Sample records for air-sea turbulent fluxes

  1. 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.

  2. 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.

  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. 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

  5. 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.

  6. 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

  7. Turbulent Surface Flux Measurements over Snow-Covered Sea Ice

    NASA Astrophysics Data System (ADS)

    Andreas, E. L.; Fairall, C. W.; Grachev, A. A.; Guest, P. S.; Jordan, R. E.; Persson, P. G.

    2006-12-01

    Our group has used eddy correlation to make over 10,000 hours of measurements of the turbulent momentum and heat fluxes over snow-covered sea ice in both the Arctic and the Antarctic. Polar sea 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 Sea, 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 fluxes 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 flux measurements, we have been using the data to develop a bulk flux algorithm and to study fundamental turbulence processes in the atmospheric surface layer. The bulk flux algorithm predicts the turbulent surface fluxes 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.

  8. 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.

  9. Version 2 Goddard Satellite-Based Surface Turbulent Fluxes (GSSTF2)

    NASA Technical Reports Server (NTRS)

    Chou, Shu-Hsien; Nelkin, Eric; Ardizzone, Joe; Atlas, Robert M.; Shie, Chung-Lin; Starr, David O'C. (Technical Monitor)

    2002-01-01

    Information on the turbulent fluxes of momentum, moisture, and heat at the air-sea 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 fluxes over global oceans from the Special Sensor Mcrowave/Imager (SSM/I) radiance measurements. This dataset, version 2 Goddard Satellite-based Surface Turbulent Fluxes (GSSTF2), has a spatial resolution of 1 degree x 1 degree latitude-longitude and a temporal resolution of 1 day. Turbulent fluxes are derived from the SSM/I surface winds and surface air humidity, as well as the 2-m air and sea surface temperatures (SST) of the NCEP/NCAR reanalysis, using a bulk aerodynamic algorithm based on the surface layer similarity theory.

  10. Accounting for observation uncertainties in an evaluation metric of low latitude turbulent air-sea fluxes: application to the comparison of a suite of IPSL model versions

    NASA Astrophysics Data System (ADS)

    Servonnat, Jérôme; Găinuşă-Bogdan, Alina; Braconnot, Pascale

    2017-09-01

    Turbulent momentum and heat (sensible heat and latent heat) fluxes at the air-sea interface are key components of the whole energetic of the Earth's climate. The evaluation of these fluxes 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 fluxes 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 sea 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 fluxes compared to the other versions. The representation of the fluxes 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 fluxes 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 air-sea temperature contrast play an

  11. 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.

  12. 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

  13. A Multiyear Dataset of SSM/I-Derived Global Ocean Surface Turbulent Fluxes

    NASA Technical Reports Server (NTRS)

    Chou, Shu-Hsien; Shie, Chung-Lin; Atlas, Robert M.; Ardizzone, Joe; Nelkin, Eric; Einaudi, Franco (Technical Monitor)

    2001-01-01

    The surface turbulent fluxes 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 air-sea fluxes 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 air-sea fluxes 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 fluxes over the global oceans from the Special Sensor microwave/Imager (SSM/I) data. Daily turbulent fluxes were derived from daily data of SSM/I surface winds and specific humidity, National Centers for Environmental Prediction (NCEP) sea surface temperatures, and European Centre for Medium-Range Weather Forecasts (ECMWF) air-sea temperature differences, using a stability-dependent bulk scheme. The retrieved instantaneous surface air 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 fluxes 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 fluxes will be presented. In addition, the global distributions of 1990-93 annual-means turbulent fluxes 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

  14. 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.

  15. 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.

  16. Observations and Modeling of Turbulent Air-Sea Coupling in Coastal and Strongly Forced Condition

    NASA Astrophysics Data System (ADS)

    Ortiz-Suslow, David G.

    The turbulent fluxes of momentum, mass, and energy across the ocean-atmosphere boundary are fundamental to our understanding of a myriad of geophysical processes, such as wind-wave generation, oceanic circulation, and air-sea gas transfer. In order to better understand these fluxes, empirical relationships were developed to quantify the interfacial exchange rates in terms of easily observed parameters (e.g., wind speed). However, mounting evidence suggests that these empirical formulae are only valid over the relatively narrow parametric space, i.e. open ocean conditions in light to moderate winds. Several near-surface processes have been observed to cause significant variance in the air-sea fluxes not predicted by the conventional functions, such as a heterogeneous surfaces, swell waves, and wave breaking. Further study is needed to fully characterize how these types of processes can modulate the interfacial exchange; in order to achieve this, a broad investigation into air-sea 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, air, and sea 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, sea 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 air-sea fluxes in terms of empirical relationships developed from a relatively narrow set of

  17. 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.

  18. 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.

  19. 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.

  20. Impact of Ocean Surface Waves on Air-Sea Momentum Flux

    NASA Astrophysics Data System (ADS)

    Tamura, H.; Drennan, W. M.; Collins, C. O., III; Graber, H. C.

    2016-02-01

    In this study, we investigated the structure of turbulent air flow over ocean waves. Observations of wind and waves were retrieved by air-sea 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 sea 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.

  1. 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

  2. Measurements of Turbulent Fluxes over Sea Ice Region in the Sea of Okhotsk.

    NASA Astrophysics Data System (ADS)

    Fujisaki, A.; Yamaguchi, H.; Toyota, T.; Futatsudera, A.; Miyanaga, M.

    2007-12-01

    The measurements of turbulent fluxes over sea ice area were done in the southern part of the Sea of Okhotsk, during the cruises of the ice-breaker P/V 'Soya' in 2000-2005. The air-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 sea-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 sea 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 flux during the measurements.

  3. 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.

  4. A 7.5-Year Dataset of SSM/I-Derived Surface Turbulent Fluxes Over Global Oceans

    NASA Technical Reports Server (NTRS)

    Chou, Shu-Hsien; Shie, Chung-Lin; Atlas, Robert M.; Adizzone, Joe; Nelkin, Eric; Starr, David OC. (Technical Monitor)

    2001-01-01

    The global air-sea turbulent fluxes are needed for driving ocean models and validating coupled ocean-atmosphere global models. A method was developed to retrieve surface air humidity from the radiances measured by the Special Sensor Microwave/Imager (SSM/I) Using both SSM/I-retrieved surface wind and air humidity, they computed daily turbulent fluxes over global oceans with a stability-dependent bulk scheme. Based on this method, we have produced Version 1 of Goddard Satellite-Based Surface Turbulent Fluxes (GSSTF) dataset from the SSM/I data and other data. It provides daily- and monthly-mean surface turbulent fluxes 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.

  5. The marine atmospheric boundary layer under strong wind conditions: Organized turbulence structure and flux estimates by airborne measurements

    NASA Astrophysics Data System (ADS)

    Brilouet, Pierre-Etienne; Durand, Pierre; Canut, Guylaine

    2017-02-01

    During winter, cold air outbreaks take place in the northwestern Mediterranean sea. They are characterized by local strong winds (Mistral and Tramontane) which transport cold and dry continental air across a warmer sea. In such conditions, high values of surface sensible and latent heat flux 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 flux profile throughout the entire MABL is essential for the estimation of air-sea exchanges, a correction of eddy covariance turbulent fluxes was developed taking into account the systematic and random errors due to sampling and data processing. This allowed the improvement of surface fluxes estimates, computed from the extrapolation of the stacked levels. A comparison between those surface fluxes and bulk fluxes computed at a moored buoy revealed considerable differences, mainly regarding the latent heat flux under strong wind conditions.

  6. Estimating Turbulent Surface Fluxes from Small Unmanned Aircraft: Evaluation of Current Abilities

    NASA Astrophysics Data System (ADS)

    de Boer, G.; Lawrence, D.; Elston, J.; Cassano, J. J.; Mack, J.; Wildmann, N.; Nigro, M. A.; Ivey, M.; Wolfe, D. E.; Muschinski, A.

    2014-12-01

    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 air-sea interface and Polar sea-ice-air interface are amongst the most challenging in which to measure these fluxes. 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) fluxes 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 fluxes at the air-land or air-sea 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 fluxes. Small Unmanned Aircraft Systems (sUAS) represent a unique platform from which to derive these fluxes. 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 fluxes. 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

  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. Boundary layers at a dynamic interface: air-sea exchange of heat and mass

    NASA Astrophysics Data System (ADS)

    Szeri, Andrew

    2017-11-01

    Exchange of mass or heat across a turbulent liquid-gas interface is a problem of critical interest, especially in air-sea transfer of natural and man-made gases involved in climate change. The goal in this research area is to determine the gas flux from air to sea or vice versa. For sparingly soluble non-reactive gases, this is controlled by liquid phase turbulent velocity fluctuations that act on the thin species concentration boundary layer on the liquid side of the interface. If the fluctuations in surface-normal velocity and gas concentration differences are known, then it is possible to determine the turbulent contribution to the gas flux. However, there is no suitable fundamental direct approach in the general case where neither of these quantities can be easily measured. A new approach is presented to deduce key aspects about the near-surface turbulent motions from remote measurements, which allows one to determine the gas transfer velocity, or gas flux per unit area if overall concentration differences are known. The approach is illustrated with conceptual examples.

  9. 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

  10. 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.

  11. Assessing Air-Sea Interaction in the Evolving NASA GEOS Model

    NASA Technical Reports Server (NTRS)

    Clayson, Carol Anne; Roberts, J. Brent

    2015-01-01

    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 fluxes are critical to the generation and decay of many coupled air-sea phenomena. These mechanisms operate across a number of scales and contain contributions from interactions between the anomalous (i.e. non-mean), often extreme-valued, flux components. Satellite-derived estimates of the surface turbulent and radiative heat fluxes 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 fluxes at the air-sea 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 fluxes 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 fluxes 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 fluxes. 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.

  12. Assessing air-sea interaction in the evolving NASA GEOS model

    NASA Astrophysics Data System (ADS)

    Clayson, C. A.; Roberts, J. B.

    2014-12-01

    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 fluxes are critical to the generation and decay of many coupled air-sea phenomena. These mechanisms operate across a number of scales and contain contributions from interactions between the anomalous (i.e. non-mean), often extreme-valued, flux components. Satellite-derived estimates of the surface turbulent and radiative heat fluxes 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 fluxes at the air-sea 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 fluxes 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 fluxes 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 fluxes. 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.

  13. 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

  14. Measurements and Modeling of Turbulent Fluxes during Persistent Cold Air Pool Events in Salt Lake Valley, Utah

    NASA Astrophysics Data System (ADS)

    Ivey, C. E.; Sun, X.; Holmes, H.

    2017-12-01

    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 fluxes, which serve as sinks or sources of energy, moisture, momentum, and atmospheric pollutants. Quantifying the surface heat and momentum fluxes 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 air pool (CAP) forms when a topographic depression (i.e., valley) fills with cold air, where the air in the stagnant layer is colder than the air 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 air pollution concentrations. Thus, realistic simulations of the land-atmosphere exchange are meaningful to achieve improved predictions of the accumulation, transport, and dispersion of air 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 Air Pool Study (PCAPS). Turbulent fluxes 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 fluxes during one persistent CAP event are evaluated using the PCAPS observations. The results show that sensible and latent

  15. 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.

  16. 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*).

  17. 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.

  18. Turbulent aerosol fluxes over the Arctic Ocean: 2. Wind-driven sources from the sea

    NASA Astrophysics Data System (ADS)

    Nilsson, E. D.; Rannik, Ü.; Swietlicki, E.; Leck, C.; Aalto, P. P.; Zhou, J.; Norman, M.

    2001-12-01

    An eddy-covariance flux system was successfully applied over open sea, leads and ice floes during the Arctic Ocean Expedition in July-August 1996. Wind-driven upward aerosol number fluxes were observed over open sea and leads in the pack ice. These particles must originate from droplets ejected into the air at the bursting of small air bubbles at the water surface. The source flux 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 sea and leads, respectively (where U¯ is the local wind speed at about 10 m height). Over the open sea the wind-driven aerosol source flux 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 sea-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 flux, but their chemical composition is unknown. Whitecaps were probably the bubble source at open sea 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 flux over the open sea was of such a magnitude that it could give a significant contribution to the condensation nuclei (CCN) population. Although the flux 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.

  19. 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

  20. Importance of ocean mesoscale variability for air-sea interactions in the Gulf of Mexico

    NASA Astrophysics Data System (ADS)

    Putrasahan, D. A.; Kamenkovich, I.; Le Hénaff, M.; Kirtman, B. P.

    2017-06-01

    Mesoscale variability of currents in the Gulf of Mexico (GoM) can affect oceanic heat advection and air-sea 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 air-sea 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 sea surface temperature (SST) and surface turbulent heat flux anomalies, while LR has negative correlation. For HR, we decompose lateral advective heat fluxes in the upper ocean into mean (slowly varying) and mesoscale-eddy (fast fluctuations) components. We find that the eddy flux divergence/convergence dominates the lateral advection and correlates well with the SST anomalies and air-sea latent heat exchanges. This result suggests that oceanic mesoscale advection supports warm SST anomalies that in turn feed surface heat flux. We identify anticyclonic warm-core circulation patterns (associated Loop Current and rings) which have an average diameter of 350 km. These warm anomalies are sustained by eddy heat flux convergence at submonthly time scales and have an identifiable imprint on surface turbulent heat flux, atmospheric circulation, and convective precipitation in the northwest portion of an averaged anticyclone.

  1. 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.

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

    NASA Astrophysics Data System (ADS)

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

    2014-05-01

    Air-sea gas exchange is important to the global partitioning of CO2.Exchange fluxes are products of an air-sea gas concentration difference, ΔC, and a gas transfer velocity, kw. The latter is controlled by the rate of turbulent diffusion at the air-sea interface but it cannot be directly measured and has a high uncertainty that is now considered one of the greatest challenges to quantifying net global air-sea CO2 exchange ...(Takahashi et al., 2009). One important control on kw is exerted by sea surface surfactants that arise both naturally from biological processes and through anthropogenic activity. They influence gas exchange in two fundamental ways: as a monolayer physical barrier and through modifying sea surface hydrodynamics and hence turbulent energy transfer. These effects have been demonstrated in the laboratory with artificial surfactants ...(Bock et al., 1999; Goldman et al., 1988) and through purposeful surfactant releases in coastal waters .(.).........().(Brockmann et al., 1982) and in the open ocean (Salter et al., 2011). Suppression of kwin these field experiments was ~5-55%. While changes in both total surfactant concentration and the composition of the natural surfactant pool might be expected to impact kw, the required in-situ studies are lacking. New data collected from the coastal North Sea in 2012-2013 shows significant spatio-temporal variability in the surfactant activity of organic matter within the sea surface microlayer that ranges from 0.07-0.94 mg/L T-X-100 (AC voltammetry). The surfactant activities show a strong winter/summer seasonal bias and general decrease in concentration with increasing distance from the coastline possibly associated with changing terrestrial vs. phytoplankton sources. Gas exchange experiments of this seawater using a novel laboratory tank and gas tracers (CH4 and SF6) demonstrate a 12-45% reduction in kw compared to surfactant-free water. Seasonally there is higher gas exchange suppression in the summer

  3. Air-Sea Interaction in the Gulf of Tehuantepec

    NASA Astrophysics Data System (ADS)

    Khelif, D.; Friehe, C. A.; Melville, W. K.

    2007-05-01

    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 fluxes 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 air-sea fluxes approximately follow previous parameterizations with some evidence of the drag coefficient leveling out at about 20 meters/sec with the latent heat flux 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.

  4. 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.

  5. A 7.5-Year Dataset of SSM/I-Derived Surface Turbulent Fluxes Over Global Oceans

    NASA Technical Reports Server (NTRS)

    Chou, Shu-Hsien; Shie, Chung-Lin; Atlas, Robert M.; Ardizzone, Joe; Nelkin, Eric; Einaudi, Franco (Technical Monitor)

    2001-01-01

    The surface turbulent fluxes 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 fluxes 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 fluxes are derived from daily data of SSM/I surface winds and specific humidity, National Centers for Environmental Prediction (NCEP) sea surface temperatures, and European Centre for Medium-Range Weather Forecasts (ECMWF) air-sea temperature differences, using a stability-dependent bulk scheme. The retrieved instantaneous surface air 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 flux) 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 fluxes 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 fluxes and input variables derived from FS and F11 SSM/Is show reasonable

  6. 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.

  7. Near bed suspended sediment flux by single turbulent events

    NASA Astrophysics Data System (ADS)

    Amirshahi, Seyed Mohammad; Kwoll, Eva; Winter, Christian

    2018-01-01

    The role of small scale single turbulent events in the vertical mixing of near bed suspended sediments was explored in a shallow shelf sea environment. High frequency velocity and suspended sediment concentration (SSC; calibrated from the backscatter intensity) were collected using an Acoustic Doppler Velocimeter (ADV). Using quadrant analysis, the despiked velocity time series was divided into turbulent events and small background fluctuations. Reynolds stress and Turbulent Kinetic Energy (TKE) calculated from all velocity samples, were compared to the same turbulent statistics calculated only from velocity samples classified as turbulent events (Reevents and TKEevents). The comparison showed that Reevents and TKEevents was increased 3 and 1.6 times, respectively, when small background fluctuations were removed and that the correlation with SSC for TKE could be improved through removal of the latter. The correlation between instantaneous vertical turbulent flux (w ‧) and SSC fluctuations (SSC ‧) exhibits a tidal pattern with the maximum correlation at peak ebb and flood currents, when strong turbulent events appear. Individual turbulent events were characterized by type, strength, duration and length. Cumulative vertical turbulent sediment fluxes and average SSC associated with individual turbulent events were calculated. Over the tidal cycle, ejections and sweeps were the most dominant events, transporting 50% and 36% of the cumulative vertical turbulent event sediment flux, respectively. Although the contribution of outward interactions to the vertical turbulent event sediment flux was low (11%), single outward interaction events were capable of inducing similar SSC ‧ as sweep events. The results suggest that on time scales of tens of minutes to hours, TKE may be appropriate to quantify turbulence in sediment transport studies, but that event characteristics, particular the upward turbulent flux need to be accounted for when considering sediment transport

  8. Boundary layers at a dynamic interface: Air-sea exchange of heat and mass

    NASA Astrophysics Data System (ADS)

    Szeri, Andrew J.

    2017-04-01

    Exchange of mass or heat across a turbulent liquid-gas interface is a problem of critical interest, especially in air-sea transfer of natural and anthropogenic gases involved in the study of climate. The goal in this research area is to determine the gas flux from air to sea or vice versa. For sparingly soluble nonreactive gases, this is controlled by liquid phase turbulent velocity fluctuations that act on the thin species concentration boundary layer on the liquid side of the interface. If the fluctuations in surface-normal velocity w' and gas concentration c' are known, then it is possible to determine the turbulent contribution to the gas flux. However, there is no suitable fundamental direct approach in the general case where neither w' nor c' can be easily measured. A new approach is presented to deduce key aspects about the near-surface turbulent motions from measurements that can be taken by an infrared (IR) camera. An equation is derived with inputs being the surface temperature and heat flux, and a solution method developed for the surface-normal strain experienced over time by boundary layers at the interface. Because the thermal and concentration boundary layers experience the same near-surface fluid motions, the solution for the surface-normal strain determines the gas flux or gas transfer velocity. Examples illustrate the approach in the cases of complete surface renewal, partial surface renewal, and insolation. The prospects for use of the approach in flows characterized by sheared interfaces or rapid boundary layer straining are explored.

  9. 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.

  10. A Multilayer Dataset of SSM/I-Derived Global Ocean Surface Turbulent Fluxes

    NASA Technical Reports Server (NTRS)

    Chou, Shu-Hsien; Shie, Chung-Lin; Atlas, Robert M.; Ardizzone, Joe; Nelkin, Eric; Einaud, Franco (Technical Monitor)

    2001-01-01

    A dataset including daily- and monthly-mean turbulent fluxes (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 air humidity is found to be generally accurate as compared to the collocated radiosonde observations over global oceans. The retrieved wind stress and latent heat flux 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 flux show reasonable patterns related to seasonal variations of the atmospheric general circulation. The patterns of 1990-93 annual-mean turbulent fluxes and input variables are generally in good agreement with one of the best global analyzed flux 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 flux and sea-air 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 air 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 flux is generally within +/-5

  11. On the impact of forced roll convection on vertical turbulent transport in cold air outbreaks

    NASA Astrophysics Data System (ADS)

    Gryschka, Micha; Fricke, Jens; Raasch, Siegfried

    2014-11-01

    We investigated the impact of roll convection on the convective boundary layer and vertical transports in different cold air outbreak (CAO) scenarios using large eddy simulations (LES). The organization of convection into rolls was triggered by upstream heterogeneities in the surface temperature, representing ice and water. By changing the sea ice distribution in our LES, we were able to simulate a roll and a nonroll case for each scenario. Furthermore, the roll wavelength was varied by changing the scale of the heterogeneity. The characteristics of the simulated rolls and cloud streets, such as aspect ratios, orientation of the roll axes, and downstream extensions of single rolls agreed closely with observations in CAO situations. The vertical turbulent fluxes, calculated for each simulation, were decomposed into contributions from rolls and from unorganized turbulence. Even though our results confirmed that rolls triggered by upstream heterogeneities can substantially contribute to vertical turbulent fluxes, the total fluxes were not affected by the rolls.

  12. 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.

  13. 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.

  14. Ocean Surface Observations of the Diurnal Cycle of Turbulence with ASIP

    NASA Astrophysics Data System (ADS)

    Ward, Brian; Sutherland, Graig; Reverdin, Gilles; Marie, Louis; Christensen, Kai; Brostrom, Goran; Harcourt, Ramsey; Breivik, Oyvind

    2015-04-01

    The STRASSE field experiment was conducted in August/September 2012 as part of the Salinity Processes in the Upper Ocean Regional Study (SPURS) campaign. The average conditions during STRASSE were low wind and high insolation, which are typical for the generation of near-surface diurnal warming. We deployed the Air-Sea Interaction Profiler (ASIP), an autonomous upwardly-rising microstructure instrument capable of resolving small-scale processes close to the air-sea interface. ASIP provides direct estimates of the dissipation rate of turbulent kinetic energy, temperature, salinity, and PAR at timescales suitable for the study of diurnal processes. In combination with the ASIP data, we had shipboard meteorological data for calculation of atmospheric forcing, and a surface mounted Lagrangian ADCP for determination of the near-surface velocity. There was a strong diurnal cycle of temperature and dissipation (from ASIP) and shear (from an ADCP). As air-sea fluxes are driven by turbulence immediately at the air-sea interface, the presence of this enhanced shear-induced turbulence will enhance fluxes.

  15. 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.

  16. Aqueous turbulence structure immediately adjacent to the air - water interface and interfacial gas exchange

    NASA Astrophysics Data System (ADS)

    Wang, Binbin

    Air-sea interaction and the interfacial exchange of gas across the air-water interface are of great importance in coupled atmospheric-oceanic environmental systems. Aqueous turbulence structure immediately adjacent to the air-water interface is the combined result of wind, surface waves, currents and other environmental forces and plays a key role in energy budgets, gas fluxes and hence the global climate system. However, the quantification of turbulence structure sufficiently close to the air-water interface is extremely difficult. The physical relationship between interfacial gas exchange and near surface turbulence remains insufficiently investigated. This dissertation aims to measure turbulence in situ in a complex environmental forcing system on Lake Michigan and to reveal the relationship between turbulent statistics and the CO2 flux across the air-water interface. The major objective of this dissertation is to investigate the physical control of the interfacial gas exchange and to provide a universal parameterization of gas transfer velocity from environmental factors, as well as to propose a mechanistic model for the global CO2 flux that can be applied in three dimensional climate-ocean models. Firstly, this dissertation presents an advanced measurement instrument, an in situ free floating Particle Image Velocimetry (FPIV) system, designed and developed to investigate the small scale turbulence structure immediately below the air-water interface. Description of hardware components, design of the system, measurement theory, data analysis procedure and estimation of measurement error were provided. Secondly, with the FPIV system, statistics of small scale turbulence immediately below the air-water interface were investigated under a variety of environmental conditions. One dimensional wave-number spectrum and structure function sufficiently close to the water surface were examined. The vertical profiles of turbulent dissipation rate were intensively studied

  17. CAT (Clear Air Turbulence) Forecasting Using Transilient Turbulence Theory

    DTIC Science & Technology

    1988-02-20

    FILE COP.y AIOL-M-80106 CAT Fwmsft Using Transilient 00 % to, N - 0 William H. Raymond ) Rhad B. Stull O University of Wisconsin V CImSS/epannint...PROGRAM PROJECT TASK WORK UNIT ELEMENT NO. NO. NO ACCESSIO NO. 62101F 6670 10 DB 11. TITLE (Include Security Classification) CAT Forecasting Using...necessary and identify by block number) FIELD GROUP SUB-GROUP Clear Air Turbulence ( CAT ) Boundary Layer Turbulence parameterization Surface Fluxes 19

  18. Crossing turbulent boundaries: interfacial flux in environmental flows.

    PubMed

    Grant, Stanley B; Marusic, Ivan

    2011-09-01

    Advances in the visualization and prediction of turbulence are shedding new light on mass transfer in the turbulent boundary layer. These discoveries have important implications for many topics in environmental science and engineering, from the transport of earth-warming CO2 across the sea-air interface, to nutrient processing and sediment erosion in rivers, lakes, and the ocean, to pollutant removal in water and wastewater treatment systems. In this article we outline current understanding of turbulent boundary layer flows, with particular focus on coherent turbulence and its impact on mass transport across the sediment-water interface in marine and freshwater systems.

  19. 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.

  20. 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.

  1. Effects of cold front passage on turbulent fluxes over a large inland water

    NASA Astrophysics Data System (ADS)

    Zhang, Q.; Liu, H.

    2011-12-01

    Turbulent fluxes of sensible and latent heat over a large inland water in southern USA were measured using the eddy covariance method through the year of 2008. In addition, net radiation, air temperatures and relative humidity, and water temperature in different depths were also measured. The specific objective of this study is to examine effects of a cold front passage on the surface energy fluxes. For the typical cold front event selected from April 11 to 14, air temperature decreased by 16°C, while surface temperature only dropped 6°C. Atmospheric vapor pressure decreased by 1.6 kPa, while that in the water-air interface dropped 0.7 kPa. The behavior difference in the water-air interface was caused by the passage of cold, dry air masses immediately behind the cold front. During the cold front event, sensible heat and latent heat flux increased by 171 W m-2 and 284 W m-2, respectively. Linear aggression analysis showed that the sensible heat flux was proportional to the product of wind speed and the temperature gradient of water-air interface, with a correlation coefficient of 0.95. Latent heat flux was proportional to the product of wind speed and vapor pressure difference between the water surface and overlaying atmosphere, with a correlation coefficient of 0.81. Also, the correlations between both fluxes and the wind speed were weak. This result indicated that the strong wind associated with the cold front event contributed to the turbulent mixing, which indirectly enhanced surface energy exchange between the water surface and the atmosphere. The relationship between the water heat storage energy and turbulent fluxes was also examined.

  2. 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.

  3. Impact of air-sea drag coefficient for latent heat flux on large scale climate in coupled and atmosphere stand-alone simulations

    NASA Astrophysics Data System (ADS)

    Torres, Olivier; Braconnot, Pascale; Marti, Olivier; Gential, Luc

    2018-05-01

    The turbulent fluxes 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 fluxes 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 air-sea 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 fluxes 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 flux 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 fluxes 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 flux

  4. Southern Ocean air-sea heat flux, SST spatial anomalies, and implications for multi-decadal upper ocean heat content trends.

    NASA Astrophysics Data System (ADS)

    Tamsitt, V. M.; Talley, L. D.; Mazloff, M. R.

    2014-12-01

    The Southern Ocean displays a zonal dipole (wavenumber one) pattern in sea 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). Air-sea heat flux 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 fluxes from the Southern Ocean State Estimate (SOSE), a ⅙° eddy permitting model constrained to all available in situ data. This heat flux pattern is dominated by turbulent heat loss from the ocean (latent and sensible), proportional to perturbations in the difference between SST and surface air 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.

  5. Turbulent mass flux closure modeling for variable density turbulence in the wake of an air-entraining transom stern

    NASA Astrophysics Data System (ADS)

    Hendrickson, Kelli; Yue, Dick

    2016-11-01

    This work presents the development and a priori testing of closure models for the incompressible highly-variable density turbulent (IHVDT) flow in the near wake region of a transom stern. This complex, three-dimensional flow includes three regions with distinctly different flow behavior: (i) the convergent corner waves that originate from the body and collide on the ship center plane; (ii) the "rooster tail" that forms from the collision; and (iii) the diverging wave train. The characteristics of these regions involve violent free-surface flows and breaking waves with significant turbulent mass flux (TMF) at Atwood number At = (ρ2 -ρ1) / (ρ2 +ρ1) 1 for which there is little guidance in turbulence closure modeling for the momentum and scalar transport along the wake. Utilizing datasets from high-resolution simulations of the near wake of a canonical three-dimensional transom stern using conservative Volume-of-Fluid (cVOF), implicit Large Eddy Simulation (iLES), and Boundary Data Immersion Method (BDIM), we develop explicit algebraic turbulent mass flux closure models that incorporate the most relevant physical processes. Performance of these models in predicting the turbulent mass flux in all three regions of the wake will be presented. Office of Naval Research.

  6. 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

  7. Teleconnections, Midlatitude Cyclones and Aegean Sea Turbulent Heat Flux Variability on Daily Through Decadal Time Scales

    NASA Technical Reports Server (NTRS)

    Romanski, Joy; Romanou, Anastasia; Bauer, Michael; Tselioudis, George

    2013-01-01

    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 fluxes in the eastern Mediterranean basin and Aegean Sea. The relative frequency of occurrence of each state determines the heat loss from the Aegean Sea 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 Sea cooling for winters prior to 1985, the earliest year for which we have daily heat flux observations. We show that cyclone states conducive to Aegean Sea convection occurred in 1991/1992 and 1992/1993, the winters during which deep water formation was observed in the Aegean Sea, 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 Sea surface waters.

  8. The Response of the Ocean Thermal Skin Layer to Air-Sea Surface Heat Fluxes

    NASA Astrophysics Data System (ADS)

    Wong, Elizabeth Wing-See

    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 air-sea boundary. The hypothesis is that since heat lost through the air-sea 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 fluxes and emitted radiation on the incident radiative fluxes 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 flux which implies the heat sink for upward flowing heat at the air-sea interface is more

  9. Modelling deep-water formation in the north-west Mediterranean Sea with a new air-sea coupled model: sensitivity to turbulent flux parameterizations

    NASA Astrophysics Data System (ADS)

    Seyfried, Léo; Marsaleix, Patrick; Richard, Evelyne; Estournel, Claude

    2017-12-01

    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 fluxes in strong wind conditions, several simulations were carried out based on different parameterizations of the flux bulk formulas. The results point out that the choice of turbulent flux 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.

  10. Air/sea DMS gas transfer in the North Atlantic: evidence for limited interfacial gas exchange at high wind speed

    NASA Astrophysics Data System (ADS)

    Bell, T. G.; De Bruyn, W.; Miller, S. D.; Ward, B.; Christensen, K.; Saltzman, E. S.

    2013-05-01

    Shipboard measurements of eddy covariance DMS air/sea fluxes and seawater concentration were carried out in the North Atlantic bloom region in June/July 2011. Gas transfer coefficients (k660) show a linear dependence on mean horizontal wind speed at wind speeds up to 11 m s-1. At higher wind speeds the relationship between k660 and wind speed weakens. At high winds, measured DMS fluxes were lower than predicted based on the linear relationship between wind speed and interfacial stress extrapolated from low to intermediate wind speeds. In contrast, the transfer coefficient for sensible heat did not exhibit this effect. The apparent suppression of air/sea gas flux at higher wind speeds appears to be related to sea 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 air/sea exchange of DMS is controlled by interfacial rather than bubble-mediated gas transfer under high wind speed conditions.

  11. A new method for estimating the turbulent heat flux at the bottom of the daily mixed layer

    NASA Technical Reports Server (NTRS)

    Imawaki, Shiro; Niiler, Pearn P.; Gautier, Catherine H.; Knox, Robert A.; Halpern, David

    1988-01-01

    Temperature data in the mixed layer and net solar irradiance data at the sea surface are used to estimate the vertical turbulent heat flux at the bottom of the daily mixed layer. The method is applied to data obtained in the eastern tropical Pacific, where the daily cycle in the temperature field is confined to the upper 10-25 m. Equatorial turbulence measurements indicate that the turbulent heat flux is much greater during nighttime than daytime.

  12. Air-sea interaction regimes in the sub-Antarctic Southern Ocean and Antarctic marginal ice zone revealed by icebreaker measurements

    NASA Astrophysics Data System (ADS)

    Yu, Lisan; Jin, Xiangze; Schulz, Eric W.; Josey, Simon A.

