Sample records for open ocean waters

  1. Wind energy input into the upper ocean over a lengthening open water season

    NASA Astrophysics Data System (ADS)

    Mahoney, A. R.; Rolph, R.; Walsh, J. E.

    2017-12-01

    Wind energy input into the ocean has important consequences for upper ocean mixing, heat and gas exchange, and air-sea momentum transfer. In the Arctic, the open water season is increasing and extending further into the fall storm season, allowing for more wind energy input into the water column. The rate at which the delayed freeze-up timing extends into fall storm season is an important metric to evaluate because the expanding overlap between the open water period and storm season could contribute a significant amount of wind energy into the water column in a relatively short period of time. We have shown that time-integrated wind speeds over open water in the Chukchi Sea and southern Beaufort region have increased since 1979 through 2014. An integrated wind energy input value is calculated for each year in this domain over the open water season, as well as for periods over partial concentrations of ice cover. Spatial variation of this integrated wind energy is shown along the Alaskan coastline, which can have implications for different rates of coastal erosion. Spatial correlation between average wind speed over open water and open water season length from 1979-2014 show positive values in the southern Beaufort, but negative values in the northern Chukchi. This suggests possible differences in the role of the ocean on open water season length depending on region. We speculate that the warm Pacific water outflow plays a more dominant role in extending the open water season length in the northern Chukchi when compared to the southern Beaufort, and might help explain why we can show there is a relatively longer open water season length there. The negative and positive correlations in wind speeds over open water and open water season length might also be explained by oceanic changes tending to operate on longer timescales than the atmosphere. Seasonal timescales of wind events such as regional differences in overlap of the extended open water season due to regional

  2. Sensitivity of open-water ice growth and ice concentration evolution in a coupled atmosphere-ocean-sea ice model

    NASA Astrophysics Data System (ADS)

    Shi, Xiaoxu; Lohmann, Gerrit

    2017-09-01

    A coupled atmosphere-ocean-sea ice model is applied to investigate to what degree the area-thickness distribution of new ice formed in open water affects the ice and ocean properties. Two sensitivity experiments are performed which modify the horizontal-to-vertical aspect ratio of open-water ice growth. The resulting changes in the Arctic sea-ice concentration strongly affect the surface albedo, the ocean heat release to the atmosphere, and the sea-ice production. The changes are further amplified through a positive feedback mechanism among the Arctic sea ice, the Atlantic Meridional Overturning Circulation (AMOC), and the surface air temperature in the Arctic, as the Fram Strait sea ice import influences the freshwater budget in the North Atlantic Ocean. Anomalies in sea-ice transport lead to changes in sea surface properties of the North Atlantic and the strength of AMOC. For the Southern Ocean, the most pronounced change is a warming along the Antarctic Circumpolar Current (ACC), owing to the interhemispheric bipolar seasaw linked to AMOC weakening. Another insight of this study lies on the improvement of our climate model. The ocean component FESOM is a newly developed ocean-sea ice model with an unstructured mesh and multi-resolution. We find that the subpolar sea-ice boundary in the Northern Hemisphere can be improved by tuning the process of open-water ice growth, which strongly influences the sea ice concentration in the marginal ice zone, the North Atlantic circulation, salinity and Arctic sea ice volume. Since the distribution of new ice on open water relies on many uncertain parameters and the knowledge of the detailed processes is currently too crude, it is a challenge to implement the processes realistically into models. Based on our sensitivity experiments, we conclude a pronounced uncertainty related to open-water sea ice growth which could significantly affect the climate system sensitivity.

  3. Open Ocean Assessments for Management in the GEF Transboundary Waters Assessment Project (TWAP)

    NASA Astrophysics Data System (ADS)

    Fischer, A. S.; Alverson, K. D.

    2010-12-01

    A methodology for a thematic and scientifically-credible assessment of Open Ocean waters as a part of the Global Environment Facility (GEF) Transboundary Waters Assessment Project (TWAP) has been developed in the last 18 months by the Intergovernmental Oceanographic Commission of UNESCO, and is presented for feedback and comment. While developed to help the GEF International Waters focal area target investment to manage looming environmental threats in interlinked freshwater and marine systems (a very focused decision support system), the assessment methodology could contribute to other assessment and management efforts in the UN system and elsewhere. Building on a conceptual framework that describes the relationships between human systems and open ocean natural systems, and on mapping of the human impact on the marine environment, the assessment will evaluate and make projections on a thematic basis, identifying key metrics, indices, and indicators. These themes will include the threats on key ecosystem services of climate change through sea level rise, changed stratification, warming, and ocean acidification; vulnerabilities of ecosystems, habitats, and living marine resources; the impact and sustainability of fisheries; and pollution. Global-level governance arrangements will also be evaluated, with an eye to identifying scope for improved global-level management. The assessment will build on sustained ocean observing systems, model projections, and an assessment of scientific literature, as well as tools for combining knowledge to support identification of priority concerns and in developing scenarios for management. It will include an assessment of key research and observing needs as one way to deal with the scientific uncertainty inherent in such an exercise, and to better link policy and science agendas.

  4. Patterns of Genetic Diversity and Co-Existence in Open Ocean Diatoms: the Effects of Water Mass Structure, Selection and Sex

    NASA Astrophysics Data System (ADS)

    Rynearson, T. A.; Chen, G.

    2016-02-01

    The open ocean North Atlantic spring bloom influences regional ecology and global biogeochemistry. Diatoms dominate the peak of the bloom and significantly impact productivity and export of organic carbon from the bloom. Despite their key role in a yearly event with global impacts, the genetic diversity and population structure of diatoms that comprise this open ocean bloom are unknown. Here we investigated the population genetics of the diatom Thalassiosira gravida sampled during the 2008 North Atlantic Bloom Experiment using newly-developed microsatellite markers. Here, we show that the genetic diversity of open ocean diatoms is high and that their population structure differs dramatically from coastal diatoms. High levels of genetic diversity were observed across all water samples and did not change during the bloom. Four genetically distinct populations were identified but were not associated with different water masses, depths or time points during the bloom. Instead, all four populations co-existed within samples, spanning different water masses, stages of the bloom and depths of over >300 m. The pattern of genetically distinct, co-existing populations in the open ocean contrasts dramatically with coastal habitats, where distinct populations have not been observed to co-exist at the same time and place. It is likely that populations originate via transport from disparate locations combined with overwintering capacity in the water column or sediments. The pattern of co-existence suggests that the open ocean may serve as a gene pool that harbors different populations that are then available for selection to act upon, which may contribute to the ecological and biogeochemical success of diatoms and influence their long-term evolutionary survival.

  5. Factors influencing the dissolved iron input by river water to the open ocean

    NASA Astrophysics Data System (ADS)

    Krachler, R.; Jirsa, F.; Ayromlou, S.

    The influence of natural metal chelators on the bio-available iron input to the ocean by river water was studied. Ferrous and ferric ions present as suspended colloidal particles maintaining the semblance of a dissolved load are coagulated and settled as their freshwater carrier is mixed with seawater at the continental boundary. However, we might argue that different iron-binding colloids become sequentially destabilized in meeting progressively increasing salinities. By use of a 59Fe tracer method, the partitioning of the iron load from the suspended and dissolved mobile fraction to storage in the sediments was measured with high accuracy in mixtures of natural river water with artificial sea water. The results show a characteristic sequence of sedimentation. Various colloids of different stability are removed from a water of increasing salinity, such as it is the case in the transition from a river water to the open sea. However, the iron transport capacities of the investigated river waters differed greatly. A mountainous river in the Austrian Alps would add only about 5% of its dissolved Fe load, that is about 2.0 µg L-1 Fe, to coastal waters. A small tributary draining a sphagnum peat-bog, which acts as a source of refractory low-molecular-weight fulvic acids to the river water, would add approximately 20% of its original Fe load, that is up to 480 µg L-1 Fe to the ocean's bio-available iron pool. This points to a natural mechanism of ocean iron fertilization by terrigenous fulvic-iron complexes originating from weathering processes occurring in the soils upstream.

  6. Factors influencing the dissolved iron input by river water to the open ocean

    NASA Astrophysics Data System (ADS)

    Krachler, R.; Jirsa, F.; Ayromlou, S.

    2005-05-01

    The influence of natural metal chelators on the bio-available iron input to the ocean by river water was studied. Ferrous and ferric ions present as suspended colloidal particles maintaining the semblance of a dissolved load are coagulated and settled as their freshwater carrier is mixed with seawater at the continental boundary. However, we might argue that different iron-binding colloids become sequentially destabilized in meeting progressively increasing salinities. By use of a 59Fe tracer method, the partitioning of the iron load from the suspended and dissolved mobile fraction to storage in the sediments was measured with high accuracy in mixtures of natural river water with artificial sea water. The results show a characteristic sequence of sedimentation. Various colloids of different stability are removed from a water of increasing salinity, such as it is the case in the transition from a river water to the open sea. However, the iron transport capacities of the investigated river waters differed greatly. A mountainous river in the Austrian Alps would add only about 5% of its dissolved Fe load, that is about 2.0 µg L-1 Fe, to coastal waters. A small tributary draining a sphagnum peat-bog, which acts as a source of refractory low-molecular-weight fulvic acids to the river water, would add approximately 20% of its original Fe load, that is up to 480 µg L-1 Fe to the ocean's bio-available iron pool. This points to a natural mechanism of ocean iron fertilization by terrigenous fulvic-iron complexes originating from weathering processes occurring in the soils upstream.

  7. Sensitivity of Calibration Gains to Ocean Color Processing in Coastal and Open Waters Using Ensembles Members for NPP-VIIRS

    DTIC Science & Technology

    2014-07-01

    a different impact on spectral normalized water leaving radiances and the derived ocean color products (inherent optical properties, chlorophyll ). We...leaving radiances and the derived ocean color products (inherent optical properties, chlorophyll ). We evaluated the influence of gains from open and...34gain" on ocean color products. These products include the spectral Remote Sensing Reflectance (RRS), chlorophyll concentration, and Inherent Optical

  8. Manifestation, Drivers, and Emergence of Open Ocean Deoxygenation.

    PubMed

    Levin, Lisa A

    2018-01-03

    Oxygen loss in the ocean, termed deoxygenation, is a major consequence of climate change and is exacerbated by other aspects of global change. An average global loss of 2% or more has been recorded in the open ocean over the past 50-100 years, but with greater oxygen declines in intermediate waters (100-600 m) of the North Pacific, the East Pacific, tropical waters, and the Southern Ocean. Although ocean warming contributions to oxygen declines through a reduction in oxygen solubility and stratification effects on ventilation are reasonably well understood, it has been a major challenge to identify drivers and modifying factors that explain different regional patterns, especially in the tropical oceans. Changes in respiration, circulation (including upwelling), nutrient inputs, and possibly methane release contribute to oxygen loss, often indirectly through stimulation of biological production and biological consumption. Microbes mediate many feedbacks in oxygen minimum zones that can either exacerbate or ameliorate deoxygenation via interacting nitrogen, sulfur, and carbon cycles. The paleo-record reflects drivers of and feedbacks to deoxygenation that have played out through the Phanerozoic on centennial, millennial, and hundred-million-year timescales. Natural oxygen variability has made it difficult to detect the emergence of a climate-forced signal of oxygen loss, but new modeling efforts now project emergence to occur in many areas in 15-25 years. Continued global deoxygenation is projected for the next 100 or more years under most emissions scenarios, but with regional heterogeneity. Notably, even small changes in oxygenation can have significant biological effects. New efforts to systematically observe oxygen changes throughout the open ocean are needed to help address gaps in understanding of ocean deoxygenation patterns and drivers.

  9. Manifestation, Drivers, and Emergence of Open Ocean Deoxygenation

    NASA Astrophysics Data System (ADS)

    Levin, Lisa A.

    2018-01-01

    Oxygen loss in the ocean, termed deoxygenation, is a major consequence of climate change and is exacerbated by other aspects of global change. An average global loss of 2% or more has been recorded in the open ocean over the past 50-100 years, but with greater oxygen declines in intermediate waters (100-600 m) of the North Pacific, the East Pacific, tropical waters, and the Southern Ocean. Although ocean warming contributions to oxygen declines through a reduction in oxygen solubility and stratification effects on ventilation are reasonably well understood, it has been a major challenge to identify drivers and modifying factors that explain different regional patterns, especially in the tropical oceans. Changes in respiration, circulation (including upwelling), nutrient inputs, and possibly methane release contribute to oxygen loss, often indirectly through stimulation of biological production and biological consumption. Microbes mediate many feedbacks in oxygen minimum zones that can either exacerbate or ameliorate deoxygenation via interacting nitrogen, sulfur, and carbon cycles. The paleo-record reflects drivers of and feedbacks to deoxygenation that have played out through the Phanerozoic on centennial, millennial, and hundred-million-year timescales. Natural oxygen variability has made it difficult to detect the emergence of a climate-forced signal of oxygen loss, but new modeling efforts now project emergence to occur in many areas in 15-25 years. Continued global deoxygenation is projected for the next 100 or more years under most emissions scenarios, but with regional heterogeneity. Notably, even small changes in oxygenation can have significant biological effects. New efforts to systematically observe oxygen changes throughout the open ocean are needed to help address gaps in understanding of ocean deoxygenation patterns and drivers.

  10. Open ocean dead zones in the tropical North Atlantic Ocean

    NASA Astrophysics Data System (ADS)

    Karstensen, J.; Fiedler, B.; Schütte, F.; Brandt, P.; Körtzinger, A.; Fischer, G.; Zantopp, R.; Hahn, J.; Visbeck, M.; Wallace, D.

    2015-04-01

    Here we present first observations, from instrumentation installed on moorings and a float, of unexpectedly low (<2 μmol kg-1) oxygen environments in the open waters of the tropical North Atlantic, a region where oxygen concentration does normally not fall much below 40 μmol kg-1. The low-oxygen zones are created at shallow depth, just below the mixed layer, in the euphotic zone of cyclonic eddies and anticyclonic-modewater eddies. Both types of eddies are prone to high surface productivity. Net respiration rates for the eddies are found to be 3 to 5 times higher when compared with surrounding waters. Oxygen is lowest in the centre of the eddies, in a depth range where the swirl velocity, defining the transition between eddy and surroundings, has its maximum. It is assumed that the strong velocity at the outer rim of the eddies hampers the transport of properties across the eddies boundary and as such isolates their cores. This is supported by a remarkably stable hydrographic structure of the eddies core over periods of several months. The eddies propagate westward, at about 4 to 5 km day-1, from their generation region off the West African coast into the open ocean. High productivity and accompanying respiration, paired with sluggish exchange across the eddy boundary, create the "dead zone" inside the eddies, so far only reported for coastal areas or lakes. We observe a direct impact of the open ocean dead zones on the marine ecosystem as such that the diurnal vertical migration of zooplankton is suppressed inside the eddies.

  11. Inherent optical properties and satellite retrieval of chlorophyll concentration in the lagoon and open ocean waters of New Caledonia.

    PubMed

    Dupouy, Cécile; Neveux, Jacques; Ouillon, Sylvain; Frouin, Robert; Murakami, Hiroshi; Hochard, Sébastien; Dirberg, Guillaume

    2010-01-01

    The retrieval of chlorophyll-a concentration from remote sensing reflectance (Rrs) data was tested with the NASA OC4v4 algorithm on the inner New Caledonian lagoon (Case 2) and adjacent open ocean (Case 1) waters. The input to OC4v4 was Rrs measured in situ or modeled from water's inherent optical properties (2001-2007). At open ocean stations, backscattering and absorption coefficients were correlated with chlorophyll (R(2)=0.31-0.51, respectively), in agreement with models for Case 1 waters. Taking spectrofluorometric measurement as reference, the OC4v4 model leads to an average underestimation of 33% of the chlorophyll concentration. For the lagoon waters, OC4v4 performed inadequately because the backscattering coefficient, highly correlated with turbidity and suspended matter (R(2)=0.98), was poorly correlated to chlorophyll (R(2)=0.42). The OC4v4 performance was better in deep lagoon waters for stations with a TDT index (Tchla x depth/turbidity) higher than 19 mg m(-2) NTU(-1) (R(2)=0.974, bias=10.2%). Global Imager Rrs provided a good estimate of Tchla (R(2)=0.79, N=28) in the deeper part of the lagoon. Copyright (c) 2010 Elsevier Ltd. All rights reserved.

  12. The sources of Antarctic bottom water in a global ice ocean model

    NASA Astrophysics Data System (ADS)

    Goosse, Hugues; Campin, Jean-Michel; Tartinville, Benoı̂t

    Two mechanisms contribute to the formation of Antarctic bottom water (AABW). The first, and probably the most important, is initiated by the brine released on the Antarctic continental shelf during ice formation which is responsible for an increase in salinity. After mixing with ambient water at the shelf break, this salty and dense water sinks along the shelf slope and invades the deepest part of the global ocean. For the second one, the increase of surface water density is due to strong cooling at the ocean-atmosphere interface, together with a contribution from brine release. This induces deep convection and the renewal of deep waters. The relative importance of these two mechanisms is investigated in a global coupled ice-ocean model. Chlorofluorocarbon (CFC) concentrations simulated by the model compare favourably with observations, suggesting a reasonable deep water ventilation in the Southern Ocean, except close to Antarctica where concentrations are too high. Two artificial passive tracers released at surface on the Antarctic continental shelf and in the open-ocean allow to show clearly that the two mechanisms contribute significantly to the renewal of AABW in the model. This indicates that open-ocean convection is overestimated in our simulation. Additional experiments show that the amount of AABW production due to the export of dense shelf waters is quite sensitive to the parameterisation of the effect of downsloping and meso-scale eddies. Nevertheless, shelf waters always contribute significantly to deep water renewal. Besides, increasing the P.R. Gent, J.C. McWilliams [Journal of Physical Oceanography 20 (1990) 150-155] thickness diffusion can nearly suppress the AABW formation by open-ocean convection.

  13. Plastic debris in the open ocean

    PubMed Central

    Cózar, Andrés; Echevarría, Fidel; González-Gordillo, J. Ignacio; Irigoien, Xabier; Úbeda, Bárbara; Hernández-León, Santiago; Palma, Álvaro T.; Navarro, Sandra; García-de-Lomas, Juan; Ruiz, Andrea; Fernández-de-Puelles, María L.; Duarte, Carlos M.

    2014-01-01

    There is a rising concern regarding the accumulation of floating plastic debris in the open ocean. However, the magnitude and the fate of this pollution are still open questions. Using data from the Malaspina 2010 circumnavigation, regional surveys, and previously published reports, we show a worldwide distribution of plastic on the surface of the open ocean, mostly accumulating in the convergence zones of each of the five subtropical gyres with comparable density. However, the global load of plastic on the open ocean surface was estimated to be on the order of tens of thousands of tons, far less than expected. Our observations of the size distribution of floating plastic debris point at important size-selective sinks removing millimeter-sized fragments of floating plastic on a large scale. This sink may involve a combination of fast nano-fragmentation of the microplastic into particles of microns or smaller, their transference to the ocean interior by food webs and ballasting processes, and processes yet to be discovered. Resolving the fate of the missing plastic debris is of fundamental importance to determine the nature and significance of the impacts of plastic pollution in the ocean. PMID:24982135

  14. Plastic debris in the open ocean.

    PubMed

    Cózar, Andrés; Echevarría, Fidel; González-Gordillo, J Ignacio; Irigoien, Xabier; Ubeda, Bárbara; Hernández-León, Santiago; Palma, Alvaro T; Navarro, Sandra; García-de-Lomas, Juan; Ruiz, Andrea; Fernández-de-Puelles, María L; Duarte, Carlos M

    2014-07-15

    There is a rising concern regarding the accumulation of floating plastic debris in the open ocean. However, the magnitude and the fate of this pollution are still open questions. Using data from the Malaspina 2010 circumnavigation, regional surveys, and previously published reports, we show a worldwide distribution of plastic on the surface of the open ocean, mostly accumulating in the convergence zones of each of the five subtropical gyres with comparable density. However, the global load of plastic on the open ocean surface was estimated to be on the order of tens of thousands of tons, far less than expected. Our observations of the size distribution of floating plastic debris point at important size-selective sinks removing millimeter-sized fragments of floating plastic on a large scale. This sink may involve a combination of fast nano-fragmentation of the microplastic into particles of microns or smaller, their transference to the ocean interior by food webs and ballasting processes, and processes yet to be discovered. Resolving the fate of the missing plastic debris is of fundamental importance to determine the nature and significance of the impacts of plastic pollution in the ocean.

  15. Will open ocean oxygen stress intensify under climate change?

    NASA Astrophysics Data System (ADS)

    Gnanadesikan, A.; Dunne, J. P.; John, J.

    2011-07-01

    Global warming is expected to reduce oxygen solubility and vertical exchange in the ocean, changes which would be expected to result in an increase in the volume of hypoxic waters. A simulation made with a full earth system model with dynamical atmosphere, ocean, sea ice and biogeochemical cycling shows that this holds true if the condition for hypoxia is set relatively high. However, the volume of the most hypoxic waters does not increase under global warming, as these waters actually become more oxygenated. We show that the rise in oxygen is associated with a drop in ventilation time. A term-by-term analysis within the least oxygenated waters shows an increased supply of oxygen due to lateral diffusion. compensating an increase in remineralization within these highly hypoxic waters. This lateral diffusive flux is the result of an increase of ventilation along the Chilean coast, as a drying of the region under global warming opens up a region of wintertime convection in our model.

  16. Southern Ocean bottom water characteristics in CMIP5 models

    NASA Astrophysics Data System (ADS)

    Heuzé, CéLine; Heywood, Karen J.; Stevens, David P.; Ridley, Jeff K.

    2013-04-01

    Southern Ocean deep water properties and formation processes in climate models are indicative of their capability to simulate future climate, heat and carbon uptake, and sea level rise. Southern Ocean temperature and density averaged over 1986-2005 from 15 CMIP5 (Coupled Model Intercomparison Project Phase 5) climate models are compared with an observed climatology, focusing on bottom water. Bottom properties are reasonably accurate for half the models. Ten models create dense water on the Antarctic shelf, but it mixes with lighter water and is not exported as bottom water as in reality. Instead, most models create deep water by open ocean deep convection, a process occurring rarely in reality. Models with extensive deep convection are those with strong seasonality in sea ice. Optimum bottom properties occur in models with deep convection in the Weddell and Ross Gyres. Bottom Water formation processes are poorly represented in ocean models and are a key challenge for improving climate predictions.

  17. Large mesopelagic fishes biomass and trophic efficiency in the open ocean.

    PubMed

    Irigoien, Xabier; Klevjer, T A; Røstad, A; Martinez, U; Boyra, G; Acuña, J L; Bode, A; Echevarria, F; Gonzalez-Gordillo, J I; Hernandez-Leon, S; Agusti, S; Aksnes, D L; Duarte, C M; Kaartvedt, S

    2014-01-01

    With a current estimate of ~1,000 million tons, mesopelagic fishes likely dominate the world total fishes biomass. However, recent acoustic observations show that mesopelagic fishes biomass could be significantly larger than the current estimate. Here we combine modelling and a sensitivity analysis of the acoustic observations from the Malaspina 2010 Circumnavigation Expedition to show that the previous estimate needs to be revised to at least one order of magnitude higher. We show that there is a close relationship between the open ocean fishes biomass and primary production, and that the energy transfer efficiency from phytoplankton to mesopelagic fishes in the open ocean is higher than what is typically assumed. Our results indicate that the role of mesopelagic fishes in oceanic ecosystems and global ocean biogeochemical cycles needs to be revised as they may be respiring ~10% of the primary production in deep waters.

  18. Large mesopelagic fishes biomass and trophic efficiency in the open ocean

    PubMed Central

    Irigoien, Xabier; Klevjer, T. A.; Røstad, A.; Martinez, U.; Boyra, G.; Acuña, J. L.; Bode, A.; Echevarria, F.; Gonzalez-Gordillo, J. I.; Hernandez-Leon, S.; Agusti, S.; Aksnes, D. L.; Duarte, C. M.; Kaartvedt, S.

    2014-01-01

    With a current estimate of ~1,000 million tons, mesopelagic fishes likely dominate the world total fishes biomass. However, recent acoustic observations show that mesopelagic fishes biomass could be significantly larger than the current estimate. Here we combine modelling and a sensitivity analysis of the acoustic observations from the Malaspina 2010 Circumnavigation Expedition to show that the previous estimate needs to be revised to at least one order of magnitude higher. We show that there is a close relationship between the open ocean fishes biomass and primary production, and that the energy transfer efficiency from phytoplankton to mesopelagic fishes in the open ocean is higher than what is typically assumed. Our results indicate that the role of mesopelagic fishes in oceanic ecosystems and global ocean biogeochemical cycles needs to be revised as they may be respiring ~10% of the primary production in deep waters. PMID:24509953

  19. Mapping the future expansion of Arctic open water

    NASA Astrophysics Data System (ADS)

    Barnhart, Katherine R.; Miller, Christopher R.; Overeem, Irina; Kay, Jennifer E.

    2016-03-01

    Sea ice impacts most of the Arctic environment, from ocean circulation and marine ecosystems to animal migration and marine transportation. Sea ice has thinned and decreased in age over the observational record. Ice extent has decreased. Reduced ice cover has warmed the surface ocean, accelerated coastal erosion and impacted biological productivity. Declines in Arctic sea-ice extent cannot be explained by internal climate variability alone and can be attributed to anthropogenic effects. However, extent is a poor measure of ice decline at specific locations as it integrates over the entire Arctic basin and thus contains no spatial information. The open water season, in contrast, is a metric that represents the duration of open water over a year at an individual location. Here we present maps of the open water season over the period 1920-2100 using daily output from a 30-member initial-condition ensemble of business-as-usual climate simulations that characterize the expansion of Arctic open water, determine when the open water season will move away from pre-industrial conditions (`shift’ time) and identify when human forcing will take the Arctic sea-ice system outside its normal bounds (`emergence’ time). The majority of the Arctic nearshore regions began shifting in 1990 and will begin leaving the range of internal variability in 2040. Models suggest that ice will cover coastal regions for only half of the year by 2070.

  20. Open-Ocean and Coastal Properties of Recent Major Tsunamis

    NASA Astrophysics Data System (ADS)

    Rabinovich, A.; Thomson, R.; Zaytsev, O.

    2017-12-01

    The properties of six major tsunamis during the period 2009-2015 (2009 Samoa; 2010 Chile; 2011 Tohoku; 2012 Haida Gwaii; 2014 and 2015 Chile) were thoroughly examined using coastal data from British Columbia, the U.S. West Coast and Mexico, and offshore open-ocean DART and NEPTUNE stations. Based on joint spectral analyses of the tsunamis and background noise, we have developed a method to suppress the influence of local topography and to use coastal observations to determine the underlying spectra of tsunami waves in the deep ocean. The "reconstructed" open-ocean tsunami spectra were found to be in close agreement with the actual tsunami spectra evaluated from the analysis of directly measured open-ocean tsunami records. We have further used the spectral estimates to parameterize tsunamis based on their integral open-ocean spectral characteristics. Three key parameters are introduced to describe individual tsunami events: (1) Integral open-ocean energy; (2) Amplification factor (increase of the mean coastal tsunami variance relative to the open-ocean variance); and (3) Tsunami colour, the frequency composition of the open-ocean tsunami waves. In particular, we found that the strongest tsunamis, associated with large source areas (the 2010 Chile and 2011 Tohoku) are "reddish" (indicating the dominance of low-frequency motions), while small-source events (the 2009 Samoa and 2012 Haida Gwaii) are "bluish" (indicating strong prevalence of high-frequency motions).

  1. Optimizing Ocean Space: Co-siting Open Ocean Aquaculture

    NASA Astrophysics Data System (ADS)

    Cobb, B. L.; Wickliffe, L. C.; Morris, J. A., Jr.

    2016-12-01

    In January of 2016, NOAA's National Marine Fisheries Service released the Gulf Aquaculture Plan (GAP) to manage the development of environmentally sound and economically sustainable open ocean finfish aquaculture in the Gulf of Mexico (inside the U.S. Exclusive Economic Zone [EEZ]). The GAP provides the first regulatory framework for aquaculture in federal waters with estimated production of 64 million pounds of finfish, and an estimated economic impact of $264 million annually. The Gulf of Mexico is one of the most industrialized ocean basins in the world, with many existing ocean uses including oil and natural gas production, shipping and commerce, commercial fishing operations, and many protected areas to ensure conservation of valuable ecosystem resources and services. NOAA utilized spatial planning procedures and tools identifying suitable sites for establishing aquaculture through exclusion analyses using authoritative federal and state data housed in a centralized geodatabase. Through a highly collaborative, multi-agency effort a mock permitting exercise was conducted to illustrate the regulatory decision-making process for the Gulf. Further decision-making occurred through exploring co-siting opportunities with oil and natural gas platforms. Logistical co-siting was conducted to reduce overall operational costs by looking at distance to major port and commodity tonnage at each port. Importantly, the process of co-siting allows aquaculture to be coupled with other benefits, including the availability of previously established infrastructure and the reduction of environmental impacts.

  2. Open cycle ocean thermal energy conversion system

    DOEpatents

    Wittig, J. Michael

    1980-01-01

    An improved open cycle ocean thermal energy conversion system including a flash evaporator for vaporizing relatively warm ocean surface water and an axial flow, elastic fluid turbine having a vertical shaft and axis of rotation. The warm ocean water is transmitted to the evaporator through a first prestressed concrete skirt-conduit structure circumferentially situated about the axis of rotation. The unflashed warm ocean water exits the evaporator through a second prestressed concrete skirt-conduit structure located circumferentially about and radially within the first skirt-conduit structure. The radially inner surface of the second skirt conduit structure constitutes a cylinder which functions as the turbine's outer casing and obviates the need for a conventional outer housing. The turbine includes a radially enlarged disc element attached to the shaft for supporting at least one axial row of radially directed blades through which the steam is expanded. A prestressed concrete inner casing structure of the turbine has upstream and downstream portions respectively situated upstream and downstream from the disc element. The radially outer surfaces of the inner casing portions and radially outer periphery of the axially interposed disc cooperatively form a downwardly radially inwardly tapered surface. An annular steam flowpath of increasing flow area in the downward axial direction is radially bounded by the inner and outer prestressed concrete casing structures. The inner casing portions each include a transversely situated prestressed concrete circular wall for rotatably supporting the turbine shaft and associated structure. The turbine blades are substantially radially coextensive with the steam flowpath and receive steam from the evaporator through an annular array of prestressed concrete stationary vanes which extend between the inner and outer casings to provide structural support therefor and impart a desired flow direction to the steam.

  3. A review of ocean color remote sensing methods and statistical techniques for the detection, mapping and analysis of phytoplankton blooms in coastal and open oceans

    NASA Astrophysics Data System (ADS)

    Blondeau-Patissier, David; Gower, James F. R.; Dekker, Arnold G.; Phinn, Stuart R.; Brando, Vittorio E.

    2014-04-01

    The need for more effective environmental monitoring of the open and coastal ocean has recently led to notable advances in satellite ocean color technology and algorithm research. Satellite ocean color sensors' data are widely used for the detection, mapping and monitoring of phytoplankton blooms because earth observation provides a synoptic view of the ocean, both spatially and temporally. Algal blooms are indicators of marine ecosystem health; thus, their monitoring is a key component of effective management of coastal and oceanic resources. Since the late 1970s, a wide variety of operational ocean color satellite sensors and algorithms have been developed. The comprehensive review presented in this article captures the details of the progress and discusses the advantages and limitations of the algorithms used with the multi-spectral ocean color sensors CZCS, SeaWiFS, MODIS and MERIS. Present challenges include overcoming the severe limitation of these algorithms in coastal waters and refining detection limits in various oceanic and coastal environments. To understand the spatio-temporal patterns of algal blooms and their triggering factors, it is essential to consider the possible effects of environmental parameters, such as water temperature, turbidity, solar radiation and bathymetry. Hence, this review will also discuss the use of statistical techniques and additional datasets derived from ecosystem models or other satellite sensors to characterize further the factors triggering or limiting the development of algal blooms in coastal and open ocean waters.

  4. Carbon Sequestration through Sustainably Sourced Algal Fertilizer: Deep Ocean Water.

    NASA Astrophysics Data System (ADS)

    Sherman, M. T.

    2014-12-01

    Drawing down carbon from the atmosphere happens in the oceans when marine plants are growing due to the use of carbon dioxide for biological processes and by raising the pH of the water. Macro- and microscopic marine photosynthesizers are limited in their growth by the availability of light and nutrients (nitrogen, phosphorous, iron, etc.) Deep ocean water (DOW), oceanic water from bellow about 1000m, is a natural medium for marine algae, which contains all (except in rare circumstances) necessary components for algal growth and represents over 90% of the volume of the ocean. The introduction of DOW to a tropical or summer sea can increase chlorophyll from near zero to 60 mg per M3 or more. The form of the utilization infrastructure for DOW can roughly be divided into two effective types; the unconstrained release and the open pond system. Unconstrained release has the advantage of having relatively low infrastructure investment and is available to any area of the ocean. The open pond system has high infrastructure costs but enables intensive use of DOW for harvesting macro- and microalgae and sustainable mariculture. It also enables greater concomitant production of DOW's other potential products such as electricity or potable water. However, unlike an unconstrained release the open pond system can capture much of the biomaterial from the water and limits the impact to the surrounding ecosystem. The Tidal Irrigation and Electrical System (TIESystem), is an open pond that is to be constructed on a continental shelf. It harnesses the tidal flux to pump DOW into the pond on the rising tide and then uses the falling tide to pump biologically rich material out of the pond. This biomaterial represents fixed CO2 and can be used for biofuel or fertilizers. The TIESystem benefits from an economy of scale that increases at a rate that is roughly equal to the relationship of the circumference of a circle (the barrier that creates the open pond) to the area of the pond

  5. Southern Ocean Bottom Water Characteristics in CMIP5 Models

    NASA Astrophysics Data System (ADS)

    Heuzé, Céline; Heywood, Karen; Stevens, David; Ridley, Jeff

    2013-04-01

    The depiction of Southern Ocean deep water properties and formation processes in climate models is an indicator of their capability to simulate future climate, heat and carbon uptake, and sea level rise. Southern Ocean potential temperature and density averaged over 1986-2005 from fifteen CMIP5 climate models are compared with an observed climatology, focusing on bottom water properties. The mean bottom properties are reasonably accurate for half of the models, but the other half may not yet have approached an equilibrium state. Eleven models create dense water on the Antarctic shelf, but it does not spill off and propagate northwards, alternatively mixing rapidly with less dense water. Instead most models create deep water by open ocean deep convection. Models with large deep convection areas are those with a strong seasonal cycle in sea ice. The most accurate bottom properties occur in models hosting deep convection in the Weddell and Ross gyres.

  6. The Growing Human Footprint on Coastal and Open-Ocean Biogeochemistry

    NASA Astrophysics Data System (ADS)

    Doney, Scott C.

    2010-06-01

    Climate change, rising atmospheric carbon dioxide, excess nutrient inputs, and pollution in its many forms are fundamentally altering the chemistry of the ocean, often on a global scale and, in some cases, at rates greatly exceeding those in the historical and recent geological record. Major observed trends include a shift in the acid-base chemistry of seawater, reduced subsurface oxygen both in near-shore coastal water and in the open ocean, rising coastal nitrogen levels, and widespread increase in mercury and persistent organic pollutants. Most of these perturbations, tied either directly or indirectly to human fossil fuel combustion, fertilizer use, and industrial activity, are projected to grow in coming decades, resulting in increasing negative impacts on ocean biota and marine resources.

  7. The growing human footprint on coastal and open-ocean biogeochemistry.

    PubMed

    Doney, Scott C

    2010-06-18

    Climate change, rising atmospheric carbon dioxide, excess nutrient inputs, and pollution in its many forms are fundamentally altering the chemistry of the ocean, often on a global scale and, in some cases, at rates greatly exceeding those in the historical and recent geological record. Major observed trends include a shift in the acid-base chemistry of seawater, reduced subsurface oxygen both in near-shore coastal water and in the open ocean, rising coastal nitrogen levels, and widespread increase in mercury and persistent organic pollutants. Most of these perturbations, tied either directly or indirectly to human fossil fuel combustion, fertilizer use, and industrial activity, are projected to grow in coming decades, resulting in increasing negative impacts on ocean biota and marine resources.

  8. How much riverine nutrients do shelf seas allow into the open ocean?

    NASA Astrophysics Data System (ADS)

    Sharples, J.; Fennel, K.; Jickells, T. D.

    2016-02-01

    Globally rivers deliver 35 Tg of dissolved N and 2 Tg of dissolved P into the coastal zone each year. Investigating the effects of this nutrient supply on the open ocean generally takes one of two approaches: either all or none of the nutrients are assumed to enter the open ocean. Here we use some general assumptions on the behaviour of river plumes on the shelf to arrive at an estimate of the proportions of dissolved N and P that are processed on the shelf, and thus the amount of riverine nutrient that enters the open ocean. Using the Global NEWS database of 6000 rivers we assume that discharges to the shelf are initially constrained within coastal buoyancy currents of width 2 internal Rossby radii. This width is compared to the local shelf width for each river. For plume widths greater than the shelf width riverine nutrients are assumed to be transported over the shelf edge within the plume. For plume widths less than the shelf width we assume that exchange with the open ocean is controlled by physical processes at the shelf break. For each river an estimate of the residence time of riverine water is made, based on the transport or exchange rate and the shelf volume. Empirical relationships between residence time and the proportion of supplied N and P that is retained on the shelf are then used to estimate the amount of dissolved N and P that escapes to the open ocean. The results suggest that 25% of dissolved N and 20% of dissolved P are processed in shelf seas, with the rest exported to the open ocean. There is a latitudinal pattern, with tropical rivers delivering more nutrients to the open ocean. This is partially a result of the high discharges of some tropical rivers, but a key issue is our assumption of the internal Rossby radius governing plume width. A range of values for transport rates within plumes and exchange rates across the shelf break are used to assess the sensitivity of these results, which appear to be robust.

  9. Undocumented water column sink for cadmium in open ocean oxygen-deficient zones

    PubMed Central

    Janssen, David J.; Conway, Tim M.; John, Seth G.; Christian, James R.; Kramer, Dennis I.; Pedersen, Tom F.; Cullen, Jay T.

    2014-01-01

    Cadmium (Cd) is a micronutrient and a tracer of biological productivity and circulation in the ocean. The correlation between dissolved Cd and the major algal nutrients in seawater has led to the use of Cd preserved in microfossils to constrain past ocean nutrient distributions. However, linking Cd to marine biological processes requires constraints on marine sources and sinks of Cd. Here, we show a decoupling between Cd and major nutrients within oxygen-deficient zones (ODZs) in both the Northeast Pacific and North Atlantic Oceans, which we attribute to Cd sulfide (CdS) precipitation in euxinic microenvironments around sinking biological particles. We find that dissolved Cd correlates well with dissolved phosphate in oxygenated waters, but is depleted compared with phosphate in ODZs. Additionally, suspended particles from the North Atlantic show high Cd content and light Cd stable isotope ratios within the ODZ, indicative of CdS precipitation. Globally, we calculate that CdS precipitation in ODZs is an important, and to our knowledge a previously undocumented marine sink of Cd. Our results suggest that water column oxygen depletion has a substantial impact on Cd biogeochemical cycling, impacting the global relationship between Cd and major nutrients and suggesting that Cd may be a previously unidentified tracer for water column oxygen deficiency on geological timescales. Similar depletions of copper and zinc in the Northeast Pacific indicate that sulfide precipitation in ODZs may also have an influence on the global distribution of other trace metals. PMID:24778239

  10. Undocumented water column sink for cadmium in open ocean oxygen-deficient zones.

    PubMed

    Janssen, David J; Conway, Tim M; John, Seth G; Christian, James R; Kramer, Dennis I; Pedersen, Tom F; Cullen, Jay T

    2014-05-13

    Cadmium (Cd) is a micronutrient and a tracer of biological productivity and circulation in the ocean. The correlation between dissolved Cd and the major algal nutrients in seawater has led to the use of Cd preserved in microfossils to constrain past ocean nutrient distributions. However, linking Cd to marine biological processes requires constraints on marine sources and sinks of Cd. Here, we show a decoupling between Cd and major nutrients within oxygen-deficient zones (ODZs) in both the Northeast Pacific and North Atlantic Oceans, which we attribute to Cd sulfide (CdS) precipitation in euxinic microenvironments around sinking biological particles. We find that dissolved Cd correlates well with dissolved phosphate in oxygenated waters, but is depleted compared with phosphate in ODZs. Additionally, suspended particles from the North Atlantic show high Cd content and light Cd stable isotope ratios within the ODZ, indicative of CdS precipitation. Globally, we calculate that CdS precipitation in ODZs is an important, and to our knowledge a previously undocumented marine sink of Cd. Our results suggest that water column oxygen depletion has a substantial impact on Cd biogeochemical cycling, impacting the global relationship between Cd and major nutrients and suggesting that Cd may be a previously unidentified tracer for water column oxygen deficiency on geological timescales. Similar depletions of copper and zinc in the Northeast Pacific indicate that sulfide precipitation in ODZs may also have an influence on the global distribution of other trace metals.

  11. Photochemical degradation of Corexit components in ocean water.

    PubMed

    Glover, Caitlin M; Mezyk, Stephen P; Linden, Karl G; Rosario-Ortiz, Fernando L

    2014-09-01

    Due to the large quantities of dispersants used during the Deepwater Horizon spill in 2010, there were immediate concerns with regards to the fate and transport of the mixture in ocean waters. Direct and sensitized photolysis experiments were carried out for two compounds chosen as surrogates for the Corexit mixture (9500 and 9527) that were applied to surface waters during the oil spill in the Gulf of Mexico. The results showed that direct photolysis did not contribute significantly to the overall degradation (max ∼30%), therefore the focus shifted to sensitized photolysis, specifically the degradation stemming from the reaction rate with hydroxyl radical (HO). The direct photochemical degradation rates for two of the compounds, dioctyl sulfosuccinate (DOSS) and dipropylene glycol butyl ether (DGBE) were measured as 4.29×10(-6)s(-1) and 5.95×10(-6)s(-1), respectively; whereas the overall degradation rate in ocean water was 1.56×10(-5)s(-1) and 2.23×10(-5)s(-1). The formation rates and apparent quantum yields for HO formation were determined for six ocean water samples. The values ranged from 1.81×10(-5) near shore to 0.061×10(-5) for the open ocean. These degradation rates suggest the possibility for photolysis to play a role in the overall fate of Corexit. Copyright © 2014 Elsevier Ltd. All rights reserved.

  12. An original mode of symbiosis in open ocean plankton.

    PubMed

    Decelle, Johan; Probert, Ian; Bittner, Lucie; Desdevises, Yves; Colin, Sébastien; de Vargas, Colomban; Galí, Martí; Simó, Rafel; Not, Fabrice

    2012-10-30

    Symbiotic relationships are widespread in nature and are fundamental for ecosystem functioning and the evolution of biodiversity. In marine environments, photosymbiosis with microalgae is best known for sustaining benthic coral reef ecosystems. Despite the importance of oceanic microbiota in global ecology and biogeochemical cycles, symbioses are poorly characterized in open ocean plankton. Here, we describe a widespread symbiotic association between Acantharia biomineralizing microorganisms that are abundant grazers in plankton communities, and members of the haptophyte genus Phaeocystis that are cosmopolitan bloom-forming microalgae. Cophylogenetic analyses demonstrate that symbiont biogeography, rather than host taxonomy, is the main determinant of the association. Molecular dating places the origin of this photosymbiosis in the Jurassic (ca. 175 Mya), a period of accentuated marine oligotrophy. Measurements of intracellular dimethylated sulfur indicate that the host likely profits from antioxidant protection provided by the symbionts as an adaptation to life in transparent oligotrophic surface waters. In contrast to terrestrial and marine symbioses characterized to date, the symbiont reported in this association is extremely abundant and ecologically active in its free-living phase. In the vast and barren open ocean, partnership with photosymbionts that have extensive free-living populations is likely an advantageous strategy for hosts that rely on such interactions. Discovery of the Acantharia-Phaeocystis association contrasts with the widely held view that symbionts are specialized organisms that are rare and ecologically passive outside the host.

  13. Hidden biosphere in an oxygen-deficient Atlantic open ocean eddy: future implications of ocean deoxygenation on primary production in the eastern tropical North Atlantic

    NASA Astrophysics Data System (ADS)

    Loescher, Carolin; Fischer, Martin; Neulinger, Sven; Fiedler, Björn; Philippi, Miriam; Schütte, Florian; Singh, Arvind; Hauss, Helena; Karstensen, Johannes; Körtzinger, Arne; Schmitz, Ruth

    2016-04-01

    The eastern tropical North Atlantic (ETNA) is characterized by a highly productive coastal upwelling system and a moderate oxygen minimum zone with lowest open ocean oxygen (O2) concentrations of approximately 40 μmol kg-1. The recent discovery of re-occurring mesoscale eddies with close to anoxic O2 concentrations (<1 μmol kg-1) located just below the mixed layer has challenged our understanding of O2 distribution and biogeochemical processes in this area. Here, we present the first microbial community study from a deoxygenated anticyclonic modewater eddy in the open waters of the ETNA. In the eddy, we observed significantly lower bacterial diversity compared to surrounding waters, along with a significant community shift. We detected enhanced primary productivity in the surface layer of the eddy indicated by elevated chlorophyll concentrations and carbon uptake rates of up to three times as high as in surrounding waters. Carbon uptake rates below the euphotic zone correlated to the presence of a specific high-light ecotype of Prochlorococcus, which is usually underrepresented in the ETNA. Our data indicate that high primary production in the eddy fuels export production and supports enhanced respiration in a specific microbial community at shallow depths, below the mixed layer base. The O2-depleted core waters eddy promoted transcription of the key gene for denitrification, nirS. This process is usually absent from the open ETNA waters. In light of future projected ocean deoxygenation, our results show that even distinct events of anoxia have the potential to alter microbial community structure with critical impacts on primary productivity and biogeochemical processes of oceanic water bodies.

  14. Hidden biosphere in an oxygen-deficient Atlantic open-ocean eddy: future implications of ocean deoxygenation on primary production in the eastern tropical North Atlantic

    NASA Astrophysics Data System (ADS)

    Löscher, C. R.; Fischer, M. A.; Neulinger, S. C.; Fiedler, B.; Philippi, M.; Schütte, F.; Singh, A.; Hauss, H.; Karstensen, J.; Körtzinger, A.; Künzel, S.; Schmitz, R. A.

    2015-12-01

    The eastern tropical North Atlantic (ETNA) is characterized by a highly productive coastal upwelling system and a moderate oxygen minimum zone with lowest open-ocean oxygen (O2) concentrations of approximately 40 μmol kg-1. The recent discovery of re-occurring mesoscale eddies with close to anoxic O2 concentrations (< 1 μmol kg-1) located just below the mixed layer has challenged our understanding of O2 distribution and biogeochemical processes in this area. Here, we present the first microbial community study from a deoxygenated anticyclonic modewater eddy in the open waters of the ETNA. In the eddy, we observed significantly lower bacterial diversity compared to surrounding waters, along with a significant community shift. We detected enhanced primary productivity in the surface layer of the eddy indicated by elevated chlorophyll concentrations and carbon uptake rates of up to three times as high as in surrounding waters. Carbon uptake rates below the euphotic zone correlated to the presence of a specific high-light ecotype of Prochlorococcus, which is usually underrepresented in the ETNA. Our data indicate that high primary production in the eddy fuels export production and supports enhanced respiration in a specific microbial community at shallow depths, below the mixed-layer base. The transcription of the key functional marker gene for dentrification, nirS, further indicated a potential for nitrogen loss processes in O2-depleted core waters of the eddy. Dentrification is usually absent from the open ETNA waters. In light of future projected ocean deoxygenation, our results show that even distinct events of anoxia have the potential to alter microbial community structure with critical impacts on primary productivity and biogeochemical processes of oceanic water bodies.

  15. Atlantic ocean surface waters buffer declining atmospheric concentrations of persistent organic pollutants.

    PubMed

    Nizzetto, Luca; Lohmann, Rainer; Gioia, Rosalinda; Dachs, Jordi; Jones, Kevin C

    2010-09-15

    Decreasing environmental concentrations of some persistent organic pollutants (POPs) have been observed at local or regional scales in continental areas after the implementation of international measures to curb primary emissions. A decline in primary atmospheric emissions can result in re-emissions of pollutants from the environmental capacitors (or secondary sources) such as soils and oceans. This may be part of the reason why concentrations of some POPs such as polychlorinated biphenyls (PCBs) have not declined significantly in the open oceanic areas, although re-emission of POPs from open ocean water has barely been documented. In contrast, results from this study show that several polychlorinated dibenzo-p-dioxins and furans (PCDD/Fs) have undergone a marked decline (2-3 orders of magnitude for some homologues) over a major portion of the remote oligotrophic Atlantic Ocean. The decline appears to be faster than that observed over continental areas, implicating an important role of oceanic geochemical controls on levels and cycling of some POPs. For several lower chlorinated PCDD/Fs, we observed re-emission from surface water back to the atmosphere. An assessment of the effectiveness of the main sink processes highlights the role of degradation in surface waters as potentially key to explaining the different behavior between PCDD/Fs and PCBs and controlling their overall residence time in the ocean/atmosphere system. This study provides experimental evidence that the ocean has a buffering capacity - dependent on individual chemicals - which moderates the rate at which the system will respond to an underlying change in continental emissions.

  16. Sensitivity of Multiangle, Multispectral Polarimetric Remote Sensing Over Open Oceans to Water-Leaving Radiance: Analyses of RSP Data Acquired During the MILAGRO Campaign

    NASA Technical Reports Server (NTRS)

    Chowdhary, Jacek; Cairns, Brian; Waquet, Fabien; Knobelspiesse, Kirk; Ottaviani, Matteo; Redemann, Jens; Travis, Larry; Mishchenko, Michael

    2012-01-01

    For remote sensing of aerosol over the ocean, there is a contribution from light scattered underwater. The brightness and spectrum of this light depends on the biomass content of the ocean, such that variations in the color of the ocean can be observed even from space. Rayleigh scattering by pure sea water, and Rayleigh-Gans type scattering by plankton, causes this light to be polarized with a distinctive angular distribution. To study the contribution of this underwater light polarization to multiangle, multispectral observations of polarized reflectance over ocean, we previously developed a hydrosol model for use in underwater light scattering computations that produces realistic variations of the ocean color and the underwater light polarization signature of pure sea water. In this work we review this hydrosol model, include a correction for the spectrum of the particulate scattering coefficient and backscattering efficiency, and discuss its sensitivity to variations in colored dissolved organic matter (CDOM) and in the scattering function of marine particulates. We then apply this model to measurements of total and polarized reflectance that were acquired over open ocean during the MILAGRO field campaign by the airborne Research Scanning Polarimeter (RSP). Analyses show that our hydrosol model faithfully reproduces the water-leaving contributions to RSP reflectance, and that the sensitivity of these contributions to Chlorophyll a concentration [Chl] in the ocean varies with the azimuth, height, and wavelength of observations. We also show that the impact of variations in CDOM on the polarized reflectance observed by the RSP at low altitude is comparable to or much less than the standard error of this reflectance whereas their effects in total reflectance may be substantial (i.e. up to >30%). Finally, we extend our study of polarized reflectance variations with [Chl] and CDOM to include results for simulated spaceborne observations.

  17. Hidden biosphere in an oxygen-deficient Atlantic open ocean eddy: future implications of ocean deoxygenation on primary production in the eastern tropical North Atlantic

    NASA Astrophysics Data System (ADS)

    Löscher, C. R.; Fischer, M. A.; Neulinger, S. C.; Fiedler, B.; Philippi, M.; Schütte, F.; Singh, A.; Hauss, H.; Karstensen, J.; Körtzinger, A.; Künzel, S.; Schmitz, R. A.

    2015-08-01

    The eastern tropical North Atlantic (ETNA) is characterized by a highly productive coastal upwelling system and a moderate oxygen minimum zone with lowest open ocean oxygen (O2) concentrations of around 40 μmol kg-1. Only recently, the discovery of re-occurring mesoscale eddies with sometimes close to anoxic O2 concentrations (<1 μmol kg-1) and located just below the mixed layer challenged our understanding of O2 distribution and biogeochemical processes in this area. Here, we present the first metagenomic dataset from a deoxygenated anticyclonic modewater eddy in the open waters of the ETNA. In the eddy, we observed a significantly lower bacterial diversity compared to surrounding waters, along with a significant community shift. We detected enhanced primary productivity in the surface layer of the eddy indicated by elevated chlorophyll concentrations and increased carbon uptake rates up to three times as high as in surrounding waters. Carbon uptake below the euphotic zone correlated to the presence of a specific high-light ecotype of Prochlorococcus, which is usually underrepresented in the ETNA. Our combined data indicate that high primary production in the eddy fuels export production and the presence of a specific microbial community responsible for enhanced respiration at shallow depths, below the mixed layer base. Progressively decreasing O2 concentrations in the eddy were found to promote transcription of the key gene for denitrification, nirS, in the O2-depleted core waters. This process is usually absent from the open ETNA waters. In the light of future ocean deoxygenation our results show exemplarily that even distinct events of anoxia have the potential to alter microbial community structures and with that critically impact primary productivity and biogeochemical processes of oceanic water bodies.

  18. Declining oxygen in the global ocean and coastal waters.

    PubMed

    Breitburg, Denise; Levin, Lisa A; Oschlies, Andreas; Grégoire, Marilaure; Chavez, Francisco P; Conley, Daniel J; Garçon, Véronique; Gilbert, Denis; Gutiérrez, Dimitri; Isensee, Kirsten; Jacinto, Gil S; Limburg, Karin E; Montes, Ivonne; Naqvi, S W A; Pitcher, Grant C; Rabalais, Nancy N; Roman, Michael R; Rose, Kenneth A; Seibel, Brad A; Telszewski, Maciej; Yasuhara, Moriaki; Zhang, Jing

    2018-01-05

    Oxygen is fundamental to life. Not only is it essential for the survival of individual animals, but it regulates global cycles of major nutrients and carbon. The oxygen content of the open ocean and coastal waters has been declining for at least the past half-century, largely because of human activities that have increased global temperatures and nutrients discharged to coastal waters. These changes have accelerated consumption of oxygen by microbial respiration, reduced solubility of oxygen in water, and reduced the rate of oxygen resupply from the atmosphere to the ocean interior, with a wide range of biological and ecological consequences. Further research is needed to understand and predict long-term, global- and regional-scale oxygen changes and their effects on marine and estuarine fisheries and ecosystems. Copyright © 2018, American Association for the Advancement of Science.

  19. Factors controlling the photochemical degradation of methylmercury in coastal and oceanic waters

    PubMed Central

    DiMento, Brian P.; Mason, Robert P.

    2018-01-01

    Many studies have recognized abiotic photochemical degradation as an important sink of methylmercury (CH3Hg) in sunlit surface waters, but the rate-controlling factors remain poorly understood. The overall objective of this study was to improve our understanding of the relative importance of photochemical reactions in the degradation of CH3Hg in surface waters across a variety of marine ecosystems by extending the range of water types studied. Experiments were conducted using surface water collected from coastal sites in Delaware, New Jersey, Connecticut, and Maine, as well as offshore sites on the New England continental shelf break, the equatorial Pacific, and the Arctic Ocean. Filtered water amended with additional CH3Hg at environmentally relevant concentrations was allowed to equilibrate with natural ligands before being exposed to natural sunlight. Water quality parameters – salinity, dissolved organic carbon, and nitrate – were measured, and specific UV absorbance was calculated as a proxy for dissolved aromatic carbon content. Degradation rate constants (0.87–1.67 day−1) varied by a factor of two across all water types tested despite varying characteristics, and did not correlate with initial CH3Hg concentrations or other environmental parameters. The rate constants in terms of cumulative photon flux values were comparable to, but at the high end of, the range of values reported in other studies. Further experiments investigating the controlling parameters of the reaction observed little effect of nitrate and chloride, and potential for bromide involvement. The HydroLight radiative transfer model was used to compute solar irradiance with depth in three representative water bodies – coastal wetland, estuary, and open ocean – allowing for the determination of water column integrated rates. Methylmercury loss per year due to photodegradation was also modeled across a range of latitudes from the Arctic to the Equator in the three model water types

  20. Oceanic dispersion of Fukushima-derived Cs-137 in the coastal, offshore, and open oceans simulated by multiple oceanic general circulation models

    NASA Astrophysics Data System (ADS)

    Kawamura, H.; Furuno, A.; Kobayashi, T.; In, T.; Nakayama, T.; Ishikawa, Y.; Miyazawa, Y.; Usui, N.

    2017-12-01

    To understand the concentration and amount of Fukushima-derived Cs-137 in the ocean, this study simulates the oceanic dispersion of Cs-137 by an oceanic dispersion model SEA-GEARN-FDM developed at Japan Atomic Energy Agency (JAEA) and multiple oceanic general circulation models. The Cs-137 deposition amounts at the sea surface were used as the source term in oceanic dispersion simulations, which were estimated by atmospheric dispersion simulations with a Worldwide version of System for Prediction of Environmental Emergency Dose Information version II (WSPEEDI-II) developed at JAEA. The direct release from the Fukushima Daiichi Nuclear Power Plant into the ocean based on in situ Cs-137 measurements was used as the other source term in oceanic dispersion simulations. The simulated air Cs-137 concentrations qualitatively replicated those measured around the North Pacific. The accumulated Cs-137 ground deposition amount in the eastern Japanese Islands was consistent with that estimated by aircraft measurements. The oceanic dispersion simulations relatively well reproduced the measured Cs-137 concentrations in the coastal and offshore oceans during the first few months after the Fukushima disaster, and in the open ocean during the first year post-disaster. It was suggested that Cs-137 dispersed along the coast in the north-south direction during the first few months post-disaster, and were subsequently dispersed offshore by the Kuroshio Current and Kuroshio Extension. Mesoscale eddies accompanied by the Kuroshio Current and Kuroshio Extension played an important role in dilution of Cs-137. The Cs-137 amounts were quantified in the coastal, offshore, and open oceans during the first year post-disaster. It was demonstrated that Cs-137 actively dispersed from the coastal and offshore oceans to the open ocean, and from the surface layer to the deeper layer in the North Pacific.

  1. Open cycle ocean thermal energy conversion system structure

    DOEpatents

    Wittig, J. Michael

    1980-01-01

    A generally mushroom-shaped, open cycle OTEC system and distilled water producer which has a skirt-conduit structure extending from the enlarged portion of the mushroom to the ocean. The enlarged part of the mushroom houses a toroidal casing flash evaporator which produces steam which expands through a vertical rotor turbine, partially situated in the center of the blossom portion and partially situated in the mushroom's stem portion. Upon expansion through the turbine, the motive steam enters a shell and tube condenser annularly disposed about the rotor axis and axially situated beneath the turbine in the stem portion. Relatively warm ocean water is circulated up through the radially outer skirt-conduit structure entering the evaporator through a radially outer portion thereof, flashing a portion thereof into motive steam, and draining the unflashed portion from the evaporator through a radially inner skirt-conduit structure. Relatively cold cooling water enters the annular condenser through the radially inner edge and travels radially outwardly into a channel situated along the radially outer edge of the condenser. The channel is also included in the radially inner skirt-conduit structure. The cooling water is segregated from the potable, motive steam condensate which can be used for human consumption or other processes requiring high purity water. The expansion energy of the motive steam is partially converted into rotational mechanical energy of the turbine rotor when the steam is expanded through the shaft attached blades. Such mechanical energy drives a generator also included in the enlarged mushroom portion for producing electrical energy. Such power generation equipment arrangement provides a compact power system from which additional benefits may be obtained by fabricating the enclosing equipment, housings and component casings from low density materials, such as prestressed concrete, to permit those casings and housings to also function as a floating

  2. Open-ocean boundary conditions from interior data: Local and remote forcing of Massachusetts Bay

    USGS Publications Warehouse

    Bogden, P.S.; Malanotte-Rizzoli, P.; Signell, R.

    1996-01-01

    Massachusetts and Cape Cod Bays form a semienclosed coastal basin that opens onto the much larger Gulf of Maine. Subtidal circulation in the bay is driven by local winds and remotely driven flows from the gulf. The local-wind forced flow is estimated with a regional shallow water model driven by wind measurements. The model uses a gravity wave radiation condition along the open-ocean boundary. Results compare reasonably well with observed currents near the coast. In some offshore regions however, modeled flows are an order of magnitude less energetic than the data. Strong flows are observed even during periods of weak local wind forcing. Poor model-data comparisons are attributable, at least in part, to open-ocean boundary conditions that neglect the effects of remote forcing. Velocity measurements from within Massachusetts Bay are used to estimate the remotely forced component of the flow. The data are combined with shallow water dynamics in an inverse-model formulation that follows the theory of Bennett and McIntosh [1982], who considered tides. We extend their analysis to consider the subtidal response to transient forcing. The inverse model adjusts the a priori open-ocean boundary condition, thereby minimizing a combined measure of model-data misfit and boundary condition adjustment. A "consistency criterion" determines the optimal trade-off between the two. The criterion is based on a measure of plausibility for the inverse solution. The "consistent" inverse solution reproduces 56% of the average squared variation in the data. The local-wind-driven flow alone accounts for half of the model skill. The other half is attributable to remotely forced flows from the Gulf of Maine. The unexplained 44% comes from measurement errors and model errors that are not accounted for in the analysis. 

  3. Phytoplankton responses to atmospheric metal deposition in the coastal and open-ocean Sargasso Sea

    PubMed Central

    Mackey, Katherine R. M.; Buck, Kristen N.; Casey, John R.; Cid, Abigail; Lomas, Michael W.; Sohrin, Yoshiki; Paytan, Adina

    2012-01-01

    This study investigated the impact of atmospheric metal deposition on natural phytoplankton communities at open-ocean and coastal sites in the Sargasso Sea during the spring bloom. Locally collected aerosols with different metal contents were added to natural phytoplankton assemblages from each site, and changes in nitrate, dissolved metal concentration, and phytoplankton abundance and carbon content were monitored. Addition of aerosol doubled the concentrations of cadmium (Cd), cobalt (Co), copper (Cu), iron (Fe), manganese (Mn), and nickel (Ni) in the incubation water. Over the 3-day experiments, greater drawdown of dissolved metals occurred in the open ocean water, whereas little metal drawdown occurred in the coastal water. Two populations of picoeukaryotic algae and Synechococcus grew in response to aerosol additions in both experiments. Particulate organic carbon increased and was most sensitive to changes in picoeukaryote abundance. Phytoplankton community composition differed depending on the chemistry of the aerosol added. Enrichment with aerosol that had higher metal content led to a 10-fold increase in Synechococcus abundance in the oceanic experiment but not in the coastal experiment. Enrichment of aerosol-derived Co, Mn, and Ni were particularly enhanced in the oceanic experiment, suggesting the Synechococcus population may have been fertilized by these aerosol metals. Cu-binding ligand concentrations were in excess of dissolved Cu in both experiments, and increased with aerosol additions. Bioavailable free hydrated Cu2+ concentrations were below toxicity thresholds throughout both experiments. These experiments show (1) atmospheric deposition contributes biologically important metals to seawater, (2) these metals are consumed over time scales commensurate with cell growth, and (3) growth responses can differ between distinct Synechococcus or eukaryotic algal populations despite their relatively close geographic proximity and taxonomic similarity. PMID

  4. Deep Water Ocean Acoustics

    DTIC Science & Technology

    2016-08-03

    Militia Drive Lexington, MA 02421 Date Submitted: Aug 3, 2016 Notices : Distribution Statement A. Approved for public release...distribution is unlimited. OASIS, INC. 2 Report No. QSR-14C0172-Ocean Acoustics-063016 Contents Notices ...the impact of the ocean and seafloor environmental variability on deep-water (long-range) ocean acoustic propagation and to develop methodologies

  5. Retrieval of the spectral diffuse attenuation coefficient Kd(λ) in open and coastal ocean waters using a neural network inversion

    NASA Astrophysics Data System (ADS)

    Jamet, C.; Loisel, H.; Dessailly, D.

    2012-10-01

    The diffuse attenuation coefficient, Kd(λ) is a fundamental radiometric parameter that is used to assess the light availability in the water column. A neural network approach is developed to assess Kd(λ) at any visible wavelengths from the remote sensing reflectances as measured by the SeaWiFS satellite sensor. The neural network (NN) inversion is trained using a combination of simulated and in-situ data sets covering a broad range ofKd(λ), between 0.0073 m-1 at 412 nm and 12.41 m-1at 510 nm. The performance of the retrieval is evaluated against two data sets, one consisting of mainly synthetic data while the other one contains in-situ data only and is compared to those obtained with previous published empirical (NASA, Morel and Maritorena (2001) and Zhang and Fell (2007)) and semi-analytical (Lee et al., 2005b) algorithms. On the in-situ data set from the COASTLOOC campaign, the retrieval accuracy of the present algorithm is quite similar to published algorithms for oligotrophic and mesotrophic ocean waters. But for Kd(490) > 0.25 m-1, the NN approach allows to retrieve Kd(490) with a much better accuracy than the four other methods. The results are consistent when compared with other SeaWiFS wavelengths. This new inversion is as suitable in the open ocean waters as in the turbid waters. The work here is straightforwardly applicable to the MERIS sensor and with few changes to the MODIS-AQUA sensor. The algorithm in matlab and C code is provided as auxiliary material.

  6. A baroclinic quasigeostrophic open ocean model

    NASA Technical Reports Server (NTRS)

    Miller, R. N.; Robinson, A. R.; Haidvogel, D. B.

    1983-01-01

    A baroclinic quasigeostrophic open ocean model is presented, calibrated by a series of test problems, and demonstrated to be feasible and efficient for application to realistic mid-oceanic mesoscale eddy flow regimes. Two methods of treating the depth dependence of the flow, a finite difference method and a collocation method, are tested and intercompared. Sample Rossby wave calculations with and without advection are performed with constant stratification and two levels of nonlinearity, one weaker than and one typical of real ocean flows. Using exact analytical solutions for comparison, the accuracy and efficiency of the model is tabulated as a function of the computational parameters and stability limits set; typically, errors were controlled between 1 percent and 10 percent RMS after two wave periods. Further Rossby wave tests with realistic stratification and wave parameters chosen to mimic real ocean conditions were performed to determine computational parameters for use with real and simulated data. Finally, a prototype calculation with quasiturbulent simulated data was performed successfully, which demonstrates the practicality of the model for scientific use.

  7. Open-ocean fish reveal an omnidirectional solution to camouflage in polarized environments.

    PubMed

    Brady, Parrish C; Gilerson, Alexander A; Kattawar, George W; Sullivan, James M; Twardowski, Michael S; Dierssen, Heidi M; Gao, Meng; Travis, Kort; Etheredge, Robert Ian; Tonizzo, Alberto; Ibrahim, Amir; Carrizo, Carlos; Gu, Yalong; Russell, Brandon J; Mislinski, Kathryn; Zhao, Shulei; Cummings, Molly E

    2015-11-20

    Despite appearing featureless to our eyes, the open ocean is a highly variable environment for polarization-sensitive viewers. Dynamic visual backgrounds coupled with predator encounters from all possible directions make this habitat one of the most challenging for camouflage. We tested open-ocean crypsis in nature by collecting more than 1500 videopolarimetry measurements from live fish from distinct habitats under a variety of viewing conditions. Open-ocean fish species exhibited camouflage that was superior to that of both nearshore fish and mirrorlike surfaces, with significantly higher crypsis at angles associated with predator detection and pursuit. Histological measurements revealed that specific arrangements of reflective guanine platelets in the fish's skin produce angle-dependent polarization modifications for polarocrypsis in the open ocean, suggesting a mechanism for natural selection to shape reflectance properties in this complex environment. Copyright © 2015, American Association for the Advancement of Science.

  8. Southern Ocean Open Ocean Polynyas in Observations and from a Low- and a High-Resolution Fully-Coupled Earth System Model Simulation

    NASA Astrophysics Data System (ADS)

    Veneziani, C.; Kurtakoti, P. K.; Weijer, W.; Stoessel, A.

    2016-12-01

    In contrast to their better known coastal counterpart, open ocean polynyas (OOPs) form through complex driving mechanisms, involving pre-conditioning of the water column, external forcing and internal ocean dynamics, and are therefore much more elusive and less predictable than coastal polynyas. Yet, their impact on bottom water formation and the Meridional Overturning Circulation could prove substantial. Here, we characterize the formation of Southern Ocean OOPs by analyzing the full satellite NASA microwave imager and radiometer (SSMI/SMMR) data record from 1972 to present day. We repeat the same analysis within the low-resolution (LR) and high-resolution (HR) fully-coupled Earth System Model simulations that are part of the Accelerated Climate Model for Energy (ACME) v0 baseline experiments. The focus is on two OOPs that are more consistently seen in observations: the Maud Rise and the Weddell Sea polynyas. Results show that the LR simulation is unable to reproduce any OOP over the 195 years of its duration, while both Maud Rise and Weddell Sea polynyas are seen in the HR simulation, with extents similar to observations'. We explore possible mechanisms that would explain the asymmetric behavior, including topographic processes, eddy shedding events, and different water column stratification between the two simulations.

  9. Towards the impact of eddies on the response of the global ocean circulation to Southern Ocean gateway opening

    NASA Astrophysics Data System (ADS)

    Viebahn, Jan; von der Heydt, Anna S.; Dijkstra, Henk A.

    2014-05-01

    During the past 65 Million (Ma) years, Earth's climate has undergone a major change from warm 'greenhouse' to colder 'icehouse' conditions with extensive ice sheets in the polar regions of both hemispheres. The Eocene-Oligocene (~34 Ma) and Oligocene-Miocene (~23 Ma) boundaries reflect major transitions in Cenozoic global climate change. Proposed mechanisms of these transitions include reorganization of ocean circulation due to critical gateway opening/deepening, changes in atmospheric CO2-concentration, and feedback mechanisms related to land-ice formation. A long-standing hypothesis is that the formation of the Antarctic Circumpolar Current due to opening/deepening of Southern Ocean gateways led to glaciation of the Antarctic continent. However, while this hypothesis remains controversial, its assessment via coupled climate model simulations depends crucially on the spatial resolution in the ocean component. More precisely, only high-resolution modeling of the turbulent ocean circulation is capable of adequately describing reorganizations in the ocean flow field and related changes in turbulent heat transport. In this study, for the first time results of a high-resolution (0.1° horizontally) realistic global ocean model simulation with a closed Drake Passage are presented. Changes in global ocean temperatures, heat transport, and ocean circulation (e.g., Meridional Overturning Circulation and Antarctic Coastal Current) are established by comparison with an open Drake Passage high-resolution reference simulation. Finally, corresponding low-resolution simulations are also analyzed. The results highlight the essential impact of the ocean eddy field in palaeoclimatic change.

  10. Arctic Deep Water Ferromanganese-Oxide Deposits Reflect the Unique Characteristics of the Arctic Ocean

    NASA Astrophysics Data System (ADS)

    Hein, James R.; Konstantinova, Natalia; Mikesell, Mariah; Mizell, Kira; Fitzsimmons, Jessica N.; Lam, Phoebe J.; Jensen, Laramie T.; Xiang, Yang; Gartman, Amy; Cherkashov, Georgy; Hutchinson, Deborah R.; Till, Claire P.

    2017-11-01

    Little is known about marine mineral deposits in the Arctic Ocean, an ocean dominated by continental shelf and basins semi-closed to deep-water circulation. Here, we present data for ferromanganese crusts and nodules collected from the Amerasia Arctic Ocean in 2008, 2009, and 2012 (HLY0805, HLY0905, and HLY1202). We determined mineral and chemical compositions of the crusts and nodules and the onset of their formation. Water column samples from the GEOTRACES program were analyzed for dissolved and particulate scandium concentrations, an element uniquely enriched in these deposits. The Arctic crusts and nodules are characterized by unique mineral and chemical compositions with atypically high growth rates, detrital contents, Fe/Mn ratios, and low Si/Al ratios, compared to deposits found elsewhere. High detritus reflects erosion of submarine outcrops and North America and Siberia cratons, transport by rivers and glaciers to the sea, and distribution by sea ice, brines, and currents. Uniquely high Fe/Mn ratios are attributed to expansive continental shelves, where diagenetic cycling releases Fe to bottom waters, and density flows transport shelf bottom water to the open Arctic Ocean. Low Mn contents reflect the lack of a mid-water oxygen minimum zone that would act as a reservoir for dissolved Mn. The potential host phases and sources for elements with uniquely high contents are discussed with an emphasis on scandium. Scandium sorption onto Fe oxyhydroxides and Sc-rich detritus account for atypically high scandium contents. The opening of Fram Strait in the Miocene and ventilation of the deep basins initiated Fe-Mn crust growth ˜15 Myr ago.

  11. Arctic deep-water ferromanganese-oxide deposits reflect the unique characteristics of the Arctic Ocean

    USGS Publications Warehouse

    Hein, James; Konstantinova, Natalia; Mikesell, Mariah; Mizell, Kira; Fitzsimmons, Jessica N.; Lam, Phoebe; Jensen, Laramie T.; Xiang, Yang; Gartman, Amy; Cherkashov, Georgy; Hutchinson, Deborah; Till, Claire P.

    2017-01-01

    Little is known about marine mineral deposits in the Arctic Ocean, an ocean dominated by continental shelf and basins semi-closed to deep-water circulation. Here, we present data for ferromanganese crusts and nodules collected from the Amerasia Arctic Ocean in 2008, 2009, and 2012 (HLY0805, HLY0905, HLY1202). We determined mineral and chemical compositions of the crusts and nodules and the onset of their formation. Water column samples from the GEOTRACES program were analyzed for dissolved and particulate scandium concentrations, an element uniquely enriched in these deposits.The Arctic crusts and nodules are characterized by unique mineral and chemical compositions with atypically high growth rates, detrital contents, Fe/Mn ratios, and low Si/Al ratios, compared to deposits found elsewhere. High detritus reflects erosion of submarine outcrops and North America and Siberia cratons, transport by rivers and glaciers to the sea, and distribution by sea ice, brines, and currents. Uniquely high Fe/Mn ratios are attributed to expansive continental shelves, where diagenetic cycling releases Fe to bottom waters, and density flows transport shelf bottom water to the open Arctic Ocean. Low Mn contents reflect the lack of a mid-water oxygen minimum zone that would act as a reservoir for dissolved Mn. The potential host phases and sources for elements with uniquely high contents are discussed with an emphasis on scandium. Scandium sorption onto Fe oxyhydroxides and Sc-rich detritus account for atypically high scandium contents. The opening of Fram Strait in the Miocene and ventilation of the deep basins initiated Fe-Mn crust growth ∼15 Myr ago.

  12. Liquid Water Oceans in Ice Giants

    NASA Technical Reports Server (NTRS)

    Wiktorowicz, Sloane J.; Ingersoll, Andrew P.

    2007-01-01

    Aptly named, ice giants such as Uranus and Neptune contain significant amounts of water. While this water cannot be present near the cloud tops, it must be abundant in the deep interior. We investigate the likelihood of a liquid water ocean existing in the hydrogen-rich region between the cloud tops and deep interior. Starting from an assumed temperature at a given upper tropospheric pressure (the photosphere), we follow a moist adiabat downward. The mixing ratio of water to hydrogen in the gas phase is small in the photosphere and increases with depth. The mixing ratio in the condensed phase is near unity in the photosphere and decreases with depth; this gives two possible outcomes. If at some pressure level the mixing ratio of water in the gas phase is equal to that in the deep interior, then that level is the cloud base. The gas below the cloud base has constant mixing ratio. Alternately, if the mixing ratio of water in the condensed phase reaches that in the deep interior, then the surface of a liquid ocean will occur. Below this ocean surface, the mixing ratio of water will be constant. A cloud base occurs when the photospheric temperature is high. For a family of ice giants with different photospheric temperatures, the cooler ice giants will have warmer cloud bases. For an ice giant with a cool enough photospheric temperature, the cloud base will exist at the critical temperature. For still cooler ice giants, ocean surfaces will result. A high mixing ratio of water in the deep interior favors a liquid ocean. We find that Neptune is both too warm (photospheric temperature too high) and too dry (mixing ratio of water in the deep interior too low) for liquid oceans to exist at present. To have a liquid ocean, Neptune s deep interior water to gas ratio would have to be higher than current models allow, and the density at 19 kbar would have to be approx. equal to 0.8 g/cu cm. Such a high density is inconsistent with gravitational data obtained during the Voyager

  13. Deep sediment resuspension and thick nepheloid layer generation by open-ocean convection

    NASA Astrophysics Data System (ADS)

    Durrieu de Madron, X.; Ramondenc, S.; Berline, L.; Houpert, L.; Bosse, A.; Martini, S.; Guidi, L.; Conan, P.; Curtil, C.; Delsaut, N.; Kunesch, S.; Ghiglione, J. F.; Marsaleix, P.; Pujo-Pay, M.; Séverin, T.; Testor, P.; Tamburini, C.

    2017-03-01

    The Gulf of Lions in the northwestern Mediterranean is one of the few sites around the world ocean exhibiting deep open-ocean convection. Based on 6 year long (2009-2015) time series from a mooring in the convection region, shipborne measurements from repeated cruises, from 2012 to 2015, and glider measurements, we report evidence of bottom thick nepheloid layer formation, which is coincident with deep sediment resuspension induced by bottom-reaching convection events. This bottom nepheloid layer, which presents a maximum thickness of more than 2000 m in the center of the convection region, probably results from the action of cyclonic eddies that are formed during the convection period and can persist within their core while they travel through the basin. The residence time of this bottom nepheloid layer appears to be less than a year. In situ measurements of suspended particle size further indicate that the bottom nepheloid layer is primarily composed of aggregates between 100 and 1000 µm in diameter, probably constituted of fine silts. Bottom-reaching open ocean convection, as well as deep dense shelf water cascading that occurred concurrently some years, lead to recurring deep sediments resuspension episodes. They are key mechanisms that control the concentration and characteristics of the suspended particulate matter in the basin, and in turn affect the bathypelagic biological activity.

  14. Deep-sea bioluminescence blooms after dense water formation at the ocean surface.

    PubMed

    Tamburini, Christian; Canals, Miquel; Durrieu de Madron, Xavier; Houpert, Loïc; Lefèvre, Dominique; Martini, Séverine; D'Ortenzio, Fabrizio; Robert, Anne; Testor, Pierre; Aguilar, Juan Antonio; Samarai, Imen Al; Albert, Arnaud; André, Michel; Anghinolfi, Marco; Anton, Gisela; Anvar, Shebli; Ardid, Miguel; Jesus, Ana Carolina Assis; Astraatmadja, Tri L; Aubert, Jean-Jacques; Baret, Bruny; Basa, Stéphane; Bertin, Vincent; Biagi, Simone; Bigi, Armando; Bigongiari, Ciro; Bogazzi, Claudio; Bou-Cabo, Manuel; Bouhou, Boutayeb; Bouwhuis, Mieke C; Brunner, Jurgen; Busto, José; Camarena, Francisco; Capone, Antonio; Cârloganu, Christina; Carminati, Giada; Carr, John; Cecchini, Stefano; Charif, Ziad; Charvis, Philippe; Chiarusi, Tommaso; Circella, Marco; Coniglione, Rosa; Costantini, Heide; Coyle, Paschal; Curtil, Christian; Decowski, Patrick; Dekeyser, Ivan; Deschamps, Anne; Donzaud, Corinne; Dornic, Damien; Dorosti, Hasankiadeh Q; Drouhin, Doriane; Eberl, Thomas; Emanuele, Umberto; Ernenwein, Jean-Pierre; Escoffier, Stéphanie; Fermani, Paolo; Ferri, Marcelino; Flaminio, Vincenzo; Folger, Florian; Fritsch, Ulf; Fuda, Jean-Luc; Galatà, Salvatore; Gay, Pascal; Giacomelli, Giorgio; Giordano, Valentina; Gómez-González, Juan-Pablo; Graf, Kay; Guillard, Goulven; Halladjian, Garadeb; Hallewell, Gregory; van Haren, Hans; Hartman, Joris; Heijboer, Aart J; Hello, Yann; Hernández-Rey, Juan Jose; Herold, Bjoern; Hößl, Jurgen; Hsu, Ching-Cheng; de Jong, Marteen; Kadler, Matthias; Kalekin, Oleg; Kappes, Alexander; Katz, Uli; Kavatsyuk, Oksana; Kooijman, Paul; Kopper, Claudio; Kouchner, Antoine; Kreykenbohm, Ingo; Kulikovskiy, Vladimir; Lahmann, Robert; Lamare, Patrick; Larosa, Giuseppina; Lattuada, Dario; Lim, Gordon; Presti, Domenico Lo; Loehner, Herbert; Loucatos, Sotiris; Mangano, Salvatore; Marcelin, Michel; Margiotta, Annarita; Martinez-Mora, Juan Antonio; Meli, Athina; Montaruli, Teresa; Moscoso, Luciano; Motz, Holger; Neff, Max; Nezri, Emma Nuel; Palioselitis, Dimitris; Păvălaş, Gabriela E; Payet, Kevin; Payre, Patrice; Petrovic, Jelena; Piattelli, Paolo; Picot-Clemente, Nicolas; Popa, Vlad; Pradier, Thierry; Presani, Eleonora; Racca, Chantal; Reed, Corey; Riccobene, Giorgio; Richardt, Carsten; Richter, Roland; Rivière, Colas; Roensch, Kathrin; Rostovtsev, Andrei; Ruiz-Rivas, Joaquin; Rujoiu, Marius; Russo, Valerio G; Salesa, Francisco; Sánchez-Losa, Augustin; Sapienza, Piera; Schöck, Friederike; Schuller, Jean-Pierre; Schussler, Fabian; Shanidze, Rezo; Simeone, Francesco; Spies, Andreas; Spurio, Maurizio; Steijger, Jos J M; Stolarczyk, Thierry; Taiuti, Mauro G F; Toscano, Simona; Vallage, Bertrand; Van Elewyck, Véronique; Vannoni, Giulia; Vecchi, Manuela; Vernin, Pascal; Wijnker, Guus; Wilms, Jorn; de Wolf, Els; Yepes, Harold; Zaborov, Dmitry; De Dios Zornoza, Juan; Zúñiga, Juan

    2013-01-01

    The deep ocean is the largest and least known ecosystem on Earth. It hosts numerous pelagic organisms, most of which are able to emit light. Here we present a unique data set consisting of a 2.5-year long record of light emission by deep-sea pelagic organisms, measured from December 2007 to June 2010 at the ANTARES underwater neutrino telescope in the deep NW Mediterranean Sea, jointly with synchronous hydrological records. This is the longest continuous time-series of deep-sea bioluminescence ever recorded. Our record reveals several weeks long, seasonal bioluminescence blooms with light intensity up to two orders of magnitude higher than background values, which correlate to changes in the properties of deep waters. Such changes are triggered by the winter cooling and evaporation experienced by the upper ocean layer in the Gulf of Lion that leads to the formation and subsequent sinking of dense water through a process known as "open-sea convection". It episodically renews the deep water of the study area and conveys fresh organic matter that fuels the deep ecosystems. Luminous bacteria most likely are the main contributors to the observed deep-sea bioluminescence blooms. Our observations demonstrate a consistent and rapid connection between deep open-sea convection and bathypelagic biological activity, as expressed by bioluminescence. In a setting where dense water formation events are likely to decline under global warming scenarios enhancing ocean stratification, in situ observatories become essential as environmental sentinels for the monitoring and understanding of deep-sea ecosystem shifts.

  15. Deep-Sea Bioluminescence Blooms after Dense Water Formation at the Ocean Surface

    PubMed Central

    Tamburini, Christian; Canals, Miquel; Durrieu de Madron, Xavier; Houpert, Loïc; Lefèvre, Dominique; Martini, Séverine; D'Ortenzio, Fabrizio; Robert, Anne; Testor, Pierre; Aguilar, Juan Antonio; Samarai, Imen Al; Albert, Arnaud; André, Michel; Anghinolfi, Marco; Anton, Gisela; Anvar, Shebli; Ardid, Miguel; Jesus, Ana Carolina Assis; Astraatmadja, Tri L.; Aubert, Jean-Jacques; Baret, Bruny; Basa, Stéphane; Bertin, Vincent; Biagi, Simone; Bigi, Armando; Bigongiari, Ciro; Bogazzi, Claudio; Bou-Cabo, Manuel; Bouhou, Boutayeb; Bouwhuis, Mieke C.; Brunner, Jurgen; Busto, José; Camarena, Francisco; Capone, Antonio; Cârloganu, Christina; Carminati, Giada; Carr, John; Cecchini, Stefano; Charif, Ziad; Charvis, Philippe; Chiarusi, Tommaso; Circella, Marco; Coniglione, Rosa; Costantini, Heide; Coyle, Paschal; Curtil, Christian; Decowski, Patrick; Dekeyser, Ivan; Deschamps, Anne; Donzaud, Corinne; Dornic, Damien; Dorosti, Hasankiadeh Q.; Drouhin, Doriane; Eberl, Thomas; Emanuele, Umberto; Ernenwein, Jean-Pierre; Escoffier, Stéphanie; Fermani, Paolo; Ferri, Marcelino; Flaminio, Vincenzo; Folger, Florian; Fritsch, Ulf; Fuda, Jean-Luc; Galatà, Salvatore; Gay, Pascal; Giacomelli, Giorgio; Giordano, Valentina; Gómez-González, Juan-Pablo; Graf, Kay; Guillard, Goulven; Halladjian, Garadeb; Hallewell, Gregory; van Haren, Hans; Hartman, Joris; Heijboer, Aart J.; Hello, Yann; Hernández-Rey, Juan Jose; Herold, Bjoern; Hößl, Jurgen; Hsu, Ching-Cheng; de Jong, Marteen; Kadler, Matthias; Kalekin, Oleg; Kappes, Alexander; Katz, Uli; Kavatsyuk, Oksana; Kooijman, Paul; Kopper, Claudio; Kouchner, Antoine; Kreykenbohm, Ingo; Kulikovskiy, Vladimir; Lahmann, Robert; Lamare, Patrick; Larosa, Giuseppina; Lattuada, Dario; Lim, Gordon; Presti, Domenico Lo; Loehner, Herbert; Loucatos, Sotiris; Mangano, Salvatore; Marcelin, Michel; Margiotta, Annarita; Martinez-Mora, Juan Antonio; Meli, Athina; Montaruli, Teresa; Motz, Holger; Neff, Max; Nezri, Emma nuel; Palioselitis, Dimitris; Păvălaş, Gabriela E.; Payet, Kevin; Payre, Patrice; Petrovic, Jelena; Piattelli, Paolo; Picot-Clemente, Nicolas; Popa, Vlad; Pradier, Thierry; Presani, Eleonora; Racca, Chantal; Reed, Corey; Riccobene, Giorgio; Richardt, Carsten; Richter, Roland; Rivière, Colas; Roensch, Kathrin; Rostovtsev, Andrei; Ruiz-Rivas, Joaquin; Rujoiu, Marius; Russo, Valerio G.; Salesa, Francisco; Sánchez-Losa, Augustin; Sapienza, Piera; Schöck, Friederike; Schuller, Jean-Pierre; Schussler, Fabian; Shanidze, Rezo; Simeone, Francesco; Spies, Andreas; Spurio, Maurizio; Steijger, Jos J. M.; Stolarczyk, Thierry; Taiuti, Mauro G. F.; Toscano, Simona; Vallage, Bertrand; Van Elewyck, Véronique; Vannoni, Giulia; Vecchi, Manuela; Vernin, Pascal; Wijnker, Guus; Wilms, Jorn; de Wolf, Els; Yepes, Harold; Zaborov, Dmitry; De Dios Zornoza, Juan; Zúñiga, Juan

    2013-01-01

    The deep ocean is the largest and least known ecosystem on Earth. It hosts numerous pelagic organisms, most of which are able to emit light. Here we present a unique data set consisting of a 2.5-year long record of light emission by deep-sea pelagic organisms, measured from December 2007 to June 2010 at the ANTARES underwater neutrino telescope in the deep NW Mediterranean Sea, jointly with synchronous hydrological records. This is the longest continuous time-series of deep-sea bioluminescence ever recorded. Our record reveals several weeks long, seasonal bioluminescence blooms with light intensity up to two orders of magnitude higher than background values, which correlate to changes in the properties of deep waters. Such changes are triggered by the winter cooling and evaporation experienced by the upper ocean layer in the Gulf of Lion that leads to the formation and subsequent sinking of dense water through a process known as “open-sea convection”. It episodically renews the deep water of the study area and conveys fresh organic matter that fuels the deep ecosystems. Luminous bacteria most likely are the main contributors to the observed deep-sea bioluminescence blooms. Our observations demonstrate a consistent and rapid connection between deep open-sea convection and bathypelagic biological activity, as expressed by bioluminescence. In a setting where dense water formation events are likely to decline under global warming scenarios enhancing ocean stratification, in situ observatories become essential as environmental sentinels for the monitoring and understanding of deep-sea ecosystem shifts. PMID:23874425

  16. Gradients in microbial methanol uptake: productive coastal upwelling waters to oligotrophic gyres in the Atlantic Ocean

    PubMed Central

    Dixon, Joanna L; Sargeant, Stephanie; Nightingale, Philip D; Colin Murrell, J

    2013-01-01

    Methanol biogeochemistry and its importance as a carbon source in seawater is relatively unexplored. We report the first microbial methanol carbon assimilation rates (k) in productive coastal upwelling waters of up to 0.117±0.002 d−1 (∼10 nmol l−1 d−1). On average, coastal upwelling waters were 11 times greater than open ocean northern temperate (NT) waters, eight times greater than gyre waters and four times greater than equatorial upwelling (EU) waters; suggesting that all upwelling waters upon reaching the surface (⩽20 m), contain a microbial population that uses a relatively high amount of carbon (0.3–10 nmol l−1 d−1), derived from methanol, to support their growth. In open ocean Atlantic regions, microbial uptake of methanol into biomass was significantly lower, ranging between 0.04–0.68 nmol l−1 d−1. Microbes in the Mauritanian coastal upwelling used up to 57% of the total methanol for assimilation of the carbon into cells, compared with an average of 12% in the EU, and 1% in NT and gyre waters. Several methylotrophic bacterial species were identified from open ocean Atlantic waters using PCR amplification of mxaF encoding methanol dehydrogenase, the key enzyme in bacterial methanol oxidation. These included Methylophaga sp., Burkholderiales sp., Methylococcaceae sp., Ancylobacter aquaticus, Paracoccus denitrificans, Methylophilus methylotrophus, Methylobacterium oryzae, Hyphomicrobium sp. and Methylosulfonomonas methylovora. Statistically significant correlations for upwelling waters between methanol uptake into cells and both chlorophyll a concentrations and methanol oxidation rates suggest that remotely sensed chlorophyll a images, in these productive areas, could be used to derive total methanol biological loss rates, a useful tool for atmospheric and marine climatically active gas modellers, and air–sea exchange scientists. PMID:23178665

  17. Marine mammal distribution in the open ocean: a comparison of ocean color data products and levant time scales

    NASA Astrophysics Data System (ADS)

    Ohern, J.

    2016-02-01

    Marine mammals are generally located in areas of enhanced surface primary productivity, though they may forage much deeper within the water column and higher on the food chain. Numerous studies over the past several decades have utilized ocean color data from remote sensing instruments (CZCS, MODIS, and others) to asses both the quantity and time scales over which surface primary productivity relates to marine mammal distribution. In areas of sustained upwelling, primary productivity may essentially grow in the secondary levels of productivity (the zooplankton and nektonic species on which marine mammals forage). However, in many open ocean habitats a simple trophic cascade does not explain relatively short time lags between enhanced surface productivity and marine mammal presence. Other dynamic features that entrain prey or attract marine mammals may be responsible for the correlations between marine mammals and ocean color. In order to investigate these features, two MODIS (moderate imaging spectroradiometer) data products, the concentration as well as the standard deviation of surface chlorophyll were used in conjunction with marine mammal sightings collected within Ecuadorian waters. Time lags between enhanced surface chlorophyll and marine mammal presence were on the order of 2-4 weeks, however correlations were much stronger when the standard deviation of spatially binned images was used, rather than the chlorophyll concentrations. Time lags also varied between Balaenopterid and Odontocete cetaceans. Overall, the standard deviation of surface chlorophyll proved a useful tool for assessing potential relationships between marine mammal sightings and surface chlorophyll.

  18. Multi-pumping flow system for the determination of boron in eye drops, drinking water and ocean water.

    PubMed

    González, Pablo; Sixto, Alexandra; Knochen, Moisés

    2017-05-01

    A novel automated method for the determination of boron based on the use of pulsed flows was developed and applied to the determination of this element in samples of tap water, ocean water and eye drops. The method was implemented by means of a multi-pumping system consisting of three solenoid micropumps and a photometric detector and exploits the reaction of azomethine-H in the presence of boron. The system runs under control of an open-source microcontroller. The main operational parameters were optimized. Given the particular kinetics of the reaction, a stopped-flow period (1 or 5min) was included to allow for color development. The method presents linearity in the range 0.35-3.0mgL -1 , good precision (s r <3%), and detection and quantification limits of 0.10 and 0.35mgL -1 respectively. Samples of tap water or eye drops could be successfully analyzed employing a 1-minute stop time, providing a maximum sampling frequency of 32 samples h -1 . In order to overcome matrix effect caused by the high saline concentration, ocean water samples required stop times of 5min, providing a sampling frequency of 10 samples h -1 . Recoveries of 102% (eye drops), 94% (drinking water) and 93% (ocean water) were obtained. The method was considered accurate and fit for the purpose. Copyright © 2015 Elsevier B.V. All rights reserved.

  19. Atmospheric correction of AVIRIS data in ocean waters

    NASA Technical Reports Server (NTRS)

    Terrie, Gregory; Arnone, Robert

    1992-01-01

    Hyperspectral data offers unique capabilities for characterizing the ocean environment. The spectral characterization of the composition of ocean waters can be organized into biological and terrigenous components. Biological photosynthetic pigments in ocean waters have unique spectral ocean color signatures which can be associated with different biological species. Additionally, suspended sediment has different scattering coefficients which result in ocean color signatures. Measuring the spatial distributions of these components in the maritime environments provides important tools for understanding and monitoring the ocean environment. These tools have significant applications in pollution, carbon cycle, current and water mass detection, location of fronts and eddies, sewage discharge and fate etc. Ocean color was used from satellite for describing the spatial variability of chlorophyll, water clarity (K(sub 490)), suspended sediment concentration, currents etc. Additionally, with improved atmospheric correction methods, ocean color results produced global products of spectral water leaving radiance (L(sub W)). Ocean color results clearly indicated strong applications for characterizing the spatial and temporal variability of bio-optical oceanography. These studies were largely the results of advanced atmospheric correction techniques applied to multispectral imagery. The atmosphere contributes approximately 80 percent - 90 percent of the satellite received radiance in the blue-green portion of the spectrum. In deep ocean waters, maximum transmission of visible radiance is achieved at 490nm. Conversely, nearly all of the light is absorbed by the water at wavelengths greater than about 650nm and thus appears black. These spectral ocean properties are exploited by algorithms developed for the atmospheric correction used in satellite ocean color processing. The objective was to apply atmospheric correction techniques that were used for procesing satellite Coastal

  20. Degradation Signatures of Open Ocean Microplastic Debris

    NASA Astrophysics Data System (ADS)

    Lavender Law, K. L.; Donohue, J. L.; Collins, T.; Proskurowsi, G.; Andrady, A. L.

    2016-02-01

    Microplastics collected from the open ocean offer few clues about their origin and history. There is currently no method to determine how long ocean plastic has undergone environmental weathering, how quickly fragmentation has occurred, or how small microplastic particles will ultimately become before (or if) they are fully degraded by microbial action. In the current absence of results from laboratory and field experiments designed to address these questions, we meticulously examined physical and chemical characteristics of open ocean microplastic particles collected over a 16-year period for clues about their weathering history. More than 1000 microplastic particles collected in the western North Atlantic between 1991 and 2007 were analyzed to determine polymer type, material density, mass and particle size, and were used to create a detailed catalogue of common microscopic surface features likely related to environmental exposure and weathering. Polyethylene and polypropylene, the two buoyant resins most commonly collected at the sea surface, can typically be distinguished by visual microscopy alone, and their particular characteristics lead us to hypothesize that these two resins weaken and fragment in different ways and on different time scales. A subset of resin pellets collected at sea were also analyzed using FTIR-ATR and/or FTIR microscopy for signatures of chemical degradation (e.g., carbonyl index) that are related to physical weathering characteristics such as color, quantified by the yellowness index.

  1. Carbonate dissolution in mixed waters due to ocean acidification

    NASA Astrophysics Data System (ADS)

    Koski, K.; Wilson, J. L.

    2009-12-01

    Much of the anthropogenically released carbon dioxide has been stored as a dissolved gas in the ocean, causing a 0.1 decrease in ocean surface pH, with models predicting that by 2100 the surface ocean pH will be 0.5 below pre-industrial levels. In mixed ocean water - fresh water environments (e.g. estuaries, coastal aquifers, and edges of ice sheets), the decreased ocean pH couples with the mixed water geochemistry to make water more undersaturated with respect to calcium carbonate than ocean acidification alone. Mixed-water calcite dissolution may be one of the first directly observable effects of ocean acidification, as the ocean water and the fresh water can both be saturated with respect to calcium carbonate while their mixture will be undersaturated. We present a basic quantitative model describing mixed water dissolution in coastal or island freshwater aquifers, using temporally changing ocean pH, sea level, precipitation, and groundwater pumping. The model describes the potential for an increased rate of speleogenesis and porosity/permeability development along the lower edge of a fresh water lens aquifer. The model accounts the indirect effects of rising sea level and a growing coastal population on these processes. Applications are to freshwater carbonate aquifers on islands (e.g. the Bahamas) and in coastal areas (e.g. the unconfined Floridan aquifer of the United States, the Yucatan Peninsula of Mexico).

  2. North Atlantic Deep Water and the World Ocean

    NASA Technical Reports Server (NTRS)

    Gordon, A. L.

    1984-01-01

    North Atlantic Deep Water (NADW) by being warmer and more saline than the average abyssal water parcel introduces heat and salt into the abyssal ocean. The source of these properties is upper layer or thermocline water considered to occupy the ocean less dense than sigma-theta of 27.6. That NADW convects even though it's warmer than the abyssal ocean is obviously due to the high salinity. In this way, NADW formation may be viewed as saline convection. The counter force removing heat and salinity (or introducing fresh water) is usually considered to to take place in the Southern Ocean where upwelling deep water is converted to cold fresher Antarctic water masses. The Southern ocean convective process is driven by low temperatures and hence may be considered as thermal convection. A significant fresh water source may also occur in the North Pacific where the northward flowing of abyssal water from the Southern circumpolar belt is saltier and denser than the southward flowing, return abyssal water. The source of the low salinity input may be vertical mixing of the low salinity surface water or the low salinity intermediate water.

  3. Ocean Salinity Variance and the Global Water Cycle.

    NASA Astrophysics Data System (ADS)

    Schmitt, R. W.

    2012-12-01

    Ocean salinity variance is increasing and appears to be an indicator of rapid change in the global water cycle. While the small terrestrial water cycle does not reveal distinct trends, in part due to strong manipulation by civilization, the much larger oceanic water cycle seems to have an excellent proxy for its intensity in the contrasts in sea surface salinity (SSS). Change in the water cycle is arguably the most important challenge facing mankind. But how well do we understand the oceanic response? Does the ocean amplify SSS change to make it a hyper-sensitive indicator of change in the global water cycle? An overview of the research challenges to the oceanographic community for understanding the dominant component of the global water cycle is provided.

  4. Satellite altimetry in sea ice regions - detecting open water for estimating sea surface heights

    NASA Astrophysics Data System (ADS)

    Müller, Felix L.; Dettmering, Denise; Bosch, Wolfgang

    2017-04-01

    The Greenland Sea and the Farm Strait are transporting sea ice from the central Arctic ocean southwards. They are covered by a dynamic changing sea ice layer with significant influences on the Earth climate system. Between the sea ice there exist various sized open water areas known as leads, straight lined open water areas, and polynyas exhibiting a circular shape. Identifying these leads by satellite altimetry enables the extraction of sea surface height information. Analyzing the radar echoes, also called waveforms, provides information on the surface backscatter characteristics. For example waveforms reflected by calm water have a very narrow and single-peaked shape. Waveforms reflected by sea ice show more variability due to diffuse scattering. Here we analyze altimeter waveforms from different conventional pulse-limited satellite altimeters to separate open water and sea ice waveforms. An unsupervised classification approach employing partitional clustering algorithms such as K-medoids and memory-based classification methods such as K-nearest neighbor is used. The classification is based on six parameters derived from the waveform's shape, for example the maximum power or the peak's width. The open-water detection is quantitatively compared to SAR images processed while accounting for sea ice motion. The classification results are used to derive information about the temporal evolution of sea ice extent and sea surface heights. They allow to provide evidence on climate change relevant influences as for example Arctic sea level rise due to enhanced melting rates of Greenland's glaciers and an increasing fresh water influx into the Arctic ocean. Additionally, the sea ice cover extent analyzed over a long-time period provides an important indicator for a globally changing climate system.

  5. The Role of Late Summer Melt Pond Water Layers in the Ocean Mixed Layer on Enhancing Ice/Ocean Albedo Feedbacks in the Arctic

    NASA Astrophysics Data System (ADS)

    Stanton, T. P.; Shaw, W. J.

    2016-02-01

    Drainage of surface melt pond water into the top of the ocean mixed layer is seen widely in the Arctic ice pack in later summer (for example Gallaher et al 2015). Under calm conditions, this fresh water forms a thin, stratified layer immediately below the ice which is dynamically decoupled from the thicker, underlying seasonal mixed layer by the density difference between the two layers. The ephemeral surface layer is significantly warmer than the underlying ocean water owing to the higher freezing temperature of the fresh melt water. How the presence of this warm ephemeral layer enhances basal melt rate and speeds the destruction of the floes is investigated. High resolution timeseries measurements of T/S profiles in the 2m of the ocean immediately below the ice, and eddy-correlation fluxes of heat, salt and momentum 2.5m below the ice were made from an Autonomous Ocean Flux Buoy over a 2 month interval in later summer of 2015 as a component of the ONR Marginal Ice Zone project. The stratification and turbulent forcing observations are used with a 1 D turbulence closure model to understand how momentum and incoming radiative energy are stored and redistributed within the ephemeral layer. Under low wind forcing conditions both turbulent mixing energy and the water with high departure from freezing are trapped in the ephemeral layer by the strong density gradient at the base of the layer, resulting in rapid basal melting. This case is contrasted with model runs where the ephemeral layer heat is allowed to mix across the seasonal mixed layer, which results in slower basal melt rates. Consequently, the salinity-trapped warm ephemeral layer results in the formation of more open water earlier in the summer season, in turn resulting in increased cumulative heating of the ocean mixed layer, enhancing ice/ocean albedo feedbacks.

