat fluxes. Measurements show that drag coefficient will decrease in high wind speed. Sea spray generation function (SSGF), an important term of wind stress parameterization in high wind speed, usually treated as a function of wind speed/friction velocity. In this study, we introduce a wave state depended SSGG and wave age depended Charnock number into a high wind speed wind stress parameterization (Kudryavtsev et al., 2011; 2012). The proposed wind stress parameterization and sea spray heat fluxes parameterization from Andreas et al., (2014) were applied to an atmosphere-wave coupled model to test on four storm cases. Compared with measurements from the FINO1 platform in the North Sea, the new wind stress parameterization can reduce the forecast errors of wind in high wind speed range, but not in low wind speed. Only sea spray impacted on wind stress, it will intensify the storms (minimum sea level pressure and maximum wind speed) and lower the air temperature (increase the errors). Only the sea spray impacted on the heat fluxes, it can improve the model performance on storm tracks and the air temperature, but not change much in the storm intensity. If both of sea spray impacted on the wind stress and heat fluxes are taken into account, it has the best performance in all the experiment for minimum sea level pressure and maximum wind speed and air temperature. Andreas, E. L., Mahrt, L., and Vickers, D. (2014). An improved bulk air-sea surface flux algorithm, including spray-mediated transfer. Quarterly Journal of the Royal Meteorological Society. Kudryavtsev, V. and Makin, V. (2011). Impact of ocean spray on the dynamics of the marine atmospheric boundary layer. Boundary-layer meteorology, 140(3):383-410. Kudryavtsev, V., Makin, V., and S, Z. (2012). On the sea-surface drag and heat/mass transfer at strong winds. Technical report, Royal

  8. On the role of sea-state in bubble-mediated air-sea gas flux during a winter storm

    NASA Astrophysics Data System (ADS)

    Liang, Jun-Hong; Emerson, Steven R.; D'Asaro, Eric A.; McNeil, Craig L.; Harcourt, Ramsey R.; Sullivan, Peter P.; Yang, Bo; Cronin, Meghan F.

    2017-04-01

    Oceanic bubbles play an important role in the air-sea exchange of weakly soluble gases at moderate to high wind speeds. A Lagrangian bubble model embedded in a large eddy simulation model is developed to study bubbles and their influence on dissolved gases in the upper ocean. The transient evolution of mixed-layer dissolved oxygen and nitrogen gases at Ocean Station Papa (50°N, 145°W) during a winter storm is reproduced with the model. Among different physical processes, gas bubbles are the most important in elevating dissolved gas concentrations during the storm, while atmospheric pressure governs the variability of gas saturation anomaly (the relative departure of dissolved gas concentration from the saturation concentration). For the same wind speed, bubble-mediated gas fluxes are larger during rising wind with smaller wave age than during falling wind with larger wave age. Wave conditions are the primary cause for the bubble gas flux difference: when wind strengthens, waves are less-developed with respect to wind, resulting in more frequent large breaking waves. Bubble generation in large breaking waves is favorable for a large bubble-mediated gas flux. The wave-age dependence is not included in any existing bubble-mediated gas flux parameterizations.

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

    NASA Astrophysics Data System (ADS)

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

    2016-12-01

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

  10. Sea-to-air flux of dimethyl sulfide in the South and North Pacific Ocean as measured by proton transfer reaction-mass spectrometry coupled with the gradient flux technique

    NASA Astrophysics Data System (ADS)

    Omori, Yuko; Tanimoto, Hiroshi; Inomata, Satoshi; Ikeda, Kohei; Iwata, Toru; Kameyama, Sohiko; Uematsu, Mitsuo; Gamo, Toshitaka; Ogawa, Hiroshi; Furuya, Ken

    2017-07-01

    Exchange of dimethyl sulfide (DMS) between the surface ocean and the lower atmosphere was examined by using proton transfer reaction-mass spectrometry coupled with the gradient flux (PTR-MS/GF) system. We deployed the PTR-MS/GF system and observed vertical gradients of atmospheric DMS just above the sea 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 sea-to-air flux of DMS. The DMS flux determined was in the range from 1.9 to 31 μmol m-2 d-1 and increased with wind speed and biological activity, in reasonable accordance with previous observations in the open ocean. The gas transfer velocity of DMS derived from the PTR-MS/GF measurements was similar to either that of DMS determined by the eddy covariance technique or that of insoluble gases derived from the dual tracer experiments, depending on the observation sites located in different geographic regions. When atmospheric conditions were strongly stable during the daytime in the subtropical ocean, the PTR-MS/GF observations captured a daytime versus nighttime difference in DMS mixing ratios in the surface air overlying the ocean surface. The difference was mainly due to the sea-to-air 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.

  11. Spatio-temporal dynamics of biogeochemical processes and air-sea CO2 fluxes in the Western English Channel based on two years of FerryBox deployment

    NASA Astrophysics Data System (ADS)

    Marrec, P.; Cariou, T.; Latimier, M.; Macé, E.; Morin, P.; Vernet, M.; Bozec, Y.

    2014-12-01

    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 sea surface temperature (SST), sea surface salinity (SSS), dissolved oxygen (DO), fluorescence and partial pressure of CO2 (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 5.2 μatm for pCO2. Over the 2 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 air-sea CO2 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. Air-sea CO2 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 CO2 to the atmosphere of 0.9 mmol m- 2 d- 1, whereas the nWEC acted as a sink for atmospheric CO2 of 6.9 mmol m- 2 d- 1. The study of short time-scale dynamics of air-sea CO2 fluxes revealed that an intense and short (less than 10 days) summer bloom in the nWEC contributed to 29% of the CO2 sink during the productive period, highlighting the necessity for high frequency observations in coastal

  12. Atmospheric organochlorine pollutants and air-sea exchange of hexachlorocyclohexane in the Bering and Chukchi Seas

    USGS Publications Warehouse

    Hinckley, D.A.; Bidleman, T.F.; Rice, C.P.

    1991-01-01

    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 Seas (August 1988), high-volume air 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 air-sea 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 2.4 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-2 day-1 (sea to air) to 122 ng m-2 d-1 (air to sea) and averaged 25 ng m-2 d-1 air to sea. All fluxes of gamma-HCH were from air to sea, ranged from 17 to 54 ng m-2 d-1, and averaged 31 ng m-2 d-1.

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

    NASA Astrophysics Data System (ADS)

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

    2016-12-01

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

  14. A study of oceanic surface heat fluxes in the Greenland, Norwegian, and Barents Seas

    NASA Technical Reports Server (NTRS)

    Hakkinen, Sirpa; Cavalieri, Donald J.

    1989-01-01

    This study examines oceanic surface heat fluxes in the Norwegian, Greenland, and Barents seas using the gridded Navy Fleet Numerical Oceanography Central surface analysis and the First GARP Global Experiment (FGGE) IIc cloudiness data bases. Monthly and annual means of net and turbulent heat fluxes are computed for the FGGE year 1979. The FGGE IIb data base consisting of individual observations provides particularly good data coverage in this region for a comparison with the gridded Navy winds and air temperatures. The standard errors of estimate between the Navy and FGGE IIb winds and air temperatures are 3.6 m/s and 2.5 C, respectively. The computations for the latent and sensible heat fluxes are based on bulk formulas with the same constant heat exchange coefficient of 0.0015. The results show extremely strong wintertime heat fluxes in the northern Greenland Sea and especially in the Barents Sea in contrast to previous studies.

  15. The SeaFlux Turbulent Flux Dataset Version 1.0 Documentation

    NASA Technical Reports Server (NTRS)

    Clayson, Carol Anne; Roberts, J. Brent; Bogdanoff, Alec S.

    2012-01-01

    Under the auspices of the World Climate Research Programme (WCRP) Global Energy and Water cycle EXperiment (GEWEX) Data and Assessment Panel (GDAP), the SeaFlux Project was created to investigate producing a high-resolution satellite-based dataset of surface turbulent fluxes over the global oceans. The most current release of the SeaFlux product is Version 1.0; this represents the initial release of turbulent surface heat fluxes, associated near-surface variables including a diurnally varying sea surface temperature.

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

    NASA Astrophysics Data System (ADS)

