Sample records for ice-covered antarctic lake

  1. Astrobiology of Antarctic ice Covered Lakes

    NASA Astrophysics Data System (ADS)

    Doran, P. T.; Fritsen, C. H.

    2005-12-01

    Antarctica contains a number of permanently ice-covered lakes which have often been used as analogs of purported lakes on Mars in the past. Antarctic subglacial lakes, such as Lake Vostok, have also been viewed as excellent analogs for an ice covered ocean on the Jovian moon Europa, and to a lesser extend on Mars. Lakes in the McMurdo Dry Valleys of East Antarctica have ice covers that range from 3 to 20 meters thick. Water salinities range from fresh to hypersaline. The thinner ice-covered lakes have a well-documented ecology that relies on the limited available nutrients and the small amount of light energy that penetrates the ice covers. The thickest ice-covered lake (Lake Vida in Victoria Valley) has a brine beneath 20 m of ice that is 7 times sea water and maintains a temperature below -10 degrees Celsius. This lake is vastly different from the thinner ice-covered lakes in that there is no communication with the atmosphere. The permanent ice cover is so thick, that summer melt waters can not access the sub-ice brine and so the ice grows from the top up, as well as from the bottom down. Brine trapped beneath the ice is believed to be ancient, stranded thousands of years ago when the ice grew thick enough to isolate it from the surface. We view Lake Vida as an excellent analog for the last aquatic ecosystem to have existed on Mars under a planetary cooling. If, as evidence is now increasingly supporting, standing bodies of water existed on Mars in the past, their fate under a cooling would be to go through a stage of permanent ice cover establishment, followed by a thickening of that ice cover until the final stage just prior to a cold extinction would be a Lake Vida-like lake. If dust storms or mass movements covered these ancient lakes, remnants may well be in existence in the subsurface today. A NASA Astrobiology Science and Technology for Exploring Planets (ASTEP) project will drill the Lake Vida ice cover and access the brine and sediments beneath in

  2. Antarctic lakes (above and beneath the ice sheet): Analogues for Mars

    NASA Technical Reports Server (NTRS)

    Rice, J. W., Jr.

    1992-01-01

    The perennial ice covered lakes of the Antarctic 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 water 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 Antarctic 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 Antarctic sub-ice lakes raises possibilities concerning Martian lakes and exobiology.

  3. Evidence of deep circulation in two perennially ice-covered Antarctic lakes

    USGS Publications Warehouse

    Tyler, S.W.; Cook, P.G.; Butt, A.Z.; Thomas, J.M.; Doran, P.T.; Lyons, W.B.

    1998-01-01

    The perennial ice covers found on many of the lakes in the McMurdo Dry Valley region of the Antarctic have been postulated to severely limit mixing and convective turnover of these unique lakes. In this work, we utilize chlorofluorocarbon (CFC) concentration profiles from Lakes Hoare and Fryxell in the McMurdo Dry Valley to determine the extent of deep vertical mixing occurring over the last 50 years. Near the ice-water interface, CFC concentrations in both lakes were well above saturation, in accordance with atmospheric gas supersaturations resulting from freezing under the perennial ice covers. Evidence of mixing throughout the water column at Lake Hoare was confirmed by the presence of CFCs throughout the water column and suggests vertical mixing times of 20-30 years. In Lake Fryxell, CFC-11, CFC-12, and CFC-113 were found in the upper water column; however, degradation of CFC-11 and CFC-12 in the anoxic bottom waters appears to be occurring with CFC-113 only present in these bottom waters. The presence of CFC-113 in the bottom waters, in conjunction with previous work detecting tritium in these waters, strongly argues for the presence of convective mixing in Lake Fryxell. The evidence for deep mixing in these lakes may be an important, yet overlooked, phenomenon in the limnology of perennially ice-covered lakes.

  4. Lipophilic pigments from the benthos of a perennially ice-covered Antarctic lake

    NASA Technical Reports Server (NTRS)

    Palmisano, A. C.; Wharton, R. A. Jr; Cronin, S. E.; Des Marais, D. J.; Wharton RA, J. r. (Principal Investigator)

    1989-01-01

    The benthos of a perennially ice-covered Antarctic lake, Lake Hoare, contained three distinct 'signatures' of lipophilic pigments. Cyanobacterial mats found in the moat at the periphery of the lake were dominated by the carotenoid myxoxanthophyll; carotenoids: chlorophyll a ratios in this high light environment ranged from 3 to 6.8. Chlorophyll c and fucoxanthin, pigments typical of golden-brown algae, were found at 10 to 20 m depths where the benthos is aerobic. Anaerobic benthic sediments at 20 to 30 m depths were characterized by a third pigment signature dominated by a carotenoid, tentatively identified as alloxanthin from planktonic cryptomonads, and by phaeophytin b from senescent green algae. Pigments were not found associated with alternating organic and sediment layers. As microzooplankton grazers are absent from this closed system and transformation rates are reduced at low temperatures, the benthos beneath the lake ice appears to contain a record of past phytoplankton blooms undergoing decay.

  5. Perennial Antarctic lake ice: an oasis for life in a polar desert

    NASA Technical Reports Server (NTRS)

    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.

    1998-01-01

    The permanent ice covers of Antarctic lakes in the McMurdo Dry Valleys develop liquid water 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.

  6. Perennial Antarctic lake ice: an oasis for life in a polar desert.

    PubMed

    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

    1998-06-26

    The permanent ice covers of Antarctic lakes in the McMurdo Dry Valleys develop liquid water 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.

  7. Potential subglacial lake locations and meltwater drainage pathways beneath the Antarctic and Greenland ice sheets

    NASA Astrophysics Data System (ADS)

    Livingstone, S. J.; Clark, C. D.; Woodward, J.; Kingslake, J.

    2013-11-01

    We use the Shreve hydraulic potential equation as a simplified approach to investigate potential subglacial lake locations and meltwater drainage pathways beneath the Antarctic and Greenland ice sheets. We validate the method by demonstrating its ability to recall the locations of >60% of the known subglacial lakes beneath the Antarctic Ice Sheet. This is despite uncertainty in the ice-sheet bed elevation and our simplified modelling approach. However, we predict many more lakes than are observed. Hence we suggest that thousands of subglacial lakes remain to be found. Applying our technique to the Greenland Ice Sheet, where very few subglacial lakes have so far been observed, recalls 1607 potential lake locations, covering 1.2% of the bed. Our results will therefore provide suitable targets for geophysical surveys aimed at identifying lakes beneath Greenland. We also apply the technique to modelled past ice-sheet configurations and find that during deglaciation both ice sheets likely had more subglacial lakes at their beds. These lakes, inherited from past ice-sheet configurations, would not form under current surface conditions, but are able to persist, suggesting a retreating ice-sheet will have many more subglacial lakes than advancing ones. We also investigate subglacial drainage pathways of the present-day and former Greenland and Antarctic ice sheets. Key sectors of the ice sheets, such as the Siple Coast (Antarctica) and NE Greenland Ice Stream system, are suggested to have been susceptible to subglacial drainage switching. We discuss how our results impact our understanding of meltwater drainage, basal lubrication and ice-stream formation.

  8. Viruses in Antarctic lakes

    NASA Technical Reports Server (NTRS)

    Kepner, R. L. Jr; Wharton, R. A. Jr; Suttle, C. A.; Wharton RA, J. r. (Principal Investigator)

    1998-01-01

    Water samples collected from four perennially ice-covered Antarctic 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 Antarctic lakes may be a reservoir of previously undescribed viruses that possess novel biological and biochemical characteristics.

  9. Plankton assembly in an ultra-oligotrophic Antarctic lake over the summer transition from the ice-cover to ice-free period: A size spectra approach

    NASA Astrophysics Data System (ADS)

    Rochera, Carlos; Quesada, Antonio; Toro, Manuel; Rico, Eugenio; Camacho, Antonio

    2017-03-01

    Lakes from the Antarctic maritime region experience climate change as a main stressor capable of modifying their plankton community structure and function, essentially because summer temperatures are commonly over the freezing point and the lake's ice cap thaws. This study was conducted in such seasonally ice-covered lake (Lake Limnopolar, Byers Peninsula, Livingston Is., Antarctica), which exhibits a microbial dominated pelagic food web. An important feature is also the occurrence of benthic mosses (Drepanocladus longifolius) covering the lake bottom. Plankton dynamics were investigated during the ice-thawing transition to the summer maximum. Both bacterioplankton and viral-like particles were higher near the lake's bottom, suggesting a benthic support. When the lake was under dim conditions because of the snow-and-ice cover, autotrophic picoplankters dominated at deep layers. The taxa-specific photopigments indicated dominance of picocyanobacteria among them when the light availability was lower. By contrast, larger and less edible phytoplankton dominated at the onset of the ice melting. The plankton size spectra were fitted to the continuous model of Pareto distribution. Spectra evolved similarly at two sampled depths, in surface and near the bottom, with slopes increasing until mid-January. However, slopes were less steep (i.e., size classes more uniformly distributed) at the bottom, thus denoting a more efficient utilization of resources. These findings suggest that microbial loop pathways in the lake are efficiently channelized during some periods to the metazoan production (mainly the copepod Boeckella poppei). Our results point to that trophic interactions may still occur in these lakes despite environmental harshness. This results of interest in a framework of increasing temperatures that may reduce the climatic restrictions and therefore stimulate biotic interactions.

  10. Identity, ecology and ecophysiology of planktic green algae dominating in ice-covered lakes on James Ross Island (northeastern Antarctic Peninsula).

    PubMed

    Nedbalová, Linda; Mihál, Martin; Kvíderová, Jana; Procházková, Lenka; Řezanka, Tomáš; Elster, Josef

    2017-01-01

    The aim of this study was to assess the phylogenetic relationships, ecology and ecophysiological characteristics of the dominant planktic algae in ice-covered lakes on James Ross Island (northeastern Antarctic Peninsula). Phylogenetic analyses of 18S rDNA together with analysis of ITS2 rDNA secondary structure and cell morphology revealed that the two strains belong to one species of the genus Monoraphidium (Chlorophyta, Sphaeropleales, Selenastraceae) that should be described as new in future. Immotile green algae are thus apparently capable to become the dominant primary producer in the extreme environment of Antarctic lakes with extensive ice-cover. The strains grew in a wide temperature range, but the growth was inhibited at temperatures above 20 °C, indicating their adaptation to low temperature. Preferences for low irradiances reflected the light conditions in their original habitat. Together with relatively high growth rates (0.4-0.5 day -1 ) and unprecedently high content of polyunsaturated fatty acids (PUFA, more than 70% of total fatty acids), it makes these isolates interesting candidates for biotechnological applications.

  11. Ice-Covered Lakes in Gale Crater Mars: The Cold and Wet Hypothesis

    NASA Technical Reports Server (NTRS)

    Kling, A. M.; Haberle, R. M.; Mckay, C. P.; Bristow, T. F.

    2016-01-01

    Recent geological discoveries from the Mars Science Laboratory provide evidence that Gale crater may have intermittently hosted a fluvio-lacustine environment during the Hesperian, with individual lakes lasting for a period of tens to hundreds of thousands of years. (Grotzinger et al., Science, 350 (6257), 2015). Estimates of the CO2 content of the atmosphere at the time the Gale sediments formed are far less than needed by any climate model to warm early Mars (Bristow et al., Geology, submitted), given the low solar energy input available at Mars 3.5 Gya. We have therefore explored the possibility that the lakes in Gale during the Hesperian were perennially covered with ice using the Antarctic Lakes as an analog. Using our best estimate for the annual mean surface temperature at Gale at this time (approx. 230K) we computed the thickness of an ice-covered lake. These thickness range from 10-30 meters depending on the ablation rate and ice transparency and would likely inhibit sediments from entering the lake. Thus, a first conclusion is that the ice must not be too cold. Raising the mean temperature to 245K is challenging, but not quite as hard as reaching 273K. We found that a mean annual temperature of 245K ice thicknesses range from 3-10 meters. These values are comparable to the range of those for the Antarctic lakes (3-6 m), and are not implausible. And they are not so thick that sediments cannot penetrate the ice. For the ice-covered lake hypothesis to work, however, a melt water source is needed. This could come from subaqueous melting of a glacial dam in contact with the lakes (as is the case for Lake Untersee) or from seasonal melt water from nearby glaciers (as is the case for the Dry Valley lakes). More work is needed to better assess these possibilities. However, the main advantage of the ice-covered lake model (and the main reason we pursued it) is that it relaxes the requirement for a long-lived active hydrological cycle involving rainfall and runoff

  12. Sediment oxygen profiles in a super-oxygenated antarctic lake

    NASA Technical Reports Server (NTRS)

    Wharton, R. A. Jr; Meyer, M. A.; McKay, C. P.; Mancinelli, R. L.; Simmons, G. M. Jr; Wharton RA, J. r. (Principal Investigator)

    1994-01-01

    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, antarctic (and arctic) lakes have a yearly photic period. An unusual feature of the antarctic lakes is the occurrence of O2 at supersaturated levels in certain portions of the water column. Here we report the first sediment O2 profiles obtained using a microelectrode from a perennially ice-covered antarctic 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-water 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 water column.

  13. Protist diversity in a permanently ice-covered Antarctic lake during the polar night transition.

    PubMed

    Bielewicz, Scott; Bell, Elanor; Kong, Weidong; Friedberg, Iddo; Priscu, John C; Morgan-Kiss, Rachael M

    2011-09-01

    The McMurdo Dry Valleys of Antarctica harbor numerous permanently ice-covered lakes, which provide a year-round oasis for microbial life. Microbial eukaryotes in these lakes occupy a variety of trophic levels within the simple aquatic food web ranging from primary producers to tertiary predators. Here, we report the first molecular study to describe the vertical distribution of the eukaryotic community residing in the photic zone of the east lobe (ELB) and west lobe (WLB) of the chemically stratified Lake Bonney. The 18S ribosomal RNA (rRNA) libraries revealed vertically stratified populations dominated by photosynthetic protists, with a cryptophyte dominating shallow populations (ELB-6 m; WLB-10 m), a haptophyte occupying mid-depths (both lobes 13 m) and chlorophytes residing in the deepest layers (ELB-18 and 20 m; WLB-15 and 20 m) of the photic zone. A previously undetected stramenopile occurred throughout the water column of both lobes. Temporal variation in the eukaryotic populations was examined during the transition from Antarctic summer (24-h sunlight) to polar night (complete dark). Protist diversity was similar between the two lobes of Lake Bonney due to exchange between the photic zones of the two basins via a narrow bedrock sill. However, vertical and temporal variation in protist distribution occurred, indicating the influence of the unique water chemistry on the biology of the two dry valley watersheds.

  14. Ultrastructural and Single-Cell-Level Characterization Reveals Metabolic Versatility in a Microbial Eukaryote Community from an Ice-Covered Antarctic Lake

    PubMed Central

    Li, Wei; Podar, Mircea

    2016-01-01

    ABSTRACT The McMurdo Dry Valleys (MCM) of southern Victoria Land, Antarctica, harbor numerous ice-covered bodies of water that provide year-round liquid water oases for isolated food webs dominated by the microbial loop. Single-cell microbial eukaryotes (protists) occupy major trophic positions within this truncated food web, ranging from primary producers (e.g., chlorophytes, haptophytes, and cryptophytes) to tertiary predators (e.g., ciliates, dinoflagellates, and choanoflagellates). To advance the understanding of MCM protist ecology and the roles of MCM protists in nutrient and energy cycling, we investigated potential metabolic strategies and microbial interactions of key MCM protists isolated from a well-described lake (Lake Bonney). Fluorescence-activated cell sorting (FACS) of enrichment cultures, combined with single amplified genome/amplicon sequencing and fluorescence microscopy, revealed that MCM protists possess diverse potential metabolic capabilities and interactions. Two metabolically distinct bacterial clades (Flavobacteria and Methylobacteriaceae) were independently associated with two key MCM lake microalgae (Isochrysis and Chlamydomonas, respectively). We also report on the discovery of two heterotrophic nanoflagellates belonging to the Stramenopila supergroup, one of which lives as a parasite of Chlamydomonas, a dominate primary producer in the shallow, nutrient-poor layers of the lake. IMPORTANCE Single-cell eukaryotes called protists play critical roles in the cycling of organic matter in aquatic environments. In the ice-covered lakes of Antarctica, protists play key roles in the aquatic food web, providing the majority of organic carbon to the rest of the food web (photosynthetic protists) and acting as the major consumers at the top of the food web (predatory protists). In this study, we utilized a combination of techniques (microscopy, cell sorting, and genomic analysis) to describe the trophic abilities of Antarctic lake protists and

  15. Ultrastructural and Single-Cell-Level Characterization Reveals Metabolic Versatility in a Microbial Eukaryote Community from an Ice-Covered Antarctic Lake.

    PubMed

    Li, Wei; Podar, Mircea; Morgan-Kiss, Rachael M

    2016-06-15

    The McMurdo Dry Valleys (MCM) of southern Victoria Land, Antarctica, harbor numerous ice-covered bodies of water that provide year-round liquid water oases for isolated food webs dominated by the microbial loop. Single-cell microbial eukaryotes (protists) occupy major trophic positions within this truncated food web, ranging from primary producers (e.g., chlorophytes, haptophytes, and cryptophytes) to tertiary predators (e.g., ciliates, dinoflagellates, and choanoflagellates). To advance the understanding of MCM protist ecology and the roles of MCM protists in nutrient and energy cycling, we investigated potential metabolic strategies and microbial interactions of key MCM protists isolated from a well-described lake (Lake Bonney). Fluorescence-activated cell sorting (FACS) of enrichment cultures, combined with single amplified genome/amplicon sequencing and fluorescence microscopy, revealed that MCM protists possess diverse potential metabolic capabilities and interactions. Two metabolically distinct bacterial clades (Flavobacteria and Methylobacteriaceae) were independently associated with two key MCM lake microalgae (Isochrysis and Chlamydomonas, respectively). We also report on the discovery of two heterotrophic nanoflagellates belonging to the Stramenopila supergroup, one of which lives as a parasite of Chlamydomonas, a dominate primary producer in the shallow, nutrient-poor layers of the lake. Single-cell eukaryotes called protists play critical roles in the cycling of organic matter in aquatic environments. In the ice-covered lakes of Antarctica, protists play key roles in the aquatic food web, providing the majority of organic carbon to the rest of the food web (photosynthetic protists) and acting as the major consumers at the top of the food web (predatory protists). In this study, we utilized a combination of techniques (microscopy, cell sorting, and genomic analysis) to describe the trophic abilities of Antarctic lake protists and their potential

  16. Ultrastructural and Single-Cell-Level Characterization Reveals Metabolic Versatility in a Microbial Eukaryote Community from an Ice-Covered Antarctic Lake

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

    Li, Wei; Podar, Mircea; Morgan-Kiss, Rachael M.

    The McMurdo Dry Valleys (MCM) of southern Victoria Land, Antarctica, harbor numerous ice-covered bodies of water that provide year-round liquid water oases for isolated food webs dominated by the microbial loop. Single-cell microbial eukaryotes (protists) occupy major trophic positions within this truncated food web, ranging from primary producers (e.g., chlorophytes, haptophytes, and cryptophytes) to tertiary predators (e.g., ciliates, dinoflagellates, and choanoflagellates). To advance the understanding of MCM protist ecology and the roles of MCM protists in nutrient and energy cycling, we investigated potential metabolic strategies and microbial interactions of key MCM protists isolated from a well-described lake (Lake Bonney). Fluorescence-activatedmore » cell sorting (FACS) of enrichment cultures, combined with single amplified genome/amplicon sequencing and fluorescence microscopy, revealed that MCM protists possess diverse potential metabolic capabilities and interactions. Two metabolically distinct bacterial clades (FlavobacteriaandMethylobacteriaceae) were independently associated with two key MCM lake microalgae (IsochrysisandChlamydomonas, respectively). We also report on the discovery of two heterotrophic nanoflagellates belonging to the Stramenopila supergroup, one of which lives as a parasite ofChlamydomonas, a dominate primary producer in the shallow, nutrient-poor layers of the lake. Single-cell eukaryotes called protists play critical roles in the cycling of organic matter in aquatic environments. In the ice-covered lakes of Antarctica, protists play key roles in the aquatic food web, providing the majority of organic carbon to the rest of the food web (photosynthetic protists) and acting as the major consumers at the top of the food web (predatory protists). In this study, we utilized a combination of techniques (microscopy, cell sorting, and genomic analysis) to describe the trophic abilities of Antarctic lake protists and their potential

  17. Ultrastructural and Single-Cell-Level Characterization Reveals Metabolic Versatility in a Microbial Eukaryote Community from an Ice-Covered Antarctic Lake

    DOE PAGES

    Li, Wei; Podar, Mircea; Morgan-Kiss, Rachael M.

    2016-04-15

    The McMurdo Dry Valleys (MCM) of southern Victoria Land, Antarctica, harbor numerous ice-covered bodies of water that provide year-round liquid water oases for isolated food webs dominated by the microbial loop. Single-cell microbial eukaryotes (protists) occupy major trophic positions within this truncated food web, ranging from primary producers (e.g., chlorophytes, haptophytes, and cryptophytes) to tertiary predators (e.g., ciliates, dinoflagellates, and choanoflagellates). To advance the understanding of MCM protist ecology and the roles of MCM protists in nutrient and energy cycling, we investigated potential metabolic strategies and microbial interactions of key MCM protists isolated from a well-described lake (Lake Bonney). Fluorescence-activatedmore » cell sorting (FACS) of enrichment cultures, combined with single amplified genome/amplicon sequencing and fluorescence microscopy, revealed that MCM protists possess diverse potential metabolic capabilities and interactions. Two metabolically distinct bacterial clades (FlavobacteriaandMethylobacteriaceae) were independently associated with two key MCM lake microalgae (IsochrysisandChlamydomonas, respectively). We also report on the discovery of two heterotrophic nanoflagellates belonging to the Stramenopila supergroup, one of which lives as a parasite ofChlamydomonas, a dominate primary producer in the shallow, nutrient-poor layers of the lake. Single-cell eukaryotes called protists play critical roles in the cycling of organic matter in aquatic environments. In the ice-covered lakes of Antarctica, protists play key roles in the aquatic food web, providing the majority of organic carbon to the rest of the food web (photosynthetic protists) and acting as the major consumers at the top of the food web (predatory protists). In this study, we utilized a combination of techniques (microscopy, cell sorting, and genomic analysis) to describe the trophic abilities of Antarctic lake protists and their potential

  18. Formation and character of an ancient 19-m ice cover and underlying trapped brine in an "ice-sealed" east Antarctic lake.

    PubMed

    Doran, Peter T; Fritsen, Christian H; McKay, Christopher P; Priscu, John C; Adams, Edward E

    2003-01-07

    Lake Vida, one of the largest lakes in the McMurdo Dry Valleys of Antarctica, was previously believed to be shallow (<10 m) and frozen to its bed year-round. New ice-core analysis and temperature data show that beneath 19 m of ice is a water column composed of a NaCl brine with a salinity seven times that of seawater that remains liquid below -10 degrees C. The ice cover thickens at both its base and surface, sealing concentrated brine beneath. The ice cover is stabilized by a negative feedback between ice growth and the freezing-point depression of the brine. The ice cover contains frozen microbial mats throughout that are viable after thawing and has a history that extends to at least 2,800 (14)C years B.P., suggesting that the brine has been isolated from the atmosphere for as long. To our knowledge, Lake Vida has the thickest subaerial lake ice cover recorded and may represent a previously undiscovered end-member lacustrine ecosystem on Earth.

  19. Advances in modelling subglacial lakes and their interaction with the Antarctic ice sheet.

    PubMed

    Pattyn, Frank; Carter, Sasha P; Thoma, Malte

    2016-01-28

    Subglacial lakes have long been considered hydraulically isolated water bodies underneath ice sheets. This view changed radically with the advent of repeat-pass satellite altimetry and the discovery of multiple lake discharges and water infill, associated with water 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 Antarctic ice sheet is more widespread than previously thought, and subglacial melt rates may explain the availability for water storage in subglacial lakes and water transport. Modelling of subglacial water 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 water exchanges between till and ice. Most active lakes drain over short time scales and respond rapidly to upstream variations. Several Antarctic subglacial lakes exhibit complex interactions with the ice sheet due to water 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).

  20. Laser-induced fluorescence emission (L.I.F.E.): in situ nondestructive detection of microbial life in the ice covers of Antarctic lakes.

    PubMed

    Storrie-Lombardi, Michael C; Sattler, Birgit

    2009-09-01

    Laser-induced fluorescence emission (L.I.F.E.) images were obtained in situ following 532 nm excitation of cryoconite assemblages in the ice covers of annual and perennially frozen Antarctic lakes during the 2008 Tawani International Expedition to Schirmacher Oasis and Lake Untersee in Dronning Maud Land, Antarctica. Laser targeting of a single millimeter-scale cryoconite results in multiple neighboring excitation events secondary to ice/air interface reflection and refraction in the bubbles surrounding the primary target. Laser excitation at 532 nm of cyanobacteria-dominated assemblages produced red and infrared autofluorescence activity attributed to the presence of phycoerythrin photosynthetic pigments. The method avoids destruction of individual target organisms and does not require the disruption of either the structure of the microbial community or the surrounding ice matrix. L.I.F.E. survey strategies described may be of interest for orbital monitoring of photosynthetic primary productivity in polar and alpine glaciers, ice sheets, snow, and lake ice of Earth's cryosphere. The findings open up the possibility of searching from either a rover or from orbit for signs of life in the polar regions of Mars and the frozen regions of exoplanets in neighboring star systems.

  1. Sensitivity of Great Lakes Ice Cover to Air Temperature

    NASA Astrophysics Data System (ADS)

    Austin, J. A.; Titze, D.

    2016-12-01

    Ice cover is shown to exhibit a strong linear sensitivity to air temperature. Upwards of 70% of ice cover variability on all of the Great Lakes can be explained in terms of air temperature, alone, and nearly 90% of ice cover variability can be explained in some lakes. Ice cover sensitivity to air temperature is high, and a difference in seasonally-averaged (Dec-May) air temperature on the order of 1°C to 2°C can be the difference between a low-ice year and a moderate- to high- ice year. The total amount of seasonal ice cover is most influenced by air temperatures during the meteorological winter, contemporaneous with the time of ice formation. Air temperature conditions during the pre-winter conditioning period and during the spring melting period were found to have less of an impact on seasonal ice cover. This is likely due to the fact that there is a negative feedback mechanism when heat loss goes toward cooling the lake, but a positive feedback mechanism when heat loss goes toward ice formation. Ice cover sensitivity relationships were compared between shallow coastal regions of the Great Lakes and similarly shallow smaller, inland lakes. It was found that the sensitivity to air temperature is similar between these coastal regions and smaller lakes, but that the absolute amount of ice that forms varies significantly between small lakes and the Great Lakes, and amongst the Great Lakes themselves. The Lake Superior application of the ROMS three-dimensional hydrodynamic numerical model verifies a deterministic linear relationship between air temperature and ice cover, which is also strongest around the period of ice formation. When the Lake Superior bathymetry is experimentally adjusted by a constant vertical multiplier, average lake depth is shown to have a nonlinear relationship with seasonal ice cover, and this nonlinearity may be associated with a nonlinear increase in the lake-wide volume of the surface mixed layer.

  2. Formation and character of an ancient 19-m ice cover and underlying trapped brine in an “ice-sealed” east Antarctic lake

    PubMed Central

    Doran, Peter T.; Fritsen, Christian H.; McKay, Christopher P.; Priscu, John C.; Adams, Edward E.

    2003-01-01

    Lake Vida, one of the largest lakes in the McMurdo Dry Valleys of Antarctica, was previously believed to be shallow (<10 m) and frozen to its bed year-round. New ice-core analysis and temperature data show that beneath 19 m of ice is a water column composed of a NaCl brine with a salinity seven times that of seawater that remains liquid below −10°C. The ice cover thickens at both its base and surface, sealing concentrated brine beneath. The ice cover is stabilized by a negative feedback between ice growth and the freezing-point depression of the brine. The ice cover contains frozen microbial mats throughout that are viable after thawing and has a history that extends to at least 2,800 14C years B.P., suggesting that the brine has been isolated from the atmosphere for as long. To our knowledge, Lake Vida has the thickest subaerial lake ice cover recorded and may represent a previously undiscovered end-member lacustrine ecosystem on Earth. PMID:12518052

  3. Environmentally Non-Disturbing Under-ice Robotic ANtarctiC Explorer (ENDURANCE)

    NASA Astrophysics Data System (ADS)

    Doran, P. T.; Stone, W.; Priscu, J.; McKay, C.; Johnson, A.; Chen, B.

    2007-12-01

    Permanently ice-covered liquid water 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 Antarctic dry valley lakes. The ENDURANCE (Environmentally Non-Disturbing Under-ice Robotic ANtarctic 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 water column, as well as Raman Spectrometry of the water 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 Antarctic environmental protocols, but will also be useful for planetary protection and improved science in the future. We will carry out two Antarctic 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.

  4. Evidence of form II RubisCO (cbbM) in a perennially ice-covered Antarctic lake.

    PubMed

    Kong, Weidong; Dolhi, Jenna M; Chiuchiolo, Amy; Priscu, John; Morgan-Kiss, Rachael M

    2012-11-01

    The permanently ice-covered lakes of the McMurdo Dry Valleys, Antarctica, harbor microbially dominated food webs. These organisms are adapted to a variety of unusual environmental extremes, including low temperature, low light, and permanently stratified water columns with strong chemo- and oxy-clines. Owing to the low light levels during summer caused by thick ice cover as well as 6 months of darkness during the polar winter, chemolithoautotrophic microorganisms could play a key role in the production of new carbon for the lake ecosystems. We used clone library sequencing and real-time quantitative PCR of the gene encoding form II Ribulose 1, 5-bisphosphate carboxylase/oxygenase to determine spatial and seasonal changes in the chemolithoautotrophic community in Lake Bonney, a 40-m-deep lake covered by c. 4 m of permanent ice. Our results revealed that chemolithoautotrophs harboring the cbbM gene are restricted to layers just above the chemo- and oxi-cline (≤ 15 m) in the west lobe of Lake Bonney (WLB). Our data reveal that the WLB is inhabited by a unique chemolithoautotrophic community that resides in the suboxic layers of the lake where there are ample sources of alternative electron sources such as ammonium, reduced iron and reduced biogenic sulfur species. © 2012 Federation of European Microbiological Societies. Published by Blackwell Publishing Ltd. All rights reserved.

  5. Biogeochemistry and limnology in Antarctic subglacial weathering: molecular evidence of the linkage between subglacial silica input and primary producers in a perennially ice-covered lake

    NASA Astrophysics Data System (ADS)

    Takano, Yoshinori; Kojima, Hisaya; Takeda, Eriko; Yokoyama, Yusuke; Fukui, Manabu

    2015-12-01

    We report a 6,000 years record of subglacial weathering and biogeochemical processes in two perennially ice-covered glacial lakes at Rundvågshetta, on the Soya Coast of Lützow-Holm Bay, East Antarctica. The two lakes, Lake Maruwan Oike and Lake Maruwan-minami, are located in a channel that drains subglacial water from the base of the East Antarctic ice sheet. Greenish-grayish organic-rich laminations in sediment cores from the lakes indicate continuous primary production affected by the inflow of subglacial meltwater containing relict carbon, nitrogen, sulfur, and other essential nutrients. Biogenic silica, amorphous hydrated silica, and DNA-based molecular signatures of sedimentary facies indicate that diatom assemblages are the dominant primary producers, supported by the input of inorganic silicon (Si) from the subglacial inflow. This study highlights the significance of subglacial water-rock interactions during physical and chemical weathering processes and the importance of such interactions for the supply of bioavailable nutrients.

  6. Regional Changes in the Sea Ice Cover and Ice Production in the Antarctic

    NASA Technical Reports Server (NTRS)

    Comiso, Josefino C.

    2011-01-01

    Coastal polynyas around the Antarctic continent have been regarded as sea ice factories because of high ice production rates in these regions. The observation of a positive trend in the extent of Antarctic sea ice during the satellite era has been intriguing in light of the observed rapid decline of the ice extent in the Arctic. The results of analysis of the time series of passive microwave data indicate large regional variability with the trends being strongly positive in the Ross Sea, strongly negative in the Bellingshausen/Amundsen Seas and close to zero in the other regions. The atmospheric circulation in the Antarctic is controlled mainly by the Southern Annular Mode (SAM) and the marginal ice zone around the continent shows an alternating pattern of advance and retreat suggesting the presence of a propagating wave (called Antarctic Circumpolar Wave) around the circumpolar region. The results of analysis of the passive microwave data suggest that the positive trend in the Antarctic sea ice cover could be caused primarily by enhanced ice production in the Ross Sea that may be associated with more persistent and larger coastal polynyas in the region. Over the Ross Sea shelf, analysis of sea ice drift data from 1992 to 2008 yields a positive rate-of-increase in the net ice export of about 30,000 km2 per year. For a characteristic ice thickness of 0.6 m, this yields a volume transport of about 20 km3/year, which is almost identical, within error bars, to our estimate of the trend in ice production. In addition to the possibility of changes in SAM, modeling studies have also indicated that the ozone hole may have a role in that it causes the deepening of the lows in the western Antarctic region thereby causing strong winds to occur offthe Ross-ice shelf.

  7. Biological Diversity Comprising Microbial Structures of Antarctic Ice Covered Lakes

    NASA Astrophysics Data System (ADS)

    Matys, E. D.

    2015-12-01

    Analysis of microbial membrane lipids is a rapid and non-selective method for evaluating the composition of microbial communities. To fully realise the diagnostic potential of these lipids, we must first understand their structural diversity, biological sources, physiological functions, and pathways of preservation. Particular environmental conditions likely prompt the production of different membrane lipid structures. Antarctica's McMurdo Dry Valleys host numerous ice-covered lakes with sharp chemical gradients that vary in illumination, geochemical structure, and benthic mat morphologies that are structured by nutrient availability and water chemistry. The lipid contents of these benthic mats have not received extensive study nor have the communities yet been thoroughly characterized. Accordingly, a combination of lipid biomarker and nucleic acid sequence data provides the means of assessing species diversity and environmental controls on the composition and diversity of membrane lipid assemblages. We investigated the richness and diversity of benthic microbial communities and accumulated organic matter in Lake Vanda of the McMurdo Dry Valleys. We have identified diverse glycolipids, aminolipids, and phospholipids in addition to many unknown compounds that may be specific to these particular environments. Light levels fluctuate seasonally, favoring low-light-tolerant cyanobacteria and specific lipid assemblages. Adaptations to nutrient limitations are reflected in contrasting intact polar lipid assemblages. For example, under P-limiting conditions, phospholipids are subsidiary to membrane-forming lipids that do not contain P (i.e. ornithine, betaine, and sulfolipids). The bacteriohopanepolyol (BHP) composition is dominated by bacteriohopanetetrol (BHT), a ubiquitous BHP, and 2-methylhopanoids. The relative abundance of 2-methylhopanoids is unprecedented and may reflect the unusual seasonal light regime of this polar environment. By establishing correlations

  8. Were lakes on early Mars perennially were ice-covered?

    NASA Astrophysics Data System (ADS)

    Sumner, D. Y.; Rivera-Hernandez, F.; Mackey, T. J.

    2016-12-01

    Paleo-lake deposits indicate that Mars once sustained liquid water, supporting the idea of an early "wet and warm" Mars. However, liquid water can be sustained under ice in cold conditions as demonstrated by perennially ice-covered lakes (PICLs) in Antarctica. If martian lakes were ice-covered, the global climate on early Mars could have been much colder and dryer than if the atmosphere was in equilibrium with long-lived open water lakes. Modern PICLs on Earth have diagnostic sedimentary features. Unlike open water lakes that are dominated by mud, and drop stones or tills if icebergs are present, previous studies determined that deposits in PICLs can include coarser grains that are transported onto the ice cover, where they absorb solar radiation, melt through the ice and are deposited with lacustrine muds. In Lake Hoare, Antarctica, these coarse grains form conical sand mounds and ridges. Our observations of ice-covered lakes Joyce, Fryxell, Vanda and Hoare, Antarctica suggest that the distributions of grains depend significantly on ice characteristics. Deposits in these lakes contain moderately well to moderately sorted medium to very coarse sand grains, which preferentially melt through the ice whereas granules and larger grains remain on the ice surface. Similarly, high albedo grains are concentrated on the ice surface, whereas low albedo grains melt deeper into the ice, demonstrating a segregation of grains due to ice-sediment interactions. In addition, ice cover thickness may determine the spatial distribution of sand deposited in PICLs. Localized sand mounds and ridges composed of moderately sorted sand are common in PICLs with rough ice covers greater than 3 m thick. In contrast, lakes with smooth and thinner ice have disseminated sand grains and laterally extensive sand layers but may not have sand mounds. At Gale Crater, Mars, the Murray formation consists of sandy lacustrine mudstones, but the depositional process for the sand is unknown. The presence of

  9. Modular community structure suggests metabolic plasticity during the transition to polar night in ice-covered Antarctic lakes.

    PubMed

    Vick-Majors, Trista J; Priscu, John C; Amaral-Zettler, Linda A

    2014-04-01

    High-latitude environments, such as the Antarctic McMurdo Dry Valley lakes, are subject to seasonally segregated light-dark cycles, which have important consequences for microbial diversity and function on an annual basis. Owing largely to the logistical difficulties of sampling polar environments during the darkness of winter, little is known about planktonic microbial community responses to the cessation of photosynthetic primary production during the austral sunset, which lingers from approximately February to April. Here, we hypothesized that changes in bacterial, archaeal and eukaryotic community structure, particularly shifts in favor of chemolithotrophs and mixotrophs, would manifest during the transition to polar night. Our work represents the first concurrent molecular characterization, using 454 pyrosequencing of hypervariable regions of the small-subunit ribosomal RNA gene, of bacterial, archaeal and eukaryotic communities in permanently ice-covered lakes Fryxell and Bonney, before and during the polar night transition. We found vertically stratified populations that varied at the community and/or operational taxonomic unit-level between lakes and seasons. Network analysis based on operational taxonomic unit level interactions revealed nonrandomly structured microbial communities organized into modules (groups of taxa) containing key metabolic potential capacities, including photoheterotrophy, mixotrophy and chemolithotrophy, which are likely to be differentially favored during the transition to polar night.

  10. Microbiota within the perennial ice cover of Lake Vida, Antarctica.

    PubMed

    Mosier, Annika C; Murray, Alison E; Fritsen, Christian H

    2007-02-01

    Lake Vida, located in the McMurdo Dry Valleys, Antarctica, is an 'ice-sealed' lake with approximately 19 m of ice covering a highly saline water column (approximately 245 ppt). The lower portions of the ice cover and the lake beneath have been isolated from the atmosphere and land for circa 2800 years. Analysis of microbial assemblages within the perennial ice cover of the lake revealed a diverse array of bacteria and eukarya. Bacterial and eukaryal denaturing gradient gel electrophoresis phylotype profile similarities were low (<59%) between all of the depths compared (five depths spanning 11 m of the ice cover), with the greatest differences occurring between surface and deep ice. The majority of bacterial 16S rRNA gene sequences in the surface ice were related to Actinobacteria (42%) while Gammaproteobacteria (52%) dominated the deep ice community. Comparisons of assemblage composition suggest differences in ice habitability and organismal origin in the upper and lower portions of ice cover. Specifically, the upper ice cover microbiota likely reflect the modern day transport and colonization of biota from the terrestrial landscape, whereas assemblages in the deeper ice are more likely to be persistent remnant biota that originated from the ancient liquid water column of the lake that froze.

  11. Niche specialization of bacteria in permanently ice-covered lakes of the McMurdo Dry Valleys, Antarctica.

    PubMed

    Kwon, Miye; Kim, Mincheol; Takacs-Vesbach, Cristina; Lee, Jaejin; Hong, Soon Gyu; Kim, Sang Jong; Priscu, John C; Kim, Ok-Sun

    2017-06-01

    Perennially ice-covered lakes in the McMurdo Dry Valleys, Antarctica, are chemically stratified with depth and have distinct biological gradients. Despite long-term research on these unique environments, data on the structure of the microbial communities in the water columns of these lakes are scarce. Here, we examined bacterial diversity in five ice-covered Antarctic lakes by 16S rRNA gene-based pyrosequencing. Distinct communities were present in each lake, reflecting the unique biogeochemical characteristics of these environments. Further, certain bacterial lineages were confined exclusively to specific depths within each lake. For example, candidate division WM88 occurred solely at a depth of 15 m in Lake Fryxell, whereas unknown lineages of Chlorobi were found only at a depth of 18 m in Lake Miers, and two distinct classes of Firmicutes inhabited East and West Lobe Bonney at depths of 30 m. Redundancy analysis revealed that community variation of bacterioplankton could be explained by the distinct conditions of each lake and depth; in particular, assemblages from layers beneath the chemocline had biogeochemical associations that differed from those in the upper layers. These patterns of community composition may represent bacterial adaptations to the extreme and unique biogeochemical gradients of ice-covered lakes in the McMurdo Dry Valleys. © 2017 Society for Applied Microbiology and John Wiley & Sons Ltd.

  12. Reconstructing lake ice cover in subarctic lakes using a diatom-based inference model

    NASA Astrophysics Data System (ADS)

    Weckström, Jan; Hanhijärvi, Sami; Forsström, Laura; Kuusisto, Esko; Korhola, Atte

    2014-03-01

    A new quantitative diatom-based lake ice cover inference model was developed to reconstruct past ice cover histories and applied to four subarctic lakes. The used ice cover model is based on a calculated melting degree day value of +130 and a freezing degree day value of -30 for each lake. The reconstructed Holocene ice cover duration histories show similar trends to the independently reconstructed regional air temperature history. The ice cover duration was around 7 days shorter than the average ice cover duration during the warmer early Holocene (approximately 10 to 6.5 calibrated kyr B.P.) and around 3-5 days longer during the cool Little Ice Age (approximately 500 to 100 calibrated yr B.P.). Although the recent climate warming is represented by only 2-3 samples in the sediment series, these show a rising trend in the prolonged ice-free periods of up to 2 days. Diatom-based ice cover inference models can provide a powerful tool to reconstruct past ice cover histories in remote and sensitive areas where no measured data are available.

  13. Perennially ice-covered Lake Hoare, Antarctica: physical environment, biology and sedimentation

    NASA Technical Reports Server (NTRS)

    Wharton, R. A. Jr; Simmons, G. M. Jr; McKay, C. P.; Wharton RA, J. r. (Principal Investigator)

    1989-01-01

    Lake Hoare (77 degrees 38' S, 162 degrees 53' E) is a perennially ice-covered lake at the eastern end of Taylor Valley in southern Victoria Land, Antarctica. The environment of this lake is controlled by the relatively thick ice cover (3-5 m) which eliminates wind generated currents, restricts gas exchange and sediment deposition, and reduces light penetration. The ice cover is in turn largely controlled by the extreme seasonality of Antarctica and local climate. Lake Hoare and other dry valley lakes may be sensitive indicators of short term (< 100 yr) climatic and/or anthropogenic changes in the dry valleys since the onset of intensive exploration over 30 years ago. The time constants for turnover of the water column and lake ice are 50 and 10 years, respectively. The turnover time for atmospheric gases in the lake is 30-60 years. Therefore, the lake environment responds to changes on a 10-100 year timescale. Because the ice cover has a controlling influence on the lake (e.g. light penetration, gas content of water, and sediment deposition), it is probable that small changes in ice ablation, sediment loading on the ice cover, or glacial meltwater (or groundwater) inflow will affect ice cover dynamics and will have a major impact on the lake environment and biota.

  14. Oxygen budget of a perennially ice-covered Antarctic lake

    NASA Technical Reports Server (NTRS)

    Wharton, R. A., Jr.; Mckay, C. P.; Simmons, G. M., Jr.; Parker, B. C.

    1986-01-01

    A bulk O2 budget for Lake Hoare, Antarctica, is presented. Five years of seasonal data show the lake to be persistently supersaturated with O2. Oxygen is carried into the lake in glacial meltstreams and is left behind when this water is removed as ice by ablation and sublimation. A diffusive loss of O2 from the lake through the summer moat is suggested. Measured values of the total O2 in the water column indicate that the time scale of O2 turnover is much longer than a year. Based on these results, it is suggested that the amount of O2 in the water does not change significantly throughout the year and that the lake is also supersaturated with N2.

  15. Study of the Microbial Diversity of a Newly Discovered East Antarctic Freshwater Lake, L27C, and of a Perennially Ice-Covered Lake Untersee

    NASA Technical Reports Server (NTRS)

    Huang, Jonathan P.; Hoover, Richard B.; Andersen, Dale; Bej, Asim K.

    2010-01-01

    The microbial communities that reside within freshwater lakes of Schirmacher and Untersee Oases in East Antarctica must cope with extreme conditions that may include cold temperature, annual freeze-thaw cycles, exposure to UV radiation, especially during the austral summer months, low light beneath thick ice-cover, followed by seasonal darkness. The objective of this study was to assess the microbial biodiversity and distribution from samples taken from two freshwater lakes (L27C and Lake Untersee) that were collected during the Tawani 2008 International Antarctic Expedition that conducted research in this region of Antarctica. L27C is a small, previously unreported lake residing 2 km WNW of Maitri Station at Schirmacher Oasis. Biodiversity and distribution of microorganisms within the lake were studied using both culture-independent and culture-dependent methodologies based upon the analysis of eubacterial 16S rRNA gene sequences. Lake Untersee, a perennially ice-covered, ultra-oligotrophic, lake in the Otto-von-Gruber-Gebirge (Gruber Mountains) of central Dronning Maud Land was also sampled and the microbial diversity was analyzed by eubacterial 16S rRNA gene sequences derived from pure cultures. Direct culturing of water samples from each lake on separate R2A growth medium exhibited a variety of microorganisms including: Janthinobacterium, Hymenobacter, Sphingamonas, Subtercola, Deinococcus, Arthrobacter, Flavobacterium, Polaromonas, Rhodoferax and Duganella. The evaluation of samples from L27C through culture-independent methodology identified a rich microbial diversity consisting of six different phyla of bacteria. The culture-independent analysis also displayed the majority of bacteria (56%) belonged to the Class gamma-proteobacteria within the phylum Proteobacteria. Within the Class gamma-proteobacteria, Acinetobacter dominated (48%) the total microbial load. Overall, L27C exhibited 7 different phyla of bacteria and 20 different genera. Statistical analysis

  16. The Ice-Covered Lakes Hypothesis in Gale Crater: Implications for the Early Hesperian Climate

    NASA Technical Reports Server (NTRS)

    Kling, Alexandre M.; Haberle, Robert M.; McKay, Christopher P.; Bristow, Thomas F.; Rivera-Hernandez, Frances

    2017-01-01

    Recent geological discoveries from the Mars Science Laboratory (MSL), including stream and lake sedimentary deposits, provide evidence that Gale crater may have intermittently hosted a fluviol-acustine environment during the Hesperian, with individual lakes lasting for a period of tens to hundreds of thousands of years. Estimates of the CO2 content of the atmosphere at the time the Gale sediments formed are far less than needed by any climate model to warm early Mars, given the low solar energy input available at Mars 3.5 Gya. We have therefore explored the possibility that the lakes in Gale during the Hesperian were perennially covered with ice using the Antarctic lakes as analogs.

  17. Thickness of ice on perennially frozen lakes

    USGS Publications Warehouse

    McKay, C.P.; Clow, G.D.; Wharton, R.A.; Squyres, S. W.

    1985-01-01

    The dry valleys of southern Victoria Land, constituting the largest ice-free expanse in the Antarctic, contain numerous lakes whose perennial ice cover is the cause of some unique physical and biological properties 1-3. Although the depth, temperature and salinity of the liquid water varies considerably from lake to lake, the thickness of the ice cover is remarkably consistent1, ranging from 3.5 to 6m, which is determined primarily by the balance between conduction of energy out of the ice and the release of latent heat at the ice-water interface and is also affected by the transmission and absorption of sunlight. In the steady state, the release of latent heat at the ice bottom is controlled by ablation from the ice surface. Here we present a simple energy-balance model, using the measured ablation rate of 30 cm yr-1, which can explain the observed ice thickness. ?? 1985 Nature Publishing Group.

  18. Ice-dammed lateral lake and epishelf lake insights into Holocene dynamics of Marguerite Trough Ice Stream and George VI Ice Shelf, Alexander Island, Antarctic Peninsula

    NASA Astrophysics Data System (ADS)

    Davies, Bethan J.; Hambrey, Michael J.; Glasser, Neil F.; Holt, Tom; Rodés, Angél; Smellie, John L.; Carrivick, Jonathan L.; Blockley, Simon P. E.

    2017-12-01

    We present new data regarding the past dynamics of Marguerite Trough Ice Stream, George VI Ice Shelf and valley glaciers from Ablation Point Massif on Alexander Island, Antarctic Peninsula. This ice-free oasis preserves a geological record of ice stream lateral moraines, ice-dammed lakes, ice-shelf moraines and valley glacier moraines, which we dated using cosmogenic nuclide ages. We provide one of the first detailed sediment-landform assemblage descriptions of epishelf lake shorelines. Marguerite Trough Ice Stream imprinted lateral moraines against eastern Alexander Island at 120 m at Ablation Point Massif. During deglaciation, lateral lakes formed in the Ablation and Moutonnée valleys, dammed against the ice stream in George VI Sound. Exposure ages from boulders on these shorelines yielded ages of 13.9 to 9.7 ka. Following recession of the ice stream, George VI Ice Shelf formed in George VI Sound. An epishelf lake formed at 15-20 m asl in Ablation and Moutonnée valleys, dated from 9.4 to 4.6 ka, suggesting that the lake was stable and persistent for some 5000 years. Lake-level lowering occurred after this, with the lake level at 12 m at 3.1 ± 0.4 ka and at 5 m asl today. A readvance of the valley glaciers on Alexander Island at 4.4 ± 0.7 ka is recorded by valley glacier moraines overlying epishelf lake sediments. We speculate that the glacier readvance, which occurred during a period of warmth, may have been caused by a dynamic response of the glaciers to a lowering in surface elevation of George VI Ice Shelf.

  19. Stable isotopic biogeochemistry of carbon and nitrogen in a perennially ice-covered Antarctic lake.

    PubMed

    Wharton, R A; Lyons, W B; Des Marais, D J

    1993-01-01

    Lake Hoare (77 degrees 38' S, 162 degrees 53' E) is an amictic, oligotrophic, 34-m-deep, closed-basin lake in Taylor Valley, Antarctica. Its perennial ice cover minimizes wind-generated currents and reduces light penetration, as well as restricts sediment deposition into the lake and the exchange of atmospheric gases between the water column and the atmosphere. The biological community of Lake Hoare consists solely of microorganisms -- both planktonic populations and benthic microbial mats. Lake Hoare is one of several perennially ice-covered lakes in the McMurdo Dry Valleys that represent the end-member conditions of cold desert and saline lakes. The dry valley lakes provide a unique opportunity to examine lacustrine processes that operate at all latitudes, but under an extreme set of environmental conditions. The dry valley lakes may also offer a valuable record of catchment and global changes in the past and present. Furthermore, these lakes are modern-day equivalents of periglacial lakes that are likely to have been common during periods of glacial maxima at temperate latitudes. We have analyzed the dissolved inorganic carbon (DIC) of Lake Hoare for delta 13C and the organic matter of the sediments and sediment-trap material for delta 13C and delta 15N. The delta 13C of the DIC indicates that 12C is differentially removed in the shallow, oxic portions of the lake via photosynthesis. In the anoxic portions of the lake (27-34 m) a net addition of 12C to the DIC pool occurs via organic matter decomposition. The dissolution of CaCO3 at depth also contributes to the DIC pool. Except near the Canada Glacier where a substantial amount of allochthonous organic matter enters the lake, the organic carbon being deposited on the lake bottom at different sites is isotopically similar, suggesting an autochthonous source for the organic carbon. Preliminary inorganic carbon flux calculations suggest that a high percentage of the organic carbon fixed in the water column is

  20. Stable isotopic biogeochemistry of carbon and nitrogen in a perennially ice-covered Antarctic lake

    NASA Technical Reports Server (NTRS)

    Wharton, R. A. Jr; Lyons, W. B.; Des Marais, D. J.; Wharton RA, J. r. (Principal Investigator)

    1993-01-01

    Lake Hoare (77 degrees 38' S, 162 degrees 53' E) is an amictic, oligotrophic, 34-m-deep, closed-basin lake in Taylor Valley, Antarctica. Its perennial ice cover minimizes wind-generated currents and reduces light penetration, as well as restricts sediment deposition into the lake and the exchange of atmospheric gases between the water column and the atmosphere. The biological community of Lake Hoare consists solely of microorganisms -- both planktonic populations and benthic microbial mats. Lake Hoare is one of several perennially ice-covered lakes in the McMurdo Dry Valleys that represent the end-member conditions of cold desert and saline lakes. The dry valley lakes provide a unique opportunity to examine lacustrine processes that operate at all latitudes, but under an extreme set of environmental conditions. The dry valley lakes may also offer a valuable record of catchment and global changes in the past and present. Furthermore, these lakes are modern-day equivalents of periglacial lakes that are likely to have been common during periods of glacial maxima at temperate latitudes. We have analyzed the dissolved inorganic carbon (DIC) of Lake Hoare for delta 13C and the organic matter of the sediments and sediment-trap material for delta 13C and delta 15N. The delta 13C of the DIC indicates that 12C is differentially removed in the shallow, oxic portions of the lake via photosynthesis. In the anoxic portions of the lake (27-34 m) a net addition of 12C to the DIC pool occurs via organic matter decomposition. The dissolution of CaCO3 at depth also contributes to the DIC pool. Except near the Canada Glacier where a substantial amount of allochthonous organic matter enters the lake, the organic carbon being deposited on the lake bottom at different sites is isotopically similar, suggesting an autochthonous source for the organic carbon. Preliminary inorganic carbon flux calculations suggest that a high percentage of the organic carbon fixed in the water column is

  1. Timescales of Growth Response of Microbial Mats to Environmental Change in an Ice-Covered Antarctic Lake

    PubMed Central

    Hawes, Ian; Sumner, Dawn Y.; Andersen, Dale T.; Jungblut, Anne D.; Mackey, Tyler J.

    2013-01-01

    Lake Vanda is a perennially ice-covered, closed-basin lake in the McMurdo Dry Valleys, Antarctica. Laminated photosynthetic microbial mats cover the floor of the lake from below the ice cover to >40 m depth. In recent decades, the water level of Lake Vanda has been rising, creating a “natural experiment” on development of mat communities on newly flooded substrates and the response of deeper mats to declining irradiance. Mats in recently flooded depths accumulate one lamina (~0.3 mm) per year and accrue ~0.18 µg chlorophyll-a cm−2 y−1. As they increase in thickness, vertical zonation becomes evident, with the upper 2-4 laminae forming an orange-brown zone, rich in myxoxanthophyll and dominated by intertwined Leptolyngbya trichomes. Below this, up to six phycobilin-rich green/pink-pigmented laminae form a subsurface zone, inhabited by Leptolyngbya, Oscillatoria and Phormidium morphotypes. Laminae continued to increase in thickness for several years after burial, and PAM fluorometry indicated photosynthetic potential in all pigmented laminae. At depths that have been submerged for >40 years, mats showed similar internal zonation and formed complex pinnacle structures that were only beginning to appear in shallower mats. Chlorophyll-a did not change over time and these mats appear to represent resource-limited “climax” communities. Acclimation of microbial mats to changing environmental conditions is a slow process, and our data show how legacy effects of past change persist into the modern community structure. PMID:24832656

  2. Timescales of growth response of microbial mats to environmental change in an ice-covered antarctic lake.

    PubMed

    Hawes, Ian; Sumner, Dawn Y; Andersen, Dale T; Jungblut, Anne D; Mackey, Tyler J

    2013-01-25

    Lake Vanda is a perennially ice-covered, closed-basin lake in the McMurdo Dry Valleys, Antarctica. Laminated photosynthetic microbial mats cover the floor of the lake from below the ice cover to >40 m depth. In recent decades, the water level of Lake Vanda has been rising, creating a "natural experiment" on development of mat communities on newly flooded substrates and the response of deeper mats to declining irradiance. Mats in recently flooded depths accumulate one lamina (~0.3 mm) per year and accrue ~0.18 µg chlorophyll-a cm-2 y-1. As they increase in thickness, vertical zonation becomes evident, with the upper 2-4 laminae forming an orange-brown zone, rich in myxoxanthophyll and dominated by intertwined Leptolyngbya trichomes. Below this, up to six phycobilin-rich green/pink-pigmented laminae form a subsurface zone, inhabited by Leptolyngbya, Oscillatoria and Phormidium morphotypes. Laminae continued to increase in thickness for several years after burial, and PAM fluorometry indicated photosynthetic potential in all pigmented laminae. At depths that have been submerged for >40 years, mats showed similar internal zonation and formed complex pinnacle structures that were only beginning to appear in shallower mats. Chlorophyll-a did not change over time and these mats appear to represent resource-limited "climax" communities. Acclimation of microbial mats to changing environmental conditions is a slow process, and our data show how legacy effects of past change persist into the modern community structure.

  3. Reduced Duration of Ice Cover in Swedish Lakes and Rivers

    NASA Astrophysics Data System (ADS)

    AghaKouchak, A.; Hallerback, S. A. M.; Stensen, K.; David, G.; Persson, M.

    2016-12-01

    The worlds freshwater systems are one of the most altered ecosystems on earth. Climate change introduces additional stresses on such systems, and this study presents an example of such change in an investigation of ice cover duration in Swedish lakes and rivers. In situ observations from over 750 lakes and rivers in Sweden were analyzed, with some records dating back to the beginning of the 18th century. Results show that ice duration significantly decreased over the last century. Change in ice duration is affected by later freeze as well as (more dominantly) earlier breakup dates. Additionally, since the late 1980's there has been an increase of extreme events, meaning years with extremely short duration of ice cover. The affect of temperature on the system was also examined. Using 113 years of temperature data, we empirically show how temperature changes affect the ice duration in lakes at different latitudes as well as dependent on lake area, volume and depth.

  4. The Antarctic dry valley lakes: Relevance to Mars

    NASA Technical Reports Server (NTRS)

    Wharton, R. A., Jr.; Mckay, Christopher P.; Mancinelli, Rocco L.; Clow, G. D.; Simmons, G. M., Jr.

    1989-01-01

    The similarity of the early environments of Mars and Earth, and the biological evolution which occurred on early Earth, motivates exobiologists to seriously consider the possiblity of an early Martian biota. Environments are being identified which could contain Martian life and areas which may presently contain evidence of this former life. Sediments which were thought to be deposited in large ice-covered lakes are present on Mars. Such localities were identified within some of the canyons of the Valles Marineris and more recently in the ancient terrain in the Southern Hemisphere. Perennially ice-covered Antarctic lakes are being studied in order to develop quantitative models that relate environmental factors to the nature of the biological community and sediment forming processes. These models will be applied to the Martian paleolakes to establish the scientific rationale for the exobiological study of ancient Martian sediments.

  5. Grounding Zones, Subglacial Lakes, and Dynamics of an Antarctic Ice Stream: The WISSARD Glaciological Experiment

    NASA Astrophysics Data System (ADS)

    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.

    2015-12-01

    Interactions of West Antarctic 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 Antarctic 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 Antarctic 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 water at its bed and its grounding line.

  6. Geoethical Approach to Antarctic Subglacial Lakes Exploration

    NASA Astrophysics Data System (ADS)

    Talalay, Pavel; Markov, Alexey; Sysoev, Mikhail

    2014-05-01

    Antarctic 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 Antarctic ice sheet. Nowadays it is generally recognized that a vast network of lakes, rivers, and streams exists thousands of meters beneath Antarctic 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 water 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 Antarctic 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 Antarctic ice to reach a subglacial lake Whillans and retrieve water and sediment samples. Both activities used hot-water drilling technology to access lakes. Hot water 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-water 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-water circulation medium is thermal pollution of subglacial water. The new approach to Antarctic 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

  7. Microbial life under ice: Metagenome diversity and in situ activity of Verrucomicrobia in seasonally ice-covered lakes.

    PubMed

    Tran, Patricia; Ramachandran, Arthi; Khawasek, Ola; Beisner, Beatrix E; Rautio, Milla; Huot, Yannick; Walsh, David A

    2018-06-19

    Northern lakes are ice-covered for a large part of the year, yet our understanding of microbial diversity and activity during winter lags behind that of the ice-free period. In this study, we investigated under-ice diversity and metabolism of Verrucomicrobia in seasonally ice-covered lakes in temperate and boreal regions of Quebec, Canada using 16S rRNA sequencing, metagenomics and metatranscriptomics. Verrucomicrobia, particularly the V1, V3 and V4 subdivisions, were abundant during ice-covered periods. A diversity of Verrucomicrobia genomes were reconstructed from Quebec lake metagenomes. Several genomes were associated with the ice-covered period and were represented in winter metatranscriptomes, supporting the notion that Verrucomicrobia are metabolically active under ice. Verrucomicrobia transcriptome analysis revealed a range of metabolisms potentially occurring under ice, including carbohydrate degradation, glycolate utilization, scavenging of chlorophyll degradation products, and urea use. Genes for aerobic sulfur and hydrogen oxidation were expressed, suggesting chemolithotrophy may be an adaptation to conditions where labile carbon may be limited. The expression of genes for flagella biosynthesis and chemotaxis was detected, suggesting Verrucomicrobia may be actively sensing and responding to winter nutrient pulses, such as phytoplankton blooms. These results increase our understanding on the diversity and metabolic processes occurring under ice in northern lakes ecosystems. This article is protected by copyright. All rights reserved. © 2018 Society for Applied Microbiology and John Wiley & Sons Ltd.

  8. High geothermal heat flux measured below the West Antarctic Ice Sheet

    PubMed Central

    Fisher, Andrew T.; Mankoff, Kenneth D.; Tulaczyk, Slawek M.; Tyler, Scott W.; Foley, Neil

    2015-01-01

    The geothermal heat flux is a critical thermal boundary condition that influences the melting, flow, and mass balance of ice sheets, but measurements of this parameter are difficult to make in ice-covered regions. We report the first direct measurement of geothermal heat flux into the base of the West Antarctic Ice Sheet (WAIS), below Subglacial Lake Whillans, determined from the thermal gradient and the thermal conductivity of sediment under the lake. The heat flux at this site is 285 ± 80 mW/m2, significantly higher than the continental and regional averages estimated for this site using regional geophysical and glaciological models. Independent temperature measurements in the ice indicate an upward heat flux through the WAIS of 105 ± 13 mW/m2. The difference between these heat flux values could contribute to basal melting and/or be advected from Subglacial Lake Whillans by flowing water. The high geothermal heat flux may help to explain why ice streams and subglacial lakes are so abundant and dynamic in this region. PMID:26601210

  9. High geothermal heat flux measured below the West Antarctic Ice Sheet.

    PubMed

    Fisher, Andrew T; Mankoff, Kenneth D; Tulaczyk, Slawek M; Tyler, Scott W; Foley, Neil

    2015-07-01

    The geothermal heat flux is a critical thermal boundary condition that influences the melting, flow, and mass balance of ice sheets, but measurements of this parameter are difficult to make in ice-covered regions. We report the first direct measurement of geothermal heat flux into the base of the West Antarctic Ice Sheet (WAIS), below Subglacial Lake Whillans, determined from the thermal gradient and the thermal conductivity of sediment under the lake. The heat flux at this site is 285 ± 80 mW/m(2), significantly higher than the continental and regional averages estimated for this site using regional geophysical and glaciological models. Independent temperature measurements in the ice indicate an upward heat flux through the WAIS of 105 ± 13 mW/m(2). The difference between these heat flux values could contribute to basal melting and/or be advected from Subglacial Lake Whillans by flowing water. The high geothermal heat flux may help to explain why ice streams and subglacial lakes are so abundant and dynamic in this region.

  10. Effects of glacial meltwater inflows and moat freezing on mixing in an ice-covered antarctic lake as interpreted from stable isotope and tritium distributions

    USGS Publications Warehouse

    Miller, L.G.; Aiken, G.R.

    1996-01-01

    Perennially ice-covered lakes in the McMurdo Dry Valleys have risen several meters over the past two decades due to climatic warming and increased glacial meltwater inflow. To elucidate the hydrologic responses to changing climate and the effects on lake mixing processes we measured the stable isotope (??18O and ??D) and tritium concentrations of water and ice samples collected in the Lake Fryxell watershed from 1987 through 1990. Stable isotope enrichment resulted from evaporation in stream and moat samples and from sublimation in surface lake-ice samples. Tritium enrichment resulted from exchange with the postnuclear atmosphere in stream and moat samples. Rapid injection of tritiated water into the upper water column of the make and incorporation of this water into the ice cover resulted in uniformly elevated tritium contents (> 3.0 TU) in these reservoirs. Tritium was also present in deep water, suggesting that a component of bottom water was recently at the surface. During summer, melted lake ice and stream water forms the moat. Water excluded from ice formation during fall moat freezing (enriched in solutes and tritium, and depleted in 18O and 2H relative to water below 15-m depth) may sink as density currents to the bottom of the lake. Seasonal lake circulation, in response to climate-driven surface inflow, is therefore responsible for the distribution of both water isotopes and dissolved solutes in Lake Fryxell.

  11. Investigating the crustal elements of the central Antarctic Plate (ICECAP): How long-range aerogeophysics is critical to understanding the evolution of the East Antarctic ice sheet

    NASA Astrophysics Data System (ADS)

    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.

    2004-12-01

    The highlands of the central Antarctic Plate have been the nursery for East Antarctic 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 Antarctic ice sheet and evolve in concert with them. Understanding the evolution of the East Antarctic 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 Antarctic Plate. A complete understanding of the evolution of East Antarctic 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 Antarctic 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 Antarctic ice sheet using a Navy P-3 aircraft based in Mc

  12. The identification, examination and exploration of Antarctic subglacial lakes.

    PubMed

    Siegert, M J

    2000-01-01

    At the floor of the Antarctic ice sheet, 4 km below the Russian research base Vostok Station, lies a 2,000 km3 body of water, comparable in size to Lake Ontario. This remote water 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 water. 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 Antarctic 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.

  13. Triple Isotope Water Measurements of Lake Untersee Ice using Off-Axis ICOS

    NASA Astrophysics Data System (ADS)

    Berman, E. S.; Huang, Y. W.; Andersen, D. T.; Gupta, M.; McKay, C. P.

    2015-12-01

    Lake Untersee (71.348°S, 13.458°E) is the largest surface freshwater lake in the interior of the Gruber Mountains of central Queen Maud Land in East Antarctica. The lake is permanently covered with ice, is partly bounded by glacier ice and has a mean annual air temperature of -10°C. In contrast to other Antarctic lakes the dominating physical process controlling ice-cover dynamics is low summer temperatures and high wind speeds resulting in sublimation rather than melting as the main mass-loss process. The ice-cover of the lake is composed of lake-water ice formed during freeze-up and rafted glacial ice derived from the Anuchin Glacier. The mix of these two fractions impacts the energy balance of the lake, which directly affects ice-cover thickness. Ice-cover is important if one is to understand the physical, chemical, and biological linkages within these unique, physically driven ecosystems. We have analyzed δ2H, δ18O, and δ17O from samples of lake and glacier ice collected at Lake Untersee in Dec 2014. Using these data we seek to answer two specific questions: Are we able to determine the origin and history of the lake ice, discriminating between rafted glacial ice and lake water? Can isotopic gradients in the surface ice indicate the ablation (sublimation) rate of the surface ice? The triple isotope water analyzer developed by Los Gatos Research (LGR 912-0032) uses LGR's patented Off-Axis ICOS (Integrated Cavity Output Spectroscopy) technology and incorporates proprietary internal thermal control for high sensitivity and optimal instrument stability. This analyzer measures δ2H, δ18O, and δ17O from water, as well as the calculated d-excess and 17O-excess. The laboratory precision in high performance mode for both δ17O and δ18O is 0.03 ‰, and for δ2H is 0.2 ‰. Methodology and isotope data from Lake Untersee samples are presented. Figure: Ice samples were collected across Lake Untersee from both glacial and lake ice regions for this study.

  14. Possible connections of the opposite trends in Arctic and Antarctic sea-ice cover.

    PubMed

    Yu, Lejiang; Zhong, Shiyuan; Winkler, Julie A; Zhou, Mingyu; Lenschow, Donald H; Li, Bingrui; Wang, Xianqiao; Yang, Qinghua

    2017-04-05

    Sea ice is an important component of the global climate system and a key indicator of climate change. A decreasing trend in Arctic sea-ice concentration is evident in recent years, whereas Antarctic sea-ice concentration exhibits a generally increasing trend. Various studies have investigated the underlying causes of the observed trends for each region, but possible linkages between the regional trends have not been studied. Here, we hypothesize that the opposite trends in Arctic and Antarctic sea-ice concentration may be linked, at least partially, through interdecadal variability of the Pacific Decadal Oscillation (PDO) and the Atlantic Multidecadal Oscillation (AMO). Although evaluation of this hypothesis is constrained by the limitations of the sea-ice cover record, preliminary statistical analyses of one short-term and two long-term time series of observed and reanalysis sea-ice concentrations data suggest the possibility of the hypothesized linkages. For all three data sets, the leading mode of variability of global sea-ice concentration is positively correlated with the AMO and negatively correlated with the PDO. Two wave trains related to the PDO and the AMO appear to produce anomalous surface-air temperature and low-level wind fields in the two polar regions that contribute to the opposite changes in sea-ice concentration.

  15. Possible connections of the opposite trends in Arctic and Antarctic sea-ice cover

    PubMed Central

    Yu, Lejiang; Zhong, Shiyuan; Winkler, Julie A.; Zhou, Mingyu; Lenschow, Donald H.; Li, Bingrui; Wang, Xianqiao; Yang, Qinghua

    2017-01-01

    Sea ice is an important component of the global climate system and a key indicator of climate change. A decreasing trend in Arctic sea-ice concentration is evident in recent years, whereas Antarctic sea-ice concentration exhibits a generally increasing trend. Various studies have investigated the underlying causes of the observed trends for each region, but possible linkages between the regional trends have not been studied. Here, we hypothesize that the opposite trends in Arctic and Antarctic sea-ice concentration may be linked, at least partially, through interdecadal variability of the Pacific Decadal Oscillation (PDO) and the Atlantic Multidecadal Oscillation (AMO). Although evaluation of this hypothesis is constrained by the limitations of the sea-ice cover record, preliminary statistical analyses of one short-term and two long-term time series of observed and reanalysis sea-ice concentrations data suggest the possibility of the hypothesized linkages. For all three data sets, the leading mode of variability of global sea-ice concentration is positively correlated with the AMO and negatively correlated with the PDO. Two wave trains related to the PDO and the AMO appear to produce anomalous surface-air temperature and low-level wind fields in the two polar regions that contribute to the opposite changes in sea-ice concentration. PMID:28378830

  16. In-lake carbon dioxide concentration patterns in four distinct phases in relation to ice cover dynamics

    NASA Astrophysics Data System (ADS)

    Denfeld, B. A.; Wallin, M.; Sahlee, E.; Sobek, S.; Kokic, J.; Chmiel, H.; Weyhenmeyer, G. A.

    2014-12-01

    Global carbon dioxide (CO2) emission estimates from inland waters include emissions at ice melt that are based on simple assumptions rather than evidence. To account for CO2 accumulation below ice and potential emissions into the atmosphere at ice melt we combined continuous CO2 concentrations with spatial CO2 sampling in an ice-covered small boreal lake. From early ice cover to ice melt, our continuous surface water CO2 concentration measurements at 2 m depth showed a temporal development in four distinct phases: In early winter, CO2 accumulated continuously below ice, most likely due to biological in-lake and catchment inputs. Thereafter, in late winter, CO2 concentrations remained rather constant below ice, as catchment inputs were minimized and vertical mixing of hypolimnetic water was cut off. As ice melt began, surface water CO2 concentrations were rapidly changing, showing two distinct peaks, the first one reflecting horizontal mixing of CO2 from surface and catchment waters, the second one reflecting deep water mixing. We detected that 83% of the CO2 accumulated in the water during ice cover left the lake at ice melt which corresponded to one third of the total CO2 storage. Our results imply that CO2 emissions at ice melt must be accurately integrated into annual CO2 emission estimates from inland waters. If up-scaling approaches assume that CO2 accumulates linearly under ice and at ice melt all CO2 accumulated during ice cover period leaves the lake again, present estimates may overestimate CO2 emissions from small ice covered lakes. Likewise, neglecting CO2 spring outbursts will result in an underestimation of CO2 emissions from small ice covered lakes.

  17. Characterizing Microbial Mat Morphology with Structure from Motion Techniques in Ice-Covered Lake Joyce, McMurdo Dry Valleys, Antarctica

    NASA Astrophysics Data System (ADS)

    Mackey, T. J.; Leidman, S. Z.; Allen, B.; Hawes, I.; Lawrence, J.; Jungblut, A. D.; Krusor, M.; Coleman, L.; Sumner, D. Y.

    2015-12-01

    Structure from Motion (SFM) techniques can provide quantitative morphological documentation of otherwise inaccessible benthic ecosystems such as microbial mats in Lake Joyce, a perennially ice-covered lake of the Antarctic McMurdo Dry Valleys (MDV). Microbial mats are a key ecosystem of MDV lakes, and diverse mat morphologies like pinnacles emerge from interactions among microbial behavior, mineralization, and environmental conditions. Environmental gradients can be isolated to test mat growth models, but assessment of mat morphology along these gradients is complicated by their inaccessibility: the Lake Joyce ice cover is 4-5 m thick, water depths containing diverse pinnacle morphologies are 9-14 m, and relevant mat features are cm-scale. In order to map mat pinnacle morphology in different sedimentary settings, we deployed drop cameras (SeaViewer and GoPro) through 29 GPS referenced drill holes clustered into six stations along a transect spanning 880 m. Once under the ice cover, a boom containing a second GoPro camera was unfurled and rotated to collect oblique images of the benthic mats within dm of the mat-water interface. This setup allowed imaging from all sides over a ~1.5 m diameter area of the lake bottom. Underwater lens parameters were determined for each camera in Agisoft Lens; images were reconstructed and oriented in space with the SFM software Agisoft Photoscan, using the drop camera axis of rotation as up. The reconstructions were compared to downward facing images to assess accuracy, and similar images of an object with known geometry provided a test for expected error in reconstructions. Downward facing images identify decreasing pinnacle abundance in higher sedimentation settings, and quantitative measurements of 3D reconstructions in KeckCAVES LidarViewer supplement these mat morphological facies with measurements of pinnacle height and orientation. Reconstructions also help isolate confounding variables for mat facies trends with measurements

  18. Heating the Ice-Covered Lakes of the McMurdo Dry Valleys, Antarctica - Decadal Trends in Heat Content, Ice Thickness, and Heat Exchange

    NASA Astrophysics Data System (ADS)

    Gooseff, M. N.; Priscu, J. C.; Doran, P. T.; Chiuchiolo, A.; Obryk, M.

    2014-12-01

    Lakes integrate landscape processes and climate conditions. Most of the permanently ice-covered lakes in the McMurdo Dry Valleys, Antarctica are closed basin, receiving glacial melt water from streams for 10-12 weeks per year. Lake levels rise during the austral summer are balanced by sublimation of ice covers (year-round) and evaporation of open water moats (summer only). Vertical profiles of water temperature have been measured in three lakes in Taylor Valley since 1988. Up to 2002, lake levels were dropping, ice covers were thickening, and total heat contents were decreasing. These lakes have been gaining heat since the mid-2000s, at rates as high as 19.5x1014 cal/decade). Since 2002, lake levels have risen substantially (as much as 2.5 m), and ice covers have thinned (1.5 m on average). Analyses of lake ice thickness, meteorological conditions, and stream water heat loads indicate that the main source of heat to these lakes is from latent heat released when ice-covers form during the winter. An aditional source of heat to the lakes is water inflows from streams and direct glacieal melt. Mean lake temperatures in the past few years have stabilized or cooled, despite increases in lake level and total heat content, suggesting increased direct inflow of meltwater from glaciers. These results indicate that McMurdo Dry Valley lakes are sensitive indicators of climate processes in this polar desert landscape and demonstrate the importance of long-term data sets when addressing the effects of climate on ecosystem processes.

  19. Lake Ice Cover of Shallow Lakes and Climate Interactions in Arctic Regions (1950-2011): SAR Data Analysis and Numerical Modeling

    NASA Astrophysics Data System (ADS)

    Surdu, C.; Duguay, C.; Brown, L.; Fernàndez-Prieto, D.; Samuelsson, P.

    2012-12-01

    Lake ice cover is highly correlated with climatic conditions and has, therefore, been demonstrated to be an essential indicator of climate variability and change. Recent studies have shown that the duration of the lake ice cover has decreased, mainly as a consequence of earlier thaw dates in many parts of the Northern Hemisphere over the last 50 years, mainly as a feedback to increased winter and spring air temperature. In response to projected air temperature and winter precipitation changes by climate models until the end of the 21st century, the timing, duration, and thickness of ice cover on Arctic lakes are expected to be impacted. This, in turn, will likely alter the energy, water, and bio-geochemical cycling in various regions of the Arctic. In the case of shallow tundra lakes, many of which are less than 3-m deep, warmer climate conditions could result in a smaller fraction of lakes that fully freeze to the bottom at the time of maximum winter ice thickness since thinner ice covers are predicted to develop. Shallow thermokarst lakes of the coastal plain of northern Alaska, and of other similar Arctic regions, have likely been experiencing changes in seasonal ice phenology and thickness over the last few decades but these have not yet been comprehensively documented. Analysis of a 20-year time series of ERS-1/2 synthetic aperture radar (SAR) data and numerical lake ice modeling were employed to determine the response of ice cover (thickness, freezing to bed, and phenology) on shallow lakes of the North Slope of Alaska (NSA) to climate conditions over the last three decades. New downscaled data specific to the Arctic domain (at a resolution of 0.44 degrees using ERA Interim Reanalysis as boundary condition) produced by the Rossby Centre Regional Atmospheric Climate Model (RCA4) was used to drive the Canadian Lake Ice Model (CLIMo) for the period 1950-2011. In order to assess and integrate the SAR-derived observed changes into a longer historical context, and

  20. The geochemistry of methane in Lake Fryxell, an amictic, permanently ice-covered, antarctic lake

    USGS Publications Warehouse

    Smith, R.L.; Miller, L.G.; Howes, B.L.

    1993-01-01

    The abundance and distribution of dissolved CH4 were determined from 1987-1990 in Lake Fryxell, Antarctica, an amictic, permanently ice-covered lake in which solute movement is controlled by diffusion. CH4 concentrations were < 1 ??M in the upper oxic waters, but increased below the oxycline to 936 ??M at 18 m. Sediment CH4 was 1100 ??mol (1 sed)-1 in the 0-5 cm zone. Upward flux from the sediment was the source of the CH4, NH4 +, and DOC in the water column; CH4 was 27% of the DOC+CH4 carbon at 18 m. Incubations with surficial sediments indicated that H14CO3 - reduction was 0.4 ??mol (1 sed)-1 day-1 or 4?? the rate of acetate fermentation to CH4. There was no measurable CH4 production in the water column. However, depth profiles of CH4, NH4, and DIC normalized to bottom water concentrations demonstrated that a significant CH4 sink was evident in the anoxic, sulfate-containing zone of the water column (10-18 m). The ??13CH4 in this zone decreased from -72 % at 18 m to -76% at 12 m, indicating that the consumption mechanism did not result in an isotopic enrichment of 13CH4. In contrast, ??13CH4 increased to -55 % at 9 m due to aerobic oxidation, though this was a minor aspect of the CH4 cycle. The water column CH4 profile was modeled by coupling diffusive flux with a first order consumption term; the best-fit rate constant for anaerobic CH4 consumption was 0.012 yr-1. On a total carbon basis, CH4 consumption in the anoxic water column exerted a major effect on the flux of carbonaceous material from the underlying sediments and serves to exemplify the importance of CH4 to carbon cycling in Lake Fryxell. ?? 1993 Kluwer Academic Publishers.

  1. Ground penetrating radar detection of subsnow slush on ice-covered lakes in interior Alaska

    NASA Astrophysics Data System (ADS)

    Gusmeroli, A.; Grosse, G.

    2012-12-01

    Lakes are abundant throughout the pan-Arctic region. For many of these lakes ice cover lasts for up to two thirds of the year. The frozen cover allows human access to these lakes, which are therefore used for many subsistence and recreational activities, including water harvesting, fishing, and skiing. Safe traveling condition onto lakes may be compromised, however, when, after significant snowfall, the weight of the snow acts on the ice and causes liquid water to spill through weak spots and overflow at the snow-ice interface. Since visual detection of subsnow slush is almost impossible our understanding on overflow processes is still very limited and geophysical methods that allow water and slush detection are desirable. In this study we demonstrate that a commercially available, lightweight 1 GHz, ground penetrating radar system can detect and map extent and intensity of overflow. The strength of radar reflections from wet snow-ice interfaces are at least twice as much in strength than returns from dry snow-ice interface. The presence of overflow also affects the quality of radar returns from the base of the lake ice. During dry conditions we were able to profile ice thickness of up to 1 m, conversely, we did not retrieve any ice-water returns in areas affected by overflow.

  2. A microbial ecosystem beneath the West Antarctic ice sheet.

    PubMed

    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

    2014-08-21

    Liquid water has been known to occur beneath the Antarctic 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 water and surficial sediments obtained from direct sampling of a subglacial Antarctic 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 water 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 Antarctic 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.

  3. Modeling the Thickness of Perennial Ice Covers on Stratified Lakes of the Taylor Valley, Antarctica

    NASA Technical Reports Server (NTRS)

    Obryk, M. K.; Doran, P. T.; Hicks, J. A.; McKay, C. P.; Priscu, J. C.

    2016-01-01

    A one-dimensional ice cover model was developed to predict and constrain drivers of long term ice thickness trends in chemically stratified lakes of Taylor Valley, Antarctica. The model is driven by surface radiative heat fluxes and heat fluxes from the underlying water column. The model successfully reproduced 16 years (between 1996 and 2012) of ice thickness changes for west lobe of Lake Bonney (average ice thickness = 3.53 m; RMSE = 0.09 m, n = 118) and Lake Fryxell (average ice thickness = 4.22 m; RMSE = 0.21 m, n = 128). Long-term ice thickness trends require coupling with the thermal structure of the water column. The heat stored within the temperature maximum of lakes exceeding a liquid water column depth of 20 m can either impede or facilitate ice thickness change depending on the predominant climatic trend (temperature cooling or warming). As such, shallow (< 20 m deep water columns) perennially ice-covered lakes without deep temperature maxima are more sensitive indicators of climate change. The long-term ice thickness trends are a result of surface energy flux and heat flux from the deep temperature maximum in the water column, the latter of which results from absorbed solar radiation.

  4. Evidence for a palaeo-subglacial lake on the Antarctic continental shelf

    PubMed Central

    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.

    2017-01-01

    Subglacial lakes are widespread beneath the Antarctic 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 Antarctic 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 water 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

  5. Microbial Mat Communities along an Oxygen Gradient in a Perennially Ice-Covered Antarctic Lake

    PubMed Central

    Hawes, Ian; Mackey, Tyler J.; Krusor, Megan; Doran, Peter T.; Sumner, Dawn Y.; Eisen, Jonathan A.; Hillman, Colin; Goroncy, Alexander K.

    2015-01-01

    Lake Fryxell is a perennially ice-covered lake in the McMurdo Dry Valleys, Antarctica, with a sharp oxycline in a water column that is density stabilized by a gradient in salt concentration. Dissolved oxygen falls from 20 mg liter−1 to undetectable over one vertical meter from 8.9- to 9.9-m depth. We provide the first description of the benthic mat community that falls within this oxygen gradient on the sloping floor of the lake, using a combination of micro- and macroscopic morphological descriptions, pigment analysis, and 16S rRNA gene bacterial community analysis. Our work focused on three macroscopic mat morphologies that were associated with different parts of the oxygen gradient: (i) “cuspate pinnacles” in the upper hyperoxic zone, which displayed complex topography and were dominated by phycoerythrin-rich cyanobacteria attributable to the genus Leptolyngbya and a diverse but sparse assemblage of pennate diatoms; (ii) a less topographically complex “ridge-pit” mat located immediately above the oxic-anoxic transition containing Leptolyngbya and an increasing abundance of diatoms; and (iii) flat prostrate mats in the upper anoxic zone, dominated by a green cyanobacterium phylogenetically identified as Phormidium pseudopriestleyi and a single diatom, Diadesmis contenta. Zonation of bacteria was by lake depth and by depth into individual mats. Deeper mats had higher abundances of bacteriochlorophylls and anoxygenic phototrophs, including Chlorobi and Chloroflexi. This suggests that microbial communities form assemblages specific to niche-like locations. Mat morphologies, underpinned by cyanobacterial and diatom composition, are the result of local habitat conditions likely defined by irradiance and oxygen and sulfide concentrations. PMID:26567300

  6. Microbial Mat Communities along an Oxygen Gradient in a Perennially Ice-Covered Antarctic Lake.

    PubMed

    Jungblut, Anne D; Hawes, Ian; Mackey, Tyler J; Krusor, Megan; Doran, Peter T; Sumner, Dawn Y; Eisen, Jonathan A; Hillman, Colin; Goroncy, Alexander K

    2016-01-15

    Lake Fryxell is a perennially ice-covered lake in the McMurdo Dry Valleys, Antarctica, with a sharp oxycline in a water column that is density stabilized by a gradient in salt concentration. Dissolved oxygen falls from 20 mg liter(-1) to undetectable over one vertical meter from 8.9- to 9.9-m depth. We provide the first description of the benthic mat community that falls within this oxygen gradient on the sloping floor of the lake, using a combination of micro- and macroscopic morphological descriptions, pigment analysis, and 16S rRNA gene bacterial community analysis. Our work focused on three macroscopic mat morphologies that were associated with different parts of the oxygen gradient: (i) "cuspate pinnacles" in the upper hyperoxic zone, which displayed complex topography and were dominated by phycoerythrin-rich cyanobacteria attributable to the genus Leptolyngbya and a diverse but sparse assemblage of pennate diatoms; (ii) a less topographically complex "ridge-pit" mat located immediately above the oxic-anoxic transition containing Leptolyngbya and an increasing abundance of diatoms; and (iii) flat prostrate mats in the upper anoxic zone, dominated by a green cyanobacterium phylogenetically identified as Phormidium pseudopriestleyi and a single diatom, Diadesmis contenta. Zonation of bacteria was by lake depth and by depth into individual mats. Deeper mats had higher abundances of bacteriochlorophylls and anoxygenic phototrophs, including Chlorobi and Chloroflexi. This suggests that microbial communities form assemblages specific to niche-like locations. Mat morphologies, underpinned by cyanobacterial and diatom composition, are the result of local habitat conditions likely defined by irradiance and oxygen and sulfide concentrations. Copyright © 2016, American Society for Microbiology. All Rights Reserved.

  7. Examining Differences in Arctic and Antarctic Sea Ice Change

    NASA Astrophysics Data System (ADS)

    Nghiem, S. V.; Rigor, I. G.; Clemente-Colon, P.; Neumann, G.; Li, P.

    2015-12-01

    The paradox of the rapid reduction of Arctic sea ice versus the stability (or slight increase) of Antarctic 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 Antarctic sea ice cover. The reduction of salinity and density in the near-surface layer may weaken the convective mixing of cold and warmer waters, and thus maintaining regions of no warming around the Antarctic. A decrease in sea ice growth may reduce salt rejection and upper-ocean density to enhance thermohalocline stratification, and thus supporting Antarctic sea ice production. Melt water from Antarctic ice shelves collects in a cool and fresh surface layer to shield the surface ocean from the warmer deeper waters, and thus leading to an expansion of Antarctic sea ice. Also, wind effects may positively contribute to Antarctic 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 Antarctic, 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 Antarctic sea ice change to contribute to resolving the Arctic-Antarctic sea ice paradox.

  8. Bacteria beneath the West Antarctic ice sheet.

    PubMed

    Lanoil, Brian; Skidmore, Mark; Priscu, John C; Han, Sukkyun; Foo, Wilson; Vogel, Stefan W; Tulaczyk, Slawek; Engelhardt, Hermann

    2009-03-01

    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 Antarctic 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 Antarctic 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 water. Although in situ cell abundance and the extent of wet sediments beneath the Antarctic 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.

  9. A dynamic early East Antarctic Ice Sheet suggested by ice-covered fjord landscapes.

    PubMed

    Young, Duncan A; Wright, Andrew P; Roberts, Jason L; Warner, Roland C; Young, Neal W; Greenbaum, Jamin S; Schroeder, Dustin M; Holt, John W; Sugden, David E; Blankenship, Donald D; van Ommen, Tas D; Siegert, Martin J

    2011-06-02

    The first Cenozoic ice sheets initiated in Antarctica from the Gamburtsev Subglacial Mountains and other highlands as a result of rapid global cooling ∼34 million years ago. In the subsequent 20 million years, at a time of declining atmospheric carbon dioxide concentrations and an evolving Antarctic circumpolar current, sedimentary sequence interpretation and numerical modelling suggest that cyclical periods of ice-sheet expansion to the continental margin, followed by retreat to the subglacial highlands, occurred up to thirty times. These fluctuations were paced by orbital changes and were a major influence on global sea levels. Ice-sheet models show that the nature of such oscillations is critically dependent on the pattern and extent of Antarctic topographic lowlands. Here we show that the basal topography of the Aurora Subglacial Basin of East Antarctica, at present overlain by 2-4.5 km of ice, is characterized by a series of well-defined topographic channels within a mountain block landscape. The identification of this fjord landscape, based on new data from ice-penetrating radar, provides an improved understanding of the topography of the Aurora Subglacial Basin and its surroundings, and reveals a complex surface sculpted by a succession of ice-sheet configurations substantially different from today's. At different stages during its fluctuations, the edge of the East Antarctic Ice Sheet lay pinned along the margins of the Aurora Subglacial Basin, the upland boundaries of which are currently above sea level and the deepest parts of which are more than 1 km below sea level. Although the timing of the channel incision remains uncertain, our results suggest that the fjord landscape was carved by at least two iceflow regimes of different scales and directions, each of which would have over-deepened existing topographic depressions, reversing valley floor slopes.

  10. SIMULATED CLIMATE CHANGE EFFECTS ON DISSOLVED OXYGEN CHARACTERISTICS IN ICE-COVERED LAKES. (R824801)

    EPA Science Inventory

    A deterministic, one-dimensional model is presented which simulates daily dissolved oxygen (DO) profiles and associated water temperatures, ice covers and snow covers for dimictic and polymictic lakes of the temperate zone. The lake parameters required as model input are surface ...

  11. Microwave Observations of Snow-Covered Freshwater Lake Ice obtained during the Great Lakes Winter EXperiment (GLAWEX), 2017

    NASA Astrophysics Data System (ADS)

    Gunn, G. E.; Hall, D. K.; Nghiem, S. V.

    2017-12-01

    Studies observing lake ice using active microwave acquisitions suggest that the dominant scattering mechanism in ice is caused by double-bounce of the signal off vertical tubular bubble inclusions. Recent polarimetric SAR observations and target decomposition algorithms indicate single-bounce interactions may be the dominant source of returns, and in the absence of field observations, has been hypothesized to be the result of roughness at the ice-water interface on the order of incident wavelengths. This study presents in-situ physical observations of snow-covered lake ice in western Michigan and Wisconsin acquired during the Great Lakes Winter EXperiment in 2017 (GLAWEX'17). In conjunction with NASA's SnowEx airborne snow campaign in Colorado (http://snow.nasa.gov), C- (Sentinel-1, RADARSAT-2) and X-band (TerraSAR-X) synthetic aperture radar (SAR) observations were acquired coincidently to surface physical snow and ice observations. Small/large scale roughness features at the ice-water interface are quantified through auger transects and used as an input variable in lake ice backscatter models to assess the relative contributions from different scattering mechanisms.

  12. Modeling Antarctic Subglacial Lake Filling and Drainage Cycles

    NASA Technical Reports Server (NTRS)

    Dow, Christine F.; Werder, Mauro A.; Nowicki, Sophie; Walker, Ryan T.

    2016-01-01

    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 Antarctic 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 water 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 water in the ice stream onset region results in a buildup of pressure creating temporary channels, which then evacuate the excess water. This increased flux of water beneath the ice stream drives lake growth. As the water 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 water 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.

  13. The Antarctic Ice.

    ERIC Educational Resources Information Center

    Radok, Uwe

    1985-01-01

    The International Antarctic Glaciological Project has collected information on the East Antarctic 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)

  14. Mass Fluxes of Ice and Oxygen Across the Entire Lid of Lake Vostok from Observations of Englacial Radiowave Attenuation

    NASA Astrophysics Data System (ADS)

    Winebrenner, D. P.; Kintner, P. M. S.; MacGregor, J. A.

    2017-12-01

    Over deep Antarctic subglacial lakes, spatially varying ice thickness and the pressure-dependent melting point of ice result in areas of melting and accretion at the ice-water interface, i.e., the lake lid. These ice mass fluxes drive lake circulation and, because basal Antarctic ice contains air-clathrate, affect the input of oxygen to the lake, with implications for subglacial life. Inferences of melting and accretion from radar-layer tracking and geodesy are limited in spatial coverage and resolution. Here we develop a new method to estimate rates of accretion, melting, and the resulting oxygen input at a lake lid, using airborne radar data over Lake Vostok together with ice-temperature and chemistry data from the Vostok ice core. Because the lake lid is a coherent reflector of known reflectivity (at our radar frequency), we can infer depth-averaged radiowave attenuation in the ice, with spatial resolution 1 km along flight lines. Spatial variation in attenuation depends mostly on variation in ice temperature near the lid, which in turn varies strongly with ice mass flux at the lid. We model ice temperature versus depth with ice mass flux as a parameter, thus linking that flux to (observed) depth-averaged attenuation. The resulting map of melt- and accretion-rates independently reproduces features known from earlier studies, but now covers the entire lid. We find that accretion is dominant when integrated over the lid, with an ice imbalance of 0.05 to 0.07 km3 a-1, which is robust against uncertainties.

  15. Simulating hydrodynamics and ice cover in Lake Erie using an unstructured grid model

    NASA Astrophysics Data System (ADS)

    Fujisaki-Manome, A.; Wang, J.

    2016-02-01

    An unstructured grid Finite-Volume Coastal Ocean Model (FVCOM) is applied to Lake Erie to simulate seasonal ice cover. The model is coupled with an unstructured-grid, finite-volume version of the Los Alamos Sea Ice Model (UG-CICE). We replaced the original 2-time-step Euler forward scheme in time integration by the central difference (i.e., leapfrog) scheme to assure a neutrally inertial stability. The modified version of FVCOM coupled with the ice model is applied to the shallow freshwater lake in this study using unstructured grids to represent the complicated coastline in the Laurentian Great Lakes and refining the spatial resolution locally. We conducted multi-year simulations in Lake Erie from 2002 to 2013. The results were compared with the observed ice extent, water surface temperature, ice thickness, currents, and water temperature profiles. Seasonal and interannual variation of ice extent and water temperature was captured reasonably, while the modeled thermocline was somewhat diffusive. The modeled ice thickness tends to be systematically thinner than the observed values. The modeled lake currents compared well with measurements obtained from an Acoustic Doppler Current Profiler located in the deep part of the lake, whereas the simulated currents deviated from measurements near the surface, possibly due to the model's inability to reproduce the sharp thermocline during the summer and the lack of detailed representation of offshore wind fields in the interpolated meteorological forcing.

  16. When a habitat freezes solid: Microorganisms over-winter within the ice column of a coastal Antarctic lake

    USGS Publications Warehouse

    Foreman, C.M.; Dieser, M.; Greenwood, M.; Cory, R.M.; Laybourn-Parry, J.; Lisle, J.T.; Jaros, C.; Miller, P.L.; Chin, Y.-P.; McKnight, Diane M.

    2011-01-01

    A major impediment to understanding the biology of microorganisms inhabiting Antarctic environments is the logistical constraint of conducting field work primarily during the summer season. However, organisms that persist throughout the year encounter severe environmental changes between seasons. In an attempt to bridge this gap, we collected ice core samples from Pony Lake in early November 2004 when the lake was frozen solid to its base, providing an archive for the biological and chemical processes that occurred during winter freezeup. The ice contained bacteria and virus-like particles, while flagellated algae and ciliates over-wintered in the form of inactive cysts and spores. Both bacteria and algae were metabolically active in the ice core melt water. Bacterial production ranged from 1.8 to 37.9??gCL-1day-1. Upon encountering favorable growth conditions in the melt water, primary production ranged from 51 to 931??gCL-1day-1. Because of the strong H2S odor and the presence of closely related anaerobic organisms assigned to Pony Lake bacterial 16S rRNA gene clones, we hypothesize that the microbial assemblage was strongly affected by oxygen gradients, which ultimately restricted the majority of phylotypes to distinct strata within the ice column. This study provides evidence that the microbial community over-winters in the ice column of Pony Lake and returns to a highly active metabolic state when spring melt is initiated. ?? 2011 Federation of European Microbiological Societies.

  17. Ciliated protozoa of two antarctic lakes: analysis by quantitative protargol staining and examination of artificial substrates

    NASA Technical Reports Server (NTRS)

    Kepner, R. L. Jr; Wharton, R. A. Jr; Coats, D. W.; Wharton RA, J. r. (Principal Investigator)

    1999-01-01

    Planktonic and artificial substrate-associated ciliates have been identified in two perennially ice-covered antarctic lakes of the McMurdo Dry Valleys. Abundances estimated by quantitative protargol staining ranged from < 5 to 31690 cells l-1, levels that are comparable to those previously obtained using other methods. Nineteen ciliate taxa were identified from these lakes, with the most frequently encountered genera being Plagiocampa, Askenasia, Monodinium, Sphaerophrya and Vorticella. The taxonomic findings compare favorably with those of previous investigators; however four previously unreported genera were observed in both Lakes Fryxell and Hoare. The variability in the depth distributions of ciliates in Lake Fryxell is explained in terms of lake physicochemical properties and ciliate prey distributions, while factors related to temporal succession in the Lake Hoare assemblage remain unexplained. Local marine or temperate zone freshwater habitats are a more likely source than the surrounding dry valleys soils for present ciliate colonists in these lakes. Although the taxonomic uncertainties require further examination, our results suggest that ciliate populations in these antarctic lakes undergo significant fluctuations and are more diverse than was previously recognized.