  6. Assessing Atmospheric Water Injection from Oceanic Impacts

    NASA Technical Reports Server (NTRS)

    Pierazzo, E.

    2005-01-01

    Collisions of asteroids and comets with the Earth s surface are rare events that punctuate the geologic record. Due to the vastness of Earth s oceans, oceanic impacts of asteroids or comets are expected to be about 4 times more frequent than land impacts. The resulting injections of oceanic water into the upper atmosphere can have important repercussions on Earth s climate and atmospheric circulation. However, the duration and overall effect of these large injections are still unconstrained. This work addresses atmospheric injections of large amounts of water in oceanic impacts.

  7. Geophysical potential for wind energy over the open oceans

    PubMed Central

    2017-01-01

    Wind turbines continuously remove kinetic energy from the lower troposphere, thereby reducing the wind speed near hub height. The rate of electricity generation in large wind farms containing multiple wind arrays is, therefore, constrained by the rate of kinetic energy replenishment from the atmosphere above. In recent years, a growing body of research argues that the rate of generated power is limited to around 1.5 W m−2 within large wind farms. However, in this study, we show that considerably higher power generation rates may be sustainable over some open ocean areas. In particular, the North Atlantic is identified as a region where the downward transport of kinetic energy may sustain extraction rates of 6 W m−2 and above over large areas in the annual mean. Furthermore, our results indicate that the surface heat flux from the oceans to the atmosphere may play an important role in creating regions where sustained high rates of downward transport of kinetic energy and thus, high rates of kinetic energy extraction may be geophysical possible. While no commercial-scale deep water wind farms yet exist, our results suggest that such technologies, if they became technically and economically feasible, could potentially provide civilization-scale power. PMID:29073053

  8. Geophysical potential for wind energy over the open oceans.

    PubMed

    Possner, Anna; Caldeira, Ken

    2017-10-24

    Wind turbines continuously remove kinetic energy from the lower troposphere, thereby reducing the wind speed near hub height. The rate of electricity generation in large wind farms containing multiple wind arrays is, therefore, constrained by the rate of kinetic energy replenishment from the atmosphere above. In recent years, a growing body of research argues that the rate of generated power is limited to around 1.5 W m -2 within large wind farms. However, in this study, we show that considerably higher power generation rates may be sustainable over some open ocean areas. In particular, the North Atlantic is identified as a region where the downward transport of kinetic energy may sustain extraction rates of 6 W m -2 and above over large areas in the annual mean. Furthermore, our results indicate that the surface heat flux from the oceans to the atmosphere may play an important role in creating regions where sustained high rates of downward transport of kinetic energy and thus, high rates of kinetic energy extraction may be geophysical possible. While no commercial-scale deep water wind farms yet exist, our results suggest that such technologies, if they became technically and economically feasible, could potentially provide civilization-scale power.

  9. Open oceanic productivity changes at mid-latitudes during interglacials and its relation to the Atlantic Meridional Overturning Circulation

    NASA Astrophysics Data System (ADS)

    Nave, Silvia; Lebreiro, S.; Kissel, C.; Guihou, A.; Figueiredo, M. O.; Silva, T. P.; Michel, E.; Cortijo, E.; Labeyrie, L.; Voelker, A.

    2010-05-01

    Variations in the interactions between marine ecosystems, thermohaline circulation, external forcing and atmospheric greenhouse gases concentrations are not yet fully represented in detailed models of the glacial-interglacial transitions. Most of the research on past productivity changes has been focused so far on high-productivity areas such as upwelling areas (i.e. equatorial or coastal upwelling areas) even though those regions appraise only a little part of the ocean. Accordingly, the importance of oceanic productivity changes over glacial/interglacial cycles should be better known, as it may also play an important role on the loss of photosynthetically generated carbon as a central mechanism in the global carbon cycle. Its understanding will help quantifying the parameters needed to run comprehensive climate models, and subsequently help to better predict climate change for the near future. A high-resolution study of oceanic productivity, bottom water flow speed, surface and deep-water mass, bottom water ventilation, and terrestrial input changes during two interglacials (Holocene and Marine Isotope Stage [MIS] 5), at an open ocean site approximately 300 km west off Portugal [IMAGES core MD01-2446: 39°03'N, 12°37'W, 3547 m water depth] was conducted within the AMOCINT project (ESF-EUROCORES programme, 06-EuroMARC-FP-008). Even though siliceous productivity is expectedly low for oceanic regions, it shows a robust and consistent pattern with increased values during cold phases of MIS 5, and during the glacial stages 4 and 6 suggesting higher nutrient availability, during these periods. The same pattern is observed for MIS2 and the last deglaciation. The opal record is fully supported by the organic carbon content and to the estimated productivity using foraminifera based FA20 and SIMMAX.28 transfer functions for a near location. The benthic δ13C record suggests less North Atlantic Deep Water (NADW) coincident with periods of higher productivity. The grain

  10. Enhanced open ocean storage of CO2 from shelf sea pumping.

    PubMed

    Thomas, Helmuth; Bozec, Yann; Elkalay, Khalid; de Baar, Hein J W

    2004-05-14

    Seasonal field observations show that the North Sea, a Northern European shelf sea, is highly efficient in pumping carbon dioxide from the atmosphere to the North Atlantic Ocean. The bottom topography-controlled stratification separates production and respiration processes in the North Sea, causing a carbon dioxide increase in the subsurface layer that is ultimately exported to the North Atlantic Ocean. Globally extrapolated, the net uptake of carbon dioxide by coastal and marginal seas is about 20% of the world ocean's uptake of anthropogenic carbon dioxide, thus enhancing substantially the open ocean carbon dioxide storage.

  11. Extreme diversity in noncalcifying haptophytes explains a major pigment paradox in open oceans

    PubMed Central

    Liu, Hui; Probert, Ian; Uitz, Julia; Claustre, Hervé; Aris-Brosou, Stéphane; Frada, Miguel; Not, Fabrice; de Vargas, Colomban

    2009-01-01

    The current paradigm holds that cyanobacteria, which evolved oxygenic photosynthesis more than 2 billion years ago, are still the major light harvesters driving primary productivity in open oceans. Here we show that tiny unicellular eukaryotes belonging to the photosynthetic lineage of the Haptophyta are dramatically diverse and ecologically dominant in the planktonic photic realm. The use of Haptophyta-specific primers and PCR conditions adapted for GC-rich genomes circumvented biases inherent in classical genetic approaches to exploring environmental eukaryotic biodiversity and led to the discovery of hundreds of unique haptophyte taxa in 5 clone libraries from subpolar and subtropical oceanic waters. Phylogenetic analyses suggest that this diversity emerged in Paleozoic oceans, thrived and diversified in the permanently oxygenated Mesozoic Panthalassa, and currently comprises thousands of ribotypic species, belonging primarily to low-abundance and ancient lineages of the “rare biosphere.” This extreme biodiversity coincides with the pervasive presence in the photic zone of the world ocean of 19′-hexanoyloxyfucoxanthin (19-Hex), an accessory photosynthetic pigment found exclusively in chloroplasts of haptophyte origin. Our new estimates of depth-integrated relative abundance of 19-Hex indicate that haptophytes dominate the chlorophyll a-normalized phytoplankton standing stock in modern oceans. Their ecologic and evolutionary success, arguably based on mixotrophy, may have significantly impacted the oceanic carbon pump. These results add to the growing evidence that the evolution of complex microbial eukaryotic cells is a critical force in the functioning of the biosphere. PMID:19622724

  12. Extreme diversity in noncalcifying haptophytes explains a major pigment paradox in open oceans.

    PubMed

    Liu, Hui; Probert, Ian; Uitz, Julia; Claustre, Hervé; Aris-Brosou, Stéphane; Frada, Miguel; Not, Fabrice; de Vargas, Colomban

    2009-08-04

    The current paradigm holds that cyanobacteria, which evolved oxygenic photosynthesis more than 2 billion years ago, are still the major light harvesters driving primary productivity in open oceans. Here we show that tiny unicellular eukaryotes belonging to the photosynthetic lineage of the Haptophyta are dramatically diverse and ecologically dominant in the planktonic photic realm. The use of Haptophyta-specific primers and PCR conditions adapted for GC-rich genomes circumvented biases inherent in classical genetic approaches to exploring environmental eukaryotic biodiversity and led to the discovery of hundreds of unique haptophyte taxa in 5 clone libraries from subpolar and subtropical oceanic waters. Phylogenetic analyses suggest that this diversity emerged in Paleozoic oceans, thrived and diversified in the permanently oxygenated Mesozoic Panthalassa, and currently comprises thousands of ribotypic species, belonging primarily to low-abundance and ancient lineages of the "rare biosphere." This extreme biodiversity coincides with the pervasive presence in the photic zone of the world ocean of 19'-hexanoyloxyfucoxanthin (19-Hex), an accessory photosynthetic pigment found exclusively in chloroplasts of haptophyte origin. Our new estimates of depth-integrated relative abundance of 19-Hex indicate that haptophytes dominate the chlorophyll a-normalized phytoplankton standing stock in modern oceans. Their ecologic and evolutionary success, arguably based on mixotrophy, may have significantly impacted the oceanic carbon pump. These results add to the growing evidence that the evolution of complex microbial eukaryotic cells is a critical force in the functioning of the biosphere.

  13. Fresh Water Content Variability in the Arctic Ocean

    NASA Technical Reports Server (NTRS)

    Hakkinen, Sirpa; Proshutinsky, Andrey

    2003-01-01

    Arctic Ocean model simulations have revealed that the Arctic Ocean has a basin wide oscillation with cyclonic and anticyclonic circulation anomalies (Arctic Ocean Oscillation; AOO) which has a prominent decadal variability. This study explores how the simulated AOO affects the Arctic Ocean stratification and its relationship to the sea ice cover variations. The simulation uses the Princeton Ocean Model coupled to sea ice. The surface forcing is based on NCEP-NCAR Reanalysis and its climatology, of which the latter is used to force the model spin-up phase. Our focus is to investigate the competition between ocean dynamics and ice formation/melt on the Arctic basin-wide fresh water balance. We find that changes in the Atlantic water inflow can explain almost all of the simulated fresh water anomalies in the main Arctic basin. The Atlantic water inflow anomalies are an essential part of AOO, which is the wind driven barotropic response to the Arctic Oscillation (AO). The baroclinic response to AO, such as Ekman pumping in the Beaufort Gyre, and ice meldfreeze anomalies in response to AO are less significant considering the whole Arctic fresh water balance.

  14. Variations of the Organic Matter Composition in the Sea Surface Microlayer: A Comparison between Open Ocean, Coastal, and Upwelling Sites Off the Peruvian Coast

    PubMed Central

    Zäncker, Birthe; Bracher, Astrid; Röttgers, Rüdiger; Engel, Anja

    2017-01-01

    The sea surface microlayer (SML) is the thin boundary layer between the ocean and the atmosphere, making it important for air-sea exchange processes. However, little is known about what controls organic matter composition in the SML. In particular, there are only few studies available on the differences of the SML of various oceanic systems. Here, we compared the organic matter and neuston species composition in the SML and the underlying water (ULW) at 11 stations with varying distance from the coast in the Peruvian upwelling regime, a system with high emissions of climate relevant trace gases, such as N2O and CO2. In the open ocean, organic carbon, and amino acids were highly enriched in the SML compared to the ULW. The enrichment decreased at the coastal stations and vanished in the upwelling regime. At the same time, the degradation of organic matter increased from the open ocean to the upwelling stations. This suggests that in the open ocean, upward transport processes or new production of organic matter within the SML are faster than degradation processes. Phytoplankton was generally not enriched in the SML, one group though, the Trichodesmium-like TrL (possibly containing Trichodesmium), were enriched in the open ocean but not in the upwelling region indicating that they find a favorable habitat in the open ocean SML. Our data show that the SML is a distinct habitat; its composition is more similar among different systems than between SML and ULW of a single station. Generally the enrichment of organic matter is assumed to be reduced when encountering low primary production and high wind speeds. However, our study shows the highest enrichments of organic matter in the open ocean which had the lowest primary production and the highest wind speeds. PMID:29375483

  15. Variations of the Organic Matter Composition in the Sea Surface Microlayer: A Comparison between Open Ocean, Coastal, and Upwelling Sites Off the Peruvian Coast.

    PubMed

    Zäncker, Birthe; Bracher, Astrid; Röttgers, Rüdiger; Engel, Anja

    2017-01-01

    The sea surface microlayer (SML) is the thin boundary layer between the ocean and the atmosphere, making it important for air-sea exchange processes. However, little is known about what controls organic matter composition in the SML. In particular, there are only few studies available on the differences of the SML of various oceanic systems. Here, we compared the organic matter and neuston species composition in the SML and the underlying water (ULW) at 11 stations with varying distance from the coast in the Peruvian upwelling regime, a system with high emissions of climate relevant trace gases, such as N 2 O and CO 2 . In the open ocean, organic carbon, and amino acids were highly enriched in the SML compared to the ULW. The enrichment decreased at the coastal stations and vanished in the upwelling regime. At the same time, the degradation of organic matter increased from the open ocean to the upwelling stations. This suggests that in the open ocean, upward transport processes or new production of organic matter within the SML are faster than degradation processes. Phytoplankton was generally not enriched in the SML, one group though, the Trichodesmium -like TrL (possibly containing Trichodesmium ), were enriched in the open ocean but not in the upwelling region indicating that they find a favorable habitat in the open ocean SML. Our data show that the SML is a distinct habitat; its composition is more similar among different systems than between SML and ULW of a single station. Generally the enrichment of organic matter is assumed to be reduced when encountering low primary production and high wind speeds. However, our study shows the highest enrichments of organic matter in the open ocean which had the lowest primary production and the highest wind speeds.

  16. Changing carbonate chemistry in ocean waters surrounding coral reefs in the CMIP5 ensemble

    NASA Astrophysics Data System (ADS)

    Ricke, K.; Schneider, K.; Cao, L.; Caldeira, K.

    2012-12-01

    Coral reefs comprise some of the most biodiverse ecosystems in the world. Today they are threatened by a number of stressors, including pollution, bleaching from global warming and ocean acidification. In this study, we focus on the implications of ocean acidification for the open ocean chemistry surrounding coral reefs. We use results from 13 Earth System Models included in the Coupled Model Intercomparison Project 5 (CMIP5) to examine the changing aragonite saturations (Ωa) of open ocean waters surrounding approximately 6,000 coral reefs. These 13 Earth System Models participating in CMIP5 each have interactive ocean biogeochemistry models that output state variables including DIC, alkalinity, SST, and salinity. Variation in these values were combined with values from the GLODAP database to calculate aragonite, the form of calcium carbonate that corals use to make their skeletons. We used reef locations from ReefBase that were within one degree (in latitude or longitude) of water masses represented both in the GLODAP database and in the climate models. Carbonate chemistry calculations were performed by Dr. James C. Orr (IPSL) as part of a separate study. We find that in preindustrial times, 99.9 % of coral reefs were located in regions of the ocean with aragonite saturations of 3.5 or more. The saturation threshold for viable reef ecosystems in uncertain, but the pre-industrial distribution of water chemistry surrounding coral reefs may nevertheless provide some indication of viability. We examine the fate of coral reefs in the context of several potential aragonite saturation thresholds, i.e., when Ωa_crit equals 3, 3.25, or 3.5. We show that under a business-as-usual scenario Representative Concentration Pathway (RCP) 8.5, the specific value of Ωa_crit does not affect the long-term fate of coral reefs -- by the end of the 21st century, no coral reef considered is surrounded by water with Ωa> 3. However, under scenarios with significant CO2 emissions

  17. OpenDrift - an open source framework for ocean trajectory modeling

    NASA Astrophysics Data System (ADS)

    Dagestad, Knut-Frode; Breivik, Øyvind; Ådlandsvik, Bjørn

    2016-04-01

    We will present a new, open source tool for modeling the trajectories and fate of particles or substances (Lagrangian Elements) drifting in the ocean, or even in the atmosphere. The software is named OpenDrift, and has been developed at Norwegian Meteorological Institute in cooperation with Institute of Marine Research. OpenDrift is a generic framework written in Python, and is openly available at https://github.com/knutfrode/opendrift/. The framework is modular with respect to three aspects: (1) obtaining input data, (2) the transport/morphological processes, and (3) exporting of results to file. Modularity is achieved through well defined interfaces between components, and use of a consistent vocabulary (CF conventions) for naming of variables. Modular input implies that it is not necessary to preprocess input data (e.g. currents, wind and waves from Eulerian models) to a particular file format. Instead "reader modules" can be written/used to obtain data directly from any original source, including files or through web based protocols (e.g. OPeNDAP/Thredds). Modularity of processes implies that a model developer may focus on the geophysical processes relevant for the application of interest, without needing to consider technical tasks such as reading, reprojecting, and colocating input data, rotation and scaling of vectors and model output. We will show a few example applications of using OpenDrift for predicting drifters, oil spills, and search and rescue objects.

  18. Open science resources for the discovery and analysis of Tara Oceans data

    NASA Astrophysics Data System (ADS)

    2015-05-01

    The Tara Oceans expedition (2009-2013) sampled contrasting ecosystems of the world oceans, collecting environmental data and plankton, from viruses to metazoans, for later analysis using modern sequencing and state-of-the-art imaging technologies. It surveyed 210 ecosystems in 20 biogeographic provinces, collecting over 35,000 samples of seawater and plankton. The interpretation of such an extensive collection of samples in their ecological context requires means to explore, assess and access raw and validated data sets. To address this challenge, the Tara Oceans Consortium offers open science resources, including the use of open access archives for nucleotides (ENA) and for environmental, biogeochemical, taxonomic and morphological data (PANGAEA), and the development of on line discovery tools and collaborative annotation tools for sequences and images. Here, we present an overview of Tara Oceans Data, and we provide detailed registries (data sets) of all campaigns (from port-to-port), stations and sampling events.

  19. Open science resources for the discovery and analysis of Tara Oceans data.

    PubMed

    Pesant, Stéphane; Not, Fabrice; Picheral, Marc; Kandels-Lewis, Stefanie; Le Bescot, Noan; Gorsky, Gabriel; Iudicone, Daniele; Karsenti, Eric; Speich, Sabrina; Troublé, Romain; Dimier, Céline; Searson, Sarah

    2015-01-01

    The Tara Oceans expedition (2009-2013) sampled contrasting ecosystems of the world oceans, collecting environmental data and plankton, from viruses to metazoans, for later analysis using modern sequencing and state-of-the-art imaging technologies. It surveyed 210 ecosystems in 20 biogeographic provinces, collecting over 35,000 samples of seawater and plankton. The interpretation of such an extensive collection of samples in their ecological context requires means to explore, assess and access raw and validated data sets. To address this challenge, the Tara Oceans Consortium offers open science resources, including the use of open access archives for nucleotides (ENA) and for environmental, biogeochemical, taxonomic and morphological data (PANGAEA), and the development of on line discovery tools and collaborative annotation tools for sequences and images. Here, we present an overview of Tara Oceans Data, and we provide detailed registries (data sets) of all campaigns (from port-to-port), stations and sampling events.

  20. Fluxes of Ethanol Between the Atmosphere and Oceanic Surface Waters; Implications for the Fate of Biofuel Ethanol Released into the Environment

    NASA Astrophysics Data System (ADS)

    Avery, G. B., Jr.; Shimizu, M. S.; Willey, J. D.; Mead, R. N.; Skrabal, S. A.; Kieber, R. J.; Lathrop, T. E.; Felix, J. D. D.

    2017-12-01

    The use of ethanol as a transportation fuel has increased significantly during the past decade in the US. Some ethanol escapes the combustion process in internal combustion engines resulting in its release to the atmosphere. Ethanol can be oxidized photochemically to acetaldehyde and then converted to peroxyacetyl nitrate contributing to air pollution. Therefore it is important to determine the fate ethanol released to the atmosphere. Because of its high water solubility the oceans may act as a sink for ethanol depending on its state of saturation with respect to the gas phase. The purpose of the current study was to determine the relative saturation of oceanic surface waters by making simultaneous measurements of gas phase and surface water concentrations. Data were obtained from four separate cruises ranging from estuarine to open ocean locations in the coast of North Carolina, USA. The majority of estuarine sites were under saturated in ethanol with respect to the gas phase (11-50% saturated) representing a potential sink. Coastal surface waters tended to be supersaturated (135 - 317%) representing a net flux of ethanol to the atmosphere. Open ocean samples were generally at saturation or slightly below saturation (76-99%) indicating equilibrium between the gas and aqueous phases. The results of this study underscore to variable role the oceans play in mitigating the increases in atmospheric ethanol from increased biofuel usage and their impact on air quality.

  1. Spacebased Observation of Water Balance Over Global Oceans

    NASA Astrophysics Data System (ADS)

    Liu, W.; Xie, X.

    2008-12-01

    We demonstrated that ocean surface fresh water flux less the water discharge into the ocean from river and ice melt balances the mass loss in the ocean both in magnitude and in the phase of annual variation. The surface water flux was computed from the divergence of the water transport integrated over the depth of the atmosphere. The atmospheric water transport is estimated from the precipitable water measured by Special Sensor Microwave Imager, the surface wind vector by QuikSCAT, and the NOAA cloud drift wind through a statistical model. The transport has been extensively validated using global radiosonde and data and operational numerical weather prediction results. Its divergence has been shown to agree with the difference between evaporation estimated from the Advanced Microwave Scanning Radiometer data and the precipitation measured by Tropical Rain Measuring Mission over the global tropical and subtropical oceans both in magnitude and geographical distribution for temporal scales ranging from intraseasonal to interannual. The water loss rate in the ocean is estimated by two methods, one is from Gravity Recovery and Climate Experiment and the other is by subtracting the climatological steric change from the sea level change measured by radar altimeter on Jason. Only climatological river discharge and ice melt from in situ measurements are available and the lack of temporal variation may contribute to discrepancies in the balance. We have successfully used the spacebased surface fluxes to estimate to climatological mean heat transport in the Atlantic ocean and is attempting to estimate the meridional fresh water (or salt) transport from the surface flux. The approximate closure of the water balance gives a powerful indirect validation of the spacebased products.

  2. Vicariance biogeography of the open-ocean Pacific

    NASA Astrophysics Data System (ADS)

    White, Brian N.

    The first cladogram to treat oceanic water masses as distinct geographic units presents a ‘hydrotectonic’ history of Pacific surface water masses. It is used to test the idea that the oceanographic subdivision of the surface waters of the Pacific Basin into separate water masses shaped pelagic biogeographic patterns in much the same way that the tectonic fragmentation of Pangea influenced biogeographic patterns on land. The historical water-mass relationships depicted by the surface water-mass cladogram resemble modern pelagic biogeographic regions. The prediction that the cladistic phylogenies of monophyletic groups having allopatric taxa in three or more surface water masses will be consistent with the topology of the surface water-mass cladogram is met by the pelagic fish genera Stomias and Evermanella.

  3. Water-leaving contribution to polarized radiation field over ocean.

    PubMed

    Zhai, Peng-Wang; Knobelspiesse, Kirk; Ibrahim, Amir; Franz, Bryan A; Hu, Yongxiang; Gao, Meng; Frouin, Robert

    2017-08-07

    The top-of-atmosphere (TOA) radiation field from a coupled atmosphere-ocean system (CAOS) includes contributions from the atmosphere, surface, and water body. Atmospheric correction of ocean color imagery is to retrieve water-leaving radiance from the TOA measurement, from which ocean bio-optical properties can be obtained. Knowledge of the absolute and relative magnitudes of water-leaving signal in the TOA radiation field is important for designing new atmospheric correction algorithms and developing retrieval algorithms for new ocean biogeochemical parameters. In this paper we present a systematic sensitivity study of water-leaving contribution to the TOA radiation field, from 340 nm to 865 nm, with polarization included. Ocean water inherent optical properties are derived from bio-optical models for two kinds of waters, one dominated by phytoplankton (PDW) and the other by non-algae particles (NDW). In addition to elastic scattering, Raman scattering and fluorescence from dissolved organic matter in ocean waters are included. Our sensitivity study shows that the polarized reflectance is minimized for both CAOS and ocean signals in the backscattering half plane, which leads to numerical instability when calculating water leaving relative contribution, the ratio between polarized water leaving and CAOS signals. If the backscattering plane is excluded, the water-leaving polarized signal contributes less than 9% to the TOA polarized reflectance for PDW in the whole spectra. For NDW, the polarized water leaving contribution can be as much as 20% in the wavelength range from 470 to 670 nm. For wavelengths shorter than 452 nm or longer than 865 nm, the water leaving contribution to the TOA polarized reflectance is in general smaller than 5% for NDW. For the TOA total reflectance, the water-leaving contribution has maximum values ranging from 7% to 16% at variable wavelengths from 400 nm to 550 nm from PDW. The water leaving contribution to the TOA total reflectance can

  4. Water-Leaving Contribution to Polarized Radiation Field Over Ocean

    NASA Technical Reports Server (NTRS)

    Zhai, Peng-Wang; Knobelspiesse, Kirk D.; Ibrahim, Amir; Franz, Bryan A.; Hu, Yongxiang; Gao, Meng; Frouin, Robert

    2017-01-01

    The top-of-atmosphere (TOA) radiation field from a coupled atmosphere-ocean system (CAOS) includes contributions from the atmosphere, surface, and water body. Atmo-spheric correction of ocean color imagery is to retrieve water-leaving radiance from the TOA measurement, from which ocean bio-optical properties can be obtained. Knowledge of the ab-solute and relative magnitudes of water-leaving signal in the TOA radiation field is important for designing new atmospheric correction algorithms and developing retrieval algorithms for new ocean biogeochemical parameters. In this paper we present a systematic sensitivity study of water-leaving contribution to the TOA radiation field, from 340 nm to 865 nm, with polarization included. Ocean water inherent optical properties are derived from bio-optical models for two kinds of waters, one dominated by phytoplankton (PDW) and the other by non-algae particles (NDW). In addition to elastic scattering, Raman scattering and fluorescence from dissolved organic matter in ocean waters are included. Our sensitivity study shows that the polarized reflectance is minimized for both CAOS and ocean signals in the backscattering half plane, which leads to numerical instability when calculating water leaving relative contribution, the ratio between polarized water leaving and CAOS signals. If the backscattering plane is excluded, the water-leaving polarized signal contributes less than 9% to the TOA polarized reflectance for PDW in the whole spectra. For NDW, the polarized water leaving contribution can be as much as 20% in the wavelength range from 470 to 670 nm. For wavelengths shorter than 452 nm or longer than 865 nm, the water leaving contribution to the TOA polarized reflectance is in general smaller than 5% for NDW. For the TOA total reflectance, the water-leaving contribution has maximum values ranging from 7% to 16% at variable wavelengths from 400 nm to 550 nm from PDW. The water leaving contribution to the TOA total reflectance

  5. Open science resources for the discovery and analysis of Tara Oceans data

    PubMed Central

    Pesant, Stéphane; Not, Fabrice; Picheral, Marc; Kandels-Lewis, Stefanie; Le Bescot, Noan; Gorsky, Gabriel; Iudicone, Daniele; Karsenti, Eric; Speich, Sabrina; Troublé, Romain; Dimier, Céline; Searson, Sarah; Acinas, Silvia G.; Bork, Peer; Boss, Emmanuel; Bowler, Chris; Vargas, Colomban De; Follows, Michael; Gorsky, Gabriel; Grimsley, Nigel; Hingamp, Pascal; Iudicone, Daniele; Jaillon, Olivier; Kandels-Lewis, Stefanie; Karp-Boss, Lee; Karsenti, Eric; Krzic, Uros; Not, Fabrice; Ogata, Hiroyuki; Pesant, Stéphane; Raes, Jeroen; Reynaud, Emmanuel G.; Sardet, Christian; Sieracki, Mike; Speich, Sabrina; Stemmann, Lars; Sullivan, Matthew B.; Sunagawa, Shinichi; Velayoudon, Didier; Weissenbach, Jean; Wincker, Patrick

    2015-01-01

    The Tara Oceans expedition (2009–2013) sampled contrasting ecosystems of the world oceans, collecting environmental data and plankton, from viruses to metazoans, for later analysis using modern sequencing and state-of-the-art imaging technologies. It surveyed 210 ecosystems in 20 biogeographic provinces, collecting over 35,000 samples of seawater and plankton. The interpretation of such an extensive collection of samples in their ecological context requires means to explore, assess and access raw and validated data sets. To address this challenge, the Tara Oceans Consortium offers open science resources, including the use of open access archives for nucleotides (ENA) and for environmental, biogeochemical, taxonomic and morphological data (PANGAEA), and the development of on line discovery tools and collaborative annotation tools for sequences and images. Here, we present an overview of Tara Oceans Data, and we provide detailed registries (data sets) of all campaigns (from port-to-port), stations and sampling events. PMID:26029378

  6. Atlantic Water Advection and Ice Sheet-Ocean Feedbacks in the Arctic Ocean During the Last 200 ky

    NASA Astrophysics Data System (ADS)

    Spielhagen, R. F.; Mackensen, A.; Stein, R. H.

    2016-12-01

    Earlier work on Arctic deep-sea cores from the eastern Lomonosov Ridge and the Morris Jesup Rise had revealed that large-scale Eurasian ice sheet growth was initiated at times with seasonally open waters in the Arctic Ocean, indicating a role for the ocean in nearby ice sheet development in the last 200 ky. Here we present microfossil and geochemical data from new sediment cores obtained from the western and easternmost Lomonosov Ridge during the PS87 expedition (2014) of RV Polarstern, amended by data from refined analyses of the older cores. They allow to investigate in more detail the feedbacks between Atlantic Water (AW) advection, sea ice, and ice sheets. In all cores, high microfossil abundances are found just below layers rich in iceberg-rafted detritus, supporting the hypothesis of Arctic Ocean moisture supply for the growth of Eurasian ice sheets. On the other hand, the new microfaunal results suggest that the decay of the ice sheets and the enhanced freshwater discharge to the Arctic may have influenced the routing of subsurface AW in the Arctic Ocean, at least during marine isotope (sub)stages (MIS) 5a and 5e. In the early part of these relatively mild climatic intervals, faunal and isotopic data suggest a noticable advection of Atlantic Water, yet of rather low temperature and likely at depths comparable to the modern distribution (i.e., below 150 m) or even deeper. This may be explained by a more southerly position of AW cooling and submergence than today, caused by a thick layer of low saline waters near the surface which stemmed from the slow melting of ice sheet remnants on the Eurasian continent and shelves. In the second half of both MIS 5a and 5e, AW advection was significantly stronger and may have occurred at shallower depths, as indicated by unusually large amounts of small subpolar planktic foraminifers in central Arctic sediments. AW was apparently diverted northward from the Fram Strait and spread eastward along the Lomonosov Ridge. A

  7. Water Partitioning in Planetary Embryos and Protoplanets with Magma Oceans

    NASA Astrophysics Data System (ADS)

    Ikoma, M.; Elkins-Tanton, L.; Hamano, K.; Suckale, J.

    2018-06-01

    The water content of magma oceans is widely accepted as a key factor that determines whether a terrestrial planet is habitable. Water ocean mass is determined as a result not only of water delivery and loss, but also of water partitioning among several reservoirs. Here we review our current understanding of water partitioning among the atmosphere, magma ocean, and solid mantle of accreting planetary embryos and protoplanets just after giant collisions. Magma oceans are readily formed in planetary embryos and protoplanets in their accretion phase. Significant amounts of water are partitioned into magma oceans, provided the planetary building blocks are water-rich enough. Particularly important but still quite uncertain issues are how much water the planetary building blocks contain initially and how water goes out of the solidifying mantle and is finally degassed to the atmosphere. Constraints from both solar-system explorations and exoplanet observations and also from laboratory experiments are needed to resolve these issues.

  8. Paleobathymetric grids of the Cenozoic Southern Ocean - Opening the door towards improved reconstructions of the Southern Ocean's past

    NASA Astrophysics Data System (ADS)

    Hochmuth, K.; Gohl, K.; Leitchenkov, G. L.; Sauermilch, I.; Whittaker, J. M.; De Santis, L.; Olivo, E.; Uenzelmann-Neben, G.; Davy, B. W.

    2017-12-01

    volumes open the door towards more sophisticated paleo-topograpy studies of the Antarctic continent and more detailed studies of the paleo-circulation. Local paleo - water depths at the oceanic gateways or the position of paleo-shelf edges highly influence the regional circulation patterns supporting more elaborated climate models.

  9. Impacts of atmospheric anthropogenic nitrogen on the open ocean.

    PubMed

    Duce, R A; LaRoche, J; Altieri, K; Arrigo, K R; Baker, A R; Capone, D G; Cornell, S; Dentener, F; Galloway, J; Ganeshram, R S; Geider, R J; Jickells, T; Kuypers, M M; Langlois, R; Liss, P S; Liu, S M; Middelburg, J J; Moore, C M; Nickovic, S; Oschlies, A; Pedersen, T; Prospero, J; Schlitzer, R; Seitzinger, S; Sorensen, L L; Uematsu, M; Ulloa, O; Voss, M; Ward, B; Zamora, L

    2008-05-16

    Increasing quantities of atmospheric anthropogenic fixed nitrogen entering the open ocean could account for up to about a third of the ocean's external (nonrecycled) nitrogen supply and up to approximately 3% of the annual new marine biological production, approximately 0.3 petagram of carbon per year. This input could account for the production of up to approximately 1.6 teragrams of nitrous oxide (N2O) per year. Although approximately 10% of the ocean's drawdown of atmospheric anthropogenic carbon dioxide may result from this atmospheric nitrogen fertilization, leading to a decrease in radiative forcing, up to about two-thirds of this amount may be offset by the increase in N2O emissions. The effects of increasing atmospheric nitrogen deposition are expected to continue to grow in the future.

  10. Open ocean Internal Waves, Namibia Coast, Africa.

    NASA Technical Reports Server (NTRS)

    1990-01-01

    These open ocean Internal Waves were seen off the Namibia Coast, Africa (19.5S, 11.5E). The periodic and regularly spaced sets of incoming internal appear to be diffracting against the coastline and recombining to form a network of interference patterns. They seem to coincide with tidal periods about 12 hours apart and wave length (distance from crest to crest) varies between 1.5 and 5.0 miles and the crest lengths stretch beyond the image.

  11. Open ocean Internal Waves, Namibia Coast, Africa.

    NASA Image and Video Library

    1990-12-10

    These open ocean Internal Waves were seen off the Namibia Coast, Africa (19.5S, 11.5E). The periodic and regularly spaced sets of incoming internal appear to be diffracting against the coastline and recombining to form a network of interference patterns. They seem to coincide with tidal periods about 12 hours apart and wave length (distance from crest to crest) varies between 1.5 and 5.0 miles and the crest lengths stretch beyond the image.

  12. Open ocean Internal Waves, Namibia Coast, Africa.

    NASA Image and Video Library

    1990-12-10

    These open ocean Internal Waves were seen off the Namibia Coast, Africa (23.0S, 14.0E). The periodic and regularly spaced sets of internal waves most likely coincide with tidal periods about 12 hours apart. The wave length (distance from crest to crest) varies between 1.5 and 5.0 miles and the crest lengths stretch across and beyond the distance of the photo. The waves are intersecting the Namibia coastline at about a 30 degree angle.

  13. Open ocean Internal Waves, Namibia Coast, Africa.

    NASA Technical Reports Server (NTRS)

    1990-01-01

    These open ocean Internal Waves were seen off the Namibia Coast, Africa (23.0S, 14.0E). The periodic and regularly spaced sets of internal waves most likely coincide with tidal periods about 12 hours apart. The wave length (distance from crest to crest) varies between 1.5 and 5.0 miles and the crest lengths stretch across and beyond the distance of the photo. The waves are intersecting the Namibia coastline at about a 30 degree angle.

  14. Variation pattern of particulate organic carbon and nitrogen in oceans and inland waters

    NASA Astrophysics Data System (ADS)

    Huang, Changchun; Jiang, Quanliang; Yao, Ling; Yang, Hao; Lin, Chen; Huang, Tao; Zhu, A.-Xing; Zhang, Yimin

    2018-03-01

    We examined the relationship between, and variations in, particulate organic carbon (POC) and particulate organic nitrogen (PON) based on previously acquired ocean and inland water data. The latitudinal dependency of POC / PON is significant between 20 and 90° N but weak in low-latitude areas and in the Southern Hemisphere. The mean values of POC / PON in the Southern Hemisphere and Northern Hemisphere were 7.40 ± 3.83 and 7.80 ± 3.92, respectively. High values of POC / PON appeared between 80-90 (12.2 ± 7.5) and 70-80° N (9.4 ± 6.4), while relatively low POC / PON was found from 20 (6.6 ± 2.8) to 40° N (6.7 ± 2.7). The latitudinal variation of POC / PON in the Northern Hemisphere is much stronger than in the Southern Hemisphere due to the influence of more terrestrial organic matter. Higher POC and PON could be expected in coastal waters. POC / PON growth ranged from 6.89 ± 2.38 to 7.59 ± 4.22 in the Northern Hemisphere, with an increasing rate of 0.0024 km from the coastal to open ocean. Variations of POC / PON in lake water also showed a similar latitude-variation tendency of POC / PON with ocean water but were significantly regulated by the lakes' morphology, trophic state and climate. Small lakes and high-latitude lakes prefer relatively high POC / PON, and large lakes and low-latitude lakes tend to prefer low POC / PON. The coupling relationship between POC and PON in oceans is much stronger than in inland waters. Variations in POC, PON and POC / PON in inland waters should receive more attention due to the implications of these values for the global carbon and nitrogen cycles and the indeterminacy of the relationship between POC and PON.

  15. The growth of finfish in global open-ocean aquaculture under climate change.

    PubMed

    Klinger, Dane H; Levin, Simon A; Watson, James R

    2017-10-11

    Aquaculture production is projected to expand from land-based operations to the open ocean as demand for seafood grows and competition increases for inputs to land-based aquaculture, such as freshwater and suitable land. In contrast to land-based production, open-ocean aquaculture is constrained by oceanographic factors, such as current speeds and seawater temperature, which are dynamic in time and space, and cannot easily be controlled. As such, the potential for offshore aquaculture to increase seafood production is tied to the physical state of the oceans. We employ a novel spatial model to estimate the potential of open-ocean finfish aquaculture globally, given physical, biological and technological constraints. Finfish growth potential for three common aquaculture species representing different thermal guilds-Atlantic salmon ( Salmo salar ), gilthead seabream ( Sparus aurata ) and cobia ( Rachycentron canadum )-is compared across species and regions and with climate change, based on outputs of a high-resolution global climate model. Globally, there are ample areas that are physically suitable for fish growth and potential expansion of the nascent aquaculture industry. The effects of climate change are heterogeneous across species and regions, but areas with existing aquaculture industries are likely to see increases in growth rates. In areas where climate change results in reduced growth rates, adaptation measures, such as selective breeding, can probably offset potential production losses. © 2017 The Author(s).

  16. The symbiotic life of Symbiodinium in the open ocean within a new species of calcifying ciliate (Tiarina sp.).

    PubMed

    Mordret, Solenn; Romac, Sarah; Henry, Nicolas; Colin, Sébastien; Carmichael, Margaux; Berney, Cédric; Audic, Stéphane; Richter, Daniel J; Pochon, Xavier; de Vargas, Colomban; Decelle, Johan

    2016-06-01

    Symbiotic partnerships between heterotrophic hosts and intracellular microalgae are common in tropical and subtropical oligotrophic waters of benthic and pelagic marine habitats. The iconic example is the photosynthetic dinoflagellate genus Symbiodinium that establishes mutualistic symbioses with a wide diversity of benthic hosts, sustaining highly biodiverse reef ecosystems worldwide. Paradoxically, although various species of photosynthetic dinoflagellates are prevalent eukaryotic symbionts in pelagic waters, Symbiodinium has not yet been reported in symbiosis within oceanic plankton, despite its high propensity for the symbiotic lifestyle. Here we report a new pelagic photosymbiosis between a calcifying ciliate host and the microalga Symbiodinium in surface ocean waters. Confocal and scanning electron microscopy, together with an 18S rDNA-based phylogeny, showed that the host is a new ciliate species closely related to Tiarina fusus (Colepidae). Phylogenetic analyses of the endosymbionts based on the 28S rDNA gene revealed multiple novel closely related Symbiodinium clade A genotypes. A haplotype network using the high-resolution internal transcribed spacer-2 marker showed that these genotypes form eight divergent, biogeographically structured, subclade types that do not seem to associate with any benthic hosts. Ecological analyses using the Tara Oceans metabarcoding data set (V9 region of the 18S rDNA) and contextual oceanographic parameters showed a global distribution of the symbiotic partnership in nutrient-poor surface waters. The discovery of the symbiotic life of Symbiodinium in the open ocean provides new insights into the ecology and evolution of this pivotal microalga and raises new hypotheses about coastal pelagic connectivity.

  17. The symbiotic life of Symbiodinium in the open ocean within a new species of calcifying ciliate (Tiarina sp.)

    PubMed Central

    Mordret, Solenn; Romac, Sarah; Henry, Nicolas; Colin, Sébastien; Carmichael, Margaux; Berney, Cédric; Audic, Stéphane; Richter, Daniel J; Pochon, Xavier; de Vargas, Colomban; Decelle, Johan

    2016-01-01

    Symbiotic partnerships between heterotrophic hosts and intracellular microalgae are common in tropical and subtropical oligotrophic waters of benthic and pelagic marine habitats. The iconic example is the photosynthetic dinoflagellate genus Symbiodinium that establishes mutualistic symbioses with a wide diversity of benthic hosts, sustaining highly biodiverse reef ecosystems worldwide. Paradoxically, although various species of photosynthetic dinoflagellates are prevalent eukaryotic symbionts in pelagic waters, Symbiodinium has not yet been reported in symbiosis within oceanic plankton, despite its high propensity for the symbiotic lifestyle. Here we report a new pelagic photosymbiosis between a calcifying ciliate host and the microalga Symbiodinium in surface ocean waters. Confocal and scanning electron microscopy, together with an 18S rDNA-based phylogeny, showed that the host is a new ciliate species closely related to Tiarina fusus (Colepidae). Phylogenetic analyses of the endosymbionts based on the 28S rDNA gene revealed multiple novel closely related Symbiodinium clade A genotypes. A haplotype network using the high-resolution internal transcribed spacer-2 marker showed that these genotypes form eight divergent, biogeographically structured, subclade types that do not seem to associate with any benthic hosts. Ecological analyses using the Tara Oceans metabarcoding data set (V9 region of the 18S rDNA) and contextual oceanographic parameters showed a global distribution of the symbiotic partnership in nutrient-poor surface waters. The discovery of the symbiotic life of Symbiodinium in the open ocean provides new insights into the ecology and evolution of this pivotal microalga and raises new hypotheses about coastal pelagic connectivity. PMID:26684730

  18. Geoengineering impact of open ocean dissolution of olivine on atmospheric CO2, surface ocean pH and marine biology

    NASA Astrophysics Data System (ADS)

    Köhler, Peter; Abrams, Jesse F.; Völker, Christoph; Hauck, Judith; Wolf-Gladrow, Dieter A.

    2013-03-01

    Ongoing global warming induced by anthropogenic emissions has opened the debate as to whether geoengineering is a ‘quick fix’ option. Here we analyse the intended and unintended effects of one specific geoengineering approach, which is enhanced weathering via the open ocean dissolution of the silicate-containing mineral olivine. This approach would not only reduce atmospheric CO2 and oppose surface ocean acidification, but would also impact on marine biology. If dissolved in the surface ocean, olivine sequesters 0.28 g carbon per g of olivine dissolved, similar to land-based enhanced weathering. Silicic acid input, a byproduct of the olivine dissolution, alters marine biology because silicate is in certain areas the limiting nutrient for diatoms. As a consequence, our model predicts a shift in phytoplankton species composition towards diatoms, altering the biological carbon pumps. Enhanced olivine dissolution, both on land and in the ocean, therefore needs to be considered as ocean fertilization. From dissolution kinetics we calculate that only olivine particles with a grain size of the order of 1 μm sink slowly enough to enable a nearly complete dissolution. The energy consumption for grinding to this small size might reduce the carbon sequestration efficiency by ˜30%.

  19. The EuroSITES network: Integrating and enhancing fixed-point open ocean observatories around Europe

    NASA Astrophysics Data System (ADS)

    Lampitt, Richard S.; Larkin, Kate E.; EuroSITES Consortium

    2010-05-01

    EuroSITES is a 3 year (2008-2011) EU collaborative project (3.5MEuro) with the objective to integrate and enhance the nine existing open ocean fixed point observatories around Europe (www.eurosites.info). These observatories are primarily composed of full depth moorings and make multidisciplinary in situ observations within the water column as the European contribution to the global array OceanSITES (www.oceansites.org). In the first 18 months, all 9 observatories have been active and integration has been significant through the maintenance and enhancement of observatory hardware. Highlights include the enhancement of observatories with sensors to measure O2, pCO2, chlorophyll, and nitrate in near real-time from the upper 1000 m. In addition, some seafloor missions are also actively supported. These include seafloor platforms currently deployed in the Mediterranean, one for tsunami detection and one to monitor fluid flow related to seismic activity and slope stability. Upcoming seafloor science missions in 2010 include monitoring benthic biological communities and associated biogeochemistry as indicators of climate change in both the Northeast Atlantic and Mediterranean. EuroSITES also promotes the development of innovative sensors and samplers in order to progress capability to measure climate-relevant properties of the ocean. These include further developing current technologies for autonomous long-term monitoring of oxygen consumption in the mesopelagic, pH and mesozooplankton abundance. Many of these science missions are directly related to complementary activities in other European projects such as EPOCA, HYPOX and ESONET. In 2010 a direct collaboration including in situ field work will take place between ESONET and EuroSITES. The demonstration mission MODOO (funded by ESONET) will be implemented in 2010 at the EuroSITES PAP observatory. Field work will include deployment of a seafloor lander system with various sensors which will send data to shore in real

  20. Preconditioning and Formation Mechanisms of Maud Rise (Open Ocean) Polynyas in a High-Resolution CESM Simulation

    NASA Astrophysics Data System (ADS)

    Kurtakoti, P. K.; Veneziani, C.; Stoessel, A.; Weijer, W.

    2016-12-01

    Processes responsible for preconditioning and formation of Maud Rise Polynyas (MRP) were analyzed within the framework of a high-resolution fully coupled Community Earth System Model (CESM) simulation. Open Ocean Polynyas (OOPs) are large ice-free areas within the winter ice pack. These are regions of deep convection and strong atmosphere-ice-ocean interaction through which they play an important role in the formation of bottom waters. The data analyzed comes from a simulation conducted in a pre-industrial scenario as part of the Accelerated Climate Modeling for Energy (ACME) project. Within this simulation, persistent winter OOPs were simulated in the Weddell Sea (Weddell Sea Polynya) and over the Maud Rise seamount (Maud Rise Polynya). The sea ice concentration in the Weddell Sea shows that MRP acts as a precondition to Weddell Sea polynyas, which is consistent with mid 1970s observations of a westward expansion of MRP into the Weddell Sea. The OOPs in years 30-40 of the CESM simulation are largely over Maud Rise giving us an opportunity to investigate processes that trigger and maintain the OOP in winter over Maud Rise. The heat content of the Weddell Deep Water (WDW) is seen to be an important factor for MRPs, consistent with previous studies. The first MRP in the 30s coincides with the strongest negative wind stress curl over the Weddell Sea, which implies that this condition is a triggering mechanism for deep convection. The deep convective event associated with the OOP leads to a reduction of deep ocean heat reservoir up to 3000m depth. The simulation captures a westward flow of WDW impinging on Maud Rise seamount. Previous studies suggest Taylor column dynamics to be necessary for MRPs to emerge. We have explored how Taylor column dynamics could contribute to preconditioning and triggering deep open ocean convection over Maud Rise Seamount. We also investigate the importance of resolution of bottom topography for the formation of a strong enough Taylor

  1. Statistical Evaluation of VIIRS Ocean Color Products

    NASA Astrophysics Data System (ADS)

    Mikelsons, K.; Wang, M.; Jiang, L.

    2016-02-01

    Evaluation and validation of satellite-derived ocean color products is a complicated task, which often relies on precise in-situ measurements for satellite data quality assessment. However, in-situ measurements are only available in comparatively few locations, expensive, and not for all times. In the open ocean, the variability in spatial and temporal scales is longer, and the water conditions are generally more stable. We use this fact to perform extensive statistical evaluations of consistency for ocean color retrievals based on comparison of retrieved data at different times, and corresponding to various retrieval parameters. We have used the NOAA Multi-Sensor Level-1 to Level-2 (MSL12) ocean color data processing system for ocean color product data derived from the Visible Infrared Imaging Radiometer Suite (VIIRS). We show the results for statistical dependence of normalized water-leaving radiance spectra with respect to various parameters of retrieval geometry, such as solar- and sensor-zenith angles, as well as physical variables, such as wind speed, air pressure, ozone amount, water vapor, etc. In most cases, the results show consistent retrievals within the relevant range of retrieval parameters, showing a good performance with the MSL12 in the open ocean. The results also yield the upper bounds of solar- and sensor-zenith angles for reliable ocean color retrievals, and also show a slight increase of VIIRS-derived normalized water-leaving radiances with wind speed and water vapor concentration.

  2. Open Ocean Internal Waves, South China Sea

    NASA Technical Reports Server (NTRS)

    1989-01-01

    These open ocean internal waves were seen in the south China Sea (19.5N, 114.5E). These sets of internal waves most likely coincide with tidal periods about 12 hours apart. The wave length (distance from crest to crest) varies between 1.5 and 5.0 miles and the crest lengths stretch across and beyond this photo for over 75 miles. At lower right, the surface waves are moving at a 30% angle to the internal waves, with parallel low level clouds.

  3. Diurnal changes in ocean color in coastal waters

    NASA Astrophysics Data System (ADS)

    Arnone, Robert; Vandermeulen, Ryan; Ladner, Sherwin; Ondrusek, Michael; Kovach, Charles; Yang, Haoping; Salisbury, Joseph

    2016-05-01

    Coastal processes can change on hourly time scales in response to tides, winds and biological activity, which can influence the color of surface waters. These temporal and spatial ocean color changes require satellite validation for applications using bio-optical products to delineate diurnal processes. The diurnal color change and capability for satellite ocean color response were determined with in situ and satellite observations. Hourly variations in satellite ocean color are dependent on several properties which include: a) sensor characterization b) advection of water masses and c) diurnal response of biological and optical water properties. The in situ diurnal changes in ocean color in a dynamic turbid coastal region in the northern Gulf of Mexico were characterized using above water spectral radiometry from an AErosol RObotic NETwork (AERONET -WavCIS CSI-06) site that provides up to 8-10 observations per day (in 15-30 minute increments). These in situ diurnal changes were used to validate and quantify natural bio-optical fluctuations in satellite ocean color measurements. Satellite capability to detect changes in ocean color was characterized by using overlapping afternoon orbits of the VIIRS-NPP ocean color sensor within 100 minutes. Results show the capability of multiple satellite observations to monitor hourly color changes in dynamic coastal regions that are impacted by tides, re-suspension, and river plume dispersion. Hourly changes in satellite ocean color were validated with in situ observation on multiple occurrences during different times of the afternoon. Also, the spatial variability of VIIRS diurnal changes shows the occurrence and displacement of phytoplankton blooms and decay during the afternoon period. Results suggest that determining the temporal and spatial changes in a color / phytoplankton bloom from the morning to afternoon time period will require additional satellite coverage periods in the coastal zone.

  4. Trade Openness and Domestic Water Use

    NASA Astrophysics Data System (ADS)

    Dang, Qian; Konar, Megan

    2018-01-01

    We contribute to the debate over globalization and the environment by asking, what is the impact of trade on national water use? To address this question, we employ econometric methods to quantify the causal relationship between trade openness and water use. Specifically, we use the instrumental variables methodology to evaluate the impact of trade openness on domestic water withdrawals in agriculture and industry. We find that trade openness does not have a significant impact on total or industrial water withdrawals. However, we show that one percentage point increase in trade openness leads to a 5.21% decrease in agricultural water withdrawals. We find that trade openness reduces water use in agriculture primarily through the intensive margin effect, by leading farmers to produce more with less water, such as through the adoption of technology. We do not find evidence for extensive margin or crop mix impacts on agricultural water withdrawals. Significantly, these results demonstrate that trade openness leads to less water use in agriculture. This finding has broad scientific and policy relevance as we endeavor to untangle causal relationships in the complex global food system and develop policies to achieve water and food security.

  5. Global patterns of predator diversity in the open oceans.

    PubMed

    Worm, Boris; Sandow, Marcel; Oschlies, Andreas; Lotze, Heike K; Myers, Ransom A

    2005-08-26

    The open oceans comprise most of the biosphere, yet patterns and trends of species diversity there are enigmatic. Here, we derive worldwide patterns of tuna and billfish diversity over the past 50 years, revealing distinct subtropical "hotspots" that appeared to hold generally for other predators and zooplankton. Diversity was positively correlated with thermal fronts and dissolved oxygen and a nonlinear function of temperature (approximately 25 degrees C optimum). Diversity declined between 10 and 50% in all oceans, a trend that coincided with increased fishing pressure, superimposed on strong El Niño-Southern Oscillation-driven variability across the Pacific. We conclude that predator diversity shows a predictable yet eroding pattern signaling ecosystem-wide changes linked to climate and fishing.

  6. An alternative early opening scenario for the Central Atlantic Ocean

    NASA Astrophysics Data System (ADS)

    Labails, Cinthia; Olivet, Jean-Louis; Aslanian, Daniel; Roest, Walter R.

    2010-09-01

    The opening of the Central Atlantic Ocean basin that separated North America from northwest Africa is well documented and assumed to have started during the Late Jurassic. However, the early evolution and the initial breakup history of Pangaea are still debated: most of the existing models are based on one or multiple ridge jumps at the Middle Jurassic leaving the oldest crust on the American side, between the East Coast Magnetic Anomaly (ECMA) and the Blake Spur Magnetic Anomaly (BSMA). According to these hypotheses, the BSMA represents the limit of the initial basin and the footprint subsequent to the ridge jump. Consequently, the evolution of the northwest African margin is widely different from the northeast American margin. However, this setting is in contradiction with the existing observations. In this paper, we propose an alternative scenario for the continental breakup and the Mesozoic spreading history of the Central Atlantic Ocean. The new model is based on an analysis of geophysical data (including new seismic lines, an interpretation of the newly compiled magnetic data, and satellite derived gravimetry) and recently published results which demonstrate that the opening of the Central Atlantic Ocean started already during the Late Sinemurian (190 Ma), based on a new identification of the African conjugate to the ECMA and on the extent of salt provinces off Morocco and Nova Scotia. The identification of an African conjugate magnetic anomaly to BSMA, the African Blake Spur Magnetic Anomaly (ABSMA), together with the significant change in basement topography, are in good agreement with that initial reconstruction. The early opening history for the Central Atlantic Ocean is described in four distinct phases. During the first 20 Myr after the initial breakup (190-170 Ma, from Late Sinemurian to early Bajocian), oceanic accretion was extremely slow (˜ 0.8 cm/y). At the time of Blake Spur (170 Ma, early Bajocian), a drastic change occurred both in the relative

  7. Does deep ocean mixing drive upwelling or downwelling of abyssal waters?

    NASA Astrophysics Data System (ADS)

    Ferrari, R. M.; McDougall, T. J.; Mashayek, A.; Nikurashin, M.; Campin, J. M.

    2016-02-01

    It is generally understood that small-scale mixing, such as is caused by breaking internal waves, drives upwelling of the densest ocean waters that sink to the ocean bottom at high latitudes. However the observational evidence that the turbulent fluxes generated by small-scale mixing in the stratified ocean interior are more vigorous close to the ocean bottom than above implies that small-scale mixing converts light waters into denser ones, thus driving a net sinking of abyssal water. Using a combination of numerical models and observations, it will be shown that abyssal waters return to the surface along weakly stratified boundary layers, where the small-scale mixing of density decays to zero. The net ocean meridional overturning circulation is thus the small residual of a large sinking of waters, driven by small-scale mixing in the stratified interior, and a comparably large upwelling, driven by the reduced small-scale mixing along the ocean boundaries.

  8. Is Europa's Subsurface Water Ocean Warm?

    NASA Technical Reports Server (NTRS)

    Melosh, H. J.; Ekholm, A. G.; Showman, A. P.; Lorenz, R. D.

    2002-01-01

    Europa's subsurface water ocean may be warm: that is, at the temperature of water's maximum density. This provides a natural explanation of chaos melt-through events and leads to a correct estimate of the age of its surface. Additional information is contained in the original extended abstract.

  9. Phylogenetic comparisons of a coastal bacterioplankton community with its counterparts in open ocean and freshwater systems.

    PubMed

    Rappé; Vergin; Giovannoni

    2000-09-01

    In order to extend previous comparisons between coastal marine bacterioplankton communities and their open ocean and freshwater counterparts, here we summarize and provide new data on a clone library of 105 SSU rRNA genes recovered from seawater collected over the western continental shelf of the USA in the Pacific Ocean. Comparisons to previously published data revealed that this coastal bacterioplankton clone library was dominated by SSU rRNA gene phylotypes originally described from surface waters of the open ocean, but also revealed unique SSU rRNA gene lineages of beta Proteobacteria related to those found in clone libraries from freshwater habitats. beta Proteobacteria lineages common to coastal and freshwater samples included members of a clade of obligately methylotrophic bacteria, SSU rRNA genes affiliated with Xylophilus ampelinus, and a clade related to the genus Duganella. In addition, SSU rRNA genes were recovered from such previously recognized marine bacterioplankton SSU rRNA gene clone clusters as the SAR86, SAR11, and SAR116 clusters within the class Proteobacteria, the Roseobacter clade of the alpha subclass of the Proteobacteria, the marine group A/SAR406 cluster, and the marine Actinobacteria clade. Overall, these results support and extend previous observations concerning the global distribution of several marine planktonic prokaryote SSU rRNA gene phylotypes, but also show that coastal bacterioplankton communities contain SSU rRNA gene lineages (and presumably bacterioplankton) shown previously to be prevalent in freshwater habitats.

  10. Arctic Ocean outflow and glacier-ocean interactions modify water over the Wandel Sea shelf (northeastern Greenland)

    NASA Astrophysics Data System (ADS)

    Dmitrenko, Igor A.; Kirillov, Sergey A.; Rudels, Bert; Babb, David G.; Toudal Pedersen, Leif; Rysgaard, Søren; Kristoffersen, Yngve; Barber, David G.

    2017-12-01

    The first-ever conductivity-temperature-depth (CTD) observations on the Wandel Sea shelf in northeastern Greenland were collected in April-May 2015. They were complemented by CTDs taken along the continental slope during the Norwegian FRAM 2014-2015 drift. The CTD profiles are used to reveal the origin of water masses and interactions with ambient water from the continental slope and the tidewater glacier outlet. The subsurface water is associated with the Pacific water outflow from the Arctic Ocean. The underlying halocline separates the Pacific water from a deeper layer of polar water that has interacted with the warm Atlantic water outflow through the Fram Strait, recorded below 140 m. Over the outer shelf, the halocline shows numerous cold density-compensated intrusions indicating lateral interaction with an ambient polar water mass across the continental slope. At the front of the tidewater glacier outlet, colder and turbid water intrusions were observed at the base of the halocline. On the temperature-salinity plots these stations indicate a mixing line that is different from the ambient water and seems to be conditioned by the ocean-glacier interaction. Our observations of Pacific water are set within the context of upstream observations in the Beaufort Sea and downstream observations from the Northeast Water Polynya, and clearly show the modification of Pacific water during its advection across the Arctic Ocean. Moreover, ambient water over the Wandel Sea slope shows different thermohaline structures indicating the different origin and pathways of the on-shore and off-shore branches of the Arctic Ocean outflow through the western Fram Strait.

  11. Convective Available Potential Energy of World Ocean

    NASA Astrophysics Data System (ADS)

    Su, Z.; Ingersoll, A. P.; Thompson, A. F.

    2012-12-01

    Here, for the first time, we propose the concept of Ocean Convective Available Potential Energy (OCAPE), which is the maximum kinetic energy (KE) per unit seawater mass achievable by ocean convection. OCAPE occurs through a different mechanism from atmospheric CAPE, and involves the interplay of temperature and salinity on the equation of state of seawater. The thermobaric effect, which arises because the thermal coefficient of expansion increases with depth, is an important ingredient of OCAPE. We develop an accurate algorithm to calculate the OCAPE for a given temperature and salinity profile. We then validate our calculation of OCAPE by comparing it with the conversion of OCAPE to KE in a 2-D numerical model. We propose that OCAPE is an important energy source of ocean deep convection and contributes to deep water formation. OCAPE, like Atmospheric CAPE, can help predict deep convection and may also provide a useful constraint for modelling deep convection in ocean GCMs. We plot the global distribution of OCAPE using data from the World Ocean Atlas 2009 (WOA09) and see many important features. These include large values of OCAPE in the Labrador, Greenland, Weddell and Mediterranean Seas, which are consistent with our present observations and understanding, but also identify some new features like the OCAPE pattern in the Antarctic Circumpolar Current (ACC). We propose that the diagnosis of OCAPE can improve our understanding of global patterns of ocean convection and deep water formation as well as ocean stratification, the meridional overturning circulation and mixed layer processes. The background of this work is briefly introduced as below. Open-ocean deep convection can significantly modify water properties both at the ocean surface and throughout the water column (Gordon 1982). Open-ocean convection is also an important mechanism for Ocean Deep Water formation and the transport of heat, freshwater and nutrient (Marshall and Schott 1999). Open-ocean

  12. Deep Water Ocean Acoustics

    DTIC Science & Technology

    2015-04-15

    0 A S S PROGRESS REPORT NO. QSR-14C0172-0CEAN ACOUSTICS-033115 Contract No. N00014-14-C-0172 Office of Naval Research Task Reporting: Deep ...AND SUBTITLE Deep Water Ocean Acoustics 5a. CONTRACT NUMBER 5b. GRANT NUMBER 5c. PROGRAM ELEMENT NUMBER 6. AUTHOR(S) 5d. PROJECT NUMBER 5e...298 (Rev. 8-98) Prescribed by ANSI Std Z39-18 Cost Summary OASIS, INC. JOB STATUS RB’ORT 1172 DEEP WATER ACOUSTICS FOP. 9/27f13-316/16

  13. Modeling water clarity in oceans and coasts

    EPA Science Inventory

    In oceans and coastal waters, phytoplankton is the primary producer of organic compounds which form the base for the food chain. The concentration of phytoplankton is a major factor controlling water clarity and the depth to which light penetrates in the water column. The light i...

  14. Lagrangian analysis of multi-satellite data in support of open ocean Marine Protected Area design

    NASA Astrophysics Data System (ADS)

    Della Penna, Alice; Koubbi, Philippe; Cotté, Cedric; Bon, Cécile; Bost, Charles-André; d'Ovidio, Francesco

    2017-06-01

    Compared to ecosystem conservation in territorial seas, protecting the open ocean has peculiar geopolitical, economic and scientific challenges. One of the major obstacle is defining the boundary of an open ocean Marine Protected Area (MPA). In contrast to coastal ecosystems, which are mostly constrained by topographic structures fixed in time, the life of marine organisms in the open ocean is entrained by fluid dynamical structures like eddies and fronts, whose lifetime occurs on ecologically-relevant timescales. The position of these highly dynamical structures can vary interannually by hundreds of km, and so too will regions identified as ecologically relevant such as the foraging areas of marine predators. Thus, the expected foraging locations suggested from tracking data cannot be directly extrapolated beyond the year in which the data were collected. Here we explore the potential of Lagrangian methods applied to multisatellite data as a support tool for a MPA proposal by focusing on the Crozet archipelago oceanic area (Indian Sector of the Southern Ocean). By combining remote sensing with biologging information from a key marine top predator (Eudyptes chrysolophus, or Macaroni penguin) of the Southern Ocean foodweb, we identify a highly dynamic branch of the Subantarctic front as a foraging hotspot. By tracking this feature in historical satellite data (1993-2012) we are able to extrapolate the position of this foraging ground beyond the years in which tracking data are available and study its spatial variability.

  15. Assimilation of satellite altimeter data into an open ocean model

    NASA Astrophysics Data System (ADS)

    Vogeler, Armin; SchröTer, Jens

    1995-08-01

    Geosat sea surface height data are assimilated into an eddy-resolving quasi-geostrophic open ocean model using the adjoint technique. The method adjusts the initial conditions for all layers and is successful on the timescale of a few weeks. Time-varying values for the open boundaries are prescribed by a much larger quasi-geostrophic model of the Antarctic Circumpolar Current (ACC). Both models have the same resolution of approximately 20×20 km (1/3°×1/6°), have three layers, and include realistic bottom topography and coastlines. The open model box is embedded in the African sector of the ACC. For continuous assimilation of satellite data into the larger model the nudging technique is applied. These results are used for the adjoint optimization procedure as boundary conditions and as a first guess for the initial condition. For the open model box the difference between model and satellite sea surface height that remains after the nudging experiment amounts to a 19-cm root-mean-square error (rmse). By assimilation into the regional model this value can be reduced to a 6-cm rmse for an assimilation period of 20 days. Several experiments which attempt to improve the convergence of the iterative optimization method are reported. Scaling and regularization by smoothing have to be applied carefully. Especially during the first 10 iterations, the convergence can be improved considerably by low-pass filtering of the cost function gradient. The result of a perturbation experiment shows that for longer assimilation periods the influence of the boundary values becomes dominant and they should be determined inversely by data assimilation into the open ocean model.

  16. Abrupt turnover in calcareous-nannoplankton assemblages across the Paleocene/Eocene Thermal Maximum: implications for surface-water oligotrophy over the Kerguelen Plateau, Southern Indian Ocean

    USGS Publications Warehouse

    Jiang, Shijun; Wise, Sherwood W.

    2007-01-01

    Ocean Drilling Program (ODP) Core Section 183-1135A-25R-4 from the Kerguelen Plateau in the Indian Ocean sector of the Southern Ocean represents only the second complete, expanded sequence through the Paleocene/Eocene Thermal Maximum (PETM; ~55 Ma) recovered from Antarctic waters. Calcareous nannoplankton at this site underwent an abrupt, fundamental turnover across the PETM as defined by a carbon isotope excursion. Although Chiasmolithus, Discoaster, and Fasciculithus exponentially increase in abundance at the onset, the former abruptly drops but then rapidly recovers, whereas the latter two taxa show opposite trends due to surface-water oligotrophy. These observations confirm previous results from ODP Site 690 on Maud Rise. The elevated pCO2 that accompanied the PETM caused a shoaling of the lysocline and carbonate compensation depth, leading to intensive dissolution of susceptible holococcoliths and poor preservation of the assemblages. Similarities and contrasts between the results of this study and previous work from open-ocean sites and shelf margins further demonstrate that the response to the PETM was consistent in open-ocean environments, but could be localized on continental shelves where nutrient regimes depend on the local geologic setting and oceanographic conditions.

  17. Use of Multiangle Satellite Observations to Retrieve Aerosol Properties and Ocean Color

    NASA Technical Reports Server (NTRS)

    Martonchik, John V.; Diner, David; Khan, Ralph

    2005-01-01

    A new technique is described for retrieving aerosol over ocean water and the associated ocean color using multiangle satellite observations. Unlike current satellite aerosol retrieval algorithms which only utilize observations at red wavelengths and longer, with the assumption that these wavelengths have a negligible ocean (water-leaving radiance), this new algorithm uses all available spectral bands and simultaneously retrieves both aerosol properties and the spectral ocean color. We show some results of case studies using MISR data, performed over different water conditions (coastal water, blooms, and open water).

  18. The Proposed Surface Water and Ocean Topography (SWOT) Mission

    NASA Astrophysics Data System (ADS)

    Fu, Lee-Lueng; Alsdorf, Douglas; Rodriguez, Ernesto; Morrow, Rosemary; Mognard, Nelly; Vaze, Parag; Lafon, Thierry

    2013-09-01

    A new space mission concept called Surface Water and Ocean Topography (SWOT) is being developed jointly by a collaborative effort of the international oceanographic and hydrological communities for making high-resolution measurement of the water elevation of both the ocean and land surface water to answer the questions about the oceanic submesoscale processes and the storage and discharge of land surface water. The key instrument payload would be a Ka-band radar interferometer capable of making high-resolution wide-swath altimetry measurement. This paper describes the proposed science objectives and requirements as well as the measurement approach of SWOT, which is baselined to be launched in 2019. SWOT would demonstrate this new approach to advancing both oceanography and land hydrology and set a standard for future altimetry missions.

  19. The Proposed Surface Water and Ocean Topography (SWOT) Mission

    NASA Technical Reports Server (NTRS)

    Fu, Lee-Lueng; Alsdorf, Douglas; Rodriguez, Ernesto; Morrow, Rosemary; Mognard, Nelly; Vaze, Parag; Lafon, Thierry

    2012-01-01

    A new space mission concept called Surface Water and Ocean Topography (SWOT) is being developed jointly by a collaborative effort of the international oceanographic and hydrological communities for making high-resolution measurement of the water elevation of both the ocean and land surface water to answer the questions about the oceanic submesoscale processes and the storage and discharge of land surface water. The key instrument payload would be a Ka-band radar interferometer capable of making high-resolution wide-swath altimetry measurement. This paper describes the proposed science objectives and requirements as well as the measurement approach of SWOT, which is baselined to be launched in 2019. SWOT would demonstrate this new approach to advancing both oceanography and land hydrology and set a standard for future altimetry missions.

  20. Pathways of upwelling deep waters to the surface of the Southern Ocean

    NASA Astrophysics Data System (ADS)

    Tamsitt, Veronica; Drake, Henri; Morrison, Adele; Talley, Lynne; Dufour, Carolina; Gray, Alison; Griffies, Stephen; Mazloff, Matthew; Sarmiento, Jorge; Wang, Jinbo; Weijer, Wilbert

    2017-04-01

    Upwelling of Atlantic, Indian and Pacific deep waters to the sea surface in the Southern Ocean closes the global overturning circulation and is fundamentally important for oceanic uptake of anthropogenic carbon and heat, nutrient resupply for sustaining oceanic biological production, and the melt rate of ice shelves. Here we go beyond the two-dimensional view of Southern Ocean upwelling, to show detailed Southern Ocean upwelling pathways in three dimensions, using hydrographic observations and particle tracking in high-resolution ocean and climate models. The northern deep waters enter the Antarctic Circumpolar Current (ACC) via narrow southward currents along the boundaries of the three ocean basins, before spiraling southeastward and upward through the ACC. Upwelling is greatly enhanced at five major topographic features, associated with vigorous mesoscale eddy activity. Deep water reaches the upper ocean predominantly south of the southern ACC boundary, with a spatially nonuniform distribution, regionalizing warm water supply to Antarctic ice shelves and the delivery of nutrient and carbon-rich water to the sea surface. The timescale for half of the deep water to upwell from 30°S to the mixed layer is on the order of 60-90 years, which has important implications for the timescale for signals to propagate through the deep ocean. In addition, we quantify the diabatic transformation along particle trajectories, to identify where diabatic processes are important along the upwelling pathways.

  1. Southeast Regional Implementation Manual for Requirements and Procedures for Evaluation of the Ocean Disposal of Dredged Material in Southeastern U.S. Atlantic and Gulf Coast Waters

    EPA Pesticide Factsheets

    This Regional Implementation Manual was prepared by EPA Region 4 to provide guidance for applicants proposing open-water disposal of dredged material in southeastern U.S. coastal waters of the Atlantic Ocean and the Gulf of Mexico.

  2. Humboldt Open Ocean Disposal Site (HOODS) Survey Work 2014

    EPA Pesticide Factsheets

    The Humboldt Open Ocean Disposal Site (HOODS) is a dredged material disposal site located 3 nautical miles (nm) offshore of Humboldt Bay in Northern California. HOODS was permanently designated by EPA Region 9 in 1995, and has been actively used for dredged material disposal operations since then. The HOODS has received higher volumes of dredged material than predicted since its designation in 1995, mainly from USACE construction and maintenance dredging.

  3. A global ocean climatology of preindustrial and modern ocean δ13C

    NASA Astrophysics Data System (ADS)

    Eide, Marie; Olsen, Are; Ninnemann, Ulysses S.; Johannessen, Truls

    2017-03-01

    We present a global ocean climatology of dissolved inorganic carbon δ13C (‰) corrected for the 13C-Suess effect, preindustrial δ13C. This was constructed by first using Olsen and Ninnemann's (2010) back-calculation method on data from 25 World Ocean Circulation Experiment cruises to reconstruct the preindustrial δ13C on sections spanning all major oceans. Next, we developed five multilinear regression equations, one for each major ocean basin, which were applied on the World Ocean Atlas data to construct the climatology. This reveals the natural δ13C distribution in the global ocean. Compared to the modern distribution, the preindustrial δ13C spans a larger range of values. The maxima, of up to 1.8‰, occurs in the subtropical gyres of all basins, in the upper and intermediate waters of the North Atlantic, as well as in mode waters with a Southern Ocean origin. Particularly strong gradients occur at intermediate depths, revealing a strong potential for using δ13C as a tracer for changes in water mass geometry at these levels. Further, we identify a much tighter relationship between δ13C and apparent oxygen utilization (AOU) than between δ13C and phosphate. This arises because, in contrast to phosphate, AOU and δ13C are both partly reset when waters are ventilated in the Southern Ocean and underscore that δ13C is a highly robust proxy for past changes in ocean oxygen content and ocean ventilation. Our global preindustrial δ13C climatology is openly accessible and can be used, for example, for improved model evaluation and interpretation of sediment δ13C records.

  4. Geophysical Potential for Wind Energy over the Open Oceans

    NASA Astrophysics Data System (ADS)

    Possner, A.; Caldeira, K.

    2017-12-01

    Wind turbines continuously remove kinetic energy from the lower troposphere thereby reducing the wind speed near hub height. The rate of electricity generation in large wind farms containing multiple wind arrays is therefore constrained by the rate of kinetic energy replenishment from the atmosphere above. In particular, this study focuses on the maximum sustained transport of kinetic energy through the troposphere to the lowest hundreds of meters above the surface. In recent years, a growing body of research argues that the rate of generated power is limited to around 1.5 Wm-2 within large wind farms. However, in this study we demonstrate that considerably higher power generation rates may be sustainable over some open ocean areas in giant wind farms. We find that in the North Atlantic maximum extraction rates of up to 6.7 Wm-2 may be sustained by the atmosphere in the annual mean over giant wind farm areas approaching the size of Greenland. In contrast, only a third of this rate is sustained on land for areas of equivalent size. Our simulations indicate a fundamental difference in response of the troposphere and its vertical kinetic energy flux to giant near-surface wind farms. We find that the surface heat flux from the oceans to the atmosphere may play an important role in creating regions where large sustained rates of downward transport of kinetic energy and thus rates of kinetic energy extraction may be geophysically possible. While no commercial-scale deep-water wind turbines yet exist, our results suggest that such technologies, if they became technically and economically feasible, could potentially provide civilization-scale power.

  5. Water security and services in the ocean-aquifer system

    NASA Astrophysics Data System (ADS)

    Taniguchi, M.

    2011-12-01

    Coastal vulnerability and water security are both important research subjects on global environmental problems under the pressures of changing climate and societies. A six years research project by RIHN on the coastal subsurface environments in seven Asia cities revealed that subsurface environmental problems including saltwater intrusion, groundwater contamination and subsurface thermal anomalies occurred one after another depending on the development stage of the cities during the last 100 years. Exchanges of water between ocean and aquifer in the coastal cities depend on driving force from land of natural resources capacities such as groundwater recharge rate, and social changes such as excessive groundwater pumping due to industrialization. Risk assessments and managements for aquifers which are parts of water security have been made for seven Asian coastal cities. On the other hand, submarine groundwater discharge (SGD) into the ocean provides water services directly to the coastal ecosystem through nutrient transports from land to the ocean. Constant geophysical and geochemical conditions served by SGD provide sustainable services to the coastal environment. Flora and fauna which prefer brackish water in the coastal zone depend on not only river water discharge but also SGD. Ocean -aquifer interaction can be found in the coastal ecosystem including sea shell, sea grass and fishes in the coastal zone though SGD. In order to evaluate a coastal security and sustainable environment, not only risk assessments due to disasters but also water services are important, and the both are evaluated in Asian coastal zones.

  6. SWIM: A Semi-Analytical Ocean Color Inversion Algorithm for Optically Shallow Waters

    NASA Technical Reports Server (NTRS)

    McKinna, Lachlan I. W.; Werdell, P. Jeremy; Fearns, Peter R. C. S.; Weeks, Scarla J.; Reichstetter, Martina; Franz, Bryan A.; Shea, Donald M.; Feldman, Gene C.

    2014-01-01

    Ocean color remote sensing provides synoptic-scale, near-daily observations of marine inherent optical properties (IOPs). Whilst contemporary ocean color algorithms are known to perform well in deep oceanic waters, they have difficulty operating in optically clear, shallow marine environments where light reflected from the seafloor contributes to the water-leaving radiance. The effect of benthic reflectance in optically shallow waters is known to adversely affect algorithms developed for optically deep waters [1, 2]. Whilst adapted versions of optically deep ocean color algorithms have been applied to optically shallow regions with reasonable success [3], there is presently no approach that directly corrects for bottom reflectance using existing knowledge of bathymetry and benthic albedo.To address the issue of optically shallow waters, we have developed a semi-analytical ocean color inversion algorithm: the Shallow Water Inversion Model (SWIM). SWIM uses existing bathymetry and a derived benthic albedo map to correct for bottom reflectance using the semi-analytical model of Lee et al [4]. The algorithm was incorporated into the NASA Ocean Biology Processing Groups L2GEN program and tested in optically shallow waters of the Great Barrier Reef, Australia. In-lieu of readily available in situ matchup data, we present a comparison between SWIM and two contemporary ocean color algorithms, the Generalized Inherent Optical Property Algorithm (GIOP) and the Quasi-Analytical Algorithm (QAA).

  7. Species composition, timing, and weather correlates of autumn open-water crossings by raptors migrating along the East-Asian Oceanic Flyway

    USGS Publications Warehouse

    Concepcion, Camille B.; Dumandan, Patricia T.; Silvosa, Medel R.; Bildstein, Keith L.; Katzner, Todd E.

    2017-01-01

    Raptor migration rarely involves long-distance movements across open oceans. One exception occurs along the East-Asian Oceanic Flyway. We collected migration data at two terrestrial hawkwatch sites along this flyway to better understand open-ocean movements along this largely overwater corridor. At the northern end of the Philippines, at Basco on the island of Batan, we recorded 7587 migratory raptors in autumn 2014. Near the southern end of the Philippines, at Cape San Agustin on the island of Mindanao, we recorded 27,399 raptors migrating in autumn 2012. Chinese Sparrowhawks (Accipiter soloensis) were the most common raptors observed, making up approximately 89% and 92% of total records for Basco and Cape San Agustin, respectively. The Grey-faced Buzzard (Butastur indicus) was the second most common raptor migrant, accounting for 8% of the total counts at both watch sites. The migration period was about 1–2 wk earlier at Basco, the more northerly site, than at Cape San Agustin. Overwater flights at Basco peaked in both the morning and late afternoon, whereas at Cape San Agustin there was only a morning peak. In general, the rate of migration passage at both sites was highest with clear skies when winds were blowing from the northwest. However, we observed interspecific differences in migration behavior at both sites, with Accipiters more likely to be observed with tailwinds and eastward winds, and Grey-faced Buzzards more likely observed with headwinds. These results help to characterize poorly known aspects of raptor biology and to identify potential migratory bottlenecks or key sites for raptor conservation in little-studied Philippine tropical ecosystems.

  8. Polaro–cryptic mirror of the lookdown as a biological model for open ocean camouflage

    PubMed Central

    Brady, Parrish C.; Travis, Kort A.; Maginnis, Tara; Cummings, Molly E.

    2013-01-01

    With no object to hide behind in 3D space, the open ocean represents a challenging environment for camouflage. Conventional strategies for reflective crypsis (e.g., standard mirror) are effective against axially symmetric radiance fields associated with high solar altitudes, yet ineffective against asymmetric polarized radiance fields associated with low solar inclinations. Here we identify a biological model for polaro–crypsis. We measured the surface-reflectance Mueller matrix of live open ocean fish (lookdown, Selene vomer) and seagrass-dwelling fish (pinfish, Lagodon rhomboides) using polarization-imaging and modeling polarization camouflage for the open ocean. Lookdowns occupy the minimization basin of our polarization-contrast space, while pinfish and standard mirror measurements exhibit higher contrast values than optimal. The lookdown reflective strategy achieves significant gains in polaro–crypsis (up to 80%) in comparison with nonpolarization sensitive strategies, such as a vertical mirror. Lookdowns achieve polaro–crypsis across solar altitudes by varying reflective properties (described by 16 Mueller matrix elements mij) with incident illumination. Lookdowns preserve reflected polarization aligned with principle axes (dorsal–ventral and anterior–posterior, m22 = 0.64), while randomizing incident polarization 45° from principle axes (m33 = –0.05). These reflectance properties allow lookdowns to reflect the uniform degree and angle of polarization associated with high-noon conditions due to alignment of the principle axes and the sun, and reflect a more complex polarization pattern at asymmetrical light fields associated with lower solar elevations. Our results suggest that polaro–cryptic strategies vary by habitat, and require context-specific depolarization and angle alteration for effective concealment in the complex open ocean environment. PMID:23716701

  9. Evaporative fractionation of marine water isotopes in the Arctic Ocean help understand a changing Arctic water cycle

    NASA Astrophysics Data System (ADS)

    Klein, E. S.; Welker, J. M.

    2017-12-01

    Most of the global hydrologic cycle occurs in oceanic waters. This oceanic derived moisture is critical to the precipitation and evapotranspiration regimes that influence terrestrial Earth systems. Thus understanding oceanic water processes has important global implications for our knowledge of modern and past hydrologic cycles. As they are influenced by environmental variables such as sea surface temperature and atmospheric humidity, water isotope ratios (e.g., δ18O, δ2H) can help understand the patterns driving the water cycle. However, our knowledge of marine isotopes is relatively limited. In particular, the fractionation of water isotopes during evaporation of oceanic water, essentially the start of the hydrologic cycle, is largely based on theoretical relationships derived from spatially and temporally limited data sets. This constrained understanding of oceanic evaporation fractionation patterns is especially pronounced in the rapidly changing Arctic Ocean. These changes are associated with reduced sea ice coverage, which is increasing the amount of local Artic Ocean sourced moisture in atmospheric and terrestrial systems and amplifying the Arctic hydrologic cycle. Here we present new data revealing the nuances of evaporative fractionation of Arctic Ocean water isotopes with the first collection of continuous, contemporaneous sea water and vapor isotopes. These data, collected in situ aboard the icebreaker Healy, show that the difference between actual ocean vapor isotope values and vapor values estimated by the closure equation increases progressively with latitude (especially beyond 70°) and varies between δ18O and δ2H. These differences are likely due to more isotopic mixing in the troposphere and/or closure equation assumptions inapplicable to Arctic regions. Moreover, we find: 1) a positive relationship between fractionation magnitude and latitude; and 2) the influence of evaporative fractionation from environmental variables such as wind and

  10. Ocean acidification state in western Antarctic surface waters: drivers and interannual variability

    NASA Astrophysics Data System (ADS)

    Mattsdotter Björk, M.; Fransson, A.; Chierici, M.

    2013-05-01

    Each December during four years from 2006 to 2010, the surface water carbonate system was measured and investigated in the Amundsen Sea and Ross Sea, western Antarctica as part of the Oden Southern Ocean expeditions (OSO). The I/B Oden started in Punta Arenas in Chile and sailed southwest, passing through different regimes such as, the marginal/seasonal ice zone, fronts, coastal shelves, and polynyas. Discrete surface water was sampled underway for analysis of total alkalinity (AT), total dissolved inorganic carbon (CT) and pH. Two of these parameters were used together with sea-surface temperature (SST), and salinity to obtain a full description of the surface water carbonate system, including pH in situ and calcium carbonate saturation state of aragonite (ΩAr) and calcite (ΩCa). Multivariate analysis was used to investigate interannual variability and the major controls (sea-ice concentration, SST, salinity and chlorophyll a) on the variability in the carbonate system and Ω. This analysis showed that SST and chlorophyll a were the major drivers of the Ω variability in both the Amundsen and Ross seas. In 2007, the sea-ice edge was located further south and the area of the open polynya was relatively small compared to 2010. We found the lowest pH in situ (7.932) and Ω = 1 values in the sea-ice zone and in the coastal Amundsen Sea, nearby marine out flowing glaciers. In 2010, the sea-ice coverage was the largest and the areas of the open polynyas were the largest for the whole period. This year we found the lowest salinity and AT, coinciding with highest chl a. This implies that the highest ΩAr in 2010 was likely an effect of biological CO2 drawdown, which out-competed the dilution of carbonate ion concentration due to large melt water volumes. We predict and discuss future Ω values, using our data and reported rates of oceanic uptake of anthropogenic CO2, suggesting that the Amundsen Sea will become undersaturated with regard to aragonite about 20 yr sooner

  11. Impacts of Ocean Acidification on Sediment Processes in Shallow Waters of the Arctic Ocean

    PubMed Central

    Gazeau, Frédéric; van Rijswijk, Pieter; Pozzato, Lara; Middelburg, Jack J.

    2014-01-01

    Despite the important roles of shallow-water sediments in global biogeochemical cycling, the effects of ocean acidification on sedimentary processes have received relatively little attention. As high-latitude cold waters can absorb more CO2 and usually have a lower buffering capacity than warmer waters, acidification rates in these areas are faster than those in sub-tropical regions. The present study investigates the effects of ocean acidification on sediment composition, processes and sediment-water fluxes in an Arctic coastal system. Undisturbed sediment cores, exempt of large dwelling organisms, were collected, incubated for a period of 14 days, and subject to a gradient of pCO2 covering the range of values projected for the end of the century. On five occasions during the experimental period, the sediment cores were isolated for flux measurements (oxygen, alkalinity, dissolved inorganic carbon, ammonium, nitrate, nitrite, phosphate and silicate). At the end of the experimental period, denitrification rates were measured and sediment samples were taken at several depth intervals for solid-phase analyses. Most of the parameters and processes (i.e. mineralization, denitrification) investigated showed no relationship with the overlying seawater pH, suggesting that ocean acidification will have limited impacts on the microbial activity and associated sediment-water fluxes on Arctic shelves, in the absence of active bio-irrigating organisms. Only following a pH decrease of 1 pH unit, not foreseen in the coming 300 years, significant enhancements of calcium carbonate dissolution and anammox rates were observed. Longer-term experiments on different sediment types are still required to confirm the limited impact of ocean acidification on shallow Arctic sediment processes as observed in this study. PMID:24718610

  12. Impacts of ocean acidification on sediment processes in shallow waters of the Arctic Ocean.

    PubMed

    Gazeau, Frédéric; van Rijswijk, Pieter; Pozzato, Lara; Middelburg, Jack J

    2014-01-01

    Despite the important roles of shallow-water sediments in global biogeochemical cycling, the effects of ocean acidification on sedimentary processes have received relatively little attention. As high-latitude cold waters can absorb more CO2 and usually have a lower buffering capacity than warmer waters, acidification rates in these areas are faster than those in sub-tropical regions. The present study investigates the effects of ocean acidification on sediment composition, processes and sediment-water fluxes in an Arctic coastal system. Undisturbed sediment cores, exempt of large dwelling organisms, were collected, incubated for a period of 14 days, and subject to a gradient of pCO2 covering the range of values projected for the end of the century. On five occasions during the experimental period, the sediment cores were isolated for flux measurements (oxygen, alkalinity, dissolved inorganic carbon, ammonium, nitrate, nitrite, phosphate and silicate). At the end of the experimental period, denitrification rates were measured and sediment samples were taken at several depth intervals for solid-phase analyses. Most of the parameters and processes (i.e. mineralization, denitrification) investigated showed no relationship with the overlying seawater pH, suggesting that ocean acidification will have limited impacts on the microbial activity and associated sediment-water fluxes on Arctic shelves, in the absence of active bio-irrigating organisms. Only following a pH decrease of 1 pH unit, not foreseen in the coming 300 years, significant enhancements of calcium carbonate dissolution and anammox rates were observed. Longer-term experiments on different sediment types are still required to confirm the limited impact of ocean acidification on shallow Arctic sediment processes as observed in this study.

  13. Antarctic glaciation caused ocean circulation changes at the Eocene-Oligocene transition

    NASA Astrophysics Data System (ADS)

    Goldner, A.; Herold, N.; Huber, M.

    2014-07-01

    Two main hypotheses compete to explain global cooling and the abrupt growth of the Antarctic ice sheet across the Eocene-Oligocene transition about 34 million years ago: thermal isolation of Antarctica due to southern ocean gateway opening, and declining atmospheric CO2 (refs 5, 6). Increases in ocean thermal stratification and circulation in proxies across the Eocene-Oligocene transition have been interpreted as a unique signature of gateway opening, but at present both mechanisms remain possible. Here, using a coupled ocean-atmosphere model, we show that the rise of Antarctic glaciation, rather than altered palaeogeography, is best able to explain the observed oceanographic changes. We find that growth of the Antarctic ice sheet caused enhanced northward transport of Antarctic intermediate water and invigorated the formation of Antarctic bottom water, fundamentally reorganizing ocean circulation. Conversely, gateway openings had much less impact on ocean thermal stratification and circulation. Our results support available evidence that CO2 drawdown--not gateway opening--caused Antarctic ice sheet growth, and further show that these feedbacks in turn altered ocean circulation. The precise timing and rate of glaciation, and thus its impacts on ocean circulation, reflect the balance between potentially positive feedbacks (increases in sea ice extent and enhanced primary productivity) and negative feedbacks (stronger southward heat transport and localized high-latitude warming). The Antarctic ice sheet had a complex, dynamic role in ocean circulation and heat fluxes during its initiation, and these processes are likely to operate in the future.

  14. Antarctic glaciation caused ocean circulation changes at the Eocene-Oligocene transition.

    PubMed

    Goldner, A; Herold, N; Huber, M

    2014-07-31

    Two main hypotheses compete to explain global cooling and the abrupt growth of the Antarctic ice sheet across the Eocene-Oligocene transition about 34 million years ago: thermal isolation of Antarctica due to southern ocean gateway opening, and declining atmospheric CO2 (refs 5, 6). Increases in ocean thermal stratification and circulation in proxies across the Eocene-Oligocene transition have been interpreted as a unique signature of gateway opening, but at present both mechanisms remain possible. Here, using a coupled ocean-atmosphere model, we show that the rise of Antarctic glaciation, rather than altered palaeogeography, is best able to explain the observed oceanographic changes. We find that growth of the Antarctic ice sheet caused enhanced northward transport of Antarctic intermediate water and invigorated the formation of Antarctic bottom water, fundamentally reorganizing ocean circulation. Conversely, gateway openings had much less impact on ocean thermal stratification and circulation. Our results support available evidence that CO2 drawdown--not gateway opening--caused Antarctic ice sheet growth, and further show that these feedbacks in turn altered ocean circulation. The precise timing and rate of glaciation, and thus its impacts on ocean circulation, reflect the balance between potentially positive feedbacks (increases in sea ice extent and enhanced primary productivity) and negative feedbacks (stronger southward heat transport and localized high-latitude warming). The Antarctic ice sheet had a complex, dynamic role in ocean circulation and heat fluxes during its initiation, and these processes are likely to operate in the future.

  15. Shelf and open-ocean calcareous phytoplankton assemblages across the Paleocene-Eocene thermal maximum: Implications for global productivity gradients

    USGS Publications Warehouse

    Gibbs, S.J.; Bralower, T.J.; Bown, Paul R.; Zachos, J.C.; Bybell, L.M.

    2006-01-01

    Abrupt global warming and profound perturbation of the carbon cycle during the Paleocene-Eocene Thermal Maximum (PETM, ca. 55 Ma) have been linked to a massive release of carbon into the ocean-atmosphere system. Increased phytoplankton productivity has been invoked to cause subsequent CO2 drawdown, cooling, and environmental recovery. However, interpretations of geochemical and biotic data differ on when and where this increased productivity occurred. Here we present high-resolution nannofossil assemblage data from a shelf section (the U.S. Geological Survey [USGS] drill hole at Wilson Lake, New Jersey) and an open-ocean location (Ocean Drilling Program [ODP] Site 1209, paleoequatorial Pacific). These data combined with published biotic records indicate a transient steepening of shelf-offshelf trophic gradients across the PETM onset and peak, with a decrease in open-ocean productivity coeval with increased nutrient availability in shelf areas. Productivity levels recovered in the open ocean during the later stages of the event, which, coupled with intensified continental weathering rates, may have played an important role in carbon sequestration and CO2 drawdown. ?? 2006 Geological Society of America.

  16. Modeling Water Clarity and Light Quality in Oceans

    EPA Science Inventory

    Phytoplankton is a primary producer of organic compounds, and it forms the base of the food chain in ocean waters. The concentration of phytoplankton in the water column controls water clarity and the amount and quality of light that penetrates through it. The availability of ade...

  17. Influence of ambient water intrusion on coral reef acidification in the Chuuk lagoon, located in the coral-rich western Pacific Ocean

    NASA Astrophysics Data System (ADS)

    Ko, Young Ho; Lee, Kitack; Noh, Jae Hoon; Lee, Charity M.; Kleypas, Joan A.; Jeong, Hae Jin; Kim, Kwang Young

    2016-04-01

    Weekly carbonate chemistry condition data recorded between 2008 and 2014 in the Chuuk lagoon (7.3°N and 151.5°E) of the Federated States of Micronesia, located in the western Pacific Ocean, were analyzed. The results showed that, during periods of weak intrusion of ambient seawater from the surrounding open ocean, two internal biological processes (calcification and respiration) reinforced each other and together lowered the pH of the reef water for extended periods, ranging from a few to several months. The analysis indicated that reduced intrusion of ambient water is associated with periods of low wind speeds. Such conditions increase the residence time of reef water, thus promoting acidification by respiration and calcification. This phenomenon likely affects many other areas of the coral-rich western Pacific Ocean, which contains 50% of global coral reefs and in which the degree of ambient water intrusion into the atolls has been shown to be closely associated with the El Niño-Southern Oscillation-induced wind speed change.

  18. Characteristics of elite open-water swimmers.

    PubMed

    VanHeest, Jaci L; Mahoney, Carrie E; Herr, Larry

    2004-05-01

    Open-water swimming (5, 10, and 25 km) has many unique challenges that separate it from other endurance sports, like marathon running and cycling. The characteristics of a successful open-water swimmer are unclear. The purpose of this study was to determine the physical and metabolic characteristics of a group of elite-level open-water swimmers. The open-water swimmers were participating in a 1-week training camp. Anthropometric, metabolic, and blood chemistry assessments were performed on the athletes. The swimmers had a VO(2)peak of 5.51 +/- 0.96 and 5.06 +/- 0.57 ml.kg(-1).min(-1) for males and females, respectively. Their lactate threshold (LT) occurred at a pace equal to 88.75% of peak pace for males and 93.75% for females. These elite open-water swimmers were smaller and lighter than competitive pool swimmers. They possess aerobic metabolic alterations that resulted in enhanced performance in distance swimming. Trainers and coaches should develop dry-land programs that will improve the athlete's muscular endurance. Furthermore, programs should be designed to increase the LT velocity as a percentage of peak swimming velocity.

  19. Constraints on the sources of branched GDGTs in open ocean sediments: dust transport or in situ production?

    NASA Astrophysics Data System (ADS)

    Weijers, J.; Schefuss, E.; Kim, J.; Sinninghe Damsté, J. S.; Schouten, S.

    2012-12-01

    Branched glycerol dialkyl glycerol tetraethers (brGDGTs) are membrane lipids synthesized by soil bacteria that, upon soil erosion, are transported by rivers to the ocean where they accumulate in the near shore sedimentary archive. The degrees of cyclisation (CBT) and methylation (MBT) of these compounds have been shown to relate to soil pH and annual mean air temperature [1]. Therefore, brGDGTs in near shore sedimentary archives can be used to estimate past continental air temperatures and enable a direct comparison of these to marine sea surface temperature estimates obtained from the same samples. In addition, brGDGT abundance relative to crenarchaeol, an isoprenoid GDGT synthesized by marine pelagic Thaumarchaeota, quantified in the branched vs. isoprenoid tetraether (BIT) index, is an indicator of the relative input of soil organic matter in near shore sediments [2]. High BIT values near river outflows testify of relative strong soil organic matter input and generally the BIT index will decrease off shore to values near 0, the marine end-member value. Even in remote open ocean sediments, however, the BIT index will rarely reach 0 as small amounts of brGDGTs are often present. The occurrence of these brGDGTs in open marine settings might be a result of i) dust input, ii) sediment dispersion from near coastal areas, or iii) in situ production in marine sediments. In order to constrain the origin of branched GDGTs in open marine sediments we analyzed i) atmospheric dust samples taken along an equatorial African coastal transect, ii) marine surface waters near and away of the Congo river outflow, iii) a series of surface sediments at and around the Congo deep sea fan, and iv) a series of open marine surface sediments from different oceans with BIT values < 0.08. Our results show that brGDGTs are present, though in relative low amounts, in dust. Their distribution resembles that of soil input as also found in the Congo deep sea fan, with MBT and CBT values that

  20. Benthic foraminiferal assemblages in the Cap de Creus canyon and adjacent open slope: Potential influence of dense shelf water cascading and open-ocean convection

    NASA Astrophysics Data System (ADS)

    Nardelli, M. P.; Sabbatini, A.; Bonnot, E.; Mea, M.; Pusceddu, A.; Danovaro, R.; Durrieu de Madron, X.; Negri, A.; Bicchi, E.

    2018-06-01

    The NW Mediterranean Sea is subjected to episodically intense events of dense shelf water cascading (DSWC) and open-ocean convection (OOC) that ventilate the seafloor and also have important consequences on organic matter inputs to the seabed and sediment dynamics. The influence of the massive physico-chemical disturbance driven by these events on deep-sea ecosystems is poorly known, and, to date, no information is available on the response of benthic foraminiferal assemblages. To provide insights on these gaps of knowledge, in April 2009 we investigated the foraminiferal faunas along the major axis of the Cap de Creus canyon (at 1000, 1900 and 2400 m depth) and at two additional stations located on the adjacent open slope (at 1000 and 1900 m). The area under scrutiny was hit by intense DSWC and OOC events in winters 2005 and 2006, and during winter 2009 an intense OOC event occurred, with detectable consequences observed at > 1500 m depth. We report here foraminiferal faunas characterized by low densities but relatively high levels of biodiversity at 1000-m depth stations. On the contrary, at the deeper depths, very high densities (associated with low organic matter contents) and strong dominance of the disaster species Usbekistania charoides were observed in the > 63 μm fraction. The comparison of our results - obtained immediately after an OOC event - to those previously described in spring 2004, before DSWC and OOC events, reveals the presence of largely different foraminiferal assemblages in the two periods. Based on a detailed analysis of the ecological traits of the faunas encountered in the two sampling periods, we suggest that either DSWC or OOC can have a role in shaping deep-sea foraminiferal faunas. Moreover, we contend that, at 1000 m depth, the composition of the foraminiferal assemblages in spring 2009 is suggestive of a resilient stage following the major DSWC events in 2005/2006, whereas the low evenness of faunas at ≥ 1900 m depth is, most

  1. Charting the Course for Ocean Science in the United States for the Next Decade: An Ocean Research Priorities Plan and Implementation Strategy

    DTIC Science & Technology

    2007-01-26

    ocean affects calcifying organisms, such as corals , with significant effects to reefs , the ecosystems they support, and their ability to pro- tect...water coral reefs , to open- ocean systems. For example, increasing ocean acidity, altered biogeochemistry, changing current patterns, loss of sea ice...for example, large swings in the populations of commercial fisheries, changes in seabird-population distributions, and coral - reef -bleaching events

  2. Cascading influence of inorganic nitrogen sources on DOM production, composition, lability and microbial community structure in the open ocean.

    PubMed

    Goldberg, S J; Nelson, C E; Viviani, D A; Shulse, C N; Church, M J

    2017-09-01

    Nitrogen frequently limits oceanic photosynthesis and the availability of inorganic nitrogen sources in the surface oceans is shifting with global change. We evaluated the potential for abrupt increases in inorganic N sources to induce cascading effects on dissolved organic matter (DOM) and microbial communities in the surface ocean. We collected water from 5 m depth in the central North Pacific and amended duplicate 20 liter polycarbonate carboys with nitrate or ammonium, tracking planktonic carbon fixation, DOM production, DOM composition and microbial community structure responses over 1 week relative to controls. Both nitrogen sources stimulated bulk phytoplankton, bacterial and DOM production and enriched Synechococcus and Flavobacteriaceae; ammonium enriched for oligotrophic Actinobacteria OM1 and Gammaproteobacteria KI89A clades while nitrate enriched Gammaproteobacteria SAR86, SAR92 and OM60 clades. DOM resulting from both N enrichments was more labile and stimulated growth of copiotrophic Gammaproteobacteria (Alteromonadaceae and Oceanospirillaceae) and Alphaproteobacteria (Rhodobacteraceae and Hyphomonadaceae) in weeklong dark incubations relative to controls. Our study illustrates how nitrogen pulses may have direct and cascading effects on DOM composition and microbial community dynamics in the open ocean. © 2017 Society for Applied Microbiology and John Wiley & Sons Ltd.