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

    2010-05-01

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

  17. 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> CO2 <span class="hlt">fluxes</span> over the last 27 years. The overall effect of increasing winds over time has a smaller impact than expected as the impact in regions of outgassing is greater than for the regions acting as a CO2 sink.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16271812','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16271812"><span>Atmospheric concentrations and <span class="hlt">air-sea</span> exchanges of nonylphenol, tertiary octylphenol and nonylphenol monoethoxylate in the North <span class="hlt">Sea</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Xie, Zhiyong; Lakaschus, Soenke; Ebinghaus, Ralf; Caba, Armando; Ruck, Wolfgang</p> <p>2006-07-01</p> <p>Concentrations of nonylphenol isomers (NP), tertiary octylphenol (t-OP) and nonylphenol monoethoxylate isomers (NP1EO) have been simultaneously determined in the <span class="hlt">sea</span> water and atmosphere of the North <span class="hlt">Sea</span>. A decreasing concentration profile appeared following the distance increasing from the coast to the central part of the North <span class="hlt">Sea</span>. <span class="hlt">Air-sea</span> exchanges of t-OP and NP were estimated using the two-film resistance model based upon relative <span class="hlt">air</span>-water concentrations and experimentally derived Henry's law constant. The average of <span class="hlt">air-sea</span> exchange <span class="hlt">fluxes</span> was -12+/-6 ng m(-2)day(-1) for t-OP and -39+/-19 ng m(-2)day(-1) for NP, which indicates a net deposition is occurring. These results suggest that the <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.ncbi.nlm.nih.gov/pubmed/25046608','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25046608"><span><span class="hlt">Flux</span> measurements in the surface Marine Atmospheric Boundary Layer over the Aegean <span class="hlt">Sea</span>, Greece.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kostopoulos, V E; Helmis, C G</p> <p>2014-10-01</p> <p>Micro-meteorological measurements within the surface Marine Atmospheric Boundary Layer took place at the shoreline of two islands at northern and south-eastern Aegean <span class="hlt">Sea</span> of Greece. The primary goal of these experimental campaigns was to study the momentum, heat and humidity <span class="hlt">fluxes</span> over this part of the north-eastern Mediterranean <span class="hlt">Sea</span>, characterized by limited spatial and temporal scales which could affect these exchanges at the <span class="hlt">air-sea</span> interface. The great majority of the obtained records from both sites gave higher values up to factor of two, compared with the estimations from the most widely used parametric formulas that came mostly from measurements over open <span class="hlt">seas</span> and oceans. Friction velocity values from both campaigns varied within the same range and presented strong correlation with the wind speed at 10 m height while the calculated drag coefficient values at the same height for both sites were found to be constant in relation with the wind speed. Using eddy correlation analysis, the heat <span class="hlt">flux</span> values were calculated (virtual heat <span class="hlt">fluxes</span> varied from -60 to 40 W/m(2)) and it was found that they are affected by the limited spatial and temporal scales of the responding <span class="hlt">air-sea</span> interaction mechanism. Similarly, the humidity <span class="hlt">fluxes</span> appeared to be strongly influenced by the observed intense spatial heterogeneity of the <span class="hlt">sea</span> surface temperature. Copyright © 2014 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21141036','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21141036"><span>Advances in quantifying <span class="hlt">air-sea</span> gas exchange and environmental forcing.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wanninkhof, Rik; Asher, William E; Ho, David T; Sweeney, Colm; McGillis, Wade R</p> <p>2009-01-01</p> <p>The past decade has seen a substantial amount of research on <span class="hlt">air-sea</span> gas exchange and its environmental controls. These studies have significantly advanced the understanding of processes that control gas transfer, led to higher quality field measurements, and improved estimates of the <span class="hlt">flux</span> of climate-relevant gases between the ocean and atmosphere. This review discusses the fundamental principles of <span class="hlt">air-sea</span> gas transfer and recent developments in gas transfer theory, parameterizations, and measurement techniques in the context of the exchange of carbon dioxide. However, much of this discussion is applicable to any sparingly soluble, non-reactive gas. We show how the use of global variables of environmental forcing that have recently become available and gas exchange relationships that incorporate the main forcing factors will lead to improved estimates of global and regional <span class="hlt">air-sea</span> gas <span class="hlt">fluxes</span> based on better fundamental physical, chemical, and biological foundations.</p> </li> </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/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> CO2 <span class="hlt">fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Forest, A.; Coupel, P.; Else, B.; Nahavandian, S.; Lansard, B.; Raimbault, P.; Papakyriakou, T.; Gratton, Y.; Fortier, L.; Tremblay, J.-É.; Babin, M.</p> <p>2013-10-01</p> <p>The accelerated decline in Arctic <span class="hlt">sea</span> ice combined with an ongoing trend toward a more dynamic atmosphere is modifying carbon cycling in the Arctic Ocean. A critical issue is to understand how net community production (NCP; the balance between gross primary production and community respiration) responds to changes and modulates <span class="hlt">air-sea</span> CO2 <span class="hlt">fluxes</span>. Using data collected as part of the ArcticNet-Malina 2009 expedition in southeastern Beaufort <span class="hlt">Sea</span> (Arctic Ocean), we synthesize information on <span class="hlt">sea</span> ice, wind, river, water column properties, metabolism of the planktonic food web, organic carbon <span class="hlt">fluxes</span> and pools, as well as <span class="hlt">air-sea</span> CO2 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> CO2 <span class="hlt">fluxes</span>. The mean atmospheric forcing was a mild upwelling-favorable wind (~5 km h-1) blowing from the N-E and a decaying ice cover (<80% concentration) was observed beyond the shelf, the latter being fully exposed to the atmosphere. We detected some areas where the surface mixed layer was net autotrophic owing to high rates of primary production (PP), but the ecosystem was overall net heterotrophic. The region acted nonetheless as a sink for atmospheric CO2 with a mean uptake rate of -2.0 ± 3.3 mmol C m-2d-1. We attribute this discrepancy to: (1) elevated PP rates (>600 mg C m-2d-1) over the shelf prior to our survey, (2) 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 CO2 to the atmosphere (>10mmol C m-2d-1). Although generally <100 mg C m-2d-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 (~241.2 × 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/2015AGUFM.A43C0283L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.A43C0283L"><span><span class="hlt">Air-sea</span> Exchange of Polycyclic Aromatic Hydrocarbons (PAHs), Polychlorinated Biphenyls (PCBs), Organochlorine Pesticides (OCPs) and Polybrominated Diphenyl Ethers (PBDEs) in the Mediterranean <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lammel, G. P.; Heil, A.; Kukucka, P.; Meixner, F. X.; Mulder, M. D.; Prybilova, P.; Prokes, R.; Rusina, T. S.; Song, G. Z.; Vrana, B.</p> <p>2015-12-01</p> <p>The marine atmospheric environment is a receptor for persistent organic pollutants (POPs) which are advected from sources on land, primary, such as biomass burning by-products (PAHs, dioxins), and secondary, such as volatilization from contaminated soils (PCBs, pesticides). Primary sources do not exist in the marine environment, except for PAHs (ship engines) but following previous atmospheric deposition, the <span class="hlt">sea</span> surface may turn to a secondary source by reversal of diffusive <span class="hlt">air-sea</span> mass exchange. No monitoring is in place. We studied the vertical <span class="hlt">fluxes</span> of a wide range of primary and secondary emitted POPs based on measurements in <span class="hlt">air</span> and surface seawater at a remote coastal site in the eastern Mediterranean (2012). To this end, silicon rubbers were used as passive water samplers, vertical concentration gradients were determined in <span class="hlt">air</span> and <span class="hlt">fluxes</span> were quantified based on Eddy covariance. Diffusive <span class="hlt">air-sea</span> exchange <span class="hlt">fluxes</span> of hexachlorocyclohexanes (HCHs) and semivolatile PAHs were found close to phase equilibrium, except one PAH, retene, a wood burning tracer, was found seasonally net-volatilisational. Some PCBs, p,p'-DDE, penta- and hexachlorobenzene (PeCB, HCB) were mostly net-depositional, while PBDEs were net-volatilizational. <span class="hlt">Fluxes</span> determined at a a remote coastal site ranged -33 - +2.4 µg m-2 d-1 for PAHs and -4.0 - +0.3 µg m-2 d-1for halogenated compounds (< 0 means net-deposition, > 0 means net-volatilization). It is concluded that nowadays in open <span class="hlt">seas</span> more pollutants are undergoing reversal of the direction of <span class="hlt">air-sea</span> exchange. Recgional fire activity records in combination with box model simulations suggest that deposition of retene during summer is followed by a reversal of <span class="hlt">air-sea</span> exchange. The seawater surface as secondary source of pollution should be assessed based on <span class="hlt">flux</span> measurements across seasons and over longer time periods.</p> </li> <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 CO2 uptake: an improved multiyear estimate of the <span class="hlt">air-sea</span> CO2 <span class="hlt">flux</span> 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> CO2 <span class="hlt">fluxes</span> 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 CO2 in the surface water (pCO2w) 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 CO2 mixing ratio, and geographical position. We applied new algorithms for extracting Chl a from satellite remote sensing reflectance with close examination of uncertainty of the obtained Chl a values. The overall relationship between pCO2w and Chl a was negative, whereas the relationship varied among seasons and regions. The addition of Chl a as a parameter in the SOM process enabled us to improve the estimate of pCO2w, particularly via better representation of its decline in spring, which resulted from biologically mediated pCO2w reduction. As a result of the inclusion of Chl a, the uncertainty in the CO2 <span class="hlt">flux</span> estimate was reduced, with a net annual Arctic Ocean CO2 uptake of 180 ± 130 Tg C yr-1. Seasonal to interannual variation in the CO2 influx was also calculated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhDT........41W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhDT........41W"><span>The Response of the Ocean Thermal Skin Layer to <span class="hlt">Air-Sea</span> Surface Heat <span class="hlt">Fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wong, Elizabeth Wing-See</p> <p></p> <p>There is much evidence that the ocean is heating as a result of an increase in concentrations of greenhouse gases (GHGs) in the atmosphere from human activities. GHGs absorb infrared radiation and re-emit infrared radiation back to the ocean's surface which is subsequently absorbed. However, the incoming infrared radiation is absorbed within the top micrometers of the ocean's surface which is where the thermal skin layer exists. Thus the incident infrared radiation does not directly heat the upper few meters of the ocean. We are therefore motivated to investigate the physical mechanism between the absorption of infrared radiation and its effect on heat transfer at the <span class="hlt">air-sea</span> boundary. The hypothesis is that since heat lost through the <span class="hlt">air-sea</span> interface is controlled by the thermal skin layer, which is directly influenced by the absorption and emission of infrared radiation, the heat flow through the thermal skin layer adjusts to maintain the surface heat loss, assuming the surface heat loss does not vary, and thus modulates the upper ocean heat content. This hypothesis is investigated through utilizing clouds to represent an increase in incoming longwave radiation and analyzing retrieved thermal skin layer vertical temperature profiles from a shipboard infrared spectrometer from two research cruises. The data are limited to night-time, no precipitation and low winds of less than 2 m/s to remove effects of solar radiation, wind-driven shear and possibilities of thermal skin layer disruption. The results show independence of the turbulent <span class="hlt">fluxes</span> and emitted radiation on the incident radiative <span class="hlt">fluxes</span> which rules out the immediate release of heat from the absorption of the cloud infrared irradiance back into the atmosphere through processes such as evaporation and increase infrared emission. Furthermore, independence was confirmed between the incoming and outgoing radiative <span class="hlt">flux</span> which implies the heat sink for upward flowing heat at the <span class="hlt">air-sea</span> interface is more</p> </li> <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 pCO 2, and net <span class="hlt">sea-air</span> CO 2 <span class="hlt">flux</span> 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 pCO 2 over the global oceans in non-El Niño conditions has been constructed with spatial resolution of 4° (latitude) ×5° (longitude) for a reference year 2000 based upon about 3 million measurements of surface water pCO 2 obtained from 1970 to 2007. The database used for this study is about 3 times larger than the 0.94 million used for our earlier paper [Takahashi et al., 2002. Global <span class="hlt">sea-air</span> CO 2 <span class="hlt">flux</span> based on climatological surface ocean pCO 2, 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 pCO 2 data in portions of the North Atlantic, North and South Pacific and Southern Oceans (which cover about 27% of the global ocean areas) indicates that the surface water pCO 2 over these oceanic areas has increased on average at a mean rate of 1.5 μatm y -1 with basin-specific rates varying between 1.2±0.5 and 2.1±0.4 μatm y -1. A global ocean database for a single reference year 2000 is assembled using this mean rate for correcting observations made in different years to the reference year. The observations made during El Niño periods in the equatorial Pacific and those made in coastal zones are excluded from the database. Seasonal changes in the surface water pCO 2 and the <span class="hlt">sea-air</span> pCO 2 difference over four climatic zones in the Atlantic, Pacific, Indian and Southern Oceans are presented. Over the Southern Ocean seasonal ice zone, the seasonality is complex. Although it cannot be thoroughly documented due to the limited extent of observations, seasonal changes in pCO 2 are approximated by using the data for under-ice waters during austral winter and those for the marginal ice and ice-free zones. The net <span class="hlt">air-sea</span> CO 2 <span class="hlt">flux</span> is estimated using the <span class="hlt">sea-air</span> pCO 2 difference and the <span class="hlt">air-sea</span> gas transfer rate that is parameterized as a function of (wind speed) 2 with a scaling factor of 0.26. This is estimated by inverting</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28645049','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28645049"><span>Gaseous elemental mercury in the marine boundary layer and <span class="hlt">air-sea</span> <span class="hlt">flux</span> in the Southern Ocean in austral summer.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Jiancheng; Xie, Zhouqing; Wang, Feiyue; Kang, Hui</p> <p>2017-12-15</p> <p>Gaseous elemental mercury (GEM) in the marine boundary layer (MBL), and dissolved gaseous mercury (DGM) in surface seawater of the Southern Ocean were measured in the austral summer from December 13, 2014 to February 1, 2015. GEM concentrations in the MBL ranged from 0.4 to 1.9ngm -3 (mean±standard deviation: 0.9±0.2ngm -3 ), whereas DGM concentrations in surface seawater ranged from 7.0 to 75.9pgL -1 (mean±standard deviation: 23.7±13.2pgL -1 ). The occasionally observed low GEM in the MBL suggested either the occurrence of atmospheric mercury depletion in summer, or the transport of GEM-depleted <span class="hlt">air</span> from the Antarctic Plateau. Elevated GEM concentrations in the MBL and DGM concentrations in surface seawater were consistently observed in the ice-covered region of the Ross <span class="hlt">Sea</span> implying the influence of the <span class="hlt">sea</span> ice environment. Diminishing <span class="hlt">sea</span> ice could cause more mercury evasion from the ocean to the <span class="hlt">air</span>. Using the thin film gas exchange model, the <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> of gaseous mercury in non-ice-covered area during the study period were estimated to range from 0.0 to 6.5ngm -2 h -1 with a mean value of 1.5±1.8ngm -2 h -1 , revealing GEM (re-)emission from the East Southern Ocean in summer. Copyright © 2017 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/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> CO2 <span class="hlt">fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Forest, A.; Coupel, P.; Else, B.; Nahavandian, S.; Lansard, B.; Raimbault, P.; Papakyriakou, T.; Gratton, Y.; Fortier, L.; Tremblay, J.-É.; Babin, M.</p> <p>2014-05-01</p> <p>The accelerated decline in Arctic <span class="hlt">sea</span> ice and an ongoing trend toward more energetic atmospheric and oceanic forcings are modifying carbon cycling in the Arctic Ocean. A critical issue is to understand how net community production (NCP; the balance between gross primary production and community respiration) responds to changes and modulates <span class="hlt">air-sea</span> CO2 <span class="hlt">fluxes</span>. Using data collected as part of the ArcticNet-Malina 2009 expedition in the southeastern Beaufort <span class="hlt">Sea</span> (Arctic Ocean), we synthesize information on <span class="hlt">sea</span> ice, wind, river, water column properties, metabolism of the planktonic food web, organic carbon <span class="hlt">fluxes</span> and pools, as well as <span class="hlt">air-sea</span> CO2 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> CO2 <span class="hlt">fluxes</span>. During the field campaign, the mean wind field was a mild upwelling-favorable wind (~ 5 km h-1) from the NE. A decaying ice cover (< 80% concentration) was observed beyond the shelf, the latter being fully exposed to the atmosphere. We detected some areas where the surface mixed layer was net autotrophic owing to high rates of primary production (PP), but the ecosystem was overall net heterotrophic. The region acted nonetheless as a sink for atmospheric CO2, with an uptake rate of -2.0 ± 3.3 mmol C m-2 d-1 (mean ± standard deviation associated with spatial variability). We attribute this discrepancy to (1) elevated PP rates (> 600 mg C m-2 d-1) over the shelf prior to our survey, (2) 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 CO2 to the atmosphere (> 10 mmol C m-2 d-1). Daily PP rates were generally < 100 mg C m-2 d-1 and cumulated to a total PP of ~ 437.6 × 103 t C for the region over a 35-day period. This amount was about twice the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhDT........17O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhDT........17O"><span>Observations and Modeling of Turbulent <span class="hlt">Air-Sea</span> Coupling in Coastal and Strongly Forced Condition</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ortiz-Suslow, David G.</p> <p></p> <p>The turbulent <span class="hlt">fluxes</span> of momentum, mass, and energy across the ocean-atmosphere boundary are fundamental to our understanding of a myriad of geophysical processes, such as wind-wave generation, oceanic circulation, and <span class="hlt">air-sea</span> gas transfer. In order to better understand these <span class="hlt">fluxes</span>, empirical relationships were developed to quantify the interfacial exchange rates in terms of easily observed parameters (e.g., wind speed). However, mounting evidence suggests that these empirical formulae are only valid over the relatively narrow parametric space, i.e. open ocean conditions in light to moderate winds. Several near-surface processes have been observed to cause significant variance in the <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> not predicted by the conventional functions, such as a heterogeneous surfaces, swell waves, and wave breaking. Further study is needed to fully characterize how these types of processes can modulate the interfacial exchange; in order to achieve this, a broad investigation into <span class="hlt">air-sea</span> coupling was undertaken. The primary focus of this work was to use a combination of field and laboratory observations and numerical modeling, in regimes where conventional theories would be expected to breakdown, namely: the nearshore and in very high winds. These seemingly disparate environments represent the marine atmospheric boundary layer at its physical limit. In the nearshore, the convergence of land, <span class="hlt">air</span>, and <span class="hlt">sea</span> in a depth-limited domain marks the transition from a marine to a terrestrial boundary layer. Under extreme winds, the physical nature of the boundary layer remains unknown as an intermediate substrate layer, <span class="hlt">sea</span> spray, develops between the atmosphere and ocean surface. At these ends of the MABL physical spectrum, direct measurements of the near-surface processes were made and directly related to local sources of variance. Our results suggest that the conventional treatment of <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> in terms of empirical relationships developed from a relatively narrow set of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.4722B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.4722B"><span>Regulation of CO2 <span class="hlt">Air</span> <span class="hlt">Sea</span> <span class="hlt">Fluxes</span> by Sediments in the North <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Burt, William; Thomas, Helmuth; Hagens, Mathilde; Brenner, Heiko; Pätsch, Johannes; Clargo, Nicola; Salt, Lesley</p> <p>2016-04-01</p> <p>A multi-tracer approach is applied to assess the impact of boundary <span class="hlt">fluxes</span> (e.g. benthic input from sediments or lateral inputs from the coastline) on the acid-base buffering capacity, and overall biogeochemistry, of the North <span class="hlt">Sea</span>. Analyses of both basin-wide observations in the North <span class="hlt">Sea</span> and transects through tidal basins at the North-Frisian coastline, reveal that surface distributions of the δ13C signature of dissolved inorganic carbon (DIC) are predominantly controlled by a balance between biological production and respiration. In particular, variability in metabolic DIC throughout stations in the well-mixed southern North <span class="hlt">Sea</span> indicates the presence of an external carbon source, which is traced to the European continental coastline using naturally-occurring radium isotopes (224Ra and 228Ra). 228Ra is also shown to be a highly effective tracer of North <span class="hlt">Sea</span> total alkalinity (AT) compared to the more conventional use of salinity. Coastal inputs of metabolic DIC and AT are calculated on a basin-wide scale, and ratios of these inputs suggest denitrification as a primary metabolic pathway for their formation. The AT input paralleling the metabolic DIC release prevents a significant decline in pH as compared to aerobic (i.e. unbuffered) release of metabolic DIC. Finally, long-term pH trends mimic those of riverine nitrate loading, highlighting the importance of coastal AT production via denitrification in regulating pH in the southern North <span class="hlt">Sea</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.9500M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.9500M"><span>Spume Drops: Their Potential Role in <span class="hlt">Air-Sea</span> Gas Exchange</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Monahan, Edward C.; Staniec, Allison; Vlahos, Penny</p> <p>2017-12-01</p> <p>After summarizing the time scales defining the change of the physical properties of spume and other droplets cast up from the <span class="hlt">sea</span> surface, the time scales governing drop-atmosphere gas exchange are compared. Following a broad review of the spume drop production functions described in the literature, a subset of these functions is selected via objective criteria, to represent typical, upper bound, and lower bound production functions. Three complementary mechanisms driving spume-atmosphere gas exchange are described, and one is then used to estimate the relative importance, over a broad range of wind speeds, of this spume drop mechanism compared to the conventional, diffusional, <span class="hlt">sea</span> surface mechanism in <span class="hlt">air-sea</span> gas exchange. While remaining uncertainties in the wind dependence of the spume drop production <span class="hlt">flux</span>, and in the immediate <span class="hlt">sea</span> surface gas <span class="hlt">flux</span>, preclude a definitive conclusion, the findings of this study strongly suggest that, at high wind speeds (>20 m s-1 for dimethyl sulfide and >30 m s-1 for gases such a carbon dioxide), spume drops do make a significant contribution to <span class="hlt">air-sea</span> gas exchange.<abstract type="synopsis"><title type="main">Plain Language SummaryThis paper evaluates the existing spume drop generation functions available to date and selects a reasonable upper, lower and mid range function that are reasonable for use in <span class="hlt">air</span> <span class="hlt">sea</span> exchange models. Based on these the contribution of spume drops to overall <span class="hlt">air</span> <span class="hlt">sea</span> gas exchange at different wind speeds is then evaluated to determine the % contribution of spume. Generally below 20ms-1 spume drops contribute <1% of gas exchange but may account for a significant amount of gas exchange at higher wind speeds.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001JGR...10632139N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001JGR...10632139N"><span>Turbulent aerosol <span class="hlt">fluxes</span> over the Arctic Ocean: 2. Wind-driven sources from the <span class="hlt">sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nilsson, E. D.; Rannik, Ü.; Swietlicki, E.; Leck, C.; Aalto, P. P.; Zhou, J.; Norman, M.</p> <p>2001-12-01</p> <p>An eddy-covariance <span class="hlt">flux</span> system was successfully applied over open <span class="hlt">sea</span>, leads and ice floes during the Arctic Ocean Expedition in July-August 1996. Wind-driven upward aerosol number <span class="hlt">fluxes</span> were observed over open <span class="hlt">sea</span> and leads in the pack ice. These particles must originate from droplets ejected into the <span class="hlt">air</span> at the bursting of small <span class="hlt">air</span> bubbles at the water surface. The source <span class="hlt">flux</span> F (in 106 m-2 s-1) had a strong dependency on wind speed, log>(F>)=0.20U¯-1.71 and 0.11U¯-1.93, over the open <span class="hlt">sea</span> and leads, respectively (where U¯ is the local wind speed at about 10 m height). Over the open <span class="hlt">sea</span> the wind-driven aerosol source <span class="hlt">flux</span> consisted of a film drop mode centered at ˜100 nm diameter and a jet drop mode centered at ˜1 μm diameter. Over the leads in the pack ice, a jet drop mode at ˜2 μm diameter dominated. The jet drop mode consisted of <span class="hlt">sea</span>-salt, but oxalate indicated an organic contribution, and bacterias and other biogenic particles were identified by single particle analysis. Particles with diameters less than -100 nm appear to have contributed to the <span class="hlt">flux</span>, but their chemical composition is unknown. Whitecaps were probably the bubble source at open <span class="hlt">sea</span> and on the leads at high wind speed, but a different bubble source is needed in the leads owing to their small fetch. Melting of ice in the leads is probably the best candidate. The <span class="hlt">flux</span> over the open <span class="hlt">sea</span> was of such a magnitude that it could give a significant contribution to the condensation nuclei (CCN) population. Although the <span class="hlt">flux</span> from the leads were roughly an order of magnitude smaller and the leads cover only a small fraction of the pack ice, the local source may till be important for the CCN population in Arctic fogs. The primary marine aerosol source will increase both with increased wind speed and with decreased ice fraction and extent. The local CCN production may therefore increase and influence cloud or fog albedo and lifetime in response to greenhouse warming in the Arctic Ocean region.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMGC23K..14F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMGC23K..14F"><span>Carbon <span class="hlt">fluxes</span> in North American coastal and shelf <span class="hlt">seas</span>: Current status and trends</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fennel, K.; Alin, S. R.; Barbero, L.; Evans, W.; Martin Hernandez-Ayon, J. M.; Hu, X.; Lohrenz, S. E.; Muller-Karger, F. E.; Najjar, R.; Robbins, L. L.; Shadwick, E. H.; Siedlecki, S. A.; Steiner, N.; Turk, D.; Vlahos, P.; Wang, A. Z.</p> <p>2016-12-01</p> <p>Coastal and shelf <span class="hlt">seas</span> represent an interface between all major components of the global carbon cycle: land, atmosphere, marine sediments and the ocean. <span class="hlt">Fluxes</span> and transformations of carbon in coastal systems are complex and highly variable in space and time. The First State of the Carbon Cycle Report (http://cdiac.ornl.gov/SOCCR/final.html, Chapter 15, Chavez et al. 2007) concluded that carbon budgets of North American ocean margins were not well quantified because of insufficient observations and the complexity and highly localized spatial variability of coastal carbon dynamics. Since then significant progress has been made through the expansion of carbon observing networks, the implementation of modeling capabilities, and national and international coordination and synthesis activities. We will review the current understanding of coastal carbon <span class="hlt">fluxes</span> around the North American continent including along the Atlantic and Pacific coasts, the northern Gulf of Mexico, and the North American Arctic region and provide a compilation of regional estimates of <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> of CO2. We will discuss generalizable patterns in coastal <span class="hlt">air-sea</span> CO2 exchange and other carbon <span class="hlt">fluxes</span> as well as reasons underlying spatial heterogeneity. After providing an overview of the principal modes of carbon export from coastal systems, we will apply these mechanisms to the North American continent, and discuss observed and projected trends of key properties and <span class="hlt">fluxes</span>. The presentation will illustrate that despite significant advances in capabilities and understanding, large uncertainties remain.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOS.A24A2561T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOS.A24A2561T"><span>Impact of Ocean Surface Waves on <span class="hlt">Air-Sea</span> Momentum <span class="hlt">Flux</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tamura, H.; Drennan, W. M.; Collins, C. O., III; Graber, H. C.</p> <p>2016-02-01</p> <p>In this study, we investigated the structure of turbulent <span class="hlt">air</span> flow over ocean waves. Observations of wind and waves were retrieved by <span class="hlt">air-sea</span> interaction spar (ASIS) buoys during the shoaling waves experiment (SHOWEX) in Duck, NC in 1999. It is shown that the turbulent velocity spectra and co-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' co-spectra become negative near the fp, which suggests the upward momentum transport (i.e., negative wind stress) induced by ocean waves. Finally, we propose three turbulent flow structures for different wind-wave regimes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ACP....18.6001G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ACP....18.6001G"><span>The effects of <span class="hlt">sea</span> spray and atmosphere-wave coupling on <span class="hlt">air-sea</span> exchange during a tropical cyclone</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Garg, Nikhil; Kwee Ng, Eddie Yin; Narasimalu, Srikanth</p> <p>2018-04-01</p> <p>The study investigates the role of the <span class="hlt">air-sea</span> interface using numerical simulations of Hurricane Arthur (2014) in the Atlantic. More specifically, the present study aims to discern the role ocean surface waves and <span class="hlt">sea</span> spray play in modulating the intensity and structure of a tropical cyclone (TC). To investigate the effects of ocean surface waves and <span class="hlt">sea</span> spray, numerical simulations were carried out using a coupled atmosphere-wave model, whereby a <span class="hlt">sea</span> spray microphysical model was incorporated within the coupled model. Furthermore, this study also explores how <span class="hlt">sea</span> spray generation can be modelled using wave energy dissipation due to whitecaps; whitecaps are considered as the primary mode of spray droplets generation at hurricane intensity wind speeds. Three different numerical simulations including the <span class="hlt">sea</span>- state-dependent momentum <span class="hlt">flux</span>, the <span class="hlt">sea</span>-spray-mediated heat <span class="hlt">flux</span>, and a combination of the former two processes with the <span class="hlt">sea</span>-spray-mediated momentum <span class="hlt">flux</span> were conducted. The foregoing numerical simulations were evaluated against the National Data Buoy Center (NDBC) buoy and satellite altimeter measurements as well as a control simulation using an uncoupled atmosphere model. The results indicate that the model simulations were able to capture the storm track and intensity: the surface wave coupling results in a stronger TC. Moreover, it is also noted that when only spray-mediated heat <span class="hlt">fluxes</span> are applied in conjunction with the <span class="hlt">sea</span>-state-dependent momentum <span class="hlt">flux</span>, they result in a slightly weaker TC, albeit stronger compared to the control simulation. However, when a spray-mediated momentum <span class="hlt">flux</span> is applied together with spray heat <span class="hlt">fluxes</span>, it results in a comparably stronger TC. The results presented here allude to the role surface friction plays in the intensification of a TC.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA462427','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA462427"><span>Residual-Mean Analysis of the <span class="hlt">Air-Sea</span> <span class="hlt">Fluxes</span> and Associated Oceanic Meridional Overturning</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2006-12-01</p> <p>the adiabatic component of the MOC which is based entirely on the <span class="hlt">sea</span> surface data . The coordinate system introduced in this study is somewhat...heat capacity of water. The technique utilizes the observational data based on meteorological re- analysis (density <span class="hlt">flux</span> at the <span class="hlt">sea</span> surface) and...Figure 8. Annual mean and temporal standard deviation of the zonally-averaged mixed- layer depth. The plotted data are based on Levitus 94 climatology</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150002122','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150002122"><span>Natural <span class="hlt">Air-Sea</span> <span class="hlt">Flux</span> of CO2 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 CO2 gas exchange (natural <span class="hlt">flux</span> of CO2) between the ocean and the atmosphere are presented here using the NASA-GISS climate model, in which the same atmospheric component (modelE2) is coupled to two different ocean models, the Russell ocean model and HYCOM. Both incarnations of the GISS climate model are also coupled to the same ocean biogeochemistry module (NOBM) which estimates prognostic distributions for biotic and abiotic fields that influence the <span class="hlt">air-sea</span> <span class="hlt">flux</span> of CO2. Model intercomparison is carried out at equilibrium conditions and model differences are contrasted with biases from present day climatologies. Although the models agree on the spatial patterns of the <span class="hlt">air-sea</span> <span class="hlt">flux</span> of CO2, they disagree on the strength of the North Atlantic and Southern Ocean sinks mainly because of kinematic (winds) and chemistry (pCO2) differences rather than thermodynamic (SST) ones. Biology/chemistry dissimilarities in the models stem from the different parameterizations of advective and diffusive processes, such as overturning, mixing and horizontal tracer advection and to a lesser degree from parameterizations of biogeochemical processes such as gravitational settling and sinking. The global meridional overturning circulation illustrates much of the different behavior of the biological pump in the two models, together with differences in mixed layer depth which are responsible for different SST, DIC and nutrient distributions in the two models and consequently different atmospheric feedbacks (in the wind, net heat and freshwater <span class="hlt">fluxes</span> into the ocean).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017BGeo...14.5765F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017BGeo...14.5765F"><span>Quantification of dimethyl sulfide (DMS) production in the <span class="hlt">sea</span> anemone Aiptasia sp. to simulate the <span class="hlt">sea-to-air</span> <span class="hlt">flux</span> from coral reefs</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Franchini, Filippo; Steinke, Michael</p> <p>2017-12-01</p> <p>The production of dimethyl sulfide (DMS) is poorly quantified in tropical reef environments but forms an essential process that couples marine and terrestrial sulfur cycles and affects climate. Here we quantified net aqueous DMS production and the concentration of its cellular precursor dimethylsulfoniopropionate (DMSP) in the <span class="hlt">sea</span> anemone Aiptasia sp., a model organism to study coral-related processes. Bleached anemones did not show net DMS production whereas symbiotic anemones produced DMS concentrations (mean ± standard error) of 160.7 ± 44.22 nmol g-1 dry weight (DW) after 48 h incubation. Symbiotic and bleached individuals showed DMSP concentrations of 32.7 ± 6.00 and 0.6 ± 0.19 µmol g-1 DW, respectively. We applied these findings to a Monte Carlo simulation to demonstrate that net aqueous DMS production accounts for only 20 % of gross aqueous DMS production. Monte Carlo-based estimations of <span class="hlt">sea-to-air</span> <span class="hlt">fluxes</span> of gaseous DMS showed that reefs may release 0.1 to 26.3 µmol DMS m-2 coral surface area (CSA) d-1 into the atmosphere with 40 % probability for rates between 0.5 and 1.5 µmol m-2 CSA d-1. These predictions were in agreement with directly quantified <span class="hlt">fluxes</span> in previous studies. Conversion to a <span class="hlt">flux</span> normalised to <span class="hlt">sea</span> surface area (SSA) (range 0.1 to 17.4, with the highest probability for 0.3 to 1.0 µmol DMS m-2 SSA d-1) suggests that coral reefs emit gaseous DMS at lower rates than the average global oceanic DMS <span class="hlt">flux</span> of 4.6 µmol m-2 SSA d-1 (19.6 Tg sulfur per year). The large difference between simulated gross and quantified net aqueous DMS production in corals suggests that the current and future potential for its production in tropical reefs is critically governed by DMS consumption processes. Hence, more research is required to assess the sensitivity of DMS-consumption pathways to ongoing environmental change in order to address the impact of predicted degradation of coral reefs on DMS production in tropical coastal ecosystems and its impact on</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26975003','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26975003"><span><span class="hlt">Air-sea</span> exchange of gaseous mercury in the East China <span class="hlt">Sea</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Chunjie; Ci, Zhijia; Wang, Zhangwei; Zhang, Xiaoshan</p> <p>2016-05-01</p> <p>Two oceanographic cruises were carried out in the East China <span class="hlt">Sea</span> (ECS) during the summer and fall of 2013. The main objectives of this study are to identify the spatial-temporal distributions of gaseous elemental mercury (GEM) in <span class="hlt">air</span> and dissolved gaseous mercury (DGM) in surface seawater, and then to estimate the Hg(0) <span class="hlt">flux</span>. The GEM concentration was lower in summer (1.61 ± 0.32 ng m(-3)) than in fall (2.20 ± 0.58 ng m(-3)). The back-trajectory analysis revealed that the <span class="hlt">air</span> masses with high GEM levels during fall largely originated from the land, while the <span class="hlt">air</span> masses with low GEM levels during summer primarily originated from ocean. The spatial distribution patterns of total Hg (THg), fluorescence, and turbidity were consistent with the pattern of DGM with high levels in the nearshore area and low levels in the open <span class="hlt">sea</span>. Additionally, the levels of percentage of DGM to THg (%DGM) were higher in the open <span class="hlt">sea</span> than in the nearshore area, which was consistent with the previous studies. The THg concentration in fall was higher (1.47 ± 0.51 ng l(-1)) than those of other open oceans. The DGM concentration (60.1 ± 17.6 pg l(-1)) and Hg(0) <span class="hlt">flux</span> (4.6 ± 3.6 ng m(-2) h(-1)) in summer were higher than those in fall (DGM: 49.6 ± 12.5 pg l(-1) and Hg(0) <span class="hlt">flux</span>: 3.6 ± 2.8 ng m(-2) h(-1)). The emission <span class="hlt">flux</span> of Hg(0) from the ECS was estimated to be 27.6 tons yr(-1), accounting for ∼0.98% of the global Hg oceanic evasion though the ECS only accounts for ∼0.21% of global ocean area, indicating that the ECS plays an important role in the oceanic Hg cycle. Copyright © 2016 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMOS43A1400S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMOS43A1400S"><span>Validation of the Fully-Coupled <span class="hlt">Air-Sea</span>-Wave COAMPS System</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Smith, T.; Campbell, T. J.; Chen, S.; Gabersek, S.; Tsu, J.; Allard, R. A.</p> <p>2017-12-01</p> <p>A fully-coupled, <span class="hlt">air-sea</span>-wave numerical model, COAMPS®, has been developed by the Naval Research Laboratory to further enhance understanding of oceanic, atmospheric, and wave interactions. The fully-coupled <span class="hlt">air-sea</span>-wave system consists of an atmospheric component with full physics parameterizations, an ocean model, NCOM (Navy Coastal Ocean Model), and two wave components, SWAN (Simulating Waves Nearshore) and WaveWatch III. <span class="hlt">Air-sea</span> interactions between the atmosphere and ocean components are accomplished through bulk <span class="hlt">flux</span> formulations of wind stress and sensible and latent heat <span class="hlt">fluxes</span>. Wave interactions with the ocean include the Stokes' drift, surface radiation stresses, and enhancement of the bottom drag coefficient in shallow water due to the wave orbital velocities at the bottom. In addition, NCOM surface currents are provided to SWAN and WaveWatch III to simulate wave-current interaction. The fully-coupled COAMPS system was executed for several regions at both regional and coastal scales for the entire year of 2015, including the U.S. East Coast, Western Pacific, and Hawaii. Validation of COAMPS® includes observational data comparisons and evaluating operational performance on the High Performance Computing (HPC) system for each of these regions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.ars.usda.gov/research/publications/publication/?seqNo115=246298','TEKTRAN'); return false;" href="http://www.ars.usda.gov/research/publications/publication/?seqNo115=246298"><span>Atmospheric deposition <span class="hlt">flux</span> estimates for chlorpyrifos and trifluralin in the chukchi <span class="hlt">sea</span></span></a></p> <p><a target="_blank" href="https://www.ars.usda.gov/research/publications/find-a-publication/">USDA-ARS?s Scientific Manuscript database</a></p> <p></p> <p></p> <p>During the 1993 U.S.-Russian BERPAC expedition, residues of agricultural pesticides were detected in seawater, ice, surface microlayer, fog, and <span class="hlt">air</span> of the Bering and Chukchi <span class="hlt">Seas</span>. Gas exchange, wet deposition, and dry particle deposition <span class="hlt">fluxes</span> of trifluralin and chlorpyrifos were estimated using m...</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_2");'>2</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li class="active"><span>4</span></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_4 --> <div id="page_5" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li class="active"><span>5</span></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="81"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeoRL..44.6352P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoRL..44.6352P"><span>Importance of ocean mesoscale variability for <span class="hlt">air-sea</span> interactions in the Gulf of Mexico</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Putrasahan, D. A.; Kamenkovich, I.; Le Hénaff, M.; Kirtman, B. P.</p> <p>2017-06-01</p> <p>Mesoscale variability of currents in the Gulf of Mexico (GoM) can affect oceanic heat advection and <span class="hlt">air-sea</span> heat exchanges, which can influence climate extremes over North America. This study is aimed at understanding the influence of the oceanic mesoscale variability on the lower atmosphere and <span class="hlt">air-sea</span> heat exchanges. The study contrasts global climate model (GCM) with 0.1° ocean resolution (high resolution; HR) with its low-resolution counterpart (1° ocean resolution with the same 0.5° atmosphere resolution; LR). The LR simulation is relevant to current generation of GCMs that are still unable to resolve the oceanic mesoscale. Similar to observations, HR exhibits positive correlation between <span class="hlt">sea</span> surface temperature (SST) and surface turbulent heat <span class="hlt">flux</span> anomalies, while LR has negative correlation. For HR, we decompose lateral advective heat <span class="hlt">fluxes</span> in the upper ocean into mean (slowly varying) and mesoscale-eddy (fast fluctuations) components. We find that the eddy <span class="hlt">flux</span> divergence/convergence dominates the lateral advection and correlates well with the SST anomalies and <span class="hlt">air-sea</span> latent heat exchanges. This result suggests that oceanic mesoscale advection supports warm SST anomalies that in turn feed surface heat <span class="hlt">flux</span>. We identify anticyclonic warm-core circulation patterns (associated Loop Current and rings) which have an average diameter of 350 km. These warm anomalies are sustained by eddy heat <span class="hlt">flux</span> convergence at submonthly time scales and have an identifiable imprint on surface turbulent heat <span class="hlt">flux</span>, atmospheric circulation, and convective precipitation in the northwest portion of an averaged anticyclone.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMGC13C0652T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMGC13C0652T"><span>Southern Ocean <span class="hlt">air-sea</span> heat <span class="hlt">flux</span>, SST spatial anomalies, and implications for multi-decadal upper ocean heat content trends.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tamsitt, V. M.; Talley, L. D.; Mazloff, M. R.</p> <p>2014-12-01</p> <p>The Southern Ocean displays a zonal dipole (wavenumber one) pattern in <span class="hlt">sea</span> surface temperature (SST), with a cool zonal anomaly in the Atlantic and Indian sectors and a warm zonal anomaly in the Pacific sector, associated with the large northward excursion of the Malvinas and southeastward flow of the Antarctic Circumpolar Current (ACC). To the north of the cool Indian sector is the warm, narrow Agulhas Return Current (ARC). <span class="hlt">Air-sea</span> heat <span class="hlt">flux</span> is largely the inverse of this SST pattern, with ocean heat gain in the Atlantic/Indian, cooling in the southeastward-flowing ARC, and cooling in the Pacific, based on adjusted <span class="hlt">fluxes</span> from the Southern Ocean State Estimate (SOSE), a ⅙° eddy permitting model constrained to all available in situ data. This heat <span class="hlt">flux</span> pattern is dominated by turbulent heat loss from the ocean (latent and sensible), proportional to perturbations in the difference between SST and surface <span class="hlt">air</span> temperature, which are maintained by ocean advection. Locally in the Indian sector, intense heat loss along the ARC is contrasted by ocean heat gain of 0.11 PW south of the ARC. The IPCC AR5 50 year depth-averaged 0-700 m temperature trend shows surprising similarities in its spatial pattern, with upper ocean warming in the ARC contrasted by cooling to the south. Using diagnosed heat budget terms from the most recent (June 2014) 6-year run of the SOSE we find that surface cooling in the ARC is balanced by heating from south-eastward advection by the current whereas heat gain in the ACC is balanced by cooling due to northward Ekman transport driven by strong westerly winds. These results suggest that spatial patterns in multi-decadal upper ocean temperature trends depend on regional variations in upper ocean dynamics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AtmEn.178...31J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AtmEn.178...31J"><span>Seasonal atmospheric deposition and <span class="hlt">air-sea</span> gas exchange of polycyclic aromatic hydrocarbons over the Yangtze River Estuary, East China <span class="hlt">Sea</span>: Implications for source-sink processes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jiang, Yuqing; Lin, Tian; Wu, Zilan; Li, Yuanyuan; Li, Zhongxia; Guo, Zhigang; Yao, Xiaohong</p> <p>2018-04-01</p> <p>In this work, <span class="hlt">air</span> samples and surface seawater samples covering four seasons from March 2014 to January 2015 were collected from a background receptor site in the YRE to explore the seasonal <span class="hlt">fluxes</span> of <span class="hlt">air-sea</span> gas exchange and dry and wet deposition of 15 polycyclic aromatic hydrocarbons (PAHs) and their source-sink processes at the <span class="hlt">air-sea</span> interface. The average dry and wet deposition <span class="hlt">fluxes</span> of 15 PAHs were estimated as 879 ± 1393 ng m-2 d-1 and 755 ± 545 ng m-2 d-1, respectively. Gaseous PAH release from seawater to the atmosphere averaged 3114 ± 1999 ng m-2 d-1 in a year round. The <span class="hlt">air-sea</span> gas exchange of PAHs was the dominant process at the <span class="hlt">air-sea</span> interface in the YRE as the magnitude of volatilization <span class="hlt">flux</span> of PAHs exceeded that of total dry and wet deposition. The gas PAH exchange <span class="hlt">flux</span> was dominated by three-ring PAHs, with the highest value in summer and lowest in winter, indicating a marked seasonal variation owing to differences in Henry's law constants associated with temperature, as well as wind speed and gaseous-dissolved gradient among seasons. Based on the simplified mass balance estimation, a net 11 tons y-1 of PAHs (mainly three-ring PAHs) were volatilized from seawater to the atmosphere in a ∼20,000 km2 area in the YRE. Other than the year-round Yangtze River input and ocean ship emissions, the selective release of low-molecular-weight PAHs from bottom sediments in winter due to resuspension triggered by the East Asian winter monsoon is another potential source of PAHs. This work suggests that the source-sink processes of PAHs at the <span class="hlt">air-sea</span> interface in the YRE play a crucial role in regional cycling of PAHs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27617333','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27617333"><span>Persistent organochlorine pesticides and polychlorinated biphenyls in <span class="hlt">air</span> of the North <span class="hlt">Sea</span> region and <span class="hlt">air-sea</span> exchange.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mai, Carolin; Theobald, Norbert; Hühnerfuss, Heinrich; Lammel, Gerhard</p> <p>2016-12-01</p> <p>Organochlorine pesticides (OCPs) and polychlorinated biphenyls (PCBs) were studied to determine occurrence, levels and spatial distribution in the marine atmosphere and surface seawater during cruises in the German Bight and the wider North <span class="hlt">Sea</span> in spring and summer 2009-2010. In general, the concentrations found in <span class="hlt">air</span> are similar to, or below, the levels at coastal or near-coastal sites in Europe. Hexachlorobenzene and α-hexachlorocyclohexane (α-HCH) were close to phase equilibrium, whereas net atmospheric deposition was observed for γ-HCH. The results suggest that declining trends of HCH in seawater have been continuing for γ-HCH but have somewhat levelled off for α-HCH. Dieldrin displayed a close to phase equilibrium in nearly all the sampling sites, except in the central southwestern part of the North <span class="hlt">Sea</span>. Here atmospheric deposition dominates the <span class="hlt">air-sea</span> exchange. This region, close to the English coast, showed remarkably increased surface seawater concentrations. This observation depended neither on riverine input nor on the elevated abundances of dieldrin in the <span class="hlt">air</span> masses of central England. A net depositional <span class="hlt">flux</span> of p,p'-DDE into the North <span class="hlt">Sea</span> was indicated by both its abundance in the marine atmosphere and the changes in metabolite pattern observed in the surface water from the coast towards the open <span class="hlt">sea</span>. The long-term trends show that the atmospheric concentrations of DDT and its metabolites are not declining. Riverine input is a major source of PCBs in the German Bight and the wider North <span class="hlt">Sea</span>. Atmospheric deposition of the lower molecular weight PCBs (PCB28 and PCB52) was indicated as a major source for surface seawater pollution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/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 CO2.Exchange <span class="hlt">fluxes</span> are products of an <span class="hlt">air-sea</span> gas concentration difference, ΔC, and a gas transfer velocity, kw. The latter is controlled by the rate of turbulent diffusion at the <span class="hlt">air-sea</span> interface but it cannot be directly measured and has a high uncertainty that is now considered one of the greatest challenges to quantifying net global <span class="hlt">air-sea</span> CO2 exchange ...(Takahashi et al., 2009). One important control on kw is exerted by <span class="hlt">sea</span> surface surfactants that arise both naturally from biological processes and through anthropogenic activity. They influence gas exchange in two fundamental ways: as a monolayer physical barrier and through modifying <span class="hlt">sea</span> surface hydrodynamics and hence turbulent energy transfer. These effects have been demonstrated in the laboratory with artificial surfactants ...(Bock et al., 1999; Goldman et al., 1988) and through purposeful surfactant releases in coastal waters .(.).........().(Brockmann et al., 1982) and in the open ocean (Salter et al., 2011). Suppression of kwin these field experiments was ~5-55%. While changes in both total surfactant concentration and the composition of the natural surfactant pool might be expected to impact kw, the required in-situ studies are lacking. New data collected from the coastal North <span class="hlt">Sea</span> in 2012-2013 shows significant spatio-temporal variability in the surfactant activity of organic matter within the <span class="hlt">sea</span> surface microlayer that ranges from 0.07-0.94 mg/L T-X-100 (AC voltammetry). The surfactant activities show a strong winter/summer seasonal bias and general decrease in concentration with increasing distance from the coastline possibly associated with changing terrestrial vs. phytoplankton sources. Gas exchange experiments of this seawater using a novel laboratory tank and gas tracers (CH4 and SF6) demonstrate a 12-45% reduction in kw compared to surfactant-free water. Seasonally there is higher gas exchange suppression in the summer</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ClDy...49.2219S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ClDy...49.2219S"><span>Accounting for observation uncertainties in an evaluation metric of low latitude turbulent <span class="hlt">air-sea</span> <span class="hlt">fluxes</span>: application to the comparison of a suite of IPSL model versions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Servonnat, Jérôme; Găinuşă-Bogdan, Alina; Braconnot, Pascale</p> <p>2017-09-01</p> <p>Turbulent momentum and heat (sensible heat and latent heat) <span class="hlt">fluxes</span> at the <span class="hlt">air-sea</span> interface are key components of the whole energetic of the Earth's climate. The evaluation of these <span class="hlt">fluxes</span> in the climate models is still difficult because of the large uncertainties associated with the reference products. In this paper we present an objective metric accounting for reference uncertainties to evaluate the annual cycle of the low latitude turbulent <span class="hlt">fluxes</span> of a suite of IPSL climate models. This metric consists in a Hotelling T 2 test between the simulated and observed field in a reduce space characterized by the dominant modes of variability that are common to both the model and the reference, taking into account the observational uncertainty. The test is thus more severe when uncertainties are small as it is the case for <span class="hlt">sea</span> surface temperature (SST). The results of the test show that for almost all variables and all model versions the model-reference differences are not zero. It is not possible to distinguish between model versions for sensible heat and meridional wind stress, certainly due to the large observational uncertainties. All model versions share similar biases for the different variables. There is no improvement between the reference versions of the IPSL model used for CMIP3 and CMIP5. The test also reveals that the higher horizontal resolution fails to improve the representation of the turbulent surface <span class="hlt">fluxes</span> compared to the other versions. The representation of the <span class="hlt">fluxes</span> is further degraded in a version with improved atmospheric physics with an amplification of some of the biases in the Indian Ocean and in the intertropical convergence zone. The ranking of the model versions for the turbulent <span class="hlt">fluxes</span> is not correlated with the ranking found for SST. This highlights that despite the fact that SST gradients are important for the large-scale atmospheric circulation patterns, other factors such as wind speed, and <span class="hlt">air-sea</span> temperature contrast play an</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23932146','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23932146"><span>The <span class="hlt">sea-air</span> exchange of mercury (Hg) in the marine boundary layer of the Augusta basin (southern Italy): concentrations and evasion <span class="hlt">flux</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bagnato, E; Sproveri, M; Barra, M; Bitetto, M; Bonsignore, M; Calabrese, S; Di Stefano, V; Oliveri, E; Parello, F; Mazzola, S</p> <p>2013-11-01</p> <p>The first attempt to systematically investigate the atmospheric mercury (Hg) in the MBL of the Augusta basin (SE Sicily, Italy) has been undertaken. In the past the basin was the receptor for Hg from an intense industrial activity which contaminated the bottom sediments of the Bay, making this area a potential source of pollution for the surrounding Mediterranean. Three oceanographic cruises have been thus performed in the basin during the winter and summer 2011/2012, where we estimated averaged Hgatm concentrations of about 1.5±0.4 (range 0.9-3.1) and 2.1±0.98 (range 1.1-3.1) ng m(-3) for the two seasons, respectively. These data are somewhat higher than the background Hg atm value measured over the land (range 1.1±0.3 ng m(-3)) at downtown Augusta, while are similar to those detected in other polluted regions elsewhere. Hg evasion <span class="hlt">fluxes</span> estimated at the <span class="hlt">sea/air</span> interface over the Bay range from 3.6±0.3 (unpolluted site) to 72±0.1 (polluted site of the basin) ng m(-2) h(-1). By extending these measurements to the entire area of the Augusta basin (~23.5 km(2)), we calculated a total <span class="hlt">sea-air</span> Hg evasion <span class="hlt">flux</span> of about 9.7±0.1 g d(-1) (~0.004 tyr(-1)), accounting for ~0.0002% of the global Hg oceanic evasion (2000 tyr(-1)). The new proposed data set offers a unique and original study on the potential outflow of Hg from the <span class="hlt">sea-air</span> interface at the basin, and it represents an important step for a better comprehension of the processes occurring in the marine biogeochemical cycle of this element. Copyright © 2013 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016ECSS..176....1M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016ECSS..176....1M"><span>Temporal variability of <span class="hlt">air-sea</span> CO2 exchange in a low-emission estuary</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mørk, Eva Thorborg; Sejr, Mikael Kristian; Stæhr, Peter Anton; Sørensen, Lise Lotte</p> <p>2016-07-01</p> <p>There is the need for further study of whether global estimates of <span class="hlt">air-sea</span> CO2 exchange in estuarine systems capture the relevant temporal variability and, as such, the temporal variability of bulk parameterized and directly measured CO2 <span class="hlt">fluxes</span> was investigated in the Danish estuary, Roskilde Fjord. The <span class="hlt">air-sea</span> CO2 <span class="hlt">fluxes</span> 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 <span class="hlt">flux</span> 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 <span class="hlt">air-sea</span> CO2 exchanges and changed the net <span class="hlt">air-sea</span> CO2 exchange from an uptake to a release. The CO2 gas transfer velocity was calculated from directly measured CO2 <span class="hlt">fluxes</span> and ΔpCO2 and agreed to previous observations and parameterizations.</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> CO2 <span class="hlt">fluxes</span> and modelled pCO2 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> CO2 <span class="hlt">fluxes</span> over continental shelves vary substantially in time on both seasonal and sub-seasonal scales, driven primarily by variations in surface pCO2 due to several oceanic mechanisms. Furthermore, coastal zones have not been appropriately considered in global estimates of <span class="hlt">sea-air</span> CO2 <span class="hlt">fluxes</span>, 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> CO2 <span class="hlt">fluxes</span> by investigating the southwestern Atlantic Ocean (21-35°S) region, where physical, chemical and biological measurements were made on board the Brazilian R. V. Cruzeiro do Sul during late spring 2010 and early summer 2011. Features such as discharge from the La Plata River, intrusions of tropical waters on the outer shelf due to meandering and flow instabilities of the Brazil Current, and coastal upwelling in the Santa Marta Grande Cape and São Tomé Cape were detected by both in situ measurements and ocean colour and thermal satellite imagery. Overall, shelf waters in the study area were a source of CO2 to the atmosphere, with an average of 1.2 mmol CO2 m-2 day-1 for the late spring and 11.2 mmol CO2 m-2 day-1 for the early summer cruises. The spatial variability in ocean pCO2 was associated with surface ocean properties (temperature, salinity and chlorophyll-a concentration) in both the slope and shelf waters. Empirical algorithms for predicting temperature-normalized surface ocean pCO2 as a function of surface ocean properties were shown to perform well in both shelf and slope waters, except (a) within cyclonic eddies produced by baroclinic instability of the Brazil Current as detected by satellite SST imagery and (b) in coastal upwelling regions. In these regions, surface ocean pCO2 values were higher as a result of upwelled CO2-enriched subsurface waters. Finally, a pCO2 algorithm based on both <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/2017AGUFM.C33B1201H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C33B1201H"><span>The Impact of Moisture Intrusions from Lower Latitudes on Arctic Net Surface Radiative <span class="hlt">Fluxes</span> and <span class="hlt">Sea</span> Ice Growth in Fall and Winter</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hegyi, B. M.; Taylor, P. C.</p> <p>2017-12-01</p> <p>The fall and winter seasons mark an important period in the evolution of Arctic <span class="hlt">sea</span> ice, where energy is transferred away from the surface to facilitate the cooling of the surface and the growth of Arctic <span class="hlt">sea</span> ice extent and thickness. Climatologically, these seasons are characterized by distinct periods of increased and reduced surface cooling and <span class="hlt">sea</span> ice growth. Periods of reduced <span class="hlt">sea</span> ice growth and surface cooling are associated with cloudy conditions and the transport of warm and moist <span class="hlt">air</span> from lower latitudes, termed moisture intrusions. In the research presented, we explore the regional and Arctic-wide impact of moisture intrusions on the surface net radiative <span class="hlt">fluxes</span> and <span class="hlt">sea</span> ice growth for each fall and winter season from 2000/01-2015/16, utilizing MERRA2 reanalysis data, PIOMAS <span class="hlt">sea</span> ice thickness data, and daily CERES radiative <span class="hlt">flux</span> data. Consistent with previous studies, we find that positive anomalies in downwelling longwave surface <span class="hlt">flux</span> are associated with increased temperature and water vapor content in the atmospheric column contained within the moisture intrusions. Interestingly, there are periods of increased downwelling LW <span class="hlt">flux</span> anomalies that persist for one week or longer (i.e. longer than synoptic timescales) that are associated with persistent poleward <span class="hlt">flux</span> of warm, moist <span class="hlt">air</span> from lower latitudes. These persistent anomalies significantly reduce the regional growth of Arctic <span class="hlt">sea</span> ice, and may in part explain the interannual variability of fall and winter Arctic <span class="hlt">sea</span> ice growth.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140005396','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140005396"><span>Surface Ocean pCO2 Seasonality and <span class="hlt">Sea-Air</span> CO2 <span class="hlt">Flux</span> 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 pCO2, combined with satellite data, were used to develop pCO2 regional algorithms to analyze the seasonal and interannual variability of surface ocean pCO2 and <span class="hlt">sea-air</span> CO2 <span class="hlt">flux</span> for five physically and biologically distinct regions of the eastern North American continental shelf: the South Atlantic Bight (SAB), the Mid-Atlantic Bight (MAB), the Gulf of Maine (GoM), Nantucket Shoals and Georges Bank (NS+GB), and the Scotian Shelf (SS). Temperature and dissolved inorganic carbon variability are the most influential factors driving the seasonality of pCO2. Estimates of the <span class="hlt">sea-air</span> CO2 <span class="hlt">flux</span> were derived from the available pCO2 data, as well as from the pCO2 reconstructed by the algorithm. Two different gas exchange parameterizations were used. The SS, GB+NS, MAB, and SAB regions are net sinks of atmospheric CO2 while the GoM is a weak source. The estimates vary depending on the use of surface ocean pCO2 from the data or algorithm, as well as with the use of the two different gas exchange parameterizations. Most of the regional estimates are in general agreement with previous studies when the range of uncertainty and interannual variability are taken into account. According to the algorithm, the average annual uptake of atmospheric CO2 by eastern North American continental shelf waters is found to be between 3.4 and 5.4 Tg C/yr (areal average of 0.7 to 1.0 mol CO2 /sq m/yr) over the period 2003-2010.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.4068S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.4068S"><span><span class="hlt">Air-sea</span> heat <span class="hlt">flux</span> climatologies in the Mediterranean <span class="hlt">Sea</span>: Surface energy balance and its consistency with ocean heat storage</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Song, Xiangzhou; Yu, Lisan</p> <p>2017-05-01</p> <p>This study provides an analysis of the Mediterranean <span class="hlt">Sea</span> surface energy budget using nine surface heat <span class="hlt">flux</span> climatologies. The ensemble mean estimation shows that the net downward shortwave radiation (192 ± 19 W m-2) is balanced by latent heat <span class="hlt">flux</span> (-98 ± 10 W m-2), followed by net longwave radiation (-78 ± 13 W m-2) and sensible heat <span class="hlt">flux</span> (-13 ± 4 W m-2). The resulting net heat budget (Qnet) is 2 ± 12 W m-2 into the ocean, which appears to be warm biased. The annual-mean Qnet should be -5.6 ± 1.6 W m-2 when estimated from the observed net transport through the Strait of Gibraltar. To diagnose the uncertainty in nine Qnet climatologies, we constructed Qnet from the heat budget equation by using historic hydrological observations to determine the heat content changes and advective heat <span class="hlt">flux</span>. We also used the Qnet from a data-assimilated global ocean state estimation as an additional reference. By comparing with the two reference Qnet estimates, we found that seven products (NCEP 1, NCEP 2, CFSR, ERA-Interim, MERRA, NOCSv2.0, and OAFlux+ISCCP) overestimate Qnet, with magnitude ranging from 6 to 27 W m-2, while two products underestimate Qnet by -6 W m-2 (JRA55) and -14 W m-2 (CORE.2). Together with the previous warm pool work of Song and Yu (2013), we show that CFSR, MERRA, NOCSv2.0, and OAFlux+ISCCP are warm-biased not only in the western Pacific warm pool but also in the Mediterranean <span class="hlt">Sea</span>, while CORE.2 is cold-biased in both regions. The NCEP 1, 2, and ERA-Interim are cold-biased over the warm pool but warm-biased in the Mediterranean <span class="hlt">Sea</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A14C..03J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A14C..03J"><span><span class="hlt">Air-Sea</span> Interaction in the Somali Current Region</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jensen, T. G.; Rydbeck, A.</p> <p>2017-12-01</p> <p>The western Indian Ocean is an area of high eddy-kinetic energy generated by local wind-stress curl, instability of boundary currents as well as Rossby waves from the west coast of India and the equatorial wave guide as they reflect off the African coast. The presence of meso-scale eddies and coastal upwelling during the Southwest Monsoon affects the <span class="hlt">air-sea</span> interaction on those scales. The U.S. Navy's Coupled Ocean-Atmosphere Mesoscale Prediction System (COAMPS) is used to understand and quantify the surface <span class="hlt">flux</span>, effects on surface waves and the role of <span class="hlt">Sea</span> Surface Temperature anomalies on ocean-atmosphere coupling in that area. The COAMPS atmosphere model component with 9 km resolution is fully coupled to the Navy Coastal Ocean Model (NCOM) with 3.5 km resolution and the Simulating WAves Nearshore (SWAN) wave model with 10 km resolution. Data assimilation using a 3D-variational approach is included in hindcast runs performed daily since June 1, 2015. An interesting result is that a westward jet associated with downwelling equatorial Rossy waves initiated the reversal from the southward Somali Current found during the northeast monsoon to a northward flow in March 2016 more than a month before the beginning of the southwest monsoon. It is also found that warm SST anomalies in the Somali Current eddies, locally increase surface wind speed due to an increase in the atmospheric boundary layer height. This results in an increase in significant wave height and also an increase in heat <span class="hlt">flux</span> to the atmosphere. Cold SST anomalies over upwelling filaments have the opposite impacts on <span class="hlt">air-sea</span> <span class="hlt">fluxes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://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 (2) microwave and acoustic scattering from water surface. The task of our group in this joint effort is to conduct measurements of surface <span class="hlt">fluxes</span> (of momentum, sensible heat, and water vapor) and atmospheric radiation (longwave and shortwave) to achieve our research goal as well as to provide crucial complementary data for the APL studies. The progress of the project is summarized.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016QuRes..85...87C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016QuRes..85...87C"><span>Variability of 14C reservoir age and <span class="hlt">air-sea</span> <span class="hlt">flux</span> of CO2 in the Peru-Chile upwelling region during the past 12,000 years</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carré, Matthieu; Jackson, Donald; Maldonado, Antonio; Chase, Brian M.; Sachs, Julian P.</p> <p>2016-01-01</p> <p>The variability of radiocarbon marine reservoir age through time and space limits the accuracy of chronologies in marine paleo-environmental archives. We report here new radiocarbon reservoir ages (ΔR) from the central coast of Chile ( 32°S) for the Holocene period and compare these values to existing reservoir age reconstructions from southern Peru and northern Chile. Late Holocene ΔR values show little variability from central Chile to Peru. Prior to 6000 cal yr BP, however, ΔR values were markedly increased in southern Peru and northern Chile, while similar or slightly lower-than-modern ΔR values were observed in central Chile. This extended dataset suggests that the early Holocene was characterized by a substantial increase in the latitudinal gradient of marine reservoir age between central and northern Chile. This change in the marine reservoir ages indicates that the early Holocene <span class="hlt">air-sea</span> <span class="hlt">flux</span> of CO2 could have been up to five times more intense than in the late Holocene in the Peruvian upwelling, while slightly reduced in central Chile. Our results show that oceanic circulation changes in the Humboldt system during the Holocene have substantially modified the <span class="hlt">air-sea</span> carbon <span class="hlt">flux</span> in this region.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19820011907','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19820011907"><span>Estimating ocean-<span class="hlt">air</span> heat <span class="hlt">fluxes</span> during cold <span class="hlt">air</span> outbreaks by satellite</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chou, S. H.; Atlas, D.</p> <p>1981-01-01</p> <p>Nomograms of mean column heating due to surface sensible and latent heat <span class="hlt">fluxes</span> were developed. Mean sensible heating of the cloud free region is related to the cloud free path (CFP, the distance from the shore to the first cloud formation) and the difference between land <span class="hlt">air</span> and <span class="hlt">sea</span> surface temperatures, theta sub 1 and theta sub 0, respectively. Mean latent heating is related to the CFP and the difference between land <span class="hlt">air</span> and <span class="hlt">sea</span> surface humidities q sub 1 and q sub 0 respectively. Results are also applicable to any path within the cloud free region. Corresponding heat <span class="hlt">fluxes</span> may be obtained by multiplying the mean heating by the mean wind speed in the boundary layer. The sensible heating estimated by the present method is found to be in good agreement with that computed from the bulk transfer formula. The sensitivity of the solutions to the variations in the initial coastal soundings and large scale subsidence is also investigated. The results are not sensitive to divergence but are affected by the initial lapse rate of potential temperature; the greater the stability, the smaller the heating, other things being equal. Unless one knows the lapse rate at the shore, this requires another independent measurement. For this purpose the downwind slope of the square of the boundary layer height is used, the mean value of which is also directly proportional to the mean sensible heating. The height of the boundary layer should be measurable by future spaceborn lidar systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1713074S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1713074S"><span><span class="hlt">Air-sea</span> <span class="hlt">fluxes</span> and satellite-based estimation of water masses formation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sabia, Roberto; Klockmann, Marlene; Fernandez-Prieto, Diego; Donlon, Craig</p> <p>2015-04-01</p> <p>Recent work linking satellite-based measurements of <span class="hlt">sea</span> surface salinity (SSS) and <span class="hlt">sea</span> surface temperature (SST) with traditional physical oceanography has demonstrated the capability of generating routinely satellite-derived surface T-S diagrams [1] and analyze the distribution/dynamics of SSS and its relative surface density with respect to in-situ measurements. Even more recently [2,3], this framework has been extended by exploiting these T-S diagrams as a diagnostic tool to derive water masses formation rates and areas. A water mass describes a water body with physical properties distinct from the surrounding water, formed at the ocean surface under specific conditions which determine its temperature and salinity. The SST and SSS (and thus also density) at the ocean surface are largely determined by <span class="hlt">fluxes</span> of heat and freshwater. The surface density <span class="hlt">flux</span> is a function of the latter two and describes the change of the density of seawater at the surface. To obtain observations of water mass formation is of great interest, since they serve as indirect observations of the thermo-haline circulation. The SSS data which has become available through the SMOS [4] and Aquarius [5] satellite missions will provide the possibility of studying also the effect of temporally-varying SSS fields on water mass formation. In the present study, the formation of water masses as a function of SST and SSS is derived from the surface density <span class="hlt">flux</span> by integrating the latter over a specific area and time period in bins of SST and SSS and then taking the derivative of the total density <span class="hlt">flux</span> with respect to density. This study presents a test case using SMOS SSS, OSTIA SST, as well as Argo ISAS SST and SSS for comparison, heat <span class="hlt">fluxes</span> from the NOCS Surface <span class="hlt">Flux</span> Data Set v2.0, OAFlux evaporation and CMORPH precipitation. The study area, initially referred to the North Atlantic, is extended over two additional ocean basins and the study period covers the 2011-2012 timeframe. Yearly, seasonal</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006JESS..115..461N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006JESS..115..461N"><span>Monsoon control on trace metal <span class="hlt">fluxes</span> in the deep Arabian <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nair, T. M. Balakrishnan</p> <p>2006-08-01</p> <p>Particulate <span class="hlt">fluxes</span> of aluminium, iron, magnesium and titanium were measured using six time-series sediment traps deployed in the eastern, central and western Arabian <span class="hlt">Sea</span>. Annual Al <span class="hlt">fluxes</span> at shallow and deep trap depths were 0.47 and 0.46 g m-2 in the western Arabian <span class="hlt">Sea</span>, and 0.33 and 0.47 g m-2 in the eastern Arabian <span class="hlt">Sea</span>. There is a difference of about 0.9-1.8 g m-2y-1 in the lithogenic <span class="hlt">fluxes</span> determined analytically (residue remaining after leaching out all biogenic particles) and estimated from the Al <span class="hlt">fluxes</span> in the western Arabian <span class="hlt">Sea</span>. This arises due to higher <span class="hlt">fluxes</span> of Mg (as dolomite) in the western Arabian <span class="hlt">Sea</span> (6-11 times higher than the eastern Arabian <span class="hlt">Sea</span>). The estimated dolomite <span class="hlt">fluxes</span> at the western Arabian <span class="hlt">Sea</span> site range from 0.9 to 1.35gm-2y-1. Fe <span class="hlt">fluxes</span> in the Arabian <span class="hlt">Sea</span> were less than that of the reported atmospheric <span class="hlt">fluxes</span> without any evidence for the presence of labile fraction/excess of Fe in the settling particles. More than 75% of Al, Fe, Ti and Mg <span class="hlt">fluxes</span> occurred during the southwest (SW) monsoon in the western Arabian <span class="hlt">Sea</span>. In the eastern Arabian <span class="hlt">Sea</span>, peak Al, Fe, Mg and Ti <span class="hlt">fluxes</span> were recorded during both the northeast (NE) and SW monsoons. During the SW monsoon, there exists a time lag of around one month between the increases in lithogenic and dolomite <span class="hlt">fluxes</span>. Total lithogenic <span class="hlt">fluxes</span> increase when the southern branch of dust bearing northwesterlies is dragged by the SW monsoon winds to the trap locations. However, the dolomite <span class="hlt">fluxes</span> increase only when the northern branch of the northwesterlies (which carries a huge amount of dolomite accounting 60% of the total dust load) is dragged, from further north, by SW monsoon winds. The potential for the use of Mg/Fe ratio as a paleo-monsoonal proxy is examined.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150002539','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150002539"><span>Assessing <span class="hlt">Air-Sea</span> Interaction in the Evolving NASA GEOS Model</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Clayson, Carol Anne; Roberts, J. Brent</p> <p>2015-01-01</p> <p>In order to understand how the climate responds to variations in forcing, one necessary component is to understand the full distribution of variability of exchanges of heat and moisture between the atmosphere and ocean. Surface heat and moisture <span class="hlt">fluxes</span> are critical to the generation and decay of many coupled <span class="hlt">air-sea</span> phenomena. These mechanisms operate across a number of scales and contain contributions from interactions between the anomalous (i.e. non-mean), often extreme-valued, <span class="hlt">flux</span> components. Satellite-derived estimates of the surface turbulent and radiative heat <span class="hlt">fluxes</span> provide an opportunity to assess results from modeling systems. Evaluation of only time mean and variability statistics, however only provides limited traceability to processes controlling what are often regime-dependent errors. This work will present an approach to evaluate the representation of the turbulent <span class="hlt">fluxes</span> at the <span class="hlt">air-sea</span> interface in the current and evolving Goddard Earth Observing System (GEOS) model. A temperature and moisture vertical profile-based clustering technique is used to identify robust weather regimes, and subsequently intercompare the turbulent <span class="hlt">fluxes</span> and near-surface parameters within these regimes in both satellite estimates and GEOS-driven data sets. Both model reanalysis (MERRA) and seasonal-to-interannual coupled GEOS model simulations will be evaluated. Particular emphasis is placed on understanding the distribution of the <span class="hlt">fluxes</span> including extremes, and the representation of near-surface forcing variables directly related to their estimation. Results from these analyses will help identify the existence and source of regime-dependent biases in the GEOS model ocean surface turbulent <span class="hlt">fluxes</span>. The use of the temperature and moisture profiles for weather-state clustering will be highlighted for its potential broad application to 3-D output typical of model simulations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.A41P..05C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.A41P..05C"><span>Assessing <span class="hlt">air-sea</span> interaction in the evolving NASA GEOS model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Clayson, C. A.; Roberts, J. B.</p> <p>2014-12-01</p> <p>In order to understand how the climate responds to variations in forcing, one necessary component is to understand the full distribution of variability of exchanges of heat and moisture between the atmosphere and ocean. Surface heat and moisture <span class="hlt">fluxes</span> are critical to the generation and decay of many coupled <span class="hlt">air-sea</span> phenomena. These mechanisms operate across a number of scales and contain contributions from interactions between the anomalous (i.e. non-mean), often extreme-valued, <span class="hlt">flux</span> components. Satellite-derived estimates of the surface turbulent and radiative heat <span class="hlt">fluxes</span> provide an opportunity to assess results from modeling systems. Evaluation of only time mean and variability statistics, however only provides limited traceability to processes controlling what are often regime-dependent errors. This work will present an approach to evaluate the representation of the turbulent <span class="hlt">fluxes</span> at the <span class="hlt">air-sea</span> interface in the current and evolving Goddard Earth Observing System (GEOS) model. A temperature and moisture vertical profile-based clustering technique is used to identify robust weather regimes, and subsequently intercompare the turbulent <span class="hlt">fluxes</span> and near-surface parameters within these regimes in both satellite estimates and GEOS-driven data sets. Both model reanalysis (MERRA) and seasonal-to-interannual coupled GEOS model simulations will be evaluated. Particular emphasis is placed on understanding the distribution of the <span class="hlt">fluxes</span> including extremes, and the representation of near-surface forcing variables directly related to their estimation. Results from these analyses will help identify the existence and source of regime-dependent biases in the GEOS model ocean surface turbulent <span class="hlt">fluxes</span>. The use of the temperature and moisture profiles for weather-state clustering will be highlighted for its potential broad application to 3-D output typical of model simulations.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li class="active"><span>5</span></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_5 --> <div id="page_6" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li class="active"><span>6</span></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="101"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A43G2559J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A43G2559J"><span>Seasonal atmospheric deposition and <span class="hlt">air-sea</span> gaseous exchange of polycyclic aromatic hydrocarbons over the Yangtze River Estuary, East China <span class="hlt">Sea</span>: Implication for the source-sink processes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jiang, Y.; Guo, Z.</p> <p>2017-12-01</p> <p>As the home of the largest port in the world, the Yangtze River Estuary (YRE) in the East China <span class="hlt">Sea</span> (ECS) is adjacent to the largest economic zone in China with more than 10% of Chinese population and provides one-fifth of national GDP. The YRE is under the path of contaminated East Asian continental outflow. These make the YRE unique for the pollutant biogeochemical cycling in the world. In this work, 94 pairs of <span class="hlt">air</span> samples and 20 surface seawater samples covering four seasons were collected from a remote receptor site in the YRE from March 2014 to January 2015, in order to explore the seasonal <span class="hlt">fluxes</span> of <span class="hlt">air-sea</span> gaseous exchange and atmospheric dry and wet deposition of 15 polycyclic aromatic hydrocarbons (PAHs) and their source-sink processes at the <span class="hlt">air-sea</span> interface. The average dry and wet deposition <span class="hlt">fluxes</span> of 15 PAHs were estimated as 879 ± 1393 ng m-2 d-1 and 755 ± 545 ng m-2 d-1, respectively. The gaseous PAHs were released from seawater to atmosphere during the whole year with an average of 3039 ± 2030 ng m-2 d-1. The gaseous exchange of PAHs was referred as the dominant process at the <span class="hlt">air-sea</span> interface in the YRE as the magnitude of volatilization <span class="hlt">flux</span> of PAHs exceeded that of the total dry and wet deposition. The gaseous PAH exchange <span class="hlt">flux</span> was dominated by 3-ring PAHs, with the highest value in summer while lowest in winter, depicting a strong seasonal variation due to temperature, wind speed and <span class="hlt">air-sea</span> concentration gradient difference among seasons. Based on the simplified mass balance estimation, net 9.6 tons/y of PAHs was volatilized from seawater to atmosphere with an area of approximately 20000 km2 in the YRE. Apart from Yangtze River input and ocean ship emissions in the entire year, the selective release of low molecular weight PAHs from sediments in winter due to re-suspension triggered by the East Asian winter monsoon could be another possible source for dissolved PAHs. This work suggests that the source-sink processes of PAHs at <span class="hlt">air-sea</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeoRL..44.3887K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoRL..44.3887K"><span><span class="hlt">Air-Sea</span> exchange of biogenic volatile organic compounds and the impact on aerosol particle size distributions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kim, Michelle J.; Novak, Gordon A.; Zoerb, Matthew C.; Yang, Mingxi; Blomquist, Byron W.; Huebert, Barry J.; Cappa, Christopher D.; Bertram, Timothy H.</p> <p>2017-04-01</p> <p>We report simultaneous, underway eddy covariance measurements of the vertical <span class="hlt">flux</span> of isoprene, total monoterpenes, and dimethyl sulfide (DMS) over the Northern Atlantic Ocean during fall. Mean isoprene and monoterpene <span class="hlt">sea-to-air</span> vertical <span class="hlt">fluxes</span> were significantly lower than mean DMS <span class="hlt">fluxes</span>. While rare, intense monoterpene <span class="hlt">sea-to-air</span> <span class="hlt">fluxes</span> were observed, coincident with elevated monoterpene mixing ratios. A statistically significant correlation between isoprene vertical <span class="hlt">flux</span> and short wave radiation was not observed, suggesting that photochemical processes in the surface microlayer did not enhance isoprene emissions in this study region. Calculations of secondary organic aerosol production rates (PSOA) for mean isoprene and monoterpene emission rates sampled here indicate that PSOA is on average <0.1 μg m-3 d-1. Despite modest PSOA, low particle number concentrations permit a sizable role for condensational growth of monoterpene oxidation products in altering particle size distributions and the concentration of cloud condensation nuclei during episodic monoterpene emission events from the ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17706251','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17706251"><span><span class="hlt">Air--sea</span> gaseous exchange of PCB at the Venice lagoon (Italy).</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Manodori, L; Gambaro, A; Moret, I; Capodaglio, G; Cescon, P</p> <p>2007-10-01</p> <p>Water bodies are important storage media for persistent organic pollutants (POPs) such as polychlorinated biphenyls (PCBs) and this function is increased in coastal regions because their inputs are higher than those to the open <span class="hlt">sea</span>. The <span class="hlt">air</span>-water interface is extensively involved with the global cycling of PCBs because it is the place where they accumulate due to depositional processes and where they may be emitted by gaseous exchange. In this work the parallel collection of <span class="hlt">air</span>, microlayer and sub-superficial water samples was performed in July 2005 at a site in the Venice lagoon to evaluate the summer gaseous <span class="hlt">flux</span> of PCBs. The total concentration of PCBs (sum of 118 congeners) in <span class="hlt">air</span> varies from 87 to 273 pg m(-3), whereas in the operationally defined dissolved phase of microlayer and sub-superficial water samples it varies from 159 to 391 pg L(-1). No significant enrichment of dissolved PCB into the microlayer has been observed, although a preferential accumulation of most hydrophobic congeners occurs. Due to this behaviour, we believe that the modified two-layer model was the most suitable approach for the evaluation of the <span class="hlt">flux</span> at the <span class="hlt">air-sea</span> interface, because it takes into account the influence of the microlayer. From its application it appears that PCB volatilize from the lagoon waters with a net <span class="hlt">flux</span> varying from 58 to 195 ng m(-2)d(-1) (uncertainty: +/-50-64%) due to the strong influence of wind speed. This <span class="hlt">flux</span> is greater than those reported in the literature for the atmospheric deposition and rivers input and reveals that PCB are actively emitted from the Venice lagoon in summer months.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('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-2 and stronger). <span class="hlt">Air-sea</span> coupling damps TCs growth through a reduction of inner-core upward enthalpy <span class="hlt">fluxes</span> due to the TC-induced cooling. This reduction is particularly large for the most intense TCs of the northern Indian Ocean (up to 250 W m-2), due to higher ambient surface temperatures and larger TC-induced cooling there. The negative feedback of <span class="hlt">air-sea</span> coupling on strongest TCs is mainly associated with slow-moving storms, which spend more time over the cold wake they induce. Sensitivity experiments using a different convective parameterization yield qualitatively similar results, with a larger ( 65%) reduction in the number of TCs. Because of their relatively coarse resolution (¼°), both set of experiments however fail to reproduce the most intense observed TCs. Further studies with finer resolution models in the Bay of Bengal will be needed to assess the expectedly large impact of <span class="hlt">air-sea</span> coupling on those intense and deadly TCs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMOS33A1443Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMOS33A1443Y"><span>Diagnosing CO2 <span class="hlt">fluxes</span> and seasonality in the Arabian <span class="hlt">Sea</span> as an Ocean-Dominated Margin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, W.; Dai, M.</p> <p>2017-12-01</p> <p>The Arabian <span class="hlt">Sea</span> is a large marginal <span class="hlt">sea</span> of the Indian Ocean characterized by highly predictable annual circulation cycle driven by Asian monsoon. The Arabian <span class="hlt">Sea</span> is generally sources to atmospheric CO2. In this study, we applied the physical-biogeochemical coupled approach previously adopted for diagnosis of CO2 <span class="hlt">fluxes</span> in Ocean-dominated margin (OceMar) to assesses the CO2 <span class="hlt">fluxes</span> and their seasonality in Arabian <span class="hlt">Sea</span> using data collected during five US JGOFS Arabian <span class="hlt">Sea</span> Process Study cruises (ttn-043, ttn-045, ttn-049, ttn-053, ttn-054) conducted from September 1994 to December 1995. The pCO2 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 pCO2 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 pCO2 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> CO2 exchange should be accounted for. This presentation will also examine the seasonality of the CO2 dynamics and its controls.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JGRC..121.8787G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JGRC..121.8787G"><span>Assessing recent <span class="hlt">air-sea</span> freshwater <span class="hlt">flux</span> changes using a surface temperature-salinity space framework</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Grist, Jeremy P.; Josey, Simon A.; Zika, Jan D.; Evans, Dafydd Gwyn; Skliris, Nikolaos</p> <p>2016-12-01</p> <p>A novel assessment of recent changes in <span class="hlt">air-sea</span> freshwater <span class="hlt">fluxes</span> has been conducted using a surface temperature-salinity framework applied to four atmospheric reanalyses. Viewed in the T-S space of the ocean surface, the complex pattern of the longitude-latitude space mean global Precipitation minus Evaporation (PME) reduces to three distinct regions. The analysis is conducted for the period 1979-2007 for which there is most evidence for a broadening of the (atmospheric) tropical belt. All four of the reanalyses display an increase in strength of the water cycle. The range of increase is between 2% and 30% over the period analyzed, with an average of 14%. Considering the average across the reanalyses, the water cycle changes are dominated by changes in tropical as opposed to mid-high latitude precipitation. The increases in the water cycle strength, are consistent in sign, but larger than in a 1% greenhouse gas run of the HadGEM3 climate model. In the model a shift of the precipitation/evaporation cells to higher temperatures is more evident, due to the much stronger global warming signal. The observed changes in freshwater <span class="hlt">fluxes</span> appear to be reflected in changes in the T-S distribution of the Global Ocean. Specifically, across the diverse range of atmospheric reanalyses considered here, there was an acceleration of the hydrological cycle during 1979-2007 which led to a broadening of the ocean's salinity distribution. Finally, although the reanalyses indicate that the warm temperature tropical precipitation dominated water cycle change, ocean observations suggest that ocean processes redistributed the freshening to lower ocean temperatures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMOS33A1438C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMOS33A1438C"><span>Seasonal and spatial variations in surface pCO2 and <span class="hlt">air-sea</span> CO2 <span class="hlt">flux</span> 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 (pCO2) were conducted in May, June, August, and October 2016 to study the spatial and seasonal variations in surface pCO2 and to estimate <span class="hlt">air-sea</span> CO2 <span class="hlt">flux</span> in the Chesapeake Bay. Overall, high surface pCO2 in the upper-bay decreased downstream rapidly below the atmospheric value near the bay bridge in the mid-bay and then increased slightly to the lower-bay where pCO2 approached the atmospheric level. Over the course of a year, pCO2 was higher than 1000 µatm in the upper bay and the highest pCO2 (2500 µatm) was observed in August. Significant biologically-induced pCO2 undersaturation was observed at the upper part of the mid-bay in August with pCO2 as low as 50 µatm and oversaturated DO% of 200%. In addition to biological control, vertical mixing and upwelling controlled by wind direction and tidal stage played an important role in controlling surface pCO2 in the mid-bay as is evidenced by co-occurrence of high pCO2 with low temperature and low oxygen or high salinity from the subsurface. These physical processes occurred regularly and in short time scale of hours, suggesting they must be considered in the assessment of annual <span class="hlt">air-sea</span> CO2 <span class="hlt">flux</span>. Seasonally, the upper-bay acted as a source for atmospheric CO2 over the course of a year. The boundary of upper and mid bay transited from a CO2 source to a sink from May to August and was a source again in October due to strong biological production in summer. In contrast, the mid-bay represented as a CO2 source with large temporal variation due to dynamic hydrographic settings. The lower-bay transited from a weak sink in May to equilibrated with the atmosphere from June to August, while became a source again in October. Moreover, the CO2 <span class="hlt">flux</span> 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/2012EGUGA..14..742J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..14..742J"><span>In situ evaluation of <span class="hlt">air-sea</span> CO2 gas transfer velocity in an inner estuary using eddy covariance - with a special focus on the importance of using reliable CO2-<span class="hlt">fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jørgensen, E. T.; Sørensen, L. L.; Jensen, B.; Sejr, M. K.</p> <p>2012-04-01</p> <p>The <span class="hlt">air-sea</span> exchange of CO2 or CO2 <span class="hlt">flux</span> 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 <span class="hlt">air-sea</span> <span class="hlt">flux</span> is the parameterization of k. As an example; the estimated global <span class="hlt">air-sea</span> <span class="hlt">flux</span> increases by 70 % when using the parameterization by Wanninkhof and McGillis (1999) instead of Wanninkhof (1992) (Rutgersson et al., 2008). In coastal areas the uncertainty is even higher and only few studies have focused on determining transfer velocity for the coastal waters and even fewer on estuaries (Borges et al., 2004;Rutgersson et al., 2008). The transfer velocity (k600) of CO2 in the inner estuary of Roskilde Fjord, Denmark was investigated using eddy covariance CO2 <span class="hlt">fluxes</span> (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 <span class="hlt">air</span> and water influence k600. The wind speed parameterization of k600 using DS1 showed some scatter but when including IDM the 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 <span class="hlt">fluxes</span> calculated by the ECM are removed when including the IDM.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/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> CO2 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> CO2 <span class="hlt">flux</span> over the Baltic <span class="hlt">Sea</span> based on remote sensing data: estimates of pCO2 derived from satellite imaging using self-organizing map classifications along with class-specific linear regressions (SOMLO methodology) and remotely sensed wind estimates. The estimates have a spatial resolution of 4 km both in latitude and longitude and a monthly temporal resolution from 1998 to 2011. The CO2 <span class="hlt">fluxes</span> are estimated using two types of wind products, i.e. reanalysis winds and satellite wind products, the higher-resolution wind product generally leading to higher-amplitude <span class="hlt">flux</span> estimations. Furthermore, the CO2 <span class="hlt">fluxes</span> were also estimated using two methods: the method of Wanninkhof et al. (2013) and the method of Rutgersson and Smedman (2009). The seasonal variation in <span class="hlt">fluxes</span> reflects the seasonal variation in pCO2 unvaryingly over the whole Baltic <span class="hlt">Sea</span>, with high winter CO2 emissions and high pCO2 uptakes. All basins act as a source for the atmosphere, with a higher degree of emission in the southern regions (mean source of 1.6 mmol m-2 d-1 for the South Basin and 0.9 for the Central Basin) than in the northern regions (mean source of 0.1 mmol m-2 d-1) and the coastal areas act as a larger sink (annual uptake of -4.2 mmol m-2 d-1) than does the open <span class="hlt">sea</span> (-4 mmol m-2 d-1). In its entirety, the Baltic <span class="hlt">Sea</span> acts as a small source of 1.2 mmol m-2 d-1 on average and this annual uptake has increased from 1998 to 2012.</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; (2) improve regional-scale meteorological and <span class="hlt">air</span> quality modeling; and (3) provide a framework for advanced offshore measurements to support future needs such as emergency response, exploration and lease decisions, wind energy research and development, and meteorological and <span class="hlt">air</span> quality forecasting. In October 2010, meteorological and oceanographic sensors were deployed for an extended period (approximately 12 months) on a Chevron service platform (ST 52B, 90.5W, 29N) to collect boundary layer and <span class="hlt">sea</span> surface data sufficient to support these objectives. This project has significant importance given the large industrial presence in the Gulf, sizeable regional population nearby, and the recognized need for precise and timely pollutant forecasts. Observations from this project include surface meteorology; sodar marine boundary layer winds; microwave radiometer profiles of temperature, relative humidity, and liquid water; ceilometer cloud base heights; water temperature and current profiles; <span class="hlt">sea</span> surface temperature; wave height statistics; downwelling solar and infrared radiation; and <span class="hlt">air-sea</span> turbulent momentum and heat <span class="hlt">fluxes</span>. This project resulted in the collection of an unprecedented set of boundary layer measurements over the Gulf of Mexico that capture the range of meteorological and oceanographic interactions and processes that occur over an entire year. This presentation will provide insight into the logistical and scientific issues associated with the deployment and operations of unique measurements in offshore areas and provide results from an initial data analysis of boundary layer processes over the Gulf of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013ACPD...1313285B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013ACPD...1313285B"><span><span class="hlt">Air/sea</span> DMS gas transfer in the North Atlantic: evidence for limited interfacial gas exchange at high wind speed</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bell, T. G.; De Bruyn, W.; Miller, S. D.; Ward, B.; Christensen, K.; Saltzman, E. S.</p> <p>2013-05-01</p> <p>Shipboard measurements of eddy covariance DMS <span class="hlt">air/sea</span> <span class="hlt">fluxes</span> and seawater concentration were carried out in the North Atlantic bloom region in June/July 2011. Gas transfer coefficients (k660) show a linear dependence on mean horizontal wind speed at wind speeds up to 11 m s-1. At higher wind speeds the relationship between k660 and wind speed weakens. At high winds, measured DMS <span class="hlt">fluxes</span> were lower than predicted based on the linear relationship between wind speed and interfacial stress extrapolated from low to intermediate wind speeds. In contrast, the transfer coefficient for sensible heat did not exhibit this effect. The apparent suppression of <span class="hlt">air/sea</span> gas <span class="hlt">flux</span> at higher wind speeds appears to be related to <span class="hlt">sea</span> state, as determined from shipboard wave measurements. These observations are consistent with the idea that long waves suppress near surface water side turbulence, and decrease interfacial gas transfer. This effect may be more easily observed for DMS than for less soluble gases, such as CO2, because the <span class="hlt">air/sea</span> exchange of DMS is controlled by interfacial rather than bubble-mediated gas transfer under high wind speed conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017APS..DFDL20011S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..DFDL20011S"><span>Boundary layers at a dynamic interface: <span class="hlt">air-sea</span> exchange of heat and mass</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Szeri, Andrew</p> <p>2017-11-01</p> <p>Exchange of mass or heat across a turbulent liquid-gas interface is a problem of critical interest, especially in <span class="hlt">air-sea</span> transfer of natural and man-made gases involved in climate change. The goal in this research area is to determine the gas <span class="hlt">flux</span> from <span class="hlt">air</span> to <span class="hlt">sea</span> or vice versa. For sparingly soluble non-reactive gases, this is controlled by liquid phase turbulent velocity fluctuations that act on the thin species concentration boundary layer on the liquid side of the interface. If the fluctuations in surface-normal velocity and gas concentration differences are known, then it is possible to determine the turbulent contribution to the gas <span class="hlt">flux</span>. However, there is no suitable fundamental direct approach in the general case where neither of these quantities can be easily measured. A new approach is presented to deduce key aspects about the near-surface turbulent motions from remote measurements, which allows one to determine the gas transfer velocity, or gas <span class="hlt">flux</span> per unit area if overall concentration differences are known. The approach is illustrated with conceptual examples.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001asi..book.....C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001asi..book.....C"><span><span class="hlt">Air-Sea</span> Interaction</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Csanady, G. T.</p> <p>2001-03-01</p> <p>In recent years <span class="hlt">air-sea</span> interaction has emerged as a subject in its own right, encompassing small-scale and large-scale processes in both <span class="hlt">air</span> and <span class="hlt">sea</span>. <span class="hlt">Air-Sea</span> Interaction: Laws and Mechanisms is a comprehensive account of how the atmosphere and the ocean interact to control the global climate, what physical laws govern this interaction, and its prominent mechanisms. The topics covered range from evaporation in the oceans, to hurricanes, and on to poleward heat transport by the oceans. By developing the subject from basic physical (thermodynamic) principles, the book is accessible to graduate students and research scientists in meteorology, oceanography, and environmental engineering. It will also be of interest to the broader physics community involved in the treatment of transfer laws, and thermodynamics of the atmosphere and ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26931659','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26931659"><span><span class="hlt">Air-sea</span> exchange of gaseous mercury in the tropical coast (Luhuitou fringing reef) of the South China <span class="hlt">Sea</span>, the Hainan Island, China.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ci, Zhijia; Zhang, Xiaoshan; Wang, Zhangwei</p> <p>2016-06-01</p> <p>The <span class="hlt">air-sea</span> exchange of gaseous mercury (mainly Hg(0)) in the tropical ocean is an important part of the global Hg biogeochemical cycle, but the related investigations are limited. In this study, we simultaneously measured Hg(0) concentrations in surface waters and overlaying <span class="hlt">air</span> in the tropical coast (Luhuitou fringing reef) of the South China <span class="hlt">Sea</span> (SCS), Hainan Island, China, for 13 days on January-February 2015. The purpose of this study was to explore the temporal variation of Hg(0) concentrations in <span class="hlt">air</span> and surface waters, estimate the <span class="hlt">air-sea</span> Hg(0) <span class="hlt">flux</span>, and reveal their influencing factors in the tropical coastal environment. The mean concentrations (±SD) of Hg(0) in <span class="hlt">air</span> and total Hg (THg) in waters were 2.34 ± 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 (2) = 0.42, p < 0.001). Surface waters were always supersaturated with Hg(0) compared to <span class="hlt">air</span> (the degree of saturation, 2.46 to 13.87), indicating that the surface water was one of the atmospheric Hg(0) sources. The <span class="hlt">air-sea</span> Hg(0) <span class="hlt">fluxes</span> were estimated to be 1.73 ± 1.25 ng m(-2) h(-1) with a large range between 0.01 and 6.06 ng m(-2) h(-1). The high variation of Hg(0) <span class="hlt">fluxes</span> was mainly attributed to the greatly temporal variation of wind speed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFMOS34B..01S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMOS34B..01S"><span>Tropical Cyclone Induced <span class="hlt">Air-Sea</span> Interactions Over Oceanic Fronts</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shay, L. K.</p> <p>2012-12-01</p> <p>Recent severe tropical cyclones underscore the inherent importance of warm background ocean fronts and their interactions with the atmospheric boundary layer. Central to the question of heat and moisture <span class="hlt">fluxes</span>, the amount of heat available to the tropical cyclone is predicated by the initial mixed layer depth and strength of the stratification that essentially set the level of entrainment mixing at the base of the mixed layer. In oceanic regimes where the ocean mixed layers are thin, shear-induced mixing tends to cool the upper ocean to form cold wakes which reduces the <span class="hlt">air-sea</span> <span class="hlt">fluxes</span>. This is an example of negative feedback. By contrast, in regimes where the ocean mixed layers are deep (usually along the western part of the gyres), warm water advection by the nearly steady currents reduces the levels of turbulent mixing by shear instabilities. As these strong near-inertial shears are arrested, more heat and moisture transfers are available through the enthalpy <span class="hlt">fluxes</span> (typically 1 to 1.5 kW m-2) 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://ntrs.nasa.gov/search.jsp?R=20060032490&hterms=sonar&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dsonar','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060032490&hterms=sonar&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dsonar"><span>Combined Satellite - and ULS-Derived <span class="hlt">Sea</span>-Ice <span class="hlt">Flux</span> in the Weddell <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Drinkwater, M.; Liu, X.; Harms, S.</p> <p>2000-01-01</p> <p>Several years of daily microwave satellite ice-drift are combined with moored Upward Looking Sonar (ULS) ice-drafts into an ice volume <span class="hlt">flux</span> record at points along a <span class="hlt">flux</span> gate across the Weddell <span class="hlt">Sea</span>, Antarctica.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013ACP....1311073B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013ACP....1311073B"><span><span class="hlt">Air-sea</span> dimethylsulfide (DMS) gas transfer in the North Atlantic: evidence for limited interfacial gas exchange at high wind speed</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bell, T. G.; De Bruyn, W.; Miller, S. D.; Ward, B.; Christensen, K.; Saltzman, E. S.</p> <p>2013-11-01</p> <p>Shipboard measurements of eddy covariance dimethylsulfide (DMS) <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> and seawater concentration were carried out in the North Atlantic bloom region in June/July 2011. Gas transfer coefficients (k660) show a linear dependence on mean horizontal wind speed at wind speeds up to 11 m s-1. At higher wind speeds the relationship between k660 and wind speed weakens. At high winds, measured DMS <span class="hlt">fluxes</span> were lower than predicted based on the linear relationship between wind speed and interfacial stress extrapolated from low to intermediate wind speeds. In contrast, the transfer coefficient for sensible heat did not exhibit this effect. The apparent suppression of <span class="hlt">air-sea</span> gas <span class="hlt">flux</span> at higher wind speeds appears to be related to <span class="hlt">sea</span> state, as determined from shipboard wave measurements. These observations are consistent with the idea that long waves suppress near-surface water-side turbulence, and decrease interfacial gas transfer. This effect may be more easily observed for DMS than for less soluble gases, such as CO2, because the <span class="hlt">air-sea</span> exchange of DMS is controlled by interfacial rather than bubble-mediated gas transfer under high wind speed conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006GeoRL..3314803Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006GeoRL..3314803Z"><span>Impacts of winter storms on <span class="hlt">air-sea</span> gas exchange</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, Weiqing; Perrie, Will; Vagle, Svein</p> <p>2006-07-01</p> <p>The objective of this study is to investigate <span class="hlt">air-sea</span> gas exchange during winter storms, using field measurements from Ocean Station Papa in the Northeast Pacific (50°N, 145°W). We show that increasing gas transfer rates are coincident with increasing winds and deepening depth of bubble penetration, and that this process depends on <span class="hlt">sea</span> state. Wave-breaking is shown to be an important factor in the gas transfer velocity during the peaks of the storms, increasing the <span class="hlt">flux</span> rates by up to 20%. Gas transfer rates and concentrations can exhibit asymmetry, reflecting a sudden increase with the onset of a storm, and gradual recovery stages.