    2017-08-01

    This study analyzed shipboard air-sea 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 air temperature, leading to consequential effects on air-sea variables and fluxes. Major effort was made to estimate the air-sea fluxes in the MIZ using the bulk flux algorithms that are tuned specifically for the sea-ice effects, while computing the fluxes over the sub-Antarctic section using the COARE3.0 algorithm. The study evidenced strong sea-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 fluxes 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.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/2017EGUGA..1916884B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1916884B"><span>Vertical nutrient <span class="hlt">fluxes</span>, <span class="hlt">turbulence</span> and the distribution of chlorophyll a in the north-eastern 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>Bendtsen, Jørgen; Richardson, Katherine</p> <p>2017-04-01</p> <p>During summer the northern North <span class="hlt">Sea</span> is characterized by nutrient rich bottom water masses and nutrient poor surface layers. This explains the distribution of chlorophyll a in the water column where a subsurface maximum, referred to as the deep chlorophyll maximum (DCM), often is present during the growth season. Vertical transport of nutrients between bottom water masses and the well lit surface layer stimulates phytoplankton growth and this generally explains the location of the DCM. However, a more specific understanding of the interplay between vertical transports, nutrient <span class="hlt">fluxes</span> and phytoplankton abundance is required for identifying the nature of the vertical transport processes, e.g the role of advection versus vertical <span class="hlt">turbulent</span> diffusion or the role of localized mixing associated with mesoscale eddies. We present results from the VERMIX study in the north-eastern North <span class="hlt">Sea</span> where nutrients, chlorophyll a and <span class="hlt">turbulence</span> profiles were measured along five north-south directed transects in July 2016. A high-resolution sampling program, with horizontal distances of 1-10 km between CTD-stations, resolved the horizontal gradients of chlorophyll a across the steep bottom slope from the relatively shallow central North <span class="hlt">Sea</span> ( 50-80 m) towards the deep Norwegian Trench (>700 m). Low oxygen concentrations in the bottom water masses above the slope indicated enhanced biological production where vertical mixing would stimulate phytoplankton growth around the DCM. Measurements of variable fluorescence (Fv/Fm) showed elevated values in the DCM which demonstrates a higher potential for electron transport in the Photosystem II in the phytoplankton cells, i.e. an indication of nutrient-rich conditions favorable for phytoplankton production. Profiles of the vertical shear and microstructure of temperature and salinity were measured by a VMP-250 <span class="hlt">turbulence</span> profiler and the vertical diffusion of nutrients was calculated from the estimated vertical <span class="hlt">turbulent</span> diffusivity and the</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 <span class="hlt">turbulent</span> 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 <span class="hlt">turbulence</span> 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/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 <span class="hlt">turbulence</span>, 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/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 <span class="hlt">turbulent</span> 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 <span class="hlt">turbulent</span> 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('http://adsabs.harvard.edu/abs/2017AGUFMNG14A..09S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMNG14A..09S"><span>Effects of Langmuir <span class="hlt">Turbulence</span> on Reactive Tracers in the Upper Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Smith, K.; Hamlington, P.; Niemeyer, K.; Fox-Kemper, B.; Lovenduski, N. S.</p> <p>2017-12-01</p> <p>Reactive tracers such as carbonate chemical species play important roles in the oceanic carbon cycle, allowing the ocean to hold 60 times more carbon than the atmosphere. However, uncertainties in regional ocean sinks for anthropogenic CO2 are still relatively high. Many carbonate species are non-conserved, <span class="hlt">flux</span> across the <span class="hlt">air-sea</span> interface, and react on time scales similar to those of ocean <span class="hlt">turbulent</span> processes, such as small-scale wave-driven Langmuir <span class="hlt">turbulence</span>. All of this complexity gives rise to heterogeneous tracer distributions that are not fully understood and can greatly affect the rate at which CO2 <span class="hlt">fluxes</span> across the <span class="hlt">air-sea</span> interface. In order to more accurately model the biogeochemistry of the ocean in Earth system models (ESMs), a better understanding of the fundamental interactions between these reactive tracers and relevant <span class="hlt">turbulent</span> processes is required. Research on reacting flows in other contexts has shown that the most significant tracer-flow couplings occur when coherent structures in the flow have timescales that rival reaction time scales. Langmuir <span class="hlt">turbulence</span>, a 3D, small-scale, wave-driven process, has length and time scales on the order of O(1-100m) and O(1-10min), respectively. Once CO2 transfers across the <span class="hlt">air-sea</span> interface, it reacts with seawater in a series of reactions whose rate limiting steps have time scales of 10-25s. This similarity in scales warrants further examination into interactions between these small-scale physical and chemical processes. In this presentation, large eddy simulations are used to examine the evolution of reactive tracers in the presence of realistic upper ocean wave- and shear-driven <span class="hlt">turbulence</span>. The reactive tracers examined are those specifically involved in non-biological carbonate chemistry. The strength of Langmuir <span class="hlt">turbulence</span> is varied in order to determine a relationship between the degree of enhancement (or reduction) of carbon that is <span class="hlt">fluxed</span> across the <span class="hlt">air-sea</span> interface due to the presence of Langmuir</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS23B2025O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS23B2025O"><span>Field Observations of Coastal <span class="hlt">Air-Sea</span> Interaction</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ortiz-Suslow, D. G.; Haus, B. K.; Williams, N. J.; Graber, H. C.</p> <p>2016-12-01</p> <p>In the nearshore zone wind, waves, and currents generated from different forcing mechanisms converge in shallow water. This can profoundly affect the physical nature of the ocean surface, which can significantly modulate the exchange of momentum, heat, and mass across the <span class="hlt">air-sea</span> interface. For decades, the focus of <span class="hlt">air-sea</span> interaction research has been on the open ocean while the shallow water regime has been relatively under-explored. This bears implications for efforts to understand and model various coastal processes, such as mixing, surface transport, and <span class="hlt">air-sea</span> gas <span class="hlt">flux</span>. The results from a recent study conducted at the New River Inlet in North Carolina showed that directly measured <span class="hlt">air-sea</span> <span class="hlt">flux</span> parameters, such as the atmospheric drag coefficient, are strong functions of space as well as the ambient conditions (i.e. wind speed and direction). The drag is typically used to parameterize the wind stress magnitude. It is generally assumed that the wind direction is the direction of the atmospheric forcing (i.e. wind stress), however significant wind stress steering off of the azimuthal wind direction was observed and was found to be related to the horizontal surface current shear. The authors have just returned from a field campaign carried out within Monterey Bay in California. Surface observations made from two research vessels were complimented by an array of beach and inland <span class="hlt">flux</span> stations, high-resolution wind forecasts, and satellite image acquisitions. This is a rich data set and several case studies will be analyzed to highlight the importance of various processes for understanding the <span class="hlt">air-sea</span> <span class="hlt">fluxes</span>. Preliminary findings show that interactions between the local wind-<span class="hlt">sea</span> and the shoaling, incident swell can have a profound effect on the wind stress magnitude. The Monterey Bay coastline contains a variety of topographical features and the importance of land-<span class="hlt">air-sea</span> interactions will also be investigated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMOS51B1988M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMOS51B1988M"><span>Effect of Sampling Depth on <span class="hlt">Air-Sea</span> CO2 <span class="hlt">Flux</span> Estimates in River-Stratified Arctic Coastal Waters</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Miller, L. A.; Papakyriakou, T. N.</p> <p>2015-12-01</p> <p>In summer-time Arctic coastal waters that are strongly influenced by river run-off, extreme stratification severely limits wind mixing, making it difficult to effectively sample the surface 'mixed layer', which can be as shallow as 1 m, from a ship. During two expeditions in southwestern Hudson Bay, off the Nelson, Hayes, and Churchill River estuaries, we confirmed that sampling depth has a strong impact on estimates of 'surface' pCO2 and calculated <span class="hlt">air-sea</span> CO2 <span class="hlt">fluxes</span>. 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 <span class="hlt">air-sea</span> CO2 <span class="hlt">flux</span> of more than 0.1 mmol/(m2s). Attempting to extrapolate such <span class="hlt">fluxes</span> 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 <span class="hlt">flux</span> estimate. Our results have implications not only for the design and execution of expedition-based sampling, but also for placement of in-situ sensors. Particularly in polar waters, sensors are usually deployed on moorings, well below the surface, to avoid damage and destruction from drifting ice. However, to obtain accurate information on <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> in these areas, it is necessary to deploy sensors on ice-capable buoys that can position the sensors in true 'surface' waters.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.9712B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.9712B"><span>Impact of Langmuir <span class="hlt">Turbulence</span> on Upper Ocean Response to Hurricane Edouard: Model and Observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Blair, A.; Ginis, I.; Hara, T.; Ulhorn, E.</p> <p>2017-12-01</p> <p>Tropical cyclone intensity is strongly affected by the <span class="hlt">air-sea</span> heat <span class="hlt">flux</span> beneath the storm. When strong storm winds enhance upper ocean <span class="hlt">turbulent</span> mixing and entrainment of colder water from below the thermocline, the resulting <span class="hlt">sea</span> surface temperature cooling may reduce the heat <span class="hlt">flux</span> to the storm and weaken the storm. Recent studies suggest that this upper ocean <span class="hlt">turbulence</span> is strongly affected by different <span class="hlt">sea</span> states (Langmuir <span class="hlt">turbulence</span>), which are highly complex and variable in tropical cyclone conditions. In this study, the upper ocean response under Hurricane Edouard (2014) is investigated using a coupled ocean-wave model with and without an explicit <span class="hlt">sea</span> state dependent Langmuir <span class="hlt">turbulence</span> parameterization. The results are compared with in situ observations of <span class="hlt">sea</span> surface temperature and mixed layer depth from AXBTs, as well as satellite <span class="hlt">sea</span> surface temperature observations. Overall, the model results of mixed layer deepening and <span class="hlt">sea</span> surface temperature cooling under and behind the storm are consistent with observations. The model results show that the effects of <span class="hlt">sea</span> state dependent Langmuir <span class="hlt">turbulence</span> can be significant, particularly on the mixed layer depth evolution. Although available observations are not sufficient to confirm such effects, some observed trends suggest that the <span class="hlt">sea</span> state dependent parameterization might be more accurate than the traditional (<span class="hlt">sea</span> state independent) parameterization.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_2");'>2</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li class="active"><span>4</span></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_4 --> <div id="page_5" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li class="active"><span>5</span></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="81"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19850005886&hterms=heat+exchange&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dheat%2Bexchange','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19850005886&hterms=heat+exchange&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dheat%2Bexchange"><span><span class="hlt">Air-sea</span> heat exchange, an element of the water cycle</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chahine, M. T.</p> <p>1984-01-01</p> <p>The distribution and variation of water vapor, clouds and precipitation are examined. Principal driving forces for these distributions are energy exchange and evaporation at the <span class="hlt">air-sea</span> interface, which are also important elements of <span class="hlt">air-sea</span> interaction studies. The overall aim of <span class="hlt">air-sea</span> interaction studies is to quantitatively determine mass, momentum and energy <span class="hlt">fluxes</span>, with the goal of understanding the mechanisms controlling them. The results of general circulation simulations indicate that the atmosphere in mid-latitudes responds to changes in the oceanic surface conditions in the tropics. This correlation reflects the strong interaction between tropical and mid-latitude conditions caused by the transport of heat and momentum from the tropics. Studies of <span class="hlt">air-sea</span> exchanges involve a large number of physica, chemical and dynamical processes including heat <span class="hlt">flux</span>, radiation, <span class="hlt">sea</span>-surface temperature, precipitation, winds and ocean currents. The <span class="hlt">fluxes</span> of latent heat are studied and the potential use of satellite data in determining them evaluated. Alternative ways of inferring heat <span class="hlt">fluxes</span> will be considered.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOS.A54C2732S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOS.A54C2732S"><span>Enhanced Ahead-of-Eye TC Coastal Ocean Cooling Processes and their Impact on <span class="hlt">Air-Sea</span> Heat <span class="hlt">Fluxes</span> and Storm Intensity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Seroka, G. N.; Miles, T. N.; Glenn, S. M.; Xu, Y.; Forney, R.; Roarty, H.; Schofield, O.; Kohut, J. T.</p> <p>2016-02-01</p> <p>Any landfalling tropical cyclone (TC) must first traverse the coastal ocean. TC research, however, has focused over the deep ocean, where TCs typically spend the vast majority of their lifetime. This paper will show that the ocean's response to TCs can be different between deep and shallow water, and that the additional shallow water processes must be included in coupled models for accurate <span class="hlt">air-sea</span> <span class="hlt">flux</span> treatment and TC intensity prediction. The authors will present newly observed coastal ocean processes that occurred in response to Hurricane Irene (2011), due to the presence of a coastline, an ocean bottom, and highly stratified conditions. These newly observed processes led to enhanced ahead-of-eye SST cooling that significantly impacted <span class="hlt">air-sea</span> heat <span class="hlt">fluxes</span> and Irene's operationally over-predicted storm intensity. Using semi-idealized modeling, we find that in shallow water in Irene, only 6% of cooling due to <span class="hlt">air-sea</span> heat <span class="hlt">fluxes</span>, 17% of cooling due to 1D vertical mixing, and 50% of cooling due to all processes (1D mixing, <span class="hlt">air-sea</span> heat <span class="hlt">fluxes</span>, upwelling, and advection) occurred ahead-of-eye—consistent with previous studies. Observations from an underwater glider and buoys, however, indicated 75-100% of total SST cooling over the continental shelf was ahead-of-eye. Thus, the new coastal ocean cooling processes found in this study must occur almost completely ahead-of-eye. We show that Irene's intense cooling was not captured by basic satellite SST products and coupled ocean-atmosphere hurricane models, and that including the cooling in WRF modeling mitigated the high bias in model predictions. Finally, we provide evidence that this SST cooling—not track, wind shear, or dry <span class="hlt">air</span> intrusion—was the key missing contribution to Irene's decay just prior to NJ landfall. Ongoing work is exploring the use of coupled WRF-ROMS modeling in the coastal zone.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/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 <span class="hlt">turbulent</span> 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 <span class="hlt">turbulent</span> 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://www.dtic.mil/docs/citations/AD1025192','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1025192"><span><span class="hlt">Turbulence</span> Simulation of Laboratory Wind-Wave Interaction in High Winds and Upscaling to Ocean Conditions</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2016-12-22</p> <p>investigated <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> characterized by strong <span class="hlt">air</span> flow separation over a very steep wave field. We first investigated propagating steep wave...mechanisms for flow separation over rigid surfaces compared with unsteady surfaces with a boundary slip velocity. We investigated passive scalar <span class="hlt">fluxes</span>. In...<span class="hlt">turbulent</span> flow over steep stationary roughness, the primary mechanism for momentum <span class="hlt">flux</span> is via pressure drag resulting from flow separation. However</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28132774','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28132774"><span>Distribution and <span class="hlt">sea-to-air</span> <span class="hlt">fluxes</span> of volatile halocarbons in the Bohai <span class="hlt">Sea</span> and North Yellow <span class="hlt">Sea</span> during spring.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>He, Zhen; Liu, Qiu-Lin; Zhang, Ying-Jie; Yang, Gui-Peng</p> <p>2017-04-15</p> <p>Concentrations of volatile halocarbons (VHCs), such as CHBr 2 Cl, CHBr 3 , C 2 HCl 3 , and C 2 Cl 4 , in the Bohai <span class="hlt">Sea</span> (BS) and North Yellow <span class="hlt">Sea</span> (NYS) were measured during the spring of 2014. The VHC concentrations varied widely and decreased with distance from the coast in the investigated area, with low values observed in the open <span class="hlt">sea</span>. Depth profiles of the VHCs were characterized by the highest concentration generally found in the upper water column. The distributions of the VHCs in the BS and NYS were clearly influenced by the combined effects of biological production, anthropogenic activities, and riverine input. The <span class="hlt">sea-to-air</span> <span class="hlt">fluxes</span> of CHBr 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.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AtmEn..46..669C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AtmEn..46..669C"><span>Wind tunnel measurements of pollutant <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> in urban intersections</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carpentieri, Matteo; Hayden, Paul; Robins, Alan G.</p> <p>2012-01-01</p> <p>Wind tunnel experiments have been carried out at the EnFlo laboratory to measure mean and <span class="hlt">turbulent</span> tracer <span class="hlt">fluxes</span> in geometries of real street canyon intersections. The work was part of the major DAPPLE project, focussing on the area surrounding the intersection between Marylebone Road and Gloucester Place in Central London, UK. Understanding flow and dispersion in urban streets is a very important issue for <span class="hlt">air</span> quality management and planning, and <span class="hlt">turbulent</span> mass exchange processes are important phenomena that are very often neglected in urban modelling studies. The adopted methodology involved the combined use of laser Doppler anemometry and tracer concentration measurements. This methodology was applied to quantify the mean and <span class="hlt">turbulent</span> flow and dispersion fields within several street canyon intersections. Vertical profiles of <span class="hlt">turbulent</span> tracer <span class="hlt">flux</span> were also measured. The technique, despite a number of limitations, proved reliable and allowed tracer balance calculations to be undertaken in the selected street canyon intersections. The experience gained in this work will enable much more precise studies in the future as issues affecting the accuracy of the experimental technique have been identified and resolved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017DyAtO..80...47D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017DyAtO..80...47D"><span>An assessment of Trop<span class="hlt">Flux</span> and NCEP <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> on ROMS simulations over the Bay of Bengal region</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dey, Dipanjan; Sil, Sourav; Jana, Sudip; Pramanik, Saikat; Pandey, P. C.</p> <p>2017-12-01</p> <p>This study presents an assessment of the Trop<span class="hlt">Flux</span> and the National Centers for Environmental Prediction (NCEP) reanalysis <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> in simulating the surface and subsurface oceanic parameters over the Bay of Bengal (BoB) region during 2002-2014 using the Regional Ocean Modelling System (ROMS). The assessment has been made by comparing the simulated fields with in-situ and satellite observations. The simulated surface and subsurface temperatures in the Trop<span class="hlt">Flux</span> forced experiment (Trop<span class="hlt">Flux</span>-E) show better agreement with the Research Moored Array for African-Asian-Australian Monsoon Analysis (RAMA) and Argo observations than the NCEP forced experiment (NCEP-E). The BoB domain averaged <span class="hlt">sea</span> surface temperature (SST) simulated in the NCEP-E is consistently cooler than the satellite SST, with a root mean square error (RMSE) of 0.79 °C. Moreover, NCEP-E shows a limitation in simulating the observed seasonal cycle of the SST due to substantial underestimation of the pre-monsoon SST peak. These limitations are mostly due to the lower values of the NCEP net heat <span class="hlt">flux</span>. The seasonal and interannual variations of SST in the Trop<span class="hlt">Flux</span>-E are better comparable to the observations with correlations and skills more than 0.80 and 0.90 respectively. However, SST is overestimated during summer monsoon periods mainly due to higher net heat <span class="hlt">flux</span>. The superiority of Trop<span class="hlt">Flux</span> forcing over the NCEP reanalysis can also be seen when simulating the interannual variabilities of the magnitude and vertical extent of Wyrtki jets at two equatorial RAMA buoy locations. The jet is weaker in the NCEP-E relative to the Trop<span class="hlt">Flux</span>-E and observations. The simulated <span class="hlt">sea</span> surface height anomalies (SSHA) from both the experiments are able to capture the regions of positive and negative SSHA with respect to satellite-derived altimeter data with better performance in the Trop<span class="hlt">Flux</span>-E. The speed of the westward propagating Rossby wave along 18°N in the Trop<span class="hlt">Flux</span>-E is found to be about 4.7 cm/s, which is close to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/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> <span class="hlt">turbulent</span> 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/2017AGUFMOS21A1356K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMOS21A1356K"><span>Methanethiol Concentrations and <span class="hlt">Sea-Air</span> <span class="hlt">Fluxes</span> in the Subarctic NE Pacific Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kiene, R. P.; Williams, T. E.; Esson, K.; Tortell, P. D.; Dacey, J. W. H.</p> <p>2017-12-01</p> <p>Exchange of volatile organic sulfur from the ocean to the atmosphere impacts the global sulfur cycle and the climate system and is thought to occur mainly via the gas dimethylsulfide (DMS). DMS is produced during degradation of the abundant phytoplankton osmolyte dimethylsulfoniopropionate (DMSP) but bacteria can also convert dissolved DMSP into the sulfur gas methanethiol (MeSH). MeSH has been difficult to measure in seawater because of its high chemical and biological reactivity and, thus, information on MeSH concentrations, distribution and <span class="hlt">sea-air</span> <span class="hlt">fluxes</span> is limited. We measured MeSH in the northeast subarctic Pacific Ocean in July 2016, along transects with strong phytoplankton abundance gradients. Water samples obtained with Niskin bottles were analyzed for MeSH by purge-and-trap gas chromatography. Depth profiles showed that MeSH concentrations were high near the surface and declined with depth. Surface waters (5 m depth) had an average MeSH concentration of 0.75 nM with concentrations reaching up to 3nM. MeSH concentrations were correlated (r = 0.47) with microbial turnover of dissolved DMSP which ranged up to 236 nM per day. MeSH was also correlated with total DMSP (r = 0.93) and dissolved DMS (r = 0.63), supporting the conclusion that DMSP was a major precursor of MeSH. Surface water MeSH:DMS concentration ratios averaged 0.19 and ranged up to 0.50 indicating that MeSH was a significant fraction of the volatile sulfur pool in surface waters. <span class="hlt">Sea-air</span> <span class="hlt">fluxes</span> of MeSH averaged 15% of the combined DMS+MeSH <span class="hlt">flux</span>, therefore MeSH contributed an important fraction of the sulfur emitted to the atmosphere from the subarctic NE Pacific Ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.8634D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.8634D"><span>Interannual variability of primary production and <span class="hlt">air-sea</span> CO2 <span class="hlt">flux</span> in the Atlantic and Indian sectors of the Southern Ocean.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dufour, Carolina; Merlivat, Liliane; Le Sommer, Julien; Boutin, Jacqueline; Antoine, David</p> <p>2013-04-01</p> <p>As one of the major oceanic sinks of anthropogenic 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 <span class="hlt">air-sea</span> CO2 <span class="hlt">fluxes</span> and how these processes might respond to climate change. It is well established that primary production is one of the major drivers of <span class="hlt">air-sea</span> CO2 <span class="hlt">fluxes</span>, consuming surface Dissolved Inorganic Carbon (DIC) during Summer. Southern Ocean primary production is though constrained by several limiting factors such as iron and light availability, which are both sensitive to mixed layer depth. Mixed layer depth is known to be affected by current changes in wind stress or freshwater <span class="hlt">fluxes</span> over the Southern Ocean. But we still don't know how primary production may respond to anomalous mixed layer depth neither how physical processes may balance this response to set the seasonal cycle of <span class="hlt">air-sea</span> CO2 <span class="hlt">fluxes</span>. In this study, we investigate the impact of anomalous mixed layer depth on surface DIC in the Atlantic and Indian sectors of the Subantarctic zone of the Southern Ocean (60W-60E, 38S-55S) with a combination of in situ data, satellite data and model experiment. We use both a regional eddy permitting ocean biogeochemical model simulation based on NEMO-PISCES and data-based reconstruction of biogeochemical fields based on CARIOCA buoys and <span class="hlt">Sea</span>WiFS data. A decomposition of the physical and biological processes driving the seasonal variability of surface DIC is performed with both the model data and observations. A good agreement is found between the model and the data for the amplitude of biological and <span class="hlt">air-sea</span> <span class="hlt">flux</span> contributions. The model data are further used to investigate the impact of winter and summer anomalies in mixed layer depth on surface DIC over the period 1990-2004. The relative changes of each physical and biological process contribution are quantified and discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.9092S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.9092S"><span><span class="hlt">Turbulence</span> and Mixing in a Shallow Shelf <span class="hlt">Sea</span> From Underwater Gliders</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schultze, Larissa K. P.; Merckelbach, Lucas M.; Carpenter, Jeffrey R.</p> <p>2017-11-01</p> <p>The seasonal thermocline in shallow shelf <span class="hlt">seas</span> acts as a natural barrier for boundary-generated <span class="hlt">turbulence</span>, damping scalar transport to the upper regions of the water column and controlling primary production to a certain extent. To better understand <span class="hlt">turbulence</span> and mixing conditions within the thermocline, two unique 12 and 17 day data sets with continuous measurements of the dissipation rate of <span class="hlt">turbulent</span> kinetic energy (ɛ) collected by autonomous underwater gliders under stratified to well-mixed conditions are presented. A highly intermittent ɛ signal was observed in the stratified thermocline region, which was mainly characterized by quiescent flow (<span class="hlt">turbulent</span> activity index below 7). The rate of diapycnal mixing remained relatively constant for the majority of the time with peaks of higher <span class="hlt">fluxes</span> that were responsible for much of the increase in bottom mixed layer temperature. The water column stayed predominantly strongly stratified, with a bulk Richardson number across the thermocline well above 2. A positive relationship between the intensity of <span class="hlt">turbulence</span>, shear, and stratification was found. The trend between <span class="hlt">turbulence</span> levels and the bulk Richardson number was relatively weak but suggests that ɛ increases as the bulk Richardson number approaches 1. The results also highlight the interpretation difficulties in both quantifying <span class="hlt">turbulent</span> thermocline <span class="hlt">fluxes</span> as well as the responsible mechanisms.</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 <span class="hlt">turbulent</span> 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://pubs.er.usgs.gov/publication/70120200','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70120200"><span><span class="hlt">Air-sea</span> interactions during strong winter extratropical storms</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Nelson, Jill; He, Ruoying; Warner, John C.; Bane, John</p> <p>2014-01-01</p> <p>A high-resolution, regional coupled atmosphere–ocean model is used to investigate strong air–<span class="hlt">sea</span> interactions during a rapidly developing extratropical cyclone (ETC) off the east coast of the USA. In this two-way coupled system, surface momentum and heat <span class="hlt">fluxes</span> derived from the Weather Research and Forecasting model and <span class="hlt">sea</span> surface temperature (SST) from the Regional Ocean Modeling System are exchanged via the Model Coupling Toolkit. Comparisons are made between the modeled and observed wind velocity, <span class="hlt">sea</span> level pressure, 10 m <span class="hlt">air</span> temperature, and <span class="hlt">sea</span> surface temperature time series, as well as a comparison between the model and one glider transect. Vertical profiles of modeled <span class="hlt">air</span> temperature and winds in the marine atmospheric boundary layer and temperature variations in the upper ocean during a 3-day storm period are examined at various cross-shelf transects along the eastern seaboard. It is found that the air–<span class="hlt">sea</span> interactions near the Gulf Stream are important for generating and sustaining the ETC. In particular, locally enhanced winds over a warm <span class="hlt">sea</span> (relative to the land temperature) induce large surface heat <span class="hlt">fluxes</span> which cool the upper ocean by up to 2 °C, mainly during the cold <span class="hlt">air</span> outbreak period after the storm passage. Detailed heat budget analyses show the ocean-to-atmosphere heat <span class="hlt">flux</span> dominates the upper ocean heat content variations. Results clearly show that dynamic air–<span class="hlt">sea</span> interactions affecting momentum and buoyancy <span class="hlt">flux</span> exchanges in ETCs need to be resolved accurately in a coupled atmosphere–ocean modeling framework.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1910765G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1910765G"><span>Surface energy budget and <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> at Arctic terrestrial sites</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Grachev, Andrey; Persson, Ola; Uttal, Taneil; Konopleva-Akish, Elena; Crepinsek, Sara; Cox, Christopher; Fairall, Christopher; Makshtas, Alexander; Repina, Irina</p> <p>2017-04-01</p> <p>Determination of the surface energy budget (SEB) and all SEB components at the <span class="hlt">air</span>-surface interface are required in a wide variety of applications including atmosphere-land/snow simulations and validation of the surface <span class="hlt">fluxes</span> predicted by numerical models over different spatial and temporal scales. Here, comparisons of net surface energy budgets at two Arctic sites are made using long-term near-continuous measurements of hourly averaged surface <span class="hlt">fluxes</span> (<span class="hlt">turbulent</span>, radiation, and soil conduction). One site, Eureka (80.0 N; Nunavut, Canada), is located in complex topography near a fjord about 200 km from the Arctic Ocean. The other site, Tiksi (71.6 N; Russian East Siberia), is located on a relatively flat coastal plain less than 1 km from the shore of Tiksi Bay, a branch of the Arctic Ocean. We first analyzed diurnal and annual cycles of basic meteorological parameters and key SEB components at these locations. Although Eureka and Tiksi are located on different continents and at different latitudes, the annual course of the surface meteorology and SEB components are qualitatively similar. Surface energy balance closure is a formulation of the conservation of energy principle. Our direct measurements of energy balance for both Arctic sites show that the sum of the <span class="hlt">turbulent</span> sensible and latent heat <span class="hlt">fluxes</span> and the ground (conductive) heat <span class="hlt">flux</span> systematically underestimate the net radiation by about 25-30%. This lack of energy balance closure is a fundamental and pervasive problem in micrometeorology. We discuss a variety of factors which may be responsible for the lack of SEB closure. In particular, various storage terms (e.g., <span class="hlt">air</span> column energy storage due to radiative and/or sensible heat <span class="hlt">flux</span> divergence, ground heat storage above the soil <span class="hlt">flux</span> plate, energy used in photosynthesis, canopy biomass heat storage). For example, our observations show that the photosynthesis storage term is relatively small (about 1-2% of the net radiation), but about 8-12% of the</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 <span class="hlt">turbulence</span> 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/2016EGUGA..18.2084L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.2084L"><span>Computed and observed <span class="hlt">turbulent</span> 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 <span class="hlt">turbulent</span> <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/2010AGUFM.C43E0586E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.C43E0586E"><span>Carbon Dioxide Transfer Through <span class="hlt">Sea</span> Ice: Modelling <span class="hlt">Flux</span> in Brine Channels</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Edwards, L.; Mitchelson-Jacob, G.; Hardman-Mountford, N.</p> <p>2010-12-01</p> <p>For many years <span class="hlt">sea</span> ice was thought to act as a barrier to the <span class="hlt">flux</span> of CO2 between the ocean and atmosphere. However, laboratory-based and in-situ observations suggest that while <span class="hlt">sea</span> ice may in some circumstances reduce or prevent transfer (e.g. in regions of thick, superimposed multi-year ice), it may also be highly permeable (e.g. thin, first year ice) with some studies observing significant <span class="hlt">fluxes</span> of CO2. <span class="hlt">Sea</span> ice covered regions have been observed to act both as a sink and a source of atmospheric CO2 with the permeability of <span class="hlt">sea</span> ice and direction of <span class="hlt">flux</span> related to <span class="hlt">sea</span> ice temperature and the presence of brine channels in the ice, as well as seasonal processes such as whether the ice is freezing or thawing. Brine channels concentrate dissolved inorganic carbon (DIC) as well as salinity and as these dense waters descend through both the <span class="hlt">sea</span> ice and the surface ocean waters, they create a sink for CO2. Calcium carbonate (ikaite) precipitation in the <span class="hlt">sea</span> ice is thought to enhance this process. Micro-organisms present within the <span class="hlt">sea</span> ice will also contribute to the CO2 <span class="hlt">flux</span> dynamics. Recent evidence of decreasing <span class="hlt">sea</span> ice extent and the associated change from a multi-year ice to first-year ice dominated system suggest the potential for increased CO2 <span class="hlt">flux</span> through regions of thinner, more porous <span class="hlt">sea</span> ice. A full understanding of the processes and feedbacks controlling the <span class="hlt">flux</span> in these regions is needed to determine their possible contribution to global CO2 levels in a future warming climate scenario. Despite the significance of these regions, the <span class="hlt">air-sea</span> CO2 <span class="hlt">flux</span> in <span class="hlt">sea</span> ice covered regions is not currently included in global climate models. Incorporating this carbon <span class="hlt">flux</span> system into Earth System models requires the development of a well-parameterised <span class="hlt">sea</span> ice-<span class="hlt">air</span> <span class="hlt">flux</span> model. In our work we use the Los Alamos <span class="hlt">sea</span> ice model, CICE, with a modification to incorporate the movement of CO2 through brine channels including the addition of DIC processes and ice algae production to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.B53B0463T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.B53B0463T"><span>Similarity scaling of <span class="hlt">turbulence</span> in small temperate lake: implication for gas <span class="hlt">flux</span>: implication for gas <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>Tedford, E. W.; MacIntyre, S.; Miller, S. D.; Czikowsky, M. J.</p> <p>2013-12-01</p> <p>The actively mixing layer, or surface layer, is the region of the upper mixed layer of lakes, oceans and the atmosphere directly influenced by wind, heating and cooling. <span class="hlt">Turbulence</span> within the surface mixing layer has a direct impact on important ecological processes. The Monin-Obukhov length scale (LMO) is a critical length scale used in predicting and understanding <span class="hlt">turbulence</span> in the actively mixed layer. On the water side of the <span class="hlt">air</span>-water interface, LMO is defined as: LMO=-u*^3/(0.4 JB0) where u*, the shear velocity, is defined as (τ/rho)^0.5 where τ is the shear stress and rho is the density of water and JBO is the buoyancy <span class="hlt">flux</span> at the surface. Above the depth equal to the absolute value of the Monin-Obukhov length scale (zMO), wind shear is assumed to dominate the production of <span class="hlt">turbulent</span> kinetic energy (TKE). Below zMO, the <span class="hlt">turbulence</span> is assumed to be suppressed when JB0 is stabilizing (warming surface waters) and enhanced when the buoyancy <span class="hlt">flux</span> is destabilizing (cooling surface waters). Our observed dissipations were well represented using the canonical similarity scaling equations. The Monin-Obukhov length scale was generally effective in separating the surface-mixing layer into two regions: an upper region, dominated by wind shear; and a lower region, dominated by buoyancy <span class="hlt">flux</span>. During both heating and cooling and above a depth equal to |LMO|, <span class="hlt">turbulence</span> was dominated by wind shear and dissipation followed law of the wall scaling although was slightly augmented by buoyancy <span class="hlt">flux</span> during both heating and cooling. Below a depth equal to |LMO| during cooling, dissipation was nearly uniform with depth. Although distinguishing between an upper region of the actively mixing layer dominated by wind stress and a lower portion dominated by buoyancy <span class="hlt">flux</span> is typically accurate the most accurate estimates of dissipation include the effects of both wind stress and buoyancy <span class="hlt">flux</span> throughout the actively mixed layer. We demonstrate and discuss the impact of neglecting the</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 <span class="hlt">turbulent</span> <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/2010EGUGA..12.8339M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..12.8339M"><span>Energy balance and non-<span class="hlt">turbulent</span> <span class="hlt">fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moderow, Uta; Feigenwinter, Christian; Bernhofer, Christian</p> <p>2010-05-01</p> <p>Often, the sum of the <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> of sensible heat and latent heat from eddy covariance (EC) measurements does not match the available energy (sum of net radiation, ground heat <span class="hlt">flux</span> and storage changes). This is referred to as energy balance closure gap. The reported imbalances vary between 0% and 50% (Laubach 1996). In various publications, it has been shown that the uncertainty of the available energy itself does not explain the gap (Vogt et al. 1996; Moderow et al. 2009). Among other reasons, the underestimation is attributed to an underestimation of <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> and undetected non-<span class="hlt">turbulent</span> transport processes, i.e. advection (e.g. Foken et al. 2006). The imbalance is typically larger during nighttime than during daytime as the EC method fails to capture non-<span class="hlt">turbulent</span> transports that can be significant during night (e.g. Aubinet 2008). Results for the budget of CO2 showed that including non-<span class="hlt">turbulent</span> <span class="hlt">fluxes</span> can change the budgets considerably. Hence, it is interesting to see how the budget of energy is changed. Here, the consequences of including advective <span class="hlt">fluxes</span> of sensible heat and latent heat in the energy balance are explored with focus on nighttime conditions. Non-<span class="hlt">turbulent</span> <span class="hlt">fluxes</span> will be inspected critically regarding their plausibility. Following Bernhofer et al. (2003), a ratio similar to Bowen's ratio of the <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> are defined for the non-<span class="hlt">turbulent</span> <span class="hlt">fluxes</span> and compared to each other. This might have implications for the partitioning of the available energy into sensible heat and latent heat. Data of the ADVEX-campaigns (Feigenwinter et al. 2008) of three different sites across Europe are used and selected periods are inspected. References Aubinet M (2008) Eddy covariance CO2-<span class="hlt">flux</span> measurements in nocturnal conditions: An analysis of the problem. Ecol Appl 18: 1368-1378 Bernhofer C, Grünwald T, Schwiebus A, Vogt R (2003) Exploring the consequences of non-zero energy balance closure for total surface <span class="hlt">flux</span>. In: Bernhofer C (ed</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/2017JGRC..122.5566F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.5566F"><span>Effects of <span class="hlt">sea</span>-ice and biogeochemical processes and storms on under-ice water fCO2 during the winter-spring transition in the high Arctic Ocean: Implications for <span class="hlt">sea-air</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>Fransson, Agneta; Chierici, Melissa; Skjelvan, Ingunn; Olsen, Are; Assmy, Philipp; Peterson, Algot K.; Spreen, Gunnar; Ward, Brian</p> <p>2017-07-01</p> <p>We performed measurements of carbon dioxide fugacity (fCO2) in the surface water under Arctic <span class="hlt">sea</span> ice from January to June 2015 during the Norwegian young <span class="hlt">sea</span> ICE (N-ICE2015) expedition. Over this period, the ship drifted with four different ice floes and covered the deep Nansen Basin, the slopes north of Svalbard, and the Yermak Plateau. This unique winter-to-spring data set includes the first winter-time under-ice water 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 <span class="hlt">sea</span> ice partly prevented direct CO2 exchange between ocean and atmosphere, frequently occurring leads and breakup of the ice sheet promoted <span class="hlt">sea-air</span> CO2 <span class="hlt">fluxes</span>. 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 <span class="hlt">sea-air</span> CO2 <span class="hlt">fluxes</span> 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 <span class="hlt">sea-air</span> CO2 <span class="hlt">fluxes</span> 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%, <span class="hlt">sea-air</span> CO2 <span class="hlt">fluxes</span> 16%, and temperature and salinity insignificant.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20000072433','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20000072433"><span>Seven-Year SSM/I-Derived Global Ocean Surface <span class="hlt">Turbulent</span> <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</p> <p>2000-01-01</p> <p>A 7.5-year (July 1987-December 1994) dataset of daily surface specific humidity and <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> (momentum, latent heat, and sensible heat) over global oceans has been retrieved from the Special Sensor Microwave/Imager (SSM/I) data and other data. It has a spatial resolution of 2.0 deg.x 2.5 deg. latitude-longitude. The retrieved surface specific humidity is generally accurate over global oceans as validated against the collocated radiosonde observations. The retrieved daily wind stresses and latent heat <span class="hlt">fluxes</span> show useful accuracy as verified by those measured by the RV Moana Wave and IMET buoy in the western equatorial Pacific. The derived <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> and input variables are also found to agree generally with the global distributions of annual-and seasonal-means of those based on 4-year (1990-93) comprehensive ocean-atmosphere data set (COADS) with adjustment in wind speeds and other climatological studies. The COADS has collected the most complete surface marine observations, mainly from merchant ships. However, ship measurements generally have poor accuracy, and variable spatial coverages. Significant differences between the retrieved and COADS-based are found in some areas of the tropical and southern extratropical oceans, reflecting the paucity of ship observations outside the northern extratropical oceans. Averaged over the global oceans, the retrieved wind stress is smaller but the latent heat <span class="hlt">flux</span> is larger than those based on COADS. The former is suggested to be mainly due to overestimation of the adjusted ship-estimated wind speeds (depending on <span class="hlt">sea</span> states), while the latter is suggested to be mainly due to overestimation of ship-measured dew point temperatures. The study suggests that the SSM/I-derived <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> can be used for climate studies and coupled model validations.</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 <span class="hlt">turbulent</span> <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 <span class="hlt">turbulent</span> 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 <span class="hlt">turbulent</span> 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/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. <span class="hlt">Turbulent</span> 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 <span class="hlt">turbulent</span> 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. <span class="hlt">Turbulent</span> 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/2018GeoRL..45..418Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoRL..45..418Z"><span>The Influence of <span class="hlt">Air-Sea</span> <span class="hlt">Fluxes</span> on Atmospheric Aerosols During the Summer Monsoon Over the Tropical Indian Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zavarsky, Alex; Booge, Dennis; Fiehn, Alina; Krüger, Kirstin; Atlas, Elliot; Marandino, Christa</p> <p>2018-01-01</p> <p>During the summer monsoon, the western tropical Indian Ocean is predicted to be a hot spot for dimethylsulfide emissions, the major marine sulfur source to the atmosphere, and an important aerosol precursor. Other aerosol relevant <span class="hlt">fluxes</span>, such as isoprene and <span class="hlt">sea</span> spray, should also be enhanced, due to the steady strong winds during the monsoon. Marine <span class="hlt">air</span> masses dominate the area during the summer monsoon, excluding the influence of continentally derived pollutants. During the SO234-2/235 cruise in the western tropical Indian Ocean from July to August 2014, directly measured eddy covariance DMS <span class="hlt">fluxes</span> confirm that the area is a large source of sulfur to the atmosphere (cruise average 9.1 μmol m-2 d-1). The directly measured <span class="hlt">fluxes</span>, as well as computed isoprene and <span class="hlt">sea</span> spray <span class="hlt">fluxes</span>, were combined with FLEXPART backward and forward trajectories to track the emissions in space and time. The <span class="hlt">fluxes</span> show a significant positive correlation with aerosol data from the Terra and Suomi-NPP satellites, indicating a local influence of marine emissions on atmospheric aerosol numbers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19900018950','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19900018950"><span><span class="hlt">Turbulent</span> statistics in the vicinity of an SST front: A north wind case, FASINEX February 16, 1986</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Stage, Steven A.; Herbster, Chris</p> <p>1990-01-01</p> <p>The technique of boxcar variances and covariances is used to examine NCAR Electra data from FASINEX (Frontal <span class="hlt">Air-Sea</span> Interaction EXperiment). This technique was developed to examine changes in <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> near a <span class="hlt">sea</span> surface temperature (SST) front. The results demonstrate the influence of the SST front on the MABL (Marine Atmospheric Boundary Layer). Data shown are for February 16, 1986, when the winds blew from over cold water to warm. The front directly produced horizontal variability in the <span class="hlt">turbulence</span>. The front also induced a secondary circulation which further modified the <span class="hlt">turbulence</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013BGeo...10.2699S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013BGeo...10.2699S"><span>Coccolithophore surface distributions in the North Atlantic and their modulation of the <span class="hlt">air-sea</span> <span class="hlt">flux</span> of CO2 from 10 years of satellite Earth observation data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shutler, J. D.; Land, P. E.; Brown, C. W.; Findlay, H. S.; Donlon, C. J.; Medland, M.; Snooke, R.; Blackford, J. C.</p> <p>2013-04-01</p> <p>Coccolithophores are the primary oceanic phytoplankton responsible for the production of calcium carbonate (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 (<span class="hlt">air-sea</span>) 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 <span class="hlt">Sea</span>-viewing Wide Field-of-view Sensor (<span class="hlt">Sea</span>WiFS). We calculate the annual mean <span class="hlt">sea</span> surface areal coverage of E. huxleyi in the North Atlantic to be 474 000 ± 104 000 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 <span class="hlt">air-sea</span> <span class="hlt">flux</span> of atmospheric CO2. In regions where the blooms are prevalent, the average reduction in the monthly <span class="hlt">air-sea</span> CO2 <span class="hlt">flux</span> can reach 55%. The maximum reduction of the monthly <span class="hlt">air-sea</span> CO2 <span class="hlt">flux</span> 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 <span class="hlt">air-to-sea</span> <span class="hlt">flux</span> of CO2. We estimate that these blooms can reduce the annual N. Atlantic net sink atmospheric CO2 by between 3-28%.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.1791W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.1791W"><span>Modelling storm development and the impact when introducing waves, <span class="hlt">sea</span> spray and heat <span class="hlt">fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wu, Lichuan; Rutgersson, Anna; Sahlée, Erik</p> <p>2015-04-01</p> <p>In high wind speed conditions, <span class="hlt">sea</span> spray generated due to intensity breaking waves have big influence on the wind stress and heat <span class="hlt">fluxes</span>. Measurements show that drag coefficient will decrease in high wind speed. <span class="hlt">Sea</span> spray generation function (SSGF), an important term of wind stress parameterization in high wind speed, usually treated as a function of wind speed/friction velocity. In this study, we introduce a wave state depended SSGG and wave age depended Charnock number into a high wind speed wind stress parameterization (Kudryavtsev et al., 2011; 2012). The proposed wind stress parameterization and <span class="hlt">sea</span> spray heat <span class="hlt">fluxes</span> parameterization from Andreas et al., (2014) were applied to an atmosphere-wave coupled model to test on four storm cases. Compared with measurements from the FINO1 platform in the North <span class="hlt">Sea</span>, the new wind stress parameterization can reduce the forecast errors of wind in high wind speed range, but not in low wind speed. Only <span class="hlt">sea</span> spray impacted on wind stress, it will intensify the storms (minimum <span class="hlt">sea</span> level pressure and maximum wind speed) and lower the <span class="hlt">air</span> temperature (increase the errors). Only the <span class="hlt">sea</span> spray impacted on the heat <span class="hlt">fluxes</span>, it can improve the model performance on storm tracks and the <span class="hlt">air</span> temperature, but not change much in the storm intensity. If both of <span class="hlt">sea</span> spray impacted on the wind stress and heat <span class="hlt">fluxes</span> are taken into account, it has the best performance in all the experiment for minimum <span class="hlt">sea</span> level pressure and maximum wind speed and <span class="hlt">air</span> temperature. Andreas, E. L., Mahrt, L., and Vickers, D. (2014). An improved bulk <span class="hlt">air-sea</span> surface <span class="hlt">flux</span> algorithm, including spray-mediated transfer. Quarterly Journal of the Royal Meteorological Society. Kudryavtsev, V. and Makin, V. (2011). Impact of ocean spray on the dynamics of the marine atmospheric boundary layer. Boundary-layer meteorology, 140(3):383-410. Kudryavtsev, V., Makin, V., and S, Z. (2012). On the <span class="hlt">sea</span>-surface drag and heat/mass transfer at strong winds. Technical report, Royal</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.2671L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.2671L"><span>On the role of <span class="hlt">sea</span>-state in bubble-mediated <span class="hlt">air-sea</span> gas <span class="hlt">flux</span> during a winter storm</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liang, Jun-Hong; Emerson, Steven R.; D'Asaro, Eric A.; McNeil, Craig L.; Harcourt, Ramsey R.; Sullivan, Peter P.; Yang, Bo; Cronin, Meghan F.</p> <p>2017-04-01</p> <p>Oceanic bubbles play an important role in the <span class="hlt">air-sea</span> exchange of weakly soluble gases at moderate to high wind speeds. A Lagrangian bubble model embedded in a large eddy simulation model is developed to study bubbles and their influence on dissolved gases in the upper ocean. The transient evolution of mixed-layer dissolved oxygen and nitrogen gases at Ocean Station Papa (50°N, 145°W) during a winter storm is reproduced with the model. Among different physical processes, gas bubbles are the most important in elevating dissolved gas concentrations during the storm, while atmospheric pressure governs the variability of gas saturation anomaly (the relative departure of dissolved gas concentration from the saturation concentration). For the same wind speed, bubble-mediated gas <span class="hlt">fluxes</span> are larger during rising wind with smaller wave age than during falling wind with larger wave age. Wave conditions are the primary cause for the bubble gas <span class="hlt">flux</span> difference: when wind strengthens, waves are less-developed with respect to wind, resulting in more frequent large breaking waves. Bubble generation in large breaking waves is favorable for a large bubble-mediated gas <span class="hlt">flux</span>. The wave-age dependence is not included in any existing bubble-mediated gas <span class="hlt">flux</span> parameterizations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/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 <span class="hlt">turbulent</span> 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/2016DyAtO..76...14S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016DyAtO..76...14S"><span><span class="hlt">Air-sea</span> CO2 <span class="hlt">flux</span> pattern along the southern Bay of Bengal waters</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shanthi, R.; Poornima, D.; Naveen, M.; Thangaradjou, T.; Choudhury, S. B.; Rao, K. H.; Dadhwal, V. K.</p> <p>2016-12-01</p> <p>Physico-chemical observations made from January 2013 to March 2015 in coastal waters of the southwest Bay of Bengal show pronounced seasonal variation in physico-chemical parameters including total alkalinity (TA: 1927.390-4088.642 μmol kg-1), chlorophyll (0.13-19.41 μg l-1) and also calculated dissolved inorganic carbon (DIC: 1574.219-3790.954 μmol kg-1), partial pressure of carbon dioxide (pCO2: 155.520-1488.607 μatm) and <span class="hlt">air-sea</span> CO2 <span class="hlt">flux</span> (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 <span class="hlt">flux</span> 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, <span class="hlt">sea</span> surface temperature (SST), pH and salinity observed in principal component analysis (PCA) suggested that physical and biological parameters play vital role in the seasonal distribution of pCO2 along the southwest Bay of Bengal. The annual variability of CO2 <span class="hlt">flux</span> 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 <span class="hlt">flux</span> of 0.204 ± 1.449 mmol Cm-2 d-1.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRD..122.7216O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRD..122.7216O"><span><span class="hlt">Sea-to-air</span> <span class="hlt">flux</span> of dimethyl sulfide in the South and North Pacific Ocean as measured by proton transfer reaction-mass spectrometry coupled with the gradient <span class="hlt">flux</span> technique</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Omori, Yuko; Tanimoto, Hiroshi; Inomata, Satoshi; Ikeda, Kohei; Iwata, Toru; Kameyama, Sohiko; Uematsu, Mitsuo; Gamo, Toshitaka; Ogawa, Hiroshi; Furuya, Ken</p> <p>2017-07-01</p> <p>Exchange of dimethyl sulfide (DMS) between the surface ocean and the lower atmosphere was examined by using proton transfer reaction-mass spectrometry coupled with the gradient <span class="hlt">flux</span> (PTR-MS/GF) system. We deployed the PTR-MS/GF system and observed vertical gradients of atmospheric DMS just above the <span class="hlt">sea</span> surface in the subtropical and transitional South Pacific Ocean and the subarctic North Pacific Ocean. In total, we obtained 370 in situ profiles, and of these we used 46 data sets to calculate the <span class="hlt">sea-to-air</span> <span class="hlt">flux</span> of DMS. The DMS <span class="hlt">flux</span> determined was in the range from 1.9 to 31 μmol m-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 <span class="hlt">air</span> overlying the ocean surface. The difference was mainly due to the <span class="hlt">sea-to-air</span> DMS emissions and stable atmospheric conditions, thus affecting the gradient of DMS. This indicates that the DMS gradient is strongly controlled by diurnal variations in the vertical structure of the lower atmosphere above the ocean surface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004JGRD..10924101G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004JGRD..10924101G"><span><span class="hlt">Flux</span> and <span class="hlt">turbulence</span> measurements at a densely built-up site in Marseille: Heat, mass (water and carbon dioxide), and momentum</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Grimmond, C. S. B.; Salmond, J. A.; Oke, T. R.; Offerle, B.; Lemonsu, A.</p> <p>2004-12-01</p> <p>Eddy covariance (EC) observations above the densely built-up center of Marseille during the Expérience sur site pour contraindre les modèles de pollution atmosphérique et de transport d'émissions (ESCOMPTE) summertime measurement campaign extend current understanding of surface atmosphere exchanges in cities. The instrument array presented opportunities to address issues of the representativeness of local-scale <span class="hlt">fluxes</span> in urban settings. Separate EC systems operated at two levels, and a telescoping tower allowed the pair to be exposed at two different sets of heights. The <span class="hlt">flux</span> and <span class="hlt">turbulence</span> observations taken at the four heights, stratified by wind conditions (mistral wind and <span class="hlt">sea</span> breeze), are used to address the partitioning of the surface energy balance in an area with large roughness elements. The <span class="hlt">turbulent</span> sensible heat <span class="hlt">flux</span> dominates in the daytime, although the storage heat <span class="hlt">flux</span> is a significant term that peaks before solar noon. The <span class="hlt">turbulent</span> latent heat <span class="hlt">flux</span> is small but not negligible. Carbon dioxide <span class="hlt">fluxes</span> show that this central city district is almost always a source, but the vegetation reduces the magnitude of the <span class="hlt">fluxes</span> in the afternoon. The atmosphere in such a heavily developed area is rarely stable. The <span class="hlt">turbulence</span> characteristics support the empirical functions proposed by M. Roth.</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 <span class="hlt">turbulent</span> 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/2014JMS...140...26M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JMS...140...26M"><span>Spatio-temporal dynamics of biogeochemical processes and <span class="hlt">air-sea</span> CO2 <span class="hlt">fluxes</span> in the Western English Channel based on two years of FerryBox deployment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marrec, P.; Cariou, T.; Latimier, M.; Macé, E.; Morin, P.; Vernet, M.; Bozec, Y.</p> <p>2014-12-01</p> <p>From January 2011 to January 2013, a FerryBox system was installed on a Voluntary Observing Ship (VOS), which crossed the Western English Channel (WEC) between Roscoff (France) and Plymouth (UK) up to 3 times a day. The FerryBox continuously measured <span class="hlt">sea</span> surface temperature (SST), <span class="hlt">sea</span> surface salinity (SSS), dissolved oxygen (DO), fluorescence and partial pressure of 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 <span class="hlt">air-sea</span> CO2 <span class="hlt">fluxes</span> in the WEC. Based on this unprecedented high-frequency dataset, the physical structure of the WEC was assessed using SST anomalies and the presence of a thermal front was observed around the latitude 49.5°N, which divided the WEC in two main provinces: the seasonally stratified northern WEC (nWEC) and the all-year well-mixed southern WEC (sWEC). These hydrographical properties strongly influenced the spatial and inter-annual distributions of phytoplankton blooms, which were mainly limited by nutrients and light availability in the nWEC and the sWEC, respectively. <span class="hlt">Air-sea</span> CO2 <span class="hlt">fluxes</span> were also highly related to hydrographical properties of the WEC between late April and early September 2012, with the sWEC a weak source of 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 <span class="hlt">air-sea</span> CO2 <span class="hlt">fluxes</span> revealed that an intense and short (less than 10 days) summer bloom in the nWEC contributed to 29% of the CO2 sink during the productive period, highlighting the necessity for high frequency observations in coastal</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/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 <span class="hlt">turbulent</span> 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://www.agu.org/journals/jc/v096/iC04/90JC02642/','USGSPUBS'); return false;" href="http://www.agu.org/journals/jc/v096/iC04/90JC02642/"><span>Atmospheric organochlorine pollutants and <span class="hlt">air-sea</span> exchange of hexachlorocyclohexane in the Bering and Chukchi <span class="hlt">Seas</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Hinckley, D.A.; Bidleman, T.F.; Rice, C.P.</p> <p>1991-01-01</p> <p>Organochlorine pesticides have been found in Arctic fish, marine mammals, birds, and plankton for some time. The lack of local sources and remoteness of the region imply long-range transport and deposition of contaminants into the Arctic from sources to the south. While on the third Soviet-American Joint Ecological Expedition to the Bering and Chukchi <span class="hlt">Seas</span> (August 1988), high-volume <span class="hlt">air</span> samples were taken and analyzed for organochlorine pesticides. Hexachlorocyclohexane (HCH), hexachlorobenzene, polychlorinated camphenes, and chlordane (listed in order of abundance, highest to lowest) were quantified. The <span class="hlt">air-sea</span> gas exchange of HCH was estimated at 18 stations during the cruise. Average alpha-HCH concentrations in concurrent atmosphere and surface water samples were 250 pg m-3 and 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 <span class="hlt">flux</span> for alpha-HCH ranged from -47 ng m-2 day-1 (<span class="hlt">sea</span> to <span class="hlt">air</span>) to 122 ng m-2 d-1 (<span class="hlt">air</span> to <span class="hlt">sea</span>) and averaged 25 ng m-2 d-1 <span class="hlt">air</span> to <span class="hlt">sea</span>. All <span class="hlt">fluxes</span> of gamma-HCH were from <span class="hlt">air</span> to <span class="hlt">sea</span>, ranged from 17 to 54 ng m-2 d-1, and averaged 31 ng m-2 d-1.</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 <span class="hlt">turbulence</span> 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('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. <span class="hlt">Turbulent</span> <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('http://adsabs.harvard.edu/abs/2012AGUFMOS11C1660Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMOS11C1660Z"><span>On the relationships of gas transfer velocity with <span class="hlt">turbulent</span> kinetic energy dissipation rate and wind waves</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhao, D.</p> <p>2012-12-01</p> <p>The exchange of carbon dioxide across the <span class="hlt">air-sea</span> interface is an important component of the atmospheric CO2 budget. Understanding how future changes in climate will affect oceanic uptake and releaser CO2 requires accurate estimation of <span class="hlt">air-sea</span> CO2 <span class="hlt">flux</span>. This <span class="hlt">flux</span> is typically expressed as the product of gas transfer velocity, CO2 partial pressure difference in seawater and <span class="hlt">air</span>, and the CO2 solubility. As the key parameter, gas transfer velocity has long been known to be controlled by the near-surface <span class="hlt">turbulence</span> in water, which is affected by many factors, such as wind forcing, ocean waves, water-side convection and rainfall. Although the wind forcing is believed as the major factor dominating the near-surface <span class="hlt">turbulence</span>, many studies have shown that the wind waves and their breaking would greatly enhance <span class="hlt">turbulence</span> compared with the classical solid wall theory. Gas transfer velocity has been parameterized in terms of wind speed, <span class="hlt">turbulent</span> kinetic energy dissipation rate, and wave parameters on the basis of observational data or theoretical analysis. However, great discrepancies, as large as one order, exist among these formulas. In this study, we will systematically analyze the differences of gas transfer velocity proposed so far, and try to find the reason that leads to their uncertainties. Finally, a new formula for gas transfer velocity will be given in terms of wind speed and wind wave parameter.</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/2016AGUFMOS31A1997S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS31A1997S"><span>Comparison of <span class="hlt">Sea-Air</span> CO2 <span class="hlt">Flux</span> Estimates Using Satellite-Based Versus Mooring Wind Speed Data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sutton, A. J.; Sabine, C. L.; Feely, R. A.; Wanninkhof, R. H.</p> <p>2016-12-01</p> <p>The global ocean is a major sink of anthropogenic 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 <span class="hlt">sea-air</span> CO2 <span class="hlt">flux</span> 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 - <span class="hlt">air</span> pCO2) and wind speed from moored platforms now allow for high-resolution CO2 <span class="hlt">flux</span> time series. Here we present a comparison of CO2 <span class="hlt">flux</span> 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 <span class="hlt">flux</span> on average by 5% at the Kuroshio Extension Observatory, Ocean Station Papa, WHOI Hawaii Ocean Timeseries Station, and Stratus. In general, CO2 <span class="hlt">flux</span> 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 <span class="hlt">flux</span> estimates and discuss the potential implications for tracking variability and change in global ocean CO2 uptake.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/467663-turbulence-structure-marine-stable-boundary-layer-over-baltic-sea','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/467663-turbulence-structure-marine-stable-boundary-layer-over-baltic-sea"><span><span class="hlt">Turbulence</span> structure of the marine stable boundary layer over the Baltic <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Smedman, A.S.; Hoegstroem, U.</p> <p></p> <p>For more than half of the year the land surfaces surrounding the Baltic <span class="hlt">Sea</span> is warmer than the <span class="hlt">sea</span> surface, and the marine boundary layer over the Baltic is stable. Observations, at various sites in the Baltic <span class="hlt">Sea</span> area during the last decade. also indicate frequent occurrence of low-level jets at the top of the stable boundary layer. In many cases the marine jet can be considered as an analogy in space to the evolution of the nocturnal jet with time. The frictional decoupling occurs when warm <span class="hlt">air</span> over the land is flowing out over the <span class="hlt">sea</span>. Data from twomore » areas together with model simulations are used in this study to characterize <span class="hlt">turbulence</span> structure in the marine boundary layer. The measurements include profiles of wind and temperature on towers situated at two isolated islands, together with <span class="hlt">turbulence</span> recordings and aircraft measurements. Also wave height and water surface temperature have been measured. The model simulations are performed with a second-order closure model.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22370197-magnetic-flux-concentration-zonal-flows-magnetorotational-instability-turbulence','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22370197-magnetic-flux-concentration-zonal-flows-magnetorotational-instability-turbulence"><span>Magnetic <span class="hlt">flux</span> concentration and zonal flows in magnetorotational instability <span class="hlt">turbulence</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>Bai, Xue-Ning; Stone, James M., E-mail: xbai@cfa.harvard.edu</p> <p>2014-11-20</p> <p>Accretion disks are likely threaded by external vertical magnetic <span class="hlt">flux</span>, which enhances the level of <span class="hlt">turbulence</span> via the magnetorotational instability (MRI). Using shearing-box simulations, we find that such external magnetic <span class="hlt">flux</span> also strongly enhances the amplitude of banded radial density variations known as zonal flows. Moreover, we report that vertical magnetic <span class="hlt">flux</span> is strongly concentrated toward low-density regions of the zonal flow. Mean vertical magnetic field can be more than doubled in low-density regions, and reduced to nearly zero in high-density regions in some cases. In ideal MHD, the scale on which magnetic <span class="hlt">flux</span> concentrates can reach a few diskmore » scale heights. In the non-ideal MHD regime with strong ambipolar diffusion, magnetic <span class="hlt">flux</span> is concentrated into thin axisymmetric shells at some enhanced level, whose size is typically less than half a scale height. We show that magnetic <span class="hlt">flux</span> concentration is closely related to the fact that the <span class="hlt">turbulent</span> diffusivity of the MRI <span class="hlt">turbulence</span> is anisotropic. In addition to a conventional Ohmic-like <span class="hlt">turbulent</span> resistivity, we find that there is a correlation between the vertical velocity and horizontal magnetic field fluctuations that produces a mean electric field that acts to anti-diffuse the vertical magnetic <span class="hlt">flux</span>. The anisotropic <span class="hlt">turbulent</span> diffusivity has analogies to the Hall effect, and may have important implications for magnetic <span class="hlt">flux</span> transport in accretion disks. The physical origin of magnetic <span class="hlt">flux</span> concentration may be related to the development of channel flows followed by magnetic reconnection, which acts to decrease the mass-to-<span class="hlt">flux</span> ratio in localized regions. The association of enhanced zonal flows with magnetic <span class="hlt">flux</span> concentration may lead to global pressure bumps in protoplanetary disks that helps trap dust particles and facilitates planet formation.