  18. Persistent Ice on Lake Superior

    NASA Image and Video Library

    2017-12-08

    Though North America is a full month into astronomical spring, the Great Lakes have been slow to give up on winter. As of April 22, 2014, the Great Lakes were 33.9 percent ice covered. The lake they call Superior dominated the pack. In the early afternoon on April 20, 2014, the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA’s Aqua satellite captured this natural-color image of Lake Superior, which straddles the United States–Canada border. At the time Aqua passed over, the lake was 63.5 percent ice covered, according to the NOAA Great Lakes Environmental Research Lab (GLERL). Averaged across Lake Superior, ice was 22.6 centimeters (8.9 inches) thick; it was as much as twice that thickness in some locations. GLERL researcher George Leshkevich affirmed that ice cover this spring is significantly above normal. For comparison, Lake Superior had 3.6 percent ice cover on April 20, 2013; in 2012, ice was completely gone by April 12. In the last winter that ice cover grew so thick on Lake Superior (2009), it reached 93.7 percent on March 2 but was down to 6.7 percent by April 21. Average water temperatures on all of the Great Lakes have been rising over the past 30 to 40 years and ice cover has generally been shrinking. (Lake Superior ice was down about 79 percent since the 1970s.) But chilled by persistent polar air masses throughout the 2013-14 winter, ice cover reached 88.4 percent on February 13 and 92.2 percent on March 6, 2014, the second highest level in four decades of record-keeping. Air temperatures in the Great Lakes region were well below normal for March, and the cool pattern is being reinforced along the coasts because the water is absorbing less sunlight and warming less than in typical spring conditions. The graph below, based on data from Environment Canada, shows the 2014 conditions for all of the Great Lakes in mid-April compared to the past 33 years. Lake Superior ice cover got as high as 95.3 percent on March 19. By April 22, it was

  19. Under the ice in Antarctica.

    PubMed

    Wharton, R A

    1986-06-01

    The 1985 Antarctic Scientific Research Expedition to Lake Hoare in Taylor Valley is briefly described. Of particular interest to to the expedition is the nature of the lake's perennial ice cover and its role in concentrating dissolved gases. Also, the algal mats and sediment found on the bottom of the lake were studied. Antarctic lakes have been cited as possible analogs for possible biological habitats on Mars and on Europa.

  20. Sedimentology and geochemistry of a perennially ice-covered epishelf lake in Bunger Hills Oasis, East Antarctica.

    PubMed

    Doran, P T; Wharton, R A; Lyons, W B; Des Marais, D J; Andersen, D T

    2000-01-01

    A process-oriented study was carried out in White Smoke lake, Bunger Hills, East Antarctica, a perennially ice-covered (1.8 to 2.8 m thick) epishelf (tidally-forced) lake. The lake water has a low conductivity and is relatively well mixed. Sediments are transferred from the adjacent glacier to the lake when glacier ice surrounding the sediment is sublimated at the surface and replaced by accumulating ice from below. The lake bottom at the west end of the lake is mostly rocky with a scant sediment cover. The east end contains a thick sediment profile. Grain size and delta 13C increase with sediment depth, indicating a more proximal glacier in the past. Sedimentary 210Pb and 137Cs signals are exceptionally strong, probably a result of the focusing effect of the large glacial catchment area. The post-bomb and pre-bomb radiocarbon reservoirs are c. 725 14C yr and c. 1950 14C yr, respectively. Radiocarbon dating indicates that the east end of the lake is >3 ka BP, while photographic evidence and the absence of sediment cover indicate that the west end has formed only over the last century. Our results indicate that the southern ice edge of Bunger Hills has been relatively stable with only minor fluctuations (on the scale of hundreds of metres) over the last 3000 years.

  1. Breakup of Pack Ice, Antarctic Ice Shelf

    NASA Image and Video Library

    1991-09-18

    STS048-152-007 (12-18 Sept 1991) --- The periphery of the Antarctic ice shelf and the Antarctic 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 waters of the circum-Antarctic southern ocean.

  2. Antarctic sea ice thickness data archival and recovery at the Australian Antarctic Data Centre

    NASA Astrophysics Data System (ADS)

    Worby, A. P.; Treverrow, A.; Raymond, B.; Jordan, M.

    2007-12-01

    A new effort is underway to establish a portal for Antarctic sea ice thickness data at the Australian Antarctic 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 Antarctic 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 Antarctic 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/

  3. Mapping and Assessing Variability in the Antarctic Marginal Ice Zone, the Pack Ice and Coastal Polynyas

    NASA Astrophysics Data System (ADS)

    Stroeve, Julienne; Jenouvrier, Stephanie

    2016-04-01

    Sea ice variability within the marginal ice zone (MIZ) and polynyas plays an important role for phytoplankton productivity and krill abundance. Therefore mapping their spatial extent, seasonal and interannual variability is essential for understanding how current and future changes in these biological active regions may impact the Antarctic marine ecosystem. Knowledge of the distribution of different ice types to the total Antarctic sea ice cover may also help to shed light on the factors contributing towards recent expansion of the Antarctic ice cover in some regions and contraction in others. The long-term passive microwave satellite data record provides the longest and most consistent data record for assessing different ice types. However, estimates of the amount of MIZ, consolidated pack ice and polynyas depends strongly on what sea ice algorithm is used. This study uses two popular passive microwave sea ice algorithms, the NASA Team and Bootstrap to evaluate the distribution and variability in the MIZ, the consolidated pack ice and coastal polynyas. Results reveal the NASA Team algorithm has on average twice the MIZ and half the consolidated pack ice area as the Bootstrap algorithm. Polynya area is also larger in the NASA Team algorithm, and the timing of maximum polynya area may differ by as much as 5 months between algorithms. These differences lead to different relationships between sea ice characteristics and biological processes, as illustrated here with the breeding success of an Antarctic seabird.

  4. Carbon and hydrogen isotopic systematics of dissolved methane in small seasonally ice-covered lakes near the margin of the Greenland ice sheet

    NASA Astrophysics Data System (ADS)

    Cadieux, S. B.; White, J. R.; Pratt, L. M.; Peng, Y.; Young, S. A.

    2013-12-01

    Northern lakes contribute from 6-16% of annual methane inputs to Earth's atmosphere, yet little is known about the seasonal biogeochemistry of CH4 cycling, particularly for lakes in the Arctic. Studies during ice-free conditions have been conducted in Alaskan, Swedish and Siberian lakes. However, there is little information on CH4 cycling under ice-covered conditions, and few stable isotopic measurements, which can help elucidate production and consumption pathways. In order to better understand methane dynamics of ice-covered Arctic lakes, 4 small lakes (surface area <1 km2) within a narrow valley extending from the Russells Glacier to Søndre Strømfjord in Southwestern Greenland were examined during summer stratification and winter ice-cover. Lakes in the study area are ice-covered from mid-September to mid-June. In both seasons, variations in the concentrations and isotopic composition of methane with depth were related to redox fluctuations. During late winter under~2 m of ice, the entire water column was anoxic with wide variation in methane concentrationsand isotopic composition from lake to lake. In three of the lakes, CH4 concentrations and δ13C were relatively stable over the depth of the water column, averaging from 120 to 480μM, with δ13CH4 values from -56‰ to -66‰, respectively. Methane concentrations in the other lake increased with depth from <1 μM below the ice to 800 μM at the sediment/water interface, while δ13C decreased by 30‰ from -30‰ to -70‰ over this depth. In all the lakes, δ13C of sediment porewater was lighter than the overlying water by at least 10‰. The δD-CH4 in the water column ranged from -370‰ to -50‰, exhibiting covariance with δ13C consistent with significant methanotrophic activity. In the sediment, δD-CH4 values ranged from -330‰ to -275‰, and were inversely correlated with δ13C. We will present detailed information on redox dynamics as a controlling factor in methane cycling, and explore the

  5. Comparative Results of Using Different Methods for Discovery of Microorganisms in very Ancient Layers of the Central Antarctic Glacier above the Lake Vostok

    NASA Technical Reports Server (NTRS)

    Abyzov, S. S.; Hoover, R. B.; Imura, S.; Mitskevich, I. N.; Naganuma, T.; Poglazova, M. N.; Ivanov, M. V.

    2002-01-01

    The ice sheet of the Central Antarctic is considered by the scientific community worldwide, as a model to elaborate on different methods to search for life outside Earth. This became especially significant in connection with the discovery of the underglacial lake in the vicinity of the Russian Antarctic Station Vostok. Lake Vostok is considered by many scientists as an analog of the ice covered seas of Jupiter's satellite Europa. According to the opinion of many researchers there is the possibility that relict forms of microorganisms, well preserved since the Ice Age, may be present in this lake. Investigations throughout the thickness of the ice sheet above Lake Vostok show the presence of microorganisms belonging to different well-known taxonomic groups, even in the very ancient horizons near close to floor of the glacier. Different methods were used to search for microorganisms that are rarely found in the deep ancient layers of an ice sheet. The method of aseptic sampling from the ice cores and the results of controlled sterile conditions in all stages when conducting these investigations, are described in detail in previous reports. Primary investigations tried the usual methods of sowing samples onto different nutrient media, and the result was that only a few microorganisms grew on the media used. The possibility of isolating the organisms obtained for further investigations, by using modern methods including DNA-analysis, appears to be the preferred method. Further investigations of the very ancient layers of the ice sheet by radioisotopic, luminescence, and scanning electron microscopy methods at different modifications, revealed the quantity and morphological diversity of the cells of microorganisms that were distributed on the different horizons. Investigations over many years have shown that the microflora in the very ancient strata of the Antarctic ice cover, nearest to the bedrock, support the effectiveness of using a combination of different methods

  6. Variability of Antarctic Sea Ice 1979-1998

    NASA Technical Reports Server (NTRS)

    Zwally, H. Jay; Comiso, Josefino C.; Parkinson, Claire L.; Cavalieri, Donald J.; Gloersen, Per; Koblinsky, Chester J. (Technical Monitor)

    2001-01-01

    The principal characteristics of the variability of Antarctic sea ice cover as previously described from satellite passive-microwave observations are also evident in a systematically-calibrated and analyzed data set for 20.2 years (1979-1998). The total Antarctic sea ice extent (concentration > 15 %) increased by 13,440 +/- 4180 sq km/year (+1.18 +/- 0.37%/decade). The area of sea ice within the extent boundary increased by 16,960 +/- 3,840 sq km/year (+1.96 +/- 0.44%/decade). Regionally, the trends in extent are positive in the Weddell Sea (1.5 +/- 0.9%/decade), Pacific Ocean (2.4 +/- 1.4%/decade), and Ross (6.9 +/- 1.1 %/decade) sectors, slightly negative in the Indian Ocean (-1.5 +/- 1.8%/decade, and strongly negative in the Bellingshausen-Amundsen Seas sector (-9.5 +/- 1.5%/decade). For the entire ice pack, small ice increases occur in all seasons with the largest increase during autumn. On a regional basis, the trends differ season to season. During summer and fall, the trends are positive or near zero in all sectors except the Bellingshausen-Amundsen Seas sector. During winter and spring, the trends are negative or near zero in all sectors except the Ross Sea, which has positive trends in all seasons. Components of interannual variability with periods of about 3 to 5 years are regionally large, but tend to counterbalance each other in the total ice pack. The interannual variability of the annual mean sea-ice extent is only 1.6% overall, compared to 5% to 9% in each of five regional sectors. Analysis of the relation between regional sea ice extents and spatially-averaged surface temperatures over the ice pack gives an overall sensitivity between winter ice cover and temperature of -0.7% change in sea ice extent per K. For summer, some regional ice extents vary positively with temperature and others negatively. The observed increase in Antarctic sea ice cover is counter to the observed decreases in the Arctic. It is also qualitatively consistent with the

  7. Winter severity determines functional trait composition of phytoplankton in seasonally ice-covered lakes.

    PubMed

    Özkundakci, Deniz; Gsell, Alena S; Hintze, Thomas; Täuscher, Helgard; Adrian, Rita

    2016-01-01

    How climate change will affect the community dynamics and functionality of lake ecosystems during winter is still little understood. This is also true for phytoplankton in seasonally ice-covered temperate lakes which are particularly vulnerable to the presence or absence of ice. We examined changes in pelagic phytoplankton winter community structure in a north temperate lake (Müggelsee, Germany), covering 18 winters between 1995 and 2013. We tested how phytoplankton taxa composition varied along a winter-severity gradient and to what extent winter severity shaped the functional trait composition of overwintering phytoplankton communities using multivariate statistical analyses and a functional trait-based approach. We hypothesized that overwintering phytoplankton communities are dominated by taxa with trait combinations corresponding to the prevailing winter water column conditions, using ice thickness measurements as a winter-severity indicator. Winter severity had little effect on univariate diversity indicators (taxon richness and evenness), but a strong relationship was found between the phytoplankton community structure and winter severity when taxon trait identity was taken into account. Species responses to winter severity were mediated by the key functional traits: motility, nutritional mode, and the ability to form resting stages. Accordingly, one or the other of two functional groups dominated the phytoplankton biomass during mild winters (i.e., thin or no ice cover; phototrophic taxa) or severe winters (i.e., thick ice cover; exclusively motile taxa). Based on predicted milder winters for temperate regions and a reduction in ice-cover durations, phytoplankton communities during winter can be expected to comprise taxa that have a relative advantage when the water column is well mixed (i.e., need not be motile) and light is less limiting (i.e., need not be mixotrophic). A potential implication of this result is that winter severity promotes different

  8. Breakup of Pack Ice, Antarctic Ice Shelf

    NASA Technical Reports Server (NTRS)

    1991-01-01

    Breakup of Pack Ice along the periphery of the Antarctic Ice Shelf (53.5S, 3.0E) produced this mosaic of ice floes off the Antarctic 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

  9. Antarctic subglacial lake exploration: first results and future plans

    PubMed Central

    Siegert, Martin J.; Priscu, John C.; Wadham, Jemma L.; Lyons, W. Berry

    2016-01-01

    After more than a decade of planning, three attempts were made in 2012–2013 to access, measure in situ properties and directly sample subglacial Antarctic lake environments. First, Russian scientists drilled into the top of Lake Vostok, allowing lake water 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 water. Second, UK engineers tried unsuccessfully to deploy a clean-access hot-water drill, to sample the water 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 Antarctic 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

  10. Antarctic subglacial lake exploration: first results and future plans.

    PubMed

    Siegert, Martin J; Priscu, John C; Alekhina, Irina A; Wadham, Jemma L; Lyons, W Berry

    2016-01-28

    After more than a decade of planning, three attempts were made in 2012-2013 to access, measure in situ properties and directly sample subglacial Antarctic lake environments. First, Russian scientists drilled into the top of Lake Vostok, allowing lake water 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 water. Second, UK engineers tried unsuccessfully to deploy a clean-access hot-water drill, to sample the water 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 Antarctic 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).

  11. Turning up the Heat on the Antarctic Ice Sheet (From Below): Challenges and Near-Term Opportunities for Measuring Antarctic Geothermal Fluxes (Invited)

    NASA Astrophysics Data System (ADS)

    Tulaczyk, S. M.; Hossainzadeh, S.

    2010-12-01

    Antarctic heat flow plays an important role in determining the rate of meltwater production at the base of the Antarctic ice sheet. Basal meltwater represents a key control on ice sheet mass balance, Antarctic 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 Antarctic 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 Antarctic 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 Antarctic ice sheet in 2012-13 and 2013-14.

  12. The East Antarctic Ice Sheet and the Gamburtsev Subglacial Mountains (Invited)

    NASA Astrophysics Data System (ADS)

    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.

    2009-12-01

    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 Antarctic Craton. While ice sheet models replicate the formation of the East Antarctic 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 Antarctic 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 water that has

  13. Ross Ice Shelf, Antarctic Ice and Clouds

    NASA Technical Reports Server (NTRS)

    1991-01-01

    In this view of Antarctic 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 Antarctic cyclone. Winds stirred up these storms have been known to reach hurricane force.

  14. The Arctic's sea ice cover: trends, variability, predictability, and comparisons to the Antarctic.

    PubMed

    Serreze, Mark C; Meier, Walter N

    2018-05-28

    As assessed over the period of satellite observations, October 1978 to present, there are downward linear trends in Arctic sea ice extent for all months, largest at the end of the melt season in September. The ice cover is also thinning. Downward trends in extent and thickness have been accompanied by pronounced interannual and multiyear variability, forced by both the atmosphere and ocean. As the ice thins, its response to atmospheric and oceanic forcing may be changing. In support of a busier Arctic, there is a growing need to predict ice conditions on a variety of time and space scales. A major challenge to providing seasonal scale predictions is the 7-10 days limit of numerical weather prediction. While a seasonally ice-free Arctic Ocean is likely well within this century, there is much uncertainty in the timing. This reflects differences in climate model structure, the unknown evolution of anthropogenic forcing, and natural climate variability. In sharp contrast to the Arctic, Antarctic sea ice extent, while highly variable, has increased slightly over the period of satellite observations. The reasons for this different behavior remain to be resolved, but responses to changing atmospheric circulation patterns appear to play a strong role. © 2018 New York Academy of Sciences.

  15. Ice cover extent drives phytoplankton and bacterial community structure in a large north-temperate lake: implications for a warming climate.

    PubMed

    Beall, B F N; Twiss, M R; Smith, D E; Oyserman, B O; Rozmarynowycz, M J; Binding, C E; Bourbonniere, R A; Bullerjahn, G S; Palmer, M E; Reavie, E D; Waters, Lcdr M K; Woityra, Lcdr W C; McKay, R M L

    2016-06-01

    Mid-winter limnological surveys of Lake Erie captured extremes in ice extent ranging from expansive ice cover in 2010 and 2011 to nearly ice-free waters in 2012. Consistent with a warming climate, ice cover on the Great Lakes is in decline, thus the ice-free condition encountered may foreshadow the lakes future winter state. Here, we show that pronounced changes in annual ice cover are accompanied by equally important shifts in phytoplankton and bacterial community structure. Expansive ice cover supported phytoplankton blooms of filamentous diatoms. By comparison, ice free conditions promoted the growth of smaller sized cells that attained lower total biomass. We propose that isothermal mixing and elevated turbidity in the absence of ice cover resulted in light limitation of the phytoplankton during winter. Additional insights into microbial community dynamics were gleaned from short 16S rRNA tag (Itag) Illumina sequencing. UniFrac analysis of Itag sequences showed clear separation of microbial communities related to presence or absence of ice cover. Whereas the ecological implications of the changing bacterial community are unclear at this time, it is likely that the observed shift from a phytoplankton community dominated by filamentous diatoms to smaller cells will have far reaching ecosystem effects including food web disruptions. © 2015 Society for Applied Microbiology and John Wiley & Sons Ltd.

  16. Response of ice cover on shallow Arctic lakes to contemporary climate conditions: Numerical modeling and remote sensing data analysis

    NASA Astrophysics Data System (ADS)

    Duguay, C.; Surdu, C.; Brown, L.; Samuelsson, P.

    2012-04-01

    Lake ice cover has been shown to be a robust indicator of climate variability and change. Recent studies have demonstrated that break-up dates, in particular, have been occurring earlier in many parts of the Northern Hemisphere over the last 50 years in response to warmer climatic conditions in the winter and spring seasons. The impacts of trends in air temperature and winter precipitation over the last five decades and those projected by global climate models will affect the timing and duration of ice cover (and ice thickness) on Arctic lakes. This will likely, in turn, have an important feedback effect on energy, water, and biogeochemical cycling in various regions of the Arctic. In the case of shallow tundra lakes, many of which are less than 3-m deep, warmer climate conditions could result in a smaller fraction of lakes that freeze to their bed in winter since thinner ice covers are expected to develop. Shallow lakes of the coastal plain of northern Alaska, and other similar regions of the Arctic, have likely been experiencing changes in seasonal ice thickness (and phenology) over the last few decades but these have not yet been documented. This paper presents results from a numerical lake ice modeling experiment and the analysis of ERS-1/2 synthetic aperture radar (SAR) data to elucidate the response of ice cover (thickness, freezing to bed, and phenology) on shallow lakes of the North Slope of Alaska (NSA)to climate conditions over the last three decades. New downscaled data specific for the Arctic domain (at a resolution of 0.44 degrees using ERA Interim Reanalysis as boundary condition) produced by the Rossby Centre regional atmospheric model (RCA4) was used to force the Canadian Lake Ice Model (CLIMo) for the period 1979-2010. Output from CLIMo included freeze-up and break-up dates as well as ice thickness on a daily basis. ERS-1/2 data was used to map areas of shallow lakes that freeze to bed and when this happens (timing) in winter for the period 1991

  17. Ice Bridge Antarctic Sea Ice

    NASA Image and Video Library

    2009-10-21

    Sea ice is seen out the window of NASA's DC-8 research aircraft as it flies 2,000 feet above the Bellingshausen Sea in West Antarctica on Wednesday, Oct., 21, 2009. This was the fourth science flight of NASA’s Operation Ice Bridge airborne Earth science mission to study Antarctic ice sheets, sea ice, and ice shelves. Photo Credit: (NASA/Jane Peterson)

  18. Supraglacial lakes on Himalayan debris-covered glacier (Invited)

    NASA Astrophysics Data System (ADS)

    Sakai, A.; Fujita, K.

    2013-12-01

    Debris-covered glaciers are common in many of the world's mountain ranges, including in the Himalayas. Himalayan debris-covered glacier also contain abundant glacial lakes, including both proglacial and supraglacial types. We have revealed that heat absorption through supraglacial lakes was about 7 times greater than that averaged over the whole debris-covered zone. The heat budget analysis elucidated that at least half of the heat absorbed through the water surface was released with water outflow from the lakes, indicating that the warm water enlarge englacial conduits and produce internal ablation. We observed some portions at debris-covered area has caved at the end of melting season, and ice cliff has exposed at the side of depression. Those depression has suggested that roof of expanded water channels has collapsed, leading to the formation of ice cliffs and new lakes, which would accelerate the ablation of debris-covered glaciers. Almost glacial lakes on the debris-covered glacier are partially surrounded by ice cliffs. We observed that relatively small lakes had non-calving, whereas, calving has occurred at supraglacial lakes with fetch larger than 80 m, and those lakes expand rapidly. In the Himalayas, thick sediments at the lake bottom insulates glacier ice and lake water, then the lake water tends to have higher temperature (2-4 degrees C). Therefore, thermal undercutting at ice cliff is important for calving processes in the glacial lake expansion. We estimated and subaqueous ice melt rates during the melt and freeze seasons under simple geomorphologic conditions. In particular, we focused on valley wind-driven water currents in various fetches during the melt season. Our results demonstrate that the subaqueous ice melt rate exceeds the ice-cliff melt rate above the water surface when the fetch is larger than 20 m with the water temperature of 2-4 degrees C. Calculations suggest that onset of calving due to thermal undercutting is controlled by water

  19. Recent advances in understanding Antarctic subglacial lakes and hydrology

    PubMed Central

    Siegert, Martin J.; Ross, Neil; Le Brocq, Anne M.

    2016-01-01

    It is now well documented that over 400 subglacial lakes exist across the bed of the Antarctic Ice Sheet. They comprise a variety of sizes and volumes (from the approx. 250 km long Lake Vostok to bodies of water less than 1 km in length), relate to a number of discrete topographic settings (from those contained within valleys to lakes that reside in broad flat terrain) and exhibit a range of dynamic behaviours (from ‘active’ lakes that periodically outburst some or all of their water to those isolated hydrologically for millions of years). Here we critique recent advances in our understanding of subglacial lakes, in particular since the last inventory in 2012. We show that within 3 years our knowledge of the hydrological processes at the ice-sheet base has advanced considerably. We describe evidence for further ‘active’ subglacial lakes, based on satellite observation of ice-surface changes, and discuss why detection of many ‘active’ lakes is not resolved in traditional radio-echo sounding methods. We go on to review evidence for large-scale subglacial water flow in Antarctica, including the discovery of ancient channels developed by former hydrological processes. We end by predicting areas where future discoveries may be possible, including the detection, measurement and significance of groundwater (i.e. water held beneath the ice-bed interface). PMID:26667914

  20. Recent advances in understanding Antarctic subglacial lakes and hydrology.

    PubMed

    Siegert, Martin J; Ross, Neil; Le Brocq, Anne M

    2016-01-28

    It is now well documented that over 400 subglacial lakes exist across the bed of the Antarctic Ice Sheet. They comprise a variety of sizes and volumes (from the approx. 250 km long Lake Vostok to bodies of water less than 1 km in length), relate to a number of discrete topographic settings (from those contained within valleys to lakes that reside in broad flat terrain) and exhibit a range of dynamic behaviours (from 'active' lakes that periodically outburst some or all of their water to those isolated hydrologically for millions of years). Here we critique recent advances in our understanding of subglacial lakes, in particular since the last inventory in 2012. We show that within 3 years our knowledge of the hydrological processes at the ice-sheet base has advanced considerably. We describe evidence for further 'active' subglacial lakes, based on satellite observation of ice-surface changes, and discuss why detection of many 'active' lakes is not resolved in traditional radio-echo sounding methods. We go on to review evidence for large-scale subglacial water flow in Antarctica, including the discovery of ancient channels developed by former hydrological processes. We end by predicting areas where future discoveries may be possible, including the detection, measurement and significance of groundwater (i.e. water held beneath the ice-bed interface). © 2015 The Authors.

  1. RADARSAT-2 Polarimetry for Lake Ice Mapping

    NASA Astrophysics Data System (ADS)

    Pan, Feng; Kang, Kyung-Kuk; Duguay, Claude

    2016-04-01

    Changes in the ice regime of lakes can be employed to assess long-term climate trends and variability in high latitude regions. Lake ice cover observations are not only useful for climate monitoring, but also for improving ice and weather forecasts using numerical prediction models. In recent years, satellite remote sensing has assumed a greater role in observing lake ice cover for both purposes. Radar remote sensing has become an essential tool for mapping lake ice at high latitudes where cloud cover and polar darkness severely limits ice observations from optical systems. In Canada, there is an emerging interest by government agencies to evaluate the potential of fully polarimetric synthetic aperture radar (SAR) data from RADARSAT-2 (C-band) for lake ice monitoring. In this study, we processed and analyzed the polarization states and scattering mechanisms of fully polarimetric RADARSAT-2 data obtained over Great Bear Lake, Canada, to identify open water and different ice types during the freeze-up and break-up periods. Polarimetric decompositions were employed to separate polarimetric measurements into basic scattering mechanisms. Entropy, anisotropy, and alpha angle were derived to characterize the scattering heterogeneity and mechanisms. Ice classes were then determined based on entropy and alpha angle using the unsupervised Wishart classifier and results evaluated against Landsat 8 imagery. Preliminary results suggest that the RADARSAT-2 polarimetric data offer a strong capability for identifying open water and different lake ice types.

  2. Monitoring Antarctic ice sheet surface melting with TIMESAT algorithm

    NASA Astrophysics Data System (ADS)

    Ye, Y.; Cheng, X.; Li, X.; Liang, L.

    2011-12-01

    Antarctic 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 Antarctic 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, Antarctic 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 Antarctic ice shelf region. It is affected by land cover type, surface elevation and geographic location (latitude). In addition, the Antarctic 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 Antarctic Peninsula

  3. AVHRR imagery reveals Antarctic ice dynamics

    NASA Technical Reports Server (NTRS)

    Bindschadler, Robert A.; Vornberger, Patricia L.

    1990-01-01

    A portion of AVHRR data taken on December 5, 1987 at 06:15 GMT over a part of Antarctica is used here to show that many of the most significant dynamic features of ice sheets can be identified by a careful examination of AVHRR imagery. The relatively low resolution of this instrument makes it ideal for obtaining a broad view of the ice sheets, while its wide swath allows coverage of areas beyond the reach of high-resolution imagers either currently in orbit or planned. An interpretation is given of the present data, which cover the area of ice streams that drain the interior of the West Antarctic ice sheet into the Ross Ice Shelf.

  4. Quantitative calibration of remote mountain lake sediments as climatic recorders of ice-cover duration

    NASA Astrophysics Data System (ADS)

    Thompson, R.; Price, D.

    2003-04-01

    Using a thermal degree modelling approach ice cover duration on European mountain lakes is found to be very sensitive to temperature change. For example our thermal degree model (which incorporates a weather generator) predicts a 100 day shortening in ice-cover duration for a 3 degree Centigrade temperature rise for north facing catchments at elevations of 1200m in the southern Alps, and 1500m in the Pyrenees. 30% higher sensitivities (130d/3oC) are found for the more maritime lakes of Scotland, while lakes in NW Finland, in a more continental setting, have only half the sensitivity (50d/3oC). A pan European data set of the species abundance of 252 diatom taxa in 462 mountain and sub Arctic lakes has been compiled. Taxonomic harmonisation is based on a team effort carried out as an integral part of the AL:PE, CHILL and EMERGE projects. Transfer functions have been created relating ice-cover duration to diatom species composition based on a weighted averaging - partial least squares (WA-PLS) approach. Cross validation was used to test the transfer functions. The pan European data set yields an R-squared of 0.73, an R-squared(jack) of 0.58, and an RMSEP error of 23 days. A regional, northern Scandinavian transect, (151 lakes, 122 taxa) yields an R-squared(jack) of 0.50, and an RMSEP of 9 days. The pan European database displays greatest skill when reconstructing winter or spring temperatures. This contrasts with the summer temperatures normally studied when using local elevation gradients. The northern Scandinavian transect has a remarkably low winter RMSEP of 0.73 oC.

  5. POTENTIAL CLIMATE WARMING EFFECTS ON ICE COVERS OF SMALL LAKES IN THE CONTIGUOUS U.S. (R824801)

    EPA Science Inventory

    Abstract

    To simulate effects of projected climate change on ice covers of small lakes in the northern contiguous U.S., a process-based simulation model is applied. This winter ice/snow cover model is associated with a deterministic, one-dimensional year-round water tem...

  6. Ice Bridge Antarctic Sea Ice

    NASA Image and Video Library

    2009-10-21

    An iceberg is seen out the window of NASA's DC-8 research aircraft as it flies 2,000 feet above the Amundsen Sea in West Antarctica on Wednesday, Oct., 21, 2009. This was the fourth science flight of NASA’s Operation Ice Bridge airborne Earth science mission to study Antarctic ice sheets, sea ice, and ice shelves. Photo Credit: (NASA/Jane Peterson)

  7. Moat Development and Evolution on a Perennialy Ice-Covered Lake in East Antarctica

    NASA Astrophysics Data System (ADS)

    Wayt, M. E.; Myers, K. F.; Doran, P.

    2017-12-01

    Lake Fryxell is a closed basin lake located in the lower end of Taylor Valley in McMurdo Dry Valleys of east Antarctica. The lake has an 4 m thick perennial ice-cover, however during the austral summers an ice-free moat forms around the lake margin due to increased temperatures and stream run off. Satellite imagery paired with ground-based camera data from Lake Fryxell were used to determine onset of moat formation, moat duration, and total area of open water at peak formation from 2009 through 2015. Temperature data from a meteorological station on the shore of Lake Fryxell were used to correlate degree days above freezing (DDAF) with moat formation and extent. The results showed that overall, the moat was smallest in 2009-10, accounting for roughly .61% percent of the surface area of Lake Fryxell. In 2010-11 and 2011-12 moat extent increase by roughly 1% and then decreased by 4% in 2012-13. In 2013-14 the moat was at its largest, accounting for about 11% with a decrease in area of 6% the following summer. Preliminary analysis of temperature data suggest a correlation between DDAF and moat extent. Moats make up on average 9% of lake area and are likely sites of elevated primary productivity in the summer. Moats are ice free which allows for unobstructed photosynthetically active radiation to penetrate the shallow water column. We hypothesize projected increases in air temperatures will lead to continued rise in lake level and larger moat areas, making it critical to understand these delicate and rapidly changing ecosystems.

  8. Observational Evidence of a Hemispheric-wide Ice-ocean Albedo Feedback Effect on Antarctic Sea-ice Decay

    NASA Technical Reports Server (NTRS)

    Nihashi, Sohey; Cavalieri, Donald J.

    2007-01-01

    The effect of ice-ocean albedo feedback (a kind of ice-albedo feedback) on sea-ice decay is demonstrated over the Antarctic sea-ice zone from an analysis of satellite-derived hemispheric sea ice concentration and European Centre for Medium-Range Weather Forecasts (ERA-40) atmospheric data for the period 1979-2001. Sea ice concentration in December (time of most active melt) correlates better with the meridional component of the wind-forced ice drift (MID) in November (beginning of the melt season) than the MID in December. This 1 month lagged correlation is observed in most of the Antarctic sea-ice covered ocean. Daily time series of ice , concentration show that the ice concentration anomaly increases toward the time of maximum sea-ice melt. These findings can be explained by the following positive feedback effect: once ice concentration decreases (increases) at the beginning of the melt season, solar heating of the upper ocean through the increased (decreased) open water fraction is enhanced (reduced), leading to (suppressing) a further decrease in ice concentration by the oceanic heat. Results obtained fi-om a simple ice-ocean coupled model also support our interpretation of the observational results. This positive feedback mechanism explains in part the large interannual variability of the sea-ice cover in summer.

  9. Helium and Neon in the Accreted Ice of the Subglacial Antarctic Lake Vostok

    NASA Astrophysics Data System (ADS)

    Jean-Baptiste, P.; Fourré, E.; Petit, J. R.; Lipenkov, V.; Bulat, S.; Chetverikov, Y.; Raynaud, D.

    2018-05-01

    We analyzed helium and neon in 24 samples from between 3,607 and 3,767 m (i.e., down to 2 m above the lake-ice interface) of the accreted ice frozen to the ceiling of Lake Vostok. Within uncertainties, the neon budget of the lake is balanced, the neon supplied to the lake by the melting of glacier ice being compensated by the neon exported by lake ice. The helium concentration in the lake is about 12 times more than in the glacier ice, with a measured 3He/4He ratio of 0.12 ± 0.01 Ra. This shows that Lake Vostok's waters are enriched by a terrigenic helium source. The 3He/4He isotope ratio of this helium source was determined. Its radiogenic value (0.057 × Ra) is typical of an old continental province, ruling out any magmatic activity associated with the tectonic structure of the lake. It corresponds to a low geothermal heat flow estimated at 51 mW/m2.

  10. Composition and biodegradation of a synthetic oil spilled on the perennial ice cover of Lake Fryxell, Antarctica.

    PubMed

    Jaraula, Caroline M B; Kenig, Fabien; Doran, Peter T; Priscu, John C; Welch, Kathleen A

    2009-04-15

    A helicopter crashed in January 2003 on the 5 m-thick perennial ice cover of Lake Fryxell, spilling synthetic turbine oil Aeroshell 500. Molecular compositions of the oils were analyzed by gas chromatography-mass spectrometry and compared to the composition of contaminants in ice, meltwater, and sediments collected a year after the accident. Aeroshell 500 is based on C20-C33 Pentaerythritol triesters (PET) with C5-C10 fatty acids susbstituents and contain a number of antioxidant additives, such as tricresyl phosphates. Biodegradation of this oil in the ice cover occurs when sediments are present PETs with short fatty acids substituents are preferentially degraded, whereas long chain fatty acids seem to hinder esters from hydrolysis by esterase derived from the microbial assemblage. It remains to be seen if the microbial ecosystem can degrade tricresyl phosphates. These more recalcitrant PET species and tricresyl phosphates are likely to persist and comprise the contaminants that may eventually cross the ice cover to reach the pristine lake water.

  11. Antarctic ice-sheet loss driven by basal melting of ice shelves.

    PubMed

    Pritchard, H D; Ligtenberg, S R M; Fricker, H A; Vaughan, D G; van den Broeke, M R; Padman, L

    2012-04-25

    Accurate prediction of global sea-level rise requires that we understand the cause of recent, widespread and intensifying glacier acceleration along Antarctic 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 Antarctic 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-Antarctic pattern of ice-shelf thinning through increased basal melt. We deduce that this increased melt is the primary control of Antarctic 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 water 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 Antarctic ice shelves, through ocean upwelling in the Amundsen and Bellingshausen seas, and atmospheric warming on the Antarctic Peninsula. This implies that climate forcing through changing winds influences Antarctic ice-sheet mass balance, and hence global sea level, on annual to decadal timescales.

  12. Ice cover, landscape setting, and geological framework of Lake Vostok, East Antarctica

    USGS Publications Warehouse

    Studinger, M.; Bell, R.E.; Karner, G.D.; Tikku, A.A.; Holt, J.W.; Morse, D.L.; David, L.; Richter, T.G.; Kempf, S.D.; Peters, M.E.; Blankenship, D.D.; Sweeney, R.E.; Rystrom, V.L.

    2003-01-01

    Lake Vostok, located beneath more than 4 km of ice in the middle of East Antarctica, is a unique subglacial habitat and may contain microorganisms with distinct adaptations to such an extreme environment. Melting and freezing at the base of the ice sheet, which slowly flows across the lake, controls the flux of water, biota and sediment particles through the lake. The influx of thermal energy, however, is limited to contributions from below. Thus the geological origin of Lake Vostok is a critical boundary condition for the subglacial ecosystem. We present the first comprehensive maps of ice surface, ice thickness and subglacial topography around Lake Vostok. The ice flow across the lake and the landscape setting are closely linked to the geological origin of Lake Vostok. Our data show that Lake Vostok is located along a major geological boundary. Magnetic and gravity data are distinct east and west of the lake, as is the roughness of the subglacial topography. The physiographic setting of the lake has important consequences for the ice flow and thus the melting and freezing pattern and the lake's circulation. Lake Vostok is a tectonically controlled subglacial lake. The tectonic processes provided the space for a unique habitat and recent minor tectonic activity could have the potential to introduce small, but significant amounts of thermal energy into the lake. ?? 2002 Elsevier Science B.V. All rights reserved.

  13. Structural Uncertainty in Antarctic sea ice simulations

    NASA Astrophysics Data System (ADS)

    Schneider, D. P.

    2016-12-01

    The inability of the vast majority of historical climate model simulations to reproduce the observed increase in Antarctic sea ice has motivated many studies about the quality of the observational record, the role of natural variability versus forced changes, and the possibility of missing or inadequate forcings in the models (such as freshwater discharge from thinning ice shelves or an inadequate magnitude of stratospheric ozone depletion). In this presentation I will highlight another source of uncertainty that has received comparatively little attention: Structural uncertainty, that is, the systematic uncertainty in simulated sea ice trends that arises from model physics and mean-state biases. Using two large ensembles of experiments from the Community Earth System Model (CESM), I will show that the model is predisposed towards producing negative Antarctic sea ice trends during 1979-present, and that this outcome is not simply because the model's decadal variability is out-of-synch with that in nature. In the "Tropical Pacific Pacemaker" ensemble, in which observed tropical Pacific SST anomalies are prescribed, the model produces very realistic atmospheric circulation trends over the Southern Ocean, yet the sea ice trend is negative in every ensemble member. However, if the ensemble-mean trend (commonly interpreted as the forced response) is removed, some ensemble members show a sea ice increase that is very similar to the observed. While this results does confirm the important role of natural variability, it also suggests a strong bias in the forced response. I will discuss the reasons for this systematic bias and explore possible remedies. This an important problem to solve because projections of 21st -Century changes in the Antarctic climate system (including ice sheet surface mass balance changes and related changes in the sea level budget) have a strong dependence on the mean state of and changes in the Antarctic sea ice cover. This problem is not unique to

  14. Temperature profile for glacial ice at the South Pole: Implications for life in a nearby subglacial lake

    PubMed Central

    Price, P. Buford; Nagornov, Oleg V.; Bay, Ryan; Chirkin, Dmitry; He, Yudong; Miocinovic, Predrag; Richards, Austin; Woschnagg, Kurt; Koci, Bruce; Zagorodnov, Victor

    2002-01-01

    Airborne radar has detected ≈100 lakes under the Antarctic ice cap, the largest of which is Lake Vostok. International planning is underway to search in Lake Vostok for microbial life that may have evolved in isolation from surface life for millions of years. It is thought, however, that the lakes may be hydraulically interconnected. If so, unsterile drilling would contaminate not just one but many of them. Here we report measurements of temperature vs. depth down to 2,345 m in ice at the South Pole, within 10 km from a subglacial lake seen by airborne radar profiling. We infer a temperature at the 2,810-m deep base of the South Pole ice and at the lake of −9°C, which is 7°C below the pressure-induced melting temperature of freshwater ice. To produce the strong radar signal, the frozen lake must consist of a mix of sediment and ice in a flat bed, formed before permanent Antarctic glaciation. It may, like Siberian and Antarctic permafrost, be rich in microbial life. Because of its hydraulic isolation, proximity to South Pole Station infrastructure, and analog to a Martian polar cap, it is an ideal place to test a sterile drill before risking contamination of Lake Vostok. From the semiempirical expression for strain rate vs. shear stress, we estimate shear vs. depth and show that the IceCube neutrino observatory will be able to map the three-dimensional ice-flow field within a larger volume (0.5 km3) and at lower temperatures (−20°C to −35°C) than has heretofore been possible. PMID:12060731

  15. Response of ice cover on shallow lakes of the North Slope of Alaska to contemporary climate conditions (1950-2011): radar remote-sensing and numerical modeling data analysis

    NASA Astrophysics Data System (ADS)

    Surdu, C. M.; Duguay, C. R.; Brown, L. C.; Fernández Prieto, D.

    2014-01-01

    Air temperature and winter precipitation changes over the last five decades have impacted the timing, duration, and thickness of the ice cover on Arctic lakes as shown by recent studies. In the case of shallow tundra lakes, many of which are less than 3 m deep, warmer climate conditions could result in thinner ice covers and consequently, in a smaller fraction of lakes freezing to their bed in winter. However, these changes have not yet been comprehensively documented. The analysis of a 20 yr time series of European remote sensing satellite ERS-1/2 synthetic aperture radar (SAR) data and a numerical lake ice model were employed to determine the response of ice cover (thickness, freezing to the bed, and phenology) on shallow lakes of the North Slope of Alaska (NSA) to climate conditions over the last six decades. Given the large area covered by these lakes, changes in the regional climate and weather are related to regime shifts in the ice cover of the lakes. Analysis of available SAR data from 1991 to 2011, from a sub-region of the NSA near Barrow, shows a reduction in the fraction of lakes that freeze to the bed in late winter. This finding is in good agreement with the decrease in ice thickness simulated with the Canadian Lake Ice Model (CLIMo), a lower fraction of lakes frozen to the bed corresponding to a thinner ice cover. Observed changes of the ice cover show a trend toward increasing floating ice fractions from 1991 to 2011, with the greatest change occurring in April, when the grounded ice fraction declined by 22% (α = 0.01). Model results indicate a trend toward thinner ice covers by 18-22 cm (no-snow and 53% snow depth scenarios, α = 0.01) during the 1991-2011 period and by 21-38 cm (α = 0.001) from 1950 to 2011. The longer trend analysis (1950-2011) also shows a decrease in the ice cover duration by ~24 days consequent to later freeze-up dates by 5.9 days (α = 0.1) and earlier break-up dates by 17.7-18.6 days (α = 0.001).

  16. Rapid glass sponge expansion after climate-induced Antarctic ice shelf collapse.

    PubMed

    Fillinger, Laura; Janussen, Dorte; Lundälv, Tomas; Richter, Claudio

    2013-07-22

    Over 30% of the Antarctic 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 Antarctic 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 Antarctic 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 Antarctic 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 Antarctic glass sponges remain enigmatic. Copyright © 2013 Elsevier Ltd. All rights reserved.

  17. Climate change drives expansion of Antarctic ice-free habitat

    NASA Astrophysics Data System (ADS)

    Lee, Jasmine R.; Raymond, Ben; Bracegirdle, Thomas J.; Chadès, Iadine; Fuller, Richard A.; Shaw, Justine D.; Terauds, Aleks

    2017-07-01

    Antarctic terrestrial biodiversity occurs almost exclusively in ice-free areas that cover less than 1% of the continent. Climate change will alter the extent and configuration of ice-free areas, yet the distribution and severity of these effects remain unclear. Here we quantify the impact of twenty-first century climate change on ice-free areas under two Intergovernmental Panel on Climate Change (IPCC) climate forcing scenarios using temperature-index melt modelling. Under the strongest forcing scenario, ice-free areas could expand by over 17,000 km2 by the end of the century, close to a 25% increase. Most of this expansion will occur in the Antarctic Peninsula, where a threefold increase in ice-free area could drastically change the availability and connectivity of biodiversity habitat. Isolated ice-free areas will coalesce, and while the effects on biodiversity are uncertain, we hypothesize that they could eventually lead to increasing regional-scale biotic homogenization, the extinction of less-competitive species and the spread of invasive species.

  18. Climate change drives expansion of Antarctic ice-free habitat.

    PubMed

    Lee, Jasmine R; Raymond, Ben; Bracegirdle, Thomas J; Chadès, Iadine; Fuller, Richard A; Shaw, Justine D; Terauds, Aleks

    2017-07-06

    Antarctic terrestrial biodiversity occurs almost exclusively in ice-free areas that cover less than 1% of the continent. Climate change will alter the extent and configuration of ice-free areas, yet the distribution and severity of these effects remain unclear. Here we quantify the impact of twenty-first century climate change on ice-free areas under two Intergovernmental Panel on Climate Change (IPCC) climate forcing scenarios using temperature-index melt modelling. Under the strongest forcing scenario, ice-free areas could expand by over 17,000 km 2 by the end of the century, close to a 25% increase. Most of this expansion will occur in the Antarctic Peninsula, where a threefold increase in ice-free area could drastically change the availability and connectivity of biodiversity habitat. Isolated ice-free areas will coalesce, and while the effects on biodiversity are uncertain, we hypothesize that they could eventually lead to increasing regional-scale biotic homogenization, the extinction of less-competitive species and the spread of invasive species.

  19. Variability in sea ice cover and climate elicit sex specific responses in an Antarctic predator

    PubMed Central

    Labrousse, Sara; Sallée, Jean-Baptiste; Fraser, Alexander D.; Massom, Rob A.; Reid, Phillip; Hobbs, William; Guinet, Christophe; Harcourt, Robert; McMahon, Clive; Authier, Matthieu; Bailleul, Frédéric; Hindell, Mark A.; Charrassin, Jean-Benoit

    2017-01-01

    Contrasting regional changes in Southern Ocean sea ice have occurred over the last 30 years with distinct regional effects on ecosystem structure and function. Quantifying how Antarctic predators respond to such changes provides the context for predicting how climate variability/change will affect these assemblages into the future. Over an 11-year time-series, we examine how inter-annual variability in sea ice concentration and advance affect the foraging behaviour of a top Antarctic predator, the southern elephant seal. Females foraged longer in pack ice in years with greatest sea ice concentration and earliest sea ice advance, while males foraged longer in polynyas in years of lowest sea ice concentration. There was a positive relationship between near-surface meridional wind anomalies and female foraging effort, but not for males. This study reveals the complexities of foraging responses to climate forcing by a poleward migratory predator through varying sea ice property and dynamic anomalies. PMID:28233791

  20. Variability in sea ice cover and climate elicit sex specific responses in an Antarctic predator.

    PubMed

    Labrousse, Sara; Sallée, Jean-Baptiste; Fraser, Alexander D; Massom, Rob A; Reid, Phillip; Hobbs, William; Guinet, Christophe; Harcourt, Robert; McMahon, Clive; Authier, Matthieu; Bailleul, Frédéric; Hindell, Mark A; Charrassin, Jean-Benoit

    2017-02-24

    Contrasting regional changes in Southern Ocean sea ice have occurred over the last 30 years with distinct regional effects on ecosystem structure and function. Quantifying how Antarctic predators respond to such changes provides the context for predicting how climate variability/change will affect these assemblages into the future. Over an 11-year time-series, we examine how inter-annual variability in sea ice concentration and advance affect the foraging behaviour of a top Antarctic predator, the southern elephant seal. Females foraged longer in pack ice in years with greatest sea ice concentration and earliest sea ice advance, while males foraged longer in polynyas in years of lowest sea ice concentration. There was a positive relationship between near-surface meridional wind anomalies and female foraging effort, but not for males. This study reveals the complexities of foraging responses to climate forcing by a poleward migratory predator through varying sea ice property and dynamic anomalies.