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOS.A23A..04C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOS.A23A..04C"><span><span class="hlt">Air-Sea</span> Momentum and Enthalpy Exchange in Coupled Atmosphere-Wave-Ocean Modeling of Tropical Cyclones</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Curcic, M.; Chen, S. S.</p> <p>2016-02-01</p> <p>The atmosphere and ocean are coupled through momentum, enthalpy, and mass <span class="hlt">fluxes</span>. Accurate representation of these <span class="hlt">fluxes</span> in a wide range of weather and climate conditions is one of major challenges in prediction models. Their current parameterizations are based on sparse observations in low-to-moderate winds and are not suited for high wind conditions such as tropical cyclones (TCs) and winter storms. In this study, we use the Unified Wave INterface - Coupled Model (UWIN-CM), a high resolution, fully-coupled atmosphere-wave-ocean model, to better understand the role of ocean surface waves in mediating <span class="hlt">air-sea</span> momentum and enthalpy exchange in TCs. In particular, we focus on the explicit treatment of wave growth and dissipation for calculating atmospheric and oceanic stress, and its role in upper ocean mixing and surface cooling in the wake of the storm. Wind-wave misalignment and local wave disequilibrium result in difference between atmospheric and oceanic stress being largest on the left side of the storm. We find that explicit wave calculation in the coupled model reduces momentum transfer into the ocean by more than 10% on average, resulting in reduced cooling in TC's wake and subsequent weakening of the storm. We also investigate the impacts of <span class="hlt">sea</span> surface temperature and upper ocean parameterization on <span class="hlt">air-sea</span> enthalpy <span class="hlt">fluxes</span> in the fully coupled model. High-resolution UWIN-CM simulations of TCs with various intensities and structure are conducted in this study to better understand the complex TC-ocean interaction and improve the representation of <span class="hlt">air-sea</span> coupling processes in coupled prediction models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUSM.A23B..01K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUSM.A23B..01K"><span><span class="hlt">Air-Sea</span> Interaction in the Gulf of Tehuantepec</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Khelif, D.; Friehe, C. A.; Melville, W. K.</p> <p>2007-05-01</p> <p>Measurements of meteorological fields and turbulence were made during gap wind events in the Gulf of Tehuantepec using the NSF C-130 aircraft. The flight patterns started at the shore and progressed to approximately 300km offshore with low-level (30m) tracks, stacks and soundings. Parameterizations of the wind stress, sensible and latent heat <span class="hlt">fluxes</span> were obtained from approximately 700 5 km low-level tracks. Structure of the marine boundary layer as it evolved off-shore was obtained with stack patterns, aircraft soundings and deployment of dropsondes. The <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> approximately follow previous parameterizations with some evidence of the drag coefficient leveling out at about 20 meters/sec with the latent heat <span class="hlt">flux</span> slightly increasing. The boundary layer starts at shore as a gap wind low-level jet, thins as the jet expands out over the gulf, exhibits a hydraulic jump, and then increases due to turbulent mixing.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li class="active"><span>6</span></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_6 --> <div id="page_7" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li class="active"><span>7</span></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="121"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JMS...173...70C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JMS...173...70C"><span><span class="hlt">Air-sea</span> CO2 <span class="hlt">fluxes</span> for the Brazilian northeast continental shelf in a climatic transition region</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carvalho, A. C. O.; Marins, R. V.; Dias, F. J. S.; Rezende, C. E.; Lefèvre, N.; Cavalcante, M. S.; Eschrique, S. A.</p> <p>2017-09-01</p> <p>Oceanographic cruises were carried out in October 2012 (3°S-5°S and 38,5°W-35,5°W) and in September 2014 (1°S-4°S and 43°W-37°W), measuring atmospheric and <span class="hlt">sea</span> surface CO2 fugacity (fCO2) 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 fCO2sw, in October 2012, was in average 400.9 ± 7.3μatm and 391.1 ± 6.3 μatm in September 2014. For the atmosphere, the fCO2<span class="hlt">air</span> in October 2012 was 375.8 ± 2.0 μatm and in September 2014, 368.9 ± 2.2 μatm. The super-saturation of the seawater in relation to the atmosphere indicates a source of CO2 to the atmosphere. The entire study area presents oligotrophic conditions. Despite the low concentrations, Chl a and nutrients presented significant influence on fCO2sw, particularly in the westernmost and more humid part of the northeast coast, where river <span class="hlt">fluxes</span> are three orders of magnitude larger than eastern rivers and rainfall events are more intense and constant. fCO2sw 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 fCO2sw at the eastern portion was controlled by parameters such as temperature and salinity. At the western portion, fCO2sw was influenced by nutrient and Chl a. Calculated instantaneous CO2 <span class="hlt">flux</span> ranged from + 1.66 to + 7.24 mmol m- 2 d- 1 in the first cruise and + 0.89 to + 14.62 mmol m- 2 d- 1 in the second cruise.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25639080','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25639080"><span>[Distribution, <span class="hlt">flux</span> and biological consumption of carbon monoxide in the East China <span class="hlt">Sea</span> and the South Yellow <span class="hlt">Sea</span> in summer].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Jing; Lu, Xiao-Lan; Yang, Gui-Peng; Xu, Guan-Qiu</p> <p>2014-11-01</p> <p>Carbon monoxide (CO) concentration distribution, <span class="hlt">sea-to-air</span> <span class="hlt">flux</span> and microbial consumption rate constant, along with atmospheric CO 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 CO 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 CO displayed a decreasing trend from the coastal stations to the offshore stations. The surface water CO concentrations in the investigated area ranged from 0.23-7.10 nmol x L(-1), with an average of 2.49 nmol x L(-1) (SD = 2.11, n = 36). The surface water CO concentrations were significantly affected by sunlight. Vertical profiles showed that CO concentrations rapidly declined with depth, with the maximum values appearing in the surface water. CO 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 CO all occurred before dawn. However, the maximal concentrations of CO occurred at noon. Marked diurnal variation in the concentrations of CO in the water column indicated that CO was produced primarily by photochemistry. The surface CO 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 CO. The <span class="hlt">sea-to-air</span> <span class="hlt">fluxes</span> of CO 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 (m2 x d)(-1), with an average of 12.73 μmol x (m2 x d)(-1) (SD = 11.40, n = 29). In the incubation experiments, CO concentrations decreased exponentially with incubation time and the processes conformed to the first order reaction characteristics. The microbial CO consumption rate constants (K(co)) 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/24952420','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24952420"><span>Methods, <span class="hlt">fluxes</span> and sources of gas phase alkyl nitrates in the coastal <span class="hlt">air</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Dirtu, Alin C; Buczyńska, Anna J; Godoi, Ana F L; Favoreto, Rodrigo; Bencs, László; Potgieter-Vermaak, Sanja S; Godoi, Ricardo H M; Van Grieken, René; Van Vaeck, Luc</p> <p>2014-10-01</p> <p>The daily and seasonal atmospheric concentrations, deposition <span class="hlt">fluxes</span> and emission sources of a few C3-C9 gaseous alkyl nitrates (ANs) at the Belgian coast (De Haan) on the Southern North <span class="hlt">Sea</span> were determined. An adapted sampler design for low- and high-volume <span class="hlt">air</span>-sampling, optimized sample extraction and clean-up, as well as identification and quantification of ANs in <span class="hlt">air</span> samples by means of gas chromatography mass spectrometry, are reported. The total concentrations of ANs ranged from 0.03 to 85 pptv and consisted primarily of the nitro-butane and nitro-pentane isomers. <span class="hlt">Air</span> mass backward trajectories were calculated by the Hybrid Single-Particle Lagrangian Integrated Trajectory (HYSPLIT) model to determine the influence of main <span class="hlt">air</span> masses on AN levels in the <span class="hlt">air</span>. The shorter chain ANs have been the most abundant in the Atlantic/Channel/UK <span class="hlt">air</span> masses, while longer chain ANs prevailed in continental <span class="hlt">air</span>. The overall mean N <span class="hlt">fluxes</span> of the ANs were slightly higher for summer than those for winter-spring, although their contributions to the total nitrogen <span class="hlt">flux</span> were low. High correlations between AN and HNO₂ levels were observed during winter/spring. During summer, the shorter chain ANs correlated well with precipitation. Source apportionment by means of principal component analysis indicated that most of the gas phase ANs could be attributed to traffic/combustion, secondary photochemical formation and biomass burning, although marine sources may also have been present and a contributing factor.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUFM.C21A0064F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFM.C21A0064F"><span>Measurements of Turbulent <span class="hlt">Fluxes</span> over <span class="hlt">Sea</span> Ice Region in the <span class="hlt">Sea</span> of Okhotsk.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fujisaki, A.; Yamaguchi, H.; Toyota, T.; Futatsudera, A.; Miyanaga, M.</p> <p>2007-12-01</p> <p>The measurements of turbulent <span class="hlt">fluxes</span> over <span class="hlt">sea</span> ice area were done in the southern part of the <span class="hlt">Sea</span> of Okhotsk, during the cruises of the ice-breaker P/V 'Soya' in 2000-2005. The <span class="hlt">air</span>-ice drag coefficients CDN were 3.57×10-3 over small floes \\left(diameter:φ=20- 100m\\right), 3.38×10-3 over medium floes \\left(φ=100-500m\\right), and 2.12×10-3 over big floes \\left( φ=500m-2km\\right), which showed a decrease with the increase of floe size. This is because the smaller floes contribue to the roughness of <span class="hlt">sea</span>-ice area by their edges more than the larger ones. The average CDN values showed a gradual upslope with ice concentration, which is simply due to the rougher surface of <span class="hlt">sea</span> ice than that of open water, while they showed a slight decline at ice concentration 100%, which is possibly due to the lack of freeboard effect of lateral side of floes. We also compared the relation between the roughness length zM and the friction velocity u* with the model developed in the previous study. The zM-u* relation well corresponded with the model results, while the range of zM we obtained was larger than those obtained at the Ice Station Weddell and during the Surface Heat Budget of the Arctic Ocean project. The sensible heat transfer coefficients CHN were 1.35×10-3 at 80-90% ice concentration, and 0.95×10-3 at 100% ice concentration, which are comparable with the results of the past reaserches. On the other hand, we obtained a maximum CHN value of 2.39×10-3at 20-50% ice concentration, and 2.35×10-3 over open water, which are more than twice as the typical value of 1.0×10-3 over open water. These large CHN values are due to the significant upward sensible heat <span class="hlt">flux</span> during the measurements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('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> CO2 <span class="hlt">fluxes</span> in the Terra Nova Bay of the Ross <span class="hlt">Sea</span>, Antarctica, based on year-round pCO2 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 pCO2 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 pCO2 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, pCO2 already started decreasing after reaching the peak in October. In November, the pCO2 suddenly dropped as much as 100 matm in a week. This decrease of pCO2 continued until late February when the <span class="hlt">sea</span>-ice concentration was minimal. With growing <span class="hlt">sea</span> ice, the pCO2 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> CO2 <span class="hlt">flux</span> in the coastal area widely varied from -70 mmol m-2 d-1 to 20 mmol m-2 d-1. Based on these observations of pCO2 in Terra Nova Bay, the annual uptake of CO2 is 8 g C m-2, estimated using the fraction of <span class="hlt">sea</span>-ice concentration estimated from AMSR2 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 CO2 degassed into the atmosphere south of the Antarctic Polar Front (62°S).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1615572B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1615572B"><span>Towards Improved Estimates of Ocean Heat <span class="hlt">Flux</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bentamy, Abderrahim; Hollman, Rainer; Kent, Elisabeth; Haines, Keith</p> <p>2014-05-01</p> <p>Recommendations and priorities for ocean heat <span class="hlt">flux</span> research are for instance outlined in recent CLIVAR and WCRP reports, eg. Yu et al (2013). Among these is the need for improving the accuracy, the consistency, and the spatial and temporal resolution of <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> over global as well as at region scales. To meet the main <span class="hlt">air-sea</span> <span class="hlt">flux</span> requirements, this study is aimed at obtaining and analyzing all the heat <span class="hlt">flux</span> components (latent, sensible and radiative) at the ocean surface over global oceans using multiple satellite sensor observations in combination with in-situ measurements and numerical model analyses. The <span class="hlt">fluxes</span> will be generated daily and monthly for the 20-year (1992-2011) period, between 80N and 80S and at 0.25deg resolution. Simultaneous estimates of all surface heat <span class="hlt">flux</span> terms have not yet been calculated at such large scale and long time period. Such an effort requires a wide range of expertise and data sources that only recently are becoming available. Needed are methods for integrating many data sources to calculate energy <span class="hlt">fluxes</span> (short-wave, long wave, sensible and latent heat) across the <span class="hlt">air-sea</span> interface. We have access to all the relevant, recently available satellite data to perform such computations. Yu, L., K. Haines, M. Bourassa, M. Cronin, S. Gulev, S. Josey, S. Kato, A. Kumar, T. Lee, D. Roemmich: Towards achieving global closure of ocean heat and freshwater budgets: Recommendations for advancing research in <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> through collaborative activities. INTERNATIONAL CLIVAR PROJECT OFFICE, 2013: International CLIVAR Publication Series No 189. http://www.clivar.org/sites/default/files/ICPO189_WHOI_<span class="hlt">fluxes</span>_workshop.pdf</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A54C..02M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A54C..02M"><span>Continuous Flow Hygroscopicity-Resolved Relaxed Eddy Accumulation (Hy-Res REA) Method of Measuring Size-Resolved <span class="hlt">Sea</span>-Salt Particle <span class="hlt">Fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Meskhidze, N.; Royalty, T. M.; Phillips, B.; Dawson, K. W.; Petters, M. D.; Reed, R.; Weinstein, J.; Hook, D.; Wiener, R.</p> <p>2017-12-01</p> <p>The accurate representation of aerosols in climate models requires direct ambient measurement of the size- and composition-dependent particle production <span class="hlt">fluxes</span>. Here we present the design, testing, and analysis of data collected through the first instrument capable of measuring hygroscopicity-based, size-resolved particle <span class="hlt">fluxes</span> using a continuous-flow Hygroscopicity-Resolved Relaxed Eddy Accumulation (Hy-Res REA) technique. The different components of the instrument were extensively tested inside the US Environmental Protection Agency's Aerosol Test Facility for <span class="hlt">sea</span>-salt and ammoniums sulfate particle <span class="hlt">fluxes</span>. The new REA system design does not require particle accumulation, therefore avoids the diffusional wall losses associated with long residence times of particles inside the <span class="hlt">air</span> collectors of the traditional REA devices. The Hy-Res REA system used in this study includes a 3-D sonic anemometer, two fast-response solenoid valves, two Condensation Particle Counters (CPCs), a Scanning Mobility Particle Sizer (SMPS), and a Hygroscopicity Tandem Differential Mobility Analyzer (HTDMA). A linear relationship was found between the <span class="hlt">sea</span>-salt particle <span class="hlt">fluxes</span> measured by eddy covariance and REA techniques, with comparable theoretical (0.34) and measured (0.39) proportionality constants. The <span class="hlt">sea</span>-salt particle detection limit of the Hy-Res REA <span class="hlt">flux</span> system is estimated to be 6x105 m-2s-1. For the conditions of ammonium sulfate and <span class="hlt">sea</span>-salt particles of comparable source strength and location, the continuous-flow Hy-Res REA instrument was able to achieve better than 90% accuracy of measuring the <span class="hlt">sea</span>-salt particle <span class="hlt">fluxes</span>. In principle, the instrument can be applied to measure <span class="hlt">fluxes</span> of particles of variable size and distinct hygroscopic properties (i.e., mineral dust, black carbon, etc.).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20060044030&hterms=SLP&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DSLP','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060044030&hterms=SLP&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DSLP"><span>Ross <span class="hlt">sea</span> ice motion, area <span class="hlt">flux</span>, and deformation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>kwok, Ron</p> <p>2005-01-01</p> <p>The <span class="hlt">sea</span> ice motion, area export, and deformation of the Ross <span class="hlt">Sea</span> ice cover are examined with satellite passive microwave and RADARSAT observations. The record of high-resolution synthetic aperture radar (SAR) data, from 1998 and 2000, allows the estimation of the variability of ice deformation at the small scale (10 km) and to assess the quality of the longer record of passive microwave ice motion. Daily and subdaily deformation fields and RADARSAT imagery highlight the variability of motion and deformation in the Ross <span class="hlt">Sea</span>. With the passive microwave ice motion, the area export at a <span class="hlt">flux</span> gate positioned between Cape Adare and Land Bay is estimated. Between 1992 and 2003, a positive trend can be seen in the winter (March-November) ice area <span class="hlt">flux</span> that has a mean of 990 x 103 km2 and ranges from a low of 600 x 103 km2 in 1992 to a peak of 1600 x 103 km2 in 2001. In the mean, the southern Ross <span class="hlt">Sea</span> produces almost twice its own area of <span class="hlt">sea</span> ice during the winter. Cross-gate <span class="hlt">sea</span> level pressure (SLP) gradients explain 60% of the variance in the ice area <span class="hlt">flux</span>. A positive trend in this gradient, from reanalysis products, suggests a 'spinup' of the Ross <span class="hlt">Sea</span> Gyre over the past 12 yr. In both the NCEP-NCAR and ERA-40 surface pressure fields, longer-term trends in this gradient and mean SLP between 1979 and 2002 are explored along with positive anomalies in the monthly cross-gate SLP gradient associated with the positive phase of the Southern Hemisphere annular mode and the extrapolar Southern Oscillation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JGRC..121.1229W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JGRC..121.1229W"><span>On the calculation of <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> of CO2 in the presence of temperature and salinity gradients</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Woolf, D. K.; Land, P. E.; Shutler, J. D.; Goddijn-Murphy, L. M.; Donlon, C. J.</p> <p>2016-02-01</p> <p>The presence of vertical temperature and salinity gradients in the upper ocean and the occurrence of variations in temperature and salinity on time scales from hours to many years complicate the calculation of the <span class="hlt">flux</span> of carbon dioxide (CO2) across the <span class="hlt">sea</span> surface. Temperature and salinity affect the interfacial concentration of aqueous CO2 primarily through their effect on solubility with lesser effects related to saturated vapor pressure and the relationship between fugacity and partial pressure. The effects of temperature and salinity profiles in the water column and changes in the aqueous concentration act primarily through the partitioning of the carbonate system. Climatological calculations of <span class="hlt">flux</span> require attention to variability in the upper ocean and to the limited validity of assuming "constant chemistry" in transforming measurements to climatological values. Contrary to some recent analysis, it is shown that the effect on CO2 <span class="hlt">fluxes</span> of a cool skin on the <span class="hlt">sea</span> surface is large and ubiquitous. An opposing effect on calculated <span class="hlt">fluxes</span> is related to the occurrence of warm layers near the surface; this effect can be locally large but will usually coincide with periods of low exchange. A salty skin and salinity anomalies in the upper ocean also affect CO2 <span class="hlt">flux</span> calculations, though these haline effects are generally weaker than the thermal effects.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.7783Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.7783Z"><span>Impact of <span class="hlt">sea</span> spray on the Yellow and East China <span class="hlt">Seas</span> thermal structure during the passage of Typhoon Rammasun (2002)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, Lianxin; Zhang, Xuefeng; Chu, P. C.; Guan, Changlong; Fu, Hongli; Chao, Guofang; Han, Guijun; Li, Wei</p> <p>2017-10-01</p> <p>Strong winds lead to large amounts of <span class="hlt">sea</span> spray in the lowest part of the atmospheric boundary layer. The spray droplets affect the <span class="hlt">air-sea</span> heat <span class="hlt">fluxes</span> due to their evaporation and the momentum due to the change of <span class="hlt">sea</span> surface, and in turn change the upper ocean thermal structure. In this study, impact of <span class="hlt">sea</span> spray on upper ocean temperatures in the Yellow and East China <span class="hlt">Seas</span> (YES) during typhoon Rammasun's passage is investigated using the POMgcs ocean model with a <span class="hlt">sea</span> spray parameterization scheme, in which the <span class="hlt">sea</span> spray-induced heat <span class="hlt">fluxes</span> are based on an improved Fairall's <span class="hlt">sea</span> spray heat <span class="hlt">fluxes</span> algorithm, and the <span class="hlt">sea</span> spray-induced momentum <span class="hlt">fluxes</span> are derived from an improved COARE version 2.6 bulk model. The distribution of the <span class="hlt">sea</span> spray mediated turbulent <span class="hlt">fluxes</span> was primarily located at Rammasun eye-wall region, in accord with the maximal wind speeds regions. When Rammasun enters the Yellow <span class="hlt">sea</span>, the <span class="hlt">sea</span> spray mediated latent (sensible) heat <span class="hlt">flux</span> maximum is enhanced by 26% (13.5%) compared to that of the interfacial latent (sensible) heat <span class="hlt">flux</span>. The maximum of the total <span class="hlt">air-sea</span> momentum <span class="hlt">fluxes</span> is enhanced by 43% compared to the counterpart of the interfacial momentum <span class="hlt">flux</span>. Furthermore, the <span class="hlt">sea</span> spray plays a key role in enhancing the intensity of the typhoon-induced "cold suction" and "heat pump" processes. When the effect of <span class="hlt">sea</span> spray is considered, the maximum of the <span class="hlt">sea</span> surface cooling in the right side of Rammasun's track is increased by 0.5°C, which is closer to the available satellite observations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.C43A0587P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.C43A0587P"><span>Heat <span class="hlt">flux</span> variations over <span class="hlt">sea</span>-ice observed at the coastal area of the Sejong Station, Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Park, S.; Choi, T.; Kim, S.</p> <p>2012-12-01</p> <p>This study presents variations of sensible heat <span class="hlt">flux</span> and latent heat <span class="hlt">flux</span> over <span class="hlt">sea</span>-ice observed in 2011 from the 10-m <span class="hlt">flux</span> tower located at the coast of the Sejong Station on King George Island, Antarctica. A period from June to November was divided into three parts: "Freezing", "Frozen", and "Melting" periods based on daily monitoring of <span class="hlt">sea</span> state and hourly photos looking at the Marian Cove in front of the Sejong Station. The division of periods enabled us to look into the heat <span class="hlt">flux</span> variations depending on the <span class="hlt">sea</span>-ice conditions. Over freezing <span class="hlt">sea</span> surface during the freezing period of late June, daily mean sensible heat <span class="hlt">flux</span> was -11.9 Wm-2 and daily mean latent heat <span class="hlt">flux</span> was +16.3 Wm-2. Over the frozen <span class="hlt">sea</span>-ice, daily mean sensible heat <span class="hlt">flux</span> was -10.4 Wm-2 while daily mean latent heat <span class="hlt">flux</span> was +2.4 Wm-2. During the melting period of mid-October to early November, magnitudes of sensible heat <span class="hlt">flux</span> increased to -14.2 Wm-2 and latent heat <span class="hlt">flux</span> also increased to +13.5 Wm-2. In short, latent heat <span class="hlt">flux</span> was usually upward over <span class="hlt">sea</span>-ice most of the time while sensible heat <span class="hlt">flux</span> was downward from atmosphere to <span class="hlt">sea</span>-ice. Magnitudes of the <span class="hlt">fluxes</span> were small but increased when freezing or melting of <span class="hlt">sea</span>-ice was occurring. Especially, latent heat <span class="hlt">flux</span> increased five to six times compared to that of "frozen" period implying that early melting of <span class="hlt">sea</span>-ice may cause five to six times larger supply of moisture to the atmosphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.6547Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.6547Y"><span><span class="hlt">Air-sea</span> interaction regimes in the sub-Antarctic Southern Ocean and Antarctic marginal ice zone revealed by icebreaker measurements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yu, Lisan; Jin, Xiangze; Schulz, Eric W.; Josey, Simon A.</p> <p>2017-08-01</p> <p>This study analyzed shipboard <span class="hlt">air-sea</span> measurements acquired by the icebreaker Aurora Australis during its off-winter operation in December 2010 to May 2012. Mean conditions over 7 months (October-April) were compiled from a total of 22 ship tracks. The icebreaker traversed the water between Hobart, Tasmania, and the Antarctic continent, providing valuable in situ insight into two dynamically important, yet poorly sampled, regimes: the sub-Antarctic Southern Ocean and the Antarctic marginal ice zone (MIZ) in the Indian Ocean sector. The transition from the open water to the ice-covered surface creates sharp changes in albedo, surface roughness, and <span class="hlt">air</span> temperature, leading to consequential effects on <span class="hlt">air-sea</span> variables and <span class="hlt">fluxes</span>. Major effort was made to estimate the <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> in the MIZ using the bulk <span class="hlt">flux</span> algorithms that are tuned specifically for the <span class="hlt">sea</span>-ice effects, while computing the <span class="hlt">fluxes</span> over the sub-Antarctic section using the COARE3.0 algorithm. The study evidenced strong <span class="hlt">sea</span>-ice modulations on winds, with the southerly airflow showing deceleration (convergence) in the MIZ and acceleration (divergence) when moving away from the MIZ. Marked seasonal variations in heat exchanges between the atmosphere and the ice margin were noted. The monotonic increase in turbulent latent and sensible heat <span class="hlt">fluxes</span> after summer turned the MIZ quickly into a heat loss regime, while at the same time the sub-Antarctic surface water continued to receive heat from the atmosphere. The drastic increase in turbulent heat loss in the MIZ contrasted sharply to the nonsignificant and seasonally invariant turbulent heat loss over the sub-Antarctic open water.<abstract type="synopsis"><title type="main">Plain Language SummaryThe icebreaker Aurora Australis is a research and supply vessel that is regularly chartered by the Australian Antarctic Division during the southern summer to operate in waters between Hobart, Tasmania, and Antarctica. The vessel serves as the main lifeline to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016E%26ES...35a2003A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016E%26ES...35a2003A"><span>The potential role of <span class="hlt">sea</span> spray droplets in facilitating <span class="hlt">air-sea</span> gas transfer</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Andreas, E. L.; Vlahos, P.; Monahan, E. C.</p> <p>2016-05-01</p> <p>For over 30 years, <span class="hlt">air-sea</span> interaction specialists have been evaluating and parameterizing the role of whitecap bubbles in <span class="hlt">air-sea</span> gas 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 transfer. In this, our first formal work on this subject, we seek the rate-limiting step in spray-mediated gas transfer by evaluating the three time scales that govern the exchange: τ <span class="hlt">air</span> , which quantifies the rate of transfer between the atmospheric gas reservoir and the surface of the droplet; τ int , which quantifies the 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/2018Ocgy...58..240P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018Ocgy...58..240P"><span>Sediment <span class="hlt">Flux</span> of Particulate Organic Phosphorus in the Open Black <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Parkhomenko, A. V.; Kukushkin, A. S.</p> <p>2018-03-01</p> <p>The interannual variation of the monthly average (weighted average) concentrations of particulate organic phosphorus (PPOM) in the photosynthetic layer, oxycline, redox zone, and H2S zone in the open Black <span class="hlt">Sea</span> is estimated based on long-term observation data. The suspension sedimentation rates from the studied layers are assessed using model calculations and published data. The annual variation of PPOM sediment <span class="hlt">fluxes</span> from the photosynthetic layer, oxycline, redox zone, and upper H2S zone to the anaerobic zone of the <span class="hlt">sea</span> and the correspondingly annual average values are estimated for the first time. A regular decrease in the PPOM annual average <span class="hlt">flux</span> with depth in the upper active layer is demonstrated. A correlation between the annual average values of PPOM sediment <span class="hlt">flux</span> from the photosynthetic layer and ascending phosphate <span class="hlt">flux</span> to this layer is shown, which suggests their balance in the open <span class="hlt">sea</span>. The results are discussed in terms of the phosphorus biogeochemical cycle and the concept of new and regenerative primary production in the open Black <span class="hlt">Sea</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JAMES..10..550H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JAMES..10..550H"><span>The Impact of <span class="hlt">Air-Sea</span> Interactions on the Representation of Tropical Precipitation Extremes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hirons, L. C.; Klingaman, N. P.; Woolnough, S. J.</p> <p>2018-02-01</p> <p>The impacts of <span class="hlt">air-sea</span> interactions on the representation of tropical precipitation extremes are investigated using an atmosphere-ocean-mixed-layer coupled model. The coupled model is compared to two atmosphere-only simulations driven by the coupled-model <span class="hlt">sea</span>-surface temperatures (SSTs): one with 31 day running means (31 d), the other with a repeating mean annual cycle. This allows separation of the effects of interannual SST variability from those of coupled feedbacks on shorter timescales. Crucially, all simulations have a consistent mean state with very small SST biases against present-day climatology. 31d overestimates the frequency, intensity, and persistence of extreme tropical precipitation relative to the coupled model, likely due to excessive SST-forced precipitation variability. This implies that atmosphere-only attribution and time-slice experiments may overestimate the strength and duration of precipitation extremes. In the coupled model, <span class="hlt">air-sea</span> feedbacks damp extreme precipitation, through negative local thermodynamic feedbacks between convection, surface <span class="hlt">fluxes</span>, and SST.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017OcSci..13..997P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017OcSci..13..997P"><span>The spatial and interannual dynamics of the surface water carbonate system and <span class="hlt">air-sea</span> CO2 <span class="hlt">fluxes</span> in the outer shelf and slope of the Eurasian Arctic Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pipko, Irina I.; Pugach, Svetlana P.; Semiletov, Igor P.; Anderson, Leif G.; Shakhova, Natalia E.; Gustafsson, Örjan; Repina, Irina A.; Spivak, Eduard A.; Charkin, Alexander N.; Salyuk, Anatoly N.; Shcherbakova, Kseniia P.; Panova, Elena V.; Dudarev, Oleg V.</p> <p>2017-11-01</p> <p>The Arctic is undergoing dramatic changes which cover the entire range of natural processes, from extreme increases in the temperatures of <span class="hlt">air</span>, soil, and water, to changes in the cryosphere, the biodiversity of Arctic waters, and land vegetation. Small changes in the largest marine carbon pool, the dissolved inorganic carbon pool, can have a profound impact on the carbon dioxide (CO2) <span class="hlt">flux</span> between the ocean and the atmosphere, and the feedback of this <span class="hlt">flux</span> to climate. Knowledge of relevant processes in the Arctic <span class="hlt">seas</span> improves the evaluation and projection of carbon cycle dynamics under current conditions of rapid climate change. Investigation of the CO2 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 CO2 (pCO2) distribution, which manifested as an increase in pCO2 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 CO2 uptake. In contrast, the uptake of CO2 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/2018CSR...162...27C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018CSR...162...27C"><span>Diurnal variability of CO2 <span class="hlt">flux</span> at coastal zone of Taiwan based on eddy covariance observation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chien, Hwa; Zhong, Yao-Zhao; Yang, Kang-Hung; Cheng, Hao-Yuan</p> <p>2018-06-01</p> <p>In this study, we employed shore-based eddy covariance systems for a continuous measurement of the coastal CO2 <span class="hlt">flux</span> near the northwestern coast of Taiwan from 2011 to 2015. To ensure the validity of the analysis, the data was selected and filtered with a footprint model and an empirical mode decomposition method. The results indicate that the nearshore <span class="hlt">air-sea</span> and <span class="hlt">air</span>-land CO2 <span class="hlt">fluxes</span> exhibited a significant diurnal variability and a substantial day-night difference. The net <span class="hlt">air-sea</span> CO2 <span class="hlt">flux</span> was -1.75 ± 0.98 μmol-C m-2 s-1, whereas the net <span class="hlt">air</span>-land CO2 <span class="hlt">flux</span> was 0.54 ± 7.35 μmol-C m-2 s-1, which indicated that in northwestern Taiwan, the coastal water acts as a sink of atmospheric CO2 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> CO2 <span class="hlt">fluxes</span>. The result suggests that the strength of the diurnal <span class="hlt">air-sea</span> CO2 <span class="hlt">flux</span> is strongly influenced by the local wind speed.</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 transfer that can be used to predict the gas transfer rates with sufficient accuracy as a function of micrometeorological parameters is still lacking. State of the art are still simple gas transfer rate/wind speed relationships. Previous measurements from Coastal Ocean Experiment in the Atlantic revealed positive correlations between mean square slope, near surface turbulent dis- sipation, and wind stress. It also demonstrated a strong negative correlation between mean square slope and the fluorescence of surface-enriched colored dissolved organic matter. Using heat as a proxy tracer for gases the 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 <span class="hlt">flux</span> at the ocean surface, the temperature gradient across the <span class="hlt">air/sea</span> interface and thus the heat transfer velocity and gas transfer velocity respectively. Laboratory studies were carried out in the new Heidelberg wind-wave facility AELOTRON. Direct measurements of the Schmidt number exponent were done in conjunction with classical mass balance methods to estimate the transfer velocity. The laboratory results allowed to validate the basic assumptions of the so called controlled <span class="hlt">flux</span> 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('http://adsabs.harvard.edu/abs/2017ECSS..195...16M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ECSS..195...16M"><span><span class="hlt">Sea</span> spray aerosol <span class="hlt">fluxes</span> in the Baltic <span class="hlt">Sea</span> region: Comparison of the WAM model with measurements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Markuszewski, Piotr; Kosecki, Szymon; Petelski, Tomasz</p> <p>2017-08-01</p> <p><span class="hlt">Sea</span> spray aerosol <span class="hlt">flux</span> is an important element of sub-regional climate modeling. The majority of works related to this topic concentrate on open ocean research rather than on smaller, inland <span class="hlt">seas</span>, e.g., the Baltic <span class="hlt">Sea</span>. The Baltic <span class="hlt">Sea</span> is one of the largest brackish inland <span class="hlt">seas</span> by area, where major inflows of oceanic waters are rare. Furthermore, surface waves in the Baltic <span class="hlt">Sea</span> have a relatively shorter lifespan in comparison with oceanic waves. Therefore, emission of <span class="hlt">sea</span> spray aerosol may differ greatly from what is known from oceanic research and should be investigated. This article presents a comparison of <span class="hlt">sea</span> spray aerosol measurements carried out on-board the s/y Oceania research ship with data calculated in accordance to the WAM model. The measurements were conducted in the southern region of the Baltic <span class="hlt">Sea</span> during four scientific cruises. The gradient method was used to determinate aerosol <span class="hlt">fluxes</span>. The <span class="hlt">fluxes</span> were calculated for particles of diameter in range of 0.5-47 μm. The correlation between wind speed measured and simulated has a good agreement (correlation in range of 0.8). The comparison encompasses three different <span class="hlt">sea</span> spray generation models. First, function proposed by Massel (2006) which is based only on wave parameters, such as significant wave height and peak frequency. Second, Callaghan (2013) which is based on Gong (2003) model (wind speed relation), and a thorough experimental analysis of whitecaps. Third, Petelski et al. (2014) which is based on in-situ gradient measurements with the function dependent on wind speed. The two first models which based on whitecaps analysis are insufficient. Moreover, the research shows strong relation between aerosol emission and wind speed history.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.1015G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.1015G"><span>Evaluation of the swell effect on the <span class="hlt">air-sea</span> gas transfer in the coastal zone</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gutiérrez-Loza, Lucía; Ocampo-Torres, Francisco J.</p> <p>2016-04-01</p> <p><span class="hlt">Air-sea</span> gas transfer processes are one of the most important factors regarding global climate and long-term global climate changes. Despite its importance, there is still a huge uncertainty on how to better parametrize these processes in order to include them on the global climate models. This uncertainty exposes the need to increase our knowledge on gas transfer controlling mechanisms. In the coastal regions, breaking waves become a key factor to take into account when estimating gas <span class="hlt">fluxes</span>, however, there is still a lack of information and the influence of the ocean surface waves on the <span class="hlt">air-sea</span> interaction and gas <span class="hlt">flux</span> behavior must be validated. In this study, as part of the "<span class="hlt">Sea</span> Surface Roughness as <span class="hlt">Air-Sea</span> Interaction Control" project, we evaluate the effect of the ocean surface waves on the gas exchange in the coastal zone. Direct estimates of the <span class="hlt">flux</span> of CO2 (FCO2) and water vapor (FH2O) 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 2 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 CO2 under moderate wind and wave conditions with a mean <span class="hlt">flux</span> of -1.32 μmol/m2s. The correlation between the wind speed and FCO2 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 FCO2 and (1) wind speed, (2) significant wave height, (3) wave steepness and (4) water temperature, show that the significant wave height is the most correlated parameter with FCO2; Nevertheless, the behavior of their relation varies along the probability distribution of FCO2, with the linear regression</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/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> transfer of natural and anthropogenic gases involved in the study of climate. The goal in this research area is to determine the gas <span class="hlt">flux</span> from <span class="hlt">air</span> to <span class="hlt">sea</span> or vice versa. For sparingly soluble 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 <span class="hlt">flux</span>. 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 <span class="hlt">flux</span>, 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 <span class="hlt">flux</span> or gas transfer velocity. Examples illustrate the approach in the cases of complete surface renewal, partial surface renewal, and insolation. The prospects for use of the approach in flows characterized by sheared interfaces or rapid boundary layer straining are explored.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('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> CO2 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> <span class="hlt">fluxes</span> by up to 15%, and, therefore, play important local and regional roles in regulating <span class="hlt">air-sea</span> interactions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20100031255&hterms=sss&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dsss','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20100031255&hterms=sss&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dsss"><span>Assessing the Potential to Derive <span class="hlt">Air-Sea</span> Freshwater <span class="hlt">Fluxes</span> from Aquarius-Like Observations of Surface Salinity</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zhen, Li; Adamec, David</p> <p>2009-01-01</p> <p>A state-of-the-art numerical model is used to investigate the possibility of determining freshwater <span class="hlt">flux</span> fields from temporal changes io <span class="hlt">sea</span>-surface salinity (SSS), a goal of the satellite salinity-measuring mission, Aquarius/SAC-D. Because the estimated advective temporal scale is usually longer than the Aquarius/SAC-D revisit time, the possibility of producing freshwater <span class="hlt">flux</span> estimates from temporal salinity changes is first examined by using a correlation analysis. For the mean seasonal cycle, the patterns of the correlations between the freshwater <span class="hlt">fluxes</span> and surface salinity temporal tendencies are mainly zonally oriented, and are highest where the local precipitation is also relatively high. Nonseasonal (deviations from the monthly mean) correlations are highest along mid-latitude moon tracks and are relatively small in the tropics. The complex correlation patterns presented here suggest that a global retrieval of the difference between evaporation and precipitation (E-P) from salinity changes requires more complex techniques than a simple consideration of local balance with surface forcing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.6470A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.6470A"><span>Warm layer and cool skin corrections for bulk water temperature measurements for <span class="hlt">air-sea</span> interaction studies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Alappattu, Denny P.; Wang, Qing; Yamaguchi, Ryan; Lind, Richard J.; Reynolds, Mike; Christman, Adam J.</p> <p>2017-08-01</p> <p>The <span class="hlt">sea</span> surface temperature (SST) relevant to <span class="hlt">air-sea</span> interaction studies is the temperature immediately adjacent to the <span class="hlt">air</span>, referred to as skin SST. Generally, SST measurements from ships and buoys are taken at depths varies from several centimeters to 5 m below the surface. These measurements, known as bulk SST, can differ from skin SST up to O(1°C). Shipboard bulk and skin SST measurements were made during the Coupled <span class="hlt">Air-Sea</span> Processes and Electromagnetic ducting Research east coast field campaign (CASPER-East). An Infrared SST Autonomous Radiometer (ISAR) recorded skin SST, while R/V Sharp's Surface Mapping System (SMS) provided bulk SST from 1 m water depth. Since the ISAR is sensitive to <span class="hlt">sea</span> spray and rain, missing skin SST data occurred in these conditions. However, SMS measurement is less affected by adverse weather and provided continuous bulk SST measurements. It is desirable to correct the bulk SST to obtain a good representation of the skin SST, which is the objective of this research. Bulk-skin SST difference has been examined with respect to meteorological factors associated with cool skin and diurnal warm layers. Strong influences of wind speed, diurnal effects, and net longwave radiation <span class="hlt">flux</span> on temperature difference are noticed. A three-step scheme is established to correct for wind effect, diurnal variability, and then for dependency on net longwave radiation <span class="hlt">flux</span>. Scheme is tested and compared to existing correction schemes. This method is able to effectively compensate for multiple factors acting to modify bulk SST measurements over the range of conditions experienced during CASPER-East.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFM.C12A..01A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFM.C12A..01A"><span>Turbulent Surface <span class="hlt">Flux</span> Measurements over Snow-Covered <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>Andreas, E. L.; Fairall, C. W.; Grachev, A. A.; Guest, P. S.; Jordan, R. E.; Persson, P. G.</p> <p>2006-12-01</p> <p>Our group has used eddy correlation to make over 10,000 hours of measurements of the turbulent momentum and heat <span class="hlt">fluxes</span> over snow-covered <span class="hlt">sea</span> ice in both the Arctic and the Antarctic. Polar <span class="hlt">sea</span> ice is an ideal site for studying fundamental processes for turbulent exchange over snow. Both our Arctic and Antarctic sites---in the Beaufort Gyre and deep into the Weddell <span class="hlt">Sea</span>, respectively---were expansive, flat areas with continuous snow cover; and both were at least 300 km from any topography that might have complicated the atmospheric flow. In this presentation, we will review our measurements of the turbulent <span class="hlt">fluxes</span> of momentum and sensible and latent heat. In particular, we will describe our experiences making turbulence instruments work in the fairly harsh polar, marine boundary layer. For instance, several of our Arctic sites were remote from our main camp and ran unattended for a week at a time. Besides simply making <span class="hlt">flux</span> measurements, we have been using the data to develop a bulk <span class="hlt">flux</span> algorithm and to study fundamental turbulence processes in the atmospheric surface layer. The bulk <span class="hlt">flux</span> algorithm predicts the turbulent surface <span class="hlt">fluxes</span> from mean meteorological quantities and, thus, will find use in data analyses and models. For example, components of the algorithm are already embedded in our one- dimensional mass and energy budget model SNTHERM. Our fundamental turbulence studies have included deducing new scaling regimes in the stable boundary layer; examining the Monin-Obukhov similarity functions, especially in stable stratification; and evaluating the von Kármán constant with the largest atmospheric data set ever applied to such a study. During this presentation, we will highlight some of this work.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018BoLMe.166..475L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018BoLMe.166..475L"><span>Sensitivity of Offshore Surface <span class="hlt">Fluxes</span> and <span class="hlt">Sea</span> Breezes to the Spatial Distribution of <span class="hlt">Sea</span>-Surface Temperature</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lombardo, Kelly; Sinsky, Eric; Edson, James; Whitney, Michael M.; Jia, Yan</p> <p>2018-03-01</p> <p>A series of numerical sensitivity experiments is performed to quantify the impact of <span class="hlt">sea</span>-surface temperature (SST) distribution on offshore surface <span class="hlt">fluxes</span> and simulated <span class="hlt">sea</span>-breeze dynamics. The SST simulations of two mid-latitude <span class="hlt">sea</span>-breeze events over coastal New England are performed using a spatially-uniform SST, as well as spatially-varying SST datasets of 32- and 1-km horizontal resolutions. Offshore surface heat and buoyancy <span class="hlt">fluxes</span> vary in response to the SST distribution. Local <span class="hlt">sea</span>-breeze circulations are relatively insensitive, with minimal differences in vertical structure and propagation speed among the experiments. The largest thermal perturbations are confined to the lowest 10% of the <span class="hlt">sea</span>-breeze column due to the relatively high stability of the mid-Atlantic marine atmospheric boundary layer (ABL) suppressing vertical mixing, resulting in the depth of the marine layer remaining unchanged. Minimal impacts on the column-averaged virtual potential temperature and <span class="hlt">sea</span>-breeze depth translates to small changes in <span class="hlt">sea</span>-breeze propagation speed. This indicates that the use of datasets with a fine-scale SST may not produce more accurate <span class="hlt">sea</span>-breeze simulations in highly stable marine ABL regimes, though may prove more beneficial in less stable sub-tropical environments.</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> CO2 exchange rate on friction velocity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Landwehr, Sebastian; Miller, Scott D.; Smith, Murray J.; Bell, Thomas G.; Saltzman, Eric S.; Ward, Brian</p> <p>2018-03-01</p> <p>Parameterisation of the <span class="hlt">air-sea</span> gas transfer velocity of CO2 and other trace gases under open-ocean conditions has been a focus of <span class="hlt">air-sea</span> interaction research and is required for accurately determining ocean carbon uptake. Ships are the most widely used platform for <span class="hlt">air-sea</span> <span class="hlt">flux</span> measurements but the quality of the data can be compromised by airflow distortion and sensor cross-sensitivity effects. Recent improvements in the understanding of these effects have led to enhanced corrections to the shipboard eddy covariance (EC) measurements.Here, we present a revised analysis of eddy covariance measurements of <span class="hlt">air-sea</span> CO2 and momentum <span class="hlt">fluxes</span> from the Southern Ocean Surface Ocean Aerosol Production (SOAP) study. We show that it is possible to significantly reduce the scatter in the EC data and achieve consistency between measurements taken on station and with the ship underway. The gas transfer velocities from the EC measurements correlate better with the EC friction velocity (u*) than with mean wind speeds derived from shipboard measurements corrected with an airflow distortion model. For the observed range of wind speeds (u10 N = 3-23 m s-1), the transfer velocities can be parameterised with a linear fit to u*. The SOAP data are compared to previous gas transfer parameterisations using u10 N computed from the EC friction velocity with the drag coefficient from the Coupled Ocean-Atmosphere Response Experiment (COARE) model version 3.5. The SOAP results are consistent with previous gas transfer studies, but at high wind speeds they do not support the sharp increase in gas transfer associated with bubble-mediated transfer predicted by physically based models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.A24E..07H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.A24E..07H"><span><span class="hlt">Air-Sea</span> Heat <span class="hlt">Flux</span> Transfer for MJO Initiation Processes during DYNAMO/CINDY2011 in Extended-Range Forecasts</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hong, X.; Reynolds, C. A.; Doyle, J. D.</p> <p>2016-12-01</p> <p>In this study, two-sets of monthly forecasts for the period during the Dynamics of Madden-Julian Oscillation (MJO)/Cooperative Indian Ocean Experiment of Intraseasonal Variability (DAYNAMO/CINDY) in November 2011 are examined. Each set includes three forecasts with the first set from Navy Global Environmental Model (NAVGEM) and the second set from Navy's non-hydrostatic Coupled Ocean-Atmosphere Mesoscale Prediction System (COAMPS®1). Three NAVGEM monthly forecasts have used <span class="hlt">sea</span> surface temperature (SST) from persistent at the initial time, from Navy Coupled Ocean Data Assimilation (NCODA) analysis, and from coupled NAVGEM-Hybrid Coordinate Ocean Model (HYCOM) forecasts. Examination found that NAVGEM can predict the MJO at 20-days lead time using SST from analysis and from coupled NAVGEM-HYCOM but cannot predict the MJO using the persistent SST, in which a clear circumnavigating signal is absent. Three NAVGEM monthly forecasts are then applied as lateral boundary conditions for three COAMPS monthly forecasts. The results show that all COAMPS runs, including using lateral boundary conditions from the NAVGEM that is without the MJO signal, can predict the MJO. Vertically integrated moisture anomaly and 850-hPa wind anomaly in all COAMPS runs have indicated strong anomalous equatorial easterlies associated with Rossby wave prior to the MJO initiation. Strong surface heat <span class="hlt">fluxes</span> and turbulence kinetic energy have promoted the convective instability and triggered anomalous ascending motion, which deepens moist boundary layer and develops deep convection into the upper troposphere to form the MJO phase. The results have suggested that <span class="hlt">air-sea</span> interaction process is important for the initiation and development of the MJO. 1COAMPS® is a registered trademark of the Naval Research Laboratory</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ClDy..tmp.2382T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ClDy..tmp.2382T"><span>Impact of <span class="hlt">air-sea</span> drag coefficient for latent heat <span class="hlt">flux</span> on large scale climate in coupled and atmosphere stand-alone simulations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Torres, Olivier; Braconnot, Pascale; Marti, Olivier; Gential, Luc</p> <p>2018-05-01</p> <p>The turbulent <span class="hlt">fluxes</span> across the ocean/atmosphere interface represent one of the principal driving forces of the global atmospheric and oceanic circulation. Despite decades of effort and improvements, representation of these <span class="hlt">fluxes</span> still presents a challenge due to the small-scale acting turbulent processes compared to the resolved scales of the models. Beyond this subgrid parameterization issue, a comprehensive understanding of the impact of <span class="hlt">air-sea</span> interactions on the climate system is still lacking. In this paper we investigates the large-scale impacts of the transfer coefficient used to compute turbulent heat <span class="hlt">fluxes</span> with the IPSL-CM4 climate model in which the surface bulk formula is modified. Analyzing both atmosphere and coupled ocean-atmosphere general circulation model (AGCM, OAGCM) simulations allows us to study the direct effect and the mechanisms of adjustment to this modification. We focus on the representation of latent heat <span class="hlt">flux</span> in the tropics. We show that the heat transfer coefficients are highly similar for a given parameterization between AGCM and OAGCM simulations. Although the same areas are impacted in both kind of simulations, the differences in surface heat <span class="hlt">fluxes</span> are substantial. A regional modification of heat transfer coefficient has more impact than uniform modification in AGCM simulations while in OAGCM simulations, the opposite is observed. By studying the global energetics and the atmospheric circulation response to the modification, we highlight the role of the ocean in dampening a large part of the disturbance. Modification of the heat exchange coefficient modifies the way the coupled system works due to the link between atmospheric circulation and SST, and the different feedbacks between ocean and atmosphere. The adjustment that takes place implies a balance of net incoming solar radiation that is the same in all simulations. As there is no change in model physics other than drag coefficient, we obtain similar latent heat <span class="hlt">flux</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20030025770','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20030025770"><span>Version 2 Goddard Satellite-Based Surface Turbulent <span class="hlt">Fluxes</span> (GSSTF2)</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chou, Shu-Hsien; Nelkin, Eric; Ardizzone, Joe; Atlas, Robert M.; Shie, Chung-Lin; Starr, David O'C. (Technical Monitor)</p> <p>2002-01-01</p> <p>Information on the turbulent <span class="hlt">fluxes</span> of momentum, moisture, and heat at the <span class="hlt">air-sea</span> interface is essential in improving model simulations of climate variations and in climate studies. We have derived a 13.5-year (July 1987-December 2000) dataset of daily surface turbulent <span class="hlt">fluxes</span> over global oceans from the Special Sensor Mcrowave/Imager (SSM/I) radiance measurements. This dataset, version 2 Goddard Satellite-based Surface Turbulent <span class="hlt">Fluxes</span> (GSSTF2), has a spatial resolution of 1 degree x 1 degree latitude-longitude and a temporal resolution of 1 day. Turbulent <span class="hlt">fluxes</span> are derived from the SSM/I surface winds and surface <span class="hlt">air</span> humidity, as well as the 2-m <span class="hlt">air</span> and <span class="hlt">sea</span> surface temperatures (SST) of the NCEP/NCAR reanalysis, using a bulk aerodynamic algorithm based on the surface layer similarity theory.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AdAtS..35..469Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AdAtS..35..469Z"><span>Effects of <span class="hlt">Sea</span>-Surface Waves and Ocean Spray on <span class="hlt">Air-Sea</span> Momentum <span class="hlt">Fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, Ting; Song, Jinbao</p> <p>2018-04-01</p> <p>The effects of <span class="hlt">sea</span>-surface waves and ocean spray on the marine atmospheric boundary layer (MABL) at different wind speeds and wave ages were investigated. An MABL model was developed that introduces a wave-induced component and spray force to the total surface stress. The theoretical model solution was determined assuming the eddy viscosity coefficient varied linearly with height above the <span class="hlt">sea</span> surface. The wave-induced component was evaluated using a directional wave spectrum and growth rate. Spray force was described using interactions between ocean-spray droplets and wind-velocity shear. Wind profiles and <span class="hlt">sea</span>-surface drag coefficients were calculated for low to high wind speeds for wind-generated <span class="hlt">sea</span> at different wave ages to examine surface-wave and ocean-spray effects on MABL momentum distribution. The theoretical solutions were compared with model solutions neglecting wave-induced stress and/or spray stress. Surface waves strongly affected near-surface wind profiles and <span class="hlt">sea</span>-surface drag coefficients at low to moderate wind speeds. Drag coefficients and near-surface wind speeds were lower for young than for old waves. At high wind speeds, ocean-spray droplets produced by wind-tearing breaking-wave crests affected the MABL strongly in comparison with surface waves, implying that wave age affects the MABL only negligibly. Low drag coefficients at high wind caused by ocean-spray production increased turbulent stress in the <span class="hlt">sea</span>-spray generation layer, accelerating near-<span class="hlt">sea</span>-surface wind. Comparing the analytical drag coefficient values with laboratory measurements and field observations indicated that surface waves and ocean spray significantly affect the MABL at different wind speeds and wave ages.</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> CO2 <span class="hlt">fluxes</span> based on FerryBox measurements and satellite-based prediction of pCO2 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 CO2 (pCO2) 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 pCO2 and <span class="hlt">air-sea</span> CO2 <span class="hlt">fluxes</span>. During the productive period (from May to September), the nWEC acted as a sink for atmospheric CO2 of -5.6 mmolC m-2 d-1 and -4.6 mmolC m-2 d-1, in 2012 and 2013, respectively. During the same period, the sWEC showed significant inter-annual variability degassing CO2 to the atmosphere in 2012 (1.4 mmolC m-2 d-1) and absorbing atmospheric CO2 in 2013 (-1.6 mmolC m-2 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 CO2 drawdown during the productive period, highlighting the necessity of pCO2 high-frequency measurements in coastal ecosystems. Based on this multi-annual dataset, we developed pCO2 algorithms using multiple linear regression (MLR) based on SST, SSS, chlorophyll-a (Chl-a) concentration, time, latitude and mixed layer depth to predict pCO2 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 17.2 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://hdl.handle.net/2060/19820009925','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19820009925"><span>Sensitivity of a climatologically-driven <span class="hlt">sea</span> ice model to the ocean heat <span class="hlt">flux</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Parkinson, C. L.; Good, M. R.</p> <p>1982-01-01</p> <p>Ocean heat <span class="hlt">flux</span> sensitivity was studied on a numerical model of <span class="hlt">sea</span> ice covering the Weddell <span class="hlt">Sea</span> region of the southern ocean. The model is driven by mean monthly climatological atmospheric variables. For each model run, the ocean heat <span class="hlt">flux</span> is uniform in both space and time. Ocean heat <span class="hlt">fluxes</span> below 20 W m to the minus 2 power do not provide sufficient energy to allow the ice to melt to its summertime thicknesses and concentrations by the end of the 14 month simulation, whereas ocean heat <span class="hlt">fluxes</span> of 30 W m to the minus 2 power and above result in too much ice melt, producing the almost total disappearance of ice in the Weddell <span class="hlt">Sea</span> by the end of the 14 months. These results are dependent on the atmospheric forcing fields.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.A51L..03D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.A51L..03D"><span>Diagnosing <span class="hlt">Air-Sea</span> Interactions on Intraseasonal Timescales</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>DeMott, C. A.</p> <p>2014-12-01</p> <p>What is the role of ocean coupling in the Madden Julian Oscillation (MJO)? Consensus thinking holds that the essential physics of the MJO involve interactions between convection, atmospheric wave dynamics, and boundary layer and free troposphere moisture. However, many modeling studies demonstrate improved MJO simulation when an atmosphere-only general circulation model (AGCM) is coupled to an ocean model, so feedbacks from the ocean are probably not negligible. Assessing the importance and processes of these feedbacks is challenging for at least two reasons. First, observations of the MJO only sample the fully coupled ocean-atmosphere system; there is no "uncoupled" MJO in nature. Second, the practice of analyzing the MJO in uncoupled and coupled GCMs (CGCMs) involves using imperfect tools to study the problem. Although MJO simulation is improving in many models, shortcomings remain in both AGCMs and CGCMs, making it difficult to determine if changes brought about through coupling reflect critical <span class="hlt">air-sea</span> interactions or are simply part of the collective idiosyncracies of a given model. For the atmosphere, ocean feedbacks from intraseasonal <span class="hlt">sea</span> surface temperature (SST) variations are communicated through their effects on surface <span class="hlt">fluxes</span> of heat and moisture. This presentation suggests a set of analysis tools for diagnosing the impact of an interactive ocean on surface latent and sensible heat <span class="hlt">fluxes</span>, including their mean, variance, spectral characteristics, and phasing with respect to wind, SST, and MJO convection. The diagnostics are demonstrated with application to several CMIP5 models, and reveal a variety of responses to coupled ocean feedbacks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A23F2429Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A23F2429Z"><span>Role of North Indian Ocean <span class="hlt">Air-Sea</span> Interaction in Summer Monsoon Intraseasonal Oscillation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, L.; Han, W.; Li, Y.</p> <p>2017-12-01</p> <p><span class="hlt">Air-sea</span> coupling processes over the North Indian Ocean associated with Indian summer monsoon intraseasonal oscillation (MISO) are analyzed. Observations show that MISO convection anomalies affect underlying <span class="hlt">sea</span> surface temperature (SST) through changes in surface shortwave radiation (via cloud cover change) and surface latent heat <span class="hlt">flux</span> (associated with surface wind speed change). In turn, SST anomalies determine the changing rate of MISO precipitation (dP/dt): warm (cold) SST anomalies cause increasing (decreasing) precipitation rate through increasing (decreasing) surface convergence. <span class="hlt">Air-sea</span> interaction gives rise to a quadrature relationship between MISO precipitation and SST anomalies. A local <span class="hlt">air-sea</span> coupling model (LACM) is established based on these observed physical processes, which is a damped oscillatory system with no external forcing. The period of LACM is proportional to the square root of mean state mixed layer depth , assuming other physical parameters remain unchanged. Hence, LACM predicts a relatively short (long) MISO period over the North Indian Ocean during the May-June monsoon developing (July-August mature) phase when is shallow (deep). This result is consistent with observed MISO statistics. An oscillatory external forcing of a typical 30-day period is added to LACM, representing intraseasonal oscillations originated from the equatorial Indian Ocean and propagate into the North Indian Ocean. The period of LACM is then determined by both the inherent period associated with local <span class="hlt">air-sea</span> coupling and the period of external forcing. It is found that resonance occurs when , amplifying the MISO in situ. This result explains the larger MISO amplitude during the monsoon developing phase compared to the mature phase, which is associated with seasonal cycle of . LACM, however, fails to predict the observed small MISO amplitude during the September-October monsoon decaying phase, when is also shallow. This deficiency might be associated with the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.U33A0028H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.U33A0028H"><span>Intraseasonal Cold <span class="hlt">Air</span> Outbreak over East Asia and the preceding atmospheric condition over the Barents-Kara <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>Hori, M. E.; Inoue, J.</p> <p>2011-12-01</p> <p>Frequent occurrence of cold <span class="hlt">air</span> outbreak is a dominant feature of the East Asian winter monsoon. A contributing factor for the this cold <span class="hlt">air</span> outbreak is the role of stationary Rossby waves over the Eurasian continent which intensifies the surface Siberian High and the accompanying cold <span class="hlt">air</span> outflow. Reduced <span class="hlt">sea</span> ice and increase in turbulence heat <span class="hlt">flux</span> is hypothesized as a source of such stationary waves (Honda et al. 2009). In particular, the winter of 2009/2010 saw a strong correlation of high pressure anomaly over the Barents/Kara <span class="hlt">sea</span> and the following cold <span class="hlt">air</span> buildup over the Eurasian continent and its advection towards East Asia (Hori et al. 2011). The lag correlation of surface temperature over Japan and the 850hPa geopotential height shows a cyclonic anomaly appearing over the Barents/Kara <span class="hlt">sea</span> which creates a cold <span class="hlt">air</span> advection over the Eurasian continent. The pressure anomaly subsequently shifted westward to mature into a blocking high which created a wave- train pattern downstream advecting the cold <span class="hlt">air</span> buildup eastward toward East Asia and Japan (Fig1). We further examine this mechanism for other years including the 2005/2006, 2010/2011 winter and other winters with extreme cold <span class="hlt">air</span> outbreaks. Overall, the existence of an anticyclonic anomaly over the Barents/Kara <span class="hlt">sea</span> correlated well with the seasonal dominance of cold <span class="hlt">air</span> over the Eurasian continent thereby creating a contrast of a warm Arctic and cold Eurasian continent.In the intraseasonal timescale, the existence of this anticyclone corresponds to a persisting atmospheric blocking in the high latitudes. In the presentation, we address the underlying chain of events leading up to a strong cold <span class="hlt">air</span> outbreak over East Asia from an atmosphere - <span class="hlt">sea</span> ice - land surafce interaction point of view for paritular cold winter years.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS22B..05M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS22B..05M"><span>Atmospheric responses to sensible and latent heating <span class="hlt">fluxes</span> over the Gulf Stream</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Minobe, S.; Ida, T.; Takatama, K.</p> <p>2016-12-01</p> <p><span class="hlt">Air-sea</span> interaction over mid-latitude oceanic fronts such as the Gulf Stream attracted large attention in the last decade. Observational analyses and modelling studies revealed that atmospheric responses over the Gulf Stream including surface wind convergence, enhanced precipitation and updraft penetrating to middle-to-upper troposphere roughly on the Gulf Stream current axis or on the warmer flank of <span class="hlt">sea</span>-surface temperature (SST) front of the Gulf Stream . For these atmospheric responses, oceanic information should be transmitted to the atmosphere via turbulent heat <span class="hlt">fluxes</span>, and thus the mechanisms for atmospheric responses can be understood better by examining latent and sensible <span class="hlt">air-sea</span> heat <span class="hlt">fluxes</span> more closely. Thus, the roles of the sensible and latent heat <span class="hlt">fluxes</span> are examined by conducting a series of numerical experiments using the IPRC Regional Atmospheric Model over the Gulf Stream by applying SST smoothing for latent and sensible heating separately. The results indicate that the sensible and latent heat <span class="hlt">fluxes</span> affect the atmosphere differently. Sensible heat <span class="hlt">flux</span> intensifies surface wind convergence to produce <span class="hlt">sea</span>-level pressure (SLP) anomaly. Latent heat <span class="hlt">flux</span> supplies moistures and maintains enhanced precipitation. The different heat <span class="hlt">flux</span> components cause upward wind velocity at different levels.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.B41D0328R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.B41D0328R"><span>Methane <span class="hlt">fluxes</span> and their controlling processes 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>Rehder, G. J.; Fossing, H.; Lapham, L.; Endler, R.; Spiess, V.; Bruchert, V.; Nguyen, T.; Gülzow, W.; Schneider von Deimling, J.; Conley, D. J.; Jorgensen, B.</p> <p>2010-12-01</p> <p>The Baltic <span class="hlt">Sea</span> is an ideal natural laboratory to study the methane cycle in the framework of diagenetic processes. With its brackish character and a gradient from nearly marine to almost limnic conditions, a strong permanent haline stratification leading to large vertical redox gradients in the water column, and a sedimentation history which resulted in the deposition of organic-rich young post-glacial sediments over older glacial and post-glacial strata with very low organic content, the Baltic allows to study the role of a variety of key parameters for early diagenetic processes including the methane cycle. Within the BONUS + Project “Baltic Gas”, a 3.5 week scientific expedition of RV Maria S. Merian in August 2010 was dedicated to study the methane cycle in the various basins of the Baltic <span class="hlt">Sea</span>, with strong emphasis on the metabolic reactions of early diagenesis and the occurrence of shallow gas deposits. Various subbottom profiling systems were used to map the thickness and structure of organic-rich deposits and build the base for a detailed coring program for biogeochemical analysis, including methane, sulfur compounds, iron, and other compounds. Methane gradients in connection with the information of the areal extend of organic-rich deposits are used to estimate the diffusive <span class="hlt">flux</span> from the sediments into the water column and the rate of methane oxidation, with changing importance of sulfate as oxidant along the salinity gradient. On selected key stations, rate measurements of methanogenic and methanotrophic reactions were executed. The methane distribution in the water column was comprehensively assessed, revealing amongst other findings a drastic increase in bottom water methane concentration between the post bloom summer situation and the situation in the winter of 2009, in connection to the occurrence of a benthic nepheloid layer. <span class="hlt">Air-sea</span> <span class="hlt">flux</span> measurements were executed along the ship’s track comprising all major basins of the Baltic. The talk gives</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002JApMe..41..241B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002JApMe..41..241B"><span>An Integrated Approach to Estimate Instantaneous Near-Surface <span class="hlt">Air</span> Temperature and Sensible Heat <span class="hlt">Flux</span> Fields during the SEMAPHORE Experiment.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bourras, Denis; Eymard, Laurence; Liu, W. Timothy; Dupuis, Hélène</p> <p>2002-03-01</p> <p>A new technique was developed to retrieve near-surface instantaneous <span class="hlt">air</span> temperatures and turbulent sensible heat <span class="hlt">fluxes</span> using satellite data during the Structure des Echanges Mer-Atmosphere, Proprietes des Heterogeneites Oceaniques: Recherche Experimentale (SEMAPHORE) experiment, which was conducted in 1993 under mainly anticyclonic conditions. The method is based on a regional, horizontal atmospheric temperature advection model whose inputs are wind vectors, <span class="hlt">sea</span> surface temperature fields, <span class="hlt">air</span> temperatures around the region under study, and several constants derived from in situ measurements. The intrinsic rms error of the method is 0.7°C in terms of <span class="hlt">air</span> temperature and 9 W m2 for the <span class="hlt">fluxes</span>, both at 0.16° × 0.16° and 1.125° × 1.125° resolution. The retrieved <span class="hlt">air</span> temperature and <span class="hlt">flux</span> horizontal structures are in good agreement with fields from two operational general circulation models. The application to SEMAPHORE data involves the First European Remote Sensing Satellite (ERS-1) wind fields, Advanced Very High Resolution Radiometer (AVHRR) SST fields, and European Centre for Medium-Range Weather Forecasts (ECMWF) <span class="hlt">air</span> temperature boundary conditions. The rms errors obtained by comparing the estimations with research vessel measurements are 0.3°C and 5 W m2.</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> transfer 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 <span class="hlt">fluxes</span> 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 transfer 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 <span class="hlt">fluxes</span> 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> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li class="active"><span>8</span></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_8 --> <div id="page_9" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li class="active"><span>9</span></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="161"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AtmRe.196...62S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AtmRe.196...62S"><span>Intense <span class="hlt">air-sea</span> exchanges and heavy orographic precipitation over Italy: The role of Adriatic <span class="hlt">sea</span> surface temperature uncertainty</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stocchi, Paolo; Davolio, Silvio</p> <p>2017-11-01</p> <p>Strong and persistent low-level winds blowing over the Adriatic basin are often associated with intense precipitation events over Italy. Typically, in case of moist southeasterly wind (Sirocco), rainfall affects northeastern Italy and the Alpine chain, while with cold northeasterly currents (Bora) precipitations are localized along the eastern slopes of the Apennines and central Italy coastal areas. These events are favoured by intense <span class="hlt">air-sea</span> interactions and it is reasonable to hypothesize that the Adriatic <span class="hlt">sea</span> surface temperature (SST) can affect the amount and location of precipitation. High-resolution simulations of different Bora and Sirocco events leading to severe precipitation are performed using a convection-permitting model (MOLOCH). Sensitivity experiments varying the SST initialization field are performed with the aim of evaluating the impact of SST uncertainty on precipitation forecasts, which is a relevant topic for operational weather predictions, especially at local scales. Moreover, diagnostic tools to compute water vapour <span class="hlt">fluxes</span> across the Italian coast and atmospheric water budget over the Adriatic <span class="hlt">Sea</span> have been developed and applied in order to characterize the <span class="hlt">air</span> mass that feeds the precipitating systems. Finally, the investigation of the processes through which the SST influences location and intensity of heavy precipitation allows to gain a better understanding on mechanisms conducive to severe weather in the Mediterranean area and in the Adriatic basin in particular. Results show that the effect of the Adriatic SST (uncertainty) on precipitation is complex and can vary considerably among different events. For both Bora and Sirocco events, SST does not influence markedly the atmospheric water budget or the degree of moistening of <span class="hlt">air</span> that flows over the Adriatic <span class="hlt">Sea</span>. SST mainly affects the stability of the atmospheric boundary layer, thus influencing the flow dynamics and the orographic flow regime, and in turn, the precipitation pattern.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.A23M..04W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.A23M..04W"><span>How do Greenhouse Gases Warm the Ocean? Investigation of the Response of the Ocean Thermal Skin Layer to <span class="hlt">Air-Sea</span> Surface Heat <span class="hlt">Fluxes</span>.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wong, E.; Minnett, P. J.</p> <p>2016-12-01</p> <p>There is much evidence that the ocean is heating due to an increase in concentrations of greenhouse gases (GHG) in the atmosphere from human activities. GHGs absorbs infrared (IR) radiation and re-emits the radiation back to the ocean's surface which is subsequently absorbed resulting in a rise in the ocean heat content. However, the incoming longwave radiation, LWin, is absorbed within the top micrometers of the ocean's surface, where the thermal skin layer (TSL) exists and does not directly heat the upper few meters of the ocean. We are therefore motivated to investigate the physical mechanism between the absorption of IR radiation and its effect on heat transfer at the <span class="hlt">air-sea</span> boundary. The hypothesis is that since heat lost through the <span class="hlt">air-sea</span> interface is controlled by the TSL, which is directly influenced by the absorption and emission of IR radiation, the heat flow through the TSL adjusts to maintain the surface heat loss, and thus modulates the upper ocean heat content. This hypothesis is investigated through utilizing clouds to represent an increase in LWin and analyzing retrieved TSL vertical profiles from a shipboard IR spectrometer from two research cruises. The data is limited to night-time, no precipitation and low winds of < 2 m/s to remove effects of solar radiation, wind-driven shear and possibilities of TSL disruption. The results show independence between the turbulent <span class="hlt">fluxes</span> and radiative <span class="hlt">fluxes</span> which rules out the immediate release of heat from the absorption of the cloud infrared irradiance back into the atmosphere through processes such as evaporation. Instead, we observe the surplus energy, from absorbing increasing levels of LWin, adjusts the curvature of the TSL such that there is a lower gradient at the interface between the TSL and the mixed layer. The release of heat stored within the mixed layer is therefore hindered while the additional energy within the TSL is cycled back into the atmosphere. This results in heat beneath the TSL</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25826919','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25826919"><span>[Distributions and <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> of dissolved nitrous oxide in the Yangtze River estuary and its adjacent marine area in spring and summer].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Lan; Zhang, Gui-ling; Sun, Ming-shuang; Ren, Jing-ling</p> <p>2014-12-01</p> <p>Distributions and <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> of nitrous oxide (N2O) in the seawaters of the Yangtze River estuary and its adjacent marine area were investigated during two cruises in March and July 2012. Dissolved N2O concentrations in surface waters ranged from 9.34 to 49.08 nmol x L(-1) with an average of (13.27 ± 6.40) nmol x L(-1) in spring and ranged from 7.27 to 27.81 nmol x L(-1) with an average of (10.62 ± 5.03) nmol x L(-1) in summer. There was no obvious difference between surface and bottom N2O concentrations. N2O concentrations in both surface and bottom waters decreased along the freshwater plume from the river mouth to the open <span class="hlt">sea</span>. High values of dissolved N2O were found in turbidity maximum zone, which suggests that maximal turbidity enhances nitrification. Temperature had dual effects on dissolved N2O concentrations. N2O saturations in surface waters ranged from 86.9% to 351.3% with an average of (111.5 ± 41.4)% in spring and ranged from 111.7% to 396.0% with an average of (155.9 ± 68.4)% in summer. N2O were over-saturated at most stations. The <span class="hlt">sea-to-air</span> <span class="hlt">fluxes</span> of N2O were estimated to be (3.2 ± 10.9), (5.5 ± 19.3) and (12.2 ±52.3) μmol x (m2 x d)(-1) in spring and (7.3 ± 12.4), (12.7 ± 20.4) and (20.4 ± 35.9) μmol x (m2 x d)(-1) in summer using the LM86, W92 and RC01 relationships, respectively. The annual emissions of N2O from the Yangtze River estuary and its adjacent marine area were estimated to be 0.6 x 10(-2) Tg x a(-1) (LM86), 1.1 x 10(-2) Tg x a(-1) (W92) and 2.0 x 10(-2) Tg x a(-1) (RC01). Although the area of the Yangtze River estuary and its adjacent marine area only accounts for 0.02% of the total area of the world's oceans, their emission of N2O accounts for 0.06% of global oceanic N2O emission, indicating that the Yangtze River estuary and its adjacent marine area is an active area to produce and emit N2O.</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://www.osti.gov/biblio/467654-air-sea-interaction-subtropical-convergence-south-africa','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/467654-air-sea-interaction-subtropical-convergence-south-africa"><span><span class="hlt">Air-sea</span> interaction at the subtropical convergence south of Africa</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Rouault, M.; Lutjeharms, J.R.E.; Ballegooyen, R.C. van</p> <p>1994-12-31</p> <p>The oceanic region south of Africa plays a key role in the control of Southern Africa weather and climate. This is particularly the case for the Subtropical Convergence region, the northern border of the Southern Ocean. An extensive research cruise to investigate this specific front was carried out during June and July 1993. A strong front, the Subtropical Convergence was identified, however its geographic disposition was complicated by the presence of an intense warm eddy detached from the Agulhas current. The warm surface water in the eddy created a strong contrast between it and the overlying atmosphere. Oceanographic measurements (XBTmore » and CTD) were jointly made with radiosonde observations and <span class="hlt">air-sea</span> interaction measurements. The <span class="hlt">air-sea</span> interaction measurement system included a Gill sonic anemometer, an Ophir infrared hygrometer, an Eppley pyranometer, an Eppley pyrgeometer and a Vaissala temperature and relative humidity probe. Turbulent <span class="hlt">fluxes</span> of momentum, sensible heat and latent heat were calculated in real time using the inertial dissipation method and the bulk method. All these measurements allowed a thorough investigation of the net heat loss of the ocean, the deepening of the mixed layer during a severe storm as well as the structure of the atmospheric boundary layer and ocean-atmosphere exchanges.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19990094165&hterms=clear+pool&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dclear%2Bpool','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19990094165&hterms=clear+pool&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dclear%2Bpool"><span>Tropical Intraseasonal <span class="hlt">Air-Sea</span> Exchanges during the 1997 Pacific Warming</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sui, C.-H.; Lau, K.-M.; Chou, S.-H.; Wang, Zihou</p> <p>1999-01-01</p> <p>The Madden Julian Oscillations (MJO) and associated westerly wind (WW) events account for much of the tropical intraseasonal variability (TISV). The TISV has been suggested as an important stochastic forcing that may be one of the underlying causes for the observed irregularities of the El Nino-Southern Oscillation (ENSO). Recent observational studies and theories of interannual to interdecadal-scale variability suggest that ENSO may arise from different mechanisms depending on the basic states. The Pacific warming event of 1997, being associated with a period of strong MJO and WW events, serves as a natural experiment for studying the possible role of TISV in triggering an ENSO event. We have performed a combined statistical and composite analysis of surface WW events based on the assimilated surface wind and <span class="hlt">sea</span> level pressure for the period of 1980-1993, the SSM/I wind for the period of 1988-1997, and OLR. Results indicates that extratropical forcing contribute significantly to the evolution of MJO and establishment of WW events over the Pacific warm pool. Following the major WW events, there appeared an eastward extension of equatorial warm SST anomalies from the western Pacific warm pool. Such tropical-extratropical interaction is particularly clear in the winter of 96-97 that leads to the recent warming event in 1997/98. From the above discussion, our current study on this subject is based on the hypothesis that 1) there is an enhanced <span class="hlt">air-sea</span> interaction associated with TISV and the northerly surges from the extratropics in the initial phase of the 97/98 warming event, and 2) the relevant mechanisms are functions of the basic state of the coupled system (in terms of SST distribution and atmospheric mean circulation) that varies at the interannual and interdecadal time scale. We are analyzing the space-time structure of the northerly surges, their association with <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> and upper ocean responses during the period of September 1996 to June 1997. The</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018BGeo...15.1011M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018BGeo...15.1011M"><span>Inorganic carbon <span class="hlt">fluxes</span> on the Mackenzie Shelf of the Beaufort <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mol, Jacoba; Thomas, Helmuth; Myers, Paul G.; Hu, Xianmin; Mucci, Alfonso</p> <p>2018-02-01</p> <p>The Mackenzie Shelf in the southeastern Beaufort <span class="hlt">Sea</span> is a region that has experienced large changes in the past several decades as warming, <span class="hlt">sea</span>-ice loss, and increased river discharge have altered carbon cycling. Upwelling and downwelling events are common on the shelf, caused by strong, fluctuating along-shore winds, resulting in cross-shelf Ekman transport, and an alternating estuarine and anti-estuarine circulation. Downwelling carries dissolved inorganic carbon (DIC) and other remineralization products off the shelf and into the deep basin for possible long-term storage in the world's oceans. Upwelling carries DIC and nutrient-rich waters from the Pacific-origin upper halocline layer (UHL) onto the shelf. Profiles of DIC and total alkalinity (TA) taken in August and September of 2014 are used to investigate the cycling of carbon on the Mackenzie Shelf. The along-shore transport of water and the cross-shelf transport of DIC are quantified using velocity field output from a simulation of the Arctic and Northern Hemisphere Atlantic (ANHA4) configuration of the Nucleus of European Modelling of the Ocean (NEMO) framework. A strong upwelling event prior to sampling on the Mackenzie Shelf took place, bringing CO2-rich (elevated pCO2) water from the UHL onto the shelf bottom. The maximum on-shelf DIC <span class="hlt">flux</span> was estimated at 16.9×103 mol C d-1 m-2 during the event. The maximum on-shelf transport of DIC through the upwelling event was found to be 65±15×10-3 Tg C d-1. TA and the oxygen isotope ratio of water (δ18O-H2O) are used to examine water-mass distributions in the study area and to investigate the influence of Pacific Water, Mackenzie River freshwater, and <span class="hlt">sea</span>-ice melt on carbon dynamics and <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> of carbon dioxide (CO2) in the surface mixed layer. Understanding carbon transfer in this seasonally dynamic environment is key to quantify the importance of Arctic shelf regions to the global carbon cycle and provide a basis for understanding how it will</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013APJAS..49..443P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013APJAS..49..443P"><span>Heat <span class="hlt">flux</span> variations over <span class="hlt">sea</span> ice observed at the coastal area of the Sejong Station, Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Park, Sang-Jong; Choi, Tae-Jin; Kim, Seong-Joong</p> <p>2013-08-01</p> <p>This study presents variations of sensible heat <span class="hlt">flux</span> and latent heat <span class="hlt">flux</span> over <span class="hlt">sea</span> ice observed in 2011 from the 10-m <span class="hlt">flux</span> tower located at the coast of the Sejong Station on King George Island, Antarctica. A period from July to September was selected as a <span class="hlt">sea</span> ice period based on daily record of <span class="hlt">sea</span> state and hourly photos looking at the Marian Cove in front of the Sejong Station. For the <span class="hlt">sea</span> ice period, mean sensible heat <span class="hlt">flux</span> is about -11 Wm-2, latent heat <span class="hlt">flux</span> is about +2 W m-2, net radiation is -12 W m-2, and residual energy is -3 W m-2 with clear diurnal variations. Estimated mean values of surface exchange coefficients for momentum, heat and moisture are 5.15 × 10-3, 1.19 × 10-3, and 1.87 × 10-3, respectively. The observed exchange coefficients of heat shows clear diurnal variations while those of momentum and moisture do not show diurnal variation. The parameterized exchange coefficients of heat and moisture produces heat <span class="hlt">fluxes</span> which compare well with the observed diurnal variations of heat <span class="hlt">fluxes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1985JGR....90.2409Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1985JGR....90.2409Z"><span><span class="hlt">Air-to-sea</span> <span class="hlt">fluxes</span> of lipids at Enewetak Atoll</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zafiriou, Oliver C.; Gagosian, Robert B.; Peltzer, Edward T.; Alford, Jane B.; Loder, T.</p> <p>1985-02-01</p> <p>We report data for the Enewetak site of the SEAREX program from the rainy season in 1979. The concentrations of n-alkanes, n-alkanols, sterols, n-alkanoic acids and their salts, and total organic compounds in rain are reported, as well as the apparent gaseous hydrocarbon concentrations. These data and information on the particulate forms are analyzed in conjunction with ancillary chemical and meteorological data to draw inferences about sources, <span class="hlt">fluxes</span>, and chemical speciations. While the higher molecular weight lipid biomarker components are exclusively terrestrial, the organic carbon in rain may be derived from atmospheric transformations of terrestrial carbon. Distinctively marine components are nearly absent. Comparison of the scavenging ratios of the organic components in rain vs. those for clays reveals that the alkanoic acids and the higher molecular weight alkanols behave as essentially particulate materials, whereas lower alkanols and most hydrocarbons show much higher scavenging ratios, probably due to the involvement of a gaseous phase or sampling artifact. Vaporization in the atmosphere and scavenging of a gas phase would lead to higher scavenging ratios; vaporization during sampling would give low aerosol concentrations and high gas-phase concentrations, leading to high scavenging ratios. The major <span class="hlt">fluxes</span> at Enewetak result from rain rather than dry deposition, and extrapolating the measured values to meaningful annual averages requires adjustment for seasonally varying source intensity and rain dynamics. Aerosol data for other seasons and other substances are used to correct for source-strength intensity variations, and a 210Pb/organic compound correlation is established and extrapolated to adjust for rainfall volume effects. These corrections, assumed independent and applied together, yield inferred <span class="hlt">fluxes</span> 2.5-9 times larger than the <span class="hlt">fluxes</span> calculated for mean concentrations. The inferred <span class="hlt">fluxes</span> to the ocean, while small compared to primary</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1130204-interaction-between-marine-boundary-layer-cellular-cloudiness-surface-heat-fluxes','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1130204-interaction-between-marine-boundary-layer-cellular-cloudiness-surface-heat-fluxes"><span>On the Interaction between Marine Boundary Layer Cellular Cloudiness and Surface Heat <span class="hlt">Fluxes</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>Kazil, J.; Feingold, G.; Wang, Hailong</p> <p>2014-01-02</p> <p>The interaction between marine boundary layer cellular cloudiness and surface uxes of sensible and latent heat is investigated. The investigation focuses on the non-precipitating closed-cell state and the precipitating open-cell state at low geostrophic wind speed. The Advanced Research WRF model is used to conduct cloud-system-resolving simulations with interactive surface <span class="hlt">fluxes</span> of sensible heat, latent heat, and of <span class="hlt">sea</span> salt aerosol, and with a detailed representation of the interaction between aerosol particles and clouds. The mechanisms responsible for the temporal evolution and spatial distribution of the surface heat <span class="hlt">fluxes</span> in the closed- and open-cell state are investigated and explained. Itmore » is found that the horizontal spatial structure of the closed-cell state determines, by entrainment of dry free tropospheric <span class="hlt">air</span>, the spatial distribution of surface <span class="hlt">air</span> temperature and water vapor, and, to a lesser degree, of the surface sensible and latent heat <span class="hlt">flux</span>. The synchronized dynamics of the the open-cell state drives oscillations in surface <span class="hlt">air</span> temperature, water vapor, and in the surface <span class="hlt">fluxes</span> of sensible and latent heat, and of <span class="hlt">sea</span> salt aerosol. Open-cell cloud formation, cloud optical depth and liquid water path, and cloud and rain water path are identified as good predictors of the spatial distribution of surface <span class="hlt">air</span> temperature and sensible heat <span class="hlt">flux</span>, but not of surface water vapor and latent heat <span class="hlt">flux</span>. It is shown that by enhancing the surface sensible heat <span class="hlt">flux</span>, the open-cell state creates conditions by which it is maintained. While the open-cell state under consideration is not depleted in aerosol, and is insensitive to variations in <span class="hlt">sea</span>-salt <span class="hlt">fluxes</span>, it also enhances the <span class="hlt">sea</span>-salt <span class="hlt">flux</span> relative to the closed-cell state. In aerosol-depleted conditions, this enhancement may replenish the aerosol needed for cloud formation, and hence contribute to the perpetuation of the open-cell state as well. Spatial homogenization of the surface <span class="hlt">fluxes</span> is found</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 2.6-74, <0.1-19, <0.1-63, and <1.0-9.0 pg L(-1), respectively. The highest concentrations were determined in the estuary of the Weser and Elbe rivers and a decreasing concentration profile appeared with increasing distance from the coast toward the central part of the North <span class="hlt">Sea</span>. Gaseous FTOHs, FASAs, FASEs, and FTACs were in the range of 36-126, 3.1-26, 3.7-19, and 0.8-5.6 pg m(-3), which were consistent with the concentrations determined in 2007 in the North <span class="hlt">Sea</span>, and approximately five times lower than those reported for an urban area of Northern Germany. These results suggested continuous continental emissions of neutral PFASs followed by transport toward the marine environment. <span class="hlt">Air</span>-seawater gas exchanges of neutral PFASs were estimated using fugacity ratios and the two-film resistance model based upon paired <span class="hlt">air</span>-seawater concentrations and estimated Henry's law constant values. Volatilization dominated for all neutral PFASs in the North <span class="hlt">Sea</span>. The <span class="hlt">air</span>-seawater gas exchange <span class="hlt">fluxes</span> were in the range of 2.5×10(3)-3.6×10(5) pg m(-2) for FTOHs, 1.8×10(2)-1.0×10(5) pg m(-2) for FASAs, 1.1×10(2)-3.0×10(5) pg m(-2) for FASEs and 6.3×10(2)-2.0×10(4) pg m(-2) 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('https://ntrs.nasa.gov/search.jsp?R=20020001355&hterms=dataset&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Ddataset','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20020001355&hterms=dataset&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Ddataset"><span>A Multiyear Dataset of SSM/I-Derived Global Ocean Surface Turbulent <span class="hlt">Fluxes</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chou, Shu-Hsien; Shie, Chung-Lin; Atlas, Robert M.; Ardizzone, Joe; Nelkin, Eric; Einaudi, Franco (Technical Monitor)</p> <p>2001-01-01</p> <p>The surface turbulent <span class="hlt">fluxes</span> of momentum, latent heat, and sensible heat over global oceans are essential to weather, climate and ocean problems. Evaporation is a key component of the hydrological cycle and the surface heat budget, while the wind stress is the major forcing for driving the oceanic circulation. The global <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> of momentum, latent and sensible heat, radiation, and freshwater (precipitation-evaporation) are the forcing for driving oceanic circulation and, hence, are essential for understanding the general circulation of global oceans. The global <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> are required for driving ocean models and validating coupled ocean-atmosphere global models. We have produced a 7.5-year (July 1987-December 1994) dataset of daily surface turbulent <span class="hlt">fluxes</span> over the global oceans from the Special Sensor microwave/Imager (SSM/I) data. Daily turbulent <span class="hlt">fluxes</span> were derived from daily data of SSM/I surface winds and specific humidity, National Centers for Environmental Prediction (NCEP) <span class="hlt">sea</span> surface temperatures, and European Centre for Medium-Range Weather Forecasts (ECMWF) <span class="hlt">air-sea</span> temperature differences, using a stability-dependent bulk scheme. The retrieved instantaneous surface <span class="hlt">air</span> humidity (with a 25-km resolution) validated well with that of the collocated radiosonde observations over the global oceans. Furthermore, the retrieved daily wind stresses and latent heat <span class="hlt">fluxes</span> were found to agree well with that of the in situ measurements (IMET buoy, RV Moana Wave, and RV Wecoma) in the western Pacific warm pool during the TOGA COARE intensive observing period (November 1992-February 1993). The global distributions of 1988-94 seasonal-mean turbulent <span class="hlt">fluxes</span> will be presented. In addition, the global distributions of 1990-93 annual-means turbulent <span class="hlt">fluxes</span> and input variables will be compared with those of UWM/COADS covering the same period. The latter is based on the COADS (comprehensive ocean-atmosphere data set) and is recognized to be one of the best</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/12916843','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/12916843"><span>Improving mercury <span class="hlt">flux</span> chamber measurements over water surface.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lanzillotra, E; Ceccarini, C; Ferrara, R</p> <p>2003-07-01</p> <p>A modified floating <span class="hlt">flux</span> chamber was designed and used to measure mercury evasional <span class="hlt">fluxes</span> in a coastal area of the Mediterranean <span class="hlt">Sea</span> in different meteo-marine conditions during the hours of maximum insolation (PAR intensity 360-430 W m(-2)) in the summer season. The chamber has been modified providing a flap at the inlet port preventing the back-flow of <span class="hlt">air</span> from the interior of the chamber. Results demonstrate that the modified <span class="hlt">flux</span> chamber gives <span class="hlt">flux</span> values noticeably higher both in rippled <span class="hlt">sea</span> conditions (mean value 7.88 +/- 1.45 ng m(-2) h(-1)) and in rough <span class="hlt">sea</span> conditions (mean value 21.71 +/- 2.17 ng m(-2) h(-1)) with respect to those obtained by using the unmodified chamber (respectively 5.23 +/- 0.67 and 14.15 +/- 1.03 ng m(-2) h(-1)).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018IzAOP..54..213B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018IzAOP..54..213B"><span>Seasonal and Interannual Variations of Heat <span class="hlt">Fluxes</span> in the Barents <span class="hlt">Sea</span> Region</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bashmachnikov, I. L.; Yurova, A. Yu.; Bobylev, L. P.; Vesman, A. V.</p> <p>2018-03-01</p> <p>Seasonal and interannual variations in adjective heat <span class="hlt">fluxes</span> in the ocean ( dQ oc) and the convergence of advective heat <span class="hlt">fluxes</span> in the atmosphere ( dQ atm) in the Barents <span class="hlt">Sea</span> region have been investigated over the period of 1993-2012 using the results of the MIT regional eddy-permitting model and ERA-Interim atmospheric reanalysis. Wavelet analysis and singular spectrum analysis are used to reveal concealed periodicities. Seasonal 2- to 4- and 5- to 8-year cycles are revealed in the dQ oc and dQ atm data. It is also found that seasonal variations in dQ oc are primarily determined by the integrated volume <span class="hlt">fluxes</span> through the western boundary of the Barents <span class="hlt">Sea</span>, whereas the 20-year trend is determined by the temperature variation of the transported water. A cross-wavelet analysis of dQ oc and dQ atm in the Barents <span class="hlt">Sea</span> region shows that the seasonal variations in dQ oc and dQ atm are nearly in-phase, while their interannual variations are out-of-phase. It is concluded that the basin of the Barents <span class="hlt">Sea</span> plays an important role in maintaining the feedback mechanism (the Bjerknes compensation) of the ocean-atmosphere system in the Arctic region.</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 CO2 <span class="hlt">fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lauderdale, Jonathan M.; Dutkiewicz, Stephanie; Williams, Richard G.; Follows, Michael J.</p> <p>2016-07-01</p> <p>A mechanistic framework for quantitatively mapping the regional drivers of <span class="hlt">air-sea</span> CO2 <span class="hlt">fluxes</span> at a global scale is developed. The framework evaluates the interplay between (1) surface heat and freshwater <span class="hlt">fluxes</span> that influence the potential saturated carbon concentration, which depends on changes in <span class="hlt">sea</span> surface temperature, salinity and alkalinity, (2) a residual, disequilibrium <span class="hlt">flux</span> influenced by upwelling and entrainment of remineralized carbon- and nutrient-rich waters from the ocean interior, as well as rapid subduction of surface waters, (3) carbon uptake and export by biological activity as both soft tissue and carbonate, and (4) the effect on surface carbon concentrations due to freshwater precipitation or evaporation. In a steady state simulation of a coarse-resolution ocean circulation and biogeochemistry model, the sum of the individually determined components is close to the known total <span class="hlt">flux</span> of the simulation. The leading order balance, identified in different dynamical regimes, is between the CO2 <span class="hlt">fluxes</span> driven by surface heat <span class="hlt">fluxes</span> and a combination of biologically driven carbon uptake and disequilibrium-driven carbon outgassing. The framework is still able to reconstruct simulated <span class="hlt">fluxes</span> when evaluated using monthly averaged data and takes a form that can be applied consistently in models of different complexity and observations of the ocean. In this way, the framework may reveal differences in the balance of drivers acting across an ensemble of climate model simulations or be applied to an analysis and interpretation of the observed, real-world <span class="hlt">air-sea</span> <span class="hlt">flux</span> of CO2.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20020015705','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20020015705"><span>Modeling Biogeochemical-Physical Interactions and Carbon <span class="hlt">Flux</span> in the Sargasso <span class="hlt">Sea</span> (Bermuda Atlantic Time-series Study site)</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Signorini, Sergio R.; McClain, Charles R.; Christian, James R.</p> <p>2001-01-01</p> <p>An ecosystem-carbon cycle model is used to analyze the biogeochemical-physical interactions and carbon <span class="hlt">fluxes</span> in the Bermuda Atlantic Time-series Study (BATS) site for the period of 1992-1998. The model results compare well with observations (most variables are within 8% of observed values). The <span class="hlt">sea-air</span> <span class="hlt">flux</span> ranges from -0.32 to -0.50 mol C/sq m/yr, depending upon the gas transfer algorithm used. This estimate is within the range (-0.22 to -0.83 mol C/sq m/yr) of previously reported values which indicates that the BATS region is a weak sink of atmospheric CO2. The overall carbon balance consists of atmospheric CO2 uptake of 0.3 Mol C/sq m/yr, upward dissolved inorganic carbon (DIC) bottom <span class="hlt">flux</span> of 1.1 Mol C/sq m/yr, and carbon export of 1.4 mol C/sq m/yr via sedimentation. Upper ocean DIC levels increased between 1992 and 1996 at a rate of approximately 1.2 (micro)mol/kg/yr, consistent with observations. However, this trend was reversed during 1997-1998 to -2.7 (micro)mol/kg/yr in response to hydrographic changes imposed by the El Nino-La Nina transition, which were manifested in the Sargasso <span class="hlt">Sea</span> by the warmest SST and lowest surface salinity of the period (1992-1998).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009GeoRL..3621605V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009GeoRL..3621605V"><span>A generalized model for the <span class="hlt">air-sea</span> transfer of dimethyl sulfide at high wind speeds</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vlahos, Penny; Monahan, Edward C.</p> <p>2009-11-01</p> <p>The <span class="hlt">air-sea</span> exchange of dimethyl sulfide (DMS) is an important component of ocean biogeochemistry and global climate models. Both laboratory experiments and field measurements of DMS transfer rates have shown that the <span class="hlt">air-sea</span> <span class="hlt">flux</span> of DMS is analogous to that of other significant greenhouse gases such as CO2 at low wind speeds (<10 m/s) but that these DMS transfer rates may diverge from other gases as wind speeds increase. Herein we provide a mechanism that predicts the attenuation of DMS transfer rates at high wind speeds. The model is based on the amphiphilic nature of DMS that leads to transfer delay at the water-bubble interface and becomes significant at wind speeds above >10 m/s. The result is an attenuation of the dimensionless Henry's Law constant (H) where (Heff = H/(1 + (Cmix/Cw) ΦB) by a solubility enhancement Cmix/Cw, and the fraction of bubble surface area per m2 surface ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010JGRC..11512054V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010JGRC..11512054V"><span>Upper ocean bubble measurements from the NE Pacific and estimates of their role in <span class="hlt">air-sea</span> gas transfer of the weakly soluble gases nitrogen and oxygen</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vagle, Svein; McNeil, Craig; Steiner, Nadja</p> <p>2010-12-01</p> <p>Simultaneous observations of upper-ocean bubble clouds, and dissolved gaseous nitrogen (N2) and oxygen (O2) from three winter storms are presented and analyzed. The data were collected on the Canadian Surface Ocean Lower Atmosphere Study (C-SOLAS) mooring located near Ocean Station Papa (OSP) at 50°N, 145°W in the NE Pacific during winter of 2003/2004. The bubble field was measured using an upward looking 200 kHz echosounder. Direct estimates of bubble mediated gas <span class="hlt">fluxes</span> were made using assumed bubble size spectra and the upward looking echosounder data. A one-dimensional biogeochemical model was used to help compare data and various existing models of bubble mediated <span class="hlt">air-sea</span> gas exchange. The direct bubble <span class="hlt">flux</span> calculations show an approximate quadratic/cubic dependence on mean bubble penetration depth. After scaling from N2/O2 to carbon dioxide, near surface, nonsupersaturating, <span class="hlt">air-sea</span> transfer rates, KT, for U10 > 12 m s-1 fall between quadratic and cubic relationships. Estimates of the subsurface bubble induced <span class="hlt">air</span> injection <span class="hlt">flux</span>, VT, show an approximate quadratic/cubic dependence on mean bubble penetration depth. Both KT and VT are much higher than those measured during Hurricane Frances over the wind speed range 12 < U10 < 23 m s-1. This result implies that over the open ocean and this wind speed range, older and more developed <span class="hlt">seas</span> which occur during winter storms are more effective in exchanging gases between the atmosphere and ocean than younger less developed <span class="hlt">seas</span> which occur during the rapid passage of a hurricane.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/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 transfer, images and <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> 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('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. 2006-2, 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. 2006-2 <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. 