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..1210167G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..1210167G"><span><span class="hlt">Air</span>-ice CO2 <span class="hlt">fluxes</span> and pCO2 dynamics in the Arctic coastal area (Amundsen Gulf, Canada)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Geilfus, Nicolas-Xavier; Tison, Jean Louis; Carnat, Gauthier; Else, Brent; Borges, Alberto V.; Thomas, Helmuth; Shadwick, Elizabeth; Delille, Bruno</p> <p>2010-05-01</p> <p><span class="hlt">Sea</span> ice covers about 7% of the Earth surface at its maximum seasonal extent. For decades <span class="hlt">sea</span> ice was assumed to be an impermeable and inert barrier for <span class="hlt">air</span> - <span class="hlt">sea</span> exchange of 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 <span class="hlt">sea</span> ice cover was recently reported raising the need to further investigate pCO2 dynamics in the marine cryosphere realm and related <span class="hlt">air</span>-ice CO2 <span class="hlt">fluxes</span>. In addition, budget of CO2 <span class="hlt">fluxes</span> are poorly constrained in high latitudes continental shelves [Borges et al., 2006]. We report measurements of <span class="hlt">air</span>-ice CO2 <span class="hlt">fluxes</span> 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 <span class="hlt">air</span>-ice CO2 <span class="hlt">fluxes</span> (chamber method) in Antarctic first year pack ice ("<span class="hlt">Sea</span> Ice Mass Balance in Antarctica -SIMBA" drifting station experiment September - October 2007) and in Arctic first year land fast ice ("Circumpolar Flaw Lead" - CFL, April - June 2008). These 2 experiments were carried out in contrasted sites. SIMBA was carried out on <span class="hlt">sea</span> ice in early spring while CFL was carried out in from the middle of the winter to the late spring while <span class="hlt">sea</span> ice was melting. Both in Arctic and Antarctic, no <span class="hlt">air</span>-ice CO2 <span class="hlt">fluxes</span> were detected when <span class="hlt">sea</span> ice interface was below -10°C. Slightly above -10°C, <span class="hlt">fluxes</span> toward the atmosphere were observed. In contrast, at -7°C <span class="hlt">fluxes</span> 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 <span class="hlt">sea</span> ice temperature. The pCO2 shifted from a large over-saturation at low temperature to a marked under-saturation at high temperature. These <span class="hlt">air</span>-ice CO2 <span class="hlt">fluxes</span> are partly controlled by the permeability of the <span class="hlt">air</span>-ice interface, which depends of the temperature of this one. Moreover, <span class="hlt">air</span>-ice CO2 <span class="hlt">fluxes</span> are</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GBioC..31..961W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GBioC..31..961W"><span>The impact of changing wind speeds on gas transfer and its effect on global <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>Wanninkhof, R.; Triñanes, J.</p> <p>2017-06-01</p> <p>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 <span class="hlt">fluxes</span> 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 <span class="hlt">air</span>-water partial pressure of CO2 gradient (ΔpCO2). The latter also controls the direction of the <span class="hlt">flux</span>. <span class="hlt">Fluxes</span> 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 <span class="hlt">air-sea</span> CO2 <span class="hlt">fluxes</span> 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.<abstract type="synopsis"><title type="main">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('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 <span class="hlt">turbulence</span> 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/2016APS..DFDG10003W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..DFDG10003W"><span><span class="hlt">Turbulent</span> convection driven by internal radiative heating of melt ponds on <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>Wells, Andrew; Langton, Tom; Rees Jones, David; Moon, Woosok</p> <p>2016-11-01</p> <p>The melting of Arctic <span class="hlt">sea</span> ice is strongly influenced by heat transfer through melt ponds which form on the ice surface. Melt ponds are internally heated by the absorption of incoming radiation and cooled by surface heat <span class="hlt">fluxes</span>, resulting in vigorous buoyancy-driven convection in the pond interior. Motivated by this setting, we conduct two-dimensional direct-numerical simulations of the <span class="hlt">turbulent</span> convective flow of a Boussinesq fluid between two horizontal boundaries, with internal heating predicted from a two-stream radiation model. A linearised thermal boundary condition describes heat exchange with the overlying atmosphere, whilst the lower boundary is isothermal. Vertically asymmetric convective flow modifies the upper surface temperature, and hence controls the partitioning of the incoming heat <span class="hlt">flux</span> between emission at the upper and lower boundaries. We determine how the downward heat <span class="hlt">flux</span> into the ice varies with a Rayleigh number based on the internal heating rate, the <span class="hlt">flux</span> ratio of background surface cooling compared to internal heating, and a Biot number characterising the sensitivity of surface <span class="hlt">fluxes</span> to surface temperature. Thus we elucidate the physical controls on heat transfer through Arctic melt ponds which determine the fate of <span class="hlt">sea</span> ice in the summer.</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/17294945','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17294945"><span><span class="hlt">Flux</span> enhancement during ultrafiltration of produced water using <span class="hlt">turbulence</span> promoter.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhen, Xiang-hua; Yu, Shui-li; Wang, Bei-fu; Zheng, Hai-feng</p> <p>2006-01-01</p> <p>Concentration polarization and membrane fouling remain one of the major hurdles for the implementation of ultrafiltration of produced water. Although many applications for ultrafiltration were already suggested, only few were implemented on an industrial scale. Among those techniques, <span class="hlt">turbulence</span> promoter can be more simple and effective in overcoming membrane fouling and enhancing membrane <span class="hlt">flux</span>. As for the result that <span class="hlt">turbulence</span> promoter increase fluid velocity, wall shear rates and produce secondary flows or instabilities, the influence of <span class="hlt">turbulence</span> promoter was investigated on permeate <span class="hlt">flux</span> during produced water ultrafiltration and the potential application of this arrangement for an industrial development. Experimental investigations were performed on 100 KDa molecular weight cut-off PVDF single-channel tubular membrane module using four kinds of <span class="hlt">turbulence</span> promoters. It is observed that the significant <span class="hlt">flux</span> enhancement in the range of 83%-164% was achieved while the hydraulic dissipated power per unit volume of permeate decreased from 31%-42%, which indicated that the using of <span class="hlt">turbulence</span> promoter is more efficient than operation without the <span class="hlt">turbulence</span> promoter. The effects of transmembrane pressure and cross-flow velocity with and without <span class="hlt">turbulence</span> promoter were studied as well. Among the four kinds of <span class="hlt">turbulence</span> promoters, winding inserts with 20.0 mm pitch and 1.0 mm wire diameter showed better performances than the others did.</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('http://adsabs.harvard.edu/abs/2017JGRD..122.5298J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRD..122.5298J"><span>Interaction between <span class="hlt">turbulent</span> flow and <span class="hlt">sea</span> breeze front over urban-like coast in large-eddy simulation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jiang, Ping; Wen, Zhiping; Sha, Weiming; Chen, Guixing</p> <p>2017-05-01</p> <p><span class="hlt">Turbulent</span> flow and its interaction with a <span class="hlt">sea</span> breeze front (SBF) over an urban-like coast with a regular block array were investigated using a building-resolving computational fluid dynamics model. It was found that during daytime with an offshore ambient flow, streaky <span class="hlt">turbulent</span> structures tended to grow within the convective boundary layer (CBL) over a warm urban surface ahead of the SBF. The structures were organized as streamwise streaks at an interval of a few hundred meters, which initiated at the rooftop level with strong wind shear and strengthens in the CBL with moderate buoyancy. The streaks then interacted with the onshore-propagating SBF as it made landfall. The SBF, which was initially characterized as a shallow and quasi-linear feature over the <span class="hlt">sea</span>, developed three-dimensional structures with intensified updrafts at an elevated frontal head after landfall. Frontal updrafts were locally enhanced at intersections where the streaks merged with the SBF, which greatly increased <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> at the front. The frontal line was irregular because of merging, tilting, and transformation effects of vorticity associated with streaky structures. Inland penetration of the SBF was slowed by the frictional effect of urban-like surfaces and <span class="hlt">turbulent</span> flow on land. The overall SBF intensity weakened after the interaction with <span class="hlt">turbulent</span> flow. These findings aid understanding of local weather over coastal cities during typical <span class="hlt">sea</span> breeze conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21141036','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21141036"><span>Advances in quantifying <span class="hlt">air-sea</span> gas exchange and environmental forcing.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wanninkhof, Rik; Asher, William E; Ho, David T; Sweeney, Colm; McGillis, Wade R</p> <p>2009-01-01</p> <p>The past decade has seen a substantial amount of research on <span class="hlt">air-sea</span> gas exchange and its environmental controls. These studies have significantly advanced the understanding of processes that control gas transfer, led to higher quality field measurements, and improved estimates of the <span class="hlt">flux</span> of climate-relevant gases between the ocean and atmosphere. This review discusses the fundamental principles of <span class="hlt">air-sea</span> gas transfer and recent developments in gas transfer theory, parameterizations, and measurement techniques in the context of the exchange of carbon dioxide. However, much of this discussion is applicable to any sparingly soluble, non-reactive gas. We show how the use of global variables of environmental forcing that have recently become available and gas exchange relationships that incorporate the main forcing factors will lead to improved estimates of global and regional <span class="hlt">air-sea</span> gas <span class="hlt">fluxes</span> based on better fundamental physical, chemical, and biological foundations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16711925','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16711925"><span>Effect of heat <span class="hlt">flux</span> on differential rotation in <span class="hlt">turbulent</span> convection.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kleeorin, Nathan; Rogachevskii, Igor</p> <p>2006-04-01</p> <p>We studied the effect of the <span class="hlt">turbulent</span> heat <span class="hlt">flux</span> on the Reynolds stresses in a rotating <span class="hlt">turbulent</span> convection. To this end we solved a coupled system of dynamical equations which includes the equations for the Reynolds stresses, the entropy fluctuations, and the <span class="hlt">turbulent</span> heat <span class="hlt">flux</span>. We used a spectral tau approximation in order to close the system of dynamical equations. We found that the ratio of the contributions to the Reynolds stresses caused by the <span class="hlt">turbulent</span> heat <span class="hlt">flux</span> and the anisotropic eddy viscosity is of the order of approximately 10(L rho/l0)2, where l0 is the maximum scale of <span class="hlt">turbulent</span> motions and L rho is the fluid density variation scale. This effect is crucial for the formation of the differential rotation and should be taken into account in the theories of the differential rotation of the Sun, stars, and planets. In particular, we demonstrated that this effect may cause the differential rotation which is comparable with the typical solar differential rotation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.A41G0208Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.A41G0208Z"><span><span class="hlt">Turbulence</span> and Coherent Structure in the Atmospheric Boundary Layer near the Eyewall of Hurricane Hugo (1989)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, J. A.; Marks, F. D.; Montgomery, M. T.; Black, P. G.</p> <p>2008-12-01</p> <p>In this talk we present an analysis of observational data collected from NOAA'S WP-3D research aircraft during the eyewall penetration of category five Hurricane Hugo (1989). The 1 Hz flight level data near 450m above the <span class="hlt">sea</span> surface comprising wind velocity, temperature, pressure and relative humidity are used to estimate the <span class="hlt">turbulence</span> intensity and <span class="hlt">fluxes</span>. In the <span class="hlt">turbulent</span> <span class="hlt">flux</span> calculation, the universal shape spectra and co-spectra derived using the 40 Hz data collected during the Coupled Boundary Layer <span class="hlt">Air-sea</span> Transfer (CBLAST) Hurricane experiment are applied to correct the high frequency part of the data collected in Hurricane Hugo. Since the stationarity assumption required for standard eddy correlations is not always satisfied, different methods are summarized for computing the <span class="hlt">turbulence</span> parameters. In addition, a wavelet analysis is conducted to investigate the time and special scales of roll vortices or coherent structures that are believed important elements of the eye/eyewall mixing processes that support intense storms.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014APS..DPPTP8051M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014APS..DPPTP8051M"><span><span class="hlt">Turbulent</span> transport regimes and the SOL heat <span class="hlt">flux</span> width</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Myra, J. R.; D'Ippolito, D. A.; Russell, D. A.</p> <p>2014-10-01</p> <p>Understanding the responsible mechanisms and resulting scaling of the scrape-off layer (SOL) heat <span class="hlt">flux</span> width is important for predicting viable operating regimes in future tokamaks, and for seeking possible mitigation schemes. Simulation and theory results using reduced edge/SOL <span class="hlt">turbulence</span> models have produced SOL widths and scalings in reasonable accord with experiments in many cases. In this work, we attempt to qualitatively and conceptually understand various regimes of edge/SOL <span class="hlt">turbulence</span> and the role of <span class="hlt">turbulent</span> transport in establishing the SOL heat <span class="hlt">flux</span> width. Relevant considerations include the type and spectral characteristics of underlying instabilities, the location of the gradient drive relative to the SOL, the nonlinear saturation mechanism, and the parallel heat transport regime. Recent SOLT <span class="hlt">turbulence</span> code results are employed to understand the roles of these considerations and to develop analytical scalings. We find a heat <span class="hlt">flux</span> width scaling with major radius R that is generally positive, consistent with older results reviewed in. The possible relationship of <span class="hlt">turbulence</span> mechanisms to the heuristic drift mechanism is considered, together with implications for future experiments. Work supported by US DOE grant DE-FG02-97ER54392.</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 <span class="hlt">turbulence</span> at the water surface. We correct <span class="hlt">fluxes</span> by measuring <span class="hlt">turbulence</span> 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 <span class="hlt">turbulence</span>. 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 <span class="hlt">turbulence</span> 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 <span class="hlt">turbulence</span> at the water surface. We correct <span class="hlt">fluxes</span> by measuring <span class="hlt">turbulence</span> 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 <span class="hlt">turbulence</span>. 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 <span class="hlt">turbulence</span> alone could not fully explain the variance in gas transfer velocity. We suggest therefore, that other factors like surfactants, rain or tidal current will have an impact on gas transfer parameterizations.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/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 <span class="hlt">turbulent</span> <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) <span class="hlt">turbulence</span> 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('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> </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/2018E%26ES..149a2048J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26ES..149a2048J"><span>The influence of surface roughness and <span class="hlt">turbulence</span> on heat <span class="hlt">fluxes</span> from an oil palm plantation in Jambi, Indonesia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>June, Tania; Meijide, Ana; Stiegler, Christian; Purba Kusuma, Alan; Knohl, Alexander</p> <p>2018-05-01</p> <p>Oil palm plantations are expanding vastly in Jambi, resulted in altered surface roughness and <span class="hlt">turbulence</span> characteristics, which may influence exchange of heat and mass. Micrometeorological measurements above oil palm canopy were conducted for the period 2013–2015. The oil palms were 12.5 years old, canopy height 13 meters and 1.5 years old canopy height 2.5 m. We analyzed the influence of surface roughness and <span class="hlt">turbulence</span> strenght on heat (sensible and latent) <span class="hlt">fluxes</span> by investigating the profiles and gradient of wind speed, and temperature, surface roughness (roughness length, zo, and zero plane displacement, d), and friction velocity u*. <span class="hlt">Fluxes</span> of heat were calculated using profile similarity methods taking into account atmospheric stability calculated using Richardson number Ri and the generalized stability factor ζ. We found that roughness parameters (zo, d, and u*) directly affect <span class="hlt">turbulence</span> in oil palm canopy and hence heat <span class="hlt">fluxes</span>; they are affected by canopy height, wind speed and atmospheric stability. There is a negative trend of d towards <span class="hlt">air</span> temperature above the oil palm canopy, indicating the effect of plant volume and height in lowering <span class="hlt">air</span> temperature. We propose studying the relation between zero plane displacement d with a remote sensing vegetation index for scaling up this point based analysis.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015APS..DFDA13002H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015APS..DFDA13002H"><span>Modeling variable density <span class="hlt">turbulence</span> in the wake of an <span class="hlt">air</span>-entraining transom stern</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hendrickson, Kelli; Yue, Dick</p> <p>2015-11-01</p> <p>This work presents a priori testing of closure models for the incompressible highly-variable density <span class="hlt">turbulent</span> (IHVDT) flows in the near wake region of a transom stern. This three-dimensional flow is comprised of convergent corner waves that originate from the body and collide on the ship center plane forming the ``rooster tail'' that then widens to form the divergent wave train. These violent free-surface flows and breaking waves are characterized by significant <span class="hlt">turbulent</span> mass <span class="hlt">flux</span> (TMF) at Atwood number At = (ρ2 -ρ1) / (ρ2 +ρ1) ~ 1 for which there is little guidance in <span class="hlt">turbulence</span> closure modeling for the momentum and scalar transport along the wake. To whit, this work utilizes high-resolution simulations of the near wake of a canonical three-dimensional transom stern using conservative Volume-of-Fluid (cVOF), implicit Large Eddy Simulation (iLES), and Boundary Data Immersion Method (BDIM) to capture the <span class="hlt">turbulence</span> and large scale <span class="hlt">air</span> entrainment. Analysis of the simulation results across and along the wake for the TMF budget and <span class="hlt">turbulent</span> anisotropy provide the physical basis of the development of multiphase <span class="hlt">turbulence</span> closure models. Performance of isotropic and anisotropic <span class="hlt">turbulent</span> mass <span class="hlt">flux</span> closure models will be presented. Sponsored by the Office of Naval Research.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20000064720&hterms=passive+transport&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dpassive%2Btransport','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20000064720&hterms=passive+transport&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dpassive%2Btransport"><span>Compressibility Effects on the Passive Scalar <span class="hlt">Flux</span> Within Homogeneous <span class="hlt">Turbulence</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Blaisdell, G. A.; Mansour, N. N.; Reynolds, W. C.</p> <p>1994-01-01</p> <p>Compressibility effects on <span class="hlt">turbulent</span> transport of a passive scalar are studied within homogeneous <span class="hlt">turbulence</span> using a kinematic decomposition of the velocity field into solenoidal and dilatational parts. It is found that the dilatational velocity does not produce a passive scalar <span class="hlt">flux</span>, and that all of the passive scalar <span class="hlt">flux</span> is due to the solenoidal velocity.</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/2014BoLMe.150..235S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014BoLMe.150..235S"><span>Influence from Surrounding Land on the <span class="hlt">Turbulence</span> Measurements Above a Lake</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sahlée, Erik; Rutgersson, Anna; Podgrajsek, Eva; Bergström, Hans</p> <p>2014-02-01</p> <p><span class="hlt">Turbulence</span> measurements taken at a Swedish lake are analyzed. Although the measurements took place over a relatively large lake with several km of undisturbed fetch, the <span class="hlt">turbulence</span> structure was found to be highly influenced by the surrounding land during daytime. Variance spectra of both horizontal velocity and scalars during both unstable and stable stratification displayed a low frequency peak. The energy at lower frequencies showed a daily variation, increasing in the morning and decreasing in the afternoon. This behaviour is explained by spectral lag, where the low frequency energy due to large eddies that originate from the convective boundary layer above the surrounding land. When the <span class="hlt">air</span> is advected over the lake the small eddies rapidly equilibrate with the new surface forcing. However, the large eddies remain for an appreciable distance and influence the <span class="hlt">turbulence</span> in the developing lake boundary layer. The variances of the horizontal velocity and scalars are increased by these large eddies, while the <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> are mainly unaffected. The drag coefficient, Stanton number and Dalton number used to parametrize the momentum <span class="hlt">flux</span>, heat <span class="hlt">flux</span> and latent heat <span class="hlt">flux</span> respectively all compare well with current parametrizations developed for open <span class="hlt">sea</span> conditions. The diurnal cycle of the partial pressure of methane, pCH4, observed at this site is closely related to the diurnal cycle of the lake-<span class="hlt">air</span> methane <span class="hlt">flux</span>. An idealized two-dimensional model simulation of the boundary layer at a lake site indicates that the strong response of pCH4 to the surface methane <span class="hlt">flux</span> is due to the shallow internal boundary layer that develops above the lake, allowing methane to accumulate in a relatively small volume.</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('http://adsabs.harvard.edu/abs/2018AnPhy.389...63W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AnPhy.389...63W"><span>Potential landscape and <span class="hlt">flux</span> field theory for <span class="hlt">turbulence</span> and nonequilibrium fluid systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wu, Wei; Zhang, Feng; Wang, Jin</p> <p>2018-02-01</p> <p><span class="hlt">Turbulence</span> is a paradigm for far-from-equilibrium systems without time reversal symmetry. To capture the nonequilibrium irreversible nature of <span class="hlt">turbulence</span> and investigate its implications, we develop a potential landscape and <span class="hlt">flux</span> field theory for <span class="hlt">turbulent</span> flow and more general nonequilibrium fluid systems governed by stochastic Navier-Stokes equations. We find that equilibrium fluid systems with time reversibility are characterized by a detailed balance constraint that quantifies the detailed balance condition. In nonequilibrium fluid systems with nonequilibrium steady states, detailed balance breaking leads directly to a pair of interconnected consequences, namely, the non-Gaussian potential landscape and the irreversible probability <span class="hlt">flux</span>, forming a 'nonequilibrium trinity'. The nonequilibrium trinity characterizes the nonequilibrium irreversible essence of fluid systems with intrinsic time irreversibility and is manifested in various aspects of these systems. The nonequilibrium stochastic dynamics of fluid systems including <span class="hlt">turbulence</span> with detailed balance breaking is shown to be driven by both the non-Gaussian potential landscape gradient and the irreversible probability <span class="hlt">flux</span>, together with the reversible convective force and the stochastic stirring force. We reveal an underlying connection of the energy <span class="hlt">flux</span> essential for <span class="hlt">turbulence</span> energy cascade to the irreversible probability <span class="hlt">flux</span> and the non-Gaussian potential landscape generated by detailed balance breaking. Using the energy <span class="hlt">flux</span> as a center of connection, we demonstrate that the four-fifths law in fully developed <span class="hlt">turbulence</span> is a consequence and reflection of the nonequilibrium trinity. We also show how the nonequilibrium trinity can affect the scaling laws in <span class="hlt">turbulence</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1997APS..DFD..Gb05L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1997APS..DFD..Gb05L"><span>Modification of <span class="hlt">Turbulence</span> Structures in a Channel Flow by Uniform Magnetic <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>Lee, D.; Choi, H.; Kim, J.</p> <p>1997-11-01</p> <p>Effects of electromagnetic forcing on the near-wall <span class="hlt">turbulence</span> are investigated by applying a uniform magnetic <span class="hlt">flux</span> in a <span class="hlt">turbulent</span> channel flow in the streamwise and spanwise directions, respectively. The base flow is a fully developed <span class="hlt">turbulent</span> channel flow and the direct numerical simulation technique is used. The electromagnetic force induced from the magnetic <span class="hlt">fluxes</span> reduces the intensity of the wall-layer structures and thus drag is significantly reduced. The wall-normal and spanwise velocity fluctuations and the Reynolds shear stress decrease with the increased magnetic <span class="hlt">flux</span> in both directions. The streamwise velocity fluctuations increase with the streamwise magnetic <span class="hlt">flux</span>, whereas they decrease with the spanwise magnetic <span class="hlt">flux</span>. It is also shown that the spanwise magnetic <span class="hlt">flux</span> is much more effective than the streamwise magnetic <span class="hlt">flux</span> in reducing the skin-friction drag. Instantaneous Lorentz force vectors show that the flow motions by the near-wall vortices are directly inhibited by the spanwise magnetic <span class="hlt">flux</span>, while they are less effectively inhibited by the streamwise magnetic <span class="hlt">flux</span>. Other <span class="hlt">turbulence</span> statistics that reveal the effects of the applied magnetic forcing will be presented. ^* Supported by KOSEF Contract No. 965-1008-003-2 and ONR Grant No. N00014-95-1-0352.</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 <span class="hlt">turbulent</span> kinetic energy dissipation measurements, indicating a higher rate of <span class="hlt">turbulence</span> 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/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 <span class="hlt">turbulence</span> 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 <span class="hlt">turbulence</span> 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 <span class="hlt">turbulence</span> statistics will be determined. This will give an insight on how ice presence</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002EGSGA..27.1934B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002EGSGA..27.1934B"><span><span class="hlt">Turbulent</span> Fogwater <span class="hlt">Flux</span> Measurements Above A Forest</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Burkard, R.; Eugster, W.; Buetzberger, P.; Siegwolf, R.</p> <p></p> <p>Many forest ecosystems in elevated regions receive a significant fraction of their wa- ter and nutrient input by the interception of fogwater. Recently, several studies have demonstrated the suitability of the eddy covariance technique for the direct measure- ment of <span class="hlt">turbulent</span> liquid water <span class="hlt">fluxes</span>. Since summer 2001 a fogwater <span class="hlt">flux</span> measure- ment equipment has been running at a montane site above a mixed forest canopy in Switzerland. The measurement equipment consists of a high-speed size-resolving droplet spectrometer and a three-dimensional ultrasonic anemometer. The chemical composition of the fogwater was determined from samples collected with a modified Caltech active strand collector. The deposition of nutrients by fog (occult deposition) was calculated by multiplying the total fogwater <span class="hlt">flux</span> (total of measured <span class="hlt">turbulent</span> and calculated gravitational <span class="hlt">flux</span>) during each fog event by the ionic concentrations found in the collected fogwater. Several uncertainties still exist as far as the accuracy of the measurements is con- cerned. Although there is no universal statistical approach for testing the quality of the liquid water <span class="hlt">flux</span> data directly, results of independent data quality checks of the two time series involved in the <span class="hlt">flux</span> computation and accordingly the two instruments (ultrasonic anemometer and the droplet spectrometer) are presented. Within the measurement period, over 80 fog events with a duration longer than 2.5 hours were analyzed. An enormous physical and chemical heterogeneity among these fog events was found. We assume that some of this heterogeneity is due to the fact that fog or cloud droplets are not conservative entities: the <span class="hlt">turbulent</span> <span class="hlt">flux</span> of fog droplets, which can be referred to as the liquid water <span class="hlt">flux</span>, is affected by phase change processes and coagulation. The measured coexistence of upward <span class="hlt">fluxes</span> of small fog droplets (di- ameter < 10 µm) with the downward transport of larger droplets indicates the influ- ence of such processes. With the</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('https://ntrs.nasa.gov/search.jsp?R=19910061297&hterms=Magnetic+Flux&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3DMagnetic%2BFlux','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19910061297&hterms=Magnetic+Flux&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3DMagnetic%2BFlux"><span>On <span class="hlt">turbulent</span> diffusion of magnetic fields and the loss of magnetic <span class="hlt">flux</span> from stars</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Vainshtein, Samuel I.; Rosner, Robert</p> <p>1991-01-01</p> <p>The <span class="hlt">turbulent</span> diffusion of magnetic fields in astrophysical objects, and the processes leading to magnetic field <span class="hlt">flux</span> loss from such objects are discussed with attention to the suppression of <span class="hlt">turbulent</span> diffusion by back-reaction of magnetic fields on small spatial scales, and on the constraint imposed on magnetic <span class="hlt">flux</span> loss by <span class="hlt">flux</span>-freezing within stars. <span class="hlt">Turbulent</span> magnetic diffusion can be suppressed even for very weak large-scale magnetic fields, so that 'standard' <span class="hlt">turbulent</span> diffusion is incapable of significant magnetic <span class="hlt">flux</span> destruction within a star. Finally, magnetic <span class="hlt">flux</span> loss via winds is shown to be generally ineffective, no matter what the value of the effective magnetic Reynolds number is.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29195177','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29195177"><span>Mean and <span class="hlt">turbulent</span> mass <span class="hlt">flux</span> measurements in an idealised street network.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Carpentieri, Matteo; Robins, Alan G; Hayden, Paul; Santi, Edoardo</p> <p>2018-03-01</p> <p>Pollutant mass <span class="hlt">fluxes</span> are rarely measured in the laboratory, especially their <span class="hlt">turbulent</span> component. They play a major role in the dispersion of gases in urban areas and modern mathematical models often attempt some sort of parametrisation. An experimental technique to measure mean and <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> in an idealised urban array was developed and applied to improve our understanding of how the <span class="hlt">fluxes</span> are distributed in a dense street canyon network. As expected, horizontal advective scalar <span class="hlt">fluxes</span> were found to be dominant compared with the <span class="hlt">turbulent</span> components. This is an important result because it reduces the complexity in developing parametrisations for street network models. On the other hand, vertical mean and <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> appear to be approximately of the same order of magnitude. Building height variability does not appear to affect the exchange process significantly, while the presence of isolated taller buildings upwind of the area of interest does. One of the most interesting results, again, is the fact that even very simple and regular geometries lead to complex advective patterns at intersections: parametrisations derived from measurements in simpler geometries are unlikely to capture the full complexity of a real urban area. Copyright © 2017 Elsevier Ltd. All rights reserved.</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/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 <span class="hlt">turbulent</span> <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('http://adsabs.harvard.edu/abs/2005APS..DPPRP1084C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005APS..DPPRP1084C"><span>Suppression of <span class="hlt">turbulent</span> particle <span class="hlt">flux</span> during biased rotation in LAPD</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carter, T. A.</p> <p>2005-10-01</p> <p>The edge plasma in LAPD is rotated through the application of a bias voltage (typically 100V-200V) between the plasma source cathode and the vacuum vessel wall. Without bias, cross-field <span class="hlt">turbulent</span> particle transport causes the density profile to extend well past the cathode edge, with a fairly gentle gradient (Ln˜10 cm). As the bias voltage is applied and increased past a threshold value, the measured density profile steepens dramatically (Ln˜2 cm) at a radius near the peak of the flow shear. <span class="hlt">Turbulent</span> transport <span class="hlt">flux</span> measurements in this region show that the <span class="hlt">flux</span> is reduced and then suppressed completely as the threshold is approached. As the bias voltage is increased further, the measured <span class="hlt">turbulent</span> transport <span class="hlt">flux</span> reverses direction. The amplitude of the density and azimuthal electric field fluctuations is observed to decrease during biased rotation, the product of the amplitudes decreasing by a factor of 5. However the dominant change appears in the cross-phase, which is altered dramatically, leading to the observed suppression and reversal of the <span class="hlt">turbulent</span> <span class="hlt">flux</span>. Detailed two-dimensional <span class="hlt">turbulent</span> correlation measurements have been performed using the high repetition rate (1 Hz) and high reproducibility of LAPD plasmas. In unbiased plasmas, the correlation is localized to around 5 cm radially and a slightly smaller distance azimuthally (ρs˜0.5-1 cm). During biased rotation, a dramatic increase in the azimuthal correlation is observed, however there is little change in the radial correlation length.</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/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. <span class="hlt">Turbulence</span> 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_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/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 <span class="hlt">turbulent</span> 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 <span class="hlt">turbulence</span> 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('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 <span class="hlt">turbulent</span> 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/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/2018ACP....18.6001G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ACP....18.6001G"><span>The effects of <span class="hlt">sea</span> spray and atmosphere-wave coupling on <span class="hlt">air-sea</span> exchange during a tropical cyclone</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Garg, Nikhil; Kwee Ng, Eddie Yin; Narasimalu, Srikanth</p> <p>2018-04-01</p> <p>The study investigates the role of the <span class="hlt">air-sea</span> interface using numerical simulations of Hurricane Arthur (2014) in the Atlantic. More specifically, the present study aims to discern the role ocean surface waves and <span class="hlt">sea</span> spray play in modulating the intensity and structure of a tropical cyclone (TC). To investigate the effects of ocean surface waves and <span class="hlt">sea</span> spray, numerical simulations were carried out using a coupled atmosphere-wave model, whereby a <span class="hlt">sea</span> spray microphysical model was incorporated within the coupled model. Furthermore, this study also explores how <span class="hlt">sea</span> spray generation can be modelled using wave energy dissipation due to whitecaps; whitecaps are considered as the primary mode of spray droplets generation at hurricane intensity wind speeds. Three different numerical simulations including the <span class="hlt">sea</span>- state-dependent momentum <span class="hlt">flux</span>, the <span class="hlt">sea</span>-spray-mediated heat <span class="hlt">flux</span>, and a combination of the former two processes with the <span class="hlt">sea</span>-spray-mediated momentum <span class="hlt">flux</span> were conducted. The foregoing numerical simulations were evaluated against the National Data Buoy Center (NDBC) buoy and satellite altimeter measurements as well as a control simulation using an uncoupled atmosphere model. The results indicate that the model simulations were able to capture the storm track and intensity: the surface wave coupling results in a stronger TC. Moreover, it is also noted that when only spray-mediated heat <span class="hlt">fluxes</span> are applied in conjunction with the <span class="hlt">sea</span>-state-dependent momentum <span class="hlt">flux</span>, they result in a slightly weaker TC, albeit stronger compared to the control simulation. However, when a spray-mediated momentum <span class="hlt">flux</span> is applied together with spray heat <span class="hlt">fluxes</span>, it results in a comparably stronger TC. The results presented here allude to the role surface friction plays in the intensification of a TC.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017BoLMe.165..497P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017BoLMe.165..497P"><span>Influence of Evaporating Droplets in the <span class="hlt">Turbulent</span> Marine Atmospheric Boundary Layer</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Peng, Tianze; Richter, David</p> <p>2017-12-01</p> <p><span class="hlt">Sea</span>-spray droplets ejected into the marine atmospheric boundary layer take part in a series of complex transport processes. By capturing the <span class="hlt">air</span>-droplet coupling and feedback, we focus on how droplets modify the total heat transfer across a <span class="hlt">turbulent</span> boundary layer. We implement a high-resolution Eulerian-Lagrangian algorithm with varied droplet size and mass loading in a <span class="hlt">turbulent</span> open-channel flow, revealing that the influence from evaporating droplets varies for different dynamic and thermodynamic characteristics of droplets. Droplets that both respond rapidly to the ambient environment and have long suspension times are able to modify the latent and sensible heat <span class="hlt">fluxes</span> individually, however the competing signs of this modification lead to an overall weak effect on the total heat <span class="hlt">flux</span>. On the other hand, droplets with a slower thermodynamic response to the environment are less subjected to this compensating effect. This indicates a potential to enhance the total heat <span class="hlt">flux</span>, but the enhancement is highly dependent on the concentration and suspension time.</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/2017SCPMA..60l4711H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017SCPMA..60l4711H"><span>β-distribution for Reynolds stress and <span class="hlt">turbulent</span> heat <span class="hlt">flux</span> in relaxation <span class="hlt">turbulent</span> boundary layer of compression ramp</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hu, YanChao; Bi, WeiTao; Li, ShiYao; She, ZhenSu</p> <p>2017-12-01</p> <p>A challenge in the study of <span class="hlt">turbulent</span> boundary layers (TBLs) is to understand the non-equilibrium relaxation process after sep-aration and reattachment due to shock-wave/boundary-layer interaction. The classical boundary layer theory cannot deal with the strong adverse pressure gradient, and hence, the computational modeling of this process remains inaccurate. Here, we report the direct numerical simulation results of the relaxation TBL behind a compression ramp, which reveal the presence of intense large-scale eddies, with significantly enhanced Reynolds stress and <span class="hlt">turbulent</span> heat <span class="hlt">flux</span>. A crucial finding is that the wall-normal profiles of the excess Reynolds stress and <span class="hlt">turbulent</span> heat <span class="hlt">flux</span> obey a β-distribution, which is a product of two power laws with respect to the wall-normal distances from the wall and from the boundary layer edge. In addition, the streamwise decays of the excess Reynolds stress and <span class="hlt">turbulent</span> heat <span class="hlt">flux</span> also exhibit power laws with respect to the streamwise distance from the corner of the compression ramp. These results suggest that the relaxation TBL obeys the dilation symmetry, which is a specific form of self-organization in this complex non-equilibrium flow. The β-distribution yields important hints for the development of a <span class="hlt">turbulence</span> model.</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> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19940018829','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19940018829"><span>A representation for the <span class="hlt">turbulent</span> mass <span class="hlt">flux</span> contribution to Reynolds-stress and two-equation closures for compressible <span class="hlt">turbulence</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ristorcelli, J. R.</p> <p>1993-01-01</p> <p>The <span class="hlt">turbulent</span> mass <span class="hlt">flux</span>, or equivalently the fluctuating Favre velocity mean, appears in the first and second moment equations of compressible kappa-epsilon and Reynolds stress closures. Mathematically it is the difference between the unweighted and density-weighted averages of the velocity field and is therefore a measure of the effects of compressibility through variations in density. It appears to be fundamental to an inhomogeneous compressible <span class="hlt">turbulence</span>, in which it characterizes the effects of the mean density gradients, in the same way the anisotropy tensor characterizes the effects of the mean velocity gradients. An evolution equation for the <span class="hlt">turbulent</span> mass <span class="hlt">flux</span> is derived. A truncation of this equation produces an algebraic expression for the mass <span class="hlt">flux</span>. The mass <span class="hlt">flux</span> is found to be proportional to the mean density gradients with a tensor eddy-viscosity that depends on both the mean deformation and the Reynolds stresses. The model is tested in a wall bounded DNS at Mach 4.5 with notable results.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JGRC..120.2308C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JGRC..120.2308C"><span><span class="hlt">Turbulent</span> nitrate <span class="hlt">fluxes</span> in the Lower St. Lawrence Estuary, Canada</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cyr, Frédéric; Bourgault, Daniel; Galbraith, Peter S.; Gosselin, Michel</p> <p>2015-03-01</p> <p><span class="hlt">Turbulent</span> vertical nitrate <span class="hlt">fluxes</span> were calculated using new <span class="hlt">turbulent</span> microstructure observations in the Lower St. Lawrence Estuary (LSLE), Canada. Two stations were compared: the head of the Laurentian Channel (HLC), where intense mixing occurs on the shallow sill that marks the upstream limit of the LSLE, and another station located about 100 km downstream (St. 23), more representative of the LSLE mean mixing conditions. Mean <span class="hlt">turbulent</span> diffusivities and nitrate <span class="hlt">fluxes</span> at the base of the surface layer for both stations were, respectively (with 95% confidence intervals): K¯HLC = 8.6>(3.2,19>) × 10-3 m2 s-1,K¯23 = 4.4>(2.3,7.6>) × 10-5 m2 s-1,F¯HLC = 95>(18,300>) mmol m-2 d-1, and F¯23 = 0.21>(0.12,0.33>) mmol m-2 d-1. Observations suggest that the interplay between large isopleth heaving near the sill and strong <span class="hlt">turbulence</span> is the key mechanism to sustain such high <span class="hlt">turbulent</span> nitrate <span class="hlt">fluxes</span> at the HLC (two to three orders of magnitude higher than those at Station 23). Calculations also suggest that nitrate <span class="hlt">fluxes</span> at the HLC alone can sustain primary production rates of 3.4>(0.6,11>) g C m-2 mo-1 over the whole LSLE, approximately enough to account for a large part of the phytoplankton bloom and for most of the postbloom production. Surfacing nitrates are also believed to be consumed within the LSLE, not leaving much to be exported to the rest of the Gulf of St. Lawrence. This article was corrected on 13 APR 2015. See the end of the full text for details.</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 <span class="hlt">turbulent</span> <span class="hlt">flux</span> divergence.</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('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 <span class="hlt">turbulent</span> mixing. The depth reached by this <span class="hlt">turbulent</span> 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('https://www.ncbi.nlm.nih.gov/pubmed/27617333','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27617333"><span>Persistent organochlorine pesticides and polychlorinated biphenyls in <span class="hlt">air</span> of the North <span class="hlt">Sea</span> region and <span class="hlt">air-sea</span> exchange.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mai, Carolin; Theobald, Norbert; Hühnerfuss, Heinrich; Lammel, Gerhard</p> <p>2016-12-01</p> <p>Organochlorine pesticides (OCPs) and polychlorinated biphenyls (PCBs) were studied to determine occurrence, levels and spatial distribution in the marine atmosphere and surface seawater during cruises in the German Bight and the wider North <span class="hlt">Sea</span> in spring and summer 2009-2010. In general, the concentrations found in <span class="hlt">air</span> are similar to, or below, the levels at coastal or near-coastal sites in Europe. Hexachlorobenzene and α-hexachlorocyclohexane (α-HCH) were close to phase equilibrium, whereas net atmospheric deposition was observed for γ-HCH. The results suggest that declining trends of HCH in seawater have been continuing for γ-HCH but have somewhat levelled off for α-HCH. Dieldrin displayed a close to phase equilibrium in nearly all the sampling sites, except in the central southwestern part of the North <span class="hlt">Sea</span>. Here atmospheric deposition dominates the <span class="hlt">air-sea</span> exchange. This region, close to the English coast, showed remarkably increased surface seawater concentrations. This observation depended neither on riverine input nor on the elevated abundances of dieldrin in the <span class="hlt">air</span> masses of central England. A net depositional <span class="hlt">flux</span> of p,p'-DDE into the North <span class="hlt">Sea</span> was indicated by both its abundance in the marine atmosphere and the changes in metabolite pattern observed in the surface water from the coast towards the open <span class="hlt">sea</span>. The long-term trends show that the atmospheric concentrations of DDT and its metabolites are not declining. Riverine input is a major source of PCBs in the German Bight and the wider North <span class="hlt">Sea</span>. Atmospheric deposition of the lower molecular weight PCBs (PCB28 and PCB52) was indicated as a major source for surface seawater pollution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A52C..06M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A52C..06M"><span>Modeling Transport of <span class="hlt">Turbulent</span> <span class="hlt">Fluxes</span> in a Heterogeneous Urban Canopy Using a Spatially Explicit Energy Balance</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moody, M.; Bailey, B.; Stoll, R., II</p> <p>2017-12-01</p> <p>Understanding how changes in the microclimate near individual plants affects the surface energy budget is integral to modeling land-atmosphere interactions and a wide range of near surface atmospheric boundary layer phenomena. In urban areas, the complex geometry of the urban canopy layer results in large spatial deviations of <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> further complicating the development of models. Accurately accounting for this heterogeneity in order to model urban energy and water use requires a sub-plant level understanding of microclimate variables. We present analysis of new experimental field data taken in and around two Blue Spruce (Picea pungens) trees at the University of Utah in 2015. The test sites were chosen in order study the effects of heterogeneity in an urban environment. An array of sensors were placed in and around the conifers to quantify transport in the soil-plant-atmosphere continuum: radiative <span class="hlt">fluxes</span>, temperature, sap <span class="hlt">fluxes</span>, etc. A spatial array of LEMS (Local Energy Measurement Systems) were deployed to obtain pressure, surrounding <span class="hlt">air</span> temperature and relative humidity. These quantities are used to calculate the radiative and <span class="hlt">turbulent</span> <span class="hlt">fluxes</span>. Relying on measurements alone is insufficient to capture the complexity of microclimate distribution as one reaches sub-plant scales. A spatially-explicit radiation and energy balance model previously developed for deciduous trees was extended to include conifers. The model discretizes the tree into isothermal sub-volumes on which energy balances are performed and utilizes incoming radiation as the primary forcing input. The radiative transfer component of the model yields good agreement between measured and modeled upward longwave and shortwave radiative <span class="hlt">fluxes</span>. Ultimately, the model was validated through an examination of the full energy budget including radiative and <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> through isolated Picea pungens in an urban environment.</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 <span class="hlt">Turbulent</span> <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> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li class="active"><span>9</span></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_9 --> <div id="page_10" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li class="active"><span>10</span></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="181"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.8859G','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 <span class="hlt">turbulent</span> parameters. Over a hundred cases of <span class="hlt">sea</span> breezes, fog periods, stormy days and atmospheric front passages were investigated. Variations of <span class="hlt">turbulent</span> 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('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/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 <span class="hlt">turbulent</span> 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 <span class="hlt">turbulent</span> 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/2006AGUFMOS41A0583L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFMOS41A0583L"><span>The Dependence of Heat and Gas Transfer Velocities on Wind-Generated and Mechanically Generated Aqueous-Phase <span class="hlt">Turbulence</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liang, H.; Mukto, M.; Loewen, M.; Zappa, C.; Litchendorf, T.; Asher, W.; Jessup, A.</p> <p>2006-12-01</p> <p>The <span class="hlt">air-sea</span> <span class="hlt">flux</span>, F, of a sparingly soluble nonreactive gas can be expressed as F = kG( CS-CW), where kG is the gas transfer velocity, CS is the concentration of gas that would be expected in the water if the system were in Henry`s Gas Law equilibrium, and CW is the actual concentration of the gas in the water. An analogous relationship for the net heat <span class="hlt">flux</span> can also be written using the heat transfer velocity, kH, and the bulk-skin temperature difference in the aqueous phase. Hydrodynamical models of gas and heat exchange based on surface renewal theory predict that kG and kH will scale as the square root of the inverse of a timescale of the <span class="hlt">turbulence</span>. Furthermore, if surface renewal provides an accurate conceptual model for both transfer processes, then both kG and kH should behave identically as <span class="hlt">turbulence</span> conditions change. Here we report on recent laboratory experiments in which we measured <span class="hlt">turbulence</span>, heat <span class="hlt">fluxes</span>, kG, and kH in a 0.5 m by 0.5 m by 1 m deep tank in the presence of <span class="hlt">turbulence</span> generated mechanically using a random synthetic jet array. The <span class="hlt">turbulence</span> tank was embedded in a small wind tunnel so that kG and kH could be studied as a function of the mechanically generated <span class="hlt">turbulence</span> but also <span class="hlt">turbulence</span> generated by wind stress. Net heat transfer velocities were measured using Active Controlled <span class="hlt">Flux</span> Technique and estimated from measurements of the latent and sensible heat <span class="hlt">fluxes</span> combined with direct measurements of the bulk-skin temperature difference. Gas transfer velocities were determined by measuring the evasion rates of sulfur hexafluoride and helium. The length and velocity scales of the aqueous-phase <span class="hlt">turbulence</span> were measured using a Digital Particle-Image Velocimetry system. These combined data sets are used to study how kG and kH depend on system <span class="hlt">turbulence</span>, whether this dependence is consonant with that predicted using surface renewal, and whether there is a quantitative difference between mechanically generated <span class="hlt">turbulence</span> and <span class="hlt">turbulence</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20110011454&hterms=Koch&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DKoch','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20110011454&hterms=Koch&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DKoch"><span>Can CO2 <span class="hlt">Turbulent</span> <span class="hlt">Flux</span> Be Measured by Lidar? A Preliminary Study</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gilbert, Fabien; Koch, Grady; Beyon, Jeffrey Y.; Hilton, Timothy W.; Davis, Kenneth J.; Andrews, Arlyn; Flamant, Pierre H.; Singh, Upendra N.</p> <p>2011-01-01</p> <p>The vertical profiling ofCO2 <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> in the atmospheric boundary layer (ABL) is investigated using a coherent differential absorption lidar (CDIAL) operated nearby a tall tower in Wisconsin during June 2007. A CDIAL can perform simultaneous range-resolved CO2 DIAL and velocity measurements. The lidar eddy covariance technique is presented. The aims of the study are (i) an assessment of performance and current limitation of available CDIAL for CO2 <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> and (ii) the derivation of instrument specifications to build a future CDIAL to perform accurate range-resolved CO2 <span class="hlt">fluxes</span>. Experimental lidar CO2 mixing ratio and vertical velocity profiles are successfully compared with in situ sensors measurements. Time and space integral scales of <span class="hlt">turbulence</span> in the ABL are addressed that result in limitation for time averaging and range accumulation. A first attempt to infer CO2 <span class="hlt">fluxes</span> using an eddy covariance technique with currently available 2-mm CDIAL dataset is reported.</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/2015PhPl...22d2516M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PhPl...22d2516M"><span><span class="hlt">Turbulent</span> transport regimes and the scrape-off layer heat <span class="hlt">flux</span> width</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Myra, J. R.; D'Ippolito, D. A.; Russell, D. A.</p> <p>2015-04-01</p> <p>Understanding the responsible mechanisms and resulting scaling of the scrape-off layer (SOL) heat <span class="hlt">flux</span> width is important for predicting viable operating regimes in future tokamaks and for seeking possible mitigation schemes. In this paper, we present a qualitative and conceptual framework for understanding various regimes of edge/SOL <span class="hlt">turbulence</span> and the role of <span class="hlt">turbulent</span> transport as the mechanism for establishing the SOL heat <span class="hlt">flux</span> width. Relevant considerations include the type and spectral characteristics of underlying instabilities, the location of the gradient drive relative to the SOL, the nonlinear saturation mechanism, and the parallel heat transport regime. We find a heat <span class="hlt">flux</span> width scaling with major radius R that is generally positive, consistent with the previous findings [Connor et al., Nucl. Fusion 39, 169 (1999)]. The possible relationship of <span class="hlt">turbulence</span> mechanisms to the neoclassical orbit width or heuristic drift mechanism in core energy confinement regimes known as low (L) mode and high (H) mode is considered, together with implications for the future experiments.</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 <span class="hlt">turbulent</span> 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/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('https://www.osti.gov/biblio/6357383-anomalous-fluxes-plateau-regime-weakly-turbulent-magnetically-confined-plasma','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6357383-anomalous-fluxes-plateau-regime-weakly-turbulent-magnetically-confined-plasma"><span>Anomalous <span class="hlt">fluxes</span> in the plateau regime for a weakly <span class="hlt">turbulent</span>, magnetically confined plasma</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>Balescu, R.</p> <p>1990-09-01</p> <p>The anomalous particle and heat <span class="hlt">fluxes</span>, together with the parallel electric current, are determined for a confined plasma in the plateau regime in the presence of weak electrostatic drift-wave <span class="hlt">turbulence</span>. Proper account is taken of nonstationarity and of the finite ion Larmor radius (FLR). The quasineutrality of the drift-wave fluctuations imposes a consistency condition, by which the evaluation of the anomalous <span class="hlt">fluxes</span> is closely related to the drift-wave dispersion equation. On the other hand, these <span class="hlt">fluxes</span> are related to the thermodynamic forces via the poloidal <span class="hlt">fluxes</span>. For the weak <span class="hlt">turbulence</span> approximation considered here, a unified formulation of the anomalous transportmore » problem has been obtained, including all aspects of neoclassical theory. The complete set of transport coefficients is calculated and various relations between them are exhibited. It clearly appears, for instance, that the anomalous ion heat <span class="hlt">flux</span> is a pure FLR effect that vanishes as the Larmor radius goes to zero. The Onsager symmetry is broken for anomalous transport. The Appendix is devoted to a general discussion of the concept of heat <span class="hlt">flux</span> in <span class="hlt">turbulent</span> plasmas.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C23B0796T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C23B0796T"><span>Theoretical Studies of <span class="hlt">Turbulent</span> Transport Processes at Rough Boundaries with Application to the Interface Between <span class="hlt">Sea</span> Ice and the Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Toppaladoddi, S.; Succi, S.; Wettlaufer, J. S.</p> <p>2015-12-01</p> <p>We study the effects of rough walls on <span class="hlt">turbulent</span> flows to understand the coupling between the rough underside of Arctic <span class="hlt">sea</span> ice and the ocean. Of particular relevance is the fact that the climatological thickness of Arctic <span class="hlt">sea</span> ice is a sensitive function of the <span class="hlt">turbulent</span> ice/ocean heat <span class="hlt">flux</span>, which depends sensitively on the roughness of the phase boundary. We tailor the geometry of the upper boundary to manipulate the boundary layer - interior flow interaction and study the <span class="hlt">turbulent</span> transport of heat in two-dimensional Rayleigh-Bénard convection with numerical simulations using the Lattice Boltzmann method. By fixing the roughness amplitude of the upper boundary and varying the wavelength λλ, we find that the exponent ββ in the Nusselt-Rayleigh scaling relation, Nu-1∝RaβNu-1 ∝ Ra^β, is maximized at λ≡λmax≈(2π)-1λ ≡ λ_{max} ≈ (2 π)^{-1}, but decays to the planar value in both the large (λ≫λmaxλ ≫ λ_{max}) and small (λ≪λmaxλ ≪ λ_{max}) wavelength limits. The changes in the exponent originate in the nature of the coupling between the boundary layer and the interior flow. We present a simple scaling argument embodying this coupling, which describes the maximal convective heat <span class="hlt">flux</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFMSH14B..02E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMSH14B..02E"><span>Stochastic <span class="hlt">Flux</span>-Freezing in MHD <span class="hlt">Turbulence</span> and Reconnection in the Heliosheath</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Eyink, G. L.; Lalescu, C.; Vishniac, E.</p> <p>2012-12-01</p> <p>Fast reconnection of the sectored magnetic field in the heliosheath created by flapping of the heliospheric current sheet has been conjectured to accelerate anomalous cosmic rays and to create other signatures observed by the Voyager probes. The reconnecting <span class="hlt">flux</span> structures could have sizes up to ˜100 AU, much larger than the ion cyclotron radius ˜10^3 km. Hence MHD should be valid at those scales. To account for rapid reconnection of such large-scale structures, we note that the high Reynolds numbers in the heliosheath for motions perpendicular to the magnetic field (Re ˜10^{14}) suggest transition to <span class="hlt">turbulence</span>. The Lazarian-Vishnian theory of <span class="hlt">turbulent</span> reconnection can account for the fast rates, but it implies a puzzling breakdown of magnetic <span class="hlt">flux</span>-freezing in high-conductivity MHD plasmas. We address this paradox with a novel stochastic formulation of <span class="hlt">flux</span>-freezing for resistive MHD and a numerical Lagrangian study with a spacetime database of MHD <span class="hlt">turbulence</span>. We report the first observation of Richardson diffusion in MHD <span class="hlt">turbulence</span>, which leads to "spontaneous stochasticity" of the Lagrangian trajectories and a violation of standard <span class="hlt">flux</span>-freezing by many orders of magnitude. The work supports a prediction by Lazarian-Opher (2009) of extended thick reconnection zones within the heliosheath, perhaps up to an AU across, although the microscale reconnection events within these zones would have thickness of order the ion cyclotron radius and be described by kinetic Vlasov theory.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3352249','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3352249"><span>Wind Tunnel Measurement of <span class="hlt">Turbulent</span> and Advective Scalar <span class="hlt">Fluxes</span>: A Case Study on Intersection Ventilation</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Kukačka, Libor; Nosek, Štĕpán; Kellnerová, Radka; Jurčáková, Klára; Jaňour, Zbyněk</p> <p>2012-01-01</p> <p>The objective of this study is to determine processes of pollution ventilation in the X-shaped street intersection in an idealized symmetric urban area for the changing approach flow direction. A unique experimental setup for simultaneous wind tunnel measurement of the flow velocity and the tracer gas concentration in a high temporal resolution is assembled. Advective horizontal and vertical scalar <span class="hlt">fluxes</span> are computed from averaged measured velocity and concentration data within the street intersection. Vertical advective and <span class="hlt">turbulent</span> scalar <span class="hlt">fluxes</span> are computed from synchronized velocity and concentration signals measured in the plane above the intersection. All the results are obtained for five approach flow directions. The influence of the approach flow on the advective and <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> is determined. The contribution of the advective and <span class="hlt">turbulent</span> <span class="hlt">flux</span> to the ventilation is discussed. Wind direction with the best dispersive conditions in the area is found. The quadrant analysis is applied to the synchronized signals of velocity and concentration fluctuation to determine events with the dominant contribution to the momentum <span class="hlt">flux</span> and <span class="hlt">turbulent</span> scalar <span class="hlt">flux</span>. PMID:22649290</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22649290','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22649290"><span>Wind tunnel measurement of <span class="hlt">turbulent</span> and advective scalar <span class="hlt">fluxes</span>: a case study on intersection ventilation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kukačka, Libor; Nosek, Štĕpán; Kellnerová, Radka; Jurčáková, Klára; Jaňour, Zbyněk</p> <p>2012-01-01</p> <p>The objective of this study is to determine processes of pollution ventilation in the X-shaped street intersection in an idealized symmetric urban area for the changing approach flow direction. A unique experimental setup for simultaneous wind tunnel measurement of the flow velocity and the tracer gas concentration in a high temporal resolution is assembled. Advective horizontal and vertical scalar <span class="hlt">fluxes</span> are computed from averaged measured velocity and concentration data within the street intersection. Vertical advective and <span class="hlt">turbulent</span> scalar <span class="hlt">fluxes</span> are computed from synchronized velocity and concentration signals measured in the plane above the intersection. All the results are obtained for five approach flow directions. The influence of the approach flow on the advective and <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> is determined. The contribution of the advective and <span class="hlt">turbulent</span> <span class="hlt">flux</span> to the ventilation is discussed. Wind direction with the best dispersive conditions in the area is found. The quadrant analysis is applied to the synchronized signals of velocity and concentration fluctuation to determine events with the dominant contribution to the momentum <span class="hlt">flux</span> and <span class="hlt">turbulent</span> scalar <span class="hlt">flux</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JTurb..18.1033L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JTurb..18.1033L"><span><span class="hlt">Turbulent</span> scalar <span class="hlt">flux</span> transport in head-on quenching of <span class="hlt">turbulent</span> premixed flames: a direct numerical simulations approach to assess models for Reynolds averaged Navier Stokes simulations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lai, Jiawei; Alwazzan, Dana; Chakraborty, Nilanjan</p> <p>2017-11-01</p> <p>The statistical behaviour and the modelling of <span class="hlt">turbulent</span> scalar <span class="hlt">flux</span> transport have been analysed using a direct numerical simulation (DNS) database of head-on quenching of statistically planar <span class="hlt">turbulent</span> premixed flames by an isothermal wall. A range of different values of Damköhler, Karlovitz numbers and Lewis numbers has been considered for this analysis. The magnitudes of the <span class="hlt">turbulent</span> transport and mean velocity gradient terms in the <span class="hlt">turbulent</span> scalar <span class="hlt">flux</span> transport equation remain small in comparison to the pressure gradient, molecular dissipation and reaction-velocity fluctuation correlation terms in the <span class="hlt">turbulent</span> scalar <span class="hlt">flux</span> transport equation when the flame is away from the wall but the magnitudes of all these terms diminish and assume comparable values during flame quenching before vanishing altogether. It has been found that the existing models for the <span class="hlt">turbulent</span> transport, pressure gradient, molecular dissipation and reaction-velocity fluctuation correlation terms in the <span class="hlt">turbulent</span> scalar <span class="hlt">flux</span> transport equation do not adequately address the respective behaviours extracted from DNS data in the near-wall region during flame quenching. Existing models for transport equation-based closures of <span class="hlt">turbulent</span> scalar <span class="hlt">flux</span> have been modified in such a manner that these models provide satisfactory prediction both near to and away from the wall.</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 <span class="hlt">turbulence</span>. The stochastic forcing enters multiplicatively in this theory and produces an exponential wave growth, augmenting the growth from the Miles (1959) theory as the <span class="hlt">turbulence</span> level increases. Here we complement this concept by adding the effect of the two-phase environment near the mean interface, which introduces additional viscosity in the system (turning it into a rheological system). The two-phase environment includes <span class="hlt">air</span>-bubbles and re-entering spray (spume), which eliminates a portion of the wind-wave wavenumber spectrum that is responsible for a substantial part of the <span class="hlt">air</span> <span class="hlt">sea</span> drag coefficient. The previously developed KH-type interfacial parameterization (Soloviev and Lukas 2010) is unified with two versions of the wave growth model. The unified parameterization in both cases exhibits the increase of the drag coefficient with wind speed until approximately 30 m/s. Above this wind speed threshold, the drag coefficient either nearly levels off or even slightly drops (for the wave growth model that accounts for the shear) and then starts again increasing above approximately 65 m/s wind speed. Remarkably, the unified parameterization reveals a local minimum</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA591722','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA591722"><span>Impact of Typhoons on the Western Pacific Ocean (ITOP) DRI:Numerical Modeling of Ocean Mixed Layer <span class="hlt">Turbulence</span> and Entrainment at High Winds</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2013-09-23</p> <p>DISTRIBUTION STATEMENT A. Approved for public release; distribution is unlimited. Impact of Typhoons on the Western Pacific Ocean (ITOP) DRI...measurement and modeling activities include a focus on the impact of surface waves, <span class="hlt">air</span>- <span class="hlt">sea</span> <span class="hlt">fluxes</span> and the temperature, salinity and velocity structure...moment closure (SMC) to represent the impact of Langmuir <span class="hlt">turbulence</span>. WORK COMPLETED Encouraged by good quantitative comparisons between LES</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRD..123..649F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRD..123..649F"><span>Gravity Wave Dynamics in a Mesospheric Inversion Layer: 2. Instabilities, <span class="hlt">Turbulence</span>, <span class="hlt">Fluxes</span>, and Mixing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fritts, David C.; Wang, Ling; Laughman, Brian; Lund, Thomas S.; Collins, Richard L.</p> <p>2018-01-01</p> <p>A companion paper by Fritts, Laughman, et al. (2017) employed an anelastic numerical model to explore the dynamics of gravity waves (GWs) encountering a mesospheric inversion layer (MIL) having a moderate static stability enhancement and a layer of weaker static stability above. That study revealed that MIL responses, including GW transmission, reflection, and instabilities, are sensitive functions of GW parameters. This paper expands on two of the Fritts, Laughman, et al. (2017) simulations to examine GW instability dynamics and <span class="hlt">turbulence</span> in the MIL; forcing of the mean wind and stability environments by GW, instability, and <span class="hlt">turbulence</span> <span class="hlt">fluxes</span>; and associated heat and momentum transports. These direct numerical simulations resolve <span class="hlt">turbulence</span> inertial-range scales and yield the following results: GW breaking and <span class="hlt">turbulence</span> in the MIL occur below where they would otherwise, due to enhancements of GW amplitudes and shears in the MIL. 2-D GW and instability heat and momentum <span class="hlt">fluxes</span> are 20-30 times larger than 3-D instability and <span class="hlt">turbulence</span> <span class="hlt">fluxes</span>. Mean fields are driven largely by 2-D GW and instability dynamics rather than 3-D instabilities and <span class="hlt">turbulence</span>. 