  3. Small-scale open ocean currents have large effects on wind wave heights

    NASA Astrophysics Data System (ADS)

    Ardhuin, Fabrice; Gille, Sarah T.; Menemenlis, Dimitris; Rocha, Cesar B.; Rascle, Nicolas; Chapron, Bertrand; Gula, Jonathan; Molemaker, Jeroen

    2017-06-01

    Tidal currents and large-scale oceanic currents are known to modify ocean wave properties, causing extreme sea states that are a hazard to navigation. Recent advances in the understanding and modeling capability of open ocean currents have revealed the ubiquitous presence of eddies, fronts, and filaments at scales 10-100 km. Based on realistic numerical models, we show that these structures can be the main source of variability in significant wave heights at scales less than 200 km, including important variations down to 10 km. Model results are consistent with wave height variations along satellite altimeter tracks, resolved at scales larger than 50 km. The spectrum of significant wave heights is found to be of the order of 70>>2/>(g2>>2>) times the current spectrum, where >> is the spatially averaged significant wave height, >> is the energy-averaged period, and g is the gravity acceleration. This variability induced by currents has been largely overlooked in spite of its relevance for extreme wave heights and remote sensing.Plain Language SummaryWe show that the variations in currents at scales 10 to 100 km are the main source of variations in wave heights at the same scales. Our work uses a combination of realistic numerical models for currents and waves and data from the Jason-3 and SARAL/AltiKa satellites. This finding will be of interest for the investigation of extreme wave heights, remote sensing, and air-sea interactions. As an immediate application, the present results will help constrain the error budget of the up-coming satellite missions, in particular the Surface <span class="hlt">Water</span> and <span class="hlt">Ocean</span> Topography (SWOT) mission, and decide how the data will have to be processed to arrive at accurate sea level and wave measurements. It will also help in the analysis of wave measurements by the CFOSAT satellite.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOS.B34B0367J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOS.B34B0367J"><span>Seven persistent misconceptions about <span class="hlt">Ocean</span> Nourishment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jones, I.</p> <p>2016-02-01</p> <p>Ian S F Jones <span class="hlt">Ocean</span> Technology Group University of Sydney, F09 Australia The productivity of the <span class="hlt">open</span> <span class="hlt">ocean</span> is dependent on the flow of nutrients most of which are upwelled from the deep <span class="hlt">ocean</span>. The natural limitation posed by the restricted supply of nutrients in the soil has been overcome in agriculture by supplying mined or manufactured nutrients. This has increased the productivity of the arable land by a factor of five. Purposeful <span class="hlt">ocean</span> fertilisation, in contrast, has rarely been practiced in part because of a number of concerns about the potential environmental impacts. In some regions of the <span class="hlt">ocean</span> iron is the limiting nutrient while in the majority of the <span class="hlt">ocean</span>, the macronutrient nitrogen limits phytoplankton growth. The fertilization with macronutrients, has been termed <span class="hlt">Ocean</span> Nourishment and has a number of differences to fertilisation by iron. Some misunderstandings arise because analogies of coastal eutrophication and iron fertilisation are uncritically assumed to apply to macronutrient fertilisation. Seven misunderstandings persist and now can be discounted; Export will be low due to enhancement of the microbial loop. Phosphate and silica will need to be supplied. The quantity and cost of nitrogen make carbon sequestration uneconomic Fertilisation with urea encourages dinoflagellates. Size distribution will unsuitable (too small) for zooplankton and herbivorous fish. Fertilization will cause alarming levels of oxygen consumption. Implementation carries large ecological risk. For low fertilisation concentrations, away from shallow <span class="hlt">water</span>, in a prevailing current, in temperate <span class="hlt">waters</span>, the seven concerns above can be shown to be mild enough to justify <span class="hlt">open</span> <span class="hlt">ocean</span> small scale scientific experimentation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSME53A..01P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSME53A..01P"><span>Applications of Geostationary <span class="hlt">Ocean</span> Color Imager (GOCI) observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Park, Y. J.</p> <p>2016-02-01</p> <p><span class="hlt">Ocean</span> color remote-sensing technique <span class="hlt">opened</span> a new era for biological oceanography by providing the global distribution of phytoplankton biomass every a few days. It has been proved useful for a variety of applications in coastal <span class="hlt">waters</span> as well as <span class="hlt">oceanic</span> <span class="hlt">waters</span>. However, most <span class="hlt">ocean</span> color sensors deliver less than one image per day for low and middle latitude areas, and this once a day image is insufficient to resolve transient or high frequency processes. Korean Geostationary <span class="hlt">Ocean</span> Color Imager (GOCI), the first ever <span class="hlt">ocean</span> color instrument operated on geostationary orbit, is collecting <span class="hlt">ocean</span> color radiometry (OCR) data (multi-band radiances at the visible to NIR spectral wavelengths) since July, 2010. GOCI has an unprecedented capability to provide eight OCR images a day with a 500m resolution for the North East Asian seas Monitoring the spatial and temporal variability is important to understand many processes occurring in <span class="hlt">open</span> <span class="hlt">ocean</span> and coastal environments. With a series of images consecutively acquired by GOCI, we are now able to look into (sub-)diurnal variabilities of coastal <span class="hlt">ocean</span> color products such as phytoplankton biomass, suspended particles concentrations, and primary production. The eight images taken a day provide another way to derive maps of <span class="hlt">ocean</span> current velocity. Compared to polar orbiters, GOCI delivers more frequent images with constant viewing angle, which enables to better monitor and thus respond to coastal <span class="hlt">water</span> issues such as harmful algal blooms, floating green and brown algae. The frequent observation capability for local area allows us to respond timely to natural disasters and hazards. GOCI images are often useful to identify sea fog, sea ice, wild fires, volcanic eruptions, transport of dust aerosols, snow covered area, etc.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22348175-water-cycling-between-ocean-mantle-super-earths-need-waterworlds','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22348175-water-cycling-between-ocean-mantle-super-earths-need-waterworlds"><span><span class="hlt">Water</span> cycling between <span class="hlt">ocean</span> and mantle: Super-earths need not be waterworlds</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>Cowan, Nicolas B.; Abbot, Dorian S., E-mail: n-cowan@northwestern.edu</p> <p>2014-01-20</p> <p>Large terrestrial planets are expected to have muted topography and deep <span class="hlt">oceans</span>, implying that most super-Earths should be entirely covered in <span class="hlt">water</span>, so-called waterworlds. This is important because waterworlds lack a silicate weathering thermostat so their climate is predicted to be less stable than that of planets with exposed continents. In other words, the continuously habitable zone for waterworlds is much narrower than for Earth-like planets. A planet's <span class="hlt">water</span> is partitioned, however, between a surface reservoir, the <span class="hlt">ocean</span>, and an interior reservoir, the mantle. Plate tectonics transports <span class="hlt">water</span> between these reservoirs on geological timescales. Degassing of melt at mid-<span class="hlt">ocean</span> ridgesmore » and serpentinization of <span class="hlt">oceanic</span> crust depend negatively and positively on seafloor pressure, respectively, providing a stabilizing feedback on long-term <span class="hlt">ocean</span> volume. Motivated by Earth's approximately steady-state deep <span class="hlt">water</span> cycle, we develop a two-box model of the hydrosphere and derive steady-state solutions to the <span class="hlt">water</span> partitioning on terrestrial planets. Critically, hydrostatic seafloor pressure is proportional to surface gravity, so super-Earths with a deep <span class="hlt">water</span> cycle will tend to store more <span class="hlt">water</span> in the mantle. We conclude that a tectonically active terrestrial planet of any mass can maintain exposed continents if its <span class="hlt">water</span> mass fraction is less than ∼0.2%, dramatically increasing the odds that super-Earths are habitable. The greatest source of uncertainty in our study is Earth's current mantle <span class="hlt">water</span> inventory: the greater its value, the more robust planets are to inundation. Lastly, we discuss how future missions can test our hypothesis by mapping the <span class="hlt">oceans</span> and continents of massive terrestrial planets.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1711616B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1711616B"><span>FixO3: Advancement towards <span class="hlt">Open</span> <span class="hlt">Ocean</span> Observatory Data Management Harmonisation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Behnken, Andree; Pagnani, Maureen; Huber, Robert; Lampitt, Richard</p> <p>2015-04-01</p> <p>Since 2002 there has been a sustained effort, supported as European framework projects, to harmonise both the technology and the data management of <span class="hlt">Open</span> <span class="hlt">Ocean</span> fixed observatories run by European nations. FixO3 started in September 2013, and for 3 more years will coordinate the convergence of data management best practice across a constellation of moorings in the Atlantic, in both hemispheres, and in the Mediterranean. To ensure the continued existence of these unique sources of oceanographic data as sustained observatories it is vital to improve access to the data collected, both in terms of methods of presentation, real-time availability, long-term archiving and quality assurance. The data management component of FixO3 improves access to marine observatory data by harmonising data management standards, formats and workflows covering the complete life cycle of data from real time data acquisition to long-term archiving. Legal and data policy aspects have been examined and discussed to identify transnational barriers to <span class="hlt">open</span>-access to marine observatory data. As a result, a harmonised FixO3 data policy was drafted, which provides a formal basis for data exchange between FixO3 infrastructures, and also enables <span class="hlt">open</span> access to data for the general public. FixO3 interacts with other European infrastructures such as EMODnet, SeaDataNet, PANGAEA, and especially aims to harmonise efforts with <span class="hlt">Ocean</span>Sites and My<span class="hlt">Ocean</span>. The project landing page (www.fixo3.eu) offers detailed information about every observatory as well as data visualisations and direct downloads. In addition to this, metadata for all FixO3 - relevant data are available from the searchable FixO3 metadata catalogue, which is also accessible from the project web page. This catalogue is hosted by PANGAEA and receives updates in regular intervals. The FixO3 Standards & Services registry ties in with the GEOSS Components and Services Registry (CSR) and provides additional observatory information. The data management</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-s04-41-1206.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-s04-41-1206.html"><span>Clouds and <span class="hlt">Open</span> <span class="hlt">Ocean</span> near the Bahamas</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>1982-07-04</p> <p>STS004-41-1206 (27 June-4July 1982) --- Sunglint reflects off the <span class="hlt">water</span> of the North Atlantic <span class="hlt">Ocean</span> in an area to the east of the Bahamas Islands sometimes called the Sargasso Sea. The area has also been referred to as the ?Bermuda Triangle.? Astronauts Thomas K. Mattingly II, STS-4 commander, and Henry W. Hartsfield Jr., pilot, spent seven days and one hour aboard the Earth-orbiting space shuttle Columbia and performed a variety of duties in addition to those of recording 70mm and 35mm imagery. Photo credit: NASA</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29483242','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29483242"><span>Convergence of marine megafauna movement patterns in coastal and <span class="hlt">open</span> <span class="hlt">oceans</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sequeira, A M M; Rodríguez, J P; Eguíluz, V M; Harcourt, R; Hindell, M; Sims, D W; Duarte, C M; Costa, D P; Fernández-Gracia, J; Ferreira, L C; Hays, G C; Heupel, M R; Meekan, M G; Aven, A; Bailleul, F; Baylis, A M M; Berumen, M L; Braun, C D; Burns, J; Caley, M J; Campbell, R; Carmichael, R H; Clua, E; Einoder, L D; Friedlaender, Ari; Goebel, M E; Goldsworthy, S D; Guinet, C; Gunn, J; Hamer, D; Hammerschlag, N; Hammill, M; Hückstädt, L A; Humphries, N E; Lea, M-A; Lowther, A; Mackay, A; McHuron, E; McKenzie, J; McLeay, L; McMahon, C R; Mengersen, K; Muelbert, M M C; Pagano, A M; Page, B; Queiroz, N; Robinson, P W; Shaffer, S A; Shivji, M; Skomal, G B; Thorrold, S R; Villegas-Amtmann, S; Weise, M; Wells, R; Wetherbee, B; Wiebkin, A; Wienecke, B; Thums, M</p> <p>2018-03-20</p> <p>The extent of increasing anthropogenic impacts on large marine vertebrates partly depends on the animals' movement patterns. Effective conservation requires identification of the key drivers of movement including intrinsic properties and extrinsic constraints associated with the dynamic nature of the environments the animals inhabit. However, the relative importance of intrinsic versus extrinsic factors remains elusive. We analyze a global dataset of ∼2.8 million locations from >2,600 tracked individuals across 50 marine vertebrates evolutionarily separated by millions of years and using different locomotion modes (fly, swim, walk/paddle). Strikingly, movement patterns show a remarkable convergence, being strongly conserved across species and independent of body length and mass, despite these traits ranging over 10 orders of magnitude among the species studied. This represents a fundamental difference between marine and terrestrial vertebrates not previously identified, likely linked to the reduced costs of locomotion in <span class="hlt">water</span>. Movement patterns were primarily explained by the interaction between species-specific traits and the habitat(s) they move through, resulting in complex movement patterns when moving close to coasts compared with more predictable patterns when moving in <span class="hlt">open</span> <span class="hlt">oceans</span>. This distinct difference may be associated with greater complexity within coastal microhabitats, highlighting a critical role of preferred habitat in shaping marine vertebrate global movements. Efforts to develop understanding of the characteristics of vertebrate movement should consider the habitat(s) through which they move to identify how movement patterns will alter with forecasted severe <span class="hlt">ocean</span> changes, such as reduced Arctic sea ice cover, sea level rise, and declining oxygen content.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28769035','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28769035"><span>Spiraling pathways of global deep <span class="hlt">waters</span> to the surface of the Southern <span class="hlt">Ocean</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tamsitt, Veronica; Drake, Henri F; Morrison, Adele K; Talley, Lynne D; Dufour, Carolina O; Gray, Alison R; Griffies, Stephen M; Mazloff, Matthew R; Sarmiento, Jorge L; Wang, Jinbo; Weijer, Wilbert</p> <p>2017-08-02</p> <p>Upwelling of global deep <span class="hlt">waters</span> to the sea surface in the Southern <span class="hlt">Ocean</span> closes the global overturning circulation and is fundamentally important for <span class="hlt">oceanic</span> uptake of carbon and heat, nutrient resupply for sustaining <span class="hlt">oceanic</span> biological production, and the melt rate of ice shelves. However, the exact pathways and role of topography in Southern <span class="hlt">Ocean</span> upwelling remain largely unknown. Here we show detailed upwelling pathways in three dimensions, using hydrographic observations and particle tracking in high-resolution models. The analysis reveals that the northern-sourced deep <span class="hlt">waters</span> enter the Antarctic Circumpolar Current via southward flow along the boundaries of the three <span class="hlt">ocean</span> basins, before spiraling southeastward and upward through the Antarctic Circumpolar Current. Upwelling is greatly enhanced at five major topographic features, associated with vigorous mesoscale eddy activity. Deep <span class="hlt">water</span> reaches the upper <span class="hlt">ocean</span> predominantly south of the Antarctic Circumpolar Current, with a spatially nonuniform distribution. The timescale for half of the deep <span class="hlt">water</span> to upwell from 30° S to the mixed layer is ~60-90 years.Deep <span class="hlt">waters</span> of the Atlantic, Pacific and Indian <span class="hlt">Oceans</span> upwell in the Southern Oceanbut the exact pathways are not fully characterized. Here the authors present a three dimensional view showing a spiralling southward path, with enhanced upwelling by eddy-transport at topographic hotspots.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/18619650','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/18619650"><span>Skipjack tuna as a bioindicator of contamination by perfluorinated compounds in the <span class="hlt">oceans</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hart, Kimberly; Kannan, Kurunthachalam; Tao, Lin; Takahashi, Shin; Tanabe, Shinsuke</p> <p>2008-09-15</p> <p>Perfluorinated chemicals (PFCs) have emerged as global environmental contaminants. Studies have reported the widespread occurrence of PFCs in biota from marine coastal <span class="hlt">waters</span> and in remote polar regions. However, few studies have reported the distribution of PFCs in biota from offshore <span class="hlt">waters</span> and <span class="hlt">open</span> <span class="hlt">oceans</span>. In this study, concentrations of nine PFCs were determined in the livers of 60 skipjack tuna (Katsuwonus pelamis) collected from offshore <span class="hlt">waters</span> and the <span class="hlt">open</span> <span class="hlt">ocean</span> along the Pacific Rim, including the Sea of Japan, the East China Sea, the Indian <span class="hlt">Ocean</span>, and the Western North Pacific <span class="hlt">Ocean</span>, during 1997-1999. At least one of the nine PFCs was found in every tuna sample analyzed. Overall, perfluorooctanesulfonate (PFOS) and perfluoroundecanoic acid (PFUnDA) were the predominant compounds found in livers of tuna at concentrations of <1-58.9 and <1-31.6 ng/g, wet wt, respectively. Long-chain perfluorocarboxylates such as perfluorodecanoic acid (PFDA) and perfluorododecanoic acid (PFDoDA) were common in the tuna livers. In livers of tuna from several offshore and <span class="hlt">open-ocean</span> locations, concentrations of PFUnDA were greater than the concentrations of PFOS. The profiles and concentrations of PFCs in tuna livers suggest that the sources in East Asia are dominated by long-chain perfluorocarboxylates, especially PFUnDA. High concentrations of PFUnDA in tuna may indicate a shift in sources of PFCs in East Asia. The spatial distribution of PFOS in skipjack tuna reflected the concentrations previously reported in seawater samples from the Pacific and Indian <span class="hlt">Oceans</span>, suggesting that tuna are good bioindicators of pollution by PFOS. Despite its predominance in <span class="hlt">ocean</span> <span class="hlt">waters</span>, PFOA was rarely found in tuna livers, indicative of the low bioaccumulation potential of this compound. Our study establishes baseline concentrations of PFCs in skipjack tuna from the <span class="hlt">oceans</span> of the Asia-Pacific region, enabling future temporal trend studies of PFCs in <span class="hlt">oceans</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C42B..05K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C42B..05K"><span>Detection of Sea Ice and <span class="hlt">Open</span> <span class="hlt">Water</span> from RADARSAT-2 Images for Data Assimilation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Komarov, A.; Buehner, M.</p> <p>2016-12-01</p> <p>Automated detection of sea ice and <span class="hlt">open</span> <span class="hlt">water</span> from SAR data is very important for further assimilation into coupled <span class="hlt">ocean</span>-sea ice-atmosphere numerical models, such as the Regional Ice-<span class="hlt">Ocean</span> Prediction System being implemented at the Environment and Climate Change Canada. Conventional classification approaches based on various learning techniques are found to be limited by the fact that they typically do not indicate the level of confidence for ice and <span class="hlt">water</span> retrievals. Meanwhile, only ice/<span class="hlt">water</span> retrievals with a very high level of confidence are allowed to be assimilated into the sea ice model to avoid propagating and magnifying errors into the numerical prediction system. In this study we developed a new technique for ice and <span class="hlt">water</span> detection from dual-polarization RADARSAT-2 HH-HV images which provides the probability of ice/<span class="hlt">water</span> at a given location. We collected many hundreds of thousands of SAR signatures over various sea ice types (i.e. new, grey, first-year, and multi-year ice) and <span class="hlt">open</span> <span class="hlt">water</span> from all available RADARSAT-2 images and the corresponding Canadian Ice Service Image Analysis products over the period from November 2010 to May 2016. Our analysis of the dataset revealed that ice/<span class="hlt">water</span> separation can be effectively performed in the space of SAR-based variables independent of the incidence angle and noise floor (such as texture measures) and auxiliary Global Environmental Multiscale Model parameters (such as surface wind speed). Choice of the parameters will be specifically discussed in the presentation. An ice probability empirical model as a function of the selected predictors was built in a form of logistic regression, based on the training dataset from 2012 to 2016. The developed ice probability model showed very good performance on the independent testing subset (year 2011). With the ice/<span class="hlt">water</span> probability threshold of 0.95 reflecting a very high level of confidence, 79% of the testing ice and <span class="hlt">water</span> samples were classified with the accuracy of 99</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006Natur.441..606B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006Natur.441..606B"><span>Episodic fresh surface <span class="hlt">waters</span> in the Eocene Arctic <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brinkhuis, Henk; Schouten, Stefan; Collinson, Margaret E.; Sluijs, Appy; Damsté, Jaap S. Sinninghe; Dickens, Gerald R.; Huber, Matthew; Cronin, Thomas M.; Onodera, Jonaotaro; Takahashi, Kozo; Bujak, Jonathan P.; Stein, Ruediger; van der Burgh, Johan; Eldrett, James S.; Harding, Ian C.; Lotter, André F.; Sangiorgi, Francesca; Cittert, Han Van Konijnenburg-Van; de Leeuw, Jan W.; Matthiessen, Jens; Backman, Jan; Moran, Kathryn; Expedition 302 Scientists</p> <p>2006-06-01</p> <p>It has been suggested, on the basis of modern hydrology and fully coupled palaeoclimate simulations, that the warm greenhouse conditions that characterized the early Palaeogene period (55-45Myr ago) probably induced an intensified hydrological cycle with precipitation exceeding evaporation at high latitudes. Little field evidence, however, has been available to constrain <span class="hlt">oceanic</span> conditions in the Arctic during this period. Here we analyse Palaeogene sediments obtained during the Arctic Coring Expedition, showing that large quantities of the free-floating fern Azolla grew and reproduced in the Arctic <span class="hlt">Ocean</span> by the onset of the middle Eocene epoch (~50Myr ago). The Azolla and accompanying abundant freshwater organic and siliceous microfossils indicate an episodic freshening of Arctic surface <span class="hlt">waters</span> during an ~800,000-year interval. The abundant remains of Azolla that characterize basal middle Eocene marine deposits of all Nordic seas probably represent transported assemblages resulting from freshwater spills from the Arctic <span class="hlt">Ocean</span> that reached as far south as the North Sea. The termination of the Azolla phase in the Arctic coincides with a local sea surface temperature rise from ~10°C to 13°C, pointing to simultaneous increases in salt and heat supply owing to the influx of <span class="hlt">waters</span> from adjacent <span class="hlt">oceans</span>. We suggest that onset and termination of the Azolla phase depended on the degree of <span class="hlt">oceanic</span> exchange between Arctic <span class="hlt">Ocean</span> and adjacent seas.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70030357','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70030357"><span>Episodic fresh surface <span class="hlt">waters</span> in the Eocene Arctic <span class="hlt">Ocean</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>Brinkhuis, H.; Schouten, S.; Collinson, M.E.; Sluijs, A.; Damste, J.S.S.; Dickens, G.R.; Huber, M.; Cronin, T. M.; Onodera, J.; Takahashi, K.; Bujak, J.P.; Stein, R.; Van Der Burgh, J.; Eldrett, J.S.; Harding, I.C.; Lotter, A.F.; Sangiorgi, F.; Cittert, H.V.K.V.; De Leeuw, J. W.; Matthiessen, J.; Backman, J.; Moran, K.</p> <p>2006-01-01</p> <p>It has been suggested, on the basis of modern hydrology and fully coupled palaeoclimate simulations, that the warm greenhouse conditions that characterized the early Palaeogene period (55-45 Myr ago) probably induced an intensified hydrological cycle with precipitation exceeding evaporation at high latitudes. Little field evidence, however, has been available to constrain <span class="hlt">oceanic</span> conditions in the Arctic during this period. Here we analyse Palaeogene sediments obtained during the Arctic Coring Expedition, showing that large quantities of the free-floating fern Azolla grew and reproduced in the Arctic <span class="hlt">Ocean</span> by the onset of the middle Eocene epoch (???50 Myr ago). The Azolla and accompanying abundant freshwater organic and siliceous microfossils indicate an episodic freshening of Arctic surface <span class="hlt">waters</span> during an ???800,000-year interval. The abundant remains of Azolla that characterize basal middle Eocene marine deposits of all Nordic seas probably represent transported assemblages resulting from freshwater spills from the Arctic <span class="hlt">Ocean</span> that reached as far south as the North Sea. The termination of the Azolla phase in the Arctic coincides with a local sea surface temperature rise from ???10??C to 13??C, pointing to simultaneous increases in salt and heat supply owing to the influx of <span class="hlt">waters</span> from adjacent <span class="hlt">oceans</span>. We suggest that onset and termination of the Azolla phase depended on the degree of <span class="hlt">oceanic</span> exchange between Arctic <span class="hlt">Ocean</span> and adjacent seas. ?? 2006 Nature Publishing Group.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010GeCoA..74.5549H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010GeCoA..74.5549H"><span>Methyl mercury distributions in relation to the presence of nano- and picophytoplankton in an <span class="hlt">oceanic</span> <span class="hlt">water</span> column (Ligurian Sea, North-western Mediterranean)</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; Cossa, Daniel; Marty, Jean-Claude; Migon, Christophe; Averty, Bernard; Dufour, Aurélie; Ras, Josephine</p> <p>2010-10-01</p> <p>Recent findings on the distribution of methylated mercury (MeHg T) in <span class="hlt">waters</span> have highlighted the importance of organic carbon remineralization on the production of these compounds in the <span class="hlt">open</span> <span class="hlt">ocean</span>. Here, we present the first time-series (20 monthly samplings between July 2007 and May 2009) of high-resolution vertical profiles (10-12 depths in a 2350 m <span class="hlt">water</span> column) of MeHg T distributions in an <span class="hlt">open</span> <span class="hlt">ocean</span> environment, the Ligurian Sea (North-western Mediterranean Sea). Concentrations varied within the sub-picomolar range (general mean: 0.30 ± 0.17 pmol L -1, n = 214) with the lowest values at the surface, increasing with depth up to the oxygen minimum zone, and decreasing slowly at greater depth. Concentrations in the surface <span class="hlt">waters</span> never exceeded 0.15 pmol L -1, while the highest concentrations (up to 0.82 pmol L -1) were associated to the hypoxycline during the autumn bloom. A detailed vertical MeHg T profile reveals a "double-peak" pattern, coincidental with the two microbial layers described by Tanaka and Rassoulzadegan (2002), the so-called "microbial food web" in the euphotic zone (<100 m) and the "microbial loop" in the aphotic zone (>100 m). Temporal variations in the MeHg T abundance and distribution in the <span class="hlt">water</span> column were linked to seasonality. The highest MeHg T concentrations were found in the oxygen minimum zone during the period of stratification, and coincide with the greatest abundance of nano- and picophytoplankton (cyanobacteria, nanoflagellates, etc.) in the euphotic layer. None of our deep MeHg T measurements (˜100 m above the sea bottom) revealed a significant sedimentary source of MeHg T. We explored the correlation between MeHg T concentrations and the apparent oxygen utilization, a proxy of organic matter remineralization, over the study period. Results of this study strengthen the hypothesis that net mercury methylation in the <span class="hlt">open</span> <span class="hlt">ocean</span> occurs in the <span class="hlt">water</span> column, is linked to organic matter regeneration, and is promoted by the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1997SPIE.2963..160L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1997SPIE.2963..160L"><span>Remote sensing reflectance and inherent optical properties of <span class="hlt">oceanic</span> <span class="hlt">waters</span> derived from above-<span class="hlt">water</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>Lee, Zhongping; Carder, Kendall L.; Steward, Robert G.; Peacock, Thomas G.; Davis, Curtiss O.; Mueller, James L.</p> <p>1997-02-01</p> <p>Remote-sensing reflectance and inherent optical properties of <span class="hlt">oceanic</span> properties of <span class="hlt">oceanic</span> <span class="hlt">waters</span> are important parameters for <span class="hlt">ocean</span> optics. Due to surface reflectance, Rrs or <span class="hlt">water</span>-leaving radiance is difficult to measure from above the surface. It usually is derived by correcting for the reflected skylight in the measured above-<span class="hlt">water</span> upwelling radiance using a theoretical Fresnel reflectance value. As it is difficult to determine the reflected skylight, there are errors in the Q and E derived Rrs, and the errors may get bigger for high chl_a coastal <span class="hlt">waters</span>. For better correction of the reflected skylight,w e propose the following derivation procedure: partition the skylight into Rayleigh and aerosol contributions, remove the Rayleigh contribution using the Fresnel reflectance, and correct the aerosol contribution using an optimization algorithm. During the process, Rrs and in-<span class="hlt">water</span> inherent optical properties are derived at the same time. For measurements of 45 sites made in the Gulf of Mexico and Arabian Sea with chl_a concentrations ranging from 0.07 to 49 mg/m3, the derived Rrs and inherent optical property values were compared with those from in-<span class="hlt">water</span> measurements. These results indicate that for the <span class="hlt">waters</span> studied, the proposed algorithm performs quite well in deriving Rrs and in- <span class="hlt">water</span> inherent optical properties from above-surface measurements for clear and turbid <span class="hlt">waters</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1343648-local-atmospheric-response-open-ocean-polynya-high-resolution-climate-model','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1343648-local-atmospheric-response-open-ocean-polynya-high-resolution-climate-model"><span>Local Atmospheric Response to an <span class="hlt">Open-Ocean</span> Polynya in a High-Resolution Climate Model</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Weijer, Wilbert; Veneziani, Milena; Stössel, Achim; ...</p> <p>2017-03-01</p> <p>For this scientific paper, we study the atmospheric response to an <span class="hlt">open-ocean</span> polynya in the Southern <span class="hlt">Ocean</span> by analyzing the results from an atmospheric and <span class="hlt">oceanic</span> synoptic-scale resolving Community Earth System Model (CESM) simulation. While coarser-resolution versions of CESM generally do not produce <span class="hlt">open-ocean</span> polynyas in the Southern <span class="hlt">Ocean</span>, they do emerge and disappear on interannual timescales in the synoptic-scale simulation. This provides an ideal opportunity to study the polynya’s impact on the overlying and surrounding atmosphere. This has been pursued here by investigating the seasonal cycle of differences of surface and air-column variables between polynya and non-polynya years. Ourmore » results indicate significant local impacts on turbulent heat fluxes, precipitation, cloud characteristics, and radiative fluxes. In particular, we find that clouds over polynyas are optically thicker and higher than clouds over sea ice during non-polynya years. Although the lower albedo of polynyas significantly increases the net shortwave absorption, the enhanced cloud brightness tempers this increase by almost 50%. Also, in this model, enhanced longwave radiation emitted from the warmer surface of polynyas is balanced by stronger downwelling fluxes from the thicker cloud deck. Impacts are found to be sensitive to the synoptic wind direction. Strongest regional impacts are found when northeasterly winds cross the polynya and interact with katabatic winds. Finally, surface air pressure anomalies over the polynya are only found to be significant when cold, dry air masses strike over the polynya, i.e. in case of southerly winds.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1343648-local-atmospheric-response-open-ocean-polynya-high-resolution-climate-model','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1343648-local-atmospheric-response-open-ocean-polynya-high-resolution-climate-model"><span>Local Atmospheric Response to an <span class="hlt">Open-Ocean</span> Polynya in a High-Resolution Climate Model</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>Weijer, Wilbert; Veneziani, Milena; Stössel, Achim</p> <p></p> <p>For this scientific paper, we study the atmospheric response to an <span class="hlt">open-ocean</span> polynya in the Southern <span class="hlt">Ocean</span> by analyzing the results from an atmospheric and <span class="hlt">oceanic</span> synoptic-scale resolving Community Earth System Model (CESM) simulation. While coarser-resolution versions of CESM generally do not produce <span class="hlt">open-ocean</span> polynyas in the Southern <span class="hlt">Ocean</span>, they do emerge and disappear on interannual timescales in the synoptic-scale simulation. This provides an ideal opportunity to study the polynya’s impact on the overlying and surrounding atmosphere. This has been pursued here by investigating the seasonal cycle of differences of surface and air-column variables between polynya and non-polynya years. Ourmore » results indicate significant local impacts on turbulent heat fluxes, precipitation, cloud characteristics, and radiative fluxes. In particular, we find that clouds over polynyas are optically thicker and higher than clouds over sea ice during non-polynya years. Although the lower albedo of polynyas significantly increases the net shortwave absorption, the enhanced cloud brightness tempers this increase by almost 50%. Also, in this model, enhanced longwave radiation emitted from the warmer surface of polynyas is balanced by stronger downwelling fluxes from the thicker cloud deck. Impacts are found to be sensitive to the synoptic wind direction. Strongest regional impacts are found when northeasterly winds cross the polynya and interact with katabatic winds. Finally, surface air pressure anomalies over the polynya are only found to be significant when cold, dry air masses strike over the polynya, i.e. in case of southerly winds.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/18365803','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/18365803"><span>Effect of the South Bay <span class="hlt">Ocean</span> Outfall (SBOO) on <span class="hlt">ocean</span> beach <span class="hlt">water</span> quality near the USA-Mexico border.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gersberg, Richard; Tiedge, Jürgen; Gottstein, Dana; Altmann, Sophie; Watanabe, Kayo; Lüderitz, Volker</p> <p>2008-04-01</p> <p>In early 1999, primary treatment and discharge of sewage from Tijuana, Mexico (approximately 95 million liters per day) began through South Bay <span class="hlt">Ocean</span> Outfall (SBOO) into the <span class="hlt">ocean</span> 4.3 km offshore. In this study, statistical comparisons were made of the bacterial <span class="hlt">water</span> quality (total and fecal coliforms and enterococci densities) of the <span class="hlt">ocean</span>, both before and after discharge of sewage to the SBOO began, so that the effect of this <span class="hlt">ocean</span> discharge on nearshore <span class="hlt">ocean</span> <span class="hlt">water</span> quality could be quantitatively assessed. The frequency of exceedence of bacterial indicator thresholds was statistically analyzed for 11 shore (surfzone) stations throughout US and Mexico using the Fisher's exact test, for the years before (1995-1998) as compared to after the SBOO discharge began (1999-2003). Only four of the 11 shoreline stations (S2, S3, S11, and S12) showed significant improvement (decreased frequency of exceedence of bacterial indicator thresholds) after SBOO discharge began.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C14A..01W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C14A..01W"><span><span class="hlt">Oceans</span> Melting Greenland (OMG): 2017 Observations and the First Look at Yearly <span class="hlt">Ocean</span>/Ice Changes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Willis, J. K.; Rignot, E. J.; Fenty, I. G.; Khazendar, A.; Moller, D.; Tinto, K. J.; Morison, J.; Schodlok, M.; Thompson, A. F.; Fukumori, I.; Holland, D.; Forsberg, R.; Jakobsson, M.; Dinardo, S. J.</p> <p>2017-12-01</p> <p><span class="hlt">Oceans</span> Melting Greenland (OMG) is an airborne NASA Mission to investigate the role of the <span class="hlt">oceans</span> in ice loss around the margins of the Greenland Ice Sheet. A five-year campaign, OMG will directly measure <span class="hlt">ocean</span> warming and glacier retreat around all of Greenland. By relating these two, we will explore one of the most pressing <span class="hlt">open</span> questions about how climate change drives sea level rise: How quickly are the warming <span class="hlt">oceans</span> melting the Greenland Ice Sheet from the edges? This year, OMG collected its second set of both elevation maps of marine terminating glaciers and <span class="hlt">ocean</span> temperature and salinity profiles around all of Greenland. This give us our first look at year-to-year changes in both ice volume at the margins, as well as the volume and extent of warm, salty Atlantic <span class="hlt">water</span> present on the continental shelf. In addition, we will compare recent data in east Greenland <span class="hlt">waters</span> with historical <span class="hlt">ocean</span> observations that suggest a long-term warming trend there. Finally, we will briefly review the multi-beam sonar and airborne gravity campaigns—both of which were completed last year—and the dramatic improvement they had on bathymetry maps over the continental shelf around Greenland.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li class="active"><span>8</span></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_8 --> <div id="page_9" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li class="active"><span>9</span></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="161"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27027776','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27027776"><span><span class="hlt">Oceanic</span> oxygenation events in the anoxic Ediacaran <span class="hlt">ocean</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sahoo, S K; Planavsky, N J; Jiang, G; Kendall, B; Owens, J D; Wang, X; Shi, X; Anbar, A D; Lyons, T W</p> <p>2016-09-01</p> <p>The <span class="hlt">ocean</span>-atmosphere system is typically envisioned to have gone through a unidirectional oxygenation with significant oxygen increases in the earliest (ca. 635 Ma), middle (ca. 580 Ma), or late (ca. 560 Ma) Ediacaran Period. However, temporally discontinuous geochemical data and the patchy metazoan fossil record have been inadequate to chart the details of Ediacaran <span class="hlt">ocean</span> oxygenation, raising fundamental debates about the timing of <span class="hlt">ocean</span> oxygenation, its purported unidirectional rise, and its causal relationship, if any, with the evolution of early animal life. To better understand the Ediacaran <span class="hlt">ocean</span> redox evolution, we have conducted a multi-proxy paleoredox study of a relatively continuous, deep-<span class="hlt">water</span> section in South China that was paleogeographically connected with the <span class="hlt">open</span> <span class="hlt">ocean</span>. Iron speciation and pyrite morphology indicate locally euxinic (anoxic and sulfidic) environments throughout the Ediacaran in this section. In the same rocks, redox sensitive element enrichments and sulfur isotope data provide evidence for multiple <span class="hlt">oceanic</span> oxygenation events (OOEs) in a predominantly anoxic global Ediacaran-early Cambrian <span class="hlt">ocean</span>. This dynamic redox landscape contrasts with a recent view of a redox-static Ediacaran <span class="hlt">ocean</span> without significant change in oxygen content. The duration of the Ediacaran OOEs may be comparable to those of the <span class="hlt">oceanic</span> anoxic events (OAEs) in otherwise well-oxygenated Phanerozoic <span class="hlt">oceans</span>. Anoxic events caused mass extinctions followed by fast recovery in biologically diversified Phanerozoic <span class="hlt">oceans</span>. In contrast, oxygenation events in otherwise ecologically monotonous anoxic Ediacaran-early Cambrian <span class="hlt">oceans</span> may have stimulated biotic innovations followed by prolonged evolutionary stasis. © 2016 John Wiley & Sons Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA527419','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA527419"><span>An Autonomous Mobile Platform for Underway Surface Carbon Measurements in <span class="hlt">Open-Ocean</span> and Coastal <span class="hlt">Waters</span></span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2010-06-01</p> <p>Sarmiento , J ., Stephens, B. and Weller, R., 2004. <span class="hlt">Ocean</span> Carbon and Climate Change (OCCC): An Implementation Strategy for U. S. <span class="hlt">Ocean</span> Carbon Cycle...M. Ishii, T. Midorikawa, Y. Nojiri, A. Körtzinger, T. Steinhoff, M. Hopemma, J . Olafsson, T.S. Arnarson, B. Tilbrook, T. Johannessen, A. Olsen, R...Biogeochemical Cycles, 19, GB1009, 10.1029/2004GB002295. [5] Cai, W.- J ., Dai, M. and Wang, Y., 2006. Air-sea exchange of carbon dioxide in <span class="hlt">ocean</span> margins: A</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26213672','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26213672"><span>The salinity signature of the cross-shelf exchanges in the Southwestern Atlantic <span class="hlt">Ocean</span>: Satellite observations.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Guerrero, Raul A; Piola, Alberto R; Fenco, Harold; Matano, Ricardo P; Combes, Vincent; Chao, Yi; James, Corinne; Palma, Elbio D; Saraceno, Martin; Strub, P Ted</p> <p>2014-11-01</p> <p>Satellite-derived sea surface salinity (SSS) data from Aquarius and SMOS are used to study the shelf-<span class="hlt">open</span> <span class="hlt">ocean</span> exchanges in the western South Atlantic near 35°S. Away from the tropics, these exchanges cause the largest SSS variability throughout the South Atlantic. The data reveal a well-defined seasonal pattern of SSS during the analyzed period and of the location of the export of low-salinity shelf <span class="hlt">waters</span>. In spring and summer, low-salinity <span class="hlt">waters</span> over the shelf expand offshore and are transferred to the <span class="hlt">open</span> <span class="hlt">ocean</span> primarily southeast of the river mouth (from 36°S to 37°30'S). In contrast, in fall and winter, low-salinity <span class="hlt">waters</span> extend along a coastal plume and the export path to the <span class="hlt">open</span> <span class="hlt">ocean</span> distributes along the offshore edge of the plume. The strong seasonal SSS pattern is modulated by the seasonality of the along-shelf component of the wind stress over the shelf. However, the combined analysis of SSS, satellite-derived sea surface elevation and surface velocity data suggest that the precise location of the export of shelf <span class="hlt">waters</span> depends on offshore circulation patterns, such as the location of the Brazil Malvinas Confluence and mesoscale eddies and meanders of the Brazil Current. The satellite data indicate that in summer, mixtures of low-salinity shelf <span class="hlt">waters</span> are swiftly driven toward the <span class="hlt">ocean</span> interior along the axis of the Brazil/Malvinas Confluence. In winter, episodic wind reversals force the low-salinity coastal plume offshore where they mix with tropical <span class="hlt">waters</span> within the Brazil Current and create a warmer variety of low-salinity <span class="hlt">waters</span> in the <span class="hlt">open</span> <span class="hlt">ocean</span>. Satellite salinity sensors capture low-salinity detrainment events from shelves SW Atlantic low-salinity detrainments cause highest basin-scale variability In summer low-salinity detrainments cause extended low-salinity anomalies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4508963','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4508963"><span>The salinity signature of the cross-shelf exchanges in the Southwestern Atlantic <span class="hlt">Ocean</span>: Satellite observations</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Guerrero, Raul A; Piola, Alberto R; Fenco, Harold; Matano, Ricardo P; Combes, Vincent; Chao, Yi; James, Corinne; Palma, Elbio D; Saraceno, Martin; Strub, P Ted</p> <p>2014-01-01</p> <p>Satellite-derived sea surface salinity (SSS) data from Aquarius and SMOS are used to study the shelf-<span class="hlt">open</span> <span class="hlt">ocean</span> exchanges in the western South Atlantic near 35°S. Away from the tropics, these exchanges cause the largest SSS variability throughout the South Atlantic. The data reveal a well-defined seasonal pattern of SSS during the analyzed period and of the location of the export of low-salinity shelf <span class="hlt">waters</span>. In spring and summer, low-salinity <span class="hlt">waters</span> over the shelf expand offshore and are transferred to the <span class="hlt">open</span> <span class="hlt">ocean</span> primarily southeast of the river mouth (from 36°S to 37°30′S). In contrast, in fall and winter, low-salinity <span class="hlt">waters</span> extend along a coastal plume and the export path to the <span class="hlt">open</span> <span class="hlt">ocean</span> distributes along the offshore edge of the plume. The strong seasonal SSS pattern is modulated by the seasonality of the along-shelf component of the wind stress over the shelf. However, the combined analysis of SSS, satellite-derived sea surface elevation and surface velocity data suggest that the precise location of the export of shelf <span class="hlt">waters</span> depends on offshore circulation patterns, such as the location of the Brazil Malvinas Confluence and mesoscale eddies and meanders of the Brazil Current. The satellite data indicate that in summer, mixtures of low-salinity shelf <span class="hlt">waters</span> are swiftly driven toward the <span class="hlt">ocean</span> interior along the axis of the Brazil/Malvinas Confluence. In winter, episodic wind reversals force the low-salinity coastal plume offshore where they mix with tropical <span class="hlt">waters</span> within the Brazil Current and create a warmer variety of low-salinity <span class="hlt">waters</span> in the <span class="hlt">open</span> <span class="hlt">ocean</span>. Key Points Satellite salinity sensors capture low-salinity detrainment events from shelves SW Atlantic low-salinity detrainments cause highest basin-scale variability In summer low-salinity detrainments cause extended low-salinity anomalies PMID:26213672</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.B42C..02Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.B42C..02Z"><span>Exploring Metabolic Activities of Deeply Buried Microbial Communities in Oxic Sediments Underlying Oligotrophic <span class="hlt">Open</span> <span class="hlt">Ocean</span> Gyres</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ziebis, W.; Patel, A.; Krupke, A.; Ferdelman, T. G.</p> <p>2012-12-01</p> <p>The vast majority of scientific drilling expeditions have focused on continental margins where oxygen is depleted within the surface (1 m) layer of the sediment and buried organic carbon sustains anaerobic microbial communities. IODP expeditions 329 (South Pacific Gyre) and 336 (Mid-Atlantic Ridge - North Pond) took place in oligotrophic <span class="hlt">open</span> <span class="hlt">ocean</span> regions, which constitute 48% of the world <span class="hlt">ocean</span>. These expeditions have revealed that unlike continental margins the seafloor underneath oligotrophic <span class="hlt">ocean</span> gyres is oxic. Within the South Pacific Gyre (SPG) dissolved oxygen persists throughout the sediment cover and reaches the basement even at the sites with thickest sediment cover (62 and 75 mbsf). North Pond is a sedimented pond (< 300 m sediment cover) located on the flank of the Mid-Atlantic Ridge underlying the oligotrophic central Atlantic. Here, oxygen diffuses upward from the basaltic aquifer underlying the sediment package in addition to deep oxygen penetration from the overlying <span class="hlt">water</span>. Oxygen is the main electron acceptor available for sub-seafloor microbial activity in these vast oligotrophic <span class="hlt">open</span> <span class="hlt">ocean</span> regions. Microbial cells are present and active in the organic poor sediments, albeit numbers are near or below the detection limit (<103 cm-3 sediment) in the extremely organic-poor sediment of the SPG (below 2 -15 m sediment depth, depending on the location). However, we have very limited knowledge on the microbial community compositions and metabolic activities. Even the dominance of bacteria or archaea remains largely elusive. It has been suggested that while archaea dominate in the anoxic sediments of continental margins bacteria might be more abundant in the oxic seafloor underlying oligotrophic <span class="hlt">ocean</span> gyres where aerobic respiration prevails. Experiments were conducted with sediment samples from the SPG and North Pond to explore the pattern of microbial diversity and metabolic activity using a suite of radio and stable isotopes in combination with</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2013-title33-vol3/pdf/CFR-2013-title33-vol3-sec336-2.pdf','CFR2013'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2013-title33-vol3/pdf/CFR-2013-title33-vol3-sec336-2.pdf"><span>33 CFR 336.2 - Transportation of dredged material for the purpose of disposal into <span class="hlt">ocean</span> <span class="hlt">waters</span>.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2013&page.go=Go">Code of Federal Regulations, 2013 CFR</a></p> <p></p> <p>2013-07-01</p> <p>... material for the purpose of disposal into <span class="hlt">ocean</span> <span class="hlt">waters</span>. 336.2 Section 336.2 Navigation and Navigable <span class="hlt">Waters</span>... <span class="hlt">WATERS</span> OF THE U.S. AND <span class="hlt">OCEAN</span> <span class="hlt">WATERS</span> § 336.2 Transportation of dredged material for the purpose of disposal into <span class="hlt">ocean</span> <span class="hlt">waters</span>. (a) Applicable law. Section 103(a) of the ODA provides that the Corps of...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2014-title33-vol3/pdf/CFR-2014-title33-vol3-sec336-2.pdf','CFR2014'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2014-title33-vol3/pdf/CFR-2014-title33-vol3-sec336-2.pdf"><span>33 CFR 336.2 - Transportation of dredged material for the purpose of disposal into <span class="hlt">ocean</span> <span class="hlt">waters</span>.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2014&page.go=Go">Code of Federal Regulations, 2014 CFR</a></p> <p></p> <p>2014-07-01</p> <p>... material for the purpose of disposal into <span class="hlt">ocean</span> <span class="hlt">waters</span>. 336.2 Section 336.2 Navigation and Navigable <span class="hlt">Waters</span>... <span class="hlt">WATERS</span> OF THE U.S. AND <span class="hlt">OCEAN</span> <span class="hlt">WATERS</span> § 336.2 Transportation of dredged material for the purpose of disposal into <span class="hlt">ocean</span> <span class="hlt">waters</span>. (a) Applicable law. Section 103(a) of the ODA provides that the Corps of...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5510522-vertical-mercury-distributions-oceans','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5510522-vertical-mercury-distributions-oceans"><span>Vertical mercury distributions in the <span class="hlt">oceans</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>Gill, G.A.; Fitzgerald, W.F.</p> <p>1988-06-01</p> <p>The vertical distribution of mercury (Hg) was determined at coastal and <span class="hlt">open</span> <span class="hlt">ocean</span> sites in the northwest Atlantic and Pacific <span class="hlt">Oceans</span>. Reliable and diagnostic Hg distribution were obtained, permitting major processes governing the marine biogeochemistry of Hg to be identified. The northwest Atlantic near Bermuda showed surface <span class="hlt">water</span> Hg concentrations near 4 pM, a maximum of 10 pM within the main thermocline, and concentrations less than or equal to surface <span class="hlt">water</span> values below the depth of the maximum. The maximum appears to result from lateral transport of Hg enriched <span class="hlt">waters</span> from higher latitudes. In the central North Pacific, surface watersmore » (to 940 m) were slightly elevated (1.9 {plus minus} 0.7 pM) compared to deeper <span class="hlt">waters</span> (1.4 {plus minus} 0.4 pM), but on thermocline Hg maximum was observed. At similar depths, Hg concentrations near Bermuda were elevated compared to the central North Pacific <span class="hlt">Ocean</span>. The authors hypothesize that the source of this Hg comes from diagenetic reactions in oxic margin sediments, releasing dissolved Hg to overlying <span class="hlt">water</span>. Geochemical steady-state box modeling arguments predict a relatively short ({approximately}350 years) mean residence time for Hg in the <span class="hlt">oceans</span>, demonstrating the reactive nature of Hg in seawater and precluding significant involvement in nutrient-type recycling. Mercury's distributional features and reactive nature suggest that interaction of Hg with settling particulate matter and margin sediments play important roles in regulating <span class="hlt">oceanic</span> Hg concentrations. <span class="hlt">Oceanic</span> Hg distributions are governed by an external cycling process, in which <span class="hlt">water</span> column distributions reflect a rapid competition between the magnitude of the input source and the intensity of the (<span class="hlt">water</span> column) removal process.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ClDy...48.4093M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ClDy...48.4093M"><span>Interannual variability of Indian <span class="hlt">Ocean</span> subtropical mode <span class="hlt">water</span> subduction rate</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ma, Jie; Lan, Jian</p> <p>2017-06-01</p> <p>The interannual variation of Indian <span class="hlt">Ocean</span> subtropical mode <span class="hlt">water</span> (IOSTMW) subduction rate in the Southwest Indian <span class="hlt">Ocean</span> from 1980 to 2007 is investigated in this paper based on Simple <span class="hlt">Ocean</span> Data Assimilation (SODA) outputs. Climatology of subduction rate exceeds 75 m/year in the IOSTMW formation area. The renewal time of permanent pycnocline <span class="hlt">water</span> mass based on the subduction rate is calculated for each density class: 3-6 years for IOSTMW (25.8 < σ θ < 26.2 kg m-3). Subduction rate in the Southwest Indian <span class="hlt">Ocean</span> subtropical gyre exhibits a great year-to-year variability. This interannual variations of the IOSTMW subduction rate is primarily dominated by the lateral induction term, associated with the interannual variations of strong meridional gradient of winter mixed layer depth (MLD). The slope of the mixed layer depth in the mode <span class="hlt">water</span> is closely linked to the large variations of deep late winter MLD in the mid-latitudes and negligible variations of shallow winter MLD in lower latitudes. It is further identified that the interannual variation of late winter MLD in this area is largely controlled by the latent and sensible heat flux components. The <span class="hlt">water</span> volume of the permanent pycnocline in the IOSTMW distribution area is also found to show a significant interannual variability, and it is well correlated with the interannual variation of subduction rate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C41A0639L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C41A0639L"><span>Upper <span class="hlt">Ocean</span> Evolution Across the Beaufort Sea Marginal Ice Zone</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lee, C.; Rainville, L.; Gobat, J. I.; Perry, M. J.; Freitag, L. E.; Webster, S.</p> <p>2016-12-01</p> <p>The observed reduction of Arctic summertime sea ice extent and expansion of the marginal ice zone (MIZ) have profound impacts on the balance of processes controlling sea ice evolution, including the introduction of several positive feedback mechanisms that may act to accelerate melting. Examples of such feedbacks include increased upper <span class="hlt">ocean</span> warming though absorption of solar radiation, elevated internal wave energy and mixing that may entrain heat stored in subsurface watermasses (e.g., the relatively warm Pacific Summer and Atlantic <span class="hlt">waters</span>), and elevated surface wave energy that acts to deform and fracture sea ice. Spatial and temporal variability in ice properties and <span class="hlt">open</span> <span class="hlt">water</span> fraction impact these processes. To investigate how upper <span class="hlt">ocean</span> structure varies with changing ice cover, how the balance of processes shift as a function of ice fraction and distance from <span class="hlt">open</span> <span class="hlt">water</span>, and how these processes impact sea ice evolution, a network of autonomous platforms sampled the atmosphere-ice-<span class="hlt">ocean</span> system in the Beaufort, beginning in spring, well before the start of melt, and ending with the autumn freeze-up. Four long-endurance autonomous Seagliders occupied sections that extended from <span class="hlt">open</span> <span class="hlt">water</span>, through the marginal ice zone, deep into the pack during summer 2014 in the Beaufort Sea. Gliders penetrated up to 200 km into the ice pack, under complete ice cover for up to 10 consecutive days. Sections reveal strong fronts where cold, ice-covered <span class="hlt">waters</span> meet <span class="hlt">waters</span> that have been exposed to solar warming, and O(10 km) scale eddies near the ice edge. In the pack, Pacific Summer <span class="hlt">Water</span> and a deep chlorophyll maximum form distinct layers at roughly 60 m and 80 m, respectively, which become increasingly diffuse late in the season as they progress through the MIZ and into <span class="hlt">open</span> <span class="hlt">water</span>. Stratification just above the Pacific Summer <span class="hlt">Water</span> rapidly weakens near the ice edge and temperature variance increases, likely due to mixing or energetic vertical exchange associated with strong</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFMPP33A1651S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFMPP33A1651S"><span>Pushing <span class="hlt">open-ocean</span> organic paleo-environmental proxies to the margin: Narragansett Bay, RI</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Salacup, J. M.; Herbert, T.; Prell, W. L.</p> <p>2010-12-01</p> <p>Estuarine sediment deposits provide an under-utilized opportunity to reconstruct high-resolution records of environmental change from the highly sensitive intersection of <span class="hlt">oceanic</span> and terrestrial systems. Previous applications of both well-established and novel organic geochemical proxies to estuaries have met with mixed success. Compared to <span class="hlt">oceanic</span> settings, the large dynamic range of tidal currents, <span class="hlt">water</span> temperature, salinity, nutrients, and productivity both enrich and complicate estuarine sedimentary records. Here, we present the results of monthly samples of <span class="hlt">water</span>-column particulate organic matter and compare them to a suite of sediment cores in an effort to elucidate how the environmental signal produced in the <span class="hlt">water</span>-column is translated to the sediment. Specifically, we measured alkenones and glycerol dialkyl glycerol tetraethers (GDGTs), the bases for the Uk’37 sea-surface temperature (SST) and C-37total primary productivity proxies, and the TEX86 SST and BIT Index proxies, respectively. Alkenones, produced by haptophyte algae, are present in most of our <span class="hlt">water</span>-column samples; however, concentrations in many samples are too low to reliably calculate temperature. When reliable, <span class="hlt">water</span>-column alkenones infer SSTs between 13-16°C, consistent with sediment core-top Uk’37 SST estimates. These correlate to May and Oct SSTs, coinciding with the terminations of the summer-fall and winter-spring algal blooms in Narragansett Bay. In contrast to alkenone fingerprints reported from the much lower salinity Chesapeake Bay, Narragansett Bay samples lack significant contributions of the C37:4 ketone, consistent with production by <span class="hlt">open-ocean</span> haptophytes. Notably, sedimentary records of Uk’37-inferred SST show strong inter-core centennial-to-decadal coherence. The structure and absolute values of inferred SSTs correlate well with instrumental mean Sept-Oct air temperatures back to 1895, and contain structure consistent with the late Little Ice Age and 20th century</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28650623','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28650623"><span>Spatial Distributions of DDTs in the <span class="hlt">Water</span> Masses of the Arctic <span class="hlt">Ocean</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Carrizo, Daniel; Sobek, Anna; Salvadó, Joan A; Gustafsson, Örjan</p> <p>2017-07-18</p> <p>There is a scarcity of data on the amount and distribution of the organochlorine pesticide dichlorodiphenyltrichloroethane (DDT) and its metabolites in intermediate and deep <span class="hlt">ocean</span> <span class="hlt">water</span> masses. Here, the distribution and inventories of DDTs in <span class="hlt">water</span> of the Arctic shelf seas and the interior basin are presented. The occurrence of ∑ 6 DDT (0.10-66 pg L -1 ) in the surface <span class="hlt">water</span> was dominated by 4,4'-DDE. In the Central Arctic <span class="hlt">Ocean</span> increasing concentrations of DDE with depth were observed in the Makarov and Amundsen basins. The increasing concentrations down to 2500 m depth is in accordance with previous findings for PCBs and PBDEs. Similar concentrations of DDT and DDEs were found in the surface <span class="hlt">water</span>, while the relative contribution of DDEs increased with depth, demonstrating a transformation over time and depth. Higher concentrations of DDTs were found in the European part of the Arctic <span class="hlt">Ocean</span>; these distributions likely reflect a combination of different usage patterns, transport, and fate of these compounds. For instance, the elevated concentrations of DDTs in the Barents and Atlantic sectors of the Arctic <span class="hlt">Ocean</span> indicate the northbound Atlantic current as a significant conveyor of DDTs. This study contributes to the very rare data on OCPs in the vast deep-<span class="hlt">water</span> compartments and combined with surface <span class="hlt">water</span> distribution across the Arctic <span class="hlt">Ocean</span> helps to improve our understanding of the large-scale fate of DDTs in the Arctic.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.8998K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.8998K"><span>A multidisciplinary glider survey of an <span class="hlt">open</span> <span class="hlt">ocean</span> dead-zone eddy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Karstensen, Johannes; Schütte, Florian; Pietri, Alice; Krahmann, Gerd; Fiedler, Björn; Löscher, Carolin; Grundle, Damian; Hauss, Helena; Körtzinger, Arne; Testor, Pierre; Viera, Nuno</p> <p>2016-04-01</p> <p>The physical (temperature, salinity) and biogeochemical (oxygen, nitrate, chlorophyll fluorescence, turbidity) structure of an anticyclonic modewater eddy, hosting an <span class="hlt">open</span> <span class="hlt">ocean</span> dead zone, is investigated using observational data sampled in high temporal and spatial resolution with autonomous gliders in March and April 2014. The core of the eddy is identified in the glider data as a volume of fresher (on isopycnals) <span class="hlt">water</span> in the depth range from the mixed layer base (about 70m) to about 200m depth. The width is about 80km. The core aligns well with the 40 μmolkg-1 oxygen contour. From two surveys about 1 month apart, changes in the minimal oxygen concentrations (below 5μmolkg-1) are observed that indicate that small scale processes are in operation. Several scales of coherent variability of physical and biogeochemical variable are identified - from a few meters to the mesoscale. One of the gliders carried an autonomous Nitrate (N) sensor and the data is used to analyse the possible nitrogen pathways within the eddy. Also the highest N is accompanied by lowest oxygen concentrations, the AOU:N ratio reveals a preferred oxygen cycling per N.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70024918','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70024918"><span>Interaction of sea <span class="hlt">water</span> and lava during submarine eruptions at mid-<span class="hlt">ocean</span> ridges</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Perfit, M.R.; Cann, J.R.; Fornari, D.J.; Engels, J.; Smith, D.K.; Ridley, W.I.; Edwards, M.H.</p> <p>2003-01-01</p> <p>Lava erupts into cold sea <span class="hlt">water</span> on the <span class="hlt">ocean</span> floor at mid-<span class="hlt">ocean</span> ridges (at depths of 2,500 m and greater), and the resulting flows make up the upper part of the global <span class="hlt">oceanic</span> crust. Interactions between heated sea <span class="hlt">water</span> and molten basaltic lava could exert significant control on the dynamics of lava flows and on their chemistry. But it has been thought that heating sea <span class="hlt">water</span> at pressures of several hundred bars cannot produce significant amounts of vapour and that a thick crust of chilled glass on the exterior of lava flows minimizes the interaction of lava with sea <span class="hlt">water</span>. Here we present evidence to the contrary, and show that bubbles of vaporized sea <span class="hlt">water</span> often rise through the base of lava flows and collect beneath the chilled upper crust. These bubbles of steam at magmatic temperatures may interact both chemically and physically with flowing lava, which could influence our understanding of deep-sea volcanic processes and <span class="hlt">oceanic</span> crustal construction more generally. We infer that vapour formation plays an important role in creating the collapse features that characterize much of the upper <span class="hlt">oceanic</span> crust and may accordingly contribute to the measured low seismic velocities in this layer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.3696L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.3696L"><span>Fixed point <span class="hlt">Open</span> <span class="hlt">Ocean</span> Observatory network (FixO3): Multidisciplinary observations from the air-sea interface to the deep seafloor</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lampitt, Richard; Cristini, Luisa</p> <p>2014-05-01</p> <p>The Fixed point <span class="hlt">Open</span> <span class="hlt">Ocean</span> Observatory network (FixO3) seeks to integrate the 23 European <span class="hlt">open</span> <span class="hlt">ocean</span> fixed point observatories and to improve access to these key installations for the broader community. These will provide multidisciplinary observations in all parts of the <span class="hlt">oceans</span> from the air-sea interface to the deep seafloor. Coordinated by the National Oceanography Centre, UK, FixO3 builds on the significant advances achieved through the previous Europe-funded FP7 programmes EuroSITES, ESONET and CARBOOCEAN. Started in September 2013 with a budget of 7 Million Euros over 4 years the project has 29 partners drawn from academia, research institutions and SME's. In addition 12 international experts from a wide range of disciplines comprise an Advisory Board. On behalf of the FixO3 Consortium, we present the programme that will be achieved through the activities of 12 Work Packages: 1. Coordination activities to integrate and harmonise the current procedures and processes. Strong links will be fostered with the wider community across academia, industry, policy and the general public through outreach, knowledge exchange and training. 2. Support actions to offer a) free access to observatory infrastructures to those who do not have such access, and b) free and <span class="hlt">open</span> data services and products. 3. Joint research activities to innovate and enhance the current capability for multidisciplinary in situ <span class="hlt">ocean</span> observation. Support actions include Transnational Access (TNA) to FixO3 infrastructure, meaning that European organizations can apply to free-of-charge access to the observatories for research and testing in two international calls during the project lifetime. The first call for TNA <span class="hlt">opens</span> in summer 2014. More information can be found on FixO3 website (www.fixo3.eu/). <span class="hlt">Open</span> <span class="hlt">ocean</span> observation is currently a high priority for European marine and maritime activities. FixO3 will provide important data on environmental products and services to address the Marine Strategy</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20180002856','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20180002856"><span>SWIM: A Semi-Analytical <span class="hlt">Ocean</span> Color Inversion Algorithm for Optically Shallow <span class="hlt">Waters</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>McKinna, Lachlan I. W.; Werdell, P. Jeremy; Fearns, Peter R. C. S.; Weeks, Scarla J.; Reichstetter, Martina; Franz, Bryan A.; Bailey, Sean W.; Shea, Donald M.; Feldman, Gene C.</p> <p>2014-01-01</p> <p>In clear shallow <span class="hlt">waters</span>, light that is transmitted downward through the <span class="hlt">water</span> column can reflect off the sea floor and thereby influence the <span class="hlt">water</span>-leaving radiance signal. This effect can confound contemporary <span class="hlt">ocean</span> color algorithms designed for deep <span class="hlt">waters</span> where the seafloor has little or no effect on the <span class="hlt">water</span>-leaving radiance. Thus, inappropriate use of deep <span class="hlt">water</span> <span class="hlt">ocean</span> color algorithms in optically shallow regions can lead to inaccurate retrievals of inherent optical properties (IOPs) and therefore have a detrimental impact on IOP-based estimates of marine parameters, including chlorophyll-a and the diffuse attenuation coefficient. In order to improve IOP retrievals in optically shallow regions, a semi-analytical inversion algorithm, the Shallow <span class="hlt">Water</span> Inversion Model (SWIM), has been developed. Unlike established <span class="hlt">ocean</span> color algorithms, SWIM considers both the <span class="hlt">water</span> column depth and the benthic albedo. A radiative transfer study was conducted that demonstrated how SWIM and two contemporary <span class="hlt">ocean</span> color algorithms, the Generalized Inherent Optical Properties algorithm (GIOP) and Quasi-Analytical Algorithm (QAA), performed in optically deep and shallow scenarios. The results showed that SWIM performed well, whilst both GIOP and QAA showed distinct positive bias in IOP retrievals in optically shallow <span class="hlt">waters</span>. The SWIM algorithm was also applied to a test region: the Great Barrier Reef, Australia. Using a single test scene and time series data collected by NASA's MODIS-Aqua sensor (2002-2013), a comparison of IOPs retrieved by SWIM, GIOP and QAA was conducted.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25461969','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25461969"><span>Life-cycle modification in <span class="hlt">open</span> <span class="hlt">oceans</span> accounts for genome variability in a cosmopolitan phytoplankton.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>von Dassow, Peter; John, Uwe; Ogata, Hiroyuki; Probert, Ian; Bendif, El Mahdi; Kegel, Jessica U; Audic, Stéphane; Wincker, Patrick; Da Silva, Corinne; Claverie, Jean-Michel; Doney, Scott; Glover, David M; Flores, Daniella Mella; Herrera, Yeritza; Lescot, Magali; Garet-Delmas, Marie-José; de Vargas, Colomban</p> <p>2015-06-01</p> <p>Emiliania huxleyi is the most abundant calcifying plankton in modern <span class="hlt">oceans</span> with substantial intraspecific genome variability and a biphasic life cycle involving sexual alternation between calcified 2N and flagellated 1N cells. We show that high genome content variability in Emiliania relates to erosion of 1N-specific genes and loss of the ability to form flagellated cells. Analysis of 185 E. huxleyi strains isolated from world <span class="hlt">oceans</span> suggests that loss of flagella occurred independently in lineages inhabiting oligotrophic <span class="hlt">open</span> <span class="hlt">oceans</span> over short evolutionary timescales. This environmentally linked physiogenomic change suggests life cycling is not advantageous in very large/diluted populations experiencing low biotic pressure and low ecological variability. Gene loss did not appear to reflect pressure for genome streamlining in oligotrophic <span class="hlt">oceans</span> as previously observed in picoplankton. Life-cycle modifications might be common in plankton and cause major functional variability to be hidden from traditional taxonomic or molecular markers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110015418','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110015418"><span>Evaluation and Windspeed Dependence of MODIS Aerosol Retrievals Over <span class="hlt">Open</span> <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kleidman, Richard G.; Smirnov, Alexander; Levy, Robert C.; Mattoo, Shana; Tanre, Didier</p> <p>2011-01-01</p> <p>The Maritime Aerosol Network (MAN) data set provides high quality ground-truth to validate the MODIS aerosol product over <span class="hlt">open</span> <span class="hlt">ocean</span>. Prior validation of the <span class="hlt">ocean</span> aerosol product has been limited to coastal and island sites. Comparing MODIS Collection 5 <span class="hlt">ocean</span> aerosol retrieval products with collocated MAN measurements from ships shows that MODIS is meeting the pre-launch uncertainty estimates for aerosol optical depth (AOD) with 64% and 67% of retrievals at 550 nm, and 74% and 78% of retrievals at 870 nm, falling within expected uncertainty for Terra and Aqua, respectively. Angstrom Exponent comparisons show a high correlation between MODIS retrievals and shipboard measurements (R= 0.85 Terra, 0.83 Aqua), although the MODIS aerosol algorithm tends to underestimate particle size for large particles and overestimate size for small particles, as seen in earlier Collections. Prior analysis noted an offset between Terra and Aqua <span class="hlt">ocean</span> AOD, without concluding which sensor was more accurate. The simple linear regression reported here, is consistent with other anecdotal evidence that Aqua agreement with AERONET is marginally better. However we cannot claim based on the current study that the better Aqua comparison is statistically significant. Systematic increase of error as a function of wind speed is noted in both Terra and Aqua retrievals. This wind speed dependency enters the retrieval when winds deviate from the 6 m/s value assumed in the rough <span class="hlt">ocean</span> surface and white cap parameterizations. Wind speed dependency in the results can be mitigated by using auxiliary NCEP wind speed information in the retrieval process.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28811530','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28811530"><span>Evidence for ice-<span class="hlt">ocean</span> albedo feedback in the Arctic <span class="hlt">Ocean</span> shifting to a seasonal ice zone.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kashiwase, Haruhiko; Ohshima, Kay I; Nihashi, Sohey; Eicken, Hajo</p> <p>2017-08-15</p> <p>Ice-albedo feedback due to the albedo contrast between <span class="hlt">water</span> and ice is a major factor in seasonal sea ice retreat, and has received increasing attention with the Arctic <span class="hlt">Ocean</span> shifting to a seasonal ice cover. However, quantitative evaluation of such feedbacks is still insufficient. Here we provide quantitative evidence that heat input through the <span class="hlt">open</span> <span class="hlt">water</span> fraction is the primary driver of seasonal and interannual variations in Arctic sea ice retreat. Analyses of satellite data (1979-2014) and a simplified ice-upper <span class="hlt">ocean</span> coupled model reveal that divergent ice motion in the early melt season triggers large-scale feedback which subsequently amplifies summer sea ice anomalies. The magnitude of divergence controlling the feedback has doubled since 2000 due to a more mobile ice cover, which can partly explain the recent drastic ice reduction in the Arctic <span class="hlt">Ocean</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20110007945&hterms=water+sensor&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dwater%2Bsensor','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20110007945&hterms=water+sensor&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dwater%2Bsensor"><span>New Aerosol Models for the Retrieval of Aerosol Optical Thickness and Normalized <span class="hlt">Water</span>-Leaving Radiances from the SeaWiFS and MODIS Sensors Over Coastal Regions and <span class="hlt">Open</span> <span class="hlt">Oceans</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ahmad, Ziauddin; Franz, Bryan A.; McClain, Charles R.; Kwiatkowska, Ewa J.; Werdell, Jeremy; Shettle, Eric P.; Holben, Brent N.</p> <p>2010-01-01</p> <p>We describe the development of a new suite of aerosol models for the retrieval of atmospheric and <span class="hlt">oceanic</span> optical properties from the SeaWiFs and MODIS sensors, including aerosol optical thickness (tau), angstrom coefficient (alpha), and <span class="hlt">water</span>-leaving radiance (L(sub w)). The new aerosol models are derived from Aerosol Robotic Network (AERONET) observations and have bimodal lognormal distributions that are narrower than previous models used by the <span class="hlt">Ocean</span> Biology Processing Group. We analyzed AERONET data over <span class="hlt">open</span> <span class="hlt">ocean</span> and coastal regions and found that the seasonal variability in the modal radii, particularly in the coastal region, was related to the relative humidity, These findings were incorporated into the models by making the modal radii, as well as the refractive indices, explicitly dependent on relative humidity, From those findings, we constructed a new suite of aerosol models. We considered eight relative humidity values (30%, 50%, 70%, 75%, 80%, 85%, 90%. and 95%) and, for each relative humidity value, we constructed ten distributions by varying the fine-mode fraction from zero to 1. In all. 80 distributions (8Rh x 10 fine-mode fractions) were created to process the satellite data. We. also assumed that the coarse-mode particles were nonabsorbing (sea salt) and that all observed absorptions were entirely due to fine-mode particles. The composition of fine mode was varied to ensure that the new models exhibited the same spectral dependence of single scattering albedo as observed in the AERONET data,</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/2015AGUFM.C23B0782N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C23B0782N"><span>Spatio-temporal variability in the freshwater input to the surface <span class="hlt">water</span> of Southern <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Naidu, P. K.; Ghosh, P.; N, A.</p> <p>2015-12-01</p> <p><span class="hlt">Ocean</span> heat content is rising rapidly in high-latitude regions of both hemispheres as a consequence of global warming (e.g., Gille 2002; Karcher et al. 2003; Bindoff et al. 2007; Purkey and Johnson 2010). Recent warming and freshening of Southern <span class="hlt">Ocean</span> has affected hydrological cycle in terms of increasing tendency of precipitation as liquid <span class="hlt">water</span> instead of snow. Limited data is available on the extent of fresh <span class="hlt">water</span> flux by precipitation and sea ice melting to the surface <span class="hlt">ocean</span>. The spatial extent of sea ice formation is documented based on remote sensing observation. We investigate here spatial variability in freshwater inputs to the Indian sector of Southern <span class="hlt">Ocean</span> region using combined observation of oxygen isotopes ratios and salinity of surface <span class="hlt">water</span> during the summer of 2011, 2012 and 2013. Together with this, the measured isotopic ratios of meteoric <span class="hlt">water</span> and sea ice melt were used in the mass balance equation for deriving the contribution of both of these components in the surface <span class="hlt">water</span> of southern <span class="hlt">ocean</span>. The three component mixing equations (Meredith et al., 2013) allowed estimation of fractional contribution of rain over the years. The δ18O of meteoric <span class="hlt">water</span> followed the pattern nearly similar to the observation documented in the continental stations (Global Network of Isotopes in Precipitation, GNIP) located in the southern hemisphere. However, a slight but consistent heavier composition was documented in rainwater as compared to the GNIP stations. Our observation suggests that the meteoric <span class="hlt">water</span> is the dominant freshwater source over the <span class="hlt">ocean</span>, accounting for up to 10-15% of the <span class="hlt">water</span> present in the surface <span class="hlt">ocean</span> during the austral summer whereas Sea-ice melt accounts for a much smaller percentage (maximum around 1%). Our observation is consistent with previous studies where similar magnitude of fresh <span class="hlt">water</span> input was proposed based on observation from coastal region (Meredith et al., 2013).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP34A..03M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP34A..03M"><span>Investigating A Unique <span class="hlt">Open</span> <span class="hlt">Ocean</span> Geochemical Record Of the End Triassic Mass Extinction from Panthalassa</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marroquín, S. M.; Gill, B. C.; Them, T. R., II; Trabucho-Alexandre, J. P.; Aberhan, M.; Owens, J. D.; Gröcke, D. R.; Caruthers, A. H.</p> <p>2017-12-01</p> <p>The end-Triassic mass extinction ( 201 Ma) was a time of intense disturbance for marine communities. This event is estimated to have produced as much as a loss of 80% of known marine species. The protracted interval of elevated extinction rates is also characterized by a major carbon cycle perturbation and potentially widespread oxygen deficiency within the <span class="hlt">oceans</span>. While the causes of extinction and environmental feedbacks are still debated it is hypothesized to have been triggered by massive volcanism associated with the Central Atlantic Magmatic Province flood basalts. However, our understanding of the Latest Triassic-Earliest Jurassic interval is limited due to the lack of well-preserved stratigraphic successions outside of the Tethys <span class="hlt">Ocean</span> (present day Europe), with most of the records from epicontinental and marginal marine settings. To expand our understanding of this critical interval, our study seeks to document biological and environmental changes elsewhere. Specifically, we document and reconstruct these changes in the equatorial Panthalassan <span class="hlt">Ocean</span>. We will present new data from a sedimentary succession preserved in the Wrangell Mountains of Alaska that spans the Late Triassic through Early Jurassic. The sedimentary succession represents a mixed carbonate-siliciclastic ramp that was deposited at tropical latitudes, adjacent to an island arc in the <span class="hlt">open</span> Panthalassan <span class="hlt">Ocean</span>. This succession affords a unique view of <span class="hlt">open</span> marine conditions, and also holds the potential for excellent temporal control as it contains abundant ash layers throughout, as well as, key ammonite and bivalve fossil occurrences that provide biostratigraphic control. We will present an integrated geochemical and paleontological record from this site using several geochemical proxies (carbon, δ13Ccarb and % total organic carbon, sulfur, δ34S, as well as pyrite contents and iron speciation) along with ammonite and bivalve occurrence data to reconstruct the record of environmental and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5755909','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5755909"><span>High colored dissolved organic matter (CDOM) absorption in surface <span class="hlt">waters</span> of the central-eastern Arctic <span class="hlt">Ocean</span>: Implications for biogeochemistry and <span class="hlt">ocean</span> color algorithms</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Rabe, Benjamin; Peeken, Ilka; Bracher, Astrid</p> <p>2018-01-01</p> <p>As consequences of global warming sea-ice shrinking, permafrost thawing and changes in fresh <span class="hlt">water</span> and terrestrial material export have already been reported in the Arctic environment. These processes impact light penetration and primary production. To reach a better understanding of the current status and to provide accurate forecasts Arctic biogeochemical and physical parameters need to be extensively monitored. In this sense, bio-optical properties are useful to be measured due to the applicability of optical instrumentation to autonomous platforms, including satellites. This study characterizes the non-<span class="hlt">water</span> absorbers and their coupling to hydrographic conditions in the poorly sampled surface <span class="hlt">waters</span> of the central and eastern Arctic <span class="hlt">Ocean</span>. Over the entire sampled area colored dissolved organic matter (CDOM) dominates the light absorption in surface <span class="hlt">waters</span>. The distribution of CDOM, phytoplankton and non-algal particles absorption reproduces the hydrographic variability in this region of the Arctic <span class="hlt">Ocean</span> which suggests a subdivision into five major bio-optical provinces: Laptev Sea Shelf, Laptev Sea, Central Arctic/Transpolar Drift, Beaufort Gyre and Eurasian/Nansen Basin. Evaluating <span class="hlt">ocean</span> color algorithms commonly applied in the Arctic <span class="hlt">Ocean</span> shows that global and regionally tuned empirical algorithms provide poor chlorophyll-a (Chl-a) estimates. The semi-analytical algorithms Generalized Inherent Optical Property model (GIOP) and Garver-Siegel-Maritorena (GSM), on the other hand, provide robust estimates of Chl-a and absorption of colored matter. Applying GSM with modifications proposed for the western Arctic <span class="hlt">Ocean</span> produced reliable information on the absorption by colored matter, and specifically by CDOM. These findings highlight that only semi-analytical <span class="hlt">ocean</span> color algorithms are able to identify with low uncertainty the distribution of the different optical <span class="hlt">water</span> constituents in these high CDOM absorbing <span class="hlt">waters</span>. In addition, a clustering of the Arctic <span class="hlt">Ocean</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29304182','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29304182"><span>High colored dissolved organic matter (CDOM) absorption in surface <span class="hlt">waters</span> of the central-eastern Arctic <span class="hlt">Ocean</span>: Implications for biogeochemistry and <span class="hlt">ocean</span> color algorithms.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gonçalves-Araujo, Rafael; Rabe, Benjamin; Peeken, Ilka; Bracher, Astrid</p> <p>2018-01-01</p> <p>As consequences of global warming sea-ice shrinking, permafrost thawing and changes in fresh <span class="hlt">water</span> and terrestrial material export have already been reported in the Arctic environment. These processes impact light penetration and primary production. To reach a better understanding of the current status and to provide accurate forecasts Arctic biogeochemical and physical parameters need to be extensively monitored. In this sense, bio-optical properties are useful to be measured due to the applicability of optical instrumentation to autonomous platforms, including satellites. This study characterizes the non-<span class="hlt">water</span> absorbers and their coupling to hydrographic conditions in the poorly sampled surface <span class="hlt">waters</span> of the central and eastern Arctic <span class="hlt">Ocean</span>. Over the entire sampled area colored dissolved organic matter (CDOM) dominates the light absorption in surface <span class="hlt">waters</span>. The distribution of CDOM, phytoplankton and non-algal particles absorption reproduces the hydrographic variability in this region of the Arctic <span class="hlt">Ocean</span> which suggests a subdivision into five major bio-optical provinces: Laptev Sea Shelf, Laptev Sea, Central Arctic/Transpolar Drift, Beaufort Gyre and Eurasian/Nansen Basin. Evaluating <span class="hlt">ocean</span> color algorithms commonly applied in the Arctic <span class="hlt">Ocean</span> shows that global and regionally tuned empirical algorithms provide poor chlorophyll-a (Chl-a) estimates. The semi-analytical algorithms Generalized Inherent Optical Property model (GIOP) and Garver-Siegel-Maritorena (GSM), on the other hand, provide robust estimates of Chl-a and absorption of colored matter. Applying GSM with modifications proposed for the western Arctic <span class="hlt">Ocean</span> produced reliable information on the absorption by colored matter, and specifically by CDOM. These findings highlight that only semi-analytical <span class="hlt">ocean</span> color algorithms are able to identify with low uncertainty the distribution of the different optical <span class="hlt">water</span> constituents in these high CDOM absorbing <span class="hlt">waters</span>. In addition, a clustering of the Arctic <span class="hlt">Ocean</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016SPIE.9878E..0XS','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016SPIE.9878E..0XS"><span>Classification of case-II <span class="hlt">waters</span> using hyperspectral (HICO) data over North Indian <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Srinivasa Rao, N.; Ramarao, E. P.; Srinivas, K.; Deka, P. C.</p> <p>2016-05-01</p> <p>State of the art <span class="hlt">Ocean</span> color algorithms are proven for retrieving the <span class="hlt">ocean</span> constituents (chlorophyll-a, CDOM and Suspended Sediments) in case-I <span class="hlt">waters</span>. However, these algorithms could not perform well at case-II <span class="hlt">waters</span> because of the optical complexity. Hyperspectral data is found to be promising to classify the case-II <span class="hlt">waters</span>. The aim of this study is to propose the spectral bands for future <span class="hlt">Ocean</span> color sensors to classify the case-II <span class="hlt">waters</span>. Study has been performed with Rrs's of HICO at estuaries of the river Indus and GBM of North Indian <span class="hlt">Ocean</span>. Appropriate field samples are not available to validate and propose empirical models to retrieve concentrations. The sensor HICO is not currently operational to plan validation exercise. Aqua MODIS data at case-I and Case-II <span class="hlt">waters</span> are used as complementary to in- situ. Analysis of Spectral reflectance curves suggests the band ratios of Rrs 484 nm and Rrs 581 nm, Rrs 490 nm and Rrs 426 nm to classify the Chlorophyll -a and CDOM respectively. Rrs 610 nm gives the best scope for suspended sediment retrieval. The work suggests the need for <span class="hlt">ocean</span> color sensors with central wavelength's of 426, 484, 490, 581 and 610 nm to estimate the concentrations of Chl-a, Suspended Sediments and CDOM in case-II <span class="hlt">waters</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOS.A34A2617Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOS.A34A2617Z"><span>Numerical Investigations of Subduction of Eighteen Degree <span class="hlt">Water</span> in the Subtropical Northwest Atlantic <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhai, P.; He, R.</p> <p>2016-02-01</p> <p>Mode <span class="hlt">waters</span> are upper-<span class="hlt">ocean</span> <span class="hlt">water</span> masses with nearly uniform <span class="hlt">water</span> properties over a thickness of a few hundred meters. Subduction of mode <span class="hlt">waters</span> plays an important role in changing atmospheric and <span class="hlt">oceanic</span> long-term variability because they store "memory" of wintertime air-sea interaction. In this study, we investigated dynamic processes associated with subduction of the Eighteen Degree <span class="hlt">Water</span> (EDW, the principal mode <span class="hlt">water</span>) in the subtropical Northwest Atlantic during January to June 2007. Numerical simulations of the temporal and spatial evolutions of EDW were performed using both uncoupled (<span class="hlt">ocean</span> only) and air-sea coupled configurations and results were contrasted. We find the coupled simulation produced deeper mixed layer depth, stronger eddy kinetic energy, and larger subduction areas than their counterparts in the uncoupled <span class="hlt">ocean</span> simulation. In both configurations, mesoscale eddies enhance the total subduction and eddy-induced subduction has the same order as the mean component. Resolving strong air-sea coupling and mesoscale eddies is therefore important for understanding EDW dynamics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70179130','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70179130"><span>Barrier island breach evolution: Alongshore transport and bay-<span class="hlt">ocean</span> pressure gradient interactions</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Safak, Ilgar; Warner, John C.; List, Jeffrey</p> <p>2016-01-01</p> <p>Physical processes controlling repeated <span class="hlt">openings</span> and closures of a barrier island breach between a bay and the <span class="hlt">open</span> <span class="hlt">ocean</span> are studied using aerial photographs and atmospheric and hydrodynamic observations. The breach site is located on Pea Island along the Outer Banks, separating Pamlico Sound from the Atlantic <span class="hlt">Ocean</span>. Wind direction was a major control on the pressure gradients between the bay and the <span class="hlt">ocean</span> to drive flows that initiate or maintain the breach <span class="hlt">opening</span>. Alongshore sediment flux was found to be a major contributor to breach closure. During the analysis period from 2011 to 2016, three hurricanes had major impacts on the breach. First, Hurricane Irene <span class="hlt">opened</span> the breach with wind-driven flow from bay to <span class="hlt">ocean</span> in August 2011. Hurricane Sandy in October 2012 quadrupled the channel width from pressure gradient flows due to <span class="hlt">water</span> levels that were first higher on the <span class="hlt">ocean</span> side and then higher on the bay side. The breach closed sometime in Spring 2013, most likely due to an event associated with strong alongshore sediment flux but minimal <span class="hlt">ocean</span>-bay pressure gradients. Then, in July 2014, Hurricane Arthur briefly <span class="hlt">opened</span> the breach again from the bay side, in a similar fashion to Irene. In summary, <span class="hlt">opening</span> and closure of breaches are shown to follow a dynamic and episodic balance between along-channel pressure gradient driven flows and alongshore sediment fluxes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19790013331','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19790013331"><span><span class="hlt">Open</span> <span class="hlt">ocean</span> tide modelling</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Parke, M. E.</p> <p>1978-01-01</p> <p>Two trends evident in global tidal modelling since the first GEOP conference in 1972 are described. The first centers on the incorporation of terms for <span class="hlt">ocean</span> loading and gravitational self attraction into Laplace's tidal equations. The second centers on a better understanding of the problem of near resonant modelling and the need for realistic maps of tidal elevation for use by geodesists and geophysicists. Although new models still show significant differences, especially in the South Atlantic, there are significant similarities in many of the world's <span class="hlt">oceans</span>. This allows suggestions to be made for future locations for bottom pressure gauge measurements. Where available, estimates of M2 tidal dissipation from the new models are significantly lower than estimates from previous models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSPO41C..01S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSPO41C..01S"><span><span class="hlt">Ocean</span> to land moisture transport is reflected in sea surface salinity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schmitt, R. W.; Schanze, J. J.; Li, L.; Ummenhofer, C.</p> <p>2016-02-01</p> <p>The <span class="hlt">ocean</span> has a much larger <span class="hlt">water</span> cycle than the land, with global <span class="hlt">ocean</span> evaporation of 13 Sverdrups being 10 times larger than the sum of all river flows. This disparity and the different dynamics of dry surfaces, have led to an unfortunate disconnect between terrestrial hydrologists and oceanographers. Here we show that there is in fact a close coupling between the <span class="hlt">water</span> cycles of <span class="hlt">ocean</span> and land. In both cases there is much local recycling of moisture, since it does not travel far in the atmosphere. We argue that the most important <span class="hlt">water</span> cycle variable is the net export (or import) of <span class="hlt">water</span> from (to) an area. Over the <span class="hlt">open</span> <span class="hlt">ocean</span> this is just evaporation minus precipitation (E-P). The "P vs E" plot is a valuable tool for identifying the source and sink regions of the <span class="hlt">water</span> cycle. The subtropical high pressure systems are the source regions of the <span class="hlt">water</span> cycle, with a global net export of 4.5 Sv. The three sinks are the ITCZ in the tropics, the high latitude subpolar lows, and the land, all at about 1.5 Sv, though the subpolar lows do receive more <span class="hlt">water</span> than the tropics, where high rainfall is maintained by much local recycling. Of course, the signature of E-P in the <span class="hlt">open</span> <span class="hlt">ocean</span> is the sea surface salinity (SSS), as only net freshwater fluxes can create salinity variations. With the land receiving 1/3 of the <span class="hlt">oceanic</span> export, we should expect close coupling between terrestrial rainfall and the salinity of nearby <span class="hlt">oceans</span>, and SSS variations have indeed been found to be valuable for seasonal rainfall forecasts on land. The remarkable 3-6 month lead of winter-spring SSS over summer rainfall appears to be mediated by the recycling process on land through soil moisture. When soil moisture is high, terrestrial regions can become more <span class="hlt">oceanic</span>-like, with solar heating energizing evaporation and leading to down-stream propagation of the moisture signal (the "brown <span class="hlt">ocean</span>" effect). The correlation of high SSS with high rainfall promises to be a very valuable seasonal prediction</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.9255S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.9255S"><span>Characterization of Particle Backscattering of Global Highly Turbid <span class="hlt">Waters</span> From VIIRS <span class="hlt">Ocean</span> Color Observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shi, Wei; Wang, Menghua</p> <p>2017-11-01</p> <p>Normalized <span class="hlt">water</span>-leaving radiance spectra nLw(λ) at the near-infrared (NIR) from five years of observations (2012-2016) with the Visible Infrared Imaging Radiometer Suite (VIIRS) onboard the Suomi National Polar-orbiting Partnership (SNPP) are used to derive the particle backscattering coefficients bbp(λ) for global highly turbid coastal and inland <span class="hlt">waters</span>. Based on the fact that the absorption coefficient of sea <span class="hlt">water</span> aw(λ) is generally much larger than those of the other constituents aiop(λ) at the NIR wavelengths in coastal and inland <span class="hlt">waters</span>, an NIR-based bbp(λ) algorithm for turbid coastal and inland <span class="hlt">waters</span> has been developed and used in this study. This algorithm can be safely used for highly turbid <span class="hlt">waters</span> with nLw(745) and nLw(862) < ˜6 and ˜4 mW cm-2 μm-1 sr-1, respectively. Seasonal and interannual variations of bbp(λ) in China's east coastal region, the Amazon River Estuary, the La Plata River Estuary, the Meghna River Estuary, the Atchafalaya River Estuary, and Lake Taihu are characterized and quantified. The coefficient bbp(λ) can reach over ˜3-4 m-1 in the Amazon River Estuary and China's east coastal region. The Amazon River Estuary is identified as the most turbid region in the global <span class="hlt">ocean</span> in terms of bbp(λ) magnitude. bbp(λ) spectra in these five highly turbid regions are also seasonal-dependent and regional-dependent. In the highly turbid <span class="hlt">waters</span> of China's east coastal region and the Amazon River Estuary, bbp(λ) generally increases in wavelength from 410 to 862 nm, while it decreases in the La Plata River Estuary and Atchafalaya River Estuary. This is attributed to the different particle size distributions in these <span class="hlt">waters</span>. The geophysical implication of the bbp(λ) spectral curvatures for different <span class="hlt">waters</span> is discussed. To improve global bbp(λ) for both <span class="hlt">open</span> <span class="hlt">oceans</span> and coastal turbid <span class="hlt">waters</span>, a new combined NIR-based and Quasi-Analytical Algorithm (QAA)-based bbp(λ) algorithm is proposed and demonstrated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PalOc..32..674H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PalOc..32..674H"><span>Antarctic climate, Southern <span class="hlt">Ocean</span> circulation patterns, and deep <span class="hlt">water</span> formation during the Eocene</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Huck, Claire E.; van de Flierdt, Tina; Bohaty, Steven M.; Hammond, Samantha J.</p> <p>2017-07-01</p> <p>We assess early-to-middle Eocene seawater neodymium (Nd) isotope records from seven Southern <span class="hlt">Ocean</span> deep-sea drill sites to evaluate the role of Southern <span class="hlt">Ocean</span> circulation in long-term Cenozoic climate change. Our study sites are strategically located on either side of the Tasman Gateway and are positioned at a range of shallow (<500 m) to intermediate/deep ( 1000-2500 m) paleowater depths. Unradiogenic seawater Nd isotopic compositions, reconstructed from fish teeth at intermediate/deep Indian <span class="hlt">Ocean</span> pelagic sites (<span class="hlt">Ocean</span> Drilling Program (ODP) Sites 738 and 757 and Deep Sea Drilling Project (DSDP) Site 264), indicate a dominant Southern <span class="hlt">Ocean</span>-sourced contribution to regional deep <span class="hlt">waters</span> (ɛNd(t) = -9.3 ± 1.5). IODP Site U1356 off the coast of Adélie Land, a locus of modern-day Antarctic Bottom <span class="hlt">Water</span> production, is identified as a site of persistent deep <span class="hlt">water</span> formation from the early Eocene to the Oligocene. East of the Tasman Gateway an additional local source of intermediate/deep <span class="hlt">water</span> formation is inferred at ODP Site 277 in the SW Pacific <span class="hlt">Ocean</span> (ɛNd(t) = -8.7 ± 1.5). Antarctic-proximal shelf sites (ODP Site 1171 and Site U1356) reveal a pronounced erosional event between 49 and 48 Ma, manifested by 2 ɛNd unit negative excursions in seawater chemistry toward the composition of bulk sediments at these sites. This erosional event coincides with the termination of peak global warmth following the Early Eocene Climatic Optimum and is associated with documented cooling across the study region and increased export of Antarctic deep <span class="hlt">waters</span>, highlighting the complexity and importance of Southern <span class="hlt">Ocean</span> circulation in the greenhouse climate of the Eocene.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..14.3974B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..14.3974B"><span>Impact of <span class="hlt">opening</span> of the Central America Seaway on climate in a coupled atmosphere-<span class="hlt">ocean</span>-sea-ice model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Barrier, N.; Ferreira, D.; Marshall, J.</p> <p>2012-04-01</p> <p>We investigate the climatic impact of <span class="hlt">opening</span> the Central America Seaway (CAS) in a coupled atmosphere-<span class="hlt">ocean</span>-sea-ice model. A highly idealized land distribution is employed in which two meridional barriers extend from the North Pole in to the southern hemisphere, thus dividing the <span class="hlt">ocean</span> in to a large basin, a small basin and a circumpolar flow around the South Pole. Such a configuration captures the essential zonal and inter-hemispheric asymmetries of the current climate. These simple geometrical constraints are sufficient to localize the deep-reaching meridional overturning circulation (MOC) to the northern extremity of the small basin. Given this reference experiment, we <span class="hlt">open</span> up an analogue of the Central America Seaway on the western margin of the small basin north of the equator. Both deep and shallow passageways are considered. We find that although a major reorganization of <span class="hlt">ocean</span> circulation occurs, along with significant local <span class="hlt">water</span>-mass changes, global heat and freshwater meridional transports are largely unchanged, as are temperatures over the North Pole. In particular we do not observe a weakening of the MOC in the small basin, with salinity exchange between the large basin playing only a minor role. The simplicity of the geometrical configuration used in our experiments enables us to tease apart exactly what is going on. Experiments in which the salinity and temperature states of the small and large basins are interchanged, for example, show that our solutions are robust, with deep convection returning to the small basin after 800 years or so. Our experiments suggest to us that the closing of the CAS alone is not sufficient to lead to the onset of northern hemisphere glaciations 2 Ma years or so ago.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1111548','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1111548"><span>DE-EE0000319 Final Technical Report [National <span class="hlt">Open-ocean</span> Energy Laboratory</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>Skemp, Susan</p> <p></p> <p>Under the authorization provided by Section 634 of the Energy Independence and Security Act of 2007 (P.L. 110-140), in 2009 FAU was awarded U.S. Congressionally Directed Program (CDP) funding through the U.S. Department of Energy (DOE) to investigate and develop technologies to harness the energy of the Florida Current as a source of clean, renewable, base-load power for Florida and the U.S. A second CDP award in 2010 provided additional funding in order to enhance and extend FAU’s activities. These two CDPs in 2009 and 2010 were combined into a single DOE grant, DE-EE0000319, and are the subject of thismore » report. Subsequently, in July 2010 funding was made available under a separate contract, DE-EE0004200. Under that funding, DOE’s Wind and <span class="hlt">Water</span> Power Program designated FAU’s state of Florida marine renewable energy (MRE) center as the Southeast National Marine Renewable Energy Center (SNMREC). This report discusses SNMREC activities funded by the DE-EE0000319 grant, but will make reference, as appropriate, to activities that require further investigation under the follow-on grant. The concept of extracting energy from the motions of the <span class="hlt">oceans</span> has a long history. However, implementation on large scales of the technologies to effect renewable energy recovery from waves, tides, and <span class="hlt">open-ocean</span> currents is relatively recent. DOE’s establishment of SNMREC recognizes a significant potential for <span class="hlt">ocean</span> current energy recovery associated with the (relatively) high-speed Florida Current, the reach of the Gulf Stream System flowing through the Straits of Florida, between the Florida Peninsula and the Bahamas Archipelago. The proximity of the very large electrical load center of southeast Florida’s metropolitan area to the resource itself makes this potential all the more attractive. As attractive as this potential energy source is, it is not without its challenges. Although the technology is conceptually simple, its design and implementation in a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70170185','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70170185"><span>An analysis of <span class="hlt">water</span> data systems to inform the <span class="hlt">Open</span> <span class="hlt">Water</span> Data Initiative</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Blodgett, David L.; Read, Emily K.; Lucido, Jessica M.; Slawecki, Tad; Young, Dwane</p> <p>2016-01-01</p> <p>Improving access to data and fostering <span class="hlt">open</span> exchange of <span class="hlt">water</span> information is foundational to solving <span class="hlt">water</span> resources issues. In this vein, the Department of the Interior's Assistant Secretary for <span class="hlt">Water</span> and Science put forward the charge to undertake an <span class="hlt">Open</span> <span class="hlt">Water</span> Data Initiative (OWDI) that would prioritize and accelerate work toward better <span class="hlt">water</span> data infrastructure. The goal of the OWDI is to build out the <span class="hlt">Open</span> <span class="hlt">Water</span> Web (OWW). We therefore considered the OWW in terms of four conceptual functions: <span class="hlt">water</span> data cataloging, <span class="hlt">water</span> data as a service, enriching <span class="hlt">water</span> data, and community for <span class="hlt">water</span> data. To describe the current state of the OWW and identify areas needing improvement, we conducted an analysis of existing systems using a standard model for describing distributed systems and their business requirements. Our analysis considered three OWDI-focused use cases—flooding, drought, and contaminant transport—and then examined the landscape of other existing applications that support the <span class="hlt">Open</span> <span class="hlt">Water</span> Web. The analysis, which includes a discussion of observed successful practices of cataloging, serving, enriching, and building community around <span class="hlt">water</span> resources data, demonstrates that we have made significant progress toward the needed infrastructure, although challenges remain. The further development of the OWW can be greatly informed by the interpretation and findings of our analysis.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRC..123.1994T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRC..123.1994T"><span>Transformation of Deep <span class="hlt">Water</span> Masses Along Lagrangian Upwelling Pathways in the Southern <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tamsitt, V.; Abernathey, R. P.; Mazloff, M. R.; Wang, J.; Talley, L. D.</p> <p>2018-03-01</p> <p>Upwelling of northern deep <span class="hlt">waters</span> in the Southern <span class="hlt">Ocean</span> is fundamentally important for the closure of the global meridional overturning circulation and delivers carbon and nutrient-rich deep <span class="hlt">waters</span> to the sea surface. We quantify <span class="hlt">water</span> mass transformation along upwelling pathways originating in the Atlantic, Indian, and Pacific and ending at the surface of the Southern <span class="hlt">Ocean</span> using Lagrangian trajectories in an eddy-permitting <span class="hlt">ocean</span> state estimate. Recent related work shows that upwelling in the interior below about 400 m depth is localized at hot spots associated with major topographic features in the path of the Antarctic Circumpolar Current, while upwelling through the surface layer is more broadly distributed. In the <span class="hlt">ocean</span> interior upwelling is largely isopycnal; Atlantic and to a lesser extent Indian Deep <span class="hlt">Waters</span> cool and freshen while Pacific deep <span class="hlt">waters</span> are more stable, leading to a homogenization of <span class="hlt">water</span> mass properties. As upwelling <span class="hlt">water</span> approaches the mixed layer, there is net strong transformation toward lighter densities due to mixing of freshwater, but there is a divergence in the density distribution as Upper Circumpolar Deep <span class="hlt">Water</span> tends become lighter and dense Lower Circumpolar Deep <span class="hlt">Water</span> tends to become denser. The spatial distribution of transformation shows more rapid transformation at eddy hot spots associated with major topography where density gradients are enhanced; however, the majority of cumulative density change along trajectories is achieved by background mixing. We compare the Lagrangian analysis to diagnosed Eulerian <span class="hlt">water</span> mass transformation to attribute the mechanisms leading to the observed transformation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMGC13C0651M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMGC13C0651M"><span>Atmospheric and <span class="hlt">Oceanic</span> Response to Southern <span class="hlt">Ocean</span> Deep Convection Oscillations on Decadal to Centennial Time Scales in Climate Models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Martin, T.; Reintges, A.; Park, W.; Latif, M.</p> <p>2014-12-01</p> <p>Many current coupled global climate models simulate <span class="hlt">open</span> <span class="hlt">ocean</span> deep convection in the Southern <span class="hlt">Ocean</span> as a recurring event with time scales ranging from a few years to centennial (de Lavergne et al., 2014, Nat. Clim. Ch.). The only observation of such event, however, was the occurrence of the Weddell Polynya in the mid-1970s, an <span class="hlt">open</span> <span class="hlt">water</span> area of 350 000 km2 within the Antarctic sea ice in three consecutive winters. Both the wide range of modeled frequency of occurrence and the absence of deep convection in the Weddell Sea highlights the lack of understanding concerning the phenomenon. Nevertheless, simulations indicate that atmospheric and <span class="hlt">oceanic</span> responses to the cessation of deep convection in the Southern <span class="hlt">Ocean</span> include a strengthening of the low-level atmospheric circulation over the Southern <span class="hlt">Ocean</span> (increasing SAM index) and a reduction in the export of Antarctic Bottom <span class="hlt">Water</span> (AABW), potentially masking the regional effects of global warming (Latif et al., 2013, J. Clim.; Martin et al., 2014, Deep Sea Res. II). It is thus of great importance to enhance our understanding of Southern <span class="hlt">Ocean</span> deep convection and clarify the associated time scales. In two multi-millennial simulations with the Kiel Climate Model (KCM, ECHAM5 T31 atmosphere & NEMO-LIM2 ~2˚ <span class="hlt">ocean</span>) we showed that the deep convection is driven by strong <span class="hlt">oceanic</span> warming at mid-depth periodically overriding the stabilizing effects of precipitation and ice melt (Martin et al., 2013, Clim. Dyn.). Sea ice thickness also affects location and duration of the deep convection. A new control simulation, in which, amongst others, the atmosphere grid resolution is changed to T42 (~2.8˚), yields a faster deep convection flip-flop with a period of 80-100 years and a weaker but still significant global climate response similar to CMIP5 simulations. While model physics seem to affect the time scale and intensity of the phenomenon, the driving mechanism is a rather robust feature. Finally, we compare the atmospheric and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17813707','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17813707"><span><span class="hlt">Ocean</span> thermal gradient hydraulic 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>Beck, E J</p> <p>1975-07-25</p> <p>Solar energy stored in the <span class="hlt">oceans</span> may be used to generate power by exploiting ploiting thermal gradients. A proposed <span class="hlt">open</span>-cycle system uses low-pressure steam to elevate vate <span class="hlt">water</span>, which is then run through a hydraulic turbine to generate power. The device is analogous to an air lift pump.