Sample records for water antarctic intermediate

  1. Formation of Antarctic Intermediate Water during the Plio-Pleistocene

    NASA Astrophysics Data System (ADS)

    Karas, C.; Goldstein, S. L.; deMenocal, P. B.

    2017-12-01

    Antarctic Intermediate Water (AAIW) plays a fundamental role in modern climate change. It is an important sink for anthropogenic CO2, it represents an important source water in several (sub)tropical upwelling regions and it is the coldwater route from the Southern Hemisphere to the North Atlantic Ocean replacing North Atlantic Deep Water (NADW). During the last 4 million years, which marks the transition from the warm Pliocene climate towards icehouse conditions, the formation of this watermass is still largely unknown. We here present a multi-proxy approach using neodymium isotopes (ɛNd) on Fe-Mn encrusted foraminifera and coupled benthic Mg/Ca and stable isotopes from South Atlantic Site 516, within AAIW, to reconstruct its variability. Our data show that the modern formation of AAIW started about 3 million years ago, indicated by a distinct drop of ɛNd by 1.5, a cooling and freshening of benthic TMg/Ca by 8°C and a drop in benthic d13C values towards modern times. We interpret these changes as a reduced inflow of Pacific waters into the South Atlantic and the onset of modern deep vertical mixing at the source regions of AAIW near the polar front. These processes had significant effects on the CO2 storage of the ocean that supported global cooling and the intensification of the Northern Hemisphere Glaciation.

  2. Multi-proxy Reconstructions of Deglacial Variability of Antarctic Intermediate Water Circulation in the Western Tropical Atlantic

    NASA Astrophysics Data System (ADS)

    Huang, K.; Oppo, D.; Curry, W. B.

    2012-12-01

    Reconstruction of changes in Antarctic Intermediate Water (AAIW) circulation across the last deglaciation is critical in constraining the links between AAIW and Atlantic Meridional Overturning Circulation (AMOC) and understanding how AAIW influences oceanic heat transport and carbon budget across abrupt climate events. Here we systematically establish in situ calibrations for carbonate saturation state (B/Ca), nutrient (Cd/Ca and δ13C) and watermass proxies (ɛNd) in foraminifera using multicore tops and ambient seawater samples collected from the Demerara Rise, western tropical Atlantic. Through the multi-proxy reconstructions, deglacial variability of intermediate water circulation in the western tropical Atlantic can be further constrained. The reconstructed seawater Cd record from the Demerara Rise sediment core (KNR197-3-46CDH, at 947 m water depth) over the last 21 kyrs suggests reduced presence of AAIW during the cold intervals (LGM, H1 and YD) when AMOC was reduced. Down-core B/Ca record shows elevated intermediate water Δ[CO32-] during these cold intervals, further indicating a weaker influence of AAIW in the western tropical Atlantic. The δ13C record exhibits a pronounced deglacial minimum and a clear decoupling between δ13C and Cd/Ca after the AMOC completely recovered at around 8 kyr BP. This could be due to the carbonate ion effect on benthic Cd/Ca or the influence of organic matter remineralization on benthic δ13C. A new ɛNd record for the last deglaciation will be provided to evaluate the relative proportions of southern and northern waters at this intermediate site in the western tropical Atlantic.

  3. Deglacial variability of Antarctic Intermediate Water penetration into the North Atlantic from authigenic neodymium isotope ratios

    NASA Astrophysics Data System (ADS)

    Xie, Ruifang C.; Marcantonio, Franco; Schmidt, Matthew W.

    2012-09-01

    Understanding intermediate water circulation across the last deglacial is critical in assessing the role of oceanic heat transport associated with Atlantic Meridional Overturning Circulation variability across abrupt climate events. However, the links between intermediate water circulation and abrupt climate events such as the Younger Dryas (YD) and Heinrich Event 1 (H1) are still poorly constrained. Here, we reconstruct changes in Antarctic Intermediate Water (AAIW) circulation in the subtropical North Atlantic over the past 25 kyr by measuring authigenic neodymium isotope ratios in sediments from two sites in the Florida Straits. Our authigenic Nd isotope records suggest that there was little to no penetration of AAIW into the subtropical North Atlantic during the YD and H1. Variations in the northward penetration of AAIW into the Florida Straits documented in our authigenic Nd isotope record are synchronous with multiple climatic archives, including the Greenland ice core δ18O record, the Cariaco Basin atmosphere Δ14C reconstruction, the Bermuda Rise sedimentary Pa/Th record, and nutrient and stable isotope data from the tropical North Atlantic. The synchroneity of our Nd records with multiple climatic archives suggests a tight connection between AAIW variability and high-latitude North Atlantic climate change.

  4. Did Antarctic Intermediate Water in the Southeast Pacific expanded vertically or only deepened?

    NASA Astrophysics Data System (ADS)

    Martinez-Mendez, G.; Lamy, F.; Mohtadi, M.; Hebbeln, D.

    2017-12-01

    Paleoceanographic and modelling studies have demonstrated in the last few years that deep waters are not the single protagonists in the global circulation scheme. Intermediate waters also play various and important roles. Particularly, the Antarctic Intermediate Water (AAIW) is key for the ventilation of mid-depths and thermocline levels, with its influence being noticeable till the eastern equatorial Pacific; it is involved in rapid reorganizations of the Global Circulation and also, most plausibly, in trapping and releasing atmospheric CO2 on glacial-interglacial time scales. In recent years, several records about the past variability of the AAIW have been published while they all lay at the lower edges of the influence of this water mass and, hence, mostly only conclusions about the AAIW variability at its deep boundary could be drawn. Here we present a novel record covering several glacial-interglacial cycles from the upper levels of this water mass. Site GeoB15020 was drilled with the MARUM Sea floor drill rig (MeBo) off Chile (27.29°S; 71.05°W) at 550 m water depth (core length: 78 meters composite depth). We will present δ18O, δ13C downcore records and Mg/Ca-derived ambient temperature from peak interglacial and peak glacial periods. The records will be compared with published results from Site GeoB15016 (Martínez-Méndez et al., 2013), which lays at nearly the same position but at 956 m water depth, i.e. both cores bound the main tongue of AAIW today. The results of GeoB15016 had shown increase presence of the AAIW at the site, but it was not possible to relate unequivocally this increased presence to a deepening of the core of the AAIW or to an increase in production. Results from GeoB15020 will allow answering that dichotomy. In addition, actual changes in the intrinsic characteristics of the AAIW are poorly constrained. Therefore, we will additionally present high resolution (multi-decadal time scales) δ18O, δ13C and Sortable Silt records from

  5. Influence of Antarctic Intermediate Water on the deoxygenation of the Atlantic Ocean

    NASA Astrophysics Data System (ADS)

    Santos, Guilherme Cordova; Kerr, Rodrigo; Azevedo, José Luiz Lima; Mendes, Carlos Rafael Borges; da Cunha, Letícia Cotrim

    2016-12-01

    Hydrographic trends in the Antarctic Intermediate Water (AAIW) layer that may be associated with changes in the thickness and oxygen content of oxygen minimum zones (OMZs) in the eastern tropical South Atlantic (ETSA) and eastern tropical North Atlantic (ETNA) are investigated by using historical data (1960 to 2015). Our results reveal that the thickness of these OMZs has continually increased (2.58 ± 0.67 m yr-1 for the ETSA and 3.37 ± 0.73 m yr-1 for the ETNA), the mean oxygen concentration has decreased (- 0.12 ± 0.03 μmol kg-1 yr-1 for the ETSA and - 0.17 ± 0.05 μmol kg-1 yr-1 for the ETNA), and the mean temperature has increased. The optimum multiparameter analysis method is used to track modifications in the AAIW along its path through the South Atlantic Subtropical Gyre. We observe an AAIW layer vertical expansion rate of 1.67 ± 0.71 m yr-1, a decrease in the mean oxygen concentration of - 0.18 ± 0.04 μmol kg-1 yr-1 and an increase in the mean temperature of 0.010 ± 0.005 °C yr-1. Moreover, a similar decrease in oxygen concentrations is observed in the AAIW layer of the studied OMZ regions compared to those in the non-AAIW portions of these OMZs, which indicates strong deoxygenation in this water mass over time. Our results suggest that warming in the AAIW source region and in its extensive temporal displacement through the SASG to the eastern tropical Atlantic Ocean appreciably shifted this water mass toward lower densities with depleted oxygen (increases in ventilation age and oxygen consumption). The warming trend that is reported here suggests that global warming is one of the factors that influence oxygen solubility changes during the deoxygenation and expansion of OMZs.

  6. Asymmetric Signature of Glacial Antarctic Intermediate Water in the Central South Pacific

    NASA Astrophysics Data System (ADS)

    Tapia, R.; Nuernberg, D.; Ho, S. L.; Lamy, F.; Ullermann, J.; Gersonde, R.; Tiedemann, R.

    2017-12-01

    Southern Ocean Intermediate Waters (SOIWs) play a key role in modulating the global climate on glacial-interglacial time scales as they connect the Southern Ocean and the tropics. Despite their importance, the past evolution of the SOIWs in the central South Pacific is largely unknown due to a dearth of sedimentary archives. Here we compare Mg/Ca-temperature, stable carbon and oxygen isotope records from surface-dwelling (G. bulloides) and deep-dwelling (G. inflata) planktic foraminifera at site PS75/059-2 (54°12.9' S, 125°25.53' W; recovery 13.98 m; 3.613 m water depth), located north of the modern Subantarctic Front. Our study focuses on the temperature and salinity variability controlled by SOIWs, which were subducted at the Subantarctic Front during the Last Glacial Maximum (LGM; 29-17ka BP) and the Penultimate Glacial Maximum (PGM; 180-150ka BP). During both glacial periods conditions at the subsurface ocean were colder and fresher relative to the Holocene (<10ka) suggesting an enhanced presence of SOIWs. In spite of the comparable subsurface cooling during both glacial, the subsurface ocean during the PGM was saltier and 0.35‰ more depleted in δ13C in comparison to the LGM. Interestingly, the mean δ13C value of the PGM is comparable to the Carbon Isotope Minimum Events, which might suggests a larger contribution of "old" low δ13C deep waters to the study site during the PGM. A Latitudinal comparison of subsurface proxies suggests glacial asymmetries in the advection of SOIWs into the central Pacific, plausibly related to glacial changes in the convection depth of SOIWs at the South Antarctic Front area rather than changes in production of the SOIWs.

  7. Antarctic climate, Southern Ocean circulation patterns, and deep water formation during the Eocene

    NASA Astrophysics Data System (ADS)

    Huck, Claire E.; van de Flierdt, Tina; Bohaty, Steven M.; Hammond, Samantha J.

    2017-07-01

    We assess early-to-middle Eocene seawater neodymium (Nd) isotope records from seven Southern Ocean deep-sea drill sites to evaluate the role of Southern Ocean 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 Ocean pelagic sites (Ocean Drilling Program (ODP) Sites 738 and 757 and Deep Sea Drilling Project (DSDP) Site 264), indicate a dominant Southern Ocean-sourced contribution to regional deep waters (ɛNd(t) = -9.3 ± 1.5). IODP Site U1356 off the coast of Adélie Land, a locus of modern-day Antarctic Bottom Water production, is identified as a site of persistent deep water formation from the early Eocene to the Oligocene. East of the Tasman Gateway an additional local source of intermediate/deep water formation is inferred at ODP Site 277 in the SW Pacific Ocean (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 waters, highlighting the complexity and importance of Southern Ocean circulation in the greenhouse climate of the Eocene.

  8. Freshening of Antarctic Intermediate Water in the South Atlantic Ocean in 2005-2014

    NASA Astrophysics Data System (ADS)

    Yao, Wenjun; Shi, Jiuxin; Zhao, Xiaolong

    2017-07-01

    Basin-scale freshening of Antarctic Intermediate Water (AAIW) is reported to have occurred in the South Atlantic Ocean 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 Ocean Circulation Experiment Hydrographic Program. Freshening of the AAIW was compensated for by a salinity increase of thermocline water, 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 ocean 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 Ocean 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.

  9. Lagrangian water mass tracing from pseudo-Argo, model-derived salinity, tracer and velocity data: An application to Antarctic Intermediate Water in the South Atlantic Ocean

    NASA Astrophysics Data System (ADS)

    Blanke, Bruno; Speich, Sabrina; Rusciano, Emanuela

    2015-01-01

    We use the tracer and velocity fields of a climatological ocean model to investigate the ability of Argo-like data to estimate accurately water mass movements and transformations, in the style of analyses commonly applied to the output of ocean 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 Water in the South Atlantic Ocean 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 waters 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 ocean interior.

  10. Variability of nutrients and carbon dioxide in the Antarctic Intermediate Water between 1990 and 2014

    NASA Astrophysics Data System (ADS)

    Panassa, Essowè; Santana-Casiano, J. Magdalena; González-Dávila, Melchor; Hoppema, Mario; van Heuven, Steven M. A. C.; Völker, Christoph; Wolf-Gladrow, Dieter; Hauck, Judith

    2018-03-01

    Antarctic Intermediate Water (AAIW) formation constitutes an important mechanism for the export of macronutrients out of the Southern Ocean that fuels primary production in low latitudes. We used quality-controlled gridded data from five hydrographic cruises between 1990 and 2014 to examine decadal variability in nutrients and dissolved inorganic carbon (DIC) in the AAIW (neutral density range 27 < γ n < 27.4) along the Prime Meridian. Significant positive trends were found in DIC (0.70 ± 0.4 μmol kg- 1 year- 1) and nitrate (0.08 ± 0.06 μ mol kg- 1 year- 1) along with decreasing trends in temperature (- 0.015 ± 0.01∘C year- 1) and salinity (- 0.003 ± 0.002 year- 1) in the AAIW. Accompanying this is an increase in apparent oxygen utilization (AOU, 0.16 ± 0.07 μ mol kg- 1 year- 1). We estimated that 75% of the DIC change has an anthropogenic origin. The remainder of the trends support a scenario of a strengthening of the upper-ocean overturning circulation in the Atlantic sector of the Southern Ocean in response to the positive trend in the Southern Annular Mode. A decrease in net primary productivity (more nutrients unutilized) in the source waters of the AAIW could have contributed as well but cannot fully explain all observed changes.

  11. Comparison of Subantarctic Mode Water and Antarctic Intermediate Water formation rates in the South Pacific between NCAR-CCSM4 and observations

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Hartin, Corinne A.; Fine, Rana A.; Kamenkovich, Igor

    2014-01-28

    Average formation rates for Subantarctic Mode (SAMW) and Antarctic Intermediate Waters (AAIW) in the South Pacific are calculated from the National Center for Atmospheric Research Community Climate System Model version 4 (NCAR-CCSM4), using chlorofluorocarbon inventories. CFC-12 inventories and formation rates are compared to ocean observations. CCSM4 accurately simulates the southeast Pacific as the main formation region for SAMW and AAIW. CCSM4 formation rates for SAMW are 3.4 Sv, about half of the observational rate. Shallow mixed layers and a thinner SAMW in CCSM4 are responsible for lower formation rates. A formation rate of 8.1 Sv for AAIW in CCSM4 ismore » higher than observations. Higher inventories in CCSM4 in the southwest and central Pacific, and higher surface concentrations are the main reasons for higher formation rates of AAIW. This comparison of model and observations is useful for understanding the uptake and transport of other gases, e.g., CO2 by the model.« less

  12. Reconstruction of deglacial Antarctic Intermediate Water variations in the subtropical North Atlantic

    NASA Astrophysics Data System (ADS)

    Xie, R. C.; Marcantonio, F.; Schmidt, M. W.

    2012-12-01

    Understanding intermediate water circulation across the last deglaciation is critical in assessing the role of oceanic heat transport associated with Atlantic Meridional Overturning Circulation (AMOC) variability across abrupt climate events. Abrupt changes in the northward flow of Antarctic Intermediate Water (AAIW) associated with AMOC reduction during the Younger Dryas (YD) and Heinrich Event 1 (H1) have been hypothesized, suggesting a potential connection between the Southern Ocean and high-latitude North Atlantic climate change. However, controversy persists as to whether the northward flow of AAIW is stronger or weaker during these abrupt cold events. One school maintains that there is an increase in the northward penetration of AAIW associated with weaker AMOC during both the YD and H1 cold events (e.g., [1-2]). However, each of these previous studies analyzed sediment cores retrieved from depths deeper than the modern depth range of AAIW (500-1100 m in the tropical and subtropical North Atlantic). Another school comes to the opposite conclusion, namely that there is a weakening of AAIW at least during one of the deglacial events (e.g., [3-4]). Here, we reconstruct deglacial AAIW variations using authigenic Nd isotope ratios from sediment recovered from core VM12-107 (11.33°N, 66.63°W; 1079 m) in the Southern Caribbean Sea. VM12-107 lies at the boundary between modern AAIW and modern upper NADW and thus is ideal for investigating the shoaling/deepening of the competing water masses as well as the variations of AAIW across abrupt climate events during the last deglaciation. We measured authigenic Nd isotope compositions in three different fractions in core VM12-107: the Fe-Mn oxyhydroxide leachate of the bulk sediment, the uncleaned planktonic foraminifera (mixed species), and fish debris wherever possible. Preliminary authigenic Nd isotope results from the Fe-Mn leachate show little variability in the ɛNd values, ranging from -9.6 to -10.6, during the

  13. Multidecadal warming of Antarctic waters.

    PubMed

    Schmidtko, Sunke; Heywood, Karen J; Thompson, Andrew F; Aoki, Shigeru

    2014-12-05

    Decadal trends in the properties of seawater adjacent to Antarctica are poorly known, and the mechanisms responsible for such changes are uncertain. Antarctic ice sheet mass loss is largely driven by ice shelf basal melt, which is influenced by ocean-ice interactions and has been correlated with Antarctic Continental Shelf Bottom Water (ASBW) temperature. We document the spatial distribution of long-term large-scale trends in temperature, salinity, and core depth over the Antarctic continental shelf and slope. Warming at the seabed in the Bellingshausen and Amundsen seas is linked to increased heat content and to a shoaling of the mid-depth temperature maximum over the continental slope, allowing warmer, saltier water greater access to the shelf in recent years. Regions of ASBW warming are those exhibiting increased ice shelf melt. Copyright © 2014, American Association for the Advancement of Science.

  14. Water soluble dicarboxylic acids and related compounds in Antarctic aerosols

    NASA Astrophysics Data System (ADS)

    Kawamura, Kimitaka; SeméRé, Richard; Imai, Yoshie; Fujii, Yoshiyuki; Hayashi, Masahiko

    1996-08-01

    Antarctic aerosols collected at Syowa Station were studied for water soluble organic compounds by employing a water extraction and dibutyl ester derivatization and using a capillary gas chromatography (GC) and GC/mass spectrometry (GC/MS). Total carbon and nitrogen were also determined. A homologous series of α,ω-dicarboxylic acids (C2-C11), ω-oxocarboxylic acids (C2-C9), and α-dicarbonyls (C2-C3) were detected, as well as pyruvic acid and aromatic (phthalic) diacid. Succinic (C4) or oxalic (C2) acid was found to be the dominant diacid species, followed by azelaic (C9), adipic (C6), or malonic (C3) acid. Concentration range of the total diacids was 5.9-88 ng m-3, with an average of 29 ng m-3. Highest concentrations were observed in the summer sample with a predominance of succinic acid (61.5 ng m-3), which comprised approximately 70% of the total diacids and accounted for 3.5% of total aerosol carbon (1020 ng m-3). The succinic acid (C4) is likely produced by photooxidation of 4-oxocarboxylic acids, which are present in the atmosphere as intermediates of the photooxidation of unsaturated fatty acids. These results indicate that the Antarctic organic aerosols originate from marine-derived lipids and are transformed largely by photochemical oxidations. ω-Oxocarboxylic acids (C2-C9, 0.36-3.0 ng m-3) also showed the highest concentration in the summer sample, again suggesting a secondary production in the atmosphere of the Antarctic and in the Southern Ocean.

  15. Assessing fuel spill risks in polar waters: Temporal dynamics and behaviour of hydrocarbons from Antarctic diesel, marine gas oil and residual fuel oil.

    PubMed

    Brown, Kathryn E; King, Catherine K; Kotzakoulakis, Konstantinos; George, Simon C; Harrison, Peter L

    2016-09-15

    As part of risk assessment of fuel oil spills in Antarctic and subantarctic waters, this study describes partitioning of hydrocarbons from three fuels (Special Antarctic Blend diesel, SAB; marine gas oil, MGO; and intermediate grade fuel oil, IFO 180) into seawater at 0 and 5°C and subsequent depletion over 7days. Initial total hydrocarbon content (THC) of water accommodated fraction (WAF) in seawater was highest for SAB. Rates of THC loss and proportions in equivalent carbon number fractions differed between fuels and over time. THC was most persistent in IFO 180 WAFs and most rapidly depleted in MGO WAF, with depletion for SAB WAF strongly affected by temperature. Concentration and composition remained proportionate in dilution series over time. This study significantly enhances our understanding of fuel behaviour in Antarctic and subantarctic waters, enabling improved predictions for estimates of sensitivities of marine organisms to toxic contaminants from fuels in the region. Copyright © 2016 Elsevier Ltd. All rights reserved.

  16. Localized Rapid Warming of West Antarctic Subsurface Waters by Remote Winds

    NASA Astrophysics Data System (ADS)

    Griffies, S. M.; Spence, P.; Holmes, R.; Hogg, A. M.; Stewart, K. D.; England, M. H.

    2017-12-01

    The largest rates of Antarctic glacial ice mass loss are occurring tothe west of the Antarctica Peninsula in regions where warming ofsubsurface continental shelf waters is also largest. However, thephysical mechanisms responsible for this warming remain unknown. Herewe show how localized changes in coastal winds off East Antarctica canproduce significant subsurface temperature anomalies (>2C) around theentire continent. We demonstrate how coastal-trapped Kelvin wavescommunicate the wind disturbance around the Antarctic coastline. Thewarming is focused on the western flank of the Antarctic Peninsulabecause the anomalous circulation induced by the coastal-trapped wavesis intensified by the steep continental slope there, and because ofthe presence of pre-existing warm subsurface water. Thecoastal-trapped waves leads to an adjustment of the flow that shoalsisotherms and brings warm deep water upwards onto the continentalshelf and closer to the coast. This result demonstrates the uniquevulnerability of the West Antarctic region to a changing climate.

  17. Intense Mixing and Recirculations of Intermediate and Deep Water in the Northwest Argentine Basin

    NASA Astrophysics Data System (ADS)

    Valla, D.; Piola, A. R.

    2016-02-01

    The sources of the South Atlantic upper and intermediate waters that form the upper layer flow needed to maintain mass balance due the export of North Atlantic Deep Water from the North Atlantic are still under debate. The "cold path" scheme postulates that intermediate waters are injected into the South Atlantic from the Pacific through the Drake Passage, advected north by the Malvinas Current up to the Brazil/Malvinas Confluence (BMC) and circulated around the basin following the path of the subtropical gyre. We report high-quality hydrographic observations collected in the South Atlantic western boundary at 34.5 °S during 7 hydrographic cruises as part of the SAMOC project. We focus on the flow and characteristics of Antarctic Intermediate Water (AAIW) and Upper Circumpolar Deep Water (UCDW). The water mass analysis indicates the presence of "young" (fresh and highly oxygenated) varieties of AAIW (S<34.2, O2>6 ml·l-1) which must be derived from south of the SAMOC array. This suggests an alternative pathway for intermediate waters that involves a short circuit beneath the BMC. Simultaneous full-depth velocity measurements using lowered acoustic Doppler current profilers confirm this hypothesis. The flow direction across the SAMOC array in the UCDW range inferred from dissolved oxygen measurements also indicate the presence of UCDW (O2<4.2 ml·l-1) derived from farther south. However, the wider range of oxygen concentrations suggests strong recirculations of both water masses within the northwestern Argentine Basin.

  18. Localized rapid warming of West Antarctic subsurface waters by remote winds

    NASA Astrophysics Data System (ADS)

    Spence, Paul; Holmes, Ryan M.; Hogg, Andrew Mcc.; Griffies, Stephen M.; Stewart, Kial D.; England, Matthew H.

    2017-08-01

    The highest rates of Antarctic glacial ice mass loss are occurring to the west of the Antarctica Peninsula in regions where warming of subsurface continental shelf waters is also largest. However, the physical mechanisms responsible for this warming remain unknown. Here we show how localized changes in coastal winds off East Antarctica can produce significant subsurface temperature anomalies (>2 °C) around much of the continent. We demonstrate how coastal-trapped barotropic Kelvin waves communicate the wind disturbance around the Antarctic coastline. The warming is focused on the western flank of the Antarctic Peninsula because the circulation induced by the coastal-trapped waves is intensified by the steep continental slope there, and because of the presence of pre-existing warm subsurface water offshore. The adjustment to the coastal-trapped waves shoals the subsurface isotherms and brings warm deep water upwards onto the continental shelf and closer to the coast. This result demonstrates the vulnerability of the West Antarctic region to a changing climate.

  19. Abrupt changes in Antarctic Intermediate Water strength lead Atlantic Meridional Overturning Circulation changes during the last deglacial

    NASA Astrophysics Data System (ADS)

    Xie, R.; Marcantonio, F.; Schmidt, M. W.

    2011-12-01

    Reorganization of meridional overturning circulation that is a response to or a trigger of climate change in the North Atlantic has been a subject of intense interest. During the last deglaciation, cold periods such as the Younger Dryas (YD) and Heinrich 1 (H1) are thought to be coincident with significant reductions in North Atlantic Deep Water (NADW) formation. Yet, the role that Antarctic Intermediate Water (AAIW) played during these cold events is still poorly constrained. Benthic Cd/Ca data from sediment cores in the Florida Straits suggest a reduced contribution of AAIW in the North Atlantic western boundary current during the YD [1]. However, ɛNd evidence in sediment cores from Tobago basin suggests a greater influence of AAIW in the North Atlantic during YD and H1 [2]. In this study, we measure ɛNd values in the authigenic Fe-Mn oxyhydroxide fraction of sediment from three cores, KNR166-2-26JPC (24°19.62'N, 83°15.14'W; 546 m) and KNR166-2-31JPC (24°13.18'N, 83°17.75'W; 751 m) within the Florida Straits, and VM12-107 (11.33°N, 66.63°W; 1079 m) in the Southern Carribean Sea. All three cores lie within the path of AAIW and are, therefore, useful to gauge the waxing and waning of AAIW during the last deglaciation. Cores 26JPC and 31JPC are located within the Florida Current, which under modern conditions represents a mixture of recirculated North Atlantic subtropical gyre water and Southern origin waters. Our preliminary results from 26JPC and 31JPC show significantly less radiogenic ɛNd values during the YD and H1 than during the Holocene (~1 epsilon unit for 26JPC and ~0.6 epsilon units for 31JPC during both periods). We interpret the lower ɛNd during the YD and H1 as signifying a decreased input of Southern-sourced waters (i.e., AAIW) arriving at these sites, in agreement with the study of Came et al.[1], but not that of Pahnke et al. in the Tobago Basin [2]. We suggest that ɛNd values in the latter study, in which the core site location is at a

  20. Abrupt changes of intermediate-water oxygen in the northwestern Pacific during the last 27 kyr

    NASA Astrophysics Data System (ADS)

    Ishizaki, Yui; Ohkushi, Ken'ichi; Ito, Takashi; Kawahata, Hodaka

    2009-04-01

    An oxygen minimum zone (OMZ) currently exists at intermediate water depths on the northern Japanese margin in the northwestern Pacific. The OMZ results largely from a combination of high surface-water productivity and poor ventilation of intermediate waters. We investigated the late Quaternary history (last 27 kyr) of the intensity of this OMZ using changes in benthic foraminiferal carbon isotopes and assemblages in a sediment core taken on the continental slope off Shimokita Peninsula, northern Japan, at a water depth of 975 m. The core was located well within the region of the present-day OMZ and high surface-water productivity. The benthic foraminiferal δ13C values, which indicate millennial-scale fluctuations of nutrient contents at the sediment-water interface, were 0.48‰ lower during the last glacial maximum (LGM) than during the late Holocene. These results do not indicate the formation of glacial intermediate waters of subarctic Pacific origin, but rather the large contribution of high-nutrient water masses such as the Antarctic Intermediate Water, implying that the regional circulation pattern during the LGM was similar to that of modern times. Benthic foraminiferal assemblages underwent major changes in response to changes in dissolved oxygen concentrations in ocean floor sediments. The lowest oxygen and highest nutrient conditions, marked by dysoxic taxa and negative values of benthic foraminiferal δ13C, occurred during the Bølling/Allerød (B/A) and Pre-Boreal warming events. Dysoxic conditions in this region during these intervals were possibly caused by high surface-water productivity at times of reduced intermediate-water ventilation in the northwestern Pacific. The benthic assemblages show dysoxic events on approx. 100- to 200-year cycles during the B/A, reflecting centennial-scale productivity changes related to freshwater cycles and surface-water circulation in the North Pacific.

  1. Coherent response of Antarctic Intermediate Water and Atlantic Meridional Overturning Circulation during the last deglaciation: reconciling contrasting neodymium isotope reconstructions in tropical Atlantic

    NASA Astrophysics Data System (ADS)

    Gu, S.; Liu, Z.; Zhang, J.; Rempfer, J.; Joos, F.; Oppo, D.

    2017-12-01

    Antarctic Intermediate Water (AAIW) plays important roles in the global climate system and the global ocean nutrient and carbon cycles. However, it is unclear how AAIW responds to global climate changes. In particular, neodymium isotopic composition (ɛNd) reconstructions from different locations in tropical Atlantic, have led to a debate on the relationship between the northward penetration of AAIW into the tropical Atlantic and Atlantic Meridional Overturning Circulation (AMOC) variability during the last deglaciation. We resolve this controversy by studying the transient oceanic evolution during the last deglaciation using a neodymium-enabled ocean model. Our results suggest a coherent response of AAIW and AMOC: when AMOC weakens, the northward penetration and transport of AAIW decreases while its depth and thickness increase. Our study highlights that as part of the return flow of the North Atlantic Deep Water (NADW), the northward penetration of AAIW in Atlantic is determined predominately by AMOC intensity. Moreover, the inconsistency among different tropical Atlantic ɛNd reconstructions is reconciled by considering their corresponding core locations and depths, which were influenced by different water masses and ocean currents in the past. The very radiogenic water from the bottom of the Gulf of Mexico and Caribbean Sea, which was previously overlooked in interpretations of deglacial ɛNd variability, can be transported to shallow layers during active AMOC, and modulates ɛNd in the tropical Atlantic. Changes in the AAIW core depth must also be considered. Thus, interpretation of ɛNd reconstructions from the tropical Atlantic is more complicated than suggested in previous studies. ­­

  2. Fuel oil and dispersant toxicity to the Antarctic sea urchin (Sterechinus neumayeri).

    PubMed

    Alexander, Frances J; King, Catherine K; Reichelt-Brushett, Amanda J; Harrison, Peter L

    2017-06-01

    The risk of a major marine fuel spill in Antarctic waters is increasing, yet there are currently no standard or suitable response methods under extreme Antarctic conditions. Fuel dispersants may present a possible solution; however, little data exist on the toxicity of dispersants or fuels to Antarctic species, thereby preventing informed management decisions. Larval development toxicity tests using 3 life history stages of the Antarctic sea urchin (Sterechinus neumayeri) were completed to assess the toxicity of physically dispersed, chemically dispersed, and dispersant-only water-accommodated fractions (WAFs) of an intermediate fuel oil (IFO 180, BP) and the chemical dispersant Slickgone NS (Dasic International). Despite much lower total petroleum hydrocarbon concentrations, physically dispersed fuels contained higher proportions of low-to-intermediate weight carbon compounds and were generally at least an order of magnitude more toxic than chemically dispersed fuels. Based on concentrations that caused 50% abnormality (EC50) values, the embryonic unhatched blastula life stage was the least affected by fuels and dispersants, whereas the larval 4-armed pluteus stage was the most sensitive. The present study is the first to investigate the possible implications of the use of fuel dispersants for fuel spill response in Antarctica. The results indicate that the use of a fuel dispersant did not increase the hydrocarbon toxicity of IFO 180 to the early life stages of Antarctic sea urchins, relative to physical dispersal. Environ Toxicol Chem 2017;36:1563-1571. © 2016 SETAC. © 2016 SETAC.

  3. Intermediate and deep water mass distribution in the Pacific during the Last Glacial Maximum inferred from oxygen and carbon stable isotopes

    NASA Astrophysics Data System (ADS)

    Herguera, J. C.; Herbert, T.; Kashgarian, M.; Charles, C.

    2010-05-01

    Intermediate ocean circulation changes during the last Glacial Maximum (LGM) in the North Pacific have been linked with Northern Hemisphere climate through air-sea interactions, although the extent and the source of the variability of the processes forcing these changes are still not well resolved. The ventilated volumes and ages in the upper wind driven layer are related to the wind stress curl and surface buoyancy fluxes at mid to high latitudes in the North Pacific. In contrast, the deeper thermohaline layers are more effectively ventilated by direct atmosphere-sea exchange during convective formation of Subantarctic Mode Waters (SAMW) and Antarctic Intermediate Waters (AAIW) in the Southern Ocean, the precursors of Pacific Intermediate Waters (PIW) in the North Pacific. Results reported here show a fundamental change in the carbon isotopic gradient between intermediate and deep waters during the LGM in the eastern North Pacific indicating a deepening of nutrient and carbon rich waters. These observations suggest changes in the source and nature of intermediate waters of Southern Ocean origin that feed PIW and enhanced ventilation processes in the North Pacific, further affecting paleoproductivity and export patters in this basin. Furthermore, oxygen isotopic results indicate these changes may have been accomplished in part by changes in circulation affecting the intermediate depths during the LGM.

  4. Reconstruction of intermediate water circulation in the tropical North Atlantic during the past 22,000 years

    NASA Astrophysics Data System (ADS)

    Xie, Ruifang C.; Marcantonio, Franco; Schmidt, Matthew W.

    2014-09-01

    Decades of paleoceanographic studies have reconstructed a well-resolved water mass structure for the deep Atlantic Ocean during the Last Glacial Maximum (LGM). However, the variability of intermediate water circulation in the tropics over the LGM and deglacial abrupt climate events is still largely debated. This study aims to reconstruct intermediate northern- and southern-sourced water circulation in the tropical North Atlantic during the past 22 kyr and attempts to confine the boundary between Antarctic Intermediate Water (AAIW) and northern-sourced intermediate water (i.e., upper North Atlantic Deep Water (NADW) or Glacial North Atlantic Intermediate Water) in the past. High-resolution Nd isotopic compositions of fish debris and acid-reductive leachate of bulk sediment in core VM12-107 (1079 m depth) from the Southern Caribbean are not in agreement. We suggest that the leachate method does not reliably extract the Nd isotopic compositions of seawater at this location, and that it needs to be tested in more detail in various oceanic settings. The fish debris εNd values display a general decrease from the early deglaciation to the end of the Younger Dryas, followed by a greater drop toward less radiogenic values into the early Holocene. We propose a potentially more radiogenic glacial northern endmember water mass and interpret this pattern as recording a recovery of the upper NADW during the last deglaciation. Comparing our new fish debris Nd isotope data to authigenic Nd isotope studies in the Florida Straits (546 and 751 m depth), we propose that both glacial and deglacial AAIW do not penetrate beyond the lower depth limit of modern AAIW in the tropical Atlantic.

  5. Water masses, ocean fronts, and the structure of Antarctic seabird communities: putting the eastern Bellingshausen Sea in perspective

    USGS Publications Warehouse

    Ribic, Christine A.; Ainley, David G.; Ford, R. Glenn; Fraser, William R.; Tynan, Cynthia T.; Woehler, Eric J.

    2015-01-01

    Waters off the western Antarctic Peninsula (i.e., the eastern Bellingshausen Sea) are unusually complex owing to the convergence of several major fronts. Determining the relative influence of fronts on occurrence patterns of top-trophic species in that area, therefore, has been challenging. In one of the few ocean-wide seabird data syntheses, in this case for the Southern Ocean, we analyzed ample, previously collected cruise data, Antarctic-wide, to determine seabird species assemblages and quantitative relationships to fronts as a way to provide context to the long-term Palmer LTER and the winter Southern Ocean GLOBEC studies in the eastern Bellingshausen Sea. Fronts investigated during both winter (April–September) and summer (October–March) were the southern boundary of the Antarctic Circumpolar Current (ACC), which separates the High Antarctic from the Low Antarctic water mass, and within which are embedded the marginal ice zone and Antarctic Shelf Break Front; and the Antarctic Polar Front, which separates the Low Antarctic and the Subantarctic water masses. We used clustering to determine species' groupings with water masses, and generalized additive models to relate species' densities, biomass and diversity to distance to respective fronts. Antarctic-wide, in both periods, highest seabird densities and lowest species diversity were found in the High Antarctic water mass. In the eastern Bellingshausen, seabird density in the High Antarctic water mass was lower (as low as half that of winter) than found in other Antarctic regions. During winter, Antarctic-wide, two significant species groups were evident: one dominated by Adélie penguins (Pygoscelis adeliae) (High Antarctic water mass) and the other by petrels and prions (no differentiation among water masses); in eastern Bellingshausen waters during winter, the one significant species group was composed of species from both Antarctic-wide groups. In summer, Antarctic-wide, a High Antarctic group

  6. Structure of the shelf and slope waters of the Antarctic Seas

    NASA Astrophysics Data System (ADS)

    Artamonova, Ksenia; Antipov, Nikolay; Gangnus, Ivan; Maslennikov, Vyacheslav

    2015-04-01

    The main objective of present work is to consider characteristics of shelf and slope waters in the Commonwealth, Ross, Amundson and Bellingshausen Seas. Data of Russian surveys led during the Antarctic summer of 2006 - 2014 on RV "Academic Fedorov"and "Academic Treshnikov"was analyzed. Distribution of temperature, salinity, dissolved oxygen, silicate, phosphates and nitrates in the water masses of the Commonwealth and Amundsen seas was shown. Significant differences in the structures of the shelf and slope waters of the seas were observed. A water structure at the oceanological sections of the Commonwealth Sea was constituted by the Antarctic Surface Water (AASW) with enough high concentration of silicate, nitrate nitrogen and phosphates compare with other areas of the World Ocean; the Upper Circumpolar Deep Water (UCDW) characterized by a minimum of the oxygen content, and a maximum of nutrient concentrations; The Lower Circumpolar Deep Water (LCDW) primary characterized by a salinity maximum and a minimum of nutritive salts as well; and the Antarctic Bottom water (AABW). It was shown that the local cold, salt and dense Antarctic Shelf water (ASW) formed in the shelf area of the Commonwealth Sea. The characteristics of ASW were defined. The ASW mixed with the CDW and their mixture (The Bottom Water of the Prydz Bay (BWPB)) moved down along the slope, and reached the bottom.The characteristics of the BWPB were analyzed. The BWPB was defined by higher content of dissolved oxygen (more 5.5 ml/l) and lower contents of biogenic elements (silicon - low 120 µМ, phosphates - low 2.35 µМ and nitrates - low 29 µМ) in the bottom layer at the slope compared with the Circumpolar Deep Water (CDW) characteristics. Interannual variability of characteristics of the water masses was observed on the repeated oceanological section along 70° E in the Commonwealth Sea. It was shown that characteristics and structure of the BWPB undergo appreciable changes year by year. The

  7. 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.

  8. 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.

  9. Observations of a diapycnal shortcut to adiabatic upwelling of Antarctic Circumpolar Deep Water

    NASA Astrophysics Data System (ADS)

    Silvester, J. Mead; Lenn, Yueng-Djern; Polton, Jeff A.; Rippeth, Tom P.; Maqueda, M. Morales

    2014-11-01

    In the Southern Ocean, small-scale turbulence causes diapycnal mixing which influences important water mass transformations, in turn impacting large-scale ocean transports such as the Meridional Overturning Circulation (MOC), a key controller of Earth's climate. We present direct observations of mixing over the Antarctic continental slope between water masses that are part of the Southern Ocean MOC. A 12 h time series of microstructure turbulence measurements, hydrography, and velocity observations off Elephant Island, north of the Antarctic Peninsula, reveals two concurrent bursts of elevated dissipation of O(10-6) W kg-1, resulting in heat fluxes ˜10 times higher than basin-integrated Drake Passage estimates. This occurs across the boundary between adjacent adiabatic upwelling and downwelling overturning cells. Ray tracing to nearby topography shows mixing between 300 and 400 m is consistent with the breaking of locally generated internal tidal waves. Since similar conditions extend to much of the Antarctic continental slope where these water masses outcrop, diapycnal mixing may contribute significantly to upwelling.

  10. Freshening by glacial meltwater enhances melting of ice shelves and reduces formation of Antarctic Bottom Water

    PubMed Central

    van Wijk, Esmee

    2018-01-01

    Strong heat loss and brine release during sea ice formation in coastal polynyas act to cool and salinify waters on the Antarctic continental shelf. Polynya activity thus both limits the ocean heat flux to the Antarctic Ice Sheet and promotes formation of Dense Shelf Water (DSW), the precursor to Antarctic Bottom Water. However, despite the presence of strong polynyas, DSW is not formed on the Sabrina Coast in East Antarctica and in the Amundsen Sea in West Antarctica. Using a simple ocean model driven by observed forcing, we show that freshwater input from basal melt of ice shelves partially offsets the salt flux by sea ice formation in polynyas found in both regions, preventing full-depth convection and formation of DSW. In the absence of deep convection, warm water that reaches the continental shelf in the bottom layer does not lose much heat to the atmosphere and is thus available to drive the rapid basal melt observed at the Totten Ice Shelf on the Sabrina Coast and at the Dotson and Getz ice shelves in the Amundsen Sea. Our results suggest that increased glacial meltwater input in a warming climate will both reduce Antarctic Bottom Water formation and trigger increased mass loss from the Antarctic Ice Sheet, with consequences for the global overturning circulation and sea level rise. PMID:29675467

  11. Freshening by glacial meltwater enhances melting of ice shelves and reduces formation of Antarctic Bottom Water.

    PubMed

    Silvano, Alessandro; Rintoul, Stephen Rich; Peña-Molino, Beatriz; Hobbs, William Richard; van Wijk, Esmee; Aoki, Shigeru; Tamura, Takeshi; Williams, Guy Darvall

    2018-04-01

    Strong heat loss and brine release during sea ice formation in coastal polynyas act to cool and salinify waters on the Antarctic continental shelf. Polynya activity thus both limits the ocean heat flux to the Antarctic Ice Sheet and promotes formation of Dense Shelf Water (DSW), the precursor to Antarctic Bottom Water. However, despite the presence of strong polynyas, DSW is not formed on the Sabrina Coast in East Antarctica and in the Amundsen Sea in West Antarctica. Using a simple ocean model driven by observed forcing, we show that freshwater input from basal melt of ice shelves partially offsets the salt flux by sea ice formation in polynyas found in both regions, preventing full-depth convection and formation of DSW. In the absence of deep convection, warm water that reaches the continental shelf in the bottom layer does not lose much heat to the atmosphere and is thus available to drive the rapid basal melt observed at the Totten Ice Shelf on the Sabrina Coast and at the Dotson and Getz ice shelves in the Amundsen Sea. Our results suggest that increased glacial meltwater input in a warming climate will both reduce Antarctic Bottom Water formation and trigger increased mass loss from the Antarctic Ice Sheet, with consequences for the global overturning circulation and sea level rise.

  12. Antarctic ice discharge due to warm water intrusion into shelf cavities

    NASA Astrophysics Data System (ADS)

    Winkelmann, R.; Reese, R.; Albrecht, T.; Mengel, M.; Asay-Davis, X.

    2017-12-01

    Ocean-induced melting below ice shelves is the dominant driver for mass loss from the Antarctic Ice Sheet at present. Observations show that many Antarctic ice shelves are thinning which reduces their buttressing potential and can lead to increased ice discharge from the glaciers upstream. Melt rates from Antarctic ice shelves are determined by the temperature and salinity of the ambient ocean. In many parts, ice shelves are shielded by clearly defined density fronts which keep relatively warm Northern water from entering the cavity underneath the ice shelves. Projections show that a redirection of coastal currents might allow these warmer waters to intrude into ice shelf cavities, for instance in the Weddell Sea, and thereby cause a strong increase in sub-shelf melt rates. Using the Potsdam Ice-shelf Cavity mOdel (PICO), we assess how such a change would influence the dynamic ice loss from Antarctica. PICO is implemented as part of the Parallel Ice Sheet Model (PISM) and mimics the vertical overturning circulation in ice-shelf cavities. The model is capable of capturing the wide range of melt rates currently observed for Antarctic ice shelves and reproduces the typical pattern of comparably high melting near the grounding line and lower melting or refreezing towards the calving front. Based on regional observations of ocean temperatures, we use PISM-PICO to estimate an upper limit for ice discharge resulting from the potential erosion of ocean fronts around Antarctica.

  13. 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.

  14. Water masses transform at mid-depths over the Antarctic Continental Slope

    NASA Astrophysics Data System (ADS)

    Mead Silvester, Jess; Lenn, Yueng-Djern; Polton, Jeffrey; Phillips, Helen E.; Morales Maqueda, Miguel

    2017-04-01

    The Meridional Overturning Circulation (MOC) controls the oceans' latitudinal heat distribution, helping to regulate the Earth's climate. The Southern Ocean is the primary place where cool, deep waters return to the surface to complete this global circulation. While water mass transformations intrinsic to this process predominantly take place at the surface following upwelling, recent studies implicate vertical mixing in allowing transformation at mid-depths over the Antarctic continental slope. We deployed an EM-Apex float near Elephant Island, north of the Antarctic Peninsula's tip, to profile along the slope and use potential vorticity to diagnose observed instabilities. The float captures direct heat exchange between a lens of Upper Circumpolar Deep Water (UCDW) and surrounding Lower Circumpolar Deep Waters (LCDW) at mid-depths and over the course of several days. Heat fluxes peak across the top and bottom boundaries of the UCDW lens and peak diffusivities across the bottom boundary are associated with shear instability. Estimates of diffusivity from shear-strain finestructure parameterisation and heat fluxes are found to be in reasonable agreement. The two-dimensional Ertel potential vorticity is elevated both inside the UCDW lens and along its bottom boundary, with a strong contribution from the shear term in these regions and instabilities are associated with gravitational and symmetric forcing. Thus, shear instabilities are driving turbulent mixing across the lower boundary between these two water masses, leading to the observed heat exchange and transformation at mid-depths over the Antarctic continental slope. This has implications for our understanding of the rates of upwelling and ocean-atmosphere exchanges of heat and carbon at this critical location.

  15. Intermediate water recovery system

    NASA Technical Reports Server (NTRS)

    Deckman, G.; Anderson, A. R. (Editor)

    1973-01-01

    A water recovery system for collecting, storing, and processing urine, wash water, and humidity condensates from a crew of three aboard a spacecraft is described. The results of a 30-day test performed on a breadboard system are presented. The intermediate water recovery system produced clear, sterile, water with a 96.4 percent recovery rate from the processed urine. Recommendations for improving the system are included.

  16. A comparison of ER-2 measurements of stratospheric water vapor between the 1987 Antarctic and 1989 Arctic Airborne missions

    NASA Technical Reports Server (NTRS)

    Kelly, K. K.; Tuck, A. F.; Heidt, L. E.; Loewenstein, M.; Podolske, J. R.; Strahan, S. E.; Vedder, J. F.

    1990-01-01

    Vertical profiles of water vapor inside the Antarctic vortex have been compared with those taken outside it over Punta Arenas (53 deg S, 71 deg W). A similar exercise was performed with Arctic vortex profiles and those taken over Stavanger (59 deg N, 6 deg E). Residual water, defined as the stratospheric water vapor mixing ratio with the contribution from methane oxidation subtracted, is also shown as profiles inside and outside the vortex for both missions. The Arctic and Antarctic profiles of water vapor and residual water are compared. Locally dehydrated air was evident both inside and outside the Antarctic vortex, but such dehydration was not evident in and around the Arctic vortex. Arctic profiles of residual water are consistent with nontropical entry for some air.

  17. Applicability of ERTS to Antarctic iceberg resources. [harvesting icebergs for fresh water

    NASA Technical Reports Server (NTRS)

    Hult, J. L.; Ostrander, N. C.

    1974-01-01

    This investigation explores the applicability of ERTS to: (1) determine the Antarctic sea ice and environmental behavior that may influence the harvesting of icebergs, and (2) monitor iceberg locations, characteristics, and evolution. Imagery sampling in the western Antarctic between the Peninsula and the Ross Sea is used in the analysis. It is found that the potential applicability of ERTS to the research, planning, and harvesting operations can contribute importantly to the glowing promise derived from broader scope studies for the use of Antarctic icebergs to relieve a growing global thirst for fresh water. Several years of comprehensive monitoring will be necessary to characterize sea-ice and environmental behavior and iceberg evolution. Live ERTS services will assist harvesting control and claiming operations and offer a means for harmonizing entitlements to iceberg resources.

  18. Arctic intermediate water in the Norwegian sea

    NASA Astrophysics Data System (ADS)

    Blindheim, Johan

    1990-09-01

    At least two types of intermediate water propagate into the Norwegian Sea from the Iceland and Greenland seas. North Icelandic Winter Water flows along the slope of the Faroe-Iceland Ridge towards the Faroes. The distribution of this intermediate water is limited to the southern Norwegian Sea. The second type intrudes between the bottom water and the Atlantic Water, and can be traced as a slight salinity minimum of the entire area of the Norwegian Sea. There seems to be along-isopycnal advection of this water type along the Arctic Front from both the Iceland and Greenland Seas. Although the salinity minimum is less distinct along the slope of the continental shelf than in the western Norwegian Sea, this intermediate water separates the deep water and the Atlantic Water, and prohibits direct mixing of these two water masses.

  19. West Antarctic Ice Sheet retreat driven by Holocene warm water incursions

    PubMed Central

    Hillenbrand, Claus-Dieter; Smith, James A.; Hodell, David A.; Greaves, Mervyn; Poole, Christopher R.; Kender, Sev; Williams, Mark; Andersen, Thorbjørn Joest; Jernas, Patrycja E.; Klages, Johann P.; Roberts, Stephen J.; Gohl, Karsten; Larter, Robert D.; Kuhn, Gerhard

    2017-01-01

    Glaciological and oceanographic observations coupled with numerical models show that warm Circumpolar Deep Water (CDW) upwelling onto the West Antarctic continental shelf causes melting of the undersides of floating ice shelves. Because these ice shelves buttress glaciers feeding into them, their ocean-induced thinning is driving Antarctic ice-sheet loss today. Here we present the first multi-proxy data based reconstruction of variability in CDW inflow to the Amundsen Sea sector, the most vulnerable part of the West Antarctic Ice Sheet, during the last 11,000 years. The chemical composition of foraminifer shells and benthic foraminifer assemblages in marine sediments indicate that enhanced CDW upwelling, controlled by the latitudinal position of the Southern Hemisphere westerly winds, forced deglaciation of this sector both until 7,500 years ago, when an ice-shelf collapse may have caused rapid ice-sheet thinning further upstream, and since the 1940s. These results increase confidence in the predictive capability of current ice-sheet models. PMID:28682333

  20. Shifts in coastal Antarctic marine microbial communities during and after melt water-related surface stratification.

    PubMed

    Piquet, Anouk M-T; Bolhuis, Henk; Meredith, Michael P; Buma, Anita G J

    2011-06-01

    Antarctic coastal waters undergo major physical alterations during summer. Increased temperatures induce sea-ice melting and glacial melt water input, leading to strong stratification of the upper water column. We investigated the composition of micro-eukaryotic and bacterial communities in Ryder Bay, Antarctic Peninsula, during and after summertime melt water stratification, applying community fingerprinting (denaturing gradient gel electrophoresis) and sequencing analysis of partial 18S and 16S rRNA genes. Community fingerprinting of the eukaryotic community revealed two major patterns, coinciding with a period of melt water stratification, followed by a period characterized by regular wind-induced breakdown of surface stratification. During the first stratified period, we observed depth-related differences in eukaryotic fingerprints while differences in bacterial fingerprints were weak. Wind-induced breakdown of the melt water layer caused a shift in the eukaryotic community from an Actinocyclus sp.- to a Thalassiosira sp.-dominated community. In addition, a distinct transition in the bacterial community was found, but with a few days' delay, suggesting a response to the changes in the eukaryotic community rather than to the mixing event itself. Sequence analysis revealed a shift from an Alpha- and Gammaproteobacteria to a Cytophaga-Flavobacterium-Bacteroides-dominated community under mixed conditions. Our results show that melt water stratification and the transition to nonstabilized Antarctic surface waters may have an impact not only on micro-eukaryotic but also bacterial community composition. © 2011 Federation of European Microbiological Societies. Published by Blackwell Publishing Ltd. All rights reserved.

  1. West Antarctic Ice Sheet retreat driven by Holocene warm water incursions.

    PubMed

    Hillenbrand, Claus-Dieter; Smith, James A; Hodell, David A; Greaves, Mervyn; Poole, Christopher R; Kender, Sev; Williams, Mark; Andersen, Thorbjørn Joest; Jernas, Patrycja E; Elderfield, Henry; Klages, Johann P; Roberts, Stephen J; Gohl, Karsten; Larter, Robert D; Kuhn, Gerhard

    2017-07-05

    Glaciological and oceanographic observations coupled with numerical models show that warm Circumpolar Deep Water (CDW) incursions onto the West Antarctic continental shelf cause melting of the undersides of floating ice shelves. Because these ice shelves buttress glaciers feeding into them, their ocean-induced thinning is driving Antarctic ice-sheet retreat today. Here we present a multi-proxy data based reconstruction of variability in CDW inflow to the Amundsen Sea sector, the most vulnerable part of the West Antarctic Ice Sheet, during the Holocene epoch (from 11.7 thousand years ago to the present). The chemical compositions of foraminifer shells and benthic foraminifer assemblages in marine sediments indicate that enhanced CDW upwelling, controlled by the latitudinal position of the Southern Hemisphere westerly winds, forced deglaciation of this sector from at least 10,400 years ago until 7,500 years ago-when an ice-shelf collapse may have caused rapid ice-sheet thinning further upstream-and since the 1940s. These results increase confidence in the predictive capability of current ice-sheet models.

  2. Export of nutrient rich Northern Component Water preceded early Oligocene Antarctic glaciation

    NASA Astrophysics Data System (ADS)

    Coxall, Helen K.; Huck, Claire E.; Huber, Matthew; Lear, Caroline H.; Legarda-Lisarri, Alba; O'Regan, Matt; Sliwinska, Kasia K.; van de Flierdt, Tina; de Boer, Agatha M.; Zachos, James C.; Backman, Jan

    2018-03-01

    The onset of the North Atlantic Deep Water formation is thought to have coincided with Antarctic ice-sheet growth about 34 million years ago (Ma). However, this timing is debated, in part due to questions over the geochemical signature of the ancient Northern Component Water (NCW) formed in the deep North Atlantic. Here we present detailed geochemical records from North Atlantic sediment cores located close to sites of deep-water formation. We find that prior to 36 Ma, the northwestern Atlantic was stratified, with nutrient-rich, low-salinity bottom waters. This restricted basin transitioned into a conduit for NCW that began flowing southwards approximately one million years before the initial Antarctic glaciation. The probable trigger was tectonic adjustments in subarctic seas that enabled an increased exchange across the Greenland-Scotland Ridge. The increasing surface salinity and density strengthened the production of NCW. The late Eocene deep-water mass differed in its carbon isotopic signature from modern values as a result of the leakage of fossil carbon from the Arctic Ocean. Export of this nutrient-laden water provided a transient pulse of CO2 to the Earth system, which perhaps caused short-term warming, whereas the long-term effect of enhanced NCW formation was a greater northward heat transport that cooled Antarctica.

  3. A Deep-Sea Coral Clumped Isotope Record From Southern Ocean Intermediate Water Spanning the Most Recent Glacial Termination

    NASA Astrophysics Data System (ADS)

    Hines, S.; Eiler, J. M.; Adkins, J. F.

    2015-12-01

    Movement of intermediate waters plays an important role in global heat and carbon transport in the ocean and changes in their distribution are closely tied to glacial-interglacial climate change. Ocean temperature is necessarily linked to circulation because density is a function of temperature and salinity. In the modern ocean, stratification is dominated by differences in temperature, but this may not have been the case in the past. Coupled radiocarbon and U/Th dates on deep-sea Desmophyllum dianthus corals allow for the reconstruction of past intermediate water circulation rates. The addition of temperature measurements further aids in understanding of the mechanisms driving the observed signals, since there are different boundary conditions for resetting these two properties at the surface. In the modern Southern Ocean, temperature and radiocarbon are broadly correlated. At the surface there are meridional gradients of these properties, with colder, more radiocarbon-depleted water closer to the Antarctic continent. We present a high-resolution time series of clumped isotope temperature measurements on 30 corals spanning the Last Glacial Maximum through the end of the Antarctic Cold Reversal (ACR). These samples have previously been U/Th and radiocarbon dated. Corals were collected south of Tasmania from depths of between ~1450 - 1900 m, with 70% between 1500 and 1700 m. Uranium and thorium measurements were made by MC-ICP-MS on a ThermoFinnigan Neptune, radiocarbon was measured by AMS at the KCCAMS Laboratory at UC Irvine, and clumped isotope temperatures were measured on a MAT 253 attached to an automated carbonate preparation line. Preliminary results show constant temperature between ~20 - 18 ka, a gradual rise of ~6 ºC through Heinrich Stadial 1 (~18 - 15 ka), an abrupt drop of ~7 ºC directly preceeding the start of the Bølling at 14.7 ka, and another slight rise of ~4 ºC through the ACR (14.7 - 12.8 ka). The addition of clumped isotope temperatures to

  4. Palaeoceanography. Antarctic stratification and glacial CO2.

    PubMed

    Keeling, R F; Visbeck, M

    2001-08-09

    One way of accounting for lowered atmospheric carbon dioxide concentrations during Pleistocene glacial periods is by invoking the Antarctic stratification hypothesis, which links the reduction in CO2 to greater stratification of ocean surface waters around Antarctica. As discussed by Sigman and Boyle, this hypothesis assumes that increased stratification in the Antarctic zone (Fig. 1) was associated with reduced upwelling of deep waters around Antarctica, thereby allowing CO2 outgassing to be suppressed by biological production while also allowing biological production to decline, which is consistent with Antarctic sediment records. We point out here, however, that the response of ocean eddies to increased Antarctic stratification can be expected to increase, rather than reduce, the upwelling rate of deep waters around Antarctica. The stratification hypothesis may have difficulty in accommodating eddy feedbacks on upwelling within the constraints imposed by reconstructions of winds and Antarctic-zone productivity in glacial periods.

  5. Distribution and abundance of Antarctic krill (Euphausia superba) along the Antarctic Peninsula

    NASA Astrophysics Data System (ADS)

    Siegel, Volker; Reiss, Christian S.; Dietrich, Kimberly S.; Haraldsson, Matilda; Rohardt, Gerhard

    2013-07-01

    Net-based data on the abundance, distribution, and demographic patterns of Antarctic krill are quantified from a contemporaneous two ship survey of the Antarctic Peninsula during austral summer 2011. Two survey areas were sampled focussed on Marguerite Bay in the south, and the tip of the Antarctic Peninsula in the north. Data from 177 stations showed that the highest concentrations of krill were found in the southern sampling area. Differences between areas were associated with a few large catches of one year old krill found in anomalously warm and productive waters in Marguerite Bay, and small krill catches in the less-productive, offshore waters in the north. Estimated krill density across the survey area was 3.4 krill m-2, and was low compared to the long-term average of 45 krill m-2 for the Elephant Island area. Overall recruitment between the two survey regions was similar, but per capita recruitment was about 60% lower than historical mean recruitment levels measured at Elephant Island since the late 1970s. Demographic patterns showed small krill concentrated near the coast, and large krill concentrated offshore on the shelf and slope all along the survey area. The offshore distribution of adult krill was delineated by the warm (˜1 °C), low salinity (33.8) water at 30 m, suggesting that most krill were present shoreward of the southern boundary of Antarctic Circumpolar Current Front. Distributions of larvae indicated that three hotspot areas were important for the production of krill: slope areas outside Marguerite Bay and north of the South Shetland Islands, and near the coast around Antarctic Sound. Successful spawning, as inferred from larval abundance, was roughly coincident with the shelf break and not with inshore waters. Given the rapid changes in climate along the Antarctic Peninsula and the lower per capita recruitment observed in recent years, studies comparing and contrasting production, growth, and recruitment across the Peninsula will be

  6. Archival processes of the water stable isotope signal in East Antarctic ice cores

    NASA Astrophysics Data System (ADS)

    Casado, Mathieu; Landais, Amaelle; Picard, Ghislain; Münch, Thomas; Laepple, Thomas; Stenni, Barbara; Dreossi, Giuliano; Ekaykin, Alexey; Arnaud, Laurent; Genthon, Christophe; Touzeau, Alexandra; Masson-Delmotte, Valerie; Jouzel, Jean

    2018-05-01

    The oldest ice core records are obtained from the East Antarctic Plateau. Water isotopes are key proxies to reconstructing past climatic conditions over the ice sheet and at the evaporation source. The accuracy of climate reconstructions depends on knowledge of all processes affecting water vapour, precipitation and snow isotopic compositions. Fractionation processes are well understood and can be integrated in trajectory-based Rayleigh distillation and isotope-enabled climate models. However, a quantitative understanding of processes potentially altering snow isotopic composition after deposition is still missing. In low-accumulation sites, such as those found in East Antarctica, these poorly constrained processes are likely to play a significant role and limit the interpretability of an ice core's isotopic composition. By combining observations of isotopic composition in vapour, precipitation, surface snow and buried snow from Dome C, a deep ice core site on the East Antarctic Plateau, we found indications of a seasonal impact of metamorphism on the surface snow isotopic signal when compared to the initial precipitation. Particularly in summer, exchanges of water molecules between vapour and snow are driven by the diurnal sublimation-condensation cycles. Overall, we observe in between precipitation events modification of the surface snow isotopic composition. Using high-resolution water isotopic composition profiles from snow pits at five Antarctic sites with different accumulation rates, we identified common patterns which cannot be attributed to the seasonal variability of precipitation. These differences in the precipitation, surface snow and buried snow isotopic composition provide evidence of post-deposition processes affecting ice core records in low-accumulation areas.

  7. Antarctic Ocean Nutrient Conditions During the Last Two Glacial Cycles

    NASA Astrophysics Data System (ADS)

    Studer, A.; Sigman, D. M.; Martinez-Garcia, A.; Benz, V.; Winckler, G.; Kuhn, G.; Esper, O.; Lamy, F.; Jaccard, S.; Wacker, L.; Oleynik, S.; Gersonde, R.; Haug, G. H.

    2014-12-01

    The high concentration of the major nutrients nitrate and phosphate in the Antarctic Zone of the Southern Ocean dictates the nature of Southern Ocean ecosystems and permits these nutrients to be carried from the deep ocean into the nutrient-limited low latitudes. Incomplete nutrient consumption in the Antarctic also allows the leakage of deeply sequestered carbon dioxide (CO2) back to the atmosphere, and changes in this leakage may have driven glacial/interglacial cycles in atmospheric CO2. In a sediment core from the Pacific sector of the Antarctic Ocean, we report diatom-bound N isotope (δ15Ndb) records for total recoverable diatoms and two assemblages of diatom species. These data indicate tight coupling between the degree of nitrate consumption and Antarctic climate across the last two glacial cycles, with δ15Ndb (and thus the degree of nitrate consumption) increasing at each major Antarctic cooling event. Measurements in the same sediment core indicate that export production was reduced during ice ages, pointing to an ice age reduction in the supply of deep ocean-sourced nitrate to the Antarctic Ocean surface. The reduced export production of peak ice ages also implies a weaker winter-to-summer decline (i.e. reduced seasonality) in mixed layer nitrate concentration, providing a plausible explanation for an observed reduction in the inter-assemblage δ15Ndb difference during these coldest times. Despite the weak summertime productivity, the reduction in wintertime nitrate supply from deep waters left the Antarctic mixed layer with a low nitrate concentration, and this wintertime change also would have reduced the outgassing of CO2. Relief of light limitation fails to explain the intermediate degree of nitrate consumption that characterizes early glacial conditions, as improved light limitation coincident with reduced nitrate supply would drive nitrate consumption to completion. Thus, the data favor iron availability as the dominant control on annual Antarctic

  8. Rapid variability of Antarctic Bottom Water transport into the Pacific Ocean inferred from GRACE

    NASA Astrophysics Data System (ADS)

    Mazloff, Matthew R.; Boening, Carmen

    2016-04-01

    Air-ice-ocean interactions in the Antarctic lead to formation of the densest waters on Earth. These waters convect and spread to fill the global abyssal oceans. The heat and carbon storage capacity of these water 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 ocean 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 Water 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.

  9. Lethal and behavioral impacts of diesel and fuel oil on the Antarctic amphipod Paramoera walkeri.

    PubMed

    Brown, Kathryn E; King, Catherine K; Harrison, Peter L

    2017-09-01

    Toxicity testing with Antarctic species is required for risk assessment of fuel spills in Antarctic coastal waters. The lethal and sublethal (movement behavior) sensitivities of adults and juveniles of the Antarctic amphipod Paramoera walkeri to the water accommodated fractions (WAFs) of 3 fuels were estimated in extended-duration tests at -1 °C to 21 d. Response of P. walkeri for lethal hydrocarbon concentrations was slow, with 50% lethal concentrations (LC50s) first able to be estimated at 7 d for adults exposed to Special Antarctic Blend diesel (SAB), which had the highest hydrocarbon concentrations of the 3 fuel WAFs. Juveniles showed greater response to marine gas oil (MGO) and intermediate residual fuel oil (IFO 180) at longer exposure durations and were most sensitive at 21 d to IFO 180 (LC50 = 12 μg/L). Adults were initially more sensitive than juveniles; at 21 d, however, juveniles were more than twice as sensitive as adults to SAB (LC50 = 153 μg/L and 377 μg/L, respectively). Significant effects on movement behavior were evident at earlier time points and lower concentrations than was mortality in all 3 fuel WAFs, and juveniles were highly sensitive to sublethal effects of MGO. These first estimates of Antarctic amphipod sensitivity to diesel and fuel oils in seawater contribute to the development of ecologically relevant risk assessments for management of hydrocarbon contamination in the region. Environ Toxicol Chem 2017;36:2444-2455. © 2017 SETAC. © 2017 SETAC.

  10. The Nature of Antarctic Temperature Change

    NASA Astrophysics Data System (ADS)

    Markle, B. R.; Steig, E. J.

    2017-12-01

    The Antarctic is an important component of global climate. While the Arctic has warmed significantly in the last century, the Antarctic as a whole has shown considerably less variability. There is, however, a pronounced spatial pattern to modern Antarctic temperature change. The high East Antarctic Ice Sheet shows little to no warming over recent decades while West Antarctica and the Peninsula shows some of the largest rates of warming on the globe. Examining past climate variability can help reveal the physical processes governing this spatial pattern of Antarctic temperature change. Modern Antarctic temperature variability is known from satellite and weather station observations. Understanding changes in the past, however, requires paleoclimate-proxies such as ice-core water-isotope records. Here we assess the spatial pattern of Antarctic temperature changes across a range of timescales, from modern decadal changes to millennial and orbital-scale variability. We reconstruct past changes in absolute temperatures from a suite of deep ice core records and an improved isotope-temperature reconstruction method. We use δ18O and deuterium excess records to reconstruct both evaporation source and condensation site temperatures. In contrast to previous studies we use a novel method that accounts for nonlinearities in the water-isotope distillation process. We quantify past temperature changes over the Southern Ocean and Antarctic Continent and the magnitude of polar amplification. We identify patterns of Antarctic temperature change that are common across a wide range of timescales and independent of the source of forcing. We examine the nature of these changes and their relationship to atmospheric thermodynamics.

  11. Water masses in the Humboldt Current System: Properties, distribution, and the nitrate deficit as a chemical water mass tracer for Equatorial Subsurface Water off Chile

    NASA Astrophysics Data System (ADS)

    Silva, Nelson; Rojas, Nora; Fedele, Aldo

    2009-07-01

    Three sections are used to analyze the physical and chemical characteristics of the water masses in the eastern South Pacific and their distributions. Oceanographic data were taken from the SCORPIO (May-June 1967), PIQUERO (May-June 1969), and KRILL (June 1974) cruises. Vertical sections of temperature, salinity, σ θ, dissolved oxygen, nitrate, nitrite, phosphate, and silicate were used to analyze the water column structure. Five water masses were identified in the zone through T- S diagrams: Subantarctic Water, Subtropical Water, Equatorial Subsurface Water, Antarctic Intermediate Water, and Pacific Deep Water. Their proportions in the sea water mixture are calculated using the mixing triangle method. Vertical sections were used to describe the geographical distributions of the water mass cores in the upper 1500 m. Several characteristic oceanographic features in the study area were analyzed: the shallow salinity minimum displacement towards the equator, the equatorial subsurface salinity maximum associated with a dissolved oxygen minimum zone and a high nutrient content displacement towards the south, and the equatorward intermediate Antarctic salinity minimum associated with a dissolved oxygen maximum. The nitrate deficit generated in the denitrification area off Peru and northern Chile is proposed as a conservative chemical tracer for the Equatorial Subsurface Waters off the coast of Chile, south of 25°S.

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

    NASA Astrophysics Data System (ADS)