  1. 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 waters between Hobart, Tasmania, and Antarctica. The vessel serves as the main lifeline to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016TCry...10.1823S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016TCry...10.1823S"><span>Mapping and assessing variability in the <span class="hlt">Antarctic</span> marginal <span class="hlt">ice</span> zone, pack <span class="hlt">ice</span> and coastal polynyas in two sea <span class="hlt">ice</span> algorithms with implications on breeding success of snow petrels</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stroeve, Julienne C.; Jenouvrier, Stephanie; Campbell, G. Garrett; Barbraud, Christophe; Delord, Karine</p> <p>2016-08-01</p> <p>Sea <span class="hlt">ice</span> variability within the marginal <span class="hlt">ice</span> zone (MIZ) and polynyas plays an important role for phytoplankton productivity and krill abundance. Therefore, mapping their spatial extent as well as seasonal and interannual variability is essential for understanding how current and future changes in these biologically active regions may impact the <span class="hlt">Antarctic</span> marine ecosystem. Knowledge of the distribution of MIZ, consolidated pack <span class="hlt">ice</span> and coastal polynyas in the total <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> <span class="hlt">cover</span> may also help to shed light on the factors contributing towards recent expansion of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> <span class="hlt">cover</span> in some regions and contraction in others. The long-term passive microwave satellite data record provides the longest and most consistent record for assessing the proportion of the sea <span class="hlt">ice</span> <span class="hlt">cover</span> that is <span class="hlt">covered</span> by each of these <span class="hlt">ice</span> categories. However, estimates of the amount of MIZ, consolidated pack <span class="hlt">ice</span> and polynyas depend strongly on which sea <span class="hlt">ice</span> algorithm is used. This study uses two popular passive microwave sea <span class="hlt">ice</span> algorithms, the NASA Team and Bootstrap, and applies the same thresholds to the sea <span class="hlt">ice</span> concentrations to evaluate the distribution and variability in the MIZ, the consolidated pack <span class="hlt">ice</span> and coastal polynyas. Results reveal that the seasonal cycle in the MIZ and pack <span class="hlt">ice</span> is generally similar between both algorithms, yet the NASA Team algorithm has on average twice the MIZ and half the consolidated pack <span class="hlt">ice</span> area as the Bootstrap algorithm. Trends also differ, with the Bootstrap algorithm suggesting statistically significant trends towards increased pack <span class="hlt">ice</span> area and no statistically significant trends in the MIZ. The NASA Team algorithm on the other hand indicates statistically significant positive trends in the MIZ during spring. Potential coastal polynya area and amount of broken <span class="hlt">ice</span> within the consolidated <span class="hlt">ice</span> pack are also larger in the NASA Team algorithm. The timing of maximum polynya area may differ by as much as 5 months between algorithms. These</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20160013301&hterms=sea&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dsea','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20160013301&hterms=sea&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dsea"><span>Assessment of Arctic and <span class="hlt">Antarctic</span> Sea <span class="hlt">Ice</span> Predictability in CMIP5 Decadal Hindcasts</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Yang, Chao-Yuan; Liu, Jiping (Inventor); Hu, Yongyun; Horton, Radley M.; Chen, Liqi; Cheng, Xiao</p> <p>2016-01-01</p> <p>This paper examines the ability of coupled global climate models to predict decadal variability of Arctic and <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span>. We analyze decadal hindcasts/predictions of 11 Coupled Model Intercomparison Project Phase 5 (CMIP5) models. Decadal hindcasts exhibit a large multimodel spread in the simulated sea <span class="hlt">ice</span> extent, with some models deviating significantly from the observations as the predicted <span class="hlt">ice</span> extent quickly drifts away from the initial constraint. The anomaly correlation analysis between the decadal hindcast and observed sea <span class="hlt">ice</span> suggests that in the Arctic, for most models, the areas showing significant predictive skill become broader associated with increasing lead times. This area expansion is largely because nearly all the models are capable of predicting the observed decreasing Arctic sea <span class="hlt">ice</span> <span class="hlt">cover</span>. Sea <span class="hlt">ice</span> extent in the North Pacific has better predictive skill than that in the North Atlantic (particularly at a lead time of 3-7 years), but there is a reemerging predictive skill in the North Atlantic at a lead time of 6-8 years. In contrast to the Arctic, <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> decadal hindcasts do not show broad predictive skill at any timescales, and there is no obvious improvement linking the areal extent of significant predictive skill to lead time increase. This might be because nearly all the models predict a retreating <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> <span class="hlt">cover</span>, opposite to the observations. For the Arctic, the predictive skill of the multi-model ensemble mean outperforms most models and the persistence prediction at longer timescales, which is not the case for the <span class="hlt">Antarctic</span>. Overall, for the Arctic, initialized decadal hindcasts show improved predictive skill compared to uninitialized simulations, although this improvement is not present in the <span class="hlt">Antarctic</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1366350','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1366350"><span>West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet cloud <span class="hlt">cover</span> and surface radiation budget from NASA A-Train satellites</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>Scott, Ryan C.; Lubin, Dan; Vogelmann, Andrew M.</p> <p></p> <p>Clouds are an essential parameter of the surface energy budget influencing the West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet (WAIS) response to atmospheric warming and net contribution to global sea-level rise. A four-year record of NASA A-Train cloud observations is combined with surface radiation measurements to quantify the WAIS radiation budget and constrain the three-dimensional occurrence frequency, thermodynamic phase partitioning, and surface radiative effect of clouds over West Antarctica (WA). The skill of satellite-modeled radiative fluxes is confirmed through evaluation against measurements at four <span class="hlt">Antarctic</span> sites (WAIS Divide <span class="hlt">Ice</span> Camp, Neumayer, Syowa, and Concordia Stations). And due to perennial high-albedo snow and icemore » <span class="hlt">cover</span>, cloud infrared emission dominates over cloud solar reflection/absorption leading to a positive net all-wave cloud radiative effect (CRE) at the surface, with all monthly means and 99.15% of instantaneous CRE values exceeding zero. The annual-mean CRE at theWAIS surface is 34 W m -2, representing a significant cloud-induced warming of the <span class="hlt">ice</span> sheet. Low-level liquid-containing clouds, including thin liquid water clouds implicated in radiative contributions to surface melting, are widespread and most frequent in WA during the austral summer. Clouds warm the WAIS by 26 W m -2, in summer, on average, despite maximum offsetting shortwave CRE. Glaciated cloud systems are strongly linked to orographic forcing, with maximum incidence on the WAIS continuing downstream along the Transantarctic Mountains.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1366350-west-antarctic-ice-sheet-cloud-cover-surface-radiation-budget-from-nasa-train-satellites','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1366350-west-antarctic-ice-sheet-cloud-cover-surface-radiation-budget-from-nasa-train-satellites"><span>West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet cloud <span class="hlt">cover</span> and surface radiation budget from NASA A-Train satellites</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Scott, Ryan C.; Lubin, Dan; Vogelmann, Andrew M.; ...</p> <p>2017-04-26</p> <p>Clouds are an essential parameter of the surface energy budget influencing the West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet (WAIS) response to atmospheric warming and net contribution to global sea-level rise. A four-year record of NASA A-Train cloud observations is combined with surface radiation measurements to quantify the WAIS radiation budget and constrain the three-dimensional occurrence frequency, thermodynamic phase partitioning, and surface radiative effect of clouds over West Antarctica (WA). The skill of satellite-modeled radiative fluxes is confirmed through evaluation against measurements at four <span class="hlt">Antarctic</span> sites (WAIS Divide <span class="hlt">Ice</span> Camp, Neumayer, Syowa, and Concordia Stations). And due to perennial high-albedo snow and icemore » <span class="hlt">cover</span>, cloud infrared emission dominates over cloud solar reflection/absorption leading to a positive net all-wave cloud radiative effect (CRE) at the surface, with all monthly means and 99.15% of instantaneous CRE values exceeding zero. The annual-mean CRE at theWAIS surface is 34 W m -2, representing a significant cloud-induced warming of the <span class="hlt">ice</span> sheet. Low-level liquid-containing clouds, including thin liquid water clouds implicated in radiative contributions to surface melting, are widespread and most frequent in WA during the austral summer. Clouds warm the WAIS by 26 W m -2, in summer, on average, despite maximum offsetting shortwave CRE. Glaciated cloud systems are strongly linked to orographic forcing, with maximum incidence on the WAIS continuing downstream along the Transantarctic Mountains.« less</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> <span class="hlt">Ice</span> 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 <span class="hlt">Ice</span> sheet, far less is known about the response of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet. Here, I present the summarised results of my PhD thesis "Constraints on the minimum extent of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet during the last interglaciation". Firstly, I <span class="hlt">cover</span> 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 <span class="hlt">cover</span> climate forcings, and how they influence the <span class="hlt">ice</span> sheet, relative to present, and early Holocene. Secondly, I present thesis results, from looking at <span class="hlt">ice</span> core stable water isotopes. These are compared with Isostatic and Climatic modelling results, for various different <span class="hlt">Ice</span> sheet scenarios, as to the resulting Climate, from changes in Elevation, Temperature, Precipitation, and Sublimation, all contributing to the recorded stable water 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> <span class="hlt">Ice</span> 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> <span class="hlt">Ice</span> sheet. Model uncertainty is unable to constrain evidence of variations in <span class="hlt">ice</span> thickness in East Antarctica.</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-<span class="hlt">ice</span> 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-<span class="hlt">ice</span> habitat was investigated in the Lazarev Sea (Southern Ocean) during austral summer, autumn and winter. Data were obtained using novel Surface and Under <span class="hlt">Ice</span> Trawls (SUIT), which sampled the 0-2 m surface layer both under sea <span class="hlt">ice</span> and in open water. 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-<span class="hlt">ice</span> densities of <span class="hlt">Antarctic</span> krill were significantly higher than in open waters. In autumn, the opposite pattern was observed. Under winter sea <span class="hlt">ice</span>, 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 <span class="hlt">ice</span> coverage and shallow mixed layer depths, among other factors. In autumn and winter, density was related to hydrographical parameters. Average under-<span class="hlt">ice</span> 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-<span class="hlt">ice</span> densities far surpassed maximum 0-200 m densities on several occasions. This indicates that the importance of the <span class="hlt">ice</span>-water 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-<span class="hlt">ice</span> habitat, hundreds of kilometres into the <span class="hlt">ice-covered</span> area of the Lazarev Sea. Local concentrations of postlarval <span class="hlt">Antarctic</span> krill under winter sea <span class="hlt">ice</span> suggest that sea <span class="hlt">ice</span> biota are important for their winter survival. These findings emphasise the susceptibility of an ecological key species to changing sea <span class="hlt">ice</span> 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-<span class="hlt">Ice</span> 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-<span class="hlt">ice</span> habitat was investigated in the Lazarev Sea (Southern Ocean) during austral summer, autumn and winter. Data were obtained using novel Surface and Under <span class="hlt">Ice</span> Trawls (SUIT), which sampled the 0–2 m surface layer both under sea <span class="hlt">ice</span> and in open water. 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-<span class="hlt">ice</span> densities of <span class="hlt">Antarctic</span> krill were significantly higher than in open waters. In autumn, the opposite pattern was observed. Under winter sea <span class="hlt">ice</span>, 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 <span class="hlt">ice</span> coverage and shallow mixed layer depths, among other factors. In autumn and winter, density was related to hydrographical parameters. Average under-<span class="hlt">ice</span> 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-<span class="hlt">ice</span> densities far surpassed maximum 0–200 m densities on several occasions. This indicates that the importance of the <span class="hlt">ice</span>-water 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-<span class="hlt">ice</span> habitat, hundreds of kilometres into the <span class="hlt">ice-covered</span> area of the Lazarev Sea. Local concentrations of postlarval <span class="hlt">Antarctic</span> krill under winter sea <span class="hlt">ice</span> suggest that sea <span class="hlt">ice</span> biota are important for their winter survival. These findings emphasise the susceptibility of an ecological key species to changing sea <span class="hlt">ice</span> habitats, suggesting potential ramifications on <span class="hlt">Antarctic</span> ecosystems induced by climate</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20601510','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20601510"><span>Proteorhodopsin-bearing bacteria in <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Koh, Eileen Y; Atamna-Ismaeel, Nof; Martin, Andrew; Cowie, Rebecca O M; Beja, Oded; Davy, Simon K; Maas, Elizabeth W; Ryan, Ken G</p> <p>2010-09-01</p> <p>Proteorhodopsins (PRs) are widespread bacterial integral membrane proteins that function as light-driven proton pumps. <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> supports a complex community of autotrophic algae, heterotrophic bacteria, viruses, and protists that are an important food source for higher trophic levels in <span class="hlt">ice-covered</span> regions of the Southern Ocean. Here, we present the first report of PR-bearing bacteria, both dormant and active, in <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> from a series of sites in the Ross Sea using gene-specific primers. Positive PR sequences were generated from genomic DNA at all depths in sea <span class="hlt">ice</span>, and these sequences aligned with the classes Alphaproteobacteria, Gammaproteobacteria, and Flavobacteria. The sequences showed some similarity to previously reported PR sequences, although most of the sequences were generally distinct. Positive PR sequences were also observed from cDNA reverse transcribed from RNA isolated from sea <span class="hlt">ice</span> samples. This finding indicates that these sequences were generated from metabolically active cells and suggests that the PR gene is functional within sea <span class="hlt">ice</span>. Both blue-absorbing and green-absorbing forms of PRs were detected, and only a limited number of blue-absorbing forms were found and were in the midsection of the sea <span class="hlt">ice</span> profile in this study. Questions still remain regarding the protein's ecological functions, and ultimately, field experiments will be needed to establish the ecological and functional role of PRs in the sea <span class="hlt">ice</span> ecosystem.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70020155','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70020155"><span>Diatoms in sediments of perennially <span class="hlt">ice-covered</span> <span class="hlt">Lake</span> Hoare, and implications for interpreting <span class="hlt">lake</span> history in the McMurdo Dry Valleys of Antarctica</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Spaulding, S.A.; McKnight, Diane M.; Stoermer, E.F.; Doran, P.T.</p> <p>1997-01-01</p> <p>Diatom assemblages in surficial sediments, sediment cores, sediment traps, and inflowing streams of perennially <span class="hlt">ice-covered</span> <span class="hlt">Lake</span> Hore, South Victorialand, Antarctica were examined to determine the distribution of diatom taxa, and to ascertain if diatom species composition has changed over time. <span class="hlt">Lake</span> Hoare is a closed-basin <span class="hlt">lake</span> with an area of 1.8 km2, maximum depth of 34 m, and mean depth of 14 m, although <span class="hlt">lake</span> level has been rising at a rate of 0.09 m yr-1 in recent decades. The <span class="hlt">lake</span> has an unusual regime of sediment deposition: coarse grained sediments accumulate on the <span class="hlt">ice</span> surface and are deposited episodically on the <span class="hlt">lake</span> bottom. Benthic microbial mats are <span class="hlt">covered</span> in situ by the coarse episodic deposits, and the new surfaces are recolonized. <span class="hlt">Ice</span> <span class="hlt">cover</span> prevents wind-induced mixing, creating the unique depositional environment in which sediment cores record the history of a particular site, rather than a <span class="hlt">lake</span>=wide integration. Shallow-water (<1 m) diatom assemblages (Stauroneis anceps, Navicula molesta, Diadesmis contenta var. parallela, Navicula peraustralis) were distinct from mid-depth (4-16 m) assemblages (Diadesmis contenta, Luticola muticopsis fo. reducta, Stauroneis anceps, Diadesmis contenta var. parallela, Luticola murrayi) and deep-water (2-31 m) assemblages (Luticola murrayi, Luticola muticopsis fo. reducta, Navicula molesta. Analysis of a sediment core (30 cm long, from 11 m water depth) from <span class="hlt">Lake</span> Hoare revealed two abrupt changes in diatom assemblages. The upper section of the sediment core contained the greatest biomass of benthic microbial mat, as well as the greatest total abundance and diversity of diatoms. Relative abundances of diatoms in this section are similar to the surficial samples from mid-depths. An intermediate zone contained less organic material and lower densities of diatoms. The bottom section of core contained the least amount of microbial mat and organic material, and the lowest density of diatoms. The dominant process</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004AGUFM.B31A0201C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004AGUFM.B31A0201C"><span>Microbiological and Biogeochemical Investigations of the Accreted <span class="hlt">Ice</span> Above Subglacial <span class="hlt">Lake</span> Vostok, Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Christner, B. C.; Foreman, C. F.; Arnold, B. R.; Welch, K. A.; Lyons, W. B.; Priscu, J. C.</p> <p>2004-12-01</p> <p>Subglacial <span class="hlt">Lake</span> Vostok is located ~4 km beneath the surface of the East <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet and has been isolated from the atmosphere for at least 15 million years. The <span class="hlt">lake</span> has a surface area near 14,000 km2 and a depth exceeding 1000 m. While the nature of the environment within Subglacial <span class="hlt">Lake</span> Vostok remains uncertain, if a sustained microbial ecosystem is present, life in this subsurface environment operates under arguably the most extreme conditions in the biosphere (i.e., high pressure, constant cold, high oxygen concentrations, and no light). The <span class="hlt">lake</span> represents an analogue for ecosystems that may exist in Europa's <span class="hlt">ice-covered</span> ocean and also provides an Earthly-based model for the evaluation of technology to search for life in icy extraterrestrial subsurface environments. Concerns for environmental protection have prevented direct sampling of the <span class="hlt">lake</span> water thus far, as a prudent sampling plan that will not contaminate this pristine environment has yet to be developed and tested. However, an <span class="hlt">ice</span> core has been retrieved at Vostok Station in which the bottom ~85 meters consists of <span class="hlt">lake</span> water that has accreted to the bottom of the <span class="hlt">ice</span> sheet, providing frozen samples of water from the <span class="hlt">lakes</span>' surface. The <span class="hlt">ice</span> from 3539 to 3609 mbs (accretion <span class="hlt">ice</span> I) contains visible inclusions due to accretion in the shallow embayment or western grounding line, whereas <span class="hlt">ice</span> from 3610-3623 mbs (accretion <span class="hlt">ice</span> II) is very clean, forming above the deep eastern basin of the main <span class="hlt">lake</span>. Using a multifaceted protocol to monitor cellular and molecular decontamination of <span class="hlt">ice</span> cores, we show that the microbiology and geochemistry (i.e., dissolve organic carbon, nutrients, and ions) of accretion <span class="hlt">ice</span> is very different from the overlying glacial <span class="hlt">ice</span>. The numbers of cells are 2- to 7-fold higher in accretion <span class="hlt">ice</span> I than in the overlying glacial <span class="hlt">ice</span>, and decrease with increasing depth in accretion <span class="hlt">ice</span> II. Cell viability in accretion <span class="hlt">ice</span> samples has been confirmed by the measurable respiration of 14C</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013TCD.....7.3783S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013TCD.....7.3783S"><span>Response of <span class="hlt">ice</span> <span class="hlt">cover</span> on shallow <span class="hlt">lakes</span> of the North Slope of Alaska to contemporary climate conditions (1950-2011): radar remote sensing and numerical modeling data analysis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Surdu, C. M.; Duguay, C. R.; Brown, L. C.; Fernández Prieto, D.</p> <p>2013-07-01</p> <p>Air temperature and winter precipitation changes over the last five decades have impacted the timing, duration, and thickness of the <span class="hlt">ice</span> <span class="hlt">cover</span> on Arctic <span class="hlt">lakes</span> as shown by recent studies. In the case of shallow tundra <span class="hlt">lakes</span>, many of which are less than 3 m deep, warmer climate conditions could result in thinner <span class="hlt">ice</span> <span class="hlt">covers</span> and consequently, to a smaller fraction of <span class="hlt">lakes</span> freezing to their bed in winter. However, these changes have not yet been comprehensively documented. The analysis of a 20 yr time series of ERS-1/2 synthetic aperture radar (SAR) data and a numerical <span class="hlt">lake</span> <span class="hlt">ice</span> model were employed to determine the response of <span class="hlt">ice</span> <span class="hlt">cover</span> (thickness, freezing to the bed, and phenology) on shallow <span class="hlt">lakes</span> of the North Slope of Alaska (NSA) to climate conditions over the last six decades. Analysis of available SAR data from 1991-2011, from a sub-region of the NSA near Barrow, shows a reduction in the fraction of <span class="hlt">lakes</span> that freeze to the bed in late winter. This finding is in good agreement with the decrease in <span class="hlt">ice</span> thickness simulated with the Canadian <span class="hlt">Lake</span> <span class="hlt">Ice</span> Model (CLIMo), a lower fraction of <span class="hlt">lakes</span> frozen to the bed corresponding to a thinner <span class="hlt">ice</span> <span class="hlt">cover</span>. Observed changes of the <span class="hlt">ice</span> <span class="hlt">cover</span> show a trend toward increasing floating <span class="hlt">ice</span> fractions from 1991 to 2011, with the greatest change occurring in April, when the grounded <span class="hlt">ice</span> fraction declined by 22% (α = 0.01). Model results indicate a trend toward thinner <span class="hlt">ice</span> <span class="hlt">covers</span> by 18-22 cm (no-snow and 53% snow depth scenarios, α = 0.01) during the 1991-2011 period and by 21-38 cm (α = 0.001) from 1950-2011. The longer trend analysis (1950-2011) also shows a decrease in the <span class="hlt">ice</span> <span class="hlt">cover</span> duration by ∼24 days consequent to later freeze-up dates by 5.9 days (α = 0.1) and earlier break-up dates by 17.7-18.6 days (α = 0.001).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70170886','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70170886"><span>Climate regulates alpine <span class="hlt">lake</span> <span class="hlt">ice</span> <span class="hlt">cover</span> phenology and aquatic ecosystem structure</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Preston, Daniel L.; Caine, Nel; McKnight, Diane M.; Williams, Mark W.; Hell, Katherina; Miller, Matthew P.; Hart, Sarah J.; Johnson, Pieter T.J.</p> <p>2016-01-01</p> <p>High-elevation aquatic ecosystems are highly vulnerable to climate change, yet relatively few records are available to characterize shifts in ecosystem structure or their underlying mechanisms. Using a long-term dataset on seven alpine <span class="hlt">lakes</span> (3126 to 3620 m) in Colorado, USA, we show that <span class="hlt">ice</span>-off dates have shifted seven days earlier over the past 33 years and that spring weather conditions – especially snowfall – drive yearly variation in <span class="hlt">ice</span>-off timing. In the most well-studied <span class="hlt">lake</span>, earlier <span class="hlt">ice</span>-off associated with increases in water residence times, thermal stratification, ion concentrations, dissolved nitrogen, pH, and chlorophyll-a. Mechanistically, low spring snowfall and warm temperatures reduce summer stream flow (increasing <span class="hlt">lake</span> residence times) but enhance melting of glacial and permafrost <span class="hlt">ice</span> (increasing <span class="hlt">lake</span> solute inputs). The observed links among hydrological, chemical, and biological responses to climate factors highlight the potential for major shifts in the functioning of alpine <span class="hlt">lakes</span> due to forecasted climate change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018OcMod.121...76M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018OcMod.121...76M"><span>Impact of increasing <span class="hlt">antarctic</span> glacial freshwater release on regional sea-<span class="hlt">ice</span> <span class="hlt">cover</span> 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>Merino, Nacho; Jourdain, Nicolas C.; Le Sommer, Julien; Goosse, Hugues; Mathiot, Pierre; Durand, Gael</p> <p>2018-01-01</p> <p>The sensitivity of <span class="hlt">Antarctic</span> sea-<span class="hlt">ice</span> to increasing glacial freshwater release into the Southern Ocean is studied in a series of 31-year ocean/sea-<span class="hlt">ice</span>/iceberg model simulations. Glaciological estimates of <span class="hlt">ice</span>-shelf melting and iceberg calving are used to better constrain the spatial distribution and magnitude of freshwater forcing around Antarctica. Two scenarios of glacial freshwater forcing have been designed to account for a decadal perturbation in glacial freshwater release to the Southern Ocean. For the first time, this perturbation explicitly takes into consideration the spatial distribution of changes in the volume of <span class="hlt">Antarctic</span> <span class="hlt">ice</span> shelves, which is found to be a key component of changes in freshwater release. In addition, glacial freshwater-induced changes in sea <span class="hlt">ice</span> are compared to typical changes induced by the decadal evolution of atmospheric states. Our results show that, in general, the increase in glacial freshwater release increases <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> extent. But the response is opposite in some regions like the coastal Amundsen Sea, implying that distinct physical mechanisms are involved in the response. We also show that changes in freshwater forcing may induce large changes in sea-<span class="hlt">ice</span> thickness, explaining about one half of the total change due to the combination of atmospheric and freshwater changes. The regional contrasts in our results suggest a need for improving the representation of freshwater sources and their evolution in climate models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004AGUFM.C24A..02K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004AGUFM.C24A..02K"><span>Sublgacial <span class="hlt">Antarctic</span> <span class="hlt">Lake</span> Environments (SALE)</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.; Bell, R. E.; Priscu, J. C.</p> <p>2004-12-01</p> <p>Subglacial <span class="hlt">Antarctic</span> <span class="hlt">lake</span> environments are emerging as one of the new frontiers targeted for exploration during the IPY 2007-2009. Several campaigns by various nations are in the early stages of planning and implementation with timelines that will coincide with the IPY. The ambitious interdisciplinary objectives will best be realized by multiple exploration programs investigating diverse subglacial environments continent-wide over the next decade or more. A concerted, multi-target approach wil be taken to advance our understanding of the range of possible <span class="hlt">lake</span> evolutionary histories; the character of the physical, chemical, and biological niches; the interconnectivity of subglacial <span class="hlt">lake</span> environments; the coupling of the <span class="hlt">ice</span> sheet, climate and the evolution of life under the <span class="hlt">ice</span>; the tectonic settings; and the interplay of biogeochemical cycles. Research and exploration programs spanning the continent will investigate subglacial <span class="hlt">lake</span> environments of differing ages, evolutionary histories, and biogeochemical settings. The combined efforts will provide a holistic view of these environments over millions of years and under changing climatic conditions. The IPY will provide an opportunity for an intense period of initial exploration that will advance scientific discoveries in glaciology, biogeochemistry, paleoclimate, biology, geology and tectonics, and ecology. While early discoveries and exciting findings are expected during the IPY 2007-2009, a long term sustained program of research and exploration will continue far beyond the IPY. Within the five year period that spans the IPY, specific accomplishments will be targeted, accelerating the research agenda and setting a framework for follow-on studies. Four phases of exploration and discovery are envisioned.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ERL....12h4010L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ERL....12h4010L"><span>Improved simulation of <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> due to the radiative effects of falling snow</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, J.-L. F.; Richardson, Mark; Hong, Yulan; Lee, Wei-Liang; Wang, Yi-Hui; Yu, Jia-Yuh; Fetzer, Eric; Stephens, Graeme; Liu, Yinghui</p> <p>2017-08-01</p> <p>Southern Ocean sea-<span class="hlt">ice</span> <span class="hlt">cover</span> exerts critical control on local albedo and <span class="hlt">Antarctic</span> precipitation, but simulated <span class="hlt">Antarctic</span> sea-<span class="hlt">ice</span> concentration commonly disagrees with observations. Here we show that the radiative effects of precipitating <span class="hlt">ice</span> (falling snow) contribute substantially to this discrepancy. Many models exclude these radiative effects, so they underestimate both shortwave albedo and downward longwave radiation. Using two simulations with the climate model CESM1, we show that including falling-snow radiative effects improves the simulations relative to cloud properties from CloudSat-CALIPSO, radiation from CERES-EBAF and sea-<span class="hlt">ice</span> concentration from passive microwave sensors. From 50-70°S, the simulated sea-<span class="hlt">ice</span>-area bias is reduced by 2.12 × 106 km2 (55%) in winter and by 1.17 × 106 km2 (39%) in summer, mainly because increased wintertime longwave heating restricts sea-<span class="hlt">ice</span> growth and so reduces summer albedo. Improved <span class="hlt">Antarctic</span> sea-<span class="hlt">ice</span> simulations will increase confidence in projected <span class="hlt">Antarctic</span> sea level contributions and changes in global warming driven by long-term changes in Southern Ocean feedbacks.</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 <span class="hlt">ice</span>: 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 <span class="hlt">ice</span>. Particular emphasis is placed on comparing and contrasting the Arctic and <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> habitats, and the subsequent influence of these environments on the life history strategies of the crustacean fauna. Sea <span class="hlt">ice</span> 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 <span class="hlt">cover</span> of sea <span class="hlt">ice</span> 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 <span class="hlt">ice</span> extent, much of the <span class="hlt">ice</span> is over very deep water and more than 80% breaks out each year. In contrast, Arctic sea <span class="hlt">ice</span> often <span class="hlt">covers</span> comparatively shallow water, doubles in its extent on an annual cycle and the <span class="hlt">ice</span> may persist for several decades. Crustaceans, particularly copepods and amphipods, are abundant in the sea <span class="hlt">ice</span> zone at both poles, either living within the brine channel system of the <span class="hlt">ice</span>-crystal matrix or inhabiting the <span class="hlt">ice</span>-water interface. Many species associate with <span class="hlt">ice</span> 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 <span class="hlt">ice</span> copepod fauna by calanoids, the high euphausiid biomass in Southern Ocean waters and the lack of any species that appear fully dependent on the <span class="hlt">ice</span>. In the Arctic, the <span class="hlt">ice</span>-associated fauna is dominated by amphipods. Calanoid copepods are not tightly associated with the <span class="hlt">ice</span>, while harpacticoids and</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 <span class="hlt">ice</span></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 water masses and sea <span class="hlt">ice</span>. 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 <span class="hlt">ice</span> model and compared to small icebergs observations. Iceberg melt increases sea <span class="hlt">ice</span> <span class="hlt">cover</span>, about 10% in annual mean sea <span class="hlt">ice</span> 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 <span class="hlt">ice</span> models with a climatological iceberg fresh-water flux.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.C13A0603O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.C13A0603O"><span>Spatial Heterogeneity of <span class="hlt">Ice</span> <span class="hlt">Cover</span> Sediment and Thickness and Its Effects on Photosynthetically Active Radiation and Chlorophyll-a Distribution: <span class="hlt">Lake</span> Bonney, Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Obryk, M.; Doran, P. T.; Priscu, J. C.; Morgan-Kiss, R. M.; Siebenaler, A. G.</p> <p>2012-12-01</p> <p>The perennially <span class="hlt">ice-covered</span> <span class="hlt">lakes</span> in the McMurdo Dry Valleys, Antarctica have been extensively studied under the Long Term Ecological Research project. But sampling has been spatially restricted due to the logistical difficulty of penetrating the 3-6 m of <span class="hlt">ice</span> <span class="hlt">cover</span>. The <span class="hlt">ice</span> <span class="hlt">covers</span> restrict wind-driven turbulence and its associated mixing of water, resulting in a unique thermal stratification and a strong vertical gradient of salinity. The permanent <span class="hlt">ice</span> <span class="hlt">covers</span> also shade the underlying water column, which, in turn, controls photosynthesis. Here, we present results of a three-dimensional record of <span class="hlt">lake</span> processes obtained with an autonomous underwater vehicle (AUV). The AUV was deployed at West <span class="hlt">Lake</span> Bonney, located in Taylor Valley, Dry Valleys, to further understand biogeochemical and physical properties of the Dry Valley <span class="hlt">lakes</span>. The AUV was equipped with depth, conductivity, temperature, under water photosynthetically active radiation (PAR), turbidity, chlorophyll-and-DOM fluorescence, pH, and REDOX sensors. Measurements were taken over the course of two years in a 100 x 100 meter spaced horizontal sampling grid (and 0.2 m vertical resolution). In addition, the AUV measured <span class="hlt">ice</span> thickness and collected 200 images looking up through the <span class="hlt">ice</span>, which were used to quantify sediment distribution. Comparison with high-resolution satellite QuickBird imagery demonstrates a strong correlation between aerial sediment distribution and <span class="hlt">ice</span> <span class="hlt">cover</span> thickness. Our results are the first to show the spatial heterogeneity of lacustrine ecosystems in the McMurdo Dry Valleys, significantly improving our understanding of <span class="hlt">lake</span> processes. Surface sediment is responsible for localized thinning of <span class="hlt">ice</span> <span class="hlt">cover</span> due to absorption of solar radiation, which in turn increases total available PAR in the water column. Higher PAR values are negatively correlated with chlorophyll-a, presenting a paradox; historically, long-term studies of PAR and chlorophyll-a have shown positive trends. We hypothesized</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140017824','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140017824"><span>Changes in Arctic and <span class="hlt">Antarctic</span> Sea <span class="hlt">Ice</span> as a Microcosm of Global Climate Change</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Parkinson, Claire L.</p> <p>2014-01-01</p> <p>Polar sea <span class="hlt">ice</span> is a key element of the climate system and has now been monitored through satellite observations for over three and a half decades. The satellite observations reveal considerable information about polar <span class="hlt">ice</span> and its changes since the late 1970s, including a prominent downward trend in Arctic sea <span class="hlt">ice</span> coverage and a much lesser upward trend in <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> coverage, illustrative of the important fact that climate change entails spatial contrasts. The decreasing <span class="hlt">ice</span> coverage in the Arctic corresponds well with contemporaneous Arctic warming and exhibits particularly large decreases in the summers of 2007 and 2012, influenced by both preconditioning and atmospheric conditions. The increasing <span class="hlt">ice</span> coverage in the <span class="hlt">Antarctic</span> is not as readily explained, but spatial differences in the <span class="hlt">Antarctic</span> trends suggest a possible connection with atmospheric circulation changes that have perhaps been influenced by the <span class="hlt">Antarctic</span> ozone hole. The changes in the polar <span class="hlt">ice</span> <span class="hlt">covers</span> and the issues surrounding those changes have many commonalities with broader climate changes and their surrounding issues, allowing the sea <span class="hlt">ice</span> changes to be viewed in some important ways as a microcosm of global climate change.</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/2017EGUGA..1912539S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1912539S"><span>Analysis on variability and trend in <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> albedo between 1983 and 2009</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Seo, Minji; Kim, Hyun-cheol; Choi, Sungwon; Lee, Kyeong-sang; Han, Kyung-soo</p> <p>2017-04-01</p> <p>Sea <span class="hlt">ice</span> is key parameter in order to understand the cryosphere climate change. Several studies indicate the different trend of sea <span class="hlt">ice</span> between Antarctica and Arctic. Albedo is important factor for understanding the energy budget and factors for observing of environment changes of Cryosphere such as South Pole, due to it mainly <span class="hlt">covered</span> by <span class="hlt">ice</span> and snow with high albedo value. In this study, we analyzed variability and trend of long-term sea <span class="hlt">ice</span> albedo data to understand the changes of sea <span class="hlt">ice</span> over Antarctica. In addiction, sea <span class="hlt">ice</span> albedo researched the relationship with <span class="hlt">Antarctic</span> oscillation in order to determine the atmospheric influence. We used the sea <span class="hlt">ice</span> albedo data at The Satellite Application Facility on Climate Monitoring and <span class="hlt">Antarctic</span> Oscillation data at NOAA Climate Prediction Center (CPC). We analyzed the annual trend in albedo using linear regression to understand the spatial and temporal tendency. <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> albedo has two spatial trend. Weddle sea / Ross sea sections represent a positive trend (0.26% ˜ 0.04% yr-1) and Bellingshausen Amundsen sea represents a negative trend (- 0.14 ˜ -0.25%yr-1). Moreover, we performed the correlation analysis between albedo and <span class="hlt">Antarctic</span> oscillation. As a results, negative area indicate correlation coefficient of - 0.3639 and positive area indicates correlation coefficient of - 0.0741. Theses results sea <span class="hlt">ice</span> albedo has regional trend according to ocean. Decreasing sea <span class="hlt">ice</span> trend has negative relationship with <span class="hlt">Antarctic</span> oscillation, its represent a possibility that sea <span class="hlt">ice</span> influence atmospheric factor.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1817868T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1817868T"><span>Life under <span class="hlt">ice</span>: Investigating microbial-related biogeochemical cycles in the seasonally-<span class="hlt">covered</span> Great <span class="hlt">Lake</span> Onego, Russia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Thomas, Camille; Ariztegui, Daniel; Victor, Frossard; Emilie, Lyautey; Marie-Elodie, Perga; Life Under Ice Scientific Team</p> <p>2016-04-01</p> <p>The Great European <span class="hlt">lakes</span> Ladoga and Onego are important resources for Russia in terms of drinking water, energy, fishing and leisure. Because their northern location (North of Saint Petersburgh), these <span class="hlt">lakes</span> are usually <span class="hlt">ice-covered</span> during winter. Due to logistical reasons, their study has thus been limited to the <span class="hlt">ice</span>-free periods, and very few data are available for the winter season. As a matter of fact, comprehension of large <span class="hlt">lakes</span> behaviour in winter is very limited as compared to the knowledge available from small subpolar <span class="hlt">lakes</span> or perennially <span class="hlt">ice-covered</span> polar <span class="hlt">lakes</span>. To tackle this issue, an international consortium of scientists has gathered around the « life under <span class="hlt">ice</span> » project to investigate physical, chemical and biogeochemical changes during winter in <span class="hlt">Lake</span> Onego. Our team has mainly focused on the characterization and quantification of biological processes, from the water column to the sediment, with a special focus on methane cycling and trophic interactions. A first « on-<span class="hlt">ice</span> » campaign in March 2015 allowed the sampling of a 120 cm sedimentary core and the collection of water samples at multiple depths. The data resulting from this expedition will be correlated to physical and chemical parameters collected simultaneously. A rapid biological activity test was applied immediately after coring in order to test for microbial activity in the sediments. In situ adenosine-5'-triphosphate (ATP) measurements were carried out in the core and taken as an indication of living organisms within the sediments. The presence of ATP is a marker molecule for metabolically active cells, since it is not known to form abiotically. Deoxyribonucleic acid (DNA) and ribonucleic acid (RNA) were extracted from these samples, and quantified. Quantitative polymerase chain reactions (PCR) were performed on archaeal and bacterial 16S rRNA genes used to reconstruct phylogenies, as well as on their transcripts. Moreover, functional genes involved in the methane and nitrogen cycles</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120013478','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120013478"><span>Variability and Anomalous Trends in the Global Sea <span class="hlt">Ice</span> <span class="hlt">Cover</span></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.</p> <p>2012-01-01</p> <p>The advent of satellite data came fortuitously at a time when the global sea <span class="hlt">ice</span> <span class="hlt">cover</span> has been changing rapidly and new techniques are needed to accurately assess the true state and characteristics of the global sea <span class="hlt">ice</span> <span class="hlt">cover</span>. The extent of the sea <span class="hlt">ice</span> in the Northern Hemisphere has been declining by about -4% per decade for the period 1979 to 2011 but for the period from 1996 to 2010, the rate of decline became even more negative at -8% per decade, indicating an acceleration in the decline. More intriguing is the drastically declining perennial sea <span class="hlt">ice</span> area, which is the <span class="hlt">ice</span> that survives the summer melt and observed to be retreating at the rate of -14% per decade during the 1979 to 2012 period. Although a slight recovery occurred in the last three years from an abrupt decline in 2007, the perennial <span class="hlt">ice</span> extent was almost as low as in 2007 in 2011. The multiyear <span class="hlt">ice</span>, which is the thick component of the perennial <span class="hlt">ice</span> and regarded as the mainstay of the Arctic sea <span class="hlt">ice</span> <span class="hlt">cover</span> is declining at an even higher rate of -19% per decade. The more rapid decline of the extent of this thicker <span class="hlt">ice</span> type means that the volume of the <span class="hlt">ice</span> is also declining making the survival of the Arctic <span class="hlt">ice</span> in summer highly questionable. The slight recovery in 2008, 2009 and 2010 for the perennial <span class="hlt">ice</span> in summer was likely associated with an apparent cycle in the time series with a period of about 8 years. Results of analysis of concurrent MODIS and AMSR-E data in summer also provide some evidence of more extensive summer melt and meltponding in 2007 and 2011 than in other years. Meanwhile, the <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> <span class="hlt">cover</span>, as observed by the same set of satellite data, is showing an unexpected and counter intuitive increase of about 1 % per decade over the same period. Although a strong decline in <span class="hlt">ice</span> extent is apparent in the Bellingshausen/ Amundsen Seas region, such decline is more than compensated by increases in the extent of the sea <span class="hlt">ice</span> <span class="hlt">cover</span> in the Ross Sea region. The results of analysis of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.C44A..08S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.C44A..08S"><span>Radio-echo sounding of 'active' <span class="hlt">Antarctic</span> subglacial <span class="hlt">lakes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Siegert, M. J.; Ross, N.; Blankenship, D. D.; Young, D. A.; Greenbaum, J. S.; Richter, T.; Rippin, D. M.; Le Brocq, A. M.; Wright, A.; Bingham, R.; Corr, H.; Ferraccioli, F.; Jordan, T. A.; Smith, B. E.; Payne, A. J.; Dowdeswell, J. A.; Bamber, J. L.</p> <p>2013-12-01</p> <p>Repeat-pass satellite altimetry has revealed 124 discrete surface height changes across the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet, interpreted to be caused by subglacial <span class="hlt">lake</span> discharges (surface lowering) and inputs (surface uplift). Few of these active <span class="hlt">lakes</span> have been confirmed by radio-echo sounding (RES) despite several attempts, however. Over the last 5 years, major geophysical campaigns have acquired RES data from several 'active' <span class="hlt">lake</span> sites, including the US-UK-Australian ICECAP programme in East Antactica and the UK survey of the Institute <span class="hlt">Ice</span> Stream in West Antarctica. In the latter case, a targeted RES survey of one 'active' <span class="hlt">lake</span> was undertaken. RES evidence of the subglacial bed beneath 'active' <span class="hlt">lakes</span> in both East and West Antarctica will be presented, and the evidence for pooled subglacial water from these data will be assessed. Based on this assessment, the nature of 'active' subglacial <span class="hlt">lakes</span>, and their associated hydrology and relationship with surrounding topography will be discussed, as will the likelihood of further 'active' <span class="hlt">lakes</span> in Antarctica. Hydraulic potential map of the Byrd Glacier catchment with contours at 5 MPa intervals. Predicted subglacial flowpaths are shown in blue. Subglacial <span class="hlt">lakes</span> known from previous geophysical surveys are shown as black triangles while the newly discovered 'Three-tier <span class="hlt">lakes</span>' are shown in dashed black outline. Surface height change features within the Byrd subglacial catchment are shown in outline and are shaded to indicate whether they were rising or falling during the ICESat campaign. Those features are labelled in-line with the numbering system of Smith et al. (J. Glac. 2009).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.A41N..04H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.A41N..04H"><span>Observed and simulated changes in <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> and sea level pressure: anthropogenic or natural variability? (Invited)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hobbs, W. R.</p> <p>2013-12-01</p> <p>Statistically-significant changes in <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> <span class="hlt">cover</span> and the overlying atmosphere have been observed over the last 30 years, but there is an open question of whether these changes are due to multi-decadal natural variability or an anthropogenically-forced response. A number of recent papers have shown that the slight increase in total sea <span class="hlt">ice</span> <span class="hlt">cover</span> is within the bounds of internal variability exhibited by coupled climate models in the CMIP5 suite. Modelled changes for the same time period generally show a decrease, but again with a magnitude that is within internal variability. However, in contrast to the Arctic, sea <span class="hlt">ice</span> tends in the <span class="hlt">Antarctic</span> are spatially highly heterogeneous, and consideration of the total <span class="hlt">ice</span> <span class="hlt">cover</span> may mask important regional signals. In this work, a robust ';fingerprinting' approach is used to show that the observed spatial pattern of sea <span class="hlt">ice</span> trends is in fact outside simulated natural variability in west <span class="hlt">Antarctic</span>, and furthermore that the CMIP5 models consistently show decreased <span class="hlt">ice</span> <span class="hlt">cover</span> in the Ross and Weddell Seas, sectors which in fact have an observed increase in <span class="hlt">cover</span>. As a first step towards understanding the disagreement between models and observations, modelled sea level pressure trends are analysed using and optimal fingerprinting approach, to identify whether atmospheric deficiencies in the models can explain the model-observation discrepancy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28543018','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28543018"><span>Multiple <span class="hlt">ice</span>-binding proteins of probable prokaryotic origin in an <span class="hlt">Antarctic</span> <span class="hlt">lake</span> alga, Chlamydomonas sp. <span class="hlt">ICE</span>-MDV (Chlorophyceae).</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Raymond, James A; Morgan-Kiss, Rachael</p> <p>2017-08-01</p> <p><span class="hlt">Ice</span>-associated algae produce <span class="hlt">ice</span>-binding proteins (IBPs) to prevent freezing damage. The IBPs of the three chlorophytes that have been examined so far share little similarity across species, making it likely that they were acquired by horizontal gene transfer (HGT). To clarify the importance and source of IBPs in chlorophytes, we sequenced the IBP genes of another <span class="hlt">Antarctic</span> chlorophyte, Chlamydomonas sp. <span class="hlt">ICE</span>-MDV (Chlamy-<span class="hlt">ICE</span>). Genomic DNA and total RNA were sequenced and screened for known <span class="hlt">ice</span>-associated genes. Chlamy-<span class="hlt">ICE</span> has as many as 50 IBP isoforms, indicating that they have an important role in survival. The IBPs are of the DUF3494 type and have similar exon structures. The DUF3494 sequences are much more closely related to prokaryotic sequences than they are to sequences in other chlorophytes, and the chlorophyte IBP and ribosomal 18S phylogenies are dissimilar. The multiple IBP isoforms found in Chlamy-<span class="hlt">ICE</span> and other algae may allow the algae to adapt to a greater variety of <span class="hlt">ice</span> conditions than prokaryotes, which typically have a single IBP gene. The predicted structure of the DUF3494 domain has an <span class="hlt">ice</span>-binding face with an orderly array of hydrophilic side chains. The results indicate that Chlamy-<span class="hlt">ICE</span> acquired its IBP genes by HGT in a single event. The acquisitions of IBP genes by this and other species of <span class="hlt">Antarctic</span> algae by HGT appear to be key evolutionary events that allowed algae to extend their ranges into polar environments. © 2017 Phycological Society of America.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040088835&hterms=photosynthesis&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dphotosynthesis','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040088835&hterms=photosynthesis&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dphotosynthesis"><span>Thickness of tropical <span class="hlt">ice</span> and photosynthesis on a snowball Earth</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>McKay, C. P.</p> <p>2000-01-01</p> <p>On a completely <span class="hlt">ice-covered</span> "snowball" Earth the thickness of <span class="hlt">ice</span> in the tropical regions would be limited by the sunlight penetrating into the <span class="hlt">ice</span> <span class="hlt">cover</span> and by the latent heat flux generated by freezing at the <span class="hlt">ice</span> bottom--the freezing rate would balance the sublimation rate from the top of the <span class="hlt">ice</span> <span class="hlt">cover</span>. Heat transfer models of the perennially <span class="hlt">ice-covered</span> <span class="hlt">Antarctic</span> dry valley <span class="hlt">lakes</span> applied to the snowball Earth indicate that the tropical <span class="hlt">ice</span> <span class="hlt">cover</span> would have a thickness of 10 m or less with a corresponding transmissivity of > 0.1%. This light level is adequate for photosynthesis and could explain the survival of the eukaryotic algae.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/11543492','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/11543492"><span>Thickness of tropical <span class="hlt">ice</span> and photosynthesis on a snowball Earth.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>McKay, C P</p> <p>2000-07-15</p> <p>On a completely <span class="hlt">ice-covered</span> "snowball" Earth the thickness of <span class="hlt">ice</span> in the tropical regions would be limited by the sunlight penetrating into the <span class="hlt">ice</span> <span class="hlt">cover</span> and by the latent heat flux generated by freezing at the <span class="hlt">ice</span> bottom--the freezing rate would balance the sublimation rate from the top of the <span class="hlt">ice</span> <span class="hlt">cover</span>. Heat transfer models of the perennially <span class="hlt">ice-covered</span> <span class="hlt">Antarctic</span> dry valley <span class="hlt">lakes</span> applied to the snowball Earth indicate that the tropical <span class="hlt">ice</span> <span class="hlt">cover</span> would have a thickness of 10 m or less with a corresponding transmissivity of > 0.1%. This light level is adequate for photosynthesis and could explain the survival of the eukaryotic algae.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120010403','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120010403"><span>Satellite Observations of <span class="hlt">Antarctic</span> Sea <span class="hlt">Ice</span> Thickness and Volume</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kurtz, Nathan; Markus, Thorsten</p> <p>2012-01-01</p> <p>We utilize satellite laser altimetry data from ICESat combined with passive microwave measurements to analyze basin-wide changes in <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> thickness and volume over a 5 year period from 2003-2008. Sea <span class="hlt">ice</span> thickness exhibits a small negative trend while area increases in the summer and fall balanced losses in thickness leading to small overall volume changes. Using a five year time-series, we show that only small <span class="hlt">ice</span> thickness changes of less than -0.03 m/yr and volume changes of -266 cu km/yr and 160 cu km/yr occurred for the spring and summer periods, respectively. The calculated thickness and volume trends are small compared to the observational time period and interannual variability which masks the determination of long-term trend or cyclical variability in the sea <span class="hlt">ice</span> <span class="hlt">cover</span>. These results are in stark contrast to the much greater observed losses in Arctic sea <span class="hlt">ice</span> volume and illustrate the different hemispheric changes of the polar sea <span class="hlt">ice</span> <span class="hlt">covers</span> in recent years.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.B23G..08P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.B23G..08P"><span>Sources and sinks of methane beneath polar <span class="hlt">ice</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Priscu, J. C.; Adams, H. E.; Hand, K. P.; Dore, J. E.; Matheus-Carnevali, P.; Michaud, A. B.; Murray, A. E.; Skidmore, M. L.; Vick-Majors, T.</p> <p>2014-12-01</p> <p>Several icy moons of the outer solar system carry subsurface oceans containing many times the volume of liquid water on Earth and may provide the greatest volume of habitable space in our solar system. Functional sub-<span class="hlt">ice</span> polar ecosystems on Earth provide compelling models for the habitability of extraterrestrial sub-<span class="hlt">ice</span> oceans. A key feature of sub-<span class="hlt">ice</span> environments is that most of them receive little to no solar energy. Consequently, organisms inhabiting these environments must rely on chemical energy to assimilate either carbon dioxide or organic molecules to support their metabolism. Methane can be utilized by certain bacteria as both a carbon and energy source. Isotopic data show that methane in Earth's polar <span class="hlt">lakes</span> is derived from both biogenic and thermogenic sources. Thermogenic sources of methane in the thermokarst <span class="hlt">lakes</span> of the north slope of Alaska yield supersaturated water columns during winter <span class="hlt">ice</span> <span class="hlt">cover</span> that support active populations of methanotrophs during the polar night. Methane in the permanently <span class="hlt">ice-covered</span> <span class="hlt">lakes</span> of the McMurdo Dry Valleys, Antarctica varies widely in concentration and is produced either by contemporary methanogenesis or is a relic from subglacial flow. Rate measurements revealed that microbial methane oxidation occurs beneath the <span class="hlt">ice</span> in both the arctic and <span class="hlt">Antarctic</span> <span class="hlt">lakes</span>. The first samples collected from an <span class="hlt">Antarctic</span> subglacial environment beneath 800 m of <span class="hlt">ice</span> (Subglacial <span class="hlt">Lake</span> Whillans) revealed an active microbial ecosystem that has been isolated from the atmosphere for many thousands of years. The sediments of <span class="hlt">Lake</span> Whillans contained high levels of methane with an isotopic signature that indicates it was produced via methanogenesis. The source of this methane appears to be from the decomposition of organic carbon deposited when this region of Antarctica was <span class="hlt">covered</span> by the sea. Collectively, data from these sub-<span class="hlt">ice</span> environments show that methane transformations play a key role in microbial community metabolism. The discovery of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C33D..01P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C33D..01P"><span>Modeling <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet retreat in warm climates: a historical perspective.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pollard, D.; Deconto, R. M.; Gasson, E.</p> <p>2016-12-01</p> <p>Early modeling of <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet size vs. climate focused on asymmetry between retreat and growth, with much greater warming needed to cause retreat from full <span class="hlt">ice</span> <span class="hlt">cover</span>, due to Height Mass Balance Feedback and albedo feedback. This led to a long-standing model-data conflict, with models needing 1000 to2000 ppmv atmospheric CO2 to produce retreat from full size, vs. proxy data of large <span class="hlt">ice</span> fluctuations despite much lower CO2 since the Miocene.Subsequent modeling with marine <span class="hlt">ice</span> physics found that the West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet could undergo repeated warm-period collapses with realistic past forcing. However, that yields only 3 to 7 m equivalent sea-level rise above modern, compared to 10 to 20 m or more suggested by some geologic data. Large subglacial basins in East Antarctica could be vulnerable to the same processes,but did not retreat in most models due to narrower and shallower sills.After recent modifications, some <span class="hlt">ice</span> sheet models were able to produce warm-period collapse of major East <span class="hlt">Antarctic</span> basins, with sea-level rise of up to 15 m. The modifications are (i) hydrofracturing by surface melt, and structural failure of <span class="hlt">ice</span> cliffs, or (ii) numerical treatment at the grounding line. In these models, large retreat occurs both for past warmintervals, and also for future business-as-usual scenarios.Some interpretations of data in the late Oligocene and Miocene suggest yet larger fluctuations, between 50 to 100% of modern <span class="hlt">Antarctic</span> size. That would require surface-melt driven retreat of some terrestrial East <span class="hlt">Antarctic</span> <span class="hlt">ice</span>, despite the hysteresis issue raised above. A recent study using a coupled climate-<span class="hlt">ice</span> sheet model found that with a finer climate gridand more frequent coupling exchange, substantial retreat of terrestrial Antarctica can occur with 500 to 840 ppmv CO2, much lower than in earlier models. This will allow meaningful interactions between modeling and deeper-time geologic interpretations since the late Oligocene.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27458438','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27458438"><span>Unanticipated Geochemical and Microbial Community Structure under Seasonal <span class="hlt">Ice</span> <span class="hlt">Cover</span> in a Dilute, Dimictic Arctic <span class="hlt">Lake</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Schütte, Ursel M E; Cadieux, Sarah B; Hemmerich, Chris; Pratt, Lisa M; White, Jeffrey R</p> <p>2016-01-01</p> <p>Despite most <span class="hlt">lakes</span> in the Arctic being perennially or seasonally frozen for at least 40% of the year, little is known about microbial communities and nutrient cycling under <span class="hlt">ice</span> <span class="hlt">cover</span>. We assessed the vertical microbial community distribution and geochemical composition in early spring under <span class="hlt">ice</span> in a seasonally <span class="hlt">ice-covered</span> <span class="hlt">lake</span> in southwest Greenland using amplicon-based sequencing that targeted 16S rRNA genes and using a combination of field and laboratory aqueous geochemical methods. Microbial communities changed consistently with changes in geochemistry. Composition of the abundant members responded strongly to redox conditions, shifting downward from a predominantly heterotrophic aerobic community in the suboxic waters to a heterotrophic anaerobic community in the anoxic waters. Operational taxonomic units (OTUs) of Sporichthyaceae, Comamonadaceae, and the SAR11 Clade had higher relative abundances above the oxycline and OTUs within the genus Methylobacter, the phylum Lentisphaerae, and purple sulfur bacteria (PSB) below the oxycline. Notably, a 13-fold increase in sulfide at the oxycline was reflected in an increase and change in community composition of potential sulfur oxidizers. Purple non-sulfur bacteria were present above the oxycline and green sulfur bacteria and PSB coexisted below the oxycline, however, PSB were most abundant. For the first time we show the importance of PSB as potential sulfur oxidizers in an Arctic dimictic <span class="hlt">lake</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C33B0821P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C33B0821P"><span>RADARSAT-2 Polarimetric Radar Imaging for <span class="hlt">Lake</span> <span class="hlt">Ice</span> Mapping</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pan, F.; Kang, K.; Duguay, C. R.</p> <p>2016-12-01</p> <p>Changes in <span class="hlt">lake</span> <span class="hlt">ice</span> dates and duration are useful indicators for assessing long-term climate trends and variability in northern countries. <span class="hlt">Lake</span> <span class="hlt">ice</span> <span class="hlt">cover</span> observations are also a valuable data source for predictions with numerical <span class="hlt">ice</span> and weather forecasting models. In recent years, satellite remote sensing has assumed a greater role in providing observations of <span class="hlt">lake</span> <span class="hlt">ice</span> <span class="hlt">cover</span> extent for both modeling and climate monitoring purposes. Polarimetric radar imaging has become a promising tool for <span class="hlt">lake</span> <span class="hlt">ice</span> mapping at high latitudes where meteorological conditions and polar darkness severely limit observations from optical sensors. In this study, we assessed and characterized the physical scattering mechanisms of <span class="hlt">lake</span> <span class="hlt">ice</span> from fully polarimetric RADARSAT-2 datasets obtained over Great Bear <span class="hlt">Lake</span>, Canada, with the intent of classifying open water and different <span class="hlt">ice</span> types during the freeze-up and break-up periods. Model-based and eigen-based decompositions were employed to construct the coherency matrix into deterministic scattering mechanisms. These procedures as well as basic polarimetric parameters were integrated into modified convolutional neural networks (CNN). The CNN were modified via introduction of a Markov random field into the higher iterative layers of networks for acquiring updated priors and classifying <span class="hlt">ice</span> and open water areas over the <span class="hlt">lake</span>. We show that the selected polarimetric parameters can help with interpretation of radar-<span class="hlt">ice</span>/water interactions and can be used successfully for water-<span class="hlt">ice</span> segmentation, including different <span class="hlt">ice</span> types. As more satellite SAR sensors are being launched or planned, such as the Sentinel-1a/b series and the upcoming RADARSAT Constellation Mission, the rapid volume growth of data and their analysis require the development of robust automated algorithms. The approach developed in this study was therefore designed with the intent of moving towards fully automated mapping of <span class="hlt">lake</span> <span class="hlt">ice</span> for consideration by <span class="hlt">ice</span> services.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3721118','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3721118"><span>Diatom assemblages promote <span class="hlt">ice</span> formation in large <span class="hlt">lakes</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>D'souza, N A; Kawarasaki, Y; Gantz, J D; Lee, R E; Beall, B F N; Shtarkman, Y M; Koçer, Z A; Rogers, S O; Wildschutte, H; Bullerjahn, G S; McKay, R M L</p> <p>2013-01-01</p> <p>We present evidence for the directed formation of <span class="hlt">ice</span> by planktonic communities dominated by filamentous diatoms sampled from the <span class="hlt">ice-covered</span> Laurentian Great <span class="hlt">Lakes</span>. We hypothesize that <span class="hlt">ice</span> formation promotes attachment of these non-motile phytoplankton to overlying <span class="hlt">ice</span>, thereby maintaining a favorable position for the diatoms in the photic zone. However, it is unclear whether the diatoms themselves are responsible for <span class="hlt">ice</span> nucleation. Scanning electron microscopy revealed associations of bacterial epiphytes with the dominant diatoms of the phytoplankton assemblage, and bacteria isolated from the phytoplankton showed elevated temperatures of crystallization (Tc) as high as −3 °C. <span class="hlt">Ice</span> nucleation-active bacteria were identified as belonging to the genus Pseudomonas, but we could not demonstrate that they were sufficiently abundant to incite the observed freezing. Regardless of the source of <span class="hlt">ice</span> nucleation activity, the resulting production of frazil <span class="hlt">ice</span> may provide a means for the diatoms to be recruited to the overlying <span class="hlt">lake</span> <span class="hlt">ice</span>, thereby increasing their fitness. Bacterial epiphytes are likewise expected to benefit from their association with the diatoms as recipients of organic carbon excreted by their hosts. This novel mechanism illuminates a previously undescribed stage of the life cycle of the meroplanktonic diatoms that bloom in <span class="hlt">Lake</span> Erie and other Great <span class="hlt">Lakes</span> during winter and offers a model relevant to aquatic ecosystems having seasonal <span class="hlt">ice</span> <span class="hlt">cover</span> around the world. PMID:23552624</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27889953','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27889953"><span>Ecology under <span class="hlt">lake</span> <span class="hlt">ice</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hampton, Stephanie E; Galloway, Aaron W E; Powers, Stephen M; Ozersky, Ted; Woo, Kara H; Batt, Ryan D; Labou, Stephanie G; O'Reilly, Catherine M; Sharma, Sapna; Lottig, Noah R; Stanley, Emily H; North, Rebecca L; Stockwell, Jason D; Adrian, Rita; Weyhenmeyer, Gesa A; Arvola, Lauri; Baulch, Helen M; Bertani, Isabella; Bowman, Larry L; Carey, Cayelan C; Catalan, Jordi; Colom-Montero, William; Domine, Leah M; Felip, Marisol; Granados, Ignacio; Gries, Corinna; Grossart, Hans-Peter; Haberman, Juta; Haldna, Marina; Hayden, Brian; Higgins, Scott N; Jolley, Jeff C; Kahilainen, Kimmo K; Kaup, Enn; Kehoe, Michael J; MacIntyre, Sally; Mackay, Anson W; Mariash, Heather L; McKay, Robert M; Nixdorf, Brigitte; Nõges, Peeter; Nõges, Tiina; Palmer, Michelle; Pierson, Don C; Post, David M; Pruett, Matthew J; Rautio, Milla; Read, Jordan S; Roberts, Sarah L; Rücker, Jacqueline; Sadro, Steven; Silow, Eugene A; Smith, Derek E; Sterner, Robert W; Swann, George E A; Timofeyev, Maxim A; Toro, Manuel; Twiss, Michael R; Vogt, Richard J; Watson, Susan B; Whiteford, Erika J; Xenopoulos, Marguerite A</p> <p>2017-01-01</p> <p>Winter conditions are rapidly changing in temperate ecosystems, particularly for those that experience periods of snow and <span class="hlt">ice</span> <span class="hlt">cover</span>. Relatively little is known of winter ecology in these systems, due to a historical research focus on summer 'growing seasons'. We executed the first global quantitative synthesis on under-<span class="hlt">ice</span> <span class="hlt">lake</span> ecology, including 36 abiotic and biotic variables from 42 research groups and 101 <span class="hlt">lakes</span>, examining seasonal differences and connections as well as how seasonal differences vary with geophysical factors. Plankton were more abundant under <span class="hlt">ice</span> than expected; mean winter values were 43.2% of summer values for chlorophyll a, 15.8% of summer phytoplankton biovolume and 25.3% of summer zooplankton density. Dissolved nitrogen concentrations were typically higher during winter, and these differences were exaggerated in smaller <span class="hlt">lakes</span>. <span class="hlt">Lake</span> size also influenced winter-summer patterns for dissolved organic carbon (DOC), with higher winter DOC in smaller <span class="hlt">lakes</span>. At coarse levels of taxonomic aggregation, phytoplankton and zooplankton community composition showed few systematic differences between seasons, although literature suggests that seasonal differences are frequently <span class="hlt">lake</span>-specific, species-specific, or occur at the level of functional group. Within the subset of <span class="hlt">lakes</span> that had longer time series, winter influenced the subsequent summer for some nutrient variables and zooplankton biomass. © 2016 The Authors. Ecology Letters published by CNRS and John Wiley & Sons Ltd.</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> <span class="hlt">ice</span> 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><span class="hlt">Ice</span> discharge from large <span class="hlt">ice</span> 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 <span class="hlt">ice</span> flow since ˜ 2008. The new mapping provides complete coastal and inland coverage of <span class="hlt">ice</span> 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, <span class="hlt">ice</span> 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 <span class="hlt">Ice</span> 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> <span class="hlt">Ice</span> 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> <span class="hlt">ice</span> sheet lost <span class="hlt">ice</span> at an average rate of 183 ± 94 Gt yr-1 between 2008 and 2015. The modest increase in <span class="hlt">ice</span> discharge over the past 7 years is contrasted by high rates of <span class="hlt">ice</span> sheet mass loss and distinct spatial patters of elevation lowering. The West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> 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 <span class="hlt">ice</span> 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 <span class="hlt">ice</span> flow.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15796981','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15796981"><span>A hyperactive, Ca2+-dependent antifreeze protein in an <span class="hlt">Antarctic</span> bacterium.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gilbert, Jack A; Davies, Peter L; Laybourn-Parry, Johanna</p> <p>2005-04-01</p> <p>In cold climates, some plants and bacteria that cannot avoid freezing use antifreeze proteins (AFPs) to lessen the destructive effects of <span class="hlt">ice</span> recrystallization. These AFPs have weak freezing point depression activity, perhaps to avoid sudden, uncontrolled growth of <span class="hlt">ice</span>. Here, we report on an uncharacteristically powerful bacterial AFP found in an <span class="hlt">Antarctic</span> strain of the bacterium, Marinomonas primoryensis. It is Ca(2+)-dependent, shows evidence of cooperativity, and can produce over 2 degrees C of freezing point depression. Unlike most AFPs, it does not produce obvious crystal faceting during thermal hysteresis. This AFP might be capable of imparting freezing avoidance to M. primoryensis in <span class="hlt">ice-covered</span> <span class="hlt">Antarctic</span> <span class="hlt">lakes</span>. A hyperactive bacterial AFP has not previously been reported.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ClDy...50..655S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ClDy...50..655S"><span>Multiple climate regimes in an idealized <span class="hlt">lake-ice</span>-atmosphere model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sugiyama, Noriyuki; Kravtsov, Sergey; Roebber, Paul</p> <p>2018-01-01</p> <p>In recent decades, the Laurentian Great <span class="hlt">Lakes</span> have undergone rapid surface warming with the summertime trends substantially exceeding the warming rates of surrounding land. Warming of the deepest (<span class="hlt">Lake</span> Superior) was the strongest, and that of the shallowest (<span class="hlt">Lake</span> Erie)—the weakest of all <span class="hlt">lakes</span>. To investigate the dynamics of accelerated <span class="hlt">lake</span> warming, we considered single-column and multi-column thermodynamic <span class="hlt">lake-ice</span> models coupled to an idealized two-layer atmosphere. The variable temperature of the upper atmospheric layer—a proxy for the large-scale atmospheric forcing—consisted, in the most general case, of a linear trend mimicking the global warming and atmospheric interannual variability, both on top of the prescribed seasonal cycle of the upper-air temperature. The atmospheric boundary layer of the coupled model exchanged heat with the <span class="hlt">lake</span> and exhibited lateral diffusive heat transports between the adjacent atmospheric columns. In simpler single-column models, we find that, for a certain range of periodic atmospheric forcing, each <span class="hlt">lake</span> possesses two stable equilibrium seasonal cycles, which we call "regimes"—with and without <span class="hlt">lake-ice</span> occurrence in winter and with corresponding cold and warm temperatures in the following summer, respectively, all under an identical seasonally varying external forcing. Deeper <span class="hlt">lakes</span> exhibit larger differences in their summertime surface water temperature between the warm and cold regimes, due to their larger thermal and dynamical inertia. The regime behavior of multi-column coupled models is similar but more complex, and in some cases, they admit more than two stable equilibrium seasonal cycles, with varying degrees of wintertime <span class="hlt">ice-cover</span>. The simulated <span class="hlt">lake</span> response to climate change in the presence of the atmospheric noise rationalizes the observed accelerated warming of the <span class="hlt">lakes</span>, the correlation between wintertime <span class="hlt">ice</span> <span class="hlt">cover</span> and next summer's <span class="hlt">lake</span>-surface temperature, as well as higher warming trends of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70157522','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70157522"><span><span class="hlt">Lake</span> <span class="hlt">ice</span> records used to detect historical and future climatic changes</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Robertson, Dale M.; Ragotzkie, R.A.; Magnuson, John J.</p> <p>1992-01-01</p> <p>With the relationships between air temperature and freeze and break up dates, we can project how the <span class="hlt">ice</span> <span class="hlt">cover</span> of <span class="hlt">Lake</span> Mendota should respond to future climatic changes. If warming occurs, the <span class="hlt">ice</span> <span class="hlt">cover</span> for <span class="hlt">Lake</span> Mendota should decrease approximately 11 days per 1 °C increase. With a warming of 4 to 5 °C, years with no <span class="hlt">ice</span> <span class="hlt">cover</span> should occur in approximately 1 out of 15 to 30 years.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C43B0744A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C43B0744A"><span>Spatial scales of light transmission through <span class="hlt">Antarctic</span> pack <span class="hlt">ice</span>: Surface flooding vs. floe-size distribution</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Arndt, S.; Meiners, K.; Krumpen, T.; Ricker, R.; Nicolaus, M.</p> <p>2016-12-01</p> <p>Snow on sea <span class="hlt">ice</span> plays a crucial role for interactions between the ocean and atmosphere within the climate system of polar regions. <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> is <span class="hlt">covered</span> with snow during most of the year. The snow contributes substantially to the sea-<span class="hlt">ice</span> mass budget as the heavy snow loads can depress the <span class="hlt">ice</span> below water level causing flooding. Refreezing of the snow and seawater mixture results in snow-<span class="hlt">ice</span> formation on the <span class="hlt">ice</span> surface. The snow <span class="hlt">cover</span> determines also the amount of light being reflected, absorbed, and transmitted into the upper ocean, determining the surface energy budget of <span class="hlt">ice-covered</span> oceans. The amount of light penetrating through sea <span class="hlt">ice</span> into the upper ocean is of critical importance for the timing and amount of bottom sea-<span class="hlt">ice</span> melt, biogeochemical processes and under-<span class="hlt">ice</span> ecosystems. Here, we present results of several recent observations in the Weddell Sea measuring solar radiation under <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> with instrumented Remotely Operated Vehicles (ROV). The combination of under-<span class="hlt">ice</span> optical measurements with simultaneous characterization of surface properties, such as sea-<span class="hlt">ice</span> thickness and snow depth, allows the identification of key processes controlling the spatial distribution of the under-<span class="hlt">ice</span> light. Thus, our results show how the distinction between flooded and non-flooded sea-<span class="hlt">ice</span> regimes dominates the spatial scales of under-<span class="hlt">ice</span> light variability for areas smaller than 100-by-100m. In contrast, the variability on larger scales seems to be controlled by the floe-size distribution and the associated lateral incidence of light. These results are related to recent studies on the spatial variability of Arctic under-<span class="hlt">ice</span> light fields focusing on the distinctly differing dominant surface properties between the northern (e.g. summer melt ponds) and southern (e.g. year-round snow <span class="hlt">cover</span>, surface flooding) hemisphere sea-<span class="hlt">ice</span> <span class="hlt">cover</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_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/2017AGUFM.C41C1235L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C41C1235L"><span>Sensitivity of an <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet Model to Sub-<span class="hlt">Ice</span>-Shelf Melting</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lipscomb, W. H.; Leguy, G.; Urban, N. M.; Berdahl, M.</p> <p>2017-12-01</p> <p>Theory and observations suggest that marine-based sectors of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet could retreat rapidly under ocean warming and increased melting beneath <span class="hlt">ice</span> shelves. Numerical models of marine <span class="hlt">ice</span> sheets vary widely in sensitivity, depending on grid resolution and the parameterization of key processes (e.g., calving and hydrofracture). Here we study the sensitivity of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet to ocean warming and sub-shelf melting in standalone simulations of the Community <span class="hlt">Ice</span> Sheet Model (CISM). Melt rates either are prescribed based on observations and high-resolution ocean model output, or are derived from a plume model forced by idealized ocean temperature profiles. In CISM, we vary the model resolution (between 1 and 8 km), Stokes approximation (shallow-shelf, depth-integrated higher-order, or 3D higher-order) and calving scheme to create an ensemble of plausible responses to sub-shelf melting. This work supports a broader goal of building statistical and reduced models that can translate large-scale Earth-system model projections to changes in <span class="hlt">Antarctic</span> ocean temperatures and <span class="hlt">ice</span> sheet discharge, thus better quantifying uncertainty in <span class="hlt">Antarctic</span>-sourced sea-level rise.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMGC32B..02P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMGC32B..02P"><span>Contrasting Trends in Arctic and <span class="hlt">Antarctic</span> Sea <span class="hlt">Ice</span> Coverage Since the Late 1970s</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Parkinson, C. L.</p> <p>2016-12-01</p> <p>Satellite observations have allowed a near-continuous record of Arctic and <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> coverage since late 1978. This record has revealed considerable interannual variability in both polar regions but also significant long-term trends, with the Arctic losing, the <span class="hlt">Antarctic</span> gaining, and the Earth as a whole losing sea <span class="hlt">ice</span> coverage. Over the period 1979-2015, the trend in yearly average sea <span class="hlt">ice</span> extents in the Arctic is -53,100 km2/yr (-4.3 %/decade) and in the <span class="hlt">Antarctic</span> is 23,800 km2/yr (2.1 %/decade). For all 12 months, trends are negative in the Arctic and positive in the <span class="hlt">Antarctic</span>, with the highest magnitude monthly trend being for September in the Arctic, at -85,300 km2/yr (-10.9 %/decade). The decreases in Arctic sea <span class="hlt">ice</span> extents have been so dominant that not a single month since 1986 registered a new monthly record high, whereas 75 months registered new monthly record lows between 1987 and 2015 and several additional record lows were registered in 2016. The <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> record highs and lows are also out of balance, in the opposite direction, although not in such dramatic fashion. Geographic details on the changing <span class="hlt">ice</span> <span class="hlt">covers</span>, down to the level of individual pixels, can be seen by examining changes in the length of the sea <span class="hlt">ice</span> season. Results reveal (and quantify) shortening <span class="hlt">ice</span> seasons throughout the bulk of the Arctic marginal <span class="hlt">ice</span> zone, the main exception being within the Bering Sea, and lengthening sea <span class="hlt">ice</span> seasons through much of the Southern Ocean but shortening seasons in the Bellingshausen Sea, southern Amundsen Sea, and northwestern Weddell Sea. The decreasing Arctic sea <span class="hlt">ice</span> coverage was widely anticipated and fits well with a large array of environmental changes in the Arctic, whereas the increasing <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> coverage was not widely anticipated and explaining it remains an area of active research by many scientists exploring a variety of potential explanations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21198589','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21198589"><span><span class="hlt">Ice-cover</span> effects on competitive interactions between two fish species.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Helland, Ingeborg P; Finstad, Anders G; Forseth, Torbjørn; Hesthagen, Trygve; Ugedal, Ola</p> <p>2011-05-01</p> <p>1. Variations in the strength of ecological interactions between seasons have received little attention, despite an increased focus on climate alterations on ecosystems. Particularly, the winter situation is often neglected when studying competitive interactions. In northern temperate freshwaters, winter implies low temperatures and reduced food availability, but also strong reduction in ambient light because of <span class="hlt">ice</span> and snow <span class="hlt">cover</span>. Here, we study how brown trout [Salmo trutta (L.)] respond to variations in <span class="hlt">ice-cover</span> duration and competition with Arctic charr [Salvelinus alpinus (L.)], by linking laboratory-derived physiological performance and field data on variation in abundance among and within natural brown trout populations. 2. Both Arctic charr and brown trout reduced resting metabolic rate under simulated <span class="hlt">ice-cover</span> (darkness) in the laboratory, compared to no <span class="hlt">ice</span> (6-h daylight). However, in contrast to brown trout, Arctic charr was able to obtain positive growth rate in darkness and had higher food intake in tank experiments than brown trout. Arctic charr also performed better (lower energy loss) under simulated <span class="hlt">ice-cover</span> in a semi-natural environment with natural food supply. 3. When comparing brown trout biomass across 190 Norwegian <span class="hlt">lakes</span> along a climate gradient, longer <span class="hlt">ice-covered</span> duration decreased the biomass only in <span class="hlt">lakes</span> where brown trout lived together with Arctic charr. We were not able to detect any effect of <span class="hlt">ice-cover</span> on brown trout biomass in <span class="hlt">lakes</span> where brown trout was the only fish species. 4. Similarly, a 25-year time series from a <span class="hlt">lake</span> with both brown trout and Arctic charr showed that brown trout population growth rate depended on the interaction between <span class="hlt">ice</span> breakup date and Arctic charr abundance. High charr abundance was correlated with low trout population growth rate only in combination with long winters. 5. In conclusion, the two species differed in performance under <span class="hlt">ice</span>, and the observed outcome of competition in natural populations</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19790068799&hterms=atmospheric+rivers&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Datmospheric%2Brivers','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19790068799&hterms=atmospheric+rivers&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Datmospheric%2Brivers"><span>Evaporation of <span class="hlt">ice</span> in planetary atmospheres - <span class="hlt">Ice-covered</span> rivers on Mars</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wallace, D.; Sagan, C.</p> <p>1979-01-01</p> <p>The existence of <span class="hlt">ice</span> <span class="hlt">covered</span> rivers on Mars is considered. It is noted that the evaporation rate of water <span class="hlt">ice</span> on the surface of a planet with an atmosphere involves an equilibrium between solar heating and radiative and evaporative cooling of the <span class="hlt">ice</span> layer. It is determined that even with a mean Martian insolation rate above the <span class="hlt">ice</span> of approximately 10 to the -8th g per sq cm/sec, a flowing channel of liquid water will be <span class="hlt">covered</span> by <span class="hlt">ice</span> which evaporates sufficiently slowly that the water below can flow for hundreds of kilometers even with modest discharges. Evaporation rates are calculated for a range of frictional velocities, atmospheric pressures, and insolations and it is suggested that some subset of observed Martian channels may have formed as <span class="hlt">ice</span>-choked rivers. Finally, the exobiological implications of <span class="hlt">ice</span> <span class="hlt">covered</span> channels or <span class="hlt">lakes</span> on Mars are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=GL-2002-001602&hterms=BALANCE+SHEET&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DBALANCE%2BSHEET','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=GL-2002-001602&hterms=BALANCE+SHEET&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DBALANCE%2BSHEET"><span>Balance of the West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet</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>For several decades, measurements of the West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet showed it to be retreating rapidly. But new data derived from satellite-borne radar sensors show the <span class="hlt">ice</span> sheet to be growing. Changing <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheets remains an area of high scientific interest, particularly in light of recent global warming concerns. These new findings are significant because scientists estimate that sea level would rise 5-6 meters (16-20 feet) if the <span class="hlt">ice</span> sheet collapsed into the sea. Do these new measurements signal the end of the <span class="hlt">ice</span> sheet's 10,000-year retreat? Or, are these new satellite data simply much more accurate than the sparse <span class="hlt">ice</span> core and surface measurements that produced the previous estimates? Another possibility is that the <span class="hlt">ice</span> accumulation may simply indicate that the <span class="hlt">ice</span> sheet naturally expands and retreats in regular cycles. Cryologists will grapple with these questions, and many others, as they examine the new data. The image above depicts the region of West Antarctica where scientists measured <span class="hlt">ice</span> speed. The fast-moving central <span class="hlt">ice</span> streams are shown in red. Slower tributaries feeding the <span class="hlt">ice</span> streams are shown in blue. Green areas depict slow-moving, stable areas. Thick black lines depict the areas that collect snowfall to feed their respective <span class="hlt">ice</span> streams. Reference: Ian Joughin and Slawek Tulaczyk Science Jan 18 2002: 476-480. Image courtesy RADARSAT <span class="hlt">Antarctic</span> Mapping Project</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120009093','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120009093"><span>The <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet, Sea <span class="hlt">Ice</span>, and the Ozone Hole: Satellite Observations of how they are Changing</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Parkinson, Claire L.</p> <p>2012-01-01</p> <p>Antarctica is the Earth's coldest and highest continent and has major impacts on the climate and life of the south polar vicinity. It is <span class="hlt">covered</span> almost entirely by the Earth's largest <span class="hlt">ice</span> sheet by far, with a volume of <span class="hlt">ice</span> so great that if all the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> were to go into the ocean (as <span class="hlt">ice</span> or liquid water), this would produce a global sea level rise of about 60 meters (197 feet). The continent is surrounded by sea <span class="hlt">ice</span> that in the wintertime is even more expansive than the continent itself and in the summertime reduces to only about a sixth of its wintertime extent. Like the continent, the expansive sea <span class="hlt">ice</span> <span class="hlt">cover</span> has major impacts, reflecting the sun's radiation back to space, blocking exchanges between the ocean and the atmosphere, and providing a platform for some animal species while impeding other species. Far above the continent, the <span class="hlt">Antarctic</span> ozone hole is a major atmospheric phenomenon recognized as human-caused and potentially quite serious to many different life forms. Satellites are providing us with remarkable information about the <span class="hlt">ice</span> sheet, the sea <span class="hlt">ice</span>, and the ozone hole. Satellite visible and radar imagery are providing views of the large scale structure of the <span class="hlt">ice</span> sheet never seen before; satellite laser altimetry has produced detailed maps of the topography of the <span class="hlt">ice</span> sheet; and an innovative gravity-measuring two-part satellite has allowed mapping of regions of mass loss and mass gain on the <span class="hlt">ice</span> sheet. The surrounding sea <span class="hlt">ice</span> <span class="hlt">cover</span> has a satellite record that goes back to the 1970s, allowing trend studies that show a decreasing sea <span class="hlt">ice</span> presence in the region of the Bellingshausen and Amundsen seas, to the west of the prominent <span class="hlt">Antarctic</span> Peninsula, but increasing sea <span class="hlt">ice</span> presence around much of the rest of the continent. Overall, sea <span class="hlt">ice</span> extent around Antarctica has increased at an average rate of about 17,000 square kilometers per year since the late 1970s, as determined from satellite microwave data that can be collected under both light and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/1000536','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/1000536"><span>ROV dives under Great <span class="hlt">Lakes</span> <span class="hlt">ice</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>Bolsenga, S.J.; Gannon, John E.; Kennedy, Gregory; Norton, D.C.; Herdendorf, Charles E.</p> <p>1989-01-01</p> <p>Observations of the underside of <span class="hlt">ice</span> have a wide variety of applications. Severe under-<span class="hlt">ice</span> roughness can affect <span class="hlt">ice</span> movements, rough under-<span class="hlt">ice</span> surfaces can scour the bottom disturbing biota and man-made structures such as pipelines, and the flow rate of rivers is often affected by under-<span class="hlt">ice</span> roughness. A few reported observations of the underside of an <span class="hlt">ice</span> <span class="hlt">cover</span> have been made, usually by cutting a large block of <span class="hlt">ice</span> and overturning it, by extensive boring, or by remote sensing. Such operations are extremely labor-intensive and, in some cases, prone to inaccuracies. Remotely operated vehicles (ROV) can partially solve these problems. In this note, we describe the use, performance in a hostile environment, and results of a study in which a ROV was deployed under the <span class="hlt">ice</span> in <span class="hlt">Lake</span> Erie (North American Great <span class="hlt">Lakes</span>).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.B31D2022S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.B31D2022S"><span>Developing A Model for <span class="hlt">Lake</span> <span class="hlt">Ice</span> Phenology Using Satellite Remote Sensing Observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Skoglund, S. K.; Weathers, K. C.; Norouzi, H.; Prakash, S.; Ewing, H. A.</p> <p>2017-12-01</p> <p>Many northern temperate freshwater <span class="hlt">lakes</span> are freezing over later and thawing earlier. This shift in timing, and the resulting shorter duration of seasonal <span class="hlt">ice</span> <span class="hlt">cover</span>, is expected to impact ecological processes, negatively affecting aquatic species and the quality of water we drink. Long-term, direct observations have been used to analyze changes in <span class="hlt">ice</span> phenology, but those data are sparse relative to the number of <span class="hlt">lakes</span> affected. Here we develop a model to utilize remote sensing data in approximating the dates of <span class="hlt">ice</span>-on and <span class="hlt">ice</span>-off for many years over a variety of <span class="hlt">lakes</span>. Day and night surface temperatures from MODIS (Moderate Resolution Imaging Spectroradiometer) Aqua and Terra (MYD11A1 and MOD11A1 data products) for 2002-2017 were utilized in combination with observed <span class="hlt">ice</span>-on and <span class="hlt">ice</span>-off dates of <span class="hlt">Lake</span> Auburn, Maine, to determine the ability of MODIS data to match ground-based observations. A moving average served to interpolate MODIS temperature data to fill data gaps from cloudy days. The nighttime data were used for <span class="hlt">ice</span>-off, and the daytime measurements were used for <span class="hlt">ice</span>-on predictions to avoid fluctuations between day and night <span class="hlt">ice</span>/water status. The 0˚C intercepts of those data were used to mark approximate days of <span class="hlt">ice</span>-on or <span class="hlt">ice</span>-off. This revealed that approximations for <span class="hlt">ice</span>-off dates were satisfactory (average ±8.2 days) for <span class="hlt">Lake</span> Auburn as well as for <span class="hlt">Lake</span> Sunapee, New Hampshire (average ±8.1 days), while approximations for <span class="hlt">Lake</span> Auburn <span class="hlt">ice</span>-on were less accurate and showed consistently earlier-than-observed <span class="hlt">ice</span>-on dates (average -33.8 days). The comparison of observed and remotely sensed <span class="hlt">Lake</span> Auburn <span class="hlt">ice</span> <span class="hlt">cover</span> duration showed relative agreement with a correlation coefficient of 0.46. Other remote sensing observations, such as the new GOES-R satellite, and further exploration of the <span class="hlt">ice</span> formation process can improve <span class="hlt">ice</span>-on approximation methods. The model shows promise for estimating <span class="hlt">ice</span>-on, <span class="hlt">ice</span>-off, and <span class="hlt">ice</span> <span class="hlt">cover</span> duration for northern temperate <span class="hlt">lakes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.C33A0376M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.C33A0376M"><span>Response of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet to ocean forcing using the POPSICLES coupled <span class="hlt">ice</span> sheet-ocean model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Martin, D. F.; Asay-Davis, X.; Price, S. F.; Cornford, S. L.; Maltrud, M. E.; Ng, E. G.; Collins, W.</p> <p>2014-12-01</p> <p>We present the response of the continental <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet to sub-shelf-melt forcing derived from POPSICLES simulation results <span class="hlt">covering</span> the full <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet and the Southern Ocean spanning the period 1990 to 2010. Simulations are performed at 0.1 degree (~5 km) ocean resolution and <span class="hlt">ice</span> sheet resolution as fine as 500 m using adaptive mesh refinement. A comparison of fully-coupled and comparable standalone <span class="hlt">ice</span>-sheet model results demonstrates the importance of two-way coupling between the <span class="hlt">ice</span> sheet and the ocean. The POPSICLES model couples the POP2x ocean model, a modified version of the Parallel Ocean Program (Smith and Gent, 2002), and the BISICLES <span class="hlt">ice</span>-sheet model (Cornford et al., 2012). BISICLES makes use of adaptive mesh refinement to fully resolve dynamically-important regions like grounding lines and employs a momentum balance similar to the vertically-integrated formulation of Schoof and Hindmarsh (2009). Results of BISICLES simulations have compared favorably to comparable simulations with a Stokes momentum balance in both idealized tests like MISMIP3D (Pattyn et al., 2013) and realistic configurations (Favier et al. 2014). POP2x includes sub-<span class="hlt">ice</span>-shelf circulation using partial top cells (Losch, 2008) and boundary layer physics following Holland and Jenkins (1999), Jenkins (2001), and Jenkins et al. (2010). Standalone POP2x output compares well with standard <span class="hlt">ice</span>-ocean test cases (e.g., ISOMIP; Losch, 2008) and other continental-scale simulations and melt-rate observations (Kimura et al., 2013; Rignot et al., 2013). A companion presentation, "Present-day circum-<span class="hlt">Antarctic</span> simulations using the POPSICLES coupled land <span class="hlt">ice</span>-ocean model" in session C027 describes the ocean-model perspective of this work, while we focus on the response of the <span class="hlt">ice</span> sheet and on details of the model. The figure shows the BISICLES-computed vertically-integrated <span class="hlt">ice</span> velocity field about 1 month into a 20-year coupled <span class="hlt">Antarctic</span> run. Groundling lines are shown in green.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFM.C54A..01B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFM.C54A..01B"><span>The Distribution of <span class="hlt">Antarctic</span> Subglacial <span class="hlt">Lake</span> Environments With Implications for Their Origin and Evolution</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.; Young, D. A.; Carter, S. P.</p> <p>2006-12-01</p> <p><span class="hlt">Ice</span>-penetrating radar records across the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet show regions with strong flat mirror-like reflections from the subglacial interface that are interpreted to be from subglacial <span class="hlt">lakes</span>. The majority of subglacial <span class="hlt">lakes</span> are found in East Antarctica, primarily in topographically low areas of basins beneath the thick <span class="hlt">ice</span> divides. Occasionally <span class="hlt">lakes</span> are observed "perched" at higher elevations within local depressions of rough morphological regions. In addition, a correlation between the "onset" of enhanced glacial flow and subglacial <span class="hlt">lakes</span> was identified. The greatest concentration of known <span class="hlt">lakes</span> was found in the vicinity of Dome C. A second grouping of <span class="hlt">lakes</span> lying near Ridge B includes <span class="hlt">Lake</span> Vostok and several smaller <span class="hlt">lakes</span>. Subglacial <span class="hlt">lakes</span> were also discovered near the South Pole, within eastern Wilkes Land, west of the Transantarctic Mountains, and within West Antarctica's Whitmore Mountains. Aside from <span class="hlt">Lake</span> Vostok, typical lengths of subglacial <span class="hlt">lakes</span> were found to range from a few to about 20 kilometers. A recent inventory includes 145 subglacial <span class="hlt">lakes</span>. Approximately 81% of detected <span class="hlt">lakes</span> lie at elevations less than a few hundred meters above sea level while the majority of the remaining <span class="hlt">lakes</span> are "perched" at higher elevations. We present the locations from the subglacial <span class="hlt">lake</span> inventory on local "<span class="hlt">ice</span> divides" calculated from the satellite derived surface elevations with and find the distance of each <span class="hlt">lake</span> from these divides. Most significantly, we found that 66% of the <span class="hlt">lakes</span> identified lie within 50 km of a local <span class="hlt">ice</span> divide and 88% lie within 100 km of a local divide. In particular, note that <span class="hlt">lakes</span> located far from the Dome C/Ridge B cluster and even those associated with very narrow catchments lie either on or within a few tens of kilometers of the local divide marked by the catchment boundary. The distance correlation of subglacial <span class="hlt">lakes</span> with local <span class="hlt">ice</span> divides leads to a fundamental question for the evolution of subglacial <span class="hlt">lake</span> environments: Does the</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> <span class="hlt">Ice</span> Streams: Analog to <span class="hlt">Ice</span> 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 <span class="hlt">Ice</span> Shelf in Antarctica recently revealed large persistent patterns of longitudinal megaflutes and drumlinoid forms, which are interpreted to have formed at the base of <span class="hlt">ice</span> 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> <span class="hlt">ice</span> streams and outflow channels. <span class="hlt">Ice</span> streams are 30 to 80 km wide and hundreds of kilometers long, as are the martian channels. <span class="hlt">Ice</span> 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> <span class="hlt">ice</span> 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 <span class="hlt">ice</span> 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 <span class="hlt">ice</span> that left a conspicuous morphologic imprint. Unlike the West-<span class="hlt">Antarctic-ice</span> streams, which discharge <span class="hlt">ice</span> from an <span class="hlt">ice</span> sheet, <span class="hlt">ice</span> in the martian channels came from water erupting from the ground. In the cold martian environment, this water, if of moderate volume, would eventually freeze. Thus it may have formed <span class="hlt">icings</span> on springs, <span class="hlt">ice</span> dams and jams on constrictions in the channel path, or frozen pools. Given sufficient thickness and downhill surface gradient, these <span class="hlt">ice</span> masses would have moved; and given the right conditions, they could have moved like <span class="hlt">Antarctic</span> <span class="hlt">ice</span> streams.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1990JGR....9513411C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1990JGR....9513411C"><span>Arctic multiyear <span class="hlt">ice</span> classification and summer <span class="hlt">ice</span> <span class="hlt">cover</span> using passive microwave satellite data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Comiso, J. C.</p> <p>1990-08-01</p> <p>The ability to classify and monitor Arctic multiyear sea <span class="hlt">ice</span> <span class="hlt">cover</span> using multispectral passive microwave data is studied. Sea <span class="hlt">ice</span> concentration maps during several summer minima have been analyzed to obtain estimates of <span class="hlt">ice</span> surviving the summer. The results are compared with multiyear <span class="hlt">ice</span> concentrations derived from data the following winter, using an algorithm that assumes a certain emissivity for multiyear <span class="hlt">ice</span>. The multiyear <span class="hlt">ice</span> <span class="hlt">cover</span> inferred from the winter data is approximately 25 to 40% less than the summer <span class="hlt">ice</span> <span class="hlt">cover</span> minimum, suggesting that even during winter when the emissivity of sea <span class="hlt">ice</span> is most stable, passive microwave data may account for only a fraction of the total multiyear <span class="hlt">ice</span> <span class="hlt">cover</span>. The difference of about 2×106 km2 is considerably more than estimates of advection through Fram Strait during the intervening period. It appears that as in the <span class="hlt">Antarctic</span>, some multiyear <span class="hlt">ice</span> floes in the Arctic, especially those near the summer marginal <span class="hlt">ice</span> zone, have first-year <span class="hlt">ice</span> or intermediate signatures in the subsequent winter. A likely mechanism for this is the intrusion of seawater into the snow-<span class="hlt">ice</span> interface, which often occurs near the marginal <span class="hlt">ice</span> zone or in areas where snow load is heavy. Spatial variations in melt and melt ponding effects also contribute to the complexity of the microwave emissivity of multiyear <span class="hlt">ice</span>. Hence the multiyear <span class="hlt">ice</span> data should be studied in conjunction with the previous summer <span class="hlt">ice</span> data to obtain a more complete characterization of the state of the Arctic <span class="hlt">ice</span> <span class="hlt">cover</span>. The total extent and actual areas of the summertime Arctic pack <span class="hlt">ice</span> were estimated to be 8.4×106 km2 and 6.2×106 km2, respectively, and exhibit small interannual variability during the years 1979 through 1985, suggesting a relatively stable <span class="hlt">ice</span> <span class="hlt">cover</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.C34B..07A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.C34B..07A"><span>Present-day Circum-<span class="hlt">Antarctic</span> Simulations using the POPSICLES Coupled <span class="hlt">Ice</span> Sheet-Ocean Model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Asay-Davis, X.; Martin, D. F.; Price, S. F.; Maltrud, M. E.; Collins, W.</p> <p>2014-12-01</p> <p>We present POPSICLES simulation results <span class="hlt">covering</span> the full <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet and the Southern Ocean spanning the period 1990 to 2010. Simulations are performed at 0.1o (~5 km) ocean resolution and with adaptive <span class="hlt">ice</span>-sheet model resolution as fine as 500 m. We compare time-averaged melt rates below a number of major <span class="hlt">ice</span> shelves with those reported by Rignot et al. (2013) as well as other recent studies. We also present seasonal variability and decadal trends in submarine melting from several <span class="hlt">Antarctic</span> regions. Finally, we explore the influence on basal melting and system dynamics resulting from two different choices of climate forcing: a "normal-year" climatology and the CORE v. 2 forcing data (Large and Yeager 2008).POPSICLES couples the POP2x ocean model, a modified version of the Parallel Ocean Program (Smith and Gent, 2002), and the BISICLES <span class="hlt">ice</span>-sheet model (Cornford et al., 2012). POP2x includes sub-<span class="hlt">ice</span>-shelf circulation using partial top cells (Losch, 2008) and boundary layer physics following Holland and Jenkins (1999), Jenkins (2001), and Jenkins et al. (2010). Standalone POP2x output compares well with standard <span class="hlt">ice</span>-ocean test cases (e.g., ISOMIP; Losch, 2008) and other continental-scale simulations and melt-rate observations (Kimura et al., 2013; Rignot et al., 2013). BISICLES makes use of adaptive mesh refinement and a 1st-order accurate momentum balance similar to the L1L2 model of Schoof and Hindmarsh (2009) to accurately model regions of dynamic complexity, such as <span class="hlt">ice</span> streams, outlet glaciers, and grounding lines. Results of BISICLES simulations have compared favorably to comparable simulations with a Stokes momentum balance in both idealized tests (MISMIP-3D; Pattyn et al., 2013) and realistic configurations (Favier et al. 2014).A companion presentation, "Response of the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet to ocean forcing using the POPSICLES coupled <span class="hlt">ice</span> sheet-ocean model" in session C024 <span class="hlt">covers</span> the <span class="hlt">ice</span>-sheet response to these melt rates in the coupled simulation</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ISPAn.IV2..311X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ISPAn.IV2..311X"><span><span class="hlt">Lake</span> <span class="hlt">Ice</span> Monitoring with Webcams</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xiao, M.; Rothermel, M.; Tom, M.; Galliani, S.; Baltsavias, E.; Schindler, K.</p> <p>2018-05-01</p> <p>Continuous monitoring of climate indicators is important for understanding the dynamics and trends of the climate system. <span class="hlt">Lake</span> <span class="hlt">ice</span> has been identified as one such indicator, and has been included in the list of Essential Climate Variables (ECVs). Currently there are two main ways to survey <span class="hlt">lake</span> <span class="hlt">ice</span> <span class="hlt">cover</span> and its change over time, in-situ measurements and satellite remote sensing. The challenge with both of them is to ensure sufficient spatial and temporal resolution. Here, we investigate the possibility to monitor <span class="hlt">lake</span> <span class="hlt">ice</span> with video streams acquired by publicly available webcams. Main advantages of webcams are their high temporal frequency and dense spatial sampling. By contrast, they have low spectral resolution and limited image quality. Moreover, the uncontrolled radiometry and low, oblique viewpoints result in heavily varying appearance of water, <span class="hlt">ice</span> and snow. We present a workflow for pixel-wise semantic segmentation of images into these classes, based on state-of-the-art encoder-decoder Convolutional Neural Networks (CNNs). The proposed segmentation pipeline is evaluated on two sequences featuring different ground sampling distances. The experiment suggests that (networks of) webcams have great potential for <span class="hlt">lake</span> <span class="hlt">ice</span> monitoring. The overall per-pixel accuracies for both tested data sets exceed 95 %. Furthermore, per-image discrimination between <span class="hlt">ice</span>-on and <span class="hlt">ice</span>-off conditions, derived by accumulating per-pixel results, is 100 % correct for our test data, making it possible to precisely recover freezing and thawing dates.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70016789','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70016789"><span>Simulation of <span class="hlt">lake</span> <span class="hlt">ice</span> and its effect on the late-Pleistocene evaporation rate of <span class="hlt">Lake</span> Lahontan</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Hostetler, S.W.</p> <p>1991-01-01</p> <p>A model of <span class="hlt">lake</span> <span class="hlt">ice</span> was coupled with a model of <span class="hlt">lake</span> temperature and evaporation to assess the possible effect of <span class="hlt">ice</span> <span class="hlt">cover</span> on the late-Pleistocene evaporation rate of <span class="hlt">Lake</span> Lahontan. The simulations were done using a data set based on proxy temperature indicators and features of the simulated late-Pleistocene atmospheric circulation over western North America. When a data set based on a mean-annual air temperature of 3?? C (7?? C colder than present) and reduced solar radiation from jet-stream induced cloud <span class="hlt">cover</span> was used as input to the model, <span class="hlt">ice</span> <span class="hlt">cover</span> lasting ??? 4 months was simulated. Simulated evaporation rates (490-527 mm a-1) were ??? 60% lower than the present-day evaporation rate (1300 mm a-1) of Pyramid <span class="hlt">Lake</span>. With this reduced rate of evaporation, water inputs similar to the 1983 historical maxima that occurred in the Lahontan basin would have been sufficient to maintain the 13.5 ka BP high stand of <span class="hlt">Lake</span> Lahontan. ?? 1991 Springer-Verlag.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70048808','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70048808"><span>Recent <span class="hlt">lake</span> <span class="hlt">ice</span>-out phenology within and among <span class="hlt">lake</span> districts of Alaska, U.S.A.</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Arp, Christopher D.; Jones, Benjamin M.; Grosse, Guido</p> <p>2013-01-01</p> <p>The timing of <span class="hlt">ice</span>-out in high latitudes is a fundamental threshold for <span class="hlt">lake</span> ecosystems and an indicator of climate change. In <span class="hlt">lake</span>-rich regions, the loss of <span class="hlt">ice</span> <span class="hlt">cover</span> also plays a key role in landscape and climatic processes. Thus, there is a need to understand <span class="hlt">lake</span> <span class="hlt">ice</span> phenology at multiple scales. In this study, we observed <span class="hlt">ice</span>-out timing on 55 large <span class="hlt">lakes</span> in 11 <span class="hlt">lake</span> districts across Alaska from 2007 to 2012 using satellite imagery. Sensor networks in two <span class="hlt">lake</span> districts validated satellite observations and provided comparison with smaller <span class="hlt">lakes</span>. Over this 6 yr period, the mean <span class="hlt">lake</span> <span class="hlt">ice</span>-out for all <span class="hlt">lakes</span> was 27 May and ranged from 07 May in Kenai to 06 July in Arctic Coastal Plain <span class="hlt">lake</span> districts with relatively low inter-annual variability. Approximately 80% of the variation in <span class="hlt">ice</span>-out timing was explained by the date of 0°C air temperature isotherm and <span class="hlt">lake</span> area. Shoreline irregularity, watershed area, and river connectivity explained additional variation in some districts. Coherence in <span class="hlt">ice</span>-out timing within the <span class="hlt">lakes</span> of each district was consistently strong over this 6 yr period, ranging from r-values of 0.5 to 0.9. Inter-district analysis of coherence also showed synchronous <span class="hlt">ice</span>-out patterns with the exception of the two arctic coastal districts where <span class="hlt">ice</span>-out occurs later (June–July) and climatology is sea-<span class="hlt">ice</span> influenced. These patterns of <span class="hlt">lake</span> <span class="hlt">ice</span> phenology provide a spatially extensive baseline describing short-term temporal variability, which will help decipher longer term trends in <span class="hlt">ice</span> phenology and aid in representing the role of <span class="hlt">lake</span> <span class="hlt">ice</span> in land and climate models in northern landscapes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.C21B0326B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.C21B0326B"><span><span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Mass Balance from GRACE</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Boening, C.; Firing, Y. L.; Wiese, D. N.; Watkins, M. M.; Schlegel, N.; Larour, E. Y.</p> <p>2014-12-01</p> <p>The <span class="hlt">Antarctic</span> <span class="hlt">ice</span> mass balance and rates of change of <span class="hlt">ice</span> mass over the past decade are analyzed based on observations from the Gravity Recovery and Climate Experiment (GRACE) satellites, in the form of JPL RL05M mascon solutions. Surface mass balance (SMB) fluxes from ERA-Interim and other atmospheric reanalyses successfully account for the seasonal GRACE-measured mass variability, and explain 70-80% of the continent-wide mass variance at interannual time scales. Trends in the residual (GRACE mass - SMB accumulation) mass time series in different <span class="hlt">Antarctic</span> drainage basins are consistent with time-mean <span class="hlt">ice</span> discharge rates based on radar-derived <span class="hlt">ice</span> velocities and thicknesses. GRACE also resolves accelerations in regional <span class="hlt">ice</span> mass change rates, including increasing rates of mass gain in East Antarctica and accelerating <span class="hlt">ice</span> mass loss in West Antarctica. The observed East <span class="hlt">Antarctic</span> mass gain is only partially explained by anomalously large SMB events in the second half of the record, potentially implying that <span class="hlt">ice</span> discharge rates are also decreasing in this region. Most of the increasing mass loss rate in West Antarctica, meanwhile, is explained by decreasing SMB (principally precipitation) over this time period, part of the characteristic decadal variability in regional SMB. The residual acceleration of 2+/-1 Gt/yr, which is concentrated in the Amundsen Sea Embayment (ASE) basins, represents the contribution from increasing <span class="hlt">ice</span> discharge rates. An <span class="hlt">Ice</span> Sheet System Model (ISSM) run with constant ocean forcing and stationary grounding lines both underpredicts the largest trends in the ASE and produces negligible acceleration or interannual variability in discharge, highlighting the potential importance of ocean forcing for setting <span class="hlt">ice</span> discharge rates at interannual to decadal time scales.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012RvGeo..50.1003S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012RvGeo..50.1003S"><span>Clean access, measurement, and sampling of Ellsworth Subglacial <span class="hlt">Lake</span>: A method for exploring deep <span class="hlt">Antarctic</span> subglacial <span class="hlt">lake</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>Siegert, Martin J.; Clarke, Rachel J.; Mowlem, Matt; Ross, Neil; Hill, Christopher S.; Tait, Andrew; Hodgson, Dominic; Parnell, John; Tranter, Martyn; Pearce, David; Bentley, Michael J.; Cockell, Charles; Tsaloglou, Maria-Nefeli; Smith, Andy; Woodward, John; Brito, Mario P.; Waugh, Ed</p> <p>2012-01-01</p> <p><span class="hlt">Antarctic</span> subglacial <span class="hlt">lakes</span> are thought to be extreme habitats for microbial life and may contain important records of <span class="hlt">ice</span> sheet history and climate change within their <span class="hlt">lake</span> floor sediments. To find whether or not this is true, and to answer the science questions that would follow, direct measurement and sampling of these environments are required. Ever since the water depth of Vostok Subglacial <span class="hlt">Lake</span> was shown to be >500 m, attention has been given to how these unique, ancient, and pristine environments may be entered without contamination and adverse disturbance. Several organizations have offered guidelines on the desirable cleanliness and sterility requirements for direct sampling experiments, including the U.S. National Academy of Sciences and the Scientific Committee on <span class="hlt">Antarctic</span> Research. Here we summarize the scientific protocols and methods being developed for the exploration of Ellsworth Subglacial <span class="hlt">Lake</span> in West Antarctica, planned for 2012-2013, which we offer as a guide to future subglacial environment research missions. The proposed exploration involves accessing the <span class="hlt">lake</span> using a hot-water drill and deploying a sampling probe and sediment corer to allow sample collection. We focus here on how this can be undertaken with minimal environmental impact while maximizing scientific return without compromising the environment for future experiments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1197863-modeling-impediment-methane-ebullition-bubbles-seasonal-lake-ice','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1197863-modeling-impediment-methane-ebullition-bubbles-seasonal-lake-ice"><span>Modeling the impediment of methane ebullition bubbles by seasonal <span class="hlt">lake</span> <span class="hlt">ice</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Greene, S.; Walter Anthony, K. M.; Archer, D.</p> <p></p> <p>Microbial methane (CH 4) ebullition (bubbling) from anoxic <span class="hlt">lake</span> sediments comprises a globally significant flux to the atmosphere, but ebullition bubbles in temperate and polar <span class="hlt">lakes</span> can be trapped by winter <span class="hlt">ice</span> <span class="hlt">cover</span> and later released during spring thaw. This "<span class="hlt">ice</span>-bubble storage" (IBS) constitutes a novel mode of CH 4 emission. Before bubbles are encapsulated by downward-growing <span class="hlt">ice</span>, some of their CH 4 dissolves into the <span class="hlt">lake</span> water, where it may be subject to oxidation. We present field characterization and a model of the annual CH 4 cycle in Goldstream <span class="hlt">Lake</span>, a thermokarst (thaw) <span class="hlt">lake</span> in interior Alaska. We findmore » that summertime ebullition dominates annual CH 4 emissions to the atmosphere. Eighty percent of CH 4 in bubbles trapped by <span class="hlt">ice</span> dissolves into the <span class="hlt">lake</span> water column in winter, and about half of that is oxidized. The <span class="hlt">ice</span> growth rate and the magnitude of the CH 4 ebullition flux are important controlling factors of bubble dissolution. Seven percent of annual ebullition CH 4 is trapped as IBS and later emitted as <span class="hlt">ice</span> melts. In a future warmer climate, there will likely be less seasonal <span class="hlt">ice</span> <span class="hlt">cover</span>, less IBS, less CH 4 dissolution from trapped bubbles, and greater CH 4 emissions from northern <span class="hlt">lakes</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1197863-modeling-impediment-methane-ebullition-bubbles-seasonal-lake-ice','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1197863-modeling-impediment-methane-ebullition-bubbles-seasonal-lake-ice"><span>Modeling the impediment of methane ebullition bubbles by seasonal <span class="hlt">lake</span> <span class="hlt">ice</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Greene, S.; Walter Anthony, K. M.; Archer, D.; ...