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20000110129&hterms=3D+animation&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3D3D%2Banimation','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20000110129&hterms=3D+animation&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3D3D%2Banimation"><span>Hurricane Directional Wave Spectrum Spatial Variation in the <span class="hlt">Open</span> <span class="hlt">Ocean</span> and at Landfall</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Walsh, E. J.; Wright, C. W.; Vandemark, D.; Krabill, W. B.; Garcia, A. W.; Houston, S. H.; Powell, M. D.; Black, P. G.; Marks, F. D.; Busalacchi, Antonio J. (Technical Monitor)</p> <p>2000-01-01</p> <p>The sea surface directional wave spectrum was measured for the first time in all quadrants of a hurricane in <span class="hlt">open</span> <span class="hlt">water</span> using the NASA airborne scanning radar altimeter (SRA) carried aboard one of the NOAA WP-3D hurricane hunter aircraft at 1.5 km height. The SRA measures the energetic portion of the directional wave spectrum by generating a topographic map of the sea surface. At 8 Hz, the SRA sweeps a radar beam of 1 E half-power width (two-way) across the aircraft ground track over a swath equal to 0.8 of the aircraft height, simultaneously measuring the backscattered power at its 36 GHz (8.3 mm) operating frequency and the range to the sea surface at 64 positions. These slant ranges are multiplied by the cosine of the incidence angles to determine the vertical distances from the aircraft to the sea surface. Subtracting these distances from the aircraft height produces the sea surface elevation map. The sea surface topography is interpolated to a uniform grid, transformed by a two-dimensional FFT, and Doppler corrected. The <span class="hlt">open-ocean</span> data were acquired on 24 August 1998 when hurricane Bonnie was east of the Bahamas and moving slowly to the north. Individual waves with heights up to 18 m were observed and the spatial variation of the wave field was dramatic. The dominant waves generally propagated at significant angles to the downwind direction. At some positions there were three different wave fields of comparable energy crossing each other. The NOAA aircraft spent over five hours within 180 km of the hurricane Bonnie eye, and made five eye penetrations. A 3-minute animation of the directional wave spectrum spatial variation over this period will be shown as well as summary plots of the wave field spatial variation. On 26 August 1998, the NOAA aircraft flew at 2.2 km height when hurricane Bonnie was making landfall near Wilmington, NC, documenting the directional wave spectrum in the region between Charleston, SC and Cape Hatteras, NC. The aircraft ground track</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26691595','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26691595"><span>Resilience of SAR11 bacteria to rapid acidification in the high-latitude <span class="hlt">open</span> <span class="hlt">ocean</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hartmann, Manuela; Hill, Polly G; Tynan, Eithne; Achterberg, Eric P; Leakey, Raymond J G; Zubkov, Mikhail V</p> <p>2016-02-01</p> <p>Ubiquitous SAR11 Alphaproteobacteria numerically dominate marine planktonic communities. Because they are excruciatingly difficult to cultivate, there is comparatively little known about their physiology and metabolic responses to long- and short-term environmental changes. As surface <span class="hlt">oceans</span> take up anthropogenic, atmospheric CO2, the consequential process of <span class="hlt">ocean</span> acidification could affect the global biogeochemical significance of SAR11. Shipping accidents or inadvertent release of chemicals from industrial plants can have strong short-term local effects on <span class="hlt">oceanic</span> SAR11. This study investigated the effect of 2.5-fold acidification of seawater on the metabolism of SAR11 and other heterotrophic bacterioplankton along a natural temperature gradient crossing the North Atlantic <span class="hlt">Ocean</span>, Norwegian and Greenland Seas. Uptake rates of the amino acid leucine by SAR11 cells as well as other bacterioplankton remained similar to controls despite an instant ∼50% increase in leucine bioavailability upon acidification. This high physiological resilience to acidification even without acclimation, suggests that <span class="hlt">open</span> <span class="hlt">ocean</span> dominant bacterioplankton are able to cope even with sudden and therefore more likely with long-term acidification effects. © FEMS 2015. All rights reserved. For permissions, please e-mail: journals.permissions@oup.com.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20523584','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20523584"><span>Lambert-Beer law in <span class="hlt">ocean</span> <span class="hlt">waters</span>: optical properties of <span class="hlt">water</span> and of dissolved/suspended material, optical energy budgets.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Stavn, R H</p> <p>1988-01-15</p> <p>The role of the Lambert-Beer law in <span class="hlt">ocean</span> optics is critically examined. The Lambert-Beer law and the three-parameter model of the submarine light field are used to construct an optical energy budget for any hydrosol. It is further applied to the analytical exponential decay coefficient of the light field and used to estimate the optical properties and effects of the dissolved/suspended component in upper <span class="hlt">ocean</span> layers. The concepts of the empirical exponential decay coefficient (diffuse attenuation coefficient) of the light field and a constant exponential decay coefficient for molecular <span class="hlt">water</span> are analyzed quantitatively. A constant exponential decay coefficient for <span class="hlt">water</span> is rejected. The analytical exponential decay coefficient is used to analyze optical gradients in <span class="hlt">ocean</span> <span class="hlt">waters</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_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li class="active"><span>10</span></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_10 --> <div id="page_11" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="201"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20720921','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20720921"><span>Coherence of particulate beam attenuation and backscattering coefficients in diverse <span class="hlt">open</span> <span class="hlt">ocean</span> environments.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Westberry, Toby K; Dall'Olmo, Giorgio; Boss, Emmanuel; Behrenfeld, Michael J; Moutin, Thierry</p> <p>2010-07-19</p> <p>We present an extensive data set of particle attenuation (c(p)), backscattering (b(bp)), and chlorophyll concentration (Chl) from a diverse set of <span class="hlt">open</span> <span class="hlt">ocean</span> environments. A consistent observation in the data set is the strong coherence between c(p) and b(bp) and the resulting constancy of the backscattering ratio (0.010 +/- 0.002). The strong covariability between c(p) and b(bp) must be rooted in one or both of two explanations, 1) the size distribution of particles in the <span class="hlt">ocean</span> is remarkably conserved and particle types responsible for c(p) and b(bp) covary, 2) the same particle types exert influence on both quantities. Therefore, existing relationships between c(p) or Chl:c(p) and phytoplankton biomass and physiological indices can be conceptually extended to the use of b(bp). This finding lends support to use of satellite-derived Chl and b(bp) for investigation of phytoplankton biomass and physiology and broadens the applications of existing <span class="hlt">ocean</span> color retrievals.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/ds/0960','USGSPUBS'); return false;" href="https://pubs.usgs.gov/ds/0960"><span>Back-Island and <span class="hlt">Open-Ocean</span> Shorelines, and Sand Areas of the Undeveloped Areas of New Jersey Barrier Islands, March 9, 1991, to July 30, 2013</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Guy, Kristy K.</p> <p>2015-11-09</p> <p>This Data Series Report includes <span class="hlt">open-ocean</span> shorelines, back-island shorelines, back-island shoreline points, sand polygons, and sand lines for the undeveloped areas of New Jersey barrier islands. These data were extracted from orthoimagery (aerial photography) taken between March 9, 1991, and July 30, 2013. The images used were 0.3–1-meter (m)-resolution U.S. Geological Survey Digital Orthophoto Quarter Quads (DOQQ), U.S. Department of Agriculture National Agriculture Imagery Program (NAIP) images, National <span class="hlt">Oceanic</span> and Atmospheric Administration images, and New Jersey Geographic Information Network images. The back-island shorelines were hand-digitized at the intersects of the apparent back-island shoreline and transects spaced at 20-m intervals. The <span class="hlt">open-ocean</span> shorelines were hand-digitized at the approximate still-<span class="hlt">water</span> level, such as tide level, which was fit through the average position of waves and swash apparent on the beach. Hand-digitizing was done at a scale of approximately 1:2,000. The sand polygons were derived by an image-processing unsupervised classification technique that separates images into classes. The classes were then visually categorized as either sand or not sand. Sand lines were taken from the sand polygons. Also included in this report are 20-m-spaced transect lines and the transect base lines.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2012-04-16/pdf/2012-9061.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2012-04-16/pdf/2012-9061.pdf"><span>77 FR 22523 - Safety Zone; 2012 <span class="hlt">Ocean</span> City Air Show; Atlantic <span class="hlt">Ocean</span>, <span class="hlt">Ocean</span> City, MD</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2012-04-16</p> <p>...-AA00 Safety Zone; 2012 <span class="hlt">Ocean</span> City Air Show; Atlantic <span class="hlt">Ocean</span>, <span class="hlt">Ocean</span> City, MD AGENCY: Coast Guard, DHS... the navigable <span class="hlt">waters</span> of the Atlantic <span class="hlt">Ocean</span> in <span class="hlt">Ocean</span> City, MD. This action is necessary to provide for the safety of life on navigable <span class="hlt">waters</span> during the 2012 <span class="hlt">Ocean</span> City Air Show. This action is intended to...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21955990','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21955990"><span>Novel lineages of Prochlorococcus and Synechococcus in the global <span class="hlt">oceans</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Huang, Sijun; Wilhelm, Steven W; Harvey, H Rodger; Taylor, Karen; Jiao, Nianzhi; Chen, Feng</p> <p>2012-02-01</p> <p>Picocyanobacteria represented by Prochlorococcus and Synechococcus have an important role in <span class="hlt">oceanic</span> carbon fixation and nutrient cycling. In this study, we compared the community composition of picocyanobacteria from diverse marine ecosystems ranging from estuary to <span class="hlt">open</span> <span class="hlt">oceans</span>, tropical to polar <span class="hlt">oceans</span> and surface to deep <span class="hlt">water</span>, based on the sequences of 16S-23S rRNA internal transcribed spacer (ITS). A total of 1339 ITS sequences recovered from 20 samples unveiled diverse and several previously unknown clades of Prochlorococcus and Synechococcus. Six high-light (HL)-adapted Prochlorococcus clades were identified, among which clade HLVI had not been described previously. Prochlorococcus clades HLIII, HLIV and HLV, detected in the Equatorial Pacific samples, could be related to the HNLC clades recently found in the high-nutrient, low-chlorophyll (HNLC), iron-depleted tropical <span class="hlt">oceans</span>. At least four novel Synechococcus clades (out of six clades in total) in subcluster 5.3 were found in subtropical <span class="hlt">open</span> <span class="hlt">oceans</span> and the South China Sea. A niche partitioning with depth was observed in the Synechococcus subcluster 5.3. Members of Synechococcus subcluster 5.2 were dominant in the high-latitude <span class="hlt">waters</span> (northern Bering Sea and Chukchi Sea), suggesting a possible cold-adaptation of some marine Synechococcus in this subcluster. A distinct shift of the picocyanobacterial community was observed from the Bering Sea to the Chukchi Sea, which reflected the change of <span class="hlt">water</span> temperature. Our study demonstrates that <span class="hlt">oceanic</span> systems contain a large pool of diverse picocyanobacteria, and further suggest that new genotypes or ecotypes of picocyanobacteria will continue to emerge, as microbial consortia are explored with advanced sequencing technology.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25100482','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25100482"><span>A global <span class="hlt">ocean</span> inventory of anthropogenic mercury based on <span class="hlt">water</span> column measurements.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lamborg, Carl H; Hammerschmidt, Chad R; Bowman, Katlin L; Swarr, Gretchen J; Munson, Kathleen M; Ohnemus, Daniel C; Lam, Phoebe J; Heimbürger, Lars-Eric; Rijkenberg, Micha J A; Saito, Mak A</p> <p>2014-08-07</p> <p>Mercury is a toxic, bioaccumulating trace metal whose emissions to the environment have increased significantly as a result of anthropogenic activities such as mining and fossil fuel combustion. Several recent models have estimated that these emissions have increased the <span class="hlt">oceanic</span> mercury inventory by 36-1,313 million moles since the 1500s. Such predictions have remained largely untested owing to a lack of appropriate historical data and natural archives. Here we report oceanographic measurements of total dissolved mercury and related parameters from several recent expeditions to the Atlantic, Pacific, Southern and Arctic <span class="hlt">oceans</span>. We find that deep North Atlantic <span class="hlt">waters</span> and most intermediate <span class="hlt">waters</span> are anomalously enriched in mercury relative to the deep <span class="hlt">waters</span> of the South Atlantic, Southern and Pacific <span class="hlt">oceans</span>, probably as a result of the incorporation of anthropogenic mercury. We estimate the total amount of anthropogenic mercury present in the global <span class="hlt">ocean</span> to be 290 ± 80 million moles, with almost two-thirds residing in <span class="hlt">water</span> shallower than a thousand metres. Our findings suggest that anthropogenic perturbations to the global mercury cycle have led to an approximately 150 per cent increase in the amount of mercury in thermocline <span class="hlt">waters</span> and have tripled the mercury content of surface <span class="hlt">waters</span> compared to pre-anthropogenic conditions. This information may aid our understanding of the processes and the depths at which inorganic mercury species are converted into toxic methyl mercury and subsequently bioaccumulated in marine food webs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/5767780','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/5767780"><span>Strontium-90: concentrations in surface <span class="hlt">waters</span> of the Atlantic <span class="hlt">Ocean</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bowen, V T; Noshkin, V E; Volchok, H L; Sugihara, T T</p> <p>1969-05-16</p> <p>From the large body of analyses of strontium-90 in surface <span class="hlt">waters</span> of the Atlantic <span class="hlt">Ocean</span>, annual average concentrations (from 10 degrees N to 70 degrees N) have been compared to those predicted. The data indicate higher fall-out over <span class="hlt">ocean</span> than over land and confirm the rapid rates of down-mixing shown by most studies of subsurface strontium-90.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140010389','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140010389"><span>Spatially Resolving <span class="hlt">Ocean</span> Color and Sediment Dispersion in River Plumes, Coastal Systems, and Continental Shelf <span class="hlt">Waters</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Aurin, Dirk Alexander; Mannino, Antonio; Franz, Bryan</p> <p>2013-01-01</p> <p>Satellite remote sensing of <span class="hlt">ocean</span> color in dynamic coastal, inland, and nearshorewaters is impeded by high variability in optical constituents, demands specialized atmospheric correction, and is limited by instrument sensitivity. To accurately detect dispersion of bio-optical properties, remote sensors require ample signal-to-noise ratio (SNR) to sense small variations in <span class="hlt">ocean</span> color without saturating over bright pixels, an atmospheric correction that can accommodate significantwater-leaving radiance in the near infrared (NIR), and spatial and temporal resolution that coincides with the scales of variability in the environment. Several current and historic space-borne sensors have met these requirements with success in the <span class="hlt">open</span> <span class="hlt">ocean</span>, but are not optimized for highly red-reflective and heterogeneous <span class="hlt">waters</span> such as those found near river outflows or in the presence of sediment resuspension. Here we apply analytical approaches for determining optimal spatial resolution, dominant spatial scales of variability ("patches"), and proportions of patch variability that can be resolved from four river plumes around the world between 2008 and 2011. An offshore region in the Sargasso Sea is analyzed for comparison. A method is presented for processing Moderate Resolution Imaging Spectroradiometer (MODIS) Aqua and Terra imagery including cloud detection, stray lightmasking, faulty detector avoidance, and dynamic aerosol correction using short-wave- and near-infrared wavebands in extremely turbid regions which pose distinct optical and technical challenges. Results showthat a pixel size of approx. 520 mor smaller is generally required to resolve spatial heterogeneity in <span class="hlt">ocean</span> color and total suspended materials in river plumes. Optimal pixel size increases with distance from shore to approx. 630 m in nearshore regions, approx 750 m on the continental shelf, and approx. 1350 m in the <span class="hlt">open</span> <span class="hlt">ocean</span>. Greater than 90% of the optical variability within plume regions is resolvable with</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1013929','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1013929"><span>Deep <span class="hlt">Water</span> <span class="hlt">Ocean</span> Acoustics (DWOA): The Philippine Sea, OBSANP, and THAAW Experiments</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2015-09-30</p> <p>the travel times. 4 The <span class="hlt">ocean</span> state estimates were then re-computed to fit the acoustic travel times as integrals of the sound speed, and...1 DISTRIBUTION STATEMENT A. Approved for public release; distribution is unlimited. Deep <span class="hlt">Water</span> <span class="hlt">Ocean</span> Acoustics (DWOA): The Philippine Sea...deep-<span class="hlt">water</span> acoustic propagation and ambient noise has been collected in a wide variety of environments over the last few years with ONR support</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19196281','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19196281"><span>Use of stable isotope-labelled cells to identify active grazers of picocyanobacteria in <span class="hlt">ocean</span> surface <span class="hlt">waters</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Frias-Lopez, Jorge; Thompson, Anne; Waldbauer, Jacob; Chisholm, Sallie W</p> <p>2009-02-01</p> <p>Prochlorococcus and Synechococcus are the two most abundant marine cyanobacteria. They represent a significant fraction of the total primary production of the world <span class="hlt">oceans</span> and comprise a major fraction of the prey biomass available to phagotrophic protists. Despite relatively rapid growth rates, picocyanobacterial cell densities in <span class="hlt">open-ocean</span> surface <span class="hlt">waters</span> remain fairly constant, implying steady mortality due to viral infection and consumption by predators. There have been several studies on grazing by specific protists on Prochlorococcus and Synechococcus in culture, and of cell loss rates due to overall grazing in the field. However, the specific sources of mortality of these primary producers in the wild remain unknown. Here, we use a modification of the RNA stable isotope probing technique (RNA-SIP), which involves adding labelled cells to natural seawater, to identify active predators that are specifically consuming Prochlorococcus and Synechococcus in the surface <span class="hlt">waters</span> of the Pacific <span class="hlt">Ocean</span>. Four major groups were identified as having their 18S rRNA highly labelled: Prymnesiophyceae (Haptophyta), Dictyochophyceae (Stramenopiles), Bolidomonas (Stramenopiles) and Dinoflagellata (Alveolata). For the first three of these, the closest relative of the sequences identified was a photosynthetic organism, indicating the presence of mixotrophs among picocyanobacterial predators. We conclude that the use of RNA-SIP is a useful method to identity specific predators for picocyanobacteria in situ, and that the method could possibly be used to identify other bacterial predators important in the microbial food-web.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMNH51D..04R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMNH51D..04R"><span>The Great Chilean Tsunamis of 2010, 2014 and 2015 on the Coast and Offshore of Mexico: Comparative Features Based on <span class="hlt">Open-Ocean</span> Energy Parameterization</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rabinovich, A.; Zaytsev, O.; Thomson, R.</p> <p>2016-12-01</p> <p>The three recent great earthquakes offshore of Chile on 27 February 2010 (Maule, Mw 8.8), 1 April 2014 (Iquique, Mw 8.2) and 16 September 2015 (Illapel, Mw 8.3) generated major trans-<span class="hlt">oceanic</span> tsunamis that spread throughout the entire Pacific <span class="hlt">Ocean</span> and were measured by numerous coastal tide gauges and <span class="hlt">open-ocean</span> DART stations. Statistical and spectral analyses of the tsunami waves from the three events recorded on the Pacific coast of Mexico enabled us to compare the events and to identify coastal "hot spots", regions with maximum tsunami risk. Based on joint spectral analyses of tsunamis and background noise, we have developed a method for reconstructing the "true" tsunami spectra in the deep <span class="hlt">ocean</span>. The "reconstructed" <span class="hlt">open-ocean</span> tsunami spectra are in excellent agreement with the actual tsunami spectra evaluated from direct analysis of the DART records offshore of Mexico. We have further used the spectral estimates to parameterize the energy of the three Chilean tsunamis based on the total <span class="hlt">open-ocean</span> tsunami energy and frequency content of the individual events.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JGRG..119..929R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JGRG..119..929R"><span>UV sensitivity of planktonic net community production in <span class="hlt">ocean</span> surface <span class="hlt">waters</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Regaudie-de-Gioux, Aurore; Agustí, Susana; Duarte, Carlos M.</p> <p>2014-05-01</p> <p>The net plankton community metabolism of <span class="hlt">oceanic</span> surface <span class="hlt">waters</span> is particularly important as it more directly affects the partial pressure of CO2 in surface <span class="hlt">waters</span> and thus the air-sea fluxes of CO2. Plankton communities in surface <span class="hlt">waters</span> are exposed to high irradiance that includes significant ultraviolet blue (UVB, 280-315 nm) radiation. UVB radiation affects both photosynthetic and respiration rates, increase plankton mortality rates, and other metabolic and chemical processes. Here we test the sensitivity of net community production (NCP) to UVB of planktonic communities in surface <span class="hlt">waters</span> across contrasting regions of the <span class="hlt">ocean</span>. We observed here that UVB radiation affects net plankton community production at the <span class="hlt">ocean</span> surface, imposing a shift in NCP by, on average, 50% relative to the values measured when excluding partly UVB. Our results show that under full solar radiation, the metabolic balance shows the prevalence of net heterotrophic community production. The demonstration of an important effect of UVB radiation on NCP in surface <span class="hlt">waters</span> presented here is of particular relevance in relation to the increased UVB radiation derived from the erosion of the stratospheric ozone layer. Our results encourage design future research to further our understanding of UVB effects on the metabolic balance of plankton communities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..12210020A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..12210020A"><span>A Meteoric <span class="hlt">Water</span> Budget for the Arctic <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Alkire, Matthew B.; Morison, James; Schweiger, Axel; Zhang, Jinlun; Steele, Michael; Peralta-Ferriz, Cecilia; Dickinson, Suzanne</p> <p>2017-12-01</p> <p>A budget of meteoric <span class="hlt">water</span> (MW = river runoff, net precipitation minus evaporation, and glacial meltwater) over four regions of the Arctic <span class="hlt">Ocean</span> is constructed using a simple box model, regional precipitation-evaporation estimates from reanalysis data sets, and estimates of import and export fluxes derived from the literature with a focus on the 2003-2008 period. The budget indicates an approximate/slightly positive balance between MW imports and exports (i.e., no change in storage); thus, the observed total freshwater increase observed during this time period likely resulted primarily from changes in non-MW freshwater components (i.e., increases in sea ice melt or Pacific <span class="hlt">water</span> and/or a decrease in ice export). Further, our analysis indicates that the MW increase observed in the Canada Basin resulted from a spatial redistribution of MW over the Arctic <span class="hlt">Ocean</span>. Mean residence times for MW were estimated for the Western Arctic (5-7 years), Eastern Arctic (3-4 years), and Lincoln Sea (1-2 years). The MW content over the Siberian shelves was estimated (˜14,000 km3) based on a residence time of 3.5 years. The MW content over the entire Arctic <span class="hlt">Ocean</span> was estimated to be ≥44,000 km3. The MW export through Fram Strait consisted mostly of <span class="hlt">water</span> from the Eastern Arctic (3,237 ± 1,370 km3 yr-1) whereas the export through the Canadian Archipelago was nearly equally derived from both the Western Arctic (1,182 ± 534 km3 yr-1) and Lincoln Sea (972 ± 391 km3 yr-1).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002AGUFM.A71C0116T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002AGUFM.A71C0116T"><span>Atmospheric Transport and Input of Iron to the Southern <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tindale, N. W.</p> <p>2002-12-01</p> <p>While Australia is not generally considered to be a major source of mineral dust to the atmosphere, at least compared to Asian and African desert regions, it does appear to be the main source of mineral material to the Southern <span class="hlt">Ocean</span> region south of Australia and New Zealand. In common with most of the greater Southern <span class="hlt">Ocean</span>, this region contains high nitrate, low chlorophyll (HNLC) <span class="hlt">waters</span>. Recent <span class="hlt">open</span> <span class="hlt">ocean</span> iron enrichment experiments in this region have demonstrated that phytoplankton growth and biomass are limited by iron availability. However the flux of atmospheric iron to this <span class="hlt">open</span> <span class="hlt">ocean</span> region is poorly known with very few direct measurements of mineral aerosol levels and input. Using mineral aerosol samples collected on Macquarie Island and at Cape Grim, together with other chemical data, air mass trajectories and satellite data, the spatial and temporal variability of aerosol iron transport and input to the Southern <span class="hlt">Ocean</span> region south of Australia is estimated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5070528','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5070528"><span>Arctic pathways of Pacific <span class="hlt">Water</span>: Arctic <span class="hlt">Ocean</span> Model Intercomparison experiments</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Karcher, Michael; Proshutinsky, Andrey; Gerdes, Rüdiger; de Cuevas, Beverly; Golubeva, Elena; Kauker, Frank; Nguyen, An T.; Platov, Gennady A.; Wadley, Martin; Watanabe, Eiji; Coward, Andrew C.; Nurser, A. J. George</p> <p>2016-01-01</p> <p>Abstract Pacific <span class="hlt">Water</span> (PW) enters the Arctic <span class="hlt">Ocean</span> through Bering Strait and brings in heat, fresh <span class="hlt">water</span>, and nutrients from the northern Bering Sea. The circulation of PW in the central Arctic <span class="hlt">Ocean</span> is only partially understood due to the lack of observations. In this paper, pathways of PW are investigated using simulations with six state‐of‐the art regional and global <span class="hlt">Ocean</span> General Circulation Models (OGCMs). In the simulations, PW is tracked by a passive tracer, released in Bering Strait. Simulated PW spreads from the Bering Strait region in three major branches. One of them starts in the Barrow Canyon, bringing PW along the continental slope of Alaska into the Canadian Straits and then into Baffin Bay. The second begins in the vicinity of the Herald Canyon and transports PW along the continental slope of the East Siberian Sea into the Transpolar Drift, and then through Fram Strait and the Greenland Sea. The third branch begins near the Herald Shoal and the central Chukchi shelf and brings PW into the Beaufort Gyre. In the models, the wind, acting via Ekman pumping, drives the seasonal and interannual variability of PW in the Canadian Basin of the Arctic <span class="hlt">Ocean</span>. The wind affects the simulated PW pathways by changing the vertical shear of the relative vorticity of the <span class="hlt">ocean</span> flow in the Canada Basin. PMID:27818853</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27818853','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27818853"><span>Arctic pathways of Pacific <span class="hlt">Water</span>: Arctic <span class="hlt">Ocean</span> Model Intercomparison experiments.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Aksenov, Yevgeny; Karcher, Michael; Proshutinsky, Andrey; Gerdes, Rüdiger; de Cuevas, Beverly; Golubeva, Elena; Kauker, Frank; Nguyen, An T; Platov, Gennady A; Wadley, Martin; Watanabe, Eiji; Coward, Andrew C; Nurser, A J George</p> <p>2016-01-01</p> <p>Pacific <span class="hlt">Water</span> (PW) enters the Arctic <span class="hlt">Ocean</span> through Bering Strait and brings in heat, fresh <span class="hlt">water</span>, and nutrients from the northern Bering Sea. The circulation of PW in the central Arctic <span class="hlt">Ocean</span> is only partially understood due to the lack of observations. In this paper, pathways of PW are investigated using simulations with six state-of-the art regional and global <span class="hlt">Ocean</span> General Circulation Models (OGCMs). In the simulations, PW is tracked by a passive tracer, released in Bering Strait. Simulated PW spreads from the Bering Strait region in three major branches. One of them starts in the Barrow Canyon, bringing PW along the continental slope of Alaska into the Canadian Straits and then into Baffin Bay. The second begins in the vicinity of the Herald Canyon and transports PW along the continental slope of the East Siberian Sea into the Transpolar Drift, and then through Fram Strait and the Greenland Sea. The third branch begins near the Herald Shoal and the central Chukchi shelf and brings PW into the Beaufort Gyre. In the models, the wind, acting via Ekman pumping, drives the seasonal and interannual variability of PW in the Canadian Basin of the Arctic <span class="hlt">Ocean</span>. The wind affects the simulated PW pathways by changing the vertical shear of the relative vorticity of the <span class="hlt">ocean</span> flow in the Canada Basin.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA619524','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA619524"><span>Deep <span class="hlt">Water</span> <span class="hlt">Ocean</span> Acoustics</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2015-07-17</p> <p>under- ice scattering, bathymetric diffraction and the application of the <span class="hlt">ocean</span> acoustic Parabolic Equation to infrasound. 2. Tasks a. Task 1...and Climate of the <span class="hlt">Ocean</span>, Phase II (ECCO2): High-Resolution Global-<span class="hlt">Ocean</span> and Sea- Ice Data Synthesis) model re- analysis for the years 1992 and 1993...The ECCO2 model is a state estimation based upon data syntheses obtained by least squares fitting of the global <span class="hlt">ocean</span> and sea- ice configuration of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.9227L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.9227L"><span>Upper <span class="hlt">Ocean</span> Evolution Across the Beaufort Sea Marginal Ice Zone from Autonomous Gliders</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lee, Craig; Rainville, Luc; Perry, Mary Jane</p> <p>2016-04-01</p> <p>The observed reduction of Arctic summertime sea ice extent and expansion of the marginal ice zone (MIZ) have profound impacts on the balance of processes controlling sea ice evolution, including the introduction of several positive feedback mechanisms that may act to accelerate melting. Examples of such feedbacks include increased upper <span class="hlt">ocean</span> warming though absorption of solar radiation, elevated internal wave energy and mixing that may entrain heat stored in subsurface watermasses (e.g., the relatively warm Pacific Summer (PSW) and Atlantic (AW) <span class="hlt">waters</span>), and elevated surface wave energy that acts to deform and fracture sea ice. Spatial and temporal variability in ice properties and <span class="hlt">open</span> <span class="hlt">water</span> fraction impact these processes. To investigate how upper <span class="hlt">ocean</span> structure varies with changing ice cover, and how the balance of processes shift as a function of ice fraction and distance from <span class="hlt">open</span> <span class="hlt">water</span>, four long-endurance autonomous Seagliders occupied sections that extended from <span class="hlt">open</span> <span class="hlt">water</span>, through the marginal ice zone, deep into the pack during summer 2014 in the Beaufort Sea. Sections reveal strong fronts where cold, ice-covered <span class="hlt">waters</span> meet <span class="hlt">waters</span> that have been exposed to solar warming, and O(10 km) scale eddies near the ice edge. In the pack, Pacific Summer <span class="hlt">Water</span> and a deep chlorophyll maximum form distinct layers at roughly 60 m and 80 m, respectively, which become increasingly diffuse as they progress through the MIZ and into <span class="hlt">open</span> <span class="hlt">water</span>. The isopynal layer between 1023 and 1024 kgm-3, just above the PSW, consistently thickens near the ice edge, likely due to mixing or energetic vertical exchange associated with strong lateral gradients in this region. This presentation will discuss the upper <span class="hlt">ocean</span> variability, its relationship to sea ice extent, and evolution over the summer to the start of freeze up.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSHE21A..06L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSHE21A..06L"><span>Upper <span class="hlt">Ocean</span> Evolution Across the Beaufort Sea Marginal Ice Zone from Autonomous Gliders</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lee, C.; Rainville, L.; Perry, M. J.</p> <p>2016-02-01</p> <p>The observed reduction of Arctic summertime sea ice extent and expansion of the marginal ice zone (MIZ) have profound impacts on the balance of processes controlling sea ice evolution, including the introduction of several positive feedback mechanisms that may act to accelerate melting. Examples of such feedbacks include increased upper <span class="hlt">ocean</span> warming though absorption of solar radiation, elevated internal wave energy and mixing that may entrain heat stored in subsurface watermasses (e.g., the relatively warm Pacific Summer (PSW) and Atlantic (AW) <span class="hlt">waters</span>), and elevated surface wave energy that acts to deform and fracture sea ice. Spatial and temporal variability in ice properties and <span class="hlt">open</span> <span class="hlt">water</span> fraction impact these processes. To investigate how upper <span class="hlt">ocean</span> structure varies with changing ice cover, and how the balance of processes shift as a function of ice fraction and distance from <span class="hlt">open</span> <span class="hlt">water</span>, four long-endurance autonomous Seagliders occupied sections that extended from <span class="hlt">open</span> <span class="hlt">water</span>, through the marginal ice zone, deep into the pack during summer 2014 in the Beaufort Sea. Sections reveal strong fronts where cold, ice-covered <span class="hlt">waters</span> meet <span class="hlt">waters</span> that have been exposed to solar warming, and O(10 km) scale eddies near the ice edge. In the pack, Pacific Summer <span class="hlt">Water</span> and a deep chlorophyll maximum form distinct layers at roughly 60 m and 80 m, respectively, which become increasingly diffuse as they progress through the MIZ and into <span class="hlt">open</span> <span class="hlt">water</span>. The isopynal layer between 1023 and 1024 kg m-3, just above the PSW, consistently thickens near the ice edge, likely due to mixing or energetic vertical exchange associated with strong lateral gradients in this region. This presentation will discuss the upper <span class="hlt">ocean</span> variability, its relationship to sea ice extent, and evolution over the summer to the start of freeze up.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014BGeo...11.2531L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014BGeo...11.2531L"><span>Lytic viral infection of bacterioplankton in deep <span class="hlt">waters</span> of the western Pacific <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Y.; Luo, T.; Sun, J.; Cai, L.; Liang, Y.; Jiao, N.; Zhang, R.</p> <p>2014-05-01</p> <p>As the most abundant biological entities in the <span class="hlt">ocean</span>, viruses influence host mortality and nutrient recycling mainly through lytic infection. Yet, the ecological characteristics of virioplankton and viral impacts on host mortality and biogeochemical cycling in the deep sea are largely unknown. In the present study, viral abundance and lytic infection were investigated throughout the <span class="hlt">water</span> column in the western Pacific <span class="hlt">Ocean</span>. Both the prokaryotic and viral abundance and production showed a significantly decreasing trend from epipelagic to meso- and bathypelagic <span class="hlt">waters</span>. Viral abundance decreased from 0.36-1.05 × 1010 particles L-1 to 0.43-0.80 × 109 particles L-1, while the virus : prokaryote ratio varied from 7.21 to 16.23 to 2.45-23.40, at the surface and 2000 m, respectively. Lytic viral production rates in surface and 2000 m <span class="hlt">waters</span> were, on average, 1.03 × 1010 L-1 day-1 and 5.74 × 108 L-1 day-1. Relatively high percentages of prokaryotic cells lysed by viruses at 1000 and 2000 m were observed, suggesting a significant contribution of viruses to prokaryotic mortality in the deep <span class="hlt">ocean</span>. The carbon released by viral lysis in deep western Pacific <span class="hlt">Ocean</span> <span class="hlt">waters</span> was from 0.03 to 2.32 μg C L-1 day-1. Our findings demonstrated a highly dynamic and active viral population in these deep <span class="hlt">waters</span> and suggested that virioplankton play an important role in the microbial loop and subsequently biogeochemical cycling in deep <span class="hlt">oceans</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSHE52B..08C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSHE52B..08C"><span>An Integrative Approach to Understand a Rich Ecosystem in the Southern <span class="hlt">Ocean</span> From Carbon to Top Predators</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cotté, C.; d'Ovidio, F.; Behagle, N.; Roudaut, G.; Brehmer, P.; Bost, C. A.; Guinet, C.; Cherel, Y.</p> <p>2016-02-01</p> <p>Large parts of the Southern <span class="hlt">Ocean</span> <span class="hlt">waters</span> are rich in macronutrients, but blooms of phytoplankton occur in a patchy and localized way. This is in part due to the presence of sources of limiting micronutrients scattered along the continental breaks, whose inputs are stirred into the <span class="hlt">open</span> <span class="hlt">ocean</span> very inhomogeneously. At the highest levels of ecosystems, top predators reveal areas of ecological importance where no other information is available on the underpinning trophic web. A dramatic example of this situation is provided by the region around Kerguelen archipelago, in the Southern Indian <span class="hlt">Ocean</span>. Here, the high nutrient, low iron <span class="hlt">waters</span> transported eastward by the Antarctic Circumpolar Current encounter the iron-rich Kerguelen shelf break. As a consequence, a plume of high chlorophyll <span class="hlt">water</span> develops east of the plateau, extending from the shelf break for hundreds of kms into the <span class="hlt">open</span> <span class="hlt">ocean</span>, and strongly modulated by the intense mesoscale activity. Large populations of top predators use this area to forage during the summer periode, despite very scarce knowledge on their micronektonic prey and on mid-trophic oragnisms. By combining in campaign data, satellite observations, and biologging, we adopt an end-to-end approach and describe the mechanisms by which the <span class="hlt">ocean</span> physics impacts the regional biogeochemistry firstly by redistributing iron-rich coastal <span class="hlt">waters</span> into the <span class="hlt">open</span> <span class="hlt">ocean</span>, and then by focusing on the trophic interactions. We consider in particular the role of mesoscale eddies and submesoscale fronts, whose temporal dynamics resonates with biological processes and organises the variability of ecosystems.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_11 --> <div id="page_12" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="221"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19840018165&hterms=water&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DTitle%26N%3D0%26No%3D90%26Ntt%3Dwater','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19840018165&hterms=water&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DTitle%26N%3D0%26No%3D90%26Ntt%3Dwater"><span>Nimbus 7 SMMR Derived Seasonal Variations in the <span class="hlt">Water</span> Vapor, Liquid <span class="hlt">Water</span> and Surface Winds over the Global <span class="hlt">Oceans</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Prabhakara, C.; Short, D. A.</p> <p>1984-01-01</p> <p>Monthly mean distributions of <span class="hlt">water</span> vapor and liquid <span class="hlt">water</span> contained in a vertical column of the atmosphere and the surface wind speed were derived from Nimbus Scanning Multichannel Microwave Radiometer (SMMR) observations over the global <span class="hlt">oceans</span> for the period November 1978 to November 1979. The remote sensing techniques used to estimate these parameters from SMMR are presented to reveal the limitations, accuracies, and applicability of the satellite-derived information for climate studies. On a time scale of the order of a month, the distribution of atmospheric <span class="hlt">water</span> vapor over the <span class="hlt">oceans</span> is controlled by the sea surface temperature and the large scale atmospheric circulation. The monthly mean distribution of liquid <span class="hlt">water</span> content in the atmosphere over the <span class="hlt">oceans</span> closely reflects the precipitation patterns associated with the convectively and baroclinically active regions. Together with the remotely sensed surface wind speed that is causing the sea surface stress, the data collected reveal the manner in which the <span class="hlt">ocean</span>-atmosphere system is operating. Prominent differences in the <span class="hlt">water</span> vapor patterns from one year to the next, or from month to month, are associated with anomalies in the wind and geopotential height fields. In association with such circulation anomalies the precipitation patterns deduced from the meteorological network over adjacent continents also reveal anomalous distributions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21719036','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21719036"><span>Organic micropollutants in marine plastics debris from the <span class="hlt">open</span> <span class="hlt">ocean</span> and remote and urban beaches.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hirai, Hisashi; Takada, Hideshige; Ogata, Yuko; Yamashita, Rei; Mizukawa, Kaoruko; Saha, Mahua; Kwan, Charita; Moore, Charles; Gray, Holly; Laursen, Duane; Zettler, Erik R; Farrington, John W; Reddy, Christopher M; Peacock, Emily E; Ward, Marc W</p> <p>2011-08-01</p> <p>To understand the spatial variation in concentrations and compositions of organic micropollutants in marine plastic debris and their sources, we analyzed plastic fragments (∼10 mm) from the <span class="hlt">open</span> <span class="hlt">ocean</span> and from remote and urban beaches. Polychlorinated biphenyls (PCBs), polycyclic aromatic hydrocarbons (PAHs), dichloro-diphenyl-trichloroethane and its metabolites (DDTs), polybrominated diphenyl ethers (PBDEs), alkylphenols and bisphenol A were detected in the fragments at concentrations from 1 to 10,000 ng/g. Concentrations showed large piece-to-piece variability. Hydrophobic organic compounds such as PCBs and PAHs were sorbed from seawater to the plastic fragments. PCBs are most probably derived from legacy pollution. PAHs showed a petrogenic signature, suggesting the sorption of PAHs from oil slicks. Nonylphenol, bisphenol A, and PBDEs came mainly from additives and were detected at high concentrations in some fragments both from remote and urban beaches and the <span class="hlt">open</span> <span class="hlt">ocean</span>. Copyright © 2011 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.5643P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.5643P"><span>Combined simulation of carbon and <span class="hlt">water</span> isotopes in a global <span class="hlt">ocean</span> model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Paul, André; Krandick, Annegret; Gebbie, Jake; Marchal, Olivier; Dutkiewicz, Stephanie; Losch, Martin; Kurahashi-Nakamura, Takasumi; Tharammal, Thejna</p> <p>2013-04-01</p> <p>Carbon and <span class="hlt">water</span> isotopes are included as passive tracers in the MIT general circulation model (MITgcm). The implementation of the carbon isotopes is based on the existing MITgcm carbon cycle component and involves the fractionation processes during photosynthesis and air-sea gas exchange. Special care is given to the use of a real freshwater flux boundary condition in conjunction with the nonlinear free surface of the <span class="hlt">ocean</span> model. The isotopic content of precipitation and <span class="hlt">water</span> vapor is obtained from an atmospheric GCM (the NCAR CAM3) and mapped onto the MITgcm grid system, but the kinetic fractionation during evaporation is treated explicitly in the <span class="hlt">ocean</span> model. In a number of simulations, we test the sensitivity of the carbon isotope distributions to the formulation of fractionation during photosynthesis and compare the results to modern observations of δ13C and Δ14C from GEOSECS, WOCE and CLIVAR. Similarly, we compare the resulting distribution of oxygen isotopes to modern δ18O data from the NASA GISS Global Seawater Oxygen-18 Database. The overall agreement is good, but there are discrepancies in the carbon isotope composition of the surface <span class="hlt">water</span> and the oxygen isotope composition of the intermediate and deep <span class="hlt">waters</span>. The combined simulation of carbon and <span class="hlt">water</span> isotopes in a global <span class="hlt">ocean</span> model will provide a framework for studying present and past states of <span class="hlt">ocean</span> circulation such as postulated from deep-sea sediment records.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20120004248&hterms=climate+change+ocean&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dclimate%2Bchange%2Bocean','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20120004248&hterms=climate+change+ocean&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dclimate%2Bchange%2Bocean"><span>SWOT: The Surface <span class="hlt">Water</span> and <span class="hlt">Ocean</span> Topography Mission. Wide- Swath Altimetric Elevation on Earth</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Fu, Lee-Lueng (Editor); Alsdorf, Douglas (Editor); Morrow, Rosemary; Rodriguez, Ernesto; Mognard, Nelly</p> <p>2012-01-01</p> <p>The elevation of the surface of the <span class="hlt">ocean</span> and freshwater bodies on land holds key information on many important processes of the Earth System. The elevation of the <span class="hlt">ocean</span> surface, called <span class="hlt">ocean</span> surface topography, has been measured by conventional nadirlooking radar altimeter for the past two decades. The data collected have been used for the study of large-scale circulation and sea level change. However, the spatial resolution of the observations has limited the study to scales larger than about 200 km, leaving the smaller scales containing substantial kinetic energy of <span class="hlt">ocean</span> circulation that is responsible for the flux of heat, dissolved gas and nutrients between the upper and the deep <span class="hlt">ocean</span>. This flux is important to the understanding of the <span class="hlt">ocean</span>'s role in regulatingfuture climate change.The elevation of the <span class="hlt">water</span> bodies on land is a key parameter required for the computation of storage and discharge of freshwater in rivers, lakes, and wetlands. Globally, the spatial and temporal variability of <span class="hlt">water</span> storage and discharge is poorly known due to the lack of well-sampled observations. In situ networks measuring river flows are declining worldwide due to economic and political reasons. Conventional altimeter observations suffers from the complexity of multiple peaks caused by the reflections from <span class="hlt">water</span>, vegetation canopy and rough topography, resulting in much less valid data over land than over the <span class="hlt">ocean</span>. Another major limitation is the large inter track distance preventing good coverage of rivers and other <span class="hlt">water</span> bodies.This document provides descriptions of a new measurement technique using radar interferometry to obtain wide-swath measurement of <span class="hlt">water</span> elevation at high resolution over both the <span class="hlt">ocean</span> and land. Making this type of measurement, which addresses the shortcomings of conventional altimetry in both oceanographic and hydrologic applications, is the objective of a mission concept called Surface <span class="hlt">Water</span> and <span class="hlt">Ocean</span> Topography (SWOT), which was recommended by</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017CG....107...28B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017CG....107...28B"><span>WASS: An <span class="hlt">open</span>-source pipeline for 3D stereo reconstruction of <span class="hlt">ocean</span> waves</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bergamasco, Filippo; Torsello, Andrea; Sclavo, Mauro; Barbariol, Francesco; Benetazzo, Alvise</p> <p>2017-10-01</p> <p>Stereo 3D reconstruction of <span class="hlt">ocean</span> waves is gaining more and more popularity in the oceanographic community and industry. Indeed, recent advances of both computer vision algorithms and computer processing power now allow the study of the spatio-temporal wave field with unprecedented accuracy, especially at small scales. Even if simple in theory, multiple details are difficult to be mastered for a practitioner, so that the implementation of a sea-waves 3D reconstruction pipeline is in general considered a complex task. For instance, camera calibration, reliable stereo feature matching and mean sea-plane estimation are all factors for which a well designed implementation can make the difference to obtain valuable results. For this reason, we believe that the <span class="hlt">open</span> availability of a well tested software package that automates the reconstruction process from stereo images to a 3D point cloud would be a valuable addition for future researches in this area. We present WASS (http://www.dais.unive.it/wass), an <span class="hlt">Open</span>-Source stereo processing pipeline for sea waves 3D reconstruction. Our tool completely automates all the steps required to estimate dense point clouds from stereo images. Namely, it computes the extrinsic parameters of the stereo rig so that no delicate calibration has to be performed on the field. It implements a fast 3D dense stereo reconstruction procedure based on the consolidated <span class="hlt">Open</span>CV library and, lastly, it includes set of filtering techniques both on the disparity map and the produced point cloud to remove the vast majority of erroneous points that can naturally arise while analyzing the optically complex nature of the <span class="hlt">water</span> surface. In this paper, we describe the architecture of WASS and the internal algorithms involved. The pipeline workflow is shown step-by-step and demonstrated on real datasets acquired at sea.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSIS11A..03C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSIS11A..03C"><span>Characteristics of Airborne Lidar Profiles of the Arctic <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Churnside, J. H.; Marchbanks, R.</p> <p>2016-02-01</p> <p>In July, 2014, we flew the NOAA oceanographic lidar more than 6000 km over the Chukchi and Beaufort Seas around northern Alaska. The most obvious feature in the lidar returns was sea ice, which blocked any return from below and saturated our receivers. The flights were designed to measure profiles with varying degrees of ice cover, from <span class="hlt">open</span> <span class="hlt">water</span> to nearly completely covered <span class="hlt">water</span>. Thin phytoplankton layers were also prevalent, both in <span class="hlt">open</span> <span class="hlt">water</span> and within the pack ice. These layers were generally deeper (20 m vs. 16 m averages) and stronger (27 times the background level vs. 9 times) in <span class="hlt">open</span> <span class="hlt">water</span> than in the ice. The average layer thicknesses were similar in <span class="hlt">open</span> <span class="hlt">water</span> and in the ice (3.8 m vs. 3.4 m). The diffuse attenuation coefficient measured by the lidar did not depend strongly on ice cover. It was generally higher near the coast than farther off shore. Fish were present in a few of the returns, but these were not very numerous. More common were the sediment plumes generated by gray whales feeding on crustaceans on the bottom. Data from these flights show a high level of spatial variability that is difficult to measure from a surface vessel and significant vertical structure that is impossible to obtain from satellite <span class="hlt">ocean</span>-color instruments. One application of this type of lidar data is to estimate primary productivity in the Arctic <span class="hlt">Ocean</span>. It is clear that productivity is increasing, largely as a result of decreased ice cover, but many details remain uncertain.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013BGD....1019633L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013BGD....1019633L"><span>Lytic viral infection of bacterioplankton in deep <span class="hlt">waters</span> of the western Pacific <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Y.; Luo, T.; Sun, J.; Cai, L.; Jiao, N.; Zhang, R.</p> <p>2013-12-01</p> <p>As the most abundant biological entities in the <span class="hlt">ocean</span>, viruses can influence host mortality and nutrients recycling mainly through lytic infection. Yet ecological characteristics of virioplankton and viral impacts on host mortality and biogeochemical cycling in the deep sea are largely unknown. In present study, viral abundance and lytic infection was investigated throughout the <span class="hlt">water</span> column in the western Pacific <span class="hlt">Ocean</span>. Both the prokaryotic and viral abundance and production showed a significantly decreasing trend from epipelagic to meso- and bathypelagic <span class="hlt">waters</span>. Viral abundance decreased from 0.36-1.05 × 1010 particles L-1 to 0.43-0.80 × 109 particles L-1, while the virus : prokaryote ratio varied from 7.21-16.23 to 2.45-23.40, at surface and 2000 m depth, respectively. The lytic viral production rates in surface and 2000 m <span class="hlt">waters</span> were, averagely, 1.03 × 1010 L-1 day-1 and 5.74 × 108 L-1 day-1, respectively. Relatively high percentages of prokaryotic cells lysed by virus in 1000 m and 2000 m were observed, suggesting a significant contribution of viruses to prokaryotic mortality in deep <span class="hlt">ocean</span>. The carbon released by viral lysis in deep western Pacific <span class="hlt">Ocean</span> <span class="hlt">waters</span> was from 0.03 to 2.32 μg C L-1 day-1. Our findings demonstrated a highly dynamic and active viral population in the deep western Pacific <span class="hlt">Ocean</span> and suggested that virioplankton play an important role in the microbial loop and subsequently biogeochemical cycling in deep <span class="hlt">oceans</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/11473308','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/11473308"><span>The stability against freezing of an internal liquid-<span class="hlt">water</span> <span class="hlt">ocean</span> in Callisto.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ruiz, J</p> <p>2001-07-26</p> <p>The discovery of the induced magnetic field of Callisto-one of Jupiter's moons-has been interpreted as evidence for a subsurface <span class="hlt">ocean</span>, even though the presence of such an <span class="hlt">ocean</span> is difficult to understand in the context of existing theoretical models. Tidal heating should not be significant for Callisto, and, in the absence of such heating, it is difficult to see how this internal <span class="hlt">ocean</span> could have survived until today without freezing. Previous work indicated that an outer ice layer on the <span class="hlt">ocean</span> would be unstable against solid-state convection, which once begun would lead to total freezing of liquid <span class="hlt">water</span> in about 108 years. Here I show that when a methodology for more physically reasonable <span class="hlt">water</span> ice viscosities (that is, stress-dependent non-newtonian viscosities, rather than the stress-independent newtonian viscosities considered previously) is adopted, the outer ice shell becomes stable against convection. This implies that a subsurface <span class="hlt">ocean</span> could have survived up to the present, without the need for invoking antifreeze substances or other special conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRC..123.1519G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRC..123.1519G"><span>Seismic Characterization of <span class="hlt">Oceanic</span> <span class="hlt">Water</span> Masses, <span class="hlt">Water</span> Mass Boundaries, and Mesoscale Eddies SE of New Zealand</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gorman, Andrew R.; Smillie, Matthew W.; Cooper, Joanna K.; Bowman, M. Hamish; Vennell, Ross; Holbrook, W. Steven; Frew, Russell</p> <p>2018-02-01</p> <p>The Subtropical and Subantarctic Fronts, which separate Subtropical, Subantarctic, and Antarctic Intermediate <span class="hlt">Waters</span>, are diverted to the south of New Zealand by the submerged continental landmass of Zealandia. In the upper <span class="hlt">ocean</span> of this region, large volumes of dissolved or suspended material are intermittently transported across the Subtropical Front; however, the mechanisms of such transport processes are enigmatic. Understanding these <span class="hlt">oceanic</span> boundaries in three dimensions generally depends on measurements collected from stationary vessels and moorings. The details of these data sets, which are critical for understanding how <span class="hlt">water</span> masses interact and mix at the fine-scale (<10 m) to mesoscale (10-100 km), are inadequately constrained due to resolution considerations. Southeast of New Zealand, high-resolution seismic reflection images of <span class="hlt">oceanic</span> <span class="hlt">water</span> masses have been produced using petroleum industry data. These seismic sections clearly show three main <span class="hlt">water</span> masses, the boundary zones (fronts) between them, and associated thermohaline fine structure that may be related to the mixing of <span class="hlt">water</span> masses in this region. Interpretations of the data suggest that the Subtropical Front in this region is a landward-dipping zone, with a width that can vary between 20 and 40 km. The boundary zone between Subantarctic <span class="hlt">Waters</span> and the underlying Antarctic Intermediate <span class="hlt">Waters</span> is also observed to dip landward. Several isolated lenses have been identified on the three data sets, ranging in size from 9 to 30 km in diameter. These lenses are interpreted to be mesoscale eddies that form at relatively shallow depths along the south side of the Subtropical Front.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27059603','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27059603"><span>Impact of an intense <span class="hlt">water</span> column mixing (0-1500 m) on prokaryotic diversity and activities during an <span class="hlt">open-ocean</span> convection event in the NW Mediterranean Sea.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Severin, Tatiana; Sauret, Caroline; Boutrif, Mehdi; Duhaut, Thomas; Kessouri, Fayçal; Oriol, Louise; Caparros, Jocelyne; Pujo-Pay, Mireille; Durrieu de Madron, Xavier; Garel, Marc; Tamburini, Christian; Conan, Pascal; Ghiglione, Jean-François</p> <p>2016-12-01</p> <p><span class="hlt">Open-ocean</span> convection is a fundamental process for thermohaline circulation and biogeochemical cycles that causes spectacular mixing of the <span class="hlt">water</span> column. Here, we tested how much the depth-stratified prokaryotic communities were influenced by such an event, and also by the following re-stratification. The deep convection event (0-1500 m) that occurred in winter 2010-2011 in the NW Mediterranean Sea resulted in a homogenization of the prokaryotic communities over the entire convective cell, resulting in the predominance of typical surface Bacteria, such as Oceanospirillale and Flavobacteriales. Statistical analysis together with numerical simulation of vertical homogenization evidenced that physical turbulence only was not enough to explain the new distribution of the communities, but acted in synergy with other parameters such as exported particulate and dissolved organic matters. The convection also stimulated prokaryotic abundance (+21%) and heterotrophic production (+43%) over the 0-1500 m convective cell, and resulted in a decline of cell-specific extracellular enzymatic activities (-67%), thus suggesting an intensification of the labile organic matter turnover during the event. The rapid re-stratification of the prokaryotic diversity and activities in the intermediate layer 5 days after the intense mixing indicated a marked resilience of the communities, apart from the residual deep mixed <span class="hlt">water</span> patch. © 2016 The Authors. Environmental Microbiology published by Society for Applied Microbiology and John Wiley & Sons Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/ds/0928/ds928_abstract.html','USGSPUBS'); return false;" href="https://pubs.usgs.gov/ds/0928/ds928_abstract.html"><span>Back-island and <span class="hlt">open-ocean</span> shorelines, and sand areas of Assateague Island, Maryland and Virginia, April 12, 1989, to September 5, 2013</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Guy, Kristy K.</p> <p>2015-01-01</p> <p>This Data Series Report includes several <span class="hlt">open-ocean</span> shorelines, back-island shorelines, back-island shoreline points, sand area polygons, and sand lines for Assateague Island that were extracted from natural-color orthoimagery (aerial photography) dated from April 12, 1989, to September 5, 2013. The images used were 0.3–2-meter (m)-resolution U.S. Geological Survey Digital Orthophoto Quarter Quads (DOQQ), U.S. Department of Agriculture National Agriculture Imagery Program (NAIP) images, and Virginia Geographic Information Network Virginia Base Map Program (VBMP) images courtesy of the Commonwealth of Virginia. The back-island shorelines were hand-digitized at the intersect of the apparent back-island shoreline and transects spaced at 20-m intervals. The <span class="hlt">open-ocean</span> shorelines were hand-digitized at the approximate still <span class="hlt">water</span> level, such as tide level, which was fit through the average position of waves and swash apparent on the beach. Hand-digitizing was done at a scale of approximately 1:2,000. The sand polygons were derived by using an image-processing unsupervised classification technique that separates images into classes. The classes were then visually categorized as either sand or not sand. Also included in this report are 20-m-spaced transect lines and the transect base lines.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.A11C0030M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.A11C0030M"><span>Tropical teleconnections via the <span class="hlt">ocean</span> and atmosphere induced by Southern <span class="hlt">Ocean</span> deep convective events</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marinov, I.; Cabre, A.; Gunn, A.; Gnanadesikan, A.</p> <p>2016-12-01</p> <p>The current generation (CMIP5) of Earth System Models (ESMs) shows a huge variability in their ability to represent Southern <span class="hlt">Ocean</span> (SO) deep-<span class="hlt">ocean</span> convection and Antarctic Bottom <span class="hlt">Water</span>, with a preference for <span class="hlt">open</span>-sea convection in the Weddell and Ross gyres. A long control simulation in a coarse 3o resolution ESM (the GFDL CM2Mc model) shows a highly regular multi-decadal oscillation between periods of SO <span class="hlt">open</span> sea convection and non-convective periods. This process also happens naturally, with different frequencies and durations of convection across most CMIP5 models under preindustrial forcing (deLavergne et al, 2014). Here we assess the impact of SO deep convection and resulting sea surface temperature (SST) anomalies on the tropical atmosphere and <span class="hlt">ocean</span> via teleconnections, with a focus on interannual to multi-decadal timescales. We combine analysis of our low-resolution coupled model with inter-model analysis across historical CMIP5 simulations. SST cooling south of 60S during non-convective decades triggers a stronger, northward shifted SH Hadley cell, which results in intensified northward cross-equatorial moist heat transport and a poleward shift in the ITCZ. Resulting correlations between the cross-equatorial atmospheric heat transport and ITCZ location are in good agreement with recent theories (e.g. Frierson et al. 2013; Donohoe et al. 2014). Lagged correlations between a SO convective index and cross-equatorial heat transports (in the atmosphere and <span class="hlt">ocean</span>), as well as various tropical (and ENSO) climate indices are analyzed. In the <span class="hlt">ocean</span> realm, we find that non-convective decades result in weaker AABW formation and weaker ACC but stronger Antarctic Intermediate <span class="hlt">Water</span> (AAIW) formation, likely as a result of stronger SO westerlies (more positive SAM). The signals of AABW and AAIW are seen in the tropics on short timescales of years to decades in the temperature, heat storage and heat transport anomalies and also in deep and intermediate <span class="hlt">ocean</span> oxygen. Most</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013esm..book..439D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013esm..book..439D"><span>Remote Sensing of <span class="hlt">Ocean</span> Color</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dierssen, Heidi M.; Randolph, Kaylan</p> <p></p> <p>The <span class="hlt">oceans</span> cover over 70% of the earth's surface and the life inhabiting the <span class="hlt">oceans</span> play an important role in shaping the earth's climate. Phytoplankton, the microscopic organisms in the surface <span class="hlt">ocean</span>, are responsible for half of the photosynthesis on the planet. These organisms at the base of the food web take up light and carbon dioxide and fix carbon into biological structures releasing oxygen. Estimating the amount of microscopic phytoplankton and their associated primary productivity over the vast expanses of the <span class="hlt">ocean</span> is extremely challenging from ships. However, as phytoplankton take up light for photosynthesis, they change the color of the surface <span class="hlt">ocean</span> from blue to green. Such shifts in <span class="hlt">ocean</span> color can be measured from sensors placed high above the sea on satellites or aircraft and is called "<span class="hlt">ocean</span> color remote sensing." In <span class="hlt">open</span> <span class="hlt">ocean</span> <span class="hlt">waters</span>, the <span class="hlt">ocean</span> color is predominantly driven by the phytoplankton concentration and <span class="hlt">ocean</span> color remote sensing has been used to estimate the amount of chlorophyll a, the primary light-absorbing pigment in all phytoplankton. For the last few decades, satellite data have been used to estimate large-scale patterns of chlorophyll and to model primary productivity across the global <span class="hlt">ocean</span> from daily to interannual timescales. Such global estimates of chlorophyll and primary productivity have been integrated into climate models and illustrate the important feedbacks between <span class="hlt">ocean</span> life and global climate processes. In coastal and estuarine systems, <span class="hlt">ocean</span> color is significantly influenced by other light-absorbing and light-scattering components besides phytoplankton. New approaches have been developed to evaluate the <span class="hlt">ocean</span> color in relationship to colored dissolved organic matter, suspended sediments, and even to characterize the bathymetry and composition of the seafloor in optically shallow <span class="hlt">waters</span>. <span class="hlt">Ocean</span> color measurements are increasingly being used for environmental monitoring of harmful algal blooms, critical coastal habitats</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AIPC.1810l0001F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AIPC.1810l0001F"><span>A neural network method to correct bidirectional effects in <span class="hlt">water</span>-leaving radiance</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fan, Yongzhen; Li, Wei; Voss, Kenneth J.; Gatebe, Charles K.; Stamnes, Knut</p> <p>2017-02-01</p> <p>The standard method to convert the measured <span class="hlt">water</span>-leaving radiances from the observation direction to the nadir direction developed by Morel and coworkers requires knowledge of the chlorophyll concentration (CHL). Also, the standard method was developed for <span class="hlt">open</span> <span class="hlt">ocean</span> <span class="hlt">water</span>, which makes it unsuitable for turbid coastal <span class="hlt">waters</span>. We introduce a neural network method to convert the <span class="hlt">water</span>-leaving radiance (or the corresponding remote sensing reflectance) from the observation direction to the nadir direction. This method does not require any prior knowledge of the <span class="hlt">water</span> constituents or the inherent optical properties (IOPs). This method is fast, accurate and can be easily adapted to different remote sensing instruments. Validation using NuRADS measurements in different types of <span class="hlt">water</span> shows that this method is suitable for both <span class="hlt">open</span> <span class="hlt">ocean</span> and coastal <span class="hlt">waters</span>. In <span class="hlt">open</span> <span class="hlt">ocean</span> or chlorophyll-dominated <span class="hlt">waters</span>, our neural network method produces corrections similar to those of the standard method. In turbid coastal <span class="hlt">waters</span>, especially sediment-dominated <span class="hlt">waters</span>, a significant improvement was obtained compared to the standard method.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMPP11B1348F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMPP11B1348F"><span>Enhanced deep <span class="hlt">ocean</span> ventilation and oxygenation with global warming</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Froelicher, T. L.; Jaccard, S.; Dunne, J. P.; Paynter, D.; Gruber, N.</p> <p>2014-12-01</p> <p>Twenty-first century coupled climate model simulations, observations from the recent past, and theoretical arguments suggest a consistent trend towards warmer <span class="hlt">ocean</span> temperatures and fresher polar surface <span class="hlt">oceans</span> in response to increased radiative forcing resulting in increased upper <span class="hlt">ocean</span> stratification and reduced ventilation and oxygenation of the deep <span class="hlt">ocean</span>. Paleo-proxy records of the warming at the end of the last ice age, however, suggests a different outcome, namely a better ventilated and oxygenated deep <span class="hlt">ocean</span> with global warming. Here we use a four thousand year global warming simulation from a comprehensive Earth System Model (GFDL ESM2M) to show that this conundrum is a consequence of different rates of warming and that the deep <span class="hlt">ocean</span> is actually better ventilated and oxygenated in a future warmer equilibrated climate consistent with paleo-proxy records. The enhanced deep <span class="hlt">ocean</span> ventilation in the Southern <span class="hlt">Ocean</span> occurs in spite of increased positive surface buoyancy fluxes and a constancy of the Southern Hemisphere westerly winds - circumstances that would otherwise be expected to lead to a reduction in deep <span class="hlt">ocean</span> ventilation. This ventilation recovery occurs through a global scale interaction of the Atlantic Meridional Overturning Circulation undergoing a multi-centennial recovery after an initial century of transient decrease and transports salinity-rich <span class="hlt">waters</span> inform the subtropical surface <span class="hlt">ocean</span> to the Southern <span class="hlt">Ocean</span> interior on multi-century timescales. The subsequent upwelling of salinity-rich <span class="hlt">waters</span> in the Southern <span class="hlt">Ocean</span> strips away the freshwater cap that maintains vertical stability and increases <span class="hlt">open</span> <span class="hlt">ocean</span> convection and the formation of Antarctic Bottom <span class="hlt">Waters</span>. As a result, the global <span class="hlt">ocean</span> oxygen content and the nutrient supply from the deep <span class="hlt">ocean</span> to the surface are higher in a warmer <span class="hlt">ocean</span>. The implications for past and future changes in <span class="hlt">ocean</span> heat and carbon storage will be discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.A31C0039P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.A31C0039P"><span>A <span class="hlt">Water</span> Mass Tracer Detected in Aerosols Demonstrates <span class="hlt">Ocean</span>-Atmosphere Mass Transfer and Links Sea Spray Aerosol to Source <span class="hlt">Waters</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pendergraft, M.; Grimes, D. J.; Giddings, S. N.; Feddersen, F.; Prather, K. A.; Santander, M.; Lee, C.; Beall, C.</p> <p>2016-12-01</p> <p>During September and October of 2015 the Cross Surfzone/Inner-shelf Dye Exchange (CSIDE) project released rhodamine WT dye to study nearshore <span class="hlt">water</span> movement and exchange offshore along a Southern California sandy beach. We utilized this opportunity to investigate <span class="hlt">ocean</span>-atmosphere mass transfer via sea spray aerosol and linkage to source <span class="hlt">waters</span>. Aerosol-concentrating sampling equipment was deployed at beachside and inland locations during three dye releases. Concentrated aerosol samples were analyzed for dye content using fluorescence spectroscopy. Here we present the <span class="hlt">ocean</span> and atmosphere conditions associated with the presence and absence of dye in aerosol samples. Dye was identified in aerosol samples collected 0.1-0.3 km from the shoreline for 6 hs during the first and third dye releases of the CSIDE project. During these releases the dye persisted in the <span class="hlt">waters</span> upwind of the sampling equipment. Dye was not detected in aerosol samples collected during the second release during which dye was moved away from <span class="hlt">waters</span> upwind of the sampling equipment. Recovery of a chemical tracer in sea spray aerosol allows direct linkage to a known source area in the <span class="hlt">ocean</span> that is independent of, but supported by, wind data. Our observations demonstrate: a tight <span class="hlt">ocean</span>-atmosphere spatial coupling; a short residence time of coastal marine constituents before transfer to the atmosphere; that the <span class="hlt">ocean</span> is both a sink for and a source of atmospheric and terrestrial material; and that human inputs to the <span class="hlt">ocean</span> can return to us in sea spray aerosol.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015CRGeo.347..227S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015CRGeo.347..227S"><span>Late Eocene to present isotopic (Sr-Nd-Pb) and geochemical evolution of sediments from the Lomonosov Ridge, Arctic <span class="hlt">Ocean</span>: Implications for continental sources and linkage with the North Atlantic <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stevenson, Ross; Poirier, André; Véron, Alain; Carignan, Jean; Hillaire-Marcel, Claude</p> <p>2015-09-01</p> <p>New geochemical and isotopic (Sr, Nd, Pb) data are presented for a composite sedimentary record encompassing the past 50 Ma of history of sedimentation on the Lomonosov Ridge in the Arctic <span class="hlt">Ocean</span>. The sampled sediments encompass the transition of the Arctic basin from an enclosed anoxic basin to an <span class="hlt">open</span> and ventilated oxidized <span class="hlt">ocean</span> basin. The transition from anoxic basin to <span class="hlt">open</span> ventilated <span class="hlt">ocean</span> is accompanied by at least three geochemical and isotopic shifts and an increase in elements (e.g., K/Al) controlled by detrital minerals highlighting significant changes in sediment types and sources. The isotopic compositions of the sediments prior to ventilation are more variable but indicate a predominance of older crustal contributions consistent with sources from the Canadian Shield. Following ventilation, the isotopic compositions are more stable and indicate an increased contribution from younger material consistent with Eurasian and Pan-African crustal sources. The waxing and waning of these sources in conjunction with the passage of <span class="hlt">water</span> through Fram Strait underlines the importance of the exchange of <span class="hlt">water</span> mass between the Arctic and North Atlantic <span class="hlt">Oceans</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013BGD....10.9179S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013BGD....10.9179S"><span>On the role of mesoscale eddies for the biological productivity and biogeochemistry in the eastern tropical Pacific <span class="hlt">Ocean</span> off Peru</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stramma, L.; Bange, H. W.; Czeschel, R.; Lorenzo, A.; Frank, M.</p> <p>2013-06-01</p> <p>Mesoscale eddies seem to play an important role for both the hydrography and biogeochemistry of the eastern tropical Pacific <span class="hlt">Ocean</span> (ETSP) off Peru. However, detailed surveys of these eddies are not available, which has so far hampered an in depth understanding of their implications for nutrient distribution and biological productivity. In this study three eddies along a section at 16°45' S have been surveyed intensively during R/V Meteor cruise M90 in November 2012. A coastal mode <span class="hlt">water</span> eddy, an <span class="hlt">open</span> <span class="hlt">ocean</span> mode <span class="hlt">water</span> eddy and an <span class="hlt">open</span> <span class="hlt">ocean</span> cyclonic eddy have been identified and sampled in order to determine both their hydrographic properties and their influence on the biogeochemical setting of the ETSP. In the thermocline the temperature of the coastal anticyclonic eddy was up to 2 °C warmer, 0.2 more saline and the swirl velocity was up to 35 cm s-1. The observed temperature and salinity anomalies, as well as swirl velocities of both types of eddies were about twice as large as had been described for the mean eddies in the ETSP and the observed heat and salt anomalies (AHA, ASA) show a much larger variability than the mean AHA and ASA. We found that the eddies contributed significantly to productivity by maintaining pronounced subsurface maxima of chlorophyll. Based on a comparison of the coastal (young) mode <span class="hlt">water</span> eddy and the <span class="hlt">open</span> <span class="hlt">ocean</span> (old) mode <span class="hlt">water</span> eddy we conclude that the aging of eddies when they detach from the coast and move westward to the <span class="hlt">open</span> <span class="hlt">ocean</span> considerably influences the eddies' properties: chlorophyll maxima are weaker and nutrients are subducted. The coastal mode <span class="hlt">water</span> eddy was found to be a hotspot of nitrogen loss in the OMZ, whereas, the <span class="hlt">open</span> <span class="hlt">ocean</span> cyclonic eddy was of negligible importance for nitrogen loss. Our results show that the important role the eddies play in the ETSP can only be fully deciphered and understood through dedicated high spatial and temporal resolution oceanographic/biogeochemical surveys.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20160014496&hterms=layer&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dlayer','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20160014496&hterms=layer&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dlayer"><span>The <span class="hlt">Open-Ocean</span> Sensible Heat Flux and Its Significance for Arctic Boundary Layer Mixing During Early Fall</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ganeshan, Manisha; Wu, Dongliang</p> <p>2016-01-01</p> <p>The increasing ice-free area during late summer has transformed the Arctic to a climate system with more dynamic boundary layer (BL) clouds and seasonal sea ice growth. The <span class="hlt">open-ocean</span> sensible heat flux, a crucial mechanism of excessive <span class="hlt">ocean</span> heat loss to the atmosphere during the fall freeze season, is speculated to play an important role in the recently observed cloud cover increase and BL instability. However, lack of observations and understanding of the resilience of the proposed mechanisms, especially in relation to meteorological and interannual variability, has left a poorly constrained BL parameterization scheme in Arctic climate models. In this study, we use multiyear Japanese cruise-ship observations from RV Mirai over the <span class="hlt">open</span> Arctic <span class="hlt">Ocean</span> to characterize the surface sensible heat flux (SSHF) during early fall and investigate its contribution to BL turbulence. It is found that mixing by SSHF is favored during episodes of high surface wind speed and is also influenced by the prevailing cloud regime. The deepest BLs and maximum <span class="hlt">ocean</span>-atmosphere temperature difference are observed during cold air advection (associated with the stratocumulus regime), yet, contrary to previous speculation, the efficiency of sensible heat exchange is low. On the other hand, the SSHF contributes significantly to BL mixing during the uplift (low pressure) followed by the highly stable (stratus) regime. Overall, it can explain 10 of the <span class="hlt">open</span> <span class="hlt">ocean</span> BL height variability, whereas cloud-driven (moisture and radiative) mechanisms appear to be the other dominant source of convective turbulence. Nevertheless, there is strong interannual variability in the relationship between the SSHF and the BL height which can be intensified by the changing occurrence of Arctic climate patterns, such as positive surface wind speed anomalies and more frequent conditions of uplift. This study highlights the need for comprehensive BL observations like the RV Mirai for better understanding and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3297443','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3297443"><span>Calcification rates and the effect of <span class="hlt">ocean</span> acidification on Mediterranean cold-<span class="hlt">water</span> corals</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Maier, C.; Watremez, P.; Taviani, M.; Weinbauer, M. G.; Gattuso, J. P.</p> <p>2012-01-01</p> <p>Global environmental changes, including <span class="hlt">ocean</span> acidification, have been identified as a major threat to scleractinian corals. General predictions are that <span class="hlt">ocean</span> acidification will be detrimental to reef growth and that 40 to more than 80 per cent of present-day reefs will decline during the next 50 years. Cold-<span class="hlt">water</span> corals (CWCs) are thought to be strongly affected by changes in <span class="hlt">ocean</span> acidification owing to their distribution in deep and/or cold <span class="hlt">waters</span>, which naturally exhibit a CaCO3 saturation state lower than in shallow/warm <span class="hlt">waters</span>. Calcification was measured in three species of Mediterranean cold-<span class="hlt">water</span> scleractinian corals (Lophelia pertusa, Madrepora oculata and Desmophyllum dianthus) on-board research vessels and soon after collection. Incubations were performed in ambient sea <span class="hlt">water</span>. The species M. oculata was additionally incubated in sea <span class="hlt">water</span> reduced or enriched in CO2. At ambient conditions, calcification rates ranged between −0.01 and 0.23% d−1. Calcification rates of M. oculata under variable partial pressure of CO2 (pCO2) were the same for ambient and elevated pCO2 (404 and 867 µatm) with 0.06 ± 0.06% d−1, while calcification was 0.12 ± 0.06% d−1 when pCO2 was reduced to its pre-industrial level (285 µatm). This suggests that present-day CWC calcification in the Mediterranean Sea has already drastically declined (by 50%) as a consequence of anthropogenic-induced <span class="hlt">ocean</span> acidification. PMID:22130603</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/2011PrOce..89...31S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011PrOce..89...31S"><span>Transport of North Pacific 137Cs labeled <span class="hlt">waters</span> to the south-eastern Atlantic <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sanchez-Cabeza, J. A.; Levy, I.; Gastaud, J.; Eriksson, M.; Osvath, I.; Aoyama, M.; Povinec, P. P.; Komura, K.</p> <p>2011-04-01</p> <p>During the reoccupation of the WOCE transect A10 at 30°S by the BEAGLE2003 cruise, the SHOTS project partners collected a large number of samples for the analysis of isotopic tracers. 137Cs was mostly deposited on the <span class="hlt">oceans</span> surface during the late 1950s and early 1960s, after the atmospheric detonation of large nuclear devices, which mostly occurred in the Northern Hemisphere. The development of advanced radioanalytical and counting techniques allowed to obtain, for the first time in this region, a zonal section of 137Cs <span class="hlt">water</span> concentrations, where little information existed before, thus constituting an important benchmark for further studies. 137Cs concentrations in the upper <span class="hlt">waters</span> (0-1000 m) of the south-eastern Atlantic <span class="hlt">Ocean</span> are similar to those observed in the south-western Indian <span class="hlt">Ocean</span>, suggesting transport of 137Cs labeled <span class="hlt">waters</span> by the Agulhas current to the Benguela Current region. In contrast, bomb radiocarbon data do not show this feature, indicating the usefulness of 137Cs as a radiotracer of <span class="hlt">water</span> mass transport from the Indian to the South Atlantic <span class="hlt">Ocean</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1026542','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1026542"><span><span class="hlt">Ocean</span> Profile Measurements During the Seasonal Ice Zone Reconnaissance Surveys <span class="hlt">Ocean</span> Profiles</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2017-01-01</p> <p>repeated <span class="hlt">ocean</span>, ice, and atmospheric measurements across the Beaufort-Chukchi sea seasonal sea ice zone (SIZ) utilizing US Coast Guard Arctic Domain...contributing to the rapid decline in summer ice extent that has occurred in recent years. The SIZ is the region between maximum winter sea ice extent and...minimum summer sea ice extent. As such, it contains the full range of positions of the marginal ice zone (MIZ) where sea ice interacts with <span class="hlt">open</span> <span class="hlt">water</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3896211','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3896211"><span>Role of <span class="hlt">ocean</span> heat transport in climates of tidally locked exoplanets around M dwarf stars</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Hu, Yongyun; Yang, Jun</p> <p>2014-01-01</p> <p>The distinctive feature of tidally locked exoplanets is the very uneven heating by stellar radiation between the dayside and nightside. Previous work has focused on the role of atmospheric heat transport in preventing atmospheric collapse on the nightside for terrestrial exoplanets in the habitable zone around M dwarfs. In the present paper, we carry out simulations with a fully coupled atmosphere–<span class="hlt">ocean</span> general circulation model to investigate the role of <span class="hlt">ocean</span> heat transport in climate states of tidally locked habitable exoplanets around M dwarfs. Our simulation results demonstrate that <span class="hlt">ocean</span> heat transport substantially extends the area of <span class="hlt">open</span> <span class="hlt">water</span> along the equator, showing a lobster-like spatial pattern of <span class="hlt">open</span> <span class="hlt">water</span>, instead of an “eyeball.” For sufficiently high-level greenhouse gases or strong stellar radiation, <span class="hlt">ocean</span> heat transport can even lead to complete deglaciation of the nightside. Our simulations also suggest that <span class="hlt">ocean</span> heat transport likely narrows the width of M dwarfs’ habitable zone. This study provides a demonstration of the importance of exooceanography in determining climate states and habitability of exoplanets. PMID:24379386</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24379386','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24379386"><span>Role of <span class="hlt">ocean</span> heat transport in climates of tidally locked exoplanets around M dwarf stars.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hu, Yongyun; Yang, Jun</p> <p>2014-01-14</p> <p>The distinctive feature of tidally locked exoplanets is the very uneven heating by stellar radiation between the dayside and nightside. Previous work has focused on the role of atmospheric heat transport in preventing atmospheric collapse on the nightside for terrestrial exoplanets in the habitable zone around M dwarfs. In the present paper, we carry out simulations with a fully coupled atmosphere-<span class="hlt">ocean</span> general circulation model to investigate the role of <span class="hlt">ocean</span> heat transport in climate states of tidally locked habitable exoplanets around M dwarfs. Our simulation results demonstrate that <span class="hlt">ocean</span> heat transport substantially extends the area of <span class="hlt">open</span> <span class="hlt">water</span> along the equator, showing a lobster-like spatial pattern of <span class="hlt">open</span> <span class="hlt">water</span>, instead of an "eyeball." For sufficiently high-level greenhouse gases or strong stellar radiation, <span class="hlt">ocean</span> heat transport can even lead to complete deglaciation of the nightside. Our simulations also suggest that <span class="hlt">ocean</span> heat transport likely narrows the width of M dwarfs' habitable zone. This study provides a demonstration of the importance of exooceanography in determining climate states and habitability of exoplanets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFMOS54B..02D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFMOS54B..02D"><span>Fifty Years of <span class="hlt">Water</span> Cycle Change expressed in <span class="hlt">Ocean</span> Salinity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Durack, P. J.; Wijffels, S.</p> <p>2010-12-01</p> <p>Using over 1.6 million profiles of salinity, potential temperature and density from historical archives and Argo, we derive the global field of linear change for <span class="hlt">ocean</span> state properties over the period 1950-2008, taking care to minimise aliasing associated with seasonal and El Nino Southern Oscillation modes. We find large, robust and spatially coherent multi-decadal linear trends in <span class="hlt">ocean</span> surface salinities. Increases are found in evaporation-dominated regions and freshening in precipitation-dominated regions. The spatial patterns of surface change strongly resemble the climatological mean surface salinity field, consistent with an amplification of the global <span class="hlt">water</span> cycle. A robust amplification of the mean salinity pattern of 8% (to 200m depth) is found globally and 5-9% is found in each of the 3 key <span class="hlt">ocean</span> basins. 20th century runs from the CMIP3 model suite support the relationship between amplified patterns of freshwater flux driving an amplified pattern of <span class="hlt">ocean</span> surface salinity only in models that warm substantially. Models with volcanic aerosols show a diminished warming response and a corresponding weak response in <span class="hlt">ocean</span> surface salinity change, which implies dampened changes to the global <span class="hlt">water</span> cycle. The warming response represented in realistic (when compared to observations) 20th century simulations appear quite similar in their broad zonal patterns to those of the projected 21st century simulations, these projected runs being strongly forced by greenhouse gases. This pattern amplification is mostly absent from 20th century simulations which include volcanic forcing. While we confirm that global mean precipitation only weakly change with surface warming (2-3% K-1), the pattern amplification rate in both the freshwater flux and <span class="hlt">ocean</span> salinity fields indicate larger responses. Our new observed salinity estimates suggest a change of between 8-16% K-1, close to, or greater than, the theoretical response described by the Clausius-Clapeyron relation. The</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70177894','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70177894"><span>Dynamic reusable workflows for <span class="hlt">ocean</span> science</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Signell, Richard; Fernandez, Filipe; Wilcox, Kyle</p> <p>2016-01-01</p> <p>Digital catalogs of <span class="hlt">ocean</span> data have been available for decades, but advances in standardized services and software for catalog search and data access make it now possible to create catalog-driven workflows that automate — end-to-end — data search, analysis and visualization of data from multiple distributed sources. Further, these workflows may be shared, reused and adapted with ease. Here we describe a workflow developed within the US Integrated <span class="hlt">Ocean</span> Observing System (IOOS) which automates the skill-assessment of <span class="hlt">water</span> temperature forecasts from multiple <span class="hlt">ocean</span> forecast models, allowing improved forecast products to be delivered for an <span class="hlt">open</span> <span class="hlt">water</span> swim event. A series of Jupyter Notebooks are used to capture and document the end-to-end workflow using a collection of Python tools that facilitate working with standardized catalog and data services. The workflow first searches a catalog of metadata using the <span class="hlt">Open</span> Geospatial Consortium (OGC) Catalog Service for the Web (CSW), then accesses data service endpoints found in the metadata records using the OGC Sensor Observation Service (SOS) for in situ sensor data and OPeNDAP services for remotely-sensed and model data. Skill metrics are computed and time series comparisons of forecast model and observed data are displayed interactively, leveraging the capabilities of modern web browsers. The resulting workflow not only solves a challenging specific problem, but highlights the benefits of dynamic, reusable workflows in general. These workflows adapt as new data enters the data system, facilitate reproducible science, provide templates from which new scientific workflows can be developed, and encourage data providers to use standardized services. As applied to the <span class="hlt">ocean</span> swim event, the workflow exposed problems with two of the <span class="hlt">ocean</span> forecast products which led to improved regional forecasts once errors were corrected. While the example is specific, the approach is general, and we hope to see increased use of dynamic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26097744','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26097744"><span>A daily global mesoscale <span class="hlt">ocean</span> eddy dataset from satellite altimetry.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Faghmous, James H; Frenger, Ivy; Yao, Yuanshun; Warmka, Robert; Lindell, Aron; Kumar, Vipin</p> <p>2015-01-01</p> <p>Mesoscale <span class="hlt">ocean</span> eddies are ubiquitous coherent rotating structures of <span class="hlt">water</span> with radial scales on the order of 100 kilometers. Eddies play a key role in the transport and mixing of momentum and tracers across the World <span class="hlt">Ocean</span>. We present a global daily mesoscale <span class="hlt">ocean</span> eddy dataset that contains ~45 million mesoscale features and 3.3 million eddy trajectories that persist at least two days as identified in the AVISO dataset over a period of 1993-2014. This dataset, along with the <span class="hlt">open</span>-source eddy identification software, extract eddies with any parameters (minimum size, lifetime, etc.), to study global eddy properties and dynamics, and to empirically estimate the impact eddies have on mass or heat transport. Furthermore, our <span class="hlt">open</span>-source software may be used to identify mesoscale features in model simulations and compare them to observed features. Finally, this dataset can be used to study the interaction between mesoscale <span class="hlt">ocean</span> eddies and other components of the Earth System.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4460914','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4460914"><span>A daily global mesoscale <span class="hlt">ocean</span> eddy dataset from satellite altimetry</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Faghmous, James H.; Frenger, Ivy; Yao, Yuanshun; Warmka, Robert; Lindell, Aron; Kumar, Vipin</p> <p>2015-01-01</p> <p>Mesoscale <span class="hlt">ocean</span> eddies are ubiquitous coherent rotating structures of <span class="hlt">water</span> with radial scales on the order of 100 kilometers. Eddies play a key role in the transport and mixing of momentum and tracers across the World <span class="hlt">Ocean</span>. We present a global daily mesoscale <span class="hlt">ocean</span> eddy dataset that contains ~45 million mesoscale features and 3.3 million eddy trajectories that persist at least two days as identified in the AVISO dataset over a period of 1993–2014. This dataset, along with the <span class="hlt">open</span>-source eddy identification software, extract eddies with any parameters (minimum size, lifetime, etc.), to study global eddy properties and dynamics, and to empirically estimate the impact eddies have on mass or heat transport. Furthermore, our <span class="hlt">open</span>-source software may be used to identify mesoscale features in model simulations and compare them to observed features. Finally, this dataset can be used to study the interaction between mesoscale <span class="hlt">ocean</span> eddies and other components of the Earth System. PMID:26097744</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012GeoRL..3918601B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012GeoRL..3918601B"><span>Microbial control of diatom bloom dynamics in the <span class="hlt">open</span> <span class="hlt">ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Boyd, Philip W.; Strzepek, Robert; Chiswell, Steve; Chang, Hoe; DeBruyn, Jennifer M.; Ellwood, Michael; Keenan, Sean; King, Andrew L.; Maas, Elisabeth W.; Nodder, Scott; Sander, Sylvia G.; Sutton, Philip; Twining, Benjamin S.; Wilhelm, Steven W.; Hutchins, David A.</p> <p>2012-09-01</p> <p>Diatom blooms play a central role in supporting foodwebs and sequestering biogenic carbon to depth. <span class="hlt">Oceanic</span> conditions set bloom initiation, whereas both environmental and ecological factors determine bloom magnitude and longevity. Our study reveals another fundamental determinant of bloom dynamics. A diatom spring bloom in offshore New Zealand <span class="hlt">waters</span> was likely terminated by iron limitation, even though diatoms consumed <1/3 of the mixed-layer dissolved iron inventory. Thus, bloom duration and magnitude were primarily set by competition for dissolved iron between microbes and small phytoplankton versus diatoms. Significantly, such a microbial mode of control probably relies both upon out-competing diatoms for iron (i.e., K-strategy), and having high iron requirements (i.e., r-strategy). Such resource competition for iron has implications for carbon biogeochemistry, as, blooming diatoms fixed three-fold more carbon per unit iron than resident non-blooming microbes. Microbial sequestration of iron has major ramifications for determining the biogeochemical imprint of <span class="hlt">oceanic</span> diatom blooms.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/18793309','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/18793309"><span>Diversity of deep-<span class="hlt">water</span> cetaceans in relation to temperature: implications for <span class="hlt">ocean</span> warming.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Whitehead, Hal; McGill, Brian; Worm, Boris</p> <p>2008-11-01</p> <p>Understanding the effects of natural environmental variation on biodiversity can help predict response to future anthropogenic change. Here we analyse a large, long-term data set of sightings of deep-<span class="hlt">water</span> cetaceans from the Atlantic, Pacific and Indian <span class="hlt">Oceans</span>. Seasonal and geographic changes in the diversity of these genera are well predicted by a convex function of sea-surface temperature peaking at c. 21 degrees C. Thus, diversity is highest at intermediate latitudes - an emerging general pattern for the pelagic <span class="hlt">ocean</span>. When applied to a range of Intergovernmental Panel on Climate Change global change scenarios, the predicted response is a decline of cetacean diversity across the tropics and increases at higher latitudes. This suggests that deep-<span class="hlt">water</span> <span class="hlt">oceanic</span> communities that dominate > 60% of the planet's surface may reorganize in response to <span class="hlt">ocean</span> warming, with low-latitude losses of diversity and resilience.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EOSTr..95R.477W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EOSTr..95R.477W"><span>New data aid estimate of <span class="hlt">ocean</span>'s plastic content</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wendel, JoAnna</p> <p>2014-12-01</p> <p>Experts estimate that 5.25 trillion plastic particles—weighing in at nearly 269,000 tons—are floating in the world's <span class="hlt">oceans</span>. A new paper in the <span class="hlt">open</span> access journal PLOS ONE (doi:10.1371/journal.pone.011191) about the abundance of plastic in the <span class="hlt">oceans</span> combines data from 24 expeditions between 2007 and 2013. These expeditions cover all five subtropical gyres—areas of high pressure where seawater churns and sinks—as well as Australian coastal <span class="hlt">waters</span>, the Bay of Bengal, and even the Mediterranean Sea.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24554022','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24554022"><span>Monitoring of <span class="hlt">ocean</span> surface algal blooms in coastal and <span class="hlt">oceanic</span> <span class="hlt">waters</span> around India.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tholkapiyan, Muniyandi; Shanmugam, Palanisamy; Suresh, T</p> <p>2014-07-01</p> <p>The National Aeronautics and Space Administration's (NASA) sensor MODIS-Aqua provides an important tool for reliable observations of the changing <span class="hlt">ocean</span> surface algal bloom paradigms in coastal and <span class="hlt">oceanic</span> <span class="hlt">waters</span> around India. A time series of the MODIS-Aqua-derived OSABI (<span class="hlt">ocean</span> surface algal bloom index) and its seasonal composite images report new information and comprehensive pictures of these blooms and their evolution stages in a wide variety of events occurred at different times of the years from 2003 to 2011, providing the first large area survey of such phenomena around India. For most of the years, the results show a strong seasonal pattern of surface algal blooms elucidated by certain physical and meteorological conditions. The extent of these blooms reaches a maximum in winter (November-February) and a minimum in summer (June-September), especially in the northern Arabian Sea. Their spatial distribution and retention period are also significantly increased in the recent years. The increased spatial distribution and intensity of these blooms in the northern Arabian Sea in winter are likely caused by enhanced cooling, increased convective mixing, favorable winds, and atmospheric deposition of the mineral aerosols (from surrounding deserts) of the post-southwest monsoon period. The southward Oman coastal current and southwestward winds become apparently responsible for their extension up to the central Arabian Sea. Strong upwelling along this coast further triggers their initiation and growth. Though there is a warming condition associated with increased sea surface height anomalies along the coasts of India and Sri Lanka in winter, surface algal bloom patches are still persistent along these coasts due to northeast monsoonal winds, enhanced precipitation, and subsequent nutrient enrichment in these areas. The occurrence of the surface algal blooms in the northern Bay of Bengal coincides with a region of the well-known Ganges-Brahmaputra Estuarine Frontal</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGC53H..03F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC53H..03F"><span>Earth 2075 (CO2) - can <span class="hlt">Ocean</span>-Amplified Carbon Capture (oacc) Impart Atmospheric CO2-SINKING Ability to CCS Fossil Energy?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fry, R.; Routh, M.; Chaudhuri, S.; Fry, S.; Ison, M.; Hughes, S.; Komor, C.; Klabunde, K.; Sethi, V.; Collins, D.; Polkinghorn, W.; Wroobel, B.; Hughes, J.; Gower, G.; Shkolnik, J.</p> <p>2017-12-01</p> <p>Previous attempts to capture atmospheric CO2 by algal blooming were stalled by <span class="hlt">ocean</span> viruses, zooplankton feeding, and/or bacterial decomposition of surface blooms, re-releasing captured CO2 instead of exporting it to seafloor. CCS fossil energy coupling could bypass algal bloom limits—enabling capture of 10 GtC/yr atmospheric CO2 by selective emiliania huxleyi (EHUX) blooming in mid-latitude <span class="hlt">open</span> <span class="hlt">oceans</span>, far from coastal <span class="hlt">waters</span> and polar seas. This could enable a 500 GtC drawdown, 350 ppm restoration by 2050, 280 ppm CO2 by 2075, and <span class="hlt">ocean</span> pH 8.2. White EHUX blooms could also reflect sunlight back into outer space and seed extra <span class="hlt">ocean</span> cloud cover, via DMS release, to raise albedo 1.8%—restoring preindustrial temperature (ΔT = 0°C) by 2030. <span class="hlt">Open</span> <span class="hlt">oceans</span> would avoid post-bloom anoxia, exclusively a coastal <span class="hlt">water</span> phenomenon. The EHUX calcification reaction initially sources CO2, but net sinking prevails in follow-up equilibration reactions. Heavier-than-<span class="hlt">water</span> EHUX sink captured CO2 to the sea floor before surface decomposition occurs. Seeding EHUX high on their nonlinear growth curve could accelerate short-cycle secondary <span class="hlt">open-ocean</span> blooming—overwhelming mid-latitude viruses, zooplankton, and competition from other algae. Mid-latitude "<span class="hlt">ocean</span> deserts" exhibit low viral, zooplankton, and bacterial counts. Thermocline prevents nutrient upwelling that would otherwise promote competing algae. Adding nitrogen nutrient would foster exclusive EHUX blooming. Elevated EHUX seed levels could arise from sealed, pH-buffered, floating, seed-production bioreactors infused with 10% CO2 from carbon feedstock supplied by inland CCS fossil power plants capturing 90% of emissions as liquid CO2. Deep-<span class="hlt">water</span> SPAR platforms extract natural gas from beneath the sea floor. On-platform Haber and pH processing could convert extracted CH4 to buffered NH4+ nutrient, enabling ≥0.7 GtC/yr of bioreactor seed production and 10 GtC/yr of amplified secondary <span class="hlt">open-ocean</span> CO2 capture—making CCS</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.B51A0408R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.B51A0408R"><span>Latitudinal change in precipitation and <span class="hlt">water</span> vapor isotopes over Southern <span class="hlt">ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rahul, P.</p> <p>2015-12-01</p> <p>The evaporation process over <span class="hlt">ocean</span> is primary source of <span class="hlt">water</span> vapor in the hydrological cycle. The Global Network of Isotopes in Precipitation (GNIP) dataset of rainwater and <span class="hlt">water</span> vapor isotopes are predominantly based on continental observations, with very limited observation available from the <span class="hlt">oceanic</span> area. Stable isotope ratios in precipitation provide valuable means to understand the process of evaporation and transport of <span class="hlt">water</span> vapor. This is further extended in the study of past changes in climate from the isotopic composition of ice core. In this study we present latitudinal variability of <span class="hlt">water</span> vapor and rainwater isotopic composition and compared it with factors like physical condition of sea surface <span class="hlt">water</span> from near equator (1°S) to the polar front (56°S) during the summer time expedition of the year 2013. The <span class="hlt">water</span> vapor and rainwater isotopes showed a sharp depletion in isotopes while progressively move southward from the tropical regions (i.e. >30°S), which follows the pattern recorded in the surface <span class="hlt">ocean</span> <span class="hlt">water</span> isotopic composition. From the tropics to the southern latitudes, the <span class="hlt">water</span> vapor d18O varied between -11.8‰ to -14.7‰ while dD variation ranges between -77.7‰ to -122.2‰. Using the data we estimated the expected <span class="hlt">water</span> vapor isotopic composition under kinetic as well as equilibrium process. Our observation suggests that the <span class="hlt">water</span> vapor isotopic compositions are in equilibrium with the sea <span class="hlt">water</span> in majority of cases. At one point of observation, where trajectory of air parcel originated from the continental region, we observed a large deviation from the existing trend of latitudinal variability. The deduced rainwater composition adopting equilibrium model showed a consistent pattern with observed values at the tropical region, while role of kinetic process become dominant on progressive shift towards the southern latitudes. We will draw comparison of our observation with other data available in the literature together with isotope</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22559948','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22559948"><span>Mercury biogeochemical cycling in the <span class="hlt">ocean</span> and policy implications.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mason, Robert P; Choi, Anna L; Fitzgerald, William F; Hammerschmidt, Chad R; Lamborg, Carl H; Soerensen, Anne L; Sunderland, Elsie M</p> <p>2012-11-01</p> <p>Anthropogenic activities have enriched mercury in the biosphere by at least a factor of three, leading to increases in total mercury (Hg) in the surface <span class="hlt">ocean</span>. However, the impacts on <span class="hlt">ocean</span> fish and associated trends in human exposure as a result of such changes are less clear. Here we review our understanding of global mass budgets for both inorganic and methylated Hg species in <span class="hlt">ocean</span> seawater. We consider external inputs from atmospheric deposition and rivers as well as internal production of monomethylmercury (CH₃Hg) and dimethylmercury ((CH₃)₂Hg). Impacts of large-scale <span class="hlt">ocean</span> circulation and vertical transport processes on Hg distribution throughout the <span class="hlt">water</span> column and how this influences bioaccumulation into <span class="hlt">ocean</span> food chains are also discussed. Our analysis suggests that while atmospheric deposition is the main source of inorganic Hg to <span class="hlt">open</span> <span class="hlt">ocean</span> systems, most of the CH₃Hg accumulating in <span class="hlt">ocean</span> fish is derived from in situ production within the upper <span class="hlt">waters</span> (<1000 m). An analysis of the available data suggests that concentrations in the various <span class="hlt">ocean</span> basins are changing at different rates due to differences in atmospheric loading and that the deeper <span class="hlt">waters</span> of the <span class="hlt">oceans</span> are responding slowly to changes in atmospheric Hg inputs. Most biological exposures occur in the upper <span class="hlt">ocean</span> and therefore should respond over years to decades to changes in atmospheric mercury inputs achieved by regulatory control strategies. Migratory pelagic fish such as tuna and swordfish are an important component of CH₃Hg exposure for many human populations and therefore any reduction in anthropogenic releases of Hg and associated deposition to the <span class="hlt">ocean</span> will result in a decline in human exposure and risk. Copyright © 2012 Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3427470','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3427470"><span>Mercury Biogeochemical Cycling in the <span class="hlt">Ocean</span> and Policy Implications</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Mason, Robert P.; Choi, Anna L.; Fitzgerald, William F.; Hammerschmidt, Chad R.; Lamborg, Carl H.; Soerensen, Anne L.; Sunderland, Elsie M.</p> <p>2012-01-01</p> <p>Anthropogenic activities have enriched mercury in the biosphere by at least a factor of three, leading to increases in total mercury (Hg) in the surface <span class="hlt">ocean</span>. However, the impacts on <span class="hlt">ocean</span> fish and associated trends in human exposure as a result of such changes are less clear. Here we review our understanding of global mass budgets for both inorganic and methylated Hg species in <span class="hlt">ocean</span> seawater. We consider external inputs from atmospheric deposition and rivers as well as internal production of monomethylmercury (CH3Hg) and dimethylmercury ((CH3)2Hg). Impacts of large-scale <span class="hlt">ocean</span> circulation and vertical transport processes on Hg distribution throughout the <span class="hlt">water</span> column and how this influences bioaccumulation into <span class="hlt">ocean</span> food chains are also discussed. Our analysis suggests that while atmospheric deposition is the main source of inorganic Hg to <span class="hlt">open</span> <span class="hlt">ocean</span> systems, most of the CH3Hg accumulating in <span class="hlt">ocean</span> fish is derived from in situ production within the upper <span class="hlt">waters</span> (<1000 m). An analysis of the available data suggests that concentrations in the various <span class="hlt">ocean</span> basins are changing at different rates due to differences in atmospheric loading and that the deeper <span class="hlt">waters</span> of the <span class="hlt">oceans</span> are responding slowly to changes in atmospheric Hg inputs. Most biological exposures occur in the upper <span class="hlt">ocean</span> and therefore should respond over years to decades to changes in atmospheric mercury inputs achieved by regulatory control strategies. Migratory pelagic fish such as tuna and swordfish are an important component of CH3Hg exposure for many human populations and therefore any reduction in anthropogenic releases of Hg and associated deposition to the <span class="hlt">ocean</span> will result in a decline in human exposure and risk. PMID:22559948</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JMEP...26.2337L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JMEP...26.2337L"><span>Slow Strain Rate Testing for Hydrogen Embrittlement Susceptibility of Alloy 718 in Substitute <span class="hlt">Ocean</span> <span class="hlt">Water</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>LaCoursiere, M. P.; Aidun, D. K.; Morrison, D. J.</p> <p>2017-05-01</p> <p>The hydrogen embrittlement susceptibility of near-peak-aged UNS N07718 (Alloy 718) was evaluated by performing slow strain rate tests at room temperature in air and substitute <span class="hlt">ocean</span> <span class="hlt">water</span>. Tests in substitute <span class="hlt">ocean</span> <span class="hlt">water</span> were accomplished in an environmental cell that enabled in situ cathodic charging under an applied potential of -1.1 V versus SCE. Some specimens were cathodically precharged for 4 or 16 weeks at the same potential in a 3.5 wt.% NaCl-distilled <span class="hlt">water</span> solution at 50 °C. Unprecharged specimens tested in substitute <span class="hlt">ocean</span> <span class="hlt">water</span> exhibited only moderate embrittlement with plastic strain to failure decreasing by about 20% compared to unprecharged specimens tested in air. However, precharged specimens exhibited significant embrittlement with plastic strain to failure decreasing by about 70%. Test environment (air or substitute <span class="hlt">ocean</span> <span class="hlt">water</span> with in situ charging) and precharge time (4 or 16 weeks) had little effect on the results of the precharged specimens. Fracture surfaces of precharged specimens were typical of hydrogen embrittlement and consisted of an outer brittle ring related to the region in which hydrogen infused during precharging, a finely dimpled transition zone probably related to the region where hydrogen was drawn in by dislocation transport, and a central highly dimpled ductile region. Fracture surfaces of unprecharged specimens tested in substitute <span class="hlt">ocean</span> <span class="hlt">water</span> consisted of a finely dimpled outer ring and heavily dimpled central region typical of ductile fracture.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140011897','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140011897"><span>Hyperspectral Imager for the Coastal <span class="hlt">Ocean</span> (HICO): Overview, Operational Updates, and Coastal <span class="hlt">Ocean</span> Applications</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Davis, Curtiss O.; Kappus, Mary E.; Bowles, Jeffrey H.; Evans, Cynthia A.; Stefanov, William L.