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

    2017-08-01

    This study analyzed shipboard air-sea measurements acquired by the icebreaker Aurora Australis during its off-winter operation in December 2010 to May 2012. Mean conditions over 7 months (October-April) were compiled from a total of 22 ship tracks. The icebreaker traversed the water between Hobart, Tasmania, and the Antarctic continent, providing valuable in situ insight into two dynamically important, yet poorly sampled, regimes: the sub-Antarctic Southern Ocean and the Antarctic marginal ice zone (MIZ) in the Indian Ocean sector. The transition from the open water to the ice-covered surface creates sharp changes in albedo, surface roughness, and air temperature, leading to consequential effects on air-sea variables and fluxes. Major effort was made to estimate the air-sea fluxes in the MIZ using the bulk flux algorithms that are tuned specifically for the sea-ice effects, while computing the fluxes over the sub-Antarctic section using the COARE3.0 algorithm. The study evidenced strong sea-ice modulations on winds, with the southerly airflow showing deceleration (convergence) in the MIZ and acceleration (divergence) when moving away from the MIZ. Marked seasonal variations in heat exchanges between the atmosphere and the ice margin were noted. The monotonic increase in turbulent latent and sensible heat fluxes after summer turned the MIZ quickly into a heat loss regime, while at the same time the sub-Antarctic surface water continued to receive heat from the atmosphere. The drastic increase in turbulent heat loss in the MIZ contrasted sharply to the nonsignificant and seasonally invariant turbulent heat loss over the sub-Antarctic open water.Plain Language SummaryThe icebreaker Aurora Australis is a research and supply vessel that is regularly chartered by the Australian <span class="hlt">Antarctic</span> Division during the southern summer to operate in <span class="hlt">waters</span> between Hobart, Tasmania, and Antarctica. The vessel serves as the main lifeline to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1986DSRA...33...55P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1986DSRA...33...55P"><span>Deep and <span class="hlt">intermediate</span> mediterranean <span class="hlt">water</span> in the western Alboran Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Parrilla, Gregorio; Kinder, Thomas H.; Preller, Ruth H.</p> <p>1986-01-01</p> <p>Hydrographic and current meter data, obtained during June to October 1982, and numerical model experiments are used to study the distribution and flow of Mediterranean <span class="hlt">waters</span> in the western Alboran Sea. The <span class="hlt">Intermediate</span> <span class="hlt">Water</span> is more pronounced in the northern three-fourths of the sea, but its distribution is patchy as manifested by variability of the temperature and salinity maxima at scales ≤10 km. Current meters in the lower <span class="hlt">Intermediate</span> <span class="hlt">Water</span> showed mean flow toward the Strait at 2 cm s -1. A reversal of this flow lasted about 2 weeks. A rough estimate of the mean westward <span class="hlt">Intermediate</span> <span class="hlt">Water</span> transport was 0.4 × 10 6 m 3 s -1, about one-third of the total outflow, so that the best estimates of the contributions of traditionally defined <span class="hlt">Intermediate</span> <span class="hlt">Water</span> and Deep <span class="hlt">Water</span> account for only about one-half of the total outflow. The Deep <span class="hlt">Water</span> was uplifted against the southern continental slope from Alboran Island (3°W) to the Strait. There was also a similar but much weaker banking against the Spanish slope, but a deep current record showed that the eastward recirculation implied by this banking is probably intermittent. Two-layer numerical model experiments simulated the <span class="hlt">Intermediate</span> <span class="hlt">Water</span> flow with a flat bottom and the Deep <span class="hlt">Water</span> with realistic bottom topography. Both experiments replicated the major circulation features, and the <span class="hlt">Intermediate</span> <span class="hlt">Water</span> flow was concentrated in the north because of rotation and the Deep <span class="hlt">Water</span> flow in the south because of topographic control.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26081896','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26081896"><span>Metazoan Parasites of <span class="hlt">Antarctic</span> Fishes.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Oğuz, Mehmet Cemal; Tepe, Yahya; Belk, Mark C; Heckmann, Richard A; Aslan, Burçak; Gürgen, Meryem; Bray, Rodney A; Akgül, Ülker</p> <p>2015-06-01</p> <p>To date, there have been nearly 100 papers published on metazoan parasites of <span class="hlt">Antarctic</span> fishes, but there has not yet been any compilation of a species list of fish parasites for this large geographic area. Herein, we provide a list of all documented occurrences of monogenean, cestode, digenean, acanthocephalan, nematode, and hirudinean parasites of <span class="hlt">Antarctic</span> fishes. The list includes nearly 250 parasite species found in 142 species of host fishes. It is likely that there are more species of fish parasites, which are yet to be documented from <span class="hlt">Antarctic</span> <span class="hlt">waters</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008HMR....62..143P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008HMR....62..143P"><span>Redescription of Terebellides kerguelensis stat. nov. (Polychaeta: Trichobranchidae) from <span class="hlt">Antarctic</span> and subantarctic <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>Parapar, Julio; Moreira, Juan</p> <p>2008-06-01</p> <p>During the Spanish <span class="hlt">Antarctic</span> expeditions “Bentart” 1994, 1995 and 2003, a number of trichobranchid (Annelida: Polychaeta) specimens were collected and identified initially as Terebellides stroemii kerguelensis McIntosh, 1885, the only known species of the genus widely recognised as valid in <span class="hlt">Antarctic</span> <span class="hlt">waters</span>. In the framework of a worldwide revision of the genus Terebellides, a reconsideration of the taxonomic status of this subspecies of the boreal Terebellides stroemii Sars, 1835 is done through the examination of the syntypes of T. s. kerguelensis compared with recent descriptions of the nominal species from Norwegian <span class="hlt">waters</span> and material from Icelandic <span class="hlt">waters</span>. Thus, T. s. kerguelensis is regarded as a valid species, T. kerguelensis stat. nov., and redescribed designating a lectotype and paralectotypes. The species is mainly characterised by the presence of an anterior branchial extension (fifth lobe), lateral lappets in five anterior thoracic chaetigers, segmental organs in chaetigers 1, 4 and 5, and first thoracic acicular neurochaetae sharply bent with pointed tips. The biological role of the segmental organs, the presence and disposition of cilia in branchial lamellae and the finding of new structures located in dorsal part of thoracic notopodia are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5266476','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5266476"><span>Accelerated freshening of <span class="hlt">Antarctic</span> Bottom <span class="hlt">Water</span> over the last decade in the Southern Indian Ocean</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Menezes, Viviane V.; Macdonald, Alison M.; Schatzman, Courtney</p> <p>2017-01-01</p> <p>Southern Ocean abyssal <span class="hlt">waters</span>, in contact with the atmosphere at their formation sites around Antarctica, not only bring signals of a changing climate with them as they move around the globe but also contribute to that change through heat uptake and sea level rise. A repeat hydrographic line in the Indian sector of the Southern Ocean, occupied three times in the last two decades (1994, 2007, and, most recently, 2016), reveals that <span class="hlt">Antarctic</span> Bottom <span class="hlt">Water</span> (AABW) continues to become fresher (0.004 ± 0.001 kg/g decade−1), warmer (0.06° ± 0.01°C decade−1), and less dense (0.011 ± 0.002 kg/m3 decade−1). The most recent observations in the Australian-<span class="hlt">Antarctic</span> Basin show a particularly striking acceleration in AABW freshening between 2007 and 2016 (0.008 ± 0.001 kg/g decade−1) compared to the 0.002 ± 0.001 kg/g decade−1 seen between 1994 and 2007. Freshening is, in part, responsible for an overall shift of the mean temperature-salinity curve toward lower densities. The marked freshening may be linked to an abrupt iceberg-glacier collision and calving event that occurred in 2010 on the George V/Adélie Land Coast, the main source region of bottom <span class="hlt">waters</span> for the Australian-<span class="hlt">Antarctic</span> Basin. Because AABW is a key component of the global overturning circulation, the persistent decrease in bottom <span class="hlt">water</span> density and the associated increase in steric height that result from continued warming and freshening have important consequences beyond the Southern Indian Ocean. PMID:28138548</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28138548','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28138548"><span>Accelerated freshening of <span class="hlt">Antarctic</span> Bottom <span class="hlt">Water</span> over the last decade in the Southern Indian Ocean.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Menezes, Viviane V; Macdonald, Alison M; Schatzman, Courtney</p> <p>2017-01-01</p> <p>Southern Ocean abyssal <span class="hlt">waters</span>, in contact with the atmosphere at their formation sites around Antarctica, not only bring signals of a changing climate with them as they move around the globe but also contribute to that change through heat uptake and sea level rise. A repeat hydrographic line in the Indian sector of the Southern Ocean, occupied three times in the last two decades (1994, 2007, and, most recently, 2016), reveals that <span class="hlt">Antarctic</span> Bottom <span class="hlt">Water</span> (AABW) continues to become fresher (0.004 ± 0.001 kg/g decade -1 ), warmer (0.06° ± 0.01°C decade -1 ), and less dense (0.011 ± 0.002 kg/m 3 decade -1 ). The most recent observations in the Australian-<span class="hlt">Antarctic</span> Basin show a particularly striking acceleration in AABW freshening between 2007 and 2016 (0.008 ± 0.001 kg/g decade -1 ) compared to the 0.002 ± 0.001 kg/g decade -1 seen between 1994 and 2007. Freshening is, in part, responsible for an overall shift of the mean temperature-salinity curve toward lower densities. The marked freshening may be linked to an abrupt iceberg-glacier collision and calving event that occurred in 2010 on the George V/Adélie Land Coast, the main source region of bottom <span class="hlt">waters</span> for the Australian-<span class="hlt">Antarctic</span> Basin. Because AABW is a key component of the global overturning circulation, the persistent decrease in bottom <span class="hlt">water</span> density and the associated increase in steric height that result from continued warming and freshening have important consequences beyond the Southern Indian Ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMPP13D..03X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMPP13D..03X"><span>Deglacial Ocean Circulation Scheme at <span class="hlt">Intermediate</span> Depths in the Tropical North Atlantic</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xie, R. C.; Marcantonio, F.; Schmidt, M. W.</p> <p>2014-12-01</p> <p>In the modern Atlantic Ocean, <span class="hlt">intermediate</span> <span class="hlt">water</span> circulation is largely governed by the southward flowing upper North Atlantic Deep <span class="hlt">Water</span> (NADW) and the northward return flow <span class="hlt">Antarctic</span> <span class="hlt">Intermediate</span> <span class="hlt">Water</span> (AAIW). During the last deglaciation, it is commonly accepted that the southward flow Glacial North Atlantic <span class="hlt">Intermediate</span> <span class="hlt">Water</span>, the glacial analogue of NADW, contributed significantly to past variations in <span class="hlt">intermediate</span> <span class="hlt">water</span> circulation. However, to date, there is no common consensus of the role AAIW played during the last deglaciation, especially across abrupt climate events such as the Heinrich 1 and the Younger Dryas. This study aims to reconstruct <span class="hlt">intermediate</span> northern- and southern-sourced <span class="hlt">water</span> circulation in the tropical North Atlantic during the past 22 kyr and attempts to confine the boundary between AAIW and northern-sourced <span class="hlt">intermediate</span> <span class="hlt">waters</span> in the past. High-resolution Nd isotopic compositions (ɛNd thereafter) of fish debris and bulk sediment acid-reductive leachate from the Southern Caribbean (VM12-107; 1079 m) are inconsistent, again casting concerns, as already raised by recent studies, on the reliability of the leachate method in extracting seawater ɛNd signature. This urges the need to carefully verify the seawater ɛNd integrity in sediment acid-reductive leachate in various oceanic settings. Fish debris Nd isotope record in our study displays a two-step decreasing trend from the early deglaciation to early Holocene. We interpret this as recording a two-step deglacial recovery of the upper NADW, given the assumption on a more radiogenic glacial northern-sourced <span class="hlt">water</span> is valid. Comparing with authigenic ɛNd records in the Florida Straits [1] and the Demarara Rise [2], our new fish debris ɛNd results suggest that, in the tropical western North Atlantic, glacial and deglacial AAIW never penetrated beyond the lower depth limit of modern AAIW. [1] Xie et al., GCA (140) 2014; [2] Huang et al., EPSL (389) 2014</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1715438Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1715438Z"><span>Controls and variability of solute and sedimentary fluxes in <span class="hlt">Antarctic</span> and sub-<span class="hlt">Antarctic</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>Zwolinski, Zbigniew</p> <p>2015-04-01</p> <p>. Solute and sediment transport in the streams of analyzed environments are constrained by the relatively short <span class="hlt">water</span> runoff season that typically lasts from a few weeks to maximum of four months during the austral summer, for <span class="hlt">Antarctic</span> and sub-<span class="hlt">Antarctic</span> regions respectively. Because of high intensity of mechanical and chemical weathering processes solute and sediment transport are rather high within <span class="hlt">Antarctic</span> environments. Weathering rates on slopes and magnitude of fluvial transport in relatively short streams control the intensity of denudational processes. Both mechanical and chemical denudation varies highly through sub-<span class="hlt">Antarctic</span> and <span class="hlt">Antarctic</span> environments. To generate accurate predictions of fluvial and denudational processes we must fully understand the actual geoecological processes, which in some places are under rapid change, e.g., the <span class="hlt">Antarctic</span> Peninsula and sub-<span class="hlt">Antarctic</span> islands.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20050160457','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20050160457"><span><span class="hlt">Intermediate</span> Temperature <span class="hlt">Water</span> Heat Pipe Tests</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Devarakonda, Angirasa; Xiong, Da-Xi; Beach, Duane E.</p> <p>2005-01-01</p> <p>Heat pipes are among the most promising technologies for space radiator systems. <span class="hlt">Water</span> heat pipes are explored in the <span class="hlt">intermediate</span> temperature range of 400 to above 500 K. The thermodynamic and thermo-physical properties of <span class="hlt">water</span> are reviewed in this temperature range. Test data are reported for a copper-<span class="hlt">water</span> heat pipe. The heat pipe was tested under different orientations. <span class="hlt">Water</span> heat pipes show promise in this temperature range. Fabrication and testing issues are being addressed.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_1");'>1</a></li> <li><a href="#" onclick='return showDiv("page_2");'>2</a></li> <li class="active"><span>3</span></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_3 --> <div id="page_4" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_2");'>2</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li class="active"><span>4</span></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="61"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-s48-152-007.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-s48-152-007.html"><span>Breakup of Pack Ice, <span class="hlt">Antarctic</span> Ice Shelf</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>1991-09-18</p> <p>STS048-152-007 (12-18 Sept 1991) --- The periphery of the <span class="hlt">Antarctic</span> ice shelf and the <span class="hlt">Antarctic</span> Peninsula were photographed by the STS 48 crew members. Strong offshore winds, probably associated with katabatic winds from the interior of the continent, are peeling off the edges of the ice shelf into ribbons of sea ice, icebergs, bergy bits and growlers into the cold <span class="hlt">waters</span> of the circum-<span class="hlt">Antarctic</span> southern ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3700924','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3700924"><span><span class="hlt">Antarctic</span> Crabs: Invasion or Endurance?</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Griffiths, Huw J.; Whittle, Rowan J.; Roberts, Stephen J.; Belchier, Mark; Linse, Katrin</p> <p>2013-01-01</p> <p>Recent scientific interest following the “discovery” of lithodid crabs around Antarctica has centred on a hypothesis that these crabs might be poised to invade the <span class="hlt">Antarctic</span> shelf if the recent warming trend continues, potentially decimating its native fauna. This “invasion hypothesis” suggests that decapod crabs were driven out of Antarctica 40–15 million years ago and are only now returning as “warm” enough habitats become available. The hypothesis is based on a geographically and spatially poor fossil record of a different group of crabs (Brachyura), and examination of relatively few Recent lithodid samples from the <span class="hlt">Antarctic</span> slope. In this paper, we examine the existing lithodid fossil record and present the distribution and biogeographic patterns derived from over 16,000 records of Recent Southern Hemisphere crabs and lobsters. Globally, the lithodid fossil record consists of only two known specimens, neither of which comes from the <span class="hlt">Antarctic</span>. Recent records show that 22 species of crabs and lobsters have been reported from the Southern Ocean, with 12 species found south of 60°S. All are restricted to <span class="hlt">waters</span> warmer than 0°C, with their <span class="hlt">Antarctic</span> distribution limited to the areas of seafloor dominated by Circumpolar Deep <span class="hlt">Water</span> (CDW). Currently, CDW extends further and shallower onto the West <span class="hlt">Antarctic</span> shelf than the known distribution ranges of most lithodid species examined. Geological evidence suggests that West <span class="hlt">Antarctic</span> shelf could have been available for colonisation during the last 9,000 years. Distribution patterns, species richness, and levels of endemism all suggest that, rather than becoming extinct and recently re-invading from outside Antarctica, the lithodid crabs have likely persisted, and even radiated, on or near to <span class="hlt">Antarctic</span> slope. We conclude there is no evidence for a modern-day “crab invasion”. We recommend a repeated targeted lithodid sampling program along the West <span class="hlt">Antarctic</span> shelf to fully test the validity of the </p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C53D..01N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C53D..01N"><span>Examining Differences in Arctic and <span class="hlt">Antarctic</span> Sea Ice Change</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nghiem, S. V.; Rigor, I. G.; Clemente-Colon, P.; Neumann, G.; Li, P.</p> <p>2015-12-01</p> <p>The paradox of the rapid reduction of Arctic sea ice versus the stability (or slight increase) of <span class="hlt">Antarctic</span> sea ice remains a challenge in the cryospheric science research community. Here we start by reviewing a number of explanations that have been suggested by different researchers and authors. One suggestion is that stratospheric ozone depletion may affect atmospheric circulation and wind patterns such as the Southern Annular Mode, and thereby sustaining the <span class="hlt">Antarctic</span> sea ice cover. The reduction of salinity and density in the near-surface layer may weaken the convective mixing of cold and warmer <span class="hlt">waters</span>, and thus maintaining regions of no warming around the <span class="hlt">Antarctic</span>. A decrease in sea ice growth may reduce salt rejection and upper-ocean density to enhance thermohalocline stratification, and thus supporting <span class="hlt">Antarctic</span> sea ice production. Melt <span class="hlt">water</span> from <span class="hlt">Antarctic</span> ice shelves collects in a cool and fresh surface layer to shield the surface ocean from the warmer deeper <span class="hlt">waters</span>, and thus leading to an expansion of <span class="hlt">Antarctic</span> sea ice. Also, wind effects may positively contribute to <span class="hlt">Antarctic</span> sea ice growth. Moreover, Antarctica lacks of additional heat sources such as warm river discharge to melt sea ice as opposed to the case in the Arctic. Despite of these suggested explanations, factors that can consistently and persistently maintains the stability of sea ice still need to be identified for the <span class="hlt">Antarctic</span>, which are opposed to factors that help accelerate sea ice loss in the Arctic. In this respect, using decadal observations from multiple satellite datasets, we examine differences in sea ice properties and distributions, together with dynamic and thermodynamic processes and interactions with land, ocean, and atmosphere, causing differences in Arctic and <span class="hlt">Antarctic</span> sea ice change to contribute to resolving the Arctic-<span class="hlt">Antarctic</span> sea ice paradox.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017DSRI..128...82J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017DSRI..128...82J"><span>Arctic <span class="hlt">Intermediate</span> <span class="hlt">Water</span> in the Nordic Seas, 1991-2009</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jeansson, Emil; Olsen, Are; Jutterström, Sara</p> <p>2017-10-01</p> <p>The evolution of the different types of Arctic <span class="hlt">Intermediate</span> <span class="hlt">Water</span> (AIW) in the Nordic Seas is evaluated and compared utilising hydro-chemical data from 1991 to 2009. It has been suggested that these <span class="hlt">waters</span> are important components of the Norwegian Sea Arctic <span class="hlt">Intermediate</span> <span class="hlt">Water</span> (NSAIW), and of the dense overflows to the North Atlantic. Thus, it is important to understand how their properties and distribution vary with time. The AIWs from the Greenland and Iceland Seas, show different degrees of variability during the studied period; however, only the Greenland Sea Arctic <span class="hlt">Intermediate</span> <span class="hlt">Water</span> (GSAIW) shows an increasing temperature and salinity throughout the 2000s, which considerably changed the properties of this <span class="hlt">water</span> mass. Optimum multiparameter (OMP) analysis was conducted to assess the sources of the NSAIW. The analysis shows that the Iceland Sea Arctic <span class="hlt">Intermediate</span> <span class="hlt">Water</span> (ISAIW) and the GSAIW both contribute to NSAIW, at different densities corresponding to their respective density range. This illustrates that they flow largely isopycnally from their source regions to the Norwegian Sea. The main source of the NSAIW, however, is the upper Polar Deep <span class="hlt">Water</span>, which explains the lower concentrations of oxygen and chlorofluorocarbons, and higher salinity and nutrient concentrations of the NSAIW layer compared with the ISAIW and GSAIW. This shows how vital it is to include chemical tracers in any <span class="hlt">water</span> mass analysis to correctly assess the sources of the <span class="hlt">water</span> mass being studied.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E%26PSL.491...48D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26PSL.491...48D"><span>Reduced oxygenation at <span class="hlt">intermediate</span> depths of the southwest Pacific during the last glacial maximum</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Durand, Axel; Chase, Zanna; Noble, Taryn L.; Bostock, Helen; Jaccard, Samuel L.; Townsend, Ashley T.; Bindoff, Nathaniel L.; Neil, Helen; Jacobsen, Geraldine</p> <p>2018-06-01</p> <p>To investigate changes in oxygenation at <span class="hlt">intermediate</span> depths in the southwest Pacific between the Last Glacial Maximum (LGM) and the Holocene, redox sensitive elements uranium and rhenium were measured in 12 sediment cores located on the Campbell and Challenger plateaux offshore from New Zealand. The core sites are currently bathed by Subantarctic Mode <span class="hlt">Water</span> (SAMW), <span class="hlt">Antarctic</span> <span class="hlt">Intermediate</span> <span class="hlt">Water</span> (AAIW) and Upper Circumpolar Deep <span class="hlt">Water</span> (UCDW). The sedimentary distributions of authigenic uranium and rhenium reveal reduced oxygen content at <span class="hlt">intermediate</span> depths (800-1500 m) during the LGM compared to the Holocene. In contrast, data from deeper <span class="hlt">waters</span> (≥1500 m) indicate higher oxygen content during the LGM compared to the Holocene. These data, together with variations in benthic foraminiferal δ13C, are consistent with a shallower AAIW-UCDW boundary over the Campbell Plateau during the LGM. Whilst AAIW continued to bathe the <span class="hlt">intermediate</span> depths (≤1500 m) of the Challenger Plateau during the LGM, the data suggest that the AAIW at these core sites contained less oxygen compared to the Holocene. These results are at odds with the general notion that AAIW was better oxygenated and expanded deeper during the LGM due to stronger westerlies and colder temperatures. These findings may be explained by an important change in AAIW formation and circulation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSHE43B..02A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSHE43B..02A"><span>Observations of <span class="hlt">Antarctic</span> Slope Current Transport and Dense <span class="hlt">Water</span> Flow in the Northwestern Weddell Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Azaneu, M. V. C.; Heywood, K. J.; Queste, B. Y.; Thompson, A. F.</p> <p>2016-02-01</p> <p>In early 2012 the GENTOO project deployed three Seagliders in the northwest Weddell Sea, acquiring high temporal and spatial resolution measurements around Powell Basin for a period of 10 weeks. The <span class="hlt">Antarctic</span> Slope Front and associated currents form a physical and dynamical barrier to the cross-slope exchange of properties, influencing local and global ocean dynamics. The Seaglider dataset comprises 1598 temperature and salinity profiles and is used to better understand cross-slope processes. From this dataset, 582 glider profiles with altimetric information at the east <span class="hlt">Antarctic</span> Peninsula continental slope are used to investigate the properties and thickness of the dense bottom <span class="hlt">water</span> spilling off the shelf. The dense <span class="hlt">water</span> is identified mostly over the slope, between the 500 and 1000 m isobaths. The dense layer is thickest around ˜ 63.33 °S, along the 1000 m isobath, becoming thinner onshore and towards northern areas. We also evaluate with unprecedented resolution the along-stream velocity and potential vorticity fields along the 17 transects across the eastern <span class="hlt">Antarctic</span> Peninsula shelf-break and the 4 transects that cross the South Orkney Islands plateau. Using an improved hydrodynamic flight model, we reference the geostrophic shear to the glider-derived depth-averaged currents corrected for tides. In the western Weddell Sea, the geostrophic velocities fields indicate the presence of a surprisingly weakened <span class="hlt">Antarctic</span> Slope Current (ASC) around 63.5 °S, possibly indicative of high eddy activity in the area. ASC transport in this southernmost section is less than 0.2 Sv. In a more northerly section (˜ 63.1 °S), the ASC transport reaches 6 Sv. The transects west of the South Orkney Island indicate a northward flow, opposite to the previously assumed regime. The results also show intensified northward bottom flows close to the slope, which can be related to processes occurring in the bottom boundary layer. The potential vorticity fields are used to identify</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMOS53C1056K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMOS53C1056K"><span>Geophysical Characteristics of the Australian-<span class="hlt">Antarctic</span> Ridge</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kim, S. S.; Lin, J.; Park, S. H.; Choi, H.; Lee, S. M.</p> <p>2014-12-01</p> <p>Between 2011 and 2013, the Korea Polar Research Institute (KOPRI) conducted three consecutive geologic surveys at the little explored eastern ends of the Australian-<span class="hlt">Antarctic</span> Ridge (AAR) to characterize the tectonics, geochemistry, and hydrothermal activity of this <span class="hlt">intermediate</span> spreading system. Using the Korean icebreaker R/V Araon, the multi-disciplinary research team collected bathymetry, gravity, magnetics, and rock and <span class="hlt">water</span> column samples. In addition, Miniature Autonomous Plume Recorders (MAPRs) were deployed at wax-core rock sampling sites to detect the presence of active hydrothermal vents. Here we present a detailed analysis of a 300-km-long supersegment of the AAR to quantify the spatial variations in ridge morphology and robust axial and off-axis volcanisms. The ridge axis morphology alternates between rift valleys and axial highs within relatively short ridge segments. To obtain a geological proxy for regional variations in magma supply, we calculated residual mantle Bouguer gravity anomalies (RMBA), gravity-derived crustal thickness, and residual topography for seven sub-segments. The results of the analyses revealed that the southern flank of the AAR is associated with shallower seafloor, more negative RMBA, thicker crust, and/or less dense mantle than the conjugate northern flank. Furthermore, this north-south asymmetry becomes more prominent toward the KR1 supersegment of the AAR. The axial topography of the KR1 supersegment exhibits a sharp transition from axial highs at the western end to rift valleys at the eastern end, with regions of axial highs being associated with more magma supply as indicated by more negative RMBA. We also compare and contrast the characteristics of the AAR supersegment with that of other ridges of <span class="hlt">intermediate</span> spreading rates, including the Juan de Fuca Ridge, Galápagos Spreading Center, and Southeast Indian Ridge west of the Australian-<span class="hlt">Antarctic</span> Discordance, to investigate the influence of ridge-hotspot interaction on</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010DSRI...57..639R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010DSRI...57..639R"><span>Chemical evidence of the changes of the <span class="hlt">Antarctic</span> Bottom <span class="hlt">Water</span> ventilation in the western Ross Sea between 1997 and 2003</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rivaro, Paola; Massolo, Serena; Bergamasco, Andrea; Castagno, Pasquale; Budillon, Giorgio</p> <p>2010-05-01</p> <p>Data from three Italian CLIMA project cruises between 1997 and 2003 were used to obtain sections of the hydrographic and chemical properties of the main <span class="hlt">water</span> masses across the shelf break off Cape Adare (western Ross Sea, Antarctica). Dissolved oxygen, nitrate and phosphate data were combined on the basis of the Redfield ratio to obtain the quasi-conservative tracers NO (9[NO 3]+[O 2]), PO (135[PO 4]+[O 2]) and phosphate star PO4* ( PO4*=[PO 4]+[O 2]/175-1.95). In 1997 and 2003 the presence of the High Salinity Shelf <span class="hlt">Water</span> at the bottom depth near the sill was traced by both physical and chemical measurements. In 2001 the Modified Shelf <span class="hlt">Water</span>, characterized by warmer temperature and by a lower dissolved oxygen content than High Salinity Shelf <span class="hlt">Water</span>, was observed at the shelf edge. The distribution of the chemical tracers together with the hydrographic observations showed recently formed <span class="hlt">Antarctic</span> Bottom <span class="hlt">Water</span> on the continental slope during all of the cruises. These observations were confirmed by the extended optimum multiparameter analysis. The calculated thickness of the new <span class="hlt">Antarctic</span> Bottom <span class="hlt">Water</span>, as well as the tracer content, were variable in time and in space. The estimated volume of the new <span class="hlt">Antarctic</span> Bottom <span class="hlt">Water</span> and the export of dissolved oxygen and nutrient associated with the overflowing <span class="hlt">water</span> were different over the examined period. In particular, a lower (˜55%) export was evidenced in 2001 compared to 1997.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011DSRI...58.1002B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011DSRI...58.1002B"><span>Thermohaline variability and <span class="hlt">Antarctic</span> bottom <span class="hlt">water</span> formation at the Ross Sea shelf break</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Budillon, Giorgio; Castagno, Pasquale; Aliani, Stefano; Spezie, Giancarlo; Padman, Laurie</p> <p>2011-10-01</p> <p>We use hydrological and current meter data collected in the Ross Sea, Antarctica between 1995 and 2006 to describe the spatial and temporal variability of <span class="hlt">water</span> masses involved in the production of <span class="hlt">Antarctic</span> Bottom <span class="hlt">Water</span> (AABW). Data were collected in two regions of known outflows of dense shelf <span class="hlt">water</span> in this region; the Drygalski Trough (DT) and the Glomar-Challenger Trough (GCT). Dense shelf <span class="hlt">water</span> just inshore of the shelf break is dominated by High Salinity Shelf <span class="hlt">Water</span> (HSSW) in the DT and Ice Shelf <span class="hlt">Water</span> (ISW) in the GCT. The HSSW in the northern DT freshened by ˜0.06 in 11 y, while the ISW in the northern GCT freshened by ˜0.04 in 8 y and warmed by ˜0.04 °C in 11 y, dominated by a rapid warming during austral summer 2001/02. The <span class="hlt">Antarctic</span> Slope Front separating the warm Circumpolar Deep <span class="hlt">Water</span> (CDW) from the shelf <span class="hlt">waters</span> is more stable near GCT than near DT, with CDW and mixing products being found on the outer DT shelf but not on the outer GCT shelf. The different source <span class="hlt">waters</span> and mixing processes at the two sites lead to production of AABW with different thermohaline characteristics in the central and western Ross Sea. Multi-year time series of hydrography and currents at long-term moorings within 100 km of the shelf break in both troughs confirm the interannual signals in the dense shelf <span class="hlt">water</span> and reveal the seasonal cycle of <span class="hlt">water</span> mass properties. Near the DT the HSSW salinities experienced maxima in March/April and minima in September/October. The ISW in the GCT is warmest in March/April and coolest between August and October. Mooring data also demonstrate significant high-frequency variability associated with tides and other processes. Wavelet analysis of near-bottom moored sensors sampling the dense <span class="hlt">water</span> cascade over the continental slope west of the GCT shows intermittent energetic pulses of cold, dense <span class="hlt">water</span> with periods from ˜32 h to ˜5 days.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017DSRII.139....9V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017DSRII.139....9V"><span>Modification of deep <span class="hlt">waters</span> in Marguerite Bay, western <span class="hlt">Antarctic</span> Peninsula, caused by topographic overflows</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Venables, Hugh J.; Meredith, Michael P.; Brearley, J. Alexander</p> <p>2017-05-01</p> <p>Circumpolar Deep <span class="hlt">Water</span> (CDW) intrudes from the mid-layers of the <span class="hlt">Antarctic</span> Circumpolar Current onto the shelf of the western <span class="hlt">Antarctic</span> Peninsula, providing a source of heat and nutrients to the regional ocean. It is well known that CDW is modified as it flows across the shelf, but the mechanisms responsible for this are not fully known. Here, data from underwater gliders with high spatial resolution are used to demonstrate the importance of detailed bathymetry in inducing multiple local mixing events. Clear evidence for overflows is observed in the glider data as <span class="hlt">water</span> flows along a deep channel with multiple transverse ridges. The ridges block the densest <span class="hlt">waters</span>, with overflowing <span class="hlt">water</span> descending several hundred metres to fill subsequent basins. This vertical flow leads to entrainment of overlying colder and fresher <span class="hlt">water</span> in localised mixing events. Initially this process leads to an increase in bottom temperatures due to the temperature maximum <span class="hlt">waters</span> descending to greater depths. After several ridges, however, the mixing is sufficient to remove the temperature maximum completely and the entrainment of colder thermocline <span class="hlt">waters</span> to depth reduces the bottom temperature, to approximately the same as in the source region of Marguerite Trough. Similarly, it is shown that deep <span class="hlt">waters</span> of Palmer Deep are warmer than at the same depth at the shelf break. The exact details of the transformations observed are heavily dependent on the local bathymetry and <span class="hlt">water</span> column structure, but glacially-carved troughs and shallow sills are a common feature of the bathymetry of polar shelves, and these types of processes may be a factor in determining the hydrographic conditions close to the coast across a wider area.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JOUC...16.1109Q','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JOUC...16.1109Q"><span>Freeze concentration of proteins in <span class="hlt">Antarctic</span> krill wash <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>Qi, Xiangming; Xu, Jing; Zhao, Kuo; Guo, Hui; Ma, Lei</p> <p>2017-12-01</p> <p><span class="hlt">Water</span>-washing removes fluoride from <span class="hlt">Antarctic</span> krill but produces large volumes of wash <span class="hlt">water</span> containing <span class="hlt">water</span>- soluble proteins and fluoride. The freeze concentration method was tested to determine if it could be used to recover <span class="hlt">water</span>-soluble proteins while leaving the fluoride in solution. After freezing and thawing the wash <span class="hlt">water</span>, protein and fluoride contents of the thawed fractions were determined to explore the melting regularity of components in the wash <span class="hlt">water</span>. The highest concentration factors of protein and fluoride were obtained after 80 min of thawing, such as 1.48 ± 0.06 and 1.35 ± 0.04 times, respectively. The free amino-nitrogen (FAN) content and sodium dodecyl sulfate-polyacrylamide gel electrophoresis pattern results revealed that the highest concentrations of all ingredients were obtained after 80 min of the process. The degree of hydrolysis of all fractions from the thawing process fluctuated in a narrow range around 12% during the entire process, indicating that the thawing order did not change with various proteins or time during the entire thawing course. These results demonstrate that the freeze concentration method can be used to concentrate protein solutions, even those with fluoride. It was concluded that condensation was achieved and no ingredient could be separated, regardless of fluoride, amino acids, or different proteins in the <span class="hlt">water</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ARMS...10..503P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ARMS...10..503P"><span>A Synoptic View of the Ventilation and Circulation of <span class="hlt">Antarctic</span> Bottom <span class="hlt">Water</span> from Chlorofluorocarbons and Natural Tracers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Purkey, Sarah G.; Smethie, William M.; Gebbie, Geoffrey; Gordon, Arnold L.; Sonnerup, Rolf E.; Warner, Mark J.; Bullister, John L.</p> <p>2018-01-01</p> <p><span class="hlt">Antarctic</span> Bottom <span class="hlt">Water</span> (AABW) is the coldest, densest, most prolific <span class="hlt">water</span> mass in the global ocean. AABW forms at several distinct regions along the <span class="hlt">Antarctic</span> coast and feeds into the bottom limb of the meridional overturning circulation, filling most of the global deep ocean. AABW has warmed, freshened, and declined in volume around the globe in recent decades, which has implications for the global heat and sea level rise budgets. Over the past three decades, the use of tracers, especially time-varying tracers such as chlorofluorocarbons, has been essential to our understanding of the formation, circulation, and variability of AABW. Here, we review three decades of temperature, salinity, and tracer data and analysis that have led to our current knowledge of AABW and how the southern component of deep-ocean ventilation is changing with time.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28877009','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28877009"><span>A Synoptic View of the Ventilation and Circulation of <span class="hlt">Antarctic</span> Bottom <span class="hlt">Water</span> from Chlorofluorocarbons and Natural Tracers.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Purkey, Sarah G; Smethie, William M; Gebbie, Geoffrey; Gordon, Arnold L; Sonnerup, Rolf E; Warner, Mark J; Bullister, John L</p> <p>2018-01-03</p> <p><span class="hlt">Antarctic</span> Bottom <span class="hlt">Water</span> (AABW) is the coldest, densest, most prolific <span class="hlt">water</span> mass in the global ocean. AABW forms at several distinct regions along the <span class="hlt">Antarctic</span> coast and feeds into the bottom limb of the meridional overturning circulation, filling most of the global deep ocean. AABW has warmed, freshened, and declined in volume around the globe in recent decades, which has implications for the global heat and sea level rise budgets. Over the past three decades, the use of tracers, especially time-varying tracers such as chlorofluorocarbons, has been essential to our understanding of the formation, circulation, and variability of AABW. Here, we review three decades of temperature, salinity, and tracer data and analysis that have led to our current knowledge of AABW and how the southern component of deep-ocean ventilation is changing with time.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFMPP13A1367M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFMPP13A1367M"><span>Deglacial Neodymium Isotopic Ratios in the Florida Straits and the Response of <span class="hlt">Intermediate</span> <span class="hlt">Waters</span> to Reduced Meridional Overturning Circulation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marcantonio, F.; Schmidt, M. W.; Franklin, A.; Lynch-Stieglitz, J. M.</p> <p>2009-12-01</p> <p>Neodymium behaves quasi-conservatively in seawater, and its isotopic signature can be used as a tracer for oceanic <span class="hlt">water</span> masses. By analyzing Nd in the authigenic ferromanganese oxide component of marine sediments, past changes in <span class="hlt">water</span> mass movements have been hypothesized. In the Atlantic Ocean, Nd isotope analysis has been used to trace the variable strength of the meridional overturning circulation (MOC) during the last deglaciation (e.g., Pahnke et al., 2008). Here, we use Nd isotopes to investigate whether a decrease in the strength of the past MOC manifests itself as a reduction (Came et al., 2008) or an increase (Pahnke et al., 2008) in the northward incursion of <span class="hlt">Antarctic</span> <span class="hlt">Intermediate</span> <span class="hlt">Water</span> (AAIW) into the North Atlantic. Sediments from two core sites currently bathed by AAIW within the Florida Straits (546 m and 751 m <span class="hlt">water</span> depth) are well suited for profiling authigenic Nd isotope ratios. Because the Florida Current represents a major pathway of the Atlantic MOC surface return flow, the Florida Strait sites can shed light on how variations in AAIW are related to changes in Atlantic MOC strength. The sediments range in age from 0 to 25 kyr, and the high sedimentation rates (8 - 200 cm/kyr) ensure that millennial climate events during the deglaciation are captured. The range in ɛNd measured in the shallower core thus far is low (~ 1.5 epsilon units), but significant. There is a trend in the data which suggests more unradiogenic values during the Younger Dryas event when Atlantic MOC slowed down. Such a trend supports the idea based on benthic foraminiferal Cd/Ca data (Came et al., 2008) that, during the Younger Dryas, there was a reduction within the Florida Current of the flow of <span class="hlt">intermediate</span>, southern-sourced <span class="hlt">waters</span>. Came et al., 2008, Paleoceanography 23, PA1217. Pahnke et al., 2008, Nature Geoscience 1, 870-874.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSHE53B..07N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSHE53B..07N"><span>Meltwater Pathways and Iron Delivery to the <span class="hlt">Antarctic</span> Coastal Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Null, K. A.; Corbett, D. R.; Crenshaw, J.; Peterson, R. N.; Peterson, L.; Buck, C. S.; Lyons, W. B.</p> <p>2016-02-01</p> <p>Freshwater inputs to the <span class="hlt">Antarctic</span> coastal ocean can occur through multiple pathways including calving, streams, and groundwater discharge. The impacts of submarine groundwater discharge on polar ecosystems are generally poorly understood and, until recently, had not been considered as an important physical process along the coast of the <span class="hlt">Antarctic</span> continent. Here, we present a study utilizing multiple tracers (radium, radon, and stable <span class="hlt">water</span> isotopes) to quantify freshwater inputs and chemical constituent fluxes associated with multiple discharge pathways, including submarine groundwater discharge, along the Western <span class="hlt">Antarctic</span> Peninsula. Previous research has shown that primary production in iron-limited <span class="hlt">waters</span> offshore of the <span class="hlt">Antarctic</span> Peninsula is fueled in part by continentally-derived sediments, and our work demonstrates that subglacial/submarine groundwater discharge (SSGD) to continental shelf <span class="hlt">waters</span> in the region is also an important source of dissolved iron (6.4 Gg yr-1; dFe). For reference, this flux equates to approximately 25 times the iron flux from calving in the study area. SSGD also contributed a significantly higher macronutrient flux than calving, although calving contributed more than twice as much freshwater. Thus, SSGD is likely a much more important source of macronutrients and dFe to the nearshore coastal ocean along the Western <span class="hlt">Antarctic</span> Peninsula, and potentially to the continental shelf and offshore <span class="hlt">waters</span> of the entire continent than previously recognized. If we assume similar discharge rates along the entire <span class="hlt">Antarctic</span> coastline ( 45,000 km), the delivery of dFe via SSGD ( 216 Gg yr-1) is comparable to the other fluxes of Fe to the Southern Ocean via dust, icebergs, and glacial runoff from the <span class="hlt">Antarctic</span> Ice Sheet, and should be considered in future geochemical budgets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19740006893','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19740006893"><span>Applicability of ERTS to <span class="hlt">Antarctic</span> iceberg resources. [harvesting sea ice for fresh <span class="hlt">water</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hult, J. L. (Principal Investigator); Ostrander, N. C.</p> <p>1973-01-01</p> <p>The author has identified the following significant results. This investigation explorers the applicability of ERTS to (1) determine the <span class="hlt">Antarctic</span> sea ice and environmental behavior that may influence the harvesting of icebergs, and (2) monitor iceberg locations, characteristics, and evolution. Imagery has shown that the potential applicability of ERTS to the research, planning, and harvesting operations can contribute importantly to the glowing promise derived from broader scope studies for the use of <span class="hlt">Antarctic</span> icebergs to relieve a growing global thirst for fresh <span class="hlt">water</span>. Several years of comprehensive monitoring will be necessary to characterize sea ice and environmental behavior and iceberg evolution. Live ERTS services will assist harvesting control and claiming operations and offer a means of harmonizing entitlements of iceberg resources. The valuable ERTS services will be more cost effective than other means will be easily justified and borne by the iceberg harvesting operations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFMPP33B1687S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFMPP33B1687S"><span>No evidence for a deglacial <span class="hlt">intermediate</span> <span class="hlt">water</span> Δ14C anomaly in the SW Atlantic</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sortor, R. N.; Lund, D. C.</p> <p>2010-12-01</p> <p>Reconstructions of Δ14C from the eastern tropical Pacific show that severe depletions in 14C occurred at <span class="hlt">intermediate</span> depths during the last deglaciation (Marchitto et al. 2007; Stott et al. 2009). Marchitto et al. (2007) suggested that old radiocarbon from an isolated abyssal reservoir was injected via the Southern Ocean, and that this anomaly was then carried by <span class="hlt">Antarctic</span> <span class="hlt">Intermediate</span> <span class="hlt">Water</span> (AAIW) to the tropical Pacific. However, a core from the southeastern Pacific Ocean near Chile, which is in the direct path of modern-day AAIW, does not exhibit the excursion and therefore casts doubts upon the AAIW mechanism (De Pol-Holz et al. 2010). Here we evaluate whether or not a deglacial 14C anomaly similar to that in the eastern tropical Pacific occurred at <span class="hlt">intermediate</span> depths in the South Atlantic. We reconstructed Δ14C using planktonic and benthic foraminifera from core KNR159-5-36GGC on the Brazil Margin (27○31’S and 46○28’W, 1268 m depth). In the modern ocean, the hydrography near this core site is heavily influenced by AAIW (Oppo & Horowitz, 2000). Benthic Δ14C values were determined using raw benthic 14C ages and calendar-calibrated planktonic ages. The deglacial benthic Δ14C trend at this site is similar to the atmospheric Δ14C trend, and is consistent with U/Th-dated corals from <span class="hlt">intermediate</span> depths on the Brazil Margin (Mangini et al. 2010). The amplitude and timing of Δ14C changes in the foraminiferal and coral records are especially congruous during the Mystery Interval. We find no evidence in the southwestern Atlantic of a ~300‰ decrease in <span class="hlt">intermediate</span> <span class="hlt">water</span> Δ14C beginning at 18 kyr BP. Changes in reservoir age of ~1000 years are required to create a Baja-like Δ14C anomaly off Brazil, an implausible increase for a subtropical gyre location. Furthermore, the resulting sedimentation rates would be up to ~145 cm/kyr during the deglaciation, an order of magnitude higher than the average sedimentation rate for 36GGC. When our results are</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.1467T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.1467T"><span>Geoethical Approach to <span class="hlt">Antarctic</span> Subglacial Lakes Exploration</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Talalay, Pavel; Markov, Alexey; Sysoev, Mikhail</p> <p>2014-05-01</p> <p><span class="hlt">Antarctic</span> subglacial aquatic environment have become of great interest to the science community because they may provide unique information about microbial evolution, the past climate of the Earth, and the formation of the <span class="hlt">Antarctic</span> ice sheet. Nowadays it is generally recognized that a vast network of lakes, rivers, and streams exists thousands of meters beneath <span class="hlt">Antarctic</span> Ice Sheets. Up to date only four boreholes accessed subglacial aquatic system but three of them were filled with high-toxic drilling fluid, and the subglacial <span class="hlt">water</span> was contaminated. Two recent exploration programs proposed by UK and USA science communities anticipated direct access down to the lakes Ellsworth and Whillans, respectively, in the 2012/2013 <span class="hlt">Antarctic</span> season. A team of British scientists and engineers engaged in the first attempt to drill into Lake Ellsworth but failed. US research team has successfully drilled through 800 m of <span class="hlt">Antarctic</span> ice to reach a subglacial lake Whillans and retrieve <span class="hlt">water</span> and sediment samples. Both activities used hot-<span class="hlt">water</span> drilling technology to access lakes. Hot <span class="hlt">water</span> is considered by the world science community as the most clean drilling fluid medium from the present point of view but it cannot solve environmental problems in total because hot-<span class="hlt">water</span> even when heated to 90 °C, filtered to 0.2 μm, and UV treated at the surface could pick up microorganisms from near-surface snow and circulate them in great volume through the borehole. Another negative impact of hot-<span class="hlt">water</span> circulation medium is thermal pollution of subglacial <span class="hlt">water</span>. The new approach to <span class="hlt">Antarctic</span> subglacial lakes exploration is presented by sampling technology with recoverable autonomous sonde which is equipped by two hot-points with heating elements located on the bottom and top sides of the sonde. All down-hole sonde components will be sterilized by combination of chemical wash, HPV and UV sterilization prior using. At the beginning of the summer season sonde is installed on the surface of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=GL-2002-002282&hterms=Antarctic+icebergs&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DAntarctic%2Bicebergs','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=GL-2002-002282&hterms=Antarctic+icebergs&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DAntarctic%2Bicebergs"><span><span class="hlt">Antarctic</span> Peninsula and Weddell Sea</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>Numerous icebergs are breaking out of the sea ice in the Southern Ocean surrounding the <span class="hlt">Antarctic</span> Peninsula. This true-color MODIS image from November 13, 2001, shows several icebergs drifting out of the Weddell Sea. The <span class="hlt">Antarctic</span> Peninsula (left) reaches out into the Drake Passage, which separates the southern tip of South America from Antarctica. Warmer temperatures have cleared a tiny patch of bare ground at the Peninsula's tip. The predominant ocean current in the area is the <span class="hlt">Antarctic</span> Circumpolar Current ('circum' meaning 'around'), which is also the 'West Wind Drift.' The current is the largest permanent current in the world, and <span class="hlt">water</span> is moved eastward by westerly winds. Icebergs leaving the Weddell Sea are likely to be moved north and east by the current. Credit: Jacques Descloitres, MODIS Land Rapid Response Team, NASA/GSFC</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28599208','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28599208"><span>Occurrence of pharmaceutical, recreational and psychotropic drug residues in surface <span class="hlt">water</span> on the northern <span class="hlt">Antarctic</span> Peninsula region.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>González-Alonso, Silvia; Merino, Luis Moreno; Esteban, Sara; López de Alda, Miren; Barceló, Damià; Durán, Juan José; López-Martínez, Jerónimo; Aceña, Jaume; Pérez, Sandra; Mastroianni, Nicola; Silva, Adrián; Catalá, Myriam; Valcárcel, Yolanda</p> <p>2017-10-01</p> <p>Human presence in the <span class="hlt">Antarctic</span> is increasing due to research activities and the rise in tourism. These activities contribute a number of potentially hazardous substances. The aim of this study is to conduct the first characterisation of the pharmaceuticals and recreational drugs present in the northern <span class="hlt">Antarctic</span> Peninsula region, and to assess the potential environmental risk they pose to the environment. The study consisted of a single sampling of ten <span class="hlt">water</span> samples from different sources, including streams, ponds, glacier drains, and a wastewater discharge into the sea. Twenty-five selected pharmaceuticals and 21 recreational drugs were analysed. The highest concentrations were found for the analgesics acetaminophen (48.74 μg L -1 ), diclofenac (15.09 μg L -1 ) and ibuprofen (10.05 μg L -1 ), and for the stimulant caffeine (71.33 μg L -1 ). All these substances were detected in <span class="hlt">waters</span> that were discharged directly into the ocean without any prior purification processes. The hazard quotient (HQ) values for ibuprofen, diclofenac and acetaminophen were far in excess of 10 at several sampling points. The concentrations of each substance measured and used as measured environmental concentration values for the HQ calculations are based on a one-time sampling. The Toxic Unit values indicate that analgesics and anti-inflammatories are the therapeutic group responsible for the highest toxic burden. This study is the first to analyse a wide range of substances and to determine the presence of pharmaceuticals and psychotropic drugs in the <span class="hlt">Antarctic</span> Peninsula region. We believe it can serve as a starting point to focus attention on the need for continued environmental monitoring of these substances in the <span class="hlt">water</span> cycle, especially in protected regions such as the <span class="hlt">Antarctic</span>. This will determine whether pharmaceuticals and recreational drugs are hazardous to the environment and, if so, can be used as the basis for risk-assessment studies to prioritise the exposure to</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_2");'>2</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li class="active"><span>4</span></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_4 --> <div id="page_5" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li class="active"><span>5</span></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="81"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JOUC...16..766X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JOUC...16..766X"><span>The evolution of <span class="hlt">water</span> property in the Mackenzie Bay polynya during <span class="hlt">Antarctic</span> winter</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xu, Zhixin; Gao, Guoping; Xu, Jianping; Shi, Maochong</p> <p>2017-10-01</p> <p>Temperature and salinity profile data, collected by southern elephant seals equipped with autonomous CTD-Satellite Relay Data Loggers (CTD-SRDLs) during the <span class="hlt">Antarctic</span> wintertime in 2011 and 2012, were used to study the evolution of <span class="hlt">water</span> property and the resultant formation of the high density <span class="hlt">water</span> in the Mackenzie Bay polynya (MBP) in front of the Amery Ice Shelf (AIS). In late March the upper 100-200 m layer is characterized by strong halocline and inversion thermocline. The mixed layer keeps deepening up to 250 m by mid-April with potential temperature remaining nearly the surface freezing point and sea surface salinity increasing from 34.00 to 34.21. From then on until mid-May, the whole <span class="hlt">water</span> column stays isothermally at about -1.90℃ while the surface salinity increases by a further 0.23. Hereafter the temperature increases while salinity decreases along with the increasing depth both by 0.1 order of magnitude vertically. The upper ocean heat content ranging from 120.5 to 2.9 MJ m-2, heat flux with the values of 9.8-287.0 W m-2 loss and the sea ice growth rates of 4.3-11.7 cm d-1 were estimated by using simple 1-D heat and salt budget methods. The MBP exists throughout the whole <span class="hlt">Antarctic</span> winter (March to October) due to the air-sea-ice interaction, with an average size of about 5.0×103 km2. It can be speculated that the decrease of the salinity of the upper ocean may occur after October each year. The recurring sea-ice production and the associated brine rejection process increase the salinity of the <span class="hlt">water</span> column in the MBP progressively, resulting in, eventually, the formation of a large body of high density <span class="hlt">water</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22031725','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22031725"><span><span class="hlt">Antarctic</span> killer whales make rapid, round-trip movements to subtropical <span class="hlt">waters</span>: evidence for physiological maintenance migrations?</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Durban, J W; Pitman, R L</p> <p>2012-04-23</p> <p>Killer whales (Orcinus orca) are important predators in high latitudes, where their ecological impact is mediated through their movements. We used satellite telemetry to provide the first evidence of migration for killer whales, characterized by fast (more than 12 km h(-1), 6.5 knots) and direct movements away from <span class="hlt">Antarctic</span> <span class="hlt">waters</span> by six of 12 type B killer whales tagged when foraging near the <span class="hlt">Antarctic</span> Peninsula, including all tags transmitting for more than three weeks. Tags on five of these whales revealed consistent movements to subtropical <span class="hlt">waters</span> (30-37° S) off Uruguay and Brazil, in surface <span class="hlt">water</span> temperatures ranging from -1.9°C to 24.2°C; one 109 day track documented a non-stop round trip of almost 9400 km (5075 nmi) in just 42 days. Although whales travelled slower in the warmest <span class="hlt">waters</span>, there was no obvious interruption in swim speed or direction to indicate calving or prolonged feeding. Furthermore, these movements were aseasonal, initiating over 80 days between February and April; one whale returned to within 40 km of the tagging site at the onset of the austral winter in June. We suggest that these movements may represent periodic maintenance migrations, with warmer <span class="hlt">waters</span> allowing skin regeneration without the high cost of heat loss: a physiological constraint that may also affect other whales.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=Hydrology&pg=5&id=ED152502','ERIC'); return false;" href="https://eric.ed.gov/?q=Hydrology&pg=5&id=ED152502"><span>NTTC Course 215: <span class="hlt">Intermediate</span> <span class="hlt">Water</span> Examination.</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>Department of the Navy, Washington, DC.</p> <p></p> <p>This publication is the examination booklet used for a home study course in <span class="hlt">water</span> treatment. This course is the <span class="hlt">intermediate</span> part of a series produced by the Department of the Navy. This publication is designed to be used in conjunction with a textbook. Each of the two examinations contained in this document are referenced to a section of the…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMPP42B..02R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMPP42B..02R"><span>Development of a Regional Glycerol Dialkyl Glycerol Tetraether (GDGT) - Temperature Calibration for <span class="hlt">Antarctic</span> and sub-<span class="hlt">Antarctic</span> Lakes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Roberts, S. J.; Foster, L. C.; Pearson, E. J.; Steve, J.; Hodgson, D.; Saunders, K. M.; Verleyen, E.</p> <p>2016-12-01</p> <p>Temperature calibration models based on the relative abundances of sedimentary glycerol dialkyl glycerol tetraethers (GDGTs) have been used to reconstruct past temperatures in both marine and terrestrial environments, but have not been widely applied in high latitude environments. This is mainly because the performance of GDGT-temperature calibrations at lower temperatures and GDGT provenance in many lacustrine settings remains uncertain. To address these issues, we examined surface sediments from 32 <span class="hlt">Antarctic</span>, sub-<span class="hlt">Antarctic</span> and Southern Chilean lakes. First, we quantified GDGT compositions present and then investigated modern-day environmental controls on GDGT composition. GDGTs were found in all 32 lakes studied. Branched GDGTs (brGDGTs) were dominant in 31 lakes and statistical analyses showed that their composition was strongly correlated with mean summer air temperature (MSAT) rather than pH, conductivity or <span class="hlt">water</span> depth. Second, we developed the first regional brGDGT-temperature calibration for <span class="hlt">Antarctic</span> and sub-<span class="hlt">Antarctic</span> lakes based on four brGDGT compounds (GDGT-Ib, GDGT-II, GDGT-III and GDGT-IIIb). Of these, GDGT-IIIb proved particularly important in cold lacustrine environments. Our brGDGT-<span class="hlt">Antarctic</span> temperature calibration dataset has an improved statistical performance at low temperatures compared to previous global calibrations (r2=0.83, RMSE=1.45°C, RMSEP-LOO=1.68°C, n=36 samples), highlighting the importance of basing palaeotemperature reconstructions on regional GDGT-temperature calibrations, especially if specific compounds lead to improved model performance. Finally, we applied the new <span class="hlt">Antarctic</span> brGDGT-temperature calibration to two key lake records from the <span class="hlt">Antarctic</span> Peninsula and South Georgia. In both, downcore temperature reconstructions show similarities to known Holocene warm periods, providing proof of concept for the new <span class="hlt">Antarctic</span> calibration model.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004DSRII..51.1551M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004DSRII..51.1551M"><span>Russian deep-sea investigations of <span class="hlt">Antarctic</span> fauna</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Malyutina, Marina</p> <p>2004-07-01</p> <p>A review of the Russian deep-sea investigation of <span class="hlt">Antarctic</span> fauna beginning from the first scientific collection of Soviet whaling fleet expeditions 1946-1952 is presented. The paper deals with the following expeditions, their main tasks and results. These expeditions include three cruises of research vessel (R.V.) Ob in the Indian sector of the <span class="hlt">Antarctic</span> and in the Southern Pacific (1955-1958); 11 cruises of the R.V. Akademik Kurchatov in the southern Atlantic (November-December 1971); 16 cruises of the R.V. Dmitriy Mendeleev in the Australia-New Zealand area and adjacent <span class="hlt">water</span> of the <span class="hlt">Antarctic</span> (December 1975-March 1976); 43 cruises of the R.V. Akademik Kurchatov in the southern Atlantic (October 1985-February 1986); and 43 cruises of the R.V. Dmitriy Mendeleev in the Atlantic sector of the South Ocean (January-May 1989). A list of the main publications on the benthic taxa collected during these expeditions with data of their distribution is presented. The results of Russian explorations of the <span class="hlt">Antarctic</span> fauna are presented as theoretical conclusions in the following topics: (1) Vertical zonation in the distribution of the <span class="hlt">Antarctic</span> deep-sea fauna; (2) Biogeographic division of the abyssal and hadal zones; (3) Origin of the <span class="hlt">Antarctic</span> deep-sea fauna; (4) Distributional pathways of the <span class="hlt">Antarctic</span> abyssal fauna through the World Ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/18765160','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/18765160"><span>Environmental contamination in <span class="hlt">Antarctic</span> ecosystems.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bargagli, R</p> <p>2008-08-01</p> <p>Although the remote continent of Antarctica is perceived as the symbol of the last great wilderness, the human presence in the Southern Ocean and the continent began in the early 1900s for hunting, fishing and exploration, and many invasive plant and animal species have been deliberately introduced in several sub-<span class="hlt">Antarctic</span> islands. Over the last 50 years, the development of research and tourism have locally affected terrestrial and marine coastal ecosystems through fuel combustion (for transportation and energy production), accidental oil spills, waste incineration and sewage. Although natural "barriers" such as oceanic and atmospheric circulation protect Antarctica from lower latitude <span class="hlt">water</span> and air masses, available data on concentrations of metals, pesticides and other persistent pollutants in air, snow, mosses, lichens and marine organisms show that most persistent contaminants in the <span class="hlt">Antarctic</span> environment are transported from other continents in the Southern Hemisphere. At present, levels of most contaminants in <span class="hlt">Antarctic</span> organisms are lower than those in related species from other remote regions, except for the natural accumulation of Cd and Hg in several marine organisms and especially in albatrosses and petrels. The concentrations of organic pollutants in the eggs of an opportunistic top predator such as the south polar skua are close to those that may cause adverse health effects. Population growth and industrial development in several countries of the Southern Hemisphere are changing the global pattern of persistent anthropogenic contaminants and new classes of chemicals have already been detected in the <span class="hlt">Antarctic</span> environment. Although the Protocol on Environmental Protection to the <span class="hlt">Antarctic</span> Treaty provides strict guidelines for the protection of the <span class="hlt">Antarctic</span> environment and establishes obligations for all human activity in the continent and the Southern Ocean, global warming, population growth and industrial development in countries of the Southern</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4856368','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4856368"><span>Underwater Optics in Sub-<span class="hlt">Antarctic</span> and <span class="hlt">Antarctic</span> Coastal Ecosystems</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Huovinen, Pirjo; Ramírez, Jaime; Gómez, Iván</p> <p>2016-01-01</p> <p>Understanding underwater optics in natural <span class="hlt">waters</span> is essential in evaluating aquatic primary production and risk of UV exposure in aquatic habitats. Changing environmental conditions related with global climate change, which imply potential contrasting changes in underwater light climate further emphasize the need to gain insights into patterns related with underwater optics for more accurate future predictions. The present study evaluated penetration of solar radiation in six sub-<span class="hlt">Antarctic</span> estuaries and fjords in Chilean North Patagonian region (39–44°S) and in an <span class="hlt">Antarctic</span> bay (62°S). Based on vertical diffuse attenuation coefficients (Kd), derived from measurements with a submersible multichannel radiometer, average summer UV penetration depth (z1%) in these <span class="hlt">water</span> bodies ranged 2–11 m for UV-B (313 nm), 4–27 m for UV-A (395 nm), and 7–30 m for PAR (euphotic zone). UV attenuation was strongest in the shallow Quempillén estuary, while Fildes Bay (Antarctica) exhibited the highest transparency. Optically non-homogeneous <span class="hlt">water</span> layers and seasonal variation in transparency (lower in winter) characterized Comau Fjord and Puyuhuapi Channel. In general, multivariate analysis based on Kd values of UV and PAR wavelengths discriminated strongly Quempillén estuary and Puyuhuapi Channel from other study sites. Spatial (horizontal) variation within the estuary of Valdivia river reflected stronger attenuation in zones receiving river impact, while within Fildes Bay a lower spatial variation in <span class="hlt">water</span> transparency could in general be related to closeness of glaciers, likely due to increased turbidity through ice-driven processes. Higher transparency and deeper UV-B penetration in proportion to UV-A/visible wavelengths observed in Fildes Bay suggests a higher risk for <span class="hlt">Antarctic</span> ecosystems reflected by e.g. altered UV-B damage vs. photorepair under UV-A/PAR. Considering that damage repair processes often slow down under cool temperatures, adverse UV impact could be</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 Oceanic <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 <span class="hlt">Antarctic</span> <span class="hlt">Intermediate</span> <span class="hlt">Waters</span>, are diverted to the south of New Zealand by the submerged continental landmass of Zealandia. In the upper ocean 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 oceanic 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 oceanic <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 <span class="hlt">Antarctic</span> <span class="hlt">Intermediate</span> <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://ntrs.nasa.gov/search.jsp?R=20040120030&hterms=virus&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dvirus','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040120030&hterms=virus&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dvirus"><span>Viruses in <span class="hlt">Antarctic</span> lakes</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kepner, R. L. Jr; Wharton, R. A. Jr; Suttle, C. A.; Wharton RA, J. r. (Principal Investigator)</p> <p>1998-01-01</p> <p><span class="hlt">Water</span> samples collected from four perennially ice-covered <span class="hlt">Antarctic</span> lakes during the austral summer of 1996-1997 contained high densities of extracellular viruses. Many of these viruses were found to be morphologically similar to double-stranded DNA viruses that are known to infect algae and protozoa. These constitute the first observations of viruses in perennially ice-covered polar lakes. The abundance of planktonic viruses and data suggesting substantial production potential (relative to bacteria] secondary and photosynthetic primary production) indicate that viral lysis may be a major factor in the regulation of microbial populations in these extreme environments. Furthermore, we suggest that <span class="hlt">Antarctic</span> lakes may be a reservoir of previously undescribed viruses that possess novel biological and biochemical characteristics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.6507L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.6507L"><span>The Microphysics of <span class="hlt">Antarctic</span> Clouds - Part one Observations.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lachlan-Cope, Tom; Listowski, Constantino; O'Shea, Sebastian; Bower, Keith</p> <p>2016-04-01</p> <p>During the <span class="hlt">Antarctic</span> summer of 2010 and 2011 in-situ measurements of clouds were made over the <span class="hlt">Antarctic</span> Peninsula and in 2015 similar measurements were made over the eastern Weddell Sea using the British <span class="hlt">Antarctic</span> Surveys instrumented Twin Otter aircraft. This paper contrasts the clouds found on either side of the <span class="hlt">Antarctic</span> Peninsula with the clouds over the eastern Weddell Sea, paying particular attention to the total number of ice and <span class="hlt">water</span> particles found in the clouds. The differences found between the clouds are considered in relation to the sources of cloud condensation nuclei and ice nuclei that are expected to be active in the different cases. In particular it was found that the number of ice nuclei was very low over the Weddell Sea when compared to other regions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/6462703','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/6462703"><span>The <span class="hlt">Antarctic</span> cryptoendolithic ecosystem: relevance to exobiology.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Friedmann, E I; Ocampo-Friedmann, R</p> <p>1984-01-01</p> <p>Cryptoendolithic microorganisms in the <span class="hlt">Antarctic</span> desert live inside porous sandstone rocks, protected by a thin rock crust. While the rock surface is abiotic, the microclimate inside the rock is comparatively mild. These organisms may have descended from early, pre-glaciation <span class="hlt">Antarctic</span> life forms and thus may represent the last outpost of life in a gradually deteriorating environment. Assuming that life once arose on Mars, it is conceivable that, following the loss of <span class="hlt">water</span>, the last of surviving organisms withdrew to similar insulated microenvironments. Because such microscopic pockets have little connection with the outside environment, their detection may be difficult. The chances that the Viking lander could sample cryptoendolithic microorganisms in the <span class="hlt">Antarctic</span> desert would be infinitesimal.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19840057725&hterms=microclimate&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dmicroclimate','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19840057725&hterms=microclimate&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dmicroclimate"><span>The <span class="hlt">Antarctic</span> cryptoendolithic ecosystem - Relevance to exobiology</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Friedmann, E. I.; Ocampo-Friedmann, R.</p> <p>1984-01-01</p> <p>Cryptoendolithic microorganisms in the <span class="hlt">Antarctic</span> desert live inside porous sandstone rocks, protected by a thin rock crust. While the rock surface is abiotic, the microclimate inside the rock is comparatively mild. These organisms may have descended from early, pre-glaciation <span class="hlt">Antarctic</span> life forms and thus may represent the last outpost of life in a gradually deteriorating environment. Assuming that life once arose on Mars, it is conceivable that, following the loss of <span class="hlt">water</span>, the last of surviving organisms withdrew to similar insulated microenvironments. Because such microscopic pockets have little connection with the outside environment, their detection may be difficult. The chances that the Viking lander could sample cryptoendolithic microorganisms in the <span class="hlt">Antarctic</span> desert would be infinitesimal.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29904115','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29904115"><span>Toxic anthropogenic signature in <span class="hlt">Antarctic</span> continental shelf and deep sea sediments.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Isla, Enrique; Pérez-Albaladejo, Elisabet; Porte, Cinta</p> <p>2018-06-14</p> <p>Industrial activity generates harmful substances which can travel via aerial or <span class="hlt">water</span> currents thousands of kilometers away from the place they were used impacting the local biota where they deposit. The presence of harmful anthropogenic substances in the <span class="hlt">Antarctic</span> is particularly surprising and striking due to its remoteness and the apparent geophysical isolation developed with the flows of the <span class="hlt">Antarctic</span> Circumpolar current and the ring of westerly winds surrounding the continent. However, long-range atmospheric transport (LRAT) of pollutants has been detected in the <span class="hlt">Antarctic</span> since the 70's along the <span class="hlt">Antarctic</span> trophic food web from phytoplankton to birds. Still, no information exists on the presence of cytotoxic compounds in marine sediments neither at basin scales (thousands of kilometers) nor in <span class="hlt">water</span> depths (hundreds of meters) beyond shallow coastal areas near research stations. Our results showed for the first time that there is cytotoxic activity in marine sediment extracts from <span class="hlt">water</span> depths >1000 m and along thousands of kilometers of <span class="hlt">Antarctic</span> continental shelf, in some cases comparable to that observed in Mediterranean areas. Ongoing anthropogenic pressure appears as a serious threat to the sessile benthic communities, which have evolved in near isolation for millions of years in these environments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA241701','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA241701"><span><span class="hlt">Antarctic</span> Treaty 1991: A U.S. Position</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1990-12-01</p> <p>Hult and N. C. Ostrander, <span class="hlt">Antarctic</span> Icebergs As A Global Fresh <span class="hlt">Water</span> Resource, R-1255-NSF (Santa Monica, California: The Rand Corporation, 1973), p. iii...Law: Cases and Materials, 2nd ed. St. Paul, Minnesota: West Publishing Co. 1987. Hult , J. L. and N. C. Ostrander. <span class="hlt">Antarctic</span> Iceberas As A Global Fresh...Unknown: The International Geophysical Year (New York: McGraw- Hill Company, Inc., 1961), p. 4. 6 of England, one of the world’s leading geophysicists</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016E%26PSL.453..243Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016E%26PSL.453..243Z"><span><span class="hlt">Antarctic</span> link with East Asian summer monsoon variability during the Heinrich Stadial-Bølling interstadial transition</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, Hongbin; Griffiths, Michael L.; Huang, Junhua; Cai, Yanjun; Wang, Canfa; Zhang, Fan; Cheng, Hai; Ning, Youfeng; Hu, Chaoyong; Xie, Shucheng</p> <p>2016-11-01</p> <p> southern extent of the SH westerlies. Moreover, increased meltwater flux during IRD events would have freshened <span class="hlt">Antarctic</span> <span class="hlt">Intermediate</span> <span class="hlt">Water</span>, leading to the increased formation of North Atlantic Deep <span class="hlt">Water</span> and enhanced North Atlantic subsurface heat release, and causing a strengthening of the AMOC during the HS1-Bølling transition. The result of this sequence-of-events would have been warming in the North Atlantic whilst at the same time cooling in the <span class="hlt">Antarctic</span>. The ensuing interhemispheric temperature gradient would have acted to push the ITCZ northward, weakening the Australian-Indonesian summer monsoon (AISM) whilst intensifying the EASM.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011DSRII..58.2293H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011DSRII..58.2293H"><span>Distribution, abundance and seasonal flux of pteropods in the Sub-<span class="hlt">Antarctic</span> Zone</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Howard, W. R.; Roberts, D.; Moy, A. D.; Lindsay, M. C. M.; Hopcroft, R. R.; Trull, T. W.; Bray, S. G.</p> <p>2011-11-01</p> <p>Pteropods were identified from epipelagic net and trawl samples in the Sub-<span class="hlt">Antarctic</span> Zone during the 2007 mid-summer (January 17-February 20) Sub-<span class="hlt">Antarctic</span> Zone Sensitivity to Environmental Change (SAZ-Sense) voyage, as well as in a moored sediment trap in the same region. Overall pteropod densities during SAZ-Sense were lower than those reported for higher-latitude Southern Ocean <span class="hlt">waters</span>. The four major contributors to the Sub-<span class="hlt">Antarctic</span> Zone pteropod community during the SAZ-Sense voyage, Clio pyramidata forma antarctica, Clio recurva, Limacina helicina antarctica and Limacina retroversa australis, accounted for 93% of all pteropods observed. The distribution of the two dominant pteropods collected in the Sub-<span class="hlt">Antarctic</span> Zone, L. retroversa australis and C. pyramidata forma antarctica, is strongly related to latitude and depth. L. retroversa australis is typical of cold southern (50-54°S) polar <span class="hlt">waters</span> and C. pyramidata forma antarctica is typical of shallow (top 20 m) Sub-<span class="hlt">Antarctic</span> Zone <span class="hlt">waters</span>. A moored sediment trap deployed to 2100 m at 47°S, 141°E in 2003/04 showed the pteropod flux in the Sub-<span class="hlt">Antarctic</span> Zone had late-Spring and mid-summer peaks. The diversity, abundance and distribution of pteropods collected during SAZ-Sense provide a timely benchmark against which to monitor future changes in SAZ ocean pteropod communities, particularly in light of predictions of declining aragonite saturation in the Southern Ocean by the end of the century.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19860041743&hterms=population+characteristic&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dpopulation%2Bcharacteristic*','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19860041743&hterms=population+characteristic&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dpopulation%2Bcharacteristic*"><span><span class="hlt">Antarctic</span> and non-<span class="hlt">Antarctic</span> meteorites form different populations</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Dennison, J. E.; Lingner, D. W.; Lipschutz, M. E.</p> <p>1986-01-01</p> <p>The trace element differences between Victoria Land H5 chondrites and non-<span class="hlt">Antarctic</span> H5 chondrites are studied. The focus on common meteorites was stimulated by <span class="hlt">Antarctic</span> and non-<span class="hlt">Antarctic</span> differences in meteorite types and in the trace element contents of congeners of rare type. Thirteen elements were analyzed by neutron activation analysis with radiochemical separation, and eight differed significantly. Eliminating test biasing and the possibility of compositional difference due to <span class="hlt">Antarctic</span> weathering of the 300,000 year-old (on the average) Victoria Land falls, it is concluded that the two sets of chondrites differ due to extraterrestrial causes. The three possibilities discussed, differences in sample population, physical properties, orbital characteristics, and meteoroid flux with time, are all seen as problematic.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://pubs.water.usgs.gov/wri984091','USGSPUBS'); return false;" href="http://pubs.water.usgs.gov/wri984091"><span>Transmissivity and <span class="hlt">water</span> quality of <span class="hlt">water</span>-producing zones in the <span class="hlt">intermediate</span> aquifer system, Sarasota County, Florida</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Knochenmus, L.A.; Bowman, Geronia</p> <p>1998-01-01</p> <p>The <span class="hlt">intermediate</span> aquifer system is an important <span class="hlt">water</span> source in Sarasota County, Florida, because the quality of <span class="hlt">water</span> in it is usually better than that in the underlying Upper Floridan aquifer. The <span class="hlt">intermediate</span> aquifer system consists of a group of up to three <span class="hlt">water</span>-producing zones separated by less-permeable units that restrict the vertical movement of ground <span class="hlt">water</span> between zones. The diverse lithology, that makes up the <span class="hlt">intermediate</span> aquifer system, reflects the variety of depositional environments that occurred during the late Oligocene and Miocene epochs. Slight changes in the depositional environment resulted in aquifer heterogeneity, creating both localized connection between <span class="hlt">water</span>-producing zones and abrupt culmination of <span class="hlt">water</span>-producing zones that are not well documented. Aquifer heterogeneity results in vertical and areal variability in hydraulic and <span class="hlt">water</span>-quality properties. The uppermost <span class="hlt">water</span>-producing zone is designated producing zone 1 but is not extensively used because of its limited production capability and limited areal extent. The second <span class="hlt">water</span>-producing zone is designated producing zone 2, and most of the domestic- and irrigation-supply wells in the area are open to this zone. Additionally, producing zone 2 is utilized for public supply in southern coastal areas of Sarasota County. Producing zone 3 is the lowermost and most productive <span class="hlt">water</span>-producing zone in the <span class="hlt">intermediate</span> aquifer system. Public-supply well fields serving the cities of Sarasota and Venice, as well as the Plantation and Mabry Carlton Reserve well fields, utilize producing zone 3. Heads within the <span class="hlt">intermediate</span> aquifer system generally increase with aquifer depth. However, localized head-gradient reversals occur in the study area, coinciding with sites of intense ground-<span class="hlt">water</span> withdrawals. Heads in producing zones 1, 2, and 3 range from 1 to 23, 0.2 to 34, and 7 to 42 feet above sea level, respectively. Generally, an upward head gradient exists between producing zones 3 and 2</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28785171','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28785171"><span>Revision of Eocene <span class="hlt">Antarctic</span> carpet sharks (Elasmobranchii, Orectolobiformes) from Seymour Island, <span class="hlt">Antarctic</span> Peninsula.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Engelbrecht, Andrea; Mörs, Thomas; Reguero, Marcelo A; Kriwet, Jürgen</p> <p>2017-01-01</p> <p>Seymour Island, <span class="hlt">Antarctic</span> Peninsula, was once called the 'Rosetta Stone' of Southern Hemisphere palaeobiology, because this small island provides the most complete and richly fossiliferous Palaeogene sequence in Antarctica. Among fossil marine vertebrate remains, chondrichthyans seemingly were dominant elements in the Eocene <span class="hlt">Antarctic</span> fish fauna. The fossiliferous sediments on Seymour Island are from the La Meseta Formation, which was originally divided into seven stratigraphical levels, TELMs 1-7 (acronym for Tertiary Eocene La Meseta) ranging from the upper Ypresian (early Eocene) to the late Priabonian (late Eocene). Bulk sampling of unconsolidated sediments from TELMs 5 and 6, which are Ypresian (early Eocene) and Lutetian (middle Eocene) in age, respectively, yielded very rich and diverse chondrichthyan assemblages including over 40 teeth of carpet sharks representing two new taxa, Notoramphoscyllium woodwardi gen. et sp. nov. and Ceolometlaouia pannucae gen. et sp. nov. Two additional teeth from TELM 5 represent two different taxa that cannot be assigned to any specific taxon and thus are left in open nomenclature. The new material not only increases the diversity of Eocene <span class="hlt">Antarctic</span> selachian faunas but also allows two previous orectolobiform records to be re-evaluated. Accordingly, Stegostoma cf. faciatum is synonymized with Notoramphoscyllium woodwardi gen. et sp. nov., whereas Pseudoginglymostoma cf. brevicaudatum represents a nomen dubium . The two new taxa, and probably the additional two unidentified taxa, are interpreted as permanent residents, which most likely were endemic to <span class="hlt">Antarctic</span> <span class="hlt">waters</span> during the Eocene and adapted to shallow and estuarine environments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMOS11A1999C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMOS11A1999C"><span>The tug-of-war between the West Philippine Sea and South China Sea Tropical <span class="hlt">Waters</span> and <span class="hlt">Intermediate</span> <span class="hlt">Waters</span> in the Okinawa Trough</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, C. T. A.</p> <p>2015-12-01</p> <p>It has been known that Kuroshio subsurface <span class="hlt">waters</span> are the major source of nutrients to the East China Sea continental shelf, a major fishing ground. It has also been known that subsurface <span class="hlt">waters</span> that upwell onto the shelf are heavily affected by the South China Sea (SCS) Tropical <span class="hlt">Water</span> and the SCS <span class="hlt">Intermediate</span> <span class="hlt">Water</span> which contain more nutrients than the tropical (Smax) and <span class="hlt">intermediate</span> (Smin) <span class="hlt">waters</span> from the West Philippine Sea (WPS). A front has been found to separate the tropical and <span class="hlt">intermediate</span> <span class="hlt">waters</span> from the SCS and WPS. The reported front in the Okinawa Trough, however, was identified based only on one-time data from a single cross-section in the central Okinawa Trough. Here historical hydrographic data between Mar. 1950 and Dec. 2011 in the Okinawa Trough and its neighborhood are analyzed. A vertical front tilted toward the west is found in all seasons in all years across the World Ocean Circulation Repeated Lines PR 18 and 19 as well as at the PN cross-section in the central Okinawa Trough. The front at the Smax level (sigma theta=24.6-24.9) shows large seasonal and interannual variations. In winter during normal and La Niña periods the presence of the SCS Tropical <span class="hlt">Water</span> is the most prominent. It is the weakest in autumn during normal periods and in spring during La Nina periods. Yet during El Niño periods the SCS Tropical <span class="hlt">Water</span> is the most prominent in spring and it becomes the weakest in winter. As for <span class="hlt">intermediate</span> <span class="hlt">waters</span> (Smin at sigma theta= 26.7-26.9) the WPS <span class="hlt">Intermediate</span> <span class="hlt">Water</span> and SCS <span class="hlt">Intermediate</span> <span class="hlt">Water</span> show much weaker seasonality compared with tropical <span class="hlt">waters</span> although during normal periods in winter the WPS <span class="hlt">Intermediate</span> <span class="hlt">Water</span> contribution is slightly larger than during other times. During El Niño periods the WPS <span class="hlt">Intermediate</span> <span class="hlt">Water</span> contribution is the smallest but in spring it is much strengthened. On the other hand, the WPS <span class="hlt">Intermediate</span> <span class="hlt">Water</span> contribution is the smallest in spring, and the largest in winter during La Niña periods.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li class="active"><span>5</span></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_5 --> <div id="page_6" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li class="active"><span>6</span></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="101"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20010015246&hterms=temperature+variability&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dtemperature%2Bvariability','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20010015246&hterms=temperature+variability&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dtemperature%2Bvariability"><span>Satellite Observed Variability in <span class="hlt">Antarctic</span> and Arctic Surface Temperatures and Their Correlation to Open <span class="hlt">Water</span> Areas</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Comiso, Josefino C.; Zukor, Dorothy (Technical Monitor)</p> <p>2000-01-01</p> <p>Recent studies using meterological station data have indicated that global surface air temperature has been increasing at a rate of 0.05 K/decade. Using the same set of data but for stations in the <span class="hlt">Antarctic</span> and Arctic regions (>50 N) only, the increases in temperature were 0.08, and 0.22 K/decade, when record lengths of 100 and 50 years, respectively, were used. To gain insights into the increasing rate of warming, satellite infrared and passive microwave observations over the Arctic region during the last 20 years were processed and analyzed. The results show that during this period, the ice extent in the <span class="hlt">Antarctic</span> has been increasing at the rate of 1.2% per decade while the surface temperature has been decreasing at about 0.08 K per decade. Conversely, in the Northern Hemisphere, the ice extent has been decreasing at a rate of 2.8% per decade, while the surface temperatures have been increasing at the rate of 0.38 K per decade. In the <span class="hlt">Antarctic</span>, it is surprising that there is a short term trend of cooling during a global period of warming. Very large anomalies in open <span class="hlt">water</span> areas in the Arctic were observed especially in the western region, that includes the Beaufort Sea, where the observed open <span class="hlt">water</span> area was about 1x10(exp 6) sq km, about twice the average for the region, during the summer of 1998. In the eastern region, that includes the Laptev Sea, the area of open <span class="hlt">water</span> was also abnormally large in the summer of 1995. Note that globally, the warmest and second warmest years in this century, were 1998 and 1995, respectively. The data, however, show large spatial variability with the open <span class="hlt">water</span> area distribution showing a cyclic periodicity of about ten years, which is akin to the North Atlantic and Arctic Oscillations. This was observed in both western and eastern regions but with the phase of one lagging the other by about two years. This makes it difficult to interpret what the trends really mean. But although the record length of satellite data is still</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24353207','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24353207"><span>Surviving in a frozen desert: environmental stress physiology of terrestrial <span class="hlt">Antarctic</span> arthropods.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Teets, Nicholas M; Denlinger, David L</p> <p>2014-01-01</p> <p>Abiotic stress is one of the primary constraints limiting the range and success of arthropods, and nowhere is this more apparent than Antarctica. <span class="hlt">Antarctic</span> arthropods have evolved a suite of adaptations to cope with extremes in temperature and <span class="hlt">water</span> availability. Here, we review the current state of knowledge regarding the environmental physiology of terrestrial arthropods in Antarctica. To survive low temperatures, mites and Collembola are freeze-intolerant and rely on deep supercooling, in some cases supercooling below -30°C. Also, some of these microarthropods are capable of cryoprotective dehydration to extend their supercooling capacity and reduce the risk of freezing. In contrast, the two best-studied <span class="hlt">Antarctic</span> insects, the midges Belgica antarctica and Eretmoptera murphyi, are freeze-tolerant year-round and rely on both seasonal and rapid cold-hardening to cope with decreases in temperature. A common theme among <span class="hlt">Antarctic</span> arthropods is extreme tolerance of dehydration; some accomplish this by cuticular mechanisms to minimize <span class="hlt">water</span> loss across their cuticle, while a majority have highly permeable cuticles but tolerate upwards of 50-70% loss of body <span class="hlt">water</span>. Molecular studies of <span class="hlt">Antarctic</span> arthropod stress physiology are still in their infancy, but several recent studies are beginning to shed light on the underlying mechanisms that govern extreme stress tolerance. Some common themes that are emerging include the importance of cuticular and cytoskeletal rearrangements, heat shock proteins, metabolic restructuring and cell recycling pathways as key mediators of cold and <span class="hlt">water</span> stress in the <span class="hlt">Antarctic</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23934251','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23934251"><span>Rhodotorula portillonensis sp. nov., a basidiomycetous yeast isolated from <span class="hlt">Antarctic</span> shallow-<span class="hlt">water</span> marine sediment.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Laich, Federico; Vaca, Inmaculada; Chávez, Renato</p> <p>2013-10-01</p> <p>During the characterization of the mycobiota associated with shallow-<span class="hlt">water</span> marine environments from <span class="hlt">Antarctic</span> sea, a novel pink yeast species was isolated. Sequence analysis of the D1/D2 domain of the LSU rDNA gene and 5.8S-ITS regions revealed that the isolated yeast was closely related to Rhodotorula pallida CBS 320(T) and Rhodotorula benthica CBS 9124(T). On the basis of morphological, biochemical and physiological characterization and phylogenetic analyses, a novel basidiomycetous yeast species, Rhodotorula portillonensis sp. nov., is proposed. The type strain is Pi2(T) ( = CBS 12733(T)  = CECT 13081(T)) which was isolated from shallow-<span class="hlt">water</span> marine sediment in Fildes Bay, King George Island, Antarctica.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/12020648','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/12020648"><span>Drinking behaviour and <span class="hlt">water</span> turnover rates of <span class="hlt">Antarctic</span> fur seal pups: implications for the estimation of milk intake by isotopic dilution.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lea, Mary-Anne; Bonadonna, Francesco; Hindell, Mark A; Guinet, Christophe; Goldsworthy, Simon D</p> <p>2002-06-01</p> <p>The estimation of milk consumption in free-ranging seals using tritium dilution techniques makes the key assumption that the animals drink no pre-formed <span class="hlt">water</span> during the experimental period. However, frequent observations of unweaned <span class="hlt">Antarctic</span> fur seal pups drinking <span class="hlt">water</span> at Iles Kerguelen necessitated the testing of this assumption. We estimated <span class="hlt">water</span> flux rates of 30 pups (10.7+/-0.3 kg) in four experimental groups by isotopic dilution over 4 days. The groups were: (1) pups held in an open air enclosure without access to <span class="hlt">water</span> to estimate fasting metabolic <span class="hlt">water</span> production (MWP); (2) free-ranging pups not administered additional <span class="hlt">water</span>; (3) pups held in an open air enclosure and given a total of 300 ml of fresh <span class="hlt">water</span> to verify technique accuracy; and (4) free-ranging pups given 200 ml of fresh <span class="hlt">water</span>. Pups without access to <span class="hlt">water</span> exhibited <span class="hlt">water</span> flux rates (20.5+/-0.8 ml kg(-1)d(-1)), which were significantly lower than those observed for the free-ranging group (33.0+/-1.7 ml kg(-1) d(-1)). Mean estimated pre-formed <span class="hlt">water</span> intake for the free-ranging experimental groups was 12.6 ml kg(-1) d(-1). Thus, MWP, measured as total <span class="hlt">water</span> intake during fasting, may be significantly over-estimated in free-ranging <span class="hlt">Antarctic</span> fur seal pups at Iles Kerguelen and at other sites and subsequently milk intake rates may be underestimated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1987DSRA...34.1745F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1987DSRA...34.1745F"><span>The path of the Levantine <span class="hlt">intermediate</span> <span class="hlt">water</span> to the Alboran sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Font, Jordi</p> <p>1987-10-01</p> <p>The Levantine <span class="hlt">Intermediate</span> <span class="hlt">Water</span> (LIW) traditionally has been assumed to reach the Alboran Sea as a counter-current along the North African coast. Here data are presented that confirm the LIW flow through the sill that separates the Balearic Islands from the mainland, after contouring cyclonically the western Mediterranean along the continental slope. This seems to be a seasonal phenomenon related to the process of deep <span class="hlt">water</span> formation in the northwestern Mediterranean and to fluctuations in the Ligurian Current. In winter the LIW can circulate across the Catalan Sea without remarkable dilution, while in summer the <span class="hlt">intermediate</span> outflow has almost lost the LIW <span class="hlt">water</span> mass characteristics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24782842','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24782842"><span>Microbial ecology and biogeochemistry of continental <span class="hlt">Antarctic</span> soils.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Cowan, Don A; Makhalanyane, Thulani P; Dennis, Paul G; Hopkins, David W</p> <p>2014-01-01</p> <p>The Antarctica Dry Valleys are regarded as the coldest hyperarid desert system on Earth. While a wide variety of environmental stressors including very low minimum temperatures, frequent freeze-thaw cycles and low <span class="hlt">water</span> availability impose severe limitations to life, suitable niches for abundant microbial colonization exist. <span class="hlt">Antarctic</span> desert soils contain much higher levels of microbial diversity than previously thought. Edaphic niches, including cryptic and refuge habitats, microbial mats and permafrost soils all harbor microbial communities which drive key biogeochemical cycling processes. For example, lithobionts (hypoliths and endoliths) possess a genetic capacity for nitrogen and carbon cycling, polymer degradation, and other system processes. Nitrogen fixation rates of hypoliths, as assessed through acetylene reduction assays, suggest that these communities are a significant input source for nitrogen into these oligotrophic soils. Here we review aspects of microbial diversity in <span class="hlt">Antarctic</span> soils with an emphasis on functionality and capacity. We assess current knowledge regarding adaptations to <span class="hlt">Antarctic</span> soil environments and highlight the current threats to <span class="hlt">Antarctic</span> desert soil communities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1994HM.....48...79M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1994HM.....48...79M"><span>Leucon parasiphonatus, a new species (Crustacea: Cumacea: Leuconidae) from <span class="hlt">Antarctic</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>Mühlenhardt-Siegel, U.</p> <p>1994-03-01</p> <p>Six specimens of Leucon parasiphonatus n. sp. were collected at depths ranging from 15 to 424 m in the vicinity of King George Island (South Shetland Islands, Antarctica) and the south eastern Weddell Sea. Leucon parasiphonatus belongs to the subgenus Leucon and differs from the other already known <span class="hlt">antarctic</span> and Subantarctic species of the genus, in the absence of a serrated dorsomedian line and in the presence of a long pseudorostrum with several fine setae at its tip, surrounding the very long branchial siphon. The surface of the carapace is granulated; the carapace displays no teeth except for a few at its antero-lateral margin and at its ventral margin. The species most similar to Leucon parasiphonatus is Leucon siphonatus, reported from Mediterranean and North Atlantic <span class="hlt">waters</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP43B1345K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP43B1345K"><span><span class="hlt">Antarctic</span> Circumpolar Current Dynamics and Their Relation to <span class="hlt">Antarctic</span> Ice Sheet and Perennial Sea-Ice Variability in the Central Drake Passage During the Last Climate Cycle</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kuhn, G.; Wu, S.; Hass, H. C.; Klages, J. P.; Zheng, X.; Arz, H. W.; Esper, O.; Hillenbrand, C. D.; Lange, C.; Lamy, F.; Lohmann, G.; Müller, J.; McCave, I. N. N.; Nürnberg, D.; Roberts, J.; Tiedemann, R.; Timmermann, A.; Titschack, J.; Zhang, X.</p> <p>2017-12-01</p> <p>The evolution of the <span class="hlt">Antarctic</span> Ice Sheet during the last climate cycle and the interrelation to global atmospheric and ocean circulation remains controversial and plays an important role for our understanding of ice sheet response to modern global warming. The timing and sequence of deglacial warming is relevant for understanding the variability and sensitivity of the <span class="hlt">Antarctic</span> Ice Sheet to climatic changes, and the continuing rise of atmospheric greenhouse gas concentrations. The <span class="hlt">Antarctic</span> Ice Sheet is a pivotal component of the global <span class="hlt">water</span> budget. Freshwater fluxes from the ice sheet may affect the <span class="hlt">Antarctic</span> Circumpolar Current (ACC), which is strongly impacted by the westerly wind belt in the Southern Hemisphere (SHWW) and constricted to its narrowest extent in the Drake Passage. The flow of ACC <span class="hlt">water</span> masses through Drake Passage is, therefore, crucial for advancing our understanding of the Southern Ocean's role in global meridional overturning circulation and global climate change. In order to address orbital and millennial-scale variability of the <span class="hlt">Antarctic</span> ice sheet and the ACC, we applied a multi-proxy approach on a sediment core from the central Drake Passage including grain size, iceberg-rafted debris, mineral dust, bulk chemical and mineralogical composition, and physical properties. In combination with already published and new sediment records from the Drake Passage and Scotia Sea, as well as high-resolution data from <span class="hlt">Antarctic</span> ice cores (WDC, EDML), we now have evidence that during glacial times a more northerly extent of the perennial sea-ice zone decreased ACC current velocities in the central Drake Passage. During deglaciation the SHWW shifted southwards due to a decreasing temperature gradient between subtropical and polar latitudes caused by sea ice and ice sheet decline. This in turn caused Southern Hemisphere warming, a more vigorous ACC, stronger Southern Ocean ventilation, and warm Circumpolar Deep <span class="hlt">Water</span> (CDW) upwelling on <span class="hlt">Antarctic</span> shelves</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016GGG....17.2336D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GGG....17.2336D"><span>South Atlantic <span class="hlt">intermediate</span> <span class="hlt">water</span> advances into the North-east Atlantic with reduced Atlantic meridional overturning circulation during the last glacial period</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dubois-Dauphin, Quentin; Bonneau, Lucile; Colin, Christophe; Montero-Serrano, Jean-Carlos; Montagna, Paolo; Blamart, Dominique; Hebbeln, Dierk; Van Rooij, David; Pons-Branchu, Edwige; Hemsing, Freya; Wefing, Anne-Marie; Frank, Norbert</p> <p>2016-06-01</p> <p>The Nd isotopic composition (ɛNd) of seawater and cold-<span class="hlt">water</span> coral (CWC) samples from the Gulf of Cádiz and the Alboran Sea, at a depth of 280-827 m were investigated in order to constrain middepth <span class="hlt">water</span> mass dynamics within the Gulf of Cádiz over the past 40 ka. ɛNd of glacial and Holocene CWC from the Alboran Sea and the northern Gulf of Cádiz reveals relatively constant values (-8.6 to -9.0 and -9.5 to -10.4, respectively). Such values are similar to those of the surrounding present-day middepth <span class="hlt">waters</span> from the Mediterranean Outflow <span class="hlt">Water</span> (MOW; ɛNd ˜ -9.4) and Mediterranean Sea <span class="hlt">Water</span> (MSW; ɛNd ˜ -9.9). In contrast, glacial ɛNd values for CWC collected at thermocline depth (550-827 m) in the southern Gulf of Cádiz display a higher average value (-8.9 ± 0.4) compared to the present-day value (-11.7 ± 0.3). This implies a higher relative contribution of <span class="hlt">water</span> masses of Mediterranean (MSW) or South Atlantic origin (East <span class="hlt">Antarctic</span> <span class="hlt">Intermediate</span> <span class="hlt">Water</span>, EAAIW). Our study has produced the first evidence of significant radiogenic ɛNd values (˜ -8) at 19, 23-24, and 27 ka, which are coeval with increasing iceberg discharges and a weakening of Atlantic Meridional Overturning Circulation (AMOC). Since MOW ɛNd values remained stable during the last glacial period, it is suggested that these radiogenic ɛNd values most likely reflect an enhanced northward propagation of glacial EAAIW into the eastern Atlantic Basin.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24201563','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24201563"><span>Modern <span class="hlt">Antarctic</span> acorn worms form tubes.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Halanych, Kenneth M; Cannon, Johanna T; Mahon, Andrew R; Swalla, Billie J; Smith, Craig R</p> <p>2013-01-01</p> <p>Acorn worms, or enteropneusts, are vermiform hemichordates that occupy an important position in deuterostome phylogeny. Allied to pterobranch hemichordates, small colonial tube dwellers, modern enteropneusts were thought to be tubeless. However, understanding of hemichordate diversity is poor, as evidenced by absence of reports from some oceanic regions and recent descriptions of large epibenthic deep-<span class="hlt">water</span> enteropneusts, Torquaratoridae. Here we show, based on expeditions to Antarctica, that some acorn worms produce conspicuous tubes that persist for days. Interestingly, recent fossil descriptions show a Middle Cambrian acorn worm lived in tubes, leading to speculation that these fossils may have been pterobranch forbearers. Our discovery provides the alternative interpretation that these fossils are similar to modern-day torquaratorids and that some behaviours have been conserved for over 500 million years. Moreover, the frequency of <span class="hlt">Antarctic</span> enteropneusts observed attests to our limited knowledge of <span class="hlt">Antarctic</span> marine ecosystems, and strengthens hypotheses relating more northern deep-sea fauna to <span class="hlt">Antarctic</span> shelf fauna.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5544119','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5544119"><span>Revision of Eocene <span class="hlt">Antarctic</span> carpet sharks (Elasmobranchii, Orectolobiformes) from Seymour Island, <span class="hlt">Antarctic</span> Peninsula</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Engelbrecht, Andrea; Mörs, Thomas; Reguero, Marcelo A.; Kriwet, Jürgen</p> <p>2017-01-01</p> <p>Seymour Island, <span class="hlt">Antarctic</span> Peninsula, was once called the ‘Rosetta Stone’ of Southern Hemisphere palaeobiology, because this small island provides the most complete and richly fossiliferous Palaeogene sequence in Antarctica. Among fossil marine vertebrate remains, chondrichthyans seemingly were dominant elements in the Eocene <span class="hlt">Antarctic</span> fish fauna. The fossiliferous sediments on Seymour Island are from the La Meseta Formation, which was originally divided into seven stratigraphical levels, TELMs 1–7 (acronym for Tertiary Eocene La Meseta) ranging from the upper Ypresian (early Eocene) to the late Priabonian (late Eocene). Bulk sampling of unconsolidated sediments from TELMs 5 and 6, which are Ypresian (early Eocene) and Lutetian (middle Eocene) in age, respectively, yielded very rich and diverse chondrichthyan assemblages including over 40 teeth of carpet sharks representing two new taxa, Notoramphoscyllium woodwardi gen. et sp. nov. and Ceolometlaouia pannucae gen. et sp. nov. Two additional teeth from TELM 5 represent two different taxa that cannot be assigned to any specific taxon and thus are left in open nomenclature. The new material not only increases the diversity of Eocene <span class="hlt">Antarctic</span> selachian faunas but also allows two previous orectolobiform records to be re-evaluated. Accordingly, Stegostoma cf. faciatum is synonymized with Notoramphoscyllium woodwardi gen. et sp. nov., whereas Pseudoginglymostoma cf. brevicaudatum represents a nomen dubium. The two new taxa, and probably the additional two unidentified taxa, are interpreted as permanent residents, which most likely were endemic to <span class="hlt">Antarctic</span> <span class="hlt">waters</span> during the Eocene and adapted to shallow and estuarine environments. PMID:28785171</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMOS51B1652K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMOS51B1652K"><span>Variability of the <span class="hlt">Antarctic</span> Surface <span class="hlt">Water</span> and the Upper Circumpolar Deep <span class="hlt">Water</span> from 1992 WOCE and 2007-2008 Argo data along the section P19 in Southeastern Pacific</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kang, S.; Lee, J.; Kim, Y.; Kim, E.; Seung, Y.</p> <p>2013-12-01</p> <p>The variability of the Upper Circumpolar Deep <span class="hlt">Water</span> (UCDW) and <span class="hlt">Antarctic</span> Surface <span class="hlt">Water</span> (AASW) is examined based upon the World Ocean Circulation Experiment (WOCE) data in 1992 and Argo data in 2007 and 2008 along the section P19. D.G. Martinson (2012) examined the <span class="hlt">Antarctic</span> Circumpolar Current's role in the <span class="hlt">Antarctic</span> Ice System and showed that 3-color WOCE temperature sections, including section P19, showed that tilt of the isopycnals associated with ACC prevent warm tropical <span class="hlt">waters</span> from reaching <span class="hlt">Antarctic</span> continental margin. The paper also described that warm UCDW layer slips along the tilted isopycnals to reach the continental slope in section P19 along the Western <span class="hlt">Antarctic</span> Peninsula (WAP). It is also revealed that the UCDW, associated with the ACC in section P19, occupies the domain from 58°S to 68°S with meridional ACC width of about 1,000km. In order to estimate the fluctuation of the warm UCDW layer the Argo data both in 2007 and 2008 were collected and the location of the warm UCDW from Argo data in 2007 and 2008 was compared with that of WOCE from Martinson (2012) in 1992. The argo data in 2007 and 2008 are used to examine the tilted isopycnal pattern of the warm UCDW represented by warm <span class="hlt">waters</span> above 1.8°C. One thing to note is that the southern limit of the UCDW in the WOCE data in 1992, appears to move northward in Argo data of 2007 and 2008. Also AASW less than 2.0°C from the WAP in Argo data replaces the rather warm thin layer between 62°S nearly to 69°S shown in the WOCE data in 1992. The low salinity layer bounded by 34.0 psu extends far north compared with that of WOCE data, indicating that the ice melting <span class="hlt">water</span> from the WAP flows northward. Since all year round data in case of Argo data are used and the error by the seasonal fluctuation may be introduced in the location of the upper 500m depth. The global wind stress curl data by SCOW (Scatterometer Climatology of Ocean Wind) are available over 1997 to 2007, which reveals that the wind stress</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ESE...tmp....4B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ESE...tmp....4B"><span>Persistent Organic Pollutants in Biotic and Abiotic Components of <span class="hlt">Antarctic</span> Pristine Environment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bhardwaj, Laxmikant; Chauhan, Abhishek; Ranjan, Anuj; Jindal, Tanu</p> <p>2018-02-01</p> <p>Over the past decades, research in Antarctica has built a new understanding of Antarctica, its past, present and future. Human activities and long-range pollutants are increasing on the <span class="hlt">Antarctic</span> continent. Research on persistent organic pollutants (POPs) has been carried out internationally by several countries having their permanent research stations to explain the impact of an ever increasing range of POPs in <span class="hlt">Antarctic</span> ecosystem. POPs have been detected in Antarctica despite its geographical isolation and almost complete absence of human settlements. The presence of POPs in different abiotic (atmosphere, <span class="hlt">water</span> bodies, sediments, soil, sea ice) and biotic components (mosses, lichens, krill, penguins, skua, etc.) in Antarctica has been studied and documented around for decades and has either been banned or strictly regulated but is still found in the environment. This review focuses on recent research pertaining to sources and occurrence of POPs in <span class="hlt">Antarctic</span> lake <span class="hlt">water</span>, soil, sediment, lichen, mosses and other <span class="hlt">Antarctic</span> marine community. This review also proposes to summarize the current state of research on POPs in Antarctica environment and draw the earliest conclusions on possible significance of POPs in Antarctica based on presently available information from related <span class="hlt">Antarctic</span> environment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ESE.....2...32B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ESE.....2...32B"><span>Persistent Organic Pollutants in Biotic and Abiotic Components of <span class="hlt">Antarctic</span> Pristine Environment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bhardwaj, Laxmikant; Chauhan, Abhishek; Ranjan, Anuj; Jindal, Tanu</p> <p>2018-05-01</p> <p>Over the past decades, research in Antarctica has built a new understanding of Antarctica, its past, present and future. Human activities and long-range pollutants are increasing on the <span class="hlt">Antarctic</span> continent. Research on persistent organic pollutants (POPs) has been carried out internationally by several countries having their permanent research stations to explain the impact of an ever increasing range of POPs in <span class="hlt">Antarctic</span> ecosystem. POPs have been detected in Antarctica despite its geographical isolation and almost complete absence of human settlements. The presence of POPs in different abiotic (atmosphere, <span class="hlt">water</span> bodies, sediments, soil, sea ice) and biotic components (mosses, lichens, krill, penguins, skua, etc.) in Antarctica has been studied and documented around for decades and has either been banned or strictly regulated but is still found in the environment. This review focuses on recent research pertaining to sources and occurrence of POPs in <span class="hlt">Antarctic</span> lake <span class="hlt">water</span>, soil, sediment, lichen, mosses and other <span class="hlt">Antarctic</span> marine community. This review also proposes to summarize the current state of research on POPs in Antarctica environment and draw the earliest conclusions on possible significance of POPs in Antarctica based on presently available information from related <span class="hlt">Antarctic</span> environment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19920044190&hterms=marine+biology&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dmarine%2Bbiology','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19920044190&hterms=marine+biology&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dmarine%2Bbiology"><span>Ozone depletion - Ultraviolet radiation and phytoplankton biology in <span class="hlt">Antarctic</span> <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>Smith, R. C.; Prezelin, B. B.; Baker, K. S.; Bidigare, R. R.; Boucher, N. P.; Coley, T.; Karentz, D.; Macintyre, S.; Matlick, H. A.; Menzies, D.