</p> <p>2014-12-08</p> <p>Microbial methane (CH 4) ebullition (bubbling) from anoxic <span class="hlt">lake</span> sediments comprises a globally significant flux to the atmosphere, but ebullition bubbles in temperate and polar <span class="hlt">lakes</span> can be trapped by winter <span class="hlt">ice</span> <span class="hlt">cover</span> and later released during spring thaw. This "<span class="hlt">ice</span>-bubble storage" (IBS) constitutes a novel mode of CH 4 emission. Before bubbles are encapsulated by downward-growing <span class="hlt">ice</span>, some of their CH 4 dissolves into the <span class="hlt">lake</span> water, where it may be subject to oxidation. We present field characterization and a model of the annual CH 4 cycle in Goldstream <span class="hlt">Lake</span>, a thermokarst (thaw) <span class="hlt">lake</span> in interior Alaska. We findmore » that summertime ebullition dominates annual CH 4 emissions to the atmosphere. Eighty percent of CH 4 in bubbles trapped by <span class="hlt">ice</span> dissolves into the <span class="hlt">lake</span> water column in winter, and about half of that is oxidized. The <span class="hlt">ice</span> growth rate and the magnitude of the CH 4 ebullition flux are important controlling factors of bubble dissolution. Seven percent of annual ebullition CH 4 is trapped as IBS and later emitted as <span class="hlt">ice</span> melts. In a future warmer climate, there will likely be less seasonal <span class="hlt">ice</span> <span class="hlt">cover</span>, less IBS, less CH 4 dissolution from trapped bubbles, and greater CH 4 emissions from northern <span class="hlt">lakes</span>.« less</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_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('https://www.ncbi.nlm.nih.gov/pubmed/20890841','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20890841"><span>A close link between bacterial community composition and environmental heterogeneity in maritime <span class="hlt">Antarctic</span> <span class="hlt">lakes</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Villaescusa, Juan A; Casamayor, Emilio O; Rochera, Carlos; Velázquez, David; Chicote, Alvaro; Quesada, Antonio; Camacho, Antonio</p> <p>2010-06-01</p> <p>Seven maritime <span class="hlt">Antarctic</span> <span class="hlt">lakes</span> located on Byers Peninsula (Livingston Island, South Shetland Islands) were surveyed to determine the relationship between planktonic bacterial community composition and environmental features. Specifically, the extent to which factors other than low temperature determine the composition of bacterioplankton assemblages of maritime <span class="hlt">Antarctic</span> <span class="hlt">lakes</span> was evaluated. Both deep and shallow <span class="hlt">lakes</span> in the central plateau of the Peninsula, as well as a coastal <span class="hlt">lake</span>, were studied in order to fully account for the environmental heterogeneity of the Peninsula's <span class="hlt">lakes</span>. The results showed that shallow coastal <span class="hlt">lakes</span> display eutrophic conditions, mainly due to the influence of marine animals, whereas plateau <span class="hlt">lakes</span> are generally deeper and most are oligotrophic, with very limited inputs of nutrients and organic matter. Meso-eutrophic shallow <span class="hlt">lakes</span> are also present on the Peninsula; they contain microbial mats and a higher trophic status because of the biologically mediated active nutrient release from the sediments. Diversity studies of the <span class="hlt">lakes</span>' planktonic bacterial communities using molecular techniques showed that bacterial diversity is lower in eutrophic than in oligotrophic <span class="hlt">lakes</span>. The former also differed in community composition with respect to dominant taxa. Multivariate statistical analyses of environmental data yielded the same clustering of <span class="hlt">lakes</span> as obtained based on the DGGE band pattern after DNA extraction and amplification of 16S rRNA gene fragments. Thus, even in extremely cold <span class="hlt">lakes</span>, the bacterial community composition parallels other environmental factors, such as those related to trophic status. This correspondence is not only mediated by the influence of marine fauna but also by processes including sediment and <span class="hlt">ice</span> melting dynamics. The bacterial community can therefore be considered to be equally representative as environmental abiotic variables in demonstrating the environmental heterogeneity among maritime <span class="hlt">Antarctic</span> <span class="hlt">lakes</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 <span class="hlt">Ice</span> 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 <span class="hlt">ice</span>, 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 <span class="hlt">ice</span> reduction on photochemical processes, transport, and distribution in the polar environment. In spring 2013, there was further loss of perennial sea <span class="hlt">ice</span>, as it was not observed in the ocean region adjacent to the Alaskan north coast, where there was a stretch of perennial sea <span class="hlt">ice</span> in 2012 in the Beaufort Sea and Chukchi Sea. In contrast to the rapid and extensive loss of sea <span class="hlt">ice</span> in the Arctic, <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> 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 <span class="hlt">ice</span> may arguably be considered as having a low confidence level; however, there was no overall reduction of <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> extent anywhere close to the decreasing rate of Arctic sea <span class="hlt">ice</span>. There exist publications presenting various factors driving changes in Arctic and <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span>. After a short review of these published factors, new observations and atmospheric, oceanic, hydrological, and geological mechanisms contributed to different behaviors of sea <span class="hlt">ice</span> 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 <span class="hlt">ice</span> 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 <span class="hlt">ice</span> changes. Furthermore, similarities and differences in chemical impacts of Arctic and <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> changes are discussed. Understanding sea <span class="hlt">ice</span> changes and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29547924','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29547924"><span>Community structure and distribution of benthic cyanobacteria in <span class="hlt">Antarctic</span> lacustrine microbial mats.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Pessi, Igor S; Lara, Yannick; Durieu, Benoit; Maalouf, Pedro de C; Verleyen, Elie; Wilmotte, Annick</p> <p>2018-05-01</p> <p>The terrestrial <span class="hlt">Antarctic</span> Realm has recently been divided into 16 <span class="hlt">Antarctic</span> Conservation Biogeographic Regions (ACBRs) based on environmental properties and the distribution of biota. Despite their prominent role in the primary production and nutrient cycling in <span class="hlt">Antarctic</span> <span class="hlt">lakes</span>, cyanobacteria were only poorly represented in the biological dataset used to delineate these ACBRs. Here, we provide a first high-throughput sequencing insight into the spatial distribution of benthic cyanobacterial communities in <span class="hlt">Antarctic</span> <span class="hlt">lakes</span> located in four distinct, geographically distant ACBRs and <span class="hlt">covering</span> a range of limnological conditions. Cyanobacterial community structure differed between saline and freshwater <span class="hlt">lakes</span>. No clear bioregionalization was observed, as clusters of community similarity encompassed <span class="hlt">lakes</span> from distinct ACBRs. Most phylotypes (77.0%) were related to cyanobacterial lineages (defined at ≥99.0% 16S rRNA gene sequence similarity) restricted to the cold biosphere, including lineages potentially endemic to Antarctica (55.4%). The latter were generally rare and restricted to a small number of <span class="hlt">lakes</span>, while more ubiquitous phylotypes were generally abundant and present in different ACBRs. These results point to a widespread distribution of some cosmopolitan cyanobacterial phylotypes across the different <span class="hlt">Antarctic</span> <span class="hlt">ice</span>-free regions, but also suggest the existence of dispersal barriers both within and between Antarctica and the other continents.</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> <span class="hlt">ice</span> 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 <span class="hlt">ice</span> ages, fundamental questions remain over the response of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheets to orbital cycles. Furthermore, an understanding of the behaviour of the marine-based West <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet (WAIS) during the 'warmer-than-present' early-Pliocene epoch ( approximately 5-3 Myr ago) is needed to better constrain the possible range of <span class="hlt">ice</span>-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 <span class="hlt">ice</span> shelf by the ANDRILL programme and demonstrate well-dated, approximately 40-kyr cyclic variations in <span class="hlt">ice</span>-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 <span class="hlt">ice</span>, or <span class="hlt">ice</span> shelves, to open waters 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 <span class="hlt">ice-sheet/ice</span>-shelf model that simulates fluctuations in <span class="hlt">Antarctic</span> <span class="hlt">ice</span> 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> <span class="hlt">ice</span> sheet, in response to ocean-induced melting paced by obliquity. During interglacial times, diatomaceous sediments indicate high surface-water productivity, minimal summer sea <span class="hlt">ice</span> 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('http://hdl.handle.net/2060/20010027899','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20010027899"><span>Studies of <span class="hlt">Antarctic</span> Sea <span class="hlt">Ice</span> Concentrations from Satellite Data and Their Applications</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.; Steffen, Konrad; Zukor, Dorothy J. (Technical Monitor)</p> <p>2001-01-01</p> <p>Large changes in the sea <span class="hlt">ice</span> <span class="hlt">cover</span> have been observed recently. Because of the relevance of such changes to climate change studies it is important that key <span class="hlt">ice</span> concentration data sets used for evaluating such changes are interpreted properly. High and medium resolution visible and infrared satellite data are used in conjunction with passive microwave data to study the true characteristics of the <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> <span class="hlt">cover</span>, assess errors in currently available <span class="hlt">ice</span> concentration products, and evaluate the applications and limitations of the latter in polar process studies. Cloud-free high resolution data provide valuable information about the natural distribution, stage of formation, and composition of the <span class="hlt">ice</span> <span class="hlt">cover</span> that enables interpretation of the large spatial and temporal variability of the microwave emissivity of <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span>. Comparative analyses of co-registered visible, infrared and microwave data were used to evaluate <span class="hlt">ice</span> concentrations derived from standard <span class="hlt">ice</span> algorithms (i.e., Bootstrap and Team) and investigate the 10 to 35% difference in derived values from large areas within the <span class="hlt">ice</span> pack, especially in the Weddell Sea, Amundsen Sea, and Ross Sea regions. Landsat and OLS data show a predominance of thick consolidated <span class="hlt">ice</span> in these areas and show good agreement with the Bootstrap Algorithm. While direct measurements were not possible, the lower values from the Team Algorithm results are likely due to layering within the <span class="hlt">ice</span> and snow and/or surface flooding, which are known to affect the polarization ratio. In predominantly new <span class="hlt">ice</span> regions, the derived <span class="hlt">ice</span> concentration from passive microwave data is usually lower than the true percentage because the emissivity of new <span class="hlt">ice</span> changes with age and thickness and is lower than that of thick <span class="hlt">ice</span>. However, the product provides a more realistic characterization of the sea <span class="hlt">ice</span> <span class="hlt">cover</span>, and are more useful in polar process studies since it allows for the identification of areas of significant divergence and polynya</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C24C..01B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C24C..01B"><span>Flexural-response of the McMurdo <span class="hlt">Ice</span> Shelf to surface <span class="hlt">lake</span> filling and drainage</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Banwell, A. F.; MacAyeal, D. R.; Willis, I.; Macdonald, G. J.; Goodsell, B.</p> <p>2017-12-01</p> <p><span class="hlt">Antarctic</span> <span class="hlt">ice</span>-shelf instability and break-up, as exhibited by the Larsen B <span class="hlt">ice</span> shelf in 2002, remains one of the most difficult glaciological processes to observe directly. It is, however, vital to do so because <span class="hlt">ice</span>-shelf breakup has the potential to influence the buttressing controls on inland <span class="hlt">ice</span> discharge, and thus to affect sea level. Several mechanisms enabling Larsen B style breakup have previously been proposed, including the ability of surface <span class="hlt">lakes</span> to introduce <span class="hlt">ice</span>-shelf fractures when they fill and drain. During the austral summer of 2016/2017, we monitored the filling and draining of four surface <span class="hlt">lakes</span> on the McMurdo <span class="hlt">Ice</span> Shelf, Antarctica, and the effect of these processes on <span class="hlt">ice</span>-shelf flexure. Water-depth data from pressure sensors reveal that two <span class="hlt">lakes</span> filled to >2 m in depth and subsequently drained over multiple week timescales, which had a simultaneous effect on vertical <span class="hlt">ice</span> deflection in the area. Differential GPS data from 12 receivers over three months show that vertical deflection varies as a function of distance from the maximum load change (i.e. at the <span class="hlt">lake</span> centre). Using remote sensing techniques applied to both Landsat 8 and Worldview imagery, we also quantify the meltwater volume in these two <span class="hlt">lakes</span> through the melt season, which, together with the vertical deflection data, are used to constrain key flexural parameter values in numerical models of <span class="hlt">ice</span>-shelf flexure.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20050179461','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20050179461"><span>Sea <span class="hlt">Ice</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Parkinson, Claire L.; Cavalieri, Donald J.</p> <p>2005-01-01</p> <p>Sea <span class="hlt">ice</span> <span class="hlt">covers</span> vast areas of the polar oceans, with <span class="hlt">ice</span> extent in the Northern Hemisphere ranging from approximately 7 x 10(exp 6) sq km in September to approximately 15 x 10(exp 6) sq km in March and <span class="hlt">ice</span> extent in the Southern Hemisphere ranging from approximately 3 x 10(exp 6) sq km in February to approximately 18 x 10(exp 6) sq km in September. These <span class="hlt">ice</span> <span class="hlt">covers</span> have major impacts on the atmosphere, oceans, and ecosystems of the polar regions, and so as changes occur in them there are potential widespread consequences. Satellite data reveal considerable interannual variability in both polar sea <span class="hlt">ice</span> <span class="hlt">covers</span>, and many studies suggest possible connections between the <span class="hlt">ice</span> and various oscillations within the climate system, such as the Arctic Oscillation, North Atlantic Oscillation, and <span class="hlt">Antarctic</span> Oscillation, or Southern Annular Mode. Nonetheless, statistically significant long-term trends are also apparent, including overall trends of decreased <span class="hlt">ice</span> coverage in the Arctic and increased <span class="hlt">ice</span> coverage in the <span class="hlt">Antarctic</span> from late 1978 through the end of 2003, with the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> increases following marked decreases in the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> during the 1970s. For a detailed picture of the seasonally varying <span class="hlt">ice</span> <span class="hlt">cover</span> at the start of the 21st century, this chapter includes <span class="hlt">ice</span> concentration maps for each month of 2001 for both the Arctic and the <span class="hlt">Antarctic</span>, as well as an overview of what the satellite record has revealed about the two polar <span class="hlt">ice</span> <span class="hlt">covers</span> from the 1970s through 2003.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70191346','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70191346"><span><span class="hlt">Ice</span> duration drives winter nitrate accumulation in north temperate <span class="hlt">lakes</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>Powers, Steven M; Labou, Stephanie G.; Baulch, Helen M.; Hunt, Randall J.; Lottig, Noah R.; Hampton, Stephanie E.; Stanley, Emily H.</p> <p>2017-01-01</p> <p>The duration of winter <span class="hlt">ice</span> <span class="hlt">cover</span> on <span class="hlt">lakes</span> varies substantially with climate variability, and has decreased over the last several decades in many temperate <span class="hlt">lakes</span>. However, little is known of how changes in seasonal <span class="hlt">ice</span> <span class="hlt">cover</span> may affect biogeochemical processes under <span class="hlt">ice</span>. We examined winter nitrogen (N) dynamics under <span class="hlt">ice</span> using a 30+ yr dataset from five oligotrophic/mesotrophic north temperate <span class="hlt">lakes</span> to determine how changes in inorganic N species varied with <span class="hlt">ice</span> duration. Nitrate accumulated during winter and was strongly related to the number of days since <span class="hlt">ice</span>-on. Exogenous inputs accounted for less than 3% of nitrate accumulation in four of the five <span class="hlt">lakes</span>, suggesting a paramount role of nitrification in regulating N transformation and the timing of chemical conditions under <span class="hlt">ice</span>. Winter nitrate accumulation rates ranged from 0.15 μg N L−1 d−1 to 2.7 μg N L−1 d−1 (0.011–0.19 μM d−1), and the mean for intermediate depths was 0.94 μg N L−1 d−1(0.067 μM d−1). Given that winters with shorter <span class="hlt">ice</span> duration (< 120 d) have become more frequent in these <span class="hlt">lakes</span> since the late 1990s, peak winter nitrate concentrations and cumulative nitrate production under <span class="hlt">ice</span> may be declining. As <span class="hlt">ice</span> extent and duration change, the physical and chemical conditions supporting life will shift. This research suggests we may expect changes in the form and amount of inorganic N, and altered dissolved nitrogen : phosphorus ratios, in <span class="hlt">lakes</span> during winters with shorter <span class="hlt">ice</span> duration.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.C53A0279G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.C53A0279G"><span>Rapid Access <span class="hlt">Ice</span> Drill: A New Tool for Exploration of the Deep <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheets and Subglacial Geology</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Goodge, J. W.; Severinghaus, J. P.</p> <p>2014-12-01</p> <p>The Rapid Access <span class="hlt">Ice</span> Drill (RAID) will penetrate the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheets in order to core through deep <span class="hlt">ice</span>, the glacial bed, and into bedrock below. This new technology will provide a critical first look at the interface between major <span class="hlt">ice</span> caps and their subglacial geology. Currently in construction, RAID is a mobile drilling system capable of making several long boreholes in a single field season in Antarctica. RAID is interdisciplinary and will allow access to polar paleoclimate records in <span class="hlt">ice</span> >1 Ma, direct observation at the base of the <span class="hlt">ice</span> sheets, and recovery of rock cores from the <span class="hlt">ice-covered</span> East <span class="hlt">Antarctic</span> craton. RAID uses a diamond rock-coring system as in mineral exploration. Threaded drill-pipe with hardened metal bits will cut through <span class="hlt">ice</span> using reverse circulation of Estisol for pressure-compensation, maintenance of temperature, and removal of <span class="hlt">ice</span> cuttings. Near the bottom of the <span class="hlt">ice</span> sheet, a wireline bottom-hole assembly will enable diamond coring of <span class="hlt">ice</span>, the glacial bed, and bedrock below. Once complete, boreholes will be kept open with fluid, capped, and made available for future down-hole measurement of thermal gradient, heat flow, <span class="hlt">ice</span> chronology, and <span class="hlt">ice</span> deformation. RAID will also sample for extremophile microorganisms. RAID is designed to penetrate up to 3,300 meters of <span class="hlt">ice</span> and take sample cores in less than 200 hours. This rapid performance will allow completion of a borehole in about 10 days before moving to the next drilling site. RAID is unique because it can provide fast borehole access through thick <span class="hlt">ice</span>; take short <span class="hlt">ice</span> cores for paleoclimate study; sample the glacial bed to determine <span class="hlt">ice</span>-flow conditions; take cores of subglacial bedrock for age dating and crustal history; and create boreholes for use as an observatory in the <span class="hlt">ice</span> sheets. Together, the rapid drilling capability and mobility of the drilling system, along with <span class="hlt">ice</span>-penetrating imaging methods, will provide a unique 3D picture of the interior <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheets.</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 <span class="hlt">Ice</span> 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 <span class="hlt">ice</span> 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 <span class="hlt">ice-Antarctic</span> regions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1989QuRes..31..119P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1989QuRes..31..119P"><span>Modeling the growth and decay of the <span class="hlt">Antarctic</span> Peninsula <span class="hlt">Ice</span> Sheet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Payne, A. J.; Sugden, D. E.; Clapperton, C. M.</p> <p>1989-03-01</p> <p>A model of the growth and decay of the <span class="hlt">Antarctic</span> Peninsula <span class="hlt">Ice</span> Sheet during the last glacial/interglacial cycle is used to identify the main controls on <span class="hlt">ice</span> sheet behavior. Using as input glaciological assumptions derived by W. F. Budd and I. N. Smith (1982, Annals of Glaciology3, 42-49), bedrock topography, isostatic compensation, and mass balance relationships, the model is driven by sea-level change over the last 40,000 yr in association with assumed changes in the rate of melting beneath <span class="hlt">ice</span> shelves. An <span class="hlt">ice</span> sheet dome over 3.5 km thick grows on the offshore shelf and straits west of the <span class="hlt">Antarctic</span> Peninsula and reaches a maximum at 18,000 yr B.P. Collapse begins at 14,000 yr B.P. but becomes rapid and continuous after 10,000 yr B.P. The present stable <span class="hlt">ice</span> <span class="hlt">cover</span> is achieved at 6500 yr B.P. <span class="hlt">Ice</span> growth and decay are characterized by thresholds which separate periods of steady state from periods of rapid transition; the thresholds usually relate to topography. Tests show that <span class="hlt">ice</span> sheet behavior is most sensitive to sea-level change, basal marine melting, and accumulation and is less sensitive to isostasy, spatial variation in accumulation, calving rates, and <span class="hlt">ice</span> flow parameterization. Tests of the model against field evidence show good agreement in places, as well as discrepancies which require further work.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018TCry...12..365R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018TCry...12..365R"><span>Consistent biases in <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> concentration simulated by climate models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Roach, Lettie A.; Dean, Samuel M.; Renwick, James A.</p> <p>2018-01-01</p> <p>The simulation of <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> in global climate models often does not agree with observations. In this study, we examine the compactness of sea <span class="hlt">ice</span>, as well as the regional distribution of sea <span class="hlt">ice</span> concentration, in climate models from the latest Coupled Model Intercomparison Project (CMIP5) and in satellite observations. We find substantial differences in concentration values between different sets of satellite observations, particularly at high concentrations, requiring careful treatment when comparing to models. As a fraction of total sea <span class="hlt">ice</span> extent, models simulate too much loose, low-concentration sea <span class="hlt">ice</span> <span class="hlt">cover</span> throughout the year, and too little compact, high-concentration <span class="hlt">cover</span> in the summer. In spite of the differences in physics between models, these tendencies are broadly consistent across the population of 40 CMIP5 simulations, a result not previously highlighted. Separating models with and without an explicit lateral melt term, we find that inclusion of lateral melt may account for overestimation of low-concentration <span class="hlt">cover</span>. Targeted model experiments with a coupled ocean-sea <span class="hlt">ice</span> model show that choice of constant floe diameter in the lateral melt scheme can also impact representation of loose <span class="hlt">ice</span>. This suggests that current sea <span class="hlt">ice</span> thermodynamics contribute to the inadequate simulation of the low-concentration regime in many models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28708127','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28708127"><span>An active bacterial community linked to high chl-a concentrations in <span class="hlt">Antarctic</span> winter-pack <span class="hlt">ice</span> and evidence for the development of an anaerobic sea-<span class="hlt">ice</span> bacterial community.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Eronen-Rasimus, Eeva; Luhtanen, Anne-Mari; Rintala, Janne-Markus; Delille, Bruno; Dieckmann, Gerhard; Karkman, Antti; Tison, Jean-Louis</p> <p>2017-10-01</p> <p><span class="hlt">Antarctic</span> sea-<span class="hlt">ice</span> bacterial community composition and dynamics in various developmental stages were investigated during the austral winter in 2013. Thick snow <span class="hlt">cover</span> likely insulated the <span class="hlt">ice</span>, leading to high (<4 μg l -1 ) chlorophyll-a (chl-a) concentrations and consequent bacterial production. Typical sea-<span class="hlt">ice</span> bacterial genera, for example, Octadecabacter, Polaribacter and Glaciecola, often abundant in spring and summer during the sea-<span class="hlt">ice</span> algal bloom, predominated in the communities. The variability in bacterial community composition in the different <span class="hlt">ice</span> types was mainly explained by the chl-a concentrations, suggesting that as in spring and summer sea <span class="hlt">ice</span>, the sea-<span class="hlt">ice</span> bacteria and algae may also be coupled during the <span class="hlt">Antarctic</span> winter. Coupling between the bacterial community and sea-<span class="hlt">ice</span> algae was further supported by significant correlations between bacterial abundance and production with chl-a. In addition, sulphate-reducing bacteria (for example, Desulforhopalus) together with odour of H 2 S were observed in thick, apparently anoxic <span class="hlt">ice</span>, suggesting that the development of the anaerobic bacterial community may occur in sea <span class="hlt">ice</span> under suitable conditions. In all, the results show that bacterial community in <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> can stay active throughout the winter period and thus possible future warming of sea <span class="hlt">ice</span> and consequent increase in bacterial production may lead to changes in bacteria-mediated processes in the <span class="hlt">Antarctic</span> sea-<span class="hlt">ice</span> zone.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C24C..05S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C24C..05S"><span>Meteorological Drivers of West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet and <span class="hlt">Ice</span> Shelf Surface Melt</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Scott, R. C.; Nicolas, J. P.; Bromwich, D. H.; Norris, J. R.; Lubin, D.</p> <p>2017-12-01</p> <p>We identify synoptic patterns and surface energy balance components driving warming and surface melting on the West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet (WAIS) and <span class="hlt">ice</span> shelves using reanalysis and satellite remote sensing data from 1973-present. We have developed a synoptic climatology of atmospheric circulation patterns during the summer melt season using k-means cluster and composite analysis of daily 700-mb geopotential height and near-surface air temperature and wind fields from the ECMWF ERA-Interim reanalysis. Surface melt occurrence is detected in satellite passive microwave brightness temperature observations (K-band, horizontal polarization) beginning with the NASA Nimbus-5 Electrically Scanning Microwave Radiometer (ESMR) and continuing with its more familiar descendants SMMR, SSM/I and SSMIS. To diagnose synoptic precursors and physical processes driving surface melt we combine the circulation climatology and multi-decadal records of cloud <span class="hlt">cover</span> with surface radiative fluxes from the Extended AVHRR Polar Pathfinder (APP-x) project. We identify three distinct modes of regional summer West <span class="hlt">Antarctic</span> warming since 1979 involving anomalous ridging over West Antarctica (WA) and the Amundsen Sea (AS). During the 1970s, ESMR data reveal four extensive melt events on the Ross Sea sector of the WAIS also linked to AS blocking. We therefore define an Amundsen Sea Blocking Index (ASBI). The ASBI and synoptic circulation pattern occurrence frequencies are correlated with the tropical Pacific (ENSO) and high latitude Southern Annular Mode (SAM) indices and the West <span class="hlt">Antarctic</span> melt index. Surface melt in WA is favored by enhanced downwelling infrared and turbulent sensible heat fluxes associated with intrusions of warm, moist marine air. Consistent with recent findings from the Atmospheric Radiation Measurement (ARM) West <span class="hlt">Antarctic</span> Radiation Experiment (AWARE), marine advection to the Ross sector is favored by El Niño conditions in the tropical Pacific and a negative SAM. We also find</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70012757','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70012757"><span>Ancient <span class="hlt">ice</span> islands in salt <span class="hlt">lakes</span> of the Central Andes</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Hurlbert, S.H.; Chang, Cecily C.Y.</p> <p>1984-01-01</p> <p>Massive blocks of freshwater <span class="hlt">ice</span> and frozen sediments protrude from shallow, saline <span class="hlt">lakes</span> in the Andes of southwestern Bolivia and northeastern Chile. These <span class="hlt">ice</span> islands range up to 1.5 kilometers long, stand up to 7 meters above the water surface, and may extend out tens of meters and more beneath the unfrozen <span class="hlt">lake</span> sediments. The upper surfaces of the islands are <span class="hlt">covered</span> with dry white sediments, mostly aragonite or calcite. The <span class="hlt">ice</span> blocks may have formed by freezing of the fresh pore water of <span class="hlt">lake</span> sediments during the "little <span class="hlt">ice</span> age." The largest blocks are melting rapidly because of possibly recent increases in geothermal heat flux through the <span class="hlt">lake</span> bottom and undercutting by warm saline <span class="hlt">lake</span> water during the summer.</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 <span class="hlt">Ice</span> with NASA's Operation <span class="hlt">Ice</span>Bridge 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 <span class="hlt">ice</span> is a crucial component of the global climate system. Rapid sea <span class="hlt">ice</span> 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 Water (e.g., Orsi et al. 1999; Jacobs 2004), while the northward transport and subsequent melt of <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> 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 <span class="hlt">ice</span> (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 <span class="hlt">ice</span> production and the lack of shelf water formation over the Amundsen and Bellingshausen shelf seas promote intrusion of warm Circumpolar Deep Water onto the continental shelf and the ocean-driven melting of several <span class="hlt">ice</span> shelves fringing the West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet (e.g., Jacobs et al. 2011; Pritchard et al. 2012; Dutrieux et al. 2014). Sea <span class="hlt">ice</span> conditions around Antarctica are also increasingly considered an important factor impacting local atmospheric conditions and the surface melting of <span class="hlt">Antarctic</span> <span class="hlt">ice</span> shelves (e.g., Scambos et al. 2017). Sea <span class="hlt">ice</span> 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/2011AGUFM.C21A0462V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.C21A0462V"><span>Measurements of ethane in <span class="hlt">Antarctic</span> <span class="hlt">ice</span> cores</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Verhulst, K. R.; Fosse, E. K.; Aydin, K. M.; Saltzman, E. S.</p> <p>2011-12-01</p> <p>Ethane is one of the most abundant hydrocarbons in the atmosphere. The major ethane sources are fossil fuel production and use, biofuel combustion, and biomass-burning emissions and the primary loss pathway is via reaction with OH. A paleoatmospheric ethane record would be useful as a tracer of biomass-burning emissions, providing a constraint on past changes in atmospheric methane and methane isotopes. An independent biomass-burning tracer would improve our understanding of the relationship between biomass burning and climate. The mean annual atmospheric ethane level at high southern latitudes is about 230 parts per trillion (ppt), and <span class="hlt">Antarctic</span> firn air measurements suggest that atmospheric ethane levels in the early 20th century were considerably lower (Aydin et al., 2011). In this study, we present preliminary measurements of ethane (C2H6) in <span class="hlt">Antarctic</span> <span class="hlt">ice</span> core samples with gas ages ranging from 0-1900 C.E. Samples were obtained from dry-drilled <span class="hlt">ice</span> cores from South Pole and Vostok in East Antarctica, and from the West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet Divide (WAIS-D). Gases were extracted from the <span class="hlt">ice</span> by melting under vacuum in a glass vessel sealed by indium wire and were analyzed using high resolution GC/MS with isotope dilution. Ethane levels measured in <span class="hlt">ice</span> core samples were in the range 100-220 ppt, with a mean of 157 ± 45 ppt (n=12). System blanks contribute roughly half the amount of ethane extracted from a 300 g <span class="hlt">ice</span> core sample. These preliminary data exhibit a temporal trend, with higher ethane levels from 0-900 C.E., followed by a decline, reaching a minimum between 1600-1700 C.E. These trends are consistent with variations in <span class="hlt">ice</span> core methane isotopes and carbon monoxide isotopes (Ferretti et al., 2005, Wang et al., 2010), which indicate changes in biomass burning emissions over this time period. These preliminary data suggest that <span class="hlt">Antarctic</span> <span class="hlt">ice</span> core bubbles contain paleoatmospheric ethane levels. With further improvement of laboratory techniques it appears</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25908601','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25908601"><span>Exposure age and <span class="hlt">ice</span>-sheet model constraints on Pliocene East <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet dynamics.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yamane, Masako; Yokoyama, Yusuke; Abe-Ouchi, Ayako; Obrochta, Stephen; Saito, Fuyuki; Moriwaki, Kiichi; Matsuzaki, Hiroyuki</p> <p>2015-04-24</p> <p>The Late Pliocene epoch is a potential analogue for future climate in a warming world. Here we reconstruct Plio-Pleistocene East <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet (EAIS) variability using cosmogenic nuclide exposure ages and model simulations to better understand <span class="hlt">ice</span> sheet behaviour under such warm conditions. New and previously published exposure ages indicate interior-thickening during the Pliocene. An <span class="hlt">ice</span> sheet model with mid-Pliocene boundary conditions also results in interior thickening and suggests that both the Wilkes Subglacial and Aurora Basins largely melted, offsetting increased <span class="hlt">ice</span> volume. Considering contributions from West Antarctica and Greenland, this is consistent with the most recent IPCC AR5 estimate, which indicates that the Pliocene sea level likely did not exceed +20 m on Milankovitch timescales. The inception of colder climate since ∼3 Myr has increased the sea <span class="hlt">ice</span> <span class="hlt">cover</span> and inhibited active moisture transport to Antarctica, resulting in reduced <span class="hlt">ice</span> sheet thickness, at least in coastal areas.</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> <span class="hlt">ice</span> 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> <span class="hlt">ice</span> 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> <span class="hlt">ice</span> volume in response to the ˜110-ky eccentricity modulation of precession. Conservative minimum <span class="hlt">ice</span> 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> <span class="hlt">Ice</span> Sheet is required to explain many of the ˜110-ky cycles. <span class="hlt">Antarctic</span> <span class="hlt">ice</span> 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 <span class="hlt">ice</span> 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> <span class="hlt">ice</span> 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> <span class="hlt">ice</span> 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> <span class="hlt">ice</span> volume in response to the ∼110-ky eccentricity modulation of precession. Conservative minimum <span class="hlt">ice</span> 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> <span class="hlt">Ice</span> Sheet is required to explain many of the ∼110-ky cycles. <span class="hlt">Antarctic</span> <span class="hlt">ice</span> 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 <span class="hlt">ice</span> 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> </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/2016EGUGA..18.7692A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.7692A"><span>Timing and regional patterns of snowmelt on <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> from passive microwave satellite observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Arndt, Stefanie; Willmes, Sascha; Dierking, Wolfgang; Nicolaus, Marcel</p> <p>2016-04-01</p> <p>The better understanding of temporal variability and regional distribution of surface melt on <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> is crucial for the understanding of atmosphere-ocean interactions and the determination of mass and energy budgets of sea <span class="hlt">ice</span>. Since large regions of <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> are <span class="hlt">covered</span> with snow during most of the year, observed inter-annual and regional variations of surface melt mainly represents melt processes in the snow. It is therefore important to understand the mechanisms that drive snowmelt, both at different times of the year and in different regions around Antarctica. In this study we combine two approaches for observing both surface and volume snowmelt by means of passive microwave satellite data. The former is achieved by measuring diurnal differences of the brightness temperature TB at 37 GHz, the latter by analyzing the ratio TB(19GHz)/TB(37GHz). Moreover, we use both melt onset proxies to divide the <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> <span class="hlt">cover</span> into characteristic surface melt patterns from 1988/89 to 2014/15. Our results indicate four characteristic melt types. On average, 43% of the <span class="hlt">ice-covered</span> ocean shows diurnal freeze-thaw cycles in the surface snow layer, resulting in temporary melt (Type A), less than 1% shows continuous snowmelt throughout the snowpack, resulting in strong melt over a period of several days (Type B), 19% shows Type A and B taking place consecutively (Type C), and for 37% no melt is observed at all (Type D). Continuous melt is primarily observed in the outflow of the Weddell Gyre and in the northern Ross Sea, usually 20 days after the onset of temporary melt. Considering the entire data set, snowmelt processes and onset do not show significant temporal trends. Instead, areas of increasing (decreasing) sea-<span class="hlt">ice</span> extent have longer (shorter) periods of continuous snowmelt.</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> <span class="hlt">ice</span> 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 <span class="hlt">ice</span> ages1, fundamental questions remain over the response of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheets to orbital cycles2. Furthermore, an understanding of the behaviour of the marine-based West <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet (WAIS) during the 'warmer-than-present' early-Pliocene epoch (5–3 Myr ago) is needed to better constrain the possible range of <span class="hlt">ice</span>-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 <span class="hlt">ice</span> shelf by the ANDRILL programme and demonstrate well-dated, 40-kyr cyclic variations in <span class="hlt">ice</span>-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 <span class="hlt">ice</span>, or <span class="hlt">ice</span> shelves, to open waters 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 <span class="hlt">ice-sheet/ice</span>-shelf model7 that simulates fluctuations in <span class="hlt">Antarctic</span> <span class="hlt">ice</span> 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> <span class="hlt">ice</span> sheet, in response to ocean-induced melting paced by obliquity. During interglacial times, diatomaceous sediments indicate high surface-water productivity, minimal summer sea <span class="hlt">ice</span> 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('http://hdl.handle.net/2060/20120009528','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120009528"><span><span class="hlt">Antarctic</span> Sea <span class="hlt">Ice</span> Variability and Trends, 1979-2010</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Parkinson, C. L.; Cavalieri, D. J.</p> <p>2012-01-01</p> <p>In sharp contrast to the decreasing sea <span class="hlt">ice</span> coverage of the Arctic, in the <span class="hlt">Antarctic</span> the sea <span class="hlt">ice</span> <span class="hlt">cover</span> has, on average, expanded since the late 1970s. More specifically, satellite passive-microwave data for the period November 1978 - December 2010 reveal an overall positive trend in <span class="hlt">ice</span> extents of 17,100 +/- 2,300 square km/yr. Much of the increase, at 13,700 +/- 1,500 square km/yr, has occurred in the region of the Ross Sea, with lesser contributions from the Weddell Sea and Indian Ocean. One region, that of the Bellingshausen/Amundsen Seas, has, like the Arctic, instead experienced significant sea <span class="hlt">ice</span> decreases, with an overall <span class="hlt">ice</span> extent trend of -8,200 +/- 1,200 square km/yr. When examined through the annual cycle over the 32-year period 1979-2010, the Southern Hemisphere sea <span class="hlt">ice</span> <span class="hlt">cover</span> as a whole experienced positive <span class="hlt">ice</span> extent trends in every month, ranging in magnitude from a low of 9,100 +/- 6,300 square km/yr in February to a high of 24,700 +/- 10,000 square km/yr in May. The Ross Sea and Indian Ocean also had positive trends in each month, while the Bellingshausen/Amundsen Seas had negative trends in each month, and the Weddell Sea and Western Pacific Ocean had a mixture of positive and negative trends. Comparing <span class="hlt">ice</span>-area results to <span class="hlt">ice</span>-extent results, in each case the <span class="hlt">ice</span>-area trend has the same sign as the <span class="hlt">ice</span>-extent trend, but differences in the magnitudes of the two trends identify regions with overall increasing <span class="hlt">ice</span> concentrations and others with overall decreasing <span class="hlt">ice</span> concentrations. The strong pattern of decreasing <span class="hlt">ice</span> coverage in the Bellingshausen/Amundsen Seas region and increasing <span class="hlt">ice</span> coverage in the Ross Sea region is suggestive of changes in atmospheric circulation. This is a key topic for future research.</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> <span class="hlt">Ice</span> Sheet and Perennial Sea-<span class="hlt">Ice</span> 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> <span class="hlt">Ice</span> 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 <span class="hlt">ice</span> 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> <span class="hlt">Ice</span> Sheet to climatic changes, and the continuing rise of atmospheric greenhouse gas concentrations. The <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet is a pivotal component of the global water budget. Freshwater fluxes from the <span class="hlt">ice</span> 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 water 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> <span class="hlt">ice</span> 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> <span class="hlt">ice</span> cores (WDC, EDML), we now have evidence that during glacial times a more northerly extent of the perennial sea-<span class="hlt">ice</span> 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 <span class="hlt">ice</span> and <span class="hlt">ice</span> sheet decline. This in turn caused Southern Hemisphere warming, a more vigorous ACC, stronger Southern Ocean ventilation, and warm Circumpolar Deep Water (CDW) upwelling on <span class="hlt">Antarctic</span> shelves</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUFM.P52A..06P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFM.P52A..06P"><span><span class="hlt">Lake</span> Vostok: An earthly analogue for the geomicrobiology on Europa</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Priscu, J. C.; Christner, B. C.</p> <p>2007-12-01</p> <p>The recent discovery of more than 150 subglacial <span class="hlt">lakes</span> beneath the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet has important implications in our search for liquid water and associated life on other icy worlds. The largest of these <span class="hlt">lakes</span> is <span class="hlt">Lake</span> Vostok, which has a surface area of 14000 square km and a depth of 1000 m, making it one of the largest <span class="hlt">lakes</span> on Earth. Although we have yet to sample directly the liquid water from any of the <span class="hlt">Antarctic</span> subglacial <span class="hlt">lakes</span>, refrozen lakewater (accretion <span class="hlt">ice</span>) has been sampled just above the surface of <span class="hlt">Lake</span> Vostok. Genomic and geochemical analysis of this <span class="hlt">ice</span> reveals that the surface <span class="hlt">lake</span> water supports a microbial assemblage with a density approaching 1000 cells per milliliter. Sequencing and phylogenetic analysis of the 900 to 1000 base pair small subunit rRNA gene sequences obtained revealed a low diversity of clones that classify within the beta, gamma and delta subdivisions of the phylum Proteobacteria. Nearest phylogenetic neighbor analysis of these gene sequences imply that the <span class="hlt">lake</span> contains an aerobic and anaerobic consortium of bacteria with metabolisms dedicated to iron and sulfur respiration or oxidation indicating that these metals play a role in the bioenergetics of microorganisms that occur in <span class="hlt">Lake</span> Vostok. Sequence analysis further revealed that heterotrophic life in the <span class="hlt">lake</span> can be sustained by chemolithotrophic production of new carbon supplemented by dissolved organic carbon released from the overlying <span class="hlt">ice</span> sheet. Data obtained from orbiters have revealed that a deep ocean of liquid water lies under a thick chaotic <span class="hlt">ice</span> <span class="hlt">cover</span> on Europa where organic matter derived from comets and oxidants provided by radiation from Jupiter's magnetosphere may provide a habitat for life and a reservoir of endogenous and exogenous substances much like we observe in <span class="hlt">Lake</span> Vostok. Future studies of <span class="hlt">Antarctic</span> subglacial <span class="hlt">lake</span> environments will play a crucial role in our understanding of life on Europa and other frozen worlds.</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> <span class="hlt">ice</span> 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> <span class="hlt">ice</span> sheet, but <span class="hlt">ice</span>-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> <span class="hlt">ice</span> 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 water 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> <span class="hlt">ice</span> sheet. We interpret this erosion to be associated with retreat of the <span class="hlt">ice</span> sheet margin several hundreds of kilometres inland and conclude that the East <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet was sensitive to climatic warmth during the Pliocene.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.8907S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.8907S"><span>Toward a <span class="hlt">Lake</span> <span class="hlt">Ice</span> Phenology Derived from VIIRS Data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sütterlin, Melanie; Duguay-Tetzlaff, Anke; Wunderle, Stefan</p> <p>2017-04-01</p> <p><span class="hlt">Ice</span> <span class="hlt">cover</span> on <span class="hlt">lakes</span> plays an essential role in the physical, chemical, and biological processes of freshwater systems (e.g., <span class="hlt">ice</span> duration controls the seasonal heat budget of <span class="hlt">lakes</span>), and it also has many economic implications (e.g., for hydroelectricity, transportation, winter tourism). The variability and trends in the seasonal cycle of <span class="hlt">lake</span> <span class="hlt">ice</span> (e.g., timing of freeze-up and break-up) represent robust and direct indicators of climate change; they therefore emphasize the importance of monitoring <span class="hlt">lake</span> <span class="hlt">ice</span> phenology. Satellite remote sensing has proven its great potential for detecting and measuring the <span class="hlt">ice</span> <span class="hlt">cover</span> on <span class="hlt">lakes</span>. Different remote sensing systems have been successfully used to collect recordings of freeze-up, break-up, and <span class="hlt">ice</span> thickness and increase the spatial and temporal coverage of ground-based observations. Therefore, within the Global Climate Observing System (GCOS) Swiss project, "Integrated Monitoring of <span class="hlt">Ice</span> in Selected Swiss <span class="hlt">Lakes</span>," initiated by MeteoSwiss, satellite images from various sensors and different approaches are used and compared to perform investigations aimed at integrated monitoring of <span class="hlt">lake</span> <span class="hlt">ice</span> in Switzerland and contributing to the collection of <span class="hlt">lake</span> <span class="hlt">ice</span> phenology recordings. Within the framework of this project, the Remote Sensing Research Group of the University of Bern (RSGB) utilizes data acquired in the fine-resolution imagery (I) bands (1-5) of the Visible Infrared Imaging Radiometer Suite (VIIRS) sensor that is mounted onboard the SUOMI-NPP. Visible and near-infrared reflectances, as well as thermal infrared-derived <span class="hlt">lake</span> surface water temperatures (LSWT), are used to retrieve <span class="hlt">lake</span> <span class="hlt">ice</span> phenology dates. The VIIRS instrument, which combines a high temporal resolution ( 2 times per day) with a reasonable spatial resolution (375 m), is equipped with a single broad-band thermal I-channel (I05). Thus, a single-channel LSWT retrieval algorithm is employed to correct for the atmospheric influence. The single channel algorithm applied in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70036263','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70036263"><span>Hydrogeomorphic processes of thermokarst <span class="hlt">lakes</span> with grounded-<span class="hlt">ice</span> and floating-<span class="hlt">ice</span> regimes on the Arctic coastal plain, Alaska</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Arp, C.D.; Jones, Benjamin M.; Urban, F.E.; Grosse, G.</p> <p>2011-01-01</p> <p>Thermokarst <span class="hlt">lakes</span> <span class="hlt">cover</span> > 20% of the landscape throughout much of the Alaskan Arctic Coastal Plain (ACP) with shallow <span class="hlt">lakes</span> freezing solid (grounded <span class="hlt">ice</span>) and deeper <span class="hlt">lakes</span> maintaining perennial liquid water (floating <span class="hlt">ice</span>). Thus, <span class="hlt">lake</span> depth relative to maximum <span class="hlt">ice</span> thickness (1·5–2·0 m) represents an important threshold that impacts permafrost, aquatic habitat, and potentially geomorphic and hydrologic behaviour. We studied coupled hydrogeomorphic processes of 13 <span class="hlt">lakes</span> representing a depth gradient across this threshold of maximum <span class="hlt">ice</span> thickness by analysing remotely sensed, water quality, and climatic data over a 35-year period. Shoreline erosion rates due to permafrost degradation ranged from L) with periods of full and nearly dry basins. Shorter-term (2004–2008) specific conductance data indicated a drying pattern across <span class="hlt">lakes</span> of all depths consistent with the long-term record for only shallow <span class="hlt">lakes</span>. Our analysis suggests that grounded-<span class="hlt">ice</span> <span class="hlt">lakes</span> are <span class="hlt">ice</span>-free on average 37 days longer than floating-<span class="hlt">ice</span> <span class="hlt">lakes</span> resulting in a longer period of evaporative loss and more frequent negative P − EL. These results suggest divergent hydrogeomorphic responses to a changing Arctic climate depending on the threshold created by water depth relative to maximum <span class="hlt">ice</span> thickness in ACP <span class="hlt">lakes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16782602','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16782602"><span>Geological and geomorphological insights into <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet evolution.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sugden, David E; Bentley, Michael J; O Cofaigh, Colm</p> <p>2006-07-15</p> <p>Technical advances in the study of <span class="hlt">ice</span>-free parts of Antarctica can provide quantitative records that are useful for constraining and refining models of <span class="hlt">ice</span> sheet evolution and behaviour. Such records improve our understanding of system trajectory, influence the questions we ask about system stability and help to define the <span class="hlt">ice</span>-sheet processes that are relevant on different time-scales. Here, we illustrate the contribution of cosmogenic isotope analysis of exposed bedrock surfaces and marine geophysical surveying to the understanding of <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet evolution on a range of time-scales. In the Dry Valleys of East Antarctica, 3He dating of subglacial flood deposits that are now exposed on mountain summits provide evidence of an expanded and thicker Mid-Miocene <span class="hlt">ice</span> sheet. The survival of surface boulders for approximately 14Myr, the oldest yet measured, demonstrates exceptionally low rates of subsequent erosion and points to the persistence and stability of the dry polar desert climate since that time. Increasingly, there are constraints on West <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet fluctuations during Quaternary glacial cycles. In the Sarnoff Mountains of Marie Byrd Land in West Antarctica, 10Be and 26Al cosmogenic isotope analysis of glacial erratics and bedrock reveal steady thinning of the <span class="hlt">ice</span> sheet from 10400 years ago to the present, probably as a result of grounding line retreat. In the <span class="hlt">Antarctic</span> Peninsula, offshore analysis reveals an extensive <span class="hlt">ice</span> sheet at the last glacial maximum. Based on radiocarbon dating, deglaciation began by 17000cal yr BP and was complete by 9500cal yr BP. Deglaciation of the west and east sides of the <span class="hlt">Antarctic</span> Peninsula <span class="hlt">ice</span> sheet occurred at different times and rates, but was largely complete by the Early Holocene. At that time <span class="hlt">ice</span> shelves were less extensive on the west side of the <span class="hlt">Antarctic</span> Peninsula than they are today. The message from the past is that individual glacier drainage basins in Antarctica respond in different and distinctive</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70018727','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70018727"><span>Glacial removal of late Cenozoic subglacially emplaced volcanic edifices by the West <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Behrendt, John C.; Blankenship, D.D.; Damaske, D.; Cooper, A. K.</p> <p>1995-01-01</p> <p>Local maxima of the horizontal gradient of pseudogravity from closely spaced aeromagnetic surveys over the Ross Sea, northwestern Ross <span class="hlt">Ice</span> Shelf, and the West <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet, reveal a linear magnetic rift fabric and numerous subcircular, high-amplitude anomalies. Geophysical data indicate two or three youthful volcanic edifices at widely separated areas beneath the sea and <span class="hlt">ice</span> <span class="hlt">cover</span> in the West <span class="hlt">Antarctic</span> rift system. In contrast, we suggest glacial removal of edifices of volcanic sources of many more anomalies. Magnetic models, controlled by marine seismic reflection and radar <span class="hlt">ice</span>-sounding data, allow us to infer that glacial removal of the associated late Cenozoic volcanic edifices (probably debris, comprising pillow breccias, and hyaloclastites) has occurred essentially concomitantly with their subglacial eruption. "Removal' of unconsolidated volcanic debris erupted beneath the <span class="hlt">ice</span> is probably a more appropriate term than "erosion', given its fragmented, <span class="hlt">ice</span>-contact origin. The exposed volcanoes may have been protected from erosion by the surrounding <span class="hlt">ice</span> sheet because of more competent rock or high elevation above the <span class="hlt">ice</span> sheet. -from Authors</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4822592','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4822592"><span>Dynamic <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet during the early to mid-Miocene</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>DeConto, Robert M.; Pollard, David; Levy, Richard H.</p> <p>2016-01-01</p> <p>Geological data indicate that there were major variations in <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet volume and extent during the early to mid-Miocene. Simulating such large-scale changes is problematic because of a strong hysteresis effect, which results in stability once the <span class="hlt">ice</span> sheets have reached continental size. A relatively narrow range of atmospheric CO2 concentrations indicated by proxy records exacerbates this problem. Here, we are able to simulate large-scale variability of the early to mid-Miocene <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet because of three developments in our modeling approach. (i) We use a climate–<span class="hlt">ice</span> sheet coupling method utilizing a high-resolution atmospheric component to account for <span class="hlt">ice</span> sheet–climate feedbacks. (ii) The <span class="hlt">ice</span> sheet model includes recently proposed mechanisms for retreat into deep subglacial basins caused by <span class="hlt">ice</span>-cliff failure and <span class="hlt">ice</span>-shelf hydrofracture. (iii) We account for changes in the oxygen isotopic composition of the <span class="hlt">ice</span> sheet by using isotope-enabled climate and <span class="hlt">ice</span> sheet models. We compare our modeling results with <span class="hlt">ice</span>-proximal records emerging from a sedimentological drill core from the Ross Sea (Andrill-2A) that is presented in a companion article. The variability in <span class="hlt">Antarctic</span> <span class="hlt">ice</span> volume that we simulate is equivalent to a seawater oxygen isotope signal of 0.52–0.66‰, or a sea level equivalent change of 30–36 m, for a range of atmospheric CO2 between 280 and 500 ppm and a changing astronomical configuration. This result represents a substantial advance in resolving the long-standing model data conflict of Miocene <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet and sea level variability. PMID:26903645</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16782603','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16782603"><span>Mass balance of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wingham, D J; Shepherd, A; Muir, A; Marshall, G J</p> <p>2006-07-15</p> <p>The <span class="hlt">Antarctic</span> contribution to sea-level rise has long been uncertain. While regional variability in <span class="hlt">ice</span> dynamics has been revealed, a picture of mass changes throughout the continental <span class="hlt">ice</span> sheet is lacking. Here, we use satellite radar altimetry to measure the elevation change of 72% of the grounded <span class="hlt">ice</span> sheet during the period 1992-2003. Depending on the density of the snow giving rise to the observed elevation fluctuations, the <span class="hlt">ice</span> sheet mass trend falls in the range -5-+85Gtyr-1. We find that data from climate model reanalyses are not able to characterise the contemporary snowfall fluctuation with useful accuracy and our best estimate of the overall mass trend-growth of 27+/-29Gtyr-1-is based on an assessment of the expected snowfall variability. Mass gains from accumulating snow, particularly on the <span class="hlt">Antarctic</span> Peninsula and within East Antarctica, exceed the <span class="hlt">ice</span> dynamic mass loss from West Antarctica. The result exacerbates the difficulty of explaining twentieth century sea-level rise.</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 <span class="hlt">ice</span>.</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 <span class="hlt">ice</span> and circumpolar sea water 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 <span class="hlt">ice</span> and sea water 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 <span class="hlt">ice</span>. Anaerobic bacteria known to methylate mercury were notably absent from sea-<span class="hlt">ice</span> metagenomes. We propose that <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> can harbour a microbial source of methylmercury in the Southern Ocean.</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> <span class="hlt">Lakes</span></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 <span class="hlt">lakes</span>. First, we quantified GDGT compositions present and then investigated modern-day environmental controls on GDGT composition. GDGTs were found in all 32 <span class="hlt">lakes</span> studied. Branched GDGTs (brGDGTs) were dominant in 31 <span class="hlt">lakes</span> and statistical analyses showed that their composition was strongly correlated with mean summer air temperature (MSAT) rather than pH, conductivity or water depth. Second, we developed the first regional brGDGT-temperature calibration for <span class="hlt">Antarctic</span> and sub-<span class="hlt">Antarctic</span> <span class="hlt">lakes</span> 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 <span class="hlt">lake</span> 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/2016AGUFM.C32B..05B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C32B..05B"><span>Expanding <span class="hlt">Antarctic</span> Sea <span class="hlt">Ice</span>: Anthropogenic or Natural Variability?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bitz, C. M.</p> <p>2016-12-01</p> <p><span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> extent has increased over the last 36 years according to the satellite record. Concurrent with <span class="hlt">Antarctic</span> sea-<span class="hlt">ice</span> expansion has been broad cooling of the Southern Ocean sea-surface temperature. Not only are Southern Ocean sea <span class="hlt">ice</span> and SST trends at odds with expectations from greenhouse gas-induced warming, the trend patterns are not reproduced in historical simulations with comprehensive global climate models. While a variety of different factors may have contributed to the observed trends in recent decades, we propose that it is atmospheric circulation changes - and the changes in ocean circulation they induce - that have emerged as the most likely cause of the observed Southern Ocean sea <span class="hlt">ice</span> and SST trends. I will discuss deficiencies in models that could explain their incorrect response. In addition, I will present results from a series of experiments where the <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> and ocean are forced by atmospheric perturbations imposed within a coupled climate model. Figure caption: Linear trends of annual-mean SST (left) and annual-mean sea-<span class="hlt">ice</span> concentration (right) over 1980-2014. SST is from NOAA's Optimum Interpolation SST dataset (version 2; Reynolds et al. 2002). Sea-<span class="hlt">ice</span> concentration is from passive microwave observations using the NASA Team algorithm. Only the annual means are shown here for brevity and because the signal to noise is greater than in the seasonal means. Figure from Armour and Bitz (2015).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.6221B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.6221B"><span>The Last Interglacial History of the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> sheet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bradley, Sarah; Siddall, Mark; Milne, Glenn A.; Masson-Delmotte, Valerie; Wolff, Eric; Hindmarsh, Richard C. A.</p> <p>2014-05-01</p> <p>In this paper we present a summary of the work which was conducted as part of the 'PAST4FUTURE -WP4.1: Sea Level and <span class="hlt">Ice</span> sheets' project. The overall aim of this study was to understand the response of the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> sheet (AIS) to climate forcing during the Last interglacial (LIG) and its contribution to the observed higher than present sea level during this period. The study involved the application and development of a novel technique which combined East <span class="hlt">Antarctic</span> stable isotope <span class="hlt">ice</span> core data with the output from a Glacial Isostatic Adjustment (GIA) model [Bradley et al., 2012]. We investigated if the stable isotope <span class="hlt">ice</span> core data are sensitive to detecting isostatically driven changes in the surface elevation driven by changes in the <span class="hlt">ice</span>-loading history of the AIS and if so, could we address some key questions relating to the LIG history of the AIS. Although it is believed that the West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> sheet (WAIS) reduced in size during the LIG compared to the Holocene, major uncertainties and unknowns remain unresolved: Did the WAIS collapse? What would the contribution of such a collapse be the higher than present LIG eustatic sea level (ESL)? We will show that a simulated collapse of the WAIS does not generate a significant elevation driven signal at the EAIS LIG <span class="hlt">ice</span> core sites, and as such, these <span class="hlt">ice</span> core records cannot be used to assess WAIS stability over this period. However, we will present 'treasure maps' [Bradley et al., 2012] to identify regions of the AIS where results from geological studies and/or new paleoclimate data may be sensitive to detecting a WAIS collapse. These maps can act as a useful tool for the wider science community/field scientists as a guide to highlight sites suitable to constrain the evolution of the WAIS during the LIG. Studies have proposed that the surface temperature across the East <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet (EAIS) was significantly warmer, 2-5°C during the LIG compared to present [Lang and Wolff, 2011]. These higher</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.5867S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.5867S"><span>Changes in <span class="hlt">ice</span> dynamics along the northern <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>Seehaus, Thorsten; Marinsek, Sebastian; Cook, Alison; Van Wessem, Jan-Melchior; Braun, Matthias</p> <p>2017-04-01</p> <p>The climatic conditions along the <span class="hlt">Antarctic</span> Peninsula have undergone considerable changes during the last 50 years. A period of pronounced air temperature rise, increasing ocean temperatures as well as changes in the precipitation pattern have been reported by various authors. Consequently, the glacial systems showed changes including widespread retreat, surface lowering as well as variations in flow speeds. During the last decades numerous <span class="hlt">ice</span> shelves along the <span class="hlt">Antarctic</span> Peninsula retreated, started to break-up or disintegrated completely. The loss of the buttressing effect caused tributary glaciers to accelerate with increasing <span class="hlt">ice</span> discharge along the <span class="hlt">Antarctic</span> Peninsula. Quantification of the mass changes is still subject to considerable errors although numbers derived from the different methods are converging. The aim is to study the reaction of glaciers at the northern <span class="hlt">Antarctic</span> Peninsula to the changing climatic conditions and the readjustments of tributary glaciers to <span class="hlt">ice</span> shelf disintegration, as well as to better quantify the <span class="hlt">ice</span> mass loss and its temporal changes. We analysed time series of various satellite sensors (ERS-1/2 SAR, ENVISAT ASAR, RADARSAT-1, ALOS PALSAR, TerraSAR-X/TanDEM-X, ASTER, Landsat) to detect changes in <span class="hlt">ice</span> dynamics of 74 glacier basins along the northern <span class="hlt">Antarctic</span> Peninsula (<65°). Intensity feature tracking techniques were applied on data stacks from different SAR satellites over the last 20 years to infer temporal trends in glacier surface velocities. In combination with <span class="hlt">ice</span> thickness reconstructions and modeled climatic mass balance fields regional imbalances were calculated. Variations in <span class="hlt">ice</span> front position were mapped based on optical and SAR satellite data sets. Along the west coast of the northern <span class="hlt">Antarctic</span> Peninsula an increase in flow speeds by 40% between 1992 and 2014 was observed, whereas glaciers on the east side (north of former Prince-Gustav <span class="hlt">Ice</span> Shelf) showed a strong deceleration. Nearly all former <span class="hlt">ice</span> shelf</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C41B0665S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C41B0665S"><span>Changes in <span class="hlt">ice</span> dynamics along the northern <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>Seehaus, T.; Braun, M.; Cook, A.; Marinsek, S.</p> <p>2016-12-01</p> <p>The climatic conditions along the <span class="hlt">Antarctic</span> Peninsula have undergone considerable changes during the last 50 years. Numerous <span class="hlt">ice</span> shelves along the <span class="hlt">Antarctic</span> Peninsula retreated, started to break-up or disintegrated. The loss of the buttressing effect caused tributary glaciers to accelerate with increasing <span class="hlt">ice</span> discharge along the <span class="hlt">Antarctic</span> Peninsula. The aim is to study the reaction of glaciers at the northern <span class="hlt">Antarctic</span> Peninsula to the changing climatic conditions and the readjustments of tributary glaciers to <span class="hlt">ice</span> shelf disintegration, as well as to better quantify the <span class="hlt">ice</span> mass loss and its temporal changes.We analysed time series of various SAR satellite sensors to detect changes in <span class="hlt">ice</span> flow speed and surface elevation. Intensity feature tracking techniques were applied on data stacks from different SAR satellites over the last 20 years to infer changes in glacier surface velocities. High resolution bi-static TanDEM-X data was used to derive digital elevation models by differential SAR interferometry. In combination with ASTER and SPOT stereo images, changes in surface elevations were determined. Altimeter data from ICESat, CryoSat-2 and NASA operation <span class="hlt">Ice</span>Bridge ATM were used for vertical referencing and quality assessment of the digital elevation models. Along the west coast of the northern <span class="hlt">Antarctic</span> Peninsula an increase in flow speeds by 40% between 1992 and 2014 was observed, whereas glaciers on the east side (north of former Prince-Gustav <span class="hlt">Ice</span> Shelf) showed a strong deceleration. In total an <span class="hlt">ice</span> discharge of 17.93±6.22 Gt/a was estimated for 74 glaciers on the <span class="hlt">Antarctic</span> Peninsula north of 65°S. Most of the former <span class="hlt">ice</span> shelf tributaries showed similar reactions to <span class="hlt">ice</span> shelf disintegration. At the Sjögren-Inlet a total <span class="hlt">ice</span> mass loss of -37.5±8.2 Gt and a contribution to sea level rise of 20.9±5.2 Gt were found in the period 1993-2014. The average surface lowering rate in the period 2012-2014 amounts to -2.2 m/a. At Dinsmoor-Bombardier-Edgeworth glacier</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930063983&hterms=photography&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DTitle%26N%3D0%26No%3D50%26Ntt%3Dphotography','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930063983&hterms=photography&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DTitle%26N%3D0%26No%3D50%26Ntt%3Dphotography"><span><span class="hlt">Ice</span> patterns and hydrothermal plumes, <span class="hlt">Lake</span> Baikal, Russia - Insights from Space Shuttle hand-held photography</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Evans, Cynthia A.; Helfert, Michael R.; Helms, David R.</p> <p>1992-01-01</p> <p>Earth photography from the Space Shuttle is used to examine the <span class="hlt">ice</span> <span class="hlt">cover</span> on <span class="hlt">Lake</span> Baikal and correlate the patterns of weakened and melting <span class="hlt">ice</span> with known hydrothermal areas in the Siberian <span class="hlt">lake</span>. Particular zones of melted and broken <span class="hlt">ice</span> may be surface expressions of elevated heat flow in <span class="hlt">Lake</span> Baikal. The possibility is explored that hydrothermal vents can introduce local convective upwelling and disrupt a stable water column to the extent that the melt zones which are observed in the <span class="hlt">lake</span>'s <span class="hlt">ice</span> <span class="hlt">cover</span> are produced. A heat flow map and photographs of the <span class="hlt">lake</span> are overlaid to compare specific areas of thinned or broken <span class="hlt">ice</span> with the hot spots. The regions of known hydrothermal activity and high heat flow correlate extremely well with circular regions of thinned <span class="hlt">ice</span>, and zones of broken and recrystallized <span class="hlt">ice</span>. Local and regional climate data and other sources of warm water, such as river inlets, are considered.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C13G..05W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C13G..05W"><span><span class="hlt">Antarctic</span> <span class="hlt">ice</span> discharge due to warm water intrusion into shelf cavities</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.; Reese, R.; Albrecht, T.; Mengel, M.; Asay-Davis, X.</p> <p>2017-12-01</p> <p>Ocean-induced melting below <span class="hlt">ice</span> shelves is the dominant driver for mass loss from the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet at present. Observations show that many <span class="hlt">Antarctic</span> <span class="hlt">ice</span> shelves are thinning which reduces their buttressing potential and can lead to increased <span class="hlt">ice</span> discharge from the glaciers upstream. Melt rates from <span class="hlt">Antarctic</span> <span class="hlt">ice</span> shelves are determined by the temperature and salinity of the ambient ocean. In many parts, <span class="hlt">ice</span> shelves are shielded by clearly defined density fronts which keep relatively warm Northern water from entering the cavity underneath the <span class="hlt">ice</span> shelves. Projections show that a redirection of coastal currents might allow these warmer waters to intrude into <span class="hlt">ice</span> shelf cavities, for instance in the Weddell Sea, and thereby cause a strong increase in sub-shelf melt rates. Using the Potsdam <span class="hlt">Ice</span>-shelf Cavity mOdel (PICO), we assess how such a change would influence the dynamic <span class="hlt">ice</span> loss from Antarctica. PICO is implemented as part of the Parallel <span class="hlt">Ice</span> Sheet Model (PISM) and mimics the vertical overturning circulation in <span class="hlt">ice</span>-shelf cavities. The model is capable of capturing the wide range of melt rates currently observed for <span class="hlt">Antarctic</span> <span class="hlt">ice</span> 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 <span class="hlt">ice</span> discharge resulting from the potential erosion of ocean fronts around 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('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> <span class="hlt">Ice</span> 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> <span class="hlt">ice</span> sheet surface elevation, repeatedly, at approximately monthly intervals. These data constitute the longest continuous record of <span class="hlt">ice</span> 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> <span class="hlt">ice</span> sheets, and of parts of the <span class="hlt">Antarctic</span> Peninsula <span class="hlt">ice</span> 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 <span class="hlt">ice</span> flow, and we estimate that 3.6 % of the continental <span class="hlt">ice</span> 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> <span class="hlt">ice</span> 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/2016E%26PSL.444...75A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016E%26PSL.444...75A"><span>Late Miocene-Pliocene Asian monsoon intensification linked to <span class="hlt">Antarctic</span> <span class="hlt">ice</span>-sheet growth</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ao, Hong; Roberts, Andrew P.; Dekkers, Mark J.; Liu, Xiaodong; Rohling, Eelco J.; Shi, Zhengguo; An, Zhisheng; Zhao, Xiang</p> <p>2016-06-01</p> <p>Environmental conditions in one of Earth's most densely populated regions, East Asia, are dominated by the monsoon. While Quaternary monsoon variability is reasonably well understood, pre-Quaternary monsoon variability and dynamics remain enigmatic. In particular, little is known about potential relationships between northern hemispheric monsoon response and major Cenozoic changes in <span class="hlt">Antarctic</span> <span class="hlt">ice</span> <span class="hlt">cover</span>. Here we document long-term East Asian summer monsoon (EASM) intensification through the Late Miocene-Pliocene (∼8.2 to 2.6 Ma), and attribute this to progressive <span class="hlt">Antarctic</span> glaciation. Our new high-resolution magnetic records of long-term EASM intensification come from the Late Miocene-Pliocene Red Clay sequence on the Chinese Loess Plateau; we identify underlying mechanisms using a numerical climate-model simulation of EASM response to an idealized stepwise increase in <span class="hlt">Antarctic</span> <span class="hlt">ice</span> volume. We infer that progressive <span class="hlt">Antarctic</span> glaciation caused intensification of the cross-equatorial pressure gradient between an atmospheric high-pressure cell over Australia and a low-pressure cell over mid-latitude East Asia, as well as intensification of the cross-equatorial sea-surface temperature (SST) gradient. These combined atmospheric and oceanic adjustments led to EASM intensification. Our findings offer a new and more global perspective on the controls behind long-term Asian monsoon evolution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.A23J0359A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.A23J0359A"><span>Late Miocene-Pliocene Asian monsoon intensification linked to <span class="hlt">Antarctic</span> <span class="hlt">ice</span>-sheet growth</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ao, H.; Roberts, A. P.; Dekkers, M. J.; Liu, X.; Rohling, E. J.; Shi, Z.; An, Z.; Zhao, X.</p> <p>2016-12-01</p> <p>Environmental conditions in one of Earth's most densely populated regions, East Asia, are dominated by the monsoon. While Quaternary monsoon variability is reasonably well understood, pre-Quaternary monsoon variability and dynamics remain enigmatic. In particular, little is known about potential relationships between northern hemispheric monsoon response and major Cenozoic changes in <span class="hlt">Antarctic</span> <span class="hlt">ice</span> <span class="hlt">cover</span>. Here we document long-term East Asian summer monsoon (EASM) intensification through the Late Miocene-Pliocene (˜8.2 to 2.6 Ma), and attribute this to progressive <span class="hlt">Antarctic</span> glaciation. Our new high-resolution magnetic records of long-term EASM intensification come from the Late Miocene-Pliocene Red Clay sequence on the Chinese Loess Plateau; we identify underlying mechanisms using a numerical climate-model simulation of EASM response to an idealized stepwise increase in <span class="hlt">Antarctic</span> <span class="hlt">ice</span> volume. We infer that progressive <span class="hlt">Antarctic</span> glaciation caused intensification of the cross-equatorial pressure gradient between an atmospheric high-pressure cell over Australia and a low-pressure cell over mid-latitude East Asia, as well as intensification of the cross-equatorial sea-surface temperature (SST) gradient. These combined atmospheric and oceanic adjustments led to EASM intensification. Our findings offer a new and more global perspective on the controls behind long-term Asian monsoon evolution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20170003112&hterms=core&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dcore','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20170003112&hterms=core&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dcore"><span>Holocene Accumulation and <span class="hlt">Ice</span> Flow near the West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet Divide <span class="hlt">Ice</span> Core Site</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Koutnik, Michelle R.; Fudge, T.J.; Conway, Howard; Waddington, Edwin D.; Neumann, Thomas A.; Cuffey, Kurt M.; Buizert, Christo; Taylor, Kendrick C.</p> <p>2016-01-01</p> <p>The West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet Divide Core (WDC) provided a high-resolution climate record from near the Ross-Amundsen Divide in Central West Antarctica. In addition, radar-detected internal layers in the vicinity of the WDC site have been dated directly from the <span class="hlt">ice</span> core to provide spatial variations in the age structure of the region. Using these two data sets together, we first infer a high-resolution Holocene accumulation-rate history from 9.2 thousand years of the <span class="hlt">ice</span>-core timescale and then confirm that this climate history is consistent with internal layers upstream of the core site. Even though the WDC was drilled only 24 kilometers from the modern <span class="hlt">ice</span> divide, advection of <span class="hlt">ice</span> from upstream must be taken into account. We evaluate histories of accumulation rate by using a flowband model to generate internal layers that we compare to observed layers. Results show that the centennially averaged accumulation rate was over 20 percent lower than modern at 9.2 thousand years before present (B.P.), increased by 40 percent from 9.2 to 2.3 thousand years B.P., and decreased by at least 10 percent over the past 2 thousand years B.P. to the modern values; these Holocene accumulation-rate changes in Central West Antarctica are larger than changes inferred from East <span class="hlt">Antarctic</span> <span class="hlt">ice</span>-core records. Despite significant changes in accumulation rate, throughout the Holocene the regional accumulation pattern has likely remained similar to today, and the <span class="hlt">ice</span>-divide position has likely remained on average within 5 kilometers of its modern position. Continent-scale <span class="hlt">ice</span>-sheet models used for reconstructions of West <span class="hlt">Antarctic</span> <span class="hlt">ice</span> volume should incorporate this accumulation history.</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 <span class="hlt">lakes</span> 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> <span class="hlt">ice</span> cap and climate changes in the last several millions years. In the framework of the Project on “Exploration and characterization of Concordia <span class="hlt">Lake</span>, Antarctica”, supported by Italian Program for <span class="hlt">Antarctic</span> Research (PNRA), a glaciological investigation of the Dome C “<span class="hlt">Lake</span> District” are planned. Indeed, the glacio-chemical characterisation of the <span class="hlt">ice</span> column over subglacial <span class="hlt">lakes</span> will allow to evaluate the fluxes of major and trace chemical species along the <span class="hlt">ice</span> column and in the accreted <span class="hlt">ice</span> and, consequently, the availability of nutrients and oligo-elements for possible biological activity in the <span class="hlt">lake</span> water and sediments. Melting and freezing at the base of the <span class="hlt">ice</span> sheet should be able to deliver carbon and salts to the <span class="hlt">lake</span>, as observed for the Vostok subglacial <span class="hlt">lake</span>, 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 <span class="hlt">ice</span>, <span class="hlt">lake</span> water 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 <span class="hlt">Ice</span> Coring in Antarctica, TALDICE - TALos Dome <span class="hlt">ICE</span> core, ANDRILL MIS - <span class="hlt">ANTarctic</span> DRILLing McMurdo <span class="hlt">Ice</span> 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> <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-<span class="hlt">ice</span> expansion driven by mid-Holocene retreat of the Ross <span class="hlt">Ice</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>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-<span class="hlt">ice</span> coverage, coeval with thinning West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet (WAIS) <span class="hlt">ice</span> shelves and the rapid freshening of surface and bottom waters along the <span class="hlt">Antarctic</span> margin. The mid-Holocene Neoglacial transition represents the last comparable baseline shift in sea-<span class="hlt">ice</span> 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-<span class="hlt">ice</span>. 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 <span class="hlt">Ice</span> 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-<span class="hlt">ice</span> from 4.5 ka. This is coeval with cosmogenic nuclide evidence for a rapid thinning of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet during the mid-Holocene (Hein et al., 2016). We suggest this represents a final major pulse of deglaciation from the Ross <span class="hlt">Ice</span> Shelf, which initiates the Neoglacial, driving cool surface waters along the coast and greater sea-<span class="hlt">ice</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170003145','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170003145"><span><span class="hlt">Antarctic</span> Sea-<span class="hlt">Ice</span> Freeboard and Estimated Thickness from NASA's ICESat and <span class="hlt">Ice</span>Bridge Observations</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Yi, Donghui; Kurtz, Nathan; Harbeck, Jeremy; Manizade, Serdar; Hofton, Michelle; Cornejo, Helen G.; Zwally, H. Jay; Robbins, John</p> <p>2016-01-01</p> <p>ICESat completed 18 observational campaigns during its lifetime from 2003 to 2009. Data from all of the 18 campaign periods are used in this study. Most of the operational periods were between 34 and 38 days long. Because of laser failure and orbit transition from 8-day to 91-day orbit, there were four periods lasting 57, 16, 23, and 12 days. <span class="hlt">Ice</span>Bridge data from 2009, 2010, and 2011 are used in this study. Since 2009, there are 19 Airborne Topographic Mapper (ATM) campaigns, and eight Land, Vegetation, and <span class="hlt">Ice</span> Sensor (LVIS) campaigns over the <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span>. Freeboard heights are derived from ICESat, ATM and LVIS elevation and waveform data. With nominal densities of snow, water, and sea <span class="hlt">ice</span>, combined with snow depth data from AMSR-E/AMSR2 passive microwave observation over the southern ocean, sea-<span class="hlt">ice</span> thickness is derived from the freeboard. Combined with AMSR-E/AMSR2 <span class="hlt">ice</span> concentration, sea-<span class="hlt">ice</span> area and volume are also calculated. During the 2003-2009 period, sea-<span class="hlt">ice</span> freeboard and thickness distributions show clear seasonal variations that reflect the yearly cycle of the growth and decay of the <span class="hlt">Antarctic</span> pack <span class="hlt">ice</span>. We found no significant trend of thickness or area for the <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> during the ICESat period. <span class="hlt">Ice</span>Bridge sea <span class="hlt">ice</span> freeboard and thickness data from 2009 to 2011 over the Weddell Sea and Amundsen and Bellingshausen Seas are compared with the ICESat results.</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 <span class="hlt">ice</span>-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 <span class="hlt">ice</span> 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 <span class="hlt">ice</span>-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 <span class="hlt">ice</span>-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 <span class="hlt">ice</span> 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 <span class="hlt">ice</span>-shelf stability suggests that warming for several centuries rendered <span class="hlt">ice</span> 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 <span class="hlt">ice</span>-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/2017Natur.541...72B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Natur.541...72B"><span>Centennial-scale Holocene climate variations amplified by <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet discharge</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bakker, Pepijn; Clark, Peter U.; Golledge, Nicholas R.; Schmittner, Andreas; Weber, Michael E.</p> <p>2017-01-01</p> <p>Proxy-based indicators of past climate change show that current global climate models systematically underestimate Holocene-epoch climate variability on centennial to multi-millennial timescales, with the mismatch increasing for longer periods. Proposed explanations for the discrepancy include ocean-atmosphere coupling that is too weak in models, insufficient energy cascades from smaller to larger spatial and temporal scales, or that global climate models do not consider slow climate feedbacks related to the carbon cycle or interactions between <span class="hlt">ice</span> sheets and climate. Such interactions, however, are known to have strongly affected centennial- to orbital-scale climate variability during past glaciations, and are likely to be important in future climate change. Here we show that fluctuations in <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet discharge caused by relatively small changes in subsurface ocean temperature can amplify multi-centennial climate variability regionally and globally, suggesting that a dynamic <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet may have driven climate fluctuations during the Holocene. We analysed high-temporal-resolution records of iceberg-rafted debris derived from the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet, and performed both high-spatial-resolution <span class="hlt">ice</span>-sheet modelling of the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet and multi-millennial global climate model simulations. <span class="hlt">Ice</span>-sheet responses to decadal-scale ocean forcing appear to be less important, possibly indicating that the future response of the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet will be governed more by long-term anthropogenic warming combined with multi-centennial natural variability than by annual or decadal climate oscillations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-GSFC_20171208_Archive_e000198.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-GSFC_20171208_Archive_e000198.html"><span>NASA Launches Eighth Year of <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Change Airborne Survey</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 the southern end of the Earth, a NASA plane carrying a team of scientists and a sophisticated instrument suite to study <span class="hlt">ice</span> is returning to surveying Antarctica. For the past eight years, Operation <span class="hlt">Ice</span>Bridge has been on a mission to build a record of how polar <span class="hlt">ice</span> is evolving in a changing environment. The information <span class="hlt">Ice</span>Bridge has gathered in the <span class="hlt">Antarctic</span>, which includes data on the thickness and shape of snow and <span class="hlt">ice</span>, as well as the topography of the land and ocean floor beneath the ocean and the <span class="hlt">ice</span>, has allowed scientists to determine that the West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet may be in irreversible decline. Researchers have also used <span class="hlt">Ice</span>Bridge data to evaluate climate models of Antarctica and map the bedrock underneath <span class="hlt">Antarctic</span> <span class="hlt">ice</span>. Read more:http://go.nasa.gov/2dxczkd NASA image use policy. NASA Goddard Space Flight Center enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. Follow us on Twitter Like us on Facebook Find us on Instagram</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040015278&hterms=BALANCE+SHEET&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DBALANCE%2BSHEET','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040015278&hterms=BALANCE+SHEET&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DBALANCE%2BSHEET"><span><span class="hlt">Antarctic</span> <span class="hlt">Ice</span>-Sheet Mass Balance from Satellite Altimetry 1992 to 2001</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zwally, H. Jay; Brenner, Anita C.; Cornejo, Helen; Giovinetto, Mario; Saba, Jack L.; Yi, Donghui</p> <p>2003-01-01</p> <p>A major uncertainty in understanding the causes of the current rate of sea level rise is the potential contributions from mass imbalances of the Greenland and <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheets. Estimates of the current mass balance of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet are derived from surface- elevation changes obtained from 9 years of ERS - 1 & 2 radar altimeter data. Elevation time-series are created from altimeter crossovers among 90-day data periods on a 50 km grid to 81.5 S. The time series are fit with a multivariate linear/sinusoidal function to give the average rate of elevation change (dH/dt). On the major Rome-Filchner, Ross, and Amery <span class="hlt">ice</span> shelves, the W d t are small or near zero. In contrast, the <span class="hlt">ice</span> shelves of the <span class="hlt">Antarctic</span> Peninsula and along the West <span class="hlt">Antarctic</span> coast appear to be thinning significantly, with a 23 +/- 3 cm per year surface elevation decrease on the Larsen <span class="hlt">ice</span> shelf and a 65 +/- 4 cm per year decrease on the Dotson <span class="hlt">ice</span> shelf. On the grounded <span class="hlt">ice</span>, significant elevation decreases are obtained over most of the drainage basins of the Pine Island and Thwaites glaciers in West Antarctica and inland of Law Dome in East Antarctica. Significant elevation increases are observed within about 200 km of the coast around much of the rest of the <span class="hlt">ice</span> sheet. Farther inland, the changes are a mixed pattern of increases and decreases with increases of a few centimeters per year at the highest elevations of the East <span class="hlt">Antarctic</span> plateau. The derived elevation changes are combined with estimates of the bedrock uplift from several models to provide maps of <span class="hlt">ice</span> thickness change. The <span class="hlt">ice</span> thickness changes enable estimates of the <span class="hlt">ice</span> mass balances for the major drainage basins, the overall mass balance, and the current contribution of the <span class="hlt">ice</span> sheet to global sea level change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.B23B0573M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.B23B0573M"><span>Time-series measurements of methane (CH4) distribution during open water and <span class="hlt">ice-cover</span> in <span class="hlt">lakes</span> throughout the Mackenzie River Delta (Canada)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>McIntosh, H.; Lapham, L.; Orcutt, B.; Wheat, C. G.; Lesack, L.; Bergstresser, M.; Dallimore, S. R.; MacLeod, R.; Cote, M.</p> <p>2016-12-01</p> <p>Arctic <span class="hlt">lakes</span> are known to emit large amounts of methane to the atmosphere and their importance to the global methane (CH4) cycle has been recognized. It is well known CH4 builds up in Arctic <span class="hlt">lakes</span> during <span class="hlt">ice-cover</span>, but the amount of and when the CH4 is released to the atmosphere is not well known. Our preliminary results suggest the largest flux of CH4 from <span class="hlt">lakes</span> to the atmosphere occurs slightly before complete <span class="hlt">ice</span>-out; while others have shown the largest flux occurs when <span class="hlt">lakes</span> overturn in the spring. During <span class="hlt">ice</span>-out, CH4 can also be oxidized by methane oxidizing bacteria before it can efflux to the atmosphere from the surface water. In order to elucidate the processes contributing to Arctic <span class="hlt">lake</span> CH4 emissions, continuous, long-term and large scale spatial sampling is required; however it is difficult to achieve in these remote locations. We address this problem using two sampling techniques. 1) We deployed osmotically powered pumps (OsmoSamplers), which were able to autonomously and continuously collect <span class="hlt">lake</span> bottom water over the course of a year from multiple <span class="hlt">lakes</span> in the Mackenzie River Delta. OsmoSamplers were placed in four <span class="hlt">lakes</span> in the mid Delta near Inuvik, Northwest Territories, Canada, two <span class="hlt">lakes</span> in the outer Delta, and two coastal <span class="hlt">lakes</span> on Richard's Island in 2015. The dissolved CH4 concentration, stable isotope content of CH4 (δ13C-CH4), and dissolved sulfate concentrations in bottom water from these <span class="hlt">lakes</span> will be presented to better understand methane dynamics under the <span class="hlt">ice</span> and over time. 2) Along with the time-series data, we will also present data from discrete samples collected from 40 <span class="hlt">lakes</span> in the mid Delta during key time periods, before and immediately after the spring <span class="hlt">ice</span>-out. By determining the CH4 dynamics throughout the year we hope to improve predictions of how CH4 emissions may change in a warming Arctic environment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19940012966','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19940012966"><span>Arctic and <span class="hlt">Antarctic</span> Sea <span class="hlt">Ice</span>, 1978-1987: Satellite Passive-Microwave Observations and Analysis</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gloersen, Per; Campbell, William J.; Cavalieri, Donald J.; Comiso, Josefino C.; Parkinson, Claire L.; Zwally, H. Jay</p> <p>1992-01-01</p> <p>This book contains a description and analysis of the spatial and temporal variations in the Arctic and <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> <span class="hlt">covers</span> from October 26, 1978 through August 20, 1987. It is based on data collected by the Scanning Multichannel Microwave Radiometer (SMMR) onboard the NASA Nimbus 7 satellite. The 8.8-year period, together with the 4 years of the Nimbus 5 Electrically Scanning Microwave Radiometer (ESMR) observations presented in two earlier volumes, comprises a sea <span class="hlt">ice</span> record spanning almost 15 years.</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> <span class="hlt">Ice</span> 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> <span class="hlt">Ice</span> 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 <span class="hlt">ice</span> 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 <span class="hlt">ice</span> 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('http://adsabs.harvard.edu/abs/2018JGRC..123.1907W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRC..123.1907W"><span>Estimation of <span class="hlt">Antarctic</span> Land-Fast Sea <span class="hlt">Ice</span> Algal Biomass and Snow Thickness From Under-<span class="hlt">Ice</span> Radiance Spectra in Two Contrasting Areas</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wongpan, P.; Meiners, K. M.; Langhorne, P. J.; Heil, P.; Smith, I. J.; Leonard, G. H.; Massom, R. A.; Clementson, L. A.; Haskell, T. G.</p> <p>2018-03-01</p> <p>Fast <span class="hlt">ice</span> is an important component of <span class="hlt">Antarctic</span> coastal marine ecosystems, providing a prolific habitat for <span class="hlt">ice</span> algal communities. This work examines the relationships between normalized difference indices (NDI) calculated from under-<span class="hlt">ice</span> radiance measurements and sea <span class="hlt">ice</span> algal biomass and snow thickness for <span class="hlt">Antarctic</span> fast <span class="hlt">ice</span>. While this technique has been calibrated to assess biomass in Arctic fast <span class="hlt">ice</span> and pack <span class="hlt">ice</span>, as well as <span class="hlt">Antarctic</span> pack <span class="hlt">ice</span>, relationships are currently lacking for <span class="hlt">Antarctic</span> fast <span class="hlt">ice</span> characterized by bottom <span class="hlt">ice</span> algae communities with high algal biomass. We analyze measurements along transects at two contrasting <span class="hlt">Antarctic</span> fast <span class="hlt">ice</span> sites in terms of platelet <span class="hlt">ice</span> presence: near and distant from an <span class="hlt">ice</span> shelf, i.e., in McMurdo Sound and off Davis Station, respectively. Snow and <span class="hlt">ice</span> thickness, and <span class="hlt">ice</span> salinity and temperature measurements support our paired in situ optical and biological measurements. Analyses show that NDI wavelength pairs near the first chlorophyll a (chl a) absorption peak (≈440 nm) explain up to 70% of the total variability in algal biomass. Eighty-eight percent of snow thickness variability is explained using an NDI with a wavelength pair of 648 and 567 nm. Accounting for pigment packaging effects by including the ratio of chl a-specific absorption coefficients improved the NDI-based algal biomass estimation only slightly. Our new observation-based algorithms can be used to estimate <span class="hlt">Antarctic</span> fast <span class="hlt">ice</span> algal biomass and snow thickness noninvasively, for example, by using moored sensors (time series) or mapping their spatial distributions using underwater vehicles.</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 <span class="hlt">Ice</span> 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-<span class="hlt">ice</span> extent in the Southern Ocean and a small number of paleo sea-<span class="hlt">ice</span> 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 <span class="hlt">ice</span> 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 <span class="hlt">ice</span>, water column and sediment samples. To provide further insights into the use of these HBIs as proxies for <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span>, we here describe an assessment of their distributions in surface water, surface sediment and sea <span class="hlt">ice</span> samples collected from a number of <span class="hlt">Antarctic</span> locations experiencing contrasting sea <span class="hlt">ice</span> conditions in recent years. Our study shows that distributions of a di-unsaturated HBI (diene II) and tri-unsaturated HBI (triene III) in surface water samples were found to be extremely sensitive to the local sea-<span class="hlt">ice</span> conditions, with diene II detected for sampling sites that experienced seasonal sea <span class="hlt">ice</span> and highest concentrations found in coastal locations with longer-lasting <span class="hlt">ice</span> <span class="hlt">cover</span> 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 <span class="hlt">ice</span> edge, an observation consistent with significant environmental control over the biosynthesis of diene II and triene III by sea <span class="hlt">ice</span> diatoms and open water 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://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5510715','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5510715"><span>West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet retreat driven by Holocene warm water incursions</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>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</p> <p>2017-01-01</p> <p>Glaciological and oceanographic observations coupled with numerical models show that warm Circumpolar Deep Water (CDW) upwelling onto the West <span class="hlt">Antarctic</span> continental shelf causes melting of the undersides of floating <span class="hlt">ice</span> shelves. Because these <span class="hlt">ice</span> shelves buttress glaciers feeding into them, their ocean-induced thinning is driving <span class="hlt">Antarctic</span> <span class="hlt">ice</span>-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 <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> 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 <span class="hlt">ice</span>-shelf collapse may have caused rapid <span class="hlt">ice</span>-sheet thinning further upstream, and since the 1940s. These results increase confidence in the predictive capability of current <span class="hlt">ice</span>-sheet models. PMID:28682333</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ISPAr42.3.2625L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ISPAr42.3.2625L"><span>Compiling Techniques for East <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Velocity Mapping Based on Historical Optical Imagery</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, X.; Li, R.; Qiao, G.; Cheng, Y.; Ye, W.; Gao, T.; Huang, Y.; Tian, Y.; Tong, X.</p> <p>2018-05-01</p> <p><span class="hlt">Ice</span> flow velocity over long time series in East Antarctica plays a vital role in estimating and predicting the mass balance of <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet and its contribution to global sea level rise. However, there is no <span class="hlt">Antarctic</span> <span class="hlt">ice</span> velocity product with large space scale available showing the East <span class="hlt">Antarctic</span> <span class="hlt">ice</span> flow velocity pattern before the 1990s. We proposed three methods including parallax decomposition, grid-based NCC image matching, feature and gird-based image matching with constraints for estimation of surface velocity in East Antarctica based on ARGON KH-5 and LANDSAT imagery, showing the feasibility of using historical optical imagery to obtain <span class="hlt">Antarctic</span> <span class="hlt">ice</span> motion. Based on these previous studies, we presented a set of systematic method for developing <span class="hlt">ice</span> surface velocity product for the entire East Antarctica from the 1960s to the 1980s in this paper.</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 <span class="hlt">ice</span> 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 <span class="hlt">ice</span>. Lead-lag relationships involving regional sea <span class="hlt">ice</span> and air temperature are systematically evaluated, with an eye toward the <span class="hlt">ice</span>-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 <span class="hlt">ice</span> 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 <span class="hlt">ice</span> coverage is small but negative. Lag correlations between seasonal anomalies of the two variables are generally stronger with <span class="hlt">ice</span> lagging the summer temperatures and with <span class="hlt">ice</span> leading the winter temperatures. The implication is that summer temperatures predispose the near-surface waters to above-or below-normal <span class="hlt">ice</span> coverage in the following fall and winter.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003AGUFMPP31C0273B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003AGUFMPP31C0273B"><span><span class="hlt">Antarctic</span> Glaciological Data at NSIDC: field data, temperature, and <span class="hlt">ice</span> velocity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bauer, R.; Bohlander, J.; Scambos, T.; Berthier, E.; Raup, B.; Scharfen, G.</p> <p>2003-12-01</p> <p>An extensive collection of many <span class="hlt">Antarctic</span> glaciological parameters is available for the polar science community upon request. The National Science Foundation's Office of Polar Programs funds the <span class="hlt">Antarctic</span> Glaciological Data Center (AGDC) at the National Snow and <span class="hlt">Ice</span> Data Center (NSIDC) to archive and distribute <span class="hlt">Antarctic</span> glaciological and cryospheric system data collected by the U.S. <span class="hlt">Antarctic</span> Program. AGDC facilitates data exchange among Principal Investigators, preserves recently collected data useful to future research, gathers data sets from past research, and compiles continent-wide information useful for modeling and field work planning. Data sets are available via our web site, http://nsidc.org/agdc/. From here, users can access extensive documentation, citation information, locator maps, derived images and references, and the numerical data. More than 50 <span class="hlt">Antarctic</span> scientists have contributed data to the archive. Among the compiled products distributed by AGDC are VELMAP and THERMAP. THERMAP is a compilation of over 600 shallow firn temperature measurements ('10-meter temperatures') collected since 1950. These data provide a record of mean annual temperature, and potentially hold a record of climate change on the continent. The data are represented with maps showing the traverse route, and include data sources, measurement technique, and additional measurements made at each site, i.e., snow density and accumulation. VELMAP is an archive of surface <span class="hlt">ice</span> velocity measurements for the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet. The primary objective of VELMAP is to assemble a historic record of outlet glaciers and <span class="hlt">ice</span> shelf <span class="hlt">ice</span> motion over the <span class="hlt">Antarctic</span>. The collection includes both PI-contributed measurements and data generated at NSIDC using Landsat and SPOT satellite imagery. Tabular data contain position, speed, bearing, and data quality information, and related references. Two new VELMAP data sets are highlighted: the Mertz Glacier and the Institute <span class="hlt">Ice</span> Stream. Mertz Glacier <span class="hlt">ice</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_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://ntrs.nasa.gov/search.jsp?R=19820036704&hterms=Parkinsons+circulation&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DParkinsons%2Bcirculation','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19820036704&hterms=Parkinsons+circulation&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DParkinsons%2Bcirculation"><span>Large-scale variations in observed <span class="hlt">Antarctic</span> Sea <span class="hlt">ice</span> extent and associated atmospheric circulation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Cavalieri, D. J.; Parkinson, C. L.</p> <p>1981-01-01</p> <p>The 1974 <span class="hlt">Antarctic</span> large scale sea <span class="hlt">ice</span> extent is studied from data from Nimbus 2 and 5 and temperature and sea level pressure fields from the Australian Meteorological Data Set. Electrically Scanning Microwave Radiometer data were three-day averaged and compared with 1000 mbar atmospheric pressure and sea level pressure data, also in three-day averages. Each three-day period was subjected to a Fourier analysis and included the mean latitude of the <span class="hlt">ice</span> extent and the phases and percent variances in terms of the first six Fourier harmonics. Centers of low pressure were found to be generally east of regions which displayed rapid <span class="hlt">ice</span> growth, and winds acted to extend the <span class="hlt">ice</span> equatorward. An atmospheric response was also noted as caused by the changing <span class="hlt">ice</span> <span class="hlt">cover</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1614162B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1614162B"><span>The role of <span class="hlt">ice</span> shelves in the Holocene evolution of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bernales, Jorge; Rogozhina, Irina; Thomas, Maik</p> <p>2014-05-01</p> <p>Using the continental-scale <span class="hlt">ice</span> sheet-shelf model SICOPOLIS (Greve, 1997 [1]; Sato and Greve, 2012 [2]), we assess the influence of <span class="hlt">ice</span> shelves on the Holocene evolution and present-day geometry of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet. We have designed a series of paleoclimate simulations driven by a time-evolved climate forcing that couples the surface temperature record from the Vostok <span class="hlt">ice</span> core with precipitation pattern using an empirical relation of Dahl-Jensen et al., (1998) [3]. Our numerical experiments show that the geometry of <span class="hlt">ice</span> shelves is determined by the evolution of climate and ocean conditions over time scales of 15 to 25 kyr. This implies that the initial configuration of <span class="hlt">ice</span> shelves at the Last Glacial Maximum (LGM, about 21 kyr before present) has a significant effect on the modelled Early Holocene volume of <span class="hlt">ice</span> shelves (up to 20%) that gradually diminishes to a negligible level for the present-day <span class="hlt">ice</span> shelf configuration. Thus, the present-day geometry of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> shelves can be attained even if an <span class="hlt">ice</span>-shelf-free initial condition is chosen at the LGM. However, the grounded <span class="hlt">ice</span> volume, thickness and dynamic states are found to be sensitive to the <span class="hlt">ice</span> shelf dynamics over a longer history spanning several tens of thousands of years. A presence of extensive marine <span class="hlt">ice</span> at the LGM, supported by sediment core reconstructions (e.g. Naish et al., 2009 [4]), has a clear buttressing effect on the grounded <span class="hlt">ice</span> that remains significant over a period of 30 to 50 kyr. If <span class="hlt">ice</span>-shelf-free conditions are prescribed at the LGM, the modelled Early Holocene and present-day grounded <span class="hlt">ice</span> volumes are underestimated by up to 10%, as opposed to simulations incorporating <span class="hlt">ice</span> shelf dynamics over longer periods. The use of <span class="hlt">ice</span>-shelf-free LGM conditions thus results in 50 to over 200 meters thinner <span class="hlt">ice</span> sheet across much of East Antarctica. References [1] Greve, R. (1997). Application of a polythermal three-dimensional <span class="hlt">ice</span> sheet model to the Greenland <span class="hlt">ice</span> sheet: response to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C51C0999X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C51C0999X"><span>Snowmelt Pattern and <span class="hlt">Lake</span> <span class="hlt">Ice</span> Phenology around Tibetan Plateau Estimated from Enhanced Resolution Passive Microwave Data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xiong, C.; Shi, J.; Wang, T.</p> <p>2017-12-01</p> <p>Snow and <span class="hlt">ice</span> is very sensitive to the climate change. Rising air temperature will cause the snowmelt time change. In contrast, the change in snow state will have feedback on climate through snow albedo. The snow melt timing is also correlated with the associated runoff. <span class="hlt">Ice</span> phenology describes the seasonal cycle of <span class="hlt">lake</span> <span class="hlt">ice</span> <span class="hlt">cover</span> and includes freeze-up and breakup periods and <span class="hlt">ice</span> <span class="hlt">cover</span> duration, which is an important weather and climate indicator. It is also important for <span class="hlt">lake</span>-atmosphere interactions and hydrological and ecological processes. The enhanced resolution (up to 3.125 km) passive microwave data is used to estimate the snowmelt pattern and <span class="hlt">lake</span> <span class="hlt">ice</span> phenology on and around Tibetan Plateau. The enhanced resolution makes the estimation of snowmelt and <span class="hlt">lake</span> <span class="hlt">ice</span> phenology in more spatial detail compared to previous 25 km gridded passive microwave data. New algorithm based on smooth filters and change point detection was developed to estimate the snowmelt and <span class="hlt">lake</span> <span class="hlt">ice</span> freeze-up and break-up timing. Spatial and temporal pattern of snowmelt and <span class="hlt">lake</span> <span class="hlt">ice</span> phonology are estimated. This study provides an objective evidence of climate change impact on the cryospheric system on Tibetan Plateau. The results show significant earlier snowmelt and <span class="hlt">lake</span> <span class="hlt">ice</span> break-up in some regions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120013495','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120013495"><span>Mass Gains of the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet Exceed Losses</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zwally, H. Jay; Li, Jun; Robbins, John; Saba, Jack L.; Yi, Donghui; Brenner, Anita; Bromwich, David</p> <p>2012-01-01</p> <p>During 2003 to 2008, the mass gain of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet from snow accumulation exceeded the mass loss from <span class="hlt">ice</span> discharge by 49 Gt/yr (2.5% of input), as derived from ICESat laser measurements of elevation change. The net gain (86 Gt/yr) over the West <span class="hlt">Antarctic</span> (WA) and East <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheets (WA and EA) is essentially unchanged from revised results for 1992 to 2001 from ERS radar altimetry. Imbalances in individual drainage systems (DS) are large (-68% to +103% of input), as are temporal changes (-39% to +44%). The recent 90 Gt/yr loss from three DS (Pine Island, Thwaites-Smith, and Marie-Bryd Coast) of WA exceeds the earlier 61 Gt/yr loss, consistent with reports of accelerating <span class="hlt">ice</span> flow and dynamic thinning. Similarly, the recent 24 Gt/yr loss from three DS in the <span class="hlt">Antarctic</span> Peninsula (AP) is consistent with glacier accelerations following breakup of the Larsen B and other <span class="hlt">ice</span> shelves. In contrast, net increases in the five other DS of WA and AP and three of the 16 DS in East Antarctica (EA) exceed the increased losses. Alternate interpretations of the mass changes driven by accumulation variations are given using results from atmospheric-model re-analysis and a parameterization based on 5% change in accumulation per degree of observed surface temperature change. A slow increase in snowfall with climate waRMing, consistent with model predictions, may be offsetting increased dynamic losses.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5351862','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5351862"><span><span class="hlt">Ice-cover</span> is the principal driver of ecological change in High Arctic <span class="hlt">lakes</span> and ponds</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, Katherine; Michelutti, Neal; Sugar, Madeline; Douglas, Marianne S. V.; Smol, John P.</p> <p>2017-01-01</p> <p>Recent climate change has been especially pronounced in the High Arctic, however, the responses of aquatic biota, such as diatoms, can be modified by site-specific environmental characteristics. To assess if climate-mediated <span class="hlt">ice</span> <span class="hlt">cover</span> changes affect the diatom response to climate, we used paleolimnological techniques to examine shifts in diatom assemblages from ten High Arctic <span class="hlt">lakes</span> and ponds from Ellesmere Island and nearby Pim Island (Nunavut, Canada). The sites were divided a priori into four groups (“warm”, “cool”, “cold”, and “oasis”) based on local elevation and microclimatic differences that result in differing lengths of the <span class="hlt">ice</span>-free season, as well as about three decades of personal observations. We characterized the species changes as a shift from Condition 1 (i.e. a generally low diversity, predominantly epipelic and epilithic diatom assemblage) to Condition 2 (i.e. a typically more diverse and ecologically complex assemblage with an increasing proportion of epiphytic species). This shift from Condition 1 to Condition 2 was a consistent pattern recorded across the sites that experienced a change in <span class="hlt">ice</span> <span class="hlt">cover</span> with warming. The “warm” sites are amongst the first to lose their <span class="hlt">ice</span> <span class="hlt">covers</span> in summer and recorded the earliest and highest magnitude changes. The “cool” sites also exhibited a shift from Condition 1 to Condition 2, but, as predicted, the timing of the response lagged the “warm” sites. Meanwhile some of the “cold” sites, which until recently still retained an <span class="hlt">ice</span> raft in summer, only exhibited this shift in the upper-most sediments. The warmer “oasis” ponds likely supported aquatic vegetation throughout their records. Consequently, the diatoms of the “oasis” sites were characterized as high-diversity, Condition 2 assemblages throughout the record. Our results support the hypothesis that the length of the <span class="hlt">ice</span>-free season is the principal driver of diatom assemblage responses to climate in the High Arctic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28296897','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28296897"><span><span class="hlt">Ice-cover</span> is the principal driver of ecological change in High Arctic <span class="hlt">lakes</span> and ponds.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Griffiths, Katherine; Michelutti, Neal; Sugar, Madeline; Douglas, Marianne S V; Smol, John P</p> <p>2017-01-01</p> <p>Recent climate change has been especially pronounced in the High Arctic, however, the responses of aquatic biota, such as diatoms, can be modified by site-specific environmental characteristics. To assess if climate-mediated <span class="hlt">ice</span> <span class="hlt">cover</span> changes affect the diatom response to climate, we used paleolimnological techniques to examine shifts in diatom assemblages from ten High Arctic <span class="hlt">lakes</span> and ponds from Ellesmere Island and nearby Pim Island (Nunavut, Canada). The sites were divided a priori into four groups ("warm", "cool", "cold", and "oasis") based on local elevation and microclimatic differences that result in differing lengths of the <span class="hlt">ice</span>-free season, as well as about three decades of personal observations. We characterized the species changes as a shift from Condition 1 (i.e. a generally low diversity, predominantly epipelic and epilithic diatom assemblage) to Condition 2 (i.e. a typically more diverse and ecologically complex assemblage with an increasing proportion of epiphytic species). This shift from Condition 1 to Condition 2 was a consistent pattern recorded across the sites that experienced a change in <span class="hlt">ice</span> <span class="hlt">cover</span> with warming. The "warm" sites are amongst the first to lose their <span class="hlt">ice</span> <span class="hlt">covers</span> in summer and recorded the earliest and highest magnitude changes. The "cool" sites also exhibited a shift from Condition 1 to Condition 2, but, as predicted, the timing of the response lagged the "warm" sites. Meanwhile some of the "cold" sites, which until recently still retained an <span class="hlt">ice</span> raft in summer, only exhibited this shift in the upper-most sediments. The warmer "oasis" ponds likely supported aquatic vegetation throughout their records. Consequently, the diatoms of the "oasis" sites were characterized as high-diversity, Condition 2 assemblages throughout the record. Our results support the hypothesis that the length of the <span class="hlt">ice</span>-free season is the principal driver of diatom assemblage responses to climate in the High Arctic, largely driven by the establishment of new</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> <span class="hlt">Ice</span> [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> <span class="hlt">ice</span> 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 <span class="hlt">Ice</span> Shelf, about 12.5 miles away from open water. NASA scientists were using a borehole camera to look back up towards the <span class="hlt">ice</span> surface when they spotted this pinkish-orange creature swimming beneath the <span class="hlt">ice</span>. Credit: NASA</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C21A0687M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C21A0687M"><span>Decadal-Scale Response of the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> sheet to a Warming Ocean using the POPSICLES Coupled <span class="hlt">Ice</span> Sheet-Ocean model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Martin, D. F.; Asay-Davis, X.; Cornford, S. L.; Price, S. F.; Ng, E. G.; Collins, W.