</p> <p>2014-01-01</p> <p>The Hyperspectral Imager for the Coastal <span class="hlt">Ocean</span> (HICO) was built to measure in-<span class="hlt">water</span> properties of complex coastal regions. HICO enables synoptic coverage; 100-meter spatial resolution for sampling the variability and spatial irregularity of coastal <span class="hlt">waters</span>; and high spectral resolution to untangle the signals from chlorophyll, colored dissolved organic matter, suspended sediments and varying bottom types. HICO was built by the Naval Research Laboratory, installed on the International Space Station (ISS) in September 2009, and operated for ONR for the first three years. In 2013, NASA assumed sponsorship of operations in order to leverage HICO's ability to address their Earth monitoring mission. This has <span class="hlt">opened</span> up access of HICO data to the broad research community. Over 8000 images are now available on NASA's <span class="hlt">Ocean</span> Color Website (http://oceancolor.gsfc.nasa.gov/cgi/browse.pl?sen=hi). Oregon State University's HICO website (http://hico.coas.oregonstate.edu) remains the portal for researchers to request new collections and access their requested data. We will present updates on HICO's calibration and improvements in geolocation and show examples of the use of HICO data to address issues in the coastal <span class="hlt">ocean</span> and Great Lakes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.7429S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.7429S"><span>Interannual variability (1979-2013) of the North-Western Mediterranean deep <span class="hlt">water</span> mass formation: past observation reanalysis and coupled <span class="hlt">ocean</span>-atmosphere high-resolution modelling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Somot, Samuel; Houpert, Loic; Sevault, Florence; Testor, Pierre; Bosse, Anthony; Durrieu de Madron, Xavier; Dubois, Clotilde; Herrmann, Marine; Waldman, Robin; Bouin, Marie-Noëlle; Cassou, Christophe</p> <p>2015-04-01</p> <p>The North-Western Mediterranean Sea is known as one of the only place in the world where <span class="hlt">open</span>-sea deep convection occurs (often up to more than 2000m) with the formation of the Western Mediterranean Deep <span class="hlt">Water</span> (WMDW). This phenomena is mostly driven by local preconditioning of the <span class="hlt">water</span> column and strong buoyancy losses during Winter. At the event scale, the WMDW formation is characterized by different phases (preconditioning, strong mixing, restratification and spreading), intense air-sea interaction and strong meso-scale activity but, on a longer time scale, it also shows a large interannual variability and may be strongly affected by climate change with impact on the regional biogeochemistry. Therefore observing, simulating and understanding the long-term temporal variability of the North-Western Mediterranean deep <span class="hlt">water</span> formation is still today a very challenging task. We try here to tackle those issues thanks to (1) a thorough reanalysis of past in-situ observations (CTD, Argo, surface and deep moorings, gliders) and (2) an ERA-Interim driven simulation using a recently-developed fully coupled Regional Climate System Model (CNRM-RCSM4, Sevault et al. 2014). The multi-decadal simulation (1979-2013) is designed to be temporally and spatially homogeneous with a realistic chronology, a high resolution representation of both the regional <span class="hlt">ocean</span> and atmosphere, specific initial conditions, a long-term spin-up and a full <span class="hlt">ocean</span>-atmosphere coupling without constraint at the air-sea interface. The observation reanalysis allows to reconstruct interannual time series of deep <span class="hlt">water</span> formation indicators (<span class="hlt">ocean</span> surface variables, mixed layer depth, surface of the convective area, dense <span class="hlt">water</span> volumes and characteristics of the deep <span class="hlt">water</span>). Using the observation-based indicators and the model outputs, the 34 Winters of the period 1979-2013 are analysed in terms of weather regimes, related Winter air-sea fluxes, <span class="hlt">ocean</span> preconditioning, mixed layer depth, surface of the convective</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017LPICo2042.4050R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017LPICo2042.4050R"><span>Bacterial Growth in the Salty Liquid <span class="hlt">Water</span> <span class="hlt">Ocean</span> of Europa</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rubio, D. G.; Ramírez, S. I.</p> <p>2017-11-01</p> <p>We are interested in the adaptation strategies displayed by bacteria when exposed to laboratory-controlled conditions that represent the salinity, temperature, and available oxygen conditions of the salty liquid <span class="hlt">water</span> <span class="hlt">ocean</span> present on Europa.</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/2016EGUGA..18.5212K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.5212K"><span>Continuous, high-resolution spatial mapping of <span class="hlt">water</span> isotopes in <span class="hlt">oceanic</span> environment using a CRDS analyzer combined with a continuous <span class="hlt">water</span> sampler.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kim-Hak, David; Huang, Kuan; Winkler, Renato</p> <p>2016-04-01</p> <p>The recent advancements of the laser-based technology -in particular Cavity Ring Down Spectroscopy, CRDS- gave birth to a new generation of <span class="hlt">water</span> stable isotope analyzers that are user-friendly, compact and field deployable providing in-situ measurements. Furthermore, with last year's launch of the Continuous <span class="hlt">Water</span> Sampler front-end, CWS, the analyzer system added two additional dimensions to liquid <span class="hlt">water</span> measurements: real-time and continuous. These features enable the user to construct high resolution <span class="hlt">water</span> isotope data sets through time and space. Campaigns on the Sacramento-San Joaquin River Delta with the US Geological Survey where the CWS-CRDS system was deployed onto a boat to spatially map sections of the delta, validated the CWS performance and demonstrated its durability on brackish <span class="hlt">water</span>. The next step for the CWS is to explore <span class="hlt">oceanic</span> applications with seawater. Early in-house laboratory experiments showed stable performance with brine <span class="hlt">waters</span> (3% concentration). For the field experiment, we have collaborated with the China State <span class="hlt">Oceanic</span> Administration to deploy the CWS-CRDS in <span class="hlt">oceanic</span> environments on cruises along the costal China and Antarctic. Here, we present the results of the analysis collected onboard and compared them with discrete sampling measurements. The long-term test has also allowed us to assess the durability and expected lifetime of the CWS membrane and to recommend the proper maintenance procedure for optimum performance under <span class="hlt">oceanic</span> conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSIS52A..04K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSIS52A..04K"><span>Continuous, high-resolution spatial mapping of <span class="hlt">water</span> isotopes in <span class="hlt">oceanic</span> environment using a CRDS analyzer combined with a continuous <span class="hlt">water</span> sampler.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kim-Hak, D.; Huang, K.</p> <p>2016-02-01</p> <p>The recent advancements of the laser-based technology -in particular Cavity Ring Down Spectroscopy, CRDS- gave birth to a new generation of <span class="hlt">water</span> stable isotope analyzers that are user-friendly, compact and field deployable providing in-situ measurements. Furthermore, with last year's launch of the Continuous <span class="hlt">Water</span> Sampler front-end, CWS, the analyzer system added two additional dimensions to liquid <span class="hlt">water</span> measurements: real-time and continuous. These features enable the user to construct high resolution <span class="hlt">water</span> isotope data sets through time and space. Campaigns on the Sacramento-San Joaquin River Delta with the US Geological Survey where the CWS-CRDS system was deployed onto a boat to spatially map sections of the delta, validated the CWS performance and demonstrated its durability on brackish <span class="hlt">water</span>. The next step for the CWS is to explore <span class="hlt">oceanic</span> applications with seawater. Early in-house laboratory experiments showed stable performance with brine <span class="hlt">waters</span> (3% concentration). For the field experiment, we have collaborated with the China State <span class="hlt">Oceanic</span> Administration to deploy the CWS-CRDS in <span class="hlt">oceanic</span> environments on cruises along the costal China and Antarctic. Here, we present the results of the analysis collected onboard and compared them with discrete sampling measurements. The long-term test has also allowed us to assess the durability and expected lifetime of the CWS membrane and to recommend the proper maintenance procedure for optimum performance under <span class="hlt">oceanic</span> conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..1411524T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..1411524T"><span>Accuracy assessment of satellite <span class="hlt">Ocean</span> colour products in coastal <span class="hlt">waters</span>.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tilstone, G.; Lotliker, A.; Groom, S.</p> <p>2012-04-01</p> <p>The use of <span class="hlt">Ocean</span> Colour Remote Sensing to monitor phytoplankton blooms in coastal <span class="hlt">waters</span> is hampered by the absorption and scattering from substances in the <span class="hlt">water</span> that vary independently of phytoplankton. In this paper we compare different <span class="hlt">ocean</span> colour algorithms available for SeaWiFS, MODIS and MERIS with in situ observations of Remote Sensing Reflectance, Chlorophyll-a (Chla), Total Suspended Material and Coloured Dissolved Organic Material in coastal <span class="hlt">waters</span> of the Arabian Sea, Bay of Bengal, North Sea and Western English Channel, which have contrasting inherent optical properties. We demonstrate a clustering method on specific-Inherent Optical Properties (sIOP) that gives accurate <span class="hlt">water</span> quality products from MERIS data (HYDROPT) and also test the recently developed ESA CoastColour MERIS products. We found that for coastal <span class="hlt">waters</span> of the Bay of Bengal, OC5 gave the most accurate Chla, for the Arabian Sea GSM and OC3M Chla were more accurate and for the North Sea and Western English Channel, MERIS HYDROPT were more accurate than standard algorithms. The reasons for these differences will be discussed. A Chla time series from 2002-2011 will be presented to illustrate differences in algorithms between coastal regions and inter- and intra-annual variability in phytoplankton blooms</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS41C1989M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS41C1989M"><span>Self-organization of hydrothermal outflow and recharge in young <span class="hlt">oceanic</span> crust: Constraints from <span class="hlt">open</span>-top porous convection analog experiments</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mittelstaedt, E. L.; Olive, J. A. L.; Barreyre, T.</p> <p>2016-12-01</p> <p>Hydrothermal circulation at the axis of mid-<span class="hlt">ocean</span> ridges has a profound effect on chemical and biological processes in the deep <span class="hlt">ocean</span>, and influences the thermo-mechanical state of young <span class="hlt">oceanic</span> lithosphere. Yet, the geometry of fluid pathways beneath the seafloor and its relation to spatial gradients in crustal permeability remain enigmatic. Here we present new laboratory models of hydrothermal circulation aimed at constraining the self-organization of porous convection cells in homogeneous as well as highly heterogeneous crust analogs. <span class="hlt">Oceanic</span> crust analogs of known permeability are constructed using uniform glass spheres and 3-D printed plastics with a network of mutually perpendicular tubes. These materials are saturated with corn syrup-<span class="hlt">water</span> mixtures and heated at their base by a resistive silicone strip heater to initiate thermal convection. A layer of pure fluid (i.e., an analog <span class="hlt">ocean</span>) overlies the porous medium and allows an "<span class="hlt">open</span>-top" boundary condition. Areas of fluid discharge from the crust into the <span class="hlt">ocean</span> are identified by illuminating microscopic glass particles carried by the fluid, using laser sheets. Using particle image velocimetry, we estimate fluid discharge rates as well as the location and extent of fluid recharge. Thermo-couples distributed throughout the crust provide insights into the geometry of convection cells at depth, and enable estimates of convective heat flux, which can be compared to the heat supplied at the base of the system. Preliminary results indicate that in homogeneous crust, convection is largely confined to the narrow slot overlying the heat source. Regularly spaced discharge zones appear focused while recharge areas appear diffuse, and qualitatively resemble the along-axis distribution of hydrothermal fields at <span class="hlt">oceanic</span> spreading centers. By varying the permeability of the crustal analogs, the viscosity of the convecting fluid, and the imposed basal temperature, our experiments span Rayleigh numbers between 10 and 10</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeCoA.199..222C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeCoA.199..222C"><span>The <span class="hlt">open</span> sea as the main source of methylmercury in the <span class="hlt">water</span> column of the Gulf of Lions (Northwestern Mediterranean margin)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cossa, Daniel; Durrieu de Madron, Xavier; Schäfer, Jörg; Lanceleur, Laurent; Guédron, Stéphane; Buscail, Roselyne; Thomas, Bastien; Castelle, Sabine; Naudin, Jean-Jacques</p> <p>2017-02-01</p> <p>Despite the ecologic and economical importance of coastal areas, the neurotoxic bioaccumulable monomethylmercury (MMHg) fluxes within the <span class="hlt">ocean</span> margins and exchanges with the <span class="hlt">open</span> sea remain unassessed. The aim of this paper is to address the questions of the abundance, distribution, production and exchanges of methylated mercury species (MeHgT), including MMHg and dimethylmercury (DMHg), in the <span class="hlt">waters</span>, atmosphere and sediments of the Northwestern Mediterranean margin including the Rhône River delta, the continental shelf and its slope (Gulf of Lions) and the adjacent <span class="hlt">open</span> sea (North Gyre). Concentrations of MeHgT ranged from <0.02 to 0.48 pmol L-1 with highest values associated with the oxygen-deficient zone of the <span class="hlt">open</span> sea. The methylated mercury to total mercury proportion (MeHgT/HgT) increased from 2% to 4% in the Rhône River to up to 30% (averaging 18%) in the North Gyre <span class="hlt">waters</span>, whereas, within the shelf <span class="hlt">waters</span>, MeHgT/HgT proportions were the lowest (1-3%). We calculate that the <span class="hlt">open</span> sea is the major source of MeHgT for the shelf <span class="hlt">waters</span>, with an annual flux estimated at 0.68 ± 0.12 kmol a-1 (i.e., equivalent to 12% of the HgT flux). This MeHgT influx is more than 80 times the direct atmospheric deposition or the in situ net production, more than 40 times the estimated "maximum potential" annual efflux from shelf sediment, and more than 7 times that of the continental sources. In the <span class="hlt">open</span> sea, ratios of MMHg/DMHg in <span class="hlt">waters</span> were always <1 and minimum in the oxygen deficient zones of the <span class="hlt">water</span> column, where MeHg concentrations are maximum. This observation supports the idea that MMHg could be a degradation product of DMHg produced from inorganic divalent Hg.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013BGeo...10.2787C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013BGeo...10.2787C"><span><span class="hlt">Water</span> column distribution and carbon isotopic signal of cholesterol, brassicasterol and particulate organic carbon in the Atlantic sector of the Southern <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cavagna, A.-J.; Dehairs, F.; Bouillon, S.; Woule-Ebongué, V.; Planchon, F.; Delille, B.; Bouloubassi, I.</p> <p>2013-04-01</p> <p>The combination of concentrations and δ13C signatures of Particulate Organic Carbon (POC) and sterols provides a powerful approach to study ecological and environmental changes in both the modern and ancient <span class="hlt">ocean</span>. We applied this tool to study the biogeochemical changes in the modern <span class="hlt">ocean</span> <span class="hlt">water</span> column during the BONUS-GoodHope survey (February-March 2008) from Cape Basin to the northern part of the Weddell Gyre. Cholesterol and brassicasterol were chosen as ideal biomarkers of the heterotrophic and autotrophic carbon pools, respectively, because of their ubiquitous and relatively refractory nature. We document depth distributions of concentrations (relative to bulk POC) and δ13C signatures of cholesterol and brassicasterol combined with CO2 aq. surface concentration variation. While the relationship between CO2 aq. and δ13C of bulk POC and biomarkers have been reported by others for the surface <span class="hlt">water</span>, our data show that this persists in mesopelagic and deep <span class="hlt">waters</span>, suggesting that δ13C signatures of certain biomarkers in the <span class="hlt">water</span> column could be applied as proxies for surface <span class="hlt">water</span> CO2 aq. We observed a general increase in sterol δ13C signatures with depth, which is likely related to a combination of particle size effects, selective feeding on larger cells by zooplankton, and growth rate related effects. Our data suggest a key role of zooplankton fecal aggregates in carbon export for this part of the Southern <span class="hlt">Ocean</span> (SO). Additionally, in the southern part of the transect south of the Polar Front (PF), the release of sea-ice algae during the ice demise in the Seasonal Ice Zone (SIZ) is hypothesized to influence the isotopic signature of sterols in the <span class="hlt">open</span> <span class="hlt">ocean</span>. Overall, the combined use of δ13C values and concentrations measurements of both bulk organic C and specific sterols throughout the <span class="hlt">water</span> column offers the promising potential to explore the recent history of plankton and the fate of organic matter in the SO.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006GBioC..20.4S04K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006GBioC..20.4S04K"><span>Production of giant marine diatoms and their export at <span class="hlt">oceanic</span> frontal zones: Implications for Si and C flux from stratified <span class="hlt">oceans</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kemp, A. E. S.; Pearce, R. B.; Grigorov, I.; Rance, J.; Lange, C. B.; Quilty, P.; Salter, I.</p> <p>2006-12-01</p> <p>From a synthesis of recent <span class="hlt">oceanic</span> observations and paleo-data it is evident that certain species of giant diatoms including Rhizosolenia spp. Thalassiothrix spp. and Ethmodiscus rex may become concentrated at <span class="hlt">oceanic</span> frontal zones and subsequently form episodes of mass flux to the sediment. Within the nutrient bearing <span class="hlt">waters</span> advecting towards frontal boundaries, these species are generally not dominant, but they appear selectively segregated at fronts, and thus may dominate the export flux. Ancient Thalassiothrix diatom mat deposits in the eastern equatorial Pacific and beneath the Polar Front in the Southern <span class="hlt">Ocean</span> record the highest <span class="hlt">open</span> <span class="hlt">ocean</span> sedimentation rates ever documented and represent vast sinks of silica and carbon. Several of the species involved are adapted to a stratified <span class="hlt">water</span> column and may thrive in Deep Chlorophyll Maxima. Thus in <span class="hlt">oceanic</span> regions and/or at times prone to enhanced surface <span class="hlt">water</span> stratification (e.g., during meltwater pulses) they provide a mechanism for generating substantial biomass at depth and its subsequent export with concomitant implications for Si export and C drawdown. This ecology has important implications for <span class="hlt">ocean</span> biogeochemical models suggesting that more than one diatom "functional type" should be used. In spite of the importance of these giant diatoms for biogeochemical cycling, their large size coupled with the constraints of conventional oceanographic survey schemes and techniques means that they are undersampled. An improved insight into these key species will be an important prerequisite for enhancing our understanding of marine biogeochemical cycling and for assessing the impacts of climate change on <span class="hlt">ocean</span> export production.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1998PhDT.......230P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1998PhDT.......230P"><span>Nonhydrostatic thermohaline convection in the polar <span class="hlt">oceans</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Potts, Mark Allen</p> <p></p> <p>Sea ice cover in the polar and sub-polar seas is an important and sensitive component of the Earth's climate system. It mediates the transfer of heat and momentum between the <span class="hlt">ocean</span> and the atmosphere in high latitude <span class="hlt">oceans</span>. Where <span class="hlt">open</span> patches occur in the ice cover a large transfer of heat from the <span class="hlt">ocean</span> to the atmosphere occurs that accounts for a large fraction of energy exchange between the wintertime polar <span class="hlt">ocean</span> and atmosphere. Although the circumstances under which leads and polynyas form are considerably different, similar brine driven convection occurs under both. Convection beneath freezing ice in leads and polynyas can be modeled using either the hydrostatic or nonhydrostatic form of the governing equations. One important question is the degree of nonhydrostaticity, which depends on the vertical accelerations present. This issue is addressed through the application of a nonhydrostatic model, with accurate treatment of the turbulent mixing. The results suggest that mixing and re-freezing considerably modify the fluid dynamical processes underneath, such as the periodic shedding of saline plumes. It also appears that overall, the magnitude of the nonhydrostaticity is small, and hydrostatic models are generally adequate to deal with the problem of convection under leads. Strong wintertime cooling drives deep convection in sub-polar seas and in the coastal <span class="hlt">waters</span> surrounding Antarctica. Deep convection results in formation of deep <span class="hlt">water</span> in the global <span class="hlt">oceans</span>, which is of great importance to the maintenance of the stratification of its deep interior, and the resulting meridional circulation is central to the Earth's climatic state. Deep convection falls into two general categories: <span class="hlt">open</span> <span class="hlt">ocean</span> deep convection, which occurs in deep stretches of the high latitude seas far from topographical influences, and convection on or near the continental shelves, where topography exerts a considerable influence. Nonhydrostatic models are central to the study of deep</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19900053698&hterms=microwaves+water+structure&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dmicrowaves%2Bwater%2Bstructure','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19900053698&hterms=microwaves+water+structure&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dmicrowaves%2Bwater%2Bstructure"><span>Atmospheric <span class="hlt">water</span> vapour over <span class="hlt">oceans</span> from SSM/I measurements</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Schluessel, Peter; Emery, William J.</p> <p>1990-01-01</p> <p>A statistical retrieval technique is developed to derive the atmospheric <span class="hlt">water</span> vapor column content from the Special Sensor Microwave/Imager (SSM/I) measurements. The radiometer signals are simulated by means of radiative-transfer calculations for a large set of atmospheric/<span class="hlt">oceanic</span> situations. These simulated responses are subsequently summarized by multivariate analyses, giving <span class="hlt">water</span>-vapor coefficients and error estimates. Radiative-transfer calculations show that the SSM/I microwave imager can detect atmospheric <span class="hlt">water</span> vapor structures with an accuracy from 0.145 to 0.17 g/sq cm. The accuracy of the method is confirmed by globally distributed match-ups with radiosonde measurements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016GeoRL..43.3822M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GeoRL..43.3822M"><span>Rapid variability of Antarctic Bottom <span class="hlt">Water</span> transport into the Pacific <span class="hlt">Ocean</span> inferred from GRACE</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mazloff, Matthew R.; Boening, Carmen</p> <p>2016-04-01</p> <p>Air-ice-<span class="hlt">ocean</span> interactions in the Antarctic lead to formation of the densest <span class="hlt">waters</span> on Earth. These <span class="hlt">waters</span> convect and spread to fill the global abyssal <span class="hlt">oceans</span>. The heat and carbon storage capacity of these <span class="hlt">water</span> masses, combined with their abyssal residence times that often exceed centuries, makes this circulation pathway the most efficient sequestering mechanism on Earth. Yet monitoring this pathway has proven challenging due to the nature of the formation processes and the depth of the circulation. The Gravity Recovery and Climate Experiment (GRACE) gravity mission is providing a time series of <span class="hlt">ocean</span> mass redistribution and offers a transformative view of the abyssal circulation. Here we use the GRACE measurements to infer, for the first time, a 2003-2014 time series of Antarctic Bottom <span class="hlt">Water</span> export into the South Pacific. We find this export highly variable, with a standard deviation of 1.87 sverdrup (Sv) and a decorrelation timescale of less than 1 month. A significant trend is undetectable.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.B33J..02G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.B33J..02G"><span>Asian dust transportation and fertilizing the coastal and <span class="hlt">open</span> <span class="hlt">ocean</span> in the Northern Pacific (Invited)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gao, H.; Xiaohong Yao, Jinhui Shi, Jianhua Qi</p> <p>2010-12-01</p> <p>Dust storm carries a large amount of aerosol particles, sweeps continents and exports to <span class="hlt">oceans</span>. When these aerosol particles deposit in <span class="hlt">ocean</span>, which provides abundant nutrients such as nitrogen and iron for <span class="hlt">ocean</span> ecosystem, increases the primary production and induces algae bloom. Asian dust storm generates at a high latitude and a high elevation and is obvious a hemispheric scale phenomenon. Dust sources in East Asia are one of the major dust sources on the earth which contribute to 5%-40% of the global dust release. The regions affected by the Asian dust storm include not only China and Mongolia but also the downwind Korea, Japan, the Pacific <span class="hlt">Ocean</span>, the west coast of America, even the subarctic region and Europe. The Asian dust storm is obviously a hemispheric scale phenomenon, which has more important impact on the ecosystem in the western Pacific. Asian dust is unique not only in morphology, soil texture, and dust storm activities, but also mixing and capturing anthropogenic air pollutants on the transport pathway. Deposition of Asian dust substantially affects surface biological productivity. To improve understandings of Asian dust and its effect on <span class="hlt">ocean</span> ecosystem from the coastal sea to <span class="hlt">open</span> <span class="hlt">ocean</span>, ADOES (Asian Dust and <span class="hlt">Ocean</span> EcoSystem) was proposed under the frame of international SOLAS (Surface <span class="hlt">Ocean</span>-Lower Atmosphere Study). A series of studies were performed in high- nutrient low-chlorophyll (HNLC), low-nutrient low-chlorophyll (LNLC) and eutrophication coastal regions of the Pacific <span class="hlt">Ocean</span>. These studies provided evidence of biotic response to natural iron fertilization caused by Asian dust particles in the subarctic North Pacific and showed that dust storm episodes were significant in the initiation of spring blooms in the East China Sea. On-board incubations on the cruise in a LNLC region of the western Pacific at the southeast of Japan showed different responses of <span class="hlt">ocean</span> ecosystem to nitrogen and dust fertilization. Correlation of the Asian dust</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSHE14A1382W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSHE14A1382W"><span>Pathways of Atlantic <span class="hlt">Waters</span> in the Nordic seas: locally eddy-permitting <span class="hlt">ocean</span> simulation in a global setup</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wekerle, C.; Wang, Q.; Danilov, S.; Jung, T.; Schourup-Kristensen, V.</p> <p>2016-02-01</p> <p>Atlantic <span class="hlt">Water</span> (AW) passes through the Nordic Seas and enters the Arctic <span class="hlt">Ocean</span> through the shallow Barents Sea and the deep Fram Strait. Since the 1990's, observations indicate a series of anomalously warm pulses of Atlantic <span class="hlt">Water</span> that entered the Arctic <span class="hlt">Ocean</span>. In fact, poleward <span class="hlt">oceanic</span> heat transport may even increase in the future, which might have implications for the heat uptake in the Arctic <span class="hlt">Ocean</span> as well as for the sea ice cover. The ability of models to faithfully simulate the pathway of the AW and accompanying dynamics is thus of high climate relevance. In this study, we explore the potential of a global multi-resolution sea ice-<span class="hlt">ocean</span> model with a locally eddy-permitting resolution (around 4.5 km) in the Nordic seas region and Arctic <span class="hlt">Ocean</span> in improving the representation of Atlantic <span class="hlt">Water</span> inflow, and more broadly, the dynamics of the circulation in the Northern North Atlantic and Arctic. The simulation covers the time period 1969-2009. We find that locally increased resolution improves the localization and thickness of the Atlantic <span class="hlt">Water</span> layer in the Nordic seas, compared with a 20 km resolution reference simulation. In particular, the inflow of Atlantic <span class="hlt">Waters</span> through the Greenland Scotland Ridge and the narrow branches of the Norwegian Atlantic Current can be realistically represented. Lateral spreading due to simulated eddies essentially reduces the bias in the surface temperature. In addition, a qualitatively good agreement of the simulated eddy kinetic energy field with observations can be achieved. This study indicates that a substantial improvement in representing local <span class="hlt">ocean</span> dynamics can be reached through the local refinement, which requires a rather moderate computational effort. The successful model assessment allows us to further investigate the variability and mechanisms behind Atlantic <span class="hlt">Water</span> transport into the Arctic <span class="hlt">Ocean</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1193435','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1193435"><span>Drake passage and central american seaway controls on the distribution of the <span class="hlt">oceanic</span> carbon reservoir</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Fyke, Jeremy G.; D'Orgeville, Marc; Weaver, Andrew J.</p> <p>2015-05-01</p> <p>A coupled carbon/climate model is used to explore the impact of Drake Passage <span class="hlt">opening</span> and Central American Seaway closure on the distribution of carbon in the global <span class="hlt">oceans</span>. We find that gateway evolution likely played an important role in setting the modern day distribution of <span class="hlt">oceanic</span> dissolved inorganic carbon (DIC), which is currently characterized by relatively low concentrations in the Atlantic <span class="hlt">ocean</span>, and high concentrations in the Southern, Indian, and Pacific <span class="hlt">oceans</span>. In agreement with previous studies, we find a closed Drake Passage in the presence of an <span class="hlt">open</span> Central American Seaway results in suppressed Atlantic meridional overturning and enhancedmore » southern hemispheric deep convection. <span class="hlt">Opening</span> of the Drake Passage triggers Antarctic Circumpolar Current flow and a weak Atlantic meridional overturning circulation (AMOC). Subsequent Central American Seaway closure reinforces the AMOC while also stagnating equatorial Pacific subsurface <span class="hlt">waters</span>. These gateway-derived oceanographic changes are reflected in large shifts to the global distribution of DIC. An initially closed Drake Passage results in high DIC concentrations in the Atlantic and Arctic <span class="hlt">oceans</span>, and lower DIC concentrations in the Pacific/Indian/Southern <span class="hlt">oceans</span>. <span class="hlt">Opening</span> Drake Passage reverses this gradient by lowering mid-depth Atlantic and Arctic DIC concentrations and raising deep Pacific/Indian/Southern <span class="hlt">Ocean</span> DIC concentrations. Central American Seaway closure further reinforces this trend through additional Atlantic mid-depth DIC decreases, as well as Pacific mid-depth DIC concentration increases, with the net effect being a transition to a modern distribution of <span class="hlt">oceanic</span> DIC.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22128794','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22128794"><span>Occurrence of perfluoroalkyl compounds in surface <span class="hlt">waters</span> from the North Pacific to the Arctic <span class="hlt">Ocean</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Cai, Minghong; Zhao, Zhen; Yin, Zhigao; Ahrens, Lutz; Huang, Peng; Cai, Minggang; Yang, Haizhen; He, Jianfeng; Sturm, Renate; Ebinghaus, Ralf; Xie, Zhiyong</p> <p>2012-01-17</p> <p>Perfluoroalkyl compounds (PFCs) were determined in 22 surface <span class="hlt">water</span> samples (39-76°N) and three sea ice core and snow samples (77-87°N) collected from North Pacific to the Arctic <span class="hlt">Ocean</span> during the fourth Chinese Arctic Expedition in 2010. Geographically, the average concentration of ∑PFC in surface <span class="hlt">water</span> samples were 560 ± 170 pg L(-1) for the Northwest Pacific <span class="hlt">Ocean</span>, 500 ± 170 pg L(-1) for the Arctic <span class="hlt">Ocean</span>, and 340 ± 130 pg L(-1) for the Bering Sea, respectively. The perfluoroalkyl carboxylates (PFCAs) were the dominant PFC class in the <span class="hlt">water</span> samples, however, the spatial pattern of PFCs varied. The C(5), C(7) and C(8) PFCAs (i.e., perfluoropentanoate (PFPA), perfluoroheptanoate (PFHpA), and perfluorooctanoate (PFOA)) were the dominant PFCs in the Northwest Pacific <span class="hlt">Ocean</span> while in the Bering Sea the PFPA dominated. The changing in the pattern and concentrations in Pacific <span class="hlt">Ocean</span> indicate that the PFCs in surface <span class="hlt">water</span> were influenced by sources from the East-Asian (such as Japan and China) and North American coast, and dilution effect during their transport to the Arctic. The presence of PFCs in the snow and ice core samples indicates an atmospheric deposition of PFCs in the Arctic. The elevated PFC concentration in the Arctic <span class="hlt">Ocean</span> shows that the ice melting had an impact on the PFC levels and distribution. In addition, the C(4) and C(5) PFCAs (i.e., perfluorobutanoate (PFBA), PFPA) became the dominant PFCs in the Arctic <span class="hlt">Ocean</span> indicating that PFBA is a marker for sea ice melting as the source of exposure.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.B22C..08W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.B22C..08W"><span>Assessing the Feasibility and Risks of Using Wave-Driven Upwelling Pumps to Enhance the Biological Sequestration of Carbon in <span class="hlt">Open</span> <span class="hlt">Oceans</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>White, A.; Bjorkman, K.; Grabowski, E.; Letelier, R. M.; Poulos, S.; Watkins, B.; Karl, D. M.</p> <p>2008-12-01</p> <p>In 1976, John D. Isaacs proposed to use wave energy to pump cold and nutrient-rich deep <span class="hlt">water</span> into the sunlit surface layers. The motivation for this endeavor has taken many forms over the years, from energy production to fueling aquaculture to the more recent suggestion that artificial upwelling could be used to stimulate primary productivity and anthropogenic carbon sequestration in oligotrophic regions of the <span class="hlt">ocean</span>. However, the potential for biological carbon sequestration in response to upwelling will depend on the concentration of nutrients relative to that of dissolved inorganic carbon in the <span class="hlt">water</span> being upwelled and on the response of the marine microbial assemblage to this nutrient enrichment. In June 2008, we tested a commercially available wave pump in the vicinity of Station ALOHA, north of Oahu, Hawaii in order to assess the logistics of at-sea deployment and the survivability of the equipment in the <span class="hlt">open</span> <span class="hlt">ocean</span>. Our engineering test was also designed to evaluate a recently published hypothesis (Karl and Letelier, 2008, Marine Ecology Progress Series) that upwelling of <span class="hlt">water</span> containing excess phosphate relative to nitrogen compared to the canonical "Redfield" molar ratio of 16N:1P, would generate a two-phased phytoplankton bloom and enhance carbon sequestration. In this presentation, we analyze the results of this field test within the context of pelagic biogeochemical cycles. Furthermore, we discuss the deployment of a 300m wave pump, efforts to sample a biochemical response, the engineering challenges faced and the practical and ethical implications of these results for future experiments aimed at stimulating the growth of phytoplankton in oligotrophic regions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26208139','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26208139"><span>Co-occurring Synechococcus ecotypes occupy four major <span class="hlt">oceanic</span> regimes defined by temperature, macronutrients and iron.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sohm, Jill A; Ahlgren, Nathan A; Thomson, Zachary J; Williams, Cheryl; Moffett, James W; Saito, Mak A; Webb, Eric A; Rocap, Gabrielle</p> <p>2016-02-01</p> <p>Marine picocyanobacteria, comprised of the genera Synechococcus and Prochlorococcus, are the most abundant and widespread primary producers in the <span class="hlt">ocean</span>. More than 20 genetically distinct clades of marine Synechococcus have been identified, but their physiology and biogeography are not as thoroughly characterized as those of Prochlorococcus. Using clade-specific qPCR primers, we measured the abundance of 10 Synechococcus clades at 92 locations in surface <span class="hlt">waters</span> of the Atlantic and Pacific <span class="hlt">Oceans</span>. We found that Synechococcus partition the <span class="hlt">ocean</span> into four distinct regimes distinguished by temperature, macronutrients and iron availability. Clades I and IV were prevalent in colder, mesotrophic <span class="hlt">waters</span>; clades II, III and X dominated in the warm, oligotrophic <span class="hlt">open</span> <span class="hlt">ocean</span>; clades CRD1 and CRD2 were restricted to sites with low iron availability; and clades XV and XVI were only found in transitional <span class="hlt">waters</span> at the edges of the other biomes. Overall, clade II was the most ubiquitous clade investigated and was the dominant clade in the largest biome, the oligotrophic <span class="hlt">open</span> <span class="hlt">ocean</span>. Co-occurring clades that occupy the same regime belong to distinct evolutionary lineages within Synechococcus, indicating that multiple ecotypes have evolved independently to occupy similar niches and represent examples of parallel evolution. We speculate that parallel evolution of ecotypes may be a common feature of diverse marine microbial communities that contributes to functional redundancy and the potential for resiliency.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4737926','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4737926"><span>Co-occurring Synechococcus ecotypes occupy four major <span class="hlt">oceanic</span> regimes defined by temperature, macronutrients and iron</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Sohm, Jill A; Ahlgren, Nathan A; Thomson, Zachary J; Williams, Cheryl; Moffett, James W; Saito, Mak A; Webb, Eric A; Rocap, Gabrielle</p> <p>2016-01-01</p> <p>Marine picocyanobacteria, comprised of the genera Synechococcus and Prochlorococcus, are the most abundant and widespread primary producers in the <span class="hlt">ocean</span>. More than 20 genetically distinct clades of marine Synechococcus have been identified, but their physiology and biogeography are not as thoroughly characterized as those of Prochlorococcus. Using clade-specific qPCR primers, we measured the abundance of 10 Synechococcus clades at 92 locations in surface <span class="hlt">waters</span> of the Atlantic and Pacific <span class="hlt">Oceans</span>. We found that Synechococcus partition the <span class="hlt">ocean</span> into four distinct regimes distinguished by temperature, macronutrients and iron availability. Clades I and IV were prevalent in colder, mesotrophic <span class="hlt">waters</span>; clades II, III and X dominated in the warm, oligotrophic <span class="hlt">open</span> <span class="hlt">ocean</span>; clades CRD1 and CRD2 were restricted to sites with low iron availability; and clades XV and XVI were only found in transitional <span class="hlt">waters</span> at the edges of the other biomes. Overall, clade II was the most ubiquitous clade investigated and was the dominant clade in the largest biome, the oligotrophic <span class="hlt">open</span> <span class="hlt">ocean</span>. Co-occurring clades that occupy the same regime belong to distinct evolutionary lineages within Synechococcus, indicating that multiple ecotypes have evolved independently to occupy similar niches and represent examples of parallel evolution. We speculate that parallel evolution of ecotypes may be a common feature of diverse marine microbial communities that contributes to functional redundancy and the potential for resiliency. PMID:26208139</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=307077&Lab=NHEERL&keyword=Physical+AND+Review&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50','EPA-EIMS'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=307077&Lab=NHEERL&keyword=Physical+AND+Review&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50"><span>A Method to Identify Estuarine <span class="hlt">Water</span> Quality Exceedances Associated with <span class="hlt">Ocean</span> Conditions</span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p>Wind driven coastal upwelling along the Pacific Northwest Coast of the US results in <span class="hlt">oceanic</span> <span class="hlt">water</span> that may be periodically entrained into adjacent estuaries and which possess high nutrients and low dissolved oxygen (DO). Measurement of <span class="hlt">water</span> quality indicators during these upwe...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1992JMS.....3..279E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1992JMS.....3..279E"><span><span class="hlt">Water</span>-mass formation and Sverdrup dynamics; a comparison between climatology and a coupled <span class="hlt">ocean</span>-atmosphere model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>England, Matthew H.; Tomczak, Matthias; Stuart Godfrey, J.</p> <p>1992-06-01</p> <p>The coupled <span class="hlt">ocean</span>-atmosphere model integrations of Manabe and Stouffer (1988) are compared with climatological distributions of depth-integrated flow and <span class="hlt">water</span>-mass formation. The description of the <span class="hlt">ocean</span> circulation in their two quasi-stable equilibria is extended to include an analysis of the horizontal and meridional transport as well as the <span class="hlt">water</span>-mass formation and vertical motion in the model. In particular, the wind-driven Sverdrup flow is computed and compared with the actual mass transport streamfunction of the model. It is found that a Sverdrup model of depth-integrated flow captures the major features of the coupled model's <span class="hlt">ocean</span> circulation, except near region of deep <span class="hlt">water</span> formation, where the thermohaline field drives <span class="hlt">ocean</span> currents and wind-driven flow becomes secondary. The coupled model fails to allow for a barotropic mass transport through the Indonesian Passage. Instead, only baroclinically driven fluxes of heat and freshwater are resolved through the Indonesian Archipelago. The Sverdrup model suggests that a barotropic throughflow would transport about 16 Sv from the Pacific to Indian <span class="hlt">Oceans</span>. According to Sverdrup dynamics, this would serve to weaken the East Australian Current by about 16 Sv and strengthen the Agulhas Current by the same amount. Recent integrations of a World <span class="hlt">Ocean</span> model with and without a barotropic throughflow in the Indonesian Passage suggest that the modelled heat transport is sensitive to the nature of flow through the Indonesian Archipelago. From' a comparison of observed and simulated <span class="hlt">water</span> mass properties, it is shown that some major aspects of the global-scale <span class="hlt">water</span> masses are not captured by the coupled model. This reveals a shortcoming of the model's ability to represent the global-scale heat and freshwater balances. For example, there is an unrealistically intense halocline in the immediate vicinity of Antartica, prohibiting the formation of bottom <span class="hlt">water</span> in the Weddell and Ross Seas. Also, no low salinity traces of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2011-05-31/pdf/2011-13329.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2011-05-31/pdf/2011-13329.pdf"><span>76 FR 31235 - Safety Zone; <span class="hlt">Ocean</span> City Air Show, Atlantic <span class="hlt">Ocean</span>, <span class="hlt">Ocean</span> City, MD</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2011-05-31</p> <p>...-AA00 Safety Zone; <span class="hlt">Ocean</span> City Air Show, Atlantic <span class="hlt">Ocean</span>, <span class="hlt">Ocean</span> City, MD AGENCY: Coast Guard, DHS. ACTION... in the vicinity of <span class="hlt">Ocean</span> City, MD to support the <span class="hlt">Ocean</span> City Air Show. This action is necessary to provide for the safety of life on navigable <span class="hlt">waters</span> during the <span class="hlt">Ocean</span> City Air Show. This action is intended...</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/2016AGUFMGC33C1252H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMGC33C1252H"><span>Terrestrial <span class="hlt">water</span> cycle induced meridional overturning circulation variability over the Atlantic <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hsu, C. W.; Velicogna, I.</p> <p>2016-12-01</p> <p>Terrestrial <span class="hlt">water</span> cycle has a significant role in the long-term changes of Atlantic meridional overturning circulation (AMOC). With the fresh <span class="hlt">water</span> input over the <span class="hlt">ocean</span> from the river runoff or ice melting at the higher latitude, AMOC transport has been predicted to slow down at the end of the century. We compare <span class="hlt">ocean</span> bottom pressure measured from the GRACE satellite data with the conventional density derived transport observations from the RAPID MOC/MOCHA array to study the impact of the terrestrial <span class="hlt">water</span> cycle on the seasonal and inter annual AMOC variability detected by the RAPID MOC/MOCHA array observations. We propose that the observed short-term variability is due to coupling of wind driven and terrestrial <span class="hlt">water</span> cycle changes. We show that the proposed mechanism explains a significant portion of the transport variance and we present new possible mechanism that can explain the residual transport signal in AMOC.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19850017730&hterms=Parkinsons+circulation&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DParkinsons%2Bcirculation','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19850017730&hterms=Parkinsons+circulation&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DParkinsons%2Bcirculation"><span>Possible Sea Ice Impacts on <span class="hlt">Oceanic</span> Deep Convection</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.</p> <p>1984-01-01</p> <p>Many regions of the world <span class="hlt">ocean</span> known or suspected to have deep convection are sea-ice covered for at least a portion of the annual cycle. As this suggests that sea ice might have some impact on generating or maintaining this phenomenon, several mechanisms by which sea ice could exert an influence are presented in the following paragraphs. Sea ice formation could be a direct causal factor in deep convection by providing the surface density increase necessary to initiate the convective overturning. As sea ice forms, either by ice accretion or by in situ ice formation in <span class="hlt">open</span> <span class="hlt">water</span> or in lead areas between ice floes, salt is rejected to the underlying <span class="hlt">water</span>. This increases the <span class="hlt">water</span> salinity, thereby increasing <span class="hlt">water</span> density in the mixed layer under the ice. A sufficient increase in density will lead to mixing with deeper <span class="hlt">waters</span>, and perhaps to deep convection or even bottom <span class="hlt">water</span> formation. Observations are needed to establish whether this process is actually occurring; it is most likely in regions with extensive ice formation and a relatively unstable <span class="hlt">oceanic</span> density structure.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2013-05-31/pdf/2013-12888.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2013-05-31/pdf/2013-12888.pdf"><span>78 FR 32556 - Safety Zone; 2013 <span class="hlt">Ocean</span> City Air Show, Atlantic <span class="hlt">Ocean</span>; <span class="hlt">Ocean</span> City, MD</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2013-05-31</p> <p>...-AA00 Safety Zone; 2013 <span class="hlt">Ocean</span> City Air Show, Atlantic <span class="hlt">Ocean</span>; <span class="hlt">Ocean</span> City, MD AGENCY: Coast Guard, DHS... navigable <span class="hlt">waters</span> of the Atlantic <span class="hlt">Ocean</span> in the vicinity of <span class="hlt">Ocean</span> City, MD to support the <span class="hlt">Ocean</span> City Air Show... June 9, 2013, <span class="hlt">Ocean</span> City, MD will host an air show event between Talbot Street and 33rd Street over the...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.3059S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.3059S"><span><span class="hlt">Oceanic</span> magmatic evolution during <span class="hlt">ocean</span> <span class="hlt">opening</span> under influence of mantle plume</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sushchevskaya, Nadezhda; Melanholina, Elena; Belyatsky, Boris; Krymsky, Robert; Migdisova, Natalya</p> <p>2015-04-01</p> <p>Petrology, geochemistry and geophysics as well as numerical simulation of spreading processes in plume impact environments on examples of Atlantic <span class="hlt">Ocean</span> Iceland and the Central Atlantic plumes and Kerguelen plume in the Indian <span class="hlt">Ocean</span> reveal: - under interaction of large plume and continental landmass the plume can contribute to splitting off individual lithosphere blocks, and their subsequent movement into the emergent <span class="hlt">ocean</span>. At the same time enriched plume components often have geochemical characteristics of the intact continental lithosphere by early plume exposure. This is typical for trap magmatism in Antarctica, and for magmatism of North and Central Atlantic margins; - in the course of the geodynamic reconstruction under the whole region of the South Atlantic was formed (not in one step) metasomatized enriched sub-<span class="hlt">oceanic</span> mantle with pyroxenite mantle geochemical characteristics and isotopic composition of enriched HIMU and EM-2 sources. That is typical for most of the islands in the West Antarctic. This mantle through spreading axes jumping involved in different proportions in the melting under the influence of higher-temperature rising asthenospheric lherzolite mantle; - CAP activity was brief enough (200 ± 2 Ma), but Karoo-Maud plume worked for a longer time and continued from 180 to 170 Ma ago in the main phase. Plume impact within Antarctica distributed to the South and to the East, leading to the formation of extended igneous provinces along the Transantarctic Mountains and along the east coast (Queen Maud Land province and Schirmacher Oasis). Moreover, this plume activity may be continued later on, after about 40 million years cessation, as Kerguelen plume within the newly-formed Indian <span class="hlt">Ocean</span>, significantly affects the nature of the rift magmatism; - a large extended uplift in the eastern part of the Indian <span class="hlt">Ocean</span> - Southeastern Indian Ridge (SEIR) was formed on the ancient spreading Wharton ridge near active Kerguelen plume. The strongest plume</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016SPIE.9999E..0JP','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016SPIE.9999E..0JP"><span>Enhancing moderate-resolution <span class="hlt">ocean</span> color products over coastal/inland <span class="hlt">waters</span> (Conference Presentation)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pahlevan, Nima; Schott, John R.; Zibordi, Giuseppe</p> <p>2016-10-01</p> <p>With the successful launch of Landsat-8 in 2013 followed by a very recent launch of Sentinel-2A, we are entering a new area where frequent moderate resolution <span class="hlt">water</span> quality products over coastal/inland <span class="hlt">waters</span> will be available to scientists and operational agencies. Although designed for land observations, the Operational Land Imager (OLI) has proven to provide high-fidelity products in these aquatic systems where coarse-resolution <span class="hlt">ocean</span> color imagers fail to provide valid observations. High-quality, multi-scale <span class="hlt">ocean</span> color products can give insights into the biogeochemical/physical processes from the upstream in watersheds, into near-shore regions, and further out in <span class="hlt">ocean</span> basins. In this research, we describe a robust cross-calibration approach, which facilitates seamless <span class="hlt">ocean</span> color products at multi scales. The top-of-atmosphere (TOA) OLI imagery is cross-calibrated against near-simultaneous MODIS and VIIRS <span class="hlt">ocean</span> color observations in high-latitude regions. This allows for not only examining the overall relative performance of OLI but also for characterizing non-uniformity (i.e., banding) across its swath. The uncertainty of this approach is, on average, found to be less than 0.5% in the blue channels. The adjustments made for OLI TOA reflectance products are then validated against in-situ measurements of remote sensing reflectance collected in research cruises or at the AERONET-OC.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20000120582&hterms=coastal+zone&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dcoastal%2Bzone','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20000120582&hterms=coastal+zone&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dcoastal%2Bzone"><span>Global Distribution of Aerosols Over the <span class="hlt">Open</span> <span class="hlt">Ocean</span> as Derived from the Coastal Zone Color Scanner</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Stegmann, P. M.; Tindale, N. W.</p> <p>1999-01-01</p> <p>Climatological maps of monthly mean aerosol radiance levels derived from the coastal zone color scanner (CZCS) were constructed for the world's <span class="hlt">ocean</span> basins. This is the first study to use the 7.5.-year CZCS data set to examine the distribution and seasonality of aerosols over the <span class="hlt">open</span> <span class="hlt">ocean</span> on a global scale. Examination of our satellite images found the most prominent large-scale patch of elevated aerosol radiances in each month off the coast of northwest Africa. The well-known, large-scale plumes of elevated aerosol levels in the Arabian Sea, the northwest Pacific, and off the east coast of North America were also successfully captured. Radiance data were extracted from 13 major <span class="hlt">open-ocean</span> zones, ranging from the subpolar to equatorial regions. Results from these extractions revealed the aerosol load in both subpolar and subtropical zones to be higher in the Northern Hemisphere than in the Southern Hemisphere. Aerosol radiances in the subtropics of both hemispheres were about 2 times higher in summer than in winter. In subpolar regions, aerosol radiances in late spring/early summer were almost 3 times that observed in winter. In general, the aerosol signal was higher during the warmer months and lower during the cooler months, irrespective of location. A comparison between our mean monthly aerosol radiance maps with mean monthly chlorophyll maps (also from CZCS) showed similar seasonality between aerosol and chlorophyll levels in the subpolar zones of both hemispheres, i.e., high levels in summer, low levels in winter. In the subtropics of both hemispheres, however, chlorophyll levels were higher in winter months which coincided with a depressed aerosol signal. Our results indicate that the near-IR channel on <span class="hlt">ocean</span> color sensors can be used to successfully capture well-known, large-scale aerosol plumes on a global scale and that future <span class="hlt">ocean</span> color sensors may provide a platform for long-term synoptic studies of combined aerosol-phytoplankton productivity</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001AGUFM.U12B..03O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001AGUFM.U12B..03O"><span>Sources of <span class="hlt">Water</span> for <span class="hlt">Oceans</span> on Planets</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Owen, T. C.</p> <p>2001-12-01</p> <p>Studies of D/H in the H2O carried by three Oort cloud comets have shown that such comets could not have contributed all of the <span class="hlt">water</span> in the Earth's <span class="hlt">oceans</span>. The extent of the cometary contribution depends on the value of D/H in <span class="hlt">water</span> brought directly to the planet as hydrous minerals or adsorbed solar nebula H2O. That some cometary <span class="hlt">water</span> was in fact delivered to the inner planets is strongly suggested by the value of D/H in Shergottite minerals when viewed in the context of other isotope geochemistry on Mars (Owen and Bar-Nun, FARADAY DISCUSSIONS 109, 453-462 (1998)). This scenario is also consistent with noble gas and siderophile element abundances on Earth. The identification of comet-produced <span class="hlt">water</span> vapor around the aging carbon star IRC +10216 (Melnick et al., NATURE 412, 160-163 (2001)) provides concrete support for the widely held assumption that a cometary reservoir for the irrigation of inner planets should be a common feature of planetary systems throughout the galaxy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMOS33B1773T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMOS33B1773T"><span>Developing a low-cost <span class="hlt">open</span>-source CTD for research and outreach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Thaler, A. D.; Sturdivant, K.</p> <p>2013-12-01</p> <p>Developing a low-cost <span class="hlt">open</span>-source CTD for research and outreach Andrew David Thaler and Kersey Sturdivant Conductivity, temperature, and depth (CTD). With these three measurements, marine scientists can unlock <span class="hlt">ocean</span> patterns hidden beneath the waves. The <span class="hlt">ocean</span> is not uniform, it its filled with swirling eddies, temperature boundaries, layers of high and low salinity, changing densities, and many other physical characteristics. To reveal these patterns, oceanographers use a tool called the CTD. A CTD is found on almost every major research vessel. Rare is the scientific expedition-whether it be coastal work in shallow estuaries or journeys to the deepest <span class="hlt">ocean</span> trenches-that doesn't begin with the humble CTD cast. The CTD is not cheap. Commercial CTD's start at more the 5,000 and can climb as high as 25,000 or more. We believe that the prohibitive cost of a CTD is an unacceptable barrier to <span class="hlt">open</span> science. The price tag excludes individuals and groups who lack research grants or significant private funds from conducting oceanographic research. We want to make this tool-the workhorse of oceanographic research-available to anyone with an interest in the <span class="hlt">oceans</span>. The <span class="hlt">Open</span>CTD is a low-cost, <span class="hlt">open</span>-source CTD suitable for both educators and scientists. The platform is built using readily available parts and is powered by an Arduino-based microcontroller. Our goal is to create a device that is accurate enough to be used for scientific research and can be constructed for less than $200. Source codes, circuit diagrams, and building plans will be freely available. The final instrument will be effective to 200 meters depth. Why 200 meters? For many coastal regions, 200 meters of <span class="hlt">water</span> depth covers the majority of the <span class="hlt">ocean</span> that is accessible by small boat. The <span class="hlt">Open</span>CTD is targeted to people working in this niche, where entire research projects can be conducted for less than the cost of a commercial CTD. However, the <span class="hlt">Open</span> CTD is scalable, and anyone with the inclination can adapt our</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27723743','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27723743"><span>Upper-mantle <span class="hlt">water</span> stratification inferred from observations of the 2012 Indian <span class="hlt">Ocean</span> earthquake.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Masuti, Sagar; Barbot, Sylvain D; Karato, Shun-Ichiro; Feng, Lujia; Banerjee, Paramesh</p> <p>2016-10-20</p> <p><span class="hlt">Water</span>, the most abundant volatile in Earth's interior, preserves the young surface of our planet by catalysing mantle convection, lubricating plate tectonics and feeding arc volcanism. Since planetary accretion, <span class="hlt">water</span> has been exchanged between the hydrosphere and the geosphere, but its depth distribution in the mantle remains elusive. <span class="hlt">Water</span> drastically reduces the strength of olivine and this effect can be exploited to estimate the <span class="hlt">water</span> content of olivine from the mechanical response of the asthenosphere to stress perturbations such as the ones following large earthquakes. Here, we exploit the sensitivity to <span class="hlt">water</span> of the strength of olivine, the weakest and most abundant mineral in the upper mantle, and observations of the exceptionally large (moment magnitude 8.6) 2012 Indian <span class="hlt">Ocean</span> earthquake to constrain the stratification of <span class="hlt">water</span> content in the upper mantle. Taking into account a wide range of temperature conditions and the transient creep of olivine, we explain the transient deformation in the aftermath of the earthquake that was recorded by continuous geodetic stations along Sumatra as the result of <span class="hlt">water</span>- and stress-activated creep of olivine. This implies a minimum <span class="hlt">water</span> content of about 0.01 per cent by weight-or 1,600 H atoms per million Si atoms-in the asthenosphere (the part of the upper mantle below the lithosphere). The earthquake ruptured conjugate faults down to great depths, compatible with dry olivine in the <span class="hlt">oceanic</span> lithosphere. We attribute the steep rheological contrast to dehydration across the lithosphere-asthenosphere boundary, presumably by buoyant melt migration to form the <span class="hlt">oceanic</span> crust.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013BGeo...10.7293S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013BGeo...10.7293S"><span>On the role of mesoscale eddies for the biological productivity and biogeochemistry in the eastern tropical Pacific <span class="hlt">Ocean</span> off Peru</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stramma, L.; Bange, H. W.; Czeschel, R.; Lorenzo, A.; Frank, M.</p> <p>2013-11-01</p> <p>Mesoscale eddies seem to play an important role for both the hydrography and biogeochemistry of the eastern tropical Pacific <span class="hlt">Ocean</span> (ETSP) off Peru. However, detailed surveys of these eddies are not available, which has so far hampered an in depth understanding of their implications for nutrient distribution and biological productivity. In this study, three eddies along a section at 16°45´ S have been surveyed intensively during R/V Meteor cruise M90 in November 2012. A coastal mode <span class="hlt">water</span> eddy, an <span class="hlt">open</span> <span class="hlt">ocean</span> mode <span class="hlt">water</span> eddy and an <span class="hlt">open</span> <span class="hlt">ocean</span> cyclonic eddy have been identified and sampled in order to determine both their hydrographic properties and their influence on the biogeochemical setting of the ETSP. In the thermocline the temperature of the coastal anticyclonic eddy was up to 2 °C warmer, 0.2 more saline and the swirl velocity was up to 35 cm s-1. The observed temperature and salinity anomalies, as well as swirl velocities of both types of eddies were about twice as large as had been described for the mean eddies in the ETSP. The observed heat and salt anomalies (AHA, ASA) of the anticyclonic eddy near the shelf-break of 17.7 × 1018 J and 36.6 × 1010 kg are more than twice as large as the mean AHA and ASA for the ETSP. We found that the eddies contributed to the productivity by maintaining pronounced subsurface maxima of chlorophyll of up to 6 μg L-1. Based on a comparison of the coastal (young) mode <span class="hlt">water</span> eddy and the <span class="hlt">open</span> <span class="hlt">ocean</span> (old) mode <span class="hlt">water</span> eddy we suggest that the ageing of eddies when they detach from the shelf-break and move westward to the <span class="hlt">open</span> <span class="hlt">ocean</span> influences the eddies' properties: chlorophyll maxima are reduced to about half (2.5-3 μg L-1) and nutrients are subducted. However, different settings at the time of formation may also contribute to the observed differences between the young and old mode <span class="hlt">water</span> eddies. The coastal mode <span class="hlt">water</span> eddy was found to be a site of nitrogen (N) loss in the OMZ with a maximum ΔNO3- anomaly (i.e. N loss) of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70192848','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70192848"><span>The <span class="hlt">Open</span> <span class="hlt">Water</span> Data Initiative: <span class="hlt">Water</span> information for a thirsty nation</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Rea, Alan; Clark, Edward; Adams, Angela; Samuels, William B.</p> <p>2015-01-01</p> <p>Initial efforts of the <span class="hlt">Open</span> <span class="hlt">Water</span> Data Initiative have focused on three use cases covering flooding, drought, and contaminant spill response, with a goal of identifying critical <span class="hlt">water</span> data resources and making them more accessible. Significant progress has been made in the past year, although much remains to be done.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018NatGe..11...65M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018NatGe..11...65M"><span><span class="hlt">Water</span>-rich sublithospheric melt channel in the equatorial Atlantic <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mehouachi, Fares; Singh, Satish C.</p> <p>2018-01-01</p> <p>The lithosphere-asthenosphere boundary is the most extensive boundary on Earth, separating the mobile plate above from the convecting mantle below, but its nature remains a matter of debate. Using an ultra-deep seismic reflection technique, here we show a systematic seismic image of two deep reflectors that we interpret as the upper and lower limits of the lithosphere-asthenosphere boundary beneath a 40-70-million-year-old <span class="hlt">oceanic</span> lithosphere in the Atlantic <span class="hlt">Ocean</span>. These two reflections correspond to 1,260 °C and 1,355 °C isotherms and bound a low-velocity channel, suggesting that the lithosphere-asthenosphere boundary is thermally controlled. We observe a clear age dependency of this sublithospheric channel: its depth increases with age from 72 km where it is 40-Myr-old to 88 km where it is 70-Myr-old, whereas its thickness decreases with age from 18 km to 12 km. We suggest that partial melting, facilitated by <span class="hlt">water</span>, is the main mechanism responsible for the low-velocity channel. The required <span class="hlt">water</span> concentration for melting increases with age; nevertheless, its corresponding total mass remains relatively constant, suggesting that most of the volatiles in the <span class="hlt">oceanic</span> sublithospheric channel originate from a horizontal flux near the ridge axis.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19840019234','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19840019234"><span>Modeling of SAR signatures of shallow <span class="hlt">water</span> <span class="hlt">ocean</span> topography</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Shuchman, R. A.; Kozma, A.; Kasischke, E. S.; Lyzenga, D. R.</p> <p>1984-01-01</p> <p>A hydrodynamic/electromagnetic model was developed to explain and quantify the relationship between the SEASAT synthetic aperture radar (SAR) observed signatures and the bottom topography of the <span class="hlt">ocean</span> in the English Channel region of the North Sea. The model uses environmental data and radar system parameters as inputs and predicts SAR-observed backscatter changes over topographic changes in the <span class="hlt">ocean</span> floor. The model results compare favorably with the actual SEASAT SAR observed backscatter values. The developed model is valid for only relatively shallow <span class="hlt">water</span> areas (i.e., less than 50 meters in depth) and suggests that for bottom features to be visible on SAR imagery, a moderate to high velocity current and a moderate wind must be present.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20030067029&hterms=extinction&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dextinction','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20030067029&hterms=extinction&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dextinction"><span>Strangelove <span class="hlt">Ocean</span> and Deposition of Unusual Shallow-<span class="hlt">Water</span> Carbonates After the End-Permian Mass Extinction</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rampino, Michael R.; Caldeira, Ken</p> <p>2003-01-01</p> <p>The severe mass extinction of marine and terrestrial organisms at the end of the Permian Period (approx. 251 Ma) was accompanied by a rapid negative excursion of approx. 3 to 4 per mil in the carbon-isotope ratio of the global surface <span class="hlt">oceans</span> and atmosphere that persisted for some 500,000 into the Early Triassic. Simulations with an <span class="hlt">ocean</span>-atmosphere/carbon-cycle model suggest that the isotope excursion can be explained by collapse of <span class="hlt">ocean</span> primary productivity (a Strangelove <span class="hlt">Ocean</span>) and changes in the delivery and cycling of carbon in the <span class="hlt">ocean</span> and on land. Model results also suggest that perturbations of the global carbon cycle resulting from the extinctions led to short-term fluctuations in atmospheric pCO2 and <span class="hlt">ocean</span> carbonate deposition, and to a long-term (>1 Ma) decrease in sedimentary burial of organic carbon in the Triassic. Deposition of calcium carbonate is a major sink of river-derived <span class="hlt">ocean</span> alkalinity and for CO2 from the <span class="hlt">ocean</span>/atmosphere system. The end of the Permian was marked by extinction of most calcium carbonate secreting organisms. Therefore, the reduction of carbonate accumulation made the <span class="hlt">oceans</span> vulnerable to a build-up of alkalinity and related fluctuations in atmospheric CO2. Our model results suggest that an increase in <span class="hlt">ocean</span> carbonate-ion concentration should cause increased carbonate accumulation rates in shallow-<span class="hlt">water</span> settings. After the end-Permian extinctions, early Triassic shallow-<span class="hlt">water</span> sediments show an abundance of abiogenic and microbial carbonates that removed CaCO3 from the <span class="hlt">ocean</span> and may have prevented a full '<span class="hlt">ocean</span>-alkalinity crisis' from developing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSME34D0828B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSME34D0828B"><span>Modeling anoxic aggregates in the <span class="hlt">ocean</span> - implications for nitrogen, sulfur and trace metal cycling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bianchi, D.; Weber, T. S.; Deutsch, C.</p> <p>2016-02-01</p> <p>Anoxic conditions are uncommon in the <span class="hlt">open</span> <span class="hlt">ocean</span>, and mostly confined to the cores of oxygen minimum zones (OMZs). When oxygen runs out, a suite of alternative electron acceptors are used, leading to denitrification and, rarely in <span class="hlt">open</span> <span class="hlt">waters</span>, sulfate reduction. Anoxic conditions have been shown to develop inside millimeter-scale organic particles and aggregates, establishing microscale gradients that could sustain diverse microbial communities along a sequence of redox niches. We develop a model of the biogeochemistry of anoxic aggregates that includes aerobic and anaerobic reactions in a diffusion-limited environment, and present analytical and numerical solutions for the conditions that allow denitrification and sulfate reduction inside aggregates. The model is applied to realistic size spectra of particles sinking through the <span class="hlt">water</span> column, and used to estimate the potential for particle-bound denitrification and sulfate reduction in the global <span class="hlt">ocean</span>. We show that anoxia inside aggregates may be common throughout low oxygen <span class="hlt">waters</span>, extending the niche of denitrifying metabolisms beyond fully anoxic zones. In the OMZ cores, aggregates can sustain pockets of sulfate reduction in otherwise non-sulfidic <span class="hlt">waters</span>, depending on ambient nitrate concentrations, particle respiration rates, and other factors. We further discuss the implications for nitrogen, sulfur and trace metal cycling in the <span class="hlt">ocean</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.5429P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.5429P"><span>FixO3 : Early progress towards <span class="hlt">Open</span> <span class="hlt">Ocean</span> observatory Data Management Harmonisation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pagnani, Maureen; Huber, Robert; Lampitt, Richard</p> <p>2014-05-01</p> <p>Since 2002 there has been a sustained effort, supported as European framework projects, to harmonise both the technology and the data management of <span class="hlt">Open</span> <span class="hlt">Ocean</span> fixed observatories run by European nations. FixO3 started in September 2013, and for 4 years will coordinate the convergence of data management best practice across a constellation of moorings in the Atlantic, in both hemispheres, and in the Mediterranean. To ensure the continued existence of these unique sources of oceanographic data as sustained observatories it is vital to improve access to the data collected, both in terms of methods of presentation, real-time availability, long-term archiving and quality assurance. The data management component of FixO3 will improve access to marine observatory data by harmonizing data management standards and workflows covering the complete life cycle of data from real time data acquisition to long-term archiving. Legal and data policy aspects will be examined to identify transnational barriers to <span class="hlt">open</span>-access to marine observatory data. A harmonised FixO3 data policy is being synthesised from the partner's existing policies, which will overcome the identified barriers, and provide a formal basis for data exchange between FixO3 infrastructures. Presently, the interpretation and implementation of accepted standards has considerable incompatibilities within the observatory community, and these different approaches will be unified into the FixO3 approach. Further, FixO3 aims to harmonise data management and standardisation efforts with other European and international marine data and observatory infrastructures. The FixO3 synthesis will build on the standards established in other European infrastructures such as EDMONET, SEADATANET, PANGAEA, EuroSITES (European contribution to JCOMMP <span class="hlt">Ocean</span>SITES programme), and My<span class="hlt">Ocean</span> (the Marine Core Service for GMES) infrastructures as well as relevant international infrastructures and data centres such as the ICOS <span class="hlt">Ocean</span> Thematic Centre</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/658984-new-nitrogen-fixing-microorganisms-detected-oligotrophic-oceans-amplification-nitrogenase-nifh-genes','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/658984-new-nitrogen-fixing-microorganisms-detected-oligotrophic-oceans-amplification-nitrogenase-nifh-genes"><span>New nitrogen-fixing microorganisms detected in oligotrophic <span class="hlt">oceans</span> by amplification of nitrogenase (nifH) genes</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>Zehr, J.P.; Mellon, M.T.; Zani, S.</p> <p>1998-09-01</p> <p>Oligotrophic <span class="hlt">oceanic</span> <span class="hlt">waters</span> of the central <span class="hlt">ocean</span> gyres typically have extremely low dissolved fixed inorganic nitrogen concentrations, but few nitrogen-fixing microorganisms from the <span class="hlt">oceanic</span> environment have been cultivated. Nitrogenase gene (nifH) sequences amplified directly from <span class="hlt">oceanic</span> <span class="hlt">waters</span> showed that the <span class="hlt">open</span> <span class="hlt">ocean</span> contains more diverse diazotrophic microbial populations and more diverse habitats for nitrogen fixers than previously observed by classical microbiological techniques. Nitrogenase genes derived from unicellular and filamentous cyanobacteria, as well as from the {alpha} and {gamma} subdivisions of the class Proteobacteria, were found in both the Atlantic and Pacific <span class="hlt">oceans</span>. nifH sequences that cluster phylogenetically with sequences frommore » sulfate reducers or clostridia were found associated with planktonic crustaceans. Nitrogenase sequence types obtained from invertebrates represented phylotypes distinct from the phylotypes detected in the picoplankton size fraction. The results indicate that there are in the <span class="hlt">oceanic</span> environment several distinct potentially nitrogen-fixing microbial assemblages that include representatives of diverse phylotypes.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2010-06-21/pdf/2010-14851.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2010-06-21/pdf/2010-14851.pdf"><span>75 FR 34929 - Safety Zones: Neptune Deep <span class="hlt">Water</span> Port, Atlantic <span class="hlt">Ocean</span>, Boston, MA</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2010-06-21</p> <p>...-AA00 Safety Zones: Neptune Deep <span class="hlt">Water</span> Port, Atlantic <span class="hlt">Ocean</span>, Boston, MA AGENCY: Coast Guard, DHS. ACTION..., Boston, MA; Final Rule (USCG-2009-0589), to protect vessels from the hazard posed by the presence of the... read as follows: Sec. 165.T01-0542 Safety Zones: Neptune Deepwater Port, Atlantic <span class="hlt">Ocean</span>, Boston, MA. (a...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016DSRI..118...37M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016DSRI..118...37M"><span>Atmospheric aerosol deposition influences marine microbial communities in oligotrophic surface <span class="hlt">waters</span> of the western Pacific <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Maki, Teruya; Ishikawa, Akira; Mastunaga, Tomoki; Pointing, Stephen B.; Saito, Yuuki; Kasai, Tomoaki; Watanabe, Koichi; Aoki, Kazuma; Horiuchi, Amane; Lee, Kevin C.; Hasegawa, Hiroshi; Iwasaka, Yasunobu</p> <p>2016-12-01</p> <p>Atmospheric aerosols contain particulates that are deposited to <span class="hlt">oceanic</span> surface <span class="hlt">waters</span>. These can represent a major source of nutrients, trace metals, and organic compounds for the marine environment. The Japan Sea and the western Pacific <span class="hlt">Ocean</span> are particularly affected by aerosols due to the transport of desert dust and industrially derived particulate matter with aerodynamic diameter less than 2.5 μm (PM2.5) from continental Asia. We hypothesized that supplementing seawater with aerosol particulates would lead to measurable changes in surface <span class="hlt">water</span> nutrient composition as well as shifts in the marine microbial community. Shipboard experiments in the Pacific <span class="hlt">Ocean</span> involved the recovery of oligotrophic <span class="hlt">oceanic</span> surface <span class="hlt">water</span> and subsequent supplementation with aerosol particulates obtained from the nearby coastal mountains, to simulate marine particulate input in this region. Initial increases in nitrates due to the addition of aerosol particulates were followed by a decrease correlated with the increase in phytoplankton biomass, which was composed largely of Bacillariophyta (diatoms), including Pseudo-nitzschia and Chaetoceros species. This shift was accompanied by changes in the bacterial community, with apparent increases in the relative abundance of heterotrophic Rhodobacteraceae and Colwelliaceae in aerosol particulate treated seawater. Our findings provide empirical evidence revealing the impact of aerosol particulates on <span class="hlt">oceanic</span> surface <span class="hlt">water</span> microbiology by alleviating nitrogen limitation in the organisms.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002DSRI...49.2075Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002DSRI...49.2075Y"><span>A global <span class="hlt">ocean</span> climatological atlas of the Turner angle: implications for double-diffusion and <span class="hlt">water</span>-mass structure</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>You, Yuzhu</p> <p>2002-11-01</p> <p>The 1994 Levitus climatological atlas is used to calculate the Turner angle (named after J. Stewart Turner) to examine which <span class="hlt">oceanic</span> <span class="hlt">water</span> masses are favorable for double-diffusion in the form of diffusive convection or salt-fingering and which are doubly stable. This atlas complements the Levitus climatology. It reveals the major double-diffusive signals associated with large-scale <span class="hlt">water</span>-mass structure. In total, about 44% of the <span class="hlt">oceans</span> display double-diffusion, of which 30% is salt-fingering and 14% is diffusive double-diffusion. Results show that various central and deep <span class="hlt">waters</span> are favorable for salt-fingering. The former is due to positive evaporation minus precipitation, and the latter is due to thermohaline circulation, i.e. the southward spreading of relatively warm, salty North Atlantic Deep <span class="hlt">Water</span> (NADW) overlying cold, fresh Antarctic Bottom <span class="hlt">Water</span>. In the northern Indian <span class="hlt">Ocean</span> and eastern North Atlantic, favorable conditions for salt-fingering are found throughout the <span class="hlt">water</span> column. The Red Sea (including the Persian Gulf) and Mediterranean Sea are the sources of warm, salty <span class="hlt">water</span> for the <span class="hlt">ocean</span>. As consequence, temperature and salinity in these outflow regions both decrease from the sea surface to the bottom. On the other hand, <span class="hlt">ocean</span> currents are in general sluggish in these regions. In the polar and subpolar regions of Arctic and Antarctic, Okhotsk Sea, Gulf of Alaska, the subpolar gyre of the North Pacific, the Labrador Sea, and the Norwegian Sea, the upper layer <span class="hlt">water</span> is favorable for diffusive convection because of high latitude surface cooling and ice melting. Weak and shallow diffusive convection is also found throughout tropical regions and the Bay of Bengal. The former is due to excessive precipitation over evaporation and rain cooling, and the latter is due to both precipitation and river runoff. Diffusive convection in the <span class="hlt">ocean</span>'s interior is unique to the South Atlantic between Antarctic Intermediate <span class="hlt">Water</span> and upper NADW (uNADW). It is the</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://hdl.handle.net/2060/20050166898','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20050166898"><span>Penetration of UV Radiation in the Earth's <span class="hlt">Oceans</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mitchell, B. Greg; Lubin, Dan</p> <p>2005-01-01</p> <p>This project was a collaboration between SIO/UCSD and NASA/GSFC to develop a global estimation of the penetration of UV light into <span class="hlt">open</span> <span class="hlt">ocean</span> <span class="hlt">waters</span>, and into coastal <span class="hlt">waters</span>. We determined the <span class="hlt">ocean</span> UV reflectance spectra seen by satellites above the atmosphere by combining existing sophisticated radiative transfer models with in situ UV Visible data sets to improve coupled radiance estimates both underwater and within the atmosphere. Results included improved estimates of surface spectral irradiance, 0.3-1.0 micron, and estimates of photosynthetic inhibition, DNA mutation, and CO production. Data sets developed under this proposal have been made publicly available via submission to the SeaWiFS Bio-Optical Archive and Storage System. Numerous peer-reviewed publications and conference proceedings and abstracts resulted from the work supported by this research award.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=%22Marshall+Islands%22&pg=3&id=EJ118119','ERIC'); return false;" href="https://eric.ed.gov/?q=%22Marshall+Islands%22&pg=3&id=EJ118119"><span><span class="hlt">Water</span> Quality of a Micronesian Atoll</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Mabbett, Arthur N.</p> <p>1975-01-01</p> <p>In 1972, a <span class="hlt">water</span> quality survey of the eastern end of Majuro Atoll, Marshall Islands was conducted to determine the <span class="hlt">water</span> quality of selected lagoon and <span class="hlt">open</span> <span class="hlt">ocean</span> sites and provide guidance for the construction of a sewerage system. This study revealed that lagoon <span class="hlt">waters</span> were moderately to severely contaminated. (BT)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5064243-physical-oceanography-tracer-chemistry-southern-ocean','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5064243-physical-oceanography-tracer-chemistry-southern-ocean"><span>Physical oceanography and tracer chemistry of the southern <span class="hlt">ocean</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>Not Available</p> <p></p> <p>This report considers technical and scientific developments and research questions in studies of the Southern <span class="hlt">Ocean</span> since its predecessor, /<span class="hlt">open</span> quotes/Southern <span class="hlt">Ocean</span> Dynamics--A Strategy for Scientific Exploration 1973-1983/close quotes/ was published. The summary lists key research questions in Southern <span class="hlt">Ocean</span> oceanography. Chapter 1 describes how Southern <span class="hlt">Ocean</span> research has evolved to provide the basis for timely research toward more directed objectives. Chapter 2 recommends four research programs, encompassing many of the specific recommendations that follow. Appendix A provides the scientific background and Reference/Bibliography list for this report for: on air-sea-ice interaction; the Antarctic Circumpolar Current; <span class="hlt">water</span> mass conversion; chemical tracermore » oceanography; and numerical modeling of the Southern <span class="hlt">Ocean</span>. Appendix B describes the satellite-based observation systems expected to be active during the next decade. Appendix C is a list of relevant reports published during 1981-1987. 146 refs.« less</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 air-sea gas transfer in the sea ice zone? A synthesis of radon deficit profiles in the upper <span class="hlt">water</span> column of the Arctic <span class="hlt">Ocean</span></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-<span class="hlt">ocean</span> boundary layer of the Beaufort Sea. Including these 34, there are presently 58 published radon-deficit estimates of air-sea gas transfer velocity (k) in the Arctic <span class="hlt">Ocean</span>; 52 of these estimates were derived from <span class="hlt">water</span> covered by 10% sea 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 <span class="hlt">ocean</span> surface is ice covered. Whereas the six profiles taken from the <span class="hlt">open</span> <span class="hlt">ocean</span> indicate a statistically good fit to wind speed parameterizations, the same parameterizations could not reproduce k from the sea ice zone. We conclude that techniques for estimating k in the <span class="hlt">open</span> <span class="hlt">ocean</span> cannot be similarly applied to determine k in the presence of sea ice. The magnitude of k through gaps in the ice may reach high values as ice cover increases, possibly as a result of focused turbulence dissipation at <span class="hlt">openings</span> 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 air-sea gas exchange with no impact from air-ice gas exchange.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFMOS23A1632C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFMOS23A1632C"><span>Monitoring of hourly variations in coastal <span class="hlt">water</span> turbidity using the geostationary <span class="hlt">ocean</span> color imager (GOCI)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Choi, J.; Ryu, J.</p> <p>2011-12-01</p> <p>Temporal variations of suspended sediment concentration (SSC) in coastal <span class="hlt">water</span> are the key to understanding the pattern of sediment movement within coastal area, in particular, such as in the west coast of the Korean Peninsula which is influenced by semi-diurnal tides. Remote sensing techniques can effectively monitor the distribution and dynamic changes in seawater properties across wide areas. Thus, SSC on the sea surface has been investigated using various types of satellite-based sensors. An advantage of Geostationary <span class="hlt">Ocean</span> Color Imager (GOCI), the world's first geostationary <span class="hlt">ocean</span> color observation satellite, over other <span class="hlt">ocean</span> color satellite images is that it can obtain data every hour during the day and makes it possible to monitor the <span class="hlt">ocean</span> in real time. In this study, hourly variations in turbidity on the coastal <span class="hlt">waters</span> were estimated quantitatively using GOCI. Thirty three <span class="hlt">water</span> samples were obtained on the coastal <span class="hlt">water</span> surface in southern Gyeonggi Bay, located on the west coast of Korea. <span class="hlt">Water</span> samples were filtered using 25-mm glass fiber filters (GF/F) for the estimation of SSC. The radiometric characteristics of the surface <span class="hlt">water</span>, such as the total <span class="hlt">water</span>-leaving radiance (LwT, W/m2/nm/sr), the sky radiance (Lsky, W/m2/nm/sr) and the downwelling irradiance, were also measured at each sampling location. In situ optical properties of the surface <span class="hlt">water</span> were converted into remote sensing reflectance (Rrs) and then were used to develop an algorithm to generate SSC images in the study area. GOCI images acquired on the same day as the samples acquisition were used to generate the map of turbidity and to estimate the difference in SSC displayed in each image. The estimation of the time-series variation in SSC in a coastal, shallow-<span class="hlt">water</span> area affected by tides was successfully achieved using GOCI data that had been acquired at hourly intervals during the daytime.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1014287','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1014287"><span>Development of Automated Whistle and Click Classifiers for Odontocete Species in the Western Atlantic <span class="hlt">Ocean</span> and the <span class="hlt">Waters</span> Surrounding the Hawaiian Islands</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2015-09-30</p> <p>for Odontocete Species in the Western Atlantic <span class="hlt">Ocean</span> and the <span class="hlt">Waters</span> Surrounding the Hawaiian Islands Julie N. Oswald & Tina M. Yack Bio-Waves... Atlantic <span class="hlt">Ocean</span>, the temperate Pacific <span class="hlt">Ocean</span> and the <span class="hlt">waters</span> surrounding the Hawaiian Islands. These classifiers will also incorporate ancillary...and echolocation click classifiers for odontocete species in the northwest Atlantic <span class="hlt">Ocean</span>, the <span class="hlt">waters</span> surrounding the Hawaiian Islands and the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20040129716','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20040129716"><span>Storm Induced Injection of the Mississippi River Plume Into the <span class="hlt">Open</span> Gulf of Mexico</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Yuan, Jinchun; Miller, Richard L.; Powell, Rodney T.; Dagg, Michael J.</p> <p>2004-01-01</p> <p>The direct impact of the Mississippi River on the <span class="hlt">open</span> Gulf of Mexico is typically considered to be limited due to the predominantly along-shore current pattern. Using satellite imagery, we analyzed chl a distributions in the northern Gulf of Mexico before and after the passage of two storms: Hurricane Lili and Tropical Storm Barry. Our analyses indicate that storm-induced eddies can rapidly inject large volumes of nutrient-rich Mississippi River <span class="hlt">water</span> to the <span class="hlt">open</span> gulf, and lead to phytoplankton blooms. Although these events last only a few weeks, they transport significant amounts of fluvial substances to the <span class="hlt">ocean</span>. These river-<span class="hlt">ocean</span> interactions are especially significant in tropical and subtropical regions because receiving <span class="hlt">waters</span> are typically permanently stratified and oligotrophic.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20100040639','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20100040639"><span><span class="hlt">Water</span> in the <span class="hlt">Oceanic</span> Lithosphere: Salt Lake Crater Xenoliths, Oahu, Hawaii</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Peslier, Anne H.; Bizimis, Michael</p> <p>2010-01-01</p> <p><span class="hlt">Water</span> can be present in nominally anhydrous minerals of peridotites in the form of hydrogen bonded to structural oxygen. Such <span class="hlt">water</span> in the <span class="hlt">oceanic</span> upper mantle could have a significant effect on its physical and chemical properties. However, the <span class="hlt">water</span> content of the MORB source has been inferred indirectly from the compositions of basalts. Direct determinations on abyssal peridotites are scarce because they have been heavily hydrothermally altered. Here we present the first <span class="hlt">water</span> analyses of minerals from spinel peridotite xenoliths of Salt Lake Crater, Oahu, Hawaii, which are exceptionally fresh. These peridotites are thought to represent fragments of the Pacific <span class="hlt">oceanic</span> lithosphere that was refertilized by alkalic Hawaiian melts. A few have unradiogenic Os and radiogenic Hf isotopes and may be fragments of an ancient (2 Ga) depleted and recycled lithosphere. <span class="hlt">Water</span> contents in olivine (Ol), orthopyroxene (Opx), and clinopyroxene (Cpx) were determined by FTIR spectrometry. Preliminary H_{2}O contents show ranges of 8-10 ppm for Ol, 151-277 ppm for Opx, and 337-603 ppm for Cpx. Reconstructed bulk rock H_{2}O contents range from 88-131 ppm overlapping estimates for the MORB source. <span class="hlt">Water</span> contents between Ol minerals of the same xenolith are heterogeneous and individual OH infrared bands vary within a mineral with lower 3230 cm^{-1} and higher 3650-3400 cm^{-1} band heights from core to edge. This observation suggests disturbance of the hydrogen in Ol likely occurring during xenolith entrainment to the surface. Pyroxene <span class="hlt">water</span> contents are higher than most <span class="hlt">water</span> contents in pyroxenes from continental peridotite xenoliths and higher than those of abyssal peridotites. Cpx <span class="hlt">water</span> contents decrease with increasing degree of depletion (e.g. increasing Fo in Ol and Cr# in spinel) consistent with an incompatible behavior of <span class="hlt">water</span>. However Cpx <span class="hlt">water</span> contents also show a positive correlation with LREE/HREE ratios and LREE concentrations consistent with refertilization. Opx <span class="hlt">water</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.V53C2263P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.V53C2263P"><span><span class="hlt">Water</span> in the <span class="hlt">oceanic</span> lithosphere: Salt Lake Crater xenoliths, Oahu, Hawaii</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Peslier, A. H.; Bizimis, M.</p> <p>2010-12-01</p> <p><span class="hlt">Water</span> can be present in nominally anhydrous minerals of peridotites in the form of hydrogen bonded to structural oxygen. Such <span class="hlt">water</span> in the <span class="hlt">oceanic</span> upper mantle could have a significant effect on its physical and chemical properties. However, the <span class="hlt">water</span> content of the MORB source has been inferred indirectly from the compositions of basalts. Direct determinations on abyssal peridotites are scarce because they have been heavily hydrothermally altered. Here we present the first <span class="hlt">water</span> analyses of minerals from spinel peridotite xenoliths of Salt Lake Crater, Oahu, Hawaii, which are exceptionally fresh. These peridotites are thought to represent fragments of the Pacific <span class="hlt">oceanic</span> lithosphere that was refertilized by alkalic Hawaiian melts. A few have unradiogenic Os and radiogenic Hf isotopes and may be fragments of an ancient ( 2 Ga) depleted and recycled lithosphere. <span class="hlt">Water</span> contents in olivine (Ol), orthopyroxene (Opx), and clinopyroxene (Cpx) were determined by FTIR spectrometry. Preliminary H_{2}O contents show ranges of 8-10 ppm for Ol, 151-277 ppm for Opx, and 337-603 ppm for Cpx. Reconstructed bulk rock H_{2}O contents range from 88-131 ppm overlapping estimates for the MORB source. <span class="hlt">Water</span> contents between Ol minerals of the same xenolith are heterogeneous and individual OH infrared bands vary within a mineral with lower 3230 cm^{-1} and higher 3650-3400 cm^{-1} band heights from core to edge. This observation suggests disturbance of the hydrogen in Ol likely occurring during xenolith entrainment to the surface. Pyroxene <span class="hlt">water</span> contents are higher than most <span class="hlt">water</span> contents in pyroxenes from continental peridotite xenoliths and higher than those of abyssal peridotites. Cpx <span class="hlt">water</span> contents decrease with increasing degree of depletion (e.g. increasing Fo in Ol and Cr# in spinel) consistent with an incompatible behavior of <span class="hlt">water</span>. However Cpx <span class="hlt">water</span> contents also show a positive correlation with LREE/HREE ratios and LREE concentrations consistent with refertilization. Opx</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.5927S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.5927S"><span>Characterization and impact of "dead-zone" eddies in the tropical Northeast Atlantic <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schuette, Florian; Karstensen, Johannes; Krahmann, Gerd; Hauss, Helena; Fiedler, Björn; Brandt, Peter; Visbeck, Martin; Körtzinger, Arne</p> <p>2016-04-01</p> <p>Localized <span class="hlt">open-ocean</span> low-oxygen dead-zones in the tropical Northeast Atlantic are recently discovered <span class="hlt">ocean</span> features that can develop in dynamically isolated <span class="hlt">water</span> masses within cyclonic eddies (CE) and anticyclonic modewater eddies (ACME). Analysis of a comprehensive oxygen dataset obtained from gliders, moorings, research vessels and Argo floats shows that eddies with low oxygen concentrations at 50-150 m depths can be found in surprisingly high numbers and in a large area (from about 5°N to 20°N, from the shelf at the eastern boundary to 30°W). Minimum oxygen concentrations of about 9 μmol/kg in CEs and close to anoxic concentrations (< 1 μmol/kg) in ACMEs were observed. In total, 495 profiles with oxygen concentrations below the minimum background concentration of 40 μmol/kg could be associated with 27 independent "dead-zone" eddies (10 CEs; 17 ACMEs). The low oxygen concentration right beneath the mixed layer has been attributed to the combination of high productivity in the surface <span class="hlt">waters</span> of the eddies and the isolation of the eddies' cores. Indeed eddies of both types feature a cold sea surface temperature anomaly and enhanced chlorophyll concentrations in their center. The oxygen minimum is located in the eddy core beneath the mixed layer at around 80 m depth. The mean oxygen anomaly between 50 to 150 m depth for CEs (ACMEs) is -49 (-81) μmol/kg. Eddies south of 12°N carry weak hydrographic anomalies in their cores and seem to be generated in the <span class="hlt">open</span> <span class="hlt">ocean</span> away from the boundary. North of 12°N, eddies of both types carry anomalously low salinity <span class="hlt">water</span> of South Atlantic Central <span class="hlt">Water</span> origin from the eastern boundary upwelling region into the <span class="hlt">open</span> <span class="hlt">ocean</span>. This points to an eddy generation near the eastern boundary. A conservative estimate yields that around 5 dead-zone eddies (4 CEs; 1 ACME) per year entering the area north of 12°N between the Cap Verde Islands and 19°W. The associated contribution to the oxygen budget of the shallow oxygen minimum</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014OcMod..82...28H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014OcMod..82...28H"><span>Eddy-resolving simulations of the Fimbul Ice Shelf cavity circulation: Basal melting and exchange with <span class="hlt">open</span> <span class="hlt">ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hattermann, T.; Smedsrud, L. H.; Nøst, O. A.; Lilly, J. M.; Galton-Fenzi, B. K.</p> <p>2014-10-01</p> <p>Melting at the base of floating ice shelves is a dominant term in the overall Antarctic mass budget. This study applies a high-resolution regional ice shelf/<span class="hlt">ocean</span> model, constrained by observations, to (i) quantify present basal mass loss at the Fimbul Ice Shelf (FIS); and (ii) investigate the <span class="hlt">oceanic</span> mechanisms that govern the heat supply to ice shelves in the Eastern Weddell Sea. The simulations confirm the low melt rates suggested by observations and show that melting is primarily determined by the depth of the coastal thermocline, regulating deep <span class="hlt">ocean</span> heat fluxes towards the ice. Furthermore, the uneven distribution of ice shelf area at different depths modulates the melting response to <span class="hlt">oceanic</span> forcing, causing the existence of two distinct states of melting at the FIS. In the simulated present-day state, only small amounts of Modified Warm Deep <span class="hlt">Water</span> enter the continental shelf, and <span class="hlt">ocean</span> temperatures beneath the ice are close to the surface freezing point. The basal mass loss in this so-called state of "shallow melting" is mainly controlled by the seasonal inflow of solar-heated surface <span class="hlt">water</span> affecting large areas of shallow ice in the upper part of the cavity. This is in contrast to a state of "deep melting", in which the thermocline rises above the shelf break depth, establishing a continuous inflow of Warm Deep <span class="hlt">Water</span> towards the deep ice. The transition between the two states is found to be determined by a complex response of the Antarctic Slope Front overturning circulation to varying climate forcings. A proper representation of these frontal dynamics in climate models will therefore be crucial when assessing the evolution of ice shelf basal melting along this sector of Antarctica.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=GL-2002-001464&hterms=OPEN+AIR&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DOPEN%2BAIR','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=GL-2002-001464&hterms=OPEN+AIR&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DOPEN%2BAIR"><span><span class="hlt">Open</span>-cell cloud formation over the Bahamas</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>2002-01-01</p> <p>What atmospheric scientists refer to as <span class="hlt">open</span> cell cloud formation is a regular occurrence on the back side of a low-pressure system or cyclone in the mid-latitudes. In the Northern Hemisphere, a low-pressure system will draw in surrounding air and spin it counterclockwise. That means that on the back side of the low-pressure center, cold air will be drawn in from the north, and on the front side, warm air will be drawn up from latitudes closer to the equator. This movement of an air mass is called advection, and when cold air advection occurs over warmer <span class="hlt">waters</span>, <span class="hlt">open</span> cell cloud formations often result. This MODIS image shows <span class="hlt">open</span> cell cloud formation over the Atlantic <span class="hlt">Ocean</span> off the southeast coast of the United States on February 19, 2002. This particular formation is the result of a low-pressure system sitting out in the North Atlantic <span class="hlt">Ocean</span> a few hundred miles east of Massachusetts. (The low can be seen as the comma-shaped figure in the GOES-8 Infrared image from February 19, 2002.) Cold air is being drawn down from the north on the western side of the low and the <span class="hlt">open</span> cell cumulus clouds begin to form as the cold air passes over the warmer Caribbean <span class="hlt">waters</span>. For another look at the scene, check out the MODIS Direct Broadcast Image from the University of Wisconsin. Image courtesy Jacques Descloitres, MODIS Land Rapid Response Team at NASA GSFC</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFMOS23D..08L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMOS23D..08L"><span>Bay-<span class="hlt">Ocean</span> Coupling and the Proximal Fate of <span class="hlt">Water</span>-Borne Material Exported from San Francisco Bay</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Largier, J. L.</p> <p>2012-12-01</p> <p>The coupling between San Francisco Bay and the <span class="hlt">ocean</span> is poorly known: how <span class="hlt">ocean</span> <span class="hlt">waters</span> intrude into bay and how bay <span class="hlt">waters</span> flow out into the <span class="hlt">ocean</span>. Here we address the outflow from the Bay with a view to describing the proximal fate of <span class="hlt">water</span>-borne material in the coastal <span class="hlt">ocean</span>, specifically finer particles and dissolved material. Flow trajectories longer than that in the tidal jet are thus the focus of this study - time scales of hours to days. We present data collected in both winter/runoff and spring/upwelling seasons that reflect the importance of tides and also the importance of wind, which introduces either northward or southward along-coast flow. Southward flow is offshore and typically this Bay effluent is removed from nearshore <span class="hlt">waters</span>. In contrast, northward flow tends to remain attached to shore, and there is persistent presence of Bay <span class="hlt">waters</span> in the surface layer up to Point Reyes, only occasionally separated from the coast by local upwelling within Drakes Bay. Perhaps most dramatic is outflow during winter storms, when wind is southerly and pushes <span class="hlt">water</span> on shore in Drakes Bay as well as inducing an intense flow around Point Reyes, which turns cyclonically to reconnect with the shore in the vicinity of Bodega Bay before forming a wind-accelerated coast-attached current that looks very much like a coastal buoyancy current. This is the time when large volumes of low-salinity and high-load <span class="hlt">waters</span> are exported from the Bay.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMOS54A..06S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMOS54A..06S"><span>Processes Driving Natural Acidification of Western Pacific Coral Reef <span class="hlt">Waters</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shamberger, K. E.; Cohen, A. L.; Golbuu, Y.; McCorkle, D. C.; Lentz, S. J.; Barkley, H. C.</p> <p>2013-12-01</p> <p>Rising levels of atmospheric carbon dioxide (CO2) are acidifying the <span class="hlt">oceans</span>, reducing seawater pH, aragonite saturation state (Ωar) and the availability of carbonate ions (CO32-) that calcifying organisms use to build coral reefs. Today's most extensive reef ecosystems are located where <span class="hlt">open</span> <span class="hlt">ocean</span> CO32- concentration ([CO32-]) and Ωar exceed 200 μmol kg-1 and 3.3, respectively. However, high rates of biogeochemical cycling and long residence times of <span class="hlt">water</span> can result in carbonate chemistry conditions within coral reef systems that differ greatly from those of nearby <span class="hlt">open</span> <span class="hlt">ocean</span> <span class="hlt">waters</span>. In the Palauan archipelago, <span class="hlt">water</span> moving across the reef platform is altered by both biological and hydrographic processes that combine to produce seawater pH, Ωar, [CO32-] significantly lower than that of <span class="hlt">open</span> <span class="hlt">ocean</span> source <span class="hlt">water</span>. Just inshore of the barrier reefs, average Ωar values are 0.2 to 0.3 and pH values are 0.02 to 0.03 lower than they are offshore, declining further as <span class="hlt">water</span> moves across the back reef, lagoon and into the meandering bays and inlets that characterize the Rock Islands. In the Rock Island bays, coral communities inhabit seawater with average Ωar values of 2.7 or less, and as low as 1.9. Levels of Ωar as low as these are not predicted to occur in the western tropical Pacific <span class="hlt">open</span> <span class="hlt">ocean</span> until near the end of the century. Calcification by coral reef organisms is the principal biological process responsible for lowering Ωar and pH, accounting for 68 - 99 % of the difference in Ωar between offshore source <span class="hlt">water</span> and reef <span class="hlt">water</span> at our sites. However, in the Rock Island bays where Ωar is lowest, CO2 production by net respiration contributes between 17 - 30 % of the difference in Ωar between offshore source <span class="hlt">water</span> and reef <span class="hlt">water</span>. Furthermore, the residence time of seawater in the Rock Island bays is much longer than at the well flushed exposed sites, enabling calcification and respiration to drive Ωar to very low levels despite lower net ecosystem</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C21A0659F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C21A0659F"><span>Downscaled ice-<span class="hlt">ocean</span> simulations for the Chukchi and Eastern Siberian Seas from an <span class="hlt">oceanic</span> re-analysis product</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fujisaki-Manome, A.; Wang, J.</p> <p>2016-12-01</p> <p>Arctic summer sea ice has been declining at the rate that is much faster than any climate models predict. While the accelerated sea ice melting in the recent few decades could be attributed to several mechanisms such as the Arctic temperature amplification and the ice-albedo feedback, this does not necessarily explain why climate models underestimate the observed rate of summer sea ice loss. Clearly, an improved understanding is needed in what processes could be missed in climate models and could play roles in unprecedented loss of sea ice. This study evaluates contributions of sub-mesoscale processes in the ice edge (i.e. the boundary region between <span class="hlt">open</span> <span class="hlt">water</span> and ice covered area), which include eddies, ice bands, and the vertical mixing associated with ice bands, to the melting of sea ice and how they explain the underestimation of sea ice loss in the current state-of-art climate models. The focus area is in the pacific side of the Arctic <span class="hlt">Ocean</span>. First, several <span class="hlt">oceanic</span> re-analysis products including NCEP-Climate Forecast System Reanalysis (CFSR) and Modern-Era Retrospective Analysis for Research and Applications (MERRA) are evaluated in comparison with the in-situ observations from the Russian-American Long-term Census of the Arctic (RUSALCA) project. Second, the downscaled ice-<span class="hlt">ocean</span> simulations are conducted for the Chukchi and East Siberian Seas with initial and <span class="hlt">open</span> boundary conditions provided from a selected <span class="hlt">oceanic</span> re-analysis product.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSMM24C0459P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSMM24C0459P"><span>Abundance of genes involved in mercury methylation in <span class="hlt">oceanic</span> environments</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Palumbo, A. V.; Podar, M.; Gilmour, C. C.; Brandt, C. C.; Brown, S. D.; Crable, B. R.; Weighill, D.; Jacobson, D. A.; Somenahally, A. C.; Elias, D. A.</p> <p>2016-02-01</p> <p>The distribution and diversity of genes involved in mercury methylation in <span class="hlt">oceanic</span> environments is of interest in determining the source of mercury in <span class="hlt">ocean</span> environments and may have predictive value for mercury methylation rates. The highly conserved hgcAB genes involved in mercury methylation provide an avenue for evaluating the genetic potential for mercury methylation. The genes are sporadically present in a few diverse groups of bacteria and Archaea including Deltaproteobacteria, Firmicutes and Archaea and of over 7000 sequenced species they are only present in about 100 genomes. Examination of sequence data from methylators and non-methylators indicates that these genes are associated with other genes involved in metal transformations and transport. We examined hgcAB presence in over 3500 microbial metagenomes (from all environments) and found the hgcAB genes were present in anaerobic <span class="hlt">oceanic</span> environments but not in aerobic layers of the <span class="hlt">open</span> <span class="hlt">ocean</span>. The genes were common in sediments from marine, coastal and estuarine sources as well as polluted environments. The genes were rare, found in 7 of 138 samples, in metagenomes from the pelagic <span class="hlt">water</span> column including profiles though the oxygen minimum zone. Other oxic and sub-oxic coastal <span class="hlt">waters</span> also demonstrated a lack of hgcAB genes including the OMZ in the Eastern North Pacific <span class="hlt">Ocean</span>. There were some unique hgcA like unique sequences found in metagenomes from depth in the Pacific and Southern Atlantic <span class="hlt">Ocean</span>. Coastal "dead zone" <span class="hlt">waters</span> may be important sources of MeHg as the hgcAB genes were abundant in the anoxic <span class="hlt">waters</span> of a stratified fjord. The genes were absent in microbiomes from vertebrates but were in invertebrate microbiomes However, <span class="hlt">oceanic</span> species were underrepresented in these samples. Climate change could provide an additional flux of MeHg to the <span class="hlt">oceans</span> as we found the most abundant representation of hgcAB genes in arctic permafrost. Thus warming could increase flux of methyl mercury to arctic <span class="hlt">waters</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP33E..04G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP33E..04G"><span>500 kyr of Indian <span class="hlt">Ocean</span> Walker Circulation Variability Using Foraminiferal Mg/Ca and Stable Isotopes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Groeneveld, J.; Mohtadi, M.; Lückge, A.; Pätzold, J.</p> <p>2017-12-01</p> <p>The tropical Indian <span class="hlt">Ocean</span> is a key location for paleoclimate research affected by different oceanographic and atmospheric processes. Annual climate variations are strongly controlled by the Indian and Asian Monsoon characterized by bi-annually reversing trade winds. Inter-annual climate variations in the Walker circulation are caused by the Indian <span class="hlt">Ocean</span> Dipole and El Niño-Southern Oscillation resulting in either heavy flooding or severe droughts like for example the famine of 2011 in eastern Africa. Oceanographically the tropical western Indian <span class="hlt">Ocean</span> receives <span class="hlt">water</span> masses from the Indonesian Gateway area, sub-Antarctic <span class="hlt">waters</span> that upwell south of the equator, and the outflow <span class="hlt">waters</span> from the highly saline Red Sea. On the other hand, the tropical western Indian <span class="hlt">Ocean</span> is a major source for providing <span class="hlt">water</span> masses to the Agulhas Current system. Although the eastern Indian <span class="hlt">Ocean</span> has been studied extensively, the tropical western Indian <span class="hlt">Ocean</span> is still lacking in high quality climate-archives that have the potential to provide important information to understand how the <span class="hlt">ocean</span> and atmospheric zonal circulation have changed in the past, and possibly will change in the future. Until now there were no long sediment cores available covering several glacial-interglacial cycles in the tropical western Indian <span class="hlt">Ocean</span>. Core GeoB 12613-1, recovered during RV Meteor Cruise M75/2 east of the island of Pemba off Tanzania, provides an <span class="hlt">open-ocean</span> core with well-preserved sediments covering the last five glacial-interglacial cycles ( 500 kyr). Mg/Ca and stable isotopes on both surface- and thermocline dwelling foraminifera have been performed to test how changes in sea <span class="hlt">water</span> temperatures and relative sea <span class="hlt">water</span> salinity were coupled on orbital time scales. The results are compared with similar records generated for the tropical eastern Indian <span class="hlt">Ocean</span> in core SO139-74KL off Sumatra. <span class="hlt">Water</span> column stratification on both sides of the Indian <span class="hlt">Ocean</span> and the cross-basin gradients in sea <span class="hlt">water</span></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 air-sea interaction over North Atlantic <span class="hlt">open</span> <span class="hlt">ocean</span> 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><span class="hlt">Open</span> <span class="hlt">ocean</span> convection, where a loss of surface buoyancy leads to an overturning of the <span class="hlt">water</span> 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 air outbreaks characterized by large surface turbulent heat fluxes and convective roll cloud development. Here we compare the statistics of the air-sea interaction over these convection sites as represented in three reanalyses with horizontal grid sizes ranging from 80km to 15km. We show that increasing the resolution increases the magnitude and frequency of the most extreme total turbulent heat fluxes, 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 air outbreaks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.noaanews.noaa.gov/stories2015/20150526-national-water-center-opens-on-university-of-alabama-campus-in-tuscaloosa.html','SCIGOVWS'); return false;" href="http://www.noaanews.noaa.gov/stories2015/20150526-national-water-center-opens-on-university-of-alabama-campus-in-tuscaloosa.html"><span>National <span class="hlt">Water</span> Center <span class="hlt">opens</span> on University of Alabama campus in Tuscaloosa</span></a></p> <p><a target="_blank" href="http://www.science.gov/aboutsearch.html">Science.gov Websites</a></p> <p></p> <p></p> <p>will be the first ever clearing house for <em>research</em> and operational forecasting of all <em><span class="hlt">water</span></em>-related boasts a robust <em>research</em> program focused on the protection and restoration of the nation's <em><span class="hlt">water</span></em> supply NOAA HOME WEATHER <span class="hlt">OCEANS</span> FISHERIES CHARTING SATELLITES CLIMATE <em>RESEARCH</em> COASTS CAREERS National</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2010-03-22/pdf/2010-6159.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2010-03-22/pdf/2010-6159.pdf"><span>75 FR 13454 - Special Local Regulation, Fran Schnarr <span class="hlt">Open</span> <span class="hlt">Water</span> Championships, Huntington Bay, NY</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2010-03-22</p> <p>...-AA08 Special Local Regulation, Fran Schnarr <span class="hlt">Open</span> <span class="hlt">Water</span> Championships, Huntington Bay, NY AGENCY: Coast... navigable <span class="hlt">waters</span> of Huntington Bay, New York due to the annual Fran Schnarr <span class="hlt">Open</span> <span class="hlt">Water</span> Championships. The..., ``Special Local Regulation, Fran Schnarr <span class="hlt">Open</span> <span class="hlt">Water</span> Championships, Huntington Bay, NY'' (Docket number USCG...