</p> <p>1992-01-01</p> <p>The near-50-percent thinning of the stratospheric ozone layer over the <span class="hlt">Antarctic</span>, with increased passage of mid-UV radiation to the surface of the Southern Ocean, has prompted concern over possible radiation damage to the near-surface phytoplankton communities that are the bases of <span class="hlt">Antarctic</span> marine ecosystems. As the ozone layer thinned, a 6-week study of the marginal ice zone of the Bellingshousen Sea in the austral spring of 1990 noted sea-surface and depth-dependent ratios of mid-UV irradiance to total irradiance increased, and mid-UV inhibition of photosynthesis increased. A 6-12 percent reduction in primary production associated with ozone depletion was estimated to have occurred over the course of the present study.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040089736&hterms=oxygen+consumption&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Doxygen%2Bconsumption','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040089736&hterms=oxygen+consumption&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Doxygen%2Bconsumption"><span>Sediment oxygen profiles in a super-oxygenated <span class="hlt">antarctic</span> lake</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wharton, R. A. Jr; Meyer, M. A.; McKay, C. P.; Mancinelli, R. L.; Simmons, G. M. Jr; Wharton RA, J. r. (Principal Investigator)</p> <p>1994-01-01</p> <p>Perennially ice-covered lakes are found in the McMurdo Dry Valleys of southern Victoria Land, Antarctica. In contrast to temperate lakes that have diurnal photic periods, <span class="hlt">antarctic</span> (and arctic) lakes have a yearly photic period. An unusual feature of the <span class="hlt">antarctic</span> lakes is the occurrence of O2 at supersaturated levels in certain portions of the <span class="hlt">water</span> column. Here we report the first sediment O2 profiles obtained using a microelectrode from a perennially ice-covered <span class="hlt">antarctic</span> lake. Sediment cores collected in January and October 1987 from Lake Hoare in Taylor Valley show oxygenation down to 15, and in some cases, 25 cm. The oxygenation of sediments several centimeters below the sediment-<span class="hlt">water</span> interface is atypical for lake sediments and may be characteristic of perennially ice-covered lakes. There is a significant difference between the observed January and October sediment O2 profiles. Several explanations may account for the difference, including seasonality. A time-dependent model is presented which tests the feasibility of a seasonal cycle resulting from the long photoperiod and benthic primary production in sediments overlain by a highly oxygenated <span class="hlt">water</span> column.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1233183','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1233183"><span>Mode and <span class="hlt">Intermediate</span> <span class="hlt">Waters</span> in Earth System Models</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>Gnanadesikan, Anand; Sarmiento, Jorge L.</p> <p></p> <p>This report describes work done as part of a joint Princeton-Johns Hopkins project to look at the impact of mode and <span class="hlt">intermediate</span> <span class="hlt">waters</span> in Earth System Models. The Johns Hopkins portion of this work focussed on the role of lateral mixing in ventilating such <span class="hlt">waters</span>, with important implications for hypoxia, the uptake of anthropogenic carbon, the dynamics of El Nino and carbon pumps. The Johns Hopkins group also collaborated with the Princeton Group to help develop a watermass diagnostics framework.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24891389','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24891389"><span>Ocean processes at the <span class="hlt">Antarctic</span> continental slope.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Heywood, Karen J; Schmidtko, Sunke; Heuzé, Céline; Kaiser, Jan; Jickells, Timothy D; Queste, Bastien Y; Stevens, David P; Wadley, Martin; Thompson, Andrew F; Fielding, Sophie; Guihen, Damien; Creed, Elizabeth; Ridley, Jeff K; Smith, Walker</p> <p>2014-07-13</p> <p>The <span class="hlt">Antarctic</span> continental shelves and slopes occupy relatively small areas, but, nevertheless, are important for global climate, biogeochemical cycling and ecosystem functioning. Processes of <span class="hlt">water</span> mass transformation through sea ice formation/melting and ocean-atmosphere interaction are key to the formation of deep and bottom <span class="hlt">waters</span> as well as determining the heat flux beneath ice shelves. Climate models, however, struggle to capture these physical processes and are unable to reproduce <span class="hlt">water</span> mass properties of the region. Dynamics at the continental slope are key for correctly modelling climate, yet their small spatial scale presents challenges both for ocean modelling and for observational studies. Cross-slope exchange processes are also vital for the flux of nutrients such as iron from the continental shelf into the mixed layer of the Southern Ocean. An iron-cycling model embedded in an eddy-permitting ocean model reveals the importance of sedimentary iron in fertilizing parts of the Southern Ocean. Ocean gliders play a key role in improving our ability to observe and understand these small-scale processes at the continental shelf break. The Gliders: Excellent New Tools for Observing the Ocean (GENTOO) project deployed three Seagliders for up to two months in early 2012 to sample the <span class="hlt">water</span> to the east of the <span class="hlt">Antarctic</span> Peninsula in unprecedented temporal and spatial detail. The glider data resolve small-scale exchange processes across the shelf-break front (the <span class="hlt">Antarctic</span> Slope Front) and the front's biogeochemical signature. GENTOO demonstrated the capability of ocean gliders to play a key role in a future multi-disciplinary Southern Ocean observing system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4032510','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4032510"><span>Ocean processes at the <span class="hlt">Antarctic</span> continental slope</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Heywood, Karen J.; Schmidtko, Sunke; Heuzé, Céline; Kaiser, Jan; Jickells, Timothy D.; Queste, Bastien Y.; Stevens, David P.; Wadley, Martin; Thompson, Andrew F.; Fielding, Sophie; Guihen, Damien; Creed, Elizabeth; Ridley, Jeff K.; Smith, Walker</p> <p>2014-01-01</p> <p>The <span class="hlt">Antarctic</span> continental shelves and slopes occupy relatively small areas, but, nevertheless, are important for global climate, biogeochemical cycling and ecosystem functioning. Processes of <span class="hlt">water</span> mass transformation through sea ice formation/melting and ocean–atmosphere interaction are key to the formation of deep and bottom <span class="hlt">waters</span> as well as determining the heat flux beneath ice shelves. Climate models, however, struggle to capture these physical processes and are unable to reproduce <span class="hlt">water</span> mass properties of the region. Dynamics at the continental slope are key for correctly modelling climate, yet their small spatial scale presents challenges both for ocean modelling and for observational studies. Cross-slope exchange processes are also vital for the flux of nutrients such as iron from the continental shelf into the mixed layer of the Southern Ocean. An iron-cycling model embedded in an eddy-permitting ocean model reveals the importance of sedimentary iron in fertilizing parts of the Southern Ocean. Ocean gliders play a key role in improving our ability to observe and understand these small-scale processes at the continental shelf break. The Gliders: Excellent New Tools for Observing the Ocean (GENTOO) project deployed three Seagliders for up to two months in early 2012 to sample the <span class="hlt">water</span> to the east of the <span class="hlt">Antarctic</span> Peninsula in unprecedented temporal and spatial detail. The glider data resolve small-scale exchange processes across the shelf-break front (the <span class="hlt">Antarctic</span> Slope Front) and the front's biogeochemical signature. GENTOO demonstrated the capability of ocean gliders to play a key role in a future multi-disciplinary Southern Ocean observing system. PMID:24891389</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1764834','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1764834"><span>Marine pelagic ecosystems: the West <span class="hlt">Antarctic</span> Peninsula</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Ducklow, Hugh W; Baker, Karen; Martinson, Douglas G; Quetin, Langdon B; Ross, Robin M; Smith, Raymond C; Stammerjohn, Sharon E; Vernet, Maria; Fraser, William</p> <p>2006-01-01</p> <p>The marine ecosystem of the West <span class="hlt">Antarctic</span> Peninsula (WAP) extends from the Bellingshausen Sea to the northern tip of the peninsula and from the mostly glaciated coast across the continental shelf to the shelf break in the west. The glacially sculpted coastline along the peninsula is highly convoluted and characterized by deep embayments that are often interconnected by channels that facilitate transport of heat and nutrients into the shelf domain. The ecosystem is divided into three subregions, the continental slope, shelf and coastal regions, each with unique ocean dynamics, <span class="hlt">water</span> mass and biological distributions. The WAP shelf lies within the <span class="hlt">Antarctic</span> Sea Ice Zone (SIZ) and like other SIZs, the WAP system is very productive, supporting large stocks of marine mammals, birds and the <span class="hlt">Antarctic</span> krill, Euphausia superba. Ecosystem dynamics is dominated by the seasonal and interannual variation in sea ice extent and retreat. The <span class="hlt">Antarctic</span> Peninsula is one among the most rapidly warming regions on Earth, having experienced a 2°C increase in the annual mean temperature and a 6°C rise in the mean winter temperature since 1950. Delivery of heat from the <span class="hlt">Antarctic</span> Circumpolar Current has increased significantly in the past decade, sufficient to drive to a 0.6°C warming of the upper 300 m of shelf <span class="hlt">water</span>. In the past 50 years and continuing in the twenty-first century, the warm, moist maritime climate of the northern WAP has been migrating south, displacing the once dominant cold, dry continental <span class="hlt">Antarctic</span> climate and causing multi-level responses in the marine ecosystem. Ecosystem responses to the regional warming include increased heat transport, decreased sea ice extent and duration, local declines in ice-dependent Adélie penguins, increase in ice-tolerant gentoo and chinstrap penguins, alterations in phytoplankton and zooplankton community composition and changes in krill recruitment, abundance and availability to predators. The climate/ecological gradients</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li class="active"><span>6</span></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_6 --> <div id="page_7" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li class="active"><span>7</span></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="121"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSPO34A3022N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSPO34A3022N"><span>Distinct characteristics of the <span class="hlt">intermediate</span> <span class="hlt">water</span> observed off the east coast of Korea during two contrasting years</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nam, S.; Yoon, S.; Park, J. H.; Kim, Y. H.; Chang, K. I.</p> <p>2016-02-01</p> <p>The <span class="hlt">intermediate</span> <span class="hlt">water</span> known as `East Sea <span class="hlt">Intermediate</span> <span class="hlt">Water</span>' and its coastal mode `North Korea Cold <span class="hlt">Water</span>' found south of the Subpolar Front (SF) is formed in the northern East (Japan) Sea, and its physical properties are known to be determined by wintertime air-sea interaction north of the SF. Hydrographic data collected off the coast bi-monthly from 1994 to 2011 show significant decadal oscillations in spiciness following isopycnals of <span class="hlt">intermediate</span> <span class="hlt">water</span> (27.1-27.2 sigma-theta typically corresponding to 150 m depth), which are explained by the Arctic Oscillation (AO) and consequent cold-air outbreaks. During positive AO phases over the decades, the cold-air outbreak and <span class="hlt">water</span> formation are more active and the <span class="hlt">intermediate</span> <span class="hlt">water</span> having the same spiciness reaches higher density (higher spiciness following the same isopycnals). At interannual timescale, however, the spiciness variability is well beyond the relationship with the AO. Especially, significantly lower spiciness (or both less saline and lower temperature) <span class="hlt">intermediate</span> <span class="hlt">water</span> was observed in spring of 2010 than 2001 under the similar AO condition (negative peaks). Strong cooling with common negative peaks in surface net-heat flux (with different patterns) and common negative peaks in the AO index are prominent in winter of the two years over past two decades. Such contrasting characteristics of <span class="hlt">intermediate</span> <span class="hlt">water</span> between 2001 and 2010 are consistent with the HYCOM reanalysis results which, along with the satellite altimetry-derived sea surface height maps, indicates widespread extension of low (high) spiciness <span class="hlt">intermediate</span> <span class="hlt">water</span> in the southwestern East Sea in 2010 (2001). A clear contrast in circulation pattern, along with net-heat flux pattern, is suggested to derive the observational results in the distinctly different characteristics of the <span class="hlt">intermediate</span> <span class="hlt">water</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.H31E1446F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.H31E1446F"><span>Forest Canopy <span class="hlt">Water</span> Cycling Responses to an <span class="hlt">Intermediate</span> Disturbance Revealed Through Stable <span class="hlt">Water</span> Vapor Isotopes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fiorella, R.; Poulsen, C. J.; Matheny, A. M.; Rey Sanchez, C.; Fotis, A. T.; Morin, T. H.; Vogel, C. S.; Gough, C. M.; Aron, P.; Bohrer, G.</p> <p>2016-12-01</p> <p>Forest structure, age, and species composition modulate fluxes of carbon and <span class="hlt">water</span> between the land surface and the atmosphere. The response of forests to <span class="hlt">intermediate</span> disturbances such as ecological succession, species-specific insect invasion, or selective logging that disrupt the canopy but do not promote complete stand replacement, shape how these fluxes evolve through time. We investigate the impact of an <span class="hlt">intermediate</span> disturbance to <span class="hlt">water</span> cycling processes by comparing vertical profiles of stable <span class="hlt">water</span> isotopes in two closely located forest canopies in the northern lower peninsula of Michigan using cavity ring-down spectroscopy. In one of the canopies, an <span class="hlt">intermediate</span> disturbance was prescribed in 2008 by inducing mortality in all canopy-dominant early successional species. Isotopic compositions of atmospheric <span class="hlt">water</span> vapor are measured at six heights during two time periods (summer and early fall) at two flux towers and compared with local meteorology and calculated atmospheric back-trajectories. Disturbance has little impact on low-frequency changes in isotopic composition (e.g., >1 day); at these timescales, isotopic composition is strongly related to large-scale moisture transport. In contrast, disturbance has substantial impacts on the vertical distribution of <span class="hlt">water</span> isotopes throughout the canopy when transpiration rates are high during the summer, but impact is muted during early fall. Sub-diurnal differences in canopy <span class="hlt">water</span> vapor cycling are likely related to differences in species composition and response to disturbance and changes in canopy structure. Predictions of transpiration fluxes by land-surface models that do not account species-specific relationships and canopy structure are unlikely to capture these relationships, but addition of stable isotopes to land surface models may provide a useful parameter to improve these predictions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22384073','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22384073"><span>The association of <span class="hlt">Antarctic</span> krill Euphausia superba with the under-ice habitat.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Flores, Hauke; van Franeker, Jan Andries; Siegel, Volker; Haraldsson, Matilda; Strass, Volker; Meesters, Erik Hubert; Bathmann, Ulrich; Wolff, Willem Jan</p> <p>2012-01-01</p> <p>The association of <span class="hlt">Antarctic</span> krill Euphausia superba with the under-ice habitat was investigated in the Lazarev Sea (Southern Ocean) during austral summer, autumn and winter. Data were obtained using novel Surface and Under Ice Trawls (SUIT), which sampled the 0-2 m surface layer both under sea ice and in open <span class="hlt">water</span>. Average surface layer densities ranged between 0.8 individuals m(-2) in summer and autumn, and 2.7 individuals m(-2) in winter. In summer, under-ice densities of <span class="hlt">Antarctic</span> krill were significantly higher than in open <span class="hlt">waters</span>. In autumn, the opposite pattern was observed. Under winter sea ice, densities were often low, but repeatedly far exceeded summer and autumn maxima. Statistical models showed that during summer high densities of <span class="hlt">Antarctic</span> krill in the 0-2 m layer were associated with high ice coverage and shallow mixed layer depths, among other factors. In autumn and winter, density was related to hydrographical parameters. Average under-ice densities from the 0-2 m layer were higher than corresponding values from the 0-200 m layer collected with Rectangular Midwater Trawls (RMT) in summer. In winter, under-ice densities far surpassed maximum 0-200 m densities on several occasions. This indicates that the importance of the ice-<span class="hlt">water</span> interface layer may be under-estimated by the pelagic nets and sonars commonly used to estimate the population size of <span class="hlt">Antarctic</span> krill for management purposes, due to their limited ability to sample this habitat. Our results provide evidence for an almost year-round association of <span class="hlt">Antarctic</span> krill with the under-ice habitat, hundreds of kilometres into the ice-covered area of the Lazarev Sea. Local concentrations of postlarval <span class="hlt">Antarctic</span> krill under winter sea ice suggest that sea ice biota are important for their winter survival. These findings emphasise the susceptibility of an ecological key species to changing sea ice habitats, suggesting potential ramifications on <span class="hlt">Antarctic</span> ecosystems induced by climate change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3285626','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3285626"><span>The Association of <span class="hlt">Antarctic</span> Krill Euphausia superba with the Under-Ice Habitat</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Flores, Hauke; van Franeker, Jan Andries; Siegel, Volker; Haraldsson, Matilda; Strass, Volker; Meesters, Erik Hubert; Bathmann, Ulrich; Wolff, Willem Jan</p> <p>2012-01-01</p> <p>The association of <span class="hlt">Antarctic</span> krill Euphausia superba with the under-ice habitat was investigated in the Lazarev Sea (Southern Ocean) during austral summer, autumn and winter. Data were obtained using novel Surface and Under Ice Trawls (SUIT), which sampled the 0–2 m surface layer both under sea ice and in open <span class="hlt">water</span>. Average surface layer densities ranged between 0.8 individuals m−2 in summer and autumn, and 2.7 individuals m−2 in winter. In summer, under-ice densities of <span class="hlt">Antarctic</span> krill were significantly higher than in open <span class="hlt">waters</span>. In autumn, the opposite pattern was observed. Under winter sea ice, densities were often low, but repeatedly far exceeded summer and autumn maxima. Statistical models showed that during summer high densities of <span class="hlt">Antarctic</span> krill in the 0–2 m layer were associated with high ice coverage and shallow mixed layer depths, among other factors. In autumn and winter, density was related to hydrographical parameters. Average under-ice densities from the 0–2 m layer were higher than corresponding values from the 0–200 m layer collected with Rectangular Midwater Trawls (RMT) in summer. In winter, under-ice densities far surpassed maximum 0–200 m densities on several occasions. This indicates that the importance of the ice-<span class="hlt">water</span> interface layer may be under-estimated by the pelagic nets and sonars commonly used to estimate the population size of <span class="hlt">Antarctic</span> krill for management purposes, due to their limited ability to sample this habitat. Our results provide evidence for an almost year-round association of <span class="hlt">Antarctic</span> krill with the under-ice habitat, hundreds of kilometres into the ice-covered area of the Lazarev Sea. Local concentrations of postlarval <span class="hlt">Antarctic</span> krill under winter sea ice suggest that sea ice biota are important for their winter survival. These findings emphasise the susceptibility of an ecological key species to changing sea ice habitats, suggesting potential ramifications on <span class="hlt">Antarctic</span> ecosystems induced by climate</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013DSRI...75...52W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013DSRI...75...52W"><span>Primary production export flux in Marguerite Bay (<span class="hlt">Antarctic</span> Peninsula): Linking upper <span class="hlt">water</span>-column production to sediment trap flux</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Weston, Keith; Jickells, Timothy D.; Carson, Damien S.; Clarke, Andrew; Meredith, Michael P.; Brandon, Mark A.; Wallace, Margaret I.; Ussher, Simon J.; Hendry, Katharine R.</p> <p>2013-05-01</p> <p>A study was carried out to assess primary production and associated export flux in the coastal <span class="hlt">waters</span> of the western <span class="hlt">Antarctic</span> Peninsula at an oceanographic time-series site. New, i.e., exportable, primary production in the upper <span class="hlt">water</span>-column was estimated in two ways; by nutrient deficit measurements, and by primary production rate measurements using separate 14C-labelled radioisotope and 15N-labelled stable isotope uptake incubations. The resulting average annual exportable primary production estimates at the time-series site from nutrient deficit and primary production rates were 13 and 16 mol C m-2, respectively. Regenerated primary production was measured using 15N-labelled ammonium and urea uptake, and was low throughout the sampling period. The exportable primary production measurements were compared with sediment trap flux measurements from 2 locations; the time-series site and at a site 40 km away in deeper <span class="hlt">water</span>. Results showed ˜1% of the upper mixed layer exportable primary production was exported to traps at 200 m depth at the time-series site (total <span class="hlt">water</span> column depth 520 m). The maximum particle flux rate to sediment traps at the deeper offshore site (total <span class="hlt">water</span> column depth 820 m) was lower than the flux at the coastal time-series site. Flux of particulate organic carbon was similar throughout the spring-summer high flux period for both sites. Remineralisation of particulate organic matter predominantly occurred in the upper <span class="hlt">water</span>-column (<200 m depth), with minimal remineralisation below 200 m, at both sites. This highly productive region on the Western <span class="hlt">Antarctic</span> Peninsula is therefore best characterised as 'high recycling, low export'.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003JGRC..108.3348U','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003JGRC..108.3348U"><span><span class="hlt">Intermediate</span> <span class="hlt">water</span> circulation in the North Pacific subarctic and northern subtropical regions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ueno, Hiromichi; Yasuda, Ichiro</p> <p>2003-11-01</p> <p>The <span class="hlt">intermediate</span> <span class="hlt">water</span> circulation in the North Pacific subarctic and northern subtropical regions is investigated through inverse analysis, focusing on the volume and heat transports from the subtropical to the subarctic regions. The inverse method we adopted is a hybrid method of β-spiral and box inverse methods which permits diapycnal flux. The isopycnal velocities estimated through the inverse analysis are mostly consistent with the oxygen distribution and support the hypothesis that warm and saline <span class="hlt">intermediate</span> <span class="hlt">water</span> is transported from the transition domain east of Japan to the northern Gulf of Alaska. The northward volume transport across 46°N between 158°E and 130°W is estimated to be -0.2 to 5.3 Sv in the density range of 26.7-27.2σθ. The upward diapycnal transports in the open subarctic North Pacific (region N) across 26.7 and 27.2σθ isopycnal surfaces are estimated to be 0.2 to 1.5 Sv and -0.2 to 0.9 Sv, respectively. Part of the <span class="hlt">water</span> transported upward across 26.7σθ might outcrop and be carried to the subtropical region by the southward Ekman drift. Through the examination of heat balance of the <span class="hlt">intermediate</span> layer in the subarctic region, it is suggested quantitatively that the <span class="hlt">intermediate</span> heat transport from the south plays an essential role in maintaining the heat of the mesothermal <span class="hlt">waters</span> in the subarctic region.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25143114','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25143114"><span>A microbial ecosystem beneath the West <span class="hlt">Antarctic</span> ice sheet.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Christner, Brent C; Priscu, John C; Achberger, Amanda M; Barbante, Carlo; Carter, Sasha P; Christianson, Knut; Michaud, Alexander B; Mikucki, Jill A; Mitchell, Andrew C; Skidmore, Mark L; Vick-Majors, Trista J</p> <p>2014-08-21</p> <p>Liquid <span class="hlt">water</span> has been known to occur beneath the <span class="hlt">Antarctic</span> ice sheet for more than 40 years, but only recently have these subglacial aqueous environments been recognized as microbial ecosystems that may influence biogeochemical transformations on a global scale. Here we present the first geomicrobiological description of <span class="hlt">water</span> and surficial sediments obtained from direct sampling of a subglacial <span class="hlt">Antarctic</span> lake. Subglacial Lake Whillans (SLW) lies beneath approximately 800 m of ice on the lower portion of the Whillans Ice Stream (WIS) in West Antarctica and is part of an extensive and evolving subglacial drainage network. The <span class="hlt">water</span> column of SLW contained metabolically active microorganisms and was derived primarily from glacial ice melt with solute sources from lithogenic weathering and a minor seawater component. Heterotrophic and autotrophic production data together with small subunit ribosomal RNA gene sequencing and biogeochemical data indicate that SLW is a chemosynthetically driven ecosystem inhabited by a diverse assemblage of bacteria and archaea. Our results confirm that aquatic environments beneath the <span class="hlt">Antarctic</span> ice sheet support viable microbial ecosystems, corroborating previous reports suggesting that they contain globally relevant pools of carbon and microbes that can mobilize elements from the lithosphere and influence Southern Ocean geochemical and biological systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014E%26PSL.399...52S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014E%26PSL.399...52S"><span>Active <span class="hlt">water</span> exchange and life near the grounding line of an <span class="hlt">Antarctic</span> outlet glacier</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sugiyama, Shin; Sawagaki, Takanobu; Fukuda, Takehiro; Aoki, Shigeru</p> <p>2014-08-01</p> <p>The grounding line (GL) of the <span class="hlt">Antarctic</span> ice sheet forms the boundary between grounded and floating ice along the coast. Near this line, warm oceanic <span class="hlt">water</span> contacts the ice shelf, producing the ice sheet's highest basal-melt rate. Despite the importance of this region, <span class="hlt">water</span> properties and circulations near the GL are largely unexplored because in-situ observations are difficult. Here we present direct evidence of warm ocean-<span class="hlt">water</span> transport to the innermost part of the subshelf cavity (several hundred meters seaward from the GL) of Langhovde Glacier, an outlet glacier in East Antarctica. Our measurements come from boreholes drilled through the glacier's ∼400-m-thick grounding zone. Beneath the grounding zone, we find a 10-24-m-deep <span class="hlt">water</span> layer of uniform temperature and salinity (-1.45 °C; 34.25 PSU), values that roughly equal those measured in the ocean in front of the glacier. Moreover, living organisms are found in the thin subglacial <span class="hlt">water</span> layer. These findings indicate active transport of <span class="hlt">water</span> and nutrients from the adjacent ocean, meaning that the subshelf environment interacts directly and rapidly with the ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16346297','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16346297"><span>Bacterioplankton in <span class="hlt">antarctic</span> ocean <span class="hlt">waters</span> during late austral winter: abundance, frequency of dividing cells, and estimates of production.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hanson, R B; Shafer, D; Ryan, T; Pope, D H; Lowery, H K</p> <p>1983-05-01</p> <p>Bacterioplankton productivity in <span class="hlt">Antarctic</span> <span class="hlt">waters</span> of the eastern South Pacific Ocean and Drake Passage was estimated by direct counts and frequency of dividing cells (FDC). Total bacterioplankton assemblages were enumerated by epifluorescent microscopy. The experimentally determined relationship between in situ FDC and the potential instantaneous growth rate constant (mu) is best described by the regression equation ln mu = 0.081 FDC - 3.73. In the eastern South Pacific Ocean, bacterioplankton abundance (2 x 10 to 3.5 x 10 cells per ml) and FDC (11%) were highest at the Polar Front (<span class="hlt">Antarctic</span> Convergence). North of the Subantarctic Front, abundance and FDC were between 1 x 10 to 2 x 10 cells per ml and 3 to 5%, respectively, and were vertically homogeneous to a depth of 600 m. In Drake Passage, abundance (10 x 10 cells per ml) and FDC (16%) were highest in <span class="hlt">waters</span> south of the Polar Front and near the sea ice. Subantarctic <span class="hlt">waters</span> in Drake Passage contained 4 x 10 cells per ml with 4 to 5% FDC. Instantaneous growth rate constants ranged between 0.029 and 0.088 h. Using estimates of potential mu and measured standing stocks, we estimated productivity to range from 0.62 mug of C per liter . day in the eastern South Pacific Ocean to 17.1 mug of C per liter . day in the Drake Passage near the sea ice.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015QSRv..119...54P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015QSRv..119...54P"><span>Oceanographic variability on the West <span class="hlt">Antarctic</span> Peninsula during the Holocene and the influence of upper circumpolar deep <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>Peck, Victoria L.; Allen, Claire S.; Kender, Sev; McClymont, Erin L.; Hodgson, Dominic A.</p> <p>2015-07-01</p> <p>Recent intensification of wind-driven upwelling of warm upper circumpolar deep <span class="hlt">water</span> (UCDW) has been linked to accelerated melting of West <span class="hlt">Antarctic</span> ice shelves and glaciers. To better assess the long term relationship between UCDW upwelling and the stability of the West <span class="hlt">Antarctic</span> Ice Sheet, we present a multi-proxy reconstruction of surface and bottom <span class="hlt">water</span> conditions in Marguerite Bay, West <span class="hlt">Antarctic</span> Peninsula (WAP), through the Holocene. A combination of sedimentological, diatom and foraminiferal records are, for the first time, presented together to infer a decline in UCDW influence within Marguerite Bay through the early to mid Holocene and the dominance of cyclic forcing in the late Holocene. Extensive glacial melt, limited sea ice and enhanced primary productivity between 9.7 and 7.0 ka BP is considered to be most consistent with persistent incursions of UCDW through Marguerite Trough. From 7.0 ka BP sea ice seasons increased and productivity decreased, suggesting that UCDW influence within Marguerite Bay waned, coincident with the equatorward migration of the Southern Hemisphere Westerly Winds (SWW). UCDW influence continued through the mid Holocene, and by 4.2 ka BP lengthy sea ice seasons persisted within Marguerite Bay. Intermittent melting and reforming of this sea ice within the late Holocene may be indicative of episodic incursions of UCDW into Marguerite Bay during this period. The cyclical changes in the oceanography within Marguerite Bay during the late Holocene is consistent with enhanced sensitively to ENSO forcing as opposed to the SWW-forcing that appears to have dominated the early to mid Holocene. Current measurements of the oceanography of the WAP continental shelf suggest that the system has now returned to the early Holocene-like oceanographic configuration reported here, which in both cases has been associated with rapid deglaciation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016OcMod.104...99M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016OcMod.104...99M"><span><span class="hlt">Antarctic</span> icebergs melt over the Southern Ocean : Climatology and impact on sea ice</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Merino, Nacho; Le Sommer, Julien; Durand, Gael; Jourdain, Nicolas C.; Madec, Gurvan; Mathiot, Pierre; Tournadre, Jean</p> <p>2016-08-01</p> <p>Recent increase in <span class="hlt">Antarctic</span> freshwater release to the Southern Ocean is suggested to contribute to change in <span class="hlt">water</span> masses and sea ice. However, climate models differ in their representation of the freshwater sources. Recent improvements in altimetry-based detection of small icebergs and in estimates of the mass loss of Antarctica may help better constrain the values of <span class="hlt">Antarctic</span> freshwater releases. We propose a model-based seasonal climatology of iceberg melt over the Southern Ocean using state-of-the-art observed glaciological estimates of the <span class="hlt">Antarctic</span> mass loss. An improved version of a Lagrangian iceberg model is coupled with a global, eddy-permitting ocean/sea ice model and compared to small icebergs observations. Iceberg melt increases sea ice cover, about 10% in annual mean sea ice volume, and decreases sea surface temperature over most of the Southern Ocean, but with distinctive regional patterns. Our results underline the importance of improving the representation of <span class="hlt">Antarctic</span> freshwater sources. This can be achieved by forcing ocean/sea ice models with a climatological iceberg fresh-<span class="hlt">water</span> flux.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27670112','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27670112"><span>Microbial mercury methylation in <span class="hlt">Antarctic</span> sea ice.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gionfriddo, Caitlin M; Tate, Michael T; Wick, Ryan R; Schultz, Mark B; Zemla, Adam; Thelen, Michael P; Schofield, Robyn; Krabbenhoft, David P; Holt, Kathryn E; Moreau, John W</p> <p>2016-08-01</p> <p>Atmospheric deposition of mercury onto sea ice and circumpolar sea <span class="hlt">water</span> provides mercury for microbial methylation, and contributes to the bioaccumulation of the potent neurotoxin methylmercury in the marine food web. Little is known about the abiotic and biotic controls on microbial mercury methylation in polar marine systems. However, mercury methylation is known to occur alongside photochemical and microbial mercury reduction and subsequent volatilization. Here, we combine mercury speciation measurements of total and methylated mercury with metagenomic analysis of whole-community microbial DNA from <span class="hlt">Antarctic</span> snow, brine, sea ice and sea <span class="hlt">water</span> to elucidate potential microbially mediated mercury methylation and volatilization pathways in polar marine environments. Our results identify the marine microaerophilic bacterium Nitrospina as a potential mercury methylator within sea ice. Anaerobic bacteria known to methylate mercury were notably absent from sea-ice metagenomes. We propose that <span class="hlt">Antarctic</span> sea ice can harbour a microbial source of methylmercury in the Southern Ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29674908','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29674908"><span><span class="hlt">Antarctic</span> and Sub-<span class="hlt">Antarctic</span> Asteroidea database.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Moreau, Camille; Mah, Christopher; Agüera, Antonio; Améziane, Nadia; David Barnes; Crokaert, Guillaume; Eléaume, Marc; Griffiths, Huw; Charlène Guillaumot; Hemery, Lenaïg G; Jażdżewska, Anna; Quentin Jossart; Vladimir Laptikhovsky; Linse, Katrin; Neill, Kate; Sands, Chester; Thomas Saucède; Schiaparelli, Stefano; Siciński, Jacek; Vasset, Noémie; Bruno Danis</p> <p>2018-01-01</p> <p>The present dataset is a compilation of georeferenced occurrences of asteroids (Echinodermata: Asteroidea) in the Southern Ocean. Occurrence data south of 45°S latitude were mined from various sources together with information regarding the taxonomy, the sampling source and sampling sites when available. Records from 1872 to 2016 were thoroughly checked to ensure the quality of a dataset that reaches a total of 13,840 occurrences from 4,580 unique sampling events. Information regarding the reproductive strategy (brooders vs. broadcasters) of 63 species is also made available. This dataset represents the most exhaustive occurrence database on <span class="hlt">Antarctic</span> and Sub-<span class="hlt">Antarctic</span> asteroids.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013NatGe...6..765C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013NatGe...6..765C"><span>Dynamic behaviour of the East <span class="hlt">Antarctic</span> ice sheet during Pliocene warmth</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cook, Carys P.; van de Flierdt, Tina; Williams, Trevor; Hemming, Sidney R.; Iwai, Masao; Kobayashi, Munemasa; Jimenez-Espejo, Francisco J.; Escutia, Carlota; González, Jhon Jairo; Khim, Boo-Keun; McKay, Robert M.; Passchier, Sandra; Bohaty, Steven M.; Riesselman, Christina R.; Tauxe, Lisa; Sugisaki, Saiko; Galindo, Alberto Lopez; Patterson, Molly O.; Sangiorgi, Francesca; Pierce, Elizabeth L.; Brinkhuis, Henk; Klaus, Adam; Fehr, Annick; Bendle, James A. P.; Bijl, Peter K.; Carr, Stephanie A.; Dunbar, Robert B.; Flores, José Abel; Hayden, Travis G.; Katsuki, Kota; Kong, Gee Soo; Nakai, Mutsumi; Olney, Matthew P.; Pekar, Stephen F.; Pross, Jörg; Röhl, Ursula; Sakai, Toyosaburo; Shrivastava, Prakash K.; Stickley, Catherine E.; Tuo, Shouting; Welsh, Kevin; Yamane, Masako</p> <p>2013-09-01</p> <p>Warm intervals within the Pliocene epoch (5.33-2.58 million years ago) were characterized by global temperatures comparable to those predicted for the end of this century and atmospheric CO2 concentrations similar to today. Estimates for global sea level highstands during these times imply possible retreat of the East <span class="hlt">Antarctic</span> ice sheet, but ice-proximal evidence from the <span class="hlt">Antarctic</span> margin is scarce. Here we present new data from Pliocene marine sediments recovered offshore of Adélie Land, East Antarctica, that reveal dynamic behaviour of the East <span class="hlt">Antarctic</span> ice sheet in the vicinity of the low-lying Wilkes Subglacial Basin during times of past climatic warmth. Sedimentary sequences deposited between 5.3 and 3.3 million years ago indicate increases in Southern Ocean surface <span class="hlt">water</span> productivity, associated with elevated circum-<span class="hlt">Antarctic</span> temperatures. The geochemical provenance of detrital material deposited during these warm intervals suggests active erosion of continental bedrock from within the Wilkes Subglacial Basin, an area today buried beneath the East <span class="hlt">Antarctic</span> ice sheet. We interpret this erosion to be associated with retreat of the ice sheet margin several hundreds of kilometres inland and conclude that the East <span class="hlt">Antarctic</span> ice sheet was sensitive to climatic warmth during the Pliocene.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFMPP21B1696K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFMPP21B1696K"><span>Paleoproductivity and <span class="hlt">intermediate-water</span> ventilation in the subarctic Northwest Pacific during the last deglaciation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Khim, B.; Ikehara, K.; Sagawa, T.; Shibahara, A.; Yamamoto, M.</p> <p>2010-12-01</p> <p>Laminated sediments during the last deglaciation in the subarctic North Pacific indicate significant depletion of dissolved oxygen concentration at <span class="hlt">intermediate</span> <span class="hlt">water</span> depths. Such a strong oxygen minimum zone results primarily from a combination of high surface <span class="hlt">water</span> productivity and poor ventilation of <span class="hlt">intermediate</span> <span class="hlt">waters</span>. We investigated a variety of paleoclimatic proxies using about 8-m long piston core sediment (GH02-1030; 42o13.770N, 144o12.530E; <span class="hlt">water</span> depth, 1212 m) obtained from the continental slope off Tokachi (eastern Hokkaido Island), which is the main path of the southwestward Oyashio Current in the subarctic Northwest Pacific. Laminated sediments were identified at the two horizons in the core GH02-1030; the upper one at 11.4-12.2 cal.kyr BP and the lower one at 14.1-14.7 cal.kyr BP, corresponding to Bølling-Allerød (B/A) and Preboreal (PB), respectively. Between these laminated layers, Younger Dryas occurred. Both laminated sediment layers are characterized by Bolivina tumida, B. pacifica, and Buliminella tenuata, indicating dysoxic bottom <span class="hlt">water</span> conditions. Increased Mg/Ca-derived <span class="hlt">intermediate-water</span> temperature and δ18OW values at B/A and PB periods suggest the poor ventilation of <span class="hlt">intermediate</span> <span class="hlt">water</span> because of the surface <span class="hlt">water</span> freshening (i.e., decrease of surface-<span class="hlt">water</span> salinity). UK'37-derived temperature record also supports the increase of surface-<span class="hlt">water</span> temperature during B/A and PB intervals. During the last deglaciation, short-chain C14-C18 n-fatty acids, derived mainly from marine organisms, showed higher concentrations, indicating the increased surface-<span class="hlt">water</span> production, and at the same time, abundant lignin reflected more contribution of terrigenous organic matter, supporting increased freshwater discharge. Variation of CaCO3 contents show remarkable double peaks, corresponding to B/A and PB periods, respectively, leading to the increase of TOC contents. Opal contents also follow similar pattern to CaCO3 contents, but are much less than the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1999JGR...10420949M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1999JGR...10420949M"><span>Distribution of oxygen isotopes in the <span class="hlt">water</span> masses of Drake Passage and the 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>Meredith, Michael P.; Grose, Katie E.; McDonagh, Elaine L.; Heywood, Karen J.; Frew, Russell D.; Dennis, Paul F.</p> <p>1999-09-01</p> <p>Measurements of the ratio of stable isotopes of oxygen (18O and 16O) from samples collected on World Ocean Circulation Experiment sections SR1b (eastern Drake Passage) and A11 (Punta Arenas to Cape Town) are used, together with hydrographic data, to deduce information about the formation and variability of South Atlantic and Southern Ocean <span class="hlt">water</span> masses. The Drake Passage surface <span class="hlt">waters</span> south of the Polar Front (PF) are isotopically light (δ18O around -0.4‰) owing to the influence of meteoric <span class="hlt">waters</span>. The salinity and δ18O of the A11 surface <span class="hlt">waters</span> yield an apparent freshwater end-member which is much isotopically lighter than the local precipitation, thus advection of these <span class="hlt">waters</span> from farther south dominates over local effects in determining the surface <span class="hlt">water</span> properties. The Drake Passage section shows unusual proximity of the two main fronts of the <span class="hlt">Antarctic</span> Circumpolar Current (the PF and Subantarctic Front (SAF)), and we observe cold, fresh, and isotopically light <span class="hlt">water</span> derived from the temperature-minimum Winter <span class="hlt">Water</span> at the SAF. This <span class="hlt">water</span> is of the correct density to freshen the <span class="hlt">intermediate</span> <span class="hlt">water</span> north of the SAF and thus play a role in the formation of the comparatively fresh <span class="hlt">Antarctic</span> <span class="hlt">Intermediate</span> <span class="hlt">Water</span> (AAIW) of the South Atlantic. This confirms the role of <span class="hlt">Antarctic</span> <span class="hlt">water</span> in forming the South Atlantic variety of AAIW. Across the A11 section the oxygen isotope and salinity data at the AAIW core show very similar traces, with <span class="hlt">waters</span> in the Malvinas Current loop showing lowest values of both. At the eastern boundary of the South Atlantic, the input of Red Sea <span class="hlt">Water</span> from east of South Africa is observed via the presence of anomalously isotopically heavy AAIW. We deduce potentially significant temporal variability in the isotopic composition of Weddell Sea Deep <span class="hlt">Water</span> (WSDW) by comparing the Drake Passage data to earlier data covering the outflow of the Weddell Sea. The A11 data show WSDW consistent with such variability, indicating that its effects could</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170008477','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170008477"><span>Improving Our Understanding of <span class="hlt">Antarctic</span> Sea Ice with NASA's Operation IceBridge and the Upcoming ICESat-2 Mission</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Petty, Alek A.; Markus, Thorsten; Kurtz, Nathan T.</p> <p>2017-01-01</p> <p><span class="hlt">Antarctic</span> sea ice is a crucial component of the global climate system. Rapid sea ice production regimes around Antarctica feed the lower branch of the Southern Ocean overturning circulation through intense brine rejection and the formation of <span class="hlt">Antarctic</span> Bottom <span class="hlt">Water</span> (e.g., Orsi et al. 1999; Jacobs 2004), while the northward transport and subsequent melt of <span class="hlt">Antarctic</span> sea ice drives the upper branch of the overturning circulation through freshwater input (Abernathy et al. 2016). Wind-driven trends in <span class="hlt">Antarctic</span> sea ice (Holland Kwok 2012) have likely increased the transport of freshwater away from the <span class="hlt">Antarctic</span> coastline, significantly altering the salinity distribution of the Southern Ocean (Haumann et al. 2016). Conversely, weaker sea ice production and the lack of shelf <span class="hlt">water</span> formation over the Amundsen and Bellingshausen shelf seas promote intrusion of warm Circumpolar Deep <span class="hlt">Water</span> onto the continental shelf and the ocean-driven melting of several ice shelves fringing the West <span class="hlt">Antarctic</span> Ice Sheet (e.g., Jacobs et al. 2011; Pritchard et al. 2012; Dutrieux et al. 2014). Sea ice conditions around Antarctica are also increasingly considered an important factor impacting local atmospheric conditions and the surface melting of <span class="hlt">Antarctic</span> ice shelves (e.g., Scambos et al. 2017). Sea ice formation around Antarctica is responsive to the strong regional variability in atmospheric forcing present around Antarctica, driving this bimodal variability in the behavior and properties of the underlying shelf seas (e.g., Petty et al. 2012; Petty et al. 2014).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.7117S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.7117S"><span>Warm <span class="hlt">water</span> and life beneath the grounding zone of an <span class="hlt">Antarctic</span> outlet glacier</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sugiyama, Shin; Sawagaki, Takanobu; Fukuda, Takehiro</p> <p>2013-04-01</p> <p>Ice-ocean interaction plays a key role in rapidly changing <span class="hlt">Antarctic</span> ice sheet margins. Recent studies demonstrated that warming ocean is eroding floating part of the ice sheet, resulting in thinning, retreat and acceleration of ice shelves and outlet glaciers. Field data are necessary to understand such processes, but direct observations at the interface of ice and the ocean are lacking, particularly beneath the grounding zone. To better understand the interaction of <span class="hlt">Antarctic</span> ice sheet and the ocean, we performed subglacial measurements through boreholes drilled in the grounding zone of Langhovde Glacier, an outlet glacier in East Antarctica. Langhovde Glacier is located at 69°12'S, 39°48'E, approximately 20 km south of a Japanese research station Syowa. The glacier discharges ice into Lützow-holm Bay through a 3-km-wide floating terminus at a rate of 130 m a-1. Fast flowing feature is confined by bedrock to the west and slow moving ice to the east, and it extends about 10 km upglacier from the calving front. In 2011/12 austral summer season, we operated a hot <span class="hlt">water</span> drilling system to drill through the glacier at 2.5 and 3 km from the terminus. Inspections of the boreholes revealed the ice was underlain by a shallow saline <span class="hlt">water</span> layer. Ice and <span class="hlt">water</span> column thicknesses were found to be 398 and 24 m at the first site, and 431 and 10 m at the second site. Judging from ice surface and bed elevations, the drilling sites were situated at within a several hundred meters from the grounding line. Sensors were lowered into the boreholes to measure temperature, salinity and current within the subglacial <span class="hlt">water</span> layer. Salinity and temperature from the two sites were fairly uniform (34.25±0.05 PSU and -1.45±0.05°C), indicating vertical and horizontal mixing in the layer. The measured temperature was >0.7°C warmer than the in-situ freezing point, and very similar to the values measured in the open ocean near the glacier front. Subglacial current was up to 3 cm/s, which</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017DSRII.139..120P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017DSRII.139..120P"><span>Coastal barium cycling at the West <span class="hlt">Antarctic</span> Peninsula</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pyle, K. M.; Hendry, K. R.; Sherrell, R. M.; Meredith, M. P.; Venables, H.; Lagerström, M.; Morte-Ródenas, A.</p> <p>2017-05-01</p> <p>Barium cycling in the ocean is associated with a number of processes, including the production and recycling of organic matter, freshwater fluxes, and phenomena that affect alkalinity. As a result, the biogeochemical cycle of barium offers insights into past and present oceanic conditions, with barium currently used in various forms as a palaeoproxy for components of organic and inorganic carbon storage, and as a quasi-conservative <span class="hlt">water</span> mass tracer. However, the nature of the oceanic barium cycle is not fully understood, particularly in cases where multiple processes may be interacting simultaneously with the dissolved and particulate barium pools. This is particularly the case in coastal polar regions such as the West <span class="hlt">Antarctic</span> Peninsula, where biological drawdown and remineralisation occur in tandem with sea ice formation and melting, glacial meltwater input, and potential fluxes from shelf sediments. Here, we use a high-precision dataset of dissolved barium (Bad) from a grid of stations adjacent to the West <span class="hlt">Antarctic</span> Peninsula in conjunction with silicic acid (Si(OH)4), the oxygen isotope composition of <span class="hlt">water</span>, and salinity measurements, to determine the relative control of various coastal processes on the barium cycle throughout the <span class="hlt">water</span> column. There is a strong correlation between Bad and Si(OH)4 present in deeper samples, but nevertheless persists significantly in surface <span class="hlt">waters</span>. This indicates that the link between biogenic opal and barium is not solely due to barite precipitation and dissolution at depth, but is supplemented by an association between Bad and diatom tests in surface <span class="hlt">waters</span>, possibly due to barite formation within diatom-dominated phytodetritus present in the photic zone. Sea-ice meltwater appears to exert a significant secondary control on barium concentrations, likely due to non-conservative biotic or abiotic processes acting as a sink for Bad within the sea ice itself, or sea-ice meltwater stimulating non-siliceous productivity that acts</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003AGUFMPP31C0272S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003AGUFMPP31C0272S"><span>The <span class="hlt">Antarctic</span> Master Directory -- the Electronic Card Catalog of <span class="hlt">Antarctic</span> Data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Scharfen, G.; Bauer, R.</p> <p>2003-12-01</p> <p>The <span class="hlt">Antarctic</span> Master Directory (AMD) is a Web-based, searchable record of thousands of <span class="hlt">Antarctic</span> data descriptions. These data descriptions contain information about what data were collected, where they were collected, when they were collected, who the scientists are, who the point of contact is, how to get the data, and information about the format of the data and what documentation and bibliographic information exists. With this basic descriptive information about content and access for thousands of <span class="hlt">Antarctic</span> scientific data sets, the AMD is a resource for scientists to advertise the data they have collected and to search for data they need. The AMD has been created by more than twenty nations which conduct research in the <span class="hlt">Antarctic</span> under the auspices of the <span class="hlt">Antarctic</span> Treaty. It is a part of the International Directory Network/Global Change Master Directory (IDN/GCMD). Using the AMD is easy. Users can search on subject matter key words, data types, geographic place-names, temporal or spatial ranges, or conduct free-text searches. To search the AMD go to: http://gcmd.nasa.gov/Data/portals/amd/. Contributing your own data descriptions for <span class="hlt">Antarctic</span> data that you have collected is also easy. Scientists can start by submitting a short data description first (as a placeholder in the AMD, and to satisfy National Science Foundation (NSF) reporting requirements), and then add to, modify or update their record whenever it is appropriate. An easy to use on-line tool and a simple tutorial are available at: http://nsidc.org/usadcc. With NSF Office of Polar Programs (OPP) funding, the National Snow and Ice Data Center (NSIDC) operates the U.S. <span class="hlt">Antarctic</span> Data Coordination Center (USADCC), partly to assist scientists in using and contributing to the AMD. The USADCC website is at http://nsidc.org/usadcc.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li class="active"><span>7</span></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_7 --> <div id="page_8" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li class="active"><span>8</span></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="141"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUFM.P52A..05D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFM.P52A..05D"><span>Environmentally Non-Disturbing Under-ice Robotic <span class="hlt">ANtarctiC</span> Explorer (ENDURANCE)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Doran, P. T.; Stone, W.; Priscu, J.; McKay, C.; Johnson, A.; Chen, B.</p> <p>2007-12-01</p> <p>Permanently ice-covered liquid <span class="hlt">water</span> environments are among the leading candidate sites for finding evidence of extant life elsewhere in our solar system (e.g. on Europa and other Galiean satellites, and possibly in subglacial lakes on Mars). In order to have the proper tools and strategies for exploring the extant ice-covered planetary environments, we are developing an autonomous underwater vehicle (AUV) capable of generating for the first time 3-D biogeochemical datasets in the extreme environment of perennially ice-covered <span class="hlt">Antarctic</span> dry valley lakes. The ENDURANCE (Environmentally Non-Disturbing Under-ice Robotic <span class="hlt">ANtarctic</span> Explorer) will map the under-ice lake dimensions of West Lake Bonney in the McMurdo Dry Valleys, and be equipped to measure a comprehensive suite of physical and biogeochemical indices in the <span class="hlt">water</span> column, as well as Raman Spectrometry of the <span class="hlt">water</span> column and benthos. The AUV is being specifically designed to minimize impact on the environment it is working in. This is primarily to meet strict <span class="hlt">Antarctic</span> environmental protocols, but will also be useful for planetary protection and improved science in the future. We will carry out two <span class="hlt">Antarctic</span> field seasons (in concert with our NSF-funded Long Term Ecological Research) and test two central hypotheses: H1: The low kinetic energy of the system (diffusion dominates the spatial transport of constituents) produces an ecosystem and ecosystem limits that vary significantly in three dimensions. H2: The whole-lake physical and biogeochemical structure remains static from year to year The talk will provide an overview of the ENDURANCE project and an update on the AUV development at the time of presentation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24039844','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24039844"><span>Calling in the cold: pervasive acoustic presence of humpback whales (Megaptera novaeangliae) in <span class="hlt">Antarctic</span> coastal <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>Van Opzeeland, Ilse; Van Parijs, Sofie; Kindermann, Lars; Burkhardt, Elke; Boebel, Olaf</p> <p>2013-01-01</p> <p>Humpback whales migrate between relatively unproductive tropical or temperate breeding grounds and productive high latitude feeding areas. However, not all individuals of a population undertake the annual migration to the breeding grounds; instead some are thought to remain on the feeding grounds year-round, presumably to avoid the energetic demands of migration. In the Southern Hemisphere, ice and inclement weather conditions restrict investigations of humpback whale presence on feeding grounds as well as the extent of their southern range. Two years of near-continuous recordings from the PerenniAL Acoustic Observatory in the <span class="hlt">Antarctic</span> Ocean (PALAOA, Ekström Iceshelf, 70°31'S, 8°13'W) are used to explore the acoustic presence of humpback whales in an <span class="hlt">Antarctic</span> coastal area. Humpback whale calls were present during nine and eleven months of 2008 and 2009, respectively. In 2008, calls were present in January through April, June through August, November and December, whereas in 2009, calls were present throughout the year, except in September. Calls occurred in un-patterned sequences, representing non-song sound production. Typically, calls occurred in bouts, ranging from 2 to 42 consecutive days with February, March and April having the highest daily occurrence of calls in 2008. In 2009, February, March, April and May had the highest daily occurrence of calls. Whales were estimated to be within a 100 km radius off PALAOA. Calls were also present during austral winter when ice cover within this radius was >90%. These results demonstrate that coastal areas near the <span class="hlt">Antarctic</span> continent are likely of greater importance to humpback whales than previously assumed, presumably providing food resources year-round and open <span class="hlt">water</span> in winter where animals can breathe.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1997amc..book.....K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1997amc..book.....K"><span><span class="hlt">Antarctic</span> Meteorology and Climatology</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>King, J. C.; Turner, J.</p> <p>1997-07-01</p> <p>This book is a comprehensive survey of the climatology and meteorology of Antarctica. The first section of the book reviews the methods by which we can observe the <span class="hlt">Antarctic</span> atmosphere and presents a synthesis of climatological measurements. In the second section, the authors consider the processes that maintain the observed climate, from large-scale atmospheric circulation to small-scale processes. The final section reviews our current knowledge of the variability of <span class="hlt">Antarctic</span> climate and the possible effects of "greenhouse" warming. The authors stress links among the <span class="hlt">Antarctic</span> atmosphere, other elements of the <span class="hlt">Antarctic</span> climate system (oceans, sea ice and ice sheets), and the global climate system. This volume will be of greatest interest to meteorologists and climatologists with a specialized interest in Antarctica, but it will also appeal to researchers in <span class="hlt">Antarctic</span> glaciology, oceanography and biology. Graduates and undergraduates studying physical geography, and the earth, atmospheric and environmental sciences will find much useful background material in the book.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AcAau.131...50S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AcAau.131...50S"><span><span class="hlt">Antarctic</span> station life: The first 15 years of mixed expeditions to the <span class="hlt">Antarctic</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sarris, Aspa</p> <p>2017-02-01</p> <p>This study examined the experiences of women who lived and worked on remote and isolated <span class="hlt">Antarctic</span> stations for up to 15 months at a time. The study employed purposeful sampling and a longitudinal - processual approach to study women's experiences over the first 15 years of mixed gender <span class="hlt">Antarctic</span> expeditions. The retrospective analysis was based on a semi-structured interview administered to 14 women upon their return to Australia. The results showed that women referred to the natural physical <span class="hlt">Antarctic</span> environment as one of the best aspects of their experience and the reason they would recommend the <span class="hlt">Antarctic</span> to their friends as a good place to work. In describing the worst aspect of their experience, women referred to aspects of <span class="hlt">Antarctic</span> station life, including: (i) the male dominated nature of station culture; (ii) the impact of interpersonal conflict, including gender based conflict and friction between scientists and trades workers; and (iii) the lack of anonymity associated with living and working with the same group of individuals, mainly men, for up to 12 months or more. The results are discussed within the context of the evolution of <span class="hlt">Antarctic</span> station culture and recommendations are made in terms of the demography of expeditions, expeditioner selection and recruitment and the ongoing monitoring of <span class="hlt">Antarctic</span> station culture. The study presents a framework that can be applied to groups and teams living and working in analogous isolated, confined and extreme work environments, including outer space missions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19910031947&hterms=History+Genetics&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3DHistory%2BGenetics','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19910031947&hterms=History+Genetics&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3DHistory%2BGenetics"><span>Chemical studies of differentiated meteorites. I - Labile trace elements in <span class="hlt">Antarctic</span> and non-<span class="hlt">Antarctic</span> eucrites</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Paul, Rick L.; Lipschutz, Michael E.</p> <p>1990-01-01</p> <p>Element contents of Ag, Au, Bi, Cd, Co, Cs, Ga, In, Rb, Sb, Se, Te, Tl, U, and Zn were analyzed, using RNAA, in 25 <span class="hlt">Antarctic</span> and nine non-<span class="hlt">Antarctic</span> eucrites to determine whether these two populations differ significantly in thermal history and derive from the same or different eucrite parent body. Data for these 15 elements indicate that basaltic <span class="hlt">Antarctic</span> and non-<span class="hlt">Antarctic</span> eucrite populations reflect the same genetic processes and, hence, come from the same parent asteroid.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://pubs.water.usgs.gov/wri024009+','USGSPUBS'); return false;" href="http://pubs.water.usgs.gov/wri024009+"><span>Simulation of ground-<span class="hlt">water</span> flow in the <span class="hlt">Intermediate</span> and Floridan aquifer systems in Peninsular Florida</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Sepúlveda, Nicasio</p> <p>2002-01-01</p> <p>A numerical model of the <span class="hlt">intermediate</span> and Floridan aquifer systems in peninsular Florida was used to (1) test and refine the conceptual understanding of the regional ground-<span class="hlt">water</span> flow system; (2) develop a data base to support subregional ground-<span class="hlt">water</span> flow modeling; and (3) evaluate effects of projected 2020 ground-<span class="hlt">water</span> withdrawals on ground-<span class="hlt">water</span> levels. The four-layer model was based on the computer code MODFLOW-96, developed by the U.S. Geological Survey. The top layer consists of specified-head cells simulating the surficial aquifer system as a source-sink layer. The second layer simulates the <span class="hlt">intermediate</span> aquifer system in southwest Florida and the <span class="hlt">intermediate</span> confining unit where it is present. The third and fourth layers simulate the Upper and Lower Floridan aquifers, respectively. Steady-state ground-<span class="hlt">water</span> flow conditions were approximated for time-averaged hydrologic conditions from August 1993 through July 1994 (1993-94). This period was selected based on data from Upper Floridan a quifer wells equipped with continuous <span class="hlt">water</span>-level recorders. The grid used for the ground-<span class="hlt">water</span> flow model was uniform and composed of square 5,000-foot cells, with 210 columns and 300 rows.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012E%26PSL.325..108L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012E%26PSL.325..108L"><span>An ikaite record of late Holocene climate at the <span class="hlt">Antarctic</span> Peninsula</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lu, Zunli; Rickaby, Rosalind E. M.; Kennedy, Hilary; Kennedy, Paul; Pancost, Richard D.; Shaw, Samuel; Lennie, Alistair; Wellner, Julia; Anderson, John B.</p> <p>2012-04-01</p> <p>Calcium carbonate can crystallize in a hydrated form as ikaite at low temperatures. The hydration <span class="hlt">water</span> in ikaite grown in laboratory experiments records the δ18O of ambient <span class="hlt">water</span>, a feature potentially useful for reconstructing δ18O of local seawater. We report the first downcore δ18O record of natural ikaite hydration <span class="hlt">waters</span> and crystals collected from the <span class="hlt">Antarctic</span> Peninsula (AP), a region sensitive to climate fluctuations. We are able to establish the zone of ikaite formation within shallow sediments, based on porewater chemical and isotopic data. Having constrained the depth of ikaite formation and δ18O of ikaite crystals and hydration <span class="hlt">waters</span>, we are able to infer local changes in fjord δ18O versus time during the late Holocene. This ikaite record qualitatively supports that both the Medieval Warm Period and Little Ice Age extended to the <span class="hlt">Antarctic</span> Peninsula.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27509536','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27509536"><span>Fate of Polycyclic Aromatic Hydrocarbons in Seawater from the Western Pacific to the Southern Ocean (17.5°N to 69.2°S) and Their Inventories on the <span class="hlt">Antarctic</span> Shelf.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Cai, Minggang; Liu, Mengyang; Hong, Qingquan; Lin, Jing; Huang, Peng; Hong, Jiajun; Wang, Jun; Zhao, Wenlu; Chen, Meng; Cai, Minghong; Ye, Jun</p> <p>2016-09-06</p> <p>Semivolatile organic compounds such as polycyclic aromatic hydrocarbons (PAHs) have the potential to reach pristine environments through long-range transport. To investigate the long-range transport of the PAHs and their fate in <span class="hlt">Antarctic</span> seawater, dissolved PAHs in the surface <span class="hlt">waters</span> from the western Pacific to the Southern Ocean (17.5°N to 69.2°S), as well as down to 3500 m PAH profiles in Prydz Bay and the adjacent Southern Ocean, were observed during the 27th Chinese National <span class="hlt">Antarctic</span> Research Expedition in 2010. The concentrations of Σ9PAH in the surface seawater ranged from not detected (ND) to 21 ng L(-1), with a mean of 4.3 ng L(-1); and three-ring PAHs were the most abundant compounds. Samples close to the Australian mainland displayed the highest levels across the cruise. PAHs originated mainly from pyrogenic sources, such as grass, wood, and coal combustion. Vertical profiles of PAHs in Prydz Bay showed a maximum at a depth of 50 m and less variance with depth. In general, we inferred that the <span class="hlt">water</span> masses as well as the phytoplankton were possible influencing factors on PAH surface-enrichment depth-depletion distribution. Inventory estimation highlighted the contribution of <span class="hlt">intermediate</span> and deep seawater on storing PAHs in seawater from Prydz Bay, and suggested that climate change rarely shows the rapid release of the PAHs currently stored in the major reservoirs (<span class="hlt">intermediate</span> and deep seawater).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=analysis+AND+climatic&pg=2&id=EJ321613','ERIC'); return false;" href="https://eric.ed.gov/?q=analysis+AND+climatic&pg=2&id=EJ321613"><span>The <span class="hlt">Antarctic</span> Ice.</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>Radok, Uwe</p> <p>1985-01-01</p> <p>The International <span class="hlt">Antarctic</span> Glaciological Project has collected information on the East <span class="hlt">Antarctic</span> ice sheet since 1969. Analysis of ice cores revealed climatic history, and radar soundings helped map bedrock of the continent. Computer models of the ice sheet and its changes over time will aid in predicting the future. (DH)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19295607','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19295607"><span>Obliquity-paced Pliocene West <span class="hlt">Antarctic</span> ice sheet oscillations.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Naish, T; Powell, R; Levy, R; Wilson, G; Scherer, R; Talarico, F; Krissek, L; Niessen, F; Pompilio, M; Wilson, T; Carter, L; DeConto, R; Huybers, P; McKay, R; Pollard, D; Ross, J; Winter, D; Barrett, P; Browne, G; Cody, R; Cowan, E; Crampton, J; Dunbar, G; Dunbar, N; Florindo, F; Gebhardt, C; Graham, I; Hannah, M; Hansaraj, D; Harwood, D; Helling, D; Henrys, S; Hinnov, L; Kuhn, G; Kyle, P; Läufer, A; Maffioli, P; Magens, D; Mandernack, K; McIntosh, W; Millan, C; Morin, R; Ohneiser, C; Paulsen, T; Persico, D; Raine, I; Reed, J; Riesselman, C; Sagnotti, L; Schmitt, D; Sjunneskog, C; Strong, P; Taviani, M; Vogel, S; Wilch, T; Williams, T</p> <p>2009-03-19</p> <p>Thirty years after oxygen isotope records from microfossils deposited in ocean sediments confirmed the hypothesis that variations in the Earth's orbital geometry control the ice ages, fundamental questions remain over the response of the <span class="hlt">Antarctic</span> ice sheets to orbital cycles. Furthermore, an understanding of the behaviour of the marine-based West <span class="hlt">Antarctic</span> ice sheet (WAIS) during the 'warmer-than-present' early-Pliocene epoch ( approximately 5-3 Myr ago) is needed to better constrain the possible range of ice-sheet behaviour in the context of future global warming. Here we present a marine glacial record from the upper 600 m of the AND-1B sediment core recovered from beneath the northwest part of the Ross ice shelf by the ANDRILL programme and demonstrate well-dated, approximately 40-kyr cyclic variations in ice-sheet extent linked to cycles in insolation influenced by changes in the Earth's axial tilt (obliquity) during the Pliocene. Our data provide direct evidence for orbitally induced oscillations in the WAIS, which periodically collapsed, resulting in a switch from grounded ice, or ice shelves, to open <span class="hlt">waters</span> in the Ross embayment when planetary temperatures were up to approximately 3 degrees C warmer than today and atmospheric CO(2) concentration was as high as approximately 400 p.p.m.v. (refs 5, 6). The evidence is consistent with a new ice-sheet/ice-shelf model that simulates fluctuations in <span class="hlt">Antarctic</span> ice volume of up to +7 m in equivalent sea level associated with the loss of the WAIS and up to +3 m in equivalent sea level from the East <span class="hlt">Antarctic</span> ice sheet, in response to ocean-induced melting paced by obliquity. During interglacial times, diatomaceous sediments indicate high surface-<span class="hlt">water</span> productivity, minimal summer sea ice and air temperatures above freezing, suggesting an additional influence of surface melt under conditions of elevated CO(2).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22538614','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22538614"><span><span class="hlt">Antarctic</span> ice-sheet loss driven by basal melting of ice shelves.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Pritchard, H D; Ligtenberg, S R M; Fricker, H A; Vaughan, D G; van den Broeke, M R; Padman, L</p> <p>2012-04-25</p> <p>Accurate prediction of global sea-level rise requires that we understand the cause of recent, widespread and intensifying glacier acceleration along <span class="hlt">Antarctic</span> ice-sheet coastal margins. Atmospheric and oceanic forcing have the potential to reduce the thickness and extent of floating ice shelves, potentially limiting their ability to buttress the flow of grounded tributary glaciers. Indeed, recent ice-shelf collapse led to retreat and acceleration of several glaciers on the <span class="hlt">Antarctic</span> Peninsula. But the extent and magnitude of ice-shelf thickness change, the underlying causes of such change, and its link to glacier flow rate are so poorly understood that its future impact on the ice sheets cannot yet be predicted. Here we use satellite laser altimetry and modelling of the surface firn layer to reveal the circum-<span class="hlt">Antarctic</span> pattern of ice-shelf thinning through increased basal melt. We deduce that this increased melt is the primary control of <span class="hlt">Antarctic</span> ice-sheet loss, through a reduction in buttressing of the adjacent ice sheet leading to accelerated glacier flow. The highest thinning rates occur where warm <span class="hlt">water</span> at depth can access thick ice shelves via submarine troughs crossing the continental shelf. Wind forcing could explain the dominant patterns of both basal melting and the surface melting and collapse of <span class="hlt">Antarctic</span> ice shelves, through ocean upwelling in the Amundsen and Bellingshausen seas, and atmospheric warming on the <span class="hlt">Antarctic</span> Peninsula. This implies that climate forcing through changing winds influences <span class="hlt">Antarctic</span> ice-sheet mass balance, and hence global sea level, on annual to decadal timescales.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19900017424','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19900017424"><span>Proceedings of a workshop on Differences Between <span class="hlt">Antarctic</span> and Non-<span class="hlt">Antarctic</span> Meteorites</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Koeberl, Christian (Editor); Cassidy, William A. (Editor)</p> <p>1989-01-01</p> <p>The known facts, together with new research results are reviewed, in order to examine apparent differences between the <span class="hlt">Antarctic</span> and non-<span class="hlt">Antarctic</span> populations. In view of the statistically significant number of <span class="hlt">Antarctic</span> meteorites, and the existence of rare or previously unknown types of meteorites among the <span class="hlt">Antarctic</span> meteorite collection, the question was really not so much whether there are differences, but to define which ones are significant and what their origin is. Two main causes for the possible differences have been suggested previously, namely differences in the meteorite parent populations and secondary effects (e.g., weathering). The workshop was structured to contain sessions on chemical, isotopic, petrological, and mineralogical studies of meteorites from the two collections; terrestrial age determinations; discussions on mass frequency distributions; relative abundances of meteorite types; and terrestrial meteorite flux rates and their possible changes with time.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFMPP51A1819L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFMPP51A1819L"><span>An ikaite record of late Holocene climate at the <span class="hlt">Antarctic</span> Peninsula</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lu, Z.; Rickaby, R. E.; Kennedy, H.; Pancost, R. D.; Shaw, S.; Lennie, A. R.; Wellner, J. S.; Anderson, J. B.</p> <p>2011-12-01</p> <p>Ikaite is a low temperature polymorph of calcium carbonate which is hydrated with <span class="hlt">water</span> molecules contained in its crystal lattice (CaCO3:6H2O). Ikaite is thought to rapidly decompose into calcite and <span class="hlt">water</span> at temperatures above 4°C. The hydration <span class="hlt">water</span> in ikaite grown in laboratory experiments records the δ18O of ambient <span class="hlt">water</span>, a feature potentially useful for reconstructing δ18O of local seawater. The most recent melting of the Caley Glacier on the <span class="hlt">Antarctic</span> Peninsula (AP) during last few decades released meltwater into nearby fjords and left a strong signal of light δ18O values in shallow porewater profiles. If ikaite crystals incorporate ambient porewaters into crystal structure as the hydration <span class="hlt">water</span>, then crystals grown at different times will record the changes in bottom <span class="hlt">water</span> δ18O due to waxing and waning of (global or local) ice-sheets. U.S. <span class="hlt">Antarctic</span> Program cruise NBP0703 collected piston cores around the AP and found ikaite crystals in multiple horizons at the Firth of Tay, suitable for reconstructing a low resolution ikaite record of the last 2000 years. We report the first downcore δ18O record of natural ikaite hydration <span class="hlt">waters</span> and crystals collected from the AP, a region sensitive to climate fluctuations. We are able to establish the zone of ikaite formation within shallow sediments and derive a climatic signal, related to local changes in fjord δ18O, versus time encoded in this late Holocene ikaite record. Our interpretation, based on ikaite isotopes, provides additional qualitative evidence that both the Medieval Warm Period and Little Ice Age were extended to the Southern Ocean and the <span class="hlt">Antarctic</span> Peninsula.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19880033434&hterms=chloride&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dchloride','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19880033434&hterms=chloride&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dchloride"><span>Reaction of chlorine nitrate with hydrogen chloride and <span class="hlt">water</span> at <span class="hlt">Antarctic</span> stratospheric temperatures</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Tolbert, Margaret A.; Rossi, Michel J.; Malhotra, Ripudaman; Golden, David M.</p> <p>1987-01-01</p> <p>Laboratory studies of heterogeneous reactions important for ozone depletion over Antarctica are reported. The reaction of chlorine nitrate (ClONO2) with H2O and HCl on surfacers that simulate polar stratospheric clouds are studied at temperatures relevant to the <span class="hlt">Antarctic</span> stratosphere. The gaseous products of the resulting reactions, HOCl, Cl2O, and Cl2, could readily photolyze in the <span class="hlt">Antarctic</span> spring to produce active chlorine for ozone depletion. Furthermore, the additional formation of condensed-phase HNO3 could serve as a sink for odd nitrogen species that would otherwise scavenge the active chlorine.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3765206','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3765206"><span>Calling in the Cold: Pervasive Acoustic Presence of Humpback Whales (Megaptera novaeangliae) in <span class="hlt">Antarctic</span> Coastal <span class="hlt">Waters</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>Van Opzeeland, Ilse; Van Parijs, Sofie; Kindermann, Lars; Burkhardt, Elke; Boebel, Olaf</p> <p>2013-01-01</p> <p>Humpback whales migrate between relatively unproductive tropical or temperate breeding grounds and productive high latitude feeding areas. However, not all individuals of a population undertake the annual migration to the breeding grounds; instead some are thought to remain on the feeding grounds year-round, presumably to avoid the energetic demands of migration. In the Southern Hemisphere, ice and inclement weather conditions restrict investigations of humpback whale presence on feeding grounds as well as the extent of their southern range. Two years of near-continuous recordings from the PerenniAL Acoustic Observatory in the <span class="hlt">Antarctic</span> Ocean (PALAOA, Ekström Iceshelf, 70°31’S, 8°13’W) are used to explore the acoustic presence of humpback whales in an <span class="hlt">Antarctic</span> coastal area. Humpback whale calls were present during nine and eleven months of 2008 and 2009, respectively. In 2008, calls were present in January through April, June through August, November and December, whereas in 2009, calls were present throughout the year, except in September. Calls occurred in un-patterned sequences, representing non-song sound production. Typically, calls occurred in bouts, ranging from 2 to 42 consecutive days with February, March and April having the highest daily occurrence of calls in 2008. In 2009, February, March, April and May had the highest daily occurrence of calls. Whales were estimated to be within a 100 km radius off PALAOA. Calls were also present during austral winter when ice cover within this radius was >90%. These results demonstrate that coastal areas near the <span class="hlt">Antarctic</span> continent are likely of greater importance to humpback whales than previously assumed, presumably providing food resources year-round and open <span class="hlt">water</span> in winter where animals can breathe. PMID:24039844</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70020522','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70020522"><span>Comparison of two stable hydrogen isotope-ratio measurement techniques on <span class="hlt">Antarctic</span> surface-<span class="hlt">water</span> and ice samples</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Hopple, J.A.; Hannon, J.E.; Coplen, T.B.</p> <p>1998-01-01</p> <p>A comparison of the new hydrogen isotope-ratio technique of Vaughn et al. ([Vaughn, B.H., White, J.W.C., Delmotte, M., Trolier, M., Cattani, O., Stievenard, M., 1998. An automated system for hydrogen isotope analysis of <span class="hlt">water</span>. Chem. Geol. (Isot. Geosci. Sect.), 152, 309-319]; the article immediately preceding this article) for the analysis of <span class="hlt">water</span> samples utilizing automated on-line reduction by elemental uranium showed that 94% of 165 samples of <span class="hlt">Antarctic</span> snow, ice, and stream <span class="hlt">water</span> agreed with the ??2H values determined by H2-H2O platinum equilibration, exhibiting a bias of +0.5??? and a 2 - ?? variation of 1.9???. The isotopic results of 10 reduction technique samples, however, gave ??2H values that differed by 3.5??? or more, and were too negative by as much as 5.4??? and too positive by as much as 4.9??? with respect to those determined using the platinum equilibration technique.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20130009736','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20130009736"><span>Subsurface Salts in <span class="hlt">Antarctic</span> Dry Valley Soils</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Englert, P.; Bishop, J. L.; Gibson, E. K.; Koeberl, C.</p> <p>2013-01-01</p> <p>The distribution of <span class="hlt">water</span>-soluble ions, major and minor elements, and other parameters were examined to determine the extent and effects of chemical weathering on cold desert soils. Patterns at the study sites support theories of multiple salt forming processes, including marine aerosols and chemical weathering of mafic minerals. Periodic solar-mediated ionization of atmospheric nitrogen might also produce high nitrate concentrations found in older sediments. Chemical weathering, however, was the major contributor of salts in <span class="hlt">Antarctic</span> Dry Valleys. The <span class="hlt">Antarctic</span> Dry Valleys represent a unique analog for Mars, as they are extremely cold and dry desert environments. Similarities in the climate, surface geology, and chemical properties of the Dry Valleys to that of Mars imply the possible presence of these soil formation mechanisms on Mars, other planets and icy satellites.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T31C0636P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T31C0636P"><span>Geophysical Investigation of Upper Mantle Anomalies of the Australian-<span class="hlt">Antarctic</span> Ridge</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Park, S. H.; Choi, H.; Kim, S. S.; Lin, J.</p> <p>2017-12-01</p> <p>Australian-<span class="hlt">Antarctic</span> Ridge (AAR) is situated between the Pacific-<span class="hlt">Antarctic</span> Ridge (PAR) and Southeast Indian Ridge (SEIR), extending eastward from the Australian-<span class="hlt">Antarctic</span> Discordance (AAD). Much of the AAR has been remained uncharted until 2011 because of its remoteness and harsh weather conditions. Since 2011, four multidisciplinary expeditions initiated by the Korea Polar Research Institute (KOPRI) have surveyed the little-explored eastern ends of the AAR and investigated the tectonics, geochemistry, and hydrothermal activity of this <span class="hlt">intermediate</span> spreading system. Recent isotope studies using the new basalt samples from the AAR have led to the new hypothesis of the Southern Ocean mantle domain (SOM), which may have originated from the super-plume activity associated with the Gondwana break-up. In this study, we characterize the geophysics of the Southern Ocean mantle using the newly acquired shipboard bathymetry and available geophysical datasets. First, we computed residual mantle Bouguer gravity anomalies (RMBA), gravity-derived crustal thickness, and residual topography along the AAR in order to obtain a geological proxy for regional variations in magma supply. The results of these analyses revealed that the southern flank of the AAR is associated with shallower seafloor, more negative RMBA, thicker crust, and/or less dense mantle in comparison to the conjugate northern flank. Furthermore, this north-south asymmetry becomes more prominent toward the central ridge segments of the AAR. Interestingly, the along-axis depths of the entire AAR are significantly shallower than the neighboring ridge systems and the global ridges of <span class="hlt">intermediate</span> spreading rates. Such shallow depths are also correlated with regional negative geoid anomalies. Furthermore, recent mantle tomography models consistently showed that the upper mantle (< 250 km) below the AAR has low S-wave velocities, suggesting that it may be hotter than the nearby ridges. Such regional-scale anomalies of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JGRC..119.5690K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JGRC..119.5690K"><span>Pathways of basal meltwater from <span class="hlt">Antarctic</span> ice shelves: A model study</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kusahara, Kazuya; Hasumi, Hiroyasu</p> <p>2014-09-01</p> <p>We investigate spreading pathways of basal meltwater released from all <span class="hlt">Antarctic</span> ice shelves using a circumpolar coupled ice shelf-sea ice-ocean model that reproduces major features of the Southern Ocean circulation, including the <span class="hlt">Antarctic</span> Circumpolar Current (ACC). Several independent virtual tracers are used to identify detailed pathways of basal meltwaters. The spreading pathways of the meltwater tracers depend on formation sites, because the meltwaters are transported by local ambient ocean circulation. Meltwaters from ice shelves in the Weddell and Amundsen-Bellingshausen Seas in surface/subsurface layers are effectively advected to lower latitudes with the ACC. Although a large portion of the basal meltwaters is present in surface and subsurface layers, a part of the basal meltwaters penetrates into the bottom layer through active dense <span class="hlt">water</span> formation along the <span class="hlt">Antarctic</span> coastal margins. The signals at the seafloor extend along the topography, showing a horizontal distribution similar to the observed spreading of <span class="hlt">Antarctic</span> Bottom <span class="hlt">Water</span>. Meltwaters originating from ice shelves in the Weddell and Ross Seas and in the Indian sector significantly contribute to the bottom signals. A series of numerical experiments in which thermodynamic interaction between the ice shelf and ocean is neglected regionally demonstrates that the basal meltwater of each ice shelf impacts sea ice and/or ocean thermohaline circulation in the Southern Ocean. This article was corrected on 10 OCT 2014. See the end of the full text for details.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004ESRv...66..143B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004ESRv...66..143B"><span>Origin, signature and palaeoclimatic influence of the <span class="hlt">Antarctic</span> Circumpolar Current</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Barker, P. F.; Thomas, E.</p> <p>2004-06-01</p> <p>The <span class="hlt">Antarctic</span> Circumpolar Current (ACC) is today the strongest current in the world's ocean, with a significant influence on global climate. Its assumed history and influence on palaeoclimate, while almost certainly equally profound, are here called into question. In this paper, we review 30 years of accumulated data, interpretation and speculation about the ACC, deriving mainly from DSDP and ODP drilling in the Southern Ocean. For most of this time, a conventional view of ACC development, signature and influence has held sway among palaeoceanographers and marine geologists. In this view, the ACC began at about 34 Ma, close to the Eocene-Oligocene boundary, the time of onset of significant <span class="hlt">Antarctic</span> glaciation and the time of creation of a deep-<span class="hlt">water</span> gap (Tasmanian Seaway) between Australia and Antarctica as the South Tasman Rise separated from North Victoria Land. This is the "smoking gun" of synchroneity. The Southern Ocean sediment record shows a latest Eocene development and subsequent geographic expansion of a siliceous biofacies, its northern limit taken to indicate the palaeo-position of the ACC axis. In addition, the ACC was considered to have caused <span class="hlt">Antarctic</span> glaciation by isolating the continent within a cold-<span class="hlt">water</span> annulus, reducing north-south heat transport. A different (and later) date for <span class="hlt">Antarctic</span>-South American opening ("Drake Passage") was proposed, but the timing of ACC onset there was disputed, and the simple story survived. Recent developments, however, call it into question. Modern physical oceanography shows that all or most of present-day ACC transport is confined to narrow jets within deep-reaching circumpolar fronts, and numerical modelling has suggested that a steady reduction in greenhouse gas concentration through the Cenozoic could cause <span class="hlt">Antarctic</span> glaciation, with or without a contribution from ocean circulation change. The rapidity of <span class="hlt">Antarctic</span> glacial onset at the Eocene-Oligocene boundary and coeval creation of a deep-<span class="hlt">water</span> gap south</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li class="active"><span>8</span></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_8 --> <div id="page_9" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li class="active"><span>9</span></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="161"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..14.1904O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..14.1904O"><span>On the <span class="hlt">Antarctic</span> Slope Front and Current crossing of the South Scotia Ridge</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Orsi, A. H.; Palmer, M.; Gomis, D.; Flexas, M. M.; Kim, Y.-S.; Jordà, G.; Wiederwohl, C.; Álvarez, M.</p> <p>2012-04-01</p> <p>To unveil the contorted path followed by the <span class="hlt">Antarctic</span> Slope Current connecting the Weddell and Scotia Seas, hydrographic stations with unprecedented spatial resolution were occupied on a series of sections across the slope and multiple channels in the double-pronged western portion of the South Scotia Ridge. Fieldwork consisted of two cruises from the ESASSI (January 2008) and ACROSS (February 2009) programs, the Spanish and USA/Argentina components of the International Polar Year core project SASSI (Synoptic <span class="hlt">Antarctic</span> Shelf-Slope Interaction study). In this region the <span class="hlt">Antarctic</span> Slope Current can be located by the pronounced in-shore deepening of isopycnals over the continental slope, rendering the strong subsurface temperature and salinity gradients characteristic of the <span class="hlt">Antarctic</span> Slope Front. Before reaching the gaps in the southern Ridge near 51°W and 50°W, the ASC carries about 3 Sv of upper layer <span class="hlt">waters</span>, but it splits into shallow and deep branches upon turning north through these two gaps. The shallower branch enters the Hesperides Trough at 51°W, then shows a tight cyclonic loop back to that longitude roughly following the slope's 700-m isobath, and turns again westward through a similar gap in the northern Ridge. In the Scotia Sea the westward-flowing <span class="hlt">Antarctic</span> Slope Current is found as far west as the Elephant Island along slightly deeper levels of slope (1100 m) before it is blocked by the <span class="hlt">Antarctic</span> Circumpolar Current south of the Shackleton Fracture Zone (56°W). The deeper branch of the ASC in the Powell Basin crosses the southern Ridge near 50°W and roughly follows the 1600-m isobath before entering the Scotia Sea through the Hesperides Gap farther to the east (49°W). Thereafter the deeper <span class="hlt">waters</span> carried westward by this branch become undistinguishable from those circulating farther offshore. Repeat cross-slope sections at both southern and northern flanks of the South Scotia Ridge showed significant temporal variability in the characteristics</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA183893','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA183893"><span>Leadership at <span class="hlt">Antarctic</span> Stations.</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1987-03-01</p> <p>expeditioners, and amongst OICs themselves. Leadership in Antarctica stirs images associated with names such as Scott, Shackleton and Mawson , of men...operates three <span class="hlt">Antarctic</span> stations - Casey, Davis, and Mawson , and one sub-<span class="hlt">Antarctic</span> station - Macquarie Island. Station populations vary, but are</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012APS..MARW41012M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012APS..MARW41012M"><span>Spectroscopic Characterization of the <span class="hlt">Water</span> Oxidation <span class="hlt">Intermediates</span> in the Blue Dimer Ru-Based Catalyst for Artificial Photosynthesis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moonshiram, Dooshaye; Pushkar, Yulia; Jurss, Jonah; Concepcion, Javier; Meyer, Thomas; Zakharova, Taisiya; Alperovich, Igor</p> <p>2012-02-01</p> <p>Utilization of sunlight requires solar capture, light-to-energy conversion and storage. One effective way to store energy is to convert it into chemical energy by fuel-forming reactions, such as <span class="hlt">water</span> splitting into hydrogen and oxygen. Ruthenium complexes are among few molecular-defined catalysts capable of <span class="hlt">water</span> splitting. Mechanistic insights about such catalysts can be acquired by spectroscopic analysis of short-lived <span class="hlt">intermediates</span> of catalytic <span class="hlt">water</span> oxidation. Use of techniques such as EPR and X-ray absorption spectroscopy (XAS) are used to determine electronic requirements of catalytic <span class="hlt">water</span> oxidation. About 30 years ago Meyer and coworkers reported first ruthenium-based catalyst for <span class="hlt">water</span> oxidation, the ``blue dimer''. We performed EPR studies and characterized structures and electronic configurations of <span class="hlt">intermediates</span> of <span class="hlt">water</span> oxidation by the ``blue dimer''. <span class="hlt">Intermediates</span> were prepared chemically by oxidation of Ru-complexes with defined number of Ce (IV) equivalents and freeze-quenched at controlled times. Changes in oxidation state of Ru atom were detected by XANES at Ru K-edges. K-edges are sensitive to changes in Ru oxidation state for Blue Dimer [3,3]^4+, [3,4]^4+, [3,4]'^4+ and [4,5]^3+ allowing a clear assignment of Ru oxidation state in <span class="hlt">intermediates</span>. EXAFS demonstrated structural changes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24395505','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24395505"><span>Fungal oxygen exchange between denitrification <span class="hlt">intermediates</span> and <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>Rohe, Lena; Anderson, Traute-Heidi; Braker, Gesche; Flessa, Heinz; Giesemann, Anette; Wrage-Mönnig, Nicole; Well, Reinhard</p> <p>2014-02-28</p> <p>Fungi can contribute greatly to N2O production from denitrification. Therefore, it is important to quantify the isotopic signature of fungal N2O. The isotopic composition of N2O can be used to identify and analyze the processes of N2O production and N2O reduction. In contrast to bacteria, information about the oxygen exchange between denitrification <span class="hlt">intermediates</span> and <span class="hlt">water</span> during fungal denitrification is lacking, impeding the explanatory power of stable isotope methods. Six fungal species were anaerobically incubated with the electron acceptors nitrate or nitrite and (18)O-labeled <span class="hlt">water</span> to determine the oxygen exchange between denitrification <span class="hlt">intermediates</span> and <span class="hlt">water</span>. After seven days of incubation, gas samples were analyzed for N2O isotopologues by isotope ratio mass spectrometry. All the fungal species produced N2O. N2O production was greater when nitrite was the sole electron acceptor (129 to 6558 nmol N2O g dw(-1)  h(-1)) than when nitrate was the electron acceptor (6 to 47 nmol N2O g dw(-1)  h(-1)). Oxygen exchange was complete with nitrate as electron acceptor in one of five fungi and with nitrite in two of six fungi. Oxygen exchange of the other fungi varied (41 to 89% with nitrite and 11 to 61% with nitrate). This is the first report on oxygen exchange with <span class="hlt">water</span> during fungal denitrification. The exchange appears to be within the range previously reported for bacterial denitrification. This adds to the difficulty of differentiating N2O producing processes based on the origin of N2O-O. However, the large oxygen exchange repeatedly observed for bacteria and now also fungi could lead to less variability in the δ(18)O values of N2O from soils, which could facilitate the assessment of the extent of N2O reduction. Copyright © 2013 John Wiley & Sons, Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010ffcd.confE.150L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010ffcd.confE.150L"><span>Diagnosing <span class="hlt">Antarctic</span> Fog</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lazzara, M. A.</p> <p>2010-07-01</p> <p>Fog affects aviation and other logistical operations in the <span class="hlt">Antarctic</span>; nevertheless limited studies have been conducted to understand fog behavior in this part of the world. A study has been conducted in the Ross Island region of Antarctica, the location of McMurdo Station and Scott Base - the main stations of the United States and New Zealand <span class="hlt">Antarctic</span> programs, respectively. Using tools such as multi-channel satellites observations and supported by in situ radiosonde and ground-based automatic weather station observations, combined with back trajectory and mesoscale numerical models, discover that austral summer fog events are "advective" in temperament. The diagnosis finds a primary source region from the southeast over the Ross Ice Shelf (over 72% of the cases studied) while a minority of cases point toward a secondary fog source region to the north along the Scott Coast of the Ross Sea with influences from the East <span class="hlt">Antarctic</span> Plateau. Part of this examination confirms existing anecdotes from forecasters and weather observers, while refuting others about fog and its behavior in this environment. This effort marks the beginning of our understanding of <span class="hlt">Antarctic</span> fog behavior.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010TellB..62..621J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010TellB..62..621J"><span>Rapid changes in surface <span class="hlt">water</span> carbonate chemistry during <span class="hlt">Antarctic</span> sea ice melt</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jones, Elizabeth M.; Bakker, Dorothee C. E.; Venables, Hugh J.; Whitehouse, Michael J.; Korb, Rebecca E.; Watson, Andrew J.</p> <p>2010-11-01</p> <p>ABSTRACT The effect of sea ice melt on the carbonate chemistry of surface <span class="hlt">waters</span> in the Weddell-Scotia Confluence, Southern Ocean, was investigated during January 2008. Contrasting concentrations of dissolved inorganic carbon (DIC), total alkalinity (TA) and the fugacity of carbon dioxide (fCO2) were observed in and around the receding sea ice edge. The precipitation of carbonate minerals such as ikaite (CaCO3.6H2O) in sea ice brine has the net effect of decreasing DIC and TA and increasing the fCO2 in the brine. Deficits in DIC up to 12 +/- 3 μmol kg-1 in the marginal ice zone (MIZ) were consistent with the release of DIC-poor brines to surface <span class="hlt">waters</span> during sea ice melt. Biological utilization of carbon was the dominant processes and accounted for 41 +/- 1 μmol kg-1 of the summer DIC deficit. The data suggest that the combined effects of biological carbon uptake and the precipitation of carbonates created substantial undersaturation in fCO2 of 95 μatm in the MIZ during summer sea ice melt. Further work is required to improve the understanding of ikaite chemistry in <span class="hlt">Antarctic</span> sea ice and its importance for the sea ice carbon pump.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..12..932M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..12..932M"><span><span class="hlt">Water</span> stable isotope measurements of <span class="hlt">Antarctic</span> samples by means of IRMS and WS-CRDS techniques</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Michelini, Marzia; Bonazza, Mattia; Braida, Martina; Flora, Onelio; Dreossi, Giuliano; Stenni, Barbara</p> <p>2010-05-01</p> <p>In the last years in the scientific community there has been an increasing interest for the application of stable isotope techniques to several environmental problems such as drinking <span class="hlt">water</span> safeguarding, groundwater management, climate change, soils and paleoclimate studies etc. For example, the <span class="hlt">water</span> stable isotopes, being natural tracers of the hydrological cycle, have been extensively used as tools to characterize regional aquifers and to reconstruct past temperature changes from polar ice cores. Here the need for improvements in analytical techniques: the high request for information calls for technologies that can offer a great quantity of analyses in short times and with low costs. Furthermore, sometimes it is difficult to obtain big amount of samples (as is the case for <span class="hlt">Antarctic</span> ice cores or interstitial <span class="hlt">water</span>) preventing the possibility to replicate the analyses. Here, we present oxygen and hydrogen measurements performed on <span class="hlt">water</span> samples covering a big range of isotopic values (from very negative <span class="hlt">antarctic</span> precipitation to mid-latitude precipitation values) carried out with both the conventional Isotope Ratio Mass Spectrometry (IRMS) technique and with a new method based on laser absorption techniques, the Wavelenght Scanned Cavity Ringdown Spectroscopy (WS-CRDS). This study is focusing on improving the precision of the measurements carried out with WS-CRDS in order to extensively apply this method to <span class="hlt">Antarctic</span> ice core paleoclimate studies. The WS-CRDS is a variation of the CRDS developed in 1988 by O'Keef and Deacon. In CRDS a pulse of light goes through a box with high reflective inner surfaces; when there is no sample in the box the light beam doesn't find any obstacle in its path, but the reflectivity of the walls is not perfect so eventually there will be an absorption of the light beam; when the sample is injected in the box there is absorption and the difference between the time of absorption without and with sample is proportional to the quantity</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.7360M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.7360M"><span>Monitoring of <span class="hlt">Antarctic</span> moss ecosystems using a high spatial resolution imaging spectroscopy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Malenovsky, Zbynek; Lucieer, Arko; Robinson, Sharon; Harwin, Stephen; Turner, Darren; Veness, Tony</p> <p>2013-04-01</p> <p>The most abundant photosynthetically active plants growing along the rocky <span class="hlt">Antarctic</span> shore are mosses of three species: Schistidium antarctici, Ceratodon purpureus, and Bryum pseudotriquetrum. Even though mosses are well adapted to the extreme climate conditions, their existence in Antarctica depends strongly on availability of liquid <span class="hlt">water</span> from snowmelt during the short summer season. Recent changes in temperature, wind speed and stratospheric ozone are stimulating faster evaporation, which in turn influences moss growing rate, health state and abundance. This makes them an ideal bio-indicator of the <span class="hlt">Antarctic</span> climate change. Very short growing season, lasting only about three months, requires a time efficient, easily deployable and spatially resolved method for monitoring the <span class="hlt">Antarctic</span> moss beds. Ground and/or low-altitude airborne imaging spectroscopy (called also hyperspectral remote sensing) offers a fast and spatially explicit approach to investigate an actual spatial extent and physiological state of moss turfs. A dataset of ground-based spectral images was acquired with a mini-Hyperspec imaging spectrometer (Headwall Inc., the USA) during the <span class="hlt">Antarctic</span> summer 2012 in the surroundings of the Australian <span class="hlt">Antarctic</span> station Casey (Windmill Islands). The collection of high spatial resolution spectral images, with pixels about 2 cm in size containing from 162 up to 324 narrow spectral bands of wavelengths between 399 and 998 nm, was accompanied with point moss reflectance measurements recorded with the ASD HandHeld-2 spectroradiometer (Analytical Spectral Devices Inc., the USA). The first spectral analysis indicates significant differences in red-edge and near-infrared reflectance of differently <span class="hlt">watered</span> moss patches. Contrary to high plants, where the Normalized Difference Vegetation Index (NDVI) represents an estimate of green biomass, NDVI of mosses indicates mainly the actual <span class="hlt">water</span> content. Similarly to high plants, reflectance of visible wavelengths is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1995JGR...100.3335W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1995JGR...100.3335W"><span>Chemical studies of H chondrites. 6: <span class="hlt">Antarctic/non-Antarctic</span> compositional differences revisited</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wolf, Stephen F.; Lipschutz, Michael E.</p> <p>1995-02-01</p> <p>We report data for the trace elements Au, Co, Sb, Ga, Rb, Ag, Se, Cs, Te, Zn, Cd, Bi, T1, and In (ordered by putative volatility during nebular condensation and accretion) determined by radiochemical neutron activation analysis of 14 additional H5 and H6 chondrite falls. Data for the 10 most volatile elements (Rb to In) treated by the multivariate techniques of linear discriminant analysis and logistic regression in these and 44 other falls are compared with those of 59 H4-6 chondrites from Antarctica. Various populations are tested by the multivariate techniques, using the previously developed method of randomization-simulation to assess significance levels. An earlier conclusion, based on fewer examples, that H4-6 chondrite falls are compositionally distinguishable from the <span class="hlt">Antarctic</span> suite is verified by the additional data. This distinctiveness is highly significant because of the presence of samples from Victoria Land in the <span class="hlt">Antarctic</span> population, which differ compositionally from falls beyond any reasonable doubt. However, it cannot be proven unequivocally that falls and <span class="hlt">Antarctic</span> samples from Queen Maud Land are compositionally distinguishable. Trivial causes (e.g., analyst bias, weathering) cannot explain the Victoria Land (<span class="hlt">Antarctic)/non-Antarctic</span> compositional difference for paradigmatic H4-6 chondrites. This seems to reflect a time-dependent variation of near-Earth meteoroid source regions differing in average thermal history.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19950052480&hterms=queen+victoria&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dqueen%2Bvictoria','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19950052480&hterms=queen+victoria&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dqueen%2Bvictoria"><span>Chemical studies of H chondrites. 6: <span class="hlt">Antarctic/non-Antarctic</span> compositional differences revisited</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wolf, Stephen F.; Lipschutz, Michael E.</p> <p>1995-01-01</p> <p>We report data for the trace elements Au, Co, Sb, Ga, Rb, Ag, Se, Cs, Te, Zn, Cd, Bi, T1, and In (ordered by putative volatility during nebular condensation and accretion) determined by radiochemical neutron activation analysis of 14 additional H5 and H6 chondrite falls. Data for the 10 most volatile elements (Rb to In) treated by the multivariate techniques of linear discriminant analysis and logistic regression in these and 44 other falls are compared with those of 59 H4-6 chondrites from Antarctica. Various populations are tested by the multivariate techniques, using the previously developed method of randomization-simulation to assess significance levels. An earlier conclusion, based on fewer examples, that H4-6 chondrite falls are compositionally distinguishable from the <span class="hlt">Antarctic</span> suite is verified by the additional data. This distinctiveness is highly significant because of the presence of samples from Victoria Land in the <span class="hlt">Antarctic</span> population, which differ compositionally from falls beyond any reasonable doubt. However, it cannot be proven unequivocally that falls and <span class="hlt">Antarctic</span> samples from Queen Maud Land are compositionally distinguishable. Trivial causes (e.g., analyst bias, weathering) cannot explain the Victoria Land (<span class="hlt">Antarctic)/non-Antarctic</span> compositional difference for paradigmatic H4-6 chondrites. This seems to reflect a time-dependent variation of near-Earth meteoroid source regions differing in average thermal history.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A11L..08S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A11L..08S"><span>CCN and IN concentration measurements during the <span class="hlt">Antarctic</span> Circumnavigation Expedition</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stratmann, F.; Henning, S.; Löffler, M.; Welti, A.; Hartmann, M.; Wernli, H.; Baccarini, A.; Schmale, J.</p> <p>2017-12-01</p> <p>Cloud condensation nuclei (CCN) and ice nuclei (IN) concentrations measured during the <span class="hlt">Antarctic</span> Circumnavigation Expedition (ACE) within the Study of Preindustrial-like Aerosol-Climate Effects (SPACE) are presented. The measurements give a circumpolar transect through the Sub <span class="hlt">Antarctic</span> Ocean, where existing measurements are scarce. ACE took place during the austral summer 2016/17 and included exploration of different environments from pristine open Ocean to <span class="hlt">Antarctic</span> islands and the southernmost ports of the 3 surrounding continents. CCN concentrations are measured over the entire range of expected in-cloud supersaturations from 0.1 to 1% using a CCNc instrument from DMT. IN concentrations are determined from filter samples at <span class="hlt">water</span> saturated conditions from -5°C to -25°C, covering common temperatures of mixed-phase cloud glaciation. The sensitivity of measured IN and CCN concentrations to meteorological parameters, activity of marine biology and location is assessed to gain insight into potential sources of CCN and IN. Back trajectory modelling is used to allocate regional variations to aerosol sources originating in the marine boundary layer or long-range transport. The gained datasets constrain CCN and IN concentrations in the marine boundary layer along the cruise track. The comprehensive set of parallel measured parameters during ACE allow to evaluate contributions of local ocean-surface sources versus long-range transport to Sub-<span class="hlt">Antarctic</span> CCN and IN. The measurements can be used as input to climate models, e.g. pristine Sub <span class="hlt">Antarctic</span> conditions can provide an approximation for a pre-industrial environment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014SolED...6..869A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014SolED...6..869A"><span>Microbial biomass and basal respiration in Sub-<span class="hlt">Antarctic</span> and <span class="hlt">Antarctic</span> soils in the areas of some Russian polar stations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Abakumov, E.; Mukhametova, N.</p> <p>2014-03-01</p> <p>Antarctica is the unique place for pedological investigations. Soils of Antarctica have been studied intensively during the last century. <span class="hlt">Antarctic</span> logistic provides the possibility to scientists access the terrestrial landscapes mainly in the places of polar stations. That is why the main and most detailed pedological investigations were conducted in Mc Murdo Valleys, Transantarctic Mountains, South Shetland Islands, Larsemann hills and Schirmacher Oasis. Investigations were conducted during the 53rd and 55th Russian <span class="hlt">Antarctic</span> expeditions on the base of soil pits and samples collected in Sub-<span class="hlt">Antarctic</span> and <span class="hlt">Antarctic</span> regions. Soils of diverse <span class="hlt">Antarctic</span> landscapes were studied with aim to assess the microbial biomass level, basal respiration rates and metabolic activity of microbial communities. The investigation conducted shows that soils of <span class="hlt">Antarctic</span> are quite different in profile organization and carbon content. In general, Sub-<span class="hlt">Antarctic</span> soils are characterized by more developed humus (sod) organo-mineral horizons as well as the upper organic layer. The most developed organic layers were revealed in peat soils of King-George Island, where its thickness reach even 80 cm. These soils as well as soils under guano are characterized by the highest amount of total organic carbon (TOC) 7.22-33.70%. Coastal and continental soils of <span class="hlt">Antarctic</span> are presented by less developed Leptosols, Gleysols, Regolith and rare Ornhitosol with TOC levels about 0.37-4.67%. The metabolic ratios and basal respiration were higher in Sub-<span class="hlt">Antarctic</span> soils than in <span class="hlt">Antarctic</span> ones which can be interpreted as result of higher amounts of fresh organic remnants in organic and organo-mineral horizons. Also the soils of King-George island have higher portion of microbial biomass (max 1.54 mg g-1) than coastal (max 0.26 mg g-1) and continental (max 0.22 mg g-1) <span class="hlt">Antarctic</span> soils. Sub-<span class="hlt">Antarctic</span> soils mainly differ from <span class="hlt">Antarctic</span> ones in increased organic layers thickness and total organic carbon content</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19278447','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19278447"><span>Bacteria beneath the West <span class="hlt">Antarctic</span> ice sheet.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lanoil, Brian; Skidmore, Mark; Priscu, John C; Han, Sukkyun; Foo, Wilson; Vogel, Stefan W; Tulaczyk, Slawek; Engelhardt, Hermann</p> <p>2009-03-01</p> <p>Subglacial environments, particularly those that lie beneath polar ice sheets, are beginning to be recognized as an important part of Earth's biosphere. However, except for indirect indications of microbial assemblages in subglacial Lake Vostok, Antarctica, no sub-ice sheet environments have been shown to support microbial ecosystems. Here we report 16S rRNA gene and isolate diversity in sediments collected from beneath the Kamb Ice Stream, West <span class="hlt">Antarctic</span> Ice Sheet and stored for 15 months at 4 degrees C. This is the first report of microbes in samples from the sediment environment beneath the <span class="hlt">Antarctic</span> Ice Sheet. The cells were abundant ( approximately 10(7) cells g(-1)) but displayed low diversity (only five phylotypes), likely as a result of enrichment during storage. Isolates were cold tolerant and the 16S rRNA gene diversity was a simplified version of that found in subglacial alpine and Arctic sediments and <span class="hlt">water</span>. Although in situ cell abundance and the extent of wet sediments beneath the <span class="hlt">Antarctic</span> ice sheet can only be roughly extrapolated on the basis of this sample, it is clear that the subglacial ecosystem contains a significant and previously unrecognized pool of microbial cells and associated organic carbon that could potentially have significant implications for global geochemical processes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.5306C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.5306C"><span>Distribution of Upper Circumpolar Deep <span class="hlt">Water</span> on the warming continental shelf of the West <span class="hlt">Antarctic</span> Peninsula</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Couto, Nicole; Martinson, Douglas G.; Kohut, Josh; Schofield, Oscar</p> <p>2017-07-01</p> <p>We use autonomous underwater vehicles to characterize the spatial distribution of Upper Circumpolar Deep <span class="hlt">Water</span> (UCDW) on the continental shelf of the West <span class="hlt">Antarctic</span> Peninsula (WAP) and present the first near-synoptic measurements of mesoscale features (eddies) containing UCDW on the WAP. Thirty-three subsurface eddies with widths on the order of 10 km were detected during four glider deployments. Each eddy contributed an average of 5.8 × 1016 J to the subpycnocline <span class="hlt">waters</span>, where a cross-shelf heat flux of 1.37 × 1019 J yr-1 is required to balance the diffusive loss of heat to overlying winter <span class="hlt">water</span> and to the near-coastal <span class="hlt">waters</span>. Approximately two-thirds of the heat coming onto the shelf diffuses across the pycnocline and one-third diffuses to the coastal <span class="hlt">waters</span>; long-term warming of the subpycnocline <span class="hlt">waters</span> is a small residual of this balance. Sixty percent of the profiles that contained UCDW were part of a coherent eddy. Between 20% and 53% of the lateral onshore heat flux to the WAP can be attributed to eddies entering Marguerite Trough, a feature in the southern part of the shelf which is known to be an important conduit for UCDW. A northern trough is identified as additional important location for eddy intrusion.