2006-2, May 2006 5a. CONTRACT NUMBER 5b. GRANT NUMBER 5c. PROGRAM ELEMENT NUMBER 6. AUTHOR(S) 5d. PROJECT</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/2017EGUGA..19.7608M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.7608M"><span>The impact of horizontal resolution on the representation of <span class="hlt">air-sea</span> interaction over North Atlantic open ocean convection sites</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moore, Kent; Renfrew, Ian; Bromwich, David; Wilson, Aaron; Vage, Kjetil; Bai, Lesheng</p> <p>2017-04-01</p> <p>Open ocean convection, where a loss of surface buoyancy leads to an overturning of the water column, occurs in four distinct regions of the North Atlantic and is an integral component of the Atlantic Meridional Overturning Circulation (AMOC). The overturning typically occurs during cold <span class="hlt">air</span> outbreaks characterized by large surface turbulent heat <span class="hlt">fluxes</span> and convective roll cloud development. Here we compare the statistics of the <span class="hlt">air-sea</span> interaction over these convection sites as represented in three reanalyses with horizontal grid sizes ranging from 80km to 15km. We show that increasing the resolution increases the magnitude and frequency of the most extreme total turbulent heat <span class="hlt">fluxes</span>, as well as displacing the maxima downstream away from the ice edges. We argue that these changes are a result of the higher resolution reanalysis being better able to represent mesoscale processes that occur within the atmospheric boundary layer during cold <span class="hlt">air</span> outbreaks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27670426','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27670426"><span>Using rare earth elements to constrain particulate organic carbon <span class="hlt">flux</span> 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>Hung, Chin-Chang; Chen, Ya-Feng; Hsu, Shih-Chieh; Wang, Kui; Chen, Jianfang; Burdige, David J</p> <p>2016-09-27</p> <p><span class="hlt">Fluxes</span> of particulate organic carbon (POC) in the East China <span class="hlt">Sea</span> (ECS) have been reported to decrease from the inner continental shelf towards the outer continental shelf. Recent research has shown that POC <span class="hlt">fluxes</span> in the ECS may be overestimated due to active sediment resuspension. To better characterize the effect of sediment resuspension on particle <span class="hlt">fluxes</span> in the ECS, rare earth elements (REEs) and organic carbon (OC) were used in separate two-member mixing models to evaluate trap-collected POC <span class="hlt">fluxes</span>. The ratio of resuspended particles from sediments to total trap-collected particles in the ECS ranged from 82-94% using the OC mixing model, and 30-80% using the REEs mixing model, respectively. These results suggest that REEs may be better proxies for sediment resuspension than OC in high turbidity marginal <span class="hlt">seas</span> because REEs do not appear to undergo degradation during particle sinking as compared to organic carbon. Our results suggest that REEs can be used as tracers to provide quantitative estimates of POC <span class="hlt">fluxes</span> in marginal <span class="hlt">seas</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5037389','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5037389"><span>Using rare earth elements to constrain particulate organic carbon <span class="hlt">flux</span> in the East China <span class="hlt">Sea</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>Hung, Chin-Chang; Chen, Ya-Feng; Hsu, Shih-Chieh; Wang, Kui; Chen, Jian Feng; Burdige, David J.</p> <p>2016-01-01</p> <p><span class="hlt">Fluxes</span> of particulate organic carbon (POC) in the East China <span class="hlt">Sea</span> (ECS) have been reported to decrease from the inner continental shelf towards the outer continental shelf. Recent research has shown that POC <span class="hlt">fluxes</span> in the ECS may be overestimated due to active sediment resuspension. To better characterize the effect of sediment resuspension on particle <span class="hlt">fluxes</span> in the ECS, rare earth elements (REEs) and organic carbon (OC) were used in separate two-member mixing models to evaluate trap-collected POC <span class="hlt">fluxes</span>. The ratio of resuspended particles from sediments to total trap-collected particles in the ECS ranged from 82–94% using the OC mixing model, and 30–80% using the REEs mixing model, respectively. These results suggest that REEs may be better proxies for sediment resuspension than OC in high turbidity marginal <span class="hlt">seas</span> because REEs do not appear to undergo degradation during particle sinking as compared to organic carbon. Our results suggest that REEs can be used as tracers to provide quantitative estimates of POC <span class="hlt">fluxes</span> in marginal <span class="hlt">seas</span>. PMID:27670426</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A41C2277B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A41C2277B"><span>Understanding the Role of <span class="hlt">Air-Sea</span> Interaction on Extreme Rainfall in Aquaplanet and Earth-like CESM2</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Benedict, J. J.; Clement, A. C.; Medeiros, B.</p> <p>2017-12-01</p> <p>Extreme precipitation events are associated with anomalous, latitudinally dependent dynamical and convective weather systems. For example, plumes of excessive poleward water vapor transport and topographical effects drive extreme precipitation events in the midlatitudes, while intense tropical precipitation is associated with organized convective systems. In both cases, <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> have the potential to contribute significantly to the moisture budget of these storms, but the roles of surface <span class="hlt">fluxes</span> and upper-ocean processes and their impact on precipitation extremes have yet to be explored in sufficient detail. To examine such mechanisms, we implement a climate model hierarchy that encompasses a spectrum of ocean models, from prescribed-SST to fully dynamic, as well as both aquaplanet and Earth-like lower boundary types within version 2 of the Community Earth System Model (CESM2). Using the CESM2 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/2016AtmEn.147..200O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AtmEn.147..200O"><span>Determination of temperature dependent Henry's law constants of polychlorinated naphthalenes: Application to <span class="hlt">air-sea</span> exchange in Izmir Bay, Turkey</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Odabasi, Mustafa; Adali, Mutlu</p> <p>2016-12-01</p> <p>The Henry's law constant (H) is a crucial variable to investigate the <span class="hlt">air</span>-water exchange of persistent organic pollutants. H values for 32 polychlorinated naphthalene (PCN) congeners were measured using an inert gas-stripping technique at five temperatures ranging between 5 and 35 °C. H values in deionized water (at 25 °C) varied between 0.28 ± 0.08 Pa m3 mol-1 (PCN-73) and 18.01 ± 0.69 Pa m3 mol-1 (PCN-42). The agreement between the measured and estimated H values from the octanol-water and octanol-<span class="hlt">air</span> partition coefficients was good (measured/estimated ratio = 1.00 ± 0.41, average ± SD). The calculated phase change enthalpies (ΔHH) were within the interval previously determined for other several semivolatile organic compounds (42.0-106.4 kJ mol-1). Measured H values, paired atmospheric and aqueous concentrations and meteorological variables were also used to reveal the level and direction of <span class="hlt">air-sea</span> exchange <span class="hlt">fluxes</span> of PCNs at the coast of Izmir Bay, Turkey. The net PCN <span class="hlt">air-sea</span> exchange <span class="hlt">flux</span> varied from -0.55 (volatilization, PCN-24/14) to 2.05 (deposition, PCN-23) ng m-2 day-1. PCN-19, PCN-24/14, PCN-42, and PCN-33/34/37 were mainly volatilized from seawater while the remaining congeners were mainly deposited. The overall number of the cases showing deposition was higher (67.9%) compared to volatilization (21.4%) and near equilibrium (10.7%).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22775202','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22775202"><span>Measurement of <span class="hlt">air</span> and VOC vapor <span class="hlt">fluxes</span> during gas-driven soil remediation: bench-scale experiments.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kim, Heonki; Kim, Taeyun; Shin, Seungyeop; Annable, Michael D</p> <p>2012-09-04</p> <p>In this laboratory study, an experimental method was developed for the quantitative analyses of gas <span class="hlt">fluxes</span> in soil during advective <span class="hlt">air</span> flow. One-dimensional column and two- and three-dimensional flow chamber models were used in this study. For the <span class="hlt">air</span> <span class="hlt">flux</span> measurement, n-octane vapor was used as a tracer, and it was introduced in the <span class="hlt">air</span> flow entering the physical models. The tracer (n-octane) in the gas effluent from the models was captured for a finite period of time using a pack of activated carbon, which then was analyzed for the mass of n-octane. The <span class="hlt">air</span> <span class="hlt">flux</span> was calculated based on the mass of n-octane captured by the activated carbon and the inflow concentration. The measured <span class="hlt">air</span> <span class="hlt">fluxes</span> are in good agreement with the actual values for one- and two-dimensional model experiments. Using both the two- and three-dimensional models, the distribution of the <span class="hlt">air</span> <span class="hlt">flux</span> at the soil surface was measured. The distribution of the <span class="hlt">air</span> <span class="hlt">flux</span> was found to be affected by the depth of the saturated zone. The <span class="hlt">flux</span> and <span class="hlt">flux</span> distribution of a volatile contaminant (perchloroethene) was also measured by using the two-dimensional model. Quantitative information of both <span class="hlt">air</span> and contaminant <span class="hlt">flux</span> may be very beneficial for analyzing the performance of gas-driven subsurface remediation processes including soil vapor extraction and <span class="hlt">air</span> sparging.</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=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/2017EGUGA..19.2080D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.2080D"><span>Wind stress and heat <span class="hlt">fluxes</span> over a Brazilian Coastal Upwelling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dourado, Marcelo; Candella, Rogério</p> <p>2017-04-01</p> <p>Coastal upwelling zones have been intensively studied in the last decades especially due to their importance to the biological cycle. The coastal upwelling system of the Cabo Frio region (east coast of the Rio de Janeiro state, Brazil) keeps the surface water cold during most part of the year, what induces a stable atmospheric boundary layer associated to northeast winds. The main goal of this study is to investigate the wind stress and heat <span class="hlt">fluxes</span> exchanges between the ocean and the atmosphere in that area. For this purpose, a set of hourly data meteorological and oceanographic data collected by a Wavescan metocean buoy anchored at 23o59S; 42oW, were used, as well as solar radiation and relative humidity from a terrestrial meteorological station from the Instituto Nacional de Meteorologia (InMet). COARE 3.0 algorithm was used to calculate the latent and sensible heat <span class="hlt">fluxes</span>. In this discussion, positive values represent <span class="hlt">fluxes</span> towards the ocean. The average net heat <span class="hlt">flux</span> over our study period is 88 W m-2. The reduction of the net heat <span class="hlt">flux</span> is due to the increase of the ocean latent heat loss, although a reduction in incoming shortwave radiation and an increase in ocean long wave cooling also contributes. The latent heat is 20 times larger than the sensible heat <span class="hlt">flux</span>, but the mean value of the latent heat <span class="hlt">flux</span>, 62 W m-2, is half the typical value found in open ocean. The temporal variability of both sensible and latent heat <span class="hlt">fluxes</span> reflects their dependence on wind speed and <span class="hlt">air-sea</span> temperature differences. When upwelling events, here periods when diurnal SST is lower than 18oC, are compared with undisturbed (without upwelling) events, it can be noted the sensible heat <span class="hlt">fluxes</span> are positives and 10 times greater in magnitude. This is related to an increment, during these upwelling events, of the <span class="hlt">air-sea</span> temperature difference and an increasing of the wind speed. The cold waters of the upwelling increase the <span class="hlt">air-sea</span> temperature gradient and, also, the horizontal land-<span class="hlt">sea</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AMT.....9.5509Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AMT.....9.5509Y"><span>Comparison of two closed-path cavity-based spectrometers for measuring <span class="hlt">air</span>-water CO2 and CH4 <span class="hlt">fluxes</span> by eddy covariance</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, Mingxi; Prytherch, John; Kozlova, Elena; Yelland, Margaret J.; Parenkat Mony, Deepulal; Bell, Thomas G.</p> <p>2016-11-01</p> <p>In recent years several commercialised closed-path cavity-based spectroscopic instruments designed for eddy covariance <span class="hlt">flux</span> measurements of carbon dioxide (CO2), methane (CH4), and water vapour (H2O) 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 CO2 and CH4 based on concurrently measured H2O, temperature, and pressure. Additionally, we used a high throughput Nafion dryer to physically remove H2O from the Picarro airstream. Observed <span class="hlt">air-sea</span> CO2 and CH4 <span class="hlt">fluxes</span> from these two analysers, averaging about 12 and 0.12 mmol m-2 day-1 respectively, agree within the measurement uncertainties. For the purpose of quantifying dry CO2 and CH4 <span class="hlt">fluxes</span> downstream of a long inlet, the numerical H2O corrections appear to be reasonably effective and lead to results that are comparable to physical removal of H2O with a Nafion dryer in the mean. We estimate the high-frequency attenuation of <span class="hlt">fluxes</span> in our closed-path set-up, which was relatively small ( ≤ 10 %) for CO2 and CH4 but very large for the more polar H2O. The Picarro showed significantly lower noise and <span class="hlt">flux</span> detection limits than the LGR. The hourly <span class="hlt">flux</span> detection limit for the Picarro was about 2 mmol m-2 day-1 for CO2 and 0.02 mmol m-2 day-1 for CH4. For the LGR these detection limits were about 8 and 0.05 mmol m-2 day-1. Using global maps of monthly mean <span class="hlt">air-sea</span> CO2 <span class="hlt">flux</span> as reference, we estimate that the Picarro and LGR can resolve hourly CO2 <span class="hlt">fluxes</span> from roughly 40 and 4 % of the world's oceans respectively. Averaging over longer timescales would be required in regions with smaller <span class="hlt">fluxes</span>. Hourly <span class="hlt">flux</span> detection limits of CH4 from both instruments are generally higher than the expected emissions from the open ocean, though the signal to noise of this measurement may improve closer to the coast.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRC..123..922L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRC..123..922L"><span>Observed Seasonal Variations of the Upper Ocean Structure and <span class="hlt">Air-Sea</span> Interactions in the Andaman <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>Liu, Yanliang; Li, Kuiping; Ning, Chunlin; Yang, Yang; Wang, Haiyuan; Liu, Jianjun; Skhokiattiwong, Somkiat; Yu, Weidong</p> <p>2018-02-01</p> <p>The Andaman <span class="hlt">Sea</span> (AS) is a poorly observed basin, where even the fundamental physical characteristics have not been fully documented. Here the seasonal variations of the upper ocean structure and the <span class="hlt">air-sea</span> interactions in the central AS were studied using a moored surface buoy. The seasonal double-peak pattern of the <span class="hlt">sea</span> surface temperature (SST) was identified with the corresponding mixed layer variations. Compared with the buoys in the Bay of Bengal (BOB), the thermal stratification in the central AS was much stronger in the winter to spring, when a shallower isothermal layer and a thinner barrier layer were sustained. The temperature inversion was strongest from June to July because of substantial surface heat loss and subsurface prewarming. The heat budget analysis of the mixed layer showed that the net surface heat <span class="hlt">fluxes</span> dominated the seasonal SST cycle. Vertical entrainment was significant from April to July. It had a strong cooling effect from April to May and a striking warming effect from June to July. A sensitivity experiment highlighted the importance of salinity. The AS warmer surface water in the winter was associated with weak heat loss caused by weaker longwave radiation and latent heat losses. However, the AS latent heat loss was larger than the BOB in summer due to its lower relative humidity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013DSRII..97...43S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013DSRII..97...43S"><span>Concentration, solubility and deposition <span class="hlt">flux</span> of atmospheric particulate nutrients over the Yellow <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shi, Jin-Hui; Zhang, Jing; Gao, Hui-Wang; Tan, Sai-Chun; Yao, Xiao-Hong; Ren, Jing-Ling</p> <p>2013-12-01</p> <p>Satellite images showed that two large dust storms swept over the Yellow <span class="hlt">Sea</span> from 31 Mach to 1 April 2007; both were accompanied by precipitation. Three to four days after the dust episodes, blooms occurred in the Yellow <span class="hlt">Sea</span>. As an important and potential controlling factor of the bloom, nutrients in the total suspended particle (TSP) and size-segregated particle samples during the cruise campaign were measured and their atmospheric deposition <span class="hlt">fluxes</span> of nutrients are reported in this paper. Concentrations of total P and TIN (NH4+, NO2- and NO3-) in TSP varied from 0.01 to 1.05 μg m-3, and from 1.21 to 22.28 μg m-3, with the maximum occurring concurrently with the dust storm events. In addition, the measured solubility of Fe in these particles varied from 1.0 to 20.1%, while it ranged from 0.8 to 15% for Al. The total deposition <span class="hlt">fluxes</span> of Asian dust as well as the contained nutrients were estimated on the basis of an episodic increment of the measured concentration of dissolved Al in the surface ocean during the dust events. The estimated <span class="hlt">fluxes</span> of atmospheric deposition of soluble Fe, P and inorganic nitrogen over the Yellow <span class="hlt">Sea</span> during the dust episodes were 42.5±10.9, 10.3±2.6 and 772.0±198.0 mg m-2, respectively. The estimated <span class="hlt">fluxes</span> of nutrients via dry atmospheric deposition accounted for only ~2% of the total <span class="hlt">fluxes</span>. The deposition <span class="hlt">fluxes</span> of particulate Fe and P during the two dust storm events associated with precipitation were about 500-1000 times of that daily averaged <span class="hlt">flux</span> during non-dust days, indicating the importance of the episodic inputs to the annual budget of these metals deposited into the ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009EGUGA..11.6008T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009EGUGA..11.6008T"><span>Influences of Ocean Thermohaline Stratification on 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>Toole, J. M.; Timmermans, M.-L.; Perovich, D. K.; Krishfield, R. A.; Proshutinsky, A.; Richter-Menge, J. A.</p> <p>2009-04-01</p> <p>The Arctic Ocean's surface mixed layer constitutes the dynamical and thermodynamical link between the <span class="hlt">sea</span> ice and the underlying waters. Wind stress, acting directly on the surface mixed layer or via wind-forced ice motion, produce surface currents that can in turn drive deep ocean flow. Mixed layer temperature is intimately related to basal <span class="hlt">sea</span> ice growth and melting. Heat <span class="hlt">fluxes</span> into or out of the surface mixed layer can occur at both its upper and lower interfaces: the former via <span class="hlt">air-sea</span> exchange at leads and conduction through the ice, the latter via turbulent mixing and entrainment at the layer base. Variations in Arctic Ocean mixed layer properties are documented based on more than 16,000 temperature and salinity profiles acquired by Ice-Tethered Profilers since summer 2004 and analyzed in conjunction with <span class="hlt">sea</span> ice observations from Ice Mass Balance Buoys and atmospheric heat <span class="hlt">flux</span> estimates. Guidance interpreting the observations is provided by a one-dimensional ocean mixed layer model. The study focuses attention on the very strong density stratification about the mixed layer base in the Arctic that, in regions of <span class="hlt">sea</span> ice melting, is increasing with time. The intense stratification greatly impedes mixed layer deepening by vertical convection and shear mixing, and thus limits the <span class="hlt">flux</span> of deep ocean heat to the surface that could influence <span class="hlt">sea</span> ice growth/decay. Consistent with previous work, this study demonstrates that the Arctic <span class="hlt">sea</span> ice is most sensitive to changes in ocean mixed layer heat resulting from <span class="hlt">fluxes</span> across its upper (<span class="hlt">air-sea</span> and/or ice-water) interface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoRL..45.5002O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoRL..45.5002O"><span>Episodic Southern Ocean Heat Loss and Its Mixed Layer Impacts Revealed by the Farthest South Multiyear Surface <span class="hlt">Flux</span> Mooring</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ogle, S. E.; Tamsitt, V.; Josey, S. A.; Gille, S. T.; Cerovečki, I.; Talley, L. D.; Weller, R. A.</p> <p>2018-05-01</p> <p>The Ocean Observatories Initiative <span class="hlt">air-sea</span> <span class="hlt">flux</span> mooring deployed at 54.08°S, 89.67°W, in the southeast Pacific sector of the Southern Ocean, is the farthest south long-term open ocean <span class="hlt">flux</span> mooring ever deployed. Mooring observations (February 2015 to August 2017) provide the first in situ quantification of annual net <span class="hlt">air-sea</span> heat exchange from one of the prime Subantarctic Mode Water formation regions. Episodic turbulent heat loss events (reaching a daily mean net <span class="hlt">flux</span> of -294 W/m2) generally occur when northeastward winds bring relatively cold, dry <span class="hlt">air</span> to the mooring location, leading to large <span class="hlt">air-sea</span> temperature and humidity differences. Wintertime heat loss events promote deep mixed layer formation that lead to Subantarctic Mode Water formation. However, these processes have strong interannual variability; a higher frequency of 2 σ and 3 σ turbulent heat loss events in winter 2015 led to deep mixed layers (>300 m), which were nonexistent in winter 2016.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.8646L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.8646L"><span>Ra Tracer-Based Study of Submarine Groundwater Discharge and Associated Nutrient <span class="hlt">Fluxes</span> into the Bohai <span class="hlt">Sea</span>, China: A Highly Human-Affected Marginal <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>Liu, Jianan; Du, Jinzhou; Yi, Lixin</p> <p>2017-11-01</p> <p>Nutrient concentrations in coastal bays and estuaries are strongly influenced by not only riverine input but also submarine groundwater discharge (SGD). Here we estimate the SGD and the <span class="hlt">fluxes</span> of the associated dissolved inorganic nitrogen (DIN), phosphorus (DIP), and silicon (DSi) into the Bohai <span class="hlt">Sea</span> based on a 226Ra and 228Ra mass balance model. This procedure shows that in the Bohai <span class="hlt">Sea</span> the average radium activities (dpm 100 L-1) are 42.8 ± 6.3 (226Ra) and 212 ± 41.7 (228Ra) for the surface water and 43.0 ± 6.1 (226Ra) and 216 ± 38.4 (228Ra) for the near-bottom water. According to the 228Ra/226Ra age model, the residence time in the Bohai <span class="hlt">Sea</span> is calculated to be 1.7 ± 0.8 yrs. The mass balance of 226Ra and 228Ra suggests that the yearly SGD <span class="hlt">flux</span> into the whole Bohai <span class="hlt">Sea</span> is (2.0 ± 1.3) × 1011 m3 yr-1, of which the percentage of submarine fresh groundwater discharge (SFGD) to the total SGD is approximately (5.1 ± 4.1)%. However, the DIN and DSi <span class="hlt">fluxes</span> from SFGD constitute 29% and 10%, respectively, of the total <span class="hlt">fluxes</span> from the SGD. Moreover, nutrient loads, which exhibit high DIN/DIP from SGD, especially the SFGD, may substantially contribute to the nutrient supplies, resulting in the occurrence of red tide in the Bohai <span class="hlt">Sea</span>.</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> CO2 <span class="hlt">flux</span> is largely dependent on the parametrization chosen. In addition, the different parametrizations all the underlying processes that in some way impact the carbon cycle beyond the carbonate dissociation and <span class="hlt">fluxes</span> give results that can be significantly different. Examples of these processes are phytoplankton growth rates or remineralization rates. Despite their geographical proximity, the North and Baltic <span class="hlt">Seas</span> exhibit very different dynamics. The North <span class="hlt">Sea</span> receives important inflows of Atlantic waters, while the Baltic <span class="hlt">Sea</span> is an almost enclosed system, with very little exchange from the North <span class="hlt">Sea</span>. Wind, tides, and freshwater supply act very differently, but dominantly structure the ecosystem dynamics on spatial and temporal scales. The biological community is also different. Cyanobacteria, which are important due to their ability to fix atmospheric nitrogen, and they are only present in the Baltic <span class="hlt">Sea</span>. These differentiating features have a strong impact in the biogeochemical cycles and ultimately shape the variations in the carbonate chemistry. Here the ECOSMO model was employed on the North <span class="hlt">Sea</span> and Baltic <span class="hlt">Sea</span>. The model is set so both are modelled at the same time, instead of having them run separately. ECOSMO is a 3-D coupled</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('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/2017AGUFMOS31B1395R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMOS31B1395R"><span>Monthly <span class="hlt">Sea</span> Surface Salinity and Freshwater <span class="hlt">Flux</span> Monitoring</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ren, L.; Xie, P.; Wu, S.</p> <p>2017-12-01</p> <p>Taking advantages of the complementary nature of the <span class="hlt">Sea</span> Surface Salinity (SSS) measurements from the in-situ (CTDs, shipboard, Argo floats, etc.) and satellite retrievals from Soil Moisture Ocean Salinity (SMOS) satellite of the European Space Agency (ESA), the Aquarius of a joint venture between US and Argentina, and the Soil Moisture Active Passive (SMAP) of national Aeronautics and Space Administration (NASA), a technique is developed at NOAA/NCEP/CPC to construct an analysis of monthly SSS, called the NOAA Blended Analysis of <span class="hlt">Sea</span>-Surface Salinity (BASS). The algorithm is a two-steps approach, i.e. to remove the bias in the satellite data through Probability Density Function (PDF) matching against co-located in situ measurements; and then to combine the bias-corrected satellite data with the in situ measurements through the Optimal Interpolation (OI) method. The BASS SSS product is on a 1° by 1° grid over the global ocean for a 7-year period from 2010. Combined with the NOAA/NCEP/CPC CMORPH satellite precipitation (P) estimates and the Climate Forecast System Reanalysis (CFSR) evaporation (E) fields, a suite of monthly package of the SSS and oceanic freshwater <span class="hlt">flux</span> (E and P) was developed to monitor the global oceanic water cycle and SSS on a monthly basis. The SSS in BASS product is a suite of long-term SSS and fresh water <span class="hlt">flux</span> data sets with temporal homogeneity and inter-component consistency better suited for the examination of the long-term changes and monitoring. It presents complete spatial coverage and improved resolution and accuracy, which facilitates the diagnostic analysis of the relationship and co-variability among SSS, freshwater <span class="hlt">flux</span>, mixed layer processes, oceanic circulation, and assimilation of SSS into global models. At the AGU meeting, we will provide more details on the CPC salinity and fresh water <span class="hlt">flux</span> data package and its applications in the monitoring and analysis of SSS variations in association with the ENSO and other major climate</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('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> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li class="active"><span>10</span></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_10 --> <div id="page_11" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="201"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014DSRI...87...14H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014DSRI...87...14H"><span>Vertical export <span class="hlt">flux</span> of metals 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>Heimbürger, Lars-Eric; Migon, Christophe; Losno, Rémi; Miquel, Juan-Carlos; Thibodeau, Benoît; Stabholz, Marion; Dufour, Aurélie; Leblond, Nathalie</p> <p>2014-05-01</p> <p>We examined metal (Al, V, Cr, Mn, Fe, Ni, Cu, Zn, Cd and Pb) and particulate organic carbon (OC) concentrations of the marine vertical export <span class="hlt">flux</span> at the DYFAMED time-series station in the Northwestern Mediterranean <span class="hlt">Sea</span>. We present here the first data set of natural and anthropogenic metals from sediment trap moorings deployed at 1000 m-depth between 2003 and 2007 at the DYFAMED site. A highly significant correlation was observed between most metal concentrations, whatever the nature and emission source of the metal. Cu, Zn and Cd exhibit different behaviors, presumably due to their high solubility and complexation with organic ligands. The observed difference of atmospheric and marine <span class="hlt">fluxes</span> in terms of temporal variability and elemental concentration suggests that dense water convection and primary production and not atmospheric deposition control the marine vertical export <span class="hlt">flux</span>. This argument is strengthened by the fact that significant Saharan dust events did not result in concomitant marine vertical export <span class="hlt">fluxes</span> nor did they generate significant changes in metal concentrations of trapped particles.</p> </li> <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> transfer 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> transfer <span class="hlt">flux</span> 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 <span class="hlt">flux</span> calculation, the transfer 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 2.2 % of the total discharge amount of the coal-fired power plant in the sampling area (1 km(2)), 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://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 CO2 <span class="hlt">flux</span> in the tropical Atlantic Ocean determined from Rn-222 and pCO2 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 pCO2 data measured in the surface water and <span class="hlt">air</span> samples, the net <span class="hlt">flux</span> of CO2 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> CO2 <span class="hlt">flux</span> observed in the equatorial zone are examined.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016NatCo...710525Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016NatCo...710525Y"><span>Recent increases in Arctic freshwater <span class="hlt">flux</span> affects Labrador <span class="hlt">Sea</span> convection and Atlantic overturning circulation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, Qian; Dixon, Timothy H.; Myers, Paul G.; Bonin, Jennifer; Chambers, Don; van den Broeke, M. R.</p> <p>2016-01-01</p> <p>The Atlantic Meridional Overturning Circulation (AMOC) is an important component of ocean thermohaline circulation. Melting of Greenland's ice sheet is freshening the North Atlantic; however, whether the augmented freshwater <span class="hlt">flux</span> is disrupting the AMOC is unclear. Dense Labrador <span class="hlt">Sea</span> Water (LSW), formed by winter cooling of saline North Atlantic water and subsequent convection, is a key component of the deep southward return flow of the AMOC. Although LSW formation recently decreased, it also reached historically high values in the mid-1990s, making the connection to the freshwater <span class="hlt">flux</span> unclear. Here we derive a new estimate of the recent freshwater <span class="hlt">flux</span> from Greenland using updated GRACE satellite data, present new <span class="hlt">flux</span> estimates for heat and salt from the North Atlantic into the Labrador <span class="hlt">Sea</span> and explain recent variations in LSW formation. We suggest that changes in LSW can be directly linked to recent freshening, and suggest a possible link to AMOC weakening.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4736158','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4736158"><span>Recent increases in Arctic freshwater <span class="hlt">flux</span> affects Labrador <span class="hlt">Sea</span> convection and Atlantic overturning circulation</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Yang, Qian; Dixon, Timothy H.; Myers, Paul G.; Bonin, Jennifer; Chambers, Don; van den Broeke, M. R.; Ribergaard, Mads H.; Mortensen, John</p> <p>2016-01-01</p> <p>The Atlantic Meridional Overturning Circulation (AMOC) is an important component of ocean thermohaline circulation. Melting of Greenland's ice sheet is freshening the North Atlantic; however, whether the augmented freshwater <span class="hlt">flux</span> is disrupting the AMOC is unclear. Dense Labrador <span class="hlt">Sea</span> Water (LSW), formed by winter cooling of saline North Atlantic water and subsequent convection, is a key component of the deep southward return flow of the AMOC. Although LSW formation recently decreased, it also reached historically high values in the mid-1990s, making the connection to the freshwater <span class="hlt">flux</span> unclear. Here we derive a new estimate of the recent freshwater <span class="hlt">flux</span> from Greenland using updated GRACE satellite data, present new <span class="hlt">flux</span> estimates for heat and salt from the North Atlantic into the Labrador <span class="hlt">Sea</span> and explain recent variations in LSW formation. We suggest that changes in LSW can be directly linked to recent freshening, and suggest a possible link to AMOC weakening. PMID:26796579</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26796579','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26796579"><span>Recent increases in Arctic freshwater <span class="hlt">flux</span> affects Labrador <span class="hlt">Sea</span> convection and Atlantic overturning circulation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yang, Qian; Dixon, Timothy H; Myers, Paul G; Bonin, Jennifer; Chambers, Don; van den Broeke, M R</p> <p>2016-01-22</p> <p>The Atlantic Meridional Overturning Circulation (AMOC) is an important component of ocean thermohaline circulation. Melting of Greenland's ice sheet is freshening the North Atlantic; however, whether the augmented freshwater <span class="hlt">flux</span> is disrupting the AMOC is unclear. Dense Labrador <span class="hlt">Sea</span> Water (LSW), formed by winter cooling of saline North Atlantic water and subsequent convection, is a key component of the deep southward return flow of the AMOC. Although LSW formation recently decreased, it also reached historically high values in the mid-1990s, making the connection to the freshwater <span class="hlt">flux</span> unclear. Here we derive a new estimate of the recent freshwater <span class="hlt">flux</span> from Greenland using updated GRACE satellite data, present new <span class="hlt">flux</span> estimates for heat and salt from the North Atlantic into the Labrador <span class="hlt">Sea</span> and explain recent variations in LSW formation. We suggest that changes in LSW can be directly linked to recent freshening, and suggest a possible link to AMOC weakening.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A21H2245L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A21H2245L"><span>Impact of Land-<span class="hlt">Sea</span> Thermal Contrast on Inland Penetration of <span class="hlt">Sea</span> Fog over The Yellow <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lee, H. Y.; Chang, E. C.</p> <p>2017-12-01</p> <p><span class="hlt">Sea</span> fog can be classified into a cold <span class="hlt">sea</span> fog that occurs when <span class="hlt">sea</span> surface temperature (SST) is colder than <span class="hlt">sea</span> <span class="hlt">air</span> temperature (SAT) and a warm <span class="hlt">sea</span> fog that occurs when the SST is warmer than the SAT. We simulated two <span class="hlt">sea</span> fog events over the Yellow <span class="hlt">Sea</span> which is surrounded by Korean Peninsula and mainland China using Weather Research and Forecasting (WRF) model. Our first aim is to understand contributions of major factors for the <span class="hlt">sea</span> fog formation. First, the two <span class="hlt">sea</span> fog events are designated as cold and warm types, and cooling rates as well as moistening rates are calculated employing bulk aerodynamic methods. Both cases show cooling and moistening by turbulent <span class="hlt">fluxes</span> play an important role in condensation either favorably or unfavorably. However, longwave radiative cooling is as or even stronger than turbulent cooling, suggesting it is the most decisive factor in formation of <span class="hlt">sea</span> fogs regardless of their type. Our second purpose of the study is to understand inland penetration of <span class="hlt">sea</span> fog in terms of thermal contrast (TC) and it was conducted through sensitivity tests of SST and land skin temperature (LST). In the SST sensitivity tests, increase of SSTs lead to that of upward turbulent heat <span class="hlt">fluxes</span> so that SATs rise which are responsible for evaporation of cloud waters and it is common response of the two events. In addition, change of the SST induce that of the TC and may affect the inland penetration of <span class="hlt">sea</span> fog. However, when the cloud waters over the <span class="hlt">sea</span> evaporate, it is hard to fully determine the inland penetration. As a remedy for this limitation, LST is now modified instead of SST to minimize the evaporation effect, maintaining the equivalent TC. In the case of cold <span class="hlt">sea</span> fog, land <span class="hlt">air</span> temperature (LAT) is warmer than SAT. Here, decrease of the LAT leads to weakening of the TC and favors the inland penetration. On the other hand, LAT is colder than the SAT in the warm <span class="hlt">sea</span> fog event. When the LAT decreases, the TC is intensified resulting in blocking of the</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 CO2 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 CO2 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 pCO2(<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, pCO2(<span class="hlt">sea</span>) decreased gradually toward the west as a result of biological CO2 uptake and surface <span class="hlt">sea</span> temperature increase. Between 179°E and 170°E, the pCO2(<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, pCO2(<span class="hlt">sea</span>) was nearly equal to pCO2(<span class="hlt">air</span>). The distribution of the atmospheric CO2 concentration showed a considerable variability (±3ppm) in the area north of the Intertropical Convergence Zone due to the regional net source-sink strength of the terrestrial biosphere. The net CO2 <span class="hlt">flux</span> from the <span class="hlt">sea</span> to the atmosphere in the equatorial region of the central and western Pacific (15°S-10°N, 140°E-150°W) was evaluated from the ΔpCO2 distribution and the several gas transfer coefficients reported so far. It ranged from 0.13 GtC year<img src="/entityImage/script/2212.gif" alt="-" border="0" style="font-weight: bold"></img>1-0.29 GtC year<img src="/entityImage/script/2212.gif" alt="-" border="0" style="font-weight: bold"></img>1. This CO2 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/2017AGUFM.C33C1202F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C33C1202F"><span>Determination of a Critical <span class="hlt">Sea</span> Ice Thickness Threshold for the Central 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>Ford, V.; Frauenfeld, O. W.; Nowotarski, C. J.</p> <p>2017-12-01</p> <p>While <span class="hlt">sea</span> ice extent is readily measurable from satellite observations and can be used to assess the overall survivability of the Arctic <span class="hlt">sea</span> ice pack, determining the spatial variability of <span class="hlt">sea</span> ice thickness remains a challenge. Turbulent and conductive heat <span class="hlt">fluxes</span> are extremely sensitive to ice thickness but are dominated by the sensible heat <span class="hlt">flux</span>, with energy exchange expected to increase with thinner ice cover. <span class="hlt">Fluxes</span> over open water are strongest and have the greatest influence on the atmosphere, while <span class="hlt">fluxes</span> over thick <span class="hlt">sea</span> ice are minimal as heat conduction from the ocean through thick ice cannot reach the atmosphere. We know that turbulent energy <span class="hlt">fluxes</span> are strongest over open ocean, but is there a "critical thickness of ice" where <span class="hlt">fluxes</span> are considered non-negligible? Through polar-optimized Weather Research and Forecasting model simulations, this study assesses how the wintertime Arctic surface boundary layer, via sensible heat <span class="hlt">flux</span> exchange and surface <span class="hlt">air</span> temperature, responds to <span class="hlt">sea</span> ice thinning. The region immediately north of Franz Josef Land is characterized by a thickness gradient where <span class="hlt">sea</span> ice transitions from the thickest multi-year ice to the very thin marginal ice <span class="hlt">seas</span>. This provides an ideal location to simulate how the diminishing Arctic <span class="hlt">sea</span> ice interacts with a warming atmosphere. Scenarios include both fixed <span class="hlt">sea</span> surface temperature domains for idealized thickness variability, and fixed ice fields to detect changes in the ocean-ice-atmosphere energy exchange. Results indicate that a critical thickness threshold exists below 1 meter. The threshold is between 0.4-1 meters thinner than the critical thickness for melt season survival - the difference between first year and multi-year ice. Turbulent heat <span class="hlt">fluxes</span> and surface <span class="hlt">air</span> temperature increase as <span class="hlt">sea</span> ice thickness transitions from perennial ice to seasonal ice. While models predict a <span class="hlt">sea</span> ice free Arctic at the end of the warm season in future decades, <span class="hlt">sea</span> ice will continue to transform</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> CO 2 <span class="hlt">flux</span> based on climatological surface ocean pCO 2, 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 pCO 2 obtained since the International Geophysical Year of 1956-59, the climatological, monthly distribution of pCO 2 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> CO 2 <span class="hlt">flux</span> has been computed using the NCEP/NCAR 41-year mean monthly wind speeds. An annual net uptake <span class="hlt">flux</span> of CO 2 by the global oceans has been estimated to be 2.2 (+22% or -19%) Pg C yr -1 using the (wind speed) 2 dependence of the CO 2 gas transfer velocity of Wanninkhof (J. Geophys. Res. 97 (1992) 7373). The errors associated with the wind-speed variation have been estimated using one standard deviation (about±2 m s -1) from the mean monthly wind speed observed over each 4°×5° pixel area of the global oceans. The new global uptake <span class="hlt">flux</span> obtained with the Wanninkhof (wind speed) 2 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±0.2 Pg C yr -1. This estimate for the global ocean uptake <span class="hlt">flux</span> is consistent with the values of 2.0±0.6 Pg C yr -1 estimated on the basis of the observed changes in the atmospheric CO 2 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 CO 2. In these areas, poleward-flowing warm waters meet and mix with the cold subpolar waters rich in nutrients. The pCO 2 in the surface water is decreased by the cooling effect on warm waters and by the biological drawdown of pCO 2 in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19830046452&hterms=water+gas+exchange&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dwater%2Bgas%2Bexchange','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19830046452&hterms=water+gas+exchange&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dwater%2Bgas%2Bexchange"><span>Methane <span class="hlt">flux</span> across the <span class="hlt">air</span>-water interface - <span class="hlt">Air</span> velocity effects</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sebacher, D. I.; Harriss, R. C.; Bartlett, K. B.</p> <p>1983-01-01</p> <p>Methane loss to the atmosphere from flooded wetlands is influenced by the degree of supersaturation and wind stress at the water surface. Measurements in freshwater ponds in the St. Marks Wildlife Refuge, Florida, demonstrated that for the combined variability of CH4 concentrations in surface water and <span class="hlt">air</span> velocity over the water surface, CH4 <span class="hlt">flux</span> varied from 0.01 to 1.22 g/sq m/day. The liquid exchange coefficient for a two-layer model of the gas-liquid interface was calculated as 1.7 cm/h for CH4 at <span class="hlt">air</span> velocity of zero and as 1.1 + 1.2 v to the 1.96th power cm/h for <span class="hlt">air</span> velocities from 1.4 to 3.5 m/s and water temperatures of 20 C.</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('http://adsabs.harvard.edu/abs/2014AGUFM.A41B3033D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.A41B3033D"><span>Estimating Turbulent Surface <span class="hlt">Fluxes</span> from Small Unmanned Aircraft: Evaluation of Current Abilities</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>de Boer, G.; Lawrence, D.; Elston, J.; Cassano, J. J.; Mack, J.; Wildmann, N.; Nigro, M. A.; Ivey, M.; Wolfe, D. E.; Muschinski, A.</p> <p>2014-12-01</p> <p>Heat transfer between the atmosphere and Earth's surface represents a key component to understanding Earth energy balance, making it important in understanding and simulating climate. Arguably, the oceanic <span class="hlt">air-sea</span> interface and Polar <span class="hlt">sea-ice-air</span> interface are amongst the most challenging in which to measure these <span class="hlt">fluxes</span>. This difficulty results partially from challenges associated with infrastructure deployment on these surfaces and partially from an inability to obtain spatially representative values over a potentially inhomogeneous surface. Traditionally sensible (temperature) and latent (moisture) <span class="hlt">fluxes</span> are estimated using one of several techniques. A preferred method involves eddy-correlation where cross-correlation between anomalies in vertical motion (w) and temperature (T) or moisture (q) is used to estimate heat transfer. High-frequency measurements of these quantities can be derived using tower-mounted instrumentation. Such systems have historically been deployed over land surfaces or on ships and buoys to calculate <span class="hlt">fluxes</span> at the <span class="hlt">air</span>-land or <span class="hlt">air-sea</span> interface, but such deployments are expensive and challenging to execute, resulting in a lack of spatially diverse measurements. A second ("bulk") technique involves the observation of horizontal windspeed, temperature and moisture at a given altitude over an extended time period in order to estimate the surface <span class="hlt">fluxes</span>. Small Unmanned Aircraft Systems (sUAS) represent a unique platform from which to derive these <span class="hlt">fluxes</span>. These sUAS can be small ( 1 m), lightweight ( 700 g), low cost ( $2000) and relatively easy to deploy to remote locations and over inhomogeneous surfaces. We will give an overview of the ability of sUAS to provide measurements necessary for estimating surface turbulent <span class="hlt">fluxes</span>. This discussion is based on flights in the vicinity of the 1000 ft. Boulder Atmospheric Observatory (BAO) tower, and over the US Department of Energy facility at Oliktok Point, Alaska. We will present initial comparisons</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFMGC23D0949W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFMGC23D0949W"><span>The Oceanic <span class="hlt">Flux</span> Program: A three decade time-series of particle <span class="hlt">flux</span> in the deep Sargasso <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Weber, J. C.; Conte, M. H.</p> <p>2010-12-01</p> <p>The Oceanic <span class="hlt">Flux</span> Program (OFP), 75 km SE of Bermuda, is the longest running time-series of its kind. Initiated in 1978, the OFP has produced an unsurpassed, nearly continuous record of temporal variability in deep ocean <span class="hlt">fluxes</span>, with a >90% temporal coverage at 3200m depth. The OFP, in conjunction with the co-located Bermuda-Atlantic Time Series (BATS) and the Bermuda Testbed Mooring (BTM) time-series, has provided key observations enabling detailed assessment of how seasonal and non-seasonal variability in the deep ocean is linked with the overlying physical and biogeochemical environment. This talk will focus on the short-term <span class="hlt">flux</span> variability that overlies the seasonal <span class="hlt">flux</span> pattern in the Sargasso <span class="hlt">Sea</span>, emphasizing episodic extreme <span class="hlt">flux</span> events. Extreme <span class="hlt">flux</span> events are responsible for much of the year-to-year variability in mean annual <span class="hlt">flux</span> and are most often observed during early winter and late spring when surface stratification is weak or transient. In addition to biological phenomena (e.g. salp blooms), passage of productive meso-scale features such as eddies, which alter surface water mixing characteristics and surface export <span class="hlt">fluxes</span>, may initiate some extreme <span class="hlt">flux</span> events. Yet other productive eddies show a minimal influence on the deep <span class="hlt">flux</span>, underscoring the importance of upper ocean ecosystem structure and midwater processes on the coupling between the surface ocean environment and deep <span class="hlt">fluxes</span>. Using key organic and inorganic tracers, causative processes that influence deep <span class="hlt">flux</span> generation and the strength of the coupling with the surface ocean environment can be identified.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20020018160','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20020018160"><span>Relationships Between the Bulk-Skin <span class="hlt">Sea</span> Surface Temperature Difference, Wind, and Net <span class="hlt">Air-Sea</span> Heat <span class="hlt">Flux</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Emery, William J.; Castro, Sandra L.; Lindstrom, Eric (Technical Monitor)</p> <p>2002-01-01</p> <p>The primary purpose of this project was to evaluate and improve models for the bulk-skin temperature difference to the point where they could accurately and reliably apply under a wide variety of environmental conditions. To accomplish this goal, work was conducted in three primary areas. These included production of an archive of available data sets containing measurements of the skin and bulk temperatures and associated environmental conditions, evaluation of existing skin layer models using the compiled data archive, and additional theoretical work on the development of an improved model using the data collected under diverse environmental conditions. In this work we set the basis for a new physical model of renewal type, and propose a parameterization for the temperature difference across the cool skin of the ocean in which the effects of thermal buoyancy, wind stress, and microscale breaking are all integrated by means of the appropriate renewal time scales. Ideally, we seek to obtain a model that will accurately apply under a wide variety of environmental conditions. A summary of the work in each of these areas is included in this report. A large amount of work was accomplished under the support of this grant. The grant supported the graduate studies of Sandra Castro and the preparation of her thesis which will be completed later this year. This work led to poster presentations at the 1999 American Geophysical Union Fall Meeting and 2000 IGARSS meeting. Additional work will be presented in a talk at this year's American Meteorological Society <span class="hlt">Air-Sea</span> Interaction Meeting this May. The grant also supported Sandra Castro during a two week experiment aboard the R/P Flip (led by Dr. Andrew Jessup of the Applied Physics Laboratory) to help obtain additional shared data sets and to provide Sandra with a fundamental understanding of the physical processes needed in the models. In a related area, the funding also partially supported Dr. William Emery and Daniel</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JGRD..121.7853K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JGRD..121.7853K"><span>Re-examining the roles of surface heat <span class="hlt">flux</span> and latent heat release in a "hurricane-like" polar low over the Barents <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>Kolstad, Erik W.; Bracegirdle, Thomas J.; Zahn, Matthias</p> <p>2016-07-01</p> <p>Polar lows are intense mesoscale cyclones that occur at high latitudes in both hemispheres during winter. Their sometimes evidently convective nature, fueled by strong surface <span class="hlt">fluxes</span> and with cloud-free centers, have led to some polar lows being referred to as "arctic hurricanes." Idealized studies have shown that intensification by hurricane development mechanisms is theoretically possible in polar winter atmospheres, but the lack of observations and realistic simulations of actual polar lows have made it difficult to ascertain if this occurs in reality. Here the roles of surface heat <span class="hlt">fluxes</span> and latent heat release in the development of a Barents <span class="hlt">Sea</span> polar low, which in its cloud structures showed some similarities to hurricanes, are studied with an ensemble of sensitivity experiments, where latent heating and/or surface <span class="hlt">fluxes</span> of sensible and latent heat were switched off before the polar low peaked in intensity. To ensure that the polar lows in the sensitivity runs did not track too far away from the actual environmental conditions, a technique known as spectral nudging was applied. This was shown to be crucial for enabling comparisons between the different model runs. The results presented here show that (1) no intensification occurred during the mature, postbaroclinic stage of the simulated polar low; (2) surface heat <span class="hlt">fluxes</span>, i.e., <span class="hlt">air-sea</span> interaction, were crucial processes both in order to attain the polar low's peak intensity during the baroclinic stage and to maintain its strength in the mature stage; and (3) latent heat release played a less important role than surface <span class="hlt">fluxes</span> in both stages.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1998JGR...10325125D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1998JGR...10325125D"><span>Comparison of <span class="hlt">sea</span> surface <span class="hlt">flux</span> measured by instrumented aircraft and ship during SOFIA and SEMAPHORE experiments</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Durand, Pierre; Dupuis, HéLèNe; Lambert, Dominique; BéNech, Bruno; Druilhet, Aimé; Katsaros, Kristina; Taylor, Peter K.; Weill, Alain</p> <p>1998-10-01</p> <p>Two major campaigns (Surface of the Oceans, <span class="hlt">Fluxes</span> and Interactions with the Atmosphere (SOFIA) and Structure des Echanges Mer-Atmosphère, Propriétés des Hétérogénéités Océaniques: Recherche Expérimentale (SEMAPHORE)) devoted to the study of ocean-atmosphere interaction were conducted in 1992 and 1993, respectively, in the Azores region. Among the various platforms deployed, instrumented aircraft and ship allowed the measurement of the turbulent <span class="hlt">flux</span> of sensible heat, latent heat, and momentum. From coordinated missions we can evaluate the <span class="hlt">sea</span> surface <span class="hlt">fluxes</span> from (1) bulk relations and mean measurements performed aboard the ship in the atmospheric surface layer and (2) turbulence measurements aboard aircraft, which allowed the <span class="hlt">flux</span> profiles to be estimated through the whole atmospheric boundary layer and therefore to be extrapolated toward the <span class="hlt">sea</span> surface level. Continuous ship <span class="hlt">fluxes</span> were calculated with bulk coefficients deduced from inertial-dissipation measurements in the same experiments, whereas aircraft <span class="hlt">fluxes</span> were calculated with eddy-correlation technique. We present a comparison between these two estimations. Although momentum <span class="hlt">flux</span> agrees quite well, aircraft estimations of sensible and latent heat <span class="hlt">flux</span> are lower than those of the ship. This result is surprising, since aircraft momentum <span class="hlt">flux</span> estimates are often considered as much less accurate than scalar <span class="hlt">flux</span> estimates. The various sources of errors on the aircraft and ship <span class="hlt">flux</span> estimates are discussed. For sensible and latent heat <span class="hlt">flux</span>, random errors on aircraft estimates, as well as variability of ship <span class="hlt">flux</span> estimates, are lower than the discrepancy between the two platforms, whereas the momentum <span class="hlt">flux</span> estimates cannot be considered as significantly different. Furthermore, the consequence of the high-pass filtering of the aircraft signals on the <span class="hlt">flux</span> values is analyzed; it is weak at the lowest altitudes flown and cannot therefore explain the discrepancies between the two platforms but becomes</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26942608','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26942608"><span>Environmental Drivers of Benthic <span class="hlt">Flux</span> Variation and Ecosystem Functioning in Salish <span class="hlt">Sea</span> and Northeast Pacific Sediments.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Belley, Rénald; Snelgrove, Paul V R; Archambault, Philippe; Juniper, S Kim</p> <p>2016-01-01</p> <p>The upwelling of deep waters from the oxygen minimum zone in the Northeast Pacific from the continental slope to the shelf and into the Salish <span class="hlt">Sea</span> during spring and summer offers a unique opportunity to study ecosystem functioning in the form of benthic <span class="hlt">fluxes</span> along natural gradients. Using the ROV ROPOS we collected sediment cores from 10 sites in May and July 2011, and September 2013 to perform shipboard incubations and <span class="hlt">flux</span> measurements. Specifically, we measured benthic <span class="hlt">fluxes</span> of oxygen and nutrients to evaluate potential environmental drivers of benthic <span class="hlt">flux</span> variation and ecosystem functioning along natural gradients of temperature and bottom water dissolved oxygen concentrations. The range of temperature and dissolved oxygen encountered across our study sites allowed us to apply a suite of multivariate analyses rarely used in <span class="hlt">flux</span> studies to identify bottom water temperature as the primary environmental driver of benthic <span class="hlt">flux</span> variation and organic matter remineralization. Redundancy analysis revealed that bottom water characteristics (temperature and dissolved oxygen), quality of organic matter (chl a:phaeo and C:N ratios) and sediment characteristics (mean grain size and porosity) explained 51.5% of benthic <span class="hlt">flux</span> variation. Multivariate analyses identified significant spatial and temporal variation in benthic <span class="hlt">fluxes</span>, demonstrating key differences between the Northeast Pacific and Salish <span class="hlt">Sea</span>. Moreover, Northeast Pacific slope <span class="hlt">fluxes</span> were generally lower than shelf <span class="hlt">fluxes</span>. Spatial and temporal variation in benthic <span class="hlt">fluxes</span> in the Salish <span class="hlt">Sea</span> were driven primarily by differences in temperature and quality of organic matter on the seafloor following phytoplankton blooms. These results demonstrate the utility of multivariate approaches in differentiating among potential drivers of seafloor ecosystem functioning, and indicate that current and future predictive models of organic matter remineralization and ecosystem functioning of soft-muddy shelf and slope seafloor</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMGC24A..04P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMGC24A..04P"><span>Spatial and Temporal Variability of Surface Energy <span class="hlt">Fluxes</span> During Autumn Ice Advance: Observations and Model Validation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Persson, O. P. G.; Blomquist, B.; Grachev, A. A.; Guest, P. S.; Stammerjohn, S. E.; Solomon, A.; Cox, C. J.; Capotondi, A.; Fairall, C. W.; Intrieri, J. M.</p> <p>2016-12-01</p> <p>From Oct 4 to Nov 5, 2015, the Office of Naval Research - sponsored <span class="hlt">Sea</span> State cruise in the Beaufort <span class="hlt">Sea</span> with the new National Science Foundation R/V Sikuliaq obtained extensive in-situ and remote sensing observations of the lower troposphere, the advancing <span class="hlt">sea</span> ice, wave state, and upper ocean conditions. In addition, a coupled atmosphere, <span class="hlt">sea</span> ice, upper-ocean model, based on the RASM model, was run at NOAA/PSD in a hindcast mode for this same time period, providing a 10-day simulation of the atmosphere/ice/ocean evolution. Surface energy <span class="hlt">fluxes</span> quantitatively represent the <span class="hlt">air</span>-ice, <span class="hlt">air</span>-ocean, and ice-ocean interaction processes, determining the cooling (warming) rate of the upper ocean and the growth (melting) rate of <span class="hlt">sea</span> ice. These <span class="hlt">fluxes</span> also impact the stratification of the lower troposphere and the upper ocean. In this presentation, both direct and indirect measurements of the energy <span class="hlt">fluxes</span> during <span class="hlt">Sea</span> State will be used to explore the spatial and temporal variability of these <span class="hlt">fluxes</span> and the impacts of this variability on the upper ocean, ice, and lower atmosphere during the autumn ice advance. Analyses have suggested that these <span class="hlt">fluxes</span> are impacted by atmospheric synoptic evolution, proximity to existing ice, ice-relative wind direction, ice thickness and snow depth. In turn, these <span class="hlt">fluxes</span> impact upper-ocean heat loss and timing of ice formation, as well as stability in the lower troposphere and upper ocean, and hence heat transport to the free troposphere and ocean mixed-layer. Therefore, the atmospheric structure over the advancing first-year ice differs from that over the nearby open water. Finally, these observational analyses will be used to provide a preliminary validation of the spatial and temporal variability of the surface energy <span class="hlt">fluxes</span> and the associated lower-tropospheric and upper-ocean structures in the simulations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.8178B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.8178B"><span>Measured and parameterized energy <span class="hlt">fluxes</span> estimated for Atlantic transects of RV Polarstern</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bumke, Karl; Macke, Andreas; Kalisch, John; Kleta, Henry</p> <p>2013-04-01</p> <p>Even to date energy <span class="hlt">fluxes</span> over the oceans are difficult to assess. As an example the relative paucity of evaporation observations and the uncertainties of currently employed empirical approaches lead to large uncertainties of evaporation products over the ocean (e.g. Large and Yeager, 2009). Within the frame of OCEANET (Macke et al., 2010) we performed such measurements on Atlantic transects between Bremerhaven (Germany) and Cape Town (South Africa) or Punta Arenas (Chile) onboard RV Polarstern during the recent years. The basic measurements of sensible and latent heat <span class="hlt">fluxes</span> are inertial-dissipation (e.g. Dupuis et al., 1997) <span class="hlt">flux</span> estimates and measurements of the bulk variables. Turbulence measurements included a sonic anemometer and an infrared hygrometer, both mounted on the crow's nest. Mean meteorological sensors were those of the ship's operational measurement system. The global radiation and the down terrestrial radiation were measured on the OCEANET container placed on the monkey island. At least about 1000 time series of 1 h length were analyzed to derive bulk transfer coefficients for the <span class="hlt">fluxes</span> of sensible and latent heat. The bulk transfer coefficients were applied to the ship's meteorological data to derive the heat <span class="hlt">fluxes</span> at the <span class="hlt">sea</span> surface. The reflected solar radiation was estimated from measured global radiation. The up terrestrial radiation was derived from the skin temperature according to the Stefan-Boltzmann law. Parameterized heat <span class="hlt">fluxes</span> were compared to the widely used COARE-parameterization (Fairall et al., 2003), the agreement is excellent. Measured and parameterized heat and radiation <span class="hlt">fluxes</span> gave the total energy budget at the <span class="hlt">air</span> <span class="hlt">sea</span> interface. As expected the mean total <span class="hlt">flux</span> is positive, but there are also areas, where it is negative, indicating an energy loss of the ocean. It could be shown that the variations in the energy budget are mainly due to insolation and evaporation. A comparison between the mean values of measured 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_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_11 --> <div id="page_12" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="221"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/351688-sensing-flux-volatile-chemicals-through-air-water-interface','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/351688-sensing-flux-volatile-chemicals-through-air-water-interface"><span>Sensing the <span class="hlt">flux</span> of volatile chemicals through the <span class="hlt">air</span>-water interface</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>Mackay, D.; Schroeder, W.H.; Ooijen, H. von</p> <p>1997-12-31</p> <p>There are several situations in which there is a need to assess the direction and magnitude of the <span class="hlt">flux</span> across the <span class="hlt">air</span>-water interface. Contaminants may be evaporating or absorbing in wastewater treatment systems in natural lake, river, estuarine and marine systems, and any attempt to compile a mass balance must include this process. In this study the authors review the theory underlying <span class="hlt">air</span>-water exchange, then describe and discuss a sparging approach by which the direction and magnitude of the <span class="hlt">flux</span> can be ascertained. The principle of the method is that a known flow rate of <span class="hlt">air</span> is bubbled through themore » sparger and allowed to equilibrate with the water. The gas exiting the water surface is passed through a sorbent trap and later analyzed. The concentration, and hence the fugacity, of the contaminant in the sparged <span class="hlt">air</span> can be deduced. In parallel, a similar flow of <span class="hlt">air</span> from the atmosphere above the water is drawn through another sparger at a similar flow rate for a similar time and the trapped chemical analyzed giving the concentration and fugacity in the <span class="hlt">air</span>. These data show the direction of <span class="hlt">air</span>-water exchange (i.e. from high to low fugacity) and with information on the mass transfer coefficients and area, the <span class="hlt">flux</span>. Successful tests were conducted of the system in a laboratory tank, in Lake Ontario and in Hamilton Harbour. Analyses of the traps showed a large number of peaks on the chromatogram many of which are believed to be of petroleum origin from fuels and vessel exhaust. The system will perform best under conditions where concentrations of specific contaminants are large, as occurs in waste water treatment systems. The approach has the potential to contribute to more accurate assessment of <span class="hlt">air</span>-water <span class="hlt">fluxes</span>. It avoids the problems of different analytical methodologies and the effect of sorption in the water column.« less</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 pCO2 Variations and <span class="hlt">Sea-Air</span> CO2 <span class="hlt">Fluxes</span> During Summer in the Eastern Canadian Arctic</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Burgers, T. M.; Miller, L. A.; Thomas, H.; Else, B. G. T.; Gosselin, M.; Papakyriakou, T.</p> <p>2017-12-01</p> <p>Based on a 2 year data set, the eastern Canadian Arctic Archipelago and Baffin Bay appear to be a modest summertime sink of atmospheric CO2. We measured surface water CO2 partial pressure (pCO2), 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 pCO2 displayed considerable variability (144-364 μatm) but never exceeded atmospheric concentrations, and average calculated CO2 <span class="hlt">fluxes</span> in 2013 and 2014 were -12 and -3 mmol C m-2 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 pCO2, whereas areas of <span class="hlt">sea</span>-ice melt occur with low surface pCO2. Further assessments, extending the seasonal observation period, are needed to properly constrain both seasonal and annual CO2 <span class="hlt">fluxes</span> in this region.</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('http://adsabs.harvard.edu/abs/2017AGUFM.A43G2558W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A43G2558W"><span><span class="hlt">Air-sea</span> exchange and gas-particle partitioning of polycyclic aromatic hydrocarbons over the northwestern Pacific Ocean: Role of East Asian continental outflow</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wu, Z.; Guo, Z.</p> <p>2017-12-01</p> <p>We measured 15 parent polycyclic aromatic hydrocarbons (PAHs) in atmosphere and water during a research cruise from the East China <span class="hlt">Sea</span> (ECS) to the northwestern Pacific Ocean (NWP) in the spring of 2015 to investigate the occurrence, <span class="hlt">air-sea</span> gas exchange, and gas-particle partitioning of PAHs with a particular focus on the influence of East Asian continental outflow. The gaseous PAH composition and identification of sources were consistent with PAHs from the upwind area, indicating that the gaseous PAHs (three- to five-ring PAHs) were influenced by upwind land pollution. In addition, <span class="hlt">air-sea</span> exchange <span class="hlt">fluxes</span> of gaseous PAHs were estimated to be -54.2 to 107.4 ng m-2 d-1, and was indicative of variations of land-based PAH inputs. The logarithmic gas-particle partition coefficient (logKp) of PAHs regressed linearly against the logarithmic subcooled liquid vapor pressure, with a slope of -0.25. This was significantly larger than the theoretical value (-1), implying disequilibrium between the gaseous and particulate PAHs over the NWP. The non-equilibrium of PAH gas-particle partitioning was shielded from the volatilization of three-ring gaseous PAHs from seawater and lower soot concentrations in particular when the oceanic <span class="hlt">air</span> masses prevailed. Modeling PAH absorption into organic matter and adsorption onto soot carbon revealed that the status of PAH gas-particle partitioning deviated more from the modeling Kp for oceanic <span class="hlt">air</span> masses than those for continental <span class="hlt">air</span> masses, which coincided with higher volatilization of three-ring PAHs and confirmed the influence of <span class="hlt">air-sea</span> exchange. Meanwhile, significant linear regressions between logKp and logKoa (logKsa) for PAHs were observed for continental <span class="hlt">air</span> masses, suggesting the dominant effect of East Asian continental outflow on atmospheric PAHs over the NWP during the sampling campaign.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29300684','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29300684"><span><span class="hlt">Flux</span> and distribution of methane (CH4) in the Gunsan Basin of the southeastern Yellow <span class="hlt">Sea</span>, off the Western Korea.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lee, Jun-Ho; Woo, Han Jun; Son, Seung-Kyu; Kim, Moonkoo; Lee, Dong-Hun; Tsunogai, Urumu; Jeong, Kap-Sik</p> <p>2018-04-16</p> <p>The <span class="hlt">flux</span> and distribution of methane (CH 4 ) was investigated in the seawater column at 14 stations in the Gunsan Basin, the southeastern part of Yellow <span class="hlt">Sea</span> from 2013 to 2015. Here CH 4 is concentrated 2.4-4.7 (3.4 ± 0.7) nM in the surface and 2.5-7.4 (5.2 ± 1.7) nM in the bottom layer. The CH 4 saturation ratios ranged from 65.5% to 295.5% (162.6 ± 68.7), comprising the mean <span class="hlt">sea-to-air</span> CH 4 <span class="hlt">flux</span> of 3.8 to 25.3 (15.6 ± 5.5) µM m -2 d -1 . Methane concentration was largely different in the upper and the lower seawater layers that is separated by the thermocline of which depth is variable (20-60 m) depending on the time of sampling. The concentration of seawater dissolved CH 4 is high between the bottom surface of the thermocline layer and the <span class="hlt">sea</span> floor. Generally it tends to decrease from the south-westernmost part of the basin toward the west coast of Korea. This distribution pattern of CH 4 seems to result from the CH 4 supply by decomposition of organic matters produced in the upper seawater layer that is superimposed by the larger supply from the underlying sediment layer especially beneath the thermocline. The latter is manifested by ubiquitous CH 4 seeps from the seafloor sediments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A51E2110S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A51E2110S"><span>Relating Radiative <span class="hlt">Fluxes</span> on Arctic <span class="hlt">Sea</span> Ice Area Using Arctic Observation and Reanalysis Integrated System (ArORIS)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sledd, A.; L'Ecuyer, T. S.</p> <p>2017-12-01</p> <p>With Arctic <span class="hlt">sea</span> ice declining rapidly and Arctic temperatures rising faster than the rest of the globe, a better understanding of the Arctic climate, and ice cover-radiation feedbacks in particular, is needed. Here we present the Arctic Observation and Reanalysis Integrated System (ArORIS), a dataset of integrated products to facilitate studying the Arctic using satellite, reanalysis, and in-situ datasets. The data include cloud properties, radiative <span class="hlt">fluxes</span>, aerosols, meteorology, precipitation, and surface properties, to name just a few. Each dataset has uniform grid-spacing, time-averaging and naming conventions for ease of use between products. One intended use of ArORIS is to assess Arctic radiation and moisture budgets. Following that goal, we use observations from ArORIS - CERES-EBAF radiative <span class="hlt">fluxes</span> and NSIDC <span class="hlt">sea</span> ice fraction and area to quantify relationships between the Arctic energy balance and surface properties. We find a discernable difference between energy budgets for years with high and low September <span class="hlt">sea</span> ice areas. Surface <span class="hlt">fluxes</span> are especially responsive to the September <span class="hlt">sea</span> ice minimum in months both leading up to September and the months following. In particular, longwave <span class="hlt">fluxes</span> at the surface show increased sensitivity in the months preceding September. Using a single-layer model of solar radiation we also investigate the individual responses of surface and planetary albedos to changes in <span class="hlt">sea</span> ice area. By partitioning the planetary albedo into surface and atmospheric contributions, we find that the atmospheric contribution to planetary albedo is less sensitive to changes in <span class="hlt">sea</span> ice area than the surface contribution. Further comparisons between observations and reanalyses can be made using the available datasets in ArORIS.</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('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 transferring the water sample into laboratory conditions. The results show an enhancement of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A54D..06M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A54D..06M"><span>The Impact of Cloud Properties on Young <span class="hlt">Sea</span> Ice during Three Winter Storms at N-ICE2015</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Murphy, S. Y.; Walden, V. P.; Cohen, L.; Hudson, S. R.</p> <p>2017-12-01</p> <p>The impact of clouds on <span class="hlt">sea</span> ice varies significantly as cloud properties change. Instruments deployed during the Norwegian Young <span class="hlt">Sea</span> Ice field campaign (N-ICE2015) are used to study how differing cloud properties influence the cloud radiative forcing at the <span class="hlt">sea</span> ice surface. N-ICE2015 was the first campaign in the Arctic winter since SHEBA (1997/1998) to study the surface energy budget of <span class="hlt">sea</span> ice and the associated effects of cloud properties. Cloud characteristics, surface radiative and turbulent <span class="hlt">fluxes</span>, and meteorological properties were measured throughout the field campaign. Here we explore how cloud macrophysical and microphysical properties affect young, thin <span class="hlt">sea</span> ice during three winter storms from 31 January to 15 February 2015. This time period is of interest due to the varying surface and atmospheric conditions, which showcase the variety of conditions the newly-formed <span class="hlt">sea</span> ice can experience during the winter. This period was characterized by large variations in the ice surface and near-surface <span class="hlt">air</span> temperatures, with highs near 0°C when warm, moist <span class="hlt">air</span> was advected into the area and lows reaching -40°C during clear, calm periods between storms. The advection of warm, moist <span class="hlt">air</span> into the area influenced the cloud properties and enhanced the downwelling longwave <span class="hlt">flux</span>. For most of the period, downwelling longwave <span class="hlt">flux</span> correlates closely with the <span class="hlt">air</span> temperature. However, at the end of the first storm, a drop in downwelling longwave <span class="hlt">flux</span> of about 50 Wm-2 was observed, independent of any change in surface or <span class="hlt">air</span> temperature or cloud fraction, indicating a change in cloud properties. Lidar data show an increase in cloud height during this period and a potential shift in cloud phase from ice to mixed-phase. This study will describe the cloud properties during the three winter storms and discuss their impacts on surface energy budget.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120012563','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120012563"><span>Moisture <span class="hlt">Fluxes</span> Derived from EOS Aqua Satellite Data for the North Water Polynya Over 2003-2009</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Boisvert, Linette N.; Markus, Thorsten; Parkinson, Claire L.; Vihma, Timo</p> <p>2012-01-01</p> <p>Satellite data were applied to calculate the moisture <span class="hlt">flux</span> from the North Water polynya during a series of events spanning 2003-2009. The <span class="hlt">fluxes</span> were calculated using bulk aerodynamic formulas with the stability effects according to the Monin-Obukhov similarity theory. Input parameters were taken from three sources: <span class="hlt">air</span> relative humidity, <span class="hlt">air</span> temperature, and surface temperature from the Atmospheric Infrared Sounder (<span class="hlt">AIRS</span>) onboard NASA's Earth Observing System (EOS) Aqua satellite, <span class="hlt">sea</span> ice concentration from the Advanced Microwave Scanning Radiometer (AMSR-E, also onboard Aqua), and wind speed from the ECMWF ERA-Interim reanalysis. Our results show the progression of the moisture <span class="hlt">fluxes</span> from the polynya during each event, as well as their atmospheric effects after the polynya has closed up. These results were compared to results from studies on other polynyas, and fall within one standard deviation of the moisture <span class="hlt">flux</span> estimates from these studies. Although the estimated moisture <span class="hlt">fluxes</span> over the entire study region from <span class="hlt">AIRS</span> are smaller in magnitude than ERA-Interim, they are more accurate due to improved temperature and relative humidity profiles and ice concentration estimates over the polynya. Error estimates were calculated to be 5.56 x10(exp -3) g/sq. m/ s, only 25% of the total moisture <span class="hlt">flux</span>, thus suggesting that <span class="hlt">AIRS</span> and AMSR-E can be used with confidence to study smaller scale features in the Arctic <span class="hlt">sea</span> ice pack and can capture their atmospheric effects. These findings bode well for larger-scale studies of moisture <span class="hlt">fluxes</span> over the entire Arctic Ocean and the thinning ice pack.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/467708-measurements-co-sub-fluxes-bubbles-from-tower-during-asgasex','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/467708-measurements-co-sub-fluxes-bubbles-from-tower-during-asgasex"><span>Measurements of CO{sub 2} <span class="hlt">fluxes</span> and bubbles from a tower during ASGASEX</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Leeuw, G. de; Kunz, G.J.; Larsen, S.E.</p> <p>1994-12-31</p> <p>The <span class="hlt">Air-Sea</span> Gas Exchange experiment ASGASEX was conducted from August 30 until October 1st from the Meetpost Noordwijk (MPN), a research tower in the North <span class="hlt">Sea</span> at 9 km from the Dutch coast. The objective of ASGASEX was a study of parameters affecting the <span class="hlt">air-sea</span> exchange of gases, and a comparison of experimental methods to derive the exchange coefficient for CO{sub 2}. A detailed description of the ASGASEX experiment is presented in Oost. The authors` contribution to ASGASEX was a micro-meteorological package to measure the <span class="hlt">fluxes</span> of CO{sub 2}, 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 CO{sub 2} <span class="hlt">flux</span> measurements and the bubble measurements. The latter was made as part of a larger study on the influence of bubbles on gas exchange in cooperation with the University of Southampton and the University of Galway.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002EGSGA..27.5673F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002EGSGA..27.5673F"><span><span class="hlt">Air-sea</span> Forcing and Thermohaline Changes In The 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>Fusco, G.; Budillon, G.</p> <p></p> <p>Heat exchanges between <span class="hlt">sea</span> and atmosphere from 1986 to 2000 in the Ross <span class="hlt">Sea</span> (Antarctica) were computed from climatological data obtained from the European Centre for Medium Range Weather Forecasts. They have been related with the thermo- haline changes observed during 5 hydrological surveys performed between the austral summer 1994-1995 and 2000-2001 in the western sector of the Ross <span class="hlt">Sea</span>. The esti- mated heat <span class="hlt">fluxes</span> show extremely strong spatial and temporal variability over all the Ross <span class="hlt">Sea</span>. As can be expected the largest heat losses occur between May and August, while during the period November-February the heat budget becomes positive. In the first six years of the investigated period the heat loss is very strong with its maximum about 166 Wm-2; while during the period 1992-2000 the yearly heat losses are the lowest. Thermohaline changes in the surface layer (upper pycnocline) of the western Ross <span class="hlt">Sea</span> follow the expected seasonal pattern of warming and freshening from the be- ginning to the end of the austral summer. The heating changes are substantially lower than the estimated heat supplied by the atmosphere during the summer, which under- lines the importance in this season of the advective component carried by the currents in the total heat budget of this area. The year to year differences are about one or two orders of magnitude smaller than the seasonal changes in the surface layer. In the in- termediate and deep layers, the summer heat and salt variability is of the same order as or one order higher than from one summer to the next. Moreover a freshening of the near bottom layer has been observed, it is consistent with the High Salinity Shelf Water salinity decrease recently detected in the Ross <span class="hlt">Sea</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JAMES...9.1641P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JAMES...9.1641P"><span>Modeling the <span class="hlt">air-sea</span> feedback system of Madeira Island</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pullen, Julie; Caldeira, Rui; Doyle, James D.; May, Paul; Tomé, Ricardo</p> <p>2017-07-01</p> <p>A realistic nested data-assimilating two-way coupled ocean/atmosphere modeling study (highest resolution 2 km) of Madeira Island was conducted for June 2011, when conditions were favorable for atmospheric vortex shedding. The simulation's island lee region exhibited relatively cloud-free conditions, promoting warmer ocean temperatures (˜2°C higher than adjacent waters). The model reasonably reproduced measured fields at 14 meteorological stations, and matched the dimensions and magnitude of the warm <span class="hlt">sea</span> surface temperature (SST) wake imaged by satellite. The warm SSTs in the wake are shown to imprint onto the atmospheric boundary layer (ABL) over several diurnal cycles by modulating the ABL depth up to ˜200-500 m. The erosion and dissipation of the warm ocean wake overnight was aided by atmospheric drainage flow and offshore advection of cold <span class="hlt">air</span> (ΔT = 2°C) that produced strong upward heat <span class="hlt">fluxes</span> (˜50 W/m2 sensible and ˜250 W/m2 latent) on an episodic basis. Nevertheless, the warm wake was never entirely eroded at night due to the cumulative effect of the diurnal cycle. The spatial pattern of the diurnal warming varied day-to-day in location and extent. Significant mutual interaction of the oceanic and atmospheric boundary layers was diagnosed via <span class="hlt">fluxes</span> and temperature cross sections and reinforced by sensitivity runs. The simulation produces for the first time the interactive nature of the ocean and atmosphere boundary layers in the warm wake region of an island with complex terrain.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRD..122.2115B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRD..122.2115B"><span>The marine atmospheric boundary layer under strong wind conditions: Organized turbulence structure and <span class="hlt">flux</span> estimates by airborne measurements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brilouet, Pierre-Etienne; Durand, Pierre; Canut, Guylaine</p> <p>2017-02-01</p> <p>During winter, cold <span class="hlt">air</span> outbreaks take place in the northwestern Mediterranean <span class="hlt">sea</span>. They are characterized by local strong winds (Mistral and Tramontane) which transport cold and dry continental <span class="hlt">air</span> across a warmer <span class="hlt">sea</span>. In such conditions, high values of surface sensible and latent heat <span class="hlt">flux</span> are observed, which favor deep oceanic convection. The HyMeX/ASICS-MED field campaign was devoted to the study of these processes. Airborne measurements, gathered in the Gulf of Lion during the winter of 2013, allowed for the exploration of the mean and turbulent structure of the marine atmospheric boundary layer (MABL). A spectral analysis based on an analytical model was conducted on 181 straight and level runs. Profiles of characteristic length scales and sharpness parameter of the vertical wind spectrum revealed larger eddies along the mean wind direction associated with an organization of the turbulence field into longitudinal rolls. These were highlighted by boundary layer cloud bands on high-resolution satellite images. A one-dimensional description of the vertical exchanges is then a tricky issue. Since the knowledge of the <span class="hlt">flux</span> profile throughout the entire MABL is essential for the estimation of <span class="hlt">air-sea</span> exchanges, a correction of eddy covariance turbulent <span class="hlt">fluxes</span> was developed taking into account the systematic and random errors due to sampling and data processing. This allowed the improvement of surface <span class="hlt">fluxes</span> estimates, computed from the extrapolation of the stacked levels. A comparison between those surface <span class="hlt">fluxes</span> and bulk <span class="hlt">fluxes</span> computed at a moored buoy revealed considerable differences, mainly regarding the latent heat <span class="hlt">flux</span> under strong wind conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFMPP23C1436J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFMPP23C1436J"><span>Response of carbon <span class="hlt">fluxes</span> and climate to orbital forcing changes in the Community Climate System Model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jochum, M.; Peacock, S.; Moore, J. K.; Lindsay, K. T.</p> <p>2009-12-01</p> <p>A global general circulation model coupled to an ocean ecosystem model is used to quantify the response of carbon <span class="hlt">fluxes</span> and climate to changes in orbital forcing. Compared to the present-day simulation, the simulation with the Earth's orbital parameters from 115,000 years ago features significantly cooler northern high latitudes, but only moderately cooler southern high latitudes. This asymmetry is explained by a 30% reduction of the strength of the Atlantic Meridional Overturning Circulation that is caused by an increased Arctic <span class="hlt">sea</span>-ice export and a resulting freshening of the North Atlantic. The strong northern high-latitude cooling and the direct insolation induced tropical warming lead to global shifts in precipitation and winds to the order of 10-20%. These climate shifts lead to regional differences in <span class="hlt">air-sea</span> carbon <span class="hlt">fluxes</span> of the same order. However, the differences in global net carbon <span class="hlt">fluxes</span> are insignificant. This surprising result is due to several effects, two of which stand out: Firstly, colder <span class="hlt">sea</span> surface temperature leads to a more effective solubility pump but also to increased <span class="hlt">sea</span>-ice concentration which blocks <span class="hlt">air-sea</span> exchange; and secondly, the weakening of Southern Ocean winds, which is predicted by some idealized studies, is small compared to its interannual variability.</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('https://www.osti.gov/biblio/6029574-air-sea-fluxes-lipids-enewetak-atoll','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6029574-air-sea-fluxes-lipids-enewetak-atoll"><span><span class="hlt">Air-to-sea</span> <span class="hlt">fluxes</span> of lipids at enewetak atoll</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>Zafiriou, O.C.; Gagosian, R.B.; Peltzer, E.T.</p> <p>1985-02-20</p> <p>We report data for the Enewetak site of the SEAREX program from the rainy season in 1979. The concentrations of n-alkanes, n-alkanols, sterols, n-alkanoic acids and their salts, and total organic compounds in rain are reported, as well as the apparent gaseous hydrocarbon concentrations. These data and information on the particulate forms are analyzed in conjunction with ancillary chemical and meterological data to draw inferences about sources, <span class="hlt">fluxes</span>, and chemical speciations. While the higher molecular weight lipid biomarker components are exclusively terrestrial, the organic carbon in rain may be derived from atmospheric transformations of terrestrial carbon. Distinctively marine components aremore » nearly absent. Comparison of the scavenging ratios of the organic components in rain vs. those for clays reveals that the alkanoic acids and the higher molecular weight alkanols behave as essentially particulate materials, whereas lower alkanols and most hydrocarbons show much higher scavenging ratios, probably due to the involvement of a gaseous phase or sampling artifact. Vaporization in the atmosphere and scaveging of a gas phase would lead to higher scaveging ratios; vaporization during sampling would give low aerosol concentrations and high gas-phase concentrations, leading to high scavening ratios. The major <span class="hlt">fluxes</span> at Enewetak result from rain rather than dry deposition, and extrapolating the measured values to meaningful annual averages requires adjustment for seasonally varying source intensity and rain dynamics. Aerosol data for other seasons and other substances are used to correct for source-strength intensity variations, and a /sup 210/Pb/organic compound correlation is established and extrapolated to adjust for rainfall volume effects.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA524620','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA524620"><span><span class="hlt">Air-Sea</span> Enthalpy and Momentum Exchange at Major Hurricane Wind Speeds</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2010-06-01</p> <p>momentum <span class="hlt">fluxes</span>. Hurricane simulations using the Navy Coupled Ocean / Atmosphere Mesoscale Prediction System are also sensitive to the surface <span class="hlt">flux</span> and <span class="hlt">sea</span>... Atmospheric Research NWP Numerical Weather Prediction NOAA National Oceanic and Atmospheric Administration PTH Pressure, Temperature, relative Humidity RE87... Oceanic and Atmospheric Administration for organizing the CBLAST field program and collecting the data used for this study. xx THIS PAGE</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS54B..01D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS54B..01D"><span>Carbon Cycle in South China <span class="hlt">Sea</span>: <span class="hlt">Flux</span>, Controls and Global Implications</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dai, M.; Cao, Z.; Yang, W.; Guo, X.; Yin, Z.; Gan, J.</p> <p>2016-12-01</p> <p>The contemporary coastal ocean is generally seen as a significant CO2 sink of 0.2-0.4 Pg C/yr at the global scale. However, mechanistic understanding of the coastal ocean carbon cycle remains limited, leading to the unanswered question of why some coastal systems are sources while others are sinks of atmospheric CO2. As the largest marginal <span class="hlt">sea</span> of Northern Pacific, the South China <span class="hlt">Sea</span> (SCS) is a mini-ocean with wide shelves in both its southern and northern parts. Its northern shelf, which receives significant land inputs from the Pearl River, a world major river, can be categorized as a River-Dominated Margin (RioMar) during peak discharges, and is characterized as a CO2 sink to the atmosphere. The SCS basin is identified as an Ocean-Dominated Margin (OceMar) and a CO2 source. OceMar is characterized by exchange with the open ocean via a two-dimensional (at least) process, i.e., the horizontal intrusion of open ocean water and subsequent vertical mixing and upwelling. Depending on the different ratios of dissolved inorganic carbon (DIC) and nutrients from the source waters into the continental margins, the relative consumption or removal bwtween DIC and nutrients, when being transported into the euphotic zones where biogeochemical processes take over, determines the CO2 <span class="hlt">fluxes</span>. Thus, excess DIC relative to nutrients existing in the upper layer will lead to CO2 degassing. The CO2 <span class="hlt">fluxes</span> in both RioMars and OceMars can be quantified using a semi-analytical diagnostic approach by coupling the physical dynamics and biogeochemical processes. We extended our mechanistic studies in the SCS to other OceMars including the Caribbean <span class="hlt">Sea</span>, the Arabian <span class="hlt">Sea</span>, and the upwelling system off the Oregon-California coast, and RioMars including the East China <span class="hlt">Sea</span> and Amazon River plume to demonstrate the global implications of our SCS carbon studies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/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> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_12 --> <div id="page_13" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="241"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016BGeo...13.6385T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016BGeo...13.6385T"><span>Stable carbon isotope gradients in benthic foraminifera as proxy for organic carbon <span class="hlt">fluxes</span> 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>Theodor, Marc; Schmiedl, Gerhard; Jorissen, Frans; Mackensen, Andreas</p> <p>2016-11-01</p> <p>We have determined stable carbon isotope ratios of epifaunal and shallow infaunal benthic foraminifera in the Mediterranean <span class="hlt">Sea</span> to relate the inferred gradient of pore water δ13CDIC to varying trophic conditions. This is a prerequisite for developing this difference into a potential transfer function for organic matter <span class="hlt">flux</span> rates. The data set is based on samples retrieved from a well-defined bathymetric range (400-1500 m water depth) of sub-basins in the western, central, and eastern Mediterranean <span class="hlt">Sea</span>. Regional contrasts in organic matter <span class="hlt">fluxes</span> and associated δ13CDIC of pore water are recorded by the δ13C difference (Δδ13CUmed-Epi) between the shallow infaunal Uvigerina mediterranea and epifaunal species (Planulina ariminensis, Cibicidoides pachydermus, Cibicides lobatulus). Within epifaunal taxa, the highest δ13C values are recorded for P. ariminensis, providing the best indicator for bottom water δ13CDIC. In contrast, C. pachydermus reveals minor pore water effects at the more eutrophic sites. Because of ontogenetic trends in the δ13C signal of U. mediterranea of up to 1.04 ‰, only tests larger than 600 µm were used for the development of the transfer function. The recorded differences in the δ13C values of U. mediterranea and epifaunal taxa (Δδ13CUmed-Epi) range from -0.46 to -2.13 ‰, with generally higher offsets at more eutrophic sites. The measured δ13C differences are related to site-specific differences in microhabitat, depth of the principal sedimentary redox boundary, and TOC content of the ambient sediment. The Δδ13CUmed-Epi values reveal a consistent relation to Corg <span class="hlt">fluxes</span> estimated from satellite-derived surface water primary production in open-marine settings of the Alboran <span class="hlt">Sea</span>, Mallorca Channel, Strait of Sicily, and southern Aegean <span class="hlt">Sea</span>. In contrast, Δδ13CUmed-Epi values in areas affected by intense resuspension and riverine organic matter sources of the northern to central Aegean <span class="hlt">Sea</span> and the canyon systems of the Gulf of Lion</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ClDy...49.2491L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ClDy...49.2491L"><span><span class="hlt">Air-sea</span> heat <span class="hlt">fluxes</span> associated to mesoscale eddies in the Southwestern Atlantic Ocean and their dependence on different regional conditions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Leyba, Inés M.; Saraceno, Martín; Solman, Silvina A.</p> <p>2017-10-01</p> <p>Heat <span class="hlt">fluxes</span> between the ocean and the atmosphere largely represent the link between the two media. A possible mechanism of interaction is generated by mesoscale ocean eddies. In this work we evaluate if eddies in Southwestern Atlantic (SWA) Ocean may significantly affect flows between the ocean and the atmosphere. Atmospherics conditions associated with eddies were examined using data of <span class="hlt">sea</span> surface temperature (SST), sensible (SHF) and latent heat <span class="hlt">flux</span> (LHF) from NCEP-CFSR reanalysis. On average, we found that NCEP-CFSR reanalysis adequately reflects the variability expected from eddies in the SWA, considering the classical eddy-pumping theory: anticyclonic (cyclonic) eddies cause maximum positive (negative) anomalies with maximum mean anomalies of 0.5 °C (-0.5 °C) in SST, 6 W/m2 (-4 W/m2) in SHF and 12 W/m2 (-9 W/m2) in LHF. However, a regional dependence of heat <span class="hlt">fluxes</span> associated to mesoscale cyclonic eddies was found: in the turbulent Brazil-Malvinas Confluence (BMC) region they are related with positive heat <span class="hlt">flux</span> anomaly (ocean heat loss), while in the rest of the SWA they behave as expected (ocean heat gain). We argue that eddy-pumping do not cool enough the center of the cyclonic eddies in the BMC region simply because most of them trapped very warm waters when they originate in the subtropics. The article therefore concludes that in the SWA: (1) a robust link exists between the SST anomalies generated by eddies and the local anomalous heat flow between the ocean and the atmosphere; (2) in the BMC region cyclonic eddies are related with positive heat anomalies, contrary to what is expected.</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 2) 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.osti.gov/servlets/purl/872981','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/872981"><span>Direct control of <span class="hlt">air</span> gap <span class="hlt">flux</span> in permanent magnet machines</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Hsu, John S.</p> <p>2000-01-01</p> <p>A method and apparatus for field weakening in PM machines uses field weakening coils (35, 44, 45, 71, 72) to produce <span class="hlt">flux</span> in one or more stators (34, 49, 63, 64), including a <span class="hlt">flux</span> which counters <span class="hlt">flux</span> normally produced in <span class="hlt">air</span> gaps between the stator(s) (34, 49, 63, 64) and the rotor (20, 21, 41, 61) which carries the PM poles. Several modes of operation are introduced depending on the magnitude and polarity of current in the field weakening coils (35, 44, 45, 71, 72). The invention is particularly useful for, but not limited to, the electric vehicle drives and PM generators.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A43D2472C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A43D2472C"><span>Sensitivity of the <span class="hlt">sea</span> ice concentration over the Kara-Barents <span class="hlt">Sea</span> in autumn to the winter temperature variability over East Asia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cho, K. H.; Chang, E. C.</p> <p>2017-12-01</p> <p>In this study, we performed sensitivity experiments by utilizing the Global/Regional Integrated Model system with different conditions of the <span class="hlt">sea</span> ice concentration over the Kara-Barents (KB) <span class="hlt">Sea</span> in autumn, which can affect winter temperature variability over East Asia. Prescribed <span class="hlt">sea</span> ice conditions are 1) climatological autumn <span class="hlt">sea</span> ice concentration obtained from 1982 to 2016, 2) reduced autumn <span class="hlt">sea</span> ice concentration by 50% of the climatology, and 3) increased autumn <span class="hlt">sea</span> ice concentration by 50% of climatology. Differently prescribed <span class="hlt">sea</span> ice concentration changes surface albedo, which affects surface heat <span class="hlt">fluxes</span> and near-surface <span class="hlt">air</span> temperature. The reduced (increased) <span class="hlt">sea</span> ice concentration over the KB <span class="hlt">sea</span> increases (decreases) near-surface <span class="hlt">air</span> temperature that leads the lower (higher) <span class="hlt">sea</span> level pressure in autumn. These patterns are maintained from autumn to winter season. Furthermore, it is shown that the different <span class="hlt">sea</span> ice concentration over the KB <span class="hlt">sea</span> has remote effects on the <span class="hlt">sea</span> level pressure patterns over the East Asian region. The lower (higher) <span class="hlt">sea</span> level pressure over the KB <span class="hlt">sea</span> by the locally decreased (increased) ice concentration is related to the higher (lower) pressure pattern over the Siberian region, which induces strengthened (weakened) cold advection over the East Asian region. From these sensitivity experiments it is clarified that the decreased (increased) <span class="hlt">sea</span> ice concentration over the KB <span class="hlt">sea</span> in autumn can lead the colder (warmer) surface <span class="hlt">air</span> temperature over East Asia in winter.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28675854','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28675854"><span><span class="hlt">Air-sea</span> exchange and gas-particle partitioning of polycyclic aromatic hydrocarbons over the northwestern Pacific Ocean: Role of East Asian continental outflow.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wu, Zilan; Lin, Tian; Li, Zhongxia; Jiang, Yuqing; Li, Yuanyuan; Yao, Xiaohong; Gao, Huiwang; Guo, Zhigang</p> <p>2017-11-01</p> <p>We measured 15 parent polycyclic aromatic hydrocarbons (PAHs) in atmosphere and water during a research cruise from the East China <span class="hlt">Sea</span> (ECS) to the northwestern Pacific Ocean (NWP) in the spring of 2015 to investigate the occurrence, <span class="hlt">air-sea</span> gas exchange, and gas-particle partitioning of PAHs with a particular focus on the influence of East Asian continental outflow. The gaseous PAH composition and identification of sources were consistent with PAHs from the upwind area, indicating that the gaseous PAHs (three-to five-ring PAHs) were influenced by upwind land pollution. In addition, <span class="hlt">air-sea</span> exchange <span class="hlt">fluxes</span> of gaseous PAHs were estimated to be -54.2-107.4 ng m -2 d -1 , and was indicative of variations of land-based PAH inputs. The logarithmic gas-particle partition coefficient (logK p ) of PAHs regressed linearly against the logarithmic subcooled liquid vapor pressure (logP L 0 ), with a slope of -0.25. This was significantly larger than the theoretical value (-1), implying disequilibrium between the gaseous and particulate PAHs over the NWP. The non-equilibrium of PAH gas-particle partitioning was shielded from the volatilization of three-ring gaseous PAHs from seawater and lower soot concentrations in particular when the oceanic <span class="hlt">air</span> masses prevailed. Modeling PAH absorption into organic matter and adsorption onto soot carbon revealed that the status of PAH gas-particle partitioning deviated more from the modeling K p for oceanic <span class="hlt">air</span> masses than those for continental <span class="hlt">air</span> masses, which coincided with higher volatilization of three-ring PAHs and confirmed the influence of <span class="hlt">air-sea</span> exchange. Meanwhile, significant linear regressions between logK p and logK oa (logK sa ) for PAHs were observed for continental <span class="hlt">air</span> masses, suggesting the dominant effect of East Asian continental outflow on atmospheric PAHs over the NWP during the sampling campaign. Copyright © 2017 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.6227M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.6227M"><span>The Labrador <span class="hlt">Sea</span> during the Last Glacial Maximum: Calcite dissolution or low biogenic carbonate <span class="hlt">fluxes</span>?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marshall, Nicole; de Vernal, Anne; Mucci, Alfonso; Filippova, Alexandra; Kienast, Markus</p> <p>2017-04-01</p> <p>Low concentrations of biogenic carbonate characterize the sediments deposited in the Labrador <span class="hlt">Sea</span> during the last glaciation. This may reflect poor calcite preservation and/or low biogenic carbonate productivity and <span class="hlt">fluxes</span>. Regional bottom water ventilation was reduced during the Last Glacial Maximum (LGM), so the calcite lysocline might have been shallower than at present in the deep Labrador <span class="hlt">Sea</span> making dissolution of calcite shells in the deep Labrador <span class="hlt">Sea</span> possible. To address the issue, a multi-proxy approach based on micropaleontological counts (coccoliths, foraminifers, palynomorphs) and biogeochemical analyses (alkenones) was applied in the investigation of core HU2008-029-004-PC recovered in the northwestern Labrador <span class="hlt">Sea</span>. Calcite dissolution indices based on the relative abundance benthic foraminifera shells to their organic linings as well as on fragmentation of planktonic foraminifera shells were used to evaluate changes in calcite dissolution/ preservation since the LGM. In addition, the ratio of the concentrations of coccoliths, specifically of the alkenone-producer Emiliania huxleyi, and alkenones (Emiliania huxleyi: alkenones) was explored as a potential new proxy of calcite dissolution. A sharp increase in coccoliths, foraminifers and organic linings from nearly none to substantial concentrations at 12 ka, reflect a jump to significantly greater biogenic <span class="hlt">fluxes</span> at the glacial-interglacial transition. Furthermore, conventional dissolution indices (shells/linings of benthic foraminifera and fragmentation of planktic foraminifers) reveal that dissolution is not likely responsible for the lower glacial abundances of coccoliths and foraminifers. Only the low Emiliania huxleyi: alkenones ratios in glacial sediments could be interpreted as evidence of increased dissolution during the LGM. Given the evidence of allochthonous alkenone input into the glacial Labrador <span class="hlt">Sea</span>, the latter observations must be treated with caution. Overall, the records indicate that</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004AGUFMOS52A..01D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004AGUFMOS52A..01D"><span>Particle <span class="hlt">Fluxes</span> in the Marginal <span class="hlt">Seas</span> of Antarctica: A 20-year Synthesis in Honor of Jack Dymond</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dunbar, R. B.; Langone, L.</p> <p>2004-12-01</p> <p>One of Jack Dymond's long-standing scientific passions was the study of particles moving through the ocean water column. Jack's pioneering work in this area in the 1970's and generous mentoring of others throughout his career lead directly to the first authors involvement in sediment trap studies. Here we present a synthesis of 20 years of particle <span class="hlt">flux</span> studies in coastal Antarctic (including the work of Collier and Dymond et al.) and highlight some of the important features and unresolved issues related to integrating particle trap interceptor data with other measures of production, transport, and deposition. The first sediment trap arrays were deployed on the Antarctic shelf in 1981 and 1982 in the Antarctic Peninsula. Simple instruments were also deployed in 1984 and 1986 in the Ross <span class="hlt">Sea</span>. Since then, several nations (US, Italy, New Zealand) have recovered time series sediment trap data on moorings in both of these areas. This current synthesis makes use of data from approximately 22 sites, the majority of which are in the Ross <span class="hlt">Sea</span>, and includes about 900 discrete samples of particles in vertical transit through the water column. We now have many complete time series that extend through the winter, allowing several important generalizations to be made. For example, annual particle-mediated organic C <span class="hlt">fluxes</span> to below 200 meters in the Ross <span class="hlt">Sea</span> average 4.4±3.3 g C m-2 yr-1. These values are significantly less than export <span class="hlt">fluxes</span> calculated using short-term surface water mass balance approaches or Th isotope techniques yet are higher than seabed sediment accumulation rates. Intriguingly, seasonal seabed arrival rates of organic C estimated from in-situ summertime benthic respirometry studies yield C <span class="hlt">flux</span> values similar in magnitude to those from sediment traps deployed at the same time, lending strong support to trap data. The cause of current disagreements between various methods of <span class="hlt">flux</span> estimation may in fact not be solved until process studies are accomplished</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 1.2m/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://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 pCO2 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://hdl.handle.net/2060/19930018948','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19930018948"><span><span class="hlt">Sea</span> ice-atmospheric interaction: Application of multispectral satellite data in polar surface energy <span class="hlt">flux</span> estimates</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Steffen, Konrad; Key, J.; Maslanik, J.; Schweiger, A.</p> <p>1993-01-01</p> <p>This is the third annual report on: <span class="hlt">Sea</span> Ice-Atmosphere Interaction - Application of Multispectral Satellite Data in Polar Surface Energy <span class="hlt">Flux</span> Estimates. The main emphasis during the past year was on: radiative <span class="hlt">flux</span> estimates from satellite data; intercomparison of satellite and ground-based cloud amounts; radiative cloud forcing; calibration of the Advanced Very High Resolution Radiometer (AVHRR) visible channels and comparison of two satellite derived albedo data sets; and on <span class="hlt">flux</span> modeling for leads. Major topics covered are arctic clouds and radiation; snow and ice albedo, and leads and modeling.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19910004469','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19910004469"><span><span class="hlt">Sea</span> ice-atmosphere interaction: Application of multispectral satellite data in polar surface energy <span class="hlt">flux</span> estimates</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Steffen, K.; Schweiger, A.; Maslanik, J.; Key, J.; Weaver, R.; Barry, R.</p> <p>1990-01-01</p> <p>The application of multi-spectral satellite data to estimate polar surface energy <span class="hlt">fluxes</span> is addressed. To what accuracy and over which geographic areas large scale energy budgets can be estimated are investigated based upon a combination of available remote sensing and climatological data sets. The general approach was to: (1) formulate parameterization schemes for the appropriate <span class="hlt">sea</span> ice energy budget terms based upon the remotely sensed and/or in-situ data sets; (2) conduct sensitivity analyses using as input both natural variability (observed data in regional case studies) and theoretical variability based upon energy <span class="hlt">flux</span> model concepts; (3) assess the applicability of these parameterization schemes to both regional and basin wide energy balance estimates using remote sensing data sets; and (4) assemble multi-spectral, multi-sensor data sets for at least two regions of the Arctic Basin and possibly one region of the Antarctic. The type of data needed for a basin-wide assessment is described and the temporal coverage of these data sets are determined by data availability and need as defined by parameterization scheme. The titles of the subjects are as follows: (1) Heat <span class="hlt">flux</span> calculations from SSM/I and LANDSAT data in the Bering <span class="hlt">Sea</span>; (2) Energy <span class="hlt">flux</span> estimation using passive microwave data; (3) Fetch and stability sensitivity estimates of turbulent heat <span class="hlt">flux</span>; and (4) Surface temperature algorithm.