</p> <p>2015-12-01</p> <p>We present POPSICLES simulation results <span class="hlt">covering</span> the full <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet and the Southern Ocean spanning the period from 1990 to 2010. We use the CORE v. 2 interannual forcing data to force the ocean model. Simulations are performed at 0.1o(~5 km) ocean resolution with adaptive <span class="hlt">ice</span> sheet resolution as fine as 500 m to adequately resolve the grounding line dynamics. We discuss the effect of improved ocean mixing and subshelf bathymetry (vs. the standard Bedmap2 bathymetry) on the behavior of the coupled system, comparing time-averaged melt rates below a number of major <span class="hlt">ice</span> shelves with those reported in the literature. We also present seasonal variability and decadal melting trends from several <span class="hlt">Antarctic</span> regions, along with the response of the <span class="hlt">ice</span> shelves and the consequent dynamic response of the grounded <span class="hlt">ice</span> sheet.POPSICLES couples the POP2x ocean model, a modified version of the Parallel Ocean Program, and the BISICLES <span class="hlt">ice</span>-sheet model. POP2x includes sub-<span class="hlt">ice</span>-shelf circulation using partial top cells and the commonly used three-equation boundary layer physics. Standalone POP2x output compares well with standard <span class="hlt">ice</span>-ocean test cases (e.g., ISOMIP) and other continental-scale simulations and melt-rate observations. BISICLES makes use of adaptive mesh refinement and a 1st-order accurate momentum balance similar to the L1L2 model of Schoof and Hindmarsh to accurately model regions of dynamic complexity, such as <span class="hlt">ice</span> streams, outlet glaciers, and grounding lines. Results of BISICLES simulations have compared favorably to comparable simulations with a Stokes momentum balance in both idealized tests (MISMIP-3d) and realistic configurations.The figure shows the BISICLES-computed vertically-integrated grounded <span class="hlt">ice</span> velocity field 5 years into a 20-year coupled full-continent <span class="hlt">Antarctic</span>-Southern-Ocean simulation. Submarine melt rates are painted onto the surface of the floating <span class="hlt">ice</span> shelves. Grounding lines are shown in green.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013CliPa...9..749S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013CliPa...9..749S"><span>Direct linking of Greenland and <span class="hlt">Antarctic</span> <span class="hlt">ice</span> cores at the Toba eruption (74 ka BP)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Svensson, A.; Bigler, M.; Blunier, T.; Clausen, H. B.; Dahl-Jensen, D.; Fischer, H.; Fujita, S.; Goto-Azuma, K.; Johnsen, S. J.; Kawamura, K.; Kipfstuhl, S.; Kohno, M.; Parrenin, F.; Popp, T.; Rasmussen, S. O.; Schwander, J.; Seierstad, I.; Severi, M.; Steffensen, J. P.; Udisti, R.; Uemura, R.; Vallelonga, P.; Vinther, B. M.; Wegner, A.; Wilhelms, F.; Winstrup, M.</p> <p>2013-03-01</p> <p>The Toba eruption that occurred some 74 ka ago in Sumatra, Indonesia, is among the largest volcanic events on Earth over the last 2 million years. Tephra from this eruption has been spread over vast areas in Asia, where it constitutes a major time marker close to the Marine Isotope Stage 4/5 boundary. As yet, no tephra associated with Toba has been identified in Greenland or <span class="hlt">Antarctic</span> <span class="hlt">ice</span> cores. Based on new accurate dating of Toba tephra and on accurately dated European stalagmites, the Toba event is known to occur between the onsets of Greenland interstadials (GI) 19 and 20. Furthermore, the existing linking of Greenland and <span class="hlt">Antarctic</span> <span class="hlt">ice</span> cores by gas records and by the bipolar seesaw hypothesis suggests that the <span class="hlt">Antarctic</span> counterpart is situated between <span class="hlt">Antarctic</span> Isotope Maxima (AIM) 19 and 20. In this work we suggest a direct synchronization of Greenland (NGRIP) and <span class="hlt">Antarctic</span> (EDML) <span class="hlt">ice</span> cores at the Toba eruption based on matching of a pattern of bipolar volcanic spikes. Annual layer counting between volcanic spikes in both cores allows for a unique match. We first demonstrate this bipolar matching technique at the already synchronized Laschamp geomagnetic excursion (41 ka BP) before we apply it to the suggested Toba interval. The Toba synchronization pattern <span class="hlt">covers</span> some 2000 yr in GI-20 and AIM-19/20 and includes nine acidity peaks that are recognized in both <span class="hlt">ice</span> cores. The suggested bipolar Toba synchronization has decadal precision. It thus allows a determination of the exact phasing of inter-hemispheric climate in a time interval of poorly constrained <span class="hlt">ice</span> core records, and it allows for a discussion of the climatic impact of the Toba eruption in a global perspective. The bipolar linking gives no support for a long-term global cooling caused by the Toba eruption as Antarctica experiences a major warming shortly after the event. Furthermore, our bipolar match provides a way to place palaeo-environmental records other than <span class="hlt">ice</span> cores into a precise climatic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017NatGe..10..582M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017NatGe..10..582M"><span>Microbial oxidation as a methane sink beneath the West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Michaud, Alexander B.; Dore, John E.; Achberger, Amanda M.; Christner, Brent C.; Mitchell, Andrew C.; Skidmore, Mark L.; Vick-Majors, Trista J.; Priscu, John C.</p> <p>2017-08-01</p> <p>Aquatic habitats beneath <span class="hlt">ice</span> masses contain active microbial ecosystems capable of cycling important greenhouse gases, such as methane (CH4). A large methane reservoir is thought to exist beneath the West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet, but its quantity, source and ultimate fate are poorly understood. For instance, O2 supplied by basal melting should result in conditions favourable for aerobic methane oxidation. Here we use measurements of methane concentrations and stable isotope compositions along with genomic analyses to assess the sources and cycling of methane in Subglacial <span class="hlt">Lake</span> Whillans (SLW) in West Antarctica. We show that sub-<span class="hlt">ice</span>-sheet methane is produced through the biological reduction of CO2 using H2. This methane pool is subsequently consumed by aerobic, bacterial methane oxidation at the SLW sediment-water interface. Bacterial oxidation consumes >99% of the methane and represents a significant methane sink, and source of biomass carbon and metabolic energy to the surficial SLW sediments. We conclude that aerobic methanotrophy may mitigate the release of methane to the atmosphere upon subglacial water drainage to <span class="hlt">ice</span> sheet margins and during periods of deglaciation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFMPP11B1783E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFMPP11B1783E"><span>An unusual early Holocene diatom event north of the Getz <span class="hlt">Ice</span> Shelf (Amundsen Sea): Implications for West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet development</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Esper, O.; Gersonde, R.; Hillenbrand, C.; Kuhn, G.; Smith, J.</p> <p>2011-12-01</p> <p>Modern global change affects not only the polar north but also, and to increasing extent, the southern high latitudes, especially the <span class="hlt">Antarctic</span> regions <span class="hlt">covered</span> by the West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet (WAIS). Consequently, knowledge of the mechanisms controlling past WAIS dynamics and WAIS behaviour at the last deglaciation is critical to predict its development in a future warming world. Geological and palaeobiological information from major drainage areas of the WAIS, like the Amundsen Sea Embayment, shed light on the history of the WAIS glaciers. Sediment records obtained from a deep inner shelf basin north of Getz <span class="hlt">Ice</span> Shelf document a deglacial warming in three phases. Above a glacial diamicton and a sediment package barren of microfossils that document sediment deposition by grounded <span class="hlt">ice</span> and below an <span class="hlt">ice</span> shelf or perennial sea <span class="hlt">ice</span> <span class="hlt">cover</span> (possibly fast <span class="hlt">ice</span>), respectively, a sediment section with diatom assemblages dominated by sea <span class="hlt">ice</span> taxa indicates <span class="hlt">ice</span> shelf retreat and seasonal <span class="hlt">ice</span>-free conditions. This conclusion is supported by diatom-based summer temperature reconstructions. The early retreat was followed by a phase, when exceptional diatom ooze was deposited around 12,500 cal. years B.P. [1]. Microscopical inspection of this ooze revealed excellent preservation of diatom frustules of the species Corethron pennatum together with vegetative Chaetoceros, thus an assemblage usually not preserved in the sedimentary record. Sediments succeeding this section contain diatom assemblages indicating rather constant Holocene cold water conditions with seasonal sea <span class="hlt">ice</span>. The deposition of the diatom ooze can be related to changes in hydrographic conditions including strong advection of nutrients. However, sediment focussing in the partly steep inner shelf basins cannot be excluded as a factor enhancing the thickness of the ooze deposits. It is not only the presence of the diatom ooze but also the exceptional preservation and the species composition of the diatom assemblage</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014SolE....5..569A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014SolE....5..569A"><span>Future <span class="hlt">Antarctic</span> bed topography and its implications for <span class="hlt">ice</span> sheet dynamics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Adhikari, S.; Ivins, E. R.; Larour, E.; Seroussi, H.; Morlighem, M.; Nowicki, S.</p> <p>2014-06-01</p> <p>The <span class="hlt">Antarctic</span> bedrock is evolving as the solid Earth responds to the past and ongoing evolution of the <span class="hlt">ice</span> sheet. A recently improved <span class="hlt">ice</span> loading history suggests that the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet (AIS) has generally been losing its mass since the Last Glacial Maximum. In a sustained warming climate, the AIS is predicted to retreat at a greater pace, primarily via melting beneath the <span class="hlt">ice</span> shelves. We employ the glacial isostatic adjustment (GIA) capability of the <span class="hlt">Ice</span> Sheet System Model (ISSM) to combine these past and future <span class="hlt">ice</span> loadings and provide the new solid Earth computations for the AIS. We find that past loading is relatively less important than future loading for the evolution of the future bed topography. Our computations predict that the West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet (WAIS) may uplift by a few meters and a few tens of meters at years AD 2100 and 2500, respectively, and that the East <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet is likely to remain unchanged or subside minimally except around the Amery <span class="hlt">Ice</span> Shelf. The Amundsen Sea Sector in particular is predicted to rise at the greatest rate; one hundred years of <span class="hlt">ice</span> evolution in this region, for example, predicts that the coastline of Pine Island Bay will approach roughly 45 mm yr-1 in viscoelastic vertical motion. Of particular importance, we systematically demonstrate that the effect of a pervasive and large GIA uplift in the WAIS is generally associated with the flattening of reverse bed slope, reduction of local sea depth, and thus the extension of grounding line (GL) towards the continental shelf. Using the 3-D higher-order <span class="hlt">ice</span> flow capability of ISSM, such a migration of GL is shown to inhibit the <span class="hlt">ice</span> flow. This negative feedback between the <span class="hlt">ice</span> sheet and the solid Earth may promote stability in marine portions of the <span class="hlt">ice</span> sheet in the future.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014SolED...6..191A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014SolED...6..191A"><span>Future <span class="hlt">Antarctic</span> bed topography and its implications for <span class="hlt">ice</span> sheet dynamics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Adhikari, S.; Ivins, E.; Larour, E.; Seroussi, H.; Morlighem, M.; Nowicki, S.</p> <p>2014-01-01</p> <p>The <span class="hlt">Antarctic</span> bedrock is evolving as the solid Earth responds to the past and ongoing evolution of the <span class="hlt">ice</span> sheet. A~recently improved <span class="hlt">ice</span> loading history suggests that the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet (AIS) is generally losing its mass since the last glacial maximum (LGM). In a sustained warming climate, the AIS is predicted to retreat at a greater pace primarily via melting beneath the <span class="hlt">ice</span> shelves. We employ the glacial isostatic adjustment (GIA) capability of the <span class="hlt">Ice</span> Sheet System Model (ISSM) to combine these past and future <span class="hlt">ice</span> loadings and provide the new solid Earth computations for the AIS. We find that the past loading is relatively less important than future loading on the evolution of the future bed topography. Our computations predict that the West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet (WAIS) may uplift by a few meters and a few tens of meters at years 2100 and 2500 AD, respectively, and that the East <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet (EAIS) is likely to remain unchanged or subside minimally except around the Amery <span class="hlt">Ice</span> Shelf. The Amundsen Sea Sector in particular is predicted to rise at the greatest rate; one hundred years of <span class="hlt">ice</span> evolution in this region, for example, predicts that the coastline of Pine Island Bay approaches roughly 45 mm yr-1 in viscoelastic vertical motion. Of particular importance, we systematically demonstrate that the effect of a pervasive and large GIA uplift in the WAIS is associated with the flattening of reverse bed, reduction of local sea depth, and thus the extension of grounding line (GL) towards the continental shelf. Using the 3-D higher-order <span class="hlt">ice</span> flow capability of ISSM, such a migration of GL is shown to inhibit the <span class="hlt">ice</span> flow. This negative feedback between the <span class="hlt">ice</span> sheet and the solid Earth may promote the stability to marine portions of the <span class="hlt">ice</span> sheet in future.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140017427','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140017427"><span>Future <span class="hlt">Antarctic</span> Bed Topography and Its Implications for <span class="hlt">Ice</span> Sheet Dynamics</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Adhikari, Surendra; Ivins, Erik R.; Larour, Eric Y.; Seroussi, Helene L.; Morlighem, Mathieu; Nowicki, S.</p> <p>2014-01-01</p> <p>The <span class="hlt">Antarctic</span> bedrock is evolving as the solid Earth responds to the past and ongoing evolution of the <span class="hlt">ice</span> sheet. A recently improved <span class="hlt">ice</span> loading history suggests that the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet (AIS) has generally been losing its mass since the Last Glacial Maximum. In a sustained warming climate, the AIS is predicted to retreat at a greater pace, primarily via melting beneath the <span class="hlt">ice</span> shelves.We employ the glacial isostatic adjustment (GIA) capability of the <span class="hlt">Ice</span> Sheet System Model (ISSM) to combine these past and future <span class="hlt">ice</span> loadings and provide the new solid Earth computations for the AIS.We find that past loading is relatively less important than future loading for the evolution of the future bed topography. Our computations predict that the West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet (WAIS) may uplift by a few meters and a few tens of meters at years AD 2100 and 2500, respectively, and that the East <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet is likely to remain unchanged or subside minimally except around the Amery <span class="hlt">Ice</span> Shelf. The Amundsen Sea Sector in particular is predicted to rise at the greatest rate; one hundred years of <span class="hlt">ice</span> evolution in this region, for example, predicts that the coastline of Pine Island Bay will approach roughly 45mmyr-1 in viscoelastic vertical motion. Of particular importance, we systematically demonstrate that the effect of a pervasive and large GIA uplift in the WAIS is generally associated with the flattening of reverse bed slope, reduction of local sea depth, and thus the extension of grounding line (GL) towards the continental shelf. Using the 3-D higher-order <span class="hlt">ice</span> flow capability of ISSM, such a migration of GL is shown to inhibit the <span class="hlt">ice</span> flow. This negative feedback between the <span class="hlt">ice</span> sheet and the solid Earth may promote stability in marine portions of the <span class="hlt">ice</span> sheet in the future.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28682333','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28682333"><span>West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet retreat driven by Holocene warm water incursions.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>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</p> <p>2017-07-05</p> <p>Glaciological and oceanographic observations coupled with numerical models show that warm Circumpolar Deep Water (CDW) incursions onto the West <span class="hlt">Antarctic</span> continental shelf cause melting of the undersides of floating <span class="hlt">ice</span> shelves. Because these <span class="hlt">ice</span> shelves buttress glaciers feeding into them, their ocean-induced thinning is driving <span class="hlt">Antarctic</span> <span class="hlt">ice</span>-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 <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> 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 <span class="hlt">ice</span>-shelf collapse may have caused rapid <span class="hlt">ice</span>-sheet thinning further upstream-and since the 1940s. These results increase confidence in the predictive capability of current <span class="hlt">ice</span>-sheet models.</p> </li> <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><span class="hlt">Ice</span> in Channels and <span class="hlt">Ice</span>-Rock Mixtures in Valleys on Mars: Did They Slide on Deformable Rubble Like <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> 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 <span class="hlt">ice</span> streams in Antarctica reveal a mechanism of basal motion that may apply to channels and valleys on Mars. The mechanism is sliding of the <span class="hlt">ice</span> on deformable water-saturated till under high pore pressures. It has been suggested by Lucchitta that <span class="hlt">ice</span> was present in outflow channels on Mars and gave them their distinctive morphology. This <span class="hlt">ice</span> may have slid like <span class="hlt">Antarctic</span> <span class="hlt">ice</span> streams but on rubbly weathering products rather than till. However, to generate water under high pore pressures, elevated heatflow is needed to melt the base of the <span class="hlt">ice</span>. 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 <span class="hlt">ice</span>-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 <span class="hlt">Ice</span> 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 <span class="hlt">ice</span> streams during the last glacial advance. Additional similarities of <span class="hlt">Antarctic</span> <span class="hlt">ice</span> streams with martian outflow channels are apparent. <span class="hlt">Antarctic</span> <span class="hlt">ice</span> streams are 30 to 80 km wide and hundreds of kilometers long. Martian outflow channels have similar dimensions. <span class="hlt">Ice</span> 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> <span class="hlt">ice</span> 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('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> <span class="hlt">ice</span> 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> <span class="hlt">ice</span> shelves using a circumpolar coupled <span class="hlt">ice</span> shelf-sea <span class="hlt">ice</span>-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 <span class="hlt">ice</span> 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 water 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 Water. Meltwaters originating from <span class="hlt">ice</span> 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 <span class="hlt">ice</span> shelf and ocean is neglected regionally demonstrates that the basal meltwater of each <span class="hlt">ice</span> shelf impacts sea <span class="hlt">ice</span> 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('https://pubs.er.usgs.gov/publication/70020442','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70020442"><span><span class="hlt">Ice</span> 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> <span class="hlt">Ice</span> 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 <span class="hlt">ice</span> sheet volume. An additional way of determining <span class="hlt">ice</span> 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 <span class="hlt">ice</span> 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 <span class="hlt">ice</span> 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://ntrs.nasa.gov/search.jsp?R=19950053174&hterms=3G&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3D3G','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19950053174&hterms=3G&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3D3G"><span>Present-day <span class="hlt">Antarctic</span> <span class="hlt">ice</span> mass changes and crustal motion</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>James, Thomas S.; Ivins, Erik R.</p> <p>1995-01-01</p> <p>The peak vertical velocities predicted by three realistic, but contrasting, present-day scenarios of <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet mass balance are found to be of the order of several mm/a. One scenario predicts local uplift rates in excess of 5 mm/a. These rates are small compared to the peak <span class="hlt">Antarctic</span> vertical velocities of the <span class="hlt">ICE</span>-3G glacial rebound model, which are in excess of 20 mm/a. If the Holocene <span class="hlt">Antarctic</span> deglaciation history protrayed in <span class="hlt">ICE</span>-3G is realistic, and if regional upper mantle viscosity is not an order of magnitude below 10(exp 21) Pa(dot)s, then a vast geographical region in West Antarctica is uplifting at a rate that could be detected by a future Global Positioning System (GPS) campaign. While present-day scenarios predict small vertical crustal velocities, their overall continent-ocean mass exchange is large enough to account for a substantial portion of the observed secular polar motion (omega m(arrow dot)) and time-varying zonal gravity field.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19990100907&hterms=3G&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3D3G','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19990100907&hterms=3G&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3D3G"><span>Present-day <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Mass Changes and Crustal Motion</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>James, Thomas S.; Ivins, Erik R.</p> <p>1995-01-01</p> <p>The peak vertical velocities predicted by three realistic, but contrasting, present-day scenarios of <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet mass balance are found to be of the order of several mm/a. One scenario predicts local uplift rates in excess of 5 mm/a. These rates are small compared to the peak <span class="hlt">Antarctic</span> vertical velocities of the <span class="hlt">ICE</span>-3G glacial rebound model, which are in excess of 20 mm/a. If the Holocene <span class="hlt">Antarctic</span> deglaciation history portrayed in <span class="hlt">ICE</span>-3G is realistic, and if regional upper mantle viscosity is not an order of magnitude below 10(exp 21) pa s, then a vast geographical region in West Antarctica is uplifting at a rate that could be detected by a future Global Positioning System (GPS) campaign. While present-day scenarios predict small vertical crustal velocities, their overall continent-ocean mass exchange is large enough to account for a substantial portion of the observed secular polar motion ((Omega)m(bar)) and time-varying zonal gravity field J(sub 1).</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_13 --> <div id="page_14" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="261"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70159863','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70159863"><span>Depth, <span class="hlt">ice</span> thickness, and <span class="hlt">ice</span>-out timing cause divergent hydrologic responses among Arctic <span class="hlt">lakes</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>Arp, Christopher D.; Jones, Benjamin M.; Liljedahl, Anna K.; Hinkel, Kenneth M.; Welker, Jeffery A.</p> <p>2015-01-01</p> <p><span class="hlt">Lakes</span> are prevalent in the Arctic and thus play a key role in regional hydrology. Since many Arctic <span class="hlt">lakes</span> are shallow and <span class="hlt">ice</span> grows thick (historically 2-m or greater), seasonal <span class="hlt">ice</span> commonly freezes to the <span class="hlt">lake</span> bed (bedfast <span class="hlt">ice</span>) by winter's end. Bedfast <span class="hlt">ice</span> fundamentally alters <span class="hlt">lake</span> energy balance and melt-out processes compared to deeper <span class="hlt">lakes</span> that exceed the maximum <span class="hlt">ice</span> thickness (floating <span class="hlt">ice</span>) and maintain perennial liquid water below floating <span class="hlt">ice</span>. Our analysis of <span class="hlt">lakes</span> in northern Alaska indicated that <span class="hlt">ice</span>-out of bedfast <span class="hlt">ice</span> <span class="hlt">lakes</span> occurred on average 17 days earlier (22-June) than <span class="hlt">ice</span>-out on adjacent floating <span class="hlt">ice</span> <span class="hlt">lakes</span> (9-July). Earlier <span class="hlt">ice</span>-free conditions in bedfast <span class="hlt">ice</span> <span class="hlt">lakes</span> caused higher open-water evaporation, 28% on average, relative to floating <span class="hlt">ice</span> <span class="hlt">lakes</span> and this divergence increased in <span class="hlt">lakes</span> closer to the coast and in cooler summers. Water isotopes (18O and 2H) indicated similar differences in evaporation between these <span class="hlt">lake</span> types. Our analysis suggests that <span class="hlt">ice</span> regimes created by the combination of <span class="hlt">lake</span> depth relative to <span class="hlt">ice</span> thickness and associated <span class="hlt">ice</span>-out timing currently cause a strong hydrologic divergence among Arctic <span class="hlt">lakes</span>. Thus understanding the distribution and dynamics of <span class="hlt">lakes</span> by <span class="hlt">ice</span> regime is essential for predicting regional hydrology. An observed regime shift in <span class="hlt">lakes</span> to floating <span class="hlt">ice</span> conditions due to thinner <span class="hlt">ice</span> growth may initially offset <span class="hlt">lake</span> drying because of lower evaporative loss from this <span class="hlt">lake</span> type. This potential negative feedback caused by winter processes occurs in spite of an overall projected increase in evapotranspiration as the Arctic climate warms.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16782604','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16782604"><span>Changes in <span class="hlt">ice</span> dynamics and mass balance of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Rignot, Eric</p> <p>2006-07-15</p> <p>The concept that the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet changes with eternal slowness has been challenged by recent observations from satellites. Pronounced regional warming in the <span class="hlt">Antarctic</span> Peninsula triggered <span class="hlt">ice</span> shelf collapse, which led to a 10-fold increase in glacier flow and rapid <span class="hlt">ice</span> sheet retreat. This chain of events illustrated the vulnerability of <span class="hlt">ice</span> shelves to climate warming and their buffering role on the mass balance of Antarctica. In West Antarctica, the Pine Island Bay sector is draining far more <span class="hlt">ice</span> into the ocean than is stored upstream from snow accumulation. This sector could raise sea level by 1m and trigger widespread retreat of <span class="hlt">ice</span> in West Antarctica. Pine Island Glacier accelerated 38% since 1975, and most of the speed up took place over the last decade. Its neighbour Thwaites Glacier is widening up and may double its width when its weakened eastern <span class="hlt">ice</span> shelf breaks up. Widespread acceleration in this sector may be caused by glacier ungrounding from <span class="hlt">ice</span> shelf melting by an ocean that has recently warmed by 0.3 degrees C. In contrast, glaciers buffered from oceanic change by large <span class="hlt">ice</span> shelves have only small contributions to sea level. In East Antarctica, many glaciers are close to a state of mass balance, but sectors grounded well below sea level, such as Cook <span class="hlt">Ice</span> Shelf, Ninnis/Mertz, Frost and Totten glaciers, are thinning and losing mass. Hence, East Antarctica is not immune to changes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70175240','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70175240"><span>Arctic sea <span class="hlt">ice</span> decline contributes to thinning <span class="hlt">lake</span> <span class="hlt">ice</span> trend in northern Alaska</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Alexeev, Vladimir; Arp, Christopher D.; Jones, Benjamin M.; Cai, Lei</p> <p>2016-01-01</p> <p>Field measurements, satellite observations, and models document a thinning trend in seasonal Arctic <span class="hlt">lake</span> <span class="hlt">ice</span> growth, causing a shift from bedfast to floating <span class="hlt">ice</span> conditions. September sea <span class="hlt">ice</span> concentrations in the Arctic Ocean since 1991 correlate well (r = +0.69,p < 0.001) to this <span class="hlt">lake</span> regime shift. To understand how and to what extent sea <span class="hlt">ice</span> affects <span class="hlt">lakes</span>, we conducted model experiments to simulate winters with years of high (1991/92) and low (2007/08) sea <span class="hlt">ice</span> extent for which we also had field measurements and satellite imagery characterizing <span class="hlt">lake</span> <span class="hlt">ice</span> conditions. A <span class="hlt">lake</span> <span class="hlt">ice</span> growth model forced with Weather Research and Forecasting model output produced a 7% decrease in <span class="hlt">lake</span> <span class="hlt">ice</span> growth when 2007/08 sea <span class="hlt">ice</span> was imposed on 1991/92 climatology and a 9% increase in <span class="hlt">lake</span> <span class="hlt">ice</span> growth for the opposing experiment. Here, we clearly link early winter 'ocean-effect' snowfall and warming to reduced <span class="hlt">lake</span> <span class="hlt">ice</span> growth. Future reductions in sea <span class="hlt">ice</span> extent will alter hydrological, biogeochemical, and habitat functioning of Arctic <span class="hlt">lakes</span> and cause sub-<span class="hlt">lake</span> permafrost thaw.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5895444','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5895444"><span>Discovery of a hypersaline subglacial <span class="hlt">lake</span> complex beneath Devon <span class="hlt">Ice</span> Cap, Canadian Arctic</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Blankenship, Donald D.; Schroeder, Dustin M.; Dowdeswell, Julian A.</p> <p>2018-01-01</p> <p>Subglacial <span class="hlt">lakes</span> are unique environments that, despite the extreme dark and cold conditions, have been shown to host microbial life. Many subglacial <span class="hlt">lakes</span> have been discovered beneath the <span class="hlt">ice</span> sheets of Antarctica and Greenland, but no spatially isolated water body has been documented as hypersaline. We use radio-echo sounding measurements to identify two subglacial <span class="hlt">lakes</span> situated in bedrock troughs near the <span class="hlt">ice</span> divide of Devon <span class="hlt">Ice</span> Cap, Canadian Arctic. Modeled basal <span class="hlt">ice</span> temperatures in the <span class="hlt">lake</span> area are no higher than −10.5°C, suggesting that these <span class="hlt">lakes</span> consist of hypersaline water. This implication of hypersalinity is in agreement with the surrounding geology, which indicates that the subglacial <span class="hlt">lakes</span> are situated within an evaporite-rich sediment unit containing a bedded salt sequence, which likely act as the solute source for the brine. Our results reveal the first evidence for subglacial <span class="hlt">lakes</span> in the Canadian Arctic and the first hypersaline subglacial <span class="hlt">lakes</span> reported to date. We conclude that these previously unknown hypersaline subglacial <span class="hlt">lakes</span> may represent significant and largely isolated microbial habitats, and are compelling analogs for potential <span class="hlt">ice-covered</span> brine <span class="hlt">lakes</span> and lenses on planetary bodies across the solar system. PMID:29651462</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002cosp...34E.161A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002cosp...34E.161A"><span>Comparative results of using different methods for discovery of microorganisms in very ancient layers of the Central Antartic Glacier above the <span class="hlt">Lake</span> Vostok</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Abyzov, S.; Hoover, R.; Imura, S.; Mitskevich, I.; Naganuma, T.; Poglazova, M.; Ivanov, M.</p> <p></p> <p>The <span class="hlt">ice</span> sheet of the Central <span class="hlt">Antarctic</span> is considered by world-wide scientific community as a model for elaboration of different methods for search of the life outside of the Earth. This problem became especially significant in connection with discovery the under glacial <span class="hlt">lake</span> in the vicinity of the Russian <span class="hlt">Antarctic</span> Station Vostok. This <span class="hlt">lake</span>, later named "<span class="hlt">Lake</span> Vostok" is considered by many scientists as an analog <span class="hlt">ice</span> <span class="hlt">covered</span> seas of Jupiter's satellite Europa. According to the opinion of many researchers there is great possibility of presence in this <span class="hlt">lake</span> of relict forms of microorganisms well preserved since <span class="hlt">Ice</span> Age period. The investigations through out the thickness of the <span class="hlt">ice</span> sheet above the <span class="hlt">Lake</span> Vostok shows the presence of microorganisms belonging to well-known different taxonomic groups even in the very ancient horizons close to floor of the glacier. Different methods were used for search of microorganisms which were rarely found in the deep ancient layers of the <span class="hlt">ice</span> sheet. The method of aseptic sampling from the <span class="hlt">ice</span> cores and results of control sterile conditions in all stages of conducting of these investigations are described in detail in previous reports. Primary investigations used try usual methods of sowing samples onto the different nutrient media permitted to obtain only a few part of the microorganisms which grow on the media used. The possibility of isolation of obtained organisms for further investigations by using modern methods including DNA-analysis appears to be preferential importance of this method. In the further investigations of the very ancient layers of the <span class="hlt">ice</span> sheet by radioisotopic, luminescence and scanning electron microscopy methods of different modifications, were determined as quantity of microorganisms distributed on its different horizons, as well as the morphological diversity of obtained cells of microorganisms. Experience of many years standing investigations of micro flora in the very ancient strata of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ISPAr42.3.1597S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ISPAr42.3.1597S"><span>The Research on Elevation Change of <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet Based on CRYOSAT-2 Alimeter</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sun, Q.; Wan, J.; Liu, S.; Li, Y.</p> <p>2018-04-01</p> <p>In this paper, the Cryosat-2 altimeter data distributed by the ESA, and these data are processed to extract the information of the elevation change of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet from 2010 to 2017. Firstly, the main pretreatment preprocessing for Cryosat-2 altimetry data is crossover adjustment and elimination of rough difference. Then the grid DEM of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet was constructed by using the kriging interpolation method,and analyzed the spatial characteristic time characteristics of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet. The latitude-weighted elevation can be obtained by using the elevation data of each cycle, and then the general trend of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet elevation variation can be seen roughly.</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> <span class="hlt">ice</span> sheet and implications for <span class="hlt">ice</span>-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> <span class="hlt">ice</span> 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 <span class="hlt">ice</span> 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 <span class="hlt">ice</span> sheet could increase basal melting and thereby trigger <span class="hlt">ice</span> streaming, by providing the water for a lubricating basal layer of till on which <span class="hlt">ice</span> streams are thought to slide4,5. <span class="hlt">Ice</span> streams act to protect the reservoir of slowly moving inland <span class="hlt">ice</span> from exposure to oceanic degradation, thus enhancing <span class="hlt">ice</span>-sheet stability. Here we present aerogeophysical evidence for active volcanism and associated elevated heat flow beneath the WAIS near the critical region where <span class="hlt">ice</span> streaming begins. If this heat flow is indeed controlling <span class="hlt">ice</span>-stream formation, then penetration of ocean waters 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 <span class="hlt">ice</span> streams, and possibly trigger a collapse of the inland <span class="hlt">ice</span> reservoir.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19910004942','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19910004942"><span>Exobiology site selection for future Mars missions: Martian paleolake sediments and terrestrial analogs</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wharton, Robert A., Jr.</p> <p>1989-01-01</p> <p>This research was conducted to establish the scientific framework for the exobiological study of sediments on Mars and to encourage the selection of these sedimentary deposits as sampling sites for future Mars missions. A study was completed on the <span class="hlt">Antarctic</span> Dry Valley <span class="hlt">Lakes</span> (terrestrial analogs of the purported Martian paleolakes) and their sediments that allowed the development of quantitative models relating environmental factors to the nature of the biological community and sediment forming processes. The publications presented include: (1) Diversity of micro-fungi isolated in an <span class="hlt">Antarctic</span> dry valley; (2) <span class="hlt">Lake</span> Hoare, Antarctica--sedimentation through a thick perennial <span class="hlt">ice</span> <span class="hlt">cover</span>; (3) The possibility of life on Mars during a water-rich past; (4) An <span class="hlt">Antarctic</span> research outpost as a model for planetary exploration; (5) Early Martian environments--the <span class="hlt">Antarctic</span> and other terrestrial analogs; (6) Lipophilic pigments from the benthos of a perennially <span class="hlt">ice-covered</span> <span class="hlt">Antarctic</span> <span class="hlt">lake</span>; and (7) Perennially <span class="hlt">ice-covered</span> <span class="hlt">Lake</span> Hoare, Antarctica--physical environment, biology, and sedimentation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017NatCC...7...58L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017NatCC...7...58L"><span>Meltwater produced by wind-albedo interaction stored in an East <span class="hlt">Antarctic</span> <span class="hlt">ice</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>Lenaerts, J. T. M.; Lhermitte, S.; Drews, R.; Ligtenberg, S. R. M.; Berger, S.; Helm, V.; Smeets, C. J. P. P.; Broeke, M. R. Van Den; van de Berg, W. J.; van Meijgaard, E.; Eijkelboom, M.; Eisen, O.; Pattyn, F.</p> <p>2017-01-01</p> <p>Surface melt and subsequent firn air depletion can ultimately lead to disintegration of <span class="hlt">Antarctic</span> <span class="hlt">ice</span> shelves causing grounded glaciers to accelerate and sea level to rise. In the <span class="hlt">Antarctic</span> Peninsula, foehn winds enhance melting near the grounding line, which in the recent past has led to the disintegration of the most northerly <span class="hlt">ice</span> shelves. Here, we provide observational and model evidence that this process also occurs over an East <span class="hlt">Antarctic</span> <span class="hlt">ice</span> shelf, where meltwater-induced firn air depletion is found in the grounding zone. Unlike the <span class="hlt">Antarctic</span> Peninsula, where foehn events originate from episodic interaction of the circumpolar westerlies with the topography, in coastal East Antarctica high temperatures are caused by persistent katabatic winds originating from the <span class="hlt">ice</span> sheet’s interior. Katabatic winds warm and mix the air as it flows downward and cause widespread snow erosion, explaining >3 K higher near-surface temperatures in summer and surface melt doubling in the grounding zone compared with its surroundings. Additionally, these winds expose blue <span class="hlt">ice</span> and firn with lower surface albedo, further enhancing melt. The in situ observation of supraglacial flow and englacial storage of meltwater suggests that <span class="hlt">ice</span>-shelf grounding zones in East Antarctica, like their <span class="hlt">Antarctic</span> Peninsula counterparts, are vulnerable to hydrofracturing.</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 water underneath Wilkes Land, East <span class="hlt">Antarctic</span> <span class="hlt">ice</span> 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 <span class="hlt">lake</span> drainage close to the <span class="hlt">ice</span> divide in Wilkes Land, East Antarctica, and the subsequent cascading of water underneath the <span class="hlt">ice</span> sheet toward the coast. To analyse the event, we combined altimetry data from several sources and subglacial topography. We estimated the total volume of water that drained from <span class="hlt">Lake</span> 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 <span class="hlt">lakes</span> located downstream of CookE2. The total volume of water traveling within the theoretical 500-km-long flow paths computed with the BEDMAP2 data set is similar to the volume that drained from <span class="hlt">Lake</span> CookE2, and our observations suggest that most of the water released from <span class="hlt">Lake</span> CookE2 did not reach the coast but remained trapped underneath the <span class="hlt">ice</span> sheet. Our study illustrates how combining multiple remote sensing techniques allows monitoring of the timing and magnitude of subglacial water flow beneath the East <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFM.U14C..04K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFM.U14C..04K"><span>Subglacial <span class="hlt">Antarctic</span> <span class="hlt">Lake</span> Environment Research in the IPY</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.; Priscu, J. C.</p> <p>2006-12-01</p> <p>Subglacial environments are continental-scale phenomena that occur under thick <span class="hlt">ice</span> sheets. These environments differ in geologic setting, age, evolutionary history, and limnological conditions and may be connected by sub-<span class="hlt">ice</span> hydrologic systems. Evidence suggests that subglacial <span class="hlt">lakes</span> are linked to the onset of <span class="hlt">ice</span> streams influencing the dynamics of overlying <span class="hlt">ice</span> sheets. Outbursts of fresh water from subglacial environments have been invoked as an agent of landscape change in the past and there is speculation that subglacial freshwater discharges have influenced past climate. Subglacial environments rest at the intersection of continental <span class="hlt">ice</span> sheets and the underlying lithosphere. The distribution of subglacial <span class="hlt">lakes</span> is determined by the availability of water and basins for it to collect in. The distribution of water in subglacial environments is related to surface temperature, accumulation rates, <span class="hlt">ice</span> thickness, <span class="hlt">ice</span> velocities, and geothermal flux. The interconnectedness of these environments exerts a fundamental influence on subglacial physical, chemical, and ecological environments; the degree of isolation; and the evolution of life. Subglacial hydrology at a continental-scale must be mapped and modeled to evaluate past drainage events, map subglacial water, and quantify subglacial discharges. The geologic records of past hydrologic events will be reveal the impact of hydrological events on sediment distribution and landscape evolution. Subglacial environments are "natural" earth-bound macrocosms. In some instances these environments trace their origins to more than 35 million years before present when Antarctica became encased in <span class="hlt">ice</span>. As opposed to other habitats on Earth, where solar energy is a primary influence, processes in subglacial environments are mediated by the flow of the overlying <span class="hlt">ice</span> a glacial boundary condition and the flux of heat and possibly fluids from the underlying basin a tectonic control. Recent findings suggest that a third control on</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28135723','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28135723"><span>Vigorous lateral export of the meltwater outflow from beneath an <span class="hlt">Antarctic</span> <span class="hlt">ice</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>Garabato, Alberto C Naveira; Forryan, Alexander; Dutrieux, Pierre; Brannigan, Liam; Biddle, Louise C; Heywood, Karen J; Jenkins, Adrian; Firing, Yvonne L; Kimura, Satoshi</p> <p>2017-02-09</p> <p>The instability and accelerated melting of the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet are among the foremost elements of contemporary global climate change. The increased freshwater output from Antarctica is important in determining sea level rise, the fate of <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> and its effect on the Earth's albedo, ongoing changes in global deep-ocean ventilation, and the evolution of Southern Ocean ecosystems and carbon cycling. A key uncertainty in assessing and predicting the impacts of <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet melting concerns the vertical distribution of the exported meltwater. This is usually represented by climate-scale models as a near-surface freshwater input to the ocean, yet measurements around Antarctica reveal the meltwater to be concentrated at deeper levels. Here we use observations of the turbulent properties of the meltwater outflows from beneath a rapidly melting <span class="hlt">Antarctic</span> <span class="hlt">ice</span> shelf to identify the mechanism responsible for the depth of the meltwater. We show that the initial ascent of the meltwater outflow from the <span class="hlt">ice</span> shelf cavity triggers a centrifugal overturning instability that grows by extracting kinetic energy from the lateral shear of the background oceanic flow. The instability promotes vigorous lateral export, rapid dilution by turbulent mixing, and finally settling of meltwater at depth. We use an idealized ocean circulation model to show that this mechanism is relevant to a broad spectrum of <span class="hlt">Antarctic</span> <span class="hlt">ice</span> shelves. Our findings demonstrate that the mechanism producing meltwater at depth is a dynamically robust feature of <span class="hlt">Antarctic</span> melting that should be incorporated into climate-scale models.</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> <span class="hlt">Ice</span></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 <span class="hlt">Ice</span> 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> <span class="hlt">ice</span> 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> <span class="hlt">ice</span>, selective changes of certain chemical and mineralogical phases has occurred.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C23B1218P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C23B1218P"><span>Simple model of melange and its influence on rapid <span class="hlt">ice</span> retreat in a large-scale <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet model.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pollard, D.; Deconto, R. M.</p> <p>2017-12-01</p> <p>Theory, modeling and observations point to the prospect of runaway grounding-line retreat and marine <span class="hlt">ice</span> loss from West Antarctica and major East <span class="hlt">Antarctic</span> basins, in response to climate warming. These rapid retreats are associated with geologic evidence of past high sea-level stands, and pose a threat of drastic sea-level rise in the future.Rapid calving of <span class="hlt">ice</span> from deep grounding lines generates substantial downstream melange (floating <span class="hlt">ice</span> debris). It is unknown whether this melange has a significant effect on <span class="hlt">ice</span> dynamics during major <span class="hlt">Antarctic</span> retreats, through clogging of seaways and back pressure at the grounding line. Observations in Greenland fjords suggest that melange can have a significant buttressing effect, but the lateral scales of <span class="hlt">Antarctic</span> basins are an order of magnitude larger (100's km compared to 10's km), with presumably much less influence of confining margins.Here we attempt to include melange as a prognostic variable in a 3-DAntarctic <span class="hlt">ice</span> sheet-shelf model. Continuum mechanics is used as aheuristic representation of discrete particle physics. Melange is createdby <span class="hlt">ice</span> calving and cliff failure. Its dynamics are treated similarly to <span class="hlt">ice</span> flow, but with little or no resistance to divergence. Melange providesback pressure where adjacent to grounded tidewater <span class="hlt">ice</span> faces or <span class="hlt">ice</span>-shelf edges. We examine the influence of the new melange component during rapid <span class="hlt">Antarctic</span> retreat in warm-Pliocene and future warming scenarios.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19870027099&hterms=microwaves+water+structure&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dmicrowaves%2Bwater%2Bstructure','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19870027099&hterms=microwaves+water+structure&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dmicrowaves%2Bwater%2Bstructure"><span>Satellite microwave and in situ observations of the Weddell Sea <span class="hlt">ice</span> <span class="hlt">cover</span> and its marginal <span class="hlt">ice</span> zone</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Comiso, J. C.; Sullivan, C. W.</p> <p>1986-01-01</p> <p>The radiative and physical characteristics of the Weddell Sea <span class="hlt">ice</span> <span class="hlt">cover</span> and its marginal <span class="hlt">ice</span> zone are analyzed using multichannel satellite passive microwave data and ship and helicopter observations obtained during the 1983 <span class="hlt">Antarctic</span> Marine Ecosystem Research. Winter and spring brightness temperatures are examined; spatial variability in the brightness temperatures of consolidated <span class="hlt">ice</span> in winter and spring cyclic increases and decrease in brightness temperatures of consolidated <span class="hlt">ice</span> with an amplitude of 50 K at 37 GHz and 20 K at 18 GHz are observed. The roles of variations in air temperature and surface characteristics in the variability of spring brightness temperatures are investigated. <span class="hlt">Ice</span> concentrations are derived using the frequency and polarization techniques, and the data are compared with the helicopter and ship observations. Temporal changes in the <span class="hlt">ice</span> margin structure and the mass balance of fresh water and of biological features of the marginal <span class="hlt">ice</span> zone are studied.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2000E%26PSL.181..529S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2000E%26PSL.181..529S"><span><span class="hlt">Ice</span> formation in subglacial <span class="hlt">Lake</span> Vostok, Central Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Souchez, R.; Petit, J. R.; Tison, J.-L.; Jouzel, J.; Verbeke, V.</p> <p>2000-09-01</p> <p>The investigation of chemical and isotopic properties in the <span class="hlt">lake</span> <span class="hlt">ice</span> from the Vostok <span class="hlt">ice</span> core gives clues to the mechanisms involved in <span class="hlt">ice</span> formation within the <span class="hlt">lake</span>. A small <span class="hlt">lake</span> water salinity can be reasonably deduced from the chemical data. Possible implications for the water circulation of <span class="hlt">Lake</span> Vostok are developed. The characteristics of the isotopic composition of the <span class="hlt">lake</span> <span class="hlt">ice</span> indicate that <span class="hlt">ice</span> formation in <span class="hlt">Lake</span> Vostok occurred by frazil <span class="hlt">ice</span> crystal generation due to supercooling as a consequence of rising waters and a possible contrast in water salinity. Subsequent consolidation of the developed loose <span class="hlt">ice</span> crystals results in the accretion of <span class="hlt">ice</span> to the ceiling of the <span class="hlt">lake</span>.</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> <span class="hlt">Ice</span> 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> <span class="hlt">Ice</span> Sheet stores water equivalent to 58 meters in global sea-level rise. Here we show in simulations with the Parallel <span class="hlt">Ice</span> Sheet Model that burning the currently attainable fossil-fuel resources is sufficient to eliminate the <span class="hlt">ice</span> sheet. With cumulative fossil-fuel emissions of 10 000 GtC, Antarctica is projected to become almost <span class="hlt">ice</span>-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> <span class="hlt">Ice</span> Sheet becomes unstable with 600 to 800 GtC of additional carbon emissions. Beyond this additional carbon release, the destabilization of <span class="hlt">ice</span> 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> <span class="hlt">Ice</span> 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://adsabs.harvard.edu/abs/2017JGRC..122.9548T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.9548T"><span>Biogeochemical Impact of Snow <span class="hlt">Cover</span> and Cyclonic Intrusions on the Winter Weddell Sea <span class="hlt">Ice</span> Pack</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tison, J.-L.; Schwegmann, S.; Dieckmann, G.; Rintala, J.-M.; Meyer, H.; Moreau, S.; Vancoppenolle, M.; Nomura, D.; Engberg, S.; Blomster, L. J.; Hendrickx, S.; Uhlig, C.; Luhtanen, A.-M.; de Jong, J.; Janssens, J.; Carnat, G.; Zhou, J.; Delille, B.</p> <p>2017-12-01</p> <p>Sea <span class="hlt">ice</span> is a dynamic biogeochemical reactor and a double interface actively interacting with both the atmosphere and the ocean. However, proper understanding of its annual impact on exchanges, and therefore potentially on the climate, notably suffer from the paucity of autumnal and winter data sets. Here we present the results of physical and biogeochemical investigations on winter <span class="hlt">Antarctic</span> pack <span class="hlt">ice</span> in the Weddell Sea (R. V. Polarstern AWECS cruise, June-August 2013) which are compared with those from two similar studies conducted in the area in 1986 and 1992. The winter 2013 was characterized by a warm sea <span class="hlt">ice</span> <span class="hlt">cover</span> due to the combined effects of deep snow and frequent warm cyclones events penetrating southward from the open Southern Ocean. These conditions were favorable to high <span class="hlt">ice</span> permeability and cyclic events of brine movements within the sea <span class="hlt">ice</span> <span class="hlt">cover</span> (brine tubes), favoring relatively high chlorophyll-a (Chl-a) concentrations. We discuss the timing of this algal activity showing that arguments can be presented in favor of continued activity during the winter due to the specific physical conditions. Large-scale sea <span class="hlt">ice</span> model simulations also suggest a context of increasingly deep snow, warm <span class="hlt">ice</span>, and large brine fractions across the three observational years, despite the fact that the model is forced with a snowfall climatology. This lends support to the claim that more severe <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> conditions, characterized by a longer <span class="hlt">ice</span> season, thicker, and more concentrated <span class="hlt">ice</span> are sufficient to increase the snow depth and, somehow counterintuitively, to warm the <span class="hlt">ice</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016TCry...10.2721E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016TCry...10.2721E"><span>Estimating the extent of <span class="hlt">Antarctic</span> summer sea <span class="hlt">ice</span> during the Heroic Age of <span class="hlt">Antarctic</span> Exploration</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Edinburgh, Tom; Day, Jonathan J.</p> <p>2016-11-01</p> <p>In stark contrast to the sharp decline in Arctic sea <span class="hlt">ice</span>, there has been a steady increase in <span class="hlt">ice</span> extent around Antarctica during the last three decades, especially in the Weddell and Ross seas. In general, climate models do not to capture this trend and a lack of information about sea <span class="hlt">ice</span> coverage in the pre-satellite period limits our ability to quantify the sensitivity of sea <span class="hlt">ice</span> to climate change and robustly validate climate models. However, evidence of the presence and nature of sea <span class="hlt">ice</span> was often recorded during early <span class="hlt">Antarctic</span> exploration, though these sources have not previously been explored or exploited until now. We have analysed observations of the summer sea <span class="hlt">ice</span> edge from the ship logbooks of explorers such as Robert Falcon Scott, Ernest Shackleton and their contemporaries during the Heroic Age of <span class="hlt">Antarctic</span> Exploration (1897-1917), and in this study we compare these to satellite observations from the period 1989-2014, offering insight into the <span class="hlt">ice</span> conditions of this period, from direct observations, for the first time. This comparison shows that the summer sea <span class="hlt">ice</span> edge was between 1.0 and 1.7° further north in the Weddell Sea during this period but that <span class="hlt">ice</span> conditions were surprisingly comparable to the present day in other sectors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20170005812&hterms=sea&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dsea','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20170005812&hterms=sea&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dsea"><span>Bellingshausen Sea <span class="hlt">Ice</span> Extent Recorded in an <span class="hlt">Antarctic</span> Peninsula <span class="hlt">Ice</span> Core</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Porter, Stacy E.; Parkinson, Claire L.; Mosley-Thompson, Ellen</p> <p>2016-01-01</p> <p>Annual net accumulation (A(sub n)) from the Bruce Plateau (BP) <span class="hlt">ice</span> core retrieved from the <span class="hlt">Antarctic</span> Peninsula exhibits a notable relationship with sea <span class="hlt">ice</span> extent (SIE) in the Bellingshausen Sea. Over the satellite era, both BP A(sub n) and Bellingshausen SIE are influenced by large-scale climatic factors such as the Amundsen Sea Low, Southern Annular Mode, and Southern Oscillation. In addition to the direct response of BP A(sub n) to Bellingshausen SIE (e.g., more open water as a moisture source), these large-scale climate phenomena also link the BP and the Bellingshausen Sea indirectly such that they exhibit similar responses (e.g., northerly wind anomalies advect warm, moist air to the <span class="hlt">Antarctic</span> Peninsula and neighboring Bellingshausen Sea, which reduces SIE and increases A(sub n)). Comparison with a time series of fast <span class="hlt">ice</span> at South Orkney Islands reveals a relationship between BP A(sub n) and sea <span class="hlt">ice</span> in the northern Weddell Sea that is relatively consistent over the twentieth century, except when it is modulated by atmospheric wave patterns described by the Trans-Polar Index. The trend of increasing accumulation on the Bruce Plateau since approximately 1970 agrees with other climate records and reconstructions in the region and suggests that the current rate of sea <span class="hlt">ice</span> loss in the Bellingshausen Sea is unrivaled in the twentieth century.</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('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> <span class="hlt">Ice</span> 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> <span class="hlt">Ice</span> Sheet stores water equivalent to 58 m in global sea-level rise. We show in simulations using the Parallel <span class="hlt">Ice</span> Sheet Model that burning the currently attainable fossil fuel resources is sufficient to eliminate the <span class="hlt">ice</span> sheet. With cumulative fossil fuel emissions of 10,000 gigatonnes of carbon (GtC), Antarctica is projected to become almost <span class="hlt">ice</span>-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> <span class="hlt">Ice</span> Sheet becomes unstable with 600 to 800 GtC of additional carbon emissions. Beyond this additional carbon release, the destabilization of <span class="hlt">ice</span> 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> <span class="hlt">Ice</span> Sheet in its entirety with associated sea-level rise that far exceeds that of all other possible sources. PMID:26601273</p> </li> <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> <span class="hlt">Ice</span> 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> <span class="hlt">Ice</span> Sheet stores water equivalent to 58 m in global sea-level rise. We show in simulations using the Parallel <span class="hlt">Ice</span> Sheet Model that burning the currently attainable fossil fuel resources is sufficient to eliminate the <span class="hlt">ice</span> sheet. With cumulative fossil fuel emissions of 10,000 gigatonnes of carbon (GtC), Antarctica is projected to become almost <span class="hlt">ice</span>-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> <span class="hlt">Ice</span> Sheet becomes unstable with 600 to 800 GtC of additional carbon emissions. Beyond this additional carbon release, the destabilization of <span class="hlt">ice</span> 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> <span class="hlt">Ice</span> 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://adsabs.harvard.edu/abs/2017AGUFM.C33B1190R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C33B1190R"><span>Atmospheric Influences on the Anomalous 2016 <span class="hlt">Antarctic</span> Sea <span class="hlt">Ice</span> Decay</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Raphael, M. N.; Schlosser, E.; Haumann, A.</p> <p>2017-12-01</p> <p>Over the past three decades, a small but significant increase in sea <span class="hlt">ice</span> extent (SIE) has been observed in the <span class="hlt">Antarctic</span>. However, in 2016 there was a surprisingly early onset of the melt season. The maximum <span class="hlt">Antarctic</span> SIE was reached in August rather than end of September, and was followed by a rapid decrease. The decline of the sea <span class="hlt">ice</span> area (SIA) started even earlier, in July. The retreat of the <span class="hlt">ice</span> was particularly large in November where <span class="hlt">Antarctic</span> SIE exhibited a negative anomaly (compared to the 1981-2010 average) of almost 2 Mio. km2, which, combined with reduced Arctic SIE, led to a distinct minimum in global SIE. And, satellite observations show that from November 2016 to February 2017, the daily <span class="hlt">Antarctic</span> SIE has been at record low levels. We use sea level pressure and geopotential height data from the ECMWF- Interim reanalysis, in conjunction with sea <span class="hlt">ice</span> data obtained from the National Snow and <span class="hlt">Ice</span> Data Centre (NSIDC), to investigate possible atmospheric influences on the observed phenomena. Indications are that both the onset of the melt in July and the rapid decrease in SIA and SIE in November were triggered by atmospheric flow patterns related to a positive Zonal Wave 3 index, i.e. synoptic situations leading to strong meridional flow. Additionally the Southern Annular Mode (SAM) index reached its second lowest November value since the beginning of the satellite observations. It is likely that the SIE decrease was preconditioned by SIA decrease. Positive feedback effects led to accelerated melt and consequently to the extraordinary low November SIE.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C54A..08S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C54A..08S"><span>Tropical pacing of <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> increase</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schneider, D. P.</p> <p>2015-12-01</p> <p>One reason why coupled climate model simulations generally do not reproduce the observed increase in <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> extent may be that their internally generated climate variability does not sync with the observed phases of phenomena like the Pacific Decadal Oscillation (PDO) and ENSO. For example, it is unlikely for a free-running coupled model simulation to capture the shift of the PDO from its positive to negative phase during 1998, and the subsequent ~15 year duration of the negative PDO phase. In previously presented work based on atmospheric models forced by observed tropical SSTs and stratospheric ozone, we demonstrated that tropical variability is key to explaining the wind trends over the Southern Ocean during the past ~35 years, particularly in the Ross, Amundsen and Bellingshausen Seas, the regions of the largest trends in sea <span class="hlt">ice</span> extent and <span class="hlt">ice</span> season duration. Here, we extend this idea to coupled model simulations with the Community Earth System Model (CESM) in which the evolution of SST anomalies in the central and eastern tropical Pacific is constrained to match the observations. This ensemble of 10 "tropical pacemaker" simulations shows a more realistic evolution of <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> anomalies than does its unconstrained counterpart, the CESM Large Ensemble (both sets of runs include stratospheric ozone depletion and other time-dependent radiative forcings). In particular, the pacemaker runs show that increased sea <span class="hlt">ice</span> in the eastern Ross Sea is associated with a deeper Amundsen Sea Low (ASL) and stronger westerlies over the south Pacific. These circulation patterns in turn are linked with the negative phase of the PDO, characterized by negative SST anomalies in the central and eastern Pacific. The timing of tropical decadal variability with respect to ozone depletion further suggests a strong role for tropical variability in the recent acceleration of the <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> trend, as ozone depletion stabilized by late 1990s, prior to the most</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.U43A..01R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.U43A..01R"><span>Exploration of Subglacial <span class="hlt">Lake</span> Ellsworth</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ross, N.</p> <p>2012-12-01</p> <p><span class="hlt">Antarctic</span> subglacial <span class="hlt">lakes</span> are thought to be extreme habitats for microbial life and may contain important records of <span class="hlt">ice</span> sheet history within their <span class="hlt">lake</span>-floor sediments. To find if this is true, and to answer the science questions that would follow, direct measurement and sampling of these environments is required. Ever since the water depth of Vostok Subglacial <span class="hlt">Lake</span> in East Antarctica was shown to be >500 m, attention has been given to how these unique, ancient and pristine subglacial environments may be entered without contamination and adverse disturbance. Several organizations have offered guidelines on the desirable cleanliness and sterility requirements for direct sampling experiments, including the US National Academy of Sciences and the Scientific Committee on <span class="hlt">Antarctic</span> Research. The aims, design and implementation of subglacial <span class="hlt">lake</span> access experiments have direct relevance for the exploration of extra-terrestrial <span class="hlt">ice-covered</span> bodies (e.g. Europa) and the search for microbial life elsewhere in the Solar System. This presentation summarizes the scientific protocols and methods being developed for the exploration of Ellsworth Subglacial <span class="hlt">Lake</span> in West Antarctica, and provides an up-to-date summary of the status of the project. The proposed exploration, planned for December 2012, involves accessing the <span class="hlt">lake</span> using a hot-water drill and deploying a sampling probe and sediment corer to allow in situ measurement and sample collection. Details are presented on how this can be undertaken with minimal environmental impact that maximizes scientific return without compromising the environment for future experiments. The implications of this experiment for the search for extra-terrestrial life will be discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018TCry...12...49L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018TCry...12...49L"><span>Modelling present-day basal melt rates for <span class="hlt">Antarctic</span> <span class="hlt">ice</span> shelves using a parametrization of buoyant meltwater plumes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lazeroms, Werner M. J.; Jenkins, Adrian; Hilmar Gudmundsson, G.; van de Wal, Roderik S. W.</p> <p>2018-01-01</p> <p>Basal melting below <span class="hlt">ice</span> shelves is a major factor in mass loss from the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet, which can contribute significantly to possible future sea-level rise. Therefore, it is important to have an adequate description of the basal melt rates for use in <span class="hlt">ice</span>-dynamical models. Most current <span class="hlt">ice</span> models use rather simple parametrizations based on the local balance of heat between <span class="hlt">ice</span> and ocean. In this work, however, we use a recently derived parametrization of the melt rates based on a buoyant meltwater plume travelling upward beneath an <span class="hlt">ice</span> shelf. This plume parametrization combines a non-linear ocean temperature sensitivity with an inherent geometry dependence, which is mainly described by the grounding-line depth and the local slope of the <span class="hlt">ice</span>-shelf base. For the first time, this type of parametrization is evaluated on a two-dimensional grid <span class="hlt">covering</span> the entire <span class="hlt">Antarctic</span> continent. In order to apply the essentially one-dimensional parametrization to realistic <span class="hlt">ice</span>-shelf geometries, we present an algorithm that determines effective values for the grounding-line depth and basal slope in any point beneath an <span class="hlt">ice</span> shelf. Furthermore, since detailed knowledge of temperatures and circulation patterns in the <span class="hlt">ice</span>-shelf cavities is sparse or absent, we construct an effective ocean temperature field from observational data with the purpose of matching (area-averaged) melt rates from the model with observed present-day melt rates. Our results qualitatively replicate large-scale observed features in basal melt rates around Antarctica, not only in terms of average values, but also in terms of the spatial pattern, with high melt rates typically occurring near the grounding line. The plume parametrization and the effective temperature field presented here are therefore promising tools for future simulations of the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet requiring a more realistic oceanic forcing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19158794','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19158794"><span>Warming of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span>-sheet surface since the 1957 International Geophysical Year.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Steig, Eric J; Schneider, David P; Rutherford, Scott D; Mann, Michael E; Comiso, Josefino C; Shindell, Drew T</p> <p>2009-01-22</p> <p>Assessments of <span class="hlt">Antarctic</span> temperature change have emphasized the contrast between strong warming of the <span class="hlt">Antarctic</span> Peninsula and slight cooling of the <span class="hlt">Antarctic</span> continental interior in recent decades. This pattern of temperature change has been attributed to the increased strength of the circumpolar westerlies, largely in response to changes in stratospheric ozone. This picture, however, is substantially incomplete owing to the sparseness and short duration of the observations. Here we show that significant warming extends well beyond the <span class="hlt">Antarctic</span> Peninsula to <span class="hlt">cover</span> most of West Antarctica, an area of warming much larger than previously reported. West <span class="hlt">Antarctic</span> warming exceeds 0.1 degrees C per decade over the past 50 years, and is strongest in winter and spring. Although this is partly offset by autumn cooling in East Antarctica, the continent-wide average near-surface temperature trend is positive. Simulations using a general circulation model reproduce the essential features of the spatial pattern and the long-term trend, and we suggest that neither can be attributed directly to increases in the strength of the westerlies. Instead, regional changes in atmospheric circulation and associated changes in sea surface temperature and sea <span class="hlt">ice</span> are required to explain the enhanced warming in West Antarctica.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.H33F1751Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.H33F1751Z"><span>Remote Sensing of <span class="hlt">Lake</span> <span class="hlt">Ice</span> Phenology in Alaska</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, S.; Pavelsky, T.</p> <p>2017-12-01</p> <p><span class="hlt">Lake</span> <span class="hlt">ice</span> phenology (e.g. <span class="hlt">ice</span> break-up and freeze-up timing) in Alaska is potentially sensitive to climate change. However, there are few current <span class="hlt">lake</span> <span class="hlt">ice</span> records in this region, which hinders the comprehensive understanding of interactions between climate change and <span class="hlt">lake</span> processes. To provide a <span class="hlt">lake</span> <span class="hlt">ice</span> database with over a comparatively long time period (2000 - 2017) and large spatial coverage (4000+ <span class="hlt">lakes</span>) in Alaska, we have developed an algorithm to detect the timing of <span class="hlt">lake</span> <span class="hlt">ice</span> using Moderate Resolution Imaging Spectroradiometer (MODIS) satellite data. This approach generally consists of three major steps. First, we use a cloud mask (MOD09GA) to filter out satellite images with heavy cloud contamination. Second, daily MODIS reflectance values (MOD09GQ) of <span class="hlt">lake</span> surface are used to extract <span class="hlt">ice</span> pixels from water pixels. The <span class="hlt">ice</span> status of <span class="hlt">lakes</span> can be further identified based on the fraction of <span class="hlt">ice</span> pixels. Third, to improve the accuracy of <span class="hlt">ice</span> phenology detection, we execute post-processing quality control to reduce false <span class="hlt">ice</span> events caused by outliers. We validate the proposed algorithm over six <span class="hlt">lakes</span> by comparing with Landsat-based reference data. Validation results indicate a high correlation between the MODIS results and reference data, with normalized root mean square error (NRMSE) ranging from 1.7% to 4.6%. The time series of this <span class="hlt">lake</span> <span class="hlt">ice</span> product is then examined to analyze the spatial and temporal patterns of <span class="hlt">lake</span> <span class="hlt">ice</span> phenology.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/18804261','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/18804261"><span>SPME-GCMS study of the natural attenuation of aviation diesel spilled on the perennial <span class="hlt">ice</span> <span class="hlt">cover</span> of <span class="hlt">Lake</span> Fryxell, Antarctica.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Jaraula, Caroline M B; Kenig, Fabien; Doran, Peter T; Priscu, John C; Welch, Kathleen A</p> <p>2008-12-15</p> <p>In January 2003, a helicopter crashed on the 5 m thick perennial <span class="hlt">ice</span> <span class="hlt">cover</span> of <span class="hlt">Lake</span> Fryxell (McMurdo Dry Valleys, East Antarctica), spilling approximately 730 l of aviation diesel fuel (JP5-AN8 mixture). The molecular composition of the initial fuel was analyzed by solid phase microextraction (SPME) gas chromatography-mass spectrometry (GC-MS), then compared to the composition of the contaminated <span class="hlt">ice</span>, water, and sediments collected a year after the spill. Evaporation is the major agent of diesel weathering in meltpool waters and in the <span class="hlt">ice</span>. This process is facilitated by the light non-aqueous phase liquid properties of the aviation diesel and by the net upward movement of the <span class="hlt">ice</span> as a result of ablation. In contrast, in sediment-bearing <span class="hlt">ice</span>, biodegradation by both alkane- and aromatic-degraders was the prominent attenuation mechanism. The composition of the diesel contaminant in the <span class="hlt">ice</span> was also affected by the differential solubility of its constituents, some <span class="hlt">ice</span> containing water-washed diesel and some <span class="hlt">ice</span> containing exclusively relatively soluble low molecular weight aromatic hydrocarbons such as alkylbenzene and naphthalene homologues. The extent of evaporation, water washing and biodegradation between sites and at different depths in the <span class="hlt">ice</span> are evaluated on the basis of molecular ratios and the results of JP5-AN8 diesel evaporation experiment at 4 degrees C. Immediate spread of the aviation diesel was enhanced where the presence of aeolian sediments induced formations of meltpools. However, in absence of melt pools, slow spreading of the diesel is possible through the porous <span class="hlt">ice</span> and the <span class="hlt">ice</span> <span class="hlt">cover</span> aquifer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27487093','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27487093"><span>A model assessment of the ability of <span class="hlt">lake</span> water in Terra Nova Bay, Antarctica, to induce the photochemical degradation of emerging contaminants.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Minella, Marco; Maurino, Valter; Minero, Claudio; Vione, Davide</p> <p>2016-11-01</p> <p>The shallow <span class="hlt">lakes</span> located in Terra Nova Bay, Antarctica, are free from <span class="hlt">ice</span> for only up to a couple of months (mid December to early/mid February) during the austral summer. In the rest of the year, the <span class="hlt">ice</span> <span class="hlt">cover</span> shields the light and inhibits the photochemical processes in the water columns. Previous work has shown that chromophoric dissolved organic matter (CDOM) in these <span class="hlt">lakes</span> is very reactive photochemically. A model assessment is here provided of <span class="hlt">lake</span>-water photoreactivity in field conditions, based on experimental data of <span class="hlt">lake</span> water absorption spectra, chemistry and photochemistry obtained previously, taking into account the water depth and the irradiation conditions of the <span class="hlt">Antarctic</span> summer. The chosen sample contaminants were the solar filter benzophenone-3 and the antimicrobial agent triclosan, which have very well known photoreactivity and have been found in a variety of environmental matrices in the <span class="hlt">Antarctic</span> continent. The two compounds would have a half-life time of just a few days or less in the <span class="hlt">lake</span> water during the <span class="hlt">Antarctic</span> summertime, largely due to reaction with CDOM triplet states ((3)CDOM*). In general, pollutants that occur in the <span class="hlt">ice</span> and could be released to <span class="hlt">lake</span> water upon <span class="hlt">ice</span> melting (around or soon after the December solstice) would be quickly photodegraded if they undergo fast reaction with (3)CDOM*. With some compounds, the important (3)CDOM* reactions might favour the production of harmful secondary pollutants, such as 2,8-dichlorodibenzodioxin from the basic (anionic) form of triclosan. Copyright © 2016 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016ISPAr41B8..481B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016ISPAr41B8..481B"><span>Mass Balance Changes and <span class="hlt">Ice</span> Dynamics of Greenland and <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheets from Laser Altimetry</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Babonis, G. S.; Csatho, B.; Schenk, T.</p> <p>2016-06-01</p> <p>During the past few decades the Greenland and <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheets have lost <span class="hlt">ice</span> at accelerating rates, caused by increasing surface temperature. The melting of the two big <span class="hlt">ice</span> sheets has a big impact on global sea level rise. If the <span class="hlt">ice</span> sheets would melt down entirely, the sea level would rise more than 60 m. Even a much smaller rise would cause dramatic damage along coastal regions. In this paper we report about a major upgrade of surface elevation changes derived from laser altimetry data, acquired by NASA's <span class="hlt">Ice</span>, Cloud and land Elevation Satellite mission (ICESat) and airborne laser campaigns, such as Airborne Topographic Mapper (ATM) and Land, Vegetation and <span class="hlt">Ice</span> Sensor (LVIS). For detecting changes in <span class="hlt">ice</span> sheet elevations we have developed the Surface Elevation Reconstruction And Change detection (SERAC) method. It computes elevation changes of small surface patches by keeping the surface shape constant and considering the absolute values as surface elevations. We report about important upgrades of earlier results, for example the inclusion of local <span class="hlt">ice</span> caps and the temporal extension from 1993 to 2014 for the Greenland <span class="hlt">Ice</span> Sheet and for a comprehensive reconstruction of <span class="hlt">ice</span> thickness and mass changes for the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26394097','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26394097"><span><span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> losses drive gains in benthic carbon drawdown.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Barnes, D K A</p> <p>2015-09-21</p> <p>Climate forcing of sea-<span class="hlt">ice</span> losses from the Arctic and West <span class="hlt">Antarctic</span> are blueing the poles. These losses are accelerating, reducing Earth's albedo and increasing heat absorption. Subarctic forest (area expansion and increased growth) and <span class="hlt">ice</span>-shelf losses (resulting in new phytoplankton blooms which are eaten by benthos) are the only significant described negative feedbacks acting to counteract the effects of increasing CO2 on a warming planet, together accounting for uptake of ∼10(7) tonnes of carbon per year. Most sea-<span class="hlt">ice</span> loss to date has occurred over polar continental shelves, which are richly, but patchily, colonised by benthic animals. Most polar benthos feeds on microscopic algae (phytoplankton), which has shown increased blooms coincident with sea-<span class="hlt">ice</span> losses. Here, growth responses of <span class="hlt">Antarctic</span> shelf benthos to sea-<span class="hlt">ice</span> losses and phytoplankton increases were investigated. Analysis of two decades of benthic collections showed strong increases in annual production of shelf seabed carbon in West <span class="hlt">Antarctic</span> bryozoans. These were calculated to have nearly doubled to >2x10(5) tonnes of carbon per year since the 1980s. Annual production of bryozoans is median within wider <span class="hlt">Antarctic</span> benthos, so upscaling to include other benthos (combined study species typically constitute ∼3% benthic biomass) suggests an increased drawdown of ∼2.9x10(6) tonnes of carbon per year. This drawdown could become sequestration because polar continental shelves are typically deeper than most modern iceberg scouring, bacterial breakdown rates are slow, and benthos is easily buried. To date, most sea-<span class="hlt">ice</span> losses have been Arctic, so, if hyperboreal benthos shows a similar increase in drawdown, polar continental shelves would represent Earth's largest negative feedback to climate change. Copyright © 2015 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C41C0676G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C41C0676G"><span>A Comparison of the Seasonal Change of Albedo across Glaciers and <span class="hlt">Ice-Covered</span> <span class="hlt">Lakes</span> of the Taylor Valley, Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gooseff, M. N.; Bergstrom, A.</p> <p>2016-12-01</p> <p>The Dry Valleys of Antarctica are a polar desert ecosystem consisting of piedmont and alpine glaciers, <span class="hlt">ice-covered</span> <span class="hlt">lakes</span>, and vast expanses of bare soil. The ecosystem is highly dependent on glacial melt a water source. Because average summer temperatures are close to freezing, glacier <span class="hlt">ice</span> and <span class="hlt">lake</span> <span class="hlt">ice</span> are very closely linked to the energy balance. A slight increase in incoming radiation or decrease in albedo can have large effects on the timing and volume of available liquid water. However, we have yet to fully characterize the seasonal evolution of albedo in the valleys. In this study, we used a camera, gps, and short wave radiometer to characterize the albedo within and across landscape types in the Taylor Valley. These instruments were attached to a helicopter and flown on a prescribed path along the valley at approximately 300 feet above the ground surface five different times throughout the season from mid-November to mid-January, 2015-2016. We used these data to calculate the albedo of each glacier, <span class="hlt">lake</span>, and the soil surface of the <span class="hlt">lake</span> basins in the valley for each flight. As expected, we found that all landscape types had significantly different albedo, with the glaciers consistently the highest throughout the season and the bare soils the lowest (p-value < 0.05). We hypothesized that albedo would decrease throughout the season with snow melt and increasing sediment exposure on the glacier and <span class="hlt">lake</span> surfaces. However, small snow events (< 3 cm) caused somewhat persistent high albedo on the <span class="hlt">lakes</span> and glaciers. Furthermore, there was a range in albedo across glaciers and each responded to seasonal snow and melt differently. These findings highlight the importance of understanding the spatial and temporal variability in albedo and the close coupling of climate and landscape response. We can use this new understanding of landscape albedo to better predict how the Dry Valley ecosystems will respond to changing climate at the basin scale.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A21Q..08F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A21Q..08F"><span>Response of <span class="hlt">Antarctic</span> sea surface temperature and sea <span class="hlt">ice</span> to ozone depletion</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ferreira, D.; Gnanadesikan, A.; Kostov, Y.; Marshall, J.; Seviour, W.; Waugh, D.</p> <p>2017-12-01</p> <p>The influence of the <span class="hlt">Antarctic</span> ozone hole extends all the way from the stratosphere through the troposphere down to the surface, with clear signatures on surface winds, and SST during summer. In this talk we discuss the impact of these changes on the ocean circulation and sea <span class="hlt">ice</span> state. We are notably motivated by the observed cooling of the surface Southern Ocean and associated increase in <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> extent since the 1970s. These trends are not reproduced by CMIP5 climate models, and the underlying mechanism at work in nature and the models remain unexplained. Did the ozone hole contribute to the observed trends?Here, we review recent advances toward answering these issues using "abrupt ozone depletion" experiments. The ocean and sea <span class="hlt">ice</span> response is rather complex, comprising two timescales: a fast ( 1-2y) cooling of the surface ocean and sea <span class="hlt">ice</span> <span class="hlt">cover</span> increase, followed by a slower warming trend, which, depending on models, flip the sign of the SST and sea <span class="hlt">ice</span> responses on decadal timescale. Although the basic mechanism seems robust, comparison across climate models reveal large uncertainties in the timescales and amplitude of the response to the extent that even the sign of the ocean and sea <span class="hlt">ice</span> response to ozone hole and recovery remains unconstrained. After briefly describing the dynamics and thermodynamics behind the two-timescale response, we will discuss the main sources of uncertainties in the modeled response, namely cloud effects and air-sea heat exchanges, surface wind stress response and ocean eddy transports. Finally, we will consider the implications of our results on the ability of coupled climate models to reproduce observed Southern Ocean changes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4060491','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4060491"><span>Cyclone-induced rapid creation of extreme <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> conditions</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Wang, Zhaomin; Turner, John; Sun, Bo; Li, Bingrui; Liu, Chengyan</p> <p>2014-01-01</p> <p>Two polar vessels, Akademik Shokalskiy and Xuelong, were trapped by thick sea <span class="hlt">ice</span> in the <span class="hlt">Antarctic</span> coastal region just to the west of 144°E and between 66.5°S and 67°S in late December 2013. This event demonstrated the rapid establishment of extreme <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> conditions on synoptic time scales. The event was associated with cyclones that developed at lower latitudes. Near the event site, cyclone-enhanced strong southeasterly katabatic winds drove large westward drifts of <span class="hlt">ice</span> floes. In addition, the cyclones also gave southward <span class="hlt">ice</span> drift. The arrival and grounding of Iceberg B9B in Commonwealth Bay in March 2011 led to the growth of fast <span class="hlt">ice</span> around it, forming a northward protruding barrier. This barrier blocked the westward <span class="hlt">ice</span> drift and hence aided sea <span class="hlt">ice</span> consolidation on its eastern side. Similar cyclone-induced events have occurred at this site in the past after the grounding of Iceberg B9B. Future events may be predictable on synoptic time scales, if cyclone-induced strong wind events can be predicted. PMID:24937550</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C33B1185F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C33B1185F"><span>The role of feedbacks in <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> change</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Feltham, D. L.; Frew, R. C.; Holland, P.</p> <p>2017-12-01</p> <p>The changes in <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> over the last thirty years have a strong seasonal dependence, and the way these changes grow in spring and decay in autumn suggests that feedbacks are strongly involved. The changes may ultimately be caused by atmospheric warming, the winds, snowfall changes, etc., but we cannot understand these forcings without first untangling the feedbacks. A highly simplified coupled sea <span class="hlt">ice</span> -mixed layer model has been developed to investigate the importance of feedbacks on the evolution of sea <span class="hlt">ice</span> in two contrasting regions in the Southern Ocean; the Amundsen Sea where sea <span class="hlt">ice</span> extent has been decreasing, and the Weddell Sea where it has been expanding. The change in mixed layer depth in response to changes in the atmosphere to ocean energy flux is implicit in a strong negative feedback on <span class="hlt">ice</span> <span class="hlt">cover</span> changes in the Amundsen Sea, with atmospheric cooling leading to a deeper mixed layer resulting in greater entrainment of warm Circumpolar Deep Water, causing increased basal melting of sea <span class="hlt">ice</span>. This strong negative feedback produces counter intuitive responses to changes in forcings in the Amundsen Sea. This feedback is absent in the Weddell due to the complete destratification and strong water column cooling that occurs each winter in simulations. The impact of other feedbacks, including the albedo feedback, changes in insulation due to <span class="hlt">ice</span> thickness and changes in the freezing temperature of the mixed layer, were found to be of secondary importance compared to changes in the mixed layer depth.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014ESD.....5..271L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014ESD.....5..271L"><span>Projecting <span class="hlt">Antarctic</span> <span class="hlt">ice</span> discharge using response functions from SeaRISE <span class="hlt">ice</span>-sheet models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Levermann, A.; Winkelmann, R.; Nowicki, S.; Fastook, J. L.; Frieler, K.; Greve, R.; Hellmer, H. H.; Martin, M. A.; Meinshausen, M.; Mengel, M.; Payne, A. J.; Pollard, D.; Sato, T.; Timmermann, R.; Wang, W. L.; Bindschadler, R. A.</p> <p>2014-08-01</p> <p>The largest uncertainty in projections of future sea-level change results from the potentially changing dynamical <span class="hlt">ice</span> discharge from Antarctica. Basal <span class="hlt">ice</span>-shelf melting induced by a warming ocean has been identified as a major cause for additional <span class="hlt">ice</span> flow across the grounding line. Here we attempt to estimate the uncertainty range of future <span class="hlt">ice</span> discharge from Antarctica by combining uncertainty in the climatic forcing, the oceanic response and the <span class="hlt">ice</span>-sheet model response. The uncertainty in the global mean temperature increase is obtained from historically constrained emulations with the MAGICC-6.0 (Model for the Assessment of Greenhouse gas Induced Climate Change) model. The oceanic forcing is derived from scaling of the subsurface with the atmospheric warming from 19 comprehensive climate models of the Coupled Model Intercomparison Project (CMIP-5) and two ocean models from the EU-project <span class="hlt">Ice</span>2Sea. The dynamic <span class="hlt">ice</span>-sheet response is derived from linear response functions for basal <span class="hlt">ice</span>-shelf melting for four different <span class="hlt">Antarctic</span> drainage regions using experiments from the Sea-level Response to <span class="hlt">Ice</span> Sheet Evolution (SeaRISE) intercomparison project with five different <span class="hlt">Antarctic</span> <span class="hlt">ice</span>-sheet models. The resulting uncertainty range for the historic <span class="hlt">Antarctic</span> contribution to global sea-level rise from 1992 to 2011 agrees with the observed contribution for this period if we use the three <span class="hlt">ice</span>-sheet models with an explicit representation of <span class="hlt">ice</span>-shelf dynamics and account for the time-delayed warming of the oceanic subsurface compared to the surface air temperature. The median of the additional <span class="hlt">ice</span> loss for the 21st century is computed to 0.07 m (66% range: 0.02-0.14 m; 90% range: 0.0-0.23 m) of global sea-level equivalent for the low-emission RCP-2.6 (Representative Concentration Pathway) scenario and 0.09 m (66% range: 0.04-0.21 m; 90% range: 0.01-0.37 m) for the strongest RCP-8.5. Assuming no time delay between the atmospheric warming and the oceanic subsurface, these</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018QSRv..179..153S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018QSRv..179..153S"><span>Dating <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet collapse: Proposing a molecular genetic approach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Strugnell, Jan M.; Pedro, Joel B.; Wilson, Nerida G.</p> <p>2018-01-01</p> <p>Sea levels at the end of this century are projected to be 0.26-0.98 m higher than today. The upper end of this range, and even higher estimates, cannot be ruled out because of major uncertainties in the dynamic response of polar <span class="hlt">ice</span> sheets to a warming climate. Here, we propose an ecological genetics approach that can provide insight into the past stability and configuration of the West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet (WAIS). We propose independent testing of the hypothesis that a trans-<span class="hlt">Antarctic</span> seaway occurred at the last interglacial. Examination of the genomic signatures of bottom-dwelling marine species using the latest methods can provide an independent window into the integrity of the WAIS more than 100,000 years ago. Periods of connectivity facilitated by trans-<span class="hlt">Antarctic</span> seaways could be revealed by dating coalescent events recorded in DNA. These methods allow alternative scenarios to be tested against a fit to genomic data. Ideal candidate taxa for this work would need to possess a circumpolar distribution, a benthic habitat, and some level of genetic structure indicated by phylogeographical investigation. The purpose of this perspective piece is to set out an ecological genetics method to help resolve when the West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Shelf last collapsed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20020050249','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20020050249"><span>Hellas as a Possible Site of Ancient <span class="hlt">Ice-Covered</span> <span class="hlt">Lakes</span> on Mars</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Moore, Jeffrey M.; Wilhelms, Don E.; DeVincenzi, Donald (Technical Monitor)</p> <p>2002-01-01</p> <p>Based on topographic, morphologic, and stratigraphic evidence, we propose that ancient water-laid sediment is the dominant component of deposits within Hellas Planitia, Mars. Multiply layered sediment is manifested by alternating benches and scarps visible in Mars Orbiting Camera narrow-angle (MOC NA) images. Viking Orbiter camera and MOC NA images were used to map contacts and stratigraphically order the different materials units within Hellas. Mar's Orbiting Laser Altimeter (MOLA) data reveal that the contacts of these sedimentary units, as well as a number of scarps or other abrupt changes in landscape texture, trace contours of constant elevation for thousands of km, and in one case all around the basin. Channels, consensually interpreted to be cut by water, lead into the basin. MOLA results indicate that the area encompassed by greater Hellas' highest closed contour is nearly one-fifth that of the entire northern plains, making the Hellas 'drainage' area much larger than previously reported. If <span class="hlt">lakes</span> formed under climatic conditions similar to the modern Martian climate, they would develop thick <span class="hlt">ice</span> carapaces, then the <span class="hlt">lakes</span> would eventually sublimate away. Two units within Hellas exhibit a reticulate or honeycomb pattern we speculate are impressions made by <span class="hlt">lake</span>-lowered <span class="hlt">ice</span> blocks grounding into initially soft mud.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70023375','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70023375"><span>Hellas as a possible site of ancient <span class="hlt">ice-covered</span> <span class="hlt">lakes</span> on Mars</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Moore, Johnnie N.; Wilhelms, D.E.</p> <p>2001-01-01</p> <p>Based on topographic, morphologic, and stratigraphic evidence, we propose that ancient water-laid sediment is the dominant component of deposits within Hellas Planitia, Mars. Multiple-layered sediment is manifested by alternating benches and scarps visible in Mars orbiting camera narrow-angle (MOC NA) images. Viking Orbiter camera and MOC NA images were used to map contacts and stratigraphically order the different materials units within Hellas. Mars orbiting laser altimeter (MOLA) data reveal that the contacts of these sedimentary units, as well as a number of scarps or other abrupt changes in landscape texture, trace contours of constant elevation for thousands of km, and in one case all around the basin. Channels, consensually interpreted to be cut by water, lead into the basin. MOLA results indicate that the area encompassed by greater Hellas' highest closed contour is nearly one-fifth that of the entire northern plains, making the Hellas "drainage" area much larger than previously reported. If <span class="hlt">lakes</span> formed under climatic conditions similar to the modern Martian climate, they would develop thick <span class="hlt">ice</span> carapaces, then the <span class="hlt">lakes</span> would eventually sublimate away. Two units within Hellas exhibit a reticulate or honeycomb pattern, which we speculate are impressions made by <span class="hlt">lake</span>-lowered <span class="hlt">ice</span> blocks grounding into initially soft mud.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_15 --> <div id="page_16" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="301"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20030056665&hterms=Parkinsons&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3DParkinsons','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20030056665&hterms=Parkinsons&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3DParkinsons"><span>30-Year Satellite Record Reveals Accelerated Arctic Sea <span class="hlt">Ice</span> Loss, <span class="hlt">Antarctic</span> Sea <span class="hlt">Ice</span> Trend Reversal</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Cavalieri, Donald J.; Parkinson, C. L.; Vinnikov, K. Y.</p> <p>2003-01-01</p> <p>Arctic sea <span class="hlt">ice</span> extent decreased by 0.30 plus or minus 0.03 x 10(exp 6) square kilometers per decade from 1972 through 2002, but decreased by 0.36 plus or minus 0.05 x 10(exp 6) square kilometers per decade from 1979 through 2002, indicating an acceleration of 20% in the rate of decrease. In contrast to the Arctic, the <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> extent decreased dramatically over the period 1973-1977, then gradually increased, with an overall 30-year trend of -0.15 plus or minus 0.08 x 10(exp 6) square kilometers per 10yr. The trend reversal is attributed to a large positive anomaly in <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> extent observed in the early 1970's.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20100040620','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20100040620"><span>Comparison of the Microbial Diversity and Abundance Between the Freshwater Land-Locked <span class="hlt">Lakes</span> of Schirmacher Oasis and the Perennially <span class="hlt">Ice-Covered</span> <span class="hlt">Lake</span> Untersee in East Antarctica</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Huang, Jonathan; Hoover, Richard B.; Swain, Ashit; Murdock, Chris; Bej, Asim K.</p> <p>2010-01-01</p> <p>Extreme conditions such as low temperature, dryness, and constant UV-radiation in terrestrial Antarctica are limiting factors of the survival of microbial populations. The objective of this study was to investigate the microbial diversity and enumeration between the open water <span class="hlt">lakes</span> of Schirmacher Oasis and the permanently <span class="hlt">ice-covered</span> <span class="hlt">Lake</span> Untersee. The <span class="hlt">lakes</span> in Schirmacher Oasis possessed abundant and diverse group of microorganisms compared to the <span class="hlt">Lake</span> Untersee. Furthermore, the microbial diversity between two <span class="hlt">lakes</span> in Schirmacher Oasis (<span class="hlt">Lake</span> L27C and L47) was compared by culture-based molecular approach. It was determined that L27Chad a richer microbial diversity representing 5 different phyla and 7 different genera. In contrast L47 consisted of 4 different phyla and 6 different genera. The difference in microbial community could be due to the wide range of pH between L27C (pH 9.1) and L47 (pH 5.7). Most of the microbes isolated from these <span class="hlt">lakes</span> consisted of adaptive biological pigmentation. Characterization of the microbial community found in the freshwater <span class="hlt">lakes</span> of East Antarctica is important because it gives a further glimpse into the adaptation and survival strategies found in extreme conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009SPIE.7441E..09S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009SPIE.7441E..09S"><span>Laser induced fluorescence emission (L.I.F.E.): in situ and remote detection of life in <span class="hlt">Antarctic</span> and Alaskan <span class="hlt">ice</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Storrie-Lombardi, Michael C.; Sattler, Birgit</p> <p>2009-08-01</p> <p>Once thought to be a barren desert devoid of life, it now appears that Earth's cryosphere is an <span class="hlt">ice</span> ecosystem harbouring a rich community of metabolically active microorganisms inhabiting <span class="hlt">ice</span>, snow, water, and lithic environments. The ability to rapidly survey this ecosystem during in situ and orbital missions is of considerable interest for monitoring Earth's carbon budget and for efficiently searching for life on Mars or any exoplanet with an analogous cryosphere. Laser induced fluorescence emission (L.I.F.E.) imaging and spectroscopy using excitation in ultraviolet (UV) wavelengths have been proposed as non-destructive astrobiological survey tools to search for amino acids, nucleic acids, microbial life, and polycyclic aromatic hydrocarbons (PAHs) deep in the Mars regolith. However, the technique is easily adapted to search for larger, more complex biomolecular targets using longer wavelength sources. Of particular interest is the ability for excitation at blue, green, and red wavelengths to produce visible and near infrared fluorescence of photosynthetic pigments in cyanobacteria-dominated microbial communities populating the <span class="hlt">ice</span> of alpine, Arctic, and <span class="hlt">Antarctic</span> <span class="hlt">lakes</span>, glaciers, <span class="hlt">ice</span> sheets, and even the supercooled water-<span class="hlt">ice</span> droplets of clouds. During the Tawani 2008 International <span class="hlt">Antarctic</span> Expedition we tested the in situ use of the technique as part of a field campaign in the Dry Valleys of Schirmacher Oasis and <span class="hlt">Lake</span> Untersee, Queen Maud Land, Antarctica. In the spring of 2009, we performed airborne remote sensing tests of the technology in Alaska. In this paper we review our in situ laser detection experiments and present for the first time preliminary results on our efforts to detect cryosphere L.I.F.E. from an airborne platform.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27997388','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27997388"><span>Notable increases in nutrient concentrations in a shallow <span class="hlt">lake</span> during seasonal <span class="hlt">ice</span> growth.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Fang, Yang; Changyou, Li; Leppäranta, Matti; Xiaonghong, Shi; Shengnan, Zhao; Chengfu, Zhang</p> <p>2016-12-01</p> <p>Nutrients may be eliminated from <span class="hlt">ice</span> when liquid water is freezing, resulting in enhanced concentrations in the unfrozen water. The nutrients diluted from the <span class="hlt">ice</span> may contribute to accumulated concentrations in sediment during winter and an increased risk of algae blooms during the following spring and summer. The objective of this study was to evaluate the influence of <span class="hlt">ice</span> <span class="hlt">cover</span> on nitrogen (N) and phosphorus (P) concentrations in the water and sediment of a shallow <span class="hlt">lake</span>, through an examination of Ulansuhai <span class="hlt">Lake</span>, northern China, from the period of open water to <span class="hlt">ice</span> season in 2011-2013. The N and P concentrations were between two and five times higher, and between two and eight times higher, than in unfrozen <span class="hlt">lakes</span>, respectively. As the <span class="hlt">ice</span> thickness grew, contents of total N and total P showed C-shaped profiles in the <span class="hlt">ice</span>, and were lower in the middle layer and higher in the bottom and surface layers. Most of the nutrients were released from the <span class="hlt">ice</span> to liquid water. The results confirm that <span class="hlt">ice</span> can cause the nutrient concentrations in water and sediment during winter to increase dramatically, thereby significantly impacting on processes in the water environment of shallow <span class="hlt">lakes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20020082883','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20020082883"><span><span class="hlt">Ice</span> Shelves and Landfast <span class="hlt">Ice</span> on the <span class="hlt">Antarctic</span> Perimeter: Revised Scope of Work</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Scambos, Ted</p> <p>2002-01-01</p> <p><span class="hlt">Ice</span> shelves respond quickly and profoundly to a warming climate. Within a decade after mean summertime temperature reaches approx. O C and persistent melt pending is observed, a rapid retreat and disintegration occurs. This link was documented for <span class="hlt">ice</span> shelves in the <span class="hlt">Antarctic</span> Peninsula region (the Larsen 'A', 'B' and Wilkins <span class="hlt">Ice</span> shelves) by the results of a previous grant under ADRO-1. Modeling of <span class="hlt">ice</span> flow and the effects of meltwater indicated that melt pending accelerates shelf breakup by increasing fracture penetration. SAR data supplemented an AVHRR- and SSM/I-based image analysis of extent and surface characteristic changes. This funded grant is a revised, scaled-down version of an earlier proposal under the ADRO-2 NRA. The overall objective remains the same: we propose to build on the previous study by examining other <span class="hlt">ice</span> shelves of the <span class="hlt">Antarctic</span> and incorporate an examination of the climate-related characteristics of landfast <span class="hlt">ice</span>. The study now considers just a few shelf and fast <span class="hlt">ice</span> areas for study, and is funded for two years. The study regions are the northeastern Ross <span class="hlt">Ice</span> Shelf, the Larsen 'B' and 'C' shelves, fast <span class="hlt">ice</span> and floating shelf <span class="hlt">ice</span> in the Pine Island Glacier area, and fast <span class="hlt">ice</span> along the Wilkes Land coast. Further, rather than investigating a host of shelf and fast <span class="hlt">ice</span> processes, we will home in on developing a series of characteristics associated with climate change over shelf and fast <span class="hlt">ice</span> areas. Melt pending and break-up are the end stages of a response to a warming climate that may begin with increased melt event frequency (which changes both albedo and emissivity temporarily), changing firn backscatter (due to percolation features), and possibly increased rifting of the shelf surface. Fast <span class="hlt">ice</span> may show some of these same processes on a seasonal timescale, providing insight into shelf evolution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGC53E0944A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC53E0944A"><span>Record low <span class="hlt">lake</span> <span class="hlt">ice</span> thickness and bedfast <span class="hlt">ice</span> extent on Alaska's Arctic Coastal Plain in 2017 exemplify the value of monitoring freshwater <span class="hlt">ice</span> to understand sea-<span class="hlt">ice</span> forcing and predict permafrost dynamics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Arp, C. D.; Alexeev, V. A.; Bondurant, A. C.; Creighton, A.; Engram, M. J.; Jones, B. M.; Parsekian, A.</p> <p>2017-12-01</p> <p>The winter of 2016/2017 was exceptionally warm and snowy along the coast of Arctic Alaska partly due to low fall sea <span class="hlt">ice</span> extent. Based on several decades of field measurements, we documented a new record low maximum <span class="hlt">ice</span> thickness (MIT) for <span class="hlt">lakes</span> on the Barrow Peninsula, averaging 1.2 m. This is in comparison to a long-term average MIT of 1.7 m stretching back to 1962 with a maximum of 2.1 m in 1970 and previous minimum of 1.3 m in 2014. The relevance of thinner <span class="hlt">lake</span> <span class="hlt">ice</span> in arctic coastal lowlands, where thermokarst <span class="hlt">lakes</span> <span class="hlt">cover</span> greater than 20% of the land area, is that permafrost below <span class="hlt">lakes</span> with bedfast <span class="hlt">ice</span> is typically preserved. <span class="hlt">Lakes</span> deeper than the MIT warm and thaw sub-<span class="hlt">lake</span> permafrost forming taliks. Remote sensing analysis using synthetic aperture radar (SAR) is a valuable tool for scaling the field observations of MIT to the entire freshwater landscape to map bedfast <span class="hlt">ice</span>. A new, long-term time-series of late winter multi-platform SAR from 1992 to 2016 shows a large dynamic range of bedfast <span class="hlt">ice</span> extent, 29% of <span class="hlt">lake</span> area or 6% of the total land area over this period, and adding 2017 to this record is expected to extend this range further. Empirical models of <span class="hlt">lake</span> mean annual bed temperature suggest that permafrost begins to thaw at depths less than 60% of MIT. Based on this information and knowledge of average <span class="hlt">lake</span> <span class="hlt">ice</span> growth trajectories, we suggest that future SAR analysis of <span class="hlt">lake</span> <span class="hlt">ice</span> should focus on mid-winter (January) to evaluate the extent of bedfast <span class="hlt">ice</span> and corresponding zones of sub-<span class="hlt">lake</span> permafrost thaw. Tracking changes in these areas from year to year in mid-winter may provide the best landscape-scale evaluation of changing permafrost conditions in <span class="hlt">lake</span>-rich arctic lowlands. Because observed changes in MIT coupled with mid-winter bedfast <span class="hlt">ice</span> extent provide much information on permafrost stability, we suggest that these measurements can serve as Essential Climate Variables (EVCs) to indicate past and future changes in <span class="hlt">lake</span>-rich arctic regions. The</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27780352','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27780352"><span>Seasonal Study of Mercury Species in the <span class="hlt">Antarctic</span> Sea <span class="hlt">Ice</span> Environment.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Nerentorp Mastromonaco, Michelle G; Gårdfeldt, Katarina; Langer, Sarka; Dommergue, Aurélien</p> <p>2016-12-06</p> <p>Limited studies have been conducted on mercury concentrations in the polar cryosphere and the factors affecting the distribution of mercury within sea <span class="hlt">ice</span> and snow are poorly understood. Here we present the first comprehensive seasonal study of elemental and total mercury concentrations in the <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> environment <span class="hlt">covering</span> data from measurements in air, sea <span class="hlt">ice</span>, seawater, snow, frost flowers, and brine. The average concentration of total mercury in sea <span class="hlt">ice</span> decreased from winter (9.7 ng L -1 ) to spring (4.7 ng L -1 ) while the average elemental mercury concentration increased from winter (0.07 ng L -1 ) to summer (0.105 ng L -1 ). The opposite trends suggest potential photo- or dark oxidation/reduction processes within the <span class="hlt">ice</span> and an eventual loss of mercury via brine drainage or gas evasion of elemental mercury. Our results indicate a seasonal variation of mercury species in the polar sea <span class="hlt">ice</span> environment probably due to varying factors such as solar radiation, temperature, brine volume, and atmospheric deposition. This study shows that the sea <span class="hlt">ice</span> environment is a significant interphase between the polar ocean and the atmosphere and should be accounted for when studying how climate change may affect the mercury cycle in polar regions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1616351A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1616351A"><span>Future <span class="hlt">Antarctic</span> bed topography and its implications for <span class="hlt">ice</span> sheet dynamics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Adhikari, Surendra; Ivins, Erik; Larour, Eric; Seroussi, Helene; Morlighem, Mathieu; Nowicki, Sophie</p> <p>2014-05-01</p> <p>A recently improved <span class="hlt">ice</span> loading history suggests that the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet (AIS) has been generally losing its mass since the last glacial maximum. In a sustained warming climate, the AIS is predicted to retreat at a greater pace primarily via melting beneath the <span class="hlt">ice</span> shelves. We employ the glacial isostatic adjustment (GIA) capability of the <span class="hlt">Ice</span> Sheet System Model (ISSM) to combine these past and future <span class="hlt">ice</span> loadings and provide the new solid Earth computations for the AIS. We find that the past loading is relatively less important than future loading on the evolution of the future bed topography. Our computations predict that the West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet (WAIS) may uplift by a few meters and a few tens of meters at years 2100 and 2500 AD, respectively, and that the East <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet (EAIS) is likely to remain unchanged or subside minimally except around the Amery <span class="hlt">Ice</span> Shelf. The Amundsen Sea Sector of WAIS in particular is predicted to rise at the greatest rate; one hundred years of <span class="hlt">ice</span> evolution in this region, for example, predicts that the coastline of Pine Island Bay approaches roughly 45 mm/yr in viscoelastic vertical motion. Of particular importance, we systematically demonstrate that the effect of a pervasive and large GIA uplift in the WAIS is associated with the flattening of reverse bed, reduction of local sea depth, and thus the extension of grounding line (GL) towards the continental shelf. Using the 3-D higher-order <span class="hlt">ice</span> flow capability of ISSM, such a migration of GL is shown to inhibit the <span class="hlt">ice</span> flow. This negative feedback between the <span class="hlt">ice</span> sheet and the solid Earth may promote the stability to marine portions of the <span class="hlt">ice</span> sheet in the future.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFM.C53B..05F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFM.C53B..05F"><span>New Collaborative Aerogeophysical Survey Targets the Stability of the East <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> sheet and its Geological Boundary Conditions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ferraccioli, F.; Corr, H.; Jordan, T.; Bozzo, E.; Armadillo, E.; Caneva, G.; Frearson, N.; Robinson, C.; Smellie, J.</p> <p>2006-12-01</p> <p>At the eve of the IPY large aerogeophysical survey data gaps still remain over the East <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet (EAIS). This is due to the logistic and environmental challenges involved in exploration over these areas. During the 2005/06 <span class="hlt">Antarctic</span> field season the British <span class="hlt">Antarctic</span> Survey (BAS) collaborated with the University of Genoa to accomplish an extensive airborne geophysical survey over the EAIS. We explored the enigmatic Wilkes Subglacial Basin (WSB) and the adjacent Transantarctic Mountains (TAM). Over 60,000-line km of new data were collected during 70 survey flights. 270 hours of dedicated science flying and 45 hours of positioning and calibration flying were performed. The Italian <span class="hlt">Antarctic</span> Programme provided the logistic support and aviation fuel at Mario Zucchelli Station, Mid-Point, and at two remote field camps, Talos Dome and Sitry. Additional support and fuel was provided at Dome C, as part of a separate trilateral UK/Italian and French agreement to survey some of the subglacial <span class="hlt">lakes</span>, which characterise this region. The airborne survey platform was a BAS Twin Otter, equipped with airborne radar, aeromagnetic and airborne gravity sensors. We present key new datasets on <span class="hlt">ice</span> surface, <span class="hlt">ice</span> thickness, bedrock configurations, airborne gravity and aeromagnetic anomalies. These new data will assist in addressing four major open questions: 1) Are there Cenozoic marine sediments in the WSB, linked to controversial deglaciation over this part of the EAIS?; 2) What is the tectonic origin and deep structure of the WSB and TAM?; 3) Is there major segmentation of the TAM?, 4) what forcings and feedbacks were involved for the EAIS and for climate evolution?.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/14749827','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/14749827"><span>Enhanced <span class="hlt">ice</span> sheet growth in Eurasia owing to adjacent <span class="hlt">ice</span>-dammed <span class="hlt">lakes</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Krinner, G; Mangerud, J; Jakobsson, M; Crucifix, M; Ritz, C; Svendsen, J I</p> <p>2004-01-29</p> <p>Large proglacial <span class="hlt">lakes</span> cool regional summer climate because of their large heat capacity, and have been shown to modify precipitation through mesoscale atmospheric feedbacks, as in the case of <span class="hlt">Lake</span> Agassiz. Several large <span class="hlt">ice</span>-dammed <span class="hlt">lakes</span>, with a combined area twice that of the Caspian Sea, were formed in northern Eurasia about 90,000 years ago, during the last glacial period when an <span class="hlt">ice</span> sheet centred over the Barents and Kara seas blocked the large northbound Russian rivers. Here we present high-resolution simulations with an atmospheric general circulation model that explicitly simulates the surface mass balance of the <span class="hlt">ice</span> sheet. We show that the main influence of the Eurasian proglacial <span class="hlt">lakes</span> was a significant reduction of <span class="hlt">ice</span> sheet melting at the southern margin of the Barents-Kara <span class="hlt">ice</span> sheet through strong regional summer cooling over large parts of Russia. In our simulations, the summer melt reduction clearly outweighs <span class="hlt">lake</span>-induced decreases in moisture and hence snowfall, such as has been reported earlier for <span class="hlt">Lake</span> Agassiz. We conclude that the summer cooling mechanism from proglacial <span class="hlt">lakes</span> accelerated <span class="hlt">ice</span> sheet growth and delayed <span class="hlt">ice</span> sheet decay in Eurasia and probably also in North America.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMPP11E..02G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMPP11E..02G"><span>Simulating a Dynamic <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet in the Early to Middle Miocene</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gasson, E.; DeConto, R.; Pollard, D.; Levy, R. H.</p> <p>2015-12-01</p> <p>There are a variety of sources of geological data that suggest major variations in the volume and extent of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet during the early to middle Miocene. Simulating such variability using coupled climate-<span class="hlt">ice</span> sheet models is problematic due to a strong hysteresis effect caused by height-mass balance feedback and albedo feedback. This results in limited retreat of the <span class="hlt">ice</span> sheet once it has reached the continental size, as likely occurred prior to the Miocene. Proxy records suggest a relatively narrow range of atmospheric CO2 during the early to middle Miocene, which exacerbates this problem. We use a new climate forcing which accounts for <span class="hlt">ice</span> sheet-climate feedbacks through an asynchronous GCM-RCM coupling, which is able to better resolve the narrow <span class="hlt">Antarctic</span> ablation zone in warm climate simulations. When combined with recently suggested mechanisms for retreat into subglacial basins due to <span class="hlt">ice</span> shelf hydrofracture and <span class="hlt">ice</span> cliff failure, we are able to simulate large-scale variability of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet in the Miocene. This variability is equivalent to a seawater oxygen isotope signal of ~0.5 ‰, or a sea level equivalent change of ~35 m, for a range of atmospheric CO2 between 280 - 500 ppm.