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007QSRv...26.2113B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007QSRv...26.2113B"><span>Modelling <span class="hlt">Antarctic</span> sea-level data to explore the possibility of a dominant <span class="hlt">Antarctic</span> contribution to meltwater pulse IA</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bassett, S. E.; Milne, G. A.; Bentley, M. J.; Huybrechts, P.</p> <p>2007-09-01</p> <p>We compare numerical predictions of glaciation-induced sea-level change to data from 8 locations around the <span class="hlt">Antarctic</span> coast in order to test if the available data preclude the possibility of a dominant <span class="hlt">Antarctic</span> contribution to meltwater pulse IA (mwp-IA). Results based on a subset of 7 spherically symmetric earth viscosity models and 6 different <span class="hlt">Antarctic</span> deglaciation histories indicate that the sea-level data do not rule out a large <span class="hlt">Antarctic</span> source for this event. Our preliminary analysis indicates that the Weddell Sea is the most likely source region for a large (˜9 m) <span class="hlt">Antarctic</span> contribution to mwp-IA. The Ross Sea is also plausible as a significant contributor (˜5 m) from a sea-level perspective, but glacio-geological field observations are not compatible with such a large and rapid melt from this region. Our results suggest that the Lambert Glacier component of the East <span class="hlt">Antarctic</span> ice sheet experienced significant retreat at the time of mwp-IA, but only contributed ˜0.15 m (eustatic sea-level change). All of the ice models considered under-predicted the isostatic component of the sea-level response in the <span class="hlt">Antarctic</span> Peninsula and the Sôya Coast region of the East <span class="hlt">Antarctic</span> ice sheet, indicating that the maximum ice thickness in these regions is underestimated. It is therefore plausible that ice melt from these areas, the <span class="hlt">Antarctic</span> Peninsula in particular, could have made a significant contribution to mwp-IA.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20010049374','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20010049374"><span>Radarsat <span class="hlt">Antarctic</span> Mapping Project: <span class="hlt">Antarctic</span> Imaging Campaign 2</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>2001-01-01</p> <p>The Radarsat <span class="hlt">Antarctic</span> Mapping Project is a collaboration between NASA and the Canadian Space Agency to map Antarctica using synthetic aperture radar (SAR). The first <span class="hlt">Antarctic</span> Mapping Mission (AMM-1) was successfully completed in October 1997. Data from the acquisition phase of the 1997 campaign have been used to achieve the primary goal of producing the first, high-resolution SAR image map of Antarctica. The limited amount of data suitable for interferometric analysis have also been used to produce remarkably detailed maps of surface velocity for a few selected regions. Most importantly, the results from AMM-1 are now available to the general science community in the form of various resolution, radiometrically calibrated and geometrically accurate image mosaics. The second <span class="hlt">Antarctic</span> imaging campaign occurred during the fall of 2000. Modified from AMM-1, the satellite remained in north looking mode during AMM-2 restricting coverage to regions north of about -80 degrees latitude. But AMM-2 utilized for the first time RADARSAT-1 fine beams providing an unprecedented opportunity to image many of Antarctica's fast glaciers whose extent was revealed through AMM-1 data. AMM-2 also captured extensive data suitable for interferometric analysis of the surface velocity field. This report summarizes the science goals, mission objectives, and project status through the acquisition phase and the start of the processing phase. The reports describes the efforts of team members including Alaska SAR Facility, Jet Propulsion Laboratory, Vexcel Corporation, Goddard Space Flight Center, Wallops Flight Facility, Ohio State University, Environmental Research Institute of Michigan, White Sands Facility, Canadian Space Agency Mission Planning and Operations Groups, and the <span class="hlt">Antarctic</span> Mapping Planning Group.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=airborne&pg=4&id=EJ364056','ERIC'); return false;" href="https://eric.ed.gov/?q=airborne&pg=4&id=EJ364056"><span>The <span class="hlt">Antarctic</span> Ozone Hole.</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>Stolarski, Richard S.</p> <p>1988-01-01</p> <p>Discusses the Airborne <span class="hlt">Antarctic</span> Ozone Experiment (1987) and the findings of the British <span class="hlt">Antarctic</span> Survey (1985). Proposes two theories for the appearance of the hole in the ozone layer over Antarctica which appears each spring; air pollution and natural atmospheric shifts. Illustrates the mechanics of both. Supports worldwide chlorofluorocarbon…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70034736','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70034736"><span>Obliquity-paced Pliocene West <span class="hlt">Antarctic</span> ice sheet oscillations</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Naish, T.; Powell, R.; Levy, R.; Wilson, G.; Scherer, R.; Talarico, F.; Krissek, L.; Niessen, F.; Pompilio, M.; Wilson, T.; Carter, L.; DeConto, R.; Huybers, P.; McKay, R.; Pollard, D.; Ross, J.; Winter, D.; Barrett, P.; Browne, G.; Cody, R.; Cowan, E.; Crampton, J.; Dunbar, G.; Dunbar, N.; Florindo, F.; Gebhardt, C.; Graham, I.; Hannah, M.; Hansaraj, D.; Harwood, D.; Helling, D.; Henrys, S.; Hinnov, L.; Kuhn, G.; Kyle, P.; Laufer, A.; Maffioli, P.; Magens, D.; Mandernack, K.; McIntosh, W.; Millan, C.; Morin, R.; Ohneiser, C.; Paulsen, T.; Persico, D.; Raine, I.; Reed, J.; Riesselman, C.; Sagnotti, L.; Schmitt, D.; Sjunneskog, C.; Strong, P.; Taviani, M.; Vogel, S.; Wilch, T.; Williams, T.</p> <p>2009-01-01</p> <p>Thirty years after oxygen isotope records from microfossils deposited in ocean sediments confirmed the hypothesis that variations in the Earth's orbital geometry control the ice ages1, fundamental questions remain over the response of the <span class="hlt">Antarctic</span> ice sheets to orbital cycles2. Furthermore, an understanding of the behaviour of the marine-based West <span class="hlt">Antarctic</span> ice sheet (WAIS) during the 'warmer-than-present' early-Pliocene epoch (5–3 Myr ago) is needed to better constrain the possible range of ice-sheet behaviour in the context of future global warming3. Here we present a marine glacial record from the upper 600 m of the AND-1B sediment core recovered from beneath the northwest part of the Ross ice shelf by the ANDRILL programme and demonstrate well-dated, 40-kyr cyclic variations in ice-sheet extent linked to cycles in insolation influenced by changes in the Earth's axial tilt (obliquity) during the Pliocene. Our data provide direct evidence for orbitally induced oscillations in the WAIS, which periodically collapsed, resulting in a switch from grounded ice, or ice shelves, to open <span class="hlt">waters</span> in the Ross embayment when planetary temperatures were up to 3 °C warmer than today4 and atmospheric CO2 concentration was as high as 400 p.p.m.v. (refs 5, 6). The evidence is consistent with a new ice-sheet/ice-shelf model7 that simulates fluctuations in <span class="hlt">Antarctic</span> ice volume of up to +7 m in equivalent sea level associated with the loss of the WAIS and up to +3 m in equivalent sea level from the East <span class="hlt">Antarctic</span> ice sheet, in response to ocean-induced melting paced by obliquity. During interglacial times, diatomaceous sediments indicate high surface-<span class="hlt">water</span> productivity, minimal summer sea ice and air temperatures above freezing, suggesting an additional influence of surface melt8 under conditions of elevated CO2.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=landscape&id=EJ1131439','ERIC'); return false;" href="https://eric.ed.gov/?q=landscape&id=EJ1131439"><span>Unstable Space: Mapping the <span class="hlt">Antarctic</span> for Children in "Heroic Era" <span class="hlt">Antarctic</span> Literature</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>Moriarty, Sinead</p> <p>2017-01-01</p> <p>This article examines the <span class="hlt">Antarctic</span> landscape as one of the last places in the world to be explored and mapped, and as one of the most changeable landscapes in the world. The mapping exercises involved in the early, heroic-era <span class="hlt">Antarctic</span> expeditions, helped to reduce a once mysterious and unknown landscape into a known entity, something that could…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26465038','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26465038"><span>Designing an effective mark-recapture study of <span class="hlt">Antarctic</span> blue whales.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Peel, David; Bravington, Mark; Kelly, Natalie; Double, Michael C</p> <p>2015-06-01</p> <p>To properly conserve and manage wild populations, it is important to have information on abundance and population dynamics. In the case of rare and cryptic species, especially in remote locations, surveys can be difficult and expensive, and run the risk of not producing sample sizes large enough to produce precise estimates. Therefore, it is crucial to conduct preliminary analysis to determine if the study will produce useable estimates. The focus of this paper is a proposed mark-recapture study of <span class="hlt">Antarctic</span> blue whales (Balaenoptera musculus intermedia). <span class="hlt">Antarctic</span> blue whales were hunted to near extinction up until the mid- 1960s, when commercial exploitation of this species ended. Current abundance estimates are a decade old. Furthermore, at present, there are no formal circumpolar-level cetacean surveys operating in <span class="hlt">Antarctic</span> <span class="hlt">waters</span> and, specifically, there is no strategy to monitor the potential recovery of <span class="hlt">Antarctic</span> blue whales. Hence the work in this paper was motivated by the need to inform decisions on strategies for future monitoring of <span class="hlt">Antarctic</span> blue whale population. The paper describes a model to predict the precision and bias of estimates from a proposed survey program. The analysis showed that mark-recapture is indeed a suitable method to provide a circumpolar abundance estimate of <span class="hlt">Antarctic</span> blue whales, with precision of the abundance, at the midpoint of the program, predicted to be between 0.2 and 0.3. However, this was only if passive acoustic tracking was utilized to increase the encounter rate. The analysis also provided guidance on general design for an <span class="hlt">Antarctic</span> blue whale program, showing that it requires a 12-year duration; although surveys do not necessarily need to be run every year if multiple vessels are available to clump effort. Mark-recapture is based on a number of assumptions; it was evident from the analysis that ongoing analysis and monitoring of the data would be required to check such assumptions hold (e.g., test for</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/2015Ocgy...55..796M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015Ocgy...55..796M"><span>Flows of <span class="hlt">Antarctic</span> bottom <span class="hlt">water</span> through fractures in the southern part of the North Mid-Atlantic Ridge</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Morozov, E. G.; Tarakanov, R. Yu.; Makarenko, N. I.</p> <p>2015-11-01</p> <p>We study the flows of bottom <span class="hlt">waters</span> of the <span class="hlt">Antarctic</span> origin in deep fracture zones of the southern part of the North Mid-Atlantic Ridge. In the autumn of 2014, an expedition onboard the RV Akademik Sergey Vavilov carried out measurements of current velocities and thermohaline properties of bottom <span class="hlt">water</span> in several quasi-zonal fractures in the southern part of the Northern Mid-Atlantic Ridge, which connect the deep basins of the West and East Atlantic, the Vema Fracture Zone (FZ) (10°50' N) and a group of sub-equatorial fractures: Doldrums (8°15' N), Vernadsky (7°40' N), and a nameless fracture at 7°30' N. The estimates of bottom <span class="hlt">water</span> (θ < 2.0°C) transport through this group based on measurements from 2014 are approximately 0.28 Sv (1 Sv = 106 m3/s), which is close to 25% of the transport estimate through the Vema FZ (1.20 Sv) obtained in the same expedition. The coldest bottom <span class="hlt">water</span> temperatures among the investigated fractures were recorded in the Vema FZ.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1982AmSci..70..156C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1982AmSci..70..156C"><span><span class="hlt">Antarctic</span> meteorites</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cassidy, W. A.; Rancitelli, L. A.</p> <p>1982-04-01</p> <p>An abundance of meteorites has been discovered on two sites in the <span class="hlt">Antarctic</span> which may assist in the study of the origins of meteorites and the history of the solar system. Characteristics particular to those meteorites discovered in this region are explained. These specimens, being well preserved due to the climate, have implications in the study of the cosmic ray flux through time, the meteoroid complex in space, and cosmic ray exposure ages. Implications for the study of the <span class="hlt">Antarctic</span>, particularly the ice flow, are also discussed. Further discoveries of meteorites in this region are anticipated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AtmEn.118..135B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AtmEn.118..135B"><span>Sugars in <span class="hlt">Antarctic</span> aerosol</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Barbaro, Elena; Kirchgeorg, Torben; Zangrando, Roberta; Vecchiato, Marco; Piazza, Rossano; Barbante, Carlo; Gambaro, Andrea</p> <p>2015-10-01</p> <p>The processes and transformations occurring in the <span class="hlt">Antarctic</span> aerosol during atmospheric transport were described using selected sugars as source tracers. Monosaccharides (arabinose, fructose, galactose, glucose, mannose, ribose, xylose), disaccharides (sucrose, lactose, maltose, lactulose), alcohol-sugars (erythritol, mannitol, ribitol, sorbitol, xylitol, maltitol, galactitol) and anhydrosugars (levoglucosan, mannosan and galactosan) were measured in the <span class="hlt">Antarctic</span> aerosol collected during four different sampling campaigns. For quantification, a sensitive high-pressure anion exchange chromatography was coupled with a single quadrupole mass spectrometer. The method was validated, showing good accuracy and low method quantification limits. This study describes the first determination of sugars in the <span class="hlt">Antarctic</span> aerosol. The total mean concentration of sugars in the aerosol collected at the ;Mario Zucchelli; coastal station was 140 pg m-3; as for the aerosol collected over the <span class="hlt">Antarctic</span> plateau during two consecutive sampling campaigns, the concentration amounted to 440 and 438 pg m-3. The study of particle-size distribution allowed us to identify the natural emission from spores or from sea-spray as the main sources of sugars in the coastal area. The enrichment of sugars in the fine fraction of the aerosol collected on the <span class="hlt">Antarctic</span> plateau is due to the degradation of particles during long-range atmospheric transport. The composition of sugars in the coarse fraction was also investigated in the aerosol collected during the oceanographic cruise.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16905428','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16905428"><span>Crustacea in Arctic and <span class="hlt">Antarctic</span> sea ice: distribution, diet and life history strategies.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Arndt, Carolin E; Swadling, Kerrie M</p> <p>2006-01-01</p> <p>This review concerns crustaceans that associate with sea ice. Particular emphasis is placed on comparing and contrasting the Arctic and <span class="hlt">Antarctic</span> sea ice habitats, and the subsequent influence of these environments on the life history strategies of the crustacean fauna. Sea ice is the dominant feature of both polar marine ecosystems, playing a central role in physical processes and providing an essential habitat for organisms ranging in size from viruses to whales. Similarities between the Arctic and <span class="hlt">Antarctic</span> marine ecosystems include variable cover of sea ice over an annual cycle, a light regimen that can extend from months of total darkness to months of continuous light and a pronounced seasonality in primary production. Although there are many similarities, there are also major differences between the two regions: The <span class="hlt">Antarctic</span> experiences greater seasonal change in its sea ice extent, much of the ice is over very deep <span class="hlt">water</span> and more than 80% breaks out each year. In contrast, Arctic sea ice often covers comparatively shallow <span class="hlt">water</span>, doubles in its extent on an annual cycle and the ice may persist for several decades. Crustaceans, particularly copepods and amphipods, are abundant in the sea ice zone at both poles, either living within the brine channel system of the ice-crystal matrix or inhabiting the ice-<span class="hlt">water</span> interface. Many species associate with ice for only a part of their life cycle, while others appear entirely dependent upon it for reproduction and development. Although similarities exist between the two faunas, many differences are emerging. Most notable are the much higher abundance and biomass of <span class="hlt">Antarctic</span> copepods, the dominance of the <span class="hlt">Antarctic</span> sea ice copepod fauna by calanoids, the high euphausiid biomass in Southern Ocean <span class="hlt">waters</span> and the lack of any species that appear fully dependent on the ice. In the Arctic, the ice-associated fauna is dominated by amphipods. Calanoid copepods are not tightly associated with the ice, while harpacticoids and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28784139','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28784139"><span>Structure and application of antifreeze proteins from <span class="hlt">Antarctic</span> bacteria.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Muñoz, Patricio A; Márquez, Sebastián L; González-Nilo, Fernando D; Márquez-Miranda, Valeria; Blamey, Jenny M</p> <p>2017-08-07</p> <p>Antifreeze proteins (AFPs) production is a survival strategy of psychrophiles in ice. These proteins have potential in frozen food industry avoiding the damage in the structure of animal or vegetal foods. Moreover, there is not much information regarding the interaction of <span class="hlt">Antarctic</span> bacterial AFPs with ice, and new determinations are needed to understand the behaviour of these proteins at the <span class="hlt">water</span>/ice interface. Different <span class="hlt">Antarctic</span> places were screened for antifreeze activity and microorganisms were selected for the presence of thermal hysteresis in their crude extracts. Isolates GU1.7.1, GU3.1.1, and AFP5.1 showed higher thermal hysteresis and were characterized using a polyphasic approach. Studies using cucumber and zucchini samples showed cellular protection when samples were treated with partially purified AFPs or a commercial AFP as was determined using toluidine blue O and neutral red staining. Additionally, genome analysis of these isolates revealed the presence of genes that encode for putative AFPs. Deduced amino acids sequences from GU3.1.1 (gu3A and gu3B) and AFP5.1 (afp5A) showed high similarity to reported AFPs which crystal structures are solved, allowing then generating homology models. Modelled proteins showed a triangular prism form similar to β-helix AFPs with a linear distribution of threonine residues at one side of the prism that could correspond to the putative ice binding side. The statistically best models were used to build a protein-<span class="hlt">water</span> system. Molecular dynamics simulations were then performed to compare the antifreezing behaviour of these AFPs at the ice/<span class="hlt">water</span> interface. Docking and molecular dynamics simulations revealed that gu3B could have the most efficient antifreezing behavior, but gu3A could have a higher affinity for ice. AFPs from <span class="hlt">Antarctic</span> microorganisms GU1.7.1, GU3.1.1 and AFP5.1 protect cellular structures of frozen food showing a potential for frozen food industry. Modeled proteins possess a β-helix structure, and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19890017427','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19890017427"><span><span class="hlt">Antarctic</span> Meteorite Location Map Series</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Schutt, John (Editor); Fessler, Brian (Editor); Cassidy, William (Editor)</p> <p>1989-01-01</p> <p>Antarctica has been a prolific source of meteorites since meteorite concentrations were discovered in 1969. The <span class="hlt">Antarctic</span> Search For Meteorites (ANSMET) project has been active over much of the Trans-<span class="hlt">Antarctic</span> Mountain Range. The first ANSMET expedition (a joint U.S.-Japanese effort) discovered what turned out to be a significant concentration of meteorites at the Allan Hills in Victoria Land. Later reconnaissance in this region resulted in the discovery of meteorite concentrations on icefields to the west of the Allan Hills, at Reckling Moraine, and Elephant Moraine. <span class="hlt">Antarctic</span> meteorite location maps (reduced versions) of the Allan Hills main, near western, middle western, and far western icefields and the Elephant Moraine icefield are presented. Other <span class="hlt">Antarctic</span> meteorite location maps for the specimens found by the ANSMET project are being prepared.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3814847','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3814847"><span>Levoglucosan indicates high levels of biomass burning aerosols over oceans from the Arctic to <span class="hlt">Antarctic</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>Hu, Qi-Hou; Xie, Zhou-Qing; Wang, Xin-Ming; Kang, Hui; Zhang, Pengfei</p> <p>2013-01-01</p> <p>Biomass burning is known to affect air quality, global carbon cycle, and climate. However, the extent to which biomass burning gases/aerosols are present on a global scale, especially in the marine atmosphere, is poorly understood. Here we report the molecular tracer levoglucosan concentrations in marine air from the Arctic Ocean through the North and South Pacific Ocean to Antarctica during burning season. Levoglucosan was found to be present in all regions at ng/m3 levels with the highest atmospheric loadings present in the mid-latitudes (30°–60° N and S), <span class="hlt">intermediate</span> loadings in the Arctic, and lowest loadings in the <span class="hlt">Antarctic</span> and equatorial latitudes. As a whole, levoglucosan concentrations in the Southern Hemisphere were comparable to those in the Northern Hemisphere. Biomass burning has a significant impact on atmospheric Hg and <span class="hlt">water</span>-soluble organic carbon (WSOC) from pole-to-pole, with more contribution to WSOC in the Northern Hemisphere than in the Southern Hemisphere. PMID:24176935</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24176935','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24176935"><span>Levoglucosan indicates high levels of biomass burning aerosols over oceans from the Arctic to <span class="hlt">Antarctic</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hu, Qi-Hou; Xie, Zhou-Qing; Wang, Xin-Ming; Kang, Hui; Zhang, Pengfei</p> <p>2013-11-01</p> <p>Biomass burning is known to affect air quality, global carbon cycle, and climate. However, the extent to which biomass burning gases/aerosols are present on a global scale, especially in the marine atmosphere, is poorly understood. Here we report the molecular tracer levoglucosan concentrations in marine air from the Arctic Ocean through the North and South Pacific Ocean to Antarctica during burning season. Levoglucosan was found to be present in all regions at ng/m(3) levels with the highest atmospheric loadings present in the mid-latitudes (30°-60° N and S), <span class="hlt">intermediate</span> loadings in the Arctic, and lowest loadings in the <span class="hlt">Antarctic</span> and equatorial latitudes. As a whole, levoglucosan concentrations in the Southern Hemisphere were comparable to those in the Northern Hemisphere. Biomass burning has a significant impact on atmospheric Hg and <span class="hlt">water</span>-soluble organic carbon (WSOC) from pole-to-pole, with more contribution to WSOC in the Northern Hemisphere than in the Southern Hemisphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.9939V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.9939V"><span>Paleoceanography/climate and taphonomy at <span class="hlt">intermediate</span> <span class="hlt">water</span> depth in the Subtropical Western North Pacific Ocean over the last 1 Ma from IODP Exp 350 Sites U1436C and U1437B, Izu arc area.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vautravers, Maryline</p> <p>2015-04-01</p> <p>IODP Expedition 350 Site U1436C lies in the western part of the Izu fore arc basin, ~60 km east of the arc front volcano Aogashima, at 1776 m <span class="hlt">water</span> depth. This site is a technical hole (only a 150 m long record) for a potential future deep drilling by Chikyu. Site U1437 is located in the Izu rear arc, ~90 km west of the arc front volcanoes Myojinsho and Myojin Knoll, at 2117 m <span class="hlt">water</span> depth. At this site in order to study the evolution of the IZU rear arc crust we recovered a 1800 meter long sequence of mud and volcaniclastic sediments. These sites provide a rich and well-preserved record of volcanic eruptions within the area of the Izu Bonin-Arc. However, the material recovered, mostly mud with ash containing generally abundant planktonic foraminifera, can support additional paleoceanographic goals in an area affected by the Kuroshio Current. Also, the hydrographic divide created by the Izu rise provides a rare opportunity to gain some insight into the operation of the global <span class="hlt">intermediate</span> circulation. The <span class="hlt">Antarctic</span> <span class="hlt">Intermediate</span> <span class="hlt">Water</span> Mass is more influential at the depth of U1437B in the West and the North Pacific <span class="hlt">Intermediate</span> <span class="hlt">Water</span> at Site U1436C to the East. We analyzed 460 samples recovered at Sites U1436C and U1437B for a quantitative planktonic foraminifer study, and also for carbonate preservation indices, including: shell weight, percent planktonic foraminifera fragments planktonic foraminifer concentrations, various faunal proxies, and benthic/planktonic ratio. We measured the stable isotopes for a similar number of samples using the thermocline dwelling Neogloboquadrina dutertrei. The dataset presented here covers the last 1 Ma at Site U1437B and 0.9 Ma at Site U1436C. The age models for the two sites are largely established through stable isotope stratigraphy (this study). On their respective age models we evidence based on polar/subpolar versus subtropical faunal assemblages changes qualitative surface <span class="hlt">water</span> temperature variations recording the changing</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5954465','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5954465"><span>Shelf–ocean exchange and hydrography west of the <span class="hlt">Antarctic</span> Peninsula: a review</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>2018-01-01</p> <p>The West <span class="hlt">Antarctic</span> Peninsula (WAP) is a highly productive marine ecosystem where extended periods of change have been observed in the form of glacier retreat, reduction of sea-ice cover and shifts in marine populations, among others. The physical environment on the shelf is known to be strongly influenced by the <span class="hlt">Antarctic</span> Circumpolar Current flowing along the shelf slope and carrying warm, nutrient-rich <span class="hlt">water</span>, by cold <span class="hlt">waters</span> flooding into the northern Bransfield Strait from the Weddell Sea, by an extensive network of glaciers and ice shelves, and by strong seasonal to inter-annual variability in sea-ice formation and air–sea interactions, with significant modulation by climate modes like El Niño–Southern Oscillation and the Southern Annular Mode. However, significant gaps have remained in understanding the exchange processes between the open ocean and the shelf, the pathways and fate of oceanic <span class="hlt">water</span> intrusions, the shelf heat and salt budgets, and the long-term evolution of the shelf properties and circulation. Here, we review how recent advances in long-term monitoring programmes, process studies and newly developed numerical models have helped bridge these gaps and set future research challenges for the WAP system. This article is part of the theme issue ‘The marine system of the West <span class="hlt">Antarctic</span> Peninsula: status and strategy for progress in a region of rapid change’. PMID:29760109</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014SolE....5..705A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014SolE....5..705A"><span>Microbial biomass and basal respiration of selected Sub-<span class="hlt">Antarctic</span> and <span class="hlt">Antarctic</span> soils in the areas of some Russian polar stations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Abakumov, E.; Mukhametova, N.</p> <p>2014-07-01</p> <p>Antarctica is a unique place for soil, biological, and ecological investigations. Soils of Antarctica have been studied intensively during the last century, when different national <span class="hlt">Antarctic</span> expeditions visited the sixth continent with the aim of investigating nature and the environment. <span class="hlt">Antarctic</span> investigations are comprised of field surveys mainly in the terrestrial landscapes, where the polar stations of different countries are situated. That is why the main and most detailed soil surveys were conducted in the McMurdo Valleys, Transantarctic Mountains, South Shetland Islands, Larsemann Hills and the Schirmacher Oasis. Our investigations were conducted during the 53rd and 55th Russian <span class="hlt">Antarctic</span> expeditions in the base of soil pits, and samples were collected in Sub-<span class="hlt">Antarctic</span> and <span class="hlt">Antarctic</span> regions. Sub-<span class="hlt">Antarctic</span> or maritime landscapes are considered to be very different from <span class="hlt">Antarctic</span> landscapes due to differing climatic and geogenic conditions. Soils of diverse zonal landscapes were studied with the aim of assessing the microbial biomass level, basal respiration rates and metabolic activity of microbial communities. This investigation shows that <span class="hlt">Antarctic</span> soils are quite diverse in profile organization and carbon content. In general, Sub-<span class="hlt">Antarctic</span> soils are characterized by more developed humus (sod) organo-mineral horizons as well as by an upper organic layer. The most developed organic layers were revealed in peat soils of King George Island, where its thickness reach, in some cases, was 80 cm. These soils as well as soils formed under guano are characterized by the highest amount of total organic carbon (TOC), between 7.22 and 33.70%. Coastal and continental <span class="hlt">Antarctic</span> soils exhibit less developed Leptosols, Gleysols, Regolith and rare Ornhitosol, with TOC levels between 0.37 and 4.67%. The metabolic ratios and basal respiration were higher in Sub-<span class="hlt">Antarctic</span> soils than in <span class="hlt">Antarctic</span> ones, which can be interpreted as a result of higher amounts of fresh organic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27157132','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27157132"><span>A transcriptome resource for the <span class="hlt">Antarctic</span> pteropod Limacina helicina antarctica.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Johnson, Kevin M; Hofmann, Gretchen E</p> <p>2016-08-01</p> <p>The pteropod Limacina helicina antarctica is a dominant member of the zooplankton assemblage in the <span class="hlt">Antarctic</span> marine ecosystem, and is part of a relatively simple food web in nearshore marine <span class="hlt">Antarctic</span> <span class="hlt">waters</span>. As a shelled pteropod, Limacina has been suggested as a candidate sentinel organism for the impacts of ocean acidification, due to the potential for shell dissolution in undersaturated <span class="hlt">waters</span>. In this study, our goal was to develop a transcriptomic resource for Limacina that would support mechanistic studies to explore the physiological response of Limacina to abiotic stressors such as ocean acidification and ocean warming. To this end, RNA sequencing libraries were prepared from Limacina that had been exposed to a range of pH levels and an elevated temperature to maximize the diversity of expressed genes. RNA sequencing (RNA-seq) was conducted on an Illumina NextSeq500 which produced 339,000,000 150bp paired-end reads. The de novo transcriptome was produced using Trinity and annotation of the assembled transcriptome resulted in the identification of 81,229 transcripts in 137 KEGG pathways. This RNA-seq effort resulted in a transcriptome for the <span class="hlt">Antarctic</span> pteropod, Limacina helicina antarctica, that is a major resource for an international marine science research community studying these pelagic molluscs in a global change context. Copyright © 2016 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRC..123.1533B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRC..123.1533B"><span>Three-Dimensional Ageostrophic Motion and <span class="hlt">Water</span> Mass Subduction in the Southern Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Buongiorno Nardelli, B.; Mulet, S.; Iudicone, D.</p> <p>2018-02-01</p> <p>Vertical velocities at the ocean mesoscale are several orders of magnitude smaller than corresponding horizontal flows, making their direct monitoring a still unsolved challenge. Vertical motion is generally retrieved indirectly by applying diagnostic equations to observation-based fields. The most common approach relies on the solution of an adiabatic version of the Omega equation, neglecting the ageostrophic secondary circulation driven by frictional effects and turbulent mixing in the boundary layers. Here we apply a diabatic semigeostrophic diagnostic model to two different 3-D reconstructions covering the Southern Ocean during the period 2010-2012. We incorporate the effect of vertical mixing through a modified K-profile parameterization and using ERA-interim data, and perform an indirect validation of the ageostrophic circulation with independent drifter observations. Even if horizontal gradients and associated vertical flow are likely underestimated at 1/4° × 1/4° resolution, the exercise provides an unprecedented relative quantification of the contribution of vertical mixing and adiabatic internal dynamics on the vertical exchanges along the <span class="hlt">Antarctic</span> Circumpolar Current. Kinematic estimates of subduction rates show the destruction of poleward flowing <span class="hlt">waters</span> lighter than 26.6 kg/m3 (14 ÷ 15 Sv) and two main positive bands associated with the <span class="hlt">Antarctic</span> <span class="hlt">Intermediate</span> <span class="hlt">Water</span> (7 ÷ 11 Sv) and Sub-<span class="hlt">Antarctic</span> Mode <span class="hlt">Waters</span> (4 ÷ 7 Sv) formation, while Circumpolar Deep <span class="hlt">Water</span> upwelling attains around 3 ÷ 6 Sv. Diabatic and adiabatic terms force distinct spatial responses and vertical velocity magnitudes along the <span class="hlt">water</span> column and the restratifying effect of adiabatic internal dynamics due to mesoscale eddies is shown to at least partly compensate the contribution of wind-driven vertical exchanges to net subduction.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C13G..02S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C13G..02S"><span><span class="hlt">Antarctic</span> grounding-line migration</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Slater, T.; Konrad, H.; Shepherd, A.; Gilbert, L.; Hogg, A.; McMillan, M.; Muir, A. S.</p> <p>2017-12-01</p> <p>Knowledge of grounding-line position is critical for quantifying ice discharge into the ocean, as a boundary condition for numerical models of ice flow, and as an indicator of ice sheet stability. Although geological investigations have documented extensive grounding-line retreat since the period of the Last Glacial Maximum, observations of grounding line migration during the satellite era are restricted to a handful of locations. We combine satellite altimeter observations of ice-elevation change and airborne measurements of ice geometry to track movement of the <span class="hlt">Antarctic</span> Ice Sheet grounding line. Based on these data, we estimate that 22%, 3%, and 10% of the West <span class="hlt">Antarctic</span>, East <span class="hlt">Antarctic</span>, and <span class="hlt">Antarctic</span> Peninsula ice sheet grounding lines are retreating at rates faster than the typical pace since the Last Glacial Maximum, and that the continent loses over 200 km2 of grounded-ice area per year. Although by far the fastest rates of retreat occurred in the Amundsen Sea Sector, the Pine Island Glacier grounding line has stabilized - likely as a consequence of abated ocean forcing during the survey period.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20000070367&hterms=temperature+variability&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dtemperature%2Bvariability','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20000070367&hterms=temperature+variability&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dtemperature%2Bvariability"><span>Seasonal-to-Interannual Variability in <span class="hlt">Antarctic</span> Sea-Ice Dynamics, and Its Impact on Surface Fluxes and <span class="hlt">Water</span> Mass Production</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Drinkwater, Mark R.</p> <p>1999-01-01</p> <p>Strong seasonal and interannual signals in <span class="hlt">Antarctic</span> bottom-<span class="hlt">water</span> outflow remain unexplained yet are highly correlated with anomalies in net sea-ice growth in coastal polynyas. The mechanisms responsible for driving salination and replenishment and rejuvenation of the dense shelf "source" <span class="hlt">waters</span> likely also generate pulses of bottom <span class="hlt">water</span> outflow. The objective of this research is to investigate time-scales of variability in the dynamics of sea-ice in the Southern Ocean in order to determine the primary sites for production of dense shelf <span class="hlt">waters</span>. We are using a merged satellite/buoy sea-ice motion data set for the period 1978-present day to compute the dynamics of opening and closing of coastal polynyas over the continental shelf. The Ocean Circulation and Climate Advanced Model (OCCAM) ocean general circulation model with coupled sea-ice dynamics is presently forced using National Center for Environmental Prediction (NCEP) data to simulate fluxes and the salination impact of the ocean shelf regions. This work is relevant in the context of measuring the influence of polar sea-ice dynamics upon polar ocean characteristics, and thereby upon global thermohaline ocean circulation. Interannual variability in simulated net freezing rate in the Southern Weddell Sea is shown for the period 1986-1993. There is a pronounced maximum of ice production in 1988 and minimum in 1991 in response to anomalies in equatorward meridional wind velocity. This follows a similar approximate 8-year interannual cycle in Sea Surface Temperature (SST) and satellite-derived ice-edge anomalies reported elsewhere as the "<span class="hlt">Antarctic</span> Circumpolar Wave." The amplitude of interannual fluctuations in annual net ice production are about 40% of the mean value, implying significant interannual variance in brine rejection and upper ocean heat loss. Southward anomalies in wind stress induce negative anomalies in open <span class="hlt">water</span> production, which are observed in passive microwave satellite images. Thus, cycles of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSHE44B1515S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSHE44B1515S"><span>Spatial and temporal variation of Shelf <span class="hlt">Water</span> and its connection with <span class="hlt">Antarctic</span> Bottom <span class="hlt">Water</span> in Prydz Bay, East Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sun, Y.; Shi, J.; Yuan, X.</p> <p>2016-02-01</p> <p>Hydrographic surveys from 1981 to 2015, instrumented seal data from 2004 to 2014, and mooring data were used to reveal spatial and temporal variation of Shelf <span class="hlt">Water</span> (SW) and the connection between SW and <span class="hlt">Antarctic</span> Bottom <span class="hlt">Water</span> (AABW) in Prydz Bay. The basic spatial pattern of the SW properties was presented and 5 subregions were distinguished based on the pattern and the topography. The change of <span class="hlt">water</span> masses and the processes on the shelf are investigated in these subregions. A high salinity SW(S>34.6) is observed in the central and northern part of the Amery Basin in summer, which is like to be caused by the Circumpolar Deep <span class="hlt">Water</span> (CDW) intrusion, and the eddy activities could be the primary impact to the CDW intrusion. There could be less CDW intrusion in winter because of the ice cover in this subregion, which is supported by the mooring in Prydz Bay Channel. A high salinity SW is observed near the Mackenzie polynya in winter, which is caused by brine rejection in ice production process. But the high salinity SW seems unlikely to form the overflow denser SW and locally form AABW. A dense <span class="hlt">water</span> mass with low salinity, low temperature and high oxygen was observed on the shelf break in the 70.5°E section, which could be caused by the Ice Shelf <span class="hlt">Water</span> (ISW) export from Amery Shelf. According to the hydrographic data, the dense <span class="hlt">water</span> can form overflow DSW and flow downslope to west, which can be observed in the bottom of slope near 1500m in the 70°E section. The <span class="hlt">water</span> will form AABW if it can flow downslope to the deep basin and keep mixing with CDW, suggesting a new type of DSW overflow in Prydz Bay.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/12902283','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/12902283"><span>Influence of seasonal environmental variables on the distribution of presumptive fecal Coliforms around an <span class="hlt">Antarctic</span> research station.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hughes, Kevin A</p> <p>2003-08-01</p> <p>Factors affecting fecal microorganism survival and distribution in the <span class="hlt">Antarctic</span> marine environment include solar radiation, <span class="hlt">water</span> salinity, temperature, sea ice conditions, and fecal input by humans and local wildlife populations. This study assessed the influence of these factors on the distribution of presumptive fecal coliforms around Rothera Point, Adelaide Island, <span class="hlt">Antarctic</span> Peninsula during the austral summer and winter of February 1999 to September 1999. Each factor had a different degree of influence depending on the time of year. In summer (February), although the station population was high, presumptive fecal coliform concentrations were low, probably due to the biologically damaging effects of solar radiation. However, summer algal blooms reduced penetration of solar radiation into the <span class="hlt">water</span> column. By early winter (April), fecal coliform concentrations were high, due to increased fecal input by migrant wildlife, while solar radiation doses were low. By late winter (September), fecal coliform concentrations were high near the station sewage outfall, as sea ice formation limited solar radiation penetration into the sea and prevented wind-driven <span class="hlt">water</span> circulation near the outfall. During this study, environmental factors masked the effect of station population numbers on sewage plume size. If sewage production increases throughout the <span class="hlt">Antarctic</span>, environmental factors may become less significant and effective sewage waste management will become increasingly important. These findings highlight the need for year-round monitoring of fecal coliform distribution in <span class="hlt">Antarctic</span> <span class="hlt">waters</span> near research stations to produce realistic evaluations of sewage pollution persistence and dispersal.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMPP34B..04H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMPP34B..04H"><span>Evolution of surface and deep <span class="hlt">water</span> conditions in the <span class="hlt">Antarctic</span> Southern Ocean across the MPT</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hasenfratz, A. P.; Jaccard, S.; Martinez-Garcia, A.; Hodell, D. A.; Vance, D.; Bernasconi, S. M.; Kleiven, H. F.; Haug, G. H.</p> <p>2016-12-01</p> <p>The mid-Pleistocene transition (MPT; 1.25-0.7 Myr) marked a fundamental change in the periodicity of the climate cycles, shifting from a 41-kyr to a high-amplitude, asymmetric 100-kyr cycle without any noticeable change in orbital forcing. Hypotheses to explain the MPT involve non-linear responses to orbital forcing, changes in glacial dynamics and internal changes in the carbon cycle. Specifically, a decrease in pCO2 during peak ice age conditions and the associated global cooling has been proposed as one of the possible triggers for the MPT. Previous results have indicated that the Southern Ocean provides a coherent two-part mechanism for the timing and amplitude of the glacial/interglacial pCO2 variations. However, there is still much uncertainty and debate regarding the response of the <span class="hlt">Antarctic</span> Southern Ocean biogeochemistry to changes invoked for the MPT, and its contribution to the proposed pCO2 variations. Here, we show 1.5 Myr-long records of export production, and planktonic (Neogloboquadrina pachyderma) and benthic (Melonis pompilioides) foraminiferal stable isotopes and trace metals from ODP Site 1094 retrieved from the Atlantic sector of the <span class="hlt">Antarctic</span> Southern Ocean (53.2°S, 5.1°E, 2807m). While glacial planktonic δ18O increases across the MPT, glacial Mg/Ca-derived SST decrease later, around 700 ka, when glacial atmospheric pCO2 has already dropped. As glacial export production that is crucially related to micronutrients upwelled from the subsurface ocean remains unchanged across the past 1.5 Myr, it seems that cooling of the glacial surface ocean did not significantly alter the stability of the <span class="hlt">water</span> column. Furthermore, paired measurements of benthic δ18O and Mg/Ca enables the determination of seawater δ18O of the deep ocean, which allows us to estimate changes in the density gradient and the salinity of the deep <span class="hlt">water</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011DSRII..58...91K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011DSRII..58...91K"><span>Is there a distinct continental slope fauna in the <span class="hlt">Antarctic</span>?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kaiser, Stefanie; Griffiths, Huw J.; Barnes, David K. A.; Brandão, Simone N.; Brandt, Angelika; O'Brien, Philip E.</p> <p>2011-02-01</p> <p>The <span class="hlt">Antarctic</span> continental slope spans the depths from the shelf break (usually between 500 and 1000 m) to ˜3000 m, is very steep, overlain by 'warm' (2-2.5 °C) Circumpolar Deep <span class="hlt">Water</span> (CDW), and life there is poorly studied. This study investigates whether life on Antarctica's continental slope is essentially an extension of the shelf or the abyssal fauna, a transition zone between these or clearly distinct in its own right. Using data from several cruises to the Weddell Sea and Scotia Sea, including the ANDEEP (<span class="hlt">ANtarctic</span> benthic DEEP-sea biodiversity, colonisation history and recent community patterns) I-III, BIOPEARL (BIOdiversity, Phylogeny, Evolution and Adaptive Radiation of Life in Antarctica) 1 and EASIZ (Ecology of the <span class="hlt">Antarctic</span> Sea Ice Zone) II cruises as well as current databases (SOMBASE, SCAR-MarBIN), four different taxa were selected (i.e. cheilostome bryozoans, isopod and ostracod crustaceans and echinoid echinoderms) and two areas, the Weddell Sea and the Scotia Sea, to examine faunal composition, richness and affinities. The answer has important ramifications to the link between physical oceanography and ecology, and the potential of the slope to act as a refuge and resupply zone to the shelf during glaciations. Benthic samples were collected using Agassiz trawl, epibenthic sledge and Rauschert sled. By bathymetric definition, these data suggest that despite eurybathy in some of the groups examined and apparent similarity of physical conditions in the <span class="hlt">Antarctic</span>, the shelf, slope and abyssal faunas were clearly separated in the Weddell Sea. However, no such separation of faunas was apparent in the Scotia Sea (except in echinoids). Using a geomorphological definition of the slope, shelf-slope-abyss similarity only changed significantly in the bryozoans. Our results did not support the presence of a homogenous and unique <span class="hlt">Antarctic</span> slope fauna despite a high number of species being restricted to the slope. However, it remains the case that there may be</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C23A1212A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C23A1212A"><span>Responses of Basal Melting of <span class="hlt">Antarctic</span> Ice Shelves to the Climatic Forcing of the Last Glacial Maximum and CO2 Doubling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Abe-Ouchi, A.; Obase, T.</p> <p>2017-12-01</p> <p>Basal melting of the <span class="hlt">Antarctic</span> ice shelves is an important factor in determining the stability of the <span class="hlt">Antarctic</span> ice sheet. This study used the climatic outputs of an atmosphere?ocean general circulation model to force a circumpolar ocean model that resolves ice shelf cavity circulation to investigate the response of <span class="hlt">Antarctic</span> ice shelf melting to different climatic conditions, i.e., to an increase (doubling) of CO2 and the Last Glacial Maximum conditions. We also conducted sensitivity experiments to investigate the role of surface atmospheric change, which strongly affects sea ice production, and the change of oceanic lateral boundary conditions. We found that the rate of change of basal melt due to climate warming is much greater (by an order of magnitude) than due to cooling. This is mainly because the intrusion of warm <span class="hlt">water</span> onto the continental shelves, linked to sea ice production and climate change, is crucial in determining the basal melt rate of many ice shelves. Sensitivity experiments showed that changes of atmospheric heat flux and ocean temperature are both important for warm and cold climates. The offshore wind change together with atmospheric heat flux change strongly affected the production of sea ice and high-density <span class="hlt">water</span>, preventing warmer <span class="hlt">water</span> approaching the ice shelves under a colder climate. These results reflect the importance of both <span class="hlt">water</span> mass formation in the <span class="hlt">Antarctic</span> shelf seas and subsurface ocean temperature in understanding the long-term response to climate change of the melting of <span class="hlt">Antarctic</span> ice shelves.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li class="active"><span>10</span></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_10 --> <div id="page_11" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="201"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1991anc..book......','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1991anc..book......"><span><span class="hlt">Antarctic</span> news clips, 1991</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p></p> <p>1991-08-01</p> <p>Published stories are presented that sample a year's news coverage of Antarctica. The intent is to provide the U.S. <span class="hlt">Antarctic</span> Program participants with a digest of current issues as presented by a variety of writers and popular publications. The subject areas covered include the following: earth science; ice studies; stratospheric ozone; astrophysics; life science; operations; education; <span class="hlt">antarctic</span> treaty issues; and tourism</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007PalOc..22.3213S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007PalOc..22.3213S"><span>Late Quaternary changes in <span class="hlt">intermediate</span> <span class="hlt">water</span> oxygenation and oxygen minimum zone, northern Japan: A benthic foraminiferal perspective</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shibahara, Akihiko; Ohkushi, Ken'ichi; Kennett, James P.; Ikehara, Ken</p> <p>2007-09-01</p> <p>A strong oxygen minimum zone (OMZ) currently exists at upper <span class="hlt">intermediate</span> <span class="hlt">water</span> depths on the northern Japanese margin, NW Pacific. The OMZ results largely from a combination of high surface <span class="hlt">water</span> productivity and poor ventilation of upper <span class="hlt">intermediate</span> <span class="hlt">waters</span>. We investigated late Quaternary history (last 34 kyr) of ocean floor oxygenation and the OMZ using quantitative changes in benthic foraminiferal assemblages in three sediment cores taken from the continental slope off Shimokita Peninsula and Tokachi, northern Japan, at <span class="hlt">water</span> depths between 975 and 1363 m. These cores are well located within the present-day OMZ, a region of high surface <span class="hlt">water</span> productivity, and in close proximity to the source region of North Pacific <span class="hlt">Intermediate</span> <span class="hlt">Water</span>. Late Quaternary benthic foraminiferal assemblages experienced major changes in response to changes in dissolved oxygen concentration in ocean floor sediments. Foraminiferal assemblages are interpreted to represent three main groups representing oxic, suboxic, and dysoxic conditions. Assemblage changes in all three cores and hence in bottom <span class="hlt">water</span> oxygenation coincided with late Quaternary climatic episodes, similar to that known for the southern California margin. These episodes, in turn, are correlated with orbital and millennial climate episodes in the Greenland ice core including the last glacial episode, Bølling-Ållerød (B/A), Younger Dryas, Preboreal (earliest Holocene), early Holocene, and late Holocene. The lowest oxygen conditions, marked by dysoxic taxa and laminated sediments in one core, occurred during the B/A and the Preboreal intervals. Suboxic taxa dominated mainly during the last glacial, the Younger Dryas, and most of the Holocene. Dysoxic conditions during the B/A and Preboreal intervals in this region were possibly caused by high surface <span class="hlt">water</span> productivity at times of reduced <span class="hlt">intermediate</span> ventilation in the northwestern Pacific. Remarkable similarities are evident in the late Quaternary sequence of benthic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040031526&hterms=ocean+climate+changes&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Docean%2Bclimate%2Bchanges','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040031526&hterms=ocean+climate+changes&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Docean%2Bclimate%2Bchanges"><span>Using Satellite-derived Ice Concentration to Represent <span class="hlt">Antarctic</span> Coastal Polynyas in Ocean Climate Models</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Stoessel, Achim; Markus, Thorsten</p> <p>2003-01-01</p> <p>The focus of this paper is on the representation of <span class="hlt">Antarctic</span> coastal polynyas in global ice-ocean general circulation models (OGCMs), in particular their local, regional, and high-frequency behavior. This is verified with the aid of daily ice concentration derived from satellite passive microwave data using the NASATeam 2 (NT2) and the bootstrap (BS) algorithms. Large systematic regional and temporal discrepancies arise, some of which are related to the type of convection parameterization used in the model. An attempt is made to improve the fresh-<span class="hlt">water</span> flux associated with melting and freezing in <span class="hlt">Antarctic</span> coastal polynyas by ingesting (assimilating) satellite ice concentration where it comes to determining the thermodynamics of the open-<span class="hlt">water</span> fraction of a model grid cell. Since the NT2 coastal open-<span class="hlt">water</span> fraction (polynyas) tends to be less extensive than the simulated one in the decisive season and region, assimilating NT2 coastal ice concentration yields overall reduced net freezing rates, smaller formation rates of <span class="hlt">Antarctic</span> Bottom <span class="hlt">Water</span>, and a stronger southward flow of North Atlantic Deep <span class="hlt">Water</span> across 30 S. Enhanced net freezing rates occur regionally when NT2 coastal ice concentration is assimilated, concomitant with a more realistic ice thickness distribution and accumulation of High-Salinity Shelf <span class="hlt">Water</span>. Assimilating BS rather than NT2 coastal ice concentration, the differences to the non-assimilated simulation are generally smaller and of opposite sign. This suggests that the model reproduces coastal ice concentration in closer agreement with the BS data than with the NT2 data, while more realistic features emerge when NT2 data are assimilated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFMIN44A..01D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFMIN44A..01D"><span><span class="hlt">Antarctic</span> Data Management as Part of the IPY Legacy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>de Bruin, T.</p> <p>2006-12-01</p> <p>The <span class="hlt">Antarctic</span> Treaty states that "scientific observations and results from Antarctica shall be exchanged and made freely available". Antarctica includes the Southern Ocean. In support of this, National <span class="hlt">Antarctic</span> Data Centres (NADC) are being established to catalogue data sets and to provide information on data sets to scientists and others with interest in <span class="hlt">Antarctic</span> science. The Joint Committee on <span class="hlt">Antarctic</span> Data Management (JCADM) was established by the Scientific Committee on <span class="hlt">Antarctic</span> Research (SCAR) and the Council of Managers of National <span class="hlt">Antarctic</span> Programs (COMNAP). JCADM comprises representatives of the National <span class="hlt">Antarctic</span> Data Centres. Currently 30 nations around the world are represented in JCADM. JCADM is responsible for the <span class="hlt">Antarctic</span> Master Directory (AMD), the internationally accessible, web-based, searchable record of <span class="hlt">Antarctic</span> and Southern Ocean data set descriptions. The AMD is directly integrated into the international Global Change Master Directory (GCMD) to help further merge <span class="hlt">Antarctic</span> science into global science. The AMD is a resource for scientists to advertise the data they have collected and to search for data they may need. JCADM is the <span class="hlt">Antarctic</span> component of the IPY Data Infrastructure, which is presently being developed. This presentation will give an overview of the organization of <span class="hlt">Antarctic</span> and Southern Ocean data management with sections on the organizational structure of JCADM, contents of the <span class="hlt">Antarctic</span> Master Directory, relationships to the SCAR Scientific Research Programmes (SRP) and IPY, international embedding and connections with discipline-based peer organizations like the International Oceanographic Data and Information Exchange Committee (IODE). It will focus primarily on the role that an existing infrastructure as JCADM, may play in the development of the IPY Data Infrastructure and will provide considerations for IPY data management, based on the experiences in <span class="hlt">Antarctic</span> and oceanographic data management.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28226220','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28226220"><span><span class="hlt">Water</span> Oxidation Mechanisms of Metal Oxide Catalysts by Vibrational Spectroscopy of Transient <span class="hlt">Intermediates</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhang, Miao; Frei, Heinz</p> <p>2017-05-05</p> <p><span class="hlt">Water</span> oxidation is an essential reaction of an artificial photosystem for solar fuel generation because it provides electrons needed to reduce carbon dioxide or protons to a fuel. Earth-abundant metal oxides are among the most attractive catalytic materials for this reaction because of their robustness and scalability, but their efficiency poses a challenge. Knowledge of catalytic surface <span class="hlt">intermediates</span> gained by vibrational spectroscopy under reaction conditions plays a key role in uncovering kinetic bottlenecks and provides a basis for catalyst design improvements. Recent dynamic infrared and Raman studies reveal the molecular identity of transient surface <span class="hlt">intermediates</span> of <span class="hlt">water</span> oxidation on metal oxides. Combined with ultrafast infrared observations of how charges are delivered to active sites of the metal oxide catalyst and drive the multielectron reaction, spectroscopic advances are poised to play a key role in accelerating progress toward improved catalysts for artificial photosynthesis.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3593827','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3593827"><span>Experimental demonstration of radicaloid character in a RuV=O <span class="hlt">intermediate</span> in catalytic <span class="hlt">water</span> oxidation</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Moonshiram, Dooshaye; Alperovich, Igor; Concepcion, Javier J.; Meyer, Thomas J.; Pushkar, Yulia</p> <p>2013-01-01</p> <p><span class="hlt">Water</span> oxidation is the key half reaction in artificial photosynthesis. An absence of detailed mechanistic insight impedes design of new catalysts that are more reactive and more robust. A proposed paradigm leading to enhanced reactivity is the existence of oxyl radical <span class="hlt">intermediates</span> capable of rapid <span class="hlt">water</span> activation, but there is a dearth of experimental validation. Here, we show the radicaloid nature of an <span class="hlt">intermediate</span> reactive toward formation of the O-O bond by assessing the spin density on the oxyl group by Electron Paramagnetic Resonance (EPR). In the study, an 17O-labeled form of a highly oxidized, short-lived <span class="hlt">intermediate</span> in the catalytic cycle of the <span class="hlt">water</span> oxidation catalyst cis,cis-[(2,2-bipyridine)2(H2O)RuIIIORuIII(OH2)(bpy)2]4+ was investigated. It contains Ru centers in oxidation states [4,5], has at least one RuV = O unit, and shows |Axx| = 60G 17O hyperfine splittings (hfs) consistent with the high spin density of a radicaloid. Destabilization of π-bonding in the d3 RuV = O fragment is responsible for the high spin density on the oxygen and its high reactivity. PMID:23417296</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28873966','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28873966"><span>Draft genome of the <span class="hlt">Antarctic</span> dragonfish, Parachaenichthys charcoti.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ahn, Do-Hwan; Shin, Seung Chul; Kim, Bo-Mi; Kang, Seunghyun; Kim, Jin-Hyoung; Ahn, Inhye; Park, Joonho; Park, Hyun</p> <p>2017-08-01</p> <p>The <span class="hlt">Antarctic</span> bathydraconid dragonfish, Parachaenichthys charcoti, is an <span class="hlt">Antarctic</span> notothenioid teleost endemic to the Southern Ocean. The Southern Ocean has cooled to -1.8ºC over the past 30 million years, and the seawater had retained this cold temperature and isolated oceanic environment because of the <span class="hlt">Antarctic</span> Circumpolar Current. Notothenioids dominate <span class="hlt">Antarctic</span> fish, making up 90% of the biomass, and all notothenioids have undergone molecular and ecological diversification to survive in this cold environment. Therefore, they are considered an attractive <span class="hlt">Antarctic</span> fish model for evolutionary and ancestral genomic studies. Bathydraconidae is a speciose family of the Notothenioidei, the dominant taxonomic component of <span class="hlt">Antarctic</span> teleosts. To understand the process of evolution of <span class="hlt">Antarctic</span> fish, we select a typical <span class="hlt">Antarctic</span> bathydraconid dragonfish, P. charcoti. Here, we have sequenced, de novo assembled, and annotated a comprehensive genome from P. charcoti. The draft genome of P. charcoti is 709 Mb in size. The N50 contig length is 6145 bp, and its N50 scaffold length 178 362 kb. The genome of P. charcoti is predicted to contain 32 712 genes, 18 455 of which have been assigned preliminary functions. A total of 8951 orthologous groups common to 7 species of fish were identified, while 333 genes were identified in P. charcoti only; 2519 orthologous groups were also identified in both P. charcoti and N. coriiceps, another <span class="hlt">Antarctic</span> fish. Four gene ontology terms were statistically overrepresented among the 333 genes unique to P. charcoti, according to gene ontology enrichment analysis. The draft P. charcoti genome will broaden our understanding of the evolution of <span class="hlt">Antarctic</span> fish in their extreme environment. It will provide a basis for further investigating the unusual characteristics of <span class="hlt">Antarctic</span> fishes. © The Author 2017. Published by Oxford University Press.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.9500M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.9500M"><span>The effects of sub-ice-shelf melting on dense shelf <span class="hlt">water</span> formation and export in idealized simulations of <span class="hlt">Antarctic</span> margins</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; Stern, Alon; Harrison, Matthew; Sergienko, Olga; Hallberg, Robert</p> <p>2017-04-01</p> <p>Dense shelf <span class="hlt">water</span> (DSW) is formed in coastal polynyas around Antarctica as a result of intense cooling and brine rejection. A fraction of this <span class="hlt">water</span> reaches ice shelves cavities and is modified due to interactions with sub-ice-shelf melt <span class="hlt">water</span>. This modified <span class="hlt">water</span> mass contributes to the formation of <span class="hlt">Antarctic</span> Bottom <span class="hlt">Water</span>, and consequently, influences the large-scale ocean circulation. Here, we investigate the role of sub-ice-shelf melting in the formation and export of DSW using idealized simulations with an isopycnal ocean model (MOM6) coupled with a sea ice model (SIS2) and a thermodynamic active ice shelf. A set of experiments is conducted with variable horizontal grid resolutions (0.5, 1.0 and 2.0 km), ice shelf geometries and atmospheric forcing. In all simulations DSW is spontaneously formed in coastal polynyas due to the combined effect of the imposed atmospheric forcing and the ocean state. Our results show that sub-ice-shelf melting can significantly change the rate of dense shelf <span class="hlt">water</span> outflows, highlighting the importance of this process to correctly represent bottom <span class="hlt">water</span> formation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5472753','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5472753"><span>The influence of <span class="hlt">Antarctic</span> subglacial volcanism on the global iron cycle during the Last Glacial Maximum</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Frisia, Silvia; Weyrich, Laura S.; Hellstrom, John; Borsato, Andrea; Golledge, Nicholas R.; Anesio, Alexandre M.; Bajo, Petra; Drysdale, Russell N.; Augustinus, Paul C.; Rivard, Camille; Cooper, Alan</p> <p>2017-01-01</p> <p>Marine sediment records suggest that episodes of major atmospheric CO2 drawdown during the last glacial period were linked to iron (Fe) fertilization of subantarctic surface <span class="hlt">waters</span>. The principal source of this Fe is thought to be dust transported from southern mid-latitude deserts. However, uncertainty exists over contributions to CO2 sequestration from complementary Fe sources, such as the <span class="hlt">Antarctic</span> ice sheet, due to the difficulty of locating and interrogating suitable archives that have the potential to preserve such information. Here we present petrographic, geochemical and microbial DNA evidence preserved in precisely dated subglacial calcites from close to the East <span class="hlt">Antarctic</span> Ice-Sheet margin, which together suggest that volcanically-induced drainage of Fe-rich <span class="hlt">waters</span> during the Last Glacial Maximum could have reached the Southern Ocean. Our results support a significant contribution of <span class="hlt">Antarctic</span> volcanism to subglacial transport and delivery of nutrients with implications on ocean productivity at peak glacial conditions. PMID:28598412</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1996JGR...101.6591W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1996JGR...101.6591W"><span>Modeling the dispersal of Levantine <span class="hlt">Intermediate</span> <span class="hlt">Water</span> and its role in Mediterranean deep <span class="hlt">water</span> formation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wu, Peili; Haines, Keith</p> <p>1996-03-01</p> <p>This paper demonstrates the importance of Levantine <span class="hlt">Intermediate</span> <span class="hlt">Water</span> (LIW) in the deep <span class="hlt">water</span> formation process in the Mediterranean using the modular ocean general circulation model at 0.25° resolution, 19 vertical levels, over the entire Mediterranean with an open Gibraltar strait. LIW formation is strongly prescribed in the Rhodes Gyre region by Haney [1971] relaxation, while in other regions, surface salinity relaxation is much reduced by applying the `mixed' thermohaline surface boundary conditions. Isopycnal diagnostics are used to trace <span class="hlt">water</span> mass movements, and volume fluxes are monitored at straits. Low viscosity and diffusion are used to permit baroclinic eddies to play a role in <span class="hlt">water</span> mass dispersal. The overall <span class="hlt">water</span> budget is measured by an average flux at Gibraltar of 0.8 Sv, of which 0.7 Sv is exchanged with the eastern basin at Sicily. LIW (density around 28.95) spreads rapidly after formation throughout the entire Levantine due to baroclinic eddies. Toward the west, LIW accumulates in the northern and central Ionian, with some entering the Adriatic through Otranto and some mixing southward in eddies and exiting to the western Mediterranean through Sicily. LIW is converted to deep <span class="hlt">water</span> in the south Adriatic at an average rate of 0.4 Sv. <span class="hlt">Water</span> exchange through the Otranto strait appears to be buoyancy driven, with a strong bias to the end of winter (March-April), while at Sicily the exchange has a strong symmetric seasonal cycle, with maximum transport of 1.1 Sv in December indicating the effects of wind driving. LIW pathways in the west are complex and variable. In the Tyrrhenian, <span class="hlt">intermediate</span> <span class="hlt">water</span> becomes uniform on isopycnal surfaces due to eddy stirring. West of Sardinia, two LIW boundary currents are formed in the Balearic basin; one flows northward up the west coast of Sardinia and Corsica, and one westward along the northern African coast. The northward current is consistent with observations, while the westward current is intermittent for</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28970917','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28970917"><span>Criegee <span class="hlt">intermediate</span>-hydrogen sulfide chemistry at the air/<span class="hlt">water</span> interface.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kumar, Manoj; Zhong, Jie; Francisco, Joseph S; Zeng, Xiao C</p> <p>2017-08-01</p> <p>We carry out Born-Oppenheimer molecular dynamic simulations to show that the reaction between the smallest Criegee <span class="hlt">intermediate</span>, CH 2 OO, and hydrogen sulfide (H 2 S) at the air/<span class="hlt">water</span> interface can be observed within few picoseconds. The reaction follows both concerted and stepwise mechanisms with former being the dominant reaction pathway. The concerted reaction proceeds with or without the involvement of one or two nearby <span class="hlt">water</span> molecules. An important implication of the simulation results is that the Criegee-H 2 S reaction can provide a novel non-photochemical pathway for the formation of a C-S linkage in clouds and could be a new oxidation pathway for H 2 S in terrestrial, geothermal and volcanic regions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012PalOc..27.3203R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012PalOc..27.3203R"><span>Abrupt changes of <span class="hlt">intermediate</span> <span class="hlt">water</span> properties on the northeastern slope of the Bering Sea during the last glacial and deglacial period</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rella, Stephan F.; Tada, Ryuji; Nagashima, Kana; Ikehara, Minoru; Itaki, Takuya; Ohkushi, Ken'ichi; Sakamoto, Tatsuhiko; Harada, Naomi; Uchida, Masao</p> <p>2012-09-01</p> <p>Millennial-scale variability in the behavior of North Pacific <span class="hlt">Intermediate</span> <span class="hlt">Water</span> during the last glacial and deglacial period, and its association with Dansgaard-Oeschger (D-O) cycles and Heinrich events, are examined based on benthic foraminiferal oxygen and carbon isotopes (δ18Obf and δ13Cbf) and %CaCO3 using a sediment core recovered from the northeastern slope of the Bering Sea. A suite of positive δ18Obf excursions at <span class="hlt">intermediate</span> depths of the Bering Sea, which seem at least in part associated with increases in the δ18Obf gradients between the Bering and Okhotsk Seas, suggest the Bering Sea as a proximate source of <span class="hlt">intermediate</span> <span class="hlt">water</span> during several severe stadial episodes in the last glacial and deglacial period. Absence of such δ18Obf gradients during periods of high surface productivity in the Bering and Okhotsk Seas, which we correlate to D-O interstadials, suggests a reduction in <span class="hlt">intermediate</span> <span class="hlt">water</span> production in the Bering Sea and subsequent introduction of nutrient-rich deep <span class="hlt">waters</span> from the North Pacific into <span class="hlt">intermediate</span> depths of the Bering Sea. We argue that a reorganization of atmospheric circulation in the high-latitude North Pacific during severe cold episodes in the last glacial and deglacial period created favorable conditions for brine rejection in the northeastern Bering Sea. The resulting salinity increase in the cold surface <span class="hlt">waters</span> could have initiated <span class="hlt">intermediate</span> (and deep) <span class="hlt">water</span> formation that spread out to the North Pacific.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS13A1797G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS13A1797G"><span>Investigating the Sources of Decadal-Scale Property Changes in <span class="hlt">Antarctic</span> Bottom <span class="hlt">Water</span> in the Southeast Indian Ocean (80-90°E)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gottschalk, K.; Macdonald, A. M.</p> <p>2016-12-01</p> <p>A recognizable warming and freshening of <span class="hlt">Antarctic</span> Bottom <span class="hlt">Water</span> (AABW) throughout much of the Southern Ocean is one of the major findings of the international long-line hydrographic programs of 1990's and the 2000's. A recent GO-SHIP repeat of the I08S line in the southeast Indian Ocean in 2016 found continued, but weaker, AABW warming and significantly strong freshening in the <span class="hlt">Antarctic</span>-Australian Basin (A-AB). It has been proposed that the 2010 B9b iceberg calving along the Adélie Land Coast may be linked to the sharp increase in A-AB AABW freshening. The present study seeks to affirm or challenge this hypothesis through a quantitative investigation into the origins of A-AB (i.e. I08S) bottom <span class="hlt">water</span>. The investigation takes the form of an Extended Optimum MultiParameter mixing analysis (eOMP) to determine a) the contribution of individual formation regions to the bottom <span class="hlt">water</span> seen at I08S, and b) how these contributions may have changed over the twenty years since the first occupation of the line. The initial investigation that used mean source <span class="hlt">water</span> properties found Adélie Bottom <span class="hlt">Water</span> (ADLBW) to be the dominant source of AABW in the A-AB. However, by calculating source <span class="hlt">water</span> properties from times preceding the occupations of the I08S line (1994, 2007, 2016), it was determined that in both 1994 and 2007, Ross Sea Bottom <span class="hlt">Water</span> (RSBW) was the dominant source of AABW (approx. 61 & 75 %, respectively) in the A-AB. This dominance shifted in 2016, to ADLBW composing approximately 44% of AABW. This result suggests that it is feasible that the B9b calving that impacted ADLBW in the formation region is, at least, partially responsible for the changes seen at I08S. Nevertheless, given that there are significant contributions from both RSBW and Weddell Sea Bottom <span class="hlt">Water</span>, it seems unlikely that this single alteration of ADLBW is the sole driver of the observed freshening. Further investigation seeks to determine the sensitivity of the solution to particular source <span class="hlt">water</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1998Natur.392..708T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1998Natur.392..708T"><span>Ecological importance of the Southern Boundary of the <span class="hlt">Antarctic</span> Circumpolar Current</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tynan, Cynthia T.</p> <p>1998-04-01</p> <p>The Southern Ocean surrounds the <span class="hlt">Antarctic</span> continent and supports one of the most productive marine ecosystems. Migratory and endemic species of whales, seals and birds benefit from the high biomass of their principal prey, krill (Euphausia superba) and cephalopods, in this area. Most species of baleen whales and male sperm whales in the Southern Hemisphere migrate between low-latitude breeding grounds in winter and highly productive <span class="hlt">Antarctic</span> feeding grounds in summer. Here I show the importance of the southernmost reaches of the strongest ocean current, the <span class="hlt">Antarctic</span> Circumpolar Current (ACC), to a complex and predictable food web of the Southern Ocean. The circumpolar distributions of blue, fin and humpback whales from spring to midsummer trace the non-uniform high-latitude penetration of shoaled, nutrient-rich Upper Circumpolar Deep <span class="hlt">Water</span>, which is carried eastward by the ACC. The poleward extent of this <span class="hlt">water</span> mass delineates the Southern Boundary of the ACC and corresponds not only to the circumpolar distributions of baleen whales, but also to distributions of krill and to regions of high, seasonally averaged, phytoplankton biomass. Sperm whales, which feed on cephalopods, also congregate in highest densities near the Southern Boundary. The association of primary production, Krill, and whales with the Southern Boundary, suggests that it provides predictably productive foraging for many species, and is of critical importance to the function of the Southern Ocean ecosystem.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17082741','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17082741"><span>Lichen flora around the Korean <span class="hlt">Antarctic</span> Scientific Station, King George Island, <span class="hlt">Antarctic</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kim, Ji Hee; Ahn, In-Young; Hong, Soon Gyu; Andreev, Mikhail; Lim, Kwang-Mi; Oh, Mi Jin; Koh, Young Jin; Hur, Jae-Seoun</p> <p>2006-10-01</p> <p>As part of the long-term monitoring projects on <span class="hlt">Antarctic</span> terrestrial vegetation in relation to global climate change, a lichen floristical survey was conducted around the Korean <span class="hlt">Antarctic</span> Station (King Sejong Station), which is located on Barton Peninsula, King George Island, in January and February of 2006. Two hundred and twenty-five lichen specimens were collected and sixty-two lichen species in 38 genera were identified by morphological characteristics, chemical constituents, TLC analysis and ITS nucleotide sequence analysis.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20020039046','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20020039046"><span>RADARSAT: The <span class="hlt">Antarctic</span> Mapping Project</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Jezek, Kenneth C.; Lindstrom, E. (Technical Monitor)</p> <p>2002-01-01</p> <p>The first <span class="hlt">Antarctic</span> Imaging Campaign (AIC) occurred during the period September 9, 1997 through October 20, 1997. The AIC utilized the unique attributes of the Canadian RADARSAT-1 to acquire the first, high-resolution, synthetic aperture imagery covering the entire <span class="hlt">Antarctic</span> Continent. Although the primary goal of the mission was the acquisition of image data, the nearly flawless execution of the mission enabled additional collections of exact repeat orbit data. These data, covering an extensive portion of the interior <span class="hlt">Antarctic</span>, potentially are suitable for interferometric analysis of topography and surface velocity. This document summarizes the Project through completion with delivery of products to the NASA DAACs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26667909','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26667909"><span>Advances in modelling subglacial lakes and their interaction with the <span class="hlt">Antarctic</span> ice sheet.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Pattyn, Frank; Carter, Sasha P; Thoma, Malte</p> <p>2016-01-28</p> <p>Subglacial lakes have long been considered hydraulically isolated <span class="hlt">water</span> bodies underneath ice sheets. This view changed radically with the advent of repeat-pass satellite altimetry and the discovery of multiple lake discharges and <span class="hlt">water</span> infill, associated with <span class="hlt">water</span> transfer over distances of more than 200 km. The presence of subglacial lakes also influences ice dynamics, leading to glacier acceleration. Furthermore, subglacial melting under the <span class="hlt">Antarctic</span> ice sheet is more widespread than previously thought, and subglacial melt rates may explain the availability for <span class="hlt">water</span> storage in subglacial lakes and <span class="hlt">water</span> transport. Modelling of subglacial <span class="hlt">water</span> discharge in subglacial lakes essentially follows hydraulics of subglacial channels on a hard bed, where ice sheet surface slope is a major control on triggering subglacial lake discharge. Recent evidence also points to the development of channels in deformable sediment in West Antarctica, with significant <span class="hlt">water</span> exchanges between till and ice. Most active lakes drain over short time scales and respond rapidly to upstream variations. Several <span class="hlt">Antarctic</span> subglacial lakes exhibit complex interactions with the ice sheet due to <span class="hlt">water</span> circulation. Subglacial lakes can therefore-from a modelling point of view-be seen as confined small oceans underneath an imbedded ice shelf. © 2015 The Author(s).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27643668','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27643668"><span>Heterolobosean amoebae from Arctic and <span class="hlt">Antarctic</span> extremes: 18 novel strains of Allovahlkampfia, Vahlkampfia and Naegleria.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tyml, Tomáš; Skulinová, Kateřina; Kavan, Jan; Ditrich, Oleg; Kostka, Martin; Dyková, Iva</p> <p>2016-10-01</p> <p>The diversity of heterolobosean amoebae, important members of soil, marine and freshwater microeukaryote communities in the temperate zones, is greatly under-explored in high latitudes. To address this imbalance, we studied the diversity of this group of free-living amoebae in the Arctic and the <span class="hlt">Antarctic</span> using culture dependent methods. Eighteen strain representatives of three heterolobosean genera, Allovahlkampfia Walochnik et Mulec, 2009 (1 strain), Vahlkampfia Chatton et Lalung-Bonnaier, 1912 (2) and Naegleria Alexeieff, 1912 (15) were isolated from 179 samples of wet soil and fresh <span class="hlt">water</span> with sediments collected in 6 localities. The Allovahkampfia strain is the first representative of the genus from the <span class="hlt">Antarctic</span>; 14 strains (7 from the Arctic, 7 from the <span class="hlt">Antarctic</span>) of the highly represented genus Naegleria complete the 'polar' cluster of five Naegleria species previously known from the Arctic and Sub-<span class="hlt">Antarctic</span> regions, whereas one strain enriches the 'dobsoni' cluster of Naegleria strains of diverse origin. Present isolations of Naegleria polarisDe Jonckheere, 2006 from Svalbard, in the Arctic and Vega Island, in the <span class="hlt">Antarctic</span> and N. neopolarisDe Jonckheere, 2006 from Svalbard and Greenland in the Arctic, and James Ross Island, the <span class="hlt">Antarctic</span> demonstrate their bipolar distribution, which in free-living amoebae has so far only been known for Vermistella Morand et Anderson, 2007. Copyright © 2016 Elsevier GmbH. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19295608','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19295608"><span>Modelling West <span class="hlt">Antarctic</span> ice sheet growth and collapse through the past five million years.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Pollard, David; DeConto, Robert M</p> <p>2009-03-19</p> <p>The West <span class="hlt">Antarctic</span> ice sheet (WAIS), with ice volume equivalent to approximately 5 m of sea level, has long been considered capable of past and future catastrophic collapse. Today, the ice sheet is fringed by vulnerable floating ice shelves that buttress the fast flow of inland ice streams. Grounding lines are several hundred metres below sea level and the bed deepens upstream, raising the prospect of runaway retreat. Projections of future WAIS behaviour have been hampered by limited understanding of past variations and their underlying forcing mechanisms. Its variation since the Last Glacial Maximum is best known, with grounding lines advancing to the continental-shelf edges around approximately 15 kyr ago before retreating to near-modern locations by approximately 3 kyr ago. Prior collapses during the warmth of the early Pliocene epoch and some Pleistocene interglacials have been suggested indirectly from records of sea level and deep-sea-core isotopes, and by the discovery of open-ocean diatoms in subglacial sediments. Until now, however, little direct evidence of such behaviour has been available. Here we use a combined ice sheet/ice shelf model capable of high-resolution nesting with a new treatment of grounding-line dynamics and ice-shelf buttressing to simulate <span class="hlt">Antarctic</span> ice sheet variations over the past five million years. Modelled WAIS variations range from full glacial extents with grounding lines near the continental shelf break, <span class="hlt">intermediate</span> states similar to modern, and brief but dramatic retreats, leaving only small, isolated ice caps on West <span class="hlt">Antarctic</span> islands. Transitions between glacial, <span class="hlt">intermediate</span> and collapsed states are relatively rapid, taking one to several thousand years. Our simulation is in good agreement with a new sediment record (ANDRILL AND-1B) recovered from the western Ross Sea, indicating a long-term trend from more frequently collapsed to more glaciated states, dominant 40-kyr cyclicity in the Pliocene, and major retreats at</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17..233W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17..233W"><span>The <span class="hlt">Antarctic</span> Ice Sheet during the last Interglaciation: Insights from my Thesis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Whipple, Matthew; Lunt, Dan; Singarayer, Joy; Bradley, Sarah; Milne, Glenn; Wolff, Eric; Siddall, Mark</p> <p>2015-04-01</p> <p>The last interglaciation represents a period of warmer climates and higher sea levels, and a useful analogue to future climate. While many studies have focussed on the response of the Greenland Ice sheet, far less is known about the response of the <span class="hlt">Antarctic</span> ice sheet. Here, I present the summarised results of my PhD thesis "Constraints on the minimum extent of the <span class="hlt">Antarctic</span> ice sheet during the last interglaciation". Firstly, I cover the timings of interglaciation in Antarctica, and their differences with respect to the Northern Hemisphere timings, based on paleo sea level indicators, and oceanic temperature records. I move on to cover climate forcings, and how they influence the ice sheet, relative to present, and early Holocene. Secondly, I present thesis results, from looking at ice core stable <span class="hlt">water</span> isotopes. These are compared with Isostatic and Climatic modelling results, for various different Ice sheet scenarios, as to the resulting Climate, from changes in Elevation, Temperature, Precipitation, and Sublimation, all contributing to the recorded stable <span class="hlt">water</span> isotope record. Thirdly, I move on to looking at the mid-field relative sea level records, from Australia and Argentina. Using isostatic modelling, these are used to assess the relative contribution of the Eastern and Western <span class="hlt">Antarctic</span> Ice sheets. Although data uncertainties result in us being to identify the contribution from West Antarctica. Overall, using model-data comparison, we find a lack of evidence for a substantial retreat of the Wilkes Subglacial basin. No data location is close enough to determine the existence of the marine based West <span class="hlt">Antarctic</span> Ice sheet. Model uncertainty is unable to constrain evidence of variations in ice thickness in East Antarctica.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_11 --> <div id="page_12" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="221"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28955055','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28955055"><span>Peatland Ecosystem Processes in the Maritime <span class="hlt">Antarctic</span> During Warm Climates.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Loisel, Julie; Yu, Zicheng; Beilman, David W; Kaiser, Karl; Parnikoza, Ivan</p> <p>2017-09-27</p> <p>We discovered a 50-cm-thick peat deposit near Cape Rasmussen (65.2°S), in the maritime <span class="hlt">Antarctic</span>. To our knowledge, while aerobic 'moss banks' have often been examined, waterlogged 'peatlands' have never been described in this region before. The waterlogged system is approximately 100 m 2 , with a shallow <span class="hlt">water</span> table. Surface vegetation is dominated by Warnstorfia fontinaliopsis, a wet-adapted moss commonly found in the <span class="hlt">Antarctic</span> Peninsula. Peat inception was dated at 2750 cal. BP and was followed by relatively rapid peat accumulation (~0.1 cm/year) until 2150 cal. BP. Our multi-proxy analysis then shows a 2000-year-long stratigraphic hiatus as well as the recent resurgence of peat accumulation, sometime after 1950 AD. The existence of a thriving peatland at 2700-2150 cal. BP implies regionally warm summer conditions extending beyond the mid-Holocene; this finding is corroborated by many regional records showing moss bank initiation and decreased sea ice extent during this time period. Recent peatland recovery at the study site (<50 years ago) might have been triggered by ongoing rapid warming, as the area is experiencing climatic conditions approaching those found on milder, peatland-rich sub-<span class="hlt">Antarctic</span> islands (50-60°S). Assuming that colonization opportunities and stabilization mechanisms would allow peat to persist in Antarctica, our results suggest that longer and warmer growing seasons in the maritime <span class="hlt">Antarctic</span> region may promote a more peatland-rich landscape in the future.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19910017799','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19910017799"><span>Solutions to problems of weathering in <span class="hlt">Antarctic</span> eucrites</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Strait, Melissa M.</p> <p>1990-01-01</p> <p>Neutron activation analysis was performed for major and trace elements on a suite of eucrites from both <span class="hlt">Antarctic</span> and non-<span class="hlt">Antarctic</span> sources. The chemistry was examined to see if there was an easy way to distinguish <span class="hlt">Antarctic</span> eucrites that had been disturbed in their trace elements systematics from those that had normal abundances relative to non-<span class="hlt">Antarctic</span> eucrites. There was no simple correlation found, and identifying the disturbed meteorites still remains a problem. In addition, a set of mineral separates from an eucrite were analyzed. The results showed no abnormalities in the chemistry and provides a possible way to use <span class="hlt">Antarctic</span> eucrites that were disturbed in modelling of the eucrite parent body.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMPP13D..01O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMPP13D..01O"><span>Deglacial Evolution of Atlantic Mid-Depth and <span class="hlt">Intermediate</span>-Depth <span class="hlt">Water</span> Variability</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Oppo, D.; Gebbie, G.; Huang, K. F.; Guo, W.; Schmittner, A.; Liu, Z.; Curry, W. B.</p> <p>2014-12-01</p> <p>Deglacial variations in the Atlantic Meridional Overturning Circulation (AMOC) feature prominently in hypotheses of deglacial climate variability and atmospheric CO2rise. However, there is lingering uncertainty in the glacial deepwater mass configuration (e.g. Gebbie, 2014) and deglacial AMOC variability is even more poorly understood. For example, the deglacial evolution of the contribution of northern and southern source <span class="hlt">waters</span> to the middle and <span class="hlt">intermediate</span> depths of the Atlantic is still vigorously debated. Here, we evaluate the evolution of subsurface Atlantic ventilation, emphasizing middle and <span class="hlt">intermediate</span> depths, by comparing new and published records of <span class="hlt">water</span> mass variability to output from transient model simulations designed to provide insight into the climatic and oceanographic effects of a dramatic reduction in the AMOC, such as apparently occurred during Heinrich Stadial 1 (Liu et al., 2009; Schmittner and Lund, 2014). Gebbie, G. (2014), How much did Glacial North Atlantic <span class="hlt">Water</span> shoal? Paleoceanography, 29, 190-209, doi: 10.1002/2013PA002557. Liu, Z., B. Otto-Bliesner, F. He, E. Brady, R. Thomas, P. U. Clark, A. E. Carlson, J. Lynch-Stieglitz, W. Curry, E. Brook, D. Erickson, R. Jacob, J. Kutzbach, J., and J. Chen (2009), Transient climate simulation of last deglaciation with a new mechanism for Bølling-Allerød warming, Science, 325, 310-314. Schmittner, A., and Lund, D. C. (submitted), Carbon Isotopes Support Atlantic Meridional Overturning Circulation Decline as a Trigger for Early Deglacial CO2 rise Climate of the Past Discussions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19930010628','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19930010628"><span><span class="hlt">Antarctic</span> lakes (above and beneath the ice sheet): Analogues for Mars</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rice, J. W., Jr.</p> <p>1992-01-01</p> <p>The perennial ice covered lakes of the <span class="hlt">Antarctic</span> are considered to be excellent analogues to lakes that once existed on Mars. Field studies of ice covered lakes, paleolakes, and polar beaches were conducted in the Bunger Hills Oasis, Eastern Antarctica. These studies are extended to the Dry Valleys, Western Antarctica, and the Arctic. Important distinctions were made between ice covered and non-ice covered bodies of <span class="hlt">water</span> in terms of the geomorphic signatures produced. The most notable landforms produced by ice covered lakes are ice shoved ridges. These features form discrete segmented ramparts of boulders and sediments pushed up along the shores of lakes and/or seas. Sub-ice lakes have been discovered under the <span class="hlt">Antarctic</span> ice sheet using radio echo sounding. These lakes occur in regions of low surface slope, low surface accumulations, and low ice velocity, and occupy bedrock hollows. The presence of sub-ice lakes below the Martian polar caps is possible. The discovery of the <span class="hlt">Antarctic</span> sub-ice lakes raises possibilities concerning Martian lakes and exobiology.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFMPP12A..03S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMPP12A..03S"><span>The circum-<span class="hlt">Antarctic</span> sedimentary record; a dowsing rod for <span class="hlt">Antarctic</span> ice in 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>Scher, H.</p> <p>2012-12-01</p> <p> where δ18O values are low and decrease to -15.5 when δ18O values are highest. In contrast there is not a significant change in the ɛNd values of fossil fish teeth across the δ18O excursion at ODP Site 738. Low variability in fossil fish tooth ɛNd values precludes a major reorganization of bottom <span class="hlt">water</span> circulation that may otherwise have transported terrigenous sediment from distal areas. Thus, the results from this study provide very strong evidence for an increase in the amount of fine-grained terrigenous material that was discharged from the Prydz Bay drainage and/or a change in the sediment source. I argue that these data provide evidence for erosion/weathering of <span class="hlt">Antarctic</span> basement rocks by small ice sheets that formed in the hinterland of the Prydz Bay drainage. The approach that will be presented holds great promise for identifying short-lived glaciations on Antarctica prior to the major development of ice sheets at the Eocene Oligocene boundary. Understanding the timing, frequency, and duration of these events is paramount to evaluating the processes and feedbacks that resulted in the global transition from greenhouse to icehouse. References: Roy, M., et al. (2007), Chemical Geology, 244, 507-519. van de Flierdt T, Goldstein SL, Hemming SR, et al, Earth and Planetary Science Letters, 2007, 259, Pages:432-441.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.G43A1033W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.G43A1033W"><span>Combustion of available fossil-fuel resources sufficient to eliminate the <span class="hlt">Antarctic</span> Ice Sheet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Winkelmann, R.; Levermann, A.; Ridgwell, A.; Caldeira, K.</p> <p>2015-12-01</p> <p>The <span class="hlt">Antarctic</span> Ice Sheet stores <span class="hlt">water</span> equivalent to 58 meters in global sea-level rise. Here we show in simulations with the Parallel Ice Sheet Model that burning the currently attainable fossil-fuel resources is sufficient to eliminate the ice sheet. With cumulative fossil-fuel emissions of 10 000 GtC, Antarctica is projected to become almost ice-free with an average contribution to sea-level rise exceeding 3 meters per century during the first millennium. Consistent with recent observations and simulations, the West <span class="hlt">Antarctic</span> Ice Sheet becomes unstable with 600 to 800 GtC of additional carbon emissions. Beyond this additional carbon release, the destabilization of ice basins in both West- and East Antarctica results in a threshold-increase in global sea level. Unabated carbon emissions thus threaten the <span class="hlt">Antarctic</span> Ice Sheet in its entirety with associated sea-level rise that far exceeds that of all other possible sources.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19860019351','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19860019351"><span>Trace elements in <span class="hlt">Antarctic</span> meteorites: Weathering and genetic information</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lipschutz, M. E.</p> <p>1986-01-01</p> <p><span class="hlt">Antarctic</span> meteorite discoveries have created great scientific interest due to the large number of specimens recovered (approximately 7000) and because included are representatives of hitherto rare or unknown types. <span class="hlt">Antarctic</span> meteorites are abundant because they have fallen over long periods and were preserved, transported, and concentrated by the ice sheets. The weathering effects on the <span class="hlt">Antarctic</span> meteorites are described. Weathering effects of trace element contents of H5 chondrites were studied in detail. The results are examined. The properties of <span class="hlt">Antarctic</span> finds and non-<span class="hlt">Antarctic</span> falls are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017DSRII.138....1S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017DSRII.138....1S"><span>Eddy-Pump: Pelagic carbon pump processes along the eddying <span class="hlt">Antarctic</span> Polar Front in the Atlantic Sector of the Southern Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Strass, Volker H.; Wolf-Gladrow, Dieter; Pakhomov, Evgeny A.; Klaas, Christine</p> <p>2017-04-01</p> <p>The Southern Ocean influences earth's climate in many ways. It hosts the largest upwelling region of the world oceans where 80% of deep <span class="hlt">waters</span> resurface (Morrison et al., 2015). A prominent feature is the broad ring of cold <span class="hlt">water</span>, the <span class="hlt">Antarctic</span> Circumpolar Current (ACC), which encircles the <span class="hlt">Antarctic</span> continent and connects all other oceans. The ACC plays a major role in the global heat and freshwater transports and ocean-wide cycles of chemical and biogenic elements, and harbours a series of unique and distinct ecosystems. Due to the upwelling of deep-<span class="hlt">water</span> masses in the <span class="hlt">Antarctic</span> Divergence, there is high supply of natural CO2 as well as macronutrients, leading to the worldwide highest surface nutrient concentrations. Despite the ample macronutrients supply, phytoplankton concentration is generally low, limited either by low micronutrient (iron) availability, insufficient light due to deep wind-mixed layers or grazing by zooplankton, or by the combination of all, varying temporally and regionally.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://rosap.ntl.bts.gov/view/dot/18418','DOTNTL'); return false;" href="https://rosap.ntl.bts.gov/view/dot/18418"><span><span class="hlt">Antarctic</span> climate change and the environment</span></a></p> <p><a target="_blank" href="http://ntlsearch.bts.gov/tris/index.do">DOT National Transportation Integrated Search</a></p> <p></p> <p>2009-11-01</p> <p>This volume provides a comprehensive, up-to-date account of how the physical and biological : environment of the <span class="hlt">Antarctic</span> continent and Southern Ocean has changed from Deep Time until : the present day. It also considers how the <span class="hlt">Antarctic</span> environmen...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20455435','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20455435"><span>[Microbiological analysis of terrestrial biotopes of the <span class="hlt">Antarctic</span> region].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tashirev, A B; Romanovskaia, V A; Rokitko, P V; Shilin, S O; Chernaia, N A; Tashireva, A A</p> <p>2010-01-01</p> <p>Microbiological analysis has been made of 120 samples from biotopes of the western coast of the <span class="hlt">Antarctic</span> peninsula (Rasmussen cope, Tuxen cope, Waugh mountain), Argentine archipelago islands (Galindez, Skua, Corner, Barchans, Irizar, Uruguay, Cluls, Three Little Pigs, King-George), as well as neighbouring islands (Petermann--on the north, a group of Jalour islands--on the east, Berthelot--on the south-east); and more remote islands (Darboux, Lippmann, Booth). It was found out that the total number of chemoorganotrophic aerobic microorganisms was 10(6) - 10(8) cells/g of soil, that was by 2-3 orders lower than in the regions with temperate climate. One can observe a tendency of decreasing the quantity of chemoorganotrophic microorganisms in the Antartic biotopes (cells/g of a sample) in the following order: soil (1 x 10(7) - 8 x 10(8)), underground part of moss (1 x 10(6) - 5 x 10(7)), grass Deschampsia antarctica (10(6) - 10(8), slit of fresh-<span class="hlt">water</span> reservoir (10(5) - 10(7)), ground part of moss (10(3) - 10(6)), lichens (10(3) - 10(6)). Representatives of several phylogenetic lines: Proteobacteria (genera Pseudomonas, Methylobacterium, Enterobacter), Firmicutes (genera Bacillus, Staphylococcus), Actinobacteria (genera Brevibacterium, Actinomyces, Streptomyces) have been found in the <span class="hlt">Antarctic</span> samples. As a rule, genera of bacteria found in the <span class="hlt">Antarctic</span> Region are widely distributed in different regions of the Earth with temperate climate. Microorganisms similar to the species Exophiala nigra (Issatsch.) Haats et de Hoog 1999, which was first detected 100 years ago by Academician B.L. Isachenko in the Arctic region <span class="hlt">water</span>, were also isolated from biofilms on vertical rocks of the Galindez Island as well as from the soil of the Irizar Island.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2012-08-06/pdf/2012-19116.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2012-08-06/pdf/2012-19116.pdf"><span>77 FR 46771 - Notice of Permit Application Received Under the <span class="hlt">Antarctic</span> Conservation Act of 1978</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>2012-08-06</p> <p>... emissions and waste <span class="hlt">water</span> (urine, grey- <span class="hlt">water</span>, and human solid waste. All wastes would be packaged and... (NSF) has received a waste management permit application for Quark Expeditions' cruise ships to conduct...-8030. SUPPLEMENTARY INFORMATION: NSF's <span class="hlt">Antarctic</span> Waste Regulation, 45 CFR Part 671, requires all U.S...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21675047','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21675047"><span>[History of Polish botanical and mycological researches on sheets of land of <span class="hlt">Antarctic</span> and Sub-<span class="hlt">Antarctic</span> in the years 1977-2009].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Köhler, Piotr; Olech, Maria</p> <p>2011-01-01</p> <p>The work includes a description of the period from the moment of setting up Polish Polar Station on King George Island (1977) to the end of International Polar Year IV in 2009. Researches on flower plants focused, among others, on plants' morphology, morphological composition of the pollen and anatomical ultra-structure of the leaves. There were also carried out biochemical and other searches for the internal mutability. Within physiological studies one concentrated on the problem of reaction to temperature stress. Biological researches focused mainly on solving taxonomic and bio-geographic problems. Finally, were published several monographs and, among others, the first in history complete description of moss' flora of the whole of <span class="hlt">Antarctic</span> (2008). Research works over algae included also such issues as floristics, bio-geography, taxonomy and ecology (for instance, the rookery's impact on distribution of algae, or the influence of inanimate factors on dynamics of condensing the Diatoma in different <span class="hlt">water</span> and soil-bound tanks). Up till now, within mycological investigations has been identified a variety of lichen fungi that for the most part of <span class="hlt">Antarctic</span> are a novelty. There were scientifically described new for science genera and species of Western <span class="hlt">Antarctic</span>. Lichenological studies were made in the field of taxonomy, geography, lichenometry, biochemistry of lichens, lichenoindication, ecophysiology and from the point of analysis of base metals' content. There were also described new for science species. Since 1991, were published the results of searches for the base metals' content and vestigial chemical elements in lichens' thallus. Ecophysiological researches concerned both micro-climatic conditions' impact on primary production and lichens' adaptation to a very cold climate. One discovered a mechanism of two-phase hydratization/dehydratization of lichens' thallus. On the ground of palaeobotanical analyzes was reconstructed a development of flora in Western</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-GSFC_20171208_Archive_e002122.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-GSFC_20171208_Archive_e002122.html"><span>NASA finds Shrimp Under <span class="hlt">Antarctic</span> Ice [Video</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2017-12-08</p> <p>At a depth of 600 feet beneath the West <span class="hlt">Antarctic</span> ice sheet, a small shrimp-like creature managed to brighten up an otherwise gray polar day in late November 2009. This critter is a three-inch long Lyssianasid amphipod found beneath the Ross Ice Shelf, about 12.5 miles away from open <span class="hlt">water</span>. NASA scientists were using a borehole camera to look back up towards the ice surface when they spotted this pinkish-orange creature swimming beneath the ice. Credit: NASA</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014cfeb.conf..109Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014cfeb.conf..109Y"><span>Features of the Functioning Bacterial Ecosystems in the <span class="hlt">Antarctic</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yakushev, A. V.; Churilin, N.; Soina, V. S.; Vorobyova, E. A.; Mergelov, N. S.</p> <p>2014-10-01</p> <p>Studies of bacterial communities in the samples of <span class="hlt">Antarctic</span> soils by different methods showed that, both in liquid soil suspensions and in situ, microbial complexes are functioning presumably by forming biofilms -- the phenomenon that is more expressed in such habitat than in soils of temperate zones. Functional (trophic) diversity and physiological state of hydrolytic bacteria was studied in the samples at the upper layer (0-2 cm) of gravel pavement with algae, in the underlying peat horizon (2-4 cm) with inclusions of dead biomass and its underlying mineral horizon (4-10 cm) with signs of fungal mycelium. The investigated samples of <span class="hlt">Antarctic</span> soils revealed different trophic diversity and the maximum specific growth rate on mineral medium with different biopolymers as the sole carbon source (starch, chitin, pectin, xylan, dextran-500, tween-20, casein); this can testify to differences in the physiological state of hydrolytic bacteria in various soil horizons and their readiness for growth. The most remarkable characteristics of the studied <span class="hlt">Antarctic</span> soil as compared to the soils of temperate zone, was the unusual ability of hydrolytic community to consume chitin in the mineral horizon; this can be explained by the presence of fungal mycelium. Also, an almost complete lack in consumption of tween-20 (a <span class="hlt">water</span>-soluble analogue of fat) by bacterial community of Arctic soil horizons are not explained and needs further verification. The higher functional diversity was detected in the upper horizon of the gravel pavement, which "protects" microorganisms from exposure to extreme temperatures, UV radiation, and desiccation, but the maximum specific growth rate was higher in the lower mineral horizon; this can be explained by the specificity of bacterial colonizing processes and unique formation of <span class="hlt">Antarctic</span> soil microprofiles in the Larsemann oasis. The obtained data indicate a specific environmental strategy in the samples of <span class="hlt">Antarctic</span> soils: development in lower</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSME14C0619C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSME14C0619C"><span>Investigation of <span class="hlt">Antarctic</span> Marine Metazoan Biodiversity Through Metagenomic Analysis of Environmental DNA</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cowart, D. A.; Cheng, C. C.; Murphy, K.</p> <p>2016-02-01</p> <p>Environmental DNA (eDNA), or DNA extracted from environmental collections, is frequently used to gauge biodiversity and identify the presence of rare or invasive species within a habitat. Previous studies have demonstrated that compared to traditional surveying methods, high-throughput sequencing of eDNA can provide increased detection sensitivity of aquatic taxa, holding promise for various conservation applications. To determine the potential of eDNA for assessing biodiversity of <span class="hlt">Antarctic</span> marine metazoan communities, we have extracted eDNA from seawater sampled from four regions near Palmer Station in West <span class="hlt">Antarctic</span> Peninsula. Metagenomic sequencing of the eDNA was performed on Illumina HiSeq2500, and produced 325 million quality-processed reads. Preliminary read mapping for two regions, Gerlache Strait and Bismarck Strait, identified approximately 4% of reads mapping to eukaryotes for each region, with >50% of the those reads mapping to metazoan animals. Key groups investigated include the nototheniidae family of <span class="hlt">Antarctic</span> fishes, to which 0.2 and 0.8 % of the metazoan reads were assigned for each region respectively. The presence of the recently invading lithodidae king crabs was also detected at both regions. Additionally, to estimate the persistence of eDNA in polar seawater, a rate of eDNA decay will be quantified from seawater samples collected over 20 days from <span class="hlt">Antarctic</span> fish holding tanks and held at ambient <span class="hlt">Antarctic</span> <span class="hlt">water</span> temperatures. The ability to detect animal signatures from eDNA, as well as the quantification of eDNA decay over time, could provide another method for reliable monitoring of polar habitats at various spatial and temporal scales.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19860019339','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19860019339"><span>International Workshop on <span class="hlt">Antarctic</span> Meteorites</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Annexstad, J. O.; Schultz, L.; Waenke, H.</p> <p>1986-01-01</p> <p>Topics addressed include: meteorite concentration mechanisms; meteorites and the <span class="hlt">Antarctic</span> ice sheet; iron meteorites; iodine overabundance in meteorites; entrainment, transport, and concentration of meteorites in polar ice sheets; weathering of stony meteorites; cosmic ray records; radiocarbon dating; element distribution and noble gas isotopic abundances in lunar meteorites; thermoanalytical characterization; trace elements; thermoluminescence; parent sources; and meteorite ablation and fusion spherules in <span class="hlt">Antarctic</span> ice.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26882535','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26882535"><span>Presence of endocrine disruptors in freshwater in the northern <span class="hlt">Antarctic</span> Peninsula region.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Esteban, S; Moreno-Merino, L; Matellanes, R; Catalá, M; Gorga, M; Petrovic, M; López de Alda, M; Barceló, D; Silva, A; Durán, J J; López-Martínez, J; Valcárcel, Y</p> <p>2016-05-01</p> <p>The increasing human presence in Antarctica and the waste it generates is causing an impact on the environment at local and border scale. The main sources of anthropic pollution have a mainly local effect, and include the burning of fossil fuels, waste incineration, accidental spillage and wastewater effluents, even when treated. The aim of this work is to determine the presence and origin of 30 substances of anthropogenic origin considered to be, or suspected of being, endocrine disruptors in the continental <span class="hlt">waters</span> of the <span class="hlt">Antarctic</span> Peninsula region. We also studied a group of toxic metals, metalloids and other elements with possible endocrine activity. Ten <span class="hlt">water</span> samples were analyzed from a wide range of sources, including streams, ponds, glacier drain, and an urban wastewater discharge into the sea. Surprisingly, the concentrations detected are generally similar to those found in other studies on continental <span class="hlt">waters</span> in other parts of the world. The highest concentrations of micropollutants found correspond to the group of organophosphate flame retardants (19.60-9209ngL(-1)) and alkylphenols (1.14-7225ngL(-1)); and among toxic elements the presence of aluminum (a possible hormonal modifier) (1.7-127µgL(-1)) is significant. The concentrations detected are very low and insufficient to cause acute or subacute toxicity in aquatic organisms. However, little is known as yet of the potential sublethal and chronic effects of this type of pollutants and their capacity for bioaccumulation. These results point to the need for an ongoing system of environmental monitoring of these substances in <span class="hlt">Antarctic</span> continental <span class="hlt">waters</span>, and the advisability of regulating at least the most environmentally hazardous of these in the <span class="hlt">Antarctic</span> legislation. Copyright © 2016 Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19980151107','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19980151107"><span>West-<span class="hlt">Antarctic</span> Ice Streams: Analog to Ice Flow in Channels on Mars</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lucchitta, B. K.</p> <p>1997-01-01</p> <p>Sounding of the sea floor in front of the Ross Ice Shelf in Antarctica recently revealed large persistent patterns of longitudinal megaflutes and drumlinoid forms, which are interpreted to have formed at the base of ice streams during the list glacial advance. The flutes bear remarkable resemblance to longitudinal grooves and highly elongated streamlined islands found on the floors of some large martian channels, called outflow channels. ln addition, other similarities exist between <span class="hlt">Antarctic</span> ice streams and outflow channels. Ice streams are 30 to 80 km wide and hundreds of kilometers long, as are the martian channels. Ice stream beds are below sea level. Floors of many martian outflow channels lie below martian datum, which may have been close to or below past martian sea levels. The <span class="hlt">Antarctic</span> ice stream bed gradient is flat and locally may go uphill, and surface slopes are exceptionally low. So are gradients of martian channels. The depth to the bed in ice streams is 1 to 1.5 km. At bankful stage, the depth of the fluid in outflow channels would have been 1 to 2 km. These similarities suggest that the martian outflow channels, whose origin is commonly attributed to gigantic catastrophic floods, were locally filled by ice that left a conspicuous morphologic imprint. Unlike the West-<span class="hlt">Antarctic</span>-ice streams, which discharge ice from an ice sheet, ice in the martian channels came from <span class="hlt">water</span> erupting from the ground. In the cold martian environment, this <span class="hlt">water</span>, if of moderate volume, would eventually freeze. Thus it may have formed icings on springs, ice dams and jams on constrictions in the channel path, or frozen pools. Given sufficient thickness and downhill surface gradient, these ice masses would have moved; and given the right conditions, they could have moved like <span class="hlt">Antarctic</span> ice streams.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/18524738','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/18524738"><span>Mitochondrial sequence divergence among <span class="hlt">Antarctic</span> killer whale ecotypes is consistent with multiple species.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>LeDuc, Richard G; Robertson, Kelly M; Pitman, Robert L</p> <p>2008-08-23</p> <p>Recently, three visually distinct forms of killer whales (Orcinus orca) were described from <span class="hlt">Antarctic</span> <span class="hlt">waters</span> and designated as types A, B and C. Based on consistent differences in prey selection and habitat preferences, morphological divergence and apparent lack of interbreeding among these broadly sympatric forms, it was suggested that they may represent separate species. To evaluate this hypothesis, we compared complete sequences of the mitochondrial control region from 81 <span class="hlt">Antarctic</span> killer whale samples, including 9 type A, 18 type B, 47 type C and 7 type-undetermined individuals. We found three fixed differences that separated type A from B and C, and a single fixed difference that separated type C from A and B. These results are consistent with reproductive isolation among the different forms, although caution is needed in drawing further conclusions. Despite dramatic differences in morphology and ecology, the relatively low levels of sequence divergence in <span class="hlt">Antarctic</span> killer whales indicate that these evolutionary changes occurred relatively rapidly and recently.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4643791','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4643791"><span>Combustion of available fossil fuel resources sufficient to eliminate the <span class="hlt">Antarctic</span> Ice Sheet</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Winkelmann, Ricarda; Levermann, Anders; Ridgwell, Andy; Caldeira, Ken</p> <p>2015-01-01</p> <p>The <span class="hlt">Antarctic</span> Ice Sheet stores <span class="hlt">water</span> equivalent to 58 m in global sea-level rise. We show in simulations using the Parallel Ice Sheet Model that burning the currently attainable fossil fuel resources is sufficient to eliminate the ice sheet. With cumulative fossil fuel emissions of 10,000 gigatonnes of carbon (GtC), Antarctica is projected to become almost ice-free with an average contribution to sea-level rise exceeding 3 m per century during the first millennium. Consistent with recent observations and simulations, the West <span class="hlt">Antarctic</span> Ice Sheet becomes unstable with 600 to 800 GtC of additional carbon emissions. Beyond this additional carbon release, the destabilization of ice basins in both West and East Antarctica results in a threshold increase in global sea level. Unabated carbon emissions thus threaten the <span class="hlt">Antarctic</span> Ice Sheet in its entirety with associated sea-level rise that far exceeds that of all other possible sources. PMID:26601273</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_12 --> <div id="page_13" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="241"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26601273','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26601273"><span>Combustion of available fossil fuel resources sufficient to eliminate the <span class="hlt">Antarctic</span> Ice Sheet.