</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 (CO2), although to what extent is not clear. Here, we analyze CO2 dynamics within <span class="hlt">sea</span> ice using a one-dimensional halothermodynamic <span class="hlt">sea</span> ice model including gas physics and carbon biogeochemistry. The ice-ocean <span class="hlt">fluxes</span>, and vertical transport, of total dissolved inorganic carbon (DIC) and total alkalinity (TA) are represented using fluid transport equations. Carbonate chemistry, the consumption, and release of CO2 by primary production and respiration, the precipitation and dissolution of ikaite (CaCO3·6H2O) and ice-<span class="hlt">air</span> CO2 <span class="hlt">fluxes</span>, are also included. The model is evaluated using observations from a 6 month field study at Point Barrow, Alaska, and an ice-tank experiment. At Barrow, results show that the DIC budget is mainly driven by physical processes, wheras brine-<span class="hlt">air</span> CO2 <span class="hlt">fluxes</span>, ikaite formation, and net primary production, are secondary factors. In terms of ice-atmosphere CO2 exchanges, <span class="hlt">sea</span> ice is a net CO2 source and sink in winter and summer, respectively. The formulation of the ice-atmosphere CO2 <span class="hlt">flux</span> impacts the simulated near-surface CO2 partial pressure (pCO2), but not the DIC budget. Because the simulated ice-atmosphere CO2 <span class="hlt">fluxes</span> are limited by DIC stocks, and therefore <2 mmol m-2 d-1, we argue that the observed much larger CO2 <span class="hlt">fluxes</span> from eddy covariance retrievals cannot be explained by a <span class="hlt">sea</span> ice direct source and must involve other processes or other sources of CO2. Finally, the simulations suggest that near-surface TA/DIC ratios of ˜2, 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 (CO2), although to what extent is not clear. Here, we analyze CO2 dynamics within <span class="hlt">sea</span> ice using a one-dimensional halo-thermodynamic <span class="hlt">sea</span> ice model including gas physics and carbon biogeochemistry. The ice-ocean <span class="hlt">fluxes</span>, and vertical transport, of total dissolved inorganic carbon (DIC) and total alkalinity (TA) are represented using fluid transport equations. Carbonate chemistry, the consumption and release of CO2 by primary production and respiration, the precipitation and dissolution of ikaite (CaCO3•6H2O) and ice-<span class="hlt">air</span> CO2 <span class="hlt">fluxes</span>, are also included. The model is evaluated using observations from a 6-month field study at Point Barrow, Alaska and an ice-tank experiment. At Barrow, results show that the DIC budget is mainly driven by physical processes, wheras brine-<span class="hlt">air</span> CO2 <span class="hlt">fluxes</span>, ikaite formation, and net primary production, are secondary factors. In terms of ice-atmosphere CO2 exchanges, <span class="hlt">sea</span> ice is a net CO2 source and sink in winter and summer, respectively. The formulation of the ice-atmosphere CO2 <span class="hlt">flux</span> impacts the simulated near-surface CO2 partial pressure (pCO2), but not the DIC budget. Because the simulated ice-atmosphere CO2 <span class="hlt">fluxes</span> are limited by DIC stocks, and therefore < 2 mmol m-2 day-1, we argue that the observed much larger CO2 <span class="hlt">fluxes</span> from eddy covariance retrievals cannot be explained by a <span class="hlt">sea</span> ice direct source and must involve other processes or other sources of CO2. Finally, the simulations suggest that near surface TA/DIC ratios of ~2, 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/2008ACP.....8..555N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008ACP.....8..555N"><span>Eddy covariance measurements of <span class="hlt">sea</span> spray particles over the Atlantic Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Norris, S. J.; Brooks, I. M.; de Leeuw, G.; Smith, M. H.; Moerman, M.; Lingard, J. J. N.</p> <p>2008-02-01</p> <p>Most estimates of <span class="hlt">sea</span> spray aerosol source functions have used indirect means to infer the rate of production as a function of wind speed. Only recently has the technology become available to make high frequency measurements of aerosol spectra suitable for direct eddy correlation determination of the <span class="hlt">sea</span> spray particle <span class="hlt">flux</span>. This was accomplished in this study by combining a newly developed fast aerosol particle counter with an ultrasonic anemometer which allowed for eddy covariance measurements of size-segregated particle <span class="hlt">fluxes</span>. The aerosol instrument is the Compact Lightweight Aerosol Spectrometer Probe (CLASP) - capable of measuring 8-channel size spectra for mean radii between 0.15 and 3.5 µm at 10 Hz. The first successful measurements were made during the Waves, <span class="hlt">Air</span> <span class="hlt">Sea</span> <span class="hlt">Fluxes</span>, Aerosol and Bubbles (WASFAB) field campaign in October 2005 in Duck (NC, USA). The method and initial results are presented and comparisons are made with recent <span class="hlt">sea</span> spray source functions from the literature.</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('https://www.ncbi.nlm.nih.gov/pubmed/28472695','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28472695"><span>Perfluoroalkyl and polyfluoroalkyl substances in the lower atmosphere and surface waters of the Chinese Bohai <span class="hlt">Sea</span>, Yellow <span class="hlt">Sea</span>, and Yangtze River estuary.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhao, Zhen; Tang, Jianhui; Mi, Lijie; Tian, Chongguo; Zhong, Guangcai; Zhang, Gan; Wang, Shaorui; Li, Qilu; Ebinghaus, Ralf; Xie, Zhiyong; Sun, Hongwen</p> <p>2017-12-01</p> <p>Polyfluoroalkyl and perfluoroalkyl substances (PFASs), in the forms of neutral polyfluoroalkyl substances in the gas phase of <span class="hlt">air</span> and ionic perfluoroalkyl substances in the dissolved phase of surface water, were investigated during a sampling campaign in the Bohai <span class="hlt">Sea</span>, Yellow <span class="hlt">Sea</span>, and Yangtze River estuary in May 2012. In the gas phase, the concentrations of neutral ∑PFASs were within the range of 76-551pg/m 3 . Higher concentrations were observed in the South Yellow <span class="hlt">Sea</span>. 8:2 fluorotelomer alcohol (FTOH) was the predominant compound as it accounted for 92%-95% of neutral ∑PFASs in all <span class="hlt">air</span> samples. <span class="hlt">Air</span> mass backward trajectory analysis indicated that neutral ∑PFASs came mainly from the coast of the Yellow <span class="hlt">Sea</span>, including the Shandong, Jiangsu, and Zhejiang provinces of China, and the coastal region of South Korea. The <span class="hlt">fluxes</span> of gas phase dry deposition were simulated for neutral PFASs, and neutral ∑PFASs <span class="hlt">fluxes</span> varied from 0.37 to 2.3pg/m 2 /s. In the dissolved phase of the surface water, concentrations of ionic ∑PFASs ranged from 1.6 to 118ng/L, with the Bohai <span class="hlt">Sea</span> exhibiting higher concentrations than both the Yellow <span class="hlt">Sea</span> and the Yangtze River estuary. Perfluorooctanoic acid (PFOA) was the predominant compound accounting for 51%-90% of the ionic ∑PFAS concentrations. Releases from industrial and domestic activities as well as the semiclosed geographical conditions increased the level of ionic ∑PFASs in the Bohai <span class="hlt">Sea</span>. The spatial distributions of perfluoroalkyl carboxylic acids (PFCAs) and perfluoroalkane sulfonic acids (PFSAs) were different significantly. The Laizhou Bay was the major source region of PFCAs and the Yangtze River estuary was the major source of PFSAs. Copyright © 2017 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AIPC.1813f0001K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AIPC.1813f0001K"><span>Effect of <span class="hlt">air</span> gap variation on the performance of single stator single rotor axial <span class="hlt">flux</span> permanent magnet generator</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kasim, Muhammad; Irasari, Pudji; Hikmawan, M. Fathul; Widiyanto, Puji; Wirtayasa, Ketut</p> <p>2017-02-01</p> <p>The axial <span class="hlt">flux</span> permanent magnet generator (AFPMG) has been widely used especially for electricity generation. The effect of the <span class="hlt">air</span> gap variation on the characteristic and performances of single rotor - single stator AFPMG has been described in this paper. Effect of <span class="hlt">air</span> gap length on the magnetic <span class="hlt">flux</span> distribution, starting torque and MMF has been investigated. The two dimensional finite element magnetic method has been deployed to model and simulated the characteristics of the machine which is based on the Maxwell equation. The analysis has been done for two different <span class="hlt">air</span> gap lengths which were 2 mm and 4 mm using 2D FEMM 4.2 software at no load condition. The increasing of <span class="hlt">air</span> gap length reduces the <span class="hlt">air</span>-gap <span class="hlt">flux</span> density. For <span class="hlt">air</span> gap 2 mm, the maximum value of the <span class="hlt">flux</span> density was 1.04 T while 0.73 T occured for <span class="hlt">air</span> gap 4 mm.. Based on the experiment result, the increasing <span class="hlt">air</span> gap also reduced the starting torque of the machine with 39.2 Nm for <span class="hlt">air</span> gap 2 mm and this value decreased into 34.2 Nm when the <span class="hlt">air</span> gap increased to 4 mm. Meanwhile, the MMF that was generated by AFPMG decreased around 22% at 50 Hz due to the reduction of magnetic <span class="hlt">flux</span> induced on stator windings. Overall, the research result showed that the variation of <span class="hlt">air</span> gap has significant effect on the machine characteristics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ClDy...48.1089L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ClDy...48.1089L"><span>A multi-model ensemble view of winter heat <span class="hlt">flux</span> dynamics and the dipole mode 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>Liguori, Giovanni; Di Lorenzo, Emanuele; Cabos, William</p> <p>2017-02-01</p> <p>Changes in surface heat <span class="hlt">fluxes</span> affect several climate processes controlling the Mediterranean climate. These include the winter formation of deep waters, which is the primary driver of the Mediterranean <span class="hlt">Sea</span> overturning circulation. Previous studies that characterize the spatial and temporal variability of surface heat <span class="hlt">flux</span> anomalies over the basin reveal the existence of two statistically dominant patterns of variability: a monopole of uniform sign and an east-west dipole of opposite signs. In this work, we use the 12 regional climate model ensemble from the EU-FP6 ENSEMBLES project to diagnose the large-scale atmospheric processes that control the variability of heat <span class="hlt">fluxes</span> over the Mediterranean <span class="hlt">Sea</span> from interannual to decadal timescales (here defined as timescales > 6 year). Our findings suggest that while the monopole structure captures variability in the winter-to-winter domain-average net heat <span class="hlt">flux</span>, the dipole pattern tracks changes in the Mediterranean climate that are connected to the East Atlantic/Western Russia (EA/WR) atmospheric teleconnection pattern. Furthermore, while the monopole exhibits significant differences in the spatial structure across the multi-model ensemble, the dipole pattern is very robust and more clearly identifiable in the anomaly maps of individual years. A heat budget analysis of the dipole pattern reveals that changes in winds associated with the EA/WR pattern exert dominant control through both a direct effect on the latent heat <span class="hlt">flux</span> (i.e., wind speed) and an indirect effect through specific humidity (e.g., wind advection). A simple reconstruction of the heat <span class="hlt">flux</span> variability over the deep-water formation regions of the Gulf of Lion and the Aegean <span class="hlt">Sea</span> reveals that the combination of the monopole and dipole time series explains over 90 % of the heat <span class="hlt">flux</span> variance in these regions. Given the important role that surface heat <span class="hlt">flux</span> anomalies play in deep-water formation and the regional climate, improving our knowledge on the dynamics</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006JPhy4.139..211E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006JPhy4.139..211E"><span>Occurrence and <span class="hlt">air/sea</span>-exchange of novel organic pollutants in the marine environment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ebinghaus, R.; Xie, Z.</p> <p>2006-12-01</p> <p>A number of studies have demonstrated that several classes of chemicals act as biologically relevant signalling substances. Among these chemicals, many, including PCBs, DDT and dioxins, are semi-volatile, persistent, and are capable of long-range atmospheric transport via atmospheric circulation. Some of these compounds, e.g. phthalates and alkylphenols (APs) are still manufactured and consumed worldwide even though there is clear evidence that they are toxic to aquatic organisms and can act as endocrine disruptors. Concentrations of NP, t-OP and NP1EO, DMP, DEP, DBP, BBP, and DEHP have been simultaneously determined in the surface <span class="hlt">sea</span> water and atmosphere of the North <span class="hlt">Sea</span>. Atmospheric concentrations of NP and t-OP ranged from 7 to 110 pg m - 3, which were one to three orders of magnitude below coastal atmospheric concentrations already reported. NP1EO was detected in both vapor and particle phases, which ranged from 4 to 50 pg m - 3. The concentrations of the phthalates in the atmosphere ranged from below the method detection limit to 3.4 ng m - 3. The concentrations of t-OP, NP, and NP1EO in dissolved phase were 13-300, 90-1400, and 17-1660 pg L - 1. DBP, BBP, and DEHP were determined in the water phase with concentrations ranging from below the method detection limit to 6.6 ng L - 1. This study indicates that atmospheric deposition of APs and phthalates into the North <span class="hlt">Sea</span> is an important input pathway. The net <span class="hlt">fluxes</span> indicate that the <span class="hlt">air</span> <span class="hlt">sea</span> exchange is significant and, consequently the open ocean and polar areas will be an extensive sink for APs and phthalates.</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://pubs.er.usgs.gov/publication/70168738','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70168738"><span>Surface-<span class="hlt">air</span> mercury <span class="hlt">fluxes</span> across Western North America: A synthesis of spatial trends and controlling variables</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Eckley, Chris S.; Tate, Michael T.; Lin, Che-Jen; Gustin, Mae S.; Dent, Stephen; Eagles-Smith, Collin A.; Lutz, Michelle A; Wickland, Kimberly; Wang, Bronwen; Gray, John E.; Edwards, Grant; Krabbenhoft, David P.; Smith, David</p> <p>2016-01-01</p> <p>Mercury (Hg) emission and deposition can occur to and from soils, and are an important component of the global atmospheric Hg budget. This paper focuses on synthesizing existing surface-<span class="hlt">air</span> Hg <span class="hlt">flux</span> data collected throughout the Western North American region and is part of a series of geographically focused Hg synthesis projects. A database of existing Hg <span class="hlt">flux</span> data collected using the dynamic <span class="hlt">flux</span> chamber (DFC) approach from almost a thousand locations was created for the Western North America region. Statistical analysis was performed on the data to identify the important variables controlling Hg <span class="hlt">fluxes</span> and to allow spatiotemporal scaling. The results indicated that most of the variability in soil-<span class="hlt">air</span> Hg <span class="hlt">fluxes</span> could be explained by variations in soil-Hg concentrations, solar radiation, and soil moisture. This analysis also identified that variations in DFC methodological approaches were detectable among the field studies, with the chamber material and sampling flushing flow rate influencing the magnitude of calculated emissions. The spatiotemporal scaling of soil-<span class="hlt">air</span> Hg <span class="hlt">fluxes</span> identified that the largest emissions occurred from irrigated agricultural landscapes in California. Vegetation was shown to have a large impact on surface-<span class="hlt">air</span> Hg <span class="hlt">fluxes</span> due to both a reduction in solar radiation reaching the soil as well as from direct uptake of Hg in foliage. Despite high soil Hg emissions from some forested and other heavily vegetated regions, the net ecosystem <span class="hlt">flux</span> (soil <span class="hlt">flux</span> + vegetation uptake) was low. Conversely, sparsely vegetated regions showed larger net ecosystem emissions, which were similar in magnitude to atmospheric Hg deposition (except for the Mediterranean California region where soil emissions were higher). The net ecosystem <span class="hlt">flux</span> results highlight the important role of landscape characteristics in effecting the balance between Hg sequestration and (re-)emission to the atmosphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.B31J..05E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.B31J..05E"><span>Surface-<span class="hlt">Air</span> Mercury <span class="hlt">Fluxes</span> Across Western North America: A Synthesis of Spatial Trends and Controlling Variables.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Eckley, C.; Tate, M.; Lin, C. J.; Gustin, M. S.; Dent, S.; Eagles-Smith, C.; Lutz, M.; Wickland, K.; Wang, B.; Gray, J.; Edwards, G. C.; Krabbenhoft, D. P.; Smith, D. B.</p> <p>2016-12-01</p> <p>Mercury (Hg) emission and deposition can occur to and from soils and are an important component of the global atmospheric Hg budget. This presentation focuses on synthesizing existing surface-<span class="hlt">air</span> Hg <span class="hlt">flux</span> data collected throughout the Western North American region and is part of a series of geographically focused Hg synthesis projects. A database of existing Hg <span class="hlt">flux</span> data collected using the dynamic <span class="hlt">flux</span> chamber (DFC) approach from almost a thousand locations was created for the Western North America region. Statistical analysis was performed on the data to identify the important variables controlling Hg <span class="hlt">fluxes</span> and to allow spatiotemporal scaling. The results indicated that most of the variability in soil-<span class="hlt">air</span> Hg <span class="hlt">fluxes</span> could be explained by variations in soil-Hg concentrations, solar radiation, and soil moisture. This analysis also identified that variations in DFC methodological approaches were detectable among the field studies, with the chamber material and sampling flushing flow rate influencing the magnitude of calculated emissions. The spatiotemporal scaling of soil-<span class="hlt">air</span> Hg <span class="hlt">fluxes</span> identified that the largest emissions occurred from irrigated agricultural landscapes in California. Vegetation was shown to have a large impact on surface-<span class="hlt">air</span> Hg <span class="hlt">fluxes</span> due to both a reduction in solar radiation reaching the soil as well as from direct uptake of Hg in foliage. Despite high soil Hg emissions from some forested and other heavily vegetated regions, the net ecosystem <span class="hlt">flux</span> (soil <span class="hlt">flux</span> + vegetation uptake) was low. Conversely, sparsely vegetated regions showed larger net ecosystem emissions, which were similar in magnitude to atmospheric Hg deposition (except for the Mediterranean California region where soil emissions were higher). The net ecosystem <span class="hlt">flux</span> results highlight the important role of landscape characteristics in effecting the balance between Hg sequestration and (re-)emission to the atmosphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PolSc..13...13Q','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PolSc..13...13Q"><span>Dimethylsulfide model calibration and parametric sensitivity analysis for the Greenland <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Qu, Bo; Gabric, Albert J.; Zeng, Meifang; Xi, Jiaojiao; Jiang, Limei; Zhao, Li</p> <p>2017-09-01</p> <p><span class="hlt">Sea-to-air</span> <span class="hlt">fluxes</span> of marine biogenic aerosols have the potential to modify cloud microphysics and regional radiative budgets, and thus moderate Earth's warming. Polar regions play a critical role in the evolution of global climate. In this work, we use a well-established biogeochemical model to simulate the DMS <span class="hlt">flux</span> from the Greenland <span class="hlt">Sea</span> (20°W-10°E and 70°N-80°N) for the period 2003-2004. Parameter sensitivity analysis is employed to identify the most sensitive parameters in the model. A genetic algorithm (GA) technique is used for DMS model parameter calibration. Data from phase 5 of the Coupled Model Intercomparison Project (CMIP5) are used to drive the DMS model under 4 × CO2 conditions. DMS <span class="hlt">flux</span> under quadrupled CO2 levels increases more than 300% compared with late 20th century levels (1 × CO2). Reasons for the increase in DMS <span class="hlt">flux</span> include changes in the ocean state-namely an increase in <span class="hlt">sea</span> surface temperature (SST) and loss of <span class="hlt">sea</span> ice-and an increase in DMS transfer velocity, especially in spring and summer. Such a large increase in DMS <span class="hlt">flux</span> could slow the rate of warming in the Arctic via radiative budget changes associated with DMS-derived aerosols.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.A33G3274G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.A33G3274G"><span>Updating <span class="hlt">Sea</span> Spray Aerosol Emissions in the Community Multiscale <span class="hlt">Air</span> Quality Model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gantt, B.; Bash, J. O.; Kelly, J.</p> <p>2014-12-01</p> <p><span class="hlt">Sea</span> spray aerosols (SSA) impact the particle mass concentration and gas-particle partitioning in coastal environments, with implications for human and ecosystem health. In this study, the Community Multiscale <span class="hlt">Air</span> Quality (CMAQ) model is updated to enhance fine mode SSA emissions, include <span class="hlt">sea</span> surface temperature (SST) dependency, and revise surf zone emissions. Based on evaluation with several regional and national observational datasets in the continental U.S., the updated emissions generally improve surface concentrations predictions of primary aerosols composed of <span class="hlt">sea</span>-salt and secondary aerosols affected by <span class="hlt">sea</span>-salt chemistry in coastal and near-coastal sites. Specifically, the updated emissions lead to better predictions of the magnitude and coastal-to-inland gradient of sodium, chloride, and nitrate concentrations at Bay Regional Atmospheric Chemistry Experiment (BRACE) sites near Tampa, FL. Including SST-dependency to the SSA emission parameterization leads to increased sodium concentrations in the southeast U.S. and decreased concentrations along the Pacific coast and northeastern U.S., bringing predictions into closer agreement with observations at most Interagency Monitoring of Protected Visual Environments (IMPROVE) and Chemical Speciation Network (CSN) sites. Model comparison with California Research at the Nexus of <span class="hlt">Air</span> Quality and Climate Change (CalNex) observations will also be discussed, with particular focus on the South Coast <span class="hlt">Air</span> Basin where clean marine <span class="hlt">air</span> mixes with anthropogenic pollution in a complex environment. These SSA emission updates enable more realistic simulation of chemical processes in coastal environments, both in clean marine <span class="hlt">air</span> masses and mixtures of clean marine and polluted conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1989JGR....9418195J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1989JGR....9418195J"><span><span class="hlt">Sea</span> ice and oceanic processes on the Ross <span class="hlt">Sea</span> continental shelf</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jacobs, S. S.; Comiso, J. C.</p> <p>1989-12-01</p> <p>We have investigated the spatial and temporal variability of Antarctic <span class="hlt">sea</span> ice concentrations on the Ross <span class="hlt">Sea</span> continental shelf, in relation to oceanic and atmospheric forcing. <span class="hlt">Sea</span> ice data were derived from Nimbus 7 scanning multichannel microwave radiometer (SMMR) brightness temperatures from 1979-1986. Ice cover over the shelf was persistently lower than above the adjacent deep ocean, averaging 86% during winter with little month-to-month or interannual variability. The large spring Ross <span class="hlt">Sea</span> polynya on the western shelf results in a longer period of summer insolation, greater surface layer heat storage, and later ice formation in that region the following autumn. Newly identified Pennell and Ross Passage polynyas near the continental shelf break appear to be maintained in part by divergence above a submarine bank and by upwelling of warmer water near the slope front. Warmer subsurface water enters the shelf region year-round and will retard ice growth and enhance heat <span class="hlt">flux</span> to the atmosphere when entrained in the strong winter vertical circulation. Temperatures at 125-m depth on a mooring near the Ross Ice Shelf during July 1984 averaged 0.15°C above freezing, sufficient to support a vertical heat <span class="hlt">flux</span> above 100 W/m2. Monthly average subsurface ocean temperatures along the Ross Ice Shelf lag the <span class="hlt">air</span> temperature cycle and begin to rise several weeks before spring ice breakout. The coarse SMMR resolution and dynamic ice shelf coastlines can compromise the use of microwave <span class="hlt">sea</span> ice data near continental boundaries.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140013403','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140013403"><span>Trends and Variations of Ocean Surface Latent Heat <span class="hlt">Flux</span>: Results from GSSTF2c Data Set</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gao, Si; Chiu, Long S.; Shie, Chung-Lin</p> <p>2013-01-01</p> <p>Trends and variations of Goddard Satellite-based Surface Turbulent <span class="hlt">Fluxes</span> (GSSTF) version 2c (GSSTF2c) latent heat <span class="hlt">flux</span> (LHF) are examined. This version of LHF takes account of the correction in Earth incidence angle. The trend of global mean LHF for GSSTF2c is much reduced relative to GSSTF version 2b Set 1 and Set 2 for the same period 1988-2008. Temporal increase of GSSTF2c LHF in the two decades is 11.0%, in which 3.1%, 5.8%, and 2.1% are attributed to the increase in wind, the increase in <span class="hlt">sea</span> surface saturated <span class="hlt">air</span> humidity, and the decrease in near-surface <span class="hlt">air</span> humidity, respectively. The first empirical orthogonal function of LHF is a conventional El Nino Southern Oscillation (ENSO) mode. However, the trends in LHF are independent of conventional ENSO phenomena. After removing ENSO signal, the pattern of LHF trends is primarily determined by the pattern of <span class="hlt">air-sea</span> humidity difference trends.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('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-2 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('http://adsabs.harvard.edu/abs/2018GeoRL..45.5204H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoRL..45.5204H"><span>The Unprecedented 2016-2017 Arctic <span class="hlt">Sea</span> Ice Growth Season: The Crucial Role of Atmospheric Rivers and Longwave <span class="hlt">Fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hegyi, Bradley M.; Taylor, Patrick C.</p> <p>2018-05-01</p> <p>The 2016-2017 Arctic <span class="hlt">sea</span> ice growth season (October-March) exhibited one of the lowest values for end-of-season <span class="hlt">sea</span> ice volume and extent of any year since 1979. An analysis of Modern-Era Retrospective Analysis for Research and Applications, Version 2 atmospheric reanalysis data and Clouds and the Earth's Radiant Energy System radiative <span class="hlt">flux</span> data reveals that a record warm and moist Arctic atmosphere supported the reduced <span class="hlt">sea</span> ice growth. Numerous regional episodes of increased atmospheric temperature and moisture, transported from lower latitudes, increased the cumulative energy input from downwelling longwave surface <span class="hlt">fluxes</span>. In those same episodes, the efficiency of the atmosphere cooling radiatively to space was reduced, increasing the amount of energy retained in the Arctic atmosphere and reradiated back toward the surface. Overall, the Arctic radiative cooling efficiency shows a decreasing trend since 2000. The results presented highlight the increasing importance of atmospheric forcing on <span class="hlt">sea</span> ice variability demonstrating that episodic Arctic atmospheric rivers, regions of elevated poleward water vapor transport, and the subsequent surface energy budget response is a critical mechanism actively contributing to the evolution of Arctic <span class="hlt">sea</span> ice.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ACP....18.5861S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ACP....18.5861S"><span>Gradient <span class="hlt">flux</span> measurements of <span class="hlt">sea-air</span> DMS transfer during the Surface Ocean Aerosol Production (SOAP) experiment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Smith, Murray J.; Walker, Carolyn F.; Bell, Thomas G.; Harvey, Mike J.; Saltzman, Eric S.; Law, Cliff S.</p> <p>2018-04-01</p> <p>Direct measurements of marine dimethylsulfide (DMS) <span class="hlt">fluxes</span> are sparse, particularly in the Southern Ocean. The Surface Ocean Aerosol Production (SOAP) voyage in February-March 2012 examined the distribution and <span class="hlt">flux</span> of DMS in a biologically active frontal system in the southwest Pacific Ocean. Three distinct phytoplankton blooms were studied with oceanic DMS concentrations as high as 25 nmol L-1. Measurements of DMS <span class="hlt">fluxes</span> were made using two independent methods: the eddy covariance (EC) technique using atmospheric pressure chemical ionization-mass spectrometry (API-CIMS) and the gradient <span class="hlt">flux</span> (GF) technique from an autonomous catamaran platform. Catamaran <span class="hlt">flux</span> measurements are relatively unaffected by airflow distortion and are made close to the water surface, where gas gradients are largest. <span class="hlt">Flux</span> measurements were complemented by near-surface hydrographic measurements to elucidate physical factors influencing DMS emission. Individual DMS <span class="hlt">fluxes</span> derived by EC showed significant scatter and, at times, consistent departures from the Coupled Ocean-Atmosphere Response Experiment gas transfer algorithm (COAREG). A direct comparison between the two <span class="hlt">flux</span> methods was carried out to separate instrumental effects from environmental effects and showed good agreement with a regression slope of 0.96 (r2 = 0.89). A period of abnormal downward atmospheric heat <span class="hlt">flux</span> enhanced near-surface ocean stratification and reduced turbulent exchange, during which GF and EC transfer velocities showed good agreement but modelled COAREG values were significantly higher. The transfer velocity derived from near-surface ocean turbulence measurements on a spar buoy compared well with the COAREG model in general but showed less variation. This first direct comparison between EC and GF <span class="hlt">fluxes</span> of DMS provides confidence in compilation of <span class="hlt">flux</span> estimates from both techniques, as well as in the stable periods when the observations are not well predicted by the COAREG model.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4949426','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4949426"><span>Benthic <span class="hlt">fluxes</span> of dissolved organic carbon from gas hydrate sediments in the northern South China <span class="hlt">Sea</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>Hung, Chia-Wei; Huang, Kuo-Hao; Shih, Yung-Yen; Lin, Yu-Shih; Chen, Hsin-Hung; Wang, Chau-Chang; Ho, Chuang-Yi; Hung, Chin-Chang; Burdige, David J.</p> <p>2016-01-01</p> <p>Hydrocarbon vents have recently been reported to contribute considerable amounts of dissolved organic carbon (DOC) to the oceans. Many such hydrocarbon vents widely exist in the northern South China <span class="hlt">Sea</span> (NSCS). To investigate if these hydrocarbon vent sites release DOC, we used a real-time video multiple-corer to collect bottom seawater and surface sediments at vent sites. We analyzed concentrations of DOC in these samples and estimated DOC <span class="hlt">fluxes</span>. Elevated DOC concentrations in the porewaters were found at some sites suggesting that DOC may come from these hydrocarbon vents. Benthic <span class="hlt">fluxes</span> of DOC from these sediments were 28 to 1264 μmol m−2 d−1 (on average ~321 μmol m−2 d−1) which are several times higher than most DOC <span class="hlt">fluxes</span> in coastal and continental margin sediments. The results demonstrate that the real-time video multiple-corer can precisely collect samples at vent sites. The estimated benthic DOC <span class="hlt">flux</span> from the methane venting sites (8.6 × 106 mol y−1), is 24% of the DOC discharge from the Pearl River to the South China <span class="hlt">Sea</span>, indicating that these sediments make an important contribution to the DOC in deep waters. PMID:27432631</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A44C..08M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A44C..08M"><span>The Role of <span class="hlt">Air-sea</span> Coupling in the Response of Climate Extremes to Aerosols</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mahajan, S.</p> <p>2017-12-01</p> <p><span class="hlt">Air-sea</span> interactions dominate the climate of surrounding regions and thus also modulate the climate response to local and remote aerosol forcings. To clearly isolate the role of <span class="hlt">air-sea</span> coupling in the climate response to aerosols, we conduct experiments with a full complexity atmosphere model that is coupled to a series of ocean models progressively increasing in complexity. The ocean models range from a data ocean model with prescribed SSTs, to a slab ocean model that only allows thermodynamic interactions, to a full dynamic ocean model. In a preliminary study, we have conducted single forcing experiments with black carbon aerosols in an atmosphere GCM coupled to a data ocean model and a slab ocean model. We find that while black carbon aerosols can intensify mean and extreme summer monsoonal precipitation over the Indian sub-continent, <span class="hlt">air-sea</span> coupling can dramatically modulate this response. Black carbon aerosols in the vicinity of the Arabian <span class="hlt">Sea</span> result in an increase of <span class="hlt">sea</span> surface temperatures there in the slab ocean model, which intensify the low-level Somali Jet. The associated increase in moisture transport into Western India enhances the mean as well as extreme precipitation. In prescribed SST experiments, where SSTs are not allowed to respond BC aerosols, the response is muted. We will present results from a hierarchy of GCM simulations that investigate the role of <span class="hlt">air-sea</span> coupling in the climate response to aerosols in more detail.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUSM.B11A..01C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUSM.B11A..01C"><span>Proposed Gulf of Mexico Intensive Study on Carbon <span class="hlt">Fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Coble, P. G.; Robbins, L.; Lohrenz, S.; Cai, W.</p> <p>2009-05-01</p> <p>The Gulf of Mexico is an ideal site for the study of land-ocean carbon cycle coupling processes. A recent synthesis suggests that Gulf of Mexico <span class="hlt">air-sea</span> CO2 <span class="hlt">flux</span> may dominate the net <span class="hlt">flux</span> of the entire North American margin because of the Gulf's large size and strong carbon signals. Northern Gulf waters appear to be a strong local CO2 sink due to high primary productivity stimulated by river input of anthropogenic nutrients from the North American continent. Nutrient discharge from the Mississippi River has been implicated in widespread hypoxia on the shelf. The surface drainage system of the Gulf covers more than 60% of the U.S. and more than 40% of Mexico; thus, large-scale changes in land-use and water-management practices in both countries, as well as changes in temperature and rainfall due to climate change, will profoundly affect Gulf carbon <span class="hlt">fluxes</span>. Nevertheless, major sources of uncertainty in the North American carbon budget remain because of largely unsampled areas, undocumented key <span class="hlt">fluxes</span>, such as <span class="hlt">air-sea</span> exchange of carbon dioxide, associated carbon <span class="hlt">fluxes</span>, and poorly characterized control mechanisms. An intensive study in which the Gulf is considered as a whole system, including watersheds, margins, open Gulf of Mexico, overlying atmosphere, and underlying sediments, will be discussed. The study is best addressed using a three-pronged approach that incorporates remote sensing observations, field observations and experiments, and physical and biogeochemical modeling. Societal issues related to carbon management and land-use/land-change must be an integral part of such a study. International cooperation with Mexico, Canada, and Cuba will be essential for the success of this study.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA622312','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA622312"><span>Operationalizing <span class="hlt">Air-Sea</span> Battle in the Pacific</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2015-02-01</p> <p>Joumall 25 \\/ FEATURE Ballard, Harysch, Cole, & Hall Operationalizing Ait’-<span class="hlt">Sea</span> Battle in the Pacific tribes and nomadic marauders such as the...communications in general, the former focuses on the digital data links between different platforms. The original CSBA operational con- cept touches on this...very capable fourth-generation fighters; and it has fielded layers of upgraded and double- digit surface-to-<span class="hlt">air</span> missile systems and antiaircraft</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AcMeS..27..308F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AcMeS..27..308F"><span>Numerical study on the impacts of the bogus data assimilation and <span class="hlt">sea</span> spray parameterization on typhoon ducts</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fei, Jianfang; Ding, Juli; Huang, Xiaogang; Cheng, Xiaoping; Hu, Xiaohua</p> <p>2013-06-01</p> <p>The Weather Research and Forecasting model version 3.2 (WRF v3.2) was used with the bogus data assimilation (BDA) scheme and <span class="hlt">sea</span> spray parameterization (SSP), and experiments were conducted to assess the impacts of the BDA and SSP on prediction of the typhoon ducting process induced by Typhoon Mindule (2004). The global positioning system (GPS) dropsonde observations were used for comparison. The results show that typhoon ducts are likely to form in every direction around the typhoon center, with the main type of ducts being elevated duct. With the BDA scheme included in the model initialization, the model has a better performance in predicting the existence, distribution, and strength of typhoon ducts. This improvement is attributed to the positive effect of the BDA scheme on the typhoon's ambient boundary layer structure. <span class="hlt">Sea</span> spray affects typhoon ducts mainly by changing the latent heat (LH) <span class="hlt">flux</span> at the <span class="hlt">air-sea</span> interface beyond 270 km from the typhoon center. The strength of the typhoon duct is enhanced when the boundary layer under this duct is cooled and moistened by the <span class="hlt">sea</span> spray; otherwise, the typhoon duct is weakened. The <span class="hlt">sea</span> spray induced changes in the <span class="hlt">air-sea</span> sensible heat (SH) <span class="hlt">flux</span> and LH <span class="hlt">flux</span> are concentrated in the maximum wind speed area near the typhoon center, and the changes are significantly weakened with the increase of the radial range.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19940008108','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19940008108"><span>A study of the Merritt Island, Florida <span class="hlt">sea</span> breeze flow regimes and their effect on surface heat and moisture <span class="hlt">fluxes</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rubes, M. T.; Cooper, H. J.; Smith, E. A.</p> <p>1993-01-01</p> <p>Data collected during the Convective and Precipitation/Electrification Experiment were analyzed as part of an investigation of the <span class="hlt">sea</span> breeze in the vicinity of Merritt Island, Florida. Analysis of near-surface divergence fields shows that the classical 24-hour oscillation in divergence over the island due to the direct <span class="hlt">sea</span> breeze circulation is frequently disrupted and exhibits two distinct modes: the classical <span class="hlt">sea</span> breeze pattern and deviations from that pattern. A comparison of clear day surface energy <span class="hlt">fluxes</span> with <span class="hlt">fluxes</span> on other days indicates that changes in magnitudes were dominated by the presence or absence of clouds. Non-classical <span class="hlt">sea</span> breeze days tended to lose more available energy in the morning than classical <span class="hlt">sea</span> breeze days due to earlier development of small cumulus over the island. A composite storm of surface winds, surface energy <span class="hlt">fluxes</span>, rainfall, and satellite visible data was constructed. A spectral transmittance over the visible wavelengths for the cloud cover resulting from the composite storm was calculated. It is shown that pre-storm transmittances of 0.8 fall to values near 0.1 as the downdraft moves directly over the site. It is also found that under post-composite storm conditions of continuous clear sky days, 3.5 days are required to evaporate back into the atmosphere the latent heat energy lost to the surface by rainfall.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..1410939S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..1410939S"><span>Bioproductivity in the Southern Ocean since the last Interglacial - new high-resolution biogenic opal <span class="hlt">flux</span> records from the Scotia <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sprenk, D.; Weber, M. E.; Kuhn, G.; Rosén, P.; Röhling, H.-G.</p> <p>2012-04-01</p> <p>The Southern Ocean plays an important role in transferring CO2 via wind-induced upwelling from the deep <span class="hlt">sea</span> to the atmosphere. It is therefore one of the key areas to study climate change. Bioproductivity in the Southern Ocean is mostly influenced by the extent of <span class="hlt">sea</span> ice, upwelling of cold nutrient- and silica-rich water, and the availability of light. Biogenic opal (BSi) is a significant nutrient in the Southern Ocean, and according to recent investigations only marginally affected by preservation changes. It can therefore be used as bioproductivity proxy. Here we present several methods to determine BSi, discuss them and put the results into context with respect to regional bioproductivity changes in Southern Ocean during the last glacial cycle. We studied deep-<span class="hlt">sea</span> sediment core sites MD07-3133 and MD07-3134 from the central Scotia <span class="hlt">Sea</span> with extraordinary high sedimentation rates of up to 2.1 to 1.2 m/kyr, respectively covering the last 92.5 kyr. BSi leaching according to Müller & Schneider (1993) is very time-consuming and expensive, so we measured only 253 samples from large-amplitude variation core sections. In addition, we determined BSi using non-destructive measurements of sediment colour b*, wet-bulk density, and Ti/Si count ratios. Furthermore, we provide the first attempts to estimate BSi in marine sediment using Fourier transform infrared spectroscopy (FTIRS), a cost-efficient method, which requires only 11 mg of sediment. All estimation methods capture the main BSi trends, however FTIRS seems to be the most promising one. In the central Scotia <span class="hlt">Sea</span>, south of the modern Antarctic Polar Front, the BSi <span class="hlt">flux</span> reflects a relatively complicated glacial-to-interglacial pattern with large-amplitude, millennial-scale fluctuations in bioproductivity. During Antarctic Isotopic Maxima, BSi <span class="hlt">fluxes</span> were generally increased. Lowest bioproductivity occur at the Last Glacial Maximum, while upwelling of mid-depth water was reduced, atmospheric CO2 low, and <span class="hlt">sea</span>-ice cover</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMNH34B..07S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMNH34B..07S"><span>Oceanographic, <span class="hlt">Air-sea</span> Interaction, and Environmental Aspects of Artificial Upwelling Produced by Wave-Inertia Pumps for Potential Hurricane Intensity Mitigation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Soloviev, A.; Dean, C.</p> <p>2017-12-01</p> <p>The artificial upwelling system consisting of the wave-inertia pumps driven by surface waves can produce flow of cold deep water to the surface. One of the recently proposed potential applications of the artificial upwelling system is the hurricane intensity mitigation. Even relatively small reduction of intensity may provide significant benefits. The ocean heat content (OHC) is the "fuel" for hurricanes. The OHC can be reduced by mixing of the surface layer with the cold water produced by wave-inertia pumps. Implementation of this system for hurricane mitigation has several oceanographic and <span class="hlt">air-sea</span> interaction aspects. The cold water brought to the surface from a deeper layer has higher density than the surface water and, therefore, tends to sink back down. The mixing of the cold water produced by artificial upwelling depends on environmental conditions such as stratification, regional ocean circulation, and vertical shear. Another aspect is that as the <span class="hlt">sea</span> surface temperature drops below the <span class="hlt">air</span> temperature, the stable stratification develops in the atmospheric boundary layer. The stable atmospheric stratification suppresses sensible and latent heat <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> and reduces the net longwave irradiance from the <span class="hlt">sea</span> surface. As a result, the artificial upwelling may start increasing the OHC (though still reducing the <span class="hlt">sea</span> surface temperature). In this work, the fate of the cold water in the stratified environment with vertical shear has been studied using computational fluid dynamics (CFD) tools. A 3D large eddy simulation model is initialized with observational temperature, salinity, and current velocity data from a sample location in the Straits of Florida. A periodic boundary condition is set along the direction of the current, which allows us to simulate infinite fetch. The model results indicate that the cold water brought to the <span class="hlt">sea</span> surface by a wave-inertia pump forms a convective jet. This jet plunges into the upper ocean mixed layer and penetrates the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015PrOce.138...18D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PrOce.138...18D"><span>Nitrous oxide and methane in Atlantic and Mediterranean waters in the Strait of Gibraltar: <span class="hlt">Air-sea</span> <span class="hlt">fluxes</span> and inter-basin exchange</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>de la Paz, M.; Huertas, I. E.; Flecha, S.; Ríos, A. F.; Pérez, F. F.</p> <p>2015-11-01</p> <p>The global ocean plays an important role in the overall budget of nitrous oxide (N2O) and methane (CH4), as both gases are produced within the ocean and released to the atmosphere. However, for large parts of the open and coastal oceans there is little or no spatial data coverage for N2O and CH4. Hence, a better assessment of marine emissions estimates is necessary. As a contribution to remedying the scarcity of data on marine regions, N2O and CH4 concentrations have been determined in the Strait of Gibraltar at the ocean Fixed Time series (GIFT). During six cruises performed between July 2011 and November 2014 samples were collected at the surface and various depths in the water column, and subsequently measured using gas chromatography. From this we were able to quantify the temporal variability of the gas <span class="hlt">air-sea</span> exchange in the area and examine the vertical distribution of N2O and CH4 in Atlantic and Mediterranean waters. Results show that surface Atlantic waters are nearly in equilibrium with the atmosphere whereas deeper Mediterranean waters are oversaturated in N2O, and a gradient that gradually increases with depth was detected in the water column. Temperature was found to be the main factor responsible for the seasonal variability of N2O in the surface layer. Furthermore, although CH4 levels did not reveal any feature clearly associated with the circulation of water masses, vertical distributions showed that higher concentrations are generally observed in the Atlantic layer, and that the deeper Mediterranean waters are considerably undersaturated (by up to 50%). Even though surface waters act as a source of atmospheric N2O during certain periods, on an annual basis the net N2O <span class="hlt">flux</span> in the Strait of Gibraltar is only 0.35 ± 0.27 μmol m-2 d-1, meaning that these waters are almost in a neutral status with respect to the atmosphere. Seasonally, the region behaves as a slight sink for atmospheric CH4 in winter and as a source in spring and fall. Approximating</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007ACPD....713243N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007ACPD....713243N"><span>Eddy covariance measurements of <span class="hlt">sea</span> spray particles over the Atlantic Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Norris, S.; Brooks, I.; de Leeuw, G.; Smith, M. H.; Moeman, M.; Lingard, J.</p> <p>2007-09-01</p> <p>Most estimates of <span class="hlt">sea</span> spray aerosol source functions have used indirect means to infer the rate of production as a function of wind speed. Only recently has the technology become available to make high frequency measurements of aerosol concentration suitable for direct eddy correlation determination of the particle <span class="hlt">flux</span>. This was accomplished in this study by combining a newly developed fast aerosol particle counter with an ultrasonic anemometer which allowed for eddy covariance measurements of size-segregated particle <span class="hlt">fluxes</span>. The aerosol instrument is the Compact Lightweight Aerosol Spectrometer Probe (CLASP) - capable of measuring 8-channel size spectra for mean radii between 0.15 and 0.35 μm at 10 Hz. The first successful measurements were made during the WASFAB (Waves, <span class="hlt">Air</span> <span class="hlt">Sea</span> <span class="hlt">Fluxes</span>, Aerosol and Bubbles) field campaign in October 2005 in Duck (NC, USA). The method and results are presented and comparisons are made with recent <span class="hlt">sea</span> spray source functions from the literature.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013JGRD..118.3794P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013JGRD..118.3794P"><span>Development and evaluation of an ammonia bidirectional <span class="hlt">flux</span> parameterization for <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>Pleim, Jonathan E.; Bash, Jesse O.; Walker, John T.; Cooter, Ellen J.</p> <p>2013-05-01</p> <p>is an important contributor to particulate matter in the atmosphere and can significantly impact terrestrial and aquatic ecosystems. Surface exchange between the atmosphere and biosphere is a key part of the ammonia cycle. New modeling techniques are being developed for use in <span class="hlt">air</span> quality models that replace current ammonia emissions from fertilized crops and ammonia dry deposition with a bidirectional surface <span class="hlt">flux</span> model including linkage to a detailed biogeochemical and farm management model. Recent field studies involving surface <span class="hlt">flux</span> measurements over crops that predominate in North America have been crucial for extending earlier bidirectional <span class="hlt">flux</span> models toward more realistic treatment of NH3 <span class="hlt">fluxes</span> for croplands. Comparisons of the ammonia bidirection <span class="hlt">flux</span> algorithm to both lightly fertilized soybeans and heavily fertilized corn demonstrate that the model can capture the magnitude and dynamics of observed ammonia <span class="hlt">fluxes</span>, both net deposition and evasion, over a range of conditions with overall biases on the order of the uncertainty of the measurements. However, successful application to the field experiment in heavily fertilized corn required substantial modification of the model to include new parameterizations for in-soil diffusion resistance, ground quasi-laminar boundary layer resistance, and revised cuticular resistance that is dependent on in-canopy NH3 concentration and RH at the leaf surface. This new bidirectional <span class="hlt">flux</span> algorithm has been incorporated in an <span class="hlt">air</span> quality modeling system, which also includes an implementation of a soil nitrification model.</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/1993JGR....9810211R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1993JGR....9810211R"><span>Determination of ocean surface heat <span class="hlt">fluxes</span> by a variational method</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Roquet, H.; Planton, S.; Gaspar, P.</p> <p>1993-06-01</p> <p>A new technique of determination of the "nonsolar" heat <span class="hlt">flux</span> (sum of the latent, sensible, and net infrared <span class="hlt">fluxes</span>) at the ocean surface is proposed. It applies when oceanic advection remains weak and thus relies on a one-dimensional modeling approach. It is based on a variational data assimilation scheme using the adjoint equation formalism. This allows to take advantage of all observed data with their error estimates. Results from experiments performed with station Papa (Gulf of Alaska) and Long-Term Upper Ocean Study (LOTUS, Sargasso <span class="hlt">Sea</span>) data sets are discussed. The temperature profiles assimilation allows the one-dimensional model to reproduce correctly the temperature evolution at the surface and under the oceanic mixed layer at the two sites. The retrieved <span class="hlt">fluxes</span> are compared to the <span class="hlt">fluxes</span> calculated through classical empirical formulae. The diurnal dependence of the <span class="hlt">fluxes</span> at the LOTUS site is particularly investigated. The results are also compared with those obtained using a simpler technique based on an iterative shooting method and allowing the assimilation of the only <span class="hlt">sea</span> surface temperature. This second comparison reveals that the variability of the retrieved <span class="hlt">fluxes</span> is damped when temperature in the inner ocean are assimilated. This is the case for the diurnal cycle at the LOTUS mooring. When the available current data at this site are assimilated, the diurnal variability of the retrieved <span class="hlt">fluxes</span> is further decreased. This points out a model discrepancy in the representation of mixing processes associated to internal wave activity. The remaining part of the diurnal cycle is significant and could be due to a direct effect of <span class="hlt">air-sea</span> temperature difference.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20010099433','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20010099433"><span>A Numerical Study of Tropical <span class="hlt">Sea-Air</span> Interactions Using a Cloud Resolving Model Coupled with an Ocean Mixed-Layer Model</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Shie, Chung-Lin; Tao, Wei-Kuo; Johnson, Dan; Simpson, Joanne; Li, Xiaofan; Sui, Chung-Hsiung; Einaudi, Franco (Technical Monitor)</p> <p>2001-01-01</p> <p>Coupling a cloud resolving model (CRM) with an ocean mixed layer (OML) model can provide a powerful tool for better understanding impacts of atmospheric precipitation on <span class="hlt">sea</span> surface temperature (SST) and salinity. The objective of this study is twofold. First, by using the three dimensional (3-D) CRM-simulated (the Goddard Cumulus Ensemble model, GCE) diabatic source terms, radiation (longwave and shortwave), surface <span class="hlt">fluxes</span> (sensible and latent heat, and wind stress), and precipitation as input for the OML model, the respective impact of individual component on upper ocean heat and salt budgets are investigated. Secondly, a two-way <span class="hlt">air-sea</span> interaction between tropical atmospheric climates (involving atmospheric radiative-convective processes) and upper ocean boundary layer is also examined using a coupled two dimensional (2-D) GCE and OML model. Results presented here, however, only involve the first aspect. Complete results will be presented at the conference.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ClDy...49.1341P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ClDy...49.1341P"><span>Linking atmospheric synoptic transport, cloud phase, surface energy <span class="hlt">fluxes</span>, and <span class="hlt">sea</span>-ice growth: observations of midwinter SHEBA conditions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Persson, P. Ola G.; Shupe, Matthew D.; Perovich, Don; Solomon, Amy</p> <p>2017-08-01</p> <p>Observations from the Surface Heat Budget of the Arctic Ocean (SHEBA) project are used to describe a sequence of events linking midwinter long-range advection of atmospheric heat and moisture into the Arctic Basin, formation of supercooled liquid water clouds, enhancement of net surface energy <span class="hlt">fluxes</span> through increased downwelling longwave radiation, and reduction in near-surface conductive heat <span class="hlt">flux</span> loss due to a warming of the surface, thereby leading to a reduction in <span class="hlt">sea</span>-ice bottom growth. The analyses provide details of two events during Jan. 1-12, 1998, one entering the Arctic through Fram Strait and the other from northeast Siberia; winter statistics extend the results. Both deep, precipitating frontal clouds and post-frontal stratocumulus clouds impact the surface radiation and energy budget. Cloud liquid water, occurring preferentially in stratocumulus clouds extending into the base of the inversion, provides the strongest impact on surface radiation and hence modulates the surface forcing, as found previously. The observations suggest a minimum water vapor threshold, likely case dependent, for producing liquid water clouds. Through responses to the radiative forcing and surface warming, this cloud liquid water also modulates the turbulent and conductive heat <span class="hlt">fluxes</span>, and produces a thermal wave penetrating into the <span class="hlt">sea</span> ice. About 20-33 % of the observed variations of bottom ice growth can be directly linked to variations in surface conductive heat <span class="hlt">flux</span>, with retarded ice growth occurring several days after these moisture plumes reduce the surface conductive heat <span class="hlt">flux</span>. This sequence of events modulate pack-ice wintertime environmental conditions and total ice growth, and has implications for the annual <span class="hlt">sea</span>-ice evolution, especially for the current conditions of extensive thinner ice.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017DSRI..122...72S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017DSRI..122...72S"><span>Deep-<span class="hlt">sea</span> <span class="hlt">fluxes</span> of barium and lithogenic trace elements in the subtropical northeast Atlantic</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stern, Judith; Dellwig, Olaf; Waniek, Joanna J.</p> <p>2017-04-01</p> <p>Total particle <span class="hlt">flux</span>, Barium and lithogenic trace element <span class="hlt">fluxes</span> were measured at the mooring Kiel 276 (33°N, 22°W) in the deep-<span class="hlt">sea</span> of the subtropical Northeast Atlantic. The particulate material was collected between 2002 and 2008 with a sediment trap in 2000 m depth and analyzed with ICP-OES/-MS to determine its geochemical composition. The particle <span class="hlt">flux</span> is controlled by primary production, lithogenic particle inputs via atmospheric transport and the migration of the Azores Front. We used refractory trace elements (eg. Ti, Zr, and the rare earth elements) to demonstrate the changes in <span class="hlt">flux</span> and composition of the material due to lithogenic inputs. Shortly after periods of high dust load and enhanced primary production an increase in lithogenic trace element <span class="hlt">fluxes</span> occurred. Especially the formation of aggregates with biogenic matter seems to have a major impact on the downwards transport of lithogenic particles. The observation of particulate Ba is of great interest since it is known as a proxy for past and present primary production. Ba <span class="hlt">fluxes</span> ranging between 0.02 mg m-2 d-1 and 1.21 mg m-2 d-1 with biogenic proportions up to 97%. The <span class="hlt">fluxes</span> of particulate Barium in the water column are mainly attributed to the strength of primary production.</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 CO2 uptake. This system may be either a sink or a source for atmospheric CO2. Understanding the sources and sinks as a result of biological and physical controls for <span class="hlt">air-sea</span> carbon dioxide <span class="hlt">fluxes</span> in coastal waters may substantially alter the current view of the global carbon budget for unique terrestrial and ocean regions such as the GOT. GOT is a semi-enclosed Mediterranean basin situated in the northern part of Adriatic <span class="hlt">Sea</span>. It is one of the most productive regions in the Mediterranean and is affected by extreme fresh river input, phytoplankton blooms, and large changes of <span class="hlt">air-sea</span> exchange during Bora high wind events. The unique combination of these environmental processes and relatively small size of the area makes the region an excellent study site for investigations of <span class="hlt">air-sea</span> interaction, and changes in biology and carbon chemistry. However, there is a dearth of current data or information from the region. Here we present the first measurements of <span class="hlt">air</span> and water CO2 <span class="hlt">flux</span> in the GOT. The aqueous CO2 was measured at the Coastal Oceanographic buoy Piran, Slovenia using the SAMI CO2 sensor during spring and late summer and fall 2007. CO2 measurements were combined with hydrological and biological observations to evaluate the processes that control carbon cycling in the region.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA617029','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA617029"><span>Radar Remote Sensing of Ice and <span class="hlt">Sea</span> State and <span class="hlt">Air-Sea</span> Interaction in the Marginal Ice Zone</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2014-09-30</p> <p>1 DISTRIBUTION STATEMENT A. Approved for public release; distribution is unlimited. Radar Remote Sensing of Ice and <span class="hlt">Sea</span> State and <span class="hlt">Air-Sea</span>...Interaction in the Marginal Ice Zone Hans C. Graber RSMAS – Department of Ocean Sciences Center for Southeastern Tropical Advanced Remote Sensing...scattering and attenuation process of ocean waves interacting with ice . A nautical X-band radar on a vessel dedicated to science would be used to follow the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/638276-sea-ice-polar-climate-ncar-csm','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/638276-sea-ice-polar-climate-ncar-csm"><span><span class="hlt">Sea</span> ice and polar climate in the NCAR CSM</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>Weatherly, J.W.; Briegleb, B.P.; Large, W.G.</p> <p></p> <p>The Climate System Model (CSM) consists of atmosphere, ocean, land, and <span class="hlt">sea</span>-ice components linked by a <span class="hlt">flux</span> coupler, which computes <span class="hlt">fluxes</span> of energy and momentum between components. The <span class="hlt">sea</span>-ice component consists of a thermodynamic formulation for ice, snow, and leads within the ice pack, and ice dynamics using the cavitating-fluid ice rheology, which allows for the compressive strength of ice but ignores shear viscosity. The results of a 300-yr climate simulation are presented, with the focus on <span class="hlt">sea</span> ice and the atmospheric forcing over <span class="hlt">sea</span> ice in the polar regions. The atmospheric model results are compared to analyses from themore » European Centre for Medium-Range Weather Forecasts and other observational sources. The <span class="hlt">sea</span>-ice concentrations and velocities are compared to satellite observational data. The atmospheric <span class="hlt">sea</span> level pressure (SLP) in CSM exhibits a high in the central Arctic displaced poleward from the observed Beaufort high. The Southern Hemisphere SLP over <span class="hlt">sea</span> ice is generally 5 mb lower than observed. <span class="hlt">Air</span> temperatures over <span class="hlt">sea</span> ice in both hemispheres exhibit cold biases of 2--4 K. The precipitation-minus-evaporation fields in both hemispheres are greatly improved over those from earlier versions of the atmospheric GCM.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70134376','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70134376"><span>Decadal and annual changes in biogenic opal and carbonate <span class="hlt">fluxes</span> to the deep Sargasso <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Deuser, W.G.; Jickells, T.D.; Commeau, Judith A.</p> <p>1995-01-01</p> <p>Analyses of samples from a 14-year series of sediment-trap deployments in the deep Sargasso <span class="hlt">Sea</span> reveal a significant trend in the ratio of the sinking <span class="hlt">fluxes</span> of biogenic calcium carbonate and silica. Although there are pronounced seasonal cycles for both <span class="hlt">flux</span> components, the overall opal/CaCO3 ratio changed by 50% from 1978 to 1991 (largely due to a decrease of opal <span class="hlt">flux</span>), while total <span class="hlt">flux</span> had no significant trend. These results suggest that plankton communities respond rapidly to subtle climate change, such as is evident in regional variations of wind speed, precipitation, wintertime ventilation and midwater temperatures. If the trends we observe in the makeup of sinking particulate matter occur on a large scale, they may in turn modify climate by modulating ocean-atmosphere CO2 exchange and albedo over the ocean.</p> </li> <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 (2,600 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, PM2.5 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, PM2.5 and PM10, respectively at the lower free atmosphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..1511209H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..1511209H"><span>Seasonal cycle of oceanic mixed layer and upper-ocean heat <span class="hlt">fluxes</span> in the Mediterranean <span class="hlt">Sea</span> from in-situ observations.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Houpert, Loïc; Testor, Pierre; Durrieu de Madron, Xavier; Estournel, Claude; D'Ortenzio, Fabrizio</p> <p>2013-04-01</p> <p>Heat <span class="hlt">fluxes</span> across the ocean-atmosphere interface play a crucial role in the upper turbulent mixing. The depth reached by this turbulent mixing is indicated by an homogenization of seawater properties in the surface layer, and is defined as the Mixed Layer Depth (MLD). The thickness of the mixed layer determines also the heat content of the layer that directly interacts with the atmosphere. The seasonal variability of these <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> is crucial in the calculation of heat budget. An improvement in the estimate of these <span class="hlt">fluxes</span> is needed for a better understanding of the Mediterranean ocean circulation and climate, in particular in Regional Climate Models. There are few estimations of surface heat <span class="hlt">fluxes</span> based on oceanic observations in the Mediterranean, and none of them are based on mixed layer observations. So, we proposed here new estimations of these upper-ocean heat <span class="hlt">fluxes</span> based on mixed layer. We present high resolution Mediterranean climatology (0.5°) of the mean MLD based on a comprehensive collection of temperature profiles of last 43 years (1969-2012). The database includes more than 150,000 profiles, merging CTD, XBT, ARGO Profiling floats, and gliders observations. This dataset is first used to describe the seasonal cycle of the mixed layer depth on the whole Mediterranean on a monthly climatological basis. Our analysis discriminates several regions with coherent behaviors, in particular the deep water formation sites, characterized by significant differences in the winter mixing intensity. Heat storage rates (HSR) were calculated as the time rate of change of the heat content integrated from the surface down to a specific depth that is defined as the MLD plus an integration constant. Monthly climatology of net heat <span class="hlt">flux</span> (NHF) from ERA-Interim reanalysis was balanced by the 1°x1° resolution heat storage rate climatology. Local heat budget balance and seasonal variability in the horizontal heat <span class="hlt">flux</span> are then discussed by taking into account</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016cosp...41E1726S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016cosp...41E1726S"><span>Impact of winter cooling on the northern part of the Black <span class="hlt">Sea</span>.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Savchenko, Anatolii</p> <p>2016-07-01</p> <p>Climate change in the future may have a negative impact on many countries due to the increasing surface temperature and <span class="hlt">sea</span> level rise. Probably, unprecedented largest positive trend of surface temperature, which observed since the mid XX century, has associated with increasing human activities around the world. Moreover, this warming will continue in this century, and at the end of the XXI century will be 2 - 5 ºC. Thus, investigation and monitoring of current climate are very important and necessary tasks. Regional model data (downscaling) and satellite data are used, because of underdeveloped network of meteorological stations in the northern part of the Black <span class="hlt">Sea</span> region. Experiment of downscaling was carried out for the Black <span class="hlt">Sea</span> region with a high spatial resolution of 0.22° x 0.22° for 1958 - 2007(daily values). For the Black <span class="hlt">Sea</span> were also used satellite data of <span class="hlt">sea</span> surface temperature(SST) from MyOcean-2 Project, which CNR(Rome) has reprocessed Pathfinder V5.2 (PFV52) AVHRR data over period 1981 - 2012 with daily gap-free maps (L4) at the original PFV52 resolution at 0.04° x 0.04°. Correlation between satellite SST and surface temperature from regional model climate are amounted 0,99. Thus, surface temperature of model and satellite data for the Black <span class="hlt">Sea</span> is much correlated between yourself. The following integral characteristics of the Black <span class="hlt">Sea</span> are referred to the area of <span class="hlt">sea</span> limited by the 44 - 47º N and 28 - 34º E. Maximum cooling of the north-western part of the Black <span class="hlt">Sea</span> in winter is occurs after invasion of cold <span class="hlt">air</span> across the northern border of the basin. In addition, this water area is also interesting in the presence of her huge oil and gas reserves, as well as the construction of liquefied gas (crude oil) terminals. The maximum values of total heat <span class="hlt">flux</span> (sensible + latent heat <span class="hlt">fluxes</span>= Q) corresponding to the minimum values of SST are observed during the periods of the negative phase of the NAO. Besides, <span class="hlt">fluxes</span> with extreme days P (Q) = 95</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014OcMod..84...51L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014OcMod..84...51L"><span>Processes driving <span class="hlt">sea</span> ice variability in the Bering <span class="hlt">Sea</span> in an eddying ocean/<span class="hlt">sea</span> ice model: Mean seasonal cycle</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Linghan; McClean, Julie L.; Miller, Arthur J.; Eisenman, Ian; Hendershott, Myrl C.; Papadopoulos, Caroline A.</p> <p>2014-12-01</p> <p>The seasonal cycle of <span class="hlt">sea</span> ice variability in the Bering <span class="hlt">Sea</span>, together with the thermodynamic and dynamic processes that control it, are examined in a fine resolution (1/10°) global coupled ocean/<span class="hlt">sea</span>-ice model configured in the Community Earth System Model (CESM) framework. The ocean/<span class="hlt">sea</span>-ice model consists of the Los Alamos National Laboratory Parallel Ocean Program (POP) and the Los Alamos <span class="hlt">Sea</span> Ice Model (CICE). The model was forced with time-varying reanalysis atmospheric forcing for the time period 1970-1989. This study focuses on the time period 1980-1989. The simulated seasonal-mean fields of <span class="hlt">sea</span> ice concentration strongly resemble satellite-derived observations, as quantified by root-mean-square errors and pattern correlation coefficients. The <span class="hlt">sea</span> ice energy budget reveals that the seasonal thermodynamic ice volume changes are dominated by the surface energy <span class="hlt">flux</span> between the atmosphere and the ice in the northern region and by heat <span class="hlt">flux</span> from the ocean to the ice along the southern ice edge, especially on the western side. The <span class="hlt">sea</span> ice force balance analysis shows that <span class="hlt">sea</span> ice motion is largely associated with wind stress. The force due to divergence of the internal ice stress tensor is large near the land boundaries in the north, and it is small in the central and southern ice-covered region. During winter, which dominates the annual mean, it is found that the simulated <span class="hlt">sea</span> ice was mainly formed in the northern Bering <span class="hlt">Sea</span>, with the maximum ice growth rate occurring along the coast due to cold <span class="hlt">air</span> from northerly winds and ice motion away from the coast. South of St Lawrence Island, winds drive the model <span class="hlt">sea</span> ice southwestward from the north to the southwestern part of the ice-covered region. Along the ice edge in the western Bering <span class="hlt">Sea</span>, model <span class="hlt">sea</span> ice is melted by warm ocean water, which is carried by the simulated Bering Slope Current flowing to the northwest, resulting in the S-shaped asymmetric ice edge. In spring and fall, similar thermodynamic and dynamic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20060039424&hterms=holt+winters&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dholt%2Bwinters','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060039424&hterms=holt+winters&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dholt%2Bwinters"><span>Fall Freeze-up of <span class="hlt">Sea</span> Ice in the Beaufort-Chukchi <span class="hlt">Seas</span> Using ERS-1 SAR and Buoy Data</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Holt, B.; Winebrenner, B.; D., Nelson E.</p> <p>1993-01-01</p> <p>The lowering of <span class="hlt">air</span> temperatures below freezing in the fall indicates the end of summer melt and the onset of steady <span class="hlt">sea</span> ice growth. The thickness and condition of ice that remains at the end of summer has ramifications for the thickness that that ice will attain at the end of the following winter. This period also designates a shifting of key <span class="hlt">fluxes</span> from upper ocean freshening from ice melt to increased salinity from brine extraction during ice growth. This transitional period has been examined in the Beaufort and Chukchi <span class="hlt">Seas</span> using ERS-1 SAR imagery and <span class="hlt">air</span> temperatures from drifting buoys during 1991 and 1992. The SAR imagery is used to examine the condition and types of ice present in this period. Much of the surface melt water has drained off at this time. <span class="hlt">Air</span> temperatures from drifting buoys coincident in time and within 100 km radius of the SAR imagery have been obtained...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70039994','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70039994"><span>Coupled atmosphere-ocean-wave simulations of a storm event over the Gulf of Lion and Balearic <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Renault, Lionel; Chiggiato, Jacopo; Warner, John C.; Gomez, Marta; Vizoso, Guillermo; Tintore, Joaquin</p> <p>2012-01-01</p> <p>The coastal areas of the North-Western Mediterranean <span class="hlt">Sea</span> are one of the most challenging places for ocean forecasting. This region is exposed to severe storms events that are of short duration. During these events, significant <span class="hlt">air-sea</span> interactions, strong winds and large <span class="hlt">sea</span>-state can have catastrophic consequences in the coastal areas. To investigate these <span class="hlt">air-sea</span> interactions and the oceanic response to such events, we implemented the Coupled Ocean-Atmosphere-Wave-Sediment Transport Modeling System simulating a severe storm in the Mediterranean <span class="hlt">Sea</span> that occurred in May 2010. During this event, wind speed reached up to 25 m.s-1 inducing significant <span class="hlt">sea</span> surface cooling (up to 2°C) over the Gulf of Lion (GoL) and along the storm track, and generating surface waves with a significant height of 6 m. It is shown that the event, associated with a cyclogenesis between the Balearic Islands and the GoL, is relatively well reproduced by the coupled system. A surface heat budget analysis showed that ocean vertical mixing was a major contributor to the cooling tendency along the storm track and in the GoL where turbulent heat <span class="hlt">fluxes</span> also played an important role. Sensitivity experiments on the ocean-atmosphere coupling suggested that the coupled system is sensitive to the momentum <span class="hlt">flux</span> parameterization as well as <span class="hlt">air-sea</span> and <span class="hlt">air</span>-wave coupling. Comparisons with available atmospheric and oceanic observations showed that the use of the fully coupled system provides the most skillful simulation, illustrating the benefit of using a fully coupled ocean-atmosphere-wave model for the assessment of these storm events.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19920016738','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19920016738"><span>NASA Wallops Flight Facility <span class="hlt">Air-Sea</span> Interaction Research Facility</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Long, Steven R.</p> <p>1992-01-01</p> <p>This publication serves as an introduction to the <span class="hlt">Air-Sea</span> Interaction Research Facility at NASA/GSFC/Wallops Flight Facility. The purpose of this publication is to provide background information on the research facility itself, including capabilities, available instrumentation, the types of experiments already done, ongoing experiments, and future plans.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140011835','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140011835"><span>Teleconnections, Midlatitude Cyclones and Aegean <span class="hlt">Sea</span> Turbulent Heat <span class="hlt">Flux</span> Variability on Daily Through Decadal Time Scales</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Romanski, Joy; Romanou, Anastasia; Bauer, Michael; Tselioudis, George</p> <p>2013-01-01</p> <p>We analyze daily wintertime cyclone variability in the central and eastern Mediterranean during 1958-2001, and identify four distinct cyclone states, corresponding to the presence or absence of cyclones in each basin. Each cyclone state is associated with wind flows that induce characteristic patterns of cooling via turbulent (sensible and latent) heat <span class="hlt">fluxes</span> in the eastern Mediterranean basin and Aegean <span class="hlt">Sea</span>. The relative frequency of occurrence of each state determines the heat loss from the Aegean <span class="hlt">Sea</span> during that winter, with largest heat losses occurring when there is a storm in the eastern but not central Mediterranean (eNOTc), and the smallest occurring when there is a storm in the central but not eastern Mediterranean (cNOTe). Time series of daily cyclone states for each winter allow us to infer Aegean <span class="hlt">Sea</span> cooling for winters prior to 1985, the earliest year for which we have daily heat <span class="hlt">flux</span> observations. We show that cyclone states conducive to Aegean <span class="hlt">Sea</span> convection occurred in 1991/1992 and 1992/1993, the winters during which deep water formation was observed in the Aegean <span class="hlt">Sea</span>, and also during the mid-1970s and the winters of 1963/1964 and 1968/1969. We find that the eNOTc cyclone state is anticorrelated with the North Atlantic Oscillation (NAO) prior to 1977/1978. After 1977/1978, the cNOTe state is anticorrelated with both the NAO and the North Caspian Pattern (NCP), showing that the area of influence of large scale atmospheric teleconnections on regional cyclone activity shifted from the eastern to the central Mediterranean during the late 1970s. A trend toward more frequent occurrence of the positive phase of the NAO produced less frequent cNOTe states since the late 1970s, increasing the number of days with strong cooling of the Aegean <span class="hlt">Sea</span> surface waters.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25377990','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25377990"><span>A <span class="hlt">flux</span>-gradient system for simultaneous measurement of the CH4, CO2, and H2O <span class="hlt">fluxes</span> at a lake-<span class="hlt">air</span> interface.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Xiao, Wei; Liu, Shoudong; Li, Hanchao; Xiao, Qitao; Wang, Wei; Hu, Zhenghua; Hu, Cheng; Gao, Yunqiu; Shen, Jing; Zhao, Xiaoyan; Zhang, Mi; Lee, Xuhui</p> <p>2014-12-16</p> <p>Inland lakes play important roles in water and greenhouse gas cycling in the environment. This study aims to test the performance of a <span class="hlt">flux</span>-gradient system for simultaneous measurement of the <span class="hlt">fluxes</span> of water vapor, CO2, and CH4 at a lake-<span class="hlt">air</span> interface. The concentration gradients over the water surface were measured with an analyzer based on the wavelength-scanned cavity ring-down spectroscopy technology, and the eddy diffusivity was measured with a sonic anemometer. Results of a zero-gradient test indicate a <span class="hlt">flux</span> measurement precision of 4.8 W m(-2) for water vapor, 0.010 mg m(-2) s(-1) for CO2, and 0.029 μg m(-2) s(-1) for CH4. During the 620 day measurement period, 97%, 69%, and 67% of H2O, CO2, and CH4 hourly <span class="hlt">fluxes</span> were higher in magnitude than the measurement precision, which confirms that the <span class="hlt">flux</span>-gradient system had adequate precision for the measurement of the lake-<span class="hlt">air</span> exchanges. This study illustrates four strengths of the <span class="hlt">flux</span>-gradient method: (1) the ability to simultaneously measure the <span class="hlt">flux</span> of H2O, CO2, and CH4; (2) negligibly small density corrections; (3) the ability to resolve small CH4 gradient and <span class="hlt">flux</span>; and (4) continuous and noninvasive operation. The annual mean CH4 <span class="hlt">flux</span> (1.8 g CH4 m(-2) year(-1)) at this hypereutrophic lake was close to the median value for inland lakes in the world (1.6 g CH4 m(-2) year(-1)). The system has adequate precision for CH4 <span class="hlt">flux</span> for broad applications but requires further improvement to resolve small CO2 <span class="hlt">flux</span> in many lakes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JGRC..119.7725L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JGRC..119.7725L"><span>Exploiting satellite earth observation to quantify current global oceanic DMS <span class="hlt">flux</span> and its future climate sensitivity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Land, P. E.; Shutler, J. D.; Bell, T. G.; Yang, M.</p> <p>2014-11-01</p> <p>We used coincident Envisat RA2 and AATSR temperature and wind speed data from 2008/2009 to calculate the global net <span class="hlt">sea-air</span> <span class="hlt">flux</span> of dimethyl sulfide (DMS), which we estimate to be 19.6 Tg S a-1. Our monthly <span class="hlt">flux</span> calculations are compared to open ocean eddy correlation measurements of DMS <span class="hlt">flux</span> from 10 recent cruises, with a root mean square difference of 3.1 μmol m-2 day-1. In a sensitivity analysis, we varied temperature, salinity, surface wind speed, and aqueous DMS concentration, using fixed global changes as well as CMIP5 model output. The range of DMS <span class="hlt">flux</span> in future climate scenarios is discussed. The CMIP5 model predicts a reduction in surface wind speed and we estimate that this will decrease the global annual <span class="hlt">sea-air</span> <span class="hlt">flux</span> of DMS by 22% over 25 years. Concurrent changes in temperature, salinity, and DMS concentration increase the global <span class="hlt">flux</span> by much smaller amounts. The net effect of all CMIP5 modelled 25 year predictions was a 19% reduction in global DMS <span class="hlt">flux</span>. 25 year DMS concentration changes had significant regional effects, some positive (Southern Ocean, North Atlantic, Northwest Pacific) and some negative (isolated regions along the Equator and in the Indian Ocean). Using satellite-detected coverage of coccolithophore blooms, our estimate of their contribution to North Atlantic DMS emissions suggests that the coccolithophores contribute only a small percentage of the North Atlantic annual <span class="hlt">flux</span> estimate, but may be more important in the summertime and in the northeast Atlantic.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ClDy..tmp....5S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ClDy..tmp....5S"><span>Mediterranean <span class="hlt">sea</span> water budget long-term trend inferred from salinity observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Skliris, N.; Zika, J. D.; Herold, L.; Josey, S. A.; Marsh, R.</p> <p>2018-01-01</p> <p>Changes in the Mediterranean water cycle since 1950 are investigated using salinity and reanalysis based <span class="hlt">air-sea</span> freshwater <span class="hlt">flux</span> datasets. Salinity observations indicate a strong basin-scale multi-decadal salinification, particularly in the intermediate and deep layers. Evaporation, precipitation and river runoff variations are all shown to contribute to a very strong increase in net evaporation of order 20-30%. While large temporal uncertainties and discrepancies are found between E-P multi-decadal trend patterns in the reanalysis datasets, a more robust and spatially coherent structure of multi-decadal change is obtained for the salinity field. Salinity change implies an increase in net evaporation of 8 to 12% over 1950-2010, which is considerably lower than that suggested by <span class="hlt">air-sea</span> freshwater <span class="hlt">flux</span> products, but still largely exceeding estimates of global water cycle amplification. A new method based on water mass transformation theory is used to link changes in net evaporation over the Mediterranean <span class="hlt">Sea</span> with changes in the volumetric distribution of salinity. The water mass transformation distribution in salinity coordinates suggests that the Mediterranean basin salinification is driven by changes in the regional water cycle rather than changes in salt transports at the straits.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160013232','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160013232"><span>US Navy Submarine <span class="hlt">Sea</span> Trial of the NASA <span class="hlt">Air</span> Quality Monitor</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Limero, Thomas; Wallace, William T.; Manney, Joshua A.; Mudgett, Paul D.</p> <p>2017-01-01</p> <p>For the past four years, the <span class="hlt">Air</span> Quality Monitor (AQM) has been the operational instrument for measuring trace volatile organic compounds on the International Space Station (ISS). The key components of the AQM are the inlet preconcentrator, the gas chromatograph (GC), and the differential mobility spectrometer. Most importantly, the AQM operates at atmospheric pressure and uses <span class="hlt">air</span> as the GC carrier gas, which translates into a small reliable instrument. Onboard ISS there are two AQMs, with different GC columns that detect and quantify 22 compounds. The AQM data contributes valuable information to the assessment of <span class="hlt">air</span> quality aboard ISS for each crew increment. The U.S. Navy is looking to update its submarine <span class="hlt">air</span> monitoring suite of instruments, and the success of the AQM on ISS has led to a jointly planned submarine <span class="hlt">sea</span> trial of a NASA AQM. In addition to the AQM, the Navy is also interested in the Multi-Gas Monitor (MGM), which was successfully flown on ISS as a technology demonstration to measure major constituent gases (oxygen, carbon dioxide, water vapor, and ammonia). A separate paper will present the MGM <span class="hlt">sea</span> trial results. A prototype AQM, which is virtually identical to the operational AQM, has been readied for the <span class="hlt">sea</span> trial. Only one AQM will be deployed during the <span class="hlt">sea</span> trial, but it is sufficient to detect the compounds of interest to the Navy for the purposes of this trial. A significant benefit of the AQM is that runs can be scripted for pre-determined intervals and no crew intervention is required. The data from the <span class="hlt">sea</span> trial will be compared to archival samples collected prior to and during the trial period. This paper will give a brief overview of the AQM technology and protocols for the submarine trial. After a quick review of the AQM preparation, the main focus of the paper will be on the results of the submarine trial. Of particular interest will be the comparison of the contaminants found in the ISS and submarine atmospheres, as both represent</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_15 --> <div id="page_16" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="301"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOS.B24A0316C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOS.B24A0316C"><span>Effects of Variable Oxygen Concentrations on the Sinking <span class="hlt">Fluxes</span> and Composition of Organic Matter 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>Cisternas-Novoa, C.; Le Moigne, F. A. C.; Roa, J.; Wagner, H.; Engel, A.</p> <p>2016-02-01</p> <p>The downward <span class="hlt">flux</span> of organic matter (OM) from the euphotic zone is critical to understand the biogeochemistry cycles in the ocean. Local changes in stratification, nutrient inputs, community structure and oxygen concentrations potentially affect the magnitude of OM <span class="hlt">flux</span>. The Baltic <span class="hlt">Sea</span> is a unique environment with strong natural gradients of primary productivity, nutrients and O2 concentrations. The genuine effect of oxygen minimum deficiency on the fate of sinking OM and the efficiency of the biologic carbon pump has yet to be clarified. Previous work suggested that under oxygen deficiency, nitrogen rich amino acids are preferentially utilized causing nitrogen loss from the water column (van Mooy et al., 2002, Kalvelage et al 2013). Here, we investigate how different oxygen conditions and surface productivity affect sinking particles <span class="hlt">flux</span> and particles composition in the central Baltic <span class="hlt">Sea</span>. Sinking OM was collected in June 2015 using surface-tethered free-drifting traps in the Gotland and Landsort deeps. Sinking particles were collected for a period of 48 and 24 hours at four depths from below the mixed layer and down to hypoxic deep waters (40, 60, 110 and 180 m). <span class="hlt">Fluxes</span> of POC, PON, POP and amino acids were estimated. We will discuss the effect of low oxygen levels on the biological carbon pump associated with <span class="hlt">fluxes</span> of OM and sinking particles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ACP....18.4361K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ACP....18.4361K"><span>High-resolution measurements of elemental mercury in surface water for an improved quantitative understanding of the Baltic <span class="hlt">Sea</span> as a source of atmospheric mercury</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kuss, Joachim; Krüger, Siegfried; Ruickoldt, Johann; Wlost, Klaus-Peter</p> <p>2018-03-01</p> <p>Marginal <span class="hlt">seas</span> are directly subjected to anthropogenic and natural influences from land in addition to receiving inputs from the atmosphere and open ocean. Together these lead to pronounced gradients and strong dynamic changes. However, in the case of mercury emissions from these <span class="hlt">seas</span>, estimates often fail to adequately account for the spatial and temporal variability of the elemental mercury concentration in surface water (Hg0wat). In this study, a method to measure Hg0wat at high resolution was devised and subsequently validated. The better-resolved Hg0wat dataset, consisting of about one measurement per nautical mile, yielded insight into the <span class="hlt">sea</span>'s small-scale variability and thus improved the quantification of the <span class="hlt">sea</span>'s Hg0 emission. This is important because global marine Hg0 emissions constitute a major source of atmospheric mercury. Research campaigns in the Baltic <span class="hlt">Sea</span> were carried out between 2011 and 2015 during which Hg0 both in surface water and in ambient <span class="hlt">air</span> were measured. For the former, two types of equilibrators were used. A membrane equilibrator enabled continuous equilibration and a bottle equilibrator assured that equilibrium was reached for validation. The measurements were combined with data obtained in the Baltic <span class="hlt">Sea</span> in 2006 from a bottle equilibrator only. The Hg0 <span class="hlt">sea-air</span> <span class="hlt">flux</span> was newly calculated with the combined dataset based on current knowledge of the Hg0 Schmidt number, Henry's law constant, and a widely used gas exchange transfer velocity parameterization. By using a newly developed pump-CTD with increased pumping capability in the Hg0 equilibrator measurements, Hg0wat could also be characterized in deeper water layers. A process study carried out near the Swedish island Øland in August 2015 showed that the upwelling of Hg0-depleted water contributed to Hg0 emissions of the Baltic <span class="hlt">Sea</span>. However, a delay of a few days after contact between the upwelled water and light was apparently necessary before the biotic and abiotic transformations</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150000330','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150000330"><span>Sensitivity of Simulated Global Ocean Carbon <span class="hlt">Flux</span> Estimates to Forcing by Reanalysis Products</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gregg, Watson W.; Casey, Nancy W.; Rousseaux, Cecile S.</p> <p>2015-01-01</p> <p>Reanalysis products from MERRA, NCEP2, NCEP1, and ECMWF were used to force an established ocean biogeochemical model to estimate <span class="hlt">air-sea</span> carbon <span class="hlt">fluxes</span> (FCO2) and partial pressure of carbon dioxide (pCO2) in the global oceans. Global <span class="hlt">air-sea</span> carbon <span class="hlt">fluxes</span> and pCO2 were relatively insensitive to the choice of forcing reanalysis. All global FCO2 estimates from the model forced by the four different reanalyses were within 20% of in situ estimates (MERRA and NCEP1 were within 7%), and all models exhibited statistically significant positive correlations with in situ estimates across the 12 major oceanographic basins. Global pCO2 estimates were within 1% of in situ estimates with ECMWF being the outlier at 0.6%. Basin correlations were similar to FCO2. There were, however, substantial departures among basin estimates from the different reanalysis forcings. The high latitudes and tropics had the largest ranges in estimated <span class="hlt">fluxes</span> among the reanalyses. Regional pCO2 differences among the reanalysis forcings were muted relative to the FCO2 results. No individual reanalysis was uniformly better or worse in the major oceanographic basins. The results provide information on the characterization of uncertainty in ocean carbon models due to choice of reanalysis forcing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/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 (35.2° 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(2)/day) than in the North Pacific (-241 ± 158 pg/m(2)/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/2017AGUFM.A12F..05I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A12F..05I"><span>Measurements and Modeling of Turbulent <span class="hlt">Fluxes</span> during Persistent Cold <span class="hlt">Air</span> Pool Events in Salt Lake Valley, Utah</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ivey, C. E.; Sun, X.; Holmes, H.</p> <p>2017-12-01</p> <p>Land surface processes are important in meteorology and climate research since they control the partitioning of surface energy and water exchange at the earth's surface. The surface layer is coupled to the planetary boundary layer (PBL) by surface <span class="hlt">fluxes</span>, which serve as sinks or sources of energy, moisture, momentum, and atmospheric pollutants. Quantifying the surface heat and momentum <span class="hlt">fluxes</span> at the land-atmosphere interface, especially for different surface land cover types, is important because they can further influence the atmospheric dynamics, vertical mixing, and transport processes that impact local, regional, and global climate. A cold <span class="hlt">air</span> pool (CAP) forms when a topographic depression (i.e., valley) fills with cold <span class="hlt">air</span>, where the <span class="hlt">air</span> in the stagnant layer is colder than the <span class="hlt">air</span> aloft. Insufficient surface heating, which is not able to sufficiently erode the temperature inversion that forms during the nighttime stable boundary layer, can lead to the formation of persistent CAPs during wintertime. These persistent CAPs can last for days, or even weeks, and are associated with increased <span class="hlt">air</span> pollution concentrations. Thus, realistic simulations of the land-atmosphere exchange are meaningful to achieve improved predictions of the accumulation, transport, and dispersion of <span class="hlt">air</span> pollution concentrations. The focus of this presentation is on observations and modeling results using turbulence data collected in Salt Lake Valley, Utah during the 2010-2011 wintertime Persistent Cold <span class="hlt">Air</span> Pool Study (PCAPS). Turbulent <span class="hlt">fluxes</span> and the surface energy balance over seven land use types are quantified. The urban site has an energy balance ratio (EBR) larger than one (1.276). Negative Bowen ratio (-0.070) is found at the cropland site. In addition to turbulence observations, half-hourly WRF simulated net radiation, latent heat, sensible heat, ground heat <span class="hlt">fluxes</span> during one persistent CAP event are evaluated using the PCAPS observations. The results show that sensible and latent</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> Transfer (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> Transfer (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 2- 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/1995SPIE.2586..241X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1995SPIE.2586..241X"><span>Heat <span class="hlt">flux</span> exchange estimation by using ATSR SST data in TOGA area</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xue, Yong; Lawrence, Sean P.; Llewellyn-Jones, David T.</p> <p>1995-12-01</p> <p>The study of phenomena such as ENSO requires consideration of the dynamics and thermodynamics of the coupled ocean-atmosphere system. The dynamic and thermal properties of the atmosphere and ocean are directly affected by <span class="hlt">air-sea</span> transfers of <span class="hlt">fluxes</span> of momentum, heat and moisture. In this paper, we present results of turbulent heat <span class="hlt">fluxes</span> calculated by using two years (1992 and 1993) monthly average TOGA data and ATSR SST data in TOGA area. A comparison with published results indicates good qualitative agreement. Also, we compared the results of heat <span class="hlt">flux</span> exchange by using ATSR SST data and by using the TOGA bucket SST data. The ATSR SST data set has been shown to be useful in helping to estimate the large space scale heat <span class="hlt">flux</span> exchange.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JOL....36..139W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JOL....36..139W"><span>Rates and <span class="hlt">fluxes</span> of centennial-scale carbon storage in the fine-grained sediments from the central South Yellow <span class="hlt">Sea</span> and Min-Zhe belt, 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>Wang, Jianghai; Xiao, Xi; Zhou, Qianzhi; Xu, Xiaoming; Zhang, Chenxi; Liu, Jinzhong; Yuan, Dongliang</p> <p>2018-01-01</p> <p>The global carbon cycle has played a key role in mitigating global warming and climate change. Long-term natural and anthropogenic processes influence the composition, sources, burial rates, and <span class="hlt">fluxes</span> of carbon in sediments on the continental shelf of China. In this study, the rates, <span class="hlt">fluxes</span>, and amounts of carbon storage at the centennial scale were estimated and demonstrated using the case study of three fine-grained sediment cores from the central South Yellow <span class="hlt">Sea</span> area (SYSA) and Min-Zhe belt (MZB), East China <span class="hlt">Sea</span>. Based on the high-resolution temporal sequences of total carbon (TC) and total organic carbon (TOC) contents, we reconstructed the annual variations of historical marine carbon storage, and explored the influence of terrestrial and marine sources on carbon burial at the centennial scale. The estimated TC storage over 100 years was 1.18×108 t in the SYSA and 1.45×109 t in the MZB. The corrected TOC storage <span class="hlt">fluxes</span> at the centennial scale ranged from 17 to 28 t/(km2·a)in the SYSA and from 56 to 148 t/(km2·a) in the MZB. The decrease of terrestrial materials and the increase of marine primary production suggest that the TOC buried in the sediments in the SYSA and MZB was mainly derived from the marine autogenetic source. In the MZB, two depletion events occurred in TC and TOC storage from 1985 to 1987 and 2003 to 2006, which were coeval with the water impoundment in the Gezhouba and Three Gorges dams, respectively. The high-resolution records of the carbon storage rates and <span class="hlt">fluxes</span> in the SYSA and MZB reflect the synchronous responses to human activities and provide an important reference for assessing the carbon sequestration capacity of the marginal <span class="hlt">seas</span> of China.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20000070471','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20000070471"><span>Modeling Studies of the Effects of Winds and Heat <span class="hlt">Flux</span> on the Tropical Oceans</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Seager, R.</p> <p>1999-01-01</p> <p>Over a decade ago, funding from this NASA grant supported the development of the Cane-Zebiak ENSO prediction model which remains in use to this day. It also supported our work developing schemes for modeling the <span class="hlt">air-sea</span> heat <span class="hlt">flux</span> in ocean models used for studying climate variability. We introduced a succession of simple boundary layer models that allow the <span class="hlt">fluxes</span> to be computed internally in the model and avoid the need to specify the atmospheric thermodynamic state. These models have now reached a level of generality that allows modeling of the global, rather than just tropical, ocean, including <span class="hlt">sea</span> ice cover. The most recent versions of these boundary layer models have been widely distributed around the world and are in use by many ocean modeling groups.</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 CO2 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 14CO2 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 CO2. Using the most complete database of dissolved inorganic radiocarbon, DI14C, available to date and a suite of ocean general circulation models in an inverse mode we recalculate the ocean inventory of bomb-produced DI14C in the global ocean and confirm that there is a 25% decrease from previous estimates using older DI14C data sets. Additionally, we find a 33% lower globally averaged gas transfer velocity for CO2 compared to previous estimates (Wanninkhof, 1992) using the NCEP/NCAR Reanalysis 1 1954-2000 where the global mean winds are 6.9 m s-1. Unlike some earlier ocean radiocarbon studies, the implied gas transfer velocity finally closes the gap between small-scale deliberate tracer studies and global-scale estimates. Additionally, the total inventory of bomb-produced radiocarbon in the ocean is now in agreement with global budgets based on radiocarbon measurements made in the stratosphere and troposphere. Using the implied relationship between wind speed and gas transfer velocity ks = 0.27<u102>(Sc/660)-0.5 and standard partial pressure difference climatology of CO2 we obtain an net <span class="hlt">air-sea</span> <span class="hlt">flux</span> estimate of 1.3 ± 0.5 PgCyr-1 for 1995. After accounting for the carbon transferred from rivers to the deep ocean, our estimate of oceanic uptake (1.8 ± 0.5 PgCyr-1) compares well with estimates based on ocean inventories, ocean transport inversions using ocean concentration data, and model simulations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ClDy..tmp.2362W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ClDy..tmp.2362W"><span>Potential regulation on the climatic effect of Tibetan Plateau heating by tropical <span class="hlt">air-sea</span> coupling in regional models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Ziqian; Duan, Anmin; Yang, Song</p> <p>2018-05-01</p> <p>Based on the conventional weather research and forecasting (WRF) model and the <span class="hlt">air-sea</span> coupled mode WRF-OMLM, we investigate the potential regulation on the climatic effect of Tibetan Plateau (TP) heating by the <span class="hlt">air-sea</span> coupling over the tropical Indian Ocean and western Pacific. Results indicate that the TP heating significantly enhances the southwesterly monsoon circulation over the northern Indian Ocean and the South Asia subcontinent. The intensified southwesterly wind cools the <span class="hlt">sea</span> surface mainly through the wind-evaporation-SST (<span class="hlt">sea</span> surface temperature) feedback. Cold SST anomaly then weakens monsoon convective activity, especially that over the Bay of Bengal, and less water vapor is thus transported into the TP along its southern slope from the tropical oceans. As a result, summer precipitation decreases over the TP, which further weakens the TP local heat source. Finally, the changed TP heating continues to influence the summer monsoon precipitation and atmospheric circulation. To a certain extent, the <span class="hlt">air-sea</span> coupling over the adjacent oceans may weaken the effect of TP heating on the mean climate in summer. It is also implied that considerations of <span class="hlt">air-sea</span> interaction are necessary in future simulation studies of the TP heating effect.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/21137331-detection-air-gap-eccentricity-broken-rotor-bar-conditions-squirrel-cage-induction-motor-using-radial-flux-sensor','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/21137331-detection-air-gap-eccentricity-broken-rotor-bar-conditions-squirrel-cage-induction-motor-using-radial-flux-sensor"><span>Detection of <span class="hlt">air</span>-gap eccentricity and broken-rotor bar conditions in a squirrel-cage induction motor using the radial <span class="hlt">flux</span> sensor</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>Hwang, Don-Ha; Woo, Byung-Chul; Sun, Jong-Ho</p> <p>2008-04-01</p> <p>A new method for detecting eccentricity and broken rotor bar conditions in a squirrel-cage induction motor is proposed. <span class="hlt">Air</span>-gap <span class="hlt">flux</span> variation analysis is done using search coils, which are inserted at stator slots. Using this method, the leakage <span class="hlt">flux</span> in radial direction can be directly detected. Using finite element method, the <span class="hlt">air</span>-gap <span class="hlt">flux</span> variation is accurately modeled and analyzed. From the results of the simulation, a motor under normal condition shows maximum magnetic <span class="hlt">flux</span> density of 1.3 T. On the other hand, the eccentric <span class="hlt">air</span>-gap condition displays about 1.1 T at 60 deg. and 1.6 T at 240 deg. Amore » difference of <span class="hlt">flux</span> density is 0.5 T in the abnormal condition, whereas no difference is detected in the normal motor. In the broken rotor bar conditions, the <span class="hlt">flux</span> densities at 65 deg. and 155 deg. are about 0.4 T and 0.8 T, respectively. These simulation results are coincided with those of experiment. Consequently, the measurement of the magnetic <span class="hlt">flux</span> at <span class="hlt">air</span> gap is one of effective ways to discriminate the faulted conditions of the eccentricity and broken rotor bars.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017DSRI..122...17M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017DSRI..122...17M"><span>The <span class="hlt">air-sea</span> exchange of mercury in the low latitude Pacific and Atlantic Oceans</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mason, Robert P.; Hammerschmidt, Chad R.; Lamborg, Carl H.; Bowman, Katlin L.; Swarr, Gretchen J.; Shelley, Rachel U.</p> <p>2017-04-01</p> <p><span class="hlt">Air-sea</span> exchange is an important component of the global mercury (Hg) cycle as it mediates the rate of increase in ocean Hg, and therefore the rate of change in levels of methylmercury (MeHg), the most toxic and bioaccumulative form of Hg in seafood and the driver of human health concerns. Gas evasion of elemental Hg (Hg0) from the ocean is an important sink for ocean Hg with previous studies suggesting that evasion is not uniform across ocean basins. To understand further the factors controlling Hg0 evasion, and its relationship to atmospheric Hg deposition, we made measurements of dissolved Hg0 (DHg0) in surface waters, along with measurements of Hg in precipitation and on aerosols, and Hg0 in marine <span class="hlt">air</span>, during two GEOTRACES cruises; GP16 in the equatorial South Pacific and GA03 in the North Atlantic. We contrast the concentrations and estimated evasion <span class="hlt">fluxes</span> of Hg0 during these cruises, and the factors influencing this exchange. Concentrations of DHg0 and <span class="hlt">fluxes</span> were lower during the GP16 cruise than during the GA03 cruise, and likely reflect the lower atmospheric deposition in the South Pacific. An examination of Hg/Al ratios for aerosols from the cruises suggests that they were anthropogenically-enriched relative to crustal material, although to a lesser degree for the South Pacific than the aerosols over the North Atlantic. Both regions appear to be net sources of Hg0 to the atmosphere (evasion>deposition) and the reasons for this are discussed. Overall, the studies reported here provide further clarification on the factors controlling evasion of Hg0 from the ocean surface, and the role of anthropogenic inputs in influencing ocean Hg concentrations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://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 CO2 <span class="hlt">flux</span> in a mangrove-dominated estuary</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Ho, David T.; Ferrón, Sara; Engel, Victor C.; Larsen, Laurel G.; Barr, Jordan G.</p> <p>2014-01-01</p> <p>Mangrove forests are highly productive ecosystems, but the fate of mangrove-derived carbon remains uncertain. Part of that uncertainty stems from the fact that gas transfer velocities in mangrove-surrounded waters are not well determined, leading to uncertainty in <span class="hlt">air</span>-water CO2 <span class="hlt">fluxes</span>. Two SF6 tracer release experiments were conducted to determine gas transfer velocities (k(600) = 8.3 ± 0.4 and 8.1 ± 0.6 cm h−1), along with simultaneous measurements of pCO2 to determine the <span class="hlt">air</span>-water CO2 <span class="hlt">fluxes</span> from Shark River, Florida (232.11 ± 23.69 and 171.13 ± 20.28 mmol C m−2 d−1), an estuary within the largest contiguous mangrove forest in North America. The gas transfer velocity results are consistent with turbulent kinetic energy dissipation measurements, indicating a higher rate of turbulence and gas exchange than predicted by commonly used wind speed/gas exchange parameterizations. The results have important implications for carbon <span class="hlt">fluxes</span> in mangrove ecosystems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSPC11B..05V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSPC11B..05V"><span>The ocean mixed layer under Southern Ocean <span class="hlt">sea</span>-ice: seasonal cycle and forcing.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Violaine, P.; Sallee, J. B.; Schmidtko, S.; Roquet, F.; Charrassin, J. B.</p> <p>2016-02-01</p> <p>The mixed-layer at the surface of the ocean is the gateway for all exchanges between <span class="hlt">air</span> and <span class="hlt">sea</span>. A vast area of the Southern Ocean is however seasonally capped by <span class="hlt">sea</span>-ice, which alters this gateway and the characteristic the ocean mixed-layer. The interaction between the ocean mixed-layer and <span class="hlt">sea</span>-ice plays a key role for water-mass formation and circulation, carbon cycle, <span class="hlt">sea</span>-ice dynamics, and ultimately for the climate as a whole. However, the structure and characteristics of the mixed layer, as well as the processes responsible for its evolution, are poorly understood due to the lack of in-situ observations and measurements. We urgently need to better understand the forcing and the characteristics of the ocean mixed-layer under <span class="hlt">sea</span>-ice if we are to understand and predict the world's climate. In this study, we combine a range of distinct sources of observation to overcome this lack in our understanding of the Polar Regions. Working on Elephant Seal-derived data as well as ship-based observations and Argo float data, we describe the seasonal cycle of the characteristics and stability of the ocean mixed layer over the entire Southern Ocean (South of 40°S), and specifically under <span class="hlt">sea</span>-ice. Mixed-layer budgets of heat and freshwater are used to investigate the main forcings of the mixed-layer seasonal cycle. The seasonal variability of <span class="hlt">sea</span> surface salinity and temperature are primarily driven by surface processes, dominated by <span class="hlt">sea</span>-ice freshwater <span class="hlt">flux</span> for the salt budget, and by <span class="hlt">air-sea</span> <span class="hlt">flux</span> for the heat budget. Ekman advection, vertical diffusivity and vertical entrainment play only secondary role.Our results suggest that changes in regional <span class="hlt">sea</span>-ice distribution or <span class="hlt">sea</span>-ice seasonal cycle duration, as currently observed, would widely affect the buoyancy budget of the underlying mixed-layer, and impacts large-scale water-mass formation and transformation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.8460M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.8460M"><span>Revisiting the estimation of the North <span class="hlt">Sea</span> <span class="hlt">air-sea</span> <span class="hlt">flux</span> of CO2 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 pCO2 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 CO2 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 coastDat2 (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 coastDat2 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 coastDat2 values are larger than the ERA-40 values. The comparison of North <span class="hlt">Sea</span> wide CO2 uptake yields 1.3 for ERA-40 and 1.8 mol CO2 m-2 a-1 for coastDat2 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/2060/19970036015','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 (2) 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('http://adsabs.harvard.edu/abs/2015AGUFM.H44F..07L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.H44F..07L"><span>GRACE Mass <span class="hlt">Flux</span> Measurements of Inland and Marginal <span class="hlt">Seas</span> from Mascons: Analysis and Validation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Loomis, B.; Luthcke, S. B.; Sabaka, T. J.