2-D and 3-D heat <span class="hlt">fluxes</span> in regions of strong <span class="hlt">turbulence</span> yield small departures from initial <fi>T</fi>(<fi>z</fi>) and <fi>N</fi>2(<fi>z</fi>) profiles, hence do not yield nearly adiabatic "mixed" layers. Our MIL results are consistent with the relation between the <span class="hlt">turbulent</span> vertical velocity variance and energy dissipation rate proposed by Weinstock (1981) for the limited intervals evaluated.</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> </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/2015EGUGA..1713084S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1713084S"><span><span class="hlt">Turbulent</span> <span class="hlt">fluxes</span> by "Conditional Eddy Sampling"</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Siebicke, Lukas</p> <p>2015-04-01</p> <p><span class="hlt">Turbulent</span> <span class="hlt">flux</span> measurements are key to understanding ecosystem scale energy and matter exchange, including atmospheric trace gases. While the eddy covariance approach has evolved as an invaluable tool to quantify <span class="hlt">fluxes</span> of e.g. CO2 and H2O continuously, it is limited to very few atmospheric constituents for which sufficiently fast analyzers exist. High instrument cost, lack of field-readiness or high power consumption (e.g. many recent laser-based systems requiring strong vacuum) further impair application to other tracers. Alternative micrometeorological approaches such as conditional sampling might overcome major limitations. Although the idea of eddy accumulation has already been proposed by Desjardin in 1972 (Desjardin, 1977), at the time it could not be realized for trace gases. Major simplifications by Businger and Oncley (1990) lead to it's widespread application as 'Relaxed Eddy Accumulation' (REA). However, those simplifications (<span class="hlt">flux</span> gradient similarity with constant flow rate sampling irrespective of vertical wind velocity and introduction of a deadband around zero vertical wind velocity) have degraded eddy accumulation to an indirect method, introducing issues of scalar similarity and often lack of suitable scalar <span class="hlt">flux</span> proxies. Here we present a real implementation of a true eddy accumulation system according to the original concept. Key to our approach, which we call 'Conditional Eddy Sampling' (CES), is the mathematical formulation of conditional sampling in it's true form of a direct eddy <span class="hlt">flux</span> measurement paired with a performant real implementation. Dedicated hardware controlled by near-real-time software allows full signal recovery at 10 or 20 Hz, very fast valve switching, instant vertical wind velocity proportional flow rate control, virtually no deadband and adaptive power management. Demonstrated system performance often exceeds requirements for <span class="hlt">flux</span> measurements by orders of magnitude. The system's exceptionally low power consumption is ideal</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/2060/19910004469','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 <span class="hlt">turbulent</span> heat <span class="hlt">flux</span>; and (4) Surface temperature algorithm.</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/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 <span class="hlt">turbulent</span> <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://adsabs.harvard.edu/abs/2017APS..DFDL29008O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..DFDL29008O"><span>Measurement of <span class="hlt">Turbulent</span> <span class="hlt">Fluxes</span> of Swirling Flow in a Scaled Up Multi Inlet Vortex Reactor</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Olsen, Michael; Hitimana, Emmanual; Hill, James; Fox, Rodney</p> <p>2017-11-01</p> <p>The multi-inlet vortex reactor (MIVR) has been developed for use in the FlashNanoprecipitation (FNP) process. The MIVR has four identical square inlets connected to a central cylindrical mixing chamber with one common outlet creating a highly <span class="hlt">turbulent</span> swirling flow dominated by a strong vortex in the center. Efficient FNP requires rapid mixing within the MIVR. To investigate the mixing, instantaneous velocity and concentration fields were acquired using simultaneous stereoscopic particle image velocimetry and planar laser-induced fluorescence. The simultaneous velocity and concentration data were used to determine <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> and spatial cross-correlations of velocity and concentration fluctuations. The measurements were performed for four inlet flow Reynolds numbers (3250, 4875, 6500, and 8125) and at three measurement planes within the reactor. A correlation between <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> and vortex strength was found. For all Reynolds numbers, <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> are maximum in the vortex dominated central region of the reactor and decay away from the vortex. Increasing Reynolds number increased <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> and subsequently enhanced mixing. The mixing performance was confirmed by determining coefficients of concentration variance within the reactor.</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://adsabs.harvard.edu/abs/2012APS..DFDM22004K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012APS..DFDM22004K"><span>Local structure of scalar <span class="hlt">flux</span> in <span class="hlt">turbulent</span> passive scalar mixing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Konduri, Aditya; Donzis, Diego</p> <p>2012-11-01</p> <p>Understanding the properties of scalar <span class="hlt">flux</span> is important in the study of <span class="hlt">turbulent</span> mixing. Classical theories suggest that it mainly depends on the large scale structures in the flow. Recent studies suggest that the mean scalar <span class="hlt">flux</span> reaches an asymptotic value at high Peclet numbers, independent of molecular transport properties of the fluid. A large DNS database of isotropic <span class="hlt">turbulence</span> with passive scalars forced with a mean scalar gradient with resolution up to 40963, is used to explore the structure of scalar <span class="hlt">flux</span> based on the local topology of the flow. It is found that regions of small velocity gradients, where dissipation and enstrophy are small, constitute the main contribution to scalar <span class="hlt">flux</span>. On the other hand, regions of very small scalar gradient (and scalar dissipation) become less important to the scalar <span class="hlt">flux</span> at high Reynolds numbers. The scaling of the scalar <span class="hlt">flux</span> spectra is also investigated. The k - 7 / 3 scaling proposed by Lumley (1964) is observed at high Reynolds numbers, but collapse is not complete. A spectral bump similar to that in the velocity spectrum is observed close to dissipative scales. A number of features, including the height of the bump, appear to reach an asymptotic value at high Schmidt number.</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://www.dtic.mil/docs/citations/ADA599038','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA599038"><span>Impact of Typhoons on the Western Pacific Ocean (ITOP) DRI: Numerical Modeling of Ocean Mixed Layer <span class="hlt">Turbulence</span> and Entrainment at High Winds</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2013-09-30</p> <p>1 DISTRIBUTION STATEMENT A. Approved for public release; distribution is unlimited. Impact of Typhoons on the Western Pacific Ocean (ITOP...The measurement and modeling activities include a focus on the impact of surface waves, <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> and the temperature, salinity and velocity...SUBTITLE Impact of Typhoons on the Western Pacific Ocean (ITOP) DRI: Numerical Modeling of Ocean Mixed Layer <span class="hlt">Turbulence</span> and Entrainment at High Winds</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A43G2559J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A43G2559J"><span>Seasonal atmospheric deposition and <span class="hlt">air-sea</span> gaseous exchange of polycyclic aromatic hydrocarbons over the Yangtze River Estuary, East China <span class="hlt">Sea</span>: Implication for the source-sink processes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jiang, Y.; Guo, Z.</p> <p>2017-12-01</p> <p>As the home of the largest port in the world, the Yangtze River Estuary (YRE) in the East China <span class="hlt">Sea</span> (ECS) is adjacent to the largest economic zone in China with more than 10% of Chinese population and provides one-fifth of national GDP. The YRE is under the path of contaminated East Asian continental outflow. These make the YRE unique for the pollutant biogeochemical cycling in the world. In this work, 94 pairs of <span class="hlt">air</span> samples and 20 surface seawater samples covering four seasons were collected from a remote receptor site in the YRE from March 2014 to January 2015, in order to explore the seasonal <span class="hlt">fluxes</span> of <span class="hlt">air-sea</span> gaseous exchange and atmospheric dry and wet deposition of 15 polycyclic aromatic hydrocarbons (PAHs) and their source-sink processes at the <span class="hlt">air-sea</span> interface. The average dry and wet deposition <span class="hlt">fluxes</span> of 15 PAHs were estimated as 879 ± 1393 ng m-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/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 <span class="hlt">turbulent</span> 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/2013AGUFMSH54A..01E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMSH54A..01E"><span>Stochastic <span class="hlt">Flux</span>-Freezing in MHD <span class="hlt">Turbulence</span> and Reconnection in the Heliosheath (Invited)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Eyink, G. L.; Lalescu, C. C.; Vishniac, E. T.</p> <p>2013-12-01</p> <p>Fast reconnection of the sectored magnetic field in the heliosheath created by flapping of the heliospheric current sheet has been conjectured to accelerate anomalous cosmic rays and to create other signatures observed by the Voyager probes. The reconnecting <span class="hlt">flux</span> structures could have sizes up to ˜100 AU, much larger than the ion cyclotron radius ˜103 km. Hence MHD should be valid at those scales. To account for rapid reconnection of such large-scale structures, we note that the high Reynolds numbers in the heliosheath for motions perpendicular to the magnetic field (Re ˜1014) suggest transition to <span class="hlt">turbulence</span>. The Lazarian-Vishnian theory of <span class="hlt">turbulent</span> reconnection can account for the fast rates, but it implies a puzzling breakdown of magnetic <span class="hlt">flux</span>-freezing in high-conductivity MHD plasmas. We address this paradox with a novel stochastic formulation of <span class="hlt">flux</span>-freezing for resistive MHD and a numerical Lagrangian study with a spacetime database of MHD <span class="hlt">turbulence</span>. We report the first observation of Richardson diffusion in MHD <span class="hlt">turbulence</span>, which leads to 'spontaneous stochasticity' of the Lagrangian trajectories and a violation of standard <span class="hlt">flux</span>- freezing by many orders of magnitude. The work supports a prediction by Lazarian-Opher (2009) of extended thick reconnection zones within the heliosheath, perhaps up to an AU across, although the microscale reconnection events within these zones would have thickness of order the ion cyclotron radius and be described by kinetic Vlasov theory.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70026544','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70026544"><span>Airflows and <span class="hlt">turbulent</span> <span class="hlt">flux</span> measurements in mountainous terrain: Part 2: Mesoscale effects</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Turnipseed, A.A.; Anderson, D.E.; Burns, S.; Blanken, P.D.; Monson, Russell K.</p> <p>2004-01-01</p> <p>The location of the Niwot Ridge Ameriflux site within the rocky mountains subjects it to airflows which are common in mountainous terrain. In this study, we examine the effects of some of these mesoscale features on local <span class="hlt">turbulent</span> <span class="hlt">flux</span> measurements; most notably, the formation of valley/mountain flows and mountain lee-side waves. The valley/mountain flows created local non-stationarities in the wind flow caused by the passage of a lee-side convergence zone (LCZ) in which upslope and downslope flows met in the vicinity of the measurement tower. During June-August, 2001, possible lee-side convergences were flagged for ???26% of all half-hour daytime <span class="hlt">flux</span> measurement periods. However, there was no apparent loss of <span class="hlt">flux</span> during these periods. On some relatively stable, summer nights, <span class="hlt">turbulence</span> (designated via ??w), and scalar fluctuations (temperature and CO2, for example) exhibited periodicities that appeared congruent with passage of low frequency gravity waves (?? ??? 20 min). Spectral peaks at 0.0008 Hz (20 min) in both vertical velocity and scalar spectra were observed and indicated that 25-50% of the total scalar covariances were accounted for by the low frequency waves. During some periods of strong westerly winds (predominantly in winter), large mountain gravity waves were observed to form. Typically, the <span class="hlt">flux</span> tower resided within a region of downslope "shooting flow", which created high <span class="hlt">turbulence</span>, but had no detrimental effect on local <span class="hlt">flux</span> measurements based on valid <span class="hlt">turbulence</span> statistics and nearly complete energy budget closure. Periodically, we found evidence for re-circulating, rotor winds in the simultaneous time series of wind data from the Ameriflux tower site and a second meteorological site situated 8 km upslope and to the West. Only 14% of the half-hour time periods that we examined for a 4 month period in the winter of 2000-2001 indicated the possible existence of rotor winds. On average, energy budget closure was ???20% less during periods with</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22599892-gradient-driven-flux-tube-simulations-ion-temperature-gradient-turbulence-close-non-linear-threshold','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22599892-gradient-driven-flux-tube-simulations-ion-temperature-gradient-turbulence-close-non-linear-threshold"><span>Gradient-driven <span class="hlt">flux</span>-tube simulations of ion temperature gradient <span class="hlt">turbulence</span> close to the non-linear threshold</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>Peeters, A. G.; Rath, F.; Buchholz, R.</p> <p>2016-08-15</p> <p>It is shown that Ion Temperature Gradient <span class="hlt">turbulence</span> close to the threshold exhibits a long time behaviour, with smaller heat <span class="hlt">fluxes</span> at later times. This reduction is connected with the slow growth of long wave length zonal flows, and consequently, the numerical dissipation on these flows must be sufficiently small. Close to the nonlinear threshold for <span class="hlt">turbulence</span> generation, a relatively small dissipation can maintain a <span class="hlt">turbulent</span> state with a sizeable heat <span class="hlt">flux</span>, through the damping of the zonal flow. Lowering the dissipation causes the <span class="hlt">turbulence</span>, for temperature gradients close to the threshold, to be subdued. The heat <span class="hlt">flux</span> then doesmore » not go smoothly to zero when the threshold is approached from above. Rather, a finite minimum heat <span class="hlt">flux</span> is obtained below which no fully developed <span class="hlt">turbulent</span> state exists. The threshold value of the temperature gradient length at which this finite heat <span class="hlt">flux</span> is obtained is up to 30% larger compared with the threshold value obtained by extrapolating the heat <span class="hlt">flux</span> to zero, and the cyclone base case is found to be nonlinearly stable. Transport is subdued when a fully developed staircase structure in the E × B shearing rate forms. Just above the threshold, an incomplete staircase develops, and transport is mediated by avalanche structures which propagate through the marginally stable regions.« less</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_11 --> <div id="page_12" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="221"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/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/2018PhRvF...3d3201N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvF...3d3201N"><span>Scalar <span class="hlt">flux</span> modeling in <span class="hlt">turbulent</span> flames using iterative deconvolution</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nikolaou, Z. M.; Cant, R. S.; Vervisch, L.</p> <p>2018-04-01</p> <p>In the context of large eddy simulations, deconvolution is an attractive alternative for modeling the unclosed terms appearing in the filtered governing equations. Such methods have been used in a number of studies for non-reacting and incompressible flows; however, their application in reacting flows is limited in comparison. Deconvolution methods originate from clearly defined operations, and in theory they can be used in order to model any unclosed term in the filtered equations including the scalar <span class="hlt">flux</span>. In this study, an iterative deconvolution algorithm is used in order to provide a closure for the scalar <span class="hlt">flux</span> term in a <span class="hlt">turbulent</span> premixed flame by explicitly filtering the deconvoluted fields. The assessment of the method is conducted a priori using a three-dimensional direct numerical simulation database of a <span class="hlt">turbulent</span> freely propagating premixed flame in a canonical configuration. In contrast to most classical a priori studies, the assessment is more stringent as it is performed on a much coarser mesh which is constructed using the filtered fields as obtained from the direct simulations. For the conditions tested in this study, deconvolution is found to provide good estimates both of the scalar <span class="hlt">flux</span> and of its divergence.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1816124S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1816124S"><span>A True Eddy Accumulation - Eddy Covariance hybrid for measurements of <span class="hlt">turbulent</span> trace gas <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>Siebicke, Lukas</p> <p>2016-04-01</p> <p>Eddy covariance (EC) is state-of-the-art in directly and continuously measuring <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> of carbon dioxide and water vapor. However, low signal-to-noise ratios, high flow rates and missing or complex gas analyzers limit it's application to few scalars. True eddy accumulation, based on conditional sampling ideas by Desjardins in 1972, requires no fast response analyzers and is therefore potentially applicable to a wider range of scalars. Recently we showed possibly the first successful implementation of True Eddy Accumulation (TEA) measuring net ecosystem exchange of carbon dioxide of a grassland. However, most accumulation systems share the complexity of having to store discrete <span class="hlt">air</span> samples in physical containers representing entire <span class="hlt">flux</span> averaging intervals. The current study investigates merging principles of eddy accumulation and eddy covariance, which we here refer to as "true eddy accumulation in transient mode" (TEA-TM). This direct <span class="hlt">flux</span> method TEA-TM combines true eddy accumulation with continuous sampling. The TEA-TM setup is simpler than discrete accumulation methods while avoiding the need for fast response gas analyzers and high flow rates required for EC. We implemented the proposed TEA-TM method and measured <span class="hlt">fluxes</span> of carbon dioxide (CO2), methane (CH4) and water vapor (H2O) above a mixed beech forest at the Hainich Fluxnet and ICOS site, Germany, using a G2301 laser spectrometer (Picarro Inc., USA). We further simulated a TEA-TM sampling system using measured high frequency CO2 time series from an open-path gas analyzer. We operated TEA-TM side-by-side with open-, enclosed- and closed-path EC <span class="hlt">flux</span> systems for CO2, H2O and CH4 (LI-7500, LI-7200, LI-6262, LI-7700, Licor, USA, and FGGA LGR, USA). First results show that TEA-TM CO2 <span class="hlt">fluxes</span> were similar to EC <span class="hlt">fluxes</span>. Remaining differences were similar to those between the three eddy covariance setups (open-, enclosed- and closed-path gas analyzers). Measured TEA-TM CO2 <span class="hlt">fluxes</span> from our physical</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://hdl.handle.net/2060/20120002868','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120002868"><span>Characterization of <span class="hlt">Turbulent</span> Latent and Sensible Heat <span class="hlt">Flux</span> Exchange Between the Atmosphere and Ocean in MERRA</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Robert, J. Brent; Robertson, Franklin R.; Clayson, Carol Anne; Bosilovich, Michael G.</p> <p>2012-01-01</p> <p><span class="hlt">Turbulent</span> <span class="hlt">fluxes</span> of heat and moisture across the atmosphere-ocean interface are fundamental components of the Earth's energy and water balance. Characterizing both the spatiotemporal variability and the fidelity of these exchanges of heat and moisture is critical to understanding the global water and energy cycle variations, quantifying atmosphere-ocean feedbacks, and improving model predictability. This study examines the veracity of the recently completed NASA Modern-Era Retrospective analysis for Research and Applications (MERRA) product with respect to its representation of the surface <span class="hlt">turbulent</span> heat <span class="hlt">fluxes</span>. A validation of MERRA <span class="hlt">turbulent</span> heat <span class="hlt">fluxes</span> and near-surface bulk variables at local, high-resolution space and time scales is achieved by making comparisons to a large suite of direct observations. Both in situ and satellite-observed gridded surface heat <span class="hlt">flux</span> estimates are employed to investigate the spatial and temporal variability of the surface <span class="hlt">fluxes</span> with respect to their annual mean climatologies, their seasonal covariability of near-surface bulk parameters, and their representation of extremes. The impact of data assimilation on the near-surface parameters is assessed through evaluation of incremental analysis update tendencies produced by the assimilation procedure. It is found that MERRA <span class="hlt">turbulent</span> surface heat <span class="hlt">fluxes</span> are relatively accurate for typical conditions but have systematically weak vertical gradients in moisture and temperature and have a weaker covariability between the near-surface gradients and wind speed than found in observations. This results in an underestimate of the surface latent and sensible heat <span class="hlt">fluxes</span> over the western boundary current and storm track regions. The assimilation of observations mostly acts to bring MERRA closer to observational products by increasing moisture and temperature near the surface and decreasing the near-surface wind speeds. The major patterns of spatial and temporal variability of the <span class="hlt">turbulent</span> heat</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120007430','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120007430"><span>Characterization of <span class="hlt">Turbulent</span> Latent and Sensible Heat <span class="hlt">Flux</span> Exchange Between the Atmosphere and Ocean in MERRA</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, Franklin R.; Clayson, Carol Anne; Bosilovich, Michael G.</p> <p>2012-01-01</p> <p><span class="hlt">Turbulent</span> <span class="hlt">fluxes</span> of heat and moisture across the atmosphere-ocean interface are fundamental components of the Earth s energy and water balance. Characterizing both the spatiotemporal variability and the fidelity of these exchanges of heat and moisture is critical to understanding the global water and energy cycle variations, quantifying atmosphere-ocean feedbacks, and improving model predictability. This study examines the veracity of the recently completed NASA Modern-Era Retrospective analysis for Research and Applications (MERRA) product with respect to its representation of the surface <span class="hlt">turbulent</span> heat <span class="hlt">fluxes</span>. A validation of MERRA <span class="hlt">turbulent</span> heat <span class="hlt">fluxes</span> and near-surface bulk variables at local, high-resolution space and time scales is achieved by making comparisons to a large suite of direct observations. Both in situ and satellite-observed gridded surface heat <span class="hlt">flux</span> estimates are employed to investigate the spatial and temporal variability of the surface <span class="hlt">fluxes</span> with respect to their annual mean climatologies, their seasonal covariability of near-surface bulk parameters, and their representation of extremes. The impact of data assimilation on the near-surface parameters is assessed through evaluation of incremental analysis update tendencies produced by the assimilation procedure. It is found that MERRA <span class="hlt">turbulent</span> surface heat <span class="hlt">fluxes</span> are relatively accurate for typical conditions but have systematically weak vertical gradients in moisture and temperature and have a weaker covariability between the near-surface gradients and wind speed than found in observations. This results in an underestimate of the surface latent and sensible heat <span class="hlt">fluxes</span> over the western boundary current and storm track regions. The assimilation of observations mostly acts to bring MERRA closer to observational products by increasing moisture and temperature near the surface and decreasing the near-surface wind speeds. The major patterns of spatial and temporal variability of the <span class="hlt">turbulent</span> heat</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012JGRC..117.5035A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012JGRC..117.5035A"><span>Statistics of surface divergence and their relation to <span class="hlt">air</span>-water gas transfer velocity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Asher, William E.; Liang, Hanzhuang; Zappa, Christopher J.; Loewen, Mark R.; Mukto, Moniz A.; Litchendorf, Trina M.; Jessup, Andrew T.</p> <p>2012-05-01</p> <p><span class="hlt">Air-sea</span> gas <span class="hlt">fluxes</span> are generally defined in terms of the <span class="hlt">air</span>/water concentration difference of the gas and the gas transfer velocity,kL. Because it is difficult to measure kLin the ocean, it is often parameterized using more easily measured physical properties. Surface divergence theory suggests that infrared (IR) images of the water surface, which contain information concerning the movement of water very near the <span class="hlt">air</span>-water interface, might be used to estimatekL. Therefore, a series of experiments testing whether IR imagery could provide a convenient means for estimating the surface divergence applicable to <span class="hlt">air-sea</span> exchange were conducted in a synthetic jet array tank embedded in a wind tunnel. Gas transfer velocities were measured as a function of wind stress and mechanically generated <span class="hlt">turbulence</span>; laser-induced fluorescence was used to measure the concentration of carbon dioxide in the top 300 μm of the water surface; IR imagery was used to measure the spatial and temporal distribution of the aqueous skin temperature; and particle image velocimetry was used to measure <span class="hlt">turbulence</span> at a depth of 1 cm below the <span class="hlt">air</span>-water interface. It is shown that an estimate of the surface divergence for both wind-shear driven <span class="hlt">turbulence</span> and mechanically generated <span class="hlt">turbulence</span> can be derived from the surface skin temperature. The estimates derived from the IR images are compared to velocity field divergences measured by the PIV and to independent estimates of the divergence made using the laser-induced fluorescence data. Divergence is shown to scale withkLvalues measured using gaseous tracers as predicted by conceptual models for both wind-driven and mechanically generated <span class="hlt">turbulence</span>.</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/2016AGUFM.A21D0078L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.A21D0078L"><span>Characteristics of the Surface <span class="hlt">Turbulent</span> <span class="hlt">Flux</span> and the Components of Radiation Balance over the Grasslands in the Southeastern Tibetan Plateau</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, H.; Xiao, Z.; Wei, J.</p> <p>2016-12-01</p> <p>Characteristics of the Surface <span class="hlt">Turbulent</span> <span class="hlt">Flux</span> and the Components of Radiation Balance over the Grasslands in the Southeastern Tibetan PlateauHongyi Li 1, Ziniu Xiao 2 and Junhong Wei31 China Meteorological Administration Training Centre, Beijing, China2 State Key Laboratory of Numerical Modeling for Atmospheric Sciences and Geophysical Fluid Dynamics, Institute of Atmospheric Physics, Chinese Academy of Sciences, Beijing, China 3Theory of Atmospheric Dynamics and Climate, Institute for Atmospheric and Environmental Sciences, Goethe University of Frankfurt, Campus Riedberg, GermanyAbstract:Based on the field observation data over the grasslands in the southeastern Tibetan Plateau and the observational datasets in Nyingchi weather station for the period from May 20 to July 9, 2013, the variation characteristics of the basic meteorological elements in Nyingchi weather station, the surface <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> and the components of radiation balance over the grasslands, as well as their relationships, are analyzed in this paper. The results show that in Nyingchi weather station, the daily variations of relative humidity and average total cloud cover are consistent with that of precipitation, but that those of daily average <span class="hlt">air</span> temperature, daily average ground temperature, daily average wind speed and daily sunshine duration have an opposite change to that of precipitation. During the observation period, latent heat exchange is greater than sensible heat exchange, and latent heat <span class="hlt">flux</span> is significantly higher when there is rainfall, but sensible heat <span class="hlt">flux</span> and soil heat <span class="hlt">flux</span> are lower. The daily variation of the total solar radiation (DR) is synchronous with that of sensible heat <span class="hlt">flux</span>, and the daily variations of reflective solar radiation (UR), long wave radiation by earth (ULR), net radiation (Rn) and surface albedo are consistent with DR, but that of the long wave radiation by atmosphere (DLR) has an opposite change. The diurnal variations of sensible heat <span class="hlt">flux</span>, latent</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.C51A0627G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.C51A0627G"><span>Field Investigation of the <span class="hlt">Turbulent</span> <span class="hlt">Flux</span> Parameterization and Scalar <span class="hlt">Turbulence</span> Structure over a Melting Valley Glacier</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Guo, X.; Yang, K.; Yang, W.; Li, S.; Long, Z.</p> <p>2011-12-01</p> <p>We present a field investigation over a melting valley glacier on the Tibetan Plateau. One particular aspect lies in that three melt phases are distinguished during the glacier's ablation season, which enables us to compare results over snow, bare-ice, and hummocky surfaces [with aerodynamic roughness lengths (z0M) varying on the order of 10-4-10-2 m]. We address two issues of common concern in the study of glacio-meteorology and micrometeorology. First, we study <span class="hlt">turbulent</span> energy <span class="hlt">flux</span> estimation through a critical evaluation of three parameterizations of the scalar roughness lengths (z0T for temperature and z0q for humidity), viz. key factors for the accurate estimation of sensible heat and latent heat <span class="hlt">fluxes</span> using the bulk aerodynamic method. The first approach (Andreas 1987, Boundary-Layer Meteorol 38:159-184) is based on surface-renewal models and has been very widely applied in glaciated areas; the second (Yang et al. 2002, Q J Roy Meteorol Soc 128:2073-2087) has never received application over an ice/snow surface, despite its validity in arid regions; the third approach (Smeets and van den Broeke 2008, Boundary-Layer Meteorol 128:339-355) is proposed for use specifically over rough ice defined as z0M > 10-3 m or so. This empirical z0M threshold value is deemed of general relevance to glaciated areas (e.g. ice sheet/cap and valley/outlet glaciers), above which the first approach gives underestimated z0T and z0q. The first and the third approaches tend to underestimate and overestimate <span class="hlt">turbulent</span> heat/moisture exchange, respectively (relative errors often > 30%). Overall, the second approach produces fairly low errors in energy <span class="hlt">flux</span> estimates; it thus emerges as a practically useful choice to parameterize z0T and z0q over an ice/snow surface. Our evaluation of z0T and z0q parameterizations hopefully serves as a useful source of reference for physically based modeling of land-ice surface energy budget and mass balance. Second, we explore how scalar <span class="hlt">turbulence</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017A%26A...601A..18B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017A%26A...601A..18B"><span>Ionisation in <span class="hlt">turbulent</span> magnetic molecular clouds. I. Effect on density and mass-to-<span class="hlt">flux</span> ratio structures</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bailey, Nicole D.; Basu, Shantanu; Caselli, Paola</p> <p>2017-05-01</p> <p>Context. Previous studies show that the physical structures and kinematics of a region depend significantly on the ionisation fraction. These studies have only considered these effects in non-ideal magnetohydrodynamic simulations with microturbulence. The next logical step is to explore the effects of <span class="hlt">turbulence</span> on ionised magnetic molecular clouds and then compare model predictions with observations to assess the importance of <span class="hlt">turbulence</span> in the dynamical evolution of molecular clouds. Aims: In this paper, we extend our previous studies of the effect of ionisation fractions on star formation to clouds that include both non-ideal magnetohydrodynamics and <span class="hlt">turbulence</span>. We aim to quantify the importance of a treatment of the ionisation fraction in <span class="hlt">turbulent</span> magnetised media and investigate the effect of the <span class="hlt">turbulence</span> on shaping the clouds and filaments before star formation sets in. In particular, here we investigate how the structure, mass and width of filamentary structures depend on the amount of <span class="hlt">turbulence</span> in ionised media and the initial mass-to-<span class="hlt">flux</span> ratio. Methods: To determine the effects of <span class="hlt">turbulence</span> and mass-to-<span class="hlt">flux</span> ratio on the evolution of non-ideal magnetised clouds with varying ionisation profiles, we have run two sets of simulations. The first set assumes different initial <span class="hlt">turbulent</span> Mach values for a fixed initial mass-to-<span class="hlt">flux</span> ratio. The second set assumes different initial mass-to-<span class="hlt">flux</span> ratio values for a fixed initial <span class="hlt">turbulent</span> Mach number. Both sets explore the effect of using one of two ionisation profiles: step-like (SL) or cosmic ray only (CR-only). We compare the resulting density and mass-to-<span class="hlt">flux</span> ratio structures both qualitatively and quantitatively via filament and core masses and filament fitting techniques (Gaussian and Plummer profiles). Results: We find that even with almost no <span class="hlt">turbulence</span>, filamentary structure still exists although at lower density contours. Comparison of simulations shows that for <span class="hlt">turbulent</span> Mach numbers above 2, there is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19920018134','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19920018134"><span><span class="hlt">Turbulent</span> heat <span class="hlt">flux</span> measurements in a transitional boundary layer</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sohn, K. H.; Zaman, K. B. M. Q.; Reshotko, E.</p> <p>1992-01-01</p> <p>During an experimental investigation of the transitional boundary layer over a heated flat plate, an unexpected result was encountered for the <span class="hlt">turbulent</span> heat <span class="hlt">flux</span> (bar-v't'). This quantity, representing the correlation between the fluctuating normal velocity and the temperature, was measured to be negative near the wall under certain conditions. The result was unexpected as it implied a counter-gradient heat transfer by the <span class="hlt">turbulent</span> fluctuations. Possible reasons for this anomalous result were further investigated. The possible causes considered for this negative bar-v't' were: (1) plausible measurement error and peculiarity of the flow facility, (2) large probe size effect, (3) 'streaky structure' in the near wall boundary layer, and (4) contributions from other terms usually assumed negligible in the energy equation including the Reynolds heat <span class="hlt">flux</span> in the streamwise direction (bar-u't'). Even though the energy balance has remained inconclusive, none of the items (1) to (3) appear to be contributing directly to the anomaly.</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://hdl.handle.net/2060/20120014596','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120014596"><span>Using Indirect <span class="hlt">Turbulence</span> Measurements for Real-Time Parameter Estimation in <span class="hlt">Turbulent</span> <span class="hlt">Air</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Martos, Borja; Morelli, Eugene A.</p> <p>2012-01-01</p> <p>The use of indirect <span class="hlt">turbulence</span> measurements for real-time estimation of parameters in a linear longitudinal dynamics model in atmospheric <span class="hlt">turbulence</span> was studied. It is shown that measuring the atmospheric <span class="hlt">turbulence</span> makes it possible to treat the <span class="hlt">turbulence</span> as a measured explanatory variable in the parameter estimation problem. Commercial off-the-shelf sensors were researched and evaluated, then compared to <span class="hlt">air</span> data booms. Sources of colored noise in the explanatory variables resulting from typical <span class="hlt">turbulence</span> measurement techniques were identified and studied. A major source of colored noise in the explanatory variables was identified as frequency dependent upwash and time delay. The resulting upwash and time delay corrections were analyzed and compared to previous time shift dynamic modeling research. Simulation data as well as flight test data in atmospheric <span class="hlt">turbulence</span> were used to verify the time delay behavior. Recommendations are given for follow on flight research and instrumentation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1046432','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1046432"><span>Sensible Heat <span class="hlt">Flux</span> Related to Variations in Atmospheric <span class="hlt">Turbulence</span> Kinetic Energy on a Sandy Beach</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2017-06-01</p> <p><span class="hlt">FLUX</span> RELATED TO VARIATIONS IN ATMOSPHERIC <span class="hlt">TURBULENCE</span> KINETIC ENERGY ON A SANDY BEACH by Jessica S. Koscinski June 2017 Thesis Advisor...KINETIC ENERGY ON A SANDY BEACH 5. FUNDING NUMBERS 6. AUTHOR(S) Jessica S. Koscinski 7. PERFORMING ORGANIZATION NAME(S) AND ADDRESS(ES) Naval...Sensible heat <span class="hlt">flux</span>, <span class="hlt">turbulence</span> kinetic energy , surf zone 15. NUMBER OF PAGES 57 16. PRICE CODE 17. SECURITY CLASSIFICATION OF REPORT</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSHI44A1819K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSHI44A1819K"><span>Control of wave-driven <span class="hlt">turbulence</span> and surface heating on the mixing of microplastic marine debris</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kukulka, T.; Lavender Law, K. L.; Proskurowski, G. K.</p> <p>2016-02-01</p> <p>Buoyant microplastic marine debris (MPMD) is a pollutant in the ocean surface boundary layer (OSBL) that is submerged by <span class="hlt">turbulent</span> transport processes. Langmuir circulation (LC) is a <span class="hlt">turbulent</span> process driven by wind and surface waves that enhances mixing in the OSBL. <span class="hlt">Sea</span> surface cooling also contributes to OSBL <span class="hlt">turbulence</span> by driving convection. On the other hand, <span class="hlt">sea</span> surface heating stratifies and stabilizes the water column to reduce <span class="hlt">turbulent</span> motion. We analyze observed MPMD surface concentrations in the Atlantic and Pacific Oceans to reveal a significant increase in MPMD concentrations during surface heating and a decrease during surface cooling. <span class="hlt">Turbulence</span> resolving large eddy simulations of the OSBL for an idealized diurnal heating cycle suggest that <span class="hlt">turbulent</span> downward <span class="hlt">fluxes</span> of buoyant tracers are enhanced at night, facilitating deep submergence of plastics, and suppressed in heating conditions, resulting in surface trapped MPMD. Simulations agree with observations if enhanced mixing due to LC is included. Our results demonstrate the controlling influence of surface heat <span class="hlt">fluxes</span> and LC on <span class="hlt">turbulent</span> transport in the OSBL and on vertical distributions of buoyant marine particles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20060032490&hterms=sonar&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dsonar','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060032490&hterms=sonar&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dsonar"><span>Combined Satellite - and ULS-Derived <span class="hlt">Sea</span>-Ice <span class="hlt">Flux</span> in the Weddell <span class="hlt">Sea</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Drinkwater, M.; Liu, X.; Harms, S.</p> <p>2000-01-01</p> <p>Several years of daily microwave satellite ice-drift are combined with moored Upward Looking Sonar (ULS) ice-drafts into an ice volume <span class="hlt">flux</span> record at points along a <span class="hlt">flux</span> gate across the Weddell <span class="hlt">Sea</span>, Antarctica.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_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/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/2018PhPl...25e5905C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhPl...25e5905C"><span>Progress towards modeling tokamak boundary plasma <span class="hlt">turbulence</span> and understanding its role in setting divertor heat <span class="hlt">flux</span> widths</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, B.; Xu, X. Q.; Xia, T. Y.; Li, N. M.; Porkolab, M.; Edlund, E.; LaBombard, B.; Terry, J.; Hughes, J. W.; Ye, M. Y.; Wan, Y. X.</p> <p>2018-05-01</p> <p>The heat <span class="hlt">flux</span> distributions on divertor targets in H-mode plasmas are serious concerns for future devices. We seek to simulate the tokamak boundary plasma <span class="hlt">turbulence</span> and heat transport in the edge localized mode-suppressed regimes. The improved BOUT++ model shows that not only Ip but also the radial electric field Er plays an important role on the <span class="hlt">turbulence</span> behavior and sets the heat <span class="hlt">flux</span> width. Instead of calculating Er from the pressure gradient term (diamagnetic Er), it is calculated from the plasma transport equations with the sheath potential in the scrape-off layer and the plasma density and temperature profiles inside the separatrix from the experiment. The simulation results with the new Er model have better agreement with the experiment than using the diamagnetic Er model: (1) The electromagnetic <span class="hlt">turbulence</span> in enhanced Dα H-mode shows the characteristics of quasi-coherent modes (QCMs) and broadband <span class="hlt">turbulence</span>. The mode spectra are in agreement with the phase contrast imaging data and almost has no change in comparison to the cases which use the diamagnetic Er model; (2) the self-consistent boundary Er is needed for the <span class="hlt">turbulence</span> simulations to get the consistent heat <span class="hlt">flux</span> width with the experiment; (3) the frequencies of the QCMs are proportional to Er, while the divertor heat <span class="hlt">flux</span> widths are inversely proportional to Er; and (4) the BOUT++ <span class="hlt">turbulence</span> simulations yield a similar heat <span class="hlt">flux</span> width to the experimental Eich scaling law and the prediction from the Goldston heuristic drift model.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ThApC.tmp..235S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ThApC.tmp..235S"><span><span class="hlt">Turbulent</span> <span class="hlt">flux</span> variability and energy balance closure in the TERENO prealpine observatory: a hydrometeorological data analysis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Soltani, Mohsen; Mauder, Matthias; Laux, Patrick; Kunstmann, Harald</p> <p>2017-07-01</p> <p>The temporal multiscale variability of the surface heat <span class="hlt">fluxes</span> is assessed by the analysis of the <span class="hlt">turbulent</span> heat and moisture <span class="hlt">fluxes</span> using the eddy covariance (EC) technique at the TERrestrial ENvironmental Observatories (TERENO) prealpine region. The fast and slow response variables from three EC sites located at Fendt, Rottenbuch, and Graswang are gathered for the period of 2013 to 2014. Here, the main goals are to characterize the multiscale variations and drivers of the <span class="hlt">turbulent</span> <span class="hlt">fluxes</span>, as well as to quantify the energy balance closure (EBC) and analyze the possible reasons for the lack of EBC at the EC sites. To achieve these goals, we conducted a principal component analysis (PCA) and a climatological <span class="hlt">turbulent</span> <span class="hlt">flux</span> footprint analysis. The results show significant differences in the mean diurnal variations of the sensible heat (H) and latent heat (LE) <span class="hlt">fluxes</span>, because of variations in the solar radiation, precipitation patterns, soil moisture, and the vegetation fraction throughout the year. LE was the main consumer of net radiation. Based on the first principal component (PC1), the radiation and temperature components with a total mean contribution of 29.5 and 41.3%, respectively, were found to be the main drivers of the <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> at the study EC sites. A general lack of EBC is observed, where the energy imbalance values amount 35, 44, and 35% at the Fendt, Rottenbuch, and Graswang sites, respectively. An average energy balance ratio (EBR) of 0.65 is obtained in the region. The best closure occurred in the afternoon peaking shortly before sunset with a different pattern and intensity between the study sites. The size and shape of the annual mean half-hourly <span class="hlt">turbulent</span> <span class="hlt">flux</span> footprint climatology was analyzed. On average, 80% of the <span class="hlt">flux</span> footprint was emitted from a radius of approximately 250 m around the EC stations. Moreover, the overall shape of the <span class="hlt">flux</span> footprints was in good agreement with the prevailing wind direction for all three TERENO EC sites.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.6555S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.6555S"><span>Convectively-generated gravity waves and clear-<span class="hlt">air</span> <span class="hlt">turbulence</span> (CAT)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sharman, Robert; Lane, Todd; Trier, Stanley</p> <p>2013-04-01</p> <p>Upper-level <span class="hlt">turbulence</span> is a well-known hazard to aviation that is responsible for numerous injuries each year, with occasional fatalities, and results in millions of dollars of operational costs to airlines each year. It has been widely accepted that aviation-scale <span class="hlt">turbulence</span> that occurs in clear <span class="hlt">air</span> (CAT) at upper levels (upper troposphere and lower stratosphere) has its origins in Kelvin-Helmholtz instabilities induced by enhanced shears and reduced Richardson numbers associated with the jet stream and upper level fronts. However, it is becoming increasingly apparent that gravity waves and gravity wave "breaking" also play a major role in instigating <span class="hlt">turbulence</span> that affects aviation. Gravity waves and inertia-gravity waves may be produced by a variety of sources, but one major source that impacts aviation seems to be those produced by convection. The relation of convectively-induced gravity waves to <span class="hlt">turbulence</span> outside the cloud (either above cloud or laterally away from cloud) is examined based on high resolution cloud-resolving simulations, both with and without cloud microphysics in the simulations. Results for both warm-season and cold-season cloud systems indicate that the <span class="hlt">turbulence</span> in the clear <span class="hlt">air</span> away from cloud is often caused by gravity wave production processes in or near the cloud which once initiated, are able to propagate away from the storm, and may eventually "break." Without microphysics of course this effect is absent and <span class="hlt">turbulence</span> is not produced in the simulations. In some cases the convectively-induced <span class="hlt">turbulence</span> may be many kilometers away from the active convection and can easily be misinterpreted as "clear-<span class="hlt">air</span> <span class="hlt">turbulence</span>" (CAT). This is a significant result, and may be cause for a reassessment of the working definition of CAT ("<span class="hlt">turbulence</span> encountered outside of convective clouds", FAA Advisory Circular AC 00-30B, 1997).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20090025444','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20090025444"><span><span class="hlt">Turbulent</span> CO2 <span class="hlt">Flux</span> Measurements by Lidar: Length Scales, Results and Comparison with In-Situ Sensors</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gilbert, Fabien; Koch, Grady J.; Beyon, Jeffrey Y.; Hilton, Timothy W.; Davis, Kenneth J.; Andrews, Arlyn; Ismail, Syed; Singh, Upendra N.</p> <p>2009-01-01</p> <p>The vertical CO2 <span class="hlt">flux</span> in the atmospheric boundary layer (ABL) is investigated with a Doppler differential absorption lidar (DIAL). The instrument was operated next to the WLEF instrumented tall tower in Park Falls, Wisconsin during three days and nights in June 2007. Profiles of <span class="hlt">turbulent</span> CO2 mixing ratio and vertical velocity fluctuations are measured by in-situ sensors and Doppler DIAL. Time and space scales of <span class="hlt">turbulence</span> are precisely defined in the ABL. The eddy-covariance method is applied to calculate <span class="hlt">turbulent</span> CO2 <span class="hlt">flux</span> both by lidar and in-situ sensors. We show preliminary mean lidar CO2 <span class="hlt">flux</span> measurements in the ABL with a time and space resolution of 6 h and 1500 m respectively. The <span class="hlt">flux</span> instrumental errors decrease linearly with the standard deviation of the CO2 data, as expected. Although <span class="hlt">turbulent</span> fluctuations of CO2 are negligible with respect to the mean (0.1 %), we show that the eddy-covariance method can provide 2-h, 150-m range resolved CO2 <span class="hlt">flux</span> estimates as long as the CO2 mixing ratio instrumental error is no greater than 10 ppm and the vertical velocity error is lower than the natural fluctuations over a time resolution of 10 s.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1610587S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1610587S"><span>Analysis of small scale <span class="hlt">turbulent</span> structures and the effect of spatial scales on 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>Schnieders, Jana; Garbe, Christoph</p> <p>2014-05-01</p> <p>The exchange of gases through the <span class="hlt">air-sea</span> interface strongly depends on environmental conditions such as wind stress and waves which in turn generate near surface <span class="hlt">turbulence</span>. Near surface <span class="hlt">turbulence</span> is a main driver of surface divergence which has been shown to cause highly variable transfer rates on relatively small spatial scales. Due to the cool skin of the ocean, heat can be used as a tracer to detect areas of surface convergence and thus gather information about size and intensity of a <span class="hlt">turbulent</span> process. We use infrared imagery to visualize near surface aqueous <span class="hlt">turbulence</span> and determine the impact of <span class="hlt">turbulent</span> scales on exchange rates. Through the high temporal and spatial resolution of these types of measurements spatial scales as well as surface dynamics can be captured. The surface heat pattern is formed by distinct structures on two scales - small-scale short lived structures termed fish scales and larger scale cold streaks that are consistent with the footprints of Langmuir Circulations. There are two key characteristics of the observed surface heat patterns: 1. The surface heat patterns show characteristic features of scales. 2. The structure of these patterns change with increasing wind stress and surface conditions. In [2] <span class="hlt">turbulent</span> cell sizes have been shown to systematically decrease with increasing wind speed until a saturation at u* = 0.7 cm/s is reached. Results suggest a saturation in the tangential stress. Similar behaviour has been observed by [1] for gas transfer measurements at higher wind speeds. In this contribution a new model to estimate the heat <span class="hlt">flux</span> is applied which is based on the measured <span class="hlt">turbulent</span> cell size und surface velocities. This approach allows the direct comparison of the net effect on heat <span class="hlt">flux</span> of eddies of different sizes and a comparison to gas transfer measurements. Linking transport models with thermographic measurements, transfer velocities can be computed. In this contribution, we will quantify the effect of small scale</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ZaMP...69....2M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ZaMP...69....2M"><span>Hydrodynamical model of anisotropic, polarized <span class="hlt">turbulent</span> superfluids. I: constraints for the <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>Mongiovì, Maria Stella; Restuccia, Liliana</p> <p>2018-02-01</p> <p>This work is the first of a series of papers devoted to the study of the influence of the anisotropy and polarization of the tangle of quantized vortex lines in superfluid <span class="hlt">turbulence</span>. A thermodynamical model of inhomogeneous superfluid <span class="hlt">turbulence</span> previously formulated is here extended, to take into consideration also these effects. The model chooses as thermodynamic state vector the density, the velocity, the energy density, the heat <span class="hlt">flux</span>, and a complete vorticity tensor field, including its symmetric traceless part and its antisymmetric part. The relations which constrain the constitutive quantities are deduced from the second principle of thermodynamics using the Liu procedure. The results show that the presence of anisotropy and polarization in the vortex tangle affects in a substantial way the dynamics of the heat <span class="hlt">flux</span>, and allow us to give a physical interpretation of the vorticity tensor here introduced, and to better describe the internal structure of a <span class="hlt">turbulent</span> superfluid.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JPhCS1001a2003O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JPhCS1001a2003O"><span>Intense structures of different momentum <span class="hlt">fluxes</span> in <span class="hlt">turbulent</span> channels</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Osawa, Kosuke; Jiménez, Javier</p> <p>2018-04-01</p> <p>The effect of different definitions of the momentum <span class="hlt">flux</span> on the properties of the coherent structures of the logarithmic region of wall-bounded <span class="hlt">turbulence</span> is investigated by comparing the structures of intense tangential Reynolds stress with those of the alternative <span class="hlt">flux</span> proposed in [Jimenez (2016) J. Fluid Mech. 809:585]. Despite the fairly different statistical properties of the two <span class="hlt">flux</span> definitions, it is found that their intense structures show many similarities, such as the dominance of ‘wall-attached’ objects, and geometric self-similarity. However, the new structures are wider, although not taller, than the classical ones, and include both high- and low-momentum regions within the same object. It is concluded that they represent the same phenomenon as the classical group of a sweep, an ejection, and a roller, which should thus be considered as the fundamental coherent structure of the momentum <span class="hlt">flux</span>. The present results suggest that the properties of these momentum structures are robust with respect to the definition of the <span class="hlt">fluxes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A53I..04C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A53I..04C"><span>The Relationship Between <span class="hlt">Turbulence</span> and <span class="hlt">Air</span> Quality in California's Central Valley</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Caputi, D.; Faloona, I. C.; Trousdell, J.; Conley, S. A.</p> <p>2017-12-01</p> <p>The San Joaquin valley is known for excessive <span class="hlt">air</span> pollution, owing to local production combined with flow patterns that channel in <span class="hlt">air</span> from the bay area, with surrounding mountains trapping the <span class="hlt">air</span> inside. Understanding the role of boundary layer in the context of these dynamics is a particular challenge that will aid in effective <span class="hlt">air</span> quality attainment planning. During the summers of 2015 and 2016, a Mooney aircraft operated by Scientific Aviation Inc. collected 170 hours of airborne data between Fresno and Bakersfield, CA. Combining this data with WRF forecast output, it is possible to use a simple budget technique to estimate the kinematic surface heat <span class="hlt">fluxes</span> and thus the convective velocity scale. The 1 Hz wind measurements on the aircraft are provided by a newly developed low-cost system that utilizes the placement of dual GPS antennae on fixed positions of the airframe. Power spectra from the data indicates that the inertial subrange of <span class="hlt">turbulence</span> is detectable from wavelengths of 150-500 m. Using Kolmogorov scaling laws, it is possible to estimate that about 20% of the total variance is not being captured by the system (at spatial scales under 150 m). Similarity relationships can then be employed to estimate the convective velocity scale as a function of sampling length, which levels off at about 22 km to a value within 5% of the estimate obtained by the budgeting method. A larger goal of this work is to connect these <span class="hlt">turbulence</span> parameters with observations of <span class="hlt">air</span> quality, noting that a major finding of the field campaign is that the entrainment between the polluted boundary layer and cleaner free troposphere plays a significant role in the local daytime pollutant concentration. Nighttime dynamics are being explored as well. Using a combination of 915 MHz sounder data from Visalia, ground ozone monitors, and flight data, a relationship can be seen between the nocturnal low level jet speed and ozone concentrations the following day. This suggests a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JMS...173...70C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JMS...173...70C"><span><span class="hlt">Air-sea</span> 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('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 <span class="hlt">turbulent</span> 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/2017AGUFM.A51A2004P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A51A2004P"><span>Laboratory Study of <span class="hlt">Air</span> <span class="hlt">Turbulence</span>-Particle Coupling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Petersen, A.; Baker, L.; Coletti, F.</p> <p>2017-12-01</p> <p>Inertial particles suspended in a <span class="hlt">turbulent</span> flow are unable to follow the fluid's rapid velocity fluctuations, leading to high concentrations in regions where fluid strain dominates vorticity. This phenomenon is known as preferential concentration or clustering and is thought to affect natural processes ranging from the collisional growth of raindrops to the formation of planetesimals in proto-planetary nebulas. In the present study, we use a large jet-stirred chamber to generate homogeneous <span class="hlt">air</span> <span class="hlt">turbulence</span> into which we drop particles with an aerodynamic response time comparable to the flow time scales. Using laser imaging we find that <span class="hlt">turbulence</span> can lead to a multi-fold increase of settling velocity compared to still-<span class="hlt">air</span> conditions. We then employ Voronoi tessellation to examine the particle spatial distribution, finding strong evidence of <span class="hlt">turbulence</span>-driven particle clustering over a wide range of experimental conditions. We observe individual clusters of a larger size range than seen previously, sometimes beyond the integral length scale of the <span class="hlt">turbulence</span>. We also investigate cluster topology and find that they (i) exhibit a fractal structure, (ii) have a nearly constant particle concentration over their entire size range, and (iii) are most often vertically oriented. Furthermore, clustered particles tend to fall faster than those outside clusters, and larger clusters fall faster on average than smaller ones. Finally, by simultaneous measurement of particle and <span class="hlt">air</span> velocity fields, we provide the first experimental evidence of preferential sweeping, a mechanism previously proposed to explain the increase in particle settling velocity found in numerical simulations, and find it especially effective for clustered particles. These results are significant for the micro-scale physics of atmospheric clouds. The large cluster size range has implications for how droplets will influence the local environment through condensation, evaporation, drag and latent heat effects</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://rosap.ntl.bts.gov/view/dot/9170','DOTNTL'); return false;" href="https://rosap.ntl.bts.gov/view/dot/9170"><span>Clear <span class="hlt">air</span> <span class="hlt">turbulence</span> radiometric detection program.</span></a></p> <p><a target="_blank" href="http://ntlsearch.bts.gov/tris/index.do">DOT National Transportation Integrated Search</a></p> <p></p> <p>1971-07-01</p> <p>The report presents a review of accomplishments for the Clear <span class="hlt">Air</span> <span class="hlt">Turbulence</span> Detection Program. The objectives, instrumentation, supporting hardware and interfaces leading up to and including the test flights for the reporting period are given. The u...</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('https://pubs.er.usgs.gov/publication/70185130','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70185130"><span>Airflows and <span class="hlt">turbulent</span> <span class="hlt">flux</span> measurements in mountainous terrain: Part 1. Canopy and local effects</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Turnipseed, Andrew A.; Anderson, Dean E.; Blanken, Peter D.; Baugh, William M.; Monson, Russell K.</p> <p>2003-01-01</p> <p>We have studied the effects of local topography and canopy structure on <span class="hlt">turbulent</span> <span class="hlt">flux</span> measurements at a site located in mountainous terrain within a subalpine, coniferous forest. Our primary aim was to determine whether the complex terrain of the site affects the accuracy of eddy <span class="hlt">flux</span> measurements from a practical perspective. We observed displacement heights, roughness lengths, spectral peaks, <span class="hlt">turbulent</span> length scales, and profiles of <span class="hlt">turbulent</span> intensities that were comparable in magnitude and pattern to those reported for forest canopies in simpler terrain. We conclude that in many of these statistical measures, the local canopy exerts considerably more influence than does topographical complexity. Lack of vertical <span class="hlt">flux</span> divergence and modeling suggests that the <span class="hlt">flux</span> footprints for the site are within the standards acceptable for the application of <span class="hlt">flux</span> statistics. We investigated three different methods of coordinate rotation: double rotation (DR), triple rotation (TR), and planar-fit rotation (PF). Significant variability in rotation angles at low wind speeds was encountered with the commonly used DR and TR methods, as opposed to the PF method, causing some overestimation of the <span class="hlt">fluxes</span>. However, these differences in <span class="hlt">fluxes</span> were small when applied to large datasets involving sensible heat and CO2 <span class="hlt">fluxes</span>. We observed evidence of frequent drainage flows near the ground during stable, stratified conditions at night. Concurrent with the appearance of these flows, we observed a positive bias in the mean vertical wind speed, presumably due to subtle topographic variations inducing a flow convergence below the measurement sensors. In the presence of such drainage flows, advection of scalars and non-zero bias in the mean vertical wind speed can complicate closure of the mass conservation budget at the site.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5407354','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5407354"><span>Estimating spatially distributed <span class="hlt">turbulent</span> heat <span class="hlt">fluxes</span> from high-resolution thermal imagery acquired with a UAV system</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Brenner, Claire; Thiem, Christina Elisabeth; Wizemann, Hans-Dieter; Bernhardt, Matthias; Schulz, Karsten</p> <p>2017-01-01</p> <p>ABSTRACT In this study, high-resolution thermal imagery acquired with a small unmanned aerial vehicle (UAV) is used to map evapotranspiration (ET) at a grassland site in Luxembourg. The land surface temperature (LST) information from the thermal imagery is the key input to a one-source and two-source energy balance model. While the one-source model treats the surface as a single uniform layer, the two-source model partitions the surface temperature and <span class="hlt">fluxes</span> into soil and vegetation components. It thus explicitly accounts for the different contributions of both components to surface temperature as well as <span class="hlt">turbulent</span> <span class="hlt">flux</span> exchange with the atmosphere. Contrary to the two-source model, the one-source model requires an empirical adjustment parameter in order to account for the effect of the two components. <span class="hlt">Turbulent</span> heat <span class="hlt">flux</span> estimates of both modelling approaches are compared to eddy covariance (EC) measurements using the high-resolution input imagery UAVs provide. In this comparison, the effect of different methods for energy balance closure of the EC data on the agreement between modelled and measured <span class="hlt">fluxes</span> is also analysed. Additionally, the sensitivity of the one-source model to the derivation of the empirical adjustment parameter is tested. Due to the very dry and hot conditions during the experiment, pronounced thermal patterns developed over the grassland site. These patterns result in spatially variable <span class="hlt">turbulent</span> heat <span class="hlt">fluxes</span>. The model comparison indicates that both models are able to derive ET estimates that compare well with EC measurements under these conditions. However, the two-source model, with a more complex treatment of the energy and surface temperature partitioning between the soil and vegetation, outperformed the simpler one-source model in estimating sensible and latent heat <span class="hlt">fluxes</span>. This is consistent with findings from prior studies. For the one-source model, a time-variant expression of the adjustment parameter (to account for the difference</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28515537','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28515537"><span>Estimating spatially distributed <span class="hlt">turbulent</span> heat <span class="hlt">fluxes</span> from high-resolution thermal imagery acquired with a UAV system.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Brenner, Claire; Thiem, Christina Elisabeth; Wizemann, Hans-Dieter; Bernhardt, Matthias; Schulz, Karsten</p> <p>2017-05-19</p> <p>In this study, high-resolution thermal imagery acquired with a small unmanned aerial vehicle (UAV) is used to map evapotranspiration (ET) at a grassland site in Luxembourg. The land surface temperature (LST) information from the thermal imagery is the key input to a one-source and two-source energy balance model. While the one-source model treats the surface as a single uniform layer, the two-source model partitions the surface temperature and <span class="hlt">fluxes</span> into soil and vegetation components. It thus explicitly accounts for the different contributions of both components to surface temperature as well as <span class="hlt">turbulent</span> <span class="hlt">flux</span> exchange with the atmosphere. Contrary to the two-source model, the one-source model requires an empirical adjustment parameter in order to account for the effect of the two components. <span class="hlt">Turbulent</span> heat <span class="hlt">flux</span> estimates of both modelling approaches are compared to eddy covariance (EC) measurements using the high-resolution input imagery UAVs provide. In this comparison, the effect of different methods for energy balance closure of the EC data on the agreement between modelled and measured <span class="hlt">fluxes</span> is also analysed. Additionally, the sensitivity of the one-source model to the derivation of the empirical adjustment parameter is tested. Due to the very dry and hot conditions during the experiment, pronounced thermal patterns developed over the grassland site. These patterns result in spatially variable <span class="hlt">turbulent</span> heat <span class="hlt">fluxes</span>. The model comparison indicates that both models are able to derive ET estimates that compare well with EC measurements under these conditions. However, the two-source model, with a more complex treatment of the energy and surface temperature partitioning between the soil and vegetation, outperformed the simpler one-source model in estimating sensible and latent heat <span class="hlt">fluxes</span>. This is consistent with findings from prior studies. For the one-source model, a time-variant expression of the adjustment parameter (to account for the difference between</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009JGRC..11412023H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009JGRC..11412023H"><span>Heat and <span class="hlt">turbulent</span> kinetic energy budgets for surface layer cooling induced by the passage of Hurricane Frances (2004)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Huang, Peisheng; Sanford, Thomas B.; Imberger, JöRg</p> <p>2009-12-01</p> <p>Heat and <span class="hlt">turbulent</span> kinetic energy budgets of the ocean surface layer during the passage of Hurricane Frances were examined using a three-dimensional hydrodynamic model. In situ data obtained with the Electromagnetic-Autonomous Profiling Explorer (EM-APEX) floats were used to set up the initial conditions of the model simulation and to compare to the simulation results. The spatial heat budgets reveal that during the hurricane passage, not only the entrainment in the bottom of surface mixed layer but also the horizontal water advection were important factors determining the spatial pattern of <span class="hlt">sea</span> surface temperature. At the free surface, the hurricane-brought precipitation contributed a negligible amount to the <span class="hlt">air-sea</span> heat exchange, but the precipitation produced a negative buoyancy <span class="hlt">flux</span> in the surface layer that overwhelmed the instability induced by the heat loss to the atmosphere. Integrated over the domain within 400 km of the hurricane eye on day 245.71 of 2004, the rate of heat anomaly in the surface water was estimated to be about 0.45 PW (1 PW = 1015 W), with about 20% (0.09 PW in total) of this was due to the heat exchange at the <span class="hlt">air-sea</span> interface, and almost all the remainder (0.36 PW) was downward transported by oceanic vertical mixing. Shear production was the major source of <span class="hlt">turbulent</span> kinetic energy amounting 88.5% of the source of <span class="hlt">turbulent</span> kinetic energy, while the rest (11.5%) was attributed to the wind stirring at <span class="hlt">sea</span> surface. The increase of ocean potential energy due to vertical mixing represented 7.3% of the energy deposited by wind stress.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_13 --> <div id="page_14" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="261"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/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/2017TCry...11.2897R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017TCry...11.2897R"><span>Evaluation of different methods to model near-surface <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> for a mountain glacier in the Cariboo Mountains, BC, Canada</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Radić, Valentina; Menounos, Brian; Shea, Joseph; Fitzpatrick, Noel; Tessema, Mekdes A.; Déry, Stephen J.