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Winkelmann, Ricarda; Levermann, Anders; Ridgwell, Andy; Caldeira, Ken</p> <p>2015-09-01</p> <p>The <span class="hlt">Antarctic</span> Ice Sheet stores <span class="hlt">water</span> equivalent to 58 m in global sea-level rise. We show in simulations using the Parallel Ice Sheet Model that burning the currently attainable fossil fuel resources is sufficient to eliminate the ice sheet. With cumulative fossil fuel emissions of 10,000 gigatonnes of carbon (GtC), Antarctica is projected to become almost ice-free with an average contribution to sea-level rise exceeding 3 m per century during the first millennium. Consistent with recent observations and simulations, the West <span class="hlt">Antarctic</span> Ice Sheet becomes unstable with 600 to 800 GtC of additional carbon emissions. Beyond this additional carbon release, the destabilization of ice basins in both West and East Antarctica results in a threshold increase in global sea level. Unabated carbon emissions thus threaten the <span class="hlt">Antarctic</span> Ice Sheet in its entirety with associated sea-level rise that far exceeds that of all other possible sources.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28970064','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28970064"><span>Cross-disciplinarity in the advance of <span class="hlt">Antarctic</span> ecosystem research.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gutt, J; Isla, E; Bertler, A N; Bodeker, G E; Bracegirdle, T J; Cavanagh, R D; Comiso, J C; Convey, P; Cummings, V; De Conto, R; De Master, D; di Prisco, G; d'Ovidio, F; Griffiths, H J; Khan, A L; López-Martínez, J; Murray, A E; Nielsen, U N; Ott, S; Post, A; Ropert-Coudert, Y; Saucède, T; Scherer, R; Schiaparelli, S; Schloss, I R; Smith, C R; Stefels, J; Stevens, C; Strugnell, J M; Trimborn, S; Verde, C; Verleyen, E; Wall, D H; Wilson, N G; Xavier, J C</p> <p>2018-02-01</p> <p>The biodiversity, ecosystem services and climate variability of the <span class="hlt">Antarctic</span> continent and the Southern Ocean are major components of the whole Earth system. <span class="hlt">Antarctic</span> ecosystems are driven more strongly by the physical environment than many other marine and terrestrial ecosystems. As a consequence, to understand ecological functioning, cross-disciplinary studies are especially important in <span class="hlt">Antarctic</span> research. The conceptual study presented here is based on a workshop initiated by the Research Programme <span class="hlt">Antarctic</span> Thresholds - Ecosystem Resilience and Adaptation of the Scientific Committee on <span class="hlt">Antarctic</span> Research, which focussed on challenges in identifying and applying cross-disciplinary approaches in the <span class="hlt">Antarctic</span>. Novel ideas and first steps in their implementation were clustered into eight themes. These ranged from scale problems, through risk maps, and organism/ecosystem responses to multiple environmental changes and evolutionary processes. Scaling models and data across different spatial and temporal scales were identified as an overarching challenge. Approaches to bridge gaps in <span class="hlt">Antarctic</span> research programmes included multi-disciplinary monitoring, linking biomolecular findings and simulated physical environments, as well as integrative ecological modelling. The results of advanced cross-disciplinary approaches can contribute significantly to our knowledge of <span class="hlt">Antarctic</span> and global ecosystem functioning, the consequences of climate change, and to global assessments that ultimately benefit humankind. Crown Copyright © 2017. Published by Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GPC...166...62C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GPC...166...62C"><span>Ocean as the main driver of <span class="hlt">Antarctic</span> ice sheet retreat during the Holocene</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Crosta, Xavier; Crespin, Julien; Swingedouw, Didier; Marti, Olivier; Masson-Delmotte, Valérie; Etourneau, Johan; Goosse, Hugues; Braconnot, Pascale; Yam, Ruth; Brailovski, Irena; Shemesh, Aldo</p> <p>2018-07-01</p> <p>Ocean-driven basal melting has been shown to be the main ablation process responsible for the recession of many <span class="hlt">Antarctic</span> ice shelves and marine-terminating glaciers over the last decades. However, much less is known about the drivers of ice shelf melt prior to the short instrumental era. Based on diatom oxygen isotope (δ18Odiatom; a proxy for glacial ice discharge in solid or liquid form) records from western <span class="hlt">Antarctic</span> Peninsula (West Antarctica) and Adélie Land (East Antarctica), higher ocean temperatures were suggested to have been the main driver of enhanced ice melt during the Early-to-Mid Holocene while atmosphere temperatures were proposed to have been the main driver during the Late Holocene. Here, we present a new Holocene δ18Odiatom record from Prydz Bay, East Antarctica, also suggesting an increase in glacial ice discharge since 4500 years before present ( 4.5 kyr BP) as previously observed in <span class="hlt">Antarctic</span> Peninsula and Adélie Land. Similar results from three different regions around Antarctica thus suggest common driving mechanisms. Combining marine and ice core records along with new transient accelerated simulations from the IPSL-CM5A-LR climate model, we rule out changes in air temperatures during the last 4.5 kyr as the main driver of enhanced glacial ice discharge. Conversely, our simulations evidence the potential for significant warmer subsurface <span class="hlt">waters</span> in the Southern Ocean during the last 6 kyr in response to enhanced summer insolation south of 60°S and enhanced upwelling of Circumpolar Deep <span class="hlt">Water</span> towards the <span class="hlt">Antarctic</span> shelf. We conclude that ice front and basal melting may have played a dominant role in glacial discharge during the Late Holocene.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19920012068','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19920012068"><span>Movement of Trace Elements During Residence in the <span class="hlt">Antarctic</span> Ice: a Laboratory Simulation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Strait, Melissa M.</p> <p>1991-01-01</p> <p>Recent work has determined that differences in the trace element distribution between <span class="hlt">Antarctic</span> eucrites and non-<span class="hlt">Antarctic</span> eucrites may be due to weathering during residence in the ice, and samples that demonstrate trace element disturbances do not necessarily correspond to eucrites that appear badly weathered to the naked eye. This study constitutes a preliminary test of the idea that long-term residence in the ice is the cause of the trace element disturbances observed in the eucrites. Samples of a non-<span class="hlt">Antarctic</span> eucrite were leached in <span class="hlt">water</span> at room temperature conditions. Liquid samples were analyzed for rare earth element abundances using ion chromatography. The results for the short-term study showed little or no evidence that leaching had occurred. However, there were tantalizing hints that something may be happening. The residual solid samples are currently being analyzed for the unleached trace metals using instrumental neutron activation analysis and should show evidence of disturbance if the chromatography clues were real. In addition, another set of samples continues to be intermittently sampled for later analysis. The results should give us information about the movement of trace elements under our conditions and allow us to make some tentative extrapolations to what we observe in actual <span class="hlt">Antarctic</span> eucrite samples.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4685969','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4685969"><span><span class="hlt">Antarctic</span> subglacial lake exploration: first results and future plans</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Siegert, Martin J.; Priscu, John C.; Wadham, Jemma L.; Lyons, W. Berry</p> <p>2016-01-01</p> <p>After more than a decade of planning, three attempts were made in 2012–2013 to access, measure in situ properties and directly sample subglacial <span class="hlt">Antarctic</span> lake environments. First, Russian scientists drilled into the top of Lake Vostok, allowing lake <span class="hlt">water</span> to infiltrate, and freeze within, the lower part of the ice-core borehole, from which further coring would recover a frozen sample of surface lake <span class="hlt">water</span>. Second, UK engineers tried unsuccessfully to deploy a clean-access hot-<span class="hlt">water</span> drill, to sample the <span class="hlt">water</span> column and sediments of subglacial Lake Ellsworth. Third, a US mission successfully drilled cleanly into subglacial Lake Whillans, a shallow hydraulically active lake at the coastal margin of West Antarctica, obtaining samples that would later be used to prove the existence of microbial life and active biogeochemical cycling beneath the ice sheet. This article summarizes the results of these programmes in terms of the scientific results obtained, the operational knowledge gained and the engineering challenges revealed, to collate what is known about <span class="hlt">Antarctic</span> subglacial environments and how to explore them in future. While results from Lake Whillans testify to subglacial lakes as being viable biological habitats, the engineering challenges to explore deeper more isolated lakes where unique microorganisms and climate records may be found, as exemplified in the Lake Ellsworth and Vostok missions, are considerable. Through international cooperation, and by using equipment and knowledge of the existing subglacial lake exploration programmes, it is possible that such environments could be explored thoroughly, and at numerous sites, in the near future. PMID:26667917</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26667917','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26667917"><span><span class="hlt">Antarctic</span> subglacial lake exploration: first results and future plans.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Siegert, Martin J; Priscu, John C; Alekhina, Irina A; Wadham, Jemma L; Lyons, W Berry</p> <p>2016-01-28</p> <p>After more than a decade of planning, three attempts were made in 2012-2013 to access, measure in situ properties and directly sample subglacial <span class="hlt">Antarctic</span> lake environments. First, Russian scientists drilled into the top of Lake Vostok, allowing lake <span class="hlt">water</span> to infiltrate, and freeze within, the lower part of the ice-core borehole, from which further coring would recover a frozen sample of surface lake <span class="hlt">water</span>. Second, UK engineers tried unsuccessfully to deploy a clean-access hot-<span class="hlt">water</span> drill, to sample the <span class="hlt">water</span> column and sediments of subglacial Lake Ellsworth. Third, a US mission successfully drilled cleanly into subglacial Lake Whillans, a shallow hydraulically active lake at the coastal margin of West Antarctica, obtaining samples that would later be used to prove the existence of microbial life and active biogeochemical cycling beneath the ice sheet. This article summarizes the results of these programmes in terms of the scientific results obtained, the operational knowledge gained and the engineering challenges revealed, to collate what is known about <span class="hlt">Antarctic</span> subglacial environments and how to explore them in future. While results from Lake Whillans testify to subglacial lakes as being viable biological habitats, the engineering challenges to explore deeper more isolated lakes where unique microorganisms and climate records may be found, as exemplified in the Lake Ellsworth and Vostok missions, are considerable. Through international cooperation, and by using equipment and knowledge of the existing subglacial lake exploration programmes, it is possible that such environments could be explored thoroughly, and at numerous sites, in the near future. © 2015 The Author(s).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4659931','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4659931"><span><span class="hlt">Antarctic</span> glacio-eustatic contributions to late Miocene Mediterranean desiccation and reflooding</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Ohneiser, Christian; Florindo, Fabio; Stocchi, Paolo; Roberts, Andrew P.; DeConto, Robert M.; Pollard, David</p> <p>2015-01-01</p> <p>The Messinian Salinity Crisis (MSC) was a marked late Neogene oceanographic event during which the Mediterranean Sea evaporated. Its causes remain unresolved, with tectonic restrictions to the Atlantic Ocean or glacio-eustatic restriction of flow during sea-level lowstands, or a mixture of the two mechanisms, being proposed. Here we present the first direct geological evidence of <span class="hlt">Antarctic</span> ice-sheet (AIS) expansion at the MSC onset and use a δ18O record to model relative sea-level changes. <span class="hlt">Antarctic</span> sedimentary successions indicate AIS expansion at 6 Ma coincident with major MSC desiccation; relative sea-level modelling indicates a prolonged ∼50 m lowstand at the Strait of Gibraltar, which resulted from AIS expansion and local evaporation of sea <span class="hlt">water</span> in concert with evaporite precipitation that caused lithospheric deformation. Our results reconcile MSC events and demonstrate that desiccation and refilling were timed by the interplay between glacio-eustatic sea-level variations, glacial isostatic adjustment and mantle deformation in response to changing <span class="hlt">water</span> and evaporite loads. PMID:26556503</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6528716-antarctic-terrestrial-ecosystems','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6528716-antarctic-terrestrial-ecosystems"><span><span class="hlt">Antarctic</span> terrestrial ecosystems</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>Walton, D.W.H.</p> <p>1987-01-01</p> <p>The Maritime and Continental <span class="hlt">Antarctic</span> terrestrial ecosystems are considered in the context of environmental impacts - habitat destruction, alien introductions, and pollution. Four types of pollution are considered: nutrients, radionuclides, inert materials, and noxious chemicals. Their ability to recover from perturbation is discussed in the light of present scientific knowledge, and the methods used to control impacts are reviewed. It is concluded that techniques of waste disposal are still inadequate, adequate training in environmental and conservation principles for <span class="hlt">Antarctic</span> personnel in many countries is lacking, and scientific investigations may be a much more serious threat than tourism to the integritymore » of these ecosystems. Some priorities crucial to future management are suggested.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2012-02-03/pdf/2012-1392.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2012-02-03/pdf/2012-1392.pdf"><span>77 FR 5403 - Conservation of <span class="hlt">Antarctic</span> Animals and Plants</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>2012-02-03</p> <p>... <span class="hlt">Antarctic</span> Specially Protected Areas (ASPA), <span class="hlt">Antarctic</span> Specially Managed Areas (ASMA) and Historical Sites or... managed area (ASMA 7) and five historical sites and monuments in Antarctica (HSM 83-87). Public... <span class="hlt">Antarctic</span> Specially Managed Areas (ASMA). Detailed maps and descriptions of the sites and complete...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP52A..07R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP52A..07R"><span>How are recent changes in Southern Hemisphere Westerly Winds affecting East <span class="hlt">Antarctic</span> terrestrial plants?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Robinson, S. A.; Waterman, M. J.; Bramley-Alves, J.; Clarke, L. J.; Hua, Q.</p> <p>2017-12-01</p> <p>Antarctica has experienced major changes in temperature, wind speed, stratospheric ozone levels and ultraviolet-B radiation over the last century. However, because East Antarctica has shown little climate warming, biological changes were predicted to be relatively slow, compared to the rapid changes observed on the warmer <span class="hlt">Antarctic</span> Peninsula. Detecting the biological effects of <span class="hlt">Antarctic</span> climate change has been hindered by the paucity of long-term data sets, particularly for organisms that have been exposed to these changes throughout their lives. Recent studies using radiocarbon signals preserved along the shoots of individual mosses, as well as peat cores, enables accurate determination of the growth rates of the dominant <span class="hlt">Antarctic</span> moss flora over the last century. This allows us to explore the influence of environmental variables on growth providing a dramatic demonstration of the effects of climate change on <span class="hlt">Antarctic</span> biodiversity. We generated detailed 50-year growth records for four <span class="hlt">Antarctic</span> moss species, Ceratodon purpureus, Bryum pseudotriquetrum, Schistidium antarctici and Bryoerythrophyllum recurvirostre using the 1960s radiocarbon bomb spike. Ceratodon purpureus' growth rates are positively correlated with ozone depth and temperature and negatively correlated with wind speed. Carbon stable isotopic measurements (∂13C) suggest that the observed effects of climate variation on growth are mediated through changes in <span class="hlt">water</span> availability and mostly likely linked to the more positive phase of the Southern Annular Mode (SAM) and changing westerly wind patterns. For cold remote locations like Antarctica, where climate records are limited and of relatively short duration, this illustrates that mosses can act as microclimate proxies and have the potential to increase our knowledge of coastal <span class="hlt">Antarctic</span> climate change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24855668','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24855668"><span>The hydrodynamics of swimming at <span class="hlt">intermediate</span> Reynolds numbers in the <span class="hlt">water</span> boatman (Corixidae).</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ngo, Victoria; McHenry, Matthew James</p> <p>2014-08-01</p> <p>The fluid forces that govern propulsion determine the speed and energetic cost of swimming. These hydrodynamics are scale dependent and it is unclear what forces matter to the tremendous diversity of aquatic animals that are between a millimeter and a centimeter in length. Animals at this scale generally operate within the regime of <span class="hlt">intermediate</span> Reynolds numbers, where both viscous and inertial fluid forces have the potential to play a role in propulsion. The present study aimed to resolve which forces create thrust and drag in the paddling of the <span class="hlt">water</span> boatman (Corixidae), an animal that spans much of the <span class="hlt">intermediate</span> regime (10<Re<200). By measuring the force generated by tethered <span class="hlt">water</span> boatmen, we found that thrust is generated primarily by drag on the paddling appendages, with a negligible contribution from the acceleration reaction force. Based on these findings, we developed a forward-dynamic model of propulsion in free swimming that accurately predicted changes in the body's center of mass over time. For both tethered and free swimming, we used non-linear optimization algorithms to determine the force coefficients that best matched our measurements. With this approach, the drag coefficients on the body and paddle were found to be up to three times greater than on static structures in fully developed flow at the same Reynolds numbers. This is likely a partial consequence of unsteady interactions between the paddles or between the paddles and the body. In addition, the maximum values for these coefficients were inversely related to the Reynolds number, which suggests that viscous forces additionally play an important role in the hydrodynamics of small <span class="hlt">water</span> boatmen. This understanding for the major forces that operate at <span class="hlt">intermediate</span> Reynolds numbers offers a basis for interpreting the mechanics, energetics and functional morphology of swimming in many small aquatic animals. © 2014. Published by The Company of Biologists Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/518387-solar-uvb-induced-dna-damage-photoenzymatic-dna-repair-antarctic-zooplankton','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/518387-solar-uvb-induced-dna-damage-photoenzymatic-dna-repair-antarctic-zooplankton"><span>Solar UVB-induced DNA damage and photoenzymatic DNA repair in <span class="hlt">antarctic</span> zooplankton</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>Malloy, K.D.; Holman, M.A.; Mitchell, D.</p> <p></p> <p>The detrimental effects of elevated intensities of mid-UV radiation (UVB), a result of stratospheric ozone depletion during the austral spring, on the primary producers of the <span class="hlt">Antarctic</span> marine ecosystem have been well documented. Here we report that natural populations of <span class="hlt">Antarctic</span> zooplankton also sustain significant DNA damage [measured as cyclobutane pyrimidine dimers (CPDs)] during periods of increased UVB flux. This is the first direct evidence that increased solar UVB may result in damage to marine organisms other than primary producers in Antarctica. The extent of DNA damage in pelagic icefish eggs correlated with daily incident UVB irradiance, reflecting the differencemore » between acquisition and repair of CPDs. Patterns of DNA damage in fish larvae did not correlated with daily UVB flux, possibly due to different depth distributions and/or different capacities for DNA repair. Clearance of CPDs by <span class="hlt">Antarctic</span> fish and krill was mediated primarily by the photoenzymatic repair system. Although repair rates were large for all species evaluated, they were apparently inadequate to prevent the transient accumulation of substantial CPD burdens. The capacity for DNA repair in <span class="hlt">Antarctic</span> organisms was highest in those species whose early life history stages occupy the <span class="hlt">water</span> column during periods of ozone depletion (austral spring) and lowest in fish species whose eggs and larvae are abundant during winter. Although the potential reduction in fitness of <span class="hlt">Antarctic</span> zooplankton resulting from DNA damage is unknown, we suggest that increased solar UV may reduce recruitment and adversely affect trophic transfer of productivity by affecting heterotrophic species as well as primary producers. 54 refs., 4 figs., 2 tabs.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29760113','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29760113"><span>Impact of sea-ice melt on dimethyl sulfide (sulfoniopropionate) inventories in surface <span class="hlt">waters</span> of Marguerite Bay, West <span class="hlt">Antarctic</span> Peninsula.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Stefels, Jacqueline; van Leeuwe, Maria A; Jones, Elizabeth M; Meredith, Michael P; Venables, Hugh J; Webb, Alison L; Henley, Sian F</p> <p>2018-06-28</p> <p>The Southern Ocean is a hotspot of the climate-relevant organic sulfur compound dimethyl sulfide (DMS). Spatial and temporal variability in DMS concentration is higher than in any other oceanic region, especially in the marginal ice zone. During a one-week expedition across the continental shelf of the West <span class="hlt">Antarctic</span> Peninsula (WAP), from the shelf break into Marguerite Bay, in January 2015, spatial heterogeneity of DMS and its precursor dimethyl sulfoniopropionate (DMSP) was studied and linked with environmental conditions, including sea-ice melt events. Concentrations of sulfur compounds, particulate organic carbon (POC) and chlorophyll a in the surface <span class="hlt">waters</span> varied by a factor of 5-6 over the entire transect. DMS and DMSP concentrations were an order of magnitude higher than currently inferred in climatologies for the WAP region. Particulate DMSP concentrations were correlated most strongly with POC and the abundance of haptophyte algae within the phytoplankton community, which, in turn, was linked with sea-ice melt. The strong sea-ice signal in the distribution of DMS(P) implies that DMS(P) production is likely to decrease with ongoing reductions in sea-ice cover along the WAP. This has implications for feedback processes on the region's climate system.This article is part of the theme issue 'The marine system of the West <span class="hlt">Antarctic</span> Peninsula: status and strategy for progress in a region of rapid change'. © 2018 The Author(s).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018TCry...12..521G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018TCry...12..521G"><span>Increased West <span class="hlt">Antarctic</span> and unchanged East <span class="hlt">Antarctic</span> ice discharge over the last 7 years</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gardner, Alex S.; Moholdt, Geir; Scambos, Ted; Fahnstock, Mark; Ligtenberg, Stefan; van den Broeke, Michiel; Nilsson, Johan</p> <p>2018-02-01</p> <p>Ice discharge from large ice sheets plays a direct role in determining rates of sea-level rise. We map present-day <span class="hlt">Antarctic</span>-wide surface velocities using Landsat 7 and 8 imagery spanning 2013-2015 and compare to earlier estimates derived from synthetic aperture radar, revealing heterogeneous changes in ice flow since ˜ 2008. The new mapping provides complete coastal and inland coverage of ice velocity north of 82.4° S with a mean error of < 10 m yr-1, resulting from multiple overlapping image pairs acquired during the daylight period. Using an optimized flux gate, ice discharge from Antarctica is 1929 ± 40 Gigatons per year (Gt yr-1) in 2015, an increase of 36 ± 15 Gt yr-1 from the time of the radar mapping. Flow accelerations across the grounding lines of West Antarctica's Amundsen Sea Embayment, Getz Ice Shelf and Marguerite Bay on the western <span class="hlt">Antarctic</span> Peninsula, account for 88 % of this increase. In contrast, glaciers draining the East <span class="hlt">Antarctic</span> Ice Sheet have been remarkably constant over the period of observation. Including modeled rates of snow accumulation and basal melt, the <span class="hlt">Antarctic</span> ice sheet lost ice at an average rate of 183 ± 94 Gt yr-1 between 2008 and 2015. The modest increase in ice discharge over the past 7 years is contrasted by high rates of ice sheet mass loss and distinct spatial patters of elevation lowering. The West <span class="hlt">Antarctic</span> Ice Sheet is experiencing high rates of mass loss and displays distinct patterns of elevation lowering that point to a dynamic imbalance. We find modest increase in ice discharge over the past 7 years, which suggests that the recent pattern of mass loss in Antarctica is part of a longer-term phase of enhanced glacier flow initiated in the decades leading up to the first continent-wide radar mapping of ice flow.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19850017722&hterms=worlds+oceans&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dworlds%2Boceans','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19850017722&hterms=worlds+oceans&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dworlds%2Boceans"><span>North Atlantic Deep <span class="hlt">Water</span> and the World Ocean</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gordon, A. L.</p> <p>1984-01-01</p> <p>North Atlantic Deep <span class="hlt">Water</span> (NADW) by being warmer and more saline than the average abyssal <span class="hlt">water</span> parcel introduces heat and salt into the abyssal ocean. The source of these properties is upper layer or thermocline <span class="hlt">water</span> 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 <span class="hlt">water</span>) is usually considered to to take place in the Southern Ocean where upwelling deep <span class="hlt">water</span> is converted to cold fresher <span class="hlt">Antarctic</span> <span class="hlt">water</span> masses. The Southern ocean convective process is driven by low temperatures and hence may be considered as thermal convection. A significant fresh <span class="hlt">water</span> source may also occur in the North Pacific where the northward flowing of abyssal <span class="hlt">water</span> from the Southern circumpolar belt is saltier and denser than the southward flowing, return abyssal <span class="hlt">water</span>. The source of the low salinity input may be vertical mixing of the low salinity surface <span class="hlt">water</span> or the low salinity <span class="hlt">intermediate</span> <span class="hlt">water</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28752953','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28752953"><span>Evidence of microbial rhodopsins in <span class="hlt">Antarctic</span> Dry Valley edaphic systems.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Guerrero, Leandro D; Vikram, Surendra; Makhalanyane, Thulani P; Cowan, Don A</p> <p>2017-09-01</p> <p>Microorganisms able to synthesize rhodopsins have the capacity to translocate ions through their membranes, using solar energy to generate a proton motive force. Rhodopsins are the most abundant phototrophic proteins in oceanic surface <span class="hlt">waters</span> and are key constituents in marine bacterial ecology. However, it remains unclear how rhodopsins are used in most microorganisms. Despite their abundance in marine and fresh-<span class="hlt">water</span> systems, the presence of functional rhodopsin systems in edaphic habitats has never been reported. Here, we show the presence of several new putative H + , Na + and Cl + pumping rhodopsins identified by metagenomic analysis of <span class="hlt">Antarctic</span> desert hypolithic communities. Reconstruction of two Proteobacteria genomes harboring xanthorhodopsin-like proteins and one Bacteroidetes genome with a Na-pumping-like rhodopsin indicated that these bacteria were aerobic heterotrophs possessing the apparent capacity for the functional expression of rhodopsins. The existence of these protein systems in hypolithic bacteria expands the known role of rhodopsins to include terrestrial environments and suggests a possible predominant function as heterotrophic energy supply proteins, a feasible microbial adaptation to the harsh conditions prevalent in <span class="hlt">Antarctic</span> edaphic systems. © 2017 Society for Applied Microbiology and John Wiley & Sons Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20040027569','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20040027569"><span>Modeling and Observational Study of the Global Atmospheric Impacts of <span class="hlt">Antarctic</span> Sea Ice Anomalies</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bromwich, David H.; Hines, Keith M.</p> <p>2004-01-01</p> <p>A combined observational and modeling study considers the linkage between <span class="hlt">Antarctic</span> sea ice and the climate of non-local latitudes. The observational component is based upon analyses of monthly station observations and the National Centers for Environmental Prediction (NCEP)/National Center for Atmospheric Research (NCAR) Reanalysis (NNR). The modeling component consists of simulations of the NCAR Community Climate Model versions 2 (CCM2) and 3 (CCM3) and the recent Community Atmosphere Model (CAM2). A convenient mechanism for communication between the <span class="hlt">Antarctic</span> region (particularly the Ross Sea area) and the tropics and Northern Hemisphere is examined. The first evidence of this teleconnection came from CCM2 simulations performed during an earlier NASA supported project. Annual-cycle simulations with and without <span class="hlt">Antarctic</span> sea ice show statistically- significant responses in monsoon precipitation over central and northern China during the month of September. The changes in monsoon precipitation are physically consistent with an intensified southwest Pacific (Northern Hemisphere) subtropical high in response to all <span class="hlt">Antarctic</span> sea ice being removed and replaced with open <span class="hlt">water</span> at -1.9"C. The intensified high is the northernmost component of three primary anomalies. The southernmost anomaly includes the Ross Sea area, where sea ice has been removed. An earlier study by Peng and Domros had also found a link between <span class="hlt">Antarctic</span> sea ice and the East Asian monsoon circulation. The current project has helped to understand the teleconnection.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28246631','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28246631"><span>State dependence of climatic instability over the past 720,000 years from <span class="hlt">Antarctic</span> ice cores and climate modeling.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kawamura, Kenji; Abe-Ouchi, Ayako; Motoyama, Hideaki; Ageta, Yutaka; Aoki, Shuji; Azuma, Nobuhiko; Fujii, Yoshiyuki; Fujita, Koji; Fujita, Shuji; Fukui, Kotaro; Furukawa, Teruo; Furusaki, Atsushi; Goto-Azuma, Kumiko; Greve, Ralf; Hirabayashi, Motohiro; Hondoh, Takeo; Hori, Akira; Horikawa, Shinichiro; Horiuchi, Kazuho; Igarashi, Makoto; Iizuka, Yoshinori; Kameda, Takao; Kanda, Hiroshi; Kohno, Mika; Kuramoto, Takayuki; Matsushi, Yuki; Miyahara, Morihiro; Miyake, Takayuki; Miyamoto, Atsushi; Nagashima, Yasuo; Nakayama, Yoshiki; Nakazawa, Takakiyo; Nakazawa, Fumio; Nishio, Fumihiko; Obinata, Ichio; Ohgaito, Rumi; Oka, Akira; Okuno, Jun'ichi; Okuyama, Junichi; Oyabu, Ikumi; Parrenin, Frédéric; Pattyn, Frank; Saito, Fuyuki; Saito, Takashi; Saito, Takeshi; Sakurai, Toshimitsu; Sasa, Kimikazu; Seddik, Hakime; Shibata, Yasuyuki; Shinbori, Kunio; Suzuki, Keisuke; Suzuki, Toshitaka; Takahashi, Akiyoshi; Takahashi, Kunio; Takahashi, Shuhei; Takata, Morimasa; Tanaka, Yoichi; Uemura, Ryu; Watanabe, Genta; Watanabe, Okitsugu; Yamasaki, Tetsuhide; Yokoyama, Kotaro; Yoshimori, Masakazu; Yoshimoto, Takayasu</p> <p>2017-02-01</p> <p>Climatic variabilities on millennial and longer time scales with a bipolar seesaw pattern have been documented in paleoclimatic records, but their frequencies, relationships with mean climatic state, and mechanisms remain unclear. Understanding the processes and sensitivities that underlie these changes will underpin better understanding of the climate system and projections of its future change. We investigate the long-term characteristics of climatic variability using a new ice-core record from Dome Fuji, East Antarctica, combined with an existing long record from the Dome C ice core. <span class="hlt">Antarctic</span> warming events over the past 720,000 years are most frequent when the <span class="hlt">Antarctic</span> temperature is slightly below average on orbital time scales, equivalent to an <span class="hlt">intermediate</span> climate during glacial periods, whereas interglacial and fully glaciated climates are unfavourable for a millennial-scale bipolar seesaw. Numerical experiments using a fully coupled atmosphere-ocean general circulation model with freshwater hosing in the northern North Atlantic showed that climate becomes most unstable in <span class="hlt">intermediate</span> glacial conditions associated with large changes in sea ice and the Atlantic Meridional Overturning Circulation. Model sensitivity experiments suggest that the prerequisite for the most frequent climate instability with bipolar seesaw pattern during the late Pleistocene era is associated with reduced atmospheric CO 2 concentration via global cooling and sea ice formation in the North Atlantic, in addition to extended Northern Hemisphere ice sheets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5298857','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5298857"><span>State dependence of climatic instability over the past 720,000 years from <span class="hlt">Antarctic</span> ice cores and climate modeling</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Kawamura, Kenji; Abe-Ouchi, Ayako; Motoyama, Hideaki; Ageta, Yutaka; Aoki, Shuji; Azuma, Nobuhiko; Fujii, Yoshiyuki; Fujita, Koji; Fujita, Shuji; Fukui, Kotaro; Furukawa, Teruo; Furusaki, Atsushi; Goto-Azuma, Kumiko; Greve, Ralf; Hirabayashi, Motohiro; Hondoh, Takeo; Hori, Akira; Horikawa, Shinichiro; Horiuchi, Kazuho; Igarashi, Makoto; Iizuka, Yoshinori; Kameda, Takao; Kanda, Hiroshi; Kohno, Mika; Kuramoto, Takayuki; Matsushi, Yuki; Miyahara, Morihiro; Miyake, Takayuki; Miyamoto, Atsushi; Nagashima, Yasuo; Nakayama, Yoshiki; Nakazawa, Takakiyo; Nakazawa, Fumio; Nishio, Fumihiko; Obinata, Ichio; Ohgaito, Rumi; Oka, Akira; Okuno, Jun’ichi; Okuyama, Junichi; Oyabu, Ikumi; Parrenin, Frédéric; Pattyn, Frank; Saito, Fuyuki; Saito, Takashi; Saito, Takeshi; Sakurai, Toshimitsu; Sasa, Kimikazu; Seddik, Hakime; Shibata, Yasuyuki; Shinbori, Kunio; Suzuki, Keisuke; Suzuki, Toshitaka; Takahashi, Akiyoshi; Takahashi, Kunio; Takahashi, Shuhei; Takata, Morimasa; Tanaka, Yoichi; Uemura, Ryu; Watanabe, Genta; Watanabe, Okitsugu; Yamasaki, Tetsuhide; Yokoyama, Kotaro; Yoshimori, Masakazu; Yoshimoto, Takayasu</p> <p>2017-01-01</p> <p>Climatic variabilities on millennial and longer time scales with a bipolar seesaw pattern have been documented in paleoclimatic records, but their frequencies, relationships with mean climatic state, and mechanisms remain unclear. Understanding the processes and sensitivities that underlie these changes will underpin better understanding of the climate system and projections of its future change. We investigate the long-term characteristics of climatic variability using a new ice-core record from Dome Fuji, East Antarctica, combined with an existing long record from the Dome C ice core. <span class="hlt">Antarctic</span> warming events over the past 720,000 years are most frequent when the <span class="hlt">Antarctic</span> temperature is slightly below average on orbital time scales, equivalent to an <span class="hlt">intermediate</span> climate during glacial periods, whereas interglacial and fully glaciated climates are unfavourable for a millennial-scale bipolar seesaw. Numerical experiments using a fully coupled atmosphere-ocean general circulation model with freshwater hosing in the northern North Atlantic showed that climate becomes most unstable in <span class="hlt">intermediate</span> glacial conditions associated with large changes in sea ice and the Atlantic Meridional Overturning Circulation. Model sensitivity experiments suggest that the prerequisite for the most frequent climate instability with bipolar seesaw pattern during the late Pleistocene era is associated with reduced atmospheric CO2 concentration via global cooling and sea ice formation in the North Atlantic, in addition to extended Northern Hemisphere ice sheets. PMID:28246631</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5461483','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5461483"><span>Evidence for a palaeo-subglacial lake on the <span class="hlt">Antarctic</span> continental shelf</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Kuhn, Gerhard; Hillenbrand, Claus-Dieter; Kasten, Sabine; Smith, James A.; Nitsche, Frank O.; Frederichs, Thomas; Wiers, Steffen; Ehrmann, Werner; Klages, Johann P.; Mogollón, José M.</p> <p>2017-01-01</p> <p>Subglacial lakes are widespread beneath the <span class="hlt">Antarctic</span> Ice Sheet but their control on ice-sheet dynamics and their ability to harbour life remain poorly characterized. Here we present evidence for a palaeo-subglacial lake on the <span class="hlt">Antarctic</span> continental shelf. A distinct sediment facies recovered from a bedrock basin in Pine Island Bay indicates deposition within a low-energy lake environment. Diffusive-advection modelling demonstrates that low chloride concentrations in the pore <span class="hlt">water</span> of the corresponding sediments can only be explained by initial deposition of this facies in a freshwater setting. These observations indicate that an active subglacial meltwater network, similar to that observed beneath the extant ice sheet, was also active during the last glacial period. It also provides a new framework for refining the exploration of these unique environments. PMID:28569750</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_13 --> <div id="page_14" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="261"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2011-title45-vol3/pdf/CFR-2011-title45-vol3-sec670-9.pdf','CFR2011'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2011-title45-vol3/pdf/CFR-2011-title45-vol3-sec670-9.pdf"><span>45 CFR 670.9 - <span class="hlt">Antarctic</span> Conservation Act enforcement exception.</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>... FOUNDATION CONSERVATION OF <span class="hlt">ANTARCTIC</span> ANIMALS AND PLANTS Prohibited Acts, Exceptions § 670.9 <span class="hlt">Antarctic</span> Conservation Act enforcement exception. Paragraphs (a) through (d) of § 670.4 shall not apply to acts carried... 45 Public Welfare 3 2011-10-01 2011-10-01 false <span class="hlt">Antarctic</span> Conservation Act enforcement exception...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2014-title45-vol3/pdf/CFR-2014-title45-vol3-sec670-9.pdf','CFR2014'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2014-title45-vol3/pdf/CFR-2014-title45-vol3-sec670-9.pdf"><span>45 CFR 670.9 - <span class="hlt">Antarctic</span> Conservation Act enforcement exception.</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>... FOUNDATION CONSERVATION OF <span class="hlt">ANTARCTIC</span> ANIMALS AND PLANTS Prohibited Acts, Exceptions § 670.9 <span class="hlt">Antarctic</span> Conservation Act enforcement exception. Paragraphs (a) through (d) of § 670.4 shall not apply to acts carried... 45 Public Welfare 3 2014-10-01 2014-10-01 false <span class="hlt">Antarctic</span> Conservation Act enforcement exception...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2010-title45-vol3/pdf/CFR-2010-title45-vol3-sec670-9.pdf','CFR'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2010-title45-vol3/pdf/CFR-2010-title45-vol3-sec670-9.pdf"><span>45 CFR 670.9 - <span class="hlt">Antarctic</span> Conservation Act enforcement exception.</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>... FOUNDATION CONSERVATION OF <span class="hlt">ANTARCTIC</span> ANIMALS AND PLANTS Prohibited Acts, Exceptions § 670.9 <span class="hlt">Antarctic</span> Conservation Act enforcement exception. Paragraphs (a) through (d) of § 670.4 shall not apply to acts carried... 45 Public Welfare 3 2010-10-01 2010-10-01 false <span class="hlt">Antarctic</span> Conservation Act enforcement exception...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2012-title45-vol3/pdf/CFR-2012-title45-vol3-sec670-9.pdf','CFR2012'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2012-title45-vol3/pdf/CFR-2012-title45-vol3-sec670-9.pdf"><span>45 CFR 670.9 - <span class="hlt">Antarctic</span> Conservation Act enforcement exception.</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>... FOUNDATION CONSERVATION OF <span class="hlt">ANTARCTIC</span> ANIMALS AND PLANTS Prohibited Acts, Exceptions § 670.9 <span class="hlt">Antarctic</span> Conservation Act enforcement exception. Paragraphs (a) through (d) of § 670.4 shall not apply to acts carried... 45 Public Welfare 3 2012-10-01 2012-10-01 false <span class="hlt">Antarctic</span> Conservation Act enforcement exception...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2013-title45-vol3/pdf/CFR-2013-title45-vol3-sec670-9.pdf','CFR2013'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2013-title45-vol3/pdf/CFR-2013-title45-vol3-sec670-9.pdf"><span>45 CFR 670.9 - <span class="hlt">Antarctic</span> Conservation Act enforcement exception.</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>... FOUNDATION CONSERVATION OF <span class="hlt">ANTARCTIC</span> ANIMALS AND PLANTS Prohibited Acts, Exceptions § 670.9 <span class="hlt">Antarctic</span> Conservation Act enforcement exception. Paragraphs (a) through (d) of § 670.4 shall not apply to acts carried... 45 Public Welfare 3 2013-10-01 2013-10-01 false <span class="hlt">Antarctic</span> Conservation Act enforcement exception...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014ATsir1618....1Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014ATsir1618....1Y"><span>Study Of Functioning of Bacterial Complexes in East <span class="hlt">Antarctic</span> Soils</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yakushev, A. V.; Churilin, N. A.</p> <p>2014-11-01</p> <p>Studies of bacterial communities in the samples of <span class="hlt">Antarctic</span> soils by different methods showed that, both in liquid soil suspensions and in situ, microbial complexes are functioning presumably by forming biofilms - the phenomenon that is more expressed in such habitat than in soils of temperate zones. Functional (trophic) diversity and physiological state of hydrolytic bacteria was studied in the samples at the upper layer (0-2 cm) of gravel pavement with algae, in the underlying peat horizon (2-4 cm) with inclusions of dead biomass and its underlying mineral horizon (4-10 cm) with signs of fungal mycelium. The investigated samples of <span class="hlt">Antarctic</span> soils revealed different trophic diversity and the maximum specific growth rate on mineral medium with different biopolymers as the sole carbon source (starch, chitin, pectin, xylan, dextran-500, tween-20, casein); this can testify to differences in the physiological state of hydrolytic bacteria in various soil horizons and their readiness for growth. The most remarkable characteristics of the studied <span class="hlt">Antarctic</span> soil as compared to the soils of temperate zone, was the unusual ability of hydrolytic community to consume chitin in the mineral horizon; this can be explained by the presence of fungal mycelium. Also, an almost complete lack in consumption of tween-20 (a <span class="hlt">water</span>-soluble analogue of fat) by bacterial community of Arctic soil horizons are not explained and needs further verification. The higher functional diversity was detected in the upper horizon of the gravel pavement, which "protects" microorganisms from exposure to extreme temperatures, UV radiation, and desiccation, but the maximum specific growth rate was higher in the lower mineral horizon; this can be explained by the specificity of bacterial colonizing processes and unique formation of <span class="hlt">Antarctic</span> soil microprofiles in the Larsemann oasis. The obtained data indicate a specific environmental strategy in the samples of <span class="hlt">Antarctic</span> soils: development in lower mineral</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFMPP11A1364S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFMPP11A1364S"><span>Ventilation History of the Tropical Atlantic Thermocline: New Insights From the Sensitivity of Foraminifera to <span class="hlt">Water</span> Mass Nutrient Concentrations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sexton, P. F.; Norris, R. D.</p> <p>2008-12-01</p> <p>The sensitivity of certain species of foraminifera to nutrient distributions throughout today's oceans highlights their potential for reconstructing <span class="hlt">water</span> mass nutrient distributions in the past. Applying these new insights to reconstructed abundances of several key species during the last glacial, we find that thermocline <span class="hlt">waters</span> throughout the entire tropical Atlantic were better ventilated than today. These findings are in line with independent evidence for stronger <span class="hlt">intermediate</span>-depth ventilation driven by widespread Glacial North Atlantic <span class="hlt">Intermediate</span> <span class="hlt">Water</span> (GNAIW), supporting the validity of our new approach. Our results also suggest that well- ventilated GNAIW penetrated at least as far as 25 degrees South, thereby confining the northernmost glacial limits of poorly ventilated <span class="hlt">Antarctic</span> <span class="hlt">Intermediate</span> <span class="hlt">Water</span> (AAIW) to the southernmost Atlantic. We show that the glacial Atlantic thermocline switched to its modern, more poorly ventilated state (probably indicative of a return of AAIW dominance) in a two-step process: a transient reduction in ventilation during the Bolling/Allerod, with the definitive switch to a regime of poor thermocline ventilation occurring at the close of the Younger Dryas. Furthermore, longer-term reconstructions of past distributions of these several key foraminiferal species suggest that a major and enduring impact of glacial-interglacial cycles on Atlantic hydrography has been this vacillating behaviour in tropical thermocline ventilation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMSA31B4100T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMSA31B4100T"><span>The ANGWIN <span class="hlt">Antarctic</span> Research Program: First Results on Coordinated Trans-<span class="hlt">Antarctic</span> Gravity Wave Measurements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Taylor, M. J.; Pautet, P. D.; Zhao, Y.; Nakamura, T.; Ejiri, M. K.; Murphy, D. J.; Moffat-Griffin, T.; Kavanagh, A. J.; Takahashi, H.; Wrasse, C. M.</p> <p>2014-12-01</p> <p>ANGWIN (ANrctic Gravity Wave Instrument Network) is a new "scientist driven" research program designed to develop and utilize a network of <span class="hlt">Antarctic</span> atmospheric gravity wave observatories, operated by different nations working together in a spirit of close scientific collaboration. Our research plan has brought together colleagues from several international institutions, all with a common goal to better understand the large "continental-scale" characteristics and impacts of gravity waves on the Mesosphere and Lower Thermosphere (MLT) environment over Antarctica. ANGWIN combines complementary measurements obtained using new and existing aeronomy instrumentation with new modeling capabilities. To date, our activities have focused on developing coordinated airglow image data of gravity waves in the MLT region at the following sites: McMurdo (US), Syowa (Japan), Davis (Australia), Halley (UK), Rothera (UK), and Comandante Ferraz (Brazil). These are all well-established international research stations that are uniformly distributed around the continental perimeter, and together with ongoing measurements at South Pole Station they provide unprecedented coverage of the <span class="hlt">Antarctic</span> gravity wave field and its variability during the extended polar winter season. This presentation introduces the ANGWIN program and research goals, and presents first results on trans-<span class="hlt">Antarctic</span> wave propagation using coordinated measurements during the winter season 2011. We also discuss future plans for the development of this exciting program for <span class="hlt">Antarctic</span> research.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19910063773&hterms=1087&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3D%2526%25231087','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19910063773&hterms=1087&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3D%2526%25231087"><span><span class="hlt">Antarctic</span> Sea ice variations and seasonal air temperature relationships</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Weatherly, John W.; Walsh, John E.; Zwally, H. J.</p> <p>1991-01-01</p> <p>Data through 1987 are used to determine the regional and seasonal dependencies of recent trends of <span class="hlt">Antarctic</span> temperature and sea ice. Lead-lag relationships involving regional sea ice and air temperature are systematically evaluated, with an eye toward the ice-temperature feedbacks that may influence climatic change. Over the 1958-1087 period the temperature trends are positive in all seasons. For the 15 years (l973-l987) for which ice data are available, the trends are predominantly positive only in winter and summer, and are most strongly positive over the <span class="hlt">Antarctic</span> Peninsula. The spatially aggregated trend of temperature for this latter period is small but positive, while the corresponding trend of ice coverage is small but negative. Lag correlations between seasonal anomalies of the two variables are generally stronger with ice lagging the summer temperatures and with ice leading the winter temperatures. The implication is that summer temperatures predispose the near-surface <span class="hlt">waters</span> to above-or below-normal ice coverage in the following fall and winter.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoRL..45.2380S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoRL..45.2380S"><span>Change in Dense Shelf <span class="hlt">Water</span> and Adélie Land Bottom <span class="hlt">Water</span> Precipitated by Iceberg Calving</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Snow, K.; Rintoul, S. R.; Sloyan, B. M.; Hogg, A. McC.</p> <p>2018-03-01</p> <p><span class="hlt">Antarctic</span> Bottom <span class="hlt">Water</span> supplies the deep limb of the global overturning circulation and ventilates the abyssal ocean. <span class="hlt">Antarctic</span> Bottom <span class="hlt">Water</span> has warmed, freshened, and contracted in recent decades, but the causes remain poorly understood. We use unique multiyear observations from the continental shelf and deep ocean near the Mertz Polynya to examine the sensitivity of this bottom <span class="hlt">water</span> formation region to changes on the continental shelf, including the calving of a large iceberg. Postcalving, the seasonal cycle of Dense Shelf <span class="hlt">Water</span> (DSW) density almost halved in amplitude and the volume of DSW available for export reduced. In the deep ocean, the density and volume of Adélie Land Bottom <span class="hlt">Water</span> decreased sharply after calving, while oxygen concentrations remained high, indicating continued ventilation by DSW. This natural experiment illustrates how local changes in forcing over the <span class="hlt">Antarctic</span> continental shelf can drive large and rapid changes in the abyssal ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29682746','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29682746"><span>In situ warming in the <span class="hlt">Antarctic</span>: effects on growth and photosynthesis in <span class="hlt">Antarctic</span> vascular plants.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sáez, Patricia L; Cavieres, Lohengrin A; Galmés, Jeroni; Gil-Pelegrín, Eustaquio; Peguero-Pina, José Javier; Sancho-Knapik, Domingo; Vivas, Mercedes; Sanhueza, Carolina; Ramírez, Constanza F; Rivera, Betsy K; Corcuera, Luis J; Bravo, León A</p> <p>2018-06-01</p> <p>The <span class="hlt">Antarctic</span> Peninsula has experienced a rapid warming in the last decades. Although recent climatic evidence supports a new tendency towards stabilization of temperatures, the impacts on the biosphere, and specifically on <span class="hlt">Antarctic</span> plant species, remain unclear. We evaluated the in situ warming effects on photosynthesis, including the underlying diffusive, biochemical and anatomical determinants, and the relative growth of two <span class="hlt">Antarctic</span> vascular species, Colobanthus quitensis and Deschampsia antarctica, using open top chambers (OTCs) and gas exchange measurements in the field. In C. quitensis, the photosynthetic response to warming relied on specific adjustments in the anatomical determinants of the leaf CO 2 transfer, which enhanced mesophyll conductance and photosynthetic assimilation, thereby promoting higher leaf carbon gain and plant growth. These changes were accompanied by alterations in the leaf chemical composition. By contrast, D. antarctica showed no response to warming, with a lack of significant differences between plants grown inside OTCs and plants grown in the open field. Overall, the present results are the first reporting a contrasting effect of in situ warming on photosynthesis and its underlying determinants, of the two unique <span class="hlt">Antarctic</span> vascular plant species, which could have direct consequences on their ecological success under future climate conditions. © 2018 The Authors. New Phytologist © 2018 New Phytologist Trust.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013Ocgy...53..432T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013Ocgy...53..432T"><span>Transport of <span class="hlt">Antarctic</span> Bottom <span class="hlt">Water</span> through passages in the East Azores Ridge (37° N) in the East Atlantic</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tarakanov, R. Yu.; Morozov, E. G.; Gritsenko, A. M.; Demidova, T. A.; Makarenko, N. I.</p> <p>2013-07-01</p> <p>The structure of northerly overflow of <span class="hlt">Antarctic</span> Bottom <span class="hlt">Water</span> (AABW) through passages in the East Azores Ridge (37° N) in the East Atlantic from the Madeira Basin to the Iberian Basin is studied on the basis of hydrographic measurements carried out by the Institute of Oceanology, Russian Academy of Sciences (RAS) in October 2011, historical World Ocean Data Base 2009, and recent data on the bottom topography. The overflow of the coldest layers of this <span class="hlt">water</span> occurs through two passages with close depths at 16° W (Discovery Gap) and at 19°30' W (nameless Western Gap). It is shown that it is likely that the role of the latter passage in <span class="hlt">water</span> transport was underestimated in earlier publications because the <span class="hlt">water</span> (2.01°C) found in the region north of the Western Gap was cooler than in the region north of the Discovery Gap (2.03°C). In 2011, we found a decrease of 0.01°C in the AABW temperature near the bottom compared to previous measurements in 1982 (from 2.011°C to 2.002°C). Analysis of the historical database shows that this decrease is most likely caused by the cooling trend in the abyssal <span class="hlt">waters</span> in the East Atlantic basins.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006DSRII..53.1071P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006DSRII..53.1071P"><span>Climate-dependent evolution of <span class="hlt">Antarctic</span> ectotherms: An integrative analysis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pörtner, Hans O.</p> <p>2006-04-01</p> <p>, and the use of lipid body stores for neutral buoyancy. Important trade-offs result from obligatory energy savings in the permanent cold: low metabolic rates support cold-compensated growth but imply narrow windows of thermal tolerance and reduced scopes for activity. The degree of thermal specialization is not uniformly defined by cold temperature but varies with life style characteristics and activity levels and associated aerobic scope. Trade-offs for the sake of cold compensated growth parallel reduced capacities for exercise performance, exacerbated by the effect of high haemolymph magnesium levels in crustaceans and, possibly, other invertebrates. High magnesium levels likely exclude the group of reptant decapod crustaceans from <span class="hlt">Antarctic</span> <span class="hlt">waters</span> below 0 °C. The hypothesis is developed that energy savings imposed by the permanent cold bear specific life history consequences. Due to effects of allometry, energy savings are exacerbated at small body size, favouring passive lecithotrophic larvae. At all stages of life history, reduced energy turnover for the sake of growth causes delays and low rates in other higher functions, with the result of late maturity, fecundity and offspring release, as well as extended development. As a consequence, extended life spans evolved due to life history requirements. At the same time, polar gigantism is enabled by a combination of elevated oxygen levels in cold <span class="hlt">waters</span>, of reduced metabolism and of extended periods of growth at slow developmental rates.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016GSL.....3...13O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GSL.....3...13O"><span>Global view of sea-ice production in polynyas and its linkage to dense/bottom <span class="hlt">water</span> formation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ohshima, Kay I.; Nihashi, Sohey; Iwamoto, Katsushi</p> <p>2016-12-01</p> <p>Global overturning circulation is driven by density differences. Saline <span class="hlt">water</span> rejected during sea-ice formation in polynyas is the main source of dense <span class="hlt">water</span>, and thus sea-ice production is a key factor in the overturning circulation. Due to difficulties associated with in situ observation, sea-ice production and its interannual variability have not been well understood until recently. Methods to estimate sea-ice production on large scales have been developed using heat flux calculations based on satellite microwave radiometer data. Using these methods, we present the mapping of sea-ice production with the same definition and scale globally, and review the polynya ice production and its relationship with dense/bottom <span class="hlt">water</span>. The mapping demonstrates that ice production rate is high in <span class="hlt">Antarctic</span> coastal polynyas, in contrast to Arctic coastal polynyas. This is consistent with the formation of <span class="hlt">Antarctic</span> Bottom <span class="hlt">Water</span> (AABW), the densest <span class="hlt">water</span> mass which occupies the abyssal layer of the global ocean. The Ross Ice Shelf polynya has by far the highest ice production in the Southern Hemisphere. The Cape Darnley polynya (65°E-69°E) is found to be the second highest production area and recent observations revealed that this is the missing (fourth) source of AABW. In the region off the Mertz Glacier Tongue (MGT), the third source of AABW, sea-ice production decreased by as much as 40 %, due to the MGT calving in early 2010, resulting in a significant decrease in AABW production. The Okhotsk Northwestern polynya exhibits the highest ice production in the Northern Hemisphere, and the resultant dense <span class="hlt">water</span> formation leads to overturning in the North Pacific, extending to the <span class="hlt">intermediate</span> layer. Estimates of its ice production show a significant decrease over the past 30-50 years, likely causing the weakening of the North Pacific overturning. These regions demonstrate the strong linkage between variabilities of sea-ice production and bottom/<span class="hlt">intermediate</span> <span class="hlt">water</span> formation. The</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 ocean 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 oceanic <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 oceans 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 <span class="hlt">Antarctic</span> Bottom <span class="hlt">Water</span>. In the northern Indian Ocean 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 ocean. As consequence, temperature and salinity in these outflow regions both decrease from the sea surface to the bottom. On the other hand, ocean currents are in general sluggish in these regions. In the polar and subpolar regions of Arctic and <span class="hlt">Antarctic</span>, 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 ocean's interior is unique to the South Atlantic between <span class="hlt">Antarctic</span> <span class="hlt">Intermediate</span> <span class="hlt">Water</span> and upper NADW (uNADW). It is the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007DSRI...54.1329R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007DSRI...54.1329R"><span>Red Sea <span class="hlt">Intermediate</span> <span class="hlt">Water</span> at the Agulhas Current termination</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Roman, R. E.; Lutjeharms, J. R. E.</p> <p>2007-08-01</p> <p>The inter-ocean exchange of <span class="hlt">water</span> masses at the Agulhas Current termination comes about through the shedding of rings, and this process plays an important role in the global thermohaline circulation. Using several hydrographic sections collected during the ARC (Agulhas Retroflection Cruise), MARE (Mixing of Agulhas Rings Experiment) and WOCE (World Ocean Circulation Experiment), this investigation aims to establish the degree to which Red Sea <span class="hlt">Intermediate</span> <span class="hlt">Water</span> (RSIW) is involved in this exchange and at what level of purity. To this end a wide range of hydrographic parameters were used. Upstream from the Agulhas Current retroflection <span class="hlt">water</span> with clear RSIW origin is shown to move downstream on both the landward and seaward sides of the Agulhas Current with the highest <span class="hlt">water</span> sample purity or <span class="hlt">water</span>-mass content exceeding 15%. The least mixed <span class="hlt">water</span> was found close to the continental shelf. At the retroflection the RSIW purity shows considerable variability that ranges between 5% and 20%. This suggests that RSIW moves down the current in patches of considerably varying degrees of previous mixing. This pattern was also observed in a ring sampled during the ARC experiment. The MARE sections in turn indicate that at times RSIW may be entirely absent in the Agulhas Current. RSIW is therefore shown to travel down the current as discontinuous filaments, and this intermittency is reflected in its presence in Agulhas Rings. From the sections investigated it is therefore clear that any calculation of RSIW fluxes involved in inter-ocean exchange can only be done on the basis of event scales. RSIW not trapped in Agulhas Rings flows east with the Agulhas Return Current.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1352361-present-day-future-antarctic-ice-sheet-climate-surface-mass-balance-community-earth-system-model','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1352361-present-day-future-antarctic-ice-sheet-climate-surface-mass-balance-community-earth-system-model"><span>Present-day and future <span class="hlt">Antarctic</span> ice sheet climate and surface mass balance in the Community Earth System Model</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Lenaerts, Jan T. M.; Vizcaino, Miren; Fyke, Jeremy Garmeson; ...</p> <p>2016-02-01</p> <p>Here, we present climate and surface mass balance (SMB) of the <span class="hlt">Antarctic</span> ice sheet (AIS) as simulated by the global, coupled ocean–atmosphere–land Community Earth System Model (CESM) with a horizontal resolution of ~1° in the past, present and future (1850–2100). CESM correctly simulates present-day <span class="hlt">Antarctic</span> sea ice extent, large-scale atmospheric circulation and near-surface climate, but fails to simulate the recent expansion of <span class="hlt">Antarctic</span> sea ice. The present-day <span class="hlt">Antarctic</span> ice sheet SMB equals 2280 ± 131Gtyear –1, which concurs with existing independent estimates of AIS SMB. When forced by two CMIP5 climate change scenarios (high mitigation scenario RCP2.6 and high-emission scenariomore » RCP8.5), CESM projects an increase of <span class="hlt">Antarctic</span> ice sheet SMB of about 70 Gtyear –1 per degree warming. This increase is driven by enhanced snowfall, which is partially counteracted by more surface melt and runoff along the ice sheet’s edges. This intensifying hydrological cycle is predominantly driven by atmospheric warming, which increases (1) the moisture-carrying capacity of the atmosphere, (2) oceanic source region evaporation, and (3) summer AIS cloud liquid <span class="hlt">water</span> content.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C31B..04K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C31B..04K"><span>Subglacial meltwater channels on the <span class="hlt">Antarctic</span> continental shelf</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kirkham, J. D.; Hogan, K.; Dowdeswell, J. A.; Larter, R. D.; Arnold, N. S.; Nitsche, F. O.; Golledge, N. R.</p> <p>2017-12-01</p> <p>Extensive submarine channel networks exist on the <span class="hlt">Antarctic</span> continental shelf. The genesis of the channels has been attributed to the flow of subglacial meltwater beneath a formerly more expansive <span class="hlt">Antarctic</span> Ice Sheet (AIS), implying that there was an active subglacial hydrological system beneath the past AIS which influenced its ice flow dynamics and mass-loss behaviour. However, the dimensions of the channels are inconsistent with the minimal quantities of meltwater produced under the AIS at present; consequently, their formative mechanism, and its implications for past ice-sheet dynamics, remain unresolved. Here, analysis of >100,000 km2 of multibeam bathymetric data is used to produce the most comprehensive inventory of <span class="hlt">Antarctic</span> submarine channelised landforms to date. Over 2700 bedrock channels are mapped across four locations on the inner continental shelves of the Bellingshausen and Amundsen Seas. Morphometric analysis reveals highly similar distributions of channel widths, depths, cross-sectional areas and geometric properties, with subtle differences present between channels located in the Bellingshausen Sea compared to those situated in the Amundsen Sea region. The channels are 75-3400 m wide, 3-280 m deep, 160-290,000 m2 in cross-sectional area, and exhibit V-shaped cross-sectional geometries that are typically eight times as wide as they are deep. The features are comparable, but substantially larger, than the system of channels known as the Labyrinth in the McMurdo Dry Valleys whose genesis has been attributed to catastrophic outburst floods, sourced from subglacial lakes, during the middle Miocene. A similar process origin is proposed for the channels observed on the <span class="hlt">Antarctic</span> continental shelf, formed through the drainage of relict subglacial lake basins, including some 59 identified using submarine geomorphological evidence and numerical modelling calculations. <span class="hlt">Water</span> is predicted to accumulate in the subglacial lakes over centuries to millennia and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24687148','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24687148"><span>On Hokusai's Great wave off Kanagawa: localization, linearity and a rogue wave in sub-<span class="hlt">Antarctic</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>Dudley, J M; Sarano, V; Dias, F</p> <p>2013-06-20</p> <p>The Hokusai woodcut entitled The great wave off Kanagawa has been interpreted as an unusually large storm wave, likely to be classed as a rogue wave, and possibly generated from nonlinear wave dynamics (J. H. E. Cartwright and H. Nakamura, Notes Rec. R. Soc. 63 , 119-135 (2009)). In this paper, we present a complementary discussion of this hypothesis, discussing in particular how linear and nonlinear mechanisms can both contribute to the emergence of rogue wave events. By making reference to the Great wave 's simultaneous transverse and longitudinal localization, we show that the purely linear mechanism of directional focusing also predicts characteristics consistent with those of the Great wave . In addition, we discuss the properties of a particular rogue wave photographed on the open ocean in sub-<span class="hlt">Antarctic</span> <span class="hlt">waters</span>, which shows two-dimensional localization and breaking dynamics remarkably similar to Hokusai's depiction in the woodcut.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3645210','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3645210"><span>On Hokusai's Great wave off Kanagawa: localization, linearity and a rogue wave in sub-<span class="hlt">Antarctic</span> <span class="hlt">waters</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>Dudley, J. M.; Sarano, V.; Dias, F.</p> <p>2013-01-01</p> <p>The Hokusai woodcut entitled The great wave off Kanagawa has been interpreted as an unusually large storm wave, likely to be classed as a rogue wave, and possibly generated from nonlinear wave dynamics (J. H. E. Cartwright and H. Nakamura, Notes Rec. R. Soc. 63, 119–135 (2009)). In this paper, we present a complementary discussion of this hypothesis, discussing in particular how linear and nonlinear mechanisms can both contribute to the emergence of rogue wave events. By making reference to the Great wave's simultaneous transverse and longitudinal localization, we show that the purely linear mechanism of directional focusing also predicts characteristics consistent with those of the Great wave. In addition, we discuss the properties of a particular rogue wave photographed on the open ocean in sub-<span class="hlt">Antarctic</span> <span class="hlt">waters</span>, which shows two-dimensional localization and breaking dynamics remarkably similar to Hokusai's depiction in the woodcut. PMID:24687148</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/1988DSRA...35..311F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1988DSRA...35..311F"><span><span class="hlt">Water</span> mass modification at the Agulhas retroflection: chlorofluoromethane studies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fine, Rana A.; Warner, Mark J.; Weiss, Ray F.</p> <p>1988-03-01</p> <p>Chlorofluoromethane (CFM) and hydrographic data from the 1983 Agulhas Retroflection cruise are used to show the importance of the region in ventilating thermocline and <span class="hlt">Intermediate</span> <span class="hlt">Waters</span> of the southwest Indian ocean gyre. Generally South Atlantic <span class="hlt">waters</span> are more recently ventilated by at least two years than those of the South Indian Ocean, probably because the latter are farther downstream from the source regions near the South Atlantic subantarctic sector. A two-component mixing model shows that the outflow from the Agulhas Retroflection (14-4°C) was composed of South Indian <span class="hlt">water</span> and at least 23% South Atlantic <span class="hlt">water</span>. However, at the density of Indian sector Subantarctic Mode <span class="hlt">Water</span> the inflow into the Agulhas Retroflection was well preserved in the outflow, and the South Atlantic and Indian <span class="hlt">waters</span> appear to be ventilated by different <span class="hlt">water</span> masses. In addition, strong interleaving was found throughout the survey area (between 14 and 4°C), characterized by correlations of negative salinity anomalies with high CFM concentrations. At the density of <span class="hlt">Antarctic</span> <span class="hlt">Intermediate</span> <span class="hlt">Water</span> (AAIW) there was interleaving of both low salinity <span class="hlt">water</span> and higher salinity Red Sea <span class="hlt">Water</span>. Using estimates of past atmospheric ratios of two CFMs, we calculate that AAIW within the retroflection was 50-75% diluted by mixing with CFM-free <span class="hlt">water</span> since leaving the source region. Results from the two-component mixing model, which show substantial contributions of South Atlantic <span class="hlt">water</span> in the outflow, suggest that the return flow for the 10 Sv leakage of Indian Ocean <span class="hlt">water</span> via the Agulhas Current into the South Atlantic [ GORDON (1985) Science, 227, 1030-1033; GORDONet al. (1987) Deep-Sea Research, 34, 565-600] is occurring at thermocline and <span class="hlt">intermediate</span> depths. A combination of active mixing in this region and similarity in the ventilation processes may be the reason that the South Atlantic and Indian thermoclines are coincident in temperature and salinity space (between 15 and 7°C) as noted</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930022712&hterms=geothermal+heating&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dgeothermal%2Bheating','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930022712&hterms=geothermal+heating&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dgeothermal%2Bheating"><span>Effect of subglacial volcanism on changes in the West <span class="hlt">Antarctic</span> Ice Sheet</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Behrendt, John C.</p> <p>1993-01-01</p> <p>Rapid changes in the West <span class="hlt">Antarctic</span> Ice Sheet (WAIS) may affect future global sea-level changes. Alley and Whillans note that 'the <span class="hlt">water</span> responsible for separating the glacier from its bed is produced by frictional dissipation and geothermal heat,' but assume that changes in geothermal flux would ordinarily be expected to have slower effects than glaciological parameters. I suggest that episodic subglacial volcanism and geothermal heating may have significantly greater effects on the WAIS than is generally appreciated. The WAIS flows through the active, largely asiesmic West <span class="hlt">Antarctic</span> rift system (WS), which defines the sub-sea-level bed of the glacier. Various lines of evidence summarized in Behrendt et al. (1991) indicate high heat flow and shallow asthenosphere beneath the extended, weak lithosphere underlying the WS and the WAIS. Behrendt and Cooper suggest a possible synergistic relation between Cenozoic tectonism, episodic mountain uplift and volcanism in the West <span class="hlt">Antarctic</span> rift system, and the waxing and waning of the <span class="hlt">Antarctic</span> ice sheet beginning about earliest Oligocene time. A few active volcanoes and late-Cenozoic volcanic rocks are exposed throughout the WS along both flanks, and geophysical data suggest their presence beneath the WAIS. No part of the rift system can be considered inactive. I propose that subglacial volcanic eruptions and ice flow across areas of locally (episodically?) high heat flow--including volcanically active areas--should be considered possibly to have a forcing effect on the thermal regime resulting in increased melting at the base of the ice streams.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSHE44B1508G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSHE44B1508G"><span>Seismic Imaging of Circumpolar Deep <span class="hlt">Water</span> Exchange across the Shelf Break of the <span class="hlt">Antarctic</span> Peninsula</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gunn, K.; White, N.; Larter, R. D.; Falder, M.; Caulfield, C. C. P.</p> <p>2016-02-01</p> <p>The western <span class="hlt">Antarctic</span> Peninsula is an area of recent extreme atmospheric warming. In the adjacent ocean, there is particular interest in on-shelf movement of Circumpolar Deep <span class="hlt">Water</span> as a possible link to changing climate by affecting ice shelf processes. Here, we investigate on-shelf intrusions using two-dimensional seismic imaging of the <span class="hlt">water</span> column which has vertical and horizontal resolutions of 10 m. 8 seismic profiles were acquired in February 2015 using the RRS James Clark Ross. These profiles traverse the shelf break and cross two bathymetric features, the Marguerite and Biscoe troughs, which may play a role in <span class="hlt">water</span> exchange processes. Seismic data were acquired using two Generator-Injector air guns fired every 10 s with a pressure of 2000 psi. Reflections were recorded on a 2.4 km streamer of 192 receivers spaced every 12.5 m. Observed reflections in the processed records are caused by rapid changes of temperature ( 80%) and salinity ( 20%), delineating <span class="hlt">water</span> masses of different properties. 13 XCTDs and XBTs plus a 38 kHz echo-sounder profile were simultaneously acquired along seismic profiles and used for calibration. Preliminary results show the top of the Winter <span class="hlt">Water</span> layer as a bright reflection at 50-120 m depth across the entire survey, corresponding to temperatures ≤ -1°C. Curved, discontinuous, eddy-like reflections, also seen on echo-sounder profiles, are attributed to modified Upper Circumpolar Deep <span class="hlt">Water</span> with temperatures ≥ 1.34°C. A warm core eddy, 11 km long and 220 m high, is visible 2 km inland of the shelf break. Pure Upper Circumpolar Deep <span class="hlt">Water</span> of temperatures ≥ 1.80°C is aligned with weak but discernible, lens-shaped reflections. Eddy-like structures and the overall reflective morphology yield useful insights into shelf exchange processes, suggestive of three potential mechanisms: (i) topography controlled flow; (ii) an 'ice-pump' mechanism; and (iii) mesoscale eddies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5319791','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5319791"><span>Modelling the effects of environmental conditions on the acoustic occurrence and behaviour of <span class="hlt">Antarctic</span> blue whales</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Shabangu, Fannie W.; Yemane, Dawit; Stafford, Kathleen M.; Ensor, Paul; Findlay, Ken P.</p> <p>2017-01-01</p> <p>Harvested to perilously low numbers by commercial whaling during the past century, the large scale response of <span class="hlt">Antarctic</span> blue whales Balaenoptera musculus intermedia to environmental variability is poorly understood. This study uses acoustic data collected from 586 sonobuoys deployed in the austral summers of 1997 through 2009, south of 38°S, coupled with visual observations of blue whales during the IWC SOWER line-transect surveys. The characteristic Z-call and D-call of <span class="hlt">Antarctic</span> blue whales were detected using an automated detection template and visual verification method. Using a random forest model, we showed the environmental preferences pattern, spatial occurrence and acoustic behaviour of <span class="hlt">Antarctic</span> blue whales. Distance to the southern boundary of the <span class="hlt">Antarctic</span> Circumpolar Current (SBACC), latitude and distance from the nearest <span class="hlt">Antarctic</span> shores were the main geographic predictors of blue whale call occurrence. Satellite-derived sea surface height, sea surface temperature, and productivity (chlorophyll-a) were the most important environmental predictors of blue whale call occurrence. Call rates of D-calls were strongly predicted by the location of the SBACC, latitude and visually detected number of whales in an area while call rates of Z-call were predicted by the SBACC, latitude and longitude. Satellite-derived sea surface height, wind stress, wind direction, <span class="hlt">water</span> depth, sea surface temperatures, chlorophyll-a and wind speed were important environmental predictors of blue whale call rates in the Southern Ocean. Blue whale call occurrence and call rates varied significantly in response to inter-annual and long term variability of those environmental predictors. Our results identify the response of <span class="hlt">Antarctic</span> blue whales to inter-annual variability in environmental conditions and highlighted potential suitable habitats for this population. Such emerging knowledge about the acoustic behaviour, environmental and habitat preferences of <span class="hlt">Antarctic</span> blue whales is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28222124','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28222124"><span>Modelling the effects of environmental conditions on the acoustic occurrence and behaviour of <span class="hlt">Antarctic</span> blue whales.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Shabangu, Fannie W; Yemane, Dawit; Stafford, Kathleen M; Ensor, Paul; Findlay, Ken P</p> <p>2017-01-01</p> <p>Harvested to perilously low numbers by commercial whaling during the past century, the large scale response of <span class="hlt">Antarctic</span> blue whales Balaenoptera musculus intermedia to environmental variability is poorly understood. This study uses acoustic data collected from 586 sonobuoys deployed in the austral summers of 1997 through 2009, south of 38°S, coupled with visual observations of blue whales during the IWC SOWER line-transect surveys. The characteristic Z-call and D-call of <span class="hlt">Antarctic</span> blue whales were detected using an automated detection template and visual verification method. Using a random forest model, we showed the environmental preferences pattern, spatial occurrence and acoustic behaviour of <span class="hlt">Antarctic</span> blue whales. Distance to the southern boundary of the <span class="hlt">Antarctic</span> Circumpolar Current (SBACC), latitude and distance from the nearest <span class="hlt">Antarctic</span> shores were the main geographic predictors of blue whale call occurrence. Satellite-derived sea surface height, sea surface temperature, and productivity (chlorophyll-a) were the most important environmental predictors of blue whale call occurrence. Call rates of D-calls were strongly predicted by the location of the SBACC, latitude and visually detected number of whales in an area while call rates of Z-call were predicted by the SBACC, latitude and longitude. Satellite-derived sea surface height, wind stress, wind direction, <span class="hlt">water</span> depth, sea surface temperatures, chlorophyll-a and wind speed were important environmental predictors of blue whale call rates in the Southern Ocean. Blue whale call occurrence and call rates varied significantly in response to inter-annual and long term variability of those environmental predictors. Our results identify the response of <span class="hlt">Antarctic</span> blue whales to inter-annual variability in environmental conditions and highlighted potential suitable habitats for this population. Such emerging knowledge about the acoustic behaviour, environmental and habitat preferences of <span class="hlt">Antarctic</span> blue whales is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2669364','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2669364"><span>Trade-off between aerobic capacity and locomotor capability in an <span class="hlt">Antarctic</span> pteropod</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Rosenthal, Joshua J. C.; Seibel, Brad A.; Dymowska, Agnieszka; Bezanilla, Francisco</p> <p>2009-01-01</p> <p>At −1.8 °C, the <span class="hlt">waters</span> of Antarctica pose a formidable physiological barrier for most ectotherms. The few taxa that inhabit this zone have presumably made specific adjustments to their neuromuscular function and have enhanced their metabolic capacity. However, support for this assertion is equivocal and the details of specific compensations are largely unknown. This can generally be attributed to the fact that most <span class="hlt">Antarctic</span> organisms are either too distantly related to their temperate relatives to permit direct comparisons (e.g., notothenioid fishes) or because they are not amenable to neuromuscular recording. Here, as a comparative model, we take advantage of 2 pelagic molluscs in the genus Clione to conduct a broadly integrative investigation on neuromuscular adaptation to the extreme cold. We find that for the <span class="hlt">Antarctic</span> congener aerobic capacity is enhanced, but at a cost. To support a striking proliferation of mitochondria, the <span class="hlt">Antarctic</span> species has shed a 2-gear swim system and the associated specialized neuromuscular components, resulting in greatly reduced scope for locomotor activity. These results suggest that polar animals have undergone substantial tissue-level reorganizations to accommodate their environment, which may reduce their capacity to acclimate to a changing climate. PMID:19325127</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014Msngr.155...17K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014Msngr.155...17K"><span><span class="hlt">Antarctic</span> Air Visits Paranal — Opening New Science Windows</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kerber, F.; Kuntschner, H.; Querel, R. R.; van den Ancker, M.</p> <p>2014-03-01</p> <p>Extremely low humidity (precipitable <span class="hlt">water</span> vapour [PWV] of ~ 0.1 mm) in the atmosphere above Paranal has been measured by a <span class="hlt">water</span> vapour radiometer over a period of about 12 hours. PWV values < 0.2 mm are usually only found at very high altitude or in Antarctica. In fact a pocket of <span class="hlt">Antarctic</span> air has been shown to be responsible for this phenomenon and it may occur a few times per year at Paranal. We highlight the science opportunities — created by new atmospheric windows — that arise in such conditions. The community is invited to provide feedback on how to make best use of low PWV with the VLT.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014TCry....8..673F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014TCry....8..673F"><span>Cascading <span class="hlt">water</span> underneath Wilkes Land, East <span class="hlt">Antarctic</span> ice sheet, observed using altimetry and digital elevation models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Flament, T.; Berthier, E.; Rémy, F.</p> <p>2014-04-01</p> <p>We describe a major subglacial lake drainage close to the ice divide in Wilkes Land, East Antarctica, and the subsequent cascading of <span class="hlt">water</span> underneath the ice sheet toward the coast. To analyse the event, we combined altimetry data from several sources and subglacial topography. We estimated the total volume of <span class="hlt">water</span> that drained from Lake CookE2 by differencing digital elevation models (DEM) derived from ASTER and SPOT5 stereo imagery acquired in January 2006 and February 2012. At 5.2 ± 1.5 km3, this is the largest single subglacial drainage event reported so far in Antarctica. Elevation differences between ICESat laser altimetry spanning 2003-2009 and the SPOT5 DEM indicate that the discharge started in November 2006 and lasted approximately 2 years. A 13 m uplift of the surface, corresponding to a refilling of about 0.6 ± 0.3 km3, was observed between the end of the discharge in October 2008 and February 2012. Using the 35-day temporal resolution of Envisat radar altimetry, we monitored the subsequent filling and drainage of connected subglacial lakes located downstream of CookE2. The total volume of <span class="hlt">water</span> traveling within the theoretical 500-km-long flow paths computed with the BEDMAP2 data set is similar to the volume that drained from Lake CookE2, and our observations suggest that most of the <span class="hlt">water</span> released from Lake CookE2 did not reach the coast but remained trapped underneath the ice sheet. Our study illustrates how combining multiple remote sensing techniques allows monitoring of the timing and magnitude of subglacial <span class="hlt">water</span> flow beneath the East <span class="hlt">Antarctic</span> ice sheet.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19860019356','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19860019356"><span>Thermoluminescence and <span class="hlt">Antarctic</span> meteorites</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sears, D. W. G.; Hasan, F. A.</p> <p>1986-01-01</p> <p>The level of natural thermoluminescence (TL) in meteorites is the result of competition between build-up, due to exposure to cosmic radiation, and thermal decay. <span class="hlt">Antarctic</span> meteorites tend to have lower natural TL than non-<span class="hlt">Antarctic</span> meteorites because of their generally larger terrestrial ages. However, since a few observed falls have low TL due to a recent heating event, such as passage within approximately 0.7 astronomical units of the Sun, this could also be the case for some <span class="hlt">Antarctic</span> meteorites. Dose rate variations due to shielding, heating during atmospheric passage, and anomalous fading also cause natural TL variations, but the effects are either relatively small, occur infrequently, or can be experimentally circumvented. The TL sensitivity of meteorites reflects the abundance and nature of the feldspar. Thus intense shock, which destroys feldspar, causes the TL sensitivity to decrease by 1 to 2 orders of magnitude, while metamorphism, which generates feldspar through the devitrification of glass, causes TL sensitivity to increase by a factor of approximately 10000. The TL-metamorphism relationship is particularly strong for the lowest levels of metamorphism. The order-disorder transformation in feldspar also affect the TL emission characteristics and thus TL provides a means of paleothermometry.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26296718','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26296718"><span>A Biophysical and Economic Profile of South Georgia and the South Sandwich Islands as Potential Large-Scale <span class="hlt">Antarctic</span> Protected Areas.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Rogers, Alex D; Yesson, Christopher; Gravestock, Pippa</p> <p>2015-01-01</p> <p>The current hiatus in the establishment of a network of marine protected areas (MPAs) in the <span class="hlt">Antarctic</span> means that other routes to conservation are required. The protection of overseas territories in the <span class="hlt">Antarctic</span> and sub-<span class="hlt">Antarctic</span> represents one way to advance the initiation of such a network. This review of the physical and biological features of the United Kingdom (U.K.) overseas territories of South Georgia and South Sandwich Islands (SGSSI) is undertaken to estimate the importance of the islands in terms of marine conservation in the Southern Ocean and globally. The economy and management of SGSSI are also analysed, and the question of whether the islands already have sufficient protection to constitute part of an <span class="hlt">Antarctic</span> network of MPAs is assessed. The SGSSI comprise unique geological and physical features, a diverse marine biota, including a significant proportion of endemic species and globally important breeding populations of marine predators. Regardless of past exploitation of biotic resources, such as seals, whales and finfish, SGSSI would make a significant contribution to biological diversity in an <span class="hlt">Antarctic</span> network of MPAs. At present, conservation measures do not adequately protect all of the biological features that render the islands so important in terms of conservation at a regional and global level. However, a general lack of data on <span class="hlt">Antarctic</span> marine ecosystems (particularly needed for SGSSSI) makes it difficult to assess this fully. One barrier to achieving more complete protection is the continuing emphasis on fishing effort in these <span class="hlt">waters</span> by U.K. government. Other non-U.K. <span class="hlt">Antarctic</span> overseas territories of conservation importance are also compromised as MPAs because of the exploitation of fisheries resources in their <span class="hlt">waters</span>. The possible non-use values of SGSSI as well as the importance of ecosystem services that are indirectly used by people are outlined in this review. Technology is improving the potential for management of remote MPAs</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70184383','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70184383"><span>Bacteriophage in polar inland <span class="hlt">waters</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>Säwström, Christin; Lisle, John; Anesio, A.M.; Priscu, John C.; Laybourn-Parry, J.</p> <p>2008-01-01</p> <p>Bacteriophages are found wherever microbial life is present and play a significant role in aquatic ecosystems. They mediate microbial abundance, production, respiration, diversity, genetic transfer, nutrient cycling and particle size distribution. Most studies of bacteriophage ecology have been undertaken at temperate latitudes. Data on bacteriophages in polar inland <span class="hlt">waters</span> are scant but the indications are that they play an active and dynamic role in these microbially dominated polar ecosystems. This review summarises what is presently known about polar inland bacteriophages, ranging from subglacial <span class="hlt">Antarctic</span> lakes to glacial ecosystems in the Arctic. The review examines interactions between bacteriophages and their hosts and the abiotic and biotic variables that influence these interactions in polar inland <span class="hlt">waters</span>. In addition, we consider the proportion of the bacteria in Arctic and <span class="hlt">Antarctic</span> lake and glacial <span class="hlt">waters</span> that are lysogenic and visibly infected with viruses. We assess the relevance of bacteriophages in the microbial loop in the extreme environments of <span class="hlt">Antarctic</span> and Arctic inland <span class="hlt">waters</span> with an emphasis on carbon cycling.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=315750','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=315750"><span>Numerical Taxonomy of Some Bacteria Isolated from <span class="hlt">Antarctic</span> and Tropical Seawaters1</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Pfister, Robert M.; Burkholder, Paul R.</p> <p>1965-01-01</p> <p>Pfister, Robert M. (Lamont Geological Observatory, Palisades, N.Y.), and Paul R. Burkholder. Numerical taxonomy of some bacteria isolated from <span class="hlt">Antarctic</span> and tropical seawaters. J. Bacteriol. 90:863–872. 1965.—Microorganisms from <span class="hlt">Antarctic</span> seas and from tropical <span class="hlt">waters</span> near Puerto Rico were examined with a series of morphological, physiological, and biochemical tests. The results of these analyses were coded on punch cards, and similarity matrices were computed with a program for an IBM 1620 computer. When the matrix was reordered by use of the single-linkage technique, and the results were plotted with four symbols for different per cent similarity ranges, nine groups of microorganisms were revealed. The data suggest that organisms occurring in different areas of the open ocean may be profitably studied with standardized computer techniques. PMID:5847807</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.T13F..06T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.T13F..06T"><span>Turning up the Heat on the <span class="hlt">Antarctic</span> Ice Sheet (From Below): Challenges and Near-Term Opportunities for Measuring <span class="hlt">Antarctic</span> Geothermal Fluxes (Invited)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tulaczyk, S. M.; Hossainzadeh, S.</p> <p>2010-12-01</p> <p><span class="hlt">Antarctic</span> heat flow plays an important role in determining the rate of meltwater production at the base of the <span class="hlt">Antarctic</span> ice sheet. Basal meltwater represents a key control on ice sheet mass balance, <span class="hlt">Antarctic</span> geochemical fluxes into the Southern Ocean, and subglacial microbial habitats. However, direct measurements of heat flow are difficult in glaciated terrains. Vertical temperature profiles determined in ice boreholes are influenced by thermal energy fluxes associated with basal melting/freezing and have to be used with caution when calculating geothermal flux rates. Two published continent-wide geophysical estimates of <span class="hlt">Antarctic</span> geothermal fluxes provide valuable databases but are not fully consistent with each other and need to be verified by direct subglacial measurements. Planned drilling into <span class="hlt">Antarctic</span> subglacial environments will offer the opportunity to perform such measurements. Determination of temperature gradients in sedimentary sequences resting at the bottom of subglacial lakes will offer particularly useful insights. Temperature profiles in such environments will not be thermally or mechanically disturbed as it may be the case in till layers proximal to a sliding ice base. We will review plans for making such measurements as part of the WISSARD (Whillans Ice Stream Subglacial Access Research Drilling) project, which is scheduled to penetrate the West <span class="hlt">Antarctic</span> ice sheet in 2012-13 and 2013-14.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040090076&hterms=algae&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dalgae','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040090076&hterms=algae&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dalgae"><span>The effect of low temperature on <span class="hlt">Antarctic</span> endolithic green algae</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Meyer, M. A.; Morris, G. J.; Friedmann, E. I.</p> <p>1988-01-01</p> <p>Laboratory experiments show that undercooling to about -5 degrees C occurs in colonized Beacon sandstones of the Ross Desert, Antarctica. High-frequency temperature oscillations between 5 degrees C and -5 degrees C or -10 degrees C (which occur in nature on the rock surface) did not damage Hemichloris antarctica. In a cryomicroscope, H. antarctica appeared to be undamaged after slow or rapid cooling to -50 degrees C. 14CO2 incorporation after freezing to -20 degrees C was unaffected in H. antarctica or in Trebouxia sp. but slightly depressed in Stichococcus sp. (isolated from a less extreme <span class="hlt">Antarctic</span> habitat). These results suggest that the freezing regime in the <span class="hlt">Antarctic</span> desert is not injurious to endolithic algae. It is likely that the freezing-point depression inside the rock makes available liquid <span class="hlt">water</span> for metabolic activity at subzero temperatures. Freezing may occur more frequently on the rock surface and contribute to the abiotic nature of the surface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70030552','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70030552"><span><span class="hlt">Antarctic</span> climate cooling and response of diatoms in glacial meltwater streams</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Esposito, R.M.M.; Horn, S.L.; McKnight, Diane M.; Cox, M.J.; Grant, M.C.; Spaulding, S.A.; Doran, P.T.; Cozzetto, K.D.</p> <p>2006-01-01</p> <p>To understand biotic responses to an <span class="hlt">Antarctic</span> cooling trend diatom samples from glacial meltwater streams in the McMurdo Dry Valleys, the largest ice-free area in Antarctica. Diatoms are abundant in these streams, and 24 of 40 species have only been found in the <span class="hlt">Antarctic</span>. The percentage of these <span class="hlt">Antarctic</span> diatom species increased with decreasing annual stream flow and increasing harshness of the stream habitat. The species diversity of assemblages reached a maximum when the <span class="hlt">Antarctic</span> species accounted for 40-60% of relative diatom abundance. Decreased solar radiation and air-temperatures reduce annual stream flow, raising the dominance of these <span class="hlt">Antarctic</span> species to levels above 60%. Thus, cooling favors the <span class="hlt">Antarctic</span> species, and lowers diatom species diversity in this region. Copyright 2006 by the American Geophysical Union.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMPA32A..08R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMPA32A..08R"><span>Reaching for the Horizon: Enabling 21st Century <span class="hlt">Antarctic</span> Science</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rogan-Finnemore, M.; Kennicutt, M. C., II; Kim, Y.</p> <p>2015-12-01</p> <p>The Council of Managers of National <span class="hlt">Antarctic</span> Programs' (COMNAP) <span class="hlt">Antarctic</span> Roadmap Challenges(ARC) project translated the 80 highest priority <span class="hlt">Antarctic</span> and Southern Ocean scientific questionsidentified by the community via the SCAR <span class="hlt">Antarctic</span> Science Horizon Scan into the highest prioritytechnological, access, infrastructure and logistics needs to enable the necessary research to answer thequestions. A workshop assembled expert and experienced <span class="hlt">Antarctic</span> scientists and National <span class="hlt">Antarctic</span>Program operators from around the globe to discern the highest priority technological needs includingthe current status of development and availability, where the technologies will be utilized in the <span class="hlt">Antarctic</span> area, at what temporal scales and frequencies the technologies will be employed,and how broadly applicable the technologies are for answering the highest priority scientific questions.Secondly the logistics, access, and infrastructure requirements were defined that are necessary todeliver the science in terms of feasibility including cost and benefit as determined by expected scientific return on investment. Finally, based on consideration of the science objectives and the mix oftechnologies implications for configuring National <span class="hlt">Antarctic</span> Program logistics capabilities andinfrastructure architecture over the next 20 years were determined. In particular those elements thatwere either of a complexity, requiring long term investments to achieve and/or having an associated cost that realistically can only (or best) be achieved by international coordination, planning and partnerships were identified. Major trends (changes) in logistics, access, and infrastructure requirements were identified that allow for long-term strategic alignment of international capabilities, resources and capacity. The outcomes of this project will be reported.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1918401P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1918401P"><span>Drivers of <span class="hlt">Antarctic</span> sea-ice expansion and Southern Ocean surface cooling over the past four decades</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Purich, Ariaan; England, Matthew</p> <p>2017-04-01</p> <p>Despite global warming, total <span class="hlt">Antarctic</span> sea-ice coverage has increased overall during the past four decades. In contrast, the majority of CMIP5 models simulate a decline. In addition, Southern Ocean surface <span class="hlt">waters</span> have largely cooled, in stark contrast to almost all historical CMIP5 simulations. Subantarctic Surface <span class="hlt">Waters</span> have cooled and freshened while <span class="hlt">waters</span> to the north of the <span class="hlt">Antarctic</span> Circumpolar Current have warmed and increased in salinity. It remains unclear as to what extent the cooling and <span class="hlt">Antarctic</span> sea-ice expansion is due to natural variability versus anthropogenic forcing; due for example to changes in the Southern Annular Mode (SAM). It is also unclear what the respective role of surface buoyancy fluxes is compared to internal ocean circulation changes, and what the implications are for longer-term climate change in the region. In this presentation we will outline three distinct drivers of recent Southern Ocean surface trends that have each made a significant contribution to regional cooling: (1) wind-driven surface cooling and sea-ice expansion due to shifted westerly winds, (2) teleconnections of decadal variability from the tropical Pacific, and (3) surface cooling and ice expansion due to large-scale Southern Ocean freshening, most likely driven by SAM-related precipitation trends over the open ocean. We will also outline the main reasons why climate models for the most part miss these Southern Ocean cooling trends, despite capturing overall trends in the SAM.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22042434','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22042434"><span>Anchor ice and benthic disturbance in shallow <span class="hlt">Antarctic</span> <span class="hlt">waters</span>: interspecific variation in initiation and propagation of ice crystals.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Denny, Mark; Dorgan, Kelly M; Evangelista, Dennis; Hettinger, Annaliese; Leichter, James; Ruder, Warren C; Tuval, Idan</p> <p>2011-10-01</p> <p>Sea ice typically forms at the ocean's surface, but given a source of supercooled <span class="hlt">water</span>, an unusual form of ice--anchor ice--can grow on objects in the <span class="hlt">water</span> column or at the seafloor. For several decades, ecologists have considered anchor ice to be an important agent of disturbance in the shallow-<span class="hlt">water</span> benthic communities of McMurdo Sound, Antarctica, and potentially elsewhere in polar seas. Divers have documented anchor ice in the McMurdo communities, and its presence coincides with reduced abundance of the sponge Homaxinella balfourensis, which provides habitat for a diverse assemblage of benthic organisms. However, the mechanism of this disturbance has not been explored. Here we show interspecific differences in anchor-ice formation and propagation characteristics for <span class="hlt">Antarctic</span> benthic organisms. The sponges H. balfourensis and Suberites caminatus show increased incidence of formation and accelerated spread of ice crystals compared to urchins and sea stars. Anchor ice also forms readily on sediments, from which it can grow and adhere to organisms. Our results are consistent with, and provide a potential first step toward, an explanation for disturbance patterns observed in shallow polar benthic communities. Interspecific differences in ice formation raise questions about how surface tissue characteristics such as surface area, rugosity, and mucus coating affect ice formation on invertebrates.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28054598','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28054598"><span><span class="hlt">Antarctic</span> ice sheet discharge driven by atmosphere-ocean feedbacks at the Last Glacial Termination.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Fogwill, C J; Turney, C S M; Golledge, N R; Etheridge, D M; Rubino, M; Thornton, D P; Baker, A; Woodward, J; Winter, K; van Ommen, T D; Moy, A D; Curran, M A J; Davies, S M; Weber, M E; Bird, M I; Munksgaard, N C; Menviel, L; Rootes, C M; Ellis, B; Millman, H; Vohra, J; Rivera, A; Cooper, A</p> <p>2017-01-05</p> <p>Reconstructing the dynamic response of the <span class="hlt">Antarctic</span> ice sheets to warming during the Last Glacial Termination (LGT; 18,000-11,650 yrs ago) allows us to disentangle ice-climate feedbacks that are key to improving future projections. Whilst the sequence of events during this period is reasonably well-known, relatively poor chronological control has precluded precise alignment of ice, atmospheric and marine records, making it difficult to assess relationships between <span class="hlt">Antarctic</span> ice-sheet (AIS) dynamics, climate change and sea level. Here we present results from a highly-resolved 'horizontal ice core' from the Weddell Sea Embayment, which records millennial-scale AIS dynamics across this extensive region. Counterintuitively, we find AIS mass-loss across the full duration of the <span class="hlt">Antarctic</span> Cold Reversal (ACR; 14,600-12,700 yrs ago), with stabilisation during the subsequent millennia of atmospheric warming. Earth-system and ice-sheet modelling suggests these contrasting trends were likely <span class="hlt">Antarctic</span>-wide, sustained by feedbacks amplified by the delivery of Circumpolar Deep <span class="hlt">Water</span> onto the continental shelf. Given the anti-phase relationship between inter-hemispheric climate trends across the LGT our findings demonstrate that Southern Ocean-AIS feedbacks were controlled by global atmospheric teleconnections. With increasing stratification of the Southern Ocean and intensification of mid-latitude westerly winds today, such teleconnections could amplify AIS mass loss and accelerate global sea-level rise.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.U53C..10T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.U53C..10T"><span>Exploration of <span class="hlt">Antarctic</span> Subglacial environments: a challenge for analytical chemistry</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Traversi, R.; Becagli, S.; Castellano, E.; Ghedini, C.; Marino, F.; Rugi, F.; Severi, M.; Udisti, R.</p> <p>2009-12-01</p> <p>The large number of subglacial lakes detected in the Dome C area in East Antarctica suggests that this region may be a valuable source of paleo-records essential for understanding the evolution of the <span class="hlt">Antarctic</span> ice cap and climate changes in the last several millions years. In the framework of the Project on “Exploration and characterization of Concordia Lake, Antarctica”, supported by Italian Program for <span class="hlt">Antarctic</span> Research (PNRA), a glaciological investigation of the Dome C “Lake District” are planned. Indeed, the glacio-chemical characterisation of the ice column over subglacial lakes will allow to evaluate the fluxes of major and trace chemical species along the ice column and in the accreted ice and, consequently, the availability of nutrients and oligo-elements for possible biological activity in the lake <span class="hlt">water</span> and sediments. Melting and freezing at the base of the ice sheet should be able to deliver carbon and salts to the lake, as observed for the Vostok subglacial lake, which are thought to be able to support a low concentration of micro-organisms for extended periods of time. Thus, this investigation represents the first step for exploring the subglacial environments including sampling and analysis of accreted ice, lake <span class="hlt">water</span> and sediments. In order to perform reliable analytical measurements, especially of trace chemical species, clean sub-sampling and analytical techniques are required. For this purpose, the techniques already used by the CHIMPAC laboratory (Florence University) in the framework of international <span class="hlt">Antarctic</span> drilling Projects (EPICA - European Project for Ice Coring in Antarctica, TALDICE - TALos Dome ICE core, ANDRILL MIS - <span class="hlt">ANTarctic</span> DRILLing McMurdo Ice Shelf) were optimised and new techniques were developed to ensure a safe sample handling. CHIMPAC laboratory has been involved since several years in the study of <span class="hlt">Antarctic</span> continent, primarily focused on understanding the bio-geo-chemical cycles of chemical markers and 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/2060/19980107899','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19980107899"><span>Ice in Channels and Ice-Rock Mixtures in Valleys on Mars: Did They Slide on Deformable Rubble Like <span class="hlt">Antarctic</span> Ice Streams?</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lucchitta, B. K.</p> <p>1997-01-01</p> <p>Recent studies of ice streams in Antarctica reveal a mechanism of basal motion that may apply to channels and valleys on Mars. The mechanism is sliding of the ice on deformable <span class="hlt">water</span>-saturated till under high pore pressures. It has been suggested by Lucchitta that ice was present in outflow channels on Mars and gave them their distinctive morphology. This ice may have slid like <span class="hlt">Antarctic</span> ice streams but on rubbly weathering products rather than till. However, to generate <span class="hlt">water</span> under high pore pressures, elevated heatflow is needed to melt the base of the ice. Either volcanism or higher heatflow more than 2 b.y. ago could have raised the basal temperature. Regarding valley networks, higher heatflow 3 b.y. ago could have allowed sliding of ice-saturated overburden at a few hundred meters depth. If the original, pristine valleys were somewhat deeper than they are now, they could have formed by the same mechanism. Recent sounding of the seafloor in front of the Ross Ice Shelf in Antarctica reveals large persistent patterns of longitudinal megaflutes and drumlinoid forms, which bear remarkable resemblance to longitudinal grooves and highly elongated streamlined islands found on the floors of martian outflow channels. The flutes are interpreted to have formed at the base of ice streams during the last glacial advance. Additional similarities of <span class="hlt">Antarctic</span> ice streams with martian outflow channels are apparent. <span class="hlt">Antarctic</span> ice streams are 30 to 80 km wide and hundreds of kilometers long. Martian outflow channels have similar dimensions. Ice stream beds are below sea level. Carr determined that most common floor elevations of martian outflow channels lie below martian datum, which may have been close to or below past martian sea levels. The <span class="hlt">Antarctic</span> ice stream bed gradient is flat and locally may go uphill, and surface slopes are exceptionally. Martian channels also have floor gradients that are shallow or go uphill locally and have low surface gradients. The depth to the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70195916','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70195916"><span><span class="hlt">Antarctic</span> glacier-tongue velocities from Landsat images: First results</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Lucchitta, Baerbel K.; Mullins, K.F.; Allison, A.L.; Ferrigno, Jane G.</p> <p>1993-01-01</p> <p>We measured the velocities of six glacier tongues and a few tongues within ice shelves distributed around the <span class="hlt">Antarctic</span> coastline by determining the displacement of crevasse patterns seen on sequential Landsat images. The velocities range from less than 0.2 km a−1 for East <span class="hlt">Antarctic</span> ice-shelf tongues to more than 2.5 km a−1 for the Thwaites Glacier Tongue. All glacier tongues show increases in velocity toward their distal margins. In general, the tongues of glaciers draining the West <span class="hlt">Antarctic</span> ice sheet have moved significantly faster than those in East Antarctica. This observation may be significant in light of the hypothesized possible disintegration of the West <span class="hlt">Antarctic</span> ice sheet.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29316466','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29316466"><span>Metal complexation capacity of <span class="hlt">Antarctic</span> lacustrine sediments.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Alberti, Giancarla; Mussi, Matteo; Quattrini, Federico; Pesavento, Maria; Biesuz, Raffaela</p> <p>2018-04-01</p> <p>The purpose of this study is to implement a work that is a part of a project funded by the Italian National <span class="hlt">Antarctic</span> Research Program (PNRA, Piano Nazionale di Ricerche in Antartide) within the main thematic focus "Chemical Contamination-Global Change". This research was devoted to detect and characterize micro and nano components with strong complexing capability towards metal ions at trace level in sea <span class="hlt">water</span>, lakes and lacustrine sediments, sampled during the XXII expedition of PNRA. In particular, in the present work, the sorption complexation capacity of an <span class="hlt">Antarctic</span> lacustrine sediments toward Cu(II) and Pb(II) is described. The characterization of the sorption was undertaken, studying kinetics and isotherm profiles. The lake here considered is Tarn Flat in the area of Terra Nova Bay. The sorption equilibria of Cu(II) and Pb(II) on the lacustrine sediments were reached in about 10 h, and they were best modelled by the Langmuir equation. Preliminary, to establish if the data here obtained were consistent with those reported for the same area in other expeditions, a common multivariate techniques, namely the principal component analysis (PCA), was applied and finally the consistency of the data has been confirmed. Copyright © 2018 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C11E..03B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C11E..03B"><span>Neoglacial <span class="hlt">Antarctic</span> sea-ice expansion driven by mid-Holocene retreat of the Ross Ice Shelf.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bendle, J. A.; Newton, K.; Mckay, R. M.; Crosta, X.; Etourneau, J.; Anya, A. B.; Seki, O.; Golledge, N. R.; Bertler, N. A. N.; Willmott, V.; Schouten, S.; Riesselman, C. R.; Masse, G.; Dunbar, R. B.</p> <p>2017-12-01</p> <p>Recent decades have seen expanding <span class="hlt">Antarctic</span> sea-ice coverage, coeval with thinning West <span class="hlt">Antarctic</span> Ice Sheet (WAIS) ice shelves and the rapid freshening of surface and bottom <span class="hlt">waters</span> along the <span class="hlt">Antarctic</span> margin. The mid-Holocene Neoglacial transition represents the last comparable baseline shift in sea-ice behaviour. The drivers and feedbacks involved in both the recent and Holocene events are poorly understood and characterised by large proxy-model mismatches. We present new records of compound specific fatty acid isotope analyses (δ2H-FA), highly-branched isoprenoid alkenes (HBIs) TEX86L temperatures, grain-size, mass accumulations rates (MARs) and image analyses from a 171m Holocene sediment sequence from Site U1357 (IODP leg 318). In combination with published records we reconstruct Holocene changes in glacial meltwater, sedimentary inputs and sea-ice. The early Holocene (11 to 10 ka) is characterised by large fluctuations in inputs of deglacial meltwater and sediments and seismic evidence of downlapping material from the south, suggesting a dominating influence from glacial retreat of the local outlet glaciers. From 10 to 8 ka there is decreasing meltwater inputs, an onlapping drift and advection of material from the east. After ca. 8 ka positively correlated δ2H-FA and MARs infer that pulses of glacial melt correlate to stronger easterly currents, driving erosion of material from upstream banks and that the Ross Ice Shelf (RIS) becomes a major influence. A large mid-Holocene meltwater pulse (preceded by warming TEX86L temperatures) is evident between ca. 6 to 4.5 ka, culminating in a rapid and permanent increase in sea-ice from 4.5 ka. This is coeval with cosmogenic nuclide evidence for a rapid thinning of the <span class="hlt">Antarctic</span> ice sheet during the mid-Holocene (Hein et al., 2016). We suggest this represents a final major pulse of deglaciation from the Ross Ice Shelf, which initiates the Neoglacial, driving cool surface <span class="hlt">waters</span> along the coast and greater sea</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A53L..01B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A53L..01B"><span>Is it Becoming Warmer and Wetter in the <span class="hlt">Antarctic</span>? A Look at Evaporation from the Southern Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Boisvert, L.; Shie, C. L.