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/9974394','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/9974394"><span>Hunting behavior of a marine mammal beneath the <span class="hlt">antarctic</span> fast <span class="hlt">Ice</span></span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Davis; Fuiman; Williams; Collier; Hagey; Kanatous; Kohin; Horning</p> <p>1999-02-12</p> <p>The hunting behavior of a marine mammal was studied beneath the <span class="hlt">Antarctic</span> fast <span class="hlt">ice</span> with an animal-borne video system and data recorder. Weddell seals stalked large <span class="hlt">Antarctic</span> cod and the smaller subice fish Pagothenia borchgrevinki, often with the under-<span class="hlt">ice</span> surface for backlighting, which implies that vision is important for hunting. They approached to within centimeters of cod without startling the fish. Seals flushed P. borchgrevinki by blowing air into subice crevices or pursued them into the platelet <span class="hlt">ice</span>. These observations highlight the broad range of insights that are possible with simultaneous recordings of video, audio, three-dimensional dive paths, and locomotor effort.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C51B0986K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C51B0986K"><span>Challenges for understanding <span class="hlt">Antarctic</span> surface hydrology and <span class="hlt">ice</span>-shelf stability</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kingslake, J.; Bell, R. E.; Banwell, A. F.; Boghosian, A.; Spergel, J.; Trusel, L. D.</p> <p>2017-12-01</p> <p>It is widely hypothesized that surface meltwater can contribute to <span class="hlt">ice</span> mass loss in Antarctica through its impact on <span class="hlt">ice</span>-shelf stability. Meltwater potentially expedites <span class="hlt">ice</span>-shelf calving by flowing into and enlarging existing crevasses, and could even trigger <span class="hlt">ice</span>-shelf disintegration via stresses generated by melt ponds. When <span class="hlt">ice</span> shelves collapse, the adjacent grounded <span class="hlt">ice</span> accelerates and thins, which contributes to sea-level rise. How these mechanisms mediate the interactions between the atmosphere, the ocean and the <span class="hlt">ice</span> sheet is the subject of long-standing research efforts. The drainage of water across the surface of the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet and its <span class="hlt">ice</span> shelves is beginning to be recognized as another important aspect of the system. Recent studies have revealed that surface meltwater drainage is more widespread than previously thought and that surface hydrological systems in Antarctica may expand and proliferate this century. Contrasting hypotheses regarding the impact of the proliferation of drainage systems on <span class="hlt">ice</span>-shelf stability have emerged. Surface drainage could deliver meltwater to vulnerable area or export meltwater from <span class="hlt">ice</span> shelves entirely. Which behavior dominates may have a large impact on the future response of the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet to atmospheric warming. We will discuss these recent discoveries and hypotheses, as well as new detailed studies of specific areas where hydrological systems are well developed, such as Amery and Nimrod <span class="hlt">Ice</span> Shelves. We will highlight analogies that can be drawn with Greenlandic (near-)surface hydrology and, crucially, where hydrological systems on the two <span class="hlt">ice</span> sheets are very different, leading to potentially important gaps in our understanding. Finally, we will look ahead to the key questions that we argue will need to be if we are to determine the role <span class="hlt">Antarctic</span> surface hydrology could play in the future of the <span class="hlt">ice</span> sheet. These include: Where does meltwater pond today and how will this change this century? What</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20030102176','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20030102176"><span>30-Year Satellite Record Reveals Contrasting Arctic and <span class="hlt">Antarctic</span> Decadal Sea <span class="hlt">Ice</span> Variability</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Cavalieri, D. J.; Parkinson, C. L.; Vinnikov, K. Y.</p> <p>2003-01-01</p> <p>A 30-year satellite record of sea <span class="hlt">ice</span> extents derived mostly from satellite microwave radiometer observations reveals that the Arctic sea <span class="hlt">ice</span> extent decreased by 0.30+0.03 x 10(exp 6) square kilometers per 10 yr from 1972 through 2002, but by 0.36 plus or minus 0.05 x 10(exp 6) square kilometers per 10yr from 1979 through 2002, indicating an acceleration of 20% in the rate of decrease. In contrast, the <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> extent decreased dramatically over the period 1973-1977, then gradually increased. Over the full 30-year period, the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> extent decreased by 0.15 plus or minus 0.08 x 10(exp 6) square kilometers per 10 yr. The trend reversal is attributed to a large positive anomaly in <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> extent in the early 1970's, an anomaly that apparently began in the late 1960's, as observed in early visible and infrared satellite images.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1997JGR...10216761C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1997JGR...10216761C"><span>Annually resolved southern hemisphere volcanic history from two <span class="hlt">Antarctic</span> <span class="hlt">ice</span> cores</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cole-Dai, Jihong; Mosley-Thompson, Ellen; Thompson, Lonnie G.</p> <p>1997-07-01</p> <p>The continuous sulfate analysis of two <span class="hlt">Antarctic</span> <span class="hlt">ice</span> cores, one from the <span class="hlt">Antarctic</span> Peninsula region and one from West Antarctica, provides an annually resolved proxy history of southern semisphere volcanism since early in the 15th century. The dating is accurate within ±3 years due to the high rate of snow accumulation at both core sites and the small sample sizes used for analysis. The two sulfate records are consistent with each other. A systematic and objective method of separating outstanding sulfate events from the background sulfate flux is proposed and used to identify all volcanic signals. The resulting volcanic chronology <span class="hlt">covering</span> 1417-1989 A.D. resolves temporal ambiguities about several recently discovered events. A number of previously unknown, moderate eruptions during late 1600s are uncovered in this chronology. The eruption of Tambora (1815) and the recently discovered eruption of Kuwae (1453) in the tropical South Pacific injected the greatest amount of sulfur dioxide into the southern hemisphere stratosphere during the last half millennium. A technique for comparing the magnitude of volcanic events preserved within different <span class="hlt">ice</span> cores is developed using normalized sulfate flux. For the same eruptions the variability of the volcanic sulfate flux between the cores is within ±20% of the sulfate flux from the Tambora eruption.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018TCry...12.1103S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018TCry...12.1103S"><span>Atmospheric influences on the anomalous 2016 <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> decay</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schlosser, Elisabeth; Haumann, F. Alexander; Raphael, Marilyn N.</p> <p>2018-03-01</p> <p>In contrast to the Arctic, where total sea <span class="hlt">ice</span> extent (SIE) has been decreasing for the last three decades, <span class="hlt">Antarctic</span> SIE has shown a small, but significant, increase during the same time period. However, in 2016, an unusually early onset of the melt season was observed; the maximum <span class="hlt">Antarctic</span> SIE was already reached as early as August rather than the end of September, and was followed by a rapid decrease. The decay was particularly strong in November, when <span class="hlt">Antarctic</span> SIE exhibited a negative anomaly (compared to the 1979-2015 average) of approximately 2 million km2. ECMWF Interim reanalysis data showed that the early onset of the melt and the rapid decrease in sea <span class="hlt">ice</span> area (SIA) and SIE were associated with atmospheric flow patterns related to a positive zonal wave number three (ZW3) index, i.e., synoptic situations leading to strong meridional flow and anomalously strong southward heat advection in the regions of strongest sea <span class="hlt">ice</span> decline. A persistently positive ZW3 index from May to August suggests that SIE decrease was preconditioned by SIA decrease. In particular, in the first third of November northerly flow conditions in the Weddell Sea and the Western Pacific triggered accelerated sea <span class="hlt">ice</span> decay, which was continued in the following weeks due to positive feedback effects, leading to the unusually low November SIE. In 2016, the monthly mean Southern Annular Mode (SAM) index reached its second lowest November value since the beginning of the satellite observations. A better spatial and temporal coverage of reliable <span class="hlt">ice</span> thickness data is needed to assess the change in <span class="hlt">ice</span> mass rather than <span class="hlt">ice</span> area.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=STS048%28E%29010&hterms=Antarctic+icebergs&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DAntarctic%2Bicebergs','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=STS048%28E%29010&hterms=Antarctic+icebergs&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DAntarctic%2Bicebergs"><span>STS-48 ESC Earth observation of <span class="hlt">ice</span> pack, <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> 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>STS-48 Earth observation taken aboard Discovery, Orbiter Vehicle (OV) 103, is of the breakup of pack <span class="hlt">ice</span> along the periphery of the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Shelf. Strong offshore winds, probably associated with katabatic downdrafts from the interior of the continent, are seen peeling off the edges of the <span class="hlt">ice</span> shelf into long filaments of sea <span class="hlt">ice</span>, icebergs, bergy bits, and growlers to flow northward into the South Atlantic Ocean. These photos are used to study ocean wind, tide and current patterns. Similar views photographed during previous missions, when analyzed with these recent views may yield information about regional <span class="hlt">ice</span> drift and breakup of <span class="hlt">ice</span> packs. The image was captured using an electronic still camera (ESC), was stored on a removable hard disk or small optical disk, and was converted to a format suitable for downlink transmission. The ESC documentation was part of Development Test Objective (DTO) 648, Electronic Still Photography.</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 <span class="hlt">ice</span></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-<span class="hlt">ice</span> region. In this paper, the first observational study of sub-micron aerosols in the East <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> 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-<span class="hlt">ice</span> 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('http://adsabs.harvard.edu/abs/2017DPS....4911301O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017DPS....4911301O"><span>Modeling the Thermal Interactions of Meteorites Below the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Oldroyd, William Jared; Radebaugh, Jani; Stephens, Denise C.; Lorenz, Ralph; Harvey, Ralph; Karner, James</p> <p>2017-10-01</p> <p>Meteorites with high specific gravities, such as irons, appear to be underrepresented in <span class="hlt">Antarctic</span> collections over the last 40 years. This underrepresentation is in comparison with observed meteorite falls, which are believed to represent the actual population of meteorites striking Earth. Meteorites on the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet absorb solar flux, possibly leading to downward tunneling into the <span class="hlt">ice</span>, though observations of this in action are very limited. This descent is counteracted by <span class="hlt">ice</span> sheet flow supporting the meteorites coupled with ablation near mountain margins, which helps to force meteorites towards the surface. Meteorites that both absorb adequate thermal energy and are sufficiently dense may instead reach a shallow equilibrium depth as downward melting overcomes upward forces during the <span class="hlt">Antarctic</span> summer. Using a pyronometer, we have measured the incoming solar flux at multiple depths in two deep field sites in Antarctica, the Miller Range and Elephant Moraine. We compare these data with laboratory analogues and model the thermal and physical interactions between a variety of meteorites and their surroundings. Our Matlab code model will account for a wide range of parameters used to characterize meteorites in an <span class="hlt">Antarctic</span> environment. We will present the results of our model along with depth estimates for several types of meteorites. The recovery of an additional population of heavy meteorites would increase our knowledge of the formation and composition of the solar system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20060042623&hterms=stress+relationship&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dstress%2Brelationship','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060042623&hterms=stress+relationship&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dstress%2Brelationship"><span>Glacial isostatic stress shadowing by the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ivins, E. R.; James, T. S.; Klemann, V.</p> <p>2005-01-01</p> <p>Numerous examples of fault slip that offset late Quaternary glacial deposits and bedrock polish support the idea that the glacial loading cycle causes earthquakes in the upper crust. A semianalytical scheme is presented for quantifying glacial and postglacial lithospheric fault reactivation using contemporary rock fracture prediction methods. It extends previous studies by considering differential Mogi-von Mises stresses, in addition to those resulting from a Coulomb analysis. The approach utilizes gravitational viscoelastodynamic theory and explores the relationships between <span class="hlt">ice</span> mass history and regional seismicity and faulting in a segment of East Antarctica containing the great <span class="hlt">Antarctic</span> Plate (Balleny Island) earthquake of 25 March 1998 (Mw 8.1). Predictions of the failure stress fields within the seismogenic crust are generated for differing assumptions about background stress orientation, mantle viscosity, lithospheric thickness, and possible late Holocene deglaciation for the D91 <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet history. Similar stress fracture fields are predicted by Mogi-von Mises and Coulomb theory, thus validating previous rebound Coulomb analysis. A thick lithosphere, of the order of 150-240 km, augments stress shadowing by a late melting (middle-late Holocene) coastal East <span class="hlt">Antarctic</span> <span class="hlt">ice</span> complex and could cause present-day earthquakes many hundreds of kilometers seaward of the former Last Glacial Maximum grounding line.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_16 --> <div id="page_17" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li class="active"><span>17</span></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="321"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSHE44B1511L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSHE44B1511L"><span>Contribution of Increasing Glacial Freshwater Fluxes to Observed Trends in <span class="hlt">Antarctic</span> Sea <span class="hlt">Ice</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Le Sommer, J.; Merino, N.; Durand, G.; Jourdain, N.; Goosse, H.; Mathiot, P.; Gurvan, M.</p> <p>2016-02-01</p> <p>Southern Ocean sea-<span class="hlt">ice</span> extent has experienced an overall positive trend over recent decades. While the amplitude of this trend is open to debate, the geographical pattern of regional changes has been clearly identified by observations. Mechanisms driving changes in the <span class="hlt">Antarctic</span> Sea <span class="hlt">Ice</span> Extent (SIE) are not fully understood and climate models fail to simulate these trends. Changes in different atmospheric features such as SAM or ENSO seem to explain the observed trend of Antartic sea <span class="hlt">ice</span>, but only partly, since they can not account for the actual amplitude of the observed signal. The increasing injection of freshwater due to the accelerating <span class="hlt">ice</span> discharge from Antarctica <span class="hlt">Ice</span> Sheet (AIS) during the last two decades has been proposed as another candidate to contribute to SIE trend. However, the quantity and the distribution of the extra freshwater injection were not properly constrained. Recent glaciological estimations may improve the way the glacial freshwater is injected in the model. Here, we study the role of the glacial freshwater into the observed SIE trend, using the state-of-the-art <span class="hlt">Antarctic</span> mass loss estimations. Ocean/sea-<span class="hlt">ice</span> model simulations have been carried out with two different <span class="hlt">Antarctic</span> freshwater scenarios corresponding to 20-years of <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet evolution. The combination of an improved iceberg model with the most recent glaciological estimations has been applied to account for the most realistic possible <span class="hlt">Antarctic</span> freshwater evolution scenarios. Results suggest that Antarctica has contributed to almost a 30% of the observed trend in regions of the South Pacific and South East Indian sectors, but has little impact in the South Atlantic sector. We conclude that the observed SIE trend over the last decades is due to a combination of both an atmospheric forcing and the extra freshwater injection. Our results advocates that the evolution of glacial freshwater needs to be correctly represented in climate models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.1690J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.1690J"><span><span class="hlt">Antarctic</span> Climate Variability: Covariance of Ozone and Sea <span class="hlt">Ice</span> in Atmosphere - Ocean Coupled Model Simulations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jrrar, Amna; Abraham, N. Luke; Pyle, John A.; Holland, David</p> <p>2014-05-01</p> <p>Changes in sea <span class="hlt">ice</span> significantly modulate climate change because of its high reflective and insulating nature. While Arctic Sea <span class="hlt">Ice</span> Extent (SIE) shows a negative trend. <span class="hlt">Antarctic</span> SIE shows a weak but positive trend, estimated at 0.127 x 106 km2 per decade. The trend results from large regional cancellations, more <span class="hlt">ice</span> in the Weddell and the Ross seas, and less <span class="hlt">ice</span> in the Amundsen - Bellingshausen seas. A number of studies had demonstrated that stratospheric ozone depletion has had a major impact on the atmospheric circulation, causing a positive trend in the Southern Annular Mode (SAM), which has been linked to the observed positive trend in autumn sea <span class="hlt">ice</span> in the Ross Sea. However, other modelling studies show that models forced with prescribed ozone hole simulate decreased sea <span class="hlt">ice</span> in all regions comparative to a control run. A recent study has also shown that stratospheric ozone recovery will mitigate <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> loss. To verify this assumed relationship, it is important first to investigate the covariance between ozone's natural (dynamical) variability and <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> distribution in pre-industrial climate, to estimate the trend due to natural variability. We investigate the relationship between anomalous <span class="hlt">Antarctic</span> ozone years and the subsequent changes in <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> distribution in a multidecadal control simulation using the AO-UMUKCA model. The model has a horizontal resolution of 3.75 X 2.5 degrees in longitude and latitude; and 60 hybrid height levels in the vertical, from the surface up to a height of 84 km. The ocean component is the NEMO ocean model on the ORCA2 tripolar grid, and the sea <span class="hlt">ice</span> model is CICE. We evaluate the model's performance in terms of sea <span class="hlt">ice</span> distribution, and we calculate sea <span class="hlt">ice</span> extent trends for composites of anomalously low versus anomalously high SH polar ozone column. We apply EOF analysis to the seasonal anomalies of sea <span class="hlt">ice</span> concentration, MSLP, and Z 500, and identify the leading climate modes controlling the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-GSFC_20171208_Archive_e001453.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-GSFC_20171208_Archive_e001453.html"><span><span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Shelf Loss Comes From Underneath</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>Calving front of an <span class="hlt">ice</span> shelf in West Antarctica. The traditional view on <span class="hlt">ice</span> shelves, the floating extensions of seaward glaciers, has been that they mostly lose <span class="hlt">ice</span> by shedding icebergs. A new study by NASA and university researchers has found that warm ocean waters melting the <span class="hlt">ice</span> sheets from underneath account for 55 percent of all <span class="hlt">ice</span> shelf mass loss in Antarctica. This image was taken during the 2012 <span class="hlt">Antarctic</span> campaign of NASA's Operation <span class="hlt">Ice</span>Bridge, a mission that provided data for the new <span class="hlt">ice</span> shelf study. Read more: www.nasa.gov/topics/earth/features/earth20130613.html Credit: NASA/GSFC/Jefferson Beck NASA image use policy. NASA Goddard Space Flight Center enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. Follow us on Twitter Like us on Facebook Find us on Instagram</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19910017259','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19910017259"><span>West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet Initiative. Volume 2: Discipline Reviews</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bindschadler, Robert A. (Editor)</p> <p>1991-01-01</p> <p>Seven discipline review papers are presented on the state of the knowledge of West Antarctica and opinions on how that knowledge must be increased to predict the future behavior of this <span class="hlt">ice</span> sheet and to assess its potential to collapse, rapidly raising the global sea level. These are the goals of the West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet Initiative (WAIS).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1815826M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1815826M"><span>Evaluating <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> predictability at seasonal to interannual timescales in global climate models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marchi, Sylvain; Fichefet, Thierry; Goosse, Hugues; Zunz, Violette; Tietsche, Steffen; Day, Jonny; Hawkins, Ed</p> <p>2016-04-01</p> <p>Unlike the rapid sea <span class="hlt">ice</span> losses reported in the Arctic, satellite observations show an overall increase in <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> extent over recent decades. Although many processes have already been suggested to explain this positive trend, it remains the subject of current investigations. Understanding the evolution of the <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> turns out to be more complicated than for the Arctic for two reasons: the lack of observations and the well-known biases of climate models in the Southern Ocean. Irrespective of those issues, another one is to determine whether the positive trend in sea <span class="hlt">ice</span> extent would have been predictable if adequate observations and models were available some decades ago. This study of <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> predictability is carried out using 6 global climate models (HadGEM1.2, MPI-ESM-LR, GFDL CM3, EC-Earth V2, MIROC 5.2 and ECHAM 6-FESOM) which are all part of the APPOSITE project. These models are used to perform hindcast simulations in a perfect model approach. The predictive skill is estimated thanks to the PPP (Potential Prognostic Predictability) and the ACC (Anomaly Correlation Coefficient). The former is a measure of the uncertainty of the ensemble while the latter assesses the accuracy of the prediction. These two indicators are applied to different variables related to sea <span class="hlt">ice</span>, in particular the total sea <span class="hlt">ice</span> extent and the <span class="hlt">ice</span> edge location. This first model intercomparison study about sea <span class="hlt">ice</span> predictability in the Southern Ocean aims at giving a general overview of <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> predictability in current global climate models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1997Natur.387..897L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1997Natur.387..897L"><span>Effects of sea-<span class="hlt">ice</span> extent and krill or salp dominance on the <span class="hlt">Antarctic</span> food web</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Loeb, V.; Siegel, V.; Holm-Hansen, O.; Hewitt, R.; Fraser, W.; Trivelpiece, W.; Trivelpiece, S.</p> <p>1997-06-01</p> <p>Krill (Euphausia superba) provide a direct link between primary producers and higher trophic levels in the <span class="hlt">Antarctic</span> marine food web. The pelagic tunicate Salpa thompsoni can also be important during spring and summer through the formation of extensive and dense blooms. Although salps are not a major dietary item for <span class="hlt">Antarctic</span> vertebrate predators,, their blooms can affect adult krill reproduction and survival of krill larvae. Here we provide data from 1995 and 1996 that support hypothesized relationships between krill, salps and region-wide sea-<span class="hlt">ice</span> conditions,. We have assessed salp consumption as a proportion of net primary production, and found correlations between herbivore densities and integrated chlorophyll-a that indicate that there is a degree of competition between krill and salps. Our analysis of the relationship between annual sea-<span class="hlt">ice</span> <span class="hlt">cover</span> and a longer time series of air temperature measurements, indicates a decreased frequency of winters with extensive sea-<span class="hlt">ice</span> development over the last five decades. Our data suggest that decreased krill availability may affect the levels of their vertebrate predators. Regional warming and reduced krill abundance therefore affect the marine food web and krill resource management.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26064653','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26064653"><span>Extreme ecological response of a seabird community to unprecedented sea <span class="hlt">ice</span> <span class="hlt">cover</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Barbraud, Christophe; Delord, Karine; Weimerskirch, Henri</p> <p>2015-05-01</p> <p>Climate change has been predicted to reduce <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> but, instead, sea <span class="hlt">ice</span> surrounding Antarctica has expanded over the past 30 years, albeit with contrasted regional changes. Here we report a recent extreme event in sea <span class="hlt">ice</span> conditions in East Antarctica and investigate its consequences on a seabird community. In early 2014, the Dumont d'Urville Sea experienced the highest magnitude sea <span class="hlt">ice</span> <span class="hlt">cover</span> (76.8%) event on record (1982-2013: range 11.3-65.3%; mean±95% confidence interval: 27.7% (23.1-32.2%)). Catastrophic effects were detected in the breeding output of all sympatric seabird species, with a total failure for two species. These results provide a new view crucial to predictive models of species abundance and distribution as to how extreme sea <span class="hlt">ice</span> events might impact an entire community of top predators in polar marine ecosystems in a context of expanding sea <span class="hlt">ice</span> in eastern Antarctica.</p> </li> <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 <span class="hlt">covered</span> include the following: earth science; <span class="hlt">ice</span> 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/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> <span class="hlt">ice</span> 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> <span class="hlt">ice</span> shelves and marine-terminating glaciers over the last decades. However, much less is known about the drivers of <span class="hlt">ice</span> shelf melt prior to the short instrumental era. Based on diatom oxygen isotope (δ18Odiatom; a proxy for glacial <span class="hlt">ice</span> 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 <span class="hlt">ice</span> 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 <span class="hlt">ice</span> 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 <span class="hlt">ice</span> 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 <span class="hlt">ice</span> discharge. Conversely, our simulations evidence the potential for significant warmer subsurface waters 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 Water towards the <span class="hlt">Antarctic</span> shelf. We conclude that <span class="hlt">ice</span> 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://adsabs.harvard.edu/abs/2012AGUFMPP31D..01M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMPP31D..01M"><span>2.8 Million Years of Arctic Climate Change from Deep Drilling at <span class="hlt">Lake</span> El'gygytgyn, NE Russia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Melles, M.; Brigham-Grette, J.; Minyuk, P.; Wennrich, V.; Nowaczyk, N.; DeConto, R.; Anderson, P.; Andreev, A.; Haltia-Hovi, E.; Kukkonen, M.; Lozhkin, A.; Rosén, P.; Tarasov, P.</p> <p>2012-12-01</p> <p> coupling, which could be due to a reduction of <span class="hlt">Antarctic</span> Bottom Water formation and/or a significant global sea-level rise during times of WAIS decays. References: Melles M. et al. (2011): The El'gygytgyn Scientific Drilling Project - conquering Arctic challenges through continental drilling. - Scientific Drilling, 11: 29-40. Melles M. et al. (2012): 2.8 Million Years of Arctic Climate Change from <span class="hlt">Lake</span> El'gygytgyn, NE Russia. - Science, 337: 315-320. Nolan M. (2012): Analysis of local AWS and NCEP/NCAR reanalysis data at <span class="hlt">Lake</span> El'gygytgyn, and its implications for maintaining multi-year <span class="hlt">lake-ice</span> <span class="hlt">covers</span>. - Clim. Past Disc., 8: 1443-1483. Naish T. et al. (2009): Obliquity-paced Pliocene West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet oscillations. - Nature, 458: 322-329. Pollard D. and DeConto R.M. (2009): Modelling West <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet growth and collapse through the past five million years. - Nature, 458: 329-332.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015ACPD...1529125H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015ACPD...1529125H"><span>Unexpectedly high ultrafine aerosol concentrations above East <span class="hlt">Antarctic</span> sea-<span class="hlt">ice</span></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>2015-10-01</p> <p>The effect of aerosols on clouds and their radiative properties is one of the largest uncertainties in our understanding of radiative forcing. A recent study has concluded that better characterisation of pristine, natural aerosol processes leads to the largest reduction in these uncertainties. Antarctica, being far from anthropogenic activities, is an ideal location for the study of natural aerosol processes. Aerosol measurements in Antarctica are often limited to boundary layer air-masses at spatially sparse coastal and continental research stations, with only a handful of studies in the sea <span class="hlt">ice</span> region. In this paper, the first observational study of sub-micron aerosols in the East <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> region is presented. Measurements were conducted aboard the <span class="hlt">ice</span>-breaker 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 <span class="hlt">ice</span> boundary layer air-masses travelled equator-ward into the low albedo Southern Ocean region, transporting with them emissions and these aerosol nuclei where, after growth, may potentially impact on the region's radiative balance. The high aerosol concentrations and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24451542','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24451542"><span>Impacts of the north and tropical Atlantic Ocean on the <span class="hlt">Antarctic</span> Peninsula and sea <span class="hlt">ice</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Li, Xichen; Holland, David M; Gerber, Edwin P; Yoo, Changhyun</p> <p>2014-01-23</p> <p>In recent decades, Antarctica has experienced pronounced climate changes. The <span class="hlt">Antarctic</span> Peninsula exhibited the strongest warming of any region on the planet, causing rapid changes in land <span class="hlt">ice</span>. Additionally, in contrast to the sea-<span class="hlt">ice</span> decline over the Arctic, <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> has not declined, but has instead undergone a perplexing redistribution. <span class="hlt">Antarctic</span> climate is influenced by, among other factors, changes in radiative forcing and remote Pacific climate variability, but none explains the observed <span class="hlt">Antarctic</span> Peninsula warming or the sea-<span class="hlt">ice</span> redistribution in austral winter. However, in the north and tropical Atlantic Ocean, the Atlantic Multidecadal Oscillation (a leading mode of sea surface temperature variability) has been overlooked in this context. Here we show that sea surface warming related to the Atlantic Multidecadal Oscillation reduces the surface pressure in the Amundsen Sea and contributes to the observed dipole-like sea-<span class="hlt">ice</span> redistribution between the Ross and Amundsen-Bellingshausen-Weddell seas and to the <span class="hlt">Antarctic</span> Peninsula warming. Support for these findings comes from analysis of observational and reanalysis data, and independently from both comprehensive and idealized atmospheric model simulations. We suggest that the north and tropical Atlantic is important for projections of future climate change in Antarctica, and has the potential to affect the global thermohaline circulation and sea-level change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.7924N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.7924N"><span>Snow depth on Arctic and <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> derived from autonomous (Snow Buoy) measurements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nicolaus, Marcel; Arndt, Stefanie; Hendricks, Stefan; Heygster, Georg; Huntemann, Marcus; Katlein, Christian; Langevin, Danielle; Rossmann, Leonard; Schwegmann, Sandra</p> <p>2016-04-01</p> <p>The snow <span class="hlt">cover</span> on sea <span class="hlt">ice</span> received more and more attention in recent sea <span class="hlt">ice</span> studies and model simulations, because its physical properties dominate many sea <span class="hlt">ice</span> and upper ocean processes. In particular; the temporal and spatial distribution of snow depth is of crucial importance for the energy and mass budgets of sea <span class="hlt">ice</span>, as well as for the interaction with the atmosphere and the oceanic freshwater budget. Snow depth is also a crucial parameter for sea <span class="hlt">ice</span> thickness retrieval algorithms from satellite altimetry data. Recent time series of Arctic sea <span class="hlt">ice</span> volume only use monthly snow depth climatology, which cannot take into account annual changes of the snow depth and its properties. For <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span>, no such climatology is available. With a few exceptions, snow depth on sea <span class="hlt">ice</span> is determined from manual in-situ measurements with very limited coverage of space and time. Hence the need for more consistent observational data sets of snow depth on sea <span class="hlt">ice</span> is frequently highlighted. Here, we present time series measurements of snow depths on <span class="hlt">Antarctic</span> and Arctic sea <span class="hlt">ice</span>, recorded by an innovative and affordable platform. This Snow Buoy is optimized to autonomously monitor the evolution of snow depth on sea <span class="hlt">ice</span> and will allow new insights into its seasonality. In addition, the instruments report air temperature and atmospheric pressure directly into different international networks, e.g. the Global Telecommunication System (GTS) and the International Arctic Buoy Programme (IABP). We introduce the Snow Buoy concept together with technical specifications and results on data quality, reliability, and performance of the units. We highlight the findings from four buoys, which simultaneously drifted through the Weddell Sea for more than 1.5 years, revealing unique information on characteristic regional and seasonal differences. Finally, results from seven snow buoys co-deployed on Arctic sea <span class="hlt">ice</span> throughout the winter season 2015/16 suggest the great importance of local</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016SPIE.9878E..18J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016SPIE.9878E..18J"><span>Exploratory normalized difference water indices for semi-automated extraction of <span class="hlt">Antarctic</span> <span class="hlt">lake</span> features</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jawak, Shridhar D.; Luis, Alvarinho J.</p> <p>2016-05-01</p> <p>This work presents various normalized difference water indices (NDWI) to delineate <span class="hlt">lakes</span> from Schirmacher Oasis, East Antarctica, by using a very high resolution WorldView-2 (WV-2) satellite imagery. Schirmacher oasis region hosts a number of fresh as well as saline water <span class="hlt">lakes</span>, such as epishelf <span class="hlt">lakes</span>, <span class="hlt">ice</span>-free or landlocked <span class="hlt">lakes</span>, which are completely frozen or semi-frozen and in a <span class="hlt">ice</span>-free state. Hence, detecting all these types of <span class="hlt">lakes</span> distinctly on satellite imagery was the major challenge, as the spectral characteristics of various types of <span class="hlt">lakes</span> were identical to the other land <span class="hlt">cover</span> targets. Multiband spectral index pixel-based approach is most experimented and recently growing technique because of its unbeatable advantages such as its simplicity and comparatively lesser amount of processing-time. In present study, semiautomatic extraction of <span class="hlt">lakes</span> in cryospheric region was carried out by designing specific spectral indices. The study utilized number of existing spectral indices to extract <span class="hlt">lakes</span> but none could deliver satisfactory results and hence we modified NDWI. The potentials of newly added bands in WV-2 satellite imagery was explored by developing spectral indices comprising of Yellow (585 - 625 nm) band, in combination with Blue (450 - 510 nm), Coastal (400 - 450 nm) and Green (510 - 580 nm) bands. For extraction of frozen <span class="hlt">lakes</span>, use of Yellow (585 - 625 nm) and near-infrared 2 (NIR2) band pair, and Yellow and Green band pair worked well, whereas for <span class="hlt">ice</span>-free <span class="hlt">lakes</span> extraction, a combination of Blue and Coastal band yielded appreciable results, when compared with manually digitized data. The results suggest that the modified NDWI approach rendered bias error varying from 1 to 34 m2.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/18051650','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/18051650"><span>Trophic structure of coastal <span class="hlt">Antarctic</span> food webs associated with changes in sea <span class="hlt">ice</span> and food supply.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Norkko, A; Thrush, S F; Cummings, V J; Gibbs, M M; Andrew, N L; Norkko, J; Schwarz, A M</p> <p>2007-11-01</p> <p>Predicting the dynamics of ecosystems requires an understanding of how trophic interactions respond to environmental change. In <span class="hlt">Antarctic</span> marine ecosystems, food web dynamics are inextricably linked to sea <span class="hlt">ice</span> conditions that affect the nature and magnitude of primary food sources available to higher trophic levels. Recent attention on the changing sea <span class="hlt">ice</span> conditions in polar seas highlights the need to better understand how marine food webs respond to changes in such broad-scale environmental drivers. This study investigated the importance of sea <span class="hlt">ice</span> and advected primary food sources to the structure of benthic food webs in coastal Antarctica. We compared the isotopic composition of several seafloor taxa (including primary producers and invertebrates with a variety of feeding modes) that are widely distributed in the <span class="hlt">Antarctic</span>. We assessed shifts in the trophic role of numerically dominant benthic omnivores at five coastal Ross Sea locations. These locations vary in primary productivity and food availability, due to their different levels of sea <span class="hlt">ice</span> <span class="hlt">cover</span>, and proximity to polynyas and advected primary production. The delta15N signatures and isotope mixing model results for the bivalves Laternula elliptica and Adamussium colbecki and the urchin Sterechinus neumeyeri indicate a shift from consumption of a higher proportion of detritus at locations with more permanent sea <span class="hlt">ice</span> in the south to more freshly produced algal material associated with proximity to <span class="hlt">ice</span>-free water in the north and east. The detrital pathways utilized by many benthic species may act to dampen the impacts of large seasonal fluctuations in the availability of primary production. The limiting relationship between sea <span class="hlt">ice</span> distribution and in situ primary productivity emphasizes the role of connectivity and spatial subsidies of organic matter in fueling the food web. Our results begin to provide a basis for predicting how benthic ecosystems will respond to changes in sea <span class="hlt">ice</span> persistence and extent</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> <span class="hlt">ice</span> 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>Arguments for short-lived <span class="hlt">Antarctic</span> glacial events during the Eocene (55-34 Ma) are compelling, however the paleoceanographic proxy records upon which these arguments are based (e.g., benthic δ18O, eustatic sea level, deep sea carbonate deposition) are global signals in which the role of <span class="hlt">Antarctic</span> <span class="hlt">ice</span> volume variability is ambiguous. That is to say, the proxy response to <span class="hlt">ice</span> volume may be masked other processes. As a result broad correlations between proxies for <span class="hlt">ice</span> volume are lacking during suspected Eocene glacial events. I will present a more direct approach for detecting <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheets in the Eocene; utilizing provenance information derived from the radiogenic isotopic composition of the terrigenous component of marine sediments near Antarctica. The method relies on knowledge that marine sediments represent a mixture derived from different basement terrains with different isotopic fingerprints. A key issue when using sedimentary deposits to characterize continental sediment sources is to deconvolve different sources from the mixed signal of the bulk sample. The pioneering work of Roy et al. (2007) and van de Flierdt et al. (2007) represents a major advance in <span class="hlt">Antarctic</span> provenance studies. It is now known that the isotopic composition of neodymium (Nd) and hafnium (Hf) in modern circum-<span class="hlt">Antarctic</span> sediments are distributed in a pattern that mimics the basement age of sediment sources around Antarctica. For this study I selected two Ocean Drilling Program (ODP) sites on southern Kerguelen Plateau (ODP Sites 738 and 748) because of their proximity to Prydz Bay, where Precambrian sediment sources contribute to extremely nonradiogenic isotopic signatures in modern sediments in the Prydz Bay region. New detrital Nd isotope records from these sediment cores reveal an Nd isotope excursion at the Bartonian/Priabonian boundary (ca. 37 Ma) that coincides with a 0.5 ‰ increase in benthic foram δ18O values. Detrital sediment ɛNd values are around -12 in intervals</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012MsT..........3S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012MsT..........3S"><span>Semi-automated Digital Imaging and Processing System for Measuring <span class="hlt">Lake</span> <span class="hlt">Ice</span> Thickness</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Singh, Preetpal</p> <p></p> <p>Canada is home to thousands of freshwater <span class="hlt">lakes</span> and rivers. Apart from being sources of infinite natural beauty, rivers and <span class="hlt">lakes</span> are an important source of water, food and transportation. The northern hemisphere of Canada experiences extreme cold temperatures in the winter resulting in a freeze up of regional <span class="hlt">lakes</span> and rivers. Frozen <span class="hlt">lakes</span> and rivers tend to offer unique opportunities in terms of wildlife harvesting and winter transportation. <span class="hlt">Ice</span> roads built on frozen rivers and <span class="hlt">lakes</span> are vital supply lines for industrial operations in the remote north. Monitoring the <span class="hlt">ice</span> freeze-up and break-up dates annually can help predict regional climatic changes. <span class="hlt">Lake</span> <span class="hlt">ice</span> impacts a variety of physical, ecological and economic processes. The construction and maintenance of a winter road can cost millions of dollars annually. A good understanding of <span class="hlt">ice</span> mechanics is required to build and deem an <span class="hlt">ice</span> road safe. A crucial factor in calculating load bearing capacity of <span class="hlt">ice</span> sheets is the thickness of <span class="hlt">ice</span>. Construction costs are mainly attributed to producing and maintaining a specific thickness and density of <span class="hlt">ice</span> that can support different loads. Climate change is leading to warmer temperatures causing the <span class="hlt">ice</span> to thin faster. At a certain point, a winter road may not be thick enough to support travel and transportation. There is considerable interest in monitoring winter road conditions given the high construction and maintenance costs involved. Remote sensing technologies such as Synthetic Aperture Radar have been successfully utilized to study the extent of <span class="hlt">ice</span> <span class="hlt">covers</span> and record freeze-up and break-up dates of <span class="hlt">ice</span> on <span class="hlt">lakes</span> and rivers across the north. <span class="hlt">Ice</span> road builders often used Ultrasound equipment to measure <span class="hlt">ice</span> thickness. However, an automated monitoring system, based on machine vision and image processing technology, which can measure <span class="hlt">ice</span> thickness on <span class="hlt">lakes</span> has not been thought of. Machine vision and image processing techniques have successfully been used in manufacturing</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5906079','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5906079"><span>Freshening by glacial meltwater enhances melting of <span class="hlt">ice</span> shelves and reduces formation of <span class="hlt">Antarctic</span> Bottom Water</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 Wijk, Esmee</p> <p>2018-01-01</p> <p>Strong heat loss and brine release during sea <span class="hlt">ice</span> formation in coastal polynyas act to cool and salinify waters on the <span class="hlt">Antarctic</span> continental shelf. Polynya activity thus both limits the ocean heat flux to the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet and promotes formation of Dense Shelf Water (DSW), the precursor to <span class="hlt">Antarctic</span> 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 <span class="hlt">ice</span> shelves partially offsets the salt flux by sea <span class="hlt">ice</span> 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 <span class="hlt">Ice</span> Shelf on the Sabrina Coast and at the Dotson and Getz <span class="hlt">ice</span> shelves in the Amundsen Sea. Our results suggest that increased glacial meltwater input in a warming climate will both reduce <span class="hlt">Antarctic</span> Bottom Water formation and trigger increased mass loss from the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet, with consequences for the global overturning circulation and sea level rise. PMID:29675467</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29675467','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29675467"><span>Freshening by glacial meltwater enhances melting of <span class="hlt">ice</span> shelves and reduces formation of <span class="hlt">Antarctic</span> Bottom Water.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Silvano, Alessandro; Rintoul, Stephen Rich; Peña-Molino, Beatriz; Hobbs, William Richard; van Wijk, Esmee; Aoki, Shigeru; Tamura, Takeshi; Williams, Guy Darvall</p> <p>2018-04-01</p> <p>Strong heat loss and brine release during sea <span class="hlt">ice</span> formation in coastal polynyas act to cool and salinify waters on the <span class="hlt">Antarctic</span> continental shelf. Polynya activity thus both limits the ocean heat flux to the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet and promotes formation of Dense Shelf Water (DSW), the precursor to <span class="hlt">Antarctic</span> 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 <span class="hlt">ice</span> shelves partially offsets the salt flux by sea <span class="hlt">ice</span> 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 <span class="hlt">Ice</span> Shelf on the Sabrina Coast and at the Dotson and Getz <span class="hlt">ice</span> shelves in the Amundsen Sea. Our results suggest that increased glacial meltwater input in a warming climate will both reduce <span class="hlt">Antarctic</span> Bottom Water formation and trigger increased mass loss from the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet, with consequences for the global overturning circulation and sea level rise.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C51B0988S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C51B0988S"><span><span class="hlt">Ice</span> velocity and SAR backscatter record for 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>Scheuchl, B.; Mouginot, J.; Rignot, E. J.; Small, D.; Khazendar, A.; Seroussi, H. L.; Kellndorfer, J. M.</p> <p>2017-12-01</p> <p>The <span class="hlt">Antarctic</span> Peninsula has undergone some dramatic changes in the last three decades. The latest high-profile change was the calving of iceberg A68 off the Larsen-C <span class="hlt">ice</span> shelf, which resulted in the <span class="hlt">ice</span> shelf to have the smallest extent since the beginning of satellite observations. A first indication of the beginning of the formation of the iceberg was reported based on 2008 <span class="hlt">ice</span> velocity data by Khazendar et al. 2011 (GRL). With two long term funded missions as well as other available sensors, there is a wealth of data being collected not seen before. The European Sentinel-1 constellation provides InSAR coverage of the area every 6 days. In addition, lower resolution wide swath data are being collected over the Weddell sea and <span class="hlt">cover</span> the shelf frequently. Landsat-8 thermal infrared imagery proved another valuable data source in monitoring the progression. USGS has committed Landsat-8 for frequent acquisitions in Antarctica during periods with available daylight. Here we take a longer term view of the <span class="hlt">Antarctic</span> Peninsula and will provide a satellite data record of <span class="hlt">ice</span> velocity data generated using SAR and optical data. In difference to our MEaSUREs Antarctica-wide 1 km annual product, this regional time series will be provided at 50 m posting to facilitate research that requires higher resolution velocity maps. We also use suitable InSAR data to determine the grounding line for the region. SAR backscatter can vary dramatically in the region, particularly in Austral summer. Low backscatter is an indication for surface melt, and in the case of Larsen-C, this can engulf the entire <span class="hlt">ice</span> shelf at times. We will generate a calibrated backscatter time series using a precision DEM of the region. The maps will provide the temporal and spatial extent of surface melt and will be compared with results from the Regional Climate Model (RACMO) and, where available, with weather station data. We also use double difference interferograms, to chronicle the progression of the Larsen</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li class="active"><span>17</span></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_17 --> <div id="page_18" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="341"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=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> <span class="hlt">Ice</span> 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> <span class="hlt">ice</span> 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 <span class="hlt">ice</span> sheet in the Ross Sea began between 11,000 and 12,000 years ago. This history implies an average contribution of this <span class="hlt">ice</span> 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 waters, 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> <span class="hlt">ice</span> sheet more difficult to predict but suggest that if it loses its hold on the present shallow bed, the final retreat of the <span class="hlt">ice</span> sheet could be very rapid.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015GeoRL..42.5442L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015GeoRL..42.5442L"><span>Observed platelet <span class="hlt">ice</span> distributions in <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span>: An index for ocean-<span class="hlt">ice</span> shelf heat flux</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Langhorne, P. J.; Hughes, K. G.; Gough, A. J.; Smith, I. J.; Williams, M. J. M.; Robinson, N. J.; Stevens, C. L.; Rack, W.; Price, D.; Leonard, G. H.; Mahoney, A. R.; Haas, C.; Haskell, T. G.</p> <p>2015-07-01</p> <p><span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> that has been affected by supercooled <span class="hlt">Ice</span> Shelf Water (ISW) has a unique crystallographic structure and is called platelet <span class="hlt">ice</span>. In this paper we synthesize platelet <span class="hlt">ice</span> observations to construct a continent-wide map of the winter presence of ISW at the ocean surface. The observations demonstrate that, in some regions of coastal Antarctica, supercooled ISW drives a negative oceanic heat flux of -30 Wm-2 that persists for several months during winter, significantly affecting sea <span class="hlt">ice</span> thickness. In other regions, particularly where the thinning of <span class="hlt">ice</span> shelves is believed to be greatest, platelet <span class="hlt">ice</span> is not observed. Our new data set includes the longest <span class="hlt">ice</span>-ocean record for Antarctica, which dates back to 1902 near the McMurdo <span class="hlt">Ice</span> Shelf. These historical data indicate that, over the past 100 years, any change in the volume of very cold surface outflow from this <span class="hlt">ice</span> shelf is less than the uncertainties in the measurements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016NatCC...6..479F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016NatCC...6..479F"><span>The safety band of <span class="hlt">Antarctic</span> <span class="hlt">ice</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>Fürst, Johannes Jakob; Durand, Gaël; Gillet-Chaulet, Fabien; Tavard, Laure; Rankl, Melanie; Braun, Matthias; Gagliardini, Olivier</p> <p>2016-05-01</p> <p>The floating <span class="hlt">ice</span> shelves along the seaboard of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet restrain the outflow of upstream grounded <span class="hlt">ice</span>. Removal of these <span class="hlt">ice</span> shelves, as shown by past <span class="hlt">ice</span>-shelf recession and break-up, accelerates the outflow, which adds to sea-level rise. A key question in predicting future outflow is to quantify the extent of calving that might precondition other dynamic consequences and lead to loss of <span class="hlt">ice</span>-shelf restraint. Here we delineate frontal areas that we label as `passive shelf ice’ and that can be removed without major dynamic implications, with contrasting results across the continent. The <span class="hlt">ice</span> shelves in the Amundsen and Bellingshausen seas have limited or almost no `passive’ portion, which implies that further retreat of current <span class="hlt">ice</span>-shelf fronts will yield important dynamic consequences. This region is particularly vulnerable as <span class="hlt">ice</span> shelves have been thinning at high rates for two decades and as upstream grounded <span class="hlt">ice</span> rests on a backward sloping bed, a precondition to marine <span class="hlt">ice</span>-sheet instability. In contrast to these <span class="hlt">ice</span> shelves, Larsen C <span class="hlt">Ice</span> Shelf, in the Weddell Sea, exhibits a large `passive’ frontal area, suggesting that the imminent calving of a vast tabular iceberg will be unlikely to instantly produce much dynamic change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24892750','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24892750"><span>Ca2+-stabilized adhesin helps an <span class="hlt">Antarctic</span> bacterium reach out and bind <span class="hlt">ice</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Vance, Tyler D R; Olijve, Luuk L C; Campbell, Robert L; Voets, Ilja K; Davies, Peter L; Guo, Shuaiqi</p> <p>2014-07-04</p> <p>The large size of a 1.5-MDa <span class="hlt">ice</span>-binding adhesin [MpAFP (Marinomonas primoryensis antifreeze protein)] from an <span class="hlt">Antarctic</span> Gram-negative bacterium, M. primoryensis, is mainly due to its highly repetitive RII (Region II). MpAFP_RII contains roughly 120 tandem copies of an identical 104-residue repeat. We have previously determined that a single RII repeat folds as a Ca2+-dependent immunoglobulin-like domain. Here, we solved the crystal structure of RII tetra-tandemer (four tandem RII repeats) to a resolution of 1.8 Å. The RII tetra-tandemer reveals an extended (~190-Å × ~25-Å), rod-like structure with four RII-repeats aligned in series with each other. The inter-repeat regions of the RII tetra-tandemer are strengthened by Ca2+ bound to acidic residues. SAXS (small-angle X-ray scattering) profiles indicate the RII tetra-tandemer is significantly rigidified upon Ca2+ binding, and that the protein's solution structure is in excellent agreement with its crystal structure. We hypothesize that >600 Ca2+ help rigidify the chain of ~120 104-residue repeats to form a ~0.6 μm rod-like structure in order to project the <span class="hlt">ice</span>-binding domain of MpAFP away from the bacterial cell surface. The proposed extender role of RII can help the strictly aerobic, motile bacterium bind <span class="hlt">ice</span> in the upper reaches of the <span class="hlt">Antarctic</span> <span class="hlt">lake</span> where oxygen and nutrients are most abundant. Ca2+-induced rigidity of tandem Ig-like repeats in large adhesins might be a general mechanism used by bacteria to bind to their substrates and help colonize specific niches.</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 <span class="hlt">Ice</span> 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 <span class="hlt">ice</span> 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 <span class="hlt">ice</span> 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 <span class="hlt">ice</span> being removed and replaced with open water 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 <span class="hlt">ice</span> has been removed. An earlier study by Peng and Domros had also found a link between <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> and the East Asian monsoon circulation. The current project has helped to understand the teleconnection.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.G21B0875K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.G21B0875K"><span>Exploring the effect of East <span class="hlt">Antarctic</span> <span class="hlt">ice</span> mass loss on GIA-induced horizontal bedrock motions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Konfal, S. A.; Whitehouse, P. L.; Hermans, T.; van der Wal, W.; Wilson, T. J.; Bevis, M. G.; Kendrick, E. C.; Dalziel, I.; Smalley, R., Jr.</p> <p>2017-12-01</p> <p><span class="hlt">Ice</span> history inputs used in <span class="hlt">Antarctic</span> models of GIA include major centers of <span class="hlt">ice</span> mass loss in West Antarctica. In the Transantarctic Mountains (TAM) region spanning the boundary between East and West Antarctica, horizontal crustal motions derived from GPS observations from the <span class="hlt">Antarctic</span> Network (ANET) component of the Polar Earth Observing Network (POLENET) are towards these West <span class="hlt">Antarctic</span> <span class="hlt">ice</span> mass centers, opposite to the pattern of radial crustal motion expected in an unloading scenario. We investigate alternative <span class="hlt">ice</span> history and earth structure inputs to GIA models in an attempt to reproduce observed crustal motions in the region. The W12 <span class="hlt">ice</span> history model is altered to create scenarios including <span class="hlt">ice</span> unloading in the Wilkes Subglacial Basin based on available glaciological records. These altered <span class="hlt">ice</span> history models, along with the unmodified W12 <span class="hlt">ice</span> history model, are coupled with 60 radially varying (1D) earth model combinations, including approximations of optimal earth profiles identified in published GIA models. The resulting model-predicted motions utilizing both the modified and unmodified <span class="hlt">ice</span> history models fit ANET GPS-derived crustal motions in the northern TAM region for a suite of earth model combinations. Further south, where the influence of simulated Wilkes unloading is weakest and West <span class="hlt">Antarctic</span> unloading is strongest, observed and predicted motions do not agree. The influence of simulated Wilkes <span class="hlt">ice</span> unloading coupled with laterally heterogeneous earth models is also investigated. The resulting model-predicted motions do not differ significantly between the original W12 and W12 with simulated Wilkes unloading <span class="hlt">ice</span> histories.</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> <span class="hlt">ice</span> 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> <span class="hlt">ice</span> sheets to warming during the Last Glacial Termination (LGT; 18,000-11,650 yrs ago) allows us to disentangle <span class="hlt">ice</span>-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 <span class="hlt">ice</span>, atmospheric and marine records, making it difficult to assess relationships between <span class="hlt">Antarctic</span> <span class="hlt">ice</span>-sheet (AIS) dynamics, climate change and sea level. Here we present results from a highly-resolved 'horizontal <span class="hlt">ice</span> 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 <span class="hlt">ice</span>-sheet modelling suggests these contrasting trends were likely <span class="hlt">Antarctic</span>-wide, sustained by feedbacks amplified by the delivery of Circumpolar Deep Water 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/2018GMD....11.1257N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GMD....11.1257N"><span>Intercomparison of <span class="hlt">Antarctic</span> <span class="hlt">ice</span>-shelf, ocean, and sea-<span class="hlt">ice</span> interactions simulated by MetROMS-iceshelf and FESOM 1.4</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Naughten, Kaitlin A.; Meissner, Katrin J.; Galton-Fenzi, Benjamin K.; England, Matthew H.; Timmermann, Ralph; Hellmer, Hartmut H.; Hattermann, Tore; Debernard, Jens B.</p> <p>2018-04-01</p> <p>An increasing number of Southern Ocean models now include <span class="hlt">Antarctic</span> <span class="hlt">ice</span>-shelf cavities, and simulate thermodynamics at the <span class="hlt">ice</span>-shelf/ocean interface. This adds another level of complexity to Southern Ocean simulations, as <span class="hlt">ice</span> shelves interact directly with the ocean and indirectly with sea <span class="hlt">ice</span>. Here, we present the first model intercomparison and evaluation of present-day ocean/sea-<span class="hlt">ice/ice</span>-shelf interactions, as simulated by two models: a circumpolar <span class="hlt">Antarctic</span> configuration of MetROMS (ROMS: Regional Ocean Modelling System coupled to CICE: Community <span class="hlt">Ice</span> CodE) and the global model FESOM (Finite Element Sea-<span class="hlt">ice</span> Ocean Model), where the latter is run at two different levels of horizontal resolution. From a circumpolar <span class="hlt">Antarctic</span> perspective, we compare and evaluate simulated <span class="hlt">ice</span>-shelf basal melting and sub-<span class="hlt">ice</span>-shelf circulation, as well as sea-<span class="hlt">ice</span> properties and Southern Ocean water mass characteristics as they influence the sub-<span class="hlt">ice</span>-shelf processes. Despite their differing numerical methods, the two models produce broadly similar results and share similar biases in many cases. Both models reproduce many key features of observations but struggle to reproduce others, such as the high melt rates observed in the small warm-cavity <span class="hlt">ice</span> shelves of the Amundsen and Bellingshausen seas. Several differences in model design show a particular influence on the simulations. For example, FESOM's greater topographic smoothing can alter the geometry of some <span class="hlt">ice</span>-shelf cavities enough to affect their melt rates; this improves at higher resolution, since less smoothing is required. In the interior Southern Ocean, the vertical coordinate system affects the degree of water mass erosion due to spurious diapycnal mixing, with MetROMS' terrain-following coordinate leading to more erosion than FESOM's z coordinate. Finally, increased horizontal resolution in FESOM leads to higher basal melt rates for small <span class="hlt">ice</span> shelves, through a combination of stronger circulation and small-scale intrusions of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C34B..06P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C34B..06P"><span>An <span class="hlt">Antarctic</span> stratigraphic record of step-wise <span class="hlt">ice</span>-sheet growth through the Eocene-Oligocene transition</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Passchier, S.; Ciarletta, D. J.; Miriagos, T.; Bijl, P.; Bohaty, S. M.</p> <p>2016-12-01</p> <p>The <span class="hlt">Antarctic</span> cryosphere plays a critical role in the ocean-atmosphere system, but its early evolution is still poorly known. With a near-field record from Prydz Bay, Antarctica, we conclude that <span class="hlt">Antarctic</span> continental <span class="hlt">ice</span>-sheet growth commenced with the EOT-1 "precursor" glaciation, during a time of Subantarctic surface ocean cooling and a decline in atmospheric pCO2. Prydz Bay lies downstream of a major East <span class="hlt">Antarctic</span> <span class="hlt">ice</span>-sheet drainage system and the Gamburtsev Mountains, a likely nucleation point for the first <span class="hlt">ice</span> sheets. Its sedimentary records uniquely constrain the timing of <span class="hlt">ice</span>-sheet advance onto the continental shelf. We investigate a detrital record extracted from three Ocean Drilling Program drill holes in Prydz Bay within a new depositional and chronological framework spanning the late Eocene to early Oligocene ( 36-33 Ma). The chemical index of alteration (CIA) and the S-index, calculated from the major element geochemistry of bulk samples, yield estimates of chemical weathering intensities and mean annual temperature (MAT) on the East <span class="hlt">Antarctic</span> continent. We document evidence for late Eocene mountain glaciation along with transient warm events at 35.8-34.8 Ma. These data and our sedimentological analyses confirm the presence of ephemeral mountain glaciers on East Antarctica during the late Eocene between 35.9 and 34.4 Ma. Furthermore, we document the stepwise climate cooling of the <span class="hlt">Antarctic</span> hinterland from 34.4 Ma as the <span class="hlt">ice</span> sheet advanced towards the edges of the continent during EOT-1. The youngest part of our data set correlates to the time interval of the Oi-1 glaciation, when the <span class="hlt">ice</span>-sheet in Prydz Bay extended to the outer shelf. Cooling and <span class="hlt">ice</span> growth on Antarctica was spatially variable and <span class="hlt">ice</span> sheets formed under declining pCO2. These results point to complex <span class="hlt">ice</span> sheet - atmosphere - ocean - solid-earth feedbacks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFM.C53A..05S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFM.C53A..05S"><span>Discharge of New Subglacial <span class="hlt">Lake</span> on Whillians <span class="hlt">Ice</span> Stream: Implication for <span class="hlt">Ice</span> Stream Flow Dynamics.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sergienko, O. V.; Fricker, H. A.; Bindschadler, R. A.; Vornberger, P. L.; Macayeal, D. R.</p> <p>2006-12-01</p> <p>One of the surprise discoveries made possible by the ICESat laser altimeter mission of 2004-2006 is the presence of a large subglacial <span class="hlt">lake</span> below the grounding zone of Whillians <span class="hlt">Ice</span> Stream (dubbed here `<span class="hlt">Lake</span> Helen' after the discoverer, Helen Fricker). What is even more surprising is the fact that this <span class="hlt">lake</span> discharged a substantial portion of its volume during the ICESat mission, and changes in <span class="hlt">lake</span> volume and surface elevation of the <span class="hlt">ice</span> stream are documented in exquisite detail [Fricker et al., in press]. The presence and apparent dynamism of large subglacial <span class="hlt">lakes</span> in the grounding zone of a major <span class="hlt">ice</span> stream raises questions about their effects on <span class="hlt">ice</span>-stream dynamics. Being liquid and movable, water modifies basal friction spatially and temporally. Melting due to shear heating and geothermal flux reduces basal traction, making the <span class="hlt">ice</span> stream move fast. However, when water collects in a depression to form a <span class="hlt">lake</span>, it potentially deprives the surrounding bed of lubricating water, and additionally makes the <span class="hlt">ice</span> surface flat, thereby locally decreasing the <span class="hlt">ice</span> stream driving stress. We study the effect of formation and discharge of a subglacial <span class="hlt">lake</span> at the mouth of and <span class="hlt">ice</span> stream using a two dimensional, vertically integrated, <span class="hlt">ice</span>-stream model. The model is forced by the basal friction, <span class="hlt">ice</span> thickness and surface elevation. The basal friction is obtained by inversion of the <span class="hlt">ice</span> surface velocity, <span class="hlt">ice</span> thickness and surface elevation come from observations. To simulate the <span class="hlt">lake</span> formation we introduce zero basal friction and "inflate" the basal elevation of the <span class="hlt">ice</span> stream at the site of the <span class="hlt">lake</span>. Sensitivity studies of the response of the surrounding <span class="hlt">ice</span> stream and <span class="hlt">ice</span> shelf flow are performed to delineate the influence of near-grounding-line subglacial water storage for <span class="hlt">ice</span> streams in general.</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> <span class="hlt">Ice</span> Sheet (AIS), implying that there was an active subglacial hydrological system beneath the past AIS which influenced its <span class="hlt">ice</span> 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 <span class="hlt">ice</span>-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 <span class="hlt">lakes</span>, 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 <span class="hlt">lake</span> basins, including some 59 identified using submarine geomorphological evidence and numerical modelling calculations. Water is predicted to accumulate in the subglacial <span class="hlt">lakes</span> over centuries to millennia and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/11884754','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/11884754"><span><span class="hlt">Antarctic</span> krill under sea <span class="hlt">ice</span>: elevated abundance in a narrow band just south of <span class="hlt">ice</span> edge.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Brierley, Andrew S; Fernandes, Paul G; Brandon, Mark A; Armstrong, Frederick; Millard, Nicholas W; McPhail, Steven D; Stevenson, Peter; Pebody, Miles; Perrett, James; Squires, Mark; Bone, Douglas G; Griffiths, Gwyn</p> <p>2002-03-08</p> <p>We surveyed <span class="hlt">Antarctic</span> krill (Euphausia superba) under sea <span class="hlt">ice</span> using the autonomous underwater vehicle Autosub-2. Krill were concentrated within a band under <span class="hlt">ice</span> between 1 and 13 kilometers south of the <span class="hlt">ice</span> edge. Within this band, krill densities were fivefold greater than that of open water. The under-<span class="hlt">ice</span> environment has long been considered an important habitat for krill, but sampling difficulties have previously prevented direct observations under <span class="hlt">ice</span> over the scale necessary for robust krill density estimation. Autosub-2 enabled us to make continuous high-resolution measurements of krill density under <span class="hlt">ice</span> reaching 27 kilometers beyond the <span class="hlt">ice</span> edge.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C33B0800H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C33B0800H"><span>Landcover Mapping of the McMurdo <span class="hlt">Ice</span> Shelf Using Landsat and WorldView Image Data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hansen, E. K.; Macdonald, G.; Mayer, D. P.; MacAyeal, D. R.</p> <p>2016-12-01</p> <p><span class="hlt">Ice</span> shelves bound approximately half of the <span class="hlt">Antarctic</span> coast and act to buttress the glaciers that feed them. The collapse of the Larsen B <span class="hlt">Ice</span> Shelf on the <span class="hlt">Antarctic</span> Peninsula highlights the importance of processes at the surface for an <span class="hlt">ice</span> shelf's stability. The McMurdo <span class="hlt">Ice</span> Shelf is unique among <span class="hlt">Antarctic</span> <span class="hlt">ice</span> shelves in that it exists in a relatively warm climate zone and is thus more vulnerable to climate change than colder <span class="hlt">ice</span> shelves at similar latitudes. However, little is known quantitatively about the surface <span class="hlt">cover</span> types across the <span class="hlt">ice</span> shelf, impeding the study of its hydrology and of the origins of its features. In particular, no work has been done linking field observations of supraglacial channels to shelf-wide surface hydrology. We will present the first satellite-derived multiscale landcover map of the McMurdo <span class="hlt">Ice</span> Shelf based on Landsat 8 and WorldView-2 image data. Landcover types are extracted using supervised classification methods referenced to field observations. Landsat 8 provides coverage of the entire <span class="hlt">ice</span> shelf ( 5,000 km2) at 30 m/pixel, sufficient to distinguish glacial <span class="hlt">ice</span>, debris <span class="hlt">cover</span>, and large supraglacial <span class="hlt">lakes</span>. WorldView data <span class="hlt">cover</span> a smaller area— 300 km2 at 2 m/pixel—and thus allow detailed mapping of features that are not spatially resolved by Landsat, such as supraglacial channels and small fractures across the <span class="hlt">ice</span> shelf's surface. We take advantage of the higher resolution of WorldView-2 data to calculate the area of mid-summer surface water in channels and melt ponds within a detailed study area and use this as the basis for a spectral mixture model in order to estimate the total surface water area across the <span class="hlt">ice</span> shelf. We intend to use the maps to guide strategic planning of future field research into the seasonal surface hydrology and climate stability of the McMurdo <span class="hlt">Ice</span> Shelf.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70176362','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70176362"><span>The study of fresh-water <span class="hlt">lake</span> <span class="hlt">ice</span> using multiplexed imaging radar</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Leonard, Bryan M.; Larson, R.W.</p> <p>1975-01-01</p> <p>The study of <span class="hlt">ice</span> in the upper Great <span class="hlt">Lakes</span>, both from the operational and the scientific points of view, is receiving continued attention. Quantitative and qualitative field work is being conducted to provide the needed background for accurate interpretation of remotely sensed data. The data under discussion in this paper were obtained by a side-looking multiplexed airborne radar (SLAR) supplemented with ground-truth data.Because of its ability to penetrate adverse weather, radar is an especially important instrument for monitoring <span class="hlt">ice</span> in the upper Great <span class="hlt">Lakes</span>. It has previously been shown that imaging radars can provide maps of <span class="hlt">ice</span> <span class="hlt">cover</span> in these areas. However, questions concerning both the nature of the surfaces reflecting radar energy and the interpretation of the radar imagery continually arise.Our analysis of <span class="hlt">ice</span> in Whitefish Bay (<span class="hlt">Lake</span> Superior) indicates that the combination of the <span class="hlt">ice</span>/water interlace and the <span class="hlt">ice</span>/air interface is the major contributor to the radar backscatter as seen on the imagery At these frequencies the <span class="hlt">ice</span> has a very low relative dielectric permittivity (< 3.0) and a low loss tangent Thus, this <span class="hlt">ice</span> is somewhat transparent to the energy used by the imaging SLAR system. The <span class="hlt">ice</span> types studied include newly formed black <span class="hlt">ice</span>, pancake <span class="hlt">ice</span>, and frozen and consolidated pack and brash <span class="hlt">ice</span>.Although <span class="hlt">ice</span> thickness cannot be measured directly from the received signals, it is suspected that by combining the information pertaining to radar backscatter with data on the meteorological and sea-state history of the area, together with some basic ground truth, better estimates of the <span class="hlt">ice</span> thickness may be provided. In addition, certain <span class="hlt">ice</span> features (e.g. ridges, <span class="hlt">ice</span>-foot formation, areas of brash <span class="hlt">ice</span>) may be identified with reasonable confidence. There is a continued need for additional ground work to verify the validity of imaging radars for these types of interpretations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1714074E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1714074E"><span>Observationally constrained projections of <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet instability</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Edwards, Tamsin; Ritz, Catherine; Durand, Gael; Payne, Anthony; Peyaud, Vincent; Hindmarsh, Richard</p> <p>2015-04-01</p> <p>Large parts of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet lie on bedrock below sea level and may be vulnerable to a positive feedback known as Marine <span class="hlt">Ice</span> Sheet Instability (MISI), a self-sustaining retreat of the grounding line triggered by oceanic or atmospheric changes. There is growing evidence MISI may be underway throughout the Amundsen Sea Embayment (ASE) of West Antarctica, induced by circulation of warm Circumpolar Deep Water. If this retreat is sustained the region could contribute up to 1-2 m to global mean sea level, and if triggered in other areas the potential contribution to sea level on centennial to millennial timescales could be two to three times greater. However, physically plausible projections of <span class="hlt">Antarctic</span> MISI are challenging: numerical <span class="hlt">ice</span> sheet models are too low in spatial resolution to resolve grounding line processes or else too computationally expensive to assess modelling uncertainties, and no dynamical models exist of the ocean-atmosphere-<span class="hlt">ice</span> sheet system. Furthermore, previous numerical <span class="hlt">ice</span> sheet model projections for Antarctica have not been calibrated with observations, which can reduce uncertainties. Here we estimate the probability of dynamic mass loss in the event of MISI under a medium climate scenario, assessing 16 modelling uncertainties and calibrating the projections with observed mass losses in the ASE from 1992-2011. We project losses of up to 30 cm sea level equivalent (SLE) by 2100 and 72 cm SLE by 2200 (95% credibility interval: CI). Our results are substantially lower than previous estimates. The ASE sustains substantial losses, 83% of the continental total by 2100 and 67% by 2200 (95% CI), but in other regions losses are limited by <span class="hlt">ice</span> dynamical theory, observations, or a lack of projected triggers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70032042','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70032042"><span><span class="hlt">Ice-walled-lake</span> plains: Implications for the origin of hummocky glacial topography in middle North America</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Clayton, L.; Attig, J.W.; Ham, N.R.; Johnson, M.D.; Jennings, C.E.; Syverson, K.M.</p> <p>2008-01-01</p> <p><span class="hlt">Ice-walled-lake</span> plains are prominent in many areas of hummocky-till topography left behind as the Laurentide <span class="hlt">Ice</span> Sheet melted from middle North America. The formation of the hummocky-till topography has been explained by: (1) erosion by subglacial floods; (2) squeezing of subglacial till up into holes in stagnant glacial <span class="hlt">ice</span>; or (3) slumping of supraglacial till. The geomorphology and stratigraphy of <span class="hlt">ice-walled-lake</span> plains provide evidence that neither the <span class="hlt">lake</span> plains nor the adjacent hummocks are of subglacial origin. These flat <span class="hlt">lake</span> plains, up to a few kilometers in diameter, are perched as much as a few tens of meters above surrounding depressions. They typically are underlain by laminated, fine-grained suspended-load <span class="hlt">lake</span> sediment. Many <span class="hlt">ice-walled-lake</span> plains are surrounded by a low rim ridge of coarser-grained shore sediment or by a steeper rim ridge of debris that slumped off the surrounding <span class="hlt">ice</span> slopes. The <span class="hlt">ice</span>-walled <span class="hlt">lakes</span> persisted for hundreds to thousands of years following glacial stagnation. Shells of aquatic molluscs from several deposits of <span class="hlt">ice-walled-lake</span> sediment in south-central North Dakota have been dated from about 13 500 to 10 500??B.P. (calibrated radiocarbon ages), indicating a climate only slightly cooler than present. This is confirmed by recent palaeoecological studies in nearby non-glacial sites. To survive so long, the stagnant glacial <span class="hlt">ice</span> had to be well-insulated by a thick <span class="hlt">cover</span> of supraglacial sediment, and the associated till hummocks must be composed primarily of collapsed supraglacial till. ?? 2007 Elsevier B.V. All rights reserved.</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> <span class="hlt">Ice</span> 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> <span class="hlt">Ice</span> Sheet (WAIS) may affect future global sea-level changes. Alley and Whillans note that 'the water 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> <span class="hlt">ice</span> 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 <span class="hlt">ice</span> 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 <span class="hlt">ice</span> streams.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3997805','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3997805"><span>Marine <span class="hlt">ice</span> regulates the future stability of a large <span class="hlt">Antarctic</span> <span class="hlt">ice</span> 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>Kulessa, Bernd; Jansen, Daniela; Luckman, Adrian J.; King, Edward C.; Sammonds, Peter R.</p> <p>2014-01-01</p> <p>The collapses of the Larsen A and B <span class="hlt">ice</span> shelves on the <span class="hlt">Antarctic</span> Peninsula in 1995 and 2002 confirm the impact of southward-propagating climate warming in this region. Recent mass and dynamic changes of Larsen B’s southern neighbour Larsen C, the fourth largest <span class="hlt">ice</span> shelf in Antarctica, may herald a similar instability. Here, using a validated <span class="hlt">ice</span>-shelf model run in diagnostic mode, constrained by satellite and in situ geophysical data, we identify the nature of this potential instability. We demonstrate that the present-day spatial distribution and orientation of the principal stresses within Larsen C <span class="hlt">ice</span> shelf are akin to those within pre-collapse Larsen B. When Larsen B’s stabilizing frontal portion was lost in 1995, the unstable remaining shelf accelerated, crumbled and ultimately collapsed. We hypothesize that Larsen C <span class="hlt">ice</span> shelf may suffer a similar fate if it were not stabilized by warm and mechanically soft marine <span class="hlt">ice</span>, entrained within narrow suture zones. PMID:24751641</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29540750','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29540750"><span>Recent high-resolution <span class="hlt">Antarctic</span> <span class="hlt">ice</span> velocity maps reveal increased mass loss in Wilkes Land, East Antarctica.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Shen, Qiang; Wang, Hansheng; Shum, C K; Jiang, Liming; Hsu, Hou Tse; Dong, Jinglong</p> <p>2018-03-14</p> <p>We constructed <span class="hlt">Antarctic</span> <span class="hlt">ice</span> velocity maps from Landsat 8 images for the years 2014 and 2015 at a high spatial resolution (100 m). These maps were assembled from 10,690 scenes of displacement vectors inferred from more than 10,000 optical images acquired from December 2013 through March 2016. We estimated the mass discharge of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet in 2008, 2014, and 2015 using the Landsat <span class="hlt">ice</span> velocity maps, interferometric synthetic aperture radar (InSAR)-derived <span class="hlt">ice</span> velocity maps (~2008) available from prior studies, and <span class="hlt">ice</span> thickness data. An increased mass discharge (53 ± 14 Gt yr -1 ) was found in the East Indian Ocean sector since 2008 due to unexpected widespread glacial acceleration in Wilkes Land, East Antarctica, while the other five oceanic sectors did not exhibit significant changes. However, present-day increased mass loss was found by previous studies predominantly in west Antarctica and the <span class="hlt">Antarctic</span> Peninsula. The newly discovered increased mass loss in Wilkes Land suggests that the ocean heat flux may already be influencing <span class="hlt">ice</span> dynamics in the marine-based sector of the East <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet (EAIS). The marine-based sector could be adversely impacted by ongoing warming in the Southern Ocean, and this process may be conducive to destabilization.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFM.C12A..01A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFM.C12A..01A"><span>Turbulent Surface Flux Measurements over Snow-<span class="hlt">Covered</span> Sea <span class="hlt">Ice</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Andreas, E. L.; Fairall, C. W.; Grachev, A. A.; Guest, P. S.; Jordan, R. E.; Persson, P. G.</p> <p>2006-12-01</p> <p>Our group has used eddy correlation to make over 10,000 hours of measurements of the turbulent momentum and heat fluxes over snow-<span class="hlt">covered</span> sea <span class="hlt">ice</span> in both the Arctic and the <span class="hlt">Antarctic</span>. Polar sea <span class="hlt">ice</span> is an ideal site for studying fundamental processes for turbulent exchange over snow. Both our Arctic and <span class="hlt">Antarctic</span> sites---in the Beaufort Gyre and deep into the Weddell Sea, respectively---were expansive, flat areas with continuous snow <span class="hlt">cover</span>; and both were at least 300 km from any topography that might have complicated the atmospheric flow. In this presentation, we will review our measurements of the turbulent fluxes of momentum and sensible and latent heat. In particular, we will describe our experiences making turbulence instruments work in the fairly harsh polar, marine boundary layer. For instance, several of our Arctic sites were remote from our main camp and ran unattended for a week at a time. Besides simply making flux measurements, we have been using the data to develop a bulk flux algorithm and to study fundamental turbulence processes in the atmospheric surface layer. The bulk flux algorithm predicts the turbulent surface fluxes from mean meteorological quantities and, thus, will find use in data analyses and models. For example, components of the algorithm are already embedded in our one- dimensional mass and energy budget model SNTHERM. Our fundamental turbulence studies have included deducing new scaling regimes in the stable boundary layer; examining the Monin-Obukhov similarity functions, especially in stable stratification; and evaluating the von Kármán constant with the largest atmospheric data set ever applied to such a study. During this presentation, we will highlight some of this work.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_18 --> <div id="page_19" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="361"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19776741','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19776741"><span>Extensive dynamic thinning on the margins of the Greenland and <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheets.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Pritchard, Hamish D; Arthern, Robert J; Vaughan, David G; Edwards, Laura A</p> <p>2009-10-15</p> <p>Many glaciers along the margins of the Greenland and <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheets are accelerating and, for this reason, contribute increasingly to global sea-level rise. Globally, <span class="hlt">ice</span> losses contribute approximately 1.8 mm yr(-1) (ref. 8), but this could increase if the retreat of <span class="hlt">ice</span> shelves and tidewater glaciers further enhances the loss of grounded <span class="hlt">ice</span> or initiates the large-scale collapse of vulnerable parts of the <span class="hlt">ice</span> sheets. <span class="hlt">Ice</span> loss as a result of accelerated flow, known as dynamic thinning, is so poorly understood that its potential contribution to sea level over the twenty-first century remains unpredictable. Thinning on the <span class="hlt">ice</span>-sheet scale has been monitored by using repeat satellite altimetry observations to track small changes in surface elevation, but previous sensors could not resolve most fast-flowing coastal glaciers. Here we report the use of high-resolution ICESat (<span class="hlt">Ice</span>, Cloud and land Elevation Satellite) laser altimetry to map change along the entire grounded margins of the Greenland and <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheets. To isolate the dynamic signal, we compare rates of elevation change from both fast-flowing and slow-flowing <span class="hlt">ice</span> with those expected from surface mass-balance fluctuations. We find that dynamic thinning of glaciers now reaches all latitudes in Greenland, has intensified on key <span class="hlt">Antarctic</span> grounding lines, has endured for decades after <span class="hlt">ice</span>-shelf collapse, penetrates far into the interior of each <span class="hlt">ice</span> sheet and is spreading as <span class="hlt">ice</span> shelves thin by ocean-driven melt. In Greenland, glaciers flowing faster than 100 m yr(-1) thinned at an average rate of 0.84 m yr(-1), and in the Amundsen Sea embayment of Antarctica, thinning exceeded 9.0 m yr(-1) for some glaciers. Our results show that the most profound changes in the <span class="hlt">ice</span> sheets currently result from glacier dynamics at ocean margins.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.2609S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.2609S"><span>Combined <span class="hlt">ice</span> core and climate-model evidence for the collapse of the West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet during Marine Isotope Stage 5e.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Steig, Eric J.; Huybers, Kathleen; Singh, Hansi A.; Steiger, Nathan J.; Frierson, Dargan M. W.; Popp, Trevor; White, James W. C.</p> <p>2015-04-01</p> <p>It has been speculated that collapse of the West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet explains the very high eustatic sea level rise during the last interglacial period, marine isotope stage (MIS) 5e, but the evidence remains equivocal. Changes in atmospheric circulation resulting from a collapse of the West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet (WAIS) would have significant regional impacts that should be detectable in <span class="hlt">ice</span> core records. We conducted simulations using general circulation models (GCMs) at varying levels of complexity: a gray-radiation aquaplanet moist GCM (GRaM), the slab ocean version of GFDL-AM2 (also as an aquaplanet), and the fully-coupled version of NCAR's CESM with realistic topography. In all the experiments, decreased elevation from the removal of the WAIS leads to greater cyclonic circulation over the West <span class="hlt">Antarctic</span> region. This creates increased advection of relatively warm marine air from the Amundsen-Bellingshausen Seas towards the South Pole, and increased cold-air advection from the East <span class="hlt">Antarctic</span> plateau towards the Ross Sea and coastal Marie Byrd Land. The result is anomalous warming in some areas of the East <span class="hlt">Antarctic</span> interior, and significant cooling in Marie Byrd Land. Comparison of <span class="hlt">ice</span> core records shows good agreement with the model predictions. In particular, isotope-paleotemperature records from <span class="hlt">ice</span> cores in East Antarctica warmed more between the previous glacial period (MIS 6) and MIS 5e than coastal Marie Byrd Land. These results add substantial support to other evidence for WAIS collapse during the last interglacial period.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23185006','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23185006"><span>Microbial life at -13 °C in the brine of an <span class="hlt">ice</span>-sealed <span class="hlt">Antarctic</span> <span class="hlt">lake</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Murray, Alison E; Kenig, Fabien; Fritsen, Christian H; McKay, Christopher P; Cawley, Kaelin M; Edwards, Ross; Kuhn, Emanuele; McKnight, Diane M; Ostrom, Nathaniel E; Peng, Vivian; Ponce, Adrian; Priscu, John C; Samarkin, Vladimir; Townsend, Ashley T; Wagh, Protima; Young, Seth A; Yung, Pung To; Doran, Peter T</p> <p>2012-12-11</p> <p>The permanent <span class="hlt">ice</span> <span class="hlt">cover</span> of <span class="hlt">Lake</span> Vida (Antarctica) encapsulates an extreme cryogenic brine ecosystem (-13 °C; salinity, 200). This aphotic ecosystem is anoxic and consists of a slightly acidic (pH 6.2) sodium chloride-dominated brine. Expeditions in 2005 and 2010 were conducted to investigate the biogeochemistry of <span class="hlt">Lake</span> Vida's brine system. A phylogenetically diverse and metabolically active Bacteria dominated microbial assemblage was observed in the brine. These bacteria live under very high levels of reduced metals, ammonia, molecular hydrogen (H(2)), and dissolved organic carbon, as well as high concentrations of oxidized species of nitrogen (i.e., supersaturated nitrous oxide and ∼1 mmol⋅L(-1) nitrate) and sulfur (as sulfate). The existence of this system, with active biota, and a suite of reduced as well as oxidized compounds, is unusual given the millennial scale of its isolation from external sources of energy. The geochemistry of the brine suggests that abiotic brine-rock reactions may occur in this system and that the rich sources of dissolved electron acceptors prevent sulfate reduction and methanogenesis from being energetically favorable. The discovery of this ecosystem and the in situ biotic and abiotic processes occurring at low temperature provides a tractable system to study habitability of isolated terrestrial cryoenvironments (e.g., permafrost cryopegs and subglacial ecosystems), and is a potential analog for habitats on other icy worlds where water-rock reactions may cooccur with saline deposits and subsurface oceans.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19970006984','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19970006984"><span><span class="hlt">Ice</span> Processes and Growth History on Arctic and Sub-Arctic <span class="hlt">Lakes</span> Using ERS-1 SAR Data</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Morris, K.; Jeffries, M. O.; Weeks, W. F.</p> <p>1995-01-01</p> <p>A survey of <span class="hlt">ice</span> growth and decay processes on a selection of shallow and deep sub-Arctic and Arctic <span class="hlt">lakes</span> was conducted using radiometrically calibrated ERS-1 SAR images. Time series of radar backscatter data were compiled for selected sites on the <span class="hlt">lakes</span> during the period ot <span class="hlt">ice</span> <span class="hlt">cover</span> (September to June) for the years 1991-1992 and 1992-1993. A variety of <span class="hlt">lake-ice</span> processes could be observed, and significant changes in backscatter occurred from the time of initial <span class="hlt">ice</span> formation in autumn until the onset of the spring thaw. Backscatter also varied according to the location and depth of the <span class="hlt">lakes</span>. The spatial and temporal changes in backscatter were most constant and predictable at the shallow <span class="hlt">lakes</span> on the North Slope of Alaska. As a consequence, they represent the most promising sites for long-term monitoring and the detection of changes related to global warming and its effects on the polar regions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1394397','SCIGOV-DOEDE'); return false;" href="https://www.osti.gov/servlets/purl/1394397"><span>Historic CH4 Records from <span class="hlt">Antarctic</span> and Greenland <span class="hlt">Ice</span> Cores, <span class="hlt">Antarctic</span> Firn Data, and Archived Air Samples from Cape Grim, Tasmania</span></a></p> <p><a target="_blank" href="http://www.osti.gov/dataexplorer">DOE Data Explorer</a></p> <p>Etheridge, D. M. [Division of Atmospheric Research, CSIRO, Aspendale, Victoria, Australia; Steele, L. P. [Division of Atmospheric Research, CSIRO, Aspendale, Victoria, Australia; Francey, R. J. [Division of Atmospheric Research, CSIRO, Aspendale, Victoria, Australia; Langenfelds, R. L. [Division of Atmospheric Research, CSIRO, Aspendale, Victoria, Australia</p> <p>2002-01-01</p> <p>The <span class="hlt">Antarctic</span> CH4 records presented here are derived from three <span class="hlt">ice</span> cores obtained at Law Dome, East Antarctica (66°44'S, 112°50'E, 1390 meters above mean sea level). Law Dome has many qualities of an ideal <span class="hlt">ice</span> core site for the reconstruction of past concentrations of atmospheric gases; these qualities include: negligible melting of the <span class="hlt">ice</span> sheet surface, low concentrations of impurities, regular stratigraphic layering undisturbed by wind stress at the surface or differential <span class="hlt">ice</span> flow at depth, and a high snow accumulation rate. Further details on the site, drilling, and cores are provided by Etheridge et al. (1998), Etheridge et al. (1996), Etheridge and Wookey (1989), and Morgan et al. (1997). The two Greenland <span class="hlt">ice</span> cores are from the Summit region (72°34' N, 37°37' W, 3200 meters above mean sea level). Lower snow accumulation rate there results in lower air-age resolution, and measurements presented here <span class="hlt">cover</span> only the pre-industrial period (until 1885). More details about these measurements are presented in Etheridge et al. (1998). Additionally, this site contains firn data from Core DE08-2, and archived air samples from Cape Grim, Tasmania, for comparison.</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> <span class="hlt">ice</span> 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> <span class="hlt">ice</span> 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 <span class="hlt">ice</span> extent, large-scale atmospheric circulation and near-surface climate, but fails to simulate the recent expansion of <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span>. The present-day <span class="hlt">Antarctic</span> <span class="hlt">ice</span> 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> <span class="hlt">ice</span> 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 <span class="hlt">ice</span> 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 water content.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1811140D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1811140D"><span>Towards automated mapping of <span class="hlt">lake</span> <span class="hlt">ice</span> using RADARSAT-2 and simulated RCM compact polarimetric data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Duguay, Claude</p> <p>2016-04-01</p> <p>The Canadian <span class="hlt">Ice</span> Service (CIS) produces a weekly <span class="hlt">ice</span> fraction product (a text file with a single <span class="hlt">lake</span>-wide <span class="hlt">ice</span> fraction value, in tenth, estimated for about 140 large <span class="hlt">lakes</span> across Canada and northern United States) created from the visual interpretation of RADARSAT-2 ScanSAR dual-polarization (HH and HV) imagery, complemented by optical satellite imagery (AVHRR, MODIS and VIIRS). The weekly <span class="hlt">ice</span> product is generated in support of the Canadian Meteorological Centre (CMC) needs for <span class="hlt">lake</span> <span class="hlt">ice</span> coverage in their operational numerical weather prediction model. CIS is interested in moving from its current (manual) way of generating the <span class="hlt">ice</span> fraction product to a largely automated process. With support from the Canadian Space Agency, a project was recently initiated to assess the potential of polarimetric SAR data for <span class="hlt">lake</span> <span class="hlt">ice</span> <span class="hlt">cover</span> mapping in light of the upcoming RADARSAT Constellation Mission (to be launched in 2018). The main objectives of the project are to evaluate: 1) state-of-the-art image segmentation algorithms and 2) RADARSAT-2 polarimetric and simulated RADARSAT Constellation Mission (RCM) compact polarimetric SAR data for <span class="hlt">ice</span>/open water discrimination. The goal is to identify the best segmentation algorithm and non-polarimetric/polarimetric parameters for automated <span class="hlt">lake</span> <span class="hlt">ice</span> monitoring at CIS. In this talk, we will present the background and context of the study as well as initial results from the analysis of RADARSAT-2 Standard Quad-Pol data acquired during the break-up and freeze-up periods of 2015 on Great Bear <span class="hlt">Lake</span>, Northwest Territories.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.P43C2902L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.P43C2902L"><span>What's Cooler Than Being Cool? Icefin: Robotic Exploration Beneath <span class="hlt">Antarctic</span> <span class="hlt">Ice</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>Lawrence, J.; Schmidt, B. E.; Meister, M. R.; Glass, J. B.; Bowman, J. S.; Stockton, A. M.; Dichek, D.; Hurwitz, B.; Ramey, C.; Spears, A.; Walker, C. C.</p> <p>2017-12-01</p> <p>The 2017-18 <span class="hlt">Antarctic</span> field season marks the first of three under the RISEUP project (Ross <span class="hlt">Ice</span> Shelf & Europa Underwater Probe, NASA PSTAR program grant NNX16AL07G, PI B. E. Schmidt). RISEUP expands our efforts to understand the physical processes governing <span class="hlt">ice</span>-ocean interactions from beneath the McMurdo <span class="hlt">Ice</span> Shelf (MIS) to the Ross <span class="hlt">Ice</span> Shelf (RIS), utilizing the modular autonomous or remotely operable submersible vehicle (AUV/ROV) Icefin. The remote, aphotic regions below <span class="hlt">Antarctic</span> shelves present a unique opportunity- they are both poorly understood terrestrial environments and analogs for similar systems hypothesized to be present on other bodies in our solar system, such as Europa and Enceladus. By developing new robotic technologies to access and explore <span class="hlt">ice</span> shelf cavities we are advancing our understanding of how temperature, pressure, and salinity influence the <span class="hlt">ice</span>-ocean interface, the limits of habitable environments on Earth, and what biological processes and adaptations enable the life discovered by the RISP and WISSARD programs during initial exploration beneath the RIS. These investigations further our understanding of ocean world habitability and support planned and proposed planetary missions (e.g. Europa Clipper, Europa Lander) via improved constraint of marine <span class="hlt">ice</span> accretion processes, organic entrainment, and interface habitability. Custom built at Georgia Tech and first deployed during the 2014/15 <span class="hlt">Antarctic</span> season, Icefin is 3.5 m, 125 kg modular vehicle that now carries a full suite of oceanographic sensors (including conductivity, temperature, depth, dissolved O2, dissolved organic matter, turbidity, pH, eH, and sonar) that can be deployed through boreholes as small as 25 cm in diameter. Here we present continued analysis of basal <span class="hlt">ice</span> and oceanographic observations in the McMurdo Sound region from 2012-2015 with, pending anticipated field work, comparisons to preliminary data from the 2017/18 field season beneath both the McMurdo and Ross <span class="hlt">Ice</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930055825&hterms=algae&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dalgae','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930055825&hterms=algae&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dalgae"><span>Bromoalkane production by <span class="hlt">Antarctic</span> <span class="hlt">ice</span> algae</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sturges, W. T.; Sullivan, C. W.; Schnell, R. C.; Heidt, L. E.; Pollock, W. H.</p> <p>1993-01-01</p> <p><span class="hlt">Ice</span> microalgae, collected from the underside of annual sea <span class="hlt">ice</span> in McMurdo Sound, Antarctica, were found to contain and release to seawater a number of brominated hydrocarbons. These included bromoform, dibromomethane, mixed bromochloromethanes, and methyl bromide. Atmospheric measurements in the McMurdo Sound vicinity revealed the presence of bromoform and methyl bromide in the lower atmosphere, with lowest concentrations inland, further indicating that biogenic activity in the Sound is a source of organic bromine gases to the <span class="hlt">Antarctic</span> atmosphere. This may have important implications for boundary layer chemistry in Antarctica. In the Arctic, the presence of bromoform has been linked to loss of surface ozone in the spring. We report here preliminary evidence for similar surface ozone loss at McMurdo Station.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26667906','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26667906"><span>Microbiology: lessons from a first attempt at <span class="hlt">Lake</span> Ellsworth.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Pearce, D A; Magiopoulos, I; Mowlem, M; Tranter, M; Holt, G; Woodward, J; Siegert, M J</p> <p>2016-01-28</p> <p>During the attempt to directly access, measure and sample Subglacial <span class="hlt">Lake</span> Ellsworth in 2012-2013, we conducted microbiological analyses of the drilling equipment, scientific instrumentation, field camp and natural surroundings. From these studies, a number of lessons can be learned about the cleanliness of deep <span class="hlt">Antarctic</span> subglacial <span class="hlt">lake</span> access leading to, in particular, knowledge of the limitations of some of the most basic relevant microbiological principles. Here, we focus on five of the core challenges faced and describe how cleanliness and sterilization were implemented in the field. In the light of our field experiences, we consider how effective these actions were, and what can be learnt for future subglacial exploration missions. The five areas <span class="hlt">covered</span> are: (i) field camp environment and activities, (ii) the engineering processes surrounding the hot water drilling, (iii) sample handling, including recovery, stability and preservation, (iv) clean access methodologies and removal of sample material, and (v) the biodiversity and distribution of bacteria around the <span class="hlt">Antarctic</span>. Comparisons are made between the microbiology of the <span class="hlt">Lake</span> Ellsworth field site and other <span class="hlt">Antarctic</span> systems, including the <span class="hlt">lakes</span> on Signy Island, and on the <span class="hlt">Antarctic</span> Peninsula at <span class="hlt">Lake</span> Hodgson. Ongoing research to better define and characterize the behaviour of natural and introduced microbial populations in response to deep-<span class="hlt">ice</span> drilling is also discussed. We recommend that future access programmes: (i) assess each specific local environment in enhanced detail due to the potential for local contamination, (ii) consider the sterility of the access in more detail, specifically focusing on single cell colonization and the introduction of new species through contamination of pre-existing microbial communities, (iii) consider experimental bias in methodological approaches, (iv) undertake in situ biodiversity detection to mitigate risk of non-sample return and post-sample contamination, and (v</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20080045469&hterms=conversion+rate&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dconversion%2Brate%2527','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20080045469&hterms=conversion+rate&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dconversion%2Brate%2527"><span><span class="hlt">Antarctic</span> Sea <span class="hlt">Ice</span> Thickness and Snow-to-<span class="hlt">Ice</span> Conversion from Atmospheric Reanalysis and Passive Microwave Snow Depth</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Markus, Thorsten; Maksym, Ted</p> <p>2007-01-01</p> <p>Passive microwave snow depth, <span class="hlt">ice</span> concentration, and <span class="hlt">ice</span> motion estimates are combined with snowfall from the European Centre for Medium Range Weather Forecasting (ECMWF) reanalysis (ERA-40) from 1979-200 1 to estimate the prevalence of snow-to-<span class="hlt">ice</span> conversion (snow-<span class="hlt">ice</span> formation) on level sea <span class="hlt">ice</span> in the <span class="hlt">Antarctic</span> for April-October. Snow <span class="hlt">ice</span> is ubiquitous in all regions throughout the growth season. Calculated snow- <span class="hlt">ice</span> thicknesses fall within the range of estimates from <span class="hlt">ice</span> core analysis for most regions. However, uncertainties in both this analysis and in situ data limit the usefulness of snow depth and snow-<span class="hlt">ice</span> production to evaluate the accuracy of ERA-40 snowfall. The East <span class="hlt">Antarctic</span> is an exception, where calculated snow-<span class="hlt">ice</span> production exceeds observed <span class="hlt">ice</span> thickness over wide areas, suggesting that ERA-40 precipitation is too high there. Snow-<span class="hlt">ice</span> thickness variability is strongly controlled not just by snow accumulation rates, but also by <span class="hlt">ice</span> divergence. Surprisingly, snow-<span class="hlt">ice</span> production is largely independent of snow depth, indicating that the latter may be a poor indicator of total snow accumulation. Using the presence of snow-<span class="hlt">ice</span> formation as a proxy indicator for near-zero freeboard, we examine the possibility of estimating level <span class="hlt">ice</span> thickness from satellite snow depths. A best estimate for the mean level <span class="hlt">ice</span> thickness in September is 53 cm, comparing well with 51 cm from ship-based observations. The error is estimated to be 10-20 cm, which is similar to the observed interannual and regional variability. Nevertheless, this is comparable to expected errors for <span class="hlt">ice</span> thickness determined by satellite altimeters. Improvement in satellite snow depth retrievals would benefit both of these methods.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012TCD.....6.5225G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012TCD.....6.5225G"><span>A balanced water layer concept for subglacial hydrology in large scale <span class="hlt">ice</span> sheet models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Goeller, S.; Thoma, M.; Grosfeld, K.; Miller, H.</p> <p>2012-12-01</p> <p>There is currently no doubt about the existence of a wide-spread hydrological network under the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet, which lubricates the <span class="hlt">ice</span> base and thus leads to increased <span class="hlt">ice</span> velocities. Consequently, <span class="hlt">ice</span> models should incorporate basal hydrology to obtain meaningful results for future <span class="hlt">ice</span> dynamics and their contribution to global sea level rise. Here, we introduce the balanced water layer concept, <span class="hlt">covering</span> two prominent subglacial hydrological features for <span class="hlt">ice</span> sheet modeling on a continental scale: the evolution of subglacial <span class="hlt">lakes</span> and balance water fluxes. We couple it to the thermomechanical <span class="hlt">ice</span>-flow model RIMBAY and apply it to a synthetic model domain inspired by the Gamburtsev Mountains, Antarctica. In our experiments we demonstrate the dynamic generation of subglacial <span class="hlt">lakes</span> and their impact on the velocity field of the overlaying <span class="hlt">ice</span> sheet, resulting in a negative <span class="hlt">ice</span> mass balance. Furthermore, we introduce an elementary parametrization of the water flux-basal sliding coupling and reveal the predominance of the <span class="hlt">ice</span> loss through the resulting <span class="hlt">ice</span> streams against the stabilizing influence of less hydrologically active areas. We point out, that established balance flux schemes quantify these effects only partially as their ability to store subglacial water is lacking.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.5977S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.5977S"><span>Trends in <span class="hlt">ice</span> formation at <span class="hlt">Lake</span> Neusiedl since 1931 and large-scale oscillation patterns</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Soja, Anna-Maria; Maracek, Karl; Soja, Gerhard</p> <p>2013-04-01</p> <p><span class="hlt">Ice</span> formation at <span class="hlt">Lake</span> Neusiedl (Neusiedler See, Fertitó), a shallow steppe <span class="hlt">lake</span> (area 320 km2, mean depth 1.2 m) at the border of Austria/Hungary, is of ecological and economic importance. <span class="hlt">Ice</span> sailing and skating help to keep a touristic off-season alive. Reed harvest to maintain the ecological function of the reed belt (178 km2) is facilitated when <span class="hlt">lake</span> surface is frozen. Changes in <span class="hlt">ice</span> formation were analysed in the frame of the EULAKES-project (European <span class="hlt">Lakes</span> under Environmental Stressors, www.eulakes.eu), financed by the Central Europe Programme of the EU. Data records of <span class="hlt">ice</span>-on, <span class="hlt">ice</span> duration and <span class="hlt">ice</span>-off at <span class="hlt">Lake</span> Neusiedl starting with the year 1931, and air temperature (nearby monitoring station Eisenstadt - Sopron (HISTALP database and ZAMG)) were used to investigate nearly 80 winters. Additionally, influences of 8 teleconnection patterns, i.e. the Atlantic Multidecadal Oscillation (AMO), the East Atlantic pattern (EAP), the East Atlantic/West Russia pattern (EA/WR), the Eastern Mediterranean Pattern (EMP), the Mediterranean Oscillation (MO) for Algiers and Cairo, and for Israel and Gibraltar, resp., the North Atlantic Oscillation (NAO) and the Scandinavia pattern (SCA) were assessed. <span class="hlt">Ice</span> <span class="hlt">cover</span> of <span class="hlt">Lake</span> Neusiedl showed a high variability between the years (mean duration 71±27 days). Significant trends for later <span class="hlt">ice</span>-on (p=0.02), shorter <span class="hlt">ice</span> duration (p=0.07) and earlier <span class="hlt">ice</span>-off (p=0.02) for the period 1931-2011 were found by regression analysis and trend analysis tests. On an average, freezing of <span class="hlt">Lake</span> Neusiedl started 2 days later per decade and <span class="hlt">ice</span> melting began 2 days earlier per decade. Close relationships between mean air temperature and <span class="hlt">ice</span> formation could be found: <span class="hlt">ice</span>-on showed a dependency on summer (R=+0.28) and autumn air temperatures (R=+0.51), <span class="hlt">ice</span> duration and <span class="hlt">ice</span> off was related to autumn (R=-0.36 and -0.24), winter (R=-0.73 and -0.61) and concurrent spring air temperatures (R=-0.44). Increases of air temperature by 1° C caused an 8.4 days later</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29899456','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29899456"><span>Extensive retreat and re-advance of the West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet during the Holocene.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kingslake, J; Scherer, R P; Albrecht, T; Coenen, J; Powell, R D; Reese, R; Stansell, N D; Tulaczyk, S; Wearing, M G; Whitehouse, P L</p> <p>2018-06-01</p> <p>To predict the future contributions of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheets to sea-level rise, numerical models use reconstructions of past <span class="hlt">ice</span>-sheet retreat after the Last Glacial Maximum to tune model parameters 1 . Reconstructions of the West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet have assumed that it retreated progressively throughout the Holocene epoch (the past 11,500 years or so) 2-4 . Here we show, however, that over this period the grounding line of the West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet (which marks the point at which it is no longer in contact with the ground and becomes a floating <span class="hlt">ice</span> shelf) retreated several hundred kilometres inland of today's grounding line, before isostatic rebound caused it to re-advance to its present position. Our evidence includes, first, radiocarbon dating of sediment cores recovered from beneath the <span class="hlt">ice</span> streams of the Ross Sea sector, indicating widespread Holocene marine exposure; and second, <span class="hlt">ice</span>-penetrating radar observations of englacial structure in the Weddell Sea sector, indicating <span class="hlt">ice</span>-shelf grounding. We explore the implications of these findings with an <span class="hlt">ice</span>-sheet model. Modelled re-advance of the grounding line in the Holocene requires <span class="hlt">ice</span>-shelf grounding caused by isostatic rebound. Our findings overturn the assumption of progressive retreat of the grounding line during the Holocene in West Antarctica, and corroborate previous suggestions of <span class="hlt">ice</span>-sheet re-advance 5 . Rebound-driven stabilizing processes were apparently able to halt and reverse climate-initiated <span class="hlt">ice</span> loss. Whether these processes can reverse present-day <span class="hlt">ice</span> loss 6 on millennial timescales will depend on bedrock topography and mantle viscosity-parameters that are difficult to measure and to incorporate into <span class="hlt">ice</span>-sheet models.</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> <span class="hlt">ice</span> 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 <span class="hlt">ice</span> stream B in the West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet reveal that the base of the <span class="hlt">ice</span> stream is at the melting point and the basal water pressure is within about 1.6 bars of the <span class="hlt">ice</span> overburden pressure. These conditions allow the rapid <span class="hlt">ice</span> streaming motion to occur by basal sliding or by shear deformation of unconsolidated sediments that underlie the <span class="hlt">ice</span> in a layer at least 2 meters thick. The mechanics of <span class="hlt">ice</span> streaming plays a role in the response of the <span class="hlt">ice</span> sheet to climatic change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012TCD.....6..505F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012TCD.....6..505F"><span>Quantification of ikaite in <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fischer, M.; Thomas, D. N.; Krell, A.; Nehrke, G.; Göttlicher, J.; Norman, L.; Riaux-Gobin, C.; Dieckmann, G. S.</p> <p>2012-02-01</p> <p>Calcium carbonate precipitation in sea <span class="hlt">ice</span> can increase pCO2 during precipitation in winter and decrease pCO2 during dissolution in spring. CaCO3 precipitation in sea <span class="hlt">ice</span> is thought to potentially drive significant CO2 uptake by the ocean. However, little is known about the quantitative spatial and temporal distribution of CaCO3 within sea <span class="hlt">ice</span>. This is the first quantitative study of hydrous calcium carbonate, as ikaite, in sea <span class="hlt">ice</span> and discusses its potential significance for the carbon cycle in polar oceans. <span class="hlt">Ice</span> cores and brine samples were collected from pack and land fast sea <span class="hlt">ice</span> between September and December 2007 during an expedition in the East <span class="hlt">Antarctic</span> and another off Terre Adélie, Antarctica. Samples were analysed for CaCO3, Salinity, DOC, DON, Phosphate, and total alkalinity. A relationship between the measured parameters and CaCO3 precipitation could not be observed. We found calcium carbonate, as ikaite, mostly in the top layer of sea <span class="hlt">ice</span> with values up to 126 mg ikaite per liter melted sea <span class="hlt">ice</span>. This potentially represents a contribution between 0.12 and 9 Tg C to the annual carbon flux in polar oceans. The horizontal distribution of ikaite in sea <span class="hlt">ice</span> was heterogenous. We also found the precipitate in the snow on top of the sea <span class="hlt">ice</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20160005748&hterms=core&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dcore','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20160005748&hterms=core&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dcore"><span>Deep Radiostratigraphy of the East <span class="hlt">Antarctic</span> Plateau: Connecting the Dome C and Vostok <span class="hlt">Ice</span> Core Sites</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Cavitte, Marie G. P.; Blankenship, Donald D.; Young, Duncan A.; Schroeder, Dustin M.; Parrenin, Frederic; Lemeur, Emmanuel; Macgregor, Joseph A.; Siegert, Martin J.</p> <p>2016-01-01</p> <p>Several airborne radar-sounding surveys are used to trace internal reflections around the European Project for <span class="hlt">Ice</span> Coring in Antarctica Dome C and Vostok <span class="hlt">ice</span> core sites. Thirteen reflections, spanning the last two glacial cycles, are traced within 200 km of Dome C, a promising region for million-year-old <span class="hlt">ice</span>, using the University of Texas Institute for Geophysics High-Capacity Radar Sounder. This provides a dated stratigraphy to 2318 m depth at Dome C. Reflection age uncertainties are calculated from the radar range precision and signal-to-noise ratio of the internal reflections. The radar stratigraphy matches well with the Multichannel Coherent Radar Depth Sounder (MCoRDS) radar stratigraphy obtained independently. We show that radar sounding enables the extension of <span class="hlt">ice</span> core ages through the <span class="hlt">ice</span> sheet with an additional radar-related age uncertainty of approximately 1/3-1/2 that of the <span class="hlt">ice</span> cores. Reflections are extended along the Byrd-Totten Glacier divide, using University of Texas/Technical University of Denmark and MCoRDS surveys. However, core-to-core connection is impeded by pervasive aeolian terranes, and <span class="hlt">Lake</span> Vostok's influence on reflection geometry. Poor radar connection of the two <span class="hlt">ice</span> cores is attributed to these effects and suboptimal survey design in affected areas. We demonstrate that, while <span class="hlt">ice</span> sheet internal radar reflections are generally isochronal and can be mapped over large distances, careful survey planning is necessary to extend <span class="hlt">ice</span> core chronologies to distant regions of the East <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16465874','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16465874"><span>A 50-years record of dichloro-diphenyl-trichloroethanes and hexachlorocyclohexanes in <span class="hlt">lake</span> sediments and penguin droppings on King George Island, Maritime <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>Sun, Li-guang; Yin, Xue-bin; Pan, Can-ping; Wang, Yu-hong</p> <p>2005-01-01</p> <p>Since the ban on the use of organochlorine pesticides (OCPs) such as dichloro-diphenyl-trichloroethane (DDT) and hexachlorocyclohexane(HCH) in agriculture, their levels have generally dropped. In a number of cases, however, the levels of these OCPs were found to be unchanging or even increasing after the ban. With the aim to unveil the possible causes of these exceptions, we collected two <span class="hlt">lake</span> cores from King George Island, West Antarctica, and determined their accumulation flux profiles and temporal trends of these OCPs. In the <span class="hlt">lake</span> core sediments with glacier meltwater input, the accumulation flux of DDT shows an abnormal peak around 1980s in addition to the expected one in 1960s. In the <span class="hlt">lake</span> core sediments without glacier meltwater input, the accumulation flux of DDT shows a gradual decline trend after the peak in 1960s. This striking difference in the DDT flux profiles between the two <span class="hlt">lake</span> cores is most likely caused by the regional climate warming and the resulted discharge of the DDT stored in the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> cap into the <span class="hlt">lakes</span> in the <span class="hlt">Antarctic</span> glacier frontier. Furthermore, to investigate the change of OCPs loadings in the <span class="hlt">Antarctic</span> coastal ecosystem, we reconstructed the HCH and DDT concentration profiles in penguin droppings and observed a gradual increase for the former and a continuous decrease for the latter during the past 50 years. The increase of HCH seems to be due to the regional warming from the early 1970s and the resulted HCH discharge to the coastal ecosystem by glaciers' meltwater and the illegal use of HCH in the Southern Hemisphere in the recent decade. Thedifferent temporal trends of HCH and DDT accumulation rate in the <span class="hlt">lake</span> core with glacier meltwater input and the aged penguin droppings can be explained by their different water-soluble property.