</p> <p>2015-12-01</p> <p>The latest GRACE time-variable gravity mascon solution from the NASA Goddard Space Flight Center (GSFC) applies an optimized set of models and constraints towards the direct measurement of 1-arc-degree global mass <span class="hlt">flux</span> parameters each month. Separate mascon spatial constraint regions have been defined for the largest inland and marginal <span class="hlt">seas</span>: Mediterranean <span class="hlt">Sea</span>, Black <span class="hlt">Sea</span>, Caspian <span class="hlt">Sea</span>, Red <span class="hlt">Sea</span>, and Hudson Bay. The mascon estimation approach, when applied with well-designed constraints, minimizes signal leakage across regional boundaries and eliminates the need for post-processing strategies. These post-processing techniques (e.g. smoothed averaging kernels) are necessary for computing regional mass change from the unconstrained spherical harmonics provided by the GRACE project to reduce the effect of noisy high degree and order terms, but introduce signal leakage into and out of the considered region. These mass signals are also difficult to obtain from altimetry measurements due to the comparatively sparse temperature and salinity data in these regions, which is needed to compute and remove the steric component of <span class="hlt">sea</span> level variations. We provide new GSFC mascon measurements of these inland and marginal <span class="hlt">seas</span> and compare to results obtained from kernel-averaged spherical harmonic solutions and steric-corrected altimetry measurements. The relative accuracy of the various solutions is determined by incorporating their output into the set of forward models applied in our processing of the GRACE Level-1B data and analyzing the effect on the inter-satellite range-rate residuals, where a reduction in residuals is a direct validation of improved solution quality.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS23B2024M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS23B2024M"><span>Coastal Land <span class="hlt">Air</span> <span class="hlt">Sea</span> Interaction: "the" beach towers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>MacMahan, J. H.; Koscinski, J. S.; Ortiz-Suslow, D. G.; Haus, B. K.; Thornton, E. B.</p> <p>2016-12-01</p> <p>As part of the Coastal Land <span class="hlt">Air</span> <span class="hlt">Sea</span> Interaction (CLASI) experiment, an alongshore array of 6-m high towers instrumented with ultrasonic 3D anemometers and temperature-relative humidity sensors were deployed at five sandy beaches near the high-tide line in Monterey Bay, CA, in May-June 2016. A cross-shore array of towers was also deployed from within the active surfzone to the toe of the dune at one beach. In addition, waves and ocean temperature were obtained along the 10m isobath for each beach. The dissipative surfzone was O(80m) wide. The wave energy varies among the beaches owing to sheltering and refraction by the Monterey Canyon and headlands. The tides are semi-diurnal mixed, meso-tidal with a maximum tidal range of 2m. This results in a variable beach width from the tower to the tidal line. Footprint analysis for estimating the source region for the turbulent momentum <span class="hlt">fluxes</span>, suggests that the observations represent three scenarios described as primarily ocean, mixed beach and ocean, and primarily beach. The direct-estimate of the atmospheric stability by the sonic anemometer suggest that all of the beaches are mostly unstable except for a few occurrences in the evening during low wind conditions. The onshore neutral drag coefficient (Cd) estimated at 10m heights is 3-5 times larger than open ocean estimates. Minimal variability was found in Cd based on the footprint analysis. Beach-specific spatial variability in Cd was found related to atmospheric stability and wave energy.</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-2 were produced by the Grid-<span class="hlt">SEAs</span> (on average 5.9 ± 0.5 W m-2) 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-2, 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-2 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> </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/2018BGeo...15.3331N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018BGeo...15.3331N"><span>CO2 <span class="hlt">flux</span> over young and snow-covered Arctic pack ice in winter and spring</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nomura, Daiki; Granskog, Mats A.; Fransson, Agneta; Chierici, Melissa; Silyakova, Anna; Ohshima, Kay I.; Cohen, Lana; Delille, Bruno; Hudson, Stephen R.; Dieckmann, Gerhard S.</p> <p>2018-06-01</p> <p>Rare CO2 <span class="hlt">flux</span> measurements from Arctic pack ice show that two types of ice contribute to the release of CO2 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 CO2 <span class="hlt">flux</span> from <span class="hlt">sea</span> ice decreased due to the presence of the snow, the snow surface is still a CO2 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 CO2 <span class="hlt">fluxes</span> an order of magnitude higher than those in snow-covered older ice (+1.0 ± 0.6 mmol C m-2 day-1 for young ice and +0.2 ± 0.2 mmol C m-2 day-1 for older ice).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017DSRI..126...62L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017DSRI..126...62L"><span>Long-term variation of mesopelagic biogenic <span class="hlt">flux</span> in the central South China <span class="hlt">Sea</span>: Impact of monsoonal seasonality and mesoscale eddy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Hongliang; Wiesner, Martin G.; Chen, Jianfang; Ling, Zheng; Zhang, Jingjing; Ran, Lihua</p> <p>2017-08-01</p> <p>The East Asian Monsoon and mesoscale eddies are known to regulate primary production in South China <span class="hlt">Sea</span> (SCS), the largest tropical marginal <span class="hlt">sea</span>; however, their contributions to the deep biogenic <span class="hlt">flux</span> are yet to be quantified. Based on 7-year time series sediment trap observations at the depth of 1200 m in the central SCS, we used the monthly average sinking biogenic <span class="hlt">fluxes</span> to evaluate the impact of the monsoon and mesoscale cyclonic eddies on biogenic <span class="hlt">fluxes</span> in combination with remote sensing physical parameters. The monthly average particulate organic carbon (POC) and opal <span class="hlt">fluxes</span>, ranging from 3.0 to 5.2 and 14.8-34.9 mg m-2 d-1, respectively, were higher during the northeastern monsoon period. This corresponded to the deeper mixed layer depth and higher net primary production in this area, due to nutrient replenishment from the subsurface induced by monsoon transition and surface cooling. In contrast, lower POC and opal <span class="hlt">fluxes</span> occurred during well-stratified inter-monsoon periods. In addition, CaCO3 <span class="hlt">flux</span> (23.6-37.0 mg m-2 d-1) exhibited less seasonality and was assumed to originate from foraminifera. In terms of the long-term record, the combined effect of cyclonic eddies and mixing in the upper ocean could effectively regulate the temporal variation in the biogenic <span class="hlt">flux</span>. In particular, the opal and POC <span class="hlt">fluxes</span> in cyclonic eddies were 116% and 41% higher on average, respectively, than those during the non-cyclonic eddy period. Since the cyclonic eddies mainly occurred during the northeastern monsoon period, their contributions to biogenic <span class="hlt">flux</span> via diatom blooms might overlap the regular winter <span class="hlt">flux</span> peak, which could make the biological carbon pump more efficient at CO2 sequestration during this period thus amplifying the impact of seasonal transition.</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> Transfer 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 2 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://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 transfer from the ocean side of the <span class="hlt">air-sea</span> interface, and we discuss it in terms of the drag coefficient. For winds between 20 and 48 meters per second, this coefficient initially increases and peaks at winds of about 32 meters per second before decreasing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSHE44A1477Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSHE44A1477Z"><span>Estimation of Nutrients <span class="hlt">Flux</span> of Water-sediment Interface in the Chukchi <span class="hlt">Sea</span>, 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>Zhang, H.</p> <p>2016-02-01</p> <p>Nutrients regeneration in pore water is one of the important ways to supply nutrients of upper water column in the shelf. The pore water in sediment of the central Chukchi <span class="hlt">Sea</span> continental shelf, showed a typical benthic distribution of nutrients at water-sediment interface, in where physical and bioturbation was weak. The nutrient samples in multi-tubular short column sediment and water column were obtained from the Forth Chinese National Arctic Research Expedition, to measure the nutrient concentrations of pore water, overlying water and water column. The results show that, the typical distribution can be separated into three layers. The first layer is the exponential increasing layer (I), in which the concentrations of nutrients increased rapidly with depth. Then was the steady layer (II), the sediment demineralization was equal to the nutrient transference and nutrients' concentrations were substantially constant at this stage. The third layer was a slowly descending layer (III), in which NO3- and PO43- were reduced by bacteria and lost oxygen ions due to organic materials degradation depleting oxygen. By a two-layer mode and the Fick's first law of diffusion, diffusive <span class="hlt">fluxes</span> of silicate, phosphate and nitrate in R06 station of the Chukchi <span class="hlt">Sea</span> shelf can be calculated, and the <span class="hlt">fluxes</span> were 1.660 mmol/(m2 · d), 0.008 mmol/(m2 · d) and 0.117 mmol/(m2 · d), respectively. The diffusive <span class="hlt">fluxes</span> of silicate for CC1, R06, C07 and S23 stations were 3.101 mmol/(m2 · d), 1.660 mmol/(m2 · d), 1.307 mmol/(m2 · d) and mmol/(m2 · d), respectively, which show obvious distribution characteristics with latitude. Distribution of N * in the pore water suggested that a strong denitrification process in sedimentary environment of the Chukchi <span class="hlt">Sea</span> shelf, which is an important sink for nitrate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017TCry...11.1333L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017TCry...11.1333L"><span>Sonar gas <span class="hlt">flux</span> estimation by bubble insonification: application to methane bubble <span class="hlt">flux</span> from seep areas in the outer Laptev <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>Leifer, Ira; Chernykh, Denis; Shakhova, Natalia; Semiletov, Igor</p> <p>2017-06-01</p> <p>Sonar surveys provide an effective mechanism for mapping seabed methane <span class="hlt">flux</span> emissions, with Arctic submerged permafrost seepage having great potential to significantly affect climate. We created in situ engineered bubble plumes from 40 m depth with <span class="hlt">fluxes</span> spanning 0.019 to 1.1 L s-1 to derive the in situ calibration curve (Q(σ)). These nonlinear curves related <span class="hlt">flux</span> (Q) to sonar return (σ) for a multibeam echosounder (MBES) and a single-beam echosounder (SBES) for a range of depths. The analysis demonstrated significant multiple bubble acoustic scattering - precluding the use of a theoretical approach to derive Q(σ) from the product of the bubble σ(r) and the bubble size distribution where r is bubble radius. The bubble plume σ occurrence probability distribution function (Ψ(σ)) with respect to Q found Ψ(σ) for weak σ well described by a power law that likely correlated with small-bubble dispersion and was strongly depth dependent. Ψ(σ) for strong σ was largely depth independent, consistent with bubble plume behavior where large bubbles in a plume remain in a focused core. Ψ(σ) was bimodal for all but the weakest plumes. Q(σ) was applied to sonar observations of natural arctic Laptev <span class="hlt">Sea</span> seepage after accounting for volumetric change with numerical bubble plume simulations. Simulations addressed different depths and gases between calibration and seep plumes. Total mass <span class="hlt">fluxes</span> (Qm) were 5.56, 42.73, and 4.88 mmol s-1 for MBES data with good to reasonable agreement (4-37 %) between the SBES and MBES systems. The seepage <span class="hlt">flux</span> occurrence probability distribution function (Ψ(Q)) was bimodal, with weak Ψ(Q) in each seep area well described by a power law, suggesting primarily minor bubble plumes. The seepage-mapped spatial patterns suggested subsurface geologic control attributing methane <span class="hlt">fluxes</span> to the current state of subsea permafrost.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18...26B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18...26B"><span>Calibration of Ocean Forcing with satellite <span class="hlt">Flux</span> Estimates (COFFEE)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Barron, Charlie; Jan, Dastugue; Jackie, May; Rowley, Clark; Smith, Scott; Spence, Peter; Gremes-Cordero, Silvia</p> <p>2016-04-01</p> <p>Predicting the evolution of ocean temperature in regional ocean models depends on estimates of surface heat <span class="hlt">fluxes</span> and upper-ocean processes over the forecast period. Within the COFFEE project (Calibration of Ocean Forcing with satellite <span class="hlt">Flux</span> Estimates, real-time satellite observations are used to estimate shortwave, longwave, sensible, and latent <span class="hlt">air-sea</span> heat <span class="hlt">flux</span> corrections to a background estimate from the prior day's regional or global model forecast. These satellite-corrected <span class="hlt">fluxes</span> are used to prepare a corrected ocean hindcast and to estimate <span class="hlt">flux</span> error covariances to project the heat <span class="hlt">flux</span> corrections for a 3-5 day forecast. In this way, satellite remote sensing is applied to not only inform the initial ocean state but also to mitigate errors in surface heat <span class="hlt">flux</span> and model representations affecting the distribution of heat in the upper ocean. While traditional assimilation of <span class="hlt">sea</span> surface temperature (SST) observations re-centers ocean models at the start of each forecast cycle, COFFEE endeavors to appropriately partition and reduce among various surface heat <span class="hlt">flux</span> and ocean dynamics sources. A suite of experiments in the southern California Current demonstrates a range of COFFEE capabilities, showing the impact on forecast error relative to a baseline three-dimensional variational (3DVAR) assimilation using operational global or regional atmospheric forcing. Experiment cases combine different levels of <span class="hlt">flux</span> calibration with assimilation alternatives. The cases use the original <span class="hlt">fluxes</span>, apply full satellite corrections during the forecast period, or extend hindcast corrections into the forecast period. Assimilation is either baseline 3DVAR or standard strong-constraint 4DVAR, with work proceeding to add a 4DVAR expanded to include a weak constraint treatment of the surface <span class="hlt">flux</span> errors. Covariance of <span class="hlt">flux</span> errors is estimated from the recent time series of forecast and calibrated <span class="hlt">flux</span> terms. While the California Current examples are shown, the approach is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009DSRII..56..964F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009DSRII..56..964F"><span>Nitrous oxide and methane in the Atlantic Ocean between 50°N and 52°S: Latitudinal distribution and <span class="hlt">sea-to-air</span> <span class="hlt">flux</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Forster, Grant; Upstill-Goddard, Rob C.; Gist, Niki; Robinson, Carol; Uher, Gunther; Woodward, E. Malcolm S.</p> <p>2009-07-01</p> <p>We discuss nitrous oxide (N 2O) and methane (CH 4) distributions in 49 vertical profiles covering the upper ˜300 m of the water column along two ˜13,500 km transects between ˜50°N and ˜52°S during the Atlantic Meridional Transect (AMT) programme (AMT cruises 12 and 13). Vertical N 2O profiles were amenable to analysis on the basis of common features coincident with Longhurst provinces. In contrast, CH 4 showed no such pattern. The most striking feature of the latitudinal depth distributions was a well-defined "plume" of exceptionally high N 2O concentrations coincident with very low levels of CH 4, located between ˜23.5°N and ˜23.5°S; this feature reflects the upwelling of deep waters containing N 2O derived from nitrification, as identified by an analysis of N 2O, apparent oxygen utilization (AOU) and NO 3-, and presumably depleted in CH 4 by bacterial oxidation. <span class="hlt">Sea-to-air</span> emissions <span class="hlt">fluxes</span> for a region equivalent to ˜42% of the Atlantic Ocean surface area were in the range 0.40-0.68 Tg N 2O yr -1 and 0.81-1.43 Tg CH 4 yr -1. Based on contemporary estimates of the global ocean source strengths of atmospheric N 2O and CH 4, the Atlantic Ocean could account for ˜6-15% and 4-13%, respectively, of these source totals. Given that the Atlantic Ocean accounts for around 20% of the global ocean surface, on unit area basis it appears that the Atlantic may be a slightly weaker source of atmospheric N 2O than other ocean regions but it could make a somewhat larger contribution to marine-derived atmospheric CH 4 than previously thought.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=280765&keyword=pollution+AND+soils&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50','EPA-EIMS'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=280765&keyword=pollution+AND+soils&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50"><span>"Advances in Linked <span class="hlt">Air</span> Quality, Farm Management and Biogeochemistry Models to Address Bidrectional Ammonia <span class="hlt">Flux</span> in CMAQ"</span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p>Recent increases in anthropogenic inputs of nitrogen to <span class="hlt">air</span>, land and water media pose a growing threat to human health and ecosystems. Modeling of <span class="hlt">air</span>-surface N <span class="hlt">flux</span> is one area in need of improvement. Implementation of a linked <span class="hlt">air</span> quality and cropland management system is de...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=305692&Lab=NERL&keyword=Springer%2C+E&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50','EPA-EIMS'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=305692&Lab=NERL&keyword=Springer%2C+E&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50"><span>Advances in Linked <span class="hlt">Air</span> Quality, Farm Management and Biogeochemistry Models to Address Bidirectional Ammonia <span class="hlt">Flux</span> in CMAQ</span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p>Recent increases in anthropogenic inputs of nitrogen to <span class="hlt">air</span>, land and water media pose a growing threat to human health and ecosystems. Modeling of <span class="hlt">air</span>-surface N <span class="hlt">flux</span> is one area in need of improvement. Implementation of a linked <span class="hlt">air</span> quality and cropland management system is de...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS21B1971J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS21B1971J"><span>High-resolution modeling of local <span class="hlt">air-sea</span> interaction within the Marine Continent using COAMPS</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jensen, T. G.; Chen, S.; Flatau, M. K.; Smith, T.; Rydbeck, A.</p> <p>2016-12-01</p> <p>The Maritime Continent (MC) is a region of intense deep atmospheric convection that serves as an important source of forcing for the Hadley and Walker circulations. The convective activity in the MC region spans multiple scales from local mesoscales to regional scales, and impacts equatorial wave propagation, coupled <span class="hlt">air-sea</span> interaction and intra seasonal oscillations. The complex distribution of islands, shallow <span class="hlt">seas</span> with fairly small heat storage and deep <span class="hlt">seas</span> with large heat capacity is challenging to model. Diurnal convection over land-<span class="hlt">sea</span> is part of a land-<span class="hlt">sea</span> breeze system on a small scale, and is highly influenced by large variations in orography over land and marginal <span class="hlt">seas</span>. Daytime solar insolation, run-off from the Archipelago and nighttime rainfall tends to stabilize the water column, while mixing by tidal currents and locally forced winds promote vertical mixing. The runoff from land and rivers and high net precipitation result in fresh water lenses that enhance vertical stability in the water column and help maintain high SST. We use the fully coupled atmosphere-ocean-wave version of the Coupled Ocean-Atmosphere Mesoscale Prediction System (COAMPS) developed at NRL with resolution of a few kilometers to investigate the <span class="hlt">air-sea</span> interaction associated with the land-<span class="hlt">sea</span> breeze system in the MC under active and inactive phases of the Madden-Julian Oscillation. The high resolution enables simulation of strong SST gradients associated with local upwelling in deeper waters and strong salinity gradients near rivers and from heavy precipitation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16604693','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16604693"><span>Skyshine analysis using energy and angular dependent dose-contribution <span class="hlt">fluxes</span> obtained from <span class="hlt">air</span>-over-ground adjoint calculation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Uematsu, Mikio; Kurosawa, Masahiko</p> <p>2005-01-01</p> <p>A generalised and convenient skyshine dose analysis method has been developed based on forward-adjoint folding technique. In the method, the <span class="hlt">air</span> penetration data were prepared by performing an adjoint DOT3.5 calculation with cylindrical <span class="hlt">air</span>-over-ground geometry having an adjoint point source (importance of unit <span class="hlt">flux</span> to dose rate at detection point) in the centre. The accuracy of the present method was certified by comparing with DOT3.5 forward calculation. The adjoint <span class="hlt">flux</span> data can be used as generalised radiation skyshine data for all sorts of nuclear facilities. Moreover, the present method supplies plenty of energy-angular dependent contribution <span class="hlt">flux</span> data, which will be useful for detailed shielding design of facilities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20020001784','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20020001784"><span>A 7.5-Year Dataset of SSM/I-Derived Surface Turbulent <span class="hlt">Fluxes</span> Over Global Oceans</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chou, Shu-Hsien; Shie, Chung-Lin; Atlas, Robert M.; Adizzone, Joe; Nelkin, Eric; Starr, David OC. (Technical Monitor)</p> <p>2001-01-01</p> <p>The global <span class="hlt">air-sea</span> turbulent <span class="hlt">fluxes</span> are needed for driving ocean models and validating coupled ocean-atmosphere global models. A method was developed to retrieve surface <span class="hlt">air</span> humidity from the radiances measured by the Special Sensor Microwave/Imager (SSM/I) Using both SSM/I-retrieved surface wind and <span class="hlt">air</span> humidity, they computed daily turbulent <span class="hlt">fluxes</span> over global oceans with a stability-dependent bulk scheme. Based on this method, we have produced Version 1 of Goddard Satellite-Based Surface Turbulent <span class="hlt">Fluxes</span> (GSSTF) dataset from the SSM/I data and other data. It provides daily- and monthly-mean surface turbulent <span class="hlt">fluxes</span> and some relevant parameters over global oceans for individual F8, F10, and F11 satellites covering the period July 1987-December 1994. It also provides 1988-94 annual- and monthly-mean climatologies of the same variables, using only F8 and F1 1 satellite data. It has a spatial resolution of 2.0 degrees x 2.5 degrees lat-long and is archived at the NASA/GSFC DAAC. The purpose of this paper is to present an updated assessment of the GSSTF 1.0 dataset.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1996ApOpt..35.4905M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1996ApOpt..35.4905M"><span>Diode laser-based <span class="hlt">air</span> mass <span class="hlt">flux</span> sensor for subsonic aeropropulsion inlets</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Miller, Michael F.; Kessler, William J.; Allen, Mark G.</p> <p>1996-08-01</p> <p>An optical <span class="hlt">air</span> mass <span class="hlt">flux</span> sensor based on a compact, room-temperature diode laser in a fiber-coupled delivery system has been tested on a full-scale gas turbine engine. The sensor is based on simultaneous measurements of O 2 density and Doppler-shifted velocity along a line of sight across the inlet duct. Extensive tests spanning engine power levels from idle to full afterburner demonstrate accuracy and precision of the order of 1 2 of full scale in density, velocity, and mass <span class="hlt">flux</span>. The precision-limited velocity at atmospheric pressure was as low as 40 cm s. Multiple data-reduction procedures are quantitatively compared to suggest optimal strategies for flight sensor packages.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140013026','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140013026"><span>Connections Between the Spring Breakup of the Southern Hemisphere Polar Vortex, Stationary Waves, and <span class="hlt">Air-sea</span> Roughness</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Garfinkel, Chaim I.; Oman, Luke David; Barnes, Elizabeth A.; Waugh, Darryn W.; Hurwitz, Margaret H.; Molod, Andrea M.</p> <p>2013-01-01</p> <p>A robust connection between the drag on surface-layer winds and the stratospheric circulation is demonstrated in NASA's Goddard Earth Observing System Chemistry-Climate Model (GEOSCCM). Specifically, an updated parameterization of roughness at the <span class="hlt">air-sea</span> interface, in which surface roughness is increased for moderate wind speeds (4ms to 20ms), leads to a decrease in model biases in Southern Hemispheric ozone, polar cap temperature, stationary wave heat <span class="hlt">flux</span>, and springtime vortex breakup. A dynamical mechanism is proposed whereby increased surface roughness leads to improved stationary waves. Increased surface roughness leads to anomalous eddy momentum <span class="hlt">flux</span> convergence primarily in the Indian Ocean sector (where eddies are strongest climatologically) in September and October. The localization of the eddy momentum <span class="hlt">flux</span> convergence anomaly in the Indian Ocean sector leads to a zonally asymmetric reduction in zonal wind and, by geostrophy, to a wavenumber-1 stationary wave pattern. This tropospheric stationary wave pattern leads to enhanced upwards wave activity entering the stratosphere. The net effect is an improved Southern Hemisphere vortex: the vortex breaks up earlier in spring (i.e., the spring late-breakup bias is partially ameliorated) yet is no weaker in mid-winter. More than half of the stratospheric biases appear to be related to the surface wind speed biases. As many other chemistry climate models use a similar scheme for their surface layer momentum exchange and have similar biases in the stratosphere, we expect that results from GEOSCCM may be relevant for other climate models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.7421R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.7421R"><span>Carbon <span class="hlt">fluxes</span> in the Arabian <span class="hlt">Sea</span>: Export versus recycling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rixen, Tim; Gaye, Birgit; Ramaswamy, Venkitasubramani</p> <p>2016-04-01</p> <p>The organic carbon pump strongly influences the exchange of carbon between the ocean and the atmosphere. It is known that it responds to global change but the magnitude and the direction of change are still unpredictable. Sediment trap experiments carried out at various sites in the Arabian <span class="hlt">Sea</span> between 1986 and 1998 have shown differences in the functioning of the organic carbon pump (OCP). An OCP driven by eukaryotic phytoplankton operated in the upwelling region off Oman and during the spring bloom in the northern Arabian <span class="hlt">Sea</span>. Cyanobacteria capable of fixing nitrogen seem to dominate the phytoplankton community during all other seasons. The export driven by cyanobacteria was much lower than the export driven by eukaryotic phytoplankton. Productivity and nutrient availability seems to be a main factor controlling <span class="hlt">fluxes</span> during blooms of eukaryotic phytoplankton. The ballast effect caused by inputs of dust into the ocean and its incorporation into sinking particles seems to be the main factor controlling the export during times when cyanobacteria dominate the phytoplankton community. C/N ratios of organic matter exported from blooms dominated by nitrogen fixing cyanobacteria are enhanced and, furthermore, indicate a more efficient recycling of nutrients at shallower water depth. This implies that the bacterial-driven OCP operates more in a recycling mode that keeps nutrients closer to the euphotic zone whereas the OCP driven by eukaryotic phytoplankton reduces the recycling of nutrients by exporting them into greater water-depth.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GBioC..31..901E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GBioC..31..901E"><span>Impacts of ENSO on <span class="hlt">air-sea</span> oxygen exchange: Observations and mechanisms</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Eddebbar, Yassir A.; Long, Matthew C.; Resplandy, Laure; Rödenbeck, Christian; Rodgers, Keith B.; Manizza, Manfredi; Keeling, Ralph F.</p> <p>2017-05-01</p> <p>Models and observations of atmospheric potential oxygen (APO ≃ O2 + 1.1 * CO2) are used to investigate the influence of El Niño-Southern Oscillation (ENSO) on <span class="hlt">air-sea</span> O2 exchange. An atmospheric transport inversion of APO data from the Scripps flask network shows significant interannual variability in tropical APO <span class="hlt">fluxes</span> that is positively correlated with the Niño3.4 index, indicating anomalous ocean outgassing of APO during El Niño. Hindcast simulations of the Community Earth System Model (CESM) and the Institut Pierre-Simon Laplace model show similar APO sensitivity to ENSO, differing from the Geophysical Fluid Dynamics Laboratory model, which shows an opposite APO response. In all models, O2 accounts for most APO <span class="hlt">flux</span> variations. Detailed analysis in CESM shows that the O2 response is driven primarily by ENSO modulation of the source and rate of equatorial upwelling, which moderates the intensity of O2 uptake due to vertical transport of low-O2 waters. These upwelling changes dominate over counteracting effects of biological productivity and thermally driven O2 exchange. During El Niño, shallower and weaker upwelling leads to anomalous O2 outgassing, whereas deeper and intensified upwelling during La Niña drives enhanced O2 uptake. This response is strongly localized along the central and eastern equatorial Pacific, leading to an equatorial zonal dipole in atmospheric anomalies of APO. This dipole is further intensified by ENSO-related changes in winds, reconciling apparently conflicting APO observations in the tropical Pacific. These findings suggest a substantial and complex response of the oceanic O2 cycle to climate variability that is significantly (>50%) underestimated in magnitude by ocean models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70032028','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70032028"><span>Bora event variability and the role of <span class="hlt">air-sea</span> feedback</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Pullen, J.; Doyle, J.D.; Haack, T.; Dorman, C.; Signell, R.P.; Lee, C.M.</p> <p>2007-01-01</p> <p>A two-way interacting high resolution numerical simulation of the Adriatic <span class="hlt">Sea</span> using the Navy Coastal Ocean Model (NCOM) and Coupled Ocean/ Atmosphere Mesoscale Prediction System (COAMPS??) was conducted to improve forecast momentum and heat <span class="hlt">flux</span> fields, and to evaluate surface <span class="hlt">flux</span> field differences for two consecutive bora events during February 2003. (COAMPS?? is a registered trademark of the Naval Research Laboratory.) The strength, mean positions and extensions of the bora jets, and the atmospheric conditions driving them varied considerably between the two events. Bora 1 had 62% stronger heat <span class="hlt">flux</span> and 51% larger momentum <span class="hlt">flux</span> than bora 2. The latter displayed much greater diurnal variability characterized by inertial oscillations and the early morning strengthening of a west Adriatic barrier jet, beneath which a stronger west Adriatic ocean current developed. Elsewhere, surface ocean current differences between the two events were directly related to differences in wind stress curl generated by the position and strength of the individual bora jets. The mean heat <span class="hlt">flux</span> bias was reduced by 72%, and heat <span class="hlt">flux</span> RMSE reduced by 30% on average at four instrumented over-water sites in the two-way coupled simulation relative to the uncoupled control. Largest reductions in wind stress were found in the bora jets, while the biggest reductions in heat <span class="hlt">flux</span> were found along the north and west coasts of the Adriatic. In bora 2, SST gradients impacted the wind stress curl along the north and west coasts, and in bora 1 wind stress curl was sensitive to the Istrian front position and strength. The two-way coupled simulation produced diminished surface current speeds of ???12% over the northern Adriatic during both bora compared with a one-way coupled simulation. Copyright 2007 by the American Geophysical Union.</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 CO2 <span class="hlt">Fluxes</span> In Seasonal Hypoxia-influenced Green Bay, Lake Michigan</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lin, P.; Klump, J. V.; Guo, L.</p> <p>2016-02-01</p> <p>Increasing anthropogenic nutrient enrichment has led to seasonal hypoxia in Green Bay, the largest freshwater estuary in the Laurentian Great Lakes, but change in carbon dynamics associated with the development of hypoxia remains poorly understood. Variations in alkalinity, abundance of carbon species, and <span class="hlt">air</span>-water CO2 <span class="hlt">fluxes</span> were quantified under contrasting hypoxic conditions during summer 2014. Green Bay was characterized with high pH (average 8.62 ± 0.16 in August), high DIC concentrations (2113 - 3213 µmol/kg) and high pCO2 in the water column. pCO2 was mostly >700 µatm in June, resulting in a net CO2 source to the <span class="hlt">air</span>, while pCO2 was mostly <650 µatm in August when hypoxic conditions occurred in Green Bay. In central Green Bay, pCO2 was the highest during both sampling months, accompanying by low dissolved oxygen (DO) and lower pH in the water column. In August, pCO2 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 CO2 dynamics and consumption of DO in Green Bay. Positive CO2 <span class="hlt">fluxes</span> to the atmosphere during August were only observed in northern bay but a CO2 sink was found in southern Green Bay ( 40% of study area) with high biological production and terrestrial DOM. Daily CO2 <span class="hlt">flux</span> ranged from 10.9 to 48.5 mmol-C m-2 d-1 in June with an average of 18.29 ± 7.44 mmol-C m-2 d-1, whereas it varied from 1.82 ± 1.18 mmol m-2 d-1 in the north to -2.05 ± 1.89 mmol m-2 d-1 in the south of Green Bay in August. Even though strong biological production reduced the CO2 emission, daily CO2 <span class="hlt">fluxes</span> from Green Bay to the <span class="hlt">air</span> were as high as 7.4 × 107 mole-C in June and 4.6 × 106 mole-C in August, suggesting a significant role of high-DIC lakes in global CO2 budget and cycling.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JGRD..119.1073Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JGRD..119.1073Z"><span>Selected current-use and historic-use pesticides in <span class="hlt">air</span> and seawater of the Bohai and Yellow <span class="hlt">Seas</span>, China</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhong, Guangcai; Tang, Jianhui; Xie, Zhiyong; Möller, Axel; Zhao, Zhen; Sturm, Renate; Chen, Yingjun; Tian, Chongguo; Pan, Xiaohui; Qin, Wei; Zhang, Gan; Ebinghaus, Ralf</p> <p>2014-01-01</p> <p>Consumption of pesticides in China has increased rapidly in recent years; however, occurrence and fate of current-use pesticides (CUPs) in China coastal waters are poorly understood. Globally banned pesticides, so-called historic-use pesticides (HUPs), are still commonly observed in the environment. In this work, <span class="hlt">air</span> and surface seawater samples taken from the Bohai and Yellow <span class="hlt">Seas</span> in May 2012 were analyzed for CUPs including trifluralin, quintozene, chlorothalonil, dicofol, chlorpyrifos, and dacthal, as well as HUPs (hexachlorobenzene (HCB), hexachlorocyclohexanes (HCHs), and endosulfan). CUP profile in both <span class="hlt">air</span> and seawater samples generally reflected their consumption patterns in China. HUPs in the <span class="hlt">air</span> and seawater samples were in comparable levels as those of CUPs with high concentrations. α-Endosulfan, dicofol, and chlorothalonil showed strong net deposition likely resulting from their intensive use in recent years, while CUPs with low consumption amount (quintozene and dacthal) were close to equilibrium at most samplings sites. Another CUP with high usage amout (i.e., chlorpyrifos) underwent volatilization possibly due to its longer half-life in seawater than that in <span class="hlt">air</span>. α-HCH and γ-HCH were close to equilibrium in the Bohai <span class="hlt">Sea</span>, but mainly underwent net deposition in the Yellow <span class="hlt">Sea</span>. The net deposition of α-HCH could be attributed to polluted <span class="hlt">air</span> pulses from the East China identified by <span class="hlt">air</span> mass back trajectories. β-HCH showed net volatilization in the Bohai <span class="hlt">Sea</span>, which was driven by its relative enrichment in seawater. HCB either slightly favored net volatilization or was close to equilibrium in the Bohai and Yellow <span class="hlt">Seas</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_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/2008JGRD..113.5306C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008JGRD..113.5306C"><span>Sources and <span class="hlt">fluxes</span> of atmospheric trace elements to 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>Chen, Ying; Paytan, Adina; Chase, Zanna; Measures, Christopher; Beck, Aaron J.; SañUdo-Wilhelmy, Sergio A.; Post, Anton F.</p> <p>2008-03-01</p> <p>We present the first comprehensive investigation of the concentrations, <span class="hlt">fluxes</span> and sources of aerosol trace elements over the Gulf of Aqaba. We found that the mean atmospheric concentrations of crustally derived elements such as Al, Fe and Mn (1081, 683, and 16.7 ng m-3) are about 2-3 times higher than those reported for the neighboring Mediterranean area. This is indicative of the dominance of the mineral dust component in aerosols over the Gulf. Anthropogenic impact was lower in comparison to the more heavily populated areas of the Mediterranean. During the majority of time (69%) the <span class="hlt">air</span> masses over the Gulf originated from Europe or Mediterranean <span class="hlt">Sea</span> areas delivering anthropogenic components such as Cu, Cd, Ni, Zn, and P. Airflows derived from North Africa in contrast contained the highest concentrations of Al, Fe, and Sr but generally lower Cu, Cd, Ni, Zn, and P. Relatively high Pb, Ni, and V were found in the local and Arabian airflows suggesting a greater influence of local emission of fuel burning. We used the data and the measured trace metal seawater concentrations to calculate residence times of dissolved trace elements in the upper 50 m surface water of the Gulf (with respect to atmospheric input) and found that the residence times for most elements are in the range of 5-37 years while Cd and V residence times are longer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ACP....18.4277W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ACP....18.4277W"><span>Ozone pollution around a coastal region of South China <span class="hlt">Sea</span>: interaction between marine and continental <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>Wang, Hao; Lyu, Xiaopu; Guo, Hai; Wang, Yu; Zou, Shichun; Ling, Zhenhao; Wang, Xinming; Jiang, Fei; Zeren, Yangzong; Pan, Wenzhuo; Huang, Xiaobo; Shen, Jin</p> <p>2018-03-01</p> <p>Marine atmosphere is usually considered to be a clean environment, but this study indicates that the near-coast waters of the South China <span class="hlt">Sea</span> (SCS) suffer from even worse <span class="hlt">air</span> quality than coastal cities. The analyses were based on concurrent field measurements of target <span class="hlt">air</span> pollutants and meteorological parameters conducted at a suburban site (Tung Chung, TC) and a nearby marine site (Wan Shan, WS) from August to November 2013. The observations showed that the levels of primary <span class="hlt">air</span> pollutants were significantly lower at WS than those at TC, while the ozone (O3) value was greater at WS. Higher O3 levels at WS were attributed to the weaker NO titration and higher O3 production rate because of stronger oxidative capacity of the atmosphere. However, O3 episodes were concurrently observed at both sites under certain meteorological conditions, such as tropical cyclones, continental anticyclones and <span class="hlt">sea</span>-land breezes (SLBs). Driven by these synoptic systems and mesoscale recirculations, the interaction between continental and marine <span class="hlt">air</span> masses profoundly changed the atmospheric composition and subsequently influenced the formation and redistribution of O3 in the coastal areas. When continental <span class="hlt">air</span> intruded into marine atmosphere, the O3 pollution was magnified over the SCS, and the elevated O3 ( > 100 ppbv) could overspread the <span class="hlt">sea</span> boundary layer ˜ 8 times the area of Hong Kong. In some cases, the exaggerated O3 pollution over the SCS was recirculated to the coastal inshore by <span class="hlt">sea</span> breeze, leading to aggravated O3 pollution in coastal cities. The findings are applicable to similar mesoscale environments around the world where the maritime atmosphere is potentially influenced by severe continental <span class="hlt">air</span> pollution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ClDy...50...83B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ClDy...50...83B"><span>Greenland coastal <span class="hlt">air</span> temperatures linked to Baffin Bay and Greenland <span class="hlt">Sea</span> ice conditions during autumn through regional blocking patterns</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ballinger, Thomas J.; Hanna, Edward; Hall, Richard J.; Miller, Jeffrey; Ribergaard, Mads H.; Høyer, Jacob L.</p> <p>2018-01-01</p> <p>Variations in <span class="hlt">sea</span> ice freeze onset and regional <span class="hlt">sea</span> surface temperatures (SSTs) in Baffin Bay and Greenland <span class="hlt">Sea</span> are linked to autumn surface <span class="hlt">air</span> temperatures (SATs) around coastal Greenland through 500 hPa blocking patterns, 1979-2014. We find strong, statistically significant correlations between Baffin Bay freeze onset and SSTs and SATs across the western and southernmost coastal areas, while weaker and fewer significant correlations are found between eastern SATs, SSTs, and freeze periods observed in the neighboring Greenland <span class="hlt">Sea</span>. Autumn Greenland Blocking Index values and the incidence of meridional circulation patterns have increased over the modern <span class="hlt">sea</span> ice monitoring era. Increased anticyclonic blocking patterns promote poleward transport of warm <span class="hlt">air</span> from lower latitudes and local warm <span class="hlt">air</span> advection onshore from ocean-atmosphere sensible heat exchange through ice-free or thin ice-covered <span class="hlt">seas</span> bordering the coastal stations. Temperature composites by years of extreme late freeze conditions, occurring since 2006 in Baffin Bay, reveal positive monthly SAT departures that often exceed 1 standard deviation from the 1981-2010 climate normal over coastal areas that exhibit a similar spatial pattern as the peak correlations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('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). CO2 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 CO2 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 CO2 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> CO2 <span class="hlt">flux</span> and carbon export. Concurrently recorded in-situ bio-optical data allow direct comparison of optical measurements of biomass change and reveal key patterns in the seasonal succession of phytoplankton groups responsible for carbon drawdown.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170007396','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170007396"><span>Preparation of the NASA <span class="hlt">Air</span> Quality Monitor for a U.S. Navy Submarine <span class="hlt">Sea</span> Trial</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Limero, Thomas; Wallace, William T.; Manney, Joshua A.; Smith, Matthew J.; O'Connor, Sara Jane; Mudgett, Paul D.</p> <p>2017-01-01</p> <p>For the past 4 years, the <span class="hlt">Air</span> Quality Monitor (AQM) has been the operational instrument for measuring trace volatile organic compounds on the International Space Station (ISS). The key components of the AQM are the inlet preconcentrator, the gas chromatograph (GC), and the differential mobility spectrometer. Onboard the ISS are two AQMs with different GC columns that detect and quantify 22 compounds. The AQM data contributes valuable information to the assessment of <span class="hlt">air</span> quality aboard ISS for each crew increment. The US Navy is looking to update its submarine <span class="hlt">air</span> monitoring suite of instruments and the success of the AQM on ISS has led to a jointly planned submarine <span class="hlt">sea</span> trial of a NASA AQM. In addition to the AQM, the Navy is also interested in the Multi-Gas Monitor (MGM), which measures major constituent gases (oxygen, carbon dioxide, water vapor, and ammonia). A separate paper will present the MGM <span class="hlt">sea</span> trial preparation and the analysis of most recent ISS data. A prototype AQM, which is virtually identical to the operational AQM, has been readied for the <span class="hlt">sea</span> trial. Only one AQM will be deployed during the <span class="hlt">sea</span> trial, but this is sufficient for NASA purposes and to detect the compounds of interest to the US Navy for this trial. The data from the <span class="hlt">sea</span> trial will be compared to data from archival samples collected before, during, and after the trial period. This paper will start with a brief history of past collaborations between NASA and the U.S. and U.K. navies for trials of <span class="hlt">air</span> monitoring equipment. An overview of the AQM technology and protocols for the submarine trial will be presented. The majority of the presentation will focus on the AQM preparation and a summary of available data from the trial.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20070034010','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20070034010"><span>Correlations Between <span class="hlt">Sea</span>-Surface Salinity Tendencies and Freshwater <span class="hlt">Fluxes</span> in the Pacific Ocean</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Li, Zhen; Adamec, David</p> <p>2007-01-01</p> <p>Temporal changes in <span class="hlt">sea</span>-surface salinity (SSS) from 21 years of a high resolution model integration of the Pacific Ocean are correlated with the freshwater <span class="hlt">flux</span> that was used to force the integration. The correlations are calculated on a 1 x10 grid, and on a monthly scale to assess the possibility of deducing evaporation minus precipitation (E-P) fields from the salinity measurements to be taken by the upcoming Aquarius/SAC-D mission. Correlations between the monthly mean E-P fields and monthly mean SSS temporal tendencies are mainly zonally-oriented, and are highest where the local precipitation is relatively high. Nonseasonal (deviations from the monthly mean) correlations are highest along mid-latitude storm tracks and are relatively small in the tropics. The response of the model's surface salinity to surface forcing is very complex, and retrievals of freshwater <span class="hlt">fluxes</span> from SSS measurements alone will require consideration of other processes, including horizontal advection and vertical mixing, rather than a simple balance between the two.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19820015568','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19820015568"><span>Size distribution of oceanic <span class="hlt">air</span> bubbles entrained in <span class="hlt">sea</span>-water by wave-breaking</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Resch, F.; Avellan, F.</p> <p>1982-01-01</p> <p>The size of oceanic <span class="hlt">air</span> bubbles produced by whitecaps and wave-breaking is determined. The production of liquid aerosols at the <span class="hlt">sea</span> surface is predicted. These liquid aerosols are at the origin of most of the particulate materials exchanged between the ocean and the atmosphere. A prototype was designed and built using an optical technique based on the principle of light scattering at an angle of ninety degrees from the incident light beam. The output voltage is a direct function of the bubble diameter. Calibration of the probe was carried out within a range of 300 microns to 1.2 mm. Bubbles produced by wave-breaking in a large <span class="hlt">air-sea</span> interaction simulating facility. Experimental results are given in the form of size spectrum.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.3762D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.3762D"><span>Comparison of the ocean surface vector winds over the Nordic <span class="hlt">Seas</span> and their application for ocean modeling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dukhovskoy, Dmitry; Bourassa, Mark</p> <p>2017-04-01</p> <p>Ocean processes in the Nordic <span class="hlt">Seas</span> and northern North Atlantic are strongly controlled by <span class="hlt">air-sea</span> heat and momentum <span class="hlt">fluxes</span>. The predominantly cyclonic, large-scale atmospheric circulation brings the deep ocean layer up to the surface preconditioning the convective sites in the Nordic <span class="hlt">Seas</span> for deep convection. In winter, intensive cooling and possibly salt <span class="hlt">flux</span> from newly formed <span class="hlt">sea</span> ice erodes the near-surface stratification and the mixed layer merges with the deeper domed layer, exposing the very weakly stratified deep water mass to direct interaction with the atmosphere. Surface wind is one of the atmospheric parameters required for estimating momentum and turbulent heat <span class="hlt">fluxes</span> to the <span class="hlt">sea</span> ice and ocean surface. In the ocean models forced by atmospheric analysis, errors in surface wind fields result in errors in <span class="hlt">air-sea</span> heat and momentum <span class="hlt">fluxes</span>, water mass formation, ocean circulation, as well as volume and heat transport in the straits. The goal of the study is to assess discrepancies across the wind vector fields from reanalysis data sets and scatterometer-derived gridded products over the Nordic <span class="hlt">Seas</span> and northern North Atlantic and to demonstrate possible implications of these differences for ocean modeling. The analyzed data sets include the reanalysis data from the National Center for Environmental Prediction Reanalysis 2 (NCEPR2), Climate Forecast System Reanalysis (CFSR), Arctic System Reanalysis (ASR) and satellite wind products Cross-Calibrated Multi-Platform (CCMP) wind product version 1.1 and recently released version 2.0, and Remote Sensing Systems QuikSCAT data. Large-scale and mesoscale characteristics of winds are compared at interannual, seasonal, and synoptic timescales. Numerical sensitivity experiments are conducted with a coupled ice-ocean model forced by different wind fields. The sensitivity experiments demonstrate differences in the net surface heat <span class="hlt">fluxes</span> during storm events. Next, it is hypothesized that discrepancies in the wind vorticity</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28526196','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28526196"><span>Use of a numerical simulation approach to improve the estimation of <span class="hlt">air</span>-water exchange <span class="hlt">fluxes</span> of polycyclic aromatic hydrocarbons in a coastal zone.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lai, I-Chien; Lee, Chon-Lin; Ko, Fung-Chi; Lin, Ju-Chieh; Huang, Hu-Ching; Shiu, Ruei-Feng</p> <p>2017-07-15</p> <p>The <span class="hlt">air</span>-water exchange is important for determining the transport, fate, and chemical loading of polycyclic aromatic hydrocarbons (PAHs) in the atmosphere and in aquatic systems. Investigations of PAH <span class="hlt">air</span>-water exchange are mostly based on observational data obtained using complicated field sampling processes. This study proposes a new approach to improve the estimation of long-term PAH <span class="hlt">air</span>-water exchange <span class="hlt">fluxes</span> by using a multivariate regression model to simulate hourly gaseous PAH concentrations. Model performance analysis and the benefits from this approach indicate its effectiveness at improving the <span class="hlt">flux</span> estimations and at decreasing the field sampling difficulty. The proposed GIS mapping approach is useful for box model establishment and is tested for visualization of the spatiotemporal variations of <span class="hlt">air</span>-water exchange <span class="hlt">fluxes</span> in a coastal zone. The <span class="hlt">air</span>-water exchange <span class="hlt">fluxes</span> illustrated by contour maps suggest that the atmospheric PAHs might have greater impacts on offshore sites than on the coastal area in this study. Copyright © 2017 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRC..123.2422L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRC..123.2422L"><span>Seasonal and Interannual Variations of <span class="hlt">Sea</span> Ice Mass Balance From the Central Arctic to 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>Lei, Ruibo; Cheng, Bin; Heil, Petra; Vihma, Timo; Wang, Jia; Ji, Qing; Zhang, Zhanhai</p> <p>2018-04-01</p> <p>The seasonal evolution of <span class="hlt">sea</span> ice mass balance between the Central Arctic and Fram Strait, as well as the underlying driving forces, remain largely unknown because of a lack of observations. In this study, two and three buoys were deployed in the Central Arctic during the summers of 2010 and 2012, respectively. It was established that basal ice growth commenced between mid-October and early December. Annual basal ice growth, ranging from 0.21 to 1.14 m, was determined mainly by initial ice thickness, <span class="hlt">air</span> temperature, and oceanic heat <span class="hlt">flux</span> during winter. An analytic thermodynamic model indicated that climate warming reduces the winter growth rate of thin ice more than for thick ice because of the weak thermal inertia of the former. Oceanic heat <span class="hlt">flux</span> during the freezing season was 2-4 W m-2, which accounted for 18-31% of the basal ice energy balance. We identified two mechanisms that modified the oceanic heat <span class="hlt">flux</span>, i.e., solar energy absorbed by the upper ocean during summer, and interaction with warm waters south of Fram Strait; the latter resulted in basal ice melt, even in winter. In summer 2010, ice loss in the Central Arctic was considerable, which led to increased oceanic heat <span class="hlt">flux</span> into winter and delayed ice growth. The Transpolar Drift Stream was relatively weak in summer 2013. This reduced <span class="hlt">sea</span> ice advection out of the Arctic Ocean, and it restrained ice melt because of the cool atmospheric conditions, weakened albedo feedback, and relatively small oceanic heat <span class="hlt">flux</span> in the north.</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 CO 2 <span class="hlt">fluxes</span> with the floating chamber technique</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Ribas-Ribas, Mariana; Kilcher, Levi F.; Wurl, Oliver</p> <p></p> <p>Understanding how the ocean absorbs anthropogenic CO 2 is critical for predicting climate change. We designed Sniffle, a new autonomous drifting buoy with a floating chamber, to measure gas transfer velocities and <span class="hlt">air-sea</span> CO 2 <span class="hlt">fluxes</span> with high spatiotemporal resolution. Currently, insufficient in situ data exist to verify gas transfer parameterizations at low wind speeds (<4 m s -1), which leads to underestimation of gas transfer velocities and, therefore, of <span class="hlt">air-sea</span> CO 2 <span class="hlt">fluxes</span>. The Sniffle is equipped with a sensor to consecutively measure aqueous and atmospheric pCO 2 and to monitor increases or decreases of CO 2 inside themore » chamber. During autonomous operation, a complete cycle lasts 40 minutes, with a new cycle initiated after flushing the chamber. The Sniffle can be deployed for up to 15 hours at wind speeds up to 10 m s -1. Floating chambers often overestimate <span class="hlt">fluxes</span> because they create additional turbulence at the water surface. We correct <span class="hlt">fluxes</span> by measuring turbulence with two acoustic Doppler velocimeters, one positioned directly under the floating chamber and the other positioned sideways, to compare artificial disturbance caused by the chamber and natural turbulence. The first results of deployment in the North <span class="hlt">Sea</span> during the summer of 2016 demonstrate that the new drifting buoy is a useful tool that can improve our understanding of gas transfer velocity with in situ measurements. At low and moderate wind speeds and different conditions, the results obtained indicate that the observed tidal basin was acting as a source of atmospheric CO 2. Wind speed and turbulence alone could not fully explain the variance in gas transfer velocity. We suggest therefore, that other factors like surfactants, rain or tidal current will have an impact on gas transfer parameterizations.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1431413-sniffle-step-forward-measure-situ-co2-fluxes-floating-chamber-technique','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1431413-sniffle-step-forward-measure-situ-co2-fluxes-floating-chamber-technique"><span>Sniffle: a step forward to measure in situ CO 2 <span class="hlt">fluxes</span> with the floating chamber technique</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Ribas-Ribas, Mariana; Kilcher, Levi F.; Wurl, Oliver</p> <p>2018-01-09</p> <p>Understanding how the ocean absorbs anthropogenic CO 2 is critical for predicting climate change. We designed Sniffle, a new autonomous drifting buoy with a floating chamber, to measure gas transfer velocities and <span class="hlt">air-sea</span> CO 2 <span class="hlt">fluxes</span> with high spatiotemporal resolution. Currently, insufficient in situ data exist to verify gas transfer parameterizations at low wind speeds (<4 m s -1), which leads to underestimation of gas transfer velocities and, therefore, of <span class="hlt">air-sea</span> CO 2 <span class="hlt">fluxes</span>. The Sniffle is equipped with a sensor to consecutively measure aqueous and atmospheric pCO 2 and to monitor increases or decreases of CO 2 inside themore » chamber. During autonomous operation, a complete cycle lasts 40 minutes, with a new cycle initiated after flushing the chamber. The Sniffle can be deployed for up to 15 hours at wind speeds up to 10 m s -1. Floating chambers often overestimate <span class="hlt">fluxes</span> because they create additional turbulence at the water surface. We correct <span class="hlt">fluxes</span> by measuring turbulence with two acoustic Doppler velocimeters, one positioned directly under the floating chamber and the other positioned sideways, to compare artificial disturbance caused by the chamber and natural turbulence. The first results of deployment in the North <span class="hlt">Sea</span> during the summer of 2016 demonstrate that the new drifting buoy is a useful tool that can improve our understanding of gas transfer velocity with in situ measurements. At low and moderate wind speeds and different conditions, the results obtained indicate that the observed tidal basin was acting as a source of atmospheric CO 2. Wind speed and turbulence alone could not fully explain the variance in gas transfer velocity. We suggest therefore, that other factors like surfactants, rain or tidal current will have an impact on gas transfer parameterizations.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA601544','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA601544"><span>Assessing Maritime Aspects of the <span class="hlt">AirSea</span> Battle Concept</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2012-03-23</p> <p><span class="hlt">AirSea</span> Battle centered on the assessment that in hostilities the PRC would conduct a rapid preemptive attack to knock back U.S. and allied forces in...these factors provide the foundational need for a clear maritime strategy backed by strong naval power. ! The core of PRC maritime security strategy...Law Enforcement Command. This direct and indirect approach hearkens back to the theories of Sunzi and Mao Tse-tung. ! China’s 2010 National Defense</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1996AnGeo..14..986E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1996AnGeo..14..986E"><span>Study of the <span class="hlt">air-sea</span> interactions at the mesoscale: the SEMAPHORE experiment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Eymard, L.; Planton, S.; Durand, P.; Le Visage, C.; Le Traon, P. Y.; Prieur, L.; Weill, A.; Hauser, D.; Rolland, J.; Pelon, J.; Baudin, F.; Bénech, B.; Brenguier, J. L.; Caniaux, G.; de Mey, P.; Dombrowski, E.; Druilhet, A.; Dupuis, H.; Ferret, B.; Flamant, C.; Flamant, P.; Hernandez, F.; Jourdan, D.; Katsaros, K.; Lambert, D.; Lefèvre, J. M.; Le Borgne, P.; Le Squere, B.; Marsoin, A.; Roquet, H.; Tournadre, J.; Trouillet, V.; Tychensky, A.; Zakardjian, B.</p> <p>1996-09-01</p> <p>The SEMAPHORE (Structure des Echanges Mer-Atmosphère, Propriétés des Hétérogénéités Océaniques: Recherche Expérimentale) experiment has been conducted from June to November 1993 in the Northeast Atlantic between the Azores and Madeira. It was centered on the study of the mesoscale ocean circulation and <span class="hlt">air-sea</span> interactions. The experimental investigation was achieved at the mesoscale using moorings, floats, and ship hydrological survey, and at a smaller scale by one dedicated ship, two instrumented aircraft, and surface drifting buoys, for one and a half month in October-November (IOP: intense observing period). Observations from meteorological operational satellites as well as spaceborne microwave sensors were used in complement. The main studies undertaken concern the mesoscale ocean, the upper ocean, the atmospheric boundary layer, and the <span class="hlt">sea</span> surface, and first results are presented for the various topics. From data analysis and model simulations, the main characteristics of the ocean circulation were deduced, showing the close relationship between the Azores front meander and the occurrence of Mediterranean water lenses (meddies), and the shift between the Azores current frontal signature at the surface and within the thermocline. Using drifting buoys and ship data in the upper ocean, the gap between the scales of the atmospheric forcing and the oceanic variability was made evident. A 2 °C decrease and a 40-m deepening of the mixed layer were measured within the IOP, associated with a heating loss of about 100 W m-2. This evolution was shown to be strongly connected to the occurrence of storms at the beginning and the end of October. Above the surface, turbulent measurements from ship and aircraft were analyzed across the surface thermal front, showing a 30% difference in heat <span class="hlt">fluxes</span> between both sides during a 4-day period, and the respective contributions of the wind and the surface temperature were evaluated. The classical momentum <span class="hlt">flux</span> bulk</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 and SA is much weaker (r2 = <0.01, n = 22). While organic matter composition and sources may have variable control on <span class="hlt">air-sea</span> gas exchange between the provinces, the poor relationship observed between SA and k660 suggests that other environmental factors maybe more influential on <span class="hlt">air-sea</span> gas exchange in the open ocean compared to North <span class="hlt">Sea</span> coastal waters.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSPO54F3320B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSPO54F3320B"><span>Satellite-based Calibration of Heat <span class="hlt">Flux</span> at the Ocean Surface</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Barron, C. N.; Dastugue, J. M.; May, J. C.; Rowley, C. D.; Smith, S. R.; Spence, P. L.; Gremes-Cordero, S.</p> <p>2016-02-01</p> <p>Model forecasts of upper ocean heat content and variability on diurnal to daily scales are highly dependent on estimates of heat <span class="hlt">flux</span> through the <span class="hlt">air-sea</span> interface. Satellite remote sensing is applied to not only inform the initial ocean state but also to mitigate errors in surface heat <span class="hlt">flux</span> and model representations affecting the distribution of heat in the upper ocean. Traditional assimilation of <span class="hlt">sea</span> surface temperature (SST) observations re-centers ocean models at the start of each forecast cycle. Subsequent evolution depends on estimates of surface heat <span class="hlt">fluxes</span> and upper-ocean processes over the forecast period. The COFFEE project (Calibration of Ocean Forcing with satellite <span class="hlt">Flux</span> Estimates) endeavors to correct ocean forecast bias through a responsive error partition among surface heat <span class="hlt">flux</span> and ocean dynamics sources. A suite of experiments in the southern California Current demonstrates a range of COFFEE capabilities, showing the impact on forecast error relative to a baseline three-dimensional variational (3DVAR) assimilation using Navy operational global or regional atmospheric forcing. COFFEE addresses satellite-calibration of surface <span class="hlt">fluxes</span> to estimate surface error covariances and links these to the ocean interior. Experiment cases combine different levels of <span class="hlt">flux</span> calibration with different assimilation alternatives. The cases may use the original <span class="hlt">fluxes</span>, apply full satellite corrections during the forecast period, or extend hindcast corrections into the forecast period. Assimilation is either baseline 3DVAR or standard strong-constraint 4DVAR, with work proceeding to add a 4DVAR expanded to include a weak constraint treatment of the surface <span class="hlt">flux</span> errors. Covariance of <span class="hlt">flux</span> errors is estimated from the recent time series of forecast and calibrated <span class="hlt">flux</span> terms. While the California Current examples are shown, the approach is equally applicable to other regions. These approaches within a 3DVAR application are anticipated to be useful for global and larger</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 transfer. 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 <span class="hlt">fluxes</span>. 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 transfer. 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 transfer 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('https://ntrs.nasa.gov/search.jsp?R=19890062534&hterms=moisture+condensation&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dmoisture%2Bcondensation','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19890062534&hterms=moisture+condensation&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dmoisture%2Bcondensation"><span>Boundary layer warming by condensation - <span class="hlt">Air-sea</span> interaction during an extreme cold <span class="hlt">air</span> outbreak from the eastern coast of the United States</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Grossman, Robert L.</p> <p>1988-01-01</p> <p>Studies on an intense cold <span class="hlt">air</span> outbreak that took place after a cold <span class="hlt">air</span> cyclogenesis on January 27, 1986 are reviewed. Particular attention is given to data obtained during a multiaircraft research mission carried out on January 28, 1986 as part of the Genesis of Atlantic Lows Experiment. It was found that condensation heating of the subcloud layer <span class="hlt">air</span> was comparable to heating by turbulent <span class="hlt">flux</span> divergence.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1995JCli....8.1360G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1995JCli....8.1360G"><span>Observed Screen (<span class="hlt">Air</span>) and GCM Surface/Screen Temperatures: Implications for Outgoing Longwave <span class="hlt">Fluxes</span> at the Surface.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Garratt, J. R.</p> <p>1995-05-01</p> <p>There is direct evidence that excess net radiation calculated in general circulation models at continental surfaces [of about 11-17 W m2 (20%-27%) on an annual ~1 is not only due to overestimates in annual incoming shortwave <span class="hlt">fluxes</span> [of 9-18 W m2 (6%-9%)], but also to underestimates in outgoing longwave <span class="hlt">fluxes</span>. The bias in the outgoing longwave <span class="hlt">flux</span> is deduced from a comparison of screen-<span class="hlt">air</span> temperature observations, available as a global climatology of mean monthly values, and model-calculated surface and screen-<span class="hlt">air</span> temperatures. An underestimate in the screen temperature computed in general circulation models over continents, of about 3 K on an annual basis, implies an underestimate in the outgoing longwave <span class="hlt">flux</span>, averaged in six models under study, of 11-15 W m2 (3%-4%). For a set of 22 inland stations studied previously, the residual bias on an annual basis (the residual is the net radiation minus incoming shortwave plus outgoing longwave) varies between 18 and 23 W m2 for the models considered. Additional biases in one or both of the reflected shortwave and incoming longwave components cannot be ruled out.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20160013874&hterms=Change+climate&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3DChange%2Bclimate','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20160013874&hterms=Change+climate&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3DChange%2Bclimate"><span>The <span class="hlt">Flux</span>-Anomaly-Forced Model Intercomparison Project (FAFMIP) Contribution to CMIP6: Investigation of <span class="hlt">Sea</span>-Level and Ocean Climate Change in Response to CO2 Forcing</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gregory, Jonathan M.; Bouttes, Nathaelle; Griffies, Stephen M.; Haak, Helmuth; Hurlin, William J.; Jungclaus, Johann; Kelley, Maxwell; Lee, Warren G.; Marshall, John; Romanou, Anastasia; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20160013874'); toggleEditAbsImage('author_20160013874_show'); toggleEditAbsImage('author_20160013874_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20160013874_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20160013874_hide"></p> <p>2016-01-01</p> <p>The <span class="hlt">Flux</span>-Anomaly-Forced Model Intercomparison Project (FAFMIP) aims to investigate the spread in simulations of <span class="hlt">sea</span>-level and ocean climate change in response to CO2 forcing by atmosphere-ocean general circulation models (AOGCMs). It is particularly motivated by the uncertainties in projections of ocean heat uptake, global-mean sealevel rise due to thermal expansion and the geographical patterns of <span class="hlt">sea</span>-level change due to ocean density and circulation change. FAFMIP has three tier-1 experiments, in which prescribed surface <span class="hlt">flux</span> perturbations of momentum, heat and freshwater respectively are applied to the ocean in separate AOGCM simulations. All other conditions are as in the pre-industrial control. The prescribed fields are typical of pattern and magnitude of changes in these <span class="hlt">fluxes</span> projected by AOGCMs for doubled CO2 concentration. Five groups have tested the experimental design with existing AOGCMs. Their results show diversity in the pattern and magnitude of changes, with some common qualitative features. Heat and water <span class="hlt">flux</span> perturbation cause the dipole in <span class="hlt">sea</span>-level change in the North Atlantic, while momentum and heat <span class="hlt">flux</span> perturbation cause the gradient across the Antarctic Circumpolar Current. The Atlantic meridional overturning circulation (AMOC) declines in response to the heat <span class="hlt">flux</span> perturbation, and there is a strong positive feedback on this effect due to the consequent cooling of <span class="hlt">sea</span>-surface temperature in the North Atlantic, which enhances the local heat input to the ocean. The momentum and water <span class="hlt">flux</span> perturbations do not substantially affect the AMOC. Heat is taken up largely as a passive tracer in the Southern Ocean, which is the region of greatest heat input, while the weakening of the AMOC causes redistribution of heat towards lower latitudes. Future analysis of these and other phenomena with the wider range of CMIP6 FAFMIP AOGCMs will benefit from new diagnostics of temperature and salinity tendencies, which will enable investigation of the model</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_18 --> <div id="page_19" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="361"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27117888','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27117888"><span>Impact of Saharan dust events on radionuclide levels in Monaco <span class="hlt">air</span> and in the water column of the northwest Mediterranean <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>Pham, Mai Khanh; Chamizo, Elena; Mas Balbuena, José Luis; Miquel, Juan-Carlos; Martín, Jacobo; Osvath, Iolanda; Povinec, Pavel P</p> <p>2017-01-01</p> <p>Characterization of atmospheric aerosols collected in Monaco (2004-2008) and in sediment traps at 200 m and 1000 m water depths at the DYFAMED (Dynamics of Atmospheric <span class="hlt">Fluxes</span> in the Mediterranean <span class="hlt">Sea</span>) station (2004) was carried out to improve our understanding of the impact of Saharan dust on ground-level <span class="hlt">air</span> and on the water column. Activity concentrations of natural ( 210 Pb, 210 Po, uranium and radium isotopes) and anthropogenic ( 137 Cs, 239 Pu, 240 Pu, and 239+240 Pu) radionuclides and their isotopic ratios confirmed a Saharan impact on the investigated samples. In association with a large particulate matter deposition event in Monaco on 20 February 2004, the 137 Cs (∼40 Bq kg -1 ) and 239+240 Pu (∼1 Bq kg -1 ) activities were almost a factor of two higher than other Saharan deposition dust events. This single-day particle <span class="hlt">flux</span> represented 72% of the annual atmospheric deposition in Monaco. The annual deposition of Saharan dust on the <span class="hlt">sea</span> was 232-407 mBq m -2 for 137 Cs and 6.8-9.8 mBq m -2 for 239+240 Pu and contributed significantly (28-37% for 137 Cs and 34-45% for 239+240 Pu) to the total annual atmospheric input to the northwest Mediterranean <span class="hlt">Sea</span>. The 137 Cs/ 239+240 Pu activity ratios in dust samples collected during different Saharan dust events confirmed their global fallout origin or mixing with local re-suspended soil particles. In the sediment trap samples the 137 Cs activity varied by a factor of two, while the 239+240 Pu activity was constant, confirming the different behaviors of Cs (dissolved) and Pu (particle reactive) in the water column. The 137 Cs and 239+240 Pu activities of sinking particles during the period of the highest mass <span class="hlt">flux</span> collected in 20 February 2004 at the 200 m and 1000 m water depths represented about 10% and 15%, respectively, of annual deposition from Saharan dust events. Copyright © 2016 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.6061C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.6061C"><span>Importance of <span class="hlt">air-sea</span> interaction on wind waves, storm surge and hurricane simulations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, Yingjian; Yu, Xiping</p> <p>2017-04-01</p> <p>It was reported from field observations that wind stress coefficient levels off and even decreases when the wind speed exceeds 30-40 m/s. We propose a wave boundary layer model (WBLM) based on the momentum and energy conservation equations. Taking into account the physical details of the <span class="hlt">air-sea</span> interaction process as well as the energy dissipation due to the presence of <span class="hlt">sea</span> spray, this model successfully predicts the decreasing tendency of wind stress coefficient. Then WBLM is embedded in the current-wave coupled model FVCOM-SWAVE to simulate surface waves and storm surge under the forcing of hurricane Katrina. Numerical results based on WBLM agree well with the observed data of NDBC buoys and tide gauges. Sensitivity analysis of different wind stress evaluation methods also shows that large anomalies of significant wave height and surge elevation are captured along the passage of hurricane core. The differences of the local wave height are up to 13 m, which is in accordance with the general knowledge that the ocean dynamic processes under storm conditions are very sensitive to the amount of momentum exchange at the <span class="hlt">air-sea</span> interface. In the final part of the research, the reduced wind stress coefficient is tested in the numerical forecast of hurricane Katrina. A parabolic formula fitted to WBLM is employed in the atmosphere-ocean coupled model COAWST. Considering the joint effects of ocean cooling and reduced wind drag, the intensity metrics - the minimum <span class="hlt">sea</span> level pressure and the maximum 10 m wind speed - are in good inconsistency with the best track result. Those methods, which predict the wind stress coefficient that increase or saturate in extreme wind condition, underestimate the hurricane intensity. As a whole, we unify the evaluation methods of wind stress in different numerical models and yield reasonable results. Although it is too early to conclude that WBLM is totally applicable or the drag coefficient does decrease for high wind speed, our current</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018CSR...161...20K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018CSR...161...20K"><span>Influence of nutrient <span class="hlt">fluxes</span> on phytoplankton community and harmful algal blooms along the coastal waters of southeastern Arabian <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kumar, P. Sathish; Kumaraswami, M.; Rao, G. Durga; Ezhilarasan, P.; Sivasankar, R.; Rao, V. Ranga; Ramu, K.</p> <p>2018-06-01</p> <p>The seasonal variation in phytoplankton composition as well as the influencing factors on phytoplankton community were examined for the coastal waters of Kochi, southeastern Arabian <span class="hlt">Sea</span> during 2015. The elevated <span class="hlt">flux</span> of total nitrogen (TN) and silica (Si) during the summer monsoon (SM) induced the harmful algal blooms (HABs) of Scrippsiella trochoidea (11.9 × 105 cells L-1) and Karenia mikimotoi (6 × 105 cells L-1) near the inlets of Kochi estuary. Blooms of S. trochoidea were recorded for the first time in the Indian waters. The satellite data of chlorophyll-a showed the significant correlation with insitu observations of phytoplankton abundance and provided a better understanding of the spatio-temporal distribution. The canonical correspondence analysis indicates that the increased TN and Si <span class="hlt">fluxes</span> and lower temperature induced the HABs during the SM. The reduction in the load of N and Si in the coastal waters of southeastern Arabian <span class="hlt">Sea</span> is essential for controlling the HABs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018IzAOP..54...10S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018IzAOP..54...10S"><span>Characteristics of Winter Surface <span class="hlt">Air</span> Temperature Anomalies in Moscow in 1970-2016 under Conditions of Reduced <span class="hlt">Sea</span> Ice Area in the Barents <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>Shukurov, K. A.; Semenov, V. A.</p> <p>2018-01-01</p> <p>On the basis of observational data on daily mean surface <span class="hlt">air</span> temperature (SAT) and <span class="hlt">sea</span> ice concentration (SIC) in the Barents <span class="hlt">Sea</span> (BS), the characteristics of strong positive and negative winter SAT anomalies in Moscow have been studied in comparison with BS SIC data obtained in 1949-2016. An analysis of surface backward trajectories of <span class="hlt">air</span>-particle motions has revealed the most probable paths of both cold and warm <span class="hlt">air</span> invasions into Moscow and located regions that mostly affect strong winter SAT anomalies in Moscow. Atmospheric circulation anomalies that cause strong winter SAT anomalies in Moscow have been revealed. Changes in the ways of both cold and warm <span class="hlt">air</span> invasions have been found, as well as an increase in the frequency of blocking anticyclones in 2005-2016 when compared to 1970-1999. The results suggest that a winter SIC decrease in the BS in 2005-2016 affects strong winter SAT anomalies in Moscow due to an increase in the frequency of occurrence of blocking anticyclones to the south of and over the BS.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3965429','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3965429"><span>Effect of Redox Conditions on Bacterial Community Structure in Baltic <span class="hlt">Sea</span> Sediments with Contrasting Phosphorus <span class="hlt">Fluxes</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>Steenbergh, Anne K.; Bodelier, Paul L. E.; Slomp, Caroline P.; Laanbroek, Hendrikus J.</p> <p>2014-01-01</p> <p>Phosphorus release from sediments can exacerbate the effect of eutrophication in coastal marine ecosystems. The <span class="hlt">flux</span> of phosphorus from marine sediments to the overlying water is highly dependent on the redox conditions at the sediment-water interface. Bacteria are key players in the biological processes that release or retain phosphorus in marine sediments. To gain more insight in the role of bacteria in phosphorus release from sediments, we assessed the effect of redox conditions on the structure of bacterial communities. To do so, we incubated surface sediments from four sampling sites in the Baltic <span class="hlt">Sea</span> under oxic and anoxic conditions and analyzed the fingerprints of the bacterial community structures in these incubations and the original sediments. This paper describes the effects of redox conditions, sampling station, and sample type (DNA, RNA, or whole-cell sample) on bacterial community structure in sediments. Redox conditions explained only 5% of the variance in community structure, and bacterial communities from contrasting redox conditions showed considerable overlap. We conclude that benthic bacterial communities cannot be classified as being typical for oxic or anoxic conditions based on community structure fingerprints. Our results suggest that the overall structure of the benthic bacterial community has only a limited impact on benthic phosphate <span class="hlt">fluxes</span> in the Baltic <span class="hlt">Sea</span>. PMID:24667801</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24667801','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24667801"><span>Effect of redox conditions on bacterial community structure in Baltic <span class="hlt">Sea</span> sediments with contrasting phosphorus <span class="hlt">fluxes</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Steenbergh, Anne K; Bodelier, Paul L E; Slomp, Caroline P; Laanbroek, Hendrikus J</p> <p>2014-01-01</p> <p>Phosphorus release from sediments can exacerbate the effect of eutrophication in coastal marine ecosystems. The <span class="hlt">flux</span> of phosphorus from marine sediments to the overlying water is highly dependent on the redox conditions at the sediment-water interface. Bacteria are key players in the biological processes that release or retain phosphorus in marine sediments. To gain more insight in the role of bacteria in phosphorus release from sediments, we assessed the effect of redox conditions on the structure of bacterial communities. To do so, we incubated surface sediments from four sampling sites in the Baltic <span class="hlt">Sea</span> under oxic and anoxic conditions and analyzed the fingerprints of the bacterial community structures in these incubations and the original sediments. This paper describes the effects of redox conditions, sampling station, and sample type (DNA, RNA, or whole-cell sample) on bacterial community structure in sediments. Redox conditions explained only 5% of the variance in community structure, and bacterial communities from contrasting redox conditions showed considerable overlap. We conclude that benthic bacterial communities cannot be classified as being typical for oxic or anoxic conditions based on community structure fingerprints. Our results suggest that the overall structure of the benthic bacterial community has only a limited impact on benthic phosphate <span class="hlt">fluxes</span> in the Baltic <span class="hlt">Sea</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110011892','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110011892"><span>Observations of Recent Arctic <span class="hlt">Sea</span> Ice Volume Loss and Its Impact on Ocean-Atmosphere Energy Exchange and Ice Production</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kurtz, N. T.; Markus, T.; Farrell, S. L.; Worthen, D. L.; Boisvert, L. N.</p> <p>2011-01-01</p> <p>Using recently developed techniques we estimate snow and <span class="hlt">sea</span> ice thickness distributions for the Arctic basin through the combination of freeboard data from the Ice, Cloud, and land Elevation Satellite (ICESat) and a snow depth model. These data are used with meteorological data and a thermodynamic <span class="hlt">sea</span> ice model to calculate ocean-atmosphere heat exchange and ice volume production during the 2003-2008 fall and winter seasons. The calculated heat <span class="hlt">fluxes</span> and ice growth rates are in agreement with previous observations over multiyear ice. In this study, we calculate heat <span class="hlt">fluxes</span> and ice growth rates for the full distribution of ice thicknesses covering the Arctic basin and determine the impact of ice thickness change on the calculated values. Thinning of the <span class="hlt">sea</span> ice is observed which greatly increases the 2005-2007 fall period ocean-atmosphere heat <span class="hlt">fluxes</span> compared to those observed in 2003. Although there was also a decline in <span class="hlt">sea</span> ice thickness for the winter periods, the winter time heat <span class="hlt">flux</span> was found to be less impacted by the observed changes in ice thickness. A large increase in the net Arctic ocean-atmosphere heat output is also observed in the fall periods due to changes in the areal coverage of <span class="hlt">sea</span> ice. The anomalously low <span class="hlt">sea</span> ice coverage in 2007 led to a net ocean-atmosphere heat output approximately 3 times greater than was observed in previous years and suggests that <span class="hlt">sea</span> ice losses are now playing a role in increasing surface <span class="hlt">air</span> temperatures in the Arctic.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.7197S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.7197S"><span>SAMOS Surface <span class="hlt">Fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Smith, Shawn; Bourassa, Mark</p> <p>2014-05-01</p> <p>The development of a new surface <span class="hlt">flux</span> dataset based on underway meteorological observations from research vessels will be presented. The research vessel data center at the Florida State University routinely acquires, quality controls, and distributes underway surface meteorological and oceanographic observations from over 30 oceanographic vessels. These activities are coordinated by the Shipboard Automated Meteorological and Oceanographic System (SAMOS) initiative in partnership with the Rolling Deck to Repository (R2R) project. Recently, the SAMOS data center has used these underway observations to produce bulk <span class="hlt">flux</span> estimates for each vessel along individual cruise tracks. A description of this new <span class="hlt">flux</span> product, along with the underlying data quality control procedures applied to SAMOS observations, will be provided. Research vessels provide underway observations at high-temporal frequency (1 min. sampling interval) that include navigational (position, course, heading, and speed), meteorological (<span class="hlt">air</span> temperature, humidity, wind, surface pressure, radiation, rainfall), and oceanographic (surface <span class="hlt">sea</span> temperature and salinity) samples. Vessels recruited to the SAMOS initiative collect a high concentration of data within the U.S. continental shelf and also frequently operate well outside routine shipping lanes, capturing observations in extreme ocean environments (Southern, Arctic, South Atlantic, and South Pacific oceans). These observations are atypical for their spatial and temporal sampling, making them very useful for many applications including validation of numerical models and satellite retrievals, as well as local assessments of natural variability. Individual SAMOS observations undergo routine automated quality control and select vessels receive detailed visual data quality inspection. The result is a quality-flagged data set that is ideal for calculating turbulent <span class="hlt">flux</span> estimates. We will describe the bulk <span class="hlt">flux</span> algorithms that have been applied to the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20090028806','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20090028806"><span>Small Autonomous <span class="hlt">Air/Sea</span> System Concepts for Coast Guard Missions</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Young, Larry A.</p> <p>2005-01-01</p> <p>A number of small autonomous <span class="hlt">air/sea</span> system concepts are outlined in this paper that support and enhance U.S. Coast Guard missions. These concepts draw significantly upon technology investments made by NASA in the area of uninhabited aerial vehicles and robotic/intelligent systems. Such concepts should be considered notional elements of a greater as-yet-not-defined robotic system-of-systems designed to enable unparalleled maritime safety and security.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.8859G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.8859G"><span>Relationship between meteorological phenomena and <span class="hlt">air</span> pollution in an urbanized and industrialized coastal area in northern France</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gengembre, Cyril; Zhang, Shouwen; Dieudonné, Elsa; Sokolov, Anton; Augustin, Patrick; Riffault, Véronique; Dusanter, Sébastien; Fourmentin, Marc; Delbarre, Hervé</p> <p>2016-04-01</p> <p>Impacts of global climate evolution are quite uncertain at regional and local scales, especially on <span class="hlt">air</span> pollution. <span class="hlt">Air</span> quality is associated with local atmospheric dynamics at a time scale shorter than a few weeks, while the climate change time scale is on the order of fifty years. To infer consequences of climate evolution on <span class="hlt">air</span> pollution, it is necessary to fill the gap between these different scales. Another challenge is to understand the effect of global warming on the frequency of meteorological phenomena that influence <span class="hlt">air</span> pollution. In this work, we classified meteorological events related to <span class="hlt">air</span> pollution during a one-year long field campaign in Dunkirk (northern France). Owing to its coastal location under urban and industrial exposures, the Dunkirk agglomeration is an interesting area for studying gaseous and aerosols pollutants and their relationship with weather events such as <span class="hlt">sea</span> breezes, fogs, storms and fronts. The <span class="hlt">air</span> quality in the northern region of France is also greatly influenced by highly populated and industrialized cities along the coast of the North <span class="hlt">Sea</span>, and by London and Paris agglomerations. During a field campaign, we used simultaneously a three-dimensional sonic anemometer and a weather station network, along with a scanning Doppler Lidar system to analyse the vertical structure of the atmosphere. An Aerosol Chemical Speciation Monitor enabled investigating the PM1 behaviour during the studied events. <span class="hlt">Air</span> contaminants such as NOx (NO and NO2) were also measured by the regional pollution monitoring network ATMO Nord Pas-de-Calais. The events were identified by finding specific criteria from meteorological and turbulent parameters. Over a hundred cases of <span class="hlt">sea</span> breezes, fog periods, stormy days and atmospheric front passages were investigated. Variations of turbulent parameters (vertical sensible heat <span class="hlt">flux</span> and momentum <span class="hlt">flux</span>) give estimations on the transport and the dispersal of pollutants. As the <span class="hlt">fluxes</span> are weak during fogs, an increase</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.1180C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.1180C"><span>On which timescales do gas transfer velocities control North Atlantic CO2 <span class="hlt">flux</span> variability?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Couldrey, Matthew; Oliver, Kevin; Yool, Andrew; Halloran, Paul; Achterberg, Eric</p> <p>2016-04-01</p> <p>The North Atlantic is an important basin for the global ocean's uptake of anthropogenic and natural carbon dioxide (CO2), but the mechanisms controlling this carbon <span class="hlt">flux</span> are not fully understood. The <span class="hlt">air-sea</span> <span class="hlt">flux</span> of CO2, F, is the product of a gas transfer velocity, k, the <span class="hlt">air-sea</span> CO2concentration gradient, ΔpCO2, 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, ΔpCO2and k both contribute significantly to interannual F variability, but that k is unimportant for multidecadal variability. On some timescale between interannual and multidecadal, gas transfer velocity variability and its associated uncertainty become negligible. Here, we quantify this critical timescale for the first time. Using an ocean model, we determine the importance of k, ΔpCO2and α on a range of timescales. On interannual and shorter timescales, both ΔpCO2and k are important controls on F. In contrast, pentadal to multidecadal North Atlantic <span class="hlt">flux</span> variability is driven almost entirely by ΔpCO2; k contributes less than 25%. Finally, we explore how accurately one can estimate North Atlantic F without a knowledge of non-seasonal k variability, finding it possible for interannual and longer timescales. These findings suggest that continued efforts to better constrain gas transfer velocities are necessary to quantify interannual variability in the North Atlantic carbon sink. However, uncertainty in k variability is unlikely to limit the accuracy of estimates of longer term <span class="hlt">flux</span> variability.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016GBioC..30..787C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GBioC..30..787C"><span>On which timescales do gas transfer velocities control North Atlantic CO2 <span class="hlt">flux</span> variability?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Couldrey, Matthew P.; Oliver, Kevin I. C.; Yool, Andrew; Halloran, Paul R.; Achterberg, Eric P.</p> <p>2016-05-01</p> <p>The North Atlantic is an important basin for the global ocean's uptake of anthropogenic and natural carbon dioxide (CO2), but the mechanisms controlling this carbon <span class="hlt">flux</span> are not fully understood. The <span class="hlt">air-sea</span> <span class="hlt">flux</span> of CO2, F, is the product of a gas transfer velocity, k, the <span class="hlt">air-sea</span> CO2 concentration gradient, ΔpCO2, 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, ΔpCO2 and k both contribute significantly to interannual F variability but that k is unimportant for multidecadal variability. On some timescale between interannual and multidecadal, gas transfer velocity variability and its associated uncertainty become negligible. Here we quantify this critical timescale for the first time. Using an ocean model, we determine the importance of k, ΔpCO2, and α on a range of timescales. On interannual and shorter timescales, both ΔpCO2 and k are important controls on F. In contrast, pentadal to multidecadal North Atlantic <span class="hlt">flux</span> variability is driven almost entirely by ΔpCO2; k contributes less than 25%. Finally, we explore how accurately one can estimate North Atlantic F without a knowledge of nonseasonal k variability, finding it possible for interannual and longer timescales. These findings suggest that continued efforts to better constrain gas transfer velocities are necessary to quantify interannual variability in the North Atlantic carbon sink. However, uncertainty in k variability is unlikely to limit the accuracy of estimates of longer-term <span class="hlt">flux</span> variability.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSAH23A..06C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSAH23A..06C"><span>On which timescales do gas transfer velocities control North Atlantic CO2 <span class="hlt">flux</span> variability?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Couldrey, M.; Oliver, K. I. C.; Yool, A.; Halloran, P. R.; Achterberg, E. P.</p> <p>2016-02-01</p> <p>The North Atlantic is an important basin for the global ocean's uptake of anthropogenic and natural carbon dioxide (CO2), but the mechanisms controlling this carbon <span class="hlt">flux</span> are not fully understood. The <span class="hlt">air-sea</span> <span class="hlt">flux</span> of CO2, F, is the product of a gas transfer velocity, k, the <span class="hlt">air-sea</span> CO2 concentration gradient, ΔpCO2, 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, ΔpCO2 and k both contribute significantly to interannual F variability, but that k is unimportant for multidecadal variability. On some timescale between interannual and multidecadal, gas transfer velocity variability and its associated uncertainty become negligible. Here, we quantify this critical timescale for the first time. Using an ocean model, we determine the importance of k, ΔpCO2 and α on a range of timescales. On interannual and shorter timescales, both ΔpCO2 and k are important controls on F. In contrast, pentadal to multidecadal North Atlantic <span class="hlt">flux</span> variability is driven almost entirely by ΔpCO2; k contributes less than 25%. Finally, we explore how accurately one can estimate North Atlantic F without a knowledge of non-seasonal k variability, finding it possible for interannual and longer timescales. These findings suggest that continued efforts to better constrain gas transfer velocities are necessary to quantify interannual variability in the North Atlantic carbon sink. However, uncertainty in k variability is unlikely to limit the accuracy of estimates of longer term <span class="hlt">flux</span> variability.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004E%26PSL.221...39P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004E%26PSL.221...39P"><span>Variations in productivity and eolian <span class="hlt">fluxes</span> in the northeastern Arabian <span class="hlt">Sea</span> during the past 110 ka</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pourmand, Ali; Marcantonio, Franco; Schulz, Hartmut</p> <p>2004-04-01</p> <p>High-resolution (one to two samples/ka) radionuclide proxy records from core 93KL in the northeastern Arabian <span class="hlt">Sea</span> provide evidence for millennial climate variability over the past 110 ka. We interpret 230Th-normalized 232Th <span class="hlt">fluxes</span> as a proxy for eolian input, and authigenic uranium concentrations as a proxy for past productivity. We attribute orbital and suborbital variations in both proxies to changes in the intensity of the southwest Indian Ocean monsoon. The highest 230Th-normalized 232Th <span class="hlt">fluxes</span> occur at times that are consistent with the timing of the Younger Dryas, Heinrich events 1-7 and cold Dansgaard-Oeschger stadial events recorded in the GISP2 ice core. Such high dust <span class="hlt">fluxes</span> may be due to a weakened southwest monsoon in conjunction with strengthened northwesterlies from the Arabian Peninsula and Mesopotamia. Authigenic uranium concentrations, on the other hand, are highest during warm Dansgaard-Oeschger interstadials when the southwest monsoon is intensified relative to the northwesterly winds. Our results also indicate that on orbital timescales maximum average eolian <span class="hlt">fluxes</span> coincide with the timing of marine isotopic stage (MIS) 2 and 4, while minimum <span class="hlt">fluxes</span> occur during MIS 1, 3 and 5. Although the forcing mechanism(s) controlling suborbital variabilities in monsoonal intensity is still debated, our findings suggest an atmospheric teleconnection between the low-latitude southwest monsoon and North Atlantic climate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=PIA00435&hterms=french+system&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dfrench%2Bsystem','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=PIA00435&hterms=french+system&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dfrench%2Bsystem"><span>Hurricane Frances as Observed by NASA's Spaceborne Atmospheric Infrared Sounder (<span class="hlt">AIRS</span>) and <span class="hlt">Sea</span>Winds</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>2004-01-01</p> <p><p/> This image shows Hurricane Frances as captured by instruments onboard two different satellites: the <span class="hlt">AIRS</span> infrared instrument onboard Aqua, and the <span class="hlt">Sea</span>Winds scatterometer onboard QuikSCAT. Both are JPL-managed instruments. <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 over the ocean. <p/> The red vectors in the image show Frances' surface winds as measured by <span class="hlt">Sea</span>Winds on QuikSCAT. The background colors show the temperature of clouds and surface as viewed in the infrared by <span class="hlt">AIRS</span>, with cooler areas pushing to purple and warmer areas are pushing to red. The color scale on the right gives the temperatures in degrees Kelvin. (The top of the scale, 320 degrees Kelvin, corresponds to 117 degrees Fahrenheit, and the bottom, 180 degrees K is -135 degrees F.) The powerful circulation of this storm is evident from the combined data as well as the development of a clearly-defined central 'eye'. The infrared signal does not penetrate through clouds, so the light blue areas reveal the cold clouds tops associated with strong thunderstorms embedded within the storm. In cloud-free areas the infrared signal comes from Earth's surface, revealing warmer temperatures. <p/> The power of the <span class="hlt">Sea</span>Winds scatterometer data set lies in its ability to generate global maps of wind speed and direction, giving us a snapshot of how the atmosphere is circulating. Weather prediction centers, including the Tropical Prediction Center - a branch of NOAA that monitors the creation of ocean-born storms, use scatterometer data to help it 'see' where these storms are brewing so that warnings can be issued and the storms, with often erratic motions, can be tracked. <p/> While the <span class="hlt">Sea</span>Winds instrument isn't designed to gather hurricane data, having difficulty seeing the surface in heavy rain, it's data can be used in combination with other data sets to give us an insight into these storms. In</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=315915&Lab=NERL&keyword=dependency&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50','EPA-EIMS'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=315915&Lab=NERL&keyword=dependency&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50"><span>Updating <span class="hlt">sea</span> spray aerosol emissions in the Community Multiscale <span class="hlt">Air</span> Quality (CMAQ) model</span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p><span class="hlt">Sea</span> spray aerosols (SSA) impact the particle mass concentration and gas-particle partitioning in coastal environments, with implications for human and ecosystem health. In this study, the Community Multiscale <span class="hlt">Air</span> Quality (CMAQ) model is updated to enhance fine mode SSA emissions,...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMEP21B0874T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMEP21B0874T"><span>Bulk and export production <span class="hlt">fluxes</span> from sediment traps in the Gulf of Aqaba, north 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>Torfstein, A.; Kienast, S.; Shaked, Y.</p> <p>2016-12-01</p> <p>Real time observations of the dynamics between dust input, primary production, and export production in deep oligotrophic waters are extremely rare. This is especially true in the context of the direct response and lag time between nutrient supply (e.g., dust), the oceanic biogeochemical response and the signal transfer from the water to sedimentary record. Here, we present the first direct measurments of bulk and export production <span class="hlt">fluxes</span> in the deep oligotrophic Gulf of Aqaba (GOA), northern Red <span class="hlt">Sea</span>, located between the hyper-arid Sahara and Arabia Deserts. This study is based on a coupled sediment trap array that provides daily- and monthly- resolution since January 2014. This coupled configuration allows for a unique collection of marine particulates, whereby the annual and seasonal patterns can be evaluated in the context of discrete (daily-timescale) events such as abrupt dust storms, floods and biological blooms. The marine organic C and N <span class="hlt">fluxes</span> range annually between 0.02-0.25 and 0.001-0.1 g d-1 m-2, respectively. Both show a sharp decay with depth, corresponding to the "Martin curve" (Martin et al., 1987, Deep-<span class="hlt">Sea</span> Research, 34, 267-285). Importantly, the daily-resolution sampling provides insights to the seasonal increase in export production during the winter and early spring. Rather than a smooth seasonal cycle, this increase is driven by only very few short events, lasting no more than a few days, during which export production increases by an order of magnitude above the baseline. Yet, the nature of these export production "spikes" is non-unique because they reflect different "trigger" events such as dust storms or water column mixing. Accordingly, we present a quantitative evaluation of the observations in the context of coeval dust <span class="hlt">flux</span> records and the physical and chemical configuration of the GOA over the time of sampling period, and present and quantitative mass balance of particle <span class="hlt">fluxes</span> in this deep yet land-locked marine setting.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.5573L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.5573L"><span>Temporal variatiions of <span class="hlt">Sea</span> ice cover in the Baltic <span class="hlt">Sea</span> derived from operational <span class="hlt">sea</span> ice products used in NWP.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lange, Martin; Paul, Gerhard; Potthast, Roland</p> <p>2014-05-01</p> <p><span class="hlt">Sea</span> ice cover is a crucial parameter for surface <span class="hlt">fluxes</span> of heat and moisture over water areas. The isolating effect and the much higher albedo strongly reduces the turbulent exchange of heat and moisture from the surface to the atmosphere and allows for cold and dry <span class="hlt">air</span> mass flow with strong impact on the stability of the whole boundary layer and consequently cloud formation as well as precipitation in the downstream regions. Numerical weather centers as, ECMWF, MetoFrance or DWD use external products to initialize SST and <span class="hlt">sea</span> ice cover in their NWP models. To the knowledge of the author there are mainly two global <span class="hlt">sea</span> ice products well established with operational availability, one from NOAA NCEP that combines measurements with satellite data, and the other from OSI-SAF derived from SSMI/S sensors. The latter one is used in the Ostia product. DWD additionally uses a regional product for the Baltic <span class="hlt">Sea</span> provided by the national center for shipping and hydrografie which combines observations from ships (and icebreakers) for the German part of the Baltic <span class="hlt">Sea</span> and model analysis from the hydrodynamic HIROMB model of the Swedish meteorological service for the rest of the domain. The temporal evolution of the three different products are compared for a cold period in Februar 2012. Goods and bads will be presented and suggestions for a harmonization of strong day to day jumps over large areas are suggested.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20040034110','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20040034110"><span>A Comparison of Latent Heat <span class="hlt">Fluxes</span> over Global Oceans for Four <span class="hlt">Flux</span> Products</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chou, Shu-Hsien; Nelkin, Eric; Ardizzone, Joe; Atlas, Robert M.</p> <p>2003-01-01</p> <p>To improve our understanding of global energy and water cycle variability, and to improve model simulations of climate variations, it is vital to have accurate latent heat <span class="hlt">fluxes</span> (LHF) over global oceans. Monthly LHF, 10-m wind speed (U10m), 10-m specific humidity (Q10h), and <span class="hlt">sea-air</span> humidity difference (Qs-Q10m) of GSSTF2 (version 2 Goddard Satellite-based Surface Turbulent <span class="hlt">Fluxes</span>) over global Oceans during 1992-93 are compared with those of HOAPS (Hamburg Ocean Atmosphere Parameters and <span class="hlt">Fluxes</span> from Satellite Data), NCEP (NCEP/NCAR reanalysis). The mean differences, standard deviations of differences, and temporal correlation of these monthly variables over global Oceans during 1992-93 between GSSTF2 and each of the three datasets are analyzed. The large-scale patterns of the 2yr-mean fields for these variables are similar among these four datasets, but significant quantitative differences are found. The temporal correlation is higher in the northern extratropics than in the south for all variables, with the contrast being especially large for da Silva as a result of more missing ship data in the south. The da Silva has extremely low temporal correlation and large differences with GSSTF2 for all variables in the southern extratropics, indicating that da Silva hardly produces a realistic variability in these variables. The NCEP has extremely low temporal correlation (0.27) and large spatial variations of differences with GSSTF2 for Qs-Q10m in the tropics, which causes the low correlation for LHF. Over the tropics, the HOAPS LHF is significantly smaller than GSSTF2 by approx. 31% (37 W/sq m), whereas the other two datasets are comparable to GSSTF2. This is because the HOAPS has systematically smaller LHF than GSSTF2 in space, while the other two datasets have very large spatial variations of large positive and negative LHF differences with GSSTF2 to cancel and to produce smaller regional-mean differences. Our analyses suggest that the GSSTF2 latent heat <span class="hlt">flux</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017DSRII.143...62H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017DSRII.143...62H"><span><span class="hlt">Flux</span> and stable C and N isotope composition of sinking particles in the Ulleung Basin of the East/Japan <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>Hyun Kwak, Jung; Han, Eunah; Hwang, Jeomshik; Kim, Young, II; Lee, Chung Il; Kang, Chang-Keun</p> <p>2017-09-01</p> <p>Seasonal variability of sinking <span class="hlt">fluxes</span> of total mass (TMF), particulate organic carbon and nitrogen (POC and PON) was examined using sinking particles collected from sediment traps during July 2011 to December 2011, and December 2012 to June 2013 at an offshore channel site; and from November 2013 to August 2014 at a nearshore slope site of the Ulleung Basin in the East/Japan <span class="hlt">Sea</span>. δ13C and δ15N values of sinking particles were measured to elucidate the major export processes of POC and PON. Annual TMF (112-638 g m-2 yr-1) and <span class="hlt">fluxes</span> of POC and PON (9.6-32.1 g C m-2 yr-1 and 1.2-4.5 g N m-2 yr-1, respectively) in the Ulleung Basin corresponded to the upper limit of values reported for other open <span class="hlt">seas</span> and oceans in the world. No great seasonal variability in both quantitative (TMF, and <span class="hlt">fluxes</span> and contents of POC and PON) and qualitative (C/N ratios, and δ13C and δ15N values) estimates of vertical <span class="hlt">fluxes</span> was observed, reflecting a steady standing stock of chlorophyll a in the upper part of water column. Furthermore, high contents of POC and PON and nearly constant δ13C and δ15N values in sinking particles collected in the sediment traps, indicate that primary production in the euphotic zone may be a good predictor of TMF and export <span class="hlt">flux</span> of organic matter. In this regard, our pilot study points out the importance of high annual primary production and low water temperature (<1 °C) beneath the 200-m water depth, which would enable more sinking particles to be preserved during export process by limiting microbial decomposition activity in the water column, in determining the high annual <span class="hlt">flux</span> of sinking particles in the Ulleung Basin (UB). A simple stable isotope mixing model of sinking particles indicates that despite a slight seasonal variation, the contribution of intact phytoplankton to sinking organic <span class="hlt">flux</span> is significant to the POC and PON <span class="hlt">flux</span> in the UB. Further continuous time series sediment trap experiments are proposed to estimate the contribution 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://hdl.handle.net/2060/20140005688','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140005688"><span>Simulation of the Indian Summer Monsoon Using Comprehensive Atmosphere-land Interactions, in the Absence of Two-way <span class="hlt">Air-sea</span> Interactions</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lim, Young-Kwon; Shin, D. W.; Cocke, Steven; Kang, Sung-Dae; Kim, Hae-Dong</p> <p>2011-01-01</p> <p>Community Land Model version 2 (CLM2) as a comprehensive land surface model and a simple land surface model (SLM) were coupled to an atmospheric climate model to investigate the role of land surface processes in the development and the persistence of the South Asian summer monsoon. Two-way <span class="hlt">air-sea</span> interactions were not considered in order to identify the reproducibility of the monsoon evolution by the comprehensive land model, which includes more realistic vertical soil moisture structures, vegetation and 2-way atmosphere-land interactions at hourly intervals. In the monsoon development phase (May and June). comprehensive land-surface treatment improves the representation of atmospheric circulations and the resulting convergence/divergence through the improvements in differential heating patterns and surface energy <span class="hlt">fluxes</span>. Coupling with CLM2 also improves the timing and spatial distribution of rainfall maxima, reducing the seasonal rainfall overestimation by approx.60 % (1.8 mm/d for SLM, 0.7 mm/dI for CLM2). As for the interannual variation of the simulated rainfall, correlation coefficients of the Indian seasonal rainfall with observation increased from 0.21 (SLM) to 0.45 (CLM2). However, in the mature monsoon phase (July to September), coupling with the CLM2 does not exhibit a clear improvement. In contrast to the development phase, latent heat <span class="hlt">flux</span> is underestimated and sensible heat <span class="hlt">flux</span> and surface temperature over India are markedly overestimated. In addition, the moisture <span class="hlt">fluxes</span> do not correlate well with lower-level atmospheric convergence, yielding correlation coefficients and root mean square errors worse than those produced by coupling with the SLM. A more realistic representation of the surface temperature and energy <span class="hlt">fluxes</span> is needed to achieve an improved simulation for the mature monsoon period.