</p> <p>2017-12-01</p> <p>The process of evaporation provides <span class="hlt">water</span> vapor from the surface to the atmosphere, where it becomes the most radiatively important and abundant greenhouse gas altering the Earth's energy balance. Hence evaporation plays an essential role in a wide variety of atmospheric and oceanic problems. Evaporation is a key component of both the <span class="hlt">water</span> cycle and the surface energy balance and thus information on this process is crucial in understanding the interaction between the atmosphere and oceans, global energy and <span class="hlt">water</span> cycle variability, and in improving model simulations of climate variations. Although evaporation is an important term in climate model physics it is often poorly captured because surface in-situ measurements of evaporation are scarce in both space and time, especially over the Polar Regions, because evaporation is not easily measured directly. The <span class="hlt">Antarctic</span> sea ice acts as a barrier between the ocean and atmosphere inhibiting the exchange of heat, momentum, and moisture. However, variations in the sea ice cover could lead to changes in the amount of moisture supplied to the atmosphere. Variations in the sea ice coverage could potentially allow for larger vertical moisture fluxes that affect surface energy budgets, larger occurrences of low-level clouds, and higher near-surface humidity and temperatures. These changes to the local atmosphere could then potentially impact nearby atmospheric conditions over the <span class="hlt">Antarctic</span> ice sheet, which could be particularly important in regions that are susceptible to collapse like the West <span class="hlt">Antarctic</span> Ice Sheet. NASA's Atmospheric Infrared Sounder (AIRS) has been used in multiple studies to study sea-ice atmosphere interactions in the Arctic Ocean with great success, specifically in evaporation (i.e. the moisture flux). However, little research has been done looking at the moisture flux from the <span class="hlt">Antarctic</span> sea ice pack and nearby areas of the Southern Ocean. This work will use data from AIRS and the moisture flux scheme</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28369352','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28369352"><span>The genome of the <span class="hlt">Antarctic</span>-endemic copepod, Tigriopus kingsejongensis.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kang, Seunghyun; Ahn, Do-Hwan; Lee, Jun Hyuck; Lee, Sung Gu; Shin, Seung Chul; Lee, Jungeun; Min, Gi-Sik; Lee, Hyoungseok; Kim, Hyun-Woo; Kim, Sanghee; Park, Hyun</p> <p>2017-01-01</p> <p>The <span class="hlt">Antarctic</span> intertidal zone is continuously subjected to extremely fluctuating biotic and abiotic stressors. The West <span class="hlt">Antarctic</span> Peninsula is the most rapidly warming region on Earth. Organisms living in <span class="hlt">Antarctic</span> intertidal pools are therefore interesting for research into evolutionary adaptation to extreme environments and the effects of climate change. We report the whole genome sequence of the <span class="hlt">Antarctic</span>-endemic harpacticoid copepod Tigriopus kingsejongensi . The 37 Gb raw DNA sequence was generated using the Illumina Miseq platform. Libraries were prepared with 65-fold coverage and a total length of 295 Mb. The final assembly consists of 48 368 contigs with an N50 contig length of 17.5 kb, and 27 823 scaffolds with an N50 contig length of 159.2 kb. A total of 12 772 coding genes were inferred using the MAKER annotation pipeline. Comparative genome analysis revealed that T. kingsejongensis -specific genes are enriched in transport and metabolism processes. Furthermore, rapidly evolving genes related to energy metabolism showed positive selection signatures. The T. kingsejongensis genome provides an interesting example of an evolutionary strategy for <span class="hlt">Antarctic</span> cold adaptation, and offers new genetic insights into <span class="hlt">Antarctic</span> intertidal biota. © The Author 2017. Published by Oxford University Press.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5467011','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5467011"><span>The genome of the <span class="hlt">Antarctic</span>-endemic copepod, Tigriopus kingsejongensis</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Kang, Seunghyun; Ahn, Do-Hwan; Lee, Jun Hyuck; Lee, Sung Gu; Shin, Seung Chul; Lee, Jungeun; Min, Gi-Sik; Lee, Hyoungseok</p> <p>2017-01-01</p> <p>Abstract Background: The <span class="hlt">Antarctic</span> intertidal zone is continuously subjected to extremely fluctuating biotic and abiotic stressors. The West <span class="hlt">Antarctic</span> Peninsula is the most rapidly warming region on Earth. Organisms living in <span class="hlt">Antarctic</span> intertidal pools are therefore interesting for research into evolutionary adaptation to extreme environments and the effects of climate change. Findings: We report the whole genome sequence of the <span class="hlt">Antarctic</span>-endemic harpacticoid copepod Tigriopus kingsejongensi. The 37 Gb raw DNA sequence was generated using the Illumina Miseq platform. Libraries were prepared with 65-fold coverage and a total length of 295 Mb. The final assembly consists of 48 368 contigs with an N50 contig length of 17.5 kb, and 27 823 scaffolds with an N50 contig length of 159.2 kb. A total of 12 772 coding genes were inferred using the MAKER annotation pipeline. Comparative genome analysis revealed that T. kingsejongensis-specific genes are enriched in transport and metabolism processes. Furthermore, rapidly evolving genes related to energy metabolism showed positive selection signatures. Conclusions: The T. kingsejongensis genome provides an interesting example of an evolutionary strategy for <span class="hlt">Antarctic</span> cold adaptation, and offers new genetic insights into <span class="hlt">Antarctic</span> intertidal biota. PMID:28369352</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 ocean-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> <span class="hlt">Antarctic</span> or North Pacific <span class="hlt">Intermediate</span> <span class="hlt">Water</span> appear in the model integrations, primarily because there is no source of sufficiently dense bottom <span class="hlt">water</span> adjacent to Antarctica. Without this dense bottom <span class="hlt">water</span>, the "would-be" <span class="hlt">intermediate</span> <span class="hlt">water</span> at 60°S sinks to great depths and actually becomes the model ocean's bottom <span class="hlt">water</span>. Then, the simulated bottom <span class="hlt">water</span> is too fresh and warm in the climate model, matching the temperature—salinity signature of <span class="hlt">Antarctic</span> <span class="hlt">Intermediate</span> <span class="hlt">Water</span>. In the North Atlantic, whilst deep <span class="hlt">water</span> formation appears in one of the climate states of Manabe and Stouffer (1988), its downward penetration is not as deep as observed. This is because their deep North Atlantic is not ventilated by the thermohaline overturning of warm salty North Atlantic Deep <span class="hlt">Water</span>. Instead, a deep overturning cell centred near the equator transports relatively fresh <span class="hlt">water</span> into the region. In contrast, the location and strength of Central <span class="hlt">Water</span> formation agrees well with climatology.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.6277A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.6277A"><span>Changes in <span class="hlt">water</span> properties and flow regime on the continental shelf off the Adélie/George V Land coast, East Antarctica, after glacier tongue calving</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Aoki, S.; Kobayashi, R.; Rintoul, S. R.; Tamura, T.; Kusahara, K.</p> <p>2017-08-01</p> <p>Oceanic changes before and after the relocation of iceberg B9B and calving of the Mertz Glacier Tongue (MGT) in February 2010 are examined on the continental shelf off the Adélie Land/George V Land coast, East Antarctica. Summer hydrographic observations, including stable oxygen isotope ratio (δ18O), in 2001/2008 and 2011/2015 and results of a numerical model are used. Along the western flank of the MGT, temperature decreased between 2001 and 2015 for most of the <span class="hlt">water</span> column in the Adélie Depression. δ18O generally decreased, especially at the MGT draft depths on the northern side. West of the MGT, temperature, salinity, and δ18O decreased in the <span class="hlt">intermediate</span> layer. East of the MGT, in contrast, temperature increased between 2001 and 2011 at <span class="hlt">intermediate</span> depths, salinity increased in the <span class="hlt">intermediate</span> and deep layers, and δ18O slightly decreased in the deep layer but did not change much around 300 dbar. The numerical experiment exhibits a change in ocean circulation, revealing an increase in modified Circumpolar Deep <span class="hlt">Water</span> (mCDW) inflow in the east and a decrease in the west. The contrasting changes in mCDW intrusion are consistent between the observations and numerical model, and are indicative of the effect of removal of the ice barriers. The contrast is overlain by overall decreases in salinity and δ18O, which suggests an increase in the continental meltwater fraction of 5-20% and might reveal a wide-ranging influence from West Antarctica. The oxygen isotope ratio is, hence, effective in monitoring the increase in continental melt over the <span class="hlt">Antarctic</span> shelf.<abstract type="synopsis"><title type="main">Plain Language Summary<span class="hlt">Antarctic</span> glaciers, icebergs, and ice sheet have significant impact on the surrounding ocean, and, in turn, are affected by the ocean. The Mertz Glacier, East Antarctica, had been melted from below by the oceanic heat. The seaward extension of the glacier of about 500 m tall obstructed sea ice drift from the east and enabled a large</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25703718','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25703718"><span>A robust bioassay to assess the toxicity of metals to the <span class="hlt">Antarctic</span> marine microalga Phaeocystis antarctica.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gissi, Francesca; Adams, Merrin S; King, Catherine K; Jolley, Dianne F</p> <p>2015-07-01</p> <p>Despite evidence of contamination in <span class="hlt">Antarctic</span> coastal marine environments, no <span class="hlt">water</span>-quality guidelines have been established for the region because of a paucity of biological effects data for local <span class="hlt">Antarctic</span> species. Currently, there is limited information on the sensitivity of <span class="hlt">Antarctic</span> microalgae to metal contamination, which is exacerbated by the lack of standard toxicity testing protocols for local marine species. In the present study, a routine and robust toxicity test protocol was developed using the <span class="hlt">Antarctic</span> marine microalga Phaeocystis antarctica, and its sensitivity was investigated following 10-d exposures to dissolved copper, cadmium, lead, zinc, and nickel. In comparisons of 10% inhibition of population growth rate (IC10) values, P. antarctica was most sensitive to copper (3.3 μg/L), followed by cadmium (135 μg/L), lead (260 μg/L), and zinc (450 μg/L). Although an IC10 value for nickel could not be accurately estimated, the no-observed-effect concentration value for nickel was 1070 μg/L. Exposure to copper and cadmium caused changes in internal cell granularity and increased chlorophyll a fluorescence. Lead, zinc, and nickel had no effect on any of the cellular parameters measured. The present study provides valuable metal-ecotoxicity data for an <span class="hlt">Antarctic</span> marine microalga, with P. antarctica representing one of the most sensitive microalgal species to dissolved copper ever reported when compared with temperate and tropical species. © 2015 SETAC.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19708753','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19708753"><span>Nucleation via an unstable <span class="hlt">intermediate</span> phase.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sear, Richard P</p> <p>2009-08-21</p> <p>The pathway for crystallization from dilute vapors and solutions is often observed to take a detour via a liquid or concentrated-solution phase. For example, in moist subzero air, droplets of liquid <span class="hlt">water</span> form, which then freeze. In this example and in many others, an <span class="hlt">intermediate</span> phase (here liquid <span class="hlt">water</span>) is dramatically accelerating the kinetics of a phase transition between two other phases (<span class="hlt">water</span> vapor and ice). Here we study this phenomenon via exact computer simulations of a simple lattice model. Surprisingly, we find that the rate of nucleation of the new equilibrium phase is actually fastest when the <span class="hlt">intermediate</span> phase is slightly unstable in the bulk, i.e., has a slightly higher free energy than the phase we start in. Nucleation occurs at a concave part of the surface and microscopic amounts of the <span class="hlt">intermediate</span> phase can form there even before the phase is stable in the bulk. As the nucleus of the equilibrium phase is microscopic, this allows nucleation to occur effectively in the <span class="hlt">intermediate</span> phase before it is stable in the bulk.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA257132','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA257132"><span>Investigation of <span class="hlt">Antarctic</span> Sea Ice Concentration by Means of Selected Algorithms</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1992-05-08</p> <p>Changes in areal extent and concentration of sea ice around Antarctica may serve as sensitive indicators of global warming . A comparison study was...occurred from July, 1987 through June, 1990. <span class="hlt">Antarctic</span> Ocean, <span class="hlt">Antarctic</span> regions, Global warming , Sea ice-<span class="hlt">Antarctic</span> regions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2010-10-05/pdf/2010-24865.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2010-10-05/pdf/2010-24865.pdf"><span>75 FR 61520 - Notice of Permit Applications Received Under the <span class="hlt">Antarctic</span> Conservation Act of 1978 (Pub. L. 95-541)</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>2010-10-05</p> <p>... of marine bacteria, previously collected from <span class="hlt">Antarctic</span> <span class="hlt">waters</span>, will be used in shipboard experiments... microbes (algae and protozoa) for use in experiments, for preservation for future examination, and for...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5357866','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5357866"><span>Major advance of South Georgia glaciers during the <span class="hlt">Antarctic</span> Cold Reversal following extensive sub-<span class="hlt">Antarctic</span> glaciation</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Graham, Alastair G. C.; Kuhn, Gerhard; Meisel, Ove; Hillenbrand, Claus-Dieter; Hodgson, Dominic A.; Ehrmann, Werner; Wacker, Lukas; Wintersteller, Paul; dos Santos Ferreira, Christian; Römer, Miriam; White, Duanne; Bohrmann, Gerhard</p> <p>2017-01-01</p> <p>The history of glaciations on Southern Hemisphere sub-polar islands is unclear. Debate surrounds the extent and timing of the last glacial advance and termination on sub-<span class="hlt">Antarctic</span> South Georgia in particular. Here, using sea-floor geophysical data and marine sediment cores, we resolve the record of glaciation offshore of South Georgia through the transition from the Last Glacial Maximum to Holocene. We show a sea-bed landform imprint of a shelf-wide last glacial advance and progressive deglaciation. Renewed glacier resurgence in the fjords between c. 15,170 and 13,340 yr ago coincided with a period of cooler, wetter climate known as the <span class="hlt">Antarctic</span> Cold Reversal, revealing a cryospheric response to an <span class="hlt">Antarctic</span> climate pattern extending into the Atlantic sector of the Southern Ocean. We conclude that the last glaciation of South Georgia was extensive, and the sensitivity of its glaciers to climate variability during the last termination more significant than implied by previous studies. PMID:28303885</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15938749','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15938749"><span>Prospects for surviving climate change in <span class="hlt">Antarctic</span> aquatic species.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Peck, Lloyd S</p> <p>2005-06-06</p> <p>Maritime <span class="hlt">Antarctic</span> freshwater habitats are amongst the fastest changing environments on Earth. Temperatures have risen around 1 degrees C and ice cover has dramatically decreased in 15 years. Few animal species inhabit these sites, but the fairy shrimp Branchinecta gaini typifies those that do. This species survives up to 25 degrees C daily temperature fluctuations in summer and passes winter as eggs at temperatures down to -25 degrees C. Its annual temperature envelope is, therefore around 50 degrees C. This is typical of <span class="hlt">Antarctic</span> terrestrial species, which exhibit great physiological flexibility in coping with temperature fluctuations. The rapidly changing conditions in the Maritime <span class="hlt">Antarctic</span> are enhancing fitness in these species by increasing the time available for feeding, growth and reproduction, as well as increasing productivity in lakes. The future problem these animals face is via displacement by alien species from lower latitudes. Such invasions are now well documented from sub-<span class="hlt">Antarctic</span> sites. In contrast the marine <span class="hlt">Antarctic</span> environment has very stable temperatures. However, seasonality is intense with very short summers and long winter periods of low to no algal productivity. Marine animals grow slowly, have long generation times, low metabolic rates and low levels of activity. They also die at temperatures between +5 degrees C and +10 degrees C. Failure of oxygen supply mechanisms and loss of aerobic scope defines upper temperature limits. As temperature rises, their ability to perform work declines rapidly before lethal limits are reached, such that 50% of populations of clams and limpets cannot perform essential activities at 2-3 degrees C, and all scallops are incapable of swimming at 2 degrees C. Currently there is little evidence of temperature change in <span class="hlt">Antarctic</span> marine sites. Models predict average global sea temperatures will rise by around 2 degrees C by 2100. Such a rise would take many <span class="hlt">Antarctic</span> marine animals beyond their survival limits</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUFM.C11B0422W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFM.C11B0422W"><span><span class="hlt">Antarctic</span> sea ice thickness data archival and recovery at the Australian <span class="hlt">Antarctic</span> Data Centre</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Worby, A. P.; Treverrow, A.; Raymond, B.; Jordan, M.</p> <p>2007-12-01</p> <p>A new effort is underway to establish a portal for <span class="hlt">Antarctic</span> sea ice thickness data at the Australian <span class="hlt">Antarctic</span> Data Centre (http://aadc-maps.aad.gov.au/aadc/sitd/). The intention is to provide a central online access point for a wide range of sea ice data sets, including sea ice and snow thickness data collected using a range of techniques, and sea ice core data. The recommendation to establish this facility came from the SCAR/CliC- sponsored International Workshop on <span class="hlt">Antarctic</span> Sea Ice Thickness, held in Hobart in July 2006. It was recognised, in particular, that satellite altimetry retrievals of sea ice and snow cover thickness rely on large-scale assumptions of the sea ice and snow cover properties such as density, freeboard height, and snow stratigraphy. The synthesis of historical data is therefore particularly important for algorithm development. This will be closely coordinated with similar efforts in the Arctic. A small working group was formed to identify suitable data sets for inclusion in the archive. A series of standard proformas have been designed for converting old data, and to help standardize the collection of new data sets. These proformas are being trialled on two <span class="hlt">Antarctic</span> sea ice research cruises in September - October 2007. The web-based portal allows data custodians to remotely upload and manage their data, and for all users to search the holdings and extract data relevant to their needs. This presentation will report on the establishment of the data portal, recent progress in identifying appropriate data sets and making them available online. maps.aad.gov.au/aadc/sitd/</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1412881','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1412881"><span>Basin-scale heterogeneity in <span class="hlt">Antarctic</span> precipitation and its impact on surface mass variability</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; Lenaerts, Jan T. M.; Wang, Hailong</p> <p></p> <p>Annually averaged precipitation in the form of snow, the dominant term of the <span class="hlt">Antarctic</span> Ice Sheet surface mass balance, displays large spatial and temporal variability. Here we present an analysis of spatial patterns of regional <span class="hlt">Antarctic</span> precipitation variability and their impact on integrated <span class="hlt">Antarctic</span> surface mass balance variability simulated as part of a preindustrial 1800-year global, fully coupled Community Earth System Model simulation. Correlation and composite analyses based on this output allow for a robust exploration of <span class="hlt">Antarctic</span> precipitation variability. We identify statistically significant relationships between precipitation patterns across Antarctica that are corroborated by climate reanalyses, regional modeling and icemore » core records. These patterns are driven by variability in large-scale atmospheric moisture transport, which itself is characterized by decadal- to centennial-scale oscillations around the long-term mean. We suggest that this heterogeneity in <span class="hlt">Antarctic</span> precipitation variability has a dampening effect on overall <span class="hlt">Antarctic</span> surface mass balance variability, with implications for regulation of <span class="hlt">Antarctic</span>-sourced sea level variability, detection of an emergent anthropogenic signal in <span class="hlt">Antarctic</span> mass trends and identification of <span class="hlt">Antarctic</span> mass loss accelerations.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1412881-basin-scale-heterogeneity-antarctic-precipitation-its-impact-surface-mass-variability','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1412881-basin-scale-heterogeneity-antarctic-precipitation-its-impact-surface-mass-variability"><span>Basin-scale heterogeneity in <span class="hlt">Antarctic</span> precipitation and its impact on surface mass variability</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Fyke, Jeremy; Lenaerts, Jan T. M.; Wang, Hailong</p> <p>2017-11-15</p> <p>Annually averaged precipitation in the form of snow, the dominant term of the <span class="hlt">Antarctic</span> Ice Sheet surface mass balance, displays large spatial and temporal variability. Here we present an analysis of spatial patterns of regional <span class="hlt">Antarctic</span> precipitation variability and their impact on integrated <span class="hlt">Antarctic</span> surface mass balance variability simulated as part of a preindustrial 1800-year global, fully coupled Community Earth System Model simulation. Correlation and composite analyses based on this output allow for a robust exploration of <span class="hlt">Antarctic</span> precipitation variability. We identify statistically significant relationships between precipitation patterns across Antarctica that are corroborated by climate reanalyses, regional modeling and icemore » core records. These patterns are driven by variability in large-scale atmospheric moisture transport, which itself is characterized by decadal- to centennial-scale oscillations around the long-term mean. We suggest that this heterogeneity in <span class="hlt">Antarctic</span> precipitation variability has a dampening effect on overall <span class="hlt">Antarctic</span> surface mass balance variability, with implications for regulation of <span class="hlt">Antarctic</span>-sourced sea level variability, detection of an emergent anthropogenic signal in <span class="hlt">Antarctic</span> mass trends and identification of <span class="hlt">Antarctic</span> mass loss accelerations.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4588704','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4588704"><span>Emerging spatial patterns in <span class="hlt">Antarctic</span> prokaryotes</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Chong, Chun-Wie; Pearce, David A.; Convey, Peter</p> <p>2015-01-01</p> <p>Recent advances in knowledge of patterns of biogeography in terrestrial eukaryotic organisms have led to a fundamental paradigm shift in understanding of the controls and history of life on land in Antarctica, and its interactions over the long term with the glaciological and geological processes that have shaped the continent. However, while it has long been recognized that the terrestrial ecosystems of Antarctica are dominated by microbes and their processes, knowledge of microbial diversity and distributions has lagged far behind that of the macroscopic eukaryote organisms. Increasing human contact with and activity in the continent is leading to risks of biological contamination and change in a region whose isolation has protected it for millions of years at least; these risks may be particularly acute for microbial communities which have, as yet, received scant recognition and attention. Even a matter apparently as straightforward as Protected Area designation in Antarctica requires robust biodiversity data which, in most parts of the continent, remain almost completely unavailable. A range of important contributing factors mean that it is now timely to reconsider the state of knowledge of <span class="hlt">Antarctic</span> terrestrial prokaryotes. Rapid advances in molecular biological approaches are increasingly demonstrating that bacterial diversity in Antarctica may be far greater than previously thought, and that there is overlap in the environmental controls affecting both <span class="hlt">Antarctic</span> prokaryotic and eukaryotic communities. Bacterial dispersal mechanisms and colonization patterns remain largely unaddressed, although evidence for regional evolutionary differentiation is rapidly accruing and, with this, there is increasing appreciation of patterns in regional bacterial biogeography in this large part of the globe. In this review, we set out to describe the state of knowledge of <span class="hlt">Antarctic</span> prokaryote diversity patterns, drawing analogy with those of eukaryote groups where appropriate</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1764833','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1764833"><span>Climate change and the marine ecosystem of the western <span class="hlt">Antarctic</span> Peninsula</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Clarke, Andrew; Murphy, Eugene J; Meredith, Michael P; King, John C; Peck, Lloyd S; Barnes, David K.A; Smith, Raymond C</p> <p>2006-01-01</p> <p>The <span class="hlt">Antarctic</span> Peninsula is experiencing one of the fastest rates of regional climate change on Earth, resulting in the collapse of ice shelves, the retreat of glaciers and the exposure of new terrestrial habitat. In the nearby oceanic system, winter sea ice in the Bellingshausen and Amundsen seas has decreased in extent by 10% per decade, and shortened in seasonal duration. Surface <span class="hlt">waters</span> have warmed by more than 1 K since the 1950s, and the Circumpolar Deep <span class="hlt">Water</span> (CDW) of the <span class="hlt">Antarctic</span> Circumpolar Current has also warmed. Of the changes observed in the marine ecosystem of the western <span class="hlt">Antarctic</span> Peninsula (WAP) region to date, alterations in winter sea ice dynamics are the most likely to have had a direct impact on the marine fauna, principally through shifts in the extent and timing of habitat for ice-associated biota. Warming of seawater at depths below ca 100 m has yet to reach the levels that are biologically significant. Continued warming, or a change in the frequency of the flooding of CDW onto the WAP continental shelf may, however, induce sublethal effects that influence ecological interactions and hence food-web operation. The best evidence for recent changes in the ecosystem may come from organisms which record aspects of their population dynamics in their skeleton (such as molluscs or brachiopods) or where ecological interactions are preserved (such as in encrusting biota of hard substrata). In addition, a southwards shift of marine isotherms may induce a parallel migration of some taxa similar to that observed on land. The complexity of the Southern Ocean food web and the nonlinear nature of many interactions mean that predictions based on short-term studies of a small number of species are likely to be misleading. PMID:17405211</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/17405211','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17405211"><span>Climate change and the marine ecosystem of the western <span class="hlt">Antarctic</span> Peninsula.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Clarke, Andrew; Murphy, Eugene J; Meredith, Michael P; King, John C; Peck, Lloyd S; Barnes, David K A; Smith, Raymond C</p> <p>2007-01-29</p> <p>The <span class="hlt">Antarctic</span> Peninsula is experiencing one of the fastest rates of regional climate change on Earth, resulting in the collapse of ice shelves, the retreat of glaciers and the exposure of new terrestrial habitat. In the nearby oceanic system, winter sea ice in the Bellingshausen and Amundsen seas has decreased in extent by 10% per decade, and shortened in seasonal duration. Surface <span class="hlt">waters</span> have warmed by more than 1 K since the 1950s, and the Circumpolar Deep <span class="hlt">Water</span> (CDW) of the <span class="hlt">Antarctic</span> Circumpolar Current has also warmed. Of the changes observed in the marine ecosystem of the western <span class="hlt">Antarctic</span> Peninsula (WAP) region to date, alterations in winter sea ice dynamics are the most likely to have had a direct impact on the marine fauna, principally through shifts in the extent and timing of habitat for ice-associated biota. Warming of seawater at depths below ca 100 m has yet to reach the levels that are biologically significant. Continued warming, or a change in the frequency of the flooding of CDW onto the WAP continental shelf may, however, induce sublethal effects that influence ecological interactions and hence food-web operation. The best evidence for recent changes in the ecosystem may come from organisms which record aspects of their population dynamics in their skeleton (such as molluscs or brachiopods) or where ecological interactions are preserved (such as in encrusting biota of hard substrata). In addition, a southwards shift of marine isotherms may induce a parallel migration of some taxa similar to that observed on land. The complexity of the Southern Ocean food web and the nonlinear nature of many interactions mean that predictions based on short-term studies of a small number of species are likely to be misleading.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JGRC..121.7390P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JGRC..121.7390P"><span>Direct observations of the <span class="hlt">Antarctic</span> Slope Current transport at 113°E</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Peña-Molino, B.; McCartney, M. S.; Rintoul, S. R.</p> <p>2016-10-01</p> <p>The <span class="hlt">Antarctic</span> Slope Current (ASC), defined here as the region of westward flow along the continental slope off Antarctica, forms the southern limb of the subpolar gyres. It regulates the exchange of <span class="hlt">water</span> across the shelf break and provides a path for interbasin westward transport. Despite its significance, the ASC remains largely unobserved around most of the <span class="hlt">Antarctic</span> continent. Here we present direct velocity observations from a 17 month current meter moored array deployed across the continental slope between the 1000 and the 4200 m isobaths, in the southeastern Indian Ocean near 113°E. The observed time-mean flow consists of a surface-intensified jet associated with the <span class="hlt">Antarctic</span> Slope Front (ASF) and a broader bottom-intensified westward flow that extends out to approximately the 4000 m isobath and is strongest along the upper slope. The time-mean transport of the ASC is -29.2 Sv. Fluctuations in the transport are large, typically exceeding the mean by a factor of 2. They are mainly due to changes in the northward extent of the current over the lower slope. However, seasonal changes in the wind also drive variations in the transport of the ASF and the flow in the upper slope. Both mean and variability are largely barotropic, thus invisible to traditional geostrophic methods.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19940026114','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19940026114"><span>Dynamic constraints on CO2 uptake by an iron-fertilized <span class="hlt">Antarctic</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Peng, Tsung-Hung; Broecker, Wallace S.; Oestlund, H. G.</p> <p>1992-01-01</p> <p>The topics covered include the following: tracer distribution and dynamics in the <span class="hlt">Antarctic</span> Ocean; a model of <span class="hlt">Antarctic</span> and Non-<span class="hlt">Antarctic</span> Oceans; effects on an anthropogenically affected atmosphere; effects of seasonal iron fertilization; and implications of the South Atlantic Ventilation Experiment C-14 results.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27174849','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27174849"><span>Seasonal and spatial variabilities in the <span class="hlt">water</span> chemistry of prairie pothole wetlands influence the photoproduction of reactive <span class="hlt">intermediates</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>McCabe, Andrew J; Arnold, William A</p> <p>2016-07-01</p> <p>The hydrology and <span class="hlt">water</span> chemistry of prairie pothole wetlands vary spatially and temporally, on annual and decadal timescales. Pesticide contamination of wetlands arising from agricultural activities is a foremost concern. Photochemical reactions are important in the natural attenuation of pesticides and may be important in limiting ecological and human exposure. Little is known, however, about the variable influence of wetland <span class="hlt">water</span> chemistry on indirect photochemistry. In this study, seasonal <span class="hlt">water</span> samples were collected from seven sites throughout the prairie pothole region over three years to understand the spatiotemporal dynamics of reactive <span class="hlt">intermediate</span> photoproduction. Samples were classified by the season in which they were collected (spring, summer, or fall) and the typical hydroperiod of the wetland surface <span class="hlt">water</span> (temporary or semi-permanent). Under photostable conditions, steady-state concentrations and apparent quantum yields or quantum yield coefficients were measured for triplet excited states of dissolved organic matter, singlet oxygen, hydroxyl radical, and carbonate radical under simulated sunlight. Steady-state concentrations and quantum yields increased on average by 15% and 40% from spring to fall, respectively. Temporary wetlands had 40% higher steady-state concentrations of reactive <span class="hlt">intermediates</span> than semi-permanent wetlands, but 50% lower quantum yields. Computed quantum yields for reactive <span class="hlt">intermediate</span> formation were used to predict the indirect photochemical half-lives of seven pesticides in average temporary and semi-permanent prairie pothole wetlands. As a first approximation, the predictions agree to within two orders of magnitude of previously reported half-lives. Copyright © 2016 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP43B1348B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP43B1348B"><span>Variations of the <span class="hlt">Antarctic</span> Circumpolar Current (ACC) in the Kerguelen Sector during the Last Deglaciation : sedimentological and geochemical evidences</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bout-Roumazeilles, V.; Beny, F.; Mazaud, A.; Michel, E.; Crosta, X.; Davies, G. R.; Bory, A. J. M.</p> <p>2017-12-01</p> <p>High-resolution sedimentological and geochemical records were obtained from two sediment cores recovered by the French R/V Marion Dufresne during the INDIEN-SUD-ACC cruises near the sub-<span class="hlt">Antarctic</span> Kerguelen Islands (49°S). This area is ideal to record past oceanic and atmospheric changes in the Southern Ocean because they are currently located in the northern branch of the <span class="hlt">Antarctic</span> Circumpolar Current and under the direct influence of Southern Hemisphere Westerly wind belt. This study focuses on the last termination, with specific emphasis on the impact of severe climatic events (Heinrich Stadial 1, <span class="hlt">Antarctic</span> Cold Reversal, Younger Dryas) onto the ocean-atmospheric exchange. Results indicates that most of the sediment is derived from the Kerguelen Plateau, characterized by high smectite content. Periodically, a minor contribution of Antarctica is noticeable. In particular, illite variations suggest fast and short northward incursions of <span class="hlt">Antarctic</span> Bottom <span class="hlt">Water</span>, probably formed in the Prydz Bay during the last glaciation. Grainsize repartition combined to magnetic parameters show a southward migration of the ACC and the fronts associated from the beginning of the deglaciation, which is consistent with Southern Hemisphere climate variations. On the opposite, it highlights an asynchronous decrease of the ACC strength, with a large drop during the <span class="hlt">Antarctic</span> Cold Reversal when atmospheric CO2 increase was slowed down. Thus, at least in the studied area, the ACC strength and the <span class="hlt">Antarctic</span> Climate were not synchronous during the last deglaciation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=STS048-151-164&hterms=5S&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3D5S','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=STS048-151-164&hterms=5S&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3D5S"><span>Ross Ice Shelf, <span class="hlt">Antarctic</span> Ice and Clouds</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1991-01-01</p> <p>In this view of <span class="hlt">Antarctic</span> ice and clouds, (56.5S, 152.0W), the Ross Ice Shelf of Antarctica is almost totally clear, showing stress cracks in the ice surface caused by wind and tidal drift. Clouds on the eastern edge of the picture are associated with an <span class="hlt">Antarctic</span> cyclone. Winds stirred up these storms have been known to reach hurricane force.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28487162','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28487162"><span>Experimental evidence of chemical defence mechanisms in <span class="hlt">Antarctic</span> bryozoans.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Figuerola, Blanca; Angulo-Preckler, Carlos; Núñez-Pons, Laura; Moles, Juan; Sala-Comorera, Laura; García-Aljaro, Cristina; Blanch, Anicet R; Avila, Conxita</p> <p>2017-08-01</p> <p>Bryozoans are among the most abundant and diverse members of the <span class="hlt">Antarctic</span> benthos, however the role of bioactive metabolites in ecological interactions has been scarcely studied. To extend our knowledge about the chemical ecology of <span class="hlt">Antarctic</span> bryozoans, crude ether extracts (EE) and butanol extracts (BE) obtained from two <span class="hlt">Antarctic</span> common species (Cornucopina pectogemma and Nematoflustra flagellata), were tested for antibacterial and repellent activities. The extracts were screened for quorum quenching and antibacterial activities against four <span class="hlt">Antarctic</span> bacterial strains (Bacillus aquimaris, Micrococcus sp., Oceanobacillus sp. and Paracoccus sp.). The <span class="hlt">Antarctic</span> amphipod Cheirimedon femoratus and the sea star Odontaster validus were selected as sympatric predators to perform anti-predatory and substrate preference assays. No quorum quenching activity was detected in any of the extracts, while all EE exhibited growth inhibition towards at least one bacterium strain. Although the species were not repellent against the sea star, they caused repellence to the amphipods in both extracts, suggesting that defence activities against predation derive from both lipophilic and hydrophilic metabolites. In the substrate preference assays, one EE and one BE deriving from different specimens of the species C. pectogemma were active. This study reveals intraspecific variability of chemical defences and supports the fact that chemically mediated interactions are common in <span class="hlt">Antarctic</span> bryozoans as means of protection against fouling and predation. Copyright © 2017 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27533327','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27533327"><span>At-Sea Distribution and Prey Selection of <span class="hlt">Antarctic</span> Petrels and Commercial Krill Fisheries.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Descamps, Sébastien; Tarroux, Arnaud; Cherel, Yves; Delord, Karine; Godø, Olaf Rune; Kato, Akiko; Krafft, Bjørn A; Lorentsen, Svein-Håkon; Ropert-Coudert, Yan; Skaret, Georg; Varpe, Øystein</p> <p>2016-01-01</p> <p>Commercial fisheries may impact marine ecosystems and affect populations of predators like seabirds. In the Southern Ocean, there is an extensive fishery for <span class="hlt">Antarctic</span> krill Euphausia superba that is projected to increase further. Comparing distribution and prey selection of fishing operations versus predators is needed to predict fishery-related impacts on krill-dependent predators. In this context, it is important to consider not only predators breeding near the fishing grounds but also the ones breeding far away and that disperse during the non-breeding season where they may interact with fisheries. In this study, we first quantified the overlap between the distribution of the <span class="hlt">Antarctic</span> krill fisheries and the distribution of a krill dependent seabird, the <span class="hlt">Antarctic</span> petrel Thalassoica antarctica, during both the breeding and non-breeding season. We tracked birds from the world biggest <span class="hlt">Antarctic</span> petrel colony (Svarthamaren, Dronning Maud Land), located >1000 km from the main fishing areas, during three consecutive seasons. The overall spatial overlap between krill fisheries and <span class="hlt">Antarctic</span> petrels was limited but varied greatly among and within years, and was high in some periods during the non-breeding season. In a second step, we described the length frequency distribution of <span class="hlt">Antarctic</span> krill consumed by <span class="hlt">Antarctic</span> petrels, and compared this with results from fisheries, as well as from diet studies in other krill predators. Krill taken by <span class="hlt">Antarctic</span> petrels did not differ in size from that taken by trawls or from krill taken by most <span class="hlt">Antarctic</span> krill predators. Selectivity for specific <span class="hlt">Antarctic</span> krill stages seems generally low in <span class="hlt">Antarctic</span> predators. Overall, our results show that competition between <span class="hlt">Antarctic</span> petrels and krill fisheries is currently likely negligible. However, if krill fisheries are to increase in the future, competition with the <span class="hlt">Antarctic</span> petrel may occur, even with birds breeding thousands of kilometers away.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4988635','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4988635"><span>At-Sea Distribution and Prey Selection of <span class="hlt">Antarctic</span> Petrels and Commercial Krill Fisheries</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Descamps, Sébastien; Tarroux, Arnaud; Cherel, Yves; Delord, Karine; Godø, Olaf Rune; Kato, Akiko; Krafft, Bjørn A.; Lorentsen, Svein-Håkon; Ropert-Coudert, Yan; Skaret, Georg; Varpe, Øystein</p> <p>2016-01-01</p> <p>Commercial fisheries may impact marine ecosystems and affect populations of predators like seabirds. In the Southern Ocean, there is an extensive fishery for <span class="hlt">Antarctic</span> krill Euphausia superba that is projected to increase further. Comparing distribution and prey selection of fishing operations versus predators is needed to predict fishery-related impacts on krill-dependent predators. In this context, it is important to consider not only predators breeding near the fishing grounds but also the ones breeding far away and that disperse during the non-breeding season where they may interact with fisheries. In this study, we first quantified the overlap between the distribution of the <span class="hlt">Antarctic</span> krill fisheries and the distribution of a krill dependent seabird, the <span class="hlt">Antarctic</span> petrel Thalassoica antarctica, during both the breeding and non-breeding season. We tracked birds from the world biggest <span class="hlt">Antarctic</span> petrel colony (Svarthamaren, Dronning Maud Land), located >1000 km from the main fishing areas, during three consecutive seasons. The overall spatial overlap between krill fisheries and <span class="hlt">Antarctic</span> petrels was limited but varied greatly among and within years, and was high in some periods during the non-breeding season. In a second step, we described the length frequency distribution of <span class="hlt">Antarctic</span> krill consumed by <span class="hlt">Antarctic</span> petrels, and compared this with results from fisheries, as well as from diet studies in other krill predators. Krill taken by <span class="hlt">Antarctic</span> petrels did not differ in size from that taken by trawls or from krill taken by most <span class="hlt">Antarctic</span> krill predators. Selectivity for specific <span class="hlt">Antarctic</span> krill stages seems generally low in <span class="hlt">Antarctic</span> predators. Overall, our results show that competition between <span class="hlt">Antarctic</span> petrels and krill fisheries is currently likely negligible. However, if krill fisheries are to increase in the future, competition with the <span class="hlt">Antarctic</span> petrel may occur, even with birds breeding thousands of kilometers away. PMID:27533327</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3757972','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3757972"><span>Bone-eating worms from the <span class="hlt">Antarctic</span>: the contrasting fate of whale and wood remains on the Southern Ocean seafloor</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Glover, Adrian G.; Wiklund, Helena; Taboada, Sergio; Avila, Conxita; Cristobo, Javier; Smith, Craig R.; Kemp, Kirsty M.; Jamieson, Alan J.; Dahlgren, Thomas G.</p> <p>2013-01-01</p> <p>We report the results from the first experimental study of the fate of whale and wood remains on the <span class="hlt">Antarctic</span> seafloor. Using a baited free-vehicle lander design, we show that whale-falls in the <span class="hlt">Antarctic</span> are heavily infested by at least two new species of bone-eating worm, Osedax antarcticus sp. nov. and Osedax deceptionensis sp. nov. In stark contrast, wood remains are remarkably well preserved with the absence of typical wood-eating fauna such as the xylophagainid bivalves. The combined whale-fall and wood-fall experiment provides support to the hypothesis that the <span class="hlt">Antarctic</span> circumpolar current is a barrier to the larvae of deep-<span class="hlt">water</span> species that are broadly distributed in other ocean basins. Since humans first started exploring the <span class="hlt">Antarctic</span>, wood has been deposited on the seafloor in the form of shipwrecks and waste; our data suggest that this anthropogenic wood may be exceptionally well preserved. Alongside the new species descriptions, we conducted a comprehensive phylogenetic analyses of Osedax, suggesting the clade is most closely related to the frenulate tubeworms, not the vestimentiferans as previous reported. PMID:23945684</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26559062','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26559062"><span>Benthic Trophic Interactions in an <span class="hlt">Antarctic</span> Shallow <span class="hlt">Water</span> Ecosystem Affected by Recent Glacier Retreat.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Pasotti, Francesca; Saravia, Leonardo Ariel; De Troch, Marleen; Tarantelli, Maria Soledad; Sahade, Ricardo; Vanreusel, Ann</p> <p>2015-01-01</p> <p>The western <span class="hlt">Antarctic</span> Peninsula is experiencing strong environmental changes as a consequence of ongoing regional warming. Glaciers in the area are retreating rapidly and increased sediment-laden meltwater runoff threatens the benthic biodiversity at shallow depths. We identified three sites with a distinct glacier-retreat related history and different levels of glacial influence in the inner part of Potter Cove (King George Island, South Shetland Islands), a fjord-like embayment impacted since the 1950s by a tidewater glacier retreat. We compared the soft sediment meio- and macrofauna isotopic niche widths (δ13C and δ15N stable isotope analysis) at the three sites to investigate possible glacier retreat-related influences on benthic trophic interactions. The isotopic niches were locally shaped by the different degrees of glacier retreat-related disturbance within the Cove. Wider isotopic niche widths were found at the site that has become ice-free most recently, and narrower niches at the older ice-free sites. At an <span class="hlt">intermediate</span> state of glacier retreat-related disturbance (e.g. via ice-growler scouring) species with different strategies could settle. The site at the earliest stage of post-retreat development was characterized by an assemblage with lower trophic redundancy. Generally, the isotopic niche widths increased with increasing size spectra of organisms within the community, excepting the youngest assemblage, where the pioneer colonizer meiofauna size class displayed the highest isotopic niche width. Meiofauna at all sites generally occupied positions in the isotopic space that suggested a detrital-pool food source and/or the presence of predatory taxa. In general ice scour and glacial impact appeared to play a two-fold role within the Cove: i) either stimulating trophic diversity by allowing continuous re-colonization of meiofaunal species or, ii) over time driving the benthic assemblages into a more compact trophic structure with increased</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4641631','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4641631"><span>Benthic Trophic Interactions in an <span class="hlt">Antarctic</span> Shallow <span class="hlt">Water</span> Ecosystem Affected by Recent Glacier Retreat</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Pasotti, Francesca; Saravia, Leonardo Ariel; De Troch, Marleen; Tarantelli, Maria Soledad; Sahade, Ricardo; Vanreusel, Ann</p> <p>2015-01-01</p> <p>The western <span class="hlt">Antarctic</span> Peninsula is experiencing strong environmental changes as a consequence of ongoing regional warming. Glaciers in the area are retreating rapidly and increased sediment-laden meltwater runoff threatens the benthic biodiversity at shallow depths. We identified three sites with a distinct glacier-retreat related history and different levels of glacial influence in the inner part of Potter Cove (King George Island, South Shetland Islands), a fjord-like embayment impacted since the 1950s by a tidewater glacier retreat. We compared the soft sediment meio- and macrofauna isotopic niche widths (δ13C and δ15N stable isotope analysis) at the three sites to investigate possible glacier retreat-related influences on benthic trophic interactions. The isotopic niches were locally shaped by the different degrees of glacier retreat-related disturbance within the Cove. Wider isotopic niche widths were found at the site that has become ice-free most recently, and narrower niches at the older ice-free sites. At an <span class="hlt">intermediate</span> state of glacier retreat-related disturbance (e.g. via ice-growler scouring) species with different strategies could settle. The site at the earliest stage of post-retreat development was characterized by an assemblage with lower trophic redundancy. Generally, the isotopic niche widths increased with increasing size spectra of organisms within the community, excepting the youngest assemblage, where the pioneer colonizer meiofauna size class displayed the highest isotopic niche width. Meiofauna at all sites generally occupied positions in the isotopic space that suggested a detrital-pool food source and/or the presence of predatory taxa. In general ice scour and glacial impact appeared to play a two-fold role within the Cove: i) either stimulating trophic diversity by allowing continuous re-colonization of meiofaunal species or, ii) over time driving the benthic assemblages into a more compact trophic structure with increased</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5865725','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5865725"><span>Time- and depth-wise trophic niche shifts in <span class="hlt">Antarctic</span> benthos</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Calizza, Edoardo; Careddu, Giulio; Sporta Caputi, Simona; Costantini, Maria Letizia</p> <p>2018-01-01</p> <p>Climate change is expected to affect resource-consumer interactions underlying stability in polar food webs. Polar benthic organisms have adapted to the marked seasonality characterising their habitats by concentrating foraging and reproductive activity in summer months, when inputs from sympagic and pelagic producers increase. While this enables the persistence of biodiverse food webs, the mechanisms underlying changes in resource use and nutrient transfer are poorly understood. Thus, our understanding of how temporal and spatial variations in the supply of resources may affect food web structure and functioning is limited. By means of C and N isotopic analyses of two key <span class="hlt">Antarctic</span> benthic consumers (Adamussium colbecki, Bivalvia, and Sterechinus neumayeri, Echinoidea) and Bayesian mixing models, we describe changes in trophic niche and nutrient transfer across trophic levels associated with the long- and short-term diet and body size of specimens sampled in midsummer in both shallow and deep <span class="hlt">waters</span>. Samplings occurred soon after the sea-ice broke up at Tethys Bay, an area characterised by extreme seasonality in sea-ice coverage and productivity in the Ross Sea. In the long term, the trophic niche was broader and variation between specimens was greater, with <span class="hlt">intermediate</span>-size specimens generally consuming a higher number of resources than small and large specimens. The coupling of energy channels in the food web was consequently more direct than in the short term. Sediment and benthic algae were more frequently consumed in the long term, before the sea-ice broke up, while consumers specialised on sympagic algae and plankton in the short term. Regardless of the time scale, sympagic algae were more frequently consumed in shallow <span class="hlt">waters</span>, while plankton was more frequently consumed in deep <span class="hlt">waters</span>. Our results suggest a strong temporal relationship between resource availability and the trophic niche of benthic consumers in Antarctica. Potential climate-driven changes</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29570741','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29570741"><span>Time- and depth-wise trophic niche shifts in <span class="hlt">Antarctic</span> benthos.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Calizza, Edoardo; Careddu, Giulio; Sporta Caputi, Simona; Rossi, Loreto; Costantini, Maria Letizia</p> <p>2018-01-01</p> <p>Climate change is expected to affect resource-consumer interactions underlying stability in polar food webs. Polar benthic organisms have adapted to the marked seasonality characterising their habitats by concentrating foraging and reproductive activity in summer months, when inputs from sympagic and pelagic producers increase. While this enables the persistence of biodiverse food webs, the mechanisms underlying changes in resource use and nutrient transfer are poorly understood. Thus, our understanding of how temporal and spatial variations in the supply of resources may affect food web structure and functioning is limited. By means of C and N isotopic analyses of two key <span class="hlt">Antarctic</span> benthic consumers (Adamussium colbecki, Bivalvia, and Sterechinus neumayeri, Echinoidea) and Bayesian mixing models, we describe changes in trophic niche and nutrient transfer across trophic levels associated with the long- and short-term diet and body size of specimens sampled in midsummer in both shallow and deep <span class="hlt">waters</span>. Samplings occurred soon after the sea-ice broke up at Tethys Bay, an area characterised by extreme seasonality in sea-ice coverage and productivity in the Ross Sea. In the long term, the trophic niche was broader and variation between specimens was greater, with <span class="hlt">intermediate</span>-size specimens generally consuming a higher number of resources than small and large specimens. The coupling of energy channels in the food web was consequently more direct than in the short term. Sediment and benthic algae were more frequently consumed in the long term, before the sea-ice broke up, while consumers specialised on sympagic algae and plankton in the short term. Regardless of the time scale, sympagic algae were more frequently consumed in shallow <span class="hlt">waters</span>, while plankton was more frequently consumed in deep <span class="hlt">waters</span>. Our results suggest a strong temporal relationship between resource availability and the trophic niche of benthic consumers in Antarctica. Potential climate-driven changes</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3298955','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3298955"><span>Possible effects of global environmental changes on <span class="hlt">Antarctic</span> benthos: a synthesis across five major taxa</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Ingels, Jeroen; Vanreusel, Ann; Brandt, Angelika; Catarino, Ana I; David, Bruno; De Ridder, Chantal; Dubois, Philippe; Gooday, Andrew J; Martin, Patrick; Pasotti, Francesca; Robert, Henri</p> <p>2012-01-01</p> <p>Because of the unique conditions that exist around the <span class="hlt">Antarctic</span> continent, Southern Ocean (SO) ecosystems are very susceptible to the growing impact of global climate change and other anthropogenic influences. Consequently, there is an urgent need to understand how SO marine life will cope with expected future changes in the environment. Studies of <span class="hlt">Antarctic</span> organisms have shown that individual species and higher taxa display different degrees of sensitivity to environmental shifts, making it difficult to predict overall community or ecosystem responses. This emphasizes the need for an improved understanding of the <span class="hlt">Antarctic</span> benthic ecosystem response to global climate change using a multitaxon approach with consideration of different levels of biological organization. Here, we provide a synthesis of the ability of five important <span class="hlt">Antarctic</span> benthic taxa (Foraminifera, Nematoda, Amphipoda, Isopoda, and Echinoidea) to cope with changes in the environment (temperature, pH, ice cover, ice scouring, food quantity, and quality) that are linked to climatic changes. Responses from individual to the taxon-specific community level to these drivers will vary with taxon but will include local species extinctions, invasions of warmer-<span class="hlt">water</span> species, shifts in diversity, dominance, and trophic group composition, all with likely consequences for ecosystem functioning. Limitations in our current knowledge and understanding of climate change effects on the different levels are discussed. PMID:22423336</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2011-08-08/pdf/2011-20001.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2011-08-08/pdf/2011-20001.pdf"><span>76 FR 48182 - Notice of Permit Application Received Under the <span class="hlt">Antarctic</span> Conservation Act of 1978</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>2011-08-08</p> <p>.... Designated pollutants would be associated with camp operations [typically air emissions and waste <span class="hlt">water</span>... (NSF) has received a waste management permit application for operation of a field research camp located...: NSF's <span class="hlt">Antarctic</span> Waste Regulation, 45 CFR part 671, requires all U.S. citizens and entities to obtain a...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4023264','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4023264"><span><span class="hlt">Antarctic</span> Porifera database from the Spanish benthic expeditions</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Rios, Pilar; Cristobo, Javier</p> <p>2014-01-01</p> <p>Abstract The information about the sponges in this dataset is derived from the samples collected during five Spanish <span class="hlt">Antarctic</span> expeditions: Bentart 94, Bentart 95, Gebrap 96, Ciemar 99/00 and Bentart 2003. Samples were collected in the <span class="hlt">Antarctic</span> Peninsula and Bellingshausen Sea at depths ranging from 4 to 2044 m using various sampling gears. The <span class="hlt">Antarctic</span> Porifera database from the Spanish benthic expeditions is unique as it provides information for an under-explored region of the Southern Ocean (Bellingshausen Sea). It fills an information gap on <span class="hlt">Antarctic</span> deep-sea sponges, for which there were previously very few data. This phylum is an important part of the <span class="hlt">Antarctic</span> biota and plays a key role in the structure of the <span class="hlt">Antarctic</span> marine benthic community due to its considerable diversity and predominance in different areas. It is often a dominant component of Southern Ocean benthic communities. The quality of the data was controlled very thoroughly with GPS systems onboard the R/V Hesperides and by checking the data against the World Porifera Database (which is part of the World Register of Marine Species, WoRMS). The data are therefore fit for completing checklists, inclusion in biodiversity pattern analysis and niche modelling. The authors can be contacted if any additional information is needed before carrying out detailed biodiversity or biogeographic studies. The dataset currently contains 767 occurrence data items that have been checked for systematic reliability. This database is not yet complete and the collection is growing. Specimens are stored in the author’s collection at the Spanish Institute of Oceanography (IEO) in the city of Gijón (Spain). The data are available in GBIF. PMID:24843257</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PolSc..16...68K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PolSc..16...68K"><span>Hydrogeological characteristics of aquifer near Arctowski Polish <span class="hlt">Antarctic</span> Station on King George Island (South Shetland Islands), Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Krogulec, Ewa; Krogulec, Tomasz; Małecki, Jerzy; Pietrzykowski, Paweł; Dobak, Paweł</p> <p>2018-06-01</p> <p>During the <span class="hlt">Antarctic</span> summer season of 2015/2016, the groundwater studies were performed in the area of Henryk Arctowski Polish <span class="hlt">Antarctic</span> Station on King George Island (South Shetland Islands) in Admiralty Bay of Antarctica. Rock and groundwater samples were collected from 14 research excavations down to a depth of 0.8-2.5 m b.g.l. Analyses of surface <span class="hlt">waters</span> were performed on <span class="hlt">water</span> samples from streams, mossland, and a drinking <span class="hlt">water</span> reservoir. The scope of hydrochemical studies comprised analyses of temperature, pH, mineralization, phosphates, nitrates, macroelements and selected microelements. Using empirical formulas, granulometric analysis of rock samples from various depths, measurements of sample moisture, and calculations of the hydraulic conductivity were performed. The groundwater is poorly mineralized, representing chloride-sulfate-bicarbonate-sodium and chloride-bicarbonate-sodium-calcium types. Studies on hydrochemical indicators show a small range of the effect of animal ecosystems on the <span class="hlt">waters</span>; no effects of organic matter have been identified in the study area. Results of hydrogeochemical studies of <span class="hlt">waters</span> and observations of groundwater levels in the summer season indicate groundwater recharge in a shallow groundwater circulation system, lateral inflow direction from land toward the seashore, and a low rate of rainwater infiltration. Groundwater drainage occurs through evapotranspiration and <span class="hlt">water</span> runoff to the sea.</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 Ocean</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 Ocean. 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 <span class="hlt">Antarctic</span> <span class="hlt">Intermediate</span> <span class="hlt">Water</span>, the Indonesian Subsurface <span class="hlt">Water</span>, the Indonesian <span class="hlt">Intermediate</span> <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 Ocean <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/2014AGUFMED53A3462B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMED53A3462B"><span>Joint <span class="hlt">Antarctic</span> School Expedition - An International Collaboration for High School Students and Teachers on <span class="hlt">Antarctic</span> Science</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Botella, J.; Warburton, J.; Bartholow, S.; Reed, L. F.</p> <p>2014-12-01</p> <p>The Joint <span class="hlt">Antarctic</span> School Expedition (JASE) is an international collaboration program between high school students and teachers from the United States and Chile aimed at providing the skills required for establishing the scientific international collaborations that our globalized world demands, and to develop a new approach for science education. The National <span class="hlt">Antarctic</span> Programs of Chile and the United States worked together on a pilot program that brought high school students and teachers from both countries to Punta Arenas, Chile, in February 2014. The goals of this project included strengthening the partnership between the two countries, and building relationships between future generations of scientists, while developing the students' awareness of global scientific issues and expanding their knowledge and interest in Antarctica and polar science. A big component of the project involved the sharing by students of the acquired knowledge and experiences with the general public. JASE is based on the successful Chilean <span class="hlt">Antarctic</span> Science Fair developed by Chile´s <span class="hlt">Antarctic</span> Research Institute. For 10 years, small groups of Chilean students, each mentored by a teacher, perform experimental or bibliographical <span class="hlt">Antarctic</span> research. Winning teams are awarded an expedition to the Chilean research station on King George Island. In 2014, the Chileans invited US participation in this program in order to strengthen science ties for upcoming generations. On King George Island, students have hands-on experiences conducting experiments and learning about field research. While the total number of students directly involved in the program is relatively small, the sharing of the experience by students with the general public is a novel approach to science education. Research experiences for students, like JASE, are important as they influence new direction for students in science learning, science interest, and help increase science knowledge. We will share experiences with 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_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.ncbi.nlm.nih.gov/pubmed/26842369','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26842369"><span>Different adaptations of Chinese winter-over expeditioners during prolonged <span class="hlt">Antarctic</span> and sub-<span class="hlt">Antarctic</span> residence.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chen, Nan; Wu, Quan; Li, Hao; Zhang, Tao; Xu, Chengli</p> <p>2016-05-01</p> <p>Prolonged residence in Antarctica is characterized by exposure to isolated, confined, and extreme (ICE) environment. Winter-over expeditioners at research stations often exhibit a complex of psychophysiological symptoms, which varied by stations and sociocultural backgrounds. To understand the different patterns of psychophysiological responses provoked by environmental stress, we conducted a longitudinal assessment of mood and endocrine function in two groups of Chinese expeditioners who were deployed to sub-<span class="hlt">Antarctic</span> (Great Wall Station, 62°S, N = 12) and <span class="hlt">Antarctic</span> (Zhongshan Station, 66°S, N = 16) from December 2003 to 2005. Measures of mood, thyroid function, the levels of plasma catecholamine, and circulating interleukins were obtained at departure from China, mid-winter (Antarctica), end of winter (Antarctica), and return to China, respectively. The Zhongshan Station crew experienced significant increases in fatigue, anger, tension, confusion, and decrease in free thyroxine (FT4), norepinephrine (NE), and epinephrine (E) during the winter, increase in thyrotropin (TSH) and total triiodothyronine (TT3) when returning, whereas their counterparts at Great Wall Station only experienced increased TT3 after deployment. Moreover, compared with the Great Wall Station crew, the Zhongshan Station crew exhibited greater increase in anger, greater decrease in FT4, total thyroxine (TT4), NE and E over the winter, and greater increase in TSH when returning. Chinese expeditioners who lived and worked at the <span class="hlt">Antarctic</span> station and the sub-<span class="hlt">Antarctic</span> station for over a year showed different change patterns in mood and endocrine hormones. Negative mood and endocrine dysfunction were positively associated with the severity of environment. The study is a supplement to scientific knowledge on psychophysiological variation under ICE environment, which has certain applied value for the development of preventive countermeasures or interventions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016IJBm...60..737C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016IJBm...60..737C"><span>Different adaptations of Chinese winter-over expeditioners during prolonged <span class="hlt">Antarctic</span> and sub-<span class="hlt">Antarctic</span> residence</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, Nan; Wu, Quan; Li, Hao; Zhang, Tao; Xu, Chengli</p> <p>2016-05-01</p> <p>Prolonged residence in Antarctica is characterized by exposure to isolated, confined, and extreme (ICE) environment. Winter-over expeditioners at research stations often exhibit a complex of psychophysiological symptoms, which varied by stations and sociocultural backgrounds. To understand the different patterns of psychophysiological responses provoked by environmental stress, we conducted a longitudinal assessment of mood and endocrine function in two groups of Chinese expeditioners who were deployed to sub-<span class="hlt">Antarctic</span> (Great Wall Station, 62°S, N = 12) and <span class="hlt">Antarctic</span> (Zhongshan Station, 66°S, N = 16) from December 2003 to 2005. Measures of mood, thyroid function, the levels of plasma catecholamine, and circulating interleukins were obtained at departure from China, mid-winter (Antarctica), end of winter (Antarctica), and return to China, respectively. The Zhongshan Station crew experienced significant increases in fatigue, anger, tension, confusion, and decrease in free thyroxine (FT4), norepinephrine (NE), and epinephrine (E) during the winter, increase in thyrotropin (TSH) and total triiodothyronine (TT3) when returning, whereas their counterparts at Great Wall Station only experienced increased TT3 after deployment. Moreover, compared with the Great Wall Station crew, the Zhongshan Station crew exhibited greater increase in anger, greater decrease in FT4, total thyroxine (TT4), NE and E over the winter, and greater increase in TSH when returning. Chinese expeditioners who lived and worked at the <span class="hlt">Antarctic</span> station and the sub-<span class="hlt">Antarctic</span> station for over a year showed different change patterns in mood and endocrine hormones. Negative mood and endocrine dysfunction were positively associated with the severity of environment. The study is a supplement to scientific knowledge on psychophysiological variation under ICE environment, which has certain applied value for the development of preventive countermeasures or interventions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS31A1999K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS31A1999K"><span>Possibility of AABW source originating from meddle size polynyas along the coast of Australian-<span class="hlt">Antarctic</span> Basin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kitade, Y.; Keishi, S.; Yuki, O.; Aoki, S.; Kobayashi, T.; Suga, T.; Ohshima, K. I.</p> <p>2016-12-01</p> <p><span class="hlt">Antarctic</span> Bottom <span class="hlt">Water</span> (AABW) is the densest <span class="hlt">water</span> in the ocean and globally significant; its production at the <span class="hlt">Antarctic</span> margin is a key component of the global overturning circulation [eg. Marshall and Speer, 2012]. AABW originating from a middle size polynya called Vincennes Bay Polynya (VBP) was discovered recently [Kitade et al., 2014]. The fact that a middle size polynya can be a formation site of AABW suggests the possibility that the unknown formation area further exists along the coast of Australian-<span class="hlt">Antarctic</span> Basin. A deep profiling float, called "Deep NINJA" which is able to observe temperature and salinity at depths up to 4,000 m, was developed by Japan Agency for Marine-Earth Science and Technology and Tsurumi-Seiki Co. [Kobayashi et al., 2015]. Five deep floats were deployed along 110oE in Jan. 2014. One of them drifted west almost along the continental rise and has been observing 40 profiles within two years. However, no signal of newly formed AABW has been observed except in the region off VBP, which is consistent with the BROKE results [eg. Bindoff et al., 2000) and our analysis result of BROKE data. Although these observations do not completely negate the additional formation of AABW originating from middle size polynyas located west of VBP, their formation volume of AABW is suggested to be much smaller than that from VBP.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18..693S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18..693S"><span>Development of source specific diatom lipids biomarkers as <span class="hlt">Antarctic</span> Sea Ice proxies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Smik, Lukas; Belt, Simon T.; Brown, Thomas A.; Lieser, Jan L.; Armand, Leanne K.; Leventer, Amy; Allen, Claire S.</p> <p>2016-04-01</p> <p>C25 highly branched isoprenoid (HBI) are lipid biomarkers biosynthesised by a relatively small number of diatom genera, but are, nonetheless, common constituents of global marine sediments. The occurrence and variable abundance of certain C25 highly branched isoprenoid (HBI) biomarkers in <span class="hlt">Antarctic</span> marine sediments has previously been proposed as a proxy measure of paleo sea-ice extent in the Southern Ocean and a small number of paleo sea-ice reconstructions based on the variable abundances of these HBIs have appeared in recent years. However, the development of HBIs as proxies for <span class="hlt">Antarctic</span> sea ice is much less advanced than that for IP25 (another HBI) in the Arctic and has been based on relatively small number of analyses in sea ice, <span class="hlt">water</span> column and sediment samples. To provide further insights into the use of these HBIs as proxies for <span class="hlt">Antarctic</span> sea ice, we here describe an assessment of their distributions in surface <span class="hlt">water</span>, surface sediment and sea ice samples collected from a number of <span class="hlt">Antarctic</span> locations experiencing contrasting sea ice conditions in recent years. Our study shows that distributions of a di-unsaturated HBI (diene II) and tri-unsaturated HBI (triene III) in surface <span class="hlt">water</span> samples were found to be extremely sensitive to the local sea-ice conditions, with diene II detected for sampling sites that experienced seasonal sea ice and highest concentrations found in coastal locations with longer-lasting ice cover and a recurrent polynya. In contrast, triene III was observed in all of the samples analysed, but with highest concentrations within the region of the retreating sea ice edge, an observation consistent with significant environmental control over the biosynthesis of diene II and triene III by sea ice diatoms and open <span class="hlt">water</span> phytoplankton, respectively. However, additional local factors, such as those associated with polynya formation, may also exert some control over the distribution of triene III and the relative concentrations of diene II and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20020047116&hterms=quality+life&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dquality%2Blife','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20020047116&hterms=quality+life&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dquality%2Blife"><span>The Controlled Ecological Life Support System <span class="hlt">Antarctic</span> Analog Project: Prototype Crop Production and <span class="hlt">Water</span> Treatment System Performance</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bubenheim, David L.; Flynn, Michael T.; Bates, Maynard; Schlick, Greg; Kliss, Mark (Technical Monitor)</p> <p>1997-01-01</p> <p>The Controlled Ecological Life Support System (CELSS) <span class="hlt">Antarctic</span> Analog Project (CAAP), is a joint endeavor between the National Science Foundation, Office of Polar Programs (NSF-OPP) and the NASA. The fundamental objective is to develop, deploy, and operate a testbed of advanced life support technologies at the Amundsen-Scott South Pole Station that enable the objectives of both the NSF and NASA. The functions of food production, <span class="hlt">water</span> purification, and waste treatment, recycle and reduction provided by CAAP will improve the quality of life for the South Pole inhabitants, reduce logistics dependence, enhance safety and minimize environmental impacts associated with human presence on the polar plateau. Because of the analogous technical, scientific, and mission features with Planetary missions such as a mission to Mars, CAAP provides NASA with a method for validating technologies and overall approaches to supporting humans. Prototype systems for sewage treatment, <span class="hlt">water</span> recycle and crop production are being evaluated at Ames Research Center. The product <span class="hlt">water</span> from sewage treatment using a Wiped-Film Rotating Disk is suitable for input to the crop production system. The crop production system has provided an enhanced level of performance compared with projected performance for plant-based life support: an approximate 50% increase in productivity per unit area, more than a 65% decrease in power for plant lighting, and more than a 75% decrease in the total power requirement to produce an equivalent mass of edible biomass.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018QSRv..192...59K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018QSRv..192...59K"><span>Holocene paleoceanography of Bigo Bay, west <span class="hlt">Antarctic</span> Peninsula: Connections between surface <span class="hlt">water</span> productivity and nutrient utilization and its implication for surface-deep <span class="hlt">water</span> mass exchange</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kim, Sunghan; Yoo, Kyu-Cheul; Lee, Jae Il; Khim, Boo-Keun; Bak, Young-Suk; Lee, Min Kyung; Lee, Jongmin; Domack, Eugene W.; Christ, Andrew J.; Yoon, Ho Il</p> <p>2018-07-01</p> <p>Paleoceanographic changes in response to Holocene climate variability in Bigo Bay, west <span class="hlt">Antarctic</span> Peninsula (WAP) were reconstructed through geochemical, isotopic, sedimentological, and microfossil analysis. Core WAP13-GC47 is composed of 4 lithologic units. Unit 4 was deposited under ice shelf settings. Unit 3 represents the mid-Holocene open marine conditions. Unit 2 indicates lateral sediment transport by a glacier advance during the Neoglacial period. The chronological contrast between the timing of open marine conditions at core WAP13-GC47 (ca. 7060 cal. yr BP at 540 cm) and the ages of calcareous shell fragments (ca. 8500 cal. yr BP) in Unit 2b suggests sediment reworking during the Neoglacial period. Unit 1 was deposited during the Medieval Warm Period (MWP) and the Little Ice Age (LIA). Surface <span class="hlt">water</span> productivity, represented by biogenic opal and total organic carbon (TOC) concentrations, increased and bulk δ15N (nitrate utilization) decreased during the warmer early to middle Holocene and the MWP. In contrast, surface <span class="hlt">water</span> productivity decreased with increased bulk δ15N during the colder Neoglacial period and LIA in Bigo Bay. The nitrate utilization was enhanced during cold periods in association with strong surface <span class="hlt">water</span> stratification resulting from increased sea ice meltwater discharge or proximity to an ice shelf calving front in Bigo Bay. Reduced nitrate utilization during warm periods is related to weak stratification induced by less sea ice meltwater input and stronger Circumpolar Deep <span class="hlt">Water</span> influence.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1988RvGeo..26...89S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1988RvGeo..26...89S"><span><span class="hlt">Antarctic</span> aerosols - A review</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shaw, Glenn E.</p> <p>1988-02-01</p> <p>Tropospheric aerosols with the diameter range of half a micron reside in the atmosphere for tens of days and teleconnect Antarctica with other regions by transport that reaches planetary scales of distances; thus, the aerosol on the <span class="hlt">Antarctic</span> ice represents 'memory modules' of events that took place at regions separated from Antarctica by tens of thousands of kilometers. In terms of aerosol mass, the aerosol species include insoluble crustal products (less than 5 percent), transported sea-salt residues (highly variable but averaging about 10 percent), Ni-rich meteoric material, and anomalously enriched material with an unknown origin. Most (70-90 percent by mass) of the aerosol over the <span class="hlt">Antarctic</span> ice shield, however, is the 'natural acid sulfate aerosol', apparently deriving from biological processes taking place in the surrounding oceans.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19810053550&hterms=water+cycle&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dwater%2Bcycle','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19810053550&hterms=water+cycle&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dwater%2Bcycle"><span>The Mars <span class="hlt">water</span> cycle</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Davies, D. W.</p> <p>1981-01-01</p> <p>A model has been developed to test the hypothesis that the observed seasonal and latitudinal distribution of <span class="hlt">water</span> on Mars is controlled by the sublimation and condensation of surface ice deposits in the Arctic and <span class="hlt">Antarctic</span>, and the meridional transport of <span class="hlt">water</span> vapor. Besides reproducing the observed <span class="hlt">water</span> vapor distribution, the model correctly reproduces the presence of a large permanent ice cap in the Arctic and not in the <span class="hlt">Antarctic</span>. No permanent ice reservoirs are predicted in the temperate or equatorial zones. Wintertime ice deposits in the Arctic are shown to be the source of the large <span class="hlt">water</span> vapor abundances observed in the Arctic summertime, and the moderate <span class="hlt">water</span> vapor abundances in the northern temperate region. Model calculations suggest that a year without dust storms results in very little change in the <span class="hlt">water</span> vapor distribution. The current <span class="hlt">water</span> distribution appears to be the equilibrium distribution for present atmospheric conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015GeoRL..42.4862S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015GeoRL..42.4862S"><span>Influence of West <span class="hlt">Antarctic</span> Ice Sheet collapse on <span class="hlt">Antarctic</span> surface climate</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Steig, Eric J.; Huybers, Kathleen; Singh, Hansi A.; Steiger, Nathan J.; Ding, Qinghua; Frierson, Dargan M. W.; Popp, Trevor; White, James W. C.</p> <p>2015-06-01</p> <p>Climate model simulations are used to examine the impact of a collapse of the West <span class="hlt">Antarctic</span> Ice Sheet (WAIS) on the surface climate of Antarctica. The lowered topography following WAIS collapse produces anomalous cyclonic circulation with increased flow of warm, maritime air toward the South Pole and cold-air advection from the East <span class="hlt">Antarctic</span> plateau toward the Ross Sea and Marie Byrd Land, West Antarctica. Relative to the background climate, areas in East Antarctica that are adjacent to the WAIS warm, while substantial cooling (several °C) occurs over parts of West Antarctica. Anomalously low isotope-paleotemperature values at Mount Moulton, West Antarctica, compared with ice core records in East Antarctica, are consistent with collapse of the WAIS during the last interglacial period, Marine Isotope Stage 5e. More definitive evidence might be recoverable from an ice core record at Hercules Dome, East Antarctica, which would experience significant warming and positive oxygen isotope anomalies if the WAIS collapsed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29760112','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29760112"><span>Macronutrient and carbon supply, uptake and cycling across the <span class="hlt">Antarctic</span> Peninsula shelf during summer.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Henley, Sian F; Jones, Elizabeth M; Venables, Hugh J; Meredith, Michael P; Firing, Yvonne L; Dittrich, Ribanna; Heiser, Sabrina; Stefels, Jacqueline; Dougans, Julie</p> <p>2018-06-28</p> <p>The West <span class="hlt">Antarctic</span> Peninsula shelf is a region of high seasonal primary production which supports a large and productive food web, where macronutrients and inorganic carbon are sourced primarily from intrusions of warm saline Circumpolar Deep <span class="hlt">Water</span>. We examined the cross-shelf modification of this <span class="hlt">water</span> mass during mid-summer 2015 to understand the supply of nutrients and carbon to the productive surface ocean, and their subsequent uptake and cycling. We show that nitrate, phosphate, silicic acid and inorganic carbon are progressively enriched in subsurface <span class="hlt">waters</span> across the shelf, contrary to cross-shelf reductions in heat, salinity and density. We use nutrient stoichiometric and isotopic approaches to invoke remineralization of organic matter, including nitrification below the euphotic surface layer, and dissolution of biogenic silica in deeper <span class="hlt">waters</span> and potentially shelf sediment porewaters, as the primary drivers of cross-shelf enrichments. Regenerated nitrate and phosphate account for a significant proportion of the total pools of these nutrients in the upper ocean, with implications for the seasonal carbon sink. Understanding nutrient and carbon dynamics in this region now will inform predictions of future biogeochemical changes in the context of substantial variability and ongoing changes in the physical environment.This article is part of the theme issue 'The marine system of the West <span class="hlt">Antarctic</span> Peninsula: status and strategy for progress in a region of rapid change'. © 2018 The Authors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5954468','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5954468"><span>Macronutrient and carbon supply, uptake and cycling across the <span class="hlt">Antarctic</span> Peninsula shelf during summer</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Jones, Elizabeth M.; Venables, Hugh J.; Firing, Yvonne L.; Dittrich, Ribanna; Heiser, Sabrina; Dougans, Julie</p> <p>2018-01-01</p> <p>The West <span class="hlt">Antarctic</span> Peninsula shelf is a region of high seasonal primary production which supports a large and productive food web, where macronutrients and inorganic carbon are sourced primarily from intrusions of warm saline Circumpolar Deep <span class="hlt">Water</span>. We examined the cross-shelf modification of this <span class="hlt">water</span> mass during mid-summer 2015 to understand the supply of nutrients and carbon to the productive surface ocean, and their subsequent uptake and cycling. We show that nitrate, phosphate, silicic acid and inorganic carbon are progressively enriched in subsurface <span class="hlt">waters</span> across the shelf, contrary to cross-shelf reductions in heat, salinity and density. We use nutrient stoichiometric and isotopic approaches to invoke remineralization of organic matter, including nitrification below the euphotic surface layer, and dissolution of biogenic silica in deeper <span class="hlt">waters</span> and potentially shelf sediment porewaters, as the primary drivers of cross-shelf enrichments. Regenerated nitrate and phosphate account for a significant proportion of the total pools of these nutrients in the upper ocean, with implications for the seasonal carbon sink. Understanding nutrient and carbon dynamics in this region now will inform predictions of future biogeochemical changes in the context of substantial variability and ongoing changes in the physical environment. This article is part of the theme issue ‘The marine system of the West <span class="hlt">Antarctic</span> Peninsula: status and strategy for progress in a region of rapid change’. PMID:29760112</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/31462','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/31462"><span>Potentiometric surfaces of the <span class="hlt">intermediate</span> aquifer system, west-central Florida, September 2000</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Duerr, A.D.</p> <p>2001-01-01</p> <p>The <span class="hlt">intermediate</span> aquifer system underlies a 5,000-square-mile area within the Southwest Florida <span class="hlt">Water</span> Management District including De Soto, Sarasota, Hardee, Manatee, and parts of Charlotte, Hillsborough, Highlands, Polk, and Lee Counties.  The <span class="hlt">intermediate</span> aquifer system is overlain by the surficial aquifer system and is underlain by the Floridan aquifer system.  The <span class="hlt">intermediate</span> aquifer system consists of layers of sand, shell, clay, calcareous clay, limestone, and dolomite of the Tamiami Formation and Hawthorn Group of Oligocene to Pleistocene age (Wingard and others, 1995).  The <span class="hlt">intermediate</span> aquifer system contains one or more <span class="hlt">water</span>-bearing units separated by discontinuous confining units.  The <span class="hlt">intermediate</span> aquifer system is the principal source of potable <span class="hlt">water</span> in the southwestern part of the study area and is widely used as a source of <span class="hlt">water</span> where wells are open to the <span class="hlt">intermediate</span> aquifer system or to both the <span class="hlt">intermediate</span> and Floridan aquifer systems.  Yields of individual wells open to the <span class="hlt">intermediate</span> aquifer system vary from a few gallons to several hundred gallons per minute.  The volume of <span class="hlt">water</span> withdrawn from the <span class="hlt">intermediate</span> aquifer system is considerably less than that withdrawn from the Floridan aquifer system in the study area (Duerr and others, 1988).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2011-02-22/pdf/2011-3876.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2011-02-22/pdf/2011-3876.pdf"><span>76 FR 9849 - Comprehensive Environmental Evaluations for <span class="hlt">Antarctic</span> Activities</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>2011-02-22</p> <p>... DEPARTMENT OF STATE [Public Notice 7340] Comprehensive Environmental Evaluations for <span class="hlt">Antarctic</span>... Environmental Evaluations (CEEs) for activities proposed to be undertaken in Antarctica. Interested members of... on Environmental Protection to the <span class="hlt">Antarctic</span> Treaty requires the preparation of a CEE for any...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25489069','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25489069"><span>Impact of <span class="hlt">Antarctic</span> mixed-phase clouds on climate.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lawson, R Paul; Gettelman, Andrew</p> <p>2014-12-23</p> <p>Precious little is known about the composition of low-level clouds over the <span class="hlt">Antarctic</span> Plateau and their effect on climate. In situ measurements at the South Pole using a unique tethered balloon system and ground-based lidar reveal a much higher than anticipated incidence of low-level, mixed-phase clouds (i.e., consisting of supercooled liquid <span class="hlt">water</span> drops and ice crystals). The high incidence of mixed-phase clouds is currently poorly represented in global climate models (GCMs). As a result, the effects that mixed-phase clouds have on climate predictions are highly uncertain. We modify the National Center for Atmospheric Research (NCAR) Community Earth System Model (CESM) GCM to align with the new observations and evaluate the radiative effects on a continental scale. The net cloud radiative effects (CREs) over Antarctica are increased by +7.4 Wm(-2), and although this is a significant change, a much larger effect occurs when the modified model physics are extended beyond the <span class="hlt">Antarctic</span> continent. The simulations show significant net CRE over the Southern Ocean storm tracks, where recent measurements also indicate substantial regions of supercooled liquid. These sensitivity tests confirm that Southern Ocean CREs are strongly sensitive to mixed-phase clouds colder than -20 °C.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1235101-impact-antarctic-mixed-phase-clouds-climate','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1235101-impact-antarctic-mixed-phase-clouds-climate"><span>Impact of <span class="hlt">Antarctic</span> mixed-phase clouds on climate</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Lawson, R. Paul; Gettelman, Andrew</p> <p>2014-12-08</p> <p>Precious little is known about the composition of low-level clouds over the <span class="hlt">Antarctic</span> Plateau and their effect on climate. In situ measurements at the South Pole using a unique tethered balloon system and ground-based lidar reveal a much higher than anticipated incidence of low-level, mixed-phase clouds (i.e., consisting of supercooled liquid <span class="hlt">water</span> drops and ice crystals). The high incidence of mixed-phase clouds is currently poorly represented in global climate models (GCMs). As a result, the effects that mixed-phase clouds have on climate predictions are highly uncertain. In this paper, we modify the National Center for Atmospheric Research (NCAR) Community Earthmore » System Model (CESM) GCM to align with the new observations and evaluate the radiative effects on a continental scale. The net cloud radiative effects (CREs) over Antarctica are increased by +7.4 Wm –2, and although this is a significant change, a much larger effect occurs when the modified model physics are extended beyond the <span class="hlt">Antarctic</span> continent. The simulations show significant net CRE over the Southern Ocean storm tracks, where recent measurements also indicate substantial regions of supercooled liquid. Finally, these sensitivity tests confirm that Southern Ocean CREs are strongly sensitive to mixed-phase clouds colder than –20 °C.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4280591','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4280591"><span>Impact of <span class="hlt">Antarctic</span> mixed-phase clouds on climate</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Lawson, R. Paul; Gettelman, Andrew</p> <p>2014-01-01</p> <p>Precious little is known about the composition of low-level clouds over the <span class="hlt">Antarctic</span> Plateau and their effect on climate. In situ measurements at the South Pole using a unique tethered balloon system and ground-based lidar reveal a much higher than anticipated incidence of low-level, mixed-phase clouds (i.e., consisting of supercooled liquid <span class="hlt">water</span> drops and ice crystals). The high incidence of mixed-phase clouds is currently poorly represented in global climate models (GCMs). As a result, the effects that mixed-phase clouds have on climate predictions are highly uncertain. We modify the National Center for Atmospheric Research (NCAR) Community Earth System Model (CESM) GCM to align with the new observations and evaluate the radiative effects on a continental scale. The net cloud radiative effects (CREs) over Antarctica are increased by +7.4 Wm−2, and although this is a significant change, a much larger effect occurs when the modified model physics are extended beyond the <span class="hlt">Antarctic</span> continent. The simulations show significant net CRE over the Southern Ocean storm tracks, where recent measurements also indicate substantial regions of supercooled liquid. These sensitivity tests confirm that Southern Ocean CREs are strongly sensitive to mixed-phase clouds colder than −20 °C. PMID:25489069</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFMPP33B1922F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFMPP33B1922F"><span>Carbonate Deposition on <span class="hlt">Antarctic</span> Shelves</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Frank, T. D.; James, N. P.; Malcolm, I.</p> <p>2011-12-01</p> <p>Limestones associated with glaciomarine deposits occur throughout the geologic record but remain poorly understood. The best-described examples formed during major ice ages of the Neoproterozoic and Late Paleozoic. Quaternary analogs on <span class="hlt">Antarctic</span> shelves have received comparatively little study. Here, we report on the composition, spatial distribution, and stratigraphic context of carbonate sediments contained in piston cores from the Ross Sea. The goals of this work are to (1) document the nature and distribution of carbonate sediments on the Ross Sea continental shelf and (2) examine temporal relationships to Quaternary glaciation. Results will be used to develop criteria that will improve understanding of analogous deposits in the ancient record. All carbonate-rich intervals in piston cores from the Ross Rea, now housed at the <span class="hlt">Antarctic</span> Marine Geology Research Facility at Florida State University, were examined and described in detail. Sediment samples were disaggregated and sieved into size fractions before description with paleontological analysis carried out on the coarsest size fraction (>250 microns). Carbonate-rich sediments are concentrated in the northwestern Ross Sea, along the distal margins of Mawson and Pennell Banks. Calcareous facies include a spectrum of lithologies that range from fossiliferous mud, sand, and gravel to skeletal floatstone-rudstone and bafflestone. Floatstone-rudstone and bafflestone is most abundant along western-facing slopes in areas protected from the <span class="hlt">Antarctic</span> Coastal Current. Sand-prone facies dominate the tops of banks and mud-prone, often spicultic, facies occur in deeper areas. The carbonate factory is characterized by a low-diversity, heterozoan assemblage that is dominated by stylasterine hydrocorals, barnacles, and bryozoans. Molluscs and echinoids are present but not abundant. Planktic and benthic foraminifera are ubiquitous components of the sediment matrix, which is locally very rich in sponge spicules. Biota rarely</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19860019344','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19860019344"><span>Mysterious iodine-overabundance in <span class="hlt">Antarctic</span> meteorites</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Dreibus, G.; Waenke, H.; Schultz, L.</p> <p>1986-01-01</p> <p>Halogen as well as other trace element concentrations in meteorite finds can be influenced by alteration processes on the Earth's surface. The discovery of <span class="hlt">Antarctic</span> meteorites offered the opportunity to study meteorites which were kept in one of the most sterile environment of the Earth. Halogen determination in Antartic meteorites was compared with non-<span class="hlt">Antarctic</span> meteorites. No correlation was found between iodine concentration and the weathering index, or terrestrial age. The halogen measurements indicate a contaminating phase rich in iodine and also containing chlorine. Possible sources for this contamination are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28663586','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28663586"><span>Radiocarbon as a Novel Tracer of Extra-<span class="hlt">Antarctic</span> Feeding in Southern Hemisphere Humpback Whales.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Eisenmann, Pascale; Fry, Brian; Mazumder, Debashish; Jacobsen, Geraldine; Holyoake, Carlysle Sian; Coughran, Douglas; Bengtson Nash, Susan</p> <p>2017-06-29</p> <p>Bulk stable isotope analysis provides information regarding food web interactions, and has been applied to several cetacean species for the study of migration ecology. One limitation in bulk stable isotope analysis arises when a species, such as Southern hemisphere humpback whales, utilises geographically distinct food webs with differing isotopic baselines. Migrations to areas with different baselines can result in isotopic changes that mimic changes in feeding relations, leading to ambiguous food web interpretations. Here, we demonstrate the novel application of radiocarbon measurement for the resolution of such ambiguities. Radiocarbon was measured in baleen plates from humpback whales stranded in Australia between 2007 and 2013, and in skin samples collected in Australia and Antarctica from stranded and free-ranging animals. Radiocarbon measurements showed lower values for Southern Ocean feeding than for extra-<span class="hlt">Antarctic</span> feeding in Australian <span class="hlt">waters</span>. While the whales mostly relied on <span class="hlt">Antarctic</span>-derived energy stores during their annual migration, there was some evidence of feeding within temperate zone <span class="hlt">waters</span> in some individuals. This work, to our knowledge, provides the first definitive biochemical evidence for supplementary feeding by southern hemisphere humpback whales within temperate <span class="hlt">waters</span> during migration. Further, the work contributes a powerful new tool (radiocarbon) for tracing source regions and geographical feeding.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20010020927&hterms=words&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dwords','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20010020927&hterms=words&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dwords"><span>Latest Word on Retreat of the West <span class="hlt">Antarctic</span> Ice Sheet</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bindschadler, R.</p> <p>2000-01-01</p> <p>The West <span class="hlt">Antarctic</span> ice sheet during the Last Glacial Maximum (LGM) is estimated to have been three times its present volume and to have extended close to the edge of the continental shelf Holocene retreat of this ice sheet in the Ross Sea began between 11,000 and 12,000 years ago. This history implies an average contribution of this ice sheet to sea level of 0.9 mm/a. Evidence of dateable past grounding line positions in the Ross sector are broadly consistent with a linear retreat model. However, inferred rates of retreat for some of these grounding line positions are not consistent with a linear retreat model. More rapid retreat approximately 7600 years ago and possible near-stability in the Ross Sea sector at present suggest a slow rate of initial retreat followed by a more rapid-than-average retreat during the late Holocene, returning to a near-zero rate of retreat currently. This model is also consistent with the mid-Holocene high stand observations of eustatic sea level. Recent compilation of <span class="hlt">Antarctic</span> bed elevations (BEDMAP) illustrates that the LGM and present grounding lines occur in the shallowest <span class="hlt">waters</span>, further supporting the model of a middle phase of rapid retreat bracketed by an older and a more recent phase of modest retreat. Extension of these hypotheses into the future make subsequent behavior of the West <span class="hlt">Antarctic</span> ice sheet more difficult to predict but suggest that if it loses its hold on the present shallow bed, the final retreat of the ice sheet could be very rapid.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_18 --> <div id="page_19" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="361"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=522059','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=522059"><span>Molecular Analysis of Geographic Patterns of Eukaryotic Diversity in <span class="hlt">Antarctic</span> Soils</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Lawley, Blair; Ripley, Sarah; Bridge, Paul; Convey, Peter</p> <p>2004-01-01</p> <p>We describe the application of molecular biological techniques to estimate eukaryotic diversity (primarily fungi, algae, and protists) in <span class="hlt">Antarctic</span> soils across a latitudinal and environmental gradient between approximately 60 and 87°S. The data were used to (i) test the hypothesis that diversity would decrease with increasing southerly latitude and environmental severity, as is generally claimed for “higher” faunal and plant groups, and (ii) investigate the level of endemicity displayed in different taxonomic groups. Only limited support was obtained for a systematic decrease in diversity with latitude, and then only at the level of a gross comparison between maritime (<span class="hlt">Antarctic</span> Peninsula/Scotia Arc) and continental <span class="hlt">Antarctic</span> sites. While the most southerly continental <span class="hlt">Antarctic</span> site was three to four times less diverse than all maritime sites, there was no evidence for a trend of decreasing diversity across the entire range of the maritime <span class="hlt">Antarctic</span> (60 to 72°S). Rather, we found the reverse pattern, with highest diversity at sites on Alexander Island (ca. 72°S), at the southern limit of the maritime <span class="hlt">Antarctic</span>. The very limited overlap found between the eukaryotic biota of the different study sites, combined with their generally low relatedness to existing sequence databases, indicates a high level of <span class="hlt">Antarctic</span> site isolation and possibly endemicity, a pattern not consistent with similar studies on other continents. PMID:15466539</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRG..122.1456H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRG..122.1456H"><span>Microbes influence the biogeochemical and optical properties of maritime <span class="hlt">Antarctic</span> snow</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hodson, A. J.; Nowak, A.; Cook, J.; Sabacka, M.; Wharfe, E. S.; Pearce, D. A.; Convey, P.; Vieira, G.</p> <p>2017-06-01</p> <p>Snowmelt in the <span class="hlt">Antarctic</span> Peninsula region has increased significantly in recent decades, leading to greater liquid <span class="hlt">water</span> availability across a more expansive area. As a consequence, changes in the biological activity within wet <span class="hlt">Antarctic</span> snow require consideration if we are to better understand terrestrial carbon cycling on Earth's coldest continent. This paper therefore examines the relationship between microbial communities and the chemical and physical environment of wet snow habitats on Livingston Island of the maritime <span class="hlt">Antarctic</span>. In so doing, we reveal a strong reduction in bacterial diversity and autotrophic biomass within a short (<1 km) distance from the coast. Coastal snowpacks, fertilized by greater amounts of nutrients from rock debris and marine fauna, develop obvious, pigmented snow algal communities that control the absorption of visible light to a far greater extent than with the inland glacial snowpacks. Absorption by carotenoid pigments is most influential at the surface, while chlorophyll is most influential beneath it. The coastal snowpacks also indicate higher concentrations of dissolved inorganic carbon and CO2 in interstitial air, as well as a close relationship between chlorophyll and dissolved organic carbon (DOC). As a consequence, the DOC resource available in coastal snow can support a more diverse bacterial community that includes microorganisms from a range of nearby terrestrial and marine habitats. Therefore, since further expansion of the melt zone will influence glacial snowpacks more than coastal ones, care must be taken when considering the types of communities that may be expected to evolve there.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008DSRII..55.2404S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008DSRII..55.2404S"><span>The FOODBANCS project: Introduction and sinking fluxes of organic carbon, chlorophyll- a and phytodetritus on the western <span class="hlt">Antarctic</span> Peninsula continental shelf</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Smith, Craig R.; Mincks, Sarah; DeMaster, David J.</p> <p>2008-11-01</p> <p>The impact of the highly seasonal <span class="hlt">Antarctic</span> primary production cycle on shelf benthic ecosystems remains poorly evaluated. Here we describe a times-series research project on the West <span class="hlt">Antarctic</span> Peninsula (WAP) shelf designed to evaluate the seafloor deposition, and subsequent ecological and biogeochemical impacts, of the summer phytoplankton bloom along a transect crossing the <span class="hlt">Antarctic</span> shelf near Anvers Island. During this project, entitled Food for Benthos on the <span class="hlt">Antarctic</span> Continental Shelf (FOODBANCS), we deployed replicate sediment traps 150-170 m above the seafloor (total <span class="hlt">water</span>-column depth of 590 m) on the central shelf from December 1999 to March 2001, recovering trap samples every 3-4 months. In addition, we used a seafloor time-lapse camera system, as well as video surveys conducted at 3-4 months intervals, to monitor the presence and accumulation of phytodetritus at the sediment-<span class="hlt">water</span> interface. The fluxes of particulate organic carbon and chlorophyll- a into sediment traps (binned over 3-4 month intervals) showed patterns consistent with seasonal variability, with average summer fluxes during the first year exceeding winter fluxes by a factor of ˜2-3. However, inter-annual variability in summer fluxes was even greater than seasonal variability, with 4-10-fold differences in the flux of organic carbon and chlorophyll- a between the summer seasons of 1999-2000 and 2000-2001. Phytodetrital accumulation at the shelf floor also exhibited intense inter-annual variability, with no visible phytodetritus from essentially December 1999 to November 2000, followed by pulsed accumulation of 1-2 cm of phytodetritus over a ˜30,000 km 2 shelf area by March 2001. Comparisons with other studies suggest that the levels of inter-annual variability we observed are typical of the <span class="hlt">Antarctic</span> shelf over decadal time scales. We conclude that fluxes of particulate organic carbon, chlorophyll- a and phytodetritus to WAP-shelf sediments vary intensely on seasonal to inter</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AMT....10..825D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AMT....10..825D"><span>Simultaneous retrieval of <span class="hlt">water</span> vapour, temperature and cirrus clouds properties from measurements of far infrared spectral radiance over the <span class="hlt">Antarctic</span> Plateau</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Di Natale, Gianluca; Palchetti, Luca; Bianchini, Giovanni; Del Guasta, Massimo</p> <p>2017-03-01</p> <p>The possibility separating the contributions of the atmospheric state and ice clouds by using spectral infrared measurements is a fundamental step to quantifying the cloud effect in climate models. A simultaneous retrieval of cloud and atmospheric parameters from infrared wideband spectra will allow the disentanglement of the spectral interference between these variables. In this paper, we describe the development of a code for the simultaneous retrieval of atmospheric state and ice cloud parameters, and its application to the analysis of the spectral measurements acquired by the Radiation Explorer in the Far Infrared - Prototype for Applications and Development (REFIR-PAD) spectroradiometer, which has been in operation at Concordia Station on the <span class="hlt">Antarctic</span> Plateau since 2012. The code performs the retrieval with a computational time that is comparable with the instrument acquisition time. <span class="hlt">Water</span> vapour and temperature profiles and the cloud optical and microphysical properties, such as the generalised effective diameter and the ice <span class="hlt">water</span> path, are retrieved by exploiting the 230-980 cm-1 spectral band. To simulate atmospheric radiative transfer, the Line-By-Line Radiative Transfer Model (LBLRTM) has been integrated with a specifically developed subroutine based on the δ-Eddington two-stream approximation, whereas the single-scattering properties of cirrus clouds have been derived from a database for hexagonal column habits. In order to detect ice clouds, a backscattering and depolarisation lidar, co-located with REFIR-PAD has been used, allowing us to infer the position and the cloud thickness to be used in the retrieval. A climatology of the vertical profiles of <span class="hlt">water</span> vapour and temperature has been performed by using the daily radiosounding available at the station at 12:00 UTC. The climatology has been used to build an a priori profile correlation to constrain the fitting procedure. An optimal estimation method with the Levenberg-Marquardt approach has been</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70034090','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70034090"><span>New and interesting species of the genus Muelleria (Bacillariophyta) from the <span class="hlt">Antarctic</span> region and South Africa</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Van De Vijver, B.; Mataloni, G.; Stanish, L.; Spaulding, S.A.</p> <p>2010-01-01</p> <p>During a survey of the terrestrial diatom flora of some sub-<span class="hlt">Antarctic</span> islands in the southern Indian and Atlantic Oceans and of the <span class="hlt">Antarctic</span> continent, more than 15 taxa belonging to the genus Muelleria were observed. Nine of these taxa are described as new species using light and scanning electron microscopy. Comments are made on their systematic position and how they are distinguished from other species in the genus. Additionally, two previously unrecognized taxa within the genus were discovered in samples from South Africa. One of these, Muelleria taylorii Van de Vijver & Cocquyt sp. nov., is new to science; the other, Muelleria vandermerwei (Cholnoky) Van de Vijver & Cocquyt nov. comb., had been included in the genus Diploneis. The large number of new Muelleria taxa on the (sub)-<span class="hlt">Antarctic</span> locations is not surprising. Species in Muelleria occur rarely in collections; in many habitats, it is unusual to find more than 1-2 valves in any slide preparation. As a result, records are scarce. The practice of "force-fitting" (shoehorning) specimens into descriptions from common taxonomic keys (and species drift) results in European species, such as M. gibbula and M. linearis, being applied to <span class="hlt">Antarctic</span> forms in ecological studies. Finally, the typical terrestrial habitats of soils, mosses and ephemeral <span class="hlt">water</span> bodies of most of these taxa have been poorly studied in the past.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://rosap.ntl.bts.gov/view/dot/33846','DOTNTL'); return false;" href="https://rosap.ntl.bts.gov/view/dot/33846"><span>Notes on <span class="hlt">Antarctic</span> aviation</span></a></p> <p><a target="_blank" href="http://ntlsearch.bts.gov/tris/index.do">DOT National Transportation Integrated Search</a></p> <p></p> <p>1993-01-01</p> <p><span class="hlt">Antarctic</span> aviation has been evolving for the best part of a century, with regular air operations developing over the past three or four decades. Antarctica is the last continent where aviation still depends almost entirely on expeditionary airfields ...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1991EOSTr..72Q..84.','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1991EOSTr..72Q..84."><span>AGU honored for <span class="hlt">Antarctic</span> book</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p></p> <p></p> <p>AGU has won an honorable mention award at the Fifteenth Annual Awards Program for Excellence in Professional and Scholarly Publishing sponsored by the Association of American Publishers for the book Volcanoes of the <span class="hlt">Antarctic</span> Plate and Southern Oceans. The book is part of AGU's <span class="hlt">Antarctic</span> Research Series, an outgrowth of research done during the International Geophysical Year that was begun in 1963 with a grant from the National Science Foundation. The award was presented at the AAP Annual Awards Dinner on February 6 at the Ritz-Carlton Hotel in Washington, D.C. The award consists of a medallion and a plate on which the names of the publisher, title, and authors are engraved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17902153','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17902153"><span>Brain and sense organ anatomy and histology of the Falkland Islands mullet, Eleginops maclovinus (Eleginopidae), the sister group of the <span class="hlt">Antarctic</span> notothenioid fishes (Perciformes: Notothenioidei).</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Eastman, Joseph T; Lannoo, Michael J</p> <p>2008-01-01</p> <p>The perciform notothenioid fish Eleginops maclovinus, representing the monotypic family Eleginopidae, has a non-<span class="hlt">Antarctic</span> distribution in the Falkland Islands and southern South America. It is the sister group of the five families and 103 species of <span class="hlt">Antarctic</span> notothenioids that dominate the cold shelf <span class="hlt">waters</span> of Antarctica. Eleginops is the ideal subject for documenting the ancestral morphology of nervous and sensory systems that have not had historical exposure to the unusual <span class="hlt">Antarctic</span> thermal and light regimes, and for comparing these systems with those of the phyletically derived <span class="hlt">Antarctic</span> species. We present a detailed description of the brain and cranial nerves of Eleginops and ask how does the neural and sensory morphology of this non-<span class="hlt">Antarctic</span> notothenioid differ from that seen in the phyletically derived <span class="hlt">Antarctic</span> notothenioids? The brain of Eleginops is similar to those of visually oriented temperate and tropical perciforms. The tectum is smaller but it has well-developed olfactory and mechanoreceptive lateral line areas and a large, caudally projecting corpus cerebellum. Eye diameter is about twofold smaller in Eleginops than in many <span class="hlt">Antarctic</span> species. Eleginops has a duplex (rod and cone) retina with single and occasional twin cones conspicuous centrally. Ocular vascular structures include a large choroid rete mirabile and a small lentiform body; a falciform process and hyaloid arteries are absent. The olfactory rosette is oval with 50-55 lamellae, a large number for notothenioids. The inconspicuous bony canals of the cephalic lateral line system are simple with membranous secondary branches that lack neuromasts. In <span class="hlt">Antarctic</span> species, the corpus cerebellum is the most variable brain region, ranging in size from large and caudally projecting to small and round. "Stalked" brains showing reduction in the size of the telencephalon, tectum, and corpus cerebellum are present in the deep-living artedidraconid Dolloidraco longedorsalis and in most of the deep</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040172948&hterms=major+depression&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dmajor%2Bdepression','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040172948&hterms=major+depression&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dmajor%2Bdepression"><span><span class="hlt">Antarctic</span> isolation: immune and viral studies</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Tingate, T. R.; Lugg, D. J.; Muller, H. K.; Stowe, R. P.; Pierson, D. L.</p> <p>1997-01-01</p> <p>Stressful environmental conditions are a major determinant of immune reactivity. This effect is pronounced in Australian National <span class="hlt">Antarctic</span> Research Expedition populations exposed to prolonged periods of isolation in the <span class="hlt">Antarctic</span>. Alterations of T cell function, including depression of cutaneous delayed-type hypersensitivity responses and a peak 48.9% reduction of T cell proliferation to the mitogen phytohaemagglutinin, were documented during a 9-month period of isolation. T cell dysfunction was mediated by changes within the peripheral blood mononuclear cell compartment, including a paradoxical atypical monocytosis associated with altered production of inflammatory cytokines. There was a striking reduction in the production by peripheral blood mononuclear cells of the predominant pro-inflammatory monokine TNF-alpha and changes were also detected in the production of IL-1, IL-2, IL-6, IL-1ra and IL-10. Prolonged <span class="hlt">Antarctic</span> isolation is also associated with altered latent herpesvirus homeostasis, including increased herpesvirus shedding and expansion of the polyclonal latent Epstein-Barr virus-infected B cell population. These findings have important long-term health implications.