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70157484','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70157484"><span>Changes in winter air temperatures near <span class="hlt">Lake</span> Michigan, 1851-1993, as determined from regional <span class="hlt">lake-ice</span> records</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Assel, R.A.; Robertson, Dale M.</p> <p>1995-01-01</p> <p>Records of freezeup and breakup dates for Grand Traverse Bay, Michigan, and <span class="hlt">Lake</span> Mendota, Wisconsin, are among the longest <span class="hlt">ice</span> records available near the Great <span class="hlt">Lakes</span>, beginning in 185 1 and 1855, respectively. The timing of freezeup and breakup results from an integration of meteorological conditions (primarily air temperature) that occur before these events. Changes in the average timing of these <span class="hlt">ice</span>-events are translated into changes in air temperature by the use of empirical and process-driven models. The timing of freezeup and breakup at the two locations represents an integration of air temperatures over slightly different seasons (months). Records from both locations indicate that the early winter period before about 1890 was - 15°C cooler than the early winter period after that time; the mean temperature has, however, remained relatively constant since about 1890. Changes in breakup dates demonstrate a similar 1.0-1 .5”C increase in late winter and early spring air temperatures about 1890. More recent average breakup dates at both locations have been earlier than during 1890-1940, indicating an additional warming of 1.2”C in March since about 1940 and a warming of 1 . 1°C in January-March since about 1980. <span class="hlt">Ice</span> records at these sites will continue to provide an early indication of the anticipated climatic warming, not only because of the large response of <span class="hlt">ice</span> <span class="hlt">cover</span> to small changes in air temperature but also because these records integrate climatic conditions during the seasons (winter-spring) when most warming is forecast to occur. Future reductions in <span class="hlt">ice</span> <span class="hlt">cover</span> may strongly affect the winter ecology of the Great <span class="hlt">Lakes</span> by reducing the stable environment required by various levels of the food chain. </p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/11589227','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/11589227"><span>[Psycrophilic organisms in snow and <span class="hlt">ice</span>].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kohshima, S</p> <p>2000-12-01</p> <p>Psychrophilic and psycrotrophic organisms are important in global ecology as a large proportion of our planet is cold. Two-third of sea-water <span class="hlt">covering</span> more than 70% of Earth is cold deep sea water with temperature around 2 degrees C, and more than 90% of freshwater is in polar <span class="hlt">ice</span>-sheets and mountain glaciers. Though biological activity in snow and <span class="hlt">ice</span> had been believed to be extremely limited, various specialized biotic communities were recently discovered at glaciers of various part of the world. The glacier is relatively simple and closed ecosystem with special biotic community containing various psychrophilic and psycrotrophic organisms. Since psychrophilic organisms was discovered in the deep <span class="hlt">ice</span>-core recovered from the <span class="hlt">antarctic</span> <span class="hlt">ice</span>-sheet and a <span class="hlt">lake</span> beneath it, snow and <span class="hlt">ice</span> environments in Mars and Europa are attracting a great deal of scientific attention as possible extraterrestrial habitats of life. This paper briefly reviews the results of the studies on ecology of psychrophilic organisms living in snow and <span class="hlt">ice</span> environments and their physiological and biochemical adaptation to low temperature.</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://www.ncbi.nlm.nih.gov/pubmed/24349517','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24349517"><span>Edwardsiella andrillae, a new species of sea anemone from <span class="hlt">Antarctic</span> <span class="hlt">ice</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Daly, Marymegan; Rack, Frank; Zook, Robert</p> <p>2013-01-01</p> <p>Exploration of the lower surface of the Ross <span class="hlt">Ice</span> Shelf in Antarctica by the Submersible Capable of under-<span class="hlt">Ice</span> Navigation and Imaging (SCINI) remotely operated vehicle discovered a new species of sea anemone living in this previously undocumented ecosystem. This discovery was a significant outcome of the Coulman High Project's geophysical and environmental fieldwork in 2010-2011 as part of the ANDRILL (<span class="hlt">ANtarctic</span> geologic DRILLing) program. Edwardsiella andrillae n. sp., lives with most of its column in the <span class="hlt">ice</span> shelf, with only the tentacle crown extending into the seawater below. In addition to being the only <span class="hlt">Antarctic</span> representative of the genus, Edwardsiella andrillae is distinguished from all other species of the genus in the number of tentacles and in the size and distribution of cnidae. The anatomy and histology of Edwardsiella andrillae present no features that explain how this animal withstands the challenges of life in such an unusual habitat.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20050041627','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20050041627"><span><span class="hlt">Ice</span> Shelves and Landfast <span class="hlt">Ice</span> on the <span class="hlt">Antarctic</span> Perimeter: Revised Scope of Work</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Abdalati, Waleed (Technical Monitor); Scambos, Ted</p> <p>2004-01-01</p> <p><span class="hlt">Ice</span> shelves respond quickly and profoundly to a warming climate. Within a decade after mean summertime temperature reaches approximately 0 deg C and persistent melt ponding is observed, a rapid retreat and disintegration begins. This link was documented for <span class="hlt">ice</span> shelves in the <span class="hlt">Antarctic</span> Peninsula region (the Larsen 'A', B', and Wilkins <span class="hlt">Ice</span> shelves) in the results of a previous grant under ADRO-1. Modeling of shelf <span class="hlt">ice</span> flow and the effects of meltwater indicated that melt ponding accelerates shelf breakup by increasing fracturing. The ADRO-2 funding (topic of this report) supported further inquiry into the evolution of <span class="hlt">ice</span> shelves under warming conditions, and the post-breakup effects on their feeder glaciers. Also, this grant considered fast <span class="hlt">ice</span> and sea <span class="hlt">ice</span> characteristics, to the extent that they provide information regarding shelf stability. A major component of this work was in the form of NSIDC image data support and in situ sea <span class="hlt">ice</span> research on the Aurora Australis 'ARISE' cruise of September 9 2003 through October 28 2003.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19494912','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19494912"><span>The Gamburtsev mountains and the origin and early evolution of the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bo, Sun; Siegert, Martin J; Mudd, Simon M; Sugden, David; Fujita, Shuji; Xiangbin, Cui; Yunyun, Jiang; Xueyuan, Tang; Yuansheng, Li</p> <p>2009-06-04</p> <p><span class="hlt">Ice</span>-sheet development in Antarctica was a result of significant and rapid global climate change about 34 million years ago. <span class="hlt">Ice</span>-sheet and climate modelling suggest reductions in atmospheric carbon dioxide (less than three times the pre-industrial level of 280 parts per million by volume) that, in conjunction with the development of the <span class="hlt">Antarctic</span> Circumpolar Current, led to cooling and glaciation paced by changes in Earth's orbit. Based on the present subglacial topography, numerical models point to <span class="hlt">ice</span>-sheet genesis on mountain massifs of Antarctica, including the Gamburtsev mountains at Dome A, the centre of the present <span class="hlt">ice</span> sheet. Our lack of knowledge of the present-day topography of the Gamburtsev mountains means, however, that the nature of early glaciation and subsequent development of a continental-sized <span class="hlt">ice</span> sheet are uncertain. Here we present radar information about the base of the <span class="hlt">ice</span> at Dome A, revealing classic Alpine topography with pre-existing river valleys overdeepened by valley glaciers formed when the mean summer surface temperature was around 3 degrees C. This landscape is likely to have developed during the initial phases of <span class="hlt">Antarctic</span> glaciation. According to <span class="hlt">Antarctic</span> climate history (estimated from offshore sediment records) the Gamburtsev mountains are probably older than 34 million years and were the main centre for <span class="hlt">ice</span>-sheet growth. Moreover, the landscape has most probably been preserved beneath the present <span class="hlt">ice</span> sheet for around 14 million years.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C34B..08F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C34B..08F"><span><span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet Discharge Driven by Atmosphere-Ocean Feedbacks Across the Last Glacial Termination</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fogwill, C. J.; Turney, C. S.; Golledge, N. R.; Etheridge, D. M.; Rubino, M.; Thornton, D.; Baker, A.; Weber, M. E.; Woodward, J.; van Ommen, T. D.; Moy, A. D.; Davies, S. M.; Bird, M. I.; Winter, K.; Munksgaard, N.; Menviel, L.; Rootes, C.; Vohra, J.; Rivera, A.; Cooper, A.</p> <p>2016-12-01</p> <p>Reconstructing the dynamic response of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheets to warming during the Last Glacial Termination (LGT; 18,000-11,650 yrs ago) allows us to identify <span class="hlt">ice</span>-climate feedbacks that could improve future projections1,2. Whilst the sequence of events during this period are reasonably well-known, relatively poor chronological control has precluded precise alignment of <span class="hlt">ice</span>, atmospheric and marine records2, making it difficult to assess relationships between <span class="hlt">Antarctic</span> <span class="hlt">ice</span>-sheet dynamics, climate change and sea-level rise3-5. Here we present results from a highly-resolved `horizontal <span class="hlt">ice</span> core'6,7 from the Weddell Sea Embayment, which records millennial-scale <span class="hlt">ice</span>-sheet dynamics across this extensive sector of Antarctica. Counterintuitively, we find <span class="hlt">ice</span>-sheet surface drawdown of 600 m across the <span class="hlt">Antarctic</span> Cold Reversal (ACR; 14,600-12,700 yrs ago)5, with stabilisation during the subsequent millennia of atmospheric warming. Earth system and <span class="hlt">ice</span>-sheet modelling highlights that this response was likely sustained by strong ocean-<span class="hlt">ice</span> feedbacks4,8; however, the drivers remain uncertain. Given the coincidence of the <span class="hlt">ice</span>-sheet changes recorded with marked shifts in atmospheric circulation9,10,11we suggest that millennial-scale <span class="hlt">Antarctic</span> <span class="hlt">ice</span>-sheet behaviour was initiated and sustained by global atmospheric teleconnections across the LGT. This has important ramifications <span class="hlt">ice</span>-sheet stability under contemporary climate change, with changing atmospheric and oceanic circulation patterns. 1 Collins, M. et al. in Climate Change 2013: The Physical Science Basis. 2 Weber, M. E. et al. Nature 510, 134-138, (2014). 3 Weaver, A. J., et al., Science 299, 1709-1713, (2003). 4 Golledge, N. R. et al. Nat Commun 5, (2014). 5 Pedro, J. B. et al. Nature Geosci9. 51-55 (2015). 6 Turney, C. S. M. et al. Journal of Quaternary Science 28, 697-704 (2013). 7 Winter, K. et al. Geophys. Res. Lett.43. 5. 2019-2026 (2016). 8 Menviel, L., A. et al., Quaternary Science Reviews 30, 1155-1172 (2011). 9 Hogg</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMED33D0965N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMED33D0965N"><span>Validation of the <span class="hlt">Antarctic</span> Snow Accumulation and <span class="hlt">Ice</span> Discharge Basal Stress Boundary in the South Eastern Region of the Ross <span class="hlt">Ice</span> Shelf, Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nelson, C. B.; King, K.</p> <p>2015-12-01</p> <p>The largest <span class="hlt">ice</span> shelf in <span class="hlt">Antarctic</span>, Ross <span class="hlt">Ice</span> Shelf, was investigated over the years of (1970-2015). Near the basal stress boundary between the <span class="hlt">ice</span> shelf and the West <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet, <span class="hlt">ice</span> velocity ranges from a few meters per year to several hundred meters per year in <span class="hlt">ice</span> streams. Most of the drainage from West Antarctica into the Ross <span class="hlt">Ice</span> Shelf flows down two major <span class="hlt">ice</span> streams, each of which discharges more than 20 km3 of <span class="hlt">ice</span> each year. Along with velocity changes, the warmest water below parts of the Ross <span class="hlt">Ice</span> Shelf resides in the lowest portion of the water column because of its high salinity. Vertical mixing caused by tidal stirring can thus induce ablation by lifting the warm water into contact with the <span class="hlt">ice</span> shelf. This process can cause melting over a period of time and eventually cause breakup of <span class="hlt">ice</span> shelf. With changes occurring over many years a validation is needed for the <span class="hlt">Antarctic</span> Snow Accumulation and <span class="hlt">Ice</span> Discharge (ASAID) basal stress boundary created in 2003. After the 2002 Larsen B <span class="hlt">Ice</span> Shelf disintegration, nearby glaciers in the <span class="hlt">Antarctic</span> Peninsula accelerated up to eight times their original speed over the next 18 months. Similar losses of <span class="hlt">ice</span> tongues in Greenland have caused speed-ups of two to three times the flow rates in just one year. Rapid changes occurring in regions surrounding Antarctica are causing concern in the polar science community to research changes occurring in coastal zones over time. During the research, the team completed study on the Ross <span class="hlt">Ice</span> Shelf located on the south western coast of the <span class="hlt">Antarctic</span>. The study included a validation of the ABSB vs. the natural basal stress boundary (NBSB) along the Ross <span class="hlt">Ice</span> Shelf. The ASAID BSB was created in 2003 by a team of researchers headed by National Aeronautics and Space Administration Goddard Space Flight Center (NASA GSFC), with an aim of studying coastal deviations as it pertains to the mass balance of the entire continent. The point data file was aimed at creating a replica of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22250536','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22250536"><span>[Near infrared reflectance spectroscopy (NIRS): a novel approach to reconstructing historical changes of primary productivity in <span class="hlt">Antarctic</span> <span class="hlt">lake</span>].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chen, Qian-Qian; Liu, Xiao-Dong; Liu, Wen-Qi; Jiang, Shan</p> <p>2011-10-01</p> <p>Compared with traditional chemical analysis methods, reflectance spectroscopy has the advantages of speed, minimal or no sample preparation, non-destruction, and low cost. In order to explore the potential application of spectroscopy technology in the paleolimnological study on <span class="hlt">Antarctic</span> <span class="hlt">lakes</span>, we took a <span class="hlt">lake</span> sediment core in Mochou <span class="hlt">Lake</span> at Zhongshan Station of <span class="hlt">Antarctic</span>, and analyzed the near infrared reflectance spectroscopy (NIRS) data in the sedimentary samples. The results showed that the factor loadings of principal component analysis (PCA) displayed very similar depth-profile change pattern with the S2 index, a reliable proxy for the change in historical <span class="hlt">lake</span> primary productivity. The correlation analysis showed that the values of PCA factor loading and S2 were correlated significantly, suggesting that it is feasible to infer paleoproductivity changes recorded in <span class="hlt">Antarctic</span> <span class="hlt">lakes</span> using NIRS technology. Compared to the traditional method of the trough area between 650 and 700 nm, the authors found that the PCA statistical approach was more accurate for reconstructing the change in historical <span class="hlt">lake</span> primary productivity. The results reported here demonstrate that reflectance spectroscopy can provide a rapid method for the reconstruction of <span class="hlt">lake</span> palaeoenviro nmental change in the remote <span class="hlt">Antarctic</span> regions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C41B0666S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C41B0666S"><span>Future sea-level rise from tidewater and <span class="hlt">ice</span>-shelf tributary glaciers 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>Schannwell, C.; Barrand, N. E.; Radic, V.</p> <p>2016-12-01</p> <p>Iceberg calving and increased <span class="hlt">ice</span> discharge from <span class="hlt">ice</span>-shelf tributary glaciers contribute significant amounts to global sea-level rise (SLR) from the <span class="hlt">Antarctic</span> Peninsula (AP). Owing to ongoing <span class="hlt">ice</span> dynamical changes (collapse of buttressing <span class="hlt">ice</span> shelves), these contributions have accelerated in recent years. As the AP is one of the fastest warming regions on Earth, further <span class="hlt">ice</span> dynamical adjustment (increased <span class="hlt">ice</span> discharge) is expected over the next two centuries. Here the first regional SLR projection of the AP from both iceberg calving and increased <span class="hlt">ice</span> discharge from <span class="hlt">ice</span>-shelf tributary glaciers in response to <span class="hlt">ice</span>-shelf collapse is presented. The British <span class="hlt">Antarctic</span> Survey <span class="hlt">Antarctic</span> Peninsula <span class="hlt">Ice</span> Sheet Model (BAS-APISM), previously shown to be suitable for the unique topographic setting from the AP, is forced by temperature output from 13 global climate models (GCMs) from the Coupled Model Intercomparison Project Phase 5 (CMIP5). In response to the high greenhouse gas emission scenario (Representative Concentration Pathway (RCP)8.5), simulations project contribution to SLR of 28±16 to 32±16 mm by 2300, partitioned approximately equally between contributions from tidewater glaciers and <span class="hlt">ice</span>-shelf tributary glaciers. In the RCP4.5 scenario, sea-level rise projections to 2300 are dominated by tidewater glaciers ( ˜8-18 mm). In this cooler scenario, 2.4±1 mm is added to global sea levels from <span class="hlt">ice</span>-shelf tributary drainage basins as fewer <span class="hlt">ice</span>-shelves are projected to collapse. Sea-level projections from <span class="hlt">ice</span>-shelf tributary glaciers are dominated by drainage basins feeding George VI <span class="hlt">Ice</span> Shelf, accounting for ˜70% of simulated SLR. Combined total <span class="hlt">ice</span> dynamical SLR projections to 2300 from the AP vary between 11±2 and 32±16 mm sea-level equivalent (SLE), depending on the emission scenario used. These simulations suggest that omission of tidewater glaciers could lead to a substantial underestimation of the <span class="hlt">ice</span>-sheet's contribution to regional SLR. Iceberg calving and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C21D1155C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C21D1155C"><span>Role of the Tropical Pacific in recent <span class="hlt">Antarctic</span> Sea-<span class="hlt">Ice</span> Trends</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Codron, F.; Bardet, D.; Allouache, C.; Gastineau, G.; Friedman, A. R.; Douville, H.; Voldoire, A.</p> <p>2017-12-01</p> <p>The recent (up to 2016) trends in <span class="hlt">Antarctic</span> sea-<span class="hlt">ice</span> <span class="hlt">cover</span> - a global increase masking a dipole between the Ross and Bellingshausen-Weddel seas - are still not well understood, and not reproduced by CMIP5 coupled climate models. We here explore the potential role of atmospheric circulation changes around the Amundsen Sea, themselves possibly forced by tropical SSTs, an explanation that has been recently advanced. As a first check on this hypothesis, we compare the atmospheric circulation trends simulated by atmospheric GCMs coupled with an ocean or with imposed SSTs (AMIP experiment from CMIP5); the latter being in theory able to reproduce changes caused by natural SST variability. While coupled models simulate in aggregate trends that project on the SAM structure, strongest in summer, the AMIP simulations add in the winter season a pronounced Amundsen Sea Low signature (and a PNA signature in the northern hemisphere) both consistent with a Niña-like trend in the tropical Pacific. We then use a specific coupled GCM setup, in which surface wind anomalies over the tropical Pacific are strongly nudged towards the observed ones, including their interannual variability, but the model is free to evolve elsewhere. The two GCMs used then simulate a deepening trend in the Amundsen-Sea Low in winter, and are able to reproduce a dipole in sea-<span class="hlt">ice</span> <span class="hlt">cover</span>. Further analysis shows that the sea-<span class="hlt">ice</span> dipole is partially forced by surface heat flux anomalies in early winter - the extent varying with the region and GCM used. The turbulent heat fluxes then act to damp the anomalies in late winter, which may however be maintained by <span class="hlt">ice</span>-albedo feedbacks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5034352','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5034352"><span>Windblown Pliocene diatoms and East <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet 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>Scherer, Reed P.; DeConto, Robert M.; Pollard, David; Alley, Richard B.</p> <p>2016-01-01</p> <p>Marine diatoms in tillites along the Transantarctic Mountains (TAMs) have been used to suggest a diminished East <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet (EAIS) during Pliocene warm periods. Updated <span class="hlt">ice</span>-sheet modelling shows significant Pliocene EAIS retreat, creating marine embayments into the Wilkes and Aurora basins that were conducive to high diatom productivity and rapid accumulation of diatomaceous sediments. Here we show that subsequent isostatic uplift exposed accumulated unconsolidated marine deposits to wind erosion. We report new atmospheric modelling utilizing Pliocene climate and derived <span class="hlt">Antarctic</span> landscapes indicating that prevailing mid-altitude winds transported diatoms towards the TAMs, dominantly from extensive emerged coastal deposits of the Aurora Basin. This result unifies leading ideas from competing sides of a contentious debate about the origin of the diatoms in the TAMs and their link to EAIS history, supporting the view that parts of the EAIS are vulnerable to relatively modest warming, with possible implications for future sea-level rise. PMID:27649516</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1917509C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1917509C"><span>Dominant covarying climate signals in the Southern Ocean and <span class="hlt">Antarctic</span> Sea <span class="hlt">Ice</span> influence during last three decades</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cerrone, Dario; Fusco, Giannetta; Simmonds, Ian; Aulicino, Giuseppe; Budillon, Giorgio</p> <p>2017-04-01</p> <p>A composite dataset (comprising geopotential height, sea surface temperature, zonal and meridional surface winds, precipitation, cloud <span class="hlt">cover</span>, surface air temperature, latent plus sensible heat fluxes , and sea <span class="hlt">ice</span> concentration) has been investigated with the aim of revealing the dominant timescales of variability from 1982 to 2013. Three covarying climate signals associated with variations in the sea <span class="hlt">ice</span> distribution around Antarctica have been detected through the application of the Multiple-Taper Method with Singular Value Decomposition (MTM-SVD). Features of the established patterns of variation over the Southern Hemisphere (SH) extratropics have been identified in each of these three climate signals in the form of coupled or individual oscillations. The climate patterns considered here are the Southern Annular Mode (SAM), the Pacific-South America (PSA) teleconnection, the Semi-Annual Oscillation (SAO) and Zonal Wavenumber-3 (ZW3) mode. It is shown that most of the sea <span class="hlt">ice</span> temporal variance is concentrated at the quasi-triennial scale resulting from the constructive superposition of the PSA and ZW3 patterns. In addition the combination of the SAM and SAO patterns is found to promote the interannual sea <span class="hlt">ice</span> variations underlying a general change in the Southern Ocean atmospheric and oceanic circulations. These two modes of variability are also found consistent with the occurrence of the SAM+/PSA- or SAM-/PSA+ combinations, which could have favored the cooling of the sub-<span class="hlt">Antarctic</span> and important changes in the <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> distribution since 2000.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.P34A..05S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.P34A..05S"><span>Breaking <span class="hlt">Ice</span>: Fracture Processes in Floating <span class="hlt">Ice</span> on Earth and Elsewhere</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Scambos, T. A.</p> <p>2016-12-01</p> <p>Rapid, intense fracturing events in the <span class="hlt">ice</span> shelves of the <span class="hlt">Antarctic</span> Peninsula reveal a set of processes that were not fully appreciated prior to the series of <span class="hlt">ice</span> shelf break-ups observed in the late 1990s and early 2000s. A series of studies have uncovered a fascinating array of relationships between climate, ocean, and <span class="hlt">ice</span>: intense widespread hydrofracture; repetitive hydrofracture induced by <span class="hlt">ice</span> plate bending; the ability for sub-surface flooded firn to support hydrofracture; potential triggering by long-period wave action; accelerated fracturing by trapped tsunamic waves; iceberg disintegration, and a remarkable <span class="hlt">ice</span> rebound process from <span class="hlt">lake</span> drainage that resembles runaway nuclear fission. The events and subsequent studies have shown that rapid regional warming in <span class="hlt">ice</span> shelf areas leads to catastrophic changes in a previously stable <span class="hlt">ice</span> mass. More typical fracturing of thick <span class="hlt">ice</span> plates is a natural consequence of <span class="hlt">ice</span> flow in a complex geographic setting, i.e., it is induced by shear and divergence of spreading plate flow around obstacles. While these are not a result of climate or ocean change, weather and ocean processes may impact the exact timing of final separation of an iceberg from a shelf. Taking these terrestrial perspectives to other <span class="hlt">ice-covered</span> ocean worlds, cautiously, provides an observational framework for interpreting features on Europa and Enceladus.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C51A0963P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C51A0963P"><span>Improving Altimetry Height-change Retrieval on the Fringes of the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Paolo, F. S.; Nilsson, J.; Gardner, A. S.</p> <p>2017-12-01</p> <p>Projections of sea-level change over the next century are highly uncertain, in part, due to insufficient understanding of <span class="hlt">ice</span>-sheet sensitivity to changes in oceanic and atmospheric circulation. This limitation is, to a large degree, related to the lack of long and continuous observational records <span class="hlt">covering</span> critical regions along the <span class="hlt">ice</span>-sheet margins where the <span class="hlt">ice</span> interacts with the ocean. Of particular importance are accurate records of changes in <span class="hlt">ice</span> thickness that provide information on how mass fluctuates on the floating extensions of <span class="hlt">ice</span> streams and glaciers through which the <span class="hlt">ice</span>-sheet drains. These changes can modify the stability of the grounded <span class="hlt">ice</span> sheet through changing back-stress, for example, through loss of <span class="hlt">ice</span>-shelf buttressing. Here, we synthetize 25+ years of satellite altimetry observations to extend the time span and improve the resolution and accuracy of the existing record of <span class="hlt">Antarctic</span> floating <span class="hlt">ice</span> thickness. We incorporate data from ESA's ERS-1, ERS-2, Envisat and Cryosat-2 radar altimeters (1992-present) and NASA's ICESat laser altimeter (2003-2009) and Operation <span class="hlt">Ice</span>Bridge surveys (2009-present); with plans to include ICESat-2 data soon after its launch in September 2018. Towards this effort, we revisit some of the main corrections applied to altimeter data, such as minimization of the difference between measurements from radar and laser systems; and we improve the approach for the synthesis of heterogeneous measurements of <span class="hlt">ice</span>-surface topography and uncertainty estimation. We report on our progress in constructing this long-term and homogeneous record, with a particular focus on the floating <span class="hlt">ice</span> shelves.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3528574','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3528574"><span>Microbial life at −13 °C in the brine of an <span class="hlt">ice</span>-sealed <span class="hlt">Antarctic</span> <span class="hlt">lake</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>Murray, Alison E.; Kenig, Fabien; Fritsen, Christian H.; McKay, Christopher P.; Cawley, Kaelin M.; Edwards, Ross; Kuhn, Emanuele; McKnight, Diane M.; Ostrom, Nathaniel E.; Peng, Vivian; Ponce, Adrian; Priscu, John C.; Samarkin, Vladimir; Townsend, Ashley T.; Wagh, Protima; Young, Seth A.; Yung, Pung To; Doran, Peter T.</p> <p>2012-01-01</p> <p>The permanent <span class="hlt">ice</span> <span class="hlt">cover</span> of <span class="hlt">Lake</span> Vida (Antarctica) encapsulates an extreme cryogenic brine ecosystem (−13 °C; salinity, 200). This aphotic ecosystem is anoxic and consists of a slightly acidic (pH 6.2) sodium chloride-dominated brine. Expeditions in 2005 and 2010 were conducted to investigate the biogeochemistry of <span class="hlt">Lake</span> Vida’s brine system. A phylogenetically diverse and metabolically active Bacteria dominated microbial assemblage was observed in the brine. These bacteria live under very high levels of reduced metals, ammonia, molecular hydrogen (H2), and dissolved organic carbon, as well as high concentrations of oxidized species of nitrogen (i.e., supersaturated nitrous oxide and ∼1 mmol⋅L−1 nitrate) and sulfur (as sulfate). The existence of this system, with active biota, and a suite of reduced as well as oxidized compounds, is unusual given the millennial scale of its isolation from external sources of energy. The geochemistry of the brine suggests that abiotic brine-rock reactions may occur in this system and that the rich sources of dissolved electron acceptors prevent sulfate reduction and methanogenesis from being energetically favorable. The discovery of this ecosystem and the in situ biotic and abiotic processes occurring at low temperature provides a tractable system to study habitability of isolated terrestrial cryoenvironments (e.g., permafrost cryopegs and subglacial ecosystems), and is a potential analog for habitats on other icy worlds where water-rock reactions may cooccur with saline deposits and subsurface oceans. PMID:23185006</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.C31A0592Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.C31A0592Z"><span>Automatic detection of Floating <span class="hlt">Ice</span> at <span class="hlt">Antarctic</span> Continental Margin from Remotely Sensed Image with Object-oriented Matching</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhao, Z.</p> <p>2011-12-01</p> <p>Changes in <span class="hlt">ice</span> sheet and floating <span class="hlt">ices</span> around that have great significance for global change research. In the context of global warming, rapidly changing of <span class="hlt">Antarctic</span> continental margin, caving of <span class="hlt">ice</span> shelves, movement of iceberg are all closely related to climate change and ocean circulation. Using automatic change detection technology to rapid positioning the melting Region of Polar <span class="hlt">ice</span> sheet and the location of <span class="hlt">ice</span> drift would not only strong support for Global Change Research but also lay the foundation for establishing early warning mechanism for melting of the polar <span class="hlt">ice</span> and <span class="hlt">Ice</span> displacement. This paper proposed an automatic change detection method using object-based segmentation technology. The process includes three parts: <span class="hlt">ice</span> extraction using image segmentation, object-baed <span class="hlt">ice</span> tracking, change detection based on similarity matching. An approach based on similarity matching of eigenvector is proposed in this paper, which used area, perimeter, Hausdorff distance, contour, shape and other information of each <span class="hlt">ice</span>-object. Different time of LANDSAT ETM+ data, Chinese environment disaster satellite HJ1B date, MODIS 1B date are used to detect changes of Floating <span class="hlt">ice</span> at <span class="hlt">Antarctic</span> continental margin respectively. We select different time of ETM+ data(January 7, 2003 and January 16, 2003) with the area around <span class="hlt">Antarctic</span> continental margin near the Lazarev Bay, which is from 70.27454853 degrees south latitude, longitude 12.38573410 degrees to 71.44474167 degrees south latitude, longitude 10.39252222 degrees,included 11628 sq km of <span class="hlt">Antarctic</span> continental margin area, as a sample. Then we can obtain the area of floating <span class="hlt">ices</span> reduced 371km2, and the number of them reduced 402 during the time. In addition, the changes of all the floating <span class="hlt">ices</span> around the margin region of <span class="hlt">Antarctic</span> within 1200 km are detected using MODIS 1B data. During the time from January 1, 2008 to January 7, 2008, the floating <span class="hlt">ice</span> area decreased by 21644732 km2, and the number of them reduced by 83080</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70034704','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70034704"><span>Chronological framework for the deglaciation of the <span class="hlt">Lake</span> Michigan lobe of the Laurentide <span class="hlt">ice</span> sheet from <span class="hlt">ice</span>-walled <span class="hlt">lake</span> deposits</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Curry, B.; Petras, J.</p> <p>2011-01-01</p> <p>A revised chronological framework for the deglaciation of the <span class="hlt">Lake</span> Michigan lobe of the south-central Laurentide <span class="hlt">Ice</span> Sheet is presented based on radiocarbon ages of plant macrofossils archived in the sediments of low-relief <span class="hlt">ice</span>-walled <span class="hlt">lakes</span>. We analyze the precision and accuracy of 15 AMS 14C ages of plant macrofossils obtained from a single <span class="hlt">ice</span>-walled <span class="hlt">lake</span> deposit. The semi-circular basin is about 0.72km wide and formed of a 4- to 16-m-thick succession of loess and lacustrine sediment inset into till. The assayed material was leaves, buds and stems of Salix herbacea (snowbed willow). The pooled mean of three ages from the basal lag facies was 18 270??50 14C a BP (21 810cal. a BP), an age that approximates the switch from active <span class="hlt">ice</span> to stagnating conditions. The pooled mean of four ages for the youngest fossil-bearing horizon was 17 770??40 14C a BP (21 180cal. a BP). Material yielding the oldest and youngest ages may be obtained from sediment cores located at any place within the landform. Based on the estimated settling times of overlying barren, rhythmically bedded sand and silt, the lacustrine environment persisted for about 50 more years. At a 67% confidence level, the dated part of the <span class="hlt">ice</span>-walled <span class="hlt">lake</span> succession persisted for between 210 and 860cal. a (modal value: 610cal. a). The deglacial age of five moraines or morainal complexes formed by the fluctuating margin of the <span class="hlt">Lake</span> Michigan lobe have been assessed using this method. There is no overlap of time intervals documenting when <span class="hlt">ice</span>-walled <span class="hlt">lakes</span> persisted on these landforms. The rapid readvances of the lobe during deglaciation after the last glacial maximum probably occurred at some point between the periods of <span class="hlt">ice</span>-walled <span class="hlt">lake</span> sedimentation. ?? 2011 John Wiley & Sons, Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3859642','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3859642"><span>Edwardsiella andrillae, a New Species of Sea Anemone from <span class="hlt">Antarctic</span> <span class="hlt">Ice</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>Daly, Marymegan; Rack, Frank; Zook, Robert</p> <p>2013-01-01</p> <p>Exploration of the lower surface of the Ross <span class="hlt">Ice</span> Shelf in Antarctica by the Submersible Capable of under-<span class="hlt">Ice</span> Navigation and Imaging (SCINI) remotely operated vehicle discovered a new species of sea anemone living in this previously undocumented ecosystem. This discovery was a significant outcome of the Coulman High Project’s geophysical and environmental fieldwork in 2010-2011 as part of the ANDRILL (<span class="hlt">ANtarctic</span> geologic DRILLing) program. Edwardsiella andrillae n. sp., lives with most of its column in the <span class="hlt">ice</span> shelf, with only the tentacle crown extending into the seawater below. In addition to being the only <span class="hlt">Antarctic</span> representative of the genus, Edwardsiella andrillae is distinguished from all other species of the genus in the number of tentacles and in the size and distribution of cnidae. The anatomy and histology of Edwardsiella andrillae present no features that explain how this animal withstands the challenges of life in such an unusual habitat. PMID:24349517</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.P51F..03M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.P51F..03M"><span><span class="hlt">Antarctic</span> analogs for Enceladus</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Murray, A. E.; Andersen, D. T.; McKay, C. P.</p> <p>2014-12-01</p> <p>Enceladus is a new world for Astrobiology. The Cassini discovery of the icy plume emanating from the South Polar region indicates an active world, where detection of water, organics, sodium, and nano-particle silica in the plume strongly suggests that the source is a subsurface salty ocean reservoir. Recent gravity data from Cassini confirms the presence of a regional sea extending north to 50°S. An ocean habitat under a thick <span class="hlt">ice</span> <span class="hlt">cover</span> is perhaps a recurring theme in the Outer Solar System, but what makes Enceladus unique is that the plume jetting out into space is carrying samples of this ocean. Therefore, through the study of Enceladus' plumes we can gain new insights not only of a possible habitable world in the Solar Systems, but also about the formation and evolution of other icy-satellites. Cassini has been able to fly through this plume - effectively sampling the ocean. It is time to plan for future missions that do more detailed analyses, possibly return samples back to Earth and search for evidence of life. To help prepare for such missions, the need for earth-based analog environments is essential for logistical, methodological (life detection) and theoretical development. We have undertaken studies of two terrestrial environments that are close analogs to Enceladus' ocean: <span class="hlt">Lake</span> Vida and <span class="hlt">Lake</span> Untersee - two <span class="hlt">ice</span>-sealed <span class="hlt">Antarctic</span> <span class="hlt">lakes</span> that represent physical, chemical and possibly biological analogs for Enceladus. By studying the diverse biology and physical and chemical constraints to life in these two unique <span class="hlt">lakes</span> we will begin to understand the potential habitability of Enceladus and other icy moons, including possible sources of nutrients and energy, which together with liquid water are the key ingredients for life. Analog research such as this will also enable us to develop and test new strategies to search for evidence of life on Enceladus.</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> <span class="hlt">Ice</span> 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 <span class="hlt">ice</span> sheets. Geothermal flux is one of the most dynamically critical <span class="hlt">ice</span> 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> <span class="hlt">Ice</span> 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 water 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> <span class="hlt">Ice</span> Sheet Divide <span class="hlt">ice</span> core drilling site. PMID:24927578</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3479616','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3479616"><span>Dynamics of the last glacial maximum <span class="hlt">Antarctic</span> <span class="hlt">ice</span>-sheet and its response to ocean forcing</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Golledge, Nicholas R.; Fogwill, Christopher J.; Mackintosh, Andrew N.; Buckley, Kevin M.</p> <p>2012-01-01</p> <p>Retreat of the Last Glacial Maximum (LGM) <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet is thought to have been initiated by changes in ocean heat and eustatic sea level propagated from the Northern Hemisphere (NH) as northern <span class="hlt">ice</span> sheets melted under rising atmospheric temperatures. The extent to which spatial variability in <span class="hlt">ice</span> dynamics may have modulated the resultant pattern and timing of decay of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet has so far received little attention, however, despite the growing recognition that dynamic effects account for a sizeable proportion of mass-balance changes observed in modern <span class="hlt">ice</span> sheets. Here we use a 5-km resolution whole-continent numerical <span class="hlt">ice</span>-sheet model to assess whether differences in the mechanisms governing <span class="hlt">ice</span> sheet flow could account for discrepancies between geochronological studies in different parts of the continent. We first simulate the geometry and flow characteristics of an equilibrium LGM <span class="hlt">ice</span> sheet, using pan-<span class="hlt">Antarctic</span> terrestrial and marine geological data for constraint, then perturb the system with sea level and ocean heat flux increases to investigate <span class="hlt">ice</span>-sheet vulnerability. Our results identify that fast-flowing glaciers in the eastern Weddell Sea, the Amundsen Sea, central Ross Sea, and in the Amery Trough respond most rapidly to ocean forcings, in agreement with empirical data. Most significantly, we find that although ocean warming and sea-level rise bring about mainly localized glacier acceleration, concomitant drawdown of <span class="hlt">ice</span> from neighboring areas leads to widespread thinning of entire glacier catchments—a discovery that has important ramifications for the dynamic changes presently being observed in modern <span class="hlt">ice</span> sheets. PMID:22988078</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22988078','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22988078"><span>Dynamics of the last glacial maximum <span class="hlt">Antarctic</span> <span class="hlt">ice</span>-sheet and its response to ocean forcing.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Golledge, Nicholas R; Fogwill, Christopher J; Mackintosh, Andrew N; Buckley, Kevin M</p> <p>2012-10-02</p> <p>Retreat of the Last Glacial Maximum (LGM) <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet is thought to have been initiated by changes in ocean heat and eustatic sea level propagated from the Northern Hemisphere (NH) as northern <span class="hlt">ice</span> sheets melted under rising atmospheric temperatures. The extent to which spatial variability in <span class="hlt">ice</span> dynamics may have modulated the resultant pattern and timing of decay of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet has so far received little attention, however, despite the growing recognition that dynamic effects account for a sizeable proportion of mass-balance changes observed in modern <span class="hlt">ice</span> sheets. Here we use a 5-km resolution whole-continent numerical <span class="hlt">ice</span>-sheet model to assess whether differences in the mechanisms governing <span class="hlt">ice</span> sheet flow could account for discrepancies between geochronological studies in different parts of the continent. We first simulate the geometry and flow characteristics of an equilibrium LGM <span class="hlt">ice</span> sheet, using pan-<span class="hlt">Antarctic</span> terrestrial and marine geological data for constraint, then perturb the system with sea level and ocean heat flux increases to investigate <span class="hlt">ice</span>-sheet vulnerability. Our results identify that fast-flowing glaciers in the eastern Weddell Sea, the Amundsen Sea, central Ross Sea, and in the Amery Trough respond most rapidly to ocean forcings, in agreement with empirical data. Most significantly, we find that although ocean warming and sea-level rise bring about mainly localized glacier acceleration, concomitant drawdown of <span class="hlt">ice</span> from neighboring areas leads to widespread thinning of entire glacier catchments-a discovery that has important ramifications for the dynamic changes presently being observed in modern <span class="hlt">ice</span> sheets.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_20 --> <div id="page_21" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="401"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70028810','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70028810"><span>Negative magnetic anomaly over Mt. Resnik, a subaerially erupted volcanic peak beneath the West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Behrendt, John C.; Finn, C.; Morse, D.L.; Blankenship, D.D.</p> <p>2006-01-01</p> <p> negative anomalies indicate volcanic activity during a period of magnetic reversal and therefore must also be at least 780 ka. The spatial extent and volume of volcanism can now be reassessed for the 1.2 ?? 106 km2 region of the WAIS characterized by magnetic anomalies defining interpreted volcanic centers associated with the West <span class="hlt">Antarctic</span> rift system. The CWA <span class="hlt">covers</span> an area of 3.54 ?? 105 km2; forty-four percent of that area exhibits short-wavelength, high-amplitude anomalies indicative of volcanic centers and subvolcanic intrusions. This equates to an area of 0.51 ?? 105 km2 and a volume of 106 km3 beneath the <span class="hlt">ice-covered</span> West <span class="hlt">Antarctic</span> rift system, of sufficient extent to be classified as a large igneous province interpreted to be of Oligocene to recent age.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.C11B..03P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.C11B..03P"><span>Airborne radar surveys of snow depth over <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> during Operation <span class="hlt">Ice</span>Bridge</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Panzer, B.; Gomez-Garcia, D.; Leuschen, C.; Paden, J. D.; Gogineni, P. S.</p> <p>2012-12-01</p> <p>Over the last decade, multiple satellite-based laser and radar altimeters, optimized for polar observations, have been launched with one of the major objectives being the determination of global sea <span class="hlt">ice</span> thickness and distribution [5, 6]. Estimation of sea-<span class="hlt">ice</span> thickness from these altimeters relies on freeboard measurements and the presence of snow <span class="hlt">cover</span> on sea <span class="hlt">ice</span> affects this estimate. Current means of estimating the snow depth rely on daily precipitation products and/or data from passive microwave sensors [2, 7]. Even a small uncertainty in the snow depth leads to a large uncertainty in the sea-<span class="hlt">ice</span> thickness estimate. To improve the accuracy of the sea-<span class="hlt">ice</span> thickness estimates and provide validation for measurements from satellite-based sensors, the Center for Remote Sensing of <span class="hlt">Ice</span> Sheets deploys the Snow Radar as a part of NASA Operation <span class="hlt">Ice</span>Bridge. The Snow Radar is an ultra-wideband, frequency-modulated, continuous-wave radar capable of resolving snow depth on sea <span class="hlt">ice</span> from 5 cm to more than 2 meters from long-range, airborne platforms [4]. This paper will discuss the algorithm used to directly extract snow depth estimates exclusively using the Snow Radar data set by tracking both the air-snow and snow-<span class="hlt">ice</span> interfaces. Prior work in this regard used data from a laser altimeter for tracking the air-snow interface or worked under the assumption that the return from the snow-<span class="hlt">ice</span> interface was greater than that from the air-snow interface due to a larger dielectric contrast, which is not true for thick or higher loss snow <span class="hlt">cover</span> [1, 3]. This paper will also present snow depth estimates from Snow Radar data during the NASA Operation <span class="hlt">Ice</span>Bridge 2010-2011 <span class="hlt">Antarctic</span> campaigns. In 2010, three sea <span class="hlt">ice</span> flights were flown, two in the Weddell Sea and one in the Amundsen and Bellingshausen Seas. All three flight lines were repeated in 2011, allowing an annual comparison of snow depth. In 2011, a repeat pass of an earlier flight in the Weddell Sea was flown, allowing for a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.4343A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.4343A"><span>The impact of dynamic topography on the bedrock elevation and volume of the Pliocene <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Austermann, Jacqueline; Pollard, David; Mitrovica, Jerry X.; Moucha, Robert; Forte, Alessandro M.; DeConto, Robert M.</p> <p>2015-04-01</p> <p>Reconstructions of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet over long timescales (i.e. Myrs) require estimates of bedrock elevation through time. <span class="hlt">Ice</span> sheet models have accounted, with varying levels of sophistication, for changes in the bedrock elevation due to glacial isostatic adjustment (GIA), but they have neglected other processes that may perturb topography. One notable example is dynamic topography, the deflection of the solid surface of the Earth due to convective flow within the mantle. Numerically predicted changes in dynamic topography have been used to correct paleo shorelines for this departure from eustasy, but the effect of such changes on <span class="hlt">ice</span> sheet stability is unknown. In this study we use numerical predictions of time-varying dynamic topography to reconstruct bedrock elevation below the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet during the mid Pliocene warm period (~3 Ma). Moreover, we couple this reconstruction to a three-dimensional <span class="hlt">ice</span> sheet model to explore the impact of dynamic topography on the evolution of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet since the Pliocene. Our modeling indicates significant uplift in the area of the Transantarctic Mountains (TAM) and the adjacent Wilkes basin. This predicted uplift, which is at the lower end of geological inferences of uplift of the TAM, implies a lower elevation of the basin in the Pliocene. Relative to simulations that do not include dynamic topography, the lower elevation leads to a smaller <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet volume and a more significant retreat of the grounding line in the Wilkes basin, both of which are consistent with offshore sediment core data. We conclude that reconstructions of the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet during the mid-Pliocene warm period should be based on bedrock elevation models that include the impact of both GIA and dynamic topography.</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 <span class="hlt">Ice</span> 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 <span class="hlt">ice</span>-ocean general circulation models (OGCMs), in particular their local, regional, and high-frequency behavior. This is verified with the aid of daily <span class="hlt">ice</span> 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-water flux associated with melting and freezing in <span class="hlt">Antarctic</span> coastal polynyas by ingesting (assimilating) satellite <span class="hlt">ice</span> concentration where it comes to determining the thermodynamics of the open-water fraction of a model grid cell. Since the NT2 coastal open-water fraction (polynyas) tends to be less extensive than the simulated one in the decisive season and region, assimilating NT2 coastal <span class="hlt">ice</span> concentration yields overall reduced net freezing rates, smaller formation rates of <span class="hlt">Antarctic</span> Bottom Water, and a stronger southward flow of North Atlantic Deep Water across 30 S. Enhanced net freezing rates occur regionally when NT2 coastal <span class="hlt">ice</span> concentration is assimilated, concomitant with a more realistic <span class="hlt">ice</span> thickness distribution and accumulation of High-Salinity Shelf Water. Assimilating BS rather than NT2 coastal <span class="hlt">ice</span> concentration, the differences to the non-assimilated simulation are generally smaller and of opposite sign. This suggests that the model reproduces coastal <span class="hlt">ice</span> 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('https://ntrs.nasa.gov/search.jsp?R=20120015900&hterms=export&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dexport','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20120015900&hterms=export&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dexport"><span>Variability and Trends in Sea <span class="hlt">Ice</span> Extent and <span class="hlt">Ice</span> Production in the Ross Sea</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Comiso, Josefino; Kwok, Ronald; Martin, Seelye; Gordon, Arnold L.</p> <p>2011-01-01</p> <p>Salt release during sea <span class="hlt">ice</span> formation in the Ross Sea coastal regions is regarded as a primary forcing for the regional generation of <span class="hlt">Antarctic</span> Bottom Water. Passive microwave data from November 1978 through 2008 are used to examine the detailed seasonal and interannual characteristics of the sea <span class="hlt">ice</span> <span class="hlt">cover</span> of the Ross Sea and the adjacent Bellingshausen and Amundsen seas. For this period the sea <span class="hlt">ice</span> extent in the Ross Sea shows the greatest increase of all the <span class="hlt">Antarctic</span> seas. Variability in the <span class="hlt">ice</span> <span class="hlt">cover</span> in these regions is linked to changes in the Southern Annular Mode and secondarily to the <span class="hlt">Antarctic</span> Circumpolar Wave. Over the Ross Sea shelf, analysis of sea <span class="hlt">ice</span> drift data from 1992 to 2008 yields a positive rate of increase in the net <span class="hlt">ice</span> export of about 30,000 sq km/yr. For a characteristic <span class="hlt">ice</span> thickness of 0.6 m, this yields a volume transport of about 20 cu km/yr, which is almost identical, within error bars, to our estimate of the trend in <span class="hlt">ice</span> production. The increase in brine rejection in the Ross Shelf Polynya associated with the estimated increase with the <span class="hlt">ice</span> production, however, is not consistent with the reported Ross Sea salinity decrease. The locally generated sea <span class="hlt">ice</span> enhancement of Ross Sea salinity may be offset by an increase of relatively low salinity of the water advected into the region from the Amundsen Sea, a consequence of increased precipitation and regional glacial <span class="hlt">ice</span> melt.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMPP42B..07W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMPP42B..07W"><span>Quaternary Arctic Climate Change of the past 2.8 Ma as reconstructed from sediments of <span class="hlt">Lake</span> El'gygytgyn, NE Russia (Invited)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wennrich, V.; Melles, M.; Brigham-Grette, J.; Minyuk, P.; Nowaczyk, N. R.; Deconto, R. M.; Anderson, P. A.; Andreev, A. A.; Haltia, E.; Kukkonen, M.; Lozhkin, A. V.; Rosen, P.; Tarasov, P. E.</p> <p>2013-12-01</p> <p> intra-hemispheric climate coupling, which could be due to a reduction of <span class="hlt">Antarctic</span> Bottom Water formation and/or a significant global sea-level rise during times of WAIS decays. References Brigham-Grette, J. et al. (2013): Pliocene Warmth, Polar Amplification, and Stepped Pleistocene Cooling Recorded in NE Arctic Russia, Science, 340, 1421-1427. Melles M. et al. (2011): The El'gygytgyn Scientific Drilling Project - conquering Arctic challenges through continental drilling. - Scientific Drilling, 11: 29-40. Melles M. et al. (2012): 2.8 Million Years of Arctic Climate Change from <span class="hlt">Lake</span> El'gygytgyn, NE Russia. - Science, 337: 315-320. Naish T. et al. (2009): Obliquity-paced Pliocene West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet oscillations. -Nature, 458: 322-329. Nolan, M. (2013): Quantitative and qualitative constraints on hind-casting the formation of multiyear <span class="hlt">lake-ice</span> <span class="hlt">covers</span> at <span class="hlt">Lake</span> El'gygytgyn, Clim. Past, 9, 1253-1269. Pollard D. and DeConto R.M. (2009): Modelling West <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet growth and collapse through the past five million years. - Nature, 458: 329-332.</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-<span class="hlt">ice</span> melt on dimethyl sulfide (sulfoniopropionate) inventories in surface waters 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 <span class="hlt">ice</span> 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-<span class="hlt">ice</span> melt events. Concentrations of sulfur compounds, particulate organic carbon (POC) and chlorophyll a in the surface waters 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-<span class="hlt">ice</span> melt. The strong sea-<span class="hlt">ice</span> signal in the distribution of DMS(P) implies that DMS(P) production is likely to decrease with ongoing reductions in sea-<span class="hlt">ice</span> <span class="hlt">cover</span> 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/2017PolSc..13...23H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PolSc..13...23H"><span>Geostatistical analysis and isoscape of <span class="hlt">ice</span> core derived water 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>Water stable isotopes preserved in <span class="hlt">ice</span> 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 <span class="hlt">ice</span> cores <span class="hlt">covering</span> 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/<span class="hlt">ice</span> 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 <span class="hlt">covered</span> by the spatial variability of the existing network of <span class="hlt">ice</span> 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.ncbi.nlm.nih.gov/pubmed/26862787','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26862787"><span>Stable water isotopic composition of the <span class="hlt">Antarctic</span> subglacial <span class="hlt">Lake</span> Vostok: implications for understanding the <span class="hlt">lake</span>'s hydrology.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ekaykin, Alexey A; Lipenkov, Vladimir Y; Kozachek, Anna V; Vladimirova, Diana O</p> <p>2016-01-01</p> <p>We estimated the stable isotopic composition of water from the subglacial <span class="hlt">Lake</span> Vostok using two different sets of samples: (1) water frozen on the drill bit immediately after the first <span class="hlt">lake</span> unsealing and (2) water frozen in the borehole after the unsealing and re-drilled one year later. The most reliable values of the water isotopic composition are: -59.0 ± 0.3 ‰ for oxygen-18, -455 ± 1 ‰ for deuterium and 17 ± 1 ‰ for d-excess. This result is also confirmed by the modelling of isotopic transformations in the water which froze in the borehole, and by a laboratory experiment simulating this process. A comparison of the newly obtained water isotopic composition with that of the <span class="hlt">lake</span> <span class="hlt">ice</span> (-56.2 ‰ for oxygen-18, -442.4 ‰ for deuterium and 7.2 ‰ for d-excess) leads to the conclusion that the <span class="hlt">lake</span> <span class="hlt">ice</span> is very likely formed in isotopic equilibrium with water. In turn, this means that <span class="hlt">ice</span> is formed by a slow freezing without formation of frazil <span class="hlt">ice</span> crystals and/or water pockets. This conclusion agrees well with the observed physical and chemical properties of the <span class="hlt">lake</span>'s accreted <span class="hlt">ice</span>. However, our estimate of the water's isotopic composition is only valid for the upper water layer and may not be representative for the deeper layers of the <span class="hlt">lake</span>, so further investigations are required.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27161450','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27161450"><span>Acclimation of <span class="hlt">Antarctic</span> Chlamydomonas to the sea-<span class="hlt">ice</span> environment: a transcriptomic analysis.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Liu, Chenlin; Wang, Xiuliang; Wang, Xingna; Sun, Chengjun</p> <p>2016-07-01</p> <p>The <span class="hlt">Antarctic</span> green alga Chlamydomonas sp. <span class="hlt">ICE</span>-L was isolated from sea <span class="hlt">ice</span>. As a psychrophilic microalga, it can tolerate the environmental stress in the sea-<span class="hlt">ice</span> brine, such as freezing temperature and high salinity. We performed a transcriptome analysis to identify freezing stress responding genes and explore the extreme environmental acclimation-related strategies. Here, we show that many genes in <span class="hlt">ICE</span>-L transcriptome that encoding PUFA synthesis enzymes, molecular chaperon proteins, and cell membrane transport proteins have high similarity to the gens from <span class="hlt">Antarctic</span> bacteria. These <span class="hlt">ICE</span>-L genes are supposed to be acquired through horizontal gene transfer from its symbiotic microbes in the sea-<span class="hlt">ice</span> brine. The presence of these genes in both sea-<span class="hlt">ice</span> microalgae and bacteria indicated the biological processes they involved in are possibly contributing to <span class="hlt">ICE</span>-L success in sea <span class="hlt">ice</span>. In addition, the biological pathways were compared between <span class="hlt">ICE</span>-L and its closely related sister species, Chlamydomonas reinhardtii and Volvox carteri. In <span class="hlt">ICE</span>-L transcripome, many sequences homologous to the plant or bacteria proteins in the post-transcriptional, post-translational modification, and signal-transduction KEGG pathways, are absent in the nonpsychrophilic green algae. These complex structural components might imply enhanced stress adaptation capacity. At last, differential gene expression analysis at the transcriptome level of <span class="hlt">ICE</span>-L indicated that genes that associated with post-translational modification, lipid metabolism, and nitrogen metabolism are responding to the freezing treatment. In conclusion, the transcriptome of Chlamydomonas sp. <span class="hlt">ICE</span>-L is very useful for exploring the mutualistic interaction between microalgae and bacteria in sea <span class="hlt">ice</span>; and discovering the specific genes and metabolism pathways responding to the freezing acclimation in psychrophilic microalgae.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/12368852','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/12368852"><span>Switch of flow direction in an <span class="hlt">Antarctic</span> <span class="hlt">ice</span> stream.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Conway, H; Catania, G; Raymond, C F; Gades, A M; Scambos, T A; Engelhardt, H</p> <p>2002-10-03</p> <p>Fast-flowing <span class="hlt">ice</span> streams transport <span class="hlt">ice</span> from the interior of West Antarctica to the ocean, and fluctuations in their activity control the mass balance of the <span class="hlt">ice</span> sheet. The mass balance of the Ross Sea sector of the West <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet is now positive--that is, it is growing--mainly because one of the <span class="hlt">ice</span> streams (<span class="hlt">ice</span> stream C) slowed down about 150 years ago. Here we present evidence from both surface measurements and remote sensing that demonstrates the highly dynamic nature of the Ross drainage system. We show that the flow in an area that once discharged into <span class="hlt">ice</span> stream C has changed direction, now draining into the Whillans <span class="hlt">ice</span> stream (formerly <span class="hlt">ice</span> stream B). This switch in flow direction is a result of continuing thinning of the Whillans <span class="hlt">ice</span> stream and recent thickening of <span class="hlt">ice</span> stream C. Further abrupt reorganization of the activity and configuration of the <span class="hlt">ice</span> streams over short timescales is to be expected in the future as the surface topography of the <span class="hlt">ice</span> sheet responds to the combined effects of internal dynamics and long-term climate change. We suggest that caution is needed when using observations of short-term mass changes to draw conclusions about the large-scale mass balance of the <span class="hlt">ice</span> sheet.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70036603','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70036603"><span>Integration of MODIS-derived metrics to assess interannual variability in snowpack, <span class="hlt">lake</span> <span class="hlt">ice</span>, and NDVI in southwest Alaska</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Reed, Bradley C.; Budde, Michael E.; Spencer, Page; Miller, Amy E.</p> <p>2009-01-01</p> <p>Impacts of global climate change are expected to result in greater variation in the seasonality of snowpack, <span class="hlt">lake</span> <span class="hlt">ice</span>, and vegetation dynamics in southwest Alaska. All have wide-reaching physical and biological ecosystem effects in the region. We used Moderate Resolution Imaging Spectroradiometer (MODIS) calibrated radiance, snow <span class="hlt">cover</span> extent, and vegetation index products for interpreting interannual variation in the duration and extent of snowpack, <span class="hlt">lake</span> <span class="hlt">ice</span>, and vegetation dynamics for southwest Alaska. The approach integrates multiple seasonal metrics across large ecological regions. Throughout the observation period (2001-2007), snow <span class="hlt">cover</span> duration was stable within ecoregions, with variable start and end dates. The start of the <span class="hlt">lake</span> <span class="hlt">ice</span> season lagged the snow season by 2 to 3??months. Within a given <span class="hlt">lake</span>, freeze-up dates varied in timing and duration, while break-up dates were more consistent. Vegetation phenology varied less than snow and <span class="hlt">ice</span> metrics, with start-of-season dates comparatively consistent across years. The start of growing season and snow melt were related to one another as they are both temperature dependent. Higher than average temperatures during the El Ni??o winter of 2002-2003 were expressed in anomalous <span class="hlt">ice</span> and snow season patterns. We are developing a consistent, MODIS-based dataset that will be used to monitor temporal trends of each of these seasonal metrics and to map areas of change for the study area.</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 <span class="hlt">ice</span> 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 <span class="hlt">ice</span> 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 <span class="hlt">ice</span> 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 <span class="hlt">ice</span> 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 <span class="hlt">ice</span> 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> <span class="hlt">Ice</span> 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 water 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/2018ESSD...10..711J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ESSD...10..711J"><span>A new bed elevation model for the Weddell Sea sector of the West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jeofry, Hafeez; Ross, Neil; Corr, Hugh F. J.; Li, Jilu; Morlighem, Mathieu; Gogineni, Prasad; Siegert, Martin J.</p> <p>2018-04-01</p> <p>We present a new digital elevation model (DEM) of the bed, with a 1 km gridding, of the Weddell Sea (WS) sector of the West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet (WAIS). The DEM has a total area of ˜ 125 000 km2 <span class="hlt">covering</span> the Institute, Möller and Foundation <span class="hlt">ice</span> streams, as well as the Bungenstock <span class="hlt">ice</span> rise. In comparison with the Bedmap2 product, our DEM includes new aerogeophysical datasets acquired by the Center for Remote Sensing of <span class="hlt">Ice</span> Sheets (CReSIS) through the NASA Operation <span class="hlt">Ice</span>Bridge (OIB) program in 2012, 2014 and 2016. We also improve bed elevation information from the single largest existing dataset in the region, collected by the British <span class="hlt">Antarctic</span> Survey (BAS) Polarimetric radar Airborne Science Instrument (PASIN) in 2010-2011, from the relatively crude measurements determined in the field for quality control purposes used in Bedmap2. While the gross form of the new DEM is similar to Bedmap2, there are some notable differences. For example, the position and size of a deep subglacial trough (˜ 2 km below sea level) between the <span class="hlt">ice</span>-sheet interior and the grounding line of the Foundation <span class="hlt">Ice</span> Stream have been redefined. From the revised DEM, we are able to better derive the expected routing of basal water and, by comparison with that calculated using Bedmap2, we are able to assess regions where hydraulic flow is sensitive to change. Given the potential vulnerability of this sector to ocean-induced melting at the grounding line, especially in light of the improved definition of the Foundation <span class="hlt">Ice</span> Stream trough, our revised DEM will be of value to <span class="hlt">ice</span>-sheet modelling in efforts to quantify future glaciological changes in the region and, from this, the potential impact on global sea level. The new 1 km bed elevation product of the WS sector can be found at <a href="https://doi.org/10.5281/zenodo.1035488" target="_blank">https://doi.org/10.5281/zenodo.1035488</a>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AdSpR..48..697B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AdSpR..48..697B"><span>Searching for life in extreme environments relevant to Jovian's Europa: Lessons from subglacial <span class="hlt">ice</span> studies at <span class="hlt">Lake</span> Vostok (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>Bulat, Sergey A.; Alekhina, Irina A.; Marie, Dominique; Martins, Jean; Petit, Jean Robert</p> <p>2011-08-01</p> <p>The objective was to estimate the genuine microbial content of <span class="hlt">ice</span> samples from refrozen water (accretion <span class="hlt">ice</span>) from the subglacial <span class="hlt">Lake</span> Vostok (Antarctica) buried beneath the 4-km thick East <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet. The samples were extracted by heavy deep <span class="hlt">ice</span> drilling from 3659 m below the surface. High pressure, a low carbon and chemical content, isolation, complete darkness and the probable excess of oxygen in water for millions of years characterize this extreme environment. A decontamination protocol was first applied to samples selected for the absence of cracks to remove the outer part contaminated by handling and drilling fluid. Preliminary indications showed the accretion <span class="hlt">ice</span> samples to be almost gas free with a low impurity content. Flow cytometry showed the very low unevenly distributed biomass while repeated microscopic observations were unsuccessful.We used strategies of Ancient DNA research that include establishing contaminant databases and criteria to validate the amplification results. To date, positive results that passed the artifacts and contaminant databases have been obtained for a pair of bacterial phylotypes only in accretion <span class="hlt">ice</span> samples featured by some bedrock sediments. The phylotypes included the chemolithoautotrophic thermophile Hydrogenophilus thermoluteolus and one unclassified phylotype. Combined with geochemical and geophysical considerations, our results suggest the presence of a deep biosphere, possibly thriving within some active faults of the bedrock encircling the subglacial <span class="hlt">lake</span>, where the temperature is as high as 50 °C and in situ hydrogen is probably present.Our approach indicates that the search for life in the subglacial <span class="hlt">Lake</span> Vostok is constrained by a high probability of forward-contamination. Our strategy includes strict decontamination procedures, thorough tracking of contaminants at each step of the analysis and validation of the results along with geophysical and ecological considerations for the <span class="hlt">lake</span> setting. This may</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 <span class="hlt">Ice</span> 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 water has played an important role in the history of water on the planet Mars [1]. Subsurface water, 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 water 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 <span class="hlt">Ice</span> 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 water <span class="hlt">ice</span> (inferred as debris-<span class="hlt">covered</span> glacial <span class="hlt">ice</span>) 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/2015EGUGA..17.7564M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.7564M"><span>A Tale of Two Forcings: Present-Day Coupled <span class="hlt">Antarctic</span> <span class="hlt">Ice</span>-sheet/Southern Ocean dynamics using the POPSICLES model.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Martin, Daniel; Asay-Davis, Xylar; Cornford, Stephen; Price, Stephen; Ng, Esmond; Collins, William</p> <p>2015-04-01</p> <p>We present POPSICLES simulation results <span class="hlt">covering</span> the full <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet and the Southern Ocean spanning the period 1990 to 2010 resulting from two different choices of climate forcing: a 'normal-year' climatology and the CORE v. 2 interannual forcing data (Large and Yeager 2008). Simulations are performed at 0.1o (~5 km) ocean resolution and adaptive <span class="hlt">ice</span> sheet resolution as fine as 500 m. We compare time-averaged melt rates below a number of major <span class="hlt">ice</span> shelves with those reported by Rignot et al. (2013) as well as other recent studies. We also present seasonal variability and decadal melting trends from several <span class="hlt">Antarctic</span> regions, along with the response of the <span class="hlt">ice</span> shelves and consequent dynamics of the grounded <span class="hlt">ice</span> sheet. POPSICLES couples the POP2x ocean model, a modified version of the Parallel Ocean Program (Smith and Gent, 2002), and the BISICLES <span class="hlt">ice</span>-sheet model (Cornford et al., 2012). POP2x includes sub-<span class="hlt">ice</span>-shelf circulation using partial top cells (Losch, 2008) and boundary layer physics following Holland and Jenkins (1999), Jenkins (2001), and Jenkins et al. (2010). Standalone POP2x output compares well with standard <span class="hlt">ice</span>-ocean test cases (e.g., ISOMIP; Losch, 2008) and other continental-scale simulations and melt-rate observations (Kimura et al., 2013; Rignot et al., 2013). BISICLES makes use of adaptive mesh refinement and a 1st-order accurate momentum balance similar to the L1L2 model of Schoof and Hindmarsh (2009) to accurately model regions of dynamic complexity, such as <span class="hlt">ice</span> streams, outlet glaciers, and grounding lines. Results of BISICLES simulations have compared favorably to comparable simulations with a Stokes momentum balance in both idealized tests (MISMIP-3d; Pattyn et al., 2013) and realistic configurations (Favier et al. 2014).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5734018','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5734018"><span>Genomes of Novel Microbial Lineages Assembled from the Sub-<span class="hlt">Ice</span> Waters of <span class="hlt">Lake</span> Baikal</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Cabello-Yeves, Pedro J.; Zemskaya, Tamara I.; Rosselli, Riccardo; Coutinho, Felipe H.; Zakharenko, Alexandra S.; Blinov, Vadim V.</p> <p>2017-01-01</p> <p>ABSTRACT We present a metagenomic study of <span class="hlt">Lake</span> Baikal (East Siberia). Two samples obtained from the water column under the <span class="hlt">ice</span> <span class="hlt">cover</span> (5 and 20 m deep) in March 2016 have been deep sequenced and the reads assembled to generate metagenome-assembled genomes (MAGs) that are representative of the microbes living in this special environment. Compared with freshwater bodies studied around the world, <span class="hlt">Lake</span> Baikal had an unusually high fraction of Verrucomicrobia. Other groups, such as Actinobacteria and Proteobacteria, were in proportions similar to those found in other <span class="hlt">lakes</span>. The genomes (and probably cells) tended to be small, presumably reflecting the extremely oligotrophic and cold prevalent conditions. Baikal microbes are novel lineages recruiting very little from other water bodies and are distantly related to other freshwater microbes. Despite their novelty, they showed the closest relationship to genomes discovered by similar approaches from other freshwater <span class="hlt">lakes</span> and reservoirs. Some of them were particularly similar to MAGs from the Baltic Sea, which, although it is brackish, connected to the ocean, and much more eutrophic, has similar climatological conditions. Many of the microbes contained rhodopsin genes, indicating that, in spite of the decreased light penetration allowed by the thick <span class="hlt">ice</span>/snow <span class="hlt">cover</span>, photoheterotrophy could be widespread in the water column, either because enough light penetrates or because the microbes are already adapted to the summer <span class="hlt">ice</span>-less conditions. We have found a freshwater SAR11 subtype I/II representative showing striking synteny with Pelagibacter ubique strains, as well as a phage infecting the widespread freshwater bacterium Polynucleobacter. IMPORTANCE Despite the increasing number of metagenomic studies on different freshwater bodies, there is still a missing component in oligotrophic cold <span class="hlt">lakes</span> suffering from long seasonal frozen cycles. Here, we describe microbial genomes from metagenomic assemblies that appear in the upper</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29079621','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29079621"><span>Genomes of Novel Microbial Lineages Assembled from the Sub-<span class="hlt">Ice</span> Waters of <span class="hlt">Lake</span> Baikal.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Cabello-Yeves, Pedro J; Zemskaya, Tamara I; Rosselli, Riccardo; Coutinho, Felipe H; Zakharenko, Alexandra S; Blinov, Vadim V; Rodriguez-Valera, Francisco</p> <p>2018-01-01</p> <p>We present a metagenomic study of <span class="hlt">Lake</span> Baikal (East Siberia). Two samples obtained from the water column under the <span class="hlt">ice</span> <span class="hlt">cover</span> (5 and 20 m deep) in March 2016 have been deep sequenced and the reads assembled to generate metagenome-assembled genomes (MAGs) that are representative of the microbes living in this special environment. Compared with freshwater bodies studied around the world, <span class="hlt">Lake</span> Baikal had an unusually high fraction of Verrucomicrobia Other groups, such as Actinobacteria and Proteobacteria , were in proportions similar to those found in other <span class="hlt">lakes</span>. The genomes (and probably cells) tended to be small, presumably reflecting the extremely oligotrophic and cold prevalent conditions. Baikal microbes are novel lineages recruiting very little from other water bodies and are distantly related to other freshwater microbes. Despite their novelty, they showed the closest relationship to genomes discovered by similar approaches from other freshwater <span class="hlt">lakes</span> and reservoirs. Some of them were particularly similar to MAGs from the Baltic Sea, which, although it is brackish, connected to the ocean, and much more eutrophic, has similar climatological conditions. Many of the microbes contained rhodopsin genes, indicating that, in spite of the decreased light penetration allowed by the thick <span class="hlt">ice</span>/snow <span class="hlt">cover</span>, photoheterotrophy could be widespread in the water column, either because enough light penetrates or because the microbes are already adapted to the summer <span class="hlt">ice</span>-less conditions. We have found a freshwater SAR11 subtype I/II representative showing striking synteny with Pelagibacter ubique strains, as well as a phage infecting the widespread freshwater bacterium Polynucleobacter IMPORTANCE Despite the increasing number of metagenomic studies on different freshwater bodies, there is still a missing component in oligotrophic cold <span class="hlt">lakes</span> suffering from long seasonal frozen cycles. Here, we describe microbial genomes from metagenomic assemblies that appear in the upper water</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> <span class="hlt">Ice</span> 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> <span class="hlt">ice</span> shelves is an important factor in determining the stability of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet. This study used the climatic outputs of an atmosphere?ocean general circulation model to force a circumpolar ocean model that resolves <span class="hlt">ice</span> shelf cavity circulation to investigate the response of <span class="hlt">Antarctic</span> <span class="hlt">ice</span> 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 <span class="hlt">ice</span> 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 water onto the continental shelves, linked to sea <span class="hlt">ice</span> production and climate change, is crucial in determining the basal melt rate of many <span class="hlt">ice</span> 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 <span class="hlt">ice</span> and high-density water, preventing warmer water approaching the <span class="hlt">ice</span> shelves under a colder climate. These results reflect the importance of both water 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> <span class="hlt">ice</span> 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_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('https://www.ncbi.nlm.nih.gov/pubmed/25845501','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25845501"><span>Physicochemical control of bacterial and protist community composition and diversity in <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Torstensson, Anders; Dinasquet, Julie; Chierici, Melissa; Fransson, Agneta; Riemann, Lasse; Wulff, Angela</p> <p>2015-10-01</p> <p>Due to climate change, sea <span class="hlt">ice</span> experiences changes in terms of extent and physical properties. In order to understand how sea <span class="hlt">ice</span> microbial communities are affected by changes in physicochemical properties of the <span class="hlt">ice</span>, we used 454-sequencing of 16S and 18S rRNA genes to examine environmental control of microbial diversity and composition in <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span>. We observed a high diversity and richness of bacteria, which were strongly negatively correlated with temperature and positively with brine salinity. We suggest that bacterial diversity in sea <span class="hlt">ice</span> is mainly controlled by physicochemical properties of the <span class="hlt">ice</span>, such as temperature and salinity, and that sea <span class="hlt">ice</span> bacterial communities are sensitive to seasonal and environmental changes. For the first time in <span class="hlt">Antarctic</span> interior sea <span class="hlt">ice</span>, we observed a strong eukaryotic dominance of the dinoflagellate phylotype SL163A10, comprising 63% of the total sequences. This phylotype is known to be kleptoplastic and could be a significant primary producer in sea <span class="hlt">ice</span>. We conclude that mixotrophic flagellates may play a greater role in the sea <span class="hlt">ice</span> microbial ecosystem than previously believed, and not only during the polar night but also during summer when potential food sources are abundant. © 2015 Society for Applied Microbiology and John Wiley & Sons Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4371949','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4371949"><span>Ocean-driven thinning enhances iceberg calving and retreat of <span class="hlt">Antarctic</span> <span class="hlt">ice</span> shelves</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Liu, Yan; Moore, John C.; Cheng, Xiao; Gladstone, Rupert M.; Bassis, Jeremy N.; Liu, Hongxing; Wen, Jiahong; Hui, Fengming</p> <p>2015-01-01</p> <p>Iceberg calving from all <span class="hlt">Antarctic</span> <span class="hlt">ice</span> shelves has never been directly measured, despite playing a crucial role in <span class="hlt">ice</span> sheet mass balance. Rapid changes to iceberg calving naturally arise from the sporadic detachment of large tabular bergs but can also be triggered by climate forcing. Here we provide a direct empirical estimate of mass loss due to iceberg calving and melting from <span class="hlt">Antarctic</span> <span class="hlt">ice</span> shelves. We find that between 2005 and 2011, the total mass loss due to iceberg calving of 755 ± 24 gigatonnes per year (Gt/y) is only half the total loss due to basal melt of 1516 ± 106 Gt/y. However, we observe widespread retreat of <span class="hlt">ice</span> shelves that are currently thinning. Net mass loss due to iceberg calving for these <span class="hlt">ice</span> shelves (302 ± 27 Gt/y) is comparable in magnitude to net mass loss due to basal melt (312 ± 14 Gt/y). Moreover, we find that iceberg calving from these decaying <span class="hlt">ice</span> shelves is dominated by frequent calving events, which are distinct from the less frequent detachment of isolated tabular icebergs associated with <span class="hlt">ice</span> shelves in neutral or positive mass balance regimes. Our results suggest that thinning associated with ocean-driven increased basal melt can trigger increased iceberg calving, implying that iceberg calving may play an overlooked role in the demise of shrinking <span class="hlt">ice</span> shelves, and is more sensitive to ocean forcing than expected from steady state calving estimates. PMID:25733856</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> <span class="hlt">Ice</span> 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/water/material: Global environmental changes driven by Southern Ocean and <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> 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> <span class="hlt">ice</span> 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> <span class="hlt">Ice</span> Sheet". The <span class="hlt">Antarctic</span> <span class="hlt">ice</span> 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 <span class="hlt">ice</span> 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 <span class="hlt">ice</span> 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 <span class="hlt">ice</span> 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('http://adsabs.harvard.edu/abs/2018JGRC..123..216W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRC..123..216W"><span>Brine Convection, Temperature Fluctuations, and Permeability in Winter <span class="hlt">Antarctic</span> Land-Fast Sea <span class="hlt">Ice</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wongpan, P.; Hughes, K. G.; Langhorne, P. J.; Smith, I. J.</p> <p>2018-01-01</p> <p>Vertical temperature strings are used in sea <span class="hlt">ice</span> research to study heat flow, <span class="hlt">ice</span> growth rate, and ocean-<span class="hlt">ice</span>-atmosphere interaction. We demonstrate the feasibility of using temperature fluctuations as a proxy for fluid movement, a key process for supplying nutrients to <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> algal communities. Four strings were deployed in growing, land-fast sea <span class="hlt">ice</span> in McMurdo Sound, Antarctica. By smoothing temperature data with the robust LOESS method, we obtain temperature fluctuations that cannot be explained by insolation or atmospheric heat loss. Statistical distributions of these temperature fluctuations are investigated with sensitivities to the distance from the <span class="hlt">ice</span>-ocean interface, average <span class="hlt">ice</span> temperature, and sea <span class="hlt">ice</span> structure. Fluctuations are greatest close to the base (<50 mm) at temperatures >-3°C, and are discrete events with an average active period of 43% compared to 11% when the <span class="hlt">ice</span> is colder (-3°C to -5°C). Assuming fluctuations occur when the Rayleigh number, derived from mushy layer theory, exceeds a critical value of 10 we approximate the harmonic mean permeability of this thick (>1 m) sea <span class="hlt">ice</span> in terms of distance from the <span class="hlt">ice</span>-ocean interface. Near the base, we obtain values in the same range as those measured by others in Arctic spring and summer. The permeability between the <span class="hlt">ice</span>-ocean interface and 0.05 ± 0.04 m above it is of order 10-9 m2. Columnar and incorporated platelet <span class="hlt">ice</span> permeability distributions in the bottom 0.1 m of winter <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> are statistically significantly different although their arithmetic means are indistinguishable.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19990008060&hterms=3G&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3D3G','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19990008060&hterms=3G&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3D3G"><span>Global Geodetic Signatures of the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>James, Thomas S.; Ivins, Erik R.</p> <p>1997-01-01</p> <p>Four scenarios of present day <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet mass change are developed from comprehensive reviews of the available glaciological and oceanographic evidence. The gridded scenarios predict widely varying contributions to secular sea level change xi ranging from -1.1 to 0.45 mm/yr, and predict polar motion m and time-varying low-degree gravitational coefficients J(sub l) that differ significantly from earlier estimates. A reasonably linear relationship between the rate of sea level change from Antarctica xi(sub A) and the predicted <span class="hlt">Antarctic</span> J(sub l) is found for the four scenarios. This linearity permits a series of forward models to be constructed that incorporate the effects of <span class="hlt">ice</span> mass changes in Antarctica, Greenland, and distributed smaller glaciers, as well as postglacial rebound (assuming the <span class="hlt">ICE</span>-3G deglaciation history), with the goal of obtaining optimum reconciliation between observed constraints on J(sub l) and sea level rise xi. Numerous viable combinations of lower mantle viscosity and hydrologic sources are found that safely "observed" in the range of 1 to 2-2.5 mm/yr and observed J(sub l) for degrees 2, 3, and 4. In contrast, rates of global sea level rise above 2.5 mm/yr are inconsistent with available J(sub l) observations. The successful composite models feature a pair of lower mantle viscosity solutions arising from the sensitivity of J(sub l) to glacial rebound. The paired values are well separated at xi = 1 mm/yr, but move closer together as xi is increased, and, in fact, merge around xi = 2 - 2.5 mm/yr, revealing an intimate relation between xi and preferred lower mantle viscosity. This general pattern is quite robust and persists for different J(sub l) solutions, for variations in source assumptions, and for different styles of lower mantle viscosity stratification. Tighter J(sub l) constraints for l greater than 2 may allow some viscosity stratification schemes and source assumptions to be excluded in the future. For a given total</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.C24A..03K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.C24A..03K"><span>Seasonal climate information preserved within West <span class="hlt">Antarctic</span> <span class="hlt">ice</span> cores and its relation to large-scale atmospheric circulation and regional sea <span class="hlt">ice</span> variations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Küttel, M.; Steig, E. J.; Ding, Q.; Battisti, D. S.</p> <p>2010-12-01</p> <p>Recent evidence suggests that West Antarctica has been warming since at least the 1950s. With the instrumental record being limited to the mid-20th century, indirect information from stable isotopes (δ18O and δD, hereafter collectively δ) preserved within <span class="hlt">ice</span> cores have commonly been used to place this warming into a long term context. Here, using a large number of δ records obtained during the International Trans-<span class="hlt">Antarctic</span> Scientific Expedition (ITASE), past variations in West <span class="hlt">Antarctic</span> δ are not only investigated over time but also in space. This study therefore provides an important complement to longer records from single locations as e.g. the currently being processed West <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet (WAIS) Divide <span class="hlt">ice</span> core. Although snow accumulation rates at the ITASE sites in West Antarctica are variable, they are generally high enough to allow studies on sub-annual scale over the last 50-100 years. Here, we show that variations in δ in this region are strongly related to the state of the large-scale atmospheric circulation as well as sea <span class="hlt">ice</span> variations in the adjacent Southern Ocean, with important seasonal changes. While a strong relationship to sea <span class="hlt">ice</span> changes in the Ross and Amundsen Sea as well as to the atmospheric circulation offshore is found during austral fall (MAM) and winter (JJA), only modest correlations are found during spring (SON) and summer (DJF). Interestingly, the correlations with the atmospheric circulation in the latter two seasons have the strongest signal over the <span class="hlt">Antarctic</span> continent, but not offshore - an important difference to MAM and JJA. These seasonal changes are in good agreement with the seasonally varying predominant circulation: meridional with more frequent storms in the Amundsen Sea during MAM and JJA and more zonal and stable during SON and DJF. The relationship to regional temperature is similarly seasonally variable with highest correlations found during MAM and JJA. Notably, the circulation pattern found to be strongest</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.C13H..04S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.C13H..04S"><span>A 19-year radar altimeter elevation change time-series of the East and West <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheets</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sundal, A. V.; Shepherd, A.; Wingham, D.; Muir, A.; Mcmillan, M.; Galin, N.</p> <p>2012-12-01</p> <p>We present 19 years of continuous radar altimeter observations of the East and West <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheets acquired by the ERS-1, ERS-2, and ENVISAT satellites between May 1992 and September 2010. Time-series of surface elevation change were developed at 39,375 crossing points of the satellite orbit ground tracks using the method of dual cycle crossovers (Zwally et al., 1989; Wingham et al., 1998). In total, 46.5 million individual measurements were included in the analysis, encompassing 74 and 76 % of the East and West <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet, respectively. The satellites were cross-calibrated by calculating differences between elevation changes occurring during periods of mission overlap. We use the merged time-series to explore spatial and temporal patterns of elevation change and to characterise and quantify the signals of <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet imbalance. References: Wingham, D., Ridout, A., Scharroo, R., Arthern, R. & Shum, C.K. (1998): <span class="hlt">Antarctic</span> elevation change from 1992 to 1996. Science, 282, 456-458. Zwally, H. J., Brenner, A. C., Major, J. A., Bindschadler, R. A. & Marsh, J. G. (1989): Growth of Greenland <span class="hlt">ice</span>-sheet - measurements. Science, 246, 1587-1589.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29239353','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29239353"><span>Initiation and long-term instability of the East <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gulick, Sean P S; Shevenell, Amelia E; Montelli, Aleksandr; Fernandez, Rodrigo; Smith, Catherine; Warny, Sophie; Bohaty, Steven M; Sjunneskog, Charlotte; Leventer, Amy; Frederick, Bruce; Blankenship, Donald D</p> <p>2017-12-13</p> <p>Antarctica's continental-scale <span class="hlt">ice</span> sheets have evolved over the past 50 million years. However, the dearth of <span class="hlt">ice</span>-proximal geological records limits our understanding of past East <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet (EAIS) behaviour and thus our ability to evaluate its response to ongoing environmental change. The EAIS is marine-terminating and grounded below sea level within the Aurora subglacial basin, indicating that this catchment, which drains <span class="hlt">ice</span> to the Sabrina Coast, may be sensitive to climate perturbations. Here we show, using marine geological and geophysical data from the continental shelf seaward of the Aurora subglacial basin, that marine-terminating glaciers existed at the Sabrina Coast by the early to middle Eocene epoch. This finding implies the existence of substantial <span class="hlt">ice</span> volume in the Aurora subglacial basin before continental-scale <span class="hlt">ice</span> sheets were established about 34 million years ago. Subsequently, <span class="hlt">ice</span> advanced across and retreated from the Sabrina Coast continental shelf at least 11 times during the Oligocene and Miocene epochs. Tunnel valleys associated with half of these glaciations indicate that a surface-meltwater-rich sub-polar glacial system existed under climate conditions similar to those anticipated with continued anthropogenic warming. Cooling since the late Miocene resulted in an expanded polar EAIS and a limited glacial response to Pliocene warmth in the Aurora subglacial basin catchment. Geological records from the Sabrina Coast shelf indicate that, in addition to ocean temperature, atmospheric temperature and surface-derived meltwater influenced East <span class="hlt">Antarctic</span> <span class="hlt">ice</span> mass balance under warmer-than-present climate conditions. Our results imply a dynamic EAIS response with continued anthropogenic warming and suggest that the EAIS contribution to future global sea-level projections may be under-estimated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017Natur.552..225G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Natur.552..225G"><span>Initiation and long-term instability of the East <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gulick, Sean P. S.; Shevenell, Amelia E.; Montelli, Aleksandr; Fernandez, Rodrigo; Smith, Catherine; Warny, Sophie; Bohaty, Steven M.; Sjunneskog, Charlotte; Leventer, Amy; Frederick, Bruce; Blankenship, Donald D.</p> <p>2017-12-01</p> <p>Antarctica’s continental-scale <span class="hlt">ice</span> sheets have evolved over the past 50 million years. However, the dearth of <span class="hlt">ice</span>-proximal geological records limits our understanding of past East <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet (EAIS) behaviour and thus our ability to evaluate its response to ongoing environmental change. The EAIS is marine-terminating and grounded below sea level within the Aurora subglacial basin, indicating that this catchment, which drains <span class="hlt">ice</span> to the Sabrina Coast, may be sensitive to climate perturbations. Here we show, using marine geological and geophysical data from the continental shelf seaward of the Aurora subglacial basin, that marine-terminating glaciers existed at the Sabrina Coast by the early to middle Eocene epoch. This finding implies the existence of substantial <span class="hlt">ice</span> volume in the Aurora subglacial basin before continental-scale <span class="hlt">ice</span> sheets were established about 34 million years ago. Subsequently, <span class="hlt">ice</span> advanced across and retreated from the Sabrina Coast continental shelf at least 11 times during the Oligocene and Miocene epochs. Tunnel valleys associated with half of these glaciations indicate that a surface-meltwater-rich sub-polar glacial system existed under climate conditions similar to those anticipated with continued anthropogenic warming. Cooling since the late Miocene resulted in an expanded polar EAIS and a limited glacial response to Pliocene warmth in the Aurora subglacial basin catchment. Geological records from the Sabrina Coast shelf indicate that, in addition to ocean temperature, atmospheric temperature and surface-derived meltwater influenced East <span class="hlt">Antarctic</span> <span class="hlt">ice</span> mass balance under warmer-than-present climate conditions. Our results imply a dynamic EAIS response with continued anthropogenic warming and suggest that the EAIS contribution to future global sea-level projections may be under-estimated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..1413849P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..1413849P"><span>A common and optimized age scale for <span class="hlt">Antarctic</span> <span class="hlt">ice</span> cores</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Parrenin, F.; Veres, D.; Landais, A.; Bazin, L.; Lemieux-Dudon, B.; Toye Mahamadou Kele, H.; Wolff, E.; Martinerie, P.</p> <p>2012-04-01</p> <p>Dating <span class="hlt">ice</span> cores is a complex problem because 1) there is a age shift between the gas bubbles and the surrounding <span class="hlt">ice</span> 2) there are many different <span class="hlt">ice</span> cores which can be synchronized with various proxies and 3) there are many methods to date the <span class="hlt">ice</span> and the gas bubbles, each with advantages and drawbacks. These methods fall into the following categories: 1) <span class="hlt">Ice</span> flow (for the <span class="hlt">ice</span>) and firn densification modelling (for the gas bubbles); 2) Comparison of <span class="hlt">ice</span> core proxies with insolation variations (so-called orbital tuning methods); 3) Comparison of <span class="hlt">ice</span> core proxies with other well dated archives; 4) Identification of well-dated horizons, such as tephra layers or geomagnetic anomalies. Recently, an new dating tool has been developped (DATICE, Lemieux-Dudon et al., 2010), to take into account all the different dating information into account and produce a common and optimal chronology for <span class="hlt">ice</span> cores with estimated confidence intervals. In this talk we will review the different dating information for <span class="hlt">Antarctic</span> <span class="hlt">ice</span> cores and show how the DATICE tool can be applied.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1811977P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1811977P"><span>Sea-level response to abrupt ocean warming of <span class="hlt">Antarctic</span> <span class="hlt">ice</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>Pattyn, Frank</p> <p>2016-04-01</p> <p>Antarctica's contribution to global sea-level rise increases steadily. A fundamental question remains whether the <span class="hlt">ice</span> discharge will lead to marine <span class="hlt">ice</span> sheet instability (MISI) and collapse of certain sectors of the <span class="hlt">ice</span> sheet or whether <span class="hlt">ice</span> loss will increase linearly with the warming trends. Therefore, we employ a newly developed <span class="hlt">ice</span> sheet model of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet, called f.ETISh (fast Elementary Thermomechanical <span class="hlt">Ice</span> Sheet model) to simulate <span class="hlt">ice</span> sheet response to abrupt perturbations in ocean and atmospheric temperature. The f.ETISh model is a vertically integrated hybrid (SSA/SIA) <span class="hlt">ice</span> sheet model including <span class="hlt">ice</span> shelves. Although vertically integrated, thermomechanical coupling is ensured through a simplified representation of <span class="hlt">ice</span> sheet thermodynamics based on an analytical solution of the vertical temperature profile, including strain heating and horizontal advection. The marine boundary is represented by a flux condition either coherent with power-law basal sliding (Pollard & Deconto (2012) based on Schoof (2007)) or according to Coulomb basal friction (Tsai et al., 2015), both taking into account <span class="hlt">ice</span>-shelf buttressing. Model initialization is based on optimization of the basal friction field. Besides the traditional MISMIP tests, new tests with respect to MISI in plan-view models have been devised. The model is forced with stepwise ocean and atmosphere temperature perturbations. The former is based on a parametrised sub-shelf melt (limited to <span class="hlt">ice</span> shelves), while the latter is based on present-day mass balance/surface temperature and corrected for elevation changes. Surface melting is introduced using a PDD model. Results show a general linear response in mass loss to ocean warming. Nonlinear response due to MISI occurs under specific conditions and is highly sensitive to the basal conditions near the grounding line, governed by both the initial conditions and the basal sliding/deformation model. The Coulomb friction model leads to significantly higher</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.C53B0313F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.C53B0313F"><span>Geological Influences on Bedrock Topography and East <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet Dynamics in the Wilkes Subglacial Basin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ferraccioli, F.; Armadillo, E.; Young, D. A.; Blankenship, D. D.; Jordan, T. A.; Balbi, P.; Bozzo, E.; Siegert, M. J.</p> <p>2014-12-01</p> <p>The Wilkes Subglacial Basin (WSB) extends for 1,400 km from George V Land into the interior of East Antarctica and hosts several major glaciers that drain a large sector of the East <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet (EAIS). This region is of key significance for the long-term stability of the <span class="hlt">ice</span> sheet in East Antarctica, as it lies well below sea level and its bedrock deepens inland, making it potentially prone to marine <span class="hlt">ice</span> sheet instability, much like areas of the West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet (WAIS) that are presently experiencing significant mass loss. We present new enhanced potential field images of the WSB combined with existing radar imaging to study geological controls on bedrock topography and <span class="hlt">ice</span> flow regimes in this key sector of the <span class="hlt">ice</span> sheet. These images reveal mayor Precambrian and Paleozoic basement faults that exert tectonic controls both on the margins of the basin and its sub-basins. Several major sub-basins can be recognised: the Eastern Basin, the Central Basins and the Western Basins. Using ICECAP aerogeophysical data we show that these tectonically controlled interior basins connect to newly identified basins underlying the Cook <span class="hlt">Ice</span> Shelf region. This connection implies that any ocean-induced changes at the margin of the EAIS could potentially propagate rapidly further into the interior. With the aid of simple magnetic and gravity models we show that the WSB does not presently include major post Jurassic sedimentary infill. Its bedrock geology is highly variable and includes Proterozoic basement, Neoproterozoic and Cambrian sediments, intruded by Cambrian arc rocks, and <span class="hlt">cover</span> rocks formed by Beacon sediments intruded by Jurassic Ferrar sills. Enhanced <span class="hlt">ice</span> flow in this part of the EAIS occurs therefore in a area of mixed and spatially variable bedrock geology. This contrasts with some regions of the WAIS where more extensive sedimentary basins may represent a geological template for the onset and maintenance of fast glacial flow.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018TCry...12.1745C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018TCry...12.1745C"><span>Archival processes of the water stable isotope signal in East <span class="hlt">Antarctic</span> <span class="hlt">ice</span> cores</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>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</p> <p>2018-05-01</p> <p>The oldest <span class="hlt">ice</span> core records are obtained from the East <span class="hlt">Antarctic</span> Plateau. Water isotopes are key proxies to reconstructing past climatic conditions over the <span class="hlt">ice</span> 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 <span class="hlt">ice</span> core's isotopic composition. By combining observations of isotopic composition in vapour, precipitation, surface snow and buried snow from Dome C, a deep <span class="hlt">ice</span> core site on the East <span class="hlt">Antarctic</span> 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 <span class="hlt">Antarctic</span> 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 <span class="hlt">ice</span> core records in low-accumulation areas.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19870015824','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19870015824"><span>Part 2: Sedimentary geology of the Valles, Marineris, Mars and <span class="hlt">Antarctic</span> dry valley <span class="hlt">lakes</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Nedell, Susan S.</p> <p>1987-01-01</p> <p>Detailed mapping of the layered deposits in the Valles Marineris, Mars from high-resolution Viking orbiter images revealed that they from plateaus of rhythmically layered material whose bases are in the lowest elevations of the canyon floors, and whose tops are within a few hundred meters in elevation of the surrounding plateaus. Four hypotheses for the origin of the layered deposits were considered: that they are eolian deposits; that they are remnants of the same material as the canyon walls; that they are explosive volcanic deposits; or that they were deposited in standing bodies of water. There are serious morphologic objections to each of the first three. The deposition of the layered deposits in standing bodies of water best explains their lateral continuity, horizontality, great thickness, rhythmic nature, and stratigraphic relationships with other units within the canyons. The Martian climatic history indicated that any ancient <span class="hlt">lakes</span> were <span class="hlt">ice</span> <span class="hlt">covered</span>. Two methods for transporting sediment through a <span class="hlt">cover</span> of <span class="hlt">ice</span> on a martian <span class="hlt">lake</span> appear to be feasible. Based on the presently available data, along with the theoretical calculations presented, it appears most likely that the layered deposits in the Valles Marineris were laid down in standing bodies of water.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017FrEaS...5..100C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017FrEaS...5..100C"><span><span class="hlt">Ice</span>-dammed <span class="hlt">lake</span> drainage evolution at Russell Glacier, west Greenland</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carrivick, Jonathan L.; Tweed, Fiona S.; Ng, Felix; Quincey, Duncan J.; Mallalieu, Joseph; Ingeman-Nielsen, Thomas; Mikkelsen, Andreas B.; Palmer, Steven J.; Yde, Jacob C.; Homer, Rachel; Russell, Andrew J.; Hubbard, Alun</p> <p>2017-11-01</p> <p>Glaciological and hydraulic factors that control the timing and mechanisms of glacier <span class="hlt">lake</span> outburst floods (GLOFs) remain poorly understood. This study used measurements of <span class="hlt">lake</span> level at fifteen minute intervals and known <span class="hlt">lake</span> bathymetry to calculate <span class="hlt">lake</span> outflow during two GLOF events from the northern margin of Russell Glacier, west Greenland. We used measured <span class="hlt">ice</span> surface elevation, interpolated subglacial topography and likely conduit geometry to inform a melt enlargement model of the outburst evolution. The model was tuned to best-fit the hydrograph’s rising limb and timing of peak discharge in both events; it achieved Mean Absolute Errors of < 5 %. About one third of the way through the rising limb, conduit melt enlargement became the dominant drainage mechanism. <span class="hlt">Lake</span> water temperature, which strongly governed the enlargement rate, preconditioned the high peak discharge and short duration of these floods. We hypothesize that both GLOFs were triggered by <span class="hlt">ice</span> dam flotation, and localised hydraulic jacking sustained most of their early-stage outflow, explaining the particularly rapid water egress in comparison to that recorded at other <span class="hlt">ice</span>-marginal <span class="hlt">lakes</span>. As <span class="hlt">ice</span> overburden pressure relative to <span class="hlt">lake</span> water hydraulic head diminished, flow became confined to a subglacial conduit. This study has emphasised the inter-play between <span class="hlt">ice</span> dam thickness and <span class="hlt">lake</span> level, drainage timing, <span class="hlt">lake</span> water temperature and consequently rising stage <span class="hlt">lake</span> outflow and flood evolution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930051759&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=19930051759&hterms=Antarctic+icebergs&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DAntarctic%2Bicebergs"><span>Green icebergs formed by freezing of organic-rich seawater to the base of <span class="hlt">Antarctic</span> <span class="hlt">ice</span> shelves</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Warren, Stephen G.; Roesler, Collin S.; Morgan, Vincent I.; Brandt, Richard E.; Goodwin, Ian D.; Allison, Ian</p> <p>1993-01-01</p> <p>Samples of <span class="hlt">Antarctic</span> seawater, basal <span class="hlt">ice</span>, and green <span class="hlt">ice</span> from <span class="hlt">ice</span> cliffs and green icebergs are analyzed in order to examine green icebergs formed by the freezing of organic-rich seawater to the base of <span class="hlt">Antarctic</span> <span class="hlt">ice</span> shelves. Spectral reflectance of a green iceberg measured near 67 deg S, 62 deg E confirms that the color is inherent in the <span class="hlt">ice</span>, not an artifact of the illumination. A constituent that absorbs blue photons is identified by spectrophotometric analysis of core samples from this iceberg and from the Amery basal <span class="hlt">ice</span>, and of seawater samples from Prydz Bay off the Amery <span class="hlt">Ice</span> Shelf. Analysis of the samples by fluorescence spectroscopy indicates that the blue absorption, and hence the inherent green color, is due to the presence of marine-derived organic matter in the green iceberg, basal <span class="hlt">ice</span>, and seawater. Thick accumulations of green <span class="hlt">ice</span>, in icebergs, and at the base of <span class="hlt">ice</span> shelves indicate that high concentrations of organic matter exist in seawater for centuries at the depth of basal freezing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1611965L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1611965L"><span>The influence of supraglacial debris <span class="hlt">cover</span> variability on de-<span class="hlt">icing</span> processes - examples from Svalbard</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lukas, Sven; Benn, Douglas I.; Boston, Clare M.; Hawkins, Jack; Lehane, Niall E.; Lovell, Harold; Rooke, Michael</p> <p>2014-05-01</p> <p> downslope can lead to localised thickening of the debris <span class="hlt">cover</span>, thereby resulting in the creation of new temporarily-stable areas in downslope locations. 3. The renewed and continued re-distribution of material causes de-<span class="hlt">icing</span> to proceed in a stepwise fashion. While de-<span class="hlt">icing</span> is ongoing, this results in the formation of debris cones or even larger ridges and mounds that have been termed "moraine-mound complexes" by previous workers (e.g. Graham et al., 2007). These are temporary landforms that will not survive de-<span class="hlt">icing</span> over longer timescales, and projection of continued reworking into the future shows that perhaps an undulating spread of material will remain (cf. Lukas, 2007). The formation of supraglacial <span class="hlt">lakes</span> during overall melting can lead to the formation of thick sequences of sorted sediments that in turn insulate the underlying <span class="hlt">ice</span> after <span class="hlt">lake</span> drainage. The presence of such sorted sediments in current ridge-top locations in some of the debris <span class="hlt">covers</span> gives further weight to the interpretation of a mode of stepwise de-<span class="hlt">icing</span>; crumbling and erosion by snowmelt and wind attests the shortlived nature of such deposits in topographic highs. Our findings strongly support an interpretation of a de-<span class="hlt">icing</span> mode that takes place in a stepwise fashion that leads to several generations of sediment transfer within the debris <span class="hlt">covers</span> and repeated relief inversion. References Graham, D.J., Bennett, M.R., Glasser, N.F., Hambrey, M.J., Huddart, D., Midgley, N.G., 2007. 'A test of the englacial thrusting hypothesis of ''hummocky''moraine formation: case studies from the northwest Highlands, Scotland': Comments. Boreas 36, 103-107. Lukas, S., 2007. Englacial thrusting and (hummocky) moraine formation: a reply to comments by Graham et al. (2007). Boreas 36, 108-113.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20070034825','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20070034825"><span>Trends in the Sea <span class="hlt">Ice</span> <span class="hlt">Cover</span> Using Enhanced and Compatible AMSR-E, SSM/I and SMMR Data</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.; Nishio, Fumihiko</p> <p>2007-01-01</p> <p>Arguably, the most remarkable manifestation of change in the polar regions is the rapid decline (of about -10 %/decade) in the Arctic perennial <span class="hlt">ice</span> <span class="hlt">cover</span>. Changes in the global sea <span class="hlt">ice</span> <span class="hlt">cover</span>, however, are more modest, being slightly positive in the Southern Hemisphere and slightly negative in the Northern Hemisphere, the significance of which has not been adequately assessed because of unknown errors in the satellite historical data. We take advantage of the recent and more accurate AMSR-E data to evaluate the true seasonal and interannual variability of the sea <span class="hlt">ice</span> <span class="hlt">cover</span>, assess the accuracy of historical data, and determine the real trend. Consistently derived <span class="hlt">ice</span> concentrations from AMSR-E, SSM/I, and SMMR data were analyzed and a slight bias is observed between AMSR-E and SSM/I data mainly because of differences in resolution. Analysis of the combine SMMR, SSM/I and AMSR-E data set, with the bias corrected, shows that the trends in extent and area of sea <span class="hlt">ice</span> in the Arctic region is -3.4 +/- 0.2 and -4.0 +/- 0.2 % per decade, respectively, while the corresponding values for the <span class="hlt">Antarctic</span> region is 0.9 +/- 0.2 and 1.7 .+/- 0.3 % per decade. The higher resolution of the AMSR-E provides an improved determination of the location of the <span class="hlt">ice</span> edge while the SSM/I data show an <span class="hlt">ice</span> edge about 6 to 12 km further away from the <span class="hlt">ice</span> pack. Although the current record of AMSR-E is less than 5 years, the data can be utilized in combination with historical data for more accurate determination of the variability and trends in the <span class="hlt">ice</span> <span class="hlt">cover</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017CliPa..13..959G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017CliPa..13..959G"><span><span class="hlt">Antarctic</span> climate and <span class="hlt">ice</span>-sheet configuration during the early Pliocene interglacial at 4.23 Ma</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.; Thomas, Zoë A.; Levy, Richard H.; Gasson, Edward G. W.; Naish, Timothy R.; McKay, Robert M.; Kowalewski, Douglas E.; Fogwill, Christopher J.</p> <p>2017-07-01</p> <p>The geometry of <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheets during warm periods of the geological past is difficult to determine from geological evidence, but is important to know because such reconstructions enable a more complete understanding of how the <span class="hlt">ice</span>-sheet system responds to changes in climate. Here we investigate how Antarctica evolved under orbital and greenhouse gas conditions representative of an interglacial in the early Pliocene at 4.23 Ma, when Southern Hemisphere insolation reached a maximum. Using offline-coupled climate and <span class="hlt">ice</span>-sheet models, together with a new synthesis of high-latitude palaeoenvironmental proxy data to define a likely climate envelope, we simulate a range of <span class="hlt">ice</span>-sheet geometries and calculate their likely contribution to sea level. In addition, we use these simulations to investigate the processes by which the West and East <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheets respond to environmental forcings and the timescales over which these behaviours manifest. We conclude that the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet contributed 8.6 ± 2.8 m to global sea level at this time, under an atmospheric CO2 concentration identical to present (400 ppm). Warmer-than-present ocean temperatures led to the collapse of West Antarctica over centuries, whereas higher air temperatures initiated surface melting in parts of East Antarctica that over one to two millennia led to lowering of the <span class="hlt">ice</span>-sheet surface, flotation of grounded margins in some areas, and retreat of the <span class="hlt">ice</span> sheet into the Wilkes Subglacial Basin. The results show that regional variations in climate, <span class="hlt">ice</span>-sheet geometry, and topography produce long-term sea-level contributions that are non-linear with respect to the applied forcings, and which under certain conditions exhibit threshold behaviour associated with behavioural tipping points.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMPP51C2295L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMPP51C2295L"><span>Preliminary Cosmogenic Surface Exposure Ages on Laurentide <span class="hlt">Ice</span>-sheet Retreat and Opening of the Eastern <span class="hlt">Lake</span> Agassiz Outlets</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Leydet, D.; Carlson, A. E.; Sinclair, G.; Teller, J. T.; Breckenridge, A. J.; Caffee, M. W.; Barth, A. M.</p> <p>2015-12-01</p> <p>The chronology for the eastern outlets of glacial <span class="hlt">Lake</span> Agassiz holds important consequences for the cause of Younger Dryas cold event during the last deglaciation. Eastward routing of <span class="hlt">Lake</span> Agassiz runoff was originally hypothesized to have triggered the Younger Dryas. However, currently the chronology of the eastern outlets is only constrained by minimum-limiting radiocarbon ages that could suggest the eastern outlets were still <span class="hlt">ice</span> <span class="hlt">covered</span> at the start of the Younger Dryas at ~12.9 ka BP, requiring a different forcing of this abrupt climate event. Nevertheless, the oldest radiocarbon ages are still consistent with an <span class="hlt">ice</span>-free eastern outlet at the start of the Younger Dryas. Here we will present preliminary 10-Be cosmogenic surface exposure ages from the North <span class="hlt">Lake</span>, Flat Rock <span class="hlt">Lake</span>, glacial <span class="hlt">Lake</span> Kaministiquia, and <span class="hlt">Lake</span> Nipigon outlets located near Thunder Bay, Ontario. These ages will date the timing of the deglaciation of the Laurentide <span class="hlt">ice</span> sheet in the eastern outlet region of glacial <span class="hlt">Lake</span> Agassiz. This will provide an important constraint for the hypothesized freshwater forcing of the cause of Younger Dryas cold event.</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('https://pubs.usgs.gov/of/2007/1047/srp/srp020/of2007-1047srp020.