</p> <p>2017-12-01</p> <p>As part of surface energy balance models used to simulate glacier melting, choosing parameterizations to adequately estimate <span class="hlt">turbulent</span> heat <span class="hlt">fluxes</span> is extremely challenging. This study aims to evaluate a set of four aerodynamic bulk methods (labeled as C methods), commonly used to estimate <span class="hlt">turbulent</span> heat <span class="hlt">fluxes</span> for a sloped glacier surface, and two less commonly used bulk methods developed from katabatic flow models. The C methods differ in their parameterizations of the bulk exchange coefficient that relates the <span class="hlt">fluxes</span> to the near-surface measurements of mean wind speed, <span class="hlt">air</span> temperature, and humidity. The methods' performance in simulating 30 min sensible- and latent-heat <span class="hlt">fluxes</span> is evaluated against the measured <span class="hlt">fluxes</span> from an open-path eddy-covariance (OPEC) method. The evaluation is performed at a point scale of a mountain glacier, using one-level meteorological and OPEC observations from multi-day periods in the 2010 and 2012 summer seasons. The analysis of the two independent seasons yielded the same key findings, which include the following: first, the bulk method, with or without the commonly used Monin-Obukhov (M-O) stability functions, overestimates the <span class="hlt">turbulent</span> heat <span class="hlt">fluxes</span> over the observational period, mainly due to a substantial overestimation of the friction velocity. This overestimation is most pronounced during the katabatic flow conditions, corroborating the previous findings that the M-O theory works poorly in the presence of a low wind speed maximum. Second, the method based on a katabatic flow model (labeled as the KInt method) outperforms any C method in simulating the friction velocity; however, the C methods outperform the KInt method in simulating the sensible-heat <span class="hlt">fluxes</span>. Third, the best overall performance is given by a hybrid method, which combines the KInt approach with the C method; i.e., it parameterizes eddy viscosity differently than eddy diffusivity. An error analysis reveals that the uncertainties in the measured meteorological</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('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 <span class="hlt">turbulent</span> 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://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/2008CNSNS..13...53D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008CNSNS..13...53D"><span>Intermittency in <span class="hlt">flux</span> driven kinetic simulations of trapped ion <span class="hlt">turbulence</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Darmet, G.; Ghendrih, Ph.; Sarazin, Y.; Garbet, X.; Grandgirard, V.</p> <p>2008-02-01</p> <p><span class="hlt">Flux</span> driven kinetic transport is analysed for deeply trapped ion <span class="hlt">turbulence</span> with the code GYSELA. The main observation is the existence of a steady state situation with respect to the statistics, in particular the balance between the injected energy and the time averaged energy flowing out through the outer edge boundary layer. The temperature is characterised by a very bursty behaviour with a skewed PDF. Superimposed to these short time scale fluctuations, one finds a regime with a strong increase of the zonal flows and a quenching of the <span class="hlt">turbulent</span> energy. During this phase of such a predator-prey cycle, the core temperature rapidly increases while the edge temperature gradually decreases. The end of this reduced transport regime is governed by the onset of <span class="hlt">turbulence</span> that governs large relaxation events, and a strong modification of the zonal flow pattern.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A51A2026Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A51A2026Y"><span>Viscous and <span class="hlt">Turbulent</span> Stress Measurements 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, K.; Veron, F.; Buckley, M. P.; Hara, T.; Husain, N.</p> <p>2017-12-01</p> <p>In recent years, the exchange of momentum and scalars 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 the <span class="hlt">turbulence</span> in the airflow over surface waves remain scarce. The current incomplete physical understanding of the airflow dynamics impedes further progress in developing physically based parameterizations for improved weather and <span class="hlt">sea</span> state predictions, particularly in high winds and extreme conditions. Using combined Particle Image Velocimetry (PIV) and Laser Induced Fluorescence (LIF) in the laboratory, we have acquired detailed quantitative measurements of the airflow over wind-driven waves and down to within the viscous sub-layer. Various wind-wave conditions are examined with mean wind speeds ranging from 0.86 to 16.63 m s-1. The mean, <span class="hlt">turbulent</span>, and wave-induced velocity fields are then extracted from instantaneous two-dimensional velocity measurements. Individual airflow separation events precipitate abrupt and dramatic along-wave variations in the surface viscous stress. In the bulk flow above the waves, these separation events are a source of intense vorticity. Phase averages of the viscous stress present a pattern of along-wave asymmetry near the surface; it is highest on the upwind of wave crest with its peak value about the crest and its minimum occurs at the middle of the leeward side of waves. The contribution of the viscous stress to the total momentum <span class="hlt">flux</span> is not negligible particularly for low to moderate wind speeds and this contribution decreases with increasing wind speed. Away from the surface, the distribution of <span class="hlt">turbulent</span> Reynolds stress forms a negative-positive pattern along the wave crest with a separation-induced maximum above the downwind side of the wave. Our measurements will be discussed in the context of available previous results.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JHyd..530..103H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JHyd..530..103H"><span>Interactions of bluff-body obstacles with <span class="hlt">turbulent</span> airflows affecting evaporative <span class="hlt">fluxes</span> from porous surfaces</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Haghighi, Erfan; Or, Dani</p> <p>2015-11-01</p> <p>Bluff-body obstacles interacting with <span class="hlt">turbulent</span> airflows are common in many natural and engineering applications (from desert pavement and shrubs over natural surfaces to cylindrical elements in compact heat exchangers). Even with obstacles of simple geometry, their interactions within <span class="hlt">turbulent</span> airflows result in a complex and unsteady flow field that affects surface drag partitioning and transport of scalars from adjacent evaporating surfaces. Observations of spatio-temporal thermal patterns on evaporating porous surfaces adjacent to bluff-body obstacles depict well-defined and persistent zonation of evaporation rates that were used to construct a simple mechanistic model for surface-<span class="hlt">turbulence</span> interactions. Results from evaporative drying of sand surfaces with isolated cylindrical elements (bluff bodies) subjected to constant <span class="hlt">turbulent</span> airflows were in good agreement with model predictions for localized exchange rates. Experimental and theoretical results show persistent enhancement of evaporative <span class="hlt">fluxes</span> from bluff-rough surfaces relative to smooth flat surfaces under similar conditions. The enhancement is attributed to formation of vortices that induce a thinner boundary layer over part of the interacting surface footprint. For a practical range of <span class="hlt">air</span> velocities (0.5-4.0 m/s), low-aspect ratio cylindrical bluff elements placed on evaporating sand surfaces enhanced evaporative mass losses (relative to a flat surface) by up to 300% for high density of elements and high wind velocity, similar to observations reported in the literature. Concepts from drag partitioning were used to generalize the model and upscale predictions to evaporation from surfaces with multiple obstacles for potential applications to natural bluff-rough surfaces.</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('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 <span class="hlt">turbulence</span> 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, <span class="hlt">turbulent</span> <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('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 <span class="hlt">turbulent</span> 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 <span class="hlt">turbulent</span> <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://adsabs.harvard.edu/abs/2004APS..DFD.NK003T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004APS..DFD.NK003T"><span>Three-Dimensional Direct Numerical Simulation of Methane-<span class="hlt">Air</span> <span class="hlt">Turbulent</span> Premixed Flames with Reduced Kinetic Mechanism</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tanahashi, Mamoru; Kikuta, Satoshi; Miyauchi, Toshio</p> <p>2004-11-01</p> <p>Three-dimensional DNS of methane-<span class="hlt">air</span> <span class="hlt">turbulent</span> premixed flames have been conducted to investigate local extinction mechanism of <span class="hlt">turbulent</span> premixed flames. A reduced kinetic mechanism (MeCH-19), which is created from GRI-Mech. 2.11 and includes 23 reactive species and 19 step reactions, are used to simulate CH_4-O_2-N2 reaction in <span class="hlt">turbulence</span>. The effectiveness of this reduced kinetic mechanism has been conformed by preliminary two-dimensional DNS with the reduced kinetic mechanism and two detailed kinetic mechanisms; GRI-Mech. 2.11 and Miller & Bowman. Flame structures of methane-<span class="hlt">air</span> <span class="hlt">turbulent</span> premixed flames are compared with those of hydrogen-<span class="hlt">air</span> <span class="hlt">turbulent</span> premixed flames which have been obtained by 3D-DNS with a detailed kinetic mechanism in our previous study. Local extinctions occur in methane-<span class="hlt">air</span> <span class="hlt">turbulent</span> premixed flames, whereas no extinction is observed for hydrogen-<span class="hlt">air</span> flames in nearly same <span class="hlt">turbulence</span> condition. The local extinction mechanism is discussed based on eddy/flame interaction in small scales.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010APhy...56.1080S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010APhy...56.1080S"><span><span class="hlt">Turbulent</span> boundary layer on the surface of a <span class="hlt">sea</span> geophysical antenna</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Smol'Yakov, A. V.</p> <p>2010-11-01</p> <p>A theory is constructed that makes it possible to calculate the initial parameters necessary for calculating the hydrodynamic (<span class="hlt">turbulent</span>) noise, which is a handicap to the operation of <span class="hlt">sea</span> geophysical antennas. Algorithms are created for calculating the profile and defect of the average speed, displacement thickness, momentum thickness, and friction resistance in a <span class="hlt">turbulent</span> boundary layer on a cylinder in its axial flow. Results of calculations using the developed theory are compared to experimental data. As the diameter of the cylinder tends to infinity, all relations of the theory pass to known relations for the boundary layer on a flat plate. The developed theory represents the initial stage of creating a method to calculate hydrodynamic noise, which is handicap to the operation of <span class="hlt">sea</span> geophysical antennas.</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 <span class="hlt">turbulent</span> 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/2005AtmRe..74..381H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005AtmRe..74..381H"><span>Airborne measurements of <span class="hlt">turbulent</span> trace gas <span class="hlt">fluxes</span> and analysis of eddy structure in the convective boundary layer over complex terrain</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hasel, M.; Kottmeier, Ch.; Corsmeier, U.; Wieser, A.</p> <p>2005-03-01</p> <p>Using the new high-frequency measurement equipment of the research aircraft DO 128, which is described in detail, <span class="hlt">turbulent</span> vertical <span class="hlt">fluxes</span> of ozone and nitric oxide have been calculated from data sampled during the ESCOMPTE program in the south of France. Based on airborne <span class="hlt">turbulence</span> measurements, radiosonde data and surface energy balance measurements, the convective boundary layer (CBL) is examined under two different aspects. The analysis covers boundary-layer convection with respect to (i) the control of CBL depth by surface heating and synoptic scale influences, and (ii) the structure of convective plumes and their vertical transport of ozone and nitric oxides. The orographic structure of the terrain causes significant differences between planetary boundary layer (PBL) heights, which are found to exceed those of terrain height variations on average. A comparison of boundary-layer <span class="hlt">flux</span> profiles as well as mean quantities over flat and complex terrain and also under different pollution situations and weather conditions shows relationships between vertical gradients and corresponding <span class="hlt">turbulent</span> <span class="hlt">fluxes</span>. Generally, NO x transports are directed upward independent of the terrain, since primary emission sources are located near the ground. For ozone, negative <span class="hlt">fluxes</span> are common in the lower CBL in accordance with the deposition of O 3 at the surface. The detailed structure of thermals, which largely carry out vertical transports in the boundary layer, are examined with a conditional sampling technique. Updrafts mostly contain warm, moist and NO x loaded <span class="hlt">air</span>, while the ozone transport by thermals alternates with the background ozone gradient. Evidence for handover processes of trace gases to the free atmosphere can be found in the case of existing gradients across the boundary-layer top. An analysis of the size of eddies suggests the possibility of some influence of the heterogeneous terrain in mountainous area on the length scales of eddies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19960021423&hterms=kinetic+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dkinetic%2Benergy','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19960021423&hterms=kinetic+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dkinetic%2Benergy"><span>Multifractal scaling of the kinetic energy <span class="hlt">flux</span> in solar wind <span class="hlt">turbulence</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Marsch, E.; Rosenbauer, H.; Tu, C.-Y.</p> <p>1995-01-01</p> <p>The geometrical and scaling properties of the energy <span class="hlt">flux</span> of the <span class="hlt">turbulent</span> kinetic energy in the solar wind have been studied. By present experimental technology in solar wind measurements, we cannot directly measure the real volumetric dissipation rate, epsilon(t), but are constrained to represent it by surrogating the energy <span class="hlt">flux</span> near the dissipation range at the proton gyro scales. There is evidence for the multifractal nature of the so defined dissipation field epsilon(t), a result derived from the scaling exponents of its statistical q-th order moments. The related generalized dimension D(q) has been determined and reveals that the dissipation field has a multifractal structure. which is not compatible with a scale-invariant cascade. The associated multifractal spectrum f(alpha) has been estimated for the first time for MHD <span class="hlt">turbulence</span> in the solar wind. Its features resemble those obtained for <span class="hlt">turbulent</span> fluids and other nonlinear multifractal systems. The generalized dimension D(q) can, for <span class="hlt">turbulence</span> in high-speed streams, be fitted well by the functional dependence of the p-model with a comparatively large parameter, p = 0.87. indicating a strongly intermittent multifractal energy cascade. The experimental value for D(p)/3, if used in the scaling exponent s(p) of the velocity structure function, gives an exponent that can describe some of the observations. The scaling exponent mu of the auto correlation function of epsilon(t) has also been directly evaluated. It has the value of 0.37. Finally. the mean dissipation rate was determined, which could be used in solar wind heating models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.A14B..08L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.A14B..08L"><span><span class="hlt">Sea</span> Fog Forecasting with Lagrangian Models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lewis, J. M.</p> <p>2014-12-01</p> <p>In 1913, G. I. Taylor introduced us to a Lagrangian view of <span class="hlt">sea</span> fog formation. He conducted his study off the coast of Newfoundland in the aftermath of the Titanic disaster. We briefly review Taylor's classic work and then apply these same principles to a case of <span class="hlt">sea</span> fog formation and dissipation off the coast of California. The resources used in this study consist of: 1) land-based surface and upper-<span class="hlt">air</span> observations, 2) NDBC (National Data Buoy Center) observations from moored buoys equipped to measure dew point temperature as well as the standard surface observations at <span class="hlt">sea</span> (wind, <span class="hlt">sea</span> surface temperature, pressure, and <span class="hlt">air</span> temperature), 3) satellite observations of cloud, and 4) a one-dimensional (vertically directed) boundary layer model that tracks with the surface <span class="hlt">air</span> motion and makes use of sophisticated <span class="hlt">turbulence</span>-radiation parameterizations. Results of the investigation indicate that delicate interplay and interaction between the radiation and <span class="hlt">turbulence</span> processes makes accurate forecasts of <span class="hlt">sea</span> fog onset unlikely in the near future. This pessimistic attitude stems from inadequacy of the existing network of observations and uncertainties in modeling dynamical processes within the boundary layer.</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/2017APS..DPPJ11089F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..DPPJ11089F"><span><span class="hlt">Flux</span>-driven <span class="hlt">turbulence</span> GDB simulations of the IWL Alcator C-Mod L-mode edge compared with experiment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Francisquez, Manaure; Zhu, Ben; Rogers, Barrett</p> <p>2017-10-01</p> <p>Prior to predicting confinement regime transitions in tokamaks one may need an accurate description of L-mode profiles and <span class="hlt">turbulence</span> properties. These features determine the heat-<span class="hlt">flux</span> width upon which wall integrity depends, a topic of major interest for research aid to ITER. To this end our work uses the GDB model to simulate the Alcator C-Mod edge and contributes support for its use in studying critical edge phenomena in current and future tokamaks. We carried out 3D electromagnetic <span class="hlt">flux</span>-driven two-fluid <span class="hlt">turbulence</span> simulations of inner wall limited (IWL) C-Mod shots spanning closed and open <span class="hlt">flux</span> surfaces. These simulations are compared with gas puff imaging (GPI) and mirror Langmuir probe (MLP) data, examining global features and statistical properties of <span class="hlt">turbulent</span> dynamics. GDB reproduces important qualitative aspects of the C-Mod edge regarding global density and temperature profiles, within reasonable margins, and though the <span class="hlt">turbulence</span> statistics of the simulated <span class="hlt">turbulence</span> follow similar quantitative trends questions remain about the code's difficulty in exactly predicting quantities like the autocorrelation time A proposed breakpoint in the near SOL pressure and the posited separation between drift and ballooning dynamics it represents are examined This work was supported by DOE-SC-0010508. This research used resources of the National Energy Research Scientific Computing Center (NERSC).</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/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/2017JGRD..122.2289W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRD..122.2289W"><span>Physical controls on half-hourly, daily, and monthly <span class="hlt">turbulent</span> <span class="hlt">flux</span> and energy budget over a high-altitude small lake on the Tibetan Plateau</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Binbin; Ma, Yaoming; Ma, Weiqiang; Su, Zhongbo</p> <p>2017-02-01</p> <p>Precise measurements of evaporation and understanding of the physical controls on <span class="hlt">turbulent</span> heat <span class="hlt">flux</span> over lakes have fundamental significance for catchment-scale water balance analysis and local-scale climate modeling. The observation and simulation of lake-<span class="hlt">air</span> <span class="hlt">turbulent</span> <span class="hlt">flux</span> processes have been widely carried out, but studies that examine high-altitude lakes on the Tibetan Plateau are still rare, especially for small lakes. An eddy covariance (EC) system, together with a four-component radiation sensor and instruments for measuring water temperature profiles, was set up in a small lake within the Nam Co basin in April 2012 for long-term evaporation and energy budget observations. With the valuable measurements collected during the ice-free periods in 2012 and 2013, the main conclusions are summarized as follows: First, a bulk aerodynamic transfer model (B model), with parameters optimized for the specific wave pattern in the small lake, could provide reliable and consistent results with EC measurements, and B model simulations are suitable for data interpolation due to inadequate footprint or malfunction of the EC instrument. Second, the total evaporation in this small lake (812 mm) is approximately 200 mm larger than that from adjacent Nam Co (approximately 627 mm) during their ice-free seasons. Third, wind speed shows significance at temporal scales of half hourly, whereas water vapor and temperature gradients have higher correlations over temporal scales of daily and monthly in lake-<span class="hlt">air</span> <span class="hlt">turbulent</span> heat exchange. Finally, energy stored during April to June is mainly released during September to November, suggesting an energy balance closure value of 0.97.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AMT.....9.4375C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AMT.....9.4375C"><span><span class="hlt">Turbulence</span> <span class="hlt">fluxes</span> and variances measured with a sonic anemometer mounted on a tethered balloon</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Canut, Guylaine; Couvreux, Fleur; Lothon, Marie; Legain, Dominique; Piguet, Bruno; Lampert, Astrid; Maurel, William; Moulin, Eric</p> <p>2016-09-01</p> <p>This study presents the first deployment in field campaigns of a balloon-borne <span class="hlt">turbulence</span> probe, developed with a sonic anemometer and an inertial motion sensor suspended below a tethered balloon. This system measures temperature and horizontal and vertical wind at high frequency and allows the estimation of heat and momentum <span class="hlt">fluxes</span> as well as <span class="hlt">turbulent</span> kinetic energy in the lower part of the boundary layer. The system was validated during three field experiments with different convective boundary-layer conditions, based on <span class="hlt">turbulent</span> measurements from instrumented towers and aircraft.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19730013508','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19730013508"><span>The <span class="hlt">turbulent</span> mean-flow, Reynolds-stress, and heat <span class="hlt">flux</span> equations in mass-averaged dependent variables</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rubesin, M. W.; Rose, W. C.</p> <p>1973-01-01</p> <p>The time-dependent, <span class="hlt">turbulent</span> mean-flow, Reynolds stress, and heat <span class="hlt">flux</span> equations in mass-averaged dependent variables are presented. These equations are given in conservative form for both generalized orthogonal and axisymmetric coordinates. For the case of small viscosity and thermal conductivity fluctuations, these equations are considerably simpler than the general Reynolds system of dependent variables for a compressible fluid and permit a more direct extension of low speed <span class="hlt">turbulence</span> modeling to computer codes describing high speed <span class="hlt">turbulence</span> fields.</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('https://www.ncbi.nlm.nih.gov/pubmed/26367168','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26367168"><span>Enhanced backscatter of optical beams reflected in <span class="hlt">turbulent</span> <span class="hlt">air</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Nelson, W; Palastro, J P; Wu, C; Davis, C C</p> <p>2015-07-01</p> <p>Optical beams propagating through <span class="hlt">air</span> acquire phase distortions from <span class="hlt">turbulent</span> fluctuations in the refractive index. While these distortions are usually deleterious to propagation, beams reflected in a <span class="hlt">turbulent</span> medium can undergo a local recovery of spatial coherence and intensity enhancement referred to as enhanced backscatter (EBS). Here we validate the commonly used phase screen simulation with experimental results obtained from lab-scale experiments. We also verify theoretical predictions of the dependence of the <span class="hlt">turbulence</span> strength on EBS. Finally, we present a novel algorithm called the "tilt-shift method" which allows detection of EBS in frozen <span class="hlt">turbulence</span>, reducing the time required to detect the EBS signal.</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://hdl.handle.net/2060/19840019211','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19840019211"><span>Ocean waves and <span class="hlt">turbulence</span> as observed with an adaptive coherent multifrequency radar</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gjessing, D. T.; Hjelmstad, J.</p> <p>1984-01-01</p> <p>An adaptive coherent multifrequency radar system is developed for several applications. The velocity distribution (Doppler spectrum) and spectral intensity of 15 different irregularity scales (waves and <span class="hlt">turbulence</span>) can be measured simultaneously. Changing the azimuth angle of the antennas at regular intervals, the directivity of the wave/<span class="hlt">turbulence</span> pattern on the <span class="hlt">sea</span> surface can also be studied. A series of measurements for different <span class="hlt">air/sea</span> conditions are carried out from a coast based platform. Experiments in the Atlantic are also performed with the same equipment making use of the NASA Electra aircraft. The multifrequency radar allows the measurement of the velocity distribution (""coherent and incoherent component'') associated with 15 different ocean irregularity scales simultaneously in a directional manner. It is possible to study the different <span class="hlt">air/sea</span> mechanisms in some degree of detail.</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/2016OcMod.103..118M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016OcMod.103..118M"><span>On the modeling of wave-enhanced <span class="hlt">turbulence</span> nearshore</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moghimi, Saeed; Thomson, Jim; Özkan-Haller, Tuba; Umlauf, Lars; Zippel, Seth</p> <p>2016-07-01</p> <p>A high resolution k-ω two-equation <span class="hlt">turbulence</span> closure model, including surface wave forcing was employed to fully resolve <span class="hlt">turbulence</span> dissipation rate profiles close to the ocean surface. Model results were compared with observations from Surface Wave Instrument Floats with Tracking (SWIFTs) in the nearshore region at New River Inlet, North Carolina USA, in June 2012. A sensitivity analysis for different physical parameters and wave and <span class="hlt">turbulence</span> formulations was performed. The <span class="hlt">flux</span> of <span class="hlt">turbulent</span> kinetic energy (TKE) prescribed by wave dissipation from a numerical wave model was compared with the conventional prescription using the wind friction velocity. A surface roughness length of 0.6 times the significant wave height was proposed, and the <span class="hlt">flux</span> of TKE was applied at a distance below the mean <span class="hlt">sea</span> surface that is half of this roughness length. The wave enhanced layer had a total depth that is almost three times the significant wave height. In this layer the non-dimensionalized Terray scaling with power of - 1.8 (instead of - 2) was applicable.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016A%26A...588A.150K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016A%26A...588A.150K"><span>Magnetic <span class="hlt">flux</span> concentrations from <span class="hlt">turbulent</span> stratified convection</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Käpylä, P. J.; Brandenburg, A.; Kleeorin, N.; Käpylä, M. J.; Rogachevskii, I.</p> <p>2016-04-01</p> <p>Context. The formation of magnetic <span class="hlt">flux</span> concentrations within the solar convection zone leading to sunspot formation is unexplained. Aims: We study the self-organization of initially uniform sub-equipartition magnetic fields by highly stratified <span class="hlt">turbulent</span> convection. Methods: We perform simulations of magnetoconvection in Cartesian domains representing the uppermost 8.5-24 Mm of the solar convection zone with the horizontal size of the domain varying between 34 and 96 Mm. The density contrast in the 24 Mm deep models is more than 3 × 103 or eight density scale heights, corresponding to a little over 12 pressure scale heights. We impose either a vertical or a horizontal uniform magnetic field in a convection-driven <span class="hlt">turbulent</span> flow in set-ups where no small-scale dynamos are present. In the most highly stratified cases we employ the reduced sound speed method to relax the time step constraint arising from the high sound speed in the deep layers. We model radiation via the diffusion approximation and neglect detailed radiative transfer in order to concentrate on purely magnetohydrodynamic effects. Results: We find that super-equipartition magnetic <span class="hlt">flux</span> concentrations are formed near the surface in cases with moderate and high density stratification, corresponding to domain depths of 12.5 and 24 Mm. The size of the concentrations increases as the box size increases and the largest structures (20 Mm horizontally near the surface) are obtained in the models that are 24 Mm deep. The field strength in the concentrations is in the range of 3-5 kG, almost independent of the magnitude of the imposed field. The amplitude of the concentrations grows approximately linearly in time. The effective magnetic pressure measured in the simulations is positive near the surface and negative in the bulk of the convection zone. Its derivative with respect to the mean magnetic field, however, is positive in most of the domain, which is unfavourable for the operation of the negative</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-GSFC_20171208_Archive_e000949.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-GSFC_20171208_Archive_e000949.html"><span>The <span class="hlt">Turbulent</span> Bering <span class="hlt">Sea</span> [detail</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2017-12-08</p> <p>Large blooms of phytoplankton (likely coccolithophores) surrounded the 51-kilometer-long St. Matthew Island in the Bering <span class="hlt">Sea</span> on October 8, 2014 when the above Aqua-MODIS image was collected. The swirls and eddies of color give some indication of the <span class="hlt">turbulent</span> nature of these waters. The reflective blooms have been visible from orbit for a few months now. Credit: NASA/Goddard/Aqua/MODIS NASA image use policy. NASA Goddard Space Flight Center enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. Follow us on Twitter Like us on Facebook Find us on Instagram</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013PhDT........22R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013PhDT........22R"><span>The Development of Instrumentation and Methods for Measurement of <span class="hlt">Air-Sea</span> Interaction and Coastal Processes from Manned and Unmanned Aircraft</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Reineman, Benjamin D.</p> <p></p> <p>I present the development of instrumentation and methods for the measurement of coastal processes, ocean surface phenomena, and <span class="hlt">air-sea</span> interaction in two parts. In the first, I discuss the development of a portable scanning lidar (light detection and ranging) system for manned aircraft and demonstrate its functionality for oceanographic and coastal measurements. Measurements of the Southern California coastline and nearshore surface wave fields from seventeen research flights between August 2007 and December 2008 are analyzed and discussed. The October 2007 landslide on Mt. Soledad in La Jolla, California was documented by two of the flights. The topography, lagoon, reef, and surrounding wave field of Lady Elliot Island in Australia's Great Barrier Reef were measured with the airborne scanning lidar system on eight research flights in April 2008. Applications of the system, including coastal topographic surveys, wave measurements, ship wake studies, and coral reef research, are presented and discussed. In the second part, I detail the development of instrumentation packages for small (18 -- 28 kg) unmanned aerial vehicles (UAVs) to measure momentum <span class="hlt">fluxes</span> and latent, sensible, and radiative heat <span class="hlt">fluxes</span> in the atmospheric boundary layer (ABL), and the surface topography. Fast-response <span class="hlt">turbulence</span>, hygrometer, and temperature probes permit <span class="hlt">turbulent</span> momentum and heat <span class="hlt">flux</span> measurements, and short- and long-wave radiometers allow the determination of net radiation, surface temperature, and albedo. Careful design and testing of an accurate <span class="hlt">turbulence</span> probe, as demonstrated in this thesis, are essential for the ability to measure momentum and scalar <span class="hlt">fluxes</span>. The low altitude required for accurate <span class="hlt">flux</span> measurements (typically assumed to be 30 m) is below the typical safety limit of manned research aircraft; however, it is now within the capability of small UAV platforms. Flight tests of two instrumented BAE Manta UAVs over land were conducted in January 2011 at Mc</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ACP....18.5059D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ACP....18.5059D"><span>The influence of idealized surface heterogeneity on virtual <span class="hlt">turbulent</span> <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>De Roo, Frederik; Mauder, Matthias</p> <p>2018-04-01</p> <p>The imbalance of the surface energy budget in eddy-covariance measurements is still an unsolved problem. A possible cause is the presence of land surface heterogeneity, which affects the boundary-layer <span class="hlt">turbulence</span>. To investigate the impact of surface variables on the partitioning of the energy budget of <span class="hlt">flux</span> measurements in the surface layer under convective conditions, we set up a systematic parameter study by means of large-eddy simulation. For the study we use a virtual control volume approach, which allows the determination of advection by the mean flow, <span class="hlt">flux</span>-divergence and storage terms of the energy budget at the virtual measurement site, in addition to the standard <span class="hlt">turbulent</span> <span class="hlt">flux</span>. We focus on the heterogeneity of the surface <span class="hlt">fluxes</span> and keep the topography flat. The surface <span class="hlt">fluxes</span> vary locally in intensity and these patches have different length scales. Intensity and length scales can vary for the two horizontal dimensions but follow an idealized chessboard pattern. Our main focus lies on surface heterogeneity of the kilometer scale, and one order of magnitude smaller. For these two length scales, we investigate the average response of the <span class="hlt">fluxes</span> at a number of virtual towers, when varying the heterogeneity length within the length scale and when varying the contrast between the different patches. For each simulation, virtual measurement towers were positioned at functionally different positions (e.g., downdraft region, updraft region, at border between domains, etc.). As the storage term is always small, the non-closure is given by the sum of the advection by the mean flow and the <span class="hlt">flux</span>-divergence. Remarkably, the missing <span class="hlt">flux</span> can be described by either the advection by the mean flow or the <span class="hlt">flux</span>-divergence separately, because the latter two have a high correlation with each other. For kilometer scale heterogeneity, we notice a clear dependence of the updrafts and downdrafts on the surface heterogeneity and likewise we also see a dependence of the energy</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> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRD..123.2409X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRD..123.2409X"><span>Estimation of <span class="hlt">Turbulent</span> Heat <span class="hlt">Fluxes</span> by Assimilation of Land Surface Temperature Observations From GOES Satellites Into an Ensemble Kalman Smoother Framework</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xu, Tongren; Bateni, S. M.; Neale, C. M. U.; Auligne, T.; Liu, Shaomin</p> <p>2018-03-01</p> <p>In different studies, land surface temperature (LST) observations have been assimilated into the variational data assimilation (VDA) approaches to estimate <span class="hlt">turbulent</span> heat <span class="hlt">fluxes</span>. The VDA methods yield accurate <span class="hlt">turbulent</span> heat <span class="hlt">fluxes</span>, but they need an adjoint model, which is difficult to derive and code. They also cannot directly calculate the uncertainty of their estimates. To overcome the abovementioned drawbacks, this study assimilates LST data from Geostationary Operational Environmental Satellite into the ensemble Kalman smoother (EnKS) data assimilation system to estimate <span class="hlt">turbulent</span> heat <span class="hlt">fluxes</span>. EnKS does not need to derive the adjoint term and directly generates statistical information on the accuracy of its predictions. It uses the heat diffusion equation to simulate LST. EnKS with the state augmentation approach finds the optimal values for the unknown parameters (i.e., evaporative fraction and neutral bulk heat transfer coefficient, CHN) by minimizing the misfit between LST observations from Geostationary Operational Environmental Satellite and LST estimations from the heat diffusion equation. The augmented EnKS scheme is tested over six Ameriflux sites with a wide range of hydrological and vegetative conditions. The results show that EnKS can predict not only the model parameters and <span class="hlt">turbulent</span> heat <span class="hlt">fluxes</span> but also their uncertainties over a variety of land surface conditions. Compared to the variational method, EnKS yields suboptimal <span class="hlt">turbulent</span> heat <span class="hlt">fluxes</span>. However, suboptimality of EnKS is small, and its results are comparable to those of the VDA method. Overall, EnKS is a feasible and reliable method for estimation of <span class="hlt">turbulent</span> heat <span class="hlt">fluxes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19970010469','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19970010469"><span>Calibration of NASA <span class="hlt">Turbulent</span> <span class="hlt">Air</span> Motion Measurement System</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Barrick, John D. W.; Ritter, John A.; Watson, Catherine E.; Wynkoop, Mark W.; Quinn, John K.; Norfolk, Daniel R.</p> <p>1996-01-01</p> <p>A <span class="hlt">turbulent</span> <span class="hlt">air</span> motion measurement system (TAMMS) was integrated onboard the Lockheed 188 Electra airplane (designated NASA 429) based at the Wallops Flight Facility in support of the NASA role in global tropospheric research. The system provides <span class="hlt">air</span> motion and <span class="hlt">turbulence</span> measurements from an airborne platform which is capable of sampling tropospheric and planetary boundary-layer conditions. TAMMS consists of a gust probe with free-rotating vanes mounted on a 3.7-m epoxy-graphite composite nose boom, a high-resolution inertial navigation system (INS), and data acquisition system. A variation of the tower flyby method augmented with radar tracking was implemented for the calibration of static pressure position error and <span class="hlt">air</span> temperature probe. Additional flight calibration maneuvers were performed remote from the tower in homogeneous atmospheric conditions. System hardware and instrumentation are described and the calibration procedures discussed. Calibration and flight results are presented to illustrate the overall ability of the system to determine the three-component ambient wind fields during straight and level flight conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017Ge%26Ae..57..792A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Ge%26Ae..57..792A"><span>Diagnostics of <span class="hlt">Turbulent</span> Dynamo from the <span class="hlt">Flux</span> Emergence Rate in Solar Active Regions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Abramenko, V. I.; Tikhonova, O. I.; Kutsenko, A. S.</p> <p>2017-12-01</p> <p>Line-of-sight magnetograms acquired by the Helioseismic and Magnetic Imager (HMI) onboard the Solar Dynamic Observatory (SDO) and by the Michelson Doppler Imager (MDI) onboard the Solar and Heliospheric Observatory (SOHO) for 14 emerging ARs were used to study the derivative of the total unsigned <span class="hlt">flux</span>-the <span class="hlt">flux</span> emergence rate, R( t). We found that the emergence regime is not universal: each AR displays a unique emergence process. Nevertheless, two types of the emergence process can be identified. First type is a "regular" emergence with quasi-constant behavior of R( t) during a 1-3 day emergence interval with a rather low magnitude of the <span class="hlt">flux</span> derivative, R max = (0.57 ± 0.22) × 1022 Mx day-1. The second type can be described as "accelerated" emergence with a long interval (>1 day) of the rapidly increasing <span class="hlt">flux</span> derivative R( t) that result in a rather high magnitude of R max= (0.92 ± 0.29) × 1022 Mx day-1, which later changes to a very short (about a one third of day) interval of R( t) = const followed by a monotonous decrease of R( t). The first type events might be associated with emergence of a <span class="hlt">flux</span> tube with a constant amount of <span class="hlt">flux</span> that rises through the photosphere with a quasi-constant speed. Such events can be explained by the traditional largescale solar dynamo generating the toroidal <span class="hlt">flux</span> deep in the convective zone. The second-type events can be interpreted as a signature of sub-surface <span class="hlt">turbulent</span> dynamo action that generates additional magnetic <span class="hlt">flux</span> (via <span class="hlt">turbulent</span> motions) as the magnetic structure makes its way up to the solar surface.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_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://www.dtic.mil/docs/citations/AD1009191','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1009191"><span><span class="hlt">Turbulent</span> Structure Under Short Fetch Wind Waves</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2015-12-01</p> <p>1970) developed the LFT utilizing the concurrent measurement of <span class="hlt">sea</span> surface elevation (η) and the near surface velocities to isolate the wave...Layers and <span class="hlt">Air-Sea</span> Transfer program by making very high spatial resolution profile measurements of the 3-D velocity field into the crest-trough...distribution is unlimited <span class="hlt">TURBULENT</span> STRUCTURE UNDER SHORT FETCH WIND WAVES Michael J. Papa Lieutenant Commander, United States Navy B.S., United States Naval</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19860020813','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19860020813"><span>The physical and empirical basis for a specific clear-<span class="hlt">air</span> <span class="hlt">turbulence</span> risk index</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Keller, J. L.</p> <p>1986-01-01</p> <p>The fundamental emphasis of this research was to develop a technique which would be a significant improvement over those currently used for flight planning to avoid clear <span class="hlt">air</span> <span class="hlt">turbulence</span> (CAT). The technique should, ideally, be both quantitative in determining potential intensity and specific in locating regions of relatively high risk. Furthermore, it should not rely on specialized data but be functional using the currently available rawinsonde observation (raob) system. Encouraging results documented in an earlier investigation were considered compelling enough to warrant a closer look into the possibilities of a Specific Clear <span class="hlt">Air</span> <span class="hlt">Turbulence</span> Risk (SCATR) index approach to the clear <span class="hlt">air</span> <span class="hlt">turbulence</span> problem. Unlike that research, which considered sustained periods of flight in light to moderate clear <span class="hlt">air</span> <span class="hlt">turbulence</span>, this study focuses on several cases of documented severe CAT. Results of these case studies suggest that a SCATR index is not an unrealizable goal and that uses of such an index, event in its current prototype level of development, are also apparent.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010ems..confE..91M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010ems..confE..91M"><span>Meteorological factors controlling year-to-year variations in the spring onset of snow melt over the 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>Maksimovich, E.</p> <p>2010-09-01</p> <p>The spring onset of snow melt on the Arctic <span class="hlt">sea</span> ice shows large inter-annual variability. Surface melt triggers positive feedback mechanisms between the albedo, snow properties and thickness, as well as <span class="hlt">sea</span> ice thickness. Hence, it is important to quantify the factors contributing to inter-annual variability of the melt onset (MO) in various parts of the Arctic Ocean. Meteorological factors controlling surface heat budget and surface melting/freezing are the shortwave and longwave radiative <span class="hlt">fluxes</span> and the <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> of sensible and latent heat. These <span class="hlt">fluxes</span> depend on the weather conditions, including the radiative impact of clouds, heat advection and wind speed. We make use of SSM/I-based MO time series (Markus, Miller and Stroeve) and the ECMWF ERA Interim reanalysis on the meteorological conditions and surface <span class="hlt">fluxes</span>, both data sets spanning the period 1989-2008 and covering recent years with a rapid <span class="hlt">sea</span> ice decline. The advantage is that SSM/I-based MO time series are independent of the ERA-Interim data. Our objective is to investigate if there exists a physically consistent and statistically significant relationship between MO timing and corresponding meteorological conditions. Results based on the regression analysis between the MO timing and seasonal anomalies of surface longwave radiative <span class="hlt">fluxes</span> reveal strong relationships. Synoptic scale (3-14 days) anomalies in downward longwave radiation are essential in the Western Arctic. Regarding the longer history (20-60 days) the distinct contribution from the downward longwave radiative <span class="hlt">fluxes</span> is captured within the whole study region. Positive anomalies in the downward longwave radiation dominate over the simultaneous negative anomalies in the downward shortwave radiation. The anomalies in downward radiative <span class="hlt">fluxes</span> are consistent with the total column water vapor, <span class="hlt">sea</span> level pressure and 10-m wind direction. Sensible and latent heat <span class="hlt">fluxes</span> affect surface melt timing in the Beaufort <span class="hlt">Sea</span> and in the Atlantic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.A41M..07G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.A41M..07G"><span>Scaling Properties of <span class="hlt">Turbulent</span> Mixing for Scalars Measured at Arctic Terrestrial Sites</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Grachev, A. A.; Uttal, T.; Persson, O. P. G.; Crepinsek, S.; Fairall, C. W.; Albee, R.; Makshtas, A.; Kustov, V. Y.; Repina, I.; Artamonov, A. Y.</p> <p>2014-12-01</p> <p>Measurements of atmospheric <span class="hlt">turbulence</span> made at two different sites located near the coast of the Arctic Ocean at Eureka (Canadian territory of Nunavut) and Tiksi (East Siberia) are used to study <span class="hlt">turbulent</span> <span class="hlt">fluxes</span>, scaling laws for <span class="hlt">turbulent</span> mixing, dissipation rates, and structure parameters of various scalars (temperature, water vapour, and carbon dioxide). <span class="hlt">Turbulent</span> <span class="hlt">fluxes</span> along with other <span class="hlt">turbulent</span> statistics and mean meteorological data were measured continuously throughout the year and reported hourly at various levels on 10-m (Eureka) and 20-m (Tiksi) <span class="hlt">flux</span> towers. According to our data, strong upward sensible and latent heat <span class="hlt">fluxes</span> are observed throughout the summer months indicating unstable stratification on average. During the Polar winter and cold seasons when the <span class="hlt">air</span> temperature falls below freezing, the near-surface environment is generally stably stratified (downward sensible but upward latent heat <span class="hlt">fluxes</span>). It is found that observed temporal variability of the carbon dioxide vertical <span class="hlt">flux</span> for both sites was generally in phase with Monin-Obukhov stability parameter, z/L (L is the Obukhov length scale). On average the <span class="hlt">turbulent</span> <span class="hlt">flux</span> of carbon dioxide was mostly negative (uptake by the surface) for z/L < 0 and vice versa. Our study also analyses the similarity between the <span class="hlt">turbulent</span> mixing of sensible heat, water vapour, and carbon dioxide with a specific focus on the difference between the similarity functions for the dissipation rates. The work is supported by the NOAA Climate Program Office, the U.S. National Science Foundation (NSF) with award ARC 11-07428, and by the U.S. Civilian Research & Development Foundation (CRDF) with award RUG1-2976-ST-10.</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('http://adsabs.harvard.edu/abs/1995TellB..47..331V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1995TellB..47..331V"><span>Eddy correlation measurements of size-dependent cloud droplet <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> to complex terrain</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vong, Richard J.; Kowalski, Andrew S.</p> <p>1995-07-01</p> <p>An eddy correlation technique was used to measure the <span class="hlt">turbulent</span> <span class="hlt">flux</span> of cloud droplets to complex, forested terrain near the coast of Washington State during the spring of 1993. Excellent agreement was achieved for cloud liquid water content measured by two instruments. Substantial downward liquid water <span class="hlt">fluxes</span> of <img src="/entityImage/223C.gif" alt="~" border="0" style="font-weight: bold" align="BOTTOM"></img> 1mm per 24 h were measured at night during "steady and continuous" cloud events, about twice the magnitude of those measured by Beswick etal. in Scotland. Cloud water chemical <span class="hlt">fluxes</span> were estimated to represent up to 50% of the chemical deposition associated with precipitation at the site. An observed size-dependence in the <span class="hlt">turbulent</span> liquid water <span class="hlt">fluxes</span> suggested that both droplet impaction, which leads to downward <span class="hlt">fluxes</span>, and phase change processes, which can lead to upward <span class="hlt">fluxes</span>, consistently are important contributors to the eddy correlation results. The diameter below which phase change processes were important to observed <span class="hlt">fluxes</span> was shown to depend upon σL<img src="/entityImage/004c0304.gif" alt="L" border="0" style="font-weight: bold" align="BOTTOM"></img>, the relative standard deviation of the liquid water content (LWC) within a 30-min averaging period. The crossover from upward to downward LW <span class="hlt">flux</span> occurs at 8µm for steady and continuous cloud events but at <img src="/entityImage/223C.gif" alt="~" border="0" style="font-weight: bold" align="BOTTOM"></img> 13µm for events with a larger degree of LWC variability. This comparison of the two types of cloud events suggested that evaporation was the most likely cause of upward droplet <span class="hlt">fluxes</span> for the smaller droplets (dia<13µm) during cloud with variable LWC (σL<img src="/entityImage/004c0304.gif" alt="L" border="0" style="font-weight: bold" align="BOTTOM"></img>>0.3).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/10970675','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/10970675"><span><span class="hlt">Turbulence</span> and wave breaking effects on <span class="hlt">air</span>-water gas exchange</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Boettcher; Fineberg; Lathrop</p> <p>2000-08-28</p> <p>We present an experimental characterization of the effects of <span class="hlt">turbulence</span> and breaking gravity waves on <span class="hlt">air</span>-water gas exchange in standing waves. We identify two regimes that govern aeration rates: <span class="hlt">turbulent</span> transport when no wave breaking occurs and bubble dominated transport when wave breaking occurs. In both regimes, we correlate the qualitative changes in the aeration rate with corresponding changes in the wave dynamics. In the latter regime, the strongly enhanced aeration rate is correlated with measured acoustic emissions, indicating that bubble creation and dynamics dominate <span class="hlt">air</span>-water exchange.</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/2017JPlPh..83f9004B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JPlPh..83f9004B"><span>Driving magnetic <span class="hlt">turbulence</span> using <span class="hlt">flux</span> ropes in a moderate guide field linear system</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brookhart, Matthew I.; Stemo, Aaron; Waleffe, Roger; Forest, Cary B.</p> <p>2017-12-01</p> <p>We present a series of experiments on novel, line-tied plasma geometries as a study of the generation of chaos and <span class="hlt">turbulence</span> in line-tied systems. Plasma production and the injection scale for magnetic energy is provided by spatially discrete plasma guns that inject both plasma and current. The guns represent a technique for controlling the injection scale of magnetic energy. A two-dimensional (2-D) array of magnetic probes provides spatially resolved time histories of the magnetic fluctuations at a single cross-section of the experimental cylinder, allowing simultaneous spatial measurements of chaotic and <span class="hlt">turbulent</span> behaviour. The first experiment shows chaotic fluctuations and self-organization in a hollow-current line-tied screw pinch. These dynamics is modulated primarily by the applied magnetic field and weakly by the plasma current and safety factor. The second experiment analyses the interactions of multiple line-tied <span class="hlt">flux</span> ropes. The <span class="hlt">flux</span> ropes all exhibit chaotic behaviour, and under certain conditions develop an inverse cascade to larger scales and a <span class="hlt">turbulent</span> inertial range with magnetic energy ( ) related to perpendicular wave number ( \\bot $ ) as \\bot -2.5\\pm 0.5$ .</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/2016AGUFM.B24C..08M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.B24C..08M"><span>Methane and Carbon Dioxide Concentrations and <span class="hlt">Fluxes</span> in Amazon Floodplains</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Melack, J. M.; MacIntyre, S.; Forsberg, B.; Barbosa, P.; Amaral, J. H.</p> <p>2016-12-01</p> <p>Field studies on the central Amazon floodplain in representative aquatic habitats (open water, flooded forests, floating macrophytes) combine measurements of methane and carbon dioxide concentrations and <span class="hlt">fluxes</span> to the atmosphere over diel and seasonal times with deployment of meteorological sensors and high-resolution thermistors and dissolved oxygen sondes. A cavity ringdown spectrometer is used to determine gas concentrations, and floating chambers and bubble collectors are used to measure <span class="hlt">fluxes</span>. To further understand <span class="hlt">fluxes</span>, we measured <span class="hlt">turbulence</span> as rate of dissipation of <span class="hlt">turbulent</span> kinetic energy based on microstructure profiling. These results allow calculations of vertical mixing within the water column and of <span class="hlt">air</span>-water exchanges using surface renewal models. Methane and carbon dioxide <span class="hlt">fluxes</span> varied as a function of season, habitat and water depth. High CO2 <span class="hlt">fluxes</span> at high water are related to high pCO2; low pCO2 levels at low water result from increased phytoplankton uptake. CO2 <span class="hlt">fluxes</span> are highest at <span class="hlt">turbulent</span> open water sites, and pCO2 is highest in macrophyte beds. <span class="hlt">Fluxes</span> and pCH4 are high in macrophyte beds.</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/2016APS..DFDD17004D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..DFDD17004D"><span>Lagrangian analysis of premixed <span class="hlt">turbulent</span> combustion in hydrogen-<span class="hlt">air</span> flames</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Darragh, Ryan; Poludnenko, Alexei; Hamlington, Peter</p> <p>2016-11-01</p> <p>Lagrangian analysis has long been a tool used to analyze non-reacting <span class="hlt">turbulent</span> flows, and has recently gained attention in the reacting flow and combustion communities. The approach itself allows one to separate local molecular effects, such as those due to reactions or diffusion, from <span class="hlt">turbulent</span> advective effects along fluid pathlines, or trajectories. Accurate calculation of these trajectories can, however, be rather difficult due to the chaotic nature of <span class="hlt">turbulent</span> flows and the added complexity of reactions. In order to determine resolution requirements and verify the numerical algorithm, extensive tests are described in this talk for prescribed steady, unsteady, and chaotic flows, as well as for direct numerical simulations (DNS) of non-reacting homogeneous isotropic <span class="hlt">turbulence</span>. The Lagrangian analysis is then applied to DNS of premixed hydrogen-<span class="hlt">air</span> flames at two different <span class="hlt">turbulence</span> intensities for both single- and multi-step chemical mechanisms. Non-monotonic temperature and fuel-mass fraction evolutions are found to exist along trajectories passing through the flame brush. Such non-monotonicity is shown to be due to molecular diffusion resulting from large spatial gradients created by <span class="hlt">turbulent</span> advection. This work was supported by the <span class="hlt">Air</span> Force Office of Scientific Research (AFOSR) under Award No. FA9550-14-1-0273, and the Department of Defense (DoD) High Performance Computing Modernization Program (HPCMP) under a Frontier project award.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19860052580&hterms=marine+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dmarine%2Benergy','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19860052580&hterms=marine+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dmarine%2Benergy"><span><span class="hlt">Turbulence</span> in a convective marine atmospheric boundary layer</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.; Yeh, E.-N.</p> <p>1986-01-01</p> <p>The structure and kinetic energy budget of <span class="hlt">turbulence</span> in the convective marine atmospheric boundary layer as observed by aircraft during a cold <span class="hlt">air</span> outbreak have been studied using mixed layer scaling. The results are significantly different from those of previous studies under conditions closer to free convection. The normalized <span class="hlt">turbulent</span> kinetic energy and <span class="hlt">turbulent</span> transport are about twice those found during the <span class="hlt">Air</span> Mass Transformation Experiment (AMTEX). This implies that for a given surface heating the present case is dynamically more active. The difference is mainly due to the greater importance of wind shear in the present case. This case is closer to the roll vortex regime, whereas AMTEX observed mesoscale cellular convection which is closer to free convection. Shear generation is found to provide a significant energy source, in addition to buoyancy production, to maintain a larger normalized <span class="hlt">turbulent</span> kinetic energy and to balance a larger normalized dissipation. The interaction between <span class="hlt">turbulent</span> pressure and divergence (i.e., pressure scrambling) is also found to transfer energy from the vertical to the horizontal components, and is expected to be stronger in roll vortices than in m esoscale cells. The sensible heat <span class="hlt">flux</span> is found to fit well with a linear vertical profile in a clear or subcloud planetary boundary layer (PBL), in good agreement with the results of Lenschow et al., (1980). The heat <span class="hlt">flux</span> ratio between the PBL top and the surface, derived from the linear fitted curve, is approximately -0.14, in good agreement with that derived from the lidar data for the same case. Near the PBL top, the heat <span class="hlt">flux</span> profiles are consistent with those of Deardoff (1979) and Deardorff et al. (1980).</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/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 <span class="hlt">turbulent</span> 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://adsabs.harvard.edu/abs/2015EGUGA..17.7763G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.7763G"><span>The <span class="hlt">turbulence</span> structure of katabatic flows below and above wind-speed maximum</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Grachev, Andrey; Leo, Laura; Di Sabatino, Silvana; Fernando, Harindra; Pardyjak, Eric; Fairall, Christopher</p> <p>2015-04-01</p> <p>Measurements of atmospheric small-scale <span class="hlt">turbulence</span> made over the complex-terrain at the US Army Dugway Proving Grounds in Utah during the Mountain Terrain Atmospheric Modeling and Observations (MATERHORN) Program are used to describe the <span class="hlt">turbulence</span> structure of katabatic flows. <span class="hlt">Turbulent</span> and mean meteorological data were continuously measured at multiple levels (up to seven) on four towers deployed along East lower slope (2-4 degrees) of Granite Mountain. The multi-level, multi-tower observations obtained during a 30-day long MATERHORN-Fall field campaign in September-October 2102 allow studying temporal and spatial structure of nocturnal slope flows in detail. In this study, we focus on the various statistics (<span class="hlt">fluxes</span>, variances, spectra, cospectra, etc.) of the small-scale <span class="hlt">turbulence</span> of katabatic winds. Observed vertical profiles of velocity, <span class="hlt">turbulent</span> <span class="hlt">fluxes</span>, and other quantities show steep gradients near the surface but in the layer above the slope jet these variables vary with height more slowly than near the surface. It is found that vertical momentum <span class="hlt">flux</span> and horizontal heat (buoyancy) <span class="hlt">flux</span> in a slope-following coordinate system change their sign below and above the wind maximum of a katabatic flow. The vertical momentum <span class="hlt">flux</span> is directed downward (upward) whereas the horizontal heat <span class="hlt">flux</span> is downslope (upslope) below (above) the wind maximum. Our study, therefore, suggests that a position of the jet speed maximum can be derived from linear interpolation between positive and negative values of the momentum <span class="hlt">flux</span> (or the horizontal heat <span class="hlt">flux</span>) and determination of a height where a <span class="hlt">flux</span> becomes zero. It is shown that the standard deviations of all wind speed components (and therefore the <span class="hlt">turbulent</span> kinetic energy) and the dissipation rate of <span class="hlt">turbulent</span> kinetic energy have a local minimum, whereas the standard deviation of <span class="hlt">air</span> temperature has an absolute maximum at the height of wind speed maximum. We report several cases when the destructive effect of vertical heat</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 <span class="hlt">turbulence</span> 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/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('https://ntrs.nasa.gov/search.jsp?R=19750034251&hterms=stress+good&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dstress%2Bgood','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19750034251&hterms=stress+good&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dstress%2Bgood"><span>The measurement of shear stress and total heat <span class="hlt">flux</span> in a nonadiabatic <span class="hlt">turbulent</span> hypersonic boundary layer</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mikulla, V.; Horstman, C. C.</p> <p>1975-01-01</p> <p><span class="hlt">Turbulent</span> shear stress and direct <span class="hlt">turbulent</span> total heat-<span class="hlt">flux</span> measurements have been made across a nonadiabatic, zero pressure gradient, hypersonic boundary layer by using specially designed hot-wire probes free of strain-gauging and wire oscillation. Heat-<span class="hlt">flux</span> measurements were in reasonably good agreement with values obtained by integrating the energy equation using measured profiles of velocity and temperature. The shear-stress values deduced from the measurements, by assuming zero correlation of velocity and pressure fluctuations, were lower than the values obtained by integrating the momentum equation. Statistical properties of the cross-correlations are similar to corresponding incompressible measurements at approximately the same momentum-thickness Reynolds number.</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/2018OptCo.412..161Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018OptCo.412..161Z"><span>Spatial evolution of laser filaments in <span class="hlt">turbulent</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>Zeng, Tao; Zhu, Shiping; Zhou, Shengling; He, Yan</p> <p>2018-04-01</p> <p>In this study, the spatial evolution properties of laser filament clusters in <span class="hlt">turbulent</span> <span class="hlt">air</span> were evaluated using numerical simulations. Various statistical parameters were calculated, such as the percolation probability, filling factor, and average cluster size. The results indicate that <span class="hlt">turbulence</span>-induced multi-filamentation can be described as a new phase transition universality class. In addition, during this process, the relationship between the average cluster size and filling factor could be fit by a power function. Our results are valuable for applications involving filamentation that can be influenced by the geometrical features of multiple filaments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017NucFu..57k6025C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017NucFu..57k6025C"><span>Edge <span class="hlt">turbulence</span> and divertor heat <span class="hlt">flux</span> width simulations of Alcator C-Mod discharges using an electromagnetic two-fluid model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, B.; Xu, X. Q.; Xia, T. Y.; Porkolab, M.; Edlund, E.; LaBombard, B.; Terry, J.; Hughes, J. W.; Mao, S. F.; Ye, M. Y.; Wan, Y. X.</p> <p>2017-11-01</p> <p>The BOUT++ code has been exploited in order to improve the understanding of the role of <span class="hlt">turbulent</span> modes in controlling edge transport and resulting scaling of the scrape-off layer (SOL) heat <span class="hlt">flux</span> width. For the C-Mod enhanced D_α (EDA) H-mode discharges, BOUT++ six-field two-fluid nonlinear simulations show a reasonable agreement of upstream <span class="hlt">turbulence</span> and divertor target heat <span class="hlt">flux</span> behavior: (a) the simulated quasi-coherent modes show consistent characteristics of the frequency versus poloidal wave number spectra of the electromagnetic fluctuations when compared with experimental measurements: frequencies are around 60-120 kHz (experiment: about 70-110 kHz), k_θ are around 2.0 cm-1 which is similar to the phase contrast imaging data; (b) linear spectrum analysis is consistent with the nonlinear phase relationship calculation which indicates the dominance of resistive-ballooning modes and drift-Alfven wave instabilities; (c) the SOL heat <span class="hlt">flux</span> width λq versus current I p scaling is reproduced by <span class="hlt">turbulent</span> transport: the simulations yield similar λq to experimental measurements within a factor of 2. However the magnitudes of divertor heat <span class="hlt">fluxes</span> can be varied, depending on the physics models, sources and sinks, sheath boundary conditions, or <span class="hlt">flux</span> limiting coefficient; (d) Simple estimate by the ‘2-point model’ for λq is consistent with simulation. Moreover, blobby <span class="hlt">turbulent</span> spreading is confirmed for these relatively high B p shots.</p> </li> <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, <span class="hlt">turbulent</span>, 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('http://adsabs.harvard.edu/abs/2016EGUGA..1810951B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1810951B"><span>Gas transfer under high wind and its dependence on wave breaking and <span class="hlt">sea</span> state</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brumer, Sophia; Zappa, Christopher; Fairall, Christopher; Blomquist, Byron; Brooks, Ian; Yang, Mingxi</p> <p>2016-04-01</p> <p>Quantifying greenhouse gas <span class="hlt">fluxes</span> on regional and global scales relies on parameterizations of the gas transfer velocity K. To first order, K is dictated by wind speed (U) and is typically parameterized as a non-linear functions of U. There is however a large spread in K predicted by the traditional parameterizations at high wind speed. This is because a large variety of environmental forcing and processes (Wind, Currents, Rain, Waves, Breaking, Surfactants, Fetch) actually influence K and wind speed alone cannot capture the variability of <span class="hlt">air</span>-water gas exchange. At high wind speed especially, breaking waves become a key factor to take into account when estimating gas <span class="hlt">fluxes</span>. The High Wind Gas exchange Study (HiWinGS) presents the unique opportunity to gain new insights on this poorly understood aspects of <span class="hlt">air-sea</span> interaction under high winds. The HiWinGS cruise took place in the North Atlantic during October and November 2013. Wind speeds exceeded 15 m s-1 25% of the time, including 48 hrs with U10 > 20 m s-1. Continuous measurements of <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> of heat, momentum, and gas (CO2, DMS, acetone and methanol) were taken from the bow of the R/V Knorr. The wave field was sampled by a wave rider buoy and breaking events were tracked in visible imagery was acquired from the port and starboard side of the flying bridge during daylight hours at 20Hz. Taking advantage of the range of physical forcing and wave conditions sampled during HiWinGS, we test existing parameterizations and explore ways of better constraining K based on whitecap coverage, <span class="hlt">sea</span> state and breaking statistics contrasting pure windseas to swell dominated periods. We distinguish between windseas and swell based on a separation algorithm applied to directional wave spectra for mixed <span class="hlt">seas</span>, system alignment is considered when interpreting results. The four gases sampled during HiWinGS ranged from being mostly waterside controlled to almost entirely airside controlled. While bubble-mediated transfer</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRC..123.2172E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRC..123.2172E"><span><span class="hlt">Turbulence</span> Scaling Comparisons in the Ocean Surface Boundary Layer</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Esters, L.; Breivik, Ø.; Landwehr, S.; ten Doeschate, A.; Sutherland, G.; Christensen, K. H.; Bidlot, J.-R.; Ward, B.</p> <p>2018-03-01</p> <p>Direct observations of the dissipation rate of <span class="hlt">turbulent</span> kinetic energy, ɛ, under open ocean conditions are limited. Consequently, our understanding of what chiefly controls dissipation in the open ocean, and its functional form with depth, is poorly constrained. In this study, we report direct open ocean measurements of ɛ from the <span class="hlt">Air-Sea</span> Interaction Profiler (ASIP) collected during five different cruises in the Atlantic Ocean. We then combine these data with ocean-atmosphere <span class="hlt">flux</span> measurements and wave information in order to evaluate existing <span class="hlt">turbulence</span> scaling theories under a diverse set of open ocean conditions. Our results do not support the presence of a "breaking" or a "transition layer," which has been previously suggested. Instead, ɛ decays as |z|-1.29 over the depth interval, which was previously defined as "transition layer," and as |z|-1.15 over the mixing layer. This depth dependency does not significantly vary between nonbreaking or breaking wave conditions. A scaling relationship based on the friction velocity, the wave age, and the significant wave height describes the observations best for daytime conditions. For conditions during which convection is important, it is necessary to take buoyancy forcing into account.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1918509L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1918509L"><span>An eddy covariance system to characterize the atmospheric surface layer and <span class="hlt">turbulent</span> latent heat <span class="hlt">fluxes</span> over a debris-covered Himalayan glacier.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Litt, Maxime; Steiner, Jakob F.; Stigter, Emmy E.; Immerzeel, Walter; Shea, Joseph Michael</p> <p>2017-04-01</p> <p>Over debris-covered glaciers, water content variations in the debris layer can drive significant changes in its thermal conductivity and significantly impact melt rates. Since sublimation and evaporation are favoured in high-altitude conditions, e.g., low atmospheric pressure and high wind speeds, they are expected to strongly influence the water balance of the debris-layer. Dedicated latent heat <span class="hlt">fluxes</span> measurements at the debris surface are essential to characterize the debris heat conductivity in order to assess underlying ice melt. Furthermore, the contribution of the <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> in the surface energy balance over debris covered glacier remains uncertain since they are generally evaluated through similarity methods which might not be valid in complex terrain. We present the first results of a 15-day eddy-covariance experiment installed at the end of the monsoon (September-October) on a 3-m tower above the debris-covered Lirung glacier in Nepal. The tower also included measurements of the 4 radiation components. The eddy covariance measurements allowed for the characterization of the <span class="hlt">turbulence</span> in the atmospheric surface layer, as well as the direct measurements of evaporation, sublimation and <span class="hlt">turbulent</span> sensible heat <span class="hlt">fluxes</span>. The experiment helps us to evaluate the contribution of <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> to the surface energy balance over this debris-covered glacier, through a precise characterization of the overlying <span class="hlt">turbulent</span> atmospheric surface layer. It also helps to study the role of the debris-layer water content changes through evaporation and sublimation and its feedback on heat conduction in this layer. The large observed <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> play a significant role in the energy balance at the debris surface and significantly influence debris moisture, conductivity and subsequently underlying ice melt.