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMPA32A..07K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMPA32A..07K"><span>A Roadmap for <span class="hlt">Antarctic</span> and Southern Ocean Science for the Next Two Decades and Beyond</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kennicutt, M. C., II</p> <p>2015-12-01</p> <p>Abstract: <span class="hlt">Antarctic</span> and Southern Ocean science is vital to understanding natural variability, the processes that govern global change and the role of humans in the Earth and climate system. The potential for new knowledge to be gained from future <span class="hlt">Antarctic</span> science is substantial. Therefore, the international <span class="hlt">Antarctic</span> community came together to 'scan the horizon' to identify the highest priority scientific questions that researchers should aspire to answer in the next two decades and beyond. Wide consultation was a fundamental principle for the development of a collective, international view of the most important future directions in <span class="hlt">Antarctic</span> science. From the many possibilities, the horizon scan identified 80 key scientific questions through structured debate, discussion, revision and voting. Questions were clustered into seven topics: i) <span class="hlt">Antarctic</span> atmosphere and global connections, ii) Southern Ocean and sea ice in a warming world, iii) ice sheet and sea level, iv) the dynamic Earth, v) life on the precipice, vi) near-Earth space and beyond, and vii) human presence in Antarctica. Answering the questions identified by the horizon scan will require innovative experimental designs, novel applications of technology, invention of next-generation field and laboratory approaches, and expanded observing systems and networks. Unbiased, non-contaminating procedures will be required to retrieve the requisite air, biota, sediment, rock, ice and <span class="hlt">water</span> samples. Sustained year-round access to Antarctica and the Southern Ocean will be essential to increase winter-time measurements. Improved models are needed that represent Antarctica and the Southern Ocean in the Earth System, and provide predictions at spatial and temporal resolutions useful for decision making. A co-ordinated portfolio of cross-disciplinary science, based on new models of international collaboration, will be essential as no scientist, programme or nation can realize these aspirations alone.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19730018599','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19730018599"><span>Ionic migration and weathering in frozen <span class="hlt">Antarctic</span> soils</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ugolini, F. C.; Anderson, D. M.</p> <p>1973-01-01</p> <p>Soils of continental Antarctica are forming in one of the most severe terrestrial environments. Continuously low temperatures and the scarcity of <span class="hlt">water</span> in the liquid state result in the development of desert-type soils. In an earlier experiment to determine the degree to which radioactive Na(Cl-36) would migrate from a shallow point source in permafrost, movement was observed. To confirm this result, a similar experiment involving (Na-22)Cl was conducted. Significantly less movement of the Na-22 ion was observed. Ionic movement in the unfrozen interfacial films at mineral surfaces in frozen ground is held to be important in chemical weathering in <span class="hlt">Antarctic</span> soils.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15727038','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15727038"><span>Biological invasions in the <span class="hlt">Antarctic</span>: extent, impacts and implications.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Frenot, Yves; Chown, Steven L; Whinam, Jennie; Selkirk, Patricia M; Convey, Peter; Skotnicki, Mary; Bergstrom, Dana M</p> <p>2005-02-01</p> <p>Alien microbes, fungi, plants and animals occur on most of the sub-<span class="hlt">Antarctic</span> islands and some parts of the <span class="hlt">Antarctic</span> continent. These have arrived over approximately the last two centuries, coincident with human activity in the region. Introduction routes have varied, but are largely associated with movement of people and cargo in connection with industrial, national scientific program and tourist operations. The large majority of aliens are European in origin. They have both direct and indirect impacts on the functioning of species-poor <span class="hlt">Antarctic</span> ecosystems, in particular including substantial loss of local biodiversity and changes to ecosystem processes. With rapid climate change occurring in some parts of Antarctica, elevated numbers of introductions and enhanced success of colonization by aliens are likely, with consequent increases in impacts on ecosystems. Mitigation measures that will substantially reduce the risk of introductions to Antarctica and the sub-<span class="hlt">Antarctic</span> must focus on reducing propagule loads on humans, and their food, cargo, and transport vessels.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20050169532','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20050169532"><span>Amino Acids in the <span class="hlt">Antarctic</span> Martian Meteorite MIL03346</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Glavin, D. P.; Aubrey, A.; Dworkin, J. P.; Botta, O.; Bada, J. L.</p> <p>2005-01-01</p> <p>The report by McKay et al. that the Martian meteorite ALH84001 contains evidence for life on Mars remains controversial. Of central importance is whether ALH84001 and other <span class="hlt">Antarctic</span> Martian meteorites contain endogenous organic compounds. In any investigation of organic compounds possibly derived from Mars it is important to focus on compounds that play an essential role in biochemistry as we know it and that have properties such as chirality which can be used to distinguish between biotic versus abiotic origins. Amino acids are one of the few compounds that fulfill these requirements. Previous analyses of the <span class="hlt">Antarctic</span> Martian meteorites ALH84001 and EETA79001 have shown that these meteorites contain low levels of terrestrial amino acid contamination derived from <span class="hlt">Antarctic</span> ice meltwater. Here we report preliminary amino acid investigations of a third <span class="hlt">Antarctic</span> Martian meteorite MIL03346 which was discovered in Antarctica during the 2003-04 ANSMET season. Additional information is included in the original extended abstract</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=STS048-152-007&hterms=5S&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3D5S','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=STS048-152-007&hterms=5S&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3D5S"><span>Breakup of Pack Ice, <span class="hlt">Antarctic</span> Ice Shelf</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1991-01-01</p> <p>Breakup of Pack Ice along the periphery of the <span class="hlt">Antarctic</span> Ice Shelf (53.5S, 3.0E) produced this mosaic of ice floes off the <span class="hlt">Antarctic</span> Ice Shelf. Strong offshore winds, probably associated with strong katabatic downdrafts from the interior of the continent, are seen peeling off the edges of the ice shelf into long filamets of sea ice, icebergs, bergy bits and growlers to flow northward into the South Atlantic Ocean. 53.5S, 3.0E</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23812890','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23812890"><span>Spatial pattern in Antarctica: what can we learn from <span class="hlt">Antarctic</span> bacterial isolates?</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chong, Chun Wie; Goh, Yuh Shan; Convey, Peter; Pearce, David; Tan, Irene Kit Ping</p> <p>2013-09-01</p> <p>A range of small- to moderate-scale studies of patterns in bacterial biodiversity have been conducted in Antarctica over the last two decades, most suggesting strong correlations between the described bacterial communities and elements of local environmental heterogeneity. However, very few of these studies have advanced interpretations in terms of spatially associated patterns, despite increasing evidence of patterns in bacterial biogeography globally. This is likely to be a consequence of restricted sampling coverage, with most studies to date focusing only on a few localities within a specific <span class="hlt">Antarctic</span> region. Clearly, there is now a need for synthesis over a much larger spatial to consolidate the available data. In this study, we collated <span class="hlt">Antarctic</span> bacterial culture identities based on the 16S rRNA gene information available in the literature and the GenBank database (n > 2,000 sequences). In contrast to some recent evidence for a distinct <span class="hlt">Antarctic</span> microbiome, our phylogenetic comparisons show that a majority (~75 %) of <span class="hlt">Antarctic</span> bacterial isolates were highly similar (≥99 % sequence similarity) to those retrieved from tropical and temperate regions, suggesting widespread distribution of eurythermal mesophiles in <span class="hlt">Antarctic</span> environments. However, across different <span class="hlt">Antarctic</span> regions, the dominant bacterial genera exhibit some spatially distinct diversity patterns analogous to those recently proposed for <span class="hlt">Antarctic</span> terrestrial macroorganisms. Taken together, our results highlight the threat of cross-regional homogenisation in <span class="hlt">Antarctic</span> biodiversity, and the imperative to include microbiota within the framework of biosecurity measures for Antarctica.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20060027247','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20060027247"><span>When Will the <span class="hlt">Antarctic</span> Ozone Hole Recover?</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Newman, Paul A.; Nash, Eric R.; Kawa, S. Randolph; Montzka, Stephen A.; Schauffler, Sue</p> <p>2006-01-01</p> <p>The <span class="hlt">Antarctic</span> ozone hole demonstrates large-scale, man-made affects on our atmosphere. Surface observations now show that human produced ozone depleting substances (ODSs) are declining. The ozone hole should soon start to diminish because of this decline. Herein we demonstrate an ozone hole parametric model. This model is based upon: 1) a new algorithm for estimating C1 and Br levels over Antarctica and 2) late-spring <span class="hlt">Antarctic</span> stratospheric temperatures. This parametric model explains 95% of the ozone hole area s variance. We use future ODS levels to predict ozone hole recovery. Full recovery to 1980 levels will occur in approximately 2068. The ozone hole area will very slowly decline over the next 2 decades. Detection of a statistically significant decrease of area will not occur until approximately 2024. We further show that nominal <span class="hlt">Antarctic</span> stratospheric greenhouse gas forced temperature change should have a small impact on the ozone hole.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6463077-antarctic-ice-dynamics-southern-ocean-surface-hydrology-during-last-glacial-maximum','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6463077-antarctic-ice-dynamics-southern-ocean-surface-hydrology-during-last-glacial-maximum"><span><span class="hlt">Antarctic</span> ice dynamics and southern ocean surface hydrology during the last glacial maximum</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>Labeyrie, L.D.; Burckle, L.; Labracherie, M.</p> <p>1985-01-01</p> <p>Eight high sedimentation rate cores located between 61/sup 0/S and 43/sup 0/S in the Atlantic and Indian sectors of the Southern Ocean have been studied in detail for foraminifera and diatom /sup 18/O//sup 16/O ratios, and changes in radiolarian and diatom specific abundance. Comparison of these different parameters permits a detailed description of the surface <span class="hlt">water</span> hydrology during the last glacial maximum. The authors demonstrate that from 25 kyr BP to 15 kyr BP a large number of icebergs formed around the <span class="hlt">Antarctic</span> continent. Melting along the Polar Front decreased surface salinity by approximately 1.5 per thousand between 43/sup 0/Smore » and 50/sup 0/S. They propose that an increase of snow accumulation at the <span class="hlt">Antarctic</span> periphery and downdraw during maximum ice extension are primary causes for this major discharge of icebergs.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20025655','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20025655"><span>Are <span class="hlt">Antarctic</span> minke whales unusually abundant because of 20th century whaling?</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ruegg, Kristen C; Anderson, Eric C; Scott Baker, C; Vant, Murdoch; Jackson, Jennifer A; Palumbi, Stephen R</p> <p>2010-01-01</p> <p>Severe declines in megafauna worldwide illuminate the role of top predators in ecosystem structure. In the <span class="hlt">Antarctic</span>, the Krill Surplus Hypothesis posits that the killing of more than 2 million large whales led to competitive release for smaller krill-eating species like the <span class="hlt">Antarctic</span> minke whale. If true, the current size of the <span class="hlt">Antarctic</span> minke whale population may be unusually high as an indirect result of whaling. Here, we estimate the long-term population size of the <span class="hlt">Antarctic</span> minke whale prior to whaling by sequencing 11 nuclear genetic markers from 52 modern samples purchased in Japanese meat markets. We use coalescent simulations to explore the potential influence of population substructure and find that even though our samples are drawn from a limited geographic area, our estimate reflects ocean-wide genetic diversity. Using Bayesian estimates of the mutation rate and coalescent-based analyses of genetic diversity across loci, we calculate the long-term population size of the <span class="hlt">Antarctic</span> minke whale to be 670,000 individuals (95% confidence interval: 374,000-1,150,000). Our estimate of long-term abundance is similar to, or greater than, contemporary abundance estimates, suggesting that managing <span class="hlt">Antarctic</span> ecosystems under the assumption that <span class="hlt">Antarctic</span> minke whales are unusually abundant is not warranted.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3749108','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3749108"><span>Potential Climate Change Effects on the Habitat of <span class="hlt">Antarctic</span> Krill in the Weddell Quadrant of the Southern Ocean</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Hill, Simeon L.; Phillips, Tony; Atkinson, Angus</p> <p>2013-01-01</p> <p><span class="hlt">Antarctic</span> krill is a cold <span class="hlt">water</span> species, an increasingly important fishery resource and a major prey item for many fish, birds and mammals in the Southern Ocean. The fishery and the summer foraging sites of many of these predators are concentrated between 0° and 90°W. Parts of this quadrant have experienced recent localised sea surface warming of up to 0.2°C per decade, and projections suggest that further widespread warming of 0.27° to 1.08°C will occur by the late 21st century. We assessed the potential influence of this projected warming on <span class="hlt">Antarctic</span> krill habitat with a statistical model that links growth to temperature and chlorophyll concentration. The results divide the quadrant into two zones: a band around the <span class="hlt">Antarctic</span> Circumpolar Current in which habitat quality is particularly vulnerable to warming, and a southern area which is relatively insensitive. Our analysis suggests that the direct effects of warming could reduce the area of growth habitat by up to 20%. The reduction in growth habitat within the range of predators, such as <span class="hlt">Antarctic</span> fur seals, that forage from breeding sites on South Georgia could be up to 55%, and the habitat’s ability to support <span class="hlt">Antarctic</span> krill biomass production within this range could be reduced by up to 68%. Sensitivity analysis suggests that the effects of a 50% change in summer chlorophyll concentration could be more significant than the direct effects of warming. A reduction in primary production could lead to further habitat degradation but, even if chlorophyll increased by 50%, projected warming would still cause some degradation of the habitat accessible to predators. While there is considerable uncertainty in these projections, they suggest that future climate change could have a significant negative effect on <span class="hlt">Antarctic</span> krill growth habitat and, consequently, on Southern Ocean biodiversity and ecosystem services. PMID:23991072</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23991072','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23991072"><span>Potential climate change effects on the habitat of <span class="hlt">antarctic</span> krill in the weddell quadrant of the southern ocean.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hill, Simeon L; Phillips, Tony; Atkinson, Angus</p> <p>2013-01-01</p> <p><span class="hlt">Antarctic</span> krill is a cold <span class="hlt">water</span> species, an increasingly important fishery resource and a major prey item for many fish, birds and mammals in the Southern Ocean. The fishery and the summer foraging sites of many of these predators are concentrated between 0° and 90°W. Parts of this quadrant have experienced recent localised sea surface warming of up to 0.2°C per decade, and projections suggest that further widespread warming of 0.27° to 1.08°C will occur by the late 21(st) century. We assessed the potential influence of this projected warming on <span class="hlt">Antarctic</span> krill habitat with a statistical model that links growth to temperature and chlorophyll concentration. The results divide the quadrant into two zones: a band around the <span class="hlt">Antarctic</span> Circumpolar Current in which habitat quality is particularly vulnerable to warming, and a southern area which is relatively insensitive. Our analysis suggests that the direct effects of warming could reduce the area of growth habitat by up to 20%. The reduction in growth habitat within the range of predators, such as <span class="hlt">Antarctic</span> fur seals, that forage from breeding sites on South Georgia could be up to 55%, and the habitat's ability to support <span class="hlt">Antarctic</span> krill biomass production within this range could be reduced by up to 68%. Sensitivity analysis suggests that the effects of a 50% change in summer chlorophyll concentration could be more significant than the direct effects of warming. A reduction in primary production could lead to further habitat degradation but, even if chlorophyll increased by 50%, projected warming would still cause some degradation of the habitat accessible to predators. While there is considerable uncertainty in these projections, they suggest that future climate change could have a significant negative effect on <span class="hlt">Antarctic</span> krill growth habitat and, consequently, on Southern Ocean biodiversity and ecosystem services.</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('https://ntrs.nasa.gov/search.jsp?R=20160009149&hterms=cycles&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dcycles','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20160009149&hterms=cycles&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dcycles"><span>Modeling <span class="hlt">Antarctic</span> Subglacial Lake Filling and Drainage Cycles</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Dow, Christine F.; Werder, Mauro A.; Nowicki, Sophie; Walker, Ryan T.</p> <p>2016-01-01</p> <p>The growth and drainage of active subglacial lakes in Antarctica has previously been inferred from analysis of ice surface altimetry data. We use a subglacial hydrology model applied to a synthetic <span class="hlt">Antarctic</span> ice stream to examine internal controls on the filling and drainage of subglacial lakes. Our model outputs suggest that the highly constricted subglacial environment of our idealized ice stream, combined with relatively high rates of <span class="hlt">water</span> flow funneled from a large catchment, can combine to create a system exhibiting slow-moving pressure waves. Over a period of years, the accumulation of <span class="hlt">water</span> in the ice stream onset region results in a buildup of pressure creating temporary channels, which then evacuate the excess <span class="hlt">water</span>. This increased flux of <span class="hlt">water</span> beneath the ice stream drives lake growth. As the <span class="hlt">water</span> body builds up, it steepens the hydraulic gradient out of the overdeepened lake basin and allows greater flux. Eventually this flux is large enough to melt channels that cause the lake to drain. Lake drainage also depends on the internal hydrological development in the wider system and therefore does not directly correspond to a particular <span class="hlt">water</span> volume or depth. This creates a highly temporally and spatially variable system, which is of interest for assessing the importance of subglacial lakes in ice stream hydrology and dynamics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19860019355','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19860019355"><span>Terrestrial ages of <span class="hlt">Antarctic</span> meteorites: Implications for concentration mechanisms</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Schultz, L.</p> <p>1986-01-01</p> <p><span class="hlt">Antarctic</span> meteorites differ from meteorites fallen in other places in their mean terrestrial ages. Boeckl estimated the terrestrial half-life for the disintegration of stone meteorites by weathering under the climatic conditions of the Western United States to be about 3600 years. <span class="hlt">Antarctic</span> meteorites, however, have terrestrial ages up to 70000 years, indicating larger weathering half-lives. The terrestrial ages of meteorites are determined by their concentration of cosmic-ray-produced radionuclides with suitable half-lives (C-14, Al-26, and Cl-36). These radionuclides have yielded reliable ages for the <span class="hlt">Antarctic</span> meteorites. The distribution of terrestrial ages of Allan Hills and Yamato meteorites are examined.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29796342','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29796342"><span>Effect of elevated temperature on membrane lipid saturation in <span class="hlt">Antarctic</span> notothenioid fish.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Malekar, Vanita C; Morton, James D; Hider, Richard N; Cruickshank, Robert H; Hodge, Simon; Metcalf, Victoria J</p> <p>2018-01-01</p> <p>Homeoviscous adaptation (HVA) is a key cellular response by which fish protect their membranes against thermal stress. We investigated evolutionary HVA (long time scale) in <span class="hlt">Antarctic</span> and non-<span class="hlt">Antarctic</span> fish. Membrane lipid composition was determined for four Perciformes fish: two closely related <span class="hlt">Antarctic</span> notothenioid species ( Trematomus bernacchii and Pagothenia borchgrevinki ); a diversified related notothenioid <span class="hlt">Antarctic</span> icefish ( Chionodraco hamatus ); and a New Zealand species ( Notolabrus celidotus ). The membrane lipid compositions were consistent across the three <span class="hlt">Antarctic</span> species and these were significantly different from that of the New Zealand species. Furthermore, acclimatory HVA (short time periods with seasonal changes) was investigated to determine whether stenothermal <span class="hlt">Antarctic</span> fish, which evolved in the cold, stable environment of the Southern Ocean, have lost the acclimatory capacity to modulate their membrane saturation states, making them vulnerable to anthropogenic global warming. We compared liver membrane lipid composition in two closely related <span class="hlt">Antarctic</span> fish species acclimated at 0 °C (control temperature), 4 °C for a period of 14 days in T. bernacchii and 28 days for P. borchgrevinki, and 6 °C for 7 days in both species. Thermal acclimation at 4 °C did not result in changed membrane saturation states in either <span class="hlt">Antarctic</span> species. Despite this, membrane functions were not compromised, as indicated by declining serum osmolality, implying positive compensation by enhanced hypo-osmoregulation. Increasing the temperature to 6 °C did not change the membrane lipids of P. borchgrevinki. However, in T. bernacchii, thermal acclimation at 6 °C resulted in an increase of membrane saturated fatty acids and a decline in unsaturated fatty acids. This is the first study to show a homeoviscous response to higher temperatures in an <span class="hlt">Antarctic</span> fish, although for only one of the two species examined.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19920006245','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19920006245"><span>Observations and theories related to <span class="hlt">Antarctic</span> ozone changes</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hartmann, D.; Watson, R. T.; Cox, Richard A.; Kolb, C.; Mahlman, J.; Mcelroy, M.; Plumb, A.; Ramanathan, V.; Schoeberl, M.; Solomon, S.</p> <p>1989-01-01</p> <p>In 1985, there was a report of a large, sudden, and unanticipated decrease in the abundance of springtime <span class="hlt">Antarctic</span> ozone over the last decade. By 1987, ozone decreases of more than 50 percent in the total column, and 95 percent locally between 15 and 20 km, had been observed. The scientific community quickly rose to the challenge of explaining this remarkable discovery; theoreticians soon developed a series of chemical and dynamical hypotheses to explain the ozone loss. Three basic theories were proposed to explain the springtime ozone hole. (1) The ozone hole is caused by the increasing atmospheric loadings of manmade chemicals containing chlorine (chlorofluorocarbons (CFC's) and bromine (halons)). These chemicals efficiently destroy ozone in the lower stratosphere in the <span class="hlt">Antarctic</span> because of the special geophysical conditions, of an isolated air mass (polar vortex) with very cold temperatures, that exist there. (2) The circulation of the atmosphere in spring has changed from being predominantly downward over Antarctica to upward. This would mean that ozone poor air from the troposphere, instead of ozone rich air from the upper stratosphere, would be transported into the lower <span class="hlt">Antarctic</span> stratosphere. (3) The abundance of the oxides of nitrogen in the lower <span class="hlt">Antarctic</span> stratosphere is periodically enhanced by solar activity. Nitrogen oxides are produced in the upper mesosphere and thermosphere and then transported downward into the lower stratosphere in Antarctica, resulting in the chemical destruction of ozone. The climatology and trends of ozone, temperature, and polar stratospheric clouds are discussed. Also, the transport and chemical theories for the <span class="hlt">Antarctic</span> ozone hole are presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..14.8790T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..14.8790T"><span>Particulate export vs lateral advection in the <span class="hlt">Antarctic</span> Polar Front (Southern Pacific Ocean)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tesi, T.; Langone, L.; Ravaioli, M.; Capotondi, L.; Giglio, F.</p> <p>2012-04-01</p> <p>The overarching goal of our study was to describe and quantify the influence of lateral advection relative to the vertical export in the <span class="hlt">Antarctic</span> Polar Front (Southern Pacific Ocean). In areas where lateral advection of particulate material is significant, budgets of bioactive elements can be inaccurate if fluxes through the <span class="hlt">water</span> column and to the seabed are exclusively interpreted as passive sinking of particles. However, detailed information on the influence of lateral advection in the <span class="hlt">water</span> column in the southern ocean is lacking. With this in mind, our study focused between the twilight zone (i.e. mesopelagic) and the benthic nepheloid layer to understand the relative importance of lateral flux with increasing <span class="hlt">water</span> depth. Measurements were performed south of the <span class="hlt">Antarctic</span> Polar Front for 1 year (January 10th 1999-January 3rd 2000) at 900, 1300, 2400, and 3700 m from the sea surface. The study was carried out using a 3.5 km long mooring line instrumented with sediment traps, current meters and sensors of temperature and conductivity. Sediment trap samples were characterized via several parameters including total mass flux, elemental composition (organic carbon, total nitrogen, biogenic silica, and calcium carbonate), concentration of metals (aluminum, iron, barium, and manganese), 210Pb activity, and foraminifera taxonomy. High fluxes of biogenic particles were observed in both summer 1999 and 2000 as a result of seasonal algal blooms associated with sea ice retreat and <span class="hlt">water</span> column stratification. During no-productive periods, several high energy events occurred and resulted in advecting resuspended biogenic particles from flat-topped summits of the Pacific <span class="hlt">Antarctic</span> Ridge. Whereas the distance between seabed and uppermost sediment traps was sufficient to avoid lateral advection processes, resuspension was significant in the lowermost sediment traps accounting for ~60 and ~90% of the material caught at 2400 and 3700 m, respectively. Samples collected during</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/10177971','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/10177971"><span>The use of drilling by the U.S. <span class="hlt">Antarctic</span> program</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>Wade, M.C.; Webb, J.W.; Hedberg, W.H.</p> <p>1994-08-01</p> <p>This report on drilling in the <span class="hlt">Antarctic</span> has been prepared by the U.S. National Science Foundation (NSF) to assist principal investigators and others in complying with the National Environmental Policy Act (NEPA) and the <span class="hlt">Antarctic</span> Treaty of 1961. Implementing regulations for NEPA are spelled out in 40 CFR 1500-1508. Environmental protection under the <span class="hlt">Antarctic</span> Treaty is addressed in the Protocol on Environmental Protection to the <span class="hlt">Antarctic</span> Treaty (hereafter referred to as the Protocol), which was adopted by 26 countries in 1991. In the United States, responsibility for compliance with these requirements rests with the NSF Office of Polar Programs (OPP),more » which manages the U.S. <span class="hlt">Antarctic</span> Program (USAP). The USAP recognizes the potentially profound impacts that its presence and activities can have on the <span class="hlt">antarctic</span> environment. In its extensive support of operations and research in Antarctica, the USAP uses all practical means to foster and maintain natural conditions while supporting scientific endeavors in a safe and healthful manner. Reducing human impacts on the <span class="hlt">antarctic</span> environment is a major goal of the USAP. The USAP`s operating philosophy is based on broad yet reasonable and practical assumptions concerning environmental protection. The USAP maintains three year-round stations on the continent to support scientific research. Research and associated support operations at these stations and camps sometimes involve drilling into ice, soil, or ocean sediments. In order to comply with NEPA and the Protocol, it is necessary for principal investigators and others to assess the environmental effects of drilling. This report has been prepared to assist in this process by describing various drilling technologies currently available for use in Antarctica, generally characterizing the potential environmental impacts associated with these drilling techniques, and identifying possible mitigation measures to reduce impacts.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/41495','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/41495"><span>Potentiometric surface of the <span class="hlt">intermediate</span> aquifer system, west- central Florida, May 1987</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Lewelling, B.R.</p> <p>1988-01-01</p> <p>The <span class="hlt">intermediate</span> aquifer system within the Southwest Florida <span class="hlt">Water</span> Management District underlies a 5,000 sq mi area of De Soto, Sarasota, Hardee, Manatee, and parts of Charlotte, Hillsborough, Highlands, and Polk Counties. The <span class="hlt">intermediate</span> aquifer system occurs between the overlying surficial aquifer system and the underlying Floridan aquifer system, and consists of layers of sand, shell, clay, marl, limestone, and dolom of the Tamiami, Hawthorn, and Tampa Formations of late Tertiary age. The <span class="hlt">intermediate</span> aquifer system contains one or more <span class="hlt">water</span>-bearing units separated by discontinuous confining units. This aquifer system is the principal source of potable <span class="hlt">water</span> in the southwestern part of the study area and is widely used as a source of <span class="hlt">water</span> in other parts where wells are open to the <span class="hlt">intermediate</span> aquifer system or to both the <span class="hlt">intermediate</span> and Floridan aquifer systems. Yields of individual wells open to the <span class="hlt">intermediate</span> aquifer system range from a few gallons to several hundred gallons per minute. The volume of <span class="hlt">water</span> withdrawn from the <span class="hlt">intermediate</span> aquifer system is considerably less than that withdrawn from the Floridan aquifer system in the study area. The surface was mapped by determining the altitude of <span class="hlt">water</span> levels in a network of wells and is represented on maps by contours that connect points of equal altitude. The compos potentiometric surface of all <span class="hlt">water</span>-bearing units within the <span class="hlt">intermediate</span> aquifer system is shown. In areas where multiple aquifers exist, wells open to all aquifers were selected for <span class="hlt">water</span> level measurements whenever possible. In the southwestern and lower coastal region of the study area, two aquifers and confining units are described for the <span class="hlt">intermediate</span> aquifer system: the Tamiami-upper Hawthorn aquifer and the underlying lower Hawthorn-upper Tampa aquifer. The potentiometric surface of the Tamiami-upper Hawthorn aquifer is also shown. <span class="hlt">Water</span> levels are from wells drilled and open exclusively to that aquifer. The exact boundary for the</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 Ocean <span class="hlt">intermediate</span> <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 Ocean, and the degree to which it communicated with the surface ocean 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 Ocean 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 Ocean 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 <span class="hlt">intermediate</span> <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 Ocean (˜123°W, ˜69°S, 2500 m to 1430 m <span class="hlt">water</span> depth), with the aim of resolving deglacial <span class="hlt">intermediate</span> <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 <span class="hlt">intermediate</span> <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('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4078843','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4078843"><span>Evidence for elevated and spatially variable geothermal flux beneath the West <span class="hlt">Antarctic</span> Ice Sheet</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Schroeder, Dustin M.; Blankenship, Donald D.; Young, Duncan A.; Quartini, Enrica</p> <p>2014-01-01</p> <p>Heterogeneous hydrologic, lithologic, and geologic basal boundary conditions can exert strong control on the evolution, stability, and sea level contribution of marine ice sheets. Geothermal flux is one of the most dynamically critical ice sheet boundary conditions but is extremely difficult to constrain at the scale required to understand and predict the behavior of rapidly changing glaciers. This lack of observational constraint on geothermal flux is particularly problematic for the glacier catchments of the West <span class="hlt">Antarctic</span> Ice Sheet within the low topography of the West <span class="hlt">Antarctic</span> Rift System where geothermal fluxes are expected to be high, heterogeneous, and possibly transient. We use airborne radar sounding data with a subglacial <span class="hlt">water</span> routing model to estimate the distribution of basal melting and geothermal flux beneath Thwaites Glacier, West Antarctica. We show that the Thwaites Glacier catchment has a minimum average geothermal flux of ∼114 ± 10 mW/m2 with areas of high flux exceeding 200 mW/m2 consistent with hypothesized rift-associated magmatic migration and volcanism. These areas of highest geothermal flux include the westernmost tributary of Thwaites Glacier adjacent to the subaerial Mount Takahe volcano and the upper reaches of the central tributary near the West <span class="hlt">Antarctic</span> Ice Sheet Divide ice core drilling site. PMID:24927578</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120001959','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120001959"><span><span class="hlt">Antarctic</span> Mirabilite Mounds as Mars Analogs: The Lewis Cliffs Ice Tongue Revisited</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Socki, Richard A.; Sun, Tao; Niles, Paul B.; Harvey, Ralph P.; Bish, David L.; Tonui, Eric</p> <p>2012-01-01</p> <p>It has been proposed, based on geomorphic and geochemical arguments, that subsurface <span class="hlt">water</span> has played an important role in the history of <span class="hlt">water</span> on the planet Mars [1]. Subsurface <span class="hlt">water</span>, if present, could provide a protected and long lived environment for potential life. Discovery of gullies [2] and recurring slopes [3] on Mars suggest the potential for subsurface liquid <span class="hlt">water</span> or brines. Recent attention has also focused on small (< approx. 1km dia.) mound-like geomorphic features discovered within the mid to high latitudes on the surface of Mars which may be caused by eruptions of subsurface fluids [4, 5]. We have identified massive but highly localized Na-sulfate deposits (mirabilite mounds, Na2SO4 .10H2O) that may be derived from subsurface fluids and may provide insight into the processes associated with subsurface fluids on Mars. The mounds are found on the end moraine of the Lewis Cliffs Ice Tongue (LCIT) [6] in the Transantarctic Mountains, Antarctica, and are potential terrestrial analogs for mounds observed on the martian surface. The following characteristics distinguish LCIT evaporite mounds from other evaporite mounds found in <span class="hlt">Antarctic</span> coastal environments and/or the McMurdo Dry Valleys: (1) much greater distance from the open ocean (approx.500 km); (2) higher elevation (approx.2200 meters); and (3) colder average annual temperature (average annual temperature = -30 C for LCIT [7] vs. 20 C at sea level in the McMurdo region [8]. Furthermore, the recent detection of subsurface <span class="hlt">water</span> ice (inferred as debris-covered glacial ice) by the Mars Reconnaissance Orbiter [9] supports the use of an <span class="hlt">Antarctic</span> glacial environment, particularly with respect to the mirabilite deposits described in this work, as an ideal terrestrial analog for understanding the geochemistry associated with near-surface martian processes. S and O isotopic compositions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017DSRII.138...86P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017DSRII.138...86P"><span>Particulate organic carbon export across the <span class="hlt">Antarctic</span> Circumpolar Current at 10°E: Differences between north and south of the <span class="hlt">Antarctic</span> Polar Front</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Puigcorbé, Viena; Roca-Martí, Montserrat; Masqué, Pere; Benitez-Nelson, Claudia R.; Rutgers v. d. Loeff, Michiel; Laglera, Luis M.; Bracher, Astrid; Cheah, Wee; Strass, Volker H.; Hoppema, Mario; Santos-Echeandía, Juan; Hunt, Brian P. V.; Pakhomov, Evgeny A.; Klaas, Christine</p> <p>2017-04-01</p> <p>The vertical distribution of 234Th was measured along the 10°E meridian between 44°S and 53°S in the <span class="hlt">Antarctic</span> Circumpolar Current (ACC) during the austral summer of 2012. The overarching goal of this work was to estimate particulate organic carbon (POC) export across three fronts: the Sub-<span class="hlt">Antarctic</span> Front (SAF), the <span class="hlt">Antarctic</span> Polar Front (APF) and the Southern Polar Front (SPF). Steady state export fluxes of 234Th in the upper 100 m ranged from 1600 to 2600 dpm m-2 d-1, decreasing with increasing latitude. Using large particle (>53 μm) C/234Th ratios, the 234Th-derived POC fluxes at 100 m ranged from 25 to 41 mmol C m-2 d-1. Observed C/234Th ratios decreased with increasing depth north of the APF while south of the APF, ratios remained similar or even increased with depth. These changes in C/234Th ratios are likely due to differences in the food web. Indeed, satellite images, together with macronutrients and dissolved iron concentrations suggest two different planktonic community structures north and south of the APF. Our results indicate that higher ratios of POC flux at 100 m to primary production occurred in nanophytoplankton dominated surface <span class="hlt">waters</span>, where primary production rates were lower. Satellite images prior to the expedition suggest that the higher export efficiencies obtained in the northern half of the transect may be the result of the decoupling between production and export (Buesseler 1998). Transfer efficiencies to 400 m, i.e. the fraction of exported POC that reached 400 m, were found to be higher south of the APF, where diatoms were dominant and salps largely abundant. This suggests different remineralization pathways of sinking particles, influencing the transfer efficiency of exported POC to depth.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20060026273&hterms=ods&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dods','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060026273&hterms=ods&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dods"><span>When Will the <span class="hlt">Antarctic</span> Ozone Hole Recover?</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Newman, Paul A.</p> <p>2006-01-01</p> <p>The <span class="hlt">Antarctic</span> ozone hole demonstrates large-scale, man-made affects on our atmosphere. Surface observations now show that human produced ozone depleting substances (ODSs) are declining. The ozone hole should soon start to diminish because of this decline. In this talk we will demonstrate an ozone hole parametric model. This model is based upon: 1) a new algorithm for estimating 61 and Br levels over Antarctica and 2) late-spring <span class="hlt">Antarctic</span> stratospheric temperatures. This parametric model explains 95% of the ozone hole area's variance. We use future ODS levels to predict ozone hole recovery. Full recovery to 1980 levels will occur in approximately 2068. The ozone hole area will very slowly decline over the next 2 decades. Detection of a statistically significant decrease of area will not occur until approximately 2024. We further show that nominal <span class="hlt">Antarctic</span> stratospheric greenhouse gas forced temperature change should have a small impact on the ozone hole.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23449589','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23449589"><span>Synchronous change of atmospheric CO2 and <span class="hlt">Antarctic</span> temperature during the last deglacial warming.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Parrenin, F; Masson-Delmotte, V; Köhler, P; Raynaud, D; Paillard, D; Schwander, J; Barbante, C; Landais, A; Wegner, A; Jouzel, J</p> <p>2013-03-01</p> <p>Understanding the role of atmospheric CO2 during past climate changes requires clear knowledge of how it varies in time relative to temperature. <span class="hlt">Antarctic</span> ice cores preserve highly resolved records of atmospheric CO2 and <span class="hlt">Antarctic</span> temperature for the past 800,000 years. Here we propose a revised relative age scale for the concentration of atmospheric CO2 and <span class="hlt">Antarctic</span> temperature for the last deglacial warming, using data from five <span class="hlt">Antarctic</span> ice cores. We infer the phasing between CO2 concentration and <span class="hlt">Antarctic</span> temperature at four times when their trends change abruptly. We find no significant asynchrony between them, indicating that <span class="hlt">Antarctic</span> temperature did not begin to rise hundreds of years before the concentration of atmospheric CO2, as has been suggested by earlier studies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.4444G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.4444G"><span>Atmospheric moisture supersaturatons in the near-surface atmosphere of Dome C, <span class="hlt">Antarctic</span> Plateau</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Genthon, Christophe; Piard, Luc; Vignon, Etienne; Madeleine, Jean-Baptiste; Casado, Mathieu; Gallée, Hubert</p> <p>2017-04-01</p> <p>Moisture supersaturations occur at the top of the troposphere where cirrus clouds form, but is comparatively unusual near the surface where the air is generally warmer and laden with liquid and/or ice condensation nuclei. One exception is the surface of the high <span class="hlt">antarctic</span> plateau. This study presents one year of atmospheric moisture measurement at the surface of Dome C on the East <span class="hlt">Antarctic</span> plateau. The measurements are obtained using commercial hygrometry sensors adapted to allow air sampling without affecting the moisture content even in case of supersaturation. Supersaturation is found to be very frequent. Common unadapted hygrometry sensors generally fail to report supersaturation, and most reports of atmospheric moisture on the <span class="hlt">antarctic</span> plateau are thus likely biased low. The measurements are compared with results from 2 models with cold microphysics parametrizations: the European Center for Medium-range Weather Forecasts through its operational analyses, and the Model Atmosphérique Régional. As in the observations, supersaturation is frequent in the models but the statistical distribution differs both between models and observations and between the 2 models, leaving much room for model improvement. The representation of supersaturations is not critical for the estimations of surface sublimation since they are more frequent as temperature is lower i.e. as moisture quantities and <span class="hlt">water</span> fluxes are small. However, ignoring near-surface supersaturation may be a more serious issue for the modeling of fog and when considering <span class="hlt">water</span> isotopes, a tracer of phase change and temperature, largely used to reconstruct past climates and environments from ice cores. Because observations are easier in the surface atmosphere, longer and more continuous in situ observation series of atmospheric supersaturation can be obtained than higher in the atmosphere to test parameterizations of cold microphysics, such as those used in the formation of high altitude cirrus clouds in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22133311','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22133311"><span>Energetic consequences of repeated and prolonged dehydration in the <span class="hlt">Antarctic</span> midge, Belgica antarctica.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Teets, Nicholas M; Kawarasaki, Yuta; Lee, Richard E; Denlinger, David L</p> <p>2012-04-01</p> <p>Larvae of the <span class="hlt">Antarctic</span> midge, Belgica antarctica, routinely face periods of limited <span class="hlt">water</span> availability in their natural environments on the <span class="hlt">Antarctic</span> Peninsula. As a result, B. antarctica is one of the most dehydration-tolerant insects studied, surviving up to 70% loss of its body <span class="hlt">water</span>. While previous studies have characterized the physiological effects of a single bout of dehydration, in nature larvae are likely to experience multiple bouts of dehydration throughout their lifetime. Thus, we examined the physiological consequences of repeated dehydration and compared results to larvae exposed to a single, prolonged period of dehydration. For the repeated dehydration experiment, larvae were exposed to 1-5 cycles of 24 h dehydration at 75% RH followed by 24 h rehydration. Each bout of dehydration resulted in 30-40% loss of body <span class="hlt">water</span>, with a concomitant 2- to 3-fold increase in body fluid osmolality. While nearly 100% of larvae survived a single bout of dehydration, <65% of larvae survived five such cycles. Larvae subjected to multiple bouts of dehydration also experienced severe depletion of carbohydrate energy reserves; glycogen and trehalose content decreased with each successive cycle, with larvae losing 89% and 48% of their glycogen and trehalose, respectively, after five cycles of dehydration/rehydration. Larvae exposed to prolonged dehydration (99% RH for 10d) had 26% less <span class="hlt">water</span>, 43% less glycogen, and 27% less lipid content than controls, but did not experience any mortality. Thus, both repeated and prolonged dehydration results in substantial energetic costs that are likely to negatively impact fitness. Copyright © 2011 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70044191','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70044191"><span><span class="hlt">Antarctic</span> and Southern Ocean influences on Late Pliocene global cooling</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>McKay, Robert; Naish, Tim; Carter, Lionel; Riesselman, Christina; Dunbar, Robert; Sjunneskog, Charlotte; Winter, Diane; Sangiorgi, Francesca; Warren, Courtney; Pagani, Mark; Schouten, Stefan; Willmott, Veronica; Levy, Richard; DeConto, Robert; Powell, Ross D.</p> <p>2012-01-01</p> <p>The influence of Antarctica and the Southern Ocean on Late Pliocene global climate reconstructions has remained ambiguous due to a lack of well-dated <span class="hlt">Antarctic</span>-proximal, paleoenvironmental records. Here we present ice sheet, sea-surface temperature, and sea ice reconstructions from the ANDRILL AND-1B sediment core recovered from beneath the Ross Ice Shelf. We provide evidence for a major expansion of an ice sheet in the Ross Sea that began at ~3.3 Ma, followed by a coastal sea surface temperature cooling of ~2.5 °C, a stepwise expansion of sea ice, and polynya-style deep mixing in the Ross Sea between 3.3 and 2.5 Ma. The intensification of <span class="hlt">Antarctic</span> cooling resulted in strengthened westerly winds and invigorated ocean circulation. The associated northward migration of Southern Ocean fronts has been linked with reduced Atlantic Meridional Overturning Circulation by restricting surface <span class="hlt">water</span> connectivity between the ocean basins, with implications for heat transport to the high latitudes of the North Atlantic. While our results do not exclude low-latitude mechanisms as drivers for Pliocene cooling, they indicate an additional role played by southern high-latitude cooling during development of the bipolar world.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFMOS33A1684H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFMOS33A1684H"><span>Habitat Selection and Foraging Behavior of Southern Elephant Seals in the Western <span class="hlt">Antarctic</span> Peninsula</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Huckstadt, L.; Costa, D. P.; McDonald, B. I.; Tremblay, Y.; Crocker, D. E.; Goebel, M. E.; Fedak, M. E.</p> <p>2006-12-01</p> <p>We examined the foraging behavior of 18 southern elephant seals foraging over two seasons in the Western <span class="hlt">Antarctic</span> Peninsula. The foraging behavior and habitat utilization of 7 females in 2005 and 12 in 2006 were followed using satellite linked Satellite Relay Data Loggers that measured diving behavior as well collected salinity and temperature profiles as the animals dove. Animals were tagged after the annual molt during February at Cape Shirreff Livngston Island, South Shetland Islands. There was significant interannual variation in the regions of the Southern Ocean used by seals from Livingston Island. In 2005 of the 7 animals tagged one foraged 4700 km due west of the <span class="hlt">Antarctic</span> Peninsula going as far as 150 W. The remaining females headed south along the Western <span class="hlt">Antarctic</span> Peninsula bypassing Marguerite Bay moving south along Alexander Island. Three of these animals continued to forage in the pack ice as it developed. On their return trip all females swam past Livingston Island, continuing on to South Georgia Island where they apparently bred in the austral spring. One animal returned to Cape Shirreff to molt and her tag was recovered. During 2006 animals initially followed a similar migratory pattern going south along the <span class="hlt">Antarctic</span> Peninsula, but unlike 2005 where the majority of the animals remained in the immediate vicinity of the Western <span class="hlt">Antarctic</span> Peninsula, most of the animals in 2006 moved well to the west foraging as far as the Amundsen Sea. We compared the area restricted search (focal foraging areas) areas of these animals using a newly developed fractal landscape technique that identifies and quantifies areas of intensive search. The fractal analysis of area restricted search shows that the area, distance and coverage (Fractal D) searched were not different between years, while the time spent in the search areas was higher in 2005. Further analysis will examine how the physical properties of the <span class="hlt">water</span> column as determined from the CTD data derived from</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19880060577&hterms=Hofmann&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3DHofmann','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19880060577&hterms=Hofmann&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3DHofmann"><span>Balloon borne <span class="hlt">Antarctic</span> frost point measurements and their impact on polar stratospheric cloud theories</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rosen, James M.; Hofmann, D. J.; Carpenter, J. R.; Harder, J. W.; Oltsmans, S. J.</p> <p>1988-01-01</p> <p>Balloon-borne frost point measurements were performed over Antarctica during September-October 1987 as part of the NOZE II effort at McMurdo. The results show <span class="hlt">water</span> mixing ratios on the order of 2 ppmv in the 20 km region, suggesting that models of the springtime <span class="hlt">Antarctic</span> stratosphere should be based on approximately 2 ppmv <span class="hlt">water</span> vapor. Evidence indicating that some PSCs form at temperatures higher than the frost point in the 15 to 20 km region is discussed. This supports the binary HNO3-H2O theory of PSC composition.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhDT.........2G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhDT.........2G"><span>Oceanic Controls of North American East Coast Sea Level Rise and Ocean Warming of the <span class="hlt">Antarctic</span> Shelf</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Goddard, Paul</p> <p></p> <p>, we use a fine-resolution global climate model (GFDL CM2.6) that resolves an eddying ocean. With this state-of-the-art coupled model, we quantify the mechanisms contributing to ocean warming on the <span class="hlt">Antarctic</span> continental shelf in an idealized experiment of doubling of the atmospheric CO2 concentration. The results show that the CO2 forcing leads to the shelf region warming both in the upper 100 m ocean and at depths near the sea floor. These warming patterns are controlled by different mechanisms. In the upper 100 m, the heat anomalies are primarily controlled by increased heat transport into the shelf region associated with the warmer near-surface <span class="hlt">waters</span> from lower latitudes. Below 100 m, the heat anomalies develop due to increased onshore intrusions of relatively warm Circumpolar Deep <span class="hlt">Water</span> and reduced vertical mixing of heat in the <span class="hlt">water</span> column. A complete heat budget analysis is performed for the <span class="hlt">Antarctic</span> shelf region as well as for six subdomains and three depth ranges (0-100 m, 100-700 m, and 700-1000 m). The results show that certain regions of the <span class="hlt">Antarctic</span> shelf are more susceptible to large CO2-forced warming. These findings have implications for future <span class="hlt">Antarctic</span> Ice Sheet mass loss and SLR, and can provide more detailed and accurate ocean boundary conditions for dynamical ice sheet models. In Appendix C, we use CM2.6 to examine the connections among ocean freshening and the magnitude and location of ocean warming on the <span class="hlt">Antarctic</span> shelf. We find that CO2 forcing freshens the <span class="hlt">Antarctic</span> shelf seas via increases in local precipitation, sea ice loss, liquid runoff, and iceberg calving. The freshening induces three heat budget-relevant responses: (1) reduced vertical mixing; (2) strengthening of the <span class="hlt">Antarctic</span> Slope Front (ASF); and (3) increased eddy kinetic energy (EKE) near the ASF. First, heat can accumulate at depth (100-1000 m) as freshening increases the vertical stratification on the shelf and reduces upward mixing of heat associated with diffusion and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70019625','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70019625"><span>Minor elements in Quaternary sediment from the Sea of Japan: a record of surface-<span class="hlt">water</span> productivity and <span class="hlt">intermediate-water</span> redox conditions</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.; Isaacs, C.M.</p> <p>1995-01-01</p> <p>Records six episodes of high accumulation rates of Cd, Cr, Cu, Mo, Ni, U, V, and Zn. The high rates correspond to periods of sulfate reduction in the <span class="hlt">water</span> column at the <span class="hlt">intermediate</span> depth of Oki Ridge; the intervening low values correspond to periods of denitrification and oxygen respiration. The maxima have a period of 41 k.y., the youngest having an age of 1.10 Ma. -from Authors</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/2017AGUFMIN13C0077N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMIN13C0077N"><span>The United States <span class="hlt">Antarctic</span> Program Data Center (USAP-DC): Recent Developments</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nitsche, F. O.; Bauer, R.; Arko, R. A.; Shane, N.; Carbotte, S. M.; Scambos, T.</p> <p>2017-12-01</p> <p><span class="hlt">Antarctic</span> earth and environmental science data are highly valuable, often unique research assets. They are acquired with substantial and expensive logistical effort, frequently in areas that will not be re-visited for many years. The data acquired in support of <span class="hlt">Antarctic</span> research span a wide range of disciplines. Historically, data management for the US <span class="hlt">Antarctic</span> Program (USAP) has made use of existing disciplinary data centers, and the international <span class="hlt">Antarctic</span> Master Directory (AMD) has served as a central metadata catalog linking to data files hosted in these external repositories. However, disciplinary repositories do not exist for all USAP-generated data types and often it is unclear what repositories are appropriate, leading to many datasets being served locally from scientist's websites or not available at all. The USAP Data Center (USAP-DC; www.usap-dc.org), operated as part of the Interdisciplinary Earth Data Alliance (IEDA), contributes to the broader preservation of research data acquired with funding from NSF's Office of Polar Programs by providing a repository for diverse data from the <span class="hlt">Antarctic</span> region. USAP-DC hosts data that spans the range of <span class="hlt">Antarctic</span> research from snow radar to volcano observatory imagery to penguin counts to meteorological model outputs. Data services include data documentation, long-term preservation, and web publication, as well as scientist support for registration of data descriptions into the AMD in fulfillment of US obligations under the International <span class="hlt">Antarctic</span> Treaty. In Spring 2016, USAP-DC and the NSIDC began a new collaboration to consolidate data services for <span class="hlt">Antarctic</span> investigators and to integrate the NSF-funded glaciology collection at NSIDC with the collection hosted by USAP-DC. Investigator submissions for NSF's Glaciology program now make use of USAP-DC's web submission tools, providing a uniform interface for <span class="hlt">Antarctic</span> investigators. The tools have been redesigned to collect a broader range of metadata. Each data</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EOSTr..94..399S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EOSTr..94..399S"><span><span class="hlt">Antarctic</span> Projects Stymied by the Shutdown</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>2013-10-01</p> <p>The U.S. federal government shutdown coincided with the beginning of the <span class="hlt">Antarctic</span> austral summer research window, and many scientists told Eos they are deeply concerned about the impacts on research there. John Priscu, a lead principal investigator with the Whillans Ice Stream Subglacial Access Research Drilling (WISSARD) project in West Antarctica, said the government shutdown "threw us a curve that I did not anticipate or plan for." Pricsu, who has spent 30 seasons working in Antarctica under federal funding, said that a hole in the project's long-term data set "will have a major impact on the models we are developing to examine climate-induced changes" in <span class="hlt">Antarctic</span> ecosystems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25336089','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25336089"><span>Invited review: climate change impacts in polar regions: lessons from <span class="hlt">Antarctic</span> moss bank archives.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Royles, Jessica; Griffiths, Howard</p> <p>2015-03-01</p> <p>Mosses are the dominant plants in polar and boreal regions, areas which are experiencing rapid impacts of regional warming. Long-term monitoring programmes provide some records of the rate of recent climate change, but moss peat banks contain an unrivalled temporal record of past climate change on terrestrial plant <span class="hlt">Antarctic</span> systems. We summarise the current understanding of climatic proxies and determinants of moss growth for contrasting continental and maritime <span class="hlt">Antarctic</span> regions, as informed by 13C and 18O signals in organic material. Rates of moss accumulation are more than three times higher in the maritime <span class="hlt">Antarctic</span> than continental Antarctica with growing season length being a critical determinant of growth rate, and high carbon isotope discrimination values reflecting optimal hydration conditions. Correlation plots of 13C and 18O values show that species (Chorisodontium aciphyllum / Polytrichum strictum) and growth form (hummock / bank) are the major determinants of measured isotope ratios. The interplay between moss growth form, photosynthetic physiology, <span class="hlt">water</span> status and isotope composition are compared with developments of secondary proxies, such as chlorophyll fluorescence. These approaches provide a framework to consider the potential impact of climate change on terrestrial <span class="hlt">Antarctic</span> habitats as well as having implications for future studies of temperate, boreal and Arctic peatlands. There are many urgent ecological and environmental problems in the Arctic related to mosses in a changing climate, but the geographical ranges of species and life-forms are difficult to track individually. Our goal was to translate what we have learned from the more simple systems in Antarctica, for application to Arctic habitats. © 2014 John Wiley & Sons Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E%26PSL.481..316M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26PSL.481..316M"><span>Precipitation regime influence on oxygen triple-isotope distributions in <span class="hlt">Antarctic</span> precipitation and ice cores</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Miller, Martin F.</p> <p>2018-01-01</p> <p>The relative abundance of 17O in meteoric precipitation is usually reported in terms of the 17O-excess parameter. Variations of 17O-excess in <span class="hlt">Antarctic</span> precipitation and ice cores have hitherto been attributed to normalised relative humidity changes at the moisture source region, or to the influence of a temperature-dependent supersaturation-controlled kinetic isotope effect during in-cloud ice formation below -20 °C. Neither mechanism, however, satisfactorily explains the large range of 17O-excess values reported from measurements. A different approach, based on the regression characteristics of 103 ln (1 +δ17 O) versus 103 ln (1 +δ18 O), is applied here to previously published isotopic data sets. The analysis indicates that clear-sky precipitation ('diamond dust'), which occurs widely in inland Antarctica, is characterised by an unusual relative abundance of 17O, distinct from that associated with cloud-derived, synoptic snowfall. Furthermore, this distinction appears to be largely preserved in the ice core record. The respective mass contributions to snowfall accumulation - on both temporal and spatial scales - provides the basis of a simple, first-order explanation for the observed oxygen triple-isotope ratio variations in <span class="hlt">Antarctic</span> precipitation, surface snow and ice cores. Using this approach, it is shown that precipitation during the last major deglaciation, both in western Antarctica at the West <span class="hlt">Antarctic</span> Ice Sheet (WAIS) Divide and at Vostok on the eastern <span class="hlt">Antarctic</span> plateau, consisted essentially of diamond dust only, despite a large temperature differential (and thus different <span class="hlt">water</span> vapour supersaturation conditions) at the two locations. In contrast, synoptic snowfall events dominate the accumulation record throughout the Holocene at both sites.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005AGUSM.C42A..01K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005AGUSM.C42A..01K"><span>The Scientific Committee on <span class="hlt">Antarctic</span> Research (SCAR) in the IPY 2007-2009</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kennicutt, M. C.; Wilson, T. J.; Summerhayes, C.</p> <p>2005-05-01</p> <p>The Scientific Committee on <span class="hlt">Antarctic</span> Research (SCAR) initiates, develops, and coordinates international scientific research in the <span class="hlt">Antarctic</span> region. SCAR is assuming a leadership position in the IPY primarily through its five major Scientific Research Programs; ACE, SALE, EBA, AGCS, and ICESTAR; which will be briefly described.<span class="hlt">Antarctic</span> Climate Evolution (ACE) promotes the exchange of data and ideas between research groups focusing on the evolution of Antarctica's climate system and ice sheet. The program will: (1) quantitatively assess the climate and glacial history of Antarctica; (2) identify the processes which govern <span class="hlt">Antarctic</span> change and feed back around the globe; (3) improve our ability to model past changes in Antarctica; and (4)document past change to predict future change in Antarctica. Subglacial <span class="hlt">Antarctic</span> Lake Environments (SALE) promotes, facilitates, and champions cooperation and collaboration in the exploration and study of subglacial environments in Antarctica. SALE intends to understand the complex interplay of biological, geological, chemical, glaciological, and physical processes within subglacial lake environments through coordinated international research teams. Evolution and Biodiversity in the <span class="hlt">Antarctic</span> (EBA) will use a suite of modern techniques and interdisciplinary approaches, to explore the evolutionary history of selected modern <span class="hlt">Antarctic</span> biota, examine how modern biological diversity in the <span class="hlt">Antarctic</span> influences the way present-day ecosystems function, and thereby predict how the biota may respond to future environmental change. Antarctica and the Global Climate System (AGCS) will investigate the nature of the atmospheric and oceanic linkages between the climate of the <span class="hlt">Antarctic</span> and the rest of the Earth system, and the mechanisms involved therein. A combination of modern instrumented records of atmospheric and oceanic conditions, and the climate signals held within ice cores will be used to understand past and future climate</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23045792','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23045792"><span>Medical supplies for the expeditions of the heroic age of <span class="hlt">Antarctic</span> exploration: introduction.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Guly, H R</p> <p>2012-06-01</p> <p>During the heroic age of <span class="hlt">Antarctic</span> exploration (1895-1922) there were at least 18 expeditions to the <span class="hlt">Antarctic</span> lasting between 18 and 30 months. This is an introduction to a series of articles about the drugs taken and used in the <span class="hlt">Antarctic</span> at this time. Most of the information relates to the expeditions of Robert Scott and Ernest Shackleton and the main supplier of medical equipment was Burroughs Wellcome and Co. This article also describes the medical cases that were taken to the <span class="hlt">Antarctic</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22914090','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22914090"><span>Recent <span class="hlt">Antarctic</span> Peninsula warming relative to Holocene climate and ice-shelf history.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mulvaney, Robert; Abram, Nerilie J; Hindmarsh, Richard C A; Arrowsmith, Carol; Fleet, Louise; Triest, Jack; Sime, Louise C; Alemany, Olivier; Foord, Susan</p> <p>2012-09-06</p> <p>Rapid warming over the past 50 years on the <span class="hlt">Antarctic</span> Peninsula is associated with the collapse of a number of ice shelves and accelerating glacier mass loss. In contrast, warming has been comparatively modest over West Antarctica and significant changes have not been observed over most of East Antarctica, suggesting that the ice-core palaeoclimate records available from these areas may not be representative of the climate history of the <span class="hlt">Antarctic</span> Peninsula. Here we show that the <span class="hlt">Antarctic</span> Peninsula experienced an early-Holocene warm period followed by stable temperatures, from about 9,200 to 2,500 years ago, that were similar to modern-day levels. Our temperature estimates are based on an ice-core record of deuterium variations from James Ross Island, off the northeastern tip of the <span class="hlt">Antarctic</span> Peninsula. We find that the late-Holocene development of ice shelves near James Ross Island was coincident with pronounced cooling from 2,500 to 600 years ago. This cooling was part of a millennial-scale climate excursion with opposing anomalies on the eastern and western sides of the <span class="hlt">Antarctic</span> Peninsula. Although warming of the northeastern <span class="hlt">Antarctic</span> Peninsula began around 600 years ago, the high rate of warming over the past century is unusual (but not unprecedented) in the context of natural climate variability over the past two millennia. The connection shown here between past temperature and ice-shelf stability suggests that warming for several centuries rendered ice shelves on the northeastern <span class="hlt">Antarctic</span> Peninsula vulnerable to collapse. Continued warming to temperatures that now exceed the stable conditions of most of the Holocene epoch is likely to cause ice-shelf instability to encroach farther southward along the <span class="hlt">Antarctic</span> Peninsula.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015Natur.526..421G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015Natur.526..421G"><span>The multi-millennial <span class="hlt">Antarctic</span> commitment to future sea-level rise</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Golledge, N. R.; Kowalewski, D. E.; Naish, T. R.; Levy, R. H.; Fogwill, C. J.; Gasson, E. G. W.</p> <p>2015-10-01</p> <p>Atmospheric warming is projected to increase global mean surface temperatures by 0.3 to 4.8 degrees Celsius above pre-industrial values by the end of this century. If anthropogenic emissions continue unchecked, the warming increase may reach 8-10 degrees Celsius by 2300 (ref. 2). The contribution that large ice sheets will make to sea-level rise under such warming scenarios is difficult to quantify because the equilibrium-response timescale of ice sheets is longer than those of the atmosphere or ocean. Here we use a coupled ice-sheet/ice-shelf model to show that if atmospheric warming exceeds 1.5 to 2 degrees Celsius above present, collapse of the major <span class="hlt">Antarctic</span> ice shelves triggers a centennial- to millennial-scale response of the <span class="hlt">Antarctic</span> ice sheet in which enhanced viscous flow produces a long-term commitment (an unstoppable contribution) to sea-level rise. Our simulations represent the response of the present-day <span class="hlt">Antarctic</span> ice-sheet system to the oceanic and climatic changes of four representative concentration pathways (RCPs) from the Fifth Assessment Report of the Intergovernmental Panel on Climate Change. We find that substantial <span class="hlt">Antarctic</span> ice loss can be prevented only by limiting greenhouse gas emissions to RCP 2.6 levels. Higher-emissions scenarios lead to ice loss from <span class="hlt">Antarctic</span> that will raise sea level by 0.6-3 metres by the year 2300. Our results imply that greenhouse gas emissions in the next few decades will strongly influence the long-term contribution of the <span class="hlt">Antarctic</span> ice sheet to global sea level.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.1406G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.1406G"><span>The multi-millennial <span class="hlt">Antarctic</span> commitment to future sea-level rise</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Golledge, Nicholas R.; Kowalewski, Douglas E.; Naish, Timothy R.; Levy, Richard H.; Fogwill, Christopher J.; Gasson, Edward G. W.</p> <p>2016-04-01</p> <p>Atmospheric warming is projected to increase global mean surface temperatures by 0.3 to 4.8 degrees Celsius above present values by the end of this century (Collins et al., 2013). If anthropogenic emissions continue unchecked, the warming increase may reach 8-10 degrees Celsius by 2300 (Rogelj et al., 2012). The contribution that large ice sheets will make to sea-level rise under such warming scenarios is difficult to quantify because the equilibrium-response timescale of ice sheets is longer than those of the atmosphere or ocean. Here we use a coupled ice-sheet/ice-shelf model to show that if atmospheric warming exceeds 1.5 to 2 degrees Celsius above present, collapse of the major <span class="hlt">Antarctic</span> ice shelves triggers a centennial- to millennial-scale response of the <span class="hlt">Antarctic</span> ice sheet in which enhanced viscous flow produces a long-term commitment (an unstoppable contribution) to sea-level rise. Our simulations represent the response of the present-day <span class="hlt">Antarctic</span> ice-sheet system to the oceanic and climatic changes of four representative concentration pathways (RCPs) from the Fifth Assessment Report of the Intergovernmental Panel on Climate Change (Collins et al., 2013). We find that substantial <span class="hlt">Antarctic</span> ice loss can be prevented only by limiting greenhouse gas emissions to RCP 2.6 levels. Higher-emissions scenarios lead to ice loss from <span class="hlt">Antarctic</span> that will raise sea level by 0.6-3 metres by the year 2300. Our results imply that greenhouse gas emissions in the next few decades will strongly influence the long-term contribution of the <span class="hlt">Antarctic</span> ice sheet to global sea level.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26469052','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26469052"><span>The multi-millennial <span class="hlt">Antarctic</span> commitment to future sea-level rise.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Golledge, N R; Kowalewski, D E; Naish, T R; Levy, R H; Fogwill, C J; Gasson, E G W</p> <p>2015-10-15</p> <p>Atmospheric warming is projected to increase global mean surface temperatures by 0.3 to 4.8 degrees Celsius above pre-industrial values by the end of this century. If anthropogenic emissions continue unchecked, the warming increase may reach 8-10 degrees Celsius by 2300 (ref. 2). The contribution that large ice sheets will make to sea-level rise under such warming scenarios is difficult to quantify because the equilibrium-response timescale of ice sheets is longer than those of the atmosphere or ocean. Here we use a coupled ice-sheet/ice-shelf model to show that if atmospheric warming exceeds 1.5 to 2 degrees Celsius above present, collapse of the major <span class="hlt">Antarctic</span> ice shelves triggers a centennial- to millennial-scale response of the <span class="hlt">Antarctic</span> ice sheet in which enhanced viscous flow produces a long-term commitment (an unstoppable contribution) to sea-level rise. Our simulations represent the response of the present-day <span class="hlt">Antarctic</span> ice-sheet system to the oceanic and climatic changes of four representative concentration pathways (RCPs) from the Fifth Assessment Report of the Intergovernmental Panel on Climate Change. We find that substantial <span class="hlt">Antarctic</span> ice loss can be prevented only by limiting greenhouse gas emissions to RCP 2.6 levels. Higher-emissions scenarios lead to ice loss from <span class="hlt">Antarctic</span> that will raise sea level by 0.6-3 metres by the year 2300. Our results imply that greenhouse gas emissions in the next few decades will strongly influence the long-term contribution of the <span class="hlt">Antarctic</span> ice sheet to global sea level.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26102557','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26102557"><span>Transcriptome of the <span class="hlt">Antarctic</span> brooding gastropod mollusc Margarella antarctica.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Clark, Melody S; Thorne, Michael A S</p> <p>2015-12-01</p> <p>454 RNA-Seq transcriptome data were generated from foot tissue of the <span class="hlt">Antarctic</span> brooding gastropod mollusc Margarella antarctica. A total of 6195 contigs were assembled de novo, providing a useful resource for researchers with an interest in <span class="hlt">Antarctic</span> marine species, phylogenetics and mollusc biology, especially shell production. Copyright © 2015 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP41C1320R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP41C1320R"><span>Bering Sea Nd isotope records of North Pacific <span class="hlt">Intermediate</span> <span class="hlt">Water</span> circulation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rabbat, C.; Knudson, K. P.; Goldstein, S. L.</p> <p>2017-12-01</p> <p>North Pacific <span class="hlt">Intermediate</span> <span class="hlt">Water</span> (NPIW) is the primary <span class="hlt">water</span> mass associated with Pacific meridional overturning circulation. While the relationship between Atlantic meridional overturning circulation and climate has been extensively studied, a lack of suitable sediment cores has limited past investigations of North Pacific climate and NPIW variability. Integrated Ocean Drilling Program Site U1342 (818 m <span class="hlt">water</span> depth) on Bower's Ridge in the Bering Sea is located at a sensitive depth for detecting changes in NPIW, and it is the only available sub-arctic North Pacific site that offers long, continuous core recovery, relatively high sedimentation rates, excellent foraminifera preservation, and a well-constrained age model over multiple glacial-interglacial cycles. Previous work at Site U1342 from Knudson and Ravelo (2015), using non-quantitative circulation proxies, provides evidence for enhanced NPIW formation during extreme glacials associated with the closure of the Bering Strait and suggest that NPIW was formed locally within the Bering Sea. Our work builds on the potential importance of these results and applies more robust and potentially quantitative circulation proxies to constrain NPIW variability. Here, we present new records of NPIW circulation from Site U1342 based on Nd isotope analyses on fish debris and Fe-Mn encrusted foraminifera, which serve as semi-quantitative "<span class="hlt">water</span> mass tracers." Weak Bering Sea NPIW formation and ventilation are reflected by relatively lower eNd values indicative of open subarctic North Pacific <span class="hlt">waters</span>, which are presently predominant, whereas enhanced Bering Sea NPIW formation and ventilation are be reflected by relatively higher eNd values due to the input of Nd from regional volcanic rocks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008EOSTr..89..406B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008EOSTr..89..406B"><span><span class="hlt">Antarctic</span> Treaty Summit to Focus on Global Science Policy Lessons</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Berkman, Paul Arthur; Walton, David W. H.; Weiler, C. Susan</p> <p>2008-10-01</p> <p>The <span class="hlt">Antarctic</span> Treaty Summit, which will coincide with the fiftieth anniversary of the treaty's signing, will be held at the Smithsonian Institution's National Museum of Natural History, in Washington, D. C., from 30 November to 3 December 2009. The summit will provide an open international forum for scientists, legislators, lawyers, administrators, educators, students, corporate executives, historians, and other members of global civil society to explore science policy achievements from the first 50 years of the <span class="hlt">Antarctic</span> Treaty. In addition, the summit will complement official government celebrations of the <span class="hlt">Antarctic</span> Treaty anniversary that do not include public participation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014Ge%26Ae..54..269R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014Ge%26Ae..54..269R"><span>First geomagnetic measurements in the <span class="hlt">Antarctic</span> region</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Raspopov, O. M.; Demina, I. M.; Meshcheryakov, V. V.</p> <p>2014-05-01</p> <p>Based on data from literature and archival sources, we have further processed and analyzed the results of geomagnetic measurements made during the 1772-1775 Second World Expedition by James Cook and the 1819-1821 overseas <span class="hlt">Antarctic</span> Expedition by Russian mariners Bellingshausen and Lazarev. Comparison with the GUFM historical model showed that there are systematic differences in the spatial structure of both the declination and its secular variation. The results obtained can serve as a basis for the construction of regional models of the geomagnetic field for the <span class="hlt">Antarctic</span> region.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.1973R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.1973R"><span>Quantarctica: A Unique, Open, Standalone GIS Package for <span class="hlt">Antarctic</span> Research and Education</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Roth, George; Matsuoka, Kenichi; Skoglund, Anders; Melvær, Yngve; Tronstad, Stein</p> <p>2017-04-01</p> <p>The Norwegian Polar Institute has developed Quantarctica (http://quantarctica.npolar.no), an open GIS package for use by the international <span class="hlt">Antarctic</span> community. Quantarctica includes a wide range of cartographic basemap layers, geophysical and glaciological datasets, and satellite imagery in standardized open file formats with a consistent <span class="hlt">Antarctic</span> map projection and customized layer and labeling styles for quick, effective cartography. Quantarctica's strengths as an open science platform lie in 1) The complete, ready-to-use data package which includes full-resolution, original-quality vector and raster data, 2) A policy for freely-redistributable and modifiable data including all metadata and citations, and 3) QGIS, a free, full-featured, modular, offline-capable open-source GIS suite with a rapid and active development and support community. The Quantarctica team is actively incorporating more up-to-date, peer-reviewed, freely distributable pan-<span class="hlt">Antarctic</span> geospatial datasets for the next version release in 2017. As part of this ongoing development, we are investigating the best approaches for quickly and seamlessly distributing new and updated data to users, storing datasets in efficient, open file formats while maintaining full data integrity, and coexisting with numerous online data portals in a way that most actively benefits the <span class="hlt">Antarctic</span> community. A recent survey of Quantarctica users showed broad geographical adoption among <span class="hlt">Antarctic</span> Treaty countries, including those outside the large US and UK <span class="hlt">Antarctic</span> programs. Maps and figures produced by Quantarctica have also appeared in open-access journals and outside of the formal scientific community on popular science and GIS blogs. Our experience with the Quantarctica project has shown the tremendous value of education and outreach, not only in promoting open software, data formats, and practices, but in empowering <span class="hlt">Antarctic</span> science groups to more effectively use GIS and geospatial data. Open practices are</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMIN23E..05R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMIN23E..05R"><span>Quantarctica: A Unique, Open, Standalone GIS Package for <span class="hlt">Antarctic</span> Research and Education</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Roth, G.; Matsuoka, K.; Skoglund, A.; Melvaer, Y.; Tronstad, S.</p> <p>2016-12-01</p> <p>The Norwegian Polar Institute has developed Quantarctica, an open GIS package for use by the international <span class="hlt">Antarctic</span> community. Quantarctica includes a wide range of cartographic basemap layers, geophysical and glaciological datasets, and satellite imagery in standardized file formats with a consistent <span class="hlt">Antarctic</span> map projection and customized layer and labeling styles for quick, effective cartography. Quantarctica's strengths as an open science platform lie in 1) The complete, ready-to-use data package which includes full-resolution, original-quality vector and raster data, 2) A policy for freely-redistributable and modifiable data including all metadata and citations, and 3) QGIS, a free, full-featured, modular, offline-capable open-source GIS suite with a rapid and active development and support community. The Quantarctica team is actively seeking new contributions of peer-reviewed, freely distributable pan-<span class="hlt">Antarctic</span> geospatial datasets for the next version release in 2017. As part of this ongoing development, we are investigating the best approaches for quickly and seamlessly distributing new and updated data to users, storing datasets in efficient file formats while maintaining full quality, and coexisting with numerous online data portals in a way that most actively benefits the <span class="hlt">Antarctic</span> community. A recent survey of Quantarctica users showed broad geographical adoption among <span class="hlt">Antarctic</span> Treaty countries, including those outside the large US and UK <span class="hlt">Antarctic</span> programs. Maps and figures produced by Quantarctica have also appeared in open-access journals and outside of the formal scientific community on popular science and GIS blogs. Our experience with the Quantarctica project has shown the tremendous value of education and outreach, not only in promoting open software, data formats, and practices, but in empowering <span class="hlt">Antarctic</span> science groups to more effectively use GIS and geospatial data. Open practices are making a huge impact in <span class="hlt">Antarctic</span> GIS, where individual</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001AGUFMIP22B0701S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001AGUFMIP22B0701S"><span>Scientific Applications of two U.S. <span class="hlt">Antarctic</span> Program Projects at NSIDC</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Scharfen, G. R.; Bauer, R. J.</p> <p>2001-12-01</p> <p>The National Snow and Ice Data Center maintains two <span class="hlt">Antarctic</span> science data management programs supporting both the efforts of Principal Investigators (PIs), and the science that is funded by the NSF Office of Polar Programs. These programs directly relate to the OPP "Guidelines and Award Conditions for Scientific Data", which identify the conditions for awards and responsibilities of PIs regarding the archival of data, and submission of metadata, resulting from their NSF OPP grants. The U.S. <span class="hlt">Antarctic</span> Data Coordination Center (USADCC) is funded by NSF to assist PIs as they meet these requirements, and to provide a U.S. focal point for the <span class="hlt">Antarctic</span> Master Directory, a web-based searchable directory of <span class="hlt">Antarctic</span> scientific data. The USADCC offers access to free, easy-to-use online tools that PIs can use to create the data descriptions that the NSF policy data requires. We provide advice to PIs on how to meet the data policy requirements, and can answer specific questions on related issues. Scientists can access data set descriptions submitted to the <span class="hlt">Antarctic</span> Master Directory, by thousands of scientists around the world, from the USADCC web pages. The USADCC website is at http://nsidc.org/NSF/USADCC/. The <span class="hlt">Antarctic</span> Glaciological Data Center (AGDC) is funded by NSF to archive and distribute data collected by the NSF <span class="hlt">Antarctic</span> Glaciology Program and related cryospheric investigations. The AGDC contains data sets collected by individual investigators on specific grants, and compiled products assembled from many different PI data sets, published literature, and other sources. Data sets are available electronically and include access to the data, plus useful documentation, citation information about the PI(s), locator maps, derived images and references. The AGDC website is at http://nsidc.org/NSF/AGDC/. The utility of both of these projects for scientists is illustrated by a typical user-driven case study to research, obtain and use <span class="hlt">Antarctic</span> data for a science</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.5256R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.5256R"><span>Stable isotopes and <span class="hlt">Antarctic</span> moss banks: Plants and soil microbes respond to recent warming on the <span class="hlt">Antarctic</span> Peninsula</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Royles, Jessica; Amesbury, Matthew; Ogée, Jérôme; Wingate, Lisa; Convey, Peter; Hodgson, Dominic; Griffiths, Howard; Leng, Melanie; Charman, Dan</p> <p>2014-05-01</p> <p>The <span class="hlt">Antarctic</span> Peninsula is one of the most rapidly warming regions on Earth, with air temperature increases of as much as 3°C recorded since the 1950s. However, the longer-term context of this change is limited and existing records, largely relying on ice core data, are not suitably located to be able to trace the spatial signature of change over time. We are working on a project exploiting stable isotope records preserved in moss peat banks spanning 10 degrees of latitude along the <span class="hlt">Antarctic</span> Peninsula as an archive of late Holocene climate variability. Here we present a unique time series of past moss growth and soil microbial activity that has been produced from a 150 year old moss bank at Lazarev Bay, Alexander Island (69°S), a site at the southern limit of significant plant growth in the <span class="hlt">Antarctic</span> Peninsula region. These moss banks are ideal archives for palaeoclimate research as they are well-preserved by freezing, generally monospecific, easily dated by radiocarbon techniques, and have sufficiently high accumulation rates to permit decadal resolution. We use accumulation rates, cellulose δ13C and fossil testate amoebae to show that growth rates, assimilation and microbial productivity rose rapidly in the 1960s, consistent with temperature change, although recently may have stalled, concurrent with other evidence. The increase in biological activity is unprecedented in the last 150 years. Along with work completed on Signy Island (60°S), in the South Orkney Islands, in which we used carbon isotope evidence to show recent climate-related enhancement of CO2 assimilation and peat accumulation rates in Antarctica, the observed relationships between moss growth, microbial activity and climate suggests that moss bank records have the potential to test the regional expression of temperature variability shown by instrumental data on the <span class="hlt">Antarctic</span> Peninsula over centennial to millennial timescales, by providing long-term records of summer growth conditions</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PolSc..10..123R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PolSc..10..123R"><span>Antibiotic resistance in Escherichia coli strains isolated from <span class="hlt">Antarctic</span> bird feces, <span class="hlt">water</span> from inside a wastewater treatment plant, and seawater samples collected in the <span class="hlt">Antarctic</span> Treaty area</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rabbia, Virginia; Bello-Toledo, Helia; Jiménez, Sebastián; Quezada, Mario; Domínguez, Mariana; Vergara, Luis; Gómez-Fuentes, Claudio; Calisto-Ulloa, Nancy; González-Acuña, Daniel; López, Juana; González-Rocha, Gerardo</p> <p>2016-06-01</p> <p>Antibiotic resistance is a problem of global concern and is frequently associated with human activity. Studying antibiotic resistance in bacteria isolated from pristine environments, such as Antarctica, extends our understanding of these fragile ecosystems. Escherichia coli strains, important fecal indicator bacteria, were isolated on the Fildes Peninsula (which has the strongest human influence in Antarctica), from seawater, bird droppings, and <span class="hlt">water</span> samples from inside a local wastewater treatment plant. The strains were subjected to molecular typing with pulsed-field gel electrophoresis to determine their genetic relationships, and tested for antibiotic susceptibility with disk diffusion tests for several antibiotic families: β-lactams, quinolones, aminoglycosides, tetracyclines, phenicols, and trimethoprim-sulfonamide. The highest E. coli count in seawater samples was 2400 cfu/100 mL. Only strains isolated from seawater and the wastewater treatment plant showed any genetic relatedness between groups. Strains of both these groups were resistant to β-lactams, aminoglycosides, tetracycline, and trimethoprim-sulfonamide.In contrast, strains from bird feces were susceptible to all the antibiotics tested. We conclude that naturally occurring antibiotic resistance in E. coli strains isolated from <span class="hlt">Antarctic</span> bird feces is rare and the bacterial antibiotic resistance found in seawater is probably associated with discharged treated wastewater originating from Fildes Peninsula treatment plants.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70026949','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70026949"><span>Influence of northwest Pacific productivity on North Pacific <span class="hlt">Intermediate</span> <span class="hlt">Water</span> oxygen concentrations during the Bølling-Ållerød interval (14.7-12.9 ka)</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Crusius, John; Pedersen, Thomas F.; Kienast, Stephanie; Keigwin, Lloyd D.; Labeyrie, Laurent</p> <p>2004-01-01</p> <p>Elevated productivity in the northwest Pacific is suggested as a new possible control driving past intervals of low-O2 <span class="hlt">intermediate</span> <span class="hlt">water</span> along the western continental margin of North America. According to this mechanism, O2 consumption would occur near the site of formation of North Pacific <span class="hlt">Intermediate</span> <span class="hlt">Water</span> (NPIW), due to increased respiration of organic carbon in response to a high-productivity event. Evidence is provided for such a productivity increase during the Bølling-Ållerød interval (14.7–12.9 ka), a time when laminated sediments were deposited along the northern California margin. By this mechanism, low-O2 events in <span class="hlt">intermediate</span> <span class="hlt">waters</span> off the western North American margin could occur without significant changes in the rate of NPIW ventilation.</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/2010GeoRL..37.8703C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010GeoRL..37.8703C"><span>Twentieth century bipolar seesaw of the Arctic and <span class="hlt">Antarctic</span> surface air temperatures</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chylek, Petr; Folland, Chris K.; Lesins, Glen; Dubey, Manvendra K.</p> <p>2010-04-01</p> <p>Understanding the phase relationship between climate changes in the Arctic and <span class="hlt">Antarctic</span> regions is essential for our understanding of the dynamics of the Earth's climate system. In this paper we show that the 20th century de-trended Arctic and <span class="hlt">Antarctic</span> temperatures vary in anti-phase seesaw pattern - when the Arctic warms the Antarctica cools and visa versa. This is the first time that a bi-polar seesaw pattern has been identified in the 20th century Arctic and <span class="hlt">Antarctic</span> temperature records. The Arctic (<span class="hlt">Antarctic</span>) de-trended temperatures are highly correlated (anti-correlated) with the Atlantic Multi-decadal Oscillation (AMO) index suggesting the Atlantic Ocean as a possible link between the climate variability of the Arctic and <span class="hlt">Antarctic</span> regions. Recent accelerated warming of the Arctic results from a positive reinforcement of the linear warming trend (due to an increasing concentration of greenhouse gases and other possible forcings) by the warming phase of the multidecadal climate variability (due to fluctuations of the Atlantic Ocean circulation).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3459913','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3459913"><span>Effects of Late-Cenozoic Glaciation on Habitat Availability in <span class="hlt">Antarctic</span> Benthic Shrimps (Crustacea: Decapoda: Caridea)</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Dambach, Johannes; Thatje, Sven; Rödder, Dennis; Basher, Zeenatul; Raupach, Michael J.</p> <p>2012-01-01</p> <p>Marine invertebrates inhabiting the high <span class="hlt">Antarctic</span> continental shelves are challenged by disturbance of the seafloor by grounded ice, low but stable <span class="hlt">water</span> temperatures and variable food availability in response to seasonal sea-ice cover. Though a high diversity of life has successfully adapted to such conditions, it is generally agreed that during the Last Glacial Maximum (LGM) the large-scale cover of the Southern Ocean by multi-annual sea ice and the advance of the continental ice sheets across the shelf faced life with conditions, exceeding those seen today by an order of magnitude. Conditions prevailing at the LGM may have therefore acted as a bottleneck event to both the ecology as well as genetic diversity of today's fauna. Here, we use for the first time specific Species Distribution Models (SDMs) for marine arthropods of the Southern Ocean to assess effects of habitat contraction during the LGM on the three most common benthic caridean shrimp species that exhibit a strong depth zonation on the <span class="hlt">Antarctic</span> continental shelf. While the shallow-<span class="hlt">water</span> species Chorismus antarcticus and Notocrangon antarcticus were limited to a drastically reduced habitat during the LGM, the deep-<span class="hlt">water</span> shrimp Nematocarcinus lanceopes found refuge in the Southern Ocean deep sea. The modeling results are in accordance with genetic diversity patterns available for C. antarcticus and N. lanceopes and support the hypothesis that habitat contraction at the LGM resulted in a loss of genetic diversity in shallow <span class="hlt">water</span> benthos. PMID:23029463</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23029463','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23029463"><span>Effects of late-cenozoic glaciation on habitat availability in <span class="hlt">Antarctic</span> benthic shrimps (Crustacea: Decapoda: Caridea).</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Dambach, Johannes; Thatje, Sven; Rödder, Dennis; Basher, Zeenatul; Raupach, Michael J</p> <p>2012-01-01</p> <p>Marine invertebrates inhabiting the high <span class="hlt">Antarctic</span> continental shelves are challenged by disturbance of the seafloor by grounded ice, low but stable <span class="hlt">water</span> temperatures and variable food availability in response to seasonal sea-ice cover. Though a high diversity of life has successfully adapted to such conditions, it is generally agreed that during the Last Glacial Maximum (LGM) the large-scale cover of the Southern Ocean by multi-annual sea ice and the advance of the continental ice sheets across the shelf faced life with conditions, exceeding those seen today by an order of magnitude. Conditions prevailing at the LGM may have therefore acted as a bottleneck event to both the ecology as well as genetic diversity of today's fauna. Here, we use for the first time specific Species Distribution Models (SDMs) for marine arthropods of the Southern Ocean to assess effects of habitat contraction during the LGM on the three most common benthic caridean shrimp species that exhibit a strong depth zonation on the <span class="hlt">Antarctic</span> continental shelf. While the shallow-<span class="hlt">water</span> species Chorismus antarcticus and Notocrangon antarcticus were limited to a drastically reduced habitat during the LGM, the deep-<span class="hlt">water</span> shrimp Nematocarcinus lanceopes found refuge in the Southern Ocean deep sea. The modeling results are in accordance with genetic diversity patterns available for C. antarcticus and N. lanceopes and support the hypothesis that habitat contraction at the LGM resulted in a loss of genetic diversity in shallow <span class="hlt">water</span> benthos.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002DSRII..49..869C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002DSRII..49..869C"><span>Mesozooplankton distribution and grazing during the productive season in the Northwest <span class="hlt">Antarctic</span> Peninsula (FRUELA cruises)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cabal, Jesús A.; Alvarez-Marqués, Florentina; Acuña, José L.; Quevedo, Mario; Gonzalez-Quirós, Rafael; Huskin, Ignacio; Fernández, Diego; del Valle, Carlos Rodriguez; Anadón, Ricardo</p> <p></p> <p>Mesozooplankton distribution and community structure in the Bellinghausen-Bransfield sector of the <span class="hlt">Antarctic</span> Ocean were investigated during the FRUELA cruises (December 1995-February 1996). Total mesozooplankton biomass ranged between 0.015 and 1.43 g C m -2. Biomass was higher in the Southern boundary of the <span class="hlt">Antarctic</span> Circumpolar Current (SbyACC) area and in coastal <span class="hlt">waters</span> of the <span class="hlt">Antarctic</span> Peninsula. Total mesozooplankton abundance ranged from 0.4×10 3 to 1.3×10 5 individuals m -2, of which 41.6-99.5% corresponded to copepods, mainly families Oithonidae, Oncaeidae, Pseudocalanidae, Calanidae and Metrididae. There was no evidence of coupling between mesoscale physical features and biomass or community structure. While coastal stations mainly at the Gerlache Strait remained in a highly productive state through the spring-summer, oceanic stations experienced a marked shift from a productive condition during FRUELA 95 to a low biomass, pteropod-dominated situation during FRUELA 96, possibly due to changing weather conditions. The median ingestion rates of herbivorous crustaceans during the FRUELA cruises were 0.7 mg Chl a m -2 day -1. Measured ingestion rates represented only 0.1% of the chlorophyll standing stock or 10% of the daily primary production. Thus, crustacean mesozooplankton had little control on the development of phytoplankton blooms in the area.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120003250','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120003250"><span><span class="hlt">Antarctic</span> Meteorite Classification and Petrographic Database Enhancements</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Todd, N. S.; Satterwhite, C. E.; Righter, K.</p> <p>2012-01-01</p> <p>The <span class="hlt">Antarctic</span> Meteorite collection, which is comprised of over 18,700 meteorites, is one of the largest collections of meteorites in the world. These meteorites have been collected since the late 1970 s as part of a three-agency agreement between NASA, the National Science Foundation, and the Smithsonian Institution [1]. Samples collected each season are analyzed at NASA s Meteorite Lab and the Smithsonian Institution and results are published twice a year in the <span class="hlt">Antarctic</span> Meteorite Newsletter, which has been in publication since 1978. Each newsletter lists the samples collected and processed and provides more in-depth details on selected samples of importance to the scientific community. Data about these meteorites is also published on the NASA Curation website [2] and made available through the Meteorite Classification Database allowing scientists to search by a variety of parameters. This paper describes enhancements that have been made to the database and to the data and photo acquisition process to provide the meteorite community with faster access to meteorite data concurrent with the publication of the <span class="hlt">Antarctic</span> Meteorite Newsletter twice a year.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29046532','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29046532"><span>Cradles and museums of <span class="hlt">Antarctic</span> teleost biodiversity.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Dornburg, Alex; Federman, Sarah; Lamb, April D; Jones, Christopher D; Near, Thomas J</p> <p>2017-09-01</p> <p>Isolated in one of the most extreme marine environments on Earth, teleost fish diversity in Antarctica's Southern Ocean is dominated by one lineage: the notothenioids. Throughout the past century, the long-term persistence of this unique marine fauna has become increasingly threatened by regional atmospheric and, to a lesser extent oceanic, warming. Developing an understanding of how historical temperature shifts have shaped source-sink dynamics for Antarctica's teleost lineages provides critical insight for predicting future demographic responses to climate change. We use a combination of phylogenetic and biogeographic modelling to show that high-latitude <span class="hlt">Antarctic</span> nearshore habitats have been an evolutionary sink for notothenioid species diversity. Contrary to expectations from island biogeographic theory, lower latitude regions of the Southern Ocean that include the northern <span class="hlt">Antarctic</span> Peninsula and peripheral island archipelagos act as source areas to continental diversity. These peripheral areas facilitate both the generation of new species and repeated colonization of nearshore <span class="hlt">Antarctic</span> continental regions. Our results provide historical context to contemporary trends of global climate change that threaten to invert these evolutionary dynamics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016E%26PSL.455...73R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016E%26PSL.455...73R"><span>Meridional circulation across the <span class="hlt">Antarctic</span> Circumpolar Current serves as a double 231Pa and 230Th trap</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rutgers van der Loeff, Michiel; Venchiarutti, Celia; Stimac, Ingrid; van Ooijen, Jan; Huhn, Oliver; Rohardt, Gerd; Strass, Volker</p> <p>2016-12-01</p> <p>Upwelling of Circumpolar Deep <span class="hlt">Water</span> in the Weddell Gyre and low scavenging rates south of the <span class="hlt">Antarctic</span> Circumpolar Current (ACC) cause an accumulation of particle reactive nuclides in the Weddell Gyre. A ventilation/reversible scavenging model that successfully described the accumulation of 230Th in this area was tested with other particle reactive nuclides and failed to adequately describe the depth-distributions of 231Pa and 210Pb. We present here a modified model that includes a nutrient-like accumulation south of the <span class="hlt">Antarctic</span> Polar Front in an upper meridional circulation cell, as well as transport to a deep circulation cell in the Weddell Gyre by scavenging and subsequent release at depth. The model also explains depletion of 231Pa and 230Th in Weddell Sea Bottom <span class="hlt">Water</span> (WSBW) by ventilation of newly formed deep <span class="hlt">water</span> on a timescale of 10 years, but this <span class="hlt">water</span> mass is too dense to leave the Weddell Gyre. In order to quantify the processes responsible for the 231Pa- and 230Th-composition of newly formed <span class="hlt">Antarctic</span> Bottom <span class="hlt">Water</span> (AABW) we present a mass balance of 231Pa and 230Th in the Atlantic sector of the Southern Ocean based on new data from the GEOTRACES program. The ACC receives 6.0 ± 1.5 ×106 dpms-1 of 230Th from the Weddell Sea, similar in magnitude to the net input of 4.2 ± 3.0 ×106 dpms-1 from the north. For 231Pa, the relative contribution from the Weddell Sea is much smaller, only 0.3 ± 0.1 ×106, compared to 2.7 ± 1.4 ×106 dpms-1 from the north. Weddell Sea Deep <span class="hlt">Water</span> (WSDW) leaving the Weddell Gyre northward to form AABW is exposed in the ACC to resuspended opal-rich sediments that act as efficient scavengers with a Th/Pa fractionation factor F ≤ 1. Hydrothermal inputs may provide additional removal with low F. Scavenging in the full meridional circulation across the opal-rich ACC thus acts as a double 231Pa and 230Th trap that preconditions newly formed AABW.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19720018430','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19720018430"><span>Mechanisms of deterioration of <span class="hlt">intermediate</span> moisture food systems</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Labuza, T. P.</p> <p>1972-01-01</p> <p>A study of shelf stability in <span class="hlt">intermediate</span> moisture foods was made. Major efforts were made to control lipid oxidation and nonenzymatic browning. In order to determine means of preventing these reactions, model systems were developed having the same <span class="hlt">water</span> activity content relationship of <span class="hlt">intermediate</span> moisture foods. Models were based on a cellulose-lipid and protein-lipid system with glycerol added as the humectant. Experiments with both systems indicate that lipid oxidation is promoted significantly in the <span class="hlt">intermediate</span> moisture range. The effect appeared to be related to increased mobility of either reactants or catalysts, since when the amount of <span class="hlt">water</span> in the system reached a level where capillary condensation occurred and thus free <span class="hlt">water</span> was present, the rates of oxidation increased. With added glycerol, which is <span class="hlt">water</span> soluble and thus increases the amount of mobile phase, the increase in oxidation rate occurs at a lower relative humidity. The rates of oxidation were maximized at 61% RH and decreased again at 75% RH probably due to dilution. No significant non-enzymatic browning occurred in the protein-lipid systems. Prevention of oxidation by the use of metal chelating agents was enhanced in the cellulose system, whereas, with protein present, the lipid soluble chain terminating antioxidants (such as BHA) worked equally as well. Preliminary studies of foods adjusted to the <span class="hlt">intermediate</span> moisture range bear out the results of oxidation in model systems. It can be concluded that for most fat containing <span class="hlt">intermediate</span> moisture foods, rancidity will be the reaction most limiting stability.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/fedgov/70039167/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/fedgov/70039167/report.pdf"><span>Geographic names of the <span class="hlt">Antarctic</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>,; ,; ,; ,; Alberts, Fred G.</p> <p>1995-01-01</p> <p>This gazetteer contains 12,710 names approved by the United States Board on Geographic Names and the Secretary of the Interior for features in Antarctica and the area extending northward to the <span class="hlt">Antarctic</span> Convergence. Included in this geographic area, the <span class="hlt">Antarctic</span> region, are the off-lying South Shetland Islands, the South Orkney Islands, the South Sandwich Islands, South Georgia, Bouvetøya, Heard Island, and the Balleny Islands. These names have been approved for use by U.S. Government agencies. Their use by the <span class="hlt">Antarctic</span> specialist and the public is highly recommended for the sake of accuracy and uniformity. This publication, which supersedes previous Board gazetteers or lists for the area, contains names approved as recently as December 1994. The basic name coverage of this gazetteer corresponds to that of maps at the scale of 1:250,000 or larger for coastal Antarctica, the off-lying islands, and isolated mountains and ranges of the continent. Much of the interior of Antarctica is a featureless ice plateau. That area has been mapped at a smaller scale and is nearly devoid of toponyms. All of the names are for natural features, such as mountains, glaciers, peninsulas, capes, bays, islands, and subglacial entities. The names of scientific stations have not been listed alphabetically, but they may appear in the texts of some decisions. For the names of submarine features, reference should be made to the Gazetteer of Undersea Features, 4th edition, U.S. Board on Geographic Names, 1990.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004AGUFM.C21A0973B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004AGUFM.C21A0973B"><span>Investigating the crustal elements of the central <span class="hlt">Antarctic</span> Plate (ICECAP): How long-range aerogeophysics is critical to understanding the evolution of the East <span class="hlt">Antarctic</span> ice sheet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Blankenship, D. D.; Brozena, J. M.; Siegert, M. J.; Morse, D. L.; Dalziel, I. W.; Lawver, L. A.; Holt, J. W.; Childers, V. A.; Bamber, J. L.; Payne, A. J.</p> <p>2004-12-01</p> <p>The highlands of the central <span class="hlt">Antarctic</span> Plate have been the nursery for East <span class="hlt">Antarctic</span> ice sheets since at least the early Oligocene separation of Antarctica and Australia. Significant strides have been made in deciphering the marine geological, geophysical, and geochemical record of the deposits left by these sheets and the Pleistocene paleoclimate record from ice cores taken from the central reaches of the contemporary ice sheet. Most recently, the scientific community has realized the importance of the isolated biome represented by the subglacial lakes that characterize the domes of the central East <span class="hlt">Antarctic</span> ice sheet and evolve in concert with them. Understanding the evolution of the East <span class="hlt">Antarctic</span> ice sheet and its sub-glacial environment would be a major contribution to the IPY 2007-2008 international effort. Critical to understanding offshore and ice core records of paleoclimate, as well as the distribution/isolation of any subglacial lake systems, is developing a comprehensive understanding of the crustal elements of the central <span class="hlt">Antarctic</span> Plate. A complete understanding of the evolution of East <span class="hlt">Antarctic</span> ice sheets throughout the Cenozoic requires knowledge of the boundaries, elevation and paleolatitude of these crustal elements through time as well as evidence of their morphological, sedimentological and tectono-thermal history. The basic impediments to gaining this understanding are the subcontinental scale of the central <span class="hlt">Antarctic</span> Plate and the one to four kilometers of ice cover that inhibits direct access. It is possible however to provide a substantial framework for understanding these crustal elements through a comprehensive program of long-range airborne geophysical observations. We have proposed a plan to measure gravity, magnetics, ice-penetrating radar, and laser/radar altimetry over the Gamburtsev, Vostok and Belgica subglacial highlands beneath Domes A - C of the contemporary East <span class="hlt">Antarctic</span> ice sheet using a Navy P-3 aircraft based in Mc</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011DSRII..58..839A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011DSRII..58..839A"><span>Grazing suppression of dimethylsulphoniopropionate (DMSP) accumulation in iron-fertilised, sub-<span class="hlt">Antarctic</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>Archer, S. D.; Safi, K.; Hall, A.; Cummings, D. G.; Harvey, M.</p> <p>2011-03-01</p> <p>The impact of in situ iron fertilisation on the production of particulate dimethylsulphoniopropionate (DMSPp) and its breakdown product dimethyl sulphide (DMS) was monitored during the SOLAS air-sea gas exchange experiment (SAGE). The experiment was conducted in the high nitrate, low chlorophyll (HNLC) <span class="hlt">waters</span> of the sub-<span class="hlt">Antarctic</span> Southern Ocean (46.7°S 172.5°E) to the south-east of New Zealand, during March-April, 2004. In addition to monitoring net changes in the standing stocks of DMSPp and DMS, a series of dilution experiments were used to determine the DMSPp production and consumption rates in relation to increased iron availability. In contrast to previous experiments in the Southern Ocean, DMS concentrations decreased over the course of the 15-d iron-fertilisation experiment, from an integrated volume-specific concentration in the mixed layer on day 0 of 0.78 nM (measured values 0.65-0.91 nM) to 0.46 nM (measured values 0.42-0.47 nM) by day 15, in parallel with the surrounding <span class="hlt">waters</span>. DMSPp, chlorophyll a and the abundance of photosynthetic picoeukaryotes exhibited indiscernible or only moderate increases in response to the raised iron availability, despite an obvious physiological response by the phytoplankton. High specific growth rates of DMSPp, equivalent to 0.8-1.2 doublings d -1, occurred at the simulated 60% light level of the dilution experiments. Despite the high production rates, DMSPp accumulation was suppressed in part by microzooplankton grazers who consumed between 61% d -1 and 126% d -1 of the DMSPp production. Temporal trends in the rates of production and consumption illustrated a close coupling between the DMSP-producing phytoplankton and their microzooplankton grazers. Similar grazing and production rates were observed for the eukaryotic picophytoplankton that dominated the phytoplankton biomass, partial evidence that picoeukaryotes contributed a substantial proportion of the DMSP synthesis. These rates for DMSPp and picoeukaryotes were</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70020442','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70020442"><span>Ice Sheet History from <span class="hlt">Antarctic</span> Continental Margin Sediments: The ANTOSTRAT Approach</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Barker, P.F.; Barrett, P.J.; Camerlenghi, A.; Cooper, A. K.; Davey, F.J.; Domack, E.W.; Escutia, C.; Kristoffersen, Y.; O'Brien, P.E.</p> <p>1998-01-01</p> <p>The <span class="hlt">Antarctic</span> Ice Sheet is today an important part of the global climate engine, and probably has been so for most of its long existence. However, the details of its history are poorly known, despite the measurement and use, over two decades, of low-latitude proxies of ice sheet volume. An additional way of determining ice sheet history is now available, based on understanding terrigenous sediment transport and deposition under a glacial regime. It requires direct sampling of the prograded wedge of glacial sediments deposited at the <span class="hlt">Antarctic</span> continental margin (and of derived sediments on the continental rise) at a small number of key sites, and combines the resulting data using numerical models of ice sheet development. The new phase of sampling is embodied mainly in a suite of proposals to the Ocean Drilling Program, generated by separate regional proponent groups co-ordinated through ANTOSTRAT (the <span class="hlt">Antarctic</span> Offshore Acoustic Stratigraphy initiative). The first set of margin sites has now been drilled as ODP Leg 178 to the <span class="hlt">Antarctic</span> Peninsula margin, and a first, short season of inshore drilling at Cape Roberts, Ross Sea, has been completed. Leg 178 and Cape Roberts drilling results are described briefly here, together with an outline of key elements of the overall strategy for determining glacial history, and of the potential contributions of drilling other <span class="hlt">Antarctic</span> margins investigated by ANTOSTRAT. ODP Leg 178 also recovered continuous ultra-high-resolution Holocene biogenic sections at two sites within a protected, glacially-overdeepened basin (Palmer Deep) on the inner continental shelf of the <span class="hlt">Antarctic</span> Peninsula. These and similar sites from around the <span class="hlt">Antarctic</span> margin are a valuable resource when linked with ice cores and equivalent sections at lower latitude sites for studies of decadal and millenial-scale climate variation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1426492-trends-adsorption-electrocatalytic-water-splitting-intermediates-cubic-abo3-oxides','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1426492-trends-adsorption-electrocatalytic-water-splitting-intermediates-cubic-abo3-oxides"><span>Trends in adsorption of electrocatalytic <span class="hlt">water</span> splitting <span class="hlt">intermediates</span> on cubic ABO 3 oxides</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Montoya, Joseph H.; Doyle, Andrew D.; Nørskov, Jens K.; ...