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.2333B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.2333B"><span>On the importance of high-frequency <span class="hlt">air</span>-temperature fluctuations for spectroscopic corrections of open-path carbon dioxide <span class="hlt">flux</span> measurements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bogoev, Ivan; Helbig, Manuel; Sonnentag, Oliver</p> <p>2015-04-01</p> <p>A growing number of studies report systematic differences in CO2 <span class="hlt">flux</span> estimates obtained with the two main types of gas analyzers: compared to eddy-covariance systems based on closed-path (CP) gas analyzers, systems with open-path (OP) gas analyzers systematically overestimate CO2 uptake during daytime periods with high positive sensible heat <span class="hlt">fluxes</span>, while patterns for differences in nighttime CO2 exchange are less obvious. These biases have been shown to correlate with the sign and the magnitude of the sensible heat <span class="hlt">flux</span> and to introduce large uncertainties when calculating annual CO2 budgets. In general, CP and OP gas analyzers commonly used to measure the CO2 density in the atmosphere operate on the principle of infrared light absorption approximated by Beer-Lambert's law. Non-dispersive interference-based optical filter elements are used to select spectral bands with strong attenuation of light transmission, characteristic to the gas of interest. The intensity of the light passing through the optical sensing path depends primarily on the amount of absorber gas in the measurement volume. Besides the density of the gas, barometric pressure and <span class="hlt">air</span> temperature are additional factors affecting the strength and the half-width of the absorption lines. These so-called spectroscopic effects are accounted for by measuring barometric pressure and <span class="hlt">air</span> temperature in the sensing path and scaling the light-intensity measurements before applying the calibration equation. This approach works well for CP gas analyzers with an intake tube that acts as a low-pass filter on fast <span class="hlt">air</span>-temperature fluctuations. Low-frequency response temperature sensors in the measurement cell are therefore sufficient to account for spectroscopic temperature effects. In contrast, OP gas analyzers are exposed to high-frequency <span class="hlt">air</span>-temperature fluctuations associated with the atmospheric surface-layer turbulent heat exchange. If not corrected adequately, these fast <span class="hlt">air</span>-temperature variations can cause</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1014432','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1014432"><span>Data Serving for ASIRI Participants</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2015-09-30</p> <p>Indian satellite INSAT 3D visible satellite image (April 24, 2015) with select WHOI mooring atmospheric and <span class="hlt">air</span>- <span class="hlt">sea</span> <span class="hlt">fluxes</span> compared the NASA MERRA...evaluated the Bay of Bengal <span class="hlt">fluxes</span> from field studies against a number of re-analyses (ECMWF, NCEP-1 and NCEP-2, NASA MERRA), and is currently...<span class="hlt">fluxes</span> from the <span class="hlt">air-sea</span> <span class="hlt">flux</span> WHOI mooring at 18N and atmospheric reanalysis <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> from NASA MERRA for a week in April 2015. It also shows the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012PhDT........17F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012PhDT........17F"><span>Evaluation of bulk heat <span class="hlt">fluxes</span> from atmospheric datasets</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Farmer, Benton</p> <p></p> <p>Heat <span class="hlt">fluxes</span> at the <span class="hlt">air-sea</span> interface are an important component of the Earth's heat budget. In addition, they are an integral factor in determining the <span class="hlt">sea</span> surface temperature (SST) evolution of the oceans. Different representations of these <span class="hlt">fluxes</span> are used in both the atmospheric and oceanic communities for the purpose of heat budget studies and, in particular, for forcing oceanic models. It is currently difficult to quantify the potential impact varying heat <span class="hlt">flux</span> representations have on the ocean response. In this study, a diagnostic tool is presented that allows for a straightforward comparison of surface heat <span class="hlt">flux</span> formulations and atmospheric data sets. Two variables, relaxation time (RT) and the apparent temperature (T*), are derived from the linearization of the bulk formulas. They are then calculated to compare three bulk formulae and five atmospheric datasets. Additionally, the linearization is expanded to the second order to compare the amount of residual <span class="hlt">flux</span> present. It is found that the use of a bulk formula employing a constant heat transfer coefficient produces longer relaxation times and contains a greater amount of residual <span class="hlt">flux</span> in the higher order terms of the linearization. Depending on the temperature difference, the residual <span class="hlt">flux</span> remaining in the second order and above terms can reach as much as 40--50% of the total residual on a monthly time scale. This is certainly a non-negligible residual <span class="hlt">flux</span>. In contrast, a bulk formula using a stability and wind dependent transfer coefficient retains much of the total <span class="hlt">flux</span> in the first order term, as only a few percent remain in the residual <span class="hlt">flux</span>. Most of the difference displayed among the bulk formulas stems from the sensitivity to wind speed and the choice of a constant or spatially varying transfer coefficient. Comparing the representation of RT and T* provides insight into the differences among various atmospheric datasets. In particular, the representations of the western boundary current, upwelling</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70179159','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70179159"><span>Dissolved methane in the Beaufort <span class="hlt">Sea</span> and the Arctic Ocean, 1992-2009; sources and atmospheric <span class="hlt">flux</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>Lorenson, Thomas D.; Greinert, Jens; Coffin, Richard B.</p> <p>2016-01-01</p> <p>Methane concentration and isotopic composition was measured in ice-covered and ice-free waters of the Arctic Ocean during eleven surveys spanning the years of 1992-1995 and 2009. During ice-free periods, methane <span class="hlt">flux</span> from the Beaufort shelf varies from 0.14 to 0.43 mg CH4 m-2 day-1. Maximum <span class="hlt">fluxes</span> from localized areas of high methane concentration are up to 1.52 mg CH4 m-2 day-1. Seasonal buildup of methane under ice can produce short-term <span class="hlt">fluxes</span> of methane from the Beaufort shelf that varies from 0.28 to 1.01 to mg CH4 m-2 day-1. Scaled-up estimates of minimum methane <span class="hlt">flux</span> from the Beaufort <span class="hlt">Sea</span> and pan-Arctic shelf for both ice-free and ice-covered periods range from 0.02 Tg CH4 yr-1 and 0.30 Tg CH4 yr-1 respectively to maximum <span class="hlt">fluxes</span> of 0.18 Tg CH4 yr-1 and 2.2 Tg CH4 yr-1 respectively. A methane <span class="hlt">flux</span> of 0.36 Tg CH4 yr-1from the deep Arctic Ocean was estimated using data from 1993-94. The <span class="hlt">flux</span> can be as much as 2.35 Tg CH4 yr-1 estimated from maximum methane concentrations and wind speeds of 12 m/s, representing only 0.42% of the annual atmospheric methane budget of ~560 Tg CH4 yr-1. There were no significant changes in methane <span class="hlt">fluxes</span> during the time period of this study. Microbial methane sources predominate with minor influxes from thermogenic methane offshore Prudhoe Bay and the Mackenzie River delta and may include methane from gas hydrate. Methane oxidation is locally important on the shelf and is a methane sink in the deep Arctic Ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1130373','SCIGOV-DOEDE'); return false;" href="https://www.osti.gov/servlets/purl/1130373"><span>GSOD Based Daily Global Mean Surface Temperature and Mean <span class="hlt">Sea</span> Level <span class="hlt">Air</span> Pressure (1982-2011)</span></a></p> <p><a target="_blank" href="http://www.osti.gov/dataexplorer">DOE Data Explorer</a></p> <p>Xuan Shi, Dali Wang</p> <p>2014-05-05</p> <p>This data product contains all the gridded data set at 1/4 degree resolution in ASCII format. Both mean temperature and mean <span class="hlt">sea</span> level <span class="hlt">air</span> pressure data are available. It also contains the GSOD data (1982-2011) from NOAA site, contains station number, location, temperature and pressures (<span class="hlt">sea</span> level and station level). The data package also contains information related to the data processing methods</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011GBioC..25.1004L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011GBioC..25.1004L"><span>An updated climatology of surface dimethlysulfide concentrations and emission <span class="hlt">fluxes</span> in the global ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lana, A.; Bell, T. G.; Simó, R.; Vallina, S. M.; Ballabrera-Poy, J.; Kettle, A. J.; Dachs, J.; Bopp, L.; Saltzman, E. S.; Stefels, J.; Johnson, J. E.; Liss, P. S.</p> <p>2011-03-01</p> <p>The potentially significant role of the biogenic trace gas dimethylsulfide (DMS) in determining the Earth's radiation budget makes it necessary to accurately reproduce seawater DMS distribution and quantify its global <span class="hlt">flux</span> across the <span class="hlt">sea/air</span> interface. Following a threefold increase of data (from 15,000 to over 47,000) in the global surface ocean DMS database over the last decade, new global monthly climatologies of surface ocean DMS concentration and <span class="hlt">sea-to-air</span> emission <span class="hlt">flux</span> are presented as updates of those constructed 10 years ago. Interpolation/extrapolation techniques were applied to project the discrete concentration data onto a first guess field based on Longhurst's biogeographic provinces. Further objective analysis allowed us to obtain the final monthly maps. The new climatology projects DMS concentrations typically in the range of 1-7 nM, with higher levels occurring in the high latitudes, and with a general trend toward increasing concentration in summer. The increased size and distribution of the observations in the DMS database have produced in the new climatology substantially lower DMS concentrations in the polar latitudes and generally higher DMS concentrations in regions that were severely undersampled 10 years ago, such as the southern Indian Ocean. Using the new DMS concentration climatology in conjunction with state-of-the-art parameterizations for the <span class="hlt">sea/air</span> gas transfer velocity and climatological wind fields, we estimate that 28.1 (17.6-34.4) Tg of sulfur are transferred from the oceans into the atmosphere annually in the form of DMS. This represents a global emission increase of 17% with respect to the equivalent calculation using the previous climatology. This new DMS climatology represents a valuable tool for atmospheric chemistry, climate, and Earth System models.</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 5.0.2</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 5.0.2. Geoscientific Model Development. Copernicus Publications, Katlenburg-Lindau, GERMANY, 8: 3733-3746, (2015).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19910063773&hterms=1087&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3D%2526%25231087','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19910063773&hterms=1087&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3D%2526%25231087"><span>Antarctic <span class="hlt">Sea</span> ice variations and seasonal <span class="hlt">air</span> temperature relationships</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Weatherly, John W.; Walsh, John E.; Zwally, H. J.</p> <p>1991-01-01</p> <p>Data through 1987 are used to determine the regional and seasonal dependencies of recent trends of Antarctic temperature and <span class="hlt">sea</span> ice. Lead-lag relationships involving regional <span class="hlt">sea</span> ice and <span class="hlt">air</span> temperature are systematically evaluated, with an eye toward the ice-temperature feedbacks that may influence climatic change. Over the 1958-1087 period the temperature trends are positive in all seasons. For the 15 years (l973-l987) for which ice data are available, the trends are predominantly positive only in winter and summer, and are most strongly positive over the Antarctic Peninsula. The spatially aggregated trend of temperature for this latter period is small but positive, while the corresponding trend of ice coverage is small but negative. Lag correlations between seasonal anomalies of the two variables are generally stronger with ice lagging the summer temperatures and with ice leading the winter temperatures. The implication is that summer temperatures predispose the near-surface waters to above-or below-normal ice coverage in the following fall and winter.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018DSRI..133...59R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018DSRI..133...59R"><span>Sources, variability and fate of freshwater in the Bellingshausen <span class="hlt">Sea</span>, Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Regan, Heather C.; Holland, Paul R.; Meredith, Michael P.; Pike, Jennifer</p> <p>2018-03-01</p> <p>During the second half of the twentieth century, the Antarctic Peninsula was subjected to a rapid increase in <span class="hlt">air</span> temperatures. This was accompanied by a reduction in <span class="hlt">sea</span> ice extent, increased precipitation and a dramatic retreat of glaciers associated with an increase in heat <span class="hlt">flux</span> from deep ocean water masses. Isotopic tracers have been used previously to investigate the relative importance of the different freshwater sources to the adjacent Bellingshausen <span class="hlt">Sea</span> (BS), but the data coverage is strongly biased toward summer. Here we use a regional model to investigate the ocean's response to the observed changes in its different freshwater inputs (<span class="hlt">sea</span> ice melt/freeze, precipitation, evaporation, iceberg/glacier melt, and ice shelf melt). The model successfully recreates BS water masses and performs well against available freshwater data. By tracing the sources and pathways of the individual components of the freshwater budget, we find that <span class="hlt">sea</span> ice dominates seasonal changes in the total freshwater content and <span class="hlt">flux</span>, but all sources make a comparable contribution to the annual-mean. Interannual variability is dominated by <span class="hlt">sea</span> ice and precipitation. Decadal trends in the salinity and stratification of the ocean are investigated, and a 20-year surface freshening from 1992 to 2011 is found to be predominantly driven by decreasing autumn <span class="hlt">sea</span> ice growth. These findings will help to elucidate the role of freshwater in driving circulation and water column structure changes in this climatically-sensitive region.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2000BoLMe..95..271O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2000BoLMe..95..271O"><span>Stability Effects on Heat and Moisture <span class="hlt">Fluxes</span> at <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>Oost, W. A.; Jacobs, C. M. J.; van Oort, C.</p> <p></p> <p>During the 1996 ASGAMAGE experiment we measured windspeed, <span class="hlt">air</span> temperature Ta, watertemperature Ts, humidity and the momentum,heat and moisture <span class="hlt">fluxes</span> at a research platform offthe Dutch coast. For each quantity we used several(sets of) instruments simultaneously. This allowed usto make an extensive assessment of the quality of themeasurements and to find optimal values for thevarious quantities for each run. From these values wecalculated CH and CE, theStanton and Dalton numbers, and reduced them to 10-mheight and neutral conditions. For this reductionwe made a separate analysis for the effect ofinclusion or non-inclusion of the assumption that theroughness length for heat or moisture is the same forthe neutral and non-neutral cases. Differences inthe reduced data due to this assumption turned out tobe well within the measurement error.For CH we distinguished three separategroups of data: stable (A), unstable witha s (B) and unstablewith thetas;a > s (C), with indicating the potential temperature.The stable data separate into two groups, depending onwater temperature and/or the wave field. The data ofgroup B showed a relation with wave age. The data ofgroup C consistently gave negative values forCH, a result that might indicate conversion oflatent heat into sensible heat through condensation ofwater vapour just above the water surface. An attemptto re-analyse the data in terms of density <span class="hlt">fluxes</span>,combining the effects of heat and moisture, still gavenegative transfer coefficients for group C.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002EGSGA..27.3907W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002EGSGA..27.3907W"><span>Fram Strait: Atmospheric Forcing of The <span class="hlt">Sea</span> Ice <span class="hlt">Flux</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Widell, K.; Østerhus, S.; Gammelsrød, T.</p> <p></p> <p>Measuring the magnitude and variability of the ice and freshwater <span class="hlt">flux</span> through Fram Strait is an important element in understanding climate variability in the Arctic. Since the major part of the ice and freshwater that leaves the Arctic passes through Fram Strait, this passage can be considered a key area for estimating the net ice production in the Arctic Ocean. In 1990, the Norwegian Polar Institute (NPI) started a monitoring program in the strait, most years by means of two moorings with Upward Looking Sonars (ULS) measuring ice draft. From 1995 and on, these moorings were also equipped with Doppler Current Meters (DCM) to measure the ice velocity. These measurements give an opportunity to investigate the different forces affecting ice motion in the strait. Maximum correlation coefficient between atmospheric <span class="hlt">sea</span> level pressure (from NCEP/NCAR reanalysed data) and southward ice velocity is found when using the cross strait pressure difference along 80N between 10W and 5E (R = 0.72) consider- ing monthly means. Subtracting current velocity at 50 m depth (also measured by the DCM) from ice velocity improves the correlation to R = 0.84. This gives insight in the relative importance of current and wind on the ice motion, and indicates that pressure data can be used to make fairly good estimates of the ice velocity in the strait. In combination with data on ice thickness and ice stream width, this result is used to calculate the ice volume transport. By making assumptions on the parameters in- volved, the time series is extended back to 1948, the start of the pressure record. This time series will be presented and compared to literature, and annual and seasonal vari- ation of the ice <span class="hlt">flux</span> will be discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19810038158&hterms=Parkinsons+circulation&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DParkinsons%2Bcirculation','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19810038158&hterms=Parkinsons+circulation&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DParkinsons%2Bcirculation"><span><span class="hlt">Sea</span> ice simulations based on fields generated by the GLAS GCM. [Goddard Laboratory for Atmospheric Sciences General Circulation Model</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Parkinson, C. L.; Herman, G. F.</p> <p>1980-01-01</p> <p>The GLAS General Circulation Model (GCM) was applied to the four-month simulation of the thermodynamic part of the Parkinson-Washington <span class="hlt">sea</span> ice model using atmospheric boundary conditions. The <span class="hlt">sea</span> ice thickness and distribution were predicted for the Jan. 1-Apr. 30 period using the GCM-fields of solar and infrared radiation, specific humidity and <span class="hlt">air</span> temperature at the surface, and snow accumulation; the sensible heat and evaporative surface <span class="hlt">fluxes</span> were consistent with the ground temperatures produced by the ice model and the <span class="hlt">air</span> temperatures determined by the atmospheric concept. It was concluded that the Parkinson-Washington <span class="hlt">sea</span> ice model results in acceptable ice concentrations and thicknesses when used with GLAS GCM for the Jan.-Apr. period suggesting the feasibility of fully coupled ice-atmosphere simulations with these two approaches.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19980021232','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19980021232"><span><span class="hlt">Sea</span> Ice on the Southern Ocean</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Jacobs, Stanley S.</p> <p>1998-01-01</p> <p>Year-round satellite records of <span class="hlt">sea</span> ice distribution now extend over more than two decades, providing a valuable tool to investigate related characteristics and circulations in the Southern Ocean. We have studied a variety of features indicative of oceanic and atmospheric interactions with Antarctic <span class="hlt">sea</span> ice. In the Amundsen & Bellingshausen <span class="hlt">Seas</span>, <span class="hlt">sea</span> ice extent was found to have decreased by approximately 20% from 1973 through the early 1990's. This change coincided with and probably contributed to recently warmer surface conditions on the west side of the Antarctic Peninsula, where <span class="hlt">air</span> temperatures have increased by approximately 0.5 C/decade since the mid-1940's. The <span class="hlt">sea</span> ice decline included multiyear cycles of several years in length superimposed on high interannual variability. The retreat was strongest in summer, and would have lowered the regional mean ice thickness, with attendant impacts upon vertical heat <span class="hlt">flux</span> and the formation of snow ice and brine. The cause of the regional warming and loss of <span class="hlt">sea</span> ice is believed to be linked to large-scale circulation changes in the atmosphere and ocean. At the eastern end of the Weddell Gyre, the Cosmonaut Polyna revealed greater activity since 1986, a recurrence pattern during recent winters and two possible modes of formation. Persistence in polynya location was noted off Cape Ann, where the coastal current can interact more strongly with the Antarctic Circumpolar Current. As a result of vorticity conservation, locally enhanced upwelling brings warmer deep water into the mixed layer, causing divergence and melting. In the Ross <span class="hlt">Sea</span>, ice extent fluctuates over periods of several years, with summer minima and winter maxima roughly in phase. This leads to large interannual cycles of <span class="hlt">sea</span> ice range, which correlate positively with meridinal winds, regional <span class="hlt">air</span> temperatures and subsequent shelf water salinities. Deep shelf waters display considerable interannual variability, but have freshened by approximately 0.03/decade</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002CSR....22..779D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002CSR....22..779D"><span><span class="hlt">Sea</span> level oscillations in coastal waters of the Buenos <span class="hlt">Aires</span> province, Argentina</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dragani, W. C.; Mazio, C. A.; Nuñez, M. N.</p> <p>2002-03-01</p> <p><span class="hlt">Sea</span> level oscillations, with periods ranging from a few minutes to almost 2 h, have been observed at various tide stations located on the coast of Buenos <span class="hlt">Aires</span>. Simultaneous records of <span class="hlt">sea</span> level elevation measured in Mar de Ajó, Pinamar and Mar del Plata during 1982 have been spectrally analyzed. Significant spectral energy has been detected between 0.85 and 4.69 cycles per hour (cph) and the most energetic peaks have frequencies between 1.17 and 1.49 cph. Spectra, coherence, and phase difference have been analyzed for the most energetic event of the year. During that event, the most intensive spectral peak is at 1.17 cph for Mar de Ajó and Pinamar, and at 1.49 cph for Mar del Plata. Simultaneous total energy peaks at Mar de Ajó, Pinamar and Mar del Plata, and the coherence function estimated between Mar de Ajó and Pinamar suggests that <span class="hlt">sea</span> level oscillations could be a regional phenomenon. The analyzed data suggest that <span class="hlt">sea</span> level oscillations could be forced by atmospheric gravity waves associated with frontal passages.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016OcDyn..66..917A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016OcDyn..66..917A"><span>Surface wave effects on water temperature in the Baltic <span class="hlt">Sea</span>: simulations with the coupled NEMO-WAM model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Alari, Victor; Staneva, Joanna; Breivik, Øyvind; Bidlot, Jean-Raymond; Mogensen, Kristian; Janssen, Peter</p> <p>2016-08-01</p> <p>Coupled circulation (NEMO) and wave model (WAM) system was used to study the effects of surface ocean waves on water temperature distribution and heat exchange at regional scale (the Baltic <span class="hlt">Sea</span>). Four scenarios—including Stokes-Coriolis force, <span class="hlt">sea</span>-state dependent energy <span class="hlt">flux</span> (additional turbulent kinetic energy due to breaking waves), <span class="hlt">sea</span>-state dependent momentum <span class="hlt">flux</span> and the combination these forcings—were simulated to test the impact of different terms on simulated temperature distribution. The scenario simulations were compared to a control simulation, which included a constant wave-breaking coefficient, but otherwise was without any wave effects. The results indicate a pronounced effect of waves on surface temperature, on the distribution of vertical temperature and on upwelling's. Overall, when all three wave effects were accounted for, did the estimates of temperature improve compared to control simulation. During the summer, the wave-induced water temperature changes were up to 1 °C. In northern parts of the Baltic <span class="hlt">Sea</span>, a warming of the surface layer occurs in the wave included simulations in summer months. This in turn reduces the cold bias between simulated and measured data, e.g. the control simulation was too cold compared to measurements. The warming is related to <span class="hlt">sea</span>-state dependent energy <span class="hlt">flux</span>. This implies that a spatio-temporally varying wave-breaking coefficient is necessary, because it depends on actual <span class="hlt">sea</span> state. Wave-induced cooling is mostly observed in near-coastal areas and is the result of intensified upwelling in the scenario, when Stokes-Coriolis forcing is accounted for. Accounting for <span class="hlt">sea</span>-state dependent momentum <span class="hlt">flux</span> results in modified heat exchange at the water-<span class="hlt">air</span> boundary which consequently leads to warming of surface water compared to control simulation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.U13B..13W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.U13B..13W"><span>Implementation of an acoustic-based methane <span class="hlt">flux</span> estimation methodology in the Eastern Siberian Arctic <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>Weidner, E. F.; Weber, T. C.; Mayer, L. A.</p> <p>2017-12-01</p> <p>Quantifying methane <span class="hlt">flux</span> originating from marine seep systems in climatically sensitive regions is of critically importance for current and future climate studies. Yet, the methane contribution from these systems has been difficult to estimate given the broad spatial scale of the ocean and the heterogeneity of seep activity. One such region is the Eastern Siberian Arctic <span class="hlt">Sea</span> (ESAS), where bubble release into the shallow water column (<40 meters average depth) facilitates transport of methane to the atmosphere without oxidation. Quantifying the current seep methane <span class="hlt">flux</span> from the ESAS is necessary to understand not only the total ocean methane budget, but also to provide baseline estimates against which future climate-induced changes can be measured. At the 2016 AGU fall meeting, we presented a new acoustic-based <span class="hlt">flux</span> methodology using a calibrated broadband split-beam echosounder. The broad (14-24 kHz) bandwidth provides a vertical resolution of 10 cm, making possible the identification of single bubbles. After calibration using 64 mm copper sphere of known backscatter, the acoustic backscatter of individual bubbles is measured and compared to analytical models to estimate bubble radius. Additionally, bubbles are precisely located and traced upwards through the water column to estimate rise velocity. The combination of radius and rise velocity allows for gas <span class="hlt">flux</span> estimation. Here, we follow up with the completed implementation of this methodology applied to the Herald Canyon region of the western ESAS. From the 68 recognized seeps, bubble radii and rise velocity were computed for more than 550 individual bubbles. The range of bubble radii, 1-6 mm, is comparable to those published by other investigators, while the radius dependent rise velocities are consistent with published models. Methane <span class="hlt">flux</span> for the Herald Canyon region was estimated by extrapolation from individual seep <span class="hlt">flux</span> values.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOS.A33A..06D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOS.A33A..06D"><span>-> <span class="hlt">Air</span> entrainment and bubble statistics in three-dimensional breaking waves</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Deike, L.; Popinet, S.; Melville, W. K.</p> <p>2016-02-01</p> <p>Wave breaking in the ocean is of fundamental importance for quantifying wave dissipation and <span class="hlt">air-sea</span> interaction, including gas and momentum exchange, and for improving <span class="hlt">air-sea</span> <span class="hlt">flux</span> parametrizations for weather and climate models. Here we investigate <span class="hlt">air</span> entrainment and bubble statistics in three-dimensional breaking waves through direct numerical simulations of the two-phase <span class="hlt">air</span>-water flow using the Open Source solver Gerris. As in previous 2D simulations, the dissipation due to breaking is found to be in good agreement with previous experimental observations and inertial-scaling arguments. For radii larger than the Hinze scale, the bubble size distribution is found to follow a power law of the radius, r-10/3 and to scale linearly with the time dependent turbulent dissipation rate during the active breaking stage. The time-averaged bubble size distribution is found to follow the same power law of the radius and to scale linearly with the wave dissipation rate per unit length of breaking crest. We propose a phenomenological turbulent bubble break-up model that describes the numerical results and existing experimental results.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS42A..08S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS42A..08S"><span>Southern Ocean Carbon Dioxide and Oxygen <span class="hlt">Fluxes</span> Detected by SOCCOM Biogeochemical Profiling Floats</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sarmiento, J. L.; Bushinksy, S.; Gray, A. R.</p> <p>2016-12-01</p> <p>The Southern Ocean is known to play an important role in the global carbon cycle, yet historically our measurements of this remote region have been sparse and heavily biased towards summer. Here we present new estimates of <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> of carbon dioxide and oxygen calculated with measurements from autonomous biogeochemical profiling floats. At high latitudes in and southward of the Antarctic Circumpolar Current, we find a significant <span class="hlt">flux</span> of CO2 from the ocean to the atmosphere during 2014-2016, which is particularly enhanced during winter months. These results suggest that previous estimates may be biased towards stronger Southern Ocean CO2 uptake due to undersampling in winter. We examine various implications of having a source of CO2 that is higher than previous estimates. We also find that CO2:O2 <span class="hlt">flux</span> ratios north of the Subtropical Front are positive, consistent with the <span class="hlt">fluxes</span> being driven by changes in solubility, while south of the Polar Front biological processes and upwelling of deep water combine to produce a negative CO2:O2 <span class="hlt">flux</span> ratio.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013CorRe..32..239W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013CorRe..32..239W"><span>Spatiotemporal variations in CO2 <span class="hlt">flux</span> in a fringing reef simulated using a novel carbonate system dynamics model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Watanabe, A.; Yamamoto, T.; Nadaoka, K.; Maeda, Y.; Miyajima, T.; Tanaka, Y.; Blanco, A. C.</p> <p>2013-03-01</p> <p>A carbonate system dynamics (CSD) model was developed in a fringing reef on the east coast of Ishigaki Island, southwest Japan, by incorporating organic and inorganic carbon <span class="hlt">fluxes</span> (photosynthesis and calcification), <span class="hlt">air-sea</span> gas exchanges, and benthic cover of coral and seagrass into a three-dimensional hydrodynamic model. The CSD model could reproduce temporal variations in dissolved inorganic carbon (DIC) and total alkalinity in coral zones, but not in seagrass meadows. The poor reproduction in seagrass meadows can be attributed to significant contributions of submarine groundwater discharge as well as misclassification of remotely sensed megabenthos in this area. In comparison with offshore areas, the reef acted as a CO2 sink during the observation period when it was averaged over 24 h. The CSD model also indicated large spatiotemporal differences in the carbon dioxide (CO2) sink/source, possibly related to hydrodynamic features such as effective offshore seawater exchange and neap/spring tidal variation. This suggests that the data obtained from a single point observation may lead to misinterpretation of the overall trend and thus should be carefully considered. The model analysis also showed that the advective <span class="hlt">flux</span> of DIC from neighboring grids is several times greater than local biological <span class="hlt">flux</span> of DIC and is three orders of magnitude greater than the <span class="hlt">air-sea</span> gas <span class="hlt">flux</span> at the coral zone. Sensitivity tests in which coral or seagrass covers were altered revealed that the CO2 sink potential was much more sensitive to changes in coral cover than seagrass cover.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_20 --> <div id="page_21" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="401"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29195203','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29195203"><span>Environmental forcing on the <span class="hlt">flux</span> of organic-walled dinoflagellate cysts in recent sediments from a subtropical lagoon in the Gulf of California.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Cuellar-Martinez, Tomasa; Alonso-Rodríguez, Rosalba; Ruiz-Fernández, Ana Carolina; de Vernal, Anne; Morquecho, Lourdes; Limoges, Audrey; Henry, Maryse; Sanchez-Cabeza, Joan-Albert</p> <p>2018-04-15</p> <p>To evaluate the relationship of changes in organic-walled dinoflagellate cyst (dinocyst) <span class="hlt">fluxes</span> to sediments with environmental variables (<span class="hlt">air</span> and <span class="hlt">sea</span> surface temperatures, El Niño conditions, rainfall, and terrigenous index), cyst assemblages were analyzed in a 210 Pb-dated sediment core (~100years) from the pristine San José Lagoon (San José Island, SW Gulf of California). The dinocyst abundance ranged from 3784 to 25,108cystsg -1 and <span class="hlt">fluxes</span> were of the order of 10 3 -10 4 cystscm -2 yr -1 . Lingulodinium machaerophorum, Polysphaeridium zoharyi and Spiniferites taxa accounted for 96% of the total dinocyst assemblages, and the abundances of these species increased towards the core surface. P. zoharyi <span class="hlt">fluxes</span> increased from about 1965 onwards. Redundancy analyses, showed that mean minimum <span class="hlt">air</span> temperature and terrigenous index were the key factors governing dinocyst <span class="hlt">fluxes</span>. In this study, dinocyst <span class="hlt">fluxes</span> of dominant taxa had responded to changes in climate-dependent environmental variables during the past ~20years; this may also be the case in other subtropical coastal lagoons. Copyright © 2017 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002DSRII..49.1623S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002DSRII..49.1623S"><span>Carbon export <span class="hlt">fluxes</span> in the Southern Ocean: results from inverse modeling and comparison with satellite-based estimates</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schlitzer, Reiner</p> <p></p> <p>The use of dissolved nutrients and carbon for photosynthesis in the euphotic zone and the subsequent downward transport of particulate and dissolved organic material strongly affect carbon concentrations in surface water and thus the <span class="hlt">air-sea</span> exchange of CO 2. Efforts to quantify the downward carbon <span class="hlt">flux</span> for the whole ocean or on basin-scales are hampered by the sparseness of direct productivity or <span class="hlt">flux</span> measurements. Here, a global ocean circulation, biogeochemical model is used to determine rates of export production and vertical carbon <span class="hlt">fluxes</span> in the Southern Ocean. The model exploits the existing large sets of hydrographic, oxygen, nutrient and carbon data that contain information on the underlying biogeochemical processes. The model is fitted to the data by systematically varying circulation, <span class="hlt">air-sea</span> <span class="hlt">fluxes</span>, production, and remineralization rates simultaneously. Use of the adjoint method yields model property simulations that are in very good agreement with measurements. In the model, the total integrated export <span class="hlt">flux</span> of particulate organic matter necessary for the realistic reproduction of nutrient data is significantly larger than export estimates derived from primary productivity maps. Of the 10,000 TgC yr -1(10 GtC yr -1) required globally, the Southern Ocean south of 30°S contributes about 3000 TgC yr -1 (33%), most of it occurring in a zonal belt along the Antarctic Circumpolar Current and in the Peru, Chile and Namibia coastal upwelling regions. The export <span class="hlt">flux</span> of POC for the area south of 50°S amounts to 1000±210 TgC yr -1, and the particle <span class="hlt">flux</span> in 1000 m for the same area is 115±20 TgC yr -1. Unlike for the global ocean, the contribution of the downward <span class="hlt">flux</span> of dissolved organic carbon is significant in the Southern Ocean in the top 500 m of the water column. Comparison with satellite-based productivity estimates (CZCS and <span class="hlt">Sea</span>WiFS) shows a relatively good agreement over most of the ocean except for the Southern Ocean south of 50°S, where the model</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20000037971&hterms=round&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dround','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20000037971&hterms=round&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dround"><span>Year-Round Pack Ice in the Weddell <span class="hlt">Sea</span>, Antarctica: Response and Sensitivity to Atmospheric and Oceanic Forcing</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Geiger, Cathleen A.; Ackley, Stephen F.; Hibler, William D., III</p> <p>1997-01-01</p> <p>Using a dynamic-thermodynamic numerical <span class="hlt">sea</span>-ice model, external oceanic and atmospheric forcings on <span class="hlt">sea</span> ice in the Weddell <span class="hlt">Sea</span> are examined to identify physical processes associated with the seasonal cycle of pack ice, and to identify further the parameters that coupled models need to consider in predicting the response of the pack ice to climate and ocean-circulation changes. In agreement with earlier studies, the primary influence on the winter ice-edge maximum extent is <span class="hlt">air</span> temperature. Ocean heat <span class="hlt">flux</span> has more impact on the minimum-ice-edge extent and in reducing pack-ice thickness, especially in the eastern-Weddell <span class="hlt">Sea</span>. Low relative humidity enhances ice growth in thin ice and open-water regions, producing a more realistic ice edge along the coastal areas of the western-Weddell <span class="hlt">Sea</span> where dry continental <span class="hlt">air</span> has an impact. The modeled extent of the Weddell summer pack is equally sensitive to ocean heat <span class="hlt">flux</span> and atmospheric relative humidity variations with the more dynamic responses being from the atmosphere. Since the atmospheric regime in the eastern Weddell is dominated by marine intrusions from lower latitudes, with high humidity already, it is unlikely that either the moisture trans- port could be further raised or that it could be significantly lowered because of its distance from the continent (the lower humidity source). Ocean heat-transport variability is shown to lead to overall ice thinning in the model response and is a known feature of the actual system, as evidenced by the occurrence of the Weddell Polynya in the mid 1970s.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSPO34A3045P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSPO34A3045P"><span>Long-terms Change of <span class="hlt">Sea</span> Surface Temperature in the 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>Park, Y. G.; Choi, A.</p> <p>2016-02-01</p> <p>Using the Hadley Centre Global <span class="hlt">Sea</span> Ice and <span class="hlt">Sea</span> Surface Temperature (HadISST) the long term trend in the South China <span class="hlt">Sea</span> (SCS) <span class="hlt">sea</span> surface temperature (SST) between 1950 and 2008 is investigated. Both in winter and summer SST was increased by comparable amounts, but the warming patterns and the governing processes was different. During winter warming rate was greater in the deep basin in the central part, while during summer near the southern part. In winter the net heat <span class="hlt">flux</span> into the <span class="hlt">sea</span> was increased and could contribute to the warming. The pattern of the heat <span class="hlt">flux</span>, however, was different from that of the warming. The heat <span class="hlt">flux</span> was increased over the coastal area where warming was weaker, but decreased in deeper part where warming was stronger. The northeasterly monsoon wind weakened to lower the shoreward Ekman transport and the <span class="hlt">sea</span> surface height gradient. The cyclonic gyre that transports cold northern water to south was weakened to warm the ocean. The effect manifested more strongly southward western boundary currents, and subsequently cold advection. In summer the net surface heat <span class="hlt">flux</span>, however, was reduced and could not contribute to the warming. Over the southern part of the ocean the weakening of the southwesterly summer monsoon reduced southeastward Ekman transport, which is antiparallel to the mean SST gradient. Firstly, southeastward cold advection is reduced to warm the surface near the southeastern boundary of the SCS. The upwelling southeast of Vietnam was also weakened to raise the SST east of Vietnam. Thus the weakening of the wind in each season was the ultimate cause of the warming, but the responses of the ocean that lead to the warming were different.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.9773S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.9773S"><span>Assessing <span class="hlt">sea</span> wave and spray effects on Marine Boundary Layer structure</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stathopoulos, Christos; Galanis, George; Patlakas, Platon; Kallos, George</p> <p>2017-04-01</p> <p><span class="hlt">Air</span> <span class="hlt">sea</span> interface is characterized by several mechanical and thermodynamical processes. Heat, moisture and momentum exchanges increase the complexity in modeling the atmospheric-ocean system. Near surface atmospheric levels are subject to <span class="hlt">sea</span> surface roughness and <span class="hlt">sea</span> spray. <span class="hlt">Sea</span> spray <span class="hlt">fluxes</span> can affect atmospheric stability and induce microphysical processes such as <span class="hlt">sea</span> salt particle formation and condensation/evaporation of water in the boundary layer. Moreover, presence of <span class="hlt">sea</span> spray can alter stratification over the ocean surface with further insertion of water vapor. This can lead to modified stability conditions and to wind profiles that deviate significantly from the logarithmic approximation. To model these effects, we introduce a fully coupled system consisting of the mesoscale atmospheric model RAMS/ICLAMS and the wave model WAM. The system encompasses schemes for ocean surface roughness, <span class="hlt">sea</span> salt aerosols and droplet thermodynamic processes and handles <span class="hlt">sea</span> salt as predictive quantity. Numerical experiments using the developed atmospheric-ocean system are performed over the Atlantic and Mediterranean shoreline. Emphasis is given to the quantification of the improvement obtained in the description of the marine boundary layer, particularly in its lower part as well as in wave characteristics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.B41G2054B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.B41G2054B"><span>Carbon <span class="hlt">Fluxes</span> and Transport Along the Terrestrial Aquatic Continuum</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Butman, D. E.; Kolka, R.; Fennel, K.; Stackpoole, S. M.; Trettin, C.; Windham-Myers, L.</p> <p>2017-12-01</p> <p>Terrestrial wetlands, inland surface waters, tidal wetlands and estuaries, and the coastal ocean are distinct aquatic ecosystems that integrate carbon (C) <span class="hlt">fluxes</span> and processing among the major earth system components: the continents, oceans, and atmosphere. The development of the 2nd State of the Carbon Cycle Report (SOCCR2) noted that incorporating the C cycle dynamics for these ecosystems was necessary to reconcile some of the gaps associated with the North American C budget. We present major C stocks and <span class="hlt">fluxes</span> for Canada, Mexico and the United States. North America contains nearly 42% of the global terrestrial wetland area. Terrestrial wetlands, defined as soils that are seasonally or permanently inundated or saturated, contain significant C stocks equivalent to 174,000 Tg C in the top 40 cm of soil. While terrestrial wetlands are a C sink of approximately 64 Tg C yr-1, they also emit 21 Tg of CH4 yr-1. Inland waters are defined as lakes, reservoirs, rivers, and streams. Carbon <span class="hlt">fluxes</span>, which include lateral C export to the coast, riverine and lacustrine CO2 emissions, and C burial in lakes and reservoirs are estimated at 507 Tg yr-1. Estuaries and tidal wetlands assimilate C and nutrients from uplands and rivers, and their total C stock is 1,323 Tg C in the top 1 m of soils and sediment. Accounting for soil accretion, lateral C <span class="hlt">flux</span>, and CO2 assimilation and emission, tidal wetlands and estuaries are net sinks with a total <span class="hlt">flux</span> equal to 6 Tg C yr-1. The coastal ocean and <span class="hlt">sea</span> shelfs, defined as non-estuarine waters within 200 nautical miles (370 km) of the coast, function as net sinks, with the <span class="hlt">air-sea</span> exchange of CO2 estimated at 150 Tg C yr-1. In total, <span class="hlt">fluxes</span> from these four aquatic ecosystems are equal to a loss of 302 Tg C yr-1. Including these four discrete <span class="hlt">fluxes</span> in this assessment demonstrates the importance of linking hydrology and biogeochemical cycling to evaluate the impacts of climate change and human activities on carbon <span class="hlt">fluxes</span> across the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19800009379','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19800009379"><span>Guidelines for the <span class="hlt">air-sea</span> interaction special study: An element of the NASA climate research program, JPL/SIO workshop report</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1980-01-01</p> <p>A program in the area of <span class="hlt">air</span> <span class="hlt">sea</span> interactions is introduced. A space capability is discussed for global observations of climate parameters which will contribute to the understanding of the processes which influence climate and its predictability. The following recommendations are some of the suggestions made for <span class="hlt">air</span> <span class="hlt">sea</span> interaction studies: (1) a major effort needs to be devoted to the preparation of space based climatic data sets; (2) NASA should create a group or center for climatic data analysis due to the substantial long term effort that is needed in research and development; (3) funding for the analyses of existing data sets should be augmented and continued beyond the termination of present programs; (4) NASA should fund studies in universities, research institutions and governments' centers; and (5) the planning for an <span class="hlt">air</span> <span class="hlt">sea</span> interaction mission should be an early task.</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 CO2 concentration and increasing the pHT. Below the pycnocline of August 2012, instead, an elevated bacterial carbon production rate (0.92 μg C L- 1 h- 1) was related with net DIC increase (92 μmol kg- 1), low dissolved oxygen concentration, and strong pHT reduction, suggesting the predominance of bacterial heterotrophic respiration over primary production. The <span class="hlt">flux</span> of carbon dioxide estimated at the <span class="hlt">air-sea</span> interface exerted a low influence on the seasonal variation of the carbonate system. A complex temporal and spatial dynamic of the <span class="hlt">air-sea</span> CO2 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 CO2. 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> CO2</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1240753','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1240753"><span>CLOUDS, AEROSOLS, RADIATION AND THE <span class="hlt">AIR-SEA</span> INTERFACE OF THE SOUTHERN OCEAN: ESTABLISHING DIRECTIONS FOR FUTURE RESEARCH</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>Wood, Robert; Bretherton, Chris; McFarquhar, Greg</p> <p>2014-09-29</p> <p>A workshop sponsored by the Department of Energy was convened at the University of Washington to discuss the state of knowledge of clouds, aerosols and <span class="hlt">air-sea</span> interaction over the Southern Ocean and to identify strategies for reducing uncertainties in their representation in global and regional models. The Southern Ocean plays a critical role in the global climate system and is a unique pristine environment, yet other than from satellite, there have been sparse observations of clouds, aerosols, radiation and the <span class="hlt">air-sea</span> interface in this region. Consequently, much is unknown about atmospheric and oceanographic processes and their linkage in this region.more » Approximately 60 scientists, including graduate students, postdoctoral fellows and senior researchers working in atmospheric and oceanic sciences at U.S. and foreign universities and government laboratories, attended the Southern Ocean Workshop. It began with a day of scientific talks, partly in plenary and partly in two parallel sessions, discussing the current state of the science for clouds, aerosols and <span class="hlt">air-sea</span> interaction in the Southern Ocean. After the talks, attendees broke into two working groups; one focused on clouds and meteorology, and one focused on aerosols and their interactions with clouds. This was followed by more plenary discussion to synthesize the two working group discussions and to consider possible plans for organized activities to study clouds, aerosols and the <span class="hlt">air-sea</span> interface in the Southern Ocean. The agenda and talk slides, including short summaries of the highlights of the parallel session talks developed by the session chars, are available at http://www.atmos.washington.edu/socrates/presentations/SouthernOceanPresentations/.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSPO54B3239T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSPO54B3239T"><span>Argo float observations of basin-scale deep convection in the Irminger <span class="hlt">Sea</span> during winter 2011-2012</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Thierry, V.; Piron, A.; Mercier, H.; Caniaux, G.</p> <p>2016-02-01</p> <p>An analysis of Argo data during the 2011-2012 winter revealed the presence of an exceptionally large number of profiles over the Irminger Basin with mixed layer depths (MLD) exceeding 700 m, which was deep enough to reach the pool of the intermediate Labrador <span class="hlt">Sea</span> Water located in the Irminger <span class="hlt">Sea</span>. Among them, 4 profiles exhibited an MLD of 1000 m, which was the maximum value observed this winter. Owing to the exceptional Argo sampling in the Irminger <span class="hlt">Sea</span> during that winter the different phases of the mixed layer deepening down to 1000 m and their spatial extents were observed for the first time in the Irminger <span class="hlt">Sea</span>. Two intense convective periods occurred in late January south of Cape Farewell and in late February-early March east of Greenland. A final deepening period was observed in mid-March during which the deepest mixed layers were observed. This long deepening period occurred in large regional areas and was followed by a rapid restratification phase. A mixed layer heat budget along the trajectories of the 4 floats that sampled the deepest mixed layers showed that heat loss at the <span class="hlt">air-sea</span> interface was mainly responsible for heat content variations in the mixed layer. Greenland Tip Jets were of primary importance for the development of deep convection in the Irminger <span class="hlt">Sea</span> in the 2011-2012 winter. They enhanced the winter heat loss and two long (more than 24 hours), intense and close in time late events boosted the mixed layer deepening down to 1000m. Net <span class="hlt">air-sea</span> <span class="hlt">fluxes</span>, the number of Greenland Tip Jets, the stratification of the water column, the NAO index and Ekman-induced heat <span class="hlt">flux</span> are pertinent indicators to assess the favorable conditions for the development of deep convection in the Irminger <span class="hlt">Sea</span>. When considering each of those indicators, we concluded that the 2011-2012 event was not significantly different compared to the three other documented occurrences of deep convection in the Irminger <span class="hlt">Sea</span>.This work is a contribution to the NAOS project.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ClDy..tmp...34E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ClDy..tmp...34E"><span>The role of Amundsen-Bellingshausen <span class="hlt">Sea</span> anticyclonic circulation in forcing marine <span class="hlt">air</span> intrusions into West Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Emanuelsson, B. Daniel; Bertler, Nancy A. N.; Neff, Peter D.; Renwick, James A.; Markle, Bradley R.; Baisden, W. Troy; Keller, Elizabeth D.</p> <p>2018-01-01</p> <p>Persistent positive 500-hPa geopotential height anomalies from the ECMWF ERA-Interim reanalysis are used to quantify Amundsen-Bellingshausen <span class="hlt">Sea</span> (ABS) anticyclonic event occurrences associated with precipitation in West Antarctica (WA). We demonstrate that multi-day (minimum 3-day duration) anticyclones play a key role in the ABS by dynamically inducing meridional transport, which is associated with heat and moisture advection into WA. This affects surface climate variability and trends, precipitation rates and thus WA ice sheet surface mass balance. We show that the snow accumulation record from the Roosevelt Island Climate Evolution (RICE) ice core reflects interannual variability of blocking and geopotential height conditions in the ABS/Ross <span class="hlt">Sea</span> region. Furthermore, our analysis shows that larger precipitation events are related to enhanced anticyclonic circulation and meridional winds, which cause pronounced dipole patterns in <span class="hlt">air</span> temperature anomalies and <span class="hlt">sea</span> ice concentrations between the eastern Ross <span class="hlt">Sea</span> and the Bellingshausen <span class="hlt">Sea</span>/Weddell <span class="hlt">Sea</span>, as well as between the eastern and western Ross <span class="hlt">Sea</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.2084L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.2084L"><span>Computed and observed turbulent heat <span class="hlt">fluxes</span> during an extreme Bora event in the Adriatic using atmosphere-ocean coupling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ličer, Matjaž; Smerkol, Peter; Fettich, Anja; Ravdas, Michalis; Papapostolou, Alexandros; Mantziafou, Anneta; Strajnar, Benedikt; Cedilnik, Jure; Jeromel, Maja; Jerman, Jure; Petan, Sašo; Benetazzo, Alvise; Carniel, Sandro; Malačič, Vlado; Sofianos, Sarantis</p> <p>2016-04-01</p> <p>We have studied the performances of (a) a two-way coupled atmosphere-ocean modeling system and (b) one-way coupled ocean model (forced by the atmosphere model), as compared to the available in situ measurements during and after a strong Adriatic Bora wind event in February 2012, which led to extreme <span class="hlt">air-sea</span> interactions. The simulations span the period between January and March 2012. The models used were ALADIN (4.4 km resolution) on the atmosphere side and Adriatic setup of POM (1°/30 × 1°/30 angular resolution) on the ocean side. The atmosphere-ocean coupling was implemented using the OASIS3-MCT model coupling toolkit. Two-way coupling ocean feedback to the atmosphere is limited to <span class="hlt">sea</span> surface temperature. We have compared modeled atmosphere-ocean <span class="hlt">fluxes</span> (computed using modified Louis scheme) and <span class="hlt">sea</span> temperatures from both setups to platform and CTD measurements of <span class="hlt">fluxes</span> (computed using COARE scheme) and temperatures from three observational platforms (Vida, Paloma, Acqua Alta) in the Northern Adriatic. We show that turbulent <span class="hlt">fluxes</span> from both setups differ up to 20% during the Bora but not significantly before and after the event. The impact of the coupling on the ocean is significant while the impact on the atmosphere is less pronounced. When compared to observations, two way coupling ocean temperatures exhibit a four times lower RMSE than those from one-way coupled system. Two-way coupling improves sensible heat <span class="hlt">fluxes</span> at all stations but does not improve latent heat loss.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSPC43A..04B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSPC43A..04B"><span>Temporal Variability of North Atlantic Carbon <span class="hlt">Fluxes</span> and their Sensitivity to the Meridional Overturning Circulation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brown, P.; McDonagh, E.; Sanders, R.; King, B.; Watson, A. J.; Schuster, U.; Henson, S.</p> <p>2016-02-01</p> <p>The North Atlantic plays a critical role in the global carbon cycle both as a region of substantial <span class="hlt">air-sea</span> carbon dioxide uptake and as a location for the transfer of CO2 to depth on climatically-important timescales. While the magnitude of surface <span class="hlt">fluxes</span> is relatively well constrained, our understanding of the processes that drive variability in ocean-atmosphere exchange and subsequent subsurface carbon accumulation is not as well defined. Here we present observation-derived high-resolution estimates of short-term 10-day meridional ocean carbon transport variability across the subtropical North Atlantic for 2004-2012. Substantial seasonal, sub-annual and interannual transport variability is observed that is highly sensitive to the strength of the Atlantic Meridional Overturning Circulation. While the recently identified multi-year decrease in AMOC strength similarly impacts carbon transports, its full effect is masked by the northwards transport of increasing surface CO2 levels. A 30% slowdown in the meridional circulation in 2009-2010 and the anomalous effects it had on the transport, storage and divergence of heat and freshwater in the subtropical and subpolar gyres and local wind regimes are investigated for their impact on local <span class="hlt">air-sea</span> CO2 <span class="hlt">fluxes</span>. Temperature and salt content anomalies identified in each gyre are found to drive (subtropics) or hinder (subpolar) additional carbon uptake from the atmosphere by affecting the physical solubility pump for CO2. Additionally their simultaneous effect on mixed layer depth and the vertical supply of nutrients to the surface is shown to magnify the CO2 <span class="hlt">flux</span> observed by driving anomalous primary production rates.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..1412240S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..1412240S"><span>Disruption of the <span class="hlt">air-sea</span> interface and formation of two-phase transitional layer in hurricane conditions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Soloviev, A.; Matt, S.; Fujimura, A.</p> <p>2012-04-01</p> <p>The change of the <span class="hlt">air-sea</span> interaction regime in hurricane conditions is linked to the mechanism of direct disruption of the <span class="hlt">air-sea</span> interface by pressure fluctuations working against surface tension forces (Soloviev and Lukas, 2010). The direct disruption of the <span class="hlt">air-sea</span> interface due to the Kelvin-Helmholtz (KH) instability and formation of a two-phase transitional layer have been simulated with a computational fluid dynamics model. The volume of fluid multiphase model included surface tension at the water-<span class="hlt">air</span> interface. The model was initialized with either a flat interface or short wavelets. Wind stress was applied at the upper boundary of the <span class="hlt">air</span> layer, ranging from zero stress to hurricane force stress in different experiments. Under hurricane force wind, the numerical model demonstrated disruption of the <span class="hlt">air</span>-water interface and the formation of spume and the two-phase transition layer. In the presence of a transition layer, the <span class="hlt">air</span>-water interface is no longer explicitly identifiable. As a consequence, the analysis of dimensions suggests a linear dependence for velocity and logarithm of density on depth (which is consistent with the regime of marginal stability in the transition layer). The numerical simulations confirmed the presence of linear segments in the corresponding profiles within the transition layer. This permitted a parameterization of the equivalent drag coefficient due to the presence of the two-phase transition layer at the <span class="hlt">air-sea</span> interface. This two-phase layer parameterization represented the lower limit imposed on the drag coefficient under hurricane conditions. The numerical simulations helped to reduce the uncertainty in the critical Richardson number applicable to the <span class="hlt">air-sea</span> interface and in the values of two dimensionless constants; this reduced the uncertainty in the parameterization of the lower limit on the drag coefficient. The available laboratory data (Donelan et al., 2004) are bounded by the two-phase layer parameterization from</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23098675','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23098675"><span>The cycling and <span class="hlt">sea-air</span> exchange of mercury in the waters of the Eastern Mediterranean during the 2010 MED-OCEANOR cruise campaign.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Fantozzi, L; Manca, G; Ammoscato, I; Pirrone, N; Sprovieri, F</p> <p>2013-03-15</p> <p>An oceanographic cruise campaign on-board the Italian research vessel Urania was carried out from the 26th of August to the 13th of September 2010 in the Eastern Mediterranean. The campaign sought to investigate the mercury cycle at coastal and offshore locations in different weather conditions. The experimental activity focused on measuring mercury speciation in both seawater and in <span class="hlt">air</span>, and using meteorological parameters to estimate elemental mercury exchange at the <span class="hlt">sea</span>-atmosphere interface. Dissolved gaseous mercury (DGM), unfiltered total mercury (UTHg) and filtered total mercury (FTHg) surface concentrations ranged from 16 to 114, 300 to 18,760, and 230 to 10,990pgL(-1), respectively. The highest DGM, UTHg and FTHg values were observed close to Augusta (Sicily), a highly industrialized area of the Mediterranean region, while the lowest values were recorded at offshore stations. DGM vertical profiles partially followed the distribution of sunlight, as a result of the photoinduced transformations of elemental mercury in the surface layers of the water column. However, at some stations, we observed higher DGM concentrations in samples taken from the bottom of the water column, suggesting biological mercury production processes or the presence of tectonic activity. Moreover, two days of continuous measurement at one location demonstrated that surface DGM concentration is affected by solar radiation and atmospheric turbulence intensity. Atmospheric measurements of gaseous elemental mercury (GEM) showed an average concentration (1.6ngm(-3)) close to the background level for the northern hemisphere. For the first time this study used a numerical scheme based on a two-thin film model with a specific parameterization for mercury to estimate elemental mercury <span class="hlt">flux</span>. The calculated average mercury <span class="hlt">flux</span> during the entire cruise was 2.2±1.5ngm(-2)h(-1). The analysis of <span class="hlt">flux</span> data highlights the importance of the wind speed on the mercury evasion from <span class="hlt">sea</span> surfaces</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930038315&hterms=Onishi&qs=N%3D0%26Ntk%3DAuthor-Name%26Ntx%3Dmode%2Bmatchall%26Ntt%3DOnishi','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930038315&hterms=Onishi&qs=N%3D0%26Ntk%3DAuthor-Name%26Ntx%3Dmode%2Bmatchall%26Ntt%3DOnishi"><span>Heat <span class="hlt">flux</span> microsensor measurements</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Terrell, J. P.; Hager, J. M.; Onishi, S.; Diller, T. E.</p> <p>1992-01-01</p> <p>A thin-film heat <span class="hlt">flux</span> sensor has been fabricated on a stainless steel substrate. The thermocouple elements of the heat <span class="hlt">flux</span> sensor were nickel and nichrome, and the temperature resistance sensor was platinum. The completed heat <span class="hlt">flux</span> microsensor was calibrated at the AEDC radiation facility. The gage output was linear with heat <span class="hlt">flux</span> with no apparent temperature effect on sensitivity. The gage was used for heat <span class="hlt">flux</span> measurements at the NASA Langley Vitiated <span class="hlt">Air</span> Test Facility. Vitiated <span class="hlt">air</span> was expanded to Mach 3.0 and hydrogen fuel was injected. Measurements were made on the wall of a diverging duct downstream of the injector during all stages of the hydrogen combustion tests. Because the wall and the gage were not actively cooled, the wall temperature reached over 1000 C (1900 F) during the most severe test.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20000116506','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20000116506"><span>BOREAS AFM-2 King <span class="hlt">Air</span> 1994 Aircraft <span class="hlt">Flux</span> and Moving Window Data</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kelly, Robert D.; Hall, Forrest G. (Editor); Newcomer, Jeffrey A. (Editor); Smith, David E. (Technical Monitor)</p> <p>2000-01-01</p> <p>The BOREAS AFM-2 team collected pass-by-pass <span class="hlt">fluxes</span> (and many other statistics) for a large number of level (constant altitude), straight-line passes used in a variety of flight patterns. The data were collected by the University of Wyoming King <span class="hlt">Air</span> in 1994 BOREAS IFCs 1-3. Most of these data were collected at 60-70 m above ground level, but a significant number of passes were also flown at various levels in the planetary boundary layer, up to about the inversion height. This documentation concerns only the data from the straight and level passes that are presented as original (over the NSA and SSA) and moving window values (over the Transect). Another archive of King <span class="hlt">Air</span> data is also available, containing data from all the soundings flown by the King <span class="hlt">Air</span> 1994 IFCs 1-3. The data are stored in tabular ASCII files. The data files are available on a CD-ROM (see document number 20010000884) or from the Oak Ridge National Laboratory (ORNL) Distributed Active Archive Center (DAAC).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017OcSci..13.1093S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017OcSci..13.1093S"><span>Modelling deep-water formation in the north-west Mediterranean <span class="hlt">Sea</span> with a new <span class="hlt">air-sea</span> coupled model: sensitivity to turbulent <span class="hlt">flux</span> parameterizations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Seyfried, Léo; Marsaleix, Patrick; Richard, Evelyne; Estournel, Claude</p> <p>2017-12-01</p> <p>In the north-western Mediterranean, the strong, dry, cold winds, the Tramontane and Mistral, produce intense heat and moisture exchange at the interface between the ocean and the atmosphere leading to the formation of deep dense waters, a process that occurs only in certain regions of the world. The purpose of this study is to demonstrate the ability of a new coupled ocean-atmosphere modelling system based on MESONH-SURFEX-SYMPHONIE to simulate a deep-water formation event in real conditions. The study focuses on summer 2012 to spring 2013, a favourable period that is well documented by previous studies and for which many observations are available. Model results are assessed through detailed comparisons with different observation data sets, including measurements from buoys, moorings and floats. The good overall agreement between observations and model results shows that the new coupled system satisfactorily simulates the formation of deep dense water and can be used with confidence to study ocean-atmosphere coupling in the north-western Mediterranean. In addition, to evaluate the uncertainty associated with the representation of turbulent <span class="hlt">fluxes</span> in strong wind conditions, several simulations were carried out based on different parameterizations of the <span class="hlt">flux</span> bulk formulas. The results point out that the choice of turbulent <span class="hlt">flux</span> parameterization strongly influences the simulation of the deep-water convection and can modify the volume of the newly formed deep water by a factor of 2.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.3696L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.3696L"><span>How well does wind speed predict <span class="hlt">air-sea</span> gas transfer in the <span class="hlt">sea</span> ice zone? A synthesis of radon deficit profiles in the upper water column of the Arctic Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Loose, B.; Kelly, R. P.; Bigdeli, A.; Williams, W.; Krishfield, R.; Rutgers van der Loeff, M.; Moran, S. B.</p> <p>2017-05-01</p> <p>We present 34 profiles of radon-deficit from the ice-ocean boundary layer of the Beaufort <span class="hlt">Sea</span>. Including these 34, there are presently 58 published radon-deficit estimates of <span class="hlt">air-sea</span> gas transfer velocity (k) in the Arctic Ocean; 52 of these estimates were derived from water covered by 10% <span class="hlt">sea</span> ice or more. The average value of k collected since 2011 is 4.0 ± 1.2 m d-1. This exceeds the quadratic wind speed prediction of weighted kws = 2.85 m d-1 with mean-weighted wind speed of 6.4 m s-1. We show how ice cover changes the mixed-layer radon budget, and yields an "effective gas transfer velocity." We use these 58 estimates to statistically evaluate the suitability of a wind speed parameterization for k, when the ocean surface is ice covered. Whereas the six profiles taken from the open ocean indicate a statistically good fit to wind speed parameterizations, the same parameterizations could not reproduce k from the <span class="hlt">sea</span> ice zone. We conclude that techniques for estimating k in the open ocean cannot be similarly applied to determine k in the presence of <span class="hlt">sea</span> ice. The magnitude of k through gaps in the ice may reach high values as ice cover increases, possibly as a result of focused turbulence dissipation at openings in the free surface. These 58 profiles are presently the most complete set of estimates of k across seasons and variable ice cover; as dissolved tracer budgets they reflect <span class="hlt">air-sea</span> gas exchange with no impact from <span class="hlt">air</span>-ice gas exchange.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930039263&hterms=air+measurement&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dair%2Bmeasurement','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930039263&hterms=air+measurement&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dair%2Bmeasurement"><span><span class="hlt">Air</span>-mass <span class="hlt">flux</span> measurement system using Doppler-shifted filtered Rayleigh scattering</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Shirley, John A.; Winter, Michael</p> <p>1993-01-01</p> <p>An optical system has been investigated to measure mass <span class="hlt">flux</span> distributions in the inlet of a high speed <span class="hlt">air</span>-breathing propulsion system. Rayleigh scattered light from <span class="hlt">air</span> is proportional to the number density of molecules and hence can be used to ascertain the gas density in a calibrated system. Velocity field measurements are achieved by spectrally filtering the elastically-scattered Doppler-shifted light with an absorbing molecular filter. A novel anamorphic optical collection system is used which allows optical rays from different scattering angles, that have different Doppler shifts, to be recorded separately. This is shown to obviate the need to tune the laser through the absorption to determine velocities, while retaining the ability to make spatially-resolved measurements along a line. By properly selecting the laser tuning and filter parameters, simultaneous density measurements can be made. These properties are discussed in the paper and experiments demonstrating the velocimetry capability are described.</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/ADA629979','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA629979"><span>Analysis of Near-Surface Oceanic Measurements Obtained During the Low-Wind Component of the Coupled Boundary Layers and <span class="hlt">Air-Sea</span> Transfer (CBLAST) Experiment</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2006-09-30</p> <p>temperature and the upwelling IR radiative heat <span class="hlt">flux</span> were obtained from a pyrometer . The heat <span class="hlt">fluxes</span> are combined to compute the net heat <span class="hlt">flux</span> into or out...sampled acoustic Doppler velocimeters (ADVs) and thermistors (Figure 1b). These measurements provide inertial-range estimates of dissipation rates...horizontal velocity at the <span class="hlt">sea</span> surface were obtained with a “fanbeam” acoustic Doppler current profiler (ADCP), which produces spatial maps of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.V21C3045F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.V21C3045F"><span><span class="hlt">Flux</span>, Budget and Sources of Black Carbon (BC) in the Continental Shelf of the Bohai and Yellow <span class="hlt">Seas</span>, China</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fang, Y.; Chen, Y.; Tian, C.</p> <p>2015-12-01</p> <p>Black carbon (BC) derived from incomplete combustion of fossil fuels and biomass has received increasing attention due to their potential importance in a wide range of biogeochemical processes. China has been generally considered as the world's largest BC emitter. Due to a combination of the prevailing East Asia monsoon and large amounts of riverine outflow, BC released from China can be transported to the adjacent continental shelf <span class="hlt">seas</span>, the Bohai <span class="hlt">Sea</span> (BS) and Yellow <span class="hlt">Sea</span> (YS). Based on measurements of BC in 191 surface sediments, 36 riverine water, and 2 seawater samples, as well as the reported BC data set of the aerosol samples in the Bohai Rim, the concentration, <span class="hlt">flux</span>, and budget of BC in the BS and YS were investigated. The spatial distribution of the BC concentration in surface sediments was largely influenced by the regional hydrodynamic conditions, with high values mainly occurring in the central mud areas. The BC burial <span class="hlt">flux</span> in the BS and YS ranged from 4 to 1100 μg/cm2/yr, and averaged 166 ± 200 μg/cm2/yr. The area-integrated sedimentary BC sink <span class="hlt">flux</span> in the entire BS and YS was ~325 Gg/yr. The BC budget calculated in the BS showed that atmospheric deposition and riverine discharge played comparable importance in delivering BC to the BS, and sequestration to bottom sediments was the major BC output pattern, accounting for ~88% of the total input BC. Besides, we attempted to apportion the BC sources in the BS and YS surface sediments using PAHs (organic molecular proxies cogenerated with BC) and BC as an input data to the Positive Matrix Factorization (PMF) receptor model. Results showed that ~83% of the sediment BC was attributed to the combustion of fossil fuels, and the remaining ~17% was from biomass burning. Due to the differences in their production mechanisms and therefore physicochemical properties, the above distinction and quantification would help us better understand their different environmental behaviors in the complex continental shelf</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20000000183','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20000000183"><span><span class="hlt">Sea</span>WiFS Postlaunch Technical Report Series. Volume 7; The Fifth <span class="hlt">Sea</span>-WiFS Intercalibration Round-Robin Experiment (SIRREX-5), July 1996</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); Johnson, B. Carol; Yoon, Howard W.; Bruce, Sally S.; Shaw, Ping-Shine; Thompson, Ambler; Hooker, Stanford B.; Barnes, Robert A.; Eplee, Robert E., Jr.; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20000000183'); toggleEditAbsImage('author_20000000183_show'); toggleEditAbsImage('author_20000000183_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20000000183_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20000000183_hide"></p> <p>1999-01-01</p> <p>This report documents the fifth <span class="hlt">Sea</span>-viewing Wide Field-of-view Sensor (<span class="hlt">Sea</span>WiFS) Intercalibration Round-Robin Experiment (SIRREX-5), which was held at the National Institute of Standards and Technology (NIST) on 23-30 July 1996. The agenda for SIRREX-5 was established based on recommendations made during SIRREX-4. For the first time in a SIRREX activity, instrument intercomparisons were performed at field sites, which were near NIST. The goals of SIRREX-5 were to continue the emphasis on training and the implementation of standard measurement practices, investigate the calibration methods and measurement chains in use by the oceanographic community, provide opportunities for discussion, and intercompare selected instruments. As at SIRREX-4, the day was divided between morning lectures and afternoon laboratory exercises. A set of core laboratory sessions were performed: 1) in-water radiant <span class="hlt">flux</span> measurements; 2) in-<span class="hlt">air</span> radiant <span class="hlt">flux</span> measurements; 3) spectral radiance responsivity measurements using the plaque method; 4) device calibration or stability monitoring with portable field sources; and 5) various ancillary exercises designed to illustrate radiometric concepts. Before, during, and after SIRREX-5, NIST calibrated the SIRREX-5 participating radiometers for radiance and irradiance responsivity. The Facility for Automated Spectroradiometric Calibrations (FASCAL) was scheduled for spectral irradiance calibrations for standard lamps during SIRREX-5. Three lamps from the <span class="hlt">Sea</span>WiFS community were submitted and two were calibrated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015BGD....12.1247M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015BGD....12.1247M"><span>Downward particle <span class="hlt">flux</span> and carbon export in the Beaufort <span class="hlt">Sea</span>, Arctic Ocean; the Malina experiment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Miquel, J.-C.; Gasser, B.; Martín, J.; Marec, C.; Babin, M.; Fortier, L.; Forest, A.</p> <p>2015-01-01</p> <p>As part of the international, multidisciplinary project Malina, downward particle <span class="hlt">fluxes</span> were investigated by means of a drifting multi-sediment trap mooring deployed at three sites in the Canadian Beaufort <span class="hlt">Sea</span> in late summer 2009. Mooring deployments lasted for 28-50 h and targeted the shelf-break and the slope along the Beaufort-Mackenzie continental margin, as well as the edge between the Mackenzie Shelf and the Amundsen Gulf. Besides analyses of C and N, the collected material was investigated for pigments, phyto- and microzooplankton, faecal pellets and swimmers. The measured <span class="hlt">fluxes</span> were relatively low, in the range of 11-54 mg m-2 d-1 for the total mass, 1-15 mg C m-2 d-1 for organic carbon and 0.2-2.5 mg N m-2 d-1 for nitrogen. Comparison with a long-term trap dataset from the same sampling area showed that the short-term measurements were at the lower end of the high variability characterizing a rather high <span class="hlt">flux</span> regime during the study period. The sinking material consisted of aggregates and particles that were characterized by the presence of hetero- and autotrophic microzooplankters and diatoms and by the corresponding pigment signatures. Faecal pellets contribution to sinking carbon <span class="hlt">flux</span> was important, especially at depth where they represented up to 25% of the total carbon <span class="hlt">flux</span>. The vertical distribution of different morphotypes of pellets showed a marked pattern with cylindrical faeces (produced by calanoid copepods) present mainly within the euphotic zone, whereas elliptical pellets (produced mainly by smaller copepods) were more abundant at mesopelagic depths. These features, together with the density of matter within the pellets, highlighted the role of the zooplankton community in the transformation of carbon issued from the primary production and the transition of that carbon from the productive surface zone to the Arctic Ocean's interior. Our data indicate that sinking carbon <span class="hlt">flux</span> in this late summer period is primarily the result of a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..12..259T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..12..259T"><span>Laboratory modeling of <span class="hlt">air-sea</span> interaction under severe wind conditions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Troitskaya, Yuliya; Vasiliy, Kazakov; Nicolay, Bogatov; Olga, Ermakova; Mikhail, Salin; Daniil, Sergeev; Maxim, Vdovin</p> <p>2010-05-01</p> <p>Wind-wave interaction at extreme wind speed is of special interest now in connection with the problem of explanation of the <span class="hlt">sea</span> surface drag saturation at the wind speed exceeding 30 m/s. The idea on saturation (and even reduction) of the coefficient of aerodynamic resistance of the <span class="hlt">sea</span> surface at hurricane wind speed was first suggested by Emanuel (1995) on the basis of theoretical analysis of sensitivity of maximum wind speed in a hurricane to the ratio of the enthalpy and momentum exchange coefficients. Both field (Powell, Vickery, Reinhold, 2003, French et al, 2007, Black, et al, 2007) and laboratory (Donelan et al, 2004) experiments confirmed that at hurricane wind speed the <span class="hlt">sea</span> surface drag coefficient is significantly reduced in comparison with the parameterization obtained at moderate to strong wind conditions. Two groups of possible theoretical mechanisms for explanation of the effect of the <span class="hlt">sea</span> surface drag reduction can be specified. In the first group of models developed by Kudryavtsev & Makin (2007) and Kukulka,Hara Belcher (2007), the <span class="hlt">sea</span> surface drag reduction is explained by peculiarities of the <span class="hlt">air</span> flow over breaking waves. Another approach more appropriate for the conditions of developed <span class="hlt">sea</span> exploits the effect of <span class="hlt">sea</span> drops and sprays on the wind-wave momentum exchange (Andreas, 2004; Makin, 2005; Kudryavtsev, 2006). The main objective of this work is investigation of factors determining momentum exchange under high wind speeds basing on the laboratory experiment in a well controlled environment. The experiments were carried out in the Thermo-Stratified WInd-WAve Tank (TSWIWAT) of the Institute of Applied Physics. The parameters of the facility are as follows: airflow 0 - 25 m/s (equivalent 10-m neutral wind speed U10 up to 60 m/s), dimensions 10m x 0.4m x 0.7 m, temperature stratification of the water layer. Simultaneous measurements of the airflow velocity profiles and wind waves were carried out in the wide range of wind velocities. Airflow</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> transfer 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('http://adsabs.harvard.edu/abs/1988DSRA...35..441A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1988DSRA...35..441A"><span>Seasonal variation in the <span class="hlt">flux</span> of euthecosomatous pteropods collected in a deep sediment trap in the Sargasso <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Almogi-Labin, A.; Hemleben, Ch.; Deuser, W. G.</p> <p>1988-03-01</p> <p>A 4-year series of sediment trap samples from a depth of 3.2 km in the Sargasso <span class="hlt">Sea</span> (32°05'N, 64°15'W) has revealed seasonal variations in the <span class="hlt">flux</span> of euthecosomatous pteropods. Total pteropod <span class="hlt">flux</span> is related to seasonal variations of the total particulate and organic carbon <span class="hlt">flux</span> with a lag of 1-1.5 months. High <span class="hlt">flux</span> of pteropods (>200 specimens m -2 day -1) occurs in late winter to mid-summer. Shells of individual pteropod species arrive in deep water in a seasonal succession similar to that in the living assemblage. Peak <span class="hlt">fluxes</span> of Styliola subula, Clio pyramidata and Limacina bulimoides were recorded from February to May. Limacina inflata, Limacina lesueuri and Cuvierina columnella entered the trap in maximum numbers from April to mid-August. Creseis virgula conica and C. acicula were most abundant from June to late August. The latter two are non-migrating, epipelagic pteropods and comprise <10% of the assemblage. Diel migrators dominate the pteropod assemblage (92%). During the summer months they appear to migrate at greater depth, without reaching the surface water. Although many young are produced, only a small fraction, about 4% in the case of L. inflata and L. bulimoides, survives and reaches maturity. Adult shell size of L. inflata and L. bulimoides varies seasonally, reaching maximum size during spring, probably in response to increasing food availability.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015GeoRL..42.5442L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015GeoRL..42.5442L"><span>Observed platelet ice distributions in Antarctic <span class="hlt">sea</span> ice: An index for ocean-ice shelf heat <span class="hlt">flux</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Langhorne, P. J.; Hughes, K. G.; Gough, A. J.; Smith, I. J.; Williams, M. J. M.; Robinson, N. J.; Stevens, C. L.; Rack, W.; Price, D.; Leonard, G. H.; Mahoney, A. R.; Haas, C.; Haskell, T. G.</p> <p>2015-07-01</p> <p>Antarctic <span class="hlt">sea</span> ice that has been affected by supercooled Ice Shelf Water (ISW) has a unique crystallographic structure and is called platelet ice. In this paper we synthesize platelet ice observations to construct a continent-wide map of the winter presence of ISW at the ocean surface. The observations demonstrate that, in some regions of coastal Antarctica, supercooled ISW drives a negative oceanic heat <span class="hlt">flux</span> of -30 Wm-2 that persists for several months during winter, significantly affecting <span class="hlt">sea</span> ice thickness. In other regions, particularly where the thinning of ice shelves is believed to be greatest, platelet ice is not observed. Our new data set includes the longest ice-ocean record for Antarctica, which dates back to 1902 near the McMurdo Ice Shelf. These historical data indicate that, over the past 100 years, any change in the volume of very cold surface outflow from this ice shelf is less than the uncertainties in the measurements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20000070381&hterms=sonar&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dsonar','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20000070381&hterms=sonar&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dsonar"><span>Variability of Fram Strait Ice <span class="hlt">Flux</span> and North Atlantic Oscillation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kwok, Ron</p> <p>1999-01-01</p> <p>An important term in the mass balance of the Arctic Ocean <span class="hlt">sea</span> ice is the ice export. We estimated the winter <span class="hlt">sea</span> ice export through the Fram Strait using ice motion from satellite passive microwave data and ice thickness data from moored upward looking sonars. The average winter area <span class="hlt">flux</span> over the 18-year record (1978-1996) is 670,000 square km, approximately 7% of the area of the Arctic Ocean. The winter area <span class="hlt">flux</span> ranges from a minimum of 450,000 sq. km in 1984 to a maximum of 906,000 sq km in 1995. The daily, monthly and interannual variabilities of the ice area <span class="hlt">flux</span> are high. There is an upward trend in the ice area <span class="hlt">flux</span> over the 18-year record. The average winter volume <span class="hlt">flux</span> over the winters of October 1990 through May 1995 is 1745 cubic km ranging from a low of 1375 cubic km in 1990 to a high of 2791 cubic km in 1994. The <span class="hlt">sea</span>-level pressure gradient across the Fram Strait explains more than 80% of the variance in the ice <span class="hlt">flux</span> over the 18-year record. We use the coefficients from the regression of the time-series of area <span class="hlt">flux</span> versus pressure gradient across the Fram Strait and ice thickness data to estimate the summer area and volume <span class="hlt">flux</span>. The average 12-month area <span class="hlt">flux</span> and volume <span class="hlt">flux</span> are 919,000 sq km and 2366 cubic km. We find a significant correlation (R =0.86) between the area <span class="hlt">flux</span> and positive phases of the North Atlantic Oscillation (NAO) index over the months of December through March. Correlation between our six years of volume <span class="hlt">flux</span> estimates and the NAO index gives R =0.56. During the high NAO years, a more intense Icelandic low increases the gradient in the <span class="hlt">sea</span>-level pressure by almost 1 mbar across the Fram Strait thus increasing the atmospheric forcing on ice transport. Correlation is reduced during the negative NAO years because of decreased dominance of this large-scale atmospheric pattern on the <span class="hlt">sea</span>-level pressure gradient across the Fram Strait. Additional information is contained in the original.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ClDy...50..101R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ClDy...50..101R"><span>Evaluation of energy <span class="hlt">fluxes</span> in the NCEP climate forecast system version 2.0 (CFSv2)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rai, Archana; Saha, Subodh Kumar</p> <p>2018-01-01</p> <p>The energy <span class="hlt">fluxes</span> at the surface and top of the atmosphere (TOA) from a long free run by the NCEP climate forecast system version 2.0 (CFSv2) are validated against several observation and reanalysis datasets. This study focuses on the annual mean energy <span class="hlt">fluxes</span> and tries to link it with the systematic cold biases in the 2 m <span class="hlt">air</span> temperature, particularly over the land regions. The imbalance in the long term mean global averaged energy <span class="hlt">fluxes</span> are also evaluated. The global averaged imbalance at the surface and at the TOA is found to be 0.37 and 6.43 Wm-2, respectively. It is shown that CFSv2 overestimates the land surface albedo, particularly over the snow region, which in turn contributes to the cold biases in 2 m <span class="hlt">air</span> temperature. On the other hand, surface albedo is highly underestimated over the coastal region around Antarctica and that may have contributed to the warm bias over that oceanic region. This study highlights the need for improvements in the parameterization of snow/<span class="hlt">sea</span>-ice albedo scheme for a realistic simulation of surface temperature and that may have implications on the global energy imbalance in the model.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E%26ES..113a2223L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26ES..113a2223L"><span>Observation and difference analysis of carbon <span class="hlt">fluxes</span> in different types of soil in Tianjin 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>Li, Ya-Juan; Wang, Ting-Feng; Mao, Tian-Yu</p> <p>2018-02-01</p> <p>Tianjin Coastal Zone is located in the coastal area of the Bohai <span class="hlt">Sea</span>, belonging to the typical coastal wetland, with high carbon value. Over the past decade the development of great intensity, there are obvious characteristics of artificial influence. This study focuses on observing the carbon <span class="hlt">fluxes</span> of different soil types in the coastal area under strong artificial disturbance, summarizing the carbon sink calculation formula according to the soil type, and analyzing the main influencing factors affecting the carbon <span class="hlt">flux</span>. The results show that there are representative intertidal zones in Tianjin, and the respiration of soil and secondary soil are different. The main influencing factors are soil surface temperature or <span class="hlt">air</span> temperature. Coastal zones with different ecosystems can basically establish the relationship between temperature and soil carbon <span class="hlt">flux</span>. (R2 = 0.5990), the relationship between artificial backfill is Q = 0.2061 - 0.2129T - 0.0391T2 (R2 = 0.7469), and the artificial soil is restored by artificial soil and the herbaceous greening is carried out., The relationship is Q = -0.1019 + 0.0327T‧ (R2 = 0.6621), T-soil temperature, T’-<span class="hlt">air</span> temperature. At the same temperature, soil carbon <span class="hlt">fluxes</span> in shoal wetlands are generally stronger than artificial backfill, showing more carbon source emissions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JGRC..121.7495L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JGRC..121.7495L"><span>Vernal distribution and turnover of dimethylsulfide (DMS) in the surface water of the Yellow <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Cheng-Xuan; Yang, Gui-Peng; Wang, Bao-Dong; Xu, Zong-Jun</p> <p>2016-10-01</p> <p>The spatial and interannual variations of dimethylsulfide (DMS) and its precursors, dissolved and particulate dimethylsulfoniopropionate (DMSP), were discussed on the basis of field observations in the surface waters of the Yellow <span class="hlt">Sea</span> during spring 2007. Maxima of dimethylated sulfur compounds and low chlorophyll a concentrations were found in the central southern Yellow <span class="hlt">Sea</span>, whereas low concentrations of DMS and DMSP were detected at the boundary between the northern and southern parts of the Yellow <span class="hlt">Sea</span>. This frontal region is influenced by active water currents, <span class="hlt">air-sea</span> interface exchanges, and biological turnover. The horizontal variations in DMS production and consumption rates showed a decreasing tendency from the coastal to offshore areas mainly due to the complicated biological features. DMS positively correlated with dissolved CH4 and CO2 but negatively correlated with nutrients (nitrite and phosphate). Particulate DMSP concentrations and DMS production rates positively correlated with dinoflagellate abundances but negatively correlated with diatom cell densities. DMS and DMSP concentrations, as well as DMS production and consumption rates, exhibited approximately 2.0-2.8 fold increases from 2005 to 2012. This finding was likely caused by shifts in the phytoplankton communities from diatoms to dinoflagellates and the increases in abundances of zooplankton and bacteria. Average <span class="hlt">sea-to-air</span> DMS <span class="hlt">fluxes</span> were estimated to be 8.12 ± 1.24 µmol·(m-2·d-1), and DMS microbial consumption was approximately 1.68 times faster than the DMS <span class="hlt">sea-air</span> exchange. These findings imply that biological consumption, relative to ventilation, is a predominant mechanism in DMS removal from the surface water.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013JETPL..97..291B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013JETPL..97..291B"><span>On amplifications of photonuclear neutron <span class="hlt">flux</span> in thunderstorm atmosphere and possibility of detecting them</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Babich, L. P.; Bochkov, E. I.; Kutsyk, I. M.; Zalyalov, A. N.</p> <p>2013-05-01</p> <p>The reliability of communications reporting observations of neutron <span class="hlt">flux</span> enhancements in thunderstorm atmosphere is analyzed. The analysis is motivated by the fact that the employed gas-discharge counters on the basis of reactions 3He( n, p)3H and 10B( n; 4He, γ)7Li detect not only neutrons but any penetrating radiations. Photonuclear reactions are capable of accounting for the possible amplifications of neutron <span class="hlt">flux</span> in thunder-storm atmosphere since in correlation with thunderstorms γ-ray flashes were repeatedly observed with spectra extending high above the threshold of photonuclear reactions in <span class="hlt">air</span>. By numerical simulations, it was demonstrated that γ-ray pulses detected in thunderstorm atmosphere are capable of generating photonuclear neutrons in numbers sufficient to be detected even at <span class="hlt">sea</span> level.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28262984','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28262984"><span>Diffusive <span class="hlt">flux</span> of PAHs across sediment-water and water-<span class="hlt">air</span> interfaces at urban superfund sites.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Minick, D James; Anderson, Kim A</p> <p>2017-09-01</p> <p>Superfund sites may be a source of polycyclic aromatic hydrocarbons (PAHs) to the surrounding environment. These sites can also act as PAH sinks from present-day anthropogenic activities, especially in urban locations. Understanding PAH transport across environmental compartments helps to define the relative contributions of these sources and is therefore important for informing remedial and management decisions. In the present study, paired passive samplers were co-deployed at sediment-water and water-<span class="hlt">air</span> interfaces within the Portland Harbor Superfund Site and the McCormick and Baxter Superfund Site. These sites, located along the Willamette River (Portland, OR, USA), have PAH contamination from both legacy and modern sources. Diffusive <span class="hlt">flux</span> calculations indicate that the Willamette River acts predominantly as a sink for low molecular weight PAHs from both the sediment and the <span class="hlt">air</span>. The sediment was also predominantly a source of 4- and 5-ring PAHs to the river, and the river was a source of these same PAHs to the <span class="hlt">air</span>, indicating that legacy pollution may be contributing to PAH exposure for residents of the Portland urban center. At the remediated McCormick and Baxter Superfund Site, <span class="hlt">flux</span> measurements highlight locations within the sand and rock sediment cap where contaminant breakthrough is occurring. Environ Toxicol Chem 2017;36:2281-2289. © 2017 SETAC. © 2017 SETAC.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.1608P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.1608P"><span>The ocean mixed layer under Southern Ocean <span class="hlt">sea</span>-ice: Seasonal cycle and forcing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pellichero, Violaine; Sallée, Jean-Baptiste; Schmidtko, Sunke; Roquet, Fabien; Charrassin, Jean-Benoît</p> <p>2017-02-01</p> <p>The oceanic mixed layer is the gateway for the exchanges between the atmosphere and the ocean; in this layer, all hydrographic ocean properties are set for months to millennia. A vast area of the Southern Ocean is seasonally capped by <span class="hlt">sea</span>-ice, which alters the characteristics of the ocean mixed layer. The interaction between the ocean mixed layer and <span class="hlt">sea</span>-ice plays a key role for water mass transformation, the carbon cycle, <span class="hlt">sea</span>-ice dynamics, and ultimately for the climate as a whole. However, the structure and characteristics of the under-ice mixed layer are poorly understood due to the sparseness of in situ observations and measurements. In this study, we combine distinct sources of observations to overcome this lack in our understanding of the polar regions. Working with elephant seal-derived, ship-based, and Argo float observations, we describe the seasonal cycle of the ocean mixed-layer characteristics and stability of the ocean mixed layer over the Southern Ocean and specifically under <span class="hlt">sea</span>-ice. Mixed-layer heat and freshwater budgets are used to investigate the main forcing mechanisms of the mixed-layer seasonal cycle. The seasonal variability of <span class="hlt">sea</span> surface salinity and temperature are primarily driven by surface processes, dominated by <span class="hlt">sea</span>-ice freshwater <span class="hlt">flux</span> for the salt budget and by <span class="hlt">air-sea</span> <span class="hlt">flux</span> for the heat budget. Ekman advection, vertical diffusivity, and vertical entrainment play only secondary roles. Our results suggest that changes in regional <span class="hlt">sea</span>-ice distribution and annual duration, as currently observed, widely affect the buoyancy budget of the underlying mixed layer, and impact large-scale water mass formation and transformation with far reaching consequences for ocean ventilation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMOS41C1215M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMOS41C1215M"><span>Assimilation of Satellite <span class="hlt">Sea</span> Surface Salinity Fields: Validating Ocean Analyses and Identifying Errors in Surface Buoyancy <span class="hlt">Fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mehra, A.; Nadiga, S.; Bayler, E. J.; Behringer, D.</p> <p>2014-12-01</p> <p>Recently available satellite <span class="hlt">sea</span>-surface salinity (SSS) fields provide an important new global data stream for assimilation into ocean forecast systems. In this study, we present results from assimilating satellite SSS fields from NASA's Aquarius mission into the National Oceanic and Atmospheric Administration's (NOAA) operational Modular Ocean Model version 4 (MOM4), the oceanic component of NOAA's operational seasonal-interannual Climate Forecast System (CFS). Experiments on the sensitivity of the ocean's overall state to different relaxation time periods were run to evaluate the importance of assimilating high-frequency (daily to mesoscale) and low-frequency (seasonal) SSS variability. Aquarius SSS data (Aquarius Data Processing System (ADPS) version 3.0), mapped daily fields at 1-degree spatial resolution, were used. Four model simulations were started from the same initial ocean condition and forced with NOAA's daily Climate Forecast System Reanalysis (CFSR) <span class="hlt">fluxes</span>, using a relaxation technique to assimilate daily satellite <span class="hlt">sea</span> surface temperature (SST) fields and selected SSS fields, where, except as noted, a 30-day relaxation period is used. The simulations are: (1) WOAMC, the reference case and similar to the operational setup, assimilating monthly climatological SSS from the 2009 NOAA World Ocean Atlas; (2) AQ_D, assimilating daily Aquarius SSS; (3) AQ_M, assimilating monthly Aquarius SSS; and (4) AQ_D10, assimilating daily Aquarius SSS, but using a 10-day relaxation period. The analysis focuses on the tropical Pacific Ocean, where the salinity dynamics are intense and dominated by El Niño interannual variability in the cold tongue region and by high-frequency precipitation events in the western Pacific warm pool region. To assess the robustness of results and conclusions, we also examine the results for the tropical Atlantic and Indian Oceans. Preliminary validation studies are conducted using observations, such as satellite <span class="hlt">sea</span>-surface height (SSH</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> CO2 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 CO2, it has been hypothesized that its enrichment in the SML enhances the <span class="hlt">air-sea</span> CO2 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/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 transfer of gases in the liquid near the boundary, a molecular plus eddy diffusivity concept is used, which has been found useful for smooth flow over solid surfaces. From consideration of the boundary conditions, a similar dependence of eddy diffusivity on distance from the interface can be derived for the flow beneath a gas/liquid interface, at least in the absence of waves. The influence of waves is then discussed. It is evident from scale considerations that the effect of gravity waves is small. It is known from wind tunnel work that capillary waves enhance gas transfer considerably. The existing hypotheses are apparently not sufficient to explain the observations. Examination of field data is even more frustrating since the data do not show the expected increase of gas exchange with wind speed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMOS31B1399W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMOS31B1399W"><span>In Situ Global <span class="hlt">Sea</span> Surface Salinity and Variability from the NCEI Global Thermosalinograph Database</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Z.; Boyer, T.; Zhang, H. M.</p> <p>2017-12-01</p> <p><span class="hlt">Sea</span> surface salinity (SSS) plays an important role in the global ocean circulations. The variations of <span class="hlt">sea</span> surface salinity are key indicators of changes in <span class="hlt">air-sea</span> water <span class="hlt">fluxes</span>. Using nearly 30 years of in situ measurements of <span class="hlt">sea</span> surface salinity from thermosalinographs, we will evaluate the variations of the <span class="hlt">sea</span> surface salinity in the global ocean. The <span class="hlt">sea</span> surface salinity data used are from our newly-developed NCEI Global Thermosalinograph Database - NCEI-TSG. This database provides a comprehensive set of quality-controlled in-situ <span class="hlt">sea</span>-surface salinity and temperature measurements collected from over 340 vessels during the period 1989 to the present. The NCEI-TSG is the world's most complete TSG dataset, containing all data from the different TSG data assembly centers, e.g. COAPS (SAMOS), IODE (GOSUD) and AOML, with more historical data from NCEI's archive to be added. Using this unique dataset, we will investigate the spatial variations of the global SSS and its variability. Annual and interannual variability will also be studied at selected regions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001DSRII..48.1471C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001DSRII..48.1471C"><span>Seasonal and interannual variability in deep ocean particle <span class="hlt">fluxes</span> at the Oceanic <span class="hlt">Flux</span> Program (OFP)/Bermuda Atlantic Time Series (BATS) site in the western Sargasso <span class="hlt">Sea</span> near Bermuda</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Conte, Maureen H.; Ralph, Nate; Ross, Edith H.</p> <p></p> <p>Since 1978, the Oceanic <span class="hlt">Flux</span> Program (OFP) time-series sediment traps have measured particle <span class="hlt">fluxes</span> in the deep Sargasso <span class="hlt">Sea</span> near Bermuda. There is currently a 20+yr <span class="hlt">flux</span> record at 3200-m depth, a 12+yr <span class="hlt">flux</span> at 1500-m depth, and a 9+yr record at 500-m depth. Strong seasonality is observed in mass <span class="hlt">flux</span> at all depths, with a <span class="hlt">flux</span> maximum in February-March and a smaller maximum in December-January. There is also significant interannual variability in the <span class="hlt">flux</span>, especially with respect to the presence/absence of the December-January <span class="hlt">flux</span> maximum and in the duration of the high <span class="hlt">flux</span> period in the spring. The <span class="hlt">flux</span> records at the three depths are surprisingly coherent, with no statistically significant temporal lag between 500 and 3200-m <span class="hlt">fluxes</span> at our biweekly sample resolution. Bulk compositional data indicate an extremely rapid decrease in the <span class="hlt">flux</span> of organic constituents with depth between 500 and 1500-m, and a smaller decrease with depth between 1500 and 3200-m depth. In contrast, carbonate <span class="hlt">flux</span> is uniform or increases slightly between 500 and 1500-m, possibly reflecting deep secondary calcification by foraminifera. The lithogenic <span class="hlt">flux</span> increases by over 50% between 500 and 3200-m depth, indicating strong deep water scavenging/repackaging of suspended lithogenic material. Concurrent with the rapid changes in <span class="hlt">flux</span> composition, there is a marked reduction in the heterogeneity of the sinking particle pool with depth, especially within the mesopelagic zone. By 3200-m depth, the bulk composition of the sinking particle pool is strikingly uniform, both seasonally and over variations in mass <span class="hlt">flux</span> of more than an order of magnitude. These OFP results provide strong indirect evidence for the intensity of reprocessing of the particle pool by resident zooplankton within mesopelagic and bathypelagic waters. The rapid loss of organic components, the marked reduction in the heterogeneity of the bulk composition of the <span class="hlt">flux</span>, and the increase in terrigenous <span class="hlt">fluxes</span> with depth are most</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/2017APS..DFDD19009Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..DFDD19009Y"><span>Wave-Induced Momentum <span class="hlt">Flux</span> over Wind-driven Surface Waves</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yousefi, Kianoosh; Veron, Fabrice; Buckley, Marc; Husain, Nyla; Hara, Tetsu</p> <p>2017-11-01</p> <p>In recent years, the exchange of momentum between the atmosphere and the ocean has been the subject of several investigations. Although the role of surface waves on the <span class="hlt">air-sea</span> momentum <span class="hlt">flux</span> is now well established, detailed quantitative measurements of wave-induced momentum <span class="hlt">fluxes</span> are lacking. In the current study, using a combined Particle Image Velocimetry (PIV) and Laser Induced Fluorescence (LIF) system, we obtained laboratory measurements of the airflow velocity above surface waves for wind speeds ranging from 0.86 to 16.63 m s-1. The mean, turbulent, and wave-coherent velocity fields are then extracted from instantaneous measurements. Wave-induced stress can, therefore, be estimated. In strongly forced cases in high wind speeds, the wave-induced stress near the surface is a significant fraction of the total stress. At lower wind speeds and larger wave ages, the wave-induced stress is positive very close to the surface, below the critical height and decreases to a negative value further above the critical height. This indicates a shift in the direction of the wave-coherent momentum <span class="hlt">flux</span> across the critical layer. NSF OCE1458977, NSF OCE1634051.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29195200','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29195200"><span>Spatial distribution and seasonal variation of four current-use pesticides (CUPs) in <span class="hlt">air</span> and surface water of the Bohai <span class="hlt">Sea</span>, China.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Liu, Lin; Tang, Jianhui; Zhong, Guangcai; Zhen, Xiaomei; Pan, Xiaohui; Tian, Chongguo</p> <p>2018-04-15</p> <p>Current-use pesticides (CUPs) are widely used in agriculture, and some are listed as persistent organic pollutants (POPs) due to their bioaccumulative and toxic properties. China is one of the largest producers and users of pesticides in the world. However, very limited data are available about the environmental fates of CUPs. Four CUPs (trifluralin, chlorothalonil, chlorpyrifos, and dicofol) in surface seawater and low atmospheric samples taken during research cruises on the Bohai <span class="hlt">Sea</span> in August and December 2016 and February 2017 were analyzed, we added the spring data sampled in May 2012 to the discussion of seasonal variation. In our study, chlorpyrifos was the most abundant CUPs in the gas phase with a mean abundance of 59.06±126.94pgm -3 , and dicofol had the highest concentration dissolved in seawater (mean: 115.94±123.16pgL -1 ). The concentrations of all target compounds were higher during May and August due to intensive use and relatively high temperatures in the spring and summer. Backward trajectories indicated that <span class="hlt">air</span> masses passing through the eastern coast of the Bohai <span class="hlt">Sea</span> contained high concentrations of pollutants, while the <span class="hlt">air</span> masses from the Bohai and Yellow <span class="hlt">Seas</span> were less polluted. The high concentration of pollutants in seawater was not only influenced by high yields from the source region of production or usage, but also by input from polluted rivers. Volatilization from surface water was found to be an important source of trifluralin and chlorpyrifos in the <span class="hlt">air</span>. <span class="hlt">Air-sea</span> gas exchange of chlorothalonil underwent strong net deposition (mean FRs: 51.67), which was driven by higher concentrations in <span class="hlt">air</span> and indicates that the Bohai <span class="hlt">Sea</span> acted as a sink for chlorothalonil. Copyright © 2017 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.C23E0542F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.C23E0542F"><span>Validation and Interpretation of a New <span class="hlt">Sea</span> Ice Globice Dataset Using Buoys and the Cice <span class="hlt">Sea</span> Ice Model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Flocco, D.; Laxon, S. W.; Feltham, D. L.; Haas, C.