</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/2014ApJ...780...87M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014ApJ...780...87M"><span><span class="hlt">Turbulent</span>, Extreme Multi-zone Model for Simulating <span class="hlt">Flux</span> and Polarization Variability in Blazars</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marscher, Alan P.</p> <p>2014-01-01</p> <p>The author presents a model for variability of the <span class="hlt">flux</span> and polarization of blazars in which <span class="hlt">turbulent</span> plasma flowing at a relativistic speed down a jet crosses a standing conical shock. The shock compresses the plasma and accelerates electrons to energies up to γmax >~ 104 times their rest-mass energy, with the value of γmax determined by the direction of the magnetic field relative to the shock front. The <span class="hlt">turbulence</span> is approximated in a computer code as many cells, each with a uniform magnetic field whose direction is selected randomly. The density of high-energy electrons in the plasma changes randomly with time in a manner consistent with the power spectral density of <span class="hlt">flux</span> variations derived from observations of blazars. The variations in <span class="hlt">flux</span> and polarization are therefore caused by continuous noise processes rather than by singular events such as explosive injection of energy at the base of the jet. Sample simulations illustrate the behavior of <span class="hlt">flux</span> and linear polarization versus time that such a model produces. The variations in γ-ray <span class="hlt">flux</span> generated by the code are often, but not always, correlated with those at lower frequencies, and many of the flares are sharply peaked. The mean degree of polarization of synchrotron radiation is higher and its timescale of variability shorter toward higher frequencies, while the polarization electric vector sometimes randomly executes apparent rotations. The slope of the spectral energy distribution exhibits sharper breaks than can arise solely from energy losses. All of these results correspond to properties observed in blazars.</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://hdl.handle.net/2060/19800002218','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19800002218"><span>Flow on Magnetizable Particles in <span class="hlt">Turbulent</span> <span class="hlt">Air</span> Streams. Ph.D. Thesis</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Davey, K. R.</p> <p>1979-01-01</p> <p>The flow of magnetizable particles in a <span class="hlt">turbulent</span> <span class="hlt">air</span> stream in the presence of an imposed magnetic field and the phenomenon of drag reduction produced by the introduction of particles in <span class="hlt">turbulent</span> boundary layer are investigated. The nature of the particle magnetic force is discussed and the inherent difference between electric and magnetic precipitation is considered. The incorporation of <span class="hlt">turbulent</span> diffusion theory with an imposed magnetic migration process both with and without inertia effects is examined.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A53I..05S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A53I..05S"><span>The role of <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> in the atmospheric boundary layer above a debris-covered glacier in the Himalayas</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Steiner, J. F.; Stigter, E.; Litt, M.; Shea, J.; Bierkens, M. F.; Immerzeel, W. W.</p> <p>2017-12-01</p> <p>Debris-covered glaciers play an important role in the water cycle in high altitude catchments in the Himalaya. The melt dynamics of these glaciers are complex as a result of the debris. A thin debris layer (up to a few cm) may act as a facilitator of melt, whereas a thick layer serves primarily as an insulator. The debris cover itself shows a strong diurnal variation in temperature and humidity resulting in a complex interaction with the atmospheric boundary layer (ABL). Energy balance models are a common way to quantify sub-debris melt, but the importance of <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> in this energy balance have so far been poorly investigated. We hypothesize that they may play a substantial role during phases of wetting and drying. In this study, ABL characteristics and surface <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> are measured using an automatic weather station including an eddy-correlation (EC) system on the debris-covered Lirung glacier in Nepal over a 10 day period in late 2016, during the transition period from monsoon to the drier post-monsoon. The measurements are combined with surface temperature measurements and thermal UAV flights covering the footprint area of the EC tower to quantify the surface <span class="hlt">fluxes</span> over a larger area. Our results show that <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> do play a substantial role in the energy balance of debris-covered glaciers, and need to be accounted for to accurately simulate glacier melt. The EC tower results are subsequently evaluated against a number of different bulk approaches to quantify sensible and latent heat <span class="hlt">fluxes</span> and are evaluated against <span class="hlt">turbulence</span> characteristics. If found accurate enough, these approaches require less advanced measurement set-ups and can be applied on a wider scale.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-GSFC_20171208_Archive_e000948.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-GSFC_20171208_Archive_e000948.html"><span>The <span class="hlt">Turbulent</span> Bering <span class="hlt">Sea</span> [full frame</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2017-12-08</p> <p>Large blooms of phytoplankton (likely coccolithophores) surrounded the 51-kilometer-long St. Matthew Island in the Bering <span class="hlt">Sea</span> on October 8, 2014 when the above Aqua-MODIS image was collected. The swirls and eddies of color give some indication of the <span class="hlt">turbulent</span> nature of these waters. The reflective blooms have been visible from orbit for a few months now. Credit: NASA/Goddard/Aqua/MODIS NASA image use policy. NASA Goddard Space Flight Center enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. Follow us on Twitter Like us on Facebook Find us on Instagram</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2000JGR...10529347C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2000JGR...10529347C"><span>Sources and sinks of ozone in savanna and forest areas during EXPRESSO: Airborne <span class="hlt">turbulent</span> <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>Cros, B.; Delon, C.; Affre, C.; Marion, T.; Druilhet, A.; Perros, P. E.; Lopez, A.</p> <p>2000-12-01</p> <p>An airborne study of ozone concentrations and <span class="hlt">fluxes</span> in the lower layers of the atmosphere was conducted over the Central African Republic (CAR) and northern Congo in November/December 1996, within the framework of the Experiment of Regional Sources and Sinks of Oxidants (EXPRESSO). The first 4 km of the atmosphere above savanna, rain forest, and the transitional area between them, were investigated with the French research aircraft Avion de Recherche Atmosphérique et de Télédétection (ARAT). <span class="hlt">Turbulent</span> <span class="hlt">fluxes</span> and deposition velocities of ozone were determined using the Eddy Correlation (EC) method. A specific methodology was developed to obtain accurate airborne <span class="hlt">turbulent</span> <span class="hlt">flux</span> measurements. This methodology is linked to the <span class="hlt">turbulence</span> stationarity. The average values of ozone <span class="hlt">fluxes</span> and ozone deposition velocities in the Atmospheric Boundary Layer (ABL) increase appreciably from savanna to forest. Near the ground, the ozone <span class="hlt">fluxes</span> range between -0.115 +/-0.073 ppbv m/s above savanna and -0.350 +/-0.115 ppbv m/s above forest; for the deposition, the ranges are 0.0042 +/-0.0018 m/s and 0.015 +/-0.004 m/s. A simple empirical relationship between deposition velocity and Leaf Area Index (LAI) is proposed, giving an estimation of the deposition velocity for a whole latitudinal band. Vertical inputs of ozone to the ABL are estimated according to entrainment <span class="hlt">fluxes</span>. The role of advection is neglected for horizontal transport of ozone in the ABL. The photochemical ozone production is deduced from the photo-stationary state deviation, and compared to the net ozone increase in the ABL during the flights performed above the forest. A tentative ozone budget based on the aircraft measurements is proposed in the ABL of the rain forest. Around noon, the photochemical production dominates with a net production of about 10 ppbv/h.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26367033','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26367033"><span>General scale-dependent anisotropic <span class="hlt">turbulence</span> and its impact on free space optical communication system performance.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Toselli, Italo; Korotkova, Olga</p> <p>2015-06-01</p> <p>We generalize a recently introduced model for nonclassic <span class="hlt">turbulent</span> spatial power spectrum involving anisotropy along two mutually orthogonal axes transverse to the direction of beam propagation by including two scale-dependent weighting factors for these directions. Such a <span class="hlt">turbulent</span> model may be pertinent to atmospheric fluctuations in the refractive index in stratified regions well above the boundary layer and employed for <span class="hlt">air-air</span> communication channels. When restricting ourselves to an unpolarized, coherent Gaussian beam and a weak <span class="hlt">turbulence</span> regime, we examine the effects of such a <span class="hlt">turbulence</span> type on the OOK FSO link performance by including the results on scintillation <span class="hlt">flux</span>, probability of fade, SNR, and BERs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040111369&hterms=Hassan&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAuthor-Name%26N%3D0%26No%3D60%26Ntt%3DHassan','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040111369&hterms=Hassan&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAuthor-Name%26N%3D0%26No%3D60%26Ntt%3DHassan"><span>Role of <span class="hlt">Turbulent</span> Prandtl Number on Heat <span class="hlt">Flux</span> at Hypersonic Mach Number</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Xiao, X.; Edwards, J. R.; Hassan, H. A.</p> <p>2004-01-01</p> <p>Present simulation of <span class="hlt">turbulent</span> flows involving shock wave/boundary layer interaction invariably overestimates heat <span class="hlt">flux</span> by almost a factor of two. One possible reason for such a performance is a result of the fact that the <span class="hlt">turbulence</span> models employed make use of Morkovin's hypothesis. This hypothesis is valid for non-hypersonic Mach numbers and moderate rates of heat transfer. At hypersonic Mach numbers, high rates of heat transfer exist in regions where shock wave/boundary layer interactions are important. As a result, one should not expect traditional <span class="hlt">turbulence</span> models to yield accurate results. The goal of this investigation is to explore the role of a variable Prandtl number formulation in predicting heat <span class="hlt">flux</span> in flows dominated by strong shock wave/boundary layer interactions. The intended applications involve external flows in the absence of combustion such as those encountered in supersonic inlets. This can be achieved by adding equations for the temperature variance and its dissipation rate. Such equations can be derived from the exact Navier-Stokes equations. Traditionally, modeled equations are based on the low speed energy equation where the pressure gradient term and the term responsible for energy dissipation are ignored. It is clear that such assumptions are not valid for hypersonic flows. The approach used here is based on the procedure used in deriving the k-zeta model, in which the exact equations that governed k, the variance of velocity, and zeta, the variance of vorticity, were derived and modeled. For the variable <span class="hlt">turbulent</span> Prandtl number, the exact equations that govern the temperature variance and its dissipation rate are derived and modeled term by term. The resulting set of equations are free of damping and wall functions and are coordinate-system independent. Moreover, modeled correlations are tensorially consistent and invariant under Galilean transformation. The final set of equations will be given in the paper.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22661035-proposed-paradigm-solar-cycle-dynamics-mediated-via-turbulent-pumping-magnetic-flux-babcockleighton-type-solar-dynamos','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22661035-proposed-paradigm-solar-cycle-dynamics-mediated-via-turbulent-pumping-magnetic-flux-babcockleighton-type-solar-dynamos"><span>A PROPOSED PARADIGM FOR SOLAR CYCLE DYNAMICS MEDIATED VIA <span class="hlt">TURBULENT</span> PUMPING OF MAGNETIC <span class="hlt">FLUX</span> IN BABCOCK–LEIGHTON-TYPE SOLAR DYNAMOS</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>Hazra, Soumitra; Nandy, Dibyendu</p> <p></p> <p>At present, the Babcock–Leighton <span class="hlt">flux</span> transport solar dynamo models appear to be the most promising models for explaining diverse observational aspects of the sunspot cycle. The success of these <span class="hlt">flux</span> transport dynamo models is largely dependent upon a single-cell meridional circulation with a deep equatorward component at the base of the Sun’s convection zone. However, recent observations suggest that the meridional flow may in fact be very shallow (confined to the top 10% of the Sun) and more complex than previously thought. Taken together, these observations raise serious concerns on the validity of the <span class="hlt">flux</span> transport paradigm. By accounting formore » the <span class="hlt">turbulent</span> pumping of magnetic <span class="hlt">flux</span>, as evidenced in magnetohydrodynamic simulations of solar convection, we demonstrate that <span class="hlt">flux</span> transport dynamo models can generate solar-like magnetic cycles even if the meridional flow is shallow. Solar-like periodic reversals are recovered even when meridional circulation is altogether absent. However, in this case, the solar surface magnetic field dynamics does not extend all the way to the polar regions. Very importantly, our results demonstrate that the Parker–Yoshimura sign rule for dynamo wave propagation can be circumvented in Babcock–Leighton dynamo models by the latitudinal component of <span class="hlt">turbulent</span> pumping, which can generate equatorward propagating sunspot belts in the absence of a deep, equatorward meridional flow. We also show that variations in <span class="hlt">turbulent</span> pumping coefficients can modulate the solar cycle amplitude and periodicity. Our results suggest the viability of an alternate magnetic <span class="hlt">flux</span> transport paradigm—mediated via <span class="hlt">turbulent</span> pumping—for sustaining solar-stellar dynamo action.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JOSAA..32.1371N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JOSAA..32.1371N"><span>Enhanced backscatter of optical beams reflected in <span class="hlt">turbulent</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>Nelson, W.; Palastro, J. P.; Wu, C.; Davis, C. C.</p> <p>2015-07-01</p> <p>Optical beams propagating through <span class="hlt">air</span> acquire phase distortions from <span class="hlt">turbulent</span> fluctuations in the refractive index. While these distortions are usually deleterious to propagation, beams reflected in a <span class="hlt">turbulent</span> medium can undergo a local recovery of spatial coherence and intensity enhancement referred to as enhanced backscatter (EBS). Using a combination of lab-scale experiments and simulations, we investigate the EBS of optical beams reflected from corner cubes and rough surfaces, and identify the regimes in which EBS is most distinctly observed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD0426812','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD0426812"><span>PHYSICAL MECHANISMS OF CLEAR-<span class="hlt">AIR</span> <span class="hlt">TURBULENCE</span>,</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p></p> <p>An attempt was made to test the hypothesis that reports of clear-<span class="hlt">air</span> <span class="hlt">turbulence</span> ( CAT ) on March 14-15, 1962, were associated with narrow layers (upper...did not contradict the hypothe sis, as many reports of CAT were made in sloping baroclinic or adiabatic layers. In any case, the Richardson numbers...index of CAT intensity which should be proportional to the energy of CAT is derived from the eddy energy equation. (Author)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70020906','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70020906"><span>Spatial variability of <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> in the roughness sublayer of an even-aged pine forest</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Katul, G.; Hsieh, C.-I.; Bowling, D.; Clark, K.; Shurpali, N.; Turnipseed, A.; Albertson, J.; Tu, K.; Hollinger, D.; Evans, B. M.; Offerle, B.; Anderson, D.; Ellsworth, D.; Vogel, C.; Oren, R.</p> <p>1999-01-01</p> <p>The spatial variability of <span class="hlt">turbulent</span> flow statistics in the roughness sublayer (RSL) of a uniform even-aged 14 m (= h) tall loblolly pine forest was investigated experimentally. Using seven existing walkup towers at this stand, high frequency velocity, temperature, water vapour and carbon dioxide concentrations were measured at 15.5 m above the ground surface from October 6 to 10 in 1997. These seven towers were separated by at least 100 m from each other. The objective of this study was to examine whether single tower <span class="hlt">turbulence</span> statistics measurements represent the flow properties of RSL <span class="hlt">turbulence</span> above a uniform even-aged managed loblolly pine forest as a best-case scenario for natural forested ecosystems. From the intensive space-time series measurements, it was demonstrated that standard deviations of longitudinal and vertical velocities (??(u), ??(w)) and temperature (??(T)) are more planar homogeneous than their vertical <span class="hlt">flux</span> of momentum (u(*)2) and sensible heat (H) counterparts. Also, the measured H is more horizontally homogeneous when compared to <span class="hlt">fluxes</span> of other scalar entities such as CO2 and water vapour. While the spatial variability in <span class="hlt">fluxes</span> was significant (> 15%), this unique data set confirmed that single tower measurements represent the 'canonical' structure of single-point RSL <span class="hlt">turbulence</span> statistics, especially <span class="hlt">flux</span>-variance relationships. Implications to extending the 'moving-equilibrium' hypothesis for RSL flows are discussed. The spatial variability in all RSL flow variables was not constant in time and varied strongly with spatially averaged friction velocity u(*), especially when u(*) was small. It is shown that flow properties derived from two-point temporal statistics such as correlation functions are more sensitive to local variability in leaf area density when compared to single point flow statistics. Specifically, that the local relationship between the reciprocal of the vertical velocity integral time scale (I(w)) and the arrival</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li class="active"><span>17</span></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_17 --> <div id="page_18" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="341"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://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 <span class="hlt">turbulent</span> <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 <span class="hlt">turbulent</span> 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/2007BoLMe.124..269P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007BoLMe.124..269P"><span>Divergence of <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> in the surface layer: case of a coastal city</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pigeon, G.; Lemonsu, A.; Grimmond, C. S. B.; Durand, P.; Thouron, O.; Masson, V.</p> <p>2007-08-01</p> <p>This study quantifies the processes that take place in the layer between the mean building height and the measurement level of an energy balance micrometeorological tower located in the dense old core of a coastal European city. The contributions of storage, vertical advection, horizontal advection and radiative divergence for heat are evaluated with the available measurements and with a three-dimensional, high-resolution meteorological simulation that had been evaluated against observations. The study focused on a summer period characterized by <span class="hlt">sea</span>-breeze flows that affect the city. In this specific configuration, it appears that the horizontal advection is the dominant term. During the afternoon when the <span class="hlt">sea</span> breeze is well established, correction of the sensible heat <span class="hlt">flux</span> with horizontal heat advection increases the measured sensible heat <span class="hlt">flux</span> up to 100 W m-2. For latent heat <span class="hlt">flux</span>, the horizontal moisture advection converted to equivalent latent heat <span class="hlt">flux</span> suggests a decrease of 50 W m-2. The simulation reproduces well the temporal evolution and magnitude of these terms.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017APS..DFD.M6003K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..DFD.M6003K"><span>Visualization of an <span class="hlt">air</span>-water interface on superhydrophobic surfaces in <span class="hlt">turbulent</span> channel flows</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kim, Hyunseok; Park, Hyungmin</p> <p>2017-11-01</p> <p>In the present study, three-dimensional deformation of <span class="hlt">air</span>-water interface on superhydrophobic surfaces in <span class="hlt">turbulent</span> channel flows at the Reynolds numbers of Re = 3000 and 10000 is measured with RICM (Reflection Interference Contrast Microscopy) technique. Two different types of roughness feature of circular hole and rectangular grate are considered, whose depth is 20 μm and diameter (or width) is varied between 20-200 μm. Since the <span class="hlt">air</span>-water interface is always at de-pinned state at the considered condition, <span class="hlt">air</span>-water interface shape and its sagging velocity is maintained to be almost constant as time goes one. In comparison with the previous results under the laminar flow, due to <span class="hlt">turbulent</span> characteristics of the flow, sagging velocity is much faster. Based on the measured sagging profiles, a modified model to describe the <span class="hlt">air</span>-water interface dynamics under <span class="hlt">turbulent</span> flows is suggested. Supported by City of Seoul through Seoul Urban Data Science Laboratory Project (Grant No 0660-20170004) administered by SNU Big Data Institute.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1816453M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1816453M"><span><span class="hlt">Turbulence</span> suppression at water density interfaces: observations under moderate wind forcing.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marcello Falcieri, Francesco; Kanth, Lakshmi H.; Benetazzo, Alvise; Bergamasco, Andrea; Bonaldo, Davide; Barbariol, Francesco; Malačič, Vlado; Sclavo, Mauro; Carniel, Sandro</p> <p>2016-04-01</p> <p>Water column stratification has a strong influence on the behaviour of <span class="hlt">turbulence</span> kinetic energy (TKE) dissipation rates. Density gradient interfaces, due to thermohaline characteristics and to suspended sediment concentration, can act as a barrier and significantly damp TKE. Between January 30th - February 4th 2014 (CARPET2014 oceanographic campaign on R/V URANIA) we collected the very first <span class="hlt">turbulence</span> data in the Gulf of Trieste (a small bay located in the North-eartern part of the Adriatic <span class="hlt">Sea</span>). Observation consisted of 38 CTD casts and 478 microstructure profiles (145 ensembles) collected with a free-falling probe (MSS90L). Among those 48 were grouped in three sets of yoyo casts, each lasting for about 12 consecutive hours. The meteorological conditions during the campaign were of moderate wind (average wind speed 10 m s-1) and heat <span class="hlt">flux</span> (net negative heat <span class="hlt">flux</span> ranging from 150 to 400 W m-2). The water column characteristics in the Gulf during the campaign evolved from well-mixed to stratified conditions with waters intruding from the Adriatic <span class="hlt">Sea</span> at the bottom. Two types of water intrusions were found during yoyo casts: one coming from the Adriatic <span class="hlt">Sea</span> northern coast (i.e. warmer, saltier and more turbid) and one coming from the open <span class="hlt">sea</span> in front of the Po Delta (i.e. cooler, fresher and less turbid). Our observations show that under moderate wind forcing, the GOT was not completely mixed due to the interfaces created by the bottom waters intruding from the open <span class="hlt">sea</span>. The comparison of microstructure profiles collected during well mixed and stratified conditions permitted us to highlight the effect of different stratification on TKE dissipation rates. While during well mixed condition TKE profiles are governed just by their forcing, the two intrusions showed different impacts on TKE dissipation rate profiles. The coastal one, with high turbidity, acted as a barrier to surface driven <span class="hlt">turbulence</span> dumping it of almost two order of magnitude, while the one coming</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PhPl...23d2306W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PhPl...23d2306W"><span>Numerical study of <span class="hlt">turbulence</span>-influence mechanism on arc characteristics in an <span class="hlt">air</span> direct current circuit breaker</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wu, Mingliang; Yang, Fei; Rong, Mingzhe; Wu, Yi; Qi, Yang; Cui, Yufei; Liu, Zirui; Guo, Anxiang</p> <p>2016-04-01</p> <p>This paper focuses on the numerical investigation of arc characteristics in an <span class="hlt">air</span> direct current circuit breaker (<span class="hlt">air</span> DCCB). Using magneto-hydrodynamics (MHD) theory, 3D laminar model and <span class="hlt">turbulence</span> model are constructed and calculated. The standard k-epsilon model is utilized to consider the <span class="hlt">turbulence</span> effect in the arc chamber of the DCCB. Several important phenomena are found: the arc column in the <span class="hlt">turbulence</span>-model case is more extensive, moves much more slowly than the counterpart in the laminar-model case, and shows stagnation at the entrance of the chamber, unlike in the laminar-model case. Moreover, the arc voltage in the <span class="hlt">turbulence</span>-model case is much lower than in the laminar-model case. However, the results in the <span class="hlt">turbulence</span>-model case show a much better agreement with the results of the breaking experiments under DC condition than in the laminar-model case, which is contradictory to the previous conclusions from the arc researches of both the low-voltage circuit breaker and the sulfur hexafluoride (SF6) nozzle. First, in the previous <span class="hlt">air</span>-arc research of the low-voltage circuit breaker, it is assumed that the <span class="hlt">air</span> plasma inside the chamber is in the state of laminar, and the laminar-model application gives quite satisfactory results compared with the experiments, while in this paper, the laminar-model application works badly. Second, the <span class="hlt">turbulence</span>-model application in the arc research of the SF6-nozzle performs much better and gives higher arc voltage than the laminar-model application does, whereas in this paper, the <span class="hlt">turbulence</span>-model application predicts lower arc voltage than the laminar-model application does. Based on the analysis of simulation results in detail, the mechanism of the above phenomena is revealed. The transport coefficients are strongly changed by <span class="hlt">turbulence</span>, which will enhance the arc diffusion and make the arc volume much larger. Consequently, the arc appearance and the distribution of Lorentz force in the <span class="hlt">turbulence</span>-model case</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1020274','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1020274"><span>Eddy Correlation <span class="hlt">Flux</span> Measurement System (ECOR) Handbook</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>Cook, DR</p> <p>2011-01-31</p> <p>The eddy correlation (ECOR) <span class="hlt">flux</span> measurement system provides in situ, half-hour measurements of the surface <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> of momentum, sensible heat, latent heat, and carbon dioxide (CO2) (and methane at one Southern Great Plains extended facility (SGP EF) and the North Slope of Alaska Central Facility (NSA CF). The <span class="hlt">fluxes</span> are obtained with the eddy covariance technique, which involves correlation of the vertical wind component with the horizontal wind component, the <span class="hlt">air</span> temperature, the water vapor density, and the CO2 concentration.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016ExFl...57..189C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016ExFl...57..189C"><span>Generating and controlling homogeneous <span class="hlt">air</span> <span class="hlt">turbulence</span> using random jet arrays</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carter, Douglas; Petersen, Alec; Amili, Omid; Coletti, Filippo</p> <p>2016-12-01</p> <p>The use of random jet arrays, already employed in water tank facilities to generate zero-mean-flow homogeneous <span class="hlt">turbulence</span>, is extended to <span class="hlt">air</span> as a working fluid. A novel facility is introduced that uses two facing arrays of individually controlled jets (256 in total) to force steady homogeneous <span class="hlt">turbulence</span> with negligible mean flow, shear, and strain. Quasi-synthetic jet pumps are created by expanding pressurized <span class="hlt">air</span> through small straight nozzles and are actuated by fast-response low-voltage solenoid valves. Velocity fields, two-point correlations, energy spectra, and second-order structure functions are obtained from 2D PIV and are used to characterize the <span class="hlt">turbulence</span> from the integral-to-the Kolmogorov scales. Several metrics are defined to quantify how well zero-mean-flow homogeneous <span class="hlt">turbulence</span> is approximated for a wide range of forcing and geometric parameters. With increasing jet firing time duration, both the velocity fluctuations and the integral length scales are augmented and therefore the Reynolds number is increased. We reach a Taylor-microscale Reynolds number of 470, a large-scale Reynolds number of 74,000, and an integral-to-Kolmogorov length scale ratio of 680. The volume of the present homogeneous <span class="hlt">turbulence</span>, the largest reported to date in a zero-mean-flow facility, is much larger than the integral length scale, allowing for the natural development of the energy cascade. The <span class="hlt">turbulence</span> is found to be anisotropic irrespective of the distance between the jet arrays. Fine grids placed in front of the jets are effective at modulating the <span class="hlt">turbulence</span>, reducing both velocity fluctuations and integral scales. Varying the jet-to-jet spacing within each array has no effect on the integral length scale, suggesting that this is dictated by the length scale of the jets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOS.A34B2644S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOS.A34B2644S"><span><span class="hlt">Turbulence</span> and Biological Productivity at Dongsha Reef in the S. 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>St Laurent, L.</p> <p>2016-02-01</p> <p>The combination of the Kuroshio Current, strong tides, topography, and stratification make the South China <span class="hlt">Sea</span> one of the most energetic energy cascade environments in the global ocean. Internal waves generated in the Luzon Strait emit into the South China <span class="hlt">Sea</span> as solitons, and propagate until they dissipate along the continental shelves of China and Vietnam. The abrupt conversion of solitons to nonlinear wave trains occurs as the waves pass onto the Dongsha Plateau. The Dongsha Reef at the center of the Plateau is directly in the path of the incoming waves. A measurement program during 2015 documented the energetic <span class="hlt">turbulence</span> that results as internal waves collide with the Reef. Glider based measurements of microstructure and optical properties showed that <span class="hlt">turbulent</span> mixing and transport are correlated to biological productivity. It is speculated that the existence of the Reef itself is the result of the breaking internal waves, which moderate the temperature and nutrient levels.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JAMES..10..770T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JAMES..10..770T"><span>An Extended Eddy-Diffusivity Mass-<span class="hlt">Flux</span> Scheme for Unified Representation of Subgrid-Scale <span class="hlt">Turbulence</span> and Convection</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tan, Zhihong; Kaul, Colleen M.; Pressel, Kyle G.; Cohen, Yair; Schneider, Tapio; Teixeira, João.</p> <p>2018-03-01</p> <p>Large-scale weather forecasting and climate models are beginning to reach horizontal resolutions of kilometers, at which common assumptions made in existing parameterization schemes of subgrid-scale <span class="hlt">turbulence</span> and convection—such as that they adjust instantaneously to changes in resolved-scale dynamics—cease to be justifiable. Additionally, the common practice of representing boundary-layer <span class="hlt">turbulence</span>, shallow convection, and deep convection by discontinuously different parameterizations schemes, each with its own set of parameters, has contributed to the proliferation of adjustable parameters in large-scale models. Here we lay the theoretical foundations for an extended eddy-diffusivity mass-<span class="hlt">flux</span> (EDMF) scheme that has explicit time-dependence and memory of subgrid-scale variables and is designed to represent all subgrid-scale <span class="hlt">turbulence</span> and convection, from boundary layer dynamics to deep convection, in a unified manner. Coherent up and downdrafts in the scheme are represented as prognostic plumes that interact with their environment and potentially with each other through entrainment and detrainment. The more isotropic <span class="hlt">turbulence</span> in their environment is represented through diffusive <span class="hlt">fluxes</span>, with diffusivities obtained from a <span class="hlt">turbulence</span> kinetic energy budget that consistently partitions <span class="hlt">turbulence</span> kinetic energy between plumes and environment. The cross-sectional area of up and downdrafts satisfies a prognostic continuity equation, which allows the plumes to cover variable and arbitrarily large fractions of a large-scale grid box and to have life cycles governed by their own internal dynamics. Relatively simple preliminary proposals for closure parameters are presented and are shown to lead to a successful simulation of shallow convection, including a time-dependent life cycle.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5947327','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5947327"><span>An Extended Eddy‐Diffusivity Mass‐<span class="hlt">Flux</span> Scheme for Unified Representation of Subgrid‐Scale <span class="hlt">Turbulence</span> and Convection</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Tan, Zhihong; Kaul, Colleen M.; Pressel, Kyle G.; Cohen, Yair; Teixeira, João</p> <p>2018-01-01</p> <p>Abstract Large‐scale weather forecasting and climate models are beginning to reach horizontal resolutions of kilometers, at which common assumptions made in existing parameterization schemes of subgrid‐scale <span class="hlt">turbulence</span> and convection—such as that they adjust instantaneously to changes in resolved‐scale dynamics—cease to be justifiable. Additionally, the common practice of representing boundary‐layer <span class="hlt">turbulence</span>, shallow convection, and deep convection by discontinuously different parameterizations schemes, each with its own set of parameters, has contributed to the proliferation of adjustable parameters in large‐scale models. Here we lay the theoretical foundations for an extended eddy‐diffusivity mass‐<span class="hlt">flux</span> (EDMF) scheme that has explicit time‐dependence and memory of subgrid‐scale variables and is designed to represent all subgrid‐scale <span class="hlt">turbulence</span> and convection, from boundary layer dynamics to deep convection, in a unified manner. Coherent up and downdrafts in the scheme are represented as prognostic plumes that interact with their environment and potentially with each other through entrainment and detrainment. The more isotropic <span class="hlt">turbulence</span> in their environment is represented through diffusive <span class="hlt">fluxes</span>, with diffusivities obtained from a <span class="hlt">turbulence</span> kinetic energy budget that consistently partitions <span class="hlt">turbulence</span> kinetic energy between plumes and environment. The cross‐sectional area of up and downdrafts satisfies a prognostic continuity equation, which allows the plumes to cover variable and arbitrarily large fractions of a large‐scale grid box and to have life cycles governed by their own internal dynamics. Relatively simple preliminary proposals for closure parameters are presented and are shown to lead to a successful simulation of shallow convection, including a time‐dependent life cycle. PMID:29780442</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://hdl.handle.net/2060/20150023475','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150023475"><span>The Impact of Trends in the Large Scale Atmospheric Circulation on Mediterranean Surface <span class="hlt">Turbulent</span> Heat <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>Romanski, Joy; Hameed, Sultan</p> <p>2015-01-01</p> <p>Interannual variations of latent heat <span class="hlt">fluxes</span> (LHF) and sensible heat <span class="hlt">fluxes</span> (SHF) over the Mediterranean for the boreal winter season (DJF) show positive trends during 1958-2011. Comparison of correlations between the heat <span class="hlt">fluxes</span> and the intensity and location of the Azores High (AH), and the NAO and East Atlantic-West Russia (EAWR) teleconnections, along with analysis of composites of surface temperature, humidity and wind fields for different teleconnection states, demonstrates that variations of the AH are found to explain the heat <span class="hlt">flux</span> changes more successfully than the NAO and the EAWR. Trends in <span class="hlt">sea</span> level pressure and longitude of the Azores High during DJF show a strengthening, and an eastward shift. DJF Azores High pressure and longitude are shown to co-vary such that variability of the Azores High occurs along an axis defined by lower pressure and westward location at one extreme, and higher pressure and eastward location at the other extreme. The shift of the Azores High from predominance of the low/west state to the high/east state induces trends in Mediterranean <span class="hlt">Sea</span> surface winds, temperature and moisture. These, combined with <span class="hlt">sea</span> surface warming trends, produce trends in wintertime Mediterranean <span class="hlt">Sea</span> sensible and latent heat <span class="hlt">fluxes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010ApJ...714..442S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010ApJ...714..442S"><span>Diffusion of Magnetic Field and Removal of Magnetic <span class="hlt">Flux</span> from Clouds Via <span class="hlt">Turbulent</span> Reconnection</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Santos-Lima, R.; Lazarian, A.; de Gouveia Dal Pino, E. M.; Cho, J.</p> <p>2010-05-01</p> <p>The diffusion of astrophysical magnetic fields in conducting fluids in the presence of <span class="hlt">turbulence</span> depends on whether magnetic fields can change their topology via reconnection in highly conducting media. Recent progress in understanding fast magnetic reconnection in the presence of <span class="hlt">turbulence</span> reassures that the magnetic field behavior in computer simulations and <span class="hlt">turbulent</span> astrophysical environments is similar, as far as magnetic reconnection is concerned. This makes it meaningful to perform MHD simulations of <span class="hlt">turbulent</span> flows in order to understand the diffusion of magnetic field in astrophysical environments. Our studies of magnetic field diffusion in <span class="hlt">turbulent</span> medium reveal interesting new phenomena. First of all, our three-dimensional MHD simulations initiated with anti-correlating magnetic field and gaseous density exhibit at later times a de-correlation of the magnetic field and density, which corresponds well to the observations of the interstellar media. While earlier studies stressed the role of either ambipolar diffusion or time-dependent <span class="hlt">turbulent</span> fluctuations for de-correlating magnetic field and density, we get the effect of permanent de-correlation with one fluid code, i.e., without invoking ambipolar diffusion. In addition, in the presence of gravity and <span class="hlt">turbulence</span>, our three-dimensional simulations show the decrease of the magnetic <span class="hlt">flux</span>-to-mass ratio as the gaseous density at the center of the gravitational potential increases. We observe this effect both in the situations when we start with equilibrium distributions of gas and magnetic field and when we follow the evolution of collapsing dynamically unstable configurations. Thus, the process of <span class="hlt">turbulent</span> magnetic field removal should be applicable both to quasi-static subcritical molecular clouds and cores and violently collapsing supercritical entities. The increase of the gravitational potential as well as the magnetization of the gas increases the segregation of the mass and magnetic <span class="hlt">flux</span> in the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003EAEJA.....5126S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003EAEJA.....5126S"><span>Evaluation of parameterization for <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> of momentum and heat in stably stratified surface layers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sodemann, H.; Foken, Th.</p> <p>2003-04-01</p> <p>General Circulation Models calculate the energy exchange between surface and atmosphere by means of parameterisations for <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> of momentum and heat in the surface layer. However, currently implemented parameterisations after Louis (1979) create large discrepancies between predictions and observational data, especially in stably stratified surface layers. This work evaluates a new surface layer parameterisation proposed by Zilitinkevich et al. (2002), which was specifically developed to improve energy <span class="hlt">flux</span> predictions in stable stratification. The evaluation comprises a detailed study of important surface layer characteristics, a sensitivity study of the parameterisation, and a direct comparison to observational data from Antarctica and predictions by the Louis (1979) parameterisation. The stability structure of the stable surface layer was found to be very complex, and strongly influenced <span class="hlt">fluxes</span> in the surface layer. The sensitivity study revealed that the new parameterisation depends strongly on the ratio between roughness length and roughness temperature, which were both observed to be very variable parameters. The comparison between predictions and measurements showed good agreement for momentum <span class="hlt">fluxes</span>, but large discrepancies for heat <span class="hlt">fluxes</span>. A stability dependent evaluation of selected data showed better agreement for the new parameterisation of Zilitinkevich et al. (2002) than for the Louis (1979) scheme. Nevertheless, this comparison underlines the need for more detailed and physically sound concepts for parameterisations of heat <span class="hlt">fluxes</span> in stably stratified surface layers. Zilitinkevich, S. S., V. Perov and J. C. King (2002). "Near-surface <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> in stable stratification: Calculation techniques for use in General Circulation Models." Q. J. R. Meteorol. Soc. 128(583): 1571--1587. Louis, J. F. (1979). "A Parametric Model of Vertical Eddy <span class="hlt">Fluxes</span> in the Atmosphere." Bound.-Layer Meteor. 17(2): 187--202.</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> <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/2017AGUFMGC21D0969Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC21D0969Z"><span>Uncertainty analysis of scintillometers methods in measuring sensible heat <span class="hlt">fluxes</span> of forest ecosystem</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zheng, N.</p> <p>2017-12-01</p> <p>Sensible heat <span class="hlt">flux</span> (H) is one of the driving factors of surface <span class="hlt">turbulent</span> motion and energy exchange. Therefore, it is particularly important to measure sensible heat <span class="hlt">flux</span> accurately at the regional scale. However, due to the heterogeneity of the underlying surface, hydrothermal regime, and different weather conditions, it is difficult to estimate the represented <span class="hlt">flux</span> at the kilometer scale. The scintillometer have been developed into an effective and universal equipment for deriving heat <span class="hlt">flux</span> at the regional-scale which based on the <span class="hlt">turbulence</span> effect of light in the atmosphere since the 1980s. The parameter directly obtained by the scintillometer is the structure parameter of the refractive index of <span class="hlt">air</span> based on the changes of light intensity fluctuation. Combine with parameters such as temperature structure parameter, zero-plane displacement, surface roughness, wind velocity, <span class="hlt">air</span> temperature and the other meteorological data heat <span class="hlt">fluxes</span> can be derived. These additional parameters increase the uncertainties of <span class="hlt">flux</span> because the difference between the actual feature of <span class="hlt">turbulent</span> motion and the applicable conditions of <span class="hlt">turbulence</span> theory. Most previous studies often focused on the constant <span class="hlt">flux</span> layers that are above the rough sub-layers and homogeneous flat surfaces underlying surfaces with suitable weather conditions. Therefore, the criteria and modified forms of key parameters are invariable. In this study, we conduct investment over the hilly area of northern China with different plants, such as cork oak, cedar-black and locust. On the basis of key research on the threshold and modified forms of saturation with different <span class="hlt">turbulence</span> intensity, modified forms of Bowen ratio with different drying-and-wetting conditions, universal function for the temperature structure parameter under different atmospheric stability, the dominant sources of uncertainty will be determined. The above study is significant to reveal influence mechanism of uncertainty and explore influence</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. <span class="hlt">Turbulence</span> 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('http://adsabs.harvard.edu/abs/2015AtmRe.164..328D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AtmRe.164..328D"><span>Fog chemical composition and its feedback to fog water <span class="hlt">fluxes</span>, water vapor <span class="hlt">fluxes</span>, and microphysical evolution of two events near Paris</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Degefie, D. T.; El-Madany, T.-S.; Held, M.; Hejkal, J.; Hammer, E.; Dupont, J.-C.; Haeffelin, M.; Fleischer, E.; Klemm, O.</p> <p>2015-10-01</p> <p>The chemical composition of collected fog water and its temporal evolution was studied during the PARISFOG campaign in winter 2012/2013 at the SIRTA (Site Instrumental de Recherche par Télédétection Atmosphéric) atmospheric observatory outside Paris, France. A further development of the caltech active fog collector was applied, in which the collected fog water gets into contact with Teflon and polyether ether ketone (PEEK) material exclusively. The collector was operational whenever the visibility was below 1000 m. In addition, the <span class="hlt">turbulent</span> and gravitational <span class="hlt">fluxes</span> of fog water and water vapor <span class="hlt">flux</span> were used to examine in detail the temporal evolution the chemical composition of two fogs. The technique was applied to two fog events, one representing a radiation fog and the other one representing a stratus lowering fog. The result revealed that the dominant inorganic species in the fog water were NH4+, NO3-, Ca2 + and SO42 -, which accounted for more than 85% of the ion balance. The pH ranged from 3.7 to 6.2. In the evolution the two fog events, the interaction among the <span class="hlt">turbulent</span> fog water <span class="hlt">flux</span>, gravitational fog water <span class="hlt">flux</span> and water vapor <span class="hlt">flux</span> controlled the major ion loads (amount of ions, dissolved in fog droplets per volume of <span class="hlt">air</span>) and ion concentrations (amount dissolved per volume of liquid water) of the fog water. In the radiation fog event, an increase of ion loads and ion concentrations occurred when the direction of water vapor <span class="hlt">flux</span> towards to the place where the condensation process occurred. A decrease of ion loads and ion concentrations mainly happened by gravitational fog water <span class="hlt">flux</span> with a minor contribution from <span class="hlt">turbulent</span> fog water <span class="hlt">flux</span>. However, when the <span class="hlt">turbulent</span> water vapor <span class="hlt">flux</span> was oriented downward, it turned the <span class="hlt">turbulent</span> fog water <span class="hlt">flux</span> upward and offset the removal of ions in the fog. In the stratus lowering fog event, the <span class="hlt">turbulent</span> fog water <span class="hlt">flux</span> and the gravitational water <span class="hlt">flux</span> together mainly contributed to the fog water deposition 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_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_18 --> <div id="page_19" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="361"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/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 <span class="hlt">turbulent</span> 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/2012APS..DPPTP8048U','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012APS..DPPTP8048U"><span>Analysis of plasma particle and energy <span class="hlt">fluxes</span> to material surfaces from tokamak edge <span class="hlt">turbulence</span> simulations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Umansky, M. V.; Cohen, B. I.; Rognlien, T. D.; Boedo, J. A.; Rudakov, D. L.</p> <p>2012-10-01</p> <p>Recent BOUT simulations of edge plasma <span class="hlt">turbulence</span> in L-mode regime in the boundary region of DIII-D tokamak have demonstrated reasonable match with key edge diagnostics [1]. Order-of-magnitude level agreement has been found in the characteristic amplitude, wavenumber, and frequency of <span class="hlt">turbulent</span> fluctuations, as compared with experimental data from reciprocating edge Langmuir probe and Beam Emission Spectroscopy systems. Owing to this encouraging agreement, output data from these simulations are analyzed to get insights on physical mechanisms and properties of plasma particle and energy <span class="hlt">fluxes</span> to material surfaces. Of particular interest is plasma <span class="hlt">turbulence</span> propagating into, or generated in, the far scrape-off layer region where plasma interacts with material walls. Results of statistical analyses of simulated <span class="hlt">turbulence</span> plasma transport will be presented and physical implications will be discussed. [4pt] [1] B.I. Cohen et al., APS-DPP 2012</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1035130','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1035130"><span><span class="hlt">Air-Sea</span> Interactions 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>2016-03-31</p> <p>Arctic Ocean has increased with the significant retreat of the seasonal <span class="hlt">sea</span>-ice extent. Here, we use wind, wave, <span class="hlt">turbulence</span>, and ice measurements to...which has experienced a significant retreat of the seasonal ice extent (Comiso and Nishio, 2008; Comiso et al., 2008). Thomson and Rogers (2014) showed</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017TCry...11..971L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017TCry...11..971L"><span>Surface-layer <span class="hlt">turbulence</span>, energy balance and links to atmospheric circulations over a mountain glacier in the French Alps</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Litt, Maxime; Sicart, Jean-Emmanuel; Six, Delphine; Wagnon, Patrick; Helgason, Warren D.</p> <p>2017-04-01</p> <p>Over Saint-Sorlin Glacier in the French Alps (45° N, 6.1° E; ˜ 3 km2) in summer, we study the atmospheric surface-layer dynamics, <span class="hlt">turbulent</span> <span class="hlt">fluxes</span>, their uncertainties and their impact on surface energy balance (SEB) melt estimates. Results are classified with regard to large-scale forcing. We use high-frequency eddy-covariance data and mean <span class="hlt">air</span>-temperature and wind-speed vertical profiles, collected in 2006 and 2009 in the glacier's atmospheric surface layer. We evaluate the <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> with the eddy-covariance (sonic) and the profile method, and random errors and parametric uncertainties are evaluated by including different stability corrections and assuming different values for surface roughness lengths. For weak synoptic forcing, local thermal effects dominate the wind circulation. On the glacier, weak katabatic flows with a wind-speed maximum at low height (2-3 m) are detected 71 % of the time and are generally associated with small <span class="hlt">turbulent</span> kinetic energy (TKE) and small net <span class="hlt">turbulent</span> <span class="hlt">fluxes</span>. Radiative <span class="hlt">fluxes</span> dominate the SEB. When the large-scale forcing is strong, the wind in the valley aligns with the glacier flow, intense downslope flows are observed, no wind-speed maximum is visible below 5 m, and TKE and net <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> are often intense. The net <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> contribute significantly to the SEB. The surface-layer <span class="hlt">turbulence</span> production is probably not at equilibrium with dissipation because of interactions of large-scale orographic disturbances with the flow when the forcing is strong or low-frequency oscillations of the katabatic flow when the forcing is weak. In weak forcing when TKE is low, all <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> calculation methods provide similar <span class="hlt">fluxes</span>. In strong forcing when TKE is large, the choice of roughness lengths impacts strongly the net <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> from the profile method <span class="hlt">fluxes</span> and their uncertainties. However, the uncertainty on the total SEB remains too high with regard to the net observed melt to be able to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22599120-numerical-study-turbulence-influence-mechanism-arc-characteristics-air-direct-current-circuit-breaker','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22599120-numerical-study-turbulence-influence-mechanism-arc-characteristics-air-direct-current-circuit-breaker"><span>Numerical study of <span class="hlt">turbulence</span>-influence mechanism on arc characteristics in an <span class="hlt">air</span> direct current circuit breaker</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>Wu, Mingliang; Yang, Fei, E-mail: yfei2007@mail.xjtu.edu.cn; Rong, Mingzhe</p> <p></p> <p>This paper focuses on the numerical investigation of arc characteristics in an <span class="hlt">air</span> direct current circuit breaker (<span class="hlt">air</span> DCCB). Using magneto-hydrodynamics (MHD) theory, 3D laminar model and <span class="hlt">turbulence</span> model are constructed and calculated. The standard k-epsilon model is utilized to consider the <span class="hlt">turbulence</span> effect in the arc chamber of the DCCB. Several important phenomena are found: the arc column in the <span class="hlt">turbulence</span>-model case is more extensive, moves much more slowly than the counterpart in the laminar-model case, and shows stagnation at the entrance of the chamber, unlike in the laminar-model case. Moreover, the arc voltage in the <span class="hlt">turbulence</span>-model case ismore » much lower than in the laminar-model case. However, the results in the <span class="hlt">turbulence</span>-model case show a much better agreement with the results of the breaking experiments under DC condition than in the laminar-model case, which is contradictory to the previous conclusions from the arc researches of both the low-voltage circuit breaker and the sulfur hexafluoride (SF6) nozzle. First, in the previous <span class="hlt">air</span>-arc research of the low-voltage circuit breaker, it is assumed that the <span class="hlt">air</span> plasma inside the chamber is in the state of laminar, and the laminar-model application gives quite satisfactory results compared with the experiments, while in this paper, the laminar-model application works badly. Second, the <span class="hlt">turbulence</span>-model application in the arc research of the SF6-nozzle performs much better and gives higher arc voltage than the laminar-model application does, whereas in this paper, the <span class="hlt">turbulence</span>-model application predicts lower arc voltage than the laminar-model application does. Based on the analysis of simulation results in detail, the mechanism of the above phenomena is revealed. The transport coefficients are strongly changed by <span class="hlt">turbulence</span>, which will enhance the arc diffusion and make the arc volume much larger. Consequently, the arc appearance and the distribution of Lorentz force in the <span class="hlt">turbulence</span></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 <span class="hlt">turbulence</span> dissipation at openings in the free surface. These 58 profiles are presently the most complete set of estimates of k across seasons and variable ice cover; as dissolved tracer budgets they reflect <span class="hlt">air-sea</span> gas exchange with no impact from <span class="hlt">air</span>-ice gas exchange.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ERL....13c4015W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ERL....13c4015W"><span>Effects of anthropogenic heat due to <span class="hlt">air</span>-conditioning systems on an extreme high temperature event in Hong Kong</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Y.; Li, Y.; Di Sabatino, S.; Martilli, A.; Chan, P. W.</p> <p>2018-03-01</p> <p>Anthropogenic heat <span class="hlt">flux</span> is the heat generated by human activities in the urban canopy layer, which is considered the main contributor to the urban heat island (UHI). The UHI can in turn increase the use and energy consumption of <span class="hlt">air</span>-conditioning systems. In this study, two effective methods for water-cooling <span class="hlt">air</span>-conditioning systems in non-domestic areas, including the direct cooling system and central piped cooling towers (CPCTs), are physically based, parameterized, and implemented in a weather research and forecasting model at the city scale of Hong Kong. An extreme high temperature event (June 23-28, 2016) in the urban areas was examined, and we assessed the effects on the surface thermal environment, the interaction of <span class="hlt">sea</span>-land breeze circulation and urban heat island circulation, boundary layer dynamics, and a possible reduction of energy consumption. The results showed that both water-cooled <span class="hlt">air</span>-conditioning systems could reduce the 2 m <span class="hlt">air</span> temperature by around 0.5 °C-0.8 °C during the daytime, and around 1.5 °C around 7:00-8:00 pm when the planetary boundary layer (PBL) height was confined to a few hundred meters. The CPCT contributed around 80%-90% latent heat <span class="hlt">flux</span> and significantly increased the water vapor mixing ratio in the atmosphere by around 0.29 g kg-1 on average. The implementation of the two alternative <span class="hlt">air</span>-conditioning systems could modify the heat and momentum of <span class="hlt">turbulence</span>, which inhibited the evolution of the PBL height (a reduction of 100-150 m), reduced the vertical mixing, presented lower horizontal wind speed and buoyant production of <span class="hlt">turbulent</span> kinetic energy, and reduced the strength of <span class="hlt">sea</span> breeze and UHI circulation, which in turn affected the removal of <span class="hlt">air</span> pollutants. Moreover, the two alternative <span class="hlt">air</span>-conditioning systems could significantly reduce the energy consumption by around 30% during extreme high temperature events. The results of this study suggest potential UHI mitigation strategies and can be extended to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMNG23A1823S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMNG23A1823S"><span>A Coupled Model of Langmuir Circulations and Ramp-like Structures in the Upper Ocean <span class="hlt">Turbulent</span> Boundary Layer</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.; Lukas, R.; Donelan, M. A.; Terray, E. A.</p> <p>2016-12-01</p> <p>Surface-wave breaking is a powerful mechanism producing significant energy <span class="hlt">flux</span> to small scale <span class="hlt">turbulence</span>. Most of the <span class="hlt">turbulent</span> energy produced by breaking waves dissipates within one significant wave height, while the <span class="hlt">turbulent</span> diffusion layer extends to approximately ten significant wave heights. Notably, the near-surface shear may practically vanish within the wave-stirred layer due to small-scale <span class="hlt">turbulent</span> mixing. The surface ocean temperature-salinity structure, circulation, and mass exchanges (including greenhouse gases and pollutants) substantially depend on <span class="hlt">turbulent</span> mixing and non-local transport in the near-surface layer of the ocean. Spatially coherent organized motions have been recognized as an important part of non-local transport. Langmuir circulation (LC) and ramp-like structures are believed to vertically transfer an appreciable portion of the momentum, heat, gases, pollutants (e.g., oil), and other substances in the upper layer of the ocean. Free surface significantly complicates the analysis of <span class="hlt">turbulent</span> exchanges at the <span class="hlt">air-sea</span> interface and the coherent structures are not yet completely understood. In particular, there is growing observational evidence that in the case of developing <span class="hlt">seas</span> when the wind direction may not coincide with the direction of the energy containing waves, the Langmuir lines are oriented in the wind rather than the wave direction. In addition, the vortex force due to Stokes drift in traditional models is altered in the breaking-wave-stirred layer. Another complication is that the ramp-like structures in the upper ocean <span class="hlt">turbulent</span> boundary layer have axes perpendicular to the axes of LC. The ramp-like structures are not considered in the traditional model. We have developed a new model, which treats the LC and ramp-like structures in the near-surface layer of the ocean as a coupled system. Using computational fluid dynamics tools (LES), we have been able to reproduce both LC and ramp-like structures coexisting in space</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('http://adsabs.harvard.edu/abs/2013AGUFMSM53A2208M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMSM53A2208M"><span>Spatial Transport of Magnetic <span class="hlt">Flux</span> Surfaces in Strongly Anisotropic <span class="hlt">Turbulence</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Matthaeus, W. H.; Servidio, S.; Wan, M.; Ruffolo, D. J.; Rappazzo, A. F.; Oughton, S.</p> <p>2013-12-01</p> <p>Magnetic <span class="hlt">flux</span> surfaces afford familiar descriptions of spatial structure, dynamics, and connectivity of magnetic fields, with particular relevance in contexts such as solar coronal <span class="hlt">flux</span> tubes, magnetic field connectivity in the interplanetary and interstellar medium, as well as in laboratory plasmas and dynamo problems [1-4]. Typical models assume that field-lines are orderly, and <span class="hlt">flux</span> tubes remain identifiable over macroscopic distances; however, a previous study has shown that <span class="hlt">flux</span> tubes shred in the presence of fluctuations, typically losing identity after several correlation scales [5]. Here, the structure of magnetic <span class="hlt">flux</span> surfaces is numerically investigated in a reduced magnetohydrodynamic (RMHD) model of homogeneous <span class="hlt">turbulence</span>. Short and long-wavelength behavior is studied statistically by propagating magnetic surfaces along the mean field. At small scales magnetic surfaces become complex, experiencing an exponential thinning. At large scales, instead, the magnetic <span class="hlt">flux</span> undergoes a diffusive behavior. The link between the diffusion of the coarse-grained <span class="hlt">flux</span> and field-line random walk is established by means of a multiple scale analysis. Both large and small scales limits are controlled by the Kubo number. These results have consequences for understanding and interpreting processes such as magnetic reconnection and field-line diffusion in plasmas [6]. [1] E. N. Parker, Cosmical Magnetic Fields (Oxford Univ. Press, New York, 1979). [2] J. R. Jokipii and E. N. Parker, Phys. Rev. Lett. 21, 44 (1968). [3] R. Bruno et al., Planet. Space Sci. 49, 1201 (2001). [4] M. N. Rosenbluth et al., Nuclear Fusion 6, 297 (1966). [5] W. H. Matthaeus et al., Phys. Rev. Lett. 75, 2136 (1995). [6] S. Servidio et al., submitted (2013).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19930094559','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19930094559"><span>Investigation of Ignition and Combustion Processes of Diesel Engines Operating with <span class="hlt">Turbulence</span> and <span class="hlt">Air</span>-storage Chambers</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Petersen, Hans</p> <p>1938-01-01</p> <p>The flame photographs obtained with combustion-chamber models of engines operating respectively, with <span class="hlt">turbulence</span> chamber and <span class="hlt">air</span>-storage chambers or cells, provide an insight into the <span class="hlt">air</span> and fuel movements that take place before and during combustion in the combustion chamber. The relation between <span class="hlt">air</span> velocity, start of injection, and time of combustion was determined for the combustion process employing a <span class="hlt">turbulence</span> chamber.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20060029193&hterms=air+measurement&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dair%2Bmeasurement','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060029193&hterms=air+measurement&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dair%2Bmeasurement"><span><span class="hlt">Sea</span> surface temperature measurements with <span class="hlt">AIRS</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Aumann, H.</p> <p>2003-01-01</p> <p>The comparison of global <span class="hlt">sea</span> surface skin temperature derived from cloud-free <span class="hlt">AIRS</span> super window channel at 2616 cm-1 (sst2616) with the Real-Time Global <span class="hlt">Sea</span> Surface Temperature for September 2002 shows surprisingly small standard deviation of 0.44K.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1912944Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1912944Y"><span><span class="hlt">Turbulence</span> influence on urban <span class="hlt">air</span> pollution in a hot spot in Madrid: comparison of winter and summer field campaigns</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yagüe, Carlos; Román-Cascón, Carlos; Sastre, Mariano; Maqueda, Gregorio; Arrillaga, Jon A.; Artiñano, Begoña; Díaz-Ramiro, Elías; Gómez-Moreno, Francisco J.; Borge, Rafael; Narros, Adolfo; Pérez, Javier; Quaassdorff, Christina</p> <p>2017-04-01</p> <p><span class="hlt">Air</span> pollution is a major problem in the city of Madrid during weak synoptic forcing, since the presence of atmospheric stability conditions often develops night surface-based thermal inversions and subsidence inversions during daytime for several consecutive days, reaching high levels of NOx and Particulate Matter (PM) concentration. In this context, the TECNAIRE-CM (Innovative technologies for the assessment and improvement of urban <span class="hlt">air</span> quality) research project has developed two field campaigns along 2015 (winter and summer) in a hot spot in the city of Madrid (Fernández Ladreda square). This hot spot includes one important intersection of different streets and also the start of the A42 motorway, which crosses down the square through a tunnel of about 150 m length. Besides, the location has numerous traffic lights and a lot of pedestrians walking in the vicinity. In addition to direct measurements related to <span class="hlt">air</span> quality, data from different meteorological variables were recorded in order to characterize the atmospheric conditions. Moreover, two sonic anemometers where deployed to carry out a micrometeorological assessment of physical processes that take place in the urban atmospheric surface layer (TKE, friction velocity and sensible heat <span class="hlt">flux</span> were evaluated). The evolution of the <span class="hlt">turbulence</span> will be analyzed and compared for both campaigns (winter and summer), searching for the key seasonal differences as well as the importance of the different scales influencing the diffusion of pollutants (from multi resolution <span class="hlt">flux</span> decomposition -MRFD- analysis). Specific case studies corresponding to high levels of pollution will be studied in detailed, to understand local pollution dynamics under the influence of both high traffic density and low <span class="hlt">turbulence</span> situations. This work has been financed by Madrid Regional Research Plan through TECNAIRE (P2013/MAE-2972).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25057511','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25057511"><span>Simulation analysis of <span class="hlt">air</span> flow and <span class="hlt">turbulence</span> statistics in a rib grit roughened duct.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Vogiatzis, I I; Denizopoulou, A C; Ntinas, G K; Fragos, V P</p> <p>2014-01-01</p> <p>The implementation of variable artificial roughness patterns on a surface is an effective technique to enhance the rate of heat transfer to fluid flow in the ducts of solar <span class="hlt">air</span> heaters. Different geometries of roughness elements investigated have demonstrated the pivotal role that vortices and associated <span class="hlt">turbulence</span> have on the heat transfer characteristics of solar <span class="hlt">air</span> heater ducts by increasing the convective heat transfer coefficient. In this paper we investigate the two-dimensional, <span class="hlt">turbulent</span>, unsteady flow around rectangular ribs of variable aspect ratios by directly solving the transient Navier-Stokes and continuity equations using the finite elements method. Flow characteristics and several aspects of <span class="hlt">turbulent</span> flow are presented and discussed including velocity components and statistics of <span class="hlt">turbulence</span>. The results reveal the impact that different rib lengths have on the computed mean quantities and <span class="hlt">turbulence</span> statistics of the flow. The computed <span class="hlt">turbulence</span> parameters show a clear tendency to diminish downstream with increasing rib length. Furthermore, the applied numerical method is capable of capturing small-scale flow structures resulting from the direct solution of Navier-Stokes and continuity equations.</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://hdl.handle.net/2060/20120011951','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120011951"><span>Simulation of a Wall-Bounded Flow using a Hybrid LES/RAS Approach with <span class="hlt">Turbulence</span> Recycling</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Quinlan, Jesse R.; Mcdaniel, James; Baurle, Robert A.</p> <p>2012-01-01</p> <p>Simulations of a supersonic recessed-cavity flow are performed using a hybrid large-eddy/ Reynolds-averaged simulation approach utilizing an inflow <span class="hlt">turbulence</span> recycling procedure and hybridized inviscid <span class="hlt">flux</span> scheme. Calorically perfect <span class="hlt">air</span> enters the three-dimensional domain at a free stream Mach number of 2.92. Simulations are performed to assess grid sensitivity of the solution, efficacy of the <span class="hlt">turbulence</span> recycling, and effect of the shock sensor used with the hybridized inviscid <span class="hlt">flux</span> scheme. Analysis of the <span class="hlt">turbulent</span> boundary layer upstream of the rearward-facing step for each case indicates excellent agreement with theoretical predictions. Mean velocity and pressure results are compared to Reynolds-averaged simulations and experimental data for each case, and these comparisons indicate good agreement on the finest grid. Simulations are repeated on a coarsened grid, and results indicate strong grid density sensitivity. The effect of <span class="hlt">turbulence</span> recycling on the solution is illustrated by performing coarse grid simulations with and without inflow <span class="hlt">turbulence</span> recycling. Two shock sensors, one of Ducros and one of Larsson, are assessed for use with the hybridized inviscid <span class="hlt">flux</span> reconstruction scheme.