</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_16 --> <div id="page_17" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li class="active"><span>17</span></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="321"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26929361','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26929361"><span>Insights into global diatom distribution and diversity in the world's <span class="hlt">ocean</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Malviya, Shruti; Scalco, Eleonora; Audic, Stéphane; Vincent, Flora; Veluchamy, Alaguraj; Poulain, Julie; Wincker, Patrick; Iudicone, Daniele; de Vargas, Colomban; Bittner, Lucie; Zingone, Adriana; Bowler, Chris</p> <p>2016-03-15</p> <p>Diatoms (Bacillariophyta) constitute one of the most diverse and ecologically important groups of phytoplankton. They are considered to be particularly important in nutrient-rich coastal ecosystems and at high latitudes, but considerably less so in the oligotrophic <span class="hlt">open</span> <span class="hlt">ocean</span>. The Tara <span class="hlt">Oceans</span> circumnavigation collected samples from a wide range of <span class="hlt">oceanic</span> regions using a standardized sampling procedure. Here, a total of ∼12 million diatom V9-18S ribosomal DNA (rDNA) ribotypes, derived from 293 size-fractionated plankton communities collected at 46 sampling sites across the global <span class="hlt">ocean</span> euphotic zone, have been analyzed to explore diatom global diversity and community composition. We provide a new estimate of diversity of marine planktonic diatoms at 4,748 operational taxonomic units (OTUs). Based on the total assigned ribotypes, Chaetoceros was the most abundant and diverse genus, followed by Fragilariopsis, Thalassiosira, and Corethron We found only a few cosmopolitan ribotypes displaying an even distribution across stations and high abundance, many of which could not be assigned with confidence to any known genus. Three distinct communities from South Pacific, Mediterranean, and Southern <span class="hlt">Ocean</span> <span class="hlt">waters</span> were identified that share a substantial percentage of ribotypes within them. Sudden drops in diversity were observed at Cape Agulhas, which separates the Indian and Atlantic <span class="hlt">Oceans</span>, and across the Drake Passage between the Atlantic and Southern <span class="hlt">Oceans</span>, indicating the importance of these <span class="hlt">ocean</span> circulation choke points in constraining diatom distribution and diversity. We also observed high diatom diversity in the <span class="hlt">open</span> <span class="hlt">ocean</span>, suggesting that diatoms may be more relevant in these <span class="hlt">oceanic</span> systems than generally considered.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24461428','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24461428"><span>Concentrations of mercury in tissues of striped dolphins suggest decline of pollution in Mediterranean <span class="hlt">open</span> <span class="hlt">waters</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Borrell, A; Aguilar, A; Tornero, V; Drago, M</p> <p>2014-07-01</p> <p>The Mediterranean is a semi-enclosed sea subject to high mercury (Hg) pollution from both natural and anthropogenic sources. With the objective of discerning temporal changes in marine Hg pollution in the <span class="hlt">oceanic</span> <span class="hlt">waters</span> of the northwestern Mediterranean Sea, we analysed liver and kidney from striped dolphins (Stenella coeruleoalba) collected during 2007-2009 and compared them with previous results from a similar sample from 1990-1993. The effect of body length and sex on tissue Hg concentrations was investigated to ensure an unbiased comparison between the periods. The Hg concentrations did not show significant sex-related differences in any tissue or period but were correlated positively with body length. Using body length as a covariate, Hg concentrations in liver and kidney were higher in 1990-1993 than in 2007-2009. This result suggests that measures to reduce emissions in Western European countries have been effective in reducing mercury pollution in Mediterranean <span class="hlt">open</span> <span class="hlt">waters</span>. Copyright © 2014 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140002781','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140002781"><span>Origin and Distribution of <span class="hlt">Water</span> Contents in Continental and <span class="hlt">Oceanic</span> Lithospheric Mantle</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Peslier, Anne H.</p> <p>2013-01-01</p> <p>The <span class="hlt">water</span> content distribution of the upper mantle will be reviewed as based on the peridotite record. The amount of <span class="hlt">water</span> in cratonic xenoliths appears controlled by metasomatism while that of the <span class="hlt">oceanic</span> mantle retains in part the signature of melting events. In both cases, the <span class="hlt">water</span> distribution is heterogeneous both with depth and laterally, depending on localized <span class="hlt">water</span> re-enrichments next to melt/fluid channels. The consequence of the <span class="hlt">water</span> distribution on the rheology of the upper mantle and the location of the lithosphere-asthenosphere boundary will also be discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS41B1955X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS41B1955X"><span>Observation of <span class="hlt">water</span> mass characteristics in the southwestern Mariana Trench</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xu, H.; Xie, Q.; Hong, B.</p> <p>2016-12-01</p> <p>The identification of large <span class="hlt">water</span> mass characteristic can help oceanographer to better understand the <span class="hlt">oceanic</span> circulation structures and other physical processes in <span class="hlt">open</span> <span class="hlt">oceans</span>. In current stage, the <span class="hlt">water</span> mass characteristics were recognized well by extensive observation in the upper <span class="hlt">ocean</span>, however, it was rarely studied in deep <span class="hlt">oceans</span>, especially for deep trench with > 6000 m depth. In this study, we use observed data collected by CTDs during several surveys to investigate the <span class="hlt">water</span> mass physical characteristic and transport in the world deepest trench, `Challenger Deep', in the southwestern Mariana Trench. The preliminary results show complex vertical structures of <span class="hlt">water</span> mass in this trench. From surface to 4500 m, the <span class="hlt">water</span> masses are occupied by typical tropical surface <span class="hlt">water</span>, NPTUW, NPMW, NPIW and NPDW. Under 4500m, the <span class="hlt">water</span> mass shows mixing characteristics of NPDW and AABW, which indicate AABW can be transported by form the deep <span class="hlt">ocean</span> of the South <span class="hlt">Ocean</span> to Northwestern Pacific and it can affect local <span class="hlt">water</span> mass characteristics. The baroclinic geostrophic current calculated from the CTDs data shows the westerly transport of <span class="hlt">water</span> mass can reach about 1.0 SV in the trench which is close to previous results.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA624783','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA624783"><span>Deep <span class="hlt">Water</span> <span class="hlt">Ocean</span> Acoustics</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2015-10-19</p> <p>and has a large number of hydroacoustic signals generated by seismic events. Results Many of these results were reported in the previous July 15...noise, under-ice scattering, bathymetric diffraction and the application of the <span class="hlt">ocean</span> acoustic Parabolic Equation to infrasound . 2. Tasks a. Task...of long-range signals is a seismic event on the Kerguelen Plateau (-53°S 71°E) in the southern <span class="hlt">ocean</span>. This region of the world, which includes Heard</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.5084M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.5084M"><span><span class="hlt">Open</span> data for <span class="hlt">water</span>-related operational services, the SWITCH-ON approach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mazzoli, Paolo; Bagli, Stefano; Valerio, Luzzi; Broccoli, Davide; Piccinini, Francesca</p> <p>2017-04-01</p> <p>Recently, a collaborative project started called SWITCH-ON (EU FP7 project No 603587) coordinated by SMHI (http://<span class="hlt">water</span>-switch-on.eu/) as part of the contemporary European movement imposed by the INSPIRE directive and the <span class="hlt">Open</span> Data Strategy. Among It's R&D activities GECOsistema develops and expands inside SWITCH-ON a set of online services to tackle major <span class="hlt">water</span> related issues, from reservoir and irrigation supply, to hydrological change adaptation and hydropower potential mapping. Here we present major releases of APRIL, HyCAW and High-resolution European HydroPower Atlas; all of which make intense use of <span class="hlt">open</span> data. APRIL is a tool for seasonal run-off forecasts, that takes advantage of <span class="hlt">open</span> datasets or low-cost data and performs forecasts through calibrated machine learning algorithms. HyCAW is a wizard that supports the assessment of adaptation options to cope with change in the temporal distribution of <span class="hlt">water</span> availability as well as in the total <span class="hlt">water</span> quantity. EU HPA provides all relevant information necessary to appraise the feasibility of a micro-hydropower plant at a specific site, taking into account hydrological as well as technical and economic factors. All the tools share a common vision of the project to address <span class="hlt">water</span> concerns and currently untapped potential of <span class="hlt">open</span> data for improved <span class="hlt">water</span> management across the EU. Users are guided through a Web GIS interface, created using <span class="hlt">open</span> source Web Mapping Applications, <span class="hlt">Open</span>-Layers and Map Server, to explore available hydrological information in the area of interest, plot available data, perform analysis, and get reports and statistics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3346459','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3346459"><span>Microbial Functioning and Community Structure Variability in the Mesopelagic and Epipelagic <span class="hlt">Waters</span> of the Subtropical Northeast Atlantic <span class="hlt">Ocean</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>Arístegui, Javier; Gasol, Josep M.; Herndl, Gerhard J.</p> <p>2012-01-01</p> <p>We analyzed the regional distribution of bulk heterotrophic prokaryotic activity (leucine incorporation) and selected single-cell parameters (cell viability and nucleic acid content) as parameters for microbial functioning, as well as bacterial and archaeal community structure in the epipelagic (0 to 200 m) and mesopelagic (200 to 1,000 m) subtropical Northeast Atlantic <span class="hlt">Ocean</span>. We selectively sampled three contrasting regions covering a wide range of surface productivity and oceanographic properties within the same basin: (i) the eddy field south of the Canary Islands, (ii) the <span class="hlt">open-ocean</span> NE Atlantic Subtropical Gyre, and (iii) the upwelling filament off Cape Blanc. In the epipelagic <span class="hlt">waters</span>, a high regional variation in hydrographic parameters and bacterial community structure was detected, accompanied, however, by a low variability in microbial functioning. In contrast, mesopelagic microbial functioning was highly variable between the studied regions despite the homogeneous abiotic conditions found therein. More microbial functioning parameters indicated differences among the three regions within the mesopelagic (i.e., viability of cells, nucleic acid content, cell-specific heterotrophic activity, nanoflagellate abundance, prokaryote-to-nanoflagellate abundance ratio) than within the epipelagic (i.e., bulk activity, nucleic acid content, and nanoflagellate abundance) <span class="hlt">waters</span>. Our results show that the mesopelagic realm in the Northeast Atlantic is, in terms of microbial activity, more heterogeneous than its epipelagic counterpart, probably linked to mesoscale hydrographical variations. PMID:22344670</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ACP....18.6207L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ACP....18.6207L"><span>Sources of reactive nitrogen in marine aerosol over the Northwest Pacific <span class="hlt">Ocean</span> in spring</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Luo, Li; Kao, Shuh-Ji; Bao, Hongyan; Xiao, Huayun; Xiao, Hongwei; Yao, Xiaohong; Gao, Huiwang; Li, Jiawei; Lu, Yangyang</p> <p>2018-05-01</p> <p>Atmospheric deposition of long-range transport of anthropogenic reactive nitrogen (Nr, mainly comprised of NHx, NOy and <span class="hlt">water</span>-soluble organic nitrogen, WSON) from continents may have profound impact on marine biogeochemistry. In addition, surface <span class="hlt">ocean</span> dissolved organic nitrogen (DON) may also contribute to aerosol WSON in the overlying atmosphere. Despite the importance of off-continent dispersion and Nr interactions at the atmosphere-<span class="hlt">ocean</span> boundary, our knowledge of the sources of various nitrogen species in the atmosphere over the <span class="hlt">open</span> <span class="hlt">ocean</span> remains limited due to insufficient observations. We conducted two cruises in the spring of 2014 and 2015 from the coast of China through the East China seas (ECSs, i.e. the Yellow Sea and East China Sea) to the <span class="hlt">open</span> <span class="hlt">ocean</span> (i.e. the Northwest Pacific <span class="hlt">Ocean</span>, NWPO). Concentrations of <span class="hlt">water</span>-soluble total nitrogen (WSTN), NO3- and NH4+, as well as the δ15N of WSTN and NO3- in marine aerosol, were measured during both cruises. In the spring of 2015, we also analysed the concentrations and δ15N of NO3- and the DON of surface seawater (SSW; at a depth of 5 m) along the cruise track. Aerosol NO3-, NH4+ and WSON decreased logarithmically (1-2 orders of magnitude) with distance from the shore, reflecting strong anthropogenic emission sources of NO3-, NH4+ and WSON in China. Average aerosol NO3- and NH4+ concentrations were significantly higher in 2014 (even in the remote NWOP) than in 2015 due to the stronger wind field in 2014, underscoring the role of the Asian winter monsoon in the seaward transport of anthropogenic NO3- and NH4+. However, the background aerosol WSON over the NWPO in 2015 (13.3 ± 8.5 nmol m-3) was similar to that in 2014 (12.2 ± 6.3 nmol m-3), suggesting an additional non-anthropogenic WSON source in the <span class="hlt">open</span> <span class="hlt">ocean</span>. Obviously, marine DON emissions should be considered in model and field assessments of net atmospheric WSON deposition in the <span class="hlt">open</span> <span class="hlt">ocean</span>. This study contributes information on parallel isotopic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23891244','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23891244"><span>Heat stroke risk for <span class="hlt">open-water</span> swimmers during long-distance events.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Macaluso, Filippo; Barone, Rosario; Isaacs, Ashwin W; Farina, Felicia; Morici, Giuseppe; Di Felice, Valentina</p> <p>2013-12-01</p> <p><span class="hlt">Open-water</span> swimming is a rapidly growing sport discipline worldwide, and clinical problems associated with long-distance swimming are now better recognized and managed more effectively. The most prevalent medical risk associated with an <span class="hlt">open-water</span> swimming event is hypothermia; therefore, the Federation Internationale De Natation (FINA) has instituted 2 rules to reduce this occurrence related to the minimum <span class="hlt">water</span> temperature and the time taken to complete the race. Another medical risk that is relevant to <span class="hlt">open-water</span> swimmers is heat stroke, a condition that can easily go unnoticed. The purpose of this review is to shed light on this physiological phenomenon by examining the physiological response of swimmers during long-distance events, to define a maximum <span class="hlt">water</span> temperature limit for competitions. We conclude that competing in <span class="hlt">water</span> temperatures exceeding 33°C should be avoided. Copyright © 2013 Wilderness Medical Society. Published by Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19920019347&hterms=magma&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dmagma','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19920019347&hterms=magma&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dmagma"><span>A magma <span class="hlt">ocean</span> and the Earth's internal <span class="hlt">water</span> budget</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ahrens, Thomas J.</p> <p>1992-01-01</p> <p>There are lines of evidence which relate bounds on the primordial <span class="hlt">water</span> content of the Earth's mantle to a magma <span class="hlt">ocean</span> and the accompanying Earth accretion process. We assume initially (before a magma <span class="hlt">ocean</span> could form) that as the Earth accreted, it grew from volatile- (H2O, CO2, NH3, CH4, SO2, plus noble) gas-rich planetesimals, which accreted to form an initial 'primitive accretion core' (PAC). The PAC retained the initial complement of planetesimal gaseous components. Shock wave experiments in which both solid, and more recently, the gaseous components of materials such as serpentine and the Murchison meteorite have demonstrated that planetesimal infall velocities of less than 0.5 km/sec, induce shock pressures of less than 0.5 GPa and result in virtually complete retention of planetary gases.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSPC14E2102M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSPC14E2102M"><span>Global decadal climate variability driven by Southern <span class="hlt">Ocean</span> convection</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marinov, I.; Cabre, A.</p> <p>2016-02-01</p> <p>Here we suggest a set of new "teleconnections" by which the Southern <span class="hlt">Ocean</span> (SO) can induce anomalies in the tropical <span class="hlt">oceans</span> and atmosphere. A 5000-year long control simulation in a coupled atmosphere-<span class="hlt">ocean</span> model (CM2Mc, a low-resolution GFDL model) shows a natural, highly regular multi-decadal oscillation between periods of SO <span class="hlt">open</span> sea convection and non-convective periods. This process happens naturally, with different frequencies and durations of convection across the majority of CMIP5 under preindustrial forcing (deLavergne et al., 2014). In our model, oscillations in Weddell Sea convection drive multidecadal variability in SO and global SSTs, as well as SO heat storage, with convective decades warm due to the heat released from the Circumpolar Deep <span class="hlt">Water</span> and non-convective decades cold due to subsurface heat storage. Convective pulses drive local SST and sea ice variations south of 60S, immediately triggering changes in the Ferrell and Hadley cells, atmospheric energy budget and cross-equatorial heat exchange, ultimately influencing the position of the Intertropical Convergence Zone and rain patterns in the tropics. Additionally, the SO convection pulse is propagated to the tropics and the North Atlantic MOC via <span class="hlt">oceanic</span> pathways on relatively fast (decadal) timescales, in agreement with recent observational constraints. <span class="hlt">Open</span> sea convection is the major mode of Antarctic Bottom <span class="hlt">Water</span> (AABW) formation in the CMIP5 models. Future improvements in the representation of shelf convection and sea-ice interaction in the SO are a clear necessity. These model improvements should render the AABW representation more realistic, and might influence (a) the connectivity of the SO with the rest of the planet, as described above and (b) the <span class="hlt">oceanic</span> and global carbon cycle, of which the AABW is a fundamental conduit.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1990InEPS..99..425S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1990InEPS..99..425S"><span>Entrainment of circumpolar <span class="hlt">water</span> in the Indian <span class="hlt">Ocean</span> region of the Antarctic</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sharma, G. S.; Peter, Benny N.</p> <p>1990-09-01</p> <p>The net influx of the circumpolar <span class="hlt">water</span> on the western (approximately along 10°E) and eastern (approximately 115°E) boundaries of the Indian <span class="hlt">Ocean</span>, adopting the method of Montgomery and Stroup is computed on bivariate distribution of potential thermosteric anomaly and salinity to identify the characteristics of the flux. The zonal flux at both the boundaries indicates an alternate strong easterly and westerly flow between 36°S and 45°S, south of which the flow is mainly easterly but weak up to 56°S. At the western boundary the easterly flow is 146 Sv and westerly is 98.07 Sv, while at the eastern boundary (115°E) the corresponding fluxes are 123.46 Sv and 27.20 Sv respectively, indicating a net outflux of 48.33 Sv. This <span class="hlt">water</span> should have been accounted by the melting of ice and influx of the Equatorial Pacific <span class="hlt">Ocean</span> <span class="hlt">Water</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70031083','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70031083"><span>Rare-earth elements in the Permian Phosphoria Formation: Paleo proxies of <span class="hlt">ocean</span> geochemistry</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Piper, D.Z.; Perkins, R.B.; Rowe, H.D.</p> <p>2007-01-01</p> <p>The geochemistry of deposition of the Meade Peak Member of the Phosphoria Formation (MPM) in southeast Idaho, USA, a world-class sedimentary phosphate deposit of Permian age that extends over 300,000 km2, is ascertained from its rare earth element (REE) composition. Ratios of REE:Al2O3 suggest two sources-seawater and terrigenous debris. The seawater-derived marine fraction identifies bottom <span class="hlt">water</span> in the Phosphoria Sea as O2-depleted, denitrifying (suboxic) most of the time, and seldom sulfate-reducing (anoxic). This interpretation is supported by earlier research that showed progressively greater ratios in the marine sediment fraction of Cr:Ni>V:Ni???Mo:Ni, relative to their ratios in seawater; for which marine Cr, V, and Mo can have a dominantly O2-depleted bottom-<span class="hlt">water</span> source and Ni a photic-zone, largely algal, source. The <span class="hlt">water</span> chemistry was maintained by a balance between bacterial oxidation of organic matter settling through the <span class="hlt">water</span> column, determined largely by primary productivity in the photic zone, and the flux of oxidants into the bottom <span class="hlt">water</span> via advection of seawater from the <span class="hlt">open</span> <span class="hlt">ocean</span>. Samples strongly enriched in carbonate fluorapatite, the dominant REE host mineral, have variable Er/Sm, Tm/Sm, and Yb/Sm ratios. Their distribution may represent greater advection of seawater between the Phosphoria Sea and <span class="hlt">open</span> <span class="hlt">ocean</span> during deposition of two ore zones than a center waste and greater upwelling of nutrient-enriched <span class="hlt">water</span> into the photic zone. However, the mean rate of deposition of marine Ni, a trace nutrient of algae, and PO43-, a limiting nutrient, indicate that primary productivity was probably high throughout the depositional history. An alternative interpretation of the variable enrichments of Er, Tm, and Yb, relative to Sm, is that they may reflect temporally variable carbonate alkalinity of <span class="hlt">open-ocean</span> seawater in Permian time. A more strongly negative Ce anomaly for all phosphatic units than the Ce anomaly of modern pelletal phosphate is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007DSRII..54.1396P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007DSRII..54.1396P"><span>Rare-earth elements in the Permian Phosphoria Formation: Paleo proxies of <span class="hlt">ocean</span> geochemistry</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Piper, D. Z.; Perkins, R. B.; Rowe, H. D.</p> <p>2007-06-01</p> <p>The geochemistry of deposition of the Meade Peak Member of the Phosphoria Formation (MPM) in southeast Idaho, USA, a world-class sedimentary phosphate deposit of Permian age that extends over 300,000 km 2, is ascertained from its rare earth element (REE) composition. Ratios of REE:Al 2O 3 suggest two sources—seawater and terrigenous debris. The seawater-derived marine fraction identifies bottom <span class="hlt">water</span> in the Phosphoria Sea as O 2-depleted, denitrifying (suboxic) most of the time, and seldom sulfate-reducing (anoxic). This interpretation is supported by earlier research that showed progressively greater ratios in the marine sediment fraction of Cr:Ni>V:Ni≫Mo:Ni, relative to their ratios in seawater; for which marine Cr, V, and Mo can have a dominantly O 2-depleted bottom-<span class="hlt">water</span> source and Ni a photic-zone, largely algal, source. The <span class="hlt">water</span> chemistry was maintained by a balance between bacterial oxidation of organic matter settling through the <span class="hlt">water</span> column, determined largely by primary productivity in the photic zone, and the flux of oxidants into the bottom <span class="hlt">water</span> via advection of seawater from the <span class="hlt">open</span> <span class="hlt">ocean</span>. Samples strongly enriched in carbonate fluorapatite, the dominant REE host mineral, have variable Er/Sm, Tm/Sm, and Yb/Sm ratios. Their distribution may represent greater advection of seawater between the Phosphoria Sea and <span class="hlt">open</span> <span class="hlt">ocean</span> during deposition of two ore zones than a center waste and greater upwelling of nutrient-enriched <span class="hlt">water</span> into the photic zone. However, the mean rate of deposition of marine Ni, a trace nutrient of algae, and PO 43-, a limiting nutrient, indicate that primary productivity was probably high throughout the depositional history. An alternative interpretation of the variable enrichments of Er, Tm, and Yb, relative to Sm, is that they may reflect temporally variable carbonate alkalinity of <span class="hlt">open-ocean</span> seawater in Permian time. A more strongly negative Ce anomaly for all phosphatic units than the Ce anomaly of modern pelletal phosphate</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6565360-ocean-thermal-energy-conversion-perspective-status','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6565360-ocean-thermal-energy-conversion-perspective-status"><span><span class="hlt">Ocean</span> thermal energy conversion: Perspective and status</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>Thomas, A.; Hillis, D.L.</p> <p>1990-01-01</p> <p>The use of the thermal gradient between the warm surface <span class="hlt">waters</span> and the deep cold <span class="hlt">waters</span> of tropical <span class="hlt">oceans</span> was first proposed by J. A. d'Arsonval in 1881 and tried unsuccessfully be George Claude in 1930. Interest in <span class="hlt">Ocean</span> Thermal Energy Conversion (OTEC) and other renewable energy sources revived in the 1970s as a result of oil embargoes. At that time, the emphasis was on large floating plants miles from shore producing 250--400 MW for maintained grids. When the problems of such plants became better understood and the price of oil reversed its upward trend, the emphasis shifted to smallermore » (10 MW) shore-based plants on tropical islands. Such plants would be especially attractive if they produce fresh <span class="hlt">water</span> as a by-product. During the past 15 years, major progress has been made in converting OTEC unknowns into knowns. Mini-OTEC proved the closed-cycle concept. Cost-effective heat-exchanger concepts were identified. An effective biofouling control technique was discovered. Aluminum was determined to be promising for OTEC heat exchangers. Heat-transfer augmentation techniques were identified, which promised a reduction on heat-exchanger size and cost. Fresh <span class="hlt">water</span> was produced by an OTEC <span class="hlt">open</span>-cycle flash evaporator, using the heat energy in the seawater itself. The current R D emphasis is on the design and construction of a test facility to demonstrate the technical feasibility of the <span class="hlt">open</span>-cycle process. The 10 MW shore-based, closed-cycle plant can be built with today's technology; with the incorporation of a flash evaporator, it will produce fresh <span class="hlt">water</span> as well as electrical power -- both valuable commodities on many tropical islands. The <span class="hlt">open</span>-cycle process has unknowns that require solution before the technical feasibility can be demonstrated. The economic viability of either cycle depends on reducing the capital costs of OTEC plants and on future trends in the costs of conventional energy sources. 7 refs.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1990STIN...9111299T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1990STIN...9111299T"><span><span class="hlt">Ocean</span> thermal energy conversion: Perspective and status</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Thomas, Anthony; Hillis, David L.</p> <p></p> <p>The use of the thermal gradient between the warm surface <span class="hlt">waters</span> and the deep cold <span class="hlt">waters</span> of tropical <span class="hlt">oceans</span> was first proposed by J. A. d'Arsonval in 1881 and tried unsuccessfully by George Claude in 1930. Interest in <span class="hlt">Ocean</span> Thermal Energy Conversion (OTEC) and other renewable energy sources revived in the 1970s as a result of oil embargoes. At that time, the emphasis was on large floating plants miles from shore producing 250 to 400 MW for maintained grids. When the problems of such plants became better understood and the price of oil reversed its upward trend, the emphasis shifted to smaller (10 MW) shore based plants on tropical islands. Such plants would be especially attractive if they produce fresh <span class="hlt">water</span> as a by-product. During the past 15 years, major progress has been made in converting OTEC unknowns into knowns. Mini-OTEC proved the closed cycle concept. Cost effective heat exchanger concepts were identified. An effective biofouling control technique was discovered. Aluminum was determined to be promising for OTEC heat exchangers. Heat transfer augmentation techniques were identified, which promised a reduction on heat exchanger size and cost. Fresh <span class="hlt">water</span> was produced by an OTEC <span class="hlt">open</span> cycle flash evaporator, using the heat energy in the seawater itself. The current R and D emphasis is on the design and construction of a test facility to demonstrate the technical feasibility of the <span class="hlt">open</span> cycle process. The 10 MW shore-based, closed cycle plant can be built with today's technology; with the incorporation of a flash evaporator, it will produce fresh <span class="hlt">water</span> as well as electrical power; both valuable commodities on many tropical islands. The <span class="hlt">open</span> cycle process has unknowns that require solution before the technical feasibility can be demonstrated. The economic viability of either cycle depends on reducing the capital costs of OTEC plants and on future trends in the costs of conventional energy sources.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1997JGR...102.7915S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1997JGR...102.7915S"><span>Evidence from <span class="hlt">Ocean</span> Drilling Program Leg 149 mafic igneous rocks for <span class="hlt">oceanic</span> crust in the Iberia Abyssal Plain <span class="hlt">ocean</span>-continent transition zone</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Seifert, Karl E.; Chang, Cheng-Wen; Brunotte, Dale A.</p> <p>1997-04-01</p> <p>Leg 149 of the <span class="hlt">Ocean</span> Drilling Program explored the <span class="hlt">ocean</span>-continent transition (OCT) on the Iberia Abyssal Plain and its role in the <span class="hlt">opening</span> of the Atlantic <span class="hlt">Ocean</span> approximately 130 Ma. Mafic igneous rocks recovered from Holes 899B and 900A have Mid-<span class="hlt">Ocean</span> Ridge Basalt (MORB) trace element and isotopic characteristics indicating that a spreading center was active during the <span class="hlt">opening</span> of the Iberia Abyssal Plain OCT. The Hole 899B weathered basalt and diabase clasts have transitional to enriched MORB rare earth element characteristics, and the Hole 900A metamorphosed gabbros have MORB initial epsilon Nd values between +6 and +11. During the <span class="hlt">opening</span> event the Iberia Abyssal Plain OCT is envisioned to have resembled the central and northern parts of the present Red Sea with localized spreading centers and magma chambers producing localized patches of MORB mafic rocks. The lack of a normal <span class="hlt">ocean</span> floor magnetic anomaly pattern in the Iberia Abyssal Plain means that a continuous spreading center similar to that observed in the present southern Red Sea was not formed before spreading ceased in the Iberia Abyssal Plain OCT and jumped to the present Mid-Atlantic Ridge.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24667305','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24667305"><span>Nutrition considerations for <span class="hlt">open-water</span> swimming.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Shaw, Gregory; Koivisto, Anu; Gerrard, David; Burke, Louise M</p> <p>2014-08-01</p> <p><span class="hlt">Open-water</span> swimming (OWS) is a rapidly developing discipline. Events of 5-25 km are featured at FINA World Championships, and the international circuit includes races of 5-88 km. The Olympic OWS event, introduced in 2008, is contested over 10 km. Differing venues present changing environmental conditions, including <span class="hlt">water</span> and ambient temperatures, humidity, solar radiation, and unpredictable tides. Furthermore, the duration of most OWS events (1-6 hr) creates unique physiological challenges to thermoregulation, hydration status, and muscle fuel stores. Current nutrition recommendations for <span class="hlt">open-water</span> training and competition are either an extension of recommendations from pool swimming or are extrapolated from other athletic populations with similar physiological requirements. Competition nutrition should focus on optimizing prerace hydration and glycogen stores. Although swimmers should rely on self-supplied fuel and fluid sources for shorter events, for races of 10 km or greater, fluid and fuel replacement can occur from feeding pontoons when tactically appropriate. Over the longer races, feeding pontoons should be used to achieve desirable targets of up to 90 g/ hr of carbohydrates from multitransportable sources. Exposure to variable <span class="hlt">water</span> and ambient temperatures will play a significant role in determining race nutrition strategies. For example, in extreme environments, thermoregulation may be assisted by manipulating the temperature of the ingested fluids. Swimmers are encouraged to work with nutrition experts to develop effective and efficient strategies that enhance performance through appropriate in-competition nutrition.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28718095','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28718095"><span>Changes in sub-soil river <span class="hlt">water</span> quality upon its <span class="hlt">open</span> storage-a case study.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mohanty, A K; Satpathy, K K; Prasad, M V R</p> <p>2017-08-01</p> <p>A study was carried out to investigate the changes in the physicochemical and biological properties of sub-soil river <span class="hlt">water</span> upon its storage in a man-made reservoir. Palar sub-soil and reservoir <span class="hlt">water</span> samples were collated fortnightly for a period of 5 years (2010-2014). The <span class="hlt">open</span> reservoir is used as a reliable raw <span class="hlt">water</span> source for condenser cooling systems and for the demineralizing (DM) plant input of Fast Breeder Test Reactor (FBTR), Madras Atomic Power Station (MAPS), and other laboratories at Kalpakkam, southeast coast of India. Relatively high nutrient concentration was observed in the Palar sub-soil <span class="hlt">water</span>, and a significant reduction in average concentration (μmol l -1 ) of phosphate (Palar 1.92; <span class="hlt">open</span> reservoir 1.54) and nitrate (Palar 9.78; <span class="hlt">open</span> reservoir 5.67) was observed from Palar to <span class="hlt">open</span> reservoir. Substantial increase in pH (Palar 8.05; <span class="hlt">open</span> reservoir 8.45), dissolved oxygen (mg l -1 ) (Palar 6.07; <span class="hlt">open</span> reservoir 8.47), and chlorophyll-a (mg m -3 ) (Palar 1.66; <span class="hlt">open</span> reservoir 8.43) values were noticed from the Palar sub-soil <span class="hlt">water</span> to <span class="hlt">open</span> reservoir <span class="hlt">water</span>. It is concluded that sub-soil <span class="hlt">water</span> with higher nutrient concentrations when stored <span class="hlt">openly</span>, exposing to the sun, resulted in growth of plants, planktonic, and macrophytes, which led to substantial deterioration in <span class="hlt">water</span> quality from its utility point of view as a condenser cooling medium and raw <span class="hlt">water</span> input for DM plant.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMPP31D2336F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMPP31D2336F"><span>δ18O and δD of lake <span class="hlt">waters</span> across the Coast Range and Cascades, central Oregon: Modern insights from hydrologically <span class="hlt">open</span> lakes into the control of landscape on lake <span class="hlt">water</span> composition in deep time</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Finkelstein, D. B.; Curtin, T.</p> <p>2016-12-01</p> <p>Reconstructing the stable isotopic composition of paleolake <span class="hlt">water</span> normally requires an assumption of paleotemperature. However, hydrologically <span class="hlt">open</span> paleolakes with short <span class="hlt">water</span> residence times may have recorded paleoprecipitation along topographic gradients that are independent of lake <span class="hlt">water</span> temperature. To identify the environmental and geographic controls on the isotopic composition of lake <span class="hlt">water</span>, we sampled 22 natural lakes and reservoirs along a longitudinal and elevation gradient from the Pacific <span class="hlt">Ocean</span> up and over the Coast and Cascade Ranges of central Oregon to the High Lava Plains in 2013 and 2015. The transect spans lakes of different origins, 6 geomorphic regions and an elevation range of 2-1942 m absl. The Coast Range lakes are sand hosted whereas the remaining are bedrock (volcanic and sedimentary) hosted. The lakes are hydrologically <span class="hlt">open</span> and dominated by meteoric recharge. The <span class="hlt">water</span> residence time ranges from months to decades. Samples were analyzed for temperature, pH, and total dissolved solids (TDS) in the field, and alkalinity and major cations and anions and stable isotopes of D and O in the lab. The pH ranges from 7 to 9.8 and shows no systematic variation based on substrate type or elevation. The lakes are dilute (avg. TDS = 35.8 ppm) and have low alkalinties (18.9 mg/L CaCO3) except for those in the High Lava Plains (avg. TDS = 337 ppm, alk: 291.2 mg/L CaCO3). In the Coast Range, Na is the major cation on an equivalent basis, reflecting proximity to the <span class="hlt">ocean</span>. The easternmost lakes within the Coast Range are dominated by Ca, reflecting different drainage basins and substrate type. Lakes in the Western and High Cascades are dominated by Ca. The dominant cation and stable isotopic analyses clearly differentiate <span class="hlt">waters</span> from different geomorphic regions. The δ18O ranges from -5.7 to -9.3 ‰ (VSMOW), and δD ranges from -37.8 to -63.6 ‰ (VSMOW) in the Coast Range whereas the δ18O ranges from -9.7 to -12.1 ‰ (VSMOW) and δD ranges from -71</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li class="active"><span>17</span></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_17 --> <div id="page_18" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="341"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2012-title43-vol2/pdf/CFR-2012-title43-vol2-sec2091-5-4.pdf','CFR2012'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2012-title43-vol2/pdf/CFR-2012-title43-vol2-sec2091-5-4.pdf"><span>43 CFR 2091.5-4 - Segregative effect and <span class="hlt">opening</span>: <span class="hlt">Water</span> power withdrawals.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2012&page.go=Go">Code of Federal Regulations, 2012 CFR</a></p> <p></p> <p>2012-10-01</p> <p>... 43 Public Lands: Interior 2 2012-10-01 2012-10-01 false Segregative effect and <span class="hlt">opening</span>: <span class="hlt">Water</span> power withdrawals. 2091.5-4 Section 2091.5-4 Public Lands: Interior Regulations Relating to Public Lands... LAWS AND RULES Segregation and <span class="hlt">Opening</span> of Lands § 2091.5-4 Segregative effect and <span class="hlt">opening</span>: <span class="hlt">Water</span> power...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2014-title43-vol2/pdf/CFR-2014-title43-vol2-sec2091-5-4.pdf','CFR2014'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2014-title43-vol2/pdf/CFR-2014-title43-vol2-sec2091-5-4.pdf"><span>43 CFR 2091.5-4 - Segregative effect and <span class="hlt">opening</span>: <span class="hlt">Water</span> power withdrawals.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2014&page.go=Go">Code of Federal Regulations, 2014 CFR</a></p> <p></p> <p>2014-10-01</p> <p>... 43 Public Lands: Interior 2 2014-10-01 2014-10-01 false Segregative effect and <span class="hlt">opening</span>: <span class="hlt">Water</span> power withdrawals. 2091.5-4 Section 2091.5-4 Public Lands: Interior Regulations Relating to Public Lands... LAWS AND RULES Segregation and <span class="hlt">Opening</span> of Lands § 2091.5-4 Segregative effect and <span class="hlt">opening</span>: <span class="hlt">Water</span> power...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2013-title43-vol2/pdf/CFR-2013-title43-vol2-sec2091-5-4.pdf','CFR2013'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2013-title43-vol2/pdf/CFR-2013-title43-vol2-sec2091-5-4.pdf"><span>43 CFR 2091.5-4 - Segregative effect and <span class="hlt">opening</span>: <span class="hlt">Water</span> power withdrawals.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2013&page.go=Go">Code of Federal Regulations, 2013 CFR</a></p> <p></p> <p>2013-10-01</p> <p>... 43 Public Lands: Interior 2 2013-10-01 2013-10-01 false Segregative effect and <span class="hlt">opening</span>: <span class="hlt">Water</span> power withdrawals. 2091.5-4 Section 2091.5-4 Public Lands: Interior Regulations Relating to Public Lands... LAWS AND RULES Segregation and <span class="hlt">Opening</span> of Lands § 2091.5-4 Segregative effect and <span class="hlt">opening</span>: <span class="hlt">Water</span> power...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27087798','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27087798"><span>The impact of post-exercise hydration with deep-<span class="hlt">ocean</span> mineral <span class="hlt">water</span> on rehydration and exercise performance.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Keen, Douglas A; Constantopoulos, Eleni; Konhilas, John P</p> <p>2016-01-01</p> <p>Dehydration caused by prolonged exercise impairs thermoregulation, endurance and exercise performance. Evidence from animal and human studies validates the potential of desalinated deep-<span class="hlt">ocean</span> mineral <span class="hlt">water</span> to positively impact physiological and pathophysiological conditions. Here, we hypothesize that deep-<span class="hlt">ocean</span> mineral <span class="hlt">water</span> drawn from a depth of 915 m off the Kona, HI coast enhances recovery of hydration and exercise performance following a dehydrating exercise protocol compared to mountain spring <span class="hlt">water</span> and a carbohydrate-based sports drink. Subjects (n = 8) were exposed to an exercise-dehydration protocol (stationary biking) under warm conditions (30 °C) to achieve a body mass loss of 3 % (93.4 ± 21.7 total exercise time). During the post-exercise recovery period, subjects received deep-<span class="hlt">ocean</span> mineral <span class="hlt">water</span> (Kona), mountain spring <span class="hlt">water</span> (Spring) or a carbohydrate-based sports drink (Sports) at a volume (in L) equivalent to body mass loss (in Kg). Salivary samples were collected at regular intervals during exercise and post-exercise rehydration. Additionally, each participant performed peak torque knee extension as a measure of lower body muscle performance. Subjects who received Kona during the rehydrating period showed a significantly more rapid return to pre-exercise (baseline) hydration state, measured as the rate of decline in peak to baseline salivary osmolality, compared to Sports and Spring groups. In addition, subjects demonstrated significantly improved recovery of lower body muscle performance following rehydration with Kona versus Sports or Spring groups. Deep-<span class="hlt">ocean</span> mineral <span class="hlt">water</span> shows promise as an optimal rehydrating source over spring <span class="hlt">water</span> and/or sports drink.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5046902','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5046902"><span>The effect of aggregation on visibility in <span class="hlt">open</span> <span class="hlt">water</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p></p> <p>2016-01-01</p> <p>Aggregation is a common life-history trait in <span class="hlt">open-water</span> taxa. Qualitative understanding of how aggregation by prey influences their encounter rates with predators is critical for understanding pelagic predator–prey interactions and trophic webs. We extend a recently developed theory on underwater visibility to predict the consequences of grouping in <span class="hlt">open-water</span> species in terms of increased visual detection of groups by predators. Our model suggests that enhanced visibility will be relatively modest, with maximum detection distance typically only doubling for a 100-fold increase in the number of prey in a group. This result suggests that although larger groups are more easily detected, this cost to aggregation will in many cases be dominated by benefits, especially through risk dilution in situations where predators cannot consume all members of a discovered group. This, in turn, helps to explain the ubiquity of grouping across a great variety of <span class="hlt">open-water</span> taxa. PMID:27655767</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28580419','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28580419"><span>Light penetration structures the deep acoustic scattering layers in the global <span class="hlt">ocean</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Aksnes, Dag L; Røstad, Anders; Kaartvedt, Stein; Martinez, Udane; Duarte, Carlos M; Irigoien, Xabier</p> <p>2017-05-01</p> <p>The deep scattering layer (DSL) is a ubiquitous acoustic signature found across all <span class="hlt">oceans</span> and arguably the dominant feature structuring the pelagic <span class="hlt">open</span> <span class="hlt">ocean</span> ecosystem. It is formed by mesopelagic fishes and pelagic invertebrates. The DSL animals are an important food source for marine megafauna and contribute to the biological carbon pump through the active flux of organic carbon transported in their daily vertical migrations. They occupy depths from 200 to 1000 m at daytime and migrate to a varying degree into surface <span class="hlt">waters</span> at nighttime. Their daytime depth, which determines the migration amplitude, varies across the global <span class="hlt">ocean</span> in concert with <span class="hlt">water</span> mass properties, in particular the oxygen regime, but the causal underpinning of these correlations has been unclear. We present evidence that the broad variability in the <span class="hlt">oceanic</span> DSL daytime depth observed during the Malaspina 2010 Circumnavigation Expedition is governed by variation in light penetration. We find that the DSL depth distribution conforms to a common optical depth layer across the global <span class="hlt">ocean</span> and that a correlation between dissolved oxygen and light penetration provides a parsimonious explanation for the association of shallow DSL distributions with hypoxic <span class="hlt">waters</span>. In enhancing understanding of this phenomenon, our results should improve the ability to predict and model the dynamics of one of the largest animal biomass components on earth, with key roles in the <span class="hlt">oceanic</span> biological carbon pump and food web.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2014-title33-vol2/pdf/CFR-2014-title33-vol2-sec165-T05-0494.pdf','CFR2014'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2014-title33-vol2/pdf/CFR-2014-title33-vol2-sec165-T05-0494.pdf"><span>33 CFR 165.T05-0494 - Safety Zone, Atlantic <span class="hlt">Ocean</span>; <span class="hlt">Ocean</span> City, NJ.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2014&page.go=Go">Code of Federal Regulations, 2014 CFR</a></p> <p></p> <p>2014-07-01</p> <p>... 33 Navigation and Navigable <span class="hlt">Waters</span> 2 2014-07-01 2014-07-01 false Safety Zone, Atlantic <span class="hlt">Ocean</span>; <span class="hlt">Ocean</span> City, NJ. 165.T05-0494 Section 165.T05-0494 Navigation and Navigable <span class="hlt">Waters</span> COAST GUARD... § 165.T05-0494 Safety Zone, Atlantic <span class="hlt">Ocean</span>; <span class="hlt">Ocean</span> City, NJ. (a) Location. The following area is a safety...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSOD14B2414C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSOD14B2414C"><span>Investigating the Potential Impact of the Surface <span class="hlt">Water</span> and <span class="hlt">Ocean</span> Topography (SWOT) Altimeter on <span class="hlt">Ocean</span> Mesoscale Prediction</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carrier, M.; Ngodock, H.; Smith, S. R.; Souopgui, I.</p> <p>2016-02-01</p> <p>NASA's Surface <span class="hlt">Water</span> and <span class="hlt">Ocean</span> Topography (SWOT) satellite, scheduled for launch in 2020, will provide sea surface height anomaly (SSHA) observations with a wider swath width and higher spatial resolution than current satellite altimeters. It is expected that this will help to further constrain <span class="hlt">ocean</span> models in terms of the mesoscale circulation. In this work, this expectation is investigated by way of twin data assimilation experiments using the Navy Coastal <span class="hlt">Ocean</span> Model Four Dimensional Variational (NCOM-4DVAR) data assimilation system using a weak constraint formulation. Here, a nature run is created from which SWOT observations are sampled, as well as along-track SSHA observations from simulated Jason-2 tracks. The simulated SWOT data has appropriate spatial coverage, resolution, and noise characteristics based on an observation-simulator program provided by the SWOT science team. The experiment is run for a three-month period during which the analysis is updated every 24 hours and each analysis is used to initialize a 96 hour forecast. The forecasts in each experiment are compared to the available nature run to determine the impact of the assimilated data. It is demonstrated here that the SWOT observations help to constrain the model mesoscale in a more consistent manner than traditional altimeter observations. The findings of this study suggest that data from SWOT may have a substantial impact on improving the <span class="hlt">ocean</span> model analysis and forecast of mesoscale features and surface <span class="hlt">ocean</span> transport.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19..135B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19..135B"><span>Interannual and Decadal Changes in Salinity in the <span class="hlt">Oceanic</span> Subtropical Gyres</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bulusu, Subrahmanyam</p> <p>2017-04-01</p> <p>There is evidence that the global <span class="hlt">water</span> cycle has been undergoing an intensification over several decades as a response to increasing atmospheric temperatures, particularly in regions with skewed evaporation - precipitation (E-P) patterns such as the <span class="hlt">oceanic</span> subtropical gyres. Moreover, observational data (rain gauges, etc.) are quite sparse over such areas due to the inaccessibility of <span class="hlt">open</span> <span class="hlt">ocean</span> regions. In this work, a comparison of observational and model simulations are conducted to highlight the potential applications of satellite derived salinity from NASA Aquarius Salinity mission, NASA Soil Moisture and <span class="hlt">Ocean</span> Salinity (SMOS), and ESA's Soil Moisture Active Passive (SMAP). We explored spatial and temporal salinity changes (and trends) in surface and subsurface in the <span class="hlt">oceanic</span> subtropical gyres using Argo floats salinity data, Simple <span class="hlt">Ocean</span> Data Assimilation (SODA) reanalysis, Estimating the Circulations & Climate of the <span class="hlt">Ocean</span> GECCO (German ECCO) model simulations, and Hybrid Coordinate <span class="hlt">Ocean</span> Model (HYCOM). Our results based on SODA reanalysis reveals that a positive rising trend in sea surface salinity in the subtropical gyres emphasizing evidence for decadal intensification in the surface forcing in these regions. Zonal drift in the location of the salinity maximum of the south Pacific, north Atlantic, and south Indian regions implies a change in the mean near-surface currents responsible for advecting high salinity <span class="hlt">waters</span> into the region. Also we found out that an overall salinity increase within the mixed layer, and a subsurface salinity decrease at depths greater than 200m in the global subtropical gyres over 61 years. We determine that freshwater fluxes at the air-sea interface are the primary drivers of the sea surface salinity (SSS) signature over these <span class="hlt">open</span> <span class="hlt">ocean</span> regions by quantifying the advective contribution within the surface layer. This was demonstrated through a mixed layer salinity budget in each subtropical gyre based on the vertically</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1999JGR...10420801C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1999JGR...10420801C"><span>Seasonal <span class="hlt">water</span> mass distribution in the Indonesian throughflow entering the Indian <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Coatanoan, C.; Metzl, N.; Fieux, M.; Coste, B.</p> <p>1999-09-01</p> <p>A multiparametric approach is used to analyze the seasonal properties of <span class="hlt">water</span> masses in the eastern Indian <span class="hlt">Ocean</span>. The data were measured during two cruises of the Java Australia Dynamic Experiment (JADE) program carried out during two opposite seasons: August 1989 (SE monsoon) and February-March 1992 (NW monsoon). These cruises took place at the end of a La Niña event and during an El Niño episode, respectively. Seven sources have been identified in the studied region for the 200-800 m layer: the Subtropical Indian <span class="hlt">Water</span>, the Indian Central <span class="hlt">Water</span>, the modified Antarctic Intermediate <span class="hlt">Water</span>, the Indonesian Subsurface <span class="hlt">Water</span>, the Indonesian Intermediate <span class="hlt">Water</span>, the Arabian Sea-Persian Gulf <span class="hlt">Water</span> (AS-PGW), and the Arabian Sea-Red Sea <span class="hlt">Water</span> (AS-RSW). The selected tracers are potential temperature, salinity and oxygen with mass conservation and positive mixing coefficients as constraints. The analysis indicates the proportion of each <span class="hlt">water</span> source along the Australia-Bali section and into the Indonesian channels. Although no large changes are observed for Indonesian <span class="hlt">waters</span>, significant seasonal variations are found for the southern and northern Indian <span class="hlt">Ocean</span> <span class="hlt">water</span>. During the NW monsoon, the contribution of the AS-RSW increases at the entrance of the Indonesian archipelago whereas the contribution of the south Indian <span class="hlt">waters</span> decreases in the northwest Australia basin. In a complementary study, nutrients are introduced into the multiparametric analysis in order to more clearly separate the signature of the north Indian <span class="hlt">waters</span> (AS-PGW, AS-RSW) and to provide supplementary information on the biological history of the <span class="hlt">water</span> masses, which is compared to large-scale primary production estimates.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.6303M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.6303M"><span>Baroclinic stabilization effect of the Atlantic-Arctic <span class="hlt">water</span> exchange simulated by the eddy-permitting <span class="hlt">ocean</span> model and global atmosphere-<span class="hlt">ocean</span> model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moshonkin, Sergey; Bagno, Alexey; Gritsun, Andrey; Gusev, Anatoly</p> <p>2017-04-01</p> <p>Numerical experiments were performed with the global atmosphere-<span class="hlt">ocean</span> model INMCM5 (for version of the international project CMIP6, resolution for atmosphere is 2°x1.5°, 21 level) and with the three-dimensional, free surface, sigma coordinate eddy-permitting <span class="hlt">ocean</span> circulation model for Atlantic (from 30°S) - Arctic and Bering sea domain (0.25 degrees resolution, Institute of Numerical Mathematics <span class="hlt">Ocean</span> Model or INMOM). Spatial resolution of the INMCM5 <span class="hlt">oceanic</span> component is 0.5°x0.25°. Both models have 40 s-levels in <span class="hlt">ocean</span>. Previously, the simulations were carried out for INMCM5 to generate climatic system stable state. Then model was run for 180 years. In the experiment with INMOM, CORE-II data for 1948-2009 were used. As the goal for comparing results of two these numerical models, we selected evolution of the density and velocity anomalies in the 0-300m active <span class="hlt">ocean</span> layer near Fram Strait in the Greenland Sea, where <span class="hlt">oceanic</span> cyclonic circulation influences Atlantic-Arctic <span class="hlt">water</span> exchange. Anomalies were count without climatic seasonal cycle for time scales smaller than 30 years. We use Singular Value Decomposition analysis (SVD) for density-velocity anomalies with time lag from minus one to six months. Both models perform identical stable physical result. They reveal that changes of heat and salt transports by West Spitsbergen and East Greenland currents, caused by atmospheric forcing, produce the baroclinic modes of velocity anomalies in 0-300m layer, thereby stabilizing <span class="hlt">ocean</span> response on the atmospheric forcing, which stimulates keeping <span class="hlt">water</span> exchange between the North Atlantic and Arctic <span class="hlt">Ocean</span> at the certain climatological level. The first SVD-mode of density-velocity anomalies is responsible for the cyclonic circulation variability. The second and third SVD-modes stabilize existing <span class="hlt">ocean</span> circulation by the anticyclonic vorticity generation. The second and third SVD-modes give 35% of the input to the total dispersion of density anomalies and 16-18% of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26140748','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26140748"><span>Development of wavelet-ANN models to predict <span class="hlt">water</span> quality parameters in Hilo Bay, Pacific <span class="hlt">Ocean</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Alizadeh, Mohamad Javad; Kavianpour, Mohamad Reza</p> <p>2015-09-15</p> <p>The main objective of this study is to apply artificial neural network (ANN) and wavelet-neural network (WNN) models for predicting a variety of <span class="hlt">ocean</span> <span class="hlt">water</span> quality parameters. In this regard, several <span class="hlt">water</span> quality parameters in Hilo Bay, Pacific <span class="hlt">Ocean</span>, are taken under consideration. Different combinations of <span class="hlt">water</span> quality parameters are applied as input variables to predict daily values of salinity, temperature and DO as well as hourly values of DO. The results demonstrate that the WNN models are superior to the ANN models. Also, the hourly models developed for DO prediction outperform the daily models of DO. For the daily models, the most accurate model has R equal to 0.96, while for the hourly model it reaches up to 0.98. Overall, the results show the ability of the model to monitor the <span class="hlt">ocean</span> parameters, in condition with missing data, or when regular measurement and monitoring are impossible. Copyright © 2015 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.4327R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.4327R"><span>Impacts of <span class="hlt">ocean</span> acidification on the carbonate system at the sediment-<span class="hlt">water</span> interface: a case-study in the NW Mediterranean Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rassmann, Jens; Lansard, Bruno; Gazeau, Frédéric; Grenz, Christian; Alliouane, Samir; Petit, Franck; Pozzato, Lara; Bombled, Bruno; Rabouille, Christophe</p> <p>2016-04-01</p> <p>According to common predictions, carbon dioxide (CO2) uptake from the atmosphere into the <span class="hlt">oceans</span> will decrease the average pH of seawater by 0.06-0.32 pH units by 2100. <span class="hlt">Ocean</span> acidification alters chemical equilibria in seawater and thus potentially impacts marine ecosystem structure and functioning. Shelf regions play a key role for an important fraction of marine life and represent an important part of the global carbon cycle. Due to shallow <span class="hlt">water</span> depth, chemistry in the <span class="hlt">water</span> column is strongly coupled with biogeochemistry in the sediments. The aim of the present work is to investigate the impact of <span class="hlt">ocean</span> acidification on carbonate chemistry. It focuses especially on exchange fluxes of dissolved inorganic carbon (DIC), total alkalinity (TA) and calcium through the sediment-<span class="hlt">water</span> interface, and its impact on calcium carbonate precipitation or dissolution. For this purpose, sediment cores were incubated ex situ with an <span class="hlt">open</span> flow of CO2 enriched seawater for 22 days (pHT=7,4, pH reported on the total proton scale). In parallel, sediment cores were incubated as a control with untreated seawater. Incubations took place in a <span class="hlt">water</span> bath in a dark room with controlled temperature (14°C). Oxygen and pH microprofiles were recorded in the top first mm of the sediment during the whole experiment every 3 days. On 7 occasions, cores were isolated and incubated for 12 hours to estimate fluxes of DIC, TA, oxygen and nutrients. Porewater profiles of DIC, TA, calcium and nutrients were analyzed before and after incubation. On the solid phase, the content of particulate organic carbon, the C:N ratio and its isotopic δ15N and δ13C signature have been determined. In addition, total carbon contents have been measured and X-Ray diffraction was used to look for phase shifts between calcite and aragonite. A net decrease of pH was observed in the upper sediment layers, as well as an increase of DIC and TA pore <span class="hlt">water</span> concentrations. The acidified cores showed higher DIC and TA exchange</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26473861','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26473861"><span>Comparative analysis of GOCI <span class="hlt">ocean</span> color products.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Amin, Ruhul; Lewis, Mark David; Lawson, Adam; Gould, Richard W; Martinolich, Paul; Li, Rong-Rong; Ladner, Sherwin; Gallegos, Sonia</p> <p>2015-10-12</p> <p>The Geostationary <span class="hlt">Ocean</span> Color Imager (GOCI) is the first geostationary <span class="hlt">ocean</span> color sensor in orbit that provides bio-optical properties from coastal and <span class="hlt">open</span> <span class="hlt">waters</span> around the Korean Peninsula at unprecedented temporal resolution. In this study, we compare the normalized <span class="hlt">water</span>-leaving radiance (nLw) products generated by the Naval Research Laboratory Automated Processing System (APS) with those produced by the stand-alone software package, the GOCI Data Processing System (GDPS), developed by the Korean <span class="hlt">Ocean</span> Research & Development Institute (KORDI). Both results are then compared to the nLw measured by the above <span class="hlt">water</span> radiometer at the Ieodo site. This above-<span class="hlt">water</span> radiometer is part of the Aerosol Robotic NETwork (AeroNET). The results indicate that the APS and GDPS processed  correlates well within the same image slot where the coefficient of determination (r²) is higher than 0.84 for all the bands from 412 nm to 745 nm. The agreement between APS and the AeroNET data is higher when compared to the GDPS results. The Root-Mean-Squared-Error (RMSE) between AeroNET and APS data ranges from 0.24 [mW/(cm²srμm)] at 555 nm to 0.52 [mW/(cm²srμm)]  at 412 nm while RMSE between AeroNET and GDPS data ranges from 0.47 [mW/(cm²srμm)] at 443 nm to 0.69 [mW/(cm²srμm)]  at 490 nm.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4634472','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4634472"><span>Comparative Analysis of GOCI <span class="hlt">Ocean</span> Color Products</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Amin, Ruhul; Lewis, Mark David; Lawson, Adam; Gould, Richard W.; Martinolich, Paul; Li, Rong-Rong; Ladner, Sherwin; Gallegos, Sonia</p> <p>2015-01-01</p> <p>The Geostationary <span class="hlt">Ocean</span> Color Imager (GOCI) is the first geostationary <span class="hlt">ocean</span> color sensor in orbit that provides bio-optical properties from coastal and <span class="hlt">open</span> <span class="hlt">waters</span> around the Korean Peninsula at unprecedented temporal resolution. In this study, we compare the normalized <span class="hlt">water</span>-leaving radiance (nLw) products generated by the Naval Research Laboratory Automated Processing System (APS) with those produced by the stand-alone software package, the GOCI Data Processing System (GDPS), developed by the Korean <span class="hlt">Ocean</span> Research & Development Institute (KORDI). Both results are then compared to the nLw measured by the above <span class="hlt">water</span> radiometer at the Ieodo site. This above-<span class="hlt">water</span> radiometer is part of the Aerosol Robotic NETwork (AeroNET). The results indicate that the APS and GDPS processed nLw correlates well within the same image slot where the coefficient of determination (r2) is higher than 0.84 for all the bands from 412 nm to 745 nm. The agreement between APS and the AeroNET data is higher when compared to the GDPS results. The Root-Mean-Squared-Error (RMSE) between AeroNET and APS data ranges from 0.24 [mW/(cm2srμm)] at 555 nm to 0.52 [mW/(cm2srμm)] at 412 nm while RMSE between AeroNET and GDPS data ranges from 0.47 [mW/(cm2srμm)] at 443 nm to 0.69 [mW/(cm2srμm)] at 490 nm. PMID:26473861</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4052348','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4052348"><span>Moving in extreme environments: <span class="hlt">open</span> <span class="hlt">water</span> swimming in cold and warm <span class="hlt">water</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p></p> <p>2014-01-01</p> <p><span class="hlt">Open</span> <span class="hlt">water</span> swimming (OWS), either ‘wild’ such as river swimming or competitive, is a fast growing pastime as well as a part of events such as triathlons. Little evidence is available on which to base high and low <span class="hlt">water</span> temperature limits. Also, due to factors such as acclimatisation, which disassociates thermal sensation and comfort from thermal state, individuals cannot be left to monitor their own physical condition during swims. Deaths have occurred during OWS; these have been due to not only thermal responses but also cardiac problems. This paper, which is part of a series on ‘Moving in Extreme Environments’, briefly reviews current understanding in pertinent topics associated with OWS. Guidelines are presented for the organisation of <span class="hlt">open</span> <span class="hlt">water</span> events to minimise risk, and it is concluded that more information on the responses to immersion in cold and warm <span class="hlt">water</span>, the causes of the individual variation in these responses and the precursors to the cardiac events that appear to be the primary cause of death in OWS events will help make this enjoyable sport even safer. PMID:24921042</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/12396177','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/12396177"><span>Inversion of <span class="hlt">oceanic</span> constituents in case I and II <span class="hlt">waters</span> with genetic programming algorithms.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chami, Malik; Robilliard, Denis</p> <p>2002-10-20</p> <p>A stochastic inverse technique based on agenetic programming (GP) algorithm was developed toinvert <span class="hlt">oceanic</span> constituents from simulated data for case I and case II <span class="hlt">water</span> applications. The simulations were carried out with the Ordre Successifs <span class="hlt">Ocean</span> Atmosphere (OSOA) radiative transfer model. They include the effects of <span class="hlt">oceanic</span> substances such as algal-related chlorophyll, nonchlorophyllous suspended matter, and dissolved organic matter. The synthetic data set also takes into account the directional effects of particles through a variation of their phase function that makes the simulated data realistic. It is shown that GP can be successfully applied to the inverse problem with acceptable stability in the presence of realistic noise in the data. GP is compared with neural network methodology for case I <span class="hlt">waters</span>; GP exhibits similar retrieval accuracy, which is greater than for traditional techniques such as band ratio algorithms. The application of GP to real satellite data [a Sea-viewing Wide Field-of-view Sensor (SeaWiFS)] was also carried out for case I <span class="hlt">waters</span> as a validation. Good agreement was obtained when GP results were compared with the SeaWiFS empirical algorithm. For case II <span class="hlt">waters</span> the accuracy of GP is less than 33%, which remains satisfactory, at the present time, for remote-sensing purposes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1814515Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1814515Y"><span>Observed microphysical changes in Arctic mixed-phase clouds when transitioning from sea-ice to <span class="hlt">open</span> <span class="hlt">ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Young, Gillian; Jones, Hazel M.; Crosier, Jonathan; Bower, Keith N.; Darbyshire, Eoghan; Taylor, Jonathan W.; Liu, Dantong; Allan, James D.; Williams, Paul I.; Gallagher, Martin W.; Choularton, Thomas W.</p> <p>2016-04-01</p> <p>The Arctic sea-ice is intricately coupled to the atmosphere[1]. The decreasing sea-ice extent with the changing climate raises questions about how Arctic cloud structure will respond. Any effort to answer these questions is hindered by the scarcity of atmospheric observations in this region. Comprehensive cloud and aerosol measurements could allow for an improved understanding of the relationship between surface conditions and cloud structure; knowledge which could be key in validating weather model forecasts. Previous studies[2] have shown via remote sensing that cloudiness increases over the marginal ice zone (MIZ) and <span class="hlt">ocean</span> with comparison to the sea-ice; however, to our knowledge, detailed in-situ data of this transition have not been previously presented. In 2013, the Aerosol-Cloud Coupling and Climate Interactions in the Arctic (ACCACIA) campaign was carried out in the vicinity of Svalbard, Norway to collect in-situ observations of the Arctic atmosphere and investigate this issue. Fitted with a suite of remote sensing, cloud and aerosol instrumentation, the FAAM BAe-146 aircraft was used during the spring segment of the campaign (Mar-Apr 2013). One case study (23rd Mar 2013) produced excellent coverage of the atmospheric changes when transitioning from sea-ice, through the MIZ, to the <span class="hlt">open</span> <span class="hlt">ocean</span>. Clear microphysical changes were observed, with the cloud liquid-<span class="hlt">water</span> content increasing by almost four times over the transition. Cloud base, depth and droplet number also increased, whilst ice number concentrations decreased slightly. The surface warmed by ~13 K from sea-ice to <span class="hlt">ocean</span>, with minor differences in aerosol particle number (of sizes corresponding to Cloud Condensation Nuclei or Ice Nucleating Particles) observed, suggesting that the primary driver of these microphysical changes was the increased heat fluxes and induced turbulence from the warm <span class="hlt">ocean</span> surface as expected. References: [1] Kapsch, M.L., Graversen, R.G. and Tjernström, M. Springtime</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFMPP24A..09G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFMPP24A..09G"><span>Southern <span class="hlt">Ocean</span> intermediate <span class="hlt">water</span> pH information provided by modern and fossil scleraxonian deep-sea corals</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gutjahr, M.; Vance, D.; Foster, G. L.; Hillenbrand, C.; Kuhn, G.</p> <p>2010-12-01</p> <p>There is a great deal of current interest in the chemistry of the deep glacial Southern <span class="hlt">Ocean</span>, and the degree to which it communicated with the surface <span class="hlt">ocean</span> and atmosphere. Recent findings that include high surface <span class="hlt">water</span> radiocarbon ages [1] and renewed upwelling during the deglacial [2], suggest a re-organisation in Southern <span class="hlt">Ocean</span> circulation that led to the demise of a deep <span class="hlt">water</span> mass rich in dissolved inorganic carbon (DIC), leading to its renewed equilibration with the atmosphere and the deglacial rise in atmospheric CO2. However, conclusive evidence for higher Southern <span class="hlt">Ocean</span> deep <span class="hlt">water</span> DIC during the glacial is scarce, largely due to the lack of suitable substrates for recording it. Boron isotopic compositions measured in deep marine organisms may help to provide records of intermediate <span class="hlt">water</span> pH, and hence DIC changes [3]. We will present boron isotope compositions of a selection of radiocarbon-dated, calcitic, deep-sea octocorals from the Amundsen Sea sector of the Southern <span class="hlt">Ocean</span> (˜123°W, ˜69°S, 2500 m to 1430 m <span class="hlt">water</span> depth), with the aim of resolving deglacial intermediate <span class="hlt">water</span> pH changes. Since boron isotopic studies have not been carried out on these types of octocorals before, we will first present the δ11B distribution within a modern sample in order to examine biological fractionation that may potentially compromise the coral δ11B (cf. [4, 5]). Contrary to previously employed scleractinia [6], the corals analysed here appear to be internally homogenous and have only slightly elevated δ11B compared to that of ambient intermediate <span class="hlt">water</span> borate ion. Moreover, modern and early Holocene coral δ11B display fairly constant compositions, whereas deglacial coral δ11B are higher. These boron isotopic changes are accompanied by corresponding deglacial changes in the coral Nd isotopic composition (expressed in ɛNd), which has been determined on the same specimens. Together, the striking co-variation between the deep-<span class="hlt">water</span> coral δ11B and ɛNd suggest</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.8631A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.8631A"><span><span class="hlt">Open</span> Data, <span class="hlt">Open</span> Specifications and Free and <span class="hlt">Open</span> Source Software: A powerful mix to create distributed Web-based <span class="hlt">water</span> information systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Arias, Carolina; Brovelli, Maria Antonia; Moreno, Rafael</p> <p>2015-04-01</p> <p>We are in an age when <span class="hlt">water</span> resources are increasingly scarce and the impacts of human activities on them are ubiquitous. These problems don't respect administrative or political boundaries and they must be addressed integrating information from multiple sources at multiple spatial and temporal scales. Communication, coordination and data sharing are critical for addressing the <span class="hlt">water</span> conservation and management issues of the 21st century. However, different countries, provinces, local authorities and agencies dealing with <span class="hlt">water</span> resources have diverse organizational, socio-cultural, economic, environmental and information technology (IT) contexts that raise challenges to the creation of information systems capable of integrating and distributing information across their areas of responsibility in an efficient and timely manner. Tight and disparate financial resources, and dissimilar IT infrastructures (data, hardware, software and personnel expertise) further complicate the creation of these systems. There is a pressing need for distributed interoperable <span class="hlt">water</span> information systems that are user friendly, easily accessible and capable of managing and sharing large volumes of spatial and non-spatial data. In a distributed system, data and processes are created and maintained in different locations each with competitive advantages to carry out specific activities. <span class="hlt">Open</span> Data (data that can be freely distributed) is available in the <span class="hlt">water</span> domain, and it should be further promoted across countries and organizations. Compliance with <span class="hlt">Open</span> Specifications for data collection, storage and distribution is the first step toward the creation of systems that are capable of interacting and exchanging data in a seamlessly (interoperable) way. The features of Free and <span class="hlt">Open</span> Source Software (FOSS) offer low access cost that facilitate scalability and long-term viability of information systems. The World Wide Web (the Web) will be the platform of choice to deploy and access these systems</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/2013GeoRL..40.5194G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013GeoRL..40.5194G"><span>Critical role for mesoscale eddy diffusion in supplying oxygen to hypoxic <span class="hlt">ocean</span> <span class="hlt">waters</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gnanadesikan, Anand; Bianchi, Daniele; Pradal, Marie-Aude</p> <p>2013-10-01</p> <p>of the <span class="hlt">oceanic</span> lateral eddy diffusion coefficient Aredi vary by more than an order of magnitude, ranging from less than a few hundred m2/s to thousands of m2/s. This uncertainty has first-order implications for the intensity of <span class="hlt">oceanic</span> hypoxia, which is poorly simulated by the current generation of Earth System Models. Using satellite-based estimate of oxygen consumption in hypoxic <span class="hlt">waters</span> to estimate the required diffusion coefficient for these <span class="hlt">waters</span> gives a value of order 1000 m2/s. Varying Aredi across a suite of Earth System Models yields a broadly consistent result given a thermocline diapycnal diffusion coefficient of 1 × 10-5 m2/s.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFMOS51E1931C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMOS51E1931C"><span>Rolling the dice on the ice; New modes for underway data acquisition in the Arctic <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Coakley, B.; Dove, D.</p> <p>2012-12-01</p> <p>Exploration of the Arctic <span class="hlt">Ocean</span> has always depended on the sea ice. It has been a platform supporting drifting ice stations and an obstacle to be over come by force (icebreakers) or finesse (US Navy fast attack submarines). Reduced seasonal sea ice cover has made it possible to work more freely in the peripheral Arctic <span class="hlt">Ocean</span>, <span class="hlt">opening</span> relatively unknown regions to scientific exploration and study. In September 2011, the RV Marcus G. Langseth set sail from Dutch Harbor, Alaska bound through Bering Strait for the Arctic <span class="hlt">Ocean</span>. This was the first Arctic <span class="hlt">Ocean</span> trip for MGG data acquisition by a US academic research vessel since 1994, when the RV Maurice Ewing collected a 2-D MCS profile across the Bering Shelf, through the Strait and along the Beaufort Shelf, stopping near Barrow, Alaska. RV Langseth arrived on the mid-Chukchi shelf and streamed gear just south of the "Crackerjack" well, drilled by Shell Exploration in the late eighties. The ship sailed north, crossing the "Popcorn" well and then set a course to the NW, setting the baseline for the survey parallel to the Beaufort Shelf edge. Sailing through almost entirely ice-free <span class="hlt">waters</span>, approximately 5300 km of multi-channel seismic reflection data were acquired on a NW-SE oriented grid, which straddled the transition from Chukchi Shelf to the Chukchi Borderland. It would not have been possible for Langseth, which is not ice reinforced, to acquire these data prior to 2007. The dramatic expansion of late Summer <span class="hlt">open</span> <span class="hlt">water</span> in the western Arctic <span class="hlt">Ocean</span> made it possible to use this ship effectively across a broad swath of the shelf and the periphery of the deep central basin. While the survey region was almost entirely ice free during this cruise, which straddled the ice minimum for 2011, it was not possible to predict this a priori, despite expectations set by the previous five years of ice edge retreat. For this reason, the Canadian Ice Service was engaged to provide interpreted ice imagery, multiple times per day</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.B22C..06C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.B22C..06C"><span><span class="hlt">Ocean</span> Fertilization and <span class="hlt">Ocean</span> Acidification</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cao, L.; Caldeira, K.</p> <p>2008-12-01</p> <p> aragonite is 8.18 and 3.5). As a result of <span class="hlt">ocean</span> fertilization, 10 years from now, the depth of saturation horizon (the depth below which <span class="hlt">ocean</span> <span class="hlt">water</span> is undersaturated with respect to calcium carbonate) for aragonite in the Southern <span class="hlt">Ocean</span> shoals from its present average value of about 700 m to 100 m. In contrast, no significant change in the depth of aragonite saturation horizontal is seen in the scenario without fertilization for the corresponding period. By year 2100, global mean calcite saturation horizon shoals from its present value of 3150 m to 2965 and 2534 m in the case without fertilization and with it. In contrast, if the sale of carbon credits from <span class="hlt">ocean</span> fertilization leads to greater CO2 emissions to the atmosphere (e.g., if carbon credits from <span class="hlt">ocean</span> fertilization are used to offset CO2 emissions from a coal plant), then there is the potential that <span class="hlt">ocean</span> fertilization would further acidify the deep <span class="hlt">ocean</span> without conferring any chemical benefit to surface <span class="hlt">ocean</span> <span class="hlt">waters</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMIN44A..06B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMIN44A..06B"><span>Addressing <span class="hlt">Open</span> <span class="hlt">Water</span> Data Challenges in the Bureau of Reclamation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brekke, L. D.; Danner, A.; Nagode, J.; Rocha, J.; Poulton, S.; Anderson, A.</p> <p>2017-12-01</p> <p>The Bureau of Reclamation is largest wholesaler of <span class="hlt">water</span> in the United States. Located in the 17 western states, Reclamation serves <span class="hlt">water</span> to 31 million people, provides irrigated <span class="hlt">water</span> to 20 percent of Western farmers, and is the second largest producer of hydroelectric power in the United States. Through these activities, Reclamation generates large amounts of <span class="hlt">water</span> and <span class="hlt">water</span>-related data, describing reservoirs and river system conditions, hydropower, environmental compliance activities, infrastructure assets, and other aspects of Reclamation's mission activities. Reclamation aims to make <span class="hlt">water</span> and <span class="hlt">water</span>-related data sets more easily found, accessed, and used in decision-making activities in order to benefit the public, private sector, and research communities. Historically, there has not been an integrated, bureau-wide system to store data in machine-readable formats; nor a system to permit centralized browsing, <span class="hlt">open</span> access, and web-services. Reclamation began addressing these limitations by developing the Reclamation <span class="hlt">Water</span> Information System (RWIS), released in Spring 2017 (https://<span class="hlt">water</span>.usbr.gov/). A bureau-wide team contributed to RWIS development, including <span class="hlt">water</span> data stewards, database administrators, and information technology (IT) specialists. The first RWIS release publishes reservoir time series data from Reclamation's five regions and includes a map interface for sites identification, a query interface for data discovery and access, and web-services for automated retrieval. As RWIS enhancement continues, the development team is developing a companion system - the Reclamation Information Sharing Environment (RISE) - to provide access to the other data subjects and types (geospatial, documents). While RWIS and RISE are promising starts, Reclamation continues to face challenges in addressing <span class="hlt">open</span> <span class="hlt">water</span> data goals: making data consolidation and <span class="hlt">open</span> publishing a value-added activity for programs that publish data locally, going beyond providing <span class="hlt">open</span> access</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018Geote..52..173M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018Geote..52..173M"><span>Tectono-Magmatic Evolution of the South Atlantic Continental Margins with Respect to <span class="hlt">Opening</span> of the <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Melankholina, E. N.; Sushchevskaya, N. M.</p> <p>2018-03-01</p> <p>The history of the <span class="hlt">opening</span> of the South Atlantic in Early Cretaceous time is considered. It is shown that the determining role for continental breakup preparation has been played by tectono-magmatic events within the limits of the distal margins that developed above the plume head. The formation of the Rio Grande Rise-Walvis Ridge volcanic system along the trace of the hot spot is considered. The magmatism in the South Atlantic margins, its sources, and changes in composition during the evolution are described. On the basis of petrogeochemical data, the peculiarities of rocks with a continental signature are shown. Based on Pb-Sr-Nd isotopic studies, it is found that the manifestations of magmatism in the proximal margins had features of enriched components related to the EM I and EM II sources, sometimes with certain participation of the HIMU source. Within the limits of the Walvis Ridge, as magmatism expanded to the newly formed <span class="hlt">oceanic</span> crust, the participation of depleted asthenospheric mantle became larger in the composition of magmas. The role played by the Tristan plume in magma generation is discussed: it is the most considered as the heat source that determined the melting of the ancient enriched lithosphere. The specifics of the tectono-magmatic evolution of the South Atlantic is pointed out: the origination during spreading of a number of hot spots above the periphery of the African superplume. The diachronous character of the <span class="hlt">opening</span> of the <span class="hlt">ocean</span> is considered in the context of northward progradation of the breakup line and its connection with the northern branch of the Atlantic <span class="hlt">Ocean</span> in the Mid-Cretaceous.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15898670','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15898670"><span>Instrumenting free-swimming dolphins echolocating in <span class="hlt">open</span> <span class="hlt">water</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Martin, Stephen W; Phillips, Michael; Bauer, Eric J; Moore, Patrick W; Houser, Dorian S</p> <p>2005-04-01</p> <p>Dolphins within the Navy Marine Mammal Program use echolocation to effectively locate underwater mines. They currently outperform manmade systems at similar tasks, particularly in cluttered environments and on buried targets. In hopes of improving manmade mine-hunting sonar systems, two instrumentation packages were developed to monitor free-swimming dolphin motion and echolocation during <span class="hlt">open-water</span> target detection tasks. The biosonar measurement tool (BMT) is carried by a dolphin and monitors underwater position and attitude while simultaneously recording echolocation clicks and returning echoes through high-gain binaural receivers. The instrumented mine simulator (IMS) is a modified bottom target that monitors echolocation signals arriving at the target during ensonification. Dolphin subjects were trained to carry the BMT in <span class="hlt">open</span>-bay bottom-object target searches in which the IMS could serve as a bottom object. The instrumentation provides detailed data that reveal hereto-unavailable information on the search strategies of free-swimming dolphins conducting <span class="hlt">open-water</span>, bottom-object search tasks with echolocation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005ASAJ..117.2301M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005ASAJ..117.2301M"><span>Instrumenting free-swimming dolphins echolocating in <span class="hlt">open</span> <span class="hlt">water</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Martin, Stephen W.; Phillips, Michael; Bauer, Eric J.; Moore, Patrick W.; Houser, Dorian S.</p> <p>2005-04-01</p> <p>Dolphins within the Navy Marine Mammal Program use echolocation to effectively locate underwater mines. They currently outperform manmade systems at similar tasks, particularly in cluttered environments and on buried targets. In hopes of improving manmade mine-hunting sonar systems, two instrumentation packages were developed to monitor free-swimming dolphin motion and echolocation during <span class="hlt">open-water</span> target detection tasks. The biosonar measurement tool (BMT) is carried by a dolphin and monitors underwater position and attitude while simultaneously recording echolocation clicks and returning echoes through high-gain binaural receivers. The instrumented mine simulator (IMS) is a modified bottom target that monitors echolocation signals arriving at the target during ensonification. Dolphin subjects were trained to carry the BMT in <span class="hlt">open</span>-bay bottom-object target searches in which the IMS could serve as a bottom object. The instrumentation provides detailed data that reveal hereto-unavailable information on the search strategies of free-swimming dolphins conducting <span class="hlt">open-water</span>, bottom-object search tasks with echolocation. .</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009ECSS...85...12C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009ECSS...85...12C"><span>The divergent environmental characteristics of permanently-<span class="hlt">open</span>, seasonally-<span class="hlt">open</span> and normally-closed estuaries of south-western Australia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chuwen, Benjamin M.; Hoeksema, Steeg D.; Potter, Ian C.</p> <p>2009-10-01</p> <p>This study has compared the environmental characteristics of the basins and saline lower reaches of the tributaries of eight estuaries on the south coast of Western Australia, which differ in their degree of connectivity with the <span class="hlt">ocean</span>. Although four estuaries between 115.1° and 121.8° E along that coast remain permanently <span class="hlt">open</span> to the <span class="hlt">ocean</span>, the others only become <span class="hlt">open</span> when the volume of river discharge is sufficient to breach the prominent sand bars at their mouths, which occurs annually following heavy winter and early spring rainfall in some estuaries (seasonally <span class="hlt">open</span>) and infrequently in others (normally closed). Estuaries to the west of 118.5° E are predominantly permanently <span class="hlt">open</span>, e.g. Oyster Harbour, or seasonally <span class="hlt">open</span>, e.g. Broke, Irwin and Wilson inlets, whereas those further east, e.g. Wellstead Estuary and Hamersley, Culham and Stokes inlets, where annual rainfall and thus discharge are much lower, only become <span class="hlt">open</span> after exceptionally heavy discharge. In permanently and seasonally-<span class="hlt">open</span> estuaries, pronounced haloclines and oxyclines are present in the narrow rivers but not the wide basins where the <span class="hlt">waters</span> are subjected to wind-driven mixing. The extent of cyclical seasonal fluctuations in environmental conditions differed markedly among the three seasonally-<span class="hlt">open</span> estuaries and between years in one of those systems. These differences reflected variations in the relationship between the volume of fluvial discharge, which is determined by a combination of the amount of local rainfall, catchment size and extent of clearing of native vegetation, and the amount of intrusion by marine <span class="hlt">waters</span>, which is largely controlled by the size and duration of the <span class="hlt">opening</span> of the estuary mouth. The mean seasonal salinities in the basins of the three normally-closed estuaries increased over three years of very low rainfall to 64 in the deepest of these estuaries (Stokes Inlet) to 145 in Hamersley Inlet and to 296 in the shallowest estuary (Culham Inlet). These results</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4801293','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4801293"><span>Insights into global diatom distribution and diversity in the world’s <span class="hlt">ocean</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>Malviya, Shruti; Scalco, Eleonora; Audic, Stéphane; Vincent, Flora; Veluchamy, Alaguraj; Poulain, Julie; Wincker, Patrick; Iudicone, Daniele; de Vargas, Colomban; Bittner, Lucie; Zingone, Adriana; Bowler, Chris</p> <p>2016-01-01</p> <p>Diatoms (Bacillariophyta) constitute one of the most diverse and ecologically important groups of phytoplankton. They are considered to be particularly important in nutrient-rich coastal ecosystems and at high latitudes, but considerably less so in the oligotrophic <span class="hlt">open</span> <span class="hlt">ocean</span>. The Tara <span class="hlt">Oceans</span> circumnavigation collected samples from a wide range of <span class="hlt">oceanic</span> regions using a standardized sampling procedure. Here, a total of ∼12 million diatom V9-18S ribosomal DNA (rDNA) ribotypes, derived from 293 size-fractionated plankton communities collected at 46 sampling sites across the global <span class="hlt">ocean</span> euphotic zone, have been analyzed to explore diatom global diversity and community composition. We provide a new estimate of diversity of marine planktonic diatoms at 4,748 operational taxonomic units (OTUs). Based on the total assigned ribotypes, Chaetoceros was the most abundant and diverse genus, followed by Fragilariopsis, Thalassiosira, and Corethron. We found only a few cosmopolitan ribotypes displaying an even distribution across stations and high abundance, many of which could not be assigned with confidence to any known genus. Three distinct communities from South Pacific, Mediterranean, and Southern <span class="hlt">Ocean</span> <span class="hlt">waters</span> were identified that share a substantial percentage of ribotypes within them. Sudden drops in diversity were observed at Cape Agulhas, which separates the Indian and Atlantic <span class="hlt">Oceans</span>, and across the Drake Passage between the Atlantic and Southern <span class="hlt">Oceans</span>, indicating the importance of these <span class="hlt">ocean</span> circulation choke points in constraining diatom distribution and diversity. We also observed high diatom diversity in the <span class="hlt">open</span> <span class="hlt">ocean</span>, suggesting that diatoms may be more relevant in these <span class="hlt">oceanic</span> systems than generally considered. PMID:26929361</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP34A..06D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP34A..06D"><span>Meridional contrasts in productivity changes driven by the Cenozoic <span class="hlt">opening</span> of Drake Passage</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Donnadieu, Y.; Ladant, J. B.; Bopp, L.; Wilson, P. A.; Lear, C. H.</p> <p>2017-12-01</p> <p>The progressive <span class="hlt">opening</span> of Drake Passage across the Eocene and the Oligocene occurs contemporaneously to the long-term global cooling of the late Eocene, which culminated with the Eocene-Oligocene glaciation of Antarctica. Atmospheric pCO2 decline during the late Eocene is thought to have played a major role in the climatic shifts of the Eocene-Oligocene boundary, yet reasons behind CO2 variations remain obscure. Changes in marine productivity affecting the biological <span class="hlt">oceanic</span> carbon pump represent a possible cause. Here, we explore whether and how the <span class="hlt">opening</span> of Drake Passage may have affected the marine biogeochemistry, and in particular paleoproductivity changes, with the use of a fully coupled atmosphere-<span class="hlt">ocean</span>-biogeochemical model (IPSL-CM5A). We find that the simulated changes to Drake Passage <span class="hlt">opening</span> exhibit a uniform decrease in the low latitudes while the high latitude response is more spatially heterogeneous. Mechanistically, the low latitude productivity decrease is a consequence of the dramatic reorganization of the <span class="hlt">ocean</span> circulation when Drake Passage <span class="hlt">opens</span>, as the shift from a well ventilated to a swampier <span class="hlt">ocean</span> drives nutrient depletion in the low latitudes. In the high latitudes, the onset of the Antarctic Circumpolar Current in the model exerts a strong control both on nutrient availability but also on regions of deep <span class="hlt">water</span> formation, which results in non-uniform patterns of productivity change in the Southern <span class="hlt">Ocean</span>. The qualitative agreement between geographically diverse long-term paleoproductivity records and the simulated variations suggests that the <span class="hlt">opening</span> of Drake Passage may contribute to part of the long-term paleoproductivity signal recorded in the data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20030064112&hterms=impacts+ocean&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dimpacts%2Bocean','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20030064112&hterms=impacts+ocean&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dimpacts%2Bocean"><span>Ejecta from <span class="hlt">Ocean</span> Impacts</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kyte, Frank T.</p> <p>2003-01-01</p> <p>Numerical simulations of deep-<span class="hlt">ocean</span> impact provide some limits on the size of a projectile that will not mix with the <span class="hlt">ocean</span> floor during a deep-<span class="hlt">ocean</span> impact. For a vertical impact at asteroidal velocities (approx. 20 km/s), mixing is only likely when the projectile diameter is greater than 112 of the <span class="hlt">water</span> depth. For oblique impacts, even larger projectiles will not mix with <span class="hlt">ocean</span> floor silicates. Given the typical <span class="hlt">water</span> depths of 4 to 5 km in deep-<span class="hlt">ocean</span> basins, asteroidal projectiles with diameters as large as 2 or 3 km may commonly produce silicate ejecta that is composed only of meteoritic materials and seawater salts. However, the compressed <span class="hlt">water</span> column beneath the projectile can still disrupt and shock metamorphose the <span class="hlt">ocean</span> floor. Therefore, production of a separate, terrestrial ejecta component is not ruled out in the most extreme case. With increasing projectile size (or energy) relative to <span class="hlt">water</span> depths, there must be a gradation between <span class="hlt">oceanic</span> impacts and more conventional continental impacts. Given that 60% of the Earth's surface is covered by <span class="hlt">oceanic</span> lithosphere and 500 m projectiles impact the Earth on 10(exp 5) y timescales, there must be hundreds of <span class="hlt">oceanic</span> impact deposits in the sediment record awaiting discovery.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T54B..01K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T54B..01K"><span><span class="hlt">Opening</span> of the Central Atlantic <span class="hlt">Ocean</span>: Implications for Geometric Rifting and Asymmetric Initial Seafloor Spreading after Continental Breakup</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Klingelhoefer, F.; Biari, Y.; Sahabi, M.; Funck, T.; Benabdellouahed, M.; Schnabel, M.; Reichert, C. J.; Gutscher, M. A.; Bronner, A.; Austin, J. A., Jr.</p> <p>2017-12-01</p> <p>The structure of conjugate passive margins provides information about rifting styles, the initial phases of the <span class="hlt">opening</span> of an <span class="hlt">ocean</span> and the formation of its associated sedimentary basins. The study of the deep structure of conjugate passive continental margins combined with precise plate kinematic reconstructions can provide constraints on the mechanisms of rifting and formation of initial <span class="hlt">oceanic</span> crust. In this study the Central Atlantic conjugate margins are compared, based on compilation of wide-angle seismic profiles from the NW-Africa Nova Scotian and US passive margins. Plate cinematic reconstructions were used to place the profiles in the position at <span class="hlt">opening</span> and at the M25 magnetic anomaly. The patterns of volcanism, crustal thickness, geometry, and seismic velocities in the transition zone. suggest symmetric rifting followed by asymmetric <span class="hlt">oceanic</span> crustal accretion. Conjugate profiles in the southern Central Atlantic image differences in the continental crustal thickness. While profiles on the eastern US margin are characterized by thick layers of magmatic underplating, no such underplate was imaged along the NW-African continental margin. It has been proposed that these volcanic products form part of the CAMP (Central Atlantic Magmatic Province). In the north, two wide-angle seismic profiles acquired in exactly conjugate positions show that the crustal geometry of the unthinned continental crust and the necking zone are nearly symmetric. A region including seismic velocities too high to be explained by either continental or <span class="hlt">oceanic</span> crust is imaged along the Nova Scotia margin off Eastern Canada, corresponding on the African side to an <span class="hlt">oceanic</span> crust with slightly elevated velocities. These might result from asymmetric spreading creating seafloor by faulting the existing lithosphere on the Canadian side and the emplacement of magmatic <span class="hlt">oceanic</span> crust including pockets of serpentinite on the Moroccan margin. A slightly elevated crustal thickness along the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008PhDT........55Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008PhDT........55Y"><span><span class="hlt">Water</span> mass formation and circulation in the Persian Gulf and <span class="hlt">water</span> exchange with the Indian <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yao, Fengchao</p> <p></p> <p>The Persian Gulf is a shallow, semi-enclosed marginal sea where the Persian Gulf <span class="hlt">Water</span> (PGW), one of the most saline <span class="hlt">water</span> masses in the world, is formed due to the arid climate. The PGW flushes out of the Persian Gulf as a deep outflow and induces a surface inflow of the Indian <span class="hlt">Ocean</span> Surface <span class="hlt">Water</span> (IOSW), driving an inverse-estuarine type <span class="hlt">water</span> exchange through the Strait of Hormuz. In this dissertation, the circulation and <span class="hlt">water</span> mass transformation processes in the Persian Gulf and the <span class="hlt">water</span> exchange with the Indian <span class="hlt">Ocean</span> through the Strait of Hormuz, in response to the atmospheric forcing, are studied using the HYbrid Coordinate <span class="hlt">Ocean</span> Model (HYCOM). The model is driven by surface wind stress, heat and fresh <span class="hlt">water</span> fluxes derived from two sources: the COADS (Comprehensive <span class="hlt">Ocean</span>-Atmosphere Data Set) monthly climatology and high frequency (2-hourly) MM5 (The Fifth-Generation NCAR/Penn State Mesoscale Model) output. This study is motivated by the time series measurements in the Strait during December 1996 to March 1998 by Johns et al. (2003), which also serve as a major benchmark for evaluating the model results. The simulations with climatological forcing show that the IOSW propagates in two branches into the Gulf, one along the Iranian coast toward the northern gulf and the other one onto the southern banks driven by the Ekman drift by the prevailing northwesterly winds. These two branches of inflow form two cyclonic gyres in the northern and in the southern gulf respectively. Cold, saline deep <span class="hlt">waters</span> are formed both in the northern gulf and in the southern gulf during the wintertime cooling period and their exports contribute seasonally to the outflow in the strait. After formation in winter, the dense <span class="hlt">water</span> in the shallow southwestern gulf spills off into the strait and causes high-salinity pulses in the outflow in the strait, a phenomenon also present in the observations. The export of dense <span class="hlt">waters</span> from the northern gulf persists throughout the year, with the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/11002893','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/11002893"><span>Ultraviolet radiation and the photobiology of earth's early <span class="hlt">oceans</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Cockell, C S</p> <p>2000-10-01</p> <p>During the Archean era (3.9-2.5 Ga ago) the earth was dominated by an <span class="hlt">oceanic</span> lithosphere. Thus, understanding how life arose and persisted in the Archean <span class="hlt">oceans</span> constitutes a major challenge in understanding early life on earth. Using a radiative transfer model of the late Archean <span class="hlt">oceans</span>, the photobiological environment of the photic zone and the surface microlayer is explored at the time before the formation of a significant ozone column. DNA damage rates might have been approximately three orders of magnitude higher in the surface layer of the Archean <span class="hlt">oceans</span> than on the present-day <span class="hlt">oceans</span>, but at 30 m depth, damage may have been similar to the surface of the present-day <span class="hlt">oceans</span>. However at this depth the risk of being transported to surface <span class="hlt">waters</span> in the mixed layer was high. The mixed layer may have been inhabited by a low diversity UV-resistant biota. But it could have been numerically abundant. Repair capabilities similar to Deinococcus radiodurans would be sufficient to survive in the mixed layer. Diversity may have been greater in the region below the mixed layer and above the light compensation point corresponding to today's 'deep chlorophyll maximum'. During much of the Archean the air-<span class="hlt">water</span> interface was probably an uninhabitable extreme environment for neuston. The habitability of some regions of the photic zone is consistent with the evidence embodied in the geologic record, which suggests an oxygenated upper layer in the Archean <span class="hlt">oceans</span>. During the early Proterozoic, as ozone concentrations increased to a column abundance above 1 x 10(17) cm-2, UV stress would have been reduced and possibly a greater diversity of organisms could have inhabited the mixed layer. However, nutrient upwelling from newly emergent continental crusts may have been more significant in increasing total planktonic abundance in the <span class="hlt">open</span> <span class="hlt">oceans</span> and coastal regions than photobiological factors. The phohobiological environment of the Archean <span class="hlt">oceans</span> has implications for the potential</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4585736','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4585736"><span>Fast Episodes of West-Mediterranean-Tyrrhenian <span class="hlt">Oceanic</span> <span class="hlt">Opening</span> and Revisited Relations with Tectonic Setting</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Savelli, Carlo</p> <p>2015-01-01</p> <p>Extension and calc-alkaline volcanism of the submerged orogen of alpine age (OAA) initiated in Early Oligocene (~33/32 Ma) and reached the stage of <span class="hlt">oceanic</span> <span class="hlt">opening</span> in Early-Miocene (Burdigalian), Late-Miocene and Late-Pliocene. In the Burdigalian (~20–16 Ma) period of widespread volcanism of calcalkaline type on the margins of <span class="hlt">oceanic</span> domain, seafloor spreading originated the deep basins of north Algeria (western part of OAA) and Sardinia/Provence (European margin). Conversely, when conjugate margins’ volcanism has been absent or scarce seafloor spreading formed the plains Vavilov (7.5–6.3 Ma) and Marsili (1.87–1.67 Ma) within OAA eastern part (Tyrrhenian Sea). The contrast between occurrence and lack of margin’s igneous activity probably implies the diversity of the geotectonic setting at the times of <span class="hlt">oceanization</span>. It appears that the Burdigalian calcalkaline volcanism on the continental margins developed in the absence of subduction. The WNW-directed subduction of African plate probably commenced at ~16/15 Ma (waning Burdigalian seafloor spreading) after ~18/16 Ma of rifting. Space-time features indicate that calcalkaline volcanism is not linked only to subduction. From this view, temporal gap would exist between the steep subduction beneath the Apennines and the previous, flat-type plunge of European plate with opposite direction producing the OAA accretion and double vergence. PMID:26391973</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003ASAJ..113.2191O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003ASAJ..113.2191O"><span>Frechet derivatives for shallow <span class="hlt">water</span> <span class="hlt">ocean</span> acoustic inverse problems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Odom, Robert I.</p> <p>2003-04-01</p> <p>For any inverse problem, finding a model fitting the data is only half the problem. Most inverse problems of interest in <span class="hlt">ocean</span> acoustics yield nonunique model solutions, and involve inevitable trade-offs between model and data resolution and variance. Problems of uniqueness and resolution and variance trade-offs can be addressed by examining the Frechet derivatives of the model-data functional with respect to the model variables. Tarantola [Inverse Problem Theory (Elsevier, Amsterdam, 1987), p. 613] published analytical formulas for the basic derivatives, e.g., derivatives of pressure with respect to elastic moduli and density. Other derivatives of interest, such as the derivative of transmission loss with respect to attenuation, can be easily constructed using the chain rule. For a range independent medium the analytical formulas involve only the Green's function and the vertical derivative of the Green's function for the medium. A crucial advantage of the analytical formulas for the Frechet derivatives over numerical differencing is that they can be computed with a single pass of any program which supplies the Green's function. Various derivatives of interest in shallow <span class="hlt">water</span> <span class="hlt">ocean</span> acoustics are presented and illustrated by an application to the sensitivity of measured pressure to shallow <span class="hlt">water</span> sediment properties. [Work supported by ONR.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA01799.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA01799.html"><span>Space Radar Image of North Atlantic <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>1999-04-15</p> <p>This is a radar image showing surface features on the <span class="hlt">open</span> <span class="hlt">ocean</span> in the northeast Atlantic <span class="hlt">Ocean</span>. There is no land mass in this image. The purple line in the lower left of the image is the stern wake of a ship. The ship creating the wake is the bright white spot on the middle, left side of the image. The ship's wake is about 28 kilometers (17 miles) long in this image and investigators believe that is because the ship may be discharging oil. The oil makes the wake last longer and causes it to stand out in this radar image. A fairly sharp boundary or front extends from the lower left to the upper right corner of the image and separates two distinct <span class="hlt">water</span> masses that have different temperatures. The different <span class="hlt">water</span> temperature affects the wind patterns on the <span class="hlt">ocean</span>. In this image, the light green area depicts rougher <span class="hlt">water</span> with more wind, while the purple area is calmer <span class="hlt">water</span> with less wind. The dark patches are smooth areas of low wind, probably related to clouds along the front, and the bright green patches are likely due to ice crystals in the clouds that scatter the radar waves. The overall "fuzzy" look of this image is caused by long <span class="hlt">ocean</span> waves, also called swells. <span class="hlt">Ocean</span> radar imagery allows the fine detail of <span class="hlt">ocean</span> features and interactions to be seen, such as the wake, swell, <span class="hlt">ocean</span> front and cloud effects, which can then be used to enhance the understanding of <span class="hlt">ocean</span> dynamics on smaller and smaller scales. The image is centered at 42.8 degrees north latitude, 26.2 degrees west longitude and shows an area approximately 35 kilometers by 65 kilometers (22 by 40 miles). The colors in the image are assigned to different frequencies and polarizations of the radar as follows: red is L-band horizontally transmitted, horizontally received; green is C-band horizontally transmitted, horizontally received; blue is L-band vertically transmitted, vertically received. This image was acquired by the Spaceborne Imaging Radar-C/X-band Synthetic Aperture Radar (SIR</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19900055325&hterms=relationship+form&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Drelationship%2Bform','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19900055325&hterms=relationship+form&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Drelationship%2Bform"><span>On the relationship between <span class="hlt">water</span> vapor over the <span class="hlt">oceans</span> and sea surface temperature</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Stephens, Graeme L.</p> <p>1990-01-01</p> <p>Monthly mean precipitable <span class="hlt">water</span> data obtained from passive microwave radiometry were correlated with the National Meteorological Center (NMC) blended sea surface temperature data. It is shown that the monthly mean <span class="hlt">water</span> vapor content of the atmosphere above the <span class="hlt">oceans</span> can generally be prescribed from the sea surface temperature with a standard deviation of 0.36 g/sq cm. The form of the relationship between precipitable <span class="hlt">water</span> and sea surface temperature in the range T (sub s) greater than 18 C also resembles that predicted from simple arguments based on the Clausius-Clapeyron relationship. The annual cycle of the globally integrated mass of Scanning Multichannel Microwave Radiometer (SMMR) <span class="hlt">water</span> vapor is shown to differ from analyses of other <span class="hlt">water</span> vapor data in both phase and amplitude and these differences point to a significant influence of the continents on <span class="hlt">water</span> vapor. Regional scale analyses of <span class="hlt">water</span> vapor demonstrate that monthly averaged <span class="hlt">water</span> vapor data, when contrasted with the bulk sea surface temperature relationship developed in this study, reflect various known characteristics of the time mean large-scale circulation over the <span class="hlt">oceans</span>. A <span class="hlt">water</span> vapor parameter is introduced to highlight the effects of large-scale motion on atmospheric <span class="hlt">water</span> vapor. Based on the magnitude of this parameter, it is shown that the effects of large-scale flow on precipitable <span class="hlt">water</span> vapor are regionally dependent, but for the most part, the influence of circulation is generally less than about + or - 20 percent of the seasonal mean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19900008811','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19900008811"><span>On the relationship between <span class="hlt">water</span> vapor over the <span class="hlt">oceans</span> and sea surface temperature</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Stephens, Graeme L.</p> <p>1989-01-01</p> <p>Monthly mean precipitable <span class="hlt">water</span> data obtained from passive microwave radiometry were correlated with the National Meteorological Center (NMC) blended sea surface temperature data. It is shown that the monthly mean <span class="hlt">water</span> vapor content of the atmosphere above the <span class="hlt">oceans</span> can generally be prescribed from the sea surface temperature with a standard deviation of 0.36 g/sq cm. The form of the relationship between precipitable <span class="hlt">water</span> and sea surface temperature in the range T(sub s) greater than 18 C also resembles that predicted from simple arguments based on the Clausius-Clapeyron relationship. The annual cycle of the globally integrated mass of Scanning Multichannel Microwave Radiometer (SMMR) <span class="hlt">water</span> vapor is shown to differ from analyses of other <span class="hlt">water</span> vapor data in both phase and amplitude and these differences point to a significant influence of the continents on <span class="hlt">water</span> vapor. Regional scale analyses of <span class="hlt">water</span> vapor demonstrate that monthly averaged <span class="hlt">water</span> vapor data, when contrasted with the bulk sea surface temperature relationship developed in this study, reflect various known characteristics of the time mean large-scale circulation over the <span class="hlt">oceans</span>. A <span class="hlt">water</span> vapor parameter is introduced to highlight the effects of large-scale motion on atmospheric <span class="hlt">water</span> vapor. Based on the magnitude of this parameter, it is shown that the effects of large-scale flow on precipitable <span class="hlt">water</span> vapor are regionally dependent, but for the most part, the influence of circulation is generally less than about + or - 20 percent of the seasonal mean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26723303','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26723303"><span><span class="hlt">Ocean</span> acoustic reverberation tomography.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Dunn, Robert A</p> <p>2015-12-01</p> <p>Seismic wide-angle imaging using ship-towed acoustic sources and networks of <span class="hlt">ocean</span> bottom seismographs is a common technique for exploring earth structure beneath the <span class="hlt">oceans</span>. In these studies, the recorded data are dominated by acoustic waves propagating as reverberations in the <span class="hlt">water</span> column. For surveys with a small receiver spacing (e.g., <10 km), the acoustic wave field densely samples properties of the <span class="hlt">water</span> column over the width of the receiver array. A method, referred to as <span class="hlt">ocean</span> acoustic reverberation tomography, is developed that uses the travel times of direct and reflected waves to image <span class="hlt">ocean</span> acoustic structure. Reverberation tomography offers an alternative approach for determining the structure of the <span class="hlt">oceans</span> and advancing the understanding of <span class="hlt">ocean</span> heat content and mixing processes. The technique has the potential for revealing small-scale <span class="hlt">ocean</span> thermal structure over the entire vertical height of the <span class="hlt">water</span> column and along long survey profiles or across three-dimensional volumes of the <span class="hlt">ocean</span>. For realistic experimental geometries and data noise levels, the method can produce images of <span class="hlt">ocean</span> sound speed on a smaller scale than traditional acoustic tomography.