</p> <p>2011-12-01</p> <p>The GlobIce project has provided high resolution <span class="hlt">sea</span> ice product datasets over the Arctic derived from SAR data in the ESA archive. The products are validated <span class="hlt">sea</span> ice motion, deformation and <span class="hlt">fluxes</span> through straits. GlobIce <span class="hlt">sea</span> ice velocities, deformation data and <span class="hlt">sea</span> ice concentration have been validated using buoy data provided by the International Arctic Buoy Program (IABP). Over 95% of the GlobIce and buoy data analysed fell within 5 km of each other. The GlobIce Eulerian image pair product showed a high correlation with buoy data. The <span class="hlt">sea</span> ice concentration product was compared to SSM/I data. An evaluation of the validity of the GlobICE data will be presented in this work. GlobICE <span class="hlt">sea</span> ice velocity and deformation were compared with runs of the CICE <span class="hlt">sea</span> ice model: in particular the mass <span class="hlt">fluxes</span> through the straits were used to investigate the correlation between the winter behaviour of <span class="hlt">sea</span> ice and the <span class="hlt">sea</span> ice state in the following summer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JMS...167...33K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JMS...167...33K"><span>Biogeochemical properties of sinking particles in the southwestern part of the East <span class="hlt">Sea</span> (Japan <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>Kim, Minkyoung; Hwang, Jeomshik; Rho, TaeKeun; Lee, Tongsup; Kang, Dong-Jin; Chang, Kyung-Il; Noh, Suyun; Joo, HuiTae; Kwak, Jung Hyun; Kang, Chang-Keun; Kim, Kyung-Ryul</p> <p>2017-03-01</p> <p>This study investigates the biological pump system in the East <span class="hlt">Sea</span> (Japan <span class="hlt">Sea</span>) by conducting an analysis of the total particle <span class="hlt">flux</span>, biogenic material composition, and carbon isotope ratios of sinking particles. The samples were collected for one year starting from March 2011 using time-series sediment traps deployed at depths of 1040 m and 2280 m on bottom-tethered mooring at Station EC1 (37.33°N, 131.45°E; 2300 m water depth) in the Ulleung Basin (UB), southwestern part of the East <span class="hlt">Sea</span>. The temporal variation in the particulate organic carbon (POC) <span class="hlt">flux</span> at 1000 m shows a good relationship with the primary production in the corresponding surface water. The ratio of POC <span class="hlt">flux</span> at 1000 m to satellite-based primary production in the corresponding region in the UB was 3%, which is comparable to the values of 2 to 5% estimated from previous studies of other part of the East <span class="hlt">Sea</span>. The lithogenic material accounted for > 17% of the sinking particles at 1000 m and for a larger fraction of 40 to 60% at 2280 m. The radiocarbon contents of the sinking POC at both trap depths imply the additional supply of aged POC, with a much greater contribution at 2280 m. Overall, the particle <span class="hlt">flux</span> in the deep interior of the East <span class="hlt">Sea</span> appears to be controlled by the supply of complex sources, including aeolian input, the lateral supply of resuspended sediments, and biological production in the surface water.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20010069509','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20010069509"><span>A Multilayer Dataset of SSM/I-Derived Global Ocean Surface Turbulent <span class="hlt">Fluxes</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chou, Shu-Hsien; Shie, Chung-Lin; Atlas, Robert M.; Ardizzone, Joe; Nelkin, Eric; Einaud, Franco (Technical Monitor)</p> <p>2001-01-01</p> <p>A dataset including daily- and monthly-mean turbulent <span class="hlt">fluxes</span> (momentum, latent heat, and sensible heat) and some relevant parameters over global oceans, derived from the Special Sensor Microwave/Imager (SSM/I) data, for the period July 1987-December 1994 and the 1988-94 annual and monthly-mean climatologies of the same variables is created. It has a spatial resolution of 2.0deg x 2.5deg latitude-longitude. The retrieved surface <span class="hlt">air</span> humidity is found to be generally accurate as compared to the collocated radiosonde observations over global oceans. The retrieved wind stress and latent heat <span class="hlt">flux</span> show useful accuracy as verified against research quality measurements of ship and buoy in the western equatorial Pacific. The 1988-94 seasonal-mean wind stress and latent heat <span class="hlt">flux</span> show reasonable patterns related to seasonal variations of the atmospheric general circulation. The patterns of 1990-93 annual-mean turbulent <span class="hlt">fluxes</span> and input variables are generally in good agreement with one of the best global analyzed <span class="hlt">flux</span> datasets that based on COADS (comprehensive ocean-atmosphere data set) with corrections on wind speeds and covered the same period. The retrieved wind speed is generally within +/-1 m/s of the COADS-based, but is stronger by approx. 1-2 m/s in the northern extratropical oceans. The discrepancy is suggested to be mainly due to higher COADS-modified wind speeds resulting from underestimation of anemometer heights. Compared to the COADS-based, the retrieved latent heat <span class="hlt">flux</span> and <span class="hlt">sea-air</span> humidity difference are generally larger with significant differences in the trade wind zones and the ocean south of 40degS (up to approx. 40-60 W/sq m and approx. 1-1.5 g/kg). The discrepancy is believed to be mainly caused by higher COADS-based surface <span class="hlt">air</span> humidity arising from the overestimation of dew point temperatures and from the extrapolation of observed high humidity southward into data-void regions south of 40degS. The retrieved sensible heat <span class="hlt">flux</span> is generally within +/-5</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040082184&hterms=hear&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dhear','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040082184&hterms=hear&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dhear"><span>Offline GCSS Intercomparison of Cloud-Radiation Interaction and Surface <span class="hlt">Fluxes</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Tao, W.-K.; Johnson, D.; Krueger, S.; Zulauf, M.; Donner, L.; Seman, C.; Petch, J.; Gregory, J.</p> <p>2004-01-01</p> <p>Simulations of deep tropical clouds by both cloud-resolving models (CRMs) and single-column models (SCMs) in the GEWEX Cloud System Study (GCSS) Working Group 4 (WG4; Precipitating Convective Cloud Systems), Case 2 (19-27 December 1992, TOGA-COARE IFA) have produced large differences in the mean heating and moistening rates (-1 to -5 K and -2 to 2 grams per kilogram respectively). Since the large-scale advective temperature and moisture "forcing" are prescribed for this case, a closer examination of two of the remaining external types of "forcing", namely radiative heating and <span class="hlt">air/sea</span> hear and moisture transfer, are warranted. This paper examines the current radiation and surface <span class="hlt">flux</span> of parameterizations used in the cloud models participating in the GCSS WG4, be executing the models "offline" for one time step (12 s) for a prescribed atmospheric state, then examining the surface and radiation <span class="hlt">fluxes</span> from each model. The dynamic, thermodynamic, and microphysical fluids are provided by the GCE-derived model output for Case 2 during a period of very active deep convection (westerly wind burst). The surface and radiation <span class="hlt">fluxes</span> produced from the models are then divided into prescribed convective, stratiform, and clear regions in order to examine the role that clouds play in the <span class="hlt">flux</span> parameterizations. The results suggest that the differences between the models are attributed more to the surface <span class="hlt">flux</span> parameterizations than the radiation schemes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19351614','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19351614"><span>Effect of duration of exposure to polluted <span class="hlt">air</span> environment on lung function in subjects exposed to crude oil spill into <span class="hlt">sea</span> water.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Meo, Sultan Ayoub; Al-Drees, Abdul Majeed; Rasheed, Shahzad; Meo, Imran Mu; Khan, Muhammad Mujahid; Al-Saadi, Muslim M; Alkandari, Jasem Ramadan</p> <p>2009-01-01</p> <p>Oil spill in <span class="hlt">sea</span> water represents a huge environmental disaster for marine life and humans in the vicinity. The aim was to investigate the effect of duration of exposure to polluted <span class="hlt">air</span> environment on lung function in subjects exposed to crude oil spill into <span class="hlt">sea</span> water. The present study was conducted under the supervision of Department of Physiology, College of Medicine, King Khalid University Hospital, King Saud University, Riyadh, Saudi Arabia, during the period July 2003 - December 2004. This was a comparative study of spirometry in 31 apparently healthy, non smoking, male workers, exposed to crude oil spill environment during the oil cleaning operation. The exposed group was matched with similar number of male, non smoking control subjects. Pulmonary function test was performed by using an electronic spirometer. Subjects exposed to polluted <span class="hlt">air</span> for periods longer than 15 days showed a significant reduction in Forced Vital Capacity (FVC), Forced Expiratory Volume in First Second (FEV1), Forced Expiratory Flow in 25-25% (FEF25-75%) and Maximal Voluntary Ventilation (MVV). <span class="hlt">Air</span> environment polluted due to crude oil spill into <span class="hlt">sea</span> water caused impaired lung function and this impairment was associated with dose response effect of duration of exposure to <span class="hlt">air</span> polluted by crude oil spill into <span class="hlt">sea</span> water.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSPO44C3170S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSPO44C3170S"><span>The Impact of Salinity on the Seasonal and Interannual Variability of the Upper Ocean Structure and <span class="hlt">Air/Sea</span> Interaction in the South Eastern Tropical Indian Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Soares, S. M.; Richards, K. J.; Annamalai, H.; Natarov, A.</p> <p>2016-02-01</p> <p>The Seychelles-Chagos thermocline ridge (SCRT) in the south-eastern tropical Indian Ocean is believed to play an important role on <span class="hlt">air/sea</span> interactions at monsoonal and intraseasonal timescales. Large gains in predictability of monsoon and intraseasonal variability may result from studying the mechanisms of ocean feedback to the atmosphere in the SCRT region. ARGO data from 2005-2014 show a marked salinity and temperature annual cycle, where mixed layer waters are freshest and warmest around February-March and saltiest and coldest around July-August in the eastern side of the SCRT. An analysis of the mixed-layer salt budget using a mix of observational gridded products and a coupled model shows that: i) surface freshwater <span class="hlt">fluxes</span> do not play a significant role on the SCRT salinity annual cycle, ii) the freshening during austral Spring is primarily driven by zonal advection of the large pool of less saline waters off the coast of southeast Asia and bay of Bengal, while meridional advection accounts for a large fraction of the salting during Fall. The largest interannual anomalies in the ARGO salinity record occur in the aftermath of the negative Indian Ocean Dipole events of 2005 and 2010, when February mixed layer freshening was much reduced. The appearance of the fresher waters were evident in the DYNAMO/CINDY data collected in the area during Spring 2011 following the passage of a downwelling Rossby wave. Lagrangian parcel tracking indicates a variety of sources for these fresher waters, but generally agrees with the ARGO results above. The fresh surface layer had a significant impact on the measured turbulence and mixing and may have impacted the development of Madden-Julien Oscillation events observed during DYNAMO/CINDY. Given these findings, we examine in detail the suite of DYNAMO observations, combining them with numerical modeling experiments to determine the role of eddy <span class="hlt">fluxes</span> and vertical processes on the formation of these freshwater layers, as well as</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21815160','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21815160"><span>Quality changes in <span class="hlt">sea</span> urchin (Strongylocentrotus nudus) during storage in artificial seawater saturated with oxygen, nitrogen and <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>Wang, Chao; Xue, Changhu; Xue, Yong; Li, Zhaojie; Lv, Yingchun; Zhang, Hao</p> <p>2012-01-15</p> <p><span class="hlt">Sea</span> urchin gonads are highly valued seafood that degenerates rapidly during the storage period. To study the influence of dissolved oxygen concentration on quality changes of <span class="hlt">sea</span> urchin (Strongylocentrotus nudus) gonads, they were stored in artificial seawater saturated with oxygen, nitrogen or <span class="hlt">air</span> at 5 ± 1 °C for 12 days. The sensory acceptability limit was 11-12, 6-7 and 7-8 days for gonads with oxygen, nitrogen or <span class="hlt">air</span> packaging, respectively. Total volatile basic nitrogen (TVB-N) values reached 22.60 ± 1.32, 32.37 ± 1.37 and 24.91 ± 1.54 mg 100 g(-1) for gonads with oxygen, nitrogen or <span class="hlt">air</span> packaging at the points of near to, exceeding and reaching the limit of sensory acceptability, indicating that TVB-N values of about 25 mg 100 g(-1) should be regarded as the limit of acceptability for <span class="hlt">sea</span> urchin gonads. Relative ATP content values were 56.55%, 17.36% and 18.75% for gonads with oxygen, nitrogen or <span class="hlt">air</span> packaging, respectively, on day 2. K-values were 19.37%, 25.05% and 29.02% for gonads with oxygen, nitrogen or <span class="hlt">air</span> packaging, respectively, on day 2. Both pH and aerobic plate count values showed no significant difference (P > 0.05) for gonads with the three treatments. Gonads with oxygen packaging had lower sensory demerit point (P < 0.05) and TVB-N values (P < 0.05), and higher relative ATP content (P < 0.01) and K-values (P < 0.05), than that with nitrogen or <span class="hlt">air</span> packaging, with an extended shelf life of 4-5 days during storage in artificial seawater at 5 ± 1 °C. Copyright © 2011 Society of Chemical Industry.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29440667','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29440667"><span>Poleward upgliding Siberian atmospheric rivers over <span class="hlt">sea</span> ice heat up Arctic upper <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>Komatsu, Kensuke K; Alexeev, Vladimir A; Repina, Irina A; Tachibana, Yoshihiro</p> <p>2018-02-13</p> <p>We carried out upper <span class="hlt">air</span> measurements with radiosondes during the summer over the Arctic Ocean from an icebreaker moving poleward from an ice-free region, through the ice edge, and into a region of thick ice. Rapid warming of the Arctic is a significant environmental issue that occurs not only at the surface but also throughout the troposphere. In addition to the widely accepted mechanisms responsible for the increase of tropospheric warming during the summer over the Arctic, we showed a new potential contributing process to the increase, based on our direct observations and supporting numerical simulations and statistical analyses using a long-term reanalysis dataset. We refer to this new process as "Siberian Atmospheric Rivers (SARs)". Poleward upglides of SARs over cold <span class="hlt">air</span> domes overlying <span class="hlt">sea</span> ice provide the upper atmosphere with extra heat via condensation of water vapour. This heating drives increased buoyancy and further strengthens the ascent and heating of the mid-troposphere. This process requires the combination of SARs and <span class="hlt">sea</span> ice as a land-ocean-atmosphere system, the implication being that large-scale heat and moisture transport from the lower latitudes can remotely amplify the warming of the Arctic troposphere in the summer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24570212','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24570212"><span>Mercury in precipitation at an urbanized coastal zone of the Baltic <span class="hlt">Sea</span> (Poland).</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Saniewska, Dominika; Bełdowska, Magdalena; Bełdowski, Jacek; Falkowska, Lucyna</p> <p>2014-11-01</p> <p>Wet deposition is an important source of metals to the <span class="hlt">sea</span>. The temporal variability of Hg concentrations in precipitation, and the impact of <span class="hlt">air</span> masses of different origins over the Polish coastal zone were assessed. Samples of precipitation were collected (August 2008-May 2009) at an urbanized coastal station in Poland. Hg analyses were conducted using CVAFS. These were the first measurements of Hg concentration in precipitation obtained in the Polish coastal zone. Since Poland was identified as the biggest emitter of Hg to the Baltic, these data are very important. In the heating and non-heating season, Hg concentrations in precipitation were similar. Hg wet deposition <span class="hlt">flux</span> dominated in summer, when the production of biomass in the aquatic system was able to actively adsorb Hg. Input of metal to the <span class="hlt">sea</span> was attributed to regional and distant sources. Maritime <span class="hlt">air</span> masses, through transformation of Hg(0), were an essential vector of mercury in precipitation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19800015467','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19800015467"><span>Gas and aerosol <span class="hlt">fluxes</span>. [emphasizing sulfur, nitrogen, and carbon</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Martens, C. S.</p> <p>1980-01-01</p> <p>The development of remote sensing techniques to address the global need for accurate distribution and <span class="hlt">flux</span> determinations of both man made and natural materials which affect the chemical composition of the atmosphere, the heat budget of the Earth, and the depletion, of stratospheric ozone is considered. Specifically, trace gas <span class="hlt">fluxes</span>, <span class="hlt">sea</span> salt aerosol production, and the effect of <span class="hlt">sea</span> surface microlayer on gas and aerosol <span class="hlt">fluxes</span> are examined. Volatile sulfur, carbon, nitrogen, and halocarbon compounds are discussed including a statement of the problem associated with each compound or group of compounds, a brief summary of current understanding, and suggestions for needed research.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012BGD.....914751L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012BGD.....914751L"><span>Plankton ecosystem functioning and nitrogen <span class="hlt">fluxes</span> in the most oligotrophic waters of the Beaufort <span class="hlt">Sea</span>, Arctic Ocean: a modeling study</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Le Fouest, V.; Zakardjian, B.; Xie, H.; Raimbault, P.; Joux, F.; Babin, M.</p> <p>2012-10-01</p> <p>The Arctic Ocean (AO) undergoes profound changes of its physical and biotic environments due to climate change. The greater light exposure and stratification alter its plankton ecosystem structure, functioning and productivity promoting oligotrophy in some areas as the Beaufort <span class="hlt">Sea</span>. A one-dimension (1-D) physical-biological coupled model based on the large multiparametric database of the Malina project in the Beaufort <span class="hlt">Sea</span> was used (i) to infer the functioning and nitrogen <span class="hlt">fluxes</span> within the summer plankton ecosystem and (ii) to assess the model sensitivity to key light-associated processes involved in nutrient recycling and phytoplankton growth. The coupled model suggested that ammonium photochemically produced from photosensitive dissolved organic nitrogen (i.e. photoammonification process) was a necessary nitrogen source to achieve the observed levels of microbial biomass and production. It contributed to ca. two-thirds and one-third of the simulated surface (0-10 m) and depth-integrated primary and bacterial production, respectively. The model also suggested that carbon to chlorophyll ratios for small (< 5 μm) phytoplankton (ca. 15-45 g g-1) lower than those commonly used in biogeochemical models applied to the AO were required to simulate the observed herbivorous versus microbial food web competition and realistic nitrogen <span class="hlt">fluxes</span> in the Beaufort <span class="hlt">Sea</span> oligotrophic waters. In face of accelerating Arctic warming, more attention should be paid in the future to the mechanistic processes involved in food webs and functional groups competition, nutrient recycling and primary production in poorly productive waters of the AO as they are expected to expand rapidly.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..14.3174F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..14.3174F"><span>Validation and Interpretation of a new <span class="hlt">sea</span> ice GlobIce dataset using buoys and the CICE <span class="hlt">sea</span> ice model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Flocco, D.; Laxon, S. W.; Feltham, D. L.; Haas, C.</p> <p>2012-04-01</p> <p>The GlobIce project has provided high resolution <span class="hlt">sea</span> ice product datasets over the Arctic derived from SAR data in the ESA archive. The products are validated <span class="hlt">sea</span> ice motion, deformation and <span class="hlt">fluxes</span> through straits. GlobIce <span class="hlt">sea</span> ice velocities, deformation data and <span class="hlt">sea</span> ice concentration have been validated using buoy data provided by the International Arctic Buoy Program (IABP). Over 95% of the GlobIce and buoy data analysed fell within 5 km of each other. The GlobIce Eulerian image pair product showed a high correlation with buoy data. The <span class="hlt">sea</span> ice concentration product was compared to SSM/I data. An evaluation of the validity of the GlobICE data will be presented in this work. GlobICE <span class="hlt">sea</span> ice velocity and deformation were compared with runs of the CICE <span class="hlt">sea</span> ice model: in particular the mass <span class="hlt">fluxes</span> through the straits were used to investigate the correlation between the winter behaviour of <span class="hlt">sea</span> ice and the <span class="hlt">sea</span> ice state in the following summer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015BGeo...12.5103M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015BGeo...12.5103M"><span>Downward particle <span class="hlt">flux</span> and carbon export in the Beaufort <span class="hlt">Sea</span>, Arctic Ocean; the role of zooplankton</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Miquel, J.-C.; Gasser, B.; Martín, J.; Marec, C.; Babin, M.; Fortier, L.; Forest, A.</p> <p>2015-08-01</p> <p>As part of the international, multidisciplinary project Malina, downward particle <span class="hlt">fluxes</span> were investigated by means of a drifting multi-sediment trap mooring deployed at three sites in the Canadian Beaufort <span class="hlt">Sea</span> in late summer 2009. Mooring deployments lasted between 28 and 50 h and targeted the shelf-break and the slope along the Beaufort-Mackenzie continental margin, as well as the edge between the Mackenzie Shelf and the Amundsen Gulf. Besides analyses of C and N, the collected material was investigated for pigments, phyto- and microzooplankton, faecal pellets and swimmers. The measured <span class="hlt">fluxes</span> were relatively low, in the range of 11-54 mg m-2 d-1 for the total mass, 1-15 mg C m-2 d-1 for organic carbon and 0.2-2.5 mg N m-2 d-1 for nitrogen. Comparison with a long-term trap data set from the same sampling area showed that the short-term measurements were at the lower end of the high variability characterizing a rather high <span class="hlt">flux</span> regime during the study period. The sinking material consisted of aggregates and particles that were characterized by the presence of hetero- and autotrophic microzooplankters and diatoms and by the corresponding pigment signatures. Faecal pellets contribution to sinking carbon <span class="hlt">flux</span> was important, especially at depths below 100 m, where they represented up to 25 % of the total carbon <span class="hlt">flux</span>. The vertical distribution of different morphotypes of pellets showed a marked pattern with cylindrical faeces (produced by calanoid copepods) present mainly within the euphotic zone, whereas elliptical pellets (produced mainly by smaller copepods) were more abundant at mesopelagic depths. These features, together with the density of matter within the pellets, highlighted the role of the zooplankton community in the transformation of carbon issued from the primary production and the transition of that carbon from the productive surface zone to the Arctic Ocean's interior. Our data indicate that sinking carbon <span class="hlt">flux</span> in this late summer period is primarily</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2000DSRII..47.3423G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2000DSRII..47.3423G"><span>Seasonal patterns of water column particulate organic carbon and <span class="hlt">fluxes</span> in the Ross <span class="hlt">Sea</span>, Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gardner, Wilford D.; Richardson, Mary Jo; Smith, Walker O.</p> <p></p> <p>The standing stock of particulate organic carbon (POC) was determined during five cruises in the Ross <span class="hlt">Sea</span> in 1996 and 1997 and compared with primary production of carbon measured in short-term 14C-incubations and the <span class="hlt">flux</span> of organic carbon collected in moored sediment traps. POC concentrations were estimated from transmissometer profiles that were calibrated with discrete POC bottle samples from each cruise. The mean standing stock of POC integrated to a depth of 100 m and averaged along a 330 km transect at 76.5°S in mid-October (early spring) was only 240 mmol C m -2, but more than doubled to 560 mmol C m -2 10 days later. By mid-January (summer) the standing stock had increased by an order of magnitude to ˜5300 mmol C m -2, but dropped to 3500 mmol C m -2 one week later. By late April (autumn), the standing stock was only 200 mmol C m -2. The following spring the standing stock increased from 700 mmol C m -2 in late November to 2200 mmol C m -2 in early December. Despite the high standing stock in the photic zone in summer, 1997, little POC was collected in the moored sediment traps until late summer (February-March) when the traps showed an increase in POC and silica <span class="hlt">flux</span>. A three-fold increase in POC <span class="hlt">flux</span> occurred in autumn (March-April) dominated by pteropods, but the standing stock of POC in the photic zone at that time was very low. Light-scattering sensor data suggest that, although present in all seasons, aggregates were most abundant in autumn and were distributed throughout the water column. These aggregates may have temporarily stored POC and provided food support for a pteropod population that died and settled into the traps in March-April. Still, the trap POC <span class="hlt">flux</span> was only 5% of the peak standing stock. Resuspension and lateral advection of recently settled organic matter from a nearby topographic high may explain the larger <span class="hlt">flux</span> measured in the deep sediment traps, a <span class="hlt">flux</span> that continued into winter.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20020033022','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20020033022"><span>Estimating the Ocean Flow Field from Combined <span class="hlt">Sea</span> Surface Temperature and <span class="hlt">Sea</span> Surface Height Data</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Stammer, Detlef; Lindstrom, Eric (Technical Monitor)</p> <p>2002-01-01</p> <p>This project was part of a previous grant at MIT that was moved over to the Scripps Institution of Oceanography (SIO) together with the principal investigator. The final report provided here is concerned only with the work performed at SIO since January 2000. The primary focus of this project was the study of the three-dimensional, absolute and time-evolving general circulation of the global ocean from a combined analysis of remotely sensed fields of <span class="hlt">sea</span> surface temperature (SST) and <span class="hlt">sea</span> surface height (SSH). The synthesis of those two fields was performed with other relevant physical data, and appropriate dynamical ocean models with emphasis on constraining ocean general circulation models by a combination of both SST and SSH data. The central goal of the project was to improve our understanding and modeling of the relationship between the SST and its variability to internal ocean dynamics, and the overlying atmosphere, and to explore the relative roles of <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> and internal ocean dynamics in establishing anomalies in SST on annual and longer time scales. An understanding of those problems will feed into the general discussion on how SST anomalies vary with time and the extend to which they interact with the atmosphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70173622','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70173622"><span>Shifts in controls on the temporal coherence of throughfall chemical <span class="hlt">flux</span> in Acadia National Park, Maine, USA</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Nelson, Sarah J.; Webster, Katherine E.; Loftin, Cynthia S.; Weathers, Kathleen C.</p> <p>2013-01-01</p> <p>Major ion and mercury (Hg) inputs to terrestrial ecosystems include both wet and dry deposition (total deposition). Estimating total deposition to sensitive receptor sites is hampered by limited information regarding its spatial heterogeneity and seasonality. We used measurements of throughfall <span class="hlt">flux</span>, which includes atmospheric inputs to forests and the net effects of canopy leaching or uptake, for ten major ions and Hg collected during 35 time periods in 1999–2005 at over 70 sites within Acadia National Park, Maine to (1) quantify coherence in temporal dynamics of seasonal throughfall deposition and (2) examine controls on these patterns at multiple scales. We quantified temporal coherence as the correlation between all possible site pairs for each solute on a seasonal basis. In the summer growing season and autumn, coherence among pairs of sites with similar vegetation was stronger than for site-pairs that differed in vegetation suggesting that interaction with the canopy and leaching of solutes differed in coniferous, deciduous, mixed, and shrub or open canopy sites. The spatial pattern in throughfall hydrologic inputs across Acadia National Park was more variable during the winter snow season, suggesting that snow re-distribution affects net hydrologic input, which consequently affects chemical <span class="hlt">flux</span>. <span class="hlt">Sea</span>-salt corrected calcium concentrations identified a shift in <span class="hlt">air</span> mass sources from maritime in winter to the continental industrial corridor in summer. Our results suggest that the spatial pattern of throughfall hydrologic <span class="hlt">flux</span>, dominant seasonal <span class="hlt">air</span> mass source, and relationship with vegetation in winter differ from the spatial pattern of throughfall <span class="hlt">flux</span> in these solutes in summer and autumn. The coherence approach applied here made clear the strong influence of spatial heterogeneity in throughfall hydrologic inputs and a maritime <span class="hlt">air</span> mass source on winter patterns of throughfall <span class="hlt">flux</span>. By contrast, vegetation type was the most important influence on</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=236017&Lab=NERL&keyword=evapotranspiration&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50','EPA-EIMS'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=236017&Lab=NERL&keyword=evapotranspiration&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50"><span>Surface <span class="hlt">Flux</span> Modeling for <span class="hlt">Air</span> Quality Applications</span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p>For many gasses and aerosols, dry deposition is an important sink of atmospheric mass. Dry deposition <span class="hlt">fluxes</span> are also important sources of pollutants to terrestrial and aquatic ecosystems. The surface <span class="hlt">fluxes</span> of some gases, such as ammonia, mercury, and certain volatile organic c...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017CSR...143...29J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017CSR...143...29J"><span>Short-term variability in particle <span class="hlt">flux</span>: Storms, blooms and river discharge in a coastal <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>Johannessen, Sophia C.; Macdonald, Robie W.; Wright, Cynthia A.; Spear, David J.</p> <p>2017-07-01</p> <p>The <span class="hlt">flux</span> and composition of particles sinking in the surface ocean vary on a wide range of time scales. This variability is a component of underwater weather that is analogous to rain. The rain of particles in the coastal ocean is affected by atmospheric events, such as rainstorms and windstorms; by events on land, such as peaks in river discharge or coastal erosion; and by events within the surface ocean, such as phytoplankton blooms. Here, we use a four-year record of sinking particles collected using sediment traps moored at 50 m depth at two locations in the Strait of Georgia, a coastal <span class="hlt">sea</span> off the west coast of Canada, to determine the relative importance of short-term events to particle <span class="hlt">flux</span>. We identify four dominant types of particle-<span class="hlt">flux</span> events: those associated with 1) summer freshet of the Fraser River, 2) rainstorms, 3) phytoplankton blooms, and 4) a jellyfish bloom. The relative importance of these events differs between the southern Strait, where the Fraser River freshet dominates <span class="hlt">flux</span> and variability, and the northern Strait, where the effects of phytoplankton blooms, rainstorms and small local rivers are more evident. During 2008-2012, half of each year's total <span class="hlt">flux</span> accumulated over 10-26% of the year in the southern Strait, mainly during the Fraser River freshet. In the northern Strait half of the annual <span class="hlt">flux</span> accumulated over 22-36% of the year, distributed among small events during spring to fall. The composition of the sinking particulate matter also varied widely, with organic carbon and biogenic silica ranging over 0.70-5.7% (excluding one event) and 0.4-14%, respectively, in the south, compared with 0.17-22% and 0.31-33% in the north. Windstorms had no immediate effect on particle <span class="hlt">flux</span> in either basin. A large phytoplankton bloom in April 2011, in the northern Strait contributed 25% of the year's organic carbon at that site and 53% of the biogenic silica. A jellyfish bloom in July 2008 contributed 16% of the year's nitrogen and 12% of the year</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_23 --> <div id="page_24" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="461"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A53B2224L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A53B2224L"><span>The Siberian High and Arctic <span class="hlt">Sea</span> Ice: Long-term Climate Change and Impacts on <span class="hlt">Air</span> Pollution during Wintertime 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>Long, X.; Zhao, S.; Feng, T.; Tie, X.; Li, G.</p> <p>2017-12-01</p> <p>China has undergone severe <span class="hlt">air</span> pollution during wintertime as national industrialization and urbanization have been increasingly developed in the past three decades. It has been suggested that high emission and adverse weather patterns contribute to wintertime <span class="hlt">air</span> pollution. Recent studies propose that climate change and Arctic <span class="hlt">sea</span> ice loss likely lead to extreme haze events in winter. Here we use two reanalysis and observational datasets to present the trends of Siberian High (SH) intensity over Eurasia, and Arctic temperature and <span class="hlt">sea</span> ice. The results show the Arctic region of Asia is becoming warming accompanied by a rapid decline of <span class="hlt">sea</span> ice while Eurasia is cooling and SH intensity is gradually enhancing. Wind patterns induced by these changes cause straight westerly prevailing over Eurasia at the year of weak SH while strengthened northerly winds at the year of strong SH. Therefore, we utilize regional dynamical and chemical WRF-Chem model to determine the impact of SH intensity difference on wintertime <span class="hlt">air</span> pollution in China. As a result, enhancing northerly winds at the year of strong SH rapidly dilute and transport <span class="hlt">air</span> pollution, causing a decline of 50 - 400 µg m-3 PM2.5 concentrations relative to that at the year of weak SH. We also assess the impact of emission reduction to half the current level on <span class="hlt">air</span> pollution. The results show that emission reduction by 50% has an equivalent impact as the variability of SH intensity. This suggests that climate change over Eurasia has largely offset the negative impact of emission on <span class="hlt">air</span> pollution and it is urgently needed to take measures to mitigate <span class="hlt">air</span> pollution. In view of current high emission scenario in China, it will be a long way to effectively mitigate, or ultimately prevent wintertime <span class="hlt">air</span> pollution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19950031271&hterms=coriolis+effect&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dcoriolis%2Beffect','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19950031271&hterms=coriolis+effect&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dcoriolis%2Beffect"><span><span class="hlt">Sea</span> breezes and advective effects in southwest James Bay</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mckendry, Ian; Roulet, Nigel</p> <p>1994-01-01</p> <p>Observations from a transect extending 100 km inland during the Northern Wetlands Study (NOWES) in 1990 show that the <span class="hlt">sea</span> breeze develops on approximately 25% of days during summer and may penetrate up to 100 km inland on occasions. The <span class="hlt">sea</span> breeze exhibits a marked diurnal clockwise rotation as a result of the Coriolis effect along the unobstructed coastline. The marine advective effect is shown to depend on gradient wind direction. With northwesterly upper level flow the <span class="hlt">sea</span> breeze tends to be northeasterly in direction and is associated with decreased temperatures and vapor pressure deficits (VPD). With southwesterly upper level flow the <span class="hlt">sea</span> breeze tends to have a southeasterly direction and less effect on temperatures and VPD. This is attributed to shorter residence times of <span class="hlt">air</span> parcels over water. For two cases, Colorado State University mesoscale model simulations show good agreement with surface wind observations and suggest that under northwesterly gradient flow, Bowen ratios are increased in the onshore flow along western James Bay, while during southwesterly gradient flow these effects are negligible. These results have implications for the interpretation of local climate, ecology, and hydrology as well as land-based and airborne turbulent <span class="hlt">flux</span> measurements made during NOWES.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19920010531','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19920010531"><span><span class="hlt">Sea</span> ice-atmosphere interaction. Application of multispectral satellite data in polar surface energy <span class="hlt">flux</span> estimates</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Steffen, Konrad; Key, Jeff; Maslanik, Jim; Haefliger, Marcel; Fowler, Chuck</p> <p>1992-01-01</p> <p>Satellite data for the estimation of radiative and turbulent heat <span class="hlt">fluxes</span> is becoming an increasingly important tool in large-scale studies of climate. One parameter needed in the estimation of these <span class="hlt">fluxes</span> is surface temperature. To our knowledge, little effort has been directed to the retrieval of the <span class="hlt">sea</span> ice surface temperature (IST) in the Arctic, an area where the first effects of a changing climate are expected to be seen. The reason is not one of methodology, but rather our limited knowledge of atmospheric temperature, humidity, and aerosol profiles, the microphysical properties of polar clouds, and the spectral characteristics of the wide variety of surface types found there. We have developed a means to correct for the atmospheric attenuation of satellite-measured clear sky brightness temperatures used in the retrieval of ice surface temperature from the split-window thermal channels of the advanced very high resolution radiometer (AVHRR) sensors on-board three of the NOAA series satellites. These corrections are specified for three different 'seasons' and as a function of satellite viewing angle, and are expected to be applicable to the perennial ice pack in the central Arctic Basin.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.A43B3262V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.A43B3262V"><span>Land- and <span class="hlt">sea</span>-surface impacts on local coastal breezes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Veron, D. E.; Hughes, C.; Gilchrist, J.; Lodise, J.; Goldman, W.</p> <p>2014-12-01</p> <p>The state of Delaware has seen significant increases in population along the coastline in the past three decades. With this increase in population have come changes to the land surface, as forest and farmland has been converted to residential and commercial purposes, causing changes in the surface roughness, temperature, and land-atmosphere <span class="hlt">fluxes</span>. There is also a semi-permanent upwelling center in the spring and summer outside the Delaware Bay mouth that significantly changes the structure of the <span class="hlt">sea</span> surface temperature both inside and outside the Bay. Through a series of high resolution modeling and observational studies, we have determined that in cases of strong synoptic forcing, the impact of the land-surface on the boundary layer properties can be advected offshore, creating a false coastline and modifying the location and timing of the <span class="hlt">sea</span> breeze circulation. In cases of weak synoptic forcing, the influence of the upwelling and the tidal circulation of the Delaware Bay waters can greatly change the location, strength, and penetration of the <span class="hlt">sea</span> breeze. Understanding the importance of local variability in the surface-atmosphere interactions on the <span class="hlt">sea</span> breeze can lead to improved prediction of <span class="hlt">sea</span> breeze onset, penetration, and duration which is important for monitoring <span class="hlt">air</span> quality and developing offshore wind power production.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015SPIE.9456E..1DB','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015SPIE.9456E..1DB"><span><span class="hlt">Sea-air</span> boundary meteorological sensor</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Barbosa, Jose G.</p> <p>2015-05-01</p> <p>The atmospheric environment can significantly affect radio frequency and optical propagation. In the RF spectrum refraction and ducting can degrade or enhance communications and radar coverage. Platforms in or beneath refractive boundaries can exploit the benefits or suffer the effects of the atmospheric boundary layers. Evaporative ducts and surface-base ducts are of most concern for ocean surface platforms and evaporative ducts are almost always present along the <span class="hlt">sea-air</span> interface. The atmospheric environment also degrades electro-optical systems resolution and visibility. The atmospheric environment has been proven not to be uniform and under heterogeneous conditions substantial propagation errors may be present for large distances from homogeneous models. An accurate and portable atmospheric sensor to profile the vertical index of refraction is needed for mission planning, post analysis, and in-situ performance assessment. The meteorological instrument used in conjunction with a radio frequency and electro-optical propagation prediction tactical decision aid tool would give military platforms, in real time, the ability to make assessments on communication systems propagation ranges, radar detection and vulnerability ranges, satellite communications vulnerability, laser range finder performance, and imaging system performance predictions. Raman lidar has been shown to be capable of measuring the required atmospheric parameters needed to profile the atmospheric environment. The atmospheric profile could then be used as input to a tactical decision aid tool to make propagation predictions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AtmEn.112...20C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AtmEn.112...20C"><span>Dissolved organic nitrogen in wet deposition in a coastal city (Keelung) of the southern East China <span class="hlt">Sea</span>: Origin, molecular composition and <span class="hlt">flux</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, You-Xin; Chen, Hung-Yu; Wang, Wei; Yeh, Jun-Xian; Chou, Wen-Chen; Gong, Gwo-Ching; Tsai, Fu-Jung; Huang, Shih-Jen; Lin, Cheng-Ting</p> <p>2015-07-01</p> <p>In this study, we collected and analyzed rainwater samples from Keelung, Taiwan, which is a coastal city located south of the East China <span class="hlt">Sea</span> (ECS). From January 2012 until June 2013, 78 rainwater samples were collected over an 18-month period and were analyzed to examine the total dissolved nitrogen (TDN) and major ions in the rainwater. TDN can be divided into dissolved inorganic nitrogen (DIN) and dissolved organic nitrogen (DON). This study, which focused on the composition of DON, is the first study to employ ultrafiltration to separate DON in wet deposition into low molecular weight-DON (LMW-DON) and high molecular weight-DON (HMW-DON). The concentrations of dissolved nitrogen species observed in the research area between November 2012 and April 2013 were relatively high, whereas those observed between May 2013 and October 2012 were relatively low. The patterns of changes over time were similar to those of non-<span class="hlt">sea</span>-salt (nss) ions. The concentration of nss-ions was high during months in which the total dissolved nitrogen concentration was also high, which occur frequently during the spring and winter. In addition, the concentration of nss-ions was low during months in which the TDN concentration was low, which primarily occurs during the summer. The amounts of DIN and DON accounted for 63 ± 5% and 37 ± 5% of the TDN, respectively, and the percentage of the DIN was higher during the spring and winter. The concentrations of LMW-DON and HMW-DON, which accounted for 84 ± 3% and 16 ± 3% of the DON, respectively, were both high in the winter and low in the summer. The percentage of LMW-DON increased in the summer, possibly because of the numerous oceanic <span class="hlt">air</span> masses and typhoons. Furthermore, the percentage of HMW-DON increased in the spring, potentially due to biomass burning during agricultural activities. Regarding the wet deposition <span class="hlt">fluxes</span>, the DIN (197 ± 10.27 mmol m-2 yr-1) and DON (129 ± 6.82 mmol m-2 yr-1) accounted for approximately 64% and 36% of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015PalOc..30..384S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PalOc..30..384S"><span>Red <span class="hlt">Sea</span> circulation during marine isotope stage 5e</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Siccha, Michael; Biton, Eli; Gildor, Hezi</p> <p>2015-04-01</p> <p>We have employed a regional Massachusetts Institute of Technology oceanic general circulation model of the Red <span class="hlt">Sea</span> to investigate its circulation during marine isotope stage (MIS) 5e, the peak of the last interglacial, approximately 125 ka before present. Compared to present-day conditions, MIS 5e was characterized by higher Northern Hemisphere summer insolation, accompanied by increases in <span class="hlt">air</span> temperature of more than 2°C and global <span class="hlt">sea</span> level approximately 8 m higher than today. As a consequence of the increased seasonality, intensified monsoonal conditions with increased winds, rainfall, and humidity in the Red <span class="hlt">Sea</span> region are evident in speleothem records and supported by model simulations. To assess the dominant factors responsible for the observed changes, we conducted several sensitivity experiments in which the MIS 5 boundary conditions or forcing parameters were used individually. Overall, our model simulation for the last interglacial maximum reconstructs a Red <span class="hlt">Sea</span> that is colder, less ventilated and probably more oligotrophic than at present day. The largest alteration in Red <span class="hlt">Sea</span> circulation and properties was found for the simulation of the northward displacement and intensification of the African tropical rain belt during MIS 5e, leading to a notable increase in the fresh water <span class="hlt">flux</span> into the Red <span class="hlt">Sea</span>. Such an increase significantly reduced the Red <span class="hlt">Sea</span> salinity and exchange volume of the Red <span class="hlt">Sea</span> with the Gulf of Aden. The Red <span class="hlt">Sea</span> reacted to the MIS 5e insolation forcing by the expected increase in seasonal <span class="hlt">sea</span> surface temperature amplitude and overall cooling caused by lower temperatures during deep water formation in winter.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20020082936&hterms=time+series+modeling&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dtime%2Bseries%2Bmodeling','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20020082936&hterms=time+series+modeling&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dtime%2Bseries%2Bmodeling"><span>Bayesian Hierarchical <span class="hlt">Air-Sea</span> Interaction Modeling: Application to the Labrador <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Niiler, Pearn P.</p> <p>2002-01-01</p> <p>The objectives are to: 1) Organize data from 26 MINIMET drifters in the Labrador <span class="hlt">Sea</span>, including sensor calibration and error checking of ARGOS transmissions. 2) Produce wind direction, barometer, and <span class="hlt">sea</span> surface temperature time series. In addition, provide data from historical file of 150 SHARP drifters in the Labrador <span class="hlt">Sea</span>. 3) Work with data interpretation and data-modeling assimilation issues.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25460953','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25460953"><span>Physical and chemical processes of <span class="hlt">air</span> masses in the Aegean <span class="hlt">Sea</span> during Etesians: Aegean-GAME airborne campaign.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tombrou, M; Bossioli, E; Kalogiros, J; Allan, J D; Bacak, A; Biskos, G; Coe, H; Dandou, A; Kouvarakis, G; Mihalopoulos, N; Percival, C J; Protonotariou, A P; Szabó-Takács, B</p> <p>2015-02-15</p> <p>High-resolution measurements of gas and aerosols' chemical composition along with meteorological and turbulence parameters were performed over the Aegean <span class="hlt">Sea</span> (AS) during an Etesian outbreak in the framework of the Aegean-GAME airborne campaign. This study focuses on two distinct Etesian patterns, with similarities inside the Marine Atmospheric Boundary Layer (MABL) and differences at higher levels. Under long-range transport and subsidence the pollution load is enhanced (by 17% for CO, 11% for O3, 28% for sulfate, 62% for organic mass, 47% for elemental carbon), compared to the pattern with a weaker synoptic system. <span class="hlt">Sea</span> surface temperature (SST) was a critical parameter for the MABL structure, turbulent <span class="hlt">fluxes</span> and pollutants' distribution at lower levels. The MABL height was below 500 m asl over the eastern AS (favoring higher accumulation), and deeper over the western AS. The most abundant components of total PM1 were sulfate (40-50%) and organics (30-45%). Higher average concentrations measured over the eastern AS (131 ± 76 ppbv for CO, 62.5 ± 4.1 ppbv for O3, 5.0 ± 1.1 μg m(-3) for sulfate, 4.7 ± 0.9 μg m(-3) for organic mass and 0.5 ± 0.2 μg m(-3) for elemental carbon). Under the weaker synoptic system, cleaner but more acidic <span class="hlt">air</span> masses prevailed over the eastern part, while distinct aerosol layers of different signature were observed over the western part. The Aitken and accumulation modes contributed equally during the long-range transport, while the Aitken modes dominated during local or medium range transport. Copyright © 2014 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20010048424&hterms=dataset&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Ddataset','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20010048424&hterms=dataset&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Ddataset"><span>A 7.5-Year Dataset of SSM/I-Derived Surface Turbulent <span class="hlt">Fluxes</span> Over Global Oceans</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chou, Shu-Hsien; Shie, Chung-Lin; Atlas, Robert M.; Ardizzone, Joe; Nelkin, Eric; Einaudi, Franco (Technical Monitor)</p> <p>2001-01-01</p> <p>The surface turbulent <span class="hlt">fluxes</span> of momentum, latent heat, and sensible heat over global oceans are essential to weather, climate and ocean problems. Wind stress is the major forcing for driving the oceanic circulation, while Evaporation is a key component of hydrological cycle and surface heat budget. We have produced a 7.5-year (July 1987-December 1994) dataset of daily, individual monthly-mean and climatological (1988-94) monthly-mean surface turbulent <span class="hlt">fluxes</span> over the global oceans from measurements of the Special Sensor Microwave/Imager (SSM/I) on board the US Defense Meteorological Satellite Program F8, F10, and F11 satellites. It has a spatial resolution of 2.0x2.5 latitude-longitude. Daily turbulent <span class="hlt">fluxes</span> are derived from daily data of SSM/I surface winds and specific humidity, National Centers for Environmental Prediction (NCEP) <span class="hlt">sea</span> surface temperatures, and European Centre for Medium-Range Weather Forecasts (ECMWF) <span class="hlt">air-sea</span> temperature differences, using a stability-dependent bulk scheme. The retrieved instantaneous surface <span class="hlt">air</span> humidity (with a 25-km resolution) IS found to be generally accurate as compared to the collocated radiosonde observations over global oceans. The surface wind speed and specific humidity (latent heat <span class="hlt">flux</span>) derived from the F10 SSM/I are found to be -encrally smaller (larger) than those retrieved from the F11 SSM/I. The F11 SSM/I appears to have slightly better retrieval accuracy for surface wind speed and humidity as compared to the F10 SSM/I. This difference may be due to the orbital drift of the F10 satellite. The daily wind stresses and latent heat <span class="hlt">fluxes</span> retrieved from F10 and F11 SSM/Is show useful accuracy as verified against the research quality in si -neasurerrients (IMET buoy, RV Moana Wave, and RV Wecoma) in the western Pacific warm pool during the TOGA COARE Intensive observing period (November 1992-February 1993). The 1988-94 seasonal-mean turbulent <span class="hlt">fluxes</span> and input variables derived from FS and F11 SSM/Is show reasonable</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ACP....1710837S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ACP....1710837S"><span>Oxygenated volatile organic carbon in the western Pacific convective center: ocean cycling, <span class="hlt">air-sea</span> gas exchange and atmospheric transport</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schlundt, Cathleen; Tegtmeier, Susann; Lennartz, Sinikka T.; Bracher, Astrid; Cheah, Wee; Krüger, Kirstin; Quack, Birgit; Marandino, Christa A.</p> <p>2017-09-01</p> <p>A suite of oxygenated volatile organic compounds (OVOCs - acetaldehyde, acetone, propanal, butanal and butanone) were measured concurrently in the surface water and atmosphere of the South China <span class="hlt">Sea</span> and Sulu <span class="hlt">Sea</span> in November 2011. A strong correlation was observed between all OVOC concentrations in the surface seawater along the entire cruise track, except for acetaldehyde, suggesting similar sources and sinks in the surface ocean. Additionally, several phytoplankton groups, such as haptophytes or pelagophytes, were also correlated to all OVOCs, indicating that phytoplankton may be an important source of marine OVOCs in the South China and Sulu <span class="hlt">seas</span>. Humic- and protein-like fluorescent dissolved organic matter (FDOM) components seemed to be additional precursors for butanone and acetaldehyde. The measurement-inferred OVOC <span class="hlt">fluxes</span> generally showed an uptake of atmospheric OVOCs by the ocean for all gases, except for butanal. A few important exceptions were found along the Borneo coast, where OVOC <span class="hlt">fluxes</span> from the ocean to the atmosphere were inferred. The atmospheric OVOC mixing ratios over the northern coast of Borneo were relatively high compared with literature values, suggesting that this coastal region is a local hotspot for atmospheric OVOCs. The calculated amount of OVOCs entrained into the ocean seemed to be an important source of OVOCs to the surface ocean. When the <span class="hlt">fluxes</span> were out of the ocean, marine OVOCs were found to be enough to control the locally measured OVOC distribution in the atmosphere. Based on our model calculations, at least 0.4 ppb of marine-derived acetone and butanone can reach the upper troposphere, where they may have an important influence on hydrogen oxide radical formation over the western Pacific Ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ESD.....9...69K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ESD.....9...69K"><span>Contribution of atmospheric circulation to recent off-shore <span class="hlt">sea</span>-level variations in the Baltic <span class="hlt">Sea</span> and 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>Karabil, Sitar; Zorita, Eduardo; Hünicke, Birgit</p> <p>2018-01-01</p> <p> physical mechanisms which may explain the link between the <span class="hlt">sea</span>-level variability and the atmospheric pattern described by the BANOS index. These mechanisms include the inverse barometer effect (IBE), freshwater balance, net energy surface <span class="hlt">flux</span> and wind-induced water transport. We found that the most important mechanism is the IBE in both wintertime and summertime. Assuming a complete equilibration of seasonal <span class="hlt">sea</span> level to the SLP gradients over this region, the IBE can explain up to 88 % of the <span class="hlt">sea</span>-level variability attributed to the BANOS index in wintertime and 34 % in summertime. The net energy <span class="hlt">flux</span> at the surface is found to be an important factor for the variation of <span class="hlt">sea</span> level, explaining 35 % of <span class="hlt">sea</span>-level variance in wintertime and a very small amount in summer. The freshwater <span class="hlt">flux</span> could only explain 27 % of the variability in summertime and a negligible part in winter. In contrast to the NAO, the direct wind forcing associated with the SLP BANOS pattern does not lead to transport of water from the North <span class="hlt">Sea</span> into the Baltic <span class="hlt">Sea</span> in wintertime.</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>CO2 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 CO2 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 CO2 sink with a mean annual <span class="hlt">flux</span> of 36 mg m-2 day-1. The northern part absorbs more carbon (68 mg m-2 day-1) due to an efficient continental shelf pump process, whereas the southern part behaves similar to an open ocean. Nonetheless, the Southern Adriatic <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 CO2 is reduced by approximately 15% due to alterations of the solubility pump and reduced dense water formation. The seasonal cycle of temperature and biological productivity modulates the efficiency of the carbon pump at the surface, whereas the intensity of winter cooling in the northern sub-basin leads to the export of C-rich dense water to the deep layer of the southern sub-basin and, subsequently, to the interior of the Mediterranean <span class="hlt">Sea</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013PrOce.109..104C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013PrOce.109..104C"><span><span class="hlt">Sea</span> surface microlayers: A unified physicochemical and biological perspective of the <span class="hlt">air</span>-ocean interface</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cunliffe, Michael; Engel, Anja; Frka, Sanja; Gašparović, Blaženka; Guitart, Carlos; Murrell, J. Colin; Salter, Matthew; Stolle, Christian; Upstill-Goddard, Robert; Wurl, Oliver</p> <p>2013-02-01</p> <p>The <span class="hlt">sea</span> surface microlayer (SML) covers more than 70% of the Earth's surface and is the boundary layer interface between the ocean and the atmosphere. This important biogeochemical and ecological system is critical to a diverse range of Earth system processes, including the synthesis, transformation and cycling of organic material, and the <span class="hlt">air-sea</span> exchange of gases, particles and aerosols. In this review we discuss the SML paradigm, taking into account physicochemical and biological characteristics that define SML structure and function. These include enrichments in biogenic molecules such as carbohydrates, lipids and proteinaceous material that contribute to organic carbon cycling, distinct microbial assemblages that participate in <span class="hlt">air-sea</span> gas exchange, the generation of climate-active aerosols and the accumulation of anthropogenic pollutants with potentially serious implications for the health of the ocean. Characteristically large physical, chemical and biological gradients thus separate the SML from the underlying water and the available evidence implies that the SML retains its integrity over wide ranging environmental conditions. In support of this we present previously unpublished time series data on bacterioneuston composition and SML surfactant activity immediately following physical SML disruption; these imply timescales of the order of minutes for the reestablishment of the SML following disruption. A progressive approach to understanding the SML and hence its role in global biogeochemistry can only be achieved by considering as an integrated whole, all the key components of this complex environment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.B33B0408B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.B33B0408B"><span>Eddy Covariance Measurements of Methane <span class="hlt">Flux</span> Using an Open-Path Gas Analyzer</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Burba, G.; Anderson, T.; Zona, D.; Schedlbauer, J.; Anderson, D.; Eckles, R.; Hastings, S.; Ikawa, H.; McDermitt, D.; Oberbauer, S.; Oechel, W.; Riensche, B.; Starr, G.; Sturtevant, C.; Xu, L.</p> <p>2008-12-01</p> <p>Methane is an important greenhouse gas with a warming potential of about 23 times that of carbon dioxide over a 100-year cycle (Houghton et al., 2001). Measurements of methane <span class="hlt">fluxes</span> from the terrestrial biosphere have mostly been made using <span class="hlt">flux</span> chambers, which have many advantages, but are discrete in time and space and may disturb surface integrity and <span class="hlt">air</span> pressure. Open-path analyzers offer a number of advantages for measuring methane <span class="hlt">fluxes</span>, including undisturbed in- situ <span class="hlt">flux</span> measurements, spatial integration using the Eddy Covariance approach, zero frequency response errors due to tube attenuation, confident water and thermal density terms from co-located fast measurements of water and sonic temperature, and remote deployment due to lower power demands in the absence of a pump. The prototype open-path methane analyzer is a VCSEL (vertical-cavity surface-emitting laser)-based instrument. It employs an open Herriott cell and measures levels of methane with RMS noise below 6 ppb at 10 Hz sampling in controlled laboratory environment. Field maintenance is minimized by a self-cleaning mechanism to keep the lower mirror free of contamination. Eddy Covariance measurements of methane <span class="hlt">flux</span> using the prototype open-path methane analyzer are presented for the period between 2006 and 2008 in three ecosystems with contrasting weather and moisture conditions: (1) <span class="hlt">Fluxes</span> over a short-hydroperiod sawgrass wetland in the Florida Everglades were measured in a warm and humid environment with temperatures often exceeding 25oC, variable winds, and frequent heavy dew at night; (2) <span class="hlt">Fluxes</span> over coastal wetlands in an Arctic tundra were measured in an environment with frequent sub-zero temperatures, moderate winds, and ocean mist; (3) <span class="hlt">Fluxes</span> over pacific mangroves in Mexico were measured in an environment with moderate <span class="hlt">air</span> temperatures high winds, and <span class="hlt">sea</span> spray. Presented eddy covariance <span class="hlt">flux</span> data were collected from a co-located prototype open-path methane analyzer, LI-7500, and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA483634','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA483634"><span>CV or Not to Be? Alternatives to U.S. <span class="hlt">Sea</span>-Based <span class="hlt">Air</span> Power</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2008-06-01</p> <p>decisionmakers’ ability to respond to crises nearly anywhere in the world. Despite this, a fundamental question arises: What does the future hold for...much concentrated striking power to U.S. decisionmakers’ ability to respond to crises nearly anywhere in the world. Despite this, a fundamental ...certainties, a fundamental question arises: What does the future hold for <span class="hlt">sea</span>-based <span class="hlt">air</span> power? Aircraft carriers are among the military’s costliest assets</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoRL..45.2542P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoRL..45.2542P"><span>Linking Low-Frequency Large-Scale Circulation Patterns to Cold <span class="hlt">Air</span> Outbreak Formation in the Northeastern North Atlantic</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Papritz, L.; Grams, C. M.</p> <p>2018-03-01</p> <p>The regional variability of wintertime marine cold <span class="hlt">air</span> outbreaks (CAOs) in the northeastern North Atlantic is studied focusing on the role of weather regimes in modulating the large-scale circulation. Each regime is characterized by a typical CAO frequency anomaly pattern and a corresponding imprint in <span class="hlt">air-sea</span> heat <span class="hlt">fluxes</span>. Cyclonically dominated regimes, Greenland blocking and the Atlantic ridge regime are found to provide favorable conditions for CAO formation in at least one major <span class="hlt">sea</span> of the study region; CAO occurrence is suppressed, however, by blocked regimes whose associated anticyclones are centered over northern Europe (European / Scandinavian blocking). Kinematic trajectories reveal that strength and location of the storm tracks are closely linked to the pathways of CAO <span class="hlt">air</span> masses and, thus, CAO occurrence. Finally, CAO frequencies are also linked to the strength of the stratospheric polar vortex, which is understood in terms of associated variations in the frequency of weather regimes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1997DSRI...44.1377L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1997DSRI...44.1377L"><span>Particle <span class="hlt">flux</span> in deep <span class="hlt">seas</span>: regional characteristics and temporal variability</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lampitt, R. S.; Antia, A. N.</p> <p>1997-08-01</p> <p>Particle <span class="hlt">flux</span> data have been collated from the literature representing most areas of the open ocean to determine regional trends in deep water <span class="hlt">flux</span> and its seasonal variability. Organic carbon <span class="hlt">flux</span> data normalised to a depth of 2000 m exhibits a range of an order of magnitude in areas outside the polar domains (0.38 to 4.2 g/m2/y). In polar regions the range is wider (0.01-5.9 g/m2/y). Latitudinal trends are not apparent for most components of the <span class="hlt">flux</span> although calcite <span class="hlt">flux</span> exhibits a poleward decrease. Limited data from polar regions show <span class="hlt">fluxes</span> of opaline silica not significantly higher than elsewhere. The variability of <span class="hlt">flux</span> over annual cycles was calculated and expressed as a <span class="hlt">Flux</span> Stability Index (FSI) and the relationship between this and vertical <span class="hlt">flux</span> of material examined. Somewhat surprisingly there is no significant relationship between FSI and <span class="hlt">fluxes</span> of dry mass, organic carbon, inorganic carbon or opaline silica. At each site, net annual primary production was determined using published satellite derived estimates. There is a negative but weak relationship between FSI and the proportion of primary production exported to 2000 m (e2000 ratio). The most variable of the non-polar environments export to 2000 m about twice as much of the primary production as the most stable ones. Polar environments have very low e2000 ratios with no apparent relationship to FSI. At primary production levels below 200 g C/m2/y there is a positive correlation between production and organic carbon <span class="hlt">flux</span> at 2000 m but above this level, <span class="hlt">flux</span> remains constant at about 3.5g C/m2/y. A curve derived to describe this relationship was applied to estimates of annual primary production in each of 34 of the open ocean biogeochemical provinces proposed by Longhurst et al. (1995). Globally, open ocean <span class="hlt">flux</span> of organic carbon at 2000 m is 0.34 Gt/yr which is 1% of the total net primary production in these regions. This <span class="hlt">flux</span> is nearly equally divided between the Atlantic, Pacific and Southern</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1711590F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1711590F"><span>Chemical Atmosphere-Snow-<span class="hlt">Sea</span> Ice Interactions: defining future research in the field, lab and modeling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Frey, Markus</p> <p>2015-04-01</p> <p>The <span class="hlt">air-snow-sea</span> ice system plays an important role in the global cycling of nitrogen, halogens, trace metals or carbon, including greenhouse gases (e.g. CO2 <span class="hlt">air-sea</span> <span class="hlt">flux</span>), and therefore influences also climate. Its impact on atmospheric composition is illustrated for example by dramatic ozone and mercury depletion events which occur within or close to the <span class="hlt">sea</span> ice zone (SIZ) mostly during polar spring and are catalysed by halogens released from SIZ ice, snow or aerosol. Recent field campaigns in the high Arctic (e.g. BROMEX, OASIS) and Antarctic (Weddell <span class="hlt">sea</span> cruises) highlight the importance of snow on <span class="hlt">sea</span> ice as a chemical reservoir and reactor, even during polar night. However, many processes, participating chemical species and their interactions are still poorly understood and/or lack any representation in current models. Furthermore, recent lab studies provide a lot of detail on the chemical environment and processes but need to be integrated much better to improve our understanding of a rapidly changing natural environment. During a 3-day workshop held in Cambridge/UK in October 2013 more than 60 scientists from 15 countries who work on the physics, chemistry or biology of the atmosphere-snow-<span class="hlt">sea</span> ice system discussed research status and challenges, which need to be addressed in the near future. In this presentation I will give a summary of the main research questions identified during this workshop as well as ways forward to answer them through a community-based interdisciplinary approach.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C13C0833H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C13C0833H"><span>A New Fast, Reliable Technique for the Sampling of Dissolved Inorganic Carbon in <span class="hlt">Sea</span> Ice</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hu, Y.; Wang, F.; Rysgaard, S.; Barber, D. G.</p> <p>2015-12-01</p> <p>For a long time, <span class="hlt">sea</span> ice was considered to act as a lid over seawater preventing CO2 exchange between the atmosphere and ocean. Recent observations suggest that <span class="hlt">sea</span> ice can be an active source or a sink for CO2, although its magnitude is not very clear. The direct measurements on CO2 <span class="hlt">flux</span> based on the chamber method and eddy covariance often do not agree with each other. It is therefore important to measure the dissolved inorganic carbon (DIC) stock in <span class="hlt">sea</span> ice precisely in order to better understand the CO2 <span class="hlt">flux</span> through <span class="hlt">sea</span> ice. The challenges in <span class="hlt">sea</span> ice DIC sampling is how to melt the ice core without being exposed to the <span class="hlt">air</span> gaining or losing CO2. A common practice is to seal the ice core in a self-prepared gas-tight plastic bag and suck the <span class="hlt">air</span> out of the bag gently using a syringe (together with a needle) through a valve mounted on one side of the bag. However, this method is time consuming (takes up to several minutes to suck the <span class="hlt">air</span> out) and very often there is large headspace found in the bag after the ice melts due to the imperfect bag-preparation, which might affect the DIC concentration in melt ice-water. We developed a new technique by using a commercially available plastic bag with a vacuum sealer to seal the ice core. In comparison to syringe-based method, this technique is fast and easy to operate; it takes less than 10 seconds to vacuum and seal the bag all in one button with no headspace left in the bag. Experimental tests with replicate ice cores sealed by those two methods showed that there is no difference in the DIC concentration measured after these two methods, suggesting that there is no loss of DIC during the course of vacuum sealing. In addition, a time series experiment on DIC in melt ice-water stored in the new bag shows that when the samples were not poisoned, the DIC concentration remains unchanged for at least 3 days in the bag; while poisoned by HgCl2, there is no change in DIC for at least 21 days, indicating that this new bag is</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_24 --> <div id="page_25" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li class="active"><span>25</span></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="481"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002PhDT........76A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002PhDT........76A"><span>Whitecaps, <span class="hlt">sea</span>-salt aerosols, and climate</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Anguelova, Magdalena Dimitrova</p> <p></p> <p>Oceanic whitecaps are the major source of <span class="hlt">sea</span>-salt aerosols. Because these aerosols are dominant in remote marine <span class="hlt">air</span>, they control the radiative properties of the clean background atmosphere by scattering sunlight, changing cloud properties and lifetime, and providing media for chemical reactions. Including <span class="hlt">sea</span>-salt effects in climate models improves predictions, but simulating their generation is first necessary. To make the <span class="hlt">sea</span>-salt generation function currently used in climate models more relevant for aerosol investigations, this study proposes two modifications. First, the conventional relation between whitecap coverage, W, and the 10-meter wind speed, U10, used in typical generation functions is expanded to include additional factors that affect whitecaps and <span class="hlt">sea</span>-salt aerosol formation. Second, the <span class="hlt">sea</span>-salt generation function is extended to smaller sizes; <span class="hlt">sea</span>-salt aerosol with initial radii from 0.4 to 20 mum can now be modeled. To achieve these goals, this thesis develops a new method for estimating whitecap coverage on a global scale using satellite measurements of the brightness temperature of the ocean surface. Whitecap coverage evaluated with this method incorporates the effects of atmospheric stability, <span class="hlt">sea</span>-surface temperature, salinity, wind fetch, wind duration, and the amount of surface-active material. Assimilating satellite-derived values for whitecap coverage in the <span class="hlt">sea</span>-salt generation function incorporates the effects of all environmental factors on <span class="hlt">sea</span>-salt production and predicts realistic <span class="hlt">sea</span>-salt aerosol loadings into the atmosphere. An extensive database of whitecap coverage and <span class="hlt">sea</span>-salt aerosol <span class="hlt">fluxes</span> has been compiled with the new method and is used to investigate their spatial and temporal characteristics. The composite effect of all environmental factors suggests a more uniform latitudinal distribution of whitecaps and <span class="hlt">sea</span>-salt aerosols than that predicted from wind speed alone. The effect of <span class="hlt">sea</span>-surface temperature, TS, is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PhDT.......210M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PhDT.......210M"><span>Development and application of gravity-capillary wave fourier analysis for the study of <span class="hlt">air-sea</span> interaction physics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>MacKenzie Laxague, Nathan Jean</p> <p></p> <p> short ocean surface waves to atmospheric forcing. Another is the exploration of long wave-short wave interactions and their effects on <span class="hlt">air-sea</span> interaction vis-a-vis hydrodynamic modulation. The third and final topic is the characterization of the gravity-capillary regime of the wavenumber-frequency spectrum for the purpose of retrieving near-surface, wind-driven current. All of these fit as part of the desire to more fully describe the mechanism by which momentum is transferred across the <span class="hlt">air-sea</span> interface and to discuss the consequences of this <span class="hlt">flux</span> in the very near-surface layer of the ocean. Gravity-capillary waves are found to have an outsize share of ocean surface roughness, with short wave spectral peaks showing a connection to turbulent atmospheric stress. Short wave modulation is found to occur strongest at high wavenumbers at the lowest wind speeds, with peak modulation occurring immediately downwind of the long wave crest. Furthermore, short scale roughness enhancement is found to occur upwind of the long wave crest for increasing wind forcing magnitude. Observations of the near-surface current profile show that flows retrieved via this method agree well with the results of camera-tracked dye. Application of this method to data collected in the mouth of the Columbia River (MCR) indicates the presence of a near-surface current component that departs considerably from the tidal flow and orients into the wind stress direction. These observations demonstrate that wind speed-based parameterizations may not be sufficient to estimate wind drift and hold implications for the way in which surface material (e.g., debris or spilled oil) transport is estimated when atmospheric stress is of relatively high magnitude or is steered off the mean wind direction.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018OcSci..14..127P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018OcSci..14..127P"><span>Observations of brine plumes below melting 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>Peterson, Algot K.</p> <p>2018-02-01</p> <p>In <span class="hlt">sea</span> ice, interconnected pockets and channels of brine are surrounded by fresh ice. Over time, brine is lost by gravity drainage and flushing. The timing of salt release and its interaction with the underlying water can impact subsequent <span class="hlt">sea</span> ice melt. Turbulence measurements 1 m below melting <span class="hlt">sea</span> ice north of Svalbard reveal anticorrelated heat and salt <span class="hlt">fluxes</span>. From the observations, 131 salty plumes descending from the warm <span class="hlt">sea</span> ice are identified, confirming previous observations from a Svalbard fjord. The plumes are likely triggered by oceanic heat through bottom melt. Calculated over a composite plume, oceanic heat and salt <span class="hlt">fluxes</span> during the plumes account for 6 and 9 % of the total <span class="hlt">fluxes</span>, respectively, while only lasting in total 0.5 % of the time. The observed salt <span class="hlt">flux</span> accumulates to 7.6 kg m-2, indicating nearly full desalination of the ice. Bulk salinity reduction between two nearby ice cores agrees with accumulated salt <span class="hlt">fluxes</span> to within a factor of 2. The increasing fraction of younger, more saline ice in the Arctic suggests an increase in desalination processes with the transition to the <q>new Arctic</q>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1167255','SCIGOV-DOEDE'); return false;" href="https://www.osti.gov/servlets/purl/1167255"><span>CO2 CH4 <span class="hlt">flux</span> <span class="hlt">Air</span> temperature Soil temperature and Soil moisture, Barrow, Alaska 2013 ver. 1</span></a></p> <p><a target="_blank" href="http://www.osti.gov/dataexplorer">DOE Data Explorer</a></p> <p>Margaret Torn</p> <p>2015-01-14</p> <p>This dataset consists of field measurements of CO2 and CH4 <span class="hlt">flux</span>, as well as soil properties made during 2013 in Areas A-D of Intensive Site 1 at the Next-Generation Ecosystem Experiments (NGEE) Arctic site near Barrow, Alaska. Included are i) measurements of CO2 and CH4 <span class="hlt">flux</span> made from June to September (ii) Calculation of corresponding Gross Primary Productivity (GPP) and CH4 exchange (transparent minus opaque) between atmosphere and the ecosystem (ii) Measurements of Los Gatos Research (LGR) chamber <span class="hlt">air</span> temperature made from June to September (ii) measurements of surface layer depth, type of surface layer, soil temperature and soil moisture from June to September.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.V14A..08P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.V14A..08P"><span>Global <span class="hlt">Flux</span> Balance in the Terrestrial H2O Cycle: Reconsidering the Post-Arc Subducted H2O <span class="hlt">Flux</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Parai, R.; Mukhopadhyay, S.</p> <p>2010-12-01</p> <p>Quantitative estimates of H2O <span class="hlt">fluxes</span> between the mantle and the exosphere (i.e., the atmosphere, oceans and crust) are critical to our understanding of the chemistry and dynamics of the solid Earth: the abundance and distribution of water in the mantle has dramatic impacts upon mantle melting, degassing history, structure and style of convection. Water is outgassed from the mantle is association with volcanism at mid-ocean ridges, ocean islands and convergent margins. H2O is removed from the exosphere at subduction zones, and some fraction of the subducted <span class="hlt">flux</span> may be recycled past the arc into the Earth’s deep interior. Estimates of the post-arc subducted H2O <span class="hlt">flux</span> are primarily based on the stability of hydrous phases at subduction zone pressures and temperatures (e.g. Schmidt and Poli, 1998; Rüpke et al., 2004; Hacker, 2008). However, the post-arc H2O <span class="hlt">flux</span> remains poorly quantified, in part due to large uncertainties in the water content of the subducting slab. Here we evaluate estimated post-arc subducted <span class="hlt">fluxes</span> in the context of mantle-exosphere water cycling, using a Monte Carlo simulation of the global H2O cycle. Literature estimates of primary magmatic H2O abundances and magmatic production rates at different tectonic settings are used with estimates of the total subducted H2O <span class="hlt">flux</span> to establish the parameter space under consideration. Random sampling of the allowed parameter space affords insight into which input and output <span class="hlt">fluxes</span> satisfy basic constraints on global <span class="hlt">flux</span> balance, such as a limit on <span class="hlt">sea</span>-level change over time. The net <span class="hlt">flux</span> of H2O between mantle and exosphere is determined by the total mantle output <span class="hlt">flux</span> (via ridges and ocean islands, with a small contribution from mantle-derived arc output) and the input <span class="hlt">flux</span> subducted beyond the arc. Arc and back-arc output is derived mainly from the slab, and therefore cancels out a fraction of the trench intake in an H2O subcycle. Limits on <span class="hlt">sea</span>-level change since the end of the Archaean place</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..12210174S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..12210174S"><span>Is the State of the <span class="hlt">Air-Sea</span> Interface a Factor in Rapid Intensification and Rapid Decline 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>Soloviev, Alexander V.; Lukas, Roger; Donelan, Mark A.; Haus, Brian K.; Ginis, Isaac</p> <p>2017-12-01</p> <p>Tropical storm intensity prediction remains a challenge in tropical meteorology. Some tropical storms undergo dramatic rapid intensification and rapid decline. Hurricane researchers have considered particular ambient environmental conditions including the ocean thermal and salinity structure and internal vortex dynamics (e.g., eyewall replacement cycle, hot towers) as factors creating favorable conditions for rapid intensification. At this point, however, it is not exactly known to what extent the state of the <span class="hlt">sea</span> surface controls tropical cyclone dynamics. Theoretical considerations, laboratory experiments, and numerical simulations suggest that the <span class="hlt">air-sea</span> interface under tropical cyclones is subject to the Kelvin-Helmholtz type instability. Ejection of large quantities of spray particles due to this instability can produce a two-phase environment, which can attenuate gravity-capillary waves and alter the <span class="hlt">air-sea</span> coupling. The unified parameterization of waveform and two-phase drag based on the physics of the <span class="hlt">air-sea</span> interface shows the increase of the aerodynamic drag coefficient Cd with wind speed up to hurricane force (U10≈35 m s-1). Remarkably, there is a local Cd minimum—"an aerodynamic drag well"—at around U10≈60 m s-1. The negative slope of the Cd dependence on wind-speed between approximately 35 and 60 m s-1 favors rapid storm intensification. In contrast, the positive slope of Cd wind-speed dependence above 60 m s-1 is favorable for a rapid storm decline of the most powerful storms. In fact, the storms that intensify to Category 5 usually rapidly weaken afterward.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA601421','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA601421"><span><span class="hlt">Air</span> <span class="hlt">Sea</span> Battle Intelligence, Surveillance, and Reconnaissance Concept of Operations: Getting Back to Fundamentals</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2012-05-08</p> <p>Assessment” phase. This phase will be constant throughout the <span class="hlt">AirSea</span> Battle. A subset of this phase includes battle damage assessment ( BDA ). BDA ...taskings for assessment. There may be situations where operations will cease until the proper BDA is desired. This possibility directly... BDA assessments. It is paramount to task fifth generation fighter with this mission set due to their advanced capabilities. 15 The USAF and USN</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/12469825','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/12469825"><span>Design and performance of a dynaniic gas <span class="hlt">flux</span> chamber.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Reichman, Rivka; Rolston, Dennis E</p> <p>2002-01-01</p> <p>Chambers are commonly used to measure the emission of many trace gases and chemicals from soil. An aerodynamic (flow through) chamber was designed and fabricated to accurately measure the surface <span class="hlt">flux</span> of trace gases. Flow through the chamber was controlled with a small vacuum at the outlet. Due to the design using fans, a partition plate, and aerodynamic ends, <span class="hlt">air</span> is forced to sweep parallel and uniform over the entire soil surface. A fraction of the <span class="hlt">air</span> flowing inside the chamber is sampled in the outlet. The <span class="hlt">air</span> velocity inside the chamber is controlled by fan speed and outlet suction flow rate. The chamber design resulted in a uniform distribution of <span class="hlt">air</span> velocity at the soil surface. Steady state <span class="hlt">flux</span> was attained within 5 min when the outlet <span class="hlt">air</span> suction rate was 20 L/min or higher. For expected <span class="hlt">flux</span> rates, the presence of the chamber did not affect the measured <span class="hlt">fluxes</span> at outlet suction rates of around 20 L/min, except that the chamber caused some cooling of the surface in field experiments. Sensitive measurements of the pressure deficit across the soil layer in conjunction with measured <span class="hlt">fluxes</span> in the source box and chamber outlet show that the outflow rate must be controlled carefully to minimize errors in the <span class="hlt">flux</span> measurements. Both over- and underestimation of the <span class="hlt">fluxes</span> are possible if the outlet flow rate is not controlled carefully. For this design, the chamber accurately measured steady <span class="hlt">flux</span> at outlet <span class="hlt">air</span> suction rates of approximately 20 L/min when the pressure deficit within the chamber with respect to the ambient atmosphere ranged between 0.46 and 0.79 Pa.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.7955K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.7955K"><span>Springtime atmospheric transport controls Arctic summer <span class="hlt">sea</span>-ice extent</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kapsch, Marie; Graversen, Rune; Tjernström, Michael</p> <p>2013-04-01</p> <p>The <span class="hlt">sea</span>-ice extent in the Arctic has been steadily decreasing during the satellite remote sensing era, 1979 to present, with the highest rate of retreat found in September. Contributing factors causing the ice retreat are among others: changes in surface <span class="hlt">air</span> temperature (SAT; Lindsay and Zhang, 2005), ice circulation in response to winds/pressure patterns (Overland et al., 2008) and ocean currents (Comiso et al., 2008), as well as changes in radiative <span class="hlt">fluxes</span> (e.g. due to changes in cloud cover; Francis and Hunter, 2006; Maksimovich and Vihma, 2012) and ocean conditions. However, large interannual variability is superimposed onto the declining trend - the ice extent by the end of the summer varies by several million square kilometer between successive years (Serreze et al., 2007). But what are the processes causing the year-to-year ice variability? A comparison of years with an anomalously large September <span class="hlt">sea</span>-ice extent (HIYs - high ice years) with years showing an anomalously small ice extent (LIYs - low ice years) reveals that the ice variability is most pronounced in the Arctic Ocean north of Siberia (which became almost entirely ice free in September of 2007 and 2012). Significant ice-concentration anomalies of up to 30% are observed for LIYs and HIYs in this area. Focusing on this area we find that the greenhouse effect associated with clouds and water-vapor in spring is crucial for the development of the <span class="hlt">sea</span> ice during the subsequent months. In years where the end-of-summer <span class="hlt">sea</span>-ice extent is well below normal, a significantly enhanced transport of humid <span class="hlt">air</span> is evident during spring into the region where the ice retreat is encountered. The anomalous convergence of humidity increases the cloudiness, resulting in an enhancement of the greenhouse effect. As a result, downward longwave radiation at the surface is larger than usual. In mid May, when the ice anomaly begins to appear and the surface albedo therefore becomes anomalously low, the net shortwave radiation</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMOS51B1667W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMOS51B1667W"><span>Development and evaluation of an empirical diurnal <span class="hlt">sea</span> surface temperature model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Weihs, R. R.; Bourassa, M. A.</p> <p>2013-12-01</p> <p>An innovative method is developed to determine the diurnal heating amplitude of <span class="hlt">sea</span> surface temperatures (SSTs) using observations of high-quality satellite SST measurements and NWP atmospheric meteorological data. The diurnal cycle results from heating that develops at the surface of the ocean from low mechanical or shear produced turbulence and large solar radiation absorption. During these typically calm weather conditions, the absorption of solar radiation causes heating of the upper few meters of the ocean, which become buoyantly stable; this heating causes a temperature differential between the surface and the mixed [or bulk] layer on the order of a few degrees. It has been shown that capturing the diurnal cycle is important for a variety of applications, including surface heat <span class="hlt">flux</span> estimates, which have been shown to be underestimated when neglecting diurnal warming, and satellite and buoy calibrations, which can be complicated because of the heating differential. An empirical algorithm using a pre-dawn <span class="hlt">sea</span> surface temperature, peak solar radiation, and accumulated wind stress is used to estimate the cycle. The empirical algorithm is derived from a multistep process in which SSTs from MTG's SEVIRI SST experimental hourly data set are combined with hourly wind stress fields derived from a bulk <span class="hlt">flux</span> algorithm. Inputs for the <span class="hlt">flux</span> model are taken from NASA's MERRA reanalysis product. NWP inputs are necessary because the inputs need to incorporate diurnal and <span class="hlt">air-sea</span> interactive processes, which are vital to the ocean surface dynamics, with a high enough temporal resolution. The MERRA winds are adjusted with CCMP winds to obtain more realistic spatial and variance characteristics and the other atmospheric inputs (<span class="hlt">air</span> temperature, specific humidity) are further corrected on the basis of in situ comparisons. The SSTs are fitted to a Gaussian curve (using one or two peaks), forming a set of coefficients used to fit the data. The coefficient data are combined with</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016DSRI..113...90S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016DSRI..113...90S"><span>Salp contributions to vertical carbon <span class="hlt">flux</span> in the Sargasso <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stone, Joshua P.; Steinberg, Deborah K.</p> <p>2016-07-01</p> <p>We developed a one-dimensional model to estimate salp contributions to vertical carbon <span class="hlt">flux</span> at the Bermuda Atlantic Time-series Study (BATS) site in the North Atlantic subtropical gyre for a 17-yr period (April 1994 to December 2011). We based the model parameters on published rates of salp physiology and experimentally determined sinking and decomposition rates of salp carcasses. Salp grazing was low during non-bloom conditions, but routinely exceeded 100% of chlorophyll standing stock and primary production during blooms. Fecal pellet production was the largest source of salp carbon <span class="hlt">flux</span> (78% of total), followed by respiration below 200 m (19%), sinking of carcasses (3%), and DOC excretion below 200 m (<0.1%). Thalia democratica, Salpa fusiformis, Salpa aspera, Wheelia cylindrica, and Iasis zonaria were the five highest contributors, accounting for 95% of total salp-mediated carbon <span class="hlt">flux</span>. Seasonally, salp <span class="hlt">flux</span> was higher during spring-summer than fall-winter, due to seasonal changes in species composition and abundance. Salp carbon export to 200 m was on average 2.3 mg C m-2 d-1 across the entire time series. This is equivalent to 11% of the mean 200 m POC <span class="hlt">flux</span> measured by sediment traps in the region. During years with significant salp blooms, however, annually-averaged salp carbon export was the equivalent of up to 60% of trap POC <span class="hlt">flux</span> at 200 m. Salp carbon <span class="hlt">flux</span> attenuated slowly, and at 3200 m the average modeled carbon from salps was 109% of the POC <span class="hlt">flux</span> measured in sediment traps at that depth. Migratory and carcass carbon export pathways should also be considered (alongside fecal pellet <span class="hlt">flux</span>) as facilitating carbon export to sequestration depths in future studies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA00435.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA00435.html"><span>Hurricane Frances as Observed by NASA Spaceborne Atmospheric Infrared Sounder <span class="hlt">AIRS</span> and <span class="hlt">Sea</span>Winds Scatterometer</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2004-08-30</p> <p>This image shows Hurricane Frances in August 2004 as captured by instruments onboard two different NASA satellites: the <span class="hlt">AIRS</span> infrared instrument onboard Aqua, and the <span class="hlt">Sea</span>Winds scatterometer onboard QuikSCAT. Both are JPL-managed instruments. <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 over the ocean. The red vectors in the image show Frances' surface winds as measured by <span class="hlt">Sea</span>Winds on QuikSCAT. The background colors show the temperature of clouds and surface as viewed in the infrared by <span class="hlt">AIRS</span>, with cooler areas pushing to purple and warmer areas are pushing to red. The color scale on the right gives the temperatures in degrees Kelvin. (The top of the scale, 320 degrees Kelvin, corresponds to 117 degrees Fahrenheit, and the bottom, 180 degrees K is -135 degrees F.) The powerful circulation of this storm is evident from the combined data as well as the development of a clearly-defined central "eye." The infrared signal does not penetrate through clouds, so the light blue areas reveal the cold clouds tops associated with strong thunderstorms embedded within the storm. In cloud-free areas the infrared signal comes from Earth's surface, revealing warmer temperatures. http://photojournal.jpl.nasa.gov/catalog/PIA00435</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013BGeo...10.1379C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013BGeo...10.1379C"><span>Technical Note: A simple method for <span class="hlt">air-sea</span> gas 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 CO2 with the atmosphere. Here, we present a simple method for precise determination of <span class="hlt">air-sea</span> gas exchange in mesocosms using N2O as a deliberate tracer. Beside the application for carbon budgeting, transfer 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 CO2 <span class="hlt">fluxes</span> 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('http://adsabs.harvard.edu/abs/1993DSRI...40..653J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1993DSRI...40..653J"><span>Annual cycles of mass <span class="hlt">flux</span> and isotopic composition of pteropod shells settling into the deep Sargasso <span class="hlt">sea</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jasper, John P.; Deuser, Werner G.</p> <p>1993-04-01</p> <p>Mass <span class="hlt">fluxes</span> and stable isotopic compositions ( δ18O and δ13C) pteropod shells collected during a 6-year series of 2-month sediment-trap deployments in the deep (3.2 km) Sargasso <span class="hlt">Sea</span> provide information on annual population changes, habitat depths and life spans of thecosome pteropods (Euthecosomata). The <span class="hlt">flux</span> of pteropod shells responds to the annual cycle of primary production in the upper ocean. <span class="hlt">Flux</span> maxima of the shells (> 1 mm) of eight species occur from late winter through autumn. Seasonal changes in the hydrography of the upper water column are quite accurately recorded in the δ18O variations of six perennial species, which generally confirm the distinction between non-migratory ( Creseis acicula, Creseis virgula conica, and Diacria quadridentata) and diurnally migratory taxa ( Styliola subula, Cuvierina columnella, and Clio pyramidata). Isotopic records of C. acicula and C. virgula conica are consistent with shell formation above 50 m. The records of the migratory species reflect what appear to be average calcification depths of 50-75 m. Average annual δ13C variations reveal the annual cycles of primary production and stratification of near-surface waters. Adult life spans of the species studied appear to be no more than a few months. The results of this study should be useful in paleoceanographic reconstructions based on isotopic measurements of sedimentary pteropod shells.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFMGP51B0762S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFMGP51B0762S"><span>The Brunhes/Matuyama polarity transition recorded as Be-10 <span class="hlt">flux</span> changes in 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>Suganuma, Y.; Yokoyama, Y.; Yamazaki, T.</p> <p>2008-12-01</p> <p><span class="hlt">Fluxes</span> of meteoric cosmogenic radionuclide, Be-10, is thought to be varied due to changes of incoming comic-ray <span class="hlt">flux</span> modulated by geomagnetic field intensity variation. Enhanced production rate of the nuclides during a geomagnetic polarity transition period is expected as a result of the low dipole field strength. We therefore measured Be-10 concentrations in deep-<span class="hlt">sea</span> sediments including the Brunhes/Matuyama geomagnetic polarity transition to reconstruct the detailed structures of the geomagnetic field behavior. A piston core, MD982187 was taken from the West Caroline Basin, the western equatorial Pacific Ocean, during the IMAGES IV campaign. The water depth of the site of MD982187 core is about 4600 m, which is close to the carbonate compensation depth (CCD) in this area at present (Berger et al., 1976). Measurement of Be-10 was conducted using the accelerator mass spectrometry (AMS) of the University of Tokyo, Japan. The result shows significant increase of Be-10 concentration during the polarity transition, indicating that the geomagnetic field intensity was low during this interval. In detail, well-defined double highs of Be-10 concentration are recognized. These highs are thought to correspond to the B/M polarity boundary and the "precursor" event, 15 kyr before the M/B boundary (e.g., Hartl and Tauxe, 1996; Singer et al., 2005), respectively. This feature is very similar to the relative paleointensity record of MR982187 core by Yamazaki and Oda (2005) and other published relative paleointensity records of the Brunhes/Matuyama geomagnetic polarity transition, indicating that Be-10 concentration of the deep-<span class="hlt">sea</span> sedimentary sequence well records the variation of the geomagnetic field intensity. However, ca. 18 cm of clear depth offset between the Be-10 concentration and the relative paleointensity record was observed from the same sedimentary sequence of MR982187 core. This indicates that the relative paleointensity record of MR982187 core is offset by ca. 18 cm</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20100017476','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20100017476"><span>Analysis of Atmosphere-Ocean Surface <span class="hlt">Flux</span> Feedbacks in Recent Satellite and Model Reanalysis Products</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Roberts, J. Brent; Robertson, F. R.; Clayson, C. A.</p> <p>2010-01-01</p> <p>Recent investigations have examined observations in an attempt to determine when and how the ocean forces the atmosphere, and vice versa. These studies focus primarily on relationships between <span class="hlt">sea</span> surface temperature anomalies and the turbulent and radiative surface heat <span class="hlt">fluxes</span>. It has been found that both positive and negative feedbacks, which enhance or reduce <span class="hlt">sea</span> surface temperature anomaly amplitudes, can be generated through changes in the surface boundary layer. Consequent changes in <span class="hlt">sea</span> surface temperature act to change boundary layer characteristics through changes in static stability or turbulent <span class="hlt">fluxes</span>. Previous studies over the global oceans have used coarse-resolution observational and model products such as ICOADS and the NCEP Reanalysis. This study focuses on documenting the atmosphere ocean feedbacks that exist in recently produced higher resolution products, namely the <span class="hlt">SeaFlux</span> v1.0 product and the NASA Modern Era Retrospective-Analysis for Research and Applications (MERRA). It has been noted in recent studies that evidence of oceanic forcing of the atmosphere exists on smaller scales than the usually more dominant atmospheric forcing of the ocean, particularly in higher latitudes. It is expected that use of these higher resolution products will allow for a more comprehensive description of these small-scale ocean-atmosphere feedbacks. The <span class="hlt">SeaFlux</span> intercomparisons have revealed large scatter between various surface <span class="hlt">flux</span> climatologies. This study also investigates the uncertainty in surface <span class="hlt">flux</span> feedbacks based on several of these recent satellite based climatologies</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20040120981','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20040120981"><span>EOS Aqua AMSR-E Arctic <span class="hlt">Sea</span> Ice Validation Program: Arctic2003 Aircraft Campaign Flight Report</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Cavalieri, D. J.; Markus,T.</p> <p>2003-01-01</p> <p>In March 2003 a coordinated Arctic <span class="hlt">sea</span> ice validation field campaign using the NASA Wallops P-3B aircraft was successfully completed. This campaign was part of the program for validating the Earth Observing System (EOS) Aqua Advanced Microwave Scanning Radiometer (AMSR-E) <span class="hlt">sea</span> ice products. The AMSR-E, designed and built by the Japanese National Space Development Agency for NASA, was launched May 4, 2002 on the EOS Aqua spacecraft. The AMSR-E <span class="hlt">sea</span> ice products to be validated include <span class="hlt">sea</span> ice concentration, <span class="hlt">sea</span> ice temperature, and snow depth on <span class="hlt">sea</span> ice. This flight report describes the suite of instruments flown on the P-3, the objectives of each of the seven flights, the Arctic regions overflown, and the coordination among satellite, aircraft, and surface-based measurements. Two of the seven aircraft flights were coordinated with scientists making surface measurements of snow and ice properties including <span class="hlt">sea</span> ice temperature and snow depth on <span class="hlt">sea</span> ice at a study area near Barrow, AK and at a Navy ice camp located in the Beaufort <span class="hlt">Sea</span>. Two additional flights were dedicated to making heat and moisture <span class="hlt">flux</span> measurements over the St. Lawrence Island polynya to support ongoing <span class="hlt">air-sea</span>-ice processes studies of Arctic coastal polynyas. The remaining flights covered portions of the Bering <span class="hlt">Sea</span> ice edge, the Chukchi <span class="hlt">Sea</span>, and Norton Sound.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1994GMS....85..313O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1994GMS....85..313O"><span>Variability of the atmospheric energy <span class="hlt">flux</span> across 70°N computed from the GFDL data set</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Overland, James E.; Turet, Philip</p> <p></p> <p>The primary energy balance for the arctic atmosphere is through northward advection of moist static energy—sensible heat, potential energy, and latent heat—balanced by long wave radiation to space. Energy <span class="hlt">flux</span> from <span class="hlt">sea</span> ice and marginal <span class="hlt">seas</span> contributes perhaps 20-30% of the outgoing radiation north of 70°N in winter and absorbs a nearly equal amount during summer. Thorndike's toy model shows that extreme climate states with no ice growth or melt can occur by changing the latitudinal energy <span class="hlt">flux</span> by ±20-30% out of an annual mean <span class="hlt">flux</span> of 100 W m-2. We extend the previous work on latitudinal energy <span class="hlt">flux</span> by Nakamura and Oort (NO) to a 25-year record and investigate temporal variability. Our annual latitudinal energy <span class="hlt">flux</span> was 103 W m-2 compared to the NO value of 98 W m-2 this difference was from greater <span class="hlt">fluxes</span> during the winter. We found that mean winter (NDJFM) energy <span class="hlt">flux</span> was 121 W m-2 with a standard deviation of 11 W m-2. There were no large outliers in any year. An analysis of variance showed that interannual variability does not contribute towards explaining monthly variability of northward energy transport for the winter, summer or annual periods. Transient eddy <span class="hlt">flux</span> of sensible heat into the arctic basin was the largest component of the total energy <span class="hlt">flux</span> and is concentrated near the longitudes of the Greenland <span class="hlt">Sea</span> (˜10°W) and the Bering and Chukchi <span class="hlt">Seas</span> (180°). There is a minimum in atmospheric heating north of Greenland, a known region of thick ice. While there was little interannual variability of energy <span class="hlt">flux</span> across 70°N, there was considerable month-to-month variability and regional variability in poleward energy <span class="hlt">flux</span>. <span class="hlt">Sea</span> ice may playa role in storage and redistribution of energy in the arctic climate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013BGeo...10.4785L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013BGeo...10.4785L"><span>Modeling plankton ecosystem functioning and nitrogen <span class="hlt">fluxes</span> in the oligotrophic waters of the Beaufort <span class="hlt">Sea</span>, Arctic Ocean: a focus on light-driven processes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Le Fouest, V.; Zakardjian, B.; Xie, H.; Raimbault, P.; Joux, F.; Babin, M.</p> <p>2013-07-01</p> <p>The Arctic Ocean (AO) undergoes profound changes of its physical and biotic environments due to climate change. In some areas of the Beaufort <span class="hlt">Sea</span>, the stronger haline stratification observed in summer alters the plankton ecosystem structure, functioning and productivity, promoting oligotrophy. A one-dimension (1-D) physical-biological coupled model based on the large multiparametric database of the Malina project in the Beaufort <span class="hlt">Sea</span> was used (i) to infer the plankton ecosystem functioning and related nitrogen <span class="hlt">fluxes</span> and (ii) to assess the model sensitivity to key light-driven processes involved in nutrient recycling and phytoplankton growth. The coupled model suggested that ammonium photochemically produced from photosensitive dissolved organic nitrogen (i.e., photoammonification process) was a necessary nitrogen source to achieve the observed levels of microbial biomass and production. Photoammonification directly and indirectly (by stimulating the microbial food web activity) contributed to 70% and 18.5% of the 0-10 m and whole water column, respectively, simulated primary production (respectively 66% and 16% for the bacterial production). The model also suggested that variable carbon to chlorophyll ratios were required to simulate the observed herbivorous versus microbial food web competition and realistic nitrogen <span class="hlt">fluxes</span> in the Beaufort <span class="hlt">Sea</span> oligotrophic waters. In face of accelerating Arctic warming, more attention should be paid in the future to the mechanistic processes involved in food webs and functional group competition, nutrient recycling and primary production in poorly productive waters of the AO, as they are expected to expand rapidly.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.5500K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.5500K"><span>Impact of a nitrogen emission control area (NECA) for ship traffic on the future <span class="hlt">air</span> quality in the Baltic <span class="hlt">Sea</span> region</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Karl, Matthias; Geyer, Beate; Bieser, Johannes; Matthias, Volker; Quante, Markus; Jalkanen, Jukka-Pekka; Johansson, Lasse; Fridell, Erik</p> <p>2017-04-01</p> <p>Deposition of nitrogen compounds originating from shipping activities contribute to eutrophication of the Baltic <span class="hlt">Sea</span> and coastal areas in the Baltic <span class="hlt">Sea</span> region. Emissions of nitrogen oxides (NOx) from shipping on the Baltic <span class="hlt">Sea</span> are comparable to the combined land-based emissions of NOx from Finland and Sweden and have been relatively stable over the last decade. However, expected future growth of maritime transport will result in higher fuel consumption and, if not compensated by increased transport efficiency or other measures, lead to higher total emissions of NOx from shipping. For the Baltic <span class="hlt">Sea</span> a nitrogen emission control area (NECA) will become effective in 2021 - permitting only new built ships that are compliant with stringent Tier III emission limits - with the target of reducing NOx-emissions. In order to study the effect of implementing a Baltic <span class="hlt">Sea</span> NECA-2021 on <span class="hlt">air</span> quality and nitrogen deposition two future scenarios were designed; one with implementation of a NECA for the Baltic <span class="hlt">Sea</span> starting in 2021 and another with no NECA implemented. The same increase of ship traffic was assumed for both future scenarios. Since complete fleet renewal with low NOx-emitting engines is not expected until 20-30 years after the NECA entry date, year 2040 was chosen as future scenario year. The Community Multiscale <span class="hlt">Air</span> Quality (CMAQ) model was used to simulate the current and future <span class="hlt">air</span> quality situation. The nested simulation runs with CMAQ were performed on a horizontal resolution of 4 km × 4 km for the entire Baltic <span class="hlt">Sea</span> region. The meteorological year 2012 was chosen for the simulation of the current and future <span class="hlt">air</span> quality situation since the 2m-temperature and precipitation anomalies of 2012 are closely aligned to the 2004-2014 decadal average over Baltic Proper. High-resolution meteorology obtained from COSMO-CLM was used for the regional simulations. Ship emissions were generated with the Ship Traffic Emission Assessment Model (STEAM) by the Finnish Meteorological</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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