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2007/1047/srp/srp020/of2007-1047srp020.pdf"><span><span class="hlt">Antarctic</span> <span class="hlt">ice</span>-rafted detritus (IRD) in the South Atlantic: Indicators of iceshelf dynamics or ocean surface 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>Nielsen, Simon H.H.; Hodell, D.A.</p> <p>2007-01-01</p> <p>Ocean sediment core TN057-13PC4/ODP1094, from the Atlantic sector of the Southern Ocean, contains elevated lithogenic material in sections representing the last glacial period compared to the Holocene. This <span class="hlt">ice</span>-rafted detritus is mainly comprised of volcanic glass and ash, but has a significant input of what was previously interpreted as quartz during peak intervals (Kanfoush et al., 2000, 2002). Our analysis of these clear mineral grains indicates that most are plagioclase, and that South Sandwich Islands is the predominant source, similar to that inferred for the volcanic glass (Nielsen et al., in review). In addition, quartz and feldspar with possible <span class="hlt">Antarctic</span> origin occur in conjunction with postulated episodes of <span class="hlt">Antarctic</span> deglaciation. We conclude that while sea <span class="hlt">ice</span> was the dominant <span class="hlt">ice</span> rafting agent in the Polar Frontal Zone of the South Atlantic during the last glacial period, the Holocene IRD variability may reflect <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet dynamics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017QSRv..155...50M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017QSRv..155...50M"><span><span class="hlt">Ice</span> core and climate reanalysis analogs to predict <span class="hlt">Antarctic</span> and Southern Hemisphere climate changes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mayewski, P. A.; Carleton, A. M.; Birkel, S. D.; Dixon, D.; Kurbatov, A. V.; Korotkikh, E.; McConnell, J.; Curran, M.; Cole-Dai, J.; Jiang, S.; Plummer, C.; Vance, T.; Maasch, K. A.; Sneed, S. B.; Handley, M.</p> <p>2017-01-01</p> <p>A primary goal of the SCAR (Scientific Committee for <span class="hlt">Antarctic</span> Research) initiated AntClim21 (<span class="hlt">Antarctic</span> Climate in the 21st Century) Scientific Research Programme is to develop analogs for understanding past, present and future climates for the <span class="hlt">Antarctic</span> and Southern Hemisphere. In this contribution to AntClim21 we provide a framework for achieving this goal that includes: a description of basic climate parameters; comparison of existing climate reanalyses; and <span class="hlt">ice</span> core sodium records as proxies for the frequencies of marine air mass intrusion spanning the past ∼2000 years. The resulting analog examples include: natural variability, a continuation of the current trend in <span class="hlt">Antarctic</span> and Southern Ocean climate characterized by some regions of warming and some cooling at the surface of the Southern Ocean, <span class="hlt">Antarctic</span> ozone healing, a generally warming climate and separate increases in the meridional and zonal winds. We emphasize changes in atmospheric circulation because the atmosphere rapidly transports heat, moisture, momentum, and pollutants, throughout the middle to high latitudes. In addition, atmospheric circulation interacts with temporal variations (synoptic to monthly scales, inter-annual, decadal, etc.) of sea <span class="hlt">ice</span> extent and concentration. We also investigate associations between <span class="hlt">Antarctic</span> atmospheric circulation features, notably the Amundsen Sea Low (ASL), and primary climate teleconnections including the SAM (Southern Annular Mode), ENSO (El Nîno Southern Oscillation), the Pacific Decadal Oscillation (PDO), the AMO (Atlantic Multidecadal Oscillation), and solar irradiance variations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70014725','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70014725"><span>The distribution, structure, and composition of freshwater <span class="hlt">ice</span> deposits in Bolivian salt <span class="hlt">lakes</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>Hurlbert, S.H.; Chang, Cecily C.Y.</p> <p>1988-01-01</p> <p>Freshwater <span class="hlt">ice</span> deposits are described from seven, high elevation (4117-4730 m), shallow (mean depth <30 cm), saline (10-103 g l-1) <span class="hlt">lakes</span> in the southwestern corner of Bolivia. The <span class="hlt">ice</span> deposits range to several hundred meters in length and to 7 m in height above the <span class="hlt">lake</span> or playa surface. They are located near the <span class="hlt">lake</span> or salar margins; some are completely surrounded by water, others by playa deposits or salt crusts. Upper surfaces and sides of the <span class="hlt">ice</span> deposits usually are <span class="hlt">covered</span> by 20-40 cm of white to light brown, dry sedimentary materials. Calcite is the dominant crystalline mineral in these, and amorphous materials such as diatom frustules and volcanic glass are also often abundant. Beneath the dry overburden the <span class="hlt">ice</span> occurs primarily as horizontal lenses 1-1000 mm thick, irregularly alternating with strata of frozen sedimentary materials. <span class="hlt">Ice</span> represents from 10 to 87% of the volume of the deposits and yields freshwater (TFR <3 g l-1) when melted. Oxygen isotope ratios for <span class="hlt">ice</span> are similar to those for regional precipitation and shoreline seeps but much lower than those for the lakewaters. Geothermal flux is high in the region as evidenced by numerous hot springs and deep (3.0-3.5 m) sediment temperatures of 5-10??C. This flux is one cause of the present gradual wasting away of these deposits. Mean annual air temperatures for the different <span class="hlt">lakes</span> probably are all in the range of -2 to 4??C, and mean midwinter temperatures about 5??C lower. These deposits apparently formed during colder climatic conditions by the freezing of low salinity porewaters and the building up of segregation <span class="hlt">ice</span> lenses. ?? 1988 Dr W. Junk Publishers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA601068','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA601068"><span>Sunlight, Sea <span class="hlt">Ice</span>, and the <span class="hlt">Ice</span> Albedo Feedback in a Changing Arctic Sea <span class="hlt">Ice</span> <span class="hlt">Cover</span></span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2013-09-30</p> <p>Sea <span class="hlt">Ice</span> , and the <span class="hlt">Ice</span> Albedo Feedback in a...<span class="hlt">COVERED</span> 00-00-2013 to 00-00-2013 4. TITLE AND SUBTITLE Sunlight, Sea <span class="hlt">Ice</span> , and the <span class="hlt">Ice</span> Albedo Feedback in a Changing Arctic Sea <span class="hlt">Ice</span> <span class="hlt">Cover</span> 5a...during a period when incident solar irradiance is large increasing solar heat input to the <span class="hlt">ice</span> . Seasonal sea <span class="hlt">ice</span> typically has a smaller albedo</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003EAEJA.....3580D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003EAEJA.....3580D"><span>Samarium-Neodymium model age and Geochemical (Sr-Nd) signature of a bedrock inclusion from <span class="hlt">lake</span> Vostok accretion <span class="hlt">ice</span>.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Delmonte, B.; Petit, J. R.; Michard, A.; Basile-Doelsch, I.; Lipenkov, V.</p> <p>2003-04-01</p> <p>We investigated properties of the basal <span class="hlt">ice</span> from Vostok <span class="hlt">ice</span> core as well as the sediment inclusions within the accreted <span class="hlt">ice</span>. The Vostok <span class="hlt">ice</span> core preserves climatic information for the last 420 kyrs down to 3310m depth, but below this depth the horizontal layers of the climatic record are disrupted by the glacier dynamics. From 3450 m to 3538 m depth thin bedrock particles, as glacial flour, are entrapped. Glacial flour is released in the northern area <span class="hlt">lake</span>, where glacier mostly melts and contributes to sediment accumulation. In the southern area, close to Vostok station, the <span class="hlt">lake</span> water freezes and the upstream glacial flour does not contribute to sedimentation. The accreted <span class="hlt">ice</span> contains visible sediment inclusions down to 3608 m (accretion <span class="hlt">ice</span> 1), while below this depth and likely down to the water interface (˜3750 m), the <span class="hlt">ice</span> is clear (accretion <span class="hlt">ice</span> 2). The fine inclusions (1-2mm in diameter) from Accretion <span class="hlt">Ice</span> 1 mostly consist of fine clays and quartz aggregates and we suggest they are entrained into <span class="hlt">ice</span> as the glacier floats over shallow depth bay then it grounds against a relief rise. Afterward the glacier freely floats over the deep <span class="hlt">lake</span> before reaching Vostok, and accreted <span class="hlt">ice</span> 2 is clean. Sm-Nd dating of one of two inclusions at 3570 m depth gives 1.88 (+/-0.13)Ga (DM model age), corresponding to 1.47 Ga (TCHUR), suggesting a Precambrian origin. Also the isotopic signature of such inclusion (87Sr/86Sr= 0.8232 and eNd= -16) and that of a second one (87Sr/86Sr= 0.7999 and eNd= -15) are coherent with the nature of an old continental shield. Sediments that may initially accumulate in the shallow bay prior the <span class="hlt">Antarctic</span> glaciation, should have been eroded and exported out of the <span class="hlt">lake</span> by the glacier movement, this assuming processes for <span class="hlt">ice</span> accretion and for sediment entrapping operate since a long time. As the glacial flour from upstream does not contribute to sedimentation, sediments need to be renewed at the surface of the bedrock rising question about the way</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JAMES..10..262B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JAMES..10..262B"><span>A Mathematical Model of Melt <span class="hlt">Lake</span> Development on an <span class="hlt">Ice</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>Buzzard, S. C.; Feltham, D. L.; Flocco, D.</p> <p>2018-02-01</p> <p>The accumulation of surface meltwater on <span class="hlt">ice</span> shelves can lead to the formation of melt <span class="hlt">lakes</span>. Melt <span class="hlt">lakes</span> have been implicated in <span class="hlt">ice</span> shelf collapse; Antarctica's Larsen B <span class="hlt">Ice</span> Shelf was observed to have a large amount of surface melt <span class="hlt">lakes</span> present preceding its collapse in 2002. Such collapse can affect ocean circulation and temperature, cause habitat loss and contribute to sea level rise through the acceleration of tributary glaciers. We present a mathematical model of a surface melt <span class="hlt">lake</span> on an idealized <span class="hlt">ice</span> shelf. The model incorporates a calculation of the <span class="hlt">ice</span> shelf surface energy balance, heat transfer through the firn, the production and percolation of meltwater into the firn, the formation of <span class="hlt">ice</span> lenses, and the development and refreezing of surface melt <span class="hlt">lakes</span>. The model is applied to the Larsen C <span class="hlt">Ice</span> Shelf, where melt <span class="hlt">lakes</span> have been observed. This region has warmed several times the global average over the last century and the Larsen C firn layer could become saturated with meltwater by the end of the century. When forced with weather station data, our model produces surface melting, meltwater accumulation, and melt <span class="hlt">lake</span> development consistent with observations. We examine the sensitivity of <span class="hlt">lake</span> formation to uncertain parameters and provide evidence of the importance of processes such as lateral meltwater transport. We conclude that melt <span class="hlt">lakes</span> impact surface melt and firn density and warrant inclusion in dynamic-thermodynamic models of <span class="hlt">ice</span> shelf evolution within climate models, of which our model could form the basis for the thermodynamic component.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110012858','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110012858"><span>Airborne Polarimetric, Two-Color Laser Altimeter Measurements of <span class="hlt">Lake</span> <span class="hlt">Ice</span> <span class="hlt">Cover</span>: A Pathfinder for NASA's ICESat-2 Spaceflight Mission</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Harding, David; Dabney, Philip; Valett, Susan; Yu, Anthony; Vasilyev, Aleksey; Kelly, April</p> <p>2011-01-01</p> <p>The ICESat-2 mission will continue NASA's spaceflight laser altimeter measurements of <span class="hlt">ice</span> sheets, sea <span class="hlt">ice</span> and vegetation using a new measurement approach: micropulse, single photon ranging at 532 nm. Differential penetration of green laser energy into snow, <span class="hlt">ice</span> and water could introduce errors in sea <span class="hlt">ice</span> freeboard determination used for estimation of <span class="hlt">ice</span> thickness. Laser pulse scattering from these surface types, and resulting range biasing due to pulse broadening, is assessed using SIMPL airborne data acquired over icecovered <span class="hlt">Lake</span> Erie. SIMPL acquires polarimetric lidar measurements at 1064 and 532 nm using the micropulse, single photon ranging measurement approach.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040172041&hterms=balance+sheet&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dbalance%2Bsheet','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040172041&hterms=balance+sheet&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dbalance%2Bsheet"><span>Advances in Measuring <span class="hlt">Antarctic</span> Sea-<span class="hlt">Ice</span> Thickness and <span class="hlt">Ice</span>-Sheet Elevations with ICESat Laser Altimetry</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zwally, H. Jay</p> <p>2004-01-01</p> <p>NASA's <span class="hlt">Ice</span>, Cloud and Land Elevation Satellite (ICESat) has been measuring elevations of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet and sea-<span class="hlt">ice</span> freeboard elevations with unprecedented accuracy. Since February 20,2003, data has been acquired during three periods of laser operation varying from 36 to 54 days, which is less than the continuous operation of 3 to 5 years planned for the mission. The primary purpose of ICESat is to measure time-series of <span class="hlt">ice</span>-sheet elevation changes for determination of the present-day mass balance of the <span class="hlt">ice</span> sheets, study of associations between observed <span class="hlt">ice</span> changes and polar climate, and estimation of the present and future contributions of the <span class="hlt">ice</span> sheets to global sea level rise. ICESat data will continue to be acquired for approximately 33 days periods at 3 to 6 month intervals with the second of ICESat's three lasers, and eventually with the third laser. The laser footprints are about 70 m on the surface and are spaced at 172 m along-track. The on-board GPS receiver enables radial orbit determinations to an accuracy better than 5 cm. The orbital altitude is around 600 km at an inclination of 94 degrees with a 8-day repeat pattern for the calibration and validation period, followed by a 91 -day repeat period for the rest of the mission. The expected range precision of single footprint measurements was 10 cm, but the actual range precision of the data has been shown to be much better at 2 to 3 cm. The star-tracking attitude-determination system should enable footprints to be located to 6 m horizontally when attitude calibrations are completed. With the present attitude calibration, the elevation accuracy over the <span class="hlt">ice</span> sheets ranges from about 30 cm over the low-slope areas to about 80 cm over areas with slopes of 1 to 2 degrees, which is much better than radar altimetry. After the first period of data collection, the spacecraft attitude was controlled to point the laser beam to within 50 m of reference surface tracks over the <span class="hlt">ice</span> sheets. Detection of <span class="hlt">ice</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.V13D2642I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.V13D2642I"><span>Improvements in the chronology, geochemistry and correlation techniques of tephra in <span class="hlt">Antarctic</span> <span class="hlt">ice</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Iverson, N. A.; Dunbar, N. W.; McIntosh, W. C.; Pearce, N. J.; Kyle, P. R.</p> <p>2013-12-01</p> <p>Visible and crypto tephra layers found in West <span class="hlt">Antarctic</span> <span class="hlt">ice</span> provide an excellent record of <span class="hlt">Antarctic</span> volcanism over the past 100ka. Tephra layers are deposited almost instantaneously across wide areas creating horizons that, if found in several locations, provide 'pinning points' to adjust <span class="hlt">ice</span> time scales that may otherwise be lacking detailed chronology. Individual tephra layers can have distinct chemical fingerprints allowing them to correlate over great distances. Advances in sample preparation, geochemical analyses (major and trace elements) of fine grained tephra and higher precision 40Ar/39Ar dating of young (<100ka) proximal volcanic deposits are improving an already established tephra record in West Antarctica. Forty three of the potential hundreds of silicate layers found in a recently drilled deep West <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet Divide core (WDC06A) have been analyzed for major elements and a subset for trace elements. Of these layers, at least 16 are homogenous tephra that could be correlated to other <span class="hlt">ice</span> cores (e.g. Siple Dome, SDMA) and/or to source volcanoes found throughout Antarctica and even extra-continental eruptions (e.g. Sub-<span class="hlt">Antarctic</span> islands and South America). Combining <span class="hlt">ice</span> core tephra with those exposed in blue <span class="hlt">ice</span> areas provide more locations to correlate widespread eruptions. For example, a period of heightened eruptive activity at Mt. Berlin, West Antarctica between 24 and 28ka produced a set of tephra layers that are found in WDC06A and SDMA <span class="hlt">ice</span> cores, as well as at a nearby blue <span class="hlt">ice</span> area at Mt. Moulton (BIT-151 and BIT-152). Possible correlative tephra layers are found at <span class="hlt">ice</span> ages of 26.4, 26.9 and 28.8ka in WDC06A and 26.5, 27.0, and 28.7ka in SDMA cores. The geochemical similarities of major elements in these layers mean that ongoing trace element analyses will be vital to decipher the sequence of events during this phase of activity at Mt. Berlin. Sample WDC06A-2767.117 (<span class="hlt">ice</span> age of 28.6×1.0ka) appears to correlate to blue <span class="hlt">ice</span> tephra BIT</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.nsf.gov/pubs/2005/nsf0539/nsf0539_5.pdf','USGSPUBS'); return false;" href="http://www.nsf.gov/pubs/2005/nsf0539/nsf0539_5.pdf"><span>Correlated declines in Pacific arctic snow and sea <span class="hlt">ice</span> <span class="hlt">cover</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>Stone, Robert P.; Douglas, David C.; Belchansky, Gennady I.; Drobot, Sheldon</p> <p>2005-01-01</p> <p>Simulations of future climate suggest that global warming will reduce Arctic snow and <span class="hlt">ice</span> <span class="hlt">cover</span>, resulting in decreased surface albedo (reflectivity). Lowering of the surface albedo leads to further warming by increasing solar absorption at the surface. This phenomenon is referred to as “temperature–albedo feedback.” Anticipation of such a feedback is one reason why scientists look to the Arctic for early indications of global warming. Much of the Arctic has warmed significantly. Northern Hemisphere snow <span class="hlt">cover</span> has decreased, and sea <span class="hlt">ice</span> has diminished in area and thickness. As reported in the Arctic Climate Impact Assessment in 2004, the trends are considered to be outside the range of natural variability, implicating global warming as an underlying cause. Changing climatic conditions in the high northern latitudes have influenced biogeochemical cycles on a broad scale. Warming has already affected the sea <span class="hlt">ice</span>, the tundra, the plants, the animals, and the indigenous populations that depend on them. Changing annual cycles of snow and sea <span class="hlt">ice</span> also affect sources and sinks of important greenhouse gases (such as carbon dioxide and methane), further complicating feedbacks involving the global budgets of these important constituents. For instance, thawing permafrost increases the extent of tundra wetlands and <span class="hlt">lakes</span>, releasing greater amounts of methane into the atmosphere. Variable sea <span class="hlt">ice</span> <span class="hlt">cover</span> may affect the hemispheric carbon budget by altering the ocean–atmosphere exchange of carbon dioxide. There is growing concern that amplification of global warming in the Arctic will have far-reaching effects on lower latitude climate through these feedback mechanisms. Despite the diverse and convincing observational evidence that the Arctic environment is changing, it remains unclear whether these changes are anthropogenically forced or result from natural variations of the climate system. A better understanding of what controls the seasonal distributions of snow and <span class="hlt">ice</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017IzAOP..53.1050K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017IzAOP..53.1050K"><span>The First Results of Monitoring the Formation and Destruction of the <span class="hlt">Ice</span> <span class="hlt">Cover</span> in Winter 2014-2015 on Ilmen <span class="hlt">Lake</span> according to the Measurements of Dual-Frequency Precipitation Radar</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Karaev, V. Yu.; Panfilova, M. A.; Titchenko, Yu. A.; Meshkov, E. M.; Balandina, G. N.; Andreeva, Z. V.</p> <p>2017-12-01</p> <p>The launch of the Dual-frequency Precipitation Radar (DPR) opens up new opportunities for studying and monitoring the land and inland waters. It is the first time radar with a swath (±65°) <span class="hlt">covering</span> regions with cold climate where waters are <span class="hlt">covered</span> with <span class="hlt">ice</span> and land with snow for prolonged periods of time has been used. It is also the first time that the remote sensing is carried out at small incidence angles (less than 19°) at two frequencies (13.6 and 35.5 GHz). The high spatial resolution (4-5 km) significantly increases the number of objects that can be studied using the new radar. Ilmen <span class="hlt">Lake</span> is chosen as the first test object for the development of complex programs for processing and analyzing data obtained by the DPR. The problem of diagnostics of <span class="hlt">ice-cover</span> formation and destruction according to DPR data has been considered. It is shown that the dependence of the radar backscatter cross section on the incidence angle for autumn <span class="hlt">ice</span> is different from that of spring <span class="hlt">ice</span>, and can be used for classification. A comparison with scattering on the water surface has shown that, at incidence angles exceeding 10°, it is possible to discern all three types of reflecting surfaces: open water, autumn <span class="hlt">ice</span>, and spring <span class="hlt">ice</span>, under the condition of making repeated measurements to avoid possible ambiguity caused by wind.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17314977','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17314977"><span>Large subglacial <span class="hlt">lakes</span> in East Antarctica at the onset of fast-flowing <span class="hlt">ice</span> streams.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bell, Robin E; Studinger, Michael; Shuman, Christopher A; Fahnestock, Mark A; Joughin, Ian</p> <p>2007-02-22</p> <p>Water plays a crucial role in <span class="hlt">ice</span>-sheet stability and the onset of <span class="hlt">ice</span> streams. Subglacial <span class="hlt">lake</span> water moves between <span class="hlt">lakes</span> and rapidly drains, causing catastrophic floods. The exact mechanisms by which subglacial <span class="hlt">lakes</span> influence <span class="hlt">ice</span>-sheet dynamics are unknown, however, and large subglacial <span class="hlt">lakes</span> have not been closely associated with rapidly flowing <span class="hlt">ice</span> streams. Here we use satellite imagery and <span class="hlt">ice</span>-surface elevations to identify a region of subglacial <span class="hlt">lakes</span>, similar in total area to <span class="hlt">Lake</span> Vostok, at the onset region of the Recovery Glacier <span class="hlt">ice</span> stream in East Antarctica and predicted by <span class="hlt">ice</span>-sheet models. We define four <span class="hlt">lakes</span> through extensive, flat, featureless regions of <span class="hlt">ice</span> surface bounded by upstream troughs and downstream ridges. Using <span class="hlt">ice</span> velocities determined using interferometric synthetic aperture radar (InSAR), we find the onset of rapid flow (moving at 20 to 30 m yr(-1)) of the tributaries to the Recovery Glacier <span class="hlt">ice</span> stream in a 280-km-wide segment at the downslope margins of these four subglacial <span class="hlt">lakes</span>. We conclude that the subglacial <span class="hlt">lakes</span> initiate and maintain rapid <span class="hlt">ice</span> flow through either active modification of the basal thermal regime of the <span class="hlt">ice</span> sheet by <span class="hlt">lake</span> accretion or through scouring bedrock channels in periodic drainage events. We suggest that the role of subglacial <span class="hlt">lakes</span> needs to be considered in <span class="hlt">ice</span>-sheet mass balance assessments.</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> <span class="hlt">ice</span> 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> <span class="hlt">ice</span> sheet (WAIS), with <span class="hlt">ice</span> volume equivalent to approximately 5 m of sea level, has long been considered capable of past and future catastrophic collapse. Today, the <span class="hlt">ice</span> sheet is fringed by vulnerable floating <span class="hlt">ice</span> shelves that buttress the fast flow of inland <span class="hlt">ice</span> 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 <span class="hlt">ice</span> sheet/<span class="hlt">ice</span> shelf model capable of high-resolution nesting with a new treatment of grounding-line dynamics and <span class="hlt">ice</span>-shelf buttressing to simulate <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet variations over the past five million years. Modelled WAIS variations range from full glacial extents with grounding lines near the continental shelf break, intermediate states similar to modern, and brief but dramatic retreats, leaving only small, isolated <span class="hlt">ice</span> caps on West <span class="hlt">Antarctic</span> islands. Transitions between glacial, intermediate 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('https://ntrs.nasa.gov/search.jsp?R=20160007571&hterms=information&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dinformation','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20160007571&hterms=information&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dinformation"><span>New Visualizations Highlight New Information on the Contrasting Arctic and <span class="hlt">Antarctic</span> Sea-<span class="hlt">Ice</span> Trends Since the Late 1970s</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Parkinson, Claire L.; DiGirolamo, Nicolo E.</p> <p>2016-01-01</p> <p>Month-by-month ranking of 37 years (1979-2015) of satellite-derived sea-<span class="hlt">ice</span> extents in the Arctic and <span class="hlt">Antarctic</span> reveals interesting new details in the overall trends toward decreasing sea-<span class="hlt">ice</span> coverage in the Arctic and increasing sea-<span class="hlt">ice</span> coverage in the <span class="hlt">Antarctic</span>. The Arctic decreases are so definitive that there has not been a monthly record high in Arctic sea-<span class="hlt">ice</span> extents in any month since 1986, a time period during which there have been 75 monthly record lows. The <span class="hlt">Antarctic</span>, with the opposite but weaker trend toward increased <span class="hlt">ice</span> extents, experienced monthly record lows in 5 months of 1986, then 6 later monthly record lows scattered through the dataset, with the last two occurring in 2006, versus 45 record highs since 1986. However, in the last three years of the 1979-2015 dataset, the downward trends in Arctic sea-<span class="hlt">ice</span> extents eased up, with no new record lows in any month of 2013 or 2014 and only one record low in 2015,while the upward trends in <span class="hlt">Antarctic</span> <span class="hlt">ice</span> extents notably strengthened, with new record high <span class="hlt">ice</span> extents in 4 months (August-November) of 2013, in 6 months (April- September) of 2014, and in 3 months (January, April, and May) of 2015. Globally, there have been only 3 monthly record highs since 1986 (only one since 1988), whereas there have been 43 record lows, although the last record lows (in the 1979-2015 dataset) occurred in 2012.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29284198','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29284198"><span>Signals from the south; humpback whales carry messages of <span class="hlt">Antarctic</span> sea-<span class="hlt">ice</span> ecosystem variability.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bengtson Nash, Susan M; Castrillon, Juliana; Eisenmann, Pascale; Fry, Brian; Shuker, Jon D; Cropp, Roger A; Dawson, Amanda; Bignert, Anders; Bohlin-Nizzetto, Pernilla; Waugh, Courtney A; Polkinghorne, Bradley J; Dalle Luche, Greta; McLagan, David</p> <p>2018-04-01</p> <p>Southern hemisphere humpback whales (Megaptera novaeangliae) rely on summer prey abundance of <span class="hlt">Antarctic</span> krill (Euphausia superba) to fuel one of the longest-known mammalian migrations on the planet. It is hypothesized that this species, already adapted to endure metabolic extremes, will be one of the first <span class="hlt">Antarctic</span> consumers to show measurable physiological change in response to fluctuating prey availability in a changing climate; and as such, a powerful sentinel candidate for the <span class="hlt">Antarctic</span> sea-<span class="hlt">ice</span> ecosystem. Here, we targeted the sentinel parameters of humpback whale adiposity and diet, using novel, as well as established, chemical and biochemical markers, and assembled a time trend spanning 8 years. We show the synchronous, inter-annual oscillation of two measures of humpback whale adiposity with Southern Ocean environmental variables and climate indices. Furthermore, bulk stable isotope signatures provide clear indication of dietary compensation strategies, or a lower trophic level isotopic change, following years indicated as leaner years for the whales. The observed synchronicity of humpback whale adiposity and dietary markers, with climate patterns in the Southern Ocean, lends strength to the role of humpback whales as powerful <span class="hlt">Antarctic</span> sea-<span class="hlt">ice</span> ecosystem sentinels. The work carries significant potential to reform current ecosystem surveillance in the <span class="hlt">Antarctic</span> region. © 2017 John Wiley & Sons Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C11B0906W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C11B0906W"><span>Gaussian Process Model for <span class="hlt">Antarctic</span> Surface Mass Balance and <span class="hlt">Ice</span> Core Site Selection</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>White, P. A.; Reese, S.; Christensen, W. F.; Rupper, S.</p> <p>2017-12-01</p> <p>Surface mass balance (SMB) is an important factor in the estimation of sea level change, and data are collected to estimate models for prediction of SMB on the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet. Using Favier et al.'s (2013) quality-controlled aggregate data set of SMB field measurements, a fully Bayesian spatial model is posed to estimate <span class="hlt">Antarctic</span> SMB and propose new field measurement locations. Utilizing Nearest-Neighbor Gaussian process (NNGP) models, SMB is estimated over the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet. An <span class="hlt">Antarctic</span> SMB map is rendered using this model and is compared with previous estimates. A prediction uncertainty map is created to identify regions of high SMB uncertainty. The model estimates net SMB to be 2173 Gton yr-1 with 95% credible interval (2021,2331) Gton yr-1. On average, these results suggest lower <span class="hlt">Antarctic</span> SMB and higher uncertainty than previously purported [Vaughan et al. (1999); Van de Berg et al. (2006); Arthern, Winebrenner and Vaughan (2006); Bromwich et al. (2004); Lenaerts et al. (2012)], even though this model utilizes significantly more observations than previous models. Using the Gaussian process' uncertainty and model parameters, we propose 15 new measurement locations for field study utilizing a maximin space-filling, error-minimizing design; these potential measurements are identied to minimize future estimation uncertainty. Using currently accepted <span class="hlt">Antarctic</span> mass balance estimates and our SMB estimate, we estimate net mass loss [Shepherd et al. (2012); Jacob et al. (2012)]. Furthermore, we discuss modeling details for both space-time data and combining field measurement data with output from mathematical models using the NNGP framework.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JVGR..297...89C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JVGR..297...89C"><span>Volcano-<span class="hlt">ice</span>-sea interaction in the Cerro Santa Marta area, northwest James Ross Island, <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>Calabozo, Fernando M.; Strelin, Jorge A.; Orihashi, Yuji; Sumino, Hirochika; Keller, Randall A.</p> <p>2015-05-01</p> <p>We present here the results of detailed mapping, lithofacies analysis and stratigraphy of the Neogene James Ross Island Volcanic Group (<span class="hlt">Antarctic</span> Peninsula) in the Cerro Santa Marta area (northwest of James Ross Island), in order to give constraints on the evolution of a glaciated volcanic island. Our field results included recognition and interpretation of seventeen volcanic and glacial lithofacies, together with their vertical and lateral arrangements, supported by four new unspiked K-Ar ages. This allowed us to conclude that the construction of the volcanic pile in this area took place during two main eruptive stages (Eruptive Stages 1 and 2), separated from the Cretaceous bedrock and from each other by two major glacial unconformities (U1 and U2). The U1 unconformity is related to <span class="hlt">Antarctic</span> Peninsula <span class="hlt">Ice</span> sheet expansion during the late Miocene (before 6.2 Ma) and deposition of glacial lithofacies in a glaciomarine setting. Following this glacial advance, Eruptive Stage 1 (6.2-4.6 Ma) volcanism started with subaerial extrusion of lava flows from an unrecognized vent north of the study area, with eruptions later fed from vent/s centered at Cerro Santa Marta volcano, where cinder cone deposits and a volcanic conduit/lava <span class="hlt">lake</span> are preserved. These lava flows fed an extensive (> 7 km long) hyaloclastite delta system that was probably emplaced in a shallow marine environment. A second unconformity (U2) was related to expansion of a local <span class="hlt">ice</span> cap, centered on James Ross Island, which truncated all the eruptive units of Eruptive Stage 1. Concomitant with glacier advance, renewed volcanic activity (Eruptive Stage 2) started after 4.6 Ma and volcanic products were fed again by Cerro Santa Marta vents. We infer that glaciovolcanic eruptions occurred under a moderately thin (~ 300 m) glacier, in good agreement with previous estimates of paleo-<span class="hlt">ice</span> thickness for the James Ross Island area during the Pliocene.</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 <span class="hlt">ice</span> <span class="hlt">cover</span> 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 <span class="hlt">lakes</span>. 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/2016PhDT........12M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PhDT........12M"><span>Age, origin and evolution of <span class="hlt">Antarctic</span> debris-<span class="hlt">covered</span> glaciers: Implications for landscape evolution and long-term climate change</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mackay, Sean Leland</p> <p></p> <p><span class="hlt">Antarctic</span> debris-<span class="hlt">covered</span> glaciers are potential archives of long-term climate change. However, the geomorphic response of these systems to climate forcing is not well understood. To address this concern, I conducted a series of field-based and numerical modeling studies in the McMurdo Dry Valleys of Antarctica (MDV), with a focus on Mullins and Friedman glaciers. I used data and results from geophysical surveys, <span class="hlt">ice</span>-core collection and analysis, geomorphic mapping, micro-meteorological stations, and numerical-process models to (1) determine the precise origin and distribution of englacial and supraglacial debris within these buried-<span class="hlt">ice</span> systems, (2) quantify the fundamental processes and feedbacks that govern interactions among englacial and supraglacial debris, (3) establish a process-based model to quantify the inventory of cosmogenic nuclides within englacial and supraglacial debris, and (4) isolate the governing relationships between the evolution of englacial /supraglacial debris and regional climate forcing. Results from 93 field excavations, 21 <span class="hlt">ice</span> cores, and 24 km of ground-penetrating radar data show that Mullins and Friedman glaciers contain vast areas of clean glacier <span class="hlt">ice</span> interspersed with inclined layers of concentrated debris. The similarity in the pattern of englacial debris bands across both glaciers, along with model results that call for negligible basal entrainment, is best explained by episodic environmental change at valley headwalls. To constrain better the timing of debris-band formation, I developed a modeling framework that tracks the accumulation of cosmogenic 3He in englacial and supraglacial debris. Results imply that <span class="hlt">ice</span> within Mullins Glacier increases in age non-linearly from 12 ka to ˜220 ka in areas of active flow (up to >> 1.6 Ma in areas of slow-moving-to-stagnant <span class="hlt">ice</span>) and that englacial debris bands originate with a periodicity of ˜41 ka. Modeling studies suggest that debris bands originate in synchronicity with changes in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1997JCli...10..593W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1997JCli...10..593W"><span>Modeling of <span class="hlt">Antarctic</span> Sea <span class="hlt">Ice</span> in a General Circulation Model.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wu, Xingren; Simmonds, Ian; Budd, W. F.</p> <p>1997-04-01</p> <p>A dynamic-thermodynamic sea <span class="hlt">ice</span> model is developed and coupled with the Melbourne University general circulation model to simulate the seasonal cycle of the <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> distribution. The model is efficient, rapid to compute, and useful for a range of climate studies. The thermodynamic part of the sea <span class="hlt">ice</span> model is similar to that developed by Parkinson and Washington, the dynamics contain a simplified <span class="hlt">ice</span> rheology that resists compression. The thermodynamics is based on energy conservation at the top surface of the <span class="hlt">ice</span>/snow, the <span class="hlt">ice</span>/water interface, and the open water area to determine the <span class="hlt">ice</span> formation, accretion, and ablation. A lead parameterization is introduced with an effective partitioning scheme for freezing between and under the <span class="hlt">ice</span> floes. The dynamic calculation determines the motion of <span class="hlt">ice</span>, which is forced with the atmospheric wind, taking account of <span class="hlt">ice</span> resistance and rafting. The simulated sea <span class="hlt">ice</span> distribution compares reasonably well with observations. The seasonal cycle of <span class="hlt">ice</span> extent is well simulated in phase as well as in magnitude. Simulated sea <span class="hlt">ice</span> thickness and concentration are also in good agreement with observations over most regions and serve to indicate the importance of advection and ocean drift in the determination of the sea <span class="hlt">ice</span> distribution.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_23 --> <div id="page_24" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="461"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/484365-modeling-antarctic-sea-ice-general-circulation-model','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/484365-modeling-antarctic-sea-ice-general-circulation-model"><span>Modeling of <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> in a general circulation model</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Wu, Xingren; Budd, W.F.; Simmonds, I.</p> <p>1997-04-01</p> <p>A dynamic-thermodynamic sea <span class="hlt">ice</span> model is developed and coupled with the Melbourne University general circulation model to simulate the seasonal cycle of the <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> distributions The model is efficient, rapid to compute, and useful for a range of climate studies. The thermodynamic part of the sea <span class="hlt">ice</span> model is similar to that developed by Parkinson and Washington, the dynamics contain a simplified <span class="hlt">ice</span> rheology that resists compression. The thermodynamics is based on energy conservation at the top surface of the <span class="hlt">ice</span>/snow, the <span class="hlt">ice</span>/water interface, and the open water area to determine the <span class="hlt">ice</span> formation, accretion, and ablation. Amore » lead parameterization is introduced with an effective partitioning scheme for freezing between and under the <span class="hlt">ice</span> floes. The dynamic calculation determines the motion of <span class="hlt">ice</span>, which is forced with the atmospheric wind, taking account of <span class="hlt">ice</span> resistance and rafting. The simulated sea <span class="hlt">ice</span> distribution compares reasonably well with observations. The seasonal cycle of <span class="hlt">ice</span> extent is well simulated in phase as well as in magnitude. Simulated sea <span class="hlt">ice</span> thickness and concentration are also in good agreement with observations over most regions and serve to indicate the importance of advection and ocean drift in the determination of the sea <span class="hlt">ice</span> distribution. 64 refs., 15 figs., 2 tabs.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ClDy...50.4599S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ClDy...50.4599S"><span>Tropically driven and externally forced patterns of <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> change: reconciling observed and modeled trends</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schneider, David P.; Deser, Clara</p> <p>2018-06-01</p> <p>Recent work suggests that natural variability has played a significant role in the increase of <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> extent during 1979-2013. The <span class="hlt">ice</span> extent has responded strongly to atmospheric circulation changes, including a deepened Amundsen Sea Low (ASL), which in part has been driven by tropical variability. Nonetheless, this increase has occurred in the context of externally forced climate change, and it has been difficult to reconcile observed and modeled <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> trends. To understand observed-model disparities, this work defines the internally driven and radiatively forced patterns of <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> change and exposes potential model biases using results from two sets of historical experiments of a coupled climate model compared with observations. One ensemble is constrained only by external factors such as greenhouse gases and stratospheric ozone, while the other explicitly accounts for the influence of tropical variability by specifying observed SST anomalies in the eastern tropical Pacific. The latter experiment reproduces the deepening of the ASL, which drives an increase in regional <span class="hlt">ice</span> extent due to enhanced <span class="hlt">ice</span> motion and sea surface cooling. However, the overall sea <span class="hlt">ice</span> trend in every ensemble member of both experiments is characterized by <span class="hlt">ice</span> loss and is dominated by the forced pattern, as given by the ensemble-mean of the first experiment. This pervasive <span class="hlt">ice</span> loss is associated with a strong warming of the ocean mixed layer, suggesting that the ocean model does not locally store or export anomalous heat efficiently enough to maintain a surface environment conducive to sea <span class="hlt">ice</span> expansion. The pervasive upper-ocean warming, not seen in observations, likely reflects ocean mean-state biases.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ClDy..tmp..676S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ClDy..tmp..676S"><span>Tropically driven and externally forced patterns of <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> change: reconciling observed and modeled trends</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schneider, David P.; Deser, Clara</p> <p>2017-09-01</p> <p>Recent work suggests that natural variability has played a significant role in the increase of <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> extent during 1979-2013. The <span class="hlt">ice</span> extent has responded strongly to atmospheric circulation changes, including a deepened Amundsen Sea Low (ASL), which in part has been driven by tropical variability. Nonetheless, this increase has occurred in the context of externally forced climate change, and it has been difficult to reconcile observed and modeled <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> trends. To understand observed-model disparities, this work defines the internally driven and radiatively forced patterns of <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> change and exposes potential model biases using results from two sets of historical experiments of a coupled climate model compared with observations. One ensemble is constrained only by external factors such as greenhouse gases and stratospheric ozone, while the other explicitly accounts for the influence of tropical variability by specifying observed SST anomalies in the eastern tropical Pacific. The latter experiment reproduces the deepening of the ASL, which drives an increase in regional <span class="hlt">ice</span> extent due to enhanced <span class="hlt">ice</span> motion and sea surface cooling. However, the overall sea <span class="hlt">ice</span> trend in every ensemble member of both experiments is characterized by <span class="hlt">ice</span> loss and is dominated by the forced pattern, as given by the ensemble-mean of the first experiment. This pervasive <span class="hlt">ice</span> loss is associated with a strong warming of the ocean mixed layer, suggesting that the ocean model does not locally store or export anomalous heat efficiently enough to maintain a surface environment conducive to sea <span class="hlt">ice</span> expansion. The pervasive upper-ocean warming, not seen in observations, likely reflects ocean mean-state biases.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19900060082&hterms=classification+passive&qs=N%3D0%26Ntk%3DTitle%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dclassification%2Bpassive','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19900060082&hterms=classification+passive&qs=N%3D0%26Ntk%3DTitle%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dclassification%2Bpassive"><span>Arctic multiyear <span class="hlt">ice</span> classification and summer <span class="hlt">ice</span> <span class="hlt">cover</span> using passive microwave satellite data</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Comiso, J. C.</p> <p>1990-01-01</p> <p>Passive microwave data collected by Nimbus 7 were used to classify and monitor the Arctic multilayer sea <span class="hlt">ice</span> <span class="hlt">cover</span>. Sea <span class="hlt">ice</span> concentration maps during several summer minima are analyzed to obtain estimates of <span class="hlt">ice</span> floes that survived summer, and the results are compared with multiyear-<span class="hlt">ice</span> concentrations derived from these data by using an algorithm that assumes a certain emissivity for multiyear <span class="hlt">ice</span>. The multiyear <span class="hlt">ice</span> <span class="hlt">cover</span> inferred from the winter data was found to be about 25 to 40 percent less than the summer <span class="hlt">ice-cover</span> minimum, indicating that the multiyear <span class="hlt">ice</span> <span class="hlt">cover</span> in winter is inadequately represented by the passive microwave winter data and that a significant fraction of the Arctic multiyear <span class="hlt">ice</span> floes exhibits a first-year <span class="hlt">ice</span> signature.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1912084K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1912084K"><span>Impact of surface melt and ponding on the stability of Larsen C <span class="hlt">Ice</span> Shelf, <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>Kulessa, Bernd; Luckman, Adrian; Hubbard, Bryn; Bevan, Suzanne; O'Leary, Martin; Ashmore, David; Kuipers Munneke, Peter; Jansen, Daniela; Booth, Adam; Sevestre, Heidi; Holland, Paul; McGrath, Daniel; Brisbourne, Alex; Rutt, Ian</p> <p>2017-04-01</p> <p>Several <span class="hlt">ice</span> shelves on the <span class="hlt">Antarctic</span> Peninsula have disintegrated rapidly in recent decades, and surface meltwater is strongly implicated as a driver. The Larsen C <span class="hlt">Ice</span> Shelf is the largest <span class="hlt">ice</span> shelf on the peninsula and one of the largest in Antarctica, and is subject to pronounced surface melting and meltwater ponding, especially in the northern sectors and landward inlets. As part of the MIDAS project we have investigated the structure and physical properties of the firn and <span class="hlt">ice</span> layers in the 2014/15 and 2015/16 austral summers, using a combination of radar and seismic geophysical surveys together with hot water drilling and borehole optical televiewing and temperature measurements. We found that Larsen C's firn column and <span class="hlt">ice</span> temperatures are modified strongly by surface melting and ponding, including the presence of massive <span class="hlt">ice</span> bodies in the Cabinet and Whirlwind inlets. Numerical modelling reveals that these modifications have been altering <span class="hlt">ice</span> shelf deformation, flow and fracture significantly. The findings from our MIDAS project thus suggest that the response of <span class="hlt">Antarctic</span> <span class="hlt">ice</span> shelves to climatic warming is more complex than previously thought.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoRL..45.4114P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoRL..45.4114P"><span>Bedrock Erosion Surfaces Record Former East <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet Extent</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Paxman, Guy J. G.; Jamieson, Stewart S. R.; Ferraccioli, Fausto; Bentley, Michael J.; Ross, Neil; Armadillo, Egidio; Gasson, Edward G. W.; Leitchenkov, German; DeConto, Robert M.</p> <p>2018-05-01</p> <p>East Antarctica hosts large subglacial basins into which the East <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet (EAIS) likely retreated during past warmer climates. However, the extent of retreat remains poorly constrained, making quantifying past and predicted future contributions to global sea level rise from these marine basins challenging. Geomorphological analysis and flexural modeling within the Wilkes Subglacial Basin are used to reconstruct the <span class="hlt">ice</span> margin during warm intervals of the Oligocene-Miocene. Flat-lying bedrock plateaus are indicative of an <span class="hlt">ice</span> sheet margin positioned >400-500 km inland of the modern grounding zone for extended periods of the Oligocene-Miocene, equivalent to a 2-m rise in global sea level. Our findings imply that if major EAIS retreat occurs in the future, isostatic rebound will enable the plateau surfaces to act as seeding points for extensive <span class="hlt">ice</span> rises, thus limiting extensive <span class="hlt">ice</span> margin retreat of the scale seen during the early EAIS.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5013606','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5013606"><span>Source identification and distribution reveals the potential of the geochemical <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> proxy IPSO25</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Belt, S. T.; Smik, L.; Brown, T. A.; Kim, J.-H.; Rowland, S. J.; Allen, C. S.; Gal, J.-K.; Shin, K.-H.; Lee, J. I.; Taylor, K. W. R.</p> <p>2016-01-01</p> <p>The presence of a di-unsaturated highly branched isoprenoid (HBI) lipid biomarker (diene II) in Southern Ocean sediments has previously been proposed as a proxy measure of palaeo <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span>. Here we show that a source of diene II is the sympagic diatom Berkeleya adeliensis Medlin. Furthermore, the propensity for B. adeliensis to flourish in platelet <span class="hlt">ice</span> is reflected by an offshore downward gradient in diene II concentration in >100 surface sediments from <span class="hlt">Antarctic</span> coastal and near-coastal environments. Since platelet <span class="hlt">ice</span> formation is strongly associated with super-cooled freshwater inflow, we further hypothesize that sedimentary diene II provides a potentially sensitive proxy indicator of landfast sea <span class="hlt">ice</span> influenced by meltwater discharge from nearby glaciers and <span class="hlt">ice</span> shelves, and re-examination of some previous diene II downcore records supports this hypothesis. The term IPSO25—<span class="hlt">Ice</span> Proxy for the Southern Ocean with 25 carbon atoms—is proposed as a proxy name for diene II. PMID:27573030</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013Sci...341..266R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013Sci...341..266R"><span><span class="hlt">Ice</span>-Shelf Melting Around Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rignot, E.; Jacobs, S.; Mouginot, J.; Scheuchl, B.</p> <p>2013-07-01</p> <p>We compare the volume flux divergence of <span class="hlt">Antarctic</span> <span class="hlt">ice</span> shelves in 2007 and 2008 with 1979 to 2010 surface accumulation and 2003 to 2008 thinning to determine their rates of melting and mass balance. Basal melt of 1325 ± 235 gigatons per year (Gt/year) exceeds a calving flux of 1089 ± 139 Gt/year, making <span class="hlt">ice</span>-shelf melting the largest ablation process in Antarctica. The giant cold-cavity Ross, Filchner, and Ronne <span class="hlt">ice</span> shelves <span class="hlt">covering</span> two-thirds of the total <span class="hlt">ice</span>-shelf area account for only 15% of net melting. Half of the meltwater comes from 10 small, warm-cavity Southeast Pacific <span class="hlt">ice</span> shelves occupying 8% of the area. A similar high melt/area ratio is found for six East <span class="hlt">Antarctic</span> <span class="hlt">ice</span> shelves, implying undocumented strong ocean thermal forcing on their deep grounding lines.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017E%26PSL.478....1P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017E%26PSL.478....1P"><span>Evidence for a dynamic East <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet during the mid-Miocene climate transition</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pierce, Elizabeth L.; van de Flierdt, Tina; Williams, Trevor; Hemming, Sidney R.; Cook, Carys P.; Passchier, Sandra</p> <p>2017-11-01</p> <p>The East <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet underwent a major expansion during the Mid-Miocene Climate Transition, around 14 Ma, lowering sea level by ∼60 m. However, direct or indirect evidence of where changes in the <span class="hlt">ice</span> sheet occurred is limited. Here we present new insights on timing and locations of <span class="hlt">ice</span> sheet change from two drill sites offshore East Antarctica. IODP Site U1356, Wilkes Land, and ODP Site 1165, Prydz Bay are located adjacent to two major <span class="hlt">ice</span> drainage areas, the Wilkes Subglacial Basin and the Lambert Graben. <span class="hlt">Ice</span>-rafted detritus (IRD), including dropstones, was deposited in concentrations far exceeding those known in the rest of the Miocene succession at both sites between 14.1 and 13.8 Ma, indicating that large amounts of IRD-bearing icebergs were calved from independent drainage basins during this relatively short interval. At Site U1356, the IRD was delivered in distinct pulses, suggesting that the overall <span class="hlt">ice</span> advance was punctuated by short periods of <span class="hlt">ice</span> retreat in the Wilkes Subglacial Basin. Provenance analysis of the mid-Miocene IRD and fine-grained sediments provides additional insights on the movement of the <span class="hlt">ice</span> margin and subglacial geology. At Site U1356, the dominant 40Ar/39Ar thermochronological age of the <span class="hlt">ice</span>-rafted hornblende grains is 1400-1550 Ma, differing from the majority of recent IRD in the area, from which we infer an inland source area of this thermochronological age extending along the eastern part of the Adélie Craton, which forms the western side of the Wilkes Subglacial Basin. Neodymium isotopic compositions from the terrigenous fine fraction at Site U1356 imply that the <span class="hlt">ice</span> margin periodically expanded from high ground well into the Wilkes Subglacial Basin during periods of MMCT <span class="hlt">ice</span> growth. At Site 1165, MMCT pebble-sized IRD are sourced from both the local Lambert Graben and the distant Aurora Subglacial Basin drainage area. Together, the occurrence and provenance of the IRD and glacially-eroded sediment at these two marine</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.C51B..04T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.C51B..04T"><span><span class="hlt">Ice</span> Streams as the Critical Link Between the Interior <span class="hlt">Ice</span> Reservoir of the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet and the Global Climate System - a WISSARD Perspective (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.; Beem, L.; Walter, J. I.; Hossainzadeh, S.; Mankoff, K. D.</p> <p>2010-12-01</p> <p>Fast flowing <span class="hlt">ice</span> streams represent crucial features of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet because they provide discharge ‘valves’ for the interior <span class="hlt">ice</span> reservoir and because their grounding lines are exposed to ocean thermal forcing. Even with no/little topographic control <span class="hlt">ice</span> flow near the perimeter of a polar <span class="hlt">ice</span> sheet self-organizes into discrete, fast-flowing <span class="hlt">ice</span> streams. Within these features basal melting (i.e. lubrication for <span class="hlt">ice</span> sliding) is sustained through elevated basal shear heating in a region of thin <span class="hlt">ice</span> that would otherwise be characterized by basal freezing and slow <span class="hlt">ice</span> motion. Because faster basal <span class="hlt">ice</span> motion is typically associated with faster subglacial erosion, <span class="hlt">ice</span> streams tend to localize themselves over time by carving troughs into underlying rocks and sediments. Debris generated by this erosional activity is carried to the continental shelf and/or continental slope where it may be deposited at very high rates, rivaling these associated with deposition by some of the largest rivers on Earth. In terms of their hydrologic and geological functions, <span class="hlt">Antarctic</span> <span class="hlt">ice</span> streams play pretty much the same role as rivers do on non-glaciated continents. However, understanding of their dynamics is still quite rudimentary, largely because of the relative inaccessibility of the key basal and marine boundaries of <span class="hlt">ice</span> streams where pertinent measurements need to be made. The present elevated interest in predicting future contribution of Antarctica to global sea level changes is driving ambitious research programs aimed at scientific exploration of these poorly investigated environments that will play a key role in defining the response of the <span class="hlt">ice</span> sheet to near future climate changes. We will review one of these programs, the Whillans <span class="hlt">Ice</span> Stream Subglacial Access Research Drilling (WISSARD) with particular focus on its planned contributions to understanding of <span class="hlt">ice</span> stream dynamics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20010095442&hterms=Global+Warming+Climate+Change+Warning&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3DGlobal%2BWarming%2BClimate%2BChange%2BWarning','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20010095442&hterms=Global+Warming+Climate+Change+Warning&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3DGlobal%2BWarming%2BClimate%2BChange%2BWarning"><span>Sea <span class="hlt">Ice</span> and <span class="hlt">Ice</span> Temperature Variability as Observed by Microwave and Infrared Satellite Data</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.; Koblinsky, Chester J. (Technical Monitor)</p> <p>2001-01-01</p> <p>Recent reports of a retreating and thinning sea <span class="hlt">ice</span> <span class="hlt">cover</span> in the Arctic have pointed to a strong suggestion of significant warming in the polar regions. It is especially important to understand what these reports mean in light of the observed global warning and because the polar regions are expected to be most sensitive to changes in climate. To gain insight into this phenomenon, co-registered <span class="hlt">ice</span> concentrations and surface temperatures derived from two decades of satellite microwave and infrared data have been processed and analyzed. While observations from meteorological stations indicate consistent surface warming in both regions during the last fifty years, the last 20 years of the same data set show warming in the Arctic but a slight cooling in the <span class="hlt">Antarctic</span>. These results are consistent with the retreat in the Arctic <span class="hlt">ice</span> <span class="hlt">cover</span> and the advance in the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> <span class="hlt">cover</span> as revealed by historical satellite passive microwave data. Surface temperatures derived from satellite infrared data are shown to be consistent within 3 K with surface temperature data from the limited number of stations. While not as accurate, the former provides spatially detailed changes over the twenty year period. In the Arctic, for example, much of the warming occurred in the Beaufort Sea and the North American region in 1998 while slight cooling actually happened in parts of the Laptev Sea and Northern Siberia during the same time period. Big warming anomalies are also observed during the last five years but a periodic cycle of about ten years is apparent suggesting a possible influence of the North Atlantic Oscillation. In the <span class="hlt">Antarctic</span>, large interannual and seasonal changes are also observed in the circumpolar <span class="hlt">ice</span> <span class="hlt">cover</span> with regional changes showing good coherence with surface temperature anomalies. However, a mode 3 is observed to be more dominant than the mode 2 wave reported in the literature. Some of these spatial and temporal changes appear to be influenced by the <span class="hlt">Antarctic</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoRL..45.4086A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoRL..45.4086A"><span>Variable Basal Melt Rates of <span class="hlt">Antarctic</span> Peninsula <span class="hlt">Ice</span> Shelves, 1994-2016</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Adusumilli, Susheel; Fricker, Helen Amanda; Siegfried, Matthew R.; Padman, Laurie; Paolo, Fernando S.; Ligtenberg, Stefan R. M.</p> <p>2018-05-01</p> <p>We have constructed 23-year (1994-2016) time series of <span class="hlt">Antarctic</span> Peninsula (AP) <span class="hlt">ice</span>-shelf height change using data from four satellite radar altimeters (ERS-1, ERS-2, Envisat, and CryoSat-2). Combining these time series with output from atmospheric and firn models, we partitioned the total height-change signal into contributions from varying surface mass balance, firn state, <span class="hlt">ice</span> dynamics, and basal mass balance. On the Bellingshausen coast of the AP, <span class="hlt">ice</span> shelves lost 84 ± 34 Gt a-1 to basal melting, compared to contributions of 50 ± 7 Gt a-1 from surface mass balance and <span class="hlt">ice</span> dynamics. Net basal melting on the Weddell coast was 51 ± 71 Gt a-1. Recent changes in <span class="hlt">ice</span>-shelf height include increases over major AP <span class="hlt">ice</span> shelves driven by changes in firn state. Basal melt rates near Bawden <span class="hlt">Ice</span> Rise, a major pinning point of Larsen C <span class="hlt">Ice</span> Shelf, showed large increases, potentially leading to substantial loss of buttressing if sustained.</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> <span class="hlt">Ice</span>: 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 <span class="hlt">ice</span>, 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 <span class="hlt">ice</span> 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 water 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('http://adsabs.harvard.edu/abs/2015EGUGA..17..610V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17..610V"><span>Regional pattern of snow characteristics around <span class="hlt">Antarctic</span> <span class="hlt">Lake</span> Vostok</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vladimirova, Diana; Ekaykin, Alexey; Popov, Sergey; Shibaev, Yuriy; Kozachek, Anna; Lipenkov, Vladimir</p> <p>2015-04-01</p> <p>Since 1998 Russian <span class="hlt">Antarctic</span> Expedition has organized several scientific traverses in the region of subglacial <span class="hlt">Lake</span> Vostok mainly devoted to the radar echo and seismic sounding of the glacier and water (the results have been published elsewhere). Along with the geophysical studies, a number of glaciological investigations have been carried out: snow pit digging, installation of accumulation stakes, snow sampling to study the stable water isotope content. Here we for the first time present a synthesis of these works and demonstrate a series of maps that characterize the snow density, isotope content and accumulation rate the studied region. A general tendency of the snow accumulation rate and isotope content is a significant increase from south (south-west) to north (north-east) from 35 to 23 mm w.e. per year and from -53,3 ‰ to -57,3 ‰ for delta oxygen-18 respectively, which likely reflects the continental-scale pattern, i.e., increase from inland to the coast. Deuterium excess varies from 11,7 ‰ to 16,3 ‰ is negatively correlated with the isotope content, which is typical for central Antarctica. The snow density demonstrate different pattern: higher values offshore the <span class="hlt">lake</span> (up to 0,356 g/cm^3), and lower values within the <span class="hlt">lake</span>'s shoreline (lower limit is 0,328 g/cm^3). We suggest that this is related to the katabatic wind activity: very flat nearly horizontal surface of the glacier above the <span class="hlt">lake</span> is not favorable for the strong winds, which leads to lower surface snow density. Superimposed on the main trend is the regional pattern, namely, curved contour lines in the middle part of the <span class="hlt">lake</span>. We suggest that it may be related to the local anomalies of the snow drift by wind. Indeed, on the satellite images of the <span class="hlt">lake</span> one can easily see a snowdrift stretching from the <span class="hlt">lake</span>'s western shore downwind in the middle part of the <span class="hlt">lake</span>. The isolines of delta oxygen-18 and deuterium excess become perpendicular to each other in the north part of the <span class="hlt">lake</span> which also</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23705008','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23705008"><span>Change and variability in East <span class="hlt">antarctic</span> sea <span class="hlt">ice</span> seasonality, 1979/80-2009/10.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Massom, Robert; Reid, Philip; Stammerjohn, Sharon; Raymond, Ben; Fraser, Alexander; Ushio, Shuki</p> <p>2013-01-01</p> <p>Recent analyses have shown that significant changes have occurred in patterns of sea <span class="hlt">ice</span> seasonality in West Antarctica since 1979, with wide-ranging climatic, biological and biogeochemical consequences. Here, we provide the first detailed report on long-term change and variability in annual timings of sea <span class="hlt">ice</span> advance, retreat and resultant <span class="hlt">ice</span> season duration in East Antarctica. These were calculated from satellite-derived <span class="hlt">ice</span> concentration data for the period 1979/80 to 2009/10. The pattern of change in sea <span class="hlt">ice</span> seasonality off East Antarctica comprises mixed signals on regional to local scales, with pockets of strongly positive and negative trends occurring in near juxtaposition in certain regions e.g., Prydz Bay. This pattern strongly reflects change and variability in different elements of the marine "icescape", including fast <span class="hlt">ice</span>, polynyas and the marginal <span class="hlt">ice</span> zone. A trend towards shorter sea-<span class="hlt">ice</span> duration (of 1 to 3 days per annum) occurs in fairly isolated pockets in the outer pack from∼95-110°E, and in various near-coastal areas that include an area of particularly strong and persistent change near Australia's Davis Station and between the Amery and West <span class="hlt">Ice</span> Shelves. These areas are largely associated with coastal polynyas that are important as sites of enhanced sea <span class="hlt">ice</span> production/melt. Areas of positive trend in <span class="hlt">ice</span> season duration are more extensive, and include an extensive zone from 160-170°E (i.e., the western Ross Sea sector) and the near-coastal zone between 40-100°E. The East <span class="hlt">Antarctic</span> pattern is considerably more complex than the well-documented trends in West Antarctica e.g., in the <span class="hlt">Antarctic</span> Peninsula-Bellingshausen Sea and western Ross Sea sectors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27441705','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27441705"><span>Hydrological Controls on Ecosystem Dynamics in <span class="hlt">Lake</span> Fryxell, Antarctica.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Herbei, Radu; Rytel, Alexander L; Lyons, W Berry; McKnight, Diane M; Jaros, Christopher; Gooseff, Michael N; Priscu, John C</p> <p>2016-01-01</p> <p>The McMurdo Dry Valleys constitute the largest <span class="hlt">ice</span> free area of Antarctica. The area is a polar desert with an annual precipitation of ∼ 3 cm water equivalent, but contains several <span class="hlt">lakes</span> fed by glacial melt water streams that flow from four to twelve weeks of the year. Over the past ∼20 years, data have been collected on the <span class="hlt">lakes</span> located in Taylor Valley, Antarctica as part of the McMurdo Dry Valley Long-Term Ecological Research program (MCM-LTER). This work aims to understand the impact of climate variations on the biological processes in all the ecosystem types within Taylor Valley, including the <span class="hlt">lakes</span>. These <span class="hlt">lakes</span> are stratified, closed-basin systems and are perennially <span class="hlt">covered</span> with <span class="hlt">ice</span>. Each <span class="hlt">lake</span> contains a variety of planktonic and benthic algae that require nutrients for photosynthesis and growth. The work presented here focuses on <span class="hlt">Lake</span> Fryxell, one of the three main <span class="hlt">lakes</span> of Taylor Valley; it is fed by thirteen melt-water streams. We use a functional regression approach to link the physical, chemical, and biological processes within the stream-<span class="hlt">lake</span> system to evaluate the input of water and nutrients on the biological processes in the <span class="hlt">lakes</span>. The technique has been shown previously to provide important insights into these <span class="hlt">Antarctic</span> lacustrine systems where data acquisition is not temporally coherent. We use data on primary production (PPR) and chlorophyll-A (CHL)from <span class="hlt">Lake</span> Fryxell as well as discharge observations from two streams flowing into the <span class="hlt">lake</span>. Our findings show an association between both PPR, CHL and stream input.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1914847W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1914847W"><span>EBSD in <span class="hlt">Antarctic</span> and Greenland <span class="hlt">Ice</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Weikusat, Ilka; Kuiper, Ernst-Jan; Pennock, Gill; Sepp, Kipfstuhl; Drury, Martyn</p> <p>2017-04-01</p> <p> subgrain boundaries. However, an almost equal number of tilt subgrain boundaries were measured, involving dislocations gliding on non-basal planes (prism <c> or prism <c+a> slip). A few subgrain boundaries involving prism <a> edge dislocation glide, as well as boundaries involving basal <a> twist dislocation slip, were also identified. The finding that subgrain boundaries built up by dislocations gliding on non-basal planes are as frequent as those originating from basal plane slip is surprising and has impact on the discussion on rate-controlling processes for the <span class="hlt">ice</span> flow descriptions of large <span class="hlt">ice</span> masses with respect to sea-level evolution. Weikusat, I.; Miyamoto, A.; Faria, S. H.; Kipfstuhl, S.; Azuma, N. & Hondoh, T.: Subgrain boundaries in <span class="hlt">Antarctic</span> <span class="hlt">ice</span> quantified by X-ray Laue diffraction J. Glaciol., 2011, 57, 85-94</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19..443A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19..443A"><span><span class="hlt">Ice</span>-dammed <span class="hlt">lakes</span> reconstruction in the southeastern Scandinavian <span class="hlt">ice</span> sheet periphery</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Anisimov, Nikolai</p> <p>2017-04-01</p> <p>The study of glacier erosion processes, paleolake dynamics and topographical changes, together give us insight into both localized and broader landscape evolution patterns while also assisting human exploration. After carrying number of paleographic discoveries of North-West of Russia, we've gathered the data requiring generalizing, systemizing, visualizing. Objective: reconstruction of proglacial <span class="hlt">lakes</span> based on lithostratigraphic and geomorphic analysis using GIS technology. GIS modeling of <span class="hlt">ice</span>-dammed <span class="hlt">lakes</span> was done via the ArcGIS Desktop 10 software package. The GIS was used as a means to categorize published, time mapped data and thereby fuse and unify the changes into a single, integrated prototype. Publications on limnologo-glaciological and geomorphological reconstructions of paleotopography and paleolakes north of the Russian plain, along with additional copyrighted and grant-funded GIS studies, together served as resources to authenticate the paleolake contour modeling. A quaternary sediments map and an updated topography map that was designed via semiautomatic vectorization of a topographical map, served as foundations for the electronic shape modeling paleoreconstructions. Based upon preliminary results from publication summaries, and initial data collected when analyzing the maps (quaternary sediments, geomorphological, topographical), the contours and maximum glacial <span class="hlt">lake</span> rise levels in the southeastern Scandinavian <span class="hlt">ice</span> sheet periphery, including the levels and contours of their coastline, have been duly identified. Boundary reconstruction of Late Pleistocene <span class="hlt">lake</span> boundaries have been completed for five sections of the Scandinavian <span class="hlt">ice</span> sheet: the Molovo-Sheksninskoy, the Belozersko-Kubensky, the Vozhe-Lachsko-Kubensky, the Vazhskoy, and the Severodvinskoy. The territories studied revealed 13 major paleobasins <span class="hlt">covering</span> an area of more than 1,000 km2, which based upon their position most closely resemble periglacial, intraglacial and postglacial <span class="hlt">lakes</span>. Of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.C13E..04H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.C13E..04H"><span>Towards decadal time series of Arctic and <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span> thickness from radar altimetry</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hendricks, S.; Rinne, E. J.; Paul, S.; Ricker, R.; Skourup, H.; Kern, S.; Sandven, S.</p> <p>2016-12-01</p> <p>The CryoSat-2 mission has demonstrated the value of radar altimetry to assess the interannual variability and short-term trends of Arctic sea <span class="hlt">ice</span> over the existing observational record of 6 winter seasons. CryoSat-2 is a particular successful mission for sea <span class="hlt">ice</span> mass balance assessment due to its novel radar altimeter concept and orbit configuration, but radar altimetry data is available since 1993 from the ERS-1/2 and Envisat missions. Combining these datasets promises a decadal climate data record of sea <span class="hlt">ice</span> thickness, but inter-mission biases must be taken into account due to the evolution of radar altimeters and the impact of changing sea <span class="hlt">ice</span> conditions on retrieval algorithm parametrizations. The ESA Climate Change Initiative on Sea <span class="hlt">Ice</span> aims to extent the list of data records for Essential Climate Variables (ECV's) with a consistent time series of sea <span class="hlt">ice</span> thickness from available radar altimeter data. We report on the progress of the algorithm development and choices for auxiliary data sets for sea <span class="hlt">ice</span> thickness retrieval in the Arctic and <span class="hlt">Antarctic</span> Oceans. Particular challenges are the classification of surface types and freeboard retrieval based on radar waveforms with significantly varying footprint sizes. In addition, auxiliary data sets, e.g. for snow depth, are far less developed in the <span class="hlt">Antarctic</span> and we will discuss the expected skill of the sea <span class="hlt">ice</span> thickness ECV's in both hemispheres.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21805086','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21805086"><span>Direct and indirect climatic drivers of biotic interactions: <span class="hlt">ice-cover</span> and carbon runoff shaping Arctic char Salvelinus alpinus and brown trout Salmo trutta competitive asymmetries.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ulvan, Eva M; Finstad, Anders G; Ugedal, Ola; Berg, Ole Kristian</p> <p>2012-01-01</p> <p>One of the major challenges in ecological climate change impact science is to untangle the climatic effects on biological interactions and indirect cascading effects through different ecosystems. Here, we test for direct and indirect climatic drivers on competitive impact of Arctic char (Salvelinus alpinus L.) on brown trout (Salmo trutta L.) along a climate gradient in central Scandinavia, spanning from coastal to high-alpine environments. As a measure of competitive impact, trout food consumption was measured using (137)Cs tracer methodology both during the <span class="hlt">ice-covered</span> and <span class="hlt">ice</span>-free periods, and contrasted between <span class="hlt">lakes</span> with or without char coexistence along the climate gradient. Variation in food consumption between <span class="hlt">lakes</span> was best described by a linear mixed effect model including a three-way interaction between the presence/absence of Arctic char, season and Secchi depth. The latter is proxy for terrestrial dissolved organic carbon run-off, strongly governed by climatic properties of the catchment. The presence of Arctic char had a negative impact on trout food consumption. However, this effect was stronger during <span class="hlt">ice-cover</span> and in <span class="hlt">lakes</span> receiving high carbon load from the catchment, whereas no effect of water temperature was evident. In conclusion, the length of the <span class="hlt">ice-covered</span> period and the export of allochthonous material from the catchment are likely major, but contrasting, climatic drivers of the competitive interaction between two freshwater <span class="hlt">lake</span> top predators. While future climatic scenarios predict shorter <span class="hlt">ice-cover</span> duration, they also predict increased carbon run-off. The present study therefore emphasizes the complexity of cascading ecosystem effects in future effects of climate change on freshwater 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 class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_24 --> <div id="page_25" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li class="active"><span>25</span></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="481"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1919299M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1919299M"><span>Flow structure at an <span class="hlt">ice-covered</span> river confluence</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Martel, Nancy; Biron, Pascale; Buffin-Bélanger, Thomas</p> <p>2017-04-01</p> <p>River confluences are known to exhibit complex relationships between flow structure, sediment transport and bed-form development. Flow structure at these sites is influenced by the junction angle, the momentum flux ratio (Mr) and bed morphology. In cold regions where an <span class="hlt">ice</span> <span class="hlt">cover</span> is present for most of the winter period, the flow structure is also likely affected by the roughness effect of the <span class="hlt">ice</span>. However, very few studies have examined the impact of an <span class="hlt">ice</span> <span class="hlt">cover</span> on the flow structure at a confluence. The aims of this study are (1) to describe the evolution of an <span class="hlt">ice</span> <span class="hlt">cover</span> at a river confluence and (2) to characterize and compare the flow structure at a river confluence with and without an <span class="hlt">ice</span> <span class="hlt">cover</span>. The field site is a medium-sized confluence (around 40 m wide) between the Mit is and Neigette Rivers in the Bas-Saint-Laurent region, Quebec (Canada). The confluence was selected because a thick <span class="hlt">ice</span> <span class="hlt">cover</span> is present for most of the winter allowing for safe field work. Two winter field campaigns were conducted in 2015 and 2016 to obtain <span class="hlt">ice</span> <span class="hlt">cover</span> measurements in addition to hydraulic and morphological measurements. Daily monitoring of the evolution of the <span class="hlt">ice</span> <span class="hlt">cover</span> was made with a Reconyx camera. Velocity profiles were collected with an acoustic Doppler current profiler (ADCP) to reconstruct the three-dimensional flow structure. Time series of photographs allow the evolution of the <span class="hlt">ice</span> <span class="hlt">cover</span> to be mapped, linking the processes leading to the formation of the primary <span class="hlt">ice</span> <span class="hlt">cover</span> for each year. The time series suggests that these processes are closely related with both confluence flow zones and hydro-climatic conditions. Results on the thickness of the <span class="hlt">ice</span> <span class="hlt">cover</span> from in situ measurements reveal that the <span class="hlt">ice</span> thickness tends to be thinner at the center of the confluence where high turbulent exchanges take place. Velocity measurements reveal that the <span class="hlt">ice</span> <span class="hlt">cover</span> affects velocity profiles by moving the highest velocities towards the center of the profiles. A spatio</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.5000F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.5000F"><span>Long-term monitoring of glacier dynamics of Fleming Glacier after the disintegration of Wordie <span class="hlt">Ice</span> Shelf, <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>Friedl, Peter; Seehaus, Thorsten; Wendt, Anja; Braun, Matthias</p> <p>2017-04-01</p> <p>The <span class="hlt">Antarctic</span> Peninsula is one of the world`s most affected regions by Climate Change. Dense and long time series of remote sensing data enable detailed studies of the rapid glaciological changes in this area. We present results of a study on Fleming Glacier, which was the major tributary glacier of former Wordie <span class="hlt">Ice</span> Shelf, located at the south-western side of the <span class="hlt">Antarctic</span> Peninsula. Since the <span class="hlt">ice</span> shelf disintegrated in a series of events starting in the 1970s, only disconnected tidewater glaciers have remained today. As a reaction to the loss of the buttressing force of the <span class="hlt">ice</span> shelf, Fleming Glacier accelerated and dynamically thinned. However, all previous studies conducted at Wordie Bay <span class="hlt">covered</span> only relatively short investigation periods and ended in 2008 the latest. Hence it was not well known how long the process of adaption to the changing boundary conditions exactly lasts and how it is characterized in detail. We provide long time series (1994 - 2016) of glaciological parameters (i.e. <span class="hlt">ice</span> extent, velocity, grounding line position, <span class="hlt">ice</span> elevation) for Fleming Glacier obtained from multi-mission remote sensing data. For this purpose large datasets of previously active (e.g. ERS, Envisat, ALOS PALSAR, Radarsat-1) as well as currently recording SAR sensors (e.g. Sentinel-1, TerraSAR-X, TanDEM-X) were processed and combined with data from other sources (e.g. optical images, laser altimeter and <span class="hlt">ice</span> thickness data). The high temporal resolution of our dataset enables us to present a detailed history of 22 years of glacial dynamics at Fleming Glacier after the disintegration of Wordie <span class="hlt">Ice</span> Shelf. We found strong evidence for a rapid grounding line retreat of up to 13 km between 2008 and 2011, which led to a further amplification of dynamic <span class="hlt">ice</span> thinning. Today Fleming Glacier seems to be far away from approaching a new equilibrium. Our data show that the current glacier dynamics of Fleming Glacier are not primarily controlled by the loss of the <span class="hlt">ice</span> shelf anymore, but</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1378355-adaptive-mesh-refinement-versus-subgrid-friction-interpolation-simulations-antarctic-ice-dynamics','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1378355-adaptive-mesh-refinement-versus-subgrid-friction-interpolation-simulations-antarctic-ice-dynamics"><span>Adaptive mesh refinement versus subgrid friction interpolation in simulations of <span class="hlt">Antarctic</span> <span class="hlt">ice</span> dynamics</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Cornford, S. L.; Martin, D. F.; Lee, V.; ...</p> <p>2016-05-13</p> <p>At least in conventional hydrostatic <span class="hlt">ice</span>-sheet models, the numerical error associated with grounding line dynamics can be reduced by modifications to the discretization scheme. These involve altering the integration formulae for the basal traction and/or driving stress close to the grounding line and exhibit lower – if still first-order – error in the MISMIP3d experiments. MISMIP3d may not represent the variety of real <span class="hlt">ice</span> streams, in that it lacks strong lateral stresses, and imposes a large basal traction at the grounding line. We study resolution sensitivity in the context of extreme forcing simulations of the entire <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet, using the BISICLES adaptive mesh <span class="hlt">ice</span>-sheet model with two schemes: the original treatment, and a scheme, which modifies the discretization of the basal traction. The second scheme does indeed improve accuracy – by around a factor of two – for a given mesh spacing, butmore » $$\\lesssim 1$$ km resolution is still necessary. For example, in coarser resolution simulations Thwaites Glacier retreats so slowly that other <span class="hlt">ice</span> streams divert its trunk. In contrast, with $$\\lesssim 1$$ km meshes, the same glacier retreats far more quickly and triggers the final phase of West <span class="hlt">Antarctic</span> collapse a century before any such diversion can take place.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017TCry...11.1851P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017TCry...11.1851P"><span>Sea-level response to melting of <span class="hlt">Antarctic</span> <span class="hlt">ice</span> shelves on multi-centennial timescales with the fast Elementary Thermomechanical <span class="hlt">Ice</span> Sheet model (f.ETISh v1.0)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pattyn, Frank</p> <p>2017-08-01</p> <p>The magnitude of the <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet's contribution to global sea-level rise is dominated by the potential of its marine sectors to become unstable and collapse as a response to ocean (and atmospheric) forcing. This paper presents <span class="hlt">Antarctic</span> sea-level response to sudden atmospheric and oceanic forcings on multi-centennial timescales with the newly developed fast Elementary Thermomechanical <span class="hlt">Ice</span> Sheet (f.ETISh) model. The f.ETISh model is a vertically integrated hybrid <span class="hlt">ice</span> sheet-<span class="hlt">ice</span> shelf model with vertically integrated thermomechanical coupling, making the model two-dimensional. Its marine boundary is represented by two different flux conditions, coherent with power-law basal sliding and Coulomb basal friction. The model has been compared to existing benchmarks. Modelled <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet response to forcing is dominated by sub-<span class="hlt">ice</span> shelf melt and the sensitivity is highly dependent on basal conditions at the grounding line. Coulomb friction in the grounding-line transition zone leads to significantly higher mass loss in both West and East Antarctica on centennial timescales, leading to 1.5 m sea-level rise after 500 years for a limited melt scenario of 10 m a-1 under freely floating <span class="hlt">ice</span> shelves, up to 6 m for a 50 m a-1 scenario. The higher sensitivity is attributed to higher <span class="hlt">ice</span> fluxes at the grounding line due to vanishing effective pressure. Removing the <span class="hlt">ice</span> shelves altogether results in a disintegration of the West <span class="hlt">Antarctic</span> <span class="hlt">ice</span> sheet and (partially) marine basins in East Antarctica. After 500 years, this leads to a 5 m and a 16 m sea-level rise for the power-law basal sliding and Coulomb friction conditions at the grounding line, respectively. The latter value agrees with simulations by DeConto and Pollard (2016) over a similar period (but with different forcing and including processes of hydrofracturing and cliff failure). The chosen parametrizations make model results largely independent of spatial resolution so that f.ETISh can potentially be</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5776470','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5776470"><span>Changes in bacterioplankton community structure during early <span class="hlt">lake</span> ontogeny resulting from the retreat of the Greenland <span class="hlt">Ice</span> 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>Peter, Hannes; Jeppesen, Erik; De Meester, Luc; Sommaruga, Ruben</p> <p>2018-01-01</p> <p>Retreating glaciers and <span class="hlt">ice</span> sheets are among the clearest signs of global climate change. One consequence of glacier retreat is the formation of new meltwater-<span class="hlt">lakes</span> in previously <span class="hlt">ice-covered</span> terrain. These <span class="hlt">lakes</span> provide unique opportunities to understand patterns in community organization during early <span class="hlt">lake</span> ontogeny. Here, we analyzed the bacterial community structure and diversity in six <span class="hlt">lakes</span> recently formed by the retreat of the Greenland <span class="hlt">Ice</span> Sheet (GrIS). The <span class="hlt">lakes</span> represented a turbidity gradient depending on their past and present connectivity to the GrIS meltwaters. Bulk (16S rRNA genes) and putatively active (16S rRNA) fractions of the bacterioplankton communities were structured by changes in environmental conditions associated to the turbidity gradient. Differences in community structure among <span class="hlt">lakes</span> were attributed to both, rare and abundant community members. Further, positive co-occurrence relationships among phylogenetically closely related community members dominate in these <span class="hlt">lakes</span>. Our results show that environmental conditions along the turbidity gradient structure bacterial community composition, which shifts during <span class="hlt">lake</span> ontogeny. Rare taxa contribute to these shifts, suggesting that the rare biosphere has an important ecological role during early <span class="hlt">lakes</span> ontogeny. Members of the rare biosphere may be adapted to the transient niches in these nutrient poor <span class="hlt">lakes</span>. The directionality and phylogenetic structure of co-occurrence relationships indicate that competitive interactions among closely related taxa may be important in the most turbid <span class="hlt">lakes</span>. PMID:29087379</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 <span class="hlt">ice</span> discharge into the ocean, as a boundary condition for numerical models of <span class="hlt">ice</span> flow, and as an indicator of <span class="hlt">ice</span> 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 <span class="hlt">ice</span>-elevation change and airborne measurements of <span class="hlt">ice</span> geometry to track movement of the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> 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 <span class="hlt">ice</span> 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-<span class="hlt">ice</span> 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://www.ncbi.nlm.nih.gov/pubmed/25885562','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25885562"><span>In situ expression of eukaryotic <span class="hlt">ice</span>-binding proteins in microbial communities of Arctic and <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Uhlig, Christiane; Kilpert, Fabian; Frickenhaus, Stephan; Kegel, Jessica U; Krell, Andreas; Mock, Thomas; Valentin, Klaus; Beszteri, Bánk</p> <p>2015-11-01</p> <p><span class="hlt">Ice</span>-binding proteins (IBPs) have been isolated from various sea-<span class="hlt">ice</span> organisms. Their characterisation points to a crucial role in protecting the organisms in sub-zero environments. However, their in situ abundance and diversity in natural sea-<span class="hlt">ice</span> microbial communities is largely unknown. In this study, we analysed the expression and phylogenetic diversity of eukaryotic IBP transcripts from microbial communities of Arctic and <span class="hlt">Antarctic</span> sea <span class="hlt">ice</span>. IBP transcripts were found in abundances similar to those of proteins involved in core cellular processes such as photosynthesis. Eighty-nine percent of the IBP transcripts grouped with known IBP sequences from diatoms, haptophytes and crustaceans, but the majority represented novel sequences not previously characterized in cultured organisms. The observed high eukaryotic IBP expression in natural eukaryotic sea <span class="hlt">ice</span> communities underlines the essential role of IBPs for survival of many microorganisms in communities living under the extreme conditions of polar sea <span class="hlt">ice</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1918170H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1918170H"><span><span class="hlt">Antarctic</span> and Greenland <span class="hlt">ice</span> sheet mass balance products from satellite gravimetry</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Horwath, Martin; Groh, Andreas; Horvath, Alexander; Forsberg, René; Meister, Rakia; Barletta, Valentina R.; Shepherd, Andrew</p> <p>2017-04-01</p> <p>Because of their important role in the Earth's climate system, ESA's Climate Change Initiative (CCI) has identified both the <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Sheet (AIS) and the Greenland <span class="hlt">Ice</span> Sheet (GIS) as Essential Climate Variables (ECV). Since respondents of a user survey indicated that the <span class="hlt">ice</span> sheet mass balance is one of the most important ECV data products needed to better understand climate change, the AIS_cci and the GIS_cci project provide Gravimetric Mass Balance (GMB) products based on satellite gravimetry data. The GMB products are derived from GRACE (Gravity Recovery and Climate Experiment) monthly solutions of release ITSG-Grace2016 produced at TU Graz. GMB basin products (i.e. time series of monthly mass changes for the entire <span class="hlt">ice</span> sheets and selected drainage basins) and GMB gridded products (e.g. mass balance estimates with a formal resolution of about 50km, <span class="hlt">covering</span> the entire <span class="hlt">ice</span> sheets) are generated for the period from 2002 until present. The first GMB product was released in mid 2016. Here we present an extended and updated version of the ESA CCI GMB products, which are freely available through data portals hosted by the projects (https://data1.geo.tu-dresden.de/ais_gmb, http://products.esa-icesheets-cci.org/products/downloadlist/GMB). Since the initial product release, the applied processing strategies have been improved in order to further reduce GRACE errors and to enhance the separation of signals super-imposed to the <span class="hlt">ice</span> mass changes. While a regional integration approach is used by the AIS_cci project, the GMB products of the GIS_cci project are derived using a point mass inversion. The differences between both approaches are investigated through the example of the GIS, where an alternative GMB product was generated using the regional integration approach implemented by the AIS_cci. Finally, we present the latest mass balance estimates for both <span class="hlt">ice</span> sheets as well as their corresponding contributions to global sea level rise.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFMPP51D1899N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFMPP51D1899N"><span>Climatic change and evaporative processes in the development of Common Era hypersaline <span class="hlt">lakes</span>, East Antarctica: A study of <span class="hlt">Lake</span> Suribati</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nakashima, H.; Seto, K.; Katsuki, K.; Kaneko, H.; yamada, K.; Imura, S.; Dettman, D. L.</p> <p>2011-12-01</p> <p>The <span class="hlt">Antarctic</span> continent was uplifted by glacioisostatic rebound due to the regression of <span class="hlt">ice</span> sheets after the last glacial period. Today's saline <span class="hlt">lakes</span> were formed in shallow basins originally below sea level. <span class="hlt">Antarctic</span> hypersaline <span class="hlt">lakes</span> are formed by concentration of isolated seawater bodies as affected by recent climate change. Many saline <span class="hlt">lakes</span> are found in the <span class="hlt">ice</span>-free area of the Soya coast, East Antarctica. <span class="hlt">Lake</span> Suribati is located in Sukarvsnes on the Soya coast. It is a hypersaline <span class="hlt">lake</span> with maximum salinity ~200 psu, and an observable stable halocline at 7~12m depth. This study uses <span class="hlt">Lake</span> Suribati sediment core Sr4C-01, collected by the 46th Japanese Antarctica Research Expedition, to examine the relationship of climatic change to evaporative processes and solute concentration in <span class="hlt">Lake</span> Suribati in the Common Era. Sr4C-01 core was collected at 9.53m water depth in <span class="hlt">Lake</span> Suribati in 2005 (core length is 63cm). This core primarily consists of black mud and laminated black organic mud. In the interval from 10 to 24cm below the sediment surface evaporite crystals occur. The age of the Sr4C-01 core bottom is estimated to be ~3,500 cal yrs BP, based on AMS carbon-14 dating at 6 core horizons. The evaporite crystals were indentified as aragonite based on XRD. Total inorganic carbon (TIC) content is low, around 0.5%, throughout the Sr4C-01 core, with higher values, approximately 1~4%, in two intervals, 57~52cm and 29~10cm core depth. Variation in CaO content tracks TIC content. We suggest that synchronous change in CaO and TIC contents indicate the vertical change in the amount of aragonite. Two intervals of evaporite precipition imply two intervals of evaporation and concentration of <span class="hlt">lake</span> water. Hypersaline <span class="hlt">lake</span> conditions did not occur soon after the isolation from the sea, rather these occurred under repeated concentration and dilution of <span class="hlt">lake</span> water. Dilution of saline <span class="hlt">lake</span> water could occur through the inflow of melt water from local snow or <span class="hlt">ice</span>, indicating a warm</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.9626B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.9626B"><span>Circumpolar patterns of ground-fast <span class="hlt">lake</span> <span class="hlt">ice</span> and landscape development</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bartsch, Annett; Pointner, Georg; Leibmann, Marina; Dvornikov, Yuri; Khomutov, Artem</p> <p>2017-04-01</p> <p>Shallow <span class="hlt">lakes</span> in the Arctic are often associated with thermokarst processes which are characteristic for permafrost environments. They partially or completely freeze-up during winter time what can be observed from space using Synthetic Aperture Radar (SAR) data. Spatial patterns of ground-fast and floating <span class="hlt">ice</span> relate to geomorphological and hydrological processes, but no circumpolar account of this phenomenon is currently available due to challenges when dealing with the varying observation geometry typical for SAR. An approach using ENVISAT ASAR Wide Swath data (approximately 120 m resolution) has been developed supported by bathymetric measurements in Siberia and eventually applied across the entire Arctic for late winter 2008. In total about 2 Million <span class="hlt">lake</span> objects have been analyzed considering the boundaries of the Last Glacial Maximum, permafrost zones and soil organic carbon content. Distinct patterns of ground-fast <span class="hlt">lake</span> <span class="hlt">ice</span> fraction can be found across the Arctic. Clusters of variable fractions of ground-fast <span class="hlt">ice</span> occur especially in Yedoma regions of Eastern Siberia and Alaska. This reflects the nature of thaw <span class="hlt">lake</span> dynamics. Analyses of <span class="hlt">lake</span> depth measurements from several sites (Alaskan North Slope, Richards Island in Canada, Yamal Peninsula and Lena Delta) suggest that the used method yields the potential to utilize ground-fast <span class="hlt">lake</span> <span class="hlt">ice</span> information over larger areas with respect to landscape development, but results need to be treated with care, specifically for larger <span class="hlt">lakes</span> and along river courses. A combination of general <span class="hlt">lake</span> features and ground-fast <span class="hlt">ice</span> fraction may lead to an advanced understanding of landscape patterns and development. Ground-fast <span class="hlt">ice</span> fraction information may support to some extent the identification of landscape units, for example areas of adjacent <span class="hlt">lakes</span> with similar patterns (terraces) or areas with mixed ground-fast fractions which indicate different <span class="hlt">lake</span> development stages. This work was supported by the Austrian Science Fund</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AcMSn..31....1Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AcMSn..31....1Z"><span>Modeling ocean wave propagation under sea <span class="hlt">ice</span> <span class="hlt">covers</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhao, Xin; Shen, Hayley H.; Cheng, Sukun</p> <p>2015-02-01</p> <p>Operational ocean wave models need to work globally, yet current ocean wave models can only treat <span class="hlt">ice-covered</span> regions crudely. The purpose of this paper is to provide a brief overview of <span class="hlt">ice</span> effects on wave propagation and different research methodology used in studying these effects. Based on its proximity to land or sea, sea <span class="hlt">ice</span> can be classified as: landfast <span class="hlt">ice</span> zone, shear zone, and the marginal <span class="hlt">ice</span> zone. All <span class="hlt">ice</span> <span class="hlt">covers</span> attenuate wave energy. Only long swells can penetrate deep into an <span class="hlt">ice</span> <span class="hlt">cover</span>. Being closest to open water, wave propagation in the marginal <span class="hlt">ice</span> zone is the most complex to model. The physical appearance of sea <span class="hlt">ice</span> in the marginal <span class="hlt">ice</span> zone varies. Grease <span class="hlt">ice</span>, pancake <span class="hlt">ice</span>, brash <span class="hlt">ice</span>, floe aggregates, and continuous <span class="hlt">ice</span> sheet may be found in this zone at different times and locations. These types of <span class="hlt">ice</span> are formed under different thermal-mechanical forcing. There are three classic models that describe wave propagation through an idealized <span class="hlt">ice</span> <span class="hlt">cover</span>: mass loading, thin elastic plate, and viscous layer models. From physical arguments we may conjecture that mass loading model is suitable for disjoint aggregates of <span class="hlt">ice</span> floes much smaller than the wavelength, thin elastic plate model is suitable for a continuous <span class="hlt">ice</span> sheet, and the viscous layer model is suitable for grease <span class="hlt">ice</span>. For different sea <span class="hlt">ice</span> types we may need different wave <span class="hlt">ice</span> interaction models. A recently proposed viscoelastic model is able to synthesize all three classic models into one. Under suitable limiting conditions it converges to the three previous models. The complete theoretical framework for evaluating wave propagation through various <span class="hlt">ice</span> <span class="hlt">covers</span> need to be implemented in the operational ocean wave models. In this review, we introduce the sea <span class="hlt">ice</span> types, previous wave <span class="hlt">ice</span> interaction models, wave attenuation mechanisms, the methods to calculate wave reflection and transmission between different <span class="hlt">ice</span> <span class="hlt">covers</span>, and the effect of <span class="hlt">ice</span> floe breaking on shaping the sea <span class="hlt">ice</span> morphology</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23418580','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23418580"><span>Diatom-specific highly branched isoprenoids as biomarkers in <span class="hlt">Antarctic</span> consumers.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Goutte, Aurélie; Cherel, Yves; Houssais, Marie-Noëlle; Klein, Vincent; Ozouf-Costaz, Catherine; Raccurt, Mireille; Robineau, Camille; Massé, Guillaume</p> <p>2013-01-01</p> <p>The structure, functioning and dynamics of polar marine ecosystems are strongly influenced by the extent of sea <span class="hlt">ice</span>. <span class="hlt">Ice</span> algae and pelagic phytoplankton represent the primary sources of nutrition for higher trophic-level organisms in seasonally <span class="hlt">ice-covered</span> areas, but their relative contributions to polar marine consumers remain largely unexplored. Here, we investigated the potential of diatom-specific lipid markers and highly branched isoprenoids (HBIs) for estimating the importance of these two carbon pools in an <span class="hlt">Antarctic</span> pelagic ecosystem. Using GC-MS analysis, we studied HBI biomarkers in key marine species over three years in Adélie Land, Antarctica: euphausiids (<span class="hlt">ice</span> krill Euphausia crystallorophias and <span class="hlt">Antarctic</span> krill E. superba), fish (bald notothens Pagothenia borchgrevinki and <span class="hlt">Antarctic</span> silverfish Pleuragramma antarcticum) and seabirds (Adélie penguins Pygoscelis adeliae, snow petrels Pagodroma nivea and cape petrels Daption capense). This study provides the first evidence of the incorporation of HBI lipids in <span class="hlt">Antarctic</span> pelagic consumers. Specifically, a di-unsaturated HBI (diene) of sea <span class="hlt">ice</span> origin was more abundant in <span class="hlt">ice</span>-associated species than in pelagic species, whereas a tri-unsaturated HBI (triene) of phytoplanktonic origin was more abundant in pelagic species than in <span class="hlt">ice</span>-associated species. Moreover, the relative abundances of diene and triene in seabird tissues and eggs were higher during a year of good sea <span class="hlt">ice</span> conditions than in a year of poor <span class="hlt">ice</span> conditions. In turn, the higher contribution of <span class="hlt">ice</span> algal derived organic matter to the diet of seabirds was related to earlier breeding and higher breeding success. HBI biomarkers are a promising tool for estimating the contribution of organic matter derived from <span class="hlt">ice</span> algae in pelagic consumers from Antarctica.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A51E2111V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A51E2111V"><span>Toward Surface Mass Balance Modeling over <span class="hlt">Antarctic</span> Peninsula with Improved Snow/<span class="hlt">Ice</span> Physics within WRF</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Villamil-Otero, G.; Zhang, J.; Yao, Y.</p> <p>2017-12-01</p> <p>The <span class="hlt">Antarctic</span> Peninsula (AP) has long been the focus of climate change studies due to its rapid environmental changes such as significantly increased glacier melt and retreat, and <span class="hlt">ice</span>-shelf break-up. Progress has been continuously made in the use of regional modeling to simulate surface mass changes over <span class="hlt">ice</span> sheets. Most efforts, however, focus on the <span class="hlt">ice</span> sheets of Greenland with considerable fewer studies in Antarctica. In this study the Weather Research and Forecasting (WRF) model, which has been applied to the <span class="hlt">Antarctic</span> region for weather modeling, is adopted to capture the past and future surface mass balance changes over AP. In order to enhance the capabilities of WRF model simulating surface mass balance over the <span class="hlt">ice</span> surface, we implement various <span class="hlt">ice</span> and snow processes within the WRF and develop a new WRF suite (WRF-<span class="hlt">Ice</span>). The WRF-<span class="hlt">Ice</span> includes a thermodynamic <span class="hlt">ice</span> sheet model that improves the representation of internal melting and refreezing processes and the thermodynamic effects over <span class="hlt">ice</span> sheet. WRF-<span class="hlt">Ice</span> also couples a thermodynamic sea <span class="hlt">ice</span> model to improve the simulation of surface temperature and fluxes over sea <span class="hlt">ice</span>. Lastly, complex snow processes are also taken into consideration including the implementation of a snowdrift model that takes into account the redistribution of blowing snow as well as the thermodynamic impact of drifting snow sublimation on the lower atmospheric boundary layer. Intensive testing of these <span class="hlt">ice</span> and snow processes are performed to assess the capability of WRF-<span class="hlt">Ice</span> in simulating the surface mass balance changes over AP.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA14556.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA14556.html"><span>NASA Research Leads to First Complete Map of <span class="hlt">Antarctic</span> <span class="hlt">Ice</span> Flows</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2011-08-18</p> <p>This image is the first complete map of the speed and direction of <span class="hlt">ice</span> flow in Antartica. The thick black lines delineate major <span class="hlt">ice</span> divides. Subglacial <span class="hlt">lakes</span> in Antarctica interior are also outlined in black.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGC53D0926B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC53D0926B"><span>High and Increasing Shoreline Erosion Rates of Thermokarst <span class="hlt">Lakes</span> Set in <span class="hlt">Ice</span>-Rich Permafrost Terrain of the Arctic Coastal Plain of Alaska</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bondurant, A. C.; Arp, C. D.; Jones, B. M.; Shur, Y.; Daanen, R. P.</p> <p>2017-12-01</p> <p>Thermokarst <span class="hlt">lakes</span> are a dominant landform shaping landscapes and impacting permafrost on the Arctic Coastal Plain (ACP) of northern Alaska, a region of continuous permafrost. Here <span class="hlt">lakes</span> <span class="hlt">cover</span> greater than 20% of the landscape and drained <span class="hlt">lake</span> basins <span class="hlt">cover</span> an additional 50 to 60% of the landscape. The formation, expansion, and drainage of thaw <span class="hlt">lakes</span> has been described by some researchers as part of a natural cycle that has reworked the ACP landscape during the Holocene. Yet the factors and processes controlling contemporary thermokarst <span class="hlt">lake</span> expansion remain poorly described. This study focuses on the factors controlling expansion rates of thermokarst <span class="hlt">lakes</span> in three ACP regions that vary in landscape history, ground-<span class="hlt">ice</span> content, and <span class="hlt">lake</span> morphology (i.e. size and depth), as well as evaluating changes through time. Through the use of historical aerial imagery, satellite imagery, and field observations, this study identifies the controlling factors at multiple spatial and temporal scales to better understand the processes relating to thermokarst <span class="hlt">lake</span> expansion. Studies of 35 <span class="hlt">lakes</span> across the ACP shows regional differences in expansion rate related to permafrost <span class="hlt">ice</span> content ranging from an average expansion rate of 0.62 m/yr where <span class="hlt">ice</span> content is highest ( 86%) to 0.16 m/yr where <span class="hlt">ice</span> content is lowest (45%-71%). A subset of these <span class="hlt">lakes</span> analyzed over multiple time periods show increasing rates of erosion, with average rates being 37% higher over the period 1979-2002 (0.73 m/yr) compared to 1948-1979 (0.53 m/yr). These increased rates of erosion have important implications for the regional hydrologic cycle and localized permafrost degradation. Predicting how thermokarst <span class="hlt">lakes</span> will behave locally and on a landscape scale is increasingly important for managing habitat and water resources and informing models of land-climate interactions in the Arctic.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C41D1257M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C41D1257M"><span><span class="hlt">Lake</span> Generated Microseisms at Yellowstone <span class="hlt">Lake</span> as a Record of <span class="hlt">Ice</span> Phenology</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mohd Mokhdhari, A. A.; Koper, K. D.; Burlacu, R.</p> <p>2017-12-01</p> <p>It has recently been shown that wave action in <span class="hlt">lakes</span> produces microseisms, which generate noise peaks in the period range of 0.8-1.2 s as recorded by nearby seismic stations. Such noise peaks have been observed at seven seismic stations (H17A, LKWY, B208, B944, YTP, YLA, and YLT) located within 2 km of the Yellowstone <span class="hlt">Lake</span> shoreline. Initial work using 2016 data shows that the variations in the microseism signals at Yellowstone <span class="hlt">Lake</span> correspond with the freezing and thawing of <span class="hlt">lake</span> <span class="hlt">ice</span>: the seismic noise occurs more frequently in the spring, summer, and fall, and less commonly in the winter. If this can be confirmed, then <span class="hlt">lake</span>-generated microseisms could provide a consistent measure of the freezing and melting dates of high-latitude <span class="hlt">lakes</span> in remote areas. The seismic data would then be useful in assessing the effects of climate change on the <span class="hlt">ice</span> phenology of those <span class="hlt">lakes</span>. In this work, we analyze continuous seismic data recorded by the seven seismic stations around Yellowstone <span class="hlt">Lake</span> for the years of 1995 to 2016. We generate probability distribution functions of power spectral density for each station to observe the broad elevation of energy near a period of 1 s. The time dependence of this 1-s seismic noise energy is analyzed by extracting the power spectral density at 1 s from every processed hour. The seismic observations are compared to direct measurements of the dates of <span class="hlt">ice</span>-out and freeze-up as reported by rangers at Yellowstone National Park. We examine how accurate the seismic data are in recording the freezing and melting of Yellowstone <span class="hlt">Lake</span>, and how the accuracy changes as a function of the number of stations used. We also examine how sensitive the results are to the particular range of periods that are analyzed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007QuRes..68..249L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007QuRes..68..249L"><span>Nature and origin of a Pleistocene-age massive ground-<span class="hlt">ice</span> body exposed in the Chapman <span class="hlt">Lake</span> moraine complex, central Yukon Territory, Canada</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lacelle, Denis; Lauriol, Bernard; Clark, Ian D.; Cardyn, Raphaelle; Zdanowicz, Christian</p> <p>2007-09-01</p> <p>A massive ground-<span class="hlt">ice</span> body was found exposed in the headwall of a thaw flow developed within the Chapman <span class="hlt">Lake</span> terminal moraine complex on the Blackstone Plateau (Ogilvie Mountains, central Yukon Territory), which is contemporaneous to the Reid glaciation. Based on visible cryostructures in the 4-m-high headwall, two units were identified: massive ground <span class="hlt">ice</span>, overlain sharply by 2 m of icy diamicton. The nature and origin of the Chapman <span class="hlt">Lake</span> massive ground <span class="hlt">ice</span> was determined using cryostratigraphy, petrography, stable O-H isotopes and the molar concentration of occluded gases (CO 2, O 2, N 2 and Ar) entrapped in the <span class="hlt">ice</span>, a new technique in the field of periglacial geomorphology that allows to distinguish between glacial and non-glacial intrasedimental <span class="hlt">ice</span>. Collectively, the results indicate that the Chapman <span class="hlt">Lake</span> massive ground <span class="hlt">ice</span> formed by firn densification with limited melting-refreezing and underwent deformation near its margin. Given that the massive ground-<span class="hlt">ice</span> body consists of relict glacier <span class="hlt">ice</span>, it suggests that permafrost persisted, at least locally, on plateau areas in the central Yukon Territory since the middle Pleistocene. In addition, the d value of Chapman <span class="hlt">Lake</span> relict glacier <span class="hlt">ice</span> suggests that the <span class="hlt">ice</span> <span class="hlt">covering</span> the area during the Reid glaciation originated from a local alpine glaciation in the Ogilvie Mountains.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011QuRes..76..264Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011QuRes..76..264Z"><span>Freshwater control of <span class="hlt">ice</span>-rafted debris in the last glacial period at Mono <span class="hlt">Lake</span>, California, USA</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zimmerman, Susan R. H.; Pearl, Crystal; Hemming, Sidney R.; Tamulonis, Kathryn; Hemming, N. Gary; Searle, Stephanie Y.</p> <p>2011-09-01</p> <p>The type section silts of the late Pleistocene Wilson Creek Formation at Mono <span class="hlt">Lake</span> contain outsized clasts, dominantly well-rounded pebbles and cobbles of Sierran lithologies. Lithic grains > 425 μm show a similar pattern of variability as the > 10 mm clasts visible in the type section, with decreasing absolute abundance in southern and eastern outcrops. The largest concentrations of <span class="hlt">ice</span>-rafted debris (IRD) occur at 67-57 ka and 46-32 ka, with strong millennial-scale variability, while little IRD is found during the last glacial maximum and deglaciation. Stratigraphic evidence for high <span class="hlt">lake</span> level during high IRD intervals, and a lack of geomorphic evidence for coincidence of <span class="hlt">lake</span> and glaciers, strongly suggests that rafting was by shore <span class="hlt">ice</span> rather than icebergs. Correspondence of carbonate flux and IRD implies that both were mainly controlled by freshwater input, rather than disparate non-climatic controls. Conversely, the lack of IRD during the last glacial maximum and deglacial highstands may relate to secondary controls such as perennial <span class="hlt">ice</span> <span class="hlt">cover</span> or sediment supply. High IRD at Mono <span class="hlt">Lake</span> corresponds to low glacial flour flux in Owens <span class="hlt">Lake</span>, both correlative to high warm-season insolation. High-resolution, extra-basinal correlation of the millennial peaks awaits greatly improved age models for both records.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19960003125','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19960003125"><span>Backscatter from <span class="hlt">ice</span> growing on shallow tundra <span class="hlt">lakes</span> near Barrow, Alaska, winter 1991-1992</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Jeffries, M. O.; Wakabayashi, H.; Weeks, W. F.; Morris, K.</p> <p>1993-01-01</p> <p>The timing of freeze-up and break-up of Arctic <span class="hlt">lake</span> <span class="hlt">ice</span> is a potentially useful environmental indicator that could be monitored using SAR. In order to do this, it is important to understand how the properties and structure of the <span class="hlt">ice</span> during its growth and decay affect radar backscatter and thus <span class="hlt">lake</span> <span class="hlt">ice</span> SAR signatures. The availability of radiometrically and geometrically calibrated digital SAR data time series from the Alaska SAR Facility has made it possible for the first time to quantify <span class="hlt">lake</span> <span class="hlt">ice</span> backscatter intensity (sigma(sup o)) variations. This has been done for <span class="hlt">ice</span> growing on shallow tundra <span class="hlt">lakes</span> near Barrow, NW Alaska, from initial growth in September 1991 until thawing and decay in June 1992. Field and laboratory observations and measurements of the <span class="hlt">lake</span> <span class="hlt">ice</span> were made in late April 1992. The field investigations of the coastal <span class="hlt">lakes</span> near Barrow confirmed previous findings that, (1) <span class="hlt">ice</span> frozen to the <span class="hlt">lake</span> bottom had a dark signature in SAR images, indicating weak backscatter, while, (2) <span class="hlt">ice</span> that was floating had a bright signature, indicating strong backscatter. At all sites, regardless of whether the <span class="hlt">ice</span> was grounded or floating, there was a layer of clear, inclusion-free <span class="hlt">ice</span> overlaying a layer of <span class="hlt">ice</span> with dense concentrations of vertically oriented tubular bubbles. At some sites, there was a third layer of porous, snow-<span class="hlt">ice</span> overlaying the clear <span class="hlt">ice</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.C13C..01D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.C13C..01D"><span>Modes of supraglacial <span class="hlt">lake</span> drainage and dynamic <span class="hlt">ice</span> sheet response</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Das, S. B.; Behn, M. D.; Joughin, I. R.</p> <p>2011-12-01</p> <p>We investigate modes of supraglacial <span class="hlt">lake</span> drainage using geophysical, ground, and remote sensing observations over the western margin of the Greenland <span class="hlt">ice</span> sheet. <span class="hlt">Lakes</span> exhibit a characteristic life cycle defined by a pre-drainage, drainage, and post-drainage phase. In the pre-drainage phase winter snow fills pre-existing cracks and stream channels, efficiently blocking past drainage conduits. As temperatures increase in the spring, surface melting commences, initially saturating the snow pack and subsequently forming a surface network of streams that fills the <span class="hlt">lake</span> basins. Basins continue to fill until <span class="hlt">lake</span> drainage commences, which for individual <span class="hlt">lakes</span> occurs at different times depending on the previous winter snow accumulation and summer temperatures. Three styles of drainage behavior have been observed: (1) no drainage, (2) slow drainage over the side into an adjacent pre-existing crack, and (3) rapid drainage through a new crack formed beneath the <span class="hlt">lake</span> basin. Moreover, from year-to-year individual <span class="hlt">lakes</span> exhibit different drainage behaviors. <span class="hlt">Lakes</span> that drain slowly often utilize the same outflow channel for multiple years, creating dramatic canyons in the <span class="hlt">ice</span>. Ultimately, these surface channels are advected out of the <span class="hlt">lake</span> basin and a new channel forms. In the post-drainage phase, melt water continues to access the bed typically through a small conduit (e.g. moulin) formed near a local topographic minimum along the main drainage crack, draining the <span class="hlt">lake</span> catchment throughout the remainder of the melt season. This melt water input to the bed leads to continued basal lubrication and enhanced <span class="hlt">ice</span> flow compared to background velocities. <span class="hlt">Lakes</span> that do not completely drain freeze over to form a surface <span class="hlt">ice</span> layer that persists into the following year. Our results show that supraglacial <span class="hlt">lakes</span> show a spectrum of drainage behaviors and that these styles of drainage lead to varying rates and timing of surface meltwater delivery to the bed resulting in different dynamic <span class="hlt">ice</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><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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