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_19 --> <div id="page_20" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="381"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20040000500','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20040000500"><span>Algorithms for <span class="hlt">Ocean</span> Bottom Albedo Determination from In-<span class="hlt">Water</span> Natural Light Measurements</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Leathers, Robert A.; McCormick, Normal J.</p> <p>1999-01-01</p> <p>A method for determining <span class="hlt">ocean</span> bottom optical albedo, R-sub b, from in-<span class="hlt">water</span> upward and downward irradiance measurements at a shallow site is presented, tested, and compared with a more familiar approach that requires additional measurements at a nearby deep-<span class="hlt">water</span> site. Also presented are two new algorithms for the estimation of R-sub b from measurements of the downward irradiance and vertically upward radiance.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?direntryid=337050','PESTICIDES'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?direntryid=337050"><span>Assessment of the urban <span class="hlt">water</span> system with an <span class="hlt">open</span> ...</span></a></p> <p><a target="_blank" href="http://www.epa.gov/pesticides/search.htm">EPA Pesticide Factsheets</a></p> <p></p> <p></p> <p>Urban <span class="hlt">water</span> systems convey complex environmental and man-made flows. The relationships among <span class="hlt">water</span> flows and networked storages remains difficult to comprehensively evaluate. Such evaluation is important, however, as interventions are designed (e.g, conservation measures, green infrastructure) to modify specific flows of urban <span class="hlt">water</span> (e.g. drinking <span class="hlt">water</span>, stormwater) that may have systemic effects. We have developed a general model that specifies the relationships among urban <span class="hlt">water</span> system components, and a set of tools for evaluating the model for any city as the R package City<span class="hlt">Water</span>Balance. City<span class="hlt">Water</span>Balance provides a reproducible workflow for assessing urban <span class="hlt">water</span> system(s) by facilitating the retrieval of <span class="hlt">open</span> data, largely via web services, and analysis of these data using <span class="hlt">open</span>-source R functions. It allows the user to 1) quickly assemble a quantitative, unified picture of flows thorough an urban area, and 2) easily change the spatial and temporal boundaries of analysis to match scales relevant to local decision-making. We used City<span class="hlt">Water</span>Balance to evaluate the <span class="hlt">water</span> system in the Chicago metropolitan area on a monthly basis for <span class="hlt">water</span> years 2001-2010. Results, including the relative magnitudes and temporal variability of major <span class="hlt">water</span> flows in greater Chicago, are used to consider 1) trade-offs associated with management alternatives for stormwater and combined sewer overflows and 2) the significance of future changes in precipitation, which is the largest</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005E%26PSL.236..705P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005E%26PSL.236..705P"><span>Neodymium isotope evolution of NW Tethyan upper <span class="hlt">ocean</span> <span class="hlt">waters</span> throughout the Cretaceous</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pucéat, Emmanuelle; Lécuyer, Christophe; Reisberg, Laurie</p> <p>2005-08-01</p> <p>Neodymium isotope compositions of twenty-four fish teeth, nineteen from the NW Tethys and five from different locations within the Tethys, are interpreted to reflect the evolution of Tethyan upper <span class="hlt">ocean</span> <span class="hlt">water</span> composition during the Cretaceous and used to track changes in erosional inputs to the NW Tethys and in <span class="hlt">oceanic</span> circulation throughout the Cretaceous. The rather high ɛNd (up to - 7.6) of the NW Tethyan upper <span class="hlt">ocean</span> <span class="hlt">waters</span> recorded from the Late Berriasian to the Early Aptian and the absence of negative excursions during this interval support the presence of a permanent westward flowing Tethys Circumglobal Current (TCC). This implies that temperature variations during this time period, inferred from the oxygen isotope analysis of fish tooth enamel, were not driven by changes in surface <span class="hlt">oceanic</span> currents, but rather by global climatic changes. The results presented here represent a significant advance over previously published Cretaceous seawater Nd isotope records. Our newly acquired data now allow the identification of two stages of low ɛNd values in the NW Tethys, during the Early Albian-Middle Albian interval (down to - 10) and the Santonian-Early Campanian (down to - 11.4), which alternate with two stages of higher ɛNd values (up to - 9) during the Late Albian-Turonian interval and the Maastrichtian. Used in conjunction with the oxygen isotope record, the fluctuations of ɛNd values can be related to major climatic, oceanographic, and tectonic events that appeared in the western Tethyan domain.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.4537T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.4537T"><span>Contrasting sea-ice and <span class="hlt">open-water</span> boundary layers during melt and freeze-up seasons: Some result from the Arctic Clouds in Summer Experiment.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tjernström, Michael; Sotiropoulou, Georgia; Sedlar, Joseph; Achtert, Peggy; Brooks, Barbara; Brooks, Ian; Persson, Ola; Prytherch, John; Salsbury, Dominic; Shupe, Matthew; Johnston, Paul; Wolfe, Dan</p> <p>2016-04-01</p> <p>With more <span class="hlt">open</span> <span class="hlt">water</span> present in the Arctic summer, an understanding of atmospheric processes over <span class="hlt">open-water</span> and sea-ice surfaces as summer turns into autumn and ice starts forming becomes increasingly important. The Arctic Clouds in Summer Experiment (ACSE) was conducted in a mix of <span class="hlt">open</span> <span class="hlt">water</span> and sea ice in the eastern Arctic along the Siberian shelf during late summer and early autumn 2014, providing detailed observations of the seasonal transition, from melt to freeze. Measurements were taken over both ice-free and ice-covered surfaces, offering an insight to the role of the surface state in shaping the lower troposphere and the boundary-layer conditions as summer turned into autumn. During summer, strong surface inversions persisted over sea ice, while well-mixed boundary layers capped by elevated inversions were frequent over <span class="hlt">open-water</span>. The former were often associated with advection of warm air from adjacent <span class="hlt">open-water</span> or land surfaces, whereas the latter were due to a positive buoyancy flux from the warm <span class="hlt">ocean</span> surface. Fog and stratus clouds often persisted over the ice, whereas low-level liquid-<span class="hlt">water</span> clouds developed over <span class="hlt">open</span> <span class="hlt">water</span>. These differences largely disappeared in autumn, when mixed-phase clouds capped by elevated inversions dominated in both ice-free and ice-covered conditions. Low-level-jets occurred ~20-25% of the time in both seasons. The observations indicate that these jets were typically initiated at air-mass boundaries or along the ice edge in autumn, while in summer they appeared to be inertial oscillations initiated by partial frictional decoupling as warm air was advected in over the sea ice. The start of the autumn season was related to an abrupt change in atmospheric conditions, rather than to the gradual change in solar radiation. The autumn onset appeared as a rapid cooling of the whole atmosphere and the freeze up followed as the warm surface lost heat to the atmosphere. While the surface type had a pronounced impact on boundary</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/663505','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/663505"><span>Carbon 14 measurements in surface <span class="hlt">water</span> CO{sub 2} from the Atlantic, India, and Pacific <span class="hlt">Oceans</span>, 1965--1994</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>Nydal, R.; Brenkert, A.L.; Boden, T.A.</p> <p>1998-03-01</p> <p>In the 1960s, thermonuclear bomb tests released significant pulses of radioactive carbon-14 ({sup 14}C) into the atmosphere. These major perturbations allowed scientists to study the dynamics of the global carbon cycle by calculating rates of isotope exchange between the atmosphere and <span class="hlt">ocean</span> <span class="hlt">waters</span>. A total of 950 <span class="hlt">ocean</span> surface <span class="hlt">water</span> observations were made from 1965 through 1994. The measurements were taken at 30 stations in the Atlantic <span class="hlt">Ocean</span>, 14 stations in the Indian <span class="hlt">Ocean</span>, and 38 stations in the Pacific <span class="hlt">Ocean</span>. Thirty-two of the 950 samples were taken in the Atlantic <span class="hlt">Ocean</span> during the R/V Andenes research cruise. {sup 14}Cmore » was measured in 871 of the 950 samples, and those measurements have been corrected ({Delta}{sup 14}C) for isotopic fractionation and radioactive decay. The {Delta}{sup 14}C values range between {minus}113.3 and 280.9 per mille and have a mean value of 101.3 per mille. The highest yearly mean (146.5 per mille) was calculated for 1969, the lowest yearly mean value was calculated for 1990 (67.9 per mille) illustrating a decrease over time. This decrease was to be expected as a result of the ban on atmospheric thermonuclear tests and the slow mixing of the <span class="hlt">ocean</span> surface <span class="hlt">waters</span> with the deeper layers.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.9370C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.9370C"><span>A Spectrally Selective Attenuation Mechanism-Based Kpar Algorithm for Biomass Heating Effect Simulation in the <span class="hlt">Open</span> <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, Jun; Zhang, Xiangguang; Xing, Xiaogang; Ishizaka, Joji; Yu, Zhifeng</p> <p>2017-12-01</p> <p>Quantifying the diffuse attenuation coefficient of the photosynthetically available radiation (Kpar) can improve our knowledge of euphotic depth (Zeu) and biomass heating effects in the upper layers of <span class="hlt">oceans</span>. An algorithm to semianalytically derive Kpar from remote sensing reflectance (Rrs) is developed for the global <span class="hlt">open</span> <span class="hlt">oceans</span>. This algorithm includes the following two portions: (1) a neural network model for deriving the diffuse attention coefficients (Kd) that considers the residual error in satellite Rrs, and (2) a three band depth-dependent Kpar algorithm (TDKA) for describing the spectrally selective attenuation mechanism of underwater solar radiation in the <span class="hlt">open</span> <span class="hlt">oceans</span>. This algorithm is evaluated with both in situ PAR profile data and satellite images, and the results show that it can produce acceptable PAR profile estimations while clearly removing the impacts of satellite residual errors on Kpar estimations. Furthermore, the performance of the TDKA algorithm is evaluated by its applicability in Zeu derivation and mean temperature within a mixed layer depth (TML) simulation, and the results show that it can significantly decrease the uncertainty in both compared with the classical chlorophyll-a concentration-based Kpar algorithm. Finally, the TDKA algorithm is applied in simulating biomass heating effects in the Sargasso Sea near Bermuda, with new Kpar data it is found that the biomass heating effects can lead to a 3.4°C maximum positive difference in temperature in the upper layers but could result in a 0.67°C maximum negative difference in temperature in the deep layers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20547419','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20547419"><span>Nutrient characteristics of the <span class="hlt">water</span> masses and their seasonal variability in the eastern equatorial Indian <span class="hlt">Ocean</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sardessai, S; Shetye, Suhas; Maya, M V; Mangala, K R; Prasanna Kumar, S</p> <p>2010-01-01</p> <p>Nutrient characteristics of four <span class="hlt">water</span> masses in the light of their thermohaline properties are examined in the eastern Equatorial Indian <span class="hlt">Ocean</span> during winter, spring and summer monsoon. The presence of low salinity <span class="hlt">water</span> mass with "Surface enrichments" of inorganic nutrients was observed relative to 20 m in the mixed layer. Lowest oxygen levels of 19 microM at 3 degrees N in the euphotic zone indicate mixing of low oxygen high salinity Arabian Sea <span class="hlt">waters</span> with the equatorial Indian <span class="hlt">Ocean</span>. The seasonal variability of nutrients was regulated by seasonally varying physical processes like thermocline elevation, meridional and zonal transport, the equatorial undercurrent and biological processes of uptake and remineralization. Circulation of Arabian Sea high salinity <span class="hlt">waters</span> with nitrate deficit could also be seen from low N/P ratio with a minimum of 8.9 in spring and a maximum of 13.6 in winter. This large deviation from Redfield N/P ratio indicates the presence of denitrified high salinity <span class="hlt">waters</span> with a seasonal nitrate deficit ranging from -4.85 to 1.52 in the Eastern Equatorial Indian <span class="hlt">Ocean</span>. 2010 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JGRC..121.8139H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JGRC..121.8139H"><span>Observations of <span class="hlt">open-ocean</span> deep convection in the northwestern Mediterranean Sea: Seasonal and interannual variability of mixing and deep <span class="hlt">water</span> masses for the 2007-2013 Period</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Houpert, L.; Durrieu de Madron, X.; Testor, P.; Bosse, A.; D'Ortenzio, F.; Bouin, M. N.; Dausse, D.; Le Goff, H.; Kunesch, S.; Labaste, M.; Coppola, L.; Mortier, L.; Raimbault, P.</p> <p>2016-11-01</p> <p>We present here a unique oceanographic and meteorological data set focus on the deep convection processes. Our results are essentially based on in situ data (mooring, research vessel, glider, and profiling float) collected from a multiplatform and integrated monitoring system (MOOSE: Mediterranean <span class="hlt">Ocean</span> Observing System on Environment), which monitored continuously the northwestern Mediterranean Sea since 2007, and in particular high-frequency potential temperature, salinity, and current measurements from the mooring LION located within the convection region. From 2009 to 2013, the mixed layer depth reaches the seabed, at a depth of 2330m, in February. Then, the violent vertical mixing of the whole <span class="hlt">water</span> column lasts between 9 and 12 days setting up the characteristics of the newly formed deep <span class="hlt">water</span>. Each deep convection winter formed a new warmer and saltier "vintage" of deep <span class="hlt">water</span>. These sudden inputs of salt and heat in the deep <span class="hlt">ocean</span> are responsible for trends in salinity (3.3 ± 0.2 × 10-3/yr) and potential temperature (3.2 ± 0.5 × 10-3 C/yr) observed from 2009 to 2013 for the 600-2300 m layer. For the first time, the overlapping of the three "phases" of deep convection can be observed, with secondary vertical mixing events (2-4 days) after the beginning of the restratification phase, and the restratification/spreading phase still active at the beginning of the following deep convection event.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015APS..DFDL29001F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015APS..DFDL29001F"><span>Turning <span class="hlt">Ocean</span> Mixing Upside Down</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ferrari, Raffaele; Mashayek, Ali; Campin, Jean-Michael; McDougall, Trevor; Nikurashin, Maxim</p> <p>2015-11-01</p> <p>It is generally understood that small-scale mixing, such as is caused by breaking internal waves, drives upwelling of the densest <span class="hlt">ocean</span> <span class="hlt">waters</span> that sink to the <span class="hlt">ocean</span> bottom at high latitudes. However the observational evidence that small-scale mixing is more vigorous close to the <span class="hlt">ocean</span> bottom than above implies that small-scale mixing converts light <span class="hlt">waters</span> into denser ones, thus driving a net sinking of abyssal <span class="hlt">water</span>. It is shown that abyssal <span class="hlt">waters</span> return to the surface along weakly stratified boundary layers, where the small-scale mixing of density decays to zero. The net <span class="hlt">ocean</span> meridional overturning circulation is thus the small residual of a large sinking of <span class="hlt">waters</span>, driven by small-scale mixing in the stratified interior, and an equally large upwelling, driven by the reduced small-scale mixing along the <span class="hlt">ocean</span> boundaries. Thus whether abyssal <span class="hlt">waters</span> upwell or sink in the net cannot be inferred simply from the vertical profile of mixing intensity, but depends also on the <span class="hlt">ocean</span> hypsometry, i.e. the shape of the bottom topography. The implications of this result for our understanding of the abyssal <span class="hlt">ocean</span> circulation will be presented with a combination of numerical models and observations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMGC11G1102R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMGC11G1102R"><span>Impact of lengthening <span class="hlt">open</span> <span class="hlt">water</span> season on food security in Alaska coastal communities: Global impacts may outweigh local "frontline" effects</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rolph, R.; Mahoney, A. R.</p> <p>2015-12-01</p> <p>Using ice concentration data from the Alaska Sea Ice Atlas from 1953-2013 for selected communities in Alaska, we find a consistent trend toward later freeze up and earlier breakup, leading a lengthened <span class="hlt">open</span> <span class="hlt">water</span> period. Such changes are often considered to bring a variety of "frontline" local impacts to Arctic coastal communities such as increased rates of coastal erosion. However, direct consequences of these changes to local food security (e.g. through impacts on subsistence activities and marine transport of goods) may be outweighed at least in the short term by the effects of large scale Arctic sea ice change coupled with global oil markets. For example, a later freeze-up might delay local hunters' transition from boats to snow-machines, but whether this trend will affect hunting success, especially in the next few years, is uncertain. Likewise, the magnitude of change in <span class="hlt">open</span> <span class="hlt">water</span> season length is unlikely to be sufficient to increase the frequency with which communities are served by barges. However, an expanding <span class="hlt">open</span> <span class="hlt">water</span> season throughout the Arctic has implications for the global economy, which can have indirect effects on local communities. In the Chukchi and Beaufort Seas, where rapid sea ice change has been accompanied by increased interest in oil and gas development, the U.S. Bureau of <span class="hlt">Ocean</span> Energy Management currently requires drilling operations to cease 38 days prior to freeze up. Taking this into account, the lengthening <span class="hlt">open</span> <span class="hlt">water</span> season has effectively extended the drilling season for oil companies by 184% since the 1950s. If oil development goes ahead, local communities will likely experience a range of indirect impacts on food security due to increased vessel traffic and demand on infrastructure coupled with changes in local economies and employment opportunities. Increased likelihood of an oil spill in coastal <span class="hlt">waters</span> also poses a significant threat to local food security. Thus, while Arctic coastal communities are already experiencing</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27806076','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27806076"><span>Possible Ballast <span class="hlt">Water</span> Transfer of Lionfish to the Eastern Pacific <span class="hlt">Ocean</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>MacIsaac, Hugh J; De Roy, Emma M; Leung, Brian; Grgicak-Mannion, Alice; Ruiz, Gregory M</p> <p>2016-01-01</p> <p>The Indo-Pacific Red Lionfish was first reported off the Florida coast in 1985, following which it has spread across much of the SE USA, Gulf of Mexico, and Caribbean Sea. Lionfish negatively impact fish and invertebrate assemblages and abundances, thus further spread is cause for concern. To date, the fish has not been reported on the Pacific coast of North or Central America. Here we examine the possibility of ballast <span class="hlt">water</span> transfer of lionfish from colonized areas in the Atlantic <span class="hlt">Ocean</span> to USA ports on the Pacific coast. Over an eight-year period, we documented 27 commercial vessel-trips in which ballast <span class="hlt">water</span> was loaded in colonized sites and later discharged untreated into Pacific coast ports in the USA. California had the highest number of discharges including San Francisco Bay and Los Angeles-Long Beach. A species distribution model suggests that the probability of lionfish establishment is low for the western USA, Colombia and Panama, low to medium for Costa Rica, Nicaragua, El Salvador and Guatemala, medium to high for mainland Ecuador, and very high for western Mexico, Peru and the Galapagos Islands. Given the species' intolerance of freshwater conditions, we propose that ballast <span class="hlt">water</span> exchange be conducted in Gatún Lake, Panama for western-bound vessels carrying 'risky' ballast <span class="hlt">water</span> to prevent invasion of the eastern Pacific <span class="hlt">Ocean</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5091758','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5091758"><span>Possible Ballast <span class="hlt">Water</span> Transfer of Lionfish to the Eastern Pacific <span class="hlt">Ocean</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>MacIsaac, Hugh J.; De Roy, Emma M.; Leung, Brian; Grgicak-Mannion, Alice; Ruiz, Gregory M.</p> <p>2016-01-01</p> <p>The Indo-Pacific Red Lionfish was first reported off the Florida coast in 1985, following which it has spread across much of the SE USA, Gulf of Mexico, and Caribbean Sea. Lionfish negatively impact fish and invertebrate assemblages and abundances, thus further spread is cause for concern. To date, the fish has not been reported on the Pacific coast of North or Central America. Here we examine the possibility of ballast <span class="hlt">water</span> transfer of lionfish from colonized areas in the Atlantic <span class="hlt">Ocean</span> to USA ports on the Pacific coast. Over an eight-year period, we documented 27 commercial vessel-trips in which ballast <span class="hlt">water</span> was loaded in colonized sites and later discharged untreated into Pacific coast ports in the USA. California had the highest number of discharges including San Francisco Bay and Los Angeles-Long Beach. A species distribution model suggests that the probability of lionfish establishment is low for the western USA, Colombia and Panama, low to medium for Costa Rica, Nicaragua, El Salvador and Guatemala, medium to high for mainland Ecuador, and very high for western Mexico, Peru and the Galapagos Islands. Given the species’ intolerance of freshwater conditions, we propose that ballast <span class="hlt">water</span> exchange be conducted in Gatún Lake, Panama for western-bound vessels carrying ‘risky’ ballast <span class="hlt">water</span> to prevent invasion of the eastern Pacific <span class="hlt">Ocean</span>. PMID:27806076</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2996450','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2996450"><span>Toxic diatoms and domoic acid in natural and iron enriched <span class="hlt">waters</span> of the <span class="hlt">oceanic</span> Pacific</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Silver, Mary W.; Bargu, Sibel; Coale, Susan L.; Benitez-Nelson, Claudia R.; Garcia, Ana C.; Roberts, Kathryn J.; Sekula-Wood, Emily; Bruland, Kenneth W.; Coale, Kenneth H.</p> <p>2010-01-01</p> <p>Near-surface <span class="hlt">waters</span> ranging from the Pacific subarctic (58°N) to the Southern <span class="hlt">Ocean</span> (66°S) contain the neurotoxin domoic acid (DA), associated with the diatom Pseudo-nitzschia. Of the 35 stations sampled, including ones from historic iron fertilization experiments (SOFeX, IronEx II), we found Pseudo-nitzschia at 34 stations and DA measurable at 14 of the 26 stations analyzed for DA. Toxin ranged from 0.3 fg·cell−1 to 2 pg·cell−1, comparable with levels found in similar-sized cells from coastal <span class="hlt">waters</span>. In the western subarctic, descent of intact Pseudo-nitzschia likely delivered significant amounts of toxin (up to 4 μg of DA·m−2·d−1) to underlying mesopelagic <span class="hlt">waters</span> (150–500 m). By reexamining phytoplankton samples from SOFeX and IronEx II, we found substantial amounts of DA associated with Pseudo-nitzschia. Indeed, at SOFeX in the Antarctic Pacific, DA reached 220 ng·L−1, levels at which animal mortalities have occurred on continental shelves. Iron <span class="hlt">ocean</span> fertilization also occurs naturally and may have promoted blooms of these ubiquitous algae over previous glacial cycles during deposition of iron-rich aerosols. Thus, the neurotoxin DA occurs both in coastal and <span class="hlt">oceanic</span> <span class="hlt">waters</span>, and its concentration, associated with changes in Pseudo-nitzschia abundance, likely varies naturally with climate cycles, as well as with artificial iron fertilization. Given that iron fertilization in iron-depleted regions of the sea has been proposed to enhance phytoplankton growth and, thereby, both reduce atmospheric CO2 and moderate <span class="hlt">ocean</span> acidification in surface <span class="hlt">waters</span>, consideration of the potentially serious ecosystem impacts associated with DA is prudent. PMID:21068374</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21068374','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21068374"><span>Toxic diatoms and domoic acid in natural and iron enriched <span class="hlt">waters</span> of the <span class="hlt">oceanic</span> Pacific.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Silver, Mary W; Bargu, Sibel; Coale, Susan L; Benitez-Nelson, Claudia R; Garcia, Ana C; Roberts, Kathryn J; Sekula-Wood, Emily; Bruland, Kenneth W; Coale, Kenneth H</p> <p>2010-11-30</p> <p>Near-surface <span class="hlt">waters</span> ranging from the Pacific subarctic (58°N) to the Southern <span class="hlt">Ocean</span> (66°S) contain the neurotoxin domoic acid (DA), associated with the diatom Pseudo-nitzschia. Of the 35 stations sampled, including ones from historic iron fertilization experiments (SOFeX, IronEx II), we found Pseudo-nitzschia at 34 stations and DA measurable at 14 of the 26 stations analyzed for DA. Toxin ranged from 0.3 fg·cell(-1) to 2 pg·cell(-1), comparable with levels found in similar-sized cells from coastal <span class="hlt">waters</span>. In the western subarctic, descent of intact Pseudo-nitzschia likely delivered significant amounts of toxin (up to 4 μg of DA·m(-2)·d(-1)) to underlying mesopelagic <span class="hlt">waters</span> (150-500 m). By reexamining phytoplankton samples from SOFeX and IronEx II, we found substantial amounts of DA associated with Pseudo-nitzschia. Indeed, at SOFeX in the Antarctic Pacific, DA reached 220 ng·L(-1), levels at which animal mortalities have occurred on continental shelves. Iron <span class="hlt">ocean</span> fertilization also occurs naturally and may have promoted blooms of these ubiquitous algae over previous glacial cycles during deposition of iron-rich aerosols. Thus, the neurotoxin DA occurs both in coastal and <span class="hlt">oceanic</span> <span class="hlt">waters</span>, and its concentration, associated with changes in Pseudo-nitzschia abundance, likely varies naturally with climate cycles, as well as with artificial iron fertilization. Given that iron fertilization in iron-depleted regions of the sea has been proposed to enhance phytoplankton growth and, thereby, both reduce atmospheric CO(2) and moderate <span class="hlt">ocean</span> acidification in surface <span class="hlt">waters</span>, consideration of the potentially serious ecosystem impacts associated with DA is prudent.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20160008717&hterms=spices&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dspices','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20160008717&hterms=spices&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dspices"><span>Warming of the Global <span class="hlt">Ocean</span>: Spatial Structure and <span class="hlt">Water</span>-Mass Trends</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hakkinen, Sirpa; Rhines, Peter B.; Worthen, Denise L.</p> <p>2016-01-01</p> <p>This study investigates the multidecadal warming and interannual-to-decadal heat content changes in the upper <span class="hlt">ocean</span> (0-700 m), focusing on vertical and horizontal patterns of variability. These results support a nearly monotonic warming over much of the World <span class="hlt">Ocean</span>, with a shift toward Southern Hemisphere warming during the well-observed past decade. This is based on objectively analyzed gridded observational datasets and on a modeled state estimate. Besides the surface warming, a warming climate also has a subsurface effect manifesting as a strong deepening of the midthermocline isopycnals, which can be diagnosed directly from hydrographic data. This deepening appears to be a result of heat entering via subduction and spreading laterally from the high-latitude ventilation regions of subtropical mode <span class="hlt">waters</span>. The basin-average multidecadal warming mainly expands the subtropical mode <span class="hlt">water</span> volume, with weak changes in the temperature-salinity (u-S) relationship (known as ''spice'' variability). However, the spice contribution to the heat content can be locally large, for example in Southern Hemisphere. Multidecadal isopycnal sinking has been strongest over the southern basins and weaker elsewhere with the exception of the Gulf Stream/North Atlantic Current/subtropical recirculation gyre. At interannual to decadal time scales, wind-driven sinking and shoaling of density surfaces still dominate <span class="hlt">ocean</span> heat content changes, while the contribution from temperature changes along density surfaces tends to decrease as time scales shorten.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040082057&hterms=datasets&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Ddatasets','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040082057&hterms=datasets&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Ddatasets"><span>Climatic Analysis of <span class="hlt">Oceanic</span> <span class="hlt">Water</span> Vapor Transports Based on Satellite E-P Datasets</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Smith, Eric A.; Sohn, Byung-Ju; Mehta, Vikram</p> <p>2004-01-01</p> <p>Understanding the climatically varying properties of <span class="hlt">water</span> vapor transports from a robust observational perspective is an essential step in calibrating climate models. This is tantamount to measuring year-to-year changes of monthly- or seasonally-averaged, divergent <span class="hlt">water</span> vapor transport distributions. This cannot be done effectively with conventional radiosonde data over <span class="hlt">ocean</span> regions where sounding data are generally sparse. This talk describes how a methodology designed to derive atmospheric <span class="hlt">water</span> vapor transports over the world <span class="hlt">oceans</span> from satellite-retrieved precipitation (P) and evaporation (E) datasets circumvents the problem of inadequate sampling. Ultimately, the method is intended to take advantage of the relatively complete and consistent coverage, as well as continuity in sampling, associated with E and P datasets obtained from satellite measurements. Independent P and E retrievals from Special Sensor Microwave Imager (SSM/I) measurements, along with P retrievals from Tropical Rainfall Measuring Mission (TRMM) measurements, are used to obtain transports by solving a potential function for the divergence of <span class="hlt">water</span> vapor transport as balanced by large scale E - P conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/12003211','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/12003211"><span>Role of <span class="hlt">oceanic</span> air bubbles in atmospheric correction of <span class="hlt">ocean</span> color imagery.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yan, Banghua; Chen, Bingquan; Stamnes, Knut</p> <p>2002-04-20</p> <p><span class="hlt">Ocean</span> color is the radiance that emanates from the <span class="hlt">ocean</span> because of scattering by chlorophyll pigments and particles of organic and inorganic origin. Air bubbles in the <span class="hlt">ocean</span> also scatter light and thus contribute to the <span class="hlt">water</span>-leaving radiance. This additional <span class="hlt">water</span>-leaving radiance that is due to <span class="hlt">oceanic</span> air bubbles could violate the black pixel assumption at near-infrared wavelengths and be attributed to chlorophyll in the visible. Hence, the accuracy of the atmospheric correction required for the retrieval of <span class="hlt">ocean</span> color from satellite measurements is impaired. A comprehensive radiative transfer code for the coupled atmosphere--<span class="hlt">ocean</span> system is employed to assess the effect of <span class="hlt">oceanic</span> air bubbles on atmospheric correction of <span class="hlt">ocean</span> color imagery. This effect is found to depend on the wavelength-dependent optical properties of <span class="hlt">oceanic</span> air bubbles as well as atmospheric aerosols.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002ApOpt..41.2202Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002ApOpt..41.2202Y"><span>Role of <span class="hlt">oceanic</span> air bubbles in atmospheric correction of <span class="hlt">ocean</span> color imagery</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yan, Banghua; Chen, Bingquan; Stamnes, Knut</p> <p>2002-04-01</p> <p><span class="hlt">Ocean</span> color is the radiance that emanates from the <span class="hlt">ocean</span> because of scattering by chlorophyll pigments and particles of organic and inorganic origin. Air bubbles in the <span class="hlt">ocean</span> also scatter light and thus contribute to the <span class="hlt">water</span>-leaving radiance. This additional <span class="hlt">water</span>-leaving radiance that is due to <span class="hlt">oceanic</span> air bubbles could violate the black pixel assumption at near-infrared wavelengths and be attributed to chlorophyll in the visible. Hence, the accuracy of the atmospheric correction required for the retrieval of <span class="hlt">ocean</span> color from satellite measurements is impaired. A comprehensive radiative transfer code for the coupled atmosphere-<span class="hlt">ocean</span> system is employed to assess the effect of <span class="hlt">oceanic</span> air bubbles on atmospheric correction of <span class="hlt">ocean</span> color imagery. This effect is found to depend on the wavelength-dependent optical properties of <span class="hlt">oceanic</span> air bubbles as well as atmospheric aerosols.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMOS21C..03L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMOS21C..03L"><span>In situ quantitative characterisation of the <span class="hlt">ocean</span> <span class="hlt">water</span> column using acoustic multibeam backscatter data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lamarche, G.; Le Gonidec, Y.; Lucieer, V.; Lurton, X.; Greinert, J.; Dupré, S.; Nau, A.; Heffron, E.; Roche, M.; Ladroit, Y.; Urban, P.</p> <p>2017-12-01</p> <p>Detecting liquid, solid or gaseous features in the <span class="hlt">ocean</span> is generating considerable interest in the geoscience community, because of their potentially high economic values (oil & gas, mining), their significance for environmental management (oil/gas leakage, biodiversity mapping, greenhouse gas monitoring) as well as their potential cultural and traditional values (food, freshwater). Enhancing people's capability to quantify and manage the natural capital present in the <span class="hlt">ocean</span> <span class="hlt">water</span> goes hand in hand with the development of marine acoustic technology, as marine echosounders provide the most reliable and technologically advanced means to develop quantitative studies of <span class="hlt">water</span> column backscatter data. This is not developed to its full capability because (i) of the complexity of the physics involved in relation to the constantly changing marine environment, and (ii) the rapid technological evolution of high resolution multibeam echosounder (MBES) <span class="hlt">water</span>-column imaging systems. The <span class="hlt">Water</span> Column Imaging Working Group is working on a series of multibeam echosounder (MBES) <span class="hlt">water</span> column datasets acquired in a variety of environments, using a range of frequencies, and imaging a number of <span class="hlt">water</span>-column features such as gas seeps, oil leaks, suspended particulate matter, vegetation and freshwater springs. Access to data from different acoustic frequencies and <span class="hlt">ocean</span> dynamics enables us to discuss and test multifrequency approaches which is the most promising means to develop a quantitative analysis of the physical properties of acoustic scatterers, providing rigorous cross calibration of the acoustic devices. In addition, high redundancy of multibeam data, such as is available for some datasets, will allow us to develop data processing techniques, leading to quantitative estimates of <span class="hlt">water</span> column gas seeps. Each of the datasets has supporting ground-truthing data (underwater videos and photos, physical oceanography measurements) which provide information on the origin and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.C53F..05P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.C53F..05P"><span>Accurate numerical forward model for optimal retracking of SIRAL2 SAR echoes over <span class="hlt">open</span> <span class="hlt">ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Phalippou, L.; Demeestere, F.</p> <p>2011-12-01</p> <p>The SAR mode of SIRAL-2 on board Cryosat-2 has been designed to measure primarily sea-ice and continental ice (Wingham et al. 2005). In 2005, K. Raney (KR, 2005) pointed out the improvements brought by SAR altimeter for <span class="hlt">open</span> <span class="hlt">ocean</span>. KR results were mostly based on 'rule of thumb' considerations on speckle noise reduction due to the higher PRF and to speckle decorrelation after SAR processing. In 2007, Phalippou and Enjolras (PE,2007) provided the theoretical background for optimal retracking of SAR echoes over <span class="hlt">ocean</span> with a focus on the forward modelling of the power-waveforms. The accuracies of geophysical parameters (range, significant wave heights, and backscattering coefficient) retrieved from SAR altimeter data were derived accounting for SAR echo shape and speckle noise accurate modelling. The step forward to optimal retracking using numerical forward model (NFM) was also pointed out. NFM of the power waveform avoids analytical approximation, a warranty to minimise the geophysical dependent biases in the retrieval. NFM have been used for many years, in operational meteorology in particular, for retrieving temperature and humidity profiles from IR and microwave radiometers as the radiative transfer function is complex (Eyre, 1989). So far this technique was not used in the field of <span class="hlt">ocean</span> conventional altimetry as analytical models (e.g. Brown's model for instance) were found to give sufficient accuracy. However, although NFM seems desirable even for conventional nadir altimetry, it becomes inevitable if one wish to process SAR altimeter data as the transfer function is too complex to be approximated by a simple analytical function. This was clearly demonstrated in PE 2007. The paper describes the background to SAR data retracking over <span class="hlt">open</span> <span class="hlt">ocean</span>. Since PE 2007 improvements have been brought to the forward model and it is shown that the altimeter on-ground and in flight characterisation (e.g antenna pattern range impulse response, azimuth impulse response</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/2016AGUFM.G21A0976B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.G21A0976B"><span>Evaluating the performance of Sentinel-3 SRAL SAR Altimetry in the Coastal and <span class="hlt">Open</span> <span class="hlt">Ocean</span>, and developing improved retrieval methods - The ESA SCOOP Project.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Benveniste, J.; Cotton, D.; Moreau, T.; Varona, E.; Roca, M.; Cipollini, P.; Cancet, M.; Martin, F.; Fenoglio-Marc, L.; Naeije, M.; Fernandes, J.; Restano, M.; Ambrozio, A.</p> <p>2016-12-01</p> <p>The ESA Sentinel-3 satellite, launched in February 2016 as a part of the Copernicus programme, is the second satellite to operate a SAR mode altimeter. The Sentinel 3 Synthetic Aperture Radar Altimeter (SRAL) is based on the heritage from Cryosat-2, but this time complemented by a Microwave Radiometer (MWR) to provide a wet troposphere correction, and operating at Ku and C-Bands to provide an accurate along-track ionospheric correction. Together this instrument package, including both GPS and DORIS instruments for accurate positioning, allows accurate measurements of sea surface height over the <span class="hlt">ocean</span>, as well as measurements of significant wave height and surface wind speed. SCOOP (SAR Altimetry Coastal & <span class="hlt">Open</span> <span class="hlt">Ocean</span> Performance) is a project funded under the ESA SEOM (Scientific Exploitation of Operational Missions) Programme Element, started in September 2015, to characterise the expected performance of Sentinel-3 SRAL SAR mode altimeter products, in the coastal zone and <span class="hlt">open-ocean</span>, and then to develop and evaluate enhancements to the baseline processing scheme in terms of improvements to <span class="hlt">ocean</span> measurements. There is also a work package to develop and evaluate an improved Wet Troposphere correction for Sentinel-3, based on the measurements from the on-board MWR, further enhanced mostly in the coastal and polar regions using third party data, and provide recommendations for use. At the end of the project recommendations for further developments and implementations will be provided through a scientific roadmap. In this presentation we provide an overview of the SCOOP project, highlighting the key deliverables and discussing the potential impact of the results in terms of the application of delay-Doppler (SAR) altimeter measurements over the <span class="hlt">open-ocean</span> and coastal zone. We also present the initial results from the project, including: Key findings from a review of the current "state-of-the-art" for SAR altimetry, Specification of the initial "reference" delay</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27668842','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27668842"><span>Phylogeography and pigment type diversity of Synechococcus cyanobacteria in surface <span class="hlt">waters</span> of the northwestern pacific <span class="hlt">ocean</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Xia, Xiaomin; Partensky, Frédéric; Garczarek, Laurence; Suzuki, Koji; Guo, Cui; Yan Cheung, Shun; Liu, Hongbin</p> <p>2017-01-01</p> <p>The widespread unicellular cyanobacteria Synechococcus are major contributors to global marine primary production. Here, we report their abundance, phylogenetic diversity (as assessed using the RNA polymerase gamma subunit gene rpoC1) and pigment diversity (as indirectly assessed using the laterally transferred cpeBA genes, encoding phycoerythrin-I) in surface <span class="hlt">waters</span> of the northwestern Pacific <span class="hlt">Ocean</span>, sampled over nine distinct cruises (2008-2015). Abundance of Synechococcus was low in the subarctic <span class="hlt">ocean</span> and South China Sea, intermediate in the western subtropical Pacific <span class="hlt">Ocean</span>, and the highest in the Japan and East China seas. Clades I and II were by far the most abundant Synechococcus lineages, the former dominating in temperate cold <span class="hlt">waters</span> and the latter in (sub)tropical <span class="hlt">waters</span>. Clades III and VI were also fairly abundant in warm <span class="hlt">waters</span>, but with a narrower distribution than clade II. One type of chromatic acclimater (3dA) largely dominated the Synechococcus communities in the subarctic <span class="hlt">ocean</span>, while another (3dB) and/or cells with a fixed high phycourobilin to phycoerythrobilin ratio (pigment type 3c) predominated at mid and low latitudes. Altogether, our results suggest that the variety of pigment content found in most Synechococcus clades considerably extends the niches that they can colonize and therefore the whole genus habitat. © 2016 Society for Applied Microbiology and John Wiley & Sons Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1002184-multi-scale-modeling-puget-sound-using-unstructured-grid-coastal-ocean-model-from-tide-flats-estuaries-coastal-waters','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1002184-multi-scale-modeling-puget-sound-using-unstructured-grid-coastal-ocean-model-from-tide-flats-estuaries-coastal-waters"><span>Multi-scale modeling of Puget Sound using an unstructured-grid coastal <span class="hlt">ocean</span> model: from tide flats to estuaries and coastal <span class="hlt">waters</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>Yang, Zhaoqing; Khangaonkar, Tarang</p> <p>2010-11-19</p> <p><span class="hlt">Water</span> circulation in Puget Sound, a large complex estuary system in the Pacific Northwest coastal <span class="hlt">ocean</span> of the United States, is governed by multiple spatially and temporally varying forcings from tides, atmosphere (wind, heating/cooling, precipitation/evaporation, pressure), and river inflows. In addition, the hydrodynamic response is affected strongly by geomorphic features, such as fjord-like bathymetry and complex shoreline features, resulting in many distinguishing characteristics in its main and sub-basins. To better understand the details of circulation features in Puget Sound and to assist with proposed nearshore restoration actions for improving <span class="hlt">water</span> quality and the ecological health of Puget Sound, a high-resolutionmore » (around 50 m in estuaries and tide flats) hydrodynamic model for the entire Puget Sound was needed. Here, a threedimensional circulation model of Puget Sound using an unstructured-grid finite volume coastal <span class="hlt">ocean</span> model is presented. The model was constructed with sufficient resolution in the nearshore region to address the complex coastline, multi-tidal channels, and tide flats. Model <span class="hlt">open</span> boundaries were extended to the entrance of the Strait of Juan de Fuca and the northern end of the Strait of Georgia to account for the influences of <span class="hlt">ocean</span> <span class="hlt">water</span> intrusion from the Strait of Juan de Fuca and the Fraser River plume from the Strait of Georgia, respectively. Comparisons of model results, observed data, and associated error statistics for tidal elevation, velocity, temperature, and salinity indicate that the model is capable of simulating the general circulation patterns on the scale of a large estuarine system as well as detailed hydrodynamics in the nearshore tide flats. Tidal characteristics, temperature/salinity stratification, mean circulation, and river plumes in estuaries with tide flats are discussed.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19810059141&hterms=use+color&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Duse%2Bcolor','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19810059141&hterms=use+color&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Duse%2Bcolor"><span>Use of <span class="hlt">ocean</span> color scanner data in <span class="hlt">water</span> quality mapping</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Khorram, S.</p> <p>1981-01-01</p> <p>Remotely sensed data, in combination with in situ data, are used in assessing <span class="hlt">water</span> quality parameters within the San Francisco Bay-Delta. The parameters include suspended solids, chlorophyll, and turbidity. Regression models are developed between each of the <span class="hlt">water</span> quality parameter measurements and the <span class="hlt">Ocean</span> Color Scanner (OCS) data. The models are then extended to the entire study area for mapping <span class="hlt">water</span> quality parameters. The results include a series of color-coded maps, each pertaining to one of the <span class="hlt">water</span> quality parameters, and the statistical analysis of the OCS data and regression models. It is found that concurrently collected OCS data and surface truth measurements are highly useful in mapping the selected <span class="hlt">water</span> quality parameters and locating areas having relatively high biological activity. In addition, it is found to be virtually impossible, at least within this test site, to locate such areas on U-2 color and color-infrared photography.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20150022925&hterms=inversion&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dinversion','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20150022925&hterms=inversion&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dinversion"><span>A Semianalytical <span class="hlt">Ocean</span> Color Inversion Algorithm with Explicit <span class="hlt">Water</span> Column Depth and Substrate Reflectance Parameterization</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mckinna, Lachlan I. W.; Werdell, P. Jeremy; Fearns, Peter R. C.; Weeks, Scarla J.; Reichstetter, Martina; Franz, Bryan A.; Shea, Donald M.; Feldman, Gene C.</p> <p>2015-01-01</p> <p>A semianalytical <span class="hlt">ocean</span> color inversion algorithm was developed for improving retrievals of inherent optical properties (IOPs) in optically shallow <span class="hlt">waters</span>. In clear, geometrically shallow <span class="hlt">waters</span>, light reflected off the seafloor can contribute to the <span class="hlt">water</span>-leaving radiance signal. This can have a confounding effect on <span class="hlt">ocean</span> color algorithms developed for optically deep <span class="hlt">waters</span>, leading to an overestimation of IOPs. The algorithm described here, the Shallow <span class="hlt">Water</span> Inversion Model (SWIM), uses pre-existing knowledge of bathymetry and benthic substrate brightness to account for optically shallow effects. SWIM was incorporated into the NASA <span class="hlt">Ocean</span> Biology Processing Group's L2GEN code and tested in <span class="hlt">waters</span> of the Great Barrier Reef, Australia, using the Moderate Resolution Imaging Spectroradiometer (MODIS) Aqua time series (2002-2013). SWIM-derived values of the total non-<span class="hlt">water</span> absorption coefficient at 443 nm, at(443), the particulate backscattering coefficient at 443 nm, bbp(443), and the diffuse attenuation coefficient at 488 nm, Kd(488), were compared with values derived using the Generalized Inherent Optical Properties algorithm (GIOP) and the Quasi-Analytical Algorithm (QAA). The results indicated that in clear, optically shallow <span class="hlt">waters</span> SWIM-derived values of at(443), bbp(443), and Kd(443) were realistically lower than values derived using GIOP and QAA, in agreement with radiative transfer modeling. This signified that the benthic reflectance correction was performing as expected. However, in more optically complex <span class="hlt">waters</span>, SWIM had difficulty converging to a solution, a likely consequence of internal IOP parameterizations. Whilst a comprehensive study of the SWIM algorithm's behavior was conducted, further work is needed to validate the algorithm using in situ data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140006607','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140006607"><span>Mean Dynamic Topography of the Arctic <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Farrell, Sinead Louise; Mcadoo, David C.; Laxon, Seymour W.; Zwally, H. Jay; Yi, Donghui; Ridout, Andy; Giles, Katherine</p> <p>2012-01-01</p> <p>ICESat and Envisat altimetry data provide measurements of the instantaneous sea surface height (SSH) across the Arctic <span class="hlt">Ocean</span>, using lead and <span class="hlt">open</span> <span class="hlt">water</span> elevation within the sea ice pack. First, these data were used to derive two independent mean sea surface (MSS) models by stacking and averaging along-track SSH profiles gathered between 2003 and 2009. The ICESat and Envisat MSS data were combined to construct the high-resolution ICEn MSS. Second, we estimate the 5.5-year mean dynamic topography (MDT) of the Arctic <span class="hlt">Ocean</span> by differencing the ICEn MSS with the new GOCO02S geoid model, derived from GRACE and GOCE gravity. Using these satellite-only data we map the major features of Arctic <span class="hlt">Ocean</span> dynamical height that are consistent with in situ observations, including the topographical highs and lows of the Beaufort and Greenland Gyres, respectively. Smaller-scale MDT structures remain largely unresolved due to uncertainties in the geoid at short wavelengths.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19980111031','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19980111031"><span>Contribution of Phycoerythrin-Containing Phytoplankton to Remotely Sensed Signals in the <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Vernet, Maria; Iturriaga, Rodolfo</p> <p>1997-01-01</p> <p>The purpose of this project was to evaluate the importance of phycoerythrin-containing phytoplankton, in particular coccoid cyanobacteria, to remote sensing. We proposed to estimate cyanobacteria abundance and pigmentation and their relationship to <span class="hlt">water</span>-column optics. We have estimated the contribution of cyanobacteria to scattering and backscattering in both <span class="hlt">open</span> <span class="hlt">ocean</span> (Sargasso Sea) and coastal <span class="hlt">waters</span> (western coast of North Atlantic and the California Current). Sampling and data processing is performed. Relationship between <span class="hlt">water</span> column optics and phycoerythrin concentration and algorithms development are being carried out.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2012-title46-vol3/pdf/CFR-2012-title46-vol3-sec80-15.pdf','CFR2012'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2012-title46-vol3/pdf/CFR-2012-title46-vol3-sec80-15.pdf"><span>46 CFR 80.15 - <span class="hlt">Ocean</span> voyage.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2012&page.go=Go">Code of Federal Regulations, 2012 CFR</a></p> <p></p> <p>2012-10-01</p> <p>... 46 Shipping 3 2012-10-01 2012-10-01 false <span class="hlt">Ocean</span> voyage. 80.15 Section 80.15 Shipping COAST GUARD... REGISTRY § 80.15 <span class="hlt">Ocean</span> voyage. An <span class="hlt">ocean</span> voyage for the purposes of this part means: A voyage on any body of <span class="hlt">water</span> seaward of the low <span class="hlt">water</span> mark such as an <span class="hlt">ocean</span> or arm thereof, other major bodies of <span class="hlt">water</span> such as...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2013-title46-vol3/pdf/CFR-2013-title46-vol3-sec80-15.pdf','CFR2013'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2013-title46-vol3/pdf/CFR-2013-title46-vol3-sec80-15.pdf"><span>46 CFR 80.15 - <span class="hlt">Ocean</span> voyage.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2013&page.go=Go">Code of Federal Regulations, 2013 CFR</a></p> <p></p> <p>2013-10-01</p> <p>... 46 Shipping 3 2013-10-01 2013-10-01 false <span class="hlt">Ocean</span> voyage. 80.15 Section 80.15 Shipping COAST GUARD... REGISTRY § 80.15 <span class="hlt">Ocean</span> voyage. An <span class="hlt">ocean</span> voyage for the purposes of this part means: A voyage on any body of <span class="hlt">water</span> seaward of the low <span class="hlt">water</span> mark such as an <span class="hlt">ocean</span> or arm thereof, other major bodies of <span class="hlt">water</span> such as...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2010-title46-vol3/pdf/CFR-2010-title46-vol3-sec80-15.pdf','CFR'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2010-title46-vol3/pdf/CFR-2010-title46-vol3-sec80-15.pdf"><span>46 CFR 80.15 - <span class="hlt">Ocean</span> voyage.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2010&page.go=Go">Code of Federal Regulations, 2010 CFR</a></p> <p></p> <p>2010-10-01</p> <p>... 46 Shipping 3 2010-10-01 2010-10-01 false <span class="hlt">Ocean</span> voyage. 80.15 Section 80.15 Shipping COAST GUARD... REGISTRY § 80.15 <span class="hlt">Ocean</span> voyage. An <span class="hlt">ocean</span> voyage for the purposes of this part means: A voyage on any body of <span class="hlt">water</span> seaward of the low <span class="hlt">water</span> mark such as an <span class="hlt">ocean</span> or arm thereof, other major bodies of <span class="hlt">water</span> such as...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2014-title46-vol3/pdf/CFR-2014-title46-vol3-sec80-15.pdf','CFR2014'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2014-title46-vol3/pdf/CFR-2014-title46-vol3-sec80-15.pdf"><span>46 CFR 80.15 - <span class="hlt">Ocean</span> voyage.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2014&page.go=Go">Code of Federal Regulations, 2014 CFR</a></p> <p></p> <p>2014-10-01</p> <p>... 46 Shipping 3 2014-10-01 2014-10-01 false <span class="hlt">Ocean</span> voyage. 80.15 Section 80.15 Shipping COAST GUARD... REGISTRY § 80.15 <span class="hlt">Ocean</span> voyage. An <span class="hlt">ocean</span> voyage for the purposes of this part means: A voyage on any body of <span class="hlt">water</span> seaward of the low <span class="hlt">water</span> mark such as an <span class="hlt">ocean</span> or arm thereof, other major bodies of <span class="hlt">water</span> such as...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2011-title46-vol3/pdf/CFR-2011-title46-vol3-sec80-15.pdf','CFR2011'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2011-title46-vol3/pdf/CFR-2011-title46-vol3-sec80-15.pdf"><span>46 CFR 80.15 - <span class="hlt">Ocean</span> voyage.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2011&page.go=Go">Code of Federal Regulations, 2011 CFR</a></p> <p></p> <p>2011-10-01</p> <p>... 46 Shipping 3 2011-10-01 2011-10-01 false <span class="hlt">Ocean</span> voyage. 80.15 Section 80.15 Shipping COAST GUARD... REGISTRY § 80.15 <span class="hlt">Ocean</span> voyage. An <span class="hlt">ocean</span> voyage for the purposes of this part means: A voyage on any body of <span class="hlt">water</span> seaward of the low <span class="hlt">water</span> mark such as an <span class="hlt">ocean</span> or arm thereof, other major bodies of <span class="hlt">water</span> such as...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20000092882','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20000092882"><span>Projected Impact of Climate Change on the <span class="hlt">Water</span> and Salt Budgets of the Arctic <span class="hlt">Ocean</span> by a Global Climate Model</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Miller, James R.; Russell, Gary L.</p> <p>1996-01-01</p> <p>The annual flux of freshwater into the Arctic <span class="hlt">Ocean</span> by the atmosphere and rivers is balanced by the export of sea ice and <span class="hlt">oceanic</span> freshwater. Two 150-year simulations of a global climate model are used to examine how this balance might change if atmospheric greenhouse gases (GHGs) increase. Relative to the control, the last 50-year period of the GHG experiment indicates that the total inflow of <span class="hlt">water</span> from the atmosphere and rivers increases by 10% primarily due to an increase in river discharge, the annual sea-ice export decreases by about half, the <span class="hlt">oceanic</span> liquid <span class="hlt">water</span> export increases, salinity decreases, sea-ice cover decreases, and the total mass and sea-surface height of the Arctic <span class="hlt">Ocean</span> increase. The closed, compact, and multi-phased nature of the hydrologic cycle in the Arctic <span class="hlt">Ocean</span> makes it an ideal test of <span class="hlt">water</span> budgets that could be included in model intercomparisons.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1998Natur.393..774T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1998Natur.393..774T"><span>Influence of iron availability on nutrient consumption ratio of diatoms in <span class="hlt">oceanic</span> <span class="hlt">waters</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Takeda, Shigenobu</p> <p>1998-06-01</p> <p>The major nutrients (nitrate, phosphate and silicate) needed for phytoplankton growth are abundant in the surface <span class="hlt">waters</span> of the subarctic Pacific, equatorial Pacific and Southern <span class="hlt">oceans</span>, but this growth is limited by the availability of iron. Under iron-deficient conditions, phytoplankton exhibit reduced uptake of nitrate and lower cellular levels of carbon, nitrogen and phosphorus. Here I describe seawater and culture experiments which show that iron limitation can also affect the ratio of consumed silicate to nitrate and phosphate. In iron-limited <span class="hlt">waters</span> from all three of the aforementioned environments, addition of iron to phytoplankton assemblages in incubation bottles halved the silicate:nitrate and silicate:phosphate consumption ratios, in spite of the preferential growth of diatoms (silica-shelled phytoplankton). The nutrient consumption ratios of the phytoplankton assemblage from the Southern <span class="hlt">Ocean</span> were similar to those of an iron-deficient laboratory culture of Antarctic diatoms, which exhibit increased cellular silicon or decreased cellular nitrogen and phosphorus in response to iron limitation. Iron limitation therefore increases the export of biogenic silicon, relative to nitrogen and phosphorus, from the surface to deeper <span class="hlt">waters</span>. These findings suggest how the sedimentary records of carbon and silicon deposition in the glacial Southern <span class="hlt">Ocean</span> can be consistent with the idea that changes in productivity, and thus in drawdown of atmospheric CO2, during the last glaciation were stimulated by changes in iron inputs from atmospheric dust.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20000054691&hterms=recycling&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Drecycling','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20000054691&hterms=recycling&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Drecycling"><span>Extratropical Influence of Sea Surface Temperature and Wind on <span class="hlt">Water</span> Recycling Rate Over <span class="hlt">Oceans</span> and Coastal Lands</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hu, Hua; Liu, W. Timothy</p> <p>1999-01-01</p> <p><span class="hlt">Water</span> vapor and precipitation are two important parameters confining the hydrological cycle in the atmosphere and over the <span class="hlt">ocean</span> surface. In the extratropical areas, due to variations of midlatitude storm tracks and subtropical jetstreams, <span class="hlt">water</span> vapor and precipitation have large variability. Recently, a concept of <span class="hlt">water</span> recycling rate defined previously by Chahine et al. (GEWEX NEWS, August, 1997) has drawn increasing attention. The recycling rate of moisture is calculated as the ratio of precipitation to total precipitable <span class="hlt">water</span> (its inverse is the <span class="hlt">water</span> residence time). In this paper, using multi-sensor spacebased measurements we will study the role of sea surface temperature and <span class="hlt">ocean</span> surface wind in determining the <span class="hlt">water</span> recycling rate over <span class="hlt">oceans</span> and coastal lands. Response of <span class="hlt">water</span> recycling rate in midlatitudes to the El Nino event will also be discussed. Sea surface temperature data are derived from satellite observations from the Advanced Very High Resolution Radiometer (AVHRR) blended with in situ measurements, available for the period 1982-1998. Global sea surface wind observations are obtained from spaceborne scatterometers aboard on the European Remote-Sensing Satellite (ERS1 and 2), available for the period 1991-1998. Global total precipitable <span class="hlt">water</span> provided by the NASA <span class="hlt">Water</span> Vapor Project (NVAP) is available for the period 1988-1995. Global monthly mean precipitation provided by the Global Precipitation Climatology Project (GPCP) is available for the period 1987-1998.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1613996B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1613996B"><span>Atmospheric Nitrogen Deposition to the <span class="hlt">Oceans</span>: Observation- and Model-Based Estimates</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Baker, Alex; Altieri, Katye; Okin, Greg; Dentener, Frank; Uematsu, Mitsuo; Kanakidou, Maria; Sarin, Manmohan; Duce, Robert; Galloway, Jim; Keene, Bill; Singh, Arvind; Zamora, Lauren; Lamarque, Jean-Francois; Hsu, Shih-Chieh</p> <p>2014-05-01</p> <p>The reactive nitrogen (Nr) burden of the atmosphere has been increased by a factor of 3-4 by anthropogenic activity since the industrial revolution. This has led to large increases in the deposition of nitrate and ammonium to the surface <span class="hlt">waters</span> of the <span class="hlt">open</span> <span class="hlt">ocean</span>, particularly downwind of major human population centres, such as those in North America, Europe and Southeast Asia. In oligotrophic <span class="hlt">waters</span>, this deposition has the potential to significantly impact marine productivity and the global carbon cycle. Global-scale understanding of N deposition to the <span class="hlt">oceans</span> is reliant on our ability to produce effective models of reactive nitrogen emission, atmospheric chemistry, transport and deposition (including deposition to the land surface). The Atmospheric Chemistry and Climate Model Intercomparison Project (ACCMIP) recently completed a multi-model analysis of global N deposition, including comparisons to wet deposition observations from three regional networks in North America, Europe and Southeast Asia (Lamarque et al., Atmos. Chem. Phys., 13, 7977-8018, 2013). No similar datasets exist which would allow observation - model comparisons of wet deposition for the <span class="hlt">open</span> <span class="hlt">oceans</span>, because long-term wet deposition records are available for only a handful of remote island sites and rain collection over the <span class="hlt">open</span> <span class="hlt">ocean</span> itself is very difficult. In this work we attempt instead to use ~2600 observations of aerosol nitrate and ammonium concentrations, acquired chiefly from sampling aboard ships in the period 1995 - 2012, to assess the ACCMIP N deposition fields over the remote <span class="hlt">ocean</span>. This database is non-uniformly distributed in time and space. We selected four <span class="hlt">ocean</span> regions (the eastern North Atlantic, the South Atlantic, the northern Indian <span class="hlt">Ocean</span> and northwest Pacific) where we considered the density and distribution of observational data is sufficient to provide effective comparison to the model ensemble. Two of these regions are adjacent to the land networks used in the ACCMIP</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1991DSJ....41....1R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1991DSJ....41....1R"><span>The origin of blue-green window and the propagation of radiation in <span class="hlt">ocean</span> <span class="hlt">waters</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Reghunath, A. T.; Venkataramanan, V.; Suviseshamuthu, D. Victor; Krishnamohan, R.; Prasad, B. Raghavendra</p> <p>1991-01-01</p> <p>A review of the present knowledge about the origin of blue-green window in the attenuation spectrum of <span class="hlt">ocean</span> <span class="hlt">waters</span> is presented. The various physical mechanisms which contribute to the formation of the window are dealt separately and discussed. The typical values of attenuation coefficient arising out of the various processes are compiled to obtain the total beam attenuation coefficient. These values are then compared with measured values of attenuation coefficient for <span class="hlt">ocean</span> <span class="hlt">waters</span> collected from Arabian sea and Bay of Bengal. The region of minimum attenuation in pure particle-free sea <span class="hlt">water</span> is found to be at 450 to 500 nm. It is shown that in the presence of suspended particles and chlorophyll, the window shifts to longer wavelength side. Some suggestions for future work in this area are also given in the concluding section.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20060042455&hterms=water+sensor&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dwater%2Bsensor','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060042455&hterms=water+sensor&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dwater%2Bsensor"><span>Atmospheric moisture transport and fresh <span class="hlt">water</span> flux over <span class="hlt">oceans</span> derived from spacebased sensors</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Liu, W. T.; Tang, W.</p> <p>2001-01-01</p> <p>preliminary results will be shown to demonstrate the application of spacebased IMT and fresh <span class="hlt">water</span> flux in <span class="hlt">ocean</span>-atmosphere-land interaction studies, such as the hydrologica balance on Amazon rainfall and Indian monsoon.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19990076692&hterms=atmospheric+pressure&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Datmospheric%2Bpressure','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19990076692&hterms=atmospheric+pressure&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Datmospheric%2Bpressure"><span>Seasonal Variations of the Earth's Gravitational Field: An Analysis of Atmospheric Pressure, <span class="hlt">Ocean</span> Tidal, and Surface <span class="hlt">Water</span> Excitation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Dong, D,; Gross, R.S.; Dickey, J.</p> <p>1996-01-01</p> <p>Monthly mean gravitational field parameters (denoted here as C(sub even)) that represent linear combinations of the primarily even degree zonal spherical harmonic coefficients of the Earth's gravitational field have been recovered using LAGEOS I data and are compared with those derived from gridded global surface pressure data of the National meteorological center (NMC) spanning 1983-1992. The effect of equilibrium <span class="hlt">ocean</span> tides and surface <span class="hlt">water</span> variations are also considered. Atmospheric pressure and surface <span class="hlt">water</span> fluctuations are shown to be the dominant cause of observed annual C(sub even) variations. Closure with observations is seen at the 1sigma level when atmospheric pressure, <span class="hlt">ocean</span> tide and surface <span class="hlt">water</span> effects are include. Equilibrium <span class="hlt">ocean</span> tides are shown to be the main source of excitation at the semiannual period with closure at the 1sigma level seen when both atmospheric pressure and <span class="hlt">ocean</span> tide effects are included. The inverted barometer (IB) case is shown to give the best agreement with the observation series. The potential of the observed C(sub even) variations for monitoring mass variations in the polar regions of the Earth and the effect of the land-<span class="hlt">ocean</span> mask in the IB calculation are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSEC34D1210S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSEC34D1210S"><span>VIIRS validation and algorithm development efforts in coastal and inland <span class="hlt">Waters</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stengel, E.; Ondrusek, M.</p> <p>2016-02-01</p> <p>Accurate satellite <span class="hlt">ocean</span> color measurements in coastal and inland <span class="hlt">waters</span> are more challenging than <span class="hlt">open-ocean</span> measurements. Complex <span class="hlt">water</span> and atmospheric conditions can limit the utilization of remote sensing data in coastal <span class="hlt">waters</span> where it is most needed. The Coastal Optical Characterization Experiment (COCE) is an ongoing project at NOAA/NESDIS/STAR Satellite Oceanography and Climatology Division. The primary goals of COCE are satellite <span class="hlt">ocean</span> color validation and application development. Currently, this effort concentrates on the initialization and validation of the Joint Polar Satellite System (JPSS) VIIRS sensor using a Satlantic HyperPro II radiometer as a validation tool. A report on VIIRS performance in coastal <span class="hlt">waters</span> will be given by presenting comparisons between in situ ground truth measurements and VIIRS retrievals made in the Chesapeake Bay, and inland <span class="hlt">waters</span> of the Gulf of Mexico and Puerto Rico. The COCE application development effort focuses on developing new <span class="hlt">ocean</span> color satellite remote sensing tools for monitoring relevant coastal <span class="hlt">ocean</span> parameters. A new VIIRS total suspended matter algorithm will be presented for the Chesapeake Bay. These activities improve the utility of <span class="hlt">ocean</span> color satellite data in monitoring and analyzing coastal and <span class="hlt">oceanic</span> processes. Progress on these activities will be reported.</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://adsabs.harvard.edu/abs/2015AGUFMPP33B2313C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMPP33B2313C"><span>Fish Productivity in <span class="hlt">Open-Ocean</span> Gyre Systems in the Late Oligocene and Miocene</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cuevas, J. M.; Sibert, E. C.; Norris, R. D.</p> <p>2015-12-01</p> <p>Understanding how marine ecosystems respond to climate change is very important as we continue to warm the climate. Fish represent a critical protein source for a significant portion of the global population, and as such, an understanding of fish production and its interactions with climate change may help better prepare for the future. Ichthyoliths, fossil fish teeth and shark scales, are a novel fossil group which can be used as an indicator for fish productivity. Several important climate events occurred during the Miocene (7 to 23 Ma), including the Middle Miocene Climatic Optimum. Here we reconstruct fish production from across the Miocene from Pacific and Atlantic <span class="hlt">Ocean</span> gyres. South Atlantic samples, from Deep Sea Drilling Program (DSDP) Site 522 spanning from 30 to 20 Ma, show fairly variable numbers in the Oligocene (ranging from 100 to 800 ich/cm2/yr), but stabilization in the Early Miocene (around 400 ich/cm2/yr), suggesting that the beginning of the Miocene brought consistent conditions for fish production. In the North Pacific, our record from <span class="hlt">Ocean</span> Drilling Program (ODP) Site 886 shows a distinct crash in fish productivity at 11 Ma, from 3500 ich/cm2/yr to a steady decline around 100 ich/cm2/yr for the next million years. This crash is followed by a marked increase in the presence of diatoms and biogenous opal. This is somewhat surprising, since in modern <span class="hlt">oceanic</span> systems, an increase in diatoms and other large-celled phytoplankton is associated with shorter, more efficient food chains and higher levels of fish. It is also interesting to note that denticles remain consistently low at both sites, indicating consistently low shark populations through this time period. Together, these results suggest that the Late Oligocene and Miocene was a time of variable fish production and provide a window into understanding of dynamic ecosystem changes through the Miocene in <span class="hlt">open-ocean</span> gyre ecosystems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20150007763&hterms=topography&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dtopography','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20150007763&hterms=topography&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dtopography"><span>KARIN: The Ka-Band Radar Interferometer for the Proposed Surface <span class="hlt">Water</span> and <span class="hlt">Ocean</span> Topography (SWOT) Mission</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Esteban-Fernandez, Daniel; Peral, Eva; McWatters, Dalia; Pollard, Brian; Rodriguez, Ernesto; Hughes, Richard</p> <p>2013-01-01</p> <p>Over the last two decades, several nadir profiling radar altimeters have provided our first global look at the <span class="hlt">ocean</span> basin-scale circulation and the <span class="hlt">ocean</span> mesoscale at wavelengths longer than 100 km. Due to sampling limitations, nadir altimetry is unable to resolve the small wavelength <span class="hlt">ocean</span> mesoscale and sub-mesoscale that are responsible for the vertical mixing of <span class="hlt">ocean</span> heat and gases and the dissipation of kinetic energy from large to small scales. The proposed Surface <span class="hlt">Water</span> and <span class="hlt">Ocean</span> Topography (SWOT) mission would be a partnership between NASA, CNES (Centre National d'Etudes Spaciales) and the Canadian Space Agency, and would have as one of its main goals the measurement of <span class="hlt">ocean</span> topography with kilometer-scale spatial resolution and centimeter scale accuracy. In this paper, we provide an overview of all <span class="hlt">ocean</span> error sources that would contribute to the SWOT mission.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhDT.........5F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhDT.........5F"><span>The polarization of light in coastal and <span class="hlt">open</span> <span class="hlt">oceans</span>: Reflection and transmission by the air-sea interface and application for the retrieval of <span class="hlt">water</span> optical properties</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Foster, Robert</p> <p></p> <p>For decades, traditional remote sensing retrieval methods that rely solely on the spectral intensity of the <span class="hlt">water</span>-leaving light have provided indicators of aquatic ecosystem health. With the increasing demand for new <span class="hlt">water</span> quality indicators and improved accuracy of existing ones, the limits of traditional remote sensing approaches are becoming apparent. Use of the additional information intrinsic to the polarization state of light is therefore receiving more attention. One of the major challenges inherent in any above-surface determination of the <span class="hlt">water</span>-leaving radiance, scalar or vector, is the removal of extraneous light which has not interacted with the <span class="hlt">water</span> body and is therefore not useful for remote sensing of the <span class="hlt">water</span> itself. Due in-part to the lack of a proven alternative, existing polarimeter installations have thus far assumed that such light was reflected by a flat sea surface, which can lead to large inaccuracies in the <span class="hlt">water</span>-leaving polarization signal. This dissertation rigorously determines the full Mueller matrices for both surface-reflected skylight and upwardly transmitted light by a wind-driven <span class="hlt">ocean</span> surface. A Monte Carlo code models the surface in 3D and performs polarized ray-tracing, while a vector radiative transfer (VRT) simulation generates polarized light distributions from which the initial Stokes vector for each ray is inferred. Matrices are computed for the observable range of surface wind speeds, viewing and solar geometries, and atmospheric aerosol loads. Radiometer field-of-view effects are also assessed. Validation of the results is achieved using comprehensive VRT simulations of the atmosphere-<span class="hlt">ocean</span> system based on several oceanographic research cruises and specially designed polarimeters developed by the City College of New York: one submerged beneath the surface and one mounted on a research vessel. When available, additional comparisons are made at 9 km altitude with the NASA Research Scanning Polarimeter (RSP). Excellent</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017OcMod.113...66M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017OcMod.113...66M"><span>Flow splitting in numerical simulations of <span class="hlt">oceanic</span> dense-<span class="hlt">water</span> outflows</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marques, Gustavo M.; Wells, Mathew G.; Padman, Laurie; Özgökmen, Tamay M.</p> <p>2017-05-01</p> <p>Flow splitting occurs when part of a gravity current becomes neutrally buoyant and separates from the bottom-trapped plume as an interflow. This phenomenon has been previously observed in laboratory experiments, small-scale <span class="hlt">water</span> bodies (e.g., lakes) and numerical studies of small-scale systems. Here, the potential for flow splitting in <span class="hlt">oceanic</span> gravity currents is investigated using high-resolution (Δx = Δz = 5 m) two-dimensional numerical simulations of gravity flows into linearly stratified environments. The model is configured to solve the non-hydrostatic Boussinesq equations without rotation. A set of experiments is conducted by varying the initial buoyancy number B0 =Q0N3 /g‧2 (where Q0 is the volume flux of the dense <span class="hlt">water</span> flow per unit width, N is the ambient stratification and g‧ is the reduced gravity), the bottom slope (α) and the turbulent Prandtl number (Pr). Regardless of α or Pr, when B0 ≤ 0.002 the outflow always reaches the deep <span class="hlt">ocean</span> forming an underflow. Similarly, when B0 ≥ 0.13 the outflow always equilibrates at intermediate depths, forming an interflow. However, when B0 ∼ 0.016, flow splitting always occurs when Pr ≥ 10, while interflows always occur for Pr = 1. An important characteristic of simulations that result in flow splitting is the development of Holmboe-like interfacial instabilities and flow transition from a supercritical condition, where the Froude number (Fr) is greater than one, to a slower and more uniform subcritical condition (Fr < 1). This transition is associated with an internal hydraulic jump and consequent mixing enhancement. Although our experiments do not take into account three-dimensionality and rotation, which are likely to influence mixing and the transition between flow regimes, a comparison between our results and <span class="hlt">oceanic</span> observations suggests that flow splitting may occur in dense-<span class="hlt">water</span> outflows with weak ambient stratification, such as Antarctic outflows.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005AGUFM.P11A0088A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005AGUFM.P11A0088A"><span><span class="hlt">Water</span>-Ammonia Ionic <span class="hlt">Ocean</span> on Uranus and Neptune-Clue from Tropospheric Hydrogen Sulfide Clouds</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Atreya, S. K.; Egeler, P. A.; Wong, A.</p> <p>2005-12-01</p> <p>Interior models of the ice-giants, Uranus and Neptune, predict a <span class="hlt">water</span>-ammonia ionic <span class="hlt">ocean</span> at tens of kilobar pressure [1,2]. If correct, its implication for planetary formation models is profound. In this presentation we demonstrate that the existence of an ionic <span class="hlt">ocean</span> will manifest itself in the planets' tropospheric cloud structure, particularly in the form of a hydrogen sulfide, i.e. H2S-ice, cloud. In fact, an H2S cloud was introduced ad hoc in the 3-5 bar region to explain microwave absorption [3] and the methane [4] observations, but its presence cannot be proved in the absence of entry probes. Our equilibrium cloud condensation model (ECCM) shows that an H2S-ice cloud does not form when conventional enrichment factors (20-30× solar at Uranus, and 30-50× solar at Neptune) are employed for all heavy elements (mass >4) [5]. However, a deep ``cloud'' composed of a weak solution of ammonia and <span class="hlt">water</span> forms, and its base is at 370 and 500 bars, respectively, for 30× solar and 50× solar enrichment factors. If an ionic ``<span class="hlt">ocean</span>'' exists much deeper, <span class="hlt">water</span> vapor, as well as ammonia dissolved in it, would be severely depleted at levels above this <span class="hlt">ocean</span>. The consequences of such <span class="hlt">water</span> vapor and ammonia depletions are that (1) clouds of <span class="hlt">water</span> and ammonia, if present, are much less prominent; (2) only small amount of H2S vapor is removed by NH3, to form an NH4SH cloud; so that (3) a cloud of H2S-ice can now form; and (4) an H2O ``<span class="hlt">ocean</span>'' in the 1-kilobar region [6] does not form. This scenario has important implications for the design of entry probe missions, as measurements to only 10-20 bars, rather than kilobar levels, will need to be made. The heavy elements, Ar, Kr, Xe, Ne, C, and S, as well as He, D/H, GeH4, AsH3, PH3, and CO can all be accessed at pressures less than 20 bars. These measurements are critical for constraining the formation models [5,7,8]. Measurement of <span class="hlt">water</span> in the well-mixed region of Uranus and Neptune is technologically highly challenging</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006JGRC..111.8005U','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006JGRC..111.8005U"><span>Vertical distribution of phytoplankton communities in <span class="hlt">open</span> <span class="hlt">ocean</span>: An assessment based on surface chlorophyll</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Uitz, Julia; Claustre, Hervé; Morel, André; Hooker, Stanford B.</p> <p>2006-08-01</p> <p>The present study examines the potential of using the near-surface chlorophyll a concentration ([Chla]surf), as it can be derived from <span class="hlt">ocean</span> color observation, to infer the column-integrated phytoplankton biomass, its vertical distribution, and ultimately the community composition. Within this context, a large High-Performance Liquid Chromatography (HPLC) pigment database was analyzed. It includes 2419 vertical pigment profiles, sampled in case 1 <span class="hlt">waters</span> with various trophic states (0.03-6 mg Chla m-3). The relationships between [Chla]surf and the chlorophyll a vertical distribution, as previously derived by Morel and Berthon (1989), are fully confirmed. This agreement makes it possible to go further and to examine if similar relationships between [Chla]surf and the phytoplankton assemblage composition along the vertical can be derived. Thanks to the detailed pigment composition, and use of specific pigment biomarkers, the contribution to the local chlorophyll a concentration of three phytoplankton groups can be assessed. With some cautions, these groups coincide with three size classes, i.e., microplankton, nanoplankton and picoplankton. Corroborating previous regional findings (e.g., large species dominate in eutrophic environments, whereas tiny phytoplankton prevail in oligotrophic zones), the present results lead to an empirical parameterization applicable to most <span class="hlt">oceanic</span> <span class="hlt">waters</span>. The predictive skill of this parameterization is satisfactorily tested on a separate data set. With such a tool, the vertical chlorophyll a profiles of each group can be inferred solely from the knowledge of [Chla]surf. By combining this tool with satellite <span class="hlt">ocean</span> color data, it becomes possible to quantify on a global scale the phytoplankton biomass associated with each of the three algal assemblages.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016OcSci..12..101D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016OcSci..12..101D"><span><span class="hlt">Ocean</span> modelling for aquaculture and fisheries in Irish <span class="hlt">waters</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dabrowski, T.; Lyons, K.; Cusack, C.; Casal, G.; Berry, A.; Nolan, G. D.</p> <p>2016-01-01</p> <p>The Marine Institute, Ireland, runs a suite of operational regional and coastal <span class="hlt">ocean</span> models. Recent developments include several tailored products that focus on the key needs of the Irish aquaculture sector. In this article, an overview of the products and services derived from the models are presented. The authors give an overview of a shellfish model developed in-house and that was designed to predict the growth, the physiological interactions with the ecosystem, and the level of coliform contamination of the blue mussel. As such, this model is applicable in studies on the carrying capacity of embayments, assessment of the impacts of pollution on aquaculture grounds, and the determination of shellfish <span class="hlt">water</span> classes. Further services include the assimilation of the model-predicted shelf <span class="hlt">water</span> movement into a new harmful algal bloom alert system used to inform end users of potential toxic shellfish events and high biomass blooms that include fish-killing species. Models are also used to identify potential sites for offshore aquaculture, to inform studies of potential cross-contamination in farms from the dispersal of planktonic sea lice larvae and other pathogens that can infect finfish, and to provide modelled products that underpin the assessment and advisory services on the sustainable exploitation of the resources of marine fisheries. This paper demonstrates that <span class="hlt">ocean</span> models can provide an invaluable contribution to the sustainable blue growth of aquaculture and fisheries.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSMM24C0450A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSMM24C0450A"><span>Exploring the functional side of the <span class="hlt">Ocean</span> Sampling Day metagenomes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Antonio, F. G.; Kottmann, R.; Wallom, D.; Glöckner, F. O.</p> <p>2016-02-01</p> <p>The <span class="hlt">Ocean</span> Sampling Day (OSD) is a simultaneous, collaborative, standardized, and global mega-sequencing campaign to analyze marine microbial community composition and functional traits. 150 metagenomes were sequenced from the first OSD in June 2014 including a rich set of environmental and oceanographic measurements. Unlike other <span class="hlt">ocean</span> mega-surveys such as Global <span class="hlt">Ocean</span> Sampling (GOS) or the TARA expedition that mostly sampled <span class="hlt">open</span> <span class="hlt">ocean</span> <span class="hlt">waters</span> most of the OSD samples are from coastal sampling sites, an area not previously well studied in this regard. The result is that OSD adds more than three million new genes to the recently published <span class="hlt">Ocean</span> Microbial-Reference Gene Catalog (Sunawaga et al., 2015). This allows us to significantly increase our knowledge of the <span class="hlt">ocean</span> microbiome, identify hot-spots of novelty in terms of function and investigate the impact of human activities on <span class="hlt">oceans</span> coastal areas where there is the largest interaction between dense human populations and the marine world. Additionally, these cumulative samples, related in time, space and environmental parameters, are providing insights into fundamental rules describing microbial diversity and function and contribute to the blue economy through the identification of novel <span class="hlt">ocean</span>-derived biotechnologies. References: Sunagawa, Coelho, Chaffron, et al. (2015, May). Structure and function of the global <span class="hlt">ocean</span> microbiome. Science, 348(6237), 126135.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1918978S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1918978S"><span>Assessing data assimilation and model boundary error strategies for high resolution <span class="hlt">ocean</span> model downscaling in the Northern North Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sandvig Mariegaard, Jesper; Huiban, Méven Robin; Tornfeldt Sørensen, Jacob; Andersson, Henrik</p> <p>2017-04-01</p> <p>Determining the optimal domain size and associated position of <span class="hlt">open</span> boundaries in local high-resolution downscaling <span class="hlt">ocean</span> models is often difficult. As an important input data set for downscaling <span class="hlt">ocean</span> modelling, the European Copernicus Marine Environment Monitoring Service (CMEMS) provides baroclinic initial and boundary conditions for local <span class="hlt">ocean</span> models. Tidal dynamics is often neglected in CMEMS services at large scale but tides are generally crucial for coastal <span class="hlt">ocean</span> dynamics. To address this need, tides can be superposed via Flather (1976) boundary conditions and the combined flow downscaled using unstructured mesh. The surge component is also only partially represented in selected CMEMS products and must be modelled inside the domain and modelled independently and superposed if the domain becomes too small to model the effect in the downscaling model. The tide and surge components can generally be improved by assimilating <span class="hlt">water</span> level from tide gauge and altimetry data. An intrinsic part of the problem is to find the limitations of local scale data assimilation and the requirement for consistency between the larger scale <span class="hlt">ocean</span> models and the local scale assimilation methodologies. This contribution investigates the impact of domain size and associated positions of <span class="hlt">open</span> boundaries with and without data assimilation of <span class="hlt">water</span> level. We have used the baroclinic <span class="hlt">ocean</span> model, MIKE 3 FM, and its newly re-factored built-in data assimilation package. We consider boundary conditions of salinity, temperature, <span class="hlt">water</span> level and depth varying currents from the Global CMEMS 1/4 degree resolution model from 2011, where in situ ADCP velocity data is available for validation. We apply data assimilation of in-situ tide gauge <span class="hlt">water</span> levels and along track altimetry surface elevation data from selected satellites. The MIKE 3 FM data assimilation model which use the Ensemble Kalman filter have recently been parallelized with MPI allowing for much larger applications running on HPC</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70031513','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70031513"><span>MODIS imagery as a tool for synoptic <span class="hlt">water</span> quality assessments in the southern California coastal <span class="hlt">ocean</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>Nezlin, N.P.; DiGiacomo, P.M.; Jones, B.H.; Reifel, K.M.; Warrick, J.A.; Johnson, S.C.; Mengel, M.J.</p> <p>2007-01-01</p> <p>The dynamics of rainstorm plumes in the coastal <span class="hlt">waters</span> of southern California was studied during the Bight'03 Regional <span class="hlt">Water</span> Quality Program surveys. Measurements of surface salinity and bacterial counts collected from research vessels were compared to MODIS-Aqua satellite imagery. The spectra of normalized <span class="hlt">water</span>-leaving radiation (nLw) were different in plumes and ambient <span class="hlt">ocean</span> <span class="hlt">waters</span>, enabling plumes discrimination and plume area size assessments from remotely-sensed data. The plume/<span class="hlt">ocean</span> nLw differences (i.e., plume optical signatures) were most evident during first days after the rainstorm over the San Pedro shelf and in the San Diego region and less evident in Santa Monica Bay, where suspended sediments concentration in discharged <span class="hlt">water</span> was lower than in other regions. In the Ventura area, plumes contained more suspended sediments than in other regions, but the grid of ship-based stations covered only a small part of the freshwater plume and was insufficient to reveal the differences between the plume and <span class="hlt">ocean</span> optical signatures. The accuracy of plume area assessments from satellite imagery was not high (77% on average), seemingly because of inexactitude in satellite data processing. Nevertheless, satellite imagery is a useful tool for the estimation of the extent of polluted plumes, which is hardly achievable by contact methods.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007SPIE.6680E..0UL','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007SPIE.6680E..0UL"><span><span class="hlt">Ocean</span> color remote sensing of turbid plumes in the southern California coastal <span class="hlt">waters</span> during storm events</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lahet, Florence; Stramski, Dariusz</p> <p>2007-09-01</p> <p><span class="hlt">Water</span>-leaving radiance data obtained from MODIS-Aqua satellite images at spatial resolution of 250 m (band 1 at 645 nm) and 500 m (band 4 at 555 nm) were used to analyze the correlation between plume area and rainfall during strong storm events in coastal <span class="hlt">waters</span> of Southern California. Our study is focused on the area between Point Loma and the US-Mexican border in San Diego, which is influenced by terrigenous input of particulate and dissolved materials from San Diego and Tijuana watersheds and non-point sources along the shore. For several events of intense rainstorms that occurred in the winter of 2004-2005, we carried out a correlational analysis between the satellite-derived plume area and rainfall parameters. We examined several rainfall parameters and methods for the estimation of plume area. We identified the optimal threshold values of satellite-derived normalized <span class="hlt">water</span>-leaving radiances at 645 nm and 555 nm for distinguishing the plume from ambient <span class="hlt">ocean</span> <span class="hlt">waters</span>. The satellite-derived plume size showed high correlation with the amount of precipitated <span class="hlt">water</span> accumulated during storm event over the San Diego and Tijuana watersheds. Our results support the potential of <span class="hlt">ocean</span> color imagery with relatively high spatial resolution for the study of turbid plumes in the coastal <span class="hlt">ocean</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1259308','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1259308"><span>Recovery Act: <span class="hlt">Water</span> Heater ZigBee <span class="hlt">Open</span> Standard Wireless Controller</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>Butler, William P.; Buescher, Tom</p> <p>2014-04-30</p> <p>The objective of Emerson's <span class="hlt">Water</span> Heater ZigBee <span class="hlt">Open</span> Standard Wireless Controller is to support the DOE's AARA priority for Clean, Secure Energy by designing a <span class="hlt">water</span> heater control that levels out residential and small business peak electricity demand through thermal energy storage in the <span class="hlt">water</span> heater tank.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20462019','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20462019"><span>[Prokaryote diversity in <span class="hlt">water</span> environment of land-<span class="hlt">ocean</span> ecotone of Zhuhai City].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Huang, Xiao-Lan; Chen, Jian-Yao; Zhou, Shi-Ning; Xie, Li-Chun; Fu, Cong-Sheng</p> <p>2010-02-01</p> <p>By constructing 16S rDNA clone library with PCR-RFLP, the prokaryote diversity in the seawater and groundwater of land-<span class="hlt">ocean</span> ecotone of Zhuhai City was investigated, and the similarity and cluster analyses were implemented with the database of the sequences in Genbank. In the seawater, Proteobacteria was dominant, followed by Archaeon, Gemmatimonadetes, Candidate division OP3 and OP8, and Planctomycetes, etc.; while in the groundwater, Archaeon was dominant, followed by Proteobacteria, Sphingobacteria, Candidate division OP3, Actinobacterium, and Pseudomonas. The dominant taxa in the groundwater had high similarity to the unculturable groups of marine microorganisms. Large amount of bacteria capable of degrading organic matter and purifying <span class="hlt">water</span> body existed in the groundwater, suggesting that after long-term evolution, the land-<span class="hlt">ocean</span> ecotone of Zhuhai City had the characteristics of both land and <span class="hlt">ocean</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21455177','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21455177"><span>Winter cold of eastern continental boundaries induced by warm <span class="hlt">ocean</span> <span class="hlt">waters</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kaspi, Yohai; Schneider, Tapio</p> <p>2011-03-31</p> <p>In winter, northeastern North America and northeastern Asia are both colder than other regions at similar latitudes. This has been attributed to the effects of stationary weather systems set by elevated terrain (orography), and to a lack of maritime influences from the prevailing westerly winds. However, the differences in extent and orography between the two continents suggest that further mechanisms are involved. Here we show that this anomalous winter cold can result in part from westward radiation of large-scale atmospheric waves--nearly stationary Rossby waves--generated by heating of the atmosphere over warm <span class="hlt">ocean</span> <span class="hlt">waters</span>. We demonstrate this mechanism using simulations with an idealized general circulation model, with which we show that the extent of the cold region is controlled by properties of Rossby waves, such as their group velocity and its dependence on the planetary rotation rate. Our results show that warm <span class="hlt">ocean</span> <span class="hlt">waters</span> contribute to the contrast in mid-latitude winter temperatures between eastern and western continental boundaries not only by warming western boundaries, but also by cooling eastern boundaries.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003EAEJA.....5938M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003EAEJA.....5938M"><span>Indian-Southern <span class="hlt">Ocean</span> Latitudinal Transect (ISOLAT): A proposal for the recovery of high-resolution sedimentary records in the western Indian <span class="hlt">Ocean</span> sector of the Southern <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mackensen, A.; Zahn, R.; Hall, I.; Kuhn, G.; Koc, N.; Francois, R.; Hemming, S.; Goldstein, S.; Rogers, J.; Ehrmann, W.</p> <p>2003-04-01</p> <p>Quantifying <span class="hlt">oceanic</span> variability at timescales of <span class="hlt">oceanic</span>, atmospheric, and cryospheric processes are the fundamental objectives of the international IMAGES program. In this context the Southern <span class="hlt">Ocean</span> plays a leading role in that it is involved, through its influence on global <span class="hlt">ocean</span> circulation and carbon budget, with the development and maintenance of the Earth's climate system. The seas surrounding Antarctica contain the world's only zonal circum-global current system that entrains <span class="hlt">water</span> masses from the three main <span class="hlt">ocean</span> basins, and maintains the thermal isolation of Antarctica from warmer surface <span class="hlt">waters</span> to the north. Furthermore, the Southern <span class="hlt">Ocean</span> is a major site of bottom and intermediate <span class="hlt">water</span> formation and thus actively impacts the global thermohaline circulation (THC). This proposal is an outcome of the IMAGES Southern <span class="hlt">Ocean</span> Working Group and constitutes one component of a suite of new IMAGES/IODP initiatives that aim at resolving past variability of the Antarctic Circumpolar Current (ACC) on orbital and sub-orbital timescales and its involvement with rapid global <span class="hlt">ocean</span> variability and climate instability. The primary aim of this proposal is to determine millennial- to sub-centennial scale variability of the ACC and the ensuing Atlantic-Indian <span class="hlt">water</span> transports, including surface transports and deep-<span class="hlt">water</span> flow. We will focus on periods of rapid <span class="hlt">ocean</span> and climate change and assess the role of the Southern <span class="hlt">Ocean</span> in these changes, both in terms of its thermohaline circulation and biogeochemical inventories. We propose a suite of 11 sites that form a latitudinal transect across the ACC in the westernmost Indian <span class="hlt">Ocean</span> sector of the Southern <span class="hlt">Ocean</span>. The transect is designed to allow the reconstruction of ACC variability across a range of latitudes in conjunction with meridional shifts of the surface <span class="hlt">ocean</span> fronts. The northernmost reaches of the transect extend into the Agulhas Current and its retroflection system which is a key component of the THC warm <span class="hlt">water</span> return</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015E%26PSL.430...43S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015E%26PSL.430...43S"><span>A redox-stratified <span class="hlt">ocean</span> 3.2 billion years ago</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Satkoski, Aaron M.; Beukes, Nicolas J.; Li, Weiqiang; Beard, Brian L.; Johnson, Clark M.</p> <p>2015-11-01</p> <p>Before the Great Oxidation Event (GOE) 2.4-2.2 billion years ago it has been traditionally thought that <span class="hlt">oceanic</span> <span class="hlt">water</span> columns were uniformly anoxic due to a lack of oxygen-producing microorganisms. Recently, however, it has been proposed that transient oxygenation of shallow seawater occurred between 2.8 and 3.0 billion years ago. Here, we present a novel combination of stable Fe and radiogenic U-Th-Pb isotope data that demonstrate significant oxygen contents in the shallow <span class="hlt">oceans</span> at 3.2 Ga, based on analysis of the Manzimnyama Banded Iron Formation (BIF), Fig Tree Group, South Africa. This unit is exceptional in that proximal, shallow-<span class="hlt">water</span> and distal, deep-<span class="hlt">water</span> facies are preserved. When compared to the distal, deep-<span class="hlt">water</span> facies, the proximal samples show elevated U concentrations and moderately positive δ56Fe values, indicating vertical stratification in dissolved oxygen contents. Confirmation of oxidizing conditions using U abundances is robustly constrained using samples that have been closed to U and Pb mobility using U-Th-Pb geochronology. Although redox-sensitive elements have been commonly used in ancient rocks to infer redox conditions, post-depositional element mobility has been rarely tested, and U-Th-Pb geochronology can constrain <span class="hlt">open</span>- or closed-system behavior. The U abundances and δ56Fe values of the Manzimnyama BIF suggest the proximal, shallow-<span class="hlt">water</span> samples record precipitation under stronger oxidizing conditions compared to the distal deeper-<span class="hlt">water</span> facies, which in turn indicates the existence of a discrete redox boundary between deep and shallow <span class="hlt">ocean</span> <span class="hlt">waters</span> at this time; this work, therefore, documents the oldest known preserved marine redox gradient in the rock record. The relative enrichment of O2 in the upper <span class="hlt">water</span> column is likely due to the existence of oxygen-producing microorganisms such as cyanobacteria. These results provide a new approach for identifying free oxygen in Earth's ancient <span class="hlt">oceans</span>, including confirming the age of redox</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.4507G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.4507G"><span>Satellite surface salinity maps to determine fresh <span class="hlt">water</span> fluxes in the Arctic <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gabarro, Carolina; Estrella, Olmedo; Emelianov, Mikhail; Ballabrera, Joaquim; Turiel, Antonio</p> <p>2017-04-01</p> <p>Salinity and temperature gradients drive the thermohaline circulation of the <span class="hlt">oceans</span>, and play a key role in the <span class="hlt">ocean</span>-atmosphere coupling. The strong and direct interactions between the <span class="hlt">ocean</span> and the cryosphere (primarily through sea ice and ice shelves) are also a key ingredient of the thermohaline circulation. Recent observational studies have documented changes in upper Arctic <span class="hlt">Ocean</span> hydrography [1, 2]. The ESA's Soil Moisture and <span class="hlt">Ocean</span> Salinity (SMOS) mission, launched in 2009, have the objective to measure soil moisture over the continents and sea surface salinity over the <span class="hlt">oceans</span> [3]. However, SMOS is also making inroads in Cryospheric science, as the measurements of thin ice thickness and sea ice concentration. SMOS carries an innovative L-band (1.4 GHz, or 21-cm wavelength), passive interferometric radiometer (the so-called MIRAS) that measures the electromagnetic radiation emitted by the Earth's surface, at about 50 km spatial resolution wide swath (1200-km), and with a 3-day revisit time at the equator, but more frequently at the poles. Although the SMOS radiometer operating frequency offers almost the maximum sensitivity of the brightness temperature (TB) to sea surface salinity (SSS) variations, such sensitivity is rather low, even lower at cold <span class="hlt">waters</span> [4]: 90% of <span class="hlt">ocean</span> SSS values span a range of brightness temperatures of just 5K. This implies that the SMOS SSS retrieval requires a high performance of the MIRAS interferometric radiometer [5]. New algorithms, recently developed at the Barcelona Expert Center (BEC) to improve the quality of SMOS measurements [6], allow for the first time to derive cold-<span class="hlt">water</span> SSS maps from SMOS data, and to observe the variability of the SSS in the higher north Atlantic and the Arctic <span class="hlt">Ocean</span>. In this work, we will provide an assessment of the quality of these new SSS Arctic maps, and we will illustrate their potential to monitor the impact on <span class="hlt">ocean</span> state of the discharges from the main rivers to the Arctic <span class="hlt">Ocean</span>. Moreover</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4890579','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4890579"><span>Metagenomic Analysis of the Indian <span class="hlt">Ocean</span> Picocyanobacterial Community: Structure, Potential Function and Evolution</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Díez, Beatriz; Nylander, Johan A. A.; Ininbergs, Karolina; Dupont, Christopher L.; Allen, Andrew E.; Yooseph, Shibu; Rusch, Douglas B.; Bergman, Birgitta</p> <p>2016-01-01</p> <p>Unicellular cyanobacteria are ubiquitous photoautotrophic microbes that contribute substantially to global primary production. Picocyanobacteria such as Synechococcus and Prochlorococcus depend on chlorophyll a-binding protein complexes to capture light energy. In addition, Synechococcus has accessory pigments organized into phycobilisomes, and Prochlorococcus contains chlorophyll b. Across a surface <span class="hlt">water</span> transect spanning the sparsely studied tropical Indian <span class="hlt">Ocean</span>, we examined Synechococcus and Prochlorococcus occurrence, taxonomy and habitat preference in an evolutionary context. Shotgun sequencing of size fractionated microbial communities from 0.1 μm to 20 μm and subsequent phylogenetic analysis indicated that cyanobacteria account for up to 15% of annotated reads, with the genera Prochlorococcus and Synechococcus comprising 90% of the cyanobacterial reads, even in the largest size fraction (3.0–20 mm). Phylogenetic analyses of cyanobacterial light-harvesting genes (chl-binding pcb/isiA, allophycocyanin (apcAB), phycocyanin (cpcAB) and phycoerythin (cpeAB)) mostly identified picocyanobacteria clades comprised of overlapping sequences obtained from Indian <span class="hlt">Ocean</span>, Atlantic and/or Pacific <span class="hlt">Oceans</span> samples. Habitat reconstructions coupled with phylogenetic analysis of the Indian <span class="hlt">Ocean</span> samples suggested that large Synechococcus-like ancestors in coastal <span class="hlt">waters</span> expanded their ecological niche towards <span class="hlt">open</span> oligotrophic <span class="hlt">waters</span> in the Indian <span class="hlt">Ocean</span> through lineage diversification and associated streamlining of genomes (e.g. loss of phycobilisomes and acquisition of Chl b); resulting in contemporary small celled Prochlorococcus. Comparative metagenomic analysis with picocyanobacteria populations in other <span class="hlt">oceans</span> suggests that this evolutionary scenario may be globally important. PMID:27196065</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1377077-metagenomic-analysis-indian-ocean-picocyanobacterial-community-structure-potential-function-evolution','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1377077-metagenomic-analysis-indian-ocean-picocyanobacterial-community-structure-potential-function-evolution"><span>Metagenomic Analysis of the Indian <span class="hlt">Ocean</span> Picocyanobacterial Community: Structure, Potential Function and Evolution</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Diez, Beatriz; Nylander, Johan A. A.; Ininbergs, Karolina; ...</p> <p>2016-05-19</p> <p>Unicellular cyanobacteria are ubiquitous photoautotrophic microbes that contribute substantially to global primary production. Picocyanobacteria such as Synechococcus and Prochlorococcus depend on chlorophyll a-binding protein complexes to capture light energy. In addition, Synechococcus has accessory pigments organized into phycobilisomes, and Prochlorococcus contains chlorophyll b. Across a surface <span class="hlt">water</span> transect spanning the sparsely studied tropical Indian <span class="hlt">Ocean</span>, we examined Synechococcus and Prochlorococcus occurrence, taxonomy and habitat preference in an evolutionary context. Shotgun sequencing of size fractionated microbial communities from 0.1 μm to 20 μm and subsequent phylogenetic analysis indicated that cyanobacteria account for up to 15% of annotated reads, with the generamore » Prochlorococcus and Synechococcus comprising 90% of the cyanobacterial reads, even in the largest size fraction (3.0–20 mm). Phylogenetic analyses of cyanobacterial light-harvesting genes (chl-binding pcb/isiA, allophycocyanin ( apcAB), phycocyanin ( cpcAB) and phycoerythin ( cpeAB)) mostly identified picocyanobacteria clades comprised of overlapping sequences obtained from Indian <span class="hlt">Ocean</span>, Atlantic and/or Pacific <span class="hlt">Oceans</span> samples. Habitat reconstructions coupled with phylogenetic analysis of the Indian <span class="hlt">Ocean</span> samples suggested that large Synechococcus-like ancestors in coastal <span class="hlt">waters</span> expanded their ecological niche towards <span class="hlt">open</span> oligotrophic <span class="hlt">waters</span> in the Indian <span class="hlt">Ocean</span> through lineage diversification and associated streamlining of genomes (e.g. loss of phycobilisomes and acquisition of Chl b); resulting in contemporary small celled Prochlorococcus. As a result, comparative metagenomic analysis with picocyanobacteria populations in other <span class="hlt">oceans</span> suggests that this evolutionary scenario may be globally important.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1377077','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1377077"><span>Metagenomic Analysis of the Indian <span class="hlt">Ocean</span> Picocyanobacterial Community: Structure, Potential Function and Evolution</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>Diez, Beatriz; Nylander, Johan A. A.; Ininbergs, Karolina</p> <p></p> <p>Unicellular cyanobacteria are ubiquitous photoautotrophic microbes that contribute substantially to global primary production. Picocyanobacteria such as Synechococcus and Prochlorococcus depend on chlorophyll a-binding protein complexes to capture light energy. In addition, Synechococcus has accessory pigments organized into phycobilisomes, and Prochlorococcus contains chlorophyll b. Across a surface <span class="hlt">water</span> transect spanning the sparsely studied tropical Indian <span class="hlt">Ocean</span>, we examined Synechococcus and Prochlorococcus occurrence, taxonomy and habitat preference in an evolutionary context. Shotgun sequencing of size fractionated microbial communities from 0.1 μm to 20 μm and subsequent phylogenetic analysis indicated that cyanobacteria account for up to 15% of annotated reads, with the generamore » Prochlorococcus and Synechococcus comprising 90% of the cyanobacterial reads, even in the largest size fraction (3.0–20 mm). Phylogenetic analyses of cyanobacterial light-harvesting genes (chl-binding pcb/isiA, allophycocyanin ( apcAB), phycocyanin ( cpcAB) and phycoerythin ( cpeAB)) mostly identified picocyanobacteria clades comprised of overlapping sequences obtained from Indian <span class="hlt">Ocean</span>, Atlantic and/or Pacific <span class="hlt">Oceans</span> samples. Habitat reconstructions coupled with phylogenetic analysis of the Indian <span class="hlt">Ocean</span> samples suggested that large Synechococcus-like ancestors in coastal <span class="hlt">waters</span> expanded their ecological niche towards <span class="hlt">open</span> oligotrophic <span class="hlt">waters</span> in the Indian <span class="hlt">Ocean</span> through lineage diversification and associated streamlining of genomes (e.g. loss of phycobilisomes and acquisition of Chl b); resulting in contemporary small celled Prochlorococcus. As a result, comparative metagenomic analysis with picocyanobacteria populations in other <span class="hlt">oceans</span> suggests that this evolutionary scenario may be globally important.« 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_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/2016ERL....11b4007H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016ERL....11b4007H"><span>Iron fertilisation and century-scale effects of <span class="hlt">open</span> <span class="hlt">ocean</span> dissolution of olivine in a simulated CO2 removal experiment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hauck, Judith; Köhler, Peter; Wolf-Gladrow, Dieter; Völker, Christoph</p> <p>2016-02-01</p> <p>Carbon dioxide removal (CDR) approaches are efforts to reduce the atmospheric CO2 concentration. Here we use a marine carbon cycle model to investigate the effects of one CDR technique: the <span class="hlt">open</span> <span class="hlt">ocean</span> dissolution of the iron-containing mineral olivine. We analyse the maximum CDR potential of an annual dissolution of 3 Pg olivine during the 21st century and focus on the role of the micro-nutrient iron for the biological carbon pump. Distributing the products of olivine dissolution (bicarbonate, silicic acid, iron) uniformly in the global surface <span class="hlt">ocean</span> has a maximum CDR potential of 0.57 gC/g-olivine mainly due to the alkalinisation of the <span class="hlt">ocean</span>, with a significant contribution from the fertilisation of phytoplankton with silicic acid and iron. The part of the CDR caused by <span class="hlt">ocean</span> fertilisation is not permanent, while the CO2 sequestered by alkalinisation would be stored in the <span class="hlt">ocean</span> as long as alkalinity is not removed from the system. For high CO2 emission scenarios the CDR potential due to the alkalinity input becomes more efficient over time with increasing <span class="hlt">ocean</span> acidification. The alkalinity-induced CDR potential scales linearly with the amount of olivine, while the iron-induced CDR saturates at 113 PgC per century (on average ˜ 1.1 PgC yr-1) for an iron input rate of 2.3 Tg Fe yr-1 (1% of the iron contained in 3 Pg olivine). The additional iron-related CO2 uptake occurs in the Southern <span class="hlt">Ocean</span> and in the iron-limited regions of the Pacific. Effects of this approach on surface <span class="hlt">ocean</span> pH are small (\\lt 0.01).