</p> <p>2018-01-19</p> <p>The reactivity of solid oxide surfaces towards adsorption of oxygen and hydrogen is a key metric for the design of new catalysts for electrochemical <span class="hlt">water</span> splitting. Here, in this paper, we report on trends in the adsorption energy of different adsorbed <span class="hlt">intermediates</span> derived from the oxidation and reduction of <span class="hlt">water</span> for ternary ABO 3 oxides in the cubic perovskite structure. Our findings support a previously reported trend that rationalizes the observed lower bound in oxygen evolution (OER) overpotentials from correlations in OH* and OOH* adsorption energies. In addition, we report hydrogen adsorption energies that may be used to estimate hydrogenmore » evolution (HER) overpotentials along with potential metrics for electrochemical metastability in reducing environments. Finally, we also report and discuss trends between atom-projected density of states and adsorption energies, which may enable a design criteria from the local electronic structure of the active site.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1426492-trends-adsorption-electrocatalytic-water-splitting-intermediates-cubic-abo3-oxides','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1426492-trends-adsorption-electrocatalytic-water-splitting-intermediates-cubic-abo3-oxides"><span>Trends in adsorption of electrocatalytic <span class="hlt">water</span> splitting <span class="hlt">intermediates</span> on cubic ABO 3 oxides</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>Montoya, Joseph H.; Doyle, Andrew D.; Nørskov, Jens K.</p> <p></p> <p>The reactivity of solid oxide surfaces towards adsorption of oxygen and hydrogen is a key metric for the design of new catalysts for electrochemical <span class="hlt">water</span> splitting. Here, in this paper, we report on trends in the adsorption energy of different adsorbed <span class="hlt">intermediates</span> derived from the oxidation and reduction of <span class="hlt">water</span> for ternary ABO 3 oxides in the cubic perovskite structure. Our findings support a previously reported trend that rationalizes the observed lower bound in oxygen evolution (OER) overpotentials from correlations in OH* and OOH* adsorption energies. In addition, we report hydrogen adsorption energies that may be used to estimate hydrogenmore » evolution (HER) overpotentials along with potential metrics for electrochemical metastability in reducing environments. Finally, we also report and discuss trends between atom-projected density of states and adsorption energies, which may enable a design criteria from the local electronic structure of the active site.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMPP21A2276L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMPP21A2276L"><span>Abrupt Deglacial Changes in Subarctic Pacific Ventilation: <span class="hlt">Intermediate</span> and Deep <span class="hlt">Water</span> Ventilation, Oxygen Fluctuations, and the relation to carbon cycle dynamics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lembke-Jene, L.; Tiedemann, R.; Gong, X.; Max, L.; Zou, J.; Shi, X.; Lohmann, G.</p> <p>2016-12-01</p> <p>The modern subarctic Pacific halocline prevents the formation of deepwater masses andonly mid-depth <span class="hlt">waters</span> are ventilated by North Pacific <span class="hlt">Intermediate</span> <span class="hlt">Water</span> (NPIW). During the last glacial, isolation of the deep North Pacific ids thought to have been more pronounced, combined with a better ventilated and expanded NPIW. This glacial deep to <span class="hlt">intermediate</span> separation, together with upper ocean stratification, has principal implications for the deep ocean storage of carbon, as well as the mid-depth provision of nutrients by NPIW to the lower-latitude thermocline and the Pacific subarctic gyre. To date, conflicting evidence persists how the North Pacific biological and physical carbon pump reorganized during millennial-scale glacial and deglacial changes over the past 50 ka, limiting our understanding of carbon pool dynamics between Pacific ocean and the atmosphere. We present proxydata and paleoclimate modelling evidence for rapid <span class="hlt">intermediate</span> and deep ocean nutrient and ventilation changes based on a sediment core collection with good temporal and spatial resolution from the Okhotsk Sea, Bering Sea, and the open subarctic North Pacific. High sedimentation rates (20-200 cm/ka) enable us to decipher rapid climatic changes on millennial time scales through MIS 2-3 and with a higher, up to inter-decadal, resolution during the last glacial termination. Paired AMS radiocarbon planktic-benthic ages help us to constrain <span class="hlt">water</span> mass age changes, while multi-species foraminiferal stable isotope and redox-sensitive elemental time series provide information on past oxygenation and nutrient dynamics. We found evidence for a weaker chemical separation between <span class="hlt">intermediate</span> and deep <span class="hlt">water</span> during the glacial than previously thought, with rapid alternations between major NPIW ventilation areas in marginal seas, in particular during Heinrich stadials and the termination. We provide new information about the deglacial mid-depth subarctic Pacific de-oxygenation timing, extent and forcing</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/11077478','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/11077478"><span>The identification, examination and exploration of <span class="hlt">Antarctic</span> subglacial lakes.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Siegert, M J</p> <p>2000-01-01</p> <p>At the floor of the <span class="hlt">Antarctic</span> ice sheet, 4 km below the Russian research base Vostok Station, lies a 2,000 km3 body of <span class="hlt">water</span>, comparable in size to Lake Ontario. This remote <span class="hlt">water</span> mass, named Lake Vostok, is the world's largest subglacial lake by an order of magnitude (Figure 1). Despite ice-surface temperatures regularly around -60 degrees C, the ice-sheet base is kept at the melting temperature by geothermal heating from the Earth's interior. The ice sheet above the lake has been in existence for at least several million years and possibly as long as 20 million years. The origins of Lake Vostok may therefore data back across geological time to the Miocene (7-26 Ma). The hydrology of Lake Vostok can be characterised by subglacial melting across its northern side, and refreezing over the southern section. A deep ice core, located over the southern end of the lake has sampled the refrozen ice. Geochemical analysis of this ice has found that it comprises virtually pure <span class="hlt">water</span>. However, normal glacier ice contains impurities such as debris and gas hydrates. Subglacial melting and freezing over Lake Vostok may, therefore, leave the lake enriched in potential nutrients issued from the melted glacier ice. Many scientists expect microbial life to exist within the lake, adapted to the extreme conditions of low nutrient and energy levels. Indeed microbes have been found in the basal refrozen layers of the ice sheet. If Lake Vostok has been isolated from the atmosphere for several million years by the ice sheet that lays above it, the microbes within the lake must also date back several million years and may have undergone evolution over this time, yielding life that may be unique to Lake Vostok. Plans are currently being arranged to explore Lake Vostok and other <span class="hlt">Antarctic</span> subglacial lakes, and identify life in these extraordinary places. Before this happens, however, much more needs to be known about the ice-sheet above subglacial lakes, and the rocks and sediment below them.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA273018','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA273018"><span>Notes on <span class="hlt">Antarctic</span> Aviation</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1993-08-01</p> <p>4 5. Curtiss-Wright T -32 biplane used by the second Byrd <span class="hlt">Antarctic</span> Expedition...pack ice north of Mawson ............................................ 7 10. USN ski-wheel Douglas R4D-8 at McMurdo...McMurdo ................. 11 17. ANARE ski-wheel DHC-2 Beaver over Mawson ............................................ 12 18. USN ski-wheel DHC-3 Otter</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JGRC..121.7530M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JGRC..121.7530M"><span>Wind-driven export of Weddell Sea slope <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>Meijers, A. J. S.; Meredith, M. P.; Abrahamsen, E. P.; Morales Maqueda, M. A.; Jones, D. C.; Naveira Garabato, A. C.</p> <p>2016-10-01</p> <p>The export of <span class="hlt">waters</span> from the Weddell Gyre to lower latitudes is an integral component of the southern subpolar contribution to the three-dimensional oceanic circulation. Here we use more than 20 years of repeat hydrographic data on the continental slope on the northern tip of the <span class="hlt">Antarctic</span> Peninsula and 5 years of bottom lander data on the slope at 1000 m to show the intermittent presence of a relatively cold, fresh, westward flowing current. This is often bottom-intensified between 600 and 2000 dbar with velocities of over 20 cm s-1, transporting an average of 1.5 ± 1.5 Sv. By comparison with hydrography on the continental slope within the Weddell Sea and modeled tracer release experiments we show that this slope current is an extension of the <span class="hlt">Antarctic</span> Slope Current that has crossed the South Scotia Ridge west of Orkney Plateau. On monthly to interannual time scales the density of the slope current is negatively correlated (r > 0.6 with a significance of over 95%) with eastward wind stress over the northern Weddell Sea, but lagging it by 6-13 months. This relationship holds in both the high temporal resolution bottom lander time series and the 20+ year annual hydrographic occupations and agrees with Weddell Sea export variability observed further east. We compare several alternative hypotheses for this wind stress/export relationship and find that it is most consistent with wind-driven acceleration of the gyre boundary current, possibly modulated by eddy dynamics, and represents a mechanism by which climatic perturbations can be rapidly transmitted as fluctuations in the supply of <span class="hlt">intermediate</span>-level <span class="hlt">waters</span> to lower latitudes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20000040793','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20000040793"><span><span class="hlt">Antarctic</span> Meteorite Newsletter</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lindstrom, Marilyn</p> <p>2000-01-01</p> <p>This newsletter contains something for everyone! It lists classifications of about 440 meteorites mostly from the 1997 and 1998 ANSMET (<span class="hlt">Antarctic</span> Search for Meteorites) seasons. It also gives descriptions of about 45 meteorites of special petrologic type. These include 1 iron, 17 chondrites (7 CC, 1 EC, 9 OC) and 27 achondrites (25 HED, UR). Most notable are an acapoloite (GRA98028) and an olivine diogenite (GRA98108).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMPA32A..02V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMPA32A..02V"><span>Integrated Science and Logistical Planning to Support Big Questions in <span class="hlt">Antarctic</span> Science</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vaughan, D. G.; Stockings, T. M.</p> <p>2015-12-01</p> <p>Each year, British <span class="hlt">Antarctic</span> Survey (BAS) supports an extensive programme of science at five <span class="hlt">Antarctic</span> and sub-<span class="hlt">Antarctic</span> stations, ranging from the tiny Bird Island Research Station at 54°S in the South Atlantic, to the massive, and fully re-locatable, Halley Research Station on Brunt Ice Shelf at 75°S. The BAS logistics hub, Rothera Research Station on the <span class="hlt">Antarctic</span> Peninsula supports deployment of deep-field and airborne field campaigns through much of the <span class="hlt">Antarctic</span> continent, and an innovative new UK polar research vessel is under design, and planned to enter service in the Southern Ocean in 2019. BAS's core science programme covering all aspects of physical, biological and geological science is delivered by our own science teams, but every year many other UK scientists and overseas collaborators also access BAS's <span class="hlt">Antarctic</span> logistics to support their own programmes. As an integrated science and logistics provider, BAS is continuously reviewing its capabilities and operational procedures to ensure that the future long-term requirements of science are optimally supported. Current trends are towards providing the capacity for heavier remote operations and larger-scale field camps, increasing use of autonomous ocean and airborne platforms, and increasing opportunities to provide turnkey solutions for low-cost experimental deployments. This talk will review of expected trends in <span class="hlt">Antarctic</span> science and the opportunities to conduct science in Antarctica. It will outline the anticipated logistic developments required to support future stakeholder-led and strategically-directed science programmes, and the long-term ambitions of our science communities indentified in several recent horizon-scanning activities.</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/1993Metic..28..377K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1993Metic..28..377K"><span>Preliminary Compositional Comparisons of H-Chondrite Falls to <span class="hlt">Antarctic</span> H-Chondrite Populations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kallemeyn, G. W.; Krot, A. N.; Rubin, A. E.</p> <p>1993-07-01</p> <p>In a series of papers [e.g., 1,2], Lipschutz and co-workers compared trace- element RNAA data from <span class="hlt">Antarctic</span> and non-<span class="hlt">Antarctic</span> H4-6 chondrites and concluded that the two populations have significantly different concentrations of several trace elements including Co, Se, and Sb. They interpreted their data as indicating that these <span class="hlt">Antarctic</span> H chondrites form different populations than observed H falls and may have originated in separate parent bodies. Recent work by Sears and co-workers [e.g., 3] has shown that there seem to be distinct populations of <span class="hlt">Antarctic</span> H chondrites, distinguishable on the bases of induced thermoluminescence (TL) peak temperature, metallographic cooling rate, and cosmic ray exposure age. They showed that a group of <span class="hlt">Antarctic</span> H chondrites having abnormally high induced TL peak temperatures (>=190 degrees C) also has cosmic ray exposure ages <20 Ma (mostly ~8 Ma) and fast metallographic cooling rates (~100 K/Ma). Another group having induced TL peak temperatures <190 degrees C has exposure ages >20 Ma and slower cooling rates (~10-20 K/Ma). We studied 24 H4-6 chondrites from Victoria Land (including 12 previously analyzed by the Lipschutz group) by optical microscopy and electron microprobe. Many of the <span class="hlt">Antarctic</span> H chondrites studied by Lipschutz and co- workers are unsuitable for proper compositional comparisons with H chondrite falls: Four are very weathered, five are extensively shocked, and two are extensively brecciated. Furthermore, at least five of the samples contain solar-wind gas (and hence are regolith breccias) [4]. These samples were rejected because of possible compositional modification by secondary processes. For our INAA study we chose a suite of relatively unweathered and unbrecciated <span class="hlt">Antarctic</span> H chondrites (including nine from the Lipschutz set): ALHA 77294 (H5, S3); ALHA 79026 (H5, S3); ALHA 79039 (H5, S3); ALHA 80131 (H5, S3); ALHA 80132 (H5, S4); ALHA 81037 (H6, S3); EETA 79007 (H5, S4); LEW 85320 (H6, S4); LEW 85329 (H6</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19880039799&hterms=nitrate+lead&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dnitrate%2Blead','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19880039799&hterms=nitrate+lead&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dnitrate%2Blead"><span><span class="hlt">Antarctic</span> ozone - Meteoric control of HNO3</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Prather, Michael J.; Rodriguez, Jose M.</p> <p>1988-01-01</p> <p>Atmospheric circulation leads to an accumulation of debris from meteors in the <span class="hlt">Antarctic</span> stratosphere at the beginning of austral spring. The major component of meteoric material is alkaline, comprised predominantly of the oxides of magnesium and iron. These metals may neutralize the natural acidity of stratospheric aerosols, remove nitric acid from the gas phase, and bond it as metal nitrates in the aerosol phase. Removal of nitric acid vapor has been previously shown to be a critical link in the photochemical depletion of ozone in the <span class="hlt">Antarctic</span> spring, by allowing for increased catalytic loss from chlorine and bromine.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.C13A0732Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.C13A0732Y"><span>Monitoring <span class="hlt">Antarctic</span> ice sheet surface melting with TIMESAT algorithm</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ye, Y.; Cheng, X.; Li, X.; Liang, L.</p> <p>2011-12-01</p> <p><span class="hlt">Antarctic</span> ice sheet contributes significantly to the global heat budget by controlling the exchange of heat, moisture, and momentum at the surface-atmosphere interface, which directly influence the global atmospheric circulation and climate change. Ice sheet melting will cause snow humidity increase, which will accelerate the disintegration and movement of ice sheet. As a result, detecting <span class="hlt">Antarctic</span> ice sheet melting is essential for global climate change research. In the past decades, various methods have been proposed for extracting snowmelt information from multi-channel satellite passive microwave data. Some methods are based on brightness temperature values or a composite index of them, and others are based on edge detection. TIMESAT (Time-series of Satellite sensor data) is an algorithm for extracting seasonality information from time-series of satellite sensor data. With TIMESAT long-time series brightness temperature (SSM/I 19H) is simulated by Double Logistic function. Snow is classified to wet and dry snow with generalized Gaussian model. The results were compared with those from a wavelet algorithm. On this basis, <span class="hlt">Antarctic</span> automatic weather station data were used for ground verification. It shows that this algorithm is effective in ice sheet melting detection. The spatial distribution of melting areas(Fig.1) shows that, the majority of melting areas are located on the edge of <span class="hlt">Antarctic</span> ice shelf region. It is affected by land cover type, surface elevation and geographic location (latitude). In addition, the <span class="hlt">Antarctic</span> ice sheet melting varies with seasons. It is particularly acute in summer, peaking at December and January, staying low in March. In summary, from 1988 to 2008, Ross Ice Shelf and Ronnie Ice Shelf have the greatest interannual variability in amount of melting, which largely determines the overall interannual variability in Antarctica. Other regions, especially Larsen Ice Shelf and Wilkins Ice Shelf, which is in the <span class="hlt">Antarctic</span> Peninsula</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70018390','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70018390"><span>Active volcanism beneath the West <span class="hlt">Antarctic</span> ice sheet and implications for ice-sheet stability</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Blankenship, D.D.; Bell, R.E.; Hodge, S.M.; Brozena, J.M.; Behrendt, John C.; Finn, C.A.</p> <p>1993-01-01</p> <p>IT is widely understood that the collapse of the West <span class="hlt">Antarctic</span> ice sheet (WAIS) would cause a global sea level rise of 6 m, yet there continues to be considerable debate about the detailed response of this ice sheet to climate change1-3. Because its bed is grounded well below sea level, the stability of the WAIS may depend on geologically controlled conditions at the base which are independent of climate. In particular, heat supplied to the base of the ice sheet could increase basal melting and thereby trigger ice streaming, by providing the <span class="hlt">water</span> for a lubricating basal layer of till on which ice streams are thought to slide4,5. Ice streams act to protect the reservoir of slowly moving inland ice from exposure to oceanic degradation, thus enhancing ice-sheet stability. Here we present aerogeophysical evidence for active volcanism and associated elevated heat flow beneath the WAIS near the critical region where ice streaming begins. If this heat flow is indeed controlling ice-stream formation, then penetration of ocean <span class="hlt">waters</span> inland of the thin hot crust of the active portion of the West <span class="hlt">Antarctic</span> rift system could lead to the disappearance of ice streams, and possibly trigger a collapse of the inland ice reservoir.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6272659-river-gardens-intermediate-care-facility-water-air-heating-air-conditioning-demonstration-project-final-report','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6272659-river-gardens-intermediate-care-facility-water-air-heating-air-conditioning-demonstration-project-final-report"><span>River Gardens <span class="hlt">Intermediate</span>-Care Facility <span class="hlt">water</span>-to-air heating and air-conditioning demonstration project. Final report</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>Brown, R.C.</p> <p></p> <p>An integrated system of heat pumps is used to reject heat into or extract heat from circulating <span class="hlt">water</span> from a shallow well adjacent to the river to demonstrate the efficiency and fuel cost savings of <span class="hlt">water</span>-to-air heat pumps, without the expense of drilling a deep well. <span class="hlt">Water</span> is returned unpolluted to the Guadalupe River and is circulated through a five-building complex at River Gardens <span class="hlt">Intermediate</span> Care Facility for the Mentally Retarded in New Braunfels, Texas. The <span class="hlt">water</span> is used as a heat source or sink for 122 heat pumps providing space heating and cooling, and for refrigeration and freezer units.more » The system was not installed as designed, which resulted in <span class="hlt">water</span> pumping loads being higher than the original design. Electrical consumption for pumping <span class="hlt">water</span> represented 36 to 37% of system electrical consumption. Without the <span class="hlt">water</span> pumping load, the <span class="hlt">water</span>-to-air system was an average of 25% more efficient in heating than a comparable air-to-air unit with resistance heating. With <span class="hlt">water</span> pumping load included, the installed system averaged 17% less efficient in cooling and 19% more efficient in heating than the comparable unit.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.T13A2499K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.T13A2499K"><span>Ridge Tectonics, Magma Supply, and Ridge-Hotpot Interaction at the Eastern End of the Australian-<span class="hlt">Antarctic</span> Ridge</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kim, S.; Lin, J.; Park, S.; Choi, H.; Lee, S.</p> <p>2013-12-01</p> <p>During 2011-2013 the Korea Polar Research Institute (KOPRI) conducted three successive expeditions to the eastern end of the Australian-<span class="hlt">Antarctic</span> Ridge (AAR) to investigate the tectonics, geochemistry, and hydrothermal activity of this <span class="hlt">intermediate</span> fast spreading system. On board the Korean icebreaker R/V Araon, the science party collected multiple types of data including multibeam bathymetry, gravity, magnetics, as well as rock and <span class="hlt">water</span> column samples. In addition, Miniature Autonomous Plume Recorders (MAPRs) were deployed at each of the wax-core rock sampling sites to detect the presence of active hydrothermal vents. In this study, we present a detailed analysis of a 360-km-long super-segment at the eastern end of the AAR to quantify the spatial variations in ridge morphology and investigate its respond to changes in melt supply. The study region contains several intriguing bathymetric features including (1) abrupt changes in the axial topography, alternating between rift valleys and axial highs within relatively short ridge segments; (2) overshooting ridge tips at the ridge-transform intersections; (3) systematic migration patterns of hooked ridges; (4) a 350-km-long mega-transform fault; and (5) robust axial and off-axis volcanisms. To obtain a proxy for regional variations in magma supply, we calculated residual mantle Bouguer gravity anomalies (RMBA), gravity-derived crustal thickness, and residual topography for seven sub-segments. The results of the analyses revealed that the southern flank of the AAR is associated with a shallower seafloor, more negative RMBA, thicker crust, and/or less dense mantle than the conjugate northern flank. Furthermore, this N-S asymmetry becomes more prominent toward the super-segment of the AAR. Such regional variations in seafloor topography and RMBA are consistent with the hypothesis that ridge segments in the study area have interacted with the Balleny hotspot, currently lies southwest of the AAR. However, the influence of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19880001021','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19880001021"><span><span class="hlt">Antarctic</span> field tests of SARSAT personal locater beacons</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bindschadler, Robert</p> <p>1987-01-01</p> <p>Field tests of SARSAT personal locater beacons were conducted in the <span class="hlt">Antarctic</span> to assess the viability of using these beacons to increase the safety of <span class="hlt">Antarctic</span> field parties. Data were collected on the extent to which dry or wet snow, melting conditions, crevasse walls and snow bridges affected the ability of the SARSAT satellite to calculate an accurate position of the beacon. Average response time between beacon turn on and alert reception in McMurdo was between 4 and 5 hours for these tests. It is concluded that the SARSAT system is viable for <span class="hlt">Antarctic</span> operations and it is recommended that it be implemented for future field operations. Because of obstruction of line-of-sight between beacon and satellite degrades the accuracy of the location calculation (particularly in wet snow), it is further recommended that field parties have sufficient numbers of beacons to insure that in an emergency, one will be able to operate from the surface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JChPh.145h4503S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JChPh.145h4503S"><span>The temperature dependence of <span class="hlt">intermediate</span> range oxygen-oxygen correlations in liquid <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>Schlesinger, Daniel; Wikfeldt, K. Thor; Skinner, Lawrie B.; Benmore, Chris J.; Nilsson, Anders; Pettersson, Lars G. M.</p> <p>2016-08-01</p> <p>We analyze the recent temperature dependent oxygen-oxygen pair-distribution functions from experimental high-precision x-ray diffraction data of bulk <span class="hlt">water</span> by Skinner et al. [J. Chem. Phys. 141, 214507 (2014)] with particular focus on the <span class="hlt">intermediate</span> range where small, but significant, correlations are found out to 17 Å. The second peak in the pair-distribution function at 4.5 Å is connected to tetrahedral coordination and was shown by Skinner et al. to change behavior with temperature below the temperature of minimum isothermal compressibility. Here we show that this is associated also with a peak growing at 11 Å which strongly indicates a collective character of fluctuations leading to the enhanced compressibility at lower temperatures. We note that the peak at ˜13.2 Å exhibits a temperature dependence similar to that of the density with a maximum close to 277 K or 4 °C. We analyze simulations of the TIP4P/2005 <span class="hlt">water</span> model in the same manner and find excellent agreement between simulations and experiment albeit with a temperature shift of ˜20 K.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PolSc..13...23H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PolSc..13...23H"><span>Geostatistical analysis and isoscape of ice core derived <span class="hlt">water</span> stable isotope records in an <span class="hlt">Antarctic</span> macro region</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hatvani, István Gábor; Leuenberger, Markus; Kohán, Balázs; Kern, Zoltán</p> <p>2017-09-01</p> <p><span class="hlt">Water</span> stable isotopes preserved in ice cores provide essential information about polar precipitation. In the present study, multivariate regression and variogram analyses were conducted on 22 δ2H and 53 δ18O records from 60 ice cores covering the second half of the 20th century. Taking the multicollinearity of the explanatory variables into account, as also the model's adjusted R2 and its mean absolute error, longitude, elevation and distance from the coast were found to be the main independent geographical driving factors governing the spatial δ18O variability of firn/ice in the chosen <span class="hlt">Antarctic</span> macro region. After diminishing the effects of these factors, using variography, the weights for interpolation with kriging were obtained and the spatial autocorrelation structure of the dataset was revealed. This indicates an average area of influence with a radius of 350 km. This allows the determination of the areas which are as yet not covered by the spatial variability of the existing network of ice cores. Finally, the regional isoscape was obtained for the study area, and this may be considered the first step towards a geostatistically improved isoscape for Antarctica.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3340021','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3340021"><span><span class="hlt">Antarctic</span> and Southern Ocean influences on Late Pliocene global cooling</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>McKay, Robert; Naish, Tim; Carter, Lionel; Riesselman, Christina; Dunbar, Robert; Sjunneskog, Charlotte; Winter, Diane; Sangiorgi, Francesca; Warren, Courtney; Pagani, Mark; Schouten, Stefan; Willmott, Veronica; Levy, Richard; DeConto, Robert; Powell, Ross D.</p> <p>2012-01-01</p> <p>The influence of Antarctica and the Southern Ocean on Late Pliocene global climate reconstructions has remained ambiguous due to a lack of well-dated <span class="hlt">Antarctic</span>-proximal, paleoenvironmental records. Here we present ice sheet, sea-surface temperature, and sea ice reconstructions from the ANDRILL AND-1B sediment core recovered from beneath the Ross Ice Shelf. We provide evidence for a major expansion of an ice sheet in the Ross Sea that began at ∼3.3 Ma, followed by a coastal sea surface temperature cooling of ∼2.5 °C, a stepwise expansion of sea ice, and polynya-style deep mixing in the Ross Sea between 3.3 and 2.5 Ma. The intensification of <span class="hlt">Antarctic</span> cooling resulted in strengthened westerly winds and invigorated ocean circulation. The associated northward migration of Southern Ocean fronts has been linked with reduced Atlantic Meridional Overturning Circulation by restricting surface <span class="hlt">water</span> connectivity between the ocean basins, with implications for heat transport to the high latitudes of the North Atlantic. While our results do not exclude low-latitude mechanisms as drivers for Pliocene cooling, they indicate an additional role played by southern high-latitude cooling during development of the bipolar world. PMID:22496594</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016ACP....16.2185H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016ACP....16.2185H"><span>Unexpectedly high ultrafine aerosol concentrations above East <span class="hlt">Antarctic</span> sea ice</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Humphries, R. S.; Klekociuk, A. R.; Schofield, R.; Keywood, M.; Ward, J.; Wilson, S. R.</p> <p>2016-02-01</p> <p>Better characterisation of aerosol processes in pristine, natural environments, such as Antarctica, have recently been shown to lead to the largest reduction in uncertainties in our understanding of radiative forcing. Our understanding of aerosols in the <span class="hlt">Antarctic</span> region is currently based on measurements that are often limited to boundary layer air masses at spatially sparse coastal and continental research stations, with only a handful of studies in the vast sea-ice region. In this paper, the first observational study of sub-micron aerosols in the East <span class="hlt">Antarctic</span> sea ice region is presented. Measurements were conducted aboard the icebreaker Aurora Australis in spring 2012 and found that boundary layer condensation nuclei (CN3) concentrations exhibited a five-fold increase moving across the polar front, with mean polar cell concentrations of 1130 cm-3 - higher than any observed elsewhere in the <span class="hlt">Antarctic</span> and Southern Ocean region. The absence of evidence for aerosol growth suggested that nucleation was unlikely to be local. Air parcel trajectories indicated significant influence from the free troposphere above the <span class="hlt">Antarctic</span> continent, implicating this as the likely nucleation region for surface aerosol, a similar conclusion to previous <span class="hlt">Antarctic</span> aerosol studies. The highest aerosol concentrations were found to correlate with low-pressure systems, suggesting that the passage of cyclones provided an accelerated pathway, delivering air masses quickly from the free troposphere to the surface. After descent from the <span class="hlt">Antarctic</span> free troposphere, trajectories suggest that sea-ice boundary layer air masses travelled equatorward into the low-albedo Southern Ocean region, transporting with them emissions and these aerosol nuclei which, after growth, may potentially impact on the region's radiative balance. The high aerosol concentrations and their transport pathways described here, could help reduce the discrepancy currently present between simulations and observations of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040172646&hterms=bacterial+photosynthesis&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dbacterial%2Bphotosynthesis','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040172646&hterms=bacterial+photosynthesis&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dbacterial%2Bphotosynthesis"><span>Perennial <span class="hlt">Antarctic</span> lake ice: an oasis for life in a polar desert</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Priscu, J. C.; Fritsen, C. H.; Adams, E. E.; Giovannoni, S. J.; Paerl, H. W.; McKay, C. P.; Doran, P. T.; Gordon, D. A.; Lanoil, B. D.; Pinckney, J. L.</p> <p>1998-01-01</p> <p>The permanent ice covers of <span class="hlt">Antarctic</span> lakes in the McMurdo Dry Valleys develop liquid <span class="hlt">water</span> inclusions in response to solar heating of internal aeolian-derived sediments. The ice sediment particles serve as nutrient (inorganic and organic)-enriched microzones for the establishment of a physiologically and ecologically complex microbial consortium capable of contemporaneous photosynthesis, nitrogen fixation, and decomposition. The consortium is capable of physically and chemically establishing and modifying a relatively nutrient- and organic matter-enriched microbial "oasis" embedded in the lake ice cover.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/9641910','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/9641910"><span>Perennial <span class="hlt">Antarctic</span> lake ice: an oasis for life in a polar desert.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Priscu, J C; Fritsen, C H; Adams, E E; Giovannoni, S J; Paerl, H W; McKay, C P; Doran, P T; Gordon, D A; Lanoil, B D; Pinckney, J L</p> <p>1998-06-26</p> <p>The permanent ice covers of <span class="hlt">Antarctic</span> lakes in the McMurdo Dry Valleys develop liquid <span class="hlt">water</span> inclusions in response to solar heating of internal aeolian-derived sediments. The ice sediment particles serve as nutrient (inorganic and organic)-enriched microzones for the establishment of a physiologically and ecologically complex microbial consortium capable of contemporaneous photosynthesis, nitrogen fixation, and decomposition. The consortium is capable of physically and chemically establishing and modifying a relatively nutrient- and organic matter-enriched microbial "oasis" embedded in the lake ice cover.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23465574','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23465574"><span>Monitoring trace elements in <span class="hlt">Antarctic</span> penguin chicks from South Shetland Islands, Antarctica.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Jerez, Silvia; Motas, Miguel; Benzal, Jesús; Diaz, Julia; Barbosa, Andrés</p> <p>2013-04-15</p> <p>The concentration of human activities in the near-shore ecosystems from the northern <span class="hlt">Antarctic</span> Peninsula area can cause an increasing bioavailability of pollutants for the vulnerable <span class="hlt">Antarctic</span> biota. Penguin chicks can reflect this potential impact in the rookeries during the breeding season. They also can reflect biomagnification phenomena since they are on the top of the <span class="hlt">Antarctic</span> food chain. The concentrations of Al, Cr, Mn, Fe, Ni, Cu, Zn, As, Se, Cd and Pb were measured by ICP-MS in samples of liver, kidney, muscle, bone, feather and stomach content of gentoo, chinstrap and Adélie penguin chicks (n=15 individuals) collected opportunistically in the Islands of King George and Deception (South Shetland Islands, Antarctica). The detected levels of some trace elements were not as low as it could be expected in the isolated <span class="hlt">Antarctic</span> region. Penguin chicks can be useful indicators of trace elements abundance in the study areas. Carcasses of <span class="hlt">Antarctic</span> penguin chicks were used to evaluate the bioavailability of trace elements in the Islands of King George and Deception. Copyright © 2013 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27179324','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27179324"><span>Escherichia coli out in the cold: Dissemination of human-derived bacteria into the <span class="hlt">Antarctic</span> microbiome.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Power, Michelle L; Samuel, Angelingifta; Smith, James J; Stark, Jonathon S; Gillings, Michael R; Gordon, David M</p> <p>2016-08-01</p> <p>Discharge of untreated sewage into <span class="hlt">Antarctic</span> environments presents a risk of introducing non-native microorganisms, but until now, adverse consequences have not been conclusively identified. Here we show that sewage disposal introduces human derived Escherichia coli carrying mobile genetic elements and virulence traits with the potential to affect the diversity and evolution of native <span class="hlt">Antarctic</span> microbial communities. We compared E. coli recovered from environmental and animal sources in Antarctica to a reference collection of E. coli from humans and non-<span class="hlt">Antarctic</span> animals. The distribution of phylogenetic groups and frequency of 11 virulence factors amongst the <span class="hlt">Antarctic</span> isolates were characteristic of E. coli strains more commonly associated with humans. The rapidly emerging E. coli ST131 and ST95 clones were found amongst the <span class="hlt">Antarctic</span> isolates, and ST95 was the predominant E. coli recovered from Weddell seals. Class 1 integrons were found in 15% of the <span class="hlt">Antarctic</span> E. coli with 4 of 5 identified gene cassette arrays containing antibiotic resistance genes matching those common in clinical contexts. Disposing untreated sewage into the <span class="hlt">Antarctic</span> environment does disseminate non-native microorganisms, but the extent of this impact and implications for <span class="hlt">Antarctic</span> ecosystem health are, as yet, poorly understood. Copyright © 2016 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.7678M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.7678M"><span><span class="hlt">Antarctic</span> warming driven by internal Southern Ocean deep convection oscillations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Martin, Torge; Pedro, Joel B.; Steig, Eric J.; Jochum, Markus; Park, Wonsun; Rasmussen, Sune O.</p> <p>2016-04-01</p> <p>Simulations with the free-running, complex coupled Kiel Climate Model (KCM) show that heat release associated with recurring Southern Ocean deep convection can drive centennial-scale <span class="hlt">Antarctic</span> temperature variations of 0.5-2.0 °C. We propose a mechanism connecting the intrinsic ocean variability with <span class="hlt">Antarctic</span> warming that involves the following three steps: Preconditioning: heat supplied by the lower branch of the Atlantic Meridional Overturning Circulation (AMOC) accumulates at depth in the Southern Ocean, trapped by the Weddell Gyre circulation; Convection onset: wind and/or sea-ice changes tip the preconditioned, thermally unstable system into the convective state; <span class="hlt">Antarctic</span> warming: fast sea-ice-albedo feedbacks (on annual to decadal timescales) and slower Southern Ocean frontal and sea-surface temperature adjustments to the convective heat release (on multi-decadal to centennial timescales), drive an increase in atmospheric heat and moisture transport towards Antarctica resulting in warming over the continent. Further, we discuss the potential role of this mechanism to explain climate variability observed in <span class="hlt">Antarctic</span> ice-core records.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFMPP23D2084D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMPP23D2084D"><span>Eastern South Pacific <span class="hlt">water</span> mass geometry during the last glacial-interglacial transition</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>De Pol-Holz, R.; Reyes, D.; Mohtadi, M.</p> <p>2012-12-01</p> <p>The eastern South Pacific is characterized today by a complex thermocline structure where large salinity and oxygen changes as a function of depth coexist. Surface <span class="hlt">waters</span> from tropical origin float on top of subantarctic fresher <span class="hlt">water</span> (the so-called 'shallow salinity minimum of the eastern south Pacific'), which in turn, flow above aged equatorial and deeper recently ventilated <span class="hlt">Antarctic</span> <span class="hlt">Intermediate</span> <span class="hlt">waters</span>. Little is known however about the <span class="hlt">water</span> mass geometry changes that could have occurred during the last glacial maximum boundary conditions (about 20,000 years before the present), despite this information being critical for the assessment of potential mechanisms that have been proposed as explanations for the deglacial onset of low oxygen conditions in the area and the atmospheric CO2 increase during the same time. Here we present benthic and planktonic foraminifera stable isotope and radiocarbon data from a set of sediment cores from the Chilean continental margin covering a large -yet still limited- geographical area and depth range. Sedimentations rates were relatively high (>10 cm/kyr) precluding major caveats from bioturbation in all of our archives. The distribution of δ13C of ΣCO2 shows the presence of a very depleted (δ13C < -1‰ V-PDB) <span class="hlt">water</span> mass overlaying more recently ventilated <span class="hlt">waters</span> at <span class="hlt">intermediate</span> depths as indicated by thermocline foraminifer dwellers being more depleted in 13C than the benthic species. The origin of this depleted end-member is probably upwelling from the Southern Ocean as expressed by the radiocarbon content and the large reservoir effect associated with the last glacial maximum and the beginning of the deglaciation along the margin. Our data suggest that the Tropical <span class="hlt">waters</span> that today bath the lower latitude cores was displaced by surface <span class="hlt">waters</span> of southern origin and therefore in line with the evidence of a latitudinal shift of the frontal systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.G52B..03B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.G52B..03B"><span>The East <span class="hlt">Antarctic</span> Ice Sheet and the Gamburtsev Subglacial Mountains (Invited)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bell, R. E.; Studinger, M.; Ferraccioli, F.; Damaske, D.; Finn, C.; Braaten, D. A.; Fahnestock, M. A.; Jordan, T. A.; Corr, H.; Elieff, S.; Frearson, N.; Block, A. E.; Rose, K.</p> <p>2009-12-01</p> <p>Models of the onset of glaciation in Antarctica routinely document the early growth of the ice sheet on the summit of the Gamburtsev Subglacial Mountains in the center of the East <span class="hlt">Antarctic</span> Craton. While ice sheet models replicate the formation of the East <span class="hlt">Antarctic</span> ice sheet 35 million years ago, the age, evolution and structure of the Gamburtsev Mountains remain completely unresolved. During the International Polar Year scientists from seven nations have launched a major collaborative program (AGAP) to explore the Gamburtsev Subglacial Mountains buried by the East <span class="hlt">Antarctic</span> ice sheet and bounded by numerous subglacial lakes. The AGAP umbrella is a multi-national, multi-disciplinary effort and includes aerogeophysics, passive seismology, traverse programs and will be complimented by future ice core and bedrock drilling. A major new airborne data set including gravity; magnetics; ice thickness; SAR images of the ice-bed interface; near-surface and deep internal layers; and ice surface elevation is providing insights into a more dynamic East Antarctica. More than 120,000 km of aerogeophysical data have been acquired from two remote field camps during the 2008/09 field season. AGAP effort was designed to address several fundamental questions including: 1) What role does topography play in the nucleation of continental ice sheets? 2) How do tectonic processes control the formation, distribution, and stability of subglacial lakes? The preliminary analysis of this major new data set indicated these 3000m high mountains are deeply dissected by a dendritic system. The northern margin of the mountain range terminates against the inland extent of the Lambert Graben. Evidence of the onset of glaciation is preserved as cirques and U shaped valleys along the axis of the uplifted massifs. The geomorphology reflects the interaction between the ice sheet and the Gamburtsev Mountains. Bright reflectors in the radar data in the deep valleys indicate the presence of <span class="hlt">water</span> that has</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19286554','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19286554"><span>Recent changes in phytoplankton communities associated with rapid regional climate change along the western <span class="hlt">Antarctic</span> Peninsula.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Montes-Hugo, Martin; Doney, Scott C; Ducklow, Hugh W; Fraser, William; Martinson, Douglas; Stammerjohn, Sharon E; Schofield, Oscar</p> <p>2009-03-13</p> <p>The climate of the western shelf of the <span class="hlt">Antarctic</span> Peninsula (WAP) is undergoing a transition from a cold-dry polar-type climate to a warm-humid sub-<span class="hlt">Antarctic</span>-type climate. Using three decades of satellite and field data, we document that ocean biological productivity, inferred from chlorophyll a concentration (Chl a), has significantly changed along the WAP shelf. Summertime surface Chl a (summer integrated Chl a approximately 63% of annually integrated Chl a) declined by 12% along the WAP over the past 30 years, with the largest decreases equatorward of 63 degrees S and with substantial increases in Chl a occurring farther south. The latitudinal variation in Chl a trends reflects shifting patterns of ice cover, cloud formation, and windiness affecting <span class="hlt">water</span>-column mixing. Regional changes in phytoplankton coincide with observed changes in krill (Euphausia superba) and penguin populations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2007/1047/kp/kp07/of2007-1047kp07.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2007/1047/kp/kp07/of2007-1047kp07.pdf"><span>Late Cenozoic Climate History of the Ross Embayment from the AND-1B Drill Hole: Culmination of Three Decades of <span class="hlt">Antarctic</span> Margin Drilling</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Naish, T.R.; Powell, R.D.; Barrett, P.J.; Levy, R.H.; Henrys, S.; Wilson, G.S.; Krissek, L.A.; Niessen, F.; Pompilio, M.; Ross, J.; Scherer, R.; Talarico, F.; Pyne, A.; ,</p> <p>2007-01-01</p> <p>Because of the paucity of exposed rock, the direct physical record of <span class="hlt">Antarctic</span> Cenozoic glacial history has become known only recently and then largely from offshore shelf basins through seismic surveys and drilling. The number of holes on the continental shelf has been small and largely confined to three areas (McMurdo Sound, Prydz Bay, and <span class="hlt">Antarctic</span> Peninsula), but even in McMurdo Sound, where Oligocene and early Miocene strata are well cored, the late Cenozoic is poorly known and dated. The latest <span class="hlt">Antarctic</span> geological drilling program, ANDRILL, successfully cored a 1285-m-long record of climate history spanning the last 13 m.y. from subsea-floor sediment beneath the McMurdo Ice Shelf (MIS), using drilling systems specially developed for operating through ice shelves. The cores provide the most complete <span class="hlt">Antarctic</span> record to date of ice-sheet and climate fluctuations for this period of Earth’s history. The >60 cycles of advance and retreat of the grounded ice margin preserved in the AND-1B record the evolution of the <span class="hlt">Antarctic</span> ice sheet since a profound global cooling step in deep-sea oxygen isotope records ~14 m.y.a. A feature of particular interest is a ~90-m-thick interval of diatomite deposited during the warm Pliocene and representing an extended period (~200,000 years) of locally open <span class="hlt">water</span>, high phytoplankton productivity, and retreat of the glaciers on land.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_23 --> <div id="page_24" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="461"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018BGeo...15.2393H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018BGeo...15.2393H"><span>Ocean acidification changes the structure of an <span class="hlt">Antarctic</span> coastal protistan community</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hancock, Alyce M.; Davidson, Andrew T.; McKinlay, John; McMinn, Andrew; Schulz, Kai G.; van den Enden, Rick L.</p> <p>2018-04-01</p> <p><span class="hlt">Antarctic</span> near-shore <span class="hlt">waters</span> are amongst the most sensitive in the world to ocean acidification. Microbes occupying these <span class="hlt">waters</span> are critical drivers of ecosystem productivity, elemental cycling and ocean biogeochemistry, yet little is known about their sensitivity to ocean acidification. A six-level, dose-response experiment was conducted using 650 L incubation tanks (minicosms) adjusted to a gradient in fugacity of carbon dioxide (fCO2) from 343 to 1641 µatm. The six minicosms were filled with near-shore <span class="hlt">water</span> from Prydz Bay, East Antarctica, and the protistan composition and abundance was determined by microscopy during 18 days of incubation. No CO2-related change in the protistan community composition was observed during the initial 8 day acclimation period under low light. Thereafter, the response of both autotrophic and heterotrophic protists to fCO2 was species-specific. The response of diatoms was mainly cell size related; microplanktonic diatoms ( > 20 µm) increased in abundance with low to moderate fCO2 (343-634 µatm) but decreased at fCO2 ≥ 953 µatm. Similarly, the abundance of Phaeocystis antarctica increased with increasing fCO2 peaking at 634 µatm. Above this threshold the abundance of micro-sized diatoms and P. antarctica fell dramatically, and nanoplanktonic diatoms ( ≤ 20 µm) dominated, therefore culminating in a significant change in the protistan community composition. Comparisons of these results with previous experiments conducted at this site show that the fCO2 thresholds are similar, despite seasonal and interannual differences in the physical and biotic environment. This suggests that near-shore microbial communities are likely to change significantly near the end of this century if anthropogenic CO2 release continues unabated, with profound ramifications for near-shore <span class="hlt">Antarctic</span> ecosystem food webs and biogeochemical cycling.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19890005140','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19890005140"><span>NMC stratospheric analyses during the 1987 <span class="hlt">Antarctic</span> expedition</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gelman, Melvyn E.; Newman, Paul A.</p> <p>1988-01-01</p> <p>Stratospheric constant pressure analyses of geopotential height and temperature, produced as part of regular operations at the National Meteorological Center (NMC), were used by several participants of the <span class="hlt">Antarctic</span> Ozone Expedition. A brief decription is given of the NMC stratospheric analyses and the data that are used to derive them. In addition, comparisons of the analysis values at the locations of radiosonde and aircraft data are presented to provide indications for assessing the representativeness of the NMC stratospheric analyses during the 1987 <span class="hlt">Antarctic</span> winter-spring period.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA111957','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA111957"><span><span class="hlt">Antarctic</span> Atmospheric Infrasound.</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1981-11-30</p> <p>auroral infra - sonic waves and the atmospheric test of a nuclear weapon in China were all recorded and analyzed in real-time by the new system as...Detection Enhancement by a Pure State Filter, 16 February 1981 The great success of the polarization filter technique with infra - sonic data led to our...Project chronology ) 2. Summary of data collected 3. <span class="hlt">Antarctic</span> infrasonic signals 4. Noise suppression using data-adaptive polarization filters: appli</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19910053898&hterms=melting+ice+caps&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dmelting%2Bice%2Bcaps','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19910053898&hterms=melting+ice+caps&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dmelting%2Bice%2Bcaps"><span>A collection of diverse micrometeorites recovered from 100 tonnes of <span class="hlt">Antarctic</span> blue ice</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Maurette, M.; Olinger, C.; Michel-Levy, M. C.; Kurat, G.; Pourchet, M.</p> <p>1991-01-01</p> <p>A new type of meteoritic material, <span class="hlt">intermediate</span> in size between meteorites and interplanetary dust particles (IDPs), is described. Melting and filtering of about 100 tons of blue ice near Cap Prudhomme, Antarctica, yielded 7500 or more irregular, friable particles and about 1500 melted spherules, about 100 microns in size, both showing a 'chondritic' composition suggestive of an extraterrestrial origin. Analyzed irregular particles appear to be unmelted and have similarities with the fine-grained matrix of primitive carbonaceous chondrites, but are extremely diverse in composition. Isotopic analysis of trapped neon confirms an extraterrestrial origin for 16 of 47 irregular particles and 2 of 19 spherules studied and strongly suggests that they were exposed in space as micrometeoroids. These large <span class="hlt">Antarctic</span> micrometeorites constitute a new family, or at least a new population, of solar system objects, in a mass range corresponding to the bulk of extraterrestrial material accreted by the earth today.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..1215231L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..1215231L"><span>Geomagnetic field observations at a new <span class="hlt">Antarctic</span> site, within the AIMNet project</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lepidi, Stefania; Cafarella, Lili; Santarelli, Lucia; Pietrolungo, Manuela; Urbini, Stefano; Piancatelli, Andrea; Biasini, Fulvio; di Persio, Manuele; Rose, Mike</p> <p>2010-05-01</p> <p>During the 2007-2008 <span class="hlt">antarctic</span> campaign, the Italian PNRA installed a Low Power Magnetometer within the framework of the AIMNet (<span class="hlt">Antarctic</span> International Magnetometer Network) project, proposed and coordinated by BAS. The magnetometer is situated at Talos Dome, around 300 km geographically North-West from Mario Zucchelli Station (MZS), and approximately at the same geomagnetic latitude as MZS. In this work we present a preliminary analysis of the geomagnetic field 1-min data, and a comparison with simultaneous data from different <span class="hlt">Antarctic</span> stations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23850279','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23850279"><span>Rapid glass sponge expansion after climate-induced <span class="hlt">Antarctic</span> ice shelf collapse.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Fillinger, Laura; Janussen, Dorte; Lundälv, Tomas; Richter, Claudio</p> <p>2013-07-22</p> <p>Over 30% of the <span class="hlt">Antarctic</span> continental shelf is permanently covered by floating ice shelves, providing aphotic conditions for a depauperate fauna sustained by laterally advected food. In much of the remaining <span class="hlt">Antarctic</span> shallows (<300 m depth), seasonal sea-ice melting allows a patchy primary production supporting rich megabenthic communities dominated by glass sponges (Porifera, Hexactinellida). The catastrophic collapse of ice shelves due to rapid regional warming along the <span class="hlt">Antarctic</span> Peninsula in recent decades has exposed over 23,000 km(2) of seafloor to local primary production. The response of the benthos to this unprecedented flux of food is, however, still unknown. In 2007, 12 years after disintegration of the Larsen A ice shelf, a first biological survey interpreted the presence of hexactinellids as remnants of a former under-ice fauna with deep-sea characteristics. Four years later, we revisited the original transect, finding 2- and 3-fold increases in glass sponge biomass and abundance, respectively, after only two favorable growth periods. Our findings, along with other long-term studies, suggest that <span class="hlt">Antarctic</span> hexactinellids, locked in arrested growth for decades, may undergo boom-and-bust cycles, allowing them to quickly colonize new habitats. The cues triggering growth and reproduction in <span class="hlt">Antarctic</span> glass sponges remain enigmatic. Copyright © 2013 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26236479','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26236479"><span>Breeding short-tailed shearwaters buffer local environmental variability in south-eastern Australia by foraging in <span class="hlt">Antarctic</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>Berlincourt, Maud; Arnould, John P Y</p> <p>2015-01-01</p> <p>Establishing patterns of movements of free-ranging animals in marine ecosystems is crucial for a better understanding of their feeding ecology, life history traits and conservation. As central place foragers, the habitat use of nesting seabirds is heavily influenced by the resources available within their foraging range. We tested the prediction that during years with lower resource availability, short-tailed shearwaters (Puffinus tenuirostris) provisioning chicks should increase their foraging effort, by extending their foraging range and/or duration, both when foraging in neritic (short trips) and distant oceanic <span class="hlt">waters</span> (long trips). Using both GPS and geolocation data-loggers, at-sea movements and habitat use were investigated over three breeding seasons (2012-14) at two colonies in southeastern Australia. Most individuals performed daily short foraging trips over the study period and inter-annual variations observed in foraging parameters where mainly due to few individuals from Griffith Island, performing 2-day trips in 2014. When performing long foraging trips, this study showed that individuals from both colonies exploited similar zones in the Southern Ocean. The results of this study suggest that individuals could increase their foraging range while exploiting distant feeding zones, which could indicate that short-tailed shearwaters forage in <span class="hlt">Antarctic</span> <span class="hlt">waters</span> not only to maintain their body condition but may also do so to buffer against local environmental stochasticity. Lower breeding performances were associated with longer foraging trips to distant oceanic <span class="hlt">waters</span> in 2013 and 2014 indicating they could mediate reductions in food availability around the breeding colonies by extending their foraging range in the Southern Ocean. This study highlights the importance of foraging flexibility as a fundamental aspect of life history in coastal/pelagic marine central place foragers living in highly variable environments and how these foraging strategies are use to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PNAS..114.3867L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PNAS..114.3867L"><span>Evolution of the early <span class="hlt">Antarctic</span> ice ages</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liebrand, Diederik; de Bakker, Anouk T. M.; Beddow, Helen M.; Wilson, Paul A.; Bohaty, Steven M.; Ruessink, Gerben; Pälike, Heiko; Batenburg, Sietske J.; Hilgen, Frederik J.; Hodell, David A.; Huck, Claire E.; Kroon, Dick; Raffi, Isabella; Saes, Mischa J. M.; van Dijk, Arnold E.; Lourens, Lucas J.</p> <p>2017-04-01</p> <p>Understanding the stability of the early <span class="hlt">Antarctic</span> ice cap in the geological past is of societal interest because present-day atmospheric CO2 concentrations have reached values comparable to those estimated for the Oligocene and the Early Miocene epochs. Here we analyze a new high-resolution deep-sea oxygen isotope (δ18O) record from the South Atlantic Ocean spanning an interval between 30.1 My and 17.1 My ago. The record displays major oscillations in deep-sea temperature and <span class="hlt">Antarctic</span> ice volume in response to the ˜110-ky eccentricity modulation of precession. Conservative minimum ice volume estimates show that waxing and waning of at least ˜85 to 110% of the volume of the present East <span class="hlt">Antarctic</span> Ice Sheet is required to explain many of the ˜110-ky cycles. <span class="hlt">Antarctic</span> ice sheets were typically largest during repeated glacial cycles of the mid-Oligocene (˜28.0 My to ˜26.3 My ago) and across the Oligocene-Miocene Transition (˜23.0 My ago). However, the high-amplitude glacial-interglacial cycles of the mid-Oligocene are highly symmetrical, indicating a more direct response to eccentricity modulation of precession than their Early Miocene counterparts, which are distinctly asymmetrical—indicative of prolonged ice buildup and delayed, but rapid, glacial terminations. We hypothesize that the long-term transition to a warmer climate state with sawtooth-shaped glacial cycles in the Early Miocene was brought about by subsidence and glacial erosion in West Antarctica during the Late Oligocene and/or a change in the variability of atmospheric CO2 levels on astronomical time scales that is not yet captured in existing proxy reconstructions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5393229','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5393229"><span>Evolution of the early <span class="hlt">Antarctic</span> ice ages</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>de Bakker, Anouk T. M.; Beddow, Helen M.; Wilson, Paul A.; Bohaty, Steven M.; Pälike, Heiko; Batenburg, Sietske J.; Hilgen, Frederik J.; Hodell, David A.; Huck, Claire E.; Kroon, Dick; Raffi, Isabella; Saes, Mischa J. M.; van Dijk, Arnold E.; Lourens, Lucas J.</p> <p>2017-01-01</p> <p>Understanding the stability of the early <span class="hlt">Antarctic</span> ice cap in the geological past is of societal interest because present-day atmospheric CO2 concentrations have reached values comparable to those estimated for the Oligocene and the Early Miocene epochs. Here we analyze a new high-resolution deep-sea oxygen isotope (δ18O) record from the South Atlantic Ocean spanning an interval between 30.1 My and 17.1 My ago. The record displays major oscillations in deep-sea temperature and <span class="hlt">Antarctic</span> ice volume in response to the ∼110-ky eccentricity modulation of precession. Conservative minimum ice volume estimates show that waxing and waning of at least ∼85 to 110% of the volume of the present East <span class="hlt">Antarctic</span> Ice Sheet is required to explain many of the ∼110-ky cycles. <span class="hlt">Antarctic</span> ice sheets were typically largest during repeated glacial cycles of the mid-Oligocene (∼28.0 My to ∼26.3 My ago) and across the Oligocene−Miocene Transition (∼23.0 My ago). However, the high-amplitude glacial−interglacial cycles of the mid-Oligocene are highly symmetrical, indicating a more direct response to eccentricity modulation of precession than their Early Miocene counterparts, which are distinctly asymmetrical—indicative of prolonged ice buildup and delayed, but rapid, glacial terminations. We hypothesize that the long-term transition to a warmer climate state with sawtooth-shaped glacial cycles in the Early Miocene was brought about by subsidence and glacial erosion in West Antarctica during the Late Oligocene and/or a change in the variability of atmospheric CO2 levels on astronomical time scales that is not yet captured in existing proxy reconstructions. PMID:28348211</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003EAEJA....14359R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003EAEJA....14359R"><span>A Milankovitch climate control on the Middle Miocene Mediterranean <span class="hlt">Intermediate</span> <span class="hlt">Water</span>: evidence from benthic microfauna and isotope geochemistry of the Ras Il-Pellegrin composite section (Malta island, central Mediterranean)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rocca, D.; Bellanca, A.; Neri, R.; Russo, B.; Sgarrella, F.; Sprovieri, M.</p> <p>2003-04-01</p> <p>The marly sediments of the Blue Clay Formation in the upper part of the Middle Miocene Ras il-Pellegrin composite section (Malta island, central Mediterranean) have been investigated by integrated analysis of benthic microfauna and planktonic and benthic oxygen isotopes. The astronomical calibration of the whole section, obtained by using the astronomical solution of Laskar et al. (1993), indicates for deposition of the analysed sediments a time interval ranging between 13.75 and 12.32 Ma (Sprovieri et al., 2002). This time interval is useful to investigate the oceanographic evolution of the (paleo)Mediterranean after the interruption of communications between the Mediterranean and Indo-Pacific areas. This important paleogeographic event, estimated at about 16 Ma by Johnson (1985) and at about 14.5 Ma by Woodruff and Savin (1991), represented the first step of a progressive oceanographic evolution of the Tethys region <span class="hlt">water</span> masses towards present Mediterranean conditions. A comparison of long-term planktonic and benthic d18O trends suggests that the <span class="hlt">intermediate</span> outflowing Mediterranean <span class="hlt">water</span> (proto-MIW), originated in the surface eastern zone of upper Langhian lower Serravallian (paleo)Mediterranean, had hydrographic and hydrodynamic features similar to those of the present Levantine <span class="hlt">Intermediate</span> <span class="hlt">Water</span> (LIW). Focusing our attention on benthic species which can be considered the best recorders of variation of proto-MIW production, we elaborated benthic data by Q-mode varimax principal factor analysis. Spectral analysis was carried out only on two factors which have a clear paleoecological significance: Factor 1 (loaded by Cibicidoides ungerianus and Siphonina reticulata) indicative of oxic bottom <span class="hlt">waters</span> and Factor 2 (loaded by Bulimina elongata group) indicative of oxygen stressed conditions. Results of these analyses show that Factor 1 and Factor 2 curves are respectively in and out of phase with maxima of the eccentricity (100 and 400 kyr). Factor 1 is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29785671','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29785671"><span>Agarolytic culturable bacteria associated with three <span class="hlt">antarctic</span> subtidal macroalgae.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sánchez Hinojosa, Verónica; Asenjo, Joel; Leiva, Sergio</p> <p>2018-05-21</p> <p>Bacterial communities of <span class="hlt">Antarctic</span> marine macroalgae remain largely underexplored in terms of diversity and biotechnological applications. In this study, three <span class="hlt">Antarctic</span> subtidal macroalgae (Himantothallus grandifolius, Pantoneura plocamioides and Plocamium cartilagineum), two of them endemic of Antarctica, were investigated as a source for isolation of agar-degrading bacteria. A total of 21 epiphytic isolates showed agarolytic activity at low temperature on agar plates containing agar as the sole carbon source. 16S rRNA identification showed that the agar-degrading bacteria belonged to the genera Cellulophaga, Colwellia, Lacinutrix, Olleya, Paraglaciecola, Pseudoalteromonas and Winogradskyella. The agarase enzyme from a potential new species of the genus Olleya was selected for further purification. The enzyme was purified from the culture supernatant of Olleya sp. HG G5.3 by ammonium sulfate precipitation and ion-exchange chromatography. Molecular weight of the agarase was estimated to be 38 kDa by sodium dodecyl sulfate-polyacrylamide gel electrophoresis (SDS-PAGE). The purified enzyme exhibited activity at 4 °C, retaining > 50% of its maximum activity at this temperature. This is the first study reporting the phylogeny of agar-degrading bacteria isolated from <span class="hlt">Antarctic</span> subtidal macroalgae and the results suggest the huge potential of <span class="hlt">Antarctic</span> algae-associated bacteria as a source of cold-active hydrolytic enzymes of biotechnological interest.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFMGC23E0968K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFMGC23E0968K"><span>Integrating <span class="hlt">Antarctic</span> Science Into Geospace System Science</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kelly, J. D.</p> <p>2010-12-01</p> <p>Addressing the scientific, technical, and sociological challenges of the future requires both detailed basic research and system based approaches to the entire geospace system from the Earth’s core, through solid Earth, ice, oceans, atmosphere, ionosphere, and magnetosphere to the Sun’s outer atmosphere and even beyond. Fully integrating <span class="hlt">Antarctic</span> science, and fully exploiting the scientific research possibilities of the <span class="hlt">Antarctic</span> continent through effective and efficient support infrastructure, will be a very important contribution to future success. Amongst many new facilities and programs which can and are being proposed, the Moveable <span class="hlt">Antarctic</span> Incoherent Scatter Radar (MAISR) at McMurdo illustrates the potential for innovative future science. This poster uses some of the proposed science programs to show how the scientific community can use the data products of this facility, and how they can contribute to the development of the tools and mechanisms for proposing, executing, and utilizing such new research capabilities. In particular, incoherent scatter radars played a big role in data collection during the recent International Polar Year and plans for future extended operations, including those in Antarctica, will be discussed in the light of lessons learnt in applying observations to global modeling developments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017RvGeo..55..434H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017RvGeo..55..434H"><span>Instability of the <span class="hlt">Antarctic</span> Ross Sea Embayment as climate warms</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hughes, Terence; Zhao, Zihong; Hintz, Raymond; Fastook, James</p> <p>2017-06-01</p> <p>Collapse of the <span class="hlt">Antarctic</span> Ice Sheet since the Last Glacial Maximum 18,000 years ago is most pronounced in the Ross Sea Embayment, which is partly ice-free during <span class="hlt">Antarctic</span> summers, thereby breaching the O-ring of ice shelves and sea ice surrounding Antarctica that stabilizes the ice sheet. The O-ring may have vanished during Early Holocene (5000 to 3000 B.C.), Roman (1 to 400 A.D.), and Medieval (900 to 1300 A.D.) warm periods and reappeared during the Little Ice Age (1300 to 1900 A.D.). We postulate further collapse in the embayment during the post-1900 warming may be forestalled because East <span class="hlt">Antarctic</span> outlet glaciers "nail" the Ross Ice Shelf to the Transantarctic Mountains so it can resist the push from West <span class="hlt">Antarctic</span> ice streams. Our hypothesis is examined for Byrd Glacier and a static ice shelf using three modeling experiments having plastic, viscous, and viscoplastic solutions as more data and improved modeling became available. Observed crevasse patterns were not reproduced. A new research study is needed to model a dynamic Ross Ice Shelf with all its feeder ice streams, outlet glaciers, and ice calving dynamics in three dimensions over time to fully test our hypothesis. The required model must allow accelerated calving if further warming melts sea ice and discerps the ice shelf. Calving must then successively pull the outlet glacier "nails" so collapse of the marine West <span class="hlt">Antarctic</span> Ice Sheet proceeds to completion.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26674690','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26674690"><span>Levoglucosan and phenols in <span class="hlt">Antarctic</span> marine, coastal and plateau aerosols.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zangrando, Roberta; Barbaro, Elena; Vecchiato, Marco; Kehrwald, Natalie M; Barbante, Carlo; Gambaro, Andrea</p> <p>2016-02-15</p> <p>Due to its isolated location, Antarctica is a natural laboratory for studying atmospheric aerosols and pollution in remote areas. Here, we determined levoglucosan and phenolic compounds (PCs) at diverse <span class="hlt">Antarctic</span> sites: on the plateau, a coastal station and during an oceanographic cruise. Levoglucosan and PCs reached the <span class="hlt">Antarctic</span> plateau where they were observed in accumulation mode aerosols (with median levoglucosan concentrations of 6.4 pg m(-3) and 4.1 pg m(-3), and median PC concentrations of 15.0 pg m(-3) and 7.3 pg m(-3)). Aged aerosols arrived at the coastal site through katabatic circulation with the majority of the levoglucosan mass distributed on larger particulates (24.8 pg m(-3)), while PCs were present in fine particles (34.0 pg m(-3)). The low levoglucosan/PC ratios in <span class="hlt">Antarctic</span> aerosols suggest that biomass burning aerosols only had regional, rather than local, sources. General acid/aldehyde ratios were lower at the coastal site than on the plateau. Levoglucosan and PCs determined during the oceanographic cruise were 37.6 pg m(-3) and 58.5 pg m(-3) respectively. Unlike levoglucosan, which can only be produced by biomass burning, PCs have both biomass burning and other sources. Our comparisons of these two types of compounds across a range of <span class="hlt">Antarctic</span> marine, coastal, and plateau sites demonstrate that local marine sources dominate <span class="hlt">Antarctic</span> PC concentrations. Copyright © 2015 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19860006697','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19860006697"><span><span class="hlt">Antarctic</span> Meteorite Newsletter, Volume 8, Number 2</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1985-01-01</p> <p>Requests for samples are welcomed from research scientists of all countries, regardless of their current state of funding for meteorite studies. All sample requests will be reviewed by the Meteorite Working Group (MWG), a peer-review committee that guides the collection, curation, allocation, and distribution of the U.S. <span class="hlt">Antarctic</span> meteorites. Issurance of samples does not imply a commitment by any agency to fund the proposed research. Requests for financial support must be submitted separately to the appropriate funding agencies. As a matter of policy, U.S. <span class="hlt">Antarctic</span> meteorites are the property of the National Science Foundation and all allocations are subject to recall.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA596885','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA596885"><span>Designing a Maintainable and Sustainable Coast Guard Icebreaker for Arctic and <span class="hlt">Antarctic</span> Operations</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2014-03-21</p> <p>03-2014 Technical June 2013-August 2013 Designing a Maintainable and Sustainable Coast Guard Icebreaker for Arctic and <span class="hlt">Antarctic</span> Operations...of Engineering Designing a Maintainable and Sustainable Coast Guard Icebreaker for Arctic and <span class="hlt">Antarctic</span> Operations Abstract The U.S. Coast Guard is...Pollution (MARPOL) of which Annex V prohibits the discharge of solid waste other than food refuge less than 25mm in diameter into the <span class="hlt">Antarctic</span> Region [6</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.G21B0871F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.G21B0871F"><span>A new research project on the interaction of the solid Earth and the <span class="hlt">Antarctic</span> Ice Sheet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fukuda, Y.; Nishijima, J.; Kazama, T.; Nakamura, K.; Doi, K.; Suganuma, Y.; Okuno, J.; Araya, A.; Kaneda, H.; Aoyama, Y.</p> <p>2017-12-01</p> <p>A new research project of "Grant-in-Aid for Scientific Research on Innovative Areas" funded by JSPS (Japan Society for the Promotion of Science) has recently been launched. The title of the project is "Giant reservoirs of heat/<span class="hlt">water</span>/material: Global environmental changes driven by Southern Ocean and <span class="hlt">Antarctic</span> Ice Sheet", and as a five years project, is aiming to establish a new research area for <span class="hlt">Antarctic</span> environmental system science. The project consists of 7 research topics, including <span class="hlt">Antarctic</span> ice sheet and Southern ocean sciences, new observation methodology, modeling and other interdisciplinary topics, and we are involved in the topic A02-2, "Interaction of the solid Earth and the <span class="hlt">Antarctic</span> Ice Sheet". The <span class="hlt">Antarctic</span> ice sheet, which relates to the global climate changes through the sea level rise and ocean circulation, is an essential element of the Earth system for predicting the future environment changes. Thus many studies of the ice sheet changes have been conducted by means of geomorphological, geological, geodetic surveys, as well as satellite gravimetry and satellite altimetry. For these studies, one of the largest uncertainties is the effects of GIA. Therefore, GIA as a key to investigate the interaction between the solid Earth and the ice sheet changes, we plan to conduct geomorphological, geological and geodetic surveys in the inland mountain areas and the coastal areas including the surrounding areas of a Japanese station Syowa in East Antarctica, where the in-situ data for constraining GIA models are very few. Combining these new observations with other in-site data, various satellite data and numerical modeling, we aim to estimating a precise GIA model, constructing a reliable ice melting history after the last glacial maximum and obtaining the viscoelastic structure of the Earth's interior. In the presentation, we also show the five years research plans as well. This study was partially supported by JSPS KAKENHI Grant No. 17H06321.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20020048255&hterms=enrichment&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Denrichment','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20020048255&hterms=enrichment&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Denrichment"><span>Sublimation: A Mechanism for the Enrichment of Organics in <span class="hlt">Antarctic</span> Ice</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Becker, Luann; McDonald, Gene D.; Glavin, Daniel P.; Bada, Jeffrey L.; Bunch, Theodore E.; Chang, Sherwood (Technical Monitor)</p> <p>1997-01-01</p> <p>Recent analyses of the carbonate globules present in the Martian meteorite ALH84001 have detected polycyclic aromatic hydrocarbons (PAHs) at the ppm level. The distribution of PAHs observed in ALH84001 was interpreted as being inconsistent with a terrestrial origin and were claimed to be indigenous to the meteorite, perhaps derived from an ancient Martian biota. However, Becker et al., have examined PAHs in the Martian meteorite EETA79001, in several <span class="hlt">Antarctic</span> carbonaceous chondrites and <span class="hlt">Antarctic</span> Allan Hills Ice and detected many of the same PAHs found in ALH84001. The reported presence of L-amino acids of apparent terrestrial origin in the EETA79001 druse material, suggests that this meteorite is contaminated with terrestrial/extraterrestrial organics probably derived from <span class="hlt">Antarctic</span> ice meltwater that had percolated through the meteorite. The detection of PAHs and L-amino acids in these Martian meteorites suggests that despite storage in the <span class="hlt">Antarctic</span> ice, selective changes of certain chemical and mineralogical phases has occurred.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011PolSc...5..239V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011PolSc...5..239V"><span>Food preferences of larvae of <span class="hlt">Antarctic</span> silverfish Pleuragramma antarcticum Boulenger, 1902 from Terre Adélie coastal <span class="hlt">waters</span> during summer 2004</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vallet, Carole; Beans, Cristina; Koubbi, Philippe; Courcot, Lucie; Hecq, Jean-Henri; Goffart, Anne</p> <p>2011-08-01</p> <p>Ichthyoplankton samples were collected from 19 to 31 January 2004 in the Dumont d’Urville Sea (East <span class="hlt">Antarctic</span> shelf). The Nototheniidae Pleuragramma antarcticum comprised more than 90% of the sampled larvae. Gut contents of 95 P antarcticum larvae were examined. Most larvae fed on phytoplankton, especially diatoms, whereas some other specimens had a mixed diet with phyto- and zooplankton prey. A single specimen fed exclusively on copepods. The stomach contents was dominated by three diatoms taxa, such as Thalassiothrix antarctica, Fragilariopsis spp. and Chaetoceros spp. Prey selection was apparently food density dependent, with an inverse relationship between food abundance and selection feeding. Larvae selected positively some diatoms, such as Coscinodiscus spp. and T. antarctica, presenting a low concentration in the <span class="hlt">water</span> column compared to Fragilariopsis spp., which were strongly negatively selected. During summer, larvae were opportunistic feeders with a broad trophic niche, which allowed them to switch between different food types.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2013-05-13/pdf/2013-11265.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2013-05-13/pdf/2013-11265.pdf"><span>78 FR 28000 - Notice of Permit Applications Received Under the <span class="hlt">Antarctic</span> Conservation Act of 1978</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>2013-05-13</p> <p>... Conservation Act of 1978 AGENCY: National Science Foundation. ACTION: Notice of Permit Applications Received under the <span class="hlt">Antarctic</span> Conservation Act of 1978, Public Law 95-541. SUMMARY: The National Science... regulated under the <span class="hlt">Antarctic</span> Conservation Act of 1978. NSF has published regulations under the <span class="hlt">Antarctic</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_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_24 --> <div id="page_25" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li class="active"><span>25</span></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="481"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2012-11-09/pdf/2012-27383.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2012-11-09/pdf/2012-27383.pdf"><span>77 FR 67407 - Notice of Permit Applications Received Under the <span class="hlt">Antarctic</span> Conservation Act of 1978</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>2012-11-09</p> <p>... Conservation Act of 1978 AGENCY: National Science Foundation. ACTION: Notice of Permit Applications Received under the <span class="hlt">Antarctic</span> Conservation Act of 1978, Public Law 95-541. SUMMARY: The National Science... regulated under the <span class="hlt">Antarctic</span> Conservation Act of 1978. NSF has published regulations under the <span class="hlt">Antarctic</span>...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2012-06-29/pdf/2012-15885.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2012-06-29/pdf/2012-15885.pdf"><span>77 FR 38834 - Notice of Permit Applications Received Under the <span class="hlt">Antarctic</span> Conservation Act of 1978</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>2012-06-29</p> <p>... Conservation Act of 1978 AGENCY: National Science Foundation. ACTION: Notice of permit applications received under the <span class="hlt">Antarctic</span> Conservation Act of 1978. SUMMARY: The National Science Foundation (NSF) is required... <span class="hlt">Antarctic</span> Conservation Act of 1978. NSF has published regulations under the <span class="hlt">Antarctic</span> Conservation Act. This...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C13D..08T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C13D..08T"><span>Grounding Zones, Subglacial Lakes, and Dynamics of an <span class="hlt">Antarctic</span> Ice Stream: The WISSARD Glaciological Experiment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tulaczyk, S. M.; Schwartz, S. Y.; Fisher, A. T.; Powell, R. D.; Fricker, H. A.; Anandakrishnan, S.; Horgan, H. J.; Scherer, R. P.; Walter, J. I.; Siegfried, M. R.; Mikucki, J.; Christianson, K.; Beem, L.; Mankoff, K. D.; Carter, S. P.; Hodson, T. O.; Marsh, O.; Barcheck, C. G.; Branecky, C.; Neuhaus, S.; Jacobel, R. W.</p> <p>2015-12-01</p> <p>Interactions of West <span class="hlt">Antarctic</span> ice streams with meltwater at their beds, and with seawater at their grounding lines, are widely considered to be the primary drivers of ice stream flow variability on different timescales. Understanding of processes controlling ice flow variability is needed to build quantitative models of the <span class="hlt">Antarctic</span> Ice Sheet that can be used to help predict its future behavior and to reconstruct its past evolution. The ice plain of Whillans Ice Stream provides a natural glaciological laboratory for investigations of <span class="hlt">Antarctic</span> ice flow dynamics because of its highly variable flow rate modulated by tidal processes and fill-drain cycles of subglacial lakes. Moreover, this part of Antarctica has one of the longest time series of glaciological observations, which can be used to put recently acquired datasets in a multi-decadal context. Since 2007 Whillans Ice Stream has been the focus of a regional glaciological experiment, which included surface GPS and passive-source seismic sensors, radar and seismic imaging of subglacial properties, as well as deep borehole geophysical sensors. This experiment was possible thanks to the NSF-funded multidisciplinary WISSARD project (Whillans Ice Stream Subglacial Access Research Drilling). Here we will review the datasets collected during the WISSARD glaciological experiment and report on selected results pertaining to interactions of this ice stream with <span class="hlt">water</span> at its bed and its grounding line.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1988ClDy....3...93C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1988ClDy....3...93C"><span>Late Pleistocene variations in <span class="hlt">Antarctic</span> sea ice II: effect of interhemispheric deep-ocean heat exchange</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Crowley, Thomas J.; Parkinson, Claire L.</p> <p>1988-10-01</p> <p>Variations in production rates of warm North Atlantic Deep <span class="hlt">Water</span> (NADW) have been proposed as a mechanism for linking climate fluctuations in the northern and southern hemispheres during the Pleistocene. We have tested this hypothesis by examining the sensitivity of a thermodynamic/dynamic model for <span class="hlt">Antarctic</span> sea ice to changes in vertical ocean heat flux and comparing the simulations with modified CLIMAP sea-ice maps for 18 000 B.P. Results suggest that changes in NADW production rates, and the consequent changes in the vertical ocean heat flux in the <span class="hlt">Antarctic</span>, can only account for about 20% 30% of the overall variance in <span class="hlt">Antarctic</span> sea-ice extent. This conclusion has been validated against an independent geological data set involving a time series of sea-surface temperatures from the subantarctic. The latter comparison suggests that, although the overall influence of NADW is relatively minor, the linkage may be much more significant at the 41 000-year obliquity period. Despite some limitations in the models and geological data, we conclude that NADW variations may have played only a modest role in causing late Pleistocene climate change in the high latitudes of the southern hemisphere. Our conclusion is consistent with calculations by Manabe and Broccoli (1985) suggesting that atmospheric CO2 changes may be more important for linking the two hemispheres.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..14..221R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..14..221R"><span>Integral Quantification of Soil <span class="hlt">Water</span> Content at the <span class="hlt">Intermediate</span> Catchment Scale by Ground Albedo Neutron Sensing (GANS)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rivera Villarreyes, C. A.; Baroni, G.; Oswald, S. E.</p> <p>2012-04-01</p> <p>Soil <span class="hlt">water</span> content at the plot or hill-slope scale is an important link between local vadose zone hydrology and catchment hydrology. However, so far only few methods are on the way to close this gap between point measurements and remote sensing. One new measurement methodology for integral quantifications of mean areal soil <span class="hlt">water</span> content at the <span class="hlt">intermediate</span> catchment scale is the aboveground sensing of cosmic-ray neutrons, more precisely ground albedo neutron sensing (GANS). Ground albedo natural neutrons, are generated by collisions of secondary cosmic rays with land surface materials (soil, <span class="hlt">water</span>, biomass, snow, etc). Neutrons measured at the air/ground interface correlate with soil moisture contained in a footprint of ca. 600 m diameter and a depth ranging down to a few decimeters. This correlation is based on the crucial role of hydrogen as neutron moderator compared to others landscape materials. The present study performed ground albedo neutron sensing in different locations in Germany under different vegetative situations (cropped and bare field) and different seasonal conditions (summer, autumn and winter). Ground albedo neutrons were measured at (i) a farmland close to Potsdam (Brandenburg, Germany) cropped with corn in 2010 and sunflowers in 2011, and (ii) a mountainous farmland catchment (Schaefertal, Harz Mountains, Germany) in 2011. In order to test this method, classical soil moisture devices and meteorological data were used for comparison. Moreover, calibration approach, and transferability of calibration parameters to different times and locations are also evaluated. Our observations suggest that GANS can overcome the lack of data for hydrological processes at the <span class="hlt">intermediate</span> scale. Soil <span class="hlt">water</span> content from GANS compared quantitatively with mean <span class="hlt">water</span> content values derived from a network of classical devices (RMSE = 0.02 m3/m3 and r2 = 0.98) in three calibration periods with cropped-field conditions. Then, same calibration parameters corresponded</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120010315','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120010315"><span>Decadal Trends in Abundance, Size and Condition of <span class="hlt">Antarctic</span> Toothfish in McMurdo Sound, Antarctica, 1972-2010</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ainley, David G.; Nur, Nadav; Eastman, Joseph T.; Ballard. Grant; Parkinson, Claire L; Evans, Clive W.; DeVries, Arthur L.</p> <p>2012-01-01</p> <p>We report analyses of a dataset spanning 38 years of near-annual fishing for <span class="hlt">Antarctic</span> toothfish Dissostichus mawsoni, using a vertical setline through the fast ice of McMurdo Sound, Antarctica, 1972-2010. This constitutes one of the longest biological time series in the Southern Ocean, and certainly the longest for any fish. Fish total length, condition and catch per unit effort (CPUE) were derived from the more than 5500 fish caught. Contrary to expectation, length-frequency was dominated by fish in the upper half of the industrial catch. The discrepancy may be due to biases in the sampling capabilities of vertical (this study) versus benthic (horizontal) fishing gear (industry long lines), related to the fact that only large <span class="hlt">Antarctic</span> toothfish (more than 100 cm TL) are neutrally buoyant and occur in the <span class="hlt">water</span> column. Fish length and condition increased from the early 1970s to the early 1990s and then decreased, related to sea ice cover, with lags of 8 months to 5 years, and may ultimately be related to the fishery (which targets large fish) and changes in the Southern Annular Mode through effects on toothfish main prey, <span class="hlt">Antarctic</span> silverfish Pleuragramma antarcticum. CPUE was constant through 2001 and then decreased dramatically, likely related to the industrial fishery, which began in 1996 and which concentrates effort over the Ross Sea slope, where tagged McMurdo fish have been found. Due to limited prey choices and, therefore, close coupling among mesopredators of the Ross Sea, <span class="hlt">Antarctic</span> toothfish included, the fishery may be altering the trophic structure of the Ross Sea.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/9750970','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/9750970"><span>Studies of evolutionary temperature adaptation: muscle function and locomotor performance in <span class="hlt">Antarctic</span> fish.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Franklin, C E</p> <p>1998-09-01</p> <p>1. Studies of evolutionary temperature adaptation of muscle and locomotor performance in fish are reviewed with a focus on the <span class="hlt">Antarctic</span> fauna living at subzero temperatures. 2. Only limited data are available to compare the sustained and burst swimming kinematics and performance of <span class="hlt">Antarctic</span>, temperate and tropical species. Available data indicate that low temperatures limit maximum swimming performance and this is especially evident in fish larvae. 3. In a recent study, muscle performance in the <span class="hlt">Antarctic</span> rock cod Notothenia coriiceps at 0 degree C was found to be sufficient to produce maximum velocities during burst swimming that were similar to those seen in the sculpin Myoxocephalus scorpius at 10 degrees C, indicating temperature compensation of muscle and locomotor performance in the <span class="hlt">Antarctic</span> fish. However, at 15 degrees C, sculpin produce maximum swimming velocities greater than N. coriiceps at 0 degree C. 4. It is recommended that strict hypothesis-driven investigations using ecologically relevant measures of performance are undertaken to study temperature adaptation in <span class="hlt">Antarctic</span> fish. Recent detailed phylogenetic analyses of the <span class="hlt">Antarctic</span> fish fauna and their temperate relatives will allow a stronger experimental approach by helping to separate what is due to adaptation to the cold and what is due to phylogeny alone.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011DSRII..58.1729F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011DSRII..58.1729F"><span>Ecological niche modeling of sympatric krill predators around Marguerite Bay, Western <span class="hlt">Antarctic</span> Peninsula</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Friedlaender, Ari S.; Johnston, David W.; Fraser, William R.; Burns, Jennifer; Halpin, Patrick N.; Costa, Daniel P.</p> <p>2011-07-01</p> <p>Adélie penguins ( Pygoscelis adeliae), carabeater seals ( Lobodon carcinophagus), humpback ( Megaptera novaeangliae), and minke whales ( Balaenoptera bonaernsis) are found in the <span class="hlt">waters</span> surrounding the Western <span class="hlt">Antarctic</span> Peninsula. Each species relies primarily on <span class="hlt">Antarctic</span> krill ( Euphausia superba) and has physiological constraints and foraging behaviors that dictate their ecological niches. Understanding the degree of ecological overlap between sympatric krill predators is critical to understanding and predicting the impacts on climate-driven changes to the <span class="hlt">Antarctic</span> marine ecosystem. To explore ecological relationships amongst sympatric krill predators, we developed ecological niche models using a maximum entropy modeling approach (Maxent) that allows the integration of data collected by a variety of means (e.g. satellite-based locations and visual observations). We created spatially explicit probability distributions for the four krill predators in fall 2001 and 2002 in conjunction with a suite of environmental variables. We find areas within Marguerite Bay with high krill predator occurrence rates or biological hot spots. We find the modeled ecological niches for Adélie penguins and crabeater seals may be affected by their physiological needs to haul-out on substrate. Thus, their distributions may be less dictated by proximity to prey and more so by physical features that over time provide adequate access to prey. Humpback and minke whales, being fully marine and having greater energetic demands, occupy ecological niches more directly proximate to prey. We also find evidence to suggest that the amount of overlap between modeled niches is relatively low, even for species with similar energetic requirements. In a rapidly changing and variable environment, our modeling work shows little indication that krill predators maintain similar ecological niches across years around Marguerite Bay. Given the amount of variability in the marine environment around the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17843316','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17843316"><span>Physical conditions at the base of a fast moving <span class="hlt">antarctic</span> ice stream.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Engelhardt, H; Humphrey, N; Kamb, B; Fahnestock, M</p> <p>1990-04-06</p> <p>Boreholes drilled to the bottom of ice stream B in the West <span class="hlt">Antarctic</span> Ice Sheet reveal that the base of the ice stream is at the melting point and the basal <span class="hlt">water</span> pressure is within about 1.6 bars of the ice overburden pressure. These conditions allow the rapid ice streaming motion to occur by basal sliding or by shear deformation of unconsolidated sediments that underlie the ice in a layer at least 2 meters thick. The mechanics of ice streaming plays a role in the response of the ice sheet to climatic change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSAH54A0112S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSAH54A0112S"><span>Temperature and pH effects on feeding and growth of <span class="hlt">Antarctic</span> krill</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Saba, G.; Bockus, A.; Fantasia, R. L.; Shaw, C.; Sugla, M.; Seibel, B.</p> <p>2016-02-01</p> <p>Rapid warming in the Western <span class="hlt">Antarctic</span> Peninsula (WAP) region is occurring, and is associated with an overall decline in primary, secondary, and higher trophic levels, including <span class="hlt">Antarctic</span> krill (Euphausia superba), a key species in <span class="hlt">Antarctic</span> food webs. Additionally, there are predictions that by the end of this century the Southern Ocean will be one of the first regions to be affected by seawater chemistry changes associated with enhanced CO2. Ocean acidification and warming may act synergistically to impair animal performance, which may negatively impact <span class="hlt">Antarctic</span> krill. We assessed the effects of temperature (ambient temperature, ambient +3 degrees C) and pH (Experiment 1 = 8.0, 7.7; Experiment 2 = 8.0, 7.5, 7.1) on juvenile <span class="hlt">Antarctic</span> krill feeding and growth (growth increment and intermolt period) during incubation experiments at Palmer Station, Antarctica. Food intake was lower in krill exposed to reduced pH. Krill intermolt period (IMP) was significantly lower in the elevated temperature treatments (16.9 days) compared to those at 0 degrees (22.8 days). Within the elevated temperature treatment, minor increases in IMP occurred in krill exposed reduced pH. Growth increment (GI) was lower with decreased pH at the first molt, and this was exacerbated at elevated temperature. However, differences in GI were eliminated between the first and second molts suggesting potential ability of <span class="hlt">Antarctic</span> krill to acclimate to changes in temperature and pH. Reductions in juvenile krill growth and feeding under elevated temperature and reduced pH are likely caused by higher demands for internal acid-base regulation or a metabolic suppression. However, the subtlety of these feeding and growth responses leaves an open question as to how krill populations will tolerate prolonged future climate change in the <span class="hlt">Antarctic</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24299658','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24299658"><span>Ocean acidification and fertilization in the <span class="hlt">antarctic</span> sea urchin Sterechinus neumayeri: the importance of polyspermy.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sewell, Mary A; Millar, Russell B; Yu, Pauline C; Kapsenberg, Lydia; Hofmann, Gretchen E</p> <p>2014-01-01</p> <p>Ocean acidification (OA), the reduction of the seawater pH as a result of increasing levels of atmospheric CO2, is an important climate change stressor in the Southern Ocean and <span class="hlt">Antarctic</span>. We examined the impact of OA on fertilization success in the <span class="hlt">Antarctic</span> sea urchin Sterechinus neumayeri using pH treatment conditions reflective of the current and near-future "pH seascape" for this species: current (control: pH 8.052, 384.1 μatm of pCO2), a high CO2 treatment approximating the 0.2-0.3 unit decrease in pH predicted for 2100 (high CO2: pH 7.830, 666.0 μatm of pCO2), and an <span class="hlt">intermediate</span> medium CO2 (pH 7.967, 473.4 μatm of pCO2). Using a fertilization kinetics approach and mixed-effect models, we observed significant variation in the OA response between individual male/female pairs (N = 7) and a significant population-level increase (70-100%) in tb (time for a complete block to polyspermy) at medium and high CO2, a mechanism that potentially explains the higher levels of abnormal development seen in OA conditions. However, two pairs showed higher fertilization success with CO2 treatment and a nonsignificant effect. Future studies should focus on the mechanisms and levels of interindividual variability in OA response, so that we can consider the potential for selection and adaptation of organisms to a future ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.8308R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.8308R"><span><span class="hlt">Antarctic</span> sub-shelf melt rates via SIMPEL</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Reese, Ronja; Albrecht, Torsten; Winkelmann, Ricarda</p> <p>2017-04-01</p> <p>Ocean-induced melting below ice-shelves is currently suspected to be the dominant cause of mass loss from the <span class="hlt">Antarctic</span> Ice Sheet (e.g. Depoorter et al. 2013). Although thinning of ice shelves does not directly contribute to sea-level rise, it may have a significant indirect impact through the potential of ice shelves to buttress their adjacent ice sheet. Hence, an appropriate representation of sub-shelf melt rates is essential for modelling the evolution of ice sheets with marine terminating outlet glaciers. Due to computational limits of fully-coupled ice and ocean models, sub-shelf melt rates are often parametrized in large-scale or long-term simulations (e.g. Matin et al. 2011, Pollard & DeConto 2012). These parametrizations usually depend on the depth of the ice shelf base or its local slope but do not include the physical processes in ice shelf cavities. Here, we present the Sub Ice shelf Melt Potsdam modEL (SIMPEL) which mimics the first-order large-scale circulation in ice shelf cavities based on an ocean box model (Olbers & Hellmer, 2010), implemented in the Parallel Ice Sheet Model (Bueler & Brown 2009, Winkelmann et al. 2011, www.pism-docs.org). In SIMPEL, ocean <span class="hlt">water</span> is transported at depth towards the grounding line where sub-shelf melt rates are highest, and then rises along the shelf base towards the calving front where refreezing can occur. Melt rates are computed by a description of ice-ocean interaction commonly used in high-resolution models (McPhee 1992, Holland & Jenkins 1999). This enables the model to capture a wide-range of melt rates, comparable to the observed range for <span class="hlt">Antarctic</span> ice shelves (Rignot et al. 2013).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C51A0962S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C51A0962S"><span>A 25-year Record of <span class="hlt">Antarctic</span> Ice Sheet Elevation and Mass Change</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shepherd, A.; Muir, A. S.; Sundal, A.; McMillan, M.; Briggs, K.; Hogg, A.; Engdahl, M.; Gilbert, L.</p> <p>2017-12-01</p> <p>Since 1992, the European Remote-Sensing (ERS-1 and ERS-2), ENVISAT, and CryoSat-2 satellite radar altimeters have measured the <span class="hlt">Antarctic</span> ice sheet surface elevation, repeatedly, at approximately monthly intervals. These data constitute the longest continuous record of ice sheet wide change. In this paper, we use these observations to determine changes in the elevation, volume and mass of the East <span class="hlt">Antarctic</span> and West <span class="hlt">Antarctic</span> ice sheets, and of parts of the <span class="hlt">Antarctic</span> Peninsula ice sheet, over a 25-year period. The root mean square difference between elevation rates computed from our survey and 257,296 estimates determined from airborne laser measurements is 54 cm/yr. The longevity of the satellite altimeter data record allows to identify and chart the evolution of changes associated with meteorology and ice flow, and we estimate that 3.6 % of the continental ice sheet, and 21.7 % of West Antarctica, is in a state of dynamical imbalance. Based on this partitioning, we estimate the mass balance of the East and West <span class="hlt">Antarctic</span> ice sheet drainage basins and the root mean square difference between these and independent estimates derived from satellite gravimetry is less than 5 Gt yr-1.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMPP11A2001W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMPP11A2001W"><span>A Critical Test of Nd isotopes as a Paleocirculation Proxy in the Southwest Atlantic</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wu, Y.; Goldstein, S. L.; Pena, L.; Hartman, A. E.; Rijkenberg, M. J. A.; de Baar, H. J. W.</p> <p>2016-12-01</p> <p>The application of Nd isotopes as a paleo-ocean circulation tracer assumes that Nd isotope ratios (ɛNd) effectively fingerprint different <span class="hlt">water</span> masses and approximate expected values from <span class="hlt">water</span> mass mixing. The Southwest Atlantic, with the major <span class="hlt">water</span> masses involved in the Atlantic Meridional Ocean Circulation (southward flowing North Atlantic Deep <span class="hlt">Water</span>, northward flowing <span class="hlt">Antarctic</span> <span class="hlt">Intermediate</span> <span class="hlt">Water</span> and <span class="hlt">Antarctic</span> Bottom <span class="hlt">Water</span>), is one of the best places on Earth to evaluate how well Nd isotope ratios act like a conservative <span class="hlt">water</span> mass tracer in the modern ocean. Seawater profiles and core-top sediments from 17 stations were sampled in the Southwest Atlantic in the South Atlantic Meridional GEOTRACES cruise (GA02 Leg 3; RRS James Cook 057) between Tierra del Fuego and the Equator. Along the cruise track, along with the possibility of "boundary exchange", there are several additional potential sources that could add external Nd to seawater and disturb the "quasi-conservative" behavior of ɛNd. For example, it transects the continental shelf in the far south, the Rio Grande Rise, volcanic seamounts, and the major geological age boundaries of South America. It also crosses the major Southern Hemisphere wind zones, allowing us to test the impacts of eolian dust input, as well as inputs from major rivers. Our results on seawater ɛNd show strikingly that the Southwest Atlantic transect confirms "quasi-conservative" behavior of ɛNd in <span class="hlt">intermediate</span> and deep <span class="hlt">water</span>. Shallow depths show local impacts but these are not transferred to <span class="hlt">intermediate</span> and deep <span class="hlt">water</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5666255','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5666255"><span>Genetic signature of Last Glacial Maximum regional refugia in a circum-<span class="hlt">Antarctic</span> sea spider</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Soler-Membrives, Anna; Linse, Katrin; Miller, Karen J.</p> <p>2017-01-01</p> <p>The evolutionary history of <span class="hlt">Antarctic</span> organisms is becoming increasingly important to understand and manage population trajectories under rapid environmental change. The <span class="hlt">Antarctic</span> sea spider Nymphon australe, with an apparently large population size compared with other sea spider species, is an ideal target to look for molecular signatures of past climatic events. We analysed mitochondrial DNA of specimens collected from the <span class="hlt">Antarctic</span> continent and two <span class="hlt">Antarctic</span> islands (AI) to infer past population processes and understand current genetic structure. Demographic history analyses suggest populations survived in refugia during the Last Glacial Maximum. The high genetic diversity found in the <span class="hlt">Antarctic</span> Peninsula and East <span class="hlt">Antarctic</span> (EA) seems related to multiple demographic contraction–expansion events associated with deep-sea refugia, while the low genetic diversity in the Weddell Sea points to a more recent expansion from a shelf refugium. We suggest the genetic structure of N. australe from AI reflects recent colonization from the continent. At a local level, EA populations reveal generally low genetic differentiation, geographically and bathymetrically, suggesting limited restrictions to dispersal. Results highlight regional differences in demographic histories and how these relate to the variation in intensity of glaciation–deglaciation events around Antarctica, critical for the study of local evolutionary processes. These are valuable data for understanding the remarkable success of <span class="hlt">Antarctic</span> pycnogonids, and how environmental changes have shaped the evolution and diversification of Southern Ocean benthic biodiversity. PMID:29134072</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017RSOS....470615S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017RSOS....470615S"><span>Genetic signature of Last Glacial Maximum regional refugia in a circum-<span class="hlt">Antarctic</span> sea spider</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Soler-Membrives, Anna; Linse, Katrin; Miller, Karen J.; Arango, Claudia P.</p> <p>2017-10-01</p> <p>The evolutionary history of <span class="hlt">Antarctic</span> organisms is becoming increasingly important to understand and manage population trajectories under rapid environmental change. The <span class="hlt">Antarctic</span> sea spider Nymphon australe, with an apparently large population size compared with other sea spider species, is an ideal target to look for molecular signatures of past climatic events. We analysed mitochondrial DNA of specimens collected from the <span class="hlt">Antarctic</span> continent and two <span class="hlt">Antarctic</span> islands (AI) to infer past population processes and understand current genetic structure. Demographic history analyses suggest populations survived in refugia during the Last Glacial Maximum. The high genetic diversity found in the <span class="hlt">Antarctic</span> Peninsula and East <span class="hlt">Antarctic</span> (EA) seems related to multiple demographic contraction-expansion events associated with deep-sea refugia, while the low genetic diversity in the Weddell Sea points to a more recent expansion from a shelf refugium. We suggest the genetic structure of N. australe from AI reflects recent colonization from the continent. At a local level, EA populations reveal generally low genetic differentiation, geographically and bathymetrically, suggesting limited restrictions to dispersal. Results highlight regional differences in demographic histories and how these relate to the variation in intensity of glaciation-deglaciation events around Antarctica, critical for the study of local evolutionary processes. These are valuable data for understanding the remarkable success of <span class="hlt">Antarctic</span> pycnogonids, and how environmental changes have shaped the evolution and diversification of Southern Ocean benthic biodiversity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.T13B2699M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.T13B2699M"><span>The Presence and Characterization of <span class="hlt">Antarctic</span> Bottom <span class="hlt">Water</span> Located Between the Mid-Atlantic Ridge and the Rio Grande Rise</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Miller, R. H.; Reece, R.; Estep, J.; Christeson, G. L.; Acquisto, T. M.</p> <p>2016-12-01</p> <p>Circumpolar <span class="hlt">waters</span> of widely varying properties enter South Atlantic Ocean circulation, interleaving their properties. <span class="hlt">Antarctic</span> bottom <span class="hlt">water</span> (ABW) flows northward into the South Atlantic at the eastern edge of the South American continent and around the Rio Grande Rise (RGR), a large aseismic ocean ridge in the deep <span class="hlt">water</span> off the coast of Brazil. The majority of ABW transport occurs below depths of 3500 m, so very little is lost at the top of the RGR. In early 2016, the CREST (Crustal Reflectivity Experiment Southern Transect) expedition acquired multichannel seismic (MCS) and ocean bottom seismometer (OBS) datasets along a crustal segment in the South Atlantic, stretching from the Mid Atlantic Ridge (MAR) west to the RGR. During OBS recovery, a communications problem occurred in which the OBS received the transducer pulse from the ship, but the ship did not receive the OBS return pulse. The nine shallowest instruments, closest to the MAR, did not experience this problem, but all remaining instruments did. All instruments were extensively tested in the <span class="hlt">water</span> column and in the lab and exhibited no malfunctions. We hypothesize that a deepwater layer of differing physical properties, located nearer the OBS than the boat, dispersed the return pulse resulting in the break in communications. ABW is a good candidate for a potential cold deepwater body in this region. We will examine multi-beam bathymetry returns and seismic reflection data for indications of reflections in the deepwater column. If observations support the presence of cold deepwater, we will fully characterize its properties and boundaries and determine if the characteristics match that of ABW. This study will characterize the behavior and nature of potential cold deepwater currents east of the Rio Grande Rise in an attempt to verify the presence of ABW. Information regarding the effects of differential <span class="hlt">water</span> layering on acoustic communication with seafloor instruments could benefit future deployments to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1993JGR....9812997C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1993JGR....9812997C"><span>Synoptic aspects of <span class="hlt">Antarctic</span> mesocyclones</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carleton, Andrew M.; Fitch, Mark</p> <p>1993-07-01</p> <p>The characteristic regimes (formation and dissipation areas, tracks) and synoptic environments of cold air mesocyclones over <span class="hlt">Antarctic</span> and Subantarctic latitudes are determined for the contrasting winters (June, July, and August) of 1988 and 1989. Defense Meteorological Satellite Program (DMSP) thermal infrared (IR) imagery is used in conjunction with southern hemisphere pressure/height analyses. Outbreaks of mesocyclones ("active periods") are frequent in the Ross Sea sector in 1988. They are associated most often with areas of maximum horizontal gradient of the 1000- to 500-mbar thickness. Over higher latitudes of the Southeast Pacific in 1989, mesocyclones develop in association with a "cold pool" that migrates equatorward. The between-winter differences in mesocyclone frequencies are examined for associations with sea ice conditions and the continental katabatic winds using correlation and "superposed epoch" analysis of temperature data from selected automatic weather stations (AWSs). The results support a katabatic wind-sea ice extent-mesocyclone link for key sectors of the <span class="hlt">Antarctic</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.C24A..01N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.C24A..01N"><span>Arctic and <span class="hlt">Antarctic</span> Sea Ice Changes and Impacts (Invited)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nghiem, S. V.</p> <p>2013-12-01</p> <p>The extent of springtime Arctic perennial sea ice, important to preconditioning summer melt and to polar sunrise photochemistry, continues its precipitous reduction in the last decade marked by a record low in 2012, as the Bromine, Ozone, and Mercury Experiment (BROMEX) was conducted around Barrow, Alaska, to investigate impacts of sea ice reduction on photochemical processes, transport, and distribution in the polar environment. In spring 2013, there was further loss of perennial sea ice, as it was not observed in the ocean region adjacent to the Alaskan north coast, where there was a stretch of perennial sea ice in 2012 in the Beaufort Sea and Chukchi Sea. In contrast to the rapid and extensive loss of sea ice in the Arctic, <span class="hlt">Antarctic</span> sea ice has a trend of a slight increase in the past three decades. Given the significant variability in time and in space together with uncertainties in satellite observations, the increasing trend of <span class="hlt">Antarctic</span> sea ice may arguably be considered as having a low confidence level; however, there was no overall reduction of <span class="hlt">Antarctic</span> sea ice extent anywhere close to the decreasing rate of Arctic sea ice. There exist publications presenting various factors driving changes in Arctic and <span class="hlt">Antarctic</span> sea ice. After a short review of these published factors, new observations and atmospheric, oceanic, hydrological, and geological mechanisms contributed to different behaviors of sea ice changes in the Arctic and <span class="hlt">Antarctic</span> are presented. The contribution from of hydrologic factors may provide a linkage to and enhance thermal impacts from lower latitudes. While geological factors may affect the sensitivity of sea ice response to climate change, these factors can serve as the long-term memory in the system that should be exploited to improve future projections or predictions of sea ice changes. Furthermore, similarities and differences in chemical impacts of Arctic and <span class="hlt">Antarctic</span> sea ice changes are discussed. Understanding sea ice changes and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AsBio...7..275G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AsBio...7..275G"><span>Microbial Populations in <span class="hlt">Antarctic</span> Permafrost: Biodiversity, State, Age, and Implication for Astrobiology</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gilichinsky, D. A.; Wilson, G. S.; Friedmann, E. I.; McKay, C. P.; Sletten, R. S.; Rivkina, E. M.; Vishnivetskaya, T. A.; Erokhina, L. G.; Ivanushkina, N. E.; Kochkina, G. A.; Shcherbakova, V. A.; Soina, V. S.; Spirina, E. V.; Vorobyova, E. A.; Fyodorov-Davydov, D. G.; Hallet, B.; Ozerskaya, S. M.; Sorokovikov, V. A.; Laurinavichyus, K. S.; Shatilovich, A. V.; Chanton, J. P.; Ostroumov, V. E.; Tiedje, J. M.</p> <p>2007-05-01</p> <p><span class="hlt">Antarctic</span> permafrost soils have not received as much geocryological and biological study as has been devoted to the ice sheet, though the permafrost is more stable and older and inhabited by more microbes. This makes these soils potentially more informative and a more significant microbial repository than ice sheets. Due to the stability of the subsurface physicochemical regime, <span class="hlt">Antarctic</span> permafrost is not an extreme environment but a balanced natural one. Up to 104 viable cells/g, whose age presumably corresponds to the longevity of the permanently frozen state of the sediments, have been isolated from <span class="hlt">Antarctic</span> permafrost. Along with the microbes, metabolic by-products are preserved. This presumed natural cryopreservation makes it possible to observe what may be the oldest microbial communities on Earth. Here, we describe the <span class="hlt">Antarctic</span> permafrost habitat and biodiversity and provide a model for martian 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_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li class="active"><span>25</span></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_25 --> <div class="footer-extlink text-muted" style="margin-bottom:1rem; text-align:center;">Some links on this page may take you to non-federal websites. 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