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.H33B1669L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.H33B1669L"><span><span class="hlt">Turbulent</span> water vapor exchanges and two source energy balance model estimated <span class="hlt">fluxes</span> of heterogeneous vineyard canopies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Los, S.; Hipps, L.; Alfieri, J. G.; Prueger, J. H.; Kustas, W. P.</p> <p>2017-12-01</p> <p>Agriculture in semi-arid regions is globally facing increasing stress on water resources. Hence, knowledge of water used in irrigated crops is essential for water resource management. However, quantifying spatial and temporal distribution of evapotranspiration (ET) has proven difficult because of the inherent complexities involved. Understanding of the complex biophysical relationships that govern ET is incomplete, particularly for heterogeneous vegetation. The USDA-ARS is developing a remotely-sensed ET modeling system that utilizes a two-source energy balance (TSEB) model capable of simulating <span class="hlt">turbulent</span> water and energy exchange from measurements of radiometric land surface temperature. The modeling system has been tested over a number of vegetated surfaces and is currently being validated for vineyard sites in the Central Valley of California through the Grape Remote sensing Atmospheric Profiling & Evapotranspiration eXperiment (GRAPEX). The highly variable, elevated canopy structure and semi-arid climatic conditions of these sites give the opportunity to gain knowledge of both <span class="hlt">turbulent</span> exchange processes and the TSEB model's ability to simulate <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> for heterogeneous vegetation. Analyzed are fast-response (20 Hz) 3-D velocity, temperature, and humidity measurements gathered over 4 years at two vineyard sites. These data were collected at a height of 5 m, within the surface layer but above the canopy, and at 1.5 m, below the canopy top. Power spectra and cross-spectra are used to study behavior of <span class="hlt">turbulent</span> water vapor exchanges and coupling between the canopy layer and surface layer under various atmospheric conditions. Frequent light winds and unstable daytime conditions, combined with the complicated canopy structure, often induce intermittent and episodic <span class="hlt">turbulence</span> transport. This resulted in a modal behavior alternating between periods of more continuous canopy venting and periods where water vapor <span class="hlt">fluxes</span> are dominated by transient, low</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> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_19 --> <div id="page_20" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="381"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.A13P..07S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.A13P..07S"><span><span class="hlt">Turbulence</span> characteristics of velocity and scalars in an internal boundary-layer above a lake</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sahlee, E.; Rutgersson, A.; Podgrajsek, E.</p> <p>2012-12-01</p> <p>We analyze <span class="hlt">turbulence</span> measurements, including methane, from a small island in a Swedish lake. The <span class="hlt">turbulence</span> structure was found to be highly influenced by the surrounding land during daytime. Variance spectra of both horizontal velocity and scalars during both unstable and stable stratification displayed a low frequency peak. The energy at lower frequencies displayed a daily variation, increasing in the morning and decreasing in the afternoon. We interpret this behavior as a sign of spectral lag, where the low frequency energy, large eddies, originate from the convective boundary layer above the surrounding land. When the <span class="hlt">air</span> is advected over the lake the small eddies rapidly equilibrates with new surface forcing. However, the larger eddies remain for an appreciable distance and influence the <span class="hlt">turbulence</span> in the developing lake boundary layer. The variance of the horizontal velocity is increased by these large eddies however, momentum <span class="hlt">fluxes</span> and scalar variances and <span class="hlt">fluxes</span> appear unaffected. The drag coefficient, Stanton number and Dalton number used to parameterize the momentum <span class="hlt">flux</span>, heat <span class="hlt">flux</span> and latent heat <span class="hlt">flux</span> respectively all compare very well with parameterizations developed for open ocean conditions.</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 <span class="hlt">turbulent</span> <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://adsabs.harvard.edu/abs/2016AGUFMOS23B2026K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS23B2026K"><span>A Study of Variations in Atmospheric <span class="hlt">Turbulence</span> Kinetic Energy on a Sandy Beach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Koscinski, J. S.; MacMahan, J. H.; Wang, Q.; Thornton, E. B.</p> <p>2016-12-01</p> <p>A 6-m high, meteorological tower consisting six evenly spaced ultrasonic anemometers and temperature-relative humidity sensors was deployed at the high tide line on sandy, wave-dissipative, meso-tidal beach in southern Monterey Bay, CA in October 2015. The micro-meteorology study focus is to explore the momentum <span class="hlt">fluxes</span> and <span class="hlt">turbulent</span> kinetic energy influenced by the interaction between an intensive wave-breaking surf zone and a sandy beach associated with onshore & cross-shore winds, diurnal heating, and differences in ocean-<span class="hlt">air</span> temperatures. The tower was deployed for approximately 1-month and experienced diurnal wind variations and synoptic storm events with winds measuring up to 10 m/s and an <span class="hlt">air</span> temperature range of 5-28 oC. This beach environment was found to be primarily unstable in thermal stratification indicating that the <span class="hlt">air</span> temperature is colder than underlying surface, either the ocean or the sandy beach. The drag coefficient was found to be dependent upon the atmospheric stability. Direct-estimates of atmospheric stability were obtained with the sonic anemometer. The direct estimates are a ratio of w*/u*, where the w*, vertically scaled buoyancy velocity, is greater than u*, horizontally scaled friction velocity. Hypotheses for the enhanced buoyancy are 1) diurnal heating of the sandy beach, 2) warmer ocean temperatures relative to <span class="hlt">air</span> temperatures, and 3) the wave breaking within the surf zone. Further exploration into these hypotheses is conducted by using vertical tower sensor pairs for estimating the temporal variability of the mechanical shear production and buoyancy production terms in <span class="hlt">turbulent</span> kinetic energy budget. These results are part of the Coastal Land <span class="hlt">Air</span> <span class="hlt">Sea</span> Interaction (CLASI) experiment.</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('http://www.ars.usda.gov/research/publications/publication/?seqNo115=309893','TEKTRAN'); return false;" href="http://www.ars.usda.gov/research/publications/publication/?seqNo115=309893"><span>Temperature regimes and <span class="hlt">turbulent</span> heat <span class="hlt">fluxes</span> across a heterogeneous canopy in an Alaskan boreal forest</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>We evaluate local differences in thermal regimes and <span class="hlt">turbulent</span> heat <span class="hlt">fluxes</span> across the heterogeneous canopy of a black spruce boreal forest on discontinuous permafrost in interior Alaska. The data was taken during an intensive observing period in the summer of 2013 from two micrometeorological tower...</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('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 <span class="hlt">turbulent</span> 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/29348695','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29348695"><span>Synchronization of Clocks Through 12 km of Strongly <span class="hlt">Turbulent</span> <span class="hlt">Air</span> Over a City.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sinclair, Laura C; Swann, William C; Bergeron, Hugo; Baumann, Esther; Cermak, Michael; Coddington, Ian; Deschênes, Jean-Daniel; Giorgetta, Fabrizio R; Juarez, Juan C; Khader, Isaac; Petrillo, Keith G; Souza, Katherine T; Dennis, Michael L; Newbury, Nathan R</p> <p>2016-10-15</p> <p>We demonstrate real-time, femtosecond-level clock synchronization across a low-lying, strongly <span class="hlt">turbulent</span>, 12-km horizontal <span class="hlt">air</span> path by optical two-way time transfer. For this long horizontal free-space path, the integrated <span class="hlt">turbulence</span> extends well into the strong <span class="hlt">turbulence</span> regime corresponding to multiple scattering with a Rytov variance up to 7 and with the number of signal interruptions exceeding 100 per second. Nevertheless, optical two-way time transfer is used to synchronize a remote clock to a master clock with femtosecond-level agreement and with a relative time deviation dropping as low as a few hundred attoseconds. Synchronization is shown for a remote clock based on either an optical or microwave oscillator and using either tip-tilt or adaptive-optics free-space optical terminals. The performance is unaltered from optical two-way time transfer in weak <span class="hlt">turbulence</span> across short links. These results confirm that the two-way reciprocity of the free-space time-of-flight is maintained both under strong <span class="hlt">turbulence</span> and with the use of adaptive optics. The demonstrated robustness of optical two-way time transfer against strong <span class="hlt">turbulence</span> and its compatibility with adaptive optics is encouraging for future femtosecond clock synchronization over very long distance ground-to-<span class="hlt">air</span> free-space paths.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5769483','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5769483"><span>Synchronization of Clocks Through 12 km of Strongly <span class="hlt">Turbulent</span> <span class="hlt">Air</span> Over a City</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Sinclair, Laura C.; Swann, William C.; Bergeron, Hugo; Baumann, Esther; Cermak, Michael; Coddington, Ian; Deschênes, Jean-Daniel; Giorgetta, Fabrizio R.; Juarez, Juan C.; Khader, Isaac; Petrillo, Keith G.; Souza, Katherine T.; Dennis, Michael L.; Newbury, Nathan R.</p> <p>2018-01-01</p> <p>We demonstrate real-time, femtosecond-level clock synchronization across a low-lying, strongly <span class="hlt">turbulent</span>, 12-km horizontal <span class="hlt">air</span> path by optical two-way time transfer. For this long horizontal free-space path, the integrated <span class="hlt">turbulence</span> extends well into the strong <span class="hlt">turbulence</span> regime corresponding to multiple scattering with a Rytov variance up to 7 and with the number of signal interruptions exceeding 100 per second. Nevertheless, optical two-way time transfer is used to synchronize a remote clock to a master clock with femtosecond-level agreement and with a relative time deviation dropping as low as a few hundred attoseconds. Synchronization is shown for a remote clock based on either an optical or microwave oscillator and using either tip-tilt or adaptive-optics free-space optical terminals. The performance is unaltered from optical two-way time transfer in weak <span class="hlt">turbulence</span> across short links. These results confirm that the two-way reciprocity of the free-space time-of-flight is maintained both under strong <span class="hlt">turbulence</span> and with the use of adaptive optics. The demonstrated robustness of optical two-way time transfer against strong <span class="hlt">turbulence</span> and its compatibility with adaptive optics is encouraging for future femtosecond clock synchronization over very long distance ground-to-<span class="hlt">air</span> free-space paths. PMID:29348695</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1313561-flux-driven-simulations-turbulence-collapse','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1313561-flux-driven-simulations-turbulence-collapse"><span><span class="hlt">Flux</span>-driven simulations of <span class="hlt">turbulence</span> collapse</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Park, G. Y.; Kim, S. S.; Jhang, Hogun; ...</p> <p>2015-03-12</p> <p>In this study, using self-consistent three-dimensional nonlinear simulations of tokamak <span class="hlt">turbulence</span>, we show that an edge transport barrier (ETB) forms naturally due to mean E x B shear feedback through evolving pressure gradient once input power exceeds a threshold value. The temporal evolution and development of the transition are elucidated. Profiles, <span class="hlt">turbulence</span>-driven flows and neoclassical coefficients are evolved self-consistently. A slow power ramp-up simulation shows that ETB transition is triggered by the <span class="hlt">turbulence</span>-driven flows via an intermediate phase which involves coherent oscillation of <span class="hlt">turbulence</span> intensity and E x B flow shear. A novel observation of the evolution is that themore » <span class="hlt">turbulence</span> collapses and the ETB transition begins when R T > 1 at t = t R (R T : normalized Reynolds power), while the conventional transition criterion (ω E x B > γlin) is satisfied only after t = t C (> t R), when the mean ow shear grows due to positive feedback.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1998PhDT........55A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1998PhDT........55A"><span><span class="hlt">Turbulent</span> convection in microchannels</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Adams, Thomas Mcdaniel</p> <p>1998-10-01</p> <p>Single-phase forced convection in microchannels is an effective cooling mechanism capable of accommodating the high heat <span class="hlt">fluxes</span> encountered in fission reactor cores, accelerator targets, microelectronic heat sinks and micro-heat exchangers. Traditional Nusselt type correlations, however, have generally been obtained using data from channels with hydraulic diameters >2 cm. Application of such relationships to microchannels is therefore questionable. A diameter limit below which traditional correlations are invalid had not been established. The objective of this investigation was to systematically address the effect of small hydraulic diameter on <span class="hlt">turbulent</span> single-phase forced convection of water. A number of microchannels having hydraulic diameters ranging from 0.76 to 1.13 mm were constructed and tested over a wide range of flow rates and heat <span class="hlt">fluxes</span>. Experimentally obtained Nusselt numbers were significantly higher than the values predicted by the Gnielinski correlation for large channels, the effect of decreasing diameter being to further increase heat transfer enhancement. A working correlation predicting the heat transfer enhancement for <span class="hlt">turbulent</span> convection in microchannels was developed. The correlation predicts the lower diameter limit below which traditional correlations are no longer valid to be approximately 1.2 mm. Of further interest was the effect of the desorption of noncondensable gases dissolved in the water on <span class="hlt">turbulent</span> convection. In large channels noncondensables undergo little desorption and their effect is negligible. The large pressure drops coupled with large temperature increases for high heat <span class="hlt">fluxes</span> in microchannels, however, leads to a two-phase, two-component flow thereby enhancing heat transfer coefficients above their liquid- only values. A detailed mathematical model was developed to predict the resulting void fractions and liquid- coolant accelerations due to the desorption of noncondensables in microchannels. Experiments were also</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1910024R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1910024R"><span>Under-ice <span class="hlt">turbulent</span> microstructure and upper ocean vertical <span class="hlt">fluxes</span> in the Makarov and Eurasian basins, Arctic Ocean, during late spring and late summer / autumn in 2015</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rabe, Benjamin; Janout, Markus; Graupner, Rainer; Hoelemann, Jens; Hampe, Hendrik; Hoppmann, Mario; Horn, Myriel; Juhls, Bennet; Korhonen, Meri; Nikolopoulos, Anna; Pisarev, Sergey; Randelhoff, Achim; Savy, Jean-Philippe; Villacieros Robineau, Nicolas</p> <p>2017-04-01</p> <p>The Arctic Ocean is generally assumed to be fairly quiescent when compared to many other oceans. The <span class="hlt">sea</span>-ice cover, a strong halocline and a shallow, cold mixed-layer prevents much of the ocean to be affected by atmospheric conditions and properties of the ocean mixed-layer. In turn, the mixed-layer and the <span class="hlt">sea</span>-ice is largely isolated from the warm layer of Atlantic origin below by the lower halocline. Yet, the content of heat, freshwater and biologically important nutrients differs strongly between these different layers. Hence, it is crucial to be able to estimate vertical <span class="hlt">fluxes</span> of salt, heat and nutrients to understand variability in the upper Arctic Ocean and the <span class="hlt">sea</span>-ice, including the ecosystem. Yet, it is difficult to obtain direct <span class="hlt">flux</span> measurements, and estimates are sparse. We present several sets of under-ice <span class="hlt">turbulent</span> microstructure profiles in the Eurasian and Makarov Basin of the Arctic Ocean from two expeditions, in 2015. These cover melt during late spring north of Svalbard and freeze-up during late summer / autumn across the Eurasian and Makarov basins. Our results are presented against a background of the anomalously warm atmospheric conditions during summer 2015 followed by unusually low temperatures in September. 4 - 24 h averages of the measurements generally show elevated dissipation rates at the base of the mixed-layer. We found highest levels of dissipation near the Eurasian continental slope and smaller peaks in the profiles where Bering <span class="hlt">Sea</span> Summer Water (sBSW) lead to additional stratification within the upper halocline in the Makarov Basin. The elevated levels of dissipation associated with sBSW and the base of the mixed-layer were associated with the relatively low levels of vertical eddy diffusivity. We discuss these findings in the light of the anomalous conditions in the upper ocean, <span class="hlt">sea</span>-ice and the atmosphere during 2015 and present estimates of vertical <span class="hlt">fluxes</span> of heat, salt and other dissolved substances measured in water samples.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1810602G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1810602G"><span>Annual and latitudinal variations of surface <span class="hlt">fluxes</span> and meteorological variables at Arctic terrestrial sites</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Grachev, Andrey; Uttal, Taneil; Persson, Ola; Konopleva-Akish, Elena; Crepinsek, Sara; Cox, Christopher; Fairall, Christopher; Makshtas, Alexander; Repina, Irina</p> <p>2016-04-01</p> <p>This study analyzes and discusses seasonal and latitudinal variations of surface <span class="hlt">fluxes</span> (<span class="hlt">turbulent</span>, radiative, and soil ground heat) and other ancillary surface/snow/permafrost data based on in-situ measurements made at two long-term research observatories near the coast of the Arctic Ocean located in Canada and Russia. The hourly averaged data collected at Eureka (Canadian territory of Nunavut) and Tiksi (East Siberia) located at two quite different latitudes (80.0 N and 71.6 N respectively) are analyzed in details to describe the seasons in the Arctic. Although Eureka and Tiksi are located at the different continents and at the different latitudes, the annual course of the surface meteorology and the surface <span class="hlt">fluxes</span> are qualitatively very similar. The <span class="hlt">air</span> and soil temperatures display the familiar strong seasonal trend with maximum of measured temperatures in mid-summer and minimum during winter. According to our data, variation in incoming short-wave solar radiation led the seasonal pattern of the <span class="hlt">air</span> and soil temperatures, and the <span class="hlt">turbulent</span> <span class="hlt">fluxes</span>. During the dark Polar nights, <span class="hlt">air</span> and ground temperatures are strongly controlled by long-wave radiation associated generally with cloud cover. Due to the fact that in average the higher latitudes receive less solar radiation than lower latitudes, a length of the convective atmospheric boundary layer (warm season) is shorter and middle-summer amplitude of the <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> is generally less in Eureka than in Tiksi. However, since solar elevation angle at local midnight in the middle of Arctic summer is higher for Eureka as compared to Tiksi, stable stratification and upward <span class="hlt">turbulent</span> <span class="hlt">flux</span> for carbon dioxide is generally did not observed at Eureka site during summer seasons. It was found a high correlation between the <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> of sensible and latent heat, carbon dioxide and the net solar radiation. A comprehensive evaluation of energy balance closure problem is performed based on the multi-year data sets</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 <span class="hlt">Turbulent</span> <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('https://www.osti.gov/biblio/1043299-turbulent-flame-wall-interaction-dns-study','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1043299-turbulent-flame-wall-interaction-dns-study"><span><span class="hlt">Turbulent</span> flame-wall interaction: a DNS study</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Chen, Jackie; Hawkes, Evatt R; Sankaran, Ramanan</p> <p>2010-01-01</p> <p>A <span class="hlt">turbulent</span> flame-wall interaction (FWI) configuration is studied using three-dimensional direct numerical simulation (DNS) and detailed chemical kinetics. The simulations are used to investigate the effects of the wall <span class="hlt">turbulent</span> boundary layer (i) on the structure of a hydrogen-<span class="hlt">air</span> premixed flame, (ii) on its near-wall propagation characteristics and (iii) on the spatial and temporal patterns of the convective wall heat <span class="hlt">flux</span>. Results show that the local flame thickness and propagation speed vary between the core flow and the boundary layer, resulting in a regime change from flamelet near the channel centreline to a thickened flame at the wall. This findingmore » has strong implications for the modelling of <span class="hlt">turbulent</span> combustion using Reynolds-averaged Navier-Stokes or large-eddy simulation techniques. Moreover, the DNS results suggest that the near-wall coherent <span class="hlt">turbulent</span> structures play an important role on the convective wall heat transfer by pushing the hot reactive zone towards the cold solid surface. At the wall, exothermic radical recombination reactions become important, and are responsible for approximately 70% of the overall heat release rate at the wall. Spectral analysis of the convective wall heat <span class="hlt">flux</span> provides an unambiguous picture of its spatial and temporal patterns, previously unobserved, that is directly related to the spatial and temporal characteristic scalings of the coherent near-wall <span class="hlt">turbulent</span> structures.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19780019748','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19780019748"><span>A scheme for computing surface layer <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> from mean flow surface observations</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hoffert, M. I.; Storch, J.</p> <p>1978-01-01</p> <p>A physical model and computational scheme are developed for generating <span class="hlt">turbulent</span> surface stress, sensible heat <span class="hlt">flux</span> and humidity <span class="hlt">flux</span> from mean velocity, temperature and humidity at some fixed height in the atmospheric surface layer, where conditions at this reference level are presumed known from observations or the evolving state of a numerical atmospheric circulation model. The method is based on coupling the Monin-Obukov surface layer similarity profiles which include buoyant stability effects on mean velocity, temperature and humidity to a force-restore formulation for the evolution of surface soil temperature to yield the local values of shear stress, heat <span class="hlt">flux</span> and surface temperature. A self-contained formulation is presented including parameterizations for solar and infrared radiant <span class="hlt">fluxes</span> at the surface. Additional parameters needed to implement the scheme are the thermal heat capacity of the soil per unit surface area, surface aerodynamic roughness, latitude, solar declination, surface albedo, surface emissivity and atmospheric transmissivity to solar radiation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930064218&hterms=engine+step+step&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dengine%2Bstep%2Bstep','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930064218&hterms=engine+step+step&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dengine%2Bstep%2Bstep"><span>Comparison of liquid rocket engine base region heat <span class="hlt">flux</span> computations using three <span class="hlt">turbulence</span> models</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kumar, Ganesh N.; Griffith, Dwaine O., II; Prendergast, Maurice J.; Seaford, C. M.</p> <p>1993-01-01</p> <p>The flow in the base region of launch vehicles is characterized by flow separation, flow reversals, and reattachment. Computation of the convective heat <span class="hlt">flux</span> in the base region and on the nozzle external surface of Space Shuttle Main Engine and Space Transportation Main Engine (STME) is an important part of defining base region thermal environments. Several <span class="hlt">turbulence</span> models were incorporated in a CFD code and validated for flow and heat transfer computations in the separated and reattaching regions associated with subsonic and supersonic flows over backward facing steps. Heat <span class="hlt">flux</span> computations in the base region of a single STME engine and a single S1C engine were performed using three different wall functions as well as a renormalization-group based k-epsilon model. With the very limited data available, the computed values are seen to be of the right order of magnitude. Based on the validation comparisons, it is concluded that all the <span class="hlt">turbulence</span> models studied have predicted the reattachment location and the velocity profiles at various axial stations downstream of the step very well.</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://hdl.handle.net/2060/19720018770','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19720018770"><span>Development of carbon dioxide laser doppler instrumentation detection of clear <span class="hlt">air</span> <span class="hlt">turbulence</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sonnenschein, C.; Jelalian, A.; Keene, W.</p> <p>1970-01-01</p> <p>The analytical, experimental, and developmental aspects of an airborne, pulsed, carbon dioxide laser-optical radar system are described. The laser detects clear <span class="hlt">air</span> <span class="hlt">turbulence</span> and performs Doppler measurements of this <span class="hlt">air</span>-motion phenomenon. Conclusions and recommendations arising from the development of the laser system are presented.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_20 --> <div id="page_21" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="401"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/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('https://ntrs.nasa.gov/search.jsp?R=19930040408&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=19930040408&hterms=air+measurement&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dair%2Bmeasurement"><span><span class="hlt">Turbulence</span> measurements in axisymmetric jets of <span class="hlt">air</span> and helium. I - <span class="hlt">Air</span> jet. II - Helium jet</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Panchapakesan, N. R.; Lumley, J. L.</p> <p>1993-01-01</p> <p>Results are presented of measurements on <span class="hlt">turbulent</span> round jets of <span class="hlt">air</span> and of helium of the same nozzle momentum efflux, using, for the <span class="hlt">air</span> jets, x-wire hot-wire probes mounted on a moving shuttle and, for He jets, a composite probe consisting of an interference probe of the Way-Libby type and an x-probe. Current models for scalar triple moments were evaluated. It was found that the performance of the model termed the Full model, which includes all terms except advection, was very good for both the <span class="hlt">air</span> and the He jets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015PhRvL.115j3901G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PhRvL.115j3901G"><span>Broadband Phase Spectroscopy over <span class="hlt">Turbulent</span> <span class="hlt">Air</span> Paths</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Giorgetta, Fabrizio R.; Rieker, Gregory B.; Baumann, Esther; Swann, William C.; Sinclair, Laura C.; Kofler, Jon; Coddington, Ian; Newbury, Nathan R.</p> <p>2015-09-01</p> <p>Broadband atmospheric phase spectra are acquired with a phase-sensitive dual-frequency-comb spectrometer by implementing adaptive compensation for the strong decoherence from atmospheric <span class="hlt">turbulence</span>. The compensation is possible due to the pistonlike behavior of <span class="hlt">turbulence</span> across a single spatial-mode path combined with the intrinsic frequency stability and high sampling speed associated with dual-comb spectroscopy. The atmospheric phase spectrum is measured across 2 km of <span class="hlt">air</span> at each of the 70 000 comb teeth spanning 233 cm-1 across hundreds of near-infrared rovibrational resonances of CO2 , CH4 , and H2O with submilliradian uncertainty, corresponding to a 10-13 refractive index sensitivity. Trace gas concentrations extracted directly from the phase spectrum reach 0.7 ppm uncertainty, demonstrated here for CO2 . While conventional broadband spectroscopy only measures intensity absorption, this approach enables measurement of the full complex susceptibility even in practical open path sensing.</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/2016OcSci..12..433M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016OcSci..12..433M"><span><span class="hlt">Turbulence</span> observations in the Gulf of Trieste under moderate wind forcing and different water column stratification</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marcello Falcieri, Francesco; Kantha, Lakshmi; Benetazzo, Alvise; Bergamasco, Andrea; Bonaldo, Davide; Barbariol, Francesco; Malačič, Vlado; Sclavo, Mauro; Carniel, Sandro</p> <p>2016-03-01</p> <p>The oceanographic campaign CARPET2014 (Characterizing Adriatic Region Preconditionig EvenTs), (30 January-4 February 2014) collected the very first <span class="hlt">turbulence</span> data in the Gulf of Trieste (northern Adriatic <span class="hlt">Sea</span>) under moderate wind (average wind speed 10 m s-1) and heat <span class="hlt">flux</span> (net negative heat <span class="hlt">flux</span> ranging from 150 to 400 W m-2). Observations consisted of 38 CTD (Conductivity, Temperature, Depth) casts and 478 microstructure profiles (grouped into 145 ensembles) with three sets of yoyo casts, each lasting for about 12 consecutive hours. Averaging closely repeated casts, such as the ensembles, can lead to a smearing effect when in the presence of a vertical density structure with strong interfaces that can move up or down between subsequent casts under the influence of tides and internal waves. In order to minimize the smearing effect of such displacements on mean quantities, we developed an algorithm to realign successive microstructure profiles to produce sharper and more meaningful mean profiles of measured <span class="hlt">turbulence</span> parameters. During the campaign, the water column in the gulf evolved from well-mixed to stratified conditions due to Adriatic waters intruding at the bottom along the gulf's south-eastern coast. We show that during the warm and relatively dry winter, the water column in the Gulf of Trieste, even under moderate wind forcing, was not completely mixed due to the influence of bottom waters intruding from the open <span class="hlt">sea</span>. Inside the gulf, two types of water intrusions were found during yoyo casts: one coming from the northern coast of the Adriatic <span class="hlt">Sea</span> (i.e. cooler, fresher and more turbid) and one coming from the open <span class="hlt">sea</span> in front of the Po Delta (i.e. warmer, saltier and less turbid). The two intrusions had different impacts on <span class="hlt">turbulence</span> kinetic energy dissipation rate profiles. The former, with high turbidity, acted as a barrier to wind-driven <span class="hlt">turbulence</span>, while the latter, with low sediment concentrations and a smaller vertical density gradient, was not</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.H21J..07N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.H21J..07N"><span>Thermal circulation patterns and <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> along steep mountain slopes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nadeau, D. F.; Pardyjak, E.; Higgins, C. W.; Huwald, H.; Baerenbold, F.; Parlange, M. B.</p> <p>2010-12-01</p> <p>In hydrology, it is crucial to understand the atmospheric flow dynamics in mountainous terrain to predict <span class="hlt">turbulent</span> exchanges of heat and moisture accurately at the regional scale. Under clear sky and weak synoptic conditions, these land-atmosphere interactions are driven by thermal circulations that take place over a strong diurnal cycle. During the day, winds travel up the mountain slopes and at night, they travel down toward to the bottom of the valley. Little is known about how the transition between these two regimes takes place over steep slopes. The Slope Experiment at La Fouly (SELF) in the Swiss Alps was designed to investigate these transition periods throughout summer 2010. In this paper, we will present the first results obtained from this field campaign. Data from a network of 16 wireless surface stations is used to define catchment wide micrometeorological processes such as slope and valley wind system development, while detailed measurements of the <span class="hlt">turbulent</span> processes on a steep idealized slope (20 to 45 degrees) were also made. The slope was instrumented along a transect with four towers (including a surface energy budget station and 10 m tower with sonic anemometers), 13 surface temperature measurement stations and a tethered balloon system to capture the complex interplay between surface and atmosphere. Initial data presented will include basic circulation pattern development and measurements of the <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> of water vapor, heat and momentum on the slope.</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/2017JGRC..122.8876Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.8876Y"><span>Observations of Tidal Straining Within Two Different Ocean Environments in the East China <span class="hlt">Sea</span>: Stratification and Near-Bottom <span class="hlt">Turbulence</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, Wei; Wei, Hao; Zhao, Liang</p> <p>2017-11-01</p> <p>Tidal straining describes the straining effect induced by the vertical shear of oscillatory tidal currents that act on horizontal density gradients. It tends to create tidal periodic stratification and modulate the <span class="hlt">turbulence</span> in the bottom boundary layer (BBL). Here, we present observations of current, hydrology and <span class="hlt">turbulence</span> obtained at two mooring stations that are characterized by two typical hydrological environments in the East China <span class="hlt">Sea</span> (ECS). One is located adjacent to the Changjiang River's mouth, and the other is located over a sloping shelf which is far from the freshwater sources. Tidal straining induces a semidiurnal switching between stable and unstable stratification at both stations. Near-bottom high-frequency velocity measurements further reveal that the dissipation rate of <span class="hlt">turbulent</span> kinetic energy (TKE) is highly elevated during periods when unstable stratification occurs. A comparison between the TKE dissipation rate (ɛ) and the shear production (P) further reveals that the near-bottom mixing is locally shear-induced most of the time except during the unstable stratification period. Within this period, the magnitude of dissipation exceeds the expected value based on the law of the wall by an order of magnitude. The buoyancy <span class="hlt">flux</span> that calculated by the balance method is too small to compensate for the existing discrepancy between the dissipation and shear production. Another plausible candidate is the advection of TKE, which may play an important role in the TKE budget during the unstable stratification period.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22525314-time-dependent-turbulent-heating-open-flux-tubes-chromosphere-corona-solar-wind','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22525314-time-dependent-turbulent-heating-open-flux-tubes-chromosphere-corona-solar-wind"><span>TIME-DEPENDENT <span class="hlt">TURBULENT</span> HEATING OF OPEN <span class="hlt">FLUX</span> TUBES IN THE CHROMOSPHERE, CORONA, AND SOLAR WIND</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>Woolsey, L. N.; Cranmer, S. R., E-mail: lwoolsey@cfa.harvard.edu</p> <p></p> <p>We investigate several key questions of plasma heating in open-field regions of the corona that connect to the solar wind. We present results for a model of Alfvén-wave-driven <span class="hlt">turbulence</span> for three typical open magnetic field structures: a polar coronal hole, an open <span class="hlt">flux</span> tube neighboring an equatorial streamer, and an open <span class="hlt">flux</span> tube near a strong-field active region. We compare time-steady, one-dimensional <span class="hlt">turbulent</span> heating models against fully time-dependent three-dimensional reduced-magnetohydrodynamic modeling of BRAID. We find that the time-steady results agree well with time-averaged results from BRAID. The time dependence allows us to investigate the variability of the magnetic fluctuations andmore » of the heating in the corona. The high-frequency tail of the power spectrum of fluctuations forms a power law whose exponent varies with height, and we discuss the possible physical explanation for this behavior. The variability in the heating rate is bursty and nanoflare-like in nature, and we analyze the amount of energy lost via dissipative heating in transient events throughout the simulation. The average energy in these events is 10{sup 21.91} erg, within the “picoflare” range, and many events reach classical “nanoflare” energies. We also estimated the multithermal distribution of temperatures that would result from the heating-rate variability, and found good agreement with observed widths of coronal differential emission measure distributions. The results of the modeling presented in this paper provide compelling evidence that <span class="hlt">turbulent</span> heating in the solar atmosphere by Alfvén waves accelerates the solar wind in open <span class="hlt">flux</span> tubes.« less</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 <span class="hlt">turbulence</span> 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('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, <span class="hlt">turbulent</span> 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('https://www.ncbi.nlm.nih.gov/pubmed/18851149','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/18851149"><span>A priori study of subgrid-scale <span class="hlt">flux</span> of a passive scalar in isotropic homogeneous <span class="hlt">turbulence</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chumakov, Sergei G</p> <p>2008-09-01</p> <p>We perform a direct numerical simulation (DNS) of forced homogeneous isotropic <span class="hlt">turbulence</span> with a passive scalar that is forced by mean gradient. The DNS data are used to study the properties of subgrid-scale <span class="hlt">flux</span> of a passive scalar in the framework of large eddy simulation (LES), such as alignment trends between the <span class="hlt">flux</span>, resolved, and subgrid-scale flow structures. It is shown that the direction of the <span class="hlt">flux</span> is strongly coupled with the subgrid-scale stress axes rather than the resolved flow quantities such as strain, vorticity, or scalar gradient. We derive an approximate transport equation for the subgrid-scale <span class="hlt">flux</span> of a scalar and look at the relative importance of the terms in the transport equation. A particular form of LES tensor-viscosity model for the scalar <span class="hlt">flux</span> is investigated, which includes the subgrid-scale stress. Effect of different models for the subgrid-scale stress on the model for the subgrid-scale <span class="hlt">flux</span> is studied.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.4569M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.4569M"><span>Mixing rates and vertical heat <span class="hlt">fluxes</span> north of Svalbard from Arctic winter to spring</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Meyer, Amelie; Fer, Ilker; Sundfjord, Arild; Peterson, Algot K.</p> <p>2017-06-01</p> <p>Mixing and heat <span class="hlt">flux</span> rates collected in the Eurasian Basin north of Svalbard during the N-ICE2015 drift expedition are presented. The observations cover the deep Nansen Basin, the Svalbard continental slope, and the shallow Yermak Plateau from winter to summer. Mean quiescent winter heat <span class="hlt">flux</span> values in the Nansen Basin are 2 W m-2 at the ice-ocean interface, 3 W m-2 in the pycnocline, and 1 W m-2 below the pycnocline. Large heat <span class="hlt">fluxes</span> exceeding 300 W m-2 are observed in the late spring close to the surface over the Yermak Plateau. The data consisting of 588 microstructure profiles and 50 days of high-resolution under-ice <span class="hlt">turbulence</span> measurements are used to quantify the impact of several forcing factors on <span class="hlt">turbulent</span> dissipation and heat <span class="hlt">flux</span> rates. Wind forcing increases <span class="hlt">turbulent</span> dissipation seven times in the upper 50 m, and doubles heat <span class="hlt">fluxes</span> at the ice-ocean interface. The presence of warm Atlantic Water close to the surface increases the temperature gradient in the water column, leading to enhanced heat <span class="hlt">flux</span> rates within the pycnocline. Steep topography consistently enhances dissipation rates by a factor of four and episodically increases heat <span class="hlt">flux</span> at depth. It is, however, the combination of storms and shallow Atlantic Water that leads to the highest heat <span class="hlt">flux</span> rates observed: ice-ocean interface heat <span class="hlt">fluxes</span> average 100 W m-2 during peak events and are associated with rapid basal <span class="hlt">sea</span> ice melt, reaching 25 cm/d.</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/2004AGUFM.C31A0309E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004AGUFM.C31A0309E"><span>Variations in Below Canopy <span class="hlt">Turbulent</span> <span class="hlt">Flux</span> From Snow in North American Mountain Environments</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Essery, R.; Marks, D.; Pomeroy, J.; Grangere, R.; Reba, M.; Hedstrom, N.; Link, T.; Winstral, A.</p> <p>2004-12-01</p> <p>Sensible and latent heat and mass <span class="hlt">fluxes</span> from the snow surface are modulated by site canopy density and structure. Forest and shrub canopies reduce wind speeds and alter the radiation and thermal environment which will alter the below canopy energetics that control the magnitude of <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> between the snow surface and the atmosphere. In this study eddy covariance (EC) systems were located in three experimental catchments along a mountain transect through the North American Cordillera. Within each catchment, a variety of sites representing the local range of climate, weather, and canopy conditions were selected for measurement of sensible and latent heat and mass <span class="hlt">flux</span> from the snow surface. EC measurements were made 1) below a uniform pine canopy (2745m) in the Fraser Experimental Forest in Colorado from February through June melt-out in 2003; 2) at an open, unforested site (2100m), and below an Aspen canopy (2055m) within a small headwater catchment in the Reynolds Creek Experimental Watershed, Owyhee Mts., Idaho from October, 2003, through June melt-out, 2004; and 3) at five sites, representing a range of conditions: a) below a dense spruce forest (750m); b) a north-facing shrub-tundra slope (1383m); c) a south-facing shrub-tundra slope; d) the valley bottom between b) and c) (1363m); and e) a tundra site (1402m) in the Wolf Creek Research Basin (WCRB) in the Yukon, Canada during the 2001 and 2002 snow seasons. Summary data from all sites are presented and compared including the relative significance of sublimation losses at each site, the importance of interception losses to the snowcover mass balance, and the occurrence of condensation events. Site and weather conditions that inhibit or enhance <span class="hlt">flux</span> from the snow surface are discussed. This research will improve snow modeling by allowing better representation of <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> from snow in forested regions, and improved simulation of the snowcover mass balance over low deposition, high latitude sites</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 <span class="hlt">turbulent</span> 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/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('https://www.ncbi.nlm.nih.gov/pubmed/24514524','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24514524"><span>Effects of source spatial partial coherence on temporal fade statistics of irradiance <span class="hlt">flux</span> in free-space optical links through atmospheric <span class="hlt">turbulence</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chen, Chunyi; Yang, Huamin; Zhou, Zhou; Zhang, Weizhi; Kavehrad, Mohsen; Tong, Shoufeng; Wang, Tianshu</p> <p>2013-12-02</p> <p>The temporal covariance function of irradiance-<span class="hlt">flux</span> fluctua-tions for Gaussian Schell-model (GSM) beams propagating in atmospheric <span class="hlt">turbulence</span> is theoretically formulated by making use of the method of effective beam parameters. Based on this formulation, new expressions for the root-mean-square (RMS) bandwidth of the irradiance-<span class="hlt">flux</span> temporal spectrum due to GSM beams passing through atmospheric <span class="hlt">turbulence</span> are derived. With the help of these expressions, the temporal fade statistics of the irradiance <span class="hlt">flux</span> in free-space optical (FSO) communication systems, using spatially partially coherent sources, impaired by atmospheric <span class="hlt">turbulence</span> are further calculated. Results show that with a given receiver aperture size, the use of a spatially partially coherent source can reduce both the fractional fade time and average fade duration of the received light signal; however, when atmospheric <span class="hlt">turbulence</span> grows strong, the reduction in the fractional fade time becomes insignificant for both large and small receiver apertures and in the average fade duration turns inconsiderable for small receiver apertures. It is also illustrated that if the receiver aperture size is fixed, changing the transverse correlation length of the source from a larger value to a smaller one can reduce the average fade frequency of the received light signal only when a threshold parameter in decibels greater than the critical threshold level is specified.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19910012352','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19910012352"><span>Estimations of ABL <span class="hlt">fluxes</span> and other <span class="hlt">turbulence</span> parameters from Doppler lidar data</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gal-Chen, Tzvi; Xu, Mei; Eberhard, Wynn</p> <p>1989-01-01</p> <p>Techniques for extraction boundary layer parameters from measurements of a short-pulse CO2 Doppler lidar are described. The measurements are those collected during the First International Satellites Land Surface Climatology Project (ISLSCP) Field Experiment (FIFE). By continuously operating the lidar for about an hour, stable statistics of the radial velocities can be extracted. Assuming that the <span class="hlt">turbulence</span> is horizontally homogeneous, the mean wind, its standard deviations, and the momentum <span class="hlt">fluxes</span> were estimated. Spectral analysis of the radial velocities is also performed from which, by examining the amplitude of the power spectrum at the inertial range, the kinetic energy dissipation was deduced. Finally, using the statistical form of the Navier-Stokes equations, the surface heat <span class="hlt">flux</span> is derived as the residual balance between the vertical gradient of the third moment of the vertical velocity and the kinetic energy dissipation. Combining many measurements would normally reduce the error provided that, it is unbiased and uncorrelated. The nature of some of the algorithms however, is such that, biased and correlated errors may be generated even though the raw measurements are not. Data processing procedures were developed that eliminate bias and minimize error correlation. Once bias and error correlations are accounted for, the large sample size is shown to reduce the errors substantially. The principal features of the derived <span class="hlt">turbulence</span> statistics for two case studied are presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19910063111&hterms=heat+stress&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dheat%2Bstress','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19910063111&hterms=heat+stress&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dheat%2Bstress"><span>Reynolds shear stress and heat <span class="hlt">flux</span> calculations in a fully developed <span class="hlt">turbulent</span> duct flow</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Antonia, R. A.; Kim, J.</p> <p>1991-01-01</p> <p>The use of a modified form of the Van Driest mixing length for a fully developed <span class="hlt">turbulent</span> channel flow leads to mean velocity and Reynolds stress distributions that are in close agreement with data obtained either from experiments or direct numerical simulations. The calculations are then extended to a nonisothermal flow by assuming a constant <span class="hlt">turbulent</span> Prandtl number, the value of which depends on the molecular Prandtl number. Calculated distributions of mean temperature and lateral heat <span class="hlt">flux</span> are in reasonable agreement with the simulations. The extension of the calculations to higher Reynolds numbers provides some idea of the Reynolds number required for scaling on wall variables to apply in the inner region of the flow.</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/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> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002JGRD..107.4425S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002JGRD..107.4425S"><span>Evapotranspiration and <span class="hlt">turbulent</span> transport in an irrigated desert orchard</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stoughton, Thomas E.; Miller, David R.; Huddleston, Ellis W.; Ross, James B.</p> <p>2002-10-01</p> <p>Micrometeorological measurements were recorded in an irrigated pecan orchard for 2 weeks in the summer of 1996 near Las Cruces, NM. A vertical array of five sonic anemometers recorded three-dimensional wind and temperature data within and above the orchard. The measured energy budget closure error was only 3.2% of net radiation, indicating freedom from local edge advection. The effects of regional (oasis) advection and unsteady winds on evapotranspiration (ET) were considered by comparing the observed latent heat <span class="hlt">flux</span> values to estimates of ET using the Penman-Monteith and Advection-Aridity approaches. Penman-Monteith underestimated observed ET values by 82%. The Advection-Aridity modifications of potential evapotranspiration (PET) underestimated ET by 11%. Profiles of <span class="hlt">turbulence</span> statistics demonstrated vertical heterogeneity of <span class="hlt">turbulence</span> within the canopy. Directly above the canopy, momentum <span class="hlt">flux</span> profiles showed little divergence. However, at a level of two times the tree heights, sensible heat <span class="hlt">flux</span> profiles did show divergence, confirming the presence of "oasis" advection resulting from warm, dry <span class="hlt">air</span> moving above the internal boundary layer. Upward convection from the hot soil surface between the trees diluted the oasis condition to the point where a weak upward sensible heat <span class="hlt">flux</span> was observed during the midday periods when the soil was not shaded. Convection ratios, and exuberance ratios, generated from quadrant analyses of the heat and momentum <span class="hlt">flux</span> events, showed that <span class="hlt">turbulent</span> motions moved freely up and down within this canopy with little attenuation due to the open spaces between the trees.</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://hdl.handle.net/2060/19790019601','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19790019601"><span>Meteorological and operational aspects of 46 clear <span class="hlt">air</span> <span class="hlt">turbulent</span> sampling missions with an instrumented B-57B aircraft. Volume 2, appendix C: <span class="hlt">Turbulence</span> missions</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Waco, D. E.</p> <p>1979-01-01</p> <p>The results of 46 clear <span class="hlt">air</span> <span class="hlt">turbulence</span> (CAT) probing missions conducted with an extensively instrumented B-57B aircraft are summarized from a meteorological viewpoint in a two-volume technical memorandum. The missions were part of the NASA Langley Research Center's MAT (Measurement of Atmospheric <span class="hlt">Turbulence</span>) program, which was conducted between March 1974, and September 1975, at altitudes ranging up to 15 km. <span class="hlt">Turbulence</span> samples were obtained under diverse conditions including mountain waves, jet streams, upper level fronts and troughs, and low altitude mechanical and thermal <span class="hlt">turbulence</span>. CAT was encountered on 20 flights comprising 77 data runs. In all, approximately 4335 km were flown in light <span class="hlt">turbulence</span>, 1415 km in moderate <span class="hlt">turbulence</span>, and 255 km in severe <span class="hlt">turbulence</span> during the program.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A53K..05K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A53K..05K"><span>Properties and <span class="hlt">Fluxes</span> of Primary Marine Aerosol Generated Via Detrainment of <span class="hlt">Turbulence</span>-Modulated Bubble Plumes from Fresh North Atlantic Seawater</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Keene, W. C.; Long, M. S.; Duplessis, P.; Kieber, D. J.; Maben, J. R.; Frossard, A. A.; Kinsey, J. D.; Beaupre, S. R.; Lu, X.; Chang, R.; Zhu, Y.; Bisgrove, J.</p> <p>2017-12-01</p> <p>During a September-October 2016 cruise of the R/V Endeavor in the western North Atlantic Ocean, primary marine aerosol (PMA) was produced in a high capacity generator during day and night via detrainment of bubbles from biologically productive and oligotrophic seawater. The <span class="hlt">turbulent</span> mixing of clean <span class="hlt">air</span> and seawater in a Venturi nozzle produced bubble plumes with tunable size distributions. Physicochemical characteristics of size-resolved PMA and seawater were measured. PMA number production efficiencies per unit <span class="hlt">air</span> detrained (PEnum) increased with increasing detainment rate. For given conditions, PEnum values summed over size distributions were roughly ten times greater than those for frits whereas normalized size distributions were similar. Results show that bubble size distributions significantly modulated number production <span class="hlt">fluxes</span> but not relative shapes of corresponding size distributions. In contrast, mass production efficiencies (PEmass) decreased with increasing <span class="hlt">air</span> detrainment and were similar to those for frits, consistent with the hypothesis that bubble rafts on the seawater surface modulate emissions of larger jet droplets that dominate PMA mass production. Production efficiencies of organic matter were about three times greater than those for frits whereas organic enrichment factors integrated over size distributions were similar.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005AGUFMNG23D0117C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005AGUFMNG23D0117C"><span>Long-term persistence of the spatial organization of plume lifetime in <span class="hlt">turbulent</span> <span class="hlt">air</span> avalanches</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Crouzeix, C.; Le Mouël, J.; Perrier, F.; Shnirman, M. G.</p> <p>2005-12-01</p> <p>Temperature measurements have been performed in the vertical access pit of an underground quarry in winter, when outside temperature is low and induce <span class="hlt">turbulent</span> avalanches of cold <span class="hlt">air</span> in the pit. The measured time series are studied with a non-linear method based on absolute differences, which has been recently proposed as an adequate tool in the case of modulated jitter: a high-frequency signal multiplied by a long-term component (for example the sunspot number). The thermal fluctuations associated with the <span class="hlt">turbulent</span> plumes are proved to offer an almost perfect realization of a modulated jitter. The lifetime, estimated from the method as a function of time and position in the pit, is of the order of 10 to 25 minutes, remarkably constant in time for each sensor and independent of the forcing. A significant and persistent spatial variation is also observed, indicating a long-term intrinsic organization of the <span class="hlt">turbulent</span> <span class="hlt">air</span> flow in the pit. Such stable organization may be a universal feature of chaotic phenomena. Furthermore, the properties of <span class="hlt">turbulent</span> <span class="hlt">air</span> avalanches and of sunspots determined by this method appear similar. This may be due to a common underlying physical mechanism. Modulated jitter, which are probably present in numerous natural processes, can be studied using the method presented here.</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/2016EGUGA..18.3373A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.3373A"><span>Estimating sensible heat <span class="hlt">flux</span> in agricultural screenhouses by the <span class="hlt">flux</span>-variance and half-order time derivative methods</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Achiman, Ori; Mekhmandarov, Yonatan; Pirkner, Moran; Tanny, Josef</p> <p>2016-04-01</p> <p>Previous studies have established that the eddy covariance (EC) technique is reliable for whole canopy <span class="hlt">flux</span> measurements in agricultural crops covered by porous screens, i.e., screenhouses. Nevertheless, the eddy covariance technique remains difficult to apply in the farm due to costs, operational complexity, and post-processing of data - thereby inviting alternative techniques to be developed. The subject of this research was estimating the sensible heat <span class="hlt">flux</span> by two <span class="hlt">turbulent</span> transport techniques, namely, <span class="hlt">Flux</span>-Variance (FV) and Half-order Time Derivative (HTD) whose instrumentation needs and operational demands are not as elaborate as the EC. The FV is based on the standard deviation of high frequency temperature measurements and a similarity constant CT. The HTD method requires mean <span class="hlt">air</span> temperature and <span class="hlt">air</span> velocity data. Measurements were carried out in two types of screenhouses: (i) a banana plantation in a light shading (8%) screenhouse; (ii) a pepper crop in a dense insect-proof (50-mesh) screenhouse. In each screenhouse an EC system was deployed for reference and high frequency <span class="hlt">air</span> temperature measurements were conducted using miniature thermocouples installed at several levels to identify the optimal measurement height. Quality control analysis showed that <span class="hlt">turbulence</span> development and flow stationarity conditions in the two structures were suitable for <span class="hlt">flux</span> measurements by the EC technique. Energy balance closure slopes in the two screenhouses were larger than 0.71, in agreement with results for open fields. Regressions between sensible heat <span class="hlt">flux</span> measured by EC and estimated by FV resulted with CT values that were usually larger than 1, the typical value for open field. In both shading and insect-proof screenhouses the CT value generally increased with height. The optimal measurement height, defined as the height with maximum R2 of the regression between EC and FV sensible heat <span class="hlt">fluxes</span>, was just above the screen. CT value at optimal height was 2.64 and 1.52 for</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('https://www.osti.gov/biblio/22599996-causal-relation-between-turbulent-particle-flux-density-gradient','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22599996-causal-relation-between-turbulent-particle-flux-density-gradient"><span>The causal relation between <span class="hlt">turbulent</span> particle <span class="hlt">flux</span> and density gradient</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>Milligen, B. Ph. van; Martín de Aguilera, A.; Hidalgo, C.</p> <p></p> <p>A technique for detecting the causal relationship between fluctuating signals is used to investigate the relation between <span class="hlt">flux</span> and gradient in fusion plasmas. Both a resistive pressure gradient driven <span class="hlt">turbulence</span> model and experimental Langmuir probe data from the TJ-II stellarator are studied. It is found that the maximum influence occurs at a finite time lag (non-instantaneous response) and that quasi-periodicities exist. Furthermore, the model results show very long range radial influences, extending over most of the investigated regions, possibly related to coupling effects associated with plasma self-organization. These results clearly show that transport in fusion plasmas is not local andmore » instantaneous, as is sometimes assumed.« less</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/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 <span class="hlt">turbulence</span> 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('http://adsabs.harvard.edu/abs/2018OptCo.413..196G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018OptCo.413..196G"><span>Aperture averaging in strong oceanic <span class="hlt">turbulence</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gökçe, Muhsin Caner; Baykal, Yahya</p> <p>2018-04-01</p> <p>Receiver aperture averaging technique is employed in underwater wireless optical communication (UWOC) systems to mitigate the effects of oceanic <span class="hlt">turbulence</span>, thus to improve the system performance. The irradiance <span class="hlt">flux</span> variance is a measure of the intensity fluctuations on a lens of the receiver aperture. Using the modified Rytov theory which uses the small-scale and large-scale spatial filters, and our previously presented expression that shows the atmospheric structure constant in terms of oceanic <span class="hlt">turbulence</span> parameters, we evaluate the irradiance <span class="hlt">flux</span> variance and the aperture averaging factor of a spherical wave in strong oceanic <span class="hlt">turbulence</span>. Irradiance <span class="hlt">flux</span> variance variations are examined versus the oceanic <span class="hlt">turbulence</span> parameters and the receiver aperture diameter are examined in strong oceanic <span class="hlt">turbulence</span>. Also, the effect of the receiver aperture diameter on the aperture averaging factor is presented in strong oceanic <span class="hlt">turbulence</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_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/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 <span class="hlt">turbulent</span> 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('https://ntrs.nasa.gov/search.jsp?R=20080016482&hterms=website+traffic&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dwebsite%2Btraffic','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20080016482&hterms=website+traffic&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dwebsite%2Btraffic"><span>Wake <span class="hlt">Turbulence</span>: An Obstacle to Increased <span class="hlt">Air</span> Traffic Capacity</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>2008-01-01</p> <p>Wingtip vortices were first described by British aerodynamicist F.W. Lanchester in 1907. A product of lift on a finite-span wing, these counterrotating masses of <span class="hlt">air</span> trail behind an aircraft, gradually diffusing while convecting downward and moving about under mutual induction and the influence of wind and stratification. Should a smaller aircraft happen to be following the first aircraft, it could be buffeted and even flipped if it flew into the vortex, with dangerous consequences. Given the amount of <span class="hlt">air</span> traffic in 1907, the wake vortex hazard was not initially much of a concern. The demand for <span class="hlt">air</span> transportation continues to increase, and it is estimated that demand could double or even triple by 2025. One factor in the capacity of the <span class="hlt">air</span> transportation system is wake <span class="hlt">turbulence</span> and the consequent separation distances that must be maintained between aircraft to ensure safety.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://rosap.ntl.bts.gov/view/dot/11045','DOTNTL'); return false;" href="https://rosap.ntl.bts.gov/view/dot/11045"><span>Clear <span class="hlt">Air</span> <span class="hlt">Turbulence</span> Radiometric Detection Program : Operating Procedures - Flight Test : Supplement</span></a></p> <p><a target="_blank" href="http://ntlsearch.bts.gov/tris/index.do">DOT National Transportation Integrated Search</a></p> <p></p> <p>1973-02-01</p> <p>The report presents the accomplishments of the Clear <span class="hlt">Air</span> <span class="hlt">Turbulence</span> Detection Program for the Period July 1 1971 to June 30, 1972. The experimental effort during this time period was devoted mainly tothe flight test program, acquisitoin of the glight...</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/2002GMS...127..141S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002GMS...127..141S"><span>A model of <span class="hlt">air-sea</span> gas exchange incorporating the physics of the <span class="hlt">turbulent</span> boundary layer and the properties of the <span class="hlt">sea</span> surface</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Soloviev, Alexander; Schluessel, Peter</p> <p></p> <p>The model presented contains interfacial, bubble-mediated, ocean mixed layer, and remote sensing components. The interfacial (direct) gas transfer dominates under conditions of low and—for quite soluble gases like CO2—moderate wind speeds. Due to the similarity between the gas and heat transfer, the temperature difference, ΔT, across the thermal molecular boundary layer (cool skin of the ocean) and the interfacial gas transfer coefficient, Kint are presumably interrelated. A coupled parameterization for ΔT and Kint has been derived in the context of a surface renewal model [Soloviev and Schluessel, 1994]. In addition to the Schmidt, Sc, and Prandtl, Pr, numbers, the important parameters are the surface Richardson number, Rƒ0, and the Keulegan number, Ke. The more readily available cool skin data are used to determine the coefficients that enter into both parameterizations. At high wind speeds, the Ke-number dependence is further verified with the formula for transformation of the surface wind stress to form drag and white capping, which follows from the renewal model. A further extension of the renewal model includes effects of solar radiation and rainfall. The bubble-mediated component incorporates the Merlivat et al. [1993] parameterization with the empirical coefficients estimated by Asher and Wanninkhof [1998]. The oceanic mixed layer component accounts for stratification effects on the <span class="hlt">air-sea</span> gas exchange. Based on the example of GasEx-98, we demonstrate how the results of parameterization and modeling of the <span class="hlt">air-sea</span> gas exchange can be extended to the global scale, using remote sensing techniques.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.3291C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.3291C"><span>Progress in remote sensing of global land surface heat <span class="hlt">fluxes</span> and evaporations with a <span class="hlt">turbulent</span> heat exchange parameterization method</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, Xuelong; Su, Bob</p> <p>2017-04-01</p> <p>Remote sensing has provided us an opportunity to observe Earth land surface with a much higher resolution than any of GCM simulation. Due to scarcity of information for land surface physical parameters, up-to-date GCMs still have large uncertainties in the coupled land surface process modeling. One critical issue is a large amount of parameters used in their land surface models. Thus remote sensing of land surface spectral information can be used to provide information on these parameters or assimilated to decrease the model uncertainties. Satellite imager could observe the Earth land surface with optical, thermal and microwave bands. Some basic Earth land surface status (land surface temperature, canopy height, canopy leaf area index, soil moisture etc.) has been produced with remote sensing technique, which already help scientists understanding Earth land and atmosphere interaction more precisely. However, there are some challenges when applying remote sensing variables to calculate global land-<span class="hlt">air</span> heat and water exchange <span class="hlt">fluxes</span>. Firstly, a global <span class="hlt">turbulent</span> exchange parameterization scheme needs to be developed and verified, especially for global momentum and heat roughness length calculation with remote sensing information. Secondly, a compromise needs to be innovated to overcome the spatial-temporal gaps in remote sensing variables to make the remote sensing based land surface <span class="hlt">fluxes</span> applicable for GCM model verification or comparison. A <span class="hlt">flux</span> network data library (more 200 <span class="hlt">flux</span> towers) was collected to verify the designed method. Important progress in remote sensing of global land <span class="hlt">flux</span> and evaporation will be presented and its benefits for GCM models will also be discussed. Some in-situ studies on the Tibetan Plateau and problems of land surface process simulation will also be discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018BoLMe.166..301G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018BoLMe.166..301G"><span>An Efficient Non-iterative Bulk Parametrization of Surface <span class="hlt">Fluxes</span> for Stable Atmospheric Conditions Over Polar <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>Gryanik, Vladimir M.; Lüpkes, Christof</p> <p>2018-02-01</p> <p>In climate and weather prediction models the near-surface <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> of heat and momentum and related transfer coefficients are usually parametrized on the basis of Monin-Obukhov similarity theory (MOST). To avoid iteration, required for the numerical solution of the MOST equations, many models apply parametrizations of the transfer coefficients based on an approach relating these coefficients to the bulk Richardson number Rib. However, the parametrizations that are presently used in most climate models are valid only for weaker stability and larger surface roughnesses than those documented during the Surface Heat Budget of the Arctic Ocean campaign (SHEBA). The latter delivered a well-accepted set of <span class="hlt">turbulence</span> data in the stable surface layer over polar <span class="hlt">sea</span>-ice. Using stability functions based on the SHEBA data, we solve the MOST equations applying a new semi-analytic approach that results in transfer coefficients as a function of Rib and roughness lengths for momentum and heat. It is shown that the new coefficients reproduce the coefficients obtained by the numerical iterative method with a good accuracy in the most relevant range of stability and roughness lengths. For small Rib, the new bulk transfer coefficients are similar to the traditional coefficients, but for large Rib they are much smaller than currently used coefficients. Finally, a possible adjustment of the latter and the implementation of the new proposed parametrizations in models are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1214444-modeling-effect-lithium-induced-pedestal-profiles-scrape-off-layer-turbulence-heat-flux-width','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1214444-modeling-effect-lithium-induced-pedestal-profiles-scrape-off-layer-turbulence-heat-flux-width"><span>Modeling the effect of lithium-induced pedestal profiles on scrape-off-layer <span class="hlt">turbulence</span> and the heat <span class="hlt">flux</span> width</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Russell, David A.; D'Ippolito, Daniel A.; Myra, James R.; ...</p> <p>2015-09-01</p> <p>The effect of lithium (Li) wall coatings on scrape-off-layer (SOL) <span class="hlt">turbulence</span> in the National Spherical Torus Experiment (NSTX) is modeled with the Lodestar SOLT (“SOL Turbulence”) code. Specifically, the implications for the SOL heat <span class="hlt">flux</span> width of experimentally observed, Li-induced changes in the pedestal profiles are considered. The SOLT code used in the modeling has been expanded recently to include ion temperature evolution and ion diamagnetic drift effects. This work focuses on two NSTX discharges occurring pre- and with-Li deposition. The simulation density and temperature profiles are constrained, inside the last closed <span class="hlt">flux</span> surface only, to match those measured inmore » the two experiments, and the resulting drift-interchange-driven <span class="hlt">turbulence</span> is explored. The effect of Li enters the simulation only through the pedestal profile constraint: Li modifies the experimental density and temperature profiles in the pedestal, and these profiles affect the simulated SOL <span class="hlt">turbulence</span>. The power entering the SOL measured in the experiments is matched in the simulations by adjusting “free” dissipation parameters (e.g., diffusion coefficients) that are not measured directly in the experiments. With power-matching, (a) the heat <span class="hlt">flux</span> SOL width is smaller, as observed experimentally by infra-red thermography, and (b) the simulated density fluctuation amplitudes are reduced with Li, as inferred for the experiments as well from reflectometry analysis. The instabilities and saturation mechanisms that underlie the SOLT model equilibria are also discussed.