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2000GeoRL..27.2941R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2000GeoRL..27.2941R"><span>Sensitivity of equatorial Pacific and Indian <span class="hlt">Ocean</span> watermasses to the position of the Indonesian Throughflow</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rodgers, Keith B.; Latif, Mojib; Legutke, Stephanie</p> <p>2000-09-01</p> <p>The sensitivity of the thermal structure of the equatorial Pacific and Indian <span class="hlt">Ocean</span> pycnoclines to a model's representation of the Indonesian Straits connecting the two basins is investigated. Two integrations are performed using the global HOPE <span class="hlt">ocean</span> model. The initial conditions and surface forcing for both cases are identical; the only difference between the runs is that one has an <span class="hlt">opening</span> for the Indonesian Straits which spans the equator on the Pacific side, and the other has an <span class="hlt">opening</span> which lies fully north of the equator. The resulting sensitivity throughout much of the upper <span class="hlt">ocean</span> is greater than 0.5°C for both the equatorial Indian and Pacific. A realistic simulation of net Indonesian Throughflow (ITF) transport (measured in Sverdrups) is not sufficient for an adequate simulation of equatorial watermasses. The ITF must also contain a realistic admixture of northern and southern Pacific source <span class="hlt">water</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1917389S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1917389S"><span>The <span class="hlt">Ocean</span> as a teaching tool: the first MOOC on <span class="hlt">Ocean</span> Literacy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Santin, Selvaggia; Santoro, Francesca</p> <p>2017-04-01</p> <p>Education its broader understanding (in both formal and informal settings) serves as a high potential channel to reach young citizens. As a lack of sufficient '<span class="hlt">Ocean</span> Literacy' has been identified in many countries, this clearly presents a barrier for citizens to engage in <span class="hlt">ocean</span> responsible behaviour or consider <span class="hlt">ocean</span>-related careers. In order to sensitize and enable teachers and students to incorporate <span class="hlt">ocean</span> literacy into educational programmes we build up a first Massive <span class="hlt">Open</span> Online Course on Emma Platform, an European Multiple MOOC Aggregator that provides a system for the delivery of free, <span class="hlt">open</span>, online courses in multiple languages from different European universities. Almost 500 students were enrolled from all over the world and we proposed a multi-perspective approach building on the UNESCO experience in the field of education for sustainable development. The course had two sections: a narrative format which introduces to the <span class="hlt">Ocean</span> Literacy principles, focusing on how to incorporate them into lessons with tips, advice, references and activities; and an interactive section with webinairs which covers contemporary and emerging issues such as seafood, marine pollution and human health, simulating a "real-world experiences" with a problems-solutions approach.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23948091','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23948091"><span>Towards environmental management of <span class="hlt">water</span> turbidity within <span class="hlt">open</span> coastal <span class="hlt">waters</span> of the Great Barrier Reef.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Macdonald, Rachael K; Ridd, Peter V; Whinney, James C; Larcombe, Piers; Neil, David T</p> <p>2013-09-15</p> <p><span class="hlt">Water</span> turbidity and suspended sediment concentration (SSC) are commonly used as part of marine monitoring and <span class="hlt">water</span> quality plans. Current management plans utilise threshold SSC values derived from mean-annual turbidity concentrations. Little published work documents typical ranges of turbidity for reefs within <span class="hlt">open</span> coastal <span class="hlt">waters</span>. Here, time-series turbidity measurements from 61 sites in the Great Barrier Reef (GBR) and Moreton Bay, Australia, are presented as turbidity exceedance curves and derivatives. This contributes to the understanding of turbidity and SSC in the context of environmental management in <span class="hlt">open</span>-coastal reef environments. Exceedance results indicate strong spatial and temporal variability in <span class="hlt">water</span> turbidity across inter/intraregional scales. The highest turbidity across 61 sites, at 50% exceedance (T50) is 15.3 NTU and at 90% exceedance (T90) 4.1 NTU. Mean/median turbidity comparisons show strong differences between the two, consistent with a strongly skewed turbidity regime. Results may contribute towards promoting refinement of <span class="hlt">water</span> quality management protocols. Copyright © 2013 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017E%26PSL.471...94X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017E%26PSL.471...94X"><span>Non-Rayleigh control of upper-<span class="hlt">ocean</span> Cd isotope fractionation in the western South Atlantic</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xie, Ruifang C.; Galer, Stephen J. G.; Abouchami, Wafa; Rijkenberg, Micha J. A.; de Baar, Hein J. W.; De Jong, Jeroen; Andreae, Meinrat O.</p> <p>2017-08-01</p> <p>We present seawater Cd isotopic compositions in five depth profiles and a continuous surface <span class="hlt">water</span> transect, from 50°S to the Equator, in the western South Atlantic, sampled during GEOTRACES cruise 74JC057 (GA02 section, Leg 3), and investigate the mechanisms governing Cd isotope cycling in the upper and deep <span class="hlt">ocean</span>. The depth profiles generally display high ε 112 / 110Cd at the surface and decrease with increasing depth toward values typical of Antarctic Bottom <span class="hlt">Water</span> (AABW). However, at stations north of the Subantarctic Front, the decrease in ε 112 / 110Cd is interrupted by a shift to values intermediate between those of surface and bottom <span class="hlt">waters</span>, which occurs at depths occupied by North Atlantic Deep <span class="hlt">Water</span> (NADW). This pattern is associated with variations in Cd concentration from low surface values to a maximum at mid-depths and is attributed to preferential utilization of light Cd by phytoplankton in the surface <span class="hlt">ocean</span>. Our new results show that in this region Cd-deficient <span class="hlt">waters</span> do not display the extreme, highly fractionated ε 112 / 110Cd reported in some earlier studies from other <span class="hlt">oceanic</span> regions. Instead, in the surface and subsurface southwest (SW) Atlantic, when [Cd] drops below 0.1 nmol kg-1, ε 112 / 110Cd are relatively homogeneous and cluster around a value of +3.7, in agreement with the mean value of 3.8 ± 3.3 (2SD, n = 164) obtained from a statistical evaluation of the global <span class="hlt">ocean</span> Cd isotope dataset. We suggest that Cd-deficient surface <span class="hlt">waters</span> may acquire their Cd isotope signature via sorption of Cd onto organic ligands, colloids or bacterial/picoplankton extracellular functional groups. Alternatively, we show that an <span class="hlt">open</span> system, steady-state model is in good accord with the observed Cd isotope systematics in the upper <span class="hlt">ocean</span> north of the Southern <span class="hlt">Ocean</span>. The distribution of ε 112 / 110Cd in intermediate and deep <span class="hlt">waters</span> is consistent with the <span class="hlt">water</span> mass distribution, with the north-south variations reflecting changes in the mixing proportion</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSPO44C3162D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSPO44C3162D"><span>The Indian <span class="hlt">Ocean</span> as a Connector</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Durgadoo, J. V.; Biastoch, A.; Boning, C. W.</p> <p>2016-02-01</p> <p>The Indian <span class="hlt">Ocean</span> is a conduit for the upper <span class="hlt">ocean</span> flow of the global thermohaline circulation. It receives <span class="hlt">water</span> from the Pacific <span class="hlt">Ocean</span> through the Indonesian throughflow and the Tasman leakage, and exports <span class="hlt">water</span> into the Atlantic by means of Agulhas leakage. A small contribution from the northern Indian <span class="hlt">Ocean</span> is also detectable within Agulhas leakage. Changes on different timescales in the various components of the Pacific inflows and the Atlantic outflow have been reported. Little is known on the role of the Indian <span class="hlt">Ocean</span> circulation in communicating changes from the Pacific into the Atlantic, let alone any eventual alterations in response to climate change. The precise routes and timescales of Indonesian throughflow, Tasman leakage, Red Sea and Persian Gulf <span class="hlt">Waters</span> towards the Atlantic are examined in a Lagrangian framework within a high-resolution global <span class="hlt">ocean</span> model. In this presentation, the following questions are addressed: How are Pacific <span class="hlt">waters</span> modified in the Indian <span class="hlt">Ocean</span> before reaching the Agulhas system? On what timescale is <span class="hlt">water</span> that enters the Indian <span class="hlt">Ocean</span> from the Pacific flushed out? How important are detours in the Bay of Bengal and Arabian Sea?</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150003055','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150003055"><span><span class="hlt">Water</span> Distribution in the Continental and <span class="hlt">Oceanic</span> Upper Mantle</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Peslier, Anne H.</p> <p>2015-01-01</p> <p>Nominally anhydrous minerals such as olivine, pyroxene and garnet can accommodate tens to hundreds of ppm H2O in the form of hydrogen bonded to structural oxygen in lattice defects. Although in seemingly small amounts, this <span class="hlt">water</span> can significantly alter chemical and physical properties of the minerals and rocks. <span class="hlt">Water</span> in particular can modify their rheological properties and its distribution in the mantle derives from melting and metasomatic processes and lithology repartition (pyroxenite vs peridotite). These effects will be examined here using Fourier transform infrared spectrometry (FTIR) <span class="hlt">water</span> analyses on minerals from mantle xenoliths from cratons, plume-influenced cratons and <span class="hlt">oceanic</span> settings. In particular, our results on xenoliths from three different cratons will be compared. Each craton has a different <span class="hlt">water</span> distribution and only the mantle root of Kaapvaal has evidence for dry olivine at its base. This challenges the link between olivine <span class="hlt">water</span> content and survival of Archean cratonic mantle, and questions whether xenoliths are representative of the whole cratonic mantle. We will also present our latest data on Hawaii and Tanzanian craton xenoliths which both suggest the intriguing result that mantle lithosphere is not enriched in <span class="hlt">water</span> when it interacts with melts from deep mantle upwellings (plumes).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1996Natur.383..330T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1996Natur.383..330T"><span>The role of heterotrophic bacteria in iron-limited <span class="hlt">ocean</span> ecosystems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tortell, Philippe D.; Maldonado, Maria T.; Price, Nell M.</p> <p>1996-09-01</p> <p>IRON availability limits phytoplankton growth in large areas of the world's <span class="hlt">oceans</span>1-3 and may influence the strength of the biological carbon pump4,5. Very little is known of the iron requirements of <span class="hlt">oceanic</span> heterotrophic bacteria, which constitute up to 50% of the total particulate organic carbon in <span class="hlt">open</span> <span class="hlt">ocean</span> <span class="hlt">waters</span>6,7 and are important in carbon cycling as remineralizers of dissolved organic matter and hence producers of CO2 (ref. 8). Here we report that <span class="hlt">oceanic</span> bacteria contain more iron per biomass than phytoplankton. In the subarctic Pacific, they constitute a large fraction of biogenic iron and account for 20-45% of biological iron uptake. Bacterial iron quotas in the field are similar to those of iron-deficient laboratory cultures, which exhibit reduced elec-tron transport, slow growth, and low carbon growth efficiency. Heterotrophic bacteria therefore play a major role in the biogeo-chemical cycling of iron. In situ iron limitation of heterotrophic metabolism may have profound effects on carbon flux in the <span class="hlt">ocean</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3894553','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3894553"><span>A new simple concept for <span class="hlt">ocean</span> colour remote sensing using parallel polarisation radiance</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>He, Xianqiang; Pan, Delu; Bai, Yan; Wang, Difeng; Hao, Zengzhou</p> <p>2014-01-01</p> <p><span class="hlt">Ocean</span> colour remote sensing has supported research on subjects ranging from marine ecosystems to climate change for almost 35 years. However, as the framework for <span class="hlt">ocean</span> colour remote sensing is based on the radiation intensity at the top-of-atmosphere (TOA), the polarisation of the radiation, which contains additional information on atmospheric and <span class="hlt">water</span> optical properties, has largely been neglected. In this study, we propose a new simple concept to <span class="hlt">ocean</span> colour remote sensing that uses parallel polarisation radiance (PPR) instead of the traditional radiation intensity. We use vector radiative transfer simulation and polarimetric satellite sensing data to demonstrate that using PPR has two significant advantages in that it effectively diminishes the sun glint contamination and enhances the <span class="hlt">ocean</span> colour signal at the TOA. This concept may <span class="hlt">open</span> new doors for <span class="hlt">ocean</span> colour remote sensing. We suggest that the next generation of <span class="hlt">ocean</span> colour sensors should measure PPR to enhance observational capability. PMID:24434904</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006GBioC..20.1012D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006GBioC..20.1012D"><span>Mangroves, a major source of dissolved organic carbon to the <span class="hlt">oceans</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dittmar, Thorsten; Hertkorn, Norbert; Kattner, Gerhard; Lara, RubéN. J.</p> <p>2006-03-01</p> <p>Organic matter, which is dissolved in low concentrations in the vast <span class="hlt">waters</span> of the <span class="hlt">oceans</span>, contains a total amount of carbon similar to atmospheric carbon dioxide. To understand global biogeochemical cycles, it is crucial to quantify the sources of marine dissolved organic carbon (DOC). We investigated the impact of mangroves, the dominant intertidal vegetation of the tropics, on marine DOC inventories. Stable carbon isotopes and proton nuclear magnetic resonance spectroscopy showed that mangroves are the main source of terrigenous DOC in the <span class="hlt">open</span> <span class="hlt">ocean</span> off northern Brazil. Sunlight efficiently destroyed aromatic molecules during transport offshore, removing about one third of mangrove-derived DOC. The remainder was refractory and may thus be distributed over the <span class="hlt">oceans</span>. On a global scale, we estimate that mangroves account for >10% of the terrestrially derived, refractory DOC transported to the <span class="hlt">ocean</span>, while they cover only <0.1% of the continents' surface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=336309&Lab=NHEERL&keyword=Initiative&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50','EPA-EIMS'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=336309&Lab=NHEERL&keyword=Initiative&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50"><span>Spatial and Temporal <span class="hlt">Water</span> Quality Patterns in <span class="hlt">Open-Water</span> Lake Michigan from the 2015 CSMI</span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p><span class="hlt">Water</span> quality patterns in the Laurentian Great Lakes broadly reflect climate, surficial geography, and landuse but are also shaped by limnological and biological processes. <span class="hlt">Open-water</span> sampling conducted as part of the 2015 Lake Michigan interagency coordinated science and monito...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009ECSS...85...22H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009ECSS...85...22H"><span>Comparisons between the characteristics of ichthyofaunas in nearshore <span class="hlt">waters</span> of five estuaries with varying degrees of connectivity with the <span class="hlt">ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hoeksema, S. D.; Chuwen, B. M.; Potter, I. C.</p> <p>2009-10-01</p> <p>The characteristics of the fish faunas in nearshore, shallow (<1.2 m) <span class="hlt">waters</span> of the basins of estuaries along the same coastline, but which were <span class="hlt">open</span> to the <span class="hlt">ocean</span> for varying periods, have been determined and compared. The fish faunas of the permanently-<span class="hlt">open</span> Oyster Harbour, the seasonally-<span class="hlt">open</span> Broke, Irwin and Wilson inlets and the normally-closed Wellstead Estuary on the south coast of Western Australia were sampled by seine net seasonally for 2 years. Irrespective of the frequency and duration that the estuary mouth was <span class="hlt">open</span>, the ichthyofauna of each estuary was numerically dominated by three atherinid species and three gobiid species (92.9-99.7%), each of which completes its life cycle within these estuaries. The ichthyofaunal compositions of each estuary differed significantly, however, from that of each other estuary. These differences were largely attributable to the relative abundances of the above six species varying between estuaries, which, in turn, reflected differences in such factors as estuary mouth status, macrophyte cover and salinity. For example, Favonigobius lateralis and Leptatherina presbyteroides, which are also represented by marine populations, were most abundant in the permanently-<span class="hlt">open</span> estuary (Oyster Harbour), which, in terms of substrate and salinity, most closely resembled the nearshore marine environment. In contrast, Leptatherina wallacei made its greatest contribution in the only estuary to exhibit a protracted period of greatly reduced salinities, which is consistent with its distribution in permanently-<span class="hlt">open</span> estuaries on the lower west coast of Australia, while Atherinosoma elongata and Pseudogobius olorum were particularly numerous in estuaries containing dense stands of the seagrass Ruppia megacarpa. Marine species made the greatest contribution to species richness in the permanently-<span class="hlt">open</span> estuary and least in the normally-closed estuary. Species richness was greatest in summer and least in winter in each estuary, but differed</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27582222','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27582222"><span>Sea-ice transport driving Southern <span class="hlt">Ocean</span> salinity and its recent trends.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Haumann, F Alexander; Gruber, Nicolas; Münnich, Matthias; Frenger, Ivy; Kern, Stefan</p> <p>2016-09-01</p> <p>Recent salinity changes in the Southern <span class="hlt">Ocean</span> are among the most prominent signals of climate change in the global <span class="hlt">ocean</span>, yet their underlying causes have not been firmly established. Here we propose that trends in the northward transport of Antarctic sea ice are a major contributor to these changes. Using satellite observations supplemented by sea-ice reconstructions, we estimate that wind-driven northward freshwater transport by sea ice increased by 20 ± 10 per cent between 1982 and 2008. The strongest and most robust increase occurred in the Pacific sector, coinciding with the largest observed salinity changes. We estimate that the additional freshwater for the entire northern sea-ice edge entails a freshening rate of -0.02 ± 0.01 grams per kilogram per decade in the surface and intermediate <span class="hlt">waters</span> of the <span class="hlt">open</span> <span class="hlt">ocean</span>, similar to the observed freshening. The enhanced rejection of salt near the coast of Antarctica associated with stronger sea-ice export counteracts the freshening of both continental shelf and newly formed bottom <span class="hlt">waters</span> due to increases in glacial meltwater. Although the data sources underlying our results have substantial uncertainties, regional analyses and independent data from an atmospheric reanalysis support our conclusions. Our finding that northward sea-ice freshwater transport is also a key determinant of the mean salinity distribution in the Southern <span class="hlt">Ocean</span> further underpins the importance of the sea-ice-induced freshwater flux. Through its influence on the density structure of the <span class="hlt">ocean</span>, this process has critical consequences for the global climate by affecting the exchange of heat, carbon and nutrients between the deep <span class="hlt">ocean</span> and surface <span class="hlt">waters</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..1410581M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..1410581M"><span><span class="hlt">Open</span>Danubia - An integrated, modular simulation system to support regional <span class="hlt">water</span> resource management</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Muerth, M.; Waldmann, D.; Heinzeller, C.; Hennicker, R.; Mauser, W.</p> <p>2012-04-01</p> <p>The already completed, multi-disciplinary research project GLOWA-Danube has developed a regional scale, integrated modeling system, which was successfully applied on the 77,000 km2 Upper Danube basin to investigate the impact of Global Change on both the natural and anthropogenic <span class="hlt">water</span> cycle. At the end of the last project phase, the integrated modeling system was transferred into the <span class="hlt">open</span> source project <span class="hlt">Open</span>Danubia, which now provides both the core system as well as all major model components to the general public. First, this will enable decision makers from government, business and management to use <span class="hlt">Open</span>Danubia as a tool for proactive management of <span class="hlt">water</span> resources in the context of global change. Secondly, the model framework to support integrated simulations and all simulation models developed for <span class="hlt">Open</span>Danubia in the scope of GLOWA-Danube are further available for future developments and research questions. <span class="hlt">Open</span>Danubia allows for the investigation of <span class="hlt">water</span>-related scenarios considering different ecological and economic aspects to support both scientists and policy makers to design policies for sustainable environmental management. <span class="hlt">Open</span>Danubia is designed as a framework-based, distributed system. The model system couples spatially distributed physical and socio-economic process during run-time, taking into account their mutual influence. To simulate the potential future impacts of Global Change on agriculture, industrial production, <span class="hlt">water</span> supply, households and tourism businesses, so-called deep actor models are implemented in <span class="hlt">Open</span>Danubia. All important <span class="hlt">water</span>-related fluxes and storages in the natural environment are implemented in <span class="hlt">Open</span>Danubia as spatially explicit, process-based modules. This includes the land surface <span class="hlt">water</span> and energy balance, dynamic plant <span class="hlt">water</span> uptake, ground <span class="hlt">water</span> recharge and flow as well as river routing and reservoirs. Although the complete system is relatively demanding on data requirements and hardware requirements, the modular structure</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012BGD.....9.1667C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012BGD.....9.1667C"><span>Whole <span class="hlt">water</span> column distribution and carbon isotopic composition of bulk particulate organic carbon, cholesterol and brassicasterol from the Cape Basin to the northern Weddell Gyre in the Southern <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cavagna, A.-J.; Dehairs, F.; Woule-Ebongué, V.; Bouillon, S.; Planchon, F.; Delille, B.; Bouloubassi, I.</p> <p>2012-02-01</p> <p>The combination of concentrations and δ13C signatures of Particulate Organic Carbon (POC) and sterols provides a powerful approach to study ecological and environmental changes both in the modern and ancient <span class="hlt">ocean</span>, but its application has so far been restricted to the surface area. We applied this tool to study the biogeochemical changes in the modern <span class="hlt">ocean</span> <span class="hlt">water</span> column during the BONUS-GoodHope survey (Feb-Mar 2008) from Cape Basin to the northern part of the Weddell Gyre. Cholesterol and brassicasterol were chosen as ideal biomarkers of the heterotrophic and autotrophic carbon pools, respectively, because of their ubiquitous and relatively refractory nature. We document depth distributions of concentrations (relative to bulk POC) and δ13C signatures of cholesterol and brassicasterol from the Cape Basin to the northern Weddell Gyre combined with CO2 aq. surface concentration variation. While relationships between surface <span class="hlt">water</span> CO2 aq. and δ13C of bulk POC and biomarkers have been previously established for surface <span class="hlt">waters</span>, our data show that these remain valid in deeper <span class="hlt">waters</span>, suggesting that δ13C signatures of certain biomarkers could be developed as proxies for surface <span class="hlt">water</span> CO2 aq. Our data suggest a key role of zooplankton fecal aggregates in carbon export for this part of the Southern <span class="hlt">Ocean</span>. We observed a general increase in sterol δ13C signatures with depth, which is likely related to a combination of particle size effects, selective feeding on larger cells by zooplankton, and growth rate related effects Additionally, in the southern part of the transect south of the Polar Front (PF), the release of sea-ice algae is hypothesized to influence the isotopic signature of sterols in the <span class="hlt">open</span> <span class="hlt">ocean</span>. Overall, combined use of δ13C and concentrations measurements of both bulk organic C and specific sterol markers throughout the <span class="hlt">water</span> column shows the promising potential of analyzing δ13C signatures of individual marine sterols to explore the recent history of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20030032183','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20030032183"><span>Remote Sensing of Suspended Sediments and Shallow Coastal <span class="hlt">Waters</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Li, Rong-Rong; Kaufman, Yoram J.; Gao, Bo-Cai; Davis, Curtiss O.</p> <p>2002-01-01</p> <p><span class="hlt">Ocean</span> color sensors were designed mainly for remote sensing of chlorophyll concentrations over the clear <span class="hlt">open</span> <span class="hlt">oceanic</span> areas (case 1 <span class="hlt">water</span>) using channels between 0.4 and 0.86 micrometers. The Moderate Resolution Imaging Spectroradiometer (MODIS) launched on the NASA Terra and Aqua Spacecrafts is equipped with narrow channels located within a wider wavelength range between 0.4 and 2.5 micrometers for a variety of remote sensing applications. The wide spectral range can provide improved capabilities for remote sensing of the more complex and turbid coastal <span class="hlt">waters</span> (case 2 <span class="hlt">water</span>) and for improved atmospheric corrections for <span class="hlt">Ocean</span> scenes. In this article, we describe an empirical algorithm that uses this wide spectral range to identifying areas with suspended sediments in turbid <span class="hlt">waters</span> and shallow <span class="hlt">waters</span> with bottom reflections. The algorithm takes advantage of the strong <span class="hlt">water</span> absorption at wavelengths longer than 1 micrometer that does not allow illumination of sediments in the <span class="hlt">water</span> or a shallow <span class="hlt">ocean</span> floor. MODIS data acquired over the east coast of China, west coast of Africa, Arabian Sea, Mississippi Delta, and west coast of Florida are used in this study.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeoRL..4412375H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoRL..4412375H"><span>Rapid <span class="hlt">Water</span> Transport by Long-Lasting Modon Eddy Pairs in the Southern Midlatitude <span class="hlt">Oceans</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hughes, Chris W.; Miller, Peter I.</p> <p>2017-12-01</p> <p><span class="hlt">Water</span> in the <span class="hlt">ocean</span> is generally carried with the mean flow, mixed by eddies, or transported westward by coherent eddies at speeds close to the long baroclinic Rossby wave speed. Modons (dipole eddy pairs) are a theoretically predicted exception to this behavior, which can carry <span class="hlt">water</span> to the east or west at speeds much larger than the Rossby wave speed, leading to unusual transports of heat, nutrients, and carbon. We provide the first observational evidence of such rapidly moving modons propagating over large distances. These modons are found in the midlatitude <span class="hlt">oceans</span> around Australia, with one also seen in the South Atlantic west of the Agulhas region. They can travel at more than 10 times the Rossby wave speed of 1-2 cm s-1 and typically persist for about 6 months carrying their unusual <span class="hlt">water</span> mass properties with them, before splitting into individual vortices, which can persist for many months longer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.6582P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.6582P"><span><span class="hlt">Ocean</span> Research - Perspectives from an international <span class="hlt">Ocean</span> Research Coordination Network</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pearlman, Jay; Williams, Albert, III</p> <p>2013-04-01</p> <p>The need for improved coordination in <span class="hlt">ocean</span> observations is more urgent now given the issues of climate change, sustainable food sources and increased need for energy. <span class="hlt">Ocean</span> researchers must work across disciplines to provide policy makers with clear and understandable assessments of the state of the <span class="hlt">ocean</span>. With advances in technology, not only in observation, but also communication and computer science, we are in a new era where we can answer questions asked over the last 100 years at the time and space scales that are relevant. Programs like GLOBEC moved us forward but we are still challenged by the disciplinary divide. Interdisciplinary problem solving must be addressed not only by the exchange of data between the many sides, but through levels where questions require day-to-day collaboration. A National Science Foundation-funded Research Coordination Network (RCN) is addressing approaches for improving interdisciplinary research capabilities in the <span class="hlt">ocean</span> sciences. During the last year, the RCN had a working group for <span class="hlt">Open</span> Data led by John Orcutt, Peter Pissierssens and Albert Williams III. The teams has focused on three areas: 1. Data and Information formats and standards; 2. Data access models (including IPR, business models for <span class="hlt">open</span> data, data policies,...); 3. Data publishing, data citation. There has been a significant trend toward free and <span class="hlt">open</span> access to data in the last few years. In 2007, the US announced that Landsat data would be available at no charge. Float data from the US (NDBC), JCOMM and <span class="hlt">Ocean</span>Sites offer web-based access. The IODE is developing its <span class="hlt">Ocean</span> Data Portal giving immediate and free access to <span class="hlt">ocean</span> data. However, from the aspect of long-term collaborations across communities, this global trend is less robust than might appear at the surface. While there are many standard data formats for data exchange, there is not yet widespread uniformity in their adoption. Use of standard data formats can be encouraged in several ways: sponsors of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A11G1952F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A11G1952F"><span>Seasonal variation of marine organic aerosols in the North Pacific <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fu, P.; Kawamura, K.</p> <p>2017-12-01</p> <p>Atmospheric aerosols were collected in the marine boundary layer during five marine cruises in the northern Pacific <span class="hlt">Ocean</span> from October 1996 to July 1997. Organic molecular compositions of the marine aerosols were measured using gas chromatography/mass spectrometry (GC/MS). Higher concentrations of levoglucosan and its isomers, the biomass-burning tracers, were observed in the coastal regions than those in the central north Pacific. Seasonal trends of biomass burning tracers were found to be higher in fall-winter-spring than in summer, suggesting an enhanced influence of continental aerosols to the marine atmosphere during cold seasons when the westerlies prevail. However, the atmospheric levels of secondary organic aerosol (SOA) tracers from the photooxidation of isoprene and monoterpenes were higher in warm seasons than cold seasons, which are in accordance with the enhanced emissions of biogenic volatile organic compounds (BVOCs) in summer. Stable C isotope ratios of total carbon (δ13CTC) in the marine aerosols ranged from -28.5‰ to -23.6‰ (mean -26.4‰), suggesting an important input of terrestrial/continental aerosol particles. Stable N isotope ratios (2.6‰ to 12.9‰, mean 7.1‰) were found to be higher in the coastal regions than those in the <span class="hlt">open</span> <span class="hlt">oceans</span>, suggesting an enhanced emission of marine aerosols in the <span class="hlt">open</span> <span class="hlt">oceans</span>. The fluorescence properties of the <span class="hlt">water</span>-soluble organic carbon (WSOC) in the marine aerosols conform the importance of marine emitted organics in the <span class="hlt">open</span> <span class="hlt">ocean</span>, especially during the high biological activity periods.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19990092487&hterms=neither+deep+shallow&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dneither%2Bdeep%2Bshallow','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19990092487&hterms=neither+deep+shallow&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dneither%2Bdeep%2Bshallow"><span>Tidal Energy Available for Deep <span class="hlt">Ocean</span> Mixing: Bounds from Altimetry Data</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Egbert, Gary D.; Ray, Richard D.</p> <p>1999-01-01</p> <p>Maintenance of the large-scale thermohaline circulation has long presented a problem to oceanographers. Observed mixing rates in the pelagic <span class="hlt">ocean</span> are an order of magnitude too small to balance the rate at which dense bottom <span class="hlt">water</span> is created at high latitudes. Recent observational and theoretical work suggests that much of this mixing may occur in hot spots near areas of rough topography (e.g., mid-<span class="hlt">ocean</span> ridges and island arcs). Barotropic tidal currents provide a very plausible source of energy to maintain these mixing processes. Topex/Poseidon (T/P) satellite altimetry data have made precise mapping of <span class="hlt">open</span> <span class="hlt">ocean</span> tidal elevations possible for the first time. We can thus obtain empirical, spatially localized, estimates of barotropic tidal dissipation. These provide an upper bound on the amount of tidal energy that is dissipated in the deep <span class="hlt">ocean</span>, and hence is available for deep mixing. We will present and compare maps of <span class="hlt">open</span> <span class="hlt">ocean</span> tidal energy flux divergence, and estimates of tidal energy flux into shallow seas, derived from T/P altimetry data using both formal data assimilation methods and empirical approaches. With the data assimilation methods we can place formal error bars on the fluxes. Our results show that 20-25% of tidal energy dissipation occurs outside of the shallow seas, the traditional sink for tidal energy. This suggests that up to 1 TW of energy may be available from the tides (lunar and solar) for mixing the deep <span class="hlt">ocean</span>. The dissipation indeed appears to be concentrated over areas of rough topography.</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('https://ntrs.nasa.gov/search.jsp?R=19990115479&hterms=neither+deep+shallow&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dneither%2Bdeep%2Bshallow','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19990115479&hterms=neither+deep+shallow&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dneither%2Bdeep%2Bshallow"><span>Tidal Energy Available for Deep <span class="hlt">Ocean</span> Mixing: Bounds From Altimetry Data</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Egbert, Gary D.; Ray, Richard D.</p> <p>1999-01-01</p> <p>Maintenance of the large-scale thermohaline circulation has long presented a problem to oceanographers. Observed mixing rates in the pelagic <span class="hlt">ocean</span> are an order of magnitude too small to balance the rate at which dense bottom <span class="hlt">water</span> is created at high latitudes. Recent observational and theoretical work suggests that much of this mixing may occur in hot spots near areas of rough topography (e.g., mid-<span class="hlt">ocean</span> ridges and island arcs). Barotropic tidal currents provide a very plausible source of energy to maintain these mixing processes. Topex/Poseidon satellite altimetry data have made precise mapping of <span class="hlt">open</span> <span class="hlt">ocean</span> tidal elevations possible for the first time. We can thus obtain empirical, spatially localized, estimates of barotropic tidal dissipation. These provide an upper bound on the amount of tidal energy that is dissipated in the deep <span class="hlt">ocean</span>, and hence is available for deep mixing. We will present and compare maps of <span class="hlt">open</span> <span class="hlt">ocean</span> tidal energy flux divergence, and estimates of tidal energy flux into shallow seas, derived from T/P altimetry data using both formal data assimilation methods and empirical approaches. With the data assimilation methods we can place formal error bars on the fluxes. Our results show that 20-25% of tidal energy dissipation occurs outside of the shallow seas, the traditional sink for tidal energy. This suggests that up to 1 TW of energy may be available from the tides (lunar and solar) for mixing the deep <span class="hlt">ocean</span>. The dissipation indeed appears to be concentrated over areas of rough topography.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19990114316&hterms=neither+deep+shallow&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dneither%2Bdeep%2Bshallow','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19990114316&hterms=neither+deep+shallow&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dneither%2Bdeep%2Bshallow"><span>Tidal Energy Available for Deep <span class="hlt">Ocean</span> Mixing: Bounds from Altimetry Data</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ray, Richard D.; Egbert, Gary D.</p> <p>1999-01-01</p> <p>Maintenance of the large-scale thermohaline circulation has long presented an interesting problem. Observed mixing rates in the pelagic <span class="hlt">ocean</span> are an order of magnitude too small to balance the rate at which dense bottom <span class="hlt">water</span> is created at high latitudes. Recent observational and theoretical work suggests that much of this mixing may occur in hot spots near areas of rough topography (e.g., mid-<span class="hlt">ocean</span> ridges and island arcs). Barotropic tidal currents provide a very plausible source of energy to maintain these mixing processes. Topex/Poseidon satellite altimetry data have made precise mapping of <span class="hlt">open</span> <span class="hlt">ocean</span> tidal elevations possible for the first time. We can thus obtain empirical, spatially localized, estimates of barotropic tidal dissipation. These provide an upper bound on the amount of tidal energy that is dissipated in the deep <span class="hlt">ocean</span>, and hence is available for deep mixing. We will present and compare maps of <span class="hlt">open</span> <span class="hlt">ocean</span> tidal energy flux divergence, and estimates of tidal energy flux into shallow seas, derived from T/P altimetry data using both formal data assimilation methods and empirical approaches. With the data assimilation methods we can place formal error bars on the fluxes. Our results show that 20-25% of tidal energy dissipation occurs outside of the shallow seas, the traditional sink for tidal energy. This suggests that up to 1 TW of energy may be available from the tides (lunar and solar) for mixing the deep <span class="hlt">ocean</span>. The dissipation indeed appears to be concentrated over areas of rough topography.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMPP13A1862Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMPP13A1862Z"><span>Causes of strong <span class="hlt">ocean</span> heating during glacial periods</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zimov, N.; Zimov, S. A.</p> <p>2013-12-01</p> <p>During the last deglaciation period, the strongest climate changes occurred across the North Atlantic regions. Analyses of borehole temperatures from the Greenland ice sheet have yielded air temperature change estimates of 25°C over the deglaciation period (Dahl-Jensen et al. 1998). Such huge temperature changes cannot currently be explained in the frames of modern knowledge about climate. We propose that glacial-interglacial cycles are connected with gradual warming of <span class="hlt">ocean</span> interior <span class="hlt">waters</span> over the course of glaciations and quick transport of accumulated heat from <span class="hlt">ocean</span> to the atmosphere during the deglaciation periods. Modern day <span class="hlt">ocean</span> circulation is dominated by thermal convection with cold <span class="hlt">waters</span> subsiding in the Northern Atlantic and filling up the <span class="hlt">ocean</span> interior with cold and heavy <span class="hlt">water</span>. However during the glaciation thermal circulation stopped and <span class="hlt">ocean</span> circulation was driven by 'haline pumps' -Red and Mediterranean seas connected with <span class="hlt">ocean</span> with only narrow but deep straights acts as evaporative basins, separating <span class="hlt">ocean</span> <span class="hlt">water</span> into fresh <span class="hlt">water</span> which returns to the <span class="hlt">ocean</span> surface (precipitation) and warm but salty, and therefore heavy, <span class="hlt">water</span> which flows down to the <span class="hlt">ocean</span> floor. This haline pump is stratifying the <span class="hlt">ocean</span>, allowing warmer <span class="hlt">water</span> locate under the colder <span class="hlt">water</span> and thus stopping thermal convection in the <span class="hlt">ocean</span>. Additional <span class="hlt">ocean</span> interior warming is driven by geothermal heat flux and decomposition of organic rain. To test the hypothesis we present simple <span class="hlt">ocean</span> box model that describes thermohaline circulation in the World <span class="hlt">Ocean</span>. The first box is the Red and Mediterranean sea, the second is united high-latitude seas, the third is the <span class="hlt">ocean</span> surface, and the fourth the <span class="hlt">ocean</span> interior. The volume of these <span class="hlt">water</span> masses and straight cross-sections are taken to be close to real values. We have accepted that the exchange of <span class="hlt">water</span> between boxes is proportional to the difference in <span class="hlt">water</span> density in these boxes, Sun energy inputs to the <span class="hlt">ocean</span> and sea surface</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009DSRI...56.1449M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009DSRI...56.1449M"><span>The relationship between dissolved hydrogen and nitrogen fixation in <span class="hlt">ocean</span> <span class="hlt">waters</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, Robert M.; Punshon, Stephen; Mahaffey, Claire; Karl, David</p> <p>2009-09-01</p> <p>Fixed nitrogen is a key nutrient involved in regulating global marine productivity and hence the global <span class="hlt">oceanic</span> carbon cycle. <span class="hlt">Oceanic</span> nitrogen (N 2) fixation is estimated to supply 8×10 12 moles N y -1 to the <span class="hlt">ocean</span>, approximately equal to current riverine and the atmospheric inputs of fixed N, and between 50 and 100% of current estimates of <span class="hlt">oceanic</span> denitrification. However, the spatial and temporal variability of N 2 fixation remains uncertain, mostly because of the normal low resolution sampling for diazotroph distribution and fixation rates. It is well established that N 2 fixation, mediated by the enzyme nitrogenase, is a source of hydrogen (H 2), but the extent to which it leads to supersaturation of H 2 in <span class="hlt">oceanic</span> <span class="hlt">waters</span> is unresolved. Here, we present simultaneous measurements of upper <span class="hlt">ocean</span> dissolved H 2 concentration (nmol L -1), and rates of N 2 fixation (μmol N m -3 d -1), determined using 15N 2 tracer techniques (at 7 or 15 m), on a transect from Fiji to Hawaii. We find a significant correlation ( r=0.98) between dissolved H 2 and rates of N 2 fixation, with the greatest supersaturation of H 2 and highest rates of N 2 fixation being observed in the subtropical gyres at the southern (˜18°S) and northern (18°N) reaches of the transect. The lowest H 2 saturation and N 2 fixation were observed in the equatorial region between 8°S and 14°N. We propose that an empirical relationship between H 2 supersaturations and N 2 fixation measurements could be used to guide sampling for 15N fixation measurements or to aid the spatial interpolation of such measurements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMOS24A..04D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMOS24A..04D"><span>Diagnosis of CO2 Fluxes in the Coastal <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dai, M.; Cao, Z.; Yang, W.; Guo, X.; Yin, Z.; Zhao, Y.</p> <p>2017-12-01</p> <p>Coastal <span class="hlt">ocean</span> carbon is an important component of the global carbon cycle. However, its mechanistic-based conceptualization, a prerequisite of coastal carbon modeling and its inclusion in the Earth System Model, remains difficult due to the highest variability in both time and space. Here we show that the inter-seasonal change of the global coastal pCO2 is more determined by non-temperature factors such as biological drawdown and <span class="hlt">water</span> mass mixing, the latter of which features the dynamic boundary processes of the coastal <span class="hlt">ocean</span> at both land-margin and margin-<span class="hlt">open</span> <span class="hlt">ocean</span> interfaces. Considering these unique features, we resolve the coastal CO2 fluxes using a semi-analytical approach coupling physics-biogeochemistry and carbon-nutrients and conceptualize the coastal carbon cycle into <span class="hlt">Ocean</span>-dominated Margins (OceMar) and River-dominated <span class="hlt">Ocean</span> Margins (RiOMar). The diagnostic result of CO2 fluxes in the South China Sea basin and the Arabian Sea as OceMars and in the Pearl River Plume as a RioMar is consistent with field observations. Our mechanistic-based diagnostic approach therefore helps better understand and model coastal carbon cycle yet the stoichiometry of carbon-nutrients coupling needs scrutiny when applying our approach.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRC..123.2172E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRC..123.2172E"><span>Turbulence Scaling Comparisons in the <span class="hlt">Ocean</span> 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 turbulent kinetic energy, ɛ, under <span class="hlt">open</span> <span class="hlt">ocean</span> conditions are limited. Consequently, our understanding of what chiefly controls dissipation in the <span class="hlt">open</span> <span class="hlt">ocean</span>, and its functional form with depth, is poorly constrained. In this study, we report direct <span class="hlt">open</span> <span class="hlt">ocean</span> measurements of ɛ from the Air-Sea Interaction Profiler (ASIP) collected during five different cruises in the Atlantic <span class="hlt">Ocean</span>. We then combine these data with <span class="hlt">ocean</span>-atmosphere flux measurements and wave information in order to evaluate existing turbulence scaling theories under a diverse set of <span class="hlt">open</span> <span class="hlt">ocean</span> 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/2008AGUFM.P13C1333G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.P13C1333G"><span><span class="hlt">Ocean</span>-bearing planets near the ice line: How far does the <span class="hlt">water</span>'s edge go?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gaidos, E.; Seager, S.; Gaudi, S.</p> <p>2008-12-01</p> <p>A leading theory for giant planet formation involves the accretion of a solid core, probably ice-rich, that in turn accretes a massive mantle of hydrogen-helium gas from a primordial disk. The relative timing of core formation and disappearance of nebular gas in a few millions of years is critical; the correlation between heavy element abundance in stellar photospheres and their propensity to host giant planets is cited as support for the theory. Conversely, systems that are relatively heavy element-poor or lose their gas earlier should contain either "failed" cores or a set of icy planetary embryos that did not accrete. Indeed, Uranus and Neptune may represent similar embryos that were scattered by Jupiter into the outer disk where they efficiently accreted planetesimals rich in volatiles with low condensation temperatures. We propose that a region straddling the "snowline" (3-5~AU for solar-mass stars) could frequently be inhabited by one or more <span class="hlt">water</span> ice-rich, super-Earth-mass objects that accreted only a modest amount of nebular gas. We predict that metal-poor bulge and halo stars are more likely to host such objects. Current and future microlensing surveys will be able to determine the population of Earth-mass planets in this range of semimajor axes and test this hypothesis. If they are sufficiently frequent, the nearest examples will be detectable by the Space Interferometer Mission and perhaps a visible-light Terrestrial Planet Finder mission. We show that retention of a ~1~bar hydrogen-helium atmosphere is sufficient to maintain a surface <span class="hlt">water</span> <span class="hlt">ocean</span>, depending on semimajor axis and thermal history, and that sufficiently massive, "naked" ice planets can have interior <span class="hlt">oceans</span> a la Europa. Planets with more substantial (>200~bar) atmospheres will be devoid of a liquid <span class="hlt">water</span> phase at the surface. The existence of a surface <span class="hlt">water</span> <span class="hlt">ocean</span> could be inferred by the absence of highly soluble molecules such as NH3 or SO2 in the atmosphere. Objects with such <span class="hlt">oceans</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013ESASP.710E...9E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013ESASP.710E...9E"><span>Twenty Years of Progress on Global <span class="hlt">Ocean</span> Tide: The Impact of Satellite Altimetry</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Egbert, Gary D.; Ray, Richard D.</p> <p>2013-09-01</p> <p>At the dawn of the era of high-precision altimetry, before the launch of TOPEX/Poseidon, <span class="hlt">ocean</span> tides were properly viewed as a source of noise-tidal variations in <span class="hlt">ocean</span> height would represent a very substantial fraction of what the altimeter measures, and would have to be accurately predicted and subtracted if altimetry were to achieve its potential for <span class="hlt">ocean</span> and climate studies. But to the extent that the altimetry could be severely contaminated by tides, it also represented an unprecedented global-scale tidal data set. These new data, together with research stimulated by the need for accurate tidal corrections, led to a renaissance in tidal studies in the oceanographic community. In this paper we review contributions of altimetry to tidal science over the past 20 years, emphasizing recent progress. Mapping of tides has now been extended from the early focus on major constituents in the <span class="hlt">open</span> <span class="hlt">ocean</span> to include minor constituents, (e.g., long-period tides; non-linear tides in shelf <span class="hlt">waters</span>, and in the <span class="hlt">open</span> <span class="hlt">ocean</span>), and into shallow and coastal <span class="hlt">waters</span>. Global and spatially local estimates of tidal energy balance have been refined, and the role of internal tide conversion in dissipating barotropic tidal energy is now well established through modeling, altimetry, and in situ observations. However, energy budgets for internal tides, and the role of tidal dissipation in vertical <span class="hlt">ocean</span> mixing remain controversial topics. Altimetry may contribute to resolving some of these important questions through improved mapping of low-mode internal tides. This area has advanced significantly in recent years, with several global maps now available, and progress on constraining temporally incoherent components. For the future, new applications of altimetry (e.g., in the coastal <span class="hlt">ocean</span>, where barotropic tidal models remain inadequate), and new mission concepts (studies of the sub-mesoscale with SWOT, which will require correction for internal tides) may bring us full circle, again pushing</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120009634','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120009634"><span>Twenty Years of Progress on Global <span class="hlt">Ocean</span> Tides: The Impact of Satellite Altimetry</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Egbert, Gary; Ray, Richard</p> <p>2012-01-01</p> <p>At the dawn of the era of high-precision altimetry, before the launch of TOPEX/Poseidon, <span class="hlt">ocean</span> tides were properly viewed as a source of noise--tidal variations in <span class="hlt">ocean</span> height would represent a very substantial fraction of what the altimeter measures, and would have to be accurately predicted and subtracted if altimetry were to achieve its potential for <span class="hlt">ocean</span> and climate studies. But to the extent that the altimetry could be severely contaminated by tides, it also represented an unprecedented global-scale tidal data set. These new data, together with research stimulated by the need for accurate tidal corrections, led to a renaissance in tidal studies in the oceanographic community. In this paper we review contributions of altimetry to tidal science over the past 20 years, emphasizing recent progress. Mapping of tides has now been extended from the early focus on major constituents in the <span class="hlt">open</span> <span class="hlt">ocean</span> to include minor constituents, (e.g., long-period tides; non-linear tides in shelf <span class="hlt">waters</span>, and in the <span class="hlt">open</span> <span class="hlt">ocean</span>), and into shallow and coastal <span class="hlt">waters</span>. Global and spatially local estimates of tidal energy balance have been refined, and the role of internal tide conversion in dissipating barotropic tidal energy is now well established through modeling, altimetry, and in situ observations. However, energy budgets for internal tides, and the role of tidal dissipation in vertical <span class="hlt">ocean</span> mixing remain controversial topics. Altimetry may contribute to resolving some of these important questions through improved mapping of low-mode internal tides. This area has advanced significantly in recent years, with several global maps now available, and progress on constraining temporally incoherent components. For the future, new applications of altimetry (e.g., in the coastal <span class="hlt">ocean</span>, where barotropic tidal models remain inadequate), and new mission concepts (studies of the submesoscale with SWOT, which will require correction for internal tides) may bring us full circle, again pushing</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017NatSR...743436H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017NatSR...743436H"><span>Hydrogen peroxide in deep <span class="hlt">waters</span> from the Mediterranean Sea, South Atlantic and South Pacific <span class="hlt">Oceans</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hopwood, Mark J.; Rapp, Insa; Schlosser, Christian; Achterberg, Eric P.</p> <p>2017-03-01</p> <p>Hydrogen peroxide (H2O2) is present ubiquitously in marine surface <span class="hlt">waters</span> where it is a reactive intermediate in the cycling of many trace elements. Photochemical processes are considered the dominant natural H2O2 source, yet cannot explain nanomolar H2O2 concentrations below the photic zone. Here, we determined the concentration of H2O2 in full depth profiles across three <span class="hlt">ocean</span> basins (Mediterranean Sea, South Atlantic and South Pacific <span class="hlt">Oceans</span>). To determine the accuracy of H2O2 measurements in the deep <span class="hlt">ocean</span> we also re-assessed the contribution of interfering species to ‘apparent H2O2’, as analysed by the luminol based chemiluminescence technique. Within the vicinity of coastal oxygen minimum zones, accurate measurement of H2O2 was not possible due to interference from Fe(II). Offshore, in deep (>1000 m) <span class="hlt">waters</span> H2O2 concentrations ranged from 0.25 ± 0.27 nM (Mediterranean, Balearics-Algeria) to 2.9 ± 2.2 nM (Mediterranean, Corsica-France). Our results indicate that a dark, pelagic H2O2 production mechanism must occur throughout the deep <span class="hlt">ocean</span>. A bacterial source of H2O2 is the most likely origin and we show that this source is likely sufficient to account for all of the observed H2O2 in the deep <span class="hlt">ocean</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5339902','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5339902"><span>Hydrogen peroxide in deep <span class="hlt">waters</span> from the Mediterranean Sea, South Atlantic and South Pacific <span class="hlt">Oceans</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>Hopwood, Mark J.; Rapp, Insa; Schlosser, Christian; Achterberg, Eric P.</p> <p>2017-01-01</p> <p>Hydrogen peroxide (H2O2) is present ubiquitously in marine surface <span class="hlt">waters</span> where it is a reactive intermediate in the cycling of many trace elements. Photochemical processes are considered the dominant natural H2O2 source, yet cannot explain nanomolar H2O2 concentrations below the photic zone. Here, we determined the concentration of H2O2 in full depth profiles across three <span class="hlt">ocean</span> basins (Mediterranean Sea, South Atlantic and South Pacific <span class="hlt">Oceans</span>). To determine the accuracy of H2O2 measurements in the deep <span class="hlt">ocean</span> we also re-assessed the contribution of interfering species to ‘apparent H2O2’, as analysed by the luminol based chemiluminescence technique. Within the vicinity of coastal oxygen minimum zones, accurate measurement of H2O2 was not possible due to interference from Fe(II). Offshore, in deep (>1000 m) <span class="hlt">waters</span> H2O2 concentrations ranged from 0.25 ± 0.27 nM (Mediterranean, Balearics-Algeria) to 2.9 ± 2.2 nM (Mediterranean, Corsica-France). Our results indicate that a dark, pelagic H2O2 production mechanism must occur throughout the deep <span class="hlt">ocean</span>. A bacterial source of H2O2 is the most likely origin and we show that this source is likely sufficient to account for all of the observed H2O2 in the deep <span class="hlt">ocean</span>. PMID:28266529</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017FrEaS...5...34N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017FrEaS...5...34N"><span>Distribution and sources of dissolved black carbon in surface <span class="hlt">waters</span> of the Chukchi Sea, Bering Sea, and the North Pacific <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nakane, Motohiro; Ajioka, Taku; Yamashita, Youhei</p> <p>2017-05-01</p> <p>Pyrogenic carbon, also called black carbon (BC), is an important component in the global carbon cycle. BC produced by biomass burning or fossil fuel combustion is transported to <span class="hlt">oceans</span> by the atmosphere or rivers. However, environmental dynamics (i.e., major sources and sinks) of BC in marine environments have not been well documented. In this study, dissolved BC (DBC) collected from surface <span class="hlt">waters</span> of the Chukchi Sea, the Bering Sea, and the subarctic and subtropical North Pacific were analyzed using the benzene polycarboxylic acid (BPCA) method. The DBC concentration and the ratio of B5CA and B6CA to all BPCAs (an index of the DBC condensation degree) ranged from 4.8 to 15.5 µg-C L-1 and from 0.20 to 0.43, respectively, in surface <span class="hlt">waters</span> of the Chukchi/Bering Seas and the North Pacific <span class="hlt">Ocean</span>. The concentration and condensation degree of DBC in the Chukchi/Bering Seas were higher and more variable than those in the subarctic and subtropical North Pacific, which implies that the major factors controlling DBC distribution were different in these marine provinces. In the Chukchi/Bering Seas, the DBC concentration was negatively correlated to salinity but positively correlated to chromophoric dissolved organic matter (CDOM) quantity and total dissolved lignin phenol concentration estimated by CDOM parameters. These correlations indicated that the possible major source of DBC in the Chukchi/Bering Seas was Arctic rivers. However, in the North Pacific, where riverine inputs are negligible for most sampling sites, DBC was possibly derived from the atmosphere. Although spectral slopes of CDOM at 275-295 nm (an index of the photodegradation degree of CDOM) differed widely between the subarctic and subtropical North Pacific, the concentration and condensation degrees of DBC were similar between the subarctic and subtropical North Pacific, which suggests that photodegradation was not the only major factor controlling DBC distribution. Therefore, DBC distributions of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017OcSci..13..521Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017OcSci..13..521Y"><span>Freshening of Antarctic Intermediate <span class="hlt">Water</span> in the South Atlantic <span class="hlt">Ocean</span> in 2005-2014</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yao, Wenjun; Shi, Jiuxin; Zhao, Xiaolong</p> <p>2017-07-01</p> <p>Basin-scale freshening of Antarctic Intermediate <span class="hlt">Water</span> (AAIW) is reported to have occurred in the South Atlantic <span class="hlt">Ocean</span> during the period from 2005 to 2014, as shown by the gridded monthly means of the Array for Real-time Geostrophic Oceanography (Argo) data. This phenomenon was also revealed by two repeated transects along a section at 30° S, performed during the World <span class="hlt">Ocean</span> Circulation Experiment Hydrographic Program. Freshening of the AAIW was compensated for by a salinity increase of thermocline <span class="hlt">water</span>, indicating a hydrological cycle intensification. This was supported by the precipitation-minus-evaporation change in the Southern Hemisphere from 2000 to 2014. Freshwater input from atmosphere to <span class="hlt">ocean</span> surface increased in the subpolar high-precipitation region and vice versa in the subtropical high-evaporation region. Against the background of hydrological cycle changes, a decrease in the transport of Agulhas Leakage (AL), which was revealed by the simulated velocity field, was proposed to be a contributor to the associated freshening of AAIW. Further calculation showed that such a decrease could account for approximately 53 % of the observed freshening (mean salinity reduction of about 0.012 over the AAIW layer). The estimated variability of AL was inferred from a weakening of wind stress over the South Indian <span class="hlt">Ocean</span> since the beginning of the 2000s, which would facilitate freshwater input from the source region. The mechanical analysis of wind data here was qualitative, but it is contended that this study would be helpful to validate and test predictably coupled sea-air model simulations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..14.3467K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..14.3467K"><span>High-resolution paleoenvironmental records during the late Quaternary from the marginal seas of East Asia: the intrusion of <span class="hlt">open-ocean</span> current</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kong, G. S.; Kim, S. P.; Choi, H. S.</p> <p>2012-04-01</p> <p> nearly to the present level, the southeastern coast area began to change into a modern-type shelf environment influenced by the intrusion of the Tsushima Current, which is supported by significantly high TOC contents, high CaCO3 contents, and predominance of marine-type organic matters. In summary, long mud-dominated Holocene cores provided the opportunity to elucidate the onset of inflow of the <span class="hlt">open-ocean</span> warm current during Holocene marine transgression in the marginal seas around the Korean Peninsula. The results of four long cores suggest that the timings of intrusion of warm currents are different from each other due to the influence of brackish coastal currents and river discharge rather than increased <span class="hlt">water</span> depth. Also, a relative abundance of marine-type organic matter characteristic of oxygen and carbon isotopes showed differences even after establishing a modern-type marine environment, implying that properties of their environments are altered according to the changes of strength between river discharge and <span class="hlt">open-ocean</span> current at their location.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.5749L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.5749L"><span>Dense <span class="hlt">water</span> formation in the north-western Mediterranean area during HyMeX-SOP2 in 1/36° <span class="hlt">ocean</span> simulations: <span class="hlt">Ocean</span>-atmosphere coupling impact</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lebeaupin Brossier, Cindy; Léger, Fabien; Giordani, Hervé; Beuvier, Jonathan; Bouin, Marie-Noëlle; Ducrocq, Véronique; Fourrié, Nadia</p> <p>2017-07-01</p> <p>The north-western Mediterranean Sea is a key location for the thermohaline circulation of the basin. The area is characterized by intense air-sea exchanges favored by the succession of strong northerly and north-westerly wind situations (mistral and tramontane) in autumn and winter. Such meteorological conditions lead to significant evaporation and <span class="hlt">ocean</span> heat loss that are well known as the main triggering factor for the Dense <span class="hlt">Water</span> Formation (DWF) and winter deep convection episodes. During the HyMeX second field campaign (SOP2, 1 February to 15 March 2013), several platforms were deployed in the area in order to document the DWF and the <span class="hlt">ocean</span> deep convection, as the air-sea interface conditions. This study investigates the role of the <span class="hlt">ocean</span>-atmosphere coupling on DWF during winter 2012-2013. The coupled system, based on the NEMO-WMED36 <span class="hlt">ocean</span> model (1/36° resolution) and the AROME-WMED atmospheric model (2.5 km resolution), was run during 2 months covering the SOP2 and is compared to an <span class="hlt">ocean</span>-only simulation forced by AROME-WMED real-time forecasts and to observations collected in the north-western Mediterranean area during the HyMeX SOP2. The comparison shows small differences in terms of net heat, <span class="hlt">water</span>, and momentum fluxes. On average, DWF is slightly sensitive to air-sea coupling. However, fine-scale <span class="hlt">ocean</span> processes, such as shelf DWF and export or eddies and fronts at the rim of the convective patch, are significantly modified. The wind-current interactions constitute an efficient coupled process at fine scale, acting as a turbulence propagating vectors, producing large mixing and convection at the rim of the convective patch.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1987AdSpR...7....3D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1987AdSpR...7....3D"><span>Future U.S. <span class="hlt">ocean</span> color missions-OCI, MODIS and HIRIS</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Davis, C. O.</p> <p></p> <p>The Coastal Zone Color Scanner (CZCS) launched by the National Aeronautics and Space Administration (NASA) on the Nimbus-7 Satellite in 1978 has provided exceptionally valuable data for studies of the productivity of the <span class="hlt">ocean</span>, fisheries, the detection of <span class="hlt">oceanic</span> fronts and currents, and the optical properties of the <span class="hlt">ocean</span>. NASA has been working with the scientific community, the National Oceanographic and Atmospheric Administration (NOAA), France's Centre National d'Etudes Spatiales (CNES), and industry to develop an <span class="hlt">Ocean</span> Color Imager (OCI), a follow-on instrument which would provide the near real-time and global data necessary to fill these needs in the 1990's. The Earth Observing Satellite Company (EOSAT) is considering flying an <span class="hlt">ocean</span> and land wide-field color instrument which would meet these needs on Landsat 6 or 7 planned for launch in 1989 and 1991, respectively. It would provide eight <span class="hlt">ocean</span> color channels for improved atmospheric correction and in-<span class="hlt">water</span> algorithms, global coverage and near real-time data for operational uses. In the mid 1990's NASA is planning to fly a Moderate Resolution Imaging Spectrometer (MODIS) and a High Resolution Imaging Spectrometer (HIRIS) as part of the Earth Observing System (Eos) on the Polar Platform of the Space Station. These instruments are array spectrometers which would provide full spectral resolution in the visible and infrared. This <span class="hlt">opens</span> the possibility of separating different groups of phytoplankton, suspended sediments and other substances in the <span class="hlt">water</span>. Also, HIRIS would have across track pointing ability which will allow high resolution rapid sampling of dynamic coastal areas and estuaries.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JGRC..121.7619S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JGRC..121.7619S"><span>Asymmetric <span class="hlt">oceanic</span> response to a hurricane: Deep <span class="hlt">water</span> observations during Hurricane Isaac</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Spencer, Laura J.; DiMarco, Steven F.; Wang, Zhankun; Kuehl, Joseph J.; Brooks, David A.</p> <p>2016-10-01</p> <p>The eye of Hurricane Isaac passed through the center of an array of six deep <span class="hlt">water</span> <span class="hlt">water</span>-column current meter moorings deployed in the northern Gulf of Mexico. The trajectory of the hurricane provided for a unique opportunity to quantify differences in the full <span class="hlt">water</span>-column <span class="hlt">oceanic</span> response to a hurricane to the left and right of the hurricane trajectory. Prior to the storm passage, relative vorticity on the right side of the hurricane was strongly negative, while on the left, relative vorticity was positive. This resulted in an asymmetry in the near-inertial frequencies <span class="hlt">oceanic</span> response at depth and horizontally. A shift in the response to a slightly larger inertial frequencies ˜1.11f was observed and verified by theory. Additionally, the storm passage coincided with an asymmetric change in relative vorticity in the upper 1000 m, which persisted for ˜15 inertial periods. Vertical propagation of inertial energy was estimated at 29 m/d, while horizontal propagation at this frequency was approximately 5.7 km/d. Wavelet analysis showed two distinct subinertial responses, one with a period of 2-5 days and another with a period of 5-12 days. Analysis of the subinertial bands reveals that the spatial and temporal scales are shorter and less persistent than the near-inertial variance. As the array is geographically located near the site of the Deep <span class="hlt">Water</span> Horizon oil spill, the spatial and temporal scales of response have significant implications for the fate, transport, and distribution of hydrocarbons following a deep <span class="hlt">water</span> spill event.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20000083900&hterms=3D+animation&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3D3D%2Banimation','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20000083900&hterms=3D+animation&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3D3D%2Banimation"><span>Hurricane Directional Wave Spectrum Spatial Variation in the <span class="hlt">Open</span> <span class="hlt">Ocean</span> and at Landfall</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Walsh, Edward J.; Wright, C. Wayne; Vandemark, Douglas C.; Krabill, William B.; Garcia, Andrew W.; Houston, Samuel H.; Powell, Mark D.; Black, Peter G.; Marks, Frank D.</p> <p>2000-01-01</p> <p>The sea surface directional wave spectrum was measured for the first time in all quadrants of a hurricane in <span class="hlt">open</span> <span class="hlt">water</span> using the NASA airborne scanning radar altimeter (SRA) carried aboard one of the NOAA WP-3D hurricane hunter aircraft at 1.5 km height. The SRA measures the energetic portion of the directional wave spectrum by generating a topographic map of the sea surface. At 8 Hz, the SRA sweeps a radar beam of 1' half-power width (two-way) across the aircraft ground track over a swath equal to 0.8 of the aircraft height, simultaneously measuring the backscattered power at its 36 GHz (8.3 mm) operating frequency and the range to the sea surface at 64 positions. These slant ranges are multiplied by the cosine of the off-nadir angles to determine the vertical distances from the aircraft to the sea surface. Subtracting these distances from the aircraft height produces the sea surface elevation map. The sea surface topography is interpolated to a uniform grid, transformed by a two dimensional FFT, and Doppler corrected. The <span class="hlt">open-ocean</span> data were acquired on 24 August 1998 when hurricane Bonnie was east of the Bahamas and moving toward 330 deg at about 5 m/s. Individual waves up to 18 m height were observed and the spatial variation of the wave field was dramatic. The dominant waves generally propagated at significant angles to the downwind direction. At some positions there were three different wave fields of comparable energy crossing each other. The NOAA aircraft spent over five hours within 180 km of the eye, and made five eye penetrations. On 26 August 1998, the NOAA aircraft flew at 2.2 km height when hurricane Bonnie was making landfall near Wilmington, NC, documenting the directional wave spectrum in the region between Charleston, SC and Cape Hatteras, NC. The aircraft flight lines included segments near and along the shoreline as well as far offshore. Animations of the directional wave spectrum spatial variation along the aircraft tracks on the two flights</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24553471','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24553471"><span>Phagotrophy by the picoeukaryotic green alga Micromonas: implications for Arctic <span class="hlt">Oceans</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>McKie-Krisberg, Zaid M; Sanders, Robert W</p> <p>2014-10-01</p> <p>Photosynthetic picoeukaryotes (PPE) are recognized as major primary producers and contributors to phytoplankton biomass in <span class="hlt">oceanic</span> and coastal environments. Molecular surveys indicate a large phylogenetic diversity in the picoeukaryotes, with members of the Prymnesiophyceae and Chrysophyseae tending to be more common in <span class="hlt">open</span> <span class="hlt">ocean</span> <span class="hlt">waters</span> and Prasinophyceae dominating coastal and Arctic <span class="hlt">waters</span>. In addition to their role as primary producers, PPE have been identified in several studies as mixotrophic and major predators of prokaryotes. Mixotrophy, the combination of photosynthesis and phagotrophy in a single organism, is well established for most photosynthetic lineages. However, green algae, including prasinophytes, were widely considered as a purely photosynthetic group. The prasinophyte Micromonas is perhaps the most common picoeukaryote in coastal and Arctic <span class="hlt">waters</span> and is one of the relatively few cultured representatives of the picoeukaryotes available for physiological investigations. In this study, we demonstrate phagotrophy by a strain of Micromonas (CCMP2099) isolated from Arctic <span class="hlt">waters</span> and show that environmental factors (light and nutrient concentration) affect ingestion rates in this mixotroph. In addition, we show size-selective feeding with a preference for smaller particles, and determine P vs I (photosynthesis vs irradiance) responses in different nutrient conditions. If other strains have mixotrophic abilities similar to Micromonas CCMP2099, the widespread distribution and frequently high abundances of Micromonas suggest that these green algae may have significant impact on prokaryote populations in several <span class="hlt">oceanic</span> regimes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSHE34A1459H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSHE34A1459H"><span>Assessing the role of solar radiation in heating, photosynthesis, and photo-oxidation in upper Arctic <span class="hlt">Ocean</span> <span class="hlt">waters</span> via autonomous buoys</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hill, V. J.; Steele, M.; Light, B.</p> <p>2016-02-01</p> <p>As part of the Arctic Observing Network, a new ice-tethered buoy has been developed for monitoring the role of sunlight in regulating <span class="hlt">ocean</span> temperature, phytoplankton growth, and carbon cycling. A 20 or 50 m string (depending on local bathymetry) supports sensors both within and below the ice for the hourly measurement of downwelling irradiance, temperature, Chlorophyll a, light backscattering, and dissolved organic material (DOM). Two buoys were deployed in March 2014 and two in March 2015. Because the buoys are engineered to survive melting out of first year ice, they have successfully provided complete seasonal records of <span class="hlt">water</span> column warming, phytoplankton abundance and photo-oxidation patterns in the Pacific Arctic Region. The data collected will be used to determine whether reduced ice extent and thinner ice are driving increases in under ice warming, accelerating bottom ice ablation, increasing available photosynthetic radiation to support large under ice blooms, and to quantify photo-oxidation of the DOM pool. Observations so far have revealed strong under ice daily warming as high as ±0.5 °C driven by local solar radiation. <span class="hlt">Water</span> column absorption was dominated by colored dissolved organic material which served to trap solar radiation in the upper <span class="hlt">water</span> column. Chlorophyll concentrations observed in June and July indicated high phytoplankton abundance beneath the ice. Light intensity at this time was not sufficient to support growth rates high enough to produce the 8 to 10 mg m-3 of chlorophyll observed. We hypothesize that phytoplankton were advected under the ice from the ice edge. However, once there phytoplankton were able to sustain low growth rates leading to nutrient limitation before <span class="hlt">open</span> <span class="hlt">water</span> status was reached. Strong daily cycles of photo-oxidation have also been observed in the late summer that indicate the fast cycling of highly labile DOM in the <span class="hlt">open</span> <span class="hlt">waters</span> of the Pacific Arctic Region.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_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://hdl.handle.net/2060/19920016369','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19920016369"><span>Microwave radiometer studies of atmospheric <span class="hlt">water</span> over the <span class="hlt">oceans</span>, volume 1</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.</p> <p>1992-01-01</p> <p>Since Seasat carried the Scanning Multichannel Microwave Radiometer (SMMR) into space, shortly followed by the SMMR on Nimbus 7, a new type of data source on atmospheric <span class="hlt">water</span> vapor and other meteorological parameters has been available for analysis of weather systems over the <span class="hlt">ocean</span>. Since 1987, the Scanning Multichannel Microwave/Imager (SMM/I) has provided similar data. A collection of work using this data is presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.B43G2220A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.B43G2220A"><span>Peatland <span class="hlt">Open-water</span> Pool Biogeochemistry: The Influence of Hydrology and Vegetation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Arsenault, J.; Talbot, J.; Moore, T. R.</p> <p>2017-12-01</p> <p>Peatland <span class="hlt">open-water</span> pools are net sources of carbon to the atmosphere. However, their interaction with the surrounding peat remains poorly known. In a previous study, we showed that shallow pools are richer in nutrients than deep pools. While depth was the main driver of biogeochemistry variations across time and space, analyses also showed that pool's adjacent vegetation may have an influence on <span class="hlt">water</span> chemistry. Our goal is to understand the relationship between the biogeochemistry of <span class="hlt">open-water</span> pools and their surroundings in a subboreal ombrotrophic peatland of southern Quebec (Canada). To assess the influence of vegetation on pool <span class="hlt">water</span> chemistry, we compare two areas covered with different types of vegetation: a forested zone dominated by spruce trees and an <span class="hlt">open</span> area mostly covered by Sphagnum spp. To evaluate the direction of <span class="hlt">water</span> (in or out of the pools), we installed capacitance <span class="hlt">water</span> level probes in transects linking pools in the two zones. Wells were also installed next to each probe to collect peat pore <span class="hlt">water</span> samples. Samples were taken every month during summer 2017 and analyzed for dissolved organic carbon, nitrogen and phosphorus, pH and specific UV absorbance. Preliminary results show differences in peat <span class="hlt">water</span> chemistry depending on the dominant vegetation. In both zones, <span class="hlt">water</span> levels fluctuations are disconnected between peat and the pools, suggesting poor horizontal <span class="hlt">water</span> movement. Pool <span class="hlt">water</span> chemistry may be mostly influenced by the immediate surrounding vegetation than by the local vegetation pattern. Climate and land-use change may affect the vegetation structure of peatlands, thus affecting pool biogeochemistry. Considering the impact of pools on the overall peatland capacity to accumulate carbon, our results show that more focus must be placed on pools to better understand peatland stability over time.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T33F..08N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T33F..08N"><span>Numerical simulations of <span class="hlt">water</span> transport in subduction zone: Influences of serpentinized layer in <span class="hlt">oceanic</span> slabs on subduction dynamics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nakao, A.; Hikaru, I.; Nakakuki, T.; Suzuki, Y.; Nakamura, H.</p> <p>2017-12-01</p> <p><span class="hlt">Water</span> liberated from subducting <span class="hlt">oceanic</span> slabs can affect the subduction dynamics such as mantle wedge flows and plate motion (e.g., Gerya & Meilick, 2011; Horiuchi & Iwamori, 2016; Nakao et al., 2016). However, how <span class="hlt">water</span> liberated from the slabs, in particular a hydrated part within the <span class="hlt">oceanic</span> lithosphere (e.g., Fujie et al., 2013), is transported and affects the subduction dynamics has not been fully understood. In order to clarify the roles of <span class="hlt">water</span> in subduction dynamics, we conducted 2-D dynamical simulations of <span class="hlt">water</span> transport and mantle convection without imposing the geometry and velocity of subducting slabs. Using the simulations with various thicknesses (0-20 km) of a partially serpentinized layer (hereafter referred to as "SL") underlaying the altered <span class="hlt">oceanic</span> basalt crust (AOC) in the subducting <span class="hlt">oceanic</span> lithosphere, we estimate the subduction rate, back-arc spreading, trench migration, and slab geometry. The simulations show that the plate motion significantly changes depending on the amount of liberated <span class="hlt">water</span>. When the SL is absent (0 km thick), the AOC mostly dehydrates at shallow depths (< 70 km). In this case, the plate subducts slowly, the trench is stationary, and the slab penetrates the 660-km boundary. If the SL is 7.5 km in thickness, it dehydrates at a greater depth compared to AOC, and more <span class="hlt">water</span> enters the mantle wedge and the back-arc region. The liberated <span class="hlt">water</span> reduces the viscosity of mantle wedge, and consequently, the subduction rate increases, the trench migrates seaward, and the slab stagnates on the 660-km. If the SL is 20 km in thickness, the upper SL releases much <span class="hlt">water</span> into the mantle wedge and the back-arc region, whereas the lower SL does not dehydrate because of <span class="hlt">water</span> uptake by phase A and phase D. In this case, because buoyancy of the subducting slab increases, the subduction is slow, back-arc spreading is weakened, and the slab penetrates the 660-km. Our results imply that the observed variety of subducting slabs reflects</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/20741123-control-water-erosion-sediment-open-cut-coal-mines-tropical-areas','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/20741123-control-water-erosion-sediment-open-cut-coal-mines-tropical-areas"><span>Control of <span class="hlt">water</span> erosion and sediment in <span class="hlt">open</span> cut coal mines in tropical areas</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>Ueda, T.; Nugraha, C.; Matsui, K.</p> <p>2005-07-01</p> <p>The purpose is to reduce the environmental impacts from <span class="hlt">open</span> cut mining in tropical areas, such as Indonesia and Vietnam. Research conducted on methods for the control of <span class="hlt">water</span> erosion and sediment from <span class="hlt">open</span> cut coal mines is described. Data were collected on climate and weathering in tropical areas, mechanism of <span class="hlt">water</span> erosion and sedimentation, characteristics of rocks in coal measures under wet conditions, <span class="hlt">water</span> management at pits and haul roads and ramps, and construction of waste dumps and <span class="hlt">water</span> management. The results will be applied to the optimum control and management of erosion and sediments in <span class="hlt">open</span> cut mining.more » 6 refs., 8 figs.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29567220','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29567220"><span>Effects of electrode gap and electric current on chlorine generation of electrolyzed deep <span class="hlt">ocean</span> <span class="hlt">water</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hsu, Guoo-Shyng Wang; Hsu, Shun-Yao</p> <p>2018-04-01</p> <p>Electrolyzed <span class="hlt">water</span> is a sustainable disinfectant, which can comply with food safety regulations and is environmental friendly. A two-factor central composite design was adopted for studying the effects of electrode gap and electric current on chlorine generation efficiency of electrolyzed deep <span class="hlt">ocean</span> <span class="hlt">water</span>. Deep <span class="hlt">ocean</span> <span class="hlt">water</span> was electrolyzed in a glass electrolyzing cell equipped with platinum-plated titanium anode and cathode in a constant-current operation mode. Results showed that current density, chlorine concentration, and electrolyte temperature increased with electric current, while electric efficiency decreased with electric current and electrode gap. An electrode gap of less than 11.7 mm, and a low electric current appeared to be a more energy efficient design and operation condition for the electrolysis system. Copyright © 2017. Published by Elsevier B.V.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015OcMod..85...56B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015OcMod..85...56B"><span>Lagrangian <span class="hlt">water</span> mass tracing from pseudo-Argo, model-derived salinity, tracer and velocity data: An application to Antarctic Intermediate <span class="hlt">Water</span> in the South Atlantic <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Blanke, Bruno; Speich, Sabrina; Rusciano, Emanuela</p> <p>2015-01-01</p> <p>We use the tracer and velocity fields of a climatological <span class="hlt">ocean</span> model to investigate the ability of Argo-like data to estimate accurately <span class="hlt">water</span> mass movements and transformations, in the style of analyses commonly applied to the output of <span class="hlt">ocean</span> general circulation model. To this end, we introduce an algorithm for the reconstruction of a fully non-divergent three-dimensional velocity field from the simple knowledge of the model vertical density profiles and 1000-m horizontal velocity components. The validation of the technique consists in comparing the resulting pathways for Antarctic Intermediate <span class="hlt">Water</span> in the South Atlantic <span class="hlt">Ocean</span> to equivalent reference results based on the full model information available for velocity and tracers. We show that the inclusion of a wind-induced Ekman pumping and of a well-thought-out expression for vertical velocity at the level of the intermediate <span class="hlt">waters</span> is essential for the reliable reproduction of quantitative Lagrangian analyses. Neglecting the seasonal variability of the velocity and tracer fields is not a significant source of errors, at least well below the permanent thermocline. These results give us confidence in the success of the adaptation of the algorithm to true gridded Argo data for investigating the dynamics of flows in the <span class="hlt">ocean</span> interior.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1994PalOc...9..723L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1994PalOc...9..723L"><span>Quantitative estimation of surface <span class="hlt">ocean</span> productivity and bottom <span class="hlt">water</span> oxygen concentration using benthic foraminifera</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Loubere, Paul</p> <p>1994-10-01</p> <p>An electronic supplement of this material may be obtained on adiskette or Anonymous FTP from KOSMOS.AGU.ORG. (LOGIN toAGU's FTP account using ANONYMOUS as the usemame andGUEST as the password. Go to the right directory by typing CDAPEND. Type LS to see what files are available. Type GET and thename of the file to get it. Finally, type EXIT to leave the system.)(Paper 94PA01624, Quantitative estimation of surface oceanproductivity and bottom <span class="hlt">water</span> concentration using benthicforaminifera, by P. Loubere). Diskette may be ordered from AmericanGeophysical Union, 2000 Florida Avenue, N.W., Washington, DC20009; $15.00. Payment must accompany order.Quantitative estimation of surface <span class="hlt">ocean</span> productivity and bottom <span class="hlt">water</span> oxygen concentration with benthic foraminifera was attempted using 70 samples from equatorial and North Pacific surface sediments. These samples come from a well defined depth range in the <span class="hlt">ocean</span>, between 2200 and 3200 m, so that depth related factors do not interfere with the estimation. Samples were selected so that foraminifera were well preserved in the sediments and temperature and salinity were nearly uniform (T = 1.5° C; S = 34.6‰). The sample set was also assembled so as to minimize the correlation often seen between surface <span class="hlt">ocean</span> productivity and bottom <span class="hlt">water</span> oxygen values (r² = 0.23 for prediction purposes in this case). This procedure reduced the chances of spurious results due to correlations between the environmental variables. The samples encompass a range of productivities from about 25 to >300 gC m-2 yr-1, and a bottom <span class="hlt">water</span> oxygen range from 1.8 to 3.5 ml/L. Benthic foraminiferal assemblages were quantified using the >62 µm fraction of the sediments and 46 taxon categories. MANOVA multivariate regression was used to project the faunal matrix onto the two environmental dimensions using published values for productivity and bottom <span class="hlt">water</span> oxygen to calibrate this operation. The success of this regression was measured with the multivariate r</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28459347','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28459347"><span>Characteristics and Challenges of <span class="hlt">Open-Water</span> Swimming Performance: A Review.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Baldassarre, Roberto; Bonifazi, Marco; Zamparo, Paola; Piacentini, Maria Francesca</p> <p>2017-11-01</p> <p>Although the popularity of <span class="hlt">open-water</span> swimming (OWS) events has significantly increased in the last decades, specific studies regarding performance of elite or age-group athletes in these events are scarce. To analyze the existing literature on OWS. Relevant literature was located via computer-generated citations. During August 2016, online computer searches on PubMed and Scopus databases were conducted to locate published research. The number of participants in ultraendurance swimming events has substantially increased in the last 10 y. In elite athletes there is a higher overall competitive level of women than of men. The body composition of female athletes (different percentage and distribution of fat tissue) shows several advantages (more buoyancy and less drag) in aquatic conditions that determine the small difference between males and females. The main physiological characteristics of <span class="hlt">open-water</span> swimmers (OW swimmers) are the ability to swim at high percentage of [Formula: see text] (80-90%) for many hours. Furthermore, to sustain high velocity for many hours, endurance swimmers need a high propelling efficiency and a low energy cost. <span class="hlt">Open-water</span> races may be characterized by extreme environmental conditions (<span class="hlt">water</span> temperature, tides, currents, and waves) that have an overall impact on performance, influencing tactics and pacing. Future studies are needed to study OWS in both training and competition.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMOS11A1128B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMOS11A1128B"><span>Sentinel-3 SAR Altimetry over Coastal and <span class="hlt">Open</span> <span class="hlt">Ocean</span>: performance assessment and improved retrieval methods in the ESA SCOOP Project.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Benveniste, J.; Cotton, D.; Moreau, T.; Raynal, M.; Varona, E.; Cipollini, P.; Cancet, M.; Martin, F.; Fenoglio-Marc, L.; Naeije, M.; Fernandes, J.; Lazaro, C.; Restano, M.; Ambrózio, A.</p> <p>2017-12-01</p> <p>The ESA Sentinel-3 satellite, launched in February 2016 as a part of the Copernicus programme, is the second satellite to operate a SAR mode altimeter. The Sentinel 3 Synthetic Aperture Radar Altimeter (SRAL) is based on the heritage from Cryosat-2, but this time complemented by a Microwave Radiometer (MWR) to provide a wet troposphere correction, and operating at Ku and C-Bands to provide an accurate along-track ionospheric correction. The SRAL is operated in SAR mode over the whole <span class="hlt">ocean</span> and promises increased performance w.r.t. conventional altimetry. SCOOP (SAR Altimetry Coastal & <span class="hlt">Open</span> <span class="hlt">Ocean</span> Performance) is a project funded under the ESA SEOM (Scientific Exploitation of Operational Missions) Programme Element, started in September 2015, to characterise the expected performance of Sentinel-3 SRAL SAR mode altimeter products, in the coastal zone and <span class="hlt">open-ocean</span>, and then to develop and evaluate enhancements to the baseline processing scheme in terms of improvements to <span class="hlt">ocean</span> measurements. There is also a work package to develop and evaluate an improved Wet Troposphere correction for Sentinel-3, based on the measurements from the on-board MWR, further enhanced mostly in the coastal and polar regions using third party data, and provide recommendations for use. In this presentation we present results from the SCOOP project that demonstrate the excellent performance of SRAL in terms of measurement precision, and we illustrate the development and testing of new processing approaches designed specifically to improve performance close to the coast. The SCOOP test data sets and relevant documentation are available to external researchers on application to the project team. At the end of the project recommendations for further developments and implementations will be provided through a scientific roadmap.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1998EOSTr..79S.494S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1998EOSTr..79S.494S"><span>Taking the <span class="hlt">ocean</span> pledge</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Showstack, Randy</p> <p></p> <p>The National <span class="hlt">Oceanic</span> and Atmospheric Administration (NOAA) is sponsoring an "<span class="hlt">ocean</span> ambassadors pledge campaign" to encourage students and others to make a personal, long-term commitment to caring for the world's <span class="hlt">oceans</span>.The pledge campaign, which is part of NOAA's public awareness efforts for the International Year of the <span class="hlt">Ocean</span>, calls for people to learn what they can about <span class="hlt">oceans</span>, be considerate to <span class="hlt">ocean</span> wildlife, conserve <span class="hlt">water</span>, and implement other simple measures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20150021521&hterms=sea&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dsea','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20150021521&hterms=sea&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dsea"><span>An Assessment of Southern <span class="hlt">Ocean</span> <span class="hlt">Water</span> Masses and Sea Ice During 1988-2007 in a Suite of Interannual CORE-II Simulations</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Downes, Stephanie M.; Farneti, Riccardo; Uotila, Petteri; Griffies, Stephen M.; Marsland, Simon J.; Bailey, David; Behrens, Erik; Bentsen, Mats; Bi, Daohua; Biastoch, Arne; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20150021521'); toggleEditAbsImage('author_20150021521_show'); toggleEditAbsImage('author_20150021521_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20150021521_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20150021521_hide"></p> <p>2015-01-01</p> <p>We characterise the representation of the Southern <span class="hlt">Ocean</span> <span class="hlt">water</span> mass structure and sea ice within a suite of 15 global <span class="hlt">ocean</span>-ice models run with the Coordinated <span class="hlt">Ocean</span>-ice Reference Experiment Phase II (CORE-II) protocol. The main focus is the representation of the present (1988-2007) mode and intermediate <span class="hlt">waters</span>, thus framing an analysis of winter and summer mixed layer depths; temperature, salinity, and potential vorticity structure; and temporal variability of sea ice distributions. We also consider the interannual variability over the same 20 year period. Comparisons are made between models as well as to observation-based analyses where available. The CORE-II models exhibit several biases relative to Southern <span class="hlt">Ocean</span> observations, including an underestimation of the model mean mixed layer depths of mode and intermediate <span class="hlt">water</span> masses in March (associated with greater <span class="hlt">ocean</span> surface heat gain), and an overestimation in September (associated with greater high latitude <span class="hlt">ocean</span> heat loss and a more northward winter sea-ice extent). In addition, the models have cold and fresh/warm and salty <span class="hlt">water</span> column biases centred near 50 deg S. Over the 1988-2007 period, the CORE-II models consistently simulate spatially variable trends in sea-ice concentration, surface freshwater fluxes, mixed layer depths, and 200-700 m <span class="hlt">ocean</span> heat content. In particular, sea-ice coverage around most of the Antarctic continental shelf is reduced, leading to a cooling and freshening of the near surface <span class="hlt">waters</span>. The shoaling of the mixed layer is associated with increased surface buoyancy gain, except in the Pacific where sea ice is also influential. The models are in disagreement, despite the common CORE-II atmospheric state, in their spatial pattern of the 20-year trends in the mixed layer depth and sea-ice.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSED34B1691W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSED34B1691W"><span>The <span class="hlt">Ocean</span> Acidification Curriculum Collection - sharing <span class="hlt">ocean</span> science resources for k-12 classrooms</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>2016-02-01</p> <p>The fish and shellfish provided by ecosystems that abound in the <span class="hlt">waters</span> of Puget Sound have sustained the Suquamish Tribe for millennia. However, years of development, pollution and over-harvest have reduced some fish and shellfish populations to just a fraction of their former abundance. Now, <span class="hlt">ocean</span> acidification (OA) and climate change pose additional threats to these essential natural resources. <span class="hlt">Ocean</span> acidification can't be stopped; however, many of the other human-caused stressors to <span class="hlt">ocean</span> health can. If human behaviors that harm <span class="hlt">ocean</span> health can be modified to reduce impacts, fish populations and ecosystems could become more resilient to the changing <span class="hlt">ocean</span> conditions. School is arguably the best place to convey the ideas and awareness needed for people to adopt new behaviors. Students are <span class="hlt">open</span> to new ideas and they influence their peers and parents. In addition, they are captive audiences in classrooms for many years.The Suquamish Tribe is helping to foster new generations of <span class="hlt">ocean</span> stewards by creating an online searchable database (OACurriculumCollection.org). This site is designed to facilitate finding, reviewing and sharing free educational materials on OA. At the same time, the Next Generation Science Standards (NGSS) were released providing a great opportunity to get new materials into classrooms. OA provides highly appropriate context to teach many of the ideas in the new standards making it attractive to teachers looking for interesting and relevant materials. In this presentation, we will demonstrate how teachers can use the site as a place to find and share materials on OA. We will also present a framework developed by teachers for understanding OA, its impacts, and the many ways students can help ease the impacts on <span class="hlt">ocean</span> ecosystems. We will provide examples of how OA can be used as context and content for the NGSS and finally, we will discuss the failures and successes on our journey to get relevant materials into the classroom.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930005782&hterms=McDougall&qs=N%3D0%26Ntk%3DAuthor-Name%26Ntx%3Dmode%2Bmatchall%26Ntt%3DMcDougall','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930005782&hterms=McDougall&qs=N%3D0%26Ntk%3DAuthor-Name%26Ntx%3Dmode%2Bmatchall%26Ntt%3DMcDougall"><span><span class="hlt">Ocean</span> transport and variability studies of the South Pacific, Southern, and Indian <span class="hlt">Oceans</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Church, John A.; Cresswell, G. R.; Nilsson, C. S.; Mcdougall, T. J.; Coleman, R.; Rizos, C.; Penrose, J.; Hunter, J. R.; Lynch, M. J.</p> <p>1991-01-01</p> <p>The objectives of this study are to analyze <span class="hlt">ocean</span> dynamics in the western South Pacific and the adjacent Southern <span class="hlt">Ocean</span> and the eastern Indian <span class="hlt">Ocean</span>. Specifically, our objectives for these three regions are, for the South Pacific <span class="hlt">Ocean</span>: (1) To estimate the volume transport of the east Australian Current (EAC) along the Australian coast and in the Tasman Front, and to estimate the time variability (on seasonal and interannual time scales) of this transport. (2) To contribute to estimating the meridional heat and freshwater fluxes (and their variability) at about 30 deg S. Good estimates of the transport in the western boundary current are essential for accurate estimates of these fluxes. (3) To determine how the EAC transport (and its extension, the Tasman Front and the East Auckland Current) closes the subtropical gyre of the South Pacific and to better determine the structure at the confluence of this current and the Antarctic Circumpolar Current. (4) To examine the structure and time variability of the circulation in the western South Pacific and the adjacent Southern <span class="hlt">Ocean</span>, particularly at the Tasman Front. For the Indian <span class="hlt">Ocean</span>: (5) To study the seasonal interannual variations in the strength of the Leeuwin Current. (6) To monitor the Pacific-Indian <span class="hlt">Ocean</span> throughflow and the South Equatorial and the South Java Currents between northwest Australia and Indonesia. (7) To study the processes that form the <span class="hlt">water</span> of the permanent <span class="hlt">oceanic</span> thermocline and, in particular, the way in which new thermocline <span class="hlt">water</span> enters the permanent thermocline in late winter and early spring as the mixed layer restratifies. For the Southern <span class="hlt">Ocean</span>: (8) To study the mesoscale and meridional structure of the Southern <span class="hlt">Ocean</span> between 150 deg E and 170 deg E; in particular, to describe the Antarctic frontal system south of Tasmania and determine its interannual variability; to estimate the exchanges of heat, salt, and other properties between the Indian and Pacific <span class="hlt">Oceans</span>; and to investigate the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27478277','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27478277"><span>Photoreduction of Terrigenous Fe-Humic Substances Leads to Bioavailable Iron in <span class="hlt">Oceans</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Blazevic, Amir; Orlowska, Ewelina; Kandioller, Wolfgang; Jirsa, Franz; Keppler, Bernhard K; Tafili-Kryeziu, Myrvete; Linert, Wolfgang; Krachler, Rudolf F; Krachler, Regina; Rompel, Annette</p> <p>2016-05-23</p> <p>Humic substances (HS) are important iron chelators responsible for the transport of iron from freshwater systems to the <span class="hlt">open</span> sea, where iron is essential for marine organisms. Evidence suggests that iron complexed to HS comprises the bulk of the iron ligand pool in near-coastal <span class="hlt">waters</span> and shelf seas. River-derived HS have been investigated to study their transport to, and dwell in <span class="hlt">oceanic</span> <span class="hlt">waters</span>. A library of iron model compounds and river-derived Fe-HS samples were probed in a combined X-ray absorption spectroscopy (XAS) and valence-to-core X-ray emission spectroscopy (VtC-XES) study at the Fe K-edge. The analyses performed revealed that iron complexation in HS samples is only dependent on oxygen-containing HS functional groups, such as carboxyl and phenol. The photoreduction mechanism of Fe III -HS in <span class="hlt">oceanic</span> conditions into bioavailable aquatic Fe II forms, highlights the importance of river-derived HS as an iron source for marine organisms. Consequently, such mechanisms are a vital component of the upper-<span class="hlt">ocean</span> iron biogeochemistry cycle.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/486164','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/486164"><span>The Europa <span class="hlt">Ocean</span> Discovery mission</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>Edwards, B.C.; Chyba, C.F.; Abshire, J.B.</p> <p>1997-06-01</p> <p>Since it was first proposed that tidal heating of Europa by Jupiter might lead to liquid <span class="hlt">water</span> <span class="hlt">oceans</span> below Europa`s ice cover, there has been speculation over the possible exobiological implications of such an <span class="hlt">ocean</span>. Liquid <span class="hlt">water</span> is the essential ingredient for life as it is known, and the existence of a second <span class="hlt">water</span> <span class="hlt">ocean</span> in the Solar System would be of paramount importance for seeking the origin and existence of life beyond Earth. The authors present here a Discovery-class mission concept (Europa <span class="hlt">Ocean</span> Discovery) to determine the existence of a liquid <span class="hlt">water</span> <span class="hlt">ocean</span> on Europa and to characterize Europa`smore » surface structure. The technical goal of the Europa <span class="hlt">Ocean</span> Discovery mission is to study Europa with an orbiting spacecraft. This goal is challenging but entirely feasible within the Discovery envelope. There are four key challenges: entering Europan orbit, generating power, surviving long enough in the radiation environment to return valuable science, and complete the mission within the Discovery program`s launch vehicle and budget constraints. The authors will present here a viable mission that meets these challenges.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015OcScD..12.1187D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015OcScD..12.1187D"><span><span class="hlt">Ocean</span> modelling for aquaculture and fisheries in Irish <span class="hlt">waters</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dabrowski, T.; Lyons, K.; Cusack, C.; Casal, G.; Berry, A.; Nolan, G. D.</p> <p>2015-06-01</p> <p>The Marine Institute, Ireland, runs a suite of operational regional and coastal <span class="hlt">ocean</span> models. Recent developments include several tailored products that focus on the key needs of the Irish aquaculture sector. In this article, an overview of the products and services derived from the models are presented. A shellfish model that includes growth and physiological interactions of mussels with the ecosystem and is fully embedded in the 3-D numerical modelling framework has been developed at the Marine Institute. This shellfish model has a microbial module designed to predict levels of coliform contamination in mussels. This model can also be used to estimate the carrying capacity of embayments, assess impacts of pollution on aquaculture grounds and help to classify shellfish <span class="hlt">waters</span>. The physical coastal model of southwest Ireland provides a three day forecast of shelf <span class="hlt">water</span> movement in the region. This is assimilated into a new harmful algal bloom alert system used to inform end-users of potential toxic shellfish events and high biomass blooms that include fish killing species. Further services include the use of models to identify potential sites for offshore aquaculture, to inform studies of potential cross-contamination in farms from the dispersal of planktonic sea lice larvae and other pathogens that can infect finfish and to provide modelled products that underpin the assessment and advisory services on the sustainable exploitation of the marine fisheries resources. This paper demonstrates that <span class="hlt">ocean</span> models can provide an invaluable contribution to the sustainable blue growth of aquaculture and fisheries.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26119338','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26119338"><span>Pliocene cooling enhanced by flow of low-salinity Bering Sea <span class="hlt">water</span> to the Arctic <span class="hlt">Ocean</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Horikawa, Keiji; Martin, Ellen E; Basak, Chandranath; Onodera, Jonaotaro; Seki, Osamu; Sakamoto, Tatsuhiko; Ikehara, Minoru; Sakai, Saburo; Kawamura, Kimitaka</p> <p>2015-06-29</p> <p>Warming of high northern latitudes in the Pliocene (5.33-2.58 Myr ago) has been linked to the closure of the Central American Seaway and intensification of North Atlantic Deep <span class="hlt">Water</span>. Subsequent cooling in the late Pliocene may be related to the effects of freshwater input from the Arctic <span class="hlt">Ocean</span> via the Bering Strait, disrupting North Atlantic Deep <span class="hlt">Water</span> formation and enhancing sea ice formation. However, the timing of Arctic freshening has not been defined. Here we present neodymium and lead isotope records of detrital sediment from the Bering Sea for the past 4.3 million years. Isotopic data suggest the presence of Alaskan glaciers as far back as 4.2 Myr ago, while diatom and C37:4 alkenone records show a long-term trend towards colder and fresher <span class="hlt">water</span> in the Bering Sea beginning with the M2 glaciation (3.3 Myr ago). We argue that the introduction of low-salinity Bering Sea <span class="hlt">water</span> to the Arctic <span class="hlt">Ocean</span> by 3.3 Myr ago preconditioned the climate system for global cooling.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4491831','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4491831"><span>Pliocene cooling enhanced by flow of low-salinity Bering Sea <span class="hlt">water</span> to the Arctic <span class="hlt">Ocean</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>Horikawa, Keiji; Martin, Ellen E.; Basak, Chandranath; Onodera, Jonaotaro; Seki, Osamu; Sakamoto, Tatsuhiko; Ikehara, Minoru; Sakai, Saburo; Kawamura, Kimitaka</p> <p>2015-01-01</p> <p>Warming of high northern latitudes in the Pliocene (5.33–2.58 Myr ago) has been linked to the closure of the Central American Seaway and intensification of North Atlantic Deep <span class="hlt">Water</span>. Subsequent cooling in the late Pliocene may be related to the effects of freshwater input from the Arctic <span class="hlt">Ocean</span> via the Bering Strait, disrupting North Atlantic Deep <span class="hlt">Water</span> formation and enhancing sea ice formation. However, the timing of Arctic freshening has not been defined. Here we present neodymium and lead isotope records of detrital sediment from the Bering Sea for the past 4.3 million years. Isotopic data suggest the presence of Alaskan glaciers as far back as 4.2 Myr ago, while diatom and C37:4 alkenone records show a long-term trend towards colder and fresher <span class="hlt">water</span> in the Bering Sea beginning with the M2 glaciation (3.3 Myr ago). We argue that the introduction of low-salinity Bering Sea <span class="hlt">water</span> to the Arctic <span class="hlt">Ocean</span> by 3.3 Myr ago preconditioned the climate system for global cooling. PMID:26119338</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFMGC51F1060B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFMGC51F1060B"><span>Freshwater and polynya components of the shelf-derived Arctic <span class="hlt">Ocean</span> halocline in summer 2007 identified by stable oxygen isotopes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bauch, D.; Rutgers van der Loeff, M.; Andersen, N.; Torres-Valdes, S.; Bakker, K.; Abrahamsen, E.</p> <p>2011-12-01</p> <p>With the aim of determining the origin of freshwater in the halocline, fractions of river <span class="hlt">water</span> and sea-ice meltwater (or brine influence from sea-ice formation) in the upper 150 m were quantified by a combination of salinity and δ18O and nutrients in the Eurasian basins and the Makarov Basin. Our study indicates which layers of the Arctic <span class="hlt">Ocean</span> halocline are primarily influenced by sea-ice formation in coastal polynyas and which are primarily influenced by sea-ice formation over the <span class="hlt">open</span> <span class="hlt">ocean</span>. With the ongoing changes in sea-ice coverage in the Arctic <span class="hlt">Ocean</span> it can be expected that these processes will change in the immediate future and that the relative contributions to the halocline will change accordingly. Within the Eurasian Basin a west to east oriented front between net melting and production of sea-ice is observed. Outside the Atlantic regime dominated by net sea-ice melting, a pronounced layer influenced by brines released during sea-ice formation is present at about 30 to 50 m <span class="hlt">water</span> depth with a maximum over the Lomonosov Ridge. The geographically distinct definition of this maximum demonstrates the rapid release and transport of signals from the shelf regions in discrete pulses within the Transpolar Drift. We use the ratio of sea-ice derived brine influence and river <span class="hlt">water</span> to link the maximum in brine influence within the Transpolar Drift with a pulse of shelf <span class="hlt">waters</span> from the Laptev Sea likely released in summer 2005. For a distinction of Atlantic and Pacific-derived contributions the initial phosphate corrected for mineralization with oxygen (PO*) and alternatively the nitrate to phosphate ratio (N/P) in each sample were used. While PO*-based assessments systematically underestimate the contribution of Pacific-derived <span class="hlt">waters</span>, N/P-based calculations overestimate Pacific-derived <span class="hlt">waters</span> within the Transpolar Drift due to denitrification in bottom sediments of the Laptev Sea. The extent of Pacific-derived <span class="hlt">water</span> in the Arctic <span class="hlt">Ocean</span> was approximately limited</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.1396K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.1396K"><span>Tensions between <span class="hlt">opening</span> up and closing down moments in transdisciplinary <span class="hlt">water</span> research</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Krueger, Tobias; Maynard, Carly; Carr, Gemma; Bruns, Antje; Mueller, Eva; Lane, Stuart</p> <p>2016-04-01</p> <p>Research on <span class="hlt">water</span> is carried out by many disciplines that do not really talk to each other much, despite critical interactions of multiple social and biophysical processes in shaping how much and what kind of <span class="hlt">water</span> is where, at what time and for whom. What is more, <span class="hlt">water</span> has meaning to more than those who are scientists. And scientists are not so removed from the things they study as one might commonly believe. All these observations call for a transdisciplinary research agenda that brings together different scientific disciplines with the knowledge that other groups in society hold and that tries to be aware of its own limitations. The transdisciplinary perspective is especially pertinent to the scientific decade 2013-2022 of the International Association of Hydrological Sciences (IAHS) on change in hydrology and society, 'Panta Rhei,' for a balanced conceptualization and study of human-<span class="hlt">water</span> relations. Transdisciplinarity is inherently about <span class="hlt">opening</span> up traditional modes of knowledge production; in terms of framing the research problem, the methodology and the knowledge that is considered permissible. This should <span class="hlt">open</span> up the range of options for management intervention, too. While decisions on how to intervene will inevitably close down the issue periodically, the point here is to leave alternative routes of action <span class="hlt">open</span> long enough, or reopen them again, so as to counter unsustainable and inequitable path-dependencies and lock-ins. However, <span class="hlt">opening</span> up efforts are frequently in conflict with factors that work to close down knowledge production. Among those are framings, path-dependencies, vested interests, researchers' positionalities, power, and scale. In this presentation, based on Krueger et al. (2016), we will reflect on the tensions between <span class="hlt">opening</span> up and closing down moments in transdisciplinary <span class="hlt">water</span> research and draw important practical lessons. References Krueger, T., Maynard, C.M., Carr, G., Bruns, A., Mueller, E.N. and Lane, S.N. 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