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008APS..DFD.GA002C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008APS..DFD.GA002C"><span><span class="hlt">Air</span> Layer Drag Reduction</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ceccio, Steven; Elbing, Brian; Winkel, Eric; Dowling, David; Perlin, Marc</p> <p>2008-11-01</p> <p>A set of experiments have been conducted at the US Navy's Large Cavitation Channel to investigate skin-friction drag reduction with the injection of <span class="hlt">air</span> into a high Reynolds number <span class="hlt">turbulent</span> boundary layer. Testing was performed on a 12.9 m long flat-plate test model with the surface hydraulically smooth and fully rough at downstream-distance-based Reynolds numbers to 220 million and at speeds to 20 m/s. Local skin-friction, near-wall bulk void fraction, and near-wall bubble imaging were monitored along the length of the model. The instrument suite was used to access the requirements necessary to achieve <span class="hlt">air</span> layer drag reduction (ALDR). Injection of <span class="hlt">air</span> over a wide range of <span class="hlt">air</span> <span class="hlt">fluxes</span> showed that three drag reduction regimes exist when injecting <span class="hlt">air</span>; (1) bubble drag reduction that has poor downstream persistence, (2) a transitional regime with a steep rise in drag reduction, and (3) ALDR regime where the drag reduction plateaus at 90% ± 10% over the entire model length with large void fractions in the near-wall region. These investigations revealed several requirements for ALDR including; sufficient volumetric <span class="hlt">air</span> <span class="hlt">fluxes</span> that increase approximately with the square of the free-stream speed, slightly higher <span class="hlt">air</span> <span class="hlt">fluxes</span> are needed when the surface tension is reduced, higher <span class="hlt">air</span> <span class="hlt">fluxes</span> are required for rough surfaces, and the formation of ALDR is sensitive to the inlet condition.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhFl...29h5102W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhFl...29h5102W"><span>Effects of Karlovitz number on <span class="hlt">turbulent</span> kinetic energy transport in <span class="hlt">turbulent</span> lean premixed methane/<span class="hlt">air</span> flames</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Zhiyan; Abraham, John</p> <p>2017-08-01</p> <p>Direct numerical simulations of lean methane/<span class="hlt">air</span> flames are carried out to study the effects of premixed combustion on <span class="hlt">turbulence</span>. The equivalence ratio of the flame is 0.5 and non-dimensional <span class="hlt">turbulence</span> intensities (urms/SL) are between 2 and 25. The mixture pressure is 20 bars and temperature is 810 K to simulate approximate conditions in lean-burn natural gas engines. The Karlovitz number (Ka) varies from 1.1 to 49.4, and the Damköhler number (Da) varies from 0.26 to 3.2 corresponding to <span class="hlt">turbulent</span> premixed combustion in the thin reaction zone (TRZ) regime. It is found that <span class="hlt">turbulence</span> kinetic energy (TKE) and its dissipation rate decrease monotonically across the flame brush while the integral length scale increases monotonically for flames in the TRZ regime. The transport equation of TKE is then examined, and the scaling of the terms in the equation is discussed. It is found that the sink term which represents molecular diffusion and viscous dissipation is the dominant term in the TKE balance and it scales with the square of Ka. The relative importance of the other terms with respect to the dissipation term is studied. With increasing Ka, the other terms in the TKE balance become less important compared to the dissipation term.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A51A2023P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A51A2023P"><span>Insights into Evaporative Droplet Dynamics in the High-Wind Atmospheric Boundary Layer</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Peng, T.; Richter, D. H.</p> <p>2017-12-01</p> <p><span class="hlt">Sea</span>-spray droplets ejected into the <span class="hlt">air-sea</span> boundary layer take part in a series of complex transport processes. To model the <span class="hlt">air-sea</span> exchange of heat and moisture under high-wind conditions, it is important yet challenging to understand influences of evaporative droplets in the atmospheric boundary layer. We implement a high-resolution Eulerian-Lagrangian algorithm with droplets laden in a <span class="hlt">turbulent</span> open-channel flow to reveal the dynamic and thermodynamic characteristics of evaporating <span class="hlt">sea</span> spray. Our past numerical simulations demonstrated an overall weak modification to the total heat <span class="hlt">flux</span> by evaporative droplets. This is due to redistributed sensible and latent heat <span class="hlt">fluxes</span> from relatively small droplets that respond rapidly to the ambient environment or the limited residence time of larger droplets. However, droplets with a slower thermodynamic response to the environment indicate a potential to enhance the total heat <span class="hlt">flux</span>, but this is dependent on concentration and suspension time. In the current study, we focus on correlations between the residence time and thermodynamic statistics of droplets in order to better understand how best to parameterize in large-scale models. In addition, we focus in detail on the different scales of <span class="hlt">turbulence</span> to further characterize the range of influence that evaporating droplets have on the surrounding fluid.</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/2016AGUOSHE24A1439G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSHE24A1439G"><span>Quantifying the Impact of Background Atmospheric Stability on <span class="hlt">Air</span>-Ice-Ocean Interactions the Arctic Ocean During the Fall Freeze-Up</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Guest, P. S.; Persson, O. P. G.; Blomquist, B.; Fairall, C. W.</p> <p>2016-02-01</p> <p>"Background" stability refers to the effect of vertical virtual temperature variations above the surface layer on <span class="hlt">fluxes</span> within the surface layer. This is different from the classical surface layer stability quantified by the Obhukhov length scale. In most locations, changes in the background stability do not have a significant direct impact on surface <span class="hlt">fluxes</span>. However in polar regions, where there is usually a strong low-level temperature inversion capping the boundary layer, changes in background stability can have big impacts on surface <span class="hlt">fluxes</span>. Therefore, in the Arctic, there is potential for a positive feedback effect between ice cover and surface wind speed (and momentum <span class="hlt">flux</span>) due to the background stability effects. As the surface becomes more ice free, heat <span class="hlt">fluxes</span> from the surface weaken the temperature inversion which in turn increases the surface wind speed which further increases the surface <span class="hlt">turbulent</span> heat <span class="hlt">fluxes</span> and removes more <span class="hlt">sea</span> ice by melting or advection. It is not clear how important feedbacks involving the background stability are during the fall freeze up of the Arctic Ocean; that will be the focus of this study. As part of an ONR-sponsored cruise in the fall of 2015 to examine <span class="hlt">sea</span> state and boundary layer processes in the Beaufort <span class="hlt">Sea</span> on the R/V Sikuliaq, the authors will perform a variety of surface layer and upper level atmospheric measurements of temperature, humidity and wind vector using ship platform instruments, radiosonde weather balloons, tethered balloons, kites, and miniature quad-rotor unmanned aerial vehicles. In addition, the authors will deploy a full suite of <span class="hlt">turbulent</span> and radiational <span class="hlt">flux</span> measurements from the vessel. These measurements will be used to quantify the impact of changing surface conditions on atmospheric structure and vice-versa. The goal is to directly observe how the surface and atmosphere above the surface layer interact and feedback with each other through radiational and <span class="hlt">turbulent</span> <span class="hlt">fluxes</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://ntrs.nasa.gov/search.jsp?R=19730030269&hterms=background+wind&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dbackground%2Bwind','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19730030269&hterms=background+wind&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dbackground%2Bwind"><span>Internal gravity wave-atmospheric wind interaction - A cause of clear <span class="hlt">air</span> <span class="hlt">turbulence</span>.</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bekofske, K.; Liu, V. C.</p> <p>1972-01-01</p> <p>The interaction between an internal gravity wave (IGW) and a vertical wind shear is discussed as a possible cause in the production of clear <span class="hlt">air</span> <span class="hlt">turbulence</span> in the free atmosphere. It is shown that under certain typical condition the interaction of an IGW with a background wind shear near a critical level provides a mechanism for depositing sufficient momentum in certain regions of the atmosphere to significantly increase the local mean wind shear and to lead to the production of <span class="hlt">turbulence</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20160003590&hterms=strengthening&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dstrengthening','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20160003590&hterms=strengthening&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dstrengthening"><span>The Impact of Trends in the Large Scale Atmospheric Circulation on Mediterranean Surface <span class="hlt">Turbulent</span> Heat <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>Romanski, Joy; Hameed, Sultan</p> <p>2015-01-01</p> <p>Interannual variations of latent heat <span class="hlt">fluxes</span> (LHF) and sensible heat <span class="hlt">fluxes</span> (SHF) over the Mediterranean for the boreal winter season (DJF) show positive trends during 1958-2011. Using reanalysis and satellite-based products, the variability and trends in the heat <span class="hlt">fluxes</span> are compared with variations in three atmospheric teleconnection patterns: the North Atlantic Oscillation (NAO), the pressure and position of the Azores High (AH), and the East Atlantic-West Russia teleconnection pattern (EAWR). Comparison of correlations between the heat <span class="hlt">fluxes</span> and teleconnections, along with analysis of composites of surface temperature, humidity, and wind fields for different teleconnection states, demonstrates that the AH explains the heat <span class="hlt">flux</span> changes more successfully than NAO and EAWR. Trends in pressure and longitude of the Azores High show a strengthening and an eastward shift. Variations of the Azores High occur along an axis defined by lower pressure and westward location at one extreme and higher pressure and eastward location at the other extreme. The shift of the AH from predominance of the low/west state to the high/east state induces trends in Mediterranean <span class="hlt">Sea</span> surface winds, temperature, and moisture. These, combined with <span class="hlt">sea</span> surface warming trends, produce trends in wintertime sensible and latent heat <span class="hlt">fluxes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA590599','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA590599"><span><span class="hlt">Sea</span> State and Boundary Layer Physics of the Emerging Arctic Ocean</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2013-09-01</p> <p>meteorological stations; weather observations; upper-<span class="hlt">air</span> (rawinsondes, balloons and tethered kit); <span class="hlt">turbulent</span> <span class="hlt">fluxes</span>; radiation; surface temperature...remote sensing, in-field remote sensing will be employed, using small unmanned aerial vehicles (UAV), balloons , and manned aircraft (funded by other</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009EGUGA..11.6693K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009EGUGA..11.6693K"><span>Evaluation of Clear-<span class="hlt">Air</span> <span class="hlt">Turbulence</span> Diagnostics: GTG in Korea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kim, J.-H.; Chun, H.-Y.; Jang, W.; Sharman, R. D.</p> <p>2009-04-01</p> <p><span class="hlt">Turbulence</span> forecasting algorithm, the Graphical <span class="hlt">Turbulence</span> Guidance (GTG) system developed at NCAR (Sharman et al., 2006), is evaluated with available <span class="hlt">turbulence</span> observations (e.g. pilot reports; PIREPs) reported in South Korea during the recent 4 years (2003-2007). Clear-<span class="hlt">air</span> <span class="hlt">turbulence</span> (CAT) is extracted from PIREPs by using cloud-to-ground lightning flash data from Korean Meteorological Administration (KMA). The GTG system includes several steps. First, 45 <span class="hlt">turbulence</span> indices are calculated in the East Asian region near Korean peninsula using the Regional Data Assimilation and Prediction System (RDAPS) analysis data with 30 km horizontal grid spacing provided by KMA. Second, 10 CAT indices that performed ten best forecasting score are selected. The scoring method is based on the probability of detection, which is calculated using PIREPs exclusively of moderate-or-greater intensity. Various statistical examinations and sensitivity tests of the GTG system are performed by yearly and seasonally classified PIREPs in South Korea. Performance of GTG is more consistent and stable than that of any individual diagnostic in each year and season. In addition, current-year forecasting based on yearly PIREPs is better than adjacent-year forecasting and year-after-year forecasting. Seasonal forecasting is generally better than yearly forecasting, because selected CAT indices in each season represent meteorological condition much more properly than applying the selected CAT indices to all seasons. Wintertime forecasting is the best among the four seasonal forecastings. This is likely due to that the GTG system consists of many CAT indices related to jet stream, and <span class="hlt">turbulence</span> associated with the jet can be most activated in wintertime under strong jet magnitude. On the other hand, summertime forecasting skill is much less than in wintertime. To acquire better performance for summertime forecasting, it is likely to develop more <span class="hlt">turbulence</span> indices related to, for example</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> </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/2017EGUGA..1915051L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1915051L"><span>Impact of Low Level Clouds on radiative and <span class="hlt">turbulent</span> surface <span class="hlt">flux</span> in southern West Africa</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lohou, Fabienne; Kalthoff, Norbert; Dione, Cheikh; Lothon, Marie; Adler, Bianca; Babic, Karmen; Pedruzo-Bagazgoitia, Xabier; Vila-Guerau De Arellano, Jordi</p> <p>2017-04-01</p> <p>During the monsoon season in West Africa, low-level clouds form almost every night and break up between 0900 and the middle of the afternoon depending on the day. The break-up of these clouds leads to the formation of boundary-layer cumuli clouds, which can sometimes evolve into deep convection. The low-level clouds have a strong impact on the radiation and energy budget at the surface and consequently on the humidity in the boundary layer and the afternoon convection. During the DACCIWA ground campaign, which took place in June and July 2016, three supersites in Benin, Ghana, and Nigeria were instrumented to document the conditions within the lower troposphere including the cloud layers. Radiative and <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> were measured at different places by several surface stations jointly with low-level cloud occurrence during 50 days. These datasets enable the analysis of modifications in the diurnal cycle of the radiative and <span class="hlt">turbulent</span> surface <span class="hlt">flux</span> induced by the formation and presence of the low-level clouds. The final objective of this study is to estimate the error made in some NWP simulations when the diurnal cycle of low-level clouds is poorly represented or not represented at all.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.afdc.energy.gov/case/2329','SCIGOVWS'); return false;" href="https://www.afdc.energy.gov/case/2329"><span>Alternative Fuels Data Center: <span class="hlt">Sea</span>-Tac and Alaska <span class="hlt">Air</span> Group Achieve</span></a></p> <p><a target="_blank" href="http://www.science.gov/aboutsearch.html">Science.gov Websites</a></p> <p></p> <p></p> <p>pilot project, Alaska <span class="hlt">Air</span> <em>Group</em> encountered a few hurdles during the switch to eGSE. <em>One</em> was Sky-High Results with Electric Ground Support Equipment</A> <span class="hlt">Sea</span>-Tac and Alaska <span class="hlt">Air</span> <em>Group</em> Achieve Data Center: <span class="hlt">Sea</span>-Tac and Alaska <span class="hlt">Air</span> <em>Group</em> Achieve Sky-High Results with Electric Ground Support</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160000481','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160000481"><span>Comparison of <span class="hlt">Turbulent</span> Heat-Transfer Results for Uniform Wall Heat <span class="hlt">Flux</span> and Uniform Wall Temperature</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Siegel, R.; Sparrow, E. M.</p> <p>1960-01-01</p> <p>The purpose of this note is to examine in a more precise way how the Nusselt numbers for <span class="hlt">turbulent</span> heat transfer in both the fully developed and thermal entrance regions of a circular tube are affected by two different wall boundary conditions. The comparisons are made for: (a) Uniform wall temperature (UWT); and (b) uniform wall heat <span class="hlt">flux</span> (UHF). Several papers which have been concerned with the <span class="hlt">turbulent</span> thermal entrance region problem are given. 1 Although these analyses have all utilized an eigenvalue formulation for the thermal entrance region there were differences in the choices of eddy diffusivity expressions, velocity distributions, and methods for carrying out the numerical solutions. These differences were also found in the fully developed analyses. Hence when making a comparison of the analytical results for uniform wall temperature and uniform wall heat <span class="hlt">flux</span>, it was not known if differences in the Nusselt numbers could be wholly attributed to the difference in wall boundary conditions, since all the analytical results were not obtained in a consistent way. To have results which could be directly compared, computations were carried out for the uniform wall temperature case, using the same eddy diffusivity, velocity distribution, and digital computer program employed for uniform wall heat <span class="hlt">flux</span>. In addition, the previous work was extended to a lower Reynolds number range so that comparisons could be made over a wide range of both Reynolds and Prandtl numbers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMPA31A2194W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMPA31A2194W"><span><span class="hlt">Turbulence</span> Ahead! How Climate Change Will Affect <span class="hlt">Air</span> Travel</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Williams, P.</p> <p>2016-12-01</p> <p>The climate is changing, not just where we live at ground level, but also where we fly at 35,000 feet. Climate change has important consequences for aviation, because the atmosphere's meteorological characteristics strongly influence flight routes, journey times, and <span class="hlt">turbulence</span>. This presentation will review the possible impacts of climate change on aviation, which have only recently begun to emerge (as opposed to the impacts of aviation on climate change, which have long been recognised). To investigate the influence of climate change on flight routes and journey times, we feed atmospheric wind fields generated from climate model simulations into a routing algorithm of the type used operationally by flight planners. We focus on transatlantic flights between London and New York, and how they change when the atmospheric CO2 concentration is doubled. We find that a strengthening of the prevailing jet-stream winds causes eastbound flights to significantly shorten and westbound flights to significantly lengthen in all seasons. Eastbound and westbound crossings in winter become approximately twice as likely to take under 5 h 20 min and over 7 h 00 min, respectively. Even assuming no future growth in aviation, the extrapolation of our results to all transatlantic traffic suggests that aircraft will collectively be airborne for an extra 2000 h each year, burning an extra 7.2 million gallons of jet fuel at a cost of US$ 22 million, and emitting an extra 70 million kg CO2. To investigate the influence of climate change on <span class="hlt">turbulence</span>, we diagnose a basket of 21 clear-<span class="hlt">air</span> <span class="hlt">turbulence</span> measures from climate model simulations. We find that <span class="hlt">turbulence</span> strengthens significantly within the transatlantic flight corridor under climate change. For example, in winter, most <span class="hlt">turbulence</span> measures show a 10-40% increase in the median strength of <span class="hlt">turbulence</span> and a 40-170% increase in the frequency of occurrence of moderate-or-greater <span class="hlt">turbulence</span>. For reference, commercial aircraft currently</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122..726R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122..726R"><span>Surface <span class="hlt">flux</span> and ocean heat transport convergence contributions to seasonal and interannual variations of ocean heat content</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Roberts, C. D.; Palmer, M. D.; Allan, R. P.; Desbruyeres, D. G.; Hyder, P.; Liu, C.; Smith, D.</p> <p>2017-01-01</p> <p>We present an observation-based heat budget analysis for seasonal and interannual variations of ocean heat content (H) in the mixed layer (Hmld) and full-depth ocean (Htot). Surface heat <span class="hlt">flux</span> and ocean heat content estimates are combined using a novel Kalman smoother-based method. Regional contributions from ocean heat transport convergences are inferred as a residual and the dominant drivers of Hmld and Htot are quantified for seasonal and interannual time scales. We find that non-Ekman ocean heat transport processes dominate Hmld variations in the equatorial oceans and regions of strong ocean currents and substantial eddy activity. In these locations, surface temperature anomalies generated by ocean dynamics result in <span class="hlt">turbulent</span> <span class="hlt">flux</span> anomalies that drive the overlying atmosphere. In addition, we find large regions of the Atlantic and Pacific oceans where heat transports combine with local <span class="hlt">air-sea</span> <span class="hlt">fluxes</span> to generate mixed layer temperature anomalies. In all locations, except regions of deep convection and water mass transformation, interannual variations in Htot are dominated by the internal rearrangement of heat by ocean dynamics rather than the loss or addition of heat at the surface. Our analysis suggests that, even in extratropical latitudes, initialization of ocean dynamical processes could be an important source of skill for interannual predictability of Hmld and Htot. Furthermore, we expect variations in Htot (and thus thermosteric <span class="hlt">sea</span> level) to be more predictable than near surface temperature anomalies due to the increased importance of ocean heat transport processes for full-depth heat budgets.</p> </li> <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('http://adsabs.harvard.edu/abs/2014EGUGA..1616139K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1616139K"><span>Super Ensemble-based Aviation <span class="hlt">Turbulence</span> Guidance (SEATG) for <span class="hlt">Air</span> Traffic Management (ATM)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kim, Jung-Hoon; Chan, William; Sridhar, Banavar; Sharman, Robert</p> <p>2014-05-01</p> <p>Super Ensemble (ensemble of ten <span class="hlt">turbulence</span> metrics from time-lagged ensemble members of weather forecast data)-based Aviation <span class="hlt">Turbulence</span> Guidance (SEATG) is developed using Weather Research and Forecasting (WRF) model and in-situ eddy dissipation rate (EDR) observations equipped on commercial aircraft over the contiguous United States. SEATG is a sequence of five procedures including weather modeling, calculating <span class="hlt">turbulence</span> metrics, mapping EDR-scale, evaluating metrics, and producing final SEATG forecast. This uses similar methodology to the operational Graphic <span class="hlt">Turbulence</span> Guidance (GTG) with three major improvements. First, SEATG use a higher resolution (3-km) WRF model to capture cloud-resolving scale phenomena. Second, SEATG computes <span class="hlt">turbulence</span> metrics for multiple forecasts that are combined at the same valid time resulting in an time-lagged ensemble of multiple <span class="hlt">turbulence</span> metrics. Third, SEATG provides both deterministic and probabilistic <span class="hlt">turbulence</span> forecasts to take into account weather uncertainties and user demands. It is found that the SEATG forecasts match well with observed radar reflectivity along a surface front as well as convectively induced <span class="hlt">turbulence</span> outside the clouds on 7-8 Sep 2012. And, overall performance skill of deterministic SEATG against the observed EDR data during this period is superior to any single <span class="hlt">turbulence</span> metrics. Finally, probabilistic SEATG is used as an example application of <span class="hlt">turbulence</span> forecast for <span class="hlt">air</span>-traffic management. In this study, a simple Wind-Optimal Route (WOR) passing through the potential areas of probabilistic SEATG and Lateral <span class="hlt">Turbulence</span> Avoidance Route (LTAR) taking into account the SEATG are calculated at z = 35000 ft (z = 12 km) from Los Angeles to John F. Kennedy international airports. As a result, WOR takes total of 239 minutes with 16 minutes of SEATG areas for 40% of moderate <span class="hlt">turbulence</span> potential, while LTAR takes total of 252 minutes travel time that 5% of fuel would be additionally consumed to entirely</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.A33B0145K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.A33B0145K"><span>An Optimal Estimation Method to Obtain Surface Layer <span class="hlt">Turbulent</span> <span class="hlt">Fluxes</span> from Profile Measurements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kang, D.</p> <p>2015-12-01</p> <p>In the absence of direct <span class="hlt">turbulence</span> measurements, the <span class="hlt">turbulence</span> characteristics of the atmospheric surface layer are often derived from measurements of the surface layer mean properties based on Monin-Obukhov Similarity Theory (MOST). This approach requires two levels of the ensemble mean wind, temperature, and water vapor, from which the <span class="hlt">fluxes</span> of momentum, sensible heat, and water vapor can be obtained. When only one measurement level is available, the roughness heights and the assumed properties of the corresponding variables at the respective roughness heights are used. In practice, the temporal mean with large number of samples are used in place of the ensemble mean. However, in many situations the samples of data are taken from multiple levels. It is thus desirable to derive the boundary layer <span class="hlt">flux</span> properties using all measurements. In this study, we used an optimal estimation approach to derive surface layer properties based on all available measurements. This approach assumes that the samples are taken from a population whose ensemble mean profile follows the MOST. An optimized estimate is obtained when the results yield a minimum cost function defined as a weighted summation of all error variance at each sample altitude. The weights are based one sample data variance and the altitude of the measurements. This method was applied to measurements in the marine atmospheric surface layer from a small boat using radiosonde on a tethered balloon where temperature and relative humidity profiles in the lowest 50 m were made repeatedly in about 30 minutes. We will present the resultant <span class="hlt">fluxes</span> and the derived MOST mean profiles using different sets of measurements. The advantage of this method over the 'traditional' methods will be illustrated. Some limitations of this optimization method will also be discussed. Its application to quantify the effects of marine surface layer environment on radar and communication signal propagation will be shown as well.</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/2015AGUFM.H31A1400O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.H31A1400O"><span>Investigation of the influence of atmospheric stability and <span class="hlt">turbulence</span> on land-atmosphere exchange</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Osibanjo, O.; Holmes, H.</p> <p>2015-12-01</p> <p>Surface energy <span class="hlt">fluxes</span> are exchanged between the surface of the earth and the atmosphere and impact weather, climate, and <span class="hlt">air</span> quality. The radiation from the sun triggers the surface-atmosphere interaction during the day as heat is transmitted to the surface and the surface heats the <span class="hlt">air</span> directly above generating wind (i.e., thermal <span class="hlt">turbulence</span>) that transports heat, moisture, and momentum in the atmospheric boundary layer (ABL). This process is impacted by greenhouse gasses (i.e., water vapor, carbon dioxide and other trace gases) that absorb heat emitted by the earth's surface. The concentrations of atmospheric greenhouse gasses are increasing leading to changes in ABL dynamics as a result of the changing surface energy balance. The ABL processes are important to characterize because they are difficult to parameterize in global and regional scale atmospheric models. Empirical data can be collected using eddy covariance micrometeorological methods to measure <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> (e.g., sensible heat, moisture, and CO2) and quantify the exchange between the surface and the atmosphere. The objective of this work is to calculate surface <span class="hlt">fluxes</span> using observational data collected during one week in September 2014 from a monitoring site in Echo, Oregon. The site is located in the Columbia Basin with rolling terrain, irrigated farmland, and over 100 wind turbines. The 10m tower was placed in a small valley depression to isolate nighttime cold <span class="hlt">air</span> pools. This work will present observations of momentum, sensible heat, moisture, and carbon dioxide <span class="hlt">fluxes</span> from data collected at a sampling frequency of 10Hz at four heights. Atmospheric stability is determined using Monin-Obukov length and <span class="hlt">flux</span> Richardson number, and the impact of stability on surface-atmosphere exchange is investigated. This work will provide a better understanding of surface <span class="hlt">fluxes</span> and mixing, particularly during stable ABL periods, and the results can be used to compare with numerical models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.1503Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.1503Z"><span>Why <span class="hlt">turbulence</span> sustains in supercritically stratified free atmosphere?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zilitinkevich, Sergej</p> <p>2016-04-01</p> <p>It is widely believed that in very stable stratifications, at Richardson numbers (Ri) exceeding critical value Ric ˜ 0.25 <span class="hlt">turbulence</span> decays and flow becomes laminar. This is so at low Reynolds numbers (Re), e.g., in lab experiments; but this is not true in very-high-Re geophysical flows. Free atmosphere and deep ocean are <span class="hlt">turbulent</span> in spite of strongly supercritical stratifications: 1 << Ri < 103. Until recently, this paradox remained unexplained. The Energy- and <span class="hlt">Flux</span>-Budget (EFB) <span class="hlt">turbulence</span>-closure (Zilitinkevich et al., 2013) has disclosed the following <span class="hlt">turbulence</span> self-control mechanisms. Until recently, the role of negative buoyancy <span class="hlt">flux</span>, Fb > 0, in <span class="hlt">turbulence</span> energetics was treated in terms of the <span class="hlt">turbulent</span> kinetic energy (TKE) budget equation and understood as just consumption of TKE by the buoyancy forces. This has led to the conclusion that sufficiently strong static stability causes the negative buoyancy <span class="hlt">flux</span> sufficiently strong to exceed the TKE generation rate and thus to kill <span class="hlt">turbulence</span>. However, considering TKE equation together with budget equation for <span class="hlt">turbulent</span> potential energy (TPE proportional to the squared buoyancy fluctuations) shows that the role of Fb in <span class="hlt">turbulence</span> energetics is nothing but conversion of TKE into TPE (Fb just quantifies the rate of this conversion); so that Fb does not affect total <span class="hlt">turbulent</span> energy (TTE = TKE + TPE). Moreover, as follows from the buoyancy-<span class="hlt">flux</span> budget equation, TPE generates positive (directed upward) buoyancy <span class="hlt">flux</span> irrespective of the sign of the buoyancy gradient. Indeed, the warmer fluid particles (with positive buoyancy fluctuation) rise up, whereas the cooler particles sink down, so that both contribute to the positive buoyancy <span class="hlt">flux</span> opposing to the usual, negative <span class="hlt">flux</span> generated by mean buoyancy gradient. In this context, strengthening the negative buoyancy <span class="hlt">flux</span> leads to decreasing TKE and increasing TPE. The latter enhances the counter-gradient share of the total <span class="hlt">flux</span>, thus reduces |Fb| and, eventually</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011WRR....47.5517G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011WRR....47.5517G"><span>Measuring and modeling the <span class="hlt">flux</span> of fecal bacteria across the sediment-water interface in a <span class="hlt">turbulent</span> stream</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Grant, Stanley B.; Litton-Mueller, Rachel M.; Ahn, Jong H.</p> <p>2011-05-01</p> <p>Sediments are a pervasive source of fecal indicator bacteria (FIB) in rivers, lakes, estuaries, and oceans and may constitute a long-term reservoir of human disease. Previous attempts to quantify the <span class="hlt">flux</span> of FIB across the sediment-water interface (SWI) are limited to extreme flow events, for which the primary mechanism of bacterial release is disruption and/or erosion of the sediment substrate. Here we report measurements of FIB <span class="hlt">flux</span> across the SWI in a <span class="hlt">turbulent</span> stream that is not undergoing significant erosion. The stream is formed by the steady discharge of bacteria-free disinfected and highly treated wastewater effluent to an earthen channel harboring high concentrations of FIB in the sediment from in situ growth. The <span class="hlt">flux</span> j″ of FIB across the SWI, estimated from mass balance on FIB measurements in the water column, scales linearly with the concentration of bacteria in sediment pore fluids Cpore over a 3 decade change in both variables: ? The magnitude of the observed mass transfer velocity (? m s-1) is significantly larger than values predicted for either the diffusion of bacteria across a concentration boundary layer (? m s-1) or sweep and eject fluid motions at the SWI (? m s-1) but is similar to the <span class="hlt">flux</span> of water between the stream and its hyporheic zone estimated from dye injection experiments. These results support the hypothesis that hyporheic exchange controls the trafficking of bacteria, and perhaps other types of particulate organic matter, across the SWI in <span class="hlt">turbulent</span> streams.</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/2004AGUFMGC51A1049C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004AGUFMGC51A1049C"><span>Surface <span class="hlt">Flux</span> Measurements at King Sejong Station in 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>Choi, T.; Lee, B.; Lee, H.; Shim, J.</p> <p>2004-12-01</p> <p>The Antarctic Peninsula is important in terms of global warming research due to pronounced increase of <span class="hlt">air</span> temperature over the last century. The first eddy covariance system was established and <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> of heat, water vapor, CO2 and momentum have been measured at King Sejong Station (62 \\deg 13øØS, 58 \\deg 47øØW) located in the northern edge of the Antarctic Peninsula since December in 2002. Our objectives are to better understand the interactions between the Antarctic land surface and the atmosphere and to test the feasibility of the long-term operation of eddy covariance system under extreme weather conditions. Various lichens cover the study area and the dominant species is Usnea fasciata-Himantormia. Based on the analyses on <span class="hlt">turbulent</span> statistics such as integral <span class="hlt">turbulence</span> characteristics of vertical velocity (w) and heat (T), stationarity test and investigation of correlation coefficient, they follow the Monin-Obukhov similarity and eddy covariance <span class="hlt">flux</span> data were reliable. About 50 % of total retrieved sensible heat <span class="hlt">flux</span> data could be used for further analysis. We will report on seasonal variations of energy and mass <span class="hlt">fluxes</span> and environmental variables. In addition, factors controlling these <span class="hlt">fluxes</span> will be presented. Acknowledgement: This study was supported by ¡rEnvironmental Monitoring on Human Impacts at the King Sejong Station, Antarctica¡_ (Project PP04102 of Korea Polar Research Institute) and ¡rEco-technopia 21 project¡_ (Ministry of Environment of Korea).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1374317-variable-density-mixing-turbulent-jets-coflow','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1374317-variable-density-mixing-turbulent-jets-coflow"><span>Variable density mixing in <span class="hlt">turbulent</span> jets with coflow</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>Charonko, John James; Prestridge, Katherine Philomena</p> <p></p> <p>Two sets of experiments are performed to study variable-density effects in <span class="hlt">turbulent</span> round jets with co flow at density ratios, s = 4.2 and s = 1.2. 10,000 instantaneous realisations of simultaneous 2-D PIV and PLIF at three axial locations in the momentumdominated region of the jet allow us to calculate the full t.k.e. budgets, providing insights into the mechanisms of density fluctuation correlations both axially and radially in a non- Boussinesq flow. The strongest variable-density effects are observed within the velocity half-width of the jet, r ~u1/2 . Variable density effects decrease the Reynolds stresses via increased <span class="hlt">turbulent</span> massmore » <span class="hlt">flux</span> in the heavy jet, as shown by previous jet centreline measurements. Radial pro les of <span class="hlt">turbulent</span> <span class="hlt">flux</span> show that in the lighter jet t.k.e. is moving away from the centreline, while in the heavy jet it is being transported both inwards towards the centreline and radially outwards. Negative t.k.e. production is observed in the heavy jet, and we demonstrate that this is caused by both reduced gradient stretching in the axial direction and increased <span class="hlt">turbulent</span> mass <span class="hlt">fluxes</span>. Large differences in advection are also observed between the two jets. The <span class="hlt">air</span> jet has higher total advection caused by strong axial components, while density fluctuations in the heavy jet reduce the axial advection signi cantly. The budget mechanisms in the non-Boussinesq regime are best understood using effective density and velocity half-width, ρeff ¯u 3 1,CL/r ~u1/2,eff , a modi cation of previous scaling.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1374317-variable-density-mixing-turbulent-jets-coflow','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1374317-variable-density-mixing-turbulent-jets-coflow"><span>Variable density mixing in <span class="hlt">turbulent</span> jets with coflow</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Charonko, John James; Prestridge, Katherine Philomena</p> <p>2017-07-24</p> <p>Two sets of experiments are performed to study variable-density effects in <span class="hlt">turbulent</span> round jets with co flow at density ratios, s = 4.2 and s = 1.2. 10,000 instantaneous realisations of simultaneous 2-D PIV and PLIF at three axial locations in the momentumdominated region of the jet allow us to calculate the full t.k.e. budgets, providing insights into the mechanisms of density fluctuation correlations both axially and radially in a non- Boussinesq flow. The strongest variable-density effects are observed within the velocity half-width of the jet, r ~u1/2 . Variable density effects decrease the Reynolds stresses via increased <span class="hlt">turbulent</span> massmore » <span class="hlt">flux</span> in the heavy jet, as shown by previous jet centreline measurements. Radial pro les of <span class="hlt">turbulent</span> <span class="hlt">flux</span> show that in the lighter jet t.k.e. is moving away from the centreline, while in the heavy jet it is being transported both inwards towards the centreline and radially outwards. Negative t.k.e. production is observed in the heavy jet, and we demonstrate that this is caused by both reduced gradient stretching in the axial direction and increased <span class="hlt">turbulent</span> mass <span class="hlt">fluxes</span>. Large differences in advection are also observed between the two jets. The <span class="hlt">air</span> jet has higher total advection caused by strong axial components, while density fluctuations in the heavy jet reduce the axial advection signi cantly. The budget mechanisms in the non-Boussinesq regime are best understood using effective density and velocity half-width, ρeff ¯u 3 1,CL/r ~u1/2,eff , a modi cation of previous scaling.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003PhDT.......143C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003PhDT.......143C"><span>Monte-Carlo computation of <span class="hlt">turbulent</span> premixed methane/<span class="hlt">air</span> ignition</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carmen, Christina Lieselotte</p> <p></p> <p>The present work describes the results obtained by a time dependent numerical technique that simulates the early flame development of a spark-ignited premixed, lean, gaseous methane/<span class="hlt">air</span> mixture with the unsteady spherical flame propagating in homogeneous and isotropic <span class="hlt">turbulence</span>. The algorithm described is based upon a sub-model developed by an international automobile research and manufacturing corporation in order to analyze <span class="hlt">turbulence</span> conditions within internal combustion engines. Several developments and modifications to the original algorithm have been implemented including a revised chemical reaction scheme and the evaluation and calculation of various <span class="hlt">turbulent</span> flame properties. Solution of the complete set of Navier-Stokes governing equations for a <span class="hlt">turbulent</span> reactive flow is avoided by reducing the equations to a single transport equation. The transport equation is derived from the Navier-Stokes equations for a joint probability density function, thus requiring no closure assumptions for the Reynolds stresses. A Monte-Carlo method is also utilized to simulate phenomena represented by the probability density function transport equation by use of the method of fractional steps. Gaussian distributions of fluctuating velocity and fuel concentration are prescribed. Attention is focused on the evaluation of the three primary parameters that influence the initial flame kernel growth-the ignition system characteristics, the mixture composition, and the nature of the flow field. Efforts are concentrated on the effects of moderate to intense <span class="hlt">turbulence</span> on flames within the distributed reaction zone. Results are presented for lean conditions with the fuel equivalence ratio varying from 0.6 to 0.9. The present computational results, including flame regime analysis and the calculation of various flame speeds, provide excellent agreement with results obtained by other experimental and numerical researchers.</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/2016EGUGA..1818323B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1818323B"><span>Structure of the airflow above 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>Buckley, Marc; Veron, Fabrice</p> <p>2016-04-01</p> <p>Weather, climate and upper ocean patterns are controlled by the exchanges of momentum, heat, mass, and energy across the ocean surface. These <span class="hlt">fluxes</span> are, in turn, influenced by the small-scale physics at the wavy <span class="hlt">air-sea</span> interface. We present laboratory measurements of the fine-scale airflow structure above waves, achieved in over 15 different wind-wave conditions, with wave ages Cp/u* ranging from 1.4 to 66.7 (where Cp is the peak phase speed of the waves, and u* the <span class="hlt">air</span> friction velocity). The experiments were performed in the large (42-m long) wind-wave-current tank at University of Delaware's <span class="hlt">Air-Sea</span> Interaction laboratory (USA). A combined Particle Image Velocimetry and Laser Induced Fluorescence system was specifically developed for this study, and provided two-dimensional airflow velocity measurement as low as 100 um above the <span class="hlt">air</span>-water interface. Starting at very low wind speeds (U10~2m/s), we directly observe coherent <span class="hlt">turbulent</span> structures within the buffer and logarithmic layers of the airflow above the <span class="hlt">air</span>-water interface, whereby low horizontal velocity <span class="hlt">air</span> is ejected away from the surface, and higher velocity fluid is swept downward. Wave phase coherent quadrant analysis shows that such <span class="hlt">turbulent</span> momentum <span class="hlt">flux</span> events are wave-phase dependent. Airflow separation events are directly observed over young wind waves (Cp/u*<3.7) and counted using measured vorticity and surface viscous stress criteria. Detached high spanwise vorticity layers cause intense wave-coherent <span class="hlt">turbulence</span> downwind of wave crests, as shown by wave-phase averaging of <span class="hlt">turbulent</span> momentum <span class="hlt">fluxes</span>. Mean wave-coherent airflow motions and <span class="hlt">fluxes</span> also show strong phase-locked patterns, including a sheltering effect, upwind of wave crests over old mechanically generated swells (Cp/u*=31.7), and downwind of crests over young wind waves (Cp/u*=3.7). Over slightly older wind waves (Cp/u* = 6.5), the measured wave-induced airflow perturbations are qualitatively consistent with linear critical layer</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19990102922','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19990102922"><span>Mesoscale Simulations of a Florida <span class="hlt">Sea</span> Breeze Using the PLACE Land Surface Model Coupled to a 1.5-Order <span class="hlt">Turbulence</span> Parameterization</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lynn, Barry H.; Stauffer, David R.; Wetzel, Peter J.; Tao, Wei-Kuo; Perlin, Natal; Baker, R. David; Munoz, Ricardo; Boone, Aaron; Jia, Yiqin</p> <p>1999-01-01</p> <p>A sophisticated land-surface model, PLACE, the Parameterization for Land Atmospheric Convective Exchange, has been coupled to a 1.5-order <span class="hlt">turbulent</span> kinetic energy (TKE) <span class="hlt">turbulence</span> sub-model. Both have been incorporated into the Penn State/National Center for Atmospheric Research (PSU/NCAR) mesoscale model MM5. Such model improvements should have their greatest effect in conditions where surface contrasts dominate over dynamic processes, such as the simulation of warm-season, convective events. A validation study used the newly coupled model, MM5 TKE-PLACE, to simulate the evolution of Florida <span class="hlt">sea</span>-breeze moist convection during the Convection and Precipitation Electrification Experiment (CaPE). Overall, eight simulations tested the sensitivity of the MM5 model to combinations of the new and default model physics, and initialization of soil moisture and temperature. The TKE-PLACE model produced more realistic surface sensible heat <span class="hlt">flux</span>, lower biases for surface variables, more realistic rainfall, and cloud cover than the default model. Of the 8 simulations with different factors (i.e., model physics or initialization), TKE-PLACE compared very well when each simulation was ranked in terms of biases of the surface variables and rainfall, and percent and root mean square of cloud cover. A factor separation analysis showed that a successful simulation required the inclusion of a multi-layered, land surface soil vegetation model, realistic initial soil moisture, and higher order closure of the planetary boundary layer (PBL). These were needed to realistically model the effect of individual, joint, and synergistic contributions from the land surface and PBL on the CAPE <span class="hlt">sea</span>-breeze, Lake Okeechobee lake breeze, and moist convection.</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('https://www.ncbi.nlm.nih.gov/pubmed/26069469','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26069469"><span>On total <span class="hlt">turbulent</span> energy and the passive and active role of buoyancy in <span class="hlt">turbulent</span> momentum and mass transfer.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>de Nijs, Michel A J; Pietrzak, Julie D</p> <p></p> <p>Measurements of <span class="hlt">turbulent</span> fluctuations of horizontal and vertical components of velocity, salinity and suspended particulate matter are presented. <span class="hlt">Turbulent</span> Prandtl numbers are found to increase with stratification and to become larger than 1. Consequently, the vertical <span class="hlt">turbulent</span> mass transport is suppressed by buoyancy forces, before the <span class="hlt">turbulent</span> kinetic energy (TKE) and vertical <span class="hlt">turbulent</span> momentum exchange are inhibited. With increasing stratification, the buoyancy <span class="hlt">fluxes</span> do not cease, instead they become countergradient. We find that buoyantly driven motions play an active role in the transfer of mass. This is in agreement with trends derived from Monin-Obukhov scaling. For positive Richardson <span class="hlt">flux</span> numbers (Ri f ), the log velocity profile in the near-bed layer requires correction with a drag reduction. For negative Ri f , the log velocity profile should be corrected with a drag increase, with increasing |Ri f |. This highlights the active role played by buoyancy in momentum transfer and the production of TKE. However, the data do not appear to entirely follow Monin-Obukhov scaling. This is consistent with the notion that the <span class="hlt">turbulence</span> field is not in equilibrium. The large stratification results in the decay of <span class="hlt">turbulence</span> and countergradient buoyancy <span class="hlt">fluxes</span> act to restore equilibrium in the energy budget. This implies that there is a finite adjustment timescale of the <span class="hlt">turbulence</span> field to changes in velocity shear and density stratification. The energy transfers associated with the source and sink function of the buoyancy <span class="hlt">flux</span> can be modeled with the concept of total <span class="hlt">turbulent</span> energy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.4521T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.4521T"><span>The effect of agricultural structures on the quality of eddy covariance <span class="hlt">flux</span> data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tanny, Josef; Achiman, Ori; Mekhmandarov, Yonatan; Pirkner, Moran</p> <p>2015-04-01</p> <p>The Eddy Covariance (EC) is a common method to directly measure whole canopy <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> of scalars like water vapor, <span class="hlt">air</span> temperature and CO2. The method was originally developed to measure <span class="hlt">fluxes</span> from canopies in the open; however, in recent years it was also shown to be valid for <span class="hlt">flux</span> measurements of agricultural crops cultivated inside structures covered by porous screens, i.e., screenhouses. To reliably measure <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> by the EC technique, several <span class="hlt">air</span> flow conditions should prevail. The purpose of this study was to examine two criteria, commonly used to assess the suitability of <span class="hlt">turbulent</span> flow conditions for EC measurements in open fields, for <span class="hlt">flux</span> measurements in different types of agricultural screenhouses and greenhouses. The two tests are the "Integral <span class="hlt">Turbulence</span> Characteristics" (ITC), which indicates on the development of the <span class="hlt">turbulent</span> flow, and the "Steady State" (SS), which examines the variation in time of flow statistics during the averaging period. For both tests data was classified according to their suitability for <span class="hlt">flux</span> measurements. The research was conducted in 3 types of agricultural structures with 3 different plants: (S1) A banana screenhouse, 5.5 m in height, covered by an 8% shade net; (S2) A pepper screenhouse, 3.7 m in height, covered by an insect-proof, 50 mesh net; (S3) A 12-span naturally ventilated tomato greenhouse with a 6 m height arched gable, equipped with an insect-proof 50 mesh net on the sidewalls, and impermeable plastic cover on the roof. In each structure an EC system was installed between the top of the canopy and the roof, in a position that provided sufficient fetch for the prevailing wind, for a measurement period of at least 20 days. Mean <span class="hlt">fluxes</span> were calculated over half-hourly time intervals. In the present study the ITC test was applied in two different approaches: (i) according to the commonly used literature model which prevails for <span class="hlt">turbulent</span> flow in open fields (ITC1), and (ii) according to a new</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19970034949','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19970034949"><span>Modeling of <span class="hlt">Turbulent</span> Swirling Flows</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Shih, Tsan-Hsing; Zhu, Jiang; Liou, William; Chen, Kuo-Huey; Liu, Nan-Suey; Lumley, John L.</p> <p>1997-01-01</p> <p>Aircraft engine combustors generally involve <span class="hlt">turbulent</span> swirling flows in order to enhance fuel-<span class="hlt">air</span> mixing and flame stabilization. It has long been recognized that eddy viscosity <span class="hlt">turbulence</span> models are unable to appropriately model swirling flows. Therefore, it has been suggested that, for the modeling of these flows, a second order closure scheme should be considered because of its ability in the modeling of rotational and curvature effects. However, this scheme will require solution of many complicated second moment transport equations (six Reynolds stresses plus other scalar <span class="hlt">fluxes</span> and variances), which is a difficult task for any CFD implementations. Also, this scheme will require a large amount of computer resources for a general combustor swirling flow. This report is devoted to the development of a cubic Reynolds stress-strain model for <span class="hlt">turbulent</span> swirling flows, and was inspired by the work of Launder's group at UMIST. Using this type of model, one only needs to solve two <span class="hlt">turbulence</span> equations, one for the <span class="hlt">turbulent</span> kinetic energy k and the other for the dissipation rate epsilon. The cubic model developed in this report is based on a general Reynolds stress-strain relationship. Two flows have been chosen for model evaluation. One is a fully developed rotating pipe flow, and the other is a more complex flow with swirl and recirculation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016IJMPC..2750095Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016IJMPC..2750095Z"><span>Computational fluid dynamics for modeling the <span class="hlt">turbulent</span> natural convection in a double <span class="hlt">air</span>-channel solar chimney system</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zavala-Guillén, I.; Xamán, J.; Álvarez, G.; Arce, J.; Hernández-Pérez, I.; Gijón-Rivera, M.</p> <p>2016-03-01</p> <p>This study reports the modeling of the <span class="hlt">turbulent</span> natural convection in a double <span class="hlt">air</span>-channel solar chimney (SC-DC) and its comparison with a single <span class="hlt">air</span>-channel solar chimney (SC-C). Prediction of the mass flow and the thermal behavior of the SC-DC were obtained under three different climates of Mexico during one summer day. The climates correspond to: tropical savannah (Mérida), arid desert (Hermosillo) and temperate with warm summer (Mexico City). A code based on the Finite Volume Method was developed and a k-ω <span class="hlt">turbulence</span> model has been used to model <span class="hlt">air</span> <span class="hlt">turbulence</span> in the solar chimney (SC). The code was validated against experimental data. The results indicate that during the day the SC-DC extracts about 50% more mass flow than the SC-C. When the SC-DC is located in Mérida, Hermosillo and Mexico City, the <span class="hlt">air</span>-changes extracted along the day were 60, 63 and 52, respectively. The <span class="hlt">air</span> temperature at the outlet of the chimney increased up to 33%, 38% and 61% with respect to the temperature it has at the inlet for Mérida, Hermosillo and Mexico City, respectively.</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://hdl.handle.net/2060/19990032567','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19990032567"><span>Double Resonances and Spectral Scaling in the Weak <span class="hlt">Turbulence</span> Theory of Rotating and Stratified <span class="hlt">Turbulence</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rubinstein, Robert</p> <p>1999-01-01</p> <p>In rotating <span class="hlt">turbulence</span>, stably stratified <span class="hlt">turbulence</span>, and in rotating stratified <span class="hlt">turbulence</span>, heuristic arguments concerning the <span class="hlt">turbulent</span> time scale suggest that the inertial range energy spectrum scales as k(exp -2). From the viewpoint of weak <span class="hlt">turbulence</span> theory, there are three possibilities which might invalidate these arguments: four-wave interactions could dominate three-wave interactions leading to a modified inertial range energy balance, double resonances could alter the time scale, and the energy <span class="hlt">flux</span> integral might not converge. It is shown that although double resonances exist in all of these problems, they do not influence overall energy transfer. However, the resonance conditions cause the <span class="hlt">flux</span> integral for rotating <span class="hlt">turbulence</span> to diverge logarithmically when evaluated for a k(exp -2) energy spectrum; therefore, this spectrum requires logarithmic corrections. Finally, the role of four-wave interactions is briefly discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.7698W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.7698W"><span>A long term glider study of shelf <span class="hlt">sea</span> oxygen dynamics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Williams, Charlotte; Palmer, Matthew; Mahaffey, Claire; Davis, Clare</p> <p>2017-04-01</p> <p>Oxygen is involved in most biogeochemical processes in the ocean, and dissolved oxygen (DO) is a well-established indicator for biological activity via the estimate of apparent oxygen utilisation (AOU). In the deep waters of the open ocean, the AOU provides a valuable insight into the ocean's biological carbon pump. However, in the physically dynamic and highly productive shallow shelf <span class="hlt">seas</span>, interpretation of the oxygen distribution and the magnitude of AOU is complex. Physical processes, such as diapycnal mixing, entrainment and horizontal advection act to ventilate waters below the thermocline and thus increase oxygen and decrease AOU. In contrast, biological remineralisation of organic material below the thermocline will consume oxygen and increase AOU. We aim to address the following: 1. Does AOU change seasonally in a shelf <span class="hlt">sea</span> in response to seasonal changes in productivity? 2. How important is <span class="hlt">turbulence</span> in redistributing oxygen in a shelf <span class="hlt">sea</span>? Using 9 months of high-resolution data from >20 glider deployments in the seasonally stratified NW European Shelf <span class="hlt">Sea</span> we identify and quantify the physical and biological processes that control the DO distribution and magnitude of AOU in shelf <span class="hlt">seas</span>. A 200km transect between the shelf edge and the central Celtic <span class="hlt">Sea</span> (CCS) was repeated between November 2014 and August 2015, thus capturing key periods in the seasonal cycling in shelf <span class="hlt">seas</span>, specifically the onset of stratification, the spring bloom, stratified summer period and breakdown of stratification. The gliders collected data for DO, temperature, salinity, chlorophyll fluorescence, CDOM, backscatter and <span class="hlt">turbulence</span>. In addition, direct measurements of <span class="hlt">turbulent</span> dissipation from the Ocean Microstructure Glider deployed during the campaign provided estimates of mixing at CCS and the shelf break, allowing accurate quantification of the vertical <span class="hlt">fluxes</span> of oxygen. We find that oxygen decreases ubiquitously across the shelf as soon as stratification takes hold, though BML</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ClDy..tmp..849G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ClDy..tmp..849G"><span>Seasonal and latitudinal variations of surface <span class="hlt">fluxes</span> at two Arctic terrestrial sites</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Grachev, Andrey A.; Persson, P. Ola G.; Uttal, Taneil; Akish, Elena A.; Cox, Christopher J.; Morris, Sara M.; Fairall, Christopher W.; Stone, Robert S.; Lesins, Glen; Makshtas, Alexander P.; Repina, Irina A.</p> <p>2017-11-01</p> <p>This observational study compares seasonal variations of surface <span class="hlt">fluxes</span> (<span class="hlt">turbulent</span>, radiative, and soil heat) and other ancillary atmospheric/surface/permafrost data based on in-situ measurements made at terrestrial research observatories located near the coast of the Arctic Ocean. Hourly-averaged multiyear data sets collected at Eureka (Nunavut, Canada) and Tiksi (East Siberia, Russia) are analyzed in more detail to elucidate similarities and differences in the seasonal cycles at these two Arctic stations, which are situated at significantly different latitudes (80.0°N and 71.6°N, respectively). While significant gross similarities exist in the annual cycles of various meteorological parameters and <span class="hlt">fluxes</span>, the differences in latitude, local topography, cloud cover, snowfall, and soil characteristics produce noticeable differences in <span class="hlt">fluxes</span> and in the structures of the atmospheric boundary layer and upper soil temperature profiles. An important factor is that even though higher latitude sites (in this case Eureka) generally receive less annual incoming solar radiation but more total daily incoming solar radiation throughout the summer months than lower latitude sites (in this case Tiksi). This leads to a counter-intuitive state where the average active layer (or thaw line) is deeper and the topsoil temperature in midsummer are higher in Eureka which is located almost 10° north of Tiksi. The study further highlights the differences in the seasonal and latitudinal variations of the incoming shortwave and net radiation as well as the moderating cloudiness effects that lead to temporal and spatial differences in the structure of the atmospheric boundary layer and the uppermost ground layer. Specifically the warm season (Arctic summer) is shorter and mid-summer amplitude of the surface <span class="hlt">fluxes</span> near solar noon is generally less in Eureka than in Tiksi. During the dark Polar night and cold seasons (Arctic winter) when the ground is covered with snow and <span class="hlt">air</span> temperatures</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/2016AGUFM.H32B..07W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.H32B..07W"><span>Observational constraints on Arctic boundary-layer clouds, surface moisture and sensible heat <span class="hlt">fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wu, D. L.; Boisvert, L.; Klaus, D.; Dethloff, K.; Ganeshan, M.</p> <p>2016-12-01</p> <p>The dry, cold environment and dynamic surface variations make the Arctic a unique but difficult region for observations, especially in the atmospheric boundary layer (ABL). Spaceborne platforms have been the key vantage point to capture basin-scale changes during the recent Arctic warming. Using the <span class="hlt">AIRS</span> temperature, moisture and surface data, we found that the Arctic surface moisture <span class="hlt">flux</span> (SMF) had increased by 7% during 2003-2013 (18 W/m2 equivalent in latent heat), mostly in spring and fall near the Arctic coastal <span class="hlt">seas</span> where large <span class="hlt">sea</span> ice reduction and <span class="hlt">sea</span> surface temperature (SST) increase were observed. The increase in Arctic SMF correlated well with the increases in total atmospheric column water vapor and low-level clouds, when compared to CALIPSO cloud observations. It has been challenging for climate models to reliably determine Arctic cloud radiative forcing (CRF). Using the regional climate model HIRHAM5 and assuming a more efficient Bergeron-Findeisen process with generalized subgrid-scale variability for total water content, we were able to produce a cloud distribution that is more consistent with the CloudSat/CALIPSO observations. More importantly, the modified schemes decrease (increase) the cloud water (ice) content in mixed-phase clouds, which help to improve the modeled CRF and energy budget at the surface, because of the dominant role of the liquid water in CRF. Yet, the coupling between Arctic low clouds and the surface is complex and has strong impacts on ABL. Studying GPS/COSMIC radio occultation (RO) refractivity profiles in the Arctic coldest and driest months, we successfully derived ABL inversion height and surface-based inversion (SBI) frequency, and they were anti-correlated over the Arctic Ocean. For the late summer and early fall season, we further analyzed Japanese R/V Mirai ship measurements and found that the open-ocean surface sensible heat <span class="hlt">flux</span> (SSHF) can explain 10 % of the ABL height variability, whereas mechanisms such as cloud</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19950044394&hterms=kinetic+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dkinetic%2Benergy','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19950044394&hterms=kinetic+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dkinetic%2Benergy"><span>Development and analysis of prognostic equations for mesoscale kinetic energy and mesoscale (subgrid scale) <span class="hlt">fluxes</span> for large-scale atmospheric models</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Avissar, Roni; Chen, Fei</p> <p>1993-01-01</p> <p>Generated by landscape discontinuities (e.g., <span class="hlt">sea</span> breezes) mesoscale circulation processes are not represented in large-scale atmospheric models (e.g., general circulation models), which have an inappropiate grid-scale resolution. With the assumption that atmospheric variables can be separated into large scale, mesoscale, and <span class="hlt">turbulent</span> scale, a set of prognostic equations applicable in large-scale atmospheric models for momentum, temperature, moisture, and any other gaseous or aerosol material, which includes both mesoscale and <span class="hlt">turbulent</span> <span class="hlt">fluxes</span> is developed. Prognostic equations are also developed for these mesoscale <span class="hlt">fluxes</span>, which indicate a closure problem and, therefore, require a parameterization. For this purpose, the mean mesoscale kinetic energy (MKE) per unit of mass is used, defined as E-tilde = 0.5 (the mean value of u'(sub i exp 2), where u'(sub i) represents the three Cartesian components of a mesoscale circulation (the angle bracket symbol is the grid-scale, horizontal averaging operator in the large-scale model, and a tilde indicates a corresponding large-scale mean value). A prognostic equation is developed for E-tilde, and an analysis of the different terms of this equation indicates that the mesoscale vertical heat <span class="hlt">flux</span>, the mesoscale pressure correlation, and the interaction between <span class="hlt">turbulence</span> and mesoscale perturbations are the major terms that affect the time tendency of E-tilde. A-state-of-the-art mesoscale atmospheric model is used to investigate the relationship between MKE, landscape discontinuities (as characterized by the spatial distribution of heat <span class="hlt">fluxes</span> at the earth's surface), and mesoscale sensible and latent heat <span class="hlt">fluxes</span> in the atmosphere. MKE is compared with <span class="hlt">turbulence</span> kinetic energy to illustrate the importance of mesoscale processes as compared to <span class="hlt">turbulent</span> processes. This analysis emphasizes the potential use of MKE to bridge between landscape discontinuities and mesoscale <span class="hlt">fluxes</span> and, therefore, to parameterize mesoscale <span class="hlt">fluxes</span></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/2017AGUFM.A13H2190P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A13H2190P"><span>Simulating the Cyclone Induced <span class="hlt">Turbulent</span> Mixing in the Bay of Bengal using COAWST Model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Prakash, K. R.; Nigam, T.; Pant, V.</p> <p>2017-12-01</p> <p>Mixing in the upper oceanic layers (up to a few tens of meters from surface) is an important process to understand the evolution of <span class="hlt">sea</span> surface properties. Enhanced mixing due to strong wind forcing at surface leads to deepening of mixed layer that affects the <span class="hlt">air-sea</span> exchange of heat and momentum <span class="hlt">fluxes</span> and modulates <span class="hlt">sea</span> surface temperature (SST). In the present study, we used Coupled-Ocean-Atmosphere-Wave-Sediment Transport (COAWST) model to demonstrate and quantify the enhanced cyclone induced <span class="hlt">turbulent</span> mixing in case of a severe cyclonic storm. The COAWST model was configured over the Bay of Bengal (BoB) and used to simulate the atmospheric and oceanic conditions prevailing during the tropical cyclone (TC) Phailin that occurred over the BoB during 10-15 October 2013. The model simulated cyclone track was validated with IMD best-track and model SST validated with daily AVHRR SST data. Validation shows that model simulated track & intensity, SST and salinity were in good agreement with observations and the cyclone induced cooling of the <span class="hlt">sea</span> surface was well captured by the model. Model simulations show a considerable deepening (by 10-15 m) of the mixed layer and shoaling of thermocline during TC Phailin. The power spectrum analysis was performed on the zonal and meridional baroclinic current components, which shows strongest energy at 14 m depth. Model results were analyzed to investigate the non-uniform energy distribution in the water column from surface up to the thermocline depth. The rotary spectra analysis highlights the downward direction of <span class="hlt">turbulent</span> mixing during the TC Phailin period. Model simulations were used to quantify and interpret the near-inertial mixing, which were generated by cyclone induced strong wind stress and the near-inertial energy. These near-inertial oscillations are responsible for the enhancement of the mixing operative in the strong post-monsoon (October-November) stratification in the BoB.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.A31D0063S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.A31D0063S"><span>Measurements of Vertical Profiles of <span class="hlt">Turbulence</span>, Temperature, Ozone, Aerosols, and BrO over <span class="hlt">Sea</span> Ice and Tundra Snowpack during BROMEX</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shepson, P.; Caulton, D.; Cambaliza, M. L.; Dhaniyala, S.; Fuentes, J. D.; General, S.; Halfacre, J. W.; Nghiem, S. V.; Perez Perez, L.; Peterson, P. K.; Platt, U.; Pohler, D.; Pratt, K. A.; Simpson, W. R.; Stirm, B.; Walsh, S. J.; Zielcke, J.</p> <p>2012-12-01</p> <p>During the BROMEX field campaign of March 2012, we conducted measurements of boundary layer structure, ozone, BrO and aerosol, from a light, twin-engine aircraft during eleven flights originating from Barrow, AK. Flights were conducted over the <span class="hlt">sea</span> ice in the Beaufort and Chukchi <span class="hlt">Seas</span>, and over the tundra from Barrow to the Brooks Range, with vertical profiles covering altitudes from the surface to 3.5km in the free troposphere. Flights over the course of one month allowed a variety of <span class="hlt">sea</span> ice conditions, including open water, nilas, first year <span class="hlt">sea</span> ice, and frost flowers, to be examined over the Chukchi <span class="hlt">Sea</span>. Atmospheric <span class="hlt">turbulence</span> was measured using a calibrated <span class="hlt">turbulence</span> probe, which will enable characterization of both the structure and <span class="hlt">turbulence</span> of the Arctic boundary layer. Ozone was measured using a 2B UV absorption instrument. A GRIMM optical particle counter was used to measure 0.25-4 μm sized aerosol particles. The MAX-DOAS instrument enabled measurements of BrO vertical profiles. The aircraft measurements can be used to connect the surface measurements of ozone and BrO from the "Icelander" buoys, and the surface sites at Barrow, with those measured on the aircraft. Here we will discuss the spatial variability/coherence in these data. A major question that will be addressed using these data is the extent to which bromine is activated through reactions at the snowpack/ice surface versus the surface of aerosols. Here we will present a preliminary analysis of the relationships between snow/ice surface types, aerosol